SOA Set ae ees orto: ; fae ernen ge ceoek - chs veces arevatgaspanatac: s1torminaan ors desats 628 Report on Radiation in a Magnetic Field (p. 52) ...0........cceeeeeeeeeeeee ees 629 An experiment on Simultaneous Contrast. By Grorcr J. Burcu, M.A., NMR hee 93.5, oe sng oS tna 5, ewe (anaes eae Raa secede cM cen nniaass 629 . A Quartz-Calcite Symmetrical Doublet. By J. W. Grrrorp ............... 630 . The Production of an Artificial Light of the same Character as Daylight. By Artuur, Duron, M.A., B.Sc., and WattER M. GARDNER .........+4. 631 FRIDAY, SEPTEMBER 7 . On the Statistical Dynamics of Gas Theory as illustrated by Meteor Swarms and Optical Rays. By J. LARMOR, F.RBAS. .............ccecesseee sees 632 . The Partition of Energy. By G. H. Bryan, Sc.D., F.RS...............0065 634 . Note on the Propagation of Electric Waves along Parallel Wires. By IPTOLEHSON Wie, De MORTON, NUGA vascolusceccssteeresneovercsescatens -seceesarcecen’ 635 . On the Vector Potential of Electric Currents in a Field where Disturb- ances are propagated with Finite Velocity. By 8. H. Bursury, F.R.S. 685 SATURDAY, SEPTEMBER 8. 1. Report on Determining the Magnetic Force on Board Ship (p. 45)......... 637 2. Final Report on the Sizes of Pages of Scientific Periodicals (p. 46)......... 637 3. On the Similarity of Effect of Electrical Stimulus on Inorganic and Living Substances. By Professor Jacapis CuunpER Boss, M.A., D.Sc. 637 . Wireless Telephony. By Sir Witi1am Henry Preece, K.C.B., F.R.S. 658 . On the Apparent Emission of Cathode Rays from an Electrode at Zero Wotentialy By CHantps By Ss PHIMUEUPS! 2 yr2t.scced-.0s0tdsterencerccacdecses 639 . On Volta-electromotive Force of Alloys, and a Test for Chemical elerett, sprbayge Wry (NG ORB: HEY: Sieehd coed dyoantaasaianjnds tps ogeassnnmenniden sees 641 . A Lecture-room Volt and Amperemeter. By Professor F. G. Barty... 645 . On the Phosphorescent Glow in Gases. By Joun B. B. Burxn, M.A. ... 648 xil REPORT—1900. MONDAY, SEPTEMBER 10. DEPARTMENT I,— MATHEMATICS. Page 1. Report on Tables of certain Mathematical Functions (p. 46) ......eseeeees . 648 2. Report on the Present State of the Theory of Point-Groups (p. 121) ...... 643 3. A Property of the characteristic Symbolic Determinant of any n Quantics oes | in n Variables. By Major P. A. MacMaHon, F.R.S. .......ccsceeeeeseneenes 644 . Sur les Relations entre la Géométrie Projective et la Mécanique. Par IMO ICYPARISSOS ISTEPHAWOS .....<.0s0000--be0ce s-nwenn0derecenvapesenuwacedia naman 644 The use of Multiple Space in Applied Mathematics. By H.S. Carstaw 644 . Determination of Successive High Primes. By Lieutenant-Colonel ALLAN Cunninewan, R.E., and H. J. Woonaty, A.R.C.Sc. .....cccesceesereesseee . 646 *On the Construction of Magic Squares. By Dr. J. WILLIS ........00000- 646 . The Asyzygetic and Perpetuant Covariants of Systems of Binary Quantics. Ey Major P, A. MAGMAHON, FIR.S cisccoss-s00scesesnsesoassanisupeallite aoaeee 646 . On the Symbolism appropriate to the Study of Orthogonal and Boolian Invariant Systems which Appertain to Binary and other Quantics. By . Major. AL, WUAONBON, BBS 253522: ceccciseestessoeeesesecamens etcenne a eae 47 10, A Quintic Curve cannot have more than fifteen real Points of Inflexion. ESAs: ERASSIDE, MEU: a siocccece sven teeetes act csioens bess deseo aneeepens one eee 647 11. On a Central-difference Interpolation Formula. By Professor J. D. Bi VERE ABR, Sis SAN eee ehh os Pee Loans: oe ee 648 12, On Newton’s Contributions to Central Difference Interpolation. By Eroipssord. 10 VERRBET, Gk, 2. ee PNT, La ee 650 DEPARTMENT I].--MerroroLoey. - Report on Meteorological Photography (p. 56) ........cssssscessesecerseeseeeee 650 . Report on Seismological Observations (p. 59) .....-ssscceccecenseecceeeeereuseees 650 . Fifth Report on the use of Kites to obtain Meteorological Observations at Blue Hill Observatory, Massachusetts, U.S.A. By A. LAWRENCE EMOTO Sbacy, NEA coho ons ca oasieaaven ods sei ons cng sceta’ cesagus's 71s0 seat tmabene t= taect due ce deacinece ae eens 701 3. “Recent Developments in Stereochemistry. By W. J. Pore .............66 701 4, The Constitution of Camphor. By A, Lapworru, D.Sc. (p. 299) ......00. 702 5, *The Degradation of Camphor. By JULIUS BREDT ..........ccecesecsceueeeee 702 6, *The Camphor Question. By Professor OssIAN ASCHAN .....0.-cccesseeeeeee 702 7. Report on Isomeric Napthalene Derivatives (p. 297) ....ccsccccccccssessveeeees 702 CONTENTS. Xv Page 8. Report on Isomorphous Derivatives of Benzene (p. 167) .............:0cc00es 702 9. Report on the Relations between the Absorption Spectra and Chemical Constitution of Organic Bodies (p. 151) v2. /0.... 6. cece. cesecceseescesevsareceee 702 10. “Action of Aluminium Powder on some Phenols and Acids. By W. R. PPR GMENSIN) Pai ets kc acencreec reset e tes settee cement ante cece eae eae es 702 11. On the Direct Preparation of 8-Naphthylamine. By Dr. Leonnarp ewe Ne and) Wis. PODER INGON 12rtiro fend sceadensecdeescts cawcel ed acdatas 702 12. Interaction of Furfuraldehyde and Caro’s Reagent. By C. F. Cross, pO HON VANM ANG A AEs RIGGS sarc rncrers sone seer ae eet ee Ee tee 702 18. On the Synthesis of Benzo-y-pyrone. By Dr. S. Ruwemann and H. E. SUNEIMPON, Mere ree (RONG) 2, sve ccasvads seitavasddaved eee oseedaedacCoesssoen tendo tne 703 14. On the Combination of Thiophenol and Guaiacol with the Esters of the Acids of the Acetylene Series. By Dr. S. Ruaemann and H. E. SUAS, Eee (OL ONG) a atanc «xc cs sgn gudsuadcagetsemagahia dakeaos shnsgaguronsnieee 704 15, *Chlorination of Aromatic Hydro-carbons. By H. D. Daxin and J. B. | UTTIT. ed 3 ie ee i ea A RR ON “ee ame IN ad Dy Bee 704 TUESDAY, SEPTEMBER 11. DEPARTMENT [. 1. *On some Recent Work on the Diffusion of Gases and Liquids. By 2 MITORAGH Ty, SROWNG FUR Ss. © asc sssevcangaancceseuddttdewentee teens atte necator c 704. - *On Recent Developments in the Textile Industries. By Dr. A. Lippmann 705 . Influence of Pressure on the Formation of Oceanic Salt Deposits. By EE DAWSON AE Ds BS Cig bascash «cee sa ajcnan et daees oabecen. Biccadae Meee se eae 705 . On the Sensitiveness of Metallic Silver to Light. By Major-General MN ATER OUSH, TSO. sicuces sac decscaecs cde cease (cet eae tenah none cee rete 706 5. Some Thoughts on Atomic Weights and the Periodic Law. By J. H. 1 2 3 4 Guapstone, D.Sc., F.R.S., and GEORGE GLADSTONE..........cececeeeceeeeuece 706 DEPARTMENT IT. . Bradford Sewage and its Treatment. By F. W. Ricwarpson, F.1.C. ... 707 . “On the Treatment of Woolcombers’ Effluents. By W. LEAH ............ 708 . On a Simple and Accurate Method for Estimating the Dissolved Oxygen in Fresh Water, Sea Water, Sewage Effluents, &c. By Professor Darr, D.Se¢,, Ph.D; &c.,.amd KR. WS Briar, OC. BOS, ...ccscecveess0s 708 The Utilisation of Sewage Sludge. By Professor W. B. Borrominy, EAS AP NSD) ir. « ovo petals sasie vientsssteed ices’ & dos te 754 4, Ona Glacial ‘Extra-morainic’ Lake occupying the Valley of the Brad- ae be Roe Es ci Big NU LEAUN Ziewcr. lecasencotetecvosecrousittisnedeccies octenns 755 5, A Preliminary Note on the Glaciation of the Keighley and Bradford Dis- ' trict. By Atsert Jowrrt, M.Sc., and Hersert B. Murr .................. 756 6, The Source and Distribution of the far-travelled Boulders of East York- pire. By J. W. STATHER, F.GiS. ooo cscs. cannecns Go dais «dso ennls palace eeiathr ap 759 7. On the Glacial Phenomena of the North-east Corner of the Yorkshire Seelage syed. WW. SPARE MR EA a to c2f uecémihraaaceeins dabeay cas 797 7. The Locust Plague and its Suppression. By Ai. Munro, M.D. ............ 798 Section E.—GEOGRAPHY. THURSDAY, SEPTEMBER 6. _ Address by Sir Georer S. Rozserrtson, K.C.S.1., President of the Section...... 800 1, Attempts to improve the teaching of Geceapka: in Elementary Schools, especially in the West Riding. By T. G. Rooppr, H.M.I................... 809 2. Commercial Geography in Education. By E. R. Weruey, M.A.,F.R.G.S. 810 FRIDAY, SEPTEMBER 7. 1, The a of Regional Geography. By Hvocu Roxsert Muir1, erases eters dnd ane cle aaa AR ige Amen. anatles f, ASAI: 810 2. *Foreign 2 Colonial Surveys. By E. G. RAVENSTBIN ...:...ccisceeeceeees 811 a 2 xx REPORT—1900. Page 8. Military Maps. By B. V. DaRBISHIRE, M.A. .....ceseesee vec. sNRVSR MVE 811 4, Journeys in Central Asia. - By Captain H. H. P. DBASY ....,...-ssssesseeeee 812 5. Large Earthquakes recorded in 1899. By JoHN MIEND ........0..sseseeeees 812 6. Report on the Climates of Tropical Africa (p. 418) .....ssceseeeeeeeseeeseeee 813 MONDAY, SEPTEMBER 10. 1. Railway Connection with India. By Colonel Sir T. H. Horprcu, K.C.1.E. 815 2, The Siberian Railway. By C. RAYMOND BEAZLEY .........cseceeeeeesereeee 814 3. *On the Possibility of Obtaining more Reliable Measurements of the Changes of the Land-level of the Phlegrean Fields. By R. T. GintuEr 814 . The British Antarctic Expedition, 1899-1900. By C. E. Borcnerevink 814 . Through Arctic Lapland. By C. J. Curciirre Hyne, M.A, ............04 815 . Report on Physical and Chemical Constants of Sea Water (p. 421) ...... 815 TUESDAY, SEPTEMBER ll. . Some Consequences that may be anticipated from the Development of the Resources of China by Modern Methods. By Gxo. G. CuHIsHoim, RN MES SCs cas S— nee aetna 818 . On the Pettersson-Nansen Insulating Water-hottle. By Huen Roserr INUIT IDS (hol Ud ) ADS Sa odetonk aoarechecnbasdeo ued annonsoansnbareesacersrah sacs - 819 Section F.—ECONOMIC SCIENCE AND STATISTICS. THURSDAY, SEPTEMBER 6. Address by Major P. G. Cratern, V.P.S.8., President of the Section ......... 820 1. Report on Future Dealings in Raw Produce (p. 421) ........secseeeeeseeeees 837 2, Report on State Monopolies in other Countries (p, 421) ........eceeecseeeees 837 3. Population and Birth-rate, viewed from the historico-statistical standpoint. By MARCUSURUBIN, coseccrcsss eee A re i oe 873 - Power Generation—Comparative Cost by the Steam Engine, Water Turbine, and Gas Engine. By Joun B. C, KersHaw, F.LC, .ssccceeereeee 873 XXil REPORT—1900. MONDAY, SEPTEMBER 10. Page 1, *The Automobile for Electric Street Traction, By J.G. W. Aupripex.. 875 2. The Manchester and Liverpool Express Railway. By Sir W. H. PREBCH, VRS. cosnatevonnaneornauineeeareterbec ca teres orcctereces Soaweees someon semen 875 3. Manchester and Liverpool Electrical Express Railway: Brakes and Signals, By PF. B, BRS. J iisissvicAiest ccaeeness ave seats cms «swesheseboananeneers 876 4, *The Construction of Large Dynamos, as Exemplified at the Paris Exhibition. By Professor S. P. Tompson, F.RAS. ........csccsseeeeeseeeeees 877 5. *Recent Tramway Construction. By W. DAWSON........ csssesessereeeseeeers 877 6. Measurement of the Tractive Force, Resistance. and Acceleration of Prainss:) By tA... MARLOOR |....5.s.estoesse tes da vctenedbns ssbesodeh sone hens soaNaeemen 877 7. On a Combination integrating Wattmeter and Maximum Demand Indicator. By T. BaRKER .............e8eeee Hikaan bo tnhd.d. tole See + 878 8. The Design and Location of Electric Generating Stations. By ALrrEp [EE SGUBBINGS, MiInet Hal,” | 522 .s. daodusnesoosmaenite nts > dupes eunhe hE eneen 22 878 TUESDAY, SEPTEMBER 11. 1. Report on Small Screw Gauges (p. 486) ........cssssscsccccssseesseeessnessssoees 879 2, On Screw Threads used in Cycle Construction, and for Screws subject to Vabration, yO, BP. (COMMENTS cots vanssess0s0n0 dus bbeehs see ROR 879 8. The Photographic Method of Preparing Textile Designs. By Professor ROBERTS BEAUMONT, MoI. Mech.Es Sc..s-.spsnsctes sho swaatetes wwitesscteteine . 881 4, *Shop Buildings. By E. R. Crarx, M.Inst.C.E. .,...0.5..00--sasseeneweanssv¥ 882 5. *The Internal Architecture of Steel. By Professor ARNOLD ............008 882 6. “A New Form of Calorimeter for Measuring the Wetness of Steam. By ETOLESSOL J, (HOOD MAIN ©. ccppizasagesrussecuany vay? ¥ratsy+sas ches euseneeee eae 882 7. On the Reheating of Compressed Air. By Witt1am Gxuorce WALKER, ASNT GC Ey NCTGSG IM Bias seenesnvencuesnsbasersichatyedederseaea yak? aan 883 Section H.—ANTHROPOLOGY. THURSDAY, SEPTEMBER 6. Address by Professor Joun Ruys, M.A., LL.D., President of the Section...... 884 1. Some Implements of the Natives of Tasmania. By J. Paxron Morr...... 896 2. The Stone Age in Tasmania as related to the History of Civilisation. By Hh, B. TYLOR, PRS cesaiscies vasereviap out beepers sdeeevnasoWanepe eth seee tan 897 8, Report on Mental and Physical Deviations of Children in Schools (p. 461) 897 4, Report on the Silchester Excavation (p. 466) ...........sseccseeseees wen cuaticehs 897 5. Writing in Prehistoric Greece. By Arruur J. Evans, M.A., F.S.A...... 897 6. On the System of Writing in Ancient Egypt. By F. Lu. GRrirrirn ...... 899 7. *Interim Report on Anthropological Teaching ..........scseesseeey ceeeeees .-» 899 8, Report on Anthropological Photographs (p. 568) .........c0c:seeeesseeeneeeene 899 FRIDAY, SEPTEMBER 7. 1, The Cave of Psychré in Crete. By D. G. HOGARTH ............s0ceeeeseee ... 899 2, On the Japanese Gohei and the Ainu Inao. By W.G. Aston ..........: . 900 3. The Textile Patterns of the Sea-Dayaks. By Dr. A. C. Happon, F.R.8. 901 CONTENTS. XXL Page 4, Relics of the Stone Age of Borneo. By Dr. A. C. Hannon, F.R.S. ...... 901 5, Houses and Family Life in Sarawak. By Dr. A. C. Happon, F RS... eras 902 SATURDAY, SEPTEMBER 8 1, On the eee of West Yorkshire. By Joun Buppos, M.D., ON Ay: a acatina patn manana ace)us ceaieeswnaneh Te Klirksnehwancsdencanendeadtahenitee 902 2. On ‘ie Vagaries of the Kephalic Index. By Joun Beppon, M.D., Ue EUR Satnic cng cas ons oses cases sanch vase apails SutWacs an te acts oSbuifuiqaalits Usage gaeeetent 902 . On certain Markings on the Frontal Part of the Human Cranium, and their Significance. By A. FRANOIS DIXON ...........:cssssecseeceseeesenens see 903 . On the Sacral Index. By Professor D. J. Cunninenam, M.D., FBS. ... 908 . On the Microcephalic Brain. By Professor D. J. CunnineHam, M.D., Heer Sateen fe ccu con siaaths thse cactasb es saan tticash cbicweneh ct Gee tictacdoeseaaheragaacizces as 904 . Developmental Changes in the Human Skeleton from the Point of View of Anthropology. By Davip Warterston, M.D., F.R.C.S.E. «0... OL MONDAY, SEPTEMBER 10. . On the Imperfection of our Knowledge of the Black Races of the Trans- vaal and the Orange River Colony. By E. 8. Harrnann, F.S.A.. . 904 2. On a Mould showing the Finger-prints of a Roman Sculptor of mente the Third Century. By Sir Wittram Turner, M.B., F.R.S. ............084 905 3. Report on the Canadian Ethnographic Survey (p. 468) ............0.:.cceseeee 905 4, The Paganism of the Civilised Iroquois. By Davin Boy1e.................. 905 5. Notes on Malay Metal-work. By Watrer RosEnHAIN, B.A.............045 906 6. Note on the ‘ Kingfisher’ Kriss. By Professor Hunry Lovis, M.A. ...... 906 7. On some Buddhist Sites. By W. LAW BRO0S..........:.ccecssseesecuteceneceens 906 TUESDAY, SEPTEMBER 11. 1, On Permanent Skin-marks, Tattooing, Scarification, &c. By H. Live rs EU CIID nee ace anc ak bg at siaiale Seiten dh tics chaunis aacueetaaoaes aomtuGl aaphcunecoubebeeat 907 . Some Peculiar Features of the Animal-cults of the Natives of Sarawak, and their Bearing on the Probiems of Totemism. By CHaR.LzEs Hoss, D.Sc., and W. McDoveat, MEA Acsaucteccsaapscpnsnstseoshr sesnsieeacauseeeeee 931 7. Ou the Structure of the Root-nodules of Alnus glutinosa. By T. W. WOODETBAD 0520 la08 seks iv onecus va’ n'e dah Gunn eentayeNing Auld Palen Eanes ne 931 8. Fungi found in Ceylon growing upon Scale-insects (Coccide and Aleuro- dide:).!* By J. PARKIN, MA, |. ...0sssedueBerseeusninsnStansauscensenns Slee ceaa 932 FRIDAY, SEPTEMBER 7. 1, *On the so-called Optimum Strength of CO, for Assimilation. By Dr. RAB A SGACKIMAN § 51 05. avec. ues cpbacchawade coe eenUnees stvaeian cota Mie nee tama 933 2. *On the Effect of the Closure of Stomata on Assimilation. By Dr. F. F. BLACKMAN and Miss MATTHAIL...0.ciss.ccuseyarcernerecusvsnestanessehseapeenea 9354. 3. Formation of Starch from Glycollic Aldehyde by Green Plants. By HENRY JACKSON, BeA., BiSe, (a. 5shs csc beccosens ssh decease ee conse Oat ae eam 934 4, On the Effect of Salts on the CO, Assimilation of Ulva latissima, L. By EB ASAE WEL ARBER BUA}. cscteacmeeost scenester teebod thine eenee nee mene eee. O34 5. The Sea-weed Ulva latissima and its Relation to the Pollution of Sea- be | water by Sewage. By Professor Lerrs, D.Sc., Ph.D., and Joun Haw- HORNE, "BiAcsseteoeascetce on keno notes sontee eee nee BA OR icy 30 935 . Germination of the Zoospore in Laminariacew. By J. Luoyp Wititams 936 . *A Lecture on Plant-form in Relation to Nutrition. By Professor Percy (ROOM. Fee. clavate coe eee ete ES eee eee wees 1 SA eee 936 SATURDAY, SEPTEMBER 8. . On Double Fertilisation in a Dicotyledon—Caltha palustris, By Ernan ING PEEIOMAS 1... Sadicerbsthdenesbsc coos eee nee enna aekhl eohehieevestirae 936 . The Conducting Tissues of Bryophytes. By A. G. TANSLEY ......c.scs00 957 CONTENTS, XXV Page 3. On a Fourth Type of Transition from Stem to Root-structure occurring in certain Monocotyledonous Seedlings) By ETHEL SARGANT........0000-., 937 4, The Origin of Modern Cycads. By W.C. Worspitt, F.LS. .....00....c000 938 . On the Structure of the Stem of Angiopteris evecta, Hoffm. By R. F. BRUEG VP ete Sakae sok Sooseic cdi ts nah Cas cak tee eee ae reer eoserC nny Be eared ae cee 939 MONDAY, SEPTEMBER 10. 1. A Joint Discussion with Section C on the Conditions under which the Plants of the Coal Period grew (p. 746) ....s...sssccesssecccsescesesseneees veeee 940 2. Further Investigations on the Intumescences of Hibiscus vitifolius (Linn.). Beets EMME, LAE Oi ec dycseattaaduade idvdnavaven dass uae danacdataniedoeccode 940 8. On the Osmotic Properties and their Causes in the Living Plant and Animal Cell. By Professor E. F. OVERTON ........sceccscccssssccsansesscctees 940 4, The Biology and Cytology of a new Species of Pythium. By Professor BE PNW tats oe Mad, vc e Laiatess Sede e tatebua sr aavegsN cae eid ei reer . 941 5, Observations on Pythium. By G. Porravur and E. J. Burner............ 942 6. Observations on some Chytridinee. By G. Porravtr and E. J. Burter 942 7. On the Azygospores of Entomophthora gleospora. By Professor P. 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Forbes, W. Ick, R. Patterson. Sir W. J. Hooker, LL.D.......| Prof. W. Couper, E. Forbes, R. Pat- terson. John Richardson, M.D., F.R.S.| J. Couch, Dr. Lankester, R. Patterson. Hon. and Very Rev. W. Her- Dr. Lankester, R. Patterson, J. A. bert, LL.D., F.L.S. | ‘Turner, William Thompson, F.L.S.... G. J. Allman, Dr. Lankester, R. | Patterson. Very Rev. the Dean of Man- Prof. Allman, H. Goodsir, Dr. King, chester. | Dr. Lankester. Rev. Prof. Henslow, F.L.S....| Dr. Lankester, T. V. Wollaston. Sir J. Richardson, M.D., Dr. Lankester, T. V. Wollaston, H. F.R.S. Wooldridge. H. E. Strickland, M.A., F.R.S, Dr. Lankester, Dr. Melville, T. V. Wollaston. SECTION D (continwed).—ZOOLOGY AND BOTANY, INCLUDING PHYSIOLOGY. [For the Presidents and Secretaries of the Anatomical and Physiological Sub- sections and the temporary Section FE of Anatomy and Medicine, see p. 1xi.] 1848. Swansea 1849. Birmingham 1850. 1851. 1852. 1853. 1854. 1855. 1856. 1857. Edinburgh Ipswich EGU esses Liverpool... Glasgow ... Cheltenham Dublin eases peo] Mua WedDibwyn, HWS: ectecnes ...|Rev. Prof. Henslow, M.A., Dr. R. Wilbraham Falconer, A, Hen- | frey, Dr. Lankester. Dr. Lankester, Dr. Russell. Prof. J. H. Bennett, M.D., Dr. Lan- kester, Dr. Douglas Maclagan. Prof. Allman, F. W. Johnston, Dr. E. Lankester. Dr. Dickie, George C. Hyndman, Dr. Edwin Lankester. | William Spence, F.R.S. ...... |Prof. Goodsir, F.R.S. L. & E. F.R.S. Ae C. C. Babington, M.A., F.R.S. Prof. Balfour, M.D., F.R.S.... Rev. Dr. Fleeming, F.R.S.E. Thomas Bell, F.R.S., Pres.L.S. Prof. W. H. Harvey, M.D., E.R.S. Robert Harrison, Dr, E. Lankester. Isaac Byerley, Dr. E. Lankester. William Keddie, Dr. Lankester. Dr. J. Abercrombie, Prof, Buckman, | Dr. Lankester. Prof. J. R. Kinahan, Dr. E. Lankester, Robert Patterson, Dr. W. E. Steele. 1 At this Meeting Physiology and Anatomy were made a separate Committee, for Presidents and Secretaries of which see p, 1xi. ——————ee 1862. 1865. 1872. Brighton ... PRESIDENTS AND SECRETARIES OF THE SECTIONS. lix Date and Place Presidents Secretaries 1858. Leeds ...... ©. C. Babington, 1859. Aberdeen.. Oxford...... 1860. Rev. Prof. Henslow, F.L.S... 1861. Manchester | Prof. C. C. Babington, F.R.S. | Cambridge Prof. Huxley, F.R,S Neweastle Prof. Balfour, M.D., ou RS eee eee eee 1863. 1864, Dr. John E, Gray, F.R.S. Birming- T, Thomson, M.D., F.R,S. . ham ! | .|H. B. Brady, C. M.A., F.R.8.|Henry Denny, Dr. Heaton, Dr. E. Lankester, Dr. E. Perceval Wright. . Sir W. Jardine, Bart., F.R.S.E.| Prof. Dickie, M.D., Dr. E. Lankester, Dr. Ogilvy. .|W. 8. Church, Dr. E. Lankester, P. L. Sclater, Dr. E, Perceval Wright. Dr. T. Alcock, Dr. E. Lankester, - Dr. cope be Selater, Dr. E. P. Wright. Alfred Newton, Dr. E. P. Wright. . Dr. E. Charlton, A. Newton, Rev. H. B. Tristram, Dr. EK. P. Wright. E. Broom, H. T, Stainton, Dr. E. P. Wright. . Dr. J. Anthony, Rev, C. Clarke, Rev. H. B. Tristram, Dr, E. P, Wright. SECTION D (continued ),—BIOLOGY. 1866. Nottingham)Prof. Huxley, F.R.S.—Dep.|Dr. J. Beddard, W. Felkin, Rev. H. of Physiol., Prof. Humphry, F.R.S.—Dep. of Anthropol., A. R. Wallace. 1867. Dundee —Dep. of Zool. and Bot., George Busk, M.D., F.R.S. 1868. Norwich ... —Dep. of Physiology, W. H. Flower, F.R.S. 1869. Exeter......, —Dep. of Bot. and Lool., C. Spence Bate, F.R.S.— Dep. of Hthno., E. B. Tylor. Prof.G. Rolleston, M.A., M.D., | EVR.S., F.L.8.— Dep. Anat. and Physiol., Prof.M. Foster, M.D., F.L.5.—Dep. of Ethno., J. Evans, F.R.S. Prof. Allen Thomson, M.D., F.R.S.—Dep. of Bot. and Zool.,Prof.WyvilleThomson, F.R.S.—Dep. of Anthropol., Prof. W. Turner, M.D. Sir J. Lubbock, Bart., F.R.S.— Dep. of Anat. and Physiol., Dr. Burdon Sanderson, ; F.R.S.—Dep. of Anthropol., Col. A. Lane Fox, F.G.S. 1870. Liverpool... 1871. Edinburgh. 1873, Bradford ... Anat.and Physiol.,Prof. Ru- therford, M.D.— Dep. of An- thropol,, Dr. Beddoe, F.R.S. of Bb. Tristram, W. Turner, E. B. Tylor, Dr. E. P. Wright. .. Prof. Sharpey, M.D., Sec. R.S.|C. Spence Bate, Dr. S. Cobbold, Dr. M. Foster, H. T. Stainton, Rev. H. B. Tristram, Prof. W. Turner. Rev. M. J. Berkeley, F.L.S.}Dr. T. 8. Cobbold, G. W. Firth, Dr. M. Foster, Prof. Lawson, H.T. Stainton, Rey. Dr. H. B. Tristram, Dr. E. P. Wright. George Busk, F.R.S., F.L.8.| Dr. T. S. Cobbold, Prof. M. Foster, EK. Ray Lankester, Prof. Lawson, H. T, Stainton, Rev. H. B. Tris- tram. Dr. T. $. Cobbold, Sebastian Evans, Prof. Lawson, Thos. J. Moore, H. T. Stainton, Rev. H. B. Tristram, C. Staniland Wake, E. Ray Lan- kester. Dr. T. R. Fraser, Dr. Arthur Gamgee, E. Ray Lankester, Prof. Lawson, H. T. Stainton, C. Staniland Wake, Dr. W. Rutherford, Dr. Kelburne King. Prof, Thiselton- Dyer, H. T. Stainton, Prof. Lawson, F. W. Rudler, J. H. Lamprey, Dr. Gamgee, E. Ray Lankester, Dr. Pye-Smith. Prof. Allman, F.R.S.— Dep. of | Prof. Thiselton-Dyer, Prof. Lawson, R. M‘Lachlan, Dr. Pye-Smith, E. Ray Lankester, F. W. Rudler, J H. Lamprey. The title of Section D was changed to Biology. ib REFORT—1900. Date and Place Presidents Secretaries 1874. Belfast ...... Prof. Redfern, M.D.—Dep. of Zool. and Bot., Dr. Hooker, | C.B.,Pres.R.S.—Dep. of An- throp.,Sir W.R. Wilde, M.D. 1875, Bristol ...... P. L. Sclater, F.R.S.— Dep. of Anat. and Physiol., Prof. Cleland, F.R.S.—Dep. of Anth.,Prof.Rolleston,F.R.S. 1876. Glasgow ...|A. Russel Wallace, F.L.S.— Dep. of Zool. and Bot., Prof. A. Newton, F.R.S.— Dep. of Anat. and Physiol., Dr. J. G. McKendrick. 1877. Plymouth...|J. Gwyn Jeffreys, F.R.S.— Dep. of Anat. and Physiol. Prof. Macalister.—Dep. of| Anthropol.,F.Galton,F.R.S. 1878. Dublin...... Prof. W. H. Flower, F.R.S.— Dep. of Anthropol., Prof. Huxley, Sec. R.S.—Dep. of Anat. and Physiol, BR. McDonnell, M.D., F.R.S. 1879, Sheffield ,..|Prof. St. George Mivart, F.R.S.-—Dep. of Anthropol., KE. B. Tylor, D.C.L., F.R.S. —Dep. of Anat. and Phy- siol., Dr. Pye-Smith. 1880, Swansea .../ A.C. L. Giinther, F.R.S.— Dep. of Anat. 5 Physiol., F. M. Balfour, F.R.S.—Dep. of Anthropol., F, W. Budler. TSBIS YOK. scenes.) R. Owen, F'.R.S.— Dep. of An- thropol., Prof. W.H. Flower, F.R.S.—Dep. of Anat. and Physiol., Prof. J. 8. Burdon Sanderson, F.R.S. 1882. Southamp- |Prof. A. Gamgee, M.D., F.R.S. ton. — Dep. of Zool. and Bot., Prof. M. A. Lawson, F.L.S. —Dep. of Anthropol., Prof. W. Boyd Dawkins, F.R.S. 1883. Southport’ | Prof. E. Ray Lankester, M.A., F.R.S.— Dep. of Anthropol., W. Pengelly, F.R.S. 1884. Montreal ...| Prof. H. N. Moseley, M.A., F.R.S. 1885. Aberdeen ...| Prof. W.C. M‘Intosh, M.D., LL.D., F.R.S. F.R.S.E. 1886. Birmingham|/W. Carruthers, Pres. L.S., E.R.S., F.G.S. 1887. Manchester | Prof. A. Newton, M.A., ARS: W. T. Thiselton- Dyer, R. 0. Cunning- ham, Dr. J. J. Charles, Dr. P. H. Pye-Smith, J. J. Murphy, F. W. Rudler. E. R. Alston, Dr. McKendrick, Prof, W. R. M‘Nab, Dr. Martyn, F. W. Rudler, Dr. P. H. Pye-Smith, Dr. W. Spencer. E. R. Alston, Hyde Clarke, Dr. Knox, Prof. W. R. M‘Nab, Dr. Muirhead, Prof. Morrison Wat- son, E. R. Alston, F. Brent, Dr. D. J. Cunningham, Dr. C. A. Hingston, Prof. W. R. M‘Nab, J. B. Rowe, F. W. Rudler. Dr. R. J. Harvey, Dr. T. Hayden, Prof. W. R. M‘Nab, Prof. J. M. Purser, J. B. Rowe, F. W. Rudler, Arthur Jackson, Prof. W. R. M‘Nab, J. B. Rowe, F. W. Rudler, Prof, Schafer. G. W. Bloxam, John Priestley, Howard Saunders, Adam Sedg- wick. G. W. Bloxam, W. A. Forbes, Rev. W. C. Hey, Prof. W. R. M‘Nab, W. North, John Priestley, Howard Saunders, H. H. Spencer. G. W. Bloxam, W. Heape, J. B. Nias, Howard Saunders, A. Sedg- wick, T. W. Shore, jun. G. W. Bloxam, Dr. G. J. Haslam, W. Heape, W. Hurst, Prof. A. M. Marshall, Howard Saunders, Dr. G. A. Woods. Prof. W. Osler, Howard Saunders, A. Sedgwick, Prof. R. R. Wright. W. Heape, J. McGregor-Robertson, J. Duncan Matthews, Howard Saunders, H. Marshall Ward. Prof. T. W. Bridge, W. Heape, Prof. W. Hillhouse, W. L. Sclater, Prof, H. Marshall Ward. C. Bailey, F. E. Beddard, 8. F. Har- mer, W. Heape, W. L. Sclater, | E.LS., V.P.Z.8. Prof. H, Marshall Ward. * Anthropology was made a separate Section, see p. Ixviii. PRESIDENTS AND SECRETARIES OF THE SECTIONS. Date and Place Presidents Ixi Secretaries 1888. Bath se eaerene 1889. Newcastle - upon-Tyne 1890. Leeds eeeeee 1891. Cardiff...... 1892. Edinburgh 1893. Nottingham! 1894. Oxford? ... 1895. Ipswich ... 1896. Liverpool... 1897. Toronto 1898. Bristol...... 1899. Dover ...... 1900. Bradford ... |Prof. W. A. Herdman, F.R.S8. Prof. EH. B. Poulton, F.R.S. ... | a. | erot. la, CF MiallS W.RSS csc. W. T. Thiselton-Dyer, C.M.G., F.R.S., F.L.S. Prof. J. 8. Burdon Sanderson, | M.A., M.D., F.R.S. Prof. A. Milnes Marshall, M.A., M.D., D.Sc., F.R.S. Francis Darwin, M.A., M.B., E.R.S., F.L.S. Prof. W. Rutherford, E.R.S., F.R.S.E. Rev. Canon H. B. Tristram, M.A., LL.D., F.R.S. M.D. Prof. I. Bayley Balfour, M.A., F.R.S, SECTION D (continued). Prof. W. F. R. Weldon, F.R.5. | Adam Sedgwick, F.R.S. ...... Dr. R. H. Traquair, F.B.S. ... F. EK. Beddard, S. F. Harmer, Prof. H. Marshall Ward, W. Gardiner, Prof. W. D. Halliburton. C. Bailey, F. E. Beddard, S. F. Har- mer, Prof. T. Oliver, Prof. H. Mar- shall Ward. 8. F. Harmer, Prof. W. A. Herdman, 8. J. Hickson, F. W. Oliver, H. Wager, H. Marshall Ward. | I, E. Beddard, Prof. W.A. Herdman, Dr. 8. J. Hickson, G. Murray, Prof. W.N. Parker, H. Wager. G. Brook, Prof. W. A. Herdman, G. Murray, W. Stirling, H. Wager. G. C. Bourne, J. B. Farmer, Prof. W. A. Herdman, S. J. Hickson, W. B. Ransom, W. L. Sclater. W. W. Benham, Prof. J. B. Farmer, Prof. W. A. Herdman, Prof. 8. J. Hickson, G. Murray, W. L. Sclater. —ZOOLOGY. G. C. Bourne, H. Brown, W. E. Hoyle, W. L. Sclater. \H. O. Forbes, W. Garstang, W. E. Hoyle. |W. Garstang, W. E. Hoyle, Prof. E. E. Prince. Prof. R. Boyce, W. Garstang, Dr. A. J. Harrison, W. E. Hoyle. |W. Garstang, J. Graham Kerr. W. Garstang, J.G. Kerr, T. H. Taylor, Swale Vincent. ANATOMICAL AND PHYSIOLOGICAL SCIENCES. COMMITTEE OF SCIENCES, V.—ANATOMY AND PHYSIOLOGY. 1833. Cambridge 1834, Edinburgh Dr. J. Haviland........... pale Dr. Abercrombie ...... ausaeeens Dr. H. J. H. Bond, Mr. G. E. Paget, Dr. Roget, Dr. William Thomson. SECTION © (UNTIL 1847).—ANATOMY AND MEDICINE. 1835. Dublin...... 1836. Bristol ...... 1837. Liverpool... 1838. Newcastle Wry JeOs Pritehard, .s<.cscccesn Dr. P. M. Roget, F.R.S. Prof. W. Clark, M.D. T. E. Headlam, M.D. 1839, Birmingham |John Yelloly, M.D., F.R.S8.... _ 1840. Glasgow ... 1841. Plymouth.. James Watson, M.D. Dr. Harrison, Dr. Hart. .| Dr. Symonds. Dr. J. Carson, jun., James Long, Dr. J. R. W. Vose. T. M. Greenhow, Dr. J. R. W. Vose, Dr. G. O. Rees, F'. Ryland. Dr.J. Brown, Prof. Couper, Prof. Reid. SECTION E.—PHYSIOLOGY. a M. Roget, M.D., Sec. B.S. |Dr. J. Butter, J. Fuge, Dr. B.S Sargent. 1842, el lWaward Holme, M.D., F.L.8.|Dr. Chaytor, Dr, R. 8. Sargent. 1843, Cork ...... 1844, York... .| Sir James Pitcairn, M. D. .|Dr. John Popham, Dr. R. 8. Sargent, Mia brincharde WD): sscesaane I. Erichsen, Dr. R. S. Sargent. 1845, Cambridge | Prof. J. Haviland, M.D. .|Dr. R, 8, Sargent, Dr. Webster. 1 Physiology was made a separate Section, see p. Ixix, 2 The title of Section D was changed to Zoology. |xil REPORT— 1900. l Date and Place | Presidents Secretaries 1846. Southamp- | Prof. Owen, M.D., F.R.S. ... C. P. Keele, Dr. Laycock, Dr. Sar- ton. gent. 1847. Oxford’ ... Prof. Ogle, M.D., F.R.S. ......|'Z, K. Chambers, W. P, Ormerod. PHYSIOLOGICAL SUBSECTIONS OF SECTION D. 1850. Edinburgh | Prof. Bennett, M.D., F.R.S.E. 1855. Glasgow ...|Prof. Allen Thomson, F.R.S. | Prof. J. H. Corbett, Dr. J. Struthers. 1857. Dublin...... Prof. R. Harrison, M.D. ......) Dr. R. D. Lyons, Prof. Redfern, 1858. Leeds ...... Sir B. Brodie, Bart., F.R.S. |C. G. Wheelhouse. 1859. Aberdeen... |Prof. Sharpey, M.D., Sec.R.S. Prof. Bennett, Prof. Redfern. 1860. Oxford...... Prof.G.Rolleston,M.D.,F.L.S. | Dr. R. M‘Donnell, Dr. Edward Smith, 1861. Manchester | Dr. John Davy, F.R.S. L.& E.| Dr. W. Roberts, Dr. Edward Smith. 1862. Cambridge |G. E. Paget, M.D.............0+ G. F. Helm, Dr. Edward Smith. 1863. Newcastle | Prof. Rolleston, M.D., F.1t.8.| Dr. D. Embleton, Dr. W. Turner. 1964, Bath: .:....055 Dr. Edward Smith, F.R.S. |J. 8. Bartrum, Dr. W. Turner. 1865. Birming- |Prof. Acland, M.D., LL.D., Dr. A. Fleming, Dr. P. Heslop Buta | EBS. | Oliver Pembleton, Dr. W. Turner GEOGRAPHICAL AND ETHNOLOGICAL SCIENCES. [For Presidents and Secretaries for Geography previous to 1851, see Section C, Pp ly.] ETHNOLOGICAL SUBSECTIONS OF SECTION D. 1846.Southampton| Dr. J. C. Pritchard ............ |Dr. King. 1847. Oxford ...... Prof. H. H. Wilson, M.A. ...|Prof. Buckley. LB48. SWaNsea ...|.cccrcsccscccccerersenrsecrssserssnaes G. Grant Francis. SO WSN HAIN apa cancravsoensh ene svenscoildvs sakes ess Dr. R. G. Latham. 1850. Edinburgh |Vice-Admiral Sir A. Malcolm! Daniel Wilson. SECTION E.—GEOGRAPHY AND ETHNOLOGY. 1851. Ipswich ...|Sir R. I. Murchison, F.R.$.,|. Cull, Rev. J. W. Donaldson, Dr, Pres. R.G.S. | Norton Shaw. 1852. Belfast...... Col, Chesney, R.A., D.C.L.,' R. Cull, R. MacAdam, Dr. Norton F.R.S. | Shaw. 1853; Hall)... i\R. G. Latham, M.D., F.R.S. |R. Cull, Rev. H. W. Kemp, Dr. Norton Shaw. 1854. Liverpool... |Sir R. I. Murchison, D.C.L.,| Richard Cull, Rev. H. Higgins, Dr. | F.RS. Thne, Dr. Norton Shaw. 1855. Glasgow ... (ax J. Richardson, M.D.,/Dr. W. G. Blackie, R. Cull, Dr. |. “BERS. Norton Shaw. 1856. Cheltenham Col. Sir H. C. Rawlinson, R. Cull, F. D. Hartland, W. H. K.C.B. Rumsey, Dr. Norton Shaw. 1857. Dublin...... |Rev. Dr. J. Henthorn Todd,|R, Cull, 8. Ferguson, Dr. R. R. Ff Pres. R.LA. Madden, Dr. Norton Shaw. 1 By direction of the General Committee at Oxford, Sections D and E were incorporated under the name of ‘Section D—Zoology and Botany, including Phy- siology’ (see p. iviil.). Section H, being then vacant, was assigned in 1851 to Geography. 2 Vide note on page lix. PRESIDENTS AND SECRETARIES OF THE SECTIONS. * Date and Place lxiti Presidents Secretaries 1858. Leeds ...... 1859. Aberdeen... 1860. Oxford...... 1861. Manchester 1862. Cambridge 1863. Newcastle 1864. Bath......... 1865. Birmingham 1866. Nottingham 1867. Dundee 1868. Norwich ... 1869, Exéter 1870. Liverpool... 1871. Edinbutgh 1872. Brighton os 1873. Bradford ... 1874. Belfast 1875. Bristol...... 1876. Glasgow ... 1877. Plymouth... 1878. Dublin 1879. Sheffield ... 1880. Swansea ... 1881. York......... 1882. Southamp- "+ ton. 1883. Southport 1884. Montreal ... 1885. Aberdeen... 1886. Birmingham Sir R.I. Murchison, G.C.St.8., F.B.S. Rear - Admiral Sir James Clerk Ross, D.C.L., F.R.8. Sir R. I. Murchison, D.C.L.., F.R.S8. John Crawfurd, F.R.S.......... Francis Galton, F.R.S.......... Sir R. I. Murchison, K.C.B., F.B.S. Sir R. I. Murchison, K.C.B., E.R.S. Major-General Sir H. Raw- linson, M.P., K.C.B., F.R.S. Sir Charles Nicholson, Bart., LL.D. .|Sir Samuel Baker, F.R.G.S8. Capt. G. H. Richards, R.N., F.RB.S. K.C.B., LL.D., F.R.G.S. Sit R. I. Murchison, Bt.,K.C.B., LL.D., D.C.L., #.B.S., F.G.S. |Colonel Yule, C.B., F.R.G.S. Francis Galton, F.R.S........:. Sir Rutherford Alcock, K.C.B. | #.R.G.S. Lieut. - General Strachey; R.E., C.S.1., F.R.S., F.R.G.S. |Capt. Evans, C.B., F.R.S....... ‘Adm, Sir E. Ommanney, C.B. Prof. Sir C. Wyville Thom- son, LL.D.,F.R.S., F.RS.E. Clements R. Markham, C.B., F.R.S., Sec. R.G.S. Lieut.-Gen. Sir J. H. Lefroy, C.B., K.C.M.G., R.A., F.R.S. \Sir J.. D.. Hooker, K.C.S.L, C.B., E-B.S. Lieut.-Col. H. H. Godwin- Austen, F.R.S. Gen. Sir J. H. Lefroy, C.B., K.C.M.G.,.F.B.S.,V.P.R.G.S. Gen. J. T. Walker, C.B., R.E., LL.D., F.R.S. Kes. CB. PRG. Major Wilson, R.E., F.R.S.,! Sir R. Temple, Bart., G.C.S.L,| Maj.-Gen. Sir. F. J. Goldsmid, R. Cull, F. Galton, P. O’Callaghan, Dr. Norton Shaw, T. Wright. Richard Cull, Prof. Geddes, Dr. Nor- ton Shaw. Capt. Burrows, Dr. J. Hunt, Dr. C. Lempriére, Dr. Norton Shaw. Dr. J. Hunt, J. Kingsley, Dr. Nor- ton Shaw, W. Spottiswoode. J.W.Clarke, Rev. J.Glover, Dr. Hunt, Dr. Norton Shaw, T. Wright. C. Carter Blake, Hume Greenfield, C. R. Markham, R. 8. Watson. H. W. Bates, C. R. Markham, Capt. R. M. Murchison, T. Wright. H. W. Bates, S. Evans, G. Jabet, C. R. Markham, Thomas Wright. H. W. Bates, Rev. HE. T. Cusins, R. H. Major, Clements R. Markham, D. W. Nash, T. Wright. H. W. Bates, Cyril Graham, C. R. Markham, 8. J. Mackie, R. Sturrock. T, Baines, H. W. Bates, Clements R. Markham, T. Wright. | SECTION E (continued).—GHOGRAPHY. :|Sir Bartle Frere, H. W. Bates, Clements R. Matkham, J. H. Thomas. 'H.W.Bates, David Buxton, Albert J Mott, Clements R. Markham. A. Buchan, A. Keith Johnston, Cle- ments R. Markham, J. H. Thomas. H. W. Bates, A. Keith Johnston, Rev. J. Newton, J. H. Thomas. H. W. Bates, A. Keith Johnston, Clements R. Markham. E.G. Ravenstein, E. C. Rye, J. H. | Thomas. lH. W. Bates, E. C. Rye, F. F. Tuckett. H. W. Bates, E. C. Rye, R. O. Wood. H. W. Bates, F. H. Fox, H. C. Rye. John Coles, H. C. Rye. H. W. Bates, C. E. D. Black, E. C, Rye. H. W. Bates, EH. C. Rye. J. W. Barry, H. W. Bates. i. G. Ravenstein, EH. C. Kye. John Coles, E. G. Ravenstein, H. C. Rye. Rev. Abbé Lafiamme, J.S. O’Halloran, E. G. Ravenstein, J. F. Torrance. J.S. Keltie, J. 8S. O'Halloran, H. G. Ravenstein, Kev. G. A. Smith. F. T. S. Houghton, J. 8. Keltie E. G. Ravenstein, lxiv REPORT—1900, Cee eEEEEEEEEEEEEEEEE Date and Place Secretaries 1887. 1888. 1889. 1890. 1891. 1892. 1893. 1894. 1895. 1896. 1897. 1898. 1899, 1900. 1833. 1834. 1835. 1836. 1837. 1838. 1839, Birmingham 1840. 1841. 1842. 1843. 1844. 1845. 1846. 1847. Oxford 1848. 1849 Birmingham | Manchester Newcastle- | upon-Tyne, Leeds Cardiff ......| Edinburgh Nottingham Oxford :..... Ipswich .. Liverpool... Toronto PSTISUO! senses 'Lieut.-Col. Sir R. Lambert |H. Seebohm, Sec. B.8., F.L.S., 'Major L. Darwin, Sec. R.G.S. ... J. Scott-Keltie, LL.D. Presidents Col. Sir C. Warren, R.E., G.C.M.G., F.B.S., F.R.G.S. Col. Sir C. W. Wilson, R.E., K0.B:, FBS. E:R:G:S. Col. Sir F. de Winton, K.C.M.G., C.B., F.B.G.8. Playfair, K.C.M.G., F.R.G.S. E. G. Ravenstein, ¥. R.G.S8., F.S.8. Prof, J. Geikie, D.C.L., F.B.S., | V.P.R.Scot.G.s. F.Z.8. Capt. W.J. L. Wharton, R.N., F.R.S. Mackinder, ; M.A., F.B.G.S. Col. G. Earl Church, F.R.G.S. Bradford .. Cambridge Edinburgh Dublin Bristol sbeeee Liverpool... Newcastle Glasgow ... Plymouth... Manchester eee eeneee Cambridge Southamp- ton. eeeeee Swansea .., \Sir John Murray, F.R.8. .|Sir George §. Robertson, | Rt. Hon. Lord Sandon /Rt. Hon, Lord Sandon, M.P., \Lieut.-Col. Sykes, F.R.S....... iG. W. Wood, M.P., F.LS. ... | Lieut. - Col. K.C.8.1. Rev. L. C. Casartelli, J. 8. Keltie, H. J. Mackinder, E. G. Ravenstein J. S. Keltie, H. J. Mackinder, E. G. Ravenstein, J. S. Keltie, H. J. Mackinder, R. Sulivan, A. Silva White, |A. Barker, John Coles, J. 8. Keltie, A. Silva White, John Coles, J. 8. Keltie, H. J. Mac- kinder, A. Silva White, Dr. Yeats. J. G. Bartholomew, John Coles, J. 8. Keltie, A. Silva White. Col. F. Bailey, John Coles, H. O. Forbes, Dr. H. R. Mill. John Coles, W. 8. Dalgleish, H. N. Dickson, Dr. H. R. Mill. John Coles, H. N. Dickson, Dr. H. R. Mill, W. A. Taylor. Col. F. Bailey, H. N. Dickson, Dr. H. R. Mill, E. C. DuB. Phillips. Col. F. Bailey, Capt. Deville, Dr. H. R. Mill, J. B. Tyrrell. H.N. Dickson, Dr. H. R. Mill, H. C. Trapnell. H. N. Dickson, Dr. H. O. Forbes, Dr. H. R. Mill. H. N. Dickson, E. Heawood, E. R. Wethey. STATISTICAL SCIENCE. COMMITTEE OF SCIENCES, VI.—STATISTICS. Prof. Babbage, F’.R.S. ...... Sir Charles Lemon, Bart....... SECTION F.—STATI Charles Babbage, F.R.S. . Sir Chas. Lemon, Bart., F. R. Ss. eee eeeeee Colonel Sykes, F.R.S. ........ Henry Hallam, F.R.S....... F.R.S. Sir C. Lemon, Bart., M.P, Sykes, F.RB.S., F.L.S. Rt. Hon. the Earl Fitzwilliam Garb BEOLeT aN Ris. scasthenence Travers Twiss, D.C.L., F.R.S. J. H. Vivian, M.P., F.B.S. ... Rt. Hon. Lord Lyttelton...... ...(Jd. E, Drinkwater. Dr. Cleland, C. Hope Maclean. STICS, .|W. Greg, Prof. Longfield. Rev. J. E. Bromby, C. B. Fripp, James Heywood. W. BR. Greg, W. Langton, Dr. W. C. Tayler. .| W. Cargill, J. Heywood, W. R. Wood. .|F, Clarke, R. W. Rawson, Dr. W. C. Tayler. C. R. Baird, Prof, Ramsay, R. W. Rawson. Rey. Dr. Byrth, Rev. R, Luney, R. W. Rawson. Rev. R. Luney, G. W. Ormerod, Dr. W. C. Tayler. ...|Dr. D. Bullen, Dr. W. Cooke Tayler. J. Fletcher, J. Heywood, Dr. Lay- cock. ! J. Fletcher, Dr. W. Cooke Tayler. J. Fletcher, F. G, P. Neison, Dr. W. C. Tayler, Rev. T. L. Shapcott. Rev. W. H. Cox, J. J. Danson, F. G. P. Neison. J. Fletcher, Capt, R. Shortrede. Dr. Finch, Prof, Hancock, F, G. P. Neison. PRESIDENTS AND SECRETARIES OF THE SECTIONS. lxv Date and Place Presidents 1850. Edinburgh 1851. Ipswich ... 1852. Belfast...... 1858. Hull 1854. Liverpool,,. 1855. Glasgow ... Secretaries Very Rev. Dr. John Lee,|Prof. Hancock, J. Fletcher, Dr. J. V.P.R.S.E. Stark. Sir John P, Boileau, Bart. ...|J. Fletcher, Prof. Hancock. His Grace the Archbishop of | Prof. Hancock, Prof. Ingram, James Dublin. MacAdam, jun. James Heywood, M.P., F.R.S.| Edward Cheshire, W. Newmarch. Thomas Tooke, F.R.S. .........|H. Cheshire, J. T. Danson, Dr. W. H. Duncan, W. Newmarch. R. Monckton Milnes, M,P. ... | J, A. Campbell, E. Cheshire, W. New- march, Prof. R. H. Walsh. SECTION F (continued),—ECONOMIC SCIENCE AND STATISTICS. 1856. Cheltenham 1857. Dublin 1858. Leeds . eeeee 1859. Aberdeen... 1860. Oxford 1861, Manchester 1862. Cambridge 1863. Newcastle 1864. Bath......... 1865, Birmingham 1866. Nottingham 1867. Dundee feces 1868. Norwich.... 1869. Exeter 1870. Liverpool... 1871, Edinburgh 1872. Brighton... 1873, Bradford ... 1874. Belfast...... 1875. Bristol 1876. Glasgow ... 1877. Plymouth... 1878. Dublin...... 1879. Sheffield ... 1880. Swansea ... 1881. York......... Rt. Hon, Lord Stanley, M.P. , His Grace the Archbishop of Dublin, M.R.LA. Edward Baines......... caneeeel Col. Sykes, M.P., F.R.S. ...... Nassau W. Senior, M.A. ...... William Newmarch, F.R.S.... Edwin Chadwick, O©.B. ........ -| William Tite, M.P., F.R.S.... W. Farr, M.D., D.C.L., F.RB.S. Rt. Hon. Lord Stanley, LL.D., M.P. Prof. J. E. T. Rogers eee eeewesene M. EH. Grant-Duff, M.P. ....... Samuel Brown. .....se.sccosseees Rt. Hon. Sir Stafford H. North- cote, Bart., C.B., M.P. Prof. W. Stanley Jevons, M.A. Rt. Hon. Lord Neaves......... Prof. Henry Fawcett, M.P.... Rt. Hon. W. E. Forster, M.P. Lord) O7Hagar. f....vee.ctswenes James Heywood, M.A.,F.R.S., Pres. 8.8. Sir George Campbell, K.C.S.L., M.P. Rev. C. H. Bromby, E. Cheshire, Dr. W. N. Hancock, W. Newmarch, W. M. Tartt. Prof. Cairns, Dr. H. D. Hutton, W. Newmarch. T. B. Baines, Prof. Cairns, S. Brown, Capt. Fishbourne, Dr. J. Strang. Prof. Cairns, Edmund Macrory, A. M, Smith, Dr. John Strang. Edmund Macrory, W. Newmarch, Prof. J. E. T. Rogers. David Chadwick, Prof. R. C. Christie, H. Macrory, Prof. J. E. T. Rogers. ° H. D. Macleod, Edmund Macrory. T. Doubleday, Edmund Macrory, Frederick Purdy, James Potts. E. Macrory, E. T. Payne, F. Purdy. G. J. D. Goodman, G. J. Johnston E. Macrory. R. Birkin, jun., Prof. Leone Levi, E Macrory. Prof. Leone Levi, E. Macrory, A. J. Warden. Rev. W. C. Davie, Prof. Leone Levi. E. Macrory, F. Purdy, C. T. D. Acland. Chas. R. Dudley Baxter, E. Macrory. J. Miles Moss. J. G. Fitch, James Meikle. J. G. Fitch, Barclay Phillips. J. G. Fitch, Swire Smith. Prof. Donnell, F. P. Fellows, Hans MacMordie. F. P. Fellows, T. G. P. Hallett, E. Macrory. M‘Neel Caird, T.G. P. Hallett, Dr. W. Neilson Hancock, Dr. W. Jack. A. 882. Southamp- ton. 1900. Rt. Hon, the Earl Fortescue |W. F. Collier, P. Hallett, J. T. Pim. Prof. J. K. Ingram, LL.D. |W. J. Hancock, C. Molloy, J. T. Pim. G. Shaw Lefevre, M.P., Pres.|Prof. Adamson, R. E. Leader, C. 8.8. Molloy. G. W. Hastings, M.P........... N, A. Humphreys, C. Molloy. Rt. Hon. M. E. Grant-Duff,|C. Molloy, W. W. Morrell, J. F. M.A., F.R.S. Moss. Rt. Hon. G. Sclater-Booth,|G. Baden-Powell, Prof. H. 8. Iox- M.P., F.R.S, well, A. Milnes, C. Molloy. Ixvi Date and Place 1883. 1884. 1885. 1886. 1887. 1888. 1889. 1890. 1891, 1892. 1893. 1894, 1895. 1896. 1897. 1898. 1899. 1900. 1836. 1837. 1838. 1839. Birmingham | 1840. 1841. 1842. 1843. 1844. 1845. 1846, 1847. 1848, 1849, 1850. Southport Montreal ... Aberdeen... | Birmingham | nEPoRT— |) Presidents R. H. Inglis Palgrave, F.R.8. G.C.8.1., C.LE., F.R.G.S. |Prof. H. Sidgwick, ULL.D., Litt.D. J. B. Martin, M.A., F.S.S. 0, Secretaries ‘Rev. W. Cunningham, Prof. H. §. Foxwell, J. N. Keynes, C. Molloy. ‘Sir Richard Temple, Batt,| Prof. H. 8. Foxwell, J. 8. McLennan, | Prof. J. Watson. Rev. W. Cunningham, Prof. H. §. Foxwell, C. McCombie, J. F. Moss. I’, F. Barham, Rev. W. Cunningham, Prof. H. 8. Foxwell, J. F. Moss. Manchester | Robert Giffen, LL.D.,V.P.S.8. Rev. W. Cunningham, F. Y. Edge- BALD ecco ees Newcastle- upon-Tyne Leeds waeeee Edinburgh Rt. Hon. Lord Bramwell, DID D A a ase Prof. F. Y. Edgeworth, M.A., F.S.8, Prof, A. Marshall, M.A., F.{5.S. Prof. W. Cunningham, D.D., D.8c., F.8.8. Hon. Sir C. W. Fremantle, K:C.B, worth, T. H. Elliott, C. Hughes | J. E.C. Munro, G, H. Sargant. Prof. F. Y. Edgeworth, T. H. Elliott, H. S. Foxwell, L. L. F. R. Price. Rev. Dr. Cunningham, T. H. Elliott, | F.B. Jevons, L. L. F. R. Price. W. A. Brigg, Rev. Dr. Cunningham, T. H. Elliott, Prof. J. E. C. Munro, L. L. F. Ri Price. Prof. J. Brough, E. Cannan, Prof. E. Cc. K. Gonner, H. Ll. Smith, Prof. W. R. Sorley. Prof. J. Brough, J. R. Findlay, Prof. | KE. ©. K. Gonner, H. Higgs, | L, L. FR. Price. Nottingham Prof. J. 8. Nicholson, D.Sc.,, Prof. E. C. K. Gonner, H. de B. F.8.8. Gibbins, J. A. H. Green, H. Higgs, | le DL. RPrice, Oxford...... Prof. C. F. Bastable, M.A.,|E. Cannan, Prof. E. C. K. Gonner, | F.S.8. | W.A.S. Hewins, H. Higgs. Tpswioh: .s.| i. Pricey IMiA.. t0i...t..2 |E. Cannan, Prof. EH. C. K. Gonner, f | H. Higgs. Liverpool...|Rt. Hon. L. Courtney, M.P.....E. Cannan, Prof. E. C. K. Gonner, | W. ..|P. Le Neve Foster, Robert Pitt, P. Le Neve Foster, Henry Lea, W. P. Marshall, Walter May. P. Le Neve Foster, J. F. Iselin, M, O. Tarbotton. P. Le Neve Foster, John P. Smith, W. W. Urquhart. P. Le Neve Foster, J. F. Iselin, ©. Manby, W. Smith. .|P. Le Neve Foster, H. Bauerman. H. Bauerman, P. Le Neve Foster, T, King, J. N. Shoolbred. | HI. Bauerman, A. Leslie, J. P. Smith. H. M. Brunel, P. Le Neve Foster, J.G. Gamble, J. N. Shoolbred. C.Barlow,H.Bauerman. E.H.Carbutt, | J.C. Hawkshaw, J. N. Shoolbred. A. T. Atchison, J. N.Shoolbred, John Smyth, jun. W. R. Browne, H. M. Brunel, J. G. Gamble, J. N. Shoolbred. W. Bottomley, jun., W. J. Millar, J. N. Shoolbred, J. P. Smith. .|A. T. Atchison, Dr. Merrifield, J. N. Shoolbred. A. T. Atchison, R. G. Symes, H. T Wood. A. T. Atchison, Emerson Bainbridge H. T. Wood. A. T. Atchison, H. T. Wood. A. T. Atchison, J. F. Stephenson, H. T. Wood. ...(|A. i Atchison, F Churton, H. T. Wood. A. T. Atchison, E. Rigg, H. T. Wood. A. T. Atchison, W. B. Dawson, J. Kennedy, H. T. Wood. .|A. T. Atchison, F. G. Ogilvie, E. Rigg, J. N. Shoolbred. C. W. Cooke, J. Kenward, W. B, Marshall, E. Rigg. d2 Ixvili rePort——1900, Date and Place 1887. Manchester 1888. Bath Newcastle- upon-Tyne 1890. Leeds 1889. 1891, Cardiff ...... 1892. Edinburgh 1893. Nottingham 1894, Oxford...... 1895. Ipswich 1896, Liverpool... 1897. Toronto 1898. Bristol weteee 1899. Dover 1900, Bradford ... 1884. Montreal... 1885. Aberdeen... 1886. Birmingham | 1887. Manchester 1888. Bath 1889. Newcastle- upon-Tyne 1890. Leeds 1891. Cardiff...... 1892. Edinburgh 1893. Nottingham 1894. Oxford...... 1895. Ipswich .. 1896. Liverpool... 1897. Toronto see ee ween na Mevore, 1 dae Presidents Secretaries LL.D., F.B.S. a Preece, M.Inst.C.E. W. Anderson, M.Inst.C.E. .. WwW. Capt. A. Noble, C.B., F.R.S., F.R.A.S. Prof. W. M.Inst.C.B. F.C.S8. F.R.S., M.Inst.C.E. M.A., M.Inst.C.E. ...|G@. F, Deacon, M.Inst.C.E. Sir J. Wolfe-Barry, K.C.B., F.R.S. Sir W. White, K.C.B., F.R.S. Prof. Osborne Reynolds, M.A., F.RS., T, Forster Brown, M.Inst.C.. C. Unwin, F.RBS., Jeremiah Head, M.Inst.C.E., Prof. A. B. W. Kennedy, Vernon-Harcourt, Sir Douglas Fox, V.P.Inst.C.E, C. F. Budenberg, W. B. Marshall, K. Rige. C. W. Cooke, W. B. Rigg, P. K. Stothert. .|C. W. Cooke, W. B. Marshall, Hon. C. A, Parsons, E. Rigg E. K. Clark, C. W. Cooke, W. B. Marshall, E. Rigg. Cc. W. Cooke, Prof. A. C, Elliott, W. B. Marshall, E. Rigg. C. W. Cooke, W. B. Marshall, W. C, Popplewell, E. Rigg. C. W. Cooke, W. B. Marshall, E, Rigg, H. Talbot. Prof. T. Hudson Beare, C. W. Cooke, W. B. Marshall, Rev. F. J. Smith. Prof. T. Hudson Beare, C. W. Cooke, W. B. Marshall, P. G. M. Stoney. Prof. T. Hudson Beare, C. W. Cooke, S. Dunkerley, W. B. Marshall, Prof. T. Hudson Beare, Prof. Callen- dar, W. A. Price. Prof. T. H. Beare, Prof. J. Munro, H. W. Pearson, W. A. Price. Prof. T. H. Beare, W. A. Price, H, E. Stilgoe. Marshall, E. Sir Alex. R. Binnie, M.Inst. C.E. Prof. T. H. Beare, C. F, Charnock, Prof. S. Dunkerley, W. A. Price. SECTION H.—ANTHROPOLOGY. E. B. Tylor, D.C.L., F.B.S. ... Francis Galton, M.A., F.R.S. Sir G. Campbell, M.P., D.C.L., F.R.G.S. Lieut.-General D.C.L., F.R.S. LL.D., F.R.S. Dr. J. Evans, Treas. F.S.A., F.L.S., F.G.S. Prof. A. Macalister, M.D., F.B.S. Sir W. F.R.S. H. Flower, K.C.8.1L, Prof, A. H, Sayce, M.A. ....... Pitt-Rivers, Prof. Sir W. Turner, M.B., BS., Prof, F. Max Miiller, M.A. ... M.A., Dr, R. Munro, M.A., F.R.S.E. K.C.B,, G. W. Bloxam, W. Hurst. |G. W. Bloxam, Dr. J. G. Garson, W. Hurst, Dr. A. Macgregor. G. W. Bloxam, Dr. J. G. Garson, W. Hurst, Dr. R, Saundby. G. W. Bloxam, Dr. J. G. Garson, Dr. A. M. Paterson. G. W. Bloxam, Dr. J. G. Garson, J. Harris Stone. G. W. Bloxam, Dr. J. G. Garson, Dr, R. Morison, Dr. R. Howden. G. W. Bloxam, Dr. C. M. Chadwick, Dr. J. G. Garson. G. W. Bloxam, Prof. R. Howden, H, Ling Roth, E. Seward. G. W. Bloxam, Dr. D. Hepburn, Prof, R. Howden, H. Ling Roth. G. W. Bloxam, Rev. T. W. Davies, - Prof. R. Howden, F, B. Jevons, J. L. Myres. H. Balfour, Dr. J. G.Garson, H. Ling Roth, .|Prof. W. M. Flinders Petrie,/J. L. Myres, Rev. J. J. Raven, H, D.C.L Arthur i Evans, F.S.A. .....+ +» }Sir W. Turmer, F.R.S. ..,...06. Ling Roth. Prof. A. C. Haddon, J. L. Myres, Prof. A. M. Paterson. A. F. Chamberlain, H. 0, Forbes, Prof, A. C, Haddon, J, ly. Myres, LIST OF EVENING DISCOURSES. lxix Date and Place | Presidents Secretaries as ees See er | 1898. Bristol...... |i. W. Brabrook, O.B. .... ....|H. Balfour, J. L. Myres, G. Parker. 1899. Dover ...... |C. H. Read, F.S.A. |H. Balfour, W. H. East, Prof. A. C. | | Haddon, J. L. Myres. 1900. Bradford .. ake John Rhys, M.A..........) i Rev. E. Armitage, H. Balfour, W. 1894, 1896. 1897. 1899. 1895. 1896. | Crooke, J. L. Myres. SECTION I.—PHYSIOLOGY (including ExprrimEentrAL ParHoLoGy AND ExPERIMENTAL PsycHoLoGy). Oxford......|Prof. E. A. Schiifer, F.R.S.,| Prof. ¥. Gotch, Dr. J. 8. Haldane, M.R.C.S. | M.S. Pembrey. Liverpool...| Dr. W. H. Gaskell, F.R.S |Bx of. R. Boyce, Prof. C.S. Sherrington. Yoronto ...|Prof. Michael Foster, F.R.S. | Prof. R. Boyce, Prof. C. 8. Sherring- | ton, Dr, L. EH. Shore. Dover ..:... J. N. Langley, F.L.8. | Dr. Howden, Dr. L. E. Shore, Dr. E. H, Starling. SECTION K.—BOTANY. Ipswich ...|W. T. Thiselton-Dyer, F.R.S.|A. C. Seward, Prof. F. E. Weiss. Liverpool... Dr. D, H. Scott, F.R.S. ...... ‘Prof. Harvey Gibson, A. C. Seward, | | Prof. F. H. Weiss. 1897. Toronto ... Prof. Marshall Ward, F.R.S. Prof. J. B. Farmer, BH. C. Jeffrey, | | A. C. Seward, Prof. F. E. Weiss. 1898. Bristol......| Prof. I. O. Bower, F.R.8. ws [AL C, Seward, H. Wager, J. W. White. 1899. Dover ...... Sir George King, F.R.S. ......;G. Dowker, A. C. Seward, H. Wager. 1900. Bradford ...| Prof. 8. H. Vines, E.RS... we. C. Seward, H. Wager, W. West. LIST OF EVENING DISCOURSES. Date and Place Lecturer Subject of Discourse 1842. Manchester | Charles Vignoles, F.R.S...... |The Principles and Construction of Atmospheric Railways. SingMy, Te Brunely ‘...5cerectacdes The Thames Tunnel. R. I. Murchison...........s00e00e The Geology of Russia. 1843, Cork ......... Prof, Owen, M.D., F.R.S.......| The Dinornis of New Zealand. Prof. E. Forbes, F.R.S..........| The Distribution of Animal Life in the Aigean Sea. Dr. RobinsOn.........02.cceeeeeees The Karl of Rosse’s Telescope. 1844. York......... Charles Lyell, F.R.S. .........|Geology of North America. Dr. Falconer, F.R.S.......00008+ The Gigantic Tortoise of the Siwalik Hills in India. 1845. Cambridge | G.B.Airy,F.R.S.,Astron.Royal} Progress of Terrestrial Magnetism. 1846, 1847, R. I. Murchison, F.R.S. ......|Geology of Russia. Southamp- | Prof. Owen, M.D., F.R.S. ...| Fossil Mammaliaof the British Isles. ton, Charles Lyell, F.R.S. .........| Valley and Delta of the Mississippi. W. R. Grove, F.R.S........0.06+ Properties of the ExplosiveSubstance discovered by Dr. Schénbein; also some itesearches of his own on the Decomposition of Water by Heat. Oxford......] Rev. Prof. B. Powell, F.R.S. |Shooting Stars. Prof. M. Faraday, F.R.S.......| Magnetic and Diamagnetic Pheno- mena. Hugh E. Strickland, F,G.5....|The Dodo (Didus ineptus), lxx REPORT—1900. Date and Place Lecturer Subject of Discourse 1848. Swansea ...|John Percy, M.D., F.R.S....... Metallurgical Operationsof Swansea | and its Neighbourhood. 'W. Carpenter, M.D., F.R.S....|Recent Microscopical Discoveries. 1849. Birmingham| Dr. Haraday, Has. c.ccse-cese Mr. Gassiot’s Battery. |Rev. Prof. Willis, M.A., F.R.S.|Transit of different Weights with | varying Velocities on Railways. 1850. Edinburgh Prof. J. H. Bennett, M.D.,|Passage of the Blood through the | F.R.S.E. minute vesselsof Animals in con- nection with Nutrition. Dr. Mantel, HiRiSa: sicasss spas Extinct Birds of New Zealand. 1851. Ipswich ...|Prof. R. Owen, M.D., F.R.S. |Distinction between Plants and | Animals, and their changes of | Form. G.B.Airy,F.R.S.,Astron. Royal | Total Solar Eclipse of July 28, 1851. 1852. Belfast...... Prof. G. G. Stokes, D.C.L.,| Recent Discoveries in the properties F.R.S. of Light. |Colonel Portlock, R.E., F.R.S.|Recent Discovery of Rock-salt at Carrickfergus, and geological and practical considerations connected with it. 1853. Hull.........|Prof.J. Phillips, LL.D.,F.R.S.,|Some peculiar Phenomena in the F.G.S. Geology and Physical Geography of Yorkshire. Robert Hunt, F.B,S.......00008. The present state of Photography. 1854, Liverpool...) Prof. R. Owen, M.D., F.R.S. |Anthropomorphous Apes. Col. E. Sabine, V.P.R.S. ......| Progressof Researches in Terrestrial Magnetism. 1855. Glasgow ...| Dr. W. B. Carpenter, F.R.S. |Characters of Species. Lieut.-Col. H. Rawlinson ...| Assyrian and Babylonian Antiquities and Ethnology. 1856. Cheltenham) Col. Sir H. Rawlinson ......... Recent Discoveries in Assyria and Babylonia, with the results of Cuneiform Research up to the present time. | Wi, Grove; ER :Ss..scdesesscescusasbeanswecnnea 538 0 O Daler adler NICKELS unui vesesdcisececbescsaccavbecechac=seeerasbed 120 0 0 BALE OL PEMD CAULONS, feapaaelas nv aepdeuie 14 0enoen= denpegnidonn ash arcses *Roscoe, Sir H. E.—Wave-length Tables “See ee eee *Miers, Professor H. A.—Isomorphous Sulphonic Derivatives SU SUZOUE | .cidcclcs dues oO e(dvs ce sua e's sntetiadddsaeensasnenenssnests sae Geology. *Marr, Mr. J, E.—Erratic Blocks (£6 in hand)............s004+ *Geikie, Professor J.—Photographs of Geological Interest PL an EE is ve tiiimeke aed scons ton homaeautandnga sd qailds sGgialsay *Marr, Mr. J. E.—Life-zones in British Carboniferous Rocks *Lloyd-Morgan, Professor C.—Ossiferous Caves at Uphill RATEMOWED). .oe.css esses wcsadanenddewes-sunereenaqsiasveescwneseeasensiehe *Watts, Professor W. W.—Underground Water of North- WeSE NV OFESNIPG oie. 0 565 cececcecccoc sco sensenceseansteredasessesss *Scharff, Dr.—-Exploration of Irish Caves (renewed)............ Zoology. *Herdman, Professor W. A.—Table at the Zoological Station, MEADOR wn diode dessins fete Raids sve sivuis on aueida aCe eae aie Beaman *Bourne, Mr. G. C.—Table at the Biological Laboratory, ARURROME | Se veyciesccccasiacctss ss see 0nedeeqme spcamenaneasmncenmare BAND IVAD TAD eee eho eases cae es bcos a « uo cra loncemeleumeemeamaceissesciess Geography. Keltie, Dr. J. Scott—Terrestrial Surface Waves ..........++008 ae a H. R.—Changes of Land-level in the Phlegrzan 1€. Ss SOCCER H Oe HHH EHR EHHR HHS EHH SOH EHH SHH HHH SHH EHH SEE EEE Ee eeoeeveee Economic Science and Statistics. *Giffen, Sir R.—State Monopolies in other Countries GOP PomeGe in Nand) sscss0--.s0.esjcenetiaeteernen ane ncscneues Brabrook, E. W.—Legislation regulating Women’s Labour Game US CARO ATU ssi as. osacav eateeeeererissavictcauce O00 0 ** Reappointed. 1900. £ 8. 45 0O 75 O 10 O 5 0 35 «(0 20 O 5 0 50 O 15 0 100 0O 20 0 Toun0 10 O 50 50 O 15 0 f o cok n= SS = Kets eS o!1o xcviil REPORT—1900, Bi Brought Forward) caisiascivessodeesedssscanseeccscouassisensea eds (OGMED oft Mechanical Science. *Preece, Sir W. H.—Small Screw Gauge (balance in handand) 45 0 0 Binnie, Sir A.—Resistance of Road Vehicles to Traction ... 75 O O Anthropology. *Evans, Mr. A. J.—Silchester Excavation ....... ssujaee Bete *Penhallow, Professor D, P.—Ethnological Survey of Canada 30 0 0 *Garson, Dr. J. G.—Age of Stone Cir cles (balance in hand)... —— *Read, Mr. C. H.—Photographs of Anthropological Interest MeO AARP) 22. 225 nina anonnarte eee eet e acs Saat eee eee — *Tylor, Professor E. B.—Anthropological Teaching ............ 5 0 0 Evans, Sir John—Exploration in Crete. ..........00...e000001- 145 0 0 Physiology. *Schafer, Professor E. A.—Physiological Effects of Peptone... 30 0 0 Schafer, Professor E. A.—Chemistry of Bone Marrow ...... 15 0 0 Starling, Professor E. H.—Suprarenal Capsulesinthe Rabbit 5 0 0 Botany. *Farmer, Professor J. B.—Fertilisation in Pheophycee ...... DS Si a U) Marshall Ward, Professor—Morphology, Ecology, and Taxo- nomy of Podostemagesd 2.) Je Uhe, 0 wate atid EEE 20; 0° 0 Corresponding Societies, *Whitaker, Mr. W.—Preparation of Report .........sssceseeeees 15 0 0 £945 0 0 * Reappointed. The Annual Meeting in 1901. The Annual Meeting of the Association in 1901 will be held at Glasgow, commencing on : September 11. ‘ The Annual Meeting in 1902. The Annual Meeting of the Association in 1902 will he held at Belfast. GENERAL STATEMENT, Xclx General Statement of Sums which have been paid on account of Grants for Scientific Purposes 1834, £ 8. d. Tide Discussions ...... Seatanene 20 0 0 1835. Tide Discussions ........+.+e+++ 62 0 0 British Fossil Ichthyology .:. 105 0 0 £167 V0 O 1836. Tide Discussions .........s0+0++ 163 0 0 British Fossil Ichthyology ... 105 0 0 Thermometric Observations, REGoEeeaedenscxescresaresseesassiecs 50 0 0 Experiments on Long-con- tinued Heat ........ceeeeseuee Viger 30) Rain-Gauges .........scecsseeves 9 13, 0 Refraction Experiments ...... ED AO Lunar Nutation.............00+0+ 60 S050 Thermometers ......seeeeeeeeeee aeson 10 £435 0 0 1837. Tide Discussions .........ssse0e 284 1 0 Chemical Constants ............ 2413 6 Lunar Nutation.............60. 70 0 0 Observations on Waves ...... 100 12 0 Tides at Bristol .........-+-..00+. 150 0 0 Meteorology and Subterra- nean Temperature............ 93 3 0 Vitrification Experiments 150 0 0 Heart Experiments ............ a Barometric Observations ...... 30 0 0 IBALOMEEELS... 6... ..esecenscees aise leo 76 £922 12 6 1838. Tide Discussions ..........0000+ ZO 0 British Fossil Fishes............ 100 0 0 Meteorological Observations and Anemometer (construc- TORII ea vonessecs csccsascsacavavae 100 0 O Cast Iron (Strength of) ...... 60 0 0 Animal and Vegetable Sub- stances (Preservation of)... 19 1 10 Railway Constants ............ 41 12 10 PSTISEOMS LICE! i ceccasessescseeese 50 0 O Growth of Plants .............++ 75 0 O Mud in Rivers ............se00e Sie ees: Education Committee ......... 50) 0 0 - Heart Experiments ......... socisoe Jaen ama Land and Sea Level............ 267 8)” 7 Steam-vessels...............0se00e 100 0 0 Meteorological Committee oly 9! 5 £932 2 2 1839. £ 8. d. Fossil Ichthyology ........0+0 110 0 0 Meteorological Observations at. Plymouth, &. .........006 63 10 0 Mechanism of Waves ......... 144 2 0 Bristol, Dided xecasestcsadscd.coscns 35 18 6 Meteorology and Subterra- nean Temperature............ 2111 O Vitrification Experiments ... 9 4 0 Cast-iron Experiments......... 103 0 7 Railway Constants ............ 28 7 0 Land and Sea Level............ 274 1 2 Steam-vessels’ Engines ...... 100 0 4 Stars in Histoire Céleste ...... 171 18 0 Stars in Lacaille ..c..s0cscesee 11 0 6 Stars in R.A.S. Catalogue 166 16 0O Animal Secretions............. - 1010 6 Steam Engines in Cornwall... 50 0 0 Atmospheric Air ........seseeee 1461 0 Cast and Wrought Iron ...... 40 0 0 Heat on Organic Bodies ...... 38 0 0 Gases on Solar Spectrum...... 22 0 0 Hourly Meteorological Ob- servations, Inverness and KINGUSSTE Mivasasceseoatebwe eve 49 7 8 Fossil Reptiles. .......sscsesesecs 118 2) 9 Mining Statistics ............00- 50 0 0 £1595 11 0 1840. BrIshOlMMGeseeescaxcessarses eevee 100 0 0 Subterranean Temperature... 13 13 6 Heart Experiments .......... 18 19 0 Lungs Experiments ............ 813 0 Tide Discussions .........es«»s. 50 0 O Land and Sea Level....... aseenP pOnguk odd Stars (Histoire Céleste) ...... 242 10 O Stars (Lacaille) .............. wetein ea ID 3 O Stars (Catalogue) ......ssccsee 264 0 0 AtMOSPHELICEAUT (ie. ssnsmaseneve 15 15 0 ‘Water oneinany (2c. nhisvicasaes 10 0 0 Heat on Organic Bodies ...... 7 0 0 Meteorological Observations. 52 17 6 Foreign Scientific Memoirs... 112 1 6 Working Population............ 100 0 0 School Statistics .........se000. 50 0 0 Forms of Vessels .........000.0. 184 7 0 Chemical and Electrical Phe- TOO Wt eee sede a oa ncie cactenans 40 0 0 Meteorological Observations Be IVIMOUGH <5. ccccacsescanses 80 0 0 Magnetical Observations...... 185 13 9 £1546 16 4 eee BB é REPORT—1900. 1841. ; £8. a. Observations on Waves ...... 30 0 0 Meteorology and Subterra- nean Temperature............ 8 8 OQ ACtINOMETHETS ........cccceceerecee 10 0 O Earthquake Shocks ....0s...00+ We 6 {0 Acrid POiSONS......s.cececseeeeeee 6 0 0 Veins and Absorbents ......... 3.0 «0 Mud in Rivers ....sessssescesees 5. 10.70 Marine Zoology .....seccsesseeeee 1512 8 Skeleton Maps .......-.scseeeeee 207,10: 40 Mountain Barometers ......... 618 6 Stars (Histoire Céleste) ...... 185 0 0 Stars (Lacaille)...........:.+000« (car © Stars (Nomenclature of) ...... 1719 6 Stars (Catalogue of) ............ 40 0 0 Water on Tron .......e.esesenee 50 0 0 Meteorological Observations ab IMVETNESS ......0...00000e8 20 0 0 Meteorological Observations (reduction Of) ......seeeeeeee 25 0 0 Fossil Reptiles .........ceeeseeee 50 0 0 Foreign Memoirs ........ 62 0 6 Railway Sections ............. Saco IE 0 Forms of Vessels .....cscsseeees 193 12 0 Meteorological Observations Bt Plymouth cieiseawerersosee 55 0 0 Maenetical Observations...... 6118 8 Fishes of the Old Red Sand- BEONE E Pepaathacaccranstccegnsemen 100 0 O Midesiat Meith: ......ccs..se-ess 50 0 O Anemometer at Edinburgh... 69 1 10 Tabulating Observations ...... OG as Races Of Men........cccccsseceses 5 0 0 Radiate Animals ............ dc} ee weO £1235 10 11 1842. Dynamometric Instruments.. 113 11 2 Anoplura Britanniz ......... soo O02) 12NO Tides at Bristol ...........e0006. Ys) (0) Gases on Light ...-..seseseeeeee 30 14 7 Chronometers......seeseecseeeees 2617 6 Marine Zoology.........sessseeee 1) 8b") British Fossil Mammalia...... 100 0 O Statistics of Education......... 20 0 O Marine Steam-vessels’ En- FINES ..reeserererescaccensereres 28 0 0 Stars (Histoire Céleste) ...... Bo 10h 20 Stars (Brit. Assoc. Cat. of)... 110 0 0 Railway Sections ...........66 161 10 0 British Belemnites ............ 50 0 0 Fossil Reptiles (publication Of Report) .....scssescseeeseeee 210 0 0 Forms of Vessels .......sesee00 180 0 0 Galvanic Experiments on RGtisee ates ceverecsscacnecncases 5 oeab Meteorological Experiments at Plymouth .....,..-sse00. 68) (070 Constant Indicator and Dyna- strane 90 0 0 mometric Instruments © 3 Force of Wind ..s.cccssssecsevee 10 Light on Growth of Seeds ... 8 Vital Statistics .........ss0+0 « 50 Vegetative Power of Seeds... 8 Questions on Human Race... 7 £1449 1843. Revision of the Nomenclature OLS SUANSD cosaseicsceameeateer cette 2 Reduction of Stars, British Association Catalogue ...... 25 Anomalous Tides, Firth of HM OLLM yoeemersisesstencausreesceee 120 Hourly Meteorological Obser- vations at Kingussie and ITiV CENESS Bias scea senses aeons 77 Meteorological Observations abvelym Oubhn aeescsnesatseseese 55 Whewell’s Meteorological Ane- mometer at Plymouth ...... 10 Meteorological Observations, Osler’s Anemometer at Ply- THOUGD Sec rsescetessne stesso 20 Reduction of Meteorological ODServations: ...csc0....-200000 30 Meteorological Instruments andl (Gratuities sesnp.seeenees 39 Construction of Anemometer AL ANVEXNGSS© \eccnesettbione sane 56 Magnetic Co-operation......... 10 Meteorological Recorder for Kew Observatory .......0ss0« 50 Action of Gases on Light...... 18 Establishment at Kew Ob- servatory, Wages, Repairs, Furniture, and Sundries... 133 Experiments by Captive Bal- HOODS): evesteesssieeeacaserassats 81 Oxidation of the Rails of (Rail WaySics.sescencnomess caren 20 Publication of Report on Fossil Reptiles .............4 40 Coloured Drawings of Rail- Way SECbiONS .....s0..-s0cen 147 Registration of Earthquake OCG sere ersneneuckessacee aren 30 Report on Zoological Nomen CLAD UNE tween cwseesameseaapeeeaem 10 Uncovering Lower Red Sand- stone near Manchester...... 4 Vegetative Power of Seeds... 5 Marine Testacea (Habits of). 10 Marine Zoology ......cescseeseess 10 Marine Zoology cisccssssessscenss 2 Preparation of Report on Bri- tish Fossil Mammalia ...... 100 Physiological Operations of Medicinal Agents .........4 . 20 Vital Statistics .......0seecece. 36 s d. 0 0 0 O 0 0 iy 9 0 Lo 8 0 0 0 0 0 0 12 8 0 0 OO 0 0 0 0 6 0 12 2 8 10 0 0 16 1 4 7 8 0 0 0 0 0 18 3 0 0 0 0 4 6 3 8 0 0 0 0 14 11 0 0 0 0 5 8 GENERAL STATEMENT. £ 8 d. Additional Experiments on the Forms of Vessels ...... 70 0 0 Additional Experiments on the Forms of Vessels ...... 100 0 0 Reduction of Experiments on the Forms of Vessels ...... 100 0 0 Morin’s Instrument and Con- Stans INGICAtOY ..2..ccesseocre 69 14 10 Experiments on the Strength OL Maberigls) sescccscscesesese 60 0 0 £1565 10 2 1844, Meteorological Observations at Kingussie and Inverness 12 0 0 Completing Observations at A IBOUGAN sc spaccaases conscious 35 0 0 Magnetic and Meteorological Co-operation .........:seceeees 25 8 4 Publication of the British Association Catalogue of BSUCUBR Maree s clot sieisle ti a'einr'is ealsve.sie 385 0 O Observations on Tides on the East Coast of Scotland ... 100 0 O Revision of the Nomenclature REDE SGALDG cooscsoccuseeseecs 1842 29 6 Maintaining the Establish- ment at Kew’ Observa- GOLY scesesacccsceasevcccccscescees Ty Ga: Instruments for Kew Obser- WMO atte ae cacy clecdieeccs sasesclis 56 7 3 Influence of Light on Plants 10 0 0 Subterraneous Temperature RUPNGIANG occ ocerssucceseadsne be 0) 20 Coloured Drawings of Rail- way Sections ...........0cc000 1517 6 Investigation of Fossil Fishes ofthe Lower Tertiary Strata 100 0 0 Registering the Shocks of Earthquakes ............ 1842 23 11 10 Structure of Fossil Shells ... 20 0 0 Radiata and Mollusca of the figean and Red Seas 1842 100 0 0 Geographical Distributions of Marine Zoology......... 1842 010 0 Marine Zoology of Devon and. SUELW Mts cascade en's cide Gaacs 10 0 0 Marine Zoology of Corfu...... 10 0 0 Experiments on the Vitality PAS CCUS crac csscecsetsceaetnsess 9 0 0 Experiments on the Vitality DE SCCOS .c.cccessnanesites 1842 8 7 3 Exotic Anoplura ............64 15 0 0 Strength of Materials ......... 100 0 0 Completing Experiments on the Forms of Ships ......... 100 0 0 Inquiries into Asphyxia ...... OF 07* 0: Investigations on the Internal Constitution of Metals...:.. 50 0 0 Constant Indicator and Mo- rin’s Instrument .,,...1842 10 0 0 £981 12 8 1845. Publication of the British As- sociation Catalogue of Stars Meteorological Observations Bt INVerNeSS! naccscccossacceess Magnetic and Meteorological Co-OpexatiONn ......seseeveseees Meteorological Instruments at Hdinburgh..............+0+ Reduction of Anemometrical Observations at Plymouth Electrical Experiments at Kew Observatory ............ Maintaining the Establish- ment at Kew Observatory For Kreil’s Barometrograph Gases from Iron Furnaces... The Actinograph <......0c0.s+=- Microscopic Structure of Ditell S Sav eavecsnatrabengectaaenac Exotic Anoplura ..,...... 1843 Vitality of Seeds ......... 1843 Vitality of Seeds ......... 1844 Marine Zoology of Cornwall . Physiological Action of Medi- GCIMESIe cas schcctntansaccnssecceeste Statistics of Sickness and Mortality in York............ Earthquake Shocks ...... 1843 £831 9 1846. British Association Catalogue Of, StalSmwess ae enecesessene 1844 Fossil Fishes of the London Cla yiwsuusdsdeaserdeasaetecseeceeas Computation of the Gaussian Constants for 1829 ......... Maintaining the Hstablish- ment at Kew Observatory Strength of Materials ......... Researches in Asphyxia ...... Examination of Fossil Shells Vitality of Seeds ......... 1844 Vitality of Seeds ......... 1845 Marine Zoology of Cornwall Marine Zoology of Britain ... Exotic Anoplura ......... 1844 Expenses attending Anemo- Anemometers’ Repairs sAgerbens Atmospheric Waves ............ Captive Balloons ......... 1844 Varieties of the Human Race 1844 Statistics of Sickness and Mortality in York............ o ooooco coon Siac &S Comicon teioo'o a ¢ o ao = WOwrn Sooowoonwnon oO Oo So i _ oO fm BOWWN COS bo | mow bo 6 o'!o cii 1847. £ 3. d. Computation of the Gaussian Constants for 1829.......-.++ 50 0 0 Habits of Marine Animals... 10 0 0 Physiological Action of Medi- CINES .eceeceeececscececeneeerees 20 0 0 Marine Zoology of Cornwall 10 0 0 Atmospheric Waves ......:++.+. (et Ene Vitality of Seeds ........-..000+ Gamat Maintaining the Hstablish- ment at Kew Observatory 107 8 6 £208 5 4 —See eS 1848. Maintaining the Establish- ment at Kew Observatory 171 15 11 Atmospheric Waves ........+++ 310 9 Vitality of Seeds ...........0++ 915 0 Completion of Catalogue of SHEE. Bagncasedanoebeeoppeporooca 70 0 O On Colouring Matters ......... 5 0 0 On Growth of Plants ......... 15 0 0 £275 1 8 1849. Electrical Observations at Kew Observatory ........+.+. 50 0 O Maintaining the Establish- ment at Gitt0.........seeee 76 2 5 Vitality of Seeds .............4. 5-8 1 On Growth of Plants ......... 510 0 Registration of Periodical Phenomena.............seseeeee LOMO RO Bill on Account of Anemo- metrical Observations ...... 139 50 £159 19 6 1850. Maintaining the Hstablish- ment at Kew Observatory 255 1 Transit of Earthquake Waves 50 Periodical Phenomena......... 15 Meteorological Instruments, AZOTCS i) sapeseners cessor eases so 85 25 1851. Maintaining the Establish- ment at Kew Observatory (includes part of grant in TREIGDY vonged) Be cso cuando ees 510) gia, Theory of Heat ..............0+0+ 20) Periodical Phenomena of Ani- mals and Plants...........00+« 5 0-0 Vitality of Seeds ............... 5 6 4 Infiunence of Solar Radiation 30 0 0O Ethnological Inquiries......... 12 0 0 Researches on Annelida .,.... 10 0 O £391 9 7 ——S REPORT—1900. 1852. s. ad Maintaining the Hstablish- ment at Kew Observatory (including balance of grant for: 1850) Ji. ststueseseueeeners 233 17 8 Experiments on the Conduc- tion Of Heat .......s.seeeseees by 2nd Influence of Solar Radiations 20 0 0 Geological Map of Ireland ... 15 0 0 Researches on the British An- TELIA ...-eeseeeeeceeeeeneeenenee 10 0 0 Vitality of Seeds ....0...sseee 10 6 2 Strength of Boiler Plates...... 10 0 0 £304 6 7 1853. Maintaining the Establish- ment at Kew Observatory 165 0 0 Experiments on the Influence of Solar Radiation ......... 15 0 0 Researches on the British Annelida......csececeeseneereeee 10 0 0 Dredging on the East Coast Of Scotland........sseereeeseere 10 0 0 Ethnological Queries ......... 5 0 0 £205 0 0 1854. Maintaining the Establish- ment at Kew Observatory (including balance of former QTant).....sceseeeseree 330 15 4 Investigations on Flax......... 11 0 0 Effects of Temperature on Wrought Tron..........seseeee 10, 10" 10 Registration of Periodical PhenOMena........eeeeeerereree 10 0 0 British Annelida ........s+eeeee 10 0 0 Vitality of Seeds .........+e++0e 5 2 3 Conduction of Heat ..........+- 42 0 £380 19 7 1855. Maintaining the Hstablish- ment at Kew Observatory 425 0 0 Earthquake Movements ...... 10 0 0 Physical Aspect of the Moon 11 8 5 Vitality of Seeds ..........s0+0e 10 711 Map of the World............+++ 15 0 0 Ethnological Queries ........+ 5 0 0 Dredging near Belfast......... 4 0 0 £480 16 4 1856. Maintaining the Establish- ment at Kew Observa- tory :— Ss eee £75 0 0 WShDaecees 3 .£500 9 of A i GENERAL STATEMENT. o £ 3s. d. Strickland’s Ornithological SYNONYMS .....seeeeeeeeeeeees 100 0 0 Dredging and Dredging ROTM) c... 22.00 scecsersesscceoers 913 0 Chemical Action of Light ... 20 0 0 Strength of Iron Plates ...... 10 0 0 Registration of Periodical PhenoMmena.........ceeesveeeeeee 10 0 O Propagation of Salmon......... 10 0 0 £734 13 9 al 1857. Maintaining the Establish- ment at Kew Observatory 350 0 0 Earthquake Wave Experi- MENS ...c.ccccccsescsesessecoast 40 0 0 Dredging near Belfast......... 1c i0% 0 Dredging on the West Coast Of Scotland .........cceeeeseeeee 10 0 0 Investigations into the Mol- lusca of California ......... 10 0 0 Experiments on Flax ......... 5 0 0 Watural History of Mada- ZASCAT .....eseerecseeeseereewenes 20 0 0 Researches on British Anne- NYG ddeee ses-ssdsnseaaceenenasnem 25 0 0 Report on Natural Products imported into Liverpool... 10 0 0 Artificial Propagation of Sal- MOD ......scecccccecscseeecerseecs 10 0 0 Temperature of Mines......... i sO Ynermometers for Subterra- nean Observations...........- 5.7 4 Life-boats .....sccecseceeseeseuee 5 0 0 £507 15 4 1858. Maintaining the Establish- ment at Kew Observatory 500 0 0 Earthquake Wave Experi- ERIS ov craepprcgashaassssss 10 Natural History of Timor-laut 50 Screw Gauges.......scseeees aceiees 1884. Meteorological Observations on Ben: Nevistits.. cease eee 50 Collecting and Investigating Meteoric Dust......ces.ceseeee 20 Meteorological Observatory at Chepstowis-antssenapecsassess 25 Tidal Observations.............. 10 Ultra Violet Spark Spectra... 8 Earthquake Phenomena of JAPAN) soe Aicenwessduvesslcesates 75 Fossil Plants of Halifax ...... 15 Bossi Roly ZOay seeseuconssseccsexole 10 Erratic Blocks of England ... 10 Fossil Phyllopoda of Palzo- ZOLCHROCKS eesti sccaseeosde > 15 Circulation of Underground Wiahensanmets aeeasiaaecseaiecness 5 International Geological Map 20 Bibliography of Groups of Invertebrata... ...csciesss rae 50 Natural History of Timor-laut 50 Naples Zoological Station ... 80 Exploration of Mount Kili- ma-njaro, Hast Africa ...... 500 Migration of Birds............... 20 Coagulation of Blood............ 100 Zoological Literature Record 100 Anthropometric Committee... 10 £1173 a a . ROO OC OC wlocoo © w ooSoC0oO CS SC Oo Ooco Cc Oo wlecs © w Cooo0So0 05 0 oC oco oO o ® MIocoeio- c.o O° So “oO ooceS ooo “oo Eloooces os ooo co © coe s cx 1885. s. d. Synoptic Chart of Indian OCEAN .....0ssssonervccceseses ses 50 0 0 Reduction of Tidal Observa- TIONS poccn tose racsWssvesscececeses LOMION 10 Calculating Tables in Theory Of NUMbEYTS.......00.sseeeeeeree 100 0 0 Meteorological Observations on Ben NeViS ......seecseeseeee 50 0 O Meteoric Dust ..........ceseeeee 70 0 0 Vapour Pressures, &c., of Salt Solutions ..........cacoseceserers 25 0 0 Physical Constants of Solu- HNO aaSsocacdadasoa aucboadosaroe 20 0 0 Volcanic Phenomena of Vesu WALIS Moser bbs cosscecsascrstes tends 25 0 0 Raygill Hissure ........00....c00-- 15 0 0 Earthquake Phenomena of UGH O26). Bice. sacbduongs vodoanoudcbe 79 0 0 Fossil Phyllopoda of Palzeozoic PUOCKS''.tcodes leven sbecdduseten ice 25 0 0 Fossil Plants of British Ter- tiary and Secondary Beds... 50 0 0O Geological Record ............00. 50 0 O Circulation of Underground WiLEDS sami sbacesscesseeccnssabces LOOP 0 Naples Zoological Station 100 0 O Zoological Literature Record. 100 0 0 Migration of Birds ............ 30 0 0 Exploration of Mount Kilima- Map) SSssedaseSodcbdocspaaaseogs 25 0 0 Recent Polyzoa ...........sseeeee 10 0 0 Granton Biological Station... 100 0 0 Biological Stations on Coasts of United Kingdom.......... 150 0 0O Exploration of New Guinea... 200 0 0 Exploration of Mount Roraima 100 0 O £1385 0 0 1886. Hlectrical Standards............ 40 0 0 Solar Radiation...............005 910 6 Tidal Observations ............ x 0 0 Magnetic Observations......... 010 O Observations on Ben Nevis.. a 0 0 Physical and Chemical Bear- ings of Hlectrolysis ......... 20 0 0 Chemical Nomenclature ...... 5 0 0 Fossil Plants of British Ter- tiary and Secondary Beds... 20 0 0 Caves in North Wales ......... 25 0 0 Volcanic Phenomena of Vesu- VAIS sce scenneeeeturotedarsscstese 30 0 0 Geological Record............... 100 0 0 Palzozoic Phyllopoda ......... 15 0 0 Zoological Literature Record. 100 0 0 Granton Biological Station... 75 0 0 Naples Zoological Station...... 50 0 0 Researches in Food-Fishes and InvertebrataatSt.Andrews 75 0 0 REPOoRT—1900, Flora and Fauna of the Cameroons Migration of Birds Bathy-hypsographical Map of British Isles Regulation of Wages Prehistoric Race of Greek Islands....... Onan seutts Stas seca 20 Racial Photographs, Egyptian 20 a eee ee eee se eereeeeens Seat £ 3. d. Migration of Birds ......6..0 30 0 0 Secretion of Urine............... 10 0 O Exploration of New Guinea... 150 0 0 Regulation of Wages under Sliding Scales, ............... 10 0 0 Prehistoric Race in Greek TSIandS <... aunrenpuenee 20 0 0 North-Western Tribes of Ca- NAVAS tr coceseeerieeceonlene meee teate 50 0 0 £995 0 6 1887. Solar Radiation .......0....se0+ 1810 0 Electrolysis... <.-.c0s-sereesssasee 30 0 0 Ben Nevis Observatory......... 75 0 0 Standards of Light (1886 fantstel) yepprcoenabobhodarich nnason7 20 0 0 Standards of Light (1887 QUANG) tas wcastexsectecasherereeen 10 0 0 Harmonic Analysis of Tidal Observations) ;-\rssietscass ens Hoe rO sO Magnetic Observations......... 26 2 0 Electrical Standards ............ 50 0 0 Silent Discharge of Electricity 20 0 0 Absorption Spectra ............ 40 0 0 Nature of Solution ............ 20 0 0 Influence of Silicon on Steel 30 0 O Volcanic Phenomena of Vesu- WIUS neat sas conmacstcate armeen anes 20 0 0 Volcanic Phenomena of Japan (1886 grant) coor oes cese 50 0 0 Volcanic Phenomena of J apat GSS iCorarit) eccnersscemieants 50 0 0 Cae Gwyn Cave, N. Wales. .. 20 0 0 HirraticwBlOGkS) Sr.csssacseteens 10 0 O Fossil Phyllopoda ............... 20 0 0 Coal Plants of Halifax......... 25 0 0 Microscopic Structure of the Rocks of Anglesey............ 10 0 0 Exploration of the Eocene Beds of the Isleof Wight... 20 0 0 Underground Waters ......... ‘ae OO) ‘Manure’ Gravelsof Wexford 10 0 0 Provincial Museums Reports 5 0 0 Lymphatic System ............ 25 0 0 Naples Biological Station 100 0 0O Plymouth Biological Station 50 0 0 Granton Biological Station... 75 0 0 Zoological Record .........+0+++ 100 0 0 Flora of China ...........seeeees 75 0 O 0 0 0 0 6 0 0 0 0 0 0 0 0 £1186 18 GENERAL STATEMENT. o Cononac? (= i) Oo f=) ooo ooooooocoeo Ser i=) f=) eoooocoocooo fo) oor o® o|co Oo o ooo cooocooocoeooo oo So o cooocooocooco°o (=) ooo >) ouNorF 1888. £ Ben Nevis Observatory......... 150 ‘Electrical Standards...........+ 2 Magnetic Observations......... 15 Standards of Light ............ 79 Blectrolysis ....cseseeeeeeeeeeees 3 Uniform Nomenclature in MeChanics: ........cceeecseeoeee 10 Silent Discharge of Hlec- ERICIGY .0.....reresecceewseeeesore 9 Properties of Solutions ...... 25 Influence of Silicon on Steel 20 Methods of Teaching Chemis- LEXY ceeceeceeceeescescerceceeneeee 10 Tsomeric Naphthalene Deriva- HUVCSE UE scec- 0 0 £1,212 0 0 1899. Electrical Standards............ 225 0 0 Seismological Observations... 65 14 § Science Abstracts ............... 100 0 0 Heat of Combination of Metals HEUPANIOYS onsen cocoteresstikeoaz2 20 0 O Radiation ina Magnetic Field 50 0 0 Calculation of Certain In- RPT ALB asciate co's aasadessendedae-os 10 0 O Action of Light upon Dyed PEMOEES. O20) vccndcdaesciss seeds 2 La 6 Relation between Absorption Spectra and Constitution of Organic Substances ......... 50 0 0 Erratic Blocks .................. iD) 0) +0 Photographs of Geological MAHCROSHB cad tsescics estes veer 10 0 0 Remains of Irish Elk in the Tsle} OF MAM. ss ie. cocveseses. 15 0 0 Pleistocene Flora and Fauna BI CAMA titeececcerecscccescvsss 30 0 CXV 6.1 ga Records of Disappearing Drift Section at Moel Tryfaen ... 5 0 0 Ty Newydd Caves............... 40 0 0 Ossiferous Caves at Uphill... 30 0 0 Table at the Zoological Sta- GION, NAPless joceas aes cscs cross 100 0 0 Table at the Biological La- boratory, Plymouth ......... 20 0 6 Index Generum et Specierum Animalinme sc oecsats aches: 100 0 0 Migration of Birds ............ 1 0 0 Apparatus for Keeping Aqua- ticOrganisms under Definite Physical Conditions ......... 15 0 0 Plankton and Physical Con- ditions of the English Chan- Nelduring TSI... ..cseccas 100 0 0 Exploration of Sokotra ...... 35 0 0 Lake Village at Glastonbury 50 0 0 | Silchester Excavation ....... = 105.0) 0 EthnologicalSurv eyofCanada 35 0 0 | New Edition of ‘ Anthropolo- gical Notes and Queries’... 40 0 0 Age of Stone Circles............ 20 0 0 Physiological Effects of Pep- TONG i 5. tic shataccessencccnteeips 30 0 0 Electrical Changes accom- panying Discharge of Res- piratory Centres..........:.+5. 20 0 0 Influence of Drugs upon the Vascular NervousSystem... 10 0 0 Histological Changes in Nerve Cellsie ss ontecc) cncecuies Seeceseed 20 0 0 Micro-chemistry of Cells ...... 40 0 0 Histology of Suprarenal Cap- SUlOS) toss crap ates qte acme 20 0 0 | Comparative Histology of Cerebral (Context, ws cance 10°10" 0 Fertilisation in Phyxophycexe 20 0 0 Assimilation in Plants......... 20 0 0 Zoological and Botanical Pub- LiCAtIONS crrpcadaec cscs aseraks bio 0 Corresponding Societies Com- INL CC ae aad wake Leaasceteaeecte 25 0 0 £1,430 14 2 1900. Hlectrical Standards............ 25 0 0 Seismological Observations... 60 0 0 Radiationina Magnetic Field 25 0 0 Meteorological Observatory at Montreali, sii. .cdchdisedeadee 20 0 0 Tables of Mathematical Func- TRONS ircester. (as,.0cnessbaccehans de 75 0 0 Relation between Absorption Spectra and Constitution of Organic Bodies.......... =.» 30 0 O Wave-length Tables............ 5 0 0 Quantitative eee Electrolytic Analysis ., v exvl REPORT—1900. Bake ids | eames) TIsomorphous Sulphonic Deri- | Future Dealings in Raw vatives of Benzene ......... 20 0 0 | Produce .....+ssccersves ieeehete 210 0 The Nature of Alloys ......... 30 0 0 | Silchester Excavation ........ 10-:0).0 Photographs of Geological | Ethnological Survey of AGEGESD iscccrecas) se sbevest soe. Gy sO) S10) Canada <-..cwccocwesomenels elena 60 0 0 Remains of Elk in the Isle of New Edition of ‘Anthropo- WEIS spe qdeoncascogsohpoNOneE recs 5 0 0 | _ logical Notes and Queries’ 40 0 0 Pleistocene Fauna and Flora Photographs: of Anthropo- PYG OAT Cn eescdavscboecescine 10 0 O | _ logical Interest ............... 1020750 Movements of Underground | Mental and Physical Condi- Waters of Craven ............ 40 0 0 | _ tion of Children in Schools 5 0 O Table at the Zoological Sta- Ethnography of the Malay tion, Naples .....03.. s.r 100 0 0 Peninsula ..ccccccuwsscess eer 25 0 0 Table at the Biological La- Physiological Eifects of Pep- boratory, Plymouth ......... 20 0 O | COME... .eeeeeeesseeeeseenneeee nes 20 0 0 Index Generum et Specierum | Comparative Histology of PATI ALIN 55250 .00c0cces scones 50 0 0 | Suprarenal Capsules......... 20 0 0 Migration of Birds ............ 15 0 0 | Comparative Histology of Plankton and Physical Con- Cerebral Cortex..........+..++ 5-0. 0 ditions of the English Electrical Changes in Mam- OINENaIGI. danhdisedtensonodeepseto 40 0 © | malian Nerves ..............- 20 0 0 Zoology of the Sandwich | Vascular Supply of Secreting Tisibitelss ysohaagenbesshosaueep cna 100 0 0 GAMES eet dencieterecedeacent > tee 10410) 0 Coral Reefs of the Indian Fertilisation in Pheophycee 20 0 0 TAS 0ye, Ge Gaodngs acosAdenpectioge 30 0 0 | Corresp. Societies Committee 20 0 0 Physical and Chemical Con- =. AGRE stants of Sea-Water ......... 100) 0-0" | £1,072 10 0 General Meetings. On Wednesday, September 5, at 8.30 p.m., in St. George’s Hall, Brad- ford, Sir Michael Foster, K.C.B., Sec.R.S. (represented by Sir Henry E. Roscot, F.R.S.), resigned the office of President to Sir William Turner, D.C.L., F.R.S., who took the Chair, and delivered an Address, for which see page 3. On Thursday, September 6, at 8.30 p.m., a Soirée took place in St. George’s Hall. On Friday, September 7, at 8.30 p.m., in St. George’s Hall, Professor Francis Gotch, F.R.S., delivered a discourse on ‘ Animal Electricity.’ On Monday, September 10, at 8.30 p.m. in St. George’s Hall, Professor W. Stroud delivered a discourse on ‘ Range Finders,’ On Tuesday, September 11, at 8.30 p.m., a Soirée took place in St. George’s Hall. | On Wednesday, September 12, at 2.30 p.m., in the Mechanics’ Institute, the concluding General Meeting took place, when the Proceedings of the General Committee and the Grants of Money for Scientific Purposes were explained to the Members. The Meeting was then adjourned to Glasgow. [The Meeting is appointed to commence on Wednesday, September 11, 1901.] { _ PRESIDENT’S ADDRESS. 5 a : 3 ‘ —_———_~.-- ~~ ADDRESS BY Proressorn SIR WILLIAM TURNER, M.B., D.C.L., LL.D. Dees EE... PRESIDENT. TWENTY-SEVEN years ago the British Association met in Bradford, not at that time raised to the dignity of a City. The meeting was very success- ful, and was attended by nearly 2,000 persons—a forecast, let us hope, of what we may expect at the present assembly. An eminent chemist, Professor A. W. Williamson, presided. On this occasion the Associa- tion has selected for the presidential chair one whose attention has been given to the study of an important department of biological science. His claim to occupy, however unworthily, the distinguished position in which he has been placed, rests, doubtless, on the fact that, in the midst of the engrossing duties devolving on a teacher in a great University and School of Medicine, he has endeavoured to contribute to the sum of knowledge of the science which he professes. It is a matter of satis- faction to feel that the success of a meeting of this kind does not rest upon the shoulders of the occupant of the presidential chair, but is due to the eminence and active co-operation of the men of science who either pre- side over or engage in the work of the nine or ten sections into which the Association is divided, and to the energy and ability for organisation displayed by the local Secretaries and Committees. The programme pre- pared by the general and local officers of the Association shows that ne efforts have been spared to provide an ample bill of fare, both in its scientific and social aspects. Members and Associates will, I feel sure, take away from the Bradford Meeting as pleasant memories as did our colleagues of the corresponding Association Frangaise, when, in friendly collaboration at Dover last year, they testified to the common citizenship of the Universal Republic of Science. As befits a leading centre of industry in the great county of York, the applications of science to the industrial arts and to agriculture will form subjects of discussion in the papers to be read at the meeting. B2 4, REPORT—1900. Since the Association was at Dover a year ago, two of its former Presidents have joined the majority. The Duke of Argyll presided at the meeting in Glasgow so far back as 1855. Throughout his long and energetic life, he proved himself to be an eloquent and earnest speaker, one who gave to the consideration of public affairs a mind of singular independence, and a thinker and writer in a wide range of human knowledge. Sir J. Wm. Dawson was President at the meeting in Birmingham in 1886. Born in Nova Scotia in 1820, he devoted himself to the study of the Geology of Canada, and became the leading authority on the subject. He took also an active and influential part in promoting the spread of scientific education in the Dominion, and for a number of years he was Principal and Vice-Chancellor of the M‘Gill University, Montreal. Scientific Method. Edward Gibbon has told us that diligence and accuracy are the only merits which an historical writer can ascribe to himself. Without doubt they are fundamental qualities necessary for historical research, but in order to bear fruit they require to be exercised by one whose mental qualities are such as to enable him to analyse the data brought together by his diligence, to discriminate between the false and the true, to possess an insight into the complex motives that determine human action, to be able to recognise those facts and incidents which had exercised either a primary or only a secondary influence on the affairs of nations, or on the thoughts and doings of the person whose character he is depicting. In scientific research, also, diligence and accuracy are fundamental qualities. By their application new facts are discovered and tabulated, their order of succession is ascertained, and a wider and more intimate knowledge of the processes of nature is acquired. But to decide on their true significance a well-balanced mind and the exercise of prolonged thought and reflection are needed. William Harvey, the father of exact research in physiology, in his memorable work ‘De Motu Cordis et San- guinis,’ published more than two centuries ago, tells us of the great and daily diligence which he exercised in the course of his investigations, and the numerous observations and experiments which he collated. At the same time he refers repeatedly to his cogitations and reflections on the meaning of what he had observed, without which the complicated move- ments of the heart could not have been analysed, their significance deter- mined, and the circulation of the blood in a continuous stream definitely established. Early in the present century, Carl Ernst von Baer, the father of embryological research, showed the importance which he attached to the combination of observation with meditation by placing side by side on the title-page of his famous treatise ‘ Ueber Entwickelungsgeschichte der Thiere ’ (1828) the words Beobachiung und Reflexion. Though I have drawn from biological science my illustrations of the néed of this combination, it must not be inferred that it applies exclu- » ADDRESS. J sively to one branch of scientific inquiry ; the conjunction influences and determines progress in all the sciences, and when associated with a sufficient touch of imagination, when the power of seeing is conjoined with the faculty of foreseeing, of projecting the mind into the future, we may expect something more than the discovery of isolated facts ; their co- ordination and the enunciation of new principles and laws will necessarily follow. Scientific method consists, therefore, in close observation, frequently repeated so as to eliminate the possibility of erroneous seeing ; in experi- ments checked and controlled in every direction in which fallacies might arise; in continuous reflection on the appearances and phenomena observed, and in logically reasoning out their meaning and the conclusions to be drawn from them. Were the method followed out in its integrity by all who are engaged in scientific investigations, the time and labour expended in correcting errors committed by ourselves or by other observers and experimentalists would be saved, and the volumes devoted annually to scientific literature would be materially diminished in size. Were it applied, as far as the conditions of life admit, to the conduct and management of human affairs, we should not require to be told, when critical periods in our welfare as a nation arise, that we shall muddle through somehow. Recent experience has taught us that wise discretion and careful prevision are as necessary in the direction of public affairs as in the pursuit of science, and in both instances, when properly exercised, they enable us to reach with comparative certainty the goal which we strive to attain. Improvements in Means of Observation. Whilst certain principles of research are common to all the sciences, each great division requires for its investigation specialised arrangements to insure its progress. Nothing contributes so much to the advancement of knowledge as improvements in the means of observation, either by the discovery of new adjuncts to research, or by a fresh adaptation of old methods. In the industrial arts, the introduction of a new kind of raw material, the recognition that a mixture or blending is often more serviceable than when the substances employed are uncombined, the discovery of new processes of treating the articles used in manufactures, the invention of improved machinery, all lead to the expansion of trade, to the occupation of the people, and to the development of great industrial centres. In science, also, the invention and employment of new and more precise instruments and appliances enable us to appreciate more clearly the signification of facts and phenomena which were pre- viously obscure, and to penetrate more deeply into the mysteries of nature. They mark fresh departures in the history of science, and provide a firm base of support from which a continuous advance may be made and fresh conceptions of nature can be evolved 6 REPORT—1900. It is not my intention, even if I possessed the requisite knowledge, to undertake so arduous a task as to review the progress which has recently been made in the great body of sciences which lie within the domain of the British Association. As my occupation in life has required me to give attention to the science which deals with the structure and organisa- tion of the bodies of man and animals—a science which either includes within its scope or has intimate and widespread relations to comparative anatomy, embryology, morphology, zoology, physiology, and anthropology —I shall limit myself to the attempt to bring before you some of the more important observations and conclusions which have a bearing on the present position of the subject. As this is the closing year of the century, it will not, I think, be out of place to refer to the changes which a hundred years have brought about in our fundamental. conceptions of the structure of animals. In science, as in business, it is well from time to time to take stock of what we have been doing, so that we may realise where we stand and ascertain the balance to our credit in the scientific ledger. So far back as the time of the ancient Greeks it was known that the human body and those of the more highly organised animals were not homo- geneous, but were built up of parts, the partes dissimilares (ra avopow peépn) of Aristotle, which differed from each other in form, colour, texture, consistency, and properties. These parts were familiarly known as the bones, muscles, sinews, blood-vessels, glands, brain, nerves, and so on. As the centuries rolled on, and as observers and observations multiplied, a more and more precise knowledge of these parts throughout the Animal Kingdom was obtained, and various attempts were made to classify animals in accordance with their forms and structure. During the concluding years of the last century and the earlier part of the present, the Hunters, William and John, in our country, the Meckels in Germany, Cuvier and Saint-Hilaire in France, gave an enormous impetus to anatomical studies, and contributed largely to our knowledge of the construction of the bodies of animals. But whilst by these and other observers the most salient and, if I may use the expression, the grosser characters of animal organisation had been recognised, little was known of the more intimate structure or texture of the parts. So far as could be determined by the unassisted vision, and so much as could be recognised by the use of a simple lens, had indeed been ascertained, and it was known that muscles, nerves, and tendons were composed of threads or fibres, that the blood- and lymph-vessels were tubes, that the parts which we call fascise and aponeuroses were thin membranes, and so on. Early in the present century Xavier Bichat, one of the most brilliant men of science during the Napcleonic era in France, published his ‘ Anatomie Générale,’ in which he formulated important general principles. Every animal is an assemblage of different organs, each of which dis- charges a function, and acting together, each in its own way, assists in the ADDRESS. 7 preservation of the whole. The organs are, as it were, special machines situated in the general building which constitutes the factory or body of the individual. But, further, each organ or special machine is itself formed of tissues which possess different properties. ‘Some, as the blood- vessels, nerves, fibrous tissues, &c., are generally distributed throughout the animal body, whilst others, as bones, muscles, cartilage, &c., are found only in certain definite localities. Whilst Bichat had acquired a definite philosophical conception of the general principles of construction and of the distribution of the tissues, neither he nor his pupil Béclard was in a position to determine the essential nature of the structural elements. The means and appliances at their disposal and at that of other ob- servers in their generation were not sufficiently potent to complete the analysis. Attempts were made in the third decennium of this century to improve the methods of examining minute objects by the manufacture of com- pound lenses, and, by doing away with chromatic and spherical aberra- tion, to obtain, in addition to magnification of the object, a relatively large flat field of vision with clearness and sharpness of definition. When in January 1830 Joseph Jackson Lister read to the Royal Society his memoir ‘On some properties in achromatic object-glasses applicable to the improvement of microscopes,’ he announced the principles on which combinations of lenses could be arranged, which would possess these qualities. By the skill of our opticians, microscopes have now for more than half a century been constructed which, in the hands of competent observers, have influenced and extended biological science with results comparable to those obtained by the astronomer through improvements in the telescope. In the study of the minute structure of plants and animals the observer has frequently to deal with tissues and organs, most of which possess such softness and delicacy of substance and outline that, even when micro- scopes of the best construction are employed, the determination of the intimate nature of the tissue, and the precise relation which one element of an organ bears to the other constituent elements, is in many instances a matter of difficulty. Hence additional methods have had to be devised in order to facilitate -study and to give precision and accuracy to our observations. It is difficult for one of the younger generation of biologists, with all the appliances of a well-equipped laboratory at his command, with experienced teachers to direct him in his work, and with excellent text-books, in which the modern methods are described, to realise the conditions under which his predecessors worked half a century ago. Laboratories for minute biological research had not been constructed, the practical teaching of histology and embryology had not been organised, experience in methods of work had not accumulated ; each man was left to his individual efforts, and had to puzzle his way through the complica- tions of structure to the best of his power. Staining and hardening 8 REPORT—1900. reagents were unknown. ‘The double-bladed knife invented by Valentin, held in the hand, was the only improvement on the scalpel or razor for cutting thin, more or less translucent slices suitable for microscopic examination ; mechanical section-cutters and freezing arrangements had not been devised. The tools at the disposal of the microscopist were little more than knife, forceps, scissors, needles ; with acetic acid, glyce- rine, and Canada balsam as reagents. But in the employment of the newer methods of research care has to be taken, more especially when hardening and staining reagents are used, to discriminate between appearances which are to be interpreted as indicating natural characters, and those which are only artificial productions. Notwithstanding the difficulties attendant on the study of the more delicate tissues, the compound achromatic microscope provided anatomists with an instrument of great penetrative power. Between the years 1830 and 1850 a number of acute observers applied themselves with much energy and enthusiasm to the examination of the minute structure of the tissues and organs in plants and animals. Cell Theory. It had, indeed, long been recognised that the tissues of plants were to a large extent composed of minute vesicular bodies, technically called cells (Hooke, Malpighi, Grew). In 1831 the discovery was made by the great botanist, Robert Brown, that in many families of plants a circular spot, which he named areola or nucleus, was present in each cell ; and in 1838 M.J.Schleiden published the fact that a similar spot or nucleus was a universal elementary organ in vegetables. In the tissues of animals also structures had begun to be recognised comparable with the cells and nuclei of the vegetable tissues, and in 1839 Theodore Schwann announced the important generalisation that there is one universal principle of develop- ment for the elementary part of organisms, however different they may be in appearance, and that this principle is the formation of cells. The enun- ciation of the fundamental principle that the elementary tissues consisted of cells constituted a step in the progress of biological science, which will for ever stamp the century now drawing to a close with a character and renown equalling those which it has derived from the most brilliant discoveries in the physical sciences. It provided biologists with the visible anatomical units through which the external forces operating on, and the energy generated in, living matter come into play. It dispelled for ever the old mystical idea of the influence exercised by vapours or - spirits in living organisms. It supplied the physiologist and pathologist with the specific structures through the agency of which the functions of organisms are discharged in health and disease. It exerted an enormous influence on the progress of practical medicine. A review of the progress of knowledge of the cell may appropriately enter into an address on this occasion. ADDRESS, 9 Structure of Cells. A cell is a living particle, so minute that it needs a microscope for its examination ; it grows in size, maintains itself in a state of activity, responds to the action of stimuli, reproduces its kind, and in the course of time it degenerates and dies. Let us glance at the structure of a ce]l to determine its constituent parts and the ré/e which each plays in the function to be discharged. The original conception of a cell, based upon the study of the vegetable tissues, was a minute vesicle enclosed by a definite wall, which exer- cised chemical or metabolic changes on the surrounding material and secreted into the vesicle its characteristic contents. A similar conception was at first also entertained regarding the cells of animal tissues ; but as observations multiplied, it was seen that numerous elementary particles, which were obviously in their nature cells, did not possess an enclosing envelope. A wall ceased to have a primary value as a constituent part of a cell, the necessary vesicular character of which therefore could no longer be entertained. The other constituent parts of a cell are the cell plasm, which forms the body of the cell, and the nucleus embedded in its shbstance, Not- withstanding the very minute size of the nucleus, which even in the largest cells is not more than .},th inch in diameter, and usually is considerably smaller, its almost constant form, its well-defined sharp outline, and its power of resisting the action of strong reagents when applied to the cell, have from the period of its discovery by Robert Brown caused histologists to bestow on it much attention. Its structure and chemical composition ; its mode of origin ; the part which it plays in the formation of new cells, and its function in nutrition and secretion have been investigated. When examined under favourable conditions in its passive or resting state, the nucleus is seen to be bounded by a membrane which separates it from the cell plasm and gives it the characteristic sharp contour. Jt contains an apparently structureless nuclear substance, nucleoplasm or enchylema, in which are embedded one or more extremely minute particles called nucleoli, along with a network of exceedingly fine threads or fibres, which in the active living cell play an essential part in the production of new nuclei within the cell. In its chemical composition the nuclear substance consists of albuminous plastin and globulin ; and of a special material named nuclein, rich in phosphorus and with an acid reaction. The delicate network within the nucleus consists apparently of the nuclein, a substance which stains with carmine and other dyes, a property which enables the changes, which take place in the network in the production of young cells, to be more readily seen and followed out by the observer. The mode of origin of the nucleus and the part which it plays in the production of new cells have been the subject of much discussion. 10 REPORT—1900. Schleiden, whose observations, published in 1838, were made on the cells of plants, believed that within the cell a nucleolus first appeared, and that around it molecules aggregated to form the nucleus. Schwann again, whose observations were mostly made on the cells of animals, considered that an amorphous material existed in organised bodies, which he called cytoblastema. It formed the contents of cells, or it might be situated free or external to them. He figuratively compared it to a mother liquor in which crystals are formed. Hither in the cytoblastema within the cells or in that situated external to them, the aggregation of molecules around a nucleolus to form a nucleus might occur, and, when once the nucleus had been formed, in its turn it would serve as a centre of aggregation of additional molecules from which a new cell would be produced. He regarded therefore the formation of nuclei and cells as possible in two ways : one within pre-existing cells (endogenous cell-formation), the other in a free blastema lying external to cells (free cell-formation). In animals, he says, the endogenous method is rare, and the customary origin is in an external blastema. Both Schleiden and Schwann considered that after the cell was formed the nucleus had no permanent influence on the life of the cell, and usually disappeared. Under the teaching principally of Henle, the famous Professor of Anatomy in Gottingen, the conception of the free formation of nuclei and cells in a more or less fluid blastema, by an aggregation of elementary granules and molecules, obtained so much credence, especially amongst those who were engaged in the study of pathological processes, that the origin of cells within pre-existing cells was to a large extent lost sight of. That a parent cell was requisite for the production of new cells seemed to many investigators to be no longer needed. Without doubt this con- ception of free cell-formation contributed in no small degree to the belief, entertained by various observers, that the simplest plants and animals might arise, without pre-existing parents, in organic fluids desti- tute of life, by a process of spontaneous generation ; a belief which pre- vailed in many minds almost to the present day. If, as has been stated, the doctrine of abiogenesis cannot be experimentally refuted, on the other hand it has not been experimentally proved. The burden of proof lies with those who hold the doctrine, and the evidence that we possess is all the other way. Multiplication of Cells. Although von Mohl, the botanist, seems to have been the first to recognise (1835) in plants a multiplication of cells by division, it was not until attention was given to the study of the egg in various animals, and to the changes which take place in it, attendant on fertilisation, that in the course of time a much more correct conception of the origin of the nucleus and of the part which it plays in the formation of new cells was obtained. Before Schwann had published his classical memoir m 1839, ADDRESS. 1i von Baer and other observers had recognised within the animal ovum the germinal vesicle, which obviously bore to the ovum the relation of a nucleus to a cell. As the methods of observation improved, it was recog- nised that, within the developing egg, two vesicles appeared where one only had previously existed, to be followed by four vesicles, then eight, and so on in multiple progression until the ovum contained a multitude of vesicles, each of which possessed a nucleus. The vesicles were obviously cells which had arisen within the original germ-cell or ovum. ‘These changes were systematically described by Martin Barry so long ago as 1839 and 1840 in two memoirs communicated to the Royal Society of London, and the appearance produced, on account of the irregu- larities of the surface occasioned by the production of new vesicles, was named by him the mulberry-like structure. He further pointed out that the vesicles arranged themselves as a layer within the envelope of the egg or zona pellucida, and that the whole embryo was composed of cells filled with the foundations of other cells. He recognised that the new cells were derived from the germinal vesicle or nucleus of the ovum, the con- tents of which entered into the formation of the first two cells, each of which had its nucleus, which in its turn resolved itself into other cells, and by a repetition of the process into a greater number. The endogenous origin of new cells within a pre-existing cell and the process which we now term the segmentation of the yolk were successfully demonstrated. In a third memoir, published in 1841, Barry definitely stated that young cells originated through division of the nucleus of the parent cell, instead of arising, as a product of crystallisation, in the fluid cytoblastema of the parent cell or in a blastema situated external to the cell. In a memoir published in 1842, John Goodsir advocated the view that the nucleus is the reproductive organ of the cell, and that from it, as from a germinal spot, new cells were formed. In a paper, published three years later, on nutritive centres, he described cells, the nuclei of which were the permanent source of successive broods of young cells, which from time to time occupied the cavity of the parent cell. He extended also his observations on the endogenous formation of cells to the cartilage cells in the process of inflammation and to other tissues undergoing pathological changes. Corroborative observations on endogenous formation were also given by his brother Harry Goodsir in 1845. These observations on the part which the nucleus plays by cleavage in the formation of young cells by endogenous development from a parent centre—that an organic con- tinuity existed between a mother cell and its descendants through the nucleus—constituted a great step in advance of the views entertained by Schleiden and Schwann, and showed that Barry and the Goodsirs had a deeper insight into the nature and functions of cells than was possessed by most of their contemporaries, and are of the highest importance when viewed in the light of recent observations. In 1841 Robert Remak published an account of the presence of two 12 REPORT—1900. nuclei in the blood corpuscles of the chick and the pig, which he regarded as evidence of the production of new corpuscles by division of the nucleus within a parent cell ; but it was not until some years afterwards (1850 to 1855) that he recorded additional observations and recognised that division of the nucleus was the starting-point for the multiplication of cells in the ovum and in the tissues generally. Remak’s view was that the process of cell division began with the cleavage of the nucleolus, followed by that of the nucleus, and that again by cleavage of the body of the cell and of its membrane. MKdélliker had previously, in 1843, de- scribed the multiplication of nuclei in the ova of parasitic worms, and drew the inference that in the formation of young cells within the egg the nucleus underwent cleavage, and that each of its divisions entered into the formation of a new cell. By these observations, and by others subsequently made, it became obvious that the multiplication of animal _ cells, either by division of the nucleus within the cell, or by the budding off of a part of the protoplasm of the cell, was to be regarded as a widely spread and probably a universal process, and that each new cell arose from a parent cell. Pathological observers were, however, for the most part inclined to consider free cell-formation in a blastema or exudation by an aggregation of molecules, in accordance with the views of Henle, as a common pheno- menon. This proposition was attacked with great energy by Virchow in a series of memoirs published in his ‘ Archiv,’ commencing in Vol. 1, 1847, and finally received its death-blow in his published lectures on Cellular Pathology, 1858. He maintained that in pathological structures there was no instance of cell development de novo ; where a cell existed, there one must have been before. Cell-formation was a continuous develop- ment by descent, which he formulated in the expression ommis cellula e celluld. Karyokinesis. Whilst the descent of cells from pre-existing cells by division of the nucleus during the development of the egg, in the embryos of plants and animals, and in adult vegetable and animal tissues, both in healthy and diseased conditions, had now become generally recognised, the mechanism of the process by which the cleavage of the nucleus took place was fora long time unknown. The discovery had to be deferred until the optician had been able to construct lenses of a higher penetrative power, and the microscopist had learned the use of colouring agents capable of dyeing the finest elements of the tissues. There was reason to believe that in some cases a direct cleavage of the nucleus, to be followed by a corresponding division of the cell into two parts, did occur. In the period between 1870 and 1880 observations were made by Schneider, Strasburger, Biitschli, Fol, van Beneden, and Flemming, which showed that the division of the nucleus and the cell was due to a series of very remark- able changes, now known as indirect nuclear and cell division, or karyo- ADDRESS. 13 kinesis. The changes within the nucleus are of so complex a character that it is impossible to follow them in detail without the use of appropriate illustrations. I shall have to content myself, therefore, with an elemen- tary sketch of the process. T have previously stated that the nucleus in its passive or resting stage contains a very delicate network of threads or fibres. The first stage in the process of nuclear division consists in the threads arranging them- selves in loops and forming a compact coil within the nucleus. The coil then becomes looser, the loops of threads shorten and thicken, and some- what later each looped thread splits longitudinally into two portions. As the threads stain when colouring agents are applied to them, they are called chromatin fibres, and the loose coil is the chromosome (Waldeyer). As the process continues, the investing membrane of the nucleus dis- appears, and the loops of threads arrange themselves within the nucleus so that the closed ends of the loops are directed to a common centre, from which the loops radiate outwards and produce a starlike figure (aster). « At the same time clusters of extremely delicate lines appear both in the nucleoplasm and in the body of the cell, named the achromatic figure, which has a spindle-like form with two opposite poles, and stains much more feebly than the chromatic fibres. The loops of the chromatic star then arrange themselves in the equatorial plane of the spindle, and bending round turn their closed ends towards the periphery of the nucleus and the cell. The next stage marks an important step in the process of division of the nucleus. The two longitudinal portions, into which each looped thread had previously split, now separate from each other, and whilst one part migrates to one pole of the spindle, the other moves to the opposite pole, and the free ends of each loop are directed towards its equator (meta- kinesis). By this division of the chromatin fibres, and their separation from each other to opposite poles of the spindle, two star-like chromatin figures are produced (dyaster). Each group of fibres thickens, shortens, becomes surrounded by a membrane, and forms a new or daughter nucleus (dispirem). Two nuclei therefore have arisen within the cell by the division of that which had previously existed, and the expression formulated by Flemming—ommnis nucleus e nucleo—is justified. Whilst this stage is in course of being completed, the body of the cell becomes constricted in the equatorial plane of the spindle, and, as the constriction deepens, it separates into two parts, each containing a daughter nucleus, so that two nucleated cells have arisen out of a pre-existing cell. A repetition of the process in each of these cells leads to the formation of other cells, and, although modifications in details are found in different species of plants and animals, the multiplication of cells in the egg and in the tissues generally on similar lines is now a thoroughly established fact in biological science; 14 REPORT—1900. In the study of karyokinesis, importance has been attached to the number of chromosomes in the nucleus of the cell. Flemming had seen in the Salamander twenty-four chromosome fibres, which seems to be a constant number in the cells of epithelium and connective tissues. In other cells again, especially in the ova of certain animals, the number is smaller, and fourteen, twelve, four, and even two only have been described, The theory formulated by Boveri that the number of chromosomes is con- stant for each species, and that in the karyokinetic figures corresponding numbers are found in homologous cells, seems to be not improbable. In the preceding description I have incidentally referred to the appear- ance in the proliferating cell of an achromatic spindle-like figure. Although this was recognised by Fol in 1873, it is only during the last ten or twelve years that attention has been paid to its more minute arrangements and possible signification in cell-division. The pole at each end of the spindle lies in the cell plasm which sur- _ rounds the nucleus. In the centre of each pole is a somewhat opaque spot (central body) surrounded by a clear space, which, along with the spot, constitutes the centrosome or the sphere of attraction. From each centrosome extremely delicate lines may be seen to radiate in two direc- tions. One set extends towards the pole at the opposite end of the spindle and, meeting or coming into close proximity with radiations from it, con- stitutes the body of the spindle, which, like a perforated mantle, forms an imperfect envelope around the nucleus during the process of division, The other set of radiations is called the polar, and extends in the region of the pole towards the periphery of the cell. The question has been much discussed whether any constituent part of the achromatic figure, or the entire figure, exists in the cell as a permanent structure in its resting phase ; or if it is only present during the process of karyokinesis. During the development of the egg the formation of young cells, by division of the segmentation nucleus, is so rapid and continuous that the achromatic figure, with the centrosome in the pole of the spindle, is a readily recognisable object in each cell. The polar and spindle-like radiations are in evidence during karyokinesis, and have apparently a temporary endurance and function. On the other hand, van Beneden and Boveri were of opinion that the central body of the centrosome did not disappear when the division of the nucleus came to an end, but that it remained as a constituent part of a cell lying in the cell plasm near to the nucleus. Flemming has seen the central body with its sphere in leucocytes, as well as in epithelial cells and those of other tissues. Subsequently Heidenhain and other histologists have recorded similar observations. It would seem, therefore, as if there were reason to regard the centrosome, like the nucleus, as a permanent constituent of a cell. This view, however, is not universally entertained. Tf not always capable of demonstration in the resting stage of a cell, it is doubtless to be regarded as potentially present, and ready to assume, ADDRESS. 15 along with the radiations, a characteristic appearance when the process of nuclear division is about to begin. One can scarcely regard the presence of so remarkable an appearance as the achromatic figure without associating with it an important function in the economy of the cell. As from the centrosome at the pole of the spindle both sets of radiations diverge, it is not unlikely that it acts as a centre or sphere of energy and attraction. By some observers the radiations are regarded as substantive fibrillar structures, elastic or even contractile in their properties. Others, again, look upon them as morpho- logical expressions of chemical and dynamical energy in the protoplasm of the cell body. On either theory we may assume that they indicate an influence, emanating, it may be, from the centrosome, and capable of being exercised both on the cell plasm and on the nucleus contained in it. On the contractile theory, the radiations which form the body of the spindle, either by actual traction of the supposed fibrille or by their pressure on the nucleus which they surround, might impel during karyokinesis the dividing chromosome elements towards the poles of the spindle, to form there the daughter nuclei. On the dynamical theory, the chemical and physical energy in the centrosome might influence the cell plasm and the nucleus, and attract the chromosome elements of the nucleus to the poles of the spindle. The radiated appearance would therefore be consequent and attendant on the physico-chemical activity of the centrosome. One or other of these theories may also be applied to the interpretation of the significance of the polar radiations. Cell Plasm. In the cells of plants, in addition to the cell wall, the cell body and the cell juice require to be examined. The material of the cell body, or the cell contents, was named by von Mohl (1846) protoplasm, and consisted of a colourless tenacious substance which partly lined the cell wall (primordial utricle), and partly traversed the interior of the cell as deli- cate threads enclosing spaces (vacuoles) in which the cell juice was con- tained. In the protoplasm the nucleus was embedded. Nageli, about the same time, had also recognised the difference between the protoplasm and the other contents of vegetable cells, and had noticed its nitrogenous com- position. Though the analogy with a closed bladder or vesicle could no longer be sustained in the animal tissues, the name ‘cell’ continued to be retained for descriptive purposes, and the body of the cell was spoken of as a more or less soft substance enclosing a nucleus (Leydig). In 1861 Max Schultze adopted for the substance forming the body of the animal cell the term ‘protoplasm.’ He defined a cell to be a particle of protoplasm in the substance of which a nucleus was situated. He regarded the protoplasm, as indeed had previously been pointed out by the botanist Unger, as essentially the same as the contractile sarcode which 16 REPORT— 1900. constitutes the body and pseudopodia of the Amceba and other Rhizopoda. As the term ‘protoplasm,’ as well as that of ‘bioplasm’ employed by Lionel Beale in a somewhat similar though not precisely identical sense, involves certain theoretical views of the origin and function of the body of the cell, it would be better to apply to it the more purely descriptive term ‘cytoplasm’ or ‘cell plasm.’ Schultze defined protoplasm as a homogeneous, glassy, tenacious material, of a jelly-like or’ somewhat firmer consistency, in which numerous minute granules were embedded. He regarded it as the part of the cell especially endowed with vital energy, whilst the exact function of the nucleus could not be defined. Based upon this conception of the jelly- like character of protoplasm, the idea for a time prevailed that a structure- less, dimly granular, jelly or slime destitute of organisation, possessed great physiological activity, and was the medium through which the phenomena of life were displayed. More accurate conceptions of the nature of the cell plasm soon began to be entertained. Briicke recognised that the body of the cell was not simple, but had a complex organisation. Flemming observed that the cell plasm contained extremely delicate threads, which frequently formed a network, the interspaces of which were occupied by a more homo- geneous substance. Where the threads crossed each other, granular particles (mikrosomen) were situated. Biitschli considered that he could recognise in the cell plasm a honeycomb-like appearance, as if it con- sisted of excessively minute chambers in which a homogeneous more or less fluid material was contained. The polar and spindle-like radiations visible during the process of karyokinesis, which have already been referred to, and the presence of the centrosome, possibly even during the resting stage of the cell, furnished additional illustrations of differentiation within the cell plasm. In many cells there appears also to be a difference in the character of the cell plasm which immediately surrounds the nucleus and that which lies at and near the periphery of the cell. The peri- pheral part (ektoplasma) is more compact and gives a definite outline to the cell, although not necessarily differentiating into a cell membrane. The inner part (endoplasma) is softer, and is distinguished by a more distinct granular appearance, and by containing the products specially formed in each particular kind of cell during the nutritive process. By the researches of numerous investigators on the internal organisa- tion of cells in plants and animals, a large body of evidence has now been accumulated, which shows that both the nucleus and the cell plasm con- sist of something more than a homogeneous, more or less viscid, slimy material. Recognisable objects in the form of granules, threads, or fibres can be distinguished in each. The cell plasm and the nucleus respectively are therefore not of the same constitution throughout, but possess poly- morphic characters, the study of which in health and the changes produced by disease will for many years to come form important matters for investigation, ADDRESS. 17 Function of Cells. Tt has already been stated that, when new cells arise within pre- existing cells, division of the nucleus is associated with cleavage of the cell plasm, so that it participates in the process of new cell-formation. Undoubtedly, however, its ré/e is not limited to this function. It also plays an important part in secretion, nutrition, and the special functions discharged by the cells in the tissues and organs of which they form morphological elements. Between 1838 and 1842 observations were made which showed that cells were constituent parts of secreting glands and mucous membranes (Schwann, Henle). In 1842 John Goodsir communicated to the Royal Society of Edinburgh a memoir on secreting structures, in which he established the principle that cells are the ultimate secreting agents ; he recognised in the cells of the liver, kidney, and other organs the character- istic secretion of each gland. The secretion was, he said, situated between the nucleus and the cell wall. At first he thought that, as the nucleus was the reproductive organ of the cell, the secretion was formed in the interior of the cell by the agency of the cell wall ; but three years later he regarded it as a product of the nucleus. The study of the process of spermatogenesis by his brother, Harry Goodsir, in which the head of the spermatozoon was found to correspond with the nucleus of the cell in which the spermatozoon arose, gave support to the view that the nucleus played an important part in the genesis of the characteristic product of the gland cell. The physiological activity of the cell plasm and its complex chemical constitution soon after began to be recognised. Some years before Max Schultze had published his memoirs on the characters of protoplasm, Briicke had shown that the well-known changes in tint in the skin of the Chameleon were due to pigment granules situated in cells in the skin which were sometimes diffused throughout the cells, at others concen- trated in the centre. Similar observations on the skin of the frog were made in 1854 by von Wittich and Harless. The movements were regarded as due to contraction of the cell wall on its contents. In a most interesting paper on the pigmentary system in the frog, pub- lished in 1858, Lord Lister demonstrated that the pigment granules moved in the cell plasma, by forces resident within the cell itself, acting under the influence of an external stimulant, and not by a contractility of the wall. Under some conditions the pigment was attracted to the centre of the cell, when the skin became pale ; under other conditions the pigment was diffused throughout the body and the branches of the cell, and gave to the skin a dark colour. It was also experimentally shown that a potent influence over these movements was exercised by the nervous system. The study of the cells of glands engaged in secretion, even when the 1900. *¢ 18 REPORT— 1900. secretion is colourless, and the comparison of their appearance when secretion is going on with that seen when the cells are at rest, have shown that the cell plasm is much more granular and opaque, and con- tains larger particles, during activity than when the cell is passive ; the body of the cell swells out from an increase in the contents of its plasm, and chemical changes accompany the act of secretion. Ample evidence, there- fore, is at hand to support the position taken by John Goodsir, nearly sixty years ago, that secretions are formed within cells, and lie in that part of the cell which we now say consists of the cell plasm ; that each secreting cell is endowed with its own peculiar property, according to the organ in which it is situated, so that bile is formed by the cells in the liver, milk by those in the mamma, and so on. Intimately associated with the process of secretion is that of nutri- tion. As the cell plasm lies at the periphery of a cell, and as it is, alike in secretion and nutrition, brought into closest relation with the sur- rounding medium, from which the pabulum is derived, it is necessarily associated with nutritive activity. Its position enables it to absorb nutritive material directly from without, and in the process of growth it increases in amount by interstitial changes and additions throughout its substance, and not by mere accretions on its surface. Hitherto I have spoken of a cell as a unit, independent of its neighbours as regards its nutrition and the other functions which it has to discharge. The question has, however, been discussed, whether in a tissue composed of cells closely packed together cell plasm may not give origin to processes or threads which are in contact or continuous with corresponding processes of adjoining cells, and that cells may therefore, to some extent, lose their individuality in the colony of which they are members. Appearances were recognised between 1863 and 1870 by Schro6n and others in the deeper cells of the epidermis and of some mucous membranes which gave sanction to this view, and it seems possible, through contact or continuity of threads connecting a cell with its neigh- bours, that cells may exercise a direct influence on each other. Nageli, the botanist, as the foundation of a mechanico-physiological theory of descent, considered that in plants a network of cell plasm, named by him idio-plasm, extended throughout the whole of the plant, forming its specific molecular constitution, and that growth and activity were regulated by its conditions of tension and movements (1884). The study of the structure of plants with special reference to the presence of an intercellular network has for some years been pursued by Walter Gardiner (1882-97), who has demonstrated threads of cell plasm protruding through the walls of vegetable cells and continuous with similar threads from adjoining cells. Structurally, therefore, a plant may be conceived to be built up of a nucleated cytoplasmic network, each nucleus with the branching cell plasm surrounding it being a centre of activity. On this view a cell would retain to some extent its individuality, ADDRESS. 19 though, as Gardiner contends, the connecting threads would be the medium for the conduction of impulses and of food from a ceil to those which lie around it. For the plant cell therefore, as has long been accepted in the animal cell, the wall is reduced to a secondary position, and the active con- stituent is the nucleated cell plasm. Itis not unlikely that the absence of a controlling nervous system in plants requires the plasm of adjoining cells to be brought into more immediate contact and continuity than is the case with the generality of animal cells, so as to provide a mechanism for harmonising the nutritive and other functional processes in the different areas in the body of the plant. In this particular, it is of interest to note that the epithelial tissues in animals, where somewhat similar connecting arrangements occur, are only indirectly associated with the nervous and vascular systems, so that, as in plants, the cells may require, for nutritive and other purposes, to act and react directly on each other. Nerve Cells. Of recent years great attention has been paid to the intimate struc- ture of nerve cells, and to the appearance which they present when in the exercise of their functional activity. A nerve cell is not a secreting cell; that is, it does not derive from the blood or surrounding fluid a pabulum which it elaborates into a visible, palpable secretion charac- teristic of the organ of which the cell is a constituent element, to be in due course discharged into a duct which conveys the secretion out of the gland. Nerve cells, through the metabolic changes which take place in them in connection with their nutrition, are associated with the pro- duction of the form of energy termed nerve energy, specially exhibited by animals which possess a nervous system. It has long been known that every nerve cell has a body in which a relatively large nucleus is situated. A most important discovery was the recognition that the body of every nerve cell had one or more processes growing out from it. More recently it has been proved, chiefly through the researches of Schulize, His, Golgi, and Ramon y Cajal, that at least one of the processes, the axon of the nerve cell, is continued into the axial cylinder of a nerve fibre, and that in the multipolar nerve cell the other processes, or dendrites, branch and ramify for some distance away from the body. A nerve fibre is therefore an essential part of the cell with which it is continuous, and the cell, its processes, the nerve fibre and the collaterals which arise from the nerve fibre collectively form a neuron or structural nerve unit (Waldeyer). The nucleated body of the nerve cell is the physiological centre of the unit. The cell plasm occupies both the body of the nerve cell and its pro- cesses. The intimate st#ucture of the plasm has, by improved methods of observation introduced during the last eight years by Nissl, and con- ducted on similar lines by other investigators, become more definitely understood. It has been ascertained that it possesses two distinct ° c2 20 REPORT—1900. characters which imply different structures. One stains deeply on the addition of certain dyes, and is named chromophile or chromatic sub- stance ; the other, which does not possess a similar property, is the achromatic network. The chromophile is found in the cell body and the dendritic processes, but not in the axon. It occurs in the form of granular particles, which may be scattered throughout the plasm, or aggregated into little heaps which are elongated or fusiform in shape and appear as distinct coloured particles or masses. The achromatic network is found in the cell body and the dendrites, and is continued also into the axon, where it forms the axial cylinder of the nerve fibre. It consists apparently of delicate threads or fibrille, in the meshes of which a homogeneous material, such as is found in cell plasm generally, is contained. In the nerve cells, as in other cells, the plasm is without doubt concerned in the process of cell nutrition. The achromatic fibrille exercise an important influence on the axon or nerve fibre with which they are continuous, and probably they conduct the nerve impulses which manifest themselves in the form of nerve energy. The dendritic processes of a multipolar nerve cell ramify in close relation with similar processes branching from other cells in the same group. The collaterals and the free end of the axon fibre process branch and ramify in association with the body of a nerve cell or of its dendrites. We cannot say that these parts are directly continuous with each other to form an intercellular network, but they are apparently in apposition, and through contact exer- cise influence one on the other in the transmission of nerve impulses. There is evidence to show that in the nerve cell the nucleus, as well as the cell plasm, is an effective agent in nutrition. When the cell is functionally active, both the cell body and the nucleus increase in size (Vas, G. Mann, Lugaro) ; on the other hand, when nerve cells are fatigued through excessive use, the nucleus decreases in size and shrivels ; the cell plasm also shrinks, and its coloured or chromophile constituent becomes diminished in quantity, as if it had been consumed during the prolonged use of the cell (Hodge, Mann, Lugaro). It is interesting also to note that in hibernating animals in the winter season, when their functional activity is reduced to a minimum, the chromophile in the plasm of the nerve cells is much smaller in amount than when the animal is leading an active life in the spring and summer (G. Levi). When a nerve cell has attained its normal size it does not seem to be capable of reproducing new cells in its substance by a process of karyo- kinesis, such as takes place when young cells arise in the egg and in the tissues generally. It would appear that nerve cells are so highly special- ised in their association with the evolution of nerve energy, that they have ceased to have the power of reproducing their kind, and the metabolic changes both in cell plasm and nucleus are needed to enable them to discharge their very peculiar function. Hence it follows that when a portion of the brain or other nerve-centre is destroyed, the ADDRESS. 21 injury is not repaired by the production of fresh specimens of their characteristic cells, as would be the case in injuries to bones and tendons. In our endeavours to differentiate the function of the nucleus from that of the cell plasm, we should not regard the former as concerned only in the production of young cells, and the latter as the exclusive agent in growth, nutrition, and, where gland cells are concerned, in the formation of their characteristic products. As regards cell reproduction also, though the process of division begins in the nucleus in its chromo- some constituents, the achromatic figure in the cell plasm undoubtedly plays a part, and the cell plasm itself ultimately undergoes cleavage. A few years ago the tendency amongst biologists was to ignore or attach but little importance to the physiological use of the nucleus in the nucleated cell, and to regard the protoplasm as the essential and active constituent of living matter ; so much so, indeed, was this the case that independent organisms regarded as distinct species were described as con- sisting of protoplasm destitute of a nucleus; also that scraps of proto- plasm separated from larger nucleated masses could, when isolated, exhibit vital phenomena. There is reason to believe that a fragment of protoplasm, when isolated from the nucleus of a cell, though retaining its contractility and capable of nourishing itself for a short time, cannot increase in amount, act as a secreting structure, or reproduce its kind: it soon loses its activity, withers, and dies. In order that these qualities of living matter should be retained, a nucleus is by most observers regarded as necessary (Nussbaum, Gruber, Haberlandt, Korschelt), and that for the complete manifestation of vital activity both nucleus and cell plasm are required. Bacteria, The observations of Cohn, made about thirty years ago, and those of De Bary shortly afterwards, brought into notice a group of organisms to which the name ‘ bacterium’ or ‘ microbe’ is given. They were seen to vary in shape : some were rounded specks called cocci, others were straight rods called bacilli, others were curved or spiral rods, vibrios or spirille. All were characterised by their extreme minuteness, and required for their exami- nation the highest powers of the best microscopes. Many bacteria measure in their least diameter not more than 5,),,th of an inch, ith the diameter of a human white blood corpuscle. Through the re- searches of Pasteur, Lord Lister, Koch, and other observers, bacteria have been shown to play an important part in nature. They exercise a very re- markable power over organic substances, especially those which are com- plex in chemical constitution, and can resolve them into simpler combina- tions. Owing to this property, some bacteria are of great economic value, and without their agency many of our industries could not be pursued ; others again, and these are the most talked of, exercise a malign influ- ence in the production of the most deadly diseases which afflict man and the domestic animals, 22 REPORT—1900. Great attention has been given to the structure of bacteria and to their mode of propagation. When examined in the living state and magnified about 2,000 times, a bacterium appears as a homogeneous par- ticle, with a sharp definite outline, though a membranous envelope or wall, distinct from the body of the bacterium, cannot at first be recog- nised ; but when treated with reagents a membranous envelope appears, the presence of which, without doubt, gives precision of form to the bacterium. The substance within the membrane contains granules which can be dyed with colouring agents. Owing to their extreme minuteness it is difficult to pronounce an opinion on the nature of the chromatine granules and the substance in which they lie. Some observers regard this substance as nuclear material, invested by only a thin layer of protoplasm, on which view a bacterium would be a nucleated cell. Others consider the bacterium as formed of protoplasm containing granules capable of being coloured, which are a part of the protoplasm itself, and not a nuclear sub- stance. On the latter view, bacteria would consist of cell plasm enclosed in a membrane and destitute of a nucleus. Whatever be the nature of the granule-containing material, each bacterium is regarded as a cell, the minutest and simplest living particle capable of an independent existence that has yet been discovered. Bacteria cells, like cells generally, can reproduce their kind. They multiply by simple fission, probably with an ingrowth of the cell wall, but without the karyokinetic phenomena observed in nucleated cells. Each cell gives rise to two daughter cells, which may for a time remain attached to each other and form a cluster or a chain, or they may separate and become independent isolated cells. The multiplication, under favourable conditions of light, air, temperature, moisture, and food, goes on with extraordinary rapidity, so that ina few hours many thousand new indi- viduals may arise from a parent bacterium. Connected with the life-history of a bacterium cell is the formation in its substance, in many species and under certain conditions, of a highly refractile shiny particle called a spore. At first sight a spore seems as if it were the nucleus of the bacterium cell, but it is not always present when multiplication by cleavage is taking place, and when present it does not appear to take part in the fission. On the other hand, a spore, from the character of its envelope, possesses great power of resistance, so that dried bacteria, when placed in conditions favourable to germination, can through their spores germinate and resume an active existence. Spore formation seems, therefore, to be a provision for continuing the life of the bacterium under conditions which, if spores had not formed, would have been the cause of its death. The time has gone by to search for the origin of living organisms by a spontaneous aggregation of molecules in vegetable or other infusions, or from a layer of formless primordial slime diffused over the bed of the ocean. Living matter during our epoch has been, and continues to be, derived ADDRESS. 28 from pre-existing living matter, even when it possesses the simplicity of structure of a bacterium, and the morphological unit is the cell, Development of the Egg. As the future of the entire organism lies in the fertilised egg cell, we may now briefly review the arrangements, consequent on the process of segmentation, which lead to the formation, let us say in the egg of a bird, of the embryo or young chick. In the latter part of the last century, C. F. Wolff observed that the beginning of the embryo was associated with the formation of layers, and in 1817 Pander demonstrated that in the hen’s egg at first one layer, called mucous, appeared, then a second or serous layer, to be followed by a third, intermediate or vascular layer. In 1828 von Baer amplified our knowledge in his famous treatise, which from its grasp of the subject created a new epoch in the science of embryology. It was not, however, until the discovery by Schwann of cells as constant factors in the struc- ture of animals and in their relation to development that the true nature of these layers was determined. We now know that each layer consists of cells, and that all the tissues and organs of the body are derived from them. Numerous observers have devoted themselves for many years to the study of each layer, with the view of determining the share which it takes in the formation of the constituent parts of the body, more especially in the higher animals, and the important conclusion has been arrived at that each kind of tissue invariably arises from one of these layers and from no other. The layer of cells which contributes, both as regards the number and variety of the tissues derived from it, most largely to the formation of the body is the middle layer or mesoblast. From it the skeleton, the muscles, and other locomotor organs, the true skin, the vascular system, including the blood, and other structures which I need not detail, take their rise. From the inner layer of cells or hypoblast, the principal derivatives are the epithelial lining of the alimentary canal and of the glands which open into it, and the epithelial lining of the air-passages. The outer or epiblast layer of cells gives origin both to the epidermis or scarf skin and to the nervous system. It is interesting to note that from the same layer of the embryo arise parts so different in importance as the cuticle—a mere protecting structure, which is constantly being shed when the skin is subjected to the friction of a towel or the clothes—and the nervous system, including the brain, the most highly differentiated system in the animal body. How completely the cells from which they are derived had diverged from each other in the course of their differentiation in structure and properties is shown by the fact that the cells of the epidermis are continually engaged in reproducing new cells to replace those which are shed, whilst the cells of the nervous system have apparently lost the power of reproducing their kind, 24 REPORT—1900. In the early stage of the development of the egg, the cells in a given layer resemble each other in form, and, as far as can be judged from their appearance, are alike in structure and properties. As the development proceeds, the cells begin to show differences in character, and in the course of time the tissues which arise in each layer differentiate from each other and can-be readily recognised by the observer. To use the language of von Baer, a generalised structure has become specialised, and each of the special tissues produced exhibits its own structure and properties. These changes are coincident with a rapid multiplication of the cells by cleavage, and thus increase in size of the embryo accompanies specialisation of structure. As the process continues, the embryo gradually assumes the shape characteristic of the species to which its parents belonged, until at length it is fit to be born and to assume a separate existence. The conversion of cells, at first uniform in character, into tissues of a diverse kind is due to forces inherent in the cells in each layer. The cell plasm plays an active though not an exclusive part in the specialisation ; for as the nucleus influences nutrition and secretion, it acts as a factor in the differentiation of the tissues. When tissues so diverse in character as muscular fibre, cartilage, fibrous tissues, and bone arise from the cells of the middle or mesoblast layer, it is obvious that, in addition to the morphological differentiation affecting form and structure, a chemical differentiation affect- ing composition also occurs, as the result of which a physiological differen- tiation takes place. Corresponding differentiations also modify the cells of the outer and inner layers. The tissues and organs become fitted to transform the energy derived from the food into muscular energy, nerve energy, and other forms of vital activity. Hence the study of the develop- ment of the generalised cell layers in the young embryo enables us to realise how all the complex constituent parts of the body in the higher animals and in man are evolved by the process of cell growth and differen- tiation from a simple nucleated cell—the fertilised ovum. A knowledge of the cell and of its life-history is therefore the foundation-stone on which biological science in all its departments is based. If we are to understand by an organ in the biological sense a complex body capable of carrying on a natural process, a nucleated cell is an organ in its simplest form. In a unicellular animal or plant such an organ exists in its most primitive stage. The higher plants and animals again are built up of multitudes of these organs, each of which, whilst having its independent life, is associated with the others, so that the whole may act in unison for a common purpose. As in one of your great factories each spindle is engaged in twisting and winding its own thread, it is at the same time intimately associated with the hundreds of other spindles in its immediate proximity, in the manufacture of the yarn from which the web of cloth is ultimately to be woven. It has taken more than fifty years of hard and continuous work to bring our knowledge of the structure and development of the tissues and ADDRESS, 25 _ organs of plants and animals up to the level of the present day. Amidst the host of names of investigators, both at home and abroad, who have con- tributed to its progress, it may seem invidious to particularise individuals. There are, however, a few that I cannot forbear to mention, whose claim to be named on such an occasion as this will be generally conceded. Botanists will, I think, acknowledge Wilhelm Hofmeister as ar master in morphology and embryology, Julius von Sachs as the most important investigator in vegetable physiology during the last quarter of the century, and Strasburger as a leader in the study of the phenomena of nuclear division. The researches of the veteran Professor of Anatomy in Wiirzburg, Albert von Kélliker, have covered the entire field of animal histology. His first paper, published fifty-nine years ago, was followed by a suc- cession of memoirs and books on human and comparative histology and embryology, and culminated in his great treatise on the structure of the brain, published in 1896. Notwithstanding the weight of more than eighty years, he continues to prosecute histological research, and has published the results of his latest, though let us hope not his last, work during the present year. Amongst our own countrymen, and belonging to the generation which has almost passed away, was William Bowman. His investigations between 1840 and 1850 on the mucous membranes, muscular fibre, and the structure of the kidney, together with his researches on the organs of sense, were characterised by an acuteness of observation and of interpreting difficult and complicated appearances which has made his memoirs on these subjects landmarks in the history of histological inquiry. Of the younger generation of biologists Francis Maitland Balfour, whose early death is deeply deplored as a loss to British science, was one of the most distinguished. His powers of observation and philosophic perception gave him a high place as an original inquirer, and the charm of his personality—for charm is not the exclusive possession of the fairer sex—endeared him to his friends. General Morphology. Along with the study of the origin and structure of the tissues of organised bodies, much attention has been given during the century to the parts or organs in plants and animals, with the view of determining where and how they take their rise, the order of their formation, the changes which they pass through in the early stages of development, and their relative positions in the organism to which they belong. Investi- gations on these lines are spoken of as morphological, and are to be dis- tinguished from the study of their physiological or functional relations, though both are necessary for the full comprehension of the living arganism. 26 REPORT—1900. The first to recognise that morphological relations might exist between the organs of a plant, dissimilar as regards their function, was the poet Goethe, whose observations, guided by his imaginative faculty, led him to declare that the calyx, corolla, and other parts of a flower, the scales of a bulb, &c., were metamorphosed leaves, a principle generally accepted by botanists, and indeed extended to other parts of a plant, which are referred to certain common morphological forms although they exercise different functions. Goethe also applied the same principle in the study of the skeletons of vertebrate animals, and he formed the opinion that the spinal column and the skull were essentially alike in construction, and consisted of vertebre, an idea which was also independently conceived and advocated by Oken. The anatomist who in our country most strenuously applied himself to the morphological study of the skeleton was Richard Owen, whose know- ledge of animal structure, based upon his own dissections, was unrivalled in range and variety. He elaborated the conception of an ideal, archetype vertebrate form which had no existence in nature, and to which, subject to modifications in various directions, he considered ali vertebrate skeletons might be referred. Owen’s observations were conducted to a large extent on the skeletons of adult animals, of the knowledge of which he was a master. Asin the course of development modifications in shape and in the relative position of parts not unfrequently occur and their original character and place of origin become obscured, it is difficult, from the study only of adults, to arrive at a correct interpretation of their morphological significance. When the changes which take place in the skull during its development, as worked out by Reichert and Rathke, became known and their value had become appreciated, many of the conclusions arrived at by Owen were challenged and ceased to be accepted. It is, however, due to that eminent anatomist to state from my personal knowledge of the condition of anatomical science in this country fifty years ago, that an enormous impulse was given to the study of comparative morphology by his writings, and by the criticisms to which they were subjected. There can be no doubt that generalised arrangements do exist in the early embryo which, up to a certain stage, are common to animals that in their adult condition present diverse characters, and out of which the forms special to different groups are evolved. As an illustration of this principle, I may refer to the stages of development of the great arteries in the bodies of vertebrate animals. Originally, as the observations of Rathke have taught us, the main arteries are represented by pairs of symmetrically arranged vascular arches, some of which enlarge and con- stitute the permanent arteries in the adult, whilst others disappear. The increase in size of some of these arches, and the atrophy of others, are so constant for different groups that they constitute anatomical features as distinctive as the modifications in the skeleton itself. Thus in mam- mals the fourth vascular arch on the left side persists, and forms the arch ADDRESS. 2 of the aorta ; in birds the corresponding part of the aorta is an enlarge- ment of the fourth right arch, and in reptiles both arches persist to form the great artery. That this original symmetry exists also in man we know from the fact that now and again his body, instead of correspond- ing with the mammalian type, has an aortic arch like that which is natural to the bird, and in rarer cases even to the reptile. A type form common to the vertebrata does therefore in such cases exist, capable of evolution in more than one direction. The reputation of Thomas Henry Huxley as a philosophic compara- tive anatomist rests largely on his early perception of, and insistence on, the necessity of testing morphological conclusions by a reference to the development of parts and organs, and by applying this principle in his own investigations. The principle is now so generally accepted by both botanists and anatomists that morphological definitions are regarded as depending essentially on the successive phases of the development of the parts under consideration. The morphological characters exhibited by a plant or animal tend to be hereditarily transmitted from parents to offspring, and the species is perpetuated. In each species the evolution of an individual, through the developmental changes in the egg, follows the same lines in all the individuals of the same species, which possess therefore in common the features called specific characters. The transmission of these charac- ters is due, according to the theory of Weismann, to certain properties possessed by the chromosome constituents of the segmentation nucleus in the fertilised ovum, named by him the germ plasm, which is continued from one generation to another, and impresses its specific character on the egg and on the plant or animal developed from it. As has already been stated, the special tissues which build up the bodies of the more complex organisms are evolved out of cells which are at first simple in form and appearance. During the evolution of the individual, cells become modified or differentiated in structure and function, and so long as the differentiation follows certain prescribed lines the morpho- logical characters of the species are preserved. We can readily conceive that, as the process of specialisation is going on, modifications or variations in groups of cells and the tissues derived from them, notwithstanding the influence of heredity, may in an individual diverge so far from that which is characteristic of the species as to assume the arrangements found in another species, or even in another order. Anatomists had indeed long recognised that variations from the customary arrangement of parts occasionally appeared, and they described such deviations from the current descriptions as irregularities. Darwinian Theory. The signification of the variations which arise in plants and animals had not been apprehended until a flood of light was thrown on the entire 28 REPORT— 1900. subject by the genius of Charles Darwin, who formulated the wide- reaching theory that variations could be transmitted by heredity to younger generations. In this manner he conceived new characters would arise, accumulate, and be perpetuated, which would in the course of time assume specific importance. New species might thus be evolved out of organisms originally distinct from them, and their specific characters would in turn be transmitted to their descendants. By a continuance of this pro- cess new species would multiply in many directions, until at length from one or more originally simple forms the earth would become peopled by the infinite varieties of plant and animal organisms which have in past ages inhabited, or doat present inhabit, our globe. The Darwinian theory may therefore be defined as Heredity modified and influenced by Variability. It assumes that there is an heredity quality in the egg which, if we take the common fowl] for an example, shall continue to produce similar fowls. Under conditions, of which we are ignorant, which occasion molecular changes in the cells and tissues of the developing egg, variations might arise, in the first instance probably slight, but becoming intensified in successive generations, until at length the descendants would have lost the characters of the fowl and have become another species. No precise estimate has been arrived at, and indeed one does not see how it is possible to obtain it, of the length of years which might be required to convert a variation, capable of being transmitted, into a new and definite specific character. The circumstances which, according to the Darwinian theory, deter- mined the perpetuation by hereditary transmission of a variety and its assumption of a specific character depended, it was argued, on whether it possessed such properties as enabled the plant or animal in which it appeared to adapt itself more readily to its environment, 7.¢. to the surrounding conditions. If it were to be of use the organism in so far became better adapted to hold its own in the struggle for existence with its fellows and with the forces of nature operating on it. Through the accumulation of useful characters the specific variety was perpetuated by natural selection so long as the conditions were favourable for its existence, and it survived as being the best fitted te live. In the study of the transmission of variations which may arise in the course of develop- ment it should not be too exclusively thought that only those variations are likely to be preserved which can be of service during the life of the individual, or in the perpetuation of the species, and possibly available for the evolution of new species. It should also be kept in mind that morphological characters can be transmitted by hereditary descent, which, though doubtless of service in some bygone. ancestor, are in the new conditions of life of the species of no physiological value. Our knowledge of the structural and functional modifications to be found in the human body, in connection with abnormalities and with tendencies or predisposition to diseases of various kinds, teaches us that ADDRESS. 29 characters which are of no use, and indeed detrimental to the individual, may be hereditarily transmitted from parents to offspring through a suc- cession of generations. Since the conception of the possibility of the evolution of new species from pre-existing forms took possession of the minds of naturalists, attempts have been made to trace out the lines on which it has proceeded. The first to give a systematic account of what he conceived to be the order of succession in the evolution of animals was Ernst Haeckel, of Jena, in a well-known treatise. Memoirs on special departments of the subject, too numerous to particularise, have subsequently appeared. The problem has been attacked along two different lines: the one by embryologists, of whom may be named Kowalewsky, Gegenbaur, Dohrn, Ray Lankester, Balfour, and Gaskell, who with many others have conducted careful and methodical inquiries into the stages of development of numerous forms belonging to the two great divisions of the animal kingdom. Inverte- brates, as well as vertebrates, have been carefully compared with each other in the bearing of their development and structure on their affinities and descent, and the possible sequence in the evolution of the Vertebrata from the Invertebrata has been discussed. The other method pursued by palzontologists, of whom Huxley, Marsh, Cope, Osborne, and Traquair are prominent authorities, has been the study of the extinct forms pre- served in the rocksand the comparison of their structure with each other and with that of existing organisms. In the attempts to trace the line of descent the imagination has not unfrequently been called into play in con- structing various conflicting hypotheses. Though from the nature of things the order of descent is, and without doubt will continue to be, ever a matter of speculation and inference and not of demonstration, the study of the subject has been a valuable intellectual exercise and a powerful stimulant to research. We know not as regards time when the fiat went forth, ‘Let there be Life, and there was Life.’ All we can say is that it must have been in the far-distant past, at a period so remote from the present that the mind fails to grasp the duration of the interval. Prior to its genesis our earth consisted of barren rock and desolate ocean. When matter became endowed with Life, with the capacity of self-maintenance and of resisting external disintegrating forces, the face of nature began to undergo a momentous change. Living organisms multiplied, the land became covered with vegetation, and multitudinous varieties of plants, from the humble fungus and moss to the stately palm and oak, beautified its surface and fitted it to sustain higher kinds of living beings. Animal forms appeared, in the first instance simple in structure, to be followed by others more complex, until the mammalian type was produced. The ocean also became peopled with plant and animal organisms, from the microscopic diatom to the huge leviathan. Plants and animals acted and 30 REPORT—1900. reacted on each other, on the atmosphere which surrounded them and on the earth on which they dwelt, the surface of which became modified in character and aspect. At last Man came into existence. His nerve-energy, in addition to regulating the processes in his economy which he possesses in common with animals, was endowed with higher powers. When trans- lated into psychical activity it has enabled him throughout the ages to progress from the condition of a rude savage to an advanced stage of civilisation ; to produce works in literature, art, and philosophy which have exerted, and must continue to exert, a lasting influence on the development of his higher Being ; to make discoveries in natural and physical science ; to acquire a knowledge of the structure of the earth, of the ocean in its changing aspects, of the atmosphere and the stellar universe, of the chemical composition and physical properties of matter in its various forms, and to analyse, comprehend, and subdue the forces of nature. By the application of these discoveries to his own purposes Man has, to a large extent, overcome time and space ; he has studded the ecean with steamships, girdled the earth with the electric wire, tunnelled the lofty Alps, spanned the Forth with a bridge of steel, invented machines and founded industries of all kinds for the promotion of his material welfare, elaborated systems of government fitted for the management of great communities, formulated economic principles, obtained an insight into the laws of health, the causes of infective diseases, and the means of controlling and preventing them. When we reflect that many of the most important discoveries in abs- tract science and in its applications have been made during the present century, and indeed since the British Association held its first meeting in the ancient capital of your county sixty-nine years ago, we may look forward with confidence to the future. Every advance in science provides a fresh platform from which a new start can be made. The human intel- lect is still in process of evolution. The power of application and of concentration of thought for the elucidation of scientific problems is by no means exhausted. In science is no hereditary aristocracy. The army of workers is recruited from all classes. The natural ambition of even the private in the ranks to maintain and increase the reputation of the branch of knowledge which he cultivates affords an ample guarantee that the march of science is ever onwards, and justifies us in proclaiming for the next century, as in the one fast ebbing to a close, that Great is Science, and it will prevail. REPORTS ON THH STATE OF SCIENCE. REPORTS ON THE STATE OF SCIENCE. Meteorological Observatory, Montreal.—Report of the Committee, con- sisting of Professor H. L. CaLLenpAR (Chairman), Professor C, McLeop (Secretary), Professor F. Apams, aid Mr. R. F. Stupart, appointed for the purpose of establishing a Meteorological Observatory on Mount Royal, Montreal. [PLATE I.] THE following preliminary report has been received from the observers :— The difference of temperature between the College Observatory and the top of Mount Royal is continuously recorded by means of a Callendar Electric Recorder and a pair of differential platinum thermometers. The thermometers are of the usual pattern, giving a change of 2 ohms for 100° Fahr., and the scale of the record is one-fifth of an inch to the degree Vahr. By a simple change in the connections the actual tempera- ture at either station can be recorded separately instead of the difference of temperature between the two. The thermometer at the top of the mountain is placed on a platform 50 feet above the ground and 850 feet above sea level. The other thermometer is at a height of 4 feet above the ground, and 180 feet above sea level. The distance between the two is rather more than a mile. The recorder is placed in the College Observa- tory at the lower station, and is connected to the distant thermometer by four separate lines of No. 12 copper wire erected on poles with glass insulators, and covered with weather-proof insulation ordinarily used for telephone work. The recorder is of the original Callendar pattern, and was made at the McDonald Physics Building in 1897. The line to the mountain has been broken by storm on several occa- sions ; parts of it have sometimes been carried away by thieves ; on one occasion the line was struck by lightning, the thermometers were de- stroyed, and the instrument burnt out ; on another occasion the instrument was burnt out through an accidental short circuit of the electric lighting current. The original thermometers which were damaged by lightning have been replaced by new and improved instruments, and all other damages have been repaired, so that the whole apparatus is at present in good running condition. Great delay has been caused by these accidents ; and this, coupled with pressure of other work on the observers, has made it pepossiil to secure up to the present date a sufficiently extended series : a) ; oD 34 . REPORT—1900. of observations to be of value for the general discussion of results. To show the nature of the records, and the working of the apparatus, a sample record sheet for August 21, 22, 1900, including a zero test and two comparisons with mercury thermometers, which were read simultaneously at the two stations by separate observers, is given herewith. (Plate I.) The zero line on the chart was obtained by placing the thermometers at the two stations in melting ice simultaneously, and allowing them to remain for about an hour at this temperature. The differences between the simultaneous readings of the mercury thermometers at the two stations were plotted from this zero line, and show a very satisfactory agreement with the differential platinum thermometers, considering the continual variations of temperature and the difference in sensibility of the two instruments. The direction of the wind and the velocity in miles per hour are recorded by instruments placed on the summit and connected by lines to the electrical recording apparatus in the College Observatory at the lower station. The record for August 21, 22 exhibits a complete revolution in the direction of the wind from N.W. through E. and 8. and back to N.W. These changes in the direction of the wind frequently appear to be related to the changes in the difference of temperature. The amount of sunshine in tenths per hour recorded at the College Observa- tory is also marked on the charts, and the general weather conditions prevailing. The apparatus as at present arranged gives admirable results in fair weather, but it has been found impossible to preserve the insulation of the line during rain. This has steadily deteriorated since its erection, and the results cannot now be relied on when the rainfall is considerable, or for short periods after. This is unfortunate, as it would be interesting to study the changes of temperature occurring with the onset of rain. To completely obviate the insulation defects in bad weather, and to protect the line from thieves and lightning, it would be necessary to replace the present pole line with a lead-covered cable buried in the ground. It is hardly necessary to say that this was foreseen at the time when the line was originally projected, as all installations of platinum thermometers up to that date had been provided with lead-covered cables, especially in cases where the distance involved was considerable. The original estimate of 100/. for the apparatus was based on the assumption of a lead-covered cable. But when the British Association in 1897 were unable to grant more than 50/., it was decided to utilise the existing pole line rather than abandon the project entirely. There is still some hope that the necessary funds may be forthcoming for the replacement of the existing line by a cable ; but until this necessary improvement is effected it is feared that the scientific value of the work must be seriously impaired. Electrolysis and Electro-chemistry.—Report of the Committee, consisting of Mr. W. N. Suaw (Chairman), Mr. E. H. Grirrirus, Rev. T. C. Frrzpatrick, Mr. 8. Skinner, and Mr. W. ©. D. WHETHAM (Secretary), appointed to report on the Present State of our Know- ledge in Electrolysis and Electro-chemistry. Tux experiments on the conductivity of dilute aqueous solutions of salts and acids at the freezing point have been completed by Mr. Whetham, [Pate [] gare A BBiz| Peal fl ro filer else taeL oey ollege Observatory, Re “4 P | ~ Illustrating [Prats {} 70th Report Brit. Assoc., 1900.) McGill College Observatory, Record of difference of Temperature between Mount Royal and College, Aug, 21 ¢ 22, 1900. YIGTIOI NI VLNIOW WIND SUNSHINE eT E ERS BSR Re BARRE eee nee eee +++ eee ee eee eee eee | an | iB! enna Ll pp et t TW I SEE CELE ane im [ i F Poot TTT Core re +H ; See eee eee eee ] Gane Gheee Geel +E a + aaa Sam eee tH+44+ nS BEE A Gt iHEOE DER ean]: TA SS ooo te = Toot Tilustrating the Report on the Meteorological Observatory on Mount Royal, Montreal. ON ELECTROLYSIS AND ELECTRO-CHEMISTRY. 35 and the full results published in the ‘Philosophical Transactions of the Royal Society of London,’ series A, vol. exciv: 1900, p. 321. Curves and tables are given showing the values obtained for the ionisation. The méasurements of the freezing points of the same solutions, undertaken by Mr. Griffiths, are still in progress. It is hoped that his results will soon be ready, and that a useful comparison of the two lines of reséarch may then be made. The consumption of a carbon anode in electrolysis has formed the subject of some experiments by another member of the Committee, Mr. Skinner.! Carboh electrodes are used in many electrotechnhical processes, and their solution and disintegration form one of the chief difficulties to be overcome. It appears that whenever a highly oxidised product undergoes electrolytic decomposition the anion gives, directly or indirectly, a cotisiderable quantity of carbonic acid. The experiments show that as mucli as 85 per cent. of the escaping gases consists of carbon dioxide when a solution of potassium permanganate is the electrolyte. Since the publication in 1897 of the Committee’s Report on the Theoty of the Migration of Ions ahd of Specific Ionic Velocities, an important paper by Orme Masson has appeared,” giving an account of an experimental method of measuring ionic velocities and of the results for a number of ions. The original plan of the Committee, as arranged in 1890, included reports on the following additional sections :—§ d. Electro-chemical Thermo-dynamics ; § e. Electric Endosmose ; and § g. Numerical Relations. Information on some of these sections has already been made easily accessible. A small book,’ ‘ Das Leitvermiégen der Electrolyte,’ Leipzig, 1898, has been published by Dr. von Kohlrausch and Dr. Holborn, giving a complete account of the method of measuring electrolytic conductivity by means of alternating currents in conjunction with a telephone, with the precautions _ hecessary for accurate results. There are also tables of the conductivity of certain solutions, which may be used to standardise resistance vessels. The thermo-dynamics of electrolytic processes is in some degree covered by a Report by Professor E. F. J. Love on our Knowledge of the Thermo-dynamics of the Voltaic Cell, published by the Australasian Association for the Advancement of Science, Sydney, 1898. Since the original appointment of the Committee, very many and important researches upon the chemical phenomena resulting from or associated with the passage of electricity through gases have been published. In order to make the Committee’s Report in any way a complete sketch of the subject of electro-chemistry as now developed, its scope would have to be enlarged to include such phenomena as the conductivity of gases at high temperatures, and under the influence of other ionising agencies. The Committee feel unable to undertake such an extension of their work, and do not seek reappointment. 1 Proc. Camb. Phil. Soc., x. 261, 1900. 2 Phil. Trans., A, cxciii., 1899. b2 36 REPORT—1900; On Solar Radiation.— Report of the Commuttee, consisting of Dr G. JOHN- STONE Stoney (Chairman), Professor H. McLuop (Secretary), Sir G. G. Sroxes, Professor A. SCHUSTER, Sir H. E. Roscor, Captain Sir W: pe W. Asney, Dr. C. CHREE, Professor G. F'. FirZGERALD, Professor H. L. Catuenpar, Mr. W. EH. Wison, and Professor A. A. Rampaut, appointed to consider the best Methods of Recording the Direct Intensity of Solar Radiation. (Drawn up by Professor H. L. CaLLenpar. ) As already reported, the copper-cube actinometer constructed for this Committee, and described in the Report for 1886, was entrusted to Professor Callendar in August 1899 for comparison with his automatic recording instrument described in the Report for 1898. In the course of the past year a number of experiments have been made with this apparatus by Miss W. E. Walker, 1851 Exhibition Scholar, working at University College, London, under the direction of Professor Callendar. The object of the work was to obtain absolute measurements of radiation for the calibration of the more convenient form of continuous recorder. In its original form the copper-cube actinometer was not very well adapted, and probably was not intended, for absolute measurements ; but with some modifications very promising results have been already obtained, and it is believed that the method thus modified will lead to trustworthy and valuable determinations. The history of the copper-cube actinometer is contained in various reports communicated by this committee, of which the following is a brief summary. The method originally proposed was to concentrate the rays of the sun by means of a lens through a hole in one side of the cube on to . a central mercury thermometer with a flat bulb. The steady difference of temperature between the central thermometer and the walls of the cube would be approximately proportional to the intensity of solar radiation, and might be taken as a measure of the same in arbitrary units. To obtain the equivalent in absolute measure it would be necessary to know the rate of cooling of the thermometer and the coefficient of absorption of the bulb and of the lens by which the rays were concentrated . These might have been obtained by auxiliary experiments on the rate of heating or cooling under various conditions ; but as the mercury thermo- meters proved unsuitable in many respects, the apparatus was subsequently modified by the substitution of a copper disc and a thermo-junction for the central thermometer. This permitted the observation of smaller differences of temperature and the more accurate determination of the thermal capacity of the irradiated disc. The elementary theory of the instrument, assuming that for small differences of temperature the rate of cooling of the disc would be pro- portional to the difference of temperature between the disc and the walls of the cube, was given in the Report of the Committee for 1892. If 0 is the excess of temperature of the disc over the enclosure at any time ¢ measured from the commencement of the exposure to the radiation to be measured, and if 7 be the initial rate of rise of temperature of the disc in ON SOLAR RADIATION, OV degrees per second, and qf the rate of fall of temperature at any excess 0 if the radiation were cut off, we have evidently the equation di/dt=r—qd . ‘ 3 E al) the solution of which under the given initial conditions is d=(l—-e")r/q . i : : » (2) The limiting steady temperature of the disc when ¢ is infinite is 0°=7/g. In 1893 some experiments were recorded verifying the elementary theory and the constancy of the coefficient of cooling g. In 1896 a photographic recording device was applied to obtain the curves of heating of the disc by registering the deflections of the D’Arsonval galvanometer on a moving photographic plate. The curves proved to be approximately logarithmic, but the reduction of the results to absolute measure was not attempted. Absolute Measwrements.—If I be the intensity of radiation to be measured in watts per square centimetre, and A be the area in square centimetres normal to the rays over which the measured portion of the radiation is incident, the quantity of heat received is IA joules per second. This is equal to rJms, where 7 as already defined is the initial rate of rise of temperature of the disc when exposed to the radiation, J is the number of joules in one calorie, which may be taken as approximately 4:18 ; m is the mass, and s the specific heat of thedisc. In applying this method it is tacitly assumed that the whole of the disc is at a uniform temperature 0 at any moment during the rise of temperature ; it is also necessary to know accurately the specific heat s of the material of the disc, and to be able to calibrate the thermo-junction so as to interpret the indications of the galvanometer in degrees of temperature. Further, the rise of temperature must not exceed two or three degrees in order that q, the coefficient of cooling, may be taken as constant, and the rate of rise must be sufticiently slow to permit of accurate measurement, and of the uniform diffusion of heat throughout the disc. After some preliminary experiments with the apparatus it became evident that these conditions were not sufficiently satisfied by the disc and thermo-junction employed in the experiments already recorded. The disc was about two centimetres in diameter and half a millimetre thick. The aperture for admitting the radiation was about one centimetre. Under these conditions it was not possible without the use of lenses to ensure a sufficiently uniform distribution of the radiation over the surface of the disc, and the rate of rise of temperature was too rapid for accurate measurement. The disc was supported on a short iron wire nearly two millimetres thick, which conducted heat away from the centre of the dise so rapidly that the temperature of the junction was always very con- siderably below that of the disc. Owing to its form the thermo-junction could not be accurately calibrated, and the sensitiveness of the copper-iron couple, though suitable for powerful sources such as direct solar radiation, was far too small for accurate work with sources of constant intensity such as were required for absolute measurement. The Galvanometer supplied with the instrument was of the Ayrton Mather type, with a resistance of about 7‘5 ohms, and gave a deflection of about 2 millimetres at 1 metre per microvolt, equivalent to about 20 millimetres per degree with a copper-iron junction. In order to 38 REPORT—1900. increase the accuracy of reading, a good plane mirror was substituted for the original concave mirror, and observations were taken with a telescope and scale at a distance of about 3 metres. The definition of the image was such as to permit of reading with accuracy to a fifth of a millimetre. Owing to the gradual change or ‘drift’ of zero, due to imperfect elasticity of the suspension, which is always a serious source of error in galvano- meters of this type, it was found to be impossible to obtain sufficiently consistent observations by the deflection method. To minimise this source of error the potentiometer balance-method was adopted, and care was taken not to subject the suspension to excessive torsion. To increase the sensitiveness, the iron-copper thermo-junction was replaced by junctions of iron and german silver (30 microvolts per degree), and iron and con- stantan (52 microvolts). The wires employed for this purpose were very fine—about 0-2 millimetre—to minimise the cooling of the junctions by conduction, and their thermo-electric powers were determined by a special series of observations made on the particular pieces employed. With these improvements it was optically possible to observe a difference of temperature of a thousandth of a degree with certainty, as it corresponded to a deflection of about a quarter of a millimetre with the iron and constantan couple. Thermo-electric Sources of Hrror.—In observing small differences of temperature with a thermo-couple, assuming that drift of the galvano- meter zero is avoided by employing the balance method, the most trouble- some residual errors arise from accidental thermal effects due to small differences of temperature in other parts of the electric circuit, and in particular at the junctions of the bridge-wire, and at the point of contact of the slider. It is usual to employ german-silver or platinoid or platinum silver as the material for the bridge-wire to secure a low temperature- coefficient and high specific resistance. Unfortunately these materials give large thermal effects when joined to copper. The alloy known as manganin is greatly to be preferred to platinoid or constantan in this respect, but its surface is more liable to tarnish. The superiority of the bolometric method (platinum resistance) over the thermo-couple for accu- rate measurement of small differences of temperature depends chiefly on the relative ease with which these accidental thermal effects may be eliminated. In the present instance they were found to be so trouble- some that it was eventually decided to make the bridge-wire and the whole of the circuit, with the exception of the coupie itself, of pure copper. By adopting this method the accidental disturbances were reduced to a small fraction of a microvolt, without taking any special precautions to secure uniformity of temperature throughout the various parts of the measuring apparatus. The cold junctions of the thermo- couple were contained in a copper plug screwing into the copper cube, and were assumed to be at the same temperature as the walls of the cube. In order to secure this, and to minimise changes of temperature of the copper cube, it was found necessary to wrap the cube and the projecting plug in a considerable thickness of cotton-wool, even when exposed to feeble sources of radiation, The layer of felt surrounding the cube formed no protection for the copper plug containing the cold junction, and proved quite inadequate to prevent rapid changes of temperature when exposed to strong sources. Constant Source of Radiation.—-The necessity of a constant source of radiation for comparative measurements and tests was recognised at a ON SOLAR RADIATION, 39 very early period in the experiments. The first attempt at a constant source was an Argand burner with a very delicate pressure regulator, a given area of the brightest part of the flame being selected as the source. This proved to be a very good method of testing the variations in the quality of the gas, but had to be abandoned as a constant source of radia- tion. It was also objectionable on account of the difficulty of keeping the glass chimney uniformly clean, and because the excessive amount of heat generated disturbed the experimental conditions, and the gas fumes had the effect of tarnishing the contacts of the electrical apparatus and the metallic plates used as reflectors. A pair of one hundred eandle- power focus-lamps were then obtained from the Ediswan Company. These were designed to work on a pressure of 90 volts at an efficiency of about 3:6 watts per candle, and a current of 4 amperes. They were spherical in form and silvered on one half, which had the effect of nearly doubling the radiating power for a given current, while at the same time it ensured an almost perfect constancy in the proportion of radiation reflected from the rear of the source, which had proved a difficulty with the Argand burner. When used as constant sources of radiation the lamps were worked at a pressure of only 75 volts and a current of about three amperes, supplied by a large storage battery of forty-four cells, The battery was not used for any other purpose while the experi- ments were in progress, and was capable of maintaining the required pressure constant to a tenth of a volt for several hours under suitable conditions of charge. The pressure on the lamps was regulated and recorded during the experiments by means of an automatic recording potentiometer working on a scale of one inch to the volt. The readings of this instrument were adjusted by means of a Clark cell, and were accurate to about one part in 5,000. One of the focus-lamps was set apart as a standard, and was used only for occasional comparisons. When working at a voltage so far below that for which they were designed, the lamps were found to remain exceedingly constant. In the course of six months’ work the lamp in regular use did not vary with respect to the standard by more than one per cent., and its variations over short periods could easily have been controlled and corrected if the accuracy so far attained in the radiation measurements had made the application of such a correction desirable. The area of the incandescent grid was about one square inch, and the diameter of the bulb four and a half inches. The lamp was set to shine through an aperture of its own diameter in a double tin-plate screen, so as to include the whole of the radiation from the heated glass, but to exclude as far as possible radiation from the base of the lamp and heated objects in its immediate neighbourhood. This precaution was particularly important in comparing the indications of the tube form of radio-calorimeter with those to the bolometric sunshine receiver intended for the direct exposure of solar radiation, as the latter instrument was not provided with a screen and diaphragms for excluding lateral radiation, but was intended to integrate the vertical component of the whole radiation from the sky as well as that from the sun. Determination of the Initial Rate of Heating of the Disc.—To ensure uniformity of temperature of the disc, and a sufficiently slowrate of heating, it was found necessary to replace the original disc by a much thicker disc the size of which was chosen to be just sufficient to catch the whole of the rays incident on the aperture. Before commencing an observation, the reading of the galyanometer was observed with the slider at the zero of f% AO REPORT—1900. the bridge-wire in order to allow for any minute residual difference of temperature between the cube and the disc when the apparatus was screened from radiation. The time of exposure was recorded on an electric chronograph by the dropping of the screen on a suitable key. The sliding contact was then shifted to successive points on the bridge- wire, and the moment of balance at each point was observed and recorded on the chronograph. ‘These observations were continued for about five minutes, or as long as the rise continued sufficiently rapid. Occasional observations were then made to determine the final steady difference of temperature 6° during the next fifteen minutes, after which the tempera- ture remained steady. The following is a sample of observations taken with the copper-cuhe : Date, April 4, 1900, Observer, Miss W. E. WALKER. Temperature of Clark cell, 19:0° C. ; bridge-wire, 20°2° C. ; resistance per cm. of B.W., :001091 ohm ; P.D. per cm., ‘7795 microvolt ; diameter of disc, 1:40 cm. ; diameter of aperture in cube, 1:00 cm. ; distance of lamp from aperture, 60:0 cms. ; volts on lamp, 77:2 ; mass of copper dise, 08320 gramme ; Jms/A="4206. | ride | | 4 l | — | oe | Time¢ | Temperature 0 | q | r | I Le eck e) fata | (1) 398 | 7656 5966 | ‘o1036 | -01129 | 00475 (2) 59°8 | 159°35 | 8964 | *01084 | -01182 00497 (3) | 729 | Steady | 1:090=6° | —_ =7/q | == Solution of the Equations.—Assuming the elementary theory of the method as given by equation (2), the simplest method of procedure is to take the value of the ratio 7/¢ as given by the final steady difference of temperature 6°=1-090, and to calculate the values of g from the inter- mediate observations of ¢ and @ by substituting the observed value of 7 /q in equation (2). We thus obtain gt-=2'3026 log,,6°/(6°—6) »' . /) at ia Raa) The value of 7 is then found by the relation r=q0, and the intensity of radiation I by multiplying 7 by the constant factor Jms/A=-4206. The values thus obtained are given in the columns headed g, 7, I. They invariably exhibited a progressive increase with the time. The value of q could also be found by eliminating the ratio */q between any two observations, and solving the equation by trialfor g. Taking the observa- tions (1) and (2) at 39:8 and 59-8 ems. above given, we thus obtain q=00967, whence 7=-01103, and I=-00464, which illustrate the same tendency, being smaller than the results obtained by assuming the ratio of v to q from the final steady temperature. The focus-lamp in this experiment was set to shine through an aperture of nearly the same size as the incandescent grid, but this was found to be unsatisfactory, as the field of illumination was not sufficiently uniform for the bolometric receivers. This consideration, among others, ultimately necessitated the abandonment of the aperture method of limiting the radiation received by the disc. Effects of Lag.—It was clear from the results above quoted, and from a number of others obtained with the same apparatus with different discs ON SOLAR RADIATION. 41 at different distances and different rates of heating, that the equations already given did not satisfactorily represent the observations. In con- sidering the possible sources of constant error inherent in the method, it seemed unlikely that the assumption that the rate of loss of heat was proportional to the difference of temperature (q constant) could be seriously in error, as the whole difference of temperature did not exceed one or two degrees. The most probable explanation of the discrepancy appeared to be that time was required for the uniform distribution of heat through the disc, and that the indications of the thermo-junction were retarded by conduction of heat along the wires, and by lag in the movement of the galvanometer coil, which was necessarily very dead-beat when short-circuited on the couple. These various sources of error could all be approximately represented by assuming a constant time-lag in the readings ; a type of error which was necessarily inherent in the method, and could not have been detected by the experiments recorded in 1896. In order to eliminate the time-lag from the equations, it is only necessary to take two observations in addition to the final steady temperature. If we write the equations in the form (3) already given, and take the differ- ence, we thus obtain g (t/’ —t/)=2°3026 log,, (6°—6’)/(0°—@”) . . (4) Treating the observations already given in this manner we find q='01130. r=:01232. I=:00518. Time-lag=6°45 secs. With only three observations it is of course always possible to calculate a value of the lag to satisfy the readings exactly, but it appeared that a similar assumption satisfied the observations within the probable limits of error in those cases also in which a larger number of readings were taken. Defects of the Copper-cube Actinometer.—The excessive value of the time-lag observed in the observations with this apparatus appeared to be partly due to the impossibility of securing uniform illumination of the disc by the aperture method. It was necessary that the disc should be large enough to catch the whole of the radiation passing through the aperture in the cube, and this could not be secured without leaving a con- siderable margin at the edge of the disc which was either not illuminated at all, or only partly illuminated by the penumbra of the aperture. With the lamp at 60 cms. it was necessary to use a disc 1-40 cm. in diameter for an aperture of 1:00 cm. diameter. This was the more necessary because the construction of the apparatus, and the method of screwing in the copper plug by which the disc was supported, made it extremely difficult to centre the disc accurately, and to direct it so as to receive the rays normally and centrally. Another serious defect to which allusion has already been made, was the variation of temperature of the cube and the copper plug, which although greatly reduced was not entirely eliminated by the cotton- wool wrappings. For these and other reasons it was decided to design a new form of actinometer for the application of the same method in a manner more convenient for laboratory use. Tube-form of Radio-calorimeter—The terms ‘actinometer,’ ‘ bolo- meter,’ and ‘radio-micrometer,’ which are otherwise suitable for instru- ments of this class, have acquired special significations, and are in general use for instruments which are not designed for absolute measurements, 42, REPORT—1900, It appears therefore preferable to use the more general term ‘radio- calorimeter’ for this particular instrument, as it was not intended, like the ‘ pyrheliometers’ of Pouillet or Angstrom, for the direct measurement of solar radiation. The tube-form of radio-calorimeter consists of a pair of concentric tubes about nine inches long separated by an annular space of about a twentieth of an inch, through which water is caused to circulate in a spiral fashion by a helix of copper wire nearly fitting the space between the tubes. The inner tube has a diameter of about one inch, and is furnished with a series of sliding copper diaphragms, which can be set at suitable points to screen off any lateral radiation, and prevent internal reflection from the walls of the tube. The blackened copper disc for receiving and measuring the radiation is supported near the centre of the tube by means of the fine wires of the thermo-couple. The diameter of the disc is 1°30 cm., and it is set close behind a diaphragm of 14 mm. diameter, so that the whole of its surface is exposed to the radiation. In this arrangement the quantity of radiation measured is determined solely by the diameter of the disc and not by that of the apertures. The disc can be accurately centred and directed on the source of radiation by looking through a small hole at the back of the tube. The cold junctions of the thermo-couples are contained in fine copper tubes soldered to a sliding tube which carries the disc, and is a good fit for the inner tube of the water-jacket. Water at the temperature of the laboratory is con- tinuously pumped by a small motor from one large copper tank to another at a higher level, and flows back continuously and uniformly through the water-jacket of the radio-calorimeter. By this means the temperature of the jacket is maintained very constant without the necessity of making the instrument itself massive or unwieldy, Observations with different Coatings on the Dise.—With this apparatus it was possible to obtain much more consistent results owing to the greater steadiness of the experimental conditions and the greater ease of adjustment and manipulation. Among other tests, some comparative measurements were made of the relative efficiency of different coatings of black for the disc, of which the following may be taken as samples :— 1. Copper disc clean but not polished. Final excess 1:223° C, g= "00512, r=-00626, I=-00379. 2. Copper colour just visible through a thin film of smoke-black. Final excess 2°528° C. g=:00595, r=:01505, I= 00910. 3. Copper disc covered with thick opaque film of smoke-black. Final excess 2°375° C. g=:006354, r=-01508, I=-00912. 4. Copper disc covered with dead-black varnish of shellac and smoke- black. Final excess 2:159° C, g=-00703, r=:001517, I=-00918. 5. Same disc, but with new thermo-couple, thick smoke-film. Final excess 2°328° C. g='00642, r=-01494, I=-00904. 6. Same disc and couple, but thin black varnish ; back also covered. Final excess 1°831° C. g=-00812, r=-01487, I=:00900. It will be observed in the above results that the final excess tempera- ture (7/q) and the coefficient of cooling, g, vary considerably under differ- ent conditions, but that the results for the rate of heating, 7, and the intensity of radiation, g, agree fairly well for the different coatings of black. The same focus-lamp was used as a source in each case, at the same distance, and it is probable that the actual variations in the inten- sity of the radiation did not exceed one part in 500, The voltage on the ON SOLAR RADIATION, 43 lamp was kept within less than a tenth of a volt of 75:0 volts by the automatic recording potentiometer, and the observations were taken within a few days of each other. In case 1, with the clean metal surface, the value of the coefficient of cooling g=:00512 is nearly that due to convection and conduction alone, as the radiative power of clean metal is very small at these low temperatures, although the absorptive power for the lamp radiation is nearly 40 per cent. An extremely thin coating of smoke-black (2) suffices to raise the absorptive power for the lamp radiation nearly to its maximum, although the radiative power for rays of great wave-length is still very low, as shown by the small value of q='00595, and the high value of the final excess of temperature ¢ /q=2'528° C. The thicker coating of smoke-black (3) lowers the value of the final excess to 2°373° C., because the coefficient of cooling is in- creased in a much greater ratio than the absorptive power for the lamp radiation. It appears from the great increase of q, in case (4), that the dead-black varnish is a much more efficient radiator at low temperatures than the smoke-black, although the absorptive power for the lamp radia- tion is but slightly increased. The back of the disc was not covered in these experiments in order to obtain a greater rise of temperature. In ease (5), with a new thermo-couple, the diminution in the values of 7 and I, as compared with case (3), may be due simply to unavoidable errors of observation, or slight variations in the uniformity of the wires, or in the quality of the smoke-film ; but it may also be caused by a variation in the cooling of the junctions by conduction, due to slight differences in the attachment of the wires to the disc. In any case it is satisfactory to find that so large a change in the conditions produces a change of less than one per cent. in the result. Similarly, in case (6), the effect of blacking the back of the disc is to produce a very marked increase in the coefficient of cooling ; but although the rate of cooling by radiation is nearly twice as great as in case (5)—supposing that the conduction and convection effects remain the same as in case (1)—the diminution in the result for I, as compared with (4), is not greater than might reasonably be attributed to the thinness of the varnish, which possessed appreciable reflecting power. It is clear from the above summary that the method is capable of . giving fairly consistent results in spite of wide variations in the experi- mental conditions. But it is evidently necessary to investigate further the absorptive powers of different coatings for radiations of different qualities if it is desired to obtain an order of accuracy higher than one per cent. in the absolute results. Another correction of some importance is that for the cooling of the junction by conduction along the wires. This correction depends on the size of the wires and on their mode of attachment to the disc. Although enormously reduced by the adoption of very fine wires for the couple, it remains distinctly appreciable and requires further investigation. It is evidently possible to determine this correction by employing wires of different sizes simultaneously, or the whole correction may be included in the coefficient of cooling by a suit- able arrangement of the junction. Measurement of Solar Radiation.—Owing to the great intensity and incessant variations of solar radiation, it would not be possible to obtain absolute measurements directly by exposure of the instrument above described to direct sunshine, although such a course has been attempted with instruments of the class of Pouillet’s pyrheliometer. Even with the AA ~ REPORT—1900, water-jacket, the conditions of cooling are disturbed by the excessive intensity of the radiation, and the final excess of temperature is much too large to permit of the application of the elementary theory of the method. For these and other reasons it appeared preferable to employ the automatic recording instruments already described! for direct exposure to sunshine, and to calibrate the receivers in absolute measure by exposure to the radiation of the focus-lamps, which could be satisfactorily determined by the absolute method. Bolometric Sunshine Receivers.—These instruments are intended for recording on an arbitrary scale the vertical component of the radiation from the whole sky as well as the sun. This vertical component measures the heat received by the soil, and is probably the factor which chiefly influences the meteorological conditions at any part of the earth’s surface, so far as they depend on radiation. It is comparatively useless for this purpose to record merely the normal intensity of solar radiation, as the heat actually received by the earth’s surface depends so greatly on the altitude of the sun and the state of the sky. It is proved by actual experiment with these receivers, although it is by no means obvious @ priori, and will perhaps scarcely be credited at the first statement, that the heat received by reflection from the sky under certain conditions may amount to more than 40 per cent. of the whole vertical component. This being the case, the readings of an instrument which records only the normal intensity of direct sunshine, excluding the radiation from the sky, might give a very incorrect account of the total quantity of heat received by the soil. The form of bolometric receiver adapted for recording the vertical component consists of a differential pair of flat platinum ther- mometers, one blackened and the other bright, placed side by side in the same horizontal plane. The difference of temperature between the two, which is automatically recorded, is approximately a measure of the intensity of the vertical component of the radiation to which they are exposed. It would of course be possible, by providing the instrument with a water-jacketed tube and an equatorial mounting, to make it record the normal intensity of direct sunshine, excluding the greater part of the radiation from the sky ; but this would complicate the apparatus consider- ably, and it is doubtful whether the record would have so direct a bearing on meteorology. it is also certain that the coefficient of cooling by con- vection would vary at different angles of inclination, whereas it appears to be very constant in the horizontal position. Two of the bolometric receivers above described have already been compared with the radio-calorimeter by means of the focus-lamps. They were of slightly different patterns, and wound with wire of different sizes, six mils and four mils respectively, but they showed nearly the same difference of temperature when exposed to the same radiation at the same distance. This seems to show that the indications of such instruments are fairly comparable, even if they are not precisely alike. As we have already seen, the absorptive powers of different kinds of black do not appear to differ very much for this kind of radiation. The proportionality of the difference of temperature to the intensity of radiation was also tested by varying the distance from the lamp, and assuming that the radiation followed the law of the inverse square. This is very approxi- mately true for the focus-lamps, owing to the flatness of the radiating 1 B.A, Report, 1898. ON SOLAR RADIATION: A5 grid, provided that the distance is not too small. It is intended in the course of the ensuing year to continue the absolute measurements, and to test the performance of the automatic recorders under a greater variety of conditions, for which Mr. Wilson, of Daramona Observatory, has promised his assistance ; but enough has already been accomplished to show that the apparatus affords a very promising and practical method of recording and réducing to absolute measure the vertical intensity of radiation at any point of the earth’s surface. Uniformity of Size of Pages of Transactions.—Report of the Com- mittee, consisting of Professor 8. P. THomrson (Chairman), Mr. J. SWINBURNE (Secretary), Professor G. H. Bryan, Mr. C. V. Burton, Mr. R. T. Guazesprook, Professor A. W. RUCKER, and, Dr. G. JOHNSTONE STONEY, appointed to confer with British and Loreigqn Societies, publishing Mathematical and Physical Papers, as to the Desirability of securing Uniformity in the Size of the Pages of their Transactions and Proceedings. (Drawn up by J. SWINBURNE.) A LARGE number of journals were measured to find what dimensions it would be best to choose as standards. An account of this work was published in the Report for 1895, p. 77. Since that date a large volume of correspondence has been carried on with the English and foreign scientific societies. In most cases the societies’ publications come within the limits speci- fied in the first report. In some of the cases the societies agreed to alter their publications so as to come within the standard limits. In a few cases the societies prefer to continue the use of abnormal dimensions rather than alter their publications, especially when the pub- lication has been going on for many years. The importance of beginning a paper on the right-hand page is generally realised, but there are difficulties in carrying it out. In spite of this, a few of the societies are endeavouring to arrange that all important papers shall begin on the right-hand page. The Committee do not ask for reappointment. Determining Magnetic Force on Board Ship.—Report of the Conunittee, consisting of Professor A. W. Ricker (Chairman), Dr. C. H. Lees (Secretary), Lord Kevin, Professor A. ScHusTER, Captain CrEAK, Professor W. Stroup, Mr. C. VERNON Boys, and Mr. W. Watson, appointed to consider the most suitable Method of determining the Components of the Magnetic Force on Board Ship. AAN instrument which embodies the ideas of Captain Creak, mentioned in last year’s Report, has been constructed. Although specially designed for observations on board ship, it will probably from its strength of construc- tion be found suitable for travelling parties. The Committee apply for reappointment, with the unexpended grant of 10/. made last year. AG REPORT—1900. Tables of certain Mathematical Functions.—Report of the Committee consisting of Lord Keruvin (Chairman), Lieutenant-Colonel ALLAN CunnincHAM, f.EL. (Secretary), Dr. J. W. L. GLaisHEr, Professor A. G. GREENHILL, Professor W. M. Hicks, Professor A. LobeGe, and Major P. A. MacManon, f.A., appointed for caleulating Tables of certaan Mathematical Functions, and, if necessary, for taking steps to carry out.the calculations, and to publish the results in an accessible form. TuHE cost of printing the Tables (Binary Canon) was estimated at 135/. A grant of 75/. only was made at the Dover Meeting. As the Tables could not have been printed for this sum, application was made to the Royal Society for a grant in aid; and the Royal Society has grantéd the remaining sum (60/.) required. The Tables have been put in hand, and are now (September) nearly all in type: they should be finished before next Meeting. Meteorological Observations of Ben Nevis.—Report of the Committee, consisting of Lord M‘LaREN, Professor A. Crum Brown (Secretary), Sir Joun Murray, Professor CopEeLANnD, and Dr. ALEXANDER Bucuan. (Drawn up by Dr. Bucnan.) Tux Committee was appointed as in past years for the purpose of co-operating with the Scottish Meteorological Society in making metevro- logical observations at the two Ben Nevis Observatories. The hourly eye observations made by night as well as by day, which are a specialty of the High Level Observatory, have been made with complete regularity throughout the year by Mr. Rankin and his assistants. The health of the staff at the High Level Observatory continued good, and the laborious work of the observations has been carried on without the loss of an hour’s observations. The Directors desire to express their hearty thanks to Messrs. T. Affleck, George Ednie, M.A., J.S. Begg, M.A., G. A. 8. Tait, R. C. Marshall, and T. Kilgour for the invaluable service they rendered as volunteer observers during the summer of 1899, thus affording to the members of the staff the relief and rest they so much needed. Owing to the war. in South Africa some changes took place in the Observatory staff. In October J. Bell, reservist, was called out for service, and subsequently R. M. McDougall and D. Grant left to join the forces. At the Low Level Observatory at Fort William influenza of an acute form for a second time prevailed. But it is gratifying to add that no observations have been lost, and the arrears of copying and computations which necessarily occurred are being gradually worked off. The observations at the intermediate station at Ben Nevis were undertaken, single-handed, by Mr. D. W. Wilton. These valuable observations, together with the similar observations made at this station during the previous three summers, are being discussed under the superin- tendence of Mr. Omond. a ae principal results of the observations of 1899 are detailed in able I, 1899 Ben Nevis Ob- servatory Fort William Differences . Ben Nevis Ob- servatory Fort William Differences . Ben Nevis Ob- servatory Fort William Differences . Ben Nevis Ob- servatory Fort William Differences . Ben NevisOb- servatory Fort William Differences B en Nevis Ob- servatory Fort William Differences . Ben Nevis Ob- Servatory Fort William Differences . Ben Nevis Ob- servatory Fort William Differences . Ben Nevis Ob- servatory Fort William Differences . Ben Nevis Ob- servatory Fort William Differences . Ben Nevis Ob- servatory Ben Nevis Ob- servatory Fort William Differences . METEOROLOGICAL OBSERVATIONS ON BEN NEVIS. 4 Tas.e I, | Jan. | Feb. |March| April | May | June | July | Aug. | Sept. | Oct. Nov.| Dec. | Year Mean Pressure in Inches. 25°048) 25°149) 25°317| 25°146| 25°431) 25°559| 25°528) 25°598| 25-209) 25°379) 25°321| 25°163) 25°321 29°640| 29'738] 29°944) 29°730| 30-008) 30043] 30-012) 30053] 29:707| 29-923) 29875] 29:775] 29'871 4°593| 4°589| 4°627| 4:584| 4°577| 4-484| 4-484] 4-455| 4-498] 4.544] 4°554| 5°612| 4-550 Mean Temperatures. 287 | 265 | 253 | 264] aro | a7 | 451 | 487 | ao] sx7 | ata | of7 | asta 37°6 | 39:0 | 403 | 48:0 | 47-7 | 57-4] 584] 60:6 | 522] 48-7] 48:3] 381] 476 13°9 | 12°5 | 150 | 16°6 | 15 13°7 | 153 | 11°9 | 168 | 15°0 | 160 | 14:4 | 14:7 Eautremes of Temperature, Maxima. 35°1 | 39-2} 460 | 41:3 | 47°0 | 606 | 57-4 | 63:5 | 506] 48:2) 43:0) 40:0 | 63°5 520 | 500 | 544] 62-0] 660! 762! 711) 803] 654] 615 | 623) 533) 803 169 | 108 | S84] 207 | 19:0 | 156 | 13:7 | 16-81 14:8 | 13:3 | 184 | 13:3 | 16:8 Extremes of Temperature, Minima. 122 | 106 69 | 13-1 | 200 | 303 | 386 | 381] 23:3 | 19:9 | 21:0) 108 69 231 | 24:5 | 21:0 | 26-4 | 322 | 48:7 | 47-7 | 46:2 | 34:0 | 326 | 32:2 | 17-4] 17-4 10:9 | 13:9 | 141 | 13:3 | 122 | 13:4 | 141 | 1211 107 | 197] 11-2] G66 | 105 Rainfall, in Tnches. 15°30 | 10°56 | 25°21] 17°01| 688) 7°61) 15°23| 5°58] 20°78] 18+11| 32°48) 12°55 |187°30 7°38| 4:91| 865} 5°37] 256]- 205] 445] 1:77} 9-11} 9:10] 13:97| 5:96) 74:58 792| 6°65 | 16°56] 1164 4°32] 5°56/ 10-78; 3:81] 11-67] 901] 19-4 | 6-59 |119-72 Rainfall, Greatest Daily Fail. 1:82 a 334) 3:97) 1:87; 1:19] 3:21] 1:21] 226) 3:78) 4:33] 2:98) 4:33 1:74} 0°86) 1:86] 0:76| 0-48) 056| 1:26) 054] 1:50| 1:48] 1°68] 0-92] 1:74 0°08| 1:03 | 1'98| 3°21] 1:39| O63) 1:95] O67! O76} 2:30| 2°65; 2:06] 2°59 Number of Days 1 in. or more fell. 7 3 11 4 2 3 5 1 Ul 6 13 4 | 66 1 0 2 0 0 0 1 0 1 4 3 0 | 12 6 3 9 4 2 3 40), 1 6 ee) ala) 4 | 54 Number of Days 0:01 in. 07 more fell. 22 11 27 26 14 20 23 12 28 22 26 22 | 253 21 /| 13 | 22°) 20°) 11 f 14-| 19 | 12 ) 96 | 90 | 96 | 19° | 223 1 2 5 6 3 6 4 0 2 2 0 3 | 30 Mean Rainband (scale 0-8). 18 15 20 2°2 23 2'2 30 20 2:2 29 27 17 2'2 31 | 29 | 33 | 36 | 35 | 39 | 39 | 41 |] 40] 41 | 48 | 32 | 3-7 ASPs Me lca ede Teo h)|) 1%) | O'ON | Sov eas sy east fT Ih alee Number of Hours of Bright Sunshine. 33 79 | 52 56 | 164] 153] 60 | 212 12 52 12] 12 897 26 71 By 112/ 197) 168] 89 | 231 73 69 12 8 | 1,139 7 sl 31 56) 9638 | 151: 29 {eb e anh | 17 oO; 4 | 242 Mean Hourly Velocity of Wind, in Miles. 19 | DORs He Vem aon |) Tt | 10 | 10 | t2)s|y 28 | 19 | 16 | 16 Mean Percentage of Cloud. 85 68 86 88 71 73 92 60 96 86 95 88 | 82 Com\csea ie 79) W 74. 68.) 70) | 86) iP be. | 80) |, 78° | 87 OP si 1 oem 10 5 7 14 3 3 6 6 16 13 8 7 8 48 REPORT—1900. This table shows for 1899 the mean monthly and extreme pressure and temperature, amounts of rainfall with the number of days of rain and the days on which the amount equalled or exceeded one inch ; the hours of sunshine, the mean percentage of cloud, the mean velocity of the wind in miles per hour at the top of the mountain, and the mean rainband at both observatories. The mean barometric pressures at Fort William are reduced to 32° and sea level, but those at the Ben Nevis Observatory only to 32°. At Fort William the mean atmospheric pressure for the year was 29-871 inches, being 0°027 inch greater than the mean of the forty years ending 1895. The mean at the top was 25:321 inches, being 0:025 inch above the average of the observation since the opening of the Observatory in 1883. The difference for the two observatories was thus 4°550 inches, being all but identical with the difference of previous years. At the top of the mountain the absolutely highest pressure for the year was 26-058 inches, and at Fort William 30°728 inches, both readings occurring on November 17. The differences from the mean monthly barometric pressure much exceeded the averages in June, July, and August, the excess for the three months for Fort William being 0°172 inch, and for Ben Nevis 0:160 inch. On the other hand, for January and April the deficiencies from the averages were 0:164 inch and 0°160 inch for Fort William, and for Ben Nevis 0°164 inch and 0°165. In the summer months, when pres- sure was abnormally high, the type of weather was anticyclonic, but in January and April, when pressure was unusually low, the type of weather was cyclonic. The deviations of the mean temperature of the months from thew respective averages are shown in Table IT. :— Taste II. Fort Top of Fort Top of William. Ben Nevis. William. Ben Nevis. o ° ° ° January . : .--ld — | July. ; : gh yb) 24 February . p ey Oe 2°6 | August . : A i 82 March . : . —0°2 15 | September : . —08 —2°4 April 4 : . —19 --l1 | October . ; J. Seta 2-0 May. : . 23 —1:0 November : -. a0 aby June : : 2D 4-4 | December —25 —14 The highest monthly mean temperature hitherto yet observed on Ben Nevis was 48°-7 for August, which was 8°-2 above the mean of previous Augusts. The excess of méan temperature of the three summer months was 5°:0 above the average, whereas at Fort William the mean excess was only 2°-9. In the strongly marked type of anticyclonic weather which then prevailed, the temperature at the top of Ben Nevis was relatively very much higher than at Fort William. Hence, while the normal difference of temperature in August at the top and bottom of the hill is 16°-4, in August 1899 it was only 11°-9, The absolutely highest temperature for the year at Fort William was 82°-0 on August 24 ; and at the top of Ben Nevis 63°-5 on August 23. The absolutely lowest was 15°2 at Fort William on December 28; and on Ben Nevis 6°°9 on March 23. METEOROLOGICAL OBSERVATIONS ON BEN NEVIS. 49 In Table ITI. are given for each month the lowest observed hygro- metric readings at the top of Ben Nevis :— Taste III. _ Jan. | Feb. Mar, | April May | June} July | Aug. | Sept.| Oct. | Nov. Dee. | | { °o ° ° ° ° ° | °o °o ° ° ° fe} | Dry Bulb 5 - | 264 | 280} 43:5 | 19°2 | 41:0 | 526 | 47:5 | 51°4] 40°3 | 43:6 | 27°70] 19-2 Wet Bulb 5 . | 187 | 204 | 29:8 | 15:9 | 28:9] 384 |) 37:0 | 37:0) BL:2} 32:2 | 29°0 9:7 | Dew-point . ~ . |-22°9 |-10°8 | 134 | -8-1 | 13:2 | 24:1 | 25-4 | 21:2 | 194] 185 | -1-:0| -9:8 | Elastic Force . | 014 | 025 | 079 | :029 | ‘078 | *130 |) 13°7 | *114] 105 | ‘100 | -042 | -096 | Relative Humidity 10 16 28| 28 30 33] 42) 30 42 | 35 28 35 (Sat.=100) | | Day of Month : 27 19 16; 21 11 15 30 | 1 10 21 15 14 | Hour of Day . - | 84.M.)5 P.M. |5 P.M.) 44.M. |10 P.M, 9PM. | 2.4.M. 9P.M.|8P.M.|7P.M. | 2A.M, 4PM.) ( | | { Of these relative humidities, the lowest 10 occurred on January 27 with a dew-point of —22°-9, and the highest 42 on July 30 with a dew- point of 25°-4. It is to be noted that with these humidities the accom- panying dew-point fell in five of the months below zero, thus being in striking contrast with the lowest monthly humidities of the previous year, when the lowest was only 23, and the dew-point fell below zero only in December. The sunshine recorder on Ben Nevis showed 897 hours out of a possible 4,470 hours, being 132 hours more than in 1898, or 20 per cent. of the possible sunshine. This far exceeded the average of past years, which is only 750 hours, being only exceeded in 1888, when the number of hours was 970. The minimum occurred in 1884, when only 510 hours were registered by the sunshine recorder. At Fort William the number of hours was 1,139, being 102 hours fewer than in 1898. At both observa- tories the monthly maximum was in August, being 231 hours at Fort William and 212 hours at the top of Ben Nevis, amounts nearly d uble the average of any previous August. This unwonted amount of sunshine was occasioned by the strongly pronounced anticyclonic character of the weather of August 1899. In the following month, September, only 12 hours were recorded at the Ben Nevis Observatory, or less than 1 per cent. of the possible sunshine. In no previous summer month has the recorded sunshine been so decidedly deficient. At the Ben Nevis Observatory the mean percentage of cloud was 82, or a little under the average, the highest being 96 in September, and the lowest 60 in August. At Fort William the mean was 74, the highest being 87 in November, and the lowest 54 in August, or little more than a sky half covered with cloud. The mean rainband observation (scale 0-8) was 2-2 at the top for the year, the maximum being 3:0 in July, and the minimum 1°5 in February. The annual mean at Fort William was 3°7, the maximum being 4°8 in November, and the minimum 2:9 in February. The mean hourly velocity of the wind at the top of the mountain was at the rate of 15 miles per hour, the maximum monthly velocity being 20 miles in February and the minimum 10 miles in May, July, and August The rainfall for the year at the Ben Nevis Observatory was 187-30 inches, being 31:82 inches, or 22 per cent. above the average. This large annual rainfall has been only twice exceeded, viz. in 1898 and 1890, when it was respectively 240-05 inches and 197:95 inches. It is noteworthy that while the rainfall at the top of Ben Nevis was 22 per cent above 1900, A 50 REPORT——1900, the average, at the neighbouring surrounding stations near sea level the rainfall was about 10 per cent. under the average. It will be observed that the large excess on Ben Nevis was almost wholly occasioned by the extraordinarily heavy rainfall there in November and March. In these months there prevailed over Scotland an unusual excess of south-westerly winds. The largest monthly rainfall, 32:48 inch, occurred in November, when south- -westerly winds prevailed ‘eight days more than the average, and the mean temperature of the month over Scotland was 46° 4, or 5°8 above the average of the month, an excess of south-westerly winds and of mean temperature hitherto unparalleled for November. The heaviest rainfall on any single day was 4°68 inches in December. At Fort William the annual rainfall was 74:58 inches, and the largest monthly amount was 13:27 inches in November, when the rain-bringing south- westerly winds were so prevalent. The heaviest fall on any single day was 1°63 inch in March. At the top of Ben Nevis rain fell on 253 days, and at Fort William on 223 days. At the top the monthly maximum was 28 days in September, and the minimum 11 days in February, and at Fort William the maximum was 26 days in September, and the minimum 12 in August. During the year the number of days on which 1 inch of rain or more fell was 66 at the top and 12 at Fort William, the former being 18 above the average and the latter 5 below it. Auroras were observed on the following dates :—February 12 ; March 10, 16, 21, 22; May 2, 3, 4, 5, 6; and October 15. St. Elmo’s Fire was seen on January 6, 13,15 ; March 28 ; August 25 ; September 19, 20, 23 ; October 30 ; and November 6, 8, 10, 11. Zodiacal Light :—On October 15. Thunderstorms :—On August 25; September 17, 18; and October 13, 30. Lightning only :—On January 16 ; February 12 ; and September 29. Solar Halos :—January 2; March 30; April 9, 12, 18, 19, 20, 22; May 9, 12, 22, 31; June 10, 17; July 6; and August 5, 18. Lunar Halos J pau bi 1%; 26, 27, 98 ; ay y 18, 21, 22; March 24; April 19, 20; June 27 : October 21, 22 ; November 9; and Decem- ber 10, 12, 13, 23. Much time has been taken up in revising the proof-sheets of the hourly observations of the Ben Nevis Observatories now in the press, and the work of printing is proceeding at a fairly satisfactory rate. It need scarcely be added that the revision of the work, which will fill three large quarto volumes, is peculiarly heavy. The work of reduction and entering on daily sheets the hourly observations of the two observatories is practi- cally brought down to date. The daily maps of rainfall, fog, storms, and other weather phenomena are also completed to date; and for several selected months there are already entered on the same maps the details for storms, forecasts, and storm warnings. With these are compared the hourly observations at the two observatories with the view of arriving at some definite knowledge of the relations existing among the phenomena observed. Particular attention is given in the first place to the relations between the double set of observations made at Ben Nevis and the fore- casts and warnings issued from the Meteorological Office in London of storms, rain, fog, and other weather phenomena. For several months Mr. Omond had under discussion all hourly tem- peratures observed at Fort William and the top of the mountain, showing METEOROLOGICAL OBSERVATIONS ON BEN NEVIS. on a difference between the two temperatures distinctly less than the usual difference, together with all cases where the temperature at the top ex- ceeded that at Fort William at the time. It will be readily recognised that this work is largely an inquiry into the anticyclone, and its connec- tions with the cyclone and weather changes which accompany their changing relations. Dr. Buchan’s time has been largely occupied with the discussion of the fogs observed at the Scottish lighthouses night and day from 1889 to 1899. These data, as stated, are all entered on two daily maps, to each of which are attached the weather maps of the Meteorological Office for the day in question as issued in the weekly maps of the office, in addition to which the daily direction and force of the wind at eleven selected light- houses are given. Thus the general character of each day’s weather is readily seen, and the direction of the wind at the time the fogs were recorded. The fogs here examined are not land fogs, but sea fogs, a correct knowledge of which is of paramount importance to navigation. The more important results arrived at are these :—The annual maxi- mum period is from April to June, and the minimum from October to February, being thus generally the reverse of land fogs. The worst and longest continued fogs occur with easterly winds, and their occurrence is restricted to the east coast of Scotland. On the other hand, the fogs on the west coast accompany westerly winds. These are much more frequent and prolonged at places directly open to the Atlantic than at places such as Rothesay, Oban, and Stornoway, which are sheltered from the Atlantic _by land of a greater or less extent and height. Conjoined with this discussion is the excessively heavy rain brought by the easterly winds on the east coast of Scotland, and to a greater or less extent inland according to the height to which these rain-bringing easterly winds extend in the atmosphere. On this point the conjoined observations of the two Ben Nevis Observatories contribute invaluable knowledge. An examination of daily weather maps of Europe constructed from the daily weather maps of the British Islands, France, and Germany makes it clear that these heavy rains and easterly winds occur when baro- metric pressure diminishes from the Baltic and westwards through the North Sea to the West of Scotland. It is here particularly to be noted that at the same time humidities are high over those parts of the Con- tinent whence these easterly winds have come prior to their arrival in Scotland. Of these rain storms the great rains in the east of Scotland on April 27 to 30, 1898, and on August 22, 1900, are among the most remarkable ; they are therefore being investigated in great fulness of detail. It will be known, from your Committee’s previous reports, that gales and storms of wind have for many years been observed night and day at the Scottish lighthouses with a fulness and an accuracy attempted nowhere else. Much time has been given to the discussion of these obser- vations in their relations to the other weather phenomena charted on the daily weather maps. One of the results already arrived at—and it is an important one—is that the first step to be taken in any investigation of storms is the partition of Scotland into eight or ten divisions based on the physical features of the country in their relations to the more promi- ' nent storm-bringing winds, The inquiry is therefore proceeding on these lines. E2 A REPORT—1900. If a meteorologist knows the distribution of barometric pressure over Western Europe, he can then at once state what the weather is in each part of the countries for which he has this information, and he can de- scribe the weather in fulness of detail just according to the accuracy and abundance of the barometric readings supplied to him. This valuable practical result is a direct consequence of the scientific study of the rela- tions of barometer, temperature, and wind as observed over the whole world and interpreted in accordance with physical laws. Now this is not forecasting, but only the description of the weather at the time the barometric readings were taken. But it necessarily follows that if the forecaster can guess what the distribution of barometric pres- sure will be at some future time, he can state what the weather will be at that time. Hence the whole problem of forecasting resolves itself into foreseeing the arrangement of barometric pressure in the future. The distribution of pressure does not shift arbitrarily, but the areas of high and low pressure existing on any one day change into those of the next by movement over the surface of the earth and by increase or diminution in intensity, in accordance with physical laws. The scientific study of the causes of the movements of these areas of high and low pressure, called respectively anticyclones and cyclones, can only be said to be just beginning. Until this great inquiry has made some substantial progress we cannot have a science of forecasting, as we now have a science of climatological meteorology. These areas of low and high pressures are not mere surface pheno- mena, but extend upwards through the atmosphere, and their movements are largely determined by the conditions surrounding them in the upper regions of the atmosphere. Towards the expenses of publishing the hourly observations of the two Ben Nevis Observatories the Royal Society of London has made a grant of 500/., and a grant to the same amount has been made by the Royal Society of Edinburgh. These societies thus approve of the publication as a necessary preliminary to the scientific study of forecasting. The Ben Nevis Observatories have already largely contributed to the fundamental data of meteorology, and in the future the observations they supply will take a prominent place in the development of scientific forecasting. Your Committee have the greatest pleasure in adding that at the meeting of the Scottish Meteorological Society in March last J. Mackay Bernard, Esq., of Dunsinnan, intimated a third handsome donation of 500/. towards the maintenance of the observatories to the end of next year. Another gentleman, on learning that assistants were urgently required to assist Dr. Buchan and Mr. Omond in the office, at once readily and most generously intimated a donation of 300/. to the Council of the Society for the purpose. Radiation in @ Magnetic Field.—MReport of the Committee, consisting of Professor G. F. FirzGrratp (Chairman), the late Professor T. Preston (Secretary), Professor A. ScHusTER, Professor O. J. LopGe, Professor 8. P. THompson, Dr. GrraLp Mo.uoy, and Dr. W. E. ADENEY. Tue Committee regret that they are unable to sapere that any further work has been dotie with thé great spectroscope belorigirig to the Royal ON RADIATION IN A MAGNETIC FIELD. 53 University of Ireland owing to the illness and death of the Secretary of the Committee, Professor T. Preston, F.R.S. They desire to be re- appointed without a grant for the purpose of publishing copies of Professor Preston’s photographs, as they believe that a good deal of useful work could be done upon these photographs by persons who are not possessed of the spectroscopic and magnetic power required to produce the phenomenon on a large scale. Others may desire to obtain copies of the photographs as illustrations of this interesting effect of magnetisation on light. Heperiments for improving the Construction of Practical Standards for use in Electrical Measurements.—Report of the Committee, consisting of Lord RaYLeicH (Chairman), Mr. R. T. GLAZEBROOK (Secretary), Lord Kertvin, Professors W. E. Ayrton, J. Perry, W. G. ADAMs, Ouiver J. Lopae, and G. Carry Foster, Dr. A. Murrueap, Sir W. H. PrREEcE, Professors J. D. Everetr and A. SCHUSTER, Dr. J. A. Fiemine, Professors G. F. FirzGreratp and J. J. THomson, Mr. W. N. Suaw, Dr. J. T. Botromuey, Rev. T. C. Firzpatrick, Professor J. ViriaMu Jones, Dr. G. JOHNSTONE Stoney, Professor 8. P. THompson, Mr. J. Rennie, Mr. E. H. GRirriTHs, Professor A. W. Ricker, Professor H. L. CALLENDAR, Mr. GreorGe Mattruey, and Sir W. Roperts-AUSTEN. APPENDIX. —Note on an Improved Resistance Coil. By ROBERTS. WHIPPLE p. 55 Durinc the year the resistance coils and other apparatus belonging to the Committee have been removed to Richmond. Most of the apparatus has been set up in an outbuilding attached to the Kew Observatory, which has been fitted by the Committee of the National Physical Laboratory as a temporary laboratory. Tt is interesting to note that the case containing the original coils of the Association bears the words, ‘ To be deposited at Kew.’ After many wanderings the coils have at last returned to their home. The Sub-Committee on Platinum Thermometry held a meeting in the spring, and agreed to the following resolutions :— (i) That a particular sample of platinum wire be selected, and platinum thermometers be constructed therefrom to serve as standards for the measurement of high temperature. (ii) That Mr. Glazebrook and Professor Callendar be requested to consider the details of the selection of wires and construction of ther- mometers for the above purpose, and to consult with Mr. Matthey, who kindly consented to give his assistance. Since then Mr. Matthey has supplied the Sub-Committee with two specimens of very pure platinum. Portions of these have been made into thermometers and tested at the National Physical Laboratory, with the following results, Ry being the resistance at 0° and Ryo) at 100°, while 6 is the coefficient occurring in Callendar’s difference formula : Byoo/ Ry 5 Wire 1 1:3883 : 1:493 Me, 2 ’ : 1:3884 5: : 1-498 5A REPORT—1900, The question of the selection of a wire for the construction of the standards is still under the consideration of the Committee, During the summer a very full comparison has been made of the unit resistance coils of the Association, and the opportunity has been taken of comparing these with some coils belonging to the Board of Trade, and with others which have recently been obtained from the Reichsanstalt. The coils were also compared with one of the mercury resistance tubes prepared by M. Benoit in 1885, and which has been in the care of the Secretary since that date. The results have not yet been completely worked out, and publication is, therefore, necessarily deferred. Moreover, the temperature during July was very high, so that the mean temperature of the observations is much above that at which previous comparisons have been made. For the purpose, therefore, of connecting these results with the past it will be desirable to make some further observations in the autumn. It seemed desirable to set up some mercury resistance tubes in England, with a view of keeping a check on the variations of the wire standards. Preparations have been made for this. A number of selected tubes of ‘verre dur’ have been obtained, with the kind assistance of the officials of the Bureau International, from M. Baudin, while other tubes of Jena glass have been procured from Schott & Co. Steps are being taken to have some of the best of these calibrated. Some advance has been made during the year with the construction of the Ampére balance. The Committee greatly regret the serious illness of Prof. J. V. Jones, which has prevented more rapid progress. The stand for raising and lowering the outer coils has been completed. Thanks to the generosity of Sir A. Noble, the cost of this, estimated at about 100/., has been saved the Committee. During the spring the Secretary, as Director of the National Physical Laboratory, visited the Bureau International at Paris and the Reichs- anstalt at Berlin. The Committee are glad to put on record their appreciation of the great courtesy and kindness with which he was received by President Kohlrausch, M. Benoit, and the other officials con- nected with those institutions. The Committee are informed that at the recent International Electrical Congress at Paris the two following resolutions were unanimously adopted by Section I, and confirmed by the Congress and by the Chamber of Government Delegates :— 1. The Section recommends the adoption of the name of Gauss for the C.G.S. unit of magnetic field. 2. The Section recommends the adoption of the name of Maxwell for the C.G.S. unit of magnetic flux. The question of giving names to the units of magnetic force and flux has been before the Committee on several occasions. The Committee therefore were in a position to welcome cordially these resolutions, and at their last meeting agreed unanimously to a resolution adopting the two names selected by the Paris Congress. Of the sum of 25/. voted last year, 13/. 7s. 7d. has been expended on material for the new platinum thermometers and on the transport of the ap- paratus from Liverpool to Richmond. If the plan of constructing standards for platinum thermometers is adopted, it will be necessary to purchase a large stock of suitable wire, the whole of which should be made at the same time. For this a considerable expenditure will be required ; there PRACTICAL STANDARDS FOR ELECTRICAL MEASUREMENTS. 5D will also be incidental expenses connected with the making and standard- ising of the thermometers. ‘For these purposes the Committee ask for a grant of 751. ; The Committee therefore recommend that. they be reappointed, with a grant of 75/., and that Lord Rayleigh be Chairman and Mr. R. T. Glaze- brook Secretary. APPENDIX. Note on an Improved Standard Resistance Corl. By Ropert 8. WHIPPLE, The coil in question consists of a bare wire wound on a mica frame. This form of coil possesses the following advantage over the ordinary resistance coil :—(1) The coils can be annealed to a dull red heat im satu, thus relieving the wire of any strain caused by the winding. (2) The heating of a wire immersed in oil is less than one silk-covered and varnished. (3) The temperature of the wire can be accurately determined by means of a thermometer placed in the oil surrounding the wire. German physicists have adopted a form of coil in which the wire is silk-covered and varnished and then placéd in a metal case perforated with holes. The whole coil is placed in an oil bath when in use. This form of coil is open to the objection that it cannot be annealed above 140° C. without causing injury to the silk covering on the wire, and there is a certain amount of lag in the oil obtaining the temperature of the coil. By request of the Electrical Standards Department of the Board of Trade the Scientific Instrument Co., Cambridge, have designed and made two standard 1-ohm coils the wires of which are bare and immersed in oil; a modification suggested by Mr. Horace Darwin was also fitted for obtaining the temperature of the coils. The coils proper consist of 0-035 in. PtAg wire wound on mica frames, the ends of the wires being attached to stout copper terminals in the usual manner. A 0:08 in. platinum wire is wound alternately with the platinum-silver wire, and is attached similarly to stout copper leads. Both coils are adjusted to a resistance of 1 ohmat 15°-5C. Owing to the difference in the temperature coefticient of the two wires (PtAg 0:00024, Pt 0-00350), a small change in the temperature of the coil causes a comparatively large difference between the resistances of the two coils. This difference being known, the temperatures in degrees Centigrade is given by the adjoined table. The table is calculated from the difference in the temperature coefficients of the two wires 0:00350—0-00024=0-00326 for 1° C, Temperature of Difference in resistance standard coil of the coils 10°°0 C, 2 y ; - . —0:01793 O°, . oa a ‘ ; z ' 3 001487) patina coil having a lower 13°0 C. é } i ; , O-00s15/ Tesistance than the platinum- PGC AY wicigerie 0-0048| pillar ¢oil, 15°70". C : c C . —0°00163 15°'5 C, 5 j i 3 0:00000 o. . . feet & ; : : t j * 0489 ) Platinum coil having a higher weo0G 86||lClt(‘( tt! ggogis | Tesistance than the platinum- ets | er | silver eoil. 20°°0 C, . e ° : - +0:01467 REPORT—1900, oO (er) As the temperature coefficient of platinum is about fifteen times as great as that of platinum-silver, the resistance of this coil may be measured to one significant figure less than the standard coil without affecting the value for the temperature of this coil. In measuring small resistances the determination of the last figure to 0:00001 ohm requires considerable care, aud the advantage of not being compelled to measure to such a high degree of accuracy is apparent. The two wires being wound on the same frame alternately with each other and immersed in oil are at the same mean temperature. Any temperature gradient in the oil influences both wires similarly, thus doing away with the necessity of a stirrer. The platinum wire is also useful for testing the insulation of the windings of the PtAg coil one from the other. The coils are placed in a glass vessel in order that the behaviour of the insulating oil with time may be studied. Photographic Meteorology.—Tenth Report of the Committee, consisting of Professor R. Metpouia, Mr. A. W. CLaypEN (Secretary), Mr. J. Hopkinson, and Mr. H. N. Dickson. (Drawn up by the Secretary.) Tur Committee have suffered a severe loss during the past year by the death of the Chairman, Mr. G. J. Symons, F.R.S., whose genial presence and energetic support will be greatly missed from many scientific societies, and especially from those which are interested in meteorology. This is not the place to attempt any adequate eulogium of his life’s work, which, indeed, is too well known to need description. The observational work in progress was brought to an abrupt end early in October. On visiting the ground where the cameras stood in order to make some measurements it was found that the connecting wire between the two stations had been blown down by a heavy gale a few days before. The poles were snapped in two, several of the insulators broken, and the connections to the cameras damaged. It was felt that it was not worth while to re-erect the line on the same site, as the number of observations already made was rather more than 400, and also because the site had become much less convenient. It was on some waste ground belonging to the L. & 8. W. R. Co., near their engine sheds. At first this was very little disturbed, but for the last two years railway operations have been encroaching on the space, a preliminary process being the deposit of great quantities of rubbish. Attempts were made to find another suitable site, but none seemed available within a convenient distance, and the expense of re-erecting the line and repairing the apparatus would be considerable and not worth incurring unless frequent observations were possible. It seemed, therefore, that the best course would be to summarise the results so far attained and suspend measurements until a favourable opportunity should occur. . So far the total number of measurements made is 423. These include no measurements of the variety of cloud known as nimbus and very few of true stratus, the great majority being of cirrus, cirro-stratus, cirro- cumulus, alto-cumulus, and alto-stratus. ON PHOTOGRAPHIC METEOROLOGY. 5 The following tables show a comparison between the Exeter measure- ments and those made at Blue Hill and Upsala respectively :— Maarimum Altitudes in Metres. | - Blue Hill’| Upsala | Hxeter | No- of Ob- | | servations ‘Ch ee Lae le wt on 13:36) 1) 27.413 58 Cirro-stratus . “ 6 : : 12,134 11,391 | 15,503 64 Cirro-cumulus : : ; - | 105520 10,235 | 11,679 63 Alto-cumulus . : : : : 8,204 8,297 | 9,390 83 Cumulus top . = epee 3,611 | 4,582 2 Cumulus base. | 3,582 2,143 | 1,959 48 Strato-cumulus ‘i, hy See 4,324 | 6,926 27 Cumulo-nimbus top ral = 5.970 | 6,409 15 _ Cumulo-nimkus base 2 | 1,590 1,630 | 2,286 15 Minimum Altitudes in Metres. — | Blue Hill Upsala | Exeter oon ei ei Cy nnn ee ty ae Cirro-stratus : ; ; a 2,290 4,740 3,840 Cirro-cumulus. , : nt 4,772 | 3,880 3,657 Alto-cumulus : : : 5 784 1,498 | 1,828 Cumulus top he ajuda ¢ | 1,455 900 | — Cumulus base. é : | 601 | 743 | 584 | Strato-cumulus . . i ‘ 1,109 | 887 823 Cumulo-nimbus top , — 1,400 2,004 Cumulo-nimbus base... gah A Ts 766 Mean Altitudes in Metres. — | Blue Hill / Upsala Exeter Eg es Citas ug 24 9,923 | 8,878 10,230 Cirro-stratus 5 ; ; ; 7,617 | 7,226 9,540 Cirro-cumulus. ; : $ 7,606 6,465 8,624 Alto-cumulus : 3 bh F 4,787 4,178 5,348 Cumulus top A eh eet! 2,181 | 1,855 | 3,006 Cumulus base ; : ; =| 1,473 1,386 1,290 Strato-cumulus —. : 3 F 2,003 2,331 | 2,248 | Cumulo-nimbus top. : : == 2,848 8,002 | Cumulo-nimbus base . 5 fall 1,202 1,405 1,045 In making such a comparison there are many difficulties, for the different types of cloud so merge into each other that unless the figures are known to relate positively to clouds resembling a certain type picture any agreement can only be general. Tt will be seen that the maximum values at Exeter exceed those of the American and Swedish observations in every case except that of the base of cumulus. It should be noted, however, that several of these maxima occurred on one day (June 12, 1896). If that one day had been omitted, the maxima for cirrus and cirro-stratus would be only about 1,000 metres greater than the Blue Hill values. 58 REPORT—1900. In comparing the mean values a similar remark holds good, the greater values at Exeter being due to a small number of extreme observations. The minimum altitudes recorded at Exeter compare fairly well with the others, some of the ditferences being most probably due to nomenclature. Several series of observations have been made in a single day with the object of determining the rise or fall of clouds. It is clear from these that on an average day the cloud planes rise steadily until the early afternoon, between 2 and 3 p.m., when the maximum for the day is usually reached. This is followed by a fall, which gets more and more rapid towards sunset. In calm weather, or weather with only a moderate breeze and no great barometric disturbance, this diurnal rise and fall is very clearly marked ; but in broken weather, with strong winds, showers, or barometric changes, it may be completely masked. Cumulus is the result of an upward movement, but cirro-cumulus and alto-cumulus may sometimes be the result of a descending movement, in which case the lumpy form is never persistent, but passes into a stratiform cloud very quickly. True cirrus of the whispy form is described by some meteorologists as due to a rapid ascending current, by others to an equally rapid descent. The measurements made indicate that this form of cloud may exist with an upward or a downward movement, or with no recognisable movement at all. The greatest altitudes have been found with thunderstorm conditions, the lowest (excepting fog) with cyclonic. The measurements compared in the foregoing tables have all been made between April and October inclusive. In the winter months the ground has generally been too wet for use, and the figures from the foreign stations are for the summer months only. It seems difficult at first to see why the altitudes should, on the whole, be greater at Exeter, the greater humidity of the air leading rather to the expectation of more easy cloud production, and therefore lower altitudes. But the fact of thunderstorm conditions being attended, as they seem always to be attended, by great cloud altitudes suggests another explanation. This is that vapour in a cloud-producing quantity exists to a greater height above Devonshire. It will be noticed that the greater altitudes are true only of the higher clouds, and that the mean level of the base plane of cumulus and cumulo-nimbus is actually lower at Exeter than at either of the other stations, The photographs collected some years ago by the Committee have been placed in the care of the Royal Meteorological Society, with the exception of prints from the negatives belonging to the Secretary, who will add them as opportunity offers. During the past year the Secretary has made a number of experiments with the Ives and Joly processes for photography in natural colours, but has found that, although either process can be made to record the colour of a cloud, the tints of a sunset, or even the colours of the rainbow, the reproduction of the colours is so far from being an automatic process that neither method promises to be of very great meteorological value except in the hands of experts. ON SEISMOLOGICAL INVESTIGATION. 59 Seismological Investigations.—Fijth Report of the Committee, con- sisting of Professor J. W. Jupp (Chairman), Mr. JoHNn MILNE (Secretary), Lord Ketvin, Professor W. G. ApAms, Professor T. G. Bonney, Sir Ff. J. BRaMweELL, Mr. C. V. Boys, Professor G. H. Darwin, Mr. Horace Darwin, Major L. Darwin, Professor J. H. Ewine, Professor C. G. Knorr, Professor R. Metpoxa, Mr. R. D. OLDHAM, Professor J. Perry, Mr. W. E. PLummMer, Professor J. H. Poyntinc, Mr. CLeMentT Rep, Mr. Netson RicHarpson, the late Mr. G. J. Symons, and Professor H. H. Turner. [PLATES II. anp III.] CONTENTS. PAGE I. On Seismological Stations abroad and in Great Britain . ° . - 59 Il. Analyses of Harthquakes recorded in 1899. By J. MILNE. 1. Nature and Objects of these Analyses . - ‘ - 7 . 60 2. Velocities of Earthquake Waves . 2 5 : - c : gi 3. Errors affecting such Determinations F : ; : x . 62 4. Velocities for Preliminary Tremors or P.T’s . - : b . 63 5. Velocities for Large Waves or L.W.’s : : ‘ ‘ : . 64 6. Intervals between P.T’s and L.W.s . r . . - 7 ay LoD 7. Earthquake Recurrences . ; - : : . F ; . 66 8. Amplitude in relation to Continental and Sub-oceanic Paths . ud 9, Arcual Velocity in relation to Surface Configuration . 2 5 bf) 10. Harthquake Echoes . : ; : : : : : = ae! 11. The Nature of Large Waves : : : : F spies 12. Criticisms and Analy yses by Dr. C. G. ‘Knott : : : . Be ie 13. Determination of Origins . : . : : : - Fe avis: By By comparisons between time sabohenle é - ; : retifis: By method of circles. : : : ete By time intervals between P. T’s and L. Ws. : = 5 . 79 By seismic recurrences . : : : ‘ , - 80 14. The Origins for the Earthquakes Ee 1899. . : 5 : - 80 15. Illustrations of Scismograms . - : , : é ei Ill. Harthquakes and Timekeepers at Observatories. By J. MILNE . : . 105 IV. Larihquakes and Rain. By J. MILNE . : . 106 V. Harthquakes and Changes in Latitude. By J. MILNE 5 ; + 107 VI. Selection of a Fault—Locality suitable for Observations on Far th-move- ments. By CLEMENT REID . 108 VII. On the Relative Movement ov Strata at the Ridgenca y ’ Fault. By HORACE DARWIN : re OE) I. On Seismological Stations abroad and in Great Britain. In addition to the twenty-three stations referred to in the Report for 1899 instruments have been ordered for the Observatory, Melbourne, the Observatory, Sydney, N.S.W., for Ceylon, for the Johns Hopkins University, Baltimore, the Liverpool Observatory, Bidston, and the Royal Observatory, Edinburgh. The total number of similar installa- tions which may be expected to be in working order before the end of the current year will therefore be twenty-nine. The positions of these are shown on the map (Plate II.). Registers ending December 31, 1899, referring to Shide, Kew, Cal- 60 REPORT—1900. cutta, Madras, Bombay, San Fernando (Spain), Cairo, Mauvitius, Batavia, Cape of Good Hope, and Tokio, have been printed and issued as a circular to all co-operating stations, to those who have assisted this committee in their work, and to persons expressing a wish to possess the same. With the object of finding permanent quarters at which a central observing station might be established in England, at the suggestion of this Com- mittee its Secretary, in company with Mr, Horace Darwin, visited the Office of Works, the Treasury, and the Admiralty, and, with Major Leonard Darwin, the Horse Guards. Many sites were discussed, and through the kindness of Colonel Hildebrand, R.E., and commanding officers of the Royal Engineers facilities were given to visit forts and other buildings at Chatham, Folkestone, Porchester, and in the Isle of Wight. AA report on these visits and on those to other places, together with a reference to steps generally which have been taken to find the required site, has been drawn up for the Council of the British Association. In consequence of the generosity of Mr. M. H. Gray, an instrument room is now being built at Shide. Il. Analyses of Large Earthquakes recorded in 1899. By Joun Mie. 1, Nature and Object of these Analyses. In 1897 the Seismological Investigation Committee of the British «\ssociation issued to the directors of observatories and other persons in various parts of the world a circular in which they called attention to the desirability of observing earthquake waves which had travelled great distances. It was pointed out that similar instruments should be used at all stations, and the type recommended as being simple to work, and one that yielded results sufficiently accurate for the main objects in view, was described by the Committee in a report (see Reports of the British Association, 1897, p. 137 et seq.). The result of this appeal is that instruments have been forwarded to the following twenty-six stations :—Shide, Kew, Toronto, Victoria, B.C., San Fernando (Spain), Madras, Bombay, Calcutta, Mauritius, Cairo, Cape of Good Hope, Tokio, Batavia, Arequipa, Swarthmore College (Phila- delphia), Cordova (Argentina), New Zealand (two instruments), Paisley, Mexico, Beyrut, Honolulu, Trinidad, Melbourne, Sydney, Johns Hopkins University (Baltimore). For the year 1899 registers were received from the first thirteen of these stations. With the exception of those relating to Toronto and Victoria, these have been communicated to observers by the Committee asa circular. This circular is independent of the present report, but continuous with registers contained in corresponding reports subsequent to 1895. A glance at these registers, or tables based upon them (see pp. 80-87), shows that while certain earthquakes have evidently shaken the whole surface of our globe, and have probably disturbed the same throughout its mass, there are others of less intensity which have only affected certain parts of the same. For example, one set of earthquakes were only recorded at stations in Western Europe, whilst another set were appa- - rently confined to the Indian Ocean. In the following paper the earth- quakes referred to are only those which were recorded in England, from ON SEISMOLOGICAL INVESTIGATION, 61 which it follows that although the largest earthquakes of the year 1899 are discussed many earthquakes which are comparatively smaller have been omitted. The object of the discussion is to indicate by examples some of the directions in which this extensive system of earthquake observation is increasing our knowledge of dynamical phenomena inherent to the world on which we live. The plan of the discussion is as follows :—First, those earthquakes which have been recorded at the greatest number of stations, and which have known origins, have been selected from the others and analysed separately. To confirm the results towards which these analyses point, references have been made to the more trustworthy records obtained by similar instruments in previous years. The principal objects in view have been as follows. The determination of the velocities with which various types of earth vibrations are propagated and the duration of preliminary tremors at varying distances from origins; to show that earthquake repetition and echoes are fairly frequent and to point out the existence of phenomena for which satisfactory explanations are as yet wanting. In connection with these investigations references are made to hypotheses relating to the physical condition of the interior of our earth. Second, the results obtained by the above analyses are used as a means to determine the foci of disturbances not included in the first section of this paper. These foci, which for the most part are sub-oceanic, in some instances indicate localities where it would be unwise to lay cables, and where we may expect to find configurations differing from those shown upon our physical maps. Remembering that very many of the earthquakes discussed represent initial disturbances which were followed by many after-shocks, the map depicting these foci shows the regions on the surface of the earth where in the year 1899 seismic activity was most pronounced. 2. Velocities of Earthquake Waves. The knowledge hitherto at our disposal respecting the velocity of trans- mission of earthquake motion over long paths has been based on records obtained from instruments differing in type and sensibility, all of which were installed in Europe. ‘The result of this has been that, although the registers led to the determination of average velocities along paths of varying lengths, they never gave actual velocity from point to point. It was seen that along paths from 10° to 90° the velocity of transmission of the preliminary tremors increased rapidly with the lengths of these paths, whilst the average velocity for large waves increased but slightly. With regard to the former my own analyses of heterogeneous materials led to the conclusion that, if the preliminary tremors travelled along paths approximating to chords through the earth, then the average velocity of transmission to a distant station was practically dependent on the square root of the average depth of the chord connecting that station and the earthquake centre. This furnished Dr. C. G. Knott with the hypothesis that the square of the velocity of these particular vibrations, which were in all probability compressional, was a linear function of the depth. With this assumption, and with a given initial velocity, the rate of transmission at any point within the earth could be determined and wave fronts drawn ; and by atceptiiig a law respecting the increase of density within 62 REPORT—1900. our earth the elasticity governing the transmission of condensational waves could be determined. The following notes show that, although the first conclusion and the consequent hypothesis do not require modification, constants necessary in farther calculations require to be modified. With regard to the large waves my own assumption was that their apparent increase in velocity with distance might be due to the fact that it was only large waves which, travelling faster than small waves, reached great distances. The observations brought together in this paper show that this idea has to be abandoned, and in its place we are to accept either the hypothesis of a surface wave which increases its velocity in regions 90° from the focus, or of a distortional wave passing through the earth the outcrop of which gives rise to similar surface undulations. 3. Sources of Error. The phases of earthquake motion here considered are the first pre- liminary tremors and the first group of large waves, which latter in a seismogram representing an earthquake which has originated at a great distance usually correspond to the maximum movement. Although near to the origin of an earthquake there is a varying interval of several seconds between the first movements and the shock or shocks, it is the time of occurrence of this latter phase which is taken as the datum to which observations made at great distances from origins are referred. The initial time for all large earthquakes has been a matter of inference. It may be deduced from the times at which clocks have been stopped, or which have been noted with varying degrees of accuracy by survivors in an epifocal district, but more generally it has been deduced from automatic time determinations outside such an area, and subtracting from the same an interval which the shock is assumed to have taken to travel from its origin to the point or points where these chronographic records have been made. The determination of this interval is based upon repeated observations of earthquake velocities made between stations well removed from an epicentre and well outside a meizoseismal area. These figures are important, not only for this particular purpose, but also for completing velocity curves which may represent transmission over the surface and through the material of the whole globe. They have been arrived at by many observers, the last being those given by Dr. F. Omori, who for paths commencing 100 kms. from an origin and extending to distances of 1,000 Ems. gives the velocities of 2:2 km. for preliminary tremors and 1:7 km. for large waves, and within these limits the former outrace the latter at the constant rate of 15 seconds per 100 kms. When we remember that large earthquakes may sometimes originate as practically simultaneous displacements over very large areas, it is seen that the application of the method here considered might easily result in determinations of initial times from a few to some sixty seconds earlier than had really been the case. Errors of this nature would result in a general lowering of the determinations for true velocity of transmission of earthquake motion to distant stations, the deviation from the truth being most marked for the preliminary tremors, and in records referring to transmission to stations comparatively near to an origin. Another serious error affecting the determination of initial time arises from the difficulty in accurately locating the position of a focus, especially when this is sub-oceanic. ON SEISMOLOGICAL INVESTIGATION. 65 The assumption that for large earthquakes, at least, the origin has been at an epicentre rather than in a region at a certain depth below the surface, is, so far as velocity determinations are concerned, of but small importance. Although all stations have similar instruments, the records from one or two of them indicate that their adjustment has not been similar to that adopted at the remaining stations. Not only should each instrument have a period of 15 seconds, but when its boom is deflected 7 or 8 mm. from its normal position, and then set free, it should take 7 or 8 minutes before returning to rest. If this latter condition has not been observed, an instrument may not respond to the first preliminary tremors, with the result that the time recorded for the commencement of a given earthquake may be registered as one or two minutes after the true time. Although errors of this order may affect the results deduced from observations within 20° of an earthquake origin, when we deal with paths of greater length, and especially with large waves, the errors in the final results are practically inappreciable. Another assumption made in connection with velocity determinations is that the group of vibrations and waves as recorded at a distant station extending between the first preliminary tremor and the first maximum— which may extend over any interval up to 100 minutes—were all the result of the principal movement or movements at the origin ; or, in other words, they have the same initial times. To this assumption I do not know of any serious objection. The fact that pronounced phases of move- ment near to an origin are not only extended in time as they radiate, but are also more or less equalised in their amplitude, frequently renders the determination of corresponding points in seismograms obtained at different stations more or less uncertain. This source of error is sometimes serious. 4, Preliminary Tremors. In the compilation of the following table the only seismograms used are those which show a distinct commencement. Each earthquake is indicated by its British Association Register number, and the locality from which it originated. Following this are the initial letters (see p. 88) of the station or stations at which it was observed. The figures following these initial letters give the number of minutes taken by the preliminary tremors to reach these stations, and the number of degrees between the stations and the earthquake origins. These figures are respectively placed in positions corresponding to the numerators and denominators of fractions. If an initial letter is followed by a zero for a numerator, this indicates that all other time intervals are measured relatively to the observa- tion made at the station represented by the initial letter. The fewness of these récords chiefly arises from these facts : first, they only refer to earthquakes with a known origin ; secondly, the seismograms of small earthquakes recorded at distant stations do not show the preliminary tremors corresponding to those given by large earthquakes ; and lastly, in consequence of air tremors and other causes, the earlier vibrations have in many instances been eclipsed or lost. Their chief merit is that they give for several earthquakes records from point to point, and that we have for the first time records relating to paths which practically extend from an origin to its antipodes. 64. REPORT—1900. a 2 i ee eee a n | | | | | 36 Japan . |s. 1° | = : yA ee nate May Pee % ia | 87 | | | (Matias, Jeet gs BS ey Se pk Afi) See a = — Si | 133 Borneo. |S. 2h i o— = = — ye } 103 | | | | > q \ ER | ERS 9 en bce Pores 2 ey Lee ren Pah. 5, GO | z | | fosMavan (Seco) | Les = ae ey | Paani 87 | | | PrpbMtexito «|, 2-1.) K.2°,| 3 a2 ieee oe EM aa yl ee 86 | | 263 Japan . he Ke ae Tv V. oe — = ig fas bs | h, 2 | bo) 89 U5 | | Pa ale | 5, 7 19 20 |p 5 temas || || Ree | Tee eae a ea IG 20 | 76, © ; 70 | >" a0 |* 6 |? a7 | 08 | 0: CHa ray = | a! 0 19 17 25 | Ey ee ae hes lea _— — ==. Ba “| — 16.4 a eae | | 9) 70!) p40 108 |" 105 4H G5 Yr ( | 9 6 so. .(— [ein S| — ewe] = fot! — [oon | — } | = 0 |x. 0 a miel: 7 | 18 15 843 Smyrna |S. — | K. —| — Synge Wp = = _ ayes ay 3 Smyrna |S. 55 | 35 | | a7 |B a3 i G.H wa\ a vee la 16] x, 16 Jy il 19 6 0 ,4 91 | 4 2 18s —— || See rai | OU saad Peps fae Se hee 3 347 Ceram 1 | a | Vv 0K iS. I. 129 > Gi Ba =| | ra B G. H. i05 To. 7 ; - 15 ysis tS 86 | 381 Mexico. | — |K. — |T. — |V.;; _ — |Ba. — | — |) es Sa |” 86 | 85 | 83 | 148 ye The numbers given in the preceding table have been plotted on squared paper, degrees being measured horizontally and minutes vertically. From the curves thus obtained the average times for preliminary tremors to travel distances of 20°, 30°, 40°, &c. have been determined, and are shown diagrammatically in fig. 1. The initial velocity is taken at 2-2 km. per second. A glance at the table on which this curve is founded indicates that the same can for the present only be regarded as provisional. The incurvation between 50 and 80 degrees is evidently due to errors in observation. 5. Large Waves. The construction of the following table is similar to that given for the preliminary tremors. Following the initial letter of each station, in the position of a numerator, the number of minutes is given which large waves occupied in travelling to that station from the origin or from the isoseist of the locality, the initial letter of which is followed by a zero. The figures corresponding to denominators are the distances of the localities beneath which they appear from the origins of the different earthquakes. co! aeeetaot Pte Doe. [v2 92 | 25) exico | 5.95 +34) Vay Se tcl M iso | — =a | aes — = 32 2 0 86 100 } 381" a S. 83 7 36 V-35| _ ——b | a 150 = — 89 ; — — aan " 3 TB Peek ile, 8 pene 81 | ocx. 2 17 333 Alaska | 8.35 T. 79] V-39 S8.F.77 | B.705| — M. a5 | — ees ig6 | LO. 55a ae Z 20 0 |} 22 34 50 7 69 39 337 es | S. 70 Hts 7) |e |S-F. 7 |B. jus Ba. i08 ey Me. p C.G.H. 165 = /Ma. ie = | , 19 0 | 22) 35 53 6 61 | Sy ches S- a ee Ore da ieee | 2888 =) 5 8.75 | Taq S.F. 77 | B.795 | B® jog | M+ yas [Mego] CSF aes. | | -— |- 70 783,280) 28 16 40 60 18 347 Ceram | Sy Me S.F.739| B. gp |B 55 | ™M 73 | — O.G.H. 55, | To. 4; C.F 0 | 10/_ 14 34 29 30 —| —| isn! et .= | — | CG.H. = = 343 Smyrna | S. 55 | S.P.57 |B. 75 M. G5 74 | TO 85 ‘i —— = = =. = ? The times at the origin Tor thbse two earthquakes weré 21 and 22 min, before Vittoria: ON SEISMOLOGICAL INVESTIGATION: 65 When these observations are plotted on squared paper it is found that they practically lie on the straight line referring to large waves in fig. 1, indicating that this form of movement passes from its origin to its antipodes with a constant arcual velocity of 3 km. per second. If, however, the direction of propagation has been along a diameter, the average velocity becomes 1°9 km. per second. The time taken for an earthquake to travel from its origin to its antipodes, whether it does so as a surface wave or as a mass wave, is about 110 minutes. One modification to this general statement respecting a constant velocity rests on the fact that repeated observations made within ten degrees of an earthquake origin have shown that the large wave velocity within that region is about 1‘8 km. per second. Whatever the conditions may be which give rise to this increase in velocity in a wave as it radiates from its origin, it seems probable that the converse would take place as it approached its antipodes, while the maximum velocity should be sought for in the equatorial or quadrantal! region of the earthquake’s transit. Inasmuch as curves drawn for the Alaskan and Ceram earthquakes show that between 70° and 110° from their respective origins velocities may reach 4 km. per second, and that many earthquakes indicate an increased average velocity as their paths increase up to 110° in their lengths, there are strong reasons for suspecting that the suggested phenomena may exist. The comparatively small initial velocity and the slightly increased quadrantal velocity above the average arcual velocity are indicated in fig. 1 by dotted lines; but whether this modification can be retained remains to be determined by further observations. That the average arcual velocity between 0° and 90° is practically 3 km. per second finds confirmation in the records for earthquakes Nos. 36, 83, 100, 119, and 193, originating in Japan, 133 and 134, originating near Borneo, and 105, from N.E. India, all of which were recorded by the same instrument in the Isle of Wight. 6. Interval between the First Tremor and the Maximum Motion, In the British Association Reports for 1898, pp. 221-224, I dis- cussed a table showing the duration of preliminary tremors or the interval in time between the first tremor and the commencement of the large wave phase of motion at different distances from a number of known origins. One object of the discussion was to establish a working rule enabling an observer to determine from the inspection of a single seismogram the distance of an origin from the station at which such a record had been obtained. Inasmuch as the table was to a great extent based upon descriptions of records obtained from different types of instruments which had different degrees of sensibility, the results obtained could not be expected to be more than approximately correct. The following table, which gives the time in minutes by which the first tremor has outraced the maximum movement over paths of varying lengths, is based on measurements made on seismograms obtained from similar instruments. These intervals not only enable us to correct the working rule indicated above, but, as it will be shown, they enable us to check the accuracy of the curves relating to the arcual velocity of preliminary tremors and large waves. 1 This word means the district 90° distant from the earthquake origin. ‘ 66 REPORT—1900, Intervals between the First Tremor and the Maximum Motion. Observing Stations indicated by od initial letters and time intervals No. Date Origin ; Minutes and distances, as —~——— Degrees 36 =| August 30,1896 .{| Japan . : . | 8. 2 56 October 31,1896 .]| Tashkent . . | 8. 22. 83 February 6, 1897 .| Japan . ‘ . | S., 34. Record not clear. 119 August 4, 1897 * “ 8., $8. 131 September 17,1897 | Tashkent . S., 42. 132 September 17, 1897 PA Se 133 September 20, 1897 | Borneo S., 134 September 20, 1897 Pr S., 157 December 29, 1897. | Hayti . Shs 163 January 29,1898 .| Asia Minor . 8., 189 April 15, 1898. . | California . .| Ti 2 193 April 22, 1898. . | Japan . . | S., ge T., 33. 249 January 22,1899 . | Greece 8.32. K., 4. 250 January 24,1899 .]| Mexico | K., a8. 7.22. Vi. Po 333 September 3, 1899 . | Alaska. K., 38. T.,25. V., 4. S.F., 32 | B., 32? To.,33. C.G.H., #. 337 | September 10,1899.) _,, K. 3. 7. 8. CGH, 1 B., 4h. S.F., 22. Me, 28. 338 | September 10,1899.| _,, | K.20. 1,22? Me, 2. Ba., 22 343 | September 20, 1899. | Aidin . : Sy. fe Cag Rey BE 2s: | K., %. To., 22. 347 September 29, 1899. | Ceram . : 5 a885 60" C.G.H., At, Ba., 4. ' B., 28? V., 227 381 | January 20,1900 .| Mexico . .|K,82 7,2 V., 23, These observations have been plotted upon squared paper, and their mean position determined. This is shown in fig. 1 as Curve No. ITI. On Curves I, II, and III, fig. 1.—Although in fig. 1 we have three curves which have been obtained from partly independent data, it will be observed that any one of them might have been obtained from the other remaining two. Although errors exist in all our data, these are probably least in the figures relating to the arcual velocity of large waves and the duration of preliminary tremors. By subtracting the ordinates for the latter curve, marked III, from those of the first curve, marked II, the curve [6 is obtained. This should coincide with Ia. It hardly does so ; but if the second incurvature of Ia, lying between 50 and 80 degrees, be effaced as probably doubtful the agreement between these two curves becomes closer. 7. Earthquake Recurrence. It would be uaturally expected that if the large waves of earthquakes were simply surface disturbances, we should find in the seismograms obtained at stations far distant from origins not only records of the waves which had travelled over the shortest paths, but also a record of those which had travelled in an exactly opposite direction. The suppo- sition that these latter records were without existence has been used as evidence in support of the hypothesis that all the movements of a large earthquake passed through the earth. Mr. R. D. Oldham, in his account of the Indian earthquake of 1897, however, shows that in the seismo- ON SEISMOLOGICAL INVESTIGATION. 67 prams obtained in Edinburgh, Shide, Leghorn, Rocca di Papa, and Catania there are excrescences succeeding the maxima movements at JO 20 30 GW 50 60 70 G0 90 J00_I10_120_J30_140 150 _s60_170 180 bea 2 ae Bi i aces nc! Ea ea Eu miei San ta SEE ia e ae REE WEIN ie as 16 273 15 278 60 8. 2°5 300 3) 309 70 8. 3 290 5 70 K. 25 290 5? 333 20 V. >16 340 75 40 T. >17 320 b 70 K. 10 290 “bl 338 40 T. >17 320 75 347 121 8. 35 239 15 105 V. 2 255 °b 354 120 8. 2 240 5 355 120 S$. 15 240 5 364. 106 M. 3 254 1 It is satisfactory to note that the magnitude of these repetition ampli- tudes fairly accords with what might be anticipated (see p. 70). 8. Amplitude in relation to Distance from an Origin. In the following table amplitudes are expressed in millimetres and occupy a position corresponding to the numerator of a fraction, whilst in the position of a denominator distances from origins are expressed in degrees. Observing stations are indicated by their initial letter or letters. Inasmuch as there are reasons for believing that the instruments giving the subjoined records have not in all cases been adjusted to have the same frictional resistances and as these records are few, the result to which they point must be receiyed with caution. When they are 70° REPORT—1900. plotted as curves it is seen that each has the same general character. The rate at which amplitude at first decreases is about ‘2 mm. per degree of travel. Earthquakes like Nos. 343 and 347 from whatever may have been their amplitude in the epifocal district, are reduced to an amplitude of 4 mm. after about 50° of travel. Larger earth- quakes, like Nos. 337, 344, and 345, travelled 80° or 90° before their amplitude sank to this quantity ; whilst the largest of all, Nos. 333 and 338, show an amplitude of more than 4 mm. after travelling nearly halfway round the world. From an amplitude of 4 or 5 mm. the rate of decrease becomes less and less. For example, the amplitude of No. 337 between 77° and 105° falls from 5 mm. to 3 mm., or at the rate of ‘07 mm. per degree ; whilst from 105° to 165° the rate at which amplitude decreases has been ‘01 mm. per degree at travel. { | 950, Mexico. 8 & |x 4°)r. sly. egal) Ba eS ae = s Ms = "80 80| "34 30 Seer a a | fede! ye ae To,25 "70 30) 105 | 145 50 5 5 |T.>17| | O05 ’ SF 7 =| rr, - ras “oe ys 70 20) 105 S.>17 he ae S17) o 7 2018, > 17, — M.> 17 ed C.G.H 10 To, “4 70 40) 20 7 105 | 145 ; 165 50 20) 5 3] 4 2 eee arnt a iS SEB ei a7) M. C.G.H. .— —_ a 40 77 105 49) 165 eho eels ice Siti sere re te. SE a ee 70 40) f 7 105 5 145 165 la 25 2 1 0 15 05 5 a Geram iS ol — (We, | = ee Ba u. } = Nec To. Coram 121 |" 105 3 22 73 105 47 9 | 1 1 6 4 . Smyrna S. = = ote A Seay ey ul (i ee reno elrs meee I yiny 8 Ee Ee os | 43 | 65 74 85 These slow rates of decrease indicate that it is reasonable to suppose that the large waves of earthquakes may reach distant stations by travelling in opposite directions round the world. Tf the large waves of earthquakes are merely surface waves, it would be expected that oceans would exert a marked damping effect upon their ampli- tude. Indications of this apparently exist in the records for earthquakes Nos. 337, 338, and 347 (also see earthquake 263, p. 81). In the first the amplitude for Toronto is greater than that observed in Mexico, the path to the former being across North America, and the latter being sub- oceanic. In No. 338 the record for Mauritius is less than that for the Cape of Good Hope. In No. 333 this condition is, hcwever, reversed. Lastly, in No. 347 the Shide record, which refers to a comparatively long continental path, is greater than the records for Victoria, the Cape of Good Hope, Bombay, or Mauritius, the shorter paths to which are beneath - oceans. Although, for reasons already stated, stress cannot be laid upon these observations, the latter at least suggests that we are dealing with surface waves rather than with mass waves. 9. Arcual Velocity in relation to Surface Configuration of the Earth. With the object of determining whether large waves are propagated more quickly over continents than over ocean beds, whether the rate of transmission along mountain axes is greater than in directions transverse to the same, and generally to determine whether there are directions over or through our globe in which motion is transmitted more rapidly than in others, the following table has been prepared, The apparent surface ae. TOth Report Brit, Assoc, 1900.] The Large Earthquakes of 1899. (Origins are indicated by their BA. Register numbers Stations with simi] ‘ar horizontal pendalams (Milne type) are named, (Prats. I!) ki Cape of Good Hipe Atkantse & Indian Ocean Origins are vey uncertain ON SEISMOLOGICAL INVESTIGATION. viilh velocities indicated in kilometres per second are from the isoseist of the place indicated by its initial letter to the place beneath which it is written. These latter places in the top line are also indicated by their initial letters The letter O refers to a velocity measured between an origin and the place named in the upper line Ss. Ta AV. SF. | B. Ba. M. Me. |CGH.| To. 0. | | 250. Mexico. | T. 3:1/Me. 2°7|Me. 2°65 — | — |0.32|0. 32) — = = — Renee T So 8 ” 33 re tsizf 17 10 7 5 Hayti . 62 2°5 2°5 7 5 3 . 24 6 3 3 Toronto Asia Minor 25 3 4 5 Shide. Record not clear California 75 2 3 2 + as or 2 1 7 Japan ,, 86 5 33 3 a Mexico . 80 5 5 3 ey rs = MO 6 Te it Kew. Doubtful 5 Aime 33: if 8 5 Toronto 5 s pu 17 9 5 Victoria Concepcion 2°5 io 6 Toronto Alaska 6.7 e208 PS ile 22 Victoria “ *» 2A0 ig 12 22 Toronto a 70 10 7 5 Kew 53 105 17 15 4 Bombay ~ 165 7 7 9 or 20 Cape of Good Hope i 77 17 10 5 San Fernando A 40 18 25 Toronto : 105 3 2 3 Bombay 5 40 | >17 15 25 Toronto A 70 ily if 5 Kew tS 145 4 + 8 Mauritius 3 165 1l 10 17 Cape of Good Hope + pel Ob 8 7 4 Bombay " ree) 17 7 3 Mexico Smyrna . 25 a 8 5 Shide a 85 3 3 3 Tokio 3 74 7 5 5 Cape of Good Hope s 43 4 4 3 Bombay 7 25 5 5 4 Kew Alaska 7 4 3 4 Shide + 20 ie 7 4 Victoria 5 70 5 4 5 Shide 3 20 | >17 7 4 Victoria. Larger than 344 Mexico. At Victoria and Toronto the chief motion is followed by three reinforcements at intervals of 3 minutes. At Kew there are two at intervals of about 3 minutes. The second group of waves, giving the large interval for the Cape of Good Hope in 333 and 338, may possibly refer to the motion which reached that station by the longest ‘path round the earth. If so regarded, these entries do not refer to echoes, but to repetitions. The large entries for Victoria and Toronto on account of the comparative nearness of these places to the origins of earthquakes 333, 337, and 338, ON SEISMOLOGICAL INVESTIGATION. 73 cannot, however, be so regarded. Between these extremely large rem- forcements it must not be overlooked that there are others of less magni- tude separated by intervals of from two to four minutes. All that we can conclude from an inspection of the above table is that after all sensible motion of a large earthquake has ceased horizontal pendulums, whether they are situated near to its origin or at a great, distance from the same, indicate that the earth waves at intervals of from two to six minutes show marked increments in amplitude. The earth- quake does not die out gradually, but by surgings. In its latter stages, for intervals of one or two minutes, the ground may be entirely at rest, after which movement recommences. This alternation of rest and move- ment may be repeated many times. If it can be admitted that large earthquakes result from the collapse of ill-supported portions of the earth’s crust upon a more or less plastic layer beneath, it may be imagined that rest is attained by a series of more or less regular surgings, which are propagated to distant places to disturb horizontal pendulums in the way observed, ll. The Nature of Large Waves. To explain the existence of the large waves of earthquakes we are at present left to choose between two hypotheses. One is that the large waves of earthquakes are disturbances travelling partly under the influence of gravity over the surface of our earth, and the latter that they represent the outcrop of distortional waves passing through its mass. Near to the origin of a large earthquake earth waves are visible ; some distance away their existence has been inferred from the wave-like motion seen on the tops of forests, at a distance of 300 miles, and even at very much greater distances the feeling occasioned by the moving ground is similar to that which is felt upon a raft moved by an ocean swell. Bracket seismographs, hanging pictures and lamps, water in vessels, ponds, and even in lakes, do not move with their natural periods, but are clearly influenced by a forced tilting. Finally, even as far as the antipodes of an origin, the character of motion assumed by horizontal and other pendulums shows that this is due to slow but repeated changes in the inclination of their supporting foundations. If we except the movements observed within the epifocal area, all the other movements are as explicable by the assumption of the outcrop of mass waves as they are by the assumption of surface radiation. The explanation that these waves have an increased velocity in their quadrantal region (assuming such to be the case) may perhaps rest on the fact that we are not dealing with radiation in uniformly widening rings, as would be the case over a plane surface. The condition in this region is such that energy is transferred from ring to ring, the diameters of which are but little different from each other. Radiation from a pole to its antipodes over a spherical surface may be likened to that of a wave which runs along a channel, which expands for half its length and then contracts. The phenomena which give the greatest support to the idea of surface radiation are, first, the existence of earthquake recurrences or waves which have travelled from an origin to a distant station in opposite directions round the world, the one arriving last having its amplitude reduced to expected dimensions ; and second, the observations which show that waves travelling over a continental surface are not so rapidly reduced in magni- 74 REPORT—1900. tude as those which have been propagated over the beds of deep oceans. Were the large waves of earthquakes mass waves, it is assumed that the damping effect of oceanic waters would be insignificant. When considering the large waves to be distortional mass waves, an observation of importance is that they travel from their origin to their antipodes in about 110 minutes (see fig. 1). If the path was along a diameter, the average velocity of propagation must therefore have been 1:9 km. per second, which is practically the so-called initial velocity. The close correspondence of these two velocities suggests the idea that there has not been any symmetrical change in the velocity of propagation of waves through the earth with regard to its centre, or, in other words, the large waves have had a diametral velocity which is practically constant. This idea of a constant velocity for all depths indicates that arcual and diametral velocities should be equal, which is not the case. An escape from the dilemma is to suppose that the large waves do not pass through the earth, but round its surface. 12. Criticisms and Analyses by Dr. C. G. Knott. In reference to the conclusion implied in the last paragraph, Dr. Knott remarks that it does not necessarily follow from the premises, the initial speed referred to being an arcual speed, or a speed for short distances from an origin through the surface layers. When a disturbance travels straight down it very soon gets probably into more homogeneous materials beneath the crust. It may therefore be a mere coincidence that the average speed along a diameter may come out almost exactly the same as the arcual speed in the crust. The evidence seems to show that once you get into the nucleus proper, the speed of the large waves decreases with depth. But this does not prevent the speed suffering a distinct increase when the disturbance passes from the lower layers of the crust into the higher layers of the nucleus. That the arcual speed should be 1°9 for small arcs, and then become on the average three when the arc is half a circumference, seems to be an immeasurably more difficult thing to understand than that the speed downwards should first increase and then decrease as the depth increases. A not improbable change in the nature of the material could easily account for the latter variation ; but it is difficult to see how a surface wave of the size of the large waves could gain in speed as it ran round the earth. Writing more generally respecting the propagation of large waves, Dr. Knott says :— I have looked pretty carefully into your numbers and curves, and now I shall indicate some of my conclusions. As you have pointed out, the one doubtful point is the precise instant at which the disturbance began, also to some extent the exact position of the origin. I take your deter- minations as being as accurate as they can be obtained, and proceed to consider the speeds indicated. The accompanying tables will show you what I have tried todo. Take the Alaskan group, the most complete of | all you have. It is gratifying to find how similar the results are for the three different earthquakes. The greatest discrepancy is in the two numbers for the Batavian records. It is curious that these time records do not fit well into the general scheme. Can there be any mistake? The arcual speed indicated is distinctly smaller than we find in all the other ON SEISMOLOGICAL INVESTIGATION. 75 cases, except the case of Mauritius. If there is no mistake in calculating the times, then the disturbance travels comparatively slowly along the Alaskan Batavian route. This route, if it lies near the surface, is almost wholly beneath the deeps of the North Pacific. But then, on the other hand, the Alaskan Mauritius route is also a comparatively slow route, and it lies further to the west, under Siberia, India, and the Indian Ocean. Still, these two routes are in the same quarter of the globe, so that a similar value for the speed is not unlikely. It may be not merely a question as to whether sea or land is overhead, but may depend on the general character of the rocky material. These two routes left out of account, there is a very striking constancy in the value of the arcual speed calculated for these various routes. In the four routes to Shide, San Fernando, Bombay, and Cape of Good Hope, the great circles pass all very near the poles. It is beautiful to see how well these four polar routes agree. With the somewhat scanty material you have to hand, I doubt if you would be at all warranted in making any deductions as to variations of speed. The Alaskan results suggest a constant value for the arcual speed. The same constancy.is indicated in the Mexican earthquakes, but the value comes out distinctly smaller than in the Alaskan quakes. Why is this? Still thinking of great-circle routes, we see that there cannot be much difference between the Mexican Batavian and the polar routes from Alaska, unless, of course, the former goes preferably by way of the South Pole. But that possibility is not considered in calcu- lating the speeds. If we took it that way the speed would come out larger in the ratio of 210 to 150 or 7:5, giving 1:9 instead of 1-4, a remarkable coincidence truly. The Mauritius number will also be increased in much the same ratio. But what are we to make of the others? No, I think we must get at an explanation of the much smaller speeds associated with the Mexican earthquakes in some other way. Is it possible that the depth of the seismic focus might have something to do with it? Have you any facts to guide you to an estimate of the probable depth ? And now pass on to the.Ceram quake. Here the constancy, so marked a feature in the other cases, no longer holds. There is an undoubted in- crease in the arcual speed over the longerarcs. The most striking feature is the smallness of the Mauritius route speed as compared with that associated with the Cape of Good Hope route ; for there cannot be much difference in the routes for the greater part of the way. But did not Mauritius give a too small value in the Alaskan earthquake also? Again, I ask, is there no possibility of an error in the time estimate? Ceram Victoria and Mexico Batavia give approximately the same value for the arcual speed—a point which tells in favour of the accuracy of the time estimates, for the routes are very different in the two cases. Leaving out of account all but the broad features, we may conclude that the speeds (arcual) associated with the Alaskan are distinctly greater than those associated with the Mexican and Ceram earthquakes. But I confess I can give no satisfactory explanation of this, nor can I see why Batavia and Mauritius should give smaller values than the others in the Alaskan group, and why Cape of Good Hope and Shide should give comparatively large values in the Ceram group. And now let us see what comes of taking the chord as the approximate path of shortest time. Interpreted in this way the results indicate that the waves must go diametrically through the earth at a much slower average 76 REPORT— 1900. rate than along a course near the surface. Thus, from the Alaskan group we should infer an average diametrial speed of about 2°2 km. per sec. ; from the Mexican group about 1°8; and from the Ceram group about 2°5. This suggests that the speed of propagation along a diameter de- pends upon the particular diameter considered—a very curious result surely, unless, of course, the depth of the focus below the surface be very different in the different cases. As regards the general question of the diminution of speed at greater depths, all we can say is that it is not impossible. True, the result is un- expected, seeing that there can be little doubt that the preliminary tremors travel quicker at the greater depths. But then it is also certain that the elastic constants involved in the transmission of the two types of waves must be essentially different, and there is no necessity for them to obey similar laws of variation with depth. In my ‘Scottish Geographical Magazine’ article I pointed out that the bulk modulus might increase at a much quicker rate than the density, whereas the rigidity might increase at much the same rate. ‘Tio meet the new need we have merely to assume that the rigidity does not increase so. quickly as the density. We know that the density increases with the depth, and we know nothing whatever about the elastic constants except what we learn from seismic phenomena. It was, in fact, with feelings of surprise that we first recognised the high speeds of earthquake disturbances through the body of the earth. That another type of wave should travel more slowly at the greater depths should not therefore be matter of any surprise, although certainly re- markable. The hypothesis that the large waves really pass along brachistochronic paths seems to require that the speed diminishes with distance from the centre. This means that the paths are convex outwards, concave towards the centre. Hence the paths to points within 90° of the origin will tend to follow more or less closely the are of the outer crust. When the arcual distance exceeds the quadrant, then the paths begin to pass through deeper parts of the earth, and the fall off in the value of the average speed be- comes more apparent. This is precisely what is indicated in the values deduced from the Alaskan group, since it is not till the are exceeds 105° that the value of the calculated average speed shows marked diminution. The Mexican group shows the same feature, but not so the Ceram earth- quake. Still it is only one against five, and we shall be safer in following the five. Comparing the two hypotheses, the surface wave and the brachisto- chronic path, we see that up to distances of a quadrant or so they give much the same result, because the brachistochronic path is largely con- fined to the surface layers. As regards greater distances the evidence in hand is not very clear. Increased ‘arcual speed’ is hinted at, and this, if it exist, is a serious stumbling-block in the way of accepting the surface wave theory. But at best the increase is small, and, except in the case of the Ceram quake, really too small to build any conclusionsupon. I should rather be inclined to say that the evidence so far is in favour of a practi- cally constant ‘arcual speed’ over all distances. But I still entertain strong suspicion of the possibility of surface waves of the magnitude re- quired being transmitted over the earth’s surface. If we take the values of the arcual speeds in the Ceram earthquake as being accurate, we meet what seems to me to be an insurmountable difficulty in the surface wave theory. On the other hand, we have no insurmountable difficulties if we Teh Report Brit. Assoc, 1900] [Puare. 11] Apparent Paths of the Large Waves of Earthquakes from jive origins (indicated by circles) to various observing stations. ‘The Alaska origi for earthgmabes Nos. S53, S57, and S85 might possibly be mored 10° to the east. The velocities, given in kma. per sec. and placed in brackets, refer to paths or portion of Paths, indicated by dotted lines. The earthquakes are indicated by numbers (see B.A. Reports). Mustrating the Report on Seismological Investigation. ON SEISMOLOGICAL INVESTIGATION. Vis take the other theory, although there are difficulties of detail that are somewhat troublesome, Ido not think we are in a position as yet to make any serious calculations. We must get more data and look all round them before engaging in complicated calculations. Character of path in three cases on the assumption that the path is not along the chord, but more approximately along the are. Alaskan. Victoria . ‘ : : . Under sea. Toronto . : i , . Half sea, half land. Mexico . : : ; . Half sea, half land. Shide Ran te : . Mostly sea, polar archipelago, Greenland ? San Fernando . : F . Half sea and land, largely polar. Bombay . ; ‘ . - Mostly land, Siberia, Tibet. Batavia . : : é . Deep sea, east of Asia. Mauritius . : 2 é . Siberia, India, Indian Ocean: Cape of Good Hope . 3 - Polar sea, Europe, Africa. Mezico. Victoria . : ; A . Under N. America. Toronto ‘ ; : cs Fe Shide Ba ete : : . Skirting E. of N. America and then under Atlantic. Batavia . A F a . N. America, Pole, Asia. Mauritius. t : : . N. America, Pole, Russia, Persia, Indian Ocean, or by way of 8. Pole. Ceram. Batavia . : - s . East India Archipelago. Mauritius . : ; ‘ . Indian Ocean. Victoria . : . Pacific Ocean. Cape of Good Hope . : . Indian Ocean. Shide 4 ; . India, Persia, Hurope, Alaskan Earthquakes (333, 327, 338). Assuming constant speed for small distances, we find 9 min. as the time from the origin to Victoria. Hence the following table :— Speed ae of Pass¢0)| aaa Ohord Min. Are Degrees {Chord /Arc Radians| Min. Min. Min. 6 Victoria. . my aN 28 5 — = 1:3 031 ‘031 Toronto. r r 40 68 2 22 22 1:8* “Bl Seal Mexico . . . 49 “Sa| —. 29 28 1:7 ‘29 30 Shide . ri ee LOn ee Dis 39 42 41 1:8 "29 31 San Fernando VTE) (1626 44 44 44 1:75 28 “306 Bombay : . 105 | 1:59 55 55 57 19 28 33 f1- Batavia =. =. 108 | 1:62 — 65 75 | { oe 23 24 Mauritius. 146 | 1:91 90 — 88 1:63 215 284 Cape of Good Hope 165 | 1:98] 88 89 83 1:9 226 33 78 REPoRT—1900. Mexico (250, 381). Assuming 21, 22 mins. as times from origins to Victoria ! Are Chord Time in Min, oe a om in. Min. Victoria : 1-1 30-32 *B2—"55 21-22 1:4 025 Toronto ; . 84-86 *58—62 23-27 1:4 25 Shide . : 80288 | 16292Iea5 52-54 1°52 25 Batavia ; 5 DO 1:93 108 1:39 ‘18 Mauritius . 70 260 WESi7¢ 113 1:41 175 Ceram (347). Time calculated as in Alaskan earthquake. ; : Arc Degrees | Chord Are Chord Time Min. ‘Min, 2 Min. Batavia . ; : eee, 38 | 14 by ‘027 Mauritius 5 fe i83 EIS) 47 1:55 25 Victoria . : . 105 1'59 74 1:42 ‘22 Cape of Good Hope. 105 1:59 6L 1:72 “26 Shide A Bete I 1:74 71 here 246 Ebon. saa pd ES may be reduced to os by multiplying by 1:06 min. min. arc degrees sion Si ee ” ” 9 ” ” ” 1:84 min. It will be noted that there are certain slight differences between the figures used in this last table and those in the table on p. 81. These, however, do not produce any appreciable effect upon the general character of the investigations which have been made. . The Origin of Larye Earthquakes which were recorded in the Isle of Wight in the Year 1899, Tn 1899, at Shide, in the Isle of Wight, 130 earthquakes were recorded. One hundred and five of these were also recorded at one or more of the following places: Kew, Toronto, Victoria (B.C.), San Fernando, Bombay, Madras, Calcutta, Mauritius, Batavia, Cape of Good Hope, Tokio, Cairo, and Mexico. There is no doubt that many of these were also recorded at other observatories, but from these registers have not yet been received. The localities at which a certain number of these earthquakes originated have been determined with a fair amount of accuracy. Other determina- tions are somewhat indefinite, whilst a large residuum of comparatively small disturbances have been grouped as having originated somewhere in the vicinity of the one or two stations at which they were recorded. The results exhibited in map (Plate III.) are therefore of varying values, and although they give a general idea as to the distribution of seismic activity for "1899, they are chiefly of interest as-illustrating the character of the more definite information which we may expect to derive from the extension of the present system of observation, ON SEISMOLOGICAL INVESTIGATION, 79 The methods and considerations which have led to these determina- tions have been as follows: (1). Determination of Origins by Comparisons between Time Intervals. Earthquakes from the same district will arrive at distant observing stations at times the differences between which will be constant. If, for example, we have once determined the difference in time at which an earthquake originating off the coast of Japan arrives at Batavia, Bombay, Cape of Good Hope, Shide, &c., whenever these differences are repeated at four or more stations, without knowing anything about observations in Japan, we can at once say where such an earthquake has originated. It will be noted that our knowledge respecting the speed with which earth- quake motion is transmitted enables us to give approximate values for the time differences here considered. (2). By the Difference in the Times at which the Maximum Motion has been recorded at different Stations. In the present state of our knowledge all determinations of the position of origins from time intervals require the assumption that the velocity of propagation of earthquake movement is constant. This condition is most nearly fulfilled by the large waves of earthquakes. The methods by which an earthquake origin may be determined from the differences between the times at which it was recorded at distant stations are several. The method of circles which is here employed has been selected chiefly on account of its comparative simplicity in application. It is briefly as follows : If the large waves of an earthquake reach stations B, C, D, &c., four, ten, twenty, &c., minutes after reaching station A, then the centre of a circle which passes through A and touches circles drawn round B, C, D, &c., the radii of which are respectively 4 x 1°°6, 10 x 1°-6, 20 x 1°°6, &e., will be the centre of the origin required. The constant 1°°6 means that the arcual velocity for large waves is taken at 1°-6 per minute, or approximately 3 km. per second. In the British Association Report for 1899, p. 193, the speed there given was 2°5 km. per second, which appears to be too low. The operation of drawing these circles is carried out on a ‘slate’ globe. For a complete solution observations are required from at least four stations. With only three observations we are left to choose between two possible centres, but as these may be widely separated there is usually but little difficulty in selecting the one required. (3). By the Time Intervals between the Arrival of Preliminary Tremors and Maximum Movement. From what has been said respecting preliminary tremors and large Waves it may be inferred that the interval in time between the appearance of these two phases of earthquake motion at a given station has a relation to the distance of that station from the origin. This relationship is shown in fig. 1. An observer with this curve before him, although his time- keeper may have failed, or although he may be so situated that it is impossible to obtain accurate time, is immediately able to determine from a well-defined seismogram the distance at which the motion it represents originated. With this fact, the magnitude of his record, and a knowledge of the physical configuration of districts from which earthquakes originate, he is frequently able to locate an origin. With time records from several 80 REPORT—1900; stations the distancés corresponding to each of them from an origin ate read from the curve, and by the intersection of these on a globe seismic foci are determined with greater certainty. (4). By the Intervals represented by Seismic Recurrences. Whenever a seismogram shows thé interval of time between a maximum movement and a distinct reinforcement of vibrations which can- not be accounted for as forming part of the gradually decreasing surgings following the principal disturbance, this interval enables us to state the distance of the origin from the station at which the seismogram was obtained. Opportunities to apply this method are not frequent (see p. 68). 14. The Application of the above Methods to the Records for 1899. To carry into effect the method of determining origins by comparisons of time differences, the following eleven tables have been prepared. In these the 105 Shide records are referred to by their British Association register number and their date. For each of these the time intervals between the arrival of maximum motion at the station beneath which a zero is placed and its arrival at other stations are given in minutes. In those instances where the time at which an earthquake originated is approximately known, as in Table I., the zero is placed beneath the word ‘origin.’ So far as possible the various earthquakes have been analysed according to the localities from which they originated. When the time intervals in a series are less than three in number, the location of an origin is sometimes doubtful. A dash beneath a station indicates that an earthquake was observed, but for reasons which are various the time of its maximum could not be determined. A query indicates that an observation is uncertain. TaBLe I. West Pacific. Japan. o F 5 Sie : a| = ) ie | ia & = 8 ~ s Sn [tite os [ers S - | = S = a oe a é 2 z 5 i s zB 3 E = 2 Origin His/_g/a |/A8ls/also] 8 a] 8 % PIG a 0 Distance in | 87 | 87 | 90 | 62 100 65 57 |102 | 62 | 52 136 87 0 degrees Expected time | 57 | 57 | 59 | 38 | 65 43 35 | 66 | 38 | 35 85 57 0 to travel in mins, 366. Nov. 24 .| 57 | 58 | — | 32| 68 | 37 | 14] 51] 37] — 68 60 Japan . be 2) ) eee 364, Nov. 23 . | — | 20?) 58 | 32 | 64 40 31 | 64 | 54 | — 1 or 85 | f ” 360. Nov.18 .| 46}—;|—}|—/—/; — |—]—|]—|]— _ _ Py 357. Nov.10 .| 50} —}—/—]|—/ — |— — a — Pa pAb ayivdiy zp 5) sey) S|) PSS 1) 0G) |) 8 — i} — 307. July 11 . | 17?) — |} 17 | 39?) — — 17 | 21}—}— _ _ 9 306. July 10 .| 53 |—|—|—]|—)| 48 _ — and 295. Junel7 .{ —|— | 58 | — | —| 67? |} —} —}—]— — = Philippines ? 263, March7 .| 58 | 58 | 68 | 23} —| 47 17} 42)}—|— _— — Japan 323. Aug. 3 .| 57 | —] 20} 21) — _ —-}—|— _ _ as The above earthquakes were recorded by seismographs in Japan, and therefore originatedin or near that country, ON SEISMOLOGICAL INVESTIGATION. 81 _ In very many of these entries there must be errors, the reasons for the existence of which have already been explained. The values of these vary between a fraction of a minute and several minutes. Where origins are known from observations made near to the same these are stated. The geographical positions of these origins are shown in map (Plate IT.). Some of the entries on this, particularly those for the Atlantic and Indian Ocean, are conjectural, whilst others may be taken as correct. The reliance which can be placed upon any particular determination is shown in the table of time intervals on which the same is founded. 263. This earthquake, which is described in the British Association Report, 1899, p. 212, and was recorded in Tokio at Oh. 59m. 29s. G.M.T. March 7, is of interest as showing that the amplitudes of motion recorded at Shide and Kew were greater than those recorded at Toronto, whilst at Victoria, the nearest station to the origin, but reached by a sub-oceanic path, it was the smallest of all (see p. 70). Other earthquakes, approximately corresponding to entries in the Tokio register, and which may therefore have originated near to Japan, are Nos. 271, 286, 314, and 363. Nos. 351 and 352 may have originated to the east of Japan, about 40° N. lat. and 160° E. long. ‘Taste Il. West Equatorial Pacific. East Indies. Remarks ! Shide Kew Toronto Victoria (B.0.) San Ternando Bombay Batavia Mauritius Madras Caleutta Cape of Good Hope Tokio Distance in | 121 | 121 |136|] 105 | 132 62 | 22 | 73 | 53 | 60 |105| 47 | These entries re- degrees late to the Expected time | 76 76 | 85] 66 84 38 | 16 | 45 | 33 | 32 | 66 | 29 origin. intervals 1 an 0 He 18 | 60 | 18 According asthe or 57 |or57 (| or GO| or 17 jorl5 f | or33 or 5 |or47| or 5 347. Sept. 29 { 70 ig fe a0 Ber 40 Batavian max. is 17:11 or 17°24 247. Jan. 12 . 63 — |—|]; — —_— 2 0;};—};—|/—}|—]— — 298. June 24 .| 57 — | 56)! 71 — 13 0 ;15};—}/—|]—}]— = 299, June 29 . 60 _ _— 7L — 7 0o;];— ee = |) eof = emmy iets tale Gen |ees~ 3p )2)r48 fier [fe |r Or | |! ee | ep =, 324, Aug. 4 .| 65 | 26/ pare }] s2 | 1s | o | 42} a1] 32 | 58 | — As 332. Aug. 24 . 71 70 52 35 13 — 0 |}49}—|{—]59} — — 64 { 56 40 50 354, Oct. 19 { or 68 \— ~ (| or 52 \— a of or36 \i-{ or46 \ 5 c; 355. Oct. 24 . 61 — 91] 61 — _ 0 | 3} —|— | 46 | — _ 347. Dr. J. P. van der Stok in the ‘Kon. Akad. van Wettenschappen te Amsterdam,’ Nov. 25, 1899, tells us that in the night of Septem- ber 29-30, at 1.45 a.m. (September 29, 17h. 9m. G.M.T.), an earthquake, followed by sea waves, damaged the south coast of Ceram, and, in less degree, the islands of Ambou, Banda, and the Ulias Isles. Several villages on the south coast of Ceram were destroyed—in Elpapoeti Bay _ all except two. The prison at Amahei was completely destroyed, and the fortifications partly so. nok D. M. Verbeek gives an account of this earthquake in the ‘ G 82 REPORT—1900, ‘ Javasche Courant,’ 1900, No. 21. He gives Amahei time for the shock as lh. 42:2m., and that for Wahei as + lh. 43m. (17h. 7m. G.M.T.). At the former place five to ten minutes after the shock, the coast was flooded by a sea wave. This inundation, to a height of 1-7 to 9 metres, was also experienced at other places along the south coast of Ceram. At Banda, 187 km. south-east from Elpapoeti Bay, the water began to rise about half an hour after the shock. At Kawa, at the west end of Ceram, and at other places, strips of alluvium were submerged. Dr. Verbeek places the centrum a few miles inland to the west of Elpapoeti Bay, on the line - of a fault running parallel to the south coast of Ceram. The time intervals between the shock and the sea wave observed at Amahei indicate an origin at a distance of -5 to 1 degree from that place. This would probably be sub-oceanic, and on the face of the Webber Deep, where soundings have been obtained of 4,000 fathoms, As it is possible that there may have been a bodily displacement of materials lying between Ceram and the Webber Deep, this does not interfere with Dr. Verbeek’s fault line. The time at the origin may therefore be taken as lying between 17h. 7m. and 17h. 9m. If the maximum observed at Batavia took place at 17h. 24m., and the movement took 15 minutes to reach that place, we again reach the conclusion that the time at the origin was about 17h. 9m. G.M.T. Tasup III. Mid-Indian Ocean. — Shide Toronto Batavia Madras 288. May 15. . : 5 5 56 _ 0 61 313. July 20. ‘ i . 5 422 89 9 =e 319. July 29. 5 : ‘ 5 45 — 0 — TaBLE TV. North-east Pacific. West of Alaska. | 5 Ae is | Olsg es 4 a SO y rs islelalelal2 | #4312 143 [els - fife || Res | AL Gea. Es Spe (oreo R= P= | 8 & a | rd Remarks lmal|s!1s| S| E) 3 | 2 os Reg) es / Fh al seed 1 hE ar ae ae | |e | a Be S Sono 5 1 ee Ee eee | ee Distance in de- | 70] 70} 40) 20} 77 | 100 108 {145 | 105 90 | 165 | 49 | 50 | These en- grees tries refer | Expected time in- | 44 | 44 | 25 | 14 | 48 63 68 92 67 57 | 104 31 |} 32 to the tervals origin. 13 100, (7 883, Sept.3 . «| 80] 30 /f>3.J}0| 36) 47 | — | ar) — | —|{gfol}—| {761 t 337. Sept. 10 . Sale) 20 0 | — | 22 |340r33/500r43| —*|390r38} — |690r67| 7 | — | Small 338. Sept. 10 . - | 20 | 19 0} — | 22 35 63 64 _ = 61 CN i= — 246. Jan. 12. «| 23 | — | 13 o;— 2 = — —_ -- — —|— —_ 266. March 19 30 | — 97) 0") = = Bi We OF (A ll Be —_ 282. April 16 BIg (9 |! 16y)' 40 | 4) ee | oat eT ee ee | eS = 334. Sept. 4 —|— 9} 0; 3) — — |< — |---| — |—|— _ 341. Sept. 16 AS11800) eS")! 7:5 a aS tier) | EEN ee = 342, Sept. 17 27] 27 | 10 0 | 34 47 — — 48 —_ 76 — = 344. Sept, 23 25 | 81 | 11} 0| 85] 50 60 | 7727] — |—| 72 | —| 27 = 345. Sept. 23 33 | 37 | 17 0 | 38 63 _ _ _— = 87 A = 309. July 14 ata [pe 9 0 | 14 13 — 14?) — — 35 — | — | BehringSea 317. July 27 llj— 6 o;j—y; = = = — = —_ ii — | | | ON SEISMOLOGICAL INVESTIGATION. 88 Nos. 333, 337, and 338. In the ‘Toronto World’ of September 25 we read that on September 3, about 2.30 p.m., houses in Yakuta Bay were rocked violently, doors were slammed, dishes rattled, and tables moved. On September 10, about eight o’clock, a more violent movement occurred. Trees swayed, and there were slight shakes every few minutes. Just as the earthquake ceased tidal waves came rolling in. There were three of these waves following each other at intervals of about five minutes. The rise was 15 feet from low tide to a foot above the highest tide point. On the island of Kanak, opposite Yakuta, a graveyard sank so that on the next day a boat was able to row over the place where it had been, and the tops of the submerged trees could be seen. These shocks disturbed the declinometer, duplex, and vertical force magnetographs in Toronto. Scanty as these notes are, they apparently indicate an origin somewhat to the east of that shown in Plate III. The period of the earth waves for No. 333 as recorded at Shide was 15 seconds, whilst the maximum angle of tilting was 8’. With a velocity of 3 km. per second, and the assumption that the motion is simple harmonic, so that the height of the waves= Be tan a, where /=length of wave and aT a=maximum angle of tilting, we may conclude that these waves were 45 km. in length and 29 cm. in height. With periods of at first 40 and afterwards 15 seconds for the disturbance recorded in the Isle of Wight on September 10, No. 338, it would appear that at first there were waves 120 km. long and 39 cm. high, followed by others 45 km. long and 43 em. high. Whether we can accept vertical displacements of this order repre- senting accelerations not unfrequently ;\, of gravity is yet sub judice, and an experiment to confirm or modify these conclusions is now in progress. Taste V. Last Mid-Pacific. West of Mexico. d| 3 i Ei 2} a eb 2 S 3 oe aos he fe faerie _ Z| g o | +a 8 q 8 5 3g 5 o Origin 77 SOS S x 2 si 3 HH H a) a ios) i=.) S oO ° Pl a rot oS io) Distance in | 84 84 34 | 30 86 148 150 168 148 138 138 0 degrees Expected time | 52] 52 | 22| 20] 54 93 95 | 105 93 87 87 0 intervals | S| >| | —_— —_ | | , —. 250. Jan. 24 «| 31 81 38); 0; — — 92 — — — | Mexico 381. Jan.20 .| —| 32 2 )...0.), — — 86 — — — -~ 59 248, Jan.14 . | 37 { a k2}o0) —|—}—]—}]—-]-] - ql 321. Aug.2 .| 30 30 o;/—|] — oo — _ —- — | Concepcion ? 294? June 14 . | 32 30 0 | 34 16 70 — 72 _ — — | Jamaica ? 371. Dec. 25 «| 47 47 |16|] 9] 60 —_ _ _ _ 75 | 8. California 250. The key to the origin of this group is given by earthquake No. 250. From Seiior José Zandizas, director of the observatory in Mexico, we learn that it took place on January 24, 1889, at approximately 11h. 45.5m, P.M. It was severe, caused some damage, but it cannot be siad G3 84. REPORT—-1900, to have been very strong. It was felt over the whole republic: At Colima, on the Pacific side, it had a duration of Im. 20s., and on the Atlantic side, at Vera Cruz, it lasted 10s. By the method of circles and by the method of preliminary tremor intervals I place the origin at a point 30° distant from Victoria, and 34° from Toronto, or near to lat. 19° N. and 105° W. long. On January 20, 1900, *No. 381 was recorded in Mexico with time intervals similar to those for No. 250. The preliminary tremor intervals for this referring to Victoria, Toronto, and Kew read 13, 15, and 38 minutes, indicating that the Kew reading for No. 250 is the lower of the two values given. The time readings for 248 clearly correspond with that for an earth- quake with a similar origin. 294. An origin 8.W. of Jamaica roughly agrees with the time differ- ences between Toronto, Victoria, and Shide, and the preliminary tremors duration for Kew and Toronto. 371. In ‘ Nature,’ April 19, 1900, we read that on December 25, at 12.25, an earthquake took place in 8. California. In the villages of San Jacinto and Hermet every brick building was damaged. Professor F. Stupart sends me the following extract from a newspaper clipping : Los Angeles, Cal., December 25, 1899. The towns of San Jacinto and Hernet, in Riverside County, were badly shaken by an earthquake at 4.25 o’clock this morning. In San Jacinto not a brick house or block escaped injury. Nearly all of the business portion is in ruins. The new Southern California Hospital caved in. It was not occupied. At Hernet the Hernet’s Company mill is partly down. The front wall fell flat. The rear of the large Johnston block also toppled over. Hernet’s new hotel is a ruin. The damage at those places cannot be estimated now. Communication by wire is inter- rupted. The‘ Herald’ has received a telegram from San Bernardino saying that six Indians were killed at Hernet by falling walls during the earth- quake. The Santa Fé railroad report is to the effect that no lives were lost. Los Angeles, December 25.—The total damage at San Jacinto and Hernet is estimated at $50,000. No person was injured at either place so far as known. The shock was heavy at Santa Ana, Anheim, San Bernardino, Riverside, and other places, but no particular damage is reported except from San Jacinto and Hernet. In this city no damage was done, though the shock was particularly violent. The houses here are well filled with Eastern tourists, and they were in many instances terrified at the unexpected disturbances, and rushed from their rooms. San Diego, Cal,, December 25.—The most severe shock of earthquake experienced in this city in fourteen years took place at 4.25 a.m. to-day, and was accompanied by a loud rumbling noise. The taller buildings in this city were severely shaken, but no serious damage was done. A high wave struck the beach ocean front, but no |damage was done. A slight shock followed the first a few seconds later. 268. The time intervals for Shide, Victoria, Bombay, and Toronto suggest an origin near to that given for 322, with which the preliminary tremors for Victoria and Mauritius accord. In the British Association Report for 1899 this origin was placed on the western side of the Atlantic, but additional data haying since been obtained this is now modified, ON oo ON SEISMOLOGICAL INVESTIGATION. 85 TasLe VI. South-East Pacific. West Coast South America. oO ° ° 4 a i 3 a nm i] iy] ae Mets Wy fh Bo he Bo Peau bes 5 Origi n ima] 5 5 5 gS 5 5 rigin fo 8 - Q =a] S =| 5 P| & Sae,Aug. 2.) 25 23 0 _ _ — _ _ Concepcion. S21. ,, Bw 36 30 0 — a — — —_— — — | Chili? See W. | of Mexico, | list V. 268. Mar. 23.| 10 14 0 11 ? 41 — 23 | — - S.E. Pacific. 269. ,, 23. 22 29 0? 20 —= —_— — _ —_ 2 _— 270; 3°) 25. |85ors! 2 | 0 mes WETS al SEN a a = 278. April 12.| 26 36 0 20 -- — — — 43 — W, of Chili “5 ie Ca 21 31 0 14 _— — — _ 44 — — 291, June 5.]| 33°? 0 0 15 _— — 11 _ _ ~- _ 292. ,, Dien |caare SO lie, 0 Tpke | Soe ea ee lh lh id 322. The time intervals indicate a possible origin, about 80° due south from Toronto, or off the south coast of South America, near Concepcion. As this earthquake is not a large one, the whole of the preliminary tremors have not been recorded, and therefore these indications may be neglected. The similarity of the seismograms for this earthquake and that for 321, together with the fact that they succeeded each other within two hours, suggest a similar origin, and Professor F. Stupart, of Toronto, writes me to the effect that it is probable that both originated off the South American coast. TaBLe VII. North Atlantic. North Norway to Spitzbergen. o 5 S| 3 ty % a e n a a 3 S £ - § 2 5 5 = Bey 3 ° . S a EI & 5 s ba S F a 44 | Origin alB EEE |e lalelalals|a r= mS) q [<2] A s o zo) e | a 2 3 o 252. Jan.31| 0 Ob |) 124}. 16 >f—-f}f—-f—-f}f—-}-]- 954, Feb.23/ 0 | ? | 18 | 19 | — | —}| —]|—}—]—]—] = - spies SG OW Pel se | sof — | — | — | — fae = = Taste VIII. Equatorial Atlantic. |e sue] o | wo | 8 | ao] 2 | o | — 3 | 94 -|-|-|- TaBLE IX. Western Central Asia. Turkey in Asia. 343. Sept. 20 0 2 33 40 10 14 _ 34 _ _ 29 30 leet 373. Dec. 31] 4 Obs | 3ieu lle 40 5 | —|— | 14] — | — | 26 | -6 | Tiftis | { | 343. From ‘ Nature,’ January 25, 1900, we learn that more than 1,600 persons were killed, more than 2,000 were injured, whilst 11,000 houses were destroyed. The epicentre was in the Meander Valley, between Aidin and Sarakim. Along a line of sixty miles in this valley there are many 86 REPORT—1900, damaged towns and villages. This valley and the Legens Valley have subsided from 2 to 6 feet, The railway line between Aidin and Omourlou was raised fully one yard. 373. From ‘Nature,’ January 25, 1900, we learn that the earthquakes of December 31 destroyed many houses at Akhalkalaki (Transcaucasia), Here and in ten neighbouring villages over 200 people perished. At the Tiflis Physical Observatory the following observations were made. In Greenwich mean time the first shock was at 10h. 51-4m. It was severe in the hilly part of the city, on the right bank of the river Kura. The second shock was feeble and noted at 13h. 39°5m. The third shock was not noted by the seismograph at the observatory on the left bank of the Kura, but was noted at 17h. 45m. on the right bank. At Kalagelan the first was observed at 10h. 49m., and at Sviri and Zugdidi at 11h. 23m, The latter places are on the Kars Railway. At the railway stations, Abastuman and Kobi, the times were 13h. 51m. and 11h. 2m. TABLE X. Origins which are extremely doubtful. 2 3/8 wodekutt Slels a e| es - cy | casas BANo |3|/S/8/2) 5) 9/8/58 /38/ 8/6 Origin ee lslelalars/ais)s | 8 ro) Ba a | oD 245, Jan. 6 oa" 6 ? o;— ? ?}—|—|—|—]—| N. Atlantic, W. side. 249. ,, 22. 4 0o;—|—|- ?|—}]—)}] ——| — | Greece ?. DbIs 5, 30... 264 | — ?/—| 4)—{|—J| 0} —] — | Indian Ocean, E. side. 253. ,, 31.) 16) 15) —}—}]—)] OF} — | — p—}—]— ” » WwW. side, 256. Feb. 27 . 2 2. 0 | 57 ? ?/—|—|]—|—|—]| W. Indies. DAN ey eee 0/05);—}—/]—|—|—]|]—|]—| —| — | N. Atlantic, E. side. 2Dose hk 2S cer AO Oss ? ? ?}/—!|—|]—|—]—|N. Atlantic, C. Verde. 260. , 28 .)/ 0}|—}—]|—]|—]—]—]—]—]—]—] Trieste 13 min. after Shide, N. Atlantic, W. side. 262, Mar. 6 .| 22| ?}—|—{|—]—]—J|—]—|—]—| Nicolaiew, before Shide, Caspian Sea, 264 , 42 4) .28) 21) O | Lf |i—s} 2) | eel 2h) — je? | — | Origines. Pacitie: The magnitude of the seismo- grams indicates that Toronto was reached before Shide and Vic- toria, The maximum was not well defined at Victoria, whilst at Batavia the movements were only recorded as a thickening of the line. The position of the origin was apparently in the Mid-South Pacific. 26%on., 2 146}; ?}—|—] ?}/—]|—|—]—J| ?|—| Trieste, before Shide, Caspian Sea, 273. April 4 .}| 0{—/]—/]/—j]—|—|—j|]—| ?]—|—]N. Atlantic, E. side. Size SNE Sp mee (recy {lime Ue Mat Sa essen [ees Pe (PG EES | ee a 4 281. , 15 Sf ee ae ae ae dt ad ae el ad = mR 283. ,, 17 ./ 43} — | 34} 0} —]—}]—|—]}]—|—]|—| N.E. Pacific. 284. , 28 .|—}|—|]—/|—|—|]—]—]—|—! —| — |] N. Atlantic, E. side. 289. May 17 .| 19 | —| —| —|—|—J] 0|—]—J| —]| — | Indian Ocean ? 293. June 9 .| 1}—}—/]—/]—|—]—]}] OJ —}]—}]— 5 i. 297. 4 19 .};—|]—}]—|]—|—|]—]—|—]|]—]|]—|—]|N. Atlantic, E. side. LOO ATU Sf i PF | | | oS 3 301. , 2.)|30);—/]—)| 0} —} ?|/—|—]|—|—|—| E. Pacific Ocean. 302. , 38 .}/—{—]—!}—|]—|—|]—|]—|—|!—|—|N. Atlantic, E. side. 303.9, @ i) 9) 110) 4) | — | 21) —} — | — |] =| N. Atlantic, W. side. 305. 4 9 .| 46] 50] 86 | 75|—| 6] —]!]—] O| —]|— | Equatorial Indian Ocean. a2. yy Oe 2} — |} — | — 2} —|—!|—|— | —| — | N. Atlantic, E. side. 315. 4, 26 4;—]—/;}—|—] 0] —|—|—]—| — | Indian Ocean. 318. , 28 .};—|—|]—]—]—|—|]—|—]—|! —|]—] N. Atlantic, E. side. 220. , 31 .)/—|]—}]—]—|—]—]—]—]|—]| — | — | Indian Ocean ? 825, Aug. 7.| 9} 9}/—|—}]—] OJ —}/—]—| 0} — a Rs 326. , 17..| ?| ?| 386/17] 24) 0] —J|19]| 3 | —/| 28] astern Hast Indies, 827, 5, 21.) 21°?) —] —) —) — |] HK] — 1 | om Atlantic; E. side, 328. ,, 23 ..] ?| ?}/—}/—|/—|]—]—]—]|—|—-|]—- a a 329, , 28.) ? Pl—J—lm—il—l—l—J|]-l—-l- vs ON SEISMOLOGICAL INVESTIGATION. 87 TABLE X. Origins which are extremely doubtful—continued. 2 . So ° a 2 a a Hi B. A. No. 2 g g = | 2 E 8 5 3 g & Origin Als |a/alals|s|s]s ee a o e wD a io) 335. Sept. 6 . | 29 0 — —|—|—|—| W. of Mexico. Group V. aieeeeGe | Oi!) Lop —— f— | — | — | 2 || — || Midi NeAgiantre: 340, ,, 14.]/11)/—} 0) —|/—|]—}]—|—]—|—]—| N. Atlantic, W. side. 346. ,, 27./ 6| 6} 0} 15 | —| —} —}]—]—]—] 7 | Mid-Equatorial Atlantic ? 349. Oct. 4.) —|—|]—|]—}—|]—]|]—|—]|]—]|—|—|N. Atlantic, E. side. ee eeet ses |) 36's) sl |) Ti —|—.| Ol —sh—s t=) 2 = 352, . 13 .|33|38|/—| 9 0 = 63 | E. of East Indies ? 356 ai 29 o;—)/—|—!]—] — |] 5 | —| — }] — | — | Indian Ocean. 358. Nov. 12 11 | — | —} 27; —| —} 0|—}—|—]} 49 | S. Pacific. 361. 5 18 25| 2) 0|393/ 3|—|—]|—{|—]—] 3] Mid-Equatorial Atlantic, 862. ,, 20 42}—| 33] 0} 4/—}]—}]—]—|—|— | Pacific Ocean. 365. 4 24 58 | — | — | 50 | 63 | 20 0} 38/—}]— 9?| Japan ? 370. Dec. 17 .| —| — |} —| —|—|—|—]—|/—|—|—|N. Atlantic, E. side. 372. yy 26) 3 | 20 7?) 1) 18 0o|/—}|}—|—}]—|— | 35 — 374. ,, 31 .| 512] 25 | 41 | 34| 33) 0] 10} —| —| —| 48 | Japan? The origins indicated in the last table are for the most part conjectural. In those instances where a disturbance has only been recorded at Shide and Kew, and we are without evidence showing that the seismograms refer to earthquakes observed in Great Britain and Europe, it seems pro- bable that they represent adjustments in the strata on the eastern side of the North Atlantic. Time entries for these stations, a few minutes later than the corresponding entry for Toronto, suggest that we are here dealing with a disturbance originating on the western side of the same ocean. Origins indicated by terms like Indian Ocean and Pacific Ocean only show how little information can be derived from certain seismograms. Here and there a few impossible entries are recorded. For example, the greatest interval of time which could elapse between the arrival of an earthquake in Mauritius and Bombay or Madras is thirty minutes, yet for earthquake 326 it will be observed that the entries for the latter places are respectively forty-one and forty-five minutes. To correct such entries it is necessary to compare together the original seismograms, which has not been always possible, 15. Illustrations of Seismograms. The following illustrations of seismograms are only to be regarded as sketches of the original photograms. The accuracy of any given reproduc- tion has been largely dependent upon the clearness of the figure from which it was copied. They show the range of motion and the principal characteristics of wave-groups, but they do not show details like small serrations so clearly exhibited in many of the original records from which they have been reproduced. The numbers correspond with the numbers given for particular earthquakes in the preceding text and those in the Shide records contained in the first circular of earthquake registers issued by the Seismological Investigation Committee. The arrow with its time- mark gives the time for a particular phase of movement, which is usually that of the commencement. |The number following the letter S gives the time-scale in millimetres per hour. Thus S=60 means that 60 milli- metres equal one hour. 88 REPORT—1900. The locality at which a seismogram was obtained is indicated by the following initial or initials :— Isle of Wight (Shide) . S. Bombay - : : ae Kew : ; ce Calcutta ; : 2 oulG: Toronto , ; ; als Batavia ; ; : > Ba. Victoria, B.C. 5 See Mauritius : ; . ME: San Fernando é BS hIuG Cape of Good Hope. =») CGE Madras . : : «| Ma. Tokio . 5 : : 5 AMO} Mexico . 3 ‘ - Me. 17.55. a eS ee owe . | No. 278—T, S=59°5. x a Te c—) >) é pee? t a ve 18,19. : L No, 278.—V. S=60'5, 4.28.5. 4.37.7. ’ cp 4 { No. 279.—S, 7 os 4.9.1, rn Y v m ——.___a——>k——z—=xz=£=_—— No. 279.—T. S=59:5. wa I 2 a 5 4 4.26. A No. 279,.—V. S=61, No, 282.—5. §=58, No, 282 —T. S=59, ON SEISMOLOGICAL INVESTIGATION, No. 283,—S, S=58, No, 283,—T, S$=59, = 7 NY RR te or : No, 283.—V. S=60°5, No, 291.—V. 8=60'5. 15 .17.7. No 292.—T, S=52, 89 90 REPORT—1900. 11. 13.8, | No, 298.—M, S=58, 17. 56.2. =_= = No, 298.—S. S=58, Repetition 58. No. 309.—S. 8 ON SEISMOLOGICAL INVESTIGATION. 91 No, 305.—8. S=58. No. 308.—B. S=59. No. 308.—M, S=58'6. No, 308.—S,. S=58, No, 308.—S.F, “6s=S “I—"60e ON "PB" ST ‘PIS ST REPORT—1900, ‘$68-S “H'D)'0—'60E ‘ON i noiyadesy 92 ‘CLP $1 ON SEISMOLOGICAL INVESTIGATION. 93 14. 50.2, peeenateenmmnerenmen |\' cme ene eee +t No. 321. S=58, 15. 27.95 59, No, 321.—T. S=68'5. No. 309.—V. § Cee Q T No, 322.—S. S=58, No. 322.—T, S=58°5. No, 324.—B, §=59. No, 324.—Ba, S=59, 94 =59°5. No, 324.—C.G.H. 58 58, No. 324.—S. § Air Tremors REPORT—1900. cs fi { {P f iT lu > No. 324.-M. S=60, Ss . 2 a ll | a a : S Gi 2 | s a of 6 4 <= _— 16 .19.0, No, 382,—M, §=58'5, 59. s= No. 332.—0.G.H. 95 ON SEISMOLOGICAL INVESTIGATION. ee NM aaigmoe fi Beet tip af tp ‘9=S “M—EEe ‘ON axons tlt ‘6S=S ‘H'D'O—'SE6 ‘ON De {| Wt WM i‘ : tly hy beryl ‘es=S “d—‘sss ‘ON \ < a h \ pan Melis | v \ *9°se “0 “C.8S=S ‘OL—seg ‘ON ‘O9=S “ses ‘ON 1900. "G-89=S ‘“d'S—'eee ‘on hy { I REPORT “8S=S ‘S— see ‘ON ‘6s=S “NW—'Ess ‘ON 96 ‘SIS'T ‘yo woog 97 ON SEISMOLOGICAL INVESTIGATION. “\LI—"Lé6 ‘ON ‘99=8 ‘W'S—Les ‘ON “VLP LT ‘09=8 “M—Leé ‘ON ‘09=S “WA— LEE ‘ON A pee eee seme SES Peco “69=S “A—'SEE ‘ON Dre age Apwieaanijny NIN) noljjedour ui ‘¢8S=S “d—L&6 ‘ON Uh Y ‘qo “yo moog m00g Ht 98 REPORT—1900. No. 338.—Ba. S=60. < Boom off. No. 338.—Me. S=59. 2. 23.9. ; none ‘fh fh nn TT He Ne eae end Ds uty No. 343.—B. S=59. Di oe ee be Foe S a ee No. 343.—C.G.H. S=59. pee ya ee ED ON ee No. 343.—K. S=61. No. 343.—M. ==59. ON SEISMOLOGICAL INVESTIGATION. 99 Seema me 4 OS er ae \? No. 343.—To. S=61. 12, 5,7. EE arta rim cas ib No, 344,—B. 11. 23. 3. No. 344.—To. S=58. \ t No. 344.—V. S=60. ill ; 14. 42.1, \Y = —E—=E—__— No. 345.—B. No. 338—B. S=59. 1900. REPORT 100 *2.09=S “MH 8 ‘ON ti) tem — ‘6S=S ‘“H'N'0—"8és ‘ON "98S=S ‘L—'sés ON "89=S “N—'8éé ‘ON Ah. ewan hh ANIM Weyl ashy he ; "OL * SS R eter 101 98S=S ‘N—'Lbé ‘ON =§ “M—L7é ON mn acnstadenoeme agi} Uy yes il ON SEISMOLOGICAL INVESTIGATION. hm Newer ‘po moog 1900. REPORT 102 ‘8.g9=SE’s—F9¢ ‘ON a Te ee antl ye renin \ — He ff) ereaier 7 ‘6S=S ‘OL—'1P§ ‘ON ay ‘6S=S "S—LPE ‘ON BGS * LT 103 INVESTIGATION, ON SEISMOLOGICAL ‘3.89=S “L—79¢ ON "SG=S ‘W--~''96 “ON ‘6S=S ‘H'p'0—'P9é ‘ON ee es Ts sorta ore ‘6S=S ‘d—'h9s ON h ‘i : Its eS it eS air i i ‘OT’ OL ‘9.68=S “A—'b9E ON "v'98'6 1900. REPORT 104 19, 19.8, v 59. No. 366.—B. S$ S=59'5. No. 366.—Ba. "agc=9 ‘S—TLE ‘ON a emia ‘“6S=S ‘S—'998 ‘ON ‘sS=S ‘W—'99¢ ‘ON ‘09=S “A—'P9S "ON onoo dnote inthe ‘ ‘= ‘L—'TLe ‘ON ‘sirer T 7 "PEP SI ON SEISMOLOGICAL INVESTIGATION. 105 No. 371,—V. S=60. III. Harthquakes and Timekeepers at Observatories. That earthquakes we can feel frequently accelerate, retard, or stop clocks with pendulums is a fact well known, but the extent to which eryptoseismic disturbances which sweep over the whole surface of our globe many times per year affect this class of timekeepers has not yet been investigated. ; Father J. de Moidrey, 8.J., of the observatory at Zikawei, gives me the following notes on this subject. On June 12, 1897, ‘an excellent clock facing north lost 4m. 44:5s. in the afternoon, whilst another, almost identical, fixed to the same brick pillar, but facing east, was undisturbed (rate O-ls.). Secchi’s barograph shows a slight stroke at 11h. 25m. G.M.T., corresponding to an oscillation of 1 mm. of the quicksilver. ‘A fast moving barograph (mercury) shows a spot at 11h. 23m., indi- cating a swing of the mercury of 0:25mm. This increased to 0°50 mm. and died out suddenly. ‘The magnetographs, declinometer, bifilar and Lloyd’s balance were all disturbed, although it was a day of perfect magnetic calm.’ On this day, at 11h. 5m. G.M.T., a violent earthquake took place in Assam. The large waves of this would reach Zikaweiat 11h. 21m. G.M.T., or 7h. 26m. 43s. p.m. local time. In a second letter Father Moidrey writes : ‘On June 4, 1898, about midnight, our north clock lost about four seconds. That same night at a watchmaker’s in Shanghai several clocks (six, I believe), all facing north or south, were stopped. Nothing else was noticed by the watchmaker, M. Vrard, who in his surprise telephoned to the observatory to ask what was the matter. Nobody in the town felt an earthquake, nor was one referred to in the newspapers. A missionary at Nankin had his clock stopped the same night, but did not notice any other phenomena. Our magnetograph and thermograph recorded a shock at 16h. 24m. 17s., June 3, G.M.T. On that day there was an earthquake at Chemulpo, Corea.’ We are here evidently dealing with an earthquake recorded on June 3 at 17h. 14m. at Shide, and also recorded at Kew, Nicolaiew, and Potsdam. From the ‘ Bulletin Mensuel’ of Zikawei, third quarter, 1897, we learn that in the night of September 2 the two clocks were stopped and the magnetographs were disturbed at 1.42 (September 1, 17h. 36m. G.M.T.). Nothing was felt. This may refer to an earthquake recorded at Shide, September 1, 18h. 29m. G.M.T. Although Professor E. C. Pickering writes me that on September 3, 10 and 23, 1898, which are dates for heavy earthquakes in Alaska, and on September 20, when there was a severe earthquake in Asia Minor, there were no noticeable changes in the rates of the clocks at Harvard 106 REPORT—1900. University ; the observations made at Zikawei indicate that at certain observatories at least the unfelt movements of earthquakes may from time to time have serious effects on timekeepers. With the object of throwing light upon this subject I shall esteem it a favour if directors of observatories will let me know whether any changes were observed or not observed in the rates of pendulum time- keepers on dates corresponding to those of large earthquakes enumerated on p. 108, addressing their communications to me at Shide, Isle of Wight, England. IV. Earthquakes and Rain. In the British Association Reports for 1899, p. 209, I gave a quota- tion from Mr. O. H. Howarth respecting a heavy condensation of aqueous vapour which he observed for three hours after the Mexican earthquake of January 24, 1899. This was in the form of a heavy mist which settled over the head of a cafion at an elevation of 8,700 feet. Mr. Howarth states that in this place such mists are never seen at this time of the year, it being the middle of the dry season. Something similar to this occurred on June 12, 1897, after the severe earthquake which originated on that day in the highlands of Assam. Mr. H. Luttman-Johnson, I.C.S., in the ‘Journal’ of the Society of Arts, April 15, 1898, describes the weather before the earthquake as having cleared : the afternoon was lovely, and there was not a cloud in the sky. Five minutes after the earthquake the residents in Shillong were sur- rounded with cloud and mist, and they sat up all night with rain beating upon all sides. Captain A. A. Howell, I.C.8., deputy-governor of the Garo Hills, gives the actual rainfall. The records taken at 8 a.m. showed that for the twenty-four hours preceding the 12th there was no rain. There was rain at noon on the 12th, but it cleared off at 2 p.m. The earthquake occurred at about 5 p.m., and after that until next morning 3°26 inches fell. In considering whether there is any possibility of a connection between the phenomena here considered we must remember that observa- tions showing that rain and cloud have followed closely on the heels of certain earthquakes appear to be confined to tropical and semi-tropical countries ; and it is in these countries where sudden showers, indicating the collapse of critical atmospheric conditions, are frequent. . Given, therefore, such conditions at no great distance above the surface of the earth, which was probably the condition in the highlands of Assam, and then admit that beneath the gaseous covering consisting of layers of air of different temperatures and with different degrees of saturation 10,000 square miles of mountainous country was moved, or that a much larger area was thrown into violent wave-like movement, we recognise that the relationship of earthquakes and atmospheric precipitation may not be so improbable as is generally supposed. As the ground rose upwards, the air immediately above it would suffer compression, and as the ground fell there would be rarefaction, whilst layers of air differing in their physical state might be mixed, and a vigorous seismic activity might in this way result in pre- cipitation. ON SEISMOLOGICAL INVESTIGATION. 107 V. Earthquakes and Small Changes in Latitude. . In vol. xvii. of the ‘Seismological Journal of Japan,’ 1893, p. 17, I drew attention to the observation that the period of maxima increase in latitude in Berlin apparently coincided with maxima of earthquakes recorded in Japan. If we compare the wanderings of the pole from its mean position for the years 1895-1898! with registers of earthquakes which have disturbed continental areas or the whole world, we find a somewhat similar relation- ship. This is shown in the accompanying table, the pole displacements. being measured from Albrecht’s figure. 1895 1896 1897 1898 ; | 22 [4a] Se jeg] de |44) 23 |e ea |eel ea |g5| 2 |ae| 2/2: sal a Si = an oy pe Paes: (rahe 1. January 1 to February 5 0-03 | 1 0-071 1 | o14] 5 ll o12| 4 2. February 5 to March 14 0:03 | 2 || 0:04 |} 1 || O11 | 7 |} O11} O 3. March 14 to April 19 . 0:06 | O || 0:05 | 1 || 0-07 | 1 || O07 | 4 4, April 19 to May 26 007} 1 || 0:08 | 2 || O11 | 5 || O08 | 5 5. May 26 to July 1 0:08 } 1 || 0:10 | 2 |} O13) 5 || 010] 6 6. July 1 to August 7 .}| 0°03 | 1 || O11 |] O |] O11 | 6 | O16) 5 7. August 7 to September 12 . | 0:05 O || 0:10} 4 || 010] 5 || 0:15] 6 8. September 12 to October 19 | 0°06 | 1 || 0:13] 3 || 0:07} 5 9. October 19 to November 24 | 0:06} 1 || 0:10 | 4 || O11} 4 1 10. November 24 to December 31 | 0:08 | 1 || 0:13] O || 0:12 {or 4 44 Totals. ‘ «(0:53 } 9) | O:9L- | 18 || oF it 0:79 | 30 47 A conclusion suggested by this table is that, during intervals when the pole displacement has been comparatively great, large earthquakes have been fairly frequent, and vice versd. In the yearly totals this is marked. If we turn to a figure given by F. R. Helmert, showing variations in latitude as determined from 353 sets of photographic records made on forty-two days in the months of April, May, and June, 1897 (see ‘Bericht | uber eine neue Reihe von Polhéhen-Bestimmungen, &c., im Jahre 1897,’ F. R. Helmert, Potsdam), we see that successive daily means frequently differ from 0'’:1 to 0/2 amongst themselves. Equally large differences. exist between the separate observations from which these means are deduced. That is to say, successive observations may show differences as great as the annual maximum displacement of the pole, which is about 0/25 from a mean position. If on Helmert’s figure we plot the large earthquakes for these months, it is seen that in the time of their occurrence they closely coincide with 1 See Bericht wiber den Stand der Erforschung der Breiten- Variation am Schlusse des Jahres 1898, von Th. Albrecht. 108 REPORT—1900. the times at which large deviations in latitude occur. In April, when these deviations were comparatively small, large earthquakes did not occur. When considering the possibility of any relationship between earth- quakes and these extremely frequent and practically oscillatory changes in latitude, there are two points of importance to be remembered. The first is that with each of these earthquakes there is a sudden shifting of a large mass of material at a seismic origin. The molar dis- placement for the Indian earthquake of June 12, 1897, is estimated by Mr. R. D. Oldham by an area of 6,000 or 7,000 square miles, and it is not improbable that earthquakes which have caused the Pacific Ocean to oscillate for a period of twenty-four hours were accompanied by displace- ments of larger magnitude. The second consideration is that each of the large earthquakes here considered has been accompanied by surface or distortional waves which in many instances affect the whole surface of the globe. These waves, so far as we can infer from their velocity, period, and maximum angle of inclination, vary between twenty and seventy miles in length, and are from a few inche& to two or three feet in height. If they attain the magnitudes here given (see p. 83) they seem certainly sufficient to relieve a district in orogenic strain. A further test of the suggestion that slight nutational effects may result from earthquakes would be to compare observations indicating small changes in latitude made before and after the times of large earth- perce referred to in the report, the more important of which are as ollows : H. M. No. 250. Origin Mexico, January 24, 1899, 23 44 jy 808 » Alaska, September 4 ,, 0 11 ” 337 % 9 ” 10 ” 16 51 5 338 93 9 » 10 5 20 21 9» 048 » Smyrna, os 20. 29 3 OAT » Ceram, ms 2.9) eee ol ed » ool » Mexico, January 20 1900,18 31 The times given are the approximate times at the origin. These are expressed in Greenwich mean time (civil), 0 or 24 hrs.=midnight. The times at which the large waves reached any distant station may be calcu- lated by the application of Curve IIa or Id in the table on p. 67. VI. Selection of a Fault and Locality suitable for Observations on Earth-Movements. By Cimment Rep. The selection of a favourable site for observations upon differential movement between the two sides of a fauit presents many difficulties, and the locality we have chosen is more to be regarded as the best available than as ideally perfect. Leaving out of account for the present considera- tions other than geological, there are certain conditions, most of which must be complied with if the observations are to be of real value. The fault selected must be : 1. Of considerable magnitude, and not be merely a branch fault which the next earth-movement may easily leave unaffected. 2. It should be of known date, and belong to a recent geological period. This consideration is important, for a Tertiary movement is far ON SEISMOLOGICAL INVESTIGATION. 109 more likely to be still in progress than is one which can only be shown ' to affect Paleozoic or Secondary rocks. Not only have the older movements in many cases ceased long since, and have given place to move- ments in different directions ; but a fault which has long remained without movement tends to become closed and re-cemented, so that there is a considerable likelihood that any future movement may not follow exactly the same line, even though the strain be in the same direction. 3. The fault should crop out on ground fairly level, and in hard rocks, otherwise the observations may be masked by the slight irregular ‘ creep ” of the surface downhill, and no firm foundation for the apparatus be obtained. 4. It is desirable that the rocks on the two sides of the fault, though geologically far apart, should be as like as possible in lithological charac- ter, so that any surface movements due to change of temperature or absorption of rain-water should affect the two sides alike. 5. In order to avoid complications through slow solution of the rocks by percolating rain, a fault bringing together insoluble silicious rocks would be preferable to any other. 6. As the records to be obtained may throw great light on movements. of the earth’s crust, it is desirable that the fault selected for observation should be one belonging to a set of disturbances of great magnitude, having common characteristics, and affecting a considerable area. It is. therefore important that the district chosen should be one which has been carefully studied geologically, and of which the structure is thoroughly known. These various conditions, added to the consideration of convenience of access of the locality, availability of a skilled observer, availability of the land, and other minor points, made a series of requirements not easy to satisfy, and I will now indicate in what respects the site finally selected comes up to or falls short of the ideal set before us. Consideration No. 2 confines us at once to the only area in Britain in which large earth-movements of Tertiary date can clearly be proved to have taken place. This area may be taken to lie between the North Downs and the English Channel, and to extend as far west as Weymouth and Abbotsbury. But only the parts of it in which Tertiary rocks are still preserved will do for our purpose ; the reason being that older move- ments of the same general character affected the Jurassic and Lower Cretaceous rocks. These intra-Cretaceous disturbances cannot always be distinguished from the Tertiary movements, in the absence of the uncon- formable Upper Cretaceous and Tertiary strata. Thus in the Wealden area a good many faults are believed to affect the Lower Cretaceous rocks ; but they are of no great magnitude, and it is impossible at present to differentiate those of Tertiary date from the older series. We are thus confined, by a process of elimination, to the sharply folded belt which occupies the southern part of the Hampshire Basin and includes the northern half of the Isle of Wight. Even over this area it would only be possible to use Mr. Horace Darwin’s apparatus at certain points ; for much of the country is sharply folded without faulting, and any earth-movements now in progress could only be measured by careful levelling and triangulation. Thus we are confined ultimately to a limited highly disturbed and faulted belt, which extends east and west through the centre of the Isle of Wight and reappears in Dorset between Studland Bay and Abbotsbury. 110 , REPORT—1900. Within the area thus selected are various sharp monoclinal folds, all with an east and west axis, and with the strata so bent as to become nearly vertical. In places the lateral pressure and folding have been so violent as to pass into overthrust faulting on a considerable scale. None of the Tertiary disturbances in this part of England is a normal drop- fault ; the supposed north and south Tertiary fault in the Medina valley, though often shown in old maps and text books, having no existence. The date of most violent disturbance in the system of folds above alluded to is clearly later than Middle Oligocene ; for in the Isle of Wight the Hamstead Beds, which belong to that period, and are the newest Tertiary strata there preserved, are tilted at a high angle. From various considerations, which need not here be recapitulated, it seems probable that this set of disturbances commenced in Eocene times, became most violent in the Miocene period, and died away in Pliocene times.! ‘Though in our south-eastern counties older Pliocene strata to some extent have been tilted, the disturbance has not yet been shown to affect newer -deposits, or to be still in progress. This last is one of the principal points which our apparatus should decide. Consideration No. 1 limits our choice to a small group of faults, not more than half-a-dozen, and as the apparatus employed needs a fairly clean-cut fracture, unless the pipes are to be of unreasonable length, it is only at a few points on these faults that the observations can be made. We have thus so greatly reduced the number of possible points at which the apparatus could be fixed, that it will now be simplest to describe the faults one by one, and point out to what extent they do or do not fulfil the rest of the requirements. Working from east to west, the first Tertiary fault met with is in the ‘main monocline of the Isle of Wight, which occasionally passes into a thrust-fault of no great extent. In one place the basement bed of the London Clay is brought against Bracklesham Beds ; but the strata are too soft and full of water to yield satisfactory fixed points. In the others, plastic Clays of the Reading Series have slid over Chalk, the bedding being vertical and the surface slope very high. At no point in the Isle of Wight could a satisfactory site be found. Following this disturbed belt westward, we again meet with a sharp monoclinal fold, passing into a slide-fault, at Ballard Cliff in Dorset. This is the well-known ‘Isle of Purbeck Fault,’ which thrusts Chalk with flints with curved bedding over similar rock with the bedding vertical. The fault itself is very conspicuous in the cliff-face, curving through about a tenth of a circle in a height of 280 feet.2 This fault might be a good one for observation; but though it is of considerable magnitude, the locality is by no means convenient of access. The disturbance is, however, a valuable one to study, for its character is clearly shown in the section. The other faults with which we are now dealing apparently are all of this type. F The next Tertiary fault met with is close to Corfe Castle, where in the sharpest part of the monoclinal curve the London Clay has been thrust over the Reading Beds and abuts against the Upper Chalk. This slide- fault is of smal] magnitude, and as in similar slides in the Isle of Wight, 1 Reid and Strahan, ‘Geology of the Isle of Wight,’ chapter xiv. Memoirs of the Geological Survey, 1889; Reid, ‘Pliocene Deposits of Britain,’ chapter v. ibid. 1890. 2 See Strahan, ‘Geology of the Isle of Purbeck,’ chapter xv. Mem. Geol. Survey, 1898. ON SEISMOLOGICAL INVESTIGATION, 111 the ground is too steep and the rocks too soft to yield satisfactory fixed points. Along the same line the junction of the Chalk and Eocene is again slightly faulted near Lulworth ; but the fault is of small magnitude, and the adjoining rocks are too much shattered for our purpose. The Durdle fault runs parallel with and close to high cliffs, so that delicate observations might be entirely masked by movements caused by the gradual removal of large masses of rock by the sea on the south and the consequent rise of the strata qn that side. At Bat’s Head the Isle of Purbeck Fault is finally lost beneath the sea, and the shattering of the rocks is too great to allow of exact observations. This fault does not reappear in the Weymouth area. There still remains one of the most important Tertiary disturbances in the district, that known as the Ridgeway fault. This also is an over- thrust fault cutting through a monocline, or through the north limb of a sharp anticlinal fold. Its date is clearly later than the Bagshot period ; its magnitude is great, and if any of the Tertiary faults are still under- going changes, this one is likely to partake in the movement. It brings together rocks of very different ages and of varying character, so that the choice of exact locality for the observations depended on the discovery of a spot where the fault is a clean fracture, where the rocks on each side are hard and of fairly similar lithological character, and where the ground is sufficiently level for the apparatus. Along a good deal of its course there is much fault rock or broken ground, and in most parts the strata on one or both sides are soft. These parts would not be convenient or satisfactory for our purpose. For various reasons the choice narrowed down to the neighbourhood of Poxwell, where Middle or Lower Chalk abuts against Lower Purbeck ; or to the district between Upway and Portisham, a distance of four miles, where Upper Chalk is faulted against strata close to the base of the Lower Purbeck, or even against Portland Beds. Of these localities Upway was chosen (fig. 2), for there the deep railway-cutting has laid open the structure of the disturbance, and within a reasonable distance, though not too near, was a piece of fairly level ground, one end of which had been opened for chalk-pits and the other for quarries in the Purbeck Beds. The railway-cutting itself would not have been satisfactory, for in it a wide dyke of ‘fault-rock,’ composed of Oxford Clay and Cornbrash, occurs, and south of the fault there are soft rocks. Besides this, soft strata in a deep cutting will almost certainly be subject to slow ‘creep’ to such an extent as entirely to mask any deeper-seated movement. The site finally selected proved by an unexpected series of coincidences to be particularly convenient. It is broken ground, now only used ‘for rough pasture and not liable to be disturbed by the plough ; it belongs to Gonville and Caius College, Cambridge, who have most kindly done all in their power to help us in the experiment. Our thanks are not only due to the College, but also to the tenant for his assistance in carrying out the work. And last, but not least, it was conveniently accessible to the member of the Committee who was prepared to undertake the recording. While our excavations were being made I examined them, and noted as exactly as possible the geological conditions in the immediate neigh- bourhood, for the fault varies within very short distances, and has changed completely in the two hundred yards between the railway cutting and our selected site. In that short distance the dyke of Oxford REPORT—1900. 112 “spueg *purestioa1 ‘yooqing ‘Hoeqing ‘yoeqang “8098 “pueg “£810 £810 joysseg “yeu weddQ “mepTvVa aoddq aIPPIN. TOMO'T puyyazog = pueyylog: «= aS puewTy pr0jxO ‘qneg AvMospry pus oul] mooag Jo uorount qe snqered -dv Sutptooer Jo morgisod soyousd 3% 09 00 0 ees, ss sy —_ yn TS LL AO ane rH a aif "(8 A f | } Hah PAGHshm | WE ; y Gu Sars Ger oS G WN o> eek. i coon 5. es Soon cv DUS - saavccoC cao op™“e: f eve L ate et ecaceas boo ceS See Ceo SDS SAS S55 CSO Na 4 a a ES ae Se Pes ra 2 Oe eoent colt ee ee oe 5 S ————S ieee eecvecotemecescocco CD SoopP> ee ot oeSs By Sach : pr ater PIP nhs, a : . 7 Bee = = moos SesSoHs scot po Se SES pale Se [i -s hy fae ee Side co go Rae 2 ohseerooSmams qa t= L. : ‘ i ses PS SSO SOS ac" go KG gi2a Pie cosmo eSQeige [penocrowec face coo ar eae 5 Rar) [ Zele 4 eas SE eee ee oe cae ee . cold Seo a a Z st es et a aa : c \Paocaoscomoo deep Se Se OS eS PAC O KR AenseseS i Vie = 5 by aagJ Capi | =soyout g ‘ayBog) ‘CIMY LNANATO Aq SUOTIPpe WIA !NVHVULY ‘y 4q ‘KemdyQ Jo dey Aang [wordojoeaH—’s “O14 ON SEISMOLOGICAL INVESTIGATION. 1138 Clay has disappeared entirely, as is the case with the Middle Chalk on the north side of the fracture, as well as the Wealden and Upper and Middle Purbeck on the south side. The fault has also become a fracture of unusual sharpness for one of so great a magnitude. In discussing the character and extent of thrust of the fault at Ridgeway, it should not be forgotten that it does not pass through a series of conformable strata. The Upper Cretaceous rocks here rest unconformably on a folded and greatly eroded surface of Lower Cretaceous and Jurassic strata, so that the local absence of Wealden and of most of the Purbeck may be due to this unconformity. These intra-Cretaceous folds have an axis approximately parallel with the much later Tertiary disturbances. The most important of them is the wide anticline between Upway and Portland. This is followed northward by a narrow and sharp syncline, which brings in the Wealden and Purbeck between Upton and Bincombe, and passes unconformably under Upper Cretaceous rocks towards the east and towards the north-north-west. Next follows an anticline, which is almost entirely hidden by the newer rocks. It is touched at Poxwell, where the Jurassic strata dip northward at a higher angle than the Upper Cretaceous. It then seems to run beneath the Chalk parallel to the southern boundary just north of the Tertiary over- thrust. Its southern limb reappears at Bincombe, but soon disappears again beneath the overthrust mass of Chalk. The position and character of these earlier folds, their relation to the Upper Cretaceous overlap, and the relation of both to the overlap of the Bagshot Beds on to the Oolite,! are the factors which produced a continuous plane of weakness extending obliquely downward from the surface deep into the Jurassic strata, as shown in the diagram (fig. 3). The outcome of this geological structure has been that any subsequent lateral compression in a north and south direction causes the massive Chalk, over 800 feet thick, to be driven against the wide arch of rigid Purbeck and Portland rocks extending towards Portland. Any such movement must tend still more to fold and buckle the already existing small anticlines and synclines ; but the main arch of hard Upper Jurassic rocks would offer great resistance, as would the horizontal thick-bedded Chalk. Thus the Chalk must approach the main anticline, overriding the minor folds, taking with it such parts of them as happened to be above the plane of greatest weakness, and smearing the slide-plane with Oxford Clay and Cornbrash caught up in the passage over the northern limb of the anticline. : The above explanation will, I believe, account for the whole of the curious phenomena recorded along this line of fault. Granted north and south compression, any differential movement must be along this plane of weakness. The extent of the differential movement must also be greatest at the surface where the plane emerges, and must rapidly decrease down- ward and northward until the fault entirely disappears. The extent of the movement in this case is probably about half a mile. From the data in the memoirs and maps of the Geological Survey, and from my notes made more recently, I have constructed the subjoined geological section across the fault at the point where our apparatus is fixed (fig. 4) ; but though the underground structure must be not unlike that indicated, the exact curve of the fault, and also the exact character hen Reid, ‘ Geology of Dorchester,’ chapter vi., Memoirs Geol. Survey, 1899. ’ I REPORT--1900. 114 “Sur “YMC S1OTUT F *ABIO PIOJXO 2 “pues puvyyiod OL “UdplwaM §T tae) deddn 91 “pug Sagege b *aIGALJT YSOLOT ¢ ‘uRTTe10p g ‘9U0Ig PULTO TL *pursueaty raddq FT qoussed JL. *oqT[00 LOLaJUT g “YSBAqUIO) 9 “ABIO OSpPLOMITY 6 ‘sped Yooqind oT “YTVYO TOMOT pur appr et *9u900850 8T a —_ Copia [= your |] ‘eyeog) “qynvg AemoSpry ayy jo UOHVULIOF 94} BLOJoq oinyonTys erqeqord Sutmoys ‘uoToIg WIeIsVIG ‘Ss pue “N—'s ‘PIT “SBI ‘e110 AOpLoJUT ———————————— g ————— = ——-~ . LZ 116 REPORT—1900. of the hidden folds beneath the Chalk, must remain uncertain. The Eocene deposits are not shown in this section, as they happen to have been denuded along the line selected. They occur only a short distance away out of the line of section. . The actual evidence seen at the surface close to our site will now be described. On the south side of the fault the strata dip northward at varying angles for a distance of about two miles from the crest of the main anti- cline, the lowest rocks in the district occurring in this anticline north of Radipole, where the Forest Marble appears at the surface. To this succeed in order the Cornbrash, Oxford Clay, Corallian Rocks, and Kimeridge Clay, followed at Upway (at the south border of the map, fig. 2), where the slope becomes steeper, by Portland Sand, Portland Stone, and Lower Purbeck Beds. The lower quarries at Upway are in Portland Fie. 5.—Section of Lower Purbeck Rocks, dipping at 52°. \j i DV Shyi5 Rock, dipping north ; the higher are in Lower Purbeck, nearly horizontal, for at that point the lowest part of a synclinal fold is reached and the strata begin to rise again. Higher up the hill in quarry and road-cutting the sections are nearly continuous, the dip being about 8.S.W. at angles varying from 15° to 30°. Signs of lateral compression are also common, this being particularly well seen on the west side of the quarry nearest to the fault, where in a few yards the dip changes from nearly horizontal, with small sharp folds, to an angle of 15°. At the extreme north edge of this quarry the Committee undertook special excavations in order to clear up the geology at a point close to the fault. We followed a particular rock bed to a depth of 9 feet from the surface, obtaining the subjoined section, seen from the east (fig. 5). The strata laid bare belong to the ‘dirt-bed’ of the ON SEISMOLOGICAL INVESTIGATION. 117 Lower Purbeck, and occur within a few feet of the Portland Rock. The strike is almost parallel to the fault, though more nearly east and west. Thus it becomes almost certain that Portland Beds crop out at the surface immediately east of the Roman road and are probably within less than 10 feet of the surface at the point where the recording apparatus crosses the fault. Taking now the trench in which the apparatus is placed, we will describe the strata there seen on each side of the fault. The trench is 9 metres long, and at the four observing stations (see Mr. Horace Darwin’s Report, p. 119) sections were exposed to a depth varying from 5} to7 feet. At Station SS (the southernmost) the depth was 54 feet, of which the top 3 feet was in disturbed ground, the lower 2} showing hard brownish fine- grained oolite with fossils, the rock being somewhat shattered, with small open fissures, which were afterwards filled in with concrete. This rock undoubtedly belongs to the Lower Purbeck ; it seems to dip at a high angle in a southerly direction, the strike, however, not being parallel with the fault. The shallower trench between Stations SS and S showed similar strata, though no fossils or oolitic grains were observed. At Station § the hole was also 54 feet deep ; the rock being a hard splintery brown limestone, more or less nodular and containing small chert nodules. I believe that this rock corresponds with some cherty limestones which are seen in the large Upway Quarry, just below the ‘dirt-bed’ and within 5 or 10 feet of the base of the Purbecks. Near the fault, however, they are harder and more crystalline than in the quarry. I was not able to find the earthy and carbonaceous ‘dirt-bed’ at this point, though it is so well seen only 50 or 60 feet away (see fig. 5). The squeezing-out or thickening of a soft stratum is, however, a phenomenon constantly to be met with near a big disturbance, and the absence of the carbonaceous seam is probably due to this cause. The south cheek of the fault consists of brecciated white limestone with chert. These exposures seem to indicate that the Portland Stone must occur within 5 feet or so of the surface close to the fault, and on the strength of the new evidence I have added an inlier of Portland rock to the map made by Mr. Strahan, who agrees with me that such an addition is necessary. The fault itself is represented by a band of fault-rock not more than 2 feet in thickness and quite unlike the wide dyke of mingled Oolite and Oxford Clay seen in the railway-cutting. In our trench the fault-rock is a hard mass of breccia consisting of Upper Chalk and fragments of Purbeck Limestone. The north cheek of the fault consists of very hard shattered and re-crystallised flinty chalk like that associated with the similar disturb-. ances at Corfe Castle and at Ballard Cliff, though at Ridgeway I did not observe actual calcite veins. Two feet north of the fault I dug out a specimen of Ananchytes ovatus ; but this echinoderm and a few fragments of Inoceramus were the only fossils I could find in the Chalk in our trench. The flinty character cf the Chalk and the presence of the Ananchytes show, however, that we have passed suddenly from Lower Purbeck to Upper Chalk, and the character of the Chalk and of the included flints indicates, I think, that we are at an horizon above the Micraster-zones and probably at least 300 feet above the base of the Chalk. Between the fault and Station N the Chalk gradually becomes softer and less crystalline and contains small broken flints, black with moderate rinds, The hole at Station NN showed 6 feet of moderately hard Chalk, 118 REPORT—1900, with numerous brownish-grey flints ; the Chalk being fissured but not altered. At Station NN the hole was 7 feet deep and exhibited Chalk with numerous flints, the rock being much slickensided and fissured. It contained a few fragments of Jnoceramus. I was not able anywhere to get a satisfactory dip in the Chalk in the trench or holes ; though the general impression suggested was of an ascending succession northward, and of a high dip in that direction. The general results of the geological examination may thus be sum- marised. The fault, at the point where the apparatus crosses it, probably cuts out strata having a thickness of nearly 1,000 feet, made up thus :— Chalk (part of Upper, whole of Middle and Lower) . : . 300 Greensand and Gault. 3 : : F : 5 . 150 Wealden : : 3 é : ; ; . . 5 . 330 Upper Purbeck i : ; : ; : 5 : 5 Se eg 3 Middle Purbeck . : : ; : : 5 4 5 niin) Lower Purbeck (to within 5 feet of base) . ; t : - 85 Total feet 985 The break, however, is not caused by a normal fault of 985 feet throw. Tt is the result of a sliding movement over a cylindrical surface curving downward and northward from nearly vertical to nearly horizontal. This view, as pointed out by Mr. Strahan, explains the presence of a dyke of Oxford Clay and Cornbrash in the railway-cutting ; a fact which cannot be satisfactorily accounted for by normal faulting, even to the extent of 2,500 or 3,000 feet. The movement along the curve of the thrust-plane amounts to not less than 2,500 feet, even if the strata are everywhere vertical to the fault. It is just possible, however, that earlier faulting along nearly the same line in intra-Cretaceous times brought up Cornbrash, so that it occurs immediately beneath the Upper Cretaceous rocks just north of the Tertiary fault. On this supposition, and with the most favourable angle of dip throughout, the Tertiary thrust may not exceed 500 feet. The most probable estimate of the extent of the Tertiary displacement is, however, about half a mile ; a lower estimate demands an improbable series of fortuitous coincidences, such as we are not justified in postulating. There is one point that I should like to suggest for future considera- tion. The disturbances just described result from lateral compression of the strata in a north and south direction, and it is clear that levelling across the fractures will only give us one element in that motion. The horizontal movement must be of much greater magnitude than the vertical, and could be accurately tested by triangulation. As the folds have always an east and west axis, and there is no sign of disturbance in other directions, triangulation across the folds from fixed points lying east and west ought to enable us to test whether any change is now going on over wider areas. Even a comparison of the earlier Ordnance triangulation of the South of England with the later one might throw light on this question, if the stations can be identified with sufficient accuracy. No minute re-measurement of a base-line would be necessary for this test. If the movement is going on at all it must be far greater in a north and south than in an east and west direction—i.c., it will alter the latitude but not the longitude. It must therefore distort every triangle which can be re-observed from two such points as St. Catherine’s Down and the top of Portiand. ON SEISMOLOGICAL INVESTIGATION. 119 VII. An attempt to detect and measure any relative movement of the strata that may be now taking place at the Ridgeway Fault near Upway, Dorsetshire.—Preliminary Report by Horacr Darwin, August 1900. The Fault for this experiment was selected by Mr. Clement Reid, and is described by him in a separate report. It would have been better if the rock had been harder and more impervious to water ; the solubility of the carbonate of lime in the rock is also a disadvantage. The site is easy of access, an essential point in such an experiment ; this, together with the advantages pointed out by Mr. C. Reid, justify the selection of the Fault. The Fault where the apparatus is fixed is a few yards east of the Roman road and about 560 yards north of the cross roads in the village of Upway, Dorsetshire, and is about 360 feet above Ordnance datum, Gonville and Caius College, Cambridge, allowed the apparatus to be fixed on their property and did all in their power to make the experiment successful, and the Committee are most grateful to them. I must thank Mr. Nelson Richardson for the many hours’ help he gave me at Upway, and in arranging for the experiment, and for the readings he took after- wards. Thanks are also due to Mr. Loveless, the tenant of the land, for the care he has taken in carrying out the work and the help he gave in every way. Four positions were taken in a straight line approximately at right angles to the fault ; these positions will be denoted by the letters N.N., N., 8., SS. ; N.N. is 9 metres and N. 44 metres north of the Fault, and S.S. is 9 metres and 8. 44 metres south of it. The apparatus is arranged to measure the relative vertical movement of the strata at these four stations. There are advantages in selecting four instead of two stations. Jf there had been only two stations, and the apparatus got damaged at one of them, the experiment must have been a failure ; also, if there had been any accidental displacement of the apparatus relatively to the strata at either of the two stations it might have led to misleading results. With four stations such damage or movement will probably be detected, and the results, though less valuable, will not be rendered quite useless, as would be the case with only two stations. The movement of the strata at the Fault may take place in any or all of the following ways :— (1) The strata on both sides of the Fault may tilt as a whole without any slip taking place at the Fault. (2) The strata at the north side may tilt and the south side not tilt, and still no slip at the Fault. (3) The strata at the south side may tilt and the north side not tilt, and still no slip at the Fault. (4) There may be slipping at the Fault with no tilting. These four movements may be all taking place at the same time, and the use of four stations will allow of each movement being separated from the others. __ The apparatus has been designed by me and made by the Cambridge Scientific Instrument Company, Limited. I have not been able to give sufficient time this summer to overcome some difficulties which I regret that I did not foresee, and it is for this reason that no numerical results 120 REPORT—1900. are given in this report. The instrument, however, promises well, and I hope next year to give a description of it and numerical results ; now I only propose to explain its general principle. A brass casting is permanently fixed to the rock at each of the four stations, and it is the relative vertical movement of these castings which is measured. A stand carrying a microscope can be placed on any of these castings ; it has three feet, each in the form of an inverted V, and these rest on three cylindrical pieces forming part of the brass casting, This is the usual geometrical arrangement, giving six points of contact, and determining absolutely the relative position of the microscope stand and the casting. The microscope is about 4 feet long, and thus the eye is in a convenient position for taking an observation. The microscope is moved vertically in the stand by a micrometer screw, and carries at its lower end a needle pointing vertically downward. The micrometer screw is turned, the microscope is lowered till the needle point touches the surface of some oil contained in a vessel fixed to the rock, and the position of the micrometer screw noted. The microscope and stand are then removed and placed on the other castings, and the observation repeated ; in this way the relative position of the casting at each station to the oil surface is measured. The four oil vessels are connected by a pipe ; the surface of the oil is therefore at the same level. The needle point is illuminated by a mirror fixed in the oil vessel, and the light, leaving it in a nearly horizontal direction, is reflected by a vertical mirror nearly directly backwards, and is then again reflected vertically upwards through the object-glass and eyepiece of the microscope. On looking vertically downwards through the microscope, the needle point and its reflection in the surface of the oil are seen as if the eye were placed just above the surface of the oil ; and when the micrometer screw is turned the needle point and its image are seen to approach each other. The moment of contact is perfectly evident ; the needle and its image appear to run into each other in a confused manner, owing to the dis- tortion of the oil surface when the needle point touches it. The delicacy is considerable ; the divisions in the divided head of the micrometer screw correspond to a movement of +4, mm., and it is easy to estimate a tenth of these divisions, but I do not think that the readings can be trusted to this amount, and it is proposed only to read to ;1 mm., which is well within the power of the instrument. The micrometer readings give the height of each station above the oil surface, and from these readings is deduced the movement at each station relatively to a datum plane. This datum plane is taken at the mean level of the four stations. The necessary calculations also prevent any error arising from change of the oil level due to expansion or evaporation, damage to the needle point, or expansion of the microscope. It is hoped that a very small slip at the Fault will be detected and measured, but even if the movement should ever become as much as 10 mm. to 20 mm., it can still be measured with great accuracy. It is unlikely that such a movement will damage the lead pipe where it crosses the Fault ; damage to the pipe, however, can be easily remedied without impairing the accuracy of the readings. Some readings have been taken, but it is feared that they are not perfectly trustworthy ; they may, however, be useful in confirming later results. ON THE PRESENT STATE OF THE THEORY OF POINT-GROUPS. 121 Report on the Present State of the Theory of Point-groups.—Parr I. By Frances HarpcastTLe, Cambridge. CoNTENTS. PAGI § 1. Introduction. 5 ; f ‘ ; i 5 ‘ : F ; fo IPA § 2. Historical Outline. 7 4 J 5 . i ey W210 § 3. Analysis of the Subject according to Content. 5 - 123 § 4. Brill’s Memoirs on Elimination and Algebraic Correspondences, 1863— 1873 123 § 1. Inrropuction. THE term point-group is a direct translation of the German word Punkt- gruppe, first used by Brill and Noether in the year 1873 in their classic memoir on algebraic functions,! but to my knowledge, although more than a quarter of a century has elapsed since then, there has been no very systematic attempt to present the theory of point-groups to English readers along any of its lines of development. And yet it should prove of interest even to those mathematicians who do not desire to specialise in it, for, historically and logically, it touches upon many distinct branches of pure mathematics. To mention only those which are most directly brought into connection with each other, we have the intersections of plane curves, the elimination of variables from systems of equations, the algebraic theory of correspondences on a plane curve, properties of linear systems of plane curves, and applications of the theory of functions to the theory of curves and surfaces in space of any number of dimen- sions. As frequently happens when the progress of a subject has been due to many different writers, the logical and the chronological divisions do not coincide. I have therefore in view a dual arrangement of the subject-matter. In the present instalment of my Report, I have attempted to sketch this proposed arrangement under its two aspects, viz.: as an historical outline (§ 2), and as an analysis according to content (§ 3). This is followed ($ 4) by a detailed account of one of the historical divisions I hope in the subsequent portions of the Report to deal in a somewhat similar way with the remaining divisions, and to append a complete bibliography. § 2. HisroricaAL OUTLINE. A. 1720-1818. Memoirs on the intersections of plane curves from Maclaurin to Lamé. [Lamé was the first to express the linearity of the system of curves through the intersections of two given curves.” | B. 1818-1857. Memoirs and other published accounts of theorems on the intersections of curves from Lamé to Riemann, including those of Pliicker and Cayley. [Pliichker was the first to introduce explicitly projective methods by 1 * Ueber die algebraischen Functionen und ihre Anwendung in der Geometrie,’ Math. Ann., vol. vii., pp. 269-310. 2 Of. 0. A. Scott, Bull, Am. Math. Soc., vol. iv., p. 262, 1898. 122 REPORT—1900. means of homogeneous co-ordinates; ! and also to fix one curve in the discussion, treating the other curves as variable.2 Cayley’s theorems are interesting on account of the subsequent discussion as to their true Jormulation. | C. 1857-1873. (i.) Memoirs on bi-rational transformation. (ii.) Brill’s memoirs on elimination and algebraic correspondences, (1863-1873). [A detailed account of these is given in § 4, infra. | (iii.) Memoirs and other publications connecting the theory of functions with the theory of plane algebraic curves, including those of Clebsch and Gordan, Brill and Noether. [Clebsch and Gordan’s treatise attempted to found Riemann’s results in the theory of Abelian functions on an algebraic basis: the standpoint is mainly that of projective geometry. To Brill and Noether is due the initiation of the main line of enquiry in the theory of linear series of point- groups on a base-curve, from the standpoint of bi-rational transformation. | (iv.) Memoirs on the intersections of curves. D. 1873-1890. (i.) Noether’s memoirs published in the Mathematische Annalen, and in Crelle, on the theory of functions, and on analytical geometry. (ii.) Memoirs on linear systems of plane curves, treated analytically from the standpoint of bi-rational transformation. [These are chiefly by Italian writers, beginning with Caporali in 1881. ] (iii.) Castelnuovo’s memoirs on linear series of point-groups on plane curves, treated geometrically from the standpoint of bi-rational transforma- tion. (iv.) Segre’s memoirs on curves and surfaces in hyperspace. (v.) Intersection theorems as treated by Bacharach and Zeuthen. [These connect Cayley’s theorems with Brill and Noether’s theorem of residwation. | (vi.) Brill’s memoirs on algebraic correspondences in the Mathema- tesche Annalen contrasted with Castelnuovo’s memoir on the number of rational involutions to be found on a curve of given genus (deficiency). E. 1890-1900. (i.) Castelnuovo’s memoir on linear systems of plane curves as determined by given points (1891, Mem. Torino, vol. 42). (ii.) Memoirs on the theory of algebraic surfaces chiefly by Castel- nuovo and Enriques, and summarised by them in an article in vol. 48 of the Mathematische Annalen (1896). (uii.) Segre’s paper on the geometry on a simply infinite algebraic manifold, in which the properties and applications of linear series are derived from theorems in the geometry of hyperspace (Annali di Mat., vol. 22, 1894). (iv.) Bertini’s account of the principal theorems concerning linear series of point-groups on a plane curve, written chiefly from Brill and Noether’s standpoint (Annali dt Mat., vol. 22, 1894). 1 Cf. Brill and Noether, Jahresber. d. Deutschen Math. Ver., vol. iii., p. 297, 1894. ? Cf. Brill and Noether, ibid., p. 290. * Cf. Brill and Noether, Zoe. cit., p. 545. ON THE PRESENT STATE OF THE THEORY OF POINT-GROUPS. 123 (v.) Brill and Noether’s report on the theory of algebraic functions, containing succinct accounts of the contents and importance of many of the memoirs in the above divisions. (vi.) Solution of the question of the identity of the terms involution and linear series by Humbert and by Castelnuovo (1893). (vul.) F.S. Macaulay’s papers in the Proceedings of the London Mathema- tical Socrety, vols. 26, 29, 31, 1895-99, on curves through given points. § 3. ANALYSIS ACCORDING TO CoNnTENT. A. The three different methods of investigation, viz. analytical, geometrical, transcendental. B. Various definitions of the terms in use by English, French, German, and Italian writers, and the logical connection of the ideas when defined in the language of analytical geometry. C. Results obtained by the theory, expressed in the terms defined in B. (a) Concerning the linear series of point-groups on a given base-curve, e.g., Clifford’s theorem, the Riemann-Roch theorem. (8) Concerning the base-curve, proved by means of the properties of linear series of point-groups, and of linear systems of plane curves, ¢.g. : (i.) Persistence under bi-rational transformation of p (deficiency, genus). (w.) Reduction of the order of a curve with given deficiency. (vw.) Classification of plane curves into rational, hyperelliptic, k-gonal. D. Properties of surfaces in hyperspace in connection with the pro- perties of linear systems. § 4. Brint’s Memoirs on ELIMINATION AND ALGEBRAIC CORRESPONDENCES. 1863-1873. Brill’s earliest papersin the Mathematische Annalen are on problems which arose naturally out of the subject-matter of his Habilitations- schrift, viz. the transformation theory of algebraic functions in connec- tion with Riemann’s memoirs on Abelian functions. Clebsch and Gordan, in their treatise on Abelian functions, published in 1866 (the year before Brill’s Habilitationsschrift), had attempted to develop a theory of the applications of Abelian functions to geometry. Inter- preting Abel’s and Riemann’s equations as curves, they expressed the number p, which plays a fundamental part in Riemann’s theory of Abelian integrals, in terms of the singularities of the corresponding plane curve, thus identifying it with the number studied by Cayley under the name of deficiency. They further discussed the persistence of this number under bi-rational transformation—that is, the simplest type of a one-one correspondence—and the existence of certain constants (moduli) invariant under such transformation. Brill adopted their interpretation of the equations, and his work, though essentially analytical in form, is capable of direct geometrical application in its results. The number of the moduli is the subject of the first two papers. In the earlier of the two! he remarks that Riemann, by analysis, found 1 Math. Ann., vol. i., pp. 401-406, 1869, ‘ Note beziiglich der Zahl der Moduln einer Classe von algebraischen Gleichungen.’ 124 REPORT—1900, 3 p—38 to be the number of moduli of his ‘normal’ function, whereas Cayley ! obtained, by geometrical considerations, the number 4 p — 6 for the curve of (p+1)th order, the ‘normal’ curve of Clebsch and Gordan ; but by actually performing the transformation of the latter—in the case p=4 —into Riemann’s form, Brill shows that there are in fact only 3 p—3 moduli (a result which Cayley verified later.)? The second paper? was occasioned by a memoir by Casorati and Cremona,‘ in which the trans- formation of Clebsch and Gordan’s form into Riemann’s is effected, by geometrical methods, for the cases p=4, 5, 6. Brill obtains their results by different methods, employing the properties of curves in space of three dimensions. An example for p=6 is a septic with nine double points ; this he connects by a one-one transformation with a curve in space of the 8th degree, quoting Cayley ° to show that the transformation can be effected in exactly five ways, corresponding to the five straight lines in space which meet the tortuous curve of the 8th degree in four points. Similarly for p=7, the transformation of a plane curve of the 8th degree can be effected in twenty-one different ways. These examples are important, as forming a connecting link between the theory of transformation, in which they presented themselves, and the theory of elimination, to which they directly lead ; moreover, within the theory of elimination they suggest the question of the number of different solutions satisfying a system of simultaneous equations. In the year 1871, Brill begins to turn his attention to a wider theory, that of elimination when stated algebraically, or of correspondences when stated geometrically. This is shown in the title of a paper,® which con- tains proof of theorems required in the succeeding paper ;‘ but neither of these has any immediate application to our present purpose. The geometrical side of the theory of correspondences had been already attacked by Chasles, De Jonquiéres, and Cayley, but algebraical proofs of many theorems were still wanting ; and, moreover, the treat- ment of the problems in a purely symbolical and analytical manner led to the establishment of theorems in the general theory of elimination, which in their turn apply to a region intimately connected with the theory of correspondences—that of point-groups on a curve—but at the date we speak of, still comparatively unexplored. In Brill’s first important contribution to the theory of elimination,® he attacks the problem of the number of different solutions which satisfy a system of simultaneous equations.? He remarks that Roberts!® and Salmon |! confined themselves to a discussion of the degree of the eliminant in the whole number of variables, not the degree in which 1 Proc. London Math. Soc., vol. i., 1865, ‘On the transformation of plane curves.’ 2 Math. Ann., vol. viii., pp. 359-362. ‘On the group of points G. on a sextic curve with five double points,’ 1874. 8 Thid., vol. ii., pp. 471-474, 1870, ‘ Zweite Note beziiglich der Moduln einer Classe von algebraischen Gleichungen.’ + Accad. Milan, May, 1870. 5 Phil. Trans., 1870, ‘On skew surfaces.’ 6 Math. Ann., vol. iv., pp. 510-526, ‘Zur Theorie der Elimination und der algebraischen Curven.’ 7 Tbid., pp. 527-549, ‘ Ueber zwei Beriihrungsprobleme.’ 8 Math. Ann., vol. v., pp. 878-396, 1872, ‘ Ueber Elimination aus einem gewissen System von Gleichungen.’ ® See also Math. Ann., vol. iv., pp. 542-548, 1871. 10 Crelle, vol. lxvii., pp. 266-278, 1867. 1 Higher Algebra, Lessons VIII. and XVIII. ON THE PRESENT STATE OF THE THEORY OF POINT-GROUPS. 125 each variable appears. The latter is the more difficult problem, and admits of complications in which the interpretation of certain equations as correspondences is of great value (see infra, p. 129). In this paper he finds by induction, without a rigorous proof, a formula for the number of solutions of a system of equations in k inde- pendent variables (each equation being symmetrical in all the variables), the system consisting of a number of equations equivalent to i+1 inde- pendent equations ; so that 4—7—1 of the variables must have arbitrarily assigned values before the expression ‘number of solutions’ can have a meaning. When s—7z—1 have been so chosen, the ‘number of solutions’ means the number of different ways in which the remaining i+1 can be found to satisfy any 7+1 equations of the system. The number (see formula (A), infra) is made to depend on the sums and differences of the numbers of common solutions of pairs of systems of equations (in square brackets in (A) below), one system of each pair being of the same kind as the original system, but equivalent to fewer than i+1 independent equations ; while the second system of the pair is either precisely one equation, symmetrical in all the variables, or consists of a system equiva- lent to 2, or 3,. . ., or ¢+1 independent equations, involving only k—1, k—2, . k—7 variables respectively. As an important example of a system of equations of the assumed nature, he considers the original system to consist of all the equations formed by equating to zero every k-rowed determinant of the following matrix of k+7 columns and k rows, | 6104) Po (Ais + + + bese (Qy), 1 Qa)s a (Xo), + + Gi+i (Ao) | Hsia | 1 . | 91 (Ax)s i) Qx)s be sel P+ i (Ax) where ¢,, . . . ¢,,; are integral functions of the mth degree of the single variables enclosed in the brackets, these variables \,, . . . A, being all independent. Such a matrix is more shortly written as |A+4|,, and the number of solutions as (k+7),. This notation is also employed when the ¢’s are functions of more than one variable each, the variables being then connected by & relations (see infra, p. 127). The number of common solutions of all the 4-rowed determinants it contains is known to be equal to the number of common solutions of the i+1 determinants, #1 Qu); vee Gra Qi)s $d) ; x1 (A2)y $1 (Ao) $1 Ards + + = Pra (nds % Ox) where t=h,'k+1, ... +7 in turn, provided the k—1-rowed deter- minants of the matrix [a1 Qi) ++. Pra (Xr) | ot ae 1O1 (Ans - + + Pear)! do not all vanish. 126 REPORT—1900. By a generalisation of simple cases, this number of solutions is reduced to the following formula :— (A) (k+7),=[(A+7—1),(k),.]—[(A4+4—2), k—1),|+ ... Fitba eee’, where [(4+1%—1),(%),] stands for the number of common solutions of | -+7—1]||, (equivalent to 7 independent equations, provided the k—1- rowed determinants, mentioned above, do not vanish), and of ||A||, which represents precisely one equation ; and soon. A rigorous proof of this formula was not given until 1890,' but, assuming it to hold, the number of solutions, when the variables are all independent, is found by perfectly valid reasoning in the paper under consideration, and particular cases of the more general problem, to which formula (A) also applies (2.e. when there are & pairs of variables, connected by £ relations), are solved in the next paper ” by direct evaluation. When the terms of the right-hand side of (A) come to be actually evaluated, the particular case, here alone considered (7.e. of & independent variables), proves capable of direct treatment by algebraic theorems in elimination proved in the earlier part of the paper, and the final result is po —_(m—k+1) (m—h) _- . (m—k—i+1) i+t). PRD ges oye From the point of view of the theory of point-groups, a geometri- cal problem which Brill solves by means of formula (A) is of interest ; it is thus stated : Given a (k+i—1)-ply infinite family of curves of order m, viz.: a1 (X,Y) +aob(%Y)+ 2. + +erriber(My)=O. Assuming k—i-1 of the points of intersection with a straight line, to find i others such that every curve through these k—1 also passes through a certain kth point. In how many ways can this be done ? Or, in other words : In how many ways can k points be chosen on a straight line, so that an i-ply infinite system of curves, selected from a (k+i—1)-ply infinite system may pass through them ? Since the number of solutions is all that is required, the problem is not made less general by taking the intersections with a definite straight line, say y=0; substituting this value for y in the equation from the outset, we are led to finding the number of solutions of exactly the matrix con- sidered on p. 125, leading to formula (A), which, since x, ... x, arek independent variables, can be directly evaluated as above. e Brill’s investigations into the theory of correspondences definitely commenced in 1872. In the introductory remarks he attributes the origin of this theory (in geometry) to Chasles, who, in 1864, first enun- ciated the principle of correspondence for points on a straight line: ‘if to every point x there aren points y, and to every point y there are m points X, then at m+n points an x coincides with a y ;’ and who after- wards extended it, in 1866, to points on any unicursal curve.4 Cayley 1 Math. Ann., vol. ¥XxXvi., p. 326. 2 Thid., vol. vi. 8 Thid., vol. vi.. pp. 33-65, ‘ Ueber Entsprechen von Punktsystemen auf einer Curve.’ a + Comptes Rendus, vol. lviii., June 27, 1864, and vol. Ixii., p. 11. ON THE PRESENT STATE OF THE THEORY OF POINT-GROUPS. 127 had given! an extension of this principle to curves of any deficiency p;? without, however, formally proving it, and it is at this stage that Brill took up the subject. He gives an algebraic proof of Cayley’s formula for the number of wnited points of one correspondence on a given curve of deficiency p, and he finds, moreover, the proper extension to curves of any deficiency of the well-known algebraic theorem : ‘if between the points x, y of a straight line, there exists a relation (x, y)=0 by means of which « points x correspond to a point y and X points y to a pot x; and further, if by means of a second relation o'(x, y)=0 «’ points x correspond to \ points y; then the number of parrs of points which satisfy both relations is (o')=«X' +«’d.’ The first relation ¢(x, y)=0 is said to establish a correspondence («, A) between the points on the straight line ; the second, ¢/(a, y)==0, a correspondence (x’, \’), and ($¢") gives the number of pairs of points which satisfy both correspondences. Brill’s extension is as follows :—Given a fixed point z on a curve fg deficiency p, and two movable points, x, y, on the same curve, and let the two relations, » (x, y,2)=0, ’(x, y, z)=0 hold, which, regarded as functions of x have k, k! points of intersection, respectively, with f (x)=0, of which B, B’, respectively, coincide with the point z, and y, y’ with the point y; 3 and which, regarded as functions of y, have 1, V' points of intersection, respectively, with £ (y)=0, of which a, a’, respectively, coincide with the point z, and y, y' with the point x ; then the number of pairs of points, x, y, (each point being distinct from the other and not coinciding with z), which satisfy both relations is given by (¢¢')=«N' +%/'A—2pyy’s k=kh—B—y, x/=kh'—f'—y’ where Jats wens p Sis gil Wl The first application of this formula is to find in how many ways three points on a curve £=0 can be chosen, so that a singly infinite system of curves, selected from a given triply-infinite system, may pass through them. 'This is a simple case of the problem already referred to on p. 125 (viz. k=3, i=1), but now we have to deal with a base-curve of any deficiency p, instead of the straight line, and thus it is impossible to eliminate y and to obtain equations in three independent variables «), %, 3. We obtain a matrix similar, but not identical, to that on p. 125, viz. :— [prgeas)s o(ayi)s b3(%1Yr)» a(*171) \pr(2e24/o)s 2(2Y2)s Pa(%2¥2)s s(@2Yo), 1b (23Y3)s P2(@aYa)> P3(LaYa)s P4(@3Ya), and further, the three equations f (2,y)=0, f (xy2)=0, F (w3y3)=0. As before remarked, however, the formula (A) still holds and gives us (3+1)3=[(3)3(3),;]—(8—1)3 but for this simple case it is worth while to work out the problem directly in the first place, without using formula (A), as it affords insight into the geometrical meaning of a correspondence Observe, first, that before a finite number of solutions can be found, one point, z, on f=0, must be assumed arbitrarily, since k—-1—1=1. 1 Comptes Rendus, vol. |xii., 1866, p. 586. 2 Cayley’s result is that the number of ‘ united points’ is m+n + 2pk, where & is a ‘quantity afterwards known as the Wertighett of the correspondence curve. 3 B is said to be the Wertigheit of at v=2z, y at r=y; B’ ” ” ” ” ¢! at x =2 07" at ev=Y; a ” » ” » @ aty 128 REPORT—1900. Also, if any two independent curves of the triply-infinite system can be passed through this arbitrary point z and through certain other two a, y, on f=0, then a singly-infinite number passes through these three points, and they form one of the triplets whose number is required. To arrive at two independent curves of the system, take any two fixed points A, B, in the plane, and consider first the curve through z and A, then that through 2 and B ; each has still one degree of freedom, but loses this and becomes perfectly determinate if passed through a common point y on f=0. Let every curve of the triply-infinite system have M movable points of intersection with f=0—that is to say, M points whose co-ordinates depend on the variable parameters of the system—then these two independent curves determined by y have each M—2 points of intersection x with f=0 besides z and y ; and in general the M—2 2’s belonging to one curve will be all distinct from those belonging to the other ; but if y be properly chosen (or, we may say, for certain positions of y on f=() an # of one curve will coincide with an x of the other, «, y, z thus forming one of the required triplets, since two independent curves pass through them. The expression for certain positions of y on f=0 introduces the idea of the movement of the point 7 on f, which necessitates a corresponding movement of the two sets of M—2 2’s belonging to the two distinct curves ; we may say with reference to each curve, that to every position of y there correspond M —2 positions of a; moreover, since, when confining the attention to the curve through z and A, it is immaterial which of the M—1 points is called y, we say that to every position of « there correspond M—2 positions of y: we have a symmetrical correspondence (M—2, M-—-2) between the points x, y established on £=0 by means of the curve through z and A ; and, similarly, we have another established by means of the curve through z and B. But we have already pointed out that for certain positions of y, i.e. of the . one of the M—1 points which is common to both curves, there will be an « common to them as well, and it is the number of such positions of y (or of this x, since the relation of this particular x and y is reversible) that we wish to find. Again, since the original system has three degrees of freedom, the system through A (or through B) has two degrees of freedom ; hence one curve of the system can always be drawn to touch f=0 at any point on it, and no curve can have a double point. In other words, wherever z is taken on f=0, there is always one position of y which coincides with z (on the curve touching f=0 at z), or y=z satisfies the correspondence equation @ identically once. (If no curve could have been drawn to touch /=0 at any arbitrary point, y=2z would not satisfy the correspondence equation identically at all, whereas, if a curve with a double point at any arbitrary point on f=0 could have been drawn, then y=z would have satisfied the correspondence equation identically twice, &c.) The number of times that y=z satisfies the correspondence equation is called the ‘ Wertigkeit’ of the correspondence, and is denoted by [¢],... In symmetrical cor- respondences, such as the one above, a, vy, z are all interchangeable, and therefore [],,=[¢]..=[¢].,- The value of the ‘ Wertigkeit ’ is written as a subscript to the bracket (9’) ; thus, in the language of correspondences, the number of solutions to our present problem is the number of pairs of points which satisfy two correspondence equations, each given as (M—2, M—2),. But from this number must be subtracted those pairs of points which lie on that one curve of the triply-infinite system which passes through both A and B as well as z, for these do not lie on two distinct curves, and therefore not on a curve ON THE PRESENT STATE OF THE THEORY OF POINT-GROUPS. 129 of a singly-infinite system. The number of such pairs is obviously the combinations in twos of the M—1 points besides z, which lie on f=0, i.e. M-—1.M-2 pategr pat y=y’=1 in the formula given on p. 127 for (%¢’) (dividing it, however, by 2, since our correspondences are symmetrical), and then subtract M—1.M—2 it is If, therefore, we write k=x’/=\=)\’/=M—2 and from this, we obtain the number of triplets, viz. (M—2)?— p—}(M—1)(M—2)=}(M—2)(M —3)—p. Now compare the steps of this process with the formula (A) for this case, 7.e. with (3-+1)3;=[(3)3(3);]—(3—1)3 and we see that the two cor- respondences employed, exactly similar, were the determinants, the number of whose solutions was denoted by (3)3, (3)3, while (3 — 1), gives the num- ber of those solutions which needed to be subtracted from the total number. In more complicated problems, formula (A) is used at once, and the evaluation of the number of common solutions of the equations in the square brackets (the number and form of these equations is given above, pp- 125 and 126) is performed by interpreting these as correspondence equa- tions (cf. p. 124), provided we know how many points correspond to one in each correspondence (they are always symmetrical, as is seen at once from The other cases to which Brill applies the theory of correspondences in the paper under consideration are :— (a) To find the number of triplets of points on a given base-curve through which a doubly-infinite system of curves, contained within a 4-ply infinite system, can be made to pass. (6) To find the number of sets of four points on a given base-curve through which a triply-infinite system of curves, contained within a 6-ply infinite system, can be made to pass. In the first of these =3, 1=2 ; in the second k=4,i=3. They are both rather more complicated than the one we have considered in detail ; the first, namely, involves finding the number of triplets of points which satisfy three correspondences, for (3+2)s=[(3 + 1)3(3)3]—[(3)s(2)3] + (1), and the number of independent equations (see p. 126) involved in [3+ 1|[5, ||3\[] is 2+1—=8, involved in [||3}[5, |[2\l,] is 1+2—3, and involved in (1); is 3; similarly, the second involves finding the number of sets of 4 points which satisfy 4 correspondences, for here we have (4+3)4=[(6).(4)4]—[0)4(3)4] +[(4)a(2)4]- (1) a, and the total number of independent equations in each term of this expression is 4, namely, 3+1, 2+2,1+3 and 4. Moreover, it is essential to the final evaluation to take notice of the way in which the 4 inde- pendent equations are grouped ; the formule in the theory of correspond- ences for finding the number of sets of 4 points which satisfy 4 equations when these 4 are grouped as 3+1 differs from that in which they are grouped as 2+2; but since the difference only appears in the terms 1900. K 130 REPORT—1900, involving p, it does not exist when p=O, 7.e. when the base-curve is a straight line or a unicursal curve, and it was for this reason that the actual solution of the previous problem (p. 126) was possible. The required formule for i=l, 2, 3 (leading to 2, 3, and 4 simultaneous correspondences), are worked out in the earlier part of this paper for all possible different groupings of the sets, and the final results for examples (a) and (6) are M—2.M-—3.M—4_ at (a) 133 p (M—4) M-3M—4.M—5.M—6 M-—6.M-—5 __, p(p-l) 2) 12.34 Leia oo ee where, as before, M denotes the number of movable points of intersec- tion of each curve of the given system with f=0. We notice in passing that these results agree with that of p. 126, when p=0, M=m. A problem in the theory of point-groups, of which the above are par- ticular cases, was first enunciated in the most general form in a paper by Brill and Noether, in 1873.! They state it thus :— Gwen a t-ply infinite system of adjoint curves—that is, of curves passing s—1 times through every s-fold point of £=0—it is required to find F points on the base-curve, £=0, which form such a point-growp—or set of points—that the curves of the given system which pass through it form a q-ply infinite system. If the equation of the system is a1$,(%)Y) +ash(ry)+ . : ~ + 4¢419%t41(@1y)=0 this problem leads, by known theorems, to finding the common solutions of all the (¢—q+1) rowed determinants of the matrix. lpi(%141), Pe(*1%i), — - . . Oe (iY1)| |P1(B2Y2)s . . . Pe+1(Z2Y2), | : Pil@pYn) - : . - Pesi(®pYp)! where LY, CoYo, - . . . - Rp, are connected by the equations S(xy,)=9, . . . . . SF (€pY¥x)=0. The simplest case is therefore to be found by taking R=t—q+1, and this is, in fact, the only case completely solved. The formula for the number of solutions was given in this memoir, viz. :— +a (11) (8) (G1) +) 3) - (B) i 820 (—n(Q)(A*1-9 Baas ide). .2 CVE ("3 (@4y) - pin 2°). iho ' Math. Ann. vol. vii., pp. 269-310. ‘Ueber die algebraischen Functionen und ihre Anwendung in der Geometrie.’ ON THE PRESENT STATE OF THE THEORY OF POINT-GROUPS. 1381 where Q=2p—2—R and ie) stands ae sma ine st Ml ete BY m but the rigorous proof only ay ered in the year 1890. For particular values of g, however, viz. g=1, 2, 3, and assuming the rigorous proof of formula (A), formula (B) was proved in the previous papers. In fact, we see that (a) and (d) on p. 130 are particular instances in which R=4, g=1, Q=M-Aé. Report on the Chemical Compounds contained in Alloys, By ¥. H. Nevit1e, F.B.S. PART I. PAGE Methods of Discovery af Compounds . . : : 2 : ; : . 131 Chemical Methods of Isolation ; . : f j F : ‘ : . 131 Freezing-Point Curves . : : . ‘ ‘ : : ° : : . 132 Microscopical Study : : . - : : ; ; . : - Salant Rintgen-ray Photography. - A . 141 Determination of Electrical Potential and other Physical Methods. : . 142 Part II. Table of Intermetallic Compounds and Discussion of it : 2 ‘ ; . 144 Molecular Weights of the Metals . : - 146 Tables of Depression of the Freezing-point caused by dissolving other metals in Tin, Zinc, Bismuth, Cadmium, Lead . 147 Table of References ; . : F ; : : : ; . 149 PART I. Although most students of alloys are now convinced that they often contain definite chemical compounds, yet these ‘intermetallic’ com- pounds are still passed over in silence by the authors of books on descrip- tive chemistry. The cause of this omission lies in the difficulty of isolating these bodies in a pure state, and in their resemblance to the metals. It must be acknowledged that just as the metals resemble one another more than do the non-metals, so their compounds often present a great superficial resemblance to their constituent elements. Intermetallic compounds might well be compared to the somewhat intangible bodies formed by the union of the halogens with each other and with sulphur. Many of these bodies show marked dissociation—that is to say, they readily form systems in true equilibrium with their components ; it is almost certain that ‘intermetallic’ compounds present the same phenomenon when in contact with liquid alloy. Methods of Studying Intermetallic Compounds. The method that naturally suggests itself to a chemist is that of ex- tracting the pure compounds from an alloy by filtration, by volatilisation of excess of a volatile metal, or by removing the excess of metal by means of a suitable solvent. Each of these methods has been employed with some success. Filtration methods are very difficult at high temperatures, but if the difficulties can be overcome so that the first solid separating from a liquid as it freezes is isolated, we shall get invaluable information. By the filtration of a partly solidified solution of gold and cadmium in tin, Heycock and Neville (') obtained a crystalline residue approximating to the formula K 2 . 132 REPORT—1900. AuCd, even when the proportions of gold and cadmium in the original mixture varied within wide limits. Again (?), by alloying gold with excess of cadmium and distilling off the excess of cadmium they obtained a residue having the.composition AuCd. Now that many metals have been distilled in vacuo this method may meet with success in other cases. M. Lebeau (*) dissolves metals in excess of sodium and distils off the excess of sodium by the prolonged passage of ammonia gas followed by that of nitrogen. He thus obtains the bodies SbNa;, BiNa,, SnNa, in a pure state. He is also succeeding by the same method with the other alkali metals. M. Joannis (*) some years ago applied a similar method successfully. The method of fractional solution enabled Debray (°) to isolate the bodies PtSn,, RhSn;, RuSn;, by the action of dilute hydrochloric acid on alloys containing excess of tin. M. Le Chatelier(®°) has in the same way isolated the compound Cu,Sn. He emphasises the opinion that by choosing a suitable solvent, suggested by electro-chemical considerations, the method will be found generally applicable. For example, by sub- jecting alloys of copper and zinc to the prolonged action of a paste of lead chloride he has obtained crystals of pure Zn,Cu. Mr. Heycock, in a research not yet published, obtained large crystalline grains of PtAl; by the action of hydrochloric acid on a slowly cooled alloy of aluminium and platinum. Mr. Stead (7) has isolated in this way crystals of SnSb, Au,Pb, Au;Pb,, Sn;Aso, and probably of some other alloys. The work is in some cases not yet published, but he has been kind enough to com- municate the results for the purpose of this report. Other cases could no doubt be quoted in which fractional solution leaves a residue having a formula, but there is a great risk of the solvent attacking the crystals ; and, as Mr. Stead has found, the existence of mixed crystals, or, at all events, of crystals having a core different from the out- side, is a serious drawback to this method regarded as an independent method of discovery. It would seem that the proper moment for the application of these methods comes when by the microscope, by the freezing-point curve, or by potential determinations the existence of a compound has been already indicated. In a systematic study of intermetallic compounds I should therefore put first that of the chemical equilibrium of the binary system: this is generally expressed by the freezing-point curve. Next, and perhaps of equal importance, comes the microscopic examination of the solid alloys. Thirdly, as more limited in scope, but sometimes more emphatic in its indications, comes the determination of the difference of electrical potential existing between a metal and its alloys. The method of studying chemical equilibrium which we owe so largely to Professors Bakhuis Roozeboom and Le Chatelier is now familiar to most chemists, and in the case of a binary system it can be sufficiently described in a few words. A mixture of two substances, A and B, in certain proportions is melted. It is allowed to cool slowly, and the temperature is noted at which solid matter begins to separate from the liquid. This is the ‘freezing-point.’ It tells us the temperature at which this particular mixture becomes saturated—that is to say, comes into equilibrium with a particular solid. By repeating the experiment with a series of mixtures of A and B we get as many points as we need for plotting the freezing-point curve. In this curve, one ordinate is the percentage composition of the mixture expressed either in weight per cent. of A and B, or, better, in atomic or molecular ON THE CHEMICAL COMPOUNDS CONTAINED IN ALLOYS. 1338 per cents. ; the other ordinate is temperature. It is desirable to observe not only the first halt in the cooling, but also any lower ones that occur down to the moment of complete solidification, or even below it. It is also desirable to isolate by filtration the crystals which form at the freezing- point, and to analyse them. This wouid give the composition of the solid and liquid phases which could exist in equilibrium at the observed temperature. Unfortunately, on account of experimental difficulties, isolation of the solid phase has not been carried out in the case of alloys, and a later microscopic study of the wholly solid alloy is a very imperfect substitute for it. We now know pretty well the types of freezing-point or equilibrium curves that occur. In the simplest of all cases—that in which the two bodies A and B neither combine chemically nor form mixed crystals—the complete curve resembles fig. 1. It consists of two branches cutting each other at the eutectic angle. Fra, 1. One branch, which starts from the freezing-point of a liquid wholly composed of a, corresponds to the formation of primary crystals of pure A at each freezing-point, the other branch to the formation of primary crystals of pure B. When the liquid, either from its initial composition or through the separation of the primary crystals, reaches the composition of the eutectic intersection, A and B crystallise simul- taneously but in separate crystals. Thus the solid eutectic alloy is a very minute conglomerate, while all other alloys contain large primary crystals of Cone either A or B embedded in this conglomerate. This has been conclusively demonstrated by the exquisite microscopic work of M. Osmond (8) and also by that of M. Charpy (°). Curves which approximate to this type have been worked (1° 2"* !) out for the pairs Zn.Al, Zn.Sn, Au.Cu, Ag.Cu, and some other metals. Such curves do not indicate the existence of a compound, though it would be too much to say that they disprove the existence of compounds. When a compound exists whose melting-point lies in the region above the freezing-point curve of the two metals, it produces a separate branch cutting the other two branches. At points on this intermediate branch the saturated liquid deposits crystals of the compound. The summit of this branch occurs at the concentration corresponding to the formula of the compound. If more than one compound exists there is a branch for each compound, although parts of the branches may be lost by lying below the curves of more stable bodies. While the above is the usually accepted view as to the meaning of summits and eutectic angles in a freezing-point curve, two points may be noted. The first is M. Le Chatelier’s opinion as to the position of the summit caused by a compound. He thinks (!?) that when a compound partly dissociates on fusion, the summit caused by its presence may not be exactly at the percentage composition corresponding to its formula, and that the formation of mixed crystals may have a similar effect on the curve. This is a matter needing further investigation. The other point concerns the position of the eutectic angle. While it is well established that the eutectic alloy is a conglomerate, not a compound, we should be wrong to ignore the fact that the angle often comes surprisingly near to 134 penn “41900: a simple formula—for example, in the AgCu and AuCu curves. Sir George Stokes has lately recalled our attention to this point. Paterno and Ampolla (!%) have noticed a number of similar cases in ‘organic mixtures. A good many curves indicating by intermediate branches the existence of compounds have now been determined, but for the purpose of illustrating the subject further the curve of AuAl will be taken. As can be seen from fig. 2, there are seven branches, each corre- jeives 2 Atomic Percentage of Al. 0 100 es Re 3 mS oO Seal a SEY ater Bree Face eee a! Bag Sw + is Weight per Trent. of Aluminium sponding to the crystallisation of a different solid. The extreme branches, AB and 1, being regarded as those of the two metals, we have five left, each of which may indicate a compound. The branch DEF has its summit exactly at the formula Au,Al. The microscope shows that the summit alloy E is an almost homogeneous body, and that all solid alloys whose composition lies between that of Dp and F contain large crystals of the = body immersed in a mother substance. As we descend the curve from the summit the large crystals of & are found to occupy less and less of the whole alloy, until at p and F they cease to exist. Exactly similar ON THE CHEMICAL COMPOUNDS CONTAINED IN ALLOYS. 135 phenomena show themselves on the branch cui; the summit H occurs at the formula AuAl,, and large crystals of this body are found embedded in mother substance in all alloys between G and 1. These criteria taken together—(1) the occurrence of a summit at a formula percentage, (2) the presence of large crystals of the same kind, decreasing in amount as we descend the branch on either side—are, I believe, an absolute proof of the reality of a compound. The two bodies ‘Au,Al and AuAl, as certainly exist as do the two chlorides of copper. But there are other compounds more obscurely indicated by the curve ; the branch Fe has its summit, x, below the branch Gu, hence the x body which crystallises at points on GF never occurs alone in a solid alloy. The microscope shows that solid alloys between G and H contain large crystals of AuAl,, surrounded by a coating of the x body, and that outside this coating there are large independent crystals of x embedded in a minute conglomerate of x and E. The fact is that in the first stage of freezing, while the large crystals of AuAl,, or Hu, are forming, the liquid part necessarily gets richer in gold until it reaches the composition G. From this moment the H crystals cease to form, and the Fie. 3. existing ones become coated with the x body, which at lower temperatures crystallises independently in large crys- tals, that in a certain sense are primary. Finally, the residual liquid reaches the state F, and the eutectic conglo- merate forms which is com- posed of crystals of Au,Al and of x. Thus an alloy may contain a compound although that compound does not occur as the sole constituent of any particularalloy. This appears to be a very common case ; for example, Mr. Stead finds that in bronzes very rich in tin the erystals of Cu,Sn are coated with CuSn, and M. Charpy (°) has recorded a similar feature ‘In the bronzes very rich in copper. In both these cases the eutectic lies outside the coating. : MM. Le Chatelier (!*), Gautier, and Gosselin (1°) have traced a number of remarkable freezing-point curves for pairs of metals, of which examples are given here. Unfortunately the composition is stated in percentage by weight, not in atomic per cents. Copper-Aluminium (fig. 3).—Here we find two well-marked summits, one very exactly at Cu,;Al, the other near CuAl,. Copper-Antimony (fig. 3).—Here there is a well-marked intermediate summit which, if it were at a formula point, would almost certainly indicate a compound. M. Le Chatelier attributes the formula Cu,Sb to it, but measurement on the curve seems to give the summit the formula Cu,;Sb,. These two curves, and one of SnCu also due to M. Le Chatelier, 136 REPORT—1900. are especially interesting, as they were the first high-temperature curves of this kind with intermediate summits due to compounds that had been published, and the paper ('4) in which they appeared marks a new departure in the subject of alloys. Aluminium-Antimony (fig. 4).—The maximum point is very much higher than that of either metal ; it is at 1048° C. with 14°66 per cent. of aluminium. The curve is remarkable because it shows that nearly all mixtures melt above the melting-point of either component. Nickel-Tim (fig. 4).—Here the intermediate summit is at Ni,Sny. M. Gautier gives other Fia. 4. curves of great interest, some of which were simultaneously studied by Heycock and Ne- ville (1), but many of them need further work before they can be safely interpreted. Perhaps the freezing-point curves investigated by M. Kurnakovy throw as clear a light on intermetallic com- pounds as any work that has been done. This work can be readily followed from the two diagrams contained in his paper, and reproduced in figs. 5 and 6. The composition is expressed in atomic percentages. The first diagram (fig. 5) gives the freezing-point curves of amal- gams of sodium and potassium. In the HgNacurve at least six separate branches can be seen, each corresponding to the crys- tallisation of a different solid. It would be premature to as- sert that each branch proves the existence of a correspond- ing chemical compound, but there can be no doubt that the summit G proves the existence of the compound NaHg,, a body whose melting-point is much higher than that of either component. Similarly, in the curve for potassium amalgams, besides minor branches there is a well- marked summit at the formula K Hg,. The other figure (fig. 6) gives the freezing-point curves of the mixtures NaBi, NaPb, NaCd. It is unfortunate that so few alloys were examined , on the upper part of the NaBi curve, but the existence of the freezing- point m above 700° C. makes a compound very probable. M. Kurnakov seems to have no doubt that it indicates Na,Bi, a body already prepared by Joannis and by Lebeau. There are two summits on the NaPb curve— one at p, which must be very near the formula Na,Pb and one at P’ to which he does not at present assign a formula. In the NaCd curve we 1400 1300 1200 1100 1000 500 0% 10 20 30 40 «SO 60 70 80 90 00 ON THE CHEMICAL COMPOUNDS CONTAINED IN ALLOYS. 137 see two well-marked summits, at 0 and 0/, the first being exactly at the formula NaCd,. It is evident from these curves that the summits of many of the branches lie below other branches, and therefore correspond to unstable states. The position of the summit and the formula of the compound must in such cases be a matter of speculation until experi- ments of another kind have been made.! M. Kurnakoy has also studied the crystalline matter which separates at the freezing-points, and has noted great variations in this as one goes from one branch to another. He separated by filtration the hexagonal plates which crystallise at points along the branch zc, and analysed them. Fig. 5. Rylig PY RHy RHg, Rg, Ry, Rly, Rly, 0 : O%Hg = 107 "% y 50% 60% J 70% 60% 0% Na Atomic percentage. 0% Na He found, however, that the composition of the crystals varied from point to point along the branch. He attributes this to the presence of mother liquor attached to the crystals, and he thinks that the crystals, if free from mother liquor, would have had the formula Na,Hg. This is a very reasonable supposition, but it may be that he was examining mixed crystals. The formation of mixed crystals of two bodies which crystallise isomorphously is certainly common in alloys, and may be, the cause of singularities in the freezing-point curve. Indeed, it is doubtful if we ‘ The amalgams of sodium and potassium have been examined by various other methods ; for example, by the determination of their specific volume—a method recently employed by E. Maey (Zeits. Phys. Chemie, xxix. p. 119). He finds a number of angles in his plotted curve which he attributes to the existence of compounds. 138 REPORT—1900. shall arrive at certainty in the interpretation of such curves until; this question of mixed crystallisation has been thoroughly studied. M. Le Chatelier some years ago pointed out the importance of this question and studied it. The curve for mixtures of silver and gold has been quoted as a type for bodies which form mixed crystals in all proportions. It is a con- tinuous curve joining the Fia, 6. points of fusion of the two Na BiNa. Pb Na M components, and differs from —— 2 such acurve as that of fig. 1 by consisting of one branch only. Mixed crystallisation of two bodies, one or both of which were compound, might be indicated by a continuous curve joining the freezing-points of the two proximate constituents of the crystals. There are probably several such cases in the curves given by M. Gautier. Charpy and Stead have independently studied with the microscope a pe- culiar crystal structure which they conjecture to be due to mixed crystallisation. But no case of isomorphism in alloys has been worked out in a manner that is con- clusive. Until lately a satisfactory theory of the subject was lacking, but Professor Roozeboom (1°), to whom physical chemists owe so much, has lately investi- gated it, and MM. Van Eyk, Reinders, and Hissink have verified his views in the case of certain mix- tures of two salts. It seems very desirable that students of alloys should Naor 90 80 70 60 50 40 30 20 10.0% begin to work in the light Atomic percentage. of this theory. An at- tempt will therefore be made here to state Roozeboom’s view in the simplest case he gives. For this purpose we must look again at fig. 1, the curve for a pair of metals which neither combine chemically nor form mixed crystals. Here the region above the curve corresponds to liquid states, the line of the curve to equilibrium between a liquid and crystals of a for the left branch and B on the right branch ; the region below the curve, but above the angle, to mixtures of solid a or B with varying liquids ; and, finally, all the ON THE CHEMICAL COMPOUNDS CONTAINED IN ALLOYS. 139 region below the eutectic angle to solid conglomerates of separate crystals of Aand B. The range of temperature between the first appearance of crystals in a liquid alloy and its complete soliditication is measured by the vertical line drawn from a point on the curve to the level of theeutectic point. Let us now suppose that the two metals, which we will still call a and B, can form mixed crystals in all proportions. According to Roozeboom there will be no angle of intersection of the two curves, but the freezing- points of A and B will be joined by a continuous curve, the points on which correspond to exactly saturated liquids. He calls this the ‘i’ or ‘liquid’ curve. But also starting from the freezing-points of a and B, and lying under the ‘L’ curve, a continuous curve can be drawn giving the composition of the mixed crystals that form at each temperature. He calls this the ‘s’ or ‘solid’ curve. The case is represented in fig. 7, which, together with figs. 8 and 9, is taken from his paper. To find what happens at a particular temperature, draw a horizontal line cutting the ‘L’ curve inn and thes curve ino. These two points of intersection give the composition of the two phases that can exist together at the temperature of the horizontal line. In fig. 7 m gives the composition of the liquid that when it begins to freeze deposits mixed crystals of the percentage o. Fie. 7. The complete process of freezing can now be stated. Draw through m a vertical line mnqz cutting the L curve in m and the s curve ing. Then n and all points above it correspond to uniform liquid, g and all points below it to a uniform mass of mixed crystals (not, asin fig. 1, to a conglomerate of crystals of A and B). The —= temperature range during freezing isng, and ,477% during the process, if perfect equilibrium is iil ensured, the solids formed undergo continuous transformation from the composition o to that 3 of q, while the liquid remaining at any moment Gone changes from n to p, where p is the intersection of|t by a horizontal through g. Thus all the areas shaded vertically repre- sent homogeneous states—above 1 of a liquid, below s of homogeneous crystals. The part between L ands, shaded horizontally, represents states, in which a solid is mixed with a liquid. The t and s curves may have a maximum or a minimum, in both of which cases they touch each other at the maximum or minimum point, as in figs. 8 and 9. The liquid whose composition is that of the maximum or minimum will solidify completely at one temperature. Hence in the case of the maximum one might mistake the solid for a definite chemical compound, and in the case of a minimum for a eutectic mixture. One must remember that the diagram need not stand for the whole freezing-point curve of two elements, but for the horizontal space between the two points corresponding to compounds, and we can treat the compounds themselves as the components of the mixed crystals. Our copper-tin curve probably shows such a case in the region between Cu,Sn and Cu,Sn. These considerations point to a great danger in the interpretations of the minor details in complicated freezing-point curves such as those of Kurnakov, Gautier, and our AuAl curve. Given perfect equilibrium transformations during cooling, it should be fairly easy by appropriate 140 REPORT—1900. experiments to discriminate between a summit due to the existence of a chemical compound and one due to the form of a mixed crystal curve. In Fie. 8. Fig. 9, A U "1 al such cases as Kurnakov’s NaHg, and KHg,, our Au,Al, and Roberts- Austen’s AuAl,, where the formula of the summit is an exact and simple one, there can be little doubt. A microscopic examination of the summit alloy might not help, but that of alloys at some distance on either side of the summit ought to settle the matter. If they are homogeneous, give a uniform ignition colour, and etch all over at the same rates, the summit must be due to mixed crystals ; while if the alloys show primary crystalli- sation embedded in a mother substance, the primary crystals continually decreasing in amount as we go down the curve, the summit is probably a compound. This is the structure we found near the two summits of the AuAIl curve. But Roozeboom points out as the best method of attacking such questions the two following series of experiments: (1) Determine not only the freezing-point of each alloy, but also the temperature at which it sets to a solid mass. From these data, both of the curves L and s could be plotted. The setting-point would probably not be very sharply marked, but a recording pyrometer would indicate its whereabouts by a greater rapidity in cooling after the point was passed. Cooling-curves such as those of Sir W. Roberts-Austen might be made to give the information needed for plotting the s curve. We, in a very imperfect way, sought for the setting-points in determining our AuAl curves, but found instead the usual horizontal lines of second freezing-points, The existence of these renders mixed crystals improbable. The other line of research, adopted by Reinders and Van Eyk and Hissink, is to extract the first crystals that form and analyse them, as well as the mother liquor from which they were taken. If this were done for alloys on either side of a summit due to a compound, we should find the crystals having all the same composition—namely, that of the com- pound ; while if the summit were due to the existence of mixed crystals, the solids extracted from alloys of various compositions would differ widely. There can be no doubt that this process, troublesome though it would be, is the proper way to attack the interpretation of a complicated freezing- point curve. A few cases out of many may be mentioned where mixed crystals are probable in alloys : between Cu;Sn and Cu,Sn, in lead-thallium alloys, in bismuth-antimony, in gold-silver, in alloys containing zine or cadmium with either silver, copper, or gold. A careful study of some of these cases is probably the most pressing ON THE CHEMICAL COMPOUNDS CONTAINED IN ALLOYS. 141 need at present in intermetallic chemistry. The difficulty of this subject, whether we use the freezing-point curve or the microscope, is increased by the uncertainty as to the maintenance of perfect equilibrium at each stage of the cooling. Microscopic Examination. Osmond, Charpy, and Stead have shown us how much light the micro- scope throws on our subject. The microscopic examination of the pattern shown by the polished surface of an alloy that has, if necessary, been etched or heated to produce oxidation colours seems to bring us nearer to the phenomena than other methods of experiment. It is often quite easy to determine which crystals formed first in the freezing (the primary crystallisation), but there are certain types of pattern that are very puzzling. Among the points calling for an answer are the following : 1. Does the existence of coated crystals, such as one finds in gunmetal and also bronzes containing more tin than Cu,Sn, indicate the existence of a second compound? The answer is, Yes, in some cases—for example, in the AuAl curve and, as Mr. Stead thinks, in the bronzes rich in tin, where the Cu,Sn crystals are coated with CuSn. M. Le Chatelier has lately pointed out that in all such cases the solid alloy is not in equili- brium and that the effects of annealing will generally be great. 2. Can the existence of series of mixed crystals be detected by the microscope ? M. Charpy and Mr. Stead both describe a similar structure, and are disposed to attribute it to this cause. i 3. How far will the microscope supplement the very meagre indica- tions that the curve sometimes gives of a compound ? As an answer one can take the portion of our copper-tin freezing-point curve (fig. 10) between Cu,Sn and Cu,Sn. The curve is almost straight, the swelling (one cannot call it a summit) corresponding to Cu,Sn being very slight. But the microscope shows Cu,Sn as a homogeneous body, while alloys with a little more tin show new crystals embedded in this and sharply separated. These.new crystals increase as we add more tin, until at Cu,Sn they fill the whole alloy ; thus the microscope is here much more decisive in its indications than the curve. Réntgen-ray Photography. Skiagraphs of thin sections of alloy which contain one transparent metal, such as sodium or aluminium, and one metal more opaque, some- times give fine views of the crystals in the alloy. This method has the advantage of showing the structure of the alloy as it is before any etching or other reagent has modified it. The two photographs shown were taken some years ago by Mr. Heycock and myself. The first is aluminium alloyed with ten per cent. of antimony. One sees that a heavy compound has crystallised out first. This is in harmony with M. Gautier’s curve which presents no branch along which primary crystals of aluminium could form. If a series of such photographs had been taken with increas- ing percentages of Sb, we might have been able to locate the percentage at which the compound was pure. 142 REPORT—1900. The other photograph is one of aluminium containing ten per cent. of nickel. One sees that an opaque body has again crystallised first The varying thickness of some of the crystals gives them an effect of solidity which is absent from a surface photograph. Unfortunately the alloys have to be very slowly cooled in order to Fie. 10. ee ee eS eta | Ma) eel Sl Mth hh aaa oe aes 10a0e8 PORE BER OE Covi eee henna Eee eee es ? RES ERE oS ae eee ean.) || ee ee mieIv | 1 eset Ph | een NS ee CE aR Ee! Soe eeae ee selva) ||, ea S| af ah de da SERVE RAMSC CoRR eee DEERE Soe VERE ale es No] SA Ot label: te pd Sener i5y 5 Pt | PtSn, f 9 It would be very easy to amplify this list ; for example, various other arsenides and antimonides have had formule assigned to them, and some alloys of aluminium and tin with the rarer metals appear to have been isolated as crystals. Further research will no doubt enormously expand it, though it may also cause the rejection of a few that have been included. But as the list now stands it offers matter for the consideration of the student of valency. One sees that the compounds of the metalloids with the metals present formule that we should expect from the known valencies of the elements, but such bodies as NaHg,, SnCu, AlAg, are more remarkable. The first of these is evidently a well-marked type, which already occurs several times. If I rightly understand Professor Kurnakov, he thinks that Mendeléef’s law of the total valency of an element for oxygen and hydrogen being 8 will find application in the formule of alloys, the hydrogen being replaced by other metals. In this case, the alkali metals which are monovalent to oxygen should be polyvalent in alloys ; his curves certainly support this view. The freezing-point curves show that the most marked summits—that is, the most stable compounds—occur when a strongly positive metal, such as sodium or aluminium, is alloyed with a metal, such as antimony, leagd, or gold, which is far removed from it in the electro- chemical series. The Molecular Weights of Metals. With the exception of the limited number of vapour-density determi- nations which show that mercury, cadmium, and zinc, and perhaps also sodium and potassium, have monatomic molecules when gaseous, the only evidence as to the molecular weights of metals lies in experiments based on. Raoult’s methods. ON THE CHEMICAL COMPOUNDS CONTAINED IN ALLOYS. 14.7 Professor Ramsay and M. Tammann in 1890 showed that small quantities of various metals dissolved in mercury gave, for the most part, depressions of the vapour-pressure and of the freezing-point, which indi- cated that the dissolved molecule contained one atom of the added metal. At the same time, Mr. Heycock and I found that this was in general true when metals were dissolved in tin. At later dates we extended the generalisation to solutions of metals in the solvents bismuth, cadmium, lead, and zinc, and tables summarising our results are reproduced in the present report. If we could be certain that the dissolved metal did not form a chemical compound with the solvent, these results would afford very strong grounds for holding that the molecules of the dissolved metals were in most cases monatomic. But we know now that chemical com- bination is not uncommon, and it is evident that in dilute solution the dissolved metal a will tend to form compounds of the type 4 B,,, where B is the solvent. Hence the problem of the chemical compounds formed by metals with the solvent metal must be solved before we can safely dogmatise concerning the molecular weight of the metals when in solution. To take a special case, one atom of copper dissolved in tin produces the molecular depression of the freezing-point, but from Mr. Stead’s work we have good reason to attribute this to the presence of a molecule CuSn. On the other hand, the abnormal depressions obtained by us in certain cases point to the probability of the compounds Bi,As,, Bi,Cu,, Cd,,Hg., Cd,Zn,, Cd,Pd,, Cd,K,, Cd,Au;, Cd,As,, Pb,(Cd, Hg, Bi),, Pb,Sn,, Pb,,Na,, most of which have not at present been studied. It is obvious that m may be zero in any of these. The question of the depression of the freezing-point in dilute solutions, is, however, complicated by the probable appreciable solubility of the dissolved metal in the solid crystals of solvent, and by all the thermal difficulties that Nernst and Abegg have discussed. The fascinating question as to the condition of association or dis- sociation of the molecules of the compounds when melted or in solution also comes in when we attempt to interpret our tables, or, indeed, when we examine any freezing-point curve. But it is possible to study inter- metallic compounds without touching this question, and in the present report I have thought it best to do so. The vast subject of ternary and more complex mixtures has also been avoided as too complex for the present purpose, although Behrens, Stead, and especially Charpy, have made most interesting studies of such mixtures. I have to thank Mr. Heycock for continued assistance in drawing up this report. I have also to thank Mr. Stead and Professor H. Le Chatelier for valuable information and valuable references. Depression of the Freezing-point of the Metals Tin, Zinc, Bismuth, Cadmium, and Lead, caused by the Solution of Small Quantities of other Metals. The theoretical molecular depressions are calculated from the latent heat of fusion by means of the formula e 0" == O19 66 =0 x where @ is the freezing-point of the pure metal, 04 the depression,’and the latent heat of fusion. L2 148 REPORT—1900, TABLE I.—7Z%n as Solvent. Atomic Falls for a Concentration of under one Atom. Nickel . . 294 3 experiments. Silver - 293 2 =f Gold Bp PESEY Oy f Copper . é : ;: =. oo 2 - I Thallium . : : . 286 4 ; * \ Sodium : : - 284 2 Palladium . 2°78 4 experiments, Magnesium . ce rhate cAL a Lead ‘ ; . 276 8 a Zin wee A : . 264 4 me Cadmium’ . 243 3 experiments, II Mercury . 239 4 3 * ) Bismuth . 240 6 - Calcium ‘ . 240 2 A} III reat F “1 : - 186 5 experiments. * | Aluminium 5 TL 2b " Theoretical Molecular Depression = 3° ©. Taste II.—Zinc as Solvent. expts. concen, 1—3 atoms, Metal. hee ae Mean atomic Mean Mean atomic centage. percentage. depression. depression. Bismuth . : - ’ 0°386 0:2075 1:052° 5:07 Antimony é : : 0:799 0°4377 2247 5:13 eS fromcurve . 07500 0°500 2°60 (5°20) Lead : , ; 2 0°200 0150 0-78 5:20 Thallium . : r : 0:393 0°2595 1:285 4:95 Tinie, ; : ; : 1:187 0°655 3°497 5:34 Magnesium. : : 0-975 0 655 3572 5°45 Cadmium ; : - 1-464 0:732 3°377 4°61 Aluminium. ‘ : 0:99 0:99 4:10 (4:14) Theoretical Molecular Depression = 5:13° C., Taste III.— Bismuth as Solvent. No. of No. of atoms per Mean atomic ie experiments. 100 atoms Bi. depression. Lead ... - ; 5 : 20 1:1—1:'75 2:1 Thallium 2 0:3—0°9 2:07 M Mercury t 03—4:3 2°04 Tin 4 0'16—2'2 2°03. Steady. Palladium 4 0-9—2°2 2:03 Platinum 6 0:'2—1°2 2°02. Steady, Cadmium 4 1-0—4:0 2:01 Gold 4 0 4—1'8 LOT Sodium . ; 3 0:38—4:0 1:94. Steady. Silver . ; ; 3 0-7—2'5 9k Zinc 4 1:3—48 16 Copper . 5 0:23—0°6 1:23 Arsenic. 5 0:25—2°3 0-68. Very s steady. It is noticeable thas arsenic both in bismuth and cadmium gives + fall, Antimony . : : A 3 0:23—1'0 2-79. Rise. Theoretical molecular depression = 2:08° C, t ON THE CHEMICAL COMPOUNDS CONTAINED IN ALLOYS. 149 TABLE 1V.—Cadmium as Solvent. hee No. of No. of atoms per Mean atomic. de- experiments, 100 atoms Cd. pression. Antimony 2 0:3—0°5 4-71 M. Platinum . ‘ ‘ ‘ 2 0:08—0°13 4:55 F f 4 0:05—0°5 4:58 Bismuth fi ‘ 6 leh 3 2-2 -3-6 4-09 Tin 2 0'66—2°6 4:48 Sodium 3 0-6—1'3 4-44 Lead . 2 0:84—1°4 4-4. Thallium 3 0:24— 1:28 4:34 M. Copper , 8 0:2—2°0 3°5. No falling off. Mercury 3 0:23—0°68 2°77 Zine 3 0:06—1°6 2°72. No falling - off, Palladium 3 0:13—0 26 2°35 Potassium 2 05—0°6 2:26 M. Gold 3 0:14—0'7 1:48 Arsenic 1 0-2 16 Silver 1 0:05 9°33. Rise. Theoretical molecular depression = 4°5° C. Taste V.—Lead as Solvent. ; t es No. of No. of atoms per Mean atomic de- experiments. | 100 atoms of Pb. pression. Gold. 4 0:33—2°7 6°45. Steady. Palladium ; , 3 0°32—1°8 645 Silver . r i i 6 0-2—1°4 6°45 Platinum 4 0:15—0°6 6-42 Copper . : ; : 3 0-1—0:195 6°15 Arsenic : ory: ¢ 4 0°38—4'9 5°33 Magnesium . 2 15 4:56 Zinc 3 0:2—1:2 4:43 Antimony 4 0'6—4:7 3°9. Steady. Cadmium Fs : ‘ 2 0-6—6'1 3°62] Steady Mercury : : : : 3 0:73—6°7 3°31 | 3 Hg... Bismuth : é C 2 6 0:23—4'6 3°02) Steady. : 3 0-4—1'8 1:8 Tin e . . . . { D) 60—9:0 16 } t Sn,. Sodium ° : F ; 2 — 1:06 ? Theoretical molecular depression = 65° C. References. (‘) Heycock and Neville and Tin.’ 1894. (?) Heycock and Neville Chem. Soc.’ p. 914, 1892. ‘Comptes Rendus,’ exxx. p, 502. ‘Comptes Rendus,’ p. 585, 1892. ‘Comptes Rendus,’ p. 1470, 1887, (?) Lebeau . : ' (‘) Joannis , . ‘ () Debray . . . ‘The Freezing-points of Triple Alloys of Gold, Cadmium, ‘Trans. Chem. Soc.’ p. 986, 1891, and p. 65, ‘Isolation of a Compound of Gold and Cadmium,’ ‘ Trans. 150 REPORT—1900. (S) Le Chatelier . . ‘Sur les combinaisons définies des alliages métalliques.’ ‘Soc. d’encouragement pour l'industrie nationale,’ p. 388, 1895. (7) Stead. > . ‘Microstructure of alloys,’ ‘Metallographist, ii. p. 314. ‘Jour. Chem. Industry,’ xvii. 12, p. 3, and earlier numbers. (8) Osmond . : . ‘Comptes Rendus,’ exxiy. pp. 1094 and 1234. (®) Charpy . J . ‘Etude Microscopique des alliages métalliques.’ ‘Soc. dencouragement,’ p. 384, 1897; also ‘The Metallo- graphist,’ i. 2, p. 87, and ‘ Comptes Rendus,’ cxxiv. p. 957. (°) Gautier . ; . ‘Recherches sur la fusibilité des alliages métalliques.’ ‘Soc. d’encouragement,’ p. 4, 1896. (4) Heycock and Neville ‘Freezing-points of Alloys.containing Zinc and another Metal,” ‘Trans. Chem. Soc.’ p. 383, 1897; also ‘ Phil. Trans. A.’ clxxxix. p. 25, 1897, and Roberts-Austen, ‘R. Soc. Proc.’ 1900. ‘Ueber einige Higenthiimlichkeiten der Loéslichkeitscur- ven. ‘Zeits. Phys. Chemie,’ xxi. p. 557; and also ‘Comptes Rendus,’ cxxviii. p. 1444, (3) Paternoand Ampolla ‘Gazz. chim. ital.’ xxvii. p. 481, 1897. (1?) Le Chatelier (*) Le Chatelier . . ‘Les alliages métalliques.’ ‘Revue Générale des Sciences,’ xii. p. 537, 1895. (°) Kurnakov : ‘Sur les combinaisons mutuelles des métaux.’ (5) Bakhuis Roozeboom. ‘Erstarrungspuncte der Mischkrystalle zweier Stoffe’ ‘Zeits. Phys. Chemie,’ xxx. p. 385; Van Hyk, zbid. xxx, p. 430; Reinders, ibid. xxxiii. p. 494; Hissink, ibid. xxxili. p. 537. (27) Herschkowitz . . ‘Beitrage zur Kenntniss der Metallegierungen.’ ‘ Zeits. Phys. Chemie,’ xxvii. p. 123. (®) Laurie . : . ‘Chem. Soc. Trans,’ p. 104, 1888; ‘Phil. Mag.’ [5] xxxiii. p. 94. (7°) Galt : : . ‘B.A. Report,’ 1899, p. 246. (*) Tayler. : . Phil. Mag.’ July 1900. (#1) Heycock and Neville ‘ Phil. Trans.’ clxxxix. A. p. 67. (#2) Heycock and Neville ‘ Phil. Trans.’ cxciv. A. p. 201. () Myliusand Fromm . ‘Berichte der deut. chem. Gesell.’ xxyii. p. 630. (74) Roberts-Austen . ‘Metallographist,’ i. p. 342. Bibliography of Spectroscopy.—Report of the Committee, consisting of Professor H. McLeop, Professor Sir W. C. Roperts-AusTEN, Mr. H. G. Manan, and Mr. D. H. NaGEt. Tue work of collecting, verifying, and systematically arranging the titles of papers bearing on spectroscopy has been steadily carried on during the past year ; and the Committee ask to be reappointed for cne more year, with the intention of presenting to the Association at its next meeting the final instalment of the ‘Catalogue of Spectroscopic Literature,’ com- menced in 1870. It is proposed to end the catalogue with the present century, since the very satisfactory character of the proceedings at the last conference of the delegates appointed to arrange the compilation of an International Catalogue of Scientific Papers seems to warrant the conclusion that, as from January 1, 1901, the services of the Committee will be no longer needed, ABSORPTION SPECTRA AND CHEMICAL CONSTITUTION. 15) | Absorption Spectra and Chemical Constitution of Organic Substances.— Interim Report of the Committee, consisting of Professor W. NoEL Har they (Chairman and Secretary), Professor F. R. Japp, and Professor J. J. Dossiz, appointed to investigate the Relation between the Absorption Spectra and Chemical Constitution of Organic Substances. Four informal meetings have been held during the year, and, as much work is still in progress, it has been considered desirable that an interim report of that which has been completed should be presented. This consists of five communications published by the Chemical Society in their ‘ Transactions’ since March last. Two of these deal with the sub- ject of tautomerism and one with stereo-isomerism. The fourth is a study of ammonia and its derivatives, of hydroxylamine and oximes ; and the fifth an examination of some closed-chain compounds one of which contains two nitrogen atoms. Details of the measurements of the spectra are omitted from this report for the sake of brevity. In connection with the nitrogen compounds a brief abstract of a previous publication has been included. It is of interest because it leads towards the conclusion that there are two distinct classes of albuminoids, some of which have long been known to act as enzymes or soluble ferments towards the carbohydrates. Spectrographic Studies in Tautomerism. I. Absorption Curves of the Ethyl Esters of Dibenzoylsuccinic Acid.' According to theory, thirteen isomerides of diethyl dibenzoylsuccinate have a possible existence, but only three have so far been prepared and studied. On chemical grounds Knorr? regards one of the three as an enolic, and the other two as ketonic esters. He assigns to the enolic or a-ester the constitutional formula CPh(OH):C-CO,Et CPh(OH):C:CO, Et without deciding which of the three possible stereo-isomeric modifica- tions of this formula represents the substance examined by him. The two ketonic esters are structurally identical but configuratively different. To one of them, which he designates the para- or /3-ester, Knorr assigns the formula (a), and to the other, which he designates the meso-, anti or y-ester, the formula (0). H H | | CO,Et-C-COPh COPh:C:CO,Et (4) | (0) | COPh:C-CO,Et COPh'C-CO,Et | | H H } Hartley and Dobbie, Zrans. Chem. Soc., vol. 1xxvii. ? Annalen, 1896, 298, 70. 152 REPORT—1900. A mixture of the f- and y-esters is readily obtained by adding an ethereal solution of iodine to the sodium derivative of ethyl benzoy]- acetate, obtained by the action of metallic sodium on an ethereal solution of the ester. The two ketonic esters are readily separated from one another by fractional crystallisation. When either of them is treated with sodium methoxide, a yellow crystalline meal, consisting of the sodium derivative of the a-ester, is obtained. The aqueous solution of this substance, when treated with excess of dilute sulphuric acid at the freezing temperature, yields the a-ester, which separates as a thick oil possessing the colour of chlorine gas. The /3-ester, which was first described by von Baeyer and Perkin,! melts at 128-130°, the y-ester at 75°, and the former is less soluble than the latter in mostsolvents. Both esters are opticaliy inactive, the /3-ester by external, the y-ester by internal compensation, The ketonic esters are neutral to litmus, and practically insoluble in cold dilute alkalis. In their chemical properties they are exactly alike. The a-ester differs, both in physical and chemical properties, from the ketonic esters. It is an oily liquid, has a strongly acid reaction, and dissolves in cold dilute alkalis. It gives a characteristic dirty brown coloration with ferric chloride, which is not shown by the ketonic esters, and moreover is unstable, gradually passing into a mixture of the »- and y-esters at the ordinary temperature, the change taking place quickly at 130°, f the view put forward by Knorr as to the relation of the three esters to one another is correct, the - and y-esters should give very similar, if not identical, absorption curves, since stereo-isomerides which differ only in the configuration of their asymmetric carbon atoms so far as they have been investigated in essential oils and their hydrocarbons, are not found to differ either in the amount or the character of their absorption. The a-ester, on the other hand, having a different constitution, should exhibit a distinct series of absorption spectra. We have photographed and measured the spectra of alcoholic solu- tions of the three substances, and the results obtained entirely bear out the conclusions arrived at by Knorr on purely chemical grounds. The spectra of the ketonic esters are identical. The amount of absorption is considerable, all rays beyond !/\ 2795 being cut off by a layer 25 mm. thick of a solution containing 1 milligram-mol. in 100 c.c. of alcohol. There is also a well-marked band of selective absorption reaching from 1/X 3824 to 1/\ 4306 in a layer 3 mm. thick of a solution containing 1 milligram-mol. of the ester in 2500 ¢.c. of alcohol. This band is very persistent, and is still distinctly marked in a layer 4 mm. thick of a solu- tion containing only 1 milligram-mol. in 12,500 c.c. of alcohol. The spectrum of the a- or enolic form is quite different from that of the ketonic esters. The general absorption is greater, a layer 25 mm. thick of a solution containing 1 milligram-mol. in 100 ¢.c. of alcohol cutting off all rays beyond '/A 2171. The absorption band of the ketonic esters is altogether absent, whilst a well-marked band makes its appearance in a layer 5 mm. thick of a solution containing 1 milli- gram-mol. in 500 c.c. of alcohol between '/A 2546 and !/A 3148. This band quickly dies out, no trace of it being visible in a layer 4 mm. thick of a solution containing 1 milligram-mol. in 500 c.c. of alcohol. 1 Ber, 1884, 17, 60. ABSORPTION SPECTRA AND CHEMICAL CONSTITUTION. 153 The absorption curves for the ketonic and enolic forms are shown in the diagram on p. 156. When the solution of the a-ester was allowed to stand, and photo- graphs were taken after successive intervals of time, the transition from the enolic to the ketonic form could be clearly traced. After an interval of only three hours, the absorption band of the enolic ester had almost entirely disappeared, whilst the amount of general absorption had also appreciably diminished. Solutions containing 1 milligram-mol. in 100 and 500 c.c. respectively showed after forty-eight hours a great diminution in the amount of the general absorption, whilst after three weeks the curve coincided almost exactly with that of the 3- and y-esters, as shown on p. 155, The result of this investigation exemplifies the value of the spectro- graphic method, and shows how it might be applied with advantage to the investigation of similar cases of isomerism either to guide the chemical investigation or to confirm the conclusions drawn from it, especially when any doubt exists as to whether the isomerism is due to a difference in constitution or merely to a difference in the arrange- ment of the atoms in space. The amount of substance required for the experiments is small, and can generally be recovered again from the solu- tion. The esters were prepared by the method described by Knorr.! The preparation of the /- and y-esters offers no difficulty: the a-ester is only obtained when strict attention is paid to all the details given by Knorr. Two distinct preparations of each of the ketonic esters and three preparations of the a-ester were made. Each prepara- tion was photographed several times without any difference being ob- served in the photographs of the same substance. In the case of the a-ester the photographs were taken immediately after the completion of the preparation, as the change to the ketonic form sets in almost at once. II. A Study of the Absorption Spectra of o-Oxycarbanil and its Alkyl Derivatives.* The substance o-oxycarbanil, C;H,O,N, and its alkyl derivatives form a group of compounds which stand in the same relation to one another as isatin, carbostyril, and their respective alkyl derivatives. o-Oxycarbanil can be prepared by the fusion of o-aminophenol hydro- chloride with urea, or from its lactim ether by the action of concentrated hydrochloric acid.’ It can also be obtained by the distillation of o-amino- phenyl ethyl carbonate.‘ Two ethyl derivatives of o-oxycarbanil are known. One of these is prepared by boiling o-oxycarbanil for some time under a reflux condenser with equivalent quantities of ethyl iodide and alcoholic potash, the other by the interaction of o-aminophenol and ethyl iminocarbonate. The ether obtained by the first method is considered to be a lactam, that is, to have the ethyl group directly attached to the nitrogen atom, because on heating for some time with hydrochloric acid it takes up water and decomposes into carbon dioxide and the hydro- 1 Loe. cit. 2 Hartley, Dobbie, and Paliatseas, Zrans. Chem. Soc., vol, lxxvii. 3 Sandmeyer, Ber, 1886, 19, 2650. ‘ Bender, Ber., 1886, 19, 269. Scale of Oscillation Frequencies. oe Sees ez. oN Se Be es 7 eg taws nea ee 1/50 3 ua h I i fmt TTS CU A Uy —-—-- |}. BERERAEEAME cae IT a eB ae es Shee eee i A OD es es oe fee PRE fe 1/100 Proportional parts ot a milligram- a fol ict Lasky Well dts Nivth ll} an oleate ak Talal we | tal talc! eel aK ee rae 1/500 15 heed Hess lee We at 3t- {| OF ie et ei are he Py: . (cS) Pe i MR id WS Ff De Pia KT TAY Woe elo ll lal | Lebteiot st gos) Tat | keg y Curves of Molecular Vibrations. Ethyl a-, B-, and y-dibenzoylsuccinates. The curves for the B- and y-esters are identical, and are indi. eated by stars upon the line at points where measurements of the spectra were made, The curve of the a-ester is indicated by a. ABSORPTION SPECTRA AND CHEMICAL CONSTITUTION. 155 chloride of ethyl o-aminophenol. Its) structural formula is therefore CH. 00 + C,H, OH, This view is supported by the fact that it forms a well-defined compound with phenylhydrazine.! On the other hand, its direct formation from the lactim ether by the action of hydrochloric acid seems to point to the enolic or lactim structure as being the more probable. It is, however, now generally admitted that arguments based on chemical reactions are inconclusive in cases such as that under consideration, where shifting of a hydrogen atom may easily take place. 1 Bender, ‘loc. cit. ABSORPTION SPECTRA AND CHEMICAL CONSTITUTION. 157 The present investigation was undertaken with the view of ascertain- ing whether a comparison of the absorption spectra of the two ethers with the absorption spectra of o-oxycarbanil would, as in the cases of isatin and carbostyril,! yield results from which the constitution of the parent substance might be inferred. Assuming that one or other of the ethers differs from o-oxycarbanil only in the substitution of the alkyl group for an atom of hydrogen, the constitution of the two substances being otherwise identical, we should expect the absorption spectra of the parent substance and this ether to be practically the same. On the other hand, the ether which differs in constitution from the parent substance should give a different spectrum. Groenvik ? gives 136-138°, Sandmeyer 137°, and Bender 141°, as the melting-point of o-oxycarbanil. Although, apart from this slight difference, there was no reason to doubt the identity of the substances obtained by these chemists, we thought it well to ex- amine specimens prepared independently by two different methods and selected for the purpose, the substances obtained by fusion of o-amino- phenol with urea and by the decomposition of the lactim ether with hydrochloric acid. We found that the two specimens when heated side by side in capillary tubes behaved in exactly the same way, softening at 137° and melting completely at 139°5. Solutions of the two specimens gave identical spectra. The spectra of o-oxycarbanil and of the lactam ether are almost iden- tical. The amount of general absorption is practically the same in both, and the spectra of both substances show a well-marked absorption band occupying the same position and persisting, in both cases, through the same range of dilution. The spectra of the enolic ether, on the other hand, show a smaller amount of general absorption, and the absorption band does not appear until a much greater degree of dilution is reached than is required to bring out the band in the other two substances. The range of the band of the enolic ester is also very small. The above curves, drawn from the photographs, show very clearly the relations between the spectra of the various substances. The conclusion to which the investigation leads is that o-oxycarbanil has the same structure as the lactam or ketonic ether, or, at all events, that the lactam structure very greatly predominates, if the assumption is made that the parent substance in solution is a mixture of two tautomeric forms. It is worthy of note that in the three cases of this kind which have now been examined the parent substance possesses the ketonic or lactam constitution. o-Oxycarbanil, it may be noted, gives no colour reaction with ferric chloride. The substances used in this investigation were prepared exactly in accordance with the directions given in the papers already quoted. Two distinct preparations of each substance were made and several series of photographs were taken of the absorption spectra of each preparation. No appreciable difference could be detected in the various photographs of the same substance. This is satisfactory evidence of the identity of the compounds, and also of the purity of these particular preparations. ' Hartley and Dobbie, Zvans. Chem. Soc., 1899, 75, 640, ? Bull. Soc. Chim., 1876 [ii.], 25, 177. 158 REPORT—1900. The Absorption Spectra of Ammonia, Methylamine, Hydroxylamine, Aldoxime, and Acetoxime.} It was shown by L. Soret that commercial ammonia, even after many recrystallisations as sulphate, still shows an absorption band. Hartley and Huntington (‘ Phil. Trans.,’ 1879, Part I., 267) confirmed this observa- tion, and, believing the absorption to be due to traces of some constituent of gas-liquor, examined specimens of what was sold as ‘ volcanic’ ammonia of special purity for analytical purposes. Three separate samples were examined, each measuring half a gallon, with the result that all the rays beyond !/) 2638-2 (A 2747°7) were absorbed by the strong solution in acell 15 mm. in thickness. A very distinct absorption band was visible on diluting the liquid with eight volumes of water, and was still seen until sixteen volumes had been added. This result appeared remarkable in view of the fact that gaseous ammonia, at atmospheric pressure, in a tube 1 metre in length showed no selective absorption, and that ethylamine, even when solutions containing as much as 33 per cent. of the base were examined in cells 25 mm. in thickness, transmitted continuous spectra with very little absorption. Carbamide also showed no absorption band, but transmitted a con- tinuous spectrum.? a substance in which not merely one carbon is replaced by nitrogen in the benzene ring, as in pyridine, but two. It thus belongs toa group not previously examined. From the analogy between the constitution of this substance and that of pyridine, it was anticipated that it would show a marked selective absorption, and this anticipation proved to be correct. One of the principal reasons for examining a substance of this constitution lay in the fact that whilst pyridine contains the group ‘C:N: once in the benzene structure, dimethylpyrazine contains it twice, and the orginal formula proposed for cyanuric acid * contains it three times. Accordingly, if this formula were correct for cyanuric acid and its esters, we should expect that they would exhibit a powerful absorption band, more intense than that of pyrazine, just as that of pyrazine is more intense than that of pyridine. But it has been concluded, from a widely extended experience of the behaviour of such substances under the ultra-violet rays, and particularly from the results of a recent examination of the absorption spectra of its derivatives,® that cyanuric acid does not possess this structure, but one in which the acid is represented by a ring composed of ‘N:C:0 three 4 groups, a mode of single linking resembling that of a hydro- pyridine or of a hydroaromatic group with one carbon replaced by nitrogen ;° it should not therefore exhibit selective absorption. The specimen of dimethylpyrazine used in the experiments was pre- 1 Trams. Chem. Soc., 1896, 69, 177. 2 Hartley and Dobbie, 7rans. Chem. Soc., 1900, 77. Trans. Chem. Soc., 1898, '78, 598. B.A. Report, 1899. Trams. Chem. Soc., 1882, 41, 84. 5 Hartley, Proc. Chem. Sov., 1899, 15, 46. & Phil. Trans., Part II., 1885, 519 3 4 ABSORPTION SPECTRA AND CHEMICAL CONSTITUTION. 165 pared by the reduction of isonitrosoacetone in accordance with the directions given by Gabriel and Pinkus.! It boiled constantly at 154- 155° (corr.) under atmospheric pressure. Scale of Oscillation Frequencies. 93000, 2 s 4s 6 7 8 910001 2 5 4 8 ei iret | ) A hel es ell elt realleatiat 1 Milligram-molecule in 100 c.c Proportional thicknesses of liquid. || | | et ft iz iz EEE |_| @| a ——| a a |_| al fies | al ee enw Oh ad ae PT A iV PRA Sea 1 EN | a ae ASEM SNR RRM IAR A, ee et LH eset att | et tea = AR EH pea fae FR SE Ah Ch ahd ag 2: 5-Dimethylprazine. lin 500 c.c. A layer 25 mm. thick of a solution of dimethylpyrazine containing 1 mill.-mol. in 100 cc. of absolute alcohol cuts off all rays beyond 1/\ 2994. On reducing the thickness of the layer to 10 mm. an absorp- tion band makes its appearance, reaching from '/d 3064 to '/A 4821. This band is very persistent, and is still traceable in a layer 1 mm. thick of a solution containing 1 mill.-mol. of the substance dissolved in 500 c.c. alcohol. The band of dimethylpyr azine is thus both wider and also more persistent than that of pyridine. These results are shown on the curve above. Heaxamethylene.—In the paper already referred to, an account was also given of the absorption spectra of diketohexamethylene. Previous investigations had shown that piperidine? and hexachlorobenzene#* ' Ber. 1893, 26, 2206. * Hartley, Trans. Chem. Soc,, 1885, 47, 691. * Hartley, Zrans. Chem. Soc., 1881, 39, 153. 166 REPORT—1900. exhibit continuous absorption, but show no absorption band, and, as was to be expected, diketohexamethylene, in which the six carbon atoms are united with each other by a single bond, as in hexachlorobenzene and piperidine, likewise showed no bands in the spectrum. Through the kindness of Professor Sydney Young and Miss Fortey, we have recently been enabled to examine a specimen of pure hexamethy- lene prepared from Galician petroleum. This substance, in comparison with benzene and pyridine, is highly diactinic. A layer, 60 mm. thick, of a solution containing 1 mill.-mol. dissolved in 20 c.c. of alcohol, trans- mits all rays up to 1/A 3920, whilst a layer of the same solution, 10 mm. thick, transmits practically the whole spectrum. In none of the photo- graphs of the spectra of this substance could any trace of a banded struc- ture be detected. Tetrahydrobenzene.—Professor Young and Miss Fortey were also good enough to place a specimen of pure tetrahydrobenzene in our hands for examination. This substance exhibits somewhat greater general absorp- tion than hexamethylene, a layer, 60 mm. thick, of a solution containing 1 mill.-mol. in 20 c.c. alcohol absorbing all rays beyond '/A 3694, while absorption is still traceable in a layer of the same solution 1 mm. thick. Like hexamethylene, tetrahydrobenzene shows no selective absorption. The examination of these two substances thus confirms the conclusion pre- viously reached, that the banded spectrum is shown only by substances which possess the true benzenoid structure.! Ultra-violet Absorption Spectra of Albuminoids.? The first investigation of albuminoids of animal origin was made by Soret : it included albumen, white of egg, pure albumen, caseine, and serine. Absorption bands occur in their spectra in the following posi- tions :—Albumen (white of egg) A 2880-2650, pure albumen \ 2948-— 2572, caseine X 2948-2572. Serine exhibits a band similar to that of caseine. Inaddition to albumen the following substances have been examined :*— (1) Gelatine ; (2) maize starch ; (3) cane sugar ; (4) glucose ; (5) yeast water ; (6) invertase ; and (7) diastase. These are all highly diactinic substances, considering their complex constitution, and they show no absorption bands. It is evident, therefore, that the constitution of albumen, caseine, and serine is very different from that of invertase, diastase, gelatine, starch, glucose, and saccharose. This was of interest in connection with C. V. Naegeli’s theory of fermentation. Naegeli regarded fermentation as a process in which a transference takes place to fermentable matter of the molecular or rather intramolecular vibrations of the constituent substances entering into the composition of living protoplasm whereby the equilibrium of the molecules of the fermentable matter became so disturbed as to cause their resolution into simpler molecules. It appears by no means improbable that the diastatic ferments may have some such action. From this point of view 1 Hartley, Zrans., 1881, 39, 153. * Comptes Rendus, 97, p. 642; also Archives des Sciences Physiques ct Naturelles, x. p. 139. (L. Soret.) 3 Hartley, Zrans. Chem, Soe., 1887, 51, 59. ABSORPTION SPECTRA AND CHEMICAL CONSTITUTION. 167 it does not appear likely that a substance of the character of albumen, whose mode of vibration, as shown by its absorption spectrum, differs widely from that of the carbohydrates, could affect the latter, while on the other hand it is possible that the intramolecular vibrations of inver- tase and diastase night be communicated to saccharose and starch. That the sugars are highly diactinic substances is quite in character with what we know of their constitution and of the spectra of similarly constituted substances. It is of interest to learn that the albuminoid compounds associated with the carbohydrates are evidently different in constitution from those forms of albumen found in the animal organism. The probability pre- sents itself of these albuminoids being derived from the carbohydrates. Isomorphous Derivatives of Benzene—Report of the Convmittee, con- sisting of Professor H. A. Mirrs (Chairman), Dr. W. P. Wynne, and Dr. H. EK. ARMsrronG (Secretary). (Drawn wp by the Secre- tary.) THE existence of morphotropic relationships between the crystalline forms of substances which are not isomorphous in the formal sense of the term has of recent years acquired new importance, the purely geometrical work of Barlow ' and others having demonstrated the superfluity of the old view that the units of the crystalline structure are polymerides of the chemically active fundamental molecule as a means of explaining poly- morphism and kindred crystallographic phenomena, whilst Fock? has shown, from the study of the partition coefficients of two isomorphous substances in equilibrium in a liquid and a solid solution in contact, that in the case of salts, at all events, the molecular weight in the crystalline state may be that of the fundamental molecule. Moreover the work of Paterno * and others on the cryoscopic behaviour of substances possessing constitutions similar to that of the solvent indicates with certainty that isomorphism and morphotropy are phenomena which merge gradually one into the other. The consideration of facts such as these leads to the conclusion that morphotropy and isomorphism have a common cause, and that this is more likely to be discovered by the crystallographic study of substances showing morphotropic relationships than from the examination inerely of materials likely to exhibit isomorphism. The benzene series offers exceptional opportunities for the study of such questions ; indeed, it is remarkable that the publication of Groth’s important memoir,‘ calling attention to the existence of morphotropic relationships between benzene derivatives, has not acted as an incentive to really systematic work on the subject. The two investigations to be referred to form part of aseries which are being carried on in the chemical department of the Central Technical College, South Kensington, in order, as far as possible, to determine the effect on the crystalline form of certain definite changes in the composi- tion. The work will include the determination of the molecular volumes ' Proc. Roy. Dub, Soc., 1897, viii. 527. * Zeits. f. Kryst., 1897, xxviii. 337, * Gazzetta, 1895, xxv. 1, 411. 4 Poqg. Ann., 1870, 141, 31. 168 REPORT—1900, and of the melting-point curves of mixtures of the morphotropically related compounds. Morphotropic Relationships between Formanitide and its Substitution Derivatives. In order to determine the morphotropic effect of substitution upon the crystalline form of formanilide the simple anilides of the composi- tion C;,H;.NH (CO.X) (X=H, Me, Kt, Pr, &c.) as well as several of their alkyl derivatives, and also a number of the mono- and di-halogen derivatives, have been crystallographically examined by Mr. L. P. Wilson ; a list of the compounds measured is given in the accompanying table, in which the geometrical constants are also indicated. It is evident that a progressive change in the structural dimensions occurs as each series is traversed, although in most cases this only becomes obvious on rearranging the axial ratios, and sometimes on taking simple multiples of the ratios. The form in which the axial ratios are compared is indicated in the second column. Ts B. Formanilide . . . a:b: c=2188 :1:2403 9064 M Acetanilide ‘ ; » ¢€2:b%: a=2:0670:1:0°8488 90 O Propionanilide . ; » €36: a@=2:1665:1:1:0428 90 O Butyranilide . . . Ba:>6; 2¢e=2°1663.: 1 31-3788 90 O II Acetanilide . . . e2b: a=2-0670:1:0:8488 90 O Methylacetanilide . . 2620: a=0°7906 : 1208494 90 O Kthylacetanilide : - €206: a=1:0064:1:0°8401 90 O Propylacetanilide . a MeO a= 132648 108410: *90 O i GLUE P.-brom-formanilide . ; cc: 0) 2a=V 4100s = 2:2056 190 O is acetanilide . ~ @203 c=1°3904 2120-7159 90 x propionanilide . ba@:b: c=1:3400:1: 08948 90 O IV. P.-brom-acetanilide . 2 Gros ¢=1:3904 21% 0:7159 490 O 4 methyl acetanilide a:b: c=1'5546:1:09719 70 7 M 5 ethyl PY +. @:0: c=1:4063:1:1:5686 95 35 M Ve P.-chlor-acetanilide . . a:b: c=1°3263:1:0-6804 90 re) P.-brom i : » @:2b: e=1:3904:1:0°7159 90 M P.-iodo A 5 A @:b: c=1:4185:1:07415 9029 M VI. 2:4dichlor-acetanilide . a:b: c=08263:1:06828 77 33 M ,, chlorbrom-acetanilide a:b: c=0°8144:1:06722 7740 M . bromchlor A « @:6: =0:8214:1:0:7074 77 46° M ,, dibrom y - @:6: e=081381:1:06895 78 24 M In series 1, although the first member is monosymmetric, whilst the others are orthorhombic, a well-marked morphotropic similarity in the magnitudes of the ratio a/b is observed to follow the displacement of the hydrogen atom in the acidic group by Me, Et or Pr. The effect of dis- placing the aminic hydrogen atom by Me, Et or Pr is less, as is shown by ON ISOMORPHOUS DERIVATIVES OF BENZENE. 169 an inspection of series 2 ; in this case the ratio c/b is more nearly constant throughout the series than in the case in series 1. In series 3, obtained by displacing the acidic hydrogen atom in parabromoformanilide by either Me or Et, the ratio a/b again shows approximate constancy. No simple relationship is observable between parabromacetanilide and its methyl or ethyl derivative. Parabrom- and paraiod-acetanilide are isomorphous ; the corresponding chloro-derivative is not isomorphous with them, although it bears a marked morphotropic relationship to them.! Group 6 forms a well-marked isomorphous series. Otten? has observed that butyranilide is dimorphous, but has not examined the substance in great detail ; a study of this compound has shown that the dimorphism is of a very remarkable character. At ordinary temperatures the anilide separates from alcoholic solutions in large transparent crystals of pyramidal habit, which are distinctly orthorhombic, showing a characteristically orthorhombic interference figure of small optic axial angle. The axial ratios of such crystals are a:b :c=0'6920:1:0-6792. On preserving crystals which had been measured at a constant temperature of 8° to 11° they have been found to change gradually, and in the course of three months completely, into tetragonal crystals, without at the same time losing their brilliancy and transparency. The axial ratio a : c=0-6652 : 1 in these crystals ; they exhibit the characteristic uniaxial interference figure. On preserving the definitely tetragonal material at 30° for eighty days the reverse change occurs, the crystals becoming orthorhombic and biaxial, although the axial ratios never revert to quite their original values. The density of the orthorhombic form is 1-130, whilst that of the tetragonal form is 1:139. The molecular volumes of several of the anilides have been determined, with the object of examining the relations between the topic axial ratios of Muthmann ;* the ordinary axial ratios seem, however, in most cases to express the morphotropic relationships just as clearly as the topic ratios. Iso- and Poly-morphous substituted Benzene-sulphonic Chlorides and Bromides. It has already been stated * that the sulphonic chlorides and bromides derived from the 1:3: 4 dihalogen-benzene-sulphonic acids together form an isotrimorphous series. Dr. Jee’s further study of this group has led to important results. The series includes anorthic, orthorhombic, and monosymmetric terms, in the manner shown in the following table :— i} Orientation Crystallographic Systems | - ————— — | fo 1 | 5 4 | Anorthie | Orthorhombie | Monosymmetric | a SSS eee = | I.| cl | cl | S80,Br | stable | ae ue II. | Cl | Br | SO,Br {| stable -— —— DL Bes Cl SO, Br stable — . a= Wen eoresh bre) ;eSOsBn wi) Jabile> stable | — VecheBr | BES OsCl yas Gabile)=-aaml stable labile Wa.) sBr Cl S0,Cl | —- stable labile vil.| cl | Br | 80,1 aS labile> stable Vill. |; Cl | Cl | 80,Cl _ labile> / stable ) ' Compare Fels, Dissert., Leipzig, 1900. * Zits. f. Kryst. xvii. 391, 3 Zits. f. Kryst., 1894, xxii. 497. B.A, Report, 1899, p. 688. 170 REPORT—1900. Of these eight substances, three are stable in the anorthic system, three in the orthorhombic system, and two in the monosymmetric system. Change of the one form into the other has been observed in four cases (IV., V., VII., VIII.) on allowing the fused substance to cool on a microscopic slide ; the direction of the change in each case is indicated in the table by an arrow. A labile anorthic crystalline form of dibromo- benzene-sulphobromide (IV.) has been obtained from solution ; and it has been found that each of the four sulphochlorides (V.-VIII.) can be caused to crystallise in the alternative system by admixture with a sulphochloride which usually separates in that system. It has been possible to determine the symmetry of all the forms referred to in the table by crystallographic measurement, with the single exception of the labile anorthic form of dibromo-benzene-sulphochloride, but the existence of this form is indicated by the dimorphous change which occurs on cooling from the melting point to the atmospheric temperature. The detailed study of such a series of isomorphs—especially of the melting points of mixtures and of the conditions which determine the separation of the various crystalline forms-—will be of importance, as it is likely to furnish information of value in discussing the phenomena pre- sented by igneous rocks containing isomorphous minerals, The investigation has been extended by Dr. Jee to the corre- sponding derivatives of the 1: 3:5 dihalogen-benzene-sulphonic acids. The results obtained indicate the existence of an isodimorphous series having no apparent similarity with the 1:3:4 series. One of the members of this new series—1 : 3 : 5 dibromo-benzene-sulphobromide—has been obtained in two distinct crystallographic forms, both belonging to the monosymmetric system. At atmospheric temperature one of these forms is labile and isomorphous with the corresponding sulpho-chloride, and with 1 ; 3 : 5 bromo-chlorobenzene-sulphochloride. The stable form of 1: 3:5 dibromo-benzene-sulphobromide, on the other hand, is iso- morphous with 1 : 3 : 5 bromo-chlorobenzene-sulphobromide. The deriva- tives of the symmetrical dichloro-acid have not yet been satisfactorily measured. Even in their present incomplete form these results are of considerable importance as showing the manner in which the occurrence of polymor- phism may render obscure otherwise well-marked isomorphous or morpho- tropic relationships. Apparently a substance may crystallise in a whole series of different forms, A, B, C, D, the particular form obtained under ordinary conditions being the form stable at the temperature at which the crystals are grown. Another substance, the immediate homologue of the first in an isomorphous series, can also assume crystalline forms corre- sponding with A, B, C, D, &c., but the particular form stable at ordinary temperatures will not be the same as before, owing to the non-corre- spondence of the transition temperatures. Consequently the first member of an isomorphous series may crystallise in a form of type A, the second member in a form of type B, the third of type C, and so on, the isopolymorphism completely masking the isomorphism. ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 171 The Electrolytic Methods of Quantitative Analysis.— Sixth Report of the Committee, consisting of Professor J. EMERSON REYNOLDS (Chair- man), Dr. C. A. Koun (Secretary), Professor P. FranKLanD, Pro- fessor F. Crowes, Dr. Huca Marsuaui, Mr. A. E. FLETCHER, and Professor W. CARLETON WILLIAMS. Tue work of the Committee, appointed in 1894, has hitherto included a complete bibliography on electrolytic analysis up to the end of 1894 and experimental investigations on the electrolytic determination of antimony, bismuth, cobalt, nickel, zinc, and the separation of antimony and tin. The present report deals with further work on the determination of bismuth, and with the determination of iron, its separation from man- ganese, and the application of the electrolytic method to the determination of iron in organic products. These experiments cover some of the most important applications of electrolytic analysis which required further investigation, and the Committee propose to conclude their work with the present report. The more recent bibliography of the subject has been summarised by Neumann.! The Committee would also refer to Neumann’s book on electrolytic analysis,? which has been issued since their bibliographical report, and an English translation of which has been prepared by Kershaw ;% also to the annual reports on electrolytic analysis published in the ‘ Jahrbuch fiir Electrochemie.’ The Determination of Bismuth (Part II.) By Professor J. EMERSON Reynoups, D.Se., M.D., F.RS., and W. C. RaMspDEN. In a previous report (1896) it was shown :— 1. That carefully spun platinum dishes were better suited fer use as negative electrodes than any other of the various forms experimented with. _ 2. That irregular results only could be obtained with simple bismuth- nitrate solutions containing varying proportions of free nitric acid ; but that good determinations were more easily made in solutions of the sulphate when electrolysed by currents beginning at 0-08 and finishing at not more than 0-2 ampere. 3. That the best results were obtained in presence of metaphosphoric acid and of citric acid, both of which controlled deposition in a very ‘marked manner. 4, That citric acid is quite as effective as metaphosphoric acid and possesses the additional advantage that the metal can also be separated in satisfactory condition from ammoniacal solutions of the citrate. _ Two questions remained for consideration, viz. (a) the separation of bismuth from strong but simple solutions, and (b) from solutions con- taining other metals. ' Chem. Zeits. 1900, 24, 455. * Theorie u. Prawis der analytischen Electrolyse der Metalic, 1897. * The Theory and Practice of Electrolytic Methods of Analysis, 1898. 172 REPORT— 1900. The work under the first head was in progress at the time the former part of the report was published by one of the present writers and Mr. Bailey, and was subsequently carried as far as seemed desirable. The results obtained with moderately strong solutions of bismuth were very unsatisfactory, even in presence of much citric acid and when treated with all the care indicated by our former experience. We then proceeded to determine the major limit of concentration at which good determina- tions can be made. Taking 150 e.c. as the most corvenient volume for use in the electro- lytic capsules employed, we found that excellent results could be obtained in presence of 2°5 gr. of citric acid, so long as the weight of metal in 150 c.c. did not exceed 0:22 gr. With stronger solutions we failed to obtain satisfactory reguline deposits, even when the proportion of citric acid was increased and the current at the commencement of the operation was reduced to 0:005 ampere, so that the rate of deposition should be very slow. We therefore arrived at the conclusion that 150 c.c. of bismuth solution should not contain more than about 0:22 gr. of metal in the form of nitrate or sulphate, and that 2°5 to 3:0 gr. of pure citric acid suffice to control the deposition, provided the initial current used and acting for some hours be about 0:01 ampere, increased at the end, and for a short time, to 0°15 or 0-2 ampere. Separation of Bismuth from other Metals. Extended experience in the electrolytic determination of bismuth in simple solutions of varying strength led us to doubt that the purely electrolytic separation of the element from other metals would prove satis- factory. The results obtained by the present writers have justified this anticipation. The least unfavourable determinations of bismuth in such mixtures with other metals as would probably be met with in practice were those obtained with cadmium and zinc ; but even in these theoretically favour- able cases it was found that, however feeble the currents used, the deposited bismuth carried down sensible amounts of the much more positive metals. The method of experimenting was as follows :— A carefully measured volume of a bismuth-nitrate solution known to contain 6-018 gr. of metal per litre, in the form of nitrate, was placed in a platinum capsule. The special treatment to be applied in each case was then carried out ; pure citric acid added, the solution diluted with water to about 150 c.c., and a current passed through the liquid of such strength (generally 0-01 ampere) as to secure a good reguline deposit of bismuth. The whole of the metal was seldom separated under fifteen to twenty hours, and was hastened at the end by passing a current of about 0-1 ampere fora short time. The contents of the capsule were then washed with water and alcohol, and the vessel] dried and weighed. Of the experiments recorded below, the first three aimed at fixing the degree of accuracy with which bismuth could be electrolytically separated from the particular simple nitrate solution used in presence of citric acid. The citric acid used in work of this kind should be tested for lead, &e., before use, as samples are sometimes met with which contain metallic impurities. The total volume of liquid used was the same in these as in all other cases, viz. about 150 c.c. ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS, L¥3 Experiment A, 0:2407 gr. of bismuth in solution + 3 gr. of citric acid gave after eighteen hours a fairly firm reguline deposit, which weighed 0:2382 gr. Experiment B. 01805 gr. of bismuth gave under the same conditions a perfectly tirm deposit weighing 0°1807 gr. Experiment C. 0:1805 gr. of bismuth with 2°5 gr. of citric acid gave an excellent deposit of 0°1804 gr. The concentration of the solution in experiment A was too high, as already pointed out ; but the results obtained in the weaker solutions used in B and C were as good as could be obtained in any determinations of this class. The effect of the addition of sulphuric acid is shown in the next three experiments. Experiment D, 0°1805 gr. of bismuth in solution with 0°5 ¢.c. of pure freshly distilied H,SO, and 2 gr. of citric acid gave, after twenty hours, as good a deposit as in B, and weighed 0°1807 gr. HLeperiment EF. 0°1805 gr. bismuth with the same volume of H,SO,, but with 4 gr. of citric acid. The metal came down very slowly from solution, but in good condition, even when a stronger current was used for a longer time than usual: at the end the weight obtained, after twenty-six hours, was 0°1801 gr. The proportion of citric acid used was therefore needlessly large. Experiment F. 0:1504 gr. of bismuth in solution, 1 ¢c.c. of H,SO, and 2 gr. of citric acid gave a good deposit, which weighed 0:1507 gr. Therefore good results can be obtained in presence of much more free sulphuric and nitric acids than would probably be present in actual analysis, or could be separated from mixed sulphates. _ In the remaining tests cadmium or zinc salts were present. Haperiment G, 0°2106 gr. of bismuth in solution, 1 ¢.c. of H,SO,, 2 gr. of citric acid, and 0-125 gr. of cadmium in the form of sulphate. Result : 0:2687 gr. The deposit easily oxidised and contained some cadmium, though the current was kept as low as possible throughout. Haperiment H, 0°2106 gr. of bismuth in solution, in all respects as last, gave 0°2986 gr. of deposit containing cadmium. Experiment I. 0:1805 gr. of bismuth as last, except that only 0:5 c.c. of H,SO, was added, gave a fair deposit, but contained cadmium and weighed 0-2096 gr. Experiment J. 0:1925 gr. bismuth ; treated solution as last, but with 4 gr. of citric acid, gave 0:2340 gr. deposit, easily oxidised as in the other cases, and cadmium was found in the film. The results with zinc were similar; for example :— Experiment K. 0:1504 gr. bismuth ; the solution containing zinc in the form of sulphate instead of cadmium, 0°5 ¢c.c. H,SO, and 2 gr. of citricacid. The metal separated in fair condition, but was easily oxidised ; it weighed 0:1642 gr. and contained traces of zine. Experiment L. 0'1805 gr. bismuth as last, and with zinc sulphate, gave 0°1851 gr., and contained zinc also. Therefore, while bismuth can be determined electrolytically with accuracy in simple and dilute solutions containing citric acid, and even relatively large proportions of free nitric and sulphuric acids, we are unable to recommend its electrolytic separation from any of the metals with which we have experimented. 174 The best course, in our opinion, is to separate the bismuth’ by any of the well-known methods in the form of hydroxide, to dissolve the latter in sufficient nitric acid, and, after necessary dilution with addition of citric acid, to electrolyse, with the precautions already described. The Determination of Iron. By Cartes A. Koun, W.Sce., Ph.D. Bibliography. Author / Journal Year | Volume / Page Composition e | 5 Eemeiye | | denacniae oxalate. | Avery, S., and | Ber 1899 | 382 64 | | Sodium citrate. Dales, B. |) Ammorium meta- | phosphate. Avery, S., and | Ber. | 1899 82 2233 | Ammonium oxalate. Dales, B | Brand, A. . | Zeits. anal. 1889 28 581 | Sodium pyrophos- | Chem. | phate and ammo- nium carbonate. Classen, A., | Ber. 1881 14 1622 Ammonium oxalate. and Reis, | M.A. Classen, A. Ber. 1894 27 2060 Potassium and am- monium oxalates. Gibbs, W. Amer. Chem. 1891 13 570 Sulphate; as amatl- J. gam. Heidenreich, | Ber. 1896 29 1585 Sodium citrate and M. citric acid. Kohn, C. A., | J. Soc. Chem. 1889 8 256 Potassium and am- and Wood- | Ind. monium oxalates. gate, J. | Kollock, L. G. J.Amer.Chem.| 1899 21 911 Sodium citrate and Soc. citric acid. Luckow, C. Zeits. anal. 1880 19 1 Ammonium citrate Chem. and citric acid. Moore, T. Chem. News 1886 53 209 Phosphoric acid. Tartaric acid and Nicholson,and| Amer. Chem. | 1896 | 18 654 pee ey Avery, &. J | Borax and ammo- nium oxalate. Parodi, G., | Zeits:. anal. | 1879 | . 18 587 Acid ammonium and Mascaz- Chem. oxalate. zini, A. | Riidorff, F. Zeits. angew. | 1892 _ 197 | Ammonium oxalate. Chem. Thomiilen, H. | Zeits. Electro- | 1894 1 304 Ammonium oxalate. chem. Smith, E. F. | Amer. Chem. | 1888 10 330 Sodium citrate and : citric acid. Smith. E. F., | J. Analyt. & | 1891 5 488 Tartaric acid and and Muhr, F App. Chem. | ammonium hy- | drate. Verwer, H., | Ber. 1899 32 806 Ammonium oxalate. and Groll, F. / Vortmann, G. | Monatsh. ; 1893 | 14 536 Sodium potassium Chem. | tartrate and so- dium hydrate. Wolman, L. . | Zeits. Hlectro-| 1897 3 542 | Ammonium oxalate. chem. ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 175 The electrolytic methods for the determination of iron can in no way be regarded as comparable with the usual volumetric and gravimetric methods in their general applicability. Under special circumstances, how- ever, they may be found advantageous, especially in the determination of relatively small quantities of iron in organic products, an application which has been specially studied in the subjoined experiments. Of the various methods proposed, that in which the metal is deposited from a solution of the double ammonium oxalate, first suggested by Parodi and Mascazzini, and subsequently worked out by Classen, is the most reliable. When separated from a citrate or tartrate solution, the precipitated iron contains a considerable proportion of carbon, and the deposition from phosphoric acid or ammonium pyrophosphate solution is too slow to be of practical value ; further, it necessitates a high current density, and the introduction of phosphates into the solution is an obvious disadvantage from an analytical standpoint. The experiments have therefore been restricted to the investigation of the deposition of iron from the solution of the double ammonium oxalate, They may be conveniently grouped under the following heads}:— l. The conditions under which iron is deposited from ammonium oxa- late solution and the most favourable conditions for its electrolytic deter- mination. 2. The influence of ammonium chloride on the electrolytic determina- tion of iron. 3. The complete separation of the iron when deposited from ammonium oxalate solution : the sulphocyanide reaction for iron under the conditions of the experiments. 4. The presence of carbon in iron deposited from ammonium oxalate solution and the determination of its amount. 5. The electrolytic separation of iron and manganese in ammonium oxa- late solution. 6. The electrolytic determination of iron in urine and other animal pro- ducts. 1. The Conditions under which Iron is deposited from Ammonium Gxralate Solution, and the most favourable Conditions for its Electrolytic Determination. By Cuaries A. Koun, M.Sc., Ph.D., and H. H. FRroysstt. Classen recommends the addition of 6 to 8 gr. of ammonium oxalate per gr. of iron in 150-175 c.c. of solution, and conducts the electrolysis with a C.D.;9) of 1:0 to 15 ampere and 3 to 4 volts ina warm solution (40°-60° C.). Nitrates, if present, must be removed by repeated evapora- tion with sulphuric or hydrochloric acid; free sulphuric acid can be neutralised by ammonium hydrate ; any free hydrochloric acid is prefer- ably removed by evaporation on the water-bath. The complete deposition of the iron is tested with potassium sulphocyanide, after acidifying with hydrochloric acid ; 0:2 to 0:3 gr. of iron is deposited in three to four hours. In a later paper Classen states that the most favourable condition for the deposition of iron is with a current N.D.,99=1-5 ampere at the ordi- nary temperature. Neumann! adds that weaker currents (0:3 to 0°5 ampere) ean be used, but then a larger proportion of ammonium oxalate must be Theorie u: Praxis der analytischen Electrolyse der Metalle; p. 114, 176 REPORT—1900. added and the current increased to 1:0 ampere at the end of the determina- tion to ensure the precipitation of the last portion of the iron. According to Wolman, eight to ten hours are necessary for the deposition of 0:15 to 0:30 gr. of iron with a C.D. ,59=0°3 to 1:0, and finally to 1:5 ampere, and an E.M.F. of 4 volts at 50° C. The majority of the results recorded by this method are slightly low, on an average 0:2 to 0-6 per cent. on the weight of iron taken. Variations in current and in the proportion of ammonium oxalate added constitute the only real differences in the conditions of deposition recommended, and they bear on the one practical difficulty of the method— the prevention of the separation of any ferric hydrate during the electro- lysis. As pointed out ina previous report (1896) on the electrolytic de- termination of tin in ammonium oxalate solution, the electrolyte gradually becomes alkaline, owing to the decomposition of the oxalate and the for- mation of ammonium carbonate ; in presence of a sufficient excess of ammonium oxalate the iron will still remain in solution after the latter is alkaline, but otherwise ferric hydrate separates out and oxalic acid must be added from time to time during the electrolysis to redissolve it. Such addition of oxalic acid renders it necessary to watch the experiment ; a further drawback is that the quantity of ammonium oxalate solution necessary leaves little room for any further addition of liquid in an ordi- nary dish of 175 c.c. to 200 c.c. capacity. Hence the ammonium oxalate must outlast the deposition of the iron if an addition of oxalic acid is to be avoided. A series of experiments were, therefore, first arranged in which the time necessary for the solution to become alkaline, the proportion of metal deposited up to alkaline reaction, and the proportion subsequently deposited, were noted. A ferric chloride solution of known strength was used, made up from pure ferric oxide, the method of working being as follows :—The slight excess of hydrochloric acid in the measured portion of the solution was first neutralised with a few drops of ammonium hydrate, oxalic acid solution added to acid reaction, and the whole then added to the ammonium oxalate solution. The additional oxalic acid recorded was either added to the original solution or at intervais during the electrolysis. The current density, C.D.,99=1:0 to 1:5 ampere, and electromotive force of 3:5 to 4:0 volts employed in these first experiments are the values hitherto regarded as the most favourable for the deposition of iron. Both warm and cold solutions were tried. The ammonium oxalate solution contained 40 er. per 1.000 c.c. ; the oxalic acid solution 80 gr. per 1,000 c.c. Platinum dishes of about 200 c.c. capacity were used as the cathode and bored platinum discs as the anode ; the circuits and measurements were arranged as described in the Committee’s third report (1896). The following results illustrate the conclusions to be drawn from this series of experiments :— Series I. In experiments 1, 2,3, 4, and 5, 10 c.c. of oxalic acid solution were added to the solution prepared as stated above and the electrolysis continued until the mixture became alkaline, when the current was broken and the deposited metal washed, dried, and weighed in the usual manner. The solution became alkaline very quickly when electrolysed warm, but on an average about 25 per cent. of the total iron was deposited in this short period of fifteen to twenty minutes. Although alkaline, no separation of ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 177 ferric hydrate took place up to this stage, there being sufficient ammonium oxalate left to keep the iron salt in solution. In experiments 6 and 7 a larger proportion of oxalic acid solution (50 c.c.) was added to the original solution, which allowed the electrolysis to be continued for 15 hour before alkalinity was reached ; the rate of deposition is evidently slowed by this increase of free acid. When cold solutions are electrolysed the deposition is quicker, as shown in experiments 8 and 9 ; the larger pro- portion of metal deposited is also partly due to the somewhat higher current and E.M.F. employed, and, taking this into account, the solution takes longer to get alkaline when electrolysed cold, as would be expected, since the rate of the decomposition of the oxalate will be slower. A comparison of experiments 5 and 8 with the remainder shows that, with less iron and the same proportion of oxalate, there is an increase in the proportion of iron deposited, despite the retarding effect of the | if | | Ammo- Oxalic | Tron Tron de- |Per cent. | en Ee | Tem- ; d : Oxalate | Solu- |C.D.49)| E.M.F. No. | taken, posited, nor der Time Solution | age ness! | Volts. Peta: gr. gr. posite added, added, jure C.c. C.c. 1 |0:0970 0:0415 42-8 |14 min, 125 10 1:5 3°8 50° 2 00970 0:0300 20:9) ies 125 10 | 15 3°8 50° 3 0:0970 0:0270 Pap Maly Fe, 125 10 15 4:0 50° 4 |0:0970 0:0230 23:7) |) WO ys 125 10 16 39 50° 5 |0-0194. 0:0130 67:0 |20 ,, 25 10 1-4 4:0 50° 6 0:0970 ee 42°3 1y hr. i 50 |1:4-1'2'3-9_4-3 50°_56° 7 |0:0970 0:0410 | 42°3 /12 ,, 25 | 50 |1:4-1:1|3-9_4-5'50°_56° 8 00194 Goren aon |se neal, ge) | to | acl £e dem 9 00970 | 0-0790 81-4 | 14 hr. 125 50 {15-18} 4:7 | Cold 10 |0'0970 | 4.00300} @.30'9 |13 ,, 1) fs | : a [ . 00630! b.650 1° f 125 | 50 |1-4-13'3-9-4'3'50°_53° | «+ 00-0920 95-9 | | | | 11 |0:0970 (| a. 0-0410 @.42°3 |1h.10m.}] 125 | 50 |1:5-1:8) 4:8 Cold | 5.00520) 6.536 |Lhr. | | | a+00930) 959 | | i relative increase of free oxalic acid present. In experiments 10 and 11 the solutions were electrolysed till alkaline, and the deposited metal weighed (a) ; the solution was then poured back into the dish, and the electrolysis continued until a precipitate of ferric hydrate separated, when the additional iron deposited on the cathode was weighed (4). The deposition in both warm and cold solutions proceeds more rapidly after alkalinity than before, and there is evidently little difference in the results of the two experiments. Tt is clear from these results that 5 gr. of ammonium oxalate will not outlast the deposition of 0-1 gr. of iron under the above condi- tions of current and E.M.F. ; further, that an initial acidification with oxalic acid up to 4 gr. is no real help in preventing a separation of hydrate ; and, finally, that it is advantageous to electrolyse cold solutions in preference to warm. To complete the deposition of iron under these circumstances it is necessary to add oxalic acid from time to time durin the expen so as to prevent the separation of ferric hydrate ; if this . N 178 REPORT—1900. is done, accurate results can be obtained, our own determinations, which need not be detailed here, confirming those of previous experimenters. The continuous attention thus entailed of course robs the method of its practical value. Experiments were made on the use of acid ammonium oxalate instead of the neutral salt as the electrolyte, and it was found possible to complete the electrolysis without the addition of oxalic acid, 6 gr. of the acid salt being added to 0-1 gr. of iron as ferric chloride. But there is always a risk of ferrous oxalate separating out from this solution after the ferric salt has been reduced, which is extremely difficult to redissolve, so that the conditions of deposition were not regarded as worth further study. By working with a lower current density and allowing the electrolysis to proceed for six hours, or preferably overnight, in cold solutions, it was found that 5 gr. of ammonium oxalate will outlast the deposition of 0-2 gr. of iron, and these conditions afford a thoroughly satisfactory method for the electrolytic determination of iron. The metal is deposited in a steel-grey, coherent form, and adheres equally well to a polished or sand- blasted dish ; the washing and drying can be done without any fear of oxidation. After some preliminary experiments it was found that a C.D.;o9 of 0-4 to 0-5 ampere and an E.M.F. of 3-0 to 3-5 volts are best ; from five to six hours are necessary for the deposition of 0-1 gr. of iron. The following experiments illustrate the results to be obtained under these conditions ; a ferric chloride solution was used, the excess of free acid being first neutralised as in Series I. Nos. 8-12 were consecutive experiments. Serres IT, Tron Tron de- ae C.D ELF T | 5 xalate Solu- Dy, ).M.F. | Time, | | No. Cee noe tion added, | Ampere | Volts “Hours, Hewes eo | (ores | ee == —— _———$_= ae = io 1 | 01060 | 06-1060 125 | 0-42-06 | 31-30] 5 Bi 2 01060 01064 = | 125 0-4 -0°6 3°2-3'0 6 | — 3 0:1060 0°1066 125 0-4 ~0°6 32-30 Le) — 4 | 01060 01065 | 125 0:3 —0'29 | 2°8-2'9 — Overnight 5 | 01060 0°1065 125 OBA) i Gwe ey, | ? 6 | 01060 01065 | 125 OE a ar ae 7 | 01060 01062 | 125 O:3 -D:2o) |S ae stp 3 LS 0:0920 0:0920. | 125 0-4 -—0°32 | 2°3-2°6 17 Pe 9 071840 071840 125 O38=0r02 | eoneore 143 a 10 0°1050 0-1050 125 0-4 —0°36 ‘| 2°0=2°5 18 | +3 11 | 0:0920 | 00919 | 125 056-0955" 5302875 81 A 12 | 0:0920 0-0919 125 05 —0°5 28-28; 18 | a Note.—The two figures for Current and E.M.F. indicate the measurements at the beginning and end of the determinations respectively. Considerable latitude is permissible in the current density and E.M.F., but it should be on the low side of the values given above. The deter- ‘minations require no watching, and by allowing them to proceed overnight one of the most marked advantages of electrolytic analysis is gained. Experiments made under similar conditions in warm solutions indi- ‘cated no advantages whatever ; the rate of deposition is not increased, and there is always greater risk of ferric hydrate separating out, as already explained ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 179 2. The Influence of Ammoniuin Chloride on the Electrolytic Determination of Iron. Since any iron solution in the ordinary course of analysis is likely to be acid with hydrochloric acid, a few experiments were made to decide whether the ammonium chloride formed by neutralising it has any deterrent effect on the deposition of the metal, since Classen states that it is desirable to remove free hydrochloric acid by evaporation previous to the electrolysis. 1 gr. of ammonium chloride was added to each of the solutions electrolysed under the conditions tabulated below ; from the results it is evident that the addition is without influence on the determination of the iron. Series ILI, Ir Ammonium | ti von | Iron deposited, | Oxalate Solution | C. Doo E.M.F. Time, No. | a, | gr. added, | Ampere Volts Hours parte. = cc. | goes | | | : = o 1 | 0:1060 0°1058 125 0:5-0-4 | 35-36 | 5 2 0:1060 0:1063 | 125 05-04 | 3:5-3°6 5 3. The complete Separation of the Iron when deposited from Ammonium O.alate Solution: the Sulphocyanide Reaction for Lron under the conditions of the Experiments. By Cuartus A. Koun, M.Sc., Ph.D., F. J. Bristyn, and H. A, FROYSELL. The apparent accuracy of the results obtained in the electrolytic deposition of iron from ammonium oxalate solution has led the method to be regarded as free from the source of error generally associated with the deposition of metals from solutions of organic salts, viz. the separation of carbon with the metal at the cathode. Citrate and tartrate solutions both yield deposits containing a considerable proportion of carbon, and the quantitative results obtained are correspondingly high. Our own results with ammonium oxalate solution, contrary to those recorded in the litera- ture on the subject, are hardly ever on the low side ; they average from 0-2 to 0°3 per cent. high (Series II. p. 8). The possibility of com- pensating errors consisting in the presence of carbon with the deposited metal on the one hand, and the incomplete separation of the iron on the other, has recently been discussed by Avery and Dales! and by Verwer and Groll.2- The former find that the deposited iron does contain carbon, on anaverage 0:21 to 0°42 per cent. on the metal deposited, and that some iron remains in the electrolysed solution. The latter was determined gravi- metrically after evaporating the solution and igniting the residue, and in the three experiments made averages 0°35 per cent. The results published from the Aachen laboratory, on the other hand, confirm Classen’s original view, that there is no carbon with the deposited iron, and that the iron is completely precipitated. Eight experiments are given by Verwer and Groll ; the results are all low, a total of 7:6 mgr. of iron being wanting in the eight experiments. Still, no iron could be detected on evaporating all the solutions left after the electrolysis together, anda testing with potassium sulphocyanide or other reagent after ignition and solution. These ‘experiments were conducted with warm solutions, with a C. D.,o5 Ber. 1899, 82, 64 and 2233. ® Ber. 1899, 32, 806. N 2 180 REPORT—1900, =1-0 ampere, an E.M.F. of 2°5 to 3:0 volts, and the addition of 8 gr. of ammonium oxalate for 0-1 to 0:3 gr. of iron. From the contradictory nature of these results it became important to ascertain whether the accuracy of our own determinations was really due to small compensating errors. To test the complete deposition of the iron in the experiments in Series II. (p. 178) a small quantity of the solution was withdrawn by a capillary tube, and tested with potassium sulphocyanide after acidifying with hydrochloric acid. The reaction is, however, known to be inhibited by the presence of organic acids, such as oxalic, unless a large excess of hydrochloric acid is present to prevent the dissociation of the ferric sulphocyanide ; this addition may so far dilute the solution as to prevent the detection of small quantities of iron. Further, the metal is present as a ferrous salt at the end of the electrolysis, and this fact may also be a cause of any iron present escaping detection. The delicacy of the sulpho- cyanide reaction was, therefore, carefully studied under the conditions of the electrolytic experiments, as well as in presence of ammonium oxalate and of oxalic acid. Our results show that whilst up to 0:4 mgr. of iron can readily escape detection when the test is made by the usual method of withdrawing cnly a little of the solution, 0-1 mgr. can always be detected with certainty if the whole of the solution, after electrolysis, is tested by acidifying with 75 c.c. of hydrochloric acid (conc.), and then adding 10 c.c. of a 20 per cent. solution of potassium sulphocyanide. The coloration is quite distinct in presence of ammonium oxalate, oxalic acid, ammonium chloride, or of the salts remaining after the electrolysis of the mixture of these salts as used in the deposition of iron under the conditions of the experiments in Series II. The sequence of the addition of the reagents in no way affects the delicacy of the reaction, nor is the addition of any oxidising agent, such as hydrogen peroxide, necessary to convert the ferrous into ferric iron when solutions containing oxalic acid or its salts, or the products of their electrolysis, are tested ; in their presence a little stirring appears ample to completely oxidise small quantities of iron. As a matter of fact, less than 0-1 mgr. can be detected thus, but this limit is of course sufficient to check the presence of iron left in the solution after electrolysis. With this check on the complete deposition of the metal a series of determinations were made, in which the iron remaining in solution was determined colorimetrically by potassium sulphocyanide after the electrolysis. Series IV. w |] ] . ; ’ | | Tron left No Iron taken, | an op: | C.Diio0 ‘.M.F. | Time, |} in solu- ane gr. pes - } Ampere Volts | Hours tion, ES: mgr. ] 0:1036 | 01036 | 05—0-42 34-37 23 O1 | 2 | 01558 0:1550 O5—045 | 23-3:0 | 23 0-2 3 | 0°2590 0'2592 0'5 + 0°46 oi —37 || 28 03 ! The above were three consecutive experiments made with a ferric chloride solution prepared for electrolysis as in the previous experiments, and to which 5 gr. of ammonium oxalate were added. Despite the prolonged time of electrolysis a little iron still remained in solution ; other ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 181 results showed the presence of 0°2 to 0°35 mgr. of iron in the electrolysed solution. Nevertheless, as in the experiments of Series II., the error in the weight of iron deposited is on the plus side. 4. The Presence of Carbon in Iron deposited from Ammonium Oxalate Solution, and the Determination of its Amount. By Cuartus A. Koun, M.Sc., Ph.D., and F. J. BrisLer. To ascertain the presence of carbon in the metal deposited under the above conditions the following method was adopted :—A solution of ferric chloride, neutralised with ammonium hydrate, and to which ammonium oxalate was added, was electrolysed under the usual conditions, a piece of platinum foil being employed as the cathode. After the electrolysis the foil was thoroughly washed, then dried, and rolled up for combustion. The combustion was carried out in an ordinary combustion tube in a eurrent of oxygen, a solution of barium hydrate being used for the absorption of the carbon dioxide. In every case a blank experiment was conducted for one hour before the introduction of the deposited iron, and the absorption bulbs weighed both at the beginning and end of the blank experiment ; no difficulty, however, was found in keeping out all traces of carbon dioxide. The results tabulated below leave no doubt as to the presence of carbon in the deposited metal ; the quantity appears to be independent of the quantity of iron precipitated, but increases with the quantity of ammonium oxalate in the solution electrolysed, when this is completely decomposed. The results are likely to err on the low side, as the combustion of the carbon deposited with the iron is likely to be incomplete. In order to make sure that the carbon dioxide was not derived from any slight residues that might have adhered to the iron from the alcohol used in the washing of the deposit, this washing was omitted in experiments 3 and 4, and the precipitated metal dried in vacuo after washing with water. Further, in experiment 4 the deposited iron, which was beautifully crystalline, was detached as far as possible from the platinum, and this portion (a) very completely washed with water before drying, so as to be certain that the carbon did not arise from any adhering traces of the decomposed oxalate solution ; the iron that still remained on the platinum was combusted separately (0). Series V. Per cent.| Ammon- No peat fe. moa Carbon |ium Oxa-| Time, | C.D.yoo [E-M-F.! Romarks 3 P a Sees Tron late Hours} Ampere | Volts | gr. | ©" ‘deposited! added 1 00814 | 060 O74 | Ggr. | 19 0-4 5:2 | ( Washed with | | water and | i) o1908 | 082 043 | Ger. | 212 | 02 | 55 || alcohol | 3 071220 | 0-76 0°62 6 gr. 19 02 3:0 4 {| % 00674 | 055 | 0-82 ] | bs samen eet aes Wee leo. | bISer. | 48 hee aioe dried in @+b03230 | 2:02 | 0-62 j abkiie The variations in current density and electromotive force do not seem to make any appreciable difference. On an average the iron: deposited from a solution containing 6 gr. of ammonium oxalate contains 0°84 mgr. of carbon, and, therefore, proportionately the results recorded in Series II. 182 REPORT—1900, and IV., in which 5 gr. of ammonium oxalate were used, should be 0:7 mgr. too high from this source of error. In the two sets of experi- ments the values obtained average an excess of 0°2 mgr., and the weight of metal remaining in solution after the determination is 0-2 to 0°3 mgr. These compensating errors, therefore, contribute to the apparent accuracy of the method ; they are sufficiently small to bring the process within the range of practical analysis. This conclusion is in accord with the experiments recorded by Avery and Dales ; the difference in the per- centage of carbon found is in all probability due to the time of electro- lysis. It is impossible to reconcile these results with those of Verwer and Groll ; but that their results, like those obtained by Classen, are low is undoubtedly to be attributed to the method adopted for testing the completion of the deposition of iron by means of potassium sulphocyanide. The origin and direction of the errors arising in the electrolysis of ammonium oxalate solutions containing iron are clearly shown by our experiments, and it is unlikely that different conditions prevail when other metals are present in the same electrolyte. The facts thus esta- blished must be duly considered in judging of the results obtained by these methods, especially in such cases as atomic weight determinations. The quantities of carbon deposited with the iron were too small to allow of the investigation of its condition of combination. We are, how- ever, inclined to think that it is present as a carbide, for whenever the deposited metal is dissolved in acid the smell of hydrocarbons can always be noticed ; also, after the upper layer of the metal has dissolved, the underlying portion is very often darker in colour and more difficult to dissolve. P 5. The Electrolytic Separation of Iron and Manganese in Ammonium Oxalate Solution. By Cuartes A. Koun, M.Sc., Ph.D., and H. H. Froysett. Bibliography. Author Journal Year | Volume Page Composition of Electrolyte Brand, A. Zeits. anal. 1889 28 581 | Sodium — pyrophos- Chem. phateandammonium oxalate Classen, A., | Ber. 1881 14 1,622 Ammonium oxalate and Reis, | M. A. Classen, A. ée 1881 14 2,771 | Ammonium and | potassium oxalates oe FA 1884 LT 2,351 Ammonium and | potassium oxalates sy 3 1885 18 168 | Ammonium and | potassium oxalates | A s 1885 18 | 1,789 | Ammonium oxalate | Engels, C. Zeits. Elec- 1896 2 414 | Ammonium acetate trochem. | | + Chem. Rund- 1896 — 5 and 20! Sulphuric acid schau | Kaeppel, F. Zeits. anorg.| 1898 16 268 | Sodium — pyrophos- Chem. phate and phos- | phorie acid Moore, T, Chem. News 1886 53 209 | Phosphoric acid and ammonium carbonate Wieland, J. Ber. 1884 17 | 2,931 Ammonium and | potassium oxalates ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 185 In the electrolysis of manganese salts in presence of dilute mineral acids, sodium pyrophosphate, or ammonium oxalate, the manganese is separated at the anode as hydrated peroxide. This property is of little value, however, for the determination of manganese itself, because it is difficult to effect the complete separation of the metal as oxide, and special conditions must be adopted to cause the precipitate to adhere to the anode. On the other hand, the difference in the behaviour of iron and manganese when subjected to electrolysis in ammonium. oxalate solution is attractive as a method for the separation of the two metals. The practical difticulty in effecting a separation on these lines is that the precipitated manganic oxide always carries down some iron with it ; this can only be overcome by adepting such conditions of electrolysis that only one of the metals is separated, the other remaining in solution. By means of a divided cell Engels states that manganese can be completely separated as peroxide, using a sulphuric acid solution ; this involves the subsequent determination of the iron. The chief work on the subject, however, has aimed at the determination of the iron by deposition on the cathode, obviously the more useful line of separation. According to Classen, the separation is possible if 8 to 10 gr. of ammonium oxalate are added to the solution of the mixed salts and the mixture electrolysed warm with a ©.D.,9) of about 1:0 ampere. This proportion of oxalate is said to outlast the deposition of the iron ; the manganic oxide does not separate until the mass of the oxalate has been decomposed, and even with large proportions of manganese only very little peroxide separates at the anode under these conditions. Neumann! and Engels? both state that the separation is incomplete, and our own experiments confirm this view. We have not found it possible to completely deposit iron without a separation of manganese peroxide, nor to separate the latter free from iron. The presence of even small proportions of manganese has, moreover, quite a remarkable effect in hastening the separation of iron as hydrate in the electrolysis of oxalate solutions. In some early experiments on the determination of iron the results were from 3 to 4 per cent. too low, and a separation of hydrate always took place after about two hours ; on testing the precipitate it was found to contain manganese, derived from the iron wire used in making up the solution. In the subsequent work recorded above the iron was always purified from manganese by precipitation as basic acetate. The following experiments show the extent of the error when the separation is conducted under the conditions most favourable for the deposition of the iron. The mixed chlorides of the two metals were neutralised with ammonium hydrate, 5 gr. of ammonium oxalate added, and electrolysed as usual. In experiments 4, 5, and 6, a C.D.;o9 of only 0-2 ampere was used ; but still the deposition of the iron was incomplete, and in all cases manganese peroxide contaminated with iron separated at the anode or remained suspended in the solution. A comparison of the results tabulated on p. 184 shows that the error in the iron increases with the proportion of manganese taken. ' Theorie %. Prawis der analytischen Electrolyse, p. 194. 2 Chem, Rundschau, 1896, pp. 5 ana 20, 184. REPORT—1900, Series VI. Tron Manganese| Per cent. . Tron taken : Ss C.D E.M.F Time ’ k 100 . ’ No gr. sete ee dopouité a | Ampere Volts Hours 1 01104 0:1080 0:0100 | 97°82 0:4-0°2 JeoD 18 2 0'1104 01080 0:0250 | 97°82 0°4-0°3 3-3'8 18 3 071104 0:0964 01000 | 87:32 | 0°4-0°3 3-3'8 18 + 0°1104 0°1086 0:0100 98°37 | 0:2-0°16 B= aes 5 0°1104 01070 0:0250 96°92 0:2-0'3 BB oul nal He 6 071104 0:1045 0:1000 94:65 0:2-0°3 3-3'4 18 Not more than 0°1 mgr. of iron was left in the solution as determined colorimetrically with sulphocyanide ; the remainder must therefore have been carried down by the manganese peroxide ; it was detected qualita- tively in each case in the precipitate, but no quantitative estimations were made. Direct experiments on the electrolysis of solutions of manganese chloride, to which 5 gr. of ammonium oxalate were added, and in which variations both of current and of electromotive force were tried, showed that it is not possible to electrolyse such solutions, under conditions per- mitting the deposition of iron, without the separation of manganese per- oxide. Theseparation is effected the more rapidly the greater the propor- tion of manganese present and the higher the current density and the elec- tromotive force. With only 0:01 gr. of manganese in solution, an E.M.F. of 3 volts, and C.D.o) = 0°2 ampere, the precipitation of hydrate occurred after four hours’ electrolysis in the cold solution, and in eighteen hours, the time required for an electrolytic determination of iron, with only 0-002 gr. of manganese, an E M.F. of 1°35 volts, and C.D.,)) = 0°1 ampere, the hydrate also separated. With the view of delaying this separation of the manganese a series of experiments were tried in which a small quantity of hydroxylamine sulphate was added to the solution to be electrolysed. It has been shown that this reagent acts favourably in preventing the separation of stannic acid in the electrolysis of tin salts in ammonium oxalate solution,! and it might, therefore, have a similar favourable effect in the case of manganese. To a small extent this is the case; the addition of 1 gr. of hydroxyl- amine sulphate, under conditions similar to those recorded in Series II. of our experiments, considerably delays the separation of the hydrated peroxide. But the deposition of iron is also delayed, and attempts to separate the two metals with this addition gave results similar to those of Series VI. The separated peroxide contained iron, and the deposited metal was from 3 to 16 per cent. too low ; in addition, the iron deposit was uneven and showed a tendency to scale off. We therefore conclude that the quantitative separation of iron and manganese in ammonium oxalate solution cannot be effected. Further, the influence of small proportions of manganese on the electrolytic deposi- tion of iron, referred to above, is a factor that detracts very considerably from the analytical value of the electrolytic method for the determina- tion of the latter. On the other hand, very small proportions of manganese can be sepa- 1 Third Report, 1896, ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 185 rated qualitatively from iron or other metals, which are deposited at the cathode in the electrolysis of their solutions, with greater certainty than by the ordinary analytical methods. 6. The Electrolytic Determination of Iron in Urine and other Animal Products. By Cuartes A, Kony, M.S8c., Ph.D., and G. C. Crayton, Ph.D. Tron is the only heavy metal present in the body, and the part it plays in animal metabolism is of special interest. The varied conditions of its combinations can as yet only be approached by histochemical reactions F for its total and quantitative determination the ordinary volumetric, gravimetric, or colorimetric methods have been applied. As the quantities present in certain organs and excreta are extremely small, special importance attaches to the methods adopted for their estimation. The usual method of procedure is to dry and ignite the product to be tested, extract the residue with acid, and determine the iron in the resulting solution. In the case of urine, for instance, a day’s discharge (about 1,500 c.c.) is evaporated and ignited until the residual ash is quite white, then dissolved in sulphuric acid and titrated with a dilute permanganate solution, after reduction with sulphurous acid (Hamburger!) or with zinc (Damaskin,? Jolles 3), Gottlieb and Ludwig * employed a gravimetric method in which the iron is precipi- tated as Prussian blue in presence of a 1 per cent. zinc chloride solution, the precipitate subsequently decomposed by alkali, and the resulting ferric hydrate weighed after separation from the zinc by repeated precipitation with ammonium hydrate. More recently Jolles has recommended the gravimetric determination of iron in urine by precipitation with nitroso- 8 naphthol.” The great variations obtained by the adoption of these methods are shown in the following data as to the quantity of iron present in a day’s discharge of normal urine :— Hamburger - 7-6 to 14:5 mgr. per 24 hours. Gottlieb and Ludwig . ‘ . 159 to 3:69 » Lieber and Mohr . 3 : é . 08 to 1:7 as Damaskin : : » Oto 1:5 ee Jolles . : : : . 46 to di +H Kumberg b 3 § y ; . 0-47 to 1:15 3 The values found by Damaskin, Lieber and Mohr, and Kumberg are usually regarded as the most correct, and 1 mgr. iron per diem in normal urine is looked upon as the average amount.® Two sources of error beset these methods of analysis. In the first place, the very large quantity of mineral salts, especially chlorides and phosphates, left after ignition has a disturbing influence on the titration with permanganate, especially with such small proportions of iron as 1 mgr. in the total solution ; secondly, it is impossible to completely remove the organic matter in the ignition, and its presence in solution affects the titration to a marked extent. These errors, which are of necessity irregular in character, are still more serious when gravimetric ‘ Kobert, Pharmak. Mittsil., 1891, 7, 40. * Arbeiten d. phaimakolog. Inst., Dorpat, 1871, and Zeits. anal. Chem., 1892, 81, 481 3 Zits, anal, Chem., 1897, 86,149, * Archiv, eapt. Pathologic, 1889, 27, 139. 5 Loe. cit. ® Stockman, rit. Med. Journ., 1893. 186 REPORT—1900. methods are adopted, whilst they make colorimetric methods altogether unreliable. The electrolytic determination of iron presents the important advan- tage over the above by not being affected by these adverse conditions, and our results justify the conclusion that it is reliable and accurate. The presence of phosphoric acid does not interfere with the determination. Any organic matter present in the solution of the ash can be completely removed by a preliminary electrolysis in presence of sulphuric acid. This was proved in a series of experiments in which the attempt was made to effect the deposition of the metal directly in urine without concentration and ignition of the resulting ash. In order to overcome the frothing due to the decomposition of the urea in the urine, during the electrolysis, the latter was first decomposed with nitrous acid, the details of the method of decermination being as follows : 100 c.c. of urine are treated in a flask with 12 c.c. of sulphuric acid (1:5) and 5 gr. of sodium nitrite, and gently warmed. After the decomposition is complete 5 c.c. of sulphuric acid (cone.) are added, the sclution boiled to complete the decomposition of the urea, and electrolysed overnight with a C.D.,),=1:0 ampere. The urine is completely decolorised by the current, a crystal clear solution resulting, whilst a deposit of carbon quite free from iron takes place on the cathode. The solution is then neutralised with ammonium hydrate, oxalic acid added to acid reaction, then 5 gr. of ammonium oxalate, and boiled. The precipitated calcium oxalate, which does not retain any of the iron, is filtered off, washed, and the filtrate electrolysed either at 60°C. with a C.D.,99=1:0 to 1:5 ampere, or, better, overnight, cold, with a C.D.\99 of 0°5 ampere and 3-0-4:0 volts. It is important not to de- crease the proportion of oxalate, or magnesium carbonate may be formed on the cathode ; it is easily soluble in ammonium oxalate. A platinum spiral of 1 to 5 gr. weight, according to the quantity of iron present, is used as the cathode, and a platinum dish of about 200 cc. capacity as the anode. The deposited metal, which is quite bright and metallic in appearance, after being washed, dried, and weighed, can be dissolved off, and the spiral re-weighed as a check on the determination, whilst confirmatory qualitative tests can, of course, be made with the resulting solution. In the following experiments known weights of iron were added to 100 c.c. of normal urine. (The quantity of metal present in the urine is negligible, less than 0-1 mgr.) A blank experi- ment was first made, with all the reagents employed in the method as de- scribed, to determine the contained iron and to make allowance for the carbon deposited ; the total amounted to 0-2 mgr., which was deducted in all cases. Tron taken. Tron found. Tron taken. Tron found. er or. er. gr. 0°0151 0°0152 0:0030 0:0027 00101 0:0100 0:0020 00015 0:0050 0°0051 ! 00010 00008 The results show that 1 mgr. of iron per 100 ¢.c. of urine can be very satisfactorily estimated by this method ; but this amount is far in excess of that ever found in normal urine or likely to be present, even under pathogenic conditions. In both cases at least 1,000 to 1,500 c.c. should be used for a determination, and this when concentrated to, say, 200 c.c., is so highly charged with organic matter that even when electrolysed for ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 187 forty-eight hours in presence of sulphuric or nitric acid the decolorisa- tion is incomplete. This direct method of determination is therefore inapplicable. The results are recorded to prove that the salts and organic matter are practically without influence on the deposition of the iron. The only alternative, therefore, is. to evaporate to dryness, ignite, best after a preliminary drying at 180° C., and then proceed as above, omitting, of course, the decomposition with nitrous acid. Thus modified the method loses much of its absolute, but none of its relative value. A mixture of equal volumes of sulphuric acid (1:2) and hydro- chlorie acid (cone.) is best for the extraction ; the solution is then con- centrated to remove hydrochloric acid, and electrolysed to destroy all traces of organic matter ; it is then ready for treatment with ammonium oxalate and the final electrolysis as described. The following results with normal urine were obtained by this method :— Volume of urine taken, Tron found. C.c. m. gr. 3,750 19 1,320 iy 1,02¢ 09 1,600 0-9 Taking a day’s discharge at 1,500 c.c., the average amount of iron per diem in the above experiments is 0°91 mgr., a value which confirms the most reliable of the results given above. In all cases in which the determination of very small quantities of iron in organic products is concerned, the exceptional delicacy of the electrolytic method, its freedom from the sources of error that arise with other methods on account of the inherent presence of salts and of organic matter, and, finally, the ready check on the nature and amount of the deposited metal, render it capable of giving reliable and comparable results under all conditions. We have made use of it, with advantage, not only in the analysis of urine, but also in the determination of iron in liver, spleen, and feces, both under normal and pathogenic conditions, The Teaching of Science in Hlementary Schools.—Report of the Com- mittee, consisting of Dr. J. H. GLADSTONE (Chairman), Professor H. E. Armstrone (Secretary), Lord Avesury, Professor W. R. Dunstan, Mr. GrorGE GLADSTONE, Sir Pamir Maanus, Sir H. E. Roscor, Professor A. SMITHELLS, and Professor S. P. ‘THOMPSON. Ir has been the custom of your Committee to give some comparative tables derived from the return of the Education Department showing the relative attention given to the teaching of scientific subjects in elementary schools for a period of years. By these it has been shown that for the eight years prior to 1890, during which time English Grammar was an obligatory subject provided any class subject was taken in the school, and as the Code allowed only two class subjects to be taken for the purpose of a grant, it was only in those schools where two of these were taken that 188 REPORT—1900. science teaching could be given throughout the standards. But the effect of this was that as the other recognised class subjects were History, Geography, and Elementary Science, and of these Geography was by far the most popular amongst the teachers, while English History was adopted in most other cases, Elementary Science scarcely received any attention at all. It should be borne in mind, moreover, that up to that date Geography itself was but little taught from a scientific standpoint, the details of topography occupying the pupils’ time almost to the exclusion of the study of the physics of our globe. In the year 1889-90 the number of school departments in which English Grammar was taken amounted to no less than 20,304, while Elementary Science was taught in only 32. Since that year a free choice of subjects has been allowed, and the wide discrepancy between these figures has been regularly reduced year by year; in 1890-91 English dropped to 19,825, while Elementary Science rose to 173; and the table below will show the change that has been going forward since that date. It will be observed that Object Lessons were introduced in 1895, and these were made obligatory in the three lower standards on and after September 1, 1896. In the report presented by this Committee last year it was pointed out that the distinction between Object Lessons and Elementary Science was one of nomenclature rather than anything else, and now in the Government return for 1898-99 the distinction in name has been abolished, and all are included under the term Elementary Science. . | | Class Subjects—De- | 1391 99 1899-931 1893-94! 1894-95) 1895-9611896-971 1897-98 1898-09 partments | | | | English. . — . |18,175/ 17,394 | 17,032 | 16,280 | 15,327 | 14,286 | 13,456 | 13,194 Geography . . | 13,485 | 14,256 15,250 | 15,702 | 16,171 | 16,646 | 17,049 | 17,872 Elementary Science} 788 1,073) 1,215 | 1,712| 2,237| 2,617} 2,143} 91.301 | Object Lessons. | | 1,079 | 8,321 | 21,882 \ 21, The number of departments in ‘schools for older scholars’ for the year 1898-99 was 23,191, all but two of which took one or more class subjects. But History was taken in 5,879 departments, and needlework (as a class subject for girls) in 6,952 departments, and sundry minor subjects in 1,034, making, with the other three subjects of the table, a total of 66,232. This shows an average of nearly three class subjects to each department ; but it must be borne in mind that the same subject is not always taken in all the standards, in which case three or more class subjects will appear in the return fora single department. That there has been less splitting up of the subjects between the upper and lower standards is apparent ; and also that such a subject as Geography must, in some cases, have been taught by means of object lessons, as otherwise it would have been found by this time that the figure for object lessons had equal]led the number of departments, whereas the 21,301 is actually considerably less than that for the previous year. It can hardly be assumed that under the regula- tions of the Code there was any actual diminution of such teaching. It has, been previously remarked that ‘the increased teaching of scientific specific subjects in the higher standards is the natural conse- quence of the greater attention paid to natural science in the lower part of the schools,’ The following table shows that such is the actual result :— ON THE TEACHING OF SOIENCE IN ELEMENTARY SCHOOLS. 189 ] Specifi: Subjects :| 1991 99 : 1892-93 | 1893-94 | 1894-95 | 1895-96 | 1896-97 | 1897-98 |i898-99 Children | | Algebra . . | 28,542 | 31,487) 33,612) 38,237) 41,846) 47,225) 53,081\111,486) Euclid . ; 927 1,279} 1,399) 1,468} 1,584) 2,059) 2,471) 5,932 Mensuration .| 2,802 3,762} 4,018) 5,614) 6,859) 8,619, 10,828] 24.848 Mechanics . | 18,000 | 20,023) 21,532; 23,806) 24,956 26,110) 27,009) 50,324 Animal Physio- | 13,622 | 14,060) 15,271, 17,003} 18,284, 19,989) 22,877| 41,244 lo | Bolany . | 1,845 1,968) 2,052; 2483) 2,996) 3,377) 4,031 8,833 Principles of | 1,085 909; 1,231); 1,196) 1,059 825 870) 1,168 Agriculture Chemistry . | 1,935 2,387; 3,043) 3,850} 4,822) 5,545) 6,978] 14,737 Sound, Light, | 1,163 1,168} 1,175 914 937); 1,040; 1,155} 1,943 and Heat | Magnetism & | 2,338 2,181; 3,040; 3,198) 3,168) 3,431) 3,905) 7,697 Electricity | | | Domestic Hco- | 26,447 | 29,210) 32,922) 36,239} 39,794] 45,869 51,259) 95,171 nomy bal sabe ay | Total . | 98,706 | 108,434) 119,295) 134,008] 146,305] 164,089 184,464|363,378 It will be observed, however, that there is a very remarkable increase in the figures for 1898-99, and that this applies to every one of the specific subjects. Strictly speaking, the return for this year is not comparable with those for the previous years, as they represented the number of children who were presented for examination in these several ‘subjects, whereas the return for this last year represents the number of scholars qualified for grants. In order to be so qualified in each subject, not less than twenty hours’ instruction must have been received by each scholar, but calculating from the standard unit for estimating the grant, it would appear that the amount of time given during the year to such instruction was actually about fifty-two hours. The mean number of scholars in Standard V. and upwards was 716,157, which would give 50°7 per cent. as the proportion of scholars qualified for grant as compared with the possible number of students ; but it must be remembered that nearly one-third of them take two subjects, and are therefore counted twice over. Though, as indicated above, too much stress must not be laid upon these increased figures, it is quite evident that the abolition of individual examination in the specific subjects has been received with favour by school managers and teachers, with the result that much more attention is devoted to this branch of instruction, and, it is to be hoped, with much less cramming. The Code which has been introduced this year will further carry out this principle by substituting one block grant for all the elementary, class, and specific subjects, so as to avoid the temptation to study what would bring in the most grant rather than what is most adapted to the cireum- stances of the individual school. At the same time, the Code requires that ‘lessons, including object lessons, on Geography, History, and Common Things be taken as a rule in all schools,’ and that one or more of the subjects of instruction hitherto known as ‘ specific subjects’ is to be taken ‘when the circumstances of the school, in the opinion of the Inspector, make it desirable.’ For the guidance of teachers in preparing their course of study, the Board of Education (which now takes the place of the Education Department) have issued a number of specimen schemes adapted for 190 REPORT—1900. schools of different sizes and circumstances; and in the explanatory memorandum one of their objects is declared to be ‘to make the course of instruction in all schools more comprehensive, so as to give all scholars the rudiments of general information, while enabling the details of the instruction to be adapted to the special needs of various kinds of schools.’ Tt is added that in all schools both boys and girls ‘should learn something of their own country, and be taught to observe and to acquire for them- selves some knowledge of the facts of nature... . In country schools lessons on the objects and work of country life are valuable that would be inappropriate in town schools, while in the latter the instruction given in lessons on Common Things and in Elementary Science should be varied with reference to the probable future occupations of the children. . . . The introduction of a wider and more generally interesting course of instruc- tion will, it is hoped, be a welcome relief from the continued repetition of the restricted course of lessons, which has a tendency to become lifeless and wearisome. As an illustration may be quoted Scheme 5, for a boys’ school in a seaside town, in which the course for ‘ Elementary Science and Common Things’ is thus set out :—‘ Class V. to IIT. : A course of lessons on marine animals and plants, on local rocks, pebbles, &c. ; various sorts of boats, ships, &c. ; lighthouses and lightships ; the local tides ; flags of different nations, &c. Class IJ. : The magnet and compass ; practical methods of finding the cardinal points ; apparent movements of sun and moon ; measurement of sun’s altitude by shadows. Class I.: Practical measurements of areas and volumes; lever; pulley ; inclined plane ; practical examples of parallelogram of forces and parallelogram of velo- cities ; the chief constellations and the apparent movements of heavenly bodies.’ Since the issue of the Code for this year the Board of Education have issued a minute establishing Higher Elementary schools. Higher-grade schools, as they have usuatly been called, have grown up in all the large industrial centres during the last twenty years or so, with the approval] of the Education Department, though questions have been raised as to the right of School Boards to carry them on. All such doubts would he set aside by working under the minute, which provides for a four-year course, commencing at a point equivalent to Standard V., and contemplating a continuance of study up to fifteen years of age. No definite scheme of instruction is laid down in the minute, as that is to be regulated by ‘ the circumstances of the scholars and the neighbourhood,’ and the grants will be assessed at the higher or lower scale according to ‘ the thoroughness and intelligence with which the instruction is given, the sufficiency and suitability of the staff, the discipline and organisation.’ Though there are some inconvenient restrictions which it may be found necessary to modify, the effect of this minute should be in the direction advocated by your Committee. This, however, will depend absolutely upon the will of the Managers and the consent of the Board of Education, as the minute only provides that ‘the Managers of any school who desire such school to be recognised as a Higher Elementary School must submit for the approval of the Board before July 1 in any year proposals for a curriculum and time table, and supply such other information as may be required by the Board.’ In contrast to this may be quoted the provisions of the Scotch Code for Higher Grade Schools, which include the following :—‘ Such schools or departments may give an education which is either predominantly ON THE TEACHING OF SCIENCE IN ELEMENTARY SCHOOLS. 191 scientific and technical— Higher Grade (Science) Schools—or predominantly commercial— Higher Grade (Commercial) Schools, or they may give a course which is recognised by the Department as specially suited to girls or to special classes of pupils. In all cases the Department must be satisfied that the school possesses the proper provision of class rooms, laboratories, and workshops necessary for the particular type of education to be given therein. . . . Pupils following the Higher Grade Science course must take in addition the following subjects: Mathematics, Experimental Science, and asa rule some form of Manual Work. . . . In the second year of the Higher Grade Science course not less than eight, and in the third year not less than ten, hours a week must, asa rule, be allotted to Science, and at least half of this time must be spent by the pupils in individual experimental work. For the purpose of this article three hours of Drawing or of Manual Instruction, or of both conjointly, will be reckoned as equivalent to two hours of Science. In the third and following years Manual Instruction may be dropped, and the pupil should devote himself to the study of some special branch of Science.’ In Appendix V. it is further stated : ‘The course in Science should proceed from elementary exercises in measuring and weighing, and calculations based thereon, to the experimental investigation of elementary notions of Physics and Chemistry. In rural schools, and in summer, some investigation of plant life and of the elements of Botany should be added. At least half the time devoted to this subject should be spent by each pupil in practical work, . . . The Department must be satisfied that the teachers have a competent knowledge of the subjects which they are to teach in each subject individually, and in the case of Science that they have had experience in treating the subject experimentally.’ In the Reports for 1897 and 1898 your Committee referred to the improvements which were being effected in the teaching of Science in the London Board Schools, and to Professor Fitzgerald’s advocacy of the extension of the same system to Ireland. The Commission on Practical and Manual Instruction, of which he was a member, reported strongly in favour of such work, and decided that similar instruction should be given in schools under the National Board of Education. To this end Mr. Heller (whose transference from London to Birmingham has been already noted) has been appointed Organiser of Science Instruction in Irish Schools, and will take up his new duties as soon as he can be released from the Head- mastership of the Municipal Technical School of Birmingham. The syllabuses of specific subjects in the Irish Code are similar to those in the English Code of regulations. For the present a scheme corresponding to Course H of the English Code has been introduced in a slightly modified form, and notes have been added indicating the spirit in which the instruction should be given. A training laboratory is being equipped in Dublin at which selected teachers will be taken through a course of instruction in heuristic methods, and where they will receive the benefit of the experience gained in the London schools. The training colleges not under the control of the National Board are also understood to be sympathetic, so that there is very good prospect that the Science teaching in National Schools in Ireland will be energetically developed. The advance which was noted last year in the work of the Evening Continuation Schools does not seem to have been maintained, as will be evident from the following table. Nearly all the subjects show a falling off, except Elementary Physics and Chemistry, Domestic Science and 192 REPORT—1900. Navigation, which give an increase ; and Horticulture and Ambulance, which are practically stationary. Number of Scholars Science Subjects ~ - | 1896-97 | 1897-98 | 1898-99 Hchiciaees ) .porkesane Silay) SATELORG Mat agESH 1,216 Algebra . . fe A 4 rt =f 7,467 | 9,996 | 7,432 Mensuration . ; : : “ 27,388 | 29,966 | 24,369 Elementary Physiography 4 : - 1) oat | 4,807 1 aeons Elementary Physics and Chemistry : 24 8,185 | 2,902 | 3,116 Domestic Science . : , i j | bi lrg 142 Science of Common Things . P ; -| 10,910 | 13,874 11,499 Chemistry . F . : § : . 5,658 | 6,590 5,963 Mechanics . : \ : ikmelpop se: cllZo 987 Sound, Light, and Heat . 3 : : . | 726 | 813 | 437 Magnetism and Electricity . : 5 a 3,834 3,967 / 3,005 Human Beysiekey 4 4 ‘ : F 5,865 6,237 4,296 Hygiene. ; F ; . . si} 3,179 4,062 3,276 Pee hath wntentrcatin teen ratite 692 763 597 Agriculture . . : 3 ; 2 3 2,355 2,300 | 1,826 Horticulture . 5 : : ‘ , rules ak {olone 1,354 | 1,850 Navigation. | 68 on 4 46 Ambulance ; 3 5 Z | 9,086 13,030 | 12,980 Domestic Economy ls ; ‘ ; SU memlishaiirne || pez) 19,915 | | Totals . : : 107, 042 | 126, 740 106,665 In the last Report oe was Gi to te ee attention which was being given by the School Board for London to the teaching of Experimental Science in their schools, and to the preparation of a properly qualified staff of teachers for that work. In this they have had the advantage of the advice of Dr.C. W. Kimmins. The supply of suitable accommodation and appliances for carrying this out has also been seen to, so that the Board have at the present time more or less complete provision for the experimental teaching of science in 79 of their schools : of these 11 are pupil-teacher centres, 37 are classed as higher-grade schools, and 31 as ordinary schools. In some cases there are both chemical and physical laboratories, with lecture rooms furnished with demonstration tables, with gas and water laid on ; in others there is only one laboratory specially fitted for Chemistry, but which can also be made available for the teaching of Physics. In the Act of Parliament creating the Board of Education it was provided that a Consultative Committee should be established, two-thirds of the members of which should consist of ‘ persons qualified to represent the views of Universities and other bodies interested in Education ;’ and it will be noted with satisfaction that one of the members of your Committee—Professor Henry E. Armstrong—has been nominated to that office. ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 195 On Wave-length Tables of the Spectra of the Elements and Coivpounds. —Leport of the Committee, consisting of Sir H. E. Roscor (Chair- man), Dr. MarsHatL Warts (Secretary), Sir J. N. Lockyer, Pro- fessor J. Dewar, Professor G. D. Liveinc, Professor A. Scutstsr, Professor W. N. Hart ey, Professor Wotcorr Gibzs, and Captain ABNEY. Index to the Tables of Wave-lengths in the Reports of the British Association from 1884 to 1900. Abbreviations: Sp.=Spark Spectrum; A.=Arc Spectrum; Ab.=Absorption Spec- trum; Fl.= Compound-line Spectrum; Spectrum. Arr, Sp., 1884, p. 352 ; 1893, p. 387. : Ab., 1886, p. 171. Alumina, Sp., 1885, p. 310; 1892, p. 237. Aluminium, F'l., 1895, p. 334, Sp., 1884, p. 356. A., 1884, p. 356; 1893, p. Ammonia, Fl., 1885, p.310; 1898, p. Antimony, FI, 1895, p. 324, Sp. 1884, p. 357. A., 1884, p.357; 1894, p. 265. Argon, V., 1896, p. 273. Arsenic, FI., 1895, p. 322. Sp., 1884, p. 360. A., 1894, p. 264. a” Sp., 1884, p. 362. A., 1884, a4 362 ; 1892, p. 206. Barium Chloride, FL, 1885, p. 311; 1894, p. 259. Bromide, FI., 1885, p. 311. Todide, Fl., 1885, p. 311. Oxide, Fl., 1885, p. 312 p. 259; 1895, p. 321. Beryllium, Sp., 1883, p. 129; 1884, p. 364. A., 1884, p. 364. Bismuth, F1., 1895, p. 325. Sp., 1884, p. 364, A., 1894, p. 266. Bismuth Chloride, Sp., 1885, p. 312. Oxide, oe 1885, p. 312. Boron, Sp., 1880, 1894, p. 7560. Boron Oxide, Fl., 1885, p. 313. Bromine, L., 1880, p. 270; 1884, p. 367; 1900, p. 195. Ab., 1886, p. 180 ; 1892, p. 211. 2; 1894, CADMIUM, Sp., 1884, p. 368 ; 1895, p. 297. , 1892, p. 204. Cesium, Fl, 1884, p. 371. Sp. 1884, p. 371. A., 1884, p. 371; 1892, p. 196. 1900. . 274; 1884, p. 367; | Flame Spectrum; Bd.= Band Spectrum; L.=Line Spectrum; Cl.= V.=Vacuum-tube Spectrum; P.=Phosphorescent | Calcium, Sp., 1884, p. 371. A., 1884, p. 371; 1892, p. 198. | Calcium Chloride, Fi, 1885, p. 313; 1894, p. 257. | Bromide, Fl., 1885, p. 313. 2 (I Fluoride, F1., 1885, p. 313 ; 1895, p. 320. Iodide, Fl., 1885, p. 314. Oxide, Il., 1885, p. 314; 1894, p. 257,; 1895, p. 322. Carbon, Bd., 1880, p. 265; 1883, p. 129; 1884, p. 374; 1893, p. 412. L., 1880, p. 265; 1884, p. 374; 1893, p. 406. Carbon Hydride, Fl., 1885, p. 316; 1895, p. 317. Oxide, 1880, p. 269; 1895, p. 314; 1895, p. 319. Nitride, Fl., 1880, p. 268; 1885, p. 316. A., 1893, p, 418. Cerium, Sp., 1884, p. 378. Chlorine, Sp., 1880, p. 269; 1884, p. 378. | V., 1899, p. 257. | Chromium, Fl., 1895, p. 334. | Sp., 1884, p. 380. A., 1894, p. 248. Chromium Chloride, Sp., 1885, p. 318. | Cobalt, FL, 1895, p. 333. Sp., 1884, p. 382 1897, p. 75. A., 1884, p. 582; 1890, p. 1897, p. 75. | Copper, Fl., 1895, p. 335. Sp., 1884, p. 384 ; 1896, p. 308. | A., 1884, p. 384 ; 1893, p. 392. | Copper Chloride, Fl., 1885, p. 318. Bromide, F]., 1885, p. 319. Todide, Fl., 1885, p. 319. Oxide, Fl., 1885, p. 319; p. 334. ; 1890, p. 225; 90>. wim 1895 DIDYMIUM, Sp., 1884, p. 386. Didymium Chloride, Ab., 1886, p. 181. 0 194 ERBIUM, Sp., 1884, p. 388. Erbium Oxide, Fl., 1885, 319. P., 1886, p. 186. Chloride, Ab., 1886, p. 181. FLUORINE, FI., 1880, p. 272; 1884, p. 388. Sp., 1884, p. 388. GALLIUM, Sp., 1884, p. 388. A., 1884, p. 388. Gold, Sp., 1884, p. 389; 1896, p. 328. A., 1893, p. £00. Gold Chloride, F1., 1885, p. 320. HyDRoGun, L., 1884, p. 389. Cl., 1884, p. 590; 1886, p. 187. INDIUM, Sp., 1884, p. 392. A., 1884, p. 392; 1893, p. 402. Iodine, Sp., 1880, p. 271; 1884, p. 393. Ab., 1886, p. 182; 1890, p, 234. Iodine Chloride, Ab., 1886, p. 183. Jridium, Sp., 1884, p. 394. A., 1884, p. 394. Tron, Fl., 1895, p. 330. Sp., 1884, p. 395; 1898, p. 313. A., 1884, p. 395; 1891, p. 161. tron Oxide, Sp., 1885, p. 320. LANTHANUM, Sp., 1884, p. 415. Lead, Fl., 1895, p. 326. Sp., 1884, p. 417. A., 1884, p. 417; 1894, p. 262. Lead Oxide, Sp., 1885, p. 321. Lithium, F'l., 1894, p. 256; 1895, p. 319. Sp., 1884, p. 420. A., 1884, p. 420; 1892, p. 193. MAGNESIUM, Fl. 1884, p, 420. Sp., 1884, p. 420. A., 1884, p. 420; 1892, p.197. Magnesium Hydride, 1885, p. 321. Oxide, 1885, p.321; 1895, p. 821. Manganese, F1,, 1895, p. 335. Sp., 1884, p. 422. A., 1884, p. 422. Manganese Oxide, 1885, p. 322; 1895, p. 337 Mercury, Sp., 1884, p. 424; 1895, p. 800. A., 1892, p. 209; 1895, p. 300. Bd., 1895, p. 312. Molybdenum, Sp., 1884, p. 426. A., 1884, p. 426; 1899, p. 261. REPORT—1900. NICKEL, F1., 1895, p. 332. Sp., 1884, p. 427; 1890, p. 230 ; 1897, p. 108. A., 1884, p. 427; 1890, p. 230; 1897, p. 108. Nitrogen, L., 1880, p. 259; 1884, p. 428; 1893, p. 405. Bd., 1880, p. 260; 1884, p. 430; 1886, p. 188. Nitrogen Oxide, Ab., 1886, p. 183. OSMIUM, Sp., 1884, p. 431. Oxygen, L., 1880, p. 262; 1884, p. 432. Cl., 1880, p. 263 ; 1884, p, 432. Ab., 1891, p. 245. PALLADIUM, Sp., 1884, p. 434. Phosphorus, L., 1884, p. 484. Bd., 1880, p.274; 1884, p. 434. Phosphorus Oxide, F1., 1895, p. 322. Platinum, Sp., 1884, p. 486; 1898, p. 411. A., 1898, p. 411. | Potassium, Fl., 1884, p. 436; 1894, p. 256; 1895, p. 320. Sp., 1884, p.436; 1895, p. 295. A., 1884, p. 436; 1892, p. 194. Potassium Permanganate, Ab., 1886, p. 186. ROWLAND’ Standard Waye-lengths, 1895, p. 273. Rubidium, F'l., 1884, p. 438. Sp., 1884, p. 438 A., 1884, p. 438 ; 1892, p. 195, Ruthenium, Sp., 1884, p. 438. A., 1884, p. 438. SAMARIUM, Sp., 1884, p. 438. Samarium Oxide, P., 1886, p. 186. Scandium, Sp., 1884, p. 439. Selenium, Fl., 1880, p. 272; 1895, p. 323. L., 1884, p. 440. Bd., 1880, p. 272; 1884, p. 440. Silicon, Sp., 1880, p. 274; 1883, p. 129; é 1884, p. 441; 1893, p. 407. A., 1884, p. 441. Silicon Chloride, V., 1886, p. 167. Bromide, V., 1886, p. 167. Fluoride, V., 1886, p. 167. Hydride, V., 1886, p. 167. Iodide, V., 1886, p. 168. Silver, FI, 1895, p. 328. Sp., 1884, p. 442; 1896, p. 318. A., 1884, p. 442; 1893, p. 398. Sodium, Fl., 1894, p. 256; 1895, p. 320. Sp., 1884, p. 443; 1895, p. 295. A., 1884, p. 443; 1892, p. 193. Strontium, Sp., 1884, p. 444. A., 1884, p. 444; 1892, p. 202. ON WAVE-LENGTH TABLES OF THE Strontium Chloride, 1866, p. 168; 1894, p. 258. Bromide, 1866, p, 168. Fluoride, 1866, p. 168. Todide, 1866, p. 168. Oxide, Fl., 1866, p. 169; 1894, p- 258; 1895, p. 321. Sulphur, L., 1880, p. 272; 1885, p. 290. Bd., 1880, p. 272; 1885, p. 290. TANTALUM, A., 1885, p. 292. Tellurium, L., 1880, p. 273; 1885, p. 292. Bd., 1885, p. 292. F1., 1895, p. 323. Terbium, Sp., 1885, p. 296. Thallium, F1., 1885, p. 297. Sp., 1885, p. 297. A., 1885, p. 297; 1893, p. 403. Thorium, Sp. 1885, p. 298. Thulium, Sp., 1885, p. 298, Tin, Fl., 1895, p:327. Sp., 1885, p. 299. A., 1885, p. 299. Tin Oxide, 1866, p. i69. The Solar Spectrum, 1878, p. 27; 1895, SPECTRA OF THE ELEMENTS. 195 Titanium, Sp., 1885, p. 301. A., 1885, p. 301; 1896, p. 293. Tungsten, Sp., 1885, p. 304 ; 1898, p. 355. URANIUM Sp., 1885, p. 304; 1900, p.201. VANADIUM, Sp., 1885, p. 304. WATER, A., 1866, p. 169. Ab., 1886, p. 171; 1891, p 245. YTTERBIUM, Sp., 1885, p. 305. Yttrium, Sp., 1885, p. 806. A., 1885, p. 306. Yttrium Oxide, P., 1886, p. 186. ZINC, Sp., 1885, p. 307. A., 1885, p. 307 ; 1892, p. 207. Zirconium, Sp., 1885, p. 309. A., 1885, p. 309. p. 273. Telluric Lines of the Solar Spectrum, 1886, p. 171; 1891, p. 245. Bibliography of Spectroscopy, i881, p. 328; 1884, p. 295; 1894, p. 161; 1898, p. 439. Spectra of Metalloids, 1880, p. 258. On the Influence of Temperature and Pressure on Spectra, 1880, p. 275. Absorption Spectra of Rays of High Refrangibility, 1880, p. 303. General Methods of Observing and Mapping Spectra, 1881, p. 317. Genesis of Spectra, 1882, p. 120. Ultra Violet Spark Spectra, 1882, p. 143; 1883, p. 127; 1885, p. 276. BRoMINE (VACUUM-TUBE). Eder and Valenta, ‘ Denkschr. kais. Akad. Wissensch. Wien,’ Bd. Ixviii. 1899. | Previous Measurements Redtiction to | Wave-length Tptenstty, ae LS ene aw! | ae a Cee (Rowland) ~} ..27e . sna | ‘requency | Character | Salet Eldoheu es | ae a in Vacuo 6682°83 2 6990 6862 | 1°81 4:0 14959°7 32:02 5 6631 6622 1:80 4:1 | | 15074:3 6582'52 1 6581 6577 | alerds) | 187°6 60:17 4 6556 6556 | 1°78 A dl 239-4 45-00 3 | ” ” 274-7 6353-07 I 173 ‘o 7361 51-02 10 6357 6358 Nees, 55 741-2 6204.36 3 169 44 16113°3 6178°72 2 1-68 es 180:2 70:09 2 es 33 = 202°8 59°60 2 ” ” 230°4 49°95 10 6166 6159 1:67 5 255:9 42:02 4 6152 * fr 2769 23°49 3 6132 33 PF 326°2 18°89 4 | 6129 7 i 338°4 6097:05 ail | 1:66 Pr 397:0 02 196 REPORT—1900. BROMINE (VACUUM-TUBE)—continued. Previous Measurements ‘Reduction (Rowland) to Vacuum Wave-length tntennty Oscillation (Rowland) Gis akoe Heegieney Sales | Pliicker and | a+ ae RECO Hittorf A §954:°3 3 1:62 4:6 16790 50°7 4 ” ” 800 40°83 4 ” ” 8281 5871:97 3 5881 1:60 ” 17025°5 68°40 2 5869 ” ” 032°'3 64:55 3 ” ” 047':0 52°40 5 1:59 ” 082°4 33°71 3 | ” 4:7 17137 2 31:04 i 5841 5828 a5 5 1449 21-40 3 5825 wy | on 173°3 5794:50 2 5793 ESS al ts 17253°0 a = 5740 — — —_ 19:17 4 5721 5723 1:56 4:8 17480'3 16°5 3 aa WH 8439 488 11 +25 | 4 5713 ” ” 175045 ey —— 5697 — — Ss 5657°83 4 5663 1°54 ” 17669°8 43°40 3 ” ” 177150 30'3 1 ” ” 756 27'5 1b 5627 1°53 ” 765 22°38 y 1 5623 ” ” 7813 21°95 1 ” ” 782°6 5600:90 4. 5601 5599 ” 4-9 17849°4 5590715 8 1:52 * 883'7 88°40 | 2 ” ” 889°3 ~ 84°98 1 ” ” 900°3 60°10 1 5567 ” ” 980°4 45°91 1 5553 151 * 180264 39°21 1 ” ” 0482 36°52 4 ” ” 057°0 32°38 5 ” ” 070°5 29:19 2 ” ” | 080°9 Ive Ae the yil 5516 5516 9 ” 18121°3 11°04 | 2 1:50 ” 140°5 08°49 | 3 ” 99 148°9 06:97 8 | 5 55 153-9 549524 7 5501 5503 | 99 5-0 192°6 89:00 6 5496 5493 ” ” 182135'2 83:20 2 \ a as ” 232°5 8141 2 bs iss » 238°5 80-20 3b pu Ma | 242-5 66°43 5 | 1-49 Fee 288°5 50°28 3 5451 5447 ” ” 18342°7 42°55 4 ” ” 3687 33°49 1 ” ” 399°4 25°21 | 5 | 5426 | 5429 ” ” | 18427°5 23-01 | a | 5423 ” ” | 4349 539569 5 5392 | 1:47 b>) 18528:2 1 — | 5384 “5 3) == 70°51 | 2b” | | I, 99, ae at 18615'1 64 35 | 3b” | | ” / ” : 636-4 60°99 2 AE TS a eae 648°2 45°53 AbY ” ” 187021 35°30 5 5336 | 5327 i’ #5 y 7380 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 197 BROMINE (VACUUM-TUBE)—continued. Previous Measurements Reduction Ne oth Intensity (Rowland) to Vacuum Oscillation ean) d Frequenc pomiant) Chaecies in V. : Pliicker and 1 econ Salet F Ar = Hittorf A 5333°49 1 1:46 5:1 18744°4 32:1 8 10 ” ” 749:0 30°76 2 ” ” 754:0 04:31 ii 5300 1-45 a 18847'5 — — 5311 5293 ” anes || — 5272°89 4 ft 5276 | 5264 ; 1:44 52 | 18963°3 63°68 | 4 | 5267 | 5251 i A Bs 992:9 49':219 3 1:43 oy fy 1904526 39°994 2 6241 5226 ”» ” 078°79 38°472 8 ” ” 084:°34 33°65 2 §221 ” ” 102°9 27-911 3 5217 a a 129°4 Say on 9 ” ites 5199-50 3 ” 53 227°3 94:075 4b ‘ 1:42 i ot 247°4 84074 4 5188 “ +. 284°5 82:573 ii os rp 290°1 80°19 2 5186 5181 ” ” 299-0 74:09 1 141 3 321°8 64560 5 5166 5169 +i ; 361°2 43-626 2 6151 FY cf 436°3 — =e 51232 1:40 — ie iF a 5107 ” ” a — — 5093 1°39 3 — 5054°853 4 5061 5055 » 54 7776 38962 3b } | 5036 1:38 » | 840-0 20°756 3 | 1:37 5:5 911°8 11:000 1 5011 fs 7 950°6 02°96 1 a 7 982°7 4987-234 | 1 4991 1°36 Fe 20045:7 79°950 4s 4983 ‘3 is 075:0 59°51 4b 4961 rf + 157'8 45°768 3n 4956 1:35 rr 213°8 42°21 ln re 56 228°3 30°816 5s 4931 4933 oe Pe 2750 28-966 5s 4925 Fi a3 282°6 26°758 2n rs 5 291°8 21:386 3n 6) 3 313°9 21:20 In H a 3146 4867-935 3b 4869 1:33 as 537°0 66°851 3b 3 a. 5415 48988 6s 4853 “6 57 617:2 45-196 3b | 4848 ” ” 633°3 38°823 3 | 1-32 er 660°5 34:699 2n | . as 6781 16900 8s 4816 4819 5 A 7545 02°544 4s 4808 1:31 A 8166 4799-794 3n | ” ” 828°5 98-415 | oD H ” ” 834°5 91-989 | 2n af e 862°5 85'644 10s 4786 4788 - ‘ 890°1 80524 6s | 4779 a 5:8 912-4 77°30 } 38 ) * a 926°5 76605 | 7s | | aan a 929°6 Ta 4l | 38 i em}. | 934:8 1 198 REPORT—1900. BROMINE (VACUUM-TUBE)—continued. Previous Measurements | Reduction to Wavelength | Intensity Negib sey |, nee Oscillation (Rowland) an eee See Brequency Character | Salet aoe eng ers i in Vacuo 4774.01 4s 1:31 |; 5°8 20945°3 72°91 3b 4772 fe $: 945°8 67-282 8s 30>, i 970°5 66°27 dbY “a A 975:0 53°05 i 3 Es 21033°3 52:47 3b 5 “ 035-9 50°10 2b - _ 046:4 44:53 3b 4747 - = O711 42°87 8s | 4737 a - O78°5 35°67 5bY | 4731 a = 110°5 28°90 2 1:29 ms 140'8 28°49 Ba = . 142°6 20°56 1b 472i 4721 a Fe 1781 19°95 8 | a rs 180°9 I Gays 3 a Pe 191°5 14-66 In ) = 2 205-0 11-32 1 | 5 3 219-7 08°16 1 - 233:9 05:00 10b 4706 4707 a) APSR 248-1 01:93 2n ss ss 262-0 469877 2n 4696 Bs - 2763 96°59 2n - ‘s 28671 93°48 8s e x 3003 92°51 3b eB cal as 304:7 91:42 3b aid | ee 309°6 78°88 8b 4676 4681 a || Gee 3667 75°82 2s 4677 1, Peon et oaiisy 380-7 73°56 2s 1h deed Va 3911 72°750 6s PCE. 394-8 66°42 2 ed 423°8 52-18 6s 1:27 : 489-4 44-17 2n 4645 Sa Sahise 526°5 43°74 4s a ee 528-4 42°35 3 . 3, “3 534:7 29°66 3b ss eat a0 593-9 22°99 8s 4621 4626 e . 630-4 14:86 6s 1:26 . 662°6 05:90 2b x 55 7053 © 01°63 5n - Ps 725-4 4597-14 3n ” ” 7467 75:95 6br 1:25 . 847-4 58°21 4n ! 1 he 61 932:3 43°12 8s 4543 | 4544 3 Pa 22005:2 42-67 | 2n Fa 55 007-4 38°95 5b ie | | 025°4 30°21 1 Ate! real | 067°9 30:00 5s Sl es, e | 069-0 29-78 2s : | 070-0 25°82 Sbr | ., a A 089°3 13°99 iL | 1:24 " 147:2 13°67 5s . * : 148°8 08:29 Qn | ef ¥ 175°3 4477-96 5by 4486 | 23 62 325:4 72-83 8 - bd 351-0 F199 1 355°2 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS, 199 BROMINE (VACUUM-TUBE)—continued. Previous Measurements | Reduction to | | Wave-length ae (Hemland) Yaeuunt Osaillation (Rowland) ste Or aes ‘requency | Character gajot es ea xe -- | in Vacuo 4470-22 1 123 | 62 | 228641 66°42 In | 1°22 a 38371 65:99 In ms Pe 385°2 60°92 1 = * 410°7 60°39 1 ” 3 413-4 53°75 1 A i 446°8 41-94 Sb cr * 506°5 31:15 2 ” 6:3 561°3 30:07 2 pA | ee 566-7 25°32 5s » re 590°9 23°22 2 ” C 601°7 12°66 1 ” ci, 655°8 07:80 4. ” Cr 680°8 05°18 1 ” $9 694°3 4399°87 3 ” 3 7216 98°55 5 ” op 738°8 95°10 4 ” op 746°3 91:76 3 1:20 e 765°6 86°83 2n 9 5 789°2 T8311 4b ” ” 834°6 77-40 2s ” Fe 838°3 7220 3n » Fe 865°5 65°76 8s 4368 4366 » 6:4 899-2 65°31 4s 3 os 901°5 4297-27 38 5 6°5 232641 91°54 6 4287 4988 1:18 %3 300°6 36998 6s + 6:6 595-0 307101 I 4231 4242 ET hiss 633-4 23-996 8 4229 116 Pal 667-7 02°64 4s 4199 1:15 4 7880 4193-62 | 6 ” 67 839-0 93°34 | 2 3 saaay 840°6 79°76 8 4181 | 4182 " ae ||| 918-1 | %5:92 5s ” ” 940°1 (Eis 1 ” ” 941:°0 60:14 2s 114 Pe fa 240310 57-54 2 of “6 046:0 57°23 3s 9 a5 047°'8 51°52 38 ” % 080°9 44°12 2s ” 6:8 123°8 40°37 6s 4143 -f, Fr, 145°6 38°78 8b ” 3 155°9 | 35°79 5s ” is 172-4 | 17-58 3b 1:13 's 279'3 10°12 4 ” ” 323°4 09-96 1 ” ” 324:3 06°52 | 3s ” ” 344-7 05:56 J 2s cr) a5 350°4 02-62 4 % 3 368°3 4096°27 3b ” 69 405°6 90°74 3s 1:12 op 438°5 89°29 3b 3981 » ” 447-2 75-66 4b ” ” 529-0 37-486 2s 111 70 7609 36°538 4s ” ” 766°7 200 REPORT—1900. BROMINE (VACUUM-TUBE)—continued. Previous Measurements | Reduction to pwievollencth Intensity (Rowland) Vacuum (Rowland) Character Pliicker and ba Salet Hittorf A+ | ae 2 Se | eee id 402419 | 5by | 111 | 70 22:04) | 2 | | PA B95, | 1 | | bie 12°70 3s | 110 | 2 08:93 6bY ee oF 5 O7-45 5s as ‘i 05°69 2s | yy ie Maa 0160 | 13 / 5 TI 3999°77 4b | \ ee 97:27 4b » 9 92°51 4s | | ante f 91°485 3s | hes oF 85°666 8s 4 ss 80°585| | 10n | € i 80'151 | 5s | Paras] oy 68°804 5s 1:09 a 55°504 8bY oH V2 50°745 Tb’ 3 - 39862 5b¥ 1 ee be 38°801 Bbr as 5 35°310 6bY - 1:08 . 29°726 6b} ees ~ a | 24-239 SbY See | 23506 | 6 - * 20°838 6b* a s 19-770 | 6s ee ae 17°960 | 35 | 55 a 14-419 | 9 cs - 14:270 — ” 55 01-418 4 bo tees 3891°:790 8s | $500 Fules ay 88-665 4bY | 1:07 a | HLS ee 6s | fi 3 57°363 6s . Gil eae 40-775 | 3br | | 1:06 | ,, 34861 | G6br | | ; # 29-920 | Sn ig | fie a 28-640 3 | 1s eee) uae 15:771 | 4s | | | 1:05 7-4 11°55 | 3 | im Ps 01-09 Is | - 53 | 3794:153 | 4s | ” ” Pesog, it ue Ab. ail 1:04} 7:5 | 70410 | 2b | ” ” | 53°87 | 4b | ” ” 40:66 i 5b | ” ” Gein ho aed. «| . 1031 <; 35°91 1 pee ii 25°54 1 ee) URS 14:45 | 4 | ‘ “nt 3699595 | 2 | 02 1-5 84:84 | 3 | | ” ” Oscillation Frequency in Vacuo 24842°7 856:0 856°6 913°9 9 37: 3 946°5 9575 982°9 994-3 25010:0 039°8 0442 076°5 114'8 117-6 189°4 2746 304:5 3744 381-2 403°8 4409 A754 480-2 497-5 504°5 5163 539°4 540°3 624°4 687:9 709'5 $23°3 9171 26029°1 069°3 102:9 1115 199°6 228°6 300°8 349-0 498°5 514:8 631:7 725'7 7461 7597 834-1 914:3 27022°4 130°6 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 20] URANIUM. Exner and Haschek, ‘ Sitzber. kais. Akad. Wissensch. Wien,’ cvii., 1898. Reduction to 14a Wave-length Intensity Vacuum ae | spark eis =H in Vacuo | Spectrum Character x Be | i | | | 4699-95 In be LORD ab SD: & | 21270°9 99°3 In | »” ” { 274 Hl 99°02 In ie sx eer 275-1 97°55 In out Bes | 281°8 96°77 / 1 ” ” 285'3 96°30 1 ob 287°5 95-4 1b | ‘ ‘i 292 93:95 In a2 Z 298°1 92°6 lb 1:28 2 304 92°32 In i, x 305°5 92:15 In i 3063 ee In : r 309-5 90°95 In a s 311-7 es 1b tee: ‘i 312 pee 3 S 3 319-4 88:0 In - . 329 ae In A ‘ 329 85'9 Qn a + 835 ome In és ; 339-4 84:20 1 im { od 349-5 aoe u ao) i) eS ae 3440 83°29 1 a | 347-0 $2:90 . 1 x | 348-4 82:77 1 f i 349-0 §2°33 } in - - 351:0 } 81°40 | In Seen 355'1 80 85 | In ie i | 358°6 80-4 In | ts 3 | 360 78°'8 1b cd ‘. / 367 78:1 lb es : 370 15°6 In ” ” | ‘ 382°5 4-45 In i ‘ 386-9 7£0 In ” ” j 389 71°66 2 a i 399°7 | 69°55 1 | = i, 409-4 69:22 1 fs Ps 411-0 69:05 1 i 2 411-7 68-67 1 re 413-5 67:45 1 is i 419°] . 67-07 2 s st 420°8 | 66:23 1 a - 424-7 | 65-42 1 ts . 428-4 | 64-98 | 1 bs % 430°4 | 64°30 1 e ‘ / 4885 | 63:97 1 En | 4351 632 1b > ee 439 | 62-78 1 x n 440-6 62:40 1 | ” ” 442°3 Slay In Bs 4 444-7 | 610 In ” ” 449 GOL In 5 halae| 453 | 59-52 in ot tee 4555 58°92 . In ohn 4582 202 REPORT—1900. URANIUM—continued. = Reduction to Wave-length Intensity ie Oscillation Spark and > Frequency Spectrum | Character A+ he | in Vacuo iN | 4658-4 | Ib | 1:28 59 21461 576 1b 4; a 464 567 In 4 4 468°5 55°40 In n % 4745 55:03 2 D ») | AT57 54:43 In 1:27 ” 4789 53°65 . 1 % i 482-6 53°25 1 aA 3: 484-4 53:05 ] “5 Ay 485-4 52°09 1 7 ” 489:7 51°75 In ” ” 491-4 50°7 In 9 .9 496 50°24 1 0 ” 498°2 49°37 2n is A 502-2 48°15 1 Bs 5 508-0 46°85 4 3 3) 514-0 46°30 1 4 Phy 516°6 45°80 in ” a) 5189 45:13 In fe 43 522:1 44-30 1 ay 5259 43:86 i = a 527-9 42°72 In fy a 533°2 41°91 2 2 +) 536°9 40:57 If ” ” 543:'0 393 1b oy A) 549°5 38°16 in > A; 554-7 35°73 In 5 x) 565°7 35:2 In an At 568 34:2 | In 2 a 573 31°92 | 1 x 3 583°4 31°81 | 1 5 -) eS 5839 B11 1b x ” 587 30-4 | lb i fi | 590 29°94 if on 6:0 592°6 29°37 In 53 24 595°2 28°5 | 1b FA o. 599 27°30 5 5 ; 605-0 26°14: 1 | os “4 610°4 25°26 In > 55 6145 24:91 In A + 616'1 24:27 In if A 619°1 23°68 | i a - 620°8 22°23 il cs A 627°5 22°13 1 ay 5) 628°0 20°42 3r | By i. 636-9 19-4 : In oD A 642 18°60 2d s; F 645-7 17°80 In eA 5 649°3 17°33 In Rs 5 6515 16-7 | In 1:26 SS 6545 15°85 In a i 658-5 15°32 In 5 x 661:0 15:18 In + A 661°6 14°90 1 Bs *4 662-9 14:50 In 0 A | 664-6 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. URANIUM—continued. 9 ~ 0 3 ee eee Wave-length Spark Spectrum 4612°8 12°47 11-70 10:07 09-0 06-4 05:38 03:88 02-04 01:38 | 00:96 0013 4599-73 99-03 98-51 98-05 97-77 96-95 95-91 95°73 95-30 94-49 92°75 91:96 91-0 90-46 90-21 89-55 886 88:1 87-45 871 86°5 85°75 85:03 84-5 83°52 83-00 82°65 81-98 81-33 81-02 79°87 79°20 78°5 77-40 76°85 76°25 75°3 75:00 74:6 73:90 73:50 732 72-47 Intensity and Character In Reduction to Vacuum Oscillation Frequency in Vacuo 21673 6748 678:0 685-7 691 703 (077 714°8 723'5 726°6 728°6 7325 134-4 7307 740°2 TA2°4 743-7 TAT 6 7525 753°3 755-4 759°3 767-4 1712 776 778:2 T794 7825 787 789°5 7925 794 797 800'6 804-0 807 811°2 813°8 815°5 818°7 821°7 823-2 823°9 831:°9 835 840°5 843-1 846°0 850°5 851°9 854 857-2 859-1 860°5 864-0 204 REPORT—1900. rae URANIUM—continued. Reduction to | Wave-length Intensity Vacuum Spark and fe Oscillation Spectrum | Character | 1 Frequency | A+ a in Vacuo | ioe 4571'8 : — ten a. 71:50 | ae a 6:0 21867 7116 il ie ” 868-6 70:87 | 1 aT) ” 870°2 7011 i 3 } 3 ” 871°6 69°40 | 1 | # ” . 875:2 | 63841 1 uz ” 878°7 67-89 3 ” ” 883°4 67-1 1b a ” 885-9 65'8 1b | Be ” 890 64:50 | ln =) ” 896 64-26 A ” 61 902'1 63°56 | In ” ” $03°3 62710 | 1 » ” 906'7 61°6 \ In | a ” / 913°6 61-45 i » ” 916 60°50 1 4 ” 916°7 60:0 1b | ” ” 921°8 58°60 1 2 ” 924 58°32 1 a ” 930°5 58:07 1 ¥ ” 931°8 57:99 | 1 | ” ” 933:0 56°50 ] * ” 933°4 56°18 1 ” ” | 940°5 55°30 4 3 ” | 942°] 54:03 | 2 | ”? ” | 946°3 | ae | In ” | ” poe" / | 52°63 In 43 | ” | 957 | 52-24 In rd ” 959-2 | 51-87 } in ” ” 961°1 / 5131 | In ” ” 962°9 50°68 / In ” | ” 965-6 | 50°55 | In ” | ” 968°6 50°05 2 | ” 969-2 49-4 In ” ” 971-7 48°75 In ” ” 975 48-4 In i) ” 9779 48°2 ln » ” 980 47°65 ln bid ” 980°5 46°43 1 ” ” 983°3 45°76 4 vw ” 989-2 45:16 1 ” ” 992°4 45:01 1 ” ” 995°3 44°57 H 1 ” ” 996-1 43°83 7 ” ” 998°2 43°21 In ” ” 22001°8 42°75 in 1:34 ” 004-8 | 42°25 In = | ” 007:0 | 41°90 1 3 ” 009°4 | 40:70 1 | ” ” Ol11 40°41 | 1 | ” | ” | 016-9 39°4 In 3 ” } 018°3 38°37 4 | 2? | ” | 023 3735 T | ” ” 028-2 4 ” | 033 2 | 370 In ae ’ ~ ” i Bis) ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. URANIUM—continued, 205 Reduction to Wave-length pase g Spark Character pectrum | 4536°80 | 1 36°24 ] 35°45 In 35°32 In 3473 In 33°91 1 33°25 In 32:7 lod 31°95 In 31°50 in 30°93 In 29°92 1 29°3 1b 28°74 ld 28°20 1 27°85 1 26°85 1 26°20 In 25:98 1 25°87 1 25°57 1 25°14 1 24:3 1b 23°43 1 2371 lb 21°81 2n 20°7 Ind 19:97 In 19°4 in 18°80 In 18°30 In 17°45 1 16°95 1 15'8 2b 15°50 4 14°49 1 14°30 il 13°89 | 1 13°55 | I 13°04 1 12°62 1 12°37 1 11:98 1 11°88 1 11°46 1 10°53 3 10:08 1 09°55 in 09'1 1b 084 1b 07:96 1 O7'67 | 1 06°85 In 06°42 2 06°31 2 Vacuum Ae oe A 1:24 671 Oscillation Frequency in Vacuo 22035°9 038°6 0424 043-4 045°9 049°9 053°1 056 REPORT—1900. URANIUM—continued. Reduction to Wave-length Intensity Vacuum Oscillation Spark and €; Frequency Spectrum Character a cles in Vacuo A 4504-95 1 1:23 G1 22191°7 04:47 In D | 3 193°1 03:97 ] Py £ 196°5 03°86 1 5 # 197-0 02°56 In 4 Fi 203°5 O211 1 5 - 205°7 01°65 In & 208-0 00°9 In ” ” 212 00:00 In “5 | # 21671 4499°87 ln 2 Fi 216°7 99-40 1 rs i 219'1 98 47 Ind x is 2237 O77. 1b rs cr 227°5 96°83 In a9 A 231°8 96°35 In - a 234-2 95°85 In A > 236°6 95°5 In a 6:2 238 95°3 In on 4 239 94°90 1. 5 A 2412 94°09 In 4 A 245°2 93:28 1 x 55 249°3 92°60 1 h a 252°6 92°20 1 * “ 254-7 O17 1 cf _ 257°1 91°53 il a A 257°9 91:02 3 , » 260-4 90°4 1b Bs es 263 89:29 ] 7D 3 269°9 891 In a rf 270 88°40 1 5 it 273°6 87°90 In ” 5 276-0 87:27 1 5 3 279°2 87:15 1 y 5 280°0 86°52 1 ” » 282'9 8612 1 0 - 284°8 85-40 1 cb 2 288° 84:7 1b H ‘ 291 83°99 1 i ss 294°3 83°67 1 * “4 295°8 82°91 il - * 300°8 82-4 1b 5 x 303 81:25 * In a - 809:0 80°83 In + . 5110 80°55 In nS i 312-4 79°63 In % a 3167 7915 In A 3 318°9 77-93 2 53 325 9 77-67 In e . 8271 76°70 | ys ;, 337 75:91 | . a 3355 75:50 In ‘5 : 3387-7 75°04 In ” ’ 339'8 74:73 In 5 * 341°3 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. URANIUM—continued. Reduction to Vacuum Wave-length Intensity Oscillation Spark and Frequency Spectrum Character {| 44 i in Vacuo r 44745 In 1:23 6:2 22342°5 T44 In | ¥ * 343 74:0 1b : ; 345 73°6 1b ik ‘ 347 72°55 6 a ss 3524. 71°82 1 3 ; 357-7 765 In ey) at 363:3 ‘oO Fo 3 362°6 ee | Sees | ae SOS » A 367: 69°42 il Pr 2 368-1 69°05 1 - % 369:'9 68°57 1 1:22 ¥9 3723 68:49 1 : 5 372-7 68°34 1 | ‘ ie 373°5 68°16 1 ae » 374-4 oe | ” ” 375:0 A ” ” 377'5 67:27 1 Fp : 378'8 665 1b : ‘ 383 IS 5 . 65:35 3 ee: 4 3886 a eae ie: % ” ” 393°3 63°98 1 » ” 395+4 aan : » > 399-7 es » ” 400°8 0 » | FP 403'0 62°04 1 cp ‘ 40571 ees ; a 407-2 ” uP 409'7 60°77 1 ” ” 4115 59°97 In a Ei 415°5 58°85 Ind Fr i 421+1 58:15 In ae 4 424-6 58:03 1 $5 i 425-2 57°67 1 ” ” 427°0 57°33 1 ” ” 428°7 57:0 In | a 5 430 BBra4 i} | ” ” 433°2 56°08 1 | » : 435°1 553 In | : | 7 439 541 In | as 3 445 53108 In » » 445°7 53°68 1 ” ” 447-1 53°46 1 ” » 448-2 52°48 1 - 3 4531 52°19 1 » ” 454-6 5172 | eae ” 456°9 ae In » » 159°6 50°75 2 ¥ # 461-9 50°59 2 7 + 462-7 Frcs 1 ” ” 467'0 49°2 1b 470 208 REPORT—1900. URANIUM—continued. Wave-length | Intensity Spark and Spectrum Character 4448°5 1b 48:2 1b 47:30 2 46:18 1 45°70 | 1d 45°38 1 44°90 1 43°80 | 1 43°60 1 43°47 1 42°95 In 42°80 in 42:20 In 4175 In 41:29 1 41-20 1 40°94 1 40°54 1 40°22 Jn 39°32 1 38°90 . a 38°61 1 38°42 In 38°16 In 37:12 In 36°97 1 36°5 in 35°72 In 34°81 2 34:08 3 33°58 in 33°35 In 32°90 1 32°60 ] 32°2 | lb als | 1b 30:27 1 29°79 | ] 29-05 1 28°63 | 1 27°81 3 27°14 1 26°85 2 26:25 1 26:03 1 25°6* ln 25°35 i In 24:73 in 23°96 2 23°49 | uf 23°15 J 22°78 | 1 22:2 i In Reduction to Vacuum Oscillation | Frequency ate. OH Le in Vacuo | A At | 1:22 | 62 22473 >. ae 475 ” | ” AT9'2 same 4848 ” ” 487°4 ” | ” 489°1 5.) hemes 491-5 ” | ” 497°1 ” ” 498'1 | AM aes 498'8 ” ” 501°4 ” ” 50271 ™ ” | ” 505°2 ” i ” 507°5 ’ ” 509°8 ” ” 510°3 ” | is 511°6 ” ” 513°6 ” ” 5153 ” ” 519'8 ” ” 521°9 ” ” §23°3 ” ” §24°3 ” | ” 525°7 ” | ” 530°9 ” | ” 531-7 ” ” 534 ” | ” 538'0 ” | ” 542°7 ” ” 54674 22 ” 548°9 ” ” 550'1 ” ” 552°4 ” ” 5539 ” ” 556 ” 63 558 121 » 565-7 ” ’ 568°1 ” » 571°9 ” ” 5745 ” ’ 5782 ” | ” 581°6 ” | ” 5831 ” ” 586°2 ” ” 587°3 ” ” 589'5 ” ” 590°8 ” ? 593°9 ” ” 597'8 : ” 600°3 ” ” 602°0 ” ” 603°9 ” ” 607 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 209 URANIUM—continued. Reduction to | Wave-length Intensity Vacuum ” Oscillation Spark and 1 Frequency Spectrum Character | A+ oe in Vacuo | a | * ——— — 4420°89 2n 1:21 63 22613°6 | 20°57 1 39 ” 615:2 19°8 In i = 620 | 19°3 | In er, | 2 620 18°68 1 | - a | 624-9 } 18-22 1 | 3 » 627-2 17°94 | 1 os ss 628°7 . 17°61 1 “p » | 630°3 17:00 1 7 | > 633°5 | 16°73 1 » PA 634:9 16°05 1 4 a 638°3 15*46 2 ” » 641-4 14:97 1 aA = 643°9 14°85 1 se is 6445 14:50 1 » ” 6463 13:33 1 é 4 6523 13:07 il oD 4 653-7 12:7 In i: » 656 ) 12°5 In be ” 657 | 12:0 nea. 9) Fr » 659 11°65 | 1 j ” ” } 661:0 11°50 1 + 3 661°7 11°31 1 FE » 662-7 11:10 1 As 7 663°8 10°6 In ay ” 666 | 103 In oF ” 668 09:90 1 is “6 669°9 09:1 In os » 674 08°92 1 a5 » 6750 08°73 1 oo » 676-0 08°15 1 es is 679:0 07-4 In A ” 683 06°74 1 = 686°2 06°13 1 3 Fi 689°4 06-0 In Ss - 690 05°47 1 9 - 692°7 ) 05:09 tL BS 5 694:7 * 04:99* 1 3 iv 695:7 | 04°53 1 = 7 697-6 04:22 1 3 9 699°2 03°52 1 ” ” 702°8 02°70 1 A ” 7071 02°57 1 ” ” 707°7 02-06 1 ~ 7 710-4 O11 In ” » 715 00°65 In ” ” 717-6 4399°81 1 “ » 7218 98:0 In “ ” 731 97°50 1 7 » 7339 95°96 In + ” 741°8 95°45 | In As FS | T44°5 951 | In we Fe | 746 94°83 1 1:20 i a T47-7 * Fel 1900 P 210 | | REPORT—1900. URANIUM —continued. Reduction to Wave-length Intensity | Vacuum Spark and ) =: Spectrum Character e% 1 ; | aS 4393°80 | 2 { 1-20 63 92°73 a se r 92°40 1 : #1 92-04 1 4 91°69 1 : fi 91°46 7! gs if 91°30 1 zt ‘ 91-1 In = ri 90-74 1 is ; 90°50 1 i . £ 90°36 } i 4 ie 90°20 1 2 | ¥ 88:9 In e : 4 88:4 In PS : if 87°95 ln - | + 878 In a a 87:45 In x fi 86°9* In sd s 86°35 ln BE a 86°21 In fe x 85°76 In | Bs ie 84:95 iL * i 84°82 1 s , 83°77 2 i 3 83°50 2 . f 82°60 iL in if 82°32 1 - é 82-04 1 is ‘i 81:60 1 = } f 81°35 1 € ii 80°95 1 is > 80°49 1 i 4 79°9 In 3. vs 79°41 1 2 t 78:75 In i ‘ po In } ” ” 78:0 In | i Ff 17-48 In | 2? ” 77-00 1 = k 76°37 In | : ‘ 1595 les : 75°79 | In - ‘ 74:22 1 4 i | 73°61 2 Ks ‘ | 72-95 | i i j 72-78 2 a ; | 71:99 2 : if 71:26 1 i i 70-21 | 1 3 ; 69°75 In : j 69°5 In a4 i, 69:0 In - £ 68°42 1 ” 6-4 Oscillation Frequency in Vacuo 227530 758°6 760°3 762-1 763°9 T65°1 766-0 767 768°8 T7701 7708 7716 778 781 783°3 784 785°9 789 791-6 792-4 7948 799:0 7997 805°2 806°5 811-2 812-7 8141 816-4 817-7 819'8 822°2 825 827-9 831-3 832°6 835 837-9 840°4 843°7 8459 846-7 8549 858-1 8616 862°5 866-6 8703 875°9 8783 880 882 885-2 ea i i ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 21 Wave-length Spark Spectrum URANIUM—continued. Se Ss ee a Intensity and Character Reduction to Vacuum 4368°33 67-95 67-6 65°77 65°28 65:18 65:00 64°61 64:50 64:03 63°15 63°00 62°48 62°23 61°36 61:2 60°45 59°92 59°68 59°10 58°83 58°60 58°36 58:0 578 57-06 56°75 55°89 54:77 54°53 54:25 53°95 533 52°98 52°62 52°30 51:98 51°84 50°5 50°3 50:1 498 48'8 48°32 47°36 46 95 46°48 46°20 44°88 44-45 44°15 43°5 42-60 41°89 40°86 B BPW NRP RP REE HERP Pee eee een er aa = =} Pa tebe eit ES RO) ND Hem bie Be eRe =] B Oscillation Frequency in Vacuo 22885°7 887-7 889°5 899:2 901°7 902°3 903°1 905°2 905'7 908°1 912°8 913°6 916°3 917°6 922-2 923 927°1 929°8 931-1 _ 9384:2 935°6 936°8 938-0 940 941 944:9 946:5 951-1 957:0 958°3 959-7 961-4 965 966°5 968-4 970-1 971:7 972°4 979 980 982 983 988 989°6 996°1 998-2 23000°7 002°2 009°2 O114 O13'1 O16°5 0213 0250 030°5 P2 212 REPORT—1900. URANIUM—continued. ; ; St ad | Reduction to Wave-length | Intensity | Vacuum Oscillation Spark | and Ee a | Frequency Spectrum Character / “CPE Ba cae in Vacua fA : | + Ae SS. ©. Je 4340-63 1 1:19 64 23031°8 39°94 1 | a * 035-4 39°55 1 aes | ¢ | 037-4 | 39°16 1d 5 ¥ 039°5 . 38:93 1 ae f 040°7 38:80 1 - * 041-4 38-48 1 A m 043-1 38:1 1b ; . 045 37-61 1 9 } ” 047-7 36:93 In a res | 051-3 | 36°60 2n Pines ‘oa 053-0 / 39°92 2n - 7 056°8 30°44 1 - 5 059°3 35°13 1 . i 060°9 34°66 1 . 063-4 33-71 1 z i | 068" 33°15 1 ) 5: ‘ 071°5 32°47 1 | = * O7T5'1 ) 32-05 1 * . 077-4 ) 31°63. 1 x if 079°6 30:9 ! ] b ” ; ” 083°5 30°20 ln = ‘ O87:2 29°7 1b | ” ” 090 29°40 1 K | = / 091°5 28°92 1 &. - 094-0 28°35 a 5 E | 097-1 . | 28-0 1b ; et 099 ) 27°18 | 2 / Es * 103-4 36-06 | 3 | 5 | 109:3 | 25°32 1 a by) ad 113-2 | ) 24:90 | 1 | x ee 1155 | / 24°75 1 | 3 $ / 116°3 | 23-92 2 % 6°5 220°8 22-55 In 5s 4 128-2 222 | 1b | al ieee a ae 120 21°51 1 : a 133°8 21:2 lb is lea ies 135 20°6 1b + i 1385 19-97 2 - i 141°8 19-67 1 ee < / 143-4 . 19-22 | 1 “ +: 145-9 18-5 1b 1:18 a 150 18-2 1b é 55 151 17-78 1 - iM 1536 17°46 1 5 - 155-4 17-27 1 : « 156-4 16:70 1 2 is | 159°4 16°20 | In : 4 162°1 . 16:08 In ) e a 162-7 15°7 in u = 165 15°4 ln i ; 166 14-08 2 | t ¥ 173-4 13°39 2n : d 177-1 ) 12:87 1 / i :. 179-9 12°51 | 1 4 a 181°8 : ; —_— = ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 213 URANIUM— continued. Reduction to Wave-length Intensity vee Oscillation Spark and i . i Frequency Spectrum Character A Ea in Vacuo r 4311-95 | 1n 1:18 65 | 23185°0 11°66 in ss a | 186°6 113 1b ” ” | 187 10:62 1 é 4 191:1 09-95 | 1 2 i 195°8 09°40 in < cf 198'7 08'8 | 1b a el 202 08-13 In 5 op | 205°5 07°50 1 E- | 208'8 07:06 1 ) . rf 211-1 06:99 1 * = 211°5 06-71 1 . 3 213-0 06°48 1 3 is 214:3 06:1 In ‘4 x 216 O54 In i i 220 O49 ln a 5 | 223 04:67 1 b: if 224-0 04:25 | In z ® 226'3 03°53 1 a fr: | 230°3 03-43 | 1 Es fe 230°8 03-00 1 ie % 233-1 02°60 1 iz 2352 02°51 1 fy 2357 02°30 1 ee i 236°8 O19 In | ” ” 239 01:70 1 , ¥ 2401 01-60 1 is c 240°7 01-05 In if is 243°7 00-95 In f } 244-2 00:53 1 “ ok 2465 00-26 1 . i 247-9 00-08 1 - £ 2489 4299-61 2 f is 251-4 99°26 In 55 & 253°3 99-05 In _ Fs 2543 98-6 In - A 257 98°2 1 ln Be, 9 | 260 97-78 1 . fy 261-4 97°31 3 is +, 263°9 9677 1 - a 266°8 96°49 1 is F 268°3 95°93 1 : . 271°3 95-47 1 a . 273'8 95°32 | 1 a eae | 2746 94°85 i ‘i 277-2 94-40 | In ys 4 279°6 94:13 1 58 I, 281-1 93-95 In + ‘. 282-1 93:53 1 : ” 284-4 92°87 | In ” ” 287-9 91-81 1 i; ( 293-7 91:08 2 Ss Pe 297°6 90:05 2 . i 299-1 89°72 1 | < Pe 305:1 89°05 2 308°7 214 REPORT—1900. URANIUM—continued. Reduction to Wave-length Intensity | ee Oscillation Spark and | Frequency Spectrum Character Aa: oa | in Vacuo xX i — = 4288°56 1 1:18 65 23311°4 88-05 3 ” ” 314-2 87:10 3 > 7 319°3 86:5 in 4 % | 322°5 85°96 it a : 325-4 85°63 aif ” | ” 327-2 85°45 1 9 ” | 328-2 85-20 1 » ” | 329°6 85:03 1 ” ” '330°5 84°73 1 | He “3 332°2 84:15 in 55 a5 338b°3 83°65 In . a3 3381 83:3 In s 3 340 82°67 3 as 5 343°5 82:25 a4 = As 345°8 82:00 1 ” | B47°1 81:5 In | Sf ” 350 80:86 Sin per iba ke 4 / 354-7 80:4 In = A | 356 79°53 In ” ” 360°6 78°37 2 A 5 367°0 77-76 i a Fo 370°3 77-43 In a * 372°1 77-08 1 a 55 3741 76°69 2 s AS 3762 76:2 In - ; 379 7594 1 > o 838071 75:46 1 = 59 | 382°8 75:2 In 5 A 384 74:20 3 5 R: 389:7 73°64 1 5 5 392°8 73°16 In 4 | 4 395°4 72°52 1 in FA 3989 72-03 In 35 5 401°6 71°46 1 BA i 404:8 WAZ 1 A a 406°6 70°88 1 ; e 407°9 70°50 ld = . 4100 69°84 4 Pe 5 413°6 69°05 2 a F 4186 68-67 1 Es ns 420-1 68-22 1 s aS 492°5 68:12 1 3 = 423°0 67-76 i 6 f 4250 67°50 2 z 3 426°4 66°89 1 5 As 429°8 66°53 in if | Bf 431°8 658 In on > 436 65:45 il * Bs 4377 64:95 1 Be Ae ah 440°5 64:49 i ; bs 443-1 64:05 1 ’ | ” 445-4 63:97 1 ¥ Ps 445°8 63°66 i - 3, 447°5 63°38 1 - EN 449°0 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 215 URANIUM—continued. Reduction Waye-length | Intensity | to Vacuum | Oscillation Spark | and 7 Frequency Spectrum Character | a | Be in Vacuo . A 4263-12 i 1:17 | 65 23450°5 62:75 il 5 | 3 | 452°6 62°40 | In | 1 | a 454°5 61°73 1 ‘ ‘ 458:2 61:25 In | i . * 460°8 61:1 In | és 53 462 59°65 1 a | x 469°6 59°43 | 2 i Fe 470°8 59°10 1 . i) 472°6 58:7 In - + 475 58°45 In # _ 4762 58:3 | In ) . 0” ) 477 579 In a + 479 57-21 . 1 | e . / 483°] 56-75 In 53 : 4 | 485°7 5595 1 is ee 490:0 55°65 / 1 , ve 491:7 55°50 1 | a rd 492°5 55-0 | In 1 ieee i 495 54-6 In | E . 497 54:45 In | 5 e 498:3 54-10 1 > m 500-2 53-9 In / % | £ 501 52°65 2 .- | 6F 508'2 52°30 In ss + 510-2 51:9 In + ¥ 512 51-60 In | is 3 5141 511 1b | sn F 517 50-42 In % ; 520°5 50-2 In | » i" 522 49°73 . 1 s . 524:3 49:3 lb a: ;: 527 48:8 | lb es i? 529 48°13 1 % . 533°1 47-57 1 - 3 536-2 47°33 1 : . i 5376 46°45 g > f 542°5 46°18 | 1 “ % | 544-0 45°96 1 i 5 545-2 45°60 i! 4 x 547-2 45°10 1 + | " 5500 44-53 3 ‘3 | " 553°2 43°53 1 TG, ‘ 558°7 43°25 | 1 - z 560-2 42°70 1 a | a 563°3 42°52 1 - e / 564:3 41:88 4 ee | if 567'8 40°80 2 a | i 573°8 40°35 In . 3; | 3 | 5763 39-9 In ‘ 3 579 39°33 1 7 | Z 582'1 38°8 | 1b oi 585 37-93 . in Ks . 5s 589°8 36°62 | 1 cs - 597-1 36°21 3 | ee 5994 16 REPORT—1900. URANIUM—continued. Wave-length Spark Spectrum 4235°60 34:90 34:77 34:25 33°92 Intensity and Character Reduction to Vacuum Oscillation Frequency in Vacuo Wwe eH ee eee In s nol wed san ae es oe In Cn ee ell oll all are p =] 23602'5 606°7 6074 610°3 612°2 613-4 615°5 619°7 SS ON WAVE-LENGTH TABLES QF THE SPECTRA OF THE ELEMENTS. 217 URANIUM—continued. | Reduction to Wave-length Intensity | Vacuum | Oscillation Spark and lg ] ail Frequency | Spectrum | Character | A+ hae ne | in Vacuo | = pall 5 Noor meee es Beaks ‘et 4213°50 1 1:17 66 " 23726°6 ) 13:19 1 . 33 7283 | 12°94 1 Pie One 729:7 12°67 1 5 3 7313 12°47 2 “ A 732°4 12°35 1 . a 733°1 11:87 2 | 4 7 735'8 11°52 1 | * 3 737°7 11:05 ld | As - | 740-4 10°64 2 “a | “ | 742-7 097 | lb ¢ | is 748 07'4 * 1b f é ) 761 | 06 54 ld C a 765°8 06-14 1 m es 768-2 05°2 In 115 fs T7135 04°63 1 = 8 TI67 | 04:51 2 . | se 117-4 . 03:27 1 . | re | 784-4 | 02:9 In ie | fe | 786°5 | 02°60 | In Es . | 788-2 | 02°45 In | ., ih 789:0 | 01:80 In iS * | 792-7 01:59 1 ‘e Ks 793'8 01:30 1 3 3 7955 01:13 1 “ # 796°4 00:30 Oy 95 67 8011 4199°8 In 3 i 804 98°9 In | FS A 809 98°39 | 1 e 4 812:0 97-69 | 2a2 x | xf 816-0 97°35 In | > | 5 | 817°9 96°9 In ss | is 820 96:70 1 s 5 821:5 96:0 in f 825°5 95°7 In » ” 827 95°4 In ” ” $29 95:22 In 3 | 5 829:9 94:55 1 | 5 * 833°7 94:15 In * - 836-0 93°95 | In | a | J | 837-2 93°60 | In io | ¥ | 8391 93°15 In F x 8416 92°35 | In f bi 8463 92°15 1 “ . 0 | 847-4 91-76 1 cn | 5! 849'6 90°5 1b » ” 857 89°40 2 : i 863'1 89.0 In ” ” 865 88°33 2 ” ” 869°1 88:02 1 a a 870:9 87°57 1 3 FS 873°5 87°15 c I ie *) 875°9 86:95 1 ” ” 877-0 86°63 1 Ee A 8789 86:22 1 - os) 881°3 218 REPORT—1900. URANIUM —continued. Reduction to Wave-length Intensity Vacuum Oscillation Spark and Zz Frequency Spectrum | Character nee gl | in Vacuo | | > al | 4185°97 | 1 Id Ou 23882°7 85°85 1 “5 55 883 4 85:04 1 cn a3 8879 84:67 In a 3 890:0 84:27 In . is | 892-3 83:79 1 3 55 | 895-0 83°47 | 1 :, s | 896-9 83°15 1 ct) on 898°7 82°88 1 on 900°2 81-75 i “ s 906°8 80-90 1 % a. | 9116 80°53 In Fe “4 | 913°7 80°3 | 1n os a O15 79°20 o} e bs 921°3 78:69 1 7 = | 924-2 78:00 1 a 928:2 77:56 ! » rh 930°T | (ire In 3 = 933 76°75 In 5 . 935°4. 7611 1 a A 939'1 75°63 1 fe 5s 941:8 | 74:40 2 oe 948-7 | 74:01 1 “ K 950°9 73:90 1 3 if 951-7 73:19 2 oe Pp 955°'8 72°8 In 3 ees 958 72°40 1 i * 960°3 71:80 5 %5 a 963°8 71:00 1 “ 968-4 70°60 In or Pe 970°7 70°17 1 i a 973-1 69°7 In Sy : | 976 69:25 1 | is 4 | 978-4 68°3 1b 1:14 + | 984 67°87 In 5 + 986-4 67°25 | In 7 .j 989-9 66°8 in | * | * ' 992°5 65°87 2 59 * 997:9 65°35 | In a = / 24000°9 64:97 | 1 | x * ! 003°1 64-6 | In 2 : | 005 63°90 | 2 a SF 009°2 63°44 1 2 sf 011:8 63:22 1 | i 3 013-1 62°88 1 | = 2 015‘1 62°62 1 ‘ bi | 016°6 62:00 | 2 i | 020°2 6114 1 ” ” | 025°1 60°5 | 1b . mh 029 | 60:05 | 1 ‘ 3 | 031°5 | 59°59 | 1 si 034-2 | 59°30 iL | 7 ° 0385°9 59°15 i | se Aj 036°8 588 in rs i 039 58:48 2 | . iF yaed 040°5 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 219 URANIUM—continued. Reduction to Wave-length Intensity Macuun Oscillation Spark and Frequency Spectrum Character At us in Vacuo Xr 4156°81 2 1:14 6:7 24050°2 55°58 | 3 ” ” 051°3 54°16 2 Pr 4 064:5 53°75 2 np 5 066'8 51°83 if ap + 079:0 51-48 | 1 as 3 08171 51:00 1 . . 083'9 50°61 2 cf 3 086:1. 50°25 in - .f 088-2 49°57 | In pe if 092-2 49°38 In | 3 » 093°3 48°97 1 Fr * | 095-7 48°76 1 ce Oe aes 096-9 48:33 In Ff e 0993 47°62 1 co 7 103-4 47°30 1 ”» 68 105°3 47°20 1 3 A} 1059 46°83 1 es 3 1081 46°45 i i 5 110-4 45:58 2 ei . 1155 44:92 1 3 F 119°1 44°15 In a4 : 123°6 43°76 1 3 Bs 125°9 43:19 a fc 4 129°2 42:59 i! ” ” | 133°2 42-49 1 ” ” Hoot 42°32 1 Pr 3 | 1343 42:09 1 : Piet 35°6 41°45 3 a 5 139°3 40°80 In ” » 1431 40:53 In 5 F 144-7 39°34 2 F 3 1517 38°84 1 ss : 1546 38°15 1 : P 158-6 37:00 1 e rp 1653 36°68 1 a AS 167:2 36°32 1 . * 169°3 35°97 il A A 171:3 35°39 1 3 5 174-7 35°03 1 BS 3 176'8 34:23 In as f 181°5 33°71 2 a2 pS 1845 33:40 2 ” ” 186°3 32°30 1 - fi 192°8 31-98 1 1:13 * 194:7 31:55 1 P4 197:2 30°89 1 re, Ay 201°1 29°9 In 9 » 207 29°65 In _ A, 208°3 29°18 1 rf Aj 211:0 28-52 2 a A 215-0 28-13 i * 5 ‘ 2172 27°65 1d a 2 220°1 27:05 In 3 £ 223°6 2616 1b Z : 2245 REPORT—1900. URANIUM—continued. Reduction to Wave-length _ Intensity ve tte Oscillation Spark and Sea oe ee a | Frequency Spectrum Character | A+ | lig: | in Vacuo Ar | See eS I pe et 4125:3 In bis.) 4 Ge > | 24234 24:92 3 x “5 236:1 24-19 1 - 7 240-4 23°83 1 5 of | 242°5 235 In ” ” | 244 23°3 In 3 + | 246 22°58 In | Ap | 2499 22°39 In 4 7 251:0 21:45 In a 3 256°5 21:0 In - + 259 20°3 i In | 2 | * 263 19:90 In Pa if 265°6 19°1 In ie . | 270 18°59 2 amb a ee pu'| 273-4 17°75 | ln - | ie 278-3 17°10 1 sp aaa uae 282-1 16°6 | In is eae 285 16°30 | 3 eh” eee 286-9 15°10 ] a Fe 293°9 14-82 1 A ; 295°6 14-42 1 # 474:7 84:31 1 | ny ; 476-4 83°85 In = Aa 4796 83:15 In . BS 484-0 82-80 1 f Fe 486'1 82:20 1 | ” ” 489'7 81-45 1 | ” ” 494°] 80°79 3 4 Fa 498-2 80°05 In is E 502°6 79°51 1 a a 5058 79-00 1 | _ 5 508°9 78°35 in | % ss 502°8 W795 1 .s i 505-4. 76°86 2 ce 7 521°9 76:3 1b s i, 525 75°83 In | 5 hi 528:0 74:68 1d » io 5384:9 73°93 1 i 3 539-4 73°80 1 7 e. 540-2 73°38 In Fr 543 73°00 1 < ie 545°0 72°20 1 % ug 549'9 71°63 1 5 oe 553°4 71:30 2 Fe 3 5553 -70°9 | In . Pr 558 70°6 In cf) s 559°5 70:20 1 A 561:9 69°90 1 rp ; 563°7 69°23 1 3 Fs 567'8 69°15 1 ri ” 568°2 222 Wave-length Spark Spectrum 4068°75 67°90 * Pb? Intensity and Character NRHN RP eRe Ee ew on =) ee Lome on REPORT—1900. URANIUM—continued. Reduction to Vacuum 1 r 69 + Fe Oscillation Frequency in Vacuo 24570°7 575'8 5792 581-4 583-4 585 586 587 597-4 600°7 603°8 607-2 612-1 614°5 617-0 621°3 622°0 625 628 630 633-4 635°5 639 644-4 646°7 648°8 652 654-1 654-8 657°3 661 665:0 668°3 671 6718 676 678 683-1 684-7 6862 688-0 692°3 695-0 697-9 701-2 708 768°8 712-4 7143 T7171 720 725 7274 ON WAVE-LENGTH TABLES OF THE SPECTRA OF —UrANIuM—continued. Wave-length Spark Spectrum 4042°63 42-15 41-78 41-23 40°6 39°9 38:8 38°36 38-10 37-2 36°75 363 35°8 35-45 34-67 34:50 34-15 33-93 33°58 32°6 32:00 31:50 30:93 30°57 30°05 29-90 29-27 28°55 28°37 27:97 27°58 27-18 26-19 25°60 25°22 24-9 24-45 24-33 23°76 23-40 23-05 22-95 22-2 22:0 21-65 21:35 21:17 20.35 19°39 19°13 18-65 18-43 17-88 17-65 17-40 THE ELEMENTS. 223 Reduction to Intensity Vacuum Oscillation and Frequency Character 4 ji_ in Vacuo A 1 111 70 2472974 In ” ” 73273 In if " 734-6 In 3 5 738-0 In ” ” 742 In ” ” 746 lb ” ” 753 In i « 75S 1 ” » 7571 1b a > 763 2n p ° 765°8 In 4 * 768 In ” ” 771 In b: 1713-4 1 ” ” 7782 1 » ” 779-2 In a 3 7813 1 ” ” 782°7 1 > 7848 1b ” ” 791 1 * i 794°6 In a i 797-7 1 ” ” 801:2 1 ” ” 8034 In 3 » 806-6 In a fe 807°5 In +) » 811:4 in 7 B $15°8 1 » » 816.9 1 ” ” 819-7 1 Pr Le 8221 1 ” ” 824-5 2 ” ” 830°8 T » ” 834-0 1 ce) ” 836°4 In ” ” 838 1 ” cB 841-1 In Fr 9 841°8 In ” ‘9 845-4 1 » » 847 6 In ” ” 849°8 in ” nh 850-4 In ” » 855 In ” ” 856 In ” ” 858-4 In ” ” 860°3 i! ” ” 861°4 1d ” ” 8665 1 ” ” 872°4 1 ” ” 874:0 1 ” ” 877:0 1 ” ” 878°8 2 ” ” 8817 1 ” ” $83°2 1 ap y 884-7 REPORT—1900. URANIUM—continued. | Reduction to urease | ty Vacuum Oscillation park an ) FE Spectrum Character ea Le in Vars A | ae de 1 stant en a Boe 6..5* | Se 101702 1d tov aera 704. | 24887-0 "De j - fee [trac | eel ene 3920 ae 1 1:10 age 896°1 ote 3G 199 ; : sii ah : is M 901-4 “35 a * 903°7 13°6 In = | es 908 ; van 1 Sen 910-1 12-60 : ey ee a are 2-60 - a 9145 12°38 1 3 a 915-9 12-03 1 a :, 918-0 11-93 1 ¥ 918-7 1164 ld e s 920'5 11-20 1 1 - 923-2 11-00 1 k 924-4 10°88 1 ip cs 925°1 0973 1 See 9393 ode | ” 3 09-60 1 tee ie ae 933°1 . ' 2 03°89 1 : 9376 08-59 | 1 eS 939°4 08-22 In € 941-7 08:10 1 " < 942°5 mee. | ee ee i ” ” 9 3° 07-28 1 2 2 945'6 07:13 1 a ¥ 946-6 ( eeeereee, a8 05°83 : | aie if a 05:40 1 i if 959°3 05°00 1 “3 i | 961°8 ee : ; 968-7 . | “5 on 963°7 04:30 | 1 _ y 966"1 04:20 1 |: reaegs jy. 966'8 03°95 1 a a 968°3 03°58 i i“ i 970°6 03:32 1 i i; 972-2 02-14 1 : : 9797 : . 979-7 01°82 1 = 9815 01-40 1 - i 984-1 01:08 1 . s 986:2 00:87 1 . 987°5 00°47 1 we Bie 990-0 Sc ne oe ar 99°33 In ti ets | * ere 98-95 in alls 15a 999'7 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 22 UBANIUM—continued. ~ (3) Wave-length Spark Spectrum 3998-36 97°49 97:26 96°90 96°1 95°67 95°17 94°42 94:0 93:2 92°70 92°35 91:9 91°75 90°61 90°24 90:10 89°47 89:02 88°78 88°50 88:18 86:87 87:19 87:03 86°60 85°95 85°19 84:90 84:70 84:33 84:03 83°45 83'1 82°69 82:27 81:93 81-71 81:06 80°95 79°92 79°67 79°27 78°95 78-4 77-50 717-22 766 754 75-13 74:70 74:50 7415 73°40 72°51 1900. Intensity and Character Bee DEER He EEE BB > ss i al laced = BB BRR ee Hee olen eae ee Bo oe BB Reduction to Vacuum Oscillation Frequency in Vacuo 249934 998-8 25000:2 012°3 017°5 020:2 023°3 028-0 030°5 0355 038°6 040°8 044 044°6 051°7 054:0 055°5 059-2 061°2 063°8 065-0 067-0 069:0 073°2 074°2 076:9 081:0 * 085'8 087°6 088°9 091:2 093-1 096:7 099 092°6 095-1 097°3 098°7 1118 112°5 1190 120°6 123°1 1251 129 134°3 1361 140 148 1490 152°0 153'3 155°5 160°3 165°9 226 REPORT—1900. URANIUM—continued. Reduction to Wave-length Intensity | \ canes Oscillation Spark and | | Frequency Spectrum Character | A+ it in Vacuo | A | | 3971°58 1 1:09 | fis | 25171°8 | 713 In ” 99 174 70°75 1 | a 1770 70°60 1 i | a 178-0 70°30 1 5 2 179°9 69°55 1 ; i 184°6 69°23 1 he sa 189°2 68°63 2Ca ia “A 190'5 68°16 1 . an 193°5 67°8 In - A 196 67°6 in “ + 197 67°25 In | i i | 199°3 66°73 2 | a = 202°5 66°5 | In py A! 204 66°10 i oa = 206°6 66°00 M aie a 207°2 65:43 1 3 | “ | 210°8 65°15 i a 5 212°6 64:85 if - rs 214°5 64°32 1 an Bs 217°9 63°13 i 9 . 225°6 62°95 i - ed 226°7 62°60 1 i . 228°9 62°43 1 | es * | 230°0 62°18 1 y 7 231°6 61°88 In | FA 5 235°7 61:70 In a: < 234°6 61:29 1 ss 7 237°2 61:00 il a : | 239°0 60°70 1 5 5 241°0 60°4 In me s 243 59:9 1b Be as 246 59"5 1b in 2 249 58°3 1b - a 256 57:97 1 *s pe 258°4 57°65 al PD rr 260-4 57°50 1 - a” 261°4 57°08 1 es | oe | 2641 56°72 1 Pa F 266°3 56°45 In aa Ee 268:0 56:2 1n os 72 ) 270 55°91 1 - | 2 271°5 55°55 1 a | 5 273:7 54°87 2 a as 2781 54:40 1 a | me | 281:1 53-75 1 Ps a 285°2 53°13 1 3 e | 285°9 52°67 In An “5 289-0 52°45 1 et 293°6 52°03 In . j a 296°2 61°75 In i / th 298°8 50:90 1 es a i 303°5 50°27 1 rs 5 | 307'5 49-69 1 | 4 i oe 311-2 49 44 1 = a 312°8 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 227 URANIUM—continued. Reduction to Wave-length | Intensity Vacuum. Oscillation Spark | and Frequency Spectrum | Character 1 in Vacuo A+ az 3949-20 1 1:09 7:2 | 253144 48°54 1 n .; 318°5 48:13 | 1 a | A 321:2 47:05 In PP Pa 328°2 46:88 1 4 - 329°3 46:40 1 | : as 332°3 45°88 In 7 | Ff 335°1 | 45-45 1 4 es 338'5 | 45:10 i PP BS 340°S 44-77 1 is Pr 342'9 44°32 2 “A ” 345'8 43°97 1 re Pe 348°1 43°68 1 Z 33 350'0 43-00 1 > Fe 3542 42°71 1 Pe Pe 356'1 | 42°43 1 * 3s 357'9 | 42-22 1 59 2 359°2 | 41°60 1 a i 363°2 41:26 t Fe a 365-4 40°80 1 Fe z 367-4 40°64 i =f is 368-4 40:45 1 a Rs 369°6 39°93 1 i - 3780 39°56 1 of PB 380°4 39°27 in B Fe 382:2 | 38°57 In . * 3827 38:00 In of a 386°4 37:23 1 3 re 3913 36°88 | i 1:08 PS 393°6 36°55 ld ‘3 Fe 395°7 36°18 i 45 fi 3981 35°52 2 - | i 402°4 34/9 in | e | is 406 ° 33°92 i or rc 412'8 33°81 4Ca + i 413°5 33:18 1 ch oA 4176 32°20 3 on + 424-0 31°65 | 1 | 4 cs 427°6 31:37 / In e . 429-2 31:15 2 a a 4£30°6 31:0 In i = 432 30°58 iH * as 4343 30°22 1 KS iz 436°6 29:90 1 of “ 438°7 29:38 1 ' 442-1 29:22 1 3 7 443-2 28°95 1 s _ 444-9 28°60 i * % 447°2 28°45 1 Fe xs 448°5 28:20 i A 3 449°8 27:92 1 ; 5 451°6 27°10 il a 5 4569 26°90 1 | 3 458-1 26°45 In is 3 4611 25:7 In } “3 7 | 466 228 REPORT—1900. UrantuM—continued. Reduction to 5 Intensit: Vacuum Oscillation Wave-length and “f ee Frequency g Spark Character 1 in Vacuo pectrum A+ eS A 3925°45 ln 108 V2 25467°6 25:17 In ee ¥ _ 469-4 25:0 In »” » 470°5 24°67 1 Ry 5 472°7 24°45 1 “ =p AT4:1 24-11 1 ob sy + 4763 23°8 In a “yes 478 23°5 ln ” 5 480 23:25 1 “9 ro 481°8 22°60 1 ” a 486:1 22°35 1 ” ” 487-7 22°18 1 ”» “5 488°8 21°74 1 ” “3 491-7 21°40 1 ” ” 493°9 21:2 In + “A 495 20:07 In i 498-4 20:05 In 7 ” 499-7 19:95 In ' + 503°3 19:49 1 a) ah 506°3 19:22 1 ” ” 508°0 18°57 1 ” ” 612°3 18:27 1 A =) 5143 17:96 1 *” * 516°3 17:78 1 9 cr 617'5 17°55 1 53 1 518:9 17°45 1 ” 3 519°6 17:18 1 ” +, 21:4 16°75 In ” §24°2 16:60 In 7 = §25°1 16:05 2 A “5 5628'S 155 In ” ” 532 15:20 1 05 A 534:°3 14:94 1 » oy 536:0 14:45 3 as > 539°2 14:0 In ” a 542 13°63 1 * 3 5445 13:48 1 a 55 545°5 12°95 1n ¥) A 549°0 12°60 1 ” 73 55171 11:90 1 a * 555°7 11°45 ln 45 ” 558°8 11:15 In or 5 560°7 10°67 1 i "f 563'9 10:37 1 * » 566'8 09°88 1 53 A 568°9 09°22 1 » a 573:2 09:10 1 a 43 574:0 08:60 In on > 577°3 08:01 u ” 35 581:2 07°72 1 rr a 583°1 07:42 1 ” = 5851 07:17 1 oH ” 586°8 06:7 2b rs nn 590 06°1 1b ay if 594 05 00 il “f 7 600°9 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. URANIUM—continued. 229 Wave-length Spark Spectrum 3904-73 04°44 04:06 03°47 03:13 02:70 01:75 00°48 389998 99°64 99°24 98:97 98:1 97°87 97:44 97:22 96°92 96:27 96:07 95:82* 95-41 95°20 94°89 94:26 93:96 93°48 92°85 92°56 92:22* 91:93 91:22 90°51 89°54 88°72 88°32 87°85 87:36 86°6 85°83 85:12 84°83 84°47 84:09 83-4 83°20 82°79 82:52 82°05 81°61 80°8 79°88 79°73 79°12 Intensity and Character Wr St Ph Ps it Ys fat aa BBB EAA SS tnt ber eh Pn Ph 0 rad Pps tf te Ps fe ds er ND: Fr i=) ating ad gical al aaa Reduction to Vacuum 1 A+ : 1:08 i st: ” ” ” ” ” »” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” 1:07 = Oscillation Frequency in Vacuo 25602'8 604°6 607:2 611°0 613-2 6186 622°3 630°6 6339 63671 638°7 640°5 646 648°7 650°6 652'0 654:0 658°3 659°6 661:2 663°9 665°3 667°4 671°5 673°5 676:7 680°8 682°7 685 0 6869 691°6 696°3 702°7 708-1 710°8 713°8 717-2 722 7273 7319 7338 736°2 738-7 743 744:6 746°8 7478 7509 755°6 761 7669 7679 761°9 30 REPORT—1900. URANIUM—continued. Reduction to Wave-length Intensity Vacuum Oscillation Spark and — SS ee Saas Frequency Spectrum Character en 1 in Vacuo A 3878°23 2 1:07 73 2577177 7760 In a a 7819 7750 in 5 i 7825 771 In Xs “p 785 76°75 1 4 a 787-4 76°48 1 ” + 784:2 76°28 1 7 * 790°5 75°66 1 + aA 7948 75-15 In oy an 7981 74:68 1 + an 801°3 74:20 2 5 oF 804°5 73°28 il ” ” 810°5 73°22 if - + 811-0 73°03 1 *) + 8122 72°70 i 5 st 814-4 72°50 1 PA on 8158 72-06 1 7 + 818°8 71-69 1 “5 A 821°3 71°52 1 aS ri 822-4 7118 it + + 824°6 70°73 1 o a 827-7 70°22 1 x 5 831-0 69-90 1 » oF 833-2 69°05 1 5 - 838°8 68°95 1 oF Be 839°5 68°57 1 54 ne 842-0 67°32 1 a ” 851-2 67:17 1 ip 7 852°1 66°89 1 5 + 8539 66°62 1 of > 855°7 66:08 2 es & 859'3 65°65 1 (Fe) + + 862°2 65°26 EL a oa 864 ‘7 64°85 In re a 866°9 64°65 1 i os 868°4 64°48 iT 53 o 869°5 64:24 ii . * 871-1 63°90 1 aS or 873'3 63°57 1 aS .. 8755 63°25 In 4 7 877°6 62°45 In n FF 882°9 61°9 In “A 7 887 61°30 1 + 3 890°8 60°75 In - > 894-4 59°75 3 x x 901°1 59°16 1 ds 7 905:0 58°8 in a a 907-5 58°35 in 35 *) 914-2 57°8 in . se 914 57°35 In te 917:2 56°94 1 1:06 z 919°9 56°74 1 5 a3 921:°3 56°5 In (Fe) 7 ” 923 55°96 1 a = 926°5 55°60 1 929:0 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 231 URANIUM—continued. Reduction to . Wave-length . Intensity | he Oscillation Spark ‘| and -| Frequency Spectrum | Character ae ae in Vacuo A | | | 3855-00 1 | 1:06 73 25933°0 54°80 2 5. 3 934-4 54-42* 1 ee a : 987°0 53:95 1 + 3 94071 53°53 1d + . 942-9 53°16 1 fr 3 | 945°5 52°86 In Fe Fe 947-4 | 52:28 In 3 _ | 951:3 | 52-0 In % #9 953 51°45 | 1 P: “3 | 956°9 51:10 il x 3 959°3 50:95 In . <3 960°3 50°5 1 ” ” | 963 49°87 1 | 7 # 967°6 49°6* | In - - 969 48-9 | In | a 3 974 48-77 1 ” 6 9756 48-24 1 ” Sr 978°6 47-95 In ” “1 980°6 47°25 In sp is 9853 46°70 1 “5 Pe 989-0 46°38 1 + FS 991°2 45°98 1 ” Fe 993°9 45°50 2 ” eS 26997-1 45:27 1 3 Fe 998°6 44:85 1 ~ Fr 991°5 44:33 In | 7 D 995-0 44-13 1 3 3 996-4 43°92 1 ae i 997°8 43°61 1 3 by 999°9 42°86 1 ro % 015°0 42°36 1 on a 018-4 42-00 1 + Pe 020°8 41:20 1d (Fe) é Ps 026°2 40°50 1 3 % 031:0 40:05 in y x 034:0 39°77 1 a “- 035'9 39°63 1 of “1 036°9 39°15 2 ec Ee 040°2 38°28 2 = ¢ 046°1 37-95 1 “5 mC 048°3 37°63 1 = a 0504 37-40 1 - ” 052:0 37-0 In ” % 055 36°6 In | fr Si 057 36°45 In | » a 058°3 36:05 1 ee z 061-2 35°25 1 = Fe 066°6 | 34-94 1 3 y 068°7 | \ 34-72 1 a a 070°2 | | 33:90 - 1 57 0758 33°16 1 | 7 i 080'8 82°75 1 ” ” 083°6 232 REPORT—1900. URANIUM—continued. Reduction to Wave-length Intensity eo Oscillation Spark and LT | ay oo ee ee Frequency Spectrum Character ae 1 oe in Vacuo r | 3832°07 i 1:06 73 26088-2 31:60 3 oa 3 091°4 30°77 1 i - 097-0 30°36 1 4 a 099-8 29-95 f ‘4 Z 002-7 29:50* 1 . ‘ 1058 29:20 1 id i 107°8 28°92 i +5 a 109°3 28-22 1 q _ 1145 27:93* 1 * a 116°5 27-56 1 4 ‘ 119-0 27-02 1 i c 122-7 26°65 2 ce i 125-2 25°61 i 4 : 132°3 25:29 1 st f 134°5 24-85 1 id , 1375 241 In x . 143 23°62 1 » ” 146:0 23:26 l c 3 148-4 23°10 1 i = 149°5 22-71 1 i : 1522 22°56 1 ” ” 153°2 22/14 1 is ee | 1561 21-38 1 : ‘ 161-2 21:15 1 is 162°8 19:46 1 % + 174:4 19°19 1 i 3 1763 18°86 1d 3 i 178'5 18-62 1 if 2 180-1 18-28 1 # ae 182°5 17-80 1 4 3 185°7 17°30 1 . T4 189-1 16°75 1 1:05 % 192°9 16:22 1 re : 196°5 15°50 1 5 zs 201°5 15°30 7 a x 2 202°9 14:96 il ee Es 205-2 14°25 2 fe A 2101 13-94 2 i A 212°2 13°40 1 ‘, e 215'9 12°86 1 7 ¥ 219-6 12°72 1 < # 220°6 12-42 1 Bie A 229-7 12:16 1 af s 224-4 11°81 1 . 5 226°8 11-67 1 . E 227°8 11-20 1 ; < 2311 11:05 1 as , 232°1 10°33 1 "4 “* 237-0 09:73 In i‘ & 241-2 09:36 1 i s 243-7 09:12 1 if 2 245-4 08°35 In 5 ” 250°7 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS, Wave-length Spark Spectrum 3807°75 07-4 06°5 06:40 05:99 05°83 05-20 05:00 04:52 04:1 03°50 03°25 03:00 02°43 02°10 01:90 01:45 01°35 00:9 00:43 00-30 3799-75 99°36 98°99 98°40 97°93 97-70 97:2 96:98 96°70 96°62 96°38 96°20 95°76 95°29 94°50 94:15 93°74 93°45 93°24 92°69 92°50 92°03 91:50 91:25 90°94 90°50 90°36 90:03 89°76 89°36 89:02 88°77 88°37 88:15 URANIUM—oontinued. Intensity and Character ad or a i ag ag a as a a a a acca Reduction to Vacuum Oscillation Frequency in Vacuo 26254'8 257 263 2641 267:0 275:0 272°4 273°8 2771 280 2842 285°9 287°6 291°6 293°9 295-2 298-4 299:0 303 305-4 306°3 31071 312°8 3249 319-4 322°8 324°3 328 329-4 331°3 3318 333°5 3347 337°8 341°1 346°5 349:0 351°8 353'8 355°2 3591 360-4 363°7 367°4 369-1 371:3 374°3 375°3 377°6 379°5 3822 3845 386°3 389-1 390'6 9 = 33 bo oo rg REPORT—1900, URANIUM—continued., Reduction to Wave-length Intensity Gee Oscillation Spark and lia a io oan Frequency Spectrum Character Ae slg in Vacuo A | 3787°40 1 1:05 74 26395°9 | 86:99 1 “5 os 398°8 86°74 1 | 4p i 400°5 86°30 In 5 ” 403°6 85:5 In 4 = 409 85°30 1 + 5 410°6 84:90 1 | 3 - | 413°4 84:02 1 5 = 419°5 83:80 In 5: ‘As 421-1 82°99 2 * is | 4267 82°5 1b 5 B 430 82-1 1b 35 $5 433 81:60 1 PA * 436°4 81:33 i! 5 - 438°3 81:23 1 as 2 443°6 | 80°90 2 ” ” 441°3 | 80-44 1 <) os 444-5 | 79°3 In ” ” 453 | 79:18 1 5 if 453-4 78°75 In a i | 456°4 78:5 In . i, | 459 7815 1 4 e | 460°6 77°83 1 Re a 462-9 77°61 1 - 7" 464-5 77°50 In - 465-1 7717 1 , 467-2 76:87 1 1:04 wt 469°3 76°63 1 = , 471-0 | 76°15 1 “3 7 ATA3 (574 il ‘ 3 4769 75°65 1 ‘s 3 477-9 75°42 1 a e 479+5 75:02 1 ap, 482-3 74°57 1 4 ¥ 485-5 74:22 1 a ry, 488-0 73°82 1 53 ¥e 491-0 73°72 | 1 ‘2 493-7 73°57 1 4 3 492-7 | 72-97 2 E, - 496-9 72°50 1 # U5 500-1 71°55 1 x 3 506°8 70°60 1 BS D. 513+5 | 70°30 1 F $s 515-6 | 69°68 OO he 2 im, 519-8 . 68°95 1 - a. 525-0 68°67 1 a 3 527-0 68°57 ] # A 527°8 68°22 In = 7 | 530-1 | 68°02 In 4 R | 531-5 67°62 1 a a 534-3 . 67°33* 1 of B! 536-4 67:05 1 ee a 538-5 66°6 1b - is 542 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. URANIUM—continued. 235 Reduction to Wave-length Intensity Vacuum . Oscillation Spark and Frequency Spectrum Character nf ‘es in Vacuo A 3766:00 1 1:04 75 26545'9 65°47 In + P 549-6 64°95 In Pe 4 553°2 64-71 1 Fy Fe 555°0 64°30 1 2 a 557-9 64-00 1 F 4 560°0 63-43 1 PA % 564:0 63:13 1 ” » 566"1 62°89 1 * FA 567°8 62°27 1 3 4 572°2 62711 1 * 5 573°3 61°74 1 % 9 575°9 61:23 1 x m 579°5 61:02 1 Rs 581-1 60°5 In is “ 585 60-00 1 s 5 588-2 59°38 2 i PA 592°6 58-2 In i 3 601 57-09 1 is BI 608-9 56-82 In is % 610°8 55-7 1b > iy 618 55:2 1b ; Pe 622 54-46 1 ‘ i 627° 54-12 1 3 FA 629°8 53°85 In es a 631:9 53-7 In FS Fi 633 53°22 1 pS i 636:2 53-02 1 - Pa 637-7 52°84 1 3 s 639-0 52-49 di _ 3 644°4 52°30 1 . 5 642-9 51:92 1 An P 645-6 51°46 1 a é 648°8 51:3 In 5 F 650 50-51 1 = i 6555 50°14 1 * 3 658:2 50-02 1 a PA 659-0 49-35 1 5 FA 663'8 48-90 2 - a 667°0 47°34 2 a % 668°7 46°82 In 5 a 6782 46°60 2 ce A 683:3 46:10 In f 5 686°9 45°75 1 ” ” 689°3 45°53 1 + i 690°8 45°15 1 35 ¥ 693-7 44-95 FE ” | ” 695°1 44°65 1 , ) ” 697-2 44°39 1 +3 n 699-0 43°97 ld : A 702-1 43°55 1 " BS 704-9 43-07 In 3 4 7086 42-96 1 : | 709°3 42°67 In ¥ . (I) 3 42°50 1 7126 236 Wave-length Spark Spectrum 374187 41°56 41°43 41:12 40°85 40°4 39°50 39:18 38°80 38°48 38°23 37°45 36°75 36:2 35°7 35°05* 34°83 33°95 33°75 33°25 32°77 32°43 319 31°64 31:10 30:98 30°37 30:00 29°49 29-00 28°60 28°01. 27:91 27°30 27:02 26°72 26°49 26°22 25:93 25°80 25°55 25°26 25°18 24°50 24°35 23°85 22°92 22°6 21:95 21°55 20:54 20:13* 19:75 REPORT—1900, URANIUM—continued. Intensity and Character Reduction to Vacuum Oscillation Frequency in Vacuo DH RR eee eo op NON Re 5 Cellet el ae oe oe Bee ee j=} BDH eee a BBB 26717:0 719°3 7202 7224 7243 728 734:0 735°3 7380 740°2 742:0 7475 7537 758 761 766'6 767'4 T73°T 7152 778-7 782°2 7846 7885 790°4. 794°3 795-1 799°5 802-1 805°6 805°3 8122 8165 8171 821°5 823°5 828°7 827°3 829-2 8313 832-2 8340 856°1 836°6 8416 842°5 8462 853°0 855 866:0 862°9 8701 873°2 875'9 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 237 URANIUM—continued. Reduction to Wave-length Intensity Vacuum Oscillation Spark and ————S Frequency Spectrum Character 2% de, in Vacuo + x 3719°50 1 1:03 16 26877°7 18-98 In ” ” 8815 18:78 1 ” ” 882°9 18°25 2 ” ” 886°'8 17°60 1 » ” 891°5 17°23 1 ” ” 8932 16:95 1 " 1 895:2 16°72 1 ” ” 896'9 16°32 1 ” ” 899°8 15°85 1 ” ” 9041 15°63 1 % > 905°7 15:15 1 ” ” 909-2 14:93 1 ” ” 910°8 14:60 1 \ ” ” 913-2 14:40 1 7 ee 9146 13°95 1 ” ” 9179 13°82 1 ” ‘a 918-7 12:4 1b ” ” 929 11:98 1 ” ” 932:2 11:10 1 ” 1% 938°6 11:00 1 5 Fe 939°3 10°73 1 ” ” 941 2 10°36 1 ” + 948°4 10:05 1 -s ‘ 946:2 09°65 In ” ” 949°1 09:45 In cf . 950°5 09:2 In ” F 952 08°75 In ” ” 955:7 08°10 1 ” ” 960-4 07-80 1 9 ” 962°5 07°45 In 7 3 965:0 06°86 1 "7 2 969-4 06°10 2 ” ” 974:9 05°72 2 ” ” 977'7 05:20 1 ” 981°5 04°50 1 ” ” 986°6 04:25 1 “ Pp 988°4 03°80 1 ” ” 991-7 03°45 1 ” A , 994:2 02-80 1 ” ” 999-0 02:38 In " a 270021 01:9 1n ” ” 006 01:68 2 ” ” 007°3 00°74 1 ” ” 0141 00:00 1 ” 9 019°4 3699°83 1 ” ” 020'6 99:60 1 ” ” 022°3 98°63 1d ” ” 029-4 £810 iL ” ” 033°3 97:69 1 1:02 3 036-4 97°32 1 7 r 039°1 96°98 1 aa of 041°5 96°48 1 i 7 045°2 96°25 1 7 cf 046-9 | 95-98 1 f ‘, 048°8 238 ; Wave-length Spark Spectrum REPORT—1900. URANIUM—continued. Intensity and Character Reduction to Vacuum Oscillation Frequency in Vacuo 3695°35 94°95 94:46 93:89 93°46 93-08 92:48 92°15 92:07 91-65 91:15 91:00 90:43 90:18 89-80 89°37 89:19 88:93 88:53 $8-02 87°88 87°55 87-27 87-12 86:93 86°63 85:94 85:71 85°45 84:77 84:45 | 84°30 83°75 §3:00 82°63 82-25 | 81:85 | 81:07 80°68 80°45 80:10 79:99 79°54 73:93 78°3 1182 77°60 172 16°75 15°75 15°26 15:19 74:90 74:25 73°56 Bee Eee Ee ee EP Ee eee eee i=] PRR RR Re Q PREM RP RHEE 270534 0563 060:0 064:1 067°3 0701 074-4 079°6 077°5 080:5 081°6 085°3 084-2 091-3 0941 097°2 098°6 100-5 103'5 107-2 108-2 110°6 112-7 113'8 115-7 117-4 122°5 124-2 126'1 1311 133-4 134-6 138°6 144-1 146'8 149-6 152:6 158°3 161-2 162:9 165°5 1663 169°6 1741 179 182°3 184-0 187 190-2 197-6 201°3 901:8 203-9 208°7 213'8 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Reduction to Wave-length Spark Spectrum 3673-22 72°75 71:98 71:75* 70°7 70:40 70°26 69-50 69:33 68°90 68:25 68:13 | 67:9 67:30 66:95 66:35 66:28 65:6 65:3 64:92 64:69 64:40 64:0 63°5 63:2 62°8 62:50 62°10 61:60 61:47 60:90 60°5 60:27 59:76 59:28 59:19 58-8 58:30 58°01 57:50 57:09 5680 ! 56:40 56°30 56:09 5561 55°35 55:06 | 54:80 | 54:43 54:25 | 53°65 | 53°34 URANIUM —continued. Intensity and Character Vacuum A+ <- 5 BRR BEE EHP Re Re ERP RPE ERR Re Oscillation Frequency in Vacuo 27216°3 219°8 940 REPORT—1900. Uranrtum—continued. Reduction to Wave-length Intensity imate Oscillation Sp ark and Frequency Spectrum Character Ae ; - in Vacuo 3652°21 1 1:01 7:7 273730 51°6 1b ” ‘ 378 50'8 1b ” B 384 50°55 In ” 3 385°4 50:16 1 ” e 388°4 49°83 1 ” a 390°8 49°53 1 59 3931 49:02 1 ” a 3969 48°65 1 ” 5 399°7 48-27 1 ” = 402°6 47:9 In » s 405 ATT In +: yi 407 47-00 1 5) ms 412-1 46°63 1 a 3 4149 46:13 1 4 ; 4186 45°82 1 ” . 421:0 45°60 1 » 3 422°6 45°19 1 ” if 4257 44°93 1 ” a 427°7 44:38 1 ” “0 431°8 43°75 1 ” y 436°6 43-2 1b ” 3 441 42°95 1 “6 i 442°6 42°59 1 ” iS 445°3 42°20 1 » ¥ 4482 41°37 1 + i 454:5 41:09 1 s 3 456°6 40°84 2 5 = 458°5 40°17 1 ” si 463°5 39°75* In + a 4667 39°31 1 ” 7°83 469°9 38°79 1 ” a 4739 38°33 1 a 477°3 38:03 1 F af 479°6 37°63 1 0 ss 482°6 36:7 1b a uf 490 36°3 1b s + 493 35-74 in 5 3! 4969 35°45 1 9 a 499-1 85:17 1 a . 501-2 34:70 1 * a 5048 34:40 In a 5 507-1 33°42 2 - a 514°5 33°05 1 55 s, 517°3 32°9 in a 5 518 32:33 1 ‘ 4 522°7 32:0 in p z 525 30:84 3 hs “ 534-0 30°40 1 - 53 537-4 30:17 it & 3 539-1 29°70 1 4) t 542-7 29°25 1 > 43 546°1 28°96 1 9 + 548°3 a ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length Spark Spectrum 362851 28-23 27°86 27:60 272 26-95 26°80 25°65 25:25 25:00 24°75 24-49 24-00 23°6 23°21 22°83 29°45 22:25 22:00 21:72 21:65 21:20 21:03 20°68 20°31 19:95 19:56 19°32 18:94* 18-65 18-2 17°72 * 17-28 16:90 16-49 15-98 15:6 15-42 15°15 14-85 14-4 14:16 13-95 13°55 13:30 12:88 12-7 12-06 11:85 11-44 11:20 10:87 10-65 1900, URANIUM—continued. Intensity and Character RNP EE Ree RBBB Bee eee BB B as Pa re ee ee BB =} DNR ERE Reduction to Vacuum —_ A 78 Oscillation Frequency in Vacuo 27551°7 5539 556:7 558°6 562 563°6 566:2 573°5 576°5 5784 580°3 582°8 586:0 589 5920 5949 5978 599-4 601°3 603-4 603:9 607°3 608-7 611°3 614-1 616°9 619°9 621°7 6246 626°8 630 6339 637°3 640°2 643°3 647:2 650 651°5 653°6 655°9 659 6611 662°8 665°8 667°7 670'9 672 677°3 678'8 682°0 683'8 686"4 688-0 241 949 REPORT—1900. URANIUM—continucd. Reduction to Wave-length Intensity ih cies Oscillation Spark and Frequency Spectrum Character AE 1 in Vacuo a 3609°86 2 1:00 78 276941 09°53 1 | ” | ” 696°6 09:13 1 | _ a 699°7 08°84 1 ” 3 7019 08°55 1 ” | ” | TOL2 08:20 1 ” ‘ 7069 07:97 1 ” ” 708'6 07:18 in ” F 713°9 07°52 1 ” ” 712°0 07:15 1 ” ep 7149 06°51 2 ” ” 719°8 06:26 1 ” 9 721°8 06:00 1 ” = 723'8 05:90 1 ” DO 724°5 05°65 1 ” a 726°5 05°35 1 ” 7 728'8 04:80 1 ” 5 7331 04:58 1 ” 4 734-7 04:35 1 ” 5 736'5 03°95 1 ” ” 739°5 03°65 1 FA ” 741°8 03:28 1 ” mS TAT 02°67 1 ” 7A9°4 02°45 In “A p 7511 01°6 In D yy 758 01:3 1b ” ay 760 00'9 In *» x 763 00:7 In 5 os 765 00°02 2 ” ” 7698 3599'50 1 ” a 7738 99°13 1 a5 . 1768 98:72 1 ” op 7799 98:4 In “4 if 782 98°25 In rH “1 783°4 97°95 1 * 9 785'8 $7:78 1 7 ” 786°2 97°40 1 “A ‘1 7891 97°31 a 5 MD 789'8 97:01 1 ” 4 7931 96:2 In ” + 799 95°69 1 ” rh) 803-4 95°14 | 2 ” ” 807-6 94°25 ld H s 8143 93°88 1 + 79 817-1 93°68 1 PY rn 818°1 93°40 1 p Fy 820°9 92°92 ld os 7 824:7 92-50 1 A ” 827°9 92-03 1 H + 831-4 91:74 1 0 5) 833°6 91°4 In a 3 836 90°71 1 A + 8419 90°48 1 1) 7 843°6 901 1b ” Pr 846°5 ' 89°9 lb ” ” §48 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length Spark Spectrum 35893 88°5 88:05 87-70 87:2 865 86:02 85°54 85°33 85:05 84:13 83°6 83:4 83:00 82:23 82:02 81:41 80:45 80°30 79°96 79°56 79°12 78:97 78:53 781 717-26 77:05 76:78 76-41 75:97 75°64 74:98 T7455 74:25 73°40 73°10 72-75 72:55 72:27 71S5 71:42 CUA) 70°80 70°34 70°05 69°85 69°72 69°25 68:97 68°83 68°45 68:19 67:97 67°65 67:18 URANIUM—continued. Intensity and Character BPR HE Ree ee so +2 i=} B CN NN el ee ee ee ee Reduction to Vacuum 243 Oscillation Frequency in Vacuo 27853 859 862°4 865'1 869 8745 878:3 881:9 883°5 885°6 892°5 897 899 901°7 907'8 909°4 914:0 921°2 922-7 925-6 928-6 9319 9330 936:3 940 946°7 948°3 950°3 9531 9564 9589 965°3 9685 970°7 9767 9791 982-0 983-6 985°7 988'8 992°0 993°8 997-6 28000°4 002°5 004°4 0084 009'2 011°4 012°5 015°5 017°6 019:3 021°8 025°6 R2 REPORT—1900, URANIUM—continued. Pebiehon miele | ee ' : to Vacuum scillation ae | a ee Spectrum Character 1 in Vacuo At - ay | bere S| 3566°78 04 0:99 19) 28029°6 66°55 1 a4 Hs 030 2 65°93 2 y a 0351 65:56* a ; . 0381 65:20 In 3 a 040°9 65:07 1 a 041°9 64:78 1 - - 0442 64:40 A a, yi 047°3 64:1 in 9 ; 050 63°85 1 3s *p 051'7 63°60 1 = “5 053°6 63°50 1 35 55 054°4 63°23 1 - BS (056°4 62°25 In A i 064:°2 61:95 2 = : 066°6 61°62 1 a 5 069°2 61:24 1 65 P 072:°2 60:65 In cs 5 0769 60°5 in - 5 078 60°10 1 a e 081:2 59°21 i Be 3 088:2 58°71 1 4 a 092°2 58:22 1 "s - 096:0 58:00 1 - +9 097'8 DID 1 ¥ Sy 099°8 57°49 1 - - 101'8 67:15 1 a Me 104'5 56°75 1 as 3 1076 56°43 1 os 5 11071 56:05 1 e as 118°7 55°70 1 ., os 115°9 55°52 1 - oa 117°3 55:00 In s 4 121°5 54:70 In 55 Fe 1239 54°43 1 - i. 1260 54-00 In + < 129°4 53°62 In 4 . 132°4 53°1 1b a . 136 52°84 1 , ss 148°5 52°36 2 As 142°2 51:95 in . 8-0 145°5 51°49 1 hs 3 149:2 51:24 1 55 5 151:2 51:02 2 = RS 152°9 60:77 1 as Ba 154:9 50°68 1 * Es 155°6 50:43 1h 3 % 157°6 49°88 In ¥ P 161'°9 49°36 i 2% 5 166:1 48°95 In x ) 169°3 48-4 1k am 3 174 47:96 1 a 177:2 47:70 1 a 5 179'3 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length Spark Spectrum 3547°36 46°90 46°55 46°31 45°86 44°86 44°40 44-1] 43°90 43°58 43°35 42°9 42°5 42°06 41°45 41°15 40°82 40°64 39°81 39°60 39°40 39°10 38°81 38°57 38°35 38°00 37°60 37:23 36:95 36°52 36°25 36:0 35°8 35:3 35°1 34:50 34:23 33°75 33°18 32:97 32°80 32°3 31°85 31:29 311 30°30 29°95 29°75 29°35 29°26 28°87 28°50 28°20 27°78 27:00 URANIUM—continued. Intensity and Character ee be bo bo bo BB Lal sel ell peel cell cel ee ol eee ceed cel elt Ne se oe cel ae ee B i=} B ph Bet sh SSAA et es ptt Jet Rs Lo or 4. Reduction to Mee Oscillation Frequency At Le in Vacuo A 0:99 8:0 281820 ” ” 185°6 ” ” 188-4 ”» ” 190°3 ” ” H93:9 ” ” 201°8 ” ” 205°5 ” ” 207°8 ” ” 209°5 ” ” 212°1 » ” 2139 ” ” 2175 ” ” 221 ” ” 224°0 ” ” 228°9 ” ” 231°4 ” » 2340 ” ” 235°5 ” ” 242°1 ” ” 243°8 ” ” 245-4 ” ” 247'8 ” ” 250°1 ” ” 252:0 ” ” 253°8 0:98 ” 256°6 ” ” 259'8 ” ” 262°8 ” ” 265°1 ” ” 268:3 ” ” 270'°5 ” ” 272 ” ” 274 ” ” 278 ” ” 280 ” ” 284:°5 ” ” 286°'8 ” ” 290°5 ” ” 295:1 ” ” 296'8 ” ” 298°2 ” ” 302 ” * 305°7 ” Pr 310°3 ” ” 312 ” ” 318°2 ” ” 320°9 9 Fe 322°5 3 a 325'7 ” a 326°6 ” a 329°6 > -- 332°6 aD a 335°1 “ A 338°5 ” 344-7, 24.6 REPORT—1900. URANIUM— continued. Reduction to | Wave-length Intensity eeu Oscillation | Spark and | Frequency Spectrum Character A+ <- | in Vacuo | | | 3526-74 1 58 at 80 | 28346°8 26°25 1 3 5 | 350°7 25°98 il 5 * 352:9 25°88 1 5 A 353°7 25°35 1 5 ss | 358°0 24-93 1 35 | ‘3 361:4 24:62 i | aa Pa | 363°8 23°77 2 _ | Es | 370:7 23°52 1 # | i | 372°7 22'9 Ib 35 | 45 | 378 22:72 In * | a 379°2 | 22:22 1 op * 383°2 21-67 1 4 7 3876 20:98 2 by ! Pe 393'2 | 20 15 2 5 fy 399°8 19-91 1 . ¥ 401°7 19-55 ln | 3 na 404-6 19:16 1 | ” | ” | 4078 18-92 1 a | ; 409'8 18°69 1 39 ‘ | 411°6 17:84 1 55 35 4184 17:62 1 ee 4 420°3 17:40 1 Me | x | 429-1 17:23 1 ms 5 423°5 17:03 1 “6 45 425-1 16°65 1 | » » 428-2 15°56 a 5 | 9 437-0 15:43 1 a % 438-1 15:10 i . 3 440-7 14:83 1 59 %3 4429 14:65 In 2 | 444-3 13:85 In ‘ : 450-8 13°56 1 x r 453:2 13°25 1 ” ” 455°7 12:86 1 55 95 4589 12-64 1 a 5 460°7 12-40 i . 4 4626 12:06 1 a sy 465:3 11-80 1 , ; 467-7 11°65 1 ” ” 468'8 11°20 In ” ” 4723 11:03 1 is | - 473°7 10°65 Ind 5 | 5 476°7 10°25 1 4 | 4 480°0 09.85 2 7 | as 483°2 09°52 1 a | 485°8 09:25 1 5 8-1 488:0 09°21 1 4 % 488°3 08:49 In = iy 494°] 07:9 In 9 499 O7:47 1 ‘ x 402°5 07:22 1 1 s 4045 06:95 1 a Hy 4067 06°75 1 5 5 508°3 06°50 | 1 | 5 510-4 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 24:7 URANIUM —continued. Reduction to Wave-length Intensity Meuuae Oscillation Spark and Frequency Spectrum Character A+ +- in Vacuo 3505°65 In 0:98 8-1 28517°3 05:28 1 F sy 520°3 05°20 1 ‘a PA | 520°9 04°85 1 i Pr 523°7 04°62 ib s 5 525°6 04:17 In 5 Pr 529-2 03°97 In * Fp 5310 03°50 In . 8 534:8 03°16 In 2 re 537°5 02°79 1 Ee Po 540°4 02°48 In F PA 5430 01:9 1b 35 a 548 01:47 1 5 3 551-4 01:15 Ind 3 AS 554-0 00°65 1 ps x 658-2 00°55 if oS of 559'8 00:27 1 % 7 661:3 349998 1 fe re 563°5 99°53 il x Fs 567°2 99°25 1 “ ss 569°5 98°90 i 0:97 F 572°3 98°78 1 - - 573°4 98°57 1 Me a 5751 98°37 1 “a MY 5768 97:81 1 eS Zz 581-1 97°45 1 5 Ps 5841 97:23 1 _ - 5859 97:05 1 = _ 587°4 96°7 In ” % 590 96°57 1 - * 591-4 96:13 1 i BY 595:0 95°87 1 5 : 597-2 95:04 2 3 A. 604:1 94:19 1 * J 610°6 93°87 1 7 3 613°3 93°52 2 is PB 616-2 92:97 ii 9 sf 620°8 92-4 1b Bs + 6255 92:0 lb < EF 629 91°65 1 + 3 632°5 90:97 1 35 re 6373 90°77 1 + 639°0 90°43 2 as _ 641-6 89°75 2 ra = 647-2 89°53 1 3 4 649:0 89:00 1 3 | BA 653-4 88°35 In _ Pe 658°8 87-75 In = Fe 663-7 87°25 In #5 Fi] 667:9 87:07 In ha FY 669-2 86°47 1 - e 674-1 86:16 1 = Fi 676:7 85°45 # * a 682°6 85:10 1 Es " 685°5 8471 1 . . 688-7 248 REPORT—1900. URANIUM—continued. Reduction to Wave-length Intensity Vacuum Oscillation Spark and Maas? i... 3 Frequency Spectrum Character Na ae) in Vacuo A 348448 1 0:97 8-1 286901 83:98 1 ” ” 694:°7 83°73 In *Y a 6968 83:30 1 5 a5 700°3 82°67 2 ” 93 705°5 82°40 1 aS 4 TOT'7 81:9 1b ay 4 712 81:3 1b D 717 80°49 2 » 5S 723°4 79:99 1 ” 55 727°6 79°40 1 a + 7325 78:47 1 Bs H 7401 78:01 1 ” nS 744:0 77:68 1 x 4 7466 17:26 i 7H 55 7501 76°65 1 i + 7552 76°30 1 as ef 7581 76:08 1 i" > 759°9 75°88 1 = p 7616 75°18 1 " a 7674 74:75 2 a a 7700 74:35 1 5 of T74:3 73°90 In a 3 7780 73°57 In +5 7 780°7 73:19 1 sy 1 783'9 73:00 1 Ps = 785°5 7273 1 or 9 7877 72:67 1 as 788-2 72:25 1 es + (Ser 71:90 1 A = 7946 71:26 1 p oy 7999 70:8 In “5 8:2 804 70°47 1 9 a 808°8 69:96 1 n > 810°5 69:7 1b 3 ae 813 69°38 1 by 5 8154 69:28 1 A ¥ 8162 68:70 In a3 ay 821:0 68°26 In a 8247 67°85 In a 7 828'1 67:3 1b i 833 66°80 1 3 837'8 66°50 1 re aK 839°3 66-05 In es 1 843-2 65°6 Ind ae Hf 847 65:12 1 os 850°8 64°82 1 ss é 853°3 64:41 1 4 6 856°7 63:82 2 3 is 8616 63:50 1 i d. 8643 62°87 In $9 is 869'5 62°40 1 “y “ 873°5 62:17 1 45 = 875°4 61°65 In aS - 879'8 61:19 1 a ‘3 883'6 ON WAVE-~LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 249 UBANIUM—continued. Reduction to Wave-length Intensity yeh Oscillation Spark and Frequency Spectrum Character A+ x in Vacuo 3461-00 1 0:97 8:2 28885°2 60°64 1 ” + 888°2 60 55 1 ~ oF 888°9 60°10 1 tr FF 892°7 59°88 1 % * 894°6 595 In : 898 59°3 In = 7 899 59:1 lb y ro 901 58°85 1 0:96 FF 903°3 58°37 1 . “6 907-4 57°89 2 3 911°6 57:24 2 + y 916°4 56°74 1 rr % 920°7 56°50 1 5 f 922'8 56:1 In os 926 5591 1 os bs 927:9 55°57 1 f a 930°9 55:00 1 5 + 935-4 54°80 In 3 937:0 54°40 In a x 940°4 54:26 1 rp 3 941:2 53°98 1 ra ~ 943°8 53°72 2 9 " 9459 531 In 13 + 951 52°92 In ‘3 55 952°8 52°63 In Bs i 955°4 52°52 In a + 956°3 52°1 1b 2 eS 960 518 In 3 y 962 51°41 2 CF) is 965°5 50°15 In er “6 975°8 49°40 1 5 982°3 48°94 1 7" + 986°3 48°57 1 A: te 989°5 48°36 1 re : 991°3 47°95 In 5 rf 994°5 A747 In a3 5 998°7 46°88 Ik ” » 29003°3 46°73 1 ” ” 004°6 46°47 1 + x 006°7 46:23 1 % a 008'9 46:00 1 6 os 010'9 45°83 1 é + 012°4 45°45 In > * 015-7 45:15 In 7 “6 018°3 44-90 1 + “ 020:2 44°85 1 i * 020°6 44°53 1 + + 023°4 43°97 In cf “ 028°6 43°66 1 4. * 031:0 43°10 1 i. ~ 0354 42°80 1 of = 038:0 42°56 1 9 + 040°5 42°45 1 a + 041°3 41:95 1 A * 045°1 bo REPORT—-1900. URANIUM—continued. Wave-length Spark Spectrum Intensity and Character 3441°65 41:15 40°74 40°37 40:20 40:07 39°58 39°25 38:84 38°56 38-08 37°31 37:18 36:93 36:20 35°65 35°32 34:92 34:70 34°42 33°85 33'6 33:2 32°67 32°15 31°65 31:23 30°87 30:60 30°35 29°47 29°05 28°30 28-06 27:90 27°58 27:20 26°72 26°52 25°97 25°66 25°48 25°25 24°96 24°69 24°45 24°25 23:9 23:16 22°63 22°45 21°85 21°52 21:30 21:17 i i=] PR rt = he ae a Reha Sta het at a is er B BHHE ND HH eH Reduction to Vacuum & r Oscillation Frequency in Vacuo 29047'7 051'9 055'3 058'5 059°9 061-0 065:1 0680 071°5 073°9 077'8 0842 085'3 087'5 093°7 098°4 101:2 1044 106°3 109°2 113°6 116 119°5 123°5 127°'9 132°2 135'8 138°8 141:2 143°2 150°7 1543 160.7 162°7 164:1 166°7 170°0 174:1 1758 180°5 183°4 184:7 186°6 189:1 1914 193°5 195:2 198 204:5 209:0 210°5 215:7 218°5 217°3 221°5 — ee ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. URANIUM— continued. Wave-length Spark Spectrum 3420°67 20:22 20:02 19°72 19°55 19°20 18:73 18°55 18°30 17°62 17:50 17:00 16:70 16°46 16°28 16°04 15°75 15°53 14°80 14°50 14:00 13°50 13°22 12°90 12°50 12°26 11:70 ~ 11:40 11°25 10°75 10°55 10°31 09°96 09°85 09°52 09°36 09°11 08°96 08°74 08°17 08:03 07:50 07:05 06°76 06°44 05°88 05°73 05°32 05:08 04°40 04:02 03°72 03°37 02°90 02°60 Intensity and Character Reduction to Vacuum Ind el al a la Deere BBB ee ee i pg ee ee ke a Oscillation Frequency in Vacuo 29225°7 229°6 231°3 233°9 235°3 232°9 242°3 243°9 246:0 251:8 252°8 257°1 259-7 261°8 263°3 265-4 267'8 269-7 276:0 278°6 282°8 287-1 289°5 292°3 295°7 297°8 302°6 305°2 8055 3108 312°5 3201 3176 318°5 320°3 322°7 324°9 326°2 32:0 333:0 3342 338°7 342°6 345°1 3479 352°7 3541 357°5 359°6 3654 368°7 3713 BT4-4 378°'3 3810 2 2 REPORT—~1900, URANIUM—continued. Wave-length Spark Spectrum 340203 01°37 01-15 00:90 00°66 00°45 00°35 00:06 3399°83 99°64 99°40 98°75 98°40 98°10 97-75 97°30 97:10 96-71 96°58 96°20 95°73 95°48 94°92 94°45 94-05 93°33 93:12 92°81 92°50 91°37 91:19 90°98 90°45 90:10 89°88 89°50 89°21 88°65 88°50 88:17 87:30 86°65 86:26 85°79 85°50 84:7 84°58 84:37 84°15 83°94 83°55 82°80 82°45 82°11 81:00 Intensity and Character lomo a eg Ha ee oa iA lll ral atl A elaine a 6B Pee HE Ee eee bo Reduction to Vacuum Oscillation Frequency in Vacuo 293859 391°6 393°5 395°5 397°8 399°5 400-4 402-9 4049 406°6 408°6 414:3 417-2 4199 4229 426°8 428°6 432:0 433°0 436-2 440°3 442-4 447-4 451°5 459°9 461:2 463:0 465°7 466:3* 4782 479'8 481-6 486°2 489:2 491°2 594:5 597-0 500'9 503°2 506°1 513°6 519-3 522°7 526°8 529°3 536 537°4 539-2 5411 542°9 546°3 5529 556°0 565°0 568°6 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length Spark Spectrum 3380°83 80°37 79°95 79°80 79°52 79:00 78°87 78°40 | 78:15 7755 77°20 76°68 75-95 75°05 74:6 74:32 [4:22 73°84 73°57 73°20 72:74 72:18 71:45 7115 71-06 70°83 70°60 70°28 70-11 69°82 69-4 69:00 68:90 68°44 68:02 67°85 67°68 67:50 66:99 66:70 66°50 65°77 65°30 64:78 64:05 63°60 63°40 62:87 62°15 61:86 61:37 60:97 60°80 60°50 60:27 URANIUM—continued. Intensity and Character ew A dee Ra ae deed Reduction to 253 Vacuum 1 A+ — A 0:95 8-4 ” »” ” ” ” ” ” ” ” ” ” Pr ” ” ” » 0-94 D ” ; ” ” ” ” % ” ” ” » ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” 9 ” ” ” ” ” ” ” ” ” ” 3 8°5 Oscillation Frequency in Vacuo 2957071 574-2 5778 579-1 5816 586°1 587°3 591°5 593°6 598:9 601°9 606°5 612°9 620°8 623 627-2 628-1 631-4 633°8 637-0 640'1 646-0 652°4 6551 656°1 657°9 659°8 662-7 666:2 666°8 669°5 674:0 674-9 678-9 682-6 684-1 685°6 687°2 692°5 694-3 696:0 702°5 7066 711-2 CAEL 721°5 7235 728°5 734-4 737-0 7413 7448 746°3 749°0 7510 254 Wave-length Spark Spectrum 3359-73 59-2 59-05 58-75 58-60 58-06 57°70 57-32 56°65 56:35 5615 56:00 55°56 5524 54-94 54°65 54-22 53°75 53-40 53:20 52:81 51:98 51:83 51:40 51-05 50°80 50°45 50:20 49:56 49°19 48°85 / 48°45 48-00 47°72 47-17 46:87 . 46:56 46°35 46-13 46-00 45°67 | 45-00 44-45 44-9 43-60 43-1 42-83 42:5 41:83 411 40°80 40°47 40-23 39°56 \ 39°37 | REPORT—1900. UnaniuM—continued. Intensity and Character B pr Le pte plac a yo RH RD RR REE ee ee Nore BUBB Reduction to Vacuum Oscillation Frequency in Vacuo 29755'8 760°5 7618 7645 765°7 770°6 7738 7773 783°1 7858 7876 788°9 792°'8 778-0 798'3 799°9 805°7 808°9 8120 812°9 817-2 824°6 825°9 829°8 832°9 835-7 838-2 840°5 845°6 849-4 8525 856-0 860°1 862°5 867°5 870°1 8729 8748 8768 877'9 880°9 8869 891°8 894 899-4 904 906°3 909 9152 922 9245 927-4 929°6 935°6 937°3 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length Spark Spectrum 3339-715 32°00 38°62 38°10 37°93 37:50 36°84 36°42 36°12 35°78 35°4 34:99 34°60 34:40 3410 33°40 32°60 32°12 31°93 31°45 31:12 30°93 30°65 30°50 30°08 29°65 29°47 29°15 28°70 28°40 27°66 27°42 27°20 26°88 26°52 26°32 25°84 25°36 24°77 23°50 23°25 23°13 22°83 22°55 22°26 21°9 21°51 21°37 21:07 : 20°46 19°46 19:00 18°45 18°35 17-99 URANIUM—cyntinued. Intensity and Character B o j=) BREE ER REE ER ERE Re BP PS ee EE ee eee i i=] wl ol ge aaa ah lal a a) Reduction to Vacuum Oscillation Frequency in Vacuo d (Mg) o~ 29939°2 940°6 942-0 948-7 950°2 9540 960°0 963-7 966°3 969°5 973 976°6 980°1 981-9 984-6 990°9 998-1 30001'3 004°1 008°5 011-4 013'2 0155 017-0 022-2 0247 026°3 029°2 033°3 0360 0427 044°8 046°8 050°5 0534 055°2 059'1 063-4 068°5 080 0 082-1 083°5 086-1 088 7 091-4 095 098°3 099°5 002 2 007-7 016°9 1210 1262 126°9 130-1 255 256 Wave-length Spark Spectrum 331762 17°37 REPORT—1900. URANIUM—continued. Intensity and Character Lomo pet dla ah mil alte Is hoe B 6 el el ee eee eee ee ee eee Reduction to Vacuum i A+ == A 0:93 8:6 ”» ” ” ” ” bb) ” ” > ” ” ” ” ” ” ” ” ”» ” » ” ” ” ” bh) %”) 39 ” ” ” ” bb] ” ” ” ” ” 9 ” tb] +e) ” ” ” ” »”» ” ” ” ” ” ” ” ” ” ” ” ” ” bh) ” ” ” ” 9 ” 9 ” +h] ” ” ” ” be) ” th) th} ” ” te) ” ” 39 th) ” th) 2” %” 0:92 as ” ” ” ” ” ” ” ” ” ” ” »” ” ” ” ” Oscillation Frequency in Vacuo 30133°5 135°7 140:0 142 147 1552 159°8 164°4 165:2 167:2 1732 178°8 185 1858 188°8 193 197-1 2045 207°9 208°7 211°3 215'7 217°5 220 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 257 URANIUM—continued. Reduction to Wave-length Intensity Vacuum Oscillation Spark and Frequency Spectrum Character re (ee Be in Vacuo A 3295-95 1 0:92 86 30331:7 95°69 1 iy ” 3341 95°37 1 ” » 337-0 95:00 i 73 : 340°4 94°28 In ” ” 347:0 94:13 1 5 FE 348:2 93°77 1 C5 + 351-7 93°15 1 ne : 357-5 92°51 at rf 3 363-4 91°51 3 ” ” 372°6 91:23 1 Fi ss 3755 91°10 1 99 9 3764 90:63 1 3 . 380°7 90:27 1 +3 n 384:0 89°60 1 ce fh 390°3 89°50 1 % .” 391-2 88°75 1 ” 87 398:0 88°38 2 7 ” 401-4 88:06 1 7 FP 404:4 87°63 2 fr ee 408°3 86'8 In rr Fi 416 86°63 l a Fe 4176 86°42 il rf ; 419-6 86:09 1 7 s 422°6 85°76 1 55 3 425°6 85°44 2 A or 428°6 85:20 1 A 7 430°8 84:80 1 o : 434°5 84°53 1 a s 4371 84:17 1 + op 440°4 83:92 1 . * 442-7 83°30 In <1 % 448°5 82°8 In 4 5: 453 82°68 1 A: oF 454°2 82:3 In 5 5 459 81:83 1 - a 4621 81:70 1 " A 464°3 81:26 il “f a 468-4 80°95 i) ss 470°3 80°80 1 3 a 4717 80°53 1 e i 474-1 80:20 1 7 Py 477-2 79°75 1 * o 4814 79°38 1 % 484-9 79°25 1 “5 5) 486-0 78°6 1b “5 % 492-1 177 2b * 5 500°5 17:27 1 7 Cf 504°5 76°80 1 cs 5 5089 16°32 1 % 5 513°3 756 1b 2 5, : 520 74:70 1 ” 4 528°5 74:40 1 He FS 5313 74:12 1 7 Fs 533°9 73°65 In [ 4 5383 1900. s 58 Wave-length Spark Spectrum 327345 73°25 72°75 72°33 71°65 713 70°73 70°32 69°95 69°65 69-20 68°95 68°8 68°35 67°93 67:80 67-40 67:17 66°68 66°35 66:07 65:99 64°83 64°55 - 63°93 63°67 63°28 63:00 62°80 61°89 61:27 61:15 61°05 60°70 59°99 59°65 59°08 58°55 58:23 57-95 57:50 57:40 56°88 56°60 56:18 55°50 55°20 55-00 54:73 5444 53°50 52:95 52°80 52°50 52°3 REPORT-——1900. URANIUM—continued. Intensity and Character 5 Reduction to Vacuum 1 A+ as A 0:92 87 ” ” ” | ” ” ” ” ” ” ” ” ” ” ” ” | ” | ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ”” ” ” ” ” ” ” ” ” ” ” ” 09 i FOL Oscillation Frequency in Vacuo 3054071 5420 546°6 550°6 556°9 560 565°5 669°3 572'8 575°6 579°8 582-2 584 587°8 591-7 592°9 596°7 599°8 603°4 606°5 609°1 609°9 620°8 623°4 639°2 6316 6353 6379 639°8 648-4 654°2 6553 656°3 659°6 666°2 669-4 6743 679°8 682°8 685'4 689-7 690°6 695°5 698-2 602:1 708-5 711-4 713°3 7158 7185 727-4 732°6 7339 7368 739 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 259 _ URANIUM—continued. Reduction to Wave-length Intensity Vacuum Oscillation Spark and a ) an | Frequency Spectrum Character we i in Vacuo A 825115 In 0°91 87 30749°6 51:00 1 »” ” 751:0 50°50 1 FP " 7557 50:07 1 Fy “ 7598 49-62 1 ” ” 764:0 49°37 1 3 Pe 766°4 49°12 1 ” ” 768'8 48°52 1 3 of T745 48°17 1 ” ” T7178 47°96 1 PH rf 7798 47°75 1 FF fist ss 781°8 47-43 1 re of 7848 46°55 1 3 F 793'1 46°33 2 er 7 7952 45°95 In Fr Fi 798'8 44:98 1 a os 8080 44°69 1 “5 m 810°7 44°39 2 of fe 813°6 43°85 1 * a 818'8 42°90 1d Fr Fe 827:8 42°17 1 A Ef 834-7 41-77 1 4 ef 838°5 41°30 1 7 7 843°0 41:00 1 ¥ = 845°9 40°55 1 or 9 850°2 40°30 1 3 Pe 851°6 39°80 1 - FE 857:3 39°65 a ” ” 858°7 38°62 1 P | 7 868°6 38°10 In E re 873°5 37-4 1b B BE 880 36°93 I ; o 884°7 36°4 ln a5 Be 890 35°44 1 is FE 898:°9 35°20 In 3 Fa 901:2 34:70 In a # 906:0 34:14 1n - pS 911°3 33°53 hi 5 oe 917-1 32°83 In ey . 923°8 32°33 2 x “f 928°6 32:13 1 a9 = 930°5 31:2 1b = Fi 939°5 30°3 1b | oy ” | 948 29°65 3 j 5 Fe 954:3 28°7 1b ¥ 5 963 27°6 1b ns + 974 27°33 1 a Fy 976°5 26:97 1 “ BS 980:0 26°33 2 PA “e 986:2 25°9 In ae Pe 990 24-45 2 + Ne 31004°2 23°88 1 * A 009°7 23°65 1 ey ¥, 0119 23'2 1b x re 016 22°65 1 H - ss 021°6 §2 Wave-length Spark Spectrum 3222°46 22°16 REPORT—1900. URANIUM—continued. Intensity and Character BS =] Serre Pt sk Pg a a Fa a eee Reduction t° Vacuum AH a. | A 0°91 8:7 ” ” 0°90 ” ” ” Oscillation Frequency in Vacuo 31923°4 026°3 032°1 048 053°3 061°6 063°6 067°5 074'3 078°5 084:5 092°6 095'8 096°7 100'9 104°5: 1069 109°7 112°3 116°9 1243 129°7 132:1 136 142°8 146 150°3 156 160°5 169 1790 180'9 184 189°9 194°4 1977 223 206°5 208°1 212°3 2152 20371 227°5 233°3 238°2 243°5 247-2 251 256°2 257-7 271°4 278 283 290 299 Planters ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length Spark Spectrum 3193°45 93°36 92°82 92°30 91°90 91:02 90°86 90°6 89°65 89°17 88°50 87°65 86°35 85°85 85°33 84:9 84°60 84:15 83°63 83:00 82°72 81:5 81:2 80°75 80°48 80°33 79°98 79°50 79:18 79:03 78°45 77-79 77-48 76°78 76°34 75°50 74:96 74°15 73°82 728 72:24. 71:95 71°53 71:22 70°96 70°69 70°48 70:2 69°2 68°55 68°33 67:9 67:22 66°64 65°62 URANIUM—continued. Intensity and Character BR BE eRe eee Pe Speen ERA rt ee tak Fh rt NO) at Df nth It Reduction to Vacuum Oscillation Frequency in Vacuo 313049 3058 311:2 316-4 320°4 329°2 330°8 333 342°7 347°2 353°8 362-2 3750 379°9 3850 389 3923 396°7 4018 408°0 410°8 423 426 43071 432°8 434°3 437-7 442-4 445°6 447-1 452°9 4594 462°5 469-4 474°8 4821 4875 495'5 498°8 509 5145 5173 5216 524°6 527-2 529°9 532°0 535 545 5512 5534 558 564°5 570'3 580°5 261 bo Wave-length Spark Spectrum 3165°41 65°20 64:29 63°90 63°10 62°95 62°4 61:95 61°66 60:90 60°48 60 06 59:94 59°41 59:06 58-7 58'3 57:97 57:57 56:70 56°22 55°98 55°53 55°40 55:02 54°55 54:30 53°62 53°36 52°57 52°45 51°81 51-2 50°90 50°62 50°50 50°10 49°76 49°34 49°17 48°85 48°73 48-40 48°28 47-93 47-19 46°85 46-43 46:2 45°67 A547 45:09 44-84 43°45 42-74 REPORT—1900. URANIUM— continued. Intensity and Character BS Se ee eee aS te a ee eS oe ne 6B ea ae la) all al a Reduction to Vacuum he 0:90 8:7 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ”? ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” »” ” ” ” ” ” ” ” ” EE ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” fs 91 Oscillation Frequency in Vacuo 31582°6 5846 593-7 597-6 605°6 607-0 612°6 617 620:0 627°6 631°8 636-0 637-2 642°5 646:0 650 654 6569 660°9 669°6 674-4 6769 681-4 682-7 686°5 6912 693°8 700°5 703°2 (GL 712°3 718°8 725 7280 730'8 732°0 736°0 739 4 743°6 745°3 748°6 7498 753°2 7544 7579 7654 768°8 773-0 715 780-7 782-7 786°5 789°1 803°1 810°6 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 263 URANIUM—continued. Re rction to Wave-length Intensity Voowes Spark and Spectrum Character KF 1 A 3142°46 1 0:90 | 91 42-03 1 $ . 4 41°75 i 0:88 ” 39°69 2 » 9 39°29 1 a Bf 38°99 1 a sf 38°6 In ” ” 38-4 In ” ” 37°85* 1 7 A 3701 1 ” ” 36°30 in ” ” 35°92 1 is 7 349 1b ” » 33°99 1 » ” 33°69 1 ” ” 33°50 In 3 4 32°75 il E $ 32°32 In 3 5 32°07 1 »» ” 31:72 In 5 * 31°42 In a aA 30°67 2n a 4 29°86 2 a ri 28°88 In i F 28°20 In A, 4 27:75 In rs % 27°35 i a + 26°78 1 2 % 26°28 2 * FA 25:03 2 a P 24:53 1 a 4 24°28 1 Pr 3 23°82 1 » ” 23°70 1 P 4 22'8 In 3 ‘ 22°43 in Pe £ 21:97 In Fe 4 21°49 1 # Fa 21°15 1 2 4 20°97 1 3 : 20:77 In aa 4, 20°25 In x % 19:99 In s ;s 19:42 2 3 ‘ 19°13 In 4 ‘, 18°88 in 3 ¥, 18°51 In eS 5, 18:13 1 i ¥ ITT th » » 17:14 1 ¥ i, 16°83 1 ” ” 16:53 1 » ” 16:02 2 Oscillation Frequency in Vacuo 318132 8175 820-4 841°3 845'3 848°3 852 854 859°9 868°4 875°6 879°5 890 899-1 902-2 904-1 OTT 916:1 918-7 9222 925°3 933-0 949-2 951-2 958-2 962°8 966°9 972°7 977'8 990°6 935:7 998°3 32003°0 004:2 013°6 017-2 022:0 0269 030-4 032°1 034-4 039°6 042°3 0482 0511 0537 057°5 061°3 065°8 071°6 0748 077-9 083°0 264 a Wayve-length Spark Spectrum 3115-12 14°75 14°42 13°75 13:16 12°50 12°35 11°76 11°52 10°96 10°65 10°3 09:9 09-4 08:79 08°43 08:07 07:79 07°65 OT-47 069 06°42 06°29 05°73 05°50 05:20 | 04:8 04:27 03°87 03°10 02:70 02°55 REPORT—1900. URANIUM—vontinued. Intensity and Character HH NH EEE EP eee ee lemon Reduction to Vacuum Oscillation Frequency in Vacuo 32092-4 096-1 099°5 106°4 112°5 119°3 120°9 127:0 129°5 135°2 138°4 142 146 151 157°6 161°4 165°1 165:0 169°5 1713 177 180:2 183°6 189°4 191°7 194°8 199 204-5 208°7 216°7 220°8 222°4 229°7 237°9 239°'8 246°5 250 255 257 260°5 261°7 268:1 28071 2832 290:9 292°1 297°5 299°3 3018 305-4 311-7 316°5 320°3 335°5 339 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS, Wave-length Spark Spectrum 3090°70 90°45 89°98 89°10 88°68 88:05 87°80 87:23 86:90 86°13 85°60 84:8 84°37 83°75 83:2 82-7 82°14 81:18 80°83 80:10 79°40 79:05 78°55 77°95 177 7750 16-7 76:2 75:93 75°60 75°15 74°62 74:47 73°93 73°60 73°3 7291 [247 71:87 716 W117 70°80 70°40 69-6 69°3 68°74 67°85 67:37 67:00 66°43 65°8 65°4 65:02 64:70 64°30 URANIUM—continued. Intensity and Character in In In i In o> omen l=} Fe ye ple el rao Reduction to Vacuum Oscillation Frequency in Vacuo 265 32346°0 348-5 353°5 362°7 367-1 373-7 376'3 381:3 385'8 393'8 399°3 408 412°3 418°8 424-5 430 435°7 445'8 449°5 457-2 464°5 4681 4735 4799 482'5 484-6 493-1 498 512 505°7 509'4 615'1 516-7 522'3 526°8 529 533-2 537°8 549-2 548 551°6 555:5 558-8 569 571 BIT-4 586'8 591-9 595'8 601-9 609 612 616:9 620°3 624-6 to So: Wave-length Spark Spectrum REPORT—1900. URANIUM—continued. Intensity and Character Reduction to Vacuum 306398 63°62 63°25 62°97 62°62 62:23 61°74 61:30 60°80 60°15 59°68 59°3 69:1 58°05 57°35 56°83 55:99 55°71 55°18 54°86 54:5 53°42 52°96 52°56 52:00 51:43 51:20 50°61 50°30 49:9 49-05 48°75 48°45 47-98 47-66 46°96 46°6 45°55 45:1 44:26 44-1 43:3 42°85 42:0 41:3 40°6 40:00 39°3 38°58 38°01 37°63 37:38 36:7 36°53 36°05 eb BS no) lon Q am a a a Na ak a eae oh a i i=] a ee etl ool oll at coor o Oscillation Frequency in Vacuo 326280 631'8 635°8 638-7 642°5 646°6 519°3 656°9 661°9 668 8 673°9 678 680 691°3 698°8 703°3 7133 7163 722°0 725°3 729 740°4 745-7 7500 756:0 7619 764°6 7710 7743 7785 187-7 791-0 7942 799°2 802°8 810:2 814 8254 830 839°3 841 850 8545 864 871 881 885°3 893 900°7 906'9 910°9 913°7 921 923-0 928-1 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length Spark Spectrum 3035-60 34:50 34:15 33°86 33°52 33°27 32°52 32°09 31°65 30°9 30°45 29°52 29°23 28°7 28°48 28°33 27-77 26:99 26°77 26°55 26°25 25°16 24-57 23°9 23°4 22°94 22°58 22°31 21°68 21°30 21:02 20°71 20°35 19-9 19-40 18°95 18°68 18-2 17:50 17-05 16°50 16°16 15°78 15:03 14:35 13-96 13°60 13:49 13:08 12°83 12°22 12°04 11°66 11:30 10°87 URANIUM—continued. Intensity and Character i=} os i=} BER AA, FA SAEs ttt rh debt et BB io” Bo se cil ae La ag — lida la a | Reduction to Vacuum Oscillation Frequency in Vacuo 32933°0 945°5 948°8 952:0 965°6 958°3 966°4 9711 9754 984 989-0 999:2 33003°4 008 010°5 012°1 018°2 026°7 029°1 031°5 045°6 046°6 053°1 060 066 070°9 0749 077°8 084:°7 087-8 091°9 095°3 099°3 104 109°6 1146 117-6 123 133°5 135°5 1415 145:2 149-4 157'7 165'1 169°4 173°4 1746 1791 179°9 188°6 190°6 194°7 198°7 2034 267 268 REPORT—1900. URANIUM—continued. Reduction to Wave-length Intensity Vacuum Oscillation Spark and cic, a aa Frequency Spectrum Character Lae in Vacuo At+ Ey 3010°49 | 1 0°85 9-5 33207°6 09:80 1 4 2 215°3 69°51 1 if 4 2186 09-00 1 ; . 224-1 08-29 1 J - 232-0 pe | Bee ae 06:2 1b : - 255 05°65 1 - 4 261-2 05-23 1 4 : 265°8 04:9 In . A 269°5 04-70 1 is 2 271°6 04:30 1 te a 276-1 03-45 ‘ig e : 85-5 03:17 1 ; i 288-6 02:80 1 ; ‘ 292-7 02:50 1 A - 296-1 01-76 i , i 3043 re 1 ” ” i 01:32 1 B ¥ 309:2 00:90 In 4 313°8 00:26 1 4 % 329°5 2999-28 1 4 ; 3318 99-15 1 BA ‘ 333°3 98:50 In E A 340°5 98-2 In ‘ 344 97°70 In Hs ‘ 349-4 97-48 In * 9:6 351° 97-15 In 4 355° lee | | See 1 ? ” r 59 CS a ss rt ln ’ ” 95°6 In x" 373 95-00 1d ~ 5 379-4 94:57 1 ., if 3843 93-80 1 if 392°8 93-46 1 E : 396-6 aegis. eee: ; ” ” 2) 91-10 In ‘ \ 4999 90-65 In : i 428-6 90:1 1b : 434 39.51 ; : 1407 . 1 ; 5 . 88-05 In i i 457-0 87:93 1 r “4 458°5 86°35 In sf 47611 85-90 1 is : 481-1 85-24 1 S : 488-6 84-74 1 3 . 494-1 84-19 1 :, . 490°3 83°85 1 if ve 504‘ 83°60 1 “ : 507-0 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. URANIUM—continued. Wayve-length Spark- Spectrum 298289 82°40 81:95 81:3 81:18 80°80 80°46 79°31 78°30 77-95 TT41 76-46 75-97 75-73 15°25 75:0 742 73-40 73°20 72°75 72°3 71-72 71:17 70:90 70°56 69°85 69°6 69°35 68°68 68-45 68-02 66°77 66-26 65:8 65:5 65°17 6476 64:35 63°70 63-30 62:87 61:28 61-02 60°38 59:96 59-20 58-25 5785 573 56°85 56-46 56°15 “673 55°20 54-92 Intensity and Character Reduction to Vacuum an A 9°6 Ja) Oscillation Frequency in Vacuo 33514°7 520-4 525°5 533 534-2 538-4 542°3 5552 566°6 570°5 576°7 587'3 592°9 595-6 601-1 604 613 621°9 624-2 628°3 634 641°0 647°2 650°1 654:0 662°1 665 66°77 675°3 677°9 682-9 69771 702°8 708 713-4 "7152 7199 724°5 7319 7365 741-4 759°6 762-4 769°8 TT44 783°2 794-1 798°7 805 8101 8146 818°1 822°9 829'0 832°2 270 Wave-:ongth Spark Spectrum 295446 53:9 53°45 53°0 52°85 52°46 62:00 51°67 51°45 51:16 50:93 50°62 50°37 50:04 49°64 49:03 48:56 48°12 AT 52 468 46°38 45:92 44°73 44°62 44°22 43:93 43°50 43°25 42:90 42°13 41:95 41:35 40:80 40°39 40:02 39°50 38°95 38°60 38:1 37°40 37:23 37:00 36°85* 36°46 35°60 35°0 34:5 33°86 33°65 33°33 33°03 32°65 32°23 REPORT —1900. URANIUM—continued. Intensity and Character eae BBS a a a aoe a La a FSi RON Sn Seopa es a ean ta He op Reduction to Vacuum Oscillation Frequency in Vacuo 33837°4 844 849'0 854 856'1 860:1 865:6 869°4 871°9 8753 877'9 8815 884-4. 888°2 892°8 899°8 905:2 910:2 917-1 925 930°3 935°6 949-2 950°5 955'1 958°8 963°9 966°3 970°3 978°8 981:2 988-2 994:°5 999°3 003°6 34009°6 0159 020:0 026 033°9 0359 038°5 040°4 044°9 054'8 062 068 075:0 O77°4 081-1 0846 089-0 093°9 eee —@—eeeemcoOrmOrmrmCrC——™—~—~—~— ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length Spark Spectrum 2931°90 31°60 31°45 30°87 30°68 30°47 29°85 29°70 29°16 28°61 28°16 27:77 27-45 27:30 26°64 26°42 26:18 26:00 25°61 25°25 24°62 23°52 23°20 22-90 22°71 22°23 22°10 21°76 21-15 20°77 20°46 20°23 20:00 19°50 19:08 18°98 18°73 18:48 178 17:2 16°90 16°54 15°80 15°57* 15°32 14:82 14:69 14:30 14:03 13°50 12°83 12°65 11:90 URANIUM—continued, Intensity and Character PAL rat ett fo pdf eh bh Ak eke eh ft ft ooh eft ot oh dP deh BRB Ree eee Reduction to Vacuum Oscillation Frequency in Vacuo 34097°8 101'3 103:0 109°8 1120 114°4 121-7 123°3 129:7 1362 141°3 145°9 149-6 151°4 159°1 161°7 164°5 1665 182'8 1753 1827 195°6 199:3 202°8 2050 2106 212.2 2162 223°2 2276 2313 234:0 2367 242°5 247°5 248°6 251°6 254°5 262°5 269°5 2731 2773 286:0 288.7 291:°7 297°6 298-1 303°7 306°8 313°1 320°0 323'1 3319 9 “ 71 bo bo REPORT—1900. URANIUM—continued. Reduction to Wave-length Intensity aes Oscillation Spark and cs > aS ee a Frequency Spectrum Character a Les in Vacuo A 2911°60 1 0°83 9:9 34335°5 11:22 if ” ” 340°0 10°88 1 ” ” 344:0 10°75 In ” ” 345°'5 10°3 1b » 7 351 09 78 1n “a 3 357-0 09°30 i ” 362°6 08°8 1b ” ” 368°5 08°31 3 ” 7% 374:3 07°65 Ind r 382-1 07:00 in 53 a 389'8 06°85 2 % Be 3916 05°8 lb 5 ss 404 05°32 1 » x 4097 04:52 2n a % 419-2 04:07 1 » . 424-6 03°63 1 0°82 is 429'7 03-08 1 » 99 4363 02°50 1 ” ” 443°2 02"1 lb m3 19 448 01:70 1 ” ory 4517 01:27 i ” ” 457°9 00:22 In ” ” 470°2 2899°65 In # ATT'1 98°80 1 ” ” 487°1 98°12 In + - 491-2 97-70 1 ” ” 499-2 97-45 1 ” ” 503'2 97:00 In . 10:0 508°5 96-77 1 4 5 511°2 96°52 it 5 RS 514:2 96°15 In 3 517-4 95:96 1 s 3 520°9 95:60 In x uf 5251 95°30 1 2 # 528-7 9498 1 7 "4 532-5 94°60 1 ” 3 5371 94:20 1 * x 541-9 93°80 In ; f 546-6 93°5 lb + A 550 92°70 1 9 4 559°8 92-25 1 ” ” 565°1 91°80 In _ : 570°5 91-10 i a P 578-9 90°82 1 S 3 582°3 90°50 1 " % 5861 90°15 1 + : 590°3 89°65 2 ” ” 596°8 89°32 il x a 600°2 89°12 1 x x 602°7 88:76 1 * 4 606:9 88°42 1 £ , 611-0 88:28 1 ” ” 612-7 87-97 1 > : 616-4 87°65 1 3 65 6202 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length Spark Spectrum 328731 87:00 86°87 86°50 86:10 35°70 85°49 85:28 85:05 84:70 84°43 83°87 83°50 83:00 82°82 82:00 81-67 81-1 80°50 80:28 80:00 79°70 78:95 78:3 7786 7765 77:10 76°55 759 75:24 74:81 74:16 73°75 73°60 73°35 73:1 72:53 72:15 71:30 71:04 70°80 70°4 69°49 69°00 68°87 68°51 68°20 67°89 67.45 67-15 66°90 66:47 66°22 65°73 65°40 1900, URANIUM—continued. Intensity and Character Se ee len BSB Reduction to Vacuum 1 A+ =i A 0:92 86 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” | ” ” ” ” | ” ” } ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” “ 10-1 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” bbl 23 ” ” ” ”» ” ” ” ” ” ” ” Oscillation Frequency in Vacuo 30624:3 628-0 629°6 6340 638'8 643°6 646°2 649°9 651°4 655°6 658:9 665°7 670'1 6761 6783 688-1 6922 699 706°2 708°7 7122 7158 7249 723 738°0 740°6 TAT 2 7539 762 769°7 TT4:9 782°8 787-7 789°6 7926 796 802°4 807:0 817°3 820°5 823°4 828 839°3 8452 846'8 8512 8550 858-7 867°7 864'1 870°8 8760 879-1 8840 889:0 273 274 REPORT—1900. URANIUM—continued. | Reduction to Wave-length Intensity Vacuum Oscillation Spark and waar -T|| ota aa Frequency Spectrum Character A ee in Vacuo A 3265°20 1 0°92 10°1 30891°5 64°95 1 0°81 39 894°5 64°70 1 ” * 897°6 64°35 1 ” Fa 901°8 64°18 1 5 + 903-4 63°65 In ” _ 910-4 63°28 1 ” = 914°9 62:90 In ” > 9195 62°72 1n ” 5 921-7 62°45 in ” 925°0 61°8 1b *) 934 61°31 1 7 u 938°9 60°86 1 a i 944-4 60°53 1 9 A 948°5 59°85 2 3 x, 956°8 59°36 1 » a 962°8 58°95 2 > _ 967°8 58°40 In > + 9745 58°25 In ” > 976°4 57°53 in » + 985°2 57-15 In » s 987°8 56°63 i an . 996-2 56°30 In 4 35000°2 56°05 1 £ th 003°3 55°67 1 x " 008°0 55-00 1 os op 0161 54:55 1 - - 021°7 54-30 1 5 A 024°8 53°90 1d : mo 030°7 53-60 1 “) 3 033°3 53°50 1 7 5 0346 53°07 1 Ss Fr 0349 52°83 1 oy 5 042°8 52°50 1 » * 046°9 52-20* 1 ” 050°5 51-90 1 - sn 054-2 51°35 In 59 + 061:0 50°S5 1 3 5 065°9 50°57 1 + “ 070°6 50-0 in 3 + 078 49°8 In > a 080 49°55 4 5; 5. 078°2 49°26 1 * = 086°8 49-00 1 nf “ 089°9 48°75 in 9% ” 093°0 48°35 J 7 10:2 097°8 48°12 1 A ” 100°7 47°83 1 5 a3 1043 47:50 In ” x 108°3 46°95 1 > is 1148 46°70 1 5 " 1182 46°44 1 , AS 121-4 46°21 | 1 9 Fi 124-2 ———— eee leer ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 275 Wave-length Spark Spectrum 3246-00 45°70 45°43 45:10 44°78 44°60 43°95 42°98 42°60 42°30 42°20 41°48 41°25 40°78 40°60 40:00 39°2 38°73 38°40 38°10 37°86 37°40 37°31 37:00 36:1 35°88 35°68 34°82 34°70 34:2 33°90 33°35 32°75 32°53 32°16 31:7 31:05 305 29°96 29°4 29:00 28°1 27:90 27°47 , 27-05 26°77 26°60 26:28 25:90 25°65 25:5 24°95 24°70 24:45 23°65 URANIUM—continued. Intensity and Character ion B ion ec terra tage ea t= a a ear ar ee Reduction to Vacuum 1 A+ <- A O81 10:2 ” 22 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” 9 ” » ” ea ” ” ” ” 29 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” | 3 ” ” ” ” ” ” ” ” | ” | ” ” | ” | Fy | ’ ” ” ” ” ” » ” ” 0:80 é ” ” ” ” ” 10:3 Oscillation Frequency in Vacuo 351268 130°5 133°9 1380 1419 144:1 152-2 1642 168°8 172°6 173°8 182°8 185°6 191-4 193°7 201-1 211:0 2168 220°9 224°6 2277 2333 2345 238°3 248°5 252°3 2548 265°5 266°9 273 2769 283°7 291-2 T2 Wave-length Spark Spectrum 3223°24 22°80 22°63 22°27 22°08 21:48 21°20 20°75 20°57 20°34 19:89 19°26 19:06 18°85 18-70 18°43 18:05 17-75 17°3 17:00 16°88 16°52 16°15 16:05 15°85 15°30 15:18 14:90 14:73 1412 139 REPORT—1900. URANIUM—continued. Intensity and Character Reduction to Vacuum 5 ee a age ee ee stip leeds ell mentioned El Oscillation Frequency in Vacuo 35410:0 415°5 417-7 422°2 426°6 432-1 435°6 441°3 443°5 446-4 4521 460°0 461°5 » 465°2 467:0 470°5 475°2 479°0 485 488°5 4900 494-5 499-2 500°4 503:0 509'9 511-4 5149 5171 524°S 527°5 529 534 537°6 542 5475 554 558°0 562 565°9 570°6 576°3 5807 588°5 593°9 595°9 612-4 6175 622°5 630°3 636°1 651-7 6543 6649 679°2 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMEN'IS. URANIUM— continued. Reduction to Wave-length Intensity Vacuum Spark and Spectrum Character Pe i a 3202°30 1 0*80 10°3 O175 1 . g 01:45 1 d i 00°93 J . i 00°42 In ; 4 00:22 In . i 2799'8 1b f i ae a . 10-4 98°28 1 a 5 97:87 1 2 é 97°45 In £ i 97°25 In % : 96°80 1 4 i 96°1 1b 7 ‘ 95°65* 1 a ‘ 95°30 2 ke i 95-00 il ‘ y 94°50 In a I; 94:05 D) z ‘i 93°54 1 3 i 92°15 In Ks a 91-4 In 3 ‘ 91:16 1 i % 90°78 In ; : 90°4 1b qi i 89°9 1b ci k 89-2 1b et ‘ 88-7 1b bs ‘ 88°24 il ki ‘ 87-45 1 hi i 869 1b < % 86:27 ln a 4 86:0 In bi ‘ 85°76 In ‘4 a 85°50 1 7 g 85°30 1 id s 85-02 1 . ‘ 84:77 it i z 84:57 1 i ” 84:12 1 si 83:99 n | 0-79 is 83°55 in * - 83°33 In a - 82°52 © In if 82°22 1 v. Z 81:90 1 i : 81°67 1 ‘3 Z 81°52 1 : ¥ 81:16 1 ne 3 80°89 In i 3 80°13 il by . 79°53 In < ; 79°05 In Oscillation Frequency in Vacuo 35674'2 6817 685'8 692°1 698°6 7012 706°5 714 725'8 7311 7364 739°0 T44T 754 759'5 763°9 7678 TTA 1 7799 786°5 8043 814 817-0 821-9 827 833 842 849 8545 864:7 872 879'9 883 886°5 859°7 892°4 896°0 899:2 901°8 907°8 909°4 915:0 9178 9283 9321 936°2 939°2 941:2 945°8 949°3 959°1 966°9 973-1 27 7 8 REPORT—1900 URANIUM—continued. Reduction to Wave-length Intensity as Oscillation Spark and S| ae Frequency Spectrum Character Be: Le: in Vacuo r 2778°35 1 0:79 10°4 35982°2 WT20 1 ”» ” 998-1 76°66 1 ” ” 36004'1 76:45 In ” ” 006°8 75°95 In ” ” 013°3 75°60 1 ” 10°5 017'8 75°50 1 ” y) 019-1 75°37 1 ” ” 020°9 75°16 1 ” ” 023°5 74:88 1 ” ” 0271 74:54 1 ” ” 031°5 74:25 1 ” ” 035:3 73°90 1 ” ” 039°8 73°74 1 ” ” 0420 73°20 1 ” ” 048°9 42-45 1 ” ” 054°8 72°45 1 + 5 058-7 72°33 1 ” A 060°3 72:02 1 ” ” 064:3 71:69 1 1 A 068°6 71°35 In ” “ | 072°9 70°85 1 + a 079°5 70°41 i 5 i 085°3 70°15 1 es a | 088°6 69°56 1 > - 096°3 69-40 1 ” ” 098°4 69°17 1 “6 > | 101°4 68°95 1 “5 a 104:°3 68°53 1 ” 3 109°8 68°30 1 ae A 113°9 67°85 1 rs * 118:7 97:52 In 2 os 122°9 66:97 il a a 130-1 66:26 1 45 4 139°4 66:00 1 os BS 142°8 65:78 1 ” ” | 145-7 65°50 1 * 5 | 149-1 65:3 1br y ” 153 64:80 1 a “n | 158°5 64°35 1 4 A 164-4 63°82 1n 4 | x 171°4 63°57 1 = | a 174°6 62°98 1 ” | ” 182°3 62°50 In 5 | 4 | 188-6 61:90 1d a 55 196-4 61°55 1 ” ” 201'1 61:33 1 ” ” 203°9 60:46 1 - a 215°4 59°90 1 “ ” 222:7 59:05 1 | ” | ” 233°9 58:62 1 | ” ” 239°5 58°53 1 | ” ” 240°7 58:26 1 | 5 5 244°5 58-03 1 ‘, . | 246°3 57°93 1 | #5 i 35 i 248°6 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 279 URAIIUM—continued. Reduction to Wave-length Intensity Vacuum Oscillation Spark and (aia ies. rae Frequency Spectrum Character A+ S., in Vacuo A 2757-65 1 0:79 10°5 36252'3 57:40 1 r 255°5 57°25 1 ” ” 257°5 56°40 iT s ‘ 268-7 55.26 1 Bs 5 283-7 55°06 1 8 3 286°3 54:70 1d +s 5 291-0 54:27 2 FP sj 296°8 53°87 1 E . 301'8 53°52 1 ” ” 306°7 53°42 1 c . 308-0 53:09 1 4 a 312°3 52°57 1 99 4 319-2 52-03 2 ee 33 3263 51:32 1 # 10°6 335°6 50°95 1 » ” 340°5 50°69 1 » ” 343-9 50:50 1 ” ” 346°5 50:23 1 i , 350°0 50-05 1 3 i 352-4 48-98 1 4 . 366°5 48-60 1 33 $i 371-6 48-03 1 F i 3791 47-47 ‘| i 3865 47°26 1 - . 389°3 46°82 1 : r 395-1 46:27 1 + . 402-4 45-99 1 5 3 406'1 45°22 1 ; r 416°3 44-95 1 : i 419-9 44-50 1 - 3 425-9 44°38 1 % if 427°5 43°79 1 7 d 4354 43°50 2 Fe 4 439-2 43°32 1 = i 441-6 42°70 1 a 33 449-8 42°18 1 ” ” 456-7 41-88 1 0:78 ¥ 460°8 41-70 1 a F 463:1 41°34 1 7 i 467-9 41:19 i Fe Pe 469-9 40°94 1 ” ” 473°2 40°63 1 2» ” 477-4 40:40 1 ” ” 480°4 39°50 1 i 3 492-4 39:08 1 . a 498-0 38°65 1 a 34 503°8 38°50 il FS e 505'8 38°23 1 s 4 509°3 37°93 1 e if 513°3 37°75 1 - a 515°7 37°19 1 _ ” 523-2 36°45 1 3 43 533°1 36°10 1 G 537'8 35°86 1 _ 541:0 980 REPORT—1900. URANIUM—continued. Reduction to Wave-length Intensity eae Oscillation Spark and Frequency Spectrum Character Nea a in Vacuo . A 273565 1 0-78 10°6 36543°8 35°42 1 is a 546°9 35°05 1 * i 551°8 34:80 1 ” ” 5551 84:34 ul a ” 561°3 34-04 1 * ” 5653 33°85 in + ” 567°8 33°41 in ” 573°8 33°06 1 Fe 3 578-4 32°60 1br a ” 5846 32°15 In 3 ry) 590°6 81°52 1 a ” 5991 31°38 1 ey 3 600°9 30°90 in 7 ” 606°2 30°43 il RS if 613°7 30°20 1 " ” 616°7 29°75 ld 3 ie 622°8 29°35 1 7 ” 628-2 29°15 1 - é 630°9 28°8 ln 3 5) 635'5 28°65 in 3 ” 637°6 28:3 lbr zn Fr 642 27°65 1 - af | 651:0 27°40 1 a 73 6543 26°75 ln ; 10°7 663°1 26°61 al 53 oa 664°9 26:01 1 a + 673:0 25°78 1 3 si 6761 25°56 1 3 = 679:0 25°14 1 + a 684-7 24°55 in es x, 692°6 24:2 lbr 4 FF 697 23°90 il * » 701°4 23°80 1 ; a 7027 23°43 1 is ‘7 107-7 23:25 1 cr i 7101 22-90 1 & “a T7148 21°95 1n + 7 727-7 21°53 1 Fs ¥. 1343 21°25 1 ae a 7371 20°99 1 7 ai 740°6 20°78 1 5 £ 7435 20°50 1 * 93 TAT-2 20°33 1 Fe 5S 749'6 20:00 1 _ =, 754-0 19°63 1 Ps 3 759'1 19°43 1 . PF T61:7 TOS il 4 3 765°5 19:00 1 Vs - 7675 18°72 1 5 “5 T7113 18:18 1 53 7786 17°65 1 Ng 5 7858 17°25 in * ” 791°2 17:10 in A. 5S 793°2 16°63 1 Fi 799°6 EE Eee ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length Spark Spectrum 2716-48 16:20 16:09 15°66 15°40 15°10 14°68 14°40 14:04 13°57 13°33 12°68 12:20 11:86 11°64 11-23 10-70 10:20 09°63 09°12 08-60 08°45 08:05 07:79 07:59 07:09 06°85 06°6 06:3 05°87 05°33 04:90 04:2 03°83 02:9 01:95 01:68 01:50 01°08 00°38 2699°75 99°46 98°57 98°15 97:52 97:15 96°68 96:40 96:00 95°60 94.35 93°88 93°41 92°49 91:93 URANIUM— continued. Intensity and Character Reduction to Vacuum 1 r lop) Bee ee BRE RE R EP PpRPR Re Bp 6B BB ENR RRR eRe BEDPD NE NRP REPRE RP HEWN REPRE RP RE H 10°7 Oscillation Frequency in Vacuo 36801°6 8054 806°9 8128 816°3 820°3 826°1 829°8 835°7 841-1 844-4 8532 859°8 864-4 867-4 872°7 880°1 886°9 894-7 901°7 908-7 910°8 916-2 9198 922°5 929°3 932°5 936 940 946°0 953°4 959°2 969 973°9 985 999°5 370032 005'6 011-4 021:0 029-7 033-7 045-9 051-6 060°2 065°3 071°9 0758 081-2 096°7 101:2 110°5 116°9 129°5 137°3 282 REPORT—1900. URBANIUM—continued. oo a —— eee Reduction to Wave-length Intensity oes Oscillation Spark and ia? | > Stee Frequency Spectrum Character as fea in Vacuo A 2691:17 2 0:78 10°8 37147°8 90°65 1 = ks 155:0 90°15 | 1 os 3 161:9 89:23 1 B is 174:6 88°76 1 ; a 1811 88:07 1 i - 1913 87°55 In a re 1978 86°9 1br a sy 207 86:06 2 % x 218°5 85°7 In * 5 223 84:70 1 F s 237°2 84:40 1 ip 55 241°5 84:17 1 :. “J 2446 83°40 2 a “4 2554 82°40 2n 5 4 269'2 81°80 1 3 3 277°6 81°23 In = is 285°5 80:75 1 “3 Pe 292-2 80°3 In a B 298°5 80:0 In = as 303 79:1 ln fe 10:9 316 78°96 1 5 3; 317-1 78:53 1 - i 323-0 78°14 1 BS i 328°5 77:68 1 - n 335-0 77:25 1 x 5 340°9 76°75 1 S Ni 347°8 76°50 2 ss ea 3513 76:00 1 s - 358-3 75:18 2di = . 8369'S 74:63 In . i 5 377-5 74:10 In a 4 384 9 73°73 1 a * 3901 73°51 1 . ne 393-1 73°25 1 Me 7 396°8 72°80 1 * 4 403°0 72°38 1 a es 4089 72:08 1 3 _ 4131 71°40 1 - - 423-7 70:99 1 i 5 4284 70°65 In * - 433°2 70°50 in - D 438°2 69°9 1n hs 444 69°31 2 ~ i 452:0 69:02 1 Fa 2 456-0 68:28 1 * “p 466°5 68:11. 1 x a 468'8 67°25 In “ + 480°9 66°6 2br 3 : 490 65°96 1 ‘5 + | 499:0 65:76 1 55 5 501°9 64°24 2 5 x 513°6 63°95 1 | bs € 527°3 63:5 lbr | 5 i 3 534 | ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. URANIUM—continued. Intensity Reduction to Vacuum Wave-length Oscillation Spark and Frequency Spectrum Character A+ i in Vacuo A 2663-3* lbr 0:78 10:9 37536'5 62-90 1 2 ” 542-1 62:2 lbr ; ” 552 61:27 1 #3 5 5652 60:23 1 $3 5 579°8 60°00 2 fr %9 583'1 59°60 1 3 c 588°7 59:19 in ” ” 594-7 58°85 1 3 # 600°2 58-49 1 i 53 604:9 58°20 1 3 # 608°5 57:96 1 " ” 611°9 57:45 In +. * 619°2 57°25 in ” ” 622-0 56'6 1b ef . 631 55:5 1b A “4 647 55:05 in s 110 653:1 54:70 1 0°76 5 6580 54:3 1b ” ” 664 54:00 1 5 e 668:0 63°50 1 ” ” 675-1 53°20 1 ” ” 679°3 52:95 2 i? 4h 682°9 52°8 In . e 685 52:27 1 f ss ou G 51:96 1 in i 697:0 51-40 1 a - 7049 50:95 In a a 7113 50-25 In x . 7213 49-65 1 a a 729°8 49-15 2 i z 737-0 48-84 In a = 7414 48:3 1b 32 a 749 48-00 in * 753°3 47-65 In “J i 7583 AT-AT in a As 760:9 47-1 1b a fe 766 46:6 1b x i 773 45:54 2 3 3 788°5 44°50 1 ” ” 803°3 44-22 1 4 5 807:3 43 62 1 i i: 815°9 43-38 1 3 . 819°4 42°9 In 5 826 42-00 1 Bs f 8391 41°66 1 * "i 844-0 41:2 In i Ss 851 40°43 1 a ss 861°6 40:00 1 a 5 867°8 39:70 1 ‘ a 872:1 39-45 1 a Ye 875'8 39:10 1 3 Fr 880:7 38:7 1b 886 284. Wave-length Spark Spectrum 2638°4 37°82 37:48 373 36°33 35°91 35°59 35'3 346 34:2 33°35 32°74 32°50 32°08 31-74 31:42 31:15 30°7 29°95 29°26 28°99 28°57 28:02 27°62 26°70 25°98 25°30 24:99 23°62 22°50 21°86 21°39 21:08 20°80 20°30 20:18 19°37 18°25 17°36 16°99 16:13 15°21 14:0 13°35 13-00 12°52 11:70 11:23 10:75 10°51 10:01 09°82 09°34 09°13 08°62 REPORT—1900. URANIUM—continued. Intensity and Character 1b 1 lr lb ln Bo PRE HDB EHP R EEN NR REE BREE Ee Eee Hee HEE BBB allie ac al ral else a Reduction to Vacuum Oscillation Frequency in Vacuo 37891 899°] 904-0 907 920°5 926°6 931°2 935 945 951 963°4 9722 975°7 9818 986°7 991°3 995'2 38002 012°5 022°5 026-4 032°5 040°5 046°3 059°6 070°0 079°9 0844 104:3 120°6 129°8 1366 141-1 145°2 152°5 154°3 166-0 182-4 195'3 200°7 212°6 226'8 244 2540 259°1 266°2 278°1 285:0 292°1 295°6 302°9 3057 312°7 313°7 3233 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS, 285 URANIUM—continued, Reduction to Wave-length Intensity Mae Oscillation Spark and ee ae a Frequency Spectrum Character ee iL in Vacuo A 260825 1 0:75 11:2 38328°8 07°55 1 5 3 339°0 06°80 1 3 - 350'1 06°60 1 - 3 364:1 06:26 1 3 7 358:0 05°86 1 3 s 363°7 05°48 1 is i 369°5 04:93 1 9 in 377°6 04:74 1 Be if | 380°3 04:37 1 7 ‘ 3860 04:00 1 ‘5 ; 3913 03°68 1 * 5 396°0 03°50 1 % a 3920 03-10 1 es ee 405°5 02°51 In 5 *y 4133 01°62 2n : 2 4264 00°9 1b 8 FP 437 00-4 1b = - 444 2599-90 1 6 es 451°'8 98°95 1 _ 5 4659 90-77 iL i > 483°4 97:40 In 3 FS 488°8 97:10 In 3 . 4932 96:23 1 = £ 506:2 95°71 Z . 513°9 95°45 1 s 517'8 95:10 In e . 522:9 94:40 1 8 Ee 532°6 93°9 In ” 5 541 93°67 in * 5 5443 92°67 1 3 3 5592 92:2 1b 3 3 566 91°35 2 s 5 578'8 90°90 1 v $5 585°4 90°55 1 *, 3 590°7 90°22 1 - 595°6 89°70 1 3 be 603°3 89:27 1 op 3 609°8 89:00 1 of i 613-7 88°65 in Fy oo 619:0 87:9 ind * 11:3 630 87°60 1 % * 634°6 87°16 2 ss 9 641°1 86°33 1 3 A 653°'5 85°30 1 : Hs 668-9 84:9 2b | . as 675 84:50 1 Fe 3 680°'9 83°5 2b . r 686 82°72 1 be e 707°6 82°23 1 3 | " 714:9 81:83 1 ‘i | $ 720°9 81°22 2 : 7a 7301 80°67 1 | ¥ x 738°4 79°62 on | *, e 753'6 79°23 In . oF 760°0 286 REPORT—1900. URANIUM—continuet. Reduction to Wave-length Intensity ae ? Oscillation Spark and Frequency Spectrum Character Ae ihe in Vacuo Xr 2578°40 1 0-75 11:3 38772°5 77-46 1 _ 4: 7865 77-14 1 a pits 45 7T91°4 76°25 1 ” ” 804'8 75°53 ~ a 4p 815°7 753 In 5 ” 819 74:8 1b 3 ” 827 733 In . ay 849 73°04 In y y 8532 72°73 2 - ay 857°9 72°43 2 4 rh) 862°5 71-90 1 50) 4; 870'5 71°60 1 a % 874:9 71:16 1 FS <5 881:7 70°77 1 mH 4 887°4 70°43 1 5) > 892°7 69°85 if i a 901°5 69°46 1 i ro 907-4 68°95 1d 3 * 91571 68°05 1 . 33 928-7 67:22 1 5 11-4 9413 67:00 1 Pr a 944°6 66°75 1 " op 948-4 66:00 1 3 3 959'8 65:52 2 4 4 967°1 64°55 Ind 0:74 ” 9818 64:02 In 6 989°9 63°60 In . : 996°5 63:07 i op nf 004°3 62°93 1 3 ¥ 006°4 62°68 1 : cs 0103 62-19 1 3 017-7 61°76 1 y " . 024°3 61:03 i s 035°4 60°35 in 3 045'8 60:10 1 m1 " 049°6 59°60 1 = . 057°2 59°30 2 = * 061°8 58-43 In 53 if O75:1 58:07 In . © 080°6 57-5 1 - % O74 [ B71 | 1 : . 095:2 56°29 2 s ; 107-7 55:95 In + % 113:0 55°62 In i; | 3 1181 55°27 In ee : 123°4 54:9 In » ” 129 54°52 In - + 134:9 53°82 In + 7 145°7 53°53 In An 4 1504 52°47 In A ss 166°3 52-00 1 s 5 1735 51°56 1 + y 1805 51:2 in x a | 186 50°9 1nbr “R ;; 190 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length Spark Spectrum 2550°7 501 49°43 49°26 48°40 48:08 4AT-T4 4T47 47-52 46°45 46:00 45°9 45°55 45°12 44-73 44,45 44-12 43°46 43°30 42°80 41:95 41:60 41:47 41:14 40°77 40°50 40°40 39°98 39-60 39°38 39°05 38°83 38:51 38°3 37°80 37°36 36°88 36°70 36°33 36:00 35°65 35°03 34:95 33°32 33°03 32°80 32°40 31°88 31°65 315 30°95 30°38 30:14 29°60 29°06 URANIUM—continued. Intensity and Character Et et BB ee ee) i=} Baek Fk at Pt nh ttt J8Sh et tt bk Pt BB Qu Bee Reduction to Vacuum At ~~ 0°74 11:4 ” ” ” ” ” ” * 11°5 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ce) ” ” ” ” ” ” ” ” 9 ” 9 ” 9 bhi ” ” ’ ” ” ” ” ” ” be) ” ” Lh] ” ” 2” ” 29 ” bl ” ” ” ” ” ” ” 2 ” ” ” ” ” ” ” ” ” ” ” ” , ” ”° ” ” ” % ” ” ” ” ” ” ” ” » ” ” ” ” ” ” ” ” * 116 Oscillation Frequency in Vacuo 287 38193°5 203 2131 215°6 228°8 233°8 239:0 243°2 242°4 258°9 39265°8 281 272'8 279°4 285-4 289°7 2948 305°0 3075 3152 328°4 333°8 335°9 340°9 346°7 350'8 352-4 358°9 364°8 370°2 3733 3768 3817 385 392°7 399°6 407-0 409-7 415°6 420°7 426-2 435°8 437-0 462-4 4669 470°5 4768 484°9 488°5 491 499°0 508°3 o1l9 5203 528°8 Wave-length Spark Spectrum 2528°83 28°65 28°44 28°17 27°80 27°50 27:23 26°62 26:0 25°46 25:02 24°55 24:4 23°98 23°8 23°1 22°17 219 21°45 20°99 20°8 20°35 19°50 19°20 19°05 18°56 18:0 17:27 17:06 16°20 15°80 15°63 15°20 14°86 14°50 14:17 13°8 13°4 12°7 12:29 12-10 11:05 10:97 10°45 10°23 09°60 09°23 08°45 08:02 07-80 07°50 07:18 07:05 06°55 06°12 REPORT—1900. URANIUM—continued. Intensity and Character Se ae eS ee F — ae ts a5 a Reduction to Vacuum Oscillation Frequency in Vacuo 5353 538°5 542°7 548-4 5532 557-5 570°7 577 585-2 592:0 599-4 602 608-5 611 622 636°8 641 648:2 6554 658 665°5 678:°7 683°6 6859 693'8 702°5 7140 717°3 730-9 737-2 739°9 TA6-7 7520 T7577 763°0 769 775 786 779'3 7796 812°3 8135 8218 $253 835°3 841°2 853°6 860-4 863°9 868°7 873-7 875°8 883°8 890°6 39532°5 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 289 URANIUM—continued. —————— : Reduction to Wave-length Intensity \etoey | Oscillation j Spark and oF 4 Frequency Spectrum Character Fete hi in Vacuo Ar 2305°38 1 0-73 Le? 39902-4 . O47 Ind 33 = $13 . 04:0 Ind 5 4 924 03°4 1nbr 3 a 934 02°5 in 7 rf 945 02:00 1 e * 956°3 01°45 1 fe = 965-71 00°95 2 * ‘, 9731 2499-68 2n #9 ss 993°4 98°90 1 3 4 40005:9 98°35 if Fe - 014-7 97°85 ul ea fi 022°7 97:05 2n Be 3 0356 96°13 In of =e 050°3 95°85 In 5 3 0548 95:4 in FP 3 062 94°86 il Pe a 070°7 94:5 In 3 Pr 076 94:3 1n En +9 080 93°8 1b i 11:8 088 93-00 1 . 100°5 92°4 1b i Fe 110 91:43 ln a Ss 125'8 91:03 2 Py | 132°2 90°72 1 A * 137°2 89°87 I - > 150°9 89°33 1 a Ff 159-7 89°12 ut Pe 4 162:0 88-87 il Pa 5 167-1 88°63 1 es : 1710 88:25 if op ; 1771 87:95 if as ; 181:9 87-70 1 A mS 186:0 87:50 1 fe s 189-9 87:17 1 Pr ES 194:5 86°83 1 an 3 200-0 86°50 1 a a 205°4 86°27 1 ms oe 209°1 85°85 1 os Pr 215°9 85:18 1 es ‘ 226'7 | 85-00 1 3 oo 229°6 . 84:72 1 - a 2342 | 84-30 1 si es 241:0 84:08 af a a 244-6 83°88 1 FF 33 246'8 7 83°37 1 s 5 256°1 83°08 1 ‘a Pe 260°8 82°75 1 AA % 265°6 } 82°30 1 8 A 283°3 ; 82:00 1 *, Pr 278°3 h 81-60 In on iz 284:8 ; 81-10 In a » 292°9 , 80°73 1 3 bes 298°9 ; 80°58 1 - sn 301°4 ' 80°25 il 4 Fe 306-7 1900. ? 290 REPORT—1900. URANIUM—continued. Reduction to Wave-length Intensity Faconm Oscillation Spark and Frequency Spectrum Character ie 1 Ee in Vacuo A 2479-67 2 0-73 11°8 403161 73:69 3 c as 3321 78:10 In PA Ge 341-7 77°88 it A 9 3443 77-27 1 i. = 3552 76°56 2 * 1989 383°0 75:71 1 a . 380°6 75°40 1 A bs 385°6 751 1b - = 390°5 74:26 1 - 3 404:2 73°75 In 5 5 4126 73°46 1 Pe “ 417°3 73°22 1 ‘3 5 421°2 72°98 1 i‘ a 425-1 72°82 1 ee i 4278 72°28 1 . 3 436°6 71°22 1 om 5 454-0 70°93 1 *5 2 458-7 70°76 1 25 + 461-5 70°52 ) 1 3 “A 465°4 69°67 1 0:72 . 479-4 69°55 1 . °. 481°3 69°23 1 as - 486°6 68°43 il 5 * 499-7 68°35 uf * es : 501-0 67:98 1 ; s 507-1 67-41 1 ms 516-4 66°80 2b a s 526-4 65:93 1 = nN 540°8 65°25 1 a 3 5519 65:01 1 si s 5559 64:13 In aS > 570-4 63°87 In a 3 573°7 63°45 Ind 55 - 5816 62-50 il is ; 597-7 62°40 1 ‘ Fe 598-9 62-00 1 = 53 605°5 61:47 1 ., Ss 6143 60°95 In PP PA 622°8 60°75 1 a 2 626°1 60°4 In a aa 632 60°22 1 - 12:0 6349 59-79 1 - 3 641°8 59°30 i - 5 650°0 58°88 2n FD 657-0 58:4 In a is 665 58°03 1 3 ey 671-0 57-72 1 a3 a 676:2 57:25 2 — es 684:0 56°30 1 = “ 700°1 55°77 1 35 7 708°4 555 In ; - 5 718 5571 In os As 719% 54:46 2 a ge 730°2 53°9 Ind c. 5 7395 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 291 URANIUM—continued. Reduction to | | Wave-length Intensity Yea | Oscillation Spark and leas ew ces. | Frequency Spectrum Character A+ aby in Vacuo A 2453°52 1 0°72 12:0 40745°8 52°78 1 + 5 7581 52°21 1 Fh ve 7675 51°83 1 - a Mise) 51:20 1 p as 7843 50°90 1 % ca 7893 50°68 1 » _ 7930 50°51 1 9 ~ 795°8 49-92 it ” ” 805°6 49°80 1 rf = 817-6 49°55 1 “p JF 811-6 49°21 1 ” 4p 817°5 48-98 1 oH a 821-1 48°61 1 3 n 8275 48°37 1 Fe a 831-7 47-9 In % ” 839°3 47-52 1 rf | Z. 845°8 46°95 1 ” fp 8552 46°60 Ind ” ” 861-2 46°22 1 ” ” 867-4 45°78 Ind op 5 8747 ! 44-9 Ind ep “ 889°5 : 44-65 LI ” ” 893-7 44-12 2 rr 902°5 43°60 1 ” 12°1 911:3 42:97 2r ” “i 921°6 42°50 1 : 9 a 929-7 42-0 1b cf *y 938 41°63 1 ” ” 944-1 41-40 1 19 FS 953-0 : 40°52 Ind i . 962°8 39°6 1b ” FP 978 39°44 1 ” ” 980°9 39°14 1 PF, % 986-0 38°60 1 ” FP 995-1 38:13 1 ” ” 41002°9 37°75 In ” = 009°4 37°55 1 ” ” 012-7 36°70 1 ” ” 027°1 36°45 1 ” fc 031-2 35°13 1 ” ” 053°5 34°84 1 ” -c 058-4 34:44 1 a ” 065-1 33°85 2 7” ry 075:1 33°37 1 cr, es 083:2 32°97 1 a9 3 090:0 32°64 1 + of 095°6 32°41 1 3 My 099-4 31°92 In p or 107°8 31-7 In 4 3 111 31°35 J os a 117°5 30°95 Ind oF 7 124°2 30°23 1 7 - 1363 29°55 1b “6 + 147°9 29°71 1b oh f 155 bo REPORT—1900. URANIUM—continued. | Reduction o Wave-length Intensity | pas Oscillation Spark and Sern Tt Frequency Spectrum Character A+ ne in Vacuo A 2428°53 1 0-72 12:1 41165'1 28°19 1 “ 12:2 170°7 27°73 1 5 > 178°6 27°56 u 5 + 181°5 27:20 1 + = 187°5 26°65 1 45 “3 196°9 26°20 1 + i 204°5 25°46 In % a 217:1 2571 In oa i 223 24°5 In "9 s! 230 24:28 1 ” + 237-2 23°84 1 | 7 3 244-7 23°35 In ) + 253:0 23°15 1 3 + 256°4 22-7 1b “ + 264 22:0 1b r 5 276 20°6 1b O71 - 300 19°69 1 > > 315°5 18-90 1 » 3289 18°44 2 ie 5 336'8 18:00 1 en * 344:3 P iene iL ” ” 349:0 16°85 In » + 3643 16°52 In » a 370°7 14:7 Ind 6 7 401 14:20 In » * 409-4 13°77 1 ” 3 4168 13°05 1 » 9» 429-1 12°60 1 12°3 4378 12°38 1 35 =A 440°6 11:97 uh ” ” 447°6 11:50 1 + 455°7 10°35 In » -F) 4755 09°67 1 4 3 487-2 09°37 1 1 a 492°3 07°67 1 5 + 521°7 07-15 1 i 530°6 06°77 1 s = 537°2 06°54 1 Ff 541°2 06:3 In + + 545 05-87 In » $ 552°7 04:51 1 ob as 576°2 03:50 2n + - 593:°7 03-00 In “5 3 602°3 02°68 1 + =p 609°7 02°28 1 5 + 6148 01°55 In = = 6271 01:4 In “A is 63071 01-2 In x a 633°5 00°55 1 7 6449 00:42 1 5 - 64771 00-09 1 mn Of 652'8 2399°85 it 5 ¢ 657-0 98°65 In , = 6779 97-80 1 ae Las 692°5 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMEN'rS. 293 : URANIUM—continued. Reduction to Wave-length Intensity | Vacuum Oscillation Spark and Frequency Spectrum | Character | 1 in Vacuo | A+ nA 2497-45 2 \ 0°71 12:4 41698°6 : 97°20 2 i 4 703°0 96°23 1 % a 719°'8 94-14. 1 es is 756:2 93-32 In Fe a 770°6 92°8 In = 3 780 92°4 In ee 5 787 92°71 In Pe 7 792 91-68 In 3 - 799°3 91:07 1 - i 809°9 90°80 1 te Pe 814'6 90°48 1 5 3 820:2 90:2 1nb ny A 825 89°33 il a i 840°4 88°51 1 - a 854'8 87°30 ih i 3 8759 87:0 1inb a Al 881 85°65 1 55 AA 904-9 85°39 1 Fe Pe 909°5 85°18 1 a 4. 913°2 83°45 iInb . 3 943°6 83:00 1 Pf 12'5 951-4 } 80°8 In * us 990 . 79°85 1 we iy 42006°9 78°67 1 3 iA 027°8 78°24 2 ‘4 - 035-4 2 W791 2 Pa a 041:2 17-58 1 5 ik 047:3 77:05 1 5 3 056°5 76°61 1 oe 3 064°3 76°24 1 5 % 070°9 75:92 1 es Pe 076°5 74:2 inb 55 af 107 73:00 1 0:70 3 128:2 72°85 In PR id 131°1 72:0 In a 3 146 71°6 In or sf 153 70°96 1 a My 1645 70'8 1nb m7 3 167 7017 In 33 * 178°6 69°12 In Ae AS 197°3 68°50 In % 12°6 208°2 68:2 1Inb = a 214 67°5 1Inb a i 226 67°20 In 3 - 231°4 66°7 Inb 3 4 240 66:05 ln ~- F 251:9 65:7 1nb ee Ki 258 65:28 In 5 ve 265°7 64°34 1 Ee 3 282°5 64:0 1nb ss oy 289 63°50 1 iP = 297°4 62°8 inb PA a 310 62°44 1 rs wy 316°5 62:1 1inb ee * 323 294, REPORT—1900. URANIUM—continued. Reduction to Wave-length Intensity Vacuum Oscillation Spark and Frequency Spectrum Character ita in Vacuo A+ r 2461:53 1 0:70 12°6 41332°9 61:23 1 ” ” 338°2 60°85 In ” » 344-7 59°5 Inb » 33 369 58°92 In os 3 379°7 58:28 1 ” “ 391°2 58:02 1 ” , 395-9 57:67 1 = + 402°2 56°95 1 3 . 415-1 56°53 In 4 * 4227 56°13 1 x is 430°0 55°70 1 ” " 437°6 55-40 In » 3; 443°1 55:20 1 ” 4 446-7 54:83 1 * A 453-4 54:3 iInb + 12:7 463 53°6 Inb * 6 475°5 52°9 Inb ” i 488 51:96 2 “5 3 5051 50:2 Inb a 5 537 49:97 2 + a 541:0 49°70 2 FP) 2 545°9 49-00 In 35 » 558°6 48°35 In o o 570°4 47-6 ind + 6 584 47-08 i fs 5934 46°26 2 op cf 608°3 45°50 in as 3 622-1 45 08 In as “6 629°8 44-65 1 “ “A 637°6 44-02 In a 2 649°1 42-96 1 ” aS 668°3 42-50 In + i 676°7 41°45 2 s 5 695°9 40-99 1 aye 128 T7041 40-44 1 a a 714:2 38°98 In 3 > 7226 ° 38°57 1 yy s 748°4 38:07 2n (Fe) ” ” 7T5T-o 37-01 2 3 777-0 36°50 In I + 7862 35°88 In a * 797°6 35-20 1 » AD eae 810°1 34:37 In “5 95 825°3 33:13 1 o : 849°2 32°65 1 ” % 857:0 32°23 | 1 5 5 8646 31:93 1 + = 870°1 30°28 1 3 4 900°5 29°50 1 53 ” 914-7 29°40 1 Re “ 9168 28°95 1 55 0 925:0 28°58 1 ay mh 931-9 28°35 In + ” 936:1 27:93 1 %5 9 943°8 ig ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. URBANIUM—continued. 295 Wave-length Spark Spectrum 2427-45 27:07 26°50 25°72 25°51 24°90 24-07 23°44 21-6 21:1 20°22 18°51 18°21 17-9 17°6 17-2 15°92 15:07 14°43 14:22 13°87 13°23 12-60 11°67 10°71 10°43 09-80 08-80 08°35 06:94 05°68 04:46 03°95 03:70 02°75 01:97 01°55 01:0 00°80 2299°22 98-41 97°77 97°06 96°91 96°29 95°93 95°70 95°40 94°93 94:53 93°65 91°69 90°70 90°60 89°33 Intensity and Character { Reduction to Vacuum A+ Oscillation Frequency in Vacuo i=] cal aad Bae _ =] low In BB pete et Reet toh ae ee BREE HE DH eee PPE pee be 42952°8 959°6 970°0 984°6 988-4 SSSPY 3015-2 026-7 061 070 085:5 431183 123°8 130 135 143 166°6 1823 194-3 198-1 204'6 216°6 228°4 245°8 263°7 269°0 280°8 299°5 308°0 3345 358'2 381-1 390°7 395-4 4133 428-1 4360 446 450-0 4799 495:2 507-4 520°8 5237 535-4 542°2 546°6 552°3 561°2 568°8 585°5 622-8 641-7 643-6 667°8 296 REPORT-—1900. URANIUM—continued. Reduction to Wave-length Intensity Vacuum Oscillation Spark and Frequency Spectrum Character 1 in Vacuo A+ =— A 2288°97 il 0:69 13:1 43674:7 88°66 1 FS 4 680°5 88°35 1 55 13:2 6864 87°85 1 od 3 696:0 86°82 1 % > 715°6 85-76 In o 5 7359 85:23 In _ A. 746-1 84:90 1 ¥ 3 752°4 83°80 2 Ry 5 T7135 83°42 In 3 3 780°8 82°85 2 9 Fs TILT 81-9 In " = 810 ' 81-20 1 Fe a 823-4 81:08 1 5) 4 8266 80:20 1 a # 842°6 80:05 1 t 4 845°5 79:15 1 4 #3 862°8 78:7 In # Fe 8715 785 In : D 875 78:0 In ¥ 5 885 77°65 1 0°68 3 891-7 7715 In % 5 901:3 76°80 In 5) 5 908°1 76°25 In 5 a 918°7 76°10 2 FR ; 921°6 7518 1 7 13:3 939°3 74:65 1 F y 949°5 74°55 1 by 9514 74-15 2 . 3 959°2 73°93 1 3 “A 963°4 73°44 2 iS E 972°9 72:73 1 7 ‘ 986°6 72°40 1 5 . 993°0 71°85 In 9 Ft; 44003°7 10°37 1 4 5 032°4 69°8 Inbr i +3 043 68:9 Inb - : 061 68°55 In i A) 067-7 67:3 Inbr i, - 092 66:02 2n % 5 116°9 65°50 2n ie s 127-1 64-4 Inb ms = 148°5 63°90 In 5 a 158°3 63°37 In # 13°4 168°3 62-80 in ss £ 1796 62°45 In A 7 186°5 61:5 In - - 205 59-70 1 “) 4 240°2 58-00 In . 5 273'6 54:60 In i * 340°4 52°8 ln fn A 376 52:47 1 9 . 382°3 51:18 1 x 5 407-7 49°93 il As 13°5 432°3 49°35 In 443°8 — ao aes ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 297 URANIUM—continued. Reduction to Wave-length Intensity | Vacuum Oscillation Spark and | Frequency Spectrum Character 1 in Vacuo juste = A | - 2248°83 1 0-68 13°5 44454°1 48:06 - 2 i‘ <3 469°3 47:12 1 s Ms 487°9 46°34 1 cs 3 503°4 45:00 In e f 529°9 44°40 In re i 541°8 44-17 In _ 4 5464 43°65 In Fe 556-7 43°45 In aS i 560°7 42-73 In 3 7 575°0 40:18 1 ~ S 625°8 69°9 In . 3 631 38:02 1 af 136 668°8 37:46 2 os = 679'9 36°57 1 Bf ” 695°7 35°88 1n zn - 7115 34:0 Inb 5, 7 749 32°88 In FE ¥ T7116 32°41 In F- Ps 781-0 30°67 In # “ 816-0 29°6 Inb 0°67 on 837°5 28°88 1 4 . 852°0 28°39 In 3 ‘3 861°8 28:23 In x . 8651 27°95 In Fa *s 870°7 27°18 In sa * 8862 22°35 1 = 13°7 983-7 21°5 Inb a 3 45001 19°32 In r 5 045-1 17°63 In AS - 079°5 16°15 In a > 109°6 15°45 In 2 33 1239 10°96 In . 13°8 2154 06:05 In . 6 31671 00°80 1 13:9 424-1 2194°85 1 5 ii 547°3 Isomeric Naphthalene Derivatives.—Report of the Committee, consisting of Professor W. A. Titpen (Chairman) and Dr. H. EB. ArM- STRONG (Secretary). (Drawn up by the Secretary.) THE investigation of the action of bromine on betanaphthol, referred to in the 1898 Report, has been continued during the past year with the assist- ance of Mr. W. A. Davis. One of the most important points established is that the nature of the product obtained on tribrominating is largely a question of the conditions. In the presence of a solvent (glacial acetic acid) the tribromonaphthol melting at 155° is the chief product ; but if bromine be used alone, and the action take place rapidly at 100°, the isomeric tribromonaphthol (m.p. 159°), described in the 1898 Report, is principally produced. This result is more particularly of interest on account of the fact that the latter compound contains but one, whilst the 298 REPORT—1900. former contains two, of its bromine atoms in the hydroxylated ring— which is proved to be the case by their behaviour on oxidation, the tribro- monaphthol melting at 159° being convertible into dibromo-, and that melting at 155° into bromo-phthalic acid—so that in the one case the non- hydroxylated ring, and in the other the hydroxylated ring, is attacked. Unexpected difficulties have been encountered in attempting to deter- mine the position of the second bromine atom in the hydroxylated nucleus of the tribromonaphthol melting at 155°. This compound affords a dibromoquinone isomeric with that produced on decomposing the dibromo- nitroketo-compound derived from dibromonaphthol. Both these dibromo- quinones are converted into 1 : 3: 4 bromophthalic acid on oxidation. Consequently the one contains a bromine atom in position 3, and the other a bromine atom in position 4. When subjected to the action of aniline, however, both yield the same two anilides. O O wo: OH NH.Ph Sa ke , ag Br Br 2 NH.Ph NH.Ph Nor have results yet been obtained by means of alkalies which afford a solution of the problem. The dibromoquinone obtained from the bromonaphthol melting at 155° is remarkably sensitive to oxidation, being slowly converted into the dibromohydroxy-quinone when kept ; a result which appears to favour O OH Br Br O the view that bromine is present in the tribromonaphthol in position 3. The dibromoquinone in question may be recrystallised from ethylic acetate, but if left too long in contact with the solvent it is converted into an infusible condensation product. -This quinone is therefore a compound which it will be desirable to study in detail. The tribromonaphthol melting at 155° is acted on with difficulty by bromine, remaining for the most part unchanged when its solution in acetic acid is digested with bromine during thirty to forty hours at 100° to 120°, only a small portion being converted into the tetrabromonaphthol melting at 172°, described by Armstrong and Rossiter. The tribromo- naphthol melting at 159°, under similar conditions, is without difficulty converted into a tetrabromonaphthol melting at 184°, which is convertible into a tribromoquinone isomeric with that obtainable from the isomeric tetrabromonaphthol. A third tetrabromonaphthol has been obtained in small quantity together with that melting at 184° by acting directly on betanaphthol with dry bromine. It is distinguished by yielding a tetra- bromonaphthaquinone. Both tribromonaphthols are easily reduced at 100° by a saturated ON ISOMERIC NAPHTHALENE DERIVATIVES. 299 solution of hydrogen iodide, the bromine atom in position | being dis- placed. Two new dibromonaphthols are thus obtained: that from the tribromonaphthol melting at 155° melts at 137° to 138°, and that from the isomeric naphthol melts at 127°. On digesting these dibromonaphthols with alcohol and sulphuric acid under similar conditions that containing one of the bromine atoms in the hydroxylated ring yields only about 55, whilst that containing both bromine atoms in the non-hydroxylated ring yields about 61 per cent. of ether. A comparison of the behaviour of the various chloro- and bromo- betanaphthols towards hydrogen iodide with their behaviour on etherifi- cation is of interest as showing that both changes are subject to similar influences ; they therefore may be discussed from the same point of view. As the reducing effect is confined to the bromine atom contiguous to the OH group, this alone being displaced by hydrogen, the OH group must be supposed to be concerned in the change. Probably it exercises an at- tractive influence, and this influence must be regarded as subject to modi- fication by every change in the hydrocarbon radicle, so that reduction takes place less readily just as etherification takes place less readily in the case of the more fully substituted compounds. The etherification of the derivatives of betanaphthol has been discussed by Mr. Davis from this point of view in a paper published in the ‘Transactions of the Chemical Society ’ early in the present year (77, 33). On the Constitution of Camphor. By A. LarwortH, D.Sc. [Ordered by the General Committee to be printed im extenso.] THE question of the constitution of camphor has occupied the attention of a large number of chemists for many years, and it still presents oppor- tunities for much speculation. Recently, however, it has come to be fully recognised that the earlier writers on the subject were misled by the ease with which benzenoid compounds could be obtained from many camphor derivatives, and it is now quite clear that the greatest care must be exer- cised in attributing special significance to evidence based on observations of this kind. The formation of large quantities of p-cymene and carvacrol from cam- phor by the action of phosphorus pentoxide was the basis of some of these earlier speculations, and to carry the arguments to their logical conclusion it would be necessary to make the formule account for the production of m-cymene, which is obtained in considerable amount when zinc chloride or phosphorus pentasulphide is the agent,! and also of 1. 2. 4 . dimethyl ethyl benzene and 1.2.3.5 tetramethylbenzene.2 The formation of 1.3. 4 acetyldimethylbenzene by the action of sulphuric acid on camphor 3 would also require elucidation. It appears natural to suppose that, if we are still unable to discover with certainty the principles underlying the changes referred to, we should also be cautious in interpreting the meaning of other transforma- tions which involve any alteration in the structure of closed rings, and it is now pretty generally recognised that the divergence of opinion which still exists with regard to the constitution of the camphor nucleus must be due ' Armstrong and Millar, Ber. 16, 2225. 2 Thid., loc. cit. $ Armstrong and Kipping, 7rans. Chem. Soc., 68, 75. 300 REPORT—1900. to the occurrence of unsuspected intramolecular changes during reactions which are at present deemed susceptible of only one simple interpretation. In the case of a problem of this kind in which a very large amount of experimental material has to be dealt with, some of which appears to point conclusively to one view and some in an equally unequivocal manner to another, it would appear to be the most logical course to sift the material in such a way that the relative value of the evidence on each side may be compared, and, if possible, so as to gain a clue as to the exact points at which the tendency appears to change, so that particular atten- tion may then be directed to those points. In the present communication it is proposed first of all to select from the material those facts which bear directly on the points at issue, accepting only those conclusions which no longer reasonably admit of dispute, and then to discuss the significance of the rest of the evidence relating to the still undecided question of the ultimate structure of the camphor molecule. A.—_GENERAL NATURE OF CAMPHOR. Camphor has the formula C,,)H,,O0: it isa ketone, as it yields well- defined hydrazones, an oxime and a semicarbazone. It is saturated, and therefore must be considered to consist of two closed carbon rings, of which one includes the carbonyl] or ketone group > CO. As it will clearly be of importance to be able to refer to either of these rings, one will afterwards be termed the ketone ring, and the other the hydrocarbon ring. B.—PROPERTIES AND TRANSFORMATIONS OF THE KETONE RING. 1, THe Ketone RING contains THE Group —CH,.CO— That the carbonyl group >CO of camphor is in direct attachment to a methylene group —-CH,— is proved conclusively by the following considerations :— (a) Formation of Camphoric Acid by the Oxidation of Camphor. When camphor is treated with the usual oxidising agents it is con- verted into camphoric acid, C,)H,,O,, a saturated, dicarboxylic acid. This transformation is simply explained only by the assumption that the change proceeds in accordance with the scheme , os COOH H | > C,H 8 “\Nco * "coon Camphor. Camphoric Acid. (b) Formation and Properties of the simplest Substitution Derivatives of Camphor. (i) Halogen and Nitro-compownds.—Camphor ordinarily yields only mono- and di-substitution derivatives (termed a-derivatives) on treat- ment with the characteristic substituting agent such as the halogen or nitric acid, and with aliphatic saturated ketones the position of substitution is at the carbon atom contiguous to the carboxyl group. ON THE CONSTITUTION OF CAMPHOR. 301 The a-mono-halogen derivatives, such as a-monobromocamphor, on treatment with oxidising agent are converted into camphoric acid CHBr COOH ee i war COOH The a-di-derivatives are only oxidised with great difficulty, and on treatment with alkalis are usually converted into the a-mono-derivatives. Thus when a-bromocamphor is chlorinated it yields a mixture of two stereo- isomeric bromochlorocamphors, both of which are converted into a-chloro- camphor on treatment with alkali, so that both halogen atoms must be attached to the same carbon atom ! ee CClBr yee iis) CO 7 OO ‘co a-Bromocamphor. aa-Bromochlorocamphor. a-Chlorocamphor. Again the a-monohalogen derivatives when heated with nitric acid are converted into nitroderivatives, which yield a-nitrocamphor on treat- ment with alkali ; nitrocamphor when heated with acids is converted into the oxime of camphoric anhydride. Moreover the a-nitrocamphors exist in tautomeric forms, characteristic of nitrocompounds containing the group >CH.NO,.? cs Poo: CH.NO, CsHiic aes Beare C:N.OH —-C,H Beer 8 8 “\co7 (ii) Camphor yields Alkylidene Derivatives on Treatment with Alde- hydes.—When camphor is acted on by, for example, benzaldehyde, in ‘presence of sodium, condensation occurs, and a benzylidene camphor is finally obtained. Its constitution must be expressed by the formula © = CH-PE CsA s< | "Noo as only ketones containing the group —CH,.CO— are known to react in this way. (iii) Camphor is capable of taking part in the Claisen Reaction.—The Claisen condensation, which is capable of application among saturated ketones only to those containing the group —CH, . CO—, is applicable to camphor under certain conditions, and isonitro-, and hydroxy-methylene camphor, &c. are readily obtained. These can only be expressed by the formule ye : N.OH C : CH.OH | and C,H C,H 8 tac do 1 Lowry, Trans. Chem. Soc., 78, 569. * Tbid., 73, 986. 302 REPORT—1900 2. THe RELATION BETWEEN CAMPHOR AND CAMPHORIC ACID IS IN REALITY THE SIMPLE ONE EXPRESSED BY THE SCHEME It has been usual in discussing the relationship between these two substances to dismiss the subject with a few words, but the point requires much more careful consideration and proof than it is usually deemed worthy of, and it cannot be insisted too frequently that in dealing with the mutations of closed-chain compounds, such as the derivatives of cam- phor, such transformations should be regarded from all points of view, especially, as in the present instance, where the evidence derived from the different fields of work cannot be viewed in its entirety until the point is decided beyond all doubt. In the case in question, fortunately, there is no doubt whatever that the ordinary view is the correct one, as, besides the various modes in which it is possible to pass from camphor to camphoric acid, which have already been referred to, the relationship has been established by a series of simple changes which render it possible to traverse the ground in the reverse direction. The evidence is as follows : |— (a) Camphorie Acid readily yields Homocamphoric Acid. When camphoric anhydride is treated with sodium amalgam under suitable conditions, it is reduced to a lactone, campholide, as follows :— co CH 7) So aon 8 “CO”, a 8 “co and campholide when heated with potassium cyanide yields cyanocampholic acid, from which homocamphoric acid is easily obtained on hydrolysis. The changes are of the following kind :— 2 Cc So +H,0 ott: me, po. CH,.CN /CH2.COOH O>C,H C,H, .< Tad CO” <.\ .. \COGamEE fae COOEL Campholide. Cyanocampholic Acid. Homocamphoriec Acid. (b) Homocamphorie Acid and Camphor are related to one another in the following way : CH,.COOH CH, Cs. ae | COOH CO and the evidence on which this statement is based is twofold. a-Cyanocamphor yields Homocamphoric Acid on Hydrolysis. —Cyano- camphor, a product of the action of cyanogen or cyanogen bromide and C,H ' Haller, Compt. Rend., 122, 446, ————————— CC ON THE CONSTITUTION OF CAMPHOR. 303 on sodium camphor, or of the dehydration of the oxime of a-camphor- aldehyde, must necessarily be an a-derivative. CHNa CRON CH, | +Br.CN=C,H,,/ | +NaBr co eo pee :N.OH fae oe CoH pO Oak | CO CO and when this compound is boiled with alkalis it suffers hydrolysis in two senses, being converted into ammonia and homocamphorie acid.! CH.ON CH,.COOH & apie os ae + 3H,O =C,H +NH, '“\cooH (c) Camphor may be regenerated from Homocamphoric Acid. When the barium salt of homocamphoric acid is subjected to dry distillation it is broken up into barium carbonate and camphor, a change which must be expressed by the equation CH \Ba=O,5e plop BaeO, L CO 3. THE Kerrone RING Is EITHER A 4- oR A 5-Carspon RING. Since camphoric acid very readily affords an anhydride on treatment with acetyl chloride, even in the cold, it follows that it must be a deriva- tive of succinic or of glutaric acid, so that it may be represented by one of the formule 5: COCOOEL ine: C.COOH | | or Bs OS: sees C.COOH | sesseee C.COOH poset ¢—cH paula. 6—CH, : | | | or -C: ete C—co | ee males CH—CH, | C—CO C ! Haller, Dissertation, Nancy, 1879. * Haller, Compt. Rend., 122, 446; and Baeyer, Ann., 289, 6. 304: REPORT—1900. In support of this conclusion there may be advanced a number of well-established facts, and the necessity for the discussion of the points involved may be made the occasion for introducing the nomenclature necessary for reference to the derivative of camphoric acid. 1. CampHor ACID CONTAINS ONLY ONE HyproGEeN ATOM IN THE a-POSITION WITH REGARD TO A CARBOXYL GROUP. (a) Bromination of Camphorie Acid. Camphoric acid is capable of affording, by direct bromination, one, and only one, monobromo-derivative, w-bromocamphoric acid. From the study of a very large number of acids it has been ascertained that it is possible to introduce as many bromine atoms as there are hydrogen atoms in the a-position with regard to carboxyl groups, and in each case where the products have been completely investigated it has been shown that the entrant bromine atoms occupy the a-position. The conclusion thus derived regarding camphoric acid is confirmed by a large number of observations, and there is no sufficient reason to imagine that the bromination of camphoric acid pursues any but the normal course. (b) Differential Reactivity of the two Carboxryl Groups. Camphorie anhydride on treatment with ammonia yields exclusively, or almost exclusively, a-camphoramic acid. This on distillation loses water, yielding camphorimide, which when subjected to alkaline hydro- lysis affords only 6-camphoramic acid. The reactivity of carboxyl or carboxyl groups in aliphatic compounds invariably appears great or small according as the adjacent carbon atom is hydrogenised or not. The above observations, which show that there is an enormous difference between the reactivity of the carboxyl groups in the anhydro-camphoric derivatives, are doubtless accounted for by the fact that only one of the two carboxyl groups of camphoric acid is an attachment to a hydrogenised carbon atom. On this assump- tion the course of the changes referred to may probably be expressed as follows :— OH O ie ll es CH. COx mores Oe) Cagis CH.C.NH, a © .CO oi ney C .CO.0H C C Cc Camphoric Anhydride. Hypothetical Addition a-Camphoramic Acid. Caen Ye O 2 ae OH O 4 VA een). / bees CH oN Se ~~ CH. C: OH CH.C.OH > NH+HL0 > : NH > nde C.co at GOO C.CO.NH, C Camphorimide. 8-Camphoramic Acid. — ON THE CONSTITUTION OF CAMPHOR. 305 Camphoric acid also yields two series of alkyl hydrogen esters, which have been obtained in the following way :— Camphoric anhydride when treated with sodium ethoxide yields the sodium salt of ovtho-ethyl hydrogen camphorate ONa O A Vi Pes, CH. CO. SaM OLY C—OEt a CH. CLORE : J O+Et.ONa > : Pp? Sx : ee. C.CcOoO eres OT pote Ca UG)ONa, C C Camphorie Anhydride. ortho-Ethyl Hydrogen Camphorate. Diethyl camphorate when hydrolysed with soda, however, affords the sodium salt of a//o-ethyl hydrogen camphorate. OEt | vi oe CH.CO.0Et ~~ CH. COOH : +Na.OH > : ONa =. C.CO.OEt ~---C.CO.OEt C Diethyl Camphorate, a CH.CO.ONa Re : + Et.OH Beane C.CO,.OEt C allo-Ethyl Hydrogen Camphorate. The carboxyl groups of camphoric acid have therefore been referred to in two different ways, namely— CH . COOH (a- or ortho-) C.COOH (- or allo-) C The above inferences regarding the constitution of the two camphor- amic acids and the two ethyl hydrogen camphorates receive confirmation in the behaviour of the former on treatment with hypobromite (compare E. 2. c.), and of the latter when subjected to electrolysis (compare E. 2. a.). (ce) The B- or Allo-carboayl Group of Camphoric Acid represents the Carbonyl Group of Camphor. Whilst the facts on which this conclusion depends are few in number, they are such as to render their interpretation simple and beyond ques. tion. The following may be mentioned here. When isonitrosocamphor is warmed with hydrochloric acid it is converted into a-camphoramic acid,! and, in accordance with the con- ‘ Claisen and Manisse, Ann. 274, 78 1900, x 306 REPORT— 1900, stitution of the latter compound (C. |. b.), the change can only be written as follows ;— pete. CH.C:N.OH _.. CH.CO,NH, | +HOH =) cone C—O ----C.COOH C C Lowry’s observation that a-nitrocamphor yields the same camphoryloxime as is obtained directly from camphoric anhydride by treatment with hydroxylamine leads to the same conclusion (compare B. 1. b, i.), 2, FORMATION OF CAMPHENONE, When a-aminocamphor is treated with nitrous acid it is converted into diazocamphor, which loses nitrogen when heated and yields consider- able quantities of camphenone, C,)H,,O, which has all the properties of an unsaturated ketone.! N _- OH. CH.NHg cHOL I ne OCH : > | : 1) NaN Sea : so G=Co es @— CO -- C—CO C Cc C Aminocamphor. Diazocamphor. Caraphenona, 3. FoRMATION OF DEHYDROHOMOCAMPHORIC ACID, When homocamphoric acid is brominated it yields a monobromo- derivative, a-bromohomocamphoric acid. When the diethyl-ester of this monobromo acid is heated with quinoline and then with alcoholic potash it loses hydrogen bromide, affording dehydrohomocamphoric acid, which is certainly an af-unsaturated acid. Taking into consideration the relationship subsisting between camphor and homocamphoric acid, this fact is readily explained by the assumption comprised by C, and it may be added that its behaviour on oxidation is only explicable by the aid of that view (compare E, 3.). een CH—CH, -..-.-CH.CHBr.COOH _ .....C:CH.COOH aoa saa Cc —CO~ ---C.COOH ~C,COOH C C C Camphor, a-Bromohomocamphorie Acid. Dehydrohomocamphoric Acid. D.—CAMPHOR AND CAMPHORIC ACID CONTAIN TWO NON-EQUIVALENT ASYMMETRIC CARBON ATOMS. Camphor and camphoric acid are optically active, and therefore contain at least one asymmetric carbon atom. Whilst the former is only known in two enantiomorphous forms and their externally compensated _ inactive combinations, the latter is known to exist in six forms, of which two pairs are enantiomorphously related, and the other two forms are externally compensated mixtures of the other pairs. 1 Angeli, Gazzetta, 28 [2], 351. ON THE CONSTITUTION OF CAMPHOR. 307 The six forms of camphoric acid are completely explained on the assumption that in the molecule there are two asymmetric carbon atoms which are not equivalent. Designating the two carbon atoms by the letters A and B, the six forms may be represented by the combinations, no internally compensated form being possible : (A,B,) and (A,B,)...d- and /-camphoric acid. (A,B,) and (A,B,)...d- and /-isocamphoric acid. A,B,+A,B,)... Inactive camphorie acid. (A,B, +A,B,)... Inactive isocamphoric acid. It does not appear that the sign of both asymmetric carbon atoms can be reversed by simple means, but d-isocamphoric acid may be obtained from d-camphoric acid fairly readily ; as, for example, by treatment with phosphorus pentachloride and water successively, whilst the reverse change may also be effected by suitable means, such as boiling with acetyl chloride, or by the process of bromination, when ordinary bromocamphoric- anhydride is obtained. The readiness with which one of these asymmetric carbon atoms is affected makes it seem certain that this must be the atom on which a carboxyl group and a hydrogen atom are attached, as there is here the only grouping where the existence of tautomerism, or simple internal change, appears possible. A glance at the simple scheme for camphoric acid, moreover, CH.COOH C.COOH 6) wakes it appear highly probable that each carboxyl group is an attach- ment to one or other asymmetric atom, and the difficulty of conceiving any simple internal change which would affect the condition of the second asymmetric atom accounts sufficiently well for the non-occurrence of inversion in this instance. The occurrence of only two enantiomorphously related camphors is probably dependent on stereochemical considerations, analogous to the non-formation of anhydrides from ¢rans-dicarboxylie acids of the poly- methylene series. E.—_DEGRADATION OF CAMPHOR DERIVATIVES. Whilst the material which has already been deaJt with affords us much useful evidence regarding the structure of the ketone ring, there is little or none of it which affords us any assistance in coming to any conclusions regarding the hydrocarbon ring. In order to gain any conception as to the structure of the second nucleus it becomes necessary to consider the nature of products which are obtained when this ring is broken down in various ways. It will be convenient to refer to each of the various modes in turn, and to consider the constitution of the products of known character as they come under consideration. 1 Aschan, Acta soc. Sci. fennice, 21, 1. x2 308 REPORT—1900. 1. OxIDATION OF CAMPHOR AND CampHoric ACID. (a) Oaidation with Nitric or Chromic Acid. When camphor is subjected to prolonged heating with nitric or chromic acid a large number of products are obtained, of which the more important are camphoric acid and its oxidation products, namely, cam- phanic acid, camphoronic acid, and trimethylsuccinic acid, together with a small quantity of isocamphoronic acid, which is certainly an independent product, as it does not appear to be produced from camphoric acid under any circumstances. (i.) Constitution of Camphoronie Acid.—From a study of the products obtained by the dry distillation of camphoronic acid Bredt was led to the view that this acid had the structure COOH. CMe,. CMe(COOH).CH,.COOH ! and this conclusion has been rendered final by the synthesis of the acid by Perkin and J. F. Thorpe? in a manner the course of which admits of only one interpretation. (ii.) Constitution of Isocamphoronic Acid.—Isocamphoronic acid has the structure OMe,(COOH).CH(CH,.COOH),, as follows from the following observations :— When the acid is warmed with sulphuric acid it loses carbon monoxide, and is converted into a lactonic acid of known constitution, namely, terpenylic acid : CMe, . CH.CH,.COOH CMe, . CH.CH,.COOH Le fa Ba | +CO+H,0 3 COOH CH,.COOH O CH, \co7 Additional support for the formula given is supplied by the following indirect observations :— a-Keto-isocamphoronic acid, obtained by a series of changes from pinene, yields isocamphoronic acid when reduced, and when oxidised with lead peroxide and acetic acid is converted into a-dimethyltricarballylic acid. The latter acid is not a malonic derivative, and when treated with bromine is converted into the lactone of the hydroxy-acid, which yields a-dimethylsuccinic acid on fusion with potash : CMe,.CH.CO.COOH CMe, .CH.CH,. COOH | | =2 | COOH CH,.COOH COOH CH,.COOH a-Keto-isocamphoronic Acid, Isocamphoronic Acid. L CMe,.CH.COOH CMe,.CH .COOH CMe, . CH, | mon | al COOH CH,.COOH CO CH.COOH COOH COOH No a-Dimethyltricarballylic Acid. Lactonic Acid. a-Dimethylsuccinie Acid. 1 Bev., 26, 3049, 2 Trans, Chem. Soe., 71, 1169. 3 Tiemann, Ber., 29, 2612, ON THE CONSTITUTION OF CAMPHOR. 509 (b) Ovidation of Camphoric Acid with Dilute Cold Permanganate. When camphoric acid, dissolved in the requisite quantity of soda, is allowed to remain with cold dilute potassium permanganate solution for some months, it is converted into a dibasic acid having the formula C,H,,0; or C;H,,O (COOH), and oxalic acid, the products being in approximately equivalent amount. This acid yields only additive pro- ducts with hydroxylamine or hydrazines, so that the fifth oxygen atom does not possess true ketonic functions. On reduction it yields, first, a lactonic acid, C,H, .0,, and then «)3G-trimethylglutaric acid. Balbiano explains the behaviour of the acid C,H,,0, on the assump- tion that it isan acid possessing the structure of an oxide derived from a dihydroxy acid COOH . CMe. CMe, . CH . COOH, Sep qi and it is not easy to understand what other view can be taken. The successive stages of its reduction are consequently CMe. COOH CMe .COOH CHMe. COOH | one | Ne | CMe, SO is CMe,0(!) > OMe, | ae OOH CH, « CO CH, . COOH.? 2. THE PRODUCTS OBTAINED BY ELIMINATING A CARBOXYL GROUP FRoM CampHuoric ACID. (a) Electrolysis of the Isomeric Ethyl Hydrogen Camphorates. When the two isomeric ethyl hydrogen camphorates (compare C. 1. b.) are submitted to electrolysis the products consist for the most part of esters of unsaturated, ciosed-chain, monobasic acids, produced in accord- ance with the equation OH Googe = C0, +H, +CsH). COOEE. (i.) Electrolysis of Ortho-ethyl Hydrogen Camphorate.—Ortho ethyl camphorate (C. 1. b.) on electrolysis yields mostly the esters of two isomeric acids, namely, campholytic and isolauronolic acids. These two acids are inactive, and are intraconvertible by processes analogous to ae whereby fumaric and maleic acids may be converted one into the other.® } Balbiano, Ber., 27, 2133. * Compare also Balbiano, Ber., 28, 1506; Atti Lincei, 1894, i. 278, and ii. 240; Gazzetta Chim. Ital., 26,1; and Ber., 80, 289 and 1901. Also Mahla and Tiemann, Ber. 28, 2151 and 2811, * Walker, Zrans. Chem. Soc., 68, 495, and 67, 347. « 310 REPORT—1900. Structure of Isolawronolic Acid.—The structure of this acid is almost certainly represented by the formula CMe,—CMe CH, | \cH, — C. COOH first suggested implicitly by Perkin! and independently by Bouveault ;? and the grounds for this statement are briefly as follows :— It is inactive, and cannot be separated into active forms. It therefore does not contain an asymmetric carbon atom. It is an af-unsaturated acid, as its dibromide loses carbon dioxide and hydrogen bromide on treatment with soda or sodium carbonate, a behaviour associated almost exclusively with a/3-dibromo acids. Moreover, dihydroisolauronolic acid is readily brominated, as usual in the a-position, and the mono-bromo acid on treatment with alkali affords isolauronolic acid and a-hydroxydihydroisolauronolic acid.* CMe,.CHMe CMe,.CMe ‘il rd | CH, a CH, aN | CH,. CBr.COOH CH,—C.COOH 8 Isolauronolic Acid. s CMe,.CHMe | a-Bromdibydroisolauronolic Acid. CH, yo CH,—CH \CooH a-Hydroxydihydroisolauronolic Acid. The latter compound when heated with lead peroxide and acetic acid affords a ketone which is identical with «/3;3-trimethylketopentamethylene, obtained by distilling the barium salt of «33-trimethyladipic acid.* CMe, .CHMe CMe, .CHMe CMe, .CHMe Je rs i. | CH, CH, _ CH, COOH ae ot SS Di e CH, — CH,—COo CH,—COOH \cooH Striking confirmation of the above formula for isolauronolic acid is afforded by the following series of reactions. Isolauronolic acid, when heated in closed tubes at 300°, loses carbon dioxide, and is converted into a hydrocarbon, C,H ,,, which yields y-acetyl- dimethylbutyric acid on oxidation. That the production of the hydro- ' Proc. Chem. Soe., 1896, p. 191. 2 Bull. Soc. Chim. (iii.), 19, p. 462. * Noyes, Ber., 29, 2326 and 1900, and Perkin, Z7ans. Chem. Soc., 78, 838. ' Noyes, Ber. ° ON THE GONSTITUTION OF CAMPHOR. 3il ee ek hee varbon is not attended with any isomeric change is proved by the fact that it yields, on treatment with acetyl chloride in presence of aluminium chloride, a ketone identical with that obtained by the action of zinc methide on isolauronolic chloride : CMe,.CMe CMe,.0Me CMe,.COMe vA | vA A GH, a OH, Ee CHS | 4. of CH,—COOH CH,—CH CH,.COOH } U OMe,.CMe CMe,.CMe CH, —| ign, “CH, “ideal CsHi se +HBr COOH COOH. or writing it in accordance with what we know regarding the constitution of homocamphoric acid (B. 2. b.) POR dee CH.CHBr. COOH veeeee GOH COOH : = OY C . COOH scene + COOH Cc C When the latter acid is oxidised with cold dilute permanganate it is } Walther, Ann. Chim. Ph. [iii.], 9, 177; Kachler and Spitzer, Annalen, 169, 179, and Perkin, 7rans. Chem. Soc. 78,796. * Noyes, Amer. Chem. Journ., 16,500; Ber., 28, 547,and 29, 2326. * Noyes, Ame, Chem. Journ., 16, 500; Ber., 27, 917, 28, 547, and 29, 2326. 314 REPORT—1900, converted into oxalic acid and camphononie acid (compare E, 2.a ii.), ah action which apparently must be expressed as follows : _C=CH . COOH CO +COOH . COOH GH, | ra | CMe, > | CMe, CH, CH, C. COOH ‘CG. COOH Me Me or __O=CH . COOH _00+C00H . COOH CH, CH, iru elee or. eee CMe, | CMe, “G. COOH NG. COOH! Me Me 4. ForMATION AND PROPERTIES OF THE CAMPHOLENIC DERIVATIVES. The isomeric substances a- and /3-campholenic acids are obtained in several ways, the most important of these being the dehydration of cam- phoroxine by various methods, when their nitriles are produced in large quantities : CioHi,: N.OH=C,Hi, . CN+H,0. Interesting, also, is the fact that a-campholenic acid is found amongst the products obtained by the action of sodium amalgam on /-dibromo- camphor. C,)H,, Br,O+2H+H,O0=C,H,; . COOH +2HBr. The campholenic acids are undoubtedly both unsaturated monobasic acids containing one closed carbon chain. The a-acid is optically active, whilst the 5-acid and all its derivatives are quite inactive ; so that both the asymmetric carbon atoms of camphor have been involved in the change whereby this substance is produced. Both the a- and the /3-acids have the double or ethylenic linking at the y- or ¢c-position, as both are readily converted into lactones when treated with dilute acids. a-Campholenic acid may be converted into /3-campholenic acid by several processes, and invariably becomes inactive during the process. It would appear from this that 6-campholenic acid is a secondary product of change. Each acid, on oxidation with potassium permanganate, is converted into a dihydroxydihydrocampholenic acid by addition of the elements of hydrogen peroxide in the usual way. When these dihydroxy acids are distilled they are converted by loss of water into new substances, pre- sumably ketonic acids, the a-acids affording pinonic acid, which is an oxidation product of pinene. ' Lapworth, Zrans. Chem, Soc., 77, 1056, ON THE CONSTITUTION OF CAMPHOR. 315 a-Dihydroxydihydrocampholenic acid is dewtrogyrate and on oxidation with chromic acid yields inactive isoketocamphoric acid, and with nitric acid gives isodiketocamphoric acid. Both of these latter contain acetyl groups, and isoketocamphoric acid is converted into bromoform and _iso- camphoronic acid (E. 1. a. ii.) on treatment with cold hypobromite. These changes are expressed by Tiemann ! as follows :— CMe,—CH—OH,, OMe,—CH—CH,, OMe,-—COH —CH, es a ee | | | | CH. > OH, > OH, > rea | | CMe =CH COOH CMe — bog COOH COMe COOH COOH COOH COOH COOH | | OH OH g-Campholenic Acid, a-Dihydroxydihydro- Isoketocamphoric Isocamphoronie campholenic Acid. Acid. Acid, N CMe, ae —CH, CMe, —CH -—OH, OMe, -—CH —-—OH, | | | CH, | co > | | | | CHMe—CO COOH COMe COOH COOH COOH COOH COOH Pinonie Acid, Tsodiketocamphorie Dimethyltricarballylic Acid, Acid. This scheme expresses the foregoing facts in a highly satisfactory manner, including the cessation of inactivity with the passage from a-dihydroxydihydrocampholenic acid to isoketocamphoric acid, and appears, moreover, to be the only mode of doing so. The inadequacy of any formula for campholenic acid or pinonic acid which does not contain the group . CMe .UMe, C C is shown by the fact that one of the products obtained by oxidising pinonic acid is hydroxytrimethylsuccinic acid, COOH .CMe(OH) . CMe,. COOH. A-Dihydroxydihydrocampholenic acid (of course inactive, since /-cam- pholenic acid has this property) on further oxidation with dilute per- manganate yields oxalic and y-acetyldimethylbutyric acid, which affords a-dimethylglutaric acid on treatment with alkaline hypobromite. Tiemann expresses these facts in the following way :— CMe, —CH—OH, er A OMe,—CH,—CH, cit | = di.on | BT | | 4. coon..coor Cue én COOH CHMe —CH on COOH COMe Goon p-Camplenc Acid, gBibghoiydibydro. Ape Orato Aci Such a change as that assumed in the transformation of the di- hydroxy-acid is obviously inadequate without further proof. Moreover the inactivity of }-campholenic acid receives no explanation whatever, as it is scarcely conceivable that the asymmetry of the carbon atom to which the activity of a-campholenic acid is due has been in any way destroyed. Proceeding backwards in a logical manner from the fact of the formation of y-acetyldimethylbutyric acid and oxalic acid, we are led almost inevitably to the formula for /-campholenic acid which was first suggested by Bouyeault,’ namely— CMe=C —CH, | CH, | CMe,—CH, COOH ' Ber., 29, 3006, and 30, 409, 2 Bull. Soc. Chem. [iii.], 19, 565. 316 : REPORT—1900. which contains no asymmetric carbon atom ; the oxidation of the acid is then readily understood : OH OF CMe = C——CH, CMe a CH, COMe COOH COooH | | | | CH, | => CH, | => | CH, 3 | | | | | CMe,—CH, COOH CMe.—CH, COOH CMe,—CH, COOH fB-Campholenic Acid. B-Dihydrox) dilydro- y-Acetyldimethyl- Oxalic campholenie Acid, butyric Acid, Acid. 5. FoRMATION AND CONSTITUTION OF CAMPHORPHORONE. When the calcium salt of camphoric acid is subjected to the action of heat it is converted into calcium carbonate and camphorphorone, C,H,,0 _—— CO.O CoH CO.O Camphorone has the structure co GHMe ©: CMe, Sca=C,H.C 500 + CaCO,, | | CH, — CH, as it is converted into a-methylglutaric acid on oxidation, and may be synthetically prepared by the action of sodium ethoxide on a mixture of a-methylketopentamethylene and acetone. Since these condensations in saturated ketones occur only at a —CH,.CO— group, the action must be expressed _CO CO GHMe CH,+OCMe,=CHMe C:CMe,+H,0 | V/ | | CH,—CH, CH,—- CH, as camphorphorone does not contain an acetyl group.” F.—THE FORMULA OF CAMPHOR. The earlier speculations regarding the constitutional formula of camphor require no special discussion at the present time, as they are of merely historical interest, and there is no doubt that the first great advance was made by Bredt in his paper on ‘The Constitution of Camphoronic Acid,’* and the value of his deductions has been greatly enhanced since the achievement of the synthesis of this acid by Perkin and Thorpe,‘ which provided a complete proof of the formula suggested for it by Bredt. Starting from the formula of camphoronic acid, as it is generally agreed we may do, and taking into account the fact that camphor readily yields cymene by the action of various agents, Bredt was led to advance the formula associated with his name. This formula has since been assailed by several chemists, notably Noyes, Tiemann, Bouveault, Blane, ~ 1 See also Tiemann, Be7., 28, 1079, 2166, &c. 2 Bouyeault, Bull, Soc. Chim. [iii.], 28, 160. 3 Ber., 26, 3049. 4 Trans. Chem. Soc.; 71, 1169. ON THE CONSTITUTION OF GAMPHOR. 317 Walker, and Perkin, but the formula suggested by Tiemann must now be regarded as quite out of the question ; whilst the formula specially advocated by Perkin, whilst greatly preferable, is now known to have no probability in its favour. It is significant that the chemists who at the present day strenuously advocate the acceptance of any formula other than Bredt’s have made a special study of isolauronolic acid. Latterly chemists have come to regard it as definitely established that camphor contains the grouping CMe.C ae \ CMe, | C aa / and it is easily demonstrated that besides three formula containing this complex, only one other structure for camphor can be devised which contains the grouping of carbon atoms of camphoronic acid, and also conforms to the established conditions referred to in B, C, and D. ‘That formula is CH,—CMe. CMe,. CO | | He CH. CH= en. but nothing further can be said in favour of it. Conclusive proof that the above trimethylpentamethylene nucleus is present in camphor is afforded by the fact that camphononic acid, which is obtainable from camphor in three entirely different ways, two of these involving no change in the hydrogenised nucleus, undoubtedly has the formula CMe.COOH. CMe.COOH. / wai ke N Ze 2% CMe, /CHa or CMe, CH, | y | (xe) d / CH, perf esl CH, CO (Compare E. 2. a. ii. and E. 3.) The only formule which contain this complex, and conform to the established conditions, are the Bredt, Perkin, and Perkin-Bouveault formule, namely CMe.CO CMe.CO CMe.CO | fe ee: | uf CH, Zi tis CH—CH, CMe, | CMe, | Me, | one .. CH CH, Sa A | | CH—CH, CH, CH, Bredt. Perkin.” Perkin-Bouveault.. ' Trans. Chem. Soc., 71, 1169, 2 In Petkin’s original paper, Zrans. Chem. Soc., 78, 819, the position of the —CQ- and —CH,— group in the ketone ring is the inverse of the above, 318 REPORT—1900. of which the second, as has already been stated, has nothing further in its favour, and it does not appear possible to explain by its use the properties and constitution of many important products obtained by degrading the camphor molecule in the various ways detailed in E. It is quite clear, therefore, that in the light of our present knowledge only two formule for camphor can be regarded as in the slightest degree probable, namely, the Bredt and the Perkin-Bouveault formule; and although it might at first sight appear an easy matter to decide between two formule so different in configuration, each still finds support in apparently incontrovertible evidence. A list of the facts to which each formula appears capable of ready application may be dealt with in turn, only those points being taken which appear to be of use in coming to a decision as to the relative value of the two formule. 1. Brept’s Formuta: affords simple explanations of the following points :— (a) The Constitution of a-Campholenie Acid and its Oxidation Products. The formation of a nitrite having the highly probable constitution assigned to a-campholenonitrite by Tiemann is readily explained as follows _(compare E, 4.) CH CH WN Ke | CH, | €H, Ci; }. Cie | CMe, | — H,0= | OMe, | CH, | C:NOH CH CN ee -l ~CMe ~“ CMe (b) The Non-formation of an Anhydride from Homocamphorie Acid. In accordance with Bredt’s formula, homocamphoric acid must have the formula (compare B. 2. b. and E. 3.) _ CH.CH,.COOH egal CH, | | CMe, On, 4 Sale “S CMe.COOH Homocamphoric acid has been shown to be incapable of yielding an anhydride,! a fact with which the above formula is in accordaricé, as it ) Bredt, Ann., 289, 5. ON THE CONSTITUTION OF CAMPHOR. 319 represents a substituted adipic acid, derivatives of which are almost invariably incapable of affording anhydrides when treated by the ordinary processes. Using the Perkin-Bouveault formula, homocamphoric acid would have the structure /CH,.CH.CH,.COOH / / / CMe, | ~~ CMe.COOH which is that of a glutaric acid, and should therefore be expected to yield an anhydride fairly readily, unless the structure is that of a trans-acid, an assumption which appears to be excluded by the fact that d-camphoric acid from which it is easily obtained is a cis-acid, the corresponding trans-acid being represented by iso-camphoric acid. (e) The Formation of Camphor in large Amount by distilling the Barium Salt of Homocamphoric Acid (compare B. 2. ¢.). As pointed out by Bredt and Rosenburg,' Wislicenus? and Perkin and Crossley,® the formation of considerable quantities of ketones by distillation of the barium or calcium salts of dibasic acids, in the simple manner here observed, is met with only amongst the derivatives of adipic, pimetic, and suberic acids, and never amongst those of glutaric acid, so that here again the Perkin-Bouveault formula appears inadmissible. (d) The extraordinary Readiness with which p-Cymene and its Derivatives are obtained from Camphor. This change, a knowledge of which assisted Bredt in devising his formula, is very readily understood by means of it : en C.CHMe, Seat ates CH. | CH, CH. (OR CMe; | > | | CHsg.... | iis CO CH CH = / 24 CMe OMe Camphor. p-Cymene. (e) The ready Formation of the Lactonic Acid, Camphanie Acid from Bromocam- phoric Acid or its Anhydride, and of its Ethyl Ester by heating Diethyl Bromocamphorate. When w-bromocamphoric acid or its anhydride (obtained by the direct bromination of camphoric acid) is treated with water, alkalis, or sodium acetate dissolved in glacial acetic acid, it yields camphanic acid, a very stable lactonic acid. The great stability of the lactone ring of camphanic acid excludes the idea that it is of the nature of a -lactone, so that it must be a y-lactone. w-Bromocamphoric acid would therefore appear to be a y-bromo-acid, and, in accordance with Volhardt’s rule, it should also 1 Annalen, 289, 13. b 2 Thid., 275,309. % Trans. Chem, Soc., 78, 6. 320 REPORT-——1 900. be an a-bromo-acid. These facts are readily explained by Bredt’s, but not by the Perkin-Bouveault formula, as in accordance with our ordinary views the latter formula would make a-bromocamphoric acid a B- and not a y-bromo-acid. CBr . COOH CH,—CBr . COOH | I | | CH, CMe, CH, CMe. COOH | / Pad CH, CMe, Ee CMe . COOH Breat. Perkin-Bouveault. That the position of the bromine atom in the nucleus represents the posi- tion of attachment of the lactonic oxygen atom is shown by (1) the fact that diethylbromocamphorate when heated yields ethyl bromide and ethyl camphanate sosccenee CBr ae onseuaee C0 ; > : | + EtBr ene y.¢ MOO Aub ee) (2) that camphanic acid on treatment with phosphorus pentachloride (or pentabromide) regenerates ordinary chloro- (or bromo-)camphoric chloride (or bromide) ; a fact of which the author has convinced himself. ap ow eres Cong eit ee baa be ls = + POCI, Rise c.co ae, OLC1 That camphanic acid does not contain the grouping rec CH .O é | Pees. C—CO receives support in the fact that it is obtained by oxidising camphoric acid with chromic acid, and in accordance with the researches of Fittig such an oxidation occurs only at the tertiary carbon atoms, (f) The Formation of Balbiano’s Acid and Ovalie Acid in approximately equivalent Amount by the Oxidation of Camphorie Acid (compare E. 1. ).). The formation of an acid having the constitution given by Balbiano for the product .C,H,,O, is readily interpreted by the use of Bredt’s formula as follows :— 7 CH . COOH’ CH COOH ie: COOH | tr | CMe > | +O CMe OE can tect COOH ae CH, : CMe . COOH ">€Me . COOH Using the Perkin-Bouveault formula, the course of the change becomes very difficult to understand, and must necessitate the assumption that o a ON THE CONSTITUTION OF CAMPHOR. 321 —-CH,— group ina hydrocarbon ring may be converted into —CH(OH)— or —CO— or others equally improbable : CH, ——CH, CH . COOH | A CMe, > O CMe, | SI] CMe(COOH).CH .COOH CMe. COOH+COOH . COOH. (g) The Formation of Camphorphorone (compare E. 5.). The formation of a ketone having the constitution of camphor- phorone from calcium camphorate receives instant explanation by means of Bredt’s formula, as follows : CH.CO. 0 mK | a: CHa. << 2 ff ~ (ie CMe, fo% > CREE! GOL CaCo, CH, | A ee wh me COMe/ CO. O CM whilst if the Perkin-Bouveault formula is used the change must be represented as the result of the following complicated series of reactions : ! _CMe, . CMe.CO: O OMe, CHMe.CO..... ai 2 oe Ye | CH, : Ca =s) JOE H ye Der 4 \cu,—cHt “CO. 0 \cH,—CH mee CMe, CO.CHMe VA waa -CH, a necessity which leaves the probabilities greatly in favour of the first depicted. (h) The Formation of Camphononic Acid and Oxalie Acid from Dihydrohomo- Camphoric Acid (compare E. 3.). As has already been mentioned (loc. cit.) this change appears capable of only two simple explanations, one of those being the assumption that dihydrohomocamphoric acid has the formula which would be attributed to it were Bredt’s formula the correct one, namely _C=CH.COOH CH, | OMe, CH, \date.coon 1 Compare Bouveault, Bull. Soc. Chim. (iii.], 19, 462. 1900, Y 322 REPORT—1900. and not only is this the case, but the derived formula of camphononic acid is in complete accordance with the disinclination of the carbonyl group to form additive complexes (compare E. 2. a. ii.). The Perkin-Bouveault formula is, in this instance also, inapplicable, unless, as usual, a special assumption is made to meet the case. Thus, no doubt, it might be held that an intermediate compound having the formula igo s CO.COOH CH, \ ome,.Me.CooH is produced which breaks up into oxalic acid and camphononic acid by hydrolysis. Such an assumption, however, has nothing to recommend it. 2. THE PERKIN-Bovuveau.Lt Formu.a. if aera tah CH, CH. CH= Ge This formula offers simple explanations of the following points, for which the Bredt formula appears inadequate. (a) The Formation of Isolauronolie Acid from Camphoric Acid in several Ways. The formation of this acid by elimination of the allo-carboxyl group from camphoric acid is readily explained by the use of this formula : bee . CMe. COOH CMe, . CMe CH, + ne | + 2H +O, \cH,—CH . COOH Non,—¢ . COOH The change represents the formation of acids having the formula proved by Blanc to be correct for isolauronolic acid, and of course affects both asymmetric carbon atoms, thus explaining the complete disappearance of optical activity during their formation. (b) The formation and properties of B-campholenie acid. In explaining the production of a campholenonitrile from camphor- oxime, as represented by the Perkin-Bouveault formula, we are led in a most simple manner to the formula, which, as was pointed out by Bou- veault, is the most suitable one for 8-campholenonitrile which can be devised : mes _CMe.C: NOH CMe,—CMe CH, | 4 CH, | \cu,—cH—cH, \CH,— Ge Qe eee ON THE CONSTITUTION OF CAMPHOR. jee whilst it is clear that the use of Bredt’s formula would require the assumption that isomeric change of a somewhat obscure character had taken place. If this formula be the correct one, /3-campholenic acid, as might be surmised from a consideration of its inactivity and its oxidation products, is in reality homoisolauronolic acid. (c) The Formation and Properties of Hydroxydihydrolauronohe Acid. By the use of the Perkin-Bouveault formula the action of hypobromite on a-camphoramic acid would be represented CMe, .CMe. COOH _fMe, CMe. COOH CH, ae CH, | S CH,—CH . CONH, CH,—CH .NH, and the formula so deduced for the amino-acid represents a /(-amino acid, which should naturally afford a 3-hydroxy acid on treatment with nitrous acid. Since a (-hydroxy acid would yield a 6-ketonic acid on oxidation, the elimination of carbon dioxide and production of a ketone are easy to understand (compare E, 2. ¢. i.). A consideration of the whole of the preceding facts leads to the con- clusion that it is impossible to reconcile the results obtained in the various departments of camphor chemistry without having recourse to the assumption that, at certain points, intramolecular change takes place, involving new arrangements of the carbon atoms. Thus, to take only one example, the structure of the a- and /-campholenic acids cannot be re- presented by two formule which differ only in the position of the double binding as Tiemann suggested, for one acid clearly contains the grouping Ca : OMe . CMe, CH C.c -and the other the complex :C. CMe, .CH,.C.@. The formation of isocamphoronic acid on the one hand and of iso- lauronolic acid on the other is also incapable of explanation on any other grounds than that of intramolecular change ; and it would appear advis- able, therefore, to consider the whole of the evidence from a broad stand- point, and, having decided which is the more probable view, to endeavour to ascertain the points at which difficulties first arise, and only then to seek for explanations. It is obvious that it would be altogether ill-advised to adopt the usual course and to take any one derivative, however well established its structure may be, and however simple its apparent mode of derivation, and to use this as the basis on which to form our conclu- sions, employing a forced explanation for each inconvenient fact in turn. Looking at the question, first, from a general point of view, without regard to ultimate structure, it must be obvious that the probabilities are greatly in favour of the view that the ketone ring in camphor is a penta- methylene nucleus, as witness the readiness with which the substance is obtained from homocamphoric acid. Moreover the properties of homo- camphoric acid itself approach more nearly those of an adipic than glutaric acid, since under no circumstances does it appear to yield an anhydride. Y2 324, REPORT—1900. The general properties of camphoric acid are those of a glutaric acid, as its bromo-derivative at once yields a stable lactone ; a behaviour altogether inconsistent with the view that it is an a-brominated succinic acid. The supporters of the succinic acid formula for camphoric acid have raised the contention that bromocamphoric acid is a /3-brominated acid containing the complex --CHBr . CH . COOH and in support of this advance the fact that its anhydride on treatment with water or sodium carbonate loses carbon dioxide and hydrogen bromide, yielding a small quantity of lauronolic acid, a behaviour certainly in accordance with the view that it is a (-bromo-acid. The necessity for such an assumption, however, is in itself clearly an argument against the succinic formula, since the bromination of a saturated acid in the /-posi- tion is unknown. Moreover on this assumption bromocamphoric anhy- dride itself still contains an a-hydrogen atom, and should be capable of further bromination, a surmise altogether at variance with the facts. It is much more probable that the formation of lauronolic acid is due to an idiosyncrasy of the compounds involved, and little or nothing is known of the behaviour of cycloid u-bromo-acids in this respect. It obviously cannot be urged that the formation of lauronolic acid is evidence in favour of the presence of the complex ; CH, . CBr. COOH C . CCOOH Cc as such an acid would afford an isomer of lauronolic acid, possibly campho- lytic or isolauronolic, and containing the complex CH, . C. COOH I c.c Cc and, in fact, that it does not do so isi in ‘tself evidence against the succinic formula for camphoric acid. It may therefore be stated that the general properties of camphor and camphoric acid are of a kind which should be expected were Bredt’s formula the correct one. Comparing now the weight of evidence in favour of the two formule as elicited by examination of the exact structure of the degradation pro- ducts of camphor, Bredt’s formula is seen to be favoured in a high degree, and only the structure of isolauronolic acid and of /3-campholenic acid (probably, as has been pointed out, homoisolauronolic acid) appears to militate strongly against its acceptance. It is especially significant, moreover, that the j-campholenic derivatives are produced, probably in all cases, as secondary products from the a-derivatives, and the behaviour an ee ee ee ON THE CONSTITUTION OF CAMPHOR. 325 of the latter is in strict accordance with the requirements of Bredt’s formula. It is certainly difficult to understand the behaviour of hydroxydihy- drolauronolic acid, but until more is known of this acid it is possible to attach undue significance to the point. Tt is impossible to overlook the fact that the Bredt formula affords an excellent explanation of the behaviour of a very large number of camphor derivatives, and is, in fact, the only formula which will do so, and that the same words apply to the Perkin-Bouveault formula when the remainder, namely, isolauronolic acid and 3-campholenic acid, are referred to. Since the constitutions of the two different series of compounds appear to have been established with such a high degree of probability, one is led to the belief that there may, after all, be some close connection between the two series which has escaped observation owing to the occurrence of unsuspected isomeric change—a phenomenon which it is generally admitted must be the cause of the present divergence of opinion on the matter. It does not require much consideration to observe that if this explana- tion be correct the isomeric change must occur during the formation of isolauronolic acid, and in the transformation of the a- to the /-cam- pholenic derivatives, so that a comparison of the probable formule of these substances before and after the change should allow us to gather if there is any simple connection between them. __-CH.COOH = —C.COOH CH, | CH, || | CMe, | CMe CH, | CH, | ~~C.COOH C Me Me, Camphoric Acid. Tsolauronolic Acid. eu: My O11 2 eR AS 8 2 I CH wile p OH, | CMe, | | CMe | CH. | . COOH CH, |» COOH een iT - Se XC Me Me, a-Campholenic Acid. 8-Campholenic Acid. It is fairly clear that the apparent change consists in the migration of a methyl group to an adjacent carbon atom in both cases. The alteration of the position of the double binding in the campholenic derivatives is of little consequence, as the change is probably preceded by the formation of a lactone in some cases, of an imide in others, and these derivatives contain no double binding. Possibly the change in the former case may be represented -CH ere: o~ oi | ‘cH, Cn.. |) o Sen, OE, |) Ee j|_ CMe, | 3 CMe, | > | CMe CH | COOH CHa. CO CH, | COOH .c e100 Ke Me Me Me, 326 REPORT—1900. The change is not unlike that involved in the transformation of pinacone into pinacoline : CMe,.0H CMe, | | CMe, = CMe+H,O | | OH O or of pinacolyl alcohol into tetramethylethylene : CMe, CMe, | > | +H,O CHMe.OH CMe, changes apparently characteristic of complexes which contain several adjacent methyl groups. It is well known, moreover, that in the forma- tion of benzenoid derivatives from hexamethylene compounds the methyl groups usually appear to move to adjacent carbon atoms ; as, for example, in the change of isolauronic acid into paraxylic acid CMe, CMe me i CH, CO > CH CMe | | CH, CH CH CH iS at 6 ig ~C.COOH C.COOH as well as in numerous similar instances investigated by Baeyer. It may be urged that the conditions under which isolauronolic acid is produced from camphor are not such as would be expected to produce deep-seated isomeric change, but such a contention is altogether insufficient to seriously militate against the great probability that it does actually occur in this instance. It is easy to cite evidence that isomeric changes of very unexpected character do occur under conditions which would at first sight appear to be insufficient to produce them, such as, for example, the change of a-dibromocamphor into bromocamphorenic acid when warmed with an alcoholic solution of silver nitrate on the water bath, which certainly involves the absorption of a carbon atom into a ring somewhat in this manner : CH. CBr z zl a! eA N CH, | CBr, e CH | CMe, Gieeit | Bt | Ha@e= wet CMe, CH,!| co | | ie eee 4 M ==) ‘COOH e Me and the change of pinacone into pinacoline does not involve any violent action such as is usually associated with the production of benzene derivatives from cyclomethylene compounds. 1 Lapworth, Zrans. Chem.'Soc., 75, 1138. ON THE CONSTITUTION OF CAMPHOR. 327 Finally, whilst it appears unlikely that any simpler explanation than that here suggested can be offered, the question clearly awaits further investigation ; but it seems unlikely that the correct solution will be obtained until the attention of investigators is directed to the examina- tion of the points at which isomeric change probably occurs, since the discovery of isolated facts in favour of either formula can only add to the number of those already known, and can scarcely be regarded as conclusive whilst strong evidence in favour of the other formula can be brought forward. Addendum (November 3, 1900). The curious properties of lauronolic acid (2. a. ii.) may possibly be accounted for by the occurrence of a change of structure similar to that above suggested in the cases of /3-campholenic acid and isolauronolic acid, and by applying a similar rule, the change might be represented CMe . COOH CMe. COOH CH, | qr | CMe, ; CMe CH, CH, | aod a CH .COOH CMe Camphoric Acid. Lauronolic Acid, and the formula thus arrived at is in complete accordance with all that is at present known of the properties of the acid, and on oxidation the acid would be converted into a compound ‘CMe . COOH | CH, CO. Me CH, CO. Me which is, at the same time, a /-ketonic acid and a 1 :5-diketone, and would therefore lose carbon dioxide readily, and suffer condensation in alkaline solution, yielding a 3y-unsaturated ketone CHMe CHMe Yor » AUitans) 7% : } | # » recurvans. f oy * * Kee KR * 336 REPORT—1900. Distribution of Pleistocene Plants—continued. 2 | =m Don Valle S aE)#2/ 3 (2S lealeFls|al.| |#lg(zolcle —— Ol! ao (|ee2/BS\e8/5/ Al. 218) S| a|2| 8 2(e) 88!) 3 lea] ®S igo [|e s/o] Sli el al sis Biel 2S) £ SS] e3)/F2 |s|=/ 8/8] 26] 8] sl als Cla | IF |S" |e) sls] sal sles] 8 3 2 [ae lalalS| als ra LS ad ee ein vO ETC: A | Hypnum revolvens . a | ot) Spee : * Juniperus virginiana. | bail ha = _ Larix americana : cE poeta eam * * ,, cChurchbridgensis . er | | Licmophora sp. ee Lycopodium sp... : a Maclura aurantiaca . Ra i a! | Menyanthes trifoliata- . | * | Navicula lata . : * | | | Oryzopsis asperifolia | | * | Oxycoccus palustris ; | * | Picea alba A , Ra * | 3 nigra ‘ e * | | } * | |e) ] ae | eT * | » %Sp.. 7 . . | « | | | Pinus strobus . : ; | Tel ca esa Platanus occidentalis * = Populus balsamifera 5 | ih fala s grandidentata . le ci * * Potamogeton pectinatus . 4 zs perfoliatus . | ey * | * 5 pusillus . | | Balhae + rutilans | *| * 7 natans 4 * Potentilla anserina . 5 | Erle Prunus sp. : . : eral eamt | Quercus obtusiloba . : by | | 3 | alba?) ® : pall ect a rubra : 5 |* ae ba % tinctoria ; “ ss > oblongifolia j * » macrocarpa eye Ned 2 acuminata a | Robinia pseudacacia se | Salix sp. . iY os = Taxus canadensis pa [ea | * Thuya occidentalis . < Fadler) Tilia americana : ; alah tary Typha latifolia : : | i Ulmus americana Sia » racemosa ‘ 3 | Vaccinium uliginosum . | = Vallisneria spiralis... ra | cai Zostera marina : : | - ' Totals : pyle lier 2 1 | 6 1 |17/34/27/3 1/5 14/24 14/7 The most easterly of the localities in the related deposits is Montreal. The majority of the specimens recovered at this point represent drift material brought down by tributary rivers, but the great abundance of Zostera marina and the occurrence of Algae show that some of the plants at least were deposited in place. The matrix is a blue clay. Seven species in all have been recovered from this locality, and they are.all CANADIAN PLEISTOCENE FLORA AND FAUNA. 307 identical with species now common in the same district—except, of course Z4ostera—thus indicating similar climatic conditions. At Green’s Creek, near Ottawa, and at Besserer’s Wharf, a few miles below on the Ottawa River, numerous plant remains are found enclosed in clay nodules, but their very fragmentary character often renders their determination most unsatisfactory. These two localities, although sepa- rately treated, are in reality one and the same, since the deposit at each place is of the same nature, and was undoubtedly laid down at the same time, and they have proved to be among the richest in plant remains of all the localities studied—no less than twenty-eight species having been recovered from the clay nodules. An analysis of this flora shows 39°71 per cent. of the plants to be wholly aquatic, and therefore deposited in place. 35°71 per cent. are land plants, drifted in by tributary rivers, and 28°07 per cent. represent semi-aquatics and marsh plants from adjacent land areas. The vegetation, as a whole, is identical with that now found in the same region, from which we may infer similar climatic conditions. At Scarborough Heights, near Toronto, the flora is rather remarkable for the complete absence of aquatic types, showing the drift character of the entire deposit. Fourteen species in all have been found there, and of these six are trees, while the remaining eight embrace mosses, equiseta, and herbaceous or half-shrubby plants. The vegetation as a whole is of a decidedly more boreal type than that now flourishing in the same region, and, if anything, somewhat more northern than that which is to be found in the deposits at Green’s Creek and Montreal. This points to a climate equivalent to that of northern Quebec and Labrador, as we know it to-day, and somewhat colder than the climate at Green’s Creek and Montreal during Pleistocene time. In the Don Valley no less than eight separate localities have been examined. Some of them, as at Simpson’s, proved practically barren of results so far as plant remains were concerned, owing to the uncontrollable influx of water. Others again, as at Taylor's Brickyard and the Don River, proved to be exceptionally rich in material, and afforded some of the most valuable results obtained. Within this area no less that thirty-eight species have been recovered, and they point conclusively to the existence of climatic conditions differing materially from those which now prevail, and of a character more nearly allied to that of the middle United States of to-day. The Erie Clays at Hamilton, Ontario, have afforded only one example ‘of plant life, and this does not materially aid us in any conclusions relative to climatic conditions, since it is a type having a somewhat wide range within the warmer zone, represented by the more southern types of the Pleistocene flora, Only one species appears to have disappeared in Pleistocene time. Acer pleistocenicum, which was abundant in the region of the Don, bears no well-defined resemblance to existing species. With this one exception, it is a noteworthy fact that all the plants of the Pleistocene flora were such as are now represented in the same localities, or, in the case of the Don Valley, by plants which find the northern limits of their distribution at or near that region, and the somewhat unequal distribution thus indicated at once suggests definite climatic changes during Pleistocene time, as represented by the northern and southern migration of particular types of plants. This has already been referred to in previous reports and publi cations, but it may be repeated at this time that the definite and abundant occurrence of Maclura aurantiaca, Juniperus virginiana, Quercus obtusi- 1900. Zz 338 REPORT—1900, loba, Quercus oblongifolia, Asimina triloba, Chamaecyparis sphaeroidea, and Fraxinus quadrangulata points without question to the prevalence of a much warmer climate than now prevails, while, on the other hand, the equally abundant occurrence of boreal types at Scarborough points to the existence of a colder climate at the time these deposits were laid down. It is therefore clear that in the region of Toronto during Pleisto- cene time there were at least two distinct periods, characterised, on the one hand, by a climate equivalent to that of the middle United States at the present day, and, on the other hand, a climate equivalent to that of northern Quebec and Labrador. According to stratigraphical evidence obtained by Professor Coleman, these changes followed the recession of the ice sheet in the order given, from which we are to conclude that the climate of the Don Valley is now intermediate between that of the first and second periods, approaching the former. On the other hand, again, the flora of Green’s Creek and Besserer’s, as also that of Montreal, is practically identical with that now existing in the same localities. It thus represents a climate colder than that of the Don period, but somewhat warmer than that of the Scarborough period, but present evidence does not enable us to ascertain if these deposits were laid down before or after the Scarborough deposits. The following sum- mary will probably assist in conveying a clearer idea of the distinctive differences in the vegetation of these three periods. Don Period, Warm Climate Scarborough Period, Cold Climate Green’s Creek Period, Mild Climate Se Abies balsamea “ s Acer pleistocenicum . . Acer saccharinum Acer spicatum : ¢ : : Algae sp. . ‘ i : 2 : : 5 : | Alnus sp. . , ° . ‘ : F ; : Asimina triloba . f c . Betula lutea Brasena peltata . Bromus ciliatus . 5 4 5 Carex aquatilis . 5 : . » magellanica » reticulata Cara alba . ; 5 i Chamaecyparis sphaeroidea Crataegus punc'ata Cyperaceae sp. . . Drosera rotundifolia . o Elodea canadensis . 5 : Encyonema prostratum Hquisetum limosum Ay scirpoides . " = : A sylvaticum Eriocaulon sp. Fontinalis sp. . A : : : ( A : | * * * * * %¥ FRR * — Summary—continued. CANADIAN PLEISTOCENE FLORA AND FAUNA. Fucus digitatus . Fraxinus quadrargulata Af sambucifolia . americana . Festuca ovina . ; Gaylussacia resinosa . Gramineae sp. Hypnum commutatum FS fluitans ‘ * revolvens . ” Sp. 5 Juniperus virginiana : Larix americana Lycopodium sp. . Maclura aurantiaca . Oryzopsis asperifolia . Oxycoccus palustris Picea alba . : : » nigra . s . ISDS auh- rliys : Pinus strobus_ . - Platanus occidentalis . Populus balsamifera » grandidentata Potamogeton pectinatus PH perfoliatus ne pusillus a rutilans +8 natans . Potentilla anserina . Prunus sp. . ’ . Quercus obtusiloba . » alba (2). os rubra. . “3 tinctoria : “ oblongifolia . » macrocarpa . acuminata . Robinia pseudacacia . Salix sp. . ; Taxus canadensis Thuya occidentalis Tilia americana . c Typha latifolia . Ulmus americana » racemosa Vaccinium uliginosum Vallisneria spiralis . Zostera marina . Totals : F : _— —_ we 1 o By n oO ~ os 34 Ae oq 2.5 PE eS) cos Ay BS aq ac oa on ° (aye 2c e eo i) nm % ' ‘ : ‘ x ' * * ‘ * 3%} ~ * * : * * * % 2 * s . . * . . . . . . * * . F * ‘ . 5 % % * . 4 é R . ye * % * * * | . * ! a } - F | * / ; * | * * * } | . | | * | | N | * i * * * a | i SE c eT 38 14 359 Period, ate cc Green's Creel: Mild Clim * % % * 3840 REPORT—1900, Exploration of Irish Caves.—Interim Report of the Committee, con- sisting of Dr. R. F. ScHarEF (Chairman), Mr. R. Luoyp PRAEGER (Secretary), Mr. G. Correy, Professor GRENVILLE COLE, Professor D. J. Cunnincaam, Mr. A. McHenry, and Mr. R. J. Ussuer. Owine to various circumstances, especially illness of some of the members, the Committee were unable during the past year to commence the exploration of the caves in the west of Ireland. These caves promise to yield satisfactory results, and the Committee recommend that they should be reappointed, with a renewed grant of 20/. Life-zones in the British Carboniferous Rocks.—Report of the Com- mittee, consisting of Mr. J. E. Marr (Ohairman), Dr. WHEELTON Hinp (Secretary), Mr. F. A. Batuer, Mr. G. C. Crick, Mr. A. H. Foorp, Mr. H. Fox, Mr. E. J. Garwoop, Dr. G. J. HInbE, Professor P. I. Kenpaui, Mr. J. W. Kirxsy, Mr. R. Kipston, Mr. G. W. Lampiueu, Professor G. A. LEzour, the late My. G. H. Morton, Mr. B. N. Peacu, Mr. A. Srrawan, and Dr. H. Woop- WARD. (Drawn up by the Secretary.) Ir is to be regretted that since the meeting at Dover no individual reports have been received from members of the Committee, and that the lamellibranchs collected at Eccup only have been examined and named. The Secretary suggests that the most important points to settle are the faunas of (a) the beds which occur between the Millstone Grits and the Massif of Limestone in the South Pennine area, and (b) the fauna which occur in the shales between the Millstone Grits and the upper beds Limestone in the North Pennine area, This would settle at once the correlation of Pendleside Limestone and its equivalent in the Yoredale series of Wensleydale. Mr. B. N. Peach has been at work on the faunas of the Calciferous Sandstone series of Fife, and it is hoped that a full detailed report will be received next year. It would be well if a grant could be made to employ a collector to work the shales of Pendle Hill, and if possible in Swale and Teesdale. The Committee regret to report the loss, by death, of two of their number—the late Professor Alleyne Nicholson and G. H. Morton. Mr. Morton was an ardent worker at Carboniferous geology, and had specially confined his attention to North Wales ; a full list of Carboni- ferous fossils from this district was to have been prepared by him this year. APPENDIX. Interim Report by Dr. WaEEtton Hinp. In the ‘ Geological Magazine,’ 1898, Dec. IV. vol. v. pp. 61-69, I gave a brief sketch of what was known of the Life Zones of the Carboniferous deposits of Europe, and ‘at p. 68 showed the following table, which represented the main results of my investigations up te that date. ee LIFE*ZONES IN THE BRITISH CARBONIFEROUS ROCKS, 34] 1. Zone of Anthra- comya Phillipsii 2. Zone of Naia- dites modiolaris and Anthra- comya modiolaris 3. Zoneof Aviculo- pecten papyra- ceus, Gastrio- ceras carbo- narium, Posido- niella levis, and P., minor 4. Zone of Pro- ductus giganteus and Productus cora 5. Zoneof Modiola Macadamii ENGLAND Upper Coal-mea- sures of Lanca- shire, Yorkshire, Staffordshire, Bristol, including the Spirorbis Limestones Middle Coal-mea- sures universally Ganister Series Millstone Grit Shales below the Millstone Grit universally The Carboniferous | Limestone of Derbyshire Themeasuresfrom * the Great Scar to the Main Lime- stone, N. York- shire The Carbonaceous Division of Northumberland Carboniferous Limestone of Wales and the | Mendips The Lower Lime- stone Shales of the Mendips and South Wales, | with several fossils common | to the Old Red Sandstone Series andjthe Carboni- ferous ScoTLAND The Red Beds of Fifeshire The Coal-measures of Fifeshire 2? Wanting NOoTE.—Aviculo- | pecten papyraceus is said to be found | some distance | above the Ell Coal in the Wishaw dis- | trict, Lanarkshire The Carboniferous Limestone Series of Upper Lower Scotland | Middle |! The Calciferous Sandstone Series, with Schizodus Pentlandicus and Sanguinolites Ab- densis in Fifeshire, and a fauna very different from the English and Irish equivalents. Mr. Kirkby states that Productus cora is contained in the upper 500 feet of these beds TRELAND ? Wanting Coal-measures Castlecomer, Lein- ster Coalfield Limerick The Upper Lime- stone The Calp | Coal-measures of | Foynes island, co. The Lower Lime- , stone The Coomhola and Moyola beds, forming a pas- sage from the Old Red to the Carboniferous, | and containing | certain fossils common to both Series 1-3 constitute what I consider to be the ‘ Upper Carboniferous,’ and series 4 and 5 the ‘ Lower Carboniferous,’ of my paper on the Yore- dale Series. ! } Geol. Mag., April and May 1897. 842 REPORT—1900. Further work has convinced me of the correctness of these main zonal divisions, and observations on the subdivision of the lower part of Zone 3 are approaching to some degree of exactness. With regard to the subdivision of group 4 I am in hopes that Edmondia sulcata and Allorisma monensis may be found to indicate an horizon in Zone 4; but as yet these fossils have not been found in the South Pennine area. I consider interesting the discovery of Cypricardella rectangularis, C. Anna, Nuculania attenwata, Ctenodonta sinuwosa, and other shells in shale above the Underset Limestone, nine standards near Kirkby Stephen, and a very similar fauna at the same horizon on Wild Boar Fell. C. rectangularis with an identical fauna is found to be common in the Lower Limestone. Series of Strathavon and the Upper Limestone series of Orchard near Glasgow :—a full description of the section and position of the fossiliferous beds was published at p. 358 in Part IV. of my mono- graph on ‘ British Carboniferous Lamellibranchs,’ 1899. Registration of Type Specimens of British Fossils—Report of the Committee, consisting of Dr. H. Woopwarb (Chairman), Rev. G. I. Wuiwporne, Mr. R. Kinston, Professor H. G. Sretey, Mr. H. Woops, and Dr. A. 8S. Woopwarp (Secretary). DurinG the past year the Committee have received a list of type-fossils in the Norwich Museum, compiled by Mr. Frank Leney. The Museum of Practical Geology, Jermyn Street, has published a first instalment of a list of the type-fossils contained in its collections (‘Type Specimens of Eocene and Oligocene Fossils,’ by H. A. Allen, appended to the Annual Report of the Geological Survey of Great Britain for 1899). Ossiferous Caves at Uphill.—Report of the Committee, consisting of Professor Ltoyp Moraan (Chairman), H. Bouton (Secretary), Professor W. Boyp Dawkrns, Professor 8. H. Rrynoups, and E. T. NEwTon. THE excavation work of last year was continued until the approach of winter, by which time the lower caves were worked out, nothing new being added to the discoveries reported to the Association at the Dover meeting. The caves were found to lie along the bedding planes of the limestone, and had clearly formed part of a subterranean drainage system, the material in them being derived presumably from caves on higher levels. Systematic search has been made for caves of habitation higher up the hill, but hitherto with no success. Work has therefore been arrested. It is hoped to secure a visit and report from Professor Boyd Dawkins before further exploratory work is commenced. The Committee have, up to the present, incurred an expenditure of 451. 14s. 2d., 307. of which has been met by the grant made in 1898 at Bristol. : ON OSSIFEROUS CAVES AT UPHILL. 843 The Committee do not feel justified in requesting a grant for future work, but they seek reappointment with a grant of 10/. (the sum not claimed last year) to cover expenses already incurred. It is their inten- tion to further examine the ground as quarrying proceeds, Erratic Blocks of the British Isles—Report of the Committee, consisting of Professor EH. Hutu (Chairman), Mr. P. F. KENDALL (Secretary), Professor T. G. Bonney, Mr. C. E. Dr Rance, Professor W. J, Sotias, Mr. R. H. Trppeman, Rev. 8. N. Harrison, Mr. J. Horne, Mr. F. M. Burron, Mr. J. Lomas, Mr. A. R. Dwerry- HOUSE, Mr. J. W. StaTHer, and Mr. W.'T. TUCKER. (Drawn up by the Secretary.) THE records of boulders observed during the past year have been derived principally from Yorkshire, thanks to the activity of the local organisation which has for so many years occupied itself with the investigation ; but the Committee is hopeful that other areas may be subjected to an equally stringent examination. Work had been commenced in the county of Durham under the stimulus of an enthusiastic worker, the late Dr. Taylor Manson, of Darlington ; and though the Committee has to deplore his removal by death before any definite results were obtained, it is expected that the movement which he initiated will be productive of valuable contributions to the knowledge of a rich and scarcely touched field. An important advance affecting much of the eastern side of England, and particularly the counties of Northumberland, Durham, and Yorkshire, is marked by a visit paid to the Cheviot country by the Yorkshire Geological and Polytechnic Society at the instigation of members of the Boulder Committee of the county. The object of this excursion was to study the igneous rocks of the Cheviots, with a view to the recognition of any erratics of similar types, and to determine how far the ascription to this source was correct of a series of porphyrites which form a very considerable proportion of the far travelled boulders of Yorkshire. It was found that an even larger number of types of erratics could be traced to the Cheviots than had been anticipated. A large number of specimens were collected, and the Secretary of this Committee will be glad to furnish sets of examples to any geologists willing to assist in the investigation of the boulders of the East of England. A very important further result was obtained from the excursion. In the report for 1897 reference was made to the identification by Professor Brégger of the Sparagmite Sandstone of Scandinavia in a series of Yorkshire erratics submitted tohim. In subsequent reports occurrences of a similar rock in various localities in Yorkshire have been mentioned, but some doubt has been felt regarding the identification, and all such records have been given with a ‘?’. This caution has been justified by the discovery that a sandstone precisely resembling some of the erratics of Yorkshire constitutes a signi- ficant proportion of the stones in the ‘foreign’ drift of the country about Wooler and Ingram in the Cheviots. It is referred to in the Geological Survey Memoirs of the district under the name of ‘ Greywacke Sandstone,’ and its source is given as in the Silurian area of the Tweed Valley. 344 REPORT—1900. A further extension of the known distributions of Shap Granite blocks is furnished by the example reported from Gainsborough, and the interesting Riebeckite-Eurite of Ailsa Craig has been recorded from Delamere, in the very heart of Cheshire. CHESHIRE. Reported by Mr. J. Lomas, A.R.C.S., F.GS. Birkenhead.—In cutting a sewer in Woodchurch Road, near Half- way House, Boulder Clay about 25 feet thick ; boulder of diabase 3 feet diameter. Delamere Forest.—Great spreads of sands and gravels. Group near station contains Lake District andesites, Eskdale and Criffel granites, Riebeckite- Eurite from Ailsa Craig. Flints. SHROPSHIRE. Church Stretton, Watling Street-— Criffel granite, 1 foot diameter. Eskdale granite. Gravel Pit under Hazler Coppice, 800 ft. O.D.— Eskdale granite. Buttermere granophyre. Permian sandstone from north. Comley— Eskdale granite. All Stretton— Triassic sandstone. NortH WaALEs. Llandrillo, near Bala.—Section of Drift nearly 100 feet high, cut by stream near Cadwst, full of large boulders, many over 6 feet in diameter. Nearly all ash and greenstone ; exposures of similar rocks a little distance southwards. Greenstones increase in number on following up the stream Nant-cwm- Dywyll as far as the firwood. To the east the ground is strewn with large clusters of greenstone boulders. On the summit of the rising ground the rock is found in situ, and shows roches moutonnées and striations from the south. No greenstone boulders are found in the low ground south of the outcrop. Old Slate Quarry S. of Carnedd-y-ci—Many quartzite and green- stone bouiders of large size resemble rocks found in sitw on Cader Berwyn, immediately to the south. Glyn Ceiriog.—Group of boulders in field just above cottage called Pant. Some over 5 feet in diameter consist of Welsh felsites and Denbigh grits. The grits, which are fossiliferous and beautifully striated, occur in situ to the north and west. On the hills to the south of Glyn Ceiriog, Denbigh grits occur as boulders up to 1,250 feet. YORKSHIRE. Reported by the Yorkshire Boulder Committee (Mr J. H. Howarru, L'.GLS., Secretary). By Mr. H. H. Corsert, I2.2.C.S., of Doncaster, Cushworth. 1 Dolerite. ON ERRATIC BLOCKS OF THE BRITISH ISLES, 345 By Mr. P. F. KenpAat. Barugh Hill, near Robin Hood’s Bay.—Many boulders of porphyrite and two examples of a very coarse pisolite containing Verinea. Thirley, near Cloughton.—Great gravel-mounds here are strewn with large blocks, all of Jurassic sandstone, in numbers greatly exceeding what may be seen elsewhere in Yorkshire. Whithy—Cliffs to West of Town.—A. bed of gravel lying between two beds of Boulder Clay, the lower dark grey in colour, the upper reddish, contains the following rocks roughly in order of prevalence : Jurassic and other sandstones, Magnesian Limestone, Carboniferous Limestone, basalt, conglomerate (? Sparagmite), Greywacke sandstone (or ? Sparagmite), jasper, Alum Shale (a large block), Gryphza incurva, ball of red Boulder Clay. Wheatcroft, near Scarborough.—In corner of second field W. of road, Shap granite 2 feet long. Seamer.—The gravels between Seamer Quarries and Waydale House contain very high proportion of basalts. Seamer Beacon.—The tower here is built of rough blocks, mainly of Jurassic sandstone, but with large numbers of basalt or dolerite and some Cheviot porphyrite. Yedmondale.—A pit shows gravel consisting of local stones with many Cheviot porphyrites, some Greywacke, jasper, and a few granite pebbles. Fragmentary marine shells are also found. Hutton Bushel.—In gravel pit on 200 feet contour. Many local stones with Cheviot porphyrites, Magnesian Limestone (Roker type), Kimeridge clay, gneiss, granite. Reported by Boulder Committee of the Hull Geological Society. By Mr. Tuos. Suepparn, /.G.S. Burstwick Gravel Pit, Holderness— Shap granite, 8 in. by 6 in. Rhomb-porphyry, 4 in. by 4 in. By Mr. J. W. Statuer, 2.G.S. Atwick.—At the foot of cliffs — Shap granite, 18 in. by 20 in. by 14 in. Augite-syenite (Laurvikite) 18 in. by 18 in. by 12 in. Rhomb-porphyry, several pebbles. Fordon on the Wolds.—250 feet O.D.— Gneiss, 24 in. by 12 in. by 12 in. Basalt, 30 in. by 24 in. by 24 in., planed on one side. Carboniferous sandstone, 24 in. by 12 in. by 12 in, Kirkmoorgate, near Robin Hood’s Bay.—600 feet O.D.— Rhomb-porphyry, 7 in. by 4 in. by 4 in. Also two smaller pebbles of same. Peake—Yorkshire Coast—600 feet O.D.— In thick glacial gravel, quarry above railway station, Shap granite 18 in. by 15 in. by 12 in. Rhomb-porphyry, Four small boulders, 346 ? REPORT—1900. Runswick Bay— 1 Shap granite, 30 in. by 24 in. on the beach near the village. 33 66 in. by 48 in. by 36 in. on the beach near the village. 3 Brockram, 12 in, by 8 in. 4 Magnesian Limestone, 60 in, by 48 in. by 36 in. 5 Shap granite, 24 in. by 24 in, by 18 in. 6 A 48 in. by 36 in. * 36 in. by 48 in. This group, with probably many others, in the bed of the largest of the four or five becks which run into the bay. 4 Speeton— Shap granite, 12 in. by 8 in. by 8 in. Stump Howe— 8 miles west of Whitby. 650 feet O.D. Rhomb-porphyry. A pebble, LINCOLNSHIRE. Reparted by Mr. J. A. Janpban, of Doncaster. rainsborough.—On Spital Hill— Large block of Shap granite, the light variety. Block of ‘ Greenstone ’ (probably dolerite). NoRTHUMBERLAND, Reported by Mr, P. F. KENDALL. Akeld, near the ruins of castle— Gravel, comprised largely of porphyrite with some Silurian Greywacke. Calder Farm, Roddam Dene— Porphyrite and Greywacke. The Movements of Underground Waters of Craven.—First Report of the Committee, consisting of Professor W. W. Watts (Chairman), Mr. A. R. DwerryHousE (Secretary), Professor A. SMITHELLS, Rev. E. Jones, Mr. Water Morrison, Mr. G. Bray, Rev. W. Lower Carter, Mr. T. Farruey, Mr. P. F. KENDALL, and Mr. J. E. Marr. (Drawn up by the Secretary.) TE Committee is carrying out the investigation in conjunction with a Committee of the Yorkshire Geological and Polytechnic Society. The present is merely an interim report, as the work is still in progress. It was decided that the first piece of work should consist of an investigation of the underground flow of water in Ingleborough. This hill forms with its neighbour, Simon’s Fell, a detached massif, which is peculiarly suitable for investigations of this nature. The summit of the group is formed of Millstone Grit, then follow Yoredale Shales and Sandstones, the whole resting on a plateau of Carboniferous Limestone, r | | | ON THE MOVEMENTS OF UNDERGROUND WATERS OF CRAVEN, 347 Many streams rise on the upper slopes of the hills and flow over the Yoredales, but without exception their waters are swallowed directly they pass on to the Carboniferous Limestone, to reappear as springs in the valleys which trench the plateau. The Committee first turned its attention to tracing the water which flows into Gaping Ghyll. It was generally believed that the water issued at a large spring immediately above the bridge at Clapham Beck Head and immediately below the entrance to Ingleborough Cavern. On April 28 specimens of the water from this spring were taken for analysis before the introduction of any test. wo cwt. of ammonium sulphate was then put into the water flowing into Gaping Ghyll, and at the same time the amount of the water was gauged and found to be equivalent to 251,856 gallons per diem. 210 SF ee — 10 Elgin 9 _— 9 9 =, | oa 9 Fife 24 —_ 24 | 7 ee 7 Forfar 7 — 7 = rn ee Haddington 4 — 4 oa) | dat 1 Inverness 72 42 | 414 an | 1 3 32 Kirkcudbright 3 2 3 2G ape ie us Lanark T — if oye) = ha 5 Linlithgow 2 — 2 SS ee Ba Orkney 1 — 1 —— = ae Perth 20 _ 20 3) = 3 Renfrew . 1 — | J =) = was Stirling 15 15 2) —_ 2 Sutherland 6 — 6 2 pas | BS 2 Total . 268 2 310 77 :. Wes 81 | IRELAND— | Antrim 195 31 226 29 ibe Sees 30 Armagh . 2 — 2 — i= i = Cavan 1 — 1 = aa ae RES Clare 8 Be Hecate = ee al = Cork 2 —_- 2 —— = ae arr Donegal . 39 5 44 2 1 = 3 Down 71 15 86 16 —_ a= 16 Dublin 27 — 27 3 = — 3 Fermanagh 4 — 4 1 = me 1 Galway . 28 1 29 3 = = 3 Kerry 10 16 26 — — = = Limerick i 1 2 — = a = Londonderry . 22 1 23 1 ~ == 1 Louth ut — 1 er ee a ae >~ . « ns E ON PHOTOGRAPHS OF GEOLOGICAL INTEREST. 353 | | | | Decheates | | Pre- | Addi- | Previous | | === Sn SE ee | a | vious | tions | Total collec- | Additions (1900) collee- | (1900) | tion Total | tion | | | Prints | Slides eye. .| 14 ae es yy ' Meath — 2 2 — | | Sligo. ; 2 2 4 — = eae a ‘Tipperary } 1 _— 1 — — _— = 56 Total . é 428 79 507 0}! ay oar ea 58 _ Rock Srruc- | | | TURHS, kc. (i) 1G Ais Ht 31 — | — 31 ForEIGN . | ee | —- | = 27 1 1 29 Enepanp .| 1361 | 188 | 1499 187 Sie thy oe 201 WALHIES .., «| 146. a~ 27 | 173 Ames ete i 43 CHANNEL Is- | | - LANDS SB) des ust) —_ 15 —_ — |; — — | ISLE oF MAN. 53 7 60 4 -- — 4 | SCOTLAND ios) Bia | 310 77 i eter) | aih IRELAND . ; 428 79 BUT eines Dome || 2 — 58} Rock STRUC- TURES. : 75 16 91 BL — — 3 | FOREIGN . : _ _— =e ere 1 1 29 Total . ,2346 | 309 | 2655 .| 495 |. 12 10 ,| 447... | | | | | | | Mr. Bingley continues to illustrate the history of the rivers of Yorkshire and the geology of the underground waters of that county. Mr. Welch sends thirty-three beautiful platinotypes taken in Antrim, Donegal, Down, Galway, Meath, and Sligo. Special mention should also be made of the interesting Skomer Island photographs of Mr. Small, the Irish ones of Miss Andrews, Mr. Gray, and Dr. Fogerty ; those from the Lake district by Lord Avebury and from the Isle of Man by Sir Archibald Geikie ; those illustrating a paper of Dr. Blanford by My. H.R. Blanford ; and the contributions of Mr. Pledge, Mr. Tucker, and the Hull Geological Society. To the persons already named, and to Mr. Garwood, Mr. Hollingworth, Mr. Cobbold, Mr. Davies, Mr. Lamplugh, Mr. Trevor Owen, the Yorkshire Naturalists’ Union, the Belfast Naturalists’ Field Club, and Mr. Midgley the thanks of the Committee are due; the last-named has sent a con- siderable series of micro-photographs for selection, together with a series of views. The members of the Yorkshire Geological and Polytechnic Society, and especially Mr. Tate, have conferred a signal service on the Committee by giving details of the Coal-measure sections taken some years ago by Mr. Branson in the Leeds brickyards. The sections have been measured, and each individual bed marked and numbered on the photographs by Mr. Tate. The duplicate collection has not received so many accessions as usual, chiefly because it is very fairly representative already. The additions to it during the year, and some others which have not yet been acknowledged, 1900. AA 354. REPORT—1900. ; are given in List II]. Twelve prints and ten slides have been received, and “the whole collection now numbers 336 prints and 111 slides. A list of donors to this collection is appended to the list, and to each of them the Committee express their thanks. The duplicate collection has been sent to the following Societies during the year :—The Limerick Field Club, the Leeds Geological Association, the Yorkshire Philosophical Society, ‘the South-Eastern Union of Scien- tific Societies, the Faraday Society of the Morley Memorial College, and the annual conversazione of the Birmingham Philosophical and Natural History Society. A request was received from the Science and Art Department that the Committee would exhibit a typical series of geological photographs at the Paris Exhibition. An appeal was sent to photographers, who responded with their usual readiness. A small set was got together and sent to Paris, where it is now exhibited. It has recéived the award of a silver medal in Class XII. The following contributed prints or lent negatives for this purpose :—Mr. R. Welch, Mr. Godfrey Bingley, Mr. A. Str: ahan, Mr. C. A. Defieux, Mr. C. J. Watson, Mr. A. A. Armstrong, Mr. A. K. Coomara-Swamy, Mr. A. 8. Reid, Mr. R. McF. Mure, Mr. H. L. P. Lowe, Dr. F. J. Allen, Mr. W. Jerome Harrison, and Mr. AV. Sie Tucker. The question of publishing a typical series of geological photographs has been considered by the Committee, and as a suflicient number of subscribers has been obtained it has been decided to proceed to the issue of twenty photographs annually for three years, both as prints and lantern slides. A committee of selection, consisting of Professor Bonney, Mr. Garwood, Dr. Mill, Mr. Teall, Mr. H. B. Woodward, and the Secretary, has made a provisional selection of representative ‘photographs. It is hoped that the first set may be issued within the year. The subscribers’ list includes a large number of foreigners and colonials. The list will be closed on September 12, 1900. Applications by local societies for the loan of the duplicate collectien should be made to the Secretary. Hither prints or slides, or both, can be lent, with a descriptive account of the slides. The carriage, and the making good of any damage to slides or prints, are expenses borne by the borrowing society. ELEVENTH LIST OF GEOLOGICAL PHOTOGRAPHS. (To Aucustr 25, 1900.) hs This st contains the geological photographs which have been received by the Secretary of “the Committee since the publication of the last Report. Photographers are asked to ailix the registered numbers, as given below, to their negatives for convenience of future reference. Their own numbers are added in order to enable them to do so. Copies of photographs desired can, in most instances, be obtained from the photographer direct, or from the officers of the Local Society under whose auspices the views were taken. The price at which copies may be obtained depends on the size of the pom and on local circumstances over which the Committee have no control. The Committee do not asswme the copyright of any photographs included in this list. Inquiries respecting photographs, and applications ON PHOTOGRAPHS OF GEOLOGICAL INTEREST. 559 for permission to reproduce them, should be addressed to the photographers direct. The very best photographs lose half their utility, and all their value as documentary evidence, unless accurately described ; and the Secretary would be grateful if, whenever possible, such explanatory details as can be given were written on the forms supplied for the purpose, and not on the back of the photograph ov elsewhere. Much labour and error of tran- scription would thereby be saved. A local number by which the print can be recognised should be written on the back of the photograph and on the top right-hand corner of the form. Copies of photographs should be sent wnemounted to W. W. Watts, Mason University College, Birmingham, and forms may be obtained from him. The size of photographs is indicated as follows :— L= Lantern size. 1/1 = Whole plate. 1/4 = Quarter-plate. 10/8 = 10 inches by 8. 1/2 = Half-plate. 12/10 =12 inches by 10, &c. E signifies Enlargements. * indicates that photographs and slides may be purchased from the donors, or obtained through the address given with the series, EIST Ti; ACCESSIONS IN 1899-1900. ENGLAND. Beprorv.—Photographed by H. C. McNuttx, 29 North Villas, Camden Square, N.W. 1/4. ie oO. ~ 191 ( ) Gas House, Leighton Buzzard False-bedding in Lower Greensand. 1897. BucxincHam.—Photographed by J. H. Puupex,* 115 Richmond Road, N.E. 1/2. 2416 (B13) South Windmill, Long ‘Shotover Sands.’ 1899, Crendon. 2417 (B11) Littleworth Brickyard, Drift. 1899. Wing, Leighton Buzzard. 2418 (B12) Warren Farm, Stewkley Northernmost exposure of typical Portland Beds in England. 1899. CornwaLi.—Photographed by A. E. Murray, Sé, Clare, Upper Walmer, Kent. 5/4. 2419 (7c) Constantine’s Bay . . Raised Beaches? ~ 1897. 2420 (9c) +c % : : = 2421 (32) ‘ cyclase is is 2422 (33 ca) Constantine’s Church . Church surrounded by sand-dunes. 2423 (33 cb) ~ 9 . x ” ” ” ‘DerspysHine.—Photogruphed by Evan W. Sma, The Mount, Radbourne Street, Derby. 1/1 E. 2500 (D991) L.& N. W. R. cutting, Anticlinein Carboniferous Limestone. 1899. Tissington. i 2501 (D992) L.& N. W. R. cutting, Syncline in Carboniferous Limestone. 1899. Tissington. AA 356 Regd. No. 2634 REPORT—1900. (229) Lion’s Head Rock, E. side of River Dove Phatographed by W. W. Minetry, Zhe Chadwick Museum, Bolton. 1/2. Crag of Carboniferous Limestone, 1900. DeEvoNnsHIRE.—Lhotographed by A. K. Coomara-Swamy, Walden, Worplesdon, Guildford. 1/1 E. 2424 2425 2426 ( ) Hound Tor, Dartmouth ( ) Cockington Beach, near Bideford. ( ) Cockington Seach, near Bideford. Photographed by H. Preston, Waterworks, Grantham. 399 ( ) Bowerman’s Nose, Dartmoor. Granite, jointed and weathered. 1900. Anticline in Culm Measures. 1900. 1/2. Jointed and weathered granite. 1900. Dorset.—Photographed by Y, H. W. Monckton, 10 King’s Lench Walk, 2429 2430 2431 2432 2433 2434 2435 2436 2437 2438 2439 2440 2441 2442 2443 2444 2445 2446 2447 2448 2449 2450 2451 2452 Temple, £.C. (1827) Near Grange Gate, Creech Grange. (1328) Corfe Castle . (13829) » : (1530) (1334) Studland Bay (1335) ” (1836) ; ; (1338) The “Agelestone, near Studland. (1339) The Agglestone, near Studland (1340) The Agglestone, near Studland (1342) Durlston Bay, Swanage . (1843) ” ” (1345) ? f 1/4, Working of pipe-clay of Bagshot 1899. U. M. and L. Chalk. 1899. ” ” ” age ” ” 9 Reading Beds resting on Chalk. Bagshot Sands and Clays. 1899, Bagshot Sands. 1899. 1899. ” ” | indurated ” Mass of Strata. ” ” ‘The Cinder Bed,’ Middle Purbeck. 1899. Anticline of Peverel Point, Upper Purbeck. 1899. Middle Purbeck between two faults. 1899. Photographed by 8. H. Ruynoups, University College, Bristol. 1/2 and 1/4. (18) Durdle Door (12) Man-of-war Cove, Lulworth (20) Stair Cove, Lulworth (21) W. side of Lulworth Cove. (22) W. side of Pondfield Cove (23) Bacon Hole, Mewp Bay (24) ” ” (25) Mewp Bay (26) _,, ” (27) Bat’s Corner. (28) W. of Lulworth Cove Arch of denudation, Portland Beds. Sea-stacks of Portland Stone. 1899. Contortions in Lower and Middle Purbeck Rocks. 1899. Weathering and faulting of Middle Pur- beck Rocks. 1899. ‘Broken Beds’ in Lower Purbeck Rocks. 1899. Sea-stacks of Portland Stone capped by Purbeck ‘ Broken Beds.’ 1899. Sea-stacks of Portland Stone capped by Purbeck ‘ Broken Beds.’ 1899. Sea-stacks of Portland and Purbeck Rocks. 1899. 1899- ~ ” , ” > Thrust-plane in Chalk clifts. 1899. Resistent character of hard Portland Rocks. 1899. ON PHOTOGRAPHS OF GEOLOGICAL INTEREST. BO aa 0. 2453 (29) Swire Head : : . Thrust-plane and inversion in Chalk. 1899, 2454 (30) E.of Swire Head . “ nN _ m 2455 (31) Man-of-war Cove. . Inverted Upper Cretaceous Rocks. 1899, 2456 (32) Crushed Flints. 1899. 2457 = (33) Arishmell Gap 3 : . Vertical bands of erushed flints. 1899. 2458 (34) Near Durdle Door . . Masses of chert in Upper Greensand. 1899. 2459 (35) ” ” Vertical Upper Greensand with chert masses. 1899. Duruamu.—Photographed by W. W. Mipetry, The Museum, Bolton. 1/2. 2336 (7) Roker Rocks, near Sunder- Concretionary Magnesian Limestone. 1896, land. 2 Photographed by KE. J. GArwoon, Dryden Chambers, Oxford Street, W.C. OE. 2502 ( ) Marsden Rock, near Sea-stack of Magnesian Limestone. Sunderland. Essex.—Photographed by A, E. Murray, St, Clare, Upper Walmer. 1/2. 2427 (1D) HalfmileS.ofDovercourt. Rapid advance of the sea, 1899. 2428 (2 D) »” ” ” ” ” ” ” GLOUCESTER. —Photographed by 8. H. Rrynoups, University College, Bristol. 1/2. 2460 (1) Observatory Hill, Clifton . The Clifton Fault. 1899. 2461 (2) - 5 - Junction of Millstone Grit and Carboniferous Limestone. 1899. 2462 (3) ks 3 a Detail of Clitton Fault. 1899. 2463 (4) st Ree eS Minor Thrusts in Carboniferous Limestone. r 1899. 2464 (5) Observatory Hill, Clifton, Minor Thrusts in Carboniferous Lime- and Avon Gorge. stone. 1899. 2465 (6) The Gully, Avon Gorge, Oolitic band in Carboniferous Limestone, Clifton. 1899. 2466 (7) Avon Gorge, Clifton . . The ‘Gully Oolite’ in the Carboniferous Limestone, 1899. 2467 (8) Hotwells and Clifton Down Coarse Dolomitic Conglomerate. 1899. Road, Clifton. : 2468 (9) Railway Cutting, near Chip- Unconformity, Dolomitic Conglomerate on ping Sodbury, G.W.R. Carboniferous Limestone. 1899. Kent.—Photographed by A. K. Coomara-Swamy, Walden, Worplesdon, Guildford. 1/4. S 2369 ( ) Charlton . 3 5 . Lower London Tertiaries on Chalk. 1899. 2370 ( ) Erith. ; : Z . Drift, Thanet Sand, and Chalk. 1899. 2371 ( ») Cliff near Copt Point, Junction of Gault and Lower Greensand, Folkestone. 1899, LancasHire.—Photographed by W. W. Minatry, The Musewm, Bolton. be 2333 (1) Hill Pike Quarry, near Saw- Ferruginous Upper Mountain Limestone, ley, folded. 1899, 358 REPORT-——1900. Regd. No. f 2334 (2) Foxley Bank, near Grindle- Ferruginous Upper Mountain Limestone ton. folded. 1899. 2335 (5) Foxley Bank, near Grindle- Ferruginous Upper Mountain Limestone, ton, folded. 1899. Photographed by G. Binciry, Thorniehurst, Headingley, Leeds. 1/1. 2493 (5184) Pimlico Quarry, near Transverse section of Carboniferous Lime- Clitheroe. stone Knoll. 1900. 2494 (5185) Pimlico Quarry, near Escarpment edge of Limestone in Knoll. Clitheroe. 1900. 2495 (5186) Pimlico Quarry, near Slab of Carboniferous Limestone with Clitheroe. heads and stems of crinoids from Knoll. 1900. 2496 (5186 1/2) Pimlico Quarry, near Carboniferous Limestone with slicken- Clitheroe, sides. 1900. Lincotn.—Photoqgraphed by J. Houtinewortu, Holderness Road, Hull, and communicated through the Hull Geological Society. 1/2. 477 (12) ‘The Cliff” S. of Humber, M. Chalk on L. Chalk with black marl between Barton and Ferriby. between. 1897. 478 (13) ‘The Cliff,” 8. of Humber, M. Chalk on L. Chalk, with black marl between Barton and Ferriby. between. 1897. 479 (14) South of Humber, near Disturbed beds of Chalk. 1897. Ferriby ‘ Cliff.’ Norroitk.—Photographed by Messrs. Raupu and Jutyan,* King’s Lynn, and presented by W. T. Tucksr, Park Side, Loughborough. 1/1. 2497 (15432) Near Railway Station, Gravel pit showing site in which human Hunstanton. bones were found. 1897. 2498 (1543) Near Railway Station, Gravel pit showing site in which human Hunstanton. bones were found, 1897. NorTHUMBERLAND.—Photographer unknown. 2503 ( ) Coaley Hill, near New- Outcrop of Coal-seam, castle-on-Tyne. Norrincnam.—Photographed by J. T. Ritny, and enlarged by E. W. Smauu, The Mount, Derby. 1/1 E. 2499 (N 900) Quarry near Hucknall Anticline in Magnesian Limestone. 1890? Torkard. SHROPSHIRE.—Photographed by E. 8. Coppotp, Watling House, Church Stretton. 1/4. 2635 (3) Comley Quarry, near The Cambrian Olenellus Limestone, 1899. Lawley, Church Stretton. 2636 (2) Sand-pit, west slope of Sandy drift dipping steeply to N.W. Hazler, Church Stretton. 1898. 2637 (4) Lawrence Hill Quarry, Banded coarse and fine Uriconian tufts. Wrekin. 1899. 2638 (5) Lawrence Hill Quarry, Banded coarse and fine Uriconian tuffs, Wrekin. 1899, ON PHOTOGRAPHS OF GEOLOGICAL INTEREST. 359 Somunsut,— Photographed by 8. H. Reynotps, University College, Bristol. Regd. No. 2469 (13) Shore between Portishead and Clevedon. 2470 (11) . ” » 2471 (12) - is E 2472 (13) Woodhill Bay, Portishead . 2473 (14) Farley Down, Bath . ‘ 2474 (15) ” ” 8475 (16) 9 " 2476 (17) 5 iY 1/4, Unconformity of Dolomitic Conglomerate on Old Red Sandstone. 1899. Unconformity of Dolomitic Conglomerate on Old Red Sandstone. 1899. Unconformity of Dolomitic Conglomerate on Old Red Sandstone. 1899. False-bedding in Old Red Sandstone. 1899. Weathering of Great Oolite. 1899. Freestone and ‘Rag’ in Great Oolite, 1899. False-bedding in Great Oolite. ” ” 3 1899. Surrey.—Photographed by J. H. Preper,* 115 Richmond Road, N.L. 1/2. 9504 (S1) Gravelly Hill, Caterham. 2505 (S3) N. of road between Bletch- ingley and Tilburstow Hill. 2506 (S4) N. of road between Bletch- ingley and Tilburstow Hill. 2507 (S8) N. of road between Bletch- ingley and Tilburstow Hill. 2508 (S87) N.N.W. of Tilburstow Hill Farm. 2509 (S5) S. of Oxted Station 2510 (S6) N. of Oxted village . Clay-with-flints over flint-pebble gravel. 1899. Massive cherts, &e., of the Lower Green- sand. 1899. Massive cherts, &c., of the Lower Green- sand. 1899. Chert in Lower Greensand. 1900. High dip in Lower Greensand. 1900. Folkestone Sands in Lower Greensand. 1900. Folkestone Sands in Lower Greensand, 1900. Photographed by H. W. Moncxrow, 10 King’s Bench Walk, Temple, E.C. 2511 (851) Chobham Ridges, Jack- pond Hill. 2512 (854) Chobham Ridges, R. Albert Asylum. 2513 (855) Chobham Ridges, R. Albert Asylum. 2514 (856) Chobham Ridges, R, Albert Asylum, 1/4, Sarsen in gravel. 1897, Large Sarsen. 1897. Sarsens. 1897, Large Sarsen. 1897, Sussex.—Photographed by F. Cuapman, 111 Oakhall Road, Putney, S.W. 400 ( ) Cliff at Aldrington, Brighton. near 1/4. Raised Beach and Rubble drift. 1899. Wesrmoretanv.—Photographed by Lorp Avesury, High Elms, Farnborough, Kent. 2411 ( ) NearShap ° 2412 ( ) Loughrigg Fell, near Amble- side. 2413 ( ) Loughrigg Fell, near Amble- side, 1/4. ‘Grikes’ or widened joints in Carboni- ferous Limestone. Rugged Fell made of Volcanic Rocks. Smooth hills of Silurian Rocks, Ordovician No. 2414 ( 2415 ( ) Churchyard, Ambleside ) " Yorxs1rE.—Photographed Headingley, Leeds. 2392 (5051) Conyngham Hall, Knares- borough. 2393 (5052) Conyngham Hall, Knares- borough. 2394 (5053) Lingerfield Quarry, Scriven, near Knaresborough. 2395 (5054) Lingerfield Schoolhouse . 2396 (5055) Scotton gravel pit 2397 (5056) Barf Lane, Farnham 2398 (5057) ” ” 2399 (5058) Cayton Gill, Morcar Wood, Markington. 2400 (5059) Cayton Gill, Morcar Wood, Markington. 2401 (5060) Cayton Gill, Morcar Wood, Markington. : 2402 (5061) Cayton Gill, Morcar Wood, Markington. 2403 (5062) Cayton Gill, Morcar Wood, Markington. 2404 (5063) Cayton Gill, Morear Wood, Markineton. 2405 (5064) Cayton Gill, Morcar Wood, Markington. ~~ 2406 (5065) Near Ripley 2407 (5067) Gray Gill, Malham . 2408 (5070) Broach Scar, Malham 2409 (5071) ” ” 2410 (5075) Site of ‘Camden,’ over- looking the village of Malham. 2486 (5160 1/2) Ingleborough 2487 (5161 1/2) : 2488 (5187 1/2) Long Kin East, Ingle- borough, 2489 (5188 1/2) Ingleborough, HE, side 2490 (5189 1/2) ‘ Jockey Hole,’ Ingle- borough. 2491 (5180) Bashall, near Clitheroe 2492 (5181) ” 2 REPORT—1900. Roche moutonnée. Glacial grooves in roche moutonnée. by G. Binatey, Thornichurst, 1/1,1/2 and 1/4. R. Nidd flowing over highly inclined Mill- stone Grit. 1899. Kt. Nidd flowing over highly inclined Mill. stone Grit. 1899. Red Boulder-clay on Millstone Grit. 1899, Moraine gravels covered by red Boulder- clay. 1899. : Moraine sands and gravels. 1899. Extra-morainic stream course, looking W. 1899. Extra-morainic N.E. 1899. Intake of Cayton Gill Valley. stream course, looking 1899. Looking down valley (Dole Bank). 1899. Lateral escape of Markington Beck. 1899, Valley looking down stream from road at Dole Bank. 1899. Inlet of lateral stream at Shutt House, first tributary. 1899. Fan delta of first tributary lateral stream, 1899. Narrowest part. 1899. Outlet of Cayton Gill, looking over delta. 1899. Gorge in Carboniferous Limestone. 1899. Weathered joints in Carboniferous Lime- stone. 1899. Weathered joints in Carboniferous Lime- stone. 1899, ‘Waterbursts. 1899. Pot-hole in Carboniferous Limestone. 1900. Pot-hole in Carboniferous Limestone. 1900. Pot-hole in Carboniferous Limestone. 1900. Swallow-hole in Carboniferous Limestone, 1900. Pot-hole in Carboniferous Limestone. 1900. Gravel-pit in Esker. 1900. Conglomerate in situ, in Esker. 1900. Photographed by J. Houuinewortu, Holderness Road, Hull, and communicated through the Hull Geological Society. 2480 (15) Hessle . 1/2. Upper Chalk overlain by recent grayel; 1897. ON PHOTOGRAPHS OF GEOLOGICAL INTEREST. 361 a 0. 2481 (16) Hessle Quarry. : . Joints, bedding and flints in Chalk, 1897. 2482 (17) Near Skidby ‘i s . Flint-bands in Chalk. 1897. Photographed by H. W. Monckton, 10 King’s Bench Walk, Temple, me. 1/P E. 2483 (761) Carnelian Bay,Scarborough Pillar of slipped Boulder-clay. 1896. 2484 (944) ” 9 2 Slipped Boulder-clay. 1897. 2485 (1133) _,, i 52 Slipped Boulder-clay showing flow- structure, 1899. WALES. Anetisnty.—Photographed by J. Trrvor Owen, County School, Carnarvon, and presented by E. GREENLY, Achnashean, near Bangor. 1/2. 2522 (1) Dwilban Point, Redwharf Sandstone ‘pipes’ in Carboniferous Bay. Limestone. 1899. 2523 (2) Dwlban Point, Redwharf Sandstone ‘pipes’ in Carboniferous Bay. Limestone. 1899. 2524 (3) Dwlban Point, Redwharf Connexion of sandstone pipes with the Bay. overlying sandstone. 1899. 2525 (4) Dwlban Point, Redwharf Large sandstone ‘pipe’ in Carboniferous Bay. Limestone, 1899. 2526 (5) Dwiban Point, Redwharf Deflected glacial strie in mouth of sand- Bay. stone ‘pipe.’ 1899. Carnarvon.—Photographed by J. WickEem,* Bangor, and presented by FE. GREENLY on behalf of the Moel Tryfaen Committee. 1/1 and 1/2. 2527 (3) Moel Tryfaen Quarry . . Generai position of drifts relatively to the topographic features of the district. 1898. 2528 (1) Alexandra Quarry, Moel Shelly sands and gravels resting on slate. Tryfaen. 1898. 2529 (2) Alexandra Quarry, Moel Shelly sands and gravels resting on slate, Tryfaen. 1898. 2530 (4) Alexandra Quarry, Moel Boulder-clay. 1898. Tryfaen. 2531 (5) Alexandra Quarry, Moel Sandy beds below Boulder-clay. 1898. Tryfaen. 2532 (6) Alexandra Quarry, Moel N.W. termination of Boulder-clay in sand Tryfaen. and gravel. 1898. 2533 (7) Alexandra Quarry, Moel Terminal displacement of slates below Tryfaen. sands and gravels. 1898. 2534 (8) Alexandra Quarry, Moel Terminal displacement of slates below Tryfaen. sands and gravels, 1898. 2535 (9) Alexandra Quarry, Moel Terminal curvature in slate. 1898. Tryfaen. 2536 (10) Alexandra Quarry, Moel fs 4 Fe Tryfaen. 2537 (11) Summit of Hill, Moel Try- Summit rocks. 1898. faen. Prmproke.—Photographed by E. W. Smaui, The Mount, Derby. 12/9, E. 2538 (P991) Broad Haven, St. Bride’s Contorted Coal-measure strata, 1899. Bay. 2539 (P oa Broad Hayen, St. Bride’s s $3 x ii ay ¢ 7 ‘ REPORT—1900, (P931) MarloesSands ., . Vertical Silurian beds, 1897. (P 973) 7 . Coast-erosion in inclined strata. 1897. (P 971) The Wick,SkomerIsland Dip-slope of Ordovician conglomerate; inlet of the sea along fault. 1897. (P 972) i; - a Felsitic rocks faulted against Basalt. 1897. (P 976) < “A td Sediments faulted against Basalt. 1897 (P974) ‘Tom’s House,’ Skomer Dip-slope of Basalt, promontory of Rhyo- Island. lite. 1897. (P 981) ‘The Basin,’ Skomer Weathering of Spheroidal Rhyolite. 1898. Island. (P. 982) The Mewstone Inlet, Marine erosion guided by the nature of Skomer Island. the rocks. 1898 (P 983) The Mewstone Inlet, Hffect of dip on surface feature. 1898, Skomer Island. ISLE OF MAN. Photographed by Sir ARCHIBALD GEIKIE, 28 Jermyn Street, S.W. 5/4, 2515 2516 2517 2518 2519 2520 2521 (1) W. end of Cromwell’s Walk, Vertical vesicular bands in Basalt. 1899, Scarlet Point. (2) W. end of Cromwell’s Walk, Gaps in lower edge of tabular Basalt now Scarlet Point. filled with agglomerate. 1899. (8) W. end of Cromwell’s Walk, Vesicular structure in tabular Basalt Scarlet Point. parallel to the lower surface. 1899. (4) W. end of Cromwell’s Walk, Steeply inclined vesicular Basalt with Scarlet Point. wrinkled surface. 1899. (5) Foreshore under Cromwell’s Dome-like strip of Cherty Limestone Walk, Scarlet. ; amongst coarse agglomerate. 1899. (6) Cliff, 800 yards S, of Close- Laminated Ash merging into confused, un- ny-Chollagh Point, Scarlet. stratified ash. 1899. (7) Cliff, 500 yards S. of Close- Ooarse Breccia of vesicular Basalt passing ny-Chollagh Point, Scarlet. into solid Basait. 1899, SCOTLAND. INVERNESS.—Photographed by A. K. Coomaka-Swamy, Walden, 2372 2373 2374 2375 2376 2377 2378 2379 2380 2381 2382 2383 . Worplesdon, Guildford. 1/4. ( ) Arnisdale, Loch Hourn . Moine Schists of Beinn Sgriol, 1899, (¢ ) Road from Glenelg to 5 = e aa Arnisdale. ( ) N. of Beinn Mhialairidh, Weathered Lamprophyre Dyke. i899. near Glenelg. ( ) N.of Rudha Mor, Sandaig. Coast erosion of Lewisian Gneiss, 1899. ( ) Sandaig, near Glenelg . Felsite Dyke in Lewisian Gneiss. 1899. ¢ ) Half-mile S. of Sandaig- Actinolite in Lewisian Gneiss. 1899. Burn. G ) W. of Port Luinge, near Contorted Lewisian Gneiss. 1899, Sandaig. G ) E. of Camas-nan-geann, W. of Raisaidh, Loch Hourn. ( ) E. of Ghlas Eilean, W.of Basaltic Dyke with vesicular centre. 1899, Raisaidh. ( ) E. of Ghlas Eilean, W. of 5 ” Raisaidh. ( ) Scuir-na-Gillean,- from Gabbro and Granophyre. 1899. Druim-an-Hidhne, Skye. ( ) Bhasteir Tooth, Scuir-na- Gabbro with Basic Dykes and Sills. 1899. Gillean, Skye. F ( ) Druim-an-Hidhne, Cu- Gabbro, with fine Felsite veins, 1899, chullin Hills, Skye. ”? ” ” ” ” 9 Feed. 2385 2386 2387 2388 2389 2390 2391 ON PHOTOGRAPHS OF ) Bruach-na-Frithe, Skye. ) Marsco, from Druim-an- Hidhne. ) Marsco, from Glen Sli- gachan. ) Ruadh Stac, Skye . “ ) Beinn - na - Cailleach, Broadford, ) Scorr, Portree Bay . ) W. Coast of Hige, W. of Beinn Tighe. cNoN Ci Yc SN ey) o> co GEOLOGICAL INTEREST. Gabbro, 1899. Granophyre Hills, 1899, Granophyre Hill. 1899, Granophyre. 1899. Granophyre of the Red Hills, 1899, Weathering of Basalt. 1899, Sill in bedded Basalt, 1899. Photographed by A. 8. Retp, Trinity College, Glenalmond, Perth. 1/2 and 1/4. 2549 2550 2551 2552 2553 2554 2555 2556 2557 2558 2559 2560 2561 2562 2563 2564 2565 (SR50) East Cliff of Rige (SR 51) ” ” ” (SR 92) Scuir of Higg ° (SR 45), (SR 44) East end of Scuir of Higg from N.W. (KL 28) Scuir of Hige é . (KL 30) ,, F (KL 32) _,, » (KL33) ” ” (SR62)._,, (SR 80) Hast end "of Scuir of Bigg from §. (KL 34) Scuir of Hige . 2 (SR 82) ” ” (SR 79) East end of Seuir of Higg. (SR 87) North-west end of Scuir of Higg. (SR 66) Scuir of Higg, Corn- bheinne Hill. (SR 52) Laig Bay, L. of Hige . Basalt flows with paler Andesitic band intercalated. 1899. Basalt flows with paler Andesitic band intercalated, overlying Jurassic rocks, 1899. With cloud-banner. 1899. Relation to Basalt platform. 1899. Position of E. of Scuir with regard to the Basalt platform. 1899. Exposure of Conglomerate under the Scuir. 1899. Conglomerate on floor of ‘Sheep Cave.’ 1899, ” ” ” ” ”” ” ” ” East end of Scuir. Devitrified bands of Pitchstone and two exposures of the river-conglomerate, 1899. Devitrified band in the Pitchstone. 1899, Devitrified and Spherulitic bands in the Pitchstone. 1899. Banding, &c., of Pitchstone, 1899, Truncated end of Scuir. 1899, Curvi-columnar structure of the Pitchstone. 1899 Erosion of dyke and its margin of fibrous Calcite. 1899. Photographed by H. R. Buanrorp, 72 Bedford Gardens, Campden Hill, W. 1/4. ad | North end of Loch Lochy ape of hills by glacial and stream 2566 2567 2568 2569 2570 Antrim.—Photographed by W. Gray, Glenburn Park, Belfast. 2339 2340 % Hillside 8.E. of Ceann Tah; Loch Lochy. (4) Hills 8.E. of Lagean, between Loch Lochy and Loch Oich. (5) Hills W. of Laggan . . erosion, Glacial and stream erosion. 1899. ” ” 0 ” ” ” ” ” IRELAND. (86a) White Rocks, nr. Portrush. (44) th) te ” 1/2. Marine denudation of Chalk. 1895. Arch in Chalk, 1895. (45) Near Dunluce REPORT—1900. (52) Giant’s Causeway, Lord Antrim’s Parlour. (53) Giant’s Organ, Causeway. (55) Windy Gap (56) Giant’s Causeway (43) Ballycastle (42) Giant’s (58) Larry Bane Bay, Bally- castle. (54) Fair Head , (51) Ballygally, ‘Wren’s E Egg" (47) Whitehead. (46) Macedon Point. . Chalk arch and headland capped by Basalt. 1895. Columnar Basalt. 1897. Columnar Basalt with cross joints 1897, Spheroidal weathering of Basalt. 1895, Jron-ore zone. 1895. Denudation of Chalk cliffs. 1894. 3) Chalk cliffs, 1894. Denudation of Columnar Basalt. 1890. Erratic of Basalt. 1895. Basalt Dyke in New Red Sandstone. 1895. Two intersecting dykes of Basalt. 1898, Antrim.— Photographed by R. Wetou,* Lonsdale Street, Belfast. 1/1. (1176) Stack-a-boy, Rathlin Is. 2601 2602 2603 2604 2605 2606 2607 2608 2609 2610 2611 2612 2613 2614 2615 2616 2617 (496) Straidkilly, Coast Road . (250) Giant’s Chimney Tops and Amphitheatre, Giant’s Cause- way. (971) Giant’s Causeway . (976) Giant’s Causeway, Middle Causeway. (242) Giant’s Causeway, The Loom. (5165) Giant’s Causeway (978) Giant's Causeway, Port- coon Cave. (799) Giant’s Causeway, The Stookans. (5775) Carey River Head (239) Carrick-a-Rede Ravine (655) Whitepark Bay, (609) Fair Head Ballintoy. (5153) Olifts of Murlough Bay . (586) Cushendun (551) Ess-na-larach, Glenariff . (5204) Grant’s Mines, Toome Sea-stack of rudely Columnar Basalt Lavas. 1899. Village, on Lias which is continually slipping seaward, 1886. Columnar and massive Basalt flows, 1886. Floor of Columnar Basalt. 1890. Columnar Basalt. 1890. Long columns of Basalt. 1886. Spheroidal weathering of Basalt. 1897. Cave worn by marine action in Spheroidal Basalt. 1886. Breakers rolling over ledges of Columnar Basalt. 1887. Lower end of underground channel drain- ing Lough-a-veena into Carey River. 1898. Sea gully in a volcanic neck. 1890. Prehistoric settlement and middens. 1897. Coarsely Columnar sheet cf Dolerite. 1890, Chalk cliff with talus, slipping over Trias beds below. 1898. Cave worn by marine action in coarse con- glomerate of Old Red Sandstone age. 1889, Ravine in Basalt worn by waterfall. 1894. Diatomaceous Harth (‘ Bann clay’). 1899. Crare.—Photographed by G. FoceErry, 61 George’s Street, Limerick. 1/2. 2353 2354 2355 2356 2357 (3) Fanore, near Black Head (5) Caher, Lower, near Black Head. (6) Black Head (2) Farrihy Bay (4) Cliffs of Moher Jointing in Carboniferous Limestone. 1899. Terraces of Carboniferous Limestone. 1899. Escarpment Cliff of Carboniferous Lime- stone. 1899. Marine denudation of Lower Coal- measures. 1895, Steep and lofty cliffs of Carboniferous Rocks. 1899, ON PHOTOGRAPHS OF GEOLOGICAL INTEREST. Go ot Doyucat.— Photographed by R. Wutcn,* Lonsdale Strect, Belfast, and sent through the Belfast Naturalists’ Field Club. 1/1. 2618 (2242) Cratlagh Wood, Mulroy Schistose area of Donegal. 1893. Bay. 2619 (2259) Rosapenna . - . Section through sand-dune on which old kitchen-midden rests. 1895. 2620 (5209) Barnesmore Gap . . Pass in granite area. 1900. 2621 (1440) Croaghconnellagh, Mt. Granite Mountain, cliffs over talus. 1900. Barnesmore. 2622 (5135) The Pullins River, Bal- River entering underground channel. lintra. 1894. Down.—Photographed by R. Weicu,* Lonsdale Street, Belfast, and sent through the Belfast Naturalists’ Field Club. 1/1. 2623 (5208) Sampson’s Stone, Down- Large Basalt erratic. 1900. patrick. 2624 (5180) Newcastle . . . Sand-dune, showing the retaining action of Bent, &c. 1898. 2625 (5179) ep : : . Section of sand-dune, showing wind erosion and false-bedding. 1898. 2626 (5178) Newcastle and Slieve Storm ridges of raised beach partly covered Donard. with sand-dunes. 1898. 2627 (5177) Newcastle 5 . Thin-bedded Ordovician strata. 1898. 2628 (5176) Cliffsat Maggie's Leap, Thin-bedded, slightly contorted, Ordo- Newcastle. vician strata. 1898. Photographed by W. Gray, Glenburn Park, Belfast. 1/4. 2358 (49) Ards Coast, Strangford Erratic Block. 1896. Lough. 2359 (50) Ballyhalbert . . s - on Silurian Rocks. 1896. 2360 (62) Wallace’s Rocks, Bally- Folded Silurian Strata. 1895. halbert Road. 2361 (65) Ballyhalbert . ‘ . Basalt dykes in Lower Silurian Rocks, 1895. 2362 (63) Gunn's Island . : . Basalt dykes in Lower Silurian Rocks. 1895. ‘ 23863 (64) Sheepland Harbour . . Basalt dykes in Lower Silurian Rocks, 1895. Photographed by Miss Mary K. Anprews, 12 College Gardens, Belfast. 1/4. 2366 (11) Newcastle, little N. of Erosion of sea coast. 1899. Harbour. 2367 (9) Newcastle, little N. of Pe . Harbour. 2368 (10) Newcastle, little N. of $5 a Harbour. Gatway.—Photographed by R. Wetcu,* Lonsdale Street, Belfast, and sent through the Belfast Naturalists’ Field Club. 1/1. 2629 (5221) Near Ahascragh, Ballin- General character of the central Limestone asloe. Plain of Ireland. 1900. Kerry.—Photographed by 8. H. Ruynoups, University College, Bristol. 1/4. 2585 (36) Near Clogh, Clogher Head Dip of Silurian flags, 1899. District, 2365 2364 REPORT—1900. (37) Gully near Clogh Point, Clogher Head District. (39) North of Clogh Point, Clogher Head District. (40) North of Drom Point, Clogher Head District. (41) North of Drom Clogher Head District. (38) Inlet S.E. of Foilwee, Clogher Head District. Point, (42) 8. of Foilwee, Clogher Head District. (43) Coosmore, Clogher Head District. (44) Doon Pointand Sybil Head, Clogher Head District. (45) Minnaunmore Rock Croaghmarhin Hill. (46) Clogher Head District : (47) Northside of Clogher Head. (48) South-east of Foilwee, Clogher Head District. (49) Minnaunmore Rock, Clo- gher Head District. (50) West of Redcliffe Cove, Clogher Head District. (51) Off Bull’s Head, Dingle Promontory. and Influence of dip on form of gully. 1899. Inlet eroded along junction of flags with overlying tuffs. 1899. Bedded tuffs alternating with Sandstone bands.. 1899. Alternating coarse and fine tuffs and Red Sandstone. 1899. Erosion along bedding plane. 1899. Faulting in bedded tuffs. 1899. Disturbed Ludlow beds. 1899. Joint cave. 1899. Rugged rhyolite hill and smooth hill of Silurian slate. 1899. ‘Fucoid markings’ on Ludlow flags. 1899. Rhyolite blocks in coarse ash. 1899. Weathered surface of nodular rhyolite. 1899. Weathered surface of nodular rhyolite. 1899. Weathered surface of tuff. 1899. Sea-stack of Dingle beds. 1899. LimERIcK.—Photographed by G. Foczrtry, 61 George’s Street, Limerick. (1) Gahetconlish }- 6, « 1/2. Columnar porphyritic igneous rock. 1897 Lonponpirry.—Photcgraphed by W. Gray, Glenburn Park, Belfast. (66) Benbradagh ., . : 1/2. Chalk quarry, the most westerly in Europe. 1899. Meatu.—Photographed by R. Wutcu,* Lonsdale Street, Belfast, and sent through the Belfast Naturalists’ Field Club. 1/1. 2630 (1150) Gorge of the Boyne at Contorted Carboniferous Limestone cut Beaupare. through by river. 1900. 2631 (5222) Gorge of the Boyne at Contorted Carboniferous Limestone cut 2632 Beaupare. through by river: nearview. 1900. S1r1co.—Photographed by R. Wuucu,* Lonsdale Street, Belfast, and sent through the Belfast Naturalists’ Field Club. (2095) Glencar, Sligo 5 . 1/1. Escarpment cliff of Carboniferous Lime- stone. 1892. 2633 (2100) Glencar Fall, near Sligo. Cirque with waterfall in Carboniferous 2337 2338 Limestone. 1892. ROCK-STRUCTURES, &c. Photographed by W. W. Mipeuzy, Lhe Museum, Bolion. (4) Castleton, Derbyshire . . (5) Corriegills, Arran ‘ . 1/4. Coralline Mountain Limestone (micro.). Pitchstone (micro.). ON PHOTOGRAPHS OF GEOLOGICAL INTEREST, 367 Regd No. 2572 (8) Ennerdale, Cumberland . Granophyre. x 20. 2573 (9) Luxulyan, Cornwall . . Schorl-granite. x 20. 2574 (11) Tormore Shore, Arran . Pitchstone. x 60. 2575 (12) Brodick School House, Pitchstone. x 60. Arran. 2576 (14) Arran : -, + Spherulites. x20. 2577 (16) Bolton, Lancashire . Blast-furnace slag. x 20. 2578 (17) Giant’s Causeway, Antrim. Basalt. x 20. 2579 (18) River Coquet, Rothbury, Dolerite. x 20. Northumberland. 2580 (23) Cloughwater, Antrim . Rhyolite, with flow-structure. x 20. 2581 (26) Keswick, Cumberland . Agates in volcanic ash. x 20. 2582 (29) Inchcolm Rock . é - Picrite. x20. 2583 (30) Near Edinburgh “ = Pierttege 20: 2584 (36) Wolf Rock, Cornwall . Phonolite. x 20. Photographed by G. Bineiey, Thorniehurst, Headingley, Leeds. 1/4. 2571 (5190) SalthillQuarry, Clitheroe Spiriferastriata, showing spiralarms. 1900. LIST’ if NUMBERS OF OLD PHOTOGRAPHS CANCELLED. 191, 399, 400. LIST II. RENEWALS AND CORRECTIONS. Renewals. Yornswine.—Renewed by G. Binainy, Thoriiehurst, Headingley, Leeds. 1/2. 2. 506 (1755) How Stean Beck, Upper Deep Gorge in Carboniferous Limestone. Nidderdale, near Pateley 1891. Bridge. Dnvon.—FRenewed by A. K. Coomara-Swamy, Walden, Worplesdon, Guildford. 1/4. 2058 ( ) Bindon, W. of Lyme Regis. Cliff caused by Landslip. 1898. Antrim.— Renewed by J. Brown, Belair, Windsor Avenue, Belfast. 1 /2: 657 () MuckIsland. . ,. . Marine Denudation. 1892. Down.—Renewed by Miss M. K. Anpritws, 12 College Gardens, Bebfust. 1/2. 340 (¢ ) Copelandisland . .« . Lower Silurian Rocks. 1891, Lonponprrry.—Reviewed by Miss M. K. Anpruws, 12 College Gardens, Belfast. 1/2. 529 () Downhill) . . «. | Chalk underlying basalt. 1891. Corrections. Wonrcustersiiint. —Photographed by W. J. Harrison, 52 Claremont Road, Handsworth, Birmingham. 1/2. 1440 ( ) California,nearBirmingham EBoulder clay. 1896. 1441 () ” ” » ‘Indiarubber clay ’ on Till. “1896, 368 REPORT—1900. Regd. : No. 1442 ( ) Moseley, near Birmingham. Glacial sands. 1896. 2275 ( ) California,nearBirmingham Bunter Sandstone. LIST IV. THE DUPLICATE (LOAN) COLLECTION. The numbers placed after the description of the photograph refer to the list of names and addresses given at the end. The first refers to the photographer, who is also the donor in most cases. When he is not, the donor is indicated by a second number. Full localities and descriptions are given in present and previous lists under the numbers. « This collection is arranged geologically, and from time to time the less perfect and less typical photographs will be removed and better ones sub- stituted as they are given. Those laid aside can always be seen, sent, or returned by request. * Indicates that prints and slides may be bought from the photographer. P. indicates prints. §. indicates slices. Rock-Structures. Bedding. Reed. No. 4664 Bedding and Jointing in Carbo- Muckros ‘ Market House, Kilcar, Donegal. niferous Limestone. “leks Evidences of Earth-movement. Elevation and Subsidence. 4887 [aised Beach on Pilton Beds . Saunton Down End, Larnstaple Bay. a 49 8. Folding. 2425 Anticlinc in Culm-measures . Cockington Beach, near Bideford. 40 P.S. 2426 Anticline in Culm-measures . Cockington Beach, near Bideford. 40 P. ZO Folded CarboniferousLimestone Draughton, near Skipton. 215,15. 2378 Contorted Lewisian Gneiss . West of Port Luinge, near Sandaig, Glenelg. 40 P.5. Surface Agencies ; Denudation and Deposit. Weathering. 6270 Honeycomb-weathering in Keu- Budleigh Salterton. 49%, per Sandstone. 4 2437 Outstanding Rock . : . TheAgeglestone, near Studland, Dorset. 598. 2438 9 9 ». 92 ” Volcanic and Plutonic Rocks. Volcanoes. ¥.26 OraterLake . . «. « Pulvermaar, Hifel,Germany. 40 P, ON PHOTOGRAPHS OF GEOLOGICAL INTEREST. 5369 Rock-masses and their Relations, Regd, No. F.14 Alternations of Basalt lava and ‘Cascade Section,’ Mont Dore, Auvergne, tuff. France. 405. 2374 Weathered-ont Lamprophyre North of Beinn Mhialairidh, near Glenelg, dyke, 40 §. Characteristic Rocks and Landscapes, Paleozoic. 2377 Actinolite in Lewisian Gneiss . Half a mile south of Sandaig Burn, near Glenelg. 405. 438 Coal-measures above Beeston Longley’s Brickyard, Leeds. 58 P, Bed. 439 Coal-measuresincluding Beeston Grosvenor Brickyard, Leeds. 48 P. Bed Coal 440 Coal-measures above the Crow Boyle’s Quarry, Leeds. 58 P. Coal. 4141 Coal-measures including Crow a re - Coal. 442 ‘Black Bed’ CoalSeam . . Dolly Lane Brickyard, Leeds. 58 P. 143 ‘Better Bed’ CoalSeam . . Benson Street Brickyard, Leeds. 58 P. Mesozoic. 990 Paramoudras in Chalk ¢ . Soldierstown, Moira, Antrim. 56 P. Names and Addresses of Donors and Photographers. 9. R. Welch, Lonsdale Street, Belfast. 15. A. S. Reid, Trinity College, Glenalmond, Perth. 21. Professor E. Waymouth Reid, University College, Dundee, 40. A. K. Coomara-Swamy, Walden, Worplesdon, ‘ruildford. 49. Miss H. M. Partridge, 75 High Street, Barnstaple, 56. W. Gray, Glenburn Park, Belfast. 658. F. W. Branson, 14 Commercial Street, Leeds. 59. H. W. Monckton, 10 King’s Bench Walk, Temple, E.C, On the Geological Age of the Earth. By Professor J. JOLY, D.Sc., F.R.S. [Ordered by the General Committee to be printed in ewtenso.] On account of a certain small amount of arithmetical complexity involved in the statement of the method of estimating the age of the earth by solvent denudation, I have had a brief summary of it put into print, all the quantities involved being calculated into the metrical system of units (see Appendix). With this in your hands I may be permitted to leave figures aside in the few remarks I have to make. In this method, as the President of the Geological Section has already stated, the sodium contained in the sea is assumed to be a measure of the total amount of solvent denudation since the oceans were formed, and the amount of sodium annually supplied by the rivers is taken as a measure of the rate at which this denudation has been effected. Why attention is restricted to the sodiwm need not be enlarged upon further than to say that every other element supplied by solution of the rocks is again rejected by the sea to an extent which renders it unavailable. Tt will be found on reference to the summary that allowance is made for a effects of the probable amount of active acid primevally wncom- 1900, BH 370 REvOR'T-—1900. bined, on the basis that sensibly the whole of the chlorine now in the ocean was then existent in the form of HCl. This amounts to a sub- tractive correction of under 6 per cent. on geological time. After con- sideration of all the facts, I do not think any further concession to the popular assertion, that ‘the sea was salt from the first,’ can be made. A deduction is also suggested for direct solvent denudation by the sea. The correction is taken as between 3 and 6 per cent., the basis of correc- tion being the ratio of the tide-swept area to the total rainy land area, and some experiments which appear to show that over the same area of rock surface the rate of marine solution cannot be more than twenty times the rate of atmospheric denudation These experiments are communicated to this Section. They are somewhat incomplete, but their rough indica- tion may be accepted as sufficient for the present purpose. Allowance is also made for the transport of sodiwm from the sea to the rivers through the atmosphere. Data are required in order to define this allowance more precisely. The brief review of the method before you also refers to the rock-salt deposits. These appear to be quite negligible compared with the enormous mass of chloride of sodium row in the ocean—sufficient to cover the entire land area to a depth of 122 metres—unless deposits of this substance, far greater than anything at present dreamt of, are discovered. Some other possible sources of error are considered, but these will more fitly be referred to further on. It is a confirmation of the general validity of the method that accept- ing—with slight modifications—Mr. Mellard Reade’s estimate of the total mass of detrital sediments, and a mean soda content of these sediments, based on a very considerable number of analyses, we find that the resulting total mass of contained sodium added to the soda equivalent of the sodium now in the ocean suffices to restore to the adequate mass of parent igneous rock a soda percentage approximately equal to that of the mean igneous crust-rock of the earth. In other words what sodium is con- tained in the ocean is approximately equal to the amount which would have been wasted from such a mean igneous rock upon its degradation into the probable mass of detrital sediments. Finally we find the method affords on the basis of the best data available a duration since subaérial denudation began of between ninety and one hundred millions of years. Professor Sollas has really referred to the weakest point in this estimate when he questions the sufficiency of the data affording the annual river supply of sodium. However, there is much reason to believe that the nineteen rivers—a fair admixture of great and small ones—afford an approximation to the nature of what the world’s rivers yield in the form of dissolved matter to the ocean. The want emphasises Professor Sollas’s demand for more experiment, and Sir Archibald Geikie’s for geological co-operation. The data required are really of the easiest to obtain. The method is, of course, based on the principle of uniformity, but the generalised nature of the measure of uniformity actually required is worthy of attention. The claim is restricted to the association of atmospheric water and of rock over a surface of land approximately equal to the present rainy area of the globe, the climatic conditions doubtless differing in each geographical region from age to age, but on the whole preserving an approximate uniformity in denudative effect, as measured, say, by the solvent denudative work accomplished per million of years. ON THE GEOLOGICAL AGE OF THE EARTH. 371 How far will this measure of uniformity be conceded? Whether erystalline or sedimentary rocks prevail does not appear seriously involved in the long run, for we find soils derived from the latter actually exposing larger amounts of alkaline silicates : the higher resistance to disintegra- tion offered by the crystalline rocks often conferring upon their soils the réle of an exhausted and protective covering. Again, it is only within fairly wide limits a question of climate, for the rate of solution of the silicates is so slow that the amount of the solvent present is of less import- ance than its persistent operation even in minute quantities. The rate of solution would certainly not increase proportionately to the amount of the solvent, a very wet climate being very possibly, even probably, less effective than a warm and damp climate more rarely visited by rains. As regards the rainy area exposed to subaérial denudation during past geological periods, considerable latitude with respect to the effects of up- heaval or depression is suggested by the fact that the supply of water evaporated by the ocean is to-day insufficient to ensure drainage from more than four-fifths the total land area. If to-day 10 per cent. of the land subsided beneath the ocean, probably but a small change in the river discharge of dissolved matter would result. The disappearance of this 10 per cent. of the land would increase the oceanic area but 4 per cent., and the ‘rainless’ areas of the continents would diminish to one- tenth the total land surface. In short, the rainy margins would— roughly speaking—move inwards. In the opposite case, that of upheaval, the rainy margin will move outwards. Thus the deposition or upheaval of our greatest sedimentary masses was not necessarily accompanied by any notable variation in the supply of dissolved matter to the sea. Tn short, it would appear that changes of a quite abnormal or cata- strophic natwre must be looked for to seriously affect the average rate of the operations at work. I must refer to the evidence for and against such effects. As regards hydrothermal actions, due to lingering heat in the primitive oceans, on Lord Kelvin’s figures for the rate of cooling this action must be negligible. If his figures were multiplied even tenfold, the error could hardly at most amount to 1 per cent. I may also now refer to the objection urged by Professor Sollas, that underground temperature may for long have given rise to a geyser-like action of springs which would have enriched the sodium supply of the early rivers. If of a serious character this objection should be supported by more evidence of such solvent actions than our most ancient sediments reveal. Thus it isremarkable that so far from the earliest sediments or their probable metamorphosed remains being the most washed-out of the rocks they are often those possessing the largest percentages of alkalies. The oldest Cambrian and Silurian sedi- ments and gneissic rocks of archzean age and probable sedimentary origin show percentages of alkalies almost comparable to those of the mean igneous earth-crust and exceeding the average of later sediments and of sediments at present being deposited. I therefore cannot think that any exceptional solvent actions applied to these sediments when being deposited or when buried or subsequently when uplifted and exposed to atmo- spheric denudation can be generally assumed. Geyser actions or circula- tion of underground waters among unfaulted primitive igneous rocks, on the other hand, would arise only under exceptional conditions. And, again, we may ask, where in the earlier igneous rock-masses have we evidence of exceptional geyser-like actions ? BB2 372 REPORT—1900. I may point out here that Daubrée’s experiments by no means support the view that crystalline rocks are rapidly attacked by superheated water, but rather demonstrate the contrary. At a pressure which Daubrée esti- mated at more than 1,000 atmospheres, and at a red heat, water failed to appreciably attack, after many weeks, sanidine, oligoclase, pyroxene, or potash mica. The contrary is generally inferred from the general atten- tion which has been paid to his experiments on glass and obsidian, The early igneous rock crust from the general prevalence of conditions of slow cooling would almost certainly have been highly crystalline. The notion that exceptional vulcanism prevailed in the earliest times appears unproved. The traps and dykes of archean rocks are not always evidence of subaérial outbursts—the Lewisian and Torridonian rocks of Scotland may be quoted as examples, where, although there is much injec- tion of igneous matter, there is no evidence of corresponding volcanic action. And, again, it may be well questioned, granting even excessive volcanic action, how far it would affect the methodical supply to the ocean of dis- solved alkalies by the rivers. Early tides of gigantic height have been rather discredited. Any one reading Professor G. Darwin’s delightful book on ‘Tides’ will be struck with the caution and moderation of the writer. He maintains ‘the pos- sibility that a considerable part of the changes due to tidal friction may have occurred within geological history,’ yet thinks it ‘probable that the greater part of the changes due to tidal friction must be referred back to pre-geological times when the planet was partially or entirely molten.’ This involves, of course, that the epoch of most violent activity prevailed in pre-geological times before the work of denudation had begun. And here, again, even admitting higher tides, it may be seriously asked on what grounds we assume such higher tides to effect solvent denudation positively rather than negatively. If the tides of to-day rose so as to encroach five miles further on the coasts, would the loss of soil area re- sulting compensate for the gain of bare superficial rock swept by the sea ? A soil but 10 cms. deep may expose an area 50,000 times its superficial area to the solvent actions of hygroscopic water and rain, CO., organic acids, &e. Professor Perry, writing in ‘ Nature,’ has suggested the possibility of diminished sun-heat at a period as recent as some 50 x 10° years ago. But so far as I know, Professor Perry has not gone further than to suggest the possibility of this external interference with the orderly succession of events in the earth. But finally in regard to all these surmises, interesting and valuable as they undoubtedly are, can I do better than torefer to Sir A. Geikie’s reading of rock-testimony on this point? Sir A. Geikie seeks one hundred million years as sufficient for the sedimentary history of the earth. His words are recent—dating from his address to the Geological Section last year. The evidence of the sedimentary rocks, he affirms, shows no more stupendous mountain upheavals, volcanic eruptions, or greater violence in the sur- rounding envelopes of atmosphere and ocean than occurred in more recent periods or than we are acquainted with to-day. ‘Even in the most ancient of the sedimentary registers of the world’s history not only is there no evidence of colossal floods, tides, and denudation, but there is incontestable proof of continuous orderly deposition such as may be witnessed to-day in any quarter of the globe. The same tale with endless additional detail is told all through the stratified formations down to those which are in course of accumulation at the present day.’ ON THE GEOLOGICAL AGE OF THE EARTH. 373 Tf now the sodium-method affords a correct key to the age of the earth, it remains to criticise methods yielding discordant results. And first, as regards the method by rate of deposition, we find Sir A. Geikie claiming a period, as we have seen, in perfect accord with that shown by solvent denudation. Professor Sollas, however, considers the actual record indicates ashorter period. I think, however, he has very fully and fairly shown that much difficulty attends the actual measurements as well as the application of the measurements. In the first place it may be observed that the data have been obtained from an inadequate number of rivers. Again, the detrital matter discharged by rivers is most difficult to estimate, owing to the rapid variation of transporting power with current-velocity, and also owing to the fact that a very large amount of sediment is transported by creeping along the river bed. Both these facts render measurement so difficult that only the most painstaking observations could be relied on for an approximate estimate. And suppose we possessed the required estimate of detrital material, how are we to dispose of it so as to represent what we may call the average mode of maximum deposition? Some rivers form deltas which creep out- ward year by year. Here the rate of deposition is evidently not balanced by subsidence. There is in fact no one law of deposition, nor can there be. Once more, can we ever know the total maximum thickness of the sediments? It must be that the sediments of one period supply in great part those of the next. The very quantity we estimate in the rivers in order to find our denominator has been robbed, perchance, from our numerator. Have we, in fact, when all care is taken, measured the true maximum thickness, or would sediments long ago removed afford vastly greater maxima ? Now observe the method is exposed, here at its weakest point, mainly to errors of deficiency : and the method in its latest develop- ment, in the able hands of Professor Sollas, affords but some twenty-six millions of years, and according to Mr. Wallace twenty-eight millions of years. There is another method based on Jological progress which seems to go to the opposite extreme and claims immense periods of time. Lyell claimed on biological grounds 240 millions of years since the Cambrian ; Haughton, 200 millions ; Darwin speaks of a pre-Cambrian period as long as the sum of the subsequent geological ages. Professor Sollas has, with justifiable authority, dealt with this matter. And indeed we may well ask if the argument does not assume an unwarranted proportionality in the rates of evolution throughout successive ages. Surely the organism of Jater date owes something of its stability to heredity ? Can we assume that when trial was less likely to be attended with error, owing to a less severe competition, species and genera were not struck off more rapidly than later under more restricted conditions, and when ages of increasing restraints had impressed upon the germ-plasm a more stereotyped heredity? It appears difficult to imagine that the organism as we see it to-day so willing to take advantage of every loop- hole and fill up every vacancy should have dropped its opportunist character in early times and failed to profit by the more generous environment. If this is so, can we accept with Huxley the period required for the development of the horse as an indication of the length of the history of ungulates? But this argument has been taken up already by Mr. Adam Sedgwick, who has urged that in the evolution 374 REPORT—1900. of heredity a veconciliation of the demands of biologists and the restric- tions placed by the physicist on geological time may be found. His address to the Zoological Section last year will be fresh in the minds of all, and I need not further press the point. Turning to physical methods we have Professor Darwin’s age of the moon, suggesting a minimum of fifty-seven millions of years, to which Professor Sollas has referred. Lord Keivin’s method, based on the rate of cooling of the globe and the observed fall of temperature in the terrestrial crust, depends for the accuracy of its indication on data regarding the physical properties of the deeper-lying materials of the earth which we do not as yet possess. This has been fully discussed lately by Professor Perry. The distinguished author of the method has at no time denied the restrictions placed by our present ignorance on the indications of the method. The effect is not to deprive the method of value, but to restrict its present functions to the delimitation of certain bounds to our speculations, which bounds may on the minor estimate be taken as some twenty millions of years, but which may, according to the density, specific heat, and conductivity of the deeper-lying materials at elevated tempera- tures, allow of a much more extended estimate. It must be admitted that no one method of approaching the delicate question of the age of the earth can claim to have reached that con- ststentior status which we look for in scientific results. So much may possibly have happened during the long past vista which it is hoped to penetrate that more than a considerable degree of probability may never be attained by our results. Admitting this, I have to appear perhaps in the light of an advocate when I state my belief that the method by solvent denudation is not discredited by the conclusions arrived at by other methods, in so far as these assign major or minor limits to the age of the earth, and that none other approaches the question so directly or on such easily obtained data, APPENDIX. The Geological Age of the Larth. [Read before the Congrés Géologique International, 1900.] The method of determining the age of the earth summarised in this paper is based on the assumption that the ocean has retained substantially the whole of the sodium committed to it by the solvent denudation of geological time, and that the supply of the element sodium by the rivers has on the whole been uniform in rate.! Hence we derive as a numerator a number expressing the mass of sodium at present in the ocean, and a denominator expressing in the same units the amount of this element annually discharged into the ocean by the rivers of the world. The quotient is the geological age of the earth. Corrections are applied to both numerator and denominator for any certain or very probable source of error. These corrections are approxi- mate only, upper and lower limits of their values being suggested.” 1 No other dissolved substance in the ocean conforms to the first of these con- ditions. 2? A more amplified account of what follows will be found in a paper by the author, ‘An Estimate of the Geological Age of the Earth, Z7ans. Royal Dublin ON THE GEOLOGICAL AGE OF THE EARTH. 370 First Approximation to a Numerator. According to Professor Dittmar,! if the ocean has a total mass of 1-343 x 10!8 tonnes, the sodium chloride in it amounts to 36,566 x10!" tonnes, However, on Professor Wagner’s” estimate of the area of the land surface of the globe as 14,456 x 10! square kilometres, and the ratio of the areas of water and land as 2°54: 1, and on Sir John Murray’s estimate * of the mean depth as 3°851 kilometres, the total mass is more correctly 1-458 x 10'8 tonnes. On these data we can readjust Professor Dittmar’s estimate of the mass of NaCl in the ocean, finding it to be 39,703 x 10! tonnes, and from this finally arrive at the result that the mass of sodium in the ocean is 15,611 x 10!? tonnes. First Approximation to a Denominator. On Sir John Murray’s estimate ‘ the river water annually discharged into the ocean amounts to a volume of 27,191 cubic kilometres, and from his table of the mean dissolved constituents of nineteen rivers—many of them principal rivers of the world—we find that a cubic kilometre of average river water contains as sodium salts 7753 tonnes of Na,SO,, 6534 tonnes of NaNO;, and 4061 tonnes of NaCl. Calculating from these the masses of sodium in each case, and multiplying by the total number of cubic kilometres, we arrive at 15,976 x10! tonnes as the total mass of sodium carried annually into the sea by the rivers. The quotient is a first approximation to the age of the earth, and is 97°6 millions of years. Correction on the Denonunator. It is convenient to consider this first. The mass of sodium chloride carried by the rivers is in part derived from the ocean by means of the atmospheric transportation of this sub- stance from the ocean and its precipitation in rain water. Ten per cent. is allowed as a sufficient deduction for this circulation of the chloride of sodium. The allowance is thus restricted for the reason that while near the coasts a very considerable portion, and even sensibly the whole, of the chloride of sodium may be so derived, in inland areas the amounts of the salt which fall in rain become very minute.? It is just in these inland areas that the chief rivers of the world derive their supplies. Applying this correction to the NaCl of the rivers, the corrected river discharge of sodium is left at 15,542 x 10! tonnes. Corrections on the Numerator. (a) For the Original State of the Ocean.—We assume that the sodium as well as most of the metals was silicated in the original crust of the earth. The chlorine, with great probability, was gaseous and combined Society, vol, vii. (ser. ii.), 1899, p. 23 et seg. See also Geological Magazine, 4, 1900, vol. vii. et seq. ‘ «Challenger’ Report, Physics and Chemistry, vol. i. Scottish Geographical Magazine, 1895, p. 185. The measurements throughout have been converted from the British system of units. ® Loe. cit., 1888, p. 1 et seq. 4 Loe. cit., 1887, p. 76. 5 On the west and east coasts of Scotland 1:19 and 1:26 per 100,000 respectively. co valleys 0:25 to 0°76 per 100,000, and in Ootacamund, India, 0:04 per 376 REPORT—1900. with hydrogen. The resulting acid we assume as probably contained in the original atmosphere and hydrosphere. A primitive accelerated denudation can be computed on the basis of the probable mass of chloride of hydrogen and the nature of the lithosphere exposed to attack. The effects concern the present method only so far as they result in supplying sodium to the ocean. The maximum amount of chlorine available as an acid basis may be derived from. the chlorine now in the ocean less what was supplied during geological time by solution of the rocks. Referring to Sir John Murray’s table,' we deduce from the amounts of chlorides supplied annually by river discharge? (applying the deduction of 10 per cent. before mentioned to the sodium chloride) that the rivers contribute annually 75°5 x 10° tonnes of chlorine. If now our final esti- mate of the earth’s age is 95 x 10° years, the total supply by denudation has been 7169 x 10? tonnes of chlorine. The total mass of chlorine now in the ocean, calculated on Professor Dittmar’s table and the more recent estimate of the mass of the ocean (ante) less the amount calculated as above as supplied by the rivers sub- sequently, is 21,123 x 10!? tonnes.? This amount we assume free to act as a primeval denuding agent. According to Mr. F. W. Clarke‘ the older crust of the earth contained the following atomic percentages, which would be converted to chlorides by a primeval denudation such as we assume :— Percentage. | Percentage, Aluminium ; ; . 813 Magnesium . . 264 Jron . : : : Peat Potassium - * 213b Calcium . ‘ ; . 343 ; Sodium . : : . 2°68 Dividing among these the mass of chlorine already estimated, we find that the chlorine taken up by the sodium would be 6-7 per cent. of the whole. This would amount to 1415 x 10? tonnes, bringing 916°7 x 10°? tonnes of sodium into the primeval ocean. Deducting this amount from the mass of sodium now in the ocean leaves 14,694 x 10'!? tonnes to be accounted for by subsequent denuda- tion. Of the other acid-forming substances possibly present in the primeval atmosphere and ocean, sulphur and carbonic anhydride need alone be referred to. The sulphur was, however, probably only free in small amount, if at all, being present in the average igneous crust” to the extent of 0:06 per cent., and being to-day supplied by denudation in quantities more than suflicient to account for all in the ocean. Con- sidering that subdivision of its effects among the metals must also occur, an allowance is not called for. Carbonic acid is a relatively feeble and slow rock solvent. Even if Loe; crt. ? As follows in tonnes per cubic kilometre :— NaCl : ; . 3 . 4061 NELCI ag ‘ : ; : web Licl 3 é : : - 600 3 The chlorides now in the ocean are :— NaCl 4 6 , 39,703 x 10'* tonnes MgCl, 5642 x 10? tonnes * Bulletin, US. Geological Survey, 148, p. 13. ® Clarke, Joe, cit. ON THE GEOLOGICAL AGE OF THE EARTH. 377 present in the abundance thought by some, its early effects were probably compensated by the more active effects of organic acids of later times. Vegetation, too, has been a source of carbonic acid in the soils during subsequent periods. Jt may be observed that the fixation of free CO, by vegetation so abundantly in the later Paleozoic and the increase in the deposits of limestone rather point to a gradual fixation of this substance than to any special activity as a solvent in earlier times. On _ these accounts we make no correction for the possible presence of this substance in primeval times. Rock solution in heated waters persisted for periods relatively so short as to cause negligible error only. According to Lord Kelvin’s calculation as to the rate of cooling of the solidifying crust, a period of a century would have been adequate to cool the crust from its melting-point down to about 8° Centigrade above what it would be without any under- ground heat. Hence, if the mean rate of solvent denudation was as much as a thousand times what it is to-day, the result would have been the accomplishment of 100,000 years’ denudation in the first hundred years. If now we even lengthened the period of this excessive denudation, ten times the correction would be no more than about | per cent. (b) Lor Direct Marine Denudation.—So far as the sea has directly acted on the coasts, and on the sediments deposited in it, an error is in- troduced calling for a subtractive correction on our estimate of geological time ; in other words, upon our numerator, which is that part of the sodium in the ocean supplied by sub-aérial denudation only. The total tide-swept area of the ocean is calculated by Sir J. Murray and Professor Renard (‘Challenger’ Report) as 162 x10? square kilo- metres. The ‘rainy ’area of the land is about 113 x 10° square kilometres. The ratio of areas is 1 : 700. Hence, the assumption of a marine solvent denudation having an intensity twenty times that progressing over an equal area exposed to normal sub-aérial denudation would involve a sub- tractive correction of rather under 3 per cent. on geological time.! The solvent effects on sediments falling into the nearly, or quite, quiescent waters beyond this zone are assumed to be small on the grounds of the rapid flocculation and consolidation of marine sediments, as well as from the fact that the very minute mineral particles of oceanic sediments show little of such effects as would arise under conditions of sub-aérial denuda- tion. They preserve, in fact, their soda in substantial excess of their potash. There is in marine sediments generally almost complete absence of the more active acid and oxidising effects progressing in the soils. Nor will the state of consolidation of marine sediments allow us to assume anything like the enormous surface area, as much as 500 square metres per litre, exposed within the soils. On these grounds it is assumed that the correction should not exceed 6 per cent., nor be less than 3 per cert. Our numerator was left at 14,694 x 10!2 tonnes, and our denominator at 15,542 x10‘ tonnes. The resulting age of the earth would be 94 x 10° years. A subtractive correction of 4 per cent. for marine denudation leaves the geological age at 90x10° years. Future extension of our knowledge on the many points raised will, however, modify this number. Thus, according to Professor De Lapparent’s ? more recent estimation of ‘ See abstract of a paper read by the author before Section C, ‘Some Experi- ments on Denudation in Fresh and Salt Water,’ * Traité de Géologic, tome i. p. 60. ' 378 REPORT—1900, the volume of the ocean, its mass is 1:539 x10" tonnes. This would raise our result by nearly 6 per cent. We sum up the results of our inquiry, then, in the statement that the probable age of the earth, estimated from solvent denudation, is between ninety and one hundred millions of years. Rock-salt Deposits from the Ocean negligible. The amount of chloride of sodium in the ocean is sufficient to cover the entire land area with a layer of solid salt 122 metres deep. Compared with so great a mass the rock-salt deposits on the land are negligible. They are, moreover, only in part derived from the ocean, the circumstances leading to abstraction of salt from the ocean and its retention upon the land being exceptional. Likeness in chemical composition is no proof that bedded salts were derived from the ocean. Thus the proportions of salts in the Great Salt Lake are much the same as in the sea.! So far as these deposits are derived from the denudation of ‘rainless’ regions, and are being gradually conveyed by rivers to the ocean, they constitute part of the normal supply of sodium to the sea. Uniformity of sub-aérial Denudation. The uniformitarianism involved in the present mode of calculating the age of the earth is broadly restricted to the approximate persistence throughout the past of the present sub-aérial association of water and rock. The rate of solution of the rock-forming silicates is so slow that the abundance of the solvent or its rate of renewal is a relatively unimportant factor compared with the surface area exposed. Thus within certain limits climate will not seriously affect the question. The existence of a rainless area, amounting to one-fifth the land surface, subject to extreme conditions of dryness secures that subsidence or elevation of land does not necessarily involve corresponding changes in the area of active solvent denudation, In the first case the more active margin moves inwards, in the second case it moves outwards. The argument that the surface materials of the land areas must have been growing poorer in alkalies throughout geological time is met by the fact of the less resistent nature of sedimentary rocks, involving soils richer in soluble constituents. These are, in fact, more rapidly formed and removed. Observation shows that on comparing soils from the most diverse kinds of rocks the rapidly concentrated soils of limestones, or those derived from sandstones, very generally exceed in percentage of alkalies soils derived from igneous rocks.” It is within the soils that the chief work of solvent denudation is accomplished. Confirmation in the Soda-content of the Igneous and Sedimentary Rocks. We assume in our present argument necessarily that the sedimentary rocks were derived from the igneous in the process of denudation, a certain loss, representing matter gone into solution, occurring. Taking this loss into account, we may recover from the estimated mass of the siliceous detrital sedimentaries on the earth’s surface the approximate total mass of the parent igneous rock, This represents a certain mass of soda 1 Nature, December 28, 1899, p. 204. * E. G. Merrill, Rocks, Rock-weathering, and Soils (Macmillan), 1897, pp. 305, 306, 358, and 359, ON THE GEOLOGICAL AGE OF THE EARTH. 379 (deducible from our knowledge of the mean igneous rock-crust) which is to be accounted for between what is now represented in the ocean by the chlorides and what remains over in the detrital sedimentaries. Upon making the calculations, we find that the sum of the soda in the ocean and in the sedimentaries would nearly suftice to effect the full restoration of this constituent to the original rock. There is not quite enough. The bulk of the siliceous sedimentaries is assumed to be represented by a layer 1:77 kilometres deep spread over the land area. This on a specific gravity of 2-5 affords a mass of 64 x 10'° tonnes, which we assume to be 67 per cent. of the mass of the parent rock.? Hence the parent rock possessed a mass of 95:5x10!® tonnes. We restore to this the soda equivalent of the sodium now in the ocean, 210 x 1015 tonnes. The mean soda-content of these sedimentaries determined on the analyses of over one hundred typical siliceous sedimentary rocks given in Professor H. Rosenbusch’s Elemente der Gesteinslehre (Stuttgart, 1890) is found to be 1:47 per cent. This affords 9:4 10! tonnes in the layer 1°77 kilo- metres thick. Restoring this also, the parent mass of igneous rock is found to have possessed 3°20 per cent. of Na,O. According to Mr. F. W. Clarke (loc. cit.), the mean igneous rock contains 3°61 per cent. of soda. This approximate agreement between the amount of sodium in the ocean and that missing from the sedimentary rocks is a confirmation of the validity of the present mode of deducing the age of the earth. It is directly opposed to the assumption of an ocean primevally charged with sodium salts. The negation is the more emphatic, seeing that the loss revealed by the sedimentary rocks of geological time appears to be more than sufficient to account for what sodium is to-day in the sea, Plankton and Physical Conditions of the English Channel.—Second Report of the Committee, consisting of Professor E. Ray LaNKESTER (Chairman), Professor W. A. Herpman, Mr. H. N. Dickson, and M.. W. Garstang (Secretary), appointed to make Periodic Investi- gations of the Plankton and Physical Conditions of the Englhsh Channel during 1899. Tue series of periodic surveys for which provision was made at the Bristol and Dover Meetings has been completed by Mr. Garstang, under the same conditions as were described in the First Report of the Committee. Since the Dover Meeting two surveys were carried out, viz., in November 1899, and in the first week of March 1900, thus making five quarterly surveys altogether. It has been found impossible to finish the examination of the large quantity of material collected in time for report at the Bradford Meeting. The Committee therefore desire to be reappointed (without a grant) in order that they may present their final report at the Glasgow Meeting. 1 Merrill, doc. cit. pp. 209-225. 380 REPOkT—1900. Ozcupation of a Table at the Zoologicat Station at Naples.—Report of the Committee, consisting of Professor W. A. HERDMAN (Chairman), Professor E. Ray LanKester, Professor W. F. R. Wetpon, Professor S$. J. Hickson, Mr. A. Sepawick, Professor W. C. McIntosu, and Professor G. B. Howes (Secretary). APPENDIX, PAGE I. Note by the Chairman of the British Association Committee ; : . 381 Il. Leports on the Occupation of the Table " ‘ : é 383 a. The Anatomy of the Flatfishes (Heterosomata). By H. M. Kyun, M.A., B.Sc. . ; ‘ ; , : ; : : ‘ c . B83 b. The Structure of Certain Polychate Worms. By E.8.Goopricu, M.A. 384 c. Observations on Compound Ascidians. By Professor W. A. Herp- MAN, D.Sc., F.R.S8. : ‘ : E : / F ? : d. The Anatomy of Phyllirhot, the Calenterate Plankton, and certain Celenterata. By R.T. GUNTHER, M.A. . 3 i , 2 eOOO e. The Lertilisation Process in Echinoidea. By A. H. REGINALD 384 BULLER, Ph.D. . ; , , ; : : Rit ae : . B87 J. The Methods of Preservation of Specimens used at the Zoological Station. By Professor R. RAMSAY WRIGHT : ; . 388 IIL. List of Naturalists who have worked at the Zoological Station from + July 1, 1899, to June 30, 1900 ‘ : : 3 : ; ; - 389 IV. List of Papers published in 1899 by Naturalists who have occupied Lables in the Zoological Station d ; : 5 - : 2 . 9390 V. List of the Publications of the Zoological Station during the Year ending June 30, 1900 ; ‘ : A , ‘ 2 ; 392 ON entering upon the year’s occupancy of the Naples Table the advis- ability suggested itself of sending a circular letter to teachers and others likely to recommend workers ; and as the result a greater number of applications were received than it was possible to grant. Among those which were entertained no fewer than three ultimately overlapped during spring, and the best thanks of the Committee are hereby tendered to Dr. Dohrn for his magnanimity, exceeding all precedent, in having arranged for the accommodation of all workers recommended, this notwithstanding. The indebtedness of the Committee is further increased by his having, on their behalf, granted Professor Ramsay Wright, of the University of Toronto, permission to spend the leisure of two months’ residence in Naples in the study of the methods of capture and preservation in vogue in the bay, with a view to their application at the New Canadian Marine Station, the project for which received the support of the British Asso- ciation. And this has been further increased by his having allowed Miss A. Vickers to collect seaweeds between October and January, on the recommendation of the Committee. The list of British workers at the Naples Station which accompanies this Report exceeds, as regards numbers, all previous records, while that of naturalists of other countries reaches for the year seventy-four in all, bringing the total of those who have profited by the resources of the establishment since 1873-74, when Professor Waldeyer and the late Francis Maitland Balfour began work there, to nearly 1,200 persons. The recent addition to the laboratory of a filter, by which half the sea-water in circulation in the tanks is filtered and separated from — ae THE ZOOLOGICAL STATION AT NAPLES. 581 the rest, has materially increased the facilities for experimental work now greatly in vogue ; and the fishing capacity is now sufficient to provide from fifty to sixty workers at a time with all requisite material. In every department of the establishment, laboratory and library alike, thorough efficiency and complete success have to be recorded. Your Committee hereby apply for a renewal of the grant of 1002. to enable Mr. H. H. Stewart, M.A., to work at the Annelids, and to aid him and other competent researchers whom it is hoped to secure to study these and other organisms they may desire to investigate. Appended to the Report is a note by the Chairman of the Committee d propos of a visit to the Station and his own Report on the Occupancy of the Table. ; APPENDIX I. Note by the CuatrMan of the British Association Committee. As it is about ten years since a Chairman of this Committee visited the Naples Zoological Station, and reported on the condition of the insti- tution,! it may serve a useful purpose to draw attention here to the facili- ties for work at this world-renowned laboratory, and to the additions and improvements effected during the last decade. I am indebted to Dr. Dohrn, the Director, and to the Secretary, Mr. Linden, for much informa- tion given me during my recent visit. Since Dr. Sclater’s visit in 1890 additional accommodation has been obtained by a re-arrangement of the roof of the main building. This gives space for a second laboratory, a supplementary library, and various smaller rooms used as chemical and physiological laboratories, for photo- graphy and bacteriology. A good deal of the research in recent years, both on the part of those occupying tables and of the permanent staff, has been in the direction of comparative physiology, experimental embryo- logy, and the bacteriology of sea-water, and all necessary facilities for such work are now provided. The number of work-places, in some cases separate rooms, known technically as ‘ tables,’ is about fifty-five, and of these about thirty-four are rented annually by States, Universities, or Associations. Germany takes about ten of these, and Italy seven. There are three American tables, and three English (rented by the Universities of Cambridge and Oxford and the British Association respectively) ; consequently there are generally about half a.dozen English and American biologists at work in the station ; but Dr. Dohrn interprets in a most liberal spirit the rulesas to the occupancy of a table, and, as a matter of fact, during my recent visit there were, for a short time, no less than three of us occupying simultaneously the British Association ‘table,’ and provided with separate rooms. A work-table is really a small laboratory fitted up with all that is necessary for ordinary biological research, and additional apparatus and reagents can be obtained as required. The investigator is supposed to bring his own microscope and dissecting instruments, but is supplied with alcohol, acids, stains, and other chemicals, glass dishes, and bottles of various kinds and sizes, drawing materials, and mounting reagents, 1 Nature, February 1891, p. 392, 382 REPORT— 1900. Requisition forms are placed beside the worker on which to notify his wishes in regard to material or reagents, he is visited at frequent inter- vals by members of the staff, and all wants are supplied in the most perfect manner. The Staff of the station consists of :— 1. Dr. Anton Dohrn, the founder and director. 2. Seven scientific assistants—viz. Dr. Eisig, Administrator of the Laboratories ; Dr. Paul Mayer, Editor of the Publications; Dr. Gies- brecht, assistant editor and supervisor of plates; Dr. Gast, assistant editor and supervisor of microscopic drawings ; Dr. Schobel, Librarian ; Dr. Lo Bianco, administrator of fisheries and préparateur ; Dr, Hollands, temporarily in charge of the microscopic sections department—all of them well-known men, each eminent in his own line of investigation. The post of assistant in the Physiological Department, formerly held by the late Dr. Schoenlein, is now vacant ; and in addition to the foregoing there are :—Secretary, Mr. Linden ; two painters, and the engineer ; with attendants, collectors, and others employed in the laboratories, in the collecting and preserving departments, Aquarium, and elsewhere. This seems at the first thought a very large staff, but the activities of the institution are most varied and far-reaching, and everything that is undertaken is carried to a high standard of perfection. Whether it be in the exposition of living animals to the public in the wonderful tanks of the ‘ Acquario,’ in the collection and preparation of choice specimens for Museums, in the supply of laboratory material and mounted microscopic objects to Universities, in the facilities afforded for research, or in the educational influence and inspiration which all young workers in the laboratory feel in each and all of these directions, the Naples station has a world-wide renown. And the best proof of this reputation for excel- lence is seen in the long list of biologists from all civilised countries who year after year obtain material from the station or enrol as workers in the laboratory. Close on 1,200 naturalists have now, since the opening of the Zoological Station in 1873, occupied work-tables, and as these men have come from and gone back to practically all the important laboratories of Europe and America, from St. Petersburg to Madrid, and from California to Japan, Naples may fairly claim to have been for the last quarter-century a great international meeting-ground of biologists, and to have exercised a stimulating and co-ordinating influence upon biological research which it would be difficult to over-estimate. The opportunities for taking part in collecting expeditions at sea are most valuable to the young naturalist. Dredging, plankton-collection, and fishing are carried on daily in the Bay of Naples by means of the two little steamers belonging to the station, and a flotilla of fishing and other smaller boats. Many of the Neapolitan fishermen are more or less in the employ of the station, or bring in such specimens as they find in their work. But although the work of the Naples Zoological Station is thus many- sided, the leading idea is certainly original research. An investigator goes to Naples to make some particular discovery, and he goes thither because he knows he will find material, facilities, and environment such as exist nowhere else in the same favourable combination. The British Association Committee consider it most important that these opportunities for research should be open to British biologists in the future as they have THE ZOOLOGICAL STATION AT NAPLES. 383 been in the past, and it is on this ground that they confidently recom- mend the policy of sending selected investigators to Naples each year— a practice which has led to such satisfactory results in the past and is full of promise for the future. APPENDIX I. REPORTS ON THE OCCUPATION OF THE TABLE. Report on the Occupation of the British Association Table at Naples, Jrom October to December 1899-1900. a. The Anatomy of the Flatfishes (Heterosomata). By H. M. Kyi, M.A., B.Sc. During the period, from October to the third week in December, 1899, when I had the privilege of occupying the British Association Table at Naples, the special research which engaged my attention was the Anatomy of the Flatfishes (Heterosomata). The species examined there were the following :— Citharus linguatula, L. | Solea lascaris, Risso. Rhomboidichthys mancus, Risso. | (Solea Kleinit), Arnoglossus Grohmanni, Bon. | Solea ocellata, L. Arnoglossus laterna, Walb. | Microchirus variegata, Don. Lepidorhombus Boscii, Gtr. | Microchirus minuta, Parn. Scophthalmus unimaculatus, Risso. | Monochirus hispida, Cos. Rhombus maximus, Kl. | Ammopleurops lacteus, Gtr. Solea vulgaris, Quens. 7 In addition to the above, through the courtesy of the Naples staff, I was able to examine several species of other families of the Teleosts, as well as the eggs, larvee, and young of fishes to be found at that season. The main conclusions arrived at have been embodied in a paper entitled : ‘On the Classification of the Flatfishes (Heterosomata),’ which is in process of publication in the Scottish Fishery Board’s Report for 1899. In this paper it is shown that Citharus linguatula, a species very common in the Mediterranean, is a transitional form between the Halibut and Turbot groups of Flatfishes. The characters employed as tests of relationship are chiefly the position and structure of the ventral or pelvic fins, the position and structure of the olfactory organs, and the position of the eyes. Further, although C7tharus is the only form in European waters which marks the transition between these two main groups, the American fauna possesses many similar forms, and the classification has therefore been altered in order to include these within one group or subfamily. It is also shown how the various subfamilies of the Flattishes are restricted to fairly well-marked zones of distribution. In conclusion, I wish to offer my best thanks to the Committee of the British Association for the opportunity granted me of pursuing my studies at Naples, and also to the authorities of the station for their kindness and courtesy. 9 (oe) te REPORT—1900. Report on the Occupation of the Table in the Zoological Station at Naples, during part of December 1900. b. The Structure of certain Polychete Worms. By E. 8. Goopricu, M.A. O.von. During a short visit to Naples last winter, I occupied the Table of the British Association at the Zoological station. I have to thank the Committee for this opportunity of continuing my researches on the structure of Polychxete worms. My observations were restricted almost entirely to the study of living specimens of Alciopids, Phyllodocids, Polygordius, and Saccocirrus, A considerable amount of material was also preserved for future use. The nephridia of the Alciopids were found to closely resemble those of the Phyllodocids, having no internal ccelomic opening, and being pro- vided with bunches of flagellated cells, the solenocytes. The genital products are carried to the exterior by ciliated genital funnels, which at maturity open into the nephridial ducts. A detailed description of these organs is about to be published in the ‘Quart. Journ. of Micr. Science.’ Some details were also added to our knowledge of the nephridia of Polygordius ; and the structure of the interesting, but little known, Saccocirvus was carefully investigated. The results of this study, which is not yet completed, will, I hope, shortly be ready for publication. Report on the Occupation of the British Association Table at Naples during March and April 1900. c, Observations on Compound Ascidians. By W. A. Herpman, D.Sc., F.R.S. I occupied the British Association Table for a little over three weeks in March and April, 1900, with the object of examining in the living condition certain Mediterranean Compound Ascidians. Probably the first thought that occurs to any one who has worked at the Naples Zoological Station, on recalling the time he spent at that celebrated laboratory, is one of gratitude to Dr. Dohrn and his excellent assistants for their personal kindness and help, and of admiration for their highly efficient administration. I feel that if other workers desire to express their gratitude, I especially should do so, for it is probable that I gave unusual trouble at a busy period, and it seemed to me that I was treated with exceptional kindness. In addition to Dr. Dohrn, I desire to thank especially Dr. Eisig and Dr. Lo Bianco. With the latter I was brought largely into contact by the nature of my work. During the recent short visit, my intention was mainly to see and examine as many species and specimens of Compound Ascidians as possible in the living condition, and then have them killed and preserved for histological work later. I was given excellent facilities for collecting in the small steamer Johannes Miiller, belonging to the station, and twice —sometimes three times—every day fresh supplies of material, brought in by the fishermen, were placed in my aquaria. ; The Compound Ascidians of the Bay of Naples have not yet been monographed. Some species were described by Delle Chiaje and others long ago, when the genera were iitiperfectly known and anatomical characters were not recorded. Other species have been briefly diagnosed more recently (but without any figures) by Della Valle. It is now almost impossible in many cases to tell from these descriptions alone which of THE ZOOLOGICAL STATION AT NAPLES. 385 the Mediterranean species agree with those of the French coast described by H. Milne-Edwards, Giard, and Lahille, and with our British species. I_ wished, therefore, to compare these published, but sometimes in- sufficient, descriptions with living specimens from the original localities in order to determine, if possible, the systematic positions of the species and provide myself with figures and anatomical details for comparison with British species. Fortunately, also, I found that Dr. Lo Bianco had in his stores a few of Della Valle’s type specimens, or at least specimens of these species identified and labelled by Della Valle himself. These I was permitted to draw and examine. In regard to the other species, of which there were no authenticated specimens, I soon found that from the large number of examples they laid before me L was able in most cases to determine what form the original describer had before him. I then made coloured drawings of that form and examined its anatomy to settle to which modern genus it belonged, and samples of every species I examined and drew were preserved for histological purposes. In this way I hope I have secured the material necessary for an accurate comparison of a number of the Mediterranean and British species. I have brought back over thirty sheets of coloured figures, and Dr. Lo Bianco is sending a collection of bottles to Liverpool. The following is a list of the species ' I examined and determined when at Naples :— ASCIDL4 COMPOSIT A. I.—MEROSOMATA. Fam. 1.—DisToMIp™. | Leptoclinum maculatwm, M.-Edw. Distomum coste, Della Valle coccineum, V. erystallinum, Ren. Drasche 4 pancerii, Della Valle perforatum, Giard Cystodytes della-chiajie, Della dentatum, Della Valle Valle Distaplia magnilarva, Della Valle Sulgens, M.-Edw. rosea, Della Valle candidum, Della Valle Fam. 2.—POLYCLINID&. conumune, Della Valle Circinalium concrescens, Giard Amaroucium rosewm, Della Valle erystallinum, Ren. Aplidium gibbulosum, Sav. Fragarium areolatum, D.Ch. gelatinosum, Giard exaratum, Grube Fam. 4.—DIpPLosoMID&. Fam. 3.—DIDEMNID#. Diplosoma crystallinum, Giard Didemnum bicolor, V. Drasche Pseudodidemnum listerianum, gelatinosum, Giard M.-Edw. cereum, Giard Astelliwm spongiforme, Giard IT.—Ho.osomata, Fam. 1.—BorryLiip”. Polycyclus renieri, Lamk. Botryllus tapetum, Della Valle | Botrylloides luteum, V. Drasche | rubrum, M.-Edw. morio, Giard : : aurolineatus, Giard gascot, Della Valle ' To complete the record the few simple Ascidians which were brought to me with the compound, and which I examined, have been included. cc 386 REPORT— 1900, ASCIDIA) SIMPLICES. Fam. 1.—CLavVELINID&. | Ciona intestinalis, L. ; ‘ J | Phallusia mammillata, Cuv. Clavelina lepadiformis, O.F.M. | Diazona violacea, Sav. | Fam. 3.—Cynrup2. Rhopalea neapolitana, Phil. | Cynthia dura, Heller Microcosmus vulgaris, Heller | Styela canopoides, Heller | Polycarpa glomerata, Alder | Forbesella tessellata, Forbes Fam. 2.—ASscIDIIDA. Ascidia mentula, L. Report on the Occupation of a Table at the Zoological Station at Naples during March and April 1900. d. The Anatomy of Phyllirhoé, the Celenterate Plankton, and certain Celenterata. By R. T. Ginter, M.A., Maydalen College, Oxford. The Committee of the British Association permitted me to use the Table hired by the British Association during the summer months of the present year, for the prosecution of certain researches on pelagic organisms in which I have been for some time and am at present engaged. Since it was inconvenient for me to work at Naples during the months of May and June, I was, by the generous courtesy of the Director of the Zoological Station, permitted to commence the occupation of the Table during my Easter vacation at a time when the resources of the station are very severely taxed by the great concourse of zoologists who annually assemble there at that season. For this especial act of kindness, in addition to so many others I have been shown by Dr. Dohrn, I desire to offer my hearty thanks. The Table of the British Association was occupied by me for about a month—between March 24 and April 25, 1900. My attention was principally devoted to a detailed study of the anatomy of Phyllirhoé and to a daily examination of the Ccelenterate portion of the plankton of the bay. The general character of the latter was very similar to what it was on a former occasion when I had the good fortune to examine it, but owing to the prevalence of westerly winds during parts of March and April, an unusual quantity of Velella and Physalia appeared in the bay. All along the sandy foreshore of Cuma, which is open to the west, sea and beach were remarkably delimited by Velelle extending as a blue band about a foot or so broad and many miles in length. In consequence, too, of the same prevailing winds Physalia, which is extremely rare at Naples, and which has not been taken for twelve years, as I am informed by my friend Cay. Lo Bianco, appeared in great numbers, and was probably drifted in from the Atlantic as a con- sequence of the exceptional meteorological conditions. I availed myself of the opportunity of verifying the statement that the characteristic blue colouring-matter of Velella (zoocyanin) may be very conveniently extracted from the tissues by maceration in a saturated solution of potassium acetate. A solution prepared on March 26, which has been kept in the dark, still retains its blue colour, and will be sub- mitted to spectroscopic examination on my return to England. As the result of the action of the potassium acetate, the ‘yellow cells’ or sym- biotic alge, which are yellow in the tissues of the Velella, turn green. In several of the species examined the arrangement of these yellow cells was in groups of 2, 4, 8, or other multiples of 2. THE ZOOLOGICAL STATION AT NAPLES. 387 Among other observations upon Celenterata, I have observed the -existence of a continuous longitudinal strip of cells with granular proto- plasm situated in the ectoderm and extending along one side ot the tentacles of certain Hydrozoa. I have demonstrated the existence of this band of cells in the tentacles of the medusz of Carmarina and in those of the hydropolyps of Obelia, Hudendriwm, and Aglaophenia, and I have no doubt that it can be demonstrated in other genera also. This band -of specialised cells can be made obvious by keeping the living animals for some time in sea-water tinted by methylene blue in the proportion recom- mended by Zoja.!_ It was found that certain cells along one side of the tentacles became stained, thus demonstrating the existence of the above- mentioned band of differentiated histological elements. I was enabled to make very considerable progress with my work on the anatomy of Phyllirhoé, and to make several observations on the living animal, which I hope to publish before the close of the present year. Report on the Occupation of a Table at the Staxione Zoologica, Naples, during March and April 1500. e. The Fertilisation Process in Echinoidea, By A. Ti. Reetnarp BuxiEr, PA. D. I occupied the table of the British Association from March 15 until April 21. The research work undertaken was an endeavour to determine whether ‘the eggs of the Echinoidea excrete a fluid which attracts the spermatozoa chemotactically. Bergh? states that attraction by a special substance is probable. According to Strasburger * the eggs of the /ucacee (which are also fertilised after being set free in sea-water) excrete a substance which attracts the spermatozoa from a distance equal to about two diameters of an egg, The material consisted of the following animals :—Arbacia pustulosa Gray, Echinus microtuberculatus Blv., and Spherechinus granularis Ag. No attraction could be observed during artificial fertilisation experi- ments. Coliections of spermatozoa, however, take place in the outer gelatinous coat of the eggs. Observations were made tending to show that this is a physical and not a chemotactic phenomenon. Experiments were then made in which it was sought to collect in sea- water the supposed fluid excreted from the eggs. The eggs were left very thickly placed together for 2-12 hours in a very shallow layer of sea-water, and the latter, after filtration, introduced by means of an air-pump into capillary glass tubes. These were then placed in a drop containing motile spermatozoa. No gathering of the spermatozoa into the tubes could be observed. One precaution taken was to prove that just before filtration the eggs could be fertilised. In the case of Arbacia it was discovered that when spermatozoa are introduced into a drop containing freshly extruded eggs they collect into small balls, often composed of 100 or more individuals. The balls were also formed after the water had received four successive filtrations. A tactile stimulus appears to play a part in the phenomenon. ' In his experiments on Hydra, Rend. Inst. Lomb. xxv. 2 Vorlesungen iiber allgemeine Embryalogie, 1895, p. 43. * Das botanische Practicum, 2te Aufl. 1887, p. 402. ecz2 388 REPORT—1900. When a suflicient number of spermatozoa have penetrated the gela- tinous coat of an egg and have become attached by their heads to the layer which is subsequently raised and forms the vitelline membrane, rotation of the egg takes place. During the rotation, which may be in any direction, the gelatinous coat does not also rotate. By means of the capillary tube method an attempt was made to find some substance which attracts the spermatozoa. Various substances, known to give a chemical stimulus to other organisms, were tested : meat extract, peptone, cane-sugar, glycerine, asparagine, alcohol, oxalic acid, nitric acid, potassium nitrate, sodium chloride, potassium malate diastase, and distilled water. No definite chemotactic attraction could be observed in any case. The chief results arrived at were :— 1. The spermatozoa of the Hchinoidea are not attracted to the eggs by means of any special substance excreted by the latter. The vast number of spermatozoa and the large size of the eggs are sufticient to ensure the necessary contact taking place. ‘ 2. It is not improbable that the spermatozoa are unable to respond to chemical stimuli by change in the direction of movement. It gives me much pleasure to acknowledge my indebtedness to the staff of the Stazione Zoologica for supplying me with material and apparatus during the research. feport on the Occupation of a Table at Naples. ?. The Methods of Preservation of Specimens used at the Zoological Station. By Professor R. Ramsay WRricHt. In answer to my request that I might be permitted to avail myself of the arrangement existing between the British Association Committee and the Naples Zoological Station, the Secretary of the Committee was good enough to recommend me to the kind offices of the Director, Dr. A. Dohrn. Although the British Association Table was already occupied, I found Dr. Dohrn anxious to make special arrangements for my accommodation, and I accordingly took advantage of these from December 20 till the end of February. My object being to familiarise myself with the methods in use at the station, as well as with the Naples fauna in a living condition, I was installed in a room adjacent to that of Dr. Lo Bianco. Thanks to his intimate and extensive faunistic knowledge and to his untiring willingness to impart the results of his long experience in the conservation of marine animals, I felt at the close of my ten weeks’ stay more than satisfied with the results I attained. As Dr. Lo Bianco was engaged at the time in giving instruction in methods to a medical officer of the German Navy, I was enabled to share these demonstrations and to acquire some expertness in dealing with those forms which, like the Siphonophora, had long proved refractory to attempts at preservation until Dr. Lo Bianco succeeded in elaborating the methods at present in use. I hope to be able in the near future to utilise the technical experience gained at the New Canadian Marine Laboratory which has recently been brought to the notice of the British Association. THE ZOOLOGICAL STATION AT NAPLES. 389 While expressing my thanks to your Committee, as well as to Dr. Dohrn and the various members of the staff of the Zoological Station, for the many courtesies shown me, I desire to record my opinion of the high efficiency of the station and of the convenience to British naturalists incident to the partial support thereof by the British Association. APPENDIX III. A List of Naturalists who have worked at the Zoological Station from July 1, 1899, to June 30, 1900. j i Num- State or University ber on Naturalist’s Name whose Table List was made use of 1109 | Dr. F. Capobianco Italy 1110 | Prof. F. 8. Monticelli = a 1111 | Dr. Paul Juge . Switzerland 1112 | Prof. G. Corrado Italy 1113 | Dr. Sabussow . Russia 1114 | Prof. F. Sanfelice Zoolog. Station 1115 | Dr. E. Germano 1116 | Prof. A. Russo . Italy 1117 | Dr. F. Mazza . 3 1118 | Dr. E. Crisafulli oe j : | 1119 | Dr. G. Bottaro . Zoolog. Station 1120 | D. A. De Simoni - s 1121 | Dr. J. Sobotta . Prussia 1122 | Dr. F. Bottazzi. Italy 1123 | Dr. P. Enriquez 1124 | Dr. K. Reuter . Prussia : 1125 | Mr. F. B. Sumner University Table 1126 | Dr. H. Driesch . Hambure 1127 | Dr. C. Herbst Prussia 1128 | Mr. KE. Gurney . Oxford 1129 | Miss A. Vickers British Assoc iation . 1130 | Dr. F. Nissl Baden 1131 | Prof. A. Biedl . Austria 1132 | Mr.H. Kyle. British Association . 1133 | Miss S. Nichols American Women’s Table 1134 | Dr. H. Waldow . Zoolog. Station 1135 | Prof. Taschenberg Prussia . 1136 | Dr. v. Lingelsheim ” : . . 1187 | Miss E. Gregory American Women’s Table 1138 | Prof. F. Cavara Italy 1139 | Dr. Rina Monti ” 1140 | Dr. M. Pierantoni ” : 1141 | Mr. W. Cooper Cambridge : 1142 | Mr. E. Goodrich British Association and Oxford 1143 | Prof. Ramsay Wright | British Association. 1144 | Dr.G. Jatta Zoolog. Station 1145| Dr. G. Vastarini Italy Cresi 1146 | Dr. V. Diamare ” | 1147 | Dr. G. Tagliani 3 1148 | Prof. T. D’Evant Dee ation of Occupancy Apel Denies e July 1, 1899 ” 2, ” ” 14, ” ” 22, ” ” 23, ” 9 24, » Aug. 4, ,, ” 10, ” ” 11, ” ” 15, ” ” 15, ” ” 24, ” Sept. iF ” ” 6, ” ” 8, ” ” 20, ” » 25, 55 Ochriienes ” 7; ” ” 9, ” » 13, 45 ” 23, ” » 24, 5, ” 25, ” ” 27, ’ NOVA 2 ” WG ” ” 22, ” ” 29, ” Deca lt 5 ” 4, ” ” 14, ” ” 17, ” ” 18, ” » 19, Jan. 1, 1900 ” 1, ” ” 1, ” ” 1, ” 1 Nov. 15, 1899 Aug. 21, ,, ” 21, ” Nov. 4; ° 4; ”» 1 ’ ” Sept.14, Nov. 4, ,, | Oct. 22, , | » 29, » ” 29, ” ” 28, Nov. 3, May 24, ” ’ ” Jan. 14, ,, ” 6, ‘) Dec. 19, 1899 ” 17, ” June 8, 1900 Mars. <5 Dec. 1, 1899 Mar. 1,1900 June 8, ,, Syu0) REPORT—1900. A List oF NATURALISTS—continued. ee: " | Num- State or University | ber on Naturalist’s Name whose Table List | was made use of 1149 | Dr. A. Romano Italy 1150 | Dr. G. Rossi 1151 | Dr. H. Redeke . Holland . 4 1152 | Dr. V. Heiser Smithsonian Table ; 1163 | Dr. H. Przibram Austria | 1154 | Dr. O. v. Fiirth. Strassburg 1155 | Miss H. Snowden American Women’s Table 1156 | Dr. B. M. Duggar Smithsonian Table . 1157 | Dr. G. Senn Switzerland 1158 | Cand. T. Bergmann . Prussia | 1159 | Dr. H. Winkler Wiirtemberg 1160 | Dr. O. zur Strassen . | Saxony 1161 | Dr. A. Buller British Assoviation . 1162 | Dr. R. Hoffmann Prussia 5 1163 | Dr. R. Woltereck Saxony . 5 1164 | Mr. C. F. Hottes . | University Table 1165 | Prof. Zimmermann . | Switzerland 1166 | Prof. Herdman British Association . 1167 | Dr. J. Sobotta . Bavaria 1168 | Mr. R. Giinther British Assoc iation . 1169 | Dr. W. Magnus Hesse 1170 | Signa. C. Losito Italy 1171 | Dr. M. Bedot Switzerland 1172 | Prof. Ballowitz. . | Prussia 1173 | Dr. T. H. Ashworth . | Cambridge a 1174 | Sir Ch. Eliot! . British Association . 1175 | Prof. D. Carazzi Italy 1176 | Dr. P. Cerfontaine | Belgium . 1177 | Herr H. Fischer | Wiirtemberg 1178 | Dr. 8. Mollier . Bavaria . : 1179 | Prof. T. H. Morgan . | Smithsonian Table . 1180 | F. B.Sumner . University Table 1181 | Stud. C. de Dawydoff Russia 1182 Dr. J. Boeke | Holland . | | | Duration of Occupancy Arrival Departure Jan. 1, 1900 — ” 1, ” aa 6; 5 |) M8900 ” fy yy et 3 21, 5, | euHellbe By BO} ti55 April 3, ,, Hep: 1; 5; Mar. 29, ,, ” 27, ” | Apr. 9, ” ” 27, ” ” 3, ” Mar. 3, 5, » 25, 5 ” By" 95 a Maeda pes aes a yy ” 20,.1)5, ” As ” ” 22, ” yy LS 5 ” 19, ” ” 15, ” ” 20, ” 5 ekGsiy sy? .| Mai 4, LOS <5) | Soraya ” 19, ” ” 9; ” » 21, 5 » 19, 55 ” 23, ” ” 26, ” ” 24, ” ” 3, ” ” 24, »” ” 27, ” ” 27, ” ” 27, ” Apr 4, ” Pe le icy ” 4, ” June 16, ” ” 11, » | Apr. 18, 5, a, liens | a May .-2;. 55°-4 _— ” ly ” ] June 8, ” ” 20, ” ae | Junelb, ,, | — ” 20, » | Ys ” 22, ” | ir 22, — APPENDIX IV. A List of Papers published in 1899 by Naturalists who have A. Fischel G. Jatta H. Driesch occupied Tables in the Zoological Station. Ueber vitale Fiirbung von Echinodermeneiern wahre nd ihrer Entwickelung. Anat. Hefte, Abth. 1, Bd. 11, 1899. Sopra alcuni Cefalopodi della Vettor Pisani. Nat. Napoli,’ vol. 12, 1899. 1 Cf. last year’s Report. Die Localisation morphogenetischer Vorginge. Entw.-Mech. Bd. 8, 1899. ‘Boll. Soc. Arch. fiir tle H. Driesch J. Ognetf R. Hesse 8. Garten H. L. Jameson S. Metalnikoff B. Solger L. Schultze Th. Pintner G. Mazzarelli. J. von Uexkiill Th. Beer . A. Bethe F. Schiitt P E. Albrecht G. Bitter ” YV. Diamare ” F. Bancroft G. Schneider . M. Nordhausen H. M. Vernon THE ZOOLOGICAL STATION AT NAPLES. 391 . Quantitative Regulationen bei der Reparation der Tubu- laria. Ibid. Bd. 9, 1899. Notizen tiber die Auflésung und Wiederbildung des Skelets von Echinodermenlarven. did. . Prof. Gilson’s Cellules musculo-glandulaires. Biol. Cen- tralblatt, Bd. 19, 1899. Untersuchungen iiber die Organe der Lichtempfindung bei niederen Thieren. V. Die Augen der polychaeten Anneliden. Zeitschr. f. wiss. Zoologie. Bd. 65, 1899. Beitriige zur Physiologie des electrischen Organs der Zitterrochen. Centralbl. f. Physiologie, Bd. 13, 1899, and Abh. Sichs. Ges. Wiss., Bd. 25, 1899. Thalassema papillosum, a forgotten Echiuroid Gephyrean. ‘ Mitth. Zool. Station, Neapel,’ Bd. 13, 1899. Das Blut und die Excretionsorgane von Sipunculus nudus. Lbid. Mauthner’sche Fasern bei Chimaera. Morphol. Jahrbuch, Bd. 27, 1899. Zur Kenntnis des Gehérorgans von Pterotrachea. Schr. Naturf. Gesellsch., Danzig, Bd. 10, 1899. Die Regeneration des Ganglions von Ciona intestinalis. Jen. Zeitschr., Bd. 33, 1899. . Nectonema agile Verrill. Akad. Anzeiger, No. 10, Akad. Wiss. Wien, 1899. Intorno al tubo digerente ed al ‘centro stomato-gastrico ’ delle Aplisie. Zool. Anz., Bd. 22, 1899. Die Physiologie der Pedicellarien. Zeitschr. fiir Biologie, Bd, 37, 1899. Die Physiologie des Seeigelstachels. bid. Bd. 39, 1899. Vergleichende physiologische Studien zur Statocysten- function. II. Versuche an Crustaceen. Archiv f. d. ges. Physiologie, Bd. 74, 1899. Die Locomotion des Haifisches (Scyllium) und ihre Bezie- hungen zu den einzelnen Gehirntheilen und zum Laby- rinth. Jbid. Bd. 76, 1899. Centrifugales Dickenwachsthum der Membran und extra- membrandses Plasma. Jahrb. Wiss. Botanik. Bd. 33, 1899. . Untersuchungen zur Structur des Seeigeleies. Sitz. Ber. Ges. Morph. Phys. Miinchen, Bd. 14, 1899. Zur Anatomie und Physiologie von Padina pavonia. Berichte D. Botan. Ges., Bd. 17, 1899. Zur Morphologie und Physiologie von Microdictyon umbili- catum. Jahrb. Wiss. Botanik, Bd. 34, 1899. Studii comparativi sulle isole di Langerhans del Pancreas. Internat. Monatschrift f. Anat. und Physiol., Bd. 16, 1899. Sul valore anatomico e morfologico delle isole di Langer- hans. Anat. Anzeiger, Bd. 16, 1899. A new function of the vascular ampullz in the Botryllide. Zool. Anzeiger, Bd. 22, 1899. . Ueber Phagocytose und Excretion bei Anneliden. Zeit- schr. Wiss. Zool., Bd. 66, 1899. . Zur Anatomie und Physiologie einiger rankentragender Meeresalgen. Jahrb. Wiss. Botanik, Bd. 34, 1899. The death temperature of certain marine organisms. Jour- nal of Physiology, vol. 25, 1899. The effect of staleness of the sexual cells on the develop- ment of Echinoids. Prec. Royal Soc., vol. 65, 1899. 342 REPORT—1900. A. Beck. , ’ . Ueber die bei Belichtung der Netzhaut von Eledone mos- chata entstehenden Actionsstréme. Archiv f. d. ges. Physiologie, Bd. 78, 1899. C, Herbst : 4 . Ueber die Regeneration von antennendhnlichen Organen an Stelle von Augen. JIJ. and IV. Archiv f. Entw. Mech., Bd. 19, 1899. W.Stempell . ; . Zur Anatomie von Solemya togata Poli. . Zool. Jahrb. Spengel, Abth. Anat. u. Ontog., Bd. 13. W. Lindemann 4 . Ueber einige Eigenschaften der Holothurienhaut. Zeit- schr. f. Biologie, Bd. 39, 1899. F. ROhmann . ‘ . Ejinige Beobachtungen tiber die Verdauung der Kohlen- hydrate bei Aplysien. Centralblatt f. Physiol., 1899. EB. Kiister : : . Gewebespannungen und passive Wachsthum bei Meeres- algen. Sitz. Ber. Akad Wiss. Berlin, 1899. F. Bottazzi . - . Ricerche fisiologiche sul sistema nervoso viscerale delle Aplisie e di alcuni Cefalopodi. Rivista Scienze Bio- logiche. Vol. 1, 1899. APPENDIX V. A List of the Publications of the Zoological Station during the year ending June 30, 1900. 1. Fauna und Flora des Golfes von Neapel.’ Asterocheriden, by W. Giesbrecht. 216 pp., 11 plates. 2. ‘ Mittheilungen aus der zoologischen Station zu Neapel.’ Vol. xiv. parts 1 and 2, with 10 plates. 3. ‘ Zoologischer Jahresbericht’ for 1898. 4. ‘Guide to the Aquarium.’ A new German edition has been published. Index Animalium.—Report of the Committee, consisting of Dr. HENRY Woopwarp (Chairman), Mr. W. E. Hoy.e, Mr. R. McLacauan, Dr. P. L. Scuater, Rev. T. R. R. STeppina, and Mr. F. A. BATHER (Secretary). THE Committee has the honour to report that this work has made very satisfactory progress in the hands of Mr. C. Davies Sherborn, and that the literature down to the year 1800 has now been sought out and indexed. The manuscript of this portion will be ready for the printer in a few weeks, and the Committee is considering the best form of publication and estimating the cost. Meanwhile the indexing of literature after 1800 is being continued. At this stage the Committee would be glad to receive suggestions or offers of help for the publication of this great work, since the sums hitherto so generously awarded to it are only sufficient for the necessary current expenses, which continue as before. The Committee therefore earnestly requests its reappointment, with a grant of 100/. ON NATURAL HISTORY AND ETHNOGRAPHY|OF MALAY PENINSULA. 393 Natural History and Ethnography of the Malay Peninsula. Report of the Committee, consisting of Mr. C. H. REap (Chairman), Mr. W. CROOKE (Secretary), Professor A. MAcaLIsTerR, and Professor W. RIDGEWAY. THE Geaimitice have received the following report from Mr. W. W. Skeat, the leader of the expedition :— Report on Cambridge Exploring Expedition to the Malay Provinces of Lower Siam. Drawn up by W. W. Skat. This expedition was organised to carry out a scientific survey, in which Ethnology, Zoology, Botany, and Geology should all have a share, of the little-known Malay provinces of Lower Siam, and especially to extend the scope of the ethnographical collections and observations referred to in the Fourteenth Annual Report of the Antiquarian Committee to the Senate (June 6, 1899). The party comprised Messrs. R. Evans, of Jesus College, Oxford ; F. F. Laidlaw, of Trinity College, Cambridge; D. T. Gwynne-Vaughan, of Christ’s College, Cambridge ; R. H. Yapp, of St. John’s College, Cambridge ; N. Annandale, of Balliol College, Oxford, and myself. The inhabitants of these provinces are, for the most part, Malay, but Siamese influence becomes gradually predominant to the northward, and the process of fusion between these two antagonistic elements presents ‘some curious racial problems. But the most interesting subject for investigation in these provinces is perhaps presented by the very primitive jungle tribes of the interior, about whom much valuable information was obtained. Yet another interesting tribe, of whom no account seems to have yet been published, is the sacred tribe of the Prams, who claim to have come over from India, and to have established themselves in the country anterior to the coming of the Siamese or Malays. What truth there may be in their statements will (it may be hoped) now be ascertainable, as a copy of their sacred book, containing an account of their origin, was obtained by the expedition. But the special interest of the territories traversed centres, perhaps, in ‘the fact that they have hitherto formed a species of ethnical backwater, but little, if at all, affected by the ideas of a higher civilisation. These ideas, however, are already taking root, and many of the manners and customs witnessed by the expedition are becoming obsolescent or are already obsolete. Tt is hoped that when the results are known the present expedition will be found to have achieved results to some extent comparable with those obtained by the important expedition sent by the Dutch Government to Mid-Sumatra in 1877-9. The results obtained should also be of value, for purposes of comparison, with the results of the very successful Cambridge Anthropological Expedition of Dr. Haddon to the Torres Straits, Sarawak, and New Guinea. Owing to the uncertainty as to the probable reception which the expedition would experience at the hands of the inhabitants, the good offices of the Siamese Government were bespoken by the Foreign Office ; 394, REPORT—1900. and I have much pleasure in recording the extreme hospitality and enlightened help which the expedition consequently received from the local authorities, in some cases, perhaps, under rather difficult circumstances. The warmest thanks of those interested in the expedition are due to- H. EK. Phya Sukhum, the High Commissioner for the Ligor Circle of the: Siamese-Malay States ; to Luang Phrom and Kun Rat, the special com- missioners attached to the expedition as escort ; to the Commissioners and Rajas of Patalung, Singora, Patani, Raman, Jala, Jering, Nawng Chik, Ligeh, Teluban, and Kelantan, the Sultan of Kelantan, the Sultan of Trengganu, and the Sultan and Raja Muda of Kedah. We reached Singora on March 27, 1899, and were most hospitably entertained in his own house by the High Commissioner, H. E. Phya Sukhum. Next day we proceeded up the Inland Sea. This is a very shallow lake, or, perhaps, rather chain of lakes, part of which is salt and part fresh water. It measures, roughly speaking, some sixty miles in length, and in the broadest part is not less than twenty miles wide. Some: dredging was done here by Messrs. Evans and Annandale, and the Bird’s Nest Islands were visited, observations made, and photographs taken of the curious cave-dwellings of the island guards. At Lampam (Lumpumm) a short stay was made by Messrs. Evans and 7aughan, Mr. Annandale and myself proceeding into the interior to try to meet with a small Sakei (jungle) tribe of Pangans who were reported to have been seen in the vicinity, and to photograph some of the Siamese tree-graves, which method of burial, in accordance with instruc- tions from Bankok, is fast becoming obsolete. A forced march by night on elephants brought us to the spot too late to overtake the wild men, who had moved away, no one could say whither, the night before our arrival. Mr. Annandale was able, however, to photograph their late dwelling-place, which consisted of a cave under a projecting rock, near the summit of a lofty hill. He also took photographs of the tree-graves. These are usually cigar-shaped wrappers, or rather ‘ shells’ made of laths, and suspended horizontally at a height of 6 to 8 feet from the ground between two tree-trunks, branches, or posts. The corpse is exposed in one of these shells (the heels being generally left higher than the head), and allowed to decay till the bones are clean, after which the bones should be collected and burnt. Box-like receptacles on posts (as among the Madangs of Borneo) are occasionally substituted for the wrappers. On this journey some strange articles of diet were served up to us, among them being red ants, toads, bee-grubs, and a species of cicada. The manner in which the latter are caught is peculiar. ‘Two or three natives gather at night round a brightly burning wood fire, one of them holding a lighted torch. The others clap their hands at regular intervals, and the cicadz, attracted by the noise and guided by the light, fly down and settle upon the people as they stand by the fire. In the ‘wat’ (Siamese temple) at Ban Nah Mr. Annandale noticed that one of the small figures of Buddha which had been deposited in the temple as an offering, contained a fossil shell, and this clue, carefully followed up, led to the discovery of the quarry from which the fossil had been taken. The formation is of the Cretaceous age, and a number of specimens showing fossiliferous traces were secured here , well-authenticated finds of fossils in the Malay Peninsula have been of the rarest possible occurrence. On this same journey a couple of young leopard- or panther-cubs were picked out of their nest in a hollow tree by the roadside, and it being ON NATURAL HISTORY AND ETHNOGRAPHY OF MALAY PENINSULA. 395 found difficult to feed them they were, on reaching Lampam, suckled by a Siamese woman, who claimed to have previously suckled a bear. On reaching Lampam we found that Messrs. Evans and Vaughan had pro- ceeded to the ‘Talé Noi,’ or ‘ Little Lake, at the end of the Inland Sea, and followed them accordingly. We did not overtake them, but our visit to the ‘ Little Lake’ was of great interest. In one of the local ‘wats’ or temples a human embryo was found among the offerings. We also came upon a small isolated tribe called ‘Pram’ (? Brahm) people, who claimed to be a sacred tribe of Indian origin, and appear to have been hitherto undescribed. They retained several peculiar customs, notably that of burying their dead in a sitting posture, with the top-knot tied to the top of the coffin. A copy of a sacred book, describing the origin of the tribe and the story of their migration, was obtained with difficulty. It is said to be written in an Indian language, which they themselves no longer understand. Their dress consisted of a white robe, a white shoulder- cloth, and a peculiar white two-peaked turban or cap. Their chiefs claimed that they were the oldest inhabitants of the country, and that they were not constrained to make obeisance even to the sovereign. After a few days’ further stay in Singora, where we rejoined Messrs. Evans and Vaughan, we proceeded to Patani in the commissioner’s yacht, arriving after a good passage just in time to witness part of the gorgeous pageantry of a Malay ‘royal’ wedding, between the Raja of Patani’s sister and the ‘ Raja Muda’ of Kelantan. At Patani we were lodged in a big brick building ordinarily used as a school. An unfortunate accident here greatly handicapped the photo- graphic work. A big iron-bound shutter fell from its fastenings with a crash inside the building, and striking our best camera, so injured it that it had to be sent to Europe for repairs, a matter of months, and an irreparable loss so far as photographic work was concerned. It had just been used for taking a photograph of the Raja of Patani, who had most fortunately just returned to his house. Mr. Evans also had a narrow escape. On the 28th we left for Bukit Besar, or Negiri (Indragiri), an isolated mountain about 3,000 feet high, on which several days were spent. This was known to the natives as a haunted mountain possessing a pond near the summit, on which are said to grow certain magical shrubs, one of which is believed to be the means of conferring perennial youth on its finder, and another to be one of the most powerful love-charms in the world. These treasures are guarded by a host of demons, and the natives expressed great fear of them until the ascent to our camp (at a height of about 2,000 feet) had been successfully accomplished, after which their fears rapidly subsided. Mr. Evans got his first specimen of Peripatus here, and Mr. Vaughan also did well with the mountain flora. On our return to Patani Messrs. Vaughan, Annandale, and Evans proceeded up the Patani to Biserat in Jalor (Jala), which proved an excellent collecting-ground. I stayed: at Patani for some days longer, and visited the very extensive saltpans near the river mouth, the Patani potteries, and the grave and shrine of the celebrated local saint of Cape Patani, about all of which much information was gained. Of the latter many miracles are told, and his grave-posts (at the head and foot) are still believed to make prophetic movements, one instance of which I was enabled to test on the spot. Two very curious rods, such as are used in divination, were here obtained. 396 REPORT—1900. On the 26th I rejoined the rest of the party at Biserat, and then visited the magnificent limestone caves, a very complete collection of whose fauna was made by Mr. Annandale. These caves included the fine Gia Gambar, or Statue Cave, which contains a recumbent figure of Buddha, nearly 100 feet long, as well as a number of other statues in a sitting posture. Extensive zoological and botanical collections were also made at Biserat by Messrs. Evans and Vaughan. An exhibition of devil dancing was here witnessed. Smallpox having now set in badly and two deaths occurring in the village, collecting became more difficult, and presently the Raja and his household retired to the hills, and many houses were closed by means of a rattan, carried round outside the fence of the compound, whilst slipknots of jungle-grass (lalang) were hung across the gate, and a couple of stems of a bitter-tasting tree, called the Bedara Pahit, buried crosswise on the threshold. One of the annual ceremonies for the purification of a village was here witnessed, and many ethnological specimens and much information obtained. On June 6 Mr. Evans fell ill, and as he took long to recover, Messrs. Annandale and Vaughan proceeded to Kota Bharu, in Raman, whilst Mr. Evans and I went down to the coast. After spending a few days at Patani, we went to Jambu in Jering. Here, too, I witnessed the annual ceremony for the purification of the village, at which the launching of a spirit-boat, about a yard and a half long, formed the chief feature. Before leaving Jambu I paid a flying visit to Teluban. On returning to Patani we were rejoined by Messrs. Vaughan and Annandale, and proceeded by the overland route through Raman Ligeh and Ulu Kelantan, and up the Lebih, a tributary of which stream, the Aring, takes its rise in the neighbourhood of the Tahan Mountain, which it was one of the objects of the expedition, if practi- cable, to ascend. The expedition therefore started from Biserat on July 6, and proceeded to Kota Bharu, the chief town of Raman. Halts of some days’ duration for transport purposes were made at Kota Bharu, Tremangan, Belimbing, and Aur Gading (a village below the rapids on the Lebih river), but on August 10 the expedition reached the village of Kuala Aring, having covered in thirty-five days (only about half of which were spent in travelling) a distance of about 200 miles. The first eighty or ninety miles were performed on elephant back, the remainder by means of boats or bamboo rafts. Mr. Vaughan, who had only joined the expedition for the first six months, left us at Belimbing. At Kuala Aring I found the local authorities so opposed to giving information about the route to the mountain that it appeared to me safer to try to find the way for myself than to put the expedition at the mercy of local guides. I therefore left Messrs. Evans and Annandale at the village, and set out to scout with two of the Malays belonging to the expeditionary staff I decided to attempt the mountain from the Pahang side, and ascending the Lebih to its headwater crossed the watershed by way of Bukit Batu Atap, and descending the tributaries of the Tembeling eventually reached a village called Kampong Pagi, where I spent four or five days in fruitless attempts to obtain guides from the wild tribes in the neighbourhood. They were afraid to go, but I obtained the services of six of the local Malays as carriers (two of whom absconded at the end of the first day’s march), and proceeded up the banks of the Tahan river until the foot of the mountain was reached. My original plan was to ON NATURAL HISTORY AND ETHNOGRAPHY OF MALAY ‘PENINSULA. 397 ascend some of the high crags in the vicinity of the mountain, and thus ascertain its locality, but at the end of the first week’s march, finding that we were on what appeared to be a spur of the main range, I decided to go forward and ascend it as far as circumstances would permit. We therefore climbed the range peak by peak, but were at length stopped by a formidable subsidence or break, which forced us to return on our tracks for a day’s march before we could circumvent it. Eventually, after a march of about eleven days since our entry into the river, we reached the highest point that we could compass, about 200 feet to 300 feet below the peak, when we were stopped by an overhanging wall of rock which, after several attempts, we found ourselves unable to scale or circumvent. We got sight, however, here of a hitherto unrecorded companion peak to the Tahan Peak, which was identified as Gunong Larong, or ‘Coffin Moun- tain. At this time we had barely enough rice even on short rations to last three days, and the descent, till we reached the nearest human habita- tion, took five. Our difficulties were further increased by fog, rain, and fever. ' The rains were exceptionally heavy, the Tahan river being three times in flood during our ascent of the mountain, and as they had set in earlier than usual, it appeared, under the circumstances, unadvisable and unsafe to commit the rest of the expedition to the ascent of the mountain. Mr. Annandale therefore, who had been waiting at Kuala Aring with a view to participating in the ascent of the mountain, if practicable, returned to Europe, and Mr. Evans remained in camp with Mr. Yapp, who had arrived during my absence. Mr. Laidlaw accompanied me up the Aring river, and there took photographs and full measurements of several persons belonging to the wild tribes, while a good deal of information about their manners and customs, as well as a vocabulary of nearly 600 words, was collected by myself. On our return, we all descended the Lebih on rafts, as far as its juncture with the Kelantan river, and thence descended the latter as far as Kota Bharu, the capital of the important East Coast State of Kelantan, and the seat of its Raja. On the way down the river we measured and photographed several more Sakeis. At Kota Bharu Messrs. Laidlaw and I stayed for about a month, Messrs. Yapp and Evans proceeding to Trengganu, in order to pay a short visit to the coral islands off that coast. Much important ethnological work was done at Kota Bharu. Investi- gations were conducted into Malay methods of industry, and a devil- dancing performance was witnessed by Mr. Laidlaw and myself, at which the name of the winning bull at a coming bull-fight was correctly pro- phesied. Full anthropological measurements were taken by Mr. Laidlaw of ten or twelve Kelantan Malays, notes made of the colour of their skin, eyes, hair, &c., and experiments made as to their colour vision. On leaving Kota Bharu we proceeded to Trengganu, where we met Messrs. Evans and Yapp, who reported having had a narrow escape from drowning off the Redangs through the swamping of their boat. Mr. Evans was unable to swim, but I am thankful to say that both he and Mr. Yapp succeeded in holding on to the boat until they were picked up by some Malays, who went to their assistance. They were about half a mile from shore at the time. At Trengganu my investigation of Malay industries was continued, and much useful information obtained. The most interesting was perhaps 398 REPORT—1900. the method of manufacturing damasked krisses—the details of which were carefully studied. Measurements were also taken of at least ten of the Trengganu Malays, and full observations recorded. On leaving Trengganu, we proceeded to Singapore, where a few days were spent, and a visit paid to one of the villages of the ‘ Orang Laut’ (the old piratical stock of sea-gipsies, who were once the terror of the Straits, and who were found by Sir Stamford Raffles living in their boats round about the island of Singapore, when it was proclaimed a British Colony). By the first available steamer we proceeded to Penang, whence Mr. Evans proceeded to Pulau Bidan, an island off the Kedah coast, to collect marine zoological specimens, and Messrs. Yapp and Laidlaw made the ascent of Gunong Inas (a hill, upwards of 5,800 feet high), in Perak, a difficult trip, the successful accomplishment of which reflects credit on Mr. Yapp, who, as the senior member of the staff after Mr. Evans’s departure, took charge of the remainder of the party in my absence. They both brought back with them extensive collections (zoological and botanical). Mr. Evans returned to Penang on Christmas Eve, having used up the remainder of his outfit, and returned to Europe a few days later, having completed his year’s work. As soon as I was able to go up country, I proceeded to Kedah, and there, after a short excursion up the coast to Satal and Perlis, made two expeditions into the Sakei country, near the headwaters of the Muda. Here I had the good fortune to find a tribe of from twenty to thirty individuals living in a long barrack-like shelter of palm- leaves. From them, and from a neighbouring tribe, I obtained much valuable information as to their manners, customs, and language, as well as full measurements of a few individuals, and some probably unique phonographic records of their songs, which are of an extremely simple «nd primitive character. IJ also, with difficulty, procured the skeleton of an adult male. In all the States visited by me, investigations were made into the leading Malay industries, and much valuable material bearing on this subject was collected. Wherever possible, statistics were obtained showing the extent and nature of the development of trade and the stage of civilisation which had been reached by the people. Many of the leading Malay industries, such as that of weaving, are being rapidly modified by the introduction of European methods and appliances, and it is now the rarest and most difficult thing to obtain cloth actually made of home- spun thread, the use of Singapore silk and aniline dyes being already almost everywhere the fashion. In addition to the above, the departments of ethnology studied included religious and medical ceremonies, children’s games, legends, languages and dialects, under each of which headings a mass of material was collected. The Zoology of the Sandwich Islands ——Tenth Report of the Committee, consisting of Professor NEwron (Chairman), Dr. W. T. BLAN- FORD, Professor S. J. Hickson, Mr. F. Du Cane Gopman, Mr. P. L. Scuater, Mr. E. A. Smita, and Mr. D. Suarp (Secretary). THis Committee was appointed in 1890, and has been annually re- appointed. ON THE ZOOLOGY OF THE SANDWICH ISLANDS. 399 In accordance with the intention announced in the last report, Mr, R. C. L. Perkins has again been sent to the islands by the Committee. His departure from this country was delayed for some months by the out- break of plague at Honolulu ; but this difficulty having disappeared, he is now at work in the island of Kauai. Four parts of the second volume of the ‘ Fauna Hawaiiensis’ have been published since the last report. They comprise 441 pages and 14 plates, ‘the subjects and authors being as follows : ‘Orthoptera and Neuroptera,’ by R. C. L. Perkins ; ‘Coleoptera,’ pt. 1, by D. Sharp and R. C. L. Perkins ; ‘ Mollusca,’ by E. R. Sykes ; ‘ Earthworms,’ by F. E. Beddard ; ‘ Entozoa,’ by A. E. Shipley. Mr. Perkins finds that great changes have taken place in the islands during his absence, and that the forests are being extensively destroyed and replaced by sugar-cane, this industry being at present extremely remunerative there. The Committee ask for reappointment. Investigations made at the Marine Biological Laboratory, Plymouth. — Report of the Committee, consisting of Mr. G. C. BourNE (Chair- man), Professor E. Ray LANKESTER (Secretary), Professor SYDNEY H. Vines, Mr. A. Sep@wick, Professor W. F. R. WELDON, and Mr. W. GarstTana. Messrs, Woopwarp, Scott, and Brebner were prevented from visiting Plymouth during the past year. Several other naturalists, however, applied for the use of the British Association’s table, and it was accord- ingly allotted to Mr. A. D. Darbishire, of Balliol College, Oxford, for investigations on the development and natural history of Pinnotheres ; and to Mr, W. M. Aders for the collection and preparation of material for studying the spermatogenesis of ccelenterates. Mr. Darbishire oceu- pied the table for six weeks, and Mr. Aders for three weeks, during the past summer. Mr. Darbishire’s report to the Committee is given below. An application for the use of the table during the month of September has been received from Mr. R. C. Punnett, B.A., in order that he may continue some investigations on which he is at present engaged on the pelvic plexus of elasmobranch fishes. Mr. Darbishire’s Report. My original intention was to study the life-history and habits of the crab Pinnotheres, which is a well-known inhabitant of mantle-cavities of certain lamellibranchiate molluscs; but during my visit to Plymouth no breeding females could be found, and my observations were limited to the determination of some new points in the habits and structure of the male of Pinnotheres pisum. A specimen of this was dredged in company with some Cardiwm norvegicum, from which it presumably came. The habits of the male were very interesting to observe in view of the seden- tary habits of the female. Tt could swim forwards for a long time and at ® good speed, and with an accurate sense of direction. It swam ina manner hitherto undescribed in crabs by rowing with its last two pairs of thoracic legs, each of which has a double row of hairs on its posterior 4.00 REPORT—1900. edge. As the female is said to be blind I made many experiments to determine the sensitiveness of the male to light. It was conclusively shown that the male is not only not blind, but is extremely sensitive to- light in that it avoids extremes both of light and darkness, and in an avea offering various degrees of illumination invariably takes up a moderately illuminated position. As more specimens of Pinnotheres could not be found, I decided to study the myology of Calanus. It would be out of place to give here the details of the musculature of this copepod, but it is interesting to note that the arrangement and comparative size of the muscles tend to support Prof. MacBride’s recent statements as to the movements of Calanus and other copepods, viz., by means of their second antennex and pleopods, and not by means of their first antenne. I tried numerous methods for demon- strating the muscles by using various stains, fixing agents, and mounting media. The most successful was to cut the animal in half sagittally, after fixation with corrosive sublimate, stain in borax carmine, and mount in glycerine jelly (Brady’s solution). This shows the muscles of the trunk clearly. I take this opportunity of thanking the British Association for the use of their table at the Plymouth Laboratory, and Mr. Garstang and Dr. Allen for their ever-ready help and suggestions. Coral Reefs of the Indian Regions.—Intervm Report of the Committee, consisting of Mr. A. SEDGwicK (Chairman), Mr. J. GRAHAM KERR, Professor J. W. Jupp, Mr. J. J. Lister, and Mr. S. F. Harmer, appointed to investigate the Structure, Formation, and Growth of the Coral Reefs of the Indian Region. Tue Committee have received the following report from Mr. J. Stanley Gardiner :— The expedition under my charge has been carrying out work during the last eighteen months in the Laccadives, Maldives, and Ceylon. During the month of May 1899 I toured through the raised coral- reef areas of Ceylon and round the coast. In the north of the island these form a succession of higher and higher raised reefs down to Dam- bula, broken only by isolated flat-topped peaks of older rocks, on the sides of which the successive elevations are sometimes clearly visible in hori- zontal lines of wave action. It is only in the topography of the older, often much dolomitised country that the previous existence of either barrier or isolated reefs is indicated. The greater part is formed of a mixed reef sand, and appears before elevation to have borne a consider- able resemblance to the large mudflats round the islands of Viti Levu and Vanua Levu, in the Fiji group. * Round the coast of Ceylon, especially to the south, a recent elevation of five to twenty feet was found in broad flats by the sea. These are now invariably being washed away down to the low-tide level, at which they persist, to a certain extent, as fringing reefs of varying breadth. The greater part of the west and south coasts is devoid, however, of any reef-growths, the shore being rocky or formed of fine siliceous sand. In May 1899 the rocky shore near Bentota was seen to be covered with ON CORAL REEFS OF THE INDIAN REGIONS. 401 small coral colonies, which were evidently a growth of the previous north-east monsoon. In September these had completely disappeared, having been washed away in the south-west monsoon. At Galle, Talpe, and Weligama numerous recently living colonies of corals, particularly of the genera Porites and Pocillopora, of four to eight months’ growth, were found completely silted up with sand and dirt of all sorts. A noticeable point about the reefs immediately round Ceylon is the comparative absence of reef-building nullipores, which are a marked feature of all isolated oceanic reefs. In connection with this an attempt was made to examine the shoals two to six miles off the south and south- west coasts of the island, which indicate with the soundings the possible upgrowth of a barrier reef. The weather, however, at that season was so unfavourable that I was unable to dredge, land, or anchor on any. Subsequent visits to south India and north Ceylon indicated clearly a former land connection between the two. The so-called Adam’s Bridge and the islands of Manaar and Ramasserim, which the former joins, appeared indubitably to be the remains of a formerly elevated limestone flat, which has been more or less cut down by the sea to the low-tide level. The coast lines, too, of Ramasserim and to the north of the Jaffna peninsula were also probably at one time continuous. The months of June, July, and August 1899 were spent in Minikoi, an isolated atoll, the most southern of the Laccadive group. Here I was accompanied by Mr. L. A. Borrodaile, who proposed to study various points connected with the Crustacea and Chetopoda. Unfortunately Mr. Borrodaile, who had been collecting these forms in Ceylon, almost at once succumbed to the climate, and after five weeks returned to Ceylon, whence he was at once ordered home. Every part of the island was visited : a survey was made and numerous cross-sections were run. From these it was clear that there had been an elevation of the original reefs to a height of at least twenty-five feet above low-tide level. Numerous observations were made on the currents at different depths within the lagoon in reference to its shoals, &c. Work on this point could seldom be carried on outside the reefs, as originally intended, owing to the heavy north-westerly winds which prevailed. The lagoon was dredged to ascertain the distribution of its corals, and a few water samples and temperature observations were taken. Considerable attention was paid at Minikoi to the sand-feeding organ- isms, especially Holothurie, Enteropneusta, and Sipunculida. These forms appear to be largely instrumental in finely triturating the sand, the small particles being subsequently carried out of the lagoon in astate of suspen- sion. The boring organisms, too, are very important in causing the decay of dead coral and rock, especially in the lagoon. These, accordingly, do not form points of attachment for fresh reef-growths to arise, and owing to the larger surface exposed are the more readily dissolved by the water. Indeed all evidence collected showed that the lagoons of atolls may be, and are, very generally formed by the solution of the central rock of originally more or less flat reefs. Tn October 1899 I left for the Maldive group, to which I was accom- panied by Mr. Forster Cooper, who assisted me in all the work and very largely took charge of the dredging. The Sultan lent us a schooner of about eighteen tons, which we at once fitted out in Male, subsequently cruising through the northern atolls during the months of November, meet and part of January. About a hundred islands in the atolls . DD 4.02 REPORT—1900 of Goifurfehendu (Horsburgh), S. Mahlos, N. Mahlos, N. Miladummadulu, S. Miladummadulu, Fadiffolu, and Male were visited. Numerous sound- ings were made and dredgings everywhere taken. Horsburgh Atoll and the two atolls of Mahlos Madulu in particular were thoroughly worked over. Parts of January and February 1900 were spent at Hulule, a small island at the south-east corner of Male Atoll, this being the month of Ramazan. A thorough survey of this island and its reefs was made, the whole forming an atoll of the second order, an atollon on the rim of an atoll. Large collections were obtained of the fauna of this atollon from all depths, together with observations on many special points. A set of corals of known period of growth was collected from an artificial passage through the reef to the landing-place of the island. In February Mr. Forster Cooper took the schooner off for a short dredging cruise in Male Atoll, while I remained in Male making special observations on the water temperature, currents, food, &c. Tn March I was unfortunately obliged, owing to illness, to return to Ceylon, where I spent some time in hospital. Mr. Forster Cooper mean- time continued the work, taking the schooner and dredging the atolls of S. Male, Felidu, Mulaku, Kolumadulu, and Haddumati. In April I returned with the s.s. Zleaface, a vessel of about 350 tons, which I had chartered. Mr. Forster Cooper was relieved in Haddumati Atoll and joined the steamer, the schooner being sent back to Male. We then proceeded to Huvadu (Suvadiva) Atoll, which we entered by a northern passage. The lagoon to the east was dredged and sounded, the positions of islands and reefs observed, and four islands visited. A move was then made to Addu Atoll, the outer slopes of which and also the lagoon were dredged and sounded. The islands were charted in with the assistance of Captain Molony, and the majority were visited by some member of the party. On returning to Suvadiva the south and west sides of that atoll were dredged. On account of the heavy weather we were prevented from seeing Mulaku, which we had especially desired to visit. Proceeding north to Male we skirted Haddumati Atoll and crossed Kolumadulu, then visited and dredged 8S. and N. Nilandu Atolls, sub- sequently anchoring in Felidu and Ari. The passages were sounded between the following atolls: Kolumadulu and 8. Nilandu, S. and N. Nilandu, Mulaku and Wattaru, Wattaru and Felidu, N. Nilandu and Ari, S. and N. Male. Three further lines of soundings were run across the central basin between the east and west lines of atolls. More than tiree hundred dredgings were taken, and in addition large and, we believe, very complete collections were made of the reef-fauna at Minikoi and Hulule, four natives at least always accompanying and assisting us in this work. The collections of land-fauna we believe to be equally complete from these islands. Collections of the plants of five separate Maldivan islands are now in the hands of Mr. J. C. Willis, Peradeniya Gardens, Ceylon. A large number of anthropological measurements and considerable ethnological collections were procured, of which we hope to give the Asso- ciation an account at some subsequent meeting. ON BIRD MIGRATION. 4.03 Bird Migration in Great Britain and Ireland.—Third Interim Report of the Committee, consisting of Professor NEwron (Chairman), Rev. EH. P. Knusiey (Secretary), Mr. Joan A. Harvie-Brown, Mr. R. M. Barrineton, Dr. H. O. Fores, and Mr. A. H. Evans, appointed to work out the details of the Observations of Migration of Birds at Lighthouses and Inghtships, 1880-87. REFERRING to its Interim Report of last year your Committee has the satisfaction of stating that Mr. William Eagle Clarke, of the Museum of Science and Art in Edinburgh, has been diligently continuing the laborious task he undertook of working out the details of the collected observations in accordance with the scheme indicated in the Report made at Bristol in 1898, and has furnished your Committee with the following Statement, together with a Summary of the observations as regards (I.) the Song-Thrush (Zwrdus musicus) and (I1.) the White Wagtail (Motacilla alba), which throws such a light on the Natural History and especially the movements of those two species as has never been possessed before. Your Committee feels that a great debt of gratitude is due to Mr. Clarke for the courage and perseverance which he has shown in grappling with the enormous mass of statistics necessary to afford the results so lucidly and concisely summed up by him. Your Committee trusts that its feeling may be shared by the Association generally, and that as a consequence a grant of money may be renewed, if only to defray the outlay which is involved by the prosecution of Mr. Clarke’s labours. Remuneration for his invaluable services, which the Association will remark he is willing to continue, is unfortunately not to be thought of. In its Report last year your Committee mentioned that one of its -members (Mr. R. M. Barrington) was printing the results obtained from the Irish Lights, continued on his own account since 1887. That gentle- man has since prepared for publication, at the cost of a stupendous amount of labour, an Analysis of these results, which he hopes will appear before the end of the year, and your Committee desires to call early attention to what cannot fail to be one of the most important contributions to the study of Bird Migration ever made. Your Committee respectfully requests reappointment. Statement furnished to the Committee. By Wm. EsaGie CLARKE. The extraction of the records of occurr(nces of birds in Great Britain and Ireland, culled from the voluminous periodical and other literature published during the period covered by the inquiry, 1880-1887 inclusive, has at length been completed, and has resulted in many thousands of useful and important observations relating to the movements and occur- rences of birds in both maritime and inland localities being added to the data amassed by the Committee. This additional information includes not only a set of valuable records for the inland counties of Great Britain and Ireland, which was a great desideratum, but also comprises data relating to the occurrence of a con- DD2 4.04. REPORT—1900. siderable number of rare and critical species made by ornithologists—data, in fact, that it was impossible to obtain from the light-keepers, whose knowledge of birds is, naturally, limited. Since the year 1891 Mr. Harvie-Brown and myself, with the valued assistance of Mr. Lionel W. Hinxman and Mr. T. G. Laidlaw, have prosecuted an inquiry into the movements of birds in Scotland, and the investigations are still proceeding.! In addition to the observers at the light-stations, we have enlisted the services of a number of ornithologists. This again has resulted in the acquisition of much useful supplemen- tary information. Now that the data have been made as complete as possible, the time has arrived when, for the first time in the annals of British Ornithology, it is possible to write an authoritative history of the migrations of each British bird, for few indeed among our native species are entirely sedentary. This is the task I now propose, with the approval of the Committee and of the British Association, to undertake. I submit herewith a Summary of Details of the various migratory movements of two species—(I.) the Song-Thrush (Z'urdus musicus) and (II.) the White Wagtail (Motacilla alba)—as examples of my method of treatment. Summary of Details. I. Song-Thrush (Turdus musicus). Introductory.—The Song-Thrush furnishes us with a most excellent example of the complex nature of the phenomena of bird migration as observed in Great Britain and Ireland. The various movements of this species cover a period of nearly ten months of the year, June indeed being the only month in which the Thrush does not figure as a migrant in the records amassed by the Committee. During this period it plays a varied réle as a migratory bird, being a summer visitant, a bird of passage in spring and autumn, a winter visitant, a winter emigrant, and lastly, it is chiefly to be regarded as a rare casual visitor tothe most northerly of the British Isles, namely, the Shetlands. Tn addition, the Thrush is a permanent resident in certain districts, more especially in the gardens and immediate neighbourhood of cities and towns, where even in Scotland a number remain throughout the year. Such residents, however, probably form the minority of our British Thrushes. Autumn Emigration of Summer Visitors.— At the end of summer? and in the early autumn a considerable number of the Thrushes which have reared their broods with us, especially those which inhabit the elevated districts, emigrate towards the south.? 1 The Reports appeared in the Annals of Scottish Natural History for 1893, pp. 147-164; 1894, pp. 146-153; 1895, pp. 207-220; 1896, pp. 137-148; 1897, pp. 187-151; 1898, pp. 200-217; 1899, pp. 140-158; 1900, pp. 70-87. 2 On July 8, 1882, five Thrushes struck the lantern at Slyne Head Lighthouse (west coast of Ireland), one of which was killed. In 1885, on July 3 and 11, several Thrushes are recorded at the Inner Farne. On all these occasions the weather was very unsettled, and thunder prevailed. .3 Mr. T. G. Laidlaw, whose home in Peeblesshire lies 900 feet above the sea, informs me that the Thrushes leave that district ‘to a bird’ in the autumn, and return during the early months of the year. ON BIRD MIGRATION. 4.05 Some of these may not proceed at once beyond our southern counties, where the length of their sojourn is determined by the climatic con- ditions of the season ; others depart forthwith for more southern regions beyond our limits. Throughout August, but chiefly towards the end of the month, there are clear indications at the light-stations that Thrushes are quietly slipping away from Britain. There are no marked movemenis recorded for this month, but there is unmistakable evidence that a gradual and steady emigration is in progress on all the coasts of Britain. From the Trish coasts, however, this happens only rarely during August, the birds usually departing later in the season. These earliest emigrants are gene-. rally observed in small numbers, and either alone or occasionally in company with ‘ Warblers ;’ sometimes a few are killed at the lanterns.! In September and October the emigratory movements are more general and more pronounced in their nature; but it is not until the weather breaks up in the latter month that any ‘rush’ is recorded. During these months, especially in September, the Thrush departs im company with various species of summer birds, and its emigrations are recorded from all sections of the British and the east and southern coasts of Ireland. The Thrush is, however, emigratory to a lesser degree in the Sister Isle than in Britain. In October the migratory movements of the Thrush are often of a very complex nature, and are difficult to interpret. The most complicated movements are those during which emigration, immigration, and passage are in progress simultaneously, 2 phenomenon which sometimes happens under peculiar weather conditions.” Later in the year the emigratory movements, which doubtless include many of the recently arrived immigrants from the north of Europe, are dependent on and synchronous with more or less severe weather con- ditions, and these will be duly treated of in the proper place. Autumn Immigration and Passage.—There is no evidence whatever of the appearance of the Thrush upon our shores, as an immigrant from North-western Europe, until the end of the third or the beginning of the fourth week of September, when it arrives with great regularity? in company with the first Redwings (Z’urdus iliacus) ; occasionally Red- breasts (Hrithacws rubecula), Golderests (Regulus cristatus), Woodcock (Scolopaa rusticula), Jack Snipe (Gallinago gallinula), and Short-eared Owls (Asio accipitrinus) are observed at the same time.‘ The immigrations continue during October, during which month there are lulls, followed usually by two very pronounced ‘ rushes’ to our shores, when for several successive nights Thrushes pour in upon our eastern sea- board in vast numbers. These ‘rushes’ occur as a rule (1) about the middle of the month, and (2) again during its fourth week. These immigratory movements are confined to the east coast of Britain, from the Orkneys to Norfolk. North Ronaldshay, the most ' As early as August 1, 1884, six Thrushes struck the lantern of Dhuheartach Rock Lighthouse, two being killed. * See ‘ Digest of Observations,’ Brit. Assoc. Rep., 1896, p. 471. * On September 21 in 1881, 1882, 1883, and 1887. * Professor Collett, Oversigt af Christiania Omegns ornithologiske Fauna, p- 27, says that the Thrush departs from the Christiania district during September, and continues to do so until the first days of November. Statistics for S.W. N orway would be preferable, as being more intimately associated with those for Great Britain, but unfortunately they do not appear to be available. 4.06 REPORT— 1900. north-easterly of the Orkneys, and the extreme southern portion of the main island of Shetland are annually visited, but these stations mark the northern limit of the Thrush’s regular distribution during migration in Britain, for the bird is recorded very rarely further north, and is practi- cally unknown in Unst. The Thrush’s travelling companions are chiefly its congeners the Redwing (Z’wrdus iliacus), Fieldfare (7. pilaris), Ring Ousel (7. torquatus), and Blackbird (7. merula) ; and also the Brambling (Fringilla montifringilla), Golderest (Regulus cristatus), Redbreast (Erithacus rubecula), Woodcock (Scolopax rusticula), &e.' Along with these species many Thrushes perish at the lanterns of the lighthouses and light-vessels, especially when the night is hazy, with light rain. Unlike its congeners just named, it is somewhat remarkable that the Thrush does not occur as an immigrant in numbers in November. The immigration of the Thrush practically ceases with the great arrivals which characterise the latter half of October, though stragglers do arrive up to the middie of November. After this the autumn immigration of the Thrush entirely ceases. Many of the immigrants upon arrival proceed: south, as birds of passage, along our eastern and southern coasts, and finally quit our shores, the majority to seek more southern lands, others to cut across St. George’s Channel +o winter in Ireland. Others, again, remain as winter visitors, and work their way to Western Britain? and Ireland after an overland passage. Many of the birds, however, quit our islands, after a longer or shorter sojourn, under the pressure of severe: weather conditions.* Winter Movements.—The great emigratory movements of the winter commence in October, and are continued during November, December, January, and February.? They are synchronous with outbursts of cold, snow, or of extremely unsettled weather. Such untoward conditions may prevail generally over our islands, or they may be circumscribed ; and their influence on the emigrations of the Thrush is in more or less direct consonance with their distribution. In genial months little or nothing is recorded. In others the few local movements are traceable to topical weather conditions. But sooner or later during each season great outpourings take place, often extending over several successive days and nights and affecting all our coasts. The Thrushes affected are not merely our would-be resident birds, but a very 1 For the weather conditions controlling the movements of the British autumn immigrants, see the ‘ Digest of Observations,’ Brit. Assoc. Rep., 1896, pp. 469-471. 2 The Thrush isa winter visitor only to certain isles off our western coasts, among others Tiree in the Inner Hebrides. From careful observations made on that island by Mr. Peter Anderson, we learn that this bird makes its first appearance there for the winter on dates varying from October 4 to 30, some considerable time after its first arrival on our shores. 3 Tt has been stated that a small dark race of the Thrush occurs on passage on the east coast of England. These birds are supposed to be of Hebridean origin. I have never seen specimens of such a race, and I do not believe that they can have found their way to our eastern coast from the Hebrides. I have examined a number of Thrushes from Barra in the Outer Hebrides, where the bird is a resident, and do not find them to differ either in size or colour from the ordinary mainland form. 4 In 1886, as early as October 4 and 6, there were great emigratory movements on all our coasts, due to extremely unsettled weather, with thunder in the N. and N.W., accompanied on the 5th by a great fall of temperature—a fall of fifteen degrees below that of the previous day. ° There are also movements during March in some years; but they are of a local nature, and are not to be regarded as emigratory. ON BIRD MIGRATION. 407 large proportion of them are no doubt the immigrants lately arrived from the north, which, as winter visitors to our islands, remain until compelled to move further south or west. The first move on these occasions is to the coast, where some tarry, and even remain to perish ; while others pass down both the east and west coasts of Great Britain, many of those following the former route, sweeping along the south coast westward, and crossing the Channel for the Continent. Many again seek Ireland, from which, however, emigra- tions are also recorded. Should the cold spell be of great severity, or be unduly prolonged and widespread, then a still further exodus takes place (observed chiefly on the west coast of Great Britain and east coast of Ireland), and many perish even in such usually safe retreats as the Scilly Isles, and at Valentia, or other isles off the west coast of Ireland, which are largely sought on such occasions. No doubt, too, many of these emigrants perish in their continental haunts, for after winters of almost arctic severity, such as that of 1880-81,' the Thrush was conspicuous by its absence, or by its rarity, in most districts in our islands.” Spring Immigration.—Among the voluminous records relating to the movements of this species during February, there are many which clearly indicate that the Thrushes which left us in the early autumn to winter in countries to the south of us commence their return to our islands for the spring and summer. These immigrations are performed by small parties during mild periods of the month, and are chiefly observed on the southern coasts of England and Ireland. Such return movements are continued during the first half of March, when immigrant Thrushes, in company with Blackbirds (Turdus merula), Larks (Alauda arvensis), Pipits (Anthus pratensis), Starlings (Sturnus vul- garis), Lapwings ( Vanellus vulgaris), and Curlews (Wumenius arquata), are recorded from the south coast of England northwards to the Western Isles of Scotland, and from the south and south-east coast of Ireland. The arrivals on the south coast of England take place during the night or early morning. In Ireland they are recorded for both the hours of darkness and during the daytime, and the birds are noted as proceeding in a north-westerly direction at the south-east stations. In most instances the return is a gradual one, performed by small companies, and at intervals, but occasionally in March in ‘rushes’ with the other species already mentioned. Spring Emigration.—Towards the end of March the Thrushes which have wintered in Tiree and other western islands off the coasts of Scot- land and in Ireland are recorded as taking their departure. It is not, however, until April that the spring emigratory movements from the mainland of Britain set in. Then the birds which have wintered in our islands leave our shores to return to their summer haunts in Northern Europe.* Throughout April, but chiefly during the first three weeks of the ‘ During this winter twenty days of hard frost and sixteen days of deep snow prevailed on the west coast of Ireland. It was much more severe elsewhere. * Other severe seasons covered by the inquiry, during which great move- ments and much mortality among our Thrushes are recorded, are those of 1885-6 and 1887. The first half of March, 1886, was remarkably severe, and many Thrushes perished even in our southern counties. * In 1885, on March 28 and 29, a few Thrushes in company with Blackbirds ap- peared at North Ronaldshay, the most north-easterly island of the Orkneys. 4.08 REPORT—1900. month, the emigratory movements of the Thrush are pronounced, and are almost entirely confined to the north-east coast of England and to the eastern and northern stations of Scotland. Some movements are also in evidence on the west coast of Britain, where the birds departing from Ireland and the Hebridean Islands are observed.! On these occasions the Thrush is noted as emigrating in company with Blackbirds (7’urdus merula), Fieldfares (7. pilaris), Redwings (7. ilacus), and Redbreasts (Hrithacus rubecula). During April the British emigratory movements doubtless become merged with those of the Thrushes which are on passage along our coast- line, proceeding from their more southern winter to their more northern summer quarters. Spring Birds of Passage.—The first undoubted appearance of the Thrush as a bird of passage takes place at the end of March, when the birds which have wintered in South-western Europe, and are en route for breeding quarters to the north of our isles, arrive on the south coast of England in company with Blackbirds (Zwrdus merula), Fieldfares(7’. pilaris), Redwings (7. cliacus), Wheatears (Saaicola cenanthe), ‘Warblers’ (Sylviide), Larks (Alauda arvensis), Starlings (Sturnus vulgaris), and, occasionally, Wood- cocks (Scolopax rusticula). These early arrivals do not appear to proceed to North-Western Europe instanter,” for, as we have stated, there are no March emigrations. The passage continues throughout April, when the voyagewrs pass northwards along our eastern seaboard, where they are joined by many of our British emigrants of the same species ; and it is often a matter of difficulty to distinguish between these classes of migrants during certain movements in April. In the years 1881, 1883, and 1885 there were a few movements which carry the date of passage into May, the 10th of that month being the latest date on which the northern migration of the Thrush is recorded.’ Such is the history of the Song-Thrush as a British migratory bird, when the tangled skein of its various movements has been reduced to order through careful study. The main facts elicited are : 1. That many Thrushes leave us at the end of summer and during the autumn, indicating that a very considerable number are summer visitors to our islands ; 2. That the first immigrant Thrushes—winter visitors and birds of passage—appear on our shores from the N.E. during the latter days of September ; ' Professor Collett, Oversigt af Christiania Omegns ornithologiske Fauna, p. 26, gives from the early to the last days of April as the period for the Thrush’s arrival in spring in the Christiania district. 2 From March 19 to 26, 1898, the Rev. O. Pickard-Cambridge, F.R.S., records an increasing number of Thrushes around his rectory at Wareham, on the coast of Dorset. On the 25th the land was fairly covered with them, and there must have been 200 or more in one field. Onthe 26th there were even more. On the 27th there were fewer, and by the evening of the 28th all had departed. Zo0/., 1898, p. 264. 3 1881, May 2, Inner Farne, Thrushes at lantern with blackbirds (Zurdus merula) and Ring Ousels (7. torquatus). 1883, May 8 and 10, at same station, in company with the same species ; May 7, Flamborough Head, four killed. 1885, May 2, 3, 5, and 6, Pentland Skerries, with Ring Ousels (7. torquatus), Fieldfares (7. pilavis), and Red- breasts (Lrithacus rubecula); 5th and 8th, Isle of May, several with ‘ Warblers’ ( Sylwiide), Red-backed Shrike (Zamius collurio), and Rufi (Machetes pugnax). ON BIRD MIGRATION. 409 3. That the great autumn immigrations from the Continent cease with the month of October, or considerably earlier than those of the Thrush’s migratory congeners ; 4, That winter emigratory movements, due to climatic pressure, set in with the first severe weather and recur with each outburst, but in gradu- ally diminishing volume ; 5. That the return spring immigratory movement of British and Irish Thrushes—summer visitors—from Southern Europe, commences in February and continues until the middle of March ; 6. That the spring emigratory movements—the departures of winter visitors from Britain—for Northern Europe set in and are continued throughout April ; 7. That the spring birds of passage arrive upon our shores from Southern Europe late in March, and that the passage proceeds during April, and, in some years, extends to the early days of May ; 8. That the Thrush occurs annually on the British shores from Southern Shetland and North Ronaldshay southwards, and that these stations mark the northern limit of the bird’s regular distribution as a migrant in Britain ; 9. That migrants to and from North- western Europe arrive on, and depart from, our north-eastern and northern coasts, and that many birds of passage among them traverse our eastern and southern coasts on proceeding to their winter quarters (Continental*and Irish) in the autumn and on their return in the spring ; 10. That the autumn immigrants which winter with us reach Western Britain and, to a certain extent, Ireland after an overland passage ; 11. That the west coast of Britain and the eastern and southern coasts of Ireland are those chiefly visited during the great migratory movements due to severe weather ; 12. That Ireland is largely sought during the colder months, both by ordinary winter visitors and also by Thrushes driven out of Britain by severe climatic conditions ; 13. That the Thrush does not participate in the east to west autumn, and west to east spring, movements across the southern waters of the North Sea. Il. White Wagtail (Motacilla alba). The White Wagtail as a British migrant presents several points of interest. As a summer visitor it is somewhat rare, and has only been recorded to breed occasionally in some of the more southerly counties of England. It is chiefly as a bird of passage that it visits our islands, and is then en route to and from northern breeding haunts which lie both to the N.E. and N.W. of us, namely, in Scandinavia, Faroe, and Iceland. It occasion- ally reaches Southern Greenland. As a migrant it is one of those species, few in number, which are more abundantly and generally observed on our western seaboard and its vicinity than on the east coast. Spring Immigration.—The White Wagtail arrives on the south coast of England in small parties during March, sometimes during the early days of that month.! ' The earliest date with which I am acquainted relates to this bird’s occurrence near Plymouth on March 3, 1872. 410 REPORT—1900. The immigrants continue to arrive on the English shores of the Channel until late in April, and in certain seasons have been observed in numbers on the west coast of Cornwall as late as the first half of May. On arrival on our southern seaboard the birds, which are most abundant on the western section of that coastline, usually tarry for some little time before resuming their journeys. In due course, however, they pass inland or northwards along both the east and west coasts, especially the latter. Spring Passage.—During March there are few records of the White Wagtail’s appearance on either the east or west coast of Great Britain. With April, however, the regular passage northwards sets in, and continues until about the middle of May '—not beyond, so far as regular passage is concerned, On the west coast we are able to trace the birds from Cornwall along the Welsh coast to the Solway and Clyde areas, and occasionally north- wards to West Ross. .‘ Wagtails’ are, however, observed regularly on passage at Cape Wrath, the N.W. limit of the mainland of Scotland, down to the middle of May. I have little doubt that these records relate to this species. Passing thence to the western islands, we pick up the lines of flight first at the important rock station of Skerryvore, and then at the Hebrides, in whose outer and inner islands, or certain of them, it is a bird of double passage. Here it has been observed at Barra, Monach, Lewis, Tiree, and Coll. At Barra (a southern island of the outer group) and at Tiree (one of the inner isles) it is quite common on passage in both spring and autumn ; and from these stations we have during late years been furnished with a valuable set of observations, and have examined many Hebridean specimens obtained on both islands at each of the seasons.” At the Monach Isle, with the exception of St. Kilda, the most western of the Hebrides, the White Wagtail is recorded as occurring not unfre- quently during April and early May. Intimately connected, no doubt, with these far western British move- ments are those observed in Ireland. Here, however, our present know- ledge is only of a fragmentary nature, for the few observations made in the sister isle all relate to the coast and isles of a single county, namely, Mayo, where the White Wagtail has been occasionally seen on passage during April and early May.* It is strange that there is not a single instance on record of the White Wagtail’s occurrence on the east coast of Ireland, though I can scarcely bring myself to believe that the bird does not occur there on its migratory journeys. Passing to the east coast of Great Britain, we find little or no infor- mation for its southern section, not even for that county which has always been remarkable for ornithological research and for its able ornithologists, namely, Norfolk. Hereit appears to have occurred merely on two or three occasions, and in the springtime only. 1 At the island of Tiree, Inner Hebrides, it has been observed passing north in considerable numbers as late as May 15. * The following are the spring records for Tiree kindly furnished to Mr. Harvie- brown and myself by Mr. Peter Anderson: 1893, April 7 and May 1; 1894, April 7, 12, and 30; 1895, May 3 and 5; 1896, April 22 and 24; 1897, April 28 and 30 and May 1 and 4 to 8; 1898, April 19 and 26; 1899, May 3 and 15 (many). 8 The most important of these Irish movements was witnessed passing along the shores of Killala Bay early in May, 1898 (Saunders, Bull. Brit. Orn. Club, vii. p. 58). ON BIRD MIGRATION. Al} In Lincolnshire and Yorkshire, so far as actual records are concerned, the White Wagtail is decidedly uncommon on passage in the spring. It is not until we reach the coast of Haddingtonshire that we have any adequate information regarding the passage of the present species along the east coast. Here, thanks to information privately supplied to me by my friend Mr. Wm. Evans, it is possible to find the bird in numbers, sometimes in considerable numbers, by looking for i, in April and at the beginning of May. I have myself seen the bird in both spring and autumn on the southern shores of the Firth of Forth. North of this the only definite record for the eastern mainland known to me refers to its occurrence at Inverness during April. In the northern isles of Orkney and Shetland there are a considerable number of records of Pied Wagtails (IZ. /ugubris) during the late days of April and early May, for the Pentland Skerries in Orkney and for Whalsey Skerries and Dunrossness in Shetland, which, I have little doubt, from the lateness of the dates, refer to the passage of the White Wagtail.’ Saxby 2 records the bird from Unst on two occasions in spring, namely, for June 1854 and May 1867. I am, however, not a little dubious as to the identity of certain migratory flocks of Pied Wagtails which that observer mentions as appearing in the spring on their way north, ana again in September on their way south, for that bird is an uncommon “species in Scandinavia.* Autumn Passage.—The return movement from the north is initiated by the appearance of the White Wagtail upon our coasts from mid-August onwards. The earliest date I have is for August 15, 1894, at Barra. From this date until the middle of September it occurs in parties proceeding south at the Hebridean stations of Barra and Tiree’ with great regu- larity. The autumn passage, however, is not a prolonged one, and the latest record for the bird’s occurrence in Britain, known to me, refers to a pair of adults observed in Oxfordshire on September 27, 1885.’ The return movement probably affects both the east and west coasts of the mainland, as the data faintly indicate. It is remarkable, however, that outside the Hebrides and the Forth area our information is of a very meagre nature, and the bird does not appear to have been observed on the east coast of England, or anywhere in Ireland in the autumn.® 1 During a visit to the southern portion of Shetland in the latter half of September, 1900, I found the White Wagtail abundant on passage; not a single example of the Pied Wagtail was observed. 2 Birds of Shetland, p. 81. 3 At Heligoland the spring passage of the White Wagtail commences at mid- March, and continues until the early days of May. 4 The Hebridean records (1892-1899) for the autumn migration of this species are as follows :—1892, September 1; 1893, August 24, 25, and 29; 1894, August 15; 1896, August 24; 1897, August 17 and September 2 and 3; 1898, August 24, Septem- ber 7 and 15; 1899, August 18. 5 Since the above was written, a single bird was noted in Southern Shetland on October 3, 1900. 6 On the west shores of the Continent the autumn passage is regularly observed. At Heligoland it commences at mid-August, and continues until mid-October. During our ill-fated visit to the island of Ushant, which lies immediately to the south of our extreme south-west coast, in early September 1898, Mr. Laidlaw and I saw many White Wagtails on migration. On some days as many as two hundred came under our notice, and parties of from twenty to thirty were not uncommon. 412 REPORT—1900. The White Wagtail is frequently noted in company with its Pied and Yellow congeners (7. dugubris and M. raii). It sometimes occurs at the lanterns of the lighthouses along with other species ; thus at Skerryvore, on September 8, 1897, several were killed during a rush of ‘small birds,’ Wheatears (Saxicola enanthe), and Pipits (Anthus pratensis), and their vings sent to me for identification. It appears to me that the White Wagtails which traverse our western shores and isles are probably en route to and from their western summer haunts in the Feroes and Iceland. That such is the case is rendered likely not only by the routes followed in Britain, but by the dates of arrival and departure as recorded for Iceland.} On the other hand, the comparatively late date on which this bird is observed in the autumn in Southern Scandinavia,? and the fact that its numbers are so few on our eastern seaboard, seem to indicate that the main route to north-western continental Europe does not lie on the British coasts. There can be little doubt that the White Wagtail is still much over- looked as a British bird, or confounded with the Pied Wagtail, a species from which it was not differentiated for many years. We have thus even yet much to learn concerning its distribution in most districts of Great Britain and Ireland. In certain areas, notably in the Hebrides, our knowledge has been considerably advanced during recent years, thanks to the excellent observations made by Dr. MacRury and Mr. Peter Anderson. The main facts connected with the migration of the White Wagtail are :— 1. It appears on the southern coast of England during March and April, sometimes in early May. 2. During April and May—as late as the middle of the latter month —it occurs on passage on the east and west coast of Great Britain, and has been at that time occasionally observed on the north-west coast of Treland. 3. The return passage commences with mid-August, and is over by mid-September. 4. The west coasts of Britain, and especially those of the Hebridean Islands, form the main route followed by the migrants. 5. The bird has not been observed on the east coast of Ireland at any season, nor has it been observed anywhere in Ireland during the autumn passage. ‘ In 1886 the species was first observed at Reykjanes on April 24, next on the 29th, and abundantly on May 9. Lastly, on August|3 (Gunnlaugsson, Ornis, 1895, p. 344). Gr6dndal says it is the first summer visitor, and comes in April to the Reykavik district, where one was shot as late as September 7, 1879 (Ornis, 1886, p. 358). The bird evidently leaves Iceland early in the autumn. Along with Mr. Backhouse, I spent the month of September 1884 in the south-east portion of the island, and we only observed this species on one occasion, namely, a family party seen on the coast on the 10th. * Professor Collett (Oversigt af Christiania Omegns ornithologiske Fauna, p. 84) states that it arrives during the first half of April, and leaves at the end of Septem- ber and first days of October. Itis occasionally observed in October, and exception- ally as late as November 15. ee — ee eas ON BIRD MIGRATION. 413 6. It has not been observed on the east coast of England during the autumn passage. 7. Much has yet to be learned concerning the White Wagtail as a bird of passage in districts in which it is presumed to be rare or unknown. The Climatology of Africa.—Ninth Report of a Committee consisting of Mr. E. G. RaveNsTEIN (Chairman), Sir Joun Kirk, (the late) Mr. G. J. Symons, Dr. H. R. Mim, and Mr. H. N. Dickson (Secretary). (Drawn up by the Chairman.) METEOROLOGICAL returns have reached your Committee, in the course of last year, from thirty stations in Africa. WNigeria.—We are able to publish a full year’s record for Old Calabar. The observations, since September last, are being made thrice daily in accordance with our programme. We look forward with interest to the receipt of meteorological reports from Northern Nigeria, which have been promised by General F. D. Lugard, C.B., and which we hope to be able to publish in next year’s report. British Central Africa.We regret that full reports have been received only for two stations, namely, Zomba, which is in the immediate charge of Mr. J. McClounie, the director of the scientific department, and Lauderdale, the residence of our esteemed correspondent, Mr. John W. Moir. Noreports from Fort Johnston have been received, and those from thirteen other stations are more or less incomplete, owing to the occa- sional absence or the illness of the observers. Dr. James E. Mackay, of the London Missionary Society, whose valuable report for Kambola we published last year, has, we regret to say, given up his meteorological work, owing to ill health and the impossibility of finding a trustworthy native assistant. He writes: ‘I see no way to get regular observations, and have, with great regret, resolved to give it up rather than provide unre- liable and worthless reports.’ British East Africa.—Returns from ten stations have been received, including three months’ observations from Nairobi, to the north of Machako’s. The returns from Fort Smith, in Kikuyu, and from the neighbouring Scottish missionary station being incomplete, we defer their publication until next year, as we hope shortly to receive the returns for the missing months. No report has been received from Golbanti, on the Tana River. As an instance of the extent to which an injudicious exposure of the thermometers may affect the returns we refer to the ‘ Notes’ on those received from Machako’s. We record with regret the death of Mr. C. H. Craufurd, one of H.M.’s Sub-Commissioners, who has at all times taken a lively interest in the work of your Committee. Uganda.—The observations on the level of Victoria N yanza having been received only up till October, the publication of the results a deferred till next year. Your Committee cannot conclude this report without expressing their sincere regret at the death of their late colleague, Mr. G. J. Symons, F.R.S., whose valuable counsel they have enjoyed ever since their for- mation in 1891. Your Committee propose that they be reappointed for another year, to enable them to make a final report. They do not ask for a grant. 1900. 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Be ee ee S o a Ll aeshcomee A teat kK } 2 | attr wocnityue of Eee Blealwalwy) | Z| » 2 qquOyY BSEO EE emt] 2 ul Weal se heen ites g |e 1-0) PHoIO wetee ee | : 618 ®)/4 |] e-| 8 wa fia |* : + =a isa =) T WY eT ae Sn Nee D. = a Le = iS (a) — Sea as E, pea ea seis 8) 8 | 2 S wee do 8 g& . muy |S iow ad (OT-0) puolp al ee So cero 418 REPORT—1900. Mombasa. 4:07° S., 39°7° E., 60 feet. Observer: the late C. R. Craufurd. Temperature Mean Temperatures STON Humidity, 9 a.m. Rain Pressure! ae 4 ‘. Month |%Atmo- FL oe oa 12 | ott a) eam a here Dry | Wet |Mean|Mean|Mean|] & 2 Henge se] 38s aS 3 ele | a M. i 5 ee aoe em 9A.M.|9A.M.| Max.| Min. /9a.m.| S agc\|ss|Ski-8 |S lgsc EBs Pa | ea} < shar} 1899 In. o ° ° o 5 3 5 z a In P.c. | In. |No.| In. January . | 29°851 | 82°9 | 79°7 | 86:4 | 80:3 | 83-4 88 78 61 | 78:2 962 | 85 003 | 1] *03 February . *838 | 84:0 | 79°6 | 87-2 | 80:4 | 83:8 89 78 68 “4 961 82 00]; Oo; — March . "847 | 83°9 | 81°2 | 87:5 | 81°7 | 84°6 89 77 5°8 | 80°3 | 1:033 89 3°45 8 87 April 5 "844 | 85:4 | 82°9 | 887 | 83:1 | 85:7 90 845] 56 | 821 | 1:096 90 1°65 4] 111 May. . *891 | 78°9 | 77°4 | 83:8 | 75°5 | 79°6 89 74 83 | 76°7 917 92 |14°86 | 15 | 2:78 June. © *986 | 79°0 | 77:2 | 83°4 | 75:2 | 79:3 84 74 82 | 76°5 912 92 *82 4 71 July . - | 30010 | 771 | 75:1 | 83°0 | 73°3 | 78-1 83'°5| 73 97 | 744 847 91 4:92 | 14 | 1°55 August . 004 | 77°8 | 76°7 | 83:0 | 73°5 | 78:2 83 73 95 | 76:3 905 | 95 3°11 | 11 | 1-01 September “012 | 79°9 | 786 | 85:4 | 768 | 83:1 86 76 86 | 78:2 962 94 1:48 | 10 61 October . | 29°938 | 82°5 | 80°1 | 86:4 | 78:0 | 82:2 88 77 84 | 79:3 999 90 33 7 15 November "881 | 84°7 | 83°0 | 87:2 | 82°5 | 84:9 88 81 47 | 82:5 |1°108 92 2°01 | 10 69 December . "837 | 84°8 | 82°5 | 88:5 | 82-4 | 854 89 81 61 | 78:8 984 88 2:50 | 10 | 1:05 Year 1899 | 29:911 | 81°7 | 79°4 | 85°9 | 786 | 82:3 90:0} 73°0| 73 | 785 | :974 90 |35°16 | 94 | 2:78 » 1898 906 | 80°3 | 75°6 | 82°9 | 75°38 | 79:3 890) 70:0} 71 | 73°8 -| -832 81 | 63°24 | 94/41 All readings have been corrected for instrumental error, excepting those of the barometer (see Report for 1898). The barometrical observations have been reduced to 32° F. and to standard gravity in Lat. 45°, but not to the sea-level. The mean temperature is assumed to be the mean of all max. and min., and is therefore too high. The rainfall in 1899 was the highest experienced since 1895, The average, 1891-99, has been 47°36in. The relative humidity in 1899 would appear to have been about 9 p.c. in excess of that of previous years, if the wet bulb readings can be trusted. Shimoni (Wanga). Lat. 463° S., Long. 39°35° LZ. Observers: M. G. Carvatho, A. C. Hollis, and E. J. H. Russell. Humidity, : Rain Prevailing Wind at 9 A.M. Atmospheric he 2AM Mon |e ees ho aoe: al BE 23) 2 |» Bae a Lalo} S BP oboe E 23| 22 |B 8 | 2 /es8| N.|NB/ Bs.) s. |s.w.| w. |N.w.|Cal. ] Ay Ee Os A os 9 A.M.) 3 P.M. Dry| Wet A | ava 1899 Tn ain | to lo | o 1 ame | Pes] ne No:|eene January . |29°849 |29:801 | 83:8) 80°8) 79°8] 1016] 88 | 0°32} 3] 0:22} 3|16)12)—};—}; —}|—j —}]— February . *830 | °777 | 84:1) 81-6] 80°8| 1:050| 89 “00 Oo; — 2;20; 6;—;—/] —}|—]}] —|]— March . *861] *800 | 83°5| 81:5] 80°9) 1°051| 92 | 1°52 | 10 35 | 2)}—)]14}—)]14] — it —|— April 5 *903 | *850 | 80°8| 79°1] 78°5| °973| 92 | 7:53 | 14 | 3:00 | —| —|—]—] 30} —]—] —]|— May. ° *912| °872| 76°9| 75°2| 74:5) °852) 92 | 27:05 | 19 | 4°60 | — | — | — | — | 29 2;—{| —|]— June. - |80°031 | °923 | 76°0| 74°1| 73°4) °820] 92 | 2:44 8 64/—})]—}]—]}—]; 30; —|—]}] —]— July . » 028 | °995 | 75:0} 74:0] 73:6] °827| 95 | 7:71 | 13 | 1:50 | — | — | — } —] 31 —}|—|] —}]— August . *014| °971| 76°0| 75:0) 746} *855] 95 | 1:48 a 40) — | = 1) 807) fa September *029| °969| 76°7| 75:1] 74°5| 852] 93 “41 3 21);—}—|—] 35 _ —|-- —|— October . “005 | °878 | 77°7| 76:2] 75°7| *886| 94 “99 3 50 | —|— | — | 28 3 —|—}] —|]— November |29°959| °875| 81:0) 78'7| 77:9} *954| 91 “75 3 3} —|—| 7] 17 1 —| 4) —j— December. | *896} *835 | 83:2) 81:1] 80°3) 1°03 3] 91 | 2°31 8 50/—] 3/18] 3 3 —|} 4] —{[— Year 1899 |29:943 |29°879 | 79°6| 77°7| 77:0] °927| 92 | 52°51 | 91 | 460] 7 | 39 | 57 | 79 |171 2 9}; —}J— >, 1898 901} — | 80°7|79°1) 785) °974] 93 | 27°30 | 85 | 2°80 | 10 | 12 | 69 © 25 | 72) 138 | 27 12 | — Al! readings, excepting those of the ‘dry ’ bulb, have been corrected for instrumental error (see Report for 1898, p. 606). It seems there is now a second ‘dry bulb’ thermometer, in addition to that attached to the barometer. The readings of the two are in most instances identical, the mean for the year of the attached thermometer being the same as that of the ‘dry’ bulb inserted in the table, viz., 77°7° F. Nairobi, 1:3° S., 36-95° E., Alt. 5,460 feet. Rainfall in 1899 :—October, 4°62 in., on 5 days. November, 2°30 in., on 10 days. 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Wr aan sa N TIAON APIS OY} YITM ‘UOTWNIIS o[qvANOAr] B UT Tena s 2 ENA) AD NLD fo ainyouaduay puv (9-0) aauag ‘houanbasg “pont s OYD (pent1yW09) s,oynyouyy * || *zeArasqo a9 Aq WAATS JOU a1v JOJoTMOMIA0T4 parjoryqe : P Ne let Ra Od 2 == = — —— || oq, Jo sSutpvaa ox sv ‘WorgeqIsoy our (210729 219m) apysag panurjuor ae oy | wayorq AT[eyuaplooe wdeq Suravy ssejs Buy TOTBFISOT OULOS HTM poateoareq || peovld ne sedis cing a | ins: eee 4snsny 10jje SUOTyeATOSqO O ie ip a ra Firanad Damp eal an CeO enies ne “oGh “Ul UL ree ayaa Suet a eta oe ete kite Detaiec ic "810119 [RITOTAN.AYSUT LOF pa: ; Uaieds erode} pavpurys || ‘as ots : UT] 1oOULOUI-LO or) 5 ae ae SUI Loy payoa1100 are SUOTZBAIASqO ITY 04 regntes waeq SABT sSurpeax TeEMaMIOUEY a Osh oq] euvo syueTINASUy Jo 498 Meu B qoquiaydagy seam iA he a | : L| #8 | G6 |8-92 |3-82|0-68| S68T “ pe | tt — | 182 aaneen| | l Lat ere ; = S| = |= | | oe | ove, fis ese 8st sex | Ly | 2e.| Over| — lete| — \eebee| eset xeox |= aoe | Se | Eby) FE | SSF: | Gs | bee | tap | engt aeox — |= |= L : is | 28 | oF. : 26.66 | ¢ vox cs 8:16 OL . | 9g¢ | 89 | Too 5 J [= l=P= le) agree emless| comet) = t/a [Slee] = pee fuemoma| 68 | it) ar] Se te om Gab) 528 20h) antag a — |=} = | 6g | ceorleog tis ioes| * 2q0300 || — | —| oo. [eae 6-£8| — |968- | -aoquieaoy || gz, AL |G | #8 | OFS | GID | 8:29 | 1-99 | toqmeAON is — |—| — | 86 | 098. (tes 882 8.08 requisqdag || e2 pete ene leat GOB" « LPS.G6 | eos) Pel = lean | ooralltmee |e leans pO | eal tocmeutae By 06. z GO hae. lcepac (aerlgenlmarlss “aanemy ee it QZ. 16-62 |G-6L'\086- |8c0- raquiaydag ies ae o . PL eer. 0-¢¢ | L-8S | 9-89 araqmaydag ort 1s | ees | ee | eee loszizozinen/* Amel) se. | 0 set lees |o.az ote. |eo0. |> senany || gc | er. |S koe | ea | se | one | p36 ay 2 z, Oni ae ol aerel tesla: «lowes ead ’ ale - | OL | STS |Z-62 \€-82'/996- |TE0-08 | + sme 9. bike 92 | ¢2| FL. | OTS | FS | 8-69 | - * Ane io) agFelree (osgr ae ogee \suzleeulies | ~~ 5 ue |} Bit | sr | 129 Hrs BBE (008. lees. || -ebtip loge learn lo oeetten | ereheege P-V8.). PEO) | eee oe. |z | or | 9 | 266. le.62 (9.08 ie : Sain, ae: g 56-3 TZ8 |8-18 692+ $98. : KU He ae a ye GL | TL | FL9 | 09 | 8-99 | * * AvW Sage op | 296. lees lee. leea| ° Clea elke GG. 6.98 §-F8 Le GGg. . Tuy llumael eacice Ee FL a6F- 9-89 | ¥-19 | 0-29 | © qudy = — | 00. ge | zie. legs lacs loge | ° canton = = a F-28 P18 91. |L98. . yore | o.e an. : aor 09 | 2% | GF | P69 | ¢89 iden ; — | 00.0 | 98 | cee. \t-62|T-08 T.e9 | * Axenuep NE a 0. |@.18|2-08 \96Z- |ZL8- + Areniqagq || 6g 0% 4 . 19 | OFF | G-9¢ | T-09 | 6-89 BN.1G9] Te | PONG UT Ora tT i “ 668 ae 00-0 |9-18 $08 |9L2-66 |P98.66 | + 85°3 722 88 70 20°72 20 5°45 S.W. — 2 September . 2 . 80-4 72-0 90 70 10°94 20 2°45 S.W. — af October . 5 . 850 73°9 90 7 6°28 15 1°32 S.W. 1 — November . . ° 86:0 747 89 70 971 ll 2°83 N.W. 2 4 December . : 5 85°9 765 89 72 0°34 4 08 N.W. 7 = Year . . ‘ . 87-5 74:4 97 65 98°60 169 5°45 N.W. 35 39 The observations are published as recorded. REVISION OF PHYSICAL AND CHEMICAL CONSTANTS OF SEA-WATER. 4.21 The Revision of the Physical and Chemical Constants of Sea-Water.— Report of the Committee, consisting of Sir JoHn Murray (Chair- man), Mr. J. Y. Bucuanan, F.R.S., Dr. H. R. Miu, Mr. H. N. Dickson (Secretary). (Drawn up by the Secretary.) Tue Committee was appointed to co-operate in the investigations under- taken by Dr. Martin Knudsen at Copenhagen, at the instance of the Committee appointed by the International Conference held at Stockholm last year, with the view of making authoritative determinations of the constants used in reducing observations of the physical and chemical conditions of sea-water in different parts of the globe. The grant placed at the disposal of the Committee has been expended in defraying part of the cost of Dr. Knudsen’s researches. Dr. Knudsen reports that the work of obtaining samples of water from different regions has been completed, except with regard to those from the East Greenland polar current, the northern part of the Baltic, and the Indian Ocean, which it is hoped will be received in about a month’s time. The samples have been collected in six-litre bottles, prepared by standing full of hot water for a month before use. Dr. Knusden and his assistants began preliminary work in September last, and since May the regular analyses of samples have been carried on by himself, two chemists, and three physicists. The results obtained so far indicate that the methods em- ployed are adequate in scope and precision, and sufficient progress has been made to justify the expectation that the. work will be completed and pub- lished within the time arranged by the Stockholm Committee. The Committee do not ask to be reappointed. Future Dealings in Raw Produce.—Report of Committee, consisting of Mr. L. Li. Prick (Chairman), Professor A. W. FLux (Secretary), Major P. G. Craiciz, Professor W. CunninGHAM, Professor F. Y. EDGEWoRTH, Professor E. C. K. Gonner, Mr. R. H. Hooker, and Mr. H. R. RaTHeone, appointed to report on Future Dealings in Raw Produce. (Drawn up by the Secretary, with the assistance of Mr. Hooker.) . [PLATE IV.] TABLE PAGE Il. Farm Prices in December of each year, and Prices at Chicago of (a) Wheat, (6) Maize; also Average Export Prices and Prices at New York . . 433 II, Average Price of Wheat at Cincinnati, 1844-97 . . f . 484 Ill. Standard Deviation and Mean Weekly Movement of the Gazette Average Price of Wheat, 1850-99. . : 3 F : : ; IV. Average Price of Middling Uplands Cotton at Live 1801-1899 . : d cule 5 : " : - 435 rpool in each year, ° 3 . A : . 435 THE markets in which organised dealings for future delivery are carried on are concerned with many kinds of raw produce. It appears to the Committee that the circumstances of the markets which are concerned with such products as wheat, maize, cotton, and the like are so different from those in which the metals are dealt in, that no advantage would result from presenting an investigation of the two groups on common 4.22 REPORT—1900. lines. The one group of commodities manifests the general characteristic that the supply is not continuously produced, but that, speaking broadly, the supply for a year depends upon the results of a harvest which falls within a limited part of the year ; the demand for consumption is, how- ever, one which exists throughout the year, being roughly continuous. The work of dealers in these commodities is, therefore, to arrange relations between a spasmodic supply and a continuous consumption. With products of which metals may be taken as the type, there does not exist the same dependence of supply on the round of the seasons. Demand fluctuates ; but supply can, if necessary, be organised so as to provide a continuous output calculated to meet a steady demand of large or of small dimensions. It seems reasonable to suppose that the influence of the market organisation for future dealings on price and supply will not follow identical lines in cases so widely contrasted. As, further, the interest in the subject referred to the Committee is, in the main, derived from the questions raised in reference to farm products (and particularly in reference to grain), the Committee propose to confine their report to this section of the material which the reference to them might be con- sidered to cover. Should the questions connected with future dealings in metals appear of sufficient interest, a separate investigation may be directed into that subject by a committee suitably constituted. The problems which arise in connection with future dealings in produce are in some respects not unlike some of those which are discussed in Sir Robert Gitfen’s .essay on Stock Exchange Securities! but differences fundamental in their nature distinguish the cases of stock and produce dealings. If no other difference existed, the fact that the existing supply of raw cotton (for example) will be, in the main, used up in the course of a year, while at the end of a year the bulk of the existing Stock Exchange securities will still be found in existence, would differentiate the two problems sufficiently. The influences which determine the level of ‘values are certainly not identical in the two cases, so that the points which are of greatest importance in the discussion of the Stock Exchange will not necessarily need to be equally fully considered here, nor will the conclusion in regard to what Sir R. Giffen designates ‘ fictitious securities ’ be capable of simple application to what is sometimes called ‘fictitious grain.’ It may be not superfluous to sketch the leading features of the market organisation, the influence of which we seek to trace. In so doing, it will be necessary to remember that we have not simply to consider bargains, the fulfilment of which is contracted to take place at some future date. Tt need not be argued that such bargains are regularly made in every department of life, and that no very special interest attaches to the investigation of the influence of the custom of making contracts which, from the nature of the case, are incapable of instant fulfilment. More- over, such contracts are, in many cases, eminently speculative, though greater speculation may occur in cases where no such contract is made. The builder who undertakes to build a Town Hall at a definite price is making a contract for future delivery of goods ; but it is the builder who erects houses with the expectation of disposing of them when finished— who makes, in respect of them, no contract for delivery at a definite price and time—who is commonly referred to as the ‘speculative’ builder. Itis 1 Stock Exchange Securities: An Essay onthe General Causes of Fluctuations in. their Price. By Robert Giffen. 1877. —— I ON FUTURE DEALINGS IN RAW PRODUCE. 423 not unnecessary to recall such facts, inasmuch as some confusion frequently arises in reference to the relation of ‘futures’ and ‘speculation.’ As stated, then, the problem which needs investigation is not the influence on price movements of forward contracts, such as the purchase and sale of a cargo of wheat actually on passage which may be sold in anticipation of its arrival, but of an entirely different class of contracts. In these contracts one leading feature is that the goods bought and sold are not dealt in by sample, but their quality is determined by reference to certain standards established by some responsible organisation. In wheat the standard may be, for example, as in London (for American wheat), No. 1, Northern, or, as is usual in Liverpool, Vo. 2, Winter (or Spring) ; in cotton, it may be what is known as middling uplands when American cotton is in question, fully good fair for Egyptian, and similarly in re- gard to other commodities. The buyer need not be able to discriminate between good and bad wheat, he may conceivably not be capable of dis- tinguishing wheat from barley, but the quality of the wheat to which he becomes entitled is nevertheless determinate. Rules are laid down by the Associations of Grain Dealers in leading centres such as Chicago, Duluth, New York, Liverpool, &c., for maintaining the standard according to which any actual parcel of wheat is determined to be of standard giade or not, the American centres further grading into several classes, under Government supervision. One distinction between dealing by sample and dealing in standard grades is that in the former case slight difier- ences would be likely to exist between the qualities to which any two bargains had reference ; in the latter case all bargains in a standard grade are on the same level in the matter of the quality of the produce which is capable of being used for their fulfilment. Further, by custom or by rule, the quantity dealt in on any contract is, if not the same, always a multiple of a standard quantity, ¢.g. 4,800 or 5,000 centals of wheat in London and Liverpool respectively. Tf, then, the date named for delivery be the same for any two con- tracts (and the custom of naming, not a day, but a month, or two months even, within which delivery may be made, helps to produce ready coincidence in this matter), the only point of difference remaining is the price. Different contracts for the delivery in one and the same month of the same number of units (of wheat or cotton or other produce) of the usual standard grade will, except in the matter of price, be as nearly identical and as interchangeable for all practical purposes as two bonds of a municipality for equal amounts, if not as much so as two Bank of England notes of the same denomination. To the man who has bought and sold equal amounts of the same grade for the same period of delivery there remains no concern in the actual goods ; he is concerned merely in the relation of the prices of the sale and purchase. But a further development of the organisation of markets where this class of business is largely transacted is also of importance, as affecting the facilities for carrying on such dealings, namely, the establishment of Clearing Houses, and the introdiction of a system of periodical settle- ments. These are effected daily in some cases, weekly in others, while in some markets no settlement takes place before the term of the bargain has expired. To indicate the purpose and operation of clearing-houses and short settle- ments, reference to a hypothetical example may be made. Suppose that in January A sells 50,000 centals (or, say,10,000 quarters) of wheat to B, 424, REPORT— 1900. (The standard grade need not be here specified, provided that the fact that the bargain is one in wheat of a named standard grade be remembered.) The wheat is to be delivered in May, and the price to be paid is, say, 6s. per cental. Suppose the term to run out and that B has not found a convenient opportunity of reselling at a profit—in fact, that he expected that the price would rise, while it falls steadily and persistently. When May comes B must either take charge of the wheat and pay for it in full, or, if he has no facilities for doing so, will be forced to sell ; in fact, the latter may be his only means of providing the funds with which to pay for his purchase. If the price has fallen to 5s. 6d., he realises 1,250/. less than he needs to make this payment. Should this be not a solitary contract, but one of a score, averaging equally bad results, the dealer, if not a wealthy man, may find it difficult to provide the means of paying for his purchases, and his bankruptcy may prevent such payment being made. The holder of the wheat, A, may find that such a failure of B leaves him to sell the wheat as best he can, and face the loss the risk of which his sale to B ought to have removed from his shoulders. The short-settle- ment system aims at reducing the risk of loss due to the assumption by weak dealers of risks greater than the funds at their‘disposal enable them to cover, and thus at rendering business more secure, and, being more se- cure, capable of being carried on with narrower profits. The parties to the contract may (or in some cases must) deposit a sum of money sufficient to cover any probable loss due to variation of price for a short time, and, if prices vary beyond what the deposit can make good, must increase the deposit. Thus, in the above case, the deposit may have been, say, 5 per cent. of the contract price, or 7507. Should the price fall so as to indicate to one party the loss of the whole of this margin in case of realisation at the price of the day, he may decide that it is better to acceptso much of loss than to risk a greater, and he is helped to this decision by the need of providing the means of meeting a greater loss, should it occur. The man who would be most likely to fail to meet his obligations on their maturity being, in general, the man most likely to find it difficult to spare the deposit money from his business capital, is precisely the man who is, so to speak, warned off by the pressure of the need to maintain the deposit. In the case assumed, were the official price to fall to 5s. 11d. on some day shortly following the conclusion of the contract, the buyer would be required to find 50,000 pence, or 208/. 6s. 8d., and to pay it, together with a further margin. Should a further fall occur he would need to pay a corresponding sum, while, in case of a recovery, he would be entitled to receive part of his deposit again. This necessity to face losses as they occur may be a hardship to a man whose ultimate forecast of profit is realised, should the market go against him steadily and heavily for a con- siderable part of the period between the contract and the due date of its fulfilment. Yet, on the whole, the short-settlement system and the putting up of margins do certainly tend to prevent men from assuming risks beyond the power of their means to cover. The fact that, to persons who would have no desire to make a contract for future delivery of goods and to accept delivery in due course, a facility is afforded to operate on the market and to attempt to snatch profits fron day-to-day fluctuations in prices, the daily (or weekly) settlement enabling them to make their attempt and be very shortly free of all responsibility in regard to it, not needing even to wait for the distant delivery month for the realisation of o j _ ON FUTURE DEALINGS IN RAW PRODUCE. 425 the profit (if any) they may make, has been used to cast odium on the system of short intermediate settlements. It is true that the system does offer facilities for speculation in mere price-movements as distinct froin dealing in commodities, but the other fact must also be borne in mind that it serves to check wild speculation by weak dealers unable to meet the losses which they were nevertheless very ready to face before the system was introduced. The example of direct dealing between two persons, which has been used, will not serve to give an accurate idea of the situation. It is common to have a large number of persons involved in such transactions. Not only have we A selling to B, but B to C, C to D, and so on for a score of links perhaps. The liquidation of such a transaction is greatly facilitated by bringing the first seller and the last buyer into direct relations with each other, since the intermediate dealers are concerned (unless in case of a failure to fulfil contracts) only with the differences between the prices at which they have bought and sold respectively. The unravelling of the complex series of payments and passing of delivery orders, &c., which, in a long series, involved delay and difficulty when no organisation for the purpose existed, is, in many leading markets, accomplished through the medium of a clearing-house. It is unnecessary to describe the organisation in any detail,' though the existence of these facilities must be borne in mind, inasmuch as purely speculative transac- tions, as well as the process of dealing in which actual delivery of goods takes place, appear to profit by them. In particular, one feature has attracted some attention and provoked adverse criticism, namely, that where the necessities of business bring about a state of things in which the original seller becomes in turn a buyer of the same delivery, the series of dealers, A, B, C, D, &c., ends as well as begins with A, and the passing of any warehouse receipt or other form of claim to a specific lot of goods becomes a mere form. The interests of all parties in such a closed ring are confined to price differences. The settlement of such transactions by the process of ‘ ringing out,’ when an invoice and a formal tender are passed round the ring, appears to some to indicate an objection- able facility afforded to those who practically bet on price-changes, and it is apparently desired in some quarters to suppress these facilities in order to suppress the transactions thus described. The result of the elaborate organisation of markets for dealing in futures in commodities is that it has become possible to buy or sell for future delivery without difficulty, and at prices publicly and regularly quoted. Those who desire to ensure supplies of any commodity for which a market so organised exists can do so without difficulty, while those who desire to secure themselves against future fluctuations in the price of raw produce, whether as buyers or sellers, are provided with the means of doing so. Attention must be particularly given to the use of dealings in futures in providing insurance against price-changes, for no small amount of importance attaches both directly and indirectly to this. It accounts, in part, for the fact, so troublesome to some critics, that far larger amounts of produce are sold for future delivery than could possibly be delivered. The tenderable quality is determinate, and though there ' For details as to cotton dealings in Liverpool, ef. Ellison’s Cotton Trade of Great Britain, chap. iv. 426 REPORT—1900. may ke enormous quantities of produce of inferior quality, it cannot be tendered in fulfilment of an ordinary future contract ; or, if tenders below the standard quality are, as in some cases, permitted, the limits of such deficiency in quality which are acceptable are narrow, and a pecuniary allowance must be made for the deficiency. The purchase or sale of regular futures-contracts is made, however, to serve as a hedge against too great loss from the variation in price of classes of produce not actually deliverable on such contracts, and, indeed, for some dealings in goods produced from the raw material to which contracts refer. This use of the futures-contract depends on the fairly close accord between the movements in price of different quali- ties of the same commodity. The accord is not exact, but it generally suffices to render the hedge effective in some degree. To illustrate, we take the spot prices of middling American cotton and good fair Per- nambuco at Liverpool on March 29 and May 17 of the current year. The former stood at 5,%,d. at the earlier date, 5.4,d. at the later. The Pernambuco quotations were 6d. and 53d. Of the variation of 1d. shown in the latter price, ;,d. were shared by the former. Hence, in a great degree, futures in American would have served as a hedge against variations in price of Pernambuco almost as well as against variations in price of American itself. As a direct insurance in dealings in the same commodity as that named in the futures-contract, that contract is obviously serviceable. An importer who purchases a shipload of wheat, anticipating to sell it on arrival at a certain price, will sell futures to an amount corresponding to the quantity of actual wheat he has bought. Ifthe price has fallen when the goods arrive, the amount received from their sale will be reduced, but, on the other hand, the cost of repurchase of the futures-contract will have also fallen, and to an amount which will cover the bulk, if not the whole, of the loss on the sale of the actual grain. So, also, in case of a forward sale, the risk of loss through price-variation may be effectively insured against by a purchase and subsequent resale of a futures-contract. The facility of dealing in these contracts, then, affords a means of reducing risk of financial loss in the handling of the actual produce, both that which is of such quality as to be tenderable on the contracts, and that which is not of such quality. Its use in covering the latter class of dealings leads to a considerable excess of dealings in futures over actual deliveries of tenderable grades. Now, in considering the influence on prices of the modern system of dealings in futures, the reduction of the risk assumed by various sections of dealers must be given a prominent place. The margin of profit which is sufficient to support dealings of a comparatively safe character is much smaller than that necessary when risk is considerable. Even though the goods pass through the hands of more numerous dealers than formerly, the cost of handling may be reduced through the reduction of the risks of the dealers. We have been unable to obtain any satisfactory means of determining to what extent the cost of handling (apart from elevator charges and freight charges) has been reduced, but we have seen no reason for supposing that it has been increased, as seems to be suggested by some who direct atten- tion to the large number of hands through which a futures-contract may pass, and the accumulation of commissions which is suggested in conse- quence. The fact that dealings in wheat futures in Liverpool, for example, amount to from twelve to twenty or thirty times the amount of F 4 i ON FUTURE DEALINGS IN RAW PRODUCE. 4.27 the wheat actually tendered against these dealings, does not necessarily imply that every quarter of imported wheat has to bear the weight of a score of commissions to brokers for handling futures-contracts. It seems hardly necessary to repeat at length what has been sufficiently often made clear, that the futures-contract entered into by a dealer who actually proposes to demand delivery of, or make a tender of, the produce represented by it, cannot be distinguished from the contract entered into by a dealer who does not propose to handle either the goods named in the contract or any other goods in respect of the price-variations of which the said contract may be used as a hedge. The point may be made clear by giving an example of the actual form used, selecting for that purpose the following :— No. 26—FUTURE DELIVERY CONTRACT—AMERICAN RED WHEAT. THE LIVERPOOL CORN TRADE ASSOCIATION, LIMITED. VOW LA NEM AXON OD Cope spent se aSe O00 Se IIe GeO 1S heeepsock Wievhavetnisnday, SOLD NGO... .ccs....cccc oes sccaaresrebeacerseccoasnees saeedaac on the terms of the Printed Rules of the Liverpool Corn Trade Association, Limited, snensgnmhandontsnacbendanSnenens SAY... .csecesceseescceeeeeeseess-Centals American Red Wheat (grown Hast of the Rocky Mountains in the United States of North America and Canada), of quality not lower than the Standards of No. 2 Winter or No. 2 Spring, as adopted by the Liverpool Corn Trade Association, Limited, and in force for the specified time of delivery, at............scseeeeeeees per 100 lb. BOWDEVGCIIVETEO GUPING Ts ,ccatessescrciiascveacouaddsasacnd ex store, in Liverpool, or, at Sellers’ option, in Birkenhead at.an allowance to the Buyers of One Farthing per cental. The Wheat to be in fair merchantable condition; a slight dry warmth not to be objected to. Payment—as per Rule 8, allowing interest equal to three months from date of being ready for delivery. This Contract is made between yourselves and ourselves, and not by or with any person, whether disclosed or not, on whose instructions or for whose benefit the same may have been entered into. Amended 18th October, 1897. In force on and after lst January, 1898. This Contract was made on the date specified, and within the business hours fixed by the Liverpool Corn Trade Association, Limited. Entered at Stationers’ Hall and sold only at the Clearing House of the Association. The examination of this form will suffice to show that it would be a practical impossibility to distinguish the simple gambling from the (so- called) legitimate dealings for the purpose of suppressing the former. Apart from objections to gambling as gambling, the allegations as to the effect of modern dealings in futures appear to attribute to them influences of two kinds : (a) that they tend to depress prices, and are in fact respon- sible for much of the fall in price of such commodities as wheat and cotton which has taken place in the last twenty-fiye years ; (b) that they cause market-prices to be much less steady than they would be if left to be 428 REPORT—1900. determined by the transactions of dealers handling the actual goods alone. It will be convenient to consider these views separately, and to make such comparisons of the actual course of market-prices as seem most likely to throw light on the subject. First is the influence on the general price-level. The reason for asserting that this has been depressed by dealings in futures appears to be, when the statements of the advocates of this view are considered, chiefly that other causes are inadequate to produce the result actually experienced. We do not think it is necessary to support our dissent from this view by indications of the influences to which the fall in some prices, especially those of wheat, maize, and other grain, should be attributed. To do so would be to travel far outside the matter referred to us. It will suffice to say that we hold it to be necessary to show how the operation of the futures-market can depress the general price-level of the goods dealt in. In only one way can we admit a real depressing influence, and that is through reducing the cost of handling : 7.¢., the price may be reduced to the consumer without a reduction of price to the producer of the raw com- modity by cheapening the marketing (as well as the freight) charges. Such a reduction of price would reduce the return to all those producers between whom and the consuming regions but little expense of carriage intervened. It is an important point to examine, therefore, whether the return received by the American farmer in the great wheat-producing areas has been reduced largely—whether it has been reduced as much pro- portionately as have prices generally. This is a point not very easy to determine. The U.S. Department of Agriculture compiles a figure which is given as the average farm-price of wheat at the beginning of December. Comparing this with the average export-price of wheat from the U.S., we have (see for extended table Appendix) :— Ve Average farm price. Years ending Average export price. Cents per bushel June 30 Cents per bushel 1869-78 a : . 104-7 1870-79 5 27°6 1889-98 ‘ 9 . 665 1890-99 4 : “pela These figures indicate a fall of not very different proportions in the two prices. The freight-rates from Chicago to New York,’ compiled by Mr. J. C. Brown, of the New York Produce Exchange, show a reduction of the all-rail rate of over 12 cents per bushel, of the lake-and-rail rate of 11 cents, and of the lake-and-canal rate of over 9 cents, comparing the same two periods. Average Rates. Cents per Bushel. Years ~ Lake and Canal Lake and Rail All Rail 1870-79 . : 148. ‘ ; S760. 5 : 25°6 LS90=99 ae. r F Divion im ‘ Mest. . Z 13-0 The reduced cost of transportation seems, in the light of these figures, capable of accounting for all, and maybe more than all, the difference between the fall in the farm and export prices. If these figures were really representative, the conclusion would be that charges other than freight have possibly increased, since the fall in price falls short of the fall in freight, by the all-rail routes, between Chicago and New York. NOE Statistical Abstract of the United States. * ON FUTURE DEALINGS IN RAW PRODUCE. 4,29 It is not, however, satisfactory to compare the fall of price at a parti- cular date in the year on the farm with the average fall registered in a year. A distinctly useful corrective to the idea that the prices of recent years at places near the great producing regions are without precedent, is afforded by the record of monthly averages of prices of wheat at Cin- cinnati which are given in the ‘Cincinnati Price-Current’ (for table see Appendix). The range of prices of the ten years 1844-53 would compare quite closely with those of the past fifteen years. The lowest figures, those of 1894, do not touch the level reached in the course of 1846. It is true that for long periods —for example in the dozen years ending 1882—the fluctua- tions of price centred about a level some 50 per cent. above that about which the fluctuations of 1844-53, or those of the years since 1885, have centred. But it does not seem necessary to invoke the aid of the modern market organisation to account for a return to the level of half a century ago. It is further of importance to recall the fact that in another great staple, cotton, the lowest prices of recent years hardly fell below those registered early in the century. The table of average prices of middling American cotton, which is given in the Appendix (¢/. p. 435), shows that, whatever may be the influences which have depressed the prices of cotton of late years, the level reached is practically that of the period before the American Civil War. Any suggestion of the need of an influence from the futures-market to produce the actual result would appear unnecessary. It may be granted that absolute certainty cannot, on this point, be reached from the examination of statistical compilations. A considera- tion of the matter from the point of view of the probable influence of an active futures-market, however, shows no point where a permanent de- pressing influence can arise. The facilities for short-selling are, it is true, considerable, but the ‘bear’ must cover his sales, and hence he must, in the end, support the market by buying. And, it may be added, the organisation affords as great facilities to the ‘bull’ as to the ‘bear,’ so that, whatever the effect on the fluctuations of price, the increase of both buying and selling would hardly produce a strong pressure which, in the long run, is all in one direction. The depressing effect of sales of wind- wheat is hardly the same as in the stock markets is produced by the in- troduction of fictitious securities. The sales, as stated, must be covered by purchases, and that within a limited time. Hence the nature of the commodities ‘fictitious wheat’ and ‘fictitious securities’ is not the same. A not uninstructive illustration is afforded by the recent experience of the Berlin market. As a result of the Bourse Law of 1896, the active dealings in that market have been restricted within very much narrower limits than formerly. The form of contract which is no longer legal there is still legal in Liverpool, London, Amsterdam, and elsewhere, and to these- centres much of the business formerly transacted in Berlin is practically transferred. Berlin is cut off from that close contact with the world- market which was maintained so long as the methods of transacting busi-- ness there were similar to those in use elsewhere. The result is shown in the annexed table (p. 430), showing the average level of price in Liverpool, Amsterdam, and Berlin in each of the last eight years, from which it will be seen that the check on futures business in that market has certainly not raised the price there relatively to that on the great markets of the world. Berlin prices have shown, indeed, a smaller excess over those representing the free markets of Europe since than before the Bourse 430 REPORT—1900. Law. It should be added that there has been no change in the customs duty on wheat or rye to nullify the comparison. Wheat, per 100 lb, Rye, per 100 lb. Year Li 1 ; Berlin (c alifc asia Berlin Amsterdam Bees a. *d. a Sd: Sd: 1892 7 8% . ieee 7 82 5 93 1893 6 73 5 104 5 10% 4 72 1894 5 er 4 114 5 12 3 74 1895 6 2 5 22 Db op 3 74 1896 6 10 5 103 5 24 3 83 1897 7 Tz cal 5 84 4-3 1898 8 13 7 64 6 43 5 23 1899 6 92 603 6 42 b 32 Refarence may also be made to the fact that the active operation of a market in futures has not in every case been accompanied by a declining level of price. A conspicuous example to the contrary is coffee. The second, and in some sense alternative, suggestion as to the effect of dealings in futures, is that they result in greater unsteadiness of price than would exist without them. Here what may be called the theoretical presumption is rather of an opposite tendency. In the weeks following harvest, the pressure of abundant supply is likely to depress prices less, when, on the demand side, the provision for the whole season is regularly influencing buyers through the operation of a well-organised machinery ; while a secured provision for future needs through the same means seems likely to modify the pressure of buying in a market which for some reason is temporarily short of supplies. An active market will show more numerous small fluctuations, but the greater movements will, in the majority of cases, be reduced in intensity as the natural result of active dealings in futures. Corners are not excluded, but the growing magni- tude of operations is, as experience sufficiently shows, rendering successful manipulation of corners more and more difficult. An active market is frequently a sensitive market and subject to scares, but it is able to recover from these scares more completely and rapidly than an inactive market. The world-wide range of operations is a constant influence in restraint of manipulations contrary to the general movements which the actual state of supply and of demand tends to set up. The dealers who sell short in anticipation of a fall, or attempt to control supplies in order to profit by a rise, must either possess such large resources as to be able to force the market to move as they wish (and this, as stated, is becoming increasingly difficult on any extensive scale), or they must gauge correctly the movements before they set in. If dealers persistently opposed the trend of prices as resulting from actual supply and demand, they would as persistently lose, which would, in the long run, mean their disappear- ance from the market. In anticipating a movement which would in any case be realised, the force of the movement is likely to be modified. The attention of the Committee has been given to the possibility of measuring the comparative degree of stability of prices before and since the creation of the great trading in futures. For the purpose of gauging the relative degrees of fluctuation, in different markets and at different times, two indices have been worked out. One is the well-known Stan- ON FUTURE DEALINGS IN RAW PRODUCE. 431 dard Deviation, or, as it is sometimes called, the Probabie Error, of a series of quotations as compared with the mean of the whole series em- ployed. It seemed possible, however, that some serious fluctuations would escape notice in this measure, in cases where rapid but only moderately violent movements, now upwards, now downwards, charac- terised the market quotations. A few very large variations seemed capable of outweighing numerous smaller but quite serious movements. To avoid possibility of a misleading result, therefore, the mean actual difference between each quotation and that immediately following it has also been calculated, and forms a second measure of the degree of varia- bility of the price. In these comparisons the movements of wheat prices have been deemed sufticient. The available series of daily quotations did not extend over a sufficiently long period to make their use for our purpose quite satisfac- tory. To test in some degree how far less frequent quotations might be used without greatly disturbing the index obtained, some calculations were made of the Standard Deviation for certain daily quotations and other weekly quotations. The results indicate that the relative intensity of fluctuations may be fairly well measured by weekly prices. Tt may be added that the S.D. of a series of weekly prices coincided with remarkable closeness to that of a monthly series derived from them over a period of half a century. The percentage of standard deviation to average price is not widely different in the two cases. We have, there- fore, considered that the relative steadiness of prices may be sufficiently indicated from the weekly prices afforded in the Gazette Average Price of English Wheat. Has the English farmer been subject to a less or greater degree of fluctuation in the price of his wheat since futures-markets have dominated those prices ? In the diagram annexed (see Appendix, Plate IV.), and in the tables which accompany it, the comparison over fifty years is shown. Calendar years have been used because the use of a tixed date from which to reckon the cereal year introduced the difficulty that it sometimes threw price- movements of two harvests into one so-called cereal year. Were the cereal year able to be taken, the fluctuation shown might be somewhat reduced. The computation of the S.D. for these years, making each year begin with September, has been made, and no great difference would be shown had those results been plotted on the diagram in place of those for calendar years. The summary of the tables in the Appendix is as follows :— Gazette Average of English Wheat. Period . é - . 4 A | 1850-59 | 1860-69 | 1870-79 | 1880-89 | 1890-99 8.) GIN Mgs ROM eseebeds Hse “ae lise Sate Average Price s.d. per quarter ./ 53 4 |51 9 |51 5 |37 0 | 98 9 Standard Deviation . . i) Ade ae 3102) 1112) 2 68 Mean Weekly Movement 0105 | 0 8% 0 73 0 52 | 0 52 The gradual narrowing of the range of variation is a noteworthy feature of the table. The fact that, considered as a percentage of the price, the variability has hardly been reduced, is equally noteworthy ; but it is a disputable point whether the actual money amount of the variability is not rather to be taken into account than the percentage 432 REPORT—1900. variability. Attention may be especially called to the fact that, except for the disturbance due to the Leiter corner, the period of comparative stability in the Gazette Average Price, stability in the sense of freedom from violent fluctuations, sets in precisely at the time when the organisa- tion of the futures-markets had reached that stage to which their op- ponents attribute malign results. A comparison of the relative variability of prices in different centres is also not without interest. In the following table the movements in Berlin, New York, Chicago, and Liverpool are compared in each of the last four years, in shillings and pence per cental of 100 lb. B. | 1896 | 1897 1898 | 1899 Biya Sid, Sia ades Be Berlin: §.D. . 53 63 114 3 M.D.M. = = 2 8 Average Price 6.192 (sue 8 53 6 102 Winter Wheat/Spring Wheat |Winter Wheat Winter Wheat New York: §.D. | 78 1 pee | 3 M.D.M. 3 z es f Average Price 5 5t 6 3g 6 7 bY Ge Chicago (Spring): 8.D. . | 62 63 1 8 24 M.D.M. ; g z 1 4 Average Price . 4 53 6 oat Pade 4111 Liverpool: 8.D. . el + 98 1 53 1i M.D.M. é — 4 g 2 Average Price | _ 6 98 7 58 6 Of 8.D. = Standard Deviation, M.D.M. = Mean Daily Movement. The restrictions imposed on Berlin’ business have not, apparently, increased the steadiness of prices, which isa feature in which an influence was anticipated by the advocates of the restriction. We have failed to find any conclusive evidence in favour of the theory that prices have been depressed as a consequence of the development of markets for future delivery business, and have found reason for believing that in point of steadiness some change for the better is traceable since the influence of these markets became great. These conclusions are in accord with the deductions which a theoretic examination of the question ields. f In what precedes the word ‘futures’ has been uniformly used to indicate the kind of business contemplated. The distinction between the contract for delivery within a definite future period of time and the contract which confers the right to demand that such a bargain shall be entered upon at a definite price seemed to be conveniently made by reserving the name ‘option’ to the latter class of contract, although actual practice in this matter is not quite definite and consistent. To make a distinction not always made in practice seemed calculated to avoid confusion. ON FUTURE DEALINGS IN’ RAW PRODUCE. 435 APPENDIX. Taste I,—Wheat and Maize: Average Farm Price, Average Price at Chicago and New York, and Average Export Price in Cents per bushel. Wheat Maize Average | | | Average | Average Average Farm | Chicago New York) Export | Farm | Chicago|New York | Export Price Price Price Price -- J 1033 95 -— 433 57 — ~~ 46 113 95 — 31 60 — — — 113 112 — 27 61 |) — — 47 943 85 — 29 532 — — 55 96 90 —_ 4i 50 —_ — 52 974 86 — 36 503 —_ — 40 1033 104 — 25 65 — —r | 53 135 13 ==» ih 2ien| #845 = ea ie ae 131 =} | 33m) | | 63 -— — 59 =| 104 Ils |) = |, 405 | 7 62 = ay | Gere |f LOGye | 106 — | 34 | 61g = Oy tee 95% | 100 | — 33 63 — — | 41 1034 Gis, ye SS 374 66 id ete eae 1303 he | 47 71 — = 9% | 184 1650 46 (os a — 134 | 210 166 — 582 94 — = 118 159 W85 |. —=- | 425 69 te A= — 93 1483 13 | — 46 3 =~ —— 62 105 102 -—— 41 684 — as 77 123 95 = = 852 _ — (3 124 98 — a 73 —— — 714 111 123 = -H 59 64:1 93°7 734 1183 114 348 -- 59 55 114 97 1263 129 699 — 833 65°8 183-1 1403 1834 133 99°5 — 144 81:8 146°3 LY, 17534 194 46 o= 1234 130 219°6 | 1153 181 141. 68°2 = 88 81:9 SS LOS 228 127 795 — 1174 =| —-:100 142-4 176 213 190 62°8 — 120 1175 D2 elit) 14ax 139 75:3 — 100 | 96:8 104-2 | 92 118 129 54:9 = 995 | §92'5 1258 | 121 | 148 132 48:2 493 77 | 759 124 1203 1564 147 398 39 70 69°5 151 | 1142 1463 131 48°5 33 63 | 61:8 941 | 113 1423 143 64-7 64 85 Ven 100 ~—s-:101 TPA = 4| ela te 42 645 | Sle | 848 : 103-7 | 1023 123 124 37 454 623 67:2 1877 108-2 | 127 149 117 35'8 432 | 58 587 1878 acv | coos | 1212 134 318 39) j8 bs2 | 9562 ' Average farm prices frcm Reports of U.S. Department of Agriculture. Prices _ at Chicago and New York (spring wheat) from the U.S. Senate Report of 1893 on _ Wholesale Prices, Wages, and Transportation from 1840 to 1891; and for later years, _ for New York (winter wheat), from the U.S. Statistical Abstract, and for Chicago _ from Messrs. Howard, Bartels, & Co.’s Record of Statistical Information. 1900. FF 434 REPORT—1900, Table I, (continued)— Wheat and Maize: Average Farm Price, Average Price Chicago and New York, and Average Export Price in Cents per bushel. Wheat Maize ‘Average | | | Average | Average Average Year Farm | Chicago New York Export | Farm !|Chicago!| New York! Export |; (Price 4 | Price | Price | Price 1879) |) gOS 96 LG eel | 375 352 47 471 1880 | 95:1 | 1063 1230) 2b es esse 2G rs OT 55 | 54:3 1881 , 1192 | 1123 125 iil 63°6 | 49 613 55:2 1882 | 88 2 1223 | 129 ~ 4° 9 48-4 | 66 \ ya 66°8 88h a) | Ags 993 106 | its} 42:4 | 502 | 64 68:4 1884 64:5 85 | 95% 107 B57" | «54 61 611 1885 Targa 82 903 86 32°8 41 52 | 54:0 | 1886. | -68°7 77 87 87 366 | 36 47 | 4958 | 1887 68-1 75 87 89 444 | 38% 483 47-9 1888 | 92:6 | 842 923 85> | 84: 48 582° | «= 55'0 1889 |} 698 | 902 95 90 28°38 34 43 | 47:4 1890 | 83:8 85 91 83 50°6 35 | 433 | 41:8 1891 | 383'9 954 106 93 40:6 Dinu = on | 57-4 1892 | 624 (Cl ae sl 108 B93)" |) 46" | 54 5b] 18935 9|)\smpsre OB + ve 80 365) a) 39) || 250 534 1894 49:1 5 | 6ile 4) S6e 45°7 304 S61 | 46:2 | 1895 50:9 | 624 6% 4.2 358 25:3 40 473 52°9 HIG | 42:6)” | Gbe 78 65; 215 26 34 378 1897 80°8 86 | 955 75 26:3 253 32 30°6 ISGSee soerer | FQ | | Ober, |) 9398 28:7 314 375 || | 8bb 1899 | 584 713 | 793 75 303 334 41 Taste Il.—Price of Wheat at Cincinnati. Cents per bushel. Year ' Price | Year Price Year Price 1844 69 1863 | 79 | 1882 117 1845 70 | 1864 82 1883 107 1846 60 1865 115 1884 91 1847 83 1866 180 . 1885 93 1848 78 | 1867 192 | 1886 82 1849 78 1868 156 ) 1887 79 1850 86 1869 101 1888 92 1851 66 1870 100 | 1889 84 1852 62 | 1871 121 1890 89 1853 85 | 1872 141 \| 1891 99 1854 134 1873 132 | 1892 81 1855 156 1874 108 | 1898 64 { 1856 114 1875 100 1894 54 1857 107 1876 | 89 1895 66 1858 838 1877 | 131 1896 72 1859 117 1878 | 96 1897 89 1860 115 1879 104 | 1898 -— 1861 89 1880 Gh 1899 — 1862 B1 1881 12 | J Se oe ae if pe ee pat a ar ; [Prare Ty. 70th Report Brit, Assoo., 1960. L Standard De wand Mean Weekly Movement of ‘Gazotto' Price of English Wheat. Shillings a fly, - % = t I a2 SEH S76 At | S Het g? Tt eo 1 Le a +t 4 Wii i 4 Heit tt 36 1 y is + ¥ = 3 t Kd “5 10 17 *T2 75 Price of Middling American Cotton at Liverpo i isssasssecees | IT 35373535 G0 8 GE OS OF ES 85H | Tllustrating the Report on Future Dealings in Raw Produce, - ; ON FUTURE DEALINGS IN RAW PRODUCE. 435 T ‘A s Ill.—Average Gazette Price of English Wheat, Standard Deviation and ie Mean Weekly Movement. Shillings and Pence per Quarter. Average Standard Weekly lage Average | Standard ne ‘oki Price Deviation MWaveanent Price Deviation Mov al t ao d. Be the d. 8. dd. as (des d. 40 3 1114 6 1875 45 2 3 3h 83 Bie ef 2 02 52 1876 46 3 2 O88 53 40 10 1 8 1s 1877 56 10 5 102 123 bo I 10 72 13 1878 46 5 4 % 62 72 5 8 6 202 '| 1879 43 11 4 13 63 ~ 74 9 4 43 122 | 1880 44. 4 1 112 8 69 2 4 10 153 1881 45)5 2 10¢ 8t 565 3 98 105 || 1882 45 1 3 12 7 44. 3 YW | 72 {| 1883 41 7 1 32 35 43 10 3 7S 9 || 1884 3a9 2 7 $3 53° 3 6 O¢ | 102 || 1885 32 10 1 102 Ga 55 4 3 Of 82 1886 los 1 238 dy 55 6 4 73 Tz | 1887 32 6 2 12 5 44 9 2 73 54 || 1888 3111 b 102 53 40 3 eye 5 1889 29 10 0 7 3t 41 10 2 104 62 || 1890 ob 1 1 112 44 50 O 4 11} 102 | 1891 37.0 2 112 12 64 6 3 22 92 || 1892 80. 4 2 6 43 63 9 9 12 103 | 1893 26 4 0 104 23 48 3 2 104 82 || 1894 22 11 2 7% a2 46 11 4 22 92 || 1895 Zell 2 3 43 56 8 2 2 5S || 1896 263 2 104 5 HT V1 1 92 5 1897 3 3 Pe 53 58 8 2 10% 53 || 1898 34 0 6 12 102 55 10 7 (3 (Ke | 1899 25: 29 0 104 34 Pasty 1V.—Average Price of Middling American Cotton at Liverpool. In pence per pound. From Tattersall’s Cotton Trade Circular, 1899, ' Year | d. || Year d. Year d. 1826 62 1851 52 1876 62 1827 64 1852 5 1877 65, 1828 68 1853 53 1878 GE 1829 53 1854 53 1879 65 | 1830 62 1855 5a 1880 618 | 1831 6 1856 65, 1881 62 | 1832 62 1857 73 1882 62° 1833 gi 1858 62 1883 58 1834 ge 1859 63 1884 6 1835 104 1860 6+ || 1885 53 1836 94 1861 gee 1886 BL 1837 7 1862 172 1887 5h 1838 7 1863 234 1888 52 1839 Ti || 1864 272 || +1889 pis 1840 6 1865 19 1890 6* 1841 6i || 1866 152 1891 4u 1842 53 =| Ss: 1867 102 1892 45. 1843 42 || 1868 102 || 1893 43° 1844 4a 1869 +12! 1894 3:3 1845 4+ 1870 gis 1895 get 1846 4 1871 82 1896 gil 1847 62 1872 102, 1897 338 1848 42 1873 9 1898 ows 1849 BL 1874 8 1899 Be. 1850 7 1875 | 78 ad A36 REPORT—1 900. State Monopolies in other Countries—Interim Report of the Committee, consisting of the late Professor HENRy Sipewick (Chairman), Mr. H. Hiaas (Secretary), Mr, W. M. Ackwortu, the Right Hon. L. H. Courtney, and Professor H. 8. Foxwet.. Tur Committee have collected the materials for a report the lines of which were under discussion at the time of the Chairman’s last illness. It was hoped that he would be able to agree to a report by the end of June ; but as he was unable to sign a draft, the Committee have not proceeded further in the matter. They recommend that the Com- mittee be reconstituted under a new Chairman for the purpose of reporting at an early date, and be allowed to retain the unexpended balance of ihe grant. Small Serew Gauge-—Report of the Committee, consisting of Sir W. H. Preece (Chairman), Lord KEtvin, Sir F. J. BRAMWELL, Sir H. Trueman Woop, Major-Gen. WEBBER, Col. WarkIN, Messrs. R. E. Crompton, A. Strow, A. Le NEveE Foster, C. J. Hewitt, G. K. B. Evpninstone, E. Riee, C. V. Boys, J. MarsHaLL GorHaM, and W. A. PRICE (Secretary), appointed for the purpose of considering whether the British Association form of Thread for Small Serews should be modified, and, if so, in what direction. (Drawn up by the Secretary.) APPENDIX.—Report of Laperiments on Serew Threads made by J. MARSHALL GorHAM and W. A. PRICE . ° : : 5 : . : p. 444 Tris Committee was appointed at the Ipswich Meeting of the British Association in 1895, to consider repeated complaints that screws of the British Association thread, proposed by the Committee of 1882, obtained commercially, were not satisfactorily interchangeable. It was evident that the difficulty arose from the want of proper gauges, or other ready means of testing screw threads, and the Committee at once took steps to find out how these could be obtained. In a report presented at the Dover Meeting of the Association last year (1899) were described the efforts we had made to secure the production of these gauges, and to make them - generally available in a commercial way. We reported that a high degree of accuracy in dimensions, though not in form, had been attained in a small number of specimens submitted to us by the Pratt and Whitney Company ; that these were the product of exceptional skill and care ; and that they were only obtained after long delay. These gauges were sufh- ciently good for all practical requirements, and had gauges of the same character been generally available some years before, it is probable that the complaints which led to the appointment of this Committee would never have been made. Taking into consideration the difficulty that had been met in obtaining these gauges ; the representations made by the . manufacturers of the difficulty in producing them, and of the comparative ease with which a flat-topped thread can be accurately formed ; and the fact that such screws are used in foreign countries for the best class of engineering work, we reported that the form of the British Association thread was unsatisfactory, and recommended that the Committee should be reappointed to consider its modification. A proposal to alter the form of an established and generally satisfac- een 4 ON THE SMALL SCREW GAUGE. 437 tory system of screw threads may cause some apprehension among users of them, and the Committee, many members of which are intimately acquainted with the trouble and inconvenience incidental to a change of the kind, recognise that very substantial reasons are required to justify it. They think it desirable that the considerations which have led them to make this proposal should be fully stated. Consideration of the exact cause of the difficulty found in the con- struction of gauges for the British Association thread showed immediately that it was due to the rounded top and bottom of the thread. There is no difficulty in making any given angle between the straight portions or sides of the generating tool or chaser, but to arrange that these straight lines shal], at definite points, turn smoothly into circular ares of a given radius is a matter of some difficulty. The difticulty has been met with a good deal of success. The original threads, cut by Mr. Lehmann, and those produced recently by the Pratt and Whitney Company, are admirable specimens of workmanship, especially when the small size of the pieces is considered ; and to the careful work done by Mr. Lehmann in the years following 1882, when originating the threads, the success they have achieved is largely due. The production, however, of chasers, even if it can be repeated indefinitely, does not end the difficulty. The hardening of the screws produced by these tools introduces some inaccuracy. They are no longer perfectly straight, perfectly cylindrical, or of perfectly accurate pitch, and the only way to correct them is by grinding. The inaccuracies produced by hardening are not of sufficient importance to affect the use of taps, and in the case of die-plates the errors produced in the diameters are corrected by opening or closing the die ; but for gauges corresponding to modern ideas of mechanical accuracy the errors pro- duced by hardening are considerable, and much greater than those found in screws whose forms can be finally obtained by grinding. With the British Association thread this process does not seem to be practicable except perhaps in single specimens, and in this lies the inherent defect of the thread. A way out of the difficulty is offered by the adoption of a flat-topped thread, but before this can be discussed it is necessary to consider what are the peculiar advantages of the rounded thread, which have brought it into general use, and led to its adoption by the original Committee. The British Association thread was taken with a slight modification directly from Professor Thury’s Swiss system, which had been constructed by finding a formula to represent the average existing practice among Swiss clockmakers. Sir Joseph Whitworth formed his system of screws in a similar way by averaging the English engineering practice of his time. It appears that the object in view in both these cayes was to regularise exist- ing practice, not to effect a reform ; and that an alteration in the form of thread in common use was not contemplated. The same was done in America for the United States thread, so far as the pitches and diameters were concerned, but the form of the thread was determined by Dr. Sellers on general considerations. The origin of the round thread in the British Association system was in the common practice of the Swiss workshops when the rule was constructed. Now, whatever may be the prescribed shape of the thread, it is certain that small screws, produced on screw machines, will have rounded tops, and if a new rule for American threads were con- structed from the shapes of ordinary small screws found in the United States, the form obtained would have a rounded top, notwithstanding that they are ali supposed to represent the flat-topped Sellers thread. Since 438 REPORT—1900. a screw machine tends to produce rounded threads, and the natural course of trade conditions tends to the reproduction of current forms, the common use in Switzerland of screws with rounded threads does not necessarily show that such a form has especial merit, or had originally been delibe- rately designed. It may be only the result of working conditions. Professor Thury, in defining his thread, chose a form which could be easily produced with fair accuracy, is perfectly eflicient, and can be conformed Fie. 1. to in practice, but we venture to think it fails to meet other important conditions To ascertain the conditions which should determine the form of a screw thread, consider the mode of action of a screw holding two pieces together. In fig. 1 the screw serves to hold the plate a to the solid — part B, and a small part of the thread is drawn on a larger scale below. The action of the screw depends on the tensile strain due to the pressure ON THE SMALL SCREW GAUGE, 4.39 produced over the surfaces aa, aa,..., and the compression produced there by the act of screwing up relieves any pressure over the surfaces bb, 6b,.... Contact and pressure at the pointsccc... depend on the relative diameters of the screw and the tapped hole. The spaces shown in the figure along the surfaces } b, bb, . . . are of course greater than would occur in a well-fitted screw. Nowif the thread may be looked upon merely as a means of supporting the tensional strain on the bolt, without offering much frictional resistance to screwing up, it is clear that this will be most efficiently done if the pressure is evenly supported over the whole of the working surface of the thread a a, aa, . . ., and within the assigned dimensions of the thread this surface should be as large as possible. Contact and pressure at the points c, c, . . . depending on the respective diameters of the screw and the tapped hole may interfere with the fair contact of the working surfaces, involve extra resistance to screw- ing up, and, so far as the support of the tensional strain is concerned, serve no useful purpose. The best design for the thread, in view of its function of supporting the tension, is that which secures most perfectly a continuous working contact over the surface a a,a.a, . . ., and freedom from pressure atother points. These conditions are met best by a thread having straight sides, a flat top, and a clearance space at the top and bottom of the thread ‘such as is shown in fig. 2 (p. 441). The provision of straight sides gives a form to the originating tool which can be produced with more ease and accuracy than one of a curved form, and assists to secure correspondence between the surfaces of the screw and nut: the provision of a flat top gives the largest possible area to the working surface within the given limits of the thread : the provision of a clearance space at top and bottom removes the possibility of any interference with the fit of the working surface by irregularities of form at those points, and avoids unnecessary friction. Screws with straight sides and flat tops are perfectly satisfactory im in- strument practice, are employed in France and Germany for the most important engineering work, and are universal in America for work of all kinds, for instrument work as well as heavy engineering work. We understand that the provision of clearance is well recognised in the practice of American and French engineers, who use the Sellers thread, and Mr. Hewitt, at Prescot, gives a very liberal clearance in the screws manu- factured by him. The ease with which such threads are originated is a point in their favour, though it would be of small importance if it were shown that the thread is practically defective in other ways. As regards the reduction of the sectional area of the core by the pro- posed deepening of the thread, the figures obtained by Messrs. Gorham and Price, corroborated by common experience, show that screws give way under tension by breaking across the core rather than by strippmg their threads or those of the nuts ; and it has been urged against the proposal to deepen the thread that it weakens the screw in its already weakest part. The reply to this is that the strength of the screw is really determined by the strength of the core, and that the British Association series is so closely spaced that a screw can always’ be found whose core is of the required size. Moreover, in well-designed work, screws have so large a factor of safety that a reduction of the section of the core by an amount varying from 8 per cent. in large screws to 12 per cent. in small screws will not generally be a matter of great importance, though it will be remembered that the resistance to torsional fracture varies inversely as the square of the sectional area. 4.4.0 REPORT—1900. The adoption of a flat-topped thread with a clearance would, we believe, completely obviate the difficulty of producing satisfactory gauges, the question to which the attention of this Committee was originally directed. The construction of these is referred to later in the report. Other elements of the screw have received the attention of the Committee as follows. Mr. George M. Bond, of the Pratt and Whitney Company, has expressed to the Committee a strong opinion that the angle of 60° employed in the Sellers thread is most suitable for screws because of the ease with which it is formed. Tools can be ground without difficulty, and with great accuracy, to any desired angle, and Mr. Bond’s reason appears to the Committee insutticient of itself to justify a change in practice. Considering, however, the extent to which screws of the Sellers form are employed in foreign engineering work, the Committee desired to obtain some evidence of the exact value of the particular angle of 60°, since, if this angle were found to possess a great advantage over the angle of 473°, the adoption of the Sellers thread would have the additional recommendation of bringing the small screw practice into line with an already extensive engineering practice, while giving effect to the conclusions already reached by the Committee of the desirability of clear- ance and a flat-topped thread. Some experiments on lines suggested by Mr. Crompton have been carried out by Messrs. J. Marshall Gorham and W. A. Price, and their results are printed as an appendix to this report. They concluded that an angle of 471° is better for screws than an angle of 60°, on the ground that it offers much less frictional resistance to screwing and unscrewing on a given tensional load, and the general tendency of this observation is corroborated by the practice of using a thread for the leading screws of lathes, the serews of carpenters’ clamps, and of screw jacks, in which the working surface is perpendicular to the axis of the screw. Another consideration leads us to think it undesirable to adopt an angle of 60°. The advantage of bringing small screw-practice into line with that of foreign engineers will only be fully gained if their rule for the size of the flat top of the thread is also adopted. This rule gives a maximum possible clearance of +108 pitch when the thread is cut to a perfectly sharp y at the bottom. This clearance would be sufficient but tools with perfectly sharp points are maintained with difficulty, and it would not generally obtain. A tool of 474°, ground to give a clearance of +1 of the pitch, has a flat at the point one-seventh of the pitch wide. For small screws Professor Thury’s angle of 474° had the same sanction of practice among clockmakers as a larger angle had among engineers when it was adopted by Dr. Sellers ; and though it is often difficult to assign exact reasons for the particular practice of practical men, yet it cannot be disregarded unless the reasons for its use are quite clear, and are shown to be insufficient. We see no suflicient reason to change the present angle of 475°, especially as a change of angle would make existing stocks and tools altogether useless in conjunction with the existing form. The existing series of pitches and diameters, with their designating numbers, is generally approved, and the Committee have received no sug- gestion that it is otherwise than satisfactory. Thus far it has been assumed that, given the necessary tools, all forms of thread can be produced with the same ease. This, however, does not apply to the small screws used in watches, which are produced by turning the blanks into a hard die without cutting edges. In such a process ON THE SMALL SCREW GAUGE. 441 great force would be required either to squeeze the metal into sharp re-entrant angles, or to make it flow past sharp corners. On this point Mr. GC. J. Hewitt writes to the Committee respecting the proposed altera- tion of the British Association thread : ‘A die of this operating character for screws flatted top and bottom soon loses its contour, and needs con- stant replacement ; and in addition my experience leads me to believe that it requires more force than a rounded thread ; therefore it sets up more torsional strain of the metal, a factor of great moment where such Fig. 2. TABLE OF DIMENSIONS. em =pitch. EH’ ='6 pitch. AA='149 pitch, CO! =1'14 pitch. BOA'="655,, BE ='238)) ..; DD/='8 *: KODY = 415-- yr ='182 small diameters are being produced, breakage in the dies being a con- stant source of trouble even at the best.’ In the same letter Mr. Hewitt explicitly approves the proposals of the Committee for the larger threads, both as regards the flat top and the provision of clearance. Mr. Hewitt’s experience at the Prescot watch factory is so large, and his knowledge of the manufacture of watchmakers’ screws is so intimate, that the other members of the Committee have no hesitation in accepting his suggestion to divide the present series into two sections. The large section, consisting of what may be called instrument-makers’ screws, from No. 0 to No. 11, includes screws from 6 mm. to 1:5 mm., or in English _ measure from } inch to ‘059 inch. The small section, from Mo. 12 down- wards, consisting of watchmakers’ screws, includes screws below 1:5 mm., f=] ? 44.2 REPORT—-1900. or in English measure below ‘059 inch. The Committee propose to modify the form of thread of the screw of the large section only. The above considerations lead the Committee to propose to replace the present form of thread of screws from No. 0 to No. 11 inclusive by the form shown in fig. 2. Here the line A’ A A... . represents the outline of the nut, B) BB... of the screw ; andde/. . . is the outline of the present British Association thread. It will be observed that the flat part of the side, or the working surface, is increased by nearly 60 per cent. Accurately formed screws of this pattern for special purposes can be cut on the lathe with much greater ease than those with a rounded thread. The screw is cut with a single-point tool from a cylinder, and in the larger sizes the nut can be cut with a single-point tool from a cylindrical hole. The difficulty of forming chasers of a complicated form is entirely avoided. These observa- tions apply equally to the construction of taps and plates, and of gauge- pieces. Given that the pitch of the screw and the angle of the thread are accurate, and the sides straight, the fit of the screw in a correct gauge is determined by the length of the diametral line terminated by the in- clined sides of the thread, and this dimension is called the effective diameter of the screw. If this dimension is the same in the screw and the nut, they will fit without shake independently of the exact values of the external and internal diameters, or of the exact form of the ends ; and the lengths of the effective diameters of screws and nuts are definite numerical measures of their fits one with another. The point which it is important should be right is the straight between A’ and B in both nut and screw. The nut must not pass A’, nor the screw pass B ; but so long as the nut is cut as far as B or farther the shape of the excess does not matter. The same thing holds with the screw at A’, but here excessive clearance is objectionable because it weakens the core of the screw. In constructing plug-gauges for testing nuts the straight sides of the thread can be corrected after hardening by grinding with a lap, and this process corrects at once the irregularities of pitch and angle, and is continued till the effective diameter is reduced to the desired value. The top of the thread, being cylindrical, presents no difficulty. The form of the bottom of the thread is immaterial, since the clear hole in the nut is most conveniently tested with a cylinder plug-gauge. In the specimens submitted to us last year by the Pratt and Whitney Company this cylinder was constructed in one piece with the screwed plug. In ring or nut gauges for testing screws a slit is cut through the tapped hole, and closed with a screw. The hole can be polished by a corresponding screwed piece, but could only be corrected by grinding by the use of very refined appliances. After polishing the slit is closed to fit a prepared screwed plug, and the clear hole brought to its correct value with a lap. The process is not so satisfactory as with a plug-gauge, but the pieces which the ring is designed to test can be satisfactorily measured in other ways, so that the gauge is of less importance. The effective diameter of a screw is readily measured in a micrometer gauge between a conical point and a y-notch, both having an angle of 473°. An instrument of this kind constructed for 60° is figured in tool- makers’ catalogues. ‘ Ordinary taps for nuts or for the working holes in larger pieces will be different in form from the screws, and different from the taps employed to make dies or screw-plates. The ordinary dies or plates in a workshop Regi SS ‘ a i a i i a is | cael ea a 8g oe a) & = ON THE SMALL SCREW GAUGE, 443 used for making screws will not be suitable for making taps. In small workshops this may sometimes cause mistakes, but in shops having a separate tool-room this extra specialisation should present no difficulty. Objections have been raised to the above proposal on three grounds. It has been represented to us that in finely fitted work the screws should fit their holes perfectly and all over, and that the existence of a clearance gap all round the edge of the thread is inconsistent with a high standard of workmanship. This objection is evidently to some extent a matter of opinion, and it is always possible to use taps of the same form as the screws, so that the screws will fit the taps all over as in a non- clearance system. It has been objected that the introduction of the proposed system will seriously interfere with existing stocks of screws and the repairs of existing instruments. In fig. 2 it is'shown that the new thread differs from the old one by the addition of the small corners, y bh, h Bk, to the .screw, and d A’e, e A’f, to the nut. In making screws and nuts with dies and taps, these corners will always be rounded off to some extent, though the re-entrant angles at A L’ will be as sharp as the tool which makes them. In some screws and nuts prepared experimentally to test this point, the outer edges of the thread were fairly rounded, and they were perfectly interchangeable with the B.A. screws of an existing manufacturer’s stock. The Committee believe that screws made to the proposed new thread will, owing to the inevitable rounding, be interchangeable with existing stocks in a great majority of cases, and that only in cases where great care has been taken to work closely to the old standard will any difference be noticed. It has been objected that the proposed thread is unsuitable for such work as bicycles and small arms which are subject to violent concussion and vibration, whereby the screws are liable to be shaken loose and to drop out ; and the case of alternating current arc lamps has been men- tioned to the Committee as one in which the same thing is liable to occur. Mr. O. P. Clements of the Birmingham Small Arms Company contri- butes a paper to the Mechanical Section on the practice of his firm in the manufacture of screws for bicycle parts, for which it is found necessary to use rounded threads fitting very closely all over. It is clear that no one form of thread can be suitable for all purposes, and we have direct evidence that the form of thread we propose does not fail in instrument work in the way Mr. Clements anticipates that it would doin bicycle work. We beg to report that the system of screw threads recommended by the British Association for the use of instrument makers, and known as the British Association screw threads, should be modified in the following way for all screws from No. 0 to No. 11 inclusive. For screws.—That the designating numbers, pitches, outside diameters, and the common angle of 474° remain unchanged ; but that the top and bottom of the thread shail be cylindrical, showing flats in section, and that the depth of the thread shall be increased by one-tenth of the pitch, the diameter of the solid core being, in consequence, diminished by one- fifth of the pitch. for nuts.—That the designating numbers, the pitches, the diameters of the clear holes, and the common angle of 474° remain unchanged ; but that the top and bottom of the thread shall be cylindrical, showing flats in section, and that the depth of the thread shall be increased by one- tenth of the pitch. 4 AA, REPORT-—1900. The appended table gives the pitches and diameters of the different threads modified in accordance with this recommendation. Table of the pitches and diameters of the British Association thread under the rule proposed above. | Pitch | Screw Nut Outside Inside Outside Inside No. | diameter diameter diameter | diameter | | | IVE] | IVI T= 6 9S ee el) Mai Mite | e.g | Milligs| ae metres Mils | metres Mils metres Mils | metres | Mils metres Mils 0 | 10 394 | 60 236°2 | 4:6 181°1 | 6:2 | 244-1 | 4°8 | 189:0 UT es eel eis faye: I 5:8 208°7 | 4:04 159°1 | 5:48 210°8 | 4°22 ' 166-2 | Zoe acS)) 31°79 | 47 | 185:0 | 3566 140°4 | 4862 | 191°4.| 3°728 | 146°8 | 3 “73 | 28°7 | 4:1 | 161-4 | 3:°078 |-121:2 | 4:246 | 167-2 | 3-224 | 126-9 | 4 66 260 | 3:6 | 141-7 | 2°676 | 105-4 | 3-732 | 146-9 | 2°808 110°6 | | oy “59 23°2 | 32 126°0 | 2:374 93:5 | 3°318 | 130-6 | 2°492 | 98-1 | 6 | e653) 11 20:9 2°8 110°2 | 2°058 81:0 | 2906 } 114-4 | 2°164 | 85:2 | Rept |eeatS 18°9 2-5 | 98:4 | 1:828 72:0 | 2°596')' 102:2) | 1°924 757 Ce cee esi al 69 nore 86°6 | 1°598 62:9 | 2-286 | 90:0 | 1:684 | 66:3 9 "39 | 15-4 19 74:8 1:°354 53°3 | 1-978 179 | 1432 | 66:4 10 35; 13°8 IG ( 66°9 | 1:210 ATO" iO OT 21 L280) 1) 604 | 1195) 59°71 | 1:066 | 42:0 | 1:562)) GI:5 | 1-128 | 44-4 11 31 12-2 ) In order to give practical effect to our recommendations we desire to obtain a set of the proposed screws, with tools and gauges, for comparison with the present ones. We shall thus be able to exhibit in a concrete form the character of the thread, and also to show how far screws made with the new tools are interchangeable with the existing stocks. We recommend that the Committee shall be reappointed for this purpose with a grant of 50/. APPENDIX. Report of Experimenis on Screw Threads made by J. MARSHALL Goruam and W, A. Price. The object of these experiments was to determine the relative advan- tages of different angles for the threads of small screws, and two questions were proposed for trial. 1. Which angle gives the greatest frictional torque to resist unscrew- ing ? 2. Which angle gives the greatest resistance to the tearing of a steel serew out of a brass plate or nut ? To answer these questions, six pieces, of the forin of fig. 3, were made of steel. On one end, a, of each a thread was cut which was the same in every case, and was used only for the purpose of connecting the pieces in the testing-machine. The threads to be compared were cut on the ends 6. Three kinds of thread were tried, two pieces being made of each kind of thread. The mode of trial is shown in fig. 4. A pair of these steel pieces, A A, having threads of the same kind at the ends / }, were tightly screwed ON THE SMALL SCREW GAUGE. 44.5 by the ends wa into a sleeve F, so that they could not be unscrewed by the forces employed in the test. On the ends 66 were placed brass nuts BB, supported on steel collars C C, which rested in spherical seats in the brass pieces D D. ‘These last pieces D D were screwed into E E, the cast-iron terminal blocks of the testing-machine. Two experiments were made in each case. Eig. 3. a= posilior of rout: 1. With a steady pull on the specimens the torque required to turn both screws simultaneously in their nuts was measured. This was ascer- tained by means of a small spring balance acting by a lever on the hexa- gonal sleeve F. 2. The pull of the testing-machine was then steadily increased until one of the screws was pulled through the nut. Fie. 4. The screwed pieces A A were turned out of tool steel, bright drawn rods of clockmakers’ silver steel, 4/’ diameter. The main object of the experiments being to find the force required to shear the thread out of the nuts B B by screws of given form, any deformation of the screw itself had to be avoided. The } ends of the steel pieces were accordingly water- hardened and let down to a spring temper. In the course of testing, one out of each pair of steel screws broke at the point where it entered the AAG REPORT—1900. brass nut, at a strain much below the calculated breaking strain. The form of the fracture was in every case that of the dotted line c, shown in fig. 3. Professor Unwin, to whom this point was submitted, supposes that this has no bearing on the strength or weakness of the particular forms of thread used, but was due to internal strains in the steel produced by the water-hardening, and to a slight bending force acting with maxi- mum effect at the point where the screw enters the nut. The spherical seats of the collars C C will not, he points out, wholly prevent the occur- rence of this force. He suggests that had the screws been hardened in oil this probably would not have happened. The sectional area of the cores of the screws was ‘095 square inch, and the breaking strain was expected to be about 13,500 1b. Those that broke where they entered the nut broke at 5,600 1b. (60° screw), 5,860 Ib. (50° screw), and 5,330 Ib. (40° screw) respectively. In a subsequent test one of them broke along the line d (fig. 3) at 10,280 lb. Fortunately, in every case a sufficient length of the screw was left after the accident to put on another nut, and in each case a satisfactory result was obtained in a subsequent trial, the screws being drawn through the nuts without being themselves broken. The forms of the screws tested are shown in figs. 5 and 6. The Fig. 5. | Ie "3478" ae: | "3575, ‘4378 rT a ra ae -4475" diameters, both at the top and the bottom of the thread, were the same in all the screws, and also in all the nuts. The screw threads were in all cases flat-topped, with slightly rounded, but nearly flat, bottoms. The pitch of the screw was the same in every case, 16 to the inch. The three threads had angles respectively of 40°, 50°, and 60°. Each screw was cut with a single point tool, ground to the correct angle from a cylinder pre- viously turned to the correct diameter. The nuts were cut with single point inside turning tools, also accurately ground, in a cylindrical hole previously bored to the correct diameter. The outside diameter of each screw was ;/; inch (4375) ; and the inside diameter of each nut was ‘3575 inch. $ > o, °, - @" saa - e's «< <, a increased surface pressures due to the oblique thrust. The above figures, | from specimens black from the hardening process, are higher than one ___ obtained from a screw with a bright surface in a preliminary experiment, by about 90 per cent. E B.— Pull on the screw required to shear the thread out of a brass nut _ 226 inch thick (3:6 threads) cut from flat drawn strip. Angle of thread. Force required to Area of thread Shearing force per shear thread. sheared. square inch, 40° 5,500 1b. 2275 sq. in. 24,160 Ib. 50° ‘ 6,220 lb. "200 seanss 24,880 lb. 60° ; 6,590 lb. PAK ee 25,200 Ib. In this table the area of the thread sheared is obtained from a measure- ment of the space left for the thread of the nut between the successive sip ti of the screw, so that this area is less as the screw thread has a wider top. C.—Pull requiretl to shear the thread away from 4 cast brass nut ‘250 inch thiel (4 threads), y from 4 cast bras nu 448 REPORT—1900. Angle of thread. Force required to Area of thread Shearing force per shear thread. sheared. square inch, 40° (1) 4,890 Ib. 253 sq. in, (2) 4,760 lb. ‘3 * mean 4,825 lb. 19,080 lb. 50° (1) 5,400 1b. "2D Mes (2) 5,130 Tb. # rf mean 5,265 lb. 18,969 1b. 60° (1) 5,500 lb. 300 ~—s, (2) 5,600 Ib. ” ys mean 5,550 lb. 18,500 lb. In these experiments only one screw and one nut were used in each pull, the connection to the other side of the hexagonal sleeve being made with a 4’ steel bolt. Two nuts of each size were sheared. In this case no measurements were taken of twisting torque. D.—The screw of 60° was tested on a brass nut *250 inch thick (4 threads) made from hard drawn rod. 1. Screw broke at 10,280 lb. along line d, fig. 3. 9, Another similar screw sheared the nut at 10,820 lb. Area sheared ‘300 square inch. Shearing force per square inch 36,070 lb. In all cases the nut was sheared along the outside surface of the screw, not at the bottom of its own thread, so that the hole left was a tight fit for the screw which had been pulled through. These figures suggest the following conclusions :— 1. That the angle of a flat-ended thread has little effect on the resist- ance of the nut to shearing, except so far as it affects the area of the surface to be sheared ; and the advantage possessed by the 60° thread over the others is only due to the fact that its flat top is narrower than theirs, and the base of the nut thread correspondingly wider. From analogy with the relative behaviour of sharp and blunted dies used in stamping, it seems that a flat-topped thread with sharp edges should shear a nut more easily than a rounded thread. 2. That the strength of the thread of the nut, compared with that of the core of the screw, is such that generally in practice nuts are stronger than their screws. For example, a flat-ended thread of the dimensions of No. 0 B.A. of 40-ton steel will break before it strips the thread from a hard drawn brass nut + inch thick. So a similar screw of the dimensions of No. 6 B.A. of the same steel will break sooner than strip a brass nut 4'; inch thick. With steel nuts the nut will generally be very much stronger than the screw. 3. Considering (a) that the holding strength of a screw bolt is generally determined (and that especially in small screws) by the resistance of the bolt under tensile stress ; and (5) that, as ascertained by Professor Martens, the resistance of a screw bolt to fracture is very largely diminished by simultaneous torsional stress ; it is desirable that such resistance as may be desired to tightening or loosening a bolt should be obtained by means of the friction of the under surface of the nut.or screw head, and that the friction of the threaded surface of the screw itself should be as small as possible. From this point of view experiments A indicate that an angle of thread of 40° or 50° is to be preferred to an angle of 60°, and that especially so in the case of small screws. The authors of this Report are under a great obligation to Professor T. Hudson Beare for his kind assistance in ascertaining the breaking strains of the specimens. ON THE MICRO-CHEMISTRY OF CELLS. 4A9 The Micro-chenistry of Cells—Report of the Convmittee, consisting of Professor HE. A. ScCHAFER (Chairman), Professor HE. Ray LANKESTER, Professor W. D. Hatursurton, Mr. G. C. Bourne, and Professor A. B. Macauuium (Secretary). (Drawn up by the Secretary) Tue work of the Committee was directed along the following lines :— 1. Lhe Localisation of Phosphorus in the Cell.—In this investigation a wide range of animal and vegetable forms was employed as material, and solutions of molybdate of ammonia in nitric acid were used to localise the phosphorus as a phospho-molybdate compound, the distribution of the latter being revealed after the preparations were treated with solutions of phenylhydrazine hydrochloride. The results show that the element exists in ceils in at least five states of combination : (a) As a nuclein or nucleo- proteid in which the phosphorus is firmly combined in both cytoplasm and nucleus. (5) As a derivative (nucleinoid) of nuclein or nucleo- proteid, in which the phosphorus is much less firmly combined. Examples of this are found in smooth muscle fibre in the dim bands of striated muscle fibre, in the substance constituting the zymogen granules in secreting glands, and in the outer limbs of the retinal rods and cones. (c) As an inorganic metaphosphate dissolved in the cytoplasm of some cells, and apparently derived from a and b. (d) As lecithin, which is present in every cell, and markedly in nerve tissue. (e) As an inorganic orthophosphate in the tissues of various organs, e.g. liver, spleen, kidney, intestinal mucosa, placenta, &c. In the demonstration of the occurrence of these compounds of phosphorus, the length of time required to demen- strate their presence 1s an important factor ; and, further, the metaphosphate and orthophosphate may be removed from a preparation in a couple of hours by the action of dilute nitric acid, while lecithin may be extracted by repeated treatment with hot alcohol. By making preparations of cells and tissues with the molybdate method, both before and after the action of dilute nitric acid, as well as before and after extraction with alcohol, it wus found possible in every case to ascertain the occurrence of one or all of these five classes of compounds in a cellular element. This investigation has given a very large number of results which are of too detailed a character to be referred to specially here, and references to which are now being incorporated in a special paper for publication. One generalisation from these observations may, however, be in place here. The organic, usually iron-free, compounds of phosphorus, which are almost universally present in the cytoplasm of nucleated cells, bear a derivative relation to those which are in the nucleus, and which contain ‘masked’ iron, while in non-nucleated organisms the compounds of iron and phosphorus are found in the cytoplasm in all cases in a diffused form, but in some also as granules (Cyanophycee and the Yeasts). From the chemical point of view the nucleus is therefore an organ for containing the iron-holding nucleo-proteids, and it is therefore an organ of secondary and later origin in the development of the primal cell organism. f 2. The Relation of the Iron to the other Elements in the Chromatin ov Nuclein Molecule.—In this the point to be determined was whether the iron atom is directly united to a carbon atom, as it presumably is in 1900, eae GG. 450 REPORT-—1900. hemoglobin, which is derived from chromatin, or, as Ascoli! claims, to the phosphorus as a polymetaphosphate of iron. For this purpose quantities of iron holding nuclein, prepared from lamb’s testicles, were subjected to the action of water at 160° to 170° C., under pressure for four to eight hours. This brings about a decomposition of the nuclein, setting free the metaphosphorie acid as the ortho acid. It was found that in the first four to six hours nearly all the phosphorus of the compound appears in solution as ortho-phosphoric acid, with traces of iron, the rest of the iron appearing to be still in organic combination in other decomposition products either in solution or undissolved. If the iron were combined with the meta-phosphoric acid it ought to appear as ferric phosphate, which is soluble in the presence of ortho-phosphoric acid. In the absence of this result it must, therefore, be held that the iron is directly associated in the nuclein molecule with some other element, probably carbon. 3. On the Localisation of Oxidising Enzymes in the Cell.—For this pur- pose unicellular alge, and more particularly Spirogyra, were used. The tests for these enzymes are not sufficiently delicate to enable one to de- tect their distribution micro-chemically, but it was found that on subject- ng masses of the living Spirogyra threads washed with distilled water to various degrees of pressure in a specially made hydraulic press one obtained solutions of the various ferments the position of each of which in the cell is approximately determinable by the pressure used. For ex- ample, with an initial low pressure the fluid or solution expressed was largely, if not wholly, from the spaces in the cell surrounding the chro- matophore and the stellate cytoplasmic mass which contains the nucleus, while with a considerably greater pressure one obtains cytoplasmic and nuclear fluids in a second solution, and with the maximum pressure the cytoplasmic and nuclear structures, but not the chromatophore, are disin- tegrated to a certain extent and pass into the fluid expressed as suspended material, which, if kept in this condition for three or four days, partially dissolves. This forms the third solution. In testing for the occurrence of oxidising enzymes in these solutions various readily oxidisable reagents were used as indicators, but the one which gave results most to be relied upon was guaiacum in absolute alcohol, a drop of which added to a solu- tion of an oxidising enzyme results in the production of a blue solution in from a few minutes to half an hour. It was found that an oxidase is present in solution No. 1 in considerable quantities, but sparingly in No. 2, and it is not demonstrable in No. 3. In the first solution an aéro- oxidase occurs in small quantities, that is, an oxidase which is active only in contact with air. Traces of an aéro-oxidase were found in the second solution, but not in that obtained with the maximum pressure. In the last, however, was found abundant evidence of the presence of a peroxidase, that is, of an oxidase which renders guaiacum solutions (emulsions) blue only in the presence of hydrogen peroxide. This same solution also was found to contain a catalase (Loew), that is, a ferment which liberates oxygen from hydrogen peroxide, but which does not oxidise guaiacum emulsions. From such experiments it would appear that the peroxidase and catalase are very intimately associated with the protoplasmic and nuclear structures of the cell while the oxidase ‘and aéro-oxidase are in media external to the protoplasm. It is important to note that the chromatophore does not yield an oxidising ferment or catalase. 1 Zeits fiir Physiol. Chemie, vol. xxviii. p. 426. ON THE MICRO-CHEMISTRY OF CELLS. 45] 4. On the Micro-chemistry of Oxyphile Granules, by Dr. J. J. Mac- kenzie.—Observations on the eosinophilous cells of the bone marrow of the cat and frog and on the same variety of cells from the ccelomic cavity of the frog show that although there is obtained in the granules a distinct iron reaction with ammonium sulphide when the preparation is kept in a mixture of this reagent and glycerine at a temperature of 55-60° C. for 7 to 10 days the reaction is not nearly so marked as in the nuclear chromatin of the same cells and is less readily demonstrated. The method in which acid alcohol is used to liberate the iron from its ‘masked’ condition, and hematoxylin to demonstrate the liberated iron, does not reveal the iron in these granules ; at most with this method one finds a slight reaction in the perigranular protoplasm, but not in the granules themselves. These granules give a reaction for phosphorus when they are treated with a nitric acid solution of ammonium molybdate for some hours, and sub- sequently with a solution of phenylhydrazine hydrochloride, The reaction is much more marked than that in the nuclear chromatin. It is evident from these observations that the substance forming the eosinophilous granules is a nucleo-proteid containing traces of iron, and that it is probably a derivative of nuclear chromatin. 5. On the Micro-chemistry of the Nucleus, by Dr. F. H. Scott.—It was found that the non-chromatin and non-nucleolar portions of the nuclei in gland cells which constitute the /anthanin of Heidenhain and the edematin of Reinke, though soluble in gastric juice, give evidence of the presences of ‘masked’ iron and organic phosphorus in small propor- tions. Similar evidence was obtained in the case of the non-nucleolar and non-chromatin portions of the nuclei of nerve-cells. It is probable that lanthanin or cedematin, while unlike a nucleo-proteid in some respects, is a closely related compound. During the past year the following papers, including observations on the micro-chemistry of cells made during the last two years, were published :— 1. On the Structure, Micro-chemistry, and Development of Nerve Cells, with Special Reference to their Nuclein Compounds. By Dr. F. H. Scott, ‘Trans. Can. Inst.,’ vol. vi. p. 405, and University of Toronto Studies, Physiological Series, No. 1. 2. On the Cytology of Non-nucleated Organisms. By Professor A. B, Macal- lum, ‘Trans. Can. Inst.,’ vol. vi. p. 439, and University of Toronto Studies, Physiological Series, No. 2. Summary of Dir Scott's Paper. The Nissl granules were found to contain ‘masked’ iron and organic phosphorus and to be unaffected by treatment with artificial gastric juice. They are therefore constituted of a nucleo-proteid in many respects allied to chromatin. It differs, however, from the nuclear chromatin which is basophile and from the substance forming the oxyphile centre of the nucleoli and the material diffused through the nuclear cavity in fully developed nerve-cells. The latter substance also contains organic phos- phorus and ‘masked’ iron, and is digestible in artificial gastric juice. These three nucleo-proteids are derived from the original kinetic chromatin of the neuroblast, and the substance forming the Nissl granules is the only nucleo-proteid of the three that diffuses from the nucleus. In some forms this diffusion does not take place in tho fully developed cell, or does so Ge A452 REPORT —1900. only to a very slight extent. In this case few or no Nissl grantles are found ; a condition which is very much like that observed in the not fully developed nerve-cell, and therefore embryonic. This condition is markedly illustrated in the nerve-cells in Caudate Amphibia. Summary of Professor Macallum’s Observations. In the Cyanophycez the cell, which is non-nucleated, contains two zones, a central anda peripheral. The latter contains the colouring matter, and in its vesiculated cytoplasm there is a compound which gives evidence of containing traces of organic phosphorus and ‘ masked’ iron. On the other hand, the central body gives marked reactions for these two elements which are united in a compound diffused throughout its structure. This compound stains with hematoxylin like chromatin, and as it resists diges- tion it is probably chromatin. An iron-holding nucleo-proteid constitutes the red granules of Biitschli, but it differs from chromatin in that it is digestible with artificial gastric juice. Another variety of granules, called ‘cyanophycin’ granules, found only in the peripheral layer, are formed of proteid free from iron and phosphorus. The only substance in the Cyanophycex which resembles fully the chromatin of the cells of higher organisms is that holding iron and phosphorus and diffused in the central body. In the yeast all the iron and phosphorus, in addition to being diffused throughout the cytoplasm, are also localised in small granules and cor- puscles which have been held to be nuclei and nucleoli by various observers. The substance which constitutes these and that in which are combined the iron and phosphorus diffused through the cytoplasm are different from the chromatin of higher organisms, in that they are soluble in artificial gastric juice ; but they are the only chromatin-like substances present in the yeast-cell. In Beggiatow the compounds containing ‘masked’ iron and organic phosphorus are uniformly diffused throughout the cytoplasm, and when granules which stain with hematoxylin occur they also are found to con- tain iron and phosphorus in a corresponding form of combination. The Committee ask to be reappointed, with the addition of Professor J. J. Mackenzie, of Toronto. Comparative Histology of Suprarenal Capsules.—Report of the Com~ mittee, consisting of Professor KE. A. ScHAFER (Chairman), Mr. SwaLE VINCENT (Secretary), and Mr. Vicror Horstry. Durine the past year several points in connection with the comparative histology of the suprarenal capsules have been reinvestigated, and during the investigation several subsidiary inquiries have arisen, such as the histology of the pituitary body and some points in its physiology, the physiological actions of extracts of nervous tissues, &c. The results of these investigations are given at length in paper's published during the year in the ‘Journ. of Physiol.’ and in the ‘ Brit. Med. Journ.’ See also ‘ Anat. Anz.,’ Bd. xviii. 8. 69, 1900. nh ON THE COMPARATIVE HISTOLOGY OF CEREBRAL CORTEX. 453 The Comparative Histology of Cerebral Cortex.—IReport of the Com- mittee, consisting of Professor F. Gorcu (Chairman), Dr. G. Mann (Secretary), and Professor BH. H. Staruine. (Drawn up by the Secretary.) SincE the last report three complete series of sections have been made of the central nervous system of the bonnet monkey—viz., (1) transverse sections from the thalamus to and including the second dorsal nerve, from material fixed in Mann’s picro-corrosive formaldehyde ; (2) a coronal series through the lower part of the medulla and up to and including the eighth cervical segment (fixed in picro-corrosive formaldehyde) ; (3) a Weigert series extending from the fillet decussation to the dorsal cord. The reason for investigating these regions was to ascertain whether so-called motor-cells differed from ‘sensory ’ ones in any definite structural characteristics. Nothing was discovered by which one kind of cell could be distinguished from the other, and it has become evident that Nissl’s classification is a purely artificial one. All cells show a distinct fibrilla- tion, and the basophil ‘ Nissl-substance’ lying between the bundles of fibrils. Motor cells, as a rule, have a greater development of the dendra, and, in consequence, the fibrils coming from these processes in coursing through the cell break up the available space in a regular, uniform manner, and hence there results a more regular arrangement of the basophil granules. In sensory cells, on the other hand, because of the special development of one or two dendritic processes one frequently notices on that side of the nucleus looking towards the biggest dendron a pyramidal (in section tri- angular) area, occupied by non-differentiated plasm, and formed by the divergence of the fibrils coming from the big dendron and sweeping round the nucleus. In these cells, as seen most characteristically in the Locus ceruleus, Substantia nigra, lateral horns of the spinal cord and the antero- mesial visceral group of cells, Nissl’s granules form relatively coarse aggre- gations towards one side of the cell. At one time it was thought that a certain appearance first described by Mann in 1894! in the occipital lobe of the rabbit, since then rediscovered by Roncorini and discredited by Levi—viz., the presence of crescentic bodies on one side of the nucleus— would allow of a ready distinction between nerve-cells in the cerebrum and those found in the lower centres. This, however, was found not to be the case, for the same appearance is seen throughout the whole length of the spinal cord right down to the coccygeal portion. The examination of the dorsal and lower regions of the cord was made possible through the kindness of Miss M. Purefoy FitzGerald, who placed at our disposal the complete series of sections she is tabulating at Oxford. As to the real existence of these crescents there cannot be the slightest doubt, for Levi’s suggestion that we are dealing with a folding of the nuclear membrane is readily disproved by making transverse sections of the cells in the Cornu Ammonis at right angles to their long axis, and staining them by Mann’s eosin-toluidin-blue method, when these crescents in question appear one in each nucleus as distinct swellings in the nuclear membrane, while the latter is not stained at all. In addition to the com- mon crescentic type one may frequently see in surface views branches } Joyrn, Anat. and Physiol. October 1894, ADA REPORT—1900. running outwards from the main central portion. The significance of these figures is probably as follows: F. H. Scott! has shown that the Nissl’s substance is a nucleo-proteid, which amongst reptiles remains throughout life intranuclear, but which in other vertebrates is found out- side the nucleus. Taking these facts into consideration, we are led to con- clude that the crescent is a specially modified part of the nuclear membrane through which normally the nucleo-proteid is passed out into the body of the nerve-cell. That similar nucleo-proteids do pass out in ordinary epithelial cells has been ascertained in inflammatory conditions of the epidermis,” and in gland-cells generally.* On comparing epithelial with nerve cells we find in both a system of fibrils which runs right through the cell ; secondly, material secreted by the nucleus and occupying a position between the fibrils, and lastly a system of intracellular lymph channels(Holmgren). During the last year the existence of these channels in the nerve-cells of the spinal, sympathetic, and central nervous systems of the rabbit, cat, and monkey has been confirmed by using erythrosin instead of eosin in conjunction with toluidin-blue. Holmgren holds that these canals serve to carry a free supply of lymph to the nerve- cell, while Mann suggests that they are tubes which carry away from the cells and towards the fields of conjunction ensymes for the elaboration of the lymph, so as to make the latter directly assimilable by the cell processes. Nissl’s bodies, then, are zymogen granules secreted by the nucleus, stored up during rest, and discharged during activity.‘ Golgi’s intracellular network in spinal ganglia and the anterior horn cells of the spinal cord may be demonstrated by fixing tissue in 25 per cent. potassium iodide saturated with iodine, and then taking them through aceton into paraffin. The network seems in the spinal ganglia to form a framework on which Nissl’s substance is deposited. The latter is removed by the potassium iodide, while the framework remains. Other points which the serial sections have brought out are :— 1. The mesencephalic (so-called descending) root of the fifth nerve arises from cells which are quite distinct from the cells of the Locas ceruleus. Their axis cylinders have very distinct nodes of Ranvier. 2. The sensory decussation, as shown in the fillet, is only a more pro- nounced condition of a general arrangement, holding good for the whole length of the cord, the decussating fibres being derived from a small- celled nucleus situated on a level with, and lateral to, the central canal. The afferent fibres to it correspond to Pal’s dorsal bundle. The two nuclei are connected by a commissure of very fine medullated nerve-fibres run- ning dorsally to the well-known anterior white commissure. 3. Stilling’s sacral and cervical nuclei, Clarke’s dorsal column, Blu- menawu’s nucleus, Deiter’s nucleus, and the cells of the mesencephalic root of the fifth nerve seem to belong to the same system, which lies dorso- laterally, and is characterised by large cells. The nucleus above referred to under No. 2, the gracile and cuneate nuclei proper, the mesial trian- gular nucleus of the eighth nerve, and the Locus ceruleus form a dorso- mesial system containing small cells, 1 Trans. Canadian Institute, 1898-99. 2? Mann, Histology of Vaccinia, L.G.R., 1899. 3 Trambusti, Galeotti, Huie. * The intracellular lymph channels are well shown in the electrical nerve-cell of Malapterurus. ‘The structure of this cell was displayed at the Liverpool meeting of the British Association by Mann’s charts, &c, (1895). a ——— or ON ELECTRICAL CHANGES IN MAMMALIAN NERVE. 45 Electrical Changes in Mammalian Nerve-—Report of the Committee, consisting of Professor F. Gotca (Chairman), Professor E. H. Sraruina, Dr. J. S. Macponatp (Secretary). (Drawn up by the Secretary.) Tue experiments performed with the assistance of grant from the Asso- ciation have been directed towards the acquisition of information as to the effect upon the demarcation current of mammalian nerve of alterations in resistance, such as are found in mammalian nerve accom- panying changes of volume and of blood-pressure in the vesseis supplying the nerve. The nature of the changes of resistance is easily determined but the effect of such a change in presumably causing not oniy an altera tion in the magnitude, but also in the distribution of current and dit- ferences of potential in the nerve, is not easy to calculate. Not only this, but it is impossible even to decide the direction of change (addition or subtraction) in the demarcation current which would be produced by any alteration of the internal resistance of the nerve. Knowledge of an exact character is required for this purpose, defining the limits of the demarcation source and the extent to which the source is short-circuited in the tissues of the nerve itself. It was felt that such knowledge must be based entirely upon experiments upon nerve, and as far as possible upon the particular nerve for which the information was desired. With this object a large number of experiments have been performed upon excised mammalian nerve. The nerves after removal were placed upon a number of non-polarisable electrodes (four to seven), the potential differences between each pair of electrodes determined, as also the resist- ances of the whole nerve and the sections into which it was divided by the electrodes. The electrode upon which the cross-section lay was then permanently connected by a wire or through a known resistance to one of the other electrodes, and the differences of potential between each possible pair of electrodes determined again after the formation of this circuit. An analysis of the data gained by determination of the various resist- ances divides the facts of experiments into the following groups :— (a) The resistance per centimetre determined from the measurement of resistance of any given length of the nerve varies with that length, being smaller for the greater length. (b) The resistance of the whole nerve directly determined is a smaller value than its resistance calculated from a summation of the resistances of the several sections between pairs of electrodes. (c) The resistance of that section of the nerve bounded by the cross- section gives a smaller value for the resistance per centimetre of the nerve than any other section. An observation of these facts has led to a routine method for calcu- lating the resistance of any short length of nerve when the resistance required is not that to a current entering and,leaving at the extremities of the short length, but the gross longitudinal resistance to a current travelling in paths parallel to the long axis of the nerve. The resistance obtained from the longest available stretch of nerve proyided with a cross- A566 REPORT—1900, section at either end and calculated into resistance per centimetre is the standard of gross longitudinal resistance, and multiplied by the length of short piece of nerve gives the value required. The determination of the differences of potential, or, as it is preferred to call them, the available E.M.F.’s between pairs of points on nerve, and calculations based upon these and upon the known resistances, have given interesting information. («) When the cross-section is connected to a point on the longitudinal surface, the current found in the outer circuit passing from longitudinal surface to cross-section can be found traversing the nerve from cross- section to longitudinal surface, by the new differences of potential acquired by intervening points on longi- tudinal surface of nerve. Ts | 0-10 O}F | SIE SOF rea 0 See lo0 96 || 81- 90 4 11-15 | 2 | 381-40 | 409 61-70 49 | 91-100 BO=20. | oG | 41-50 215 71-80 6 } The number of arpents under cultivation was 11,448, with cattle 3,107, and sheep 85. No horses yet in the colony. All the sheep were run on at River St. Charles, near Quebec. The land under cultivation shows an average of seventeen arpents per family. The census of 1681 has the same small proportion. APPENDIX II. Notes on the Sk-qo'mic of British Columbia, a Branch of the great Salish Stock of North America. By C. H1uw-Tovr. The following notes on the Sk:q6'mic, a division of the Salish stock of British Columbia, are a summary of the writer’s studies of this tribe. While he has sought to make them as comprehensive and complete as possible, he is fully conscious that they are far from being exhaustive. There are, indeed, insuperable difficulties in the way of making really exhaustive reports on any of our tribes at the present time. There are, in the first place, many invincible prejudices to be overcome. Then there is the dithiculty of communic:.tion, and when these have been partially overcome there yet remains the difficulty of finding natives who possess the know- ledge you are seeking. Not every Indian is an Jagoo, a story-teller ; and only the older men or women remember the old practices, customs, manners, and beliefs of the tribe, and even these have forgotten much that is important to know. These and other difficulties stand in the way of complete and exhaustive investigation ; and I cannot better illustrate the need of pushing on our work among these interesting peoples without further delay than by stating that since my last report was sent in my principal informant among the N’tlaka’pamua, Chief Mischelle, from whom I secured so much valuable information a year or so ago, has passed away, and can render us no further aid. In a few years, all those who lived under the old conditions in pr-missionary days, and who now alone possess the knowledge we desire to gather, will have passed away, and our chances of obtaining any further reliable information of the past will have gone with them. In my work among the Sk’qd’mic I have been more than usually for- tunate, and have been able to bring together much interesting matter not previously known or recorded. Ethnography. The Sk‘q0’mic constitute a distinct division of the Salish of British Columbia and both in language and customs differ considerably from the coast tribes on the one hand, and the interior tribes on the other. The structural differences of their speech are so great as to shut them off from free intercourse with the contiguous Salish tribes. The tribe to-day numbers less than two hundred souls, I believe, Formerly they were a ON THE ETHNOLOGICAL SURVEY OF CANADA. 473 strong and populous tribe, numbering, when white men first came into contact with them, many thousands. Some of their larger o’kwumiq, or villages, contained as many as seven hundred people, and that less than fifty years ago. We gather this from the early white settlers themselves, The original home and territory of the Sk-qo’'mic seems to have been on the banks of the river which gives them their tribal name, and along the shores of Howe Sound, into which the Skuamish runs. Their settlements on the river extended for upwards of thirty miles along the banks. ‘Their northern neighbours were the Lillooets or StlatlumuH tribe and the Tcilkotin division of the Déné stock. Their southern neighbours were the Lower Fraser tribes. According to one of my informants the Indian villages that used to exist on English Bay, Burrard Inlet, and False Creek were not originally true Sk-qd’mic. They were said to be allied by speech and blood to the Lower Fraser tribes. How far this is correct seems impossible now to say. Sk’qd/mic is everywhere spoken throughout this territory, and has been as far back as our knowledge of it goes ; and the Sk-q0/mic villages, according to my informants, extend to and include Mali, at the mouth of the Fraser, which place Dr. Boas was informed by the River Indians belonged to them, and which he has accordingly included in their territory. It was probably the dividing line, and, like Spuzzum, farther up the river, was composed partly of the one division and partly of the other. Our first knowledge of the Sk-qo’mic dates back to rather less than a century ago. The first white man to sail into English Bay and Howe Sound and come into contact with them was Captain Vancouver. He recorded briefly his impressions of them in the diary of his voyage to this coast, a short extract from which may be of interest in this first formal account of the tribe. He writes thus :— Friday, June 15, 1792.! ‘ But for this cireumstance we might too hastily have concluded that this part of the Gulf was uninhabited. In the morning we were visited by nearly forty of the natives, on whose approach from the very material alteration that had now taken place in the face of the country we expected to find some difference in their general character. This conjec- ture was, however, premature, as they varied in no respect whatever, but in possessing a more ardent desire for commercial transactions, into the spirit of which they entered with infinitely more avidity than any of our former acquaintances, not only bartering amongst themselves the different valuables they had obtained from us, but when that trade became slack in exchanging those articles again with our people, in which traffic they always took care to gain some advantage, and would frequently exult on this occasion. Some fish, their garments, spears, bows and arrows, to which these people wisely added their copper garments, comprised their general stock-in-trade. Jron inall forms they judiciously preferred to any other article we had to offer.’ They have not altered much in these points of their character since Vancouver’s visit, and many of them have to-day, I am told, snug little sums judiciously invested by their good friend and spiritual director, the late Bishop Durieu, in safe paying concerns. It is only fair to say, how- ever, that they deserve to be prosperous. They are probably the most ! Vol. i, p. 805, 474. REPORT—1900, industrious and orderly band of Indians in the whole province, and reflect great credit upon the Roman Mission established in their midst. I obtained the following list of old village sites, not 10 per cent. of which are now inhabited. The list is not perfectly complete. There were a few more villages at the upper end of Burrard Inlet which have been long abandoned, and whose names my informants could not recall. My enumeration contains in all some ninety-three villages, each of which, according to Chief Thomas of Qé’qids and others, was formerly a genuine Sk:qd'mic o/kwumiiq, containing from fifty to several hundred inhabitants. ON Sk:QO0/MIc RIVER. Riaht Bank. Co’ tais. N’cai'te. T’k-takai’ = vine-maple. SQaqai’Ek. Kwana'ken = hollow in mountain, Yu'kuts. Sto’toii =Jeaning over (a cliff). Kémps. Slokoi. N’k-u'kapenatc= canoes transformed to stone (see story of Qais). K-wo'lan = ear. Kau’ten. Qé’qids. Sié/tekm = sandy. N’pok-wis. Ek-iks. Tcia/kamic (on creek of that name). Tokta’kamai = place of thimble-berries. Hower West Side. Tcé’ was. Swi/at. Cé'tuksEm. Ceé'tisum. Kwi'tctenEm. Ké’kelun. K-68’ koi. Stcink: (Gibson’s Landing). East Side. K-akutwo'm = waterfall, Cé’'tsakrEn. Spapa’k. Etlé’uq. *Skaui’can. Poia'm. Loft Bank. S'k'lau’ = beaver. Sta/mis. Smok:. Qa’k-siné (on Ma’mukum Creek). Kiake’n. Ikwo'psum. QEk-wai'akin. Itli/oq. Po'kaio’sum = slide. Sk-timi’n = keekwilee-house. Cémps. Tcimai’. Toeuk'teuk’ts. SouND. Cicai’dQoi Qx'IkEt6s = painted. Sk-u‘tuksEn = promontory, Ku 'latsEn. N’pa’puk-. Tumtls = paint. Teakqai. St’o'ktoks. Stcilks = sling. Ké’tlals’m=nipping grass, so called be- cause deer come here in spring to eat the fresh grass. Ské’awatsut (Point Atkinson). ISLANDS IN SOUND. TJa’qom (Anvil Island). Tca'lkunts (Gambier Island). Qolé’lagom (Bowen Island), Sau’qtite (Hat Island). Mi'tlmetle’ltc (Passage Island), ENGLISH Bay, THE NARROWS, BURRARD INLET, AND FALSE CREEK, From Coal Harbour to Mouth of North Arm of the Fraser. Tcetcé’lmen. TceEkO'alte. Papiak: (lighthouse), Qoigoi = masks. Suntz. Sk’é/akunts. . re ON THE ETHNOLOGICAL SURVEY OF CANADA, 475 Teants. : " ; North Side from Point Atkinson, through Bye ee standing up (‘Siwash rock ’). the aes up the Inlet Stetiqk. Hélcen=sandy beach; verbatim, soft to ’St’k-qé'l. the foot. SmeEla/koa. Snauq (False Creek). K’tea'm. Sk oateai’s = deep hole in water. Swai’wi. Sk wai'us. Homuw'ltcison (Capilano Creek) (former -Ta'Imuq (Jericho). headquarters of supreme chief of the Qapgapétlp = place of cedar (Point Grey). Sk-q0/mic). U'lk's’n = point (ef. radical for nose). Tlastlumanq = Saltwater Creek. Tle’atlum Stlau’n. Tcitcile’Ek. Qotlskaim = serpent pond. Kru’ laqEn. Qoa'Itca (Linn Creek). HumeElsom. Teétcilgok (Seymour Creek). — Mili. K-iaken = palisade, a fenced village, Social Organisation, The social organisation of the Skqd/mic has been so much broken up and modified by missionary and white influence that it is difficult now to learn any details about it. The tribe appears to have been divided, like the N’tlaka/pamug, into a number of d'kwwmiig, or village communi- ties, each of which was governed by its own local chief. I could gather nothing of their beliefs with regard to the origin of their different villages : they seem to have none or else to have lost or forgotten them. Of the origin of the tribe as a whole and some of the chief events of their existence I gathered an account a few years ago from an ancient member of the tribe, who was born a year or so after Captain Vancouver's visit to them in 1792. This was published in the ‘ Proceedings of the Royal Society of Canada,’ 1897-98. Briefly it tells how the first Sk-qo’mie man came into existence ; how later the tribe was overwhelmed by a flood, and only one man and his wife escaped in their canoe, which landed on the mountains contiguous to the present Sk-q0’mic territory ; and how later again a severe and prolonged snowstorm caused, by cold and famine, the death of the whole tribe save one man and his daughter. From these two the Sk-qd’mic trace their tribal descent. The people were divided into the usual threefold division of chiefs, nobles, and common people. The lines, however, between these classes were not absolutely rigid. According to my informants a member of the lower class, if a woman, could rise to the class above her by marriage with a member of that class, the wife usually taking the rank of her husband if not a slave. But a man of the lower rank, even if he suc- ceeded in marrying a woman of the middle class, could only become a member of that class by undergoing a long and severe training, in which daily washings and scrubbings of the body played an important part. This was evidently a form of initiation the further particulars of which T could not learn. As a rule the chiefs and their families and immediate relatives formed a class or caste apart, the title of chief or headman descending from father to son, patriarchate prevailing among the Sk-qo’mic. Consequently a chief usually married a chief's daughter or daughters. But this rule was sometimes broken, and a woman of a lower class was taken to wife. In these cases the chieftainship would properly descend to one of the chief’s brothers or his son, and not to his own son. This was the rule. But it was possible to break this also and transmit the headship of the tribe to his own son by giving many ‘ potlatch’ feasts, A476 ° REPORT—1900. and thus securing the goodwill of the tribe in his son’s favour, The son, too, upon his father’s death, would also give a feast and make handsome presents to all the influential men of the tribe, the result of which would be that he would be elected to the rank of chief, and be allowed to succeed his father in the chieftaincy of the tribe. From this it would seem that children took their social rank from their mother rather than from their father, which looks like a trace of matriarchate, or mother-right. It is clear from their folk-tales, however, that these class divisions were not hard and fast, but that members of a lower caste could by the per- formance of certain acts pass into that above it. Of secret societies I was unable to obtain any information whatever, and whether such formerly existed among the Sk-qo/mic—of which I am extremely doubtful— it seems impossible now to say. Among the chiefs there were some of higher rank than the others, as among the N’tlaka/pamug. The supreme sia'm of the tribe was known by the title Zz Kiapila’nda, and had his headquarters at the mouth of the Hom/ultcison Creek, now called Capilano by the whites. He was local chief also of the Hému'Itcison sept. Next in rank to him came one of the Skuamish River chiefs. He likewise had a proper title, being known as 7's Qatsila/noa.! I was unable to learn what special signification these titles had. It is possible we may see in them the special names of two powerful gentes. The gentile system of the Sk-q0’mic, if such existed, is not at all clear. The distinction between what might be regarded as a gens, or a sept, or a mere tribal division is very difficult to determine. I could gather nothing satisfactory from any of my informants on this head. Heraldic and totemic symbols, according to some of them, were never used in the old days ; but yet I was informed by others that some of the old houses had carved posts or columns, and that the figure of a bird or some other animal would sometimes be placed on a pole in front of the house or fastened to one of the gable ends. They also, sometimes at least, used masks in certain of their dances, if we may rely upon the information on these points in their folk-tales. The tribe, as my ethno- graphical notes show, was formerly divided into a number of subdivisions, or o'Jwumig. Whether each of these should be regarded simply as a tribal subdivision, as among the N’tlaka/pamua, or as a gens, as among the northern tribes, is doubtful. Each division had its own proper name— in every instance, I think, a geographical one—derived from some local physical peculiarity, exactly as among the N’tlaka’‘pamug. In every okwumiug there existed the same threefold division of the people into three classes, and in some instances the total number of souls in each village would amount to several hundreds. Generally speaking, each community would be made up of several families or clans. ‘The members of these clans were not bound together, as the gentes of the northern ‘ The distinctive part of this title bears a remarkable resemblance to the esoteric term by which one of the Nootka deities was invoked by the chiefs of that tribe. Dr. Boas has recorded the name of this being under the form Ka'tse. The two forms so clearly resemble each other as to suggest some connection between them; and in this connection I may remark that the more I extend my studies of the Salish and Kwakiutl-Nootka, the stronger is the conviction forced upon me that between these two stocks there is a deeper underlying racial connection than the structural differences of their language would seem to indicate. Morphologically speaking, they seem to have little in common ; but that little steadily increases with our larger analytical knowledge of their languages, and their vocabulary resemblances are jnany and far-reaching, ON THE ETHNOLOGICAL SURVEY OF CANADA. 477 tribes, by common totems or crests. They comprised the blood relatives of any given family on both sides of the house for six generations. After the sixth generation the kinship ceases to hold good and the clanship is broken. Under this arrangement an individual’s relatives were legion, and he would often have family connection in a score or more different d'kwwmig. Among the present Sk:q0/mic almost all of them are related in this way to one another, and their cousinships are endless and.even perplexing to themselves. Marriage within the family or clan as thus constituted was prohibited, but members of different clans in the same village could intermarry with each other. If each village community is to be regarded as a separate gens having a common origin - from some common ancestor—which I think is extremely doubtful—then ‘marriage among the Sk’q0/mic was not forbidden to members of the same gens. For my own part I am disposed to regard these separate communi- ties as mere subdivisions of the tribe which were effected at different periods in their tribal existence, and generally, probably, from the same causes which have all over the world led to the founding of new homes - and new settlements, viz., increase and stress of population. The evidence in favour of regarding these divisions as distinct gentes having each a separate origin and springing from a separate ancestor, as among the northern tribes, is scanty and doubtful. This view is strengthened by the traditional origin of the tribe, which makes them all spring from a common pair. I do not desire to be understood as asserting that totemic gentes did not formerly exist among the Sk-qo'mic, as Dr. Boas seems to hold. All I say is that after diligent inquiry from several of the chiefs and others I could myself find no evidence of it. I could not learn that any particular group or family bore names peculiar to that group or family, or possessed privileges not shared by the others other than the right to certain dances and their accompanying songs the origin and source of which was some personal dream, or vision, or experience of their own or their parents. But the ownership of these dances differed in no way from the ownership of a canoe or any other piece of property, and constituted no kind of bond or union between the owner of them and others of the tribe or d’kwumigq. The only peculiar name that I could learn other than those of the supreme chiefs was that borne by the offspring of female slaves by their masters. This was the term s’t@/cem, and was a word of reproach. Polygamy was commonly practised among the Sk-qo/mic, the number of a man’s wives being limited only by his rank and wealth. 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OBE IGE-OEE EL. ro ab wart ‘gon an if ih Meth \OGQE at 20! { F ifs moitafest ori’! » OSE ce-ahe epi eee di Pt siroth bint pL if ~ ~ it dn sad hi st ee: > Us Lig POMBE Tpit a it ail sie gunk Ist 6 ee SH Py "00% hE v0 t te are ind: 4 va? adaina 3 en loft 4 13, & See : oe . ar . ; jo ,7 etal etalt f i s TRANSACTIONS OF THE SECTIONS. Section A—MATHEMATICAL AND PHYSICAL SCIENCE. PRESIDENT OF THE SEctIoN—Dr, JosEPH Larmor, F.R.S. THURSDAY, SEPTEMBER 6. The President delivered the following Address :— Ir is fitting that before entering upon the business of the Section we should pause to take note of the losses which our department of science has recently sustained. The fame of Bertrand, apart from his official position as Secretary of the French Academy of Sciences, was long ago universally established by his classical treatise on the Infinitesimal Calculus: it has been of late years sustained by the luminous exposition and searching criticism of his books on the Theory of Probability and Thermodynamics and Electricity. The debt which we owe to that other veteran, G. Wiedemann, both on account of his own researches, which take us back to the modern revival of experimental physics, and for his great and indispensable thesaurus of the science of electricity, cannot easily be overstated. By the death of Sophus Lie, following soon after his return to a chair in his native. country Norway, we have lost one of the great constructive mathematicians of the century, who has in various directions fundamentally expanded the methods and conceptions of analysis by reverting to the fountain of direct geometrical intuition. In Italy the death of Beltrami has removed an investigator whose influence has been equally marked on the theories of transcendental geometry and on the pro- gress of mathematical physics. In our own country we have lost in D. E. Hughes one of the great scientific inventors of the age; while we specially deplore the removal, in his early prime, of one who has recently been well known at these meetings, Thomas Preston, whose experimental investigations on the relations between magnetism and light, combined with his great powers of lucid exposition, marked out for him a brilliant future. Perhaps the most important event of general scientific interest during the past year has been the definite undertaking of the great task of the international coordination of scientific literature; and it may be in some measure in the pro- longed conferences that were necessitated by that object that the recently announced international federation of scientific academies has had its origin. In the important task of rendering accessible the stores of scientific knowledge, the British Association, and in particular this Section of it, has played the part of pioneer. Our annual volumes have long been classical, through the splendid reports of the progress of the different branches of knowledge that have been from time to time contributed to them by the foremost British men of science ; and our work in this direction has received the compliment of successful imitation by the sister Associations on the Continent. The usual conferences connected with our department of scientific activity have 614 REPORT-—1900. been this year notably augmented by the very successful international congresses of mathematicians and of physicists which met a few weeks agoin Paris. The three volumes of reports on the progress of physical science during the last ten years, for which we are indebted to the initiative of the French Physical Society, will pro- vide an admirable conspectus of the present trend of activity, and form a permanent record for the history ot our subject. Another very powerful auxiliary to progress is now being rapidly provided by the republication, in suitable form and within reasonable time, of the collected works of the masters of our science. We have quite recently received, in a large quarto volume, the mass of mest important unpublished work that was left behind him by the late Professor J.C. Adams; the zealous care of Professor Sampson has worked up into order the more purely astronomical part of the volume; while the great undertaking, spread over many years, of the complete determination of the secular change of the magnetic condition of the earth, for which the practical preparations had been set on foot by Gauss himself, has been prepared for the press by Professor W.G. Adams. By the publication of the first volume of Lord Rayleigh’s papers a series of memoirs which have formed a main stimulus to the progress of mathematical physics in this country during the past twenty years has become generally accessible. The completed series will form a landmark for the end of the century that may be compared with Young's ‘ Lectures on Natural Philosophy’ for its beginning. The recent reconstruction of the University of London, and the foundation of the University of Birmingham, will, it is to be hoped, give greater free- dom to the work of our University Colleges. The system of examinations has formed an admirable stimulus to the effective acquisition of that general knowledge which is a necessary part of all education. So long as the examiner recognises that his function is a responsible and influential one, which is to be taken seriously from the point of view of moulding the teaching in places where external guidance is helpful, test by examination will remain « most valu- able means of extending the area of higher education. Except for workers in rapidly progressive branches of technical science, a broad education seems better adapted to the purposes of life than special training over a narrow range; and it is difficult to see how a reasonably elastic examination test can be considered as a hardship. But the case is changed when preparation for a specialised scientific profession, or mastery of the lines of attack in an unsolved problem, is the object. The general education has then been presumably finished ; in expanding depart- ments of knowledge, variety rather than uniformity of training should be the aim, and the genius of a great teacher should be allowed free play without external trammels. It would appear that in this country we have recently been liable to unduly mix up two methods. We have been starting students on the special and lengthy, though very instructive, processes which are known as original research at an age when their time would be more profitably employed in rapidly acquiring a broad basis of knowledge. As a result, we have been extending the examination test from the general knowledge to which it isadmirably suited into the specialised activity which is best left to the stimulus of personal interest. Informal. contact with competent advisers, themselves imbued with the scientific spirit, who can point the way towards direct appreciation of the works of the masters of the science, is far more effective than detailed instruction at second hand, as regards growing subjects that have not yet taken on an authoritative form of exposition. Fortu- nately there seems to be now no lack of such teachers to meet the requirements of the technical colleges that are being established throughout the country. The famous treatise which opened the modern era by treating magnetism and electricity on a scientific basis appeared just 300 years ago, The author, William Gilbert, M.D., of Colchester, passed from the Grammar School of his native town to St. John’s College, Cambridge: soon after taking his first degree, in 1560, he became a Fellow of the College, and seems to have remained in resi- dence, and taken part in its affairs, for about ten years. All through his subse- quent career, both at Colchester and afterwards at London, where he attained the highest position in his profession, he was an exact and diligent explorer, TRANSACTIONS OF SECTION A. 615 first of chemical and then of magnetic and electric phenomena. In the words of the historian Hallam, writing in 1839, ‘in his Latin treatise on the Magnet he not only collected all the knowledge which others had possessed, but he became at once the father of experimental philosophy in this island;’ and no demur would be raised if Hallam’s restriction to this country were removed. Working nearly a century before the time when the astronomical discoveries of Newton had originated the idea of attraction at a distance, he established a complete formu- lation of the interaction of magnets by what we now call the exploration of their fields of force. His analysis of the facts of magnetic influence, and incidentally of the points in which it differs from electric influence, is virtually the one which Faraday re-introduced. A cardinal advance was achieved, at a time when the Copernican Astronomy had still largely to make its way, by assigning the behaviour of the compass and the dip needle to the fact that the earth itself is a great magnet, by whose field of influence they are controlled. His book passed through many editions on the Continent within forty years: it won the high praise of Galileo. Gilbert has been called ‘the father of modern electricity by Priestley, and ‘the Galileo of magnetism’ by Poggendortf. When the British Association last met at Bradford in 1873 the modern theory which largely reverts to Gilbert’s way of formulation, and refers electric and magnetic phenomena to the activity of the «ther instead of attractions at a distance, was of recent growth: it had received its classical exposition only two years before by the publication of Clerk Maxwell's treatise. The new doctrine was already widely received in England on its own independent merits. On the Continent it was engaging the strenuous attention of Helmholtz, whose series of memoirs, deeply probing the new ideas in their relation to the prevalent and fairly successful theories of direct action across space, had begun to appear in 1870. During many years the search for crucial experiments that would go beyond the results equally explained by both views met with small success ; it was not until 1887 that Hertz, by the discovery of the ethereal radiation of long wave-length emitted from electric oscillators, verified the hypothesis of Faraday and Maxwell and initiated a new era in the practical development of physical science. The experimental field thus opened up was soon fully occupied both in this country and abroad; and the horderland between the sciences of optics and electricity is now being rapidly explored. The extension of experimental know- ledge was simultaneous with increased attention to directness of explanation ; the expositions of Heaviside and Hertz and other writers fixed attention, in a manner already briefly exemplified by Maxwell himself, on the inherent simplicity of the completed sthereal scheme, when once the theoretical scaffolding employed in its construction and dynamical consolidation is removed; while Poynting’s beautiful corollary specifying the path of the transmission of energy through the xther has brought the theory into simple relations with the applications of electro- dynamics. ‘Equally striking has been the great mastery obtained during the last twenty years over the practical manipulation of electric power. The installation of electric wires as the nerves connecting different regions of the earth had attained the rank of accomplished fact so long ago as 1857, when the first Atlantic cable was laid. It was largely the theoretical and practical difficulties, many of them unforeseen, encountered in carrying that great undertaking to a successful issue, that necessitated the elaboration by Lord Kelvin and his coadjutors of convenient methods and instruments for the exact measurement of electric quantities, and thus prepared the foundation for the more recent practical developments in other directions. On the other hand, the methods of theoretical explanation have been in turn improved and simplified through the new ways of considering the phenomena which have been evolved in the course of practical advances on a large scale, such as the improvement of dynamo armatures, the conception and utilisation of magnetic circuits, and the transmission of power by alternating currents. In our time the relations of civilised life have been already perhaps more profoundly altered than ever before, owing to the establishment of practically instantaneous electric communication between all parts of the world. The 616 REPORT—1900. employment of the same subtle agency is now rapidly superseding the artificial reciprocating engines and other contrivances for the manipulation of mechanical power that were introduced with the employment of steam. The possibilities of transmitting power to great distances at enormous tension, and therefore with very slight waste, along lines merely suspended in the air, are being practically realised ; and the advantages thence derived are increased manifold by the almost automatic manner in which the electric power can be transformed into mechanical rotation at the very point where it is desired to apply it. The energy is transmitted at such lightning speed that at a given instant only an exceedingly minute portion of it is in actual transit. When the tension of the alternations is high, the amount of electricity that has to oscillate backwards and forwards on the guiding wires is proportionately diminished, and the frictional waste reduced. At the terminals the direct transmission from one armature of the motor to the other, across the intervening empty space, at once takes us beyond the province of the pushing and rubbing contacts that are unavoidable in mechanical transmission; while the perfect symmetry and reversibility of the arrangement by which power is delivered from a rotatory alternator at one end, guided by the wires to another place many miles away, where it is absorbed by another alternator with precise reversal of the initial stages, makes this process of distribution of energy resemble the automatic operations of nature rather than the imperfect material connections previously in use. We are here dealing primarily with the flawless continuous medium which is the transmitter of radiant energy across the celestial spaces; the part played by the coarsely constituted material conductor is only that of a more or less imperfect guide which directs the current of «ethereal energy. The wonderful nature of this theoretically perfect, though of course practically only approximate, method of abolishing limitations of locality with regard to mechanical power is not diminished by the circumstance that its principle must have been in some manner present to the mind of the first person who fully realised the character of the reversibility of a Gramme armature. In theoretical knowledge a new domain, to which the theory as expounded twenty years ago had little to say, has recently been acquired through the experi- mental scrutiny of the electric discharge in rarefied gaseous media. The very varied electric phenomena of vacuum tubes, whose electrolytic character was first practically established by Schuster, have been largely reduced to order through the employment of the high exhaustions introduced and first utilised by Crookes, Their study under these circumstances, in which the material molecules are so sparsely distributed as but rarely to interfere with each other, has conduced to enlarged knowledge and verification of the fundamental relations in which the individual molecules stand to all electric phenomena, culminating recently in the actual determination, by J. J. Thomson and others following in his track, of the masses and velocities of the particles that carry the electric discharge across the exhausted space. The recent investigations of the circumstances of the electric dissociation produced in the atmosphere and in other gases by ultra-violet light, the Roéntgen radiation, and other agencies, constitute one of the most striking developments in experimental molecular physics since Graham determined the molecular relations of gaseous diffusion and transpiration more than half a century ago. This advance in experimental knowledge of molecular phenomena, assisted by the discovery of the precise and rational effect of magnetism on the spectrum, has brought into prominence a modification or rather development ot Maxwell's exposition of electric theory, which was dictated primarily by the requirements of the abstract theory itself; the atoms or ions are now definitely introduced as the carriers of those electric charges which interact across the wether, and so pro- duce the electric fields whose transformations were the main subject of the original theory. We are thus inevitably led, in electric and sthereal theory, as in the chemistry and dynamics of the gaseous state which is the department of abstract physics next in order of simplicity, to the consideration of the individual molecules of matter. The theoretical problems which had come clearly into view a quarter of a century ago, under Maxwell’s lead, whether in the exact dynamical relations TRANSACTIONS OF SECTION A. 617 of zthereal transmission or in the more fortuitous domain of the statistics of interacting molecules, are those around which attention is still mainly concentrated ; but as the result of the progress in each, they are now tending towards consolida- tion into one subject. 1 propose—leaving further review of the scientific aspect of the recent enormous development of the applications of physical science for hands more competent to deal with the practical side of that subject—to offer some re- marks on the scope and validity of this molecular order of ideas, to which the trend of physical explanation and development is now setting in so pronounced a manner. If it is necessary to offer an apology for detaining the attention of the Section on so abstract a topic, I can plead its intrinsic philosophical importance. The hesitation so long felt on the Continent in regard to discarding the highly de- veloped theories which analysed all physical actions into direct attractions between the separate elements of the bodies concerned, in favour of a new method in which our ideas are carried into regions deeper than the phenomena, has now given place to eager discussion of the potentialities of the new standpoint. There has even appeared a disposition to consider that the Newtonian dynamical principles, which have formed the basis of physical explanation for nearly two centuries, must be replaced in these deeper subjects by a method of direct description of the mere course of phenomena, apart from any attempt to establish causal relations ; the initiation of this method being traced, like that of the Newtonian dynamics itself, to this country. The question has arisen as to how far the new methods of ethereal physics are to be considered as an independent departure, how far they form the natural development of existing dynamical science. in England, whence the innovation came, it is the more conservative position that has all along been occupied. Maxwell was himself trained in the school of physics established in this country by Sir George Stokes and Lord Kelvin, in which the dominating idea has been that of the strictly dynamical foundation of all physical action. Although the pupil’s imagination bridged over dynamical chasms, across which the master was not always able to follow, yet the most striking feature of Max- well’s scheme was still the dynamical framework into which it was built. The more advanced reformers have now thrown overboard the apparatus of poten- tial functions which Maxwell found necessary for the dynamical consolidation or his theory, retaining only the final result as a verified descriptive basis for the phenomena. In this way all difficulties relating to dynamical development and indeed consistency are avoided, but the question remains as to how much is thereby lost. In practical electro-magnetics the transmission of power is now the most prominent phenomenon; if formal dynamics is put aside in the general theory, its guidance must here be replaced by some more empirical and tenta- tive method of describing the course of the transmission and transformation of mechanical energy in the system. The direct recognition in some form, either explicitly or tacitly, of the part pleyed by the ether has become indispensable to the development and exposition of general physics ever since the discoveries of Hertz left no further room for doubt that this physical scheme of Maxwell was not merely a brilliant speculation, but constituted, in spite of outstanding gaps and difficulties, a real formulation of the underlying unity in physical dynamics. The domain of abstract physics is in fact roughly divisible into two regions. In one of them we are mainly concerned with interactions between one portion of matter and another portion occupying a dif- ferent position in space; such interactions have very uniform and comparatively simple relations ; and the reason is traceable to the simple and uniform constitution of the intervening medium in which they have their seat. The other province is that in which the distribution of the material molecules comes into account. Set- ting aside the ordinary dynamics of matter in bulk, which is founded on the uniformity of the properties of the bodies concerned and their experimental deter- mination, we must assign to this region all phenomena which are concerned with the uncoordinated motions of the molecules, including the range of thermal and in part of radiant actions; the only possible basis for detailed theory is the statistical dynamics of the distribution of the molecules. The far more deep-seated and 618 REPORT—1900. mysterious processes which are involved in changes in the constitution of the indi- vidual molecules themselves are mainly outside the province of physics, which is competent to reason only about permanent material systems; they must be left to the sciences of chemistry and physiology. Yet the chemist proclaims that he can determine only the results of his reactions and the physical conditions under which they occur; the character of the bonds which hold atoms in their chemical combinations is at present unknown, although a large domain of very precise knowledge relating, in some diagrammatic manner, to the topography of the more complex molecules has been attained. The vast structure which chemical science has in this way raised on the narrow foundation of the atomic theory is perhaps the most wonderful existing illustration both of the rationality of natural processes and of the analytical powers of the human mind. In a word, the com- plication of the material world is referable to the vast range of structure and of states of aggregation in the material atoms; while the possibility of a science of physics is largely due to the simplicity of constitution of the universal medium through which the individual atoms interact on each other. The reference of the uniformity in the interactions at a distance between material bodies to the part played by the wether is a step towards the elimination of extraneous and random hypotheses about laws of attraction between atoms. It also places that medium on a different basis from matter, in that its mode of activity is simple and regular, whereas intimate material interactions must be of illimitable complexity. This gives strong ground for the view that we should not be tempted towards explaining the simple group of relations which have been found to define the activity of the ether, by treating them as mechanical consequences of concealed structure in that medium; we should rather rest satisfied with having attained to their exact dynamical correlation, just as geometry explores or corre- lates, without explaining, the descriptive and metric properties of space. On the other hand, a view is upheld which considers the pressures and thrusts of the engineer, and the strains and stresses in the material structures by which he transmits them from one place to another, to be the archetype of the processes by which all mecha- nical effect is transmitted in nature. This doctrine implies an expectation that we may ultimately discover something analogous to structure in the celestial spaces, by means of which the transmission of physical effect will be brought into line with the transmission of mechanical effect by material framework. At a time when the only definitely ascertained function of the ether was the undulatory propagation of radiant energy across space, Lord Kelvin pointed out that, by reason of the very great velocity of propagation, the density of the radiant energy in the medium at any place must be extremely small in comparison with the amount of energy that is transmitted in a second of time: this easily led him to the very striking conclusion that, on the hypothesis that the wther is like material elastic media, it is not necessary to assume its density to be more than 1078 of that of water, or its optical rigidity to be more than ten 10° of that of steel or glass. Thus far the zether would be merely an impalpable material atmosphere for the transference of energy by radiation, at extremely small densities but with very great speed, while ordinary matter would be the seat of practically all this energy. But this way of explaining the absence of sensible influence of the ether on the phenomena of material dynamics lost much of its basis as soon as it was recognised that the same medium must be the receptacle of very high densities of energy in the electric fields around currents and magnets. The other mode of explanation 1 We can here only allude to Lord Kelvin’s recent most interesting mechanical illustrations of a solid ether interacting with material molecules and with itself by attraction at a distance: unlike the generalised dynamical methods expounded in the text, which can leave the intimate structure of the material molecule outside the problem, a definite working constitution is there assigned to the molecular nucleus. It is pointed out in a continuation that is to appear in the Phil. Mag. for September, that a density of eether of the order of only 10-®, which would not appreciably affect the inertia of matter, would involve rigidity comparable with that of steel, and thus permit transmission of magnetic forces by stress; this solid ether is however, as usual, taken to be freely permeable to the molecules of matter. — es TRANSACTIONS OF SECTION A, 619 is to consider the «ether to be of the very essence of all physical actions, and to ° correlate the absence of obvious mechanical evidence of its intervention with its regularity and universality. On this plan of making the ether the essential factor in the transformation of energy as well as its transmission across space, the material atom must be some kind of permanent nucleus that retains around itself an ethereal field of physical influence, such as, for example, a field of strain. We can recognise the atom only through its interactions with other atoms that are so far away from it as to be practically independent systems; thus our direct knowledge of the atom will he confined to this field of force which belongs to it. Just as the exploration of the distant field of magnetic influence of a steel magnet, itself concealed from view, cannot tell us anything about the magnet except the amount and direction of its moment, so a practically complete knowledge of the field of physical influence of an atom might be expressible in terms of the numerical values of a limited number _ of physical moments associated with it, without any revelation as to its essential structure or constitution being involved. This will at any rate be the case for ultimate atoms if, as is most likely, the distances at which they are kept apart are large compared with the diameters of the atomic nuclei; it in fact forms our only chance for penetrating to definite dynamical views of molecular structure. So long as we cannot isolate a single molecule, ‘but must deal observationally with an innumerable distribution of them, even this kind of knowledge will be largely con- fined to average values. But the last half-century has witnessed the successful application of a new instrument of research, which has removed in various direc- tions the limitations that had previously been placed on the knowledge to which it was possible for human effort to look forward. The spectroscope has created a new astronomy by revealing the constitutions and the unseen internal motions of the stars. Its power lies in the fact that it does take hold of the internal relations of the individual molecule of matter, and provide a very definite and detailed, though far from complete, analysis of the vibratory motions that are going on in it ; these vibrations being in their normal state characteristic of its dynamical consti- tution, and in their deviations from the normal giving indications of the velocity of its movement and the physical state of itsenvironment. Maxwell long ago laid emphasis on the fact that a physical atomic theory is not competent even to con- template the vast mass of potentialities and correlations of the past and the future, that biological theory has to consider as latent in a single organic germ containing at most only a few million molecules. On our present view we can accept his position that the properties of such a body cannot be those of a ‘purely material system,’ provided, however, we restrict this phrase to apply to physical properties as here defined. But an exhaustive discovery of the intimate nature of the atom is beyond the scope of physics; questions as to whether it must not necessarily involve in itself some image of the complexity of the organic structures of which it. can form a correlated part must remain a subject of speculation outside the domain of that science. It might be held that this conception of discrete atoms and continuous ether really stands, like those of space and time, in intimate relation with our modes of mental apprehension, into which any consistent picture of the external world must of necessity be fitted. In any case it would involve abandonment of all the successful traditions of our subject if we ceased to hold that our analysis can be formulated in a consistent and complete manner, so far as it goes, without being necessarily an exhaustive account of phenomena that are beyond our range of experiment. Such phenomena may be more closely defined as those connected with the processes of intimate combination of the molecules: they include the activities of organic beings which all seem to depend on change of molecular structure. Tf, then, we have so small a hold on the intimate nature of matter, it will appear all the more striking that physicists have been able precisely to divine the mode of operation of the intangible ether, and to some extent explore in it the fields of hysical influence of the molecules. On consideration we recognise that this owledge of fundamental pkysical interaction has been reached by a comparative process. The mechanism of the propagation of light could never have been studied 620 REPORT—1900. in the free zether of space alone. It was possible, however, to determine the way in which the characteristics of optical propagation are modified, but not wholly transformed, when it takes place in a transparent material body instead of empty space. The change in fact arises on account of the «ther being entangled with the network of material molecules; but inasmuch as the length of a single wave of radiation covers thousands of these molecules the wave-motion still remains uni- form and does not lose its general type. A wider variation of the experimental conditions has been provided for our examination in the case of those substances in which the phenomenon of double refraction pointed to a change of the ethereal properties which varied in different directions; and minute study of this modifica- tion has proved sufficient to guide to a consistent appreciation of the nature of this change, and therefore of the mode of ethereal propagation that is thus altered. In the same way, it was the study and development of the manner in which the laws of electric phenomena in material bodies had been unravelled by Ampére and Faraday, that guided Faraday himself and Maxwell—who were impressed with the view that the zether was at the bottom of it all— in their progress towards an application of similar laws to ether devoid of matter, such as would complete a scheme of continuous action by consistently interconnecting the material bodies and banishing all untraced interaction across-empty space. Maxwell in fact chose to finally expound the theory by ascribing to the sether of free space a dielectric constant and a magnetic constant of the same types as had been found to express the properties of material media, thus extending the seat of the phenomena to all space on the plan of describing the activity of the ether in terms of the ordinary electric ideas. The converse mode of development, starting with the free ether under the directly dynamical form which has been usual in physical optics, and introducing the influence of the material atoms through the electric charges which are involved in their constitution, was hardly employed by him; in part, perhaps, because, owing to the necessity of correlating his theory with existing electric lmowledge and the mode of its expression, he seems never to have reached the stage of moulding it into a completely deductive form. The dynamics of the eether, in fact the recognition of the existence of an «ther, has thus, as a matter of history, been reached through study of the dynamical phenomena of matter. When the dynamics of a material system is worked up to its purest and most general form, it becomes a formulation of the relations between the succession of the configurations and states of motion of the system, the assist- ance of an independent idea of force not being usually required. We can, however,’ only attain to such a compact statement when the system is self-contained, when its motion is not being dissipated by agencies of frictional type, and when its con- nections can be directly specified by purely geometrical relations between the coordinates, thus excluding such mechanisms as rolling contacts. The courseof the system is then in all cases determined by some form or other of a single fundamental property, that any alteration in any small portion of its actual course must produce an increase in the total ‘ Action’ of the motion. It is to be observed that in employing this law of minimum as regards the Action expressed as an integral over the whole time of the motion, we no more introduce the future course as a determining influence on the present state of motion than we do in drawing a straight line from any point in any direction, although the length of the line is the minimum distance between itsends. In drawing the line piece by piece we have to make tentative excursions into the immediate future in order to adjust each element into straightness with the previous element; so in tracing the next stage of the motion of a material system we have similarly to secure that it is not given any such directions as would unduly increase the Action. But whatever views may be held as to the ultimate significance of this principle of Action, its importance, 1 In 1870 Maxwell, while admiring the breadth of the theory of Weber, which is virtually based on atomic charges combined with action at a distance, still regarded it as irreconcilable with his own theory, and left to the future the question as to why ‘theories apparently so fundamentally opposed should have so large a field of truth common to both.’—‘ Scientific Papers,’ ii, p. 228, TRANSACTIONS OF SECTION A. 621 not only for mathematical analysis, but asa guide to physical exploration, remains fundamental. When the principles of the dynamics of material systems are refined down to their ultimate common basis, this principle of minimum is what remains. Hertz preferred to express its contents in the form of a principle of straightness of course or path. It will be recognised, on the lines already indicated, that this is another mode of statement of the same fundamental idea; and the general equiva- lence is worked out by Hertz on the basis of Hamilton’s development of the prin- ciples of dynamics. The latter mode of statement may be adaptable so as to avoid the limitations which restrict the connections of the system, at the expense, however, of introducing new variables ; if, indeed, it does not introduce gratuitous complexity for purposes of physics to attempt to do this. However these questions may stand, this principle of straightness or directness of path forms, wherever it applies, the most general and comprehensive formulation of purely dynamical action: it involves in itself the complete course of events. In so far as we are given the algebraic formula for the time-integral which constitutes the Action, expressed in terms of any suitable coordinates, we know implicitly the whole dynamical constitution and history of the system to which it applies’ Two systems in which the Action is expressed by the same formula are mathematically identical, are physically pre- cisely correlated, so that they have all dynamical properties in common. When the structure of a dynamical system is largely concealed from view, the safest and most direct way towards an exploration of its essential relations and connections, and in fact towards answering the prior question as to whether it is a purely dynamical system at all, is through this order of ideas. The ultimate test that a system is a dynamical one is not that we shall be able to trace mechanical stresses throughout it, but that its relations can be in some way or other consolidated into accordance with this principle of minimum Action. This definition of adynamical system in terms of the simple principle of directness of path may conceivably be subject to objection as too wide; it is certainly not too narrow; and it is the conception which has naturally been evolved from two centuries of study of the dynamics of material bodies. Its very great generality may lead to the objection that we might completely formulate the future course of a system in its terms, with- out having obtained a working familiarity with its details, of the kind to which we have become accustomed in the analysis of simple material systems ; but our choice is at present between this kind of formulation, which is a real and essential one, and an empirical description of the course of phenomena combined with expla- nations relating to more or less isolated groups. The list of great names, including Kelvin, Maxwell, Helmholtz, that have been associated with the employment of the principle for the elucidation of the relations of deep-seated dynamical pheno- mena, is a strong guarantee that we shall do well by making the most of this clue. Are we then justified in treating the material molecule, so far as revealed by the spectroscope, as a dynamical system coming under this specification? Its intrinsic energy is certainly permanent and not subject to dissipation; otherwise the molecule would gradually fade out of existence. The extreme precision and regularity of detail in the spectrum shows that the vibrations which produce it are exactly synchronous, whatever be their amplitude, and in so far resemble the vibrations of small amplitude in material systems. As all indications point to the molecule being a system in a state of intrinsic motion, like a vortex ring, or a stellar system in astronomy, we must consider these radiating vibrations to take place around a steady state of motion which does not itself radiate, not around a state of rest. Now not the least of the advantages possessed by the Action prin- ciple, as a foundation for theoretical physics, is the fact that its statement can be adapted to systems involving in their constitution permanent steady motions of this kind, in such a way that only the variable motions superposed on them come into consideration. The possibilities as regards physical correlation of thus intro- ducing permanent motional states as well as permanent structure into the con- stitution of our dynamical systems have long been emphasised by Lord Kelvin; * ' For a classical exposition see his Brit. Assoc. Address of 1884 on ‘ Steps towards Kinetic Theory of Matter,’ reprinted in ‘ Popular Lectures and Addresses,’ vol. i. 622 REPORT—1900. the effective adaptation of abstract dynamics to such systems was made inide- pendently by Kelvin and Routh about 1877; the more recent exposition of the theory by Helmholtz has directed general attention to what is undoubtedly the most significant extension of dynamical analysis which has taken place since the time of Lagrange. ' Returning to the molecules, it is now verified that the Action principle forms a valid foundation throughout electrodynamics and optics; the introduction of the zether into the system has not affected its application. It is therefore a reasonable hypothesis that the principle forms an allowable foundation for the dynamical analysis of the radiant vibrations invthe system formed by a single molecule and surrounding ether; and the knowledge which is now accumulating, both of the orderly grouping of the lines of ‘the spectrum and of the modifications impressed on these lines by a magnetic field or by the density of the matter immediately surrounding the vibrating molecule, can hardly fail to be fruitful for the dynamical analysis of its constitution. But let it be repeated that this analysis would be complete when a formula for the dynamical energy of the molecule is obtained, and would go no deeper. | Starting from our definitely limited definition of the nature of a dynamical system, the problem is merely to correlate the observed relations of the periods of vibration in a molecule, when it has come into a steady state as regards constitution and is not under the influence of intimate encounter with other molecules. It may be recalled incidentally that the generalised Maxwell-Boltzmann principle of the equable distribution of the acquired store of kinetic energy of the molecule, among its various possible independent types of motion, is based directly on the validity of the Action principle for its dynamics. In the demonstrations usually offered the molecule is considered to have no permanent or constitutive energy of internal motion. It can, however, be shown, by use of the generalisa- tion aforesaid of the Action principle, that no discrepancy will arise on that account. Such intrinsic kinetic energy virtually adds on to the potential energy of the system; and the remaining or acquired part of the kinetic energy of the molecule may be made the subject of the same train of reasoning as before. Let us now return to the general question whether our definition of a dyna- mical system may not be too wide. As acase in point, the single principle of Action has been shown to provide a definite and sufficient basis for electro- dynamics; yet when, for example, one armature of an electric motor pulls the other after it without material. contact, and so transmits mechanical power, no connection between them is indicated by the principle such as could by virtue of internal stress transmit the pull. The essential feature of the transmission of a pull by stress across a medium is that each element of voiume of the medium acts by itself, independently of the other elements. The stress excited in any element depends on the strain or other displacement occurring in that element alone ; and the mechanical effect that is transmitted is considered as an extraneous force applied at one place in the medium, and passed on from element to element through these internal pressures and tractions until it reaches another place. We have, however, to consider two atomic electric charges as being themselves some kind of strain configurations in the wether; each of them already involves an atmosphere of strain in the surrounding ether which is part of its essence, and cannot be considered apart from it; each of them essentially pervades the entire space, though on account of its invariable character we consider it as a unit. Thus we appear to be debarred from imagining the ether to act as an elastic connection which is merely the agent of transmission of a pull from the one nucleus to the other, because there are already stresses belonging to and consti- tuting an intrinsic part of the terminal electrons, which are distributed all along the medium. Our Action criterion of a dynamical system, in fact, allows us to reason about an electron as a single thing, notwithstanding that its field of energy is spread over the whcle medium; it is only in material solid bodies, and in problems in which the actual sphere of physical action of the molecule is small compared with the smallest element of volume that our analysis considers, that the familiar idea of transmission of force by simple stress can apply. Whatever view may TRANSACTIONS OF SECTION A, 623 ultimately commend itself, this question is one that urgently demands decision. A very large amount of effort has been expended by Maxwell, Helmholtz, Heaviside, Hertz, and other authorities in the attempt to express the mechanical phenomena of electrical action in terms of a transmitting stress. ‘The analytical results up to a certain point have been promising, most strikingly so at the beginning, when Maxwell established the mathematical validity of the way in which Faraday was accustomed to represent to himself the mechanical interactions across space, in terms of a tension along the lines of force equilibrated by an equal pressure preveuting their expansion sideways. According to the views here deve- loped, that ideal is an impossible one; if this could be established to general satisfaction the field of theoretical discussion would be much simplified. This view that the atom of matter is,so far as regards physical actions, of the nature of a structure in the «ther involving an atmosphere of «ethereal strain all around it, not a small body which exerts direct actions at a distance on other atoms according to extraneous laws of force, was practically foreign to the eighteenth century, when mathematical physics was modelled on the Newtonian astronomy and dominated by its splendid success. The scheme of material dynamics, as finally compactly systematised by Lagrange, had therefore no direct relation to such a view, although it has proved wide enough to include it. The remark has often been made that it is probably owing to Faraday’s mathematical instinct, combined with his want of acquaintance with the existing analysis, that the modern theory of the zther obtained a start: from the electric side. “Through his teaching and the weight of his authority, the notion of two electric currents exerting their mutual forces by means of an intervening medium, instead of by direct attraction across space, was at an early period firmly grasped in this country. In 1845 Lord Kelvin was already mathematically formulating, with most suggestive success, continuous elastic connections, by whose strain the fields of activity of electric currents or of electric distributions could be illustrated ; while the exposition of Maxwell’s interconnected scheme, in the earlier form in which it relied on concrete models of the electric action, goes back almost to 1860. Corresponding to the two physical ideals of isolated atoms exerting attraction at a distance, and atoms operating by atmospheres of ethereal strain, there are, as already indicated, two different developments of dynamical theory. The original Newtonian equations of motion determined the course of a system by expressing the rates at which the velocity of each of its small parts or elements is changing. This method is still fully applicable to those problems of gravitational astronomy in which dynamical explanation was first successful on a grand scale, the planets heing treated as point-masses, each subject to the gravitational attraction of the other bodies. But the more recent development of the dynamies of complex systems depends on the fact that analysis has been able to reduce within manageable limits the number of varying quantities whose course is to be explicitly traced, through taking advantage of those internal relations of the parts of the system that are invariable, either geometrically or dynamically. Thus, to take the simplest case, the dynamics of a solid body can be confined to a discussion of its three com- ponents of translation and its three components of rotation, instead of the motion of each element of its mass. With the number of independent coordinates thus diminished, when the initial state of the motion is specified the subsequent course of the complete system can be traced; but the course of the changes in any part of it can only be treated in relation to the motion of the system asawhole. It is just this mode of treatment of a system as a whole that is the main characteristic of modern physical analysis. The way in which Maxwell analysed the interactions of a system of linear electric currents, previously treated as if each were made up of small independent pieces or elements, and accumulated the evidence that they formed a single dynamical system, is a trenchant example. The interactions of vortices in fluid form a very similar problem, which is of special note in that the constitution of the system is there completely known in advance, so that the two modes of dynamical exposition can be. compared. In this case the older method forms independent equations for the motion of each material element of the fluid, aud so requires the introduction of the stress—here the fluid pressure—hy which 624 REPORT—1900: dynamical effect is passed on to it from the surrounding eléménts: if cotresjonds to a method of contact action. But Helmholtz opened up new ground in the abstract dynamics of continuous media when he recognised (after Stokes) that, if the dis- tribution of the velocity of spin at those places in the fluid where the motion is vortical be assigned, the motion in every part of the fluid is therein kinemati- cally involved. This, combined with the theorem of Lagrange and Cauchy, that the spin is always confined to the same portions of the fluid, formed a starting- point for his theory of vortices, which showed how the subsequent course of the motion can be ascertained without consideration of pressure or other stress. The recognition of the permanent state of motion constituting a vortex ring as a determining agent as regards the future course of the system was in fact justly considered by Helmholtz as one of his greatest achievements. The principle had entirely eluded the attention of Lagrange and Cauchy and Stokes, who were the pioneers in this fundamental branch of dynamics, and had virtually prepared all the necessary analytical material for Helmholtz’s use. The main import of this advance lay, not in the assistance which it afforded to the development of the complete solution of special problems in fluid motion, but in the fact that it con- stituted the discovery of the types of permanent motion of the system, which could combine and interact with each other without losing their individuality, though each of them pervaded the whole field. This rendered possible an entirely new mode of treatment; and mathematicians who were accustomed, as in astronomy, to aim directly at the determination of all the details of the special case of motion, were occasionally slow to apprehend the advantages of a procedure which stopped at formulating a description of the nature of the interaction between various typical groups of motions into which the whole disturbance could be resolved. The new train of ideas introduced into physics by Faraday was thus consolidated and emphasised by Helmholtz’s investigations of 1858 in the special domain of hydro- dynamics. In illustration let us consider the fluid medium to be pervaded by per- manent vortices circulating round solid rings as cores: the older method of analysis would form equations of motion for each element of the fluid, involving the fluid pressure, and by their integration would determine the distribution of pressure on each solid ring, and thence the way it moves. This method is hardly feasible even in the simplest cases. The natural plan is to make use of existing simplifications by regarding each vortex as a permanent reality, and directly attacking the problem of its interactions with the other vortices. The energy of the fluid arising from the vortex motion can be expressed in terms of the positions and strengths of the vor- tices alone; and then the principle of Action, in the generalised form which includes steady motional configurations as well as constant material configura- tions, affords a method of deducing the motions of the cores and the interactions between them. Ifthe cores are thin they in fact interact mechanically, as Lord Kelvin and Kirchhoff proved, in the same manner as linear electric currents would do; though the impulse thence derived towards a direct hydro-kinetic explanation of electro-magnetics was damped by the fact that repulsion and attraction have to be interchanged in the analogy. The conception of vortices, once it has been arrived at, forms the natural physical basis of investigation, although the older method of determining a distribution of pressure-stress throughout the fluid and examining how it affects the cores is still possible ; that stress, however, is not simply transmitted, asit hasto maintain the changes of velocity of the various portions of the fluid. But if the vortices have no solid cores we are at a loss to know where even this pressure can be considered as applied to them; if we follow up the stress, we lose the vortex; yet a fluid vortex can nevertheless illustrate an atom of matter, and we can consider such atoms as exerting mutual forces, only these forces cannot be consi- dered as transmitted through the agency of fluid pressure. The reason is that the vortex cannot now be identified with a mere core bounded by a definite surface, but is essentially a configuration of motion extending throughout the medium. Thus we are again in face of the fundamental question whether all attempts to * ‘We may compare G. W. Hill’s more recent introduction of the idea of permanent orbits into physical astronomy, TRANSACTIONS OF SECTION A. 625 represent the mechanical interactions of electro-dynamic systems, as transmitted from 7 to point by means of simple stress, are not doomed to failure; whether they o not, in fact, introduce unnecessary and insurmountable difficulty into the theory. The idea of identifying an atom with a state of strain or motion, pervading the region of the zether around its nucleus, appears to demand wider views as to what constitutes dynamical transmission. The idea that any small portion of the primordial medium can be isolated, by merely introducing tractions acting over its surface and transmitted from the surrounding parts, is no longer appropriate or consistent: a part of the dynamical disturbance in that element of the medium is on this hypo- thesis already classified as belonging to, and carried along with, atoms that are outside it but in its neighbourhood—and this part must not be counted twice over. The law of Poynting relating to the paths of the transmission of energy is known to hold in its simple form only when the electric charges or currents are in a steady state ; when they are changing their positions or configurations their own fields of _ intrinsic energy are carried along with them. It is not surprising, considering the previous British familiarity with this order of ideas, that the significance for general physics of Helmholtz’s doctrine of vortices was eagerly developed in this country, in the form in which it became embodied through Lord Kelvin’s famous illustration of the constitution of matter, as consisting of atoms with separate existence and mutual interactions. This vortex-atom theory has been a main source of physical suggestion because it presents, on a simple basis, a dynamical picture of an ideal material system, atomically constituted, which could go on automatically without extraneous sup- port. ‘The value of such a picture may be held to lie, not in any supposition that this is the mechanism of the actual world laid bare, but in the vivid illustration it affords of the fundamental postulate of physical science, that mechanical phenomena are not parts of a scheme too involved for us to explore, but rather present themselves in definite and consistent correlations, which we are able to dis- entangle and apprehend with continually increasing precision. It would be an interesting question to trace the origin of our preference for a theory of transmission of physical action over one of direct action at a distance. It may be held that it rests on the same order of ideas as supplies our conception of force ; that the notion of effort which we associate with change of the motion of a body involves the idea of a mechanical connection through which that effort is applied. The mere idea of a transmitting medium would then be no more an ultimate foundation for physical explanation than that of force itself. Our choice between direct distance action and mediate transmission would thus be dictated by the relative simplicity and coherence of the accounts they give of the phenomena: this is, in fact, the basis on which Maxwell’s theory had to be judged until Hertz detected the actual working of the medium. Instantaneous transmis- sion is to all intents action at a distance, except in so far as the law of action may be more easily formulated in terms of the medium than in a direct’ geometrical Statement. In connection with these questions it may be permitted to refer to the eloquent and weighty address recently delivered by M. Poincaré to the International Con- gress of Physics. M. Poincaré accepts the principle of Least Action as a reliable basis for the formulation of physical theory, but he imposes the condition that the results must satisfy the Newtonian law of equality of action and reaction between each pair of bodies concerned, considered by themselves ; this, however, he would allow to be satisfied indirectly, if the effects could be traced across the intervening xther by stress, so that the tractions on the two sides of each ideal interface are equal and opposite! As above argued, this view appears to exclude ab initio all atomic theories of the general type- of vortex atoms, in which the energy of the atom is distributed throughout ‘ Gf. also Hertz on the electro-magnetic equations, § 12, Wied. Ann., 1890. [The standpoint of Hertz’s posthumous Mechanik approximates, however, to that here maintained. | The problem of merely replacing a system of forces bya statical stress is. widely indeterminate, and therefore by itself unreal; the actual question is whether any such representation can be coordinated with existing dynamics. 1990 88 626 REPORT—1900. the medium instead of being concentrated in a nucleus; and this remark seems to go to the root of the question. On the other hand, the position here asserted is that recent dynamical developments have permitted the extension of the principle of Action to systems involving permanent motions, whether obvious or latent, as part of their constitution; that on this wider basis the atom may itself involve a state of steady disturbance extending through the medium, instead of being only a local structure acting by push and pull. The possibilities of dynamical explanation are thus enlarged. The most definite type of model yet imagined of the physical interaction of atoms through the ether is, perhaps, that which takes the ether to be a rotationally elastic medium after the manner of MacCullagh and Rankine, and makes the ultimate atom include the nucleus of a permanent rotational strain- configuration, which as a whole may be called an electron. The question how far this is a legitimate and effective model stands by itself, apart from the dynamics which it illustrates; like all representations it can only cover a limited ground. For instance, it cannot claim to include the internal structure of the nucleus of an atom or even of an electron ; for purposes of physical theory that problem can be put aside, it may even be treated as inscrutable. All that is needed is a postulate of free mobility of this nucleus through the ether. This isdefinitely hypothetical, but it is not an unreasonable postulate because a rotational ether has the properties of a perfect fluid medium except where differentially rotational motions are concerned, and so would not react on the motion of any structure moving through it except after the manner of an apparent change of inertia. It thus seems possible to hold that such a model forms an allowable representation of the dynamical activity of the sether, as distinguished from the complete constitution of the material nuclei between which that medium establishes connection. At any rate, models of this nature have certainly been most helpful in Max- well’s hands towards the effective intuitive grasp of a scheme of relations as a whole, which might have proved too complex for abstract unravelment in detail. When a physical model of concealed dynamical processes has served this kind of purpose, when its content has been explored and estimated, and has become familiar through the introduction of new terms and ideas, then the ladder by which we have ascended may be kicked away, and the scheme of relations which the model embodied can stand forth in severely abstract form. Indeed many of the most fruitful branches of abstract mathematical analysis itself have owed their start in this way to concrete physical conceptions. This gradual transition into abstract statement of physical relations in fact amounts to retaining the essentials of our working models while eliminating the accidental elements involved in them; elements of the latter kind must always be present because otherwise the model would be identical with the thing which it represents, whereas we cannot expect to mentally grasp all aspects of the content of even the simplest phenomena. Yet the abstract standpoint is always attained through the concrete; and for purposes of instruction such models, properly guarded, do not perhaps ever lose their value: they are just as legitimate aids as geometrical diagrams, and they have the same kind of limitations. In Maxwell's words, ‘ for the sake of persons of these different types scientific truth should be presented in different forms, and should be regarded as equally scientific whether it appear in the robust form and the vivid colouring of a physical illustration, or in the tenuity and paleness of a symbolical expression.’ The other side of the picture, the necessary incomplete- ness of even our legitimate images and modes of representation, comes out in the despairing opinion of Young (‘Chromatics,’ 1817), at a time when his faith in the undulatory theory of light had been eclipsed by Malus’s discovery of the pheno- mena of polarisation by reflection, that this difficulty ‘ will probably long remain, to mortify the vanity of an ambitious philosophy, completely unresolved by any theory:’ not many years afterwards the mystery was solved by Fresnel. This process of removing the intellectual scaffolding by which our knowledge is reached, and preserving only the final formula which express the correlations of the directly observable things, may moreover readily be pushed too far. It asserts the conception that the universe is like an enclosed clock that is wound up to go, and that accordingly we can observe that it is going, and can see some of TRANSACTIONS OF SECTION A. 627 its more superficial movements, but not much of them; that thus, by patient obser- vation and use of analogy, we can compile, in merely tabular form, information as to the manner in which it works and is likely to go on working, at any rate for some time to come; but that any attempt to probe the underlying connection is illusory or illegitimate. As a theoretical precept this is admirable. It minimises the danger of our ignoring or forgetting the limitations of human faculty, which can only utilise the imperfect representations that the external world impresses on our senses. On the other hand such a reminder has rarely been required by the master minds of modern science, from Descartes and Newton onwards, whatever their theories may have been. Its danger as a dogma lies in its application. Who is to decide, without risk of error, what is essential fact and what is intellec tual scaffolding ? To which class does the atomic theory of matter belong? That is, indeed, one of the intangible things which it is suggested may be thrown over- board in sorting out and classifying our scientific possessions. Is the mental idea or image, which suggests, and alone can suggest, the experiment that adds to our concrete knowledge, less real than the bare phenomenal uniformity which it has revealed? Is it not, perhaps, more real in that the uniformities might not have been there in the absence of the mind to perceive them ? No time is now left for review of the methods of molecular dynamics. Here our knowledge is entirely confined to steady states of the molecular system : it is purely statical. In ordinary statics and the dynamics of undisturbed steady notions, the form of the energy function is the sufficient basis of the whole subject. This method is extended to thermo-dynamics by making use of the mechanically available energy of Rankine and Kelvin, which is a function of the bodily contiguration and chemical constitution and temperature of the system, whose value cannot under any circumstances spontaneously increase, while it will diminish in any operation which is not reversible. In the statics of systems in equilibrium or in steady motion, this method of energy is a particular case of the method of Action; but in its extension to thermal statics it is made to include chemical as well as configurational changes, and a new point appears to arise, Whether we do or do not take it to be possible to trace the application of the principle of Action throughout the process of chemical combination of two mole- cules, we certainly here postulate that the static case of that principle, which applies to steady systems, cam be extended across chemical combinations. The question is suggested whether extension would also be valid to transformations which involve vital processes. This seems to be still considered an open question by the best authorities. If it be decided in the negative a distinction is involved between vital and merely chemical processes. It is now taken as established that vital activity cannot create energy, at any rate in the long run which is all that can from the nature of the case be tested. It seems not unreascreble to follow the analogy of chemical actions, and assert - that it cannot in the long run increase the mechanical availability of energy—that is, considering the organism as an apparatus for transforming energy without being itself in the long run changed. But we cannot establish a Carnot cycle for a portion of an organism, nor can we do so for a limited period of time; there might be creation of availability acc mpanied by changes in the organism itself, but compensated by destruction and the inverse changes a long time afterwards. This amounts to asserting that where, as in a vital system or even in a simple molecular combination, we are unable to trace or even assert complete dynamical Sequence, exact thermodynamic statements should be mainly confined to the activity of the existing organism as a whole; it may transform inorganic material without change of energy and without gain of availability, although any such Statements would be inappropriate and unmeaning as regards the details of the processes that take place inside the organism itself. In any case it would appear that there is small chance of reducing these ques- tions to direct dynamics; we should rather regard Carnot’s principle, which in- cludes the law of uniformity of temperature and is the basis of the whole theory, as a property of statistical type confined to stable or permanent aggregations of matter. Thus no dynamical proof from molecular considerations could be regarded - ESQ 628 REPORT—1900. as valid unless it explicitly restricted the argument to permanent systems; yet the conditions of permanency are unknown except in the simpler cases. The only mode of discussion that is yet possible is the method of dynamical statistics of mole- cules introduced by Maxwell. Now statistics is a method of arrangement rather than of demonstration. Every statistical argument requires to be verified by com- parison with the facts, because it is of the essence of this method to take things as fortuitously distributed except in so far as we know the contrary; and we simply may not know essential facts to the contrary. For example, if the interaction of the «ther or other cause produces no influence to the contrary, the presumption would be that the kinetic energy acquired by a molecule is, on the average, equally distributed among its various independent modes of motion, whether vibrational or translational. Assuming this type of distribution to be once established in a gaseous system, the dynamics of Boltzmann and Maxwell show that it must be permanent. But its assumption in the first instance is a result rather of the absence than of the presence of knowledge of the circumstances, and can be accepted only so far as it agrees with the facts; our knowledge of the facts of specitic heat shows that it must be restricted to modes of motion that are homo- logous. In the words of Maxwell, when he first discovered in 1860, to his great surprise, that in a system of colliding rigid atoms the energy would always be equally divided between translatory and rotatory motions, it is only necessary to assume, in order to evade this unwelcome conclusion, that * something essential to the complete statement of the physical theory of molecular encounters must have hitherto escaped us.’ Our survey thus tends to the result, that as regards the simple and uniform phenomena which involve activity of finite regions of the universal «ther, theoretical physics can lay claim to constructive functions, and can build up a definite scheme; but in the domain of matter the most that it can do is to accept the existence of such permanent molecular systems as present themselves to our notice, and fit together an outline plan of the more general and universal features in their activity. Our well-founded belief in the rationality of natural processes asserts the possibility of this, while admitting that the intimate details of atomic constitution are beyond our scrutiny and provide plenty of room for processes that transcend finite dynamical correlation. The following Papers were read :— 1. Note on M. Cremiew’s Experiment. By Prof. G. F, FitzGeraup, 7.2.8. M. Cremieu has shown that, if his experimental methods can bear criticism as well as they seem to do, there is no induced electromotive force on a coil of wire surrounding a rotating dise when the strength of an electric charge on the dise is changing. He has deduced from this the conclusion that there is no magnetic induction through the disc due to the moving charge such as Rowland’s experi- ments showed. This note is to point out that tov little is known of the theory of the ethereal effects of a charge of electricity forced to move by mechanical actions for us to be quite sure that both M. Cremieu’s and Rowland’s observations may not be true—ie., that it is possible that a charge of electricity, while it is being accelerated by moving matter, may produce such an action on the surrounding ether as to neutralise the electric force that would otherwise be produced by the changing magnetic induction due to the moving charge. 2. On the Creeping of Liquids and the Surface Tension of Mixtures. By Dr. F. T. Trovroy, 2.5. 3. On a Method of Investigating Correspondences between Spectra. By Huew Ramace. The method is graphical ; spectral lines are plotted as abscisswe, and the atomic weights of the elements, or functions of the atomic weights, as ordinates, Con- TRANSACTIONS OF SECTION A, 629 necting lines are then drawn through homologous spectral lines. The spectra studied by the author in this way are chiefly those emitted by the metals in the oxyhydrogen and oxycoal gas flames. These spectra are much simpler than those of the same metals in the electric arc or spark, and may be regarded as the funda- mental spectra of the metals. They are therefore the most suitable spectra for comparison. As the flame spectra of the metals have not been fully investigated some lines have been selected, to make the diagrams more complete, from arc and spark spectra. In these cases the selection was made after a study of the character of the lines in these spectra. Later experimental work on flame spectra has con- firmed the selection of some of these lines, and the work on the Zeeman effect, of Preston on magnesium, zinc, and cadmium, and of Lord Blythswood and Dr. Marchant on mercury, confirms it in the spectrum of the latter metal. The formule and work of Rydberg and of Kayser and Runge lead to the selection of the same lines in all cases, and with these formule as guides it is possible to extend the work to other lines and spectra. This has been done, but only to a limited extent at present. The diagrams exhibited were drawn—(1) from atomic weights and oscillation frequencies, and (2) from the squares of the atomic weigits and oscillation frequencies. The diagrams show very clearly that the spectra of similar elements are very closely related to one another. ‘That the spectra of potassium, rubidium, and cesium are more closely related to one another than to those of lithium and sodium, and that there is also a break between the spectrum of magnesium and those of zinc, cadmium, and mercury, and between that of aluminium and those of gallium, indium, and thallium. The connecting lines of the diffuse subordinate series of potassium, rubidium, and cesium approach in the more refrangible lines measured to straight lines, while those of the principal series are nearly straight lines in the second diagram. Tke lines joining the homologous lines of doublets and triplets approach one another as the atomic weight decreases, and, in the second diagram, intersect in points near the line of zero atomic weight. ‘These curves give exact information regarding the function of the atomic weight which determines the differences, in oscillation frequencies, between the lines in doublets and triplets. j Equations are given, after the form of Rydberg’s, for the principal series of lithium and sodium and of potassium, rubidium, and cesium, and the calculated numbers are in close agreement with the observed numbers. 4. Report on Radiation in a Magnetic Field.—See Reports, p. 52. 5, An Experiment on Simultaneous Contrast. By Grorce J. Burcu, I.A., LBS. It is well known that white objects seen against a red background look greenish- blue, and orange against a blue background. This phenomenon is shown in a striking manner in the following experiment due to Hering:—A small white disc is viewed with the left eye against a red background, and another similar disc is viewed against a blue background with the right eye. The discs are so placed as to occupy different positions in the field or view. The result, when the light has been properly adjusted, is that the observer sees an amethyst-blue disc and a topaz-yellow disc against a pale purple ground. The reason of thisis demonstrated by the author in the following experiment :— Two pieces of glass, one red and the other blue, are inserted in a stereoscope in place of the usual slide, each glass having two small squares of black paper on it. Viewed binocularly the four squares appear as two. In front of the instrument, but out of the direct line of sight, are two adjustable slits, and over the eye-lenses of the stereoscope are two diffraction gratings. The position of the slits is so arranged that the spectrum of the first order of the left-hand grating falls on the 630 REPORT— 1900. right-hand square, and that of the right-hand grating on the left-hand square, the two spectra, which can be adjusted to the same intensity, being thus seen side by side, one with the left eye on a red ground, and the other with the right eye on a blue ground. The red glass produces partial red blindness of the left eye, and the spectrum seen by it lacks red, the other colours being unaltered. And for a similar reason the spectrum seen by the right eye lacks blue, the effect being more notice- able owing to the contrast of sensation in the two eyes. In the author's opinion this experiment affords further confirmation of the views of Scherffer, Darwin, and Young in regard to contrast. 6. A Quartz-Calcite Symmetrical Doublet. By J. W. Girrorp. The difficulty in constructing lenses of crystals Gonsists chiefly in the double refraction, which causes confusion, As quartz is a positive, and calcite a negative, crystal, they tend to correct one another, although the separation of the lines in quartz is only one-twentieth of that in calcite. Both lenses are cut with their axes corresponding to the axes of the crystals. The wave-length situated at the point of greatest actinic activity is about 2748, as found by averaging the position of bright lines of the principal spectra as follows : W. L. Centre W. L. Centre Substance of maximum effect Substance of maximum effect Air ; 3 & . 3310 Lead . ; » B0bE Tron 5 : 3 - . 2655 J bray hy : . 2571 Magnesium . : P . 29380 Copper : . 2444 mea oy rie cali eek. we BODE. | Silver it batiag Cadmium : : 4 . 38023 | me Arsenic . 5 c : . 2600 2760°6 = Average. This was equalised with W. L. 5607 or the centre of visual activity. The indices were determined by using prisms polished on three sides, and by averaging the observations, so that the angle of the prism might be taken as exactly 60. The temperature was 59° Fahrenheit. W. iL. Element Quartz Calcite Ordinary Ray Cd | 15981316 5893 Na 15442497 16583555 dE0T Pb 15454613 16604548 2839 cd 15837464 1°7335025 2748 Cd 1:5875286 | 1:7415041 Extraordinary Ray 5893 D 15533652 | 1:4863913 5607 Pb | 15546100 | 14873448 2839 | Cd 1:5942126 15194123 2748 | 15226616 , In calculating the radii the formula W = was used, with the following R results for unity: 1 W=0 R = -4213664 S&R’=:2026631 | 8S!’ = 0 2 Sa » °33070931 » *1809102 » 1°6854657 3 th », "3160248 » ‘1746611 », 12640993 4 36 I) 4 3009760 » 1699643 » 1:0534160 5 he) | | 2809109 » . 71683743 » 8427328 6 » 25 », 2528198 » °1534578 » 6320496 7 Se » °2106832 » 1368452 » 4213664 8 Mere 6 » 1404555 » 1032977 » 2106832 a TRANSACTIONS OF SECTION A, 631 No 3x by 25 was taken, and the focus=12”. The angle tade with the axis by the ray in Calcite varied from 2°47’ 26” to 1°14’ 10” for W. L. 2748 and from 2°36’ 26” to 1°9’17” for W. L. 5607, and the spherical aberration of the combination for W. L. 2748 was —:051337, and for W. L. 5607 was —+069809. No. 5 would probably have covered better without introducing too much double refraction. 7. The Production of an Artificial Light of the same Character as Day- light. Ly Artuur Durton, W.A,, B.Sc., and WatTeR M. GARDNER, bradford Technical College. Tt is a matter of common experience that many colours alter in appearance when seen by artificial light. The extent to which colours may vary under different illumination is perhaps not commonly known, but is well illustrated by the range of dyed cloths exhibited. Amongst other patterns, one which is green by daylight becomes red-brown by gaslight ; a violet changes to purple; a grey to heliotrope; a shade of tan to a brick red. Particularly striking is a pattern woven from specially dyed yarns, which appears a uniform green colour by daylight, but which is figured by gaslight. Seen by the light of the electric arc, the patterns show similar but less marked changes. It may be of interest to indicate briefly how such peculiar changes of colour arise. The colour of a body depends in the first place on the nature of the incident light. In monochromatic red light a red appears much the same as in daylight, but a yellow changes to red, a green is almost black, while blues and violets become red. Gaslight shows a continuous spectrum from red to violet, but compared with daylight is of a strong orange colour due to an excess of rays in the red, orange, and yellow It does not, however, necessarily result that all colours appear redder by gaslight. It is, indeed, well known that the majority of colours change little by gaslight. This is due to the adaptability of the eye; if the light becomes redder, the eye becomes less sensitive to red; if the light is deficient in green, the eye becomes more sensitive to green. Persons working by guslight soon cease to notice its intense orange colour. It results that a grey produced by mixture of black and white appears grey under any illumination, and simple colours, such as reds, oranges, and some greens giving light confined practically to one part of the spectrum, undergo little change. Generally, however, the colour of a body is due to a mixture of light from different parts of the spectrum. All violet colours are transparent, not only for violet, but also for blue and red light; all blues transmit not only blue, violet, and green light, but also more or less red. Consequently, whenever a blue or violet is used in the production of what is called by artists a ‘tertiary’ colour, the general result is a colour having bright bands in different parts of the spectrum. A mixture of red, blue, and yellow to produce a neutral grey will show bright bands in the red and green—complementary colours, resulting in a proportion of white light. According to the exact position and intensity of these bands the grey will become redder or greener or may even remain unchanged by gaslight. Generally colours become redder under artificial light. This is due not merely to the redder character of artificial lights as compared with daylight, but to the peculiar transparency of colouring matters for red light. Among reds and yellow, we have many theoretically perfect colouring matters—a perfect yellow being one having sharp absorption in the violet and blue, and perfect transparency for green, yellow, orange, and red rays. A perfect blue would be transparent for violet, blue, and green, and opaque for the rest of the spectrum. Apparently such a blue can only be obtained by means of cupric salts. AJI other blue dyes and pigments we have examined agree in being more or less transparent for red light. Even greens transmit some red. This peculiar trans- parency of colours for red light is of primary importance in colour-matching. All 638 REPORT—1900: dyers know how persistent is the tendency to the development of red in the production of compound. shades, The need of an artificial light which should so closely resemble daylight as to show colours in their true relationship has long been felt by workers in colour. At present the electric are light is largely used for colour work, but, as we have seen, it is far from satisfactory. The peculiar character of daylight is due essentially to the modification produced by the atmosphere in the light from the sun. Light from a north sky as usually adopted for colour work is deficient in red, orange, and yellow rays, and consequently the light from a clear north sky is intensely blue. Starting with the electric arc light as being nearest daylight in character, we have attempted to imitate by direct absorption the effect produced by scattering in the atmosphere. The light of an arc lamp consists of two distinct parts:—(1) The light from the glowing carbons; (2) the light of the arc itself, characterised by its richness in violet rays. In lamps of the enclosed arc type the length of arc is increased, and consequently such lamps give a light richer in violet rays. Although arc lights vary somewhat in the proportion of violet light, they all agree in being richer than daylight in the amount of red, orange, and yellow rays, compared with the amount of green and blue. Owing to the peculiar transparency of colours to red light already noticed, it is of primary importance that the proportion of red light should be carefully adjusted. Small variations in the amount of violet light are of minor importance, owing to the eye being less sensitive to such rays, and also because in mixing colours there is not the same tendency to develop a band of violet as we have seen occurs in the red, since yellow colours generally have complete absorption in the violet. The required absorption of the less refrangible rays can be effected by means of blue cupric salts. A solution of copper sulphate shows strong absorption at the extreme red of the spectrum, the absorption extending with diminishing intensity into the green. For practical purposes the light from the arc is modified by passage through pale blue glass coloured by means of copper. This coloured glass may conveniently take the form of a globe veplacing the ordinary globe of the arc light. FRIDAY, SEPTEMBER 7. The following Papers were read :— 1, On the Statistical Dynamics of Gas Theory as rllustrated by Meteor Swarms and Optical Rays. By Dr. J. Larmor, £.4.8. Imagine a cloud of meteors pursuing an orbit in space under outside attraction —in fact, in any conservative field of force. Let us consider a group of the meteors around a given central one. As they keep together their velocities are nearly the same. When the central meteor has passed into another part of the orbit, the surrounding region containing these same meteors will have altered in shape; it will in fact usually have become much elongated. If we merely count large and small meteors alike, we can define the density of their distribution in space in the neighbourhood of this group: it will be inversely as the volume occupied by them. Now consider their deviations from a mean velocity, say that of the central meteor of the group; we can draw from an origin a vector repre- senting the velocity of each meteor, and the ends of these vectors will mark out a region in the velocity diagram whose shape and volume will represent the: character and range of the deviation. It results from a very general proposition in dynamics that as the central meteor moves along its path the region occupied by the’ group of its neighbours multiplied by the corresponding region in their velocity diagram remains constant. Or we may say that the density at the group asi TRANSACTIONS OF SECTION A. 633 considered, estimated by mere numbers, not by size, varies during its motion pro- portionally to the extent of the region on the velocity diagram which corresponds to it. This is true whether mutual attractions of the meteors are sensibly effective or not; in fact, the generalised form of this proposition, together with a set of similar ones relating to the various partial groups of coordinates and velocity components, forms an equivalent of the fundamental law of Action which is the unigue basis of dynamical theory. ow, suppose that the mutual attractions are insensible, and that W is the potential of the conservative field: then for a single meteor of mass m and velocity v we have the energy $mv*+mW conserved: hence if dv, be the range of velocity at any point in the initial position, and dv, that at the corresponding point in any subsequent position of the group, we have v,dv,=v,6v,, these positions remaining unvaried and the variation being due to different meteors passing through them. But if do, and do, are the initial and final conical angles of divergence of the velocity vectors, corresponding regions in the velocity diagram are of extents 6u,.v,"d0; and dv,.v,*d,: these quantities are, therefore, in all cases proportional to the densities at the group in its two positions. In our present case of mutual attractions insensible, the volume density is thus proportional to vie, because vdv remains constant. Now the number of meteors that cross per unit time per unit area of a plane at right angles to the path of the central meteor is equal to this density multiplied by v: thus here it remains proportional to v*de, as the central meteor moves on. In the corpuscular formulation of geometrical optics this result carries the general law that the concentration in cross-section of a beam of light at different points of its path is proportional to the solid angular divergence of the rays multiplied by the square of the refractive index, which is also directly necessitated by thermodynamic principles; as a special case it limits the possible brightness of images in the well-known way. In the moving stream of particles we have thus a quantity that is conserved in each group—namely, the ratio of the density at a group to the extent of the region or domain on the velocity diagram which corresponds to it; but this ratio may vary in any way from group to group along the stream, while there is no restric- tion on the velocities of the various groups. If two streams cross or interpenetrate each other, or interfere in other ways, all this will be upset owing to the collisions. Can we assign a statistical law of distribution of velocities that will remain permanent when streams, which can be thus arranged into nearly homogeneous groups, are crossing each other in all directions, so that we pass to a model of a gasP Maxwell showed that ifthe number of particles each of which has a total energy E is proportional to e~»", where h is some constant (which defines the temperature), while the particles in each group range uniformly, except as regards this factor, with respect to distribution in position and velocity jointly, as above, then this will be the case. In .act, the chance of an encounter for particles of energies Hi and KH’ will involve the product e—»¥e—b®’ or e—h+©), and an encounter does not alter this total energy E+E’; while the domains or extents of range of two colliding groups each nearly homogeneous and estimated, as above, by devia- tion from a central particle in position and velocity jointly, will have the same product after the encounter as before by virtue of the Action principle. It follows that the statistical chances of encounter, which depend on this joint pro- duct, will be the same in the actual motion as are those of reversed encounter in the same motion statistically reversed. But if the motion of a swarm with velocities fortuitously directed can be thus statistically reversed, recovering its revious statistics, its molecular statistics must have become steady ; in fact, we ave insuch a system just the same distribution of encountering groups in one direction as in the reverse direction: thus we have here one steady state. The same argument, indeed, shows that a distribution, such that the number per unit volume of particles whose velocity deviations correspond to a given region in the velocity diagram, is proportional to the extent of that region without this factor e-hF, will also be a steady one. This is the case of equable distribution in each group as regards only the position and velocity diagrams conjointly; but in this 634 REPORT—1900. case each value of the resultant velocity would occur with a frequency propor tional to its square, and a factor such as e~¥ is required to keep down very high values. The generalisations by Boltzmann and Maxwell to internal degrees of freedom would lead us too far, the aim here proposed being merely concrete illustration of the very general but purely analytical argument that is fully set forth in the treatises of Watson, Burbury, and Boltzmann. 2. The Partition of Energy. By G. H. Bryan, Se.D., F.RS. Consider a system of particles in a field of force acting on one another with forces which are functions of the distances between them. If w, v, w are the velocity components of a particle of mass m, V, the potential energy of the system, the rate of increase of the component of kinetic energy, } mu’, is given by d dV (Se) we dt G dx If the probability of any given motion of the system is equal to the probability ot the reversed motion for given positions of the particles, then since equal positive and negative values of w are equally probable it appears that the mean rate of increase of 3 mu” estimated from probability considerations is zero. Now form the second differential coefficient of $ mu? with respect to the time, which may be called the acceleration of this energy component. We obtain igen ee hap ee d d d\ dV ——\nj )=—| — —u> — ho + W— |) — de® nen n(ae) i («5 “dy . ‘) dx If we are given the probability that the coordinates of the system may be between given iimits, then a condition for the stationary state is that the mean values of the accelerations of } mv*, 4 nw, 4 mw* are zero. We thus obtain a system of equations of energy equilibrium for the system, which are sufficient to determine the mean values of the components of kinetic energy, provided the system is such that the mean values of products of velocities such as w,v,, %;¥%o, OY #0, vanish, If this is not the case the conditions for a stationary state involve writing down further expressions for the accelerations or second differential coefficients of these velocity products, and equating their mean values to zero. In this way the mean values of the squares and products of the velocity components for a stationary distribution are expressible in terms of the mean values of the squares of the force compenents, and the second differential coefficients of the potential energy with respect to the coordinates. In this preliminary investigation the simplest possible illustrative examples are considered. For a system of two particles moving in astraight line and acting on one another with finite forces, the partition of energy follows Maxwell's law, and the mean product of the velocities vanishes if there is no external field of force. If there is a field of external force, this is no longer in general the case. We thus have some justification for the belief that in a polyatomic gas Maxwell’s law of partition may no longer hold good, and this may account for the experi- mental result that this law is verified approximately only when translational and rotational energy are alone taken into account. The principal advantage of studying the problem of energy-partition from the consideration of energy accelerations is that it leads to results for a perfectly reversible dynamical system somewhat analogous to the irreversible properties of temperature. ‘The property that heat tends to flow from a hotter to a colder body is represented on this view by the property that when two stationary systems are allowed to act on one another, then if a certain inequality is satisfied energy is accelerated from one system to the other, and the direction of the acceleration is } This paper will be published im ewtenso in the dedicatory volume to Professor Lorentz published by the University of Leiden. TRANSACTIONS OF SECTION A. 6395 determined by the sign of the inequality, This last is unaltered by reversing the - yelocity components of all the particles. In order that a stationary distribution of energy may be possible certain con- ditions represented by inequalities must hold good, and further conditions, which may or may not be identical with these, must be satistied in order that the distri- butions may bestable. hese properties may perhaps have a physical interpretation in the notion that change of state takes place when the conditions in question cease to hold good. Finally, the fact that the Newtonian potential satisfies Laplace’s equation may possibly give an exceptional character to the phenomena of energy-partition in the cosmic universe. It is also evident that expressions for the second differential coefficients of squares and products of velocity components may theoretically be written down for a dynamical system of the most general character, and applied to determine the partition of energy between the molecules and the ether. 3. Note on the Propagation of Electric Waves along Parallel Wires. By Prof. W. B. Morton, I/.A. In the ‘Annalen der Physik’ for June 1900, a very complete investigation of this problem has been published by G. Mie. He finds expressions for the wave- length and damping of the oscillations, involving a series of ascending powers of the ratio of radius of wires to distance apart. The object of this note is to point out that the approximate solution, in which the square of this ratio is neglected, can be very easily obtained {rom the known solution for a-single wire, as worked out by Professor J. J. Thomson and by Sommerfeld. The formula for the damping agrees with that given by Heaviside’s simple theory when Lord Rayleigh’s high- frequency values are used for the resistance and inductance. Attention is called to anerror in the formula for the K, function in the work of Thomson, Sommerfeld, and Mie, arising probably from an erratum in Heine’s ‘Kugelfunctionen.’ It affects the numerical values worked out in Sommerfeld and Mie’s papers. 4. On the Vector Potential of Electric Currents in a Field where Disturb- ances are propagated with Finite Velocity. ByS. H. Bursury, £.£.S. 1. If uw’ v’w’ be the components of the total electric current at 2’y’ 2’ ina homogeneous isotropic transparent medium, the components of vector potential F GH at any point ays at a given instant are usually defined as follows, F = {\\" da'dy/dz = |“ar &c., where 7 = f(x? = 2+ iy’ yy a @— 2)? and the integration is over all space. Also wu’ v’w’ are the values of wu’ v’ w’ at the given instant, and therefore all at the same instant. Hence follow Poisson’s equations Vol aas =a ae Ate y 2 Bath ag . . . . . (tk) ea ba _ai_dG@ dy dz ” iF dH B =" ez = du ‘ . . (2) _aG _ ak ¥ dx dy Then dy a8, d/dk dG di dy dz BOs de dy dz : 636 REPORT—1900. and if we assume dx dy dz and therefore - + = + oA = 0 everywhere, we have er ae 2 yey eS TEI, Hence is deduced K @F 2 ——— = ‘ e . ° . 4 VE 4r dt* @) 1 where V = JES the velocity of propagation of adisturbance. Also 4(Fu+Gu+ Hw) is the energy per unit of volume atays. . : : é : , » (5) 3. The theory in this form is open to objection. If u’, the current at 2” ? changes with the time, we have a corresponding change of F given byt = = But owing to (4) no physical quantity at 2 y z can be immediately affected by the change at 2” y’ 2’. The change can have no effect whatever at « y = till after the expiration of the time “ If therefore F be any physical quantity, we must have - = 0, which is inconsistent with our definition. If F be nota physical quantity, Fu cannot denote energy, which is inconsistent with (5). 4, The fact that V is very great, and 7 very small, does not meet the difficulty, du’ because 7 ©” V dt 5. It is proposed to substitute for uw’, the current at 2’ y’ z’ at the given instant, uw,’ the current which did exist at 2’ y' x’ x seconds ago, so that our definition will is not generally small. be F, = | itar. F, is used by way of distinction from F. In this form of F the objections above taken cease to have effect. As wu’ and all its derived coefficients according to the time are supposed finite, : r du’ r? au! : : we may write w’;=w’— — 3 &e., or symbolically, for convenience = oe ie Vdt ~V? at?’ only, F rd 5 a — a il Tae, F; = Jar’ e Vatu . . = . . . (6) , 6. It is shown that, primd facie, F , G,, H,, so defined, satisfy the differential equations (1) a8 well as do the ordinary FG H. So as regards the differential equations the proposed substitution makes no difference in form to the theory. 7. An objection is considered that F and F, cannot both satisfy Poisson’s equations (1) because if they did we should have y*F = vF,, and this cannot, it is said, be true because 1 du’ r due i r? Bu’ F=F | er | pee | OC ike + eta 2) aan * a3) as & TRANSACTIONS OF SECTION A. 637 and since vr +0 "i vr? #0 Ff If the objection be valid, it is not evident whether we should use F or F,. 8. But Poisson’s equation requires only that, however small be the radius ‘a’ of a sphere described about 2 y z, when r=0, y?F=y?F, is not true. °4nr2y*Edr =—4r |'4nrudr and that is satisfied by both F and F; For the purpose of Poisson's equation we may use y’F and y’F; as interchangeable. 9. Since = has different values for different waves, F', should be the sum of a number of terms of the form (6), each corresponding to a wave-length. 10. Et seg—A calculation is made of the effect of using F; instead of F in case of a disturbance spreading in spherical waves from a source. SATURDAY, SEPTEMBER 8, The following Reports and Papers were read :— 1, Report on Determining the Magnetic Force on Board Ship, See Reports, p. 45, 2. Final Report on the Sizes of Pages of Scientific Pervodicals. See Reports, p. 45. 3. On the Similarity of Effect of Electrical Stimulus on Inorganic and Living Substances. By Jacapis CuunveR Bosz, M.A., D.Sc., Pro- Jessor of Physical Science, Presidency College, Calcutta. If we take a piece of living tissue, say a piece of muscle, and subject it to an electric stimulus, there will be produced a contraction; the stimulus causes a rearrangement of the particles of the living substance by which the form of muscle is changed. On the cessation of stimulus the muscle, recovering from the mole- cular strain, gradually attains its original shape. The effect of stimulus on nerves is, however, not apparent; there is no change of form. The molecular disturbance due to stimulus can, however, be detected in an indirect manner from certain electromotive variations that are produced. If now a mass of metallic filings be taken and subjected to electric shocks, there is no visible change. The substance appears to be irresponsive or dead to stimulus. Are inorganic substances then really irresponsive? Could this apparent want of response not be due atter all to our inability to detect the profound molecular changes that may have nevertheless taken place in the substance under the action of stimulus? In nerves it is seen that the molecular changes can only be detected indirectly by an electric method. The author describes an electric method based on the variation of conductivity, by which the molecular change due to an electric stimulus in an inorganic substance is detected and measured. Curves are in this manner obtained with the conductivity variation (proportional to molecular effect) as ordinates, and the time ; 4 exposure to the stimulus or the time of recovery from the effect of stimulus as abscisse. ‘ It is next shown that the effect on matter of electric stimulus, of widely varying 638 REPORT—1900. frequencies, is a continuous one. There is also a continuity of effect on all forms of inorganic matter, similar effects being produced not only (1) in all elementary substances—metals, non-metals, and metalloids—but also (2) in metallic compounds, such as the chlorides, bromides, iodides, oxides, and sulphides. Comparisons are next made of the molecular response in both inorganic and living substances under varying conditions :— 1. On the effect of moderate stimulus. 2. On the effect of maximum stimulus. 3. On the effect of superposition of medium stimuli—(a) effect due to slow intermittence ; (6) tetanic effect due to rapid intermittence. 4, On the opposite effect due to strong and feeble stimulus. 5. On the physical theory of ‘ fatigue ’ in inorganic and living substances. 6, On the various means of rapidly removing fatigue. 7. On the effect of injection of various substances which act as ‘ poisons.’ In all the above cases the curves for both living and inorganic substances are found to be similar. The author next explains a theory of vision, and describes an artificial retina ; the various effects of radiation on this artificial retina explain many obscure phenomena of vision. Parallel experiments are then described with the artificial and the real retina :— 1. On the effect of short exposure to the action of radiation. 2. On the effect of intermittent radiation; on the question of the presence or absence of ‘flicker’ depending on the intensity of radiation and also on the rapidity of intermittence. 3. On the peculiarity of the visual sensation curve, as explained by the curve of effect on the artificial retina. 4, On the different elements of retinal fatigue. 5. On certain curious reversal effects, G. On after-oscillation and visual recurrence. 7. On the novel phenomenon of binocular alternation of vision, and on the analysis of superposed images by alternate after-vision. 8. On the persistence of retinal oscillation, and its continuity with the phe- nomenon of memory. In ali the phenomena described above there is seen a remarkable similarity of effect of external stimulus on both living and non-living forms of matter. It is difficult to draw a line and say, ‘ Here the physical process ends and the physio- logical process begins,’ or ‘These are the lines of demarcation that separate the physical, the physiological, and the beginning of psychical processes.’ No such arbitrary lines can be drawn, there being no abrupt break of continuity. 4. Wrreless Telephony. By Sir Wittiam Henry Preece, K.C.B., PRS. The first experiments in this direction were made in the month of February 1894, across Loch Ness in the Highlands. On that occasion trials were made to determine the laws governing the transmission of Morse signals by the electro- magnetic method of wireless telegraphy, which has formed the subject of frequent reports to this Section since 1884; two parallel wires well earthed were taken, one on each side of the lake, and arrangements were made by means of which the wires could be systematically shortened with a view of ascertaining the minimum length necessary to record satisfactory signals. It occurred to Mr. Gavey, who was experimenting, to compare telephonic with telegraphic signals, ¢.e., to ascertain whether articulate speech could be maintained under the same conditions as Morse signalling. The trials showed that it was possible to exchange speech across the Loch at an average distance of 1:3 mile between the parallel wires when the eth of the wires themselves was reduced to four miles on each side of the ‘water, a TRANSACTIONS OF SECTION A. 639 What led to this train of thought was the fact that although the volume of telegraphic current was immensely greater than that of a telephonic current, whenever, through want of balance as a loop, disturbance was evident then tele- phonic cross-talk was also manifest. In other words, a weak telephonic current was apparently as powerful a disturber as a strong telegraphic one. The sensation created in 1897 by Mr. Marconi’s application of Hertzian waves, distracted attention from the more practical and older method. Myr. Evershed and Principal Oliver Lodge had, in the meantime, much advanced the system by introducing admirable call systems. In 1899 I conducted some careful experiments on the Menai Straits which determined the fact that the maximum effects with telephones are produced when the parallel wires are terminated by ‘ earth’ plates in the sea itself. It became quite evident that the ordinary inductive effects are much enhanced by conductive effects through the water, and that in consequence shorter wires are practical. No special apparatus seems necessary. The ordinary telephonic transmitters and re- ceivers were used without induction coils. It became desirable to establish communication between the islands or rocks known as the Skerries and the mainland of Anglesey, and it was determined to do this by means of wireless telephony. ‘The lighthouse at the Skerries was wanted to be in communication with the coastguard station at Cemlyn. Am. Jour. (3), 39, p. 46 (1890). 2 Astro-Phys. Jour., vol. X. p. 177. * Monthly Notiees, vol. 1x, p. 2 (1899), + Abney, Photography, TRANSACTIONS OF SECTION A. 665 diameter with an 8-inch refractor of the Liverpool Observatory. In 1852 De la Rue began experimenting in lunar photography. He employed a reflector of some 10 feet focal length and about 18 inches diameter. A very complete account of his methods is given in a paper read before the British Association. Mr. Ruther- furd at a later date having tried an 1]4-inch refractor, and also a 13-inch reflector, finally constructed a photographic refracting telescope, and produced some of the finest pictures of the moon that were ever taken until recent years. Also Henry Draper’s picture of the moon taken September 3, 1863, remained unsurpassed for a quarter of a century. Admirable photographs of the lunar surface have been published in recent years by the Lick Observatory and others. I myself devoted considerable attention to this subject at one time. Photographs surpassing anything before attempted were published in 1896-99 by MM. Loéwy and Puiseux, taken with the Equatorial _ Coudé of the Paris Observatory. Star prints were first secured at Harvard College, under the direction of W. C. Bond, in 1850 ; and his son, G. P. Bond, made in 1857 a most promising start with double-star measurements on sensitive plates, his subject being the well-known pair in the tail of the Great Bear. The competence of the photographic method to meet the stringent requirements of exact astronomy was still more decisively shown in 1866 by Dr. Gould’s determination from his plates of nearly fifty stars in the Pleiades. Their comparison with Bessel’s places for the same objects proved that the lapse of a score of years had made no difference in the configura- *tion of that immemorial cluster; and Professor Jacoby’s recent measures of Rutherfurd’s photographs taken in 1872 and 1874 enforce the same conclusion. The above facts are so forcible that no wonder that at the Astrophotographic Congress held in Paris in 1887 it was decided to make a photographic survey of the heavens, and now eighteen photographic telescopes of 13 inches aperture are in operation in various parts of world, for the purpose of preparing the international astrographic chart, and it was hoped that the catalogue plates would be completed by 1900. 4 Photography has been applied so assiduously to the discovery of minor planets that something like 450 are now known, the most noteworthy, perhaps, aa regards utility being the discovery of Eros (433) in 1898 by Herr Witt at the Observatory Urania, near Berlin. With regard to the application of photography to recording the form of various nebul, it is interesting to quote a passage from Dick’s ‘ Practical Astronomer,’ published in 1845, as opposed to Herschel’s opinion that the photography of a nebula would never be impossible. ‘It might, perhaps, be considered as beyond the bounds of probability to expect that even the distant nebulee might thus be fixed, and a delineation of their objects produced, which shall be capable of being magnified by microscopes. But we ought to consider that the art is only in its infancy, and that plates of a more delicate nature than those hitherto used may yet be prepared, and that other properties of light may yet be discovered, which shall facilitate such designs. For we ought now to set no boundaries to the discoveries of science, and to the practical applications of scientific discovery, which genius and art may accomplish.’ It was not, however, until 1880 that Draper first photographed the Orion Nebula, and later by three years I succeeded in doing the same thing with an exposure of only thirty-seven minutes. In December 1885 the brothers Henry by the aid of photography found that the Pleiades were involved in a nebula, part of which, however, had been seen by myself! with my 3-foot reflector in February 1880, and later, February 1886, it was also partly discerned at Pulkowa with the 30-inch refractor then newly erected. Still more nebulosity was shown by Dr. Roberts’s photographs,” taken with his 20-inch reflector in October and December 1886, when the whole western side of the group was shown to be involved in a vast nebula, whilst a later photograph taken by MM. Henry early in 1888 showed that practically the whole of the group was a shoal of nebulous matter. } Monthly Notices, vol. xl. p. 376. * Monthly Notices, vol, xlyii. p, 24, 666 REPORT—1900. In 1881 Draper and Janssen recorded the comet of that year by photography. Huggins! succeeded in photographing a part of the spectrum of the same object,(Tebbutt’s Comet 1881, II.) on June 24, and the Fraunhofer lines were amongst the photographic impressions, thus demonstrating that at least a part of the continuous spectrum is due to reflected sunlight. He also secured a similar result from Comet Wells.’ I propose to consider the question of the telescope on the following lines: (1) The refractor and reflector from their inception to their present state. (2) The various modifications and improvements that have been made in mounting these instruments, and (8) the instrument that has been lately introduced by a com- bination of the two, refractor and reflector, astriking example of which exists now at the Paris Exhibition. At a meeting of the British Association held nearly half a century ago (1852) (Belfast) Sir David Brewster showed a plate of rock crystal worked in the form of a Jens which had been recently found in Nineveh. Sir David Brewster asserted that this lens had been destined for optical purposes, and that it never was a dress ornament. That the ancients were acquainted with the powers of a magnifying lens may be inferred from the delicacy and minuteness of the incised work on their seals and intaglios, which could only have been done by an eye aided by a lens of some sort. There is,"however, no direct evidence that the ancients were really acquainted with the refracting telescope, though Aristotle speaks of the tubes through which the ancients observed distant objects, and compares their effect to that of a well from the bottom of which the stars may be seen in daylight.* As an historical fact without any equivocations, however, there is no serious doubt that the telescope was invented in Holland. The honour of being the originator has been claimed for three men, each of whom has had his partisans. Their names are Metius, Lippershey, and Janssen. Galileo himself says that it was through hearing that some one in France or Holland had made an instrument which magnified distant objects that he was led to inquire how such a result could be obtained. The first publisher of a result or discovery, supposing such discovery to be honestly his own, ranks as the first inventor, and there is little doubt that Galileo was the first to show the world how to make a telescope.* His first telescope was made whilst on a visit to Venice, and he there exhibited a telescope magnifying three times: this was in May 1609. Later telescopes which emanated from the hands of Galileo magnified successively four, seven, and thirty times. This latter number he never exceeded. Greater magnifying power was not attained until Kepler explained the theory and some of the advantages of a telescope made of two convex lenses in his Catoptrics (1611). The first person to actually apply this to the telescope was Father Scheiner, who describes it in his Rosa Ursina (1630), and Wm. Gascoigne was the first to appreciate practically the chief advantages by his invention of the micrometer and application of telescopic sights to instruments of precision. It was, however, not until about the middle of the seventeenth century that Kepler’s telescope came to be nearly universal, and then chiefly because its field of view exceeded that of the Galilean. The first powerful telescopes were made by Huyghens, and with one of these he discovered Titan (Saturn’s brightest satellite): his telescopes magnified from forty-eight to ninety-two times, were about 24 inches aperture, with focal lengths ranging from 12 to 28 feet. By the aid of these he gave the first explanation of Saturn’s ring, which he published in 1659. Huyghens also states that he made object-glasses of 170 feet and 210 feet focal length; also one 300 feet long, but which magnified only G00 times; he also presented one of 123 feet to the Royal Society of London. 1 Proc. Roy. Soe., vol. xxxii. No. 213. 2 Rep. Brit. Assoc., 1882, p. 442. $ De Gen. Animalium, lib. y, 4 Newcomb’s Astronomy, p. 108. —— TRANSACTIONS OF SECTION A. 667 Auzout states that the best telescopes of Campani at Rome magnified 150 times, and were of 17 feet focal length. He himself is said to have made telescopes of from 300 to 600 feet focus, but it is improbable that they were ever put to practical use. Cassini discovered Saturn’s fifth satellite (Rhea) in 1672, with a telescope made by Campani, magnifying about 150 times, whilst later, in 1684, he added the third and fourth satellites of the same planet to the list of his discoveries. Although these telescopes were unwieldy, Bradley, with his usual persistency, actually determined the diameter of Venus in 1722 with a telescope of 212 feet focal length. With such cumbersome instruments many devices were invented of pointing these atrial telescopes, as they were termed, to various parts of the sky. Huyghens contrived some ingenious arrangements for this purpose, and also for adjusting and centreing the eyepiece, the object-glass and eyepiece being connected by a long braced rod. It was not, however, until Dollond’s invention of the achromatic object-glass in 1757-58 that the refracting telescope was materially improved, and even then the difficulty of obtaining large blocks of glass free from striz limited the telescope as regards aperture, for even at the date of Airy’s report we have seen that 12 inches was about the maximum aperture for an object-glass. The work of improving glass dates back to 1784, when Guinand began experimenting with the manufacture of optical flint glass. He conveyed his secrets to the firm of Fraunhofer and Utzschneider, whom he joined in 1805, and during the period he was there they made the 9°6 inches object-glass for the Dorpat telescope. Merz and Miidler, the successors of Fraunhofer, carried out successfully the methods handed down to them by Guinand and Fraunhofer, Guinand communicated his secrets to his family before his death in 1823, and they entered into partnership with Bontemps. ‘The latter afterwards joined the firm of Chance Bros., of Birmingham, and so some of Guinand’s work came to England. At the present day MM. Feil, of Paris, who are direct descendants of Guinand and Messrs. Chance Bros., of Birmingham, are the best known manu- facturers of large discs of optical glass. It is related in history that Ptolemy Euergetes had caused to be erected on a lighthouse at Alexandria a piece of apparatus for discovering vessels a long way off; it has also been maintained that the instrument cited was a concave reflecting mirror, and it is possible to observe with the naked eye images formed by a concave mirror, and that such images are very bright. Also the Romans were well acquainted with the concentrating power of con- cave mirrors, using them as burning mirrors, as they were called. The first application of an eye lens to the image formed by reflection from a concave mirror appears to have been made by Father Zucchi, an Italian Jesuit. His work was published in 1652, though it appears he employed such an instrument as early as 1616. The priority, however, of describing, if not making, a practical reflecting telescope belongs to Gregory, who, in his ‘Optica Promota,’ 1663, discusses the forms of images of objects produced by mirrors. He was well aware of the failure of all attempts to perfect telescopes by using lenses of various curvature, and proposed the form of reflecting telescope which bears his name. Newton, however, was the first to construct a reflecting telescope, and with it he could see Jupiter's satellites, &c. Encouraged by this he made another of 62 inches focal length, which magnified thirty-eight times, and this he presented to the Royal Society on the day of his election to the Society in 1671. To Newton we owe also the idea of employing pitch, used in the working of the surfaces, A third form of telescope was invented by Cassegrain in 1672. He substituted a small convex mirror for the concave mirror in Gregory’s form, and thus rendered the telescope a little shorter. Short also, from 1730-1768, displayed uncommon ability in the manufacture of 668 REPORT—1900, reflecting telescopes, and succeeded in giving true parabolic and elliptic figures to his specula, besides obtaining a high degree of polish upon them. In Short’s first telescopes the specula were of glass, as suggested by Gregory, but it was not until after Liebig’s discovery of the process of depositing a film of metallic silver upon a glass surface from a salt in solution that glass specula became almost universal, and thus replaced the metallic ones of earlier times. Shortly after the announcement of Liebig’s discovery Steinheil \—and later, independently, Foucault *—proposed to employ glass for the specula of tele- scopes, and, as is well known, this is done in all the large reflectors of to-day. I now propose to deal with the various steps in the development of the telescope, which have resulted in the three forms that I take as examples of the highest development at the present time. These are the Yerkes telescope at Chicago, my own 5-foot reflector, and the telescope recently erected at the Paris Exhibition, dealing not only with the mountings, but with the principles of con- struction of each. When the telescope was first used all could be seen by holding it in the hand. As the magnifying power increased some kind of support would become absolutely necessary, and this would take the form of the altitude and azimuth stand, and the motion of the heavenly bodies would doubtless suggest the parallactic or equatorial movement, by which the telescope followed the object by one movement of an axis placed parallel to the pole. This did not come, however, immediately. The long-focus telescopes of which I have spoken were sometimes used with a tube, but more often the object-glass was mounted in a long cell and suspended from the top of a pole, at the right height to be in a line between the observer and the object to be looked at; and it was so arranged that by means of a cord it could be brought into a fairly correct position. Notwith- standing the extreme awkwardness of this arrangement most excellent observations were made in the seventeenth century by the users of these telescopes. Then the achromatic telescope was invented and mechanical mountings were used, with circles for finding positions, much as we have themnow. Ihave already mentioned the rivalry between the English and German forms of mountings, and Airy’s preference for the English form. The general feeling amongst astronomers has, however, been largely in favour of the German mounting for refractors, due, no doubt, to a great extent, to the enormous advance in engineering skill. We have many examples of this form of mounting. A list of the principal large refracting and reflecting telescopes now existing is given at the end of this Address. All the refractors in this list, with the exception cf the Paris telescope of 50 inches, and the Greenwich telescope of 28 inches, are mounted on the German form. Some of these carry a reflector as well as, for instance, the telescope lately presented to the Greenwich Observatory by Sir Henry Thompson, which, in addition to a 26-inch refractor, carries a 30-inch reflector at the other end of the declination axis, such as had been previously used by Sir William Huggins and Dr. Roberts; the last, and perhaps the finest, example of the German form being the Yerkes telescope at Chicago. The small reflector made by Sir Isaac Newton, probably the first ever made, and now at the Royal Society, is mounted on a ball, gripped by two curved pieces, attaéhed to the body of the telescope, which allows the telescope to be pointed in any direction. We have not much information as to the mounting of early reflectors. Sir William Herschel mounted his 4-foot telescope on a rough but admirably planned open-work mounting, capable of being turned round, and with means to tilt the telescope to any required angle. This form was not very suitable for picking up objects or determining their position, except indirectly; but for the way it was used by Sir William Herschel it was most admirably adapted: the telescope being elevated to the required angle, it was left'in that position, and became practically a transit instrument. All the objects passing through the field of view (which was of considerable extent, as the eyepiece could be moved in declination) were observed, and their places in time and declination noted, so that 1 Gaz. Univ. d Augsburg, March 24, 1856. * Comptes Rend, vol, xliv, February 1857, TRANSACTIONS OF SEOTION A. 669 the positions of all these objects in the zone observed were obtained with a considerable degree of accuracy. It was on this plan that Sir John Herschel made his general catalogue of nebule, embracing all the nebulz he could see in both hemispheres; a complete work by one man that is almost unique in the history of astronomy. Sir William Herschel’s mounting of his 4-foot reflector differs in almost every particular from the mountings of the long-focus telescopes we have just spoken of. The object-glass was at a height, the reflector was cluse to the ground. There was a tube to one telescope, but not to the other. The observer in one case stood on the ground, in the other he was on a stage at a considerable elevation. One pole sufficed with a cord for one; a whole mass of poles, wheels, pulleys, and ropes sur- rounded the other. In one respect only were they alike—they both did fine work. Lassell seems to have been the first to mount a reflector equatorially. He, like Herschel, made a 4-foot telescope, which he mounted in this way. Lord Rosse mounted his telescopes somewhat after the manner of Sir William Herschel. The present Karl has mounted a 3-foot equatorially. A 4-foot telescope was made by Thomas Grubb for Melbourne, and this he -mounted on the German plan. The telescope being a Cassegrain, the observer is practically on the ground level. A somewhat similar instrument exists at the Paris Observatory. Liassell’s 4-foot was mounted in what is called a fork mounting, as is also my own 5-foot reflector, and this in some ways seems well adapted for reflectors of the Newtonian kind. We now come to the Paris telescope. This is really the result of the combina- tion of a reflector and a refractor. JI cannot say when a plane mirror was first used to direct the light into a telescope for astronomical purposes. It seems first to have been suggested by Hooke, who, at a meeting of the Royal Society, when the difficulty of mounting the long-focus lenses of Huyghens was under discussion, pointed out that all difficulties would be done away with if, instead of giving movement to the huge telescope itself, a plane mirror were made to move in front of it.’ The Earl of Crawford, then Lord Lindsay, used a heliostat to direct the rays from the sun, on the occasion of the transit of Venus, through a lens of 40 feet focal length, in order to obtain photographs, and it was also largely used by the American observers on the same occasion. Monsieur Loéwy at Paris proposed in 1871 a most ingenious telescope made by a combination of two plane mirrors and an achromatic object-glass, which he calls a Coudé telescope, which has some most important advantages. Chief amongst these are that the observer sits in perfect comfort at the upper end of the polar axis, whence he need not move, and by suitable arrangements he can direct the telescope to any part of the visible heavens. Several have been made in France, including a large one of 24 inches aperture, erected at the Paris Observatory, and which has already made its mark by the production of perhaps the best photographs of the moon yet obtained. I have already spoken of Lord Lindsay and his 40-foot telescope, fed, as it were, with light from a heliostat. This is exactly the plan that has been followed in the design of the large telescope in the Paris Exhibition. Butin place of a lens of 4 inches aperture and a heliostat a few inches larger, the Paris telescope has a plane mirror of 6 feet and a lens exceeding 4 feet in diameter, with a focal length of 186 feet. The cost of a mounting on the German plan and of a dome to shelter such an instrument would have been enormous. The form chosen is at once the best and cheapest. One of the great disadvantages is that from the nature of things it cannot take in the whole of the heavens. The heliostat form of mounting of the plane mirror causes a rotation of the image in the field of view which in many lines of research is a strong objection. There is much to be said on the other side. The dome is dispensed with ; the tube, the equatorial mounting, and the rising floor are not wanted. The mechanical arrangements of importance are confined to the mounting of the necessary machinery to carry the large plane mirror and move it round at the proper rate. The telescope need not have any tube (that to ! Lockyer, Star-gazing, p. 453. 670 REPORT—1900. the Paris telescope is of course only placed there for effect), as the flimsiest covering is enough if it excludes false light falling on the eye end; and more important than all, the observer sits at his ease in the dark chamber. This question of the observer, and the conditions under which he observes, is a most important one as regards both the quality and quantity of the work done. We have watched the astronomer, first observing from the floor level, then mounted on a high scaffold like Sir William Herschel, Lassell, and Lord Rosse ; then starting again from the floor level and using the early achromatic telescope ; then, as these grew in size, climbing up on observing chairs to suit the various positions of the eye end of the telescope, as we see in Mr, Newall’s great telescope ; then brought to the floor again by that excellent device of Sir Howard Grubb, the rising floor. This is in use with the Lick and the Yerkes telescopes, where the observer is practically always on the floor level, though constant attention is needed, and the circular motion has to be provided for by constant movement, to say nothing of the danger of the floor going wrong. Then we have the ideal condition, as in the Equatorial Coudé at the Paris Observatory, where the observer sits comfortably sheltered and looks down the telescope, and from this position can survey the whole of the visible heavens. The comfort of the observer is a most important matter, especially for the long exposures that are given to photo- graphic plates, as well as for continued visual work. In such a form of telescope as that at Paris the heliostat form of mounting the plane mirror is most suitable, notwithstanding the rotation of the image. But there is another way in which a plane mirror can be mounted, namely, on the plan first proposed by Auguste many years ago, and lately brought forward again by Mons. Lippmann, of Paris, and that is by siwply mountirg the plane mirror on a polar axis and parallel therewith, and causing this mirror to rotate at half the speed of the earth’s rotation. Any part of the heavens seen by any person reflected from this mirror will appear to be fixed in space, and not partake of the apparent movement of the earth, so long as the mirror is kept moving at this rate. A telescope, therefore, directed to such a mirror can observe any heavenly body as if it were in an absolutely fixed position so long as the angle of the mirror shall not be such as to make the reflected beam less than will fill the object-glass. There is one disadvantage in the ccelostat, as this instrument is called, and that is its suitability only for regions near the equator. The range above and below, however, is large enough to include the greater portion of the heavens, and that portion in which the solar system is included. Here the telescope must be moved in azimuth for different portions of the sky, as is fully explained by Professor Turner in vol.1vi. of the ‘Monthly Notices,’ and it therefore becomes necessary to provide for moving the telescope in azimuth from time to time as different zones above or below the equator are observed. No instrument yet devised is suitable for all kinds of work, but this form, not- withstanding its defects, has so many and such important advantages that I think it will obviate the necessity of building any larger refractors on the usual models, The cost of producing a telescope much Jarger than the Yerkes on that model, in comparison with what could be done on the plan I now advocate, renders it most improbable that further money will be spent in that way. It may be asked, What are the lines of research which could be taken up by a telescope of , this construction, and on what lines should the telescope be built ? I willendeavour to answer this. All the work that is usually done by an astronomical telescope, excepting very long-continued observations, can be equally well done by the fixed telescope. But there are some special lines for which this form of research is admirably suited, such as photographs of the moon, which would be possible with a reflecting mirror of, say, 200 feet focal length, giving an image of some 2 feet diameter in a primary focus, or a larger image might be obtained either by a longer- focus mirror or by a combination, It might even be worth while to build a special ecelostat for lunar photography, provided with an adjustment to the polar axis and a method of regulating the rate of clock to correct the irregular motion of the moon, and thus obtain absolutely fixed images on the photographic late. 3 The advantage of large primary images in photography is row fully recog- TRANSACTIONS OF SECTION A. 671 nised. For all other kinds of astronomical photography a fixed telescope is admirably adapted; and so with all spectroscopic investigations, a little con- sideration will show that the conditions under which these investigations can be pursued are almost ideal. As to the actual form such a construction would take, we can easily imagine it. ‘The large mirror mounted as a ccelostat in the centre; circular tracts round this centre, on which a fan-shaped house can be travelled round to any azimuth, containing all the necessary apparatus for utilising the light from the large plane mirror, so as to be easily moved round to the required position in azimuth for observation. In place of a fan-shaped house movable round the plane mirror, a permanent house might encircle the greater portion round the mirror, and in this house the telescope or whatever optical combination is used might be arranged on an open framework, supported on similar rails, so as to run round to any azimuth required. The simplicity of the arrangement and the enormous saying in cost would allow in any well-equipped observatory the use of a special instrument for special work. The French telescope has a mirror about 6 feet in diameter and a lens of about 4 feet. This is a great step in advance over the Yerkes telescope, and it may be some time before the glass for a lens greater than 50 inches diameter will be made, as the difficulty in making optical glass is undoubtedly very great. But with the plane mirror there will bo no such difficulty, as 6 feet has already been made; and so with a concave mirror there would be little difficulty in beginning with 6 feet or 7 feet. The way in which the mirror would be used, always hanging in a band, is the most favour- able condition for good work, and the absence of motion during an observation, except of course that of the plane mirror (which could be given by floating the polar axis and suitable mechanical arrangements, a motion of almost perfect regularity). One extremely important thing in using silver or glass mirrors is the matter of resilvering from time to time. Up to quite recently the silvering of my 5-foot mirror was a long, uncertain, and expensive process. Now we have a method of silvering mirrors that is certain, quick, and cheap. This takes away the cne great disability from the silver or glass reflecting telescope, as the surface of silver can now be renewed with greater ease and in less time than the lenses of a large refracting telescope could be taken out and cleaned. It may be that we shall revert to speculum metal for our mirrors, or use some other deposited metal on glass; but even as it is we have the silvered glass reflectcr, which at once allows an enormous advance in power. ‘To do justice to any large telescope it should be erected in a position, as regards climate, where the conditions are as favyour- able as possible. The invention of the telescope is to me the most beautiful ever made. Famili- arity both in making and in using has only increased my admiration. With the exception of the microphone of the late Professor Hughes, which enabled one to hear otherwise inaudible sounds, sight is the only sense that we have been able to enormously increase in range. The telescope enables one to see distant objects as if they were at, say, one five-thousandth part of their distance, whilst the microscope renders visible objects so small as to be almost incredible. In order to appreciate better what optical aid does for the sense of sight, we can imagine the size of an eye, and therefore of a man, capable of seeing in a natural way what the ordinary eye sees by the aid of a large telescope, and, on the other hand, the size of a man and his eye that could see plainly small objects as we see them under a powerfui micro- scope. The man in the first case would be several miles in height, and in the latter he would not exceed a very small fraction of an inch in height. Photography also comes in as a further aid to the telescope, as it may possibly be to the microscope. For a certain amount of light is necessary to produce sen- sation in the eye. If this light is insufficient nothing is seen; but owing to the accumulative effect of light on the photographic plate, photographs can be taken of objects otherwise invisible, as I pointed out years ago, for in photographs I took in 1883 stars were shown on photographic plates that I could not see in the telescope. All photographs, when closely examined, are made up of a certain number of little dots, as it were, in the nature of stippling, and it is a very inter- 672 REPORT—1900, esting point to consider the relation of the size and separation of these dots that form the image, and the rods and cones of the reckoner which determines the power of the eye. Many years ago I tried to determine this question. I first took a photograph of the moon with a telescope of very short focus (as near as I could get it to the focus of the eye itself, which is about half an inch), The resulting photograph measured one two-hundredth of an inch in diameter, and when examined again with a microscope showed a fair amount of detail, in fact, very much as we see the moon with the naked eye; making a picture of the moon by hand on such a scale that each separate dot of which it was made corresponded with each separate sensitive point of the retina employed when viewing the moon without optical aid, I found, on looking at this picture at the proper distance, that it looked exactly like a real moon. In this case the distance of the dots was constant, mak- ing them larger or smaller forming the light or shade of the picture. I did not complete these experiments, but as far as I went I thought that there was good reason to believe that we could in this way increase the defining power of the eye. It is a subject well worthy of further consideration. I know that in this imperfect and necessarily brief address I have been obliged to omit the names of many workers, but I cannot conclude without alluding to the part that this Association has played in fostering and aiding Astronomy. A glance through the list of money grants shows that the help has been most liberal. In my youth I recollect the great value that was put on the British Association Catalogue of Stars; we know the help that was given in its early days to the Kew Observa- tory ; and the Reports of the Association show the great interest that has always been taken in our work, The formation of a separate Department of Astrenomy is, I hope, a pledge that this interest will be continued, to the advantage of our science. List of Large Telescopes in existence in 1900. Refractors 15 inches and upwards Refractors 15 inches and upwards Inches | Inches Paris (Exhibition) . . | 50 Princeton . e ° - | 23:0 Yerkes . : 5 - = 40 Mount Etna. : - «gees Wick, = 6. i x é eo eeoO Strassburg . = é A 191 Pulkowa A - : At) e380 || Milan . F ; ; = i een OP Nice — . 5 ; : - 29:9 || (Dearborn) Chicago. caleelssh Paris’ < P ; ; : 28:9 || Warner Obs., Rochester, U.S. | 160 Greenwich . : . .| 280 || Washburn Observatory, Vienna. : ; Pal ora O2 uml Madison, Wisconsin . 15°5 Washington . : i .| 26:0 || Edinburgh . : Fi » | iba Leander, McCormick Obser- | | Brussels -. : : > | amloel vatory, Virginia ; .| 26:0 || Madrid . : ; : Pe lH) Greenwich . - : .| 26:0 || Rio Janeiro . : : «jee 0 Newall’s, Cambridge . =) 25:0 Paris. . : - | cleO Cape of Good Hope. ; 24:0 Sir William Huggins . : 15-0 Harvard , : : oi 2240) 3 dienbarist ger. : : : . | 15:0 Reflectors 2 feet 6 inches and upwards | Reflectors 2 feet 6 inches and upwards Ft. In. | Hae Uns Lord Rosse . ‘ A vu 6. “0 South Kensington a a, 0 Dr. Common : : ml > OMe @rossleyaChick): - Rimes). 1) Melbourne . : : fipoce Greenwich . - A > | Zee Paris 6 m 4 0 South Kensington - |) 2G Meudon 3.3 TRANSACTIONS OF SECTION A. ~- 675 The following Papers were read :— 1. On the Application of the Electric Telegraph to the Furtherance of ‘Eclipse Research. By Professor Davip P. Topp, Director of the Observatory of Amherst College, U.S.A. In 1878 the idea first occurred to the writer! of telegraphing eastward in advance of the lunar shadow in order to enable the immediate verification of any possible discovery as of an intramercurian planet without waiting for another eclipse to take place. A scheme of application to the eclipse of 1887 was published,” but the feasibility of the method was not demonstrated till the eclipse of January 1889, when the California observations were, by the courtesy of the Western Union Telegraph Company, reported in New York with such celerity as to outstrip completely the motion of the moon’s shadow across the earth. A like experiment, only in more practical form, was carried out during the recent eclipse by co-operation with Mr. A. If. Douglass, of the Lowell Observatory, whose station was in Washington, Georgia. Totality there preceded the same phenomenon in Tripoli, the writer's station, by 2 hours 45 minutes. Immediately totality was over, Mr. Douglass reported in full the success of his observations and the instra- ments with which they were made, his despatch being forwarded at once to Washington and New York, and over the Western Union Company’s cables to Penzance. By the courtesy of J. Denison Pender, Esq., Vice-President and Managing Director of the Hastern Telegraph Company, London, the message was forwarded over this company’s cables from Penzance to Gibraltar, thence to Malta, and finally to Tripoli, where a special messenger delivered it at once to the writer at the British Consulate. This message was received and read in less than half an hour of absolute time from its leaving Georgia, and more than two hours before totality actually came on at Tripoli. Had the message announced any discovery, there was abundant time to have prepared for its special veritication. The thanks of astronomers are especially due to the managers of these two great telegraph systems for their generous gift of this service, which has now proved conclusively the practicability of communication between remote eclipse stations while the moon’s shadow is still upon the earth. It is easy to see how such communication, during the total eclipse of 188%, might have afforded data for the orbit of the comet discovered during that eclipse, and whose path is now unknown. Similarly, also, application of the land and cable lines of the globe may be of the greatest service in notifying the occurrence of future meteoric showers, 2. On the Operation of Eclipse Instruments Automatically. By Professor Davin P. Topp, Director of the Observatory of Amherst College, U.S.A. The successful application of automatic machinery to a wide variety of uses and purposes, removing the uncertainty of manual operations, indicates clearly the desirability of its application to the photography of solar eclipses. Three distinct systems of controlling the mechanical movements of such instruments are feasible, the capabilities of all of which I have tested within recent years: (a) The pneumatic system devised and built for the U.S. Eclipse Ex%dition o West Africa, 1889.4 The power requisite for the individual movements of shutters and plate- holders was obtained by small collapsible pneumatic ‘ pockets,’ connected with a } Washington Astronomical OUsertatians for 1876, Appendix iii, p. 354. 2 American Journal of Sciénce, vol. exxxiii. p. 226. ' * Total Eclipses of the Sun, by Mrs. Todd (Sampson Low, Marston, & Co., 1900) pp. 164-173, 4 Monthly Notices B.A‘S., vol. 1. p. 380. : 1900, xx 674 REPORT—1900. large exhaust bellows by lead tubes of small calibre. The operation of the pockets was controlled through a pneumatic commutator, the control sheet being of paper, and having perforations at such points as corresponded to the mechanism or instrument desired. This sheet unwound from the barrel of an ordinary chrono- graph, which thereby not only regulated the exposures, but recorded their exact times. Twenty-two photographic instruments were controlled by this scheme of operation at Cape Ledo, West Africa, on December 22, 1889. (b) The electric system devised and built for the Amherst Hclipse Expedition to Japan, 1896, through the liberality of Messrs. Willis and Arthur James, of New York, who sent the expedition out in their yacht Coronet... The power requisite for the automatic movements was here derived for the most part from spiral springs, the recoil of which was governed by specially devised escapements operated by ordinary electro-magnets. The control currents were sent through a commutator ? which was originally a chronograph, the cylinder being replaced by a copper barrel, in which pins were inserted at suitable points for making contacts with the teeth of a copper comb. Thus, as in the pneumatic system, the commu- tator regulated the exposures and recorded their times as well. ‘Twenty photo- graphic instruments were controlled by this scheme of operation at Esashi, Japan, on August 9, 1896. (c) The mechanical system, devised and built for the expedition to Tripoli, 1900, and at the charges of Mr. Percival Lowell, of Boston. By the courtesy of the Hon. T. S. Jago, H.B.M.’s Consul-General at Tripoli, the station was established on the terrace or roof of the British Consulate. This location afforded, among other advantages, an exceptional chance of utilising gravity as a motive power for the mechanical operation of shutters and plate-holders by means of cords wound upon pulleys which turned the axles, the cords being pulled by small weights which descended within the interior court of the Consulate. This system not haying been invented until after my arrival in Tripoli, its construction was neces- sarily crude and provisional. In addition to the help of native artisans I had the very efficient assistance of Messrs. W. H. Venables and W. F. Riley, of the English colony in Tripoli. The commutator was again a barrel, improvised from a large oil-drum, and turned by a cord and heavy weight, its speed being regulated to the requisite accuracy by a fan governor. By the courtesy of Mr. James A. Doughan this was built in the machine shops of Messrs. Perry, Bury, & Company. From the commutator barrel there unwound also seven cords which passed over pulleys to the various mechanical movements of the shutters and plate-barrels, held in position by escapements similar to those used in Japan for the previous eclipse; and upon these cords were fastened large beads at intervals suited to the exposures required. Each bead in passing the escapement tripped it, thus allowing gravity to advance the movement by a single stage or unit. Seven instruments were operated on this system during the recent eclipse at Tripoli, and about one hundred photographs secured. Experience with these three systems leads me to the conclusion that with slight modifications the last is simplest and best for the automatic operation of a very few instruments. But a combination of the first and second is best for a large number of instruments, the mechanisms being no more likely to get out of order than the similar movements in the pneumatic and electric action of a modern church organ, and no more likely to tail of the right exposure on the right plate at the right time than such an organ is likely to sound a false or unintended note. 3. On the Adaptation of the Principle of the Wedge Photometer to the. Biograph Camera im photographing Total Eclipses. By Professor Davip P. Topp, I.4., Ph.D., Director of the Observatory of Amherst College, U.S.A. ‘Vhis paper describes an instrument devised for photographing the reeent eclipse both the slender partial phases and the corona on a single film, with correctly The Astrophysical Journal, vol. v., p..318. : 2 Stars and Telescopes, by Professor David P, Todd (Sampson Lows Marston, & Co., 1900), p. 363. : ; _— oe eS ee TRANSACTIONS OF SECTION A. 675 graduated exposures foreach, Just in front of the film is mounted a positive wedge of yellow optical glass, backed with an equivalent negative wedge of plain optical glass, the whole having a sliding motion lengthwise. The necessary thickness and length of the wedges are first. found by experiment on the sun, entirely obscured artificially by an occulting disc, excepting only the extreme limb. ‘Through a tuby aperture in the camera the observer watches the gradually diminishing eclipse crescent on the film, and racks the wedge along, keeping the intensity of the image as nearly as possible constant. The biograph films of the recent eclipse, taken by Mr. J. N. Maskelyne, F.R.A.S., indicate the necessity of this great reduction of the strong light of the crescents, to avoid solarisation ; and show further the ease with which the inner coronal ring can be photographed, long before and after totality, —= 4, On the ‘ Square-shouldered’ Aspect of Saturn. By H. M. Anronianpt, 7. R.A.S. The author accounts for the abnormal figure assumed by Saturn, under a slight opening of the ring system, by the existence of the planet’s dark polar cans, checking irradiation along the minor axis of the disc, 5. On the Types of Sun-spot Disturbances. By Rev. A. L. Cortiz, 7. R:A.S. As an aid to researches connected with sun-spots an attempt has been made to classify them according to some prevailing typical forms. Tor this purpose the Stonyhurst drawings of the solar surface for the last twenty years have been caretully examined. From these it would follow that spots appear as scattered groups of small spots, as trains of spots, as composite groups consisting of three or more larger spots, as single spots of round and regular outline which may or may not be accompanied by smaller companions, and as single spots of irregular outline at times accompanied by a train of small companions, or with outliers not arranged in the form of a train. The chief type, however, of which the above- mentioned are in most, probably in all, cases but phases, is the double-spot formation, w:th a train of smaller spots between the two principal spots of the group. In this form the principal spot, which eventually becomes a round spot of regular outline, is generally the leading spot; but in some cases it is the following spot, while in other yet rarer cases both the chief spots develop as regular spots, The mode of development of this leading typé is described in detail. The following are suggested as the types which will be probably found to cover every case that may arise. Type J. A group of a few scattered small spots. Type II. The two-spot formation. Type II. a. In which the leader is the principal spot. Type Il. b. In which the following spot is the principal spot. Type II.c. In which both spots are more or less equal, Type III. A train of spots. Type III.a. With well-defined principal spots, Type IiI.b, Without well-defined principal spots, but mostly penumbral patches th scattered irregular umbre. Type LV. Single spots. Type IV.a. A single spot of round and regular outline. _ Type lV.b. A single spot of round and regular outline, with small com- *panions. : Type 1V.c. A single spot of irregular outline. - Type IV.d. A single spot of irregular outline with a train of small com- panions, Sie 2 676 REPORT—1900. Type IV. e. A single spot of irregular outline with smal! companions not in a train. Type V. An irregular group of larger spots. As an example, the process of formation and life-history of a composite disturbance which crossed the solar disc five times during the period May 14- September 4, 1887, could be succinctly described as follows: I. IL. b, | Vd. LV.a. | 1V.a, Ved. 1V.a.| 1V.e. 1 Taso, 6. On a Cheap Form of Micrometer for determining Star Positions on Photographic Plates. By H. H. Turner, I.A., F.RS., Savilian Professor. j ; The experience of those who have been working at the Astrographie Chart shows that for measuring star photographs a réseaw is practically indispensable. The réseaux made by M. Gautier of Paris may be treated as sensibly correct for nearly all purposes. The cost is between 2/. and 5/., according to the number of lines ruled ; and this initial expense is in any case necessary. But since a photo- graphic copy is often as gocd as the original, this expense might be shared between two or three workers, or borne by some society, which could distribute copies for a few shillings each to its members. Given the réseau, the rest of the micrometer can be made at a very small expense (say 30s. at most) with wood, glass, and paper. Ofcourse, some conveni- ence is sacrificed and a little accuracy lost. The micrometers in use at the Cape of Good Hope cost 180/. apiece ; the duplex micrometer used at Greenwich about 100/.; even the simple form used at Oxford costs 30/. It is not to be supposed that nothing is gained by such expenditure. But with a very simple form of instrument such as that exhibited, which a man could make for himself or with a little assistance from any carpenter, excellent worl can be done. The chief part of the instrument is the microscope with scale in the eyepiece. Most people have some old microscope which would do quite well, and in any case a cheap one is all that is necessary. The scale in the eyepiece can be made photographically, drawing the scale on a large sheet of cardboard and taking a miniature photograph of it. The plate-holder is merely a sheet of glass on which the plate can be easily moved backwards and forwards. The screws required for slow motion and clamping may be ordinary electrical binding-serews or something similar; the counterpoises bags of shot; the reflector a penny mirror, and so on. To measure photographs which have no réseau already impressed upon them, a photographic copy of a réseau may be bound up in contact with the plate in the manner of a lantern slide. Attention may, however, be directed to a method. of impressing the réseaw on such plates which have been alréady developed and tixed,? due to M. Bourget, of the Toulouse Observatory. SEE TUESDAY, SEPTEMBER 11, The following Papers were read :— 1. Comparison of Prominence and Corona Photographs taken at Santa Pola, Spain, and Wadesboro, in North Carolina, during the Total Solar Eclipse of May 28,1900. By Witu1am J. 8. Lockyer, U.A., Ph.D. This paper consists of .a comparison of photographs taken at eclipse stations, 5,900 miles distant from each other, namely, Santa Pola and Watlesboro. ' Given in the Obsertatdry, May 1900, p. 223; and in the Billetm Astrénomigue, March 1900. ae aa TRANSACTIONS OF SECTION A. 677 It was found that during the two and a half hours’ difference of time between the times of totality the main prominences had changed considerably in shape and form, but the polar rifts at the north polar region did not undergo any alteration. The comparison has further led the author to advocate the employment of long-focus cameras for such eclipse work, and to eliminate the necessity of enlargement afterwards. An explanation is also given to account for the extreme sharpness of the lunar limb on one of the long-exposure photographs, the chief argument employed being the very rapid diminution of intensity of the corona as the outer layers are reached. 2. Description of the New Photographic Equatorial of the Cambridge Observatory. By A. R. Hinks, J/A. 3. Diagram for Planning Observations of Lros at the Opposition of 1900-1. Ly A. R. Hinks, IA. 4. On some Points in connection with the Photography of a Moving Object. By W. E. Prummer. I have recently had occasion to make some investigations in connection with the theory of Comet 1899, I. The object of the present paper is not td call attention to the form of the orbit, so that that point need not be considered. But in the course of the examination of the observations I was led to com- pare a series of places.of the comet obtained under the superintendence of the Astronomer Royal, by means of photography with the Thompson Equatorial. There is, so far as I know, no series of equal length in which the places of a moving object have been determined by photography, and it seemed desirable to investigate the peculiarities with some care. The series extends from May 25 to June 16, 1899, during which time the comet passed over some 80° of R.A. and 30° of declination. It is not usual to compare the final elements with individual observations, but only with the normal places. The photographed places have therefore been com- pared with the preliminary orbit, in this case an hyperbola ; and the small deviations, which are removed by the solution of the Equations of Condition, are displayed in the comparison. But for the purposes of the present investigation it is sufficient to remove these discrepancies by any convenient interpolation formula, and so obtain the deviations of the observations from the true path of the comet. When this is effected the following deviations are noticeable :— da cos 6 ds da cos 6 ds 1899 ” ’” 1899 ” uw May25 .. — 42 —O7 June 9 5 ,. —J3:9 —4°6 » 26 — 60 ~0-9 PRE ee EE —76 » 29 + 18 ~1-0 | we 10% ¢ + 34 —51 30°" = £7 —1°6 ieee —9-4 eS as 1-9 0:0 | +2. [oes +111 +92 June 2 + 14 —0°6 | jo GE BG 73 208 ae + 3-1 ~1-9 Ge! Bite -h) 36 +38 phil — 36 +155 The probable error of a single observation, derived simply from the disagreement from the mean, is, in the case of a, + 4/16, and in 6, + 2/85. There seems no prima facie reason why the right ascension coordinate should not be determined with the same accuracy as the declination if the epoch of observation is successfully established. 678 REPORT—1900. The declinations in the early part of the series are eminently satisfactory; in that part the motion was very small in 6. Towards the end, when the comet was moving quicker, the agreement is not so satisfactory. The right ascension varied most rapidly at the beginning of the series, and the agreement would have been more satisfactory throughout, though more noticeable at the beginning, if the epoch of observation had been some seconds later. It is a very difficult matter to determine the proper time of exposure, since the first few seconds in the photograph of a faint object do not seem to be used in the blackening of the film. The importance of this point in the photographs of Eros recommended by the International Comité de la Carte du Ciel will not escape the attention of astronomers, There is another point: how do these observations compare with those made micrometrically in a typical observatory? ‘To illustrate this I select that of Strassburg, where the observations are of unusual excellence, and where the focal length of the instrument is fairly comparable with that of the Greenwich tele- scope. ‘The series of Strassburg within the same dates, and over which the same interpolation formula is available, is not quite so long, but fairly comparable. The Greenwich places rest in every case, it is believed, on the positions of three stars, the Strassburg never on more than two, and sometimes on a single comparison. The error in the star’s place is therefore more effective. The errors are as follows :— da cos 6 ds ) da cos 5 as 1899 ” w” 1899 ” ” May 27 . . +59 —0°5 | June Sys. il4 —72 ROT ins eABiS +1:0 | E fihon Het. > heb +29 June 1’. . —2:4 —O1 | ant UE, eae i) +0°6 po ete) eemore) +09 Ra OU he gue eent LB +10 time’ web's +0°8 | The probable error of a single observation here amounts to + 2/68 and 41/91 which is tess than that of the Greenwich observation in approximately the pro- portion of 3 to 2. Pending further experiments, which I believe are to be carried out by photo- graphic experts at the Paris Obseryatory, the importance of this comparison in the matter of the Eros observations will not be left out of sicht. 5. On Needle-hole Maps for Meteor Observation. By J. C. W. Herscukgt. 1, For an original map the stars are plotted out on squared millimetre paper to the scale of 1 dm=45° by Professor Turner’s formula,' primarily devised for the p-ates of the Astrographic Chart. As a check there is used € cot (a—A)=sin P-7 cos P.* 2. The paper for the copies is sky-blue on one side and white on the other, on which the meteors’ paths and descriptions are written. The needles used are the ordinary commercial needles Nos. 2-12 for magnitudes 1:5 to 4:0 by steps of quarter magnitudes, No. 12 is also used for all stars below 4-0, and an extra large needle for superior stars. The points are ground flat and the needles set in handles, The holes made are round and clean. ' Monthly Notices, R.A.S8., 1894, vol. liv., November. ? For a~A=90°, when the formula is indeterminate, ¢= "7. cos P = TRANSACTIONS OF SECTION A, 679 Representing light as area, these stars approximate very happily to steps of quarter magnitudes. Half-a-dozen sheets are laid, blue side down, on a sheet of lead, the original map laid over them, and the stars punched through with the proper-sized needles. 3. At night a copy is laid on a writing-desk with a sloping ground glass tor, and illuminated with a night light, which also keeps them dry. The meteor track (when observed) is marked in pencil along a celluloid ruler with a blackened bevel-edge, which, being transparent, does not hide the configuration of the stars on the map. 4. Observing. After comparing my watch with Greenwich time, I sit back in a hammock chair with the illuminated map beside me, a pencil and ruler handy. I find I can hold my eye far more steadily on the meteor’s place than a wand held in the hand, which I therefore do not use. I cannot usefully extend my field beyond 45° on either side of the point facing me, except for bright meteors. I let my eyes continually rove about, and when a meteor appears I fasten on it at once, and all the stars fade out ; but only for an instant during which I am free to observe the magnitude, colour, speed, and streak. Presently the nearest stars begin to glimmer out again and set themselves as a framework round the place of the meteor. But I do not look away at them till I have thoroughly impressed a mental picture of the meteor as part of the scene before me. Whilst doing so I estimate its duration. But the most important thing is the direction. I follow its line cautiously backwards and forwards, prolonging it until I find suitable reference stars: either, that the line lies over a star—or passes a degree or two from it—or cuts the distance between two stars in a certain proportion. Thus I get two reference points some ten or twenty degrees apart. Next I define to myself the ength of path as starting and ending on the line joining two stars, or so many degrees before or after that line. Returning to the estimation of duration, I use Professor Herschel’s excellent method of repeating the alphabet over at the rate of five letters to the second, leaving out W—the only letter not monosyllabic. Now I look at my watch and note the trme of appearance. As to the advisability of using maps at all, if the observer knows the stars by heart in configuration and by name, he may very well dispense with maps, &c., describing the meteor and defining its position in words in a notebook in the dark, while still looking at the star lest he miss another meteor. But not many have such knowledge: and the conciseness of the record —a single line on the map— recommends itself compared with a description needing many words. To look away from the sky, down on the map, is a relief to the eye—at the cost, it is true, of possibly losing a meteor, though it must be difficult to go on writing down the description of one meteor while studying another. Looking down therefore on the map, I set the transparent ruler to the best of my judgment, guiding myself by the reference points I have decided upon, and run a pencil along for the length of path, finishing with a half arrow-head to show the direction, and write the time alongside, and the description at the edge of the map; taking the line back also lightly towards the radiant. It is astonishing how slight a shift satisfies or dissatisfies one, but it is worse than useless to look up again at the sky. Next day the end points of the paths are read off for tabulation through a ‘spider web’ of R.A. and Decl. lines on tracing cloth laid over the map. 6. Stationary Meteor Radiants. 2y G. C. Bompas, .£.A.8. 7. Cosmic Evolution. By Prof. A. W. Bickerton, 680 REPORT—1900, 8, Duration of Totality of the Solar Eclipse of May 28, 1900, By C. T. WuITMELL. The Paper included the following table :— Duration Excess No. | Locality | Longitude Latitude | see Observers | Predicted | Observed | Observed OY | o | 8 3 8 1 Ovar 8 38 W.| 40 50N.| 92:7 84:5 8:2 Christie 2 Plasencia.) 6605) 40513; 88-0 82-0 6-0 Downing 3 Coria 6 30 ,, | 89 54 ,, 80-0 4 Naval- 5 34.,, |-39 52 ,, 87:0 80:0 70 Whitmell moral 5 | Navaher- | (4 29 ,,)|(89 40 ,,) 80:0 mosa (near) 6 |Santa Pola} 030 ,, | 3813 ,, 79:0 7 | Alicante | (0 25 ,,)|(38 20 ,,)| | 68:0 | 8 | Algiers 3 2H. | 36 48 ,, 670+ | 64:0 3:0 | Turner Obsy. | | 9 | Algiers, | (3 4 ,.)/(8647,,)| 673-— | 62:5 4:3. Cromme- Hotel | lin 10 | Cape BOLD 4 oOi48) Fe ay eT eO Matifou 11 | Mene:- BOO! ay | OO 4S 4, 71:0 ville 9. Duration of Annularity in a Solar Eclipse. By C. T. Wuitmety, W.A., B.Sc. 10. On the Connection between Latitude-variation and Terrestrial Magnetism. Dy J. Hat, The following propositions were advanced :— I. The changes in the motion of the pole of rotation of the earth round the pole of figure are in intimate connection with the variations of the earth-magnetic torces. II. Inasmuch as the latter phenomena are in a close relation with the state of solar activity, the motion of the pole is also indirectly dependent on the dynamical changes taking place at the sun’s surface. III. The distance between the instantaneous and mean poles decreases with increasing intensity of earth-magnetic disturbance. IV. The length of the period of latitude variation increases with increasing intensity of earth-magnetic disturbance. V. In strict analogy with the phenomena of aurore and of magnetic disturb- ance, the influence of the eleven years’ period of sun-spots, as well as of the ‘great’ period, is clearly exhibited in the phenomenon of latitude-variation ; and the same deviations from the solar curve as are manifested by the aurore are also evident in the motion of the pole. VI. The half-yearly period of the earth-magnetic phenomena influences the motion of the pole of rotation in such a way that its path, instead of being circular, assumes the form of an ellipse, having the mean pole at its centre. VI. The half-yearly period also explains the conspicuous fact of a rotation of the axes of the ellipse in a direction opposite to that of the motion of the pole. TRANSACTIONS OF SECTION B. 681 Section B.—CHEMISTRY. PRESIDENT OF THE SEcTION.—Professor W. H. Prrnin, Jun., Ph.D., F.R.S. THURSDAY, SEPTEMBER 6. The President delivered the following Address :— The Modern System of Teaching Practicai Inorganic Chemistry and its Development. In choosing for the subject of my Address to-day the development of the teaching of practical inorganic chemistry I do so, not only on account of the great import- ance of the subject, but also because it does not appear that this matter has been brought before this Section, in the President's Address at all events, during the last few years. ’ In dealing generally with the subject of the teaching of chemistry as a branch of science it may be well in the first place to consider the value of such teaching as a means of general education, and to turn our attention for a few minutes to the development of the teaching of science in schools. There can be no doubt that there has been great progress in the teaching of science in schools during the last. forty years, and this is very evident from the perusal of the essay, entitled ‘Education: Intellectual, Moral, and Physical,’ which Herbert Spencer wrote in 1859. After giving his reasons for considering the study of science of primary importance in education, Herbert Spencer con- tinues: ‘While what we call civilisation could never have arisen had it not been for science, science forms scarcely an appreciable element in our so-called civilised training,’ From this it is apparent that science was not taught to any appreciable extent in schools at that date, though doubtless in some few schools occasional lectures were given on such scientific subjects as physiology, anatomy, astronomy, and mechanics. Herbert Spencer’s pamphlet appears to have had only a very gradual effect towards the introduction of science into schemes of education. For many years chemical instruction was only given in schools at the schoolroom desk, or at the best from the lecture table, and many of the most modern of schools had no laboratories. The first school to give any practical instruction in chemistry was apparently the City of London School, at which, in the year 1847, Mr. Hall was appointed teacher of chemistry, and there he continued to teach until 1869.1 Besides the lecture theatre and a room for storing apparatus, Mr. Hall’s department 1 Mr. A. T. Pollard, M.A., Head Master of the City of London School, has kindly instituted a search among the bound copies of the boys’ terminal reports, and informs me that in the School form of Terminal Report a heading for Chemistry was intro- duced in the year 1847, the year of Mr. Hall’s appointment, 682 REPORT—1900, containcd a long room, or rather passage, leading into the lecture theatie, and closed at each end with glass doors. In this room, which was fitted up as a laboratory, and used principally as a preparation room for the lectures, Mr. Hall performed experiments with the few boys who assisted him with his lectures. As accommodation was at that time strictly limited, he used to suggest simple experiments and encourage the boys to carry them out at home, and afterwards he himself would examine the substances which they had made. From this small beginning the teaching of chemistry in the City of London > School rapidly developed, and this school now possesses laboratories which compare favourably with those of any school in the country. The Manchester Grammar School appears to have been one of the first to teach practical chemistry. In connection with this school a small laboratory was built in 1868: this was replaced by a larger one in 1872, and the present large labora- tories, under the charge of Mr. Francis Jones, were opened in 1880. Dr. Marshall Watts, who was the first science master in this school, taught practical chemistry along with the theoretical work from the commencement in 1868. As laboratories were gradually multiplied it might be supposed that boys were given the opportunity to carry out experiments which had a close connection with their lecture-room courses, But the programme of laboratory work which became all but universal was the preparation of a few gases, followed by the practice of qualitative analysis. The course adopted seems to have been largely built up on the best books of practical chemistry in use in the colleges at that time ; but it was also, no doubt, largely influenced by the requirements of the syllabus of the Science and Art Department, which contained a scheme for teaching practical chemistry.!. Even down to quite recent times it was in many schools still not considered essential that boys should have practical instruction in connection with lectures in chemistry. A Report issued in 1897 by a special Committee appointed by the Technical Education Board of the London County Council adduces evidence of this from twenty-five secondary schools in London, in which there were 3,960 boys learning chemistry. Of these 1,698 boys, or 43 per cent., did no practical work whatever ; 1 T find on inquiry at the Board of Education that practical work in qualitative analysis formed part of the examinations for teachers’ certificates in inorganic chemistry which were held at South Kensington annually in November from 1859 to 1866 inclusive. A syllabus for this examination was published in the Science Directory for 1859, the following portion of which relates to practical work :-— ‘Outlines of Qualitative Analysis. Reactions of the principal mineral acids and bases. Course pursued in the application of these reactions to the analysis of a , mixture of several acids and bases.’ Three questions were set involving the quali- tative analysis of (1) a mixture of two acids and two bases soluble in water or acids; (2) a mixture of two acids and two bases partly or entirely insoluble in water and acids; (3) more complicated mixtures. The candidates for these certificates were not examined in practical organic chemistry. The first practical examination in chemistry for students was held by the Board in 1878, inthe Advanced Stage and Honours only of inorganic chemistry, the analysis of simple salts beizg prescribed in the former, and of complex mixtures in the latter examination. Previously to this, however, special extra payments had been made on the results of instruction in practical chemistry, and questions dealing with labora- tory practice were set in the ordinary written examinations in chemistry, and were ‘as far as possible so framed as to prevent answers being given by pupils who had obtained their information merely from books and oral instruction.’ The Inspector, however, when visiting the schools might call upon any students who were to be presented for these special grants to perform experiments in his presence. This system was continued in the elementary stage of inorganic chemistry till 1882. In 1878 the syllabus for organic chemistry extended these two methods of practical examination to that branch of the subject. In the syllabus published in 1882 the present division in all stages of both organic and inorganic chemistry into distinct theoretical and practical examinations was commenced, TRANSACTIONS OF SECTION B. 685 955 boys, or 24 per cent., did practical work, consisting of a certain amount of preparation of gases, together with qualitative analysis; but of these latter 743, or 77 per cent., had not reached the study of the metals in their theoretical work, so that their testing work can have been of little educational value. It was also found that in the case of 655, or 68 per cent. of the total number of boys taking practical work, the first introduction to practical chemistry was through quali- tative analysis. But some years before this Report was issued a movement had begun which was destined to have a far-reaching effect. A Report ‘on the best means for pro- moting Scientific Education in Schools’ having been presented to the Dundee Meeting of this Association in 1867, and published in 1868, a Committee of the British Association was appointed in 1887 ‘for the purpose of inquiring and reporting upon the present methods of teaching chemistry.’ The well-known Report which this Committee presented to the Newcastle Meeting in 1889 insisted that it was worth while to teach chemistry in schools, not so much for the useful- ness of the information imparted as for the special mental discipline it afforded if the scientific method of investigating nature were employed. It was argued that ‘learners should be put in the attitude of discoverers, and led to make observations, experiments, and inferences for themselves.’ And since there can be little progress without measurement, it was pointed out that the experimental work would necessarily be largely of a quantitative character. Professor H. E, Armstrong, in a paper read at a conference at the Health Exhibition five years before this, had foreshadowed much that was in this Report. He also drew up a detailed scheme for ‘a course of elementary instruction in physical science,’ which was included in the Report of the Committee, and it cannot be doubted that this scheme and the labours of the Committee have had a very marked influence on the development of the teaching of practical chemistry in schools. That this influence has been great will be admitted when it is under- stood that schemes based on the recommendation of the Committee are now included in the codes for both Elementary Day Schools and Evening Continuation Schools. The recent syllabuses for elementary and advanced courses issued by the Incorporated Association of Headmasters and by the Oxford and Cambridge local boards and others are evidently directly inspired by the ideas set forth by the Committee. The Department of Science and Art has also adopted some of the sugges- tions of the Committee, and a revised syllabus was issued by the Department in 1895, in which qualitative analysis is replaced by quantitative experiments of a simple form, and by other exercises so framed ‘as to prevent answers being given by students who have obtained their information from books or oral instruction.’ This was a very considerable advance, but it must be admitted that there is nothing in the syllabus which encourages, or even suggests, placing the learners in the attitude of discoverers, and this, in the opinion of the Committee of this Association, is vital if the teaching is to have educational value. Many criticisms have been passed upon the 1889 Report. It has been said that life is much too short to allow of each individual adyancing from the known to the unknown, according to scientific methods, and that even were this not so too severe a tax is made upon the powers of boys and girls. In answer to the second point it will be conceded that while it is doubtless futile to try to teach chemistry to young children, on the other hand experience has abundantly shown that the average schoolboy of fourteen or fifteen can, with much success, investigate such ‘problems as were studied in the researches of Black and Scheele, of Priestley and Cavendish and Lavoisier, and it is quite remarkable with what interest such young students carry out this class of work. It may be well to quote the words which Sir Michael Foster used in this connection in his admirable Presidential Address to this Association in 1899. He said: ‘The learner may be led to old truths, even the oldest, in more ways than one. He may be brought abruptly to a truth in its finished form, coming straight to it like a thief climbing over a wall; and the hurry and press of modern life tempt many to adopt this quicker way. Or he may be more slowly guided along 684 REPORT—1900. the path by which the truth was reached by him who first laid hold of it. It is by this latter way of learning the truth, and by this alone, that the learner may hope to catch something at least of the spirit of the scientific inquirer.’ I believe that in the determination of a suitable school course in experimental science this principle of historical development is a very valuable guide, although it is not laid down in the 1889 Report of the British Association. The application of this principle will lead to the study of the solvent action of water, of crystallisation, and of the separation of mixtures of solids before the investigation of the composition of water, and also before the investigation of the phenomena of combustion. It will lead to the investigation of hydrochloric acid before chlorine, and especially to the postponement of atomic and molecular theories, chemical equations, and the laws of chemical combination, until the student has really sufficient knowledge to understand how these theories came to be necessary. There can be no doubt that this new system of teaching chemistry in schools has been most successful. Teachers are delighted with the results which have already been obtained, and those whom I have had the opportunity of consulting, directly and indirectly, cannot speak too highly of their satisfaction at the dis- appearance of the old system of qualitative analysis, and the institution of the new order of things. Especially I may mention in this connection the excellent work which is being carried on under the supervision of Dr. Bevan Lean at the Friends’ School in Ackworth, where the boys have attained results which are far in advance of anything which would have been thought possible a few years since. It is, of course, obvious that if a schoolboy is made to take the attitude of a discoverer his progress may appear to be slow. But does this matter? Most boys will not become professional chemists ; but if while at school a boy learns how to learn, and how to ‘make knowledge’! by working out for himself a few problems, a habit of mind will be formed which will enable him in future years to look in a scientific spirit at any new problems which may face him, ‘When school-days are past the details of the preparation of hydrogen may have been forgotten ; but if it was really understood at the time that it could not be decided at once whether the gas was derived from the acid or from the metal, or from the water, or in part from the one and in part from the other, an attitude of scepticism and of suspended judgment will have been formed, which will continue to guard from error. In the new system of teaching chemistry in schools much attention must necessarily be given to weights and measurements; indeed, the work must be largely of a quantitative kind, and it is in this connection that an important note of warning has been sounded by several teachers.” They consider, very rightly, that it is important to point out clearly to the scholar that science does not consist of measurement, but that measurement is only a tool in the hand of the in- quirer, and that when once sufficient skill has been developed in its use it should be employed only with a distinct object. Measurements should, in fact, be made only in reference to some actual problem which appears to be really worth solving, not in the accumulation of aimless details. And, of course, all research carried out must be genuine and not sham, and all assumption of the ‘obvious’ must be most carefully guarded against. But the young scholar must, at the same time, not forget that although the scientific method is necessary to enable him to arrive at a result, in real life it is the answer to the problem which is of the most importance.* Although, then, there has been so much discussion, during the last ten years, on the subject of teaching chemistry in schools, and such steady progress has been made towards devising a really satisfactory system of teaching the subject to young boys and girls, it is certainly very remarkable that practically nothing has been 1 Of. Professor J. G. Macgregor in Nature, September 1899. ; 2 Cf. H. Pictonin Lhe School World, November 1899; Bevan Lean, ibid., February 1890. ’ Cf. Mrs. Bryant, Special Reports on Educational Subjects, vol. ii. p. 113, TRANSACTIONS OF SECTION B. 635 said or written bearing on the training which a student who wishes to become a chemist is to undertake at the close of his school-days at the college or university in which his education is continued. One of the most remarkable points, to my mind, in connection with the teaching of chemistry is the fact that although the science has been advancing year by year with such unexampled rapidity, the course of training which the student goes through during his first two years at most colleges is still practically the same as it was thirty or forty years ago. Then, as now, after preparing a few of the principal gases, the student devotes the bull of his first year to qualitative analysis in the dry and wet way, and his second year to quantitative analysis, and, although the methods employed in teaching the latter may possibly have under- gone some slight modification, there is certainly no great difference between the routine of simple salt and mixture practised at the present day and that which was in vogue in the days of our fathers and grandfathers, Since, then, the present system has held the field for so long, not only in this country but also on the Continent, it is worth while considering whether it affords the best training which a student who wishes to become a chemist can undergo in the short time during which he can attend at a college or university. In con- sidering this matter I was led in the first place to carefully examine old books and other records, with the object of finding out how the present system originated, and I think that valuable and interesting information bearing on the subject may be obtained from a very brief sketch of the riso and development of the present system of teaching chemistry, and especially in so far as it bears on the inclusion of qualitative analysis. Unfortunately, it is not so easy to gain a good historical acquaintance with the matter as I at first imagined would be the case, and this is due in a large measure to the fact that so few of the laboratories which took an active part in the development of the present system of chemical training have left any record of the methods which they employed. In this connection I may, perhaps, be allowed to suggest that it would be a valuable help to the future historian if all prominent teachers of chemistry would leave behind them a brief record of the system of teaching adopted in their laboratories, showing the changes which they had instituted, the object of these changes, and the results which followed their adoption. There is no doubt that the progress of practical chemistry went largely hand in hand with the progress of theoretical chemistry, for as the latter gradually developed, so the necessity for the determination of the composition, first of the best known, and then of the rarer minerals and other substances, became more and more marked. The analytical examination of substances in the dry way was employed in very early times in connection with metallurgical operations, and especially in the determination of the presence of valuable constituents in samples of minerals, Cupellation was used by the Greeks in the separation of gold and silver from their ores and in the purification of these metals. Geber knew that the addition of nitre to the ore facilitated the sepdration of gold and silver, and subsequently Glauber (1604-1668) called attention to the fact that many commoner metals could easily be separated from their ores with the aid of nitre. But it was not till the eighteenth century that any marked progress was made in analysis in the dry way, and the progress which then became rapid was undoubtedly due to the discovery of the blowpipe, and to the introduction of its use into analytical operations. The blowpipe is mentioned for the first time in 1660, in the transactions of the Accademia del Cimento of Florence, but the first to recommend its use in chemical operations was Johann Andreas Cramer in 1739. The progress of blowpipe analysis was largely due to Gahn (1745- 1818), who spent much time in perfecting its use in the examination of minerals, and it was he who first used platinum wire and cobalt solution in connection with blowpipe analysis, The methods employed by Gahn were further developed by his friend Berzelius (1779-1848), who gave much attention to the matter, and who with great skill and patience gradually worked out a complete scheme of blowpipe analysis, and published it in a pamphlet, entitled ‘Ueber die Anwenduny des 686 REPORT—1900, Léthrohrs,’ which appeared in 1820, After the publication of this work blowpipe analysis rapidly came into general use in England, France, and Germany, and the scheme devised by Berzelius is essentially that employed at the present day. Indeed, the only notable additions to the methods of analysis in the dry way since the time of Berzelius are the development of flame reactions, which Bunsen worked out with such characteristic skill and ingenuity, and the introduction of the spectroscope. The necessity for some process other than that of analysis in the dry way seems, in the first instance, to have arisen in quite early times in connection with the examination of drugs, not only on account of the necessity for discovering their constituents, but also as a means of determining whether they were adul- terated. In such cases analysis in the dry way was obviously unsuitable, and ex- perience soon showed that the only way to arrive at the desired result was to treat the substance under examination with aqueous solutions of definite sub- stances, the first reagent apparently being a decoction of gallnuts, which is described by Pliny as being employed in detecting adulteration with green vitriol. The progress: made in connection with wet analysis was, however, exceedingly slow, largely owing to the lack of reagents; but as these were gradu: lly discovered wet analysis rapidly developed, especially i in the hands of Tachenius, Scheele, Boyle, Hottman, Margraf, and Bergmann, Boyle (1626-1691) especially had an extensive knowledge of reagents and their application ; and, indeed, it was Boyle who first introduced the word ‘analysis’ for those operations by which substances may be recognised in the presence of one another. Boyle knew how to ‘test for silver with hydrochloric acid, for calcium salts with sulphuric acid, and for copper by the blue solution pr oduced by aramonia. Margraf (1709-1782) introduced prussiate of potash for the detection of iron, and Bergmann (1735-1784) not only introduced new reagents and new methods for decomposing minerals and refractory substances, such as fusion with potash, diges- tion with nitric acid or hydrochloric acid, but he also was the first to suggest the application of tests in a systematic way, and, indeed, the method of analysis which he developed is on much the same lines as that in use at the present day. He paid special attention to the qualitative analysis of minerals, and gave careful instructions for the analysis of gold, platinum, silver, lead, copper, zinc, and other ores. The work of Scheele (1742-17 786) had indirectly a great influence on quali- tative analysis, as, although he did not give a eeneral systematic method of procedure in the analysis of substances of unknown composition, yet the methods which he employed in the examination of new substances were so original and exact as to remain models of how qualitative analysis shonld be conducted. Great strides in analytical chemistry in the wet way were made through the work of Berzelius, who, by the discovery of new methods, such as the decomposition of silicates by hydrofluoric acid and the introduction of new tests, greatly advanced the art. He paid special attention to perfecting the methods of analysis of mineral waters, and these researches as well as his work on ores, and particularly his investi- gation of platinum ores, stamp Berzelius as one of the great pioneers in qualitative and quantitative analytical chemistry. By the labours of the great experimenters Seeks I have mentioned qualitative analysis gradually acquired the familiar appearance of to-day, and many books were written with the object of arranging the mass of information which had accumulated, and of thus rendering it available for the student in his efforts to investigate the composition of new minerals and other substances. Among these books may be mentioned the ‘Handbuch der analytischen Chemie,’ by H. Rose, and especially the well-known analytical text-books of Fresenius, which have had an extraordinarily wide circulation and passed through many editions. The work of the great pioneers in analytical chemistry was work done often under circumstances of great difficulty, as before the end of the seventeenth cen- tury there were no public institutions af any sort in which a practical knowledge of chemistry could be acquired. Lectures were, of course, given from very early times, hut it was not until the time of Guillaume Francois Rouelle (1703-1770), at TRANSACTIONS OF SECTION B. 687 the beginning of the eighteenth century, that lectures began to be illustrated by experiments. Rouelle, who was very active as a teacher, numbered among his pupils many men of eminence, such as Lavoisier and Proust, and it was largely owing to his influence that France took such a lead in practical teaching. In Germany progress was much slower, and in our country the introduction of lectures illustrated by experiments seems to have been mainly due to Davy. When it is considered how slowly experimental work came to be recognised asa means of illustration and education, even in connection with lectures, it is not surprising that in early times practical teaching in laboratories should have been thought quite unnecessary. The few laboratories which existed in the sixteenth century were built mainly for the practice of alchemy by the reigning princes of the time, and, indeed, up to the begiuning of the nineteenth century, the private laboratories of the great masters were the only schools in which a favoured few might study, but which were not open tothe public. Thus we find that Berzelius received in his laboratory a limited number of students who worked mostly at research: these were not usually young meu, and his school cannot thus be considered as a teaching institu- tion in the ordinary sense of the word. The first really great advance in laboratory teaching is due to Liebig, who, after working for some years in Paris under Gay-Lussac, was appointed in 1824 to be Professor of Chemistry in Giessen. Liebig was strongly impressed with the neces- sity for public institutions where any student could study chemistry, and to him fell the honour of founding the world-famed Giessen Laboratory, the first public institution in Germany which brought practical chemistry within the reach of all students. Giessen rapidly became the centre of chemical interest in Germany, and students flocked to the laboratory in such numbers as to necessitate the development of a systematic course of practical chemistry, and in this way a scheme of teaching was devised which, as we shall see later, has served as the foundation for the system of practical chemistry in use at the present day. When the success of this laboratory had beer clearly established many other towns discovered the necessity for similar institutions, and in a comparatively short time every university in Germany possessed a chemical laboratory. The teaching of practical chemistry in other countries was, however, of very slow growth; in Trance, for example, Wurtz in 1869 drew attention to the fact that there was at that time only one laboratory which could compare with the German laboratories, namely, that of the Ecole Normale Supérieure. The earliest laboratory for teaching purposes in Great Britain was that of Thomas Thomson, who, after praduating in Edinburgh in 1799, began lecturing in that city in 1800, and opened a laboratory for the practical instruction of his pupils. ‘Thomson was appointed lecturer in Chemistry in Glasgow University in 1807, and Regius Professor in 1818, and in Glasgow he also opened a general laboratory. Actual progress in the general establishment of laboratories for the study ot chemistry seems to date from the time of Thomas Graham, who in 1830 was ap- pointed Professor of Chemistry at Anderson’s College in Glasgow, and in 1837 at University College, London. Whether practical chemistry was taught in Anderson’s College at that time I have not been able to ascertain, but there is no doubt that _ regular courses in testing and systematic analysis were given by Graham from 1837 \ to the date of his resignation in 1855. In 1845 the College of Chemistry was founded in London, an institution which -under A. W. Hofmann’s guidance rapidly rose to such a prominent position, and in 1851 Frankland was appointed to the chair of chemistry in the new college founded in Manchester by the trustees of John Owens, and here he equipped a laboratory for the teaching @practical chemistry. Under Sir Henry Roscoe this laboratory soon became too small for the growing number of chemical students, a defect which was removed when the new buildings of the college were opened in 1873. In 1849 Alexander Williamson was appointed Professor of Practical Chemistry at University College, London, where he introduced the practical methods of Liebigs. ' ~ 688 REPORT—1900. Following these examples, the older universities gradually came to see the necessity for providing accommodation for the practical teaching of chemistry, with the result that well-equipped laboratories haye been erected in all the centres of learning in this country. Since Liebig, by the establishment of the Giessen Laboratory, must be looked upon as the pioneer in the development of practical laboratory teaching, it will be interesting to endeavour to obtain some idea of the methods which he used in the training of the students who attended his laboratory in Giessen, From small beginnings he gradually introduced a systematic course of practical chemistry, and a careful comparison shows that this was similar in many ways to that in use at the present day. The student at Giessen, after preparing the more important gases, was carefully trained in qualitative and quantitative analysis; he was then required to make a large number of preparations, after which he engaged in original research. - Although there is, as far as I have been able to ascertain, no printed record of the nature of the quantitative work and the preparations which Liebig required from his students, the course of qualitative analysis is easily followed, owing to the existence of a most interesting book published for the use of the Giessen students. In 1846, at Liebio’s request, Henry Will, Ph.D, Extraordinary Professor of Chemistry in the University of Giessen, wrote a small bool, for use at Giessen, called ‘ Giessen Outlines of Analysis,’ which shows clearly the kind of instruction given in that laboratory at the time inso far as qualitative analysis is concerned. This book, which contains a preface by Liebig, is particularly interesting on account of the fact that it is evidently the first Introduction to Analysis intended for the training of elementary students which was ever published. In the preface Liebig writes: ‘The want of an introduction to chemical analysis adapted for the use of a laboratory has given rise to the present work, which contains an accurate description of the course I have followed in my laboratory with great advantage for twenty-five years. It has been prepared at my request by Prolessor Will, who has been my assistant during a great part of this period.’ This book undoubtedly had a considerable circulation, and was used in most of the laboratories which were in existence at that time, and thus we find, for example, that the English transiation which Liebix ‘hopes and believes will be acceptable to the English public’ was the book used by Hofmann for his students at the College of Chemistry. In this book the metals are first divided into groups much inthe same way as is done now; each group is then separately dealt with, the privcipal characteristics of the metals of the group are noted, and their reactions studied. Those tests which are useful in the detection of each metal are particularly emphasised, and the reasons given for selecting certain of them as of special value for the purposes of separating one metal from another. Throughout this section of the book there are frequent discussions as to the possible methods of the separation, not only of the metals of one group, but of those helonging to different groups; and the whole subject is treated in a manner - which shows clearly that Liebig’s great object, was to make the student think for himself. After studying in a similar mapner the behaviour of the principal acids with reagents, the student is introduced to a course of qualitative analysis com- prising, 1, preliminary examination of solids; 2, qualitative analysis of the substance in solution. Both sections are evidently written with the object not only of constructing a system of qualitative analysis, but more particularly of clearly leading the student to argue out for himself the methods of separation which he will ultimately adopt. The book concludes with a few tables which differ considerably in design from those in use at the present day, and which are so meagre that the student could not possibly have used them mechanically. % The system introduced in this book, no doubt owing to the excellent results obtained by its use, was rapidly recognised as the standard method of teaching analysis in most of the institutions existing at that time. Soon the course began to be further developed, book after book was published on the subject, and gradually the texchine of qualitative analysis assumed the shape and form with — TRANSACTIONS OF SECTION B, 689 which we are all so well acquainted. But the present-day book on qualitative analysis differs widely from ‘ Giessen Outlines’ in this respect, that whereas in the latter the tables introduced are mere indications of the methods of separation to be employed, and are of such a nature that the student who did not think for himself must have been constantly in difficulties, in the book of the present day these tables have been worked out to the minutest detail. Every contingency is provided for ; nothing is left to the originality of the student ; and that which, no doubt, was once an excellent course has now become so hopelessly mechanical as to make it doubtful whether it retains anything of its former educational value. The question which I now wish to consider more particularly is whether the system of training chemists which is at present adopted, with little variation, in our colleges and universities is a really satisfactory one, and whether it supplies the student with the kind of knowledge which will be of the most value to him in his future career. Those who study chemistry may bs roughly divided as to their future careers into two groups—those who become teachers and those who become technical chemists. Now, whether the student takes up either the one or the other career, I think that it is clear that the objects to be aimed at in training him are to give him a sound knowledge of his subject, and especially to so arrange his studies as to bring out in every possible way his capacity for original thought. A teacher who has no originality will hardly be successful, even though he may possess a very wide knowledge of what has already been done in the past. He will have little enthusiasm for his subject, and will continue to teach on the lines laid down by the text-books of the day, without himself materially improving the existing methods, and, above all, he will be unable, and will have no desire, to add to our store of knowledge by original investigation. It is in the power of almost every teacher to do some research work, and it seems probable that the reason why more is not done by teachers is that the importance of research work was not sufficiently insisted on, and their original faculty was not sufficiently trained, at the schools and colleges where they received their education. And these remarks apply with equal force to the student who subsequently becomes a technical chemist. In the chemical works of to-day sound knowledge is essential, but originality is an even more important matter. A technical chemist without originality can scarcely rise to a responsible position in a large works, whereas a chemist who is capable of constantly improving the processes in operation, and of adding new methods to those in use, becomes so valuable that he can command his own terms. Now, this being so, I think it is extraordinary that so many of the students who go through the prescribed course of training—say for the Bachelor of Science degree—not only show no originality themselves, but seem also to have no desire at the conclusion of their studies to engage in original investigation under the supervision of the teacher. That this is so is certainly my experience as a teacher examiner, and I feel sure that many other teachers will endorse this view of the and case. If we inquire into the reason for this deficiency in originality we shall, I think, ‘be forced to conclude that it is in a large measure due to the conditions of study and the nature of the courses through which the student is obliged to pass. A well-devised system of quantitative analysis is undoubtedly valuable in teaching the student accurate manipulation, but it has always seemed to me that the long course of qualitative analysis which is usually considered necessary, and which generally precedes the quantitative work, is not the most satisfactory training for a student. There can be no doubt that to many students qualitative analysis is little more than a mechanical exercise: the tables of separation are learnt by heart, and every substance is treated in precisely the same manner: such a course is surely not caleylated to develop any original faculty which the student may possess. Then, again, when the student passes on to quantitative analysis, he receives elaborate jastructions as to the little details he must observe in order to get an accurate 1900, vr 690. REPORT—1900. 4” result ; and even after he has become familiar with the simpler determinations he, rarely attempts, and indeed has no time to attempt, anything of the nature of an original investigation in qualitative or quantitative analysis. It indeed sometimes happens that a student at the end of his second year has never prepared a pure substance, and is often utterly ignorant of the methods employed in the separation of substances by crystallisation ; he has never conducted a distillation, and has no idea how to investigate the nature and amounts of substances formed in chemical reactions; practically all his time has been taken up with analysis. That this is not the way to teach chemistry was certainly the opinion of Liebig, and in support of this I quote a paragraph bearing on the subject which occurs in a very interesting book on ‘ Justus von Liebig: his Life and Work, written by W. A. Shenstone (pp. 175, 176). ‘Jnhis practical teaching Liebig laid great stress on the producing of chemical preparations ; on the students preparing, that is to say, pure substances in good quantity from crude materials. The importance of this was, even in Liebig’s time, often overlooked ; and it was, he tells us, more common to find a man who could make a good analysis than to find one who could produce a pure preparation in the most judicious way.’ ‘There is no better way of making one’s self acquainted with the properties of a substance than by first producing it from the raw material, then converting it into its compounds, and so becoming acquainted with them. By the study of crdinary analysis one does not Jearn how to use the important methods of crys- tallisation, fractional distillation, nor acquire any considerable experience in the proper use of solvents. In short, one does not, as Liebig said, become a chemist.’ One reason why the present system of training chemists has persisted so long is no doubt that it is a very convenient system: it is easily taught, does not require expensive apparatus, and, above all, it lends itself admirably for the purpose of competitive examination. The system of examination which has been developed during the last twenty years has done much harm, and is a source of great difficulty to any conscientious teacher who is ‘possessed of originality, and is desirous, particularly’ in special cases, of leaving the beaten track. In our colleges and universities most of the students work for some definite examination—frequently for the Bachelor of Science degree—either at their own University or at the University of London. For such degrees a perfectly definite course is prescribed and must be followed, because the questions which the candidate will have to answer at his examination are based on a syllabus which is either published or is known by precedent to be required. The course which the teacher is obliged to teach is thus placed beyond. his individual power of alteration, except in minor details, and originality in the teacher is thereby discouraged: he knows that all students must face the same examination, and he must urge the backward man through exacily the same course as his more talented neighbour. a In almost all examinations salts or mixtures of salts are givén for qualitative analysis. ‘ Determine the constituents of the simple salt A and of the mixture B” is a favourite examination formula; and as some practical work of this sort is sure. to be set, the teacher knows that he must contrive to get one and all of his students into a condition to enable them to answer such questions. If, then, one considers the great amount of work which is required from the present-day student, it is not surprising that every aid to rapid preparation for examination should be accepted with delight by the teacher; and thus it comes about that tables are elaborated in every detail, not only for qualitative analysis in inorganic chemistry, but, what is far worse, for the detection of some arbitrary selection of organic substances which may be set in the syllabus for the examina- tion. I question whether any really competent teacher will be found to recommend this system as one of educational value or calculated to bring out and train the faculty of original thought in students. ‘ If, then, the present system is so unsatisfactory, it will naturally be asked, > x } _. Noted. : TRANSACTIONS OF SECTION B. 691 How are students to be trained, and how are they to be examined go as to find out the extent of the knowledge of their subject which they have acquired ? In dealing with the first part of the question—that is, the training best suited to chemists—I can, of course, only give my own views on the subject—views which, no doubt, may differ much from those of many of the teachers present at this meeting. The objects to be attained are, in my opinion, to give the student a sufficient knowledge of the broad facts of chemistry, and at the same time so to arrange his practical work in particular as to always have in view the training of his faculty of original thought. I think it will be conceded that any student, if he is to make his mark in chemistry by original work, must ultimately specialise in some branch of the subject. It may be possible for some great minds to do valuable original work in more than one branch of chemistry, but these are the exceptions; and as time goes on, and the mass of facts accumulates, this will become more and more impossible. Now a student at the commencement of his career rarely knows which branch of the subject will fascinate him most, and I think, therefore, that it is necessary, in the first place, to do all that is possible to give him a thorough grounding in all branches of the subject. In my opinion the student is taken over too much ground _in the lecture courses of the present day: in inorganic chemistry, for example, the study of the rare metals and their reactions might be dispensed with, as well as many of the more difficult chapters of physical chemistry, and in organic chemistry such complicated problems as the constitutions of uric acid and the members of the camphor and terpene series, &c., might well be left out. As matters stand now, instruction must be given on these subjects simply because questions bearing on them will probably be asked at the examination. And here perhaps I might make a confession, in which I do not ask my fellow- teachers to joinme. My name is often attached to chemistry papers which I should be sorry to have to answer; and it seems to me the standard of examination papers, and especially of Honours examination papers, is far too high. Should we demand a pitch of knowledge which our own experience tells us cannot be main- tained for long ? In dealing with the question of teaching practical chemistry it may be hoped, in the first place, that in the near future a sound training will be given in ele- mentary science in most schools, very much on the Jines which I mentioned in the first part of this Address. The student will then be in a fit state to undergo a thoroughly satisfactory course of training in inorganic chemistry during his first two years at college. Without wishing in any way to map out a definite course, I may be allowed to suggest that instead of much of the usual qualitative and quantitative analysis, practical exercises similar to the following will be found to be of much greater educational value. (1) The careful experimental demonstration of the fundamental laws of chemistry and physical chemistry. (2) The preparation of a series of compounds of the more important metals, , either from their more common ores or from the metals themselves. With the ee a aid of the compounds thus prepared the reactions of the metals might be studied and the similarities and differences between the different metals then carefully (3) A course in which the student should investigate in certain selected cases : ) the conditions under which action takes place ; (6) the nature of the products ormed; (c) the yield obtained. If he were then to proceed to prepare each product in a state of purity, he would be doing a series of exercises of the highest educational value. ; (4) The determination of the combining weights of some of the more important metals. This is in most cases comparatively simple, as the determination of the combining weights of selected metals can be very accurately carried cut by measur- ing the hydrogen evolved when an acid acts upon them. ‘ Many other exercises of a similar nature will readily suggest themselves. and In_arranging the course every effort should be made to induce the student to cons YY 2 692 REPORT—1900. sult original papers and to avoid as far as possible any tendency to mere mechanical work. The exact nature of such a course must, however, necessarily be left very much in the hands of the teacher, and the details will no doubt require much considera- tion; but I feel sure that a course of practical inorganic chemistry could be con- structed which, while teaching all the important facts which it is necessary for the student to know, will, at the same time, constantly tend to develop his faculty of original thought. Supposing such a course were adopted (and the experiment is well worth trying), there still remains the problem of how the student who has had this kind of training is to be examined. With regard to his theoretical work there would be no difficulty, as the examination could be conducted on much the same lines as at the present time. In the case of the practical examination I have long felt that the only satisfactory method of arriving at the value of a student’s practical knowledge is by the in- spection of the work which he has done during the whole of his course of study. and not by depending on the results of one or two days’ set examination. I think that most examiners will agree with me that the present system of examination in practical chemistry is highly unsatisfactory. This is perhaps not so apparent in , the case of the qualitative analysis of the usual simple salt or mixture; but when the student has to do a quantitative exercise, or when a problem is set, the results sent in are frequently no indication of the value of the student’s practical work. Leaving out of the question the possibility of the student being in indifferent health during the short period of the practical examination, it not infrequently happens that he, in his excitement, has the misfortune to upset a beaker when his quantitative determination is nearly finished, and asa result he loses far more marks than he should do for so simple an accident. Again, in attacking a problem he has usually only time to try one method of solution, and if this does not yield satisfactory results he again loses marks; whereas in the ordinary course of his practical work, if he were to find that the first method was faulty he would try other methods until he ultimately arrived at the desired result. It is difficult to see why such an unsatisfactory system as this might not be replaced by one of inspection, which I think could easily be so arranged as to work well. A student taking, say, a three years’ course for the degree of Bachelor of Science might be required to keep very careful notes of all the practical work which he does during this course, and in order to avoid fraud his notebook could from time to time be initialled by the professor or demonstrator in charge of the laboratory. An inspection of these notebooks could then be made at suitable times by the examiners for the degree, by which means a very good idea would be obtained of the scope of the work which the student had been engaged in, and if thought necessary a few questions could easily be asked in regard to the work so presented. Should the examiners wish to further test the candidate by giving him an examination, I submit that it would be much better to set him some exercise of the nature of a simple original investigation, and to allow him two or three weeks to carry this out, than to depend on the hurried work of two or three days. The object which I had in view in writing this Address was to call attention to the fact that our present system of training in chemistry does not appear,> develop in the student the power of conducting original research, and at the same time to endeavour to suggest some means by which a more satisfactory state of things might be brought about. I have not been able, within the limits of this Address, to consider the conditions of study during the third year of the student’s career at college, or to discuss the increasing necessity for extending that course and insisting on the student carrying out an adequate original investigation before granting him a degree, but I hope on some future occasion to have the oppor- tunity of returning to this very important part of the subject. If any of the TRANSACTIONS OF SECTION B. 693 suggestions I have made should prove to be of practical value, and should lead to the production of more original research by our students, I shall feel that a useful purpose has been served by bringing this matter before this Section. In concluding I wish to thank Professor H. B. Dixon, Professor F. S. Kipping, and others, for many valuable suggestions, and my thanks are especially due to Dr. Bevan Lean for much information which he gave me in connection with that part of this Address which deals with the teaching of chemistry in schools. The following Reports and Papers were read :— 1. Report on the Teaching of Science in Elementary Schools. See Reports, p. 187. 2. On some Problems connected with Atmospheric Carbonic Anhydride, and on a New and Accurate Method for determining its Amount, suitable Jor Scientific Expeditions. By Professor Lurrs, D.Sc., Ph.D., &c., and R. F. Buake, £..C., £.C.S., Queen’s College, Belfast. Attention is drawn to the variations in the amount of atmospheric carbonic anhydride which correspond with at least 10 per cent. of the total amount, the causes of which are still to a large extent obscure. In the author's opinion the subject is an important one, and is worthy of a systematic investigation by a number of skilled observers working in different localities and employing the same method of determination which shall have been proved to give results which do not vary from the true amount by more than three or four parts per million of air. Among the problems relating to atmospheric carbonic anhydride which the authors think are specially deserving of attention are the following :— 1. Is Schloesing’s Theory Correct ?—Do the oceans really act as regulators of the amount of atmospheric carbonic anhydride by the production or dissociation of earthy bicarbonates according as the amount rises above the normal or falls below it? As consequences of this theory latitude should influence the quantity of atmospheric carbonic anhydride, which ought to be lower in polar than in tropical localities, and the great ocean currents should also have an etfect as they pass from warmer to colder regions, or the opposite. 2. The Influence of Day and Night at Sea.—To account for the increased quantity of atmospheric carbonic anhydride over land surfaces at night, which most of the observers have found, two theories have been advanced: (a) cessation of plant activity in decomposing the gas owing to the absence of light, and (4) the streaming out of ground air from the soil owing to the lowering of temperature. At sea no such influences can be exerted, but an absorption of atmospheric carbonic anhydride may occur at the surface of the water owing to lowering of temperature, thus reversing the land effect. 3. The Effects of Atmospheric Precipitates, and especially of Snowfall, which appears to increase the amount of Atmospheric Carbonic Anhydride.—No reason- able theory has been advanced to account for this curious phenomenon, and it would be interesting to ascertain whether it occurs at sea as well as on land; and the same remark would apply to fog and rain, both of which appear to affect the amount also, Other supposed causes of variation are worth studying, such as the effects of the seasons, direction and force of the winds, the prevailing type of weather, &c. But those which the authors think most interesting are such as a scientific mission would be under peculiarly favourable conditions for observing, and especially the proposed Antarctic expeditions. In a memoir of the authors recently published in the ‘ Proceedings of the Royal Dublin Society’ (vol, ix. N.S., Part If, No, 15) a modification of Pettenkofer’s 694 REPORT—1900, process for determining atmospheric carbonic anhydride is described by means of which results of great accuracy may be obtained. Thus in the final set of test experiments with artificial mixtures of purified air and carbonic anhydride in known volumes a mean error (in six determinations) of about 1 per cent. of the gas was found, corresponding with some four parts per million of air taken. For use by a scientific expedition it seemed, however, to the authors that a different process is required in which the operations at the place of observation should be as simple as possible, and of such a nature as to permit of the actual determinations being made at any convenient time later, when the resources of a properly equipped laboratory are available The authors have accordingly devised a method which fulfils these conditions, and which is simple and accurate. On the one hand it resembles Pettenkofer's process in that a relatively small volume of air is examined (about six litres}, while, on the other, Miintz and Aubin’s principle is adopted of absorbing the carbonic anhydride by caustic potash solution and afterwards liberating it by ebullition 7 vacuo with an acid and measuring its volume in a suitable gas analysis apparatus. A series of sealed tubes is prepared in the laboratory, each tube containing an accurately measured volume of weak potash solution (the amount of combined carbonic anhydride which such a solution always contains having been ascer- ~ tained for a given stock), The only operations which have to be performed at the place of observation are the collection of the air sample in a suitable receiver; the transfer of the contents of one of the sealed tubes to the latter, and after absorption of the atmospheric carbonic anhydride their retransfer as far as possible to the same tube, which will be again sealed. ‘The tubes can of course be kept for an indefinite period both before and after their contents have been thus treated, and the determination of the absorbed carbonic anhydride made, when convenient, with an aliquot portion of their contents. The experiments made to test the accuracy of the new method were satisfactory. Artificial mixtures of purified air and carbonic anhydride in definite volumes were employed (the two heing in about the proportion they occur in ordinary air). Five determinations in such mixtures gave a mean error of 13 per cent. of the carbonic anhydride taken equivalent to four parts per million of air, 3. On the Distribution of Chlorine in West Yorkshire. By Wituiam Ackroyp, LC. The present observations are to be regarded as the preliminaries to an attempt to construct isochlors for this part of Yorkshire. The subject is one of acknow- ledged importance, Professor Mason remarking:—‘State maps, such as those issued for the States of Massachusetts and Connecticut, are most valuable, and their construction is well worth the expenditure of public money.’! Although the work is not far enough advanced for map construction, the figures which follow, and observations thereon, will be of chemical and hygienic interest during the visit of the British Association to Bradford. In the first place these British normal chlorine figures are very high in com- parison with the published American data. The lowest Massachusetts figure is ‘O7 part of Cl per 100,000 in the area farthest removed from the Atlantic sea- border : here the lowest found has been*7 part per 100,000 in the upper reaches of the Wharf, and all round it appears that the Yorkshire figures are about ten times larger than those of the State of Massachusetts, which is to be accounted for— (1) by the closeness of the sea-border on either side to the Pennine range, and (2) by the density of population in and the antiquity of the inhabited areas. The unit isochlor area is coextensive with the highest hills and their becks, deans and gills. The following chlorine determinations with waters from the 1 W. P. Mason, Lxamination of Water, p. 29. |. TRANSACTIONS OF SECTION Bz 695 upper reaches of the Wharf, Wenning, Ribble, Aire, and Calder will ke stifficiently illustrative :— Chlorine | Chlorine parts per parts per 100,000 109,000 Barden ' . ° ghitLs Ingleborough Cave 2 Grimwith Beck 1:2 Lower Bentham 2 . (1:4 Gate-up-Gill O7 Malham Tarn outlet. Tha Bleabeck . 1:0 » Cove 0:95 Buckden Pike 1-0 Airehead 10 Starbottom . 0:8 id Smelt Mili 1G Kettlewell . 1:0 Gordale Beck 1:2 Buckden Village 1:2 Hanlith Bridge 11 Gaping Ghyll . 9 12 Hardcastle Craggs Tel Beck Head, Clapdale . 13 Walshaw Dean . 11 As the sea is approached, and more populous districts are reathed, the chlorine rises, and remarkable examples of rise may be met with on the same hill slope. Halifax furnishes a striking instance. The town rests on a sloping bed of Mill- stone grit, the ancient and most thickly populated part being towards the bottom of the incline. The ground waters of the highest parts—Mount Tabor—vary from 16 to 2:6; widely separated wells, about halfway down, yield the figure 3'8; while towards the bottom of the slope two wells give the figures 4:7 and 55, The public water supply from Pennine gathering grounds, ten milesaway, stands at, 1:5. The figures obtained for other parts of the West Riding have not yet been severely collated, and are therefore reserved for a further communication. 4. On alimiting Standard of Acidity for Moorland Waters. By Wiuu1am Ackroyd, 111.C., Public Analyst for Halifax. Many large towns, more especially in the West Riding of Yorkshire, have their public water supplies of moorland origin. The case of Milnes v. the Hudders- tield Corporation in 1881 gave great prominence to the fact that this class of water may give rise to plumbism. No satisfactory explanation could be given at the time, and it is only during the present decade that it has been clearly understood that the plumbo-solvent action of moorland waters is to be associated with acidity. An idea of the relation is furnished by the following determinations :— Parts per 100:000, Acidity in Equivalent Lead dissolved from of Sulphuric Acid. 32-inch Piping. 13 5 Fi : 0:29 Inlhour . : : 703 2. . , . 030 9 5 5 . 057 3. . . » 0:29 3 : : + 7025 = . . pelos: Injhour . : as 5. 5 . 159 3 F ? ». 95 The acidity is due to carbonic anhydride and peaty acids, and the total is found by ascertaining the number of c.c. of N/100 alkali required to neutralise 100 c.c. of the water, the result being expressed as sulphuric acid. Phenolphthaiein is used as the indicator. ; The acidity may be very high as from peaty gathering grounds of small incline, ay awe 44, or comparatively low in gathering grounds of steep incline, say in 12, ie In the former case violent action on lead precludes its use for domestic con- sumption, and in the latter even a limit must be placed on the degree of acidity allowable. During epidemics of plumbism in the West Riding much diversity of opinion has been expressed on various points connected with the matter which the ' ? Ackroyd, Journ. Chem. Soe,, 1899, p. 199. 696 REPORT—1900, author caniidt discuss here ; he contents himself with stating that after some years of experience he has néver learnt of the occurrence of any case of plumbism where the acidity of the water has been under the equivalent of 0°5 partof sulphuric acid per 106-000 of water, and this he tentatively proposes as a limiting standard of acidity for potable waters of moorland origin when the acidity is determined in the manner already described with phenolphthalein as indicator. The average acidity of nine samples of water not above suspicion in this respect was 0:63, ranging from 0:53 to 0°91; while on the other hand sixty-one samples above reproach from neighbourhoods where plumbism has not been known had an average acidity of 0:27, the extremes being 0°20 and 0:41. © 5. On the Effects of Copper on the Human Body. Ly Tuomas Wuirrsipr Hime, B.A., ID. The recrudescence of an agitation by some public analysts as to alleged danger to health produced by copper has rendered it desirable to make an investi- gation into the subject, although it was long since satisfactorily disposed of, from a point of view hitherto scarcely utilised as it deserves, and at the same time to review the general results attained. The examination of the two principal excretions, solid and liquid, by which copper is eliminated from the body, offered a promising means of judging of the effects of the agent, whether merely swallowed or also absorbed. ‘These excretions have therefore been examined during a period of severa] months, from a number of healthy persons engaged, some for many years, in dealing with copper, either in smelting works or as workers in its alloys, brass, &c., or from healthy persons unconnected with any kind of copper work, who had intentionally swallowed some compound of copper in improperly so-called -‘ greened’ vegetables (they are not rendered ‘ green’ by treatment with copper) or otherwise. Copper was found in relative abundance in the excretions of all of these persons, yet they had enjoyed perfect health, and were unconscious of any- thing abnormal existing in their excretions. It is excreted slowly, and some weeks may elapse before the whole of the copper-compound ingested is got rid of. That fact, that copper may, after being swallowed, be absorbed into the blood and exist there for months, and no doubt during at least twenty years, without indicat- ing its presence by the slightest interference with health, or indeed in any way whatever, has thus been established beyond question. In one case, a brags-finisher aged thirty-eight, who had been thirty years engaged in brass-work, copper was found on various occasions when sought, during several months. For the last fourteen years this man has never drawn any money from his sick club, and he has had perfect health. The copper exists in the excretions, as it dces in coppered vegetables, not as copper, but as an insoluble compound, which when tested directly for copper gives no indication of copper being present in any form. As a fact, no copper is present. It is entirely unjustifiable to speak of copper being a poison because when combined with some other elements poisonous effects may be produced by the compound. Because copper and arsenic combined, forming copper arsenite, which. is not copper, is poisonous, a death due to copper arsenite is reported and quoted for sixty years in all the text-books as due to ‘ poisoning by copper!’ As well call iron a poison, because it too, when combined to form a new compound, arseniate of iron, may prove poisonous. Copper exists in a great number of plants, including cereals, mineral waters, wines, shell-fish, fruits, and various kinds of animal flesh, It has been calculated that a man eating good bread, ‘ coppered’ only by nature, would consume in this way alone some 93 grains of copper, corresponding to 866 grains of the sulphate. Thousands of wealthy and educated persons who flock yearly to the health-restoring springs of Wiesbaden, Teplitz, Pyrmont, &c., consume copper in every glass of water they drink, yet their health _ improves, they return yearly to derive fresh benefit, and are unaware that they are being ‘poisoned.’ Many trustworthy observers have found copper as a normal constituent in the human body. That the consumption of vegetables which have been treated with copper to preserve their natural green is perfectly harmless has a a TRANSACTIONS OF SECTION B. 697 been proved beyond all doubt, not only by such experiments as that of Galippe, who for fourteen months took copper with his food daily without any ill effect, and the classic experiments of Lehmann and his pupils on themselves for many months; but by the infinitely larger experiments made yearly by thousands of the public who consume copper in some form or other in artificially coppered vegetables, and in their flour, fruit, various kinds of flesh, oysters, crabs, wines, mineral waters, &c. ‘coppered’ by nature. Not one case of injury to health under such circumstances has ever been brought forward, even in prosecutions for selling ‘coppered’ peas as being ‘injurious to health!’ The charge is supported by the allegation ‘copper is a poison.’ But people who eat ‘coppered’ vegetables do not consume ‘copper.’ The chemical compound of copper they swallow is not copper at all, and they are not injured. Even verdigris, so much feared, is not all the dangerous substance alleged. Copper utensils are quite harmless with ordinary cleanliness. The alleged ‘poisonings’ by food cooked in copper vessels have undoubtedly been mostly, if not all, due to ptomaine-poisoning. Copper has been known and used longer than any other metal, and in its alloys is the most generally used of all metallic substances. It has been in use from prehistoric times, and. its dangers, if they existed, must have been known to the ancient and modern world. Yet the ancients are absolutely silent on the subject, and among moderns only a few, almost entirely analysts, declaim to an incredulous public as to dangers which have not been realised. The alleged fraud in so-called ‘greening’ of vegetables is purely imaginary. The copper does not ‘green’ old peas or make them look young. Old yellow peas when ‘coppered’ still look old and yellow. The quantity of the copper compound present in the amount of artificially treated vecetables which is occasionally eaten at a meal is only a fraction of the corresponding amount of copper sulphate which physicians prescribe to be taken three times a day for weeks and months continuously. Therefore there is no sufficient ground for the prohibition of the sale of ‘coppered’ vegetables, any more than of the innumerable kinds of fruits, vegetables, shell-fish, cereals, mineral waters, wines, and animal flesh which naturally contain the metal in some form. If the latter drastic arrangement were attempted, absolute and general starvation would be the inevitable result, so widely is the natural presence of copper in articles of food extended. 6. Interim Report on the Continuation of the Bibliography of Spectroscopy.—See Reports, p. 150. 7. Report on Preparing a New Series of Wave-length Tables of the Spectra of the Elements.—See Reports, p. 193. PRIDAY, SEPTEMBER 7. The following Papers and Reports were read :— 1, The Specific Heat of Gases at Temperatures up to 400° C. By H. B. Dixon, /.R.S., and F. W. Rixon, B.Sc. The authors have found that the specific heat of gases between 15° C. and 400° C. may be directly measured by heating the gas (under pressure) in a thin steel cylinder and dropping it into a water calorimeter. A repetition of the experiment with the steel cylinder empty makes the method a differential one, eliminating most of the experimental error. The specific heat of CO, at constant volume has been thus measured between 15° and 115° C., 192° C., 298° C., and 898° C. The specific heat obtained at 115° agrees closely with that obtained by Joly under nearly similar conditions. 698 REPORT—1900, The specific heat of CO, is found to rise regularly with the temperature. Varia- tions in the pressure of the gas produce slight variations in the specific heat. The following values have been obtained by reducing the observed values by means of Joly’s formula to the same pressure :— ; Specific Heat reduced to Initial Temperature Final Temperature Pressure of 100 Atmos. 115° 16° 2000 118° Vig 2004 192° 175 ‘2092 298° aae 2884 398° 21° 3565 The authors propose to determine the specific heat of nitrogen and of argon under the same conditions with the same apparatus. 2. Interim Report on the Nature of Alloys. 3. Report on the Chemical Compounds contained in Alloys. By F. H. Nevitte, /.2.S.—See Reports, p. 131. 4. On the Mutual Relations of Iron, Phosphorus, and Carbon when together in Cast Iron and Steel. By J, E, Swap. 5. The Crystalline Structure of Metals! By J. A-Ewine, V.RS., Professor of Mechanism and Applied Mechanics in the University of Cambridge ; and Waurrr Rosenuain, B.A., St. John’s College, Cambridge, 1851 Exhibition Commissioner's Research Scholar, University of Melbourne. The paper describes the results arrived at by the authors in investigating the effects produced upon the micro-structure of metals by (1) plastic strain, and by (2) exposure of strained metal to moderate temperatures. After describing and illustrating the well-known characteristics of erystalline structure in metals as revealed by the microscope, the authors show that plastic strain is accompanied by the appearance of minute steps on a surface of the metal which had been plane polished before the application of the strain. When viewed under the microscope these steps appear as black lines under normally incident light, but they appear as bright bands when oblique light of suitable incidence is used. Their observations lead the authors to conclude that metals yield under plastic strain by the slipping of the component parts of each crystal along definite cleavage or gliding plane. The steps in the surface being a consequence of these slips, the authors have called them ‘slip-bands.’ Further evidence leads the authors to conclude that plastic strain in metals occurs without loss of crystalline character, the crystals as a whole accommodating themselves to new shapes and positions by the slipping of their elements, with the result that the crystalline structure is preserved even when the material as a whole undergoes much deformation. The use of slip-bands as a means of microscopic observation is also described and illustrated, more particularly with reference to the occurrence and formation of twin-crystals in copper, gold, nickel, lead, and other metals. Slip-bands are also illustrated in various kinds of iron and steel, nickel, zinc, tin, cadmium, lead, silver, gold, bismuth, and some alloys, the magnifications varying from 40 to 1,000 diameters, ' For other accounts of these researches see papers by the same authors, Proc. Roy. Soc., March 16 and May 18, 1899, May 81, 1900, and Phil. Trans., vol, A, 1900, and yol. A, 1901. : TRANSACTIONS OF SECTION B. 699 The second part of the paper deals with the effects of moderate temperatures ‘(up to 200° C.) on such metals as lead, zinc, tin, and cadmium. The authors have found that when these metals are subjected to a very severe plastic strain the original large crystals are broken up into much smaller ones, without, however, destroying their truly crystalline nature. They have further found that when so treated these metals readily recrystallise. In’ the case of severely strained lead they have shown that even at the ordinary temperature of a room gradual recrys- tallisation can be observed in the course of several months, while at higher tem- peratures the changes are much more rapid. A freshly strained specimen exposed to 200° C. was found to recrystallise in a few minutes. It was also found that severe plastic strain is essential to such recrystallisation, and that minute crystals obtained by chilling the metal in casting are not capable of recrystallisation at such moderate temperatures. Closer observation has shown that this recrystallisa~ tion of strained metal takes place by the growth of certain of the minute crystals at the expense of their neighbours; individual crystals have been observed to grow until they were many hundreds of times larger than their neighbours, The final section of the paper deals with a theory which one of the authors (W. Rosenbain) bas advanced as an explanation of these phenomena of annealing. According to this view, which both authors believe to be correct, the metallic im- purities present in the metal, and forming with it eutectic alloys, play an essential part in these actions. In the ordinary crystallisation of the metal these eutectics form thin films of intercrystalline cement, and, according to the theory of the authors, the growth of one crystal at the expense of its neighbour occurs by means of solution in and diffusion through the entectic films of the metal constituting the erystals, Evidence is adduced to show that such diffusion would be greater in ore direction than the other, and to support the authors’ belief that the action may be electrolytic. As a consequence of this theory ihe authors were led to make experiments on the cold welding of lead, and they have found that, as the theory would indicate, a weld between clean surfaces of lead is a barrier to crystalline growth, but that such growth readily crosses a weld into which a small amount of a suitable metallic impurity had been introduced. The authors believe that these experiments strongly support their ‘ solution theory ’ of annealing. 6. On the Electric Conductivity of the Alloys of Iron. By Professor W. F. Barrert, J.£.S, - 7. Some new Chemical Compounds discovered by the Use of the Electric Furnace. By C. 8. Brapiey. These chemical compounds, which were discovered and examined by Mr. Charles B. Jacobs, of New York, consist of the alkaline earth silicides of calcium, barium, or strontium; by a secondary step silico-acetylene is obtained. They have the formula CaSi,, BaSi,, and SrSi, respectively, and are the silicon analogues of the alkaline earth carbides, while the silico-acetylene is the analogue of acetylene having the formula Si,H, when the carbonates or oxides of the alkaline earths are mixed with silica in the form of ground quartz or sand, in which the relative atomic proportion of the alkaline earth metal to the silicon in the mixture is as 1 is to 2, and sufficient carbon to effect the reduction is added, or, when silicates of the alkaline earth metals in which the atomic relation of the earth metal to the silicon is as 1 to 2, are mixed with sufficient carbon to take up the oxygen of the compounds present, and heated in the electric furnace under conditions substantially like those maintained in the manufacture of alkaline earth carbides, silicides of the alkaline earth metals result. As an example of the process the following reactions for the formation of barium silicide from the barium compounds are given :— (1) BaCO, + 2 SiO, + 6C =BaSi, +7 CO (2) BaO+2Si0, + 5C =BaSi, +500 200 REPORT—1900, Calcium and strontium silicides are formed by exactly similar reactions from similar compounds. They are white or bluish-white substances of metallic appear- ance, and also resemble aluminium silicide and silicon somewhat in appearance. They possess a distinctly crystalline fracture, showing plate-like crystals very similar to those seen in the fracture of cast zinc, the crystals being, however, some- what smaller in size. They oxidise slowly in the air and more rapidly under the influence of heat, yielding silicon dioxide and the oxide of the alkaline earth metals present. Like the carbides they decompose with water, but yield, instead of acetylene, hydrogen in a pure state, which is evolved without explosion, the following being the reaction :— (1) CaSi, + 6H,0=Ca (OH), +2 SiO, + 10H (2) BaSi, +6 H,O = Ba (OH), +2 SiO, + 1OH (3) SrSi, + 6H,O= Sr (OH), +2 SiO, + 10H The calcium compound dissolves slowly in cold water, but more rapidly in hot water; the barium compound decomposes rapidly in both cold and hot water. The strontium compound dissolves more rapidly in water than the calcium, but not so rapidly as the barium compound. It will be noticed by considering the equations 1, 2 and 3, that all of these compounds evolve large volumes of hydrogen :— 1 1b, CaSi, producing 104 Ib, or 18°73 cubic ft. hydrogen 11b. BaSi, 53 O51 Ib. or 9:15 - bf 11b. SrSi, r ‘069 lb. or 12°36 at 0° C. and 760 mm. Calcium silicide, when treated with dilute acids, either the oxy-acids or the hydrogen acids, gives rise to the formation of a new compound which has the formula Si,H, and is therefore the silicon analogue of acetylene C,H, and must be called silico-acetylene since it bears the same relation to silico-methane (silicon hydride) SiH, as acetylene bears to methane CH, The reaction being ° CaSi, + 2 HCl = CaCl, + Si,H, Silico-acetylene is a yellow crystalline compound and differs in properties from the compound SiH, which Ogier obtained by sparking SiH, which was unstable and exploded when subjected to a shock, Si,H, being stable or non-explosive at ordinary temperatures. When treated with 20 per cent. solution of caustic soda or potash, Si,H, yields hydrogen according to the following equation :— Si,H, + 4 NaOH +2 H,O=2 Na, SiO, +1 OH Heated in air this compound Si,H, oxidises rapidly, giving 2 SiO, H,O, and when heated in a closed tube it breaks down into amorphous silicon and free hydrogen. Strontium silicide when treated with a strong acid does not produce silico-acetylene with the same facility, while the barium compound when so treated produces a mixture of gaseous compounds and free hydrogen. These silicides can be produced at low cost where electric power is cheap, are very powerful reducing agents, and we hope will find large use in the dye industries. Some experiments have been tried on molten steel carrying phosphorus and sulphur, and the requisite quantity of silicide of barium or calcium completely removed these impurities as well as all oxygen present. ” ” 8. Report on the Electrolytic Methods of Quantitative Analysis. See Reports, p. 171. TRANSACTIONS OF SECTION B. 701 MONDAY, SEPTEMBER 10. The following Papers and Reports were read :— 1. Derivatives of Methyl-furfural. By Henry J. Horstman Fenton, F.R.S., and Miss Mitprep Gostiine, B.Sc. The authors have previously shown that an intense purple colour results when levulose, cane sugar, sorbose, or inulin is acted upon by dry hydrogen bromide in ethereal solution. The colour-giving substance was isolated in a crystalline state and was shown to be bromo-methyl-furfural, its formation being characteristic of ketohexoses, or substances which yield them on hydrolysis. This substance is now the subject of further investigation, and the following results have so far been obtained. When acted upon by stannous chloride in acid solution the bromine is easily replaced by hydrogen, and the resulting liquid is identical in every way with oO methyl-furfural; so that the reaction affords by far the simplest method for the preparation of the latter substance in a pure state. The bromo-compound, when dissolved in appropriate solvents, readily reacts with various silver saits, giving rise often to beautifully crystalline compounds ; the acetoxy- and benzoxy-derivatives have, for example, been prepared and analysed. By the action of sulphurous acid, these, like the parent compound, yield the remarkable condensaiion product C,,H,O,, which gives beautiful colour- reactions with caustic alkalis and with aniline. This condensation-product has also been further studied, and the results so far favour the author’s original suggestion that it is a dicarbonyl compound. 2. A Simple Method for comparing the ‘ Affinities’ of certain Acids. By Henry |. Horsrman Fenton, £.2.S., and Humporey Owen Jonss, BA, B.Sc. In a former communication! the authors have described the isolation and properties of free oxalacetic acid, and several interesting reactions of this acid are now being investigated. During a more extended study of the Aydrazone the following somewhat remarkable behaviour has been observed. Heated with dilute sulphuric acid it is transformed, as was previously shown,” into Wislicenus’s phenyl- pyrazolon carboxylic acid (C,,H,,N,O, =C,,H,N,O, + H,0) ; but in order that this change may be complete it is now found that a certain minimum concentration of the acid is necessary. When heated with pure water an entirely different result is obtained : carbon dioxide is evolved, and the hydrazone of pyruvic acid separates in the crystalline state—C,,H,,N,O, = C,H,,N,0,+CO,. If the concentration of the acid falls below this necessary minimum both reactions occur simultaneously, even though the acid is present in excess; with decinormal sulphuric acid, for example, about 26 per cent. undergoes the second change. A preliminary set of observations has been made with the following acids, using decinormal solutions and measuring the evolved carbon dioxide in a specially constructed apparatus— hydrochloric, nitric, sulphuric, trichloracetic, tartaric, malic, succinic, citric, acetic. The results obtained indicate that the amounts of carbon dioxide evolved are in the inverse order of the concentration of the hydrogen ions, so that a comparison can be made of the relative ‘strengths’ or ‘ affinities’ of the acids. The order obtained with the above acids agrees remarkably well with that resulting from the other well-established methods. 3. Recent Developments in Stereochemistry. By W.J. Pore. 1 Trans. Chem. Sac., 77, 1900. 2 Loc. cit. 702 REPORT—1900, 4, The Constitution of Camphor. By A. Lapwortu, D.Sc. See Reports, p. 299. 5. The Degradation of Camphor. By Juuius Brept. 6, The Camphor Question. By Professor Osstan ASCHAN. 7. Report on Isomeric Naphthalene Derivatives.—See Reports, p. 297. 8. Report on Isomorphous Derivatives of Benzene.—See Reports, p. 167. 9. Report on the Relations between the Absorption Spectra and Chemical Constitution of Organic Bodies.—See Reports, p. 151. 10. Action of Aluminium Powder on some Phenols and Acids. By W. R. Hopexiyson. 11. On the Direct Preparation of }-Naphthylamine. By Dr. Lyonyarp Limpacn and W. R. Hopexryson. On nitrating naphthalene in the usual manner there results not only o-nitro, but also an appreciable quantity of the 8-derivative, as we haye several times proved by obtaining B-naphthylamine. This note has, of course, a theoretical interest only, as 8-naphthylamine can so easily be obtained from 8-naphthol ky the NH, process under pressure.! The nitro-naphthalene obtained by direct nitration of naphthalene is reduced in the usual way, and the naphthylamine converted into the HCl salt. The hydro- chloride of a-naphthylamine is comparatively insoluble, whilst the hytirodhlgane of the 8-derivative is very soluble. This ailows of an easy fractional cr ystallisation, the mother liquors containing much of the @-salt. A good method of separation. consists in treating these mother liquors with potassium hydrate in excess and steam distilling. The steam distillate, after becoming solid, or nearly so, is dried by pressure between paper or on a pump, and then sublimed. 8-Naphthylamine alone sublimes, and can in this manner be obtained quite pure, of melting point, 112°, and boiling point 304°. It sublimes in beautiful pearly plates. The amount of B-naphthylamine generally contained 1 in tlie crude naphthy lamine seems to be about 5 per cent. or under. ; - ‘We have obtained by this method about a kilog. he purs Swi from technical naphthylamine mother liquors. 12. Interaction of Furfuraldehyde and Caro’s Reagent. By C. F. Cross, E. J. Bevan, and J. F. Briaas. Tn a previous paper? it was shown that hydrogen peroxide reacted with furfural to form a monohydroxy-furfuraidehyde as the main product, with simultaneous 1 Siebermann (Anz. 123, 264) also obtained B-naphthylamine direct, but by a somewhat roundabout process. 2 Chem. Soc, J., 1899, p. 747, TRANSACTIONS OF SECTION B. 703- production of the corresponding carboxylic acid in small quantity. The substitut- Ing groups appear to occupy the J, 2 positions in the ring. The monohydroxy furfural is identified, by its very characteristic relations with phloroglucivol and resorcinol, as a constituent of the lignocelluloses. Caro's reagent, prepared from potassium persulphate and sulphuric acid, according to the directions of Baeyer and Villiger,! reacts under similar conditions in a different manner. In the first place the reaction appears to be quantitative, and when the furfural has taken up O, a trace of either reagent in excess persists. The temperature remaining at 15°-2U°, and there being no evolution of gas, we may expect to find a product of empirical formula C;H,O,, and as the aldehydic group disappears this should be a hydropyromucie acid. From the isolation and analysis of a crystalline methylphenyl-hydrazide we confirm the product as a monocarboxylic acid. On reduction with sodium amalgam an aldehydic product is obtained with the brilliant colour reactions of the monohydroxyfurfurals. Control observations on pyromucic acid proved that this acid is reduced under similar conditions to furfural. The reactions of this hydroxyfurfural, though similar to those described in our previous paper, are sufficiently differentiated to indicate that we have obtained a second isomeride. Moreover, the corresponding acids are differentiated, the one giving Pb and Ba salts, insoluble in acetic acid; the salts of the new acid are soluble, and, moreover, the acid undergoes hydrolysis with such ease as to make its isolation in the pure state a matter of great difficulty. In the course of the usual processes for isolating the Ba and Ca saits, decomposition occurs, and the crystalline salts isolated are those of a dibasic acid. On boiling the original product in solution at constant volume, formic acid distils continuously and with traces only of cther acids. The yield of formic acid amounted in one experiment to 0:7 grm. per 1 grm. of original furfural. All these observations indicate that the original product of oxidation is the acid C,H,0 . (COOH) (OH) 1-4. . . . A characteristic reaction of this original acid is the production of a yellowish-red precipitate with ferric chloride, similar to that obtained with pyromucic acid. At is to be noted that the Caro reagent oxidises the constituent of the lighocelluloses, which gives the brilliant colour reactions with phenols character- istic of these natural products, which we know to be a hydroxyfurfural. In this respect the reagent differs from the oxidants ordinarily used for bleaching purposes, eg., hypochlorites and permanganates. A quantitative experiment with a typical aldose (dextrose) and the Caro reagent gave a somewhat unexpected, entirely negative result. The cupric reduction (Fehling solution) was unaffected. The typical ketose lzvulose, on the other hand, is slowly oxidised. All of these matters are under investigation. 13. On the Synthesis of Benzo-y-pyrone. By Dr. 8. Rusemann and H. E. Srapurron, B.A. (Oxon.) The important group of yellow vegetable dyes, the éhief of which are chrysin, fisetin, and morin, are derived primarily from a phenyl! benzo-y-pyrone— \co% This was synthetised in 1898 by Kostanecki, but the mother substance itself, benzo-y-pyrone, had not, up to the middle of 1900, been isolated. The authors succeeded in preparing this compound from phenoxy-fumarie acid— COOH .C = CH. COOH ‘ . ees (UAE AE ile 1 1 Ber., 1899, 704 REPORT—1900. This acid dissolves with evolution of heat in concentrated sulphuric acid, and on diluting the solution with water a new acid is precipitated which was found to be benzo-y-pyrone carboxylic acid— COOH .C = CH—CO Ose: eH, On distillation 7 vacuo this broke up with the evolution of carbon dioxide, and a liquid distilled over which slowly solidified. It crystallised from a mixture of benzene and ligroin in flat needles which melted at 59°, and analysis showed it to be benzo-y-pyrone. The yellowish solution of benzo-y-pyrone in concentrated sulphuric acid possesses a violet fluorescence. 14. On the Combination of Thiophenol and Guaiacol with the Esters of the Acids of the Acetylene Series. By Dr. S. RuneMaAnn and H. E. Srapteton, B.A. (Oxon.) In this paper an account is given of the continvation of previous work on the combination of phenols with the esters of the acetylene acids. The authors were induced to study the action of thiophenol on these esters in the hope of finding a new method of preparing thioacetophenone, whilst the investigation of guaiacol was taken up, as no derivative of a dihydric phenol had previously been worked with. During the progress of the research various new derivatives of thiophenyl- cinnamic, fumaric, and succinic acids were discovered, but it was found that thiophenyl styrene : C,H,;.C = CH, S.C,H, ‘on boiling with dilute mineral acids is decomposed into acetophenone and hiophenol, and not into thioacetophenone and phenol, as had been expected. Guaiacol was found to combine readily with phenyl propiolic ester; guaiacolyl cinnamic acid and its ester were prepared, and it was found that the acid on heating quantitatively decomposed into carbon dioxide and guaiacolyl styrene— C,H, .C=CH, | 0. C,H, 0.CH, From the latter mineral acids regenerated guaiacol, with the additional formation of acetophenone. 15. Chlorination of Aromatic Hydrocarbons. By H. D. Dasin,and J. B. Couzn, Ph.D. —v ene, se ar TUESDAY, SEPTEMBER 11. The Section was divided into two Departments. The following Papers were read ;— DEPARTMENT I. 1. On some Recent Work on thé Difusion of Gases and Liquids, By Horace T. Brown, 2.8, TRANSACTIONS OF SECTION B. 705 9. On Recent Developments in the Textile Industries. By Dr. A. Lirpmann. 3. Influence of Pressure on the Formation of Oceanie Salt Deposits. By H.M. Dawson, Ph.D., B.Sc. The preseut paper forms one of a series of investigations carried out with a view of obtaining information in regard to the conditions of formation of the Stassfurt deposits. . ‘4 F In previous papers (van’t Hoff and pupils) the isothermal equilibrium relation- ships of salts occurring in sea-water and the influence of temperature on these has been investigated. This paper deals with the influence of pressure. One of the last phases of salt deposition in the Stassfurt layer is represented by tachhydrite (CaCi, 2MgCl, 12H,O); experiment shows that this separates from solutions of the mixed chloride of Ca and Mg if the temperature exceeds 22°4 C. Below 22°4 C. a mixture of the simple salts separates, but no tachhydrite. If the mixed chlorides be heated in the solid condition, then at 22°4 C, water is split off and tachhydrite is formed. The influence of pressure on the temperature of formation of this double salt has been studied. Careful determinations by the thermometric method show that under atmo- spheric pressure this temperature is 22°-400 C. By means of the manokryometer the temperature of formation under higher pressures was determined. The mean result of this direct determination of the influence of pressure is that for an increase of 100 atmospheres the temperature of formation is raised 1°62 C. Another and indirect determination is possible by applying the formula of Thomson for the influence of pressure on the melting point to the transition temperature at which calcium chloride, magnesium chloride, tachhydrite, and saturated solution are in equilibrium. Trom the formula in question, yiz., dT _ 10333 (v,—%,) dp 42500 gq’ the determination of av only involves the knowledge of the change of volume ard #) y 8 § the heat change accompanying the reaction, which takes place according to CMgCl,6H,O + 1:188CaCl,6H,O _—-—" vy, Saturated Solution. — °262CaC1,2MeC1,-12H,0 + °101(100H1,0 9:27 CaCl, 4:92 MgCl,) + ¢ Cals. ——_—__—__—_ ne Vg The estimation of (v,—v,) and of g from a series of experiments and substitu- tion in the thermodynamic formula gives for a the value ‘0135° C, In other words, 160 atmospheres would raise the temperature of formation 1°-35 C, Both results show that the influence of pressure on the separation of salts from solution is very small in comparison with the influence of temperature. On thermodynamic grounds it can be shown that the influence of pressure on temperature displacement in the case of other salts must be of the same order of magnitude as that found in the case of tachhydrite. The fact that certain Stassturt salts (e.g., Kieserte, Kainite, Liwéite and Langbeinite) are not deposited on’ evaporation of sea-water at a constant 1900. ZZ 706 REPORT—1900. temperature of 25° C. cannot be attributed to the influence of the pressure which has existed during the natural salt deposition, but must be accounted for by the prevalence of higher temperatures. The presence of these salts in the Stassfurt layer enables us, in fact, to draw conclusions in regard to the tempera- tures which existed during the salt deposition. 4. On the Sensitiveness of Metallic Silver to Light. By Major-General J. Warernousse, J.5.C. The paper is a continuation of that read before the Royal Society on May 31, and contains an account of further experiments on the production of visible photographic images upon plain silver surfaces by the action of solar radiations. The author has found that such visible images are formed when pure silver foils or silvered glass are exposed to sunlight in exhausted glass tubes, and, apparently, more readily in the presence of watery vapour. Invisible, but develop- able, images were readily obtained in exhausted tubes in which no signs of the presence of moisture were apparent. By prolonged exposure a visible change also takes place. When thin films of silver on glass have been fully exposed in sunlight the action has been found to penetrate the film and produce a distinctly visible image at the back as well as on the face, the exposed parts appearing always lighter than the unexposed, Fresh experiments with silver plates used as anode and cathode in a decom- position cell containing distilled water, through which a weak current was allowed to pass, showed that the pale grey deposit on the cathode and the dark olive yellow coating on the anode were both quite sensitive to light, and appeared lighter by exposure, in a manner somewhat analogous to that observed on silvered glass or plain silver foils exposed to light. It was noticed that the visible images were not dissolved away either by the usual photographic fixing agents or by dilute nitric acid. A very curious action of light upon glass has also been observed. In this case a silvered glass plate was exposed for about a month under a cut-out screen of thin aluminium, the unsilvered side of the glass being in contact with the aluminium and not protected from the air by a covering glass plate. After exposure the plate was put aside for a few days with the exposed glass side in contact with the silvered surface of another piece of polished silvered glass, which was then found to have received an impressed image from the glass of the design cut out of the aluminium screen. ‘lhe image was quite visible, clear and sharp, and somewhat similar to the images directly impressed by light, though it had not the same appearance of being bleached out, when examined by retlected light. Several days afterwards a second similar image was produced in the same way by contact with the glass upon another freshly polished silvered glass plate, and no doubt several more could be produced in the same way. These new experiments seem to show that the images formed by the action of light upon plain silver surfaces are due more to molecular or physical changes than to chemical decomposition, though the latter may also probably come into play in the presence of watery vapour, or other conditions favouring oxidation and reduction of the metallic surface. ‘The author is continuing the investigation. 5. Some Thoughts on Atomic Weights and the Periodic Law. By J. H. Guapsrone, D.Sc., 2... and GEorGE GLADSTONE, The object of this paper was to recall attention to a suggestion made during the discussion of a paper by Professor Dumas at the meeting of the Association at Ipswich in 1851, viz., that the case of‘ triads’ of analogous elements showed a resemblance to the progression in a series of organic compounds, and might be due to a similar cause. It was shown that the difference in atomic weight between the horizontal lines in Mendeljeff’s arrangement is in the first instance 16, which afterwards er eC TRANSACTIONS OF SECTION B, 707 changes to about 20, and ultimately to about 24. But this increment is really arrived at by 8 steps, giving in the first instance an average of 2-0 for each element ; in point of fact, however, the increments are not regular, being for the first line, and starting with lithium, 2'1, 1:9, 1-0, 2-0, 2:0, 3:0, and then 4:0 for two steps, the intermediate one being unknown. ‘This departure from regularity in the increment seems to show that it is of a compound nature; that the original substance may run through the whole series, but be modified by small quantities of one or more additional substances. This would seem to explain not only the slight irregularities, but how our place in Mendeljeft’s arrangement may be occupied by two or more elements which closely resemble one another, but differ very slightly in atomic weight or in other properties, such as the iron group, the plati- num group, the two didymiums, and the metals associated with yttrium. On this supposition the elements having high atomic weights may be expected to be less regular than is the case in the earlier part of the series. 6. The Heating and Lighting Power of Coal Gas. By T. Fatrury, LARS. LLC, The author pointed out the importance of knowing the heating power of gas as well as the lighting power, now that it is so largely used for heating and engine purposes. Coal gas is a complex mixture consisting chiefly of marsh gas and hydrogen with small quantities of heavy hydrocarbons, oxides of carbon, aqueous vapour, nitrogen, &c. The first two control mainly the heating value, and the heavy hydrocarbons the lighting value in ordinary burners. Incandescent g¢as-burners are not considered in this paper. That heavy hydrocarbon vapours raise the lighting more than the heating power, explains why carburetted water-gas has a less heating value than ordinary coal-gas of the same lighting power. Air or nitrogen drawn into gas lowers the lighting power more than the heating power. In gas made from one kind of coal the calorimeter may be worked constantly so as to watch the gas in place of the jet photometer. The author referred to the various calorimeters invented, and gave directions _ for securing accuracy. Finally he gave a table of average resuits showing the heating power of gas of different lighting power. Lighting power, Heating power. Pounds | Lighting power, Heating Power. Pounds Standard candles. of water heated 19°F. | Standard candles. of water heated 1° F. by 1 cubic foot of gas. by 1 cubic foot of gas. 11 533 / 15 624 12 555 16 648 13 578 17 676 14 tol 18 704 7. On Smoke. By J. B. Conen, Ph.D. Department II. 1. Bradford Sewage and its Treatment. By F. W. Ricuarpson, F.1.C., the Bradford City Analyst. ___ In times of normal trade over twenty tons of wool-grease come every weekday into the city’s sewers. Wool-suds and effluents, in addition to grease, contain enormous amounts of nitrogenous impurities; thus it is that Bradford sewage is one of the very worst sewages in the kingdom. Of the daily dry-weather flow of twelve million gallons of sewage one and a quarter millions consist of woolcombers ZZ2 708 REPORT—1900. suds and effluents and two millions of dyeworks effluents, with over half a million gallons from Messrs. Lister’s, of Manningham Mills. From experiments upon bulks of 20,000 gallons, a mixture of one part of wool-suds and seven parts of Bradford Sunday sewage requires nine times as much precipitant, and produces ten times as much wet and twelve and a half times as much settled sludge, as the Sunday sewage alone. A number of the woolcombers recover part of the wool- grease by ‘cracking’ the crude suds with oil of vitriol. The effluent so obtained is very acid, contains from 100 to 200 grains of grease per gallon, with a very large amount of nitrogenous impurities. he difliculties arising from the pre- sence of the wool-suds and effluents are twofold: (1) The peculiar emulsive character of wool-grease; (2) the excessive amount of nitrogenous impurities, With Bradford sewage have been tried :— (1) Lime, giving a clear but bad effluent with a large amount of sludge. (2) Copperas, followed by lime, producing a turbid but better effluent. (3) Alumina-ferric, z.c., alumina sulphate, giving unsatisfactory results at a high cost. (4) Acid ferric sulphate, giving a high degree of purification, but with an acid effluent. (5) Neutral ferric sulphate, yielding as good results, but with less acidity. (6) Basic ferric sulphate, giving a 62 per cent. purification and a neutral or slightly alkaline effluent.' The basic sulphate is made at the sewage works by McCulloch's Patent. As it a necessary to use a considerable weight of the basic salt, the method proves costly. The author has fully investigated the biology of Bradford sewage, and has tried different methods of bacterial treatment. It has not been very difficult to get nitrification with as high a purification in extreme cases as 70 per cent. The grease present to the extent of 40 to 50 grains per gallon very soon chokes up the filters. There can be no doubt that if the woolcombers’ suds and effluents were entirely removed the whole of the city’s sewage could be treated biologically, with an immense saving in the cost of chemicals and the treatment of the sludge. Failing the elimination of the wool-suds the best method would seem to be a preliminary treatment with the cheapest precipitant obtainable and the biological purification of the effluent, either on bacteria beds or on land, preferably on both. Several patentecs have experimented on Bradford sewage, but hitherto with unsatisfactory results, and they have all retired from the attempt, saying that the grease baffled them. After describing the chemical and biological methods in detail, the author entered at some length into the scientific causes of the difficulties of treatment. 2. On the Treatment of Woolcombers’ Effluents. By W. Leacu. 3. On a Simple and Accurate Method for estimating the Dissolved Oxygen in Fresh Water, Sea Water, Sewage Effuents, &c. By Professor Lrrrs, D.Sc. PhD. &e., and R. F. Buaxe, LLC., F.C.8., Queen’s College, Belfast. After criticising the existing methods for determining the dissolved oxygen in water volumetrically, the authors describe a very simple and accurate method for the purpose, of which the following is an outline: An ordinary separating funnel is filled with the water to be examined, and a measured volume withdrawn. A definite volume of standard ferrous sulphate solution is then added, and afterwards ammonia—the volume of these two reagents ' This effluent, after passing at a rapid rate through fine breeze beds, gives an additional 9 per cent. of purification, although no nitrification occurs. : , TRANSAGTIONS OF SECTION B. - AQG together corresponding with that of the water removed—and the stopper of the funnel is then inserted, care being taken that no air bubbles are enclosed. Within the separating funnel there is now a layer of ferrous sulphate below, next the water, and abcve all the ammonia. hese are mixed by inverting the vessel once or twice by a swinging motion, when a greenish turbid mixture results, which rapidly darkens as the dissolved oxygen is absorbed. After fifteen minutes the vessel (still stoppered) is inverted, and its tube or lower extremity (now, how- ever, the upper one) is nearly filled with a mixture of equal volumes of sulphuric acid and water. The tap is then opened, when the acid flows downwards into the alkaline mixture, and in the course of a few minutes dissolves the iron hydrates, forming a clear solution. This is then run off into a porcelain dish, and there titrated, either with permanganate or bichromate, conveniently of the strength lec. =1 cc. of dissolved oxygen at N.T.P. In the authors’ experiment the separating funnel had a capacity of 382°5 ¢.c., practically 4 litre; and its tube contained, when nearly full, about 8 cc. of diluted sulphuric acid. About 7 c.c. of the water was removed, 5c.c. of standard ferrous sulphate solution added and about 2c.c. of strong ammonia. The ferrous sulphate solution contained about 12 crams of the crystallised salt in 250c.c. of distilled water.- It was standardised for each determination by titrating 5c.c. in a porcelain basin, mixed with the same volume of the water under examination as employed in the dissolved oxygen determination and the same volume of acid. For all practical purposes the dissolved oxygen contained in the volume of water which the separating funnel holds amounts to the difference between the burette readings for the blank experiment and for the actual determination, The following are a few typical results :— Dissolved Oxygen per litre eerie f fluid Liquid Analysed pee Peas. Difference Found True Amount Distilled water saturated | Permanganate | 7:26 7:20 (Roscoe and | + 0°06 with air at 15°-7. Lunt). Belfast water — Town 6h 5°80 5:75 (Gasometric + 0:05 supply. | analysis). | Seawater from Belfast ” | 5-53 +043 Lough. \ 5:10 (Gasometric | f +48 Seawater from Uelfast | Bichromate ; analysis). d Loweh | 510, L000 Sewage effluent from | Permanganate| ,., - re ‘ Bacteria Beds.’ ee {| 0°36 (Gasometric f sige Sewage effluent from | Bichromate WO analysis). ; ‘Bacteria Beds,’ ne J | eas It will be seen that for sea water and sewage effluents bichromate gives more accurate results than permanganate, 4, The Utilisation of Sewage Sludge. By Professor W. B. Borromtey, M_A., Ph.D., King’s College, London. No one system of sewage treatment is universally applicable. Local conditions must determine which system is best for any locality. Parliamentary returns in 1894 gave 233 sanitary districts in England and Wales where systems for treating sewage by precipitation were in operation. In most cases the sludge was not only valueless, but a nuisance. The author experimented with specially prepared sewage sludge, enriched by the use of phosphatic material in treating the sewage. A crude phosphatic rock was treated with sulphuric acid slightly in excess of the amount necessary to combine with the oxides of iron and aluminium present ; the resultant substance 710 -REPORT—1900. —spoken of as Phosalite—was usel as a precipitating agent for sewage, and as a pressing agent for sewage sludge. Experiments at Chiswick Sewage Works, where Phosalite was used as a precipitating agent, yielded in the dried sludge cake :-— Nitrogen=Ammonia , . 1-44 Phosphate of Lime . . 6:21 When used as a pressing agent in conjunction with half the usual amount of lime, the dried sludge cake yielded :— Nitrogen=Ammonia . . 1°04 Phosphate of Lime . . 12:06 Experiments at Glascow Sewage Works with Phosalite as a pressing agent gave the following results :— a. Sludge pressed with } per cent. of lime and 1 per cent. of Phosalite:— Nitrogen=Ammonia . 2 v4 Phosphate of Lime , yg? Oars b. Sludge pressed with 3 per cent. of lime and 2 per cent. of Phosalite :— Nitrogen=Ammonia , . 2°04 Phosphate of Lime . . 9:49 By the use of Phosalite as a pressing agent for sludge there was obtained— (a) an economy of lime necessary for pressing ; (b) a much-improved press liquor ; (c) a greatly enhanced manurial value for the sludge. These specially enriched sludges, when dried and ground, formed excellent manures, giving results equal to those produced by many high-priced artificial manures. The experiments show that for the effective utilisation of sewage sludge as a manure there are two requisites :— 1. The use of some such phosphatic material as Phosalite when pressing the sludge. 2. The resultant sludge-cake must then be dried and ground, so that it may easily mix with the soil. TRANSACTIONS OF SECTION C. 711 Srction C.—GEOLOGY. PRESIDENT of THE SECTION—Professor W, J. Sottas, D.Sc,, LL.D., F.RS THURSDAY, SEPTEMBER 6. The President delivered the following Address :— Evolutional Geology. Tux close of one century, the dawn of another, may naturally suggest some brief retrospective glance over the path along which our science has advanced, and some general survey of its present position from which we may gather hope of its future progress; but other connection with geology the beginnings and end- ings of centuries have none. The great periods of movement have hitherto begun, as it were, in the early twilight hours, long before the dawn. Thus the first step forward, since which there has been no retreat, was taken by Steno in the year 1669 ; more than a century elapsed before James Hutton (1785) gave fresh energy and better direction to the faltering steps of the young science; while it was less than a century later (1863) when Lord Kelvin brought to its aid the powers of the higher mathematics and instructed it in the teachings of modern physics. From Steno onward the spirit of geology was catastrophic; from Hutton onward it grew increasingly uniformitarian; {rom the time of Darwin and Kelvin it has become evolutional. The ambiguity of the word ‘uniformitarian’ has led toa good deal of fruitless logomachy, against which it may be as well at once to guard by indicating the sense in which it is used here In one way we are all uniformi- tarians, 7.e., we accept the doctrine of the ‘ uniform action of natural causes,’ but, as applied to geology, uniformity means more than this. Defined in the briefest fashion it is the geology of Lyell. Hutton had given us a ‘Theory of the Earth,’ in its main outlines still faithful and true ; and this Lyell spent his life in illustrating and advocating ; but as so commonly happens the zeal of the disciple outran the wisdom of the master, and mere opinions were insisted on as necessary dogma. What did it matter if Hutton asa result of his inquiries into terrestrial history had declared that he found no vestige of a beginning, no prospect of an end? It would have been marvellous if he had! Consider that when Hutton’s ‘Theory’ was published William Smith’s famous discovery had not been made, and that nothing was then known of the orderly succession of forms of life, which it is one of the triumphs of geology to have revealed; consider, too, the existing state of physics at the time, and that the modern theories of energy had still to be for- mulated; consider also that spectroscopy had not yet lent its aid to astronomy and the consequent ignorance of the nature of nebulz ; and then, if you will, cast a stone at Hutton. With Lyell, however, the case was different : in pressing his uniformitarian creed upon geology he omitted to take into account the great 712 REPORT—1900. advances made by its sister sciences, although he had knowledge of them, and thus sinned against the light. In the last edition of the famous ‘ Principles’ we read; ‘Itis a favourite dogma of some physicists that not only the earth, but the sun itself, is continually losing a portion of its heat, and that as there is no known source by which it can be restored we can foresee the time when all life will cease to exist on this planet, and on the other hand we can look back to a period when the heat was so intense as to be incompatible with the existence of any organic beings such as are known to us in the living or fossil world. . . . A geologist in search of some renovating power by which the amount of heat may be made to continue unimpaired for millions of years, past and future, in the solid parts of the earth . . . has been compared by an eminent physicist to one who dreams he can discover a source of perpetual motion and invent a clock with a self-winding apparatus. But why should we despair of detecting proofs of such regenerating and self-sustaining power in the works of a Divine Artificer ?’ Here we catch the true spirit of uniformity ; it admittedly regards the universe as a self-winding clock, and barely conceals a conviction that the clock was warranted to keep true Greenwich time. The law of the dissipation of energy is not a dogma, but a doctrine drawn from observation, while the uniformity of Lyell is in no sense an induction : it is a dogma in the narrowest sense of the word, unproved, incapable of proof ; hence perhaps its power upon the human mind; hence also the transi- toriness of that power. Again, it is only by restricting its inquiries to the stratified rocks of our planet that the dogma of uniformity can be maintained with any pretence of argument. Directly we begin to search the heavens the possibility, nay even the likelihood, of the nebular origin of our system, with all that it involves, is borne in upon us. Lyell therefore consistently refused to extend his gaze beyond the rocks beneath his feet, and was thus led to do a serious injury to our science: he severed it from cosmogony, for which he entertained and expressed the most profound contempt, and from the mutilation thus inflicted geology is only at length making a slow and painful recovery. Why do I dwell on these facts? To depreciate Lyell? By no means. No one is more conscious than I of the noble service which Lyell rendered to our cause: his reputation is of too robust a kind to suffer from my unskilful handling, and the fame of his solid contributions to science will endure long after these controversies are forgotten. The echoes of the combat are already dying away, and uniformitarians, in the sense already defined, are now no more; indeed, were I to attempt to exhibit any distinguished living geologist as a still surviving supporter of the narrow Lyellian creed, he would probably feel, if such a one there be, that I was unfairly singling him out for unmerited obloquy. Our science has become evolutional, and in the transformation has grown more comprehensive: her petty parochial days are done, she is drawing her pro- vinces closer around her, and is fusing them together into a united and single com- monwealth—the science of the earth. Not merely the earth's crust, but the whole of earth-knowledge is the sub- ject of our research. To know all that can be known about our planet, this, and nothing less than this, is its alm and scope. From the morphological side geology inquires not only into the existing form and structure of the earth, but also into the series of successive morphological states through which it has passed in a long and changeful development. Our science inquires also into the distribution of the earth in time and space; on the physiological side it studies the movements and activities of our planet; and not content with all this it extends its researches into etiology and endeavours to arrive ata science of causation. In these pursuits geology calls all the other sciences to her aid. In our commonwealth there are no outlanders ; if an eminent physicist enter our territory we do not begin at once to prepare for war, because the very fact of his undertaking a geological inquiry of itself confers upon him all the duties and privileges of citizenship. A physicist studying geology is by definition a geologist. Our only regret is, not that physi- cists occasionally invade our borders, but that they do not yisit us oftener and make closer acquaintance with us, TRANSACTIONS OF SECTION C. 713 Early History of the Earth: First Critical Period. If I am bold enough to assert that cosmogony is no longer alien to geology, I may proceed further, and taking advantage of my temerity pass on to speak of things once not permitted to us. I propose therefore to offer some short account of the early stages in the history of the earth. Into its nebular origin we need not inquire—that is a subject for astronomers. We are content to accept the infant earth from their hands as a molten globe ready made, its birth from a gaseous nebula duly certified. If we ask, as a matier of curiosity, what was the origin of the nebula, I fear even astronomers cannot tell us. There is an hypothesis which refers it to the clashing of meteorites, but in the form in which this is usually presented it does not help us much. Such meteorites as have been observed to penetrate our atmosphere and to fall on to the surface of the earth prove on examination to have had an eventful history of their own of which not the least important chapter was a passage through a molten state; they would thus appear to be the products rather than the progenitors of a nebula. We commence our history then with a rapidly rotating molten planet, not impossibly already solidified about the centre and surrounded by an atmosphere of great depth the larger part of which was contributed by the water of our present oceans, then existing in a state of gas. This atmosphere, which exerted a pressure of something like 5,000 lb. to the square inch, must have played a very important part in the evolution of our planet. The molten exterior absorbed it to an extent which depended on the pressure, and which may some day be learnt from experiment. Under the influence of the rapid rotation of the earth the atmosphere would be much deeper in equatorial than polar regions, so that in the latter the loss of heat by radiation would be inexcess. This might of itself lead to convectional currents in the molten ocean. The effect on the atmo- sphere is very difficult to trace, but it is obvious that if a high-pressure area originated over some cooler region of the ocean, the winds blowing out of it would drive before them the cooler superticial layers of molten material, and as these were replaced by hotter lava streaming from below, the tendency would be to convert the high into a low pressure area, and to reverse the direction of the winds. Conversely under a low-pressure area the in-blowing winds would drive in the cooler superficial layers of molten matter that had been swept away from the anticyclones. If the difference in pressure under the cyclonic and anti- cyclonic areas were considerable, some of the gas absorbed under the anticyclones might escape beneath the cyclones, and in a later stage of cooling might give rise to vast floating islands of scoria. Such islands might be the first foreshadowings of the future continents. Whatever the ultimate effect of the reaction of the winds on the currents of the molten ocean, it is probable that some kind of circulation was set up in the latter. The universal molten ocean was by no means homogeneous: it was constantly undergoing changes in composition as it reacted chemically with the internal metallic nucleus: its currents would streak the different portions out in directions which in the northern hemisphere would run from N.E. to S.W., and thus the differences which distinguish particular petrological regions of our planet may have commenced their existence at a very early stage. Is it possible that as our knowledge extends we shall be able by a study of the distribution of igneous rocks and minerals to draw some conclusions as to the direction of these hypothetical lava currents? Our planet was pro- foundly disturbed by tides, produced by the sun; for as yet there was no moon; and it has been suggested that one of its tidal waves rose to a height so great as to sever its connection with the earth and to fly off as the infant moon. This event may be regarded as marking the first critical period, or catastrophe if we please, in the history of our planet. The career of our satellite, after its escape from the earth, is not known till it attained a distance of nine terrestrial radii; after this its progress can be clearly followed. At the eventful time of parturition the earth was rotating, with a period of from two to four hours, about an axis inclined at some 11° or 12° to the ecliptic, The time which has elapsed 714, REPORT—1900. since the moon occupied a position nine terrestrial radii distant from the earth is at least fifty-six to fifty-seven millions of years, but may have been much more. Professor Darwin’s story of the moon is certainly one of the most beautiful contributions ever made by astronomy to geology, and we shall all concur with him when he says, ‘ A theory reposing on vere cause, which brings into quanti- tative correlation the length of the present day and month, the obliquity of the ecliptic, and the inclination and eccentricity of the lunar orbit, must, I think, have strong claims to acceptance.’ The majority of geologists have long hankered after a metallic nucleus for the earth, composed chietly, by analogy with meteorites, of iron. Lord Kelvin has admitted the probable existence of some such nucleus, and lately Professor Wiechert has furnished us with arguments— powerful’ arguments Professor Darwin terms them—in support of its existence. The interior of the earth for four fifths of the radius is composed, according to Professor Wiechert, chiefly of metallic iron, with a density of 82; the outer envelope, one fifth of the radius, or about 400 miles in thickness, consists of silicates, such as we are familiar with in igneous rocks and meteorites, and possesses a density of 3:2. It was from this outer envelope when molten that the moon was trundled off, twenty-seven miles in depth going to its formation. The density of this material, as we have just seen, is supposed to be 3:2; the density of the moon is 3:39, a close approximation, such difference as exists being completely explicable by the comparatively low temperature of the moon. The outer envelope of the earth which was drawn off to form the moon was, as we have seen, charged with steam and other gases under a pressure of 5,000 Ib. to the square inch; but as the satellite wandered away from the parent planet this pressure continuously diminished. Under these circumstances the moon would become as explosive as a charged bomb, steam would burst forth from numberless volcanoes, and while the face of the moon might thus have ac- quired its existing features the ejected material might possibly have been shot so far away from its origin as to have acquired an independent orbit. If so we may ask whether it may not be possible that the meteorites, which sometimes descend upon our planet, are but portions of its own envelope returning to it. The facts that the average specific gravity of those meteorites which have been seen to fall is not much above 3:2, and that they have passed through a state of fusion, are consistent with this suggestion. Second Critical Period. ‘ Consistentior Status.’ The solidification of the earth probably became completed soon after the birth of the moon. The temperature of its surface at the time of consolidation was about 1170° C., and it was therefore still surrounded by its primitive deep atmosphere of steam and other gases. This was the second critical period in the history of the earth, the stage of the ‘consistentior status, the date of which Lord Kelvin would rather know than that of the Norman Conquest, though he thinks it lies between twenty and forty millions of years ago, probably nearer twenty than forty. Now that the crust was solid there was less reason why movements of the atmosphere should be unsteady, and definite regions of high and low pressure might have been established. Under the high-pressure areas the surface of the crust would be depressed ; correspondingly under the low-pressure areas it would be raised; and thus from the first the surface of the solid earth might be dimpled and embossed.? Third Critical Period. Origin of the Oceans. The cooling of the earth would continuously progress, till the temperature of the surface fell to 370° C., when that part of the atmosphere which consisted of steam would begin to liquefy; then the dimples on the surface would soon 1 It would be difficult to discuss with sufficient brevity the probable distribution - of these inequalities, but it may be pointed out that the moon is possibly responsible, and that in more ways than one, for much of the existing geographical asymmetry. TRANSACTIONS OF SECTION C. PB, become filled with superheated water, and the pools so formed would expand and deepen, till they formed the oceans. This is the third critical stage in the history of the earth, dating, according to Professor Joly, from betweeneighty and ninety millions of years ago. With the growth of the oceans the distinction between land and sea arose—in what precise manner we may proceed to inquire. If we revert to the period of the ‘consistentior status,’ when the earth had just solidified, we shall find, according to Lord Kelvin, that the temperature continuously increased from the surface, where it was 1170° C., down to a depth of twenty-five miles, where it was about 1430°C., or 260° C. above the fusion point of the matter forming the crust. That the crust at this depth was not molten but solid is to be explained by the very great pressure to which it was subjected—just so much pressure, indeed, as was required to counteract the influence of the additional 260° C. Thus if we could have reduced the pressure on the crust we should have caused it to liquefy ; by restoring the pressure it would resolidify. By the time the earth’s surface had cooled down to 370°C. the depth beneath the surface at which the pressure just kept the crust solid would have sunk some slight distance inwards, but not sufficiently to affect our argument. The average pressure of the primitive atmosphere upon the crust can readily be calculated by supposing the water of the existing oceans to be uniformly distributed over the earth’s surface, and then by a simple piece of arithmetic determining its depth: this is found to be 1:718 miles, the average depth of the oceans being taken at 2°393 miles. Thus the average pressure over the earth's surface, immediately before the formation of the oceans, was equivalent to that of a column of water 1:718 miles high on each square inch. Supposing that at its origin the ocean were all ‘ gathered together into one place,’ and ‘the dry land appeared,’ then the pressure over the ocean floor would be increased from 1:718 miles to 2°393 miles, while that over those portions of the crust that now formed the land would be diminished by 1°718 miles, This difference in pressure would tend to exaggerate those faint depressions which had arisen under the primitive anti- cyclonic areas, and if the just solidified material of the earth’s crust were set into a state of flow it might move from under the ocean into the bulgings which were rising to form the land, until static equilibrium were established. Under these circumstances the pressure of the ocean would be just able to maintain a column of rock 0'886 mile in height, or ten twenty-sevenths of its own depth. It could do no more ; but in order that the dry land may appear some cause must be found com- petent either to lower the ocean bed the remaining seventeen twenty-sevenths of its full depth or to raise the continental bulgings to the same extent. Such acause may, I think, be discovered in a further eflect of the reduction in pressure over the con- tinental areas. Previous to the condensation of the ocean these, as we have seen, were subjected to an atmospheric pressure equal to that of a column of water 1718 miles in height. This pressure was contributory to that which caused the outer twenty-five miles of the earth’s crust to become solid; it furnished indeed just about one fortieth of that pressure, or enough to raise the fusion point 6°C. What then might be expected to happen when the continental area was relieved of this load? Plainly a liquefaction and corresponding expansion of the underlying rock. But we will not go so far as to assert that actual liquefaction would result ; all we require for our explanation is a great expansion; and this would probably follow whether the crust were liquefied or not. For there is good reason to suppose that when matter at a temperature above its ordinary fusion point: is compelled into the solid state by pressure, its volume is very responsive to changes either of pressure or temperature. The remarkable expansion of liquid carbon dioxide is a case in point: 120 volumes of this fluid at —20° C. become 150 volumes at 33°C.; a temperature just below the critical point. A great change of volume also occurs when the material of igneous rocks passes from the crystalline state to that of glass; in the case of diabase ! the difference in volume of the rock in the two 1 C. Barus so names the material on which he experimented ; apparently the rock is a fresh dolerite without olivine. 716 REPORT—1900. states at ordinary temperatures is 13 per cent. If the relief of pressure over the site of continents were accompanied by volume changes at all approaching this, the additional elevation of seventeen twenty-sevenths required to raise the land to the sea-level would be accounted for.! How far down beneath the surface the unloading of the continents would be felt is difficult to say, though the problem is probably not beyond the reach of mathematical analysis; if it affected an outer envelope twenty-five miles in thickness, a linear expansion of 6 per cent. would suffice to explain the origin of ocean basins. If now we refer to the dilatation determined by Carl Barus for rise in temperature in the case of diabase, we find that between 1093° and 1112°C. the increase in volume is 3'3 per cent. As a further factor in deepening the ocean basins may be included the compressive effect of the increase in load over the ocean floor: this increase is equal to the pressure of a column of water 0-675 mile in height, and its effect in raising the fusion point would be 2° C., from which we may gain some kind of idea of the amount of compression it might produce on the yielding interior of the crust. To admit that these views are speculative will be to confess nothing; but they certainly account for a good deal. They not only give us ocean basins, but basins of the kind we want, that is, to use a crude comparison once made by the late Dr. Carpenter, basins of a tea-tray form, having a somewhat flat floor and steeply sloping sides ; they also help to explain how it is that the value of gravity is greater over the ocean than over the land. The ocean when first formed would consist of highly heated water, and this, as is well known, is an energetic chemical reagent when brought into contact with silicates like those which formed the primitive crust. As a result of its action saline solutions and chemical deposits would be formed; the latter, however, would probably be of no great thickness, for the time occupied by the ocean in cooling to a temperature not far removed from the present would probably be included within a few hundreds of years. The Stratified Series. The course of events now becomes somewhat obscure, but sooner or later the familiar processes of denudation and the deposition started into activity, and have continued acting uninterruptedly ever since. The total maximum thickness of * Professor Fitzgerald has been kind enough to express part of the preceding explanation in a more precise manner for me. He writes: ‘It would require a very nice adjustment of temperatures and pressures to work out in the simple way you state it ; but what is really involved is that in a certain state diabase (and everything that changes state with a considerable change of volume) has an enormous isothermal compressibility. Although this is very enormous in the case of bodies which melt suddenly, like ice, it would also involve very great compressibilities in the case of bodies even which melted gradually, if they did so at all quickly, i.¢., within a small range of temperature. What you postulate, then, is that ata certain depth diabase is soft enough to be squeezed from under the oceans, and that, being near its melting point, the small relief of pressure is accompanied by an enormous increase in volume which helped to raise the continents. Now that I have written the thing out in my own way it seems very likely. It is, anyway, a suggestion quite worthy cf serious consideration, and a process that in some places must almost certainly have been in operation, and maybe is still operative. Looking at it again, I hardly think it is quite likely that there is or could be much squeezing sideways of liquid or other viscous material from under one place to another, because the elastic yielding of the inside of the earth would be much quicker than any flow of this kind. This would only modify your theory, because the diabase that expands so much on the relief of pressure might be that already under the land, and raising up this latter, partly by being pushed up itself by the elastic relief of the inside of the earth and partly by its own enormous expansibility near its melting point. The action would be quite slow, because it would cool itself so much by its expansion that it would have to be warmed up from below, or by tidal earth-squeezing, or by chemical action before it could expand isothermally,’ TRANSACTIONS OF SECTION C. 717 the sedimentary deposits, so far as I can discover, appears to amount to no less than 50 miles, made up as follows :— Feet Recent and Pleistocene 4 . 4,000 ; . Man. Pliocene F : : 5,000 ; . Pithecanthropus. Miocene " . : 4 . 9,000 Oligocene . : : 7 « 12,000 . 5 Eocene. 3 3 , F . 12,000 é . Hutheria, Cretaceous . - 4 4 . 14,000 : : Jurassic F : ‘ F . 8,000 : Trias. ; C ‘ - . 13,000 ; . Mammals, Permian - ; : . 12,000 3 . Reptiles. Carboniferous . = , . 24,000 : . Amphibia, Devonian . : 3 - . 22,000 ‘ . Fish. Silurian s ‘: i . 15,000 Ordovician . - 5 : . 17,000 : 5 Cambrian . c . 5 . 16,000 5 . Invertebrata, Keweenawan 5 4 : . 50,000 Penokee ‘ 3 é 3 . 14,000 Huronian . : : < - 18,000 Geologists, impressed with the tardy pace at which sediments appear to be accumulating at the present day, could not contemplate this colossal pile of strata without feeling that it spoke of an almost inconceivably long lapse of time. They were led to compare its duration with the distances which intervene between the heavenly bodies; but while some chose the distance of the nearest fixed star as their unit, others were content to measure the years in terms of miles from the sun. Evolution of Organisms. The stratified rocks were eloquent of time, and not to the geologist alone, they appealed with equal force to the biologist. Accepting Darwin’s explanation of the origin of species, the present rate at which form flows to form seemed so slow as almost to amount to immutability. Jlow vast then must have been the period during which by s!ow degrees and innumerable stages the protozoon was transformed into the man! And if we turn to the stratified column, what do we find? Man, it is true, at the summit, the oldest fossiliferous rocks 34 miles lower down, and the fossils they contain already representing most of the great classes of the Invertebrata, including Crustacea and Worms. Thus the evolution of the Vertebrata alone is known to have occupied a period represented by a thickness of 34 miles of sediment. How much greater, then, must have been the interval required for the elaboration of the whole organic world! The human mind, dwelling on such considerations as these, seems at times to have been affected by a sur-excitation of the imagination, and a consequent paralysis of the understanding, which led to a refusal to measure geological time by years at all, or to reckon by anything less than ‘ eternities.’ Geologic Periods of Time. After the admirable Address of your President last year it might be thought neediess for me to again enter into a consideration of this subject; it has been said, however, that the question of geological time is like the Djin in Arabian tales, and will irrepressibly come up again for discussion, however often it is disposed of. For my part I do not regard the question so despondingly, but rather hope that by persevering effort we may succeed in discovering the talisman by which we may compel the unwilling Djin into our service. How immeasurable would be the advance of our science could we but bring the chief events which it records into some relation with a standard of time! Before proceeding to the discussion of estimates of time drawn from a study of stratified rocks let us first consider those which have been already suggested by other dati. These are as follows:—(1) Time which has elapsed since the 718 REPORT—1900. separation of the earth and moon, fifty-six millions of years, minimum estimate by Professor G, H. Darwin. (2) Since the ‘consistentior status,’ twenty to forty millions (Lord Kelvin). (8) Since the condensation of the oceans, eighty to ninety millions, maximum estimate by Professor J. Joly. It may be at once observed that these estimates, although independent, are all of the same order of magnitude, and so far confirmatory of each other. Nor are they opposed to conclusions drawn from a study of stratified rocks; thus Sir Archibald Geilkie, in his Address to this Section last year, affirmed that, so far as these were concerned, 100 millions of years might suffice for their formation. There is then very little to quarrel about, and our task is reduced to an attempt, by a little stretching and a little paring, to bring these various estimates into closer harmony. Professor Darwin’s estimate is admittedly a minimum; the actual time, as he himself expressly states, ‘may have been much longer.’ Lord Kelvin’s estimate, which he would make nearer twenty than forty millions, is founded on the assumption that since the period of the ‘ consistentior status’ the earth has cooled simply as a solid body, the transference of heat from within outwards having been accomplished solely by conduction. It may be at once admitted that there isa large amount of truth in this assumption; there can be no possible doubt that the earth reacts towards forces applied for a short time as asolid body. Under the influence of the tides it behaves as though it possessed a rigidity approaching that of steel, and under sudden blows, such as those which give rise to earthquakes, with twice this rigidity, as Professor Milne informs me. Astronomical considerations lead to the conclusion that its effective rigidity has not varied greatly for a long period of past time. Still, while fully recognising these facts, the geologist Inows—we all know—that the crust of the earth is not altogether solid. The existence of volcanoes by itself suggests the contrary, and although the total amount of fluid material which is brought from the interior to the exterior of the earth by volcanic action may be, and certainly is, small—from data given by Professor Penck, I estimate it as equivalent to a layer of rock uniformly distributed 2 mm. thick per century '— yet we have every reason to believe that volcanoes are but the superticial manifesta- tion of far greater bodies of molten material which lie concealed beneath the ground, Even the wide areas of plutonic rock, which are sometimes exposed to view over a country that has suffered long-continued denudation, are merely the upper portion of more extensive masses which lie remote from view. The existence of molten material within the earth’s crust naturally awakens a suspicion that the process of cooling has not been wholly by conduction, but also to some slight extent by convection, and to a still greater extent by the bodily migration of liquid lava from the deeper layers of the crust towards the surface. The existence of local reservoirs of molten rock within the crust is even still more important in another conzection, that is, in relation with the supposed ‘average rate of increase of temperature with descent below the ground.’ It is doubtful whether we have yet discovered a rate that in any useful sense can be spoken of as ‘average. The widely divergent views of different authorities as to the presumed value of this rate may well lead to reflection. The late Professor Prestwich thought a rise of 1°F. for every 45 feet of descent below the zone of constant temperature best represented the average; Lord Kelvin in his earlier estimates has adopted a value of 1°F. for every 51 feet; the Committee of this Association appointed to investigate this question arrived at arate of 1° F. for every 60 feet of descent ; Mr. Clarence King has made calculations in which a rate of 1° F. for 72 feet is adopted; a re-investigation of recorded measurements would, I believe, lead to a rate of 1° F. in 80 or 90 feet as more closely approaching the mean. This would raise Lord Kelvin’s estimate to nearly fifty millions of years. When from these various averages we turn to the observations on which they are based, we encounter a surprising divergence of extremes from the 1 The heat thus brought to the surface would amount to one seventeenth of that conveyed by conduction, > TRANSACTIONS OF SECTION Cy 719 mean; thus in the British Isles alone the rate varies from 1° F. in 34 feet to 1°F. in 92 feet, or in one case to 1° F. in 180 feet. It has been sug- gested, and to some extent shown, that these irregularities may be connected with differences in conductivity of the rocks in whieh the observations were made, or with the circulation of underground water; but many cases exist which cannot be explained away in such a manner, but are suggestive of some deep-seated cause, such as the distribution of molten matter below the ground. Inspection of the accompanying map of the British Isles, on which the rates of increase in Fic. 1—Map of the British Isles, showing the distribution of rates of increase of temperature with descent. ‘Uhe rates are taken from the ‘ British Association Report,’ except in the case of those in the south of Ireland. ee , Ts different localities have been plotted, will afford some evidence of the truth of this view. Comparatively low rates of increase are found over Wales and in the pro- vince of Leinster, districts of relatively great stability, the remnants of an island that have in all probabilty stood above the sea ever since the close of the Silurian period. To the north of this, as we enter a region which was subject to volcanic disturbances during the Tertiary period, the rate increases. It is obvious that in any attempt to estimate the rate at which the earth is cooling as a solid body the disturbing influence of subterranean lakes of molten rock must as far as possible be eliminated ; but this wi!! not be effected by taking 750) Rrevort—1900. the accepted mean of observed rates of increase of temperature! such an Average is merely a compromise, and a nearer approach to a correct result will possibly be attained by selecting some low rate of increase, provided it be based on accurate observations. It is extremely doubtful whether an area such as the British Isles, which has so frequently been the theatre of volcanic activity and other subterranean disturb- ance, 1s the best fitted to afford trustworthy results; the Archzean nucleus of a continent might be expected to afford surer indications. Unfortunately the hidden treasures of the earth are seldom buried in these regions, and bore-holes in conse- quence have rarely been made in them. One exception is afforded by the copper- bearing district of Lake Superior, and in one case, that of the Calumet and Hecla mine, which is 4,580 feet in depth, the rate of increase, as determined by Pro- fessor A. Agassiz, was 1° F. for every 223-7 feet. The Bohemian ‘horst’ is a somewhat ancient part of Europe, and in the Przibram mines, which are sunk in it, the rate was 1°F. for every 126 feet of descent. In the light of these facts it would seem that geologists are by no means compelled to accept the supposed mean rate of increase of temperature with descent into the crust as affording a safe guide to the rate of cooling of a solid globe; and if the much slower rate of increase observed in the more ancient and more stable regions of the earth has the im- portance which is suggested for it, then Lord Kelvin’s estimate of the date of the ‘consistentior status’ may be pushed backwards into a remoter past. If, as we have reason to hope, Lord Kelvin’s somewhat contracted period will yield to a little stretching, Professor Joly’s, on the other hand, may take some paring. His argument, broadly stated, is as follows. ‘The ocean consisted at first of fresh water; it is now salt, and its saltness is due to the dissolved matter that is constantly being carried into it by rivers. If, then, we know the quantity of salt which the rivers bring down each year into the sea, it is easy to calculate how many years they have taken to supply the sea with all the salt it at present contains. For several reasons it is found necessary to restrict attention to one only of the elements contained in sea salt: this is sodinm. The quantity of sodium delivered to the sea every year by rivers is about 160,000,000 tons; but the quantity of sodium which the sea contains is at least ninety millions of times greater than this. The period during which rivers have been carrying sodium into the sea must therefore be about ninety millions of years. Nothing could be simpler ; there is no serious flaw in the method, and Professor Joly’s treatment of the subject is admirable in every way ; but of course in calculations such as this everything depends on the accuracy of the data, which we may therefore proceed to discuss. Professor Joly’s estimate of the amount of sodium in the ocean may be accepted as sufficiently near the truth for all practical purposes. We may therefore pass on to the other factor, the annual contribution of sodium by river water. Here there is more room for error, Two quantities must be ascertained : one the quantity of water which the rivers of the world carry into the sea, the other the quantity or proportion of sodium present in this water. The total volume of water discharged by rivers into the ocean is estimated by Sir John Murray as 6,524 cubic miles. The estimate being based on observations of thirty-three great rivers, although only approximate, it is no doubt sufficiently exact; at all events snch alterations as it is likely to undergo will not greatly affect the final result, When, however, we pass to the last quantity to be determined, the chemical com- position of average river water, we find that only a very rough estimate is possible, and this is the more unfortunate because changes in this may very materially affect our conclusions. The total quantity of river water discharged into the sea is, as we have stated, 6,524 cubic miles. The average composition of this water is deduced from analyses of nineteen great rivers, which altogether discharge only 488 cubic miles, or 7:25 per cent. of the whole, ‘The danger in using this estimate is two- fold: in the first place 7:25 is too small a fraction from which to argue to the re- maining 92:75 per cent., and, next, the riyers which furnish it are selected rivers, z.e., they are all of large size. The eflect of this is that the drainage of the voleanic regions of the earth is not sufficiently represented, and it is precisely this drainage which is richest in sodium salts, The lavas and ashes of active volcanoes rapidly TRANSACTIONS OF SECTION. C, 721 disintegrate under the energetic action of various acid gases, and among volcanic exhalations sodium chloride has been especially noticed as abundant. Conse- quently we find that while the proportion of sodium in Professor Joly’s average river water is only 5°73 per million, in the rivers of the volcanic island of Hawaii it rises to 24°5 per million.’ No doubt the area occupied by volcanoes is trifling com- pared with the remaining land surface. On the other hand the majority of volcanoes are situated in regions of copious rainfall, of which they receive a full share owing to their mountainous form. Much of the fallen rain percolates through the porous material of the cone, and, richly charged with alkalies, finds its way by underground passages towards the sea, into which it sometimes discharges by submarine springs. Again, several considerations lead to the belief that the supply of sodium to the ocean has proceeded, not at a uniform, but at a gradually diminishing rate. The rate of increase of temperature with descent into the crust has continuously diminished with the flow of time, and this must have had its influence on the temperature of springs, which furnish an important contribution to river water. The significance of this consideration may be judged from the composition of the water of geysers. Thus Geyser, in Iceland, contains 884 parts of sodium per million, or nearly 160 times as much as Sir John Murray estimates is present in average river water. A mean of the analyses of six geysers in different parts of the world gives 400 parts of sodium per million, existing partly as chloride, but also as sulphate and carbonate. It should not be overlooked that the present is a calm and quiet epoch in the earth’s history, following after a time of fiery activity. More than once, indeed, has the past been distinguished by unusual manifestations of voleanic energy, and these must have had some effect upon the supply of sodium to the ocean. Finally, although the existing ocean water has apparently but slight effect in corroding the rocks which form its bed, yet it certainly was not inert when its temperature was not far removed from the critical point. Water begins to exert a powerful destructive action on silicates at a temperature of 180° C., and during the interval occupied in cooling, from 370° to 180° C., a considerable quantity of sodium may have entered into solution. A review of the facts before us seems to render some reduction in Dr. Joly's estimate imperative. A precise assessment is impossible, but I should be inclined myself to take off some ten or thirty millions of years. We may next take the evidence of the stratified rocks. Their total maximum thickness is, as we have seen, 265,000 feet, and consequently if they accumulated at the rate of one foot in a century, as evidence seems to suggest, more than twenty-six millions of years must have elapsed during their formation. Obscure Chapter in the Larth’s History. Before discussing the validity of the argument on which this last result de- pends let us consider how far it harmonises with previous ones. It is consistent with Lord Kelvin’s and Professor Darwin’s, but how does it accord with Professor Joly’s? Supposing we reduce his estimate to fifty-five millions: what was the earth doing during the interval between the period of fifty-five millions of years ago and that of only 264 millions ago, when, it is presumed, sedimentary rocks commenced to be formed ? Hitherto we have been able to reason on probabilities ; now we enter the dreary region of possibilities, and open that obscure chapter in the history of the earth previously hinted at. For there are many possible answers to this question. In the first place the evidence of the stratified rocks may have been wrongly interpreted, and two or three times the amount of time we have demanded may have been consumed in their formation. This is a very obvious possibility, yet again our estimate concerning these rocks may be correct, but we may have erroneously omitted to take into account certain portions of the Archean complex. which may represent primitive sedimentary rocks, formed under exceptional con- ? Walter Maxwell, Lavas and Soils of the Hawaiian Islands, p. 170. 1900, 3A Toe REPORT—1900. ditions, and subsequently transformed under the influence of the internal heat of the earth, This, I think, would be Professor Bonney’s view. Finally Lord Kelvin has argued that the life of the sun as a luminous star is even more briefly limited than that of our oceavs. In such a case if our oceans were formed fifty- five millions of years ago, it is possible that after a short existence as almost boiling water they grew colder and colder, till they became covered with thick ice, and moved only in obedience to the tides. The earth, frozen and dark, except for the red glow of her volcanoes, waited the coming of the sun, and it was not till his growing splendour had banished the long night that the cheerful sound of running waters was heard again in our midst. Then the work of denudation and deposition seriously recommenced, not to cease till the life of the sun is spent. Thus the thickness of the stratified series may be a measure rather of the duration of sunlight than of the period which has elapsed since the first formation of the ocean. It may have been so—we cannot tell—but it may be fairly urged that we lmnow less of the origin, history, and constitution of the sun than of the earth itself, and that, for aught we can say to the contrary, the sun may have been shining on the just-formed ocean as cheerfully as he shines to-day. Time required for the Evolution of the Living World, But, it will be asked, how far does a period of twenty-six millions satisfy the demands of biology ? Speaking only for myself, although I am aware that eminent biologists are not wanting who share this opinion, I answer, Amply. But it will be exclaimed, Surely there are ‘comparisons in things.’ Look at Egypt, where more than 4,000 years since the same species of man and animals lived and flourished as to-day. Examine the frescoes and study the living procession of familiar forms they so faithfully portray, and then tell us, how comes it about that from changes so slow as to be inappreciabie in the lapse of forty centuries you propose to build up the whole organic world in the course of a mere twenty-six millions of years? To all which we might reply that even changeless Egypt presents us with at least one change—the features of the ruling race are to-day not quite the same as those of the Pharaohs. But putting this on one side, the admitted constancy in some few common forms proves very little, for so long as the environment remains the same natural selection will conserve the type, and, so far as we are able to judge, conditions in Egypt have remained remarkably constant for a long period. Change the conditions, and the resulting modification of the species becomes manifest enough ; and in this connection it is only necessary to recall the remark- able mutations observed and recorded by Professor Weldon in the case of the crabs in Plymouth Harbour. In response to increasing turbidity of the sea water these crabs have undergone or are undergoing a change in the relative dimensions of the carapace, which is persistent, in one direction, and rapid enough to be determined by measurements made at intervals of a few years. Again, animals do not all change their characters at the same rate: some are stable, in spite of changing conditions, and these have been cited to prove that none of the periods we look upon as probable, not twenty-five, not a hundred millions of years, scarce any period short of eternity, is sufficient to account for the evolution of the living world. Ifthe little tongue-shell, Zingula, has endured with next to no perceptible change from the Cambrian down to the present day, how long, it is sometimes inquired, would it require for the evolution of the rest of the animal kingdom? The reply issimple: the cases are dissimilar, and the same record which assures us of the persistency of the Lingula tells us in language equally emphatic of the course of evolution which has led from the lower organisms upwards to man. In recent and Pleistocene deposits the relics of man are plentiful: in the latest Pliocene they have disappeared, and we encounter the remarkable form Pithe- canthropus; as we descend into the Tertiary systems the higher mammals are met with, always sinking lower and lower in the scale of organisation as they occur deeper in the series, till in the Mesozoic deposits they have entirely disappeared, and their place is taken by the lower mammals, a feeble folk, offering little promise of the future they were to inherit, Still lower, and even these are gone; and in the Permian TRANSACTIONS OF SECTION C. 723 We ericounter reptiles and the ancestors of reptiles, probably ancestors of mammals too ; then into the Carboniferous, where we find amphibians, but no true reptiles ; and next into the Devonian, where fish predominate, after making their earliest appearance at the close of the Silurian times ; thence downwards, and the verte- brata are no more found—we trace the evolution of the invertebrata alone, Thus the orderly procession of organic forms follows in precisely the true phylogenetic sequence: invertebrata first, then vertebrates, at first fish, then amphibia, next reptiles, soon after mammals, of the lowlier kinds first, of the higher later, and these in increasing complexity of structure till we finally arrive at man himself. While the living world was thus unfolding into new and nobler forms, tho immutable Lingula simply perpetuated its kind, To select it, or other species equally sluggish, as the sole measure of the rate of biologic change would seem as strange a proceeding as to confound the swiftness of a river with the stagnation of the pools that lie beside its banks. It is occasionally objected that the story we have drawn from the paleontological record is mere myth or is founded only on negative evidence. Cavils of this kind prove a double misapprehension, partly us to the facts, partly as to the value of negative evidence, which may be as good in its way as any other kind of evidence. Geologists are not unaware of the pitfalls which beset negative evidence, and they do not conclude trom the absence of fossils in the rocks which underlie the Cambrian that pre-Cambrian periods were devoid of life; on the contrary, they are fully persuaded that the seas of those times were teeming with a rich variety of invertebrate forms. How is it that, with the exception of some few species found in beds immediately underiving tne Cambrian, these have left behind no vestige of their existence? The explanation does not lie in the nature of the sediments, which are not unfitted for the preservation of fossils, nor in the composition of the then existing sea water, which may have contained quiteas much caleium carbonate as occurs in our present oceans; and the only plausible supposition would appear to be that the organisms of that time had not passed beyond the stage now represented by the larvee of existing invertebrata, and consequently were either unprovided with skeletons or at all events with skeletons durable enough for preservation. If so, the history of the earlier stages of the evolution of the invertebrata will receive no light from palzeontology ; and no direct answer can be expected to the question whether, eighteen or nineteen millions of years being taken as sufficient for the evolution of the vertebrata, the remaining available eight millions would provide for that of the invertebrate classes which are represented in the lowest Cambrian deposits. On é@ priori grounds there would appear to be no reason why it should not. If two millions of years afforded time enough for the conversion of fish into amphibians, a similar period should suffice for the evolution of trilobites from annelids, or of annelids from trochospheres. The step from gastrulas to trocho- spheres might be accomplished in another two millions, and two millions more would take us from gastrulas through morulas to protozoa. As things stand, biologists can have nothing to say either for or against such a conclusion: they are not at present in a position to offer independent evidence ; nor can they hope to be so until they have vastly extended those promising investigations which they are only now beginning to make into the rate of the variation of species. Unexpected Absence of Thermal Metamorphosis in Ancient Rocks. Two difficulties now remain for discussion: one based on theories of mountain chains, the other on the unaltered state of some ancient sediments. The latter may be taken first. Professor yan Hise writes as follows regarding the pre-Cambrian rocks of the Lake Superior district: ‘The Penokee series furnishes an instructive lesson as to the depth to which rocks may be buried and yet remain but slightly affected by metamorphosis. The series itself is 14,000 feet thick. It was covered before being upturned with a great thickness of Keweenaw rock. This series at the Montreal River is estimated to be 50,000 feet thick. Adding to this the known thickness of the Penokee series, we have a thickness of 64,000 feet... . The 3A 2 724 REPORT—1900, Penokee rocks were then buried to a great depth, the exact amount depending upon their horizon and upon the stage in Keweenaw time, when the tilting and erosion, which brought them to the surface, commenced. ‘That the synclinal trough of Lake Superior began to form before the end of the Keweenaw period, and consequently that the Penokee rocks were not buried under the full succession, is more than probable. However, they must have been buried to a great depth—at least several miles—and thus subjected to high pressure and temperature, notwithstanding which they are comparatively unaltered.’ ! I select this example because it is one of the best instances of a difficulty that occurs more than once in considering the history of sedimentary rocks. On the supposition that the rate cf increment of temperature with descent is 1° F. for every 84 feet, or 1° C. for every 150 feet, and that it was no greater during these early Penokee times, then at a depth of 50,000 feet the Penokee rocks would attain a temperature of nearly 833° C. ; and since water begins to exert powerful chemical action at 180° C. they should, on the theory of a solid cooling globe, have suffered a metamorphosis sufficient to obscure their resemblance to sedimentary rocks. Hither then the accepted rate of downward increase of temperature is erroneous, or the Penokee rocks were never depressed, in the place where they are exposed to observation, to a depth of 50,000 feet. Let us consider each alternative, and in the first place let us apply the rate of temperature increment deter- mined by Professor Agassiz in this very Lake Superior district: it is 1° OC. for every 402 feet, and twenty-five millions of years ago, or about the time when we may suppose the Penokee rocks were being formed, it would be 1° C. for every 305'5 feet, with a resulting temperature at a depth of 50,000 feet of 163° C. only. Thus the admission of a very low rate of temperature increment would meet the difficulty ; but on the other hand it would involve a period of several hundreds of millions of years for the age of the ‘consistentior status,’ and thus greatly exceed Professor Joly’s maximum estimate of the age of the oceans. We may therefore turn to the second alternative. As regards this it is by no means certain that the exposed portion of the Penokee series ever was depressed 50,000 feet: the beds lie in a synclinal the base of which indeed may have sunk to this extent, and entered a region of metamorphosis ; but the only part of the system that lies exposed to view is the upturned margin of the synclinal, and as to this it would seem impos- sible to make any positive assertion as to the depth to which it may or may not have been depressed. To keep an open mind on the question seems our only course for the present, but difficulties like this offer a promising field for investigation. The Formation of Mountain Ranges. It is frequently alleged that mountain chains cannot be explained on the hypo- thesis of a solid earth cooling under the conditions and for the period we have supposed. This is a question well worthy of consideration, and we may first endeavour to picture to ourselves the conditions under which mountain chains arise. The floor of the ocean lies at an average depth of 2,000 fathoms below the land, and is maintained at a constant temperature, closely approaching 0° C., by the passage over it of cold water creeping from the polar regions. The average tem-_ perature of the surface of the land is above zero, but we can afford to disregard the difference in temperature between it and the ocean floor, and may take them both at zero. Consider next the increase of temperature with descent, which occurs beneath the continents: at a depth of 13,000 feet, or at same depth as the ocean floor, a temperature of 87° C. will be reached on the supposition that the rate of increase is 1° C. for 150 feet, while with the usually accepted rate of 1° C. for 108 feet it would be 120°C. But at this depth the ocean floor, which is on the same spherical surface, is at 0° C. Thus surfaces of equal temperature within the earth’s crust will not be spherical, but will rise or fall beneath an imaginary spherical or spheroidal surface according as they occur beneath the continents or the oceans. No doubt at some depth within the earth the departure of isothermal 1 Tenth Annual Report U.S, Geol. Survey, 1888-89, p. 457. i TRANSACTIONS OF SECTION C. 725 surfaces from a spheroidal form will disappear; but considering the great breadth both of continents and oceans this depth must be considerable, possibly even forty or fifty miles. Thus the sub-continental excess of temperature may make itself felt in regions where the rocks still retain a hizh temperature, and are probably not far removed from the critical fusion point. The effect will be to render the con- tinents mobile as regards the ocean floor ; or, vice versd, the ocean floor will be stable compared with the continental masses, Next it may be observed that the con- tinents pass into the bed of the ocean by a somewhat rapid flexure, and that it is over this area of flexure that the sediments denuded from the land are deposited. Under its load of sediment the sea-floor sinks down, subsiding slowly, at about the same rate as the thickness of sediment increases; and, whether as a consequence or a cause, or both, the flexure marking the boundary of land and sea becomes more pronounced. A compensating movement occurs within the earth’s crust, and solid material may flow from under the subsiding area in the direction of least resist- ance, possibly towards the land. At length, when some thirty or forty thousand feet of sediment have accumulated in a basin-like form, or, according to our reckoning, after the lapse of three or four millions of years, the downward movement ceases, and the mass of sediment is subjected to powerful lateral compression, which, bringing its borders into closer proximity by some ten or thirty miles, causes it to rise in great folds high into the air as a mountain chain. It is this last phase in the history of mountain making which has given geo- logists more cause for painful thought than probably any other branch of their subject, not excluding even the age ot the earth. It was at first imagined that during the flow of time the interior of the earth lost so much heat, and suffered so much con- traction in consequence, that the exterior, in adapting itself to the shrunken body, was compelled to fit it like a wrinkled garment. This theory, indeed, enjoyed a happy existence till it fell into the hands of mathematicians, when it fared very badly, and now lies in a pitiable condition neglected of its friends." For it seemed proved to demonstration that the contraction consequent on cooling was wholly, even ridiculously, inadequate to explain the wrinkling. But when we summon up courage to inquire into the data on which the mathematical arguments are based, we find that they include several assumptions the truth of: which is by no means self-evident. Thus it has been assumed that the rate at which the fusion point rises with increased pressure is constant, and follows the same law as is deduced from experiments made under such pressures as we can command in our laboratories down to the very centre of the earth, where the pressures are of an altogether different order of magnitude; so with a still more important coefficient, that of expansion, our knowledge of this quantity is founded on the behaviour of rocks heated under ordinary atmospheric pressure, and it is assumed that the same coefficient as is thus obtained may he safely applied to material which is kept solid, possibly near the critical point, under the tremendous pressure of the depths of the crust. To this last assumption we owe the terrible bogies that have been conjured out of ‘the level of no strain.’ The depth of this as calculated by the Rev. O. Fisher is so trifling that it would be passed through by all very deep mines. Mr. C. Davison, however, has shown that it will lie considerably deeper, if the known increase of the coefficient of expansion with rise of temperature be taken into account. It is possible, it is even likely, that the coefficient of expansion becomes vastly greater when regions are entered, where the rocks are compelled into the solid state by pressure. So little do we actually know of the behaviour of rock under these conditions that the geologist would seem to be left very much to his own devices; but it would seem there is one temptation he must resist—he may not take refuge in the hypothesis of a liquid interior. We shall boldly assume that the contraction at some unknown depth in the interior of the earth is sufficient to afford the explanation we seek. The course of events may then proceed as follows. The contraction of the interior of the earth, 1 With some exceptions, notably Mr, C, Davison, a consistent supporter of the theory of contraction. 726 REPORT—1900. consequent on its loss of heat, causes the crust to fall upon it in folds, which rise over the continents and sink under the oceans, and the flexure of the area of sedimentation is partly a consequence of this folding, partly of overloading. By the time a depression of some 80,000 or 40,000 feet has occurred along the ocean border the relation between continents and oceans has become unstable, and readjustment takes place, probably by a giving way of the continents, and chiefly along the zone of greatest weakness, 7c. the area of sedimentation, which thus becomes the zone of mountain building. It may be observed that at great depths readjustment will be produced by a slow flowing of solid rock, and it is only comparatively near the surface, five or ten miles at the most below, that failure of support can lead to sudden fracture and collapse; hence the comparatively super- ficial origin of earthquakes. Given a sufficiently large coefficient of expansion—and there is much to suggest its existence '—and all the phenomena of mountain ranges become explicable: they begin to present an appearance that invites mathematical treatment; they inspire us with the hope that from a knowledge of the height and dimensions of a continent and its relations to the bordering ocean we may be able to predict when and where a mountain chsin should arise, and the theory which explains them promises to guide us to an interpretation of those world-wide unconformities which Suess can only account for by a transgression of the sea. Finally it relieves us of the difficulty presented by mountain formation in regard to the estimated duration of geological time. Influence of Variations in the Eccentricity of the Earth's Orbit. This may perhaps be the place to notice a highly interesting speculation which we owe to Professor Blytt, who has attempted to establish a connection between periods of readjustment of the earth’s crust and variations in the eccentricity of the earth’s orbit. Without entering into any discussion of Professor Blytt’s methods, we may offer a comparison of his results with those that follow from our rough estimate of one foot of sediment accumulated in a century. Table showing the Time that has elapsed since the Beginning of the Systems in the Jirst column, as reckoned from Thickness of Sediment in the second column, and by Professor Blytt in the third :— —_— | Years | Years EGecney! re ey) Towards the north the surface of the Boulder Clay rises, a bed of stoneless red clay intrudes in the upper portion of the gravels, a peat bed makes its appearance, one of the shell beds disappears, and the toe of a sandy balk is introduced under the warp. At the north end of this trench there are two beds of Boulder Clay separated by gravels, the red clay having disappeared ; otherwise the section is similar to that last described. The shell bed contained Cardium edule, Tellina solidula, Scrobicularia piperata, Utriculus obtusus, Rissoa ulva, Littorina rudis, L. obtusata, Mytilus edulis, Pholas candida, and Nassa incrassata, the latter five being new records for this bed. The large number of very young specimens and both valves being often intact indicate but a short journey and beach-like conditions. The surface of the clay and peat bed was level and undisturbed, except that the smaller shells of the shell bed above penetrated into numerous. crack-like crevices, and seemed to indicate that the clay had been exposed and sun-dried before the waters of the estuary formed their shell beach. The shell bed underlying the warp and the method of deposition of the warp appear to suggest that, whether the clay below was deposited under conditions due to subsidence, sudden or rapid, or not, a gradual subsidence took place during the deposition of the warp. In the clay and peat bed there were stumps of trees, including oak (Quercus pedunculata), with the roots extending several feet into the glacial beds below ; a number of perfect cherries (Prunus Padus) were found, the quantity and con- dition of which may suggest that the trees were bearing fruit at the time of the first inundation ; a few pieces of charcoal grouped together were also found in this bed, but careful search revealed nothing that could be attributed to human agency. Nore.—Upper Shell Bed and top of Clay and Peat Bed, about 13 ft. below O.D.; High Water ordinary Spring Tides, about 12 ft. above O.D.; Low Water ordinary Spring Tides, about 10 ft. below O.D. 5. The Jurassic Flora of East Yorkshire. By A. C. Suwarp, F.R.S, The plant-beds exposed in the cliff sections of the Yorkshire coast have afforded unusually rich data towards a restoration of the characteristics and com- position of a certain facies of Mesozoic vegetation. Rich collections of plants from Gristhorpe Bay and other well-known localities are found in the British Museum, also in the Museums of Scarborough, Whitby, Cambridge, Oxford, Manchester, York, Newcastle, Leeds, and elsewhere. The Natural History Museum, Paris, contains several important Yorkshire plants, some of which have been described by Brongniart and Saporta. The following species have been recognised from the East Yorkshire area :— Marchantites erectus (Leck., ex Bean, MS.); Eyuisetites columnaris, Brongn. ; Equisetites Beant (Bunb.) ; Lycopodites fulcatus, L. & H.; Cladophlebis denticu- lata (Brongn.); C. haiburnensis (L. & H.); C. lobéfolia (Phill.) ; Contopteris arguta (lL. & H.); C. hymenophylloides (Brongn.); C. guingueloba (Phill.) ; Dictyophyl- lum rugosum, L. & H.; Klukia exilis (Phill.) ; Laccopteris polypodioides (Brongn.); L. Woodwardi (Leck.); Matonidium Goepperti (Ett.); Pachypteris lanceolata, Brongn.; Ruffordia Goepperti (Dunk.) ; Sugenopteris Phillipst (Brongn.); Sphe- 766 REPORT—1900. nopteris Murrayana (Brongn.); 8. Williamsoni, Brongn.; Teniopteris major, L. & H.; T. vittata, Brongn.; Todites Williamsoni (Brongn.); Anomozamites Nilssont (Phill.); Araucarites Phillipsi, Carr; Baiera gracilis, Bunb.; B. Lindleyana (Schimp.); B. Phillipsi, Nath.; Beania gracilis, Carr; Brachyphyllum mamillare, Brongn. ; Chezrolepis setosus (Phill.); Cryptomerites divaricatus, Bunb.; Ctenis falcata, L. & H.; Czekanowskia Murrayana(L. & H.); Dioonites Nathorsti, sp. nov.; Ginkgo digitata (Brongn.) ; G. whitbiensis, Nath.; Nagetopsis anglica, sp. noy.; Nilssonia compta (Phill.); N. mediana (Leck., ex Bean, MS.); NV. tenui- nervis, Nath.; Otozamites acuminatus (L. & H.); O. Beani (L. & H.); O. Bun- buryanus, Zign.; O. Feistmanteli, Zign.; O. graphicus (Leck., ex Bean, MS.); O. obtusus (L. & H.), var. ooliticus; O. parallelus (Phill.) ; Pagiophyllum Williamsont (Brongn.); Podozamites lanceolatus (L. & H.); Pétilozamites (Leck., ex Bean, MS.); Yaaites zamioides (Leck.); Williamsonia gigas (L. & H.); W. pecten (Phill.). The English flora is compared by the author with Rhetic, Jurassic, and Weal- den floras of other regions; a comparison is made also between the fossil flora and the vegetation of the present day. 6. Note on the Age of the English Wealden Series. By G. W. Lamptueu, £.G.8., of H.M. Geological Survey. In recent discussions arising from the renewed attempts to define more closely the boundary between the Jurassic and Cretaceous systems in Russia, Germany, Belgium, and France, and also in North America, constant reference has been made to the English Wealden deposits as affording a standard of comparison. But meanwhile doubt has been thrown, by paleontologists who have studied certain portions of the Wealden flora and fauna, on the hitherto accepted classification of these English deposits with the Lower Cretaceous, on the ground that the fossils showed strong Jurassic affinities. This opinion has been expressed by the late Professor O. C. Marsh in regard to the reptiles, by Dr. A. Smith Woodward in regard to the fish, and by A. C. Seward in regard to the plants. To prevent further confusion it is therefore desirable that certain facts which have been over- looked in this discussion, though for the most part already published, should be restated, since these facts seem sufficient to prove that at any rate the greater portion of the English Wealden series must remain as part of the Lower Cre- taceous. It has not always been sufficiently borne in mind that the accumulation of the Wealden Series must have required a period of long duration. The sands of the Hastings Beds may indeed have been deposited rather rapidly, but the shaly clays with layers of shells and cyprids interstratified with these sands indicate slower sedimentation, and the great mass of Weald Clay, reaching 1,000 feet in thickness, must represent an epoch of great length. Hence, since it is universally acknow- ledged that the fresh-water conditions did not set in until the closing stages of the Jurassic period, it seems inevitable from this consideration alone that such conditions persisted into Lower Cretaceous times. Again, nearly all the ‘ Wealden’ fossils in which Jurassic affinities have been observed have been obtained from the lower part of the Wealden series (¢.e. from the Hastings Beds), and very little is known respecting the corresponding fossils from the Weald Clay which probably represents the major portion of the Wealden eriod. Moreover, the argument from the Jurassic affinities of the land and fresh-water fossils alone inspires no confidence, since if we eliminate the Lower Wealden fossils from the Lower Cretaceous lists our knowledge is practically limited to the marine life of this period; and it may be legitimately asked whether the land and fresh-water fossils of the Hastings Beds are not, after all, of the character proper to the lowermost part of the Cretaceous, wherein a close relationship to the immediately preceding period seems quite appropriate. It is from the stratigraphical evidence, however, that the Lower Cretaceous TRANSACTIONS OF SEOTION C. 767 age of at least the greater portion of the English Wealden Series can be most satisfactorily established, by its relation to the marine sequence which must form the ultimate basis of the classification. The marine beds directly overlying the Weald Clay in the south of England represent only the latest stage (Aptien) of the Lower Cretaceous period; and although there is a sharp line of demarca- tion at their base, this seems to denote a rapid change of conditions and not a lengthy time-interval, since the incoming of marine or brackish-water shells near the top of the Wealden strata in Dorset, Hampshire, and Surrey, foreshadowing the termination of the fresh-water episode, indicates that the series is practically complete, and has undergone little if any erosion in these parts before the deposition of the overlying marine strata. Such erosion may, however, have taken place locally towards the easterly and westerly terminations of the basin of deposition, where the topmost beds of the Wealden Series are not found. In the Speeton Clay, where the Lower Cretaceous marine sequence is fully represented, the equivalents of the Lower Greensand and Atherfield Clay of the south of England are comprised within a relatively narrow compass in the sparingly fossiliferous upper part of the sequence ;! and therefore by far the greater portion of the Lower Cretaceous period, if represented at all in the south of England, must be represented in the Wealden Series. The portion of the Speeton Clay unrepresented by marine sediments in the south includes the lower part of the Zone of Belemnites brunsvicensis, and the whole of the Zone of Bel. jaculum, both undoubtedly Lower Cretaceous (Barrémien, Hauterivien, and Valanginien), together with the whole of the Zone of Bed. lateralis, the fauna of which shows Jurassic affinities. Furthermore, in tracing this marine series southward from York- shire through Lincolnshire into Norfolk, the author has found that in the latter county the lower zones are apparently absent, and the remaining portion, represent- ing probably the lower part of the Zone of Bel. brunsvicensis, is characterised by the presence among the marine fossils of plant remains, chiefly fragments of a Wealden fern, Weichselia (Mantelli?), and by other indications of fluviatile influ- ence, suggesting the beginning of a lateral change into Wealden conditions.? With the well-recognised gradual development of fresh-water conditions in the Purbeck beds of the Wealden area towards the close of the Jurassic period, and indications of the reversal of this process in the top of the Weald Clay during the later stages of the Lower Cretaceous, and with evidence for a lateral passage of part of the Lower Cretaceous marine sediments of the North of England into estuarine deposits further south, there seems every reason to believe that in the fresh-water or estuarine strata of the English Wealden the whole of the time- interval between the Portlandian and Aptien stages is represented, and that it would be equally erroneous to classify the series entirely with the Jurassic system and entirely with the Cretaceous, if the hitherto recognised boundary of these systems in the marine deposits of other areas is to be maintained, The deposits classed as Wealden in Belgium, Germany, and France appear to be much more restricted in vertical range than the English series, and to represent different parts of the period in different places, but nowhere to imply the same long continuance of fresh-water conditions in a single area, ' See Summary of Progress of the Geological Survey fur 1897, p. * See Survey Mem. Borders of the Wash (sheet 69 O.8)., pp. 21- 129. 25. 7. Report on the Irish Elk Remains in the Isle of Man. See Reports, p. 349. 768 REPORT—1900. Section D,—ZOOLOGY. PRESIDENT OF THE SEctIoON—Rameay H. Traqvarr, M.D., LL.D., F.R.S, THURSDAY, SEPTEMBER 6, The President delivered the following Address :— In opening to-day the sittings of the Zoological Section, I must first express my sense of the honour which has been conferred on me in having been chosen as your President on this occasion, and I may add that I feel it not only as an honour to myself personally but also as a compliment to the field of investigation in which the greater part of my own original work has been done. It is a wel- come recognition of the doctrine, which I, and much more important men indeed than I, have always maintained, namely, that Paleontology, however valuable, nay, indispensable, its bearings on Geology may be, is in its own essence a part of Biology, and that its facts and its teachings must not be overlooked by those who would pursue the study of Organic Morphology on a truly comprehensive and scientific basis. As I have asked on a previous occasion, ‘ Does an animal cease to be an animal because it is preserved in stone instead of spirits? Is a skeleton any the less a skeleton because it has been excavated from the rock, instead of prepared in a macerating trough?’ And I may now add—Do animals, because they have been extinct for it may be millions of years, thereby give up their place in the great chain of organic being, or do they cease to be of any importance to the evolutionist because their‘soft tissues, now no longer existing, cannot be imbedded in parafline and cut with a Cambridge microtome ? These are thes2s which I think no one denies theoretically ; but what of the practical application of the rule? for though cordially thanking my biological brethren for the honour they have done me in placing me in this chair to-day, I must ask them not to be offended if I say that in times past I have a few things against some of them at least. I refer first to the apathy concerning palzonto- logical work, more especially where fishes are concerned, which one frequently meets with in the writings of biologists, as seen in the setting up of classifications and theories and the erection of genealogical trees without any, or with at least inadequate, enquiry as to whether such theories or trees are corroborated by the record of the rocks. But more vexatious still are the offhand proceedings of some biologists who, when they wish to complete their generalisations on the structure of a living organism, or group of organisms, by allusion to those which in geological time have gone before, do not take the trouble to consult the original palzonto- logical memoirs or papers, or to make themselves in any way practically acquainted with the subject, but derive their knowledge at second or third hand from some text-book or similar work, which may not in every case be exactly up to date on the matters in question, Nay, more than this, I think I have seen the authors of such text-books or treatises credited with facts and illustrations which were due to the labours of hard-working paleontologists years before. =—v TRANSACTIONS OF SECTION D, 769 But a better time, I am convinced, is not far off, when the unity of all biological science will be recognised not merely theoretically but also practically by workers in every one of its branches. Of one thing I must however warn those who have hitherto devoted their time exclusively to the investigation of things recent, namely, that a special training is necessary for the correct interpretation of fossil remains, especially those of the lower Vertebrata and many groups of Invertebrata. So it comes that what looks to the uninitiated eye a mere confused mass of broken bones or plates may to the trained observer afford a flood of valuable licht on questions of struc- ture previously undetermined. We must take into account the condition of the fossil as regards mineralisation and crushing; we must learn to recognise how the various bones may be dislocated, scattered, or shoved over each other, and to distinguish true sutures from mere fractures. We must carefully correlate the positive results obtained from one specimen with those afforded by others, and in this way it happens that to make a successful restoration of the exo- or endo- skeleton of a fossil fish or reptile may require years of patient research. But the thought sometimes does come up in my mind, that some people imagine that fossils, such as fishes, occur in the rocks all restored and ready, so that the author of such a restoration has no more scientific credit in his work than if he were an ordinary draughtsman drawing a perch ora trout for an illustrated book! But the student of fossil remains must learn not only to see what does exist in the specimen he examines, but also to refrain from seeing things which are not there —to know what he does not see as well as what he does see. For. many grave errors have arisen from want of this necessary training, as for instance where the under surface of a fish’s head has been described as the upper, or where markings of a purely petrological character have been supposed to indicate actual structures of the greatest morphological importance. Or we may find the most wonderful details described, which may indeed have existed, but for which the actual evidence is only the fertile imagination of the writer. From this it will be apparent that though Paleontology is Biology and Biology includes Paleontology, yet as regards original research a division of labour is in most cases necessary. For though paleontological investigations are absolutely impossible without an adequate knowledge of recent zoology, yet the nature of the remains with which the paleontologist has to deal renders their interpretation a task of so different a character from that allotted to the investiga- tion of the structure and development of recent forms that he will scarcely have time for the successful carrying out of a second line of research. Conversely, the same holds regarding the sphere of work of the recent biologist. Now those last remarks of mine may perhaps tend to confirm an idea which I have at least been told is prevalent in the minds of recent biologists, namely, that the results of Paleontology are so uncertain, so doubtful, and so imperfect, that they are scarcely worthy of serious attention being paid to them. And the best answer I can make to such an opinion, if it really does exist, is to try to place before you some evidence that Paleontology is not mere fossil shell hunting, or the making up of long lists of names to help the geologists to settle their stratigraphical horizons, but may present us with abundance of matter of genuine biological interest. Since the days of Darwin, there is one subject which more’than all others engrosses the attention of scientific biologists. I mean the question of Evolution, or the Doctrine of Descent. Time was when controversies raged round the very idea of Evolution, and when men of science were divided among themselves as to whether the doctrine to which Darwin’s theory of Natural Selection gaye so mighty an impetus was or was not to be accepted. Times have however changed, and I hardly think that we should now find a single true scientific worker who continues to hold on by the old special creation idea. Philosophie zoologists now busy themselves either with amassing morphological evidences of Descent or with the discussion of various theories as to the factors by which organic evolution has been brought about—whether Natural Selection has been the all-sufficient cause or not, whether acquired peculiarities are transmissible, and so on, 1900, 3D 770 REPORT—1900. From the natui'e of things it is clear that the voice of the paleontologist can only be heard on the morphological aspect of the question, but to many of us, including myself, the morphological argument is so convincing that we believe that even if the Darwinian theory were proved to-morrow to be utterly baseless, the Doctrine of Descent would not be in the slightest degree affected, but would continue to have as firm a hold on our minds as before. Now as Palwontology takes us back, far back, into the life of the past, it micht be reasonably expected that it would throw great light on the descent of animals, but the amount of its evidence is necessarily much diminished by two unfortunate circumstances. First, the terrible imperfection of the geological record, a fact so obvious to any one having any acquaintance with Geology that it need not be discussed here; and secondly, the circumstance that save in very exceptional cases only the hard parts of animals are preserved, and those too often in an extremely fragmentary and disjointed condition. But though we cannot expect that the paleontological record will ever be anything more than fragmen- tary, yet the constant occurrence of new and important discoveries leads us to entertain the hope that, in course of time, more and more of its pages will become disclosed to us. Incomplete, however, as our knowledge of Evolution as derived from Paleontology must be, that is no reason why we should not appraise it at its proper value, and now and again stop for a moment to take stock of the material which has accumulated. You are all already acquainted with the telling evidence in favour of Evolution furnished by the well-known series of Mammalian limbs, as well as of teeth, in which the progress, in the course of time, from the more general to the more special is so obvious that I cannot conceive of any unprejudiced person shutting his eyes to the inference that Descent with modification is the reason of these things being so. Suppose, then, that on this occasion we take up the paleonto- logical evidence of Descent in the case of fishes. This I do the more readily because what original work I have been able to do has lain principally in the direction of fossil ichthyology ; and again, because it does seem to me that it is in this department that one has most reason to complain of want of interest on the part of recent biologists, even, I may say, of some professed paleontologists themselves. But the subject is really of so great an extent that to exhaust it in the course of an address like the present would be simply impossible, so I shall in the main limit myself to the consideration of Palzozoic forms, and this more especially see- ing that we may hope for a large addition to our light on the fishes of the more recent geological formations from the fourth volume of the ‘Catalocue of Fossil Fishes’ in the British Museum, which will soon appear from tbe pen of my friend Dr. A. Smith Woodward. I need scarcely say how much his previous volume has conduced to a better knowledge of the Mesozoic forms. Ilere I may begin by boldly affirming that I include the Marsipobranchii as fishes, in spite of the dictum of Cope that no animal ean be a fish which does not possess a lower jaw and a shoulder-girdle. Why not? The position seems to me to be a merely arbitrary one; and it is, to say the least, not impossible that the modern Lampreys and Hags may be, as many believe, the degenerate descendants of originally gnathostomatous forms, Yo the origin of the Vertebrata Paleontology gives us no clue, as the fore- _ runners of the fishes must have been creatures which, like the lowest Chordata of the present day (Urochorda, Hemichorda, Cephalochorda), had no hard parts capable of preservation, And though I shall presently refer again to the subject, I may here affirm that, so far as I can read the record at least, it is impossible to derive from Paleontology any support to the view, recently revived, that the ancient fishes are in any way related to Crustacean or Merostomatous ancestors, What have we then to say concerning the most ancient fishes with which we are acquainted ? The idea that the minute bodies, known as Conodonts, which occur from the Cambrian to the Carboniferous, are the teeth of fishes and possibly even of ancient TRANSACTIONS OF SECTION D. Vil Marsipobranchs may now be said to be given up. They are now accepted by the most reliable authorities as appertaining to Invertebrata such as Annelides and Gephyrea. More recently, however, Rohon! has described from the Lower Silurian of the neighbourhood of St. Petersburg small teeth (Paleodus and Archodus) associated with Conodonts, and which seem to be real fish teeth, but not of Selachians, as is shown by the presence of a pulp cavity surrounded by non-vascular dentine, It is impossible to say anything more of their affinities. Obscure and fragmentary fish remains have been obtained by Walcot, and described by Jaekel, from rocks in Colorado supposed to be of Lower Silurian or Ordovician age.* But doubts have been thrown on their age, and the fossils them- selves, which have, it must be owned, a very Devonian look about them, are so extremely fragmentary that they do not help us much in our present purpose. It is not till we come to the Upper Silurian rocks that we begin to feel the ground securely under our feet, though we may be certain, from the degree of specialisation of the forms which we there find, that fishes lived in the waters of the globe for long ages previously. Characteristic of the ‘ Ludlow bone-bed’ are certain minute scales on which Pander founded the family Ccelolepidee, having a flat or sculptured crown, below which is a constricted ‘neck,’ and then a base usually perforated by an aperture leading into a central pulp cavity. As these little bodies, looked upon by Agassiz as teeth, were shown by McCoy to be scales, and as they occurred at Ludlow in England and Oeselin Russia along with small Selachian spines (Onchus), they were usually considered as appertaining, with the latter, to small Cestraciont sharks. The genera Thelodus, Celolepis, and others were founded on these dermal bodies, but it is doubtful if any but the first of these names will stand. But the aspect of affairs was altogether changed by the discovery three years ago by the officers of the Geological Survey-of entire specimens of Zhedodus in the Upper Silurian rocks of the South of Scotland, from which it was evident that the fish, though somewhat shark-like, could hardly be reckoned as a true Selachian.® Thelodus scoticus, Traq., has a broad flattened anterior part corresponding to the head and forepart of the body, very bluntly rounded in front, and passing behind into right and left angular flap-like projections, which are sharply marked off from the narrow tail, which is furnished with a deeply cleft heterocercal caudal fin. Unless the flap-like lateral projections are representatives of pectorals, no other fins are present, neither do we find any teeth or jaws, nor any trace of internal skeleton ; and itis only a few days since Mr. Tait, collector to the Geological Survey of Scotland, pointed out to me in a recently acquired specimen a right and left dark spot at the outer margins of the head near the front, which spots may indicate the position of the eyes.* A previously unknown genus, Lanarkia, Traq., also occurred, in which the creature had the very same form, but instead of having the skin clothed with small shagreen-like scales, possessed, in their place, minute sharp conical hollow spines, without base and open below. What we are to think of those two ancient forms, apparently so primitive, and yet undoubtedly also to a great extent specialised, we shall presently discuss. Let us now fora moment look at the genus Drepanaspis, Schliiter, from the Lower Devonian of Gmiinden in Western Germany,” We have here a strange ‘ «Ueber untersilurische Fische,’ Wélanges Géol. et Paléont. vol. i. (St. Petersburg, 1889), pp. 9-14. 2 Bulletin Geol. Soe. America, vol. iii. 1892, pp. 153-171, * KR. H. Traquair, ‘ Report on Fossil Fishes collected by the Geological Survey in the Silurian Rocks of the South of Scotland,’ Zrans. Roy. Soc. Hdin., vol. xxxix. 1899, pp. 827-864. A specimen of Zhelodus had, however, been found by Mr. James Young, of Lesmahagow, before the Geological Survey came on the scene, * IT am indebted to Sir A. Geikie, F.R.S., Director-General of the Geological Survey, for permission to make use of this and other facts disclosed by Mr. Tait’s work in the Lesmahagow Silurians during the present summer. 5 R. H. Traquair, Geol. Maq., April 1900. 172 REPORT—1900, creature whose shape entirely reminds us of that of Thelodus, having the same flat broad anterior part, bluntly rounded in front, and angulated behind, to which is appended a narrow tail ending in a heterocercal caudal fin, which is, however, scarcely bilobate. But here the dermal covering, instead of consisting of separate scales or spinelets, shows a close carapace of hard bony plates, of which two are especially large and prominent—the median dorsal and the median ventral—other large ones being placed around the margins, while the intervening space is occupied by a mosaic of small polygonal pieces. The position of the mouth, a transverse slit, is seen just at the anterior margin ; it is bounded behind by a median mental or chin-plate, but no jaws properly so called are visible, nor are there any teeth. Then on each margin near the front of the head is a small round pit, exactly in the position of the dark spot seen in some examples of Thelodus, which, if not an orbit, must indicate the position of some organ of sense. Again, the tail is covered with scales after the manner of a ‘ganoid’ fish, being rhombic on the sides, but assum- ing the form of long deeply imbricating fulcra on the dorsal and ventral margins. The position of the branchial opening, or openings, has not yet been definitely ascertained. All these plates are closely covered with stellate tubercles, and we cannot escape from the conclusion that they are formed by the fusion of small shagreen bodies like those of Thelodus, and united to bony matter developed in a deeper layer of the skin. Ifthe angular lateral flaps of Thelodus represent pectoral fins, then we should have the exceedingly strange phenomenon of such structures becoming functionally useless by enclosure in hard unyielding plates, though still influencing the general outline of the fish. Be that as it may, can we doubt that in Drepanaspis we have a form derived by specialisation from a Ccelolepid ancestor ? This Drepanaspis throws likewise a much-desired light on the fragmentary Devonian remains known since Agassiz’s time as Psammosteus. These consist of large plates and fragments of plates, composed of vaso-dentine, and sculptured externally by minute closely set stellate tubercles, exactly resembling the scales of some species of Thelodus. These tubercles are also frequently arranged in small polygonal areas, reminding us exactly of the small polygonal plates of Drepanaspis, and, like them, often having a specially large tubercle in the centre. That Psam- pase had an ancestry similar to that of Drepanaspis can also hardly be oubted. Finally, in the well-known Pteraspis of the Upper Silurian and Lower Devonian formations we have a creature which also has the head and anterior part of the body enveloped in a carapace, to which a tail covered with rhombic scales is appended behind, and, though the caudal fin has never been properly seen, such remains of it as have occurred distinctly indicate that it was heterocercal in its contour. The plates of the carapace have a striking resemblance in general arrangement to those of Drepanaspis, though the small polygonal pieces have disappeared, and there is a prominent pointed rostrum in front of the mouth; and it is to be noted that the small round apertures usually supposed to be orbits are in a position quite analogous to that of the sensory pits in Drepanaspis. The plates of the carapace of Pteraspis are not, however, tuberculated, but orna- mented by fine close parallel ridges, the microscopic structure of which, along with their frequent lateral crenulation, leaves no doubt in our minds that they have been formed by the running together in lines of Zhélodus-like shagreen grains. An aperture supposed to be branchial is seen on the plate forming the posterior angle of the carapace on each side. Until these recent discoveries concerning the Coelolepide and Drepanaspidie, Pteraspis and its allies, Cyathaspis and Paleaspis, constituted the only family included in the order Heterostraci of the sub-class Ostracodermi, distinguished, as shown by Lankester, by the absence of bone lacunz in the microscopic structure of their plates. It is now, however, clear that we can trace them back to an ancestral family in which the external dermal armature was still in the generalised form of separate shagreen grains or spinelets. TRANSACTIONS OF SECTION D. Vie But the Ostracodermi are usually: made to include two other groups or orders, namely the Osteostraci and the Asterolepida.! The Osteostraci are distinguished from the Heterostraci by the possession of lacunee in their bone structure, and by having the eyes in the middle of the head- shield instead of at the sides. Cephalaspis, which occurs from the Upper Silurian to the top of the Devonian, is the best known representative of this division, In- stead of a carapace, we find a large head-shield of one piece, though its structure shows evidence of its having been originally composed of a mosaic of small poly- gonal plates, and it is also to be noted that the surface is ornamented by small tubercles, there frequently being one larger in size in the centre of each polygonal area. The posterior-external angles of the shield project backwards in a right and left pointed process or cornu, scarcely developed in C. Murchisoni, internal to which, and also organically connected with the head-shield, is a rounded flap- like structure, which strongly reminds us of the lateral flaps of the Ccelolepide. The body is covered with scales, which on the sides are high and narrow; there is a small dorsal fin, and the caudal, though heterocercal, is not bilobate. It is scarcely necessary for me to add that we find just as little evidence of jaws or of teeth as in the case of the Heterostraci. The association of the Heterostraci and Osteostraci in one sub-class of Ostra- codermi has been strongly protested against by Professor Lankester and Dr. O. M. Reis, but here the Scottish Silurian strata come to the rescue with a form which I described last year under the name of Ateleaspis tessellata, and of which some more perfect examples than those at my disposal at that time have recently come to light through the labours of Mr. Tait, of the Geological Survey of Scotland. Here we have a creature whose general form reminds us strongly of Thelodus, but whose close affinity to Cephalaspis is absolutely plain, were it only on account of the indications of orbits on the top of the head: The expanded anterior part which here represents the head-shield of Cepha- laspis shows not the slightest trace of cornua, but forms posteriorly a gently rounded lobe on each side, clearly suggesting that the cornual flaps of Cephalaspis are homologous with and derivable from the lateral expanses in the Ceelolepide. This cephalic covering is composed of numerous small polygonal plates like those of which the head-shield in Cephalaspis no doubt originally con- sisted, and the minute tubercles which cover their outer surfaces also suggest that the superficial layer was formed by the fusion of Coelolepid scales. The body is covered with rhombic scales, sculptured externally with tubercles and wavy trans- verse ridges, and arranged in lines having the same general direction as the scutes of Cephalaspis, from which we may infer that the latter originated from the fusion of scales of similar form. The fins are as in Cephalaspis, there being one small dorsal situated far back, and a heterocercal caudal, which is triangular in shape, and not deeply cleft into upper and lower lobes as in the Coelolepide. Finally, the scales, on microscopic examination, show well-developed bone lacunz in their internal structure. That Ateleaspis belongs to the Osteostraci there is thus not the smallest doubt, but its general resemblance to the Ccelolepide in its contour anteriorly led me to regard it as an annectent form, and consequently to believe that there is after all a genuine genetic connection between the Heterostraci and the Osteostraci. And I have not seen reason to depart from that opinion even though Ateleaspis turns out to be still closer to Cephalaspis than was apparent in the original specimens. If this be so, then Cephalaspis, as well as Pteraspis and its allies, is traceable to the Coelolepidse, shark-like creatures in which, as we have already seen, the dermal covering consists of small shagreen-like scales, or of minute hollow spines, and consequently all theories as to the arthropod origin of the Ostracodermi, so far as they are founded on the external configuration of the carapace in the more 1 To these I myself recently added a fourth, the Anaspida, for the remarkable Upper Silurian family of Birkeniide, but as these throw no light as yet on the problem ef Descent they may at present be only mentioned. 774 REPORT—1900. specialised forms, must fall to the ground, And from the close resemblance of these scales of Thelodus to Elasmobranch shagreen bodies—for forty-five years they had been, by most authors, actually referred to the Selachii—I concluded that the Ccelolepidee owed their origin to some form of primitive Elasmobranchs. That is, however, not in accordance with the view of the late Professor Cope, that the Ostracodermi are more related to the Marsipobranchii, and that, from the apparent absence of lower jaw, they should be placed along with the last-named group in a class of Agnatha, altogether apart from the fishes proper. And Dr. Smith Woodward, who is inclined to favour Cope’s theory, has expressed his view that the similarity of the Ccelolepid scales to Elasmobranch shagreen is no proof of an Elasmobranch derivation, but that such structures, representing the simplest form of dermal hard parts, may have originated independently in far distant groups.1 Knowing what we do of the occurrence of strange parallelisms in evolution, it would not be safe to deny such a possibility. But as to a Marsipobranch affinity, I would point out that the apparent want of lower jaw among the hard parts which nature has pre- served for us is no proof of the absence of a Meckelian cartilage among the soft parts which are lost to us for ever; and also, as Professor Lankester has remarked, that there is no evidence whatever that any of the creatures classed together as Ostraco- dermi were monorhinal like the Lampreys. The only fossil vertebrate having a single median opening, presumably nasal, in the front of the head is Pal@o- spondylus, but, whatever be the true affinities of this little creature, at present the subject of so much dispute, I think we may be very sure that it is not an Ostracoderm, The Devonian ‘ Antiarcha’ or Asterolepida, of which Pterichthys is the best lmown genus, are also usually placed in the Ostracodermi, with which they agree in the possession of a carapace of bony plates, in the absence of distinct lower jaw or teeth, in the non-preservation of internal skeleton, and in having a scaly tail furnished with a heterocercal caudal fin, and, as in the Cephalaspide, also with a small dorsal. But they have in addition a pair of singular jointed thoracic limbs, evidently organs of progression, which are totally unlike anything in the Osteostraci or in the Heterostraci, or indeed in any other group of fishes. These limbs are covered with bony plates and hollow inside; but though I once fancifully compared them in that respect with the limbs of insects, I must protest strongly against this expression of mine being quoted in favour of the arthropod theory of the deriva- tion of the Vertebrata ! Nor do I think that there is any probability in the view published by Simroth nine years ago,” namely, that Pterzchthys may have been a land animal which used its limbs for progression on dry ground, and that the origin of the heterocercal tail was the bending up of the extremity of the vertebral axis caused by its being dragged behind the creature in the act of walking. That view was promulgated before the discovery of the membranous expanse of the caudal fin in this genus. But though the Asterolepida are apparently related to and inclusible in the Ostracodermi, the geological record is silent as to their immediate origin, no inter- mediate forms having been found connecting them more closely with either the Heterostraci or the Osteostraci. In the possession of bone lacunz and of a dorsal fin they have a greater resemblance to the latter, but it may be looked upon as certain that they could have had no direct origin from that group. As regards the Ostracodermi as a sub-class, they become extinct at the end of the Devonian epoch, and cannot be credited with any share in the evolution of the fishes of more recent periods, not even if we restore the Coccosteans or Arthrodira to their fellowship. ‘To the latter most enigmatical group, which I shall still continue to look upon as fishes, I shall make some reference further on. Coming now to say a word regarding the Elasmobranchii, it is plain from the fin-spines found in Upper Silurian rocks that they are of very ancient origin, and that if we only knew them properly they would have a wonderful tale of evolution 1 Geol. Mag., March 1900. 2 «Die Entstehung der Landthiere,’ Leipzig, 1891. TRANSACTIONS OF SECTION D. 779 to tell. But their internal skeleton is from its nature not calculated for preserva- tion, and for the most part we only know those creatures from scattered teeth, fin-spines, and shagreen, specimens showing either external configuration or internal structure being rare, especially in Paleozoic strata. But from what we do know, there is no doubt that the ancient sharks were less specialised than those of the present day, and that the recent Notidanids still preserve peculiarities which were common in the Selachii of past ages. If we ask whether the fossil sharks throw any light on the disputed origin of the paired limbs, whether from the specialisation of right and left lateral folds, or whether that type of limb called ‘ archipterygium’ by Gegenbaur, consisting of a central jointed axis with pre- and post-axial radial cartilage attached, was the original form, I fear we get no very definite answer from Klasmobranch paleon- tolory. The paired fins of the Upper Devonian shark, Cladoselache, as described by Bashford Dean, Smith Woodward, and others, seem to favour the lateral fold theory, and Cope pointed to the right and left series of small intermediate spines which in some Lower Devonian Acanthodei (Parevus and Climatius) extend between the pectorals and ventrals as evidence of a former cortinuous lateral fin. So also, if 1 am right in looking on the lateral flaps of the Coelolepide as fins, the’ evidence of these ancient Ostracodermi would be in the same direction. But, on the other hand, we have the remarkable group of Pleuracanthidie, extending from the Lower Permian back to the Upper Devonian, in which the aired fins are represented by an ‘archipterygium’ which in the pectoral at least is biserial. From this biserial ‘archipterygium’ in the Pleuracanthidee, Professor A. Fritsch, ten years ago,' derived the tribasal arrangement of modern sharks, much according to the Gegenbaurian method, effecting, however, a compromise with the lateral fold theory by assuming that the Pleuracanth form originated from one, consisting of simple parallel rods, like that described in Cladoselache. In my description of the pectoral tin of the Carboniferous Cladodus Netlsoni * I have shown that the cartilaginous structures apparently present a uniserial archipterygium intermediate between the arrangement in Plewracanthus and that in the modern sharks, but I felt compelled to acknowledge that the specimen might also be interpreted in exactly the opposite way, namely, as an example of a transi- tion from the ‘ ptychopterygium’ of Cladoselache to the Pieuracanth and Dipnoan limb. And so in fact this tin of Cladodus is claimed in support of their views by both parties in the dispute. When we add that Semon emphatically denies that there is any proof for considering that the pectoral fin of Cladoselache is primitive in its type,? and that Campbell Brown, in his recent paper on the Mesozoic genus Hybodus,* supports Gegenbaur’s theory, it will be seen that Elasmobranch palzontology has not as yet uttered any very clear or decided voice on the question as to whether the so- called archipterygium is the primary form of paired fin in’ the fish, or only a ‘secondary modification. We shall now inquire if we can obtain any more light ‘on the subject from the Crossopterygii and Dipnoi. The Crossopterygii are a grcup of Teleostomous fishes, characterised externally by their jugular plates and lobate paired fins, and represented in the present day only by the African genera Polypterus and Calamoichthys, which together form the peculiar family Polypteride. The Crossopterygii appear suddenly in the middle of the Devonian period, their previous ancestry being unknown to us. Your families ® are known to us in Paleozoic times—the Osteolepide, Rhizo- 1 «Fauna der Gaskohle und der Kalksteine der Permformation Béhmens,’ vol. iii, pf. i. (Prague, 1890), pp. 44-45. ? Trans. Geol. Soe. (Glasgow), vol. xi. pt. 1, 1897, pp. 41-50. 3 «Die Entwickelung der paarigen Flossen des Ceratodus Forsteri.’ Jena, 1898. +*Ueber das Genus Hybodus und seine systematische Stellung,’ Paleonto- graphica, vol. xlvi. 1900. ° Five, if we include the singular and still imperfectly known Tarrasiidw of the Lower Carboniferous, 776 REPORT—1900. dontide, Holoptychiidx, and Cceelacanthide, but it is only with the first three that we have at present to deal. The Osteolepide and Rhizodontide, which appear together in Middle, and die out together in Upper Paleozoic times, resemble eavh other very closely. In both we have the paired fins, more especially the pectoral, obtusely or subacutely lobate: there are two separate dorsal fins, one anal, and the other caudal, which is usually heterocercal, though in some genera it is more or less diphycercal. In both the teeth are conical and have the same complex structure, the dentine being towards the base thrown into vertical labyrinthic folds, exactly as in the Stegocephalian Labyrinthodonts, and this along with the lung-like development of the double air-bladder in the recent Polypteride has given rise to the view that from these forms the Stegocephalia have originated. The nasal openings must have been on the under surface of the snout, as in the Dipnoi. Of these two so closely allied families we must conclude that the Osteolepide are the more primitive, as in them the scales are acutely rhombic and usually covered with a thick layer of ganoine, while in the Rhizodontidx they are rounded, deeply imbricating, and normally devoid of the ganoine layer, which, however, occasionally recurs on the scales of Rhizodopsis and the fin-rays of Gyroptychius. What then of the structure of the paired fins? Fortunately in the Rhizodont genera Tristichopterus and Eusthenopteron the internal skeleton of the lobe was ossified, and what we see clearly exhibited in the pectoral of some specimens is striking enough. We have a basal piece attached to the shoulder-girdle and followed by a median axis of four ossicles placed end to end. The first of these shows on its postaxial margin a strong projecting process, while to its preaxial side, close to its distal extremity, a small radial piece is obliquely articulated, and a similar one is joined also to the second and third segments of the axis, The arrangement in the ventral fin is essentially similar. In fact we have in the Rhizodontide a short uniserial ‘archipterygium,’ and the question is, Has this been formed by the shortening up and degeneration of an originally elongated and biserial one, or on the other hand do we find here a condition in which the stage last referred to has not yet been attained? This question is inseparable from the next, whether the Rhizodonts or the Holopty- chians form the most advanced type. The Holoptychiidze resemble the Rhizodontide extremely closely in their external head-bones, in their rounded, deeply imbricating scales, and in the form and arrange- ment of their median fins. But the teeth show a more complex and specialised structure than those of the Rhizodontide ; the simple vertical vascular tubes formed by the repeated folding of the dentine in that family being connected by lateral branches around which the dentine tubules are grouped in such a way as to give rise in transverse sections to a radiating arborescent appearance; hence the term ‘ den- drodont.’ In this respect, then, the Holoptychiidze show an advance on the Rhizo- dontidee—what then of the paired fins? While the ventral remains subacutely lobate, as in the previous family, the pectoral has now assumed an elongated acutely lobate shape, with the fin-rays arranged along the two sides of a central scaly axis exactly as in the Dipnoi; and though the internal skeleton has not yet been seen, yet, judging by analogy, we cannot escape the belief that it was in the form of a complete biserial ‘ archipterygium.’ What, then, is the condition of affairs in the oldest known Dipnoan ? The oldest member of this group with whose configuration we are acquainted is Dipterus, which likewise appears in the middle of the Devonian period simultaneously with the Osteolepidse, Rhizodontide, and Holoptychiide. In external form it closely resembles a Holoptychian, having a heterocercal caudal fin, two similarly placed dorsals, one anal, and circular imbricating scales, which, however, have the exposed part covered with smooth ganoine. But now we have the ventrals as well as the pectorals acutely lobate in shape, and presumably archi- pterygial in structure; the top of the head is covered with many small plates, there is no longer a dentigerous maxilla, the skull is autostylic, and the palatopterygoids and the mandibular splenial are like those of Ceratodus and bear each a tooth-plate with radiating ridges. Now, comparing Dipterus with the recent Ceratodus and Protopterus, the first TRANSACTIONS OF SECTION D. V10 conclusion we are likely to draw is, that the older Dipnoan is a very specialised form, that its héterocercal tail and separate dorsals and anal are due to specialisa- tion from the continuous diphycercal dorso-ano-caudal arrangement in the recent forms, that the Holoptychiide were developed from it by shortening up of the ventral archipterygium, as well as by the changes in cranial structure, and that the Rhizodontidx and Osteolepide are a still more specialised series in which the pectoral archipterygium has also shared the fate of the ventral in becoming shortened up and uniserial. Five years ago, however, M. Dollo, of the Natural History Museum at Brussels, the well-known describer of the fossil reptiles of Bernissart, proposed a new view to the effect that the process of evolution had gone exactly in the opposite direction ; 1 and after long consideration of the subject I find it difficult to escape from the conclusion that this view is more in accordance with the facts of the case, though, as we shall see, it also has its own difficulties. T have already indicated above that we are, on account of the more specialised structure of the teeth, justified in considering the Holoptychians, with their acutely lobate pectorals, a newer type than the Rhizodonts, even though they did not survive so long in geological time. What, then, of the question of autostyly ? We do not know the suspensorium of Holoptychius, but that of the Rhizodontidse was certainly hyostylic, asin the recent Polypterus. Now as there can be no doubt that the autostylic condition of skull is a specialisation on the hyostylic form, as seen also in the Chimeroids and in the Amphibia, to suppose that the hyostylic Crossopterygii were evolved from the autostylic Dipnoi is, to say the least, highly improbable ; in my own opinion, as well as in that of M. Dollo, it will not stand. And if we assume a genetic connection between the two groups itis in accordance with all analogy to look on the Dipnoi as the children and not as the parents of the Crossopterygii. M. Dollo adopts the opinion of Messrs. Balfour and Parker that the apparently primitive diphycercal form of tail of the recent Dipnoi is secondary, and caused by the abortion of the termination of the vertebral axis as in various ‘ Teleostei, so that no argument can be based on the supposition that it represents the original ‘ protocercal’ or preheterocercal stage. Very likely that is so, but it is not of so much importance for the present inquiry, as both in the Osteolepidze and Rhizodon- tide we find among otherwise closely allied genera some which are heterocercal, others more or less diphycercal. Diplopterus, for example, differs from Thursius only by its diphycercal tail, and in like manner among the Rhizodontide Tristi- chopterus is heterocercal, Eusthenopteron is nearly diphycercal, and there can be no doubt that, in spite of this, their caudal fins are perfectly homologous structures. But of special interest is the question of the primitive or non-primitive nature of the continuity of the median fins in the recent Dipnoi. Like others I was inclined to believe it primitive, and that the broken-up condition of these fins in Dipterus was a subsequent specialisation, and in fact gave the series Phaneropleuron, Scaumenacia, Dipterus macropterus, and D. Valenciennesti as illustrating this process of differentiation.? This view of course draws on the imperfection of the geological record in assuming the existence of ancient pre-Dipterian Dipnoi with continuous median fins, which have never yet been discovered. But Dollo, using the very same series of forms, showed good reason for reading it in exactly the opposite direction. The series is as follows :— 1. Dipterus Valenciennesii Sedgw. and Murch., from the Orcadian Old Red, and the oldest Dipnoan with whose shape we are acquainted, has two dorsal fins with short bases, a heterocercal caudal, and one short-based anal. 2. Dipterus macropterus Traq., from a somewhat higher horizon in the Orcadian series, has the base of the second dorsal much extended, the other fins remaining as before. ’ ‘Sur la Phylogénie des Dipneustes,’ Bulletin Soc. belge géol. paléont. hydr,, yol. ix. 1895. * Geol, Mag. (3), vol. x. 1893, p. 268, 778 REPORT—1900. 8. In Scaumenacia curta (Whiteaves), from the Upper Devonian of Canada, the first dorsal has advanced considerably towards the head, and its base has now become elongated, while the second has become still larger and more extended, though still distinct from the caudal posteriorly. 4, In Phaneropleuron Andersoni Huxley, from the Upper Old Red of Fife- shire, the two dorsal fins are now fused with each other and with the caudal, forming a long continuous fin along the dorsal margin, while the tail has become nearly diphycercal, with elongation of the base of the lower division of the fin. But the anal still remains separate, narrow, and short-based. 5. In the Carboniferous Uronemus lobatus Ag. the anal is now also absorbed in the lower division of the caudal, forming now, likewise on the hzemal aspect, a continuous median fin behind the ventrals. There is also a last and feeble remnant of a tendency to an upward direction of the extremity of the vertebral axis. 6. In the recent Ceratodus Forsteri Krettt, the tail is diphycercal (secondary diphycercy), the median fins are continuous, the pectorals and ventrals retain the biserial archipterygium, but the cranial roof-bones have become few. 7. In Protopterus annectens Owen, the body is more eel-like, and the paired fins have lost the lanceolate leaflike appearance which they show in Ceratodus and the older Dipnoi. They are like slender filaments in shape, with a fringe on one side of minute dermal rays; internally they retain the central jointed axis of the ‘archipterygium,’ but according to Wiedersheim the radials are gone, except it may be one pair at the very base of the filament. 8. Finally in Lepidosiren paradoxa Fitz. the paired fins are still more reduced, haying become very small and short, with only the axis remaining. From this point of view, then, Dipterus, instead of being the most specialised Dipnoan, is the most archaic, and the modern Ceratodus, Protopterus, and Lepi- dosiren are degenerate forms, and instead of the Crossopterygii being the offspring of Dipterus-like forms, it is exactly the other way, the Dipnoi owing their origin to Holoptychiidee, which again are a specialisation on the Rhizodontide, though they did not survive so long as these in geological time. Consequently the Ceratodus limb, with its long median segmented axis and biserial arrangement of radials, is not an archypterygium in the literal sense of the word, but a deri- vative form traceable to the short uniserial type in the Rhizodonts, But from what form of fin that was derived is a question to which paleontology gives us no answer, for the progenitors of the Crossopterygil are as yet unknown to us. Plausible and attractive as this theory undoubtedly is, and though it relieves the paleontologist from many difficulties which force themselves upon his mind if he tries to abide by the belief that the Dipnoan form of limb had a selachian origin, and was in turn handed on by them to the Crossopterygii, yet it is not without its own stumbling-blocks. : First as to the dentition, on which, however, M. Dollo does not seem to put much stress, it is impossible to derive Dipterus directly from the Holoptychiide, unless it suddenly acquired, as so many of us have to do as we grow older, a new set of teeth. The dendrodont dentition of Holoptychius could not in any way be transformed into the ctenodont or ceratodont one of Dipterus: both are highly specialised conditions, but in different directions. Semon has recently shown that the tooth-plates of the recent Ceratodus arise trom the concrescence of numerous small simple conical teeth, at first separate from each other.' Now this stage in the embryo of the recent form represents to some extent the con- dition in the Uronemidz of the Carboniferous and Lower Permian, which stand quite in the middle of Dollo’s series. Again, the idea of the origin of the Dipnoi from the Crossopterygii in the manner sketched above cuts off every thought of a genetic connection between the biserial archipterygium in them and in the Pleuracanthidz, so that we should have to believe that this very peculiar type of limb arose independently in the Selachii as a parallel development. It may be asked, Why not? We may feel perfectly assured that the autostylic condition of the skull in the Holocephali 1 «Die Zabnentwickelung des Ceratodus Forsteri.’ Jena, 1899, TRANSACTIONS OF SECTION D. 779 arose independently of that in the Dipnoi, as did likewise a certain amount of resemblance in their dentition. But those who from embryological grounds oppose any notion of the origin of the Dipnoi from ‘Ganoids’ might here say, if they chose, If so, why should not also the same form of limb have been inde-~ pendently evolved in Crossopterygii ? Accordingly, while philosophic paleontology is much indebted to M. Dollo for his brilliant essay, and though we must agree with him in many things, such as that the Crossopterygii were not derived from the Dipnoi, and that the modern representatives of the latter group are degenerate forms, yet as to the zmmediate ancestry of the Dipnoi themselves, and the diphyletic origin of the so-called archipterygium, we had best for the present keep an open mind. Tn his ‘ Catalogue of the Fossil Fishes’ in the British Museum (vol. ii. 1891) Dr. Smith Woodward, following the suggestion of Newberry in 1875, classified the Coccosteans or ‘ Arthrodira’ as an extremely specialised group of Dipnoi. At first I was much taken with that idea, but after looking more closely into the subject I began to doubt it extremely. My own opinion at present is that the Coccosteans are ‘leleostomi belonging to the next order, Actinopterygii; but Prof. Bashford Dean, of New York, will not have them to be even ‘fishes,’ but places them in a distinct class of ‘ Arthrognatha,’ which he places next to the Ostracophori (=Ostracodermi), even hinting at a possible union with them, whereby the old ‘ Placodermata’ of McCoy would be restored. It will, therefore, be better to leave them out of consideration for the present, pending a thorough re-examination of their structure and affinities. We come then to the great order of Actinopterygii, to which a large number of the fishes of later Paleeozoic age belong, as well as the great mass of those of Mesozoic, Tertiary, and Modern times. Of these we first take into considera- tion the oldest sub-order, namely, the Acipenseroidei or Sturgeon tribe, in which the dermal rays of the median fins are more numerous than their supporting ossicles, while the tail is, in most, completely heterocercal. And the oldest family of Acipenseroids with which we are acquainted is that of the Paloniscide, which, in addition to well-developed cranial and facial bones, has the hody normally covered with rhombic ganoid scales furnished with peg-and-socket articu- lations. Of this family one genus, Chezrolepis, appears in the same Devonian strata (Oreadian series) with the earliest known Crossopterygii, and of its immediate ancestry we know no more than we do of theirs. Chetrolepis is a fully evolved paleeoniscid, as shown by its oblique suspensorium, wide gape, and other points of its structure. In the Lower Carboniferous rocks of Scotland, where the family attains an enormous development, we find one or two genera, e.g. Canobius, which appear less specialised, as the suspensorium is nearly vertical, and the mouth consequently smaller. This family endures up to the Purbeck division of the Jurassic formation, and in the Carboniferous Cryphiolepis, the Lower Permian Trissolepis, and the Jurassic Coccolepis we find the same degeneration of the rhombic scales into those of a circular form and imbricating arrangement, which we find repeated in other groups of ‘Ganoids.’ In fact, in one Carboniferous genus, Phanerosteon, the scales disappear altogether with the exception of those on the body prolongation in the upper lobe of the caudal fin, and a few just behind the shoulder-girdle. And in these Paleozoic times we notice also a side branch of the Paleoniscide, constituting the family Platysomide, in which, while the median fins acquire elongated bases, the body becomes shortened up and deep in contour. The scales become high and narrow, their internal rib and articular spine coincident with the anterior margin; the suspensorium, too, instead of swinging back as in the typical Palzoniscidze, tends to be directed obliquely forward, while the snout becomes simultaneously elongated in front of the nares. A most interesting series of forms can be set up, beginning with ZEurynotus, which, though it has the platysomid head contour and a long-based dorsal, has only a slight deepening of the body, and still retains the paleoniscid squamation and a short Bistot anal fin. In Mesolepis, which resembles Eurynotus in shape, being only slightly deeper, we have now the characteristic platysomid squamation, 780 REPORT—1 900, and the base of the anal fin is considerably elongated. Platysomus has a still more elongated anal fin, and the body is rhombic; while in Chezrodus the body is still deeper in contour, with peculiar dorsal and ventral peaks, long fringing dorsal and anal fins, while the ventrals seem to have disappeared altogether. Here also, as in the allied genus Chezrodopsis, the separate cylindro-conical teeth characteristic of the family are, on the palatal and splenial bones, replaced by dental plates, remind- ing us of those of the Dipnoi. Certainly the Platysomide seem to me to forma morphological series telling as strongly in fayour of Descent as any other in the domain of paleeontology.? If we now return to the Palwoniscidee we find that they dwindled away in numbers in the Jurassic rocks, and finally hecame extinct at the close of that epoch. But already in the Lias (leaving the Triassic Catopteride out of considera- tion for the present) we find that they have sent off another offshoot sufficiently distinct to be reckoned as a new and separate family, namely, the Chondrosteide, in which the path of degeneration, in all but the matter of size, seems to have been entered on. In the genus Chondrosteus, though the paleoniscid type is clearly traceable in the cranial structure, there is marked degeneration as regards tne amount of ossification, and though the suspensorium is still obliquely directed backward the toothless jaws are comparatively short, and the mouth seems now to have become tucked in under the snout as in the recent sturgeon. Then the scales have entirely disappeared from the skin except on the upper lobe of the heterocercal caudal fin, where they are still found arranged exactly as in the Palxoniscidee. Chondrosteus in fact conducts us to the recent Acipenseroids—the Poly- odontidz (Paddle-fishes) and Acipenseridz (Sturgeons). The first of these resembles Chondrosteus in the nakedness of the skin, except on the upper lobe of the caudal fin,? the more paleoniscid aspect of the external cranial plates, such of them as remain, for they are now still further reduced. But in front of the mouth and eyes there is an addition in the form of an enormous vertically flattened paddle-shaped snout covered above and below with a large number of small ossitications. The sturgeons have, however, nearly altogether lost the paleoniscid arrange- ment of the cranial roof-bones, which, strange to say, now exhibit an arrangement reminding us of that in Dzpteruws, and the external facial plates are still more reduced than even in Polyodon; but we may note a very strong resemblance to Chondrosteus in the position of the mouth, the edentulous jaws, and the jugal bone, indeed also in the palatal apparatus. So the sturgeons and paddle-fishes of the present day would seem to be the degenerate, though bulky, descendants of the once extensively developed group of Palzoniscide, even as the modern Dipnoi are degenerated from those of Paleozoic times. We now notice another apparent offshoot of the Paleoniscide, namely, the family of Catopteridee (Catopterus and Dictyopyge), which is limited to rocks of Triassic age. Unfortunately the osteology of the head is not well known, but Dr. Smith Woodward’s observations are to the effect that both the head and shoulder- girdle are of paleoniscoid type. The relationship of these small fishes to the Paleeoniscidze is shown by the general shape, the number and position of the fins, the rhombic ganoid scales, and the close arrangement of the rays of the median fins. But the rays of the dorsal and anal fins are now almost equal in number to their supporting ossicles, and the tail has become only abbreviate heterocercal. That is to say, the caudal body prolongation no longer proceeds to the termination of the upper lobe, which is reduced in size and in the number of its rays. The 1 R. H. Traquair, ‘Structure and Affinities of the Platysomider,’ Trans. Roy. Soc. Edin. xxix, 1879, pp. 343-391. 2 Collinge has, however, found rudimentary scales in the skin of the recent Polydon folium (Journ. Anat. and Phys. ix. pp. 485-487), and Cope has described an allied Hocene genus, Crossopholis, in which minute scales are seen (Mem. Vat. Acad, Sciences, iii, 1886, pp. 161-163), TRANSACTIONS OF SECTION D. 781 Catopterid are obviously an annectent group, as, although from their abbreviate heterocercal tail they have usually been placed in the next sub-order, Dr. Smith Woodward prefers to look upon them as Chondrostei (¢e. Acipenseroidei).' Wherever we place them they express the beginning of a set of changes towards a more modern type of fish, which are emphasised in the great series of Lepidos- teoid fishes (Protospondyli+ Atheospondyli of Smith Woodward), being the fishes more or less allied to the recent Bony Pike of North America. But these changes must have been well advanced before the Triassic era, for already in the Upper Permian occurs the genus - - - » 0°36 oc on the twenty-first day, the loss being proportional to their size and weight, the total loss during the twenty-one days being INN On a : : 6 : = . 794 grammes Se, 9 eae ee Othe : , : : : moo | i, when the chicks chipped the shells and hegan life on their own account. The other three eggs were not fertile, but during the twenty-one days lost weight also, on the first day losing inNo.4 . : : : : : . 0-23 gramme SOs De URNS FEC Fo. eee Ons 3 : 5 - 5 . 0:33 Ay the loss in No. 4 reaching 0°30 gramme on the 21st day ” ” 5 ” 0:47 ” ” ” ” ” 6 ” 0°32 ” ” ” the totals being No.4 . . E c B : . 534 grammes ty GeueKe Ya camrsdtiird'} 2b) elephant » 6 : ’ ' ; ThE LS eee, The average weight of each of the fertile egzs was 56:93 grammes, falling to 49-65 grammes on the day before the chicks liberated themselves from the shells. Thus the average loss sustained by each egg was 7°38 grammes, or 12-96 per cent ; so that the average loss per egg per day was 0°35 per cent. As the results from the unfertile eggs were useless for comparison, a fresh egg was employed to determine the weight of water and solid matter respectively. The egg weighed . : : : : : F ° - 68-40 grammes The shell and membrane (moist, 6:92) . : . ; . 5:80 Fe dry) The weight of yolk, albumen, and water in egg and membrane was. - : : : - A . 52°60 51°45 grammes of the egg were dried et 101° C., and gave of Dry matter . . ° = . 13:18 grammes, or per cent. 25:617 Moisture . . - “ : - 38:27 np Pr a 74:383 100-000 A newly hatched chick, weighing 40:8 grammes, was dried in the same manner, and after the moisture had been driven off there was left Dry matter . . : - . 10°9 grammes, or per cent. 26°715 Moisture . A i F a EO “e a 5 73:285 100°000 3E2 788 REPORT—1900. These results are curious and interesting, for they seém to show that the proportions of water and solid contents are practically the same in the fresh egg and in the newly hatched chicken. Ultimate analyses were made of the dry matter contained in the fresh egg and in the dried chicken. After deducting the weight of the shell and water from the total weight of the egg, there remained 13:21 grammes of dry matter, This gave on analysis Ash . ° > . 0568 gramme, or percent. 4°30 of dry matter Nitrogen . ‘ aon Le a = 4 Bl ss 5 Hydrogen . : sy szO2 AS a 5 0 oe 3 Oxygen } a Ud 2°295 ” ” ” 17:38 ” ” Carbon . - © 7972 ” 55 ; 60°35 , i 13:208 grammes 100:00 per cent. The same method of analysis showed the dried chicken to consist of Ash . ‘ + . 0'676 gramme, or per cent. 6:20 of dry matter Nitrogen . - a alone ny 5. - 10:00, 5 2 Hydrogen . : . 0892 5 ib “1 SB iss ” Oxygen . fk . 2261 oy + 5 20°62 =O, 7 Carbon . 4 . 6:000 or “ i B00" 5 3 10:920 grammes 100-00 per cent. Results. Ash was raised by . : : : . . 1:90 gramme per cent. Nitrogen was raised by . : A ‘ peels L Hs Hydrogen was lowered by : : : - 0:92 a a Oxygen was raised by . é rs ‘ . 3°24 * 5 Carbon was lowered by . ‘ J . . 535 35 - The increase of ash in the chicken is obviously due to lime being absorbed from the shell, and combined with phosphorus present in the yolk. The increase of nitrogen (equal to 1:13 per cent.) is apparently due to the decrease of carbon. ‘This also applies to the increase of oxygen. ‘The decrease of carbon (5°35 per cent.) and hydrogen (0°92 per cent.) is due to their oxidation, ahd may be (in part) accounted for as carbonic acid and water passing through the shell during incubation. Seemingly we have a rearrangement of the elements above named, and the fact established that water becomes altered into potential living matter, repre- senting the tissues and feathers of the living bird, &c., whilst the ash is also increased by the abstraction of lime from the shell, combined with the phosphorus derived from the yolk during the hatching process. 4. On the Physiological Effect of Local Injury in Nerve. By Professor F. Gotcn, /.2.8. 5. Report on the Comparative Histology of the Suprarenal Capsules. See Reports, p. 452. 6. Report on the Vascular Supply of Secreting Glands. _ See Reports, p. 458. 7. Report on Electrical Changes in Mammalian Nerve See Reports, p. 455. TRANSACTIONS OF SECTION D. 789 8. Report on the Comparative Histology of Cerebral Cor em, See Reports, p. 453, 9. Report on the Micro-chemistry of Cells—See Reports, » 449. 10, Observations on the Development of the Cetacean Flipper. By Professor JoHNsoN SYMINGTON. 11. The Articulations between the Occipital Bone and Atlas and Axis in the Mammalia. By Professor Jonnson SYMINGTON. MONDAY, SEPTEMBER 10. The following Papers and Report were read :— 1. Mnestra parasites, Krohn. Preliminary Account. By R. T. Gtnruer, WA., F.R.GS., Magdalen College, Oxford. During the spring of the present year the prevailing westerly winds no doubt contributed to the fact that an unusually large number of Phyllirhoé bucephala were ‘captured in the Bay of Naples. I examined every specimen I could get hold of and found that of thirty-one individuals of Phyllirhoé taken between March 28 and April 20 nineteen, or more than half, had a Mnestra adhering to them. My friend Cavaliere Lo Bianco in the kindest way placed his store of spirit-preserved material at my disposal for examination. Unfortunately the dates of capture were not noted, but of forty-three Phyllirhoé every one had or had had a Mnestra upon it. From this relative abundance of the parasite it follows that the reproductive power of the Mnestra must be far and away in excess of that of the Phyllirhoé bucephala of the Bay of Naples. Indeed, the fertility of Mnestra must, one would think, be greater than is usual even among parasites. It is therefore most remark- able that hitherto the method of the propagation of Mnestra should have remained undiscovered. We do not know whether it reproduces itself by a sexual or an asexual process, by eggs or budding. It was in consequence of our ignorance of this point that systematists have not been able to assign Mnestra to its proper place in the system of Haeckel—which primarily depends upon the place of development of the genital cells in the Medusa. I have, however, been fortunate enough to discover other characteristics of the Mnestra which will enable us to unhesitatingly affirm that it should be classed with the Cladonemide, a family of the Anthomeduse. The Mnestra is attached to the Phyllirhoé by its manubrium, which is com- paratively short and serves the purpose of obtaining nutriment, apparently by sucking the blood of the host. The shape of the body of the Mnestra varies greatly. The margin of the umbrella is sometimes notched, but this marginal notch is by no means so constaht in its presence as to justify us in regarding it as Claus! did, a characteristic of Mnestra. The shape of the Medusa can be well described as that of a bun with a large inpushing or ‘dimple’ in the middle of the exumbral surface, from which, in typical cases, four furrows proceed interradially to the margin. It is by the intensification of one of these grooves that the notch of Claus is often produced. The symmetry of the velum and circular canal is generally not much affected by these furrows on the surface of the ex-umbrella. The tentacles are four in number. The majority of specimens examined had two reduced to mere knobs, and some had three or even all the tentacles reduced to this condition. It seemed to me that the reduction of the tentacle was a mark 1 Claus, Verh, Zool, Bot, Tyst., Wien, xxv, 1876, 790 ‘ REPORT—1900, of old age. A well-developed tentacle of Mnestra is a compound tentacle of undoubted Cladonemid type. The base is swollen and simple, but the distal portion is slender and tapering, with a row of small stalked multinucleate club- shaped bodies along the entire length of one margin. These bodies contain nematocysts, and they are undoubtedly homologous with the stalked clubs containing thread cells of many of the Cladonemid genera. A further point of resemblance between Mnestra parasites and certain of the Cladonemidee is in the fact that there is a circular tract of nematocysts arranged round the umbrella margin, close to the circular canal, and from this circular tract extend four centripetal tracts along the perradii of the ex-umbrella, These perradial tracts usually extend as far as the exumbral ‘dimple’ and sometimes continue down into it. The gastro-vascular system is of the usual type. There are a central stomach, four radial canals, and a circular canal. ‘The stomach is of an irregular shape and is often provided with irregular diverticula in which corpuscles which originally belonged to the blood of the Phyllirhoé may sometimes be seen. The mouth is clogged with endoderm cells with intercellular spaces through which the organism imbibes its nutriment. Among the 100 odd individuals examined a number of varieties and abnormal forms were observed. A description of these as well as the histology of Mnestra will shortly be published in the Naples ‘ Mittheilungen,’ 2. The Respiration of Aquatic Insects. By Professor L. C. Miaut, F.R.S, 3. The Tracheal System of Simulium : a Problem in Respiration. By T. H. Tayzor. 4, The Pharynz of Eristalis. By J. J. W1LKrNson. 5. The Structure and Life History of the Gooseberry Sawfly. By N. WALKER. 6. Report on the Coral Reefs of the Indian Region.—See Reports, p. 400. 7. Contributions to the Anatomy and Systematic Position of the Lemargide. By Professor R. BurckHarpt. 8. On the Nestling of Rhinochetus. By Professor R. BurckHarptT. 9. The Dentition of the Seal. By R. J. Anperson, If,A., ID., Professor of Natural History, Galway. The dentition of the common seal is generally understood to be in the great majo- rity of cases 3 I.,} C., 4 P.-m.,4.M. ‘There may be an additional premolar, due to the persistence of one of the milk-teeth. The molars are not too much crowded in the upper jaw, but more so in the lower. The incisors have standing room, but the central of the lower jaw show a disposition to stand back; the small platform on which the latter seem to stand narrows anteriorly, and the sockets are deeply | sunk in front of this plane. The four incisors of the ower jaw correspond to the TRANSACTIONS OF SECTION D. : 791 - inner four of the upper jaw when the teeth are met, and are about the same size as these latter, whilst the two upper lateral incisors are larger than the inner two, but are far removed from the canines both in position and size. The comparison of the dentition of the seal with that of the polecat, the grison, and especially the otter, is instructive. The badger may be said to occupy a place between bears and weasels, and the upper incisors have carnivor type, formula, and arrangement. In the upper set the incisors are not embarrassed, although they stand three abreast on each side, as in better marked carnivors. In the badger the intermediates in the lower jaw stand back out of range, asin Putorius and Galictis. In the upper jaw of the otter the incisors are in range, but the second incisors of the lower jaw stand back, as if the teeth were crushed up. It is noteworthy that the first premolar of the upper jaw in this animal is placed internal to the canine, while the first pre- molar of the lower jaw is placed at an interval behind the canine. All the molar teeth of the common seal except the first are well known to have two fangs; as regards the cusps, the precise arrangement is not generally stated. The cusps of the upper molars fit into intervals between the cusps of one lower molar or of separate adjacent molars. The first premolar has a large front cusp with a shoulder (an approach to the formation of a cusp) in front, and a small cusp behind. A slight groove passes forwards and inwards, marking off an enamelled surface internal to the cusps. The second upper premolar has a large central cusp, a shoulder in front and to the inner side of this; and two cusps, one immediately behind the larger and one still farther back. The third premolar has a shoulder in front and internal to a large cusp; then there are two smaller cusps in succes- sion to this posteriorly. The fourth has a blunter chief cusp, slight irregularities on the inner shoulder, and a second cusp, with an attempt at the formation of a third cusp still farther back; this tooth is more like the last molar of the otter than the previous teeth are. The molar has a large middle cusp, with a slightly smaller one behind it and a small cusp anteriorly. The first lower premolar has three cusps; the anterior is the smallest, and the central one next. The cusps are placed near the outer surface of the tooth; internal to and behind the middle one is an elevation suggestive of a fourth cusp. The second premolar has a large cen- tral cusp curved somewhat back, a small cusp in front of this, and two behind; there is a platform internal to the cusps. The ¢Aird premolar has fowr cusps: the front cusp small, the second the largest and tumed back, the two posterior smaller. The fourth premolar has five cusps: two small ones in front of the large one, and two behind it ; the central cusp is bent back. The molar has one cusp in front of and two behind the central cusp, which is not prominent. This tooth is very small, and has a bulging opposite each of the first three cusps. The contrast in the comparison of the incisors of the lion, hyena, and dog with those in the lower jaw of the badger, the polecat, and otter is well worth noting. In the otter there would not be room for the intermediate (second) incisor to stand in rank. The second incisors in the bear stand somewhat back, but the sockets are placed behind the level of the third pair of incisors. It may seem likely that the habits of the badger and weasel should render a narrow lower jaw desirable anteriorly, but it is not clear that the otter would be well served by the same device. The lower jaw of a very young seal which was examined has lost the lower incisors, but the sockets are suggestive of a nearer approach to the otter arrangement. Halicherus grypus has the same dental formula as the common seal. The last molar of the upper jaw is at some distance from the other back teeth, which are all pointed with single cusps. In some, however, there isa shoulder suggestive ot a second cusp. This is the case in the last lower, where a slight indication of a cusp exists behind the pointed cone. A furrow is visible on the outer sides of the third and fifth lower and second and fifth upper. The lower canines extend between the upper corner incisors and the upper canines, which are about the same length as the corner incisors, but much thicker. The following animals have the intermediate incisor behind the inner and outer, either from base to apex or at the base alone :—Paradoxurus, Ailurus, Her- pestes mungos, Lutra, Galictis, Gulo, Conepatus, Brown Bear, the Malayan Bear, Snow Bear, Polar Bear, and Ursus collaris; Melursus not, Arctoidotherium 7b2 REFORT—1900, Bonariense, Gerv., behind at base, between at apex. In Ursus spelzeus behind. Australian Sea-lion, Otaria pusella, O. stelleri, O, jubata, I. 3. Elephant Seal, I. 3. Crab-eating Seal, Monachus, and Onomatophora, I. 3. The innermost is far back in the last. In Felis tigris the inner and in F. macroscelides the inner and intermediate incisors are somewhat back. 10. Note on Exhibition of Skulls of Antarctic Seals. | Sy G. KE. H. Barrerr-Hamirton. I am indebted to the authorities of the British Museum of Natural History for the opportunity of studying the collection of seals brought home from the antarctic seas by the Belgica, and now the property of the ‘ Expédition Antarctique Belge.’ The collection is not a large one, and consists almost entirely of specimens of the Phocide, the Otariide being represented by only one very immature skull. One of the main points of interest regarding the specimens is the fact that they afford no support whatsoever to the supposition, sometimes advanced, that some startlingly new forms of marine Carnivora will be found to occur in the antarctic seas. All the species known to occur in these seas, except the (perhaps extinct) sea elephant, are represented in the collection. Thus there are skulls of Leptony- chotes weddeli, Ogmorhinus leptonyx, Lobodon carcinophaga, and Ommatophoca rossi; but all these are framed on patterns so close to those of the older specimens in the British Museum that it is impossible (with the present material) to find even new sub-specific differences amongst them. At the same time it is highly interest- ing to have a series of specimens of various ages from which to amplify our know- ledge of the various forms. Probably the most interesting species represented in the collection is Ommato- phoca rosstt, of which there are two skulls. These are remarkable for the variability of their dentition ; a point to which Mr. W. Bateson has already drawn attention with reference to the only two previously known skulls. It seems now certain that variability of dentition must be regarded as one of the characteristics of Ross’s seal, and it is interesting to know that this variability is not shared by the other species of antarctic Phocide, all the specimens which I have examined being quite uniform and showing no abnormalities, IT hope at a later date to publish a more detailed account of these skulls. The following were exhibited at the Section:—Omimatophoca rossii (two skulls) and Lobodon carcinophaga. : TUESDAY, SEPTEMBER ll. The following Papers were read : 1. Photographs of some Malayan Insects.2 By Newson ANNANDALE. The photographs were taken from living insects in the Siamese Malay States last year. The first represented a Stawropus larva not dissimilar to the English Lobster Caterpillar on its food-plant, Melastoma polyanthum—the so-called ‘Straits Rhododendron.’ When it is about to change its skin this larva resembles a bird’s dropping, and is then sluggish in its movements; but after the ecdysis has taken place, the insect becomes active again, and keeps its true legs and the pro- cesses on the posterior region of its abdomen in constant agitation. Its colour also changes considerably. The second photograph represented a portion of the stem of a living Areca- valm, with a small Geometrid caterpillar that conceals itself by plastering frag- ments of a powdery lichen upon its own back. The third and fourth photographs showed two species of a peculiar type of larva, supposed to belong to Lycid beetles, and noticeable for its flattened hody, minute ' P.Z.8., 1892, pp. 106, 107. # For details see Proc, Zool. Soc., London, Noy. 1900. Se TRANSACTIONS OF SECTION D., 793 retractile head, and for the processes that project in a series along the sides of the abdomen, Nothing is known as to the metamorphosis of these larve, and some examples of the type reach a size considerably greater than that of any Lycid beetle as yet discovered. The two species shown in the photographs are found together, beneath the bark of dead trees and under fallen timber in the jungle. The broader and more highly specialised of the two bears no resemblance, as far as I have been able to discover, to any other animal; but the narrower species, which in its younger stages differs very little from the ordinary type of Lycid larva, is not unlike a Millipede (Orthomorpha sp.) found together with it. The fifth and three following photographs showed a pupa of the mantis Hymeno- pus bicornis seated on an inflorescence of Melastoma polyanthum. In its active pupal stage this insect bears so close a likeness to the flowers of the ‘ Rhododen- dron’ that I have found it impossible to assign the exact limits of true vegetable tissue and animal counterfeit, even when holding in my hand an inflorescence in which one of these mantises was seated. The resemblance is brought about by the development of broad, petal-like expansions of the femora of the second and third pairs of legs, by the pink coloration of the insect, and by the extraordinary nower-like sheen of its integument. A broad bar of vivid green runs across the thorax of the pupa, dividing the animal visually into two perfectly distinct parts: a black spot is most conspicuous on the tip of its abdomen; and five brown lines mark the dorsal surface of the abdomen longitudinally. The mantis refuses to settle on any other part of the plant than the inflorescence. It sits among the flowers with its abdomen flexed backwards, so as to lie almost parallel to the thorax ; and it sways its whole body from side to side, The movement attracts certain minute flies, which settle indiscriminately on the body of the insect (being then indistinguishable at the short distance from tho black tip of the abdomen) and on the petals it simulates. The mantis takes no notice of these small flies, but seizes and devours larger Diptera, and probably other insects, that come within its reach. When the flowers among which it is seated commence to fade, the mantis droops its abdomen, thus bringing the brown lines upon the dorsal surface into view, and finally leaps to the ground. When separated from the inflorescence of Melastoma polyanthum, it resembles an orchid that has fallen from its stem. Hymenopus bicornis has a fairly wide distribution (from Sikkim to Sarawak), but s is rare in every locality where it occurs. A white variety of the pupa is also nown, The ninth photograph showed some Siamese of the State of Patalung clapping their hands to attract the edible cicada (Dundubia intemerata). In April the females of this insect are thus captured in considerable numbers for food, during the short interval between sunset and darkness, The cicada-catchers must clap their hands in unison and observe a definite rhythm. A fire is a usual, but not a necessary, adjunct to the performance. ‘The enormous elongation of the anterior region of the head of many Fulgorinz (lantern flies) into a hollow nose-like organ has often puzzled entomologists, who have generally abandoned the old theory that this structure was lumi- nescent. I was so fortunate as to observe its use as an organ of progression, or rather of sudden flight from danger. When the insect is disturbed, it presses the tip of its ‘nose’ against the tree-stem on which it is seated, at the same instant pushes its body violently away with its powerful legs, and so is projected for a considerable distance through the air, the ‘nose’ being flexible at one point, and also so elastic that it acts as a piece of whalebone would do under like circum- stances. 2. Observations on Mimicry in South African Insects. By Guy A. K. Marsa, [Arranged and communicated by EDWARD B. Poutton, M.A., F.R.S., Fellow of Jesus College, Oxford, and Hope Professor of Zoology in the University. ] The following paper is an abstract of the results obtained by Mr. Guy A. K. Marshall in South Africa, When no locality is mentioned it is to be understood 794 REPORT—1900, that the observation was made at Salisbury, Mashonaland (5,0CO feet). The observations here briefly recorded have added in a most important manner to our knowledge of the natural history (bionomics) of South African insects, a subject of which the foundations were laid by Roland Trimen. Groups of mimetic Lepido- ptera captured on the same day as their models have been obtained both from Natal and Mashonaland (Salisbury), thus demonstrating more fully than has been done hitherto the fact that model and mimic fly at the same time as well as in the same place. The groups bring out the extraordinary power of Danaine butterflies in, so to speak, moulding the species of other sub-families into a superficial likeness to themselves. There are only four or five species of Danaine in the region under consideration, and each one of them is the centre of a group of forms superficially similar, but remote in affinity. The abundant and widespread Limnas chrysippus was largely resembled both in Natal and Mashonaland. In experiments conducted upon insect-eating animals, this butterfly appeared to be less unpalatable than the Acrea (A. encedon) which resembles it. The explanation may be found in the far wider range of the Danaine model, which would render it familiar to enemies passing from an area in which the Acrea does not, to one in which it does exist. In the case of two forms of Ewralia (£.mima and EL. wahibergi) mimicking two very different species of Amavris (A. echeria and A. dominicanus) there is good reason to believe that a single species has become dimorphic. Photographs of four mima (two male, two female) and four wahlbergi (three male, one female) were shown, the whole set having been part of a company of twelve individuals going to rest together on a small clump of fern under a steep kraantz, Umbilo River, Malvern, near Durban, Natal (June 28, 1897). The two forms have also been taken 7” coitw, and have been found together freshly emerged from the pupa on the same tree. Intermediate varieties are also known. Ifspecific identity be established, the case will constitute a new form of mimetic dimorpbism in the Lepidoptera, similar to that of the Dipterous genus Volucella. Allcases of dimorphism in mimetic Lepidoptera hitherto described are either sexual or confined to a singlesex. In one sex, indeed, a mimetic species may be polymorphic, as in the female of Papilio cenea or Hypolimnas misippus. In the case of the distasteful sub-family Acreine, the two very different species A. natalica and A. anemosa were shown captured at Salisbury on the same day. Although entirely different in detail, the pattern of the two species is broadly the same, and during flight would probably appear to be identicai, Another even more striking example of Miillerian or synaposematic resemblance was afforded by a set of eighteen specimens belonging to five species of small Acrzeas captured on the same day (December 31, 1898) in the same locality. The whole group pre- sented a wonderfully uniform appearance in size, shape, colour, and the general distribution of markings. An example of a Hesperid (Baoris netopha) mimic of an Acrea (A. double- dayi), the two captured on the same day, added another to the rare instances of mimicry in this family. The resemblance is only seen in the attitude of rest, and is confined to the undersides of the wings. The aberrant Lycznid (Alena amazoula) has a general Acreine aspect, and is very unlike the well-known appearance of its true family. It is probably dis- tasteful, and is resembled with tolerable closeness, especially upon the under- sides of the wings, by a day-flying Geometrid moth (Petovia dichroaria), They were captured together at Malvern, near Durban, on September 26, 1897, A most interesting series of injured specimens of butterflies showed the probable attacks of birds or lizards, observations in the field affording strong sup- port to this interpretation. Members of the specially protected conspicuous groups were, as Fritz Miller showed in the case of South America, also subject to attack. Comparatively few of the injuries were inflicted at the junction of the fore and hind wings, or indeed anywhere except at the apex of the fore wing, or, more commonly still, at the anal angle of the hind wing. In many cases the injury was symmetrical, indicating that a piece had been bitten out of both right and left wings during the usual attitude of rest, or as they came together momen- tarily in flight. ‘The two points of special attack are commonly rendered con- TRANSACTIONS OF SECTION D. 795 spicuous by special marks, and, in the case of the hind wing, structures such as ‘tails,’ ‘eye-spots,’ &c. In the Lycenide, where the ‘tails’ are rendered still fur- ther prominent by movement, many specimens were captured with these parts bitten out from one or both of the wings. Large additions were also made to our knowledge of mimicry and warning colours in Coleoptera. In the Carabid genus Anthia, a probable warning character common to different species consisted in a large white patch, placed in some species on the sides of the thorax, in others on the anterior surface of the elytra. The general effect was the same, but the anatomical relations entirely alien. The characteristic banded pattern of the Cantharide was shown to be resembled by beetles of widely different groups, the spotted pattern of the Coccinelhde by an Hemipterous insect (Steganocerus multipunctatus), while the appearance of many 8, African species of Lycide, light-brown auteriorly and_black posteriorly, was repreduced in beetles of many groups, many species of Hymenoptera, an Hemi- pteron, two moths from remote sections of the order, anda fly. In the vast majority of these cases of likeness to and among Coleoptera, it is probable that the resemblance is Miillerian (synaposematic) ratver than Batesian (pseudosematic). The interpretation of the remarkable likeness borne by a species of Longicorn (Phantasia gigantea) for certain Curculionide is more uncertain, although it is clear that some general principle is at work, inasmuch as resemblances between other species of the same groups are well known in many parts of the world. An interesting group of superficially similar insects from three different orders con- sisted of a Bracon, a Reduviid bug, and a Longicorn beetle. Evidence of the struggle for existence in Coleoptera was supplied by a group of five beetles taken from the crop of a Guinea-fowl (Mwmida coronata). The four species belonged to the Buprestids, Curculios, Longicorns, and Phytophaga. All the beetles had been swallowed whole and were almost uninjured, even as regards limbs and antenne. Among the other orders of Insecta the Hemiptera afforded a wonderful example of mimicry or common warning colours from Malvern, near Durban, the Reduviid bug Phonoctonus nigro-fasciatus bearing the most remarkable likeness to the somewhat smaller Lygeid Dysdercus superstitiosus. The mimetic resem- blance of Diptera to Aculeate Hymenoptera was illustrated by many examples, model and mimic having been captured in the same place and within the same month. The most remarkable of these was a splendid new species of Hyperechia, closely resembling the black, reddish-brown banded, African species of AXylocopa, such as X. flavo-r rufa. Instances of common warning (synaposematic) colours in Hymenoptera were also illustrated by a group of three species with a general resemblance to each other: the Aculeata being represented by a species of Myzine and one of Ceropales, the Terebrantia by a species of Zchnewmon. All were captured at Salisbury in January 1899. The whole of the material here briefly described may be seen in the Hope Department of Zoology, Oxford University Museum. 3. Observations on Mimicry in Bornean Insects. By R. Suerrorp, B.A., Curator of the Sarawak Museum. [Arranged and communicated by EDWARD B. PouLTON, M.A., F.R.S., Fellow of Jesus College, Oxford, and Hope Professor of Zoology in the University. ] ‘The following paper is an abstract of results obtained by Mr. R. Shelford, B.A., Curator of the Sarawak Museum, British North Borneo. The vast majority of his observations were made at or near Kuching, the capital of Sarawak ; a few, however, in Singapore. When no locality is mentioned, Sarawak is to be under- stood. The observations form a very important addition to our knowledge of mimicry in Malayan insects, especially the Coleoptera. Among Lepidoptera an ZElymnias, believed to be a new species from Mount Penrissen, is a tolerable mimic of the well-known Euplea, Tronga cramert. Among the Chalcosid moths, three species of Jsbarta mimicked two of Euplwa and 796 REPORT—1900. one of Pierine (Delias eathara). The latter is of considerable interest, inasmuch as the Pierine model appears to be excessively rare. There can be little doubt, however, as to the true relationship, for another species of the same genus, I. pandemia, is a magnificent mimic of another species of Delias (D. pandemia), both coming from Mount Kina Balu in North Borneo. In the Neuroptera the Mantispides are shown to be mimics, a splendid new species (M. simulatrix, McLachlan) resembling a common Bracon flying with it on Mount Matang, near Kuching, while a small species from Singapore (JM. ? cora) exactly mimicked an ichneumon flying with it. It is in the Bornean Coleoptera, and especially the Longicornia, that by far the largest additions to the subject of mimicry have been made. Many Longicorn species, chiefly of the genus Oberea, were excellent mimics of the Braconidae, and perhaps other Hymenoptera. The long narrow form of the beetle resembled the Bracon at rest with wings folded. As seenfrom the side, certain species of Oberea, notwithstanding their uniform diameter, were apparently ‘waisted’ like a Hymeno- pterous insect, the effect being due to a conspicuous white patch on the side of the anterior abdominal segments, The part of the body thus covered is obliterated, while the outline of the patch is such that the uncovered, and therefore conspicuous, part of the body conforms to the shape of a slender ‘ waist,’ from the posterior end of which the abdomen gradually swells. The effect in one species is as perfect as if an artist had deliberately painted the profile of a Hymenopterous abdomen upon that of a beetle. Among other examples of the same form of mimicry was a magnificent Cerambycid from Mount Penrissen (Nothopeus or n. gen., 0. sp.), a beautiful mimic of the abundant wasp, Salius sericosoma, which flew with it. The common Dammar Bee (Trigona apicalis), which does not sting, but is formidable because of its bite, is the centre of a group of three species with the most remote affinities. Not only is there a Longicorn, Lpania singaporensis, but a Bracon and a Reduviid bug. The mimicry is probably Miillerian in most, if not all, of the species of this group. 5 Another important set of Longicorns, species of Entelopes, Tropimetopa, Chreonoma,and Astathes, were extremely perfect mimics of Phytophaga( Galerucide). In one large group both models and mimics were reddish-brown, in another iridescent blue-black, in a third anteriorly blue-black, posteriorly reddish-brown. Another species of Entelopes (£. glauca) resembled a common Coccinellid (Caria dilatata), a Cassid also falling into the group. The Lycide were models for Longicorns and other insects in Borneo no less than in South Africa. Species belonging to the Longicorn genera Erythrus, Ephies, Xyaste, and Eurycephalus mimicked Lycids with remarkable accuracy. In the Jast-named genus one species, £. lundi, was a mimic, while another closely related (Z. cardinalis) exhibited a warning coloration of the most startling character, an indication that the genus is distasteful and the mimicry Miillerian. Jn addition to these, the Lycids were mimicked by a Clerid beetle, by numerous Hemiptera and a Zygzenid moth, the latter from Singapore. The resemblance of certain Longicorns to the Rhynchophora was far more evident than in South Africa, for not only was there a mimic ( 7rachystola granulata) of a Curculionid (Sipalus granulatus), but there were species belonging to no less than four genera mimetic of the Brenthide. These latter mimics hold their long antenns extended forwards side by side, the tips only, or in some species the anterior halves, diverging. Thus the rostrum of the Brenthid, together with its usually short antennz, are represented by the long antennz of the Longicorn. The Anthribide were mimicked by Longicorns of the genera Evets and Cacia. A feature of both Rhynchophorous models and their mimics, and one very unusual in mimicry, is the inconspicuous mottled colouring and the absence of strongly contrasted tints. A very interesting Longicorn mimic of an Endomychid beetle (Spathomeles sp. near ¢turitus) Was a rare species of Zelota as yet undescribed.. The curved spine on the elytron of the model was represented by a brush of hairs on that of its mimic. Ixperiments indicated that the Zndomychide as a group were distasteful, and large synaposematic sets of purplish black, yellow or orange a i @RANSACTIONS OF SECTION D. 797 Spotted species were found near Kuching together with several species of Erotylide aud a Pentatomid bug with the same general appearance. Another group of dark Endomychids was rendered conspicuous by numerous spines (Amphisternus). Two groups of Longicorns were mimicked by other Longicorns belonging to entirely different sections. The iridescent green Cerambycide of the genus Chloridolum were closely resembled by two Lamiide (Saperdine? genus, and Chiorisanis viridis) and by the Cerambycid genera Xystrocera, Psalanta, and Leptura. Many genera and species of the banded Cerambycid Clytine were very closely mimicked by Lamizde and other Cerambycide. This last case is of peculiar interest, inasmuch as the Clytine are themselves perhaps the most con- spicuous mimics of Hymenoptera to be found in the whole of the Longicornia. All over the world their numerous species commonly present a black yellow- banded appearance bearing a general resemblance to wasps, while mimicry of Mutillide, Cicindehde, and, in the allied Tillomorphine, of ants is also found. When, therefore, we also find that this group itself furnishes numerous models to other Longicorns, we are driven to conclude that it is in some way specially defended, and that its resemblance to Hymenoptera is Miillerian rather than Batesian. The mimetic resemblance to the aggressive and active Cicindelide was very marked, examples being afforded not only by Longicorn beetles of the genera Selethrus and Collyrodes, but also by a Dipterous insect found flying together with its model (Collyris emarginata) on Mount Seramba, December 1898. ‘This is the first example of the mimetic resemblance of a fly toa tiger beetle. The remark- able Locustid mimic Condylodera tricondyloides (or a closely allied species) described by Professor Westwood from Java was also rediscovered in Borneo, and its habits for the first time observed. Indirect evidence that the mimicry of Cleride is Miillerian rather than Batesian is similar to that which pointed to the same conclusion in the Longicorn Clytine. One Bornean species of a Clerid genus (Thanasimus) resembled a Mutillid, another (genus near Tenerus) a Lycid, while a third, a species of Lemidia, was mimicked by the Longicorn Daphisia pulchella. Among the Diptera a splendid black Hyperechia (H. fera) was a beautiful mimic of the abundant Aylocopa latipes, another example of parallelism with South African bionomics. An allied species, Laphria sp. near Terminalis, was an excellent mimic of Salius aurosericeus. Dipterous mimics of Hymenoptera are extremely abundant in Borneo: remarkable among them was a species which mimicked an ichneumon of the genus Mesosternus. The short antenne of the fly in no way resembled the very long black and white ones of the ichneumon. The fly, however, held up its black and white legs, applying their bases to its head and moving them so that they closely resembled the antenns of the Hymenopterous insect in movement as well as in colouring and proportions, Another species of fly possessed true anternze which were remarkably long for this order, and thus closely resembled those of an ichneumon. With few exceptions, the whole of the material here briefly described may be seen in the Hope Department of Zoology, Oxford University Museum. 4, Note on an Experiment supporting the General Principle of * Miillerian’ Mimicry. By Professor C. Luoyp Morean, /.R.S. 5. Lllustrations of Mimicry and Protective Resemblance. By Manx L. Syxzs. 6. The Colour Physiology of Hippolyte varians By F. W. Gampue and F. W. Kesste. 798 REPORT—1900, 7. The Locust Plague and its Suppression. By AB. Monro, M.D. Locusts have devastated the greater part of the habitable world, and during the last ten years have done great damage in the southern republics of South America, in North and South Africa, in India, &c.—countries widely separated from each other—and they have caused great loss of human and animal life in large areas in Africa belonging to Britain, The importance of the subject is therefore considerable. But the difficulties which hitherto have been connected with the plague seemed excessive and inguperable barriers in dealing with it effectually. To illustrate the remarks in this paper I select the four following typical and well-known species of the insect, namely, 1, the Caloptenus spretus, or Rocky Mountain locust; 2, the Stawronotus criatus, or Cyprian locust; 38, the Schistocerca paranensis; and 4, the Acridium peregrinum, or Old World locust, in order to emphasise in a more pointed way certain aspects or characteristics of the insect which I think it well to put prominently forward in attempting to bring this plague under review, and askirg favourable attention as to the best means to check it and alleviate the distress. a. Our increased and gradually accumulating knowledge of the habits of the insects is derived mainly while the insects come to and sojourn in their temporary homes, for we do rot yet know them in their permanent or true homes. The one and only success in combating the plague by human means in the whole history of the world was due to the putting in force the simple observation that the young (or the old) locusts cannot adhere to smooth surfaces, such as glass, owing to the fact which is now made abundantly clear, namely, that, unlike flies, the pro- cesses or claws on the feet of their front and middle pair of legs are too short and weak to enable them to do this. 6. The general and characteristic features of the locust run through all the species alike. This fact has been greatly lost sight of or minimised, and the dif- ferentiations which help to mark off one species from another haye been magnified into an unjustifiable and unnecessary importance. The instincts and the structure of all the varieties are very nearly alike, although one species may not be so large or haye different markings as compared with anotler. e. The direction which the ‘army’ assumes when the larve at a certain period set out for and continue on their ‘march’ is a most important matter to settle and be certain about, as this is the most destructive period in the life of the insect. They then devour everything that comes in their way. Not so with the flight of flying locusts, which only levy toll here and there as they pass or sojourn. The ‘army on the march ’ usually pursue a straight given course, irrespective of all obstacles and dangers (natural or artificial) that may be in their way, minus any with smooth surfaces owing to the reason above stated. Now the course or direction of the ‘ march’ will be found (though further observation is requisite to confirm the truth fully) to be always in a given direction in certain countries, Thus in the Argentine and South Africa they travel southwards, in Algeria north- wards, in the United States eastwards, and so on. It may not be true south, or true north, or true east in the respective instances mentioned, but it will be respectively towards the south, north, or east, as the case may be. The important thing to bear in mind is that they all march in one general direction as a body at the same time, and without any leader ; while so far as suitability and abundances of food are con- cerned to satisfy all their instincts an exactly opposite or other direction would be far better. The ‘Screen and Trap’ or ‘ Cypriote’ system was based on the suppo- sition that the insects march ina given specific direction. It has beenowing to this fact that the power of the plague was broken in the course of one year (1888) in Cyprus, although it baffled all efforts to check it for centuries before. Since the suppression of the plague, and no doubt very much on account of it, Cyprus has entered on a new era of prosperity. Outline of the Means for Checking or Suppressing the Plague, There is a sense in which a plague or pest such as that of locusts may be re- garded as the increase over the natural checks with regard to the normal number, TRANSACTIONS OF SECTION D. 799 When this gain takes place it is now almost universally admitted that human measures ought to be resorted to with the view of aiding the natural agencies, so that the insects may be reduced in number to a point that is safe or free from danger, I. The Natural Agencies for Checking the Plaque. Destruction by (1) the wind; (2) birds; (8) reptiles, lizards, toads; (4) mammals and fish; (5) wasps; (6) disease:—(a) internal larvee from the Tachino fly, (4) Mylabris parasite, (c) Mermis parasite, (d) Cynomia pictifacies parasite, (¢) Empusa grylli parasite, (/) various others, such as mites; (7) eggs destroyed by insects, animals, weather, water. Il. Artificial and Mechanical Means for Checking the Plague. 1. Ingenuity or finessing. 2. Destruction of the eggs by—(a) Machines, ploughs, harrows ; (6) eating by pigs; (c) tramping the ground ; (d) irrigation ; (e) judicious use of chemicals; (f) collecting the eggs. 3. destruction of hoppers by—(a@) maiming, (4) crushing, (c) tramping with stock, (d) diverting, (e) catching and bagging, (f) trapping, (vy) burning, (A) use of chemicals, (7) inocu- lation of fungi. 4. Destruction of the winged locusts by—(a) diverting a flock or flight, (4) shooting them on the wing, (c) maiming, (d) chemicals, (e) tramping, (f) crushing, (7) burning, (4) catching and bagging, (7) imoculation of the flying locust with a fungus. 800 REPOT—1900. Suction E—GEOGRAPHY. PRESIDENT OF THE SecTIon—Sir Georce 8. Rosertson, K.C.S.1. THURSDAY, SEPTEMBER 6. The President delivered the following Address :— Wauen the British Association for the Advancement of Science honoured me with an invitation to preside over this Section, Iaccepted the distinction, thoughtfully and with sincere gratification. The selection as your President at Bradford, this great and interesting centre of commercial energy, of a student of political movements who was also deeply interested in the science of geography, seemed to point suggestively to a particular branch of our subject as appropriate for an opening address. This consideration, and, to my thinking, the fitness of the occasion, led me to believe that the British Empire itself was a very proper subject for such reflections as could be compressed within the limits of an in- augural Presidential Address. Many of my predecessors have eloquently and wisely dealt with various topics of admitted geographical rectitude—with geography in its more strictly scientific study, with its nature and its purview, with its recent progress, and with the all-important question of how it could be best taught methodically, and how most profitably it might be studied. In dealing with the important practical application of our science to the facts of national life—Political geozraphy—lI feel that perhaps a word of explanation is necessary. Pure geography, with its placid aloofness and its far-stretching outlook, combined sometimes with a too rigid devotion to the facts and con- clusions of strict geographical research, is apt to incline many scientific minds to an admirable quiet-eyed cosmopolitanism—the cosmopolitanism of the cloistered college or the lecture theatre. It perhaps also at times has a tendency to create in purely academic students a feeling of half disdain or of amicable irritability against those who love the science for its political and social suggestiveness and elucidations. Thus there is a possible danger that geographers of high intel- lectual calibre, with enthusiasms entirely scholarly, may come to underrate nationality and to look upon the world and mankind as the units, and upon people and confederacies and amalgamations merely as specific instances of the general type. We know that geography is often looked upon as the science of foreign countries more especially. Such mental confusion is undoubtedly less common than it was, yet it still influences, unconsciously, the. minds of many people. It is well not to forget this curious fact, and to point out, as if it required emphasising, that there is nothing foreign to geographical thought in the association of geography and patriotism, and that the home country is worthy of careful study, particularly when, as with us, our home country is not Yorkshire, nor England, nor the United Kingdom, but the whole British Empire. That is my justification aud my apology for taking Political Geography and the TRANSACTIONS OF SECTION E. 801 British Empire as my subject, if justification and apology seem to any one to be necessary. To the generous hearts of our distinguished foreign visitors who honour us quite as much as they delight us by their presence, I am sure of my appeal. Every true man loves his own country the best in the world. That beautifying love of country does not require him to be ignorant of or to hate other countries, The community of the civilised nations, no longer to be described as Christendom even, for Japan has been received into it, is a mighty fact in geography no less than in politics. ‘fo love mankind one must begin by loving individuals; before attaining to true cosmopolitanism one must first be patriotic. Now, besides dealing with the topography of the globe, geography considers also the collective distribution of all animal, vegetable, and mineral productions which are found upon its surface. The aspect of the science which deals with man’s enyiron- ment, and with those influences which mould his national character and compel his social as well as his political organisation, is profoundly interesting intrinsically and of enormous practical usefulness when rightly applied. Given the minute topography of a country, a complete description of its surface features, its rivers, mountains, plains, and boundaries, a full account of its vegetable and mineral resources, a knowledge of its climatic variations, we have at once disclosed to us the scene where we may study with something like clearness man’s procession through the ages. Many of the secrets of human action in the past are explained by the land-forms of the globe, while existing social conditions and social organisa- tions can often thereby be intelligently examined and understood. Persistent national characteristics are often easy to explain from such considerations. For instance, the doggedness of the Dutch river-population, caused very greatly by a perpetual struggle against the sea, or the commercial carrier-instinct of the Nor- wegians, those northern folk born in a country which is all sea-coast of countlese indentations. Having few products to barter, the Norwegians hire themselves to transport the merchandise of other peoples. We British also were obyiously pre- destined to isolation and insularity, when perhaps in the human period the Thames ceased to be a tributary of the Rhine. Our Irish fellow-countrymen were similarly fated for all time to lead a separate, special, and national life apart from our own, when at a still earlier period, geologically, the Irish Channel was formed. Such large-scale facts are not to be overlooked; there are others, however, of varying degrees of prominence. Some merely require to be interpreted thonght- fully, while others, after diligent study, may still remain dubious and matter for speculation. Geography is the true basis of historical investigation and the elucidation of contemporary movements. At the present time great social and political changes are occurring throughout the world—in Europe, Asia, Africa, and America, and in the islands of the great seas. These changes are absolutely dependent upon the physical peculiarities of the different lands acting upon generations of men during a prolonged period of time. As a consequence of certain soils, geographical characteristics, and climates, we notice how harsh surroundings have disciplined some races to hardiness and strenuous industry, accompanied by keen commercial activity, which is itself both a result of in- creasing population and the cause of still greater overcrowding. Then we see other people at first sight more happily circumstanced. With them the struggle to live is less ferocious, their food is found with little toil, But we perceive that the outcome of generations of Nature’s favouritism has been to leave them less forceful and less ingenious in the never-ending warfare of existence. By com- parison they grow feeble of defence against the hungrier nations, ravenous for provender. Man forever preys upon his own kind, and an easy life in bland surroundings induces a flabbiness which is powerless against the iron training of harsh latitudes, or against the fierce energy and the virile strength produced by hereditary wrestling with unkindly ground. The discovery of America and Vasco da Gama’s voyage round the Cape originated movements and brought into play those subtle influences of foreign lands upon alien sojourners, and through them upon their distant kindred, which alter the course of history and modify national manners and perhaps national charac- teristics also. The colonisation of territories in the temperate zone by European 1900, 3F 802 REPORT—1900. Governments, separated by vast ocean-spaces from their offshoots, has given origin to new and distinct nations different from the parent stock in modes of thought and in ways of life, a result due mainly, no doubt, to local physical conditions, but in part also, if only in part, to detachment, to complete and actual severance from the mother country. This brings us to that most interesting and important topic, geographically speaking, of Distance, an aspect of our science which is of the utmost concern to traders and to statesmen ; indeed, an eminent German geographer defines geography as the Science of Distances. To this subject of Distance I wish in particular to direct your attention, and especially to its bearings upon the British Empire. The British Empire is equal in size to four Europes, while its population approximates four hundred millions. Although that may seem a somewhat grandiloquent method of description, it is a fairly accurate statement of fact. Still more interesting to us is another truth—that outside of these islands we have some ten millions of white-skinned English-speaking fellow-subjects. These islands are scarcely more than one-hundredth part of the whole Empire, although we count as four-fifths of its white population; of the total number of the Queen’s subjects we are, however, no more than a tenth. British Empire is somewhat of a misnomer, just as the North American and Australian Colonies were never colonies at all in the classical sense of the word. For the colonies are not independent of the mother country. An empire again really means a number of subject peoples brought together, and at first held to- gether, by force. India is an empire for instance. Some new title or phrase would have to be invented to describe accurately all the possessions of the British Crown from the Government of India through all possible grades of more or less direct control until we come to sume colony with representative institutions, and thence to the great commonwealths with responsible legislators and responsible cabinets. Happily, however, there is no need now for any novel designation. The style British Empire has become in time of stress a rallying cry for all the Queen’s subjects, and the term has been sanctified by the noble eager devotion shown to her Majesty, both as a beloved and venerated constitutional sovereign, and as the common bond of unity between those great self-governing daughter- nations which we in the past were accustomed to speak of as ‘our colonies.’ Consequently British Empire has henceforward a clearly detined, a distinct, a national significance, just as Imperialism has a special and peculiar meaning to all of us. Weunderstand by British Empire and by British Imperialism a confederacy of many lands under the rule of her Britannic Majesty. This confederacy is dominated by white peoples—Anglo-Saxons, Celts, French-Canadians, and others— Init together in most instances by the ties of blood relationship, but with equal if not greater closeness by common interests, an identical civilisation, and a love of liberty, in addition to that dignified but enthusiastic acceptance, already referred to, of the constitutional sovereignty of the same Queen. We may hope that generous demo- cratic expansiveness and social assimilation will also in time detain willingly within the limits of this British confederacy of white peoples those other Christians and distant kinsfolk of ours in South Africa who are at present so bitterly antagonistic. Ruled and controlled under liberal ideals by the centre of authority there are, in addition, the great subject territories whose non-Christian population are less advanced in moral and material progress. They exhibit indeed every degree of backwardness, from the barbarism of the savagest tribesman to the intellectual but archaic civilisation of ancient Asiatic nationalities. Concerning the British Empire, and comparing it with other empires, ancient, recent, or now existing, its two most remarkable features are its prodigious and long-continued growth and the persistency of its power. It cannot to all seeming grow much larger, from lack of expansive possibility. But it is unprofitable to predict. Every step which has been taken in the way of extension, particularly of late years, has been against the wishes and in almost passionate opposition to the views of large sections of the people. Yet the process of enlargement has gone on continually, being often in actual despite of a Government, whose members find themselves powerless to prevent absorptions and concretions which TRANSACTIONS OF SECTION E. 8038 they would gladly avoid. Objections to this perpetual growth of empire in territory, and to the resulting responsibility which we not altogether willingly accept, are unanswerable theoretically. The too heavy and continually increasing strain upon our military resources every one can appreciate. The limit in power of the strongest navy in the world is at least as obvious as the vital necessity that our Navy be largely and ungrudgingly strengthened. Naturally the ery of cautious patriotic men is the same now that it has always been—‘ Consolidate before you step farther.’ In India, owing to conscientious and strenuous opposi- tion to every suggestion of expansion and to the almost violent form which that opposition often took, our progress has been on the whole slow and comparatively sale. We have (I, of course, avoid all allusion to very recent policy) a3 a rule consolidated, strengthened ourselves, and made our ground sure before another advance. But there is a general impression that in other parts of the world we have been hastily and unfortunately acquisitive, whether we could help it or not; that the new provinces, districts, and protectorates are some of them weak to fluidity; that the great and unprecedented growth of the Empire has led toa stretching and thinning of its holding links which are overstrained by the weight of unwieldy extension and far beyond the help of a protecting hand. I hope to be able to show that in some important respects this suspicion is not altogether true; that science, human ingenuity, and racial energy have given us some com- pensations, and that it is not paradoxical nor incorrect to say that our recent enormous growth of empire has been everywhere accompanied by a remarkable shrinkage of distances—by quicker and closer intercommunication of all its parts one with another and with the heart centre. In short, the British Empire, in spite of its seemingly reckless outspread, its sometimes cloudy boundaries, its almost vague and apparently meaningless growth, is at the present day more braced together, more manageable, and more vigorous as a complete organisation than it was sixty years ago. The difference between its actual extent in the last year of the century and its size at the date of the Queen’s accession can be estimated by a glance at a remarkable series of maps published in the ‘ Statesman’s Year-book for 1897,’ while since 1897, and at this instant as we all know well, _ its‘mighty bulk is being still further increased. The world as a whole has strangely contracted owing to a bewildering increase in lines of communication, to our more detailed geographical knowledge, to the formation of new harbours, the extension of railways, the increased speed and the increased number of steamships, and the greatly augmented carrying power of great sailing vessels built of steel. Then, hardly second in importance to these influences are the great land lines and the sea-cables, the postal improvements, the telephones and, perhaps we may soon add, the proved commercial utility of wireless telegraphy. This universal time-diminution in verbal and personal contact has brought the colonies, our dependencies, protectorates, and our dependencies of dependencies, closer to each other and all of them nearer still to us. Measured by time-distance, which is the controller of the merchant and the cabinet minister just as much as of the soldier, the world has indeed wonderfully contracted, and with this lessening the dominions of the Queen have been rapidly consolidating. Nor is this powerful influence by any means exhausted. In the near future we may anticipate equally remarkable improvements of a like kind, especially in railways, telegraph lines and deep-sea cables, and in other scientific discoveries for transmitting man’s messages through water, in the air, or perhaps by the vibra- tions ofthe earth. For us particularly, railway schemes of expansion must be mainly relied upon to open up and to connect distant parts of the Empire. Our true and only trustworthy road of intercommunication between the heart of the Empire and its limits must always be the sea. For general trade purposes, such as the convenience of business travellers, all continental lines and all the great projected railways will be helpful, whatever nation controls them ; but our certain security is the sea, the sea which protects us, which has taught us to be an Imperial people. If we ever forget that, there may be a calamitous awakening. We must not be persuaded to build—or at any rate to place reliance upon—land roads or railways through regions inhabited by tribes and peoples over whom we 3r2 804 REPORT—1900. have not complete military as well as political control. Persian, Arabian, North African railway projects are happily rarely heard of now. As national enter- prises they never were and never could be practicable, or otherwise than dangerous mistakes. We are a world-power solely because of our worship and because of our command of the sea, In the future also we shall remain a world-power only so long as we hold command of the sea in the fullest sense of the term, not merely by the force and efficiency of the fighting navy, but by the excellence and the perfecting of our mercantile marine, by increasing its magnitude, carrying power, ard speed, and by anxiously attending to its recruitment by British sailors. We must not attempt to overtax our resources to guard railway lines through foreign semi-civilised or savage countries by exported or local armies. A heavy land responsibility lies upon us already. Under a little more we might be easily over- weighted and crushed down. We must concentrate all our surplus energies upon our sea communications. Therefore the railway lines which I spoke of as helping to consolidate the Empire in the near future are those only which are projected or are being built in the various colonies and dependencies, lines to distribute and collect, to connect provinces, and feed harbours. The mighty Canadian Pacific Railway is unique in the Empire. It not only complies with all these require- ments, but in addition it provides to Australia and the Eastern dependencies an alternative road, convenient and safe. AsI said before, all railways, wherever built, will probably help us directly or indirectly in the long run, provided we are never committed to the protection of any one of them outside of our own boundaries. And what has been said about railways applies, with obvious modifications, to telegraph lines and to maritime cables. The more general the extension of these, and the more numerous they become, the greater benefit will there be to this country in its double capacity as the greatest trader and the greatest carrier of merchandise in the world; while the actual equivalent to a diminution of time- distance in travelling is to be found in the instantaneous verbal message which can be despatched to the most distant point of the Empire. But we ought certainly to join all the shores of the Queen’s dominions by sea-cables completely controlled by British authority. To rely upon connection between our own cables through telegraph systems stretching across fo’eign countries, however friendly, or to permit the ends of these sentient nerves of the Empire to emerge upon shores which might possibly become an enemy’s country, is dangerous to the point of recklessness, that parent of disaster. As a melancholy instance of my meaning it is only necessary for us to remember the Pekin catastrophe—how we suffered from those dreadful intervals of dead silence, when we could not even communi- cate directly with our own naval officers at Taku, or with any one beyond Shanghai, although we have in our possession a place of arms at Wei-hai-Wei upon the Gulf of Pechili. It is obvious that we ought to have an all-British cable for pure strategic reasons as far as Wei-hai-Wei, our permanent military outpost on the mainland. Now to give some suggestion of the increased facilities for carrying mer- chandise, for conveying passengers quickly about the world, and for the sending of messages to all parts of the earth, a few, a very few, salient facts may be oe about ships—sailing ships and steam yessels—and about telegraphs and cables, In 1870 there were no more than ten British sailing ships which exceeded or reached two thousand tons burden. In 1892 the yards on the Clyde alone launched forty-six steel sailing ships which averaged two thousand tons each. In 1895 the number of Jarge steel sailing ships being built in the United Kingdom was down to twenty-three, and, speaking generally, it is inevitable that sailing vessels must Rive way to ocean steamships for most kinds of cargo—cattle, coals, wool, grain, oil, and everything else," gt Now let us turn to the results in shortening journeys accomplished by the progress made in the construction and in the driving machinery of steamships en the last forty years, which has especially been fruitful in such improve- ments, Masi) TRANSACTIONS OF SECTION E. 805 During this century the six months’ voyage round the Cape to India became a forty and then a thirty days’ journey by what was known as the overland route for mails and passengers through Egypt. By degrees it had become shorter still by the railway extensions on the Continent and by the unbroken steamship passage through the Suez Canal, until now the mails and hurrying travellers may reach London in twelve or fourteen days after leaving Bombay; and the great liners of the P. & O. Company can arrive in the Thames eight days later. This famous corporation, after her Majesty had been reigning nearly ten years, possessed only fourteen ships, with an aggregate of 14,600 tons. Now it owns a priucely fleet of fifty-three ocean steamers, with a total capacity of 142,320 tons. Practically the voyage to India in her Majesty’s reign has been diminished by one-half at least. Also since the Queen’s accession the passage between the British Isles and the Commonwealth of Australia has grown shorter, from the ninety days taken by the sailing clippers to the fifty-three days occupied by Krunel’s Great Britain. At the present time it lasts from thirty to thirty-five days by the Suez Canal route, while it has been finished in as little as twenty-eight days. Australia is conse- quently only half as far away, in time, as it was; while, if the Suez Canal were closed for any reason, we have at our disposal, in addition to the Cape route with its quick steamers, which is linked to us by the Pacific Ocean road, the splendid service of that Empire-consolidator, the Canadian Pacific Railway. The important part played by the Suez Canal in this connection will be discussed a little later. Now I am merely indicating by a few well-known facts the diminution of distance by the improvements which have been made in the ships themselves and in their propelling machines. Across the Atlantic the rapidity of travelling and the general average speed of all cargo steamers have increased remarkably. Very interesting statistics on this point were given to the British Association for the Advancement of Science last year, at Dover, by Sir William White in the Presidential Address of Section G. We may say, without repeating details, that during the last half of the nineteenth century the breadth of the Atlantic has practically been diminished one-half. In 1857 the Union Company contracted to carry mails in thirty-seven days to the Cape. Now the contract time is nineteen days. This again diminishes the distance by one-half. As an instance of the remarkable change which has been made in steamships within forty years, it may be mentioned that the first Norman of the Union Company took forty-two days to reach the Cape, while the present Norman has covered the journey in fourteen days twenty-one hours. I need not specify particularly the equivalent acceleration of speed upon other great steamship lines. All our sea distances have been shortened 50 to 60 per cent. in an identical way. It is not too bold to predict that the Atlantic, from Queenstown to New York, will, before long, be steamed in less than four days. The question has now resolved itself simply into this—will it pay shipowners to burn so much coal as to ensure these rushing journeys before a cheaper substitute for coal is found? We lmow that a torpedo-destroyer has been driven through the water at the rate of forty-three miles an hour by the use of the turbo-motor instead of reciprocating engines. Consequently an enormous increase in the present speed of the great Atlantic liners is certain if the new system can be applied to large vessels. By such very swift steamers, and by the example they will set to all established and competing steamship companies, the journey to Canada and subsequently to all other parts of the Empire will be continually quickened, until predictions which would now sound extravagant will in a few years be simple everyday facts. We must turn next to the subject of telegraphic communication, especially as it relates to the British Empire. ‘The mazes of land-lines and of sea and ocean cables are too numerous and intricate to be described in detail. Also the general effect of this means of bringing distant peoples together, and its transcendent importance for political, strategic, and trading purposes, need not be too much insisted upon in this place, so obvious must they be toevery one. Yet, great as has been its power and/advantage in all of those directions in the past, it is certain that still greater development and still greater service to the world will follow in the future even from existing systems, 806 kEPORT—1900. not to speak of their certain and enormous possibilities of growth. In the celerity ot the actual despatch of a message we need not ask for much improvement. Lightning speed will be probably sufficient for our go-ahead children of the twentieth century. But where we may expect and shall undoubtedly get increased success is in multiplied facilities for sending telegrams all over the earth, and in widening their usefulness and convenience to all ranks and sections of the community. ‘To obtain these necessary advantages there are two requisites— first a great and general cheapening of tariffs and, as a certain consequence of such reduced charges, a duplication or even a quadrupling of many of the present cables to prevent blocking ; and, secondly, an indefinite extension of both lines and cableseverywhere. Progressinsubmarine telegraphy undoubtedly means a lessening in the price of service and a firmer control by the State, as an obvious corollary to the large help to the companies already given by the general tax- payer, quite as much as it means those scientific inventions and scientific discoveries which the coming years have in store for us. At the present time the charges are far too high, ridiculously so as regards India, and the use of the great cables is therefore very often beyona the power of the small capitalist and the trader of the middle sort. Yet certain and early news is of supreme importance to large numbers of both classes. Its absence hampers or stops business, while its price is too severe a tax upon average profits, This fact has led to the invention of ingenious and elaborate codes. ‘They might possibly have been devised in any case; but there isno doubt that messages by code would be certainly expanded so as to prevent all possible ambiguity, if telegraphing to distant countries were not so costly. The spreading of land-lines and sea-cables about the earth has gone on rapidly since 1870; to the extent that those already completed would seem even to be in advance of their requirement, if that requirement were to be measured by their full employment. Nevertheless it is to be wished that new companies could be formed and new lines laid down to excite competition and thereby to cheapen rates; or else that our Government should step in and regulate charges over subsidised British lines. For the power of the great telegraph corporations, by reason of their monetary resources, enables them to overcome ordinary rivalry and to treat public opinion with indifference. A general cheapening of rates has constantly been followed by increased profits, earned by the resulting augmentation of traffic, but it needs an enterprising directorate to face the necessary initial expenditure, except under pressure. Boldness and foresight in finance are natu- rally less prominent features in the management of the great telegraph companies than contentment with a high rate of interest on invested capital. All their energy and watchfulness are employed to crush competition rather than to extend their activities indefinitely. Moreover, money-making is their business, not Imperial statesmanship. If it were a question of the added security or the close coupling- up of the Empire (which are probably synonymous) on the one hand and a loss of profit (however splendid the dividends might still remain) on the other, we know what would be the result of their deliberations. Important as are the sea-cables for statesmen, for strategy, and for commerce, they are or will be equally important socially to keep up intimacy and swift intercourse between families half in Britain and half in India for instance, or between friends and relations in these Islands and in the great Colonies. They might be made to give the sensation almost of actual contact, of holding the hand of your friend, of speaking directly to his heart, It is this interchange of per- sonal news and private wishes, quite as much as the profound political and com- mercial aspects of lightning communication with all parts of the Empire, which will bind the Empire in bonds stronger than steel, easy as affection, to hold it together with unassailable power. Consequently the health and strength of the Empire depend very greatly upon a cheapening of telegraph charges. Doubtless a time will come when all our main cables of the first importance will be in the hands of Government, when they will only touch upon British territory, and when they will be all adequately protected from an enemy. Those are truly Im- perialistic and patriotic aspirations. But we must never forget the grand part in bringing together, within whispering distance as it were, the different parts of the world, and consequently of our world-wide Empire, which has been taken in the TRANSACTIONS OF SECTION f&. 807 past by such Napoleonic organisers as the late Sir John Pender. It is to him and to such men as he that we owe those splendid beginnings which by means of vital reflexes from the nerve-centre of the Empire have helped to fire our white fellow- subjects all over the globe with a loftier patriotism and with new, brave, and broader ideals of nationality. It was coincident with the opening of the Suez Canal in 1869 that the liveliest interest began to be taken in sea-cables, and a master mind perceived their com- mercial possibilities. Before that time the success of the constructing companies had not been great. Sir John Pender then founded the famous Eastern Telegraph Company by the amalgamation of four existing lines, which had together laid down 8,500 miles of sea-cables, besides erecting land-lines also. A year later, in 1873, from three other companies he formed the Eastern Extension Australasia and China Telegraph Company, which jointly possessed 5,200 miles of submarine lines, From that date the extension of electric communication to all parts of the earth, over wild as well as over civilised countries, and beneath the salt water, has only been equalled by their average remunerativeness, Now there are 175,000 miles of submerged cables alone, of which this country owns no less than 113,000 miles. The history of some of these cables is full of interest, and might attract the delighted attention of the lover of picturesque romance no less than of the student of commercial geography. It also supplies suggestions and many facts, both to the physical geographer and to the student of seismic phenomena. Science has taught the companies to economise time, labour, and material in cable- laying operations, as well as how to improve the working instruments, Human ingenuity, business perception, and organising power have shown once more their startling possibilities when directed and controlled by cool, clear-eyed intelligence combined with general mental capacity. It is only necessary to reaffirm, for the reasons already given, the national, the imperial, the commonwealth requirement for cheap telegraphy, and the profound necessity there is both strategically and politically for complete government con- trol by purchase, guarantee, or other equitable means over main cables which connect Great Britain with her daughter states, her Indian empire, and her depen- dencies. Our communications with our own folk must be independent of private companies and completely independent of all foreign nations. All the details which I have given are illustrative of man’s successful energy and of his progressive ingenuity in enslaving the great forces of the earth to diminish distance, to shorten world-journeys, and to speed world-messages. Another human achievement, the piercing by Lesseps of the Suez isthmus, has had remarkable consequences. It had been talked of in England centuries ago. Christopher Marlowe makes Tamerlane brag :— * And here, not far from Alexandria, Whereas the Tyrrhene and the Red Sea meet, Being distant less than full a hundred leagues, I meant to cut a channel to them both That men might quickly sail to India.’ The illustrious French engineer solved one great problem in 1869, only to originate others which are of profound importance to commercial geography—and to the British Empire most of all. The Suez Canal has brought India and the Australasian Commonwealth wonderfully near to our shores, It has greatly diminished many time-distances, but why has it not injured our Eastern trade? Also is there any danger or menace of danger to that trade? From the very beginnings of the great commerce, the Eastern trade has enriched every nation which obtained its chief share. It has been the seed of the bitterest animosities. It alienated Dutch and English, blood relations, co-religionists, co-reformers, into implacable resentment, and bitter has the retribution been. On the other hand it brought into temporary alliance such strange bedfellows as the Turks of the six- teenth century and the Venetians. At the present day what international jealousies and heartburnings has the same rivalry not fostered! For all the trading peoples know how vital is that traffic. In the earliest days of commercial venturings the Eastern trade focussed at 808 REPoRT—1900. Alexandria, afterwards at Constantinople and the Italian ‘ factory ’ stations of the Eastern Mediterranean, Barbarous upheavals in Central Asia interrupted the current at times, but only as temporary dams. Then came Vasco da Gama’s voyage round the Cape and its sequels—the diversion of the rich merchandise of the Orient from the Italian ports and from the Eastern Mediterranean to the sea- coast cities of the Atlantic. Out of the relentless scramble of the Atlantic nations for this, the grandest of the trader’s prizes, the English came out bloodily trium~ phant, and the British have remained the dominant shippers ever since. But when the Suez Canal was trenched through, a geographical reversal followed: the mer- chant’s chief path may be said to have left the Cape circuit and to have regained the old line, with immensely added facilities, to debouch upon the Eastern Mediterranean. Why has it not affected us more profoundly? Are not geo- graphical canons outraged by the great steamers passing by the French and Italian ports to find distributing centres in these islands? I think that theoretically it is so, even admitting that the foreign harbours are more difficult than ours. Practi- cally only a few industries have suffered; the volume of our trade has increased greatly, and it still remains easily pre-eminent. One of the chief explana- tions I believe to be this: Geographical considerations were defeated, for the time at any rate, by the excellence of our banking system when the Suez Canal was opened. The wealth of the country, then as now, instead of being separated and divided into isolated patches, was accumulated in the hands of bankers and was readily and easily available for commercial enterprises. So the necessary steamers —huge, and ofspecial line—were built at once by our companies and launched into the valuable Eastern trade before their rivals could begin to stir. This country had the invaluable help of its monetary facilities. Wealthy shipping corporations, once fully organised and successful, have great power, by reason of their reserves and resources, to hustle and to ride off the attacks of weaker and less experienced competitors. Supposing this great change had but just occurred—our advantages, though still distinct, would have been less remarkable. And in the future inter- national trade jealousy will be keener and the competition even more severe. We must not forget that our geographical position is no longer in our favour for steam- ships plying from the Kast, and, as in the immediate past, we must throw away no chances, but seek to make up for that admitted defect by foresight, by education, by maintaining and constantly adding to our experience, and by defending and supporting that admirable system—our national banking system—which has carried us over seemingly insurmountable obstructions to brave trade triumphs. The general considerations which I have named might lead to the inference that actual geographical disadvantages, in trade competition for instance, may sometimes be conquered by man’s resourcefulness and energy. Within obvious limitations that is certainly true. At places, as we know, the borderland between geography and many of the natural sciences is often vague and confusedly inter- laced. So perhaps also with mechanical and economic science our boundaries at certain spots overlap. Quick steamers, far-reaching telegraph lines, and the piercing of isthmuses by ship-canals may at the first glance appear outside the a of the geographer. Yet from that particular aspect of geography which have already spoken of as the Science of Distances we perceive how relevant they are, how worthy of study. Truly ours is a very catholic science, and we have seen how even the comparative value of national banking systems may help to explain seeming geographical inconsistencies, to reconcile facts with possibly un- expected results, and to show how the human element modifies, perhaps, the strictly logical conclusions of the geographer intent upon physical conditions alone. It is for the statesman and the philosopher to speculate upon the character and the permanency of such influences. Our success as an Empire will probably depend for its continuance upon a high level of national sagacity, watchfulness, and resource, to make up for certain disadvantages, as I think, of our geographical position since the cutting of the Suez Canal; and it will also depend upon the comprehensive and intelligent study of all branches of geography, not the least important of which to my view is the Science of Distances—the science of the mer- chant, the statesman, and the strategist. TRANSACTIONS OF SECTION E£. 809 The following Papers were read :— 1. Attempts to improve the Teaching of Geography in Elementary Schools, especially in the West Riding. By T. G. Roopsmr, //.J/Z. Reforms were begun through the Royal Geographical Society, whose collection of foreign maps was lent for exhibition in Bradford in the year 1837. The display of maps, models, and various devices for illustrating the instruction in geography in the elementary schools of Germany, France, and Sweden attracted special attention, Conferences were held in connection with the exhibition, one of which was attended by Dr. Scott Keltie, who made the collection. One immediate result of these proceedings was the commencement of a series of local maps and models, a collection of which is exhibited. The conferences discovered the chief defects in the existing instruction: (1) Lessons in geography were not based on object teaching, nor on the observation of local features and scenery. (2) The art of ‘ reading’ maps was not taught, nor was the construction of a map led up to by making plans of short walks and diagrams of the neighbour- hood. (8) The study of political and commercial geography was not based upon the study of physical geography, neither were the details of geographical study connected as cause and eflect. There was no attempt to present a country to the scholar as a connected whole, and the lessons consisted of lists of names and figures, at the most arranged in groups. Of such details many were wholly un- suited to the elementary stage, The chief reforms consisted in the intelligent study of local geography through local maps and models, and in object lessons which explain the principles of physical geography. The reliefs and models led up to the art of reading maps and to the demand for better maps. Such lessons are an excellent introduction to reasoning, and prove how little there is that is purely arbitrary even in the sites of towns and villages in the neighbourhood, much less in the industries which are carried on in them. The necessity for good wall-maps is now apparent, and correctly drawn details are demanded in place of vague and inaccurate sketches. Maps must interpret nature, and map reading is the converse of the process of studying home geography. In studying home geography the child begins with a natural feature such as a river or hill, and learns how to represent it on paper. On the other hand,in reading a wall-map the scholar begins with the symbols or representations of natural features which he has not seen, and arrives by means of them at the natural facts which such symbols represent. Hence the extreme importance of the right study of home geography and local models and reliefs. The symbols on the wall-map are vague and meaningless unless a content and significance are given them by previous practice in the building up of local plans and maps. The scholar has to be taught with care how to translate the symbols of the wall-map back into the forms of nature which they, however inadequately, represent. The difference between a good and a bad map is now apparent. As the scholar com- mences geography by the study of nature in a triple process, which consists of observation, description, and representation, so, if the wall-map be accurate enough, he can continue to draw inferences from it much as though he were actually ob- serving the country by personal inspection. The value of graphic work in teaching geography is insisted on. The mere copying and colouring maps of various parts of the world is rather an exercise in drawing than in geography. Each map should be drawn to serve some definite purpose. It should disentangle from a complex whole some particular part which analysis brings to light, and illustrate it with precision and simplicity. Further, the sketch-maps should proceed from simpler studies to more complex, and no map should be made of a country as a whole until the leading features have been dealt with separately, and thus the ‘constructive’ method of teaching geography is introduced. The comparison of statistics of various kinds is made much more intelligible if + the scholars learn to express their statistics by the use of square-ruled paper. 810 REPORT—1900. Abstract numbers are thus converted into concrete space forms, and are then much more comprehensible. In conclusion the formation of local geographical societies for educational purposes is recommended, and an account is given of the formation and working of the Southampton Geographical Society. 2. Commercial Geography in Education. By EB. R. Wetuey, I.A., LRG. A description of a three years’ course of lectures on Commercial Geography to teachers in the West Riding, and of what has actually been done, on the diffi- culties encountered and on ways of getting over them. 1. The three years’ course: (i.) The principles of Commercial Geography and their application to the British Empire; (ii.) the Commercial Geography of foreign countries ; (ili.) special trades and commodities. Twenty-five lectures to the course—30 to 40 teachers in attendance ; average percentage of attendances 92; centres Leeds and Huddersfield. 2. The difficulties: (i.) The inadequate knowledge of general geography the main difficulty, z.c. how best to explain commercial results of Physical Geography to minds deficient in knowledge of the elements of Physical Geography. Remedy obvious but not easy of attainment owing to multiplicity of school subjects. Accessories wanted—Government grants for commercial as well as technical or industrial side of education. (ii.) The inadequate notions still existing as to what is meant by Commercial Geography. (iii.) The collection of appropriate lantern slides. 3. A selection of lantern slides illustrating some of the chief points brought out in the three years’ course.? FRIDAY, SEPTEMBER 7. The following Papers and Report were read :— 1. The Treatment of Regional Geography. By Hucu Rosert Mint, D.Sc., LL.D. The author brought a scheme for a geographical description of the British Islands, based on the l-inch map of the Ordnance Survey, before the Section at the Liverpool Meeting in 1896. He has since worked out the regional geography of the area delineated in two sheets of the l-inch map of South-west Sussex. The extension to the whole country of work on an equally minute scale appears to be rendered impracticable only by its cost and the indifference of the public to geo- graphy. It is hoped, however, that the principles of regional description laid down in the paper may be of service in promoting similar descriptions for other parts of the country, whether carried out as part of a general scheme or independently. The configuration of the district as deduced from the l-inch map is the first condition in importance, and should be treated both generally, as to the main features alone, and also specially, as to particular details which are of more imme- diate interest than the rest. The distribution of rocks and superficial drift taken from the geological map comes next in importance, and it is interesting, though not essential, to trace the causal relation of geological structure and geographical form. It is more important to indicate clearly the places where mineral products of economic value occur. The next part of the description deals with what may be called, in default of a better term, mobile distributions. These include all features 1 As it would be obviously impossible to show more than a mere fraction of the slides used (nearly 3,000 in all), a further and much larger selection was placed in the Association’s temporary museum. * See Geographical Journal, vol. xv. 1900, pp. 205, 353. eS TRANSACTIONS OF SECTION E. 811 relating to the surface which are modified in theirdistribution by the action of fixed forms and particular rock-formations. They include climate, the character of which depends greatly on altitude and on the direction of heights and valleys with regard to the prevailing winds ; water supply, including rainfall, as modified by the altitude and exposure of slopes, percolation and the return of water to the surface as springs (dependent on the geological nature of the ground), and the volume and frequency of rivers, vegetation, animal life, population in all the distributional details of birth- and death-rates, disease, migration, towns, villages, and connecting roads and railways, agriculture, industries, and trade. The particular case selected was a fairly representative one, and brought out very clearly how all the conditions of human settlement and migration depended ultimately in a more or less marked degree on the forms of the land. It became very clear from such a study that geography rightly conceived was the science which unified and made available for practical application the immense mass of distributional statistics of all kinds which are brought together at great expense by Government, but never coordinated or made available. 2. Foreign and Colonial Surveys. By E. G. RAVENSTEIN. 3. Military Maps. By B. V. Darsisuire, IZA. Our Ordnance map is primarily a military map, made by soldiers for the use of soldiers. A practical question :— What is the best form of map for the use of troops in standing camps in this country, or fer volunteers encamped for their annual training ? Arising out of this, another question :— How far do the maps supplied by the Ordnance Survey answer the above purpose ? 1. On what points can maps give us information which is useful, and even necessary, for carrying on military operations ? (a) Rivers, streams: Width, nature of banks; fords, bridges, ferries, locks. (6) Roads: Width, surface; whether enclosed or not; whether ditches alongside. (ec) Railways: Double or single track ; embankment or cutting ; tunnels. (2) Woods, copses, heather, gorse. (e) Villages: Size, shape; houses, how placed to roads, so as to favour attack or defence. (f) Hedges and ditches. (g) Footpaths. (A) Detached houses. (¢) Physical features (‘ Terrain’), 2. Specimens of British Manceuvre maps. ° vo. The British Ordnance map as a Manceuvre map. Completely satisfactory except as regards (¢.) (Terrain) and scale. 4. Representation of relief, various methods used for Ordnance maps. (a) Contours alone. Great Britain, Italy, United States, Switzerland. (6) Shading alone. Germany. a (c) Contours with shading. Switzerland, Norway, Austria-Hungary, Great ritain, 5, The Ideal Manceuvre map. Scale; topographical details; Terrain. 812 REPORT—1900. 4, Journeys in Central Asia. By Captain H. H. P. Drasy. Captain Deasy’s paper deals with explorations in Western Tibet and Chinese Turkestan, begun in 1896. The most important features of this explorer’s work are, first, the extensive use of triangulation for determining longitudes from peaks, fixed by the Great Trigonometrical Survey of India, and heights; secondly, the discovery of the sources of the Khotan River; and thirdly, the detailed survey of that exceedingly difficult mountainous region, the hitherto unknown stretch of the Yarkand River. The continued opposition of the Chinese added considerably to the physical difficulties encountered, and resulted in the explorer and his assistant being incapacitated from work by severe illnesses. The latter compelled Captain Deasy to return to India much sooner than he had intended. It may be of interest to note that the heights of about 250 peaks were determined, and over 40,000 square miles of country surveyed. Much valuable assistance was rendered by the Indian Government, especially by the Surveyor- General, and several officers of the Foreign Department. Captain Deasy is very zrateful for this, as well as for the services of the native topographers, kindly lent by Colonel Gore, R.E., now Surveyor-General of India. 5. Large Earthquakes recorded in 1899. By Joun Mine. In 1899 at Shide, in the Isle of Wight, 130 earthquakes were recorded. The greater number of these were also observed at Kew, whilst very many of them were common to registers from Canada, the Cape of Good Hope, India, Java, Japan, and other distant countries. Analysis of these records has increased our knowledge respecting the rates at which motion is transmitted through our world, and indirectly thrown new light upon its rigidity. The arcual velocity of surface waves has been investigated, and new rules based on these investigations have been formulated for determining the position of earthquake origins. It has, for example, been shown that the distance of an origin from a given station can be determined either from the interval by which the preliminary tremors cutrace the larger surface waves or from the interval between the arrivals of waves which had travelled from their origin round the world in opposite directions. With this knowledge it is frequently possible for an observer in any part of the world to name the district from which an earthquake recorded at his observatory has originated. One series of observations showed that the amplitude of the large waves of earthquakes decreased more rapidly when traversing suboceanic paths than when they radiated over continental surfaces. In discussing the nature of large waves this observation on the damping effect of oceans was used as an argument that this form of seismic movement represented gravitational surface waves rather than the outcrop of distortional waves propagated through the body of the world. One hundred and twenty-five out of the 130 records considered represented disturbances which had suboceanic origins. The principal of them may be grouped as follows:— 1. North-eastern Pacific, W. of British Columbia . 4 4 . 14 2. Kast Mid Pacific, W. of Southern California : ; ; sub 3. East Southern Pacific, W. of Peru and Chili 5 Y 28 4. West Pacific, off Japan - 5S : : 3 5 9 5. West Mid Pacific, near Java 5 5 - . 5 4082 6. Mid Indian Ocean i “ : : ; 5 5 : 5s) 7. North Atlantic, east side . d 5 2 a 8. West North Atlantic and West Indies . . 6 9 . Mid Equatorial Atlantic , RE RANSACTIONS OF SECTION E. 813 If we except the second group we see that the Pacific origins are on the face or at the bottom of ‘deeps,’ which form portions of the trough or troughs around the eastern and western margins of that ocean. If future soundings show that the indicated exception is only apparent, then the second group will also illustrate the rule that accelerations in secular adjustments of the earth’s crust are most frequent where this exhibits the greatest flexure. Inasmuch as there are reasons for believing that each of these earthquakes was accompanied by large mechanical displacements of solid materials, the import- ance of localising the sites where such changes are frequent is evident to those who select routes fur deep-sea cables. Although we are not in a position to say that these displacements are suf- ficiently large to produce a measurable effect on the moment of inertia of the earth, attention may be directed to the fact that at those times when changes in latitude have been marked large earthquakes have been frequent, whilst when they have been few such changes have been less pronounced. Another subject of interest to those engaged in geodetic work is the fact that changes in the rates of pendulum time-keepers may sometimes be traced to the unfelt movements of large earthquakes, which so frequently disturb all countries in the world. 6. Report on the Climate of Tropical Africa,—See Reports, p. 413. MONDAY, SEPTEMBER 10. The following Papers and Report were read es 1. Railway Connection with India. By Colonel Sir T. H. Hoxpicu, X.C.1.£. The paper deals with the general geographical conditions of South-west Asia which may favour a scheme of railway connection with Western India, the subject- matter of the successive sections of the paper being as follows :— 1. The impracticability of the northern approaches to India leading over the Hindu Kush into Kashmir or Afghanistan from the Oxus regions. 2. The nature of the great transverse water divide of Asia, which includes the Hindu Kush, and the most favourable points for crossing it. 3. The opening afforded by the Hari Rud river to the west of Herat. 4. The configuration of the Persian plateau and mountains, and its adaptation to railway alignment. 5. Consideration of Persian lines of communication with Western India. The coast-line between Basra, at the head of the Persian Gulf, and Karachi. Details of alignment. Commercial and climatic objections to such a line as far as Bandar Abbas. 6. Alternative central line from Western Persia to Bandar Abbas. Diffi- culties of connection with European systems. 7. Details of alignment between Bandar Abbas and Karachi. Difficulties of coast line, and possibility of interior central line. 8. The proposed connection between Kushk and Chamen (?.e. the Herat- Kandahar line). Geographical conditions that exist between Kushk aud Herat, and between Herat and Kandahar. ‘Their favourable nature. 9. Objections which have been raised to the line—political and military. Its commercial prospects. 10. Conelusion. 814. REPORT—1900. 2. The Siberian Railway. By C. Raymonp Beazury. Short account of the route traversed by the Siberian Railway as far as the Amur. The connections of the railway main trunk with the regions to the north and south, (a) as already made, (8) as in construction and projected. The bearing of the Siberian line on Central and Southern Asia by the intended link, from Tashkent to Orenburg. Primary commercial and industrial purpose of Siberian line west of Lake Baikal. Development of the country: its population, mining enterprises, agriculture, cattle-raising, manufactures, &c., through the movements created by the railway, illustrated by some details. The railway in connection with the river navigation, (a) of the West Siberian rivers, Ob, Yenisei, &c.; (8) of the Kama and Volga; (y) of the Dvina and Petchora. The railway in connection with the western ocean and inland seas: (a) White Sea, (8) Black Sea, (y) Caspian. Connections of the railway with Russia’s strips of ice-free coast and ice-free ports in the west: (a) on Arctic Ocean, especially Catherine Harbour, near the frontier of Norway; (8) on Black Sea, especially Novo-Rossiisk ; (y) on South-west Caspian, especially Baku. The railway in its eastern part: different problems here. Highly political aspect of this section. The more recent advance of the line here through Man- churia. The ice-free outlet at Port Arthur, Talien-wan, and the Kwang-tune peninsula. Projects for maritime development of trade to Japan and America from this ‘window’ as well as from Vladivostok. Connections with China through Mongolia as well as Manchuria. 3. On the Possibility of obtaining more Reliable Measurements of the Changes of the Land-level of the Phlegrean Fields. By R. T. GUNTHER. 4. The British Antarctic Hxpedition, 1899-1900. By C. E. BorncHGREVINK. Mr. Borchgrevink commenced with an account of the origin of the expedition which he commanded, thus referring to his previous work within the Antarctic Circle, and to the resolution which was carried at the Sixth International Geo- graphical Congress at the Imperial Institute in 1895. The voyage of the Southern Cross was shortly described with a few incidents; the results of some of the principal observations (both meteorological and magnetic), the landing, the camp, and the work of the land expedition from March 1899 to March 1900. An account of the principal discoveries made during one year on South Victorian Land was given, with a description of the ice conditions, in winter and summer, near Cape Adare and in the pack, What the author claims as the principal work of the expedition is the pioneer work in Victoria Land, extending over a period of one year, thus for the first time proving the possibility for an expedition to live on South Victoria Land in the winter, with the following results :— 1. Recording the meteorological and magnetic conditions at Cape Adare and at various places on the ice and on the mainland between this locality and the 78th parallel, thus locating the present approximate position of the South Mag- netic Pole, in latitude 78° 20’ S. and longitude 146° E., about 220° west by north from Wood Bay. 2. Discovery of new species in antarctic biology, with special reference to the shallow-water fauna and the flora of South Victoria’ Land, both proving bi-polarity, and suggesting a theory for the distribution of organisms. 3. Touching upon the importance of the discovery of insects as indicating an averave temperature in the neighbourhood of the locality where they were found, not deviating much from what was experienced during the years 1899-1900. 4, Furthest south 78° 50’. The author gave his views shortly in regard to further exploration within the sean Circle, as well in regard to outfit as in reference to desirable places for anding. TRANSACTIONS OF SECTION E. 815 5. Through Arctic Lapland. By C. J. Curctirre Hyneg, WA. -Finner whale fishing in Arctic Seas—Vardé—Across the Varanger fjord—The start of an eighty-five mile tramp—Boris Gleb—Skolte Laps—Up the Neiden— Arctic Finns—Enare See—Fisher Laps—Enare Town—Farmer Laps—By canoe and swamp—Life on a Lapland Farm—The Arctic mosquito—Herder Laps— Reindeer culture—Norwegian Laps—Rovaniemi—Down to Torneo-Haparanda— The Gulf of Bothnia. 6. Report on Physical and Chemical Constants of Sea Water. See Reports, p. 421. TUESDAY, SEPTEMBER 11. The following Papers were read :— 1. Some Consequences that may be anticipated from the Development of the Resources of China by Modern Methods. By Guo. G. Cuisuoim, M.A., B.Sc. Various causes are pointed out as already in operation tending to bring about that development in spite of the opposition of some sections of the people. These are of such a nature as to make it unlikely that this development, however brought about, will be long retarded. When it does come about this development is bound to have world-wide effects on a scale of extraordinary magnitude, and in one direction it seems probable that it will tend to reverse the tendency of the last generation in the economic history of the world. The peculiarity of the position of China is this, that it is the one region in the world with all the means for industrial development on a gigantic scale that remains to be opened up. In the past thirty or forty years we have chiefly seen the opening up of new countries or old countries without great resources for industrial development. Among the consequences that may he anticipated from this opening up are these :— 1. A rise in prices in China, especially in the industrial regions. 2. The creation of a demand for food-stuffs not likely to be supplied by China itself; a demand which in itself will be one of the most powerful causes contri- buting to maintain the rise in prices. 3. The imparting of a great stimulus to the food-producing regions most favourably situated for meeting this demand, more particularly M anchuria, Siberia, and western North America, probably the Pacific States of North America to a greater extent than Canada. 4, Perhaps the most important of all, the creation of a tendency to a gradual but prolonged rise in wheat and other grain prices all the world 6ver, reversing the process that has been going on since about 1870 in consequence of the successive Opeuing up of new countries. 2. The Commercial Resources of Tropical Africa. By Epwarp Heawoop, i.A. At least 70 per cent. of the total trade of Africa falls to the countries of the extreme north and south, leaving the whole of Tropical Africa, with an area of some 9 millions of square miles, a total trade of at most 30,000,0007., of which nearly 7,000,000. belongs to the small islands of Mauritius and Réunion. The object of the present paper is to examine the causes of this small commercial 816 REPORT —1900. movement as compared with that of other tropical countries, and to form some conclusion as to the permanence, or the reverse, of present conditions. Among historical reasons for the smallness of the existing trade are (1) the attraction exercised during the age of great discoveries by America and the East and the consequent neglect of Africa; (2) the political condition of the African peoples; (3) the effects of the slave trade ; while geographical causes are found in (1) the massive form of the continent and consequent absence of natural means of communication ; (2) the unhealthiness of the coastlands. That many of these causes are not necessarily permanent is shown by a comparison with Brazil, which affords a close parallel with Tropical Africa in many respects. This shows that, given natural resources capable of supporting an increased export trade, the com- mercial future of Tropical Africa need not be hopeless. The resources of a new country may be classed as (1) exhaustible, principally ninerals ; (2) permanent, chiefly animal and vegetable products, the second group being the more important. It may be again subdivided into (1) jungle products, which, though not necessarily exhaustible, are likely to suffer diminution; (2) cultivated products. ‘The former may, under cultivation, be transferred to the latter sub-group, which is the most important of all. In Brazil, e.g., the vast preponderance of the exports is made up by the four products coffee, cacao, tobacco, and cotton. Which, with rubber, make up the principal resources of the country. In Tropical Africa jungle products, principally rubber and palm-oil and kernels (total annual value over 4,000,000/.), are at present those on which the export trade mainly depends. A period of development of plantation pro- ducts has, however, set in, and coffee, cacao, cotton, tea, &c., have been grown with success in various parts. The chief difficulties to be encountered arise from (1) want of means of transport; (2) scarcity of labour; but these are now in a fair way to be overcome. The modern tendency for each country to depend for tropical produce largely on its own colonies must favour the commercial develop- ment of Africa, while the comparatively low population of Africa per square mile renders it probable that it will in the future play an important part in providing a food supply for the more thickly peopled continents. 3. On Snow Ripples. By Vaucuan Cornisx, JZSc., 2.C.S., PAGS. These observations, made in Scotland last winter, are preliminary to a general investigation of the surface forms of snow, which the author proposes to continue in a colder climate during the coming winter. The investigation is undertaken in connection with the author’s research upon terrestrial waves and wave-like sur- faces. The general conditions during the following observations are: ground already covered with snow, temperature a little below the freezing point. Case I.—Snow falling sparsely. In absence of wind the surface was uneven, owing to clinging together of flakes. In a light breeze there was a notable tendency for the prominent parts to arrange themselves transversely in ridges, the distance from ridge to ridge not more than one inch. When the breeze freshened these became regular ripples, with a smoothed surface of closer texture. One set of measurements gave the distance between successive ridges, 1:125, 1:225, 0°85, 1-05, and 1:00 inch. Their amplitude was approximate:y ‘05 inch, which gives a ratio Length : Height = 21 approximately, The steep face of these ripples is on the windward side, whereas in sand ripples and water waves the steep face is on the sheltered side. The normal movement is downwind, the most noticeable feature of the process being the retreat of the steep weather face, consequent upon the abrasion of its surface. For occasional short intervals, however, during lulls and during moments of heavier snowfall, the ripples rush upwind, owing to the sudden deposit of snow upon each weather face. Case I1.—Fresh breeze without snowfall, blowing upon uncompacted snow. The surface was beautifully covered by ripples of 3 inches to 15 inches from ridge TRANSACTIONS OF SECTION FE. 817 to ridge, which were rapidly increasing in size. The steep side faced the wind. The ridges, which were pretty accurately parallel one to another, were transverse to the wind, but with much sinuosity, no ridge being straight for more than a few inches. It is evident that the wind must be concentrated in the re-entrant angles of the steep weather slope, and this would tend by rapid erosion to destroy the arrangement of long transverse lines which is the most obvious characteristic of Tipples. The ridges, however, did not lose their transversality, which was apparently preserved by the greater deposit of drifting snow in these re-entrants, which stopped the threatened gaps; and by the collapse of the overhangine cornice of uncompacted snow at the salient angles, by which these promontories were truncated. Case I1I.—The latest-fallen layers of snow having been blown away, the wind acts upon compacted snow (this was generally in drifts which had become exposed owing to change of direction of wind). The wind abraded a fine granular ¢ drift, which did not adhere to the smooth hard surfaces. Parallel lines of bevelling or grooving transverse to the wind are the most conspicuous feature of the resulting structure in the compact, almost homogeneous, fine-grained material. The lines are much freer from minor irregularities than the ripples described above. As the action continues, however, the sinuosities are emphasised, for, the ‘drift’ not adhering well, the re-entrants are cut back more and more behind the salients. Further, the wind concentrating along the lines of the re-entrants, the general level of the surface here is lowered more quickly by abrasion than is the case along the intermediate lines of the salient angles. ‘Thus is produced a well- marked form transitional between snow ripples and sastrug?, in which inter- mediate form the transverse ridges are crossed at right angles by alternate ridges and furrows parallel to the wind, the furrows being along the line of the re-entrants. Sastrugt.—This action went on until the ridges transverse to the wind were merely a subordinate and scarcely noticeable feature, and the snow was seen to be in great ridges parallel to the wind. These corresponded perfectly with the sastrugi of the Tundras as described by A. Penck?! on the authority of F. Schmidt and G. Bore. On the opposite orientation of snow ripples and sand ripples.—Ripples in loose sand have their steep faces on the leeward, snow ripples on the windward side. The exposed face of the snow ripple becomes steeper than the sheltered face, because the cohesiveness of the snow while in mass enables the wind to carve out wind caves, in which its force is concentrated. In loose sand the slipping of the material prevents this. The friability of the snow also assists in the effect, the detailed explanation of which would, however, be too long for this abstract. Observations were also made upon the forms of snowdrifts. Photographs were taken of ripples, sastrug?, and drifts. 4, The Geographical Distribution of Relative Humidity. By KE. G. Ravenstern. The author stated that the importance of relative humidity as a climatic factor was fully recognised. Having illustrated its influence upon organic life, upon agriculture and human industries, he expressed his regret that neither in number nor in trustworthiness did humidity observations meet the requirements of a person desirous of illustrating its distribution over the globe by means of a map. This was owing largely to defects in the instruments employed, incompetence of the observers, and unsuitability of the hours chosen for the observations. As to the humidity over the ocean, we were still dependent upon the observations made on board passing vessels, and he was afraid that the time had not yet come when floating meteoro- logical observatories would be stationed permanently throughout a whole year at a few well-chosen localities in mid-ocean. N. otwithstanding this paucity of available material he had ventured, in 1894, to publish in Philip’s ‘Systematic Atlas’ a small chart of the world showing the distribution of humidity. The * Morph. der Erdoberfléiche, vol. i. pp. 388, 389. 1900. 3G 818 REPORT—1900, subject had not been lost sight of by him since then, and he now placed the results before this meeting. He did so with some diffidence, and over-cautious meteoro- logists might condemn his action, but they must remember that when Berghaus, in 1838, acting upon suggestions made by Zimmermann and Humboldt, published the first isothermal chart the observations on temperature were even less numerous than those on humidity were at present. His charts, of course, must be looked upon as sketches, but he felt confident that they brought out the broad features of the subject, and to reduce the sources of error he had limited himself to indicating four grades of mean annual humidity, the upper limits of which were respectively 50 per cent. (very dry), 65 per cent., 80 per cent., and 100 per cent. (very damp). The relative humidity over the oceans might exceed 80 per cent., but in certain regions (‘ horse latitudes’) it was certainly much less, and in a portion of the Southern Pacific it seemed not to exceed 65 per cent., a feature seemingly con- firmed by the salinity of that portion of the ocean, which exceeded 3°6 per cent. His second chart exhibited the Annual Range of Humidity, viz. the difference between the driest and the dampest months of the year. In Britain, as in many other parts of the world, where the moderating influence of the ocean was allowed free scope, this difference did not exceed 16 per cent., but in the interior of the continents it occasionally exceeded 45 per cent., spring or summer being exceedingly dry, whilst the winter was excessively damp, as at Yarkand, where a humidity of 30 per cent. in May contrasted strikingly with a humidity of 84 . per cent. in December. This great range directed attention to the influence of temperature (and of alti- tude) upon the amount of relative humidity, for during temperate weather we were able to beara great humidity with equanimity, whilst the same degree of humidity, accompanied by great heat, such as is occasionally experienced during the ‘ heat terms’ of New York and recently in London, may prove disastrous to men and beasts. Hence, combining humidity and temperature, the author suggested mapping out the earth according to sixteen hygrothermal types, as follows :-— 1. Hot (temperature 73° and over) and very damp (humidity 81 per cent. or more): Batavia, Camaroons, Mombasa. i Hot and moderately damp (66-80 per cent.): Havana, Calcutta. Hot and dry (51-65 per cent.): Bagdad, Lahore, Khartum. Hot and very dry (50 per cent. or less): Disa, Wadi Halfa, Kuka. . Warm (temperature 58° to 72°) and very damp: Walvisch Bay, Arica. Warm and moderately damp: Lisbon, Rome, Damascus, Tokio, New Orleans. . Warm and dry: Cairo, Algiers, Kimberley. Warm and very dry: Mexico, Teheran. . Cool (temperature 33° to 57°) and very damp: Greenwich, Cochabambo. 10. Cool and moderately damp: Vienna, Melbourne, Toronto, Chicago. 11. Cooland dry: Tashkent, Simla, Cheyenne. 12. Cool and very dry: Yarkand, Denver. 13. Cold (temperature 32° or less) and very damp: Ben Nevis, Sagastyr, Godt- POAT oe PS 14. Cold and moderately damp: Tomsk, Pike’s Peak, Polaris House. 15. Cold and dry: 16. Cold and very dry: Pamir. The actual mean temperature of the earth amounted, according to his computa- tion, to 57° F., and this isotherm, which separated types 8 and 9, also divided De Candolle’s ‘ Mikrothermes’ from the plants requiring a greater amount of warmth. V'he author further illustrated his paper by a number of diagrams giving the curves of the temperature, rainfall, and humidity, and also by a chart of the world exhibiting the number of rainy days. 5. The Origin of Moels, and their Subsequent Dissection By J. E. Marr, F248. In this paper, the influence of vegetation in modifying hill-outlines is first considered, and it is shown that the concave curye of water-erosion is partly iri «et TRANSACTIONS OF SECTION E, 819 replaced by a convex curve of weathering on the upper parts of hills, with herbaceous vegetation in temperate regions, and often entirely replaced by a convex curve in tropical regions, where the sides of the hills are clad with forest rowth. 3 The dissection of such round-topped hills or moels by stream action is then considered, and it is pointed out that buttress-like lateral peaks will be formed around the resultant central peak. Lateral peaks of this nature have been described by Mr. I. C. Russell on Mount Rainier, under the name tahomas; he gives reason for their production by glacial denudation in that particular case. 6. On the Pettersson-Nansen Insulating Water-bottle. Sy HueH Rosert Mitt, D.Se., LL.D. Professor Pettersson has, in conjunction with Professor Nansen, completed a modification of his well-known apparatus for obtaining samples of sea-water without change of temperature. A specimen of the improved water-bottle con- structed by Messrs. Ericsson, of Stockholm and London, was exhibited. The purpose of this apparatus is to enclose a quantity of sea-water at any desired depth, to hold it securely, and to bring it to the surface without any change of tempera- ture exceeding one hundredth of a degree Centigrade. The previous form of insu- lating water-bottle was found by Dr. Nansen in his arctic expedition to be less trustworthy at great depths than in shallow water; hence the suggestions which resulted in the new apparatus. The insulation, which is the essential feature of the water-bottle, is secured by a series of concentric chambers of non-conducting material which are simultaneously filled with water, and so protect the portion, measuring about two litres, which occupies the large central tube. The walls of the inner tubes are so constructed as not to become heated by compression at the greatest depth. This is secured by using metal, which is heated by com- pression, and indiarubber, which is cooled by compression, in such proportions as to ensure constancy of temperature for the whole structure. The water-bottle when set is held apart, so that the base, sides, and lid are separated, and the water passes freely through the tubes as the apparatus descends. When the apparatus is being drawn up a propeller (which during the descent revolves freely) engages with a screw and releases a heavy weight, which closes and locks the whole rigidly together. An arrangement is provided for the relief of pressure as the included water expands on being hauled up, The temperature is ascertained by a thermometer, protected againt pressure, enclosed in the central tube, and projecting sufficiently far to be easily read. If preferred, the aperture for the thermometer may be closed by a screw and the thermometer inserted when the water-bottle is brought up. A reversing thermometer to give the temperature of the water independently may be attached to the upper part of the water-bottle, and is set in action at the moment of closing. The whole apparatus weighs about 58 lb., and is used on a wire line and worked by a steam winch. During August of this year the improved water-bottle was tested by Professor Nansen on board the Michael Sars in the sea between Iceland and Spitsbergen, and at the greatest depth met with (3,000 metres =1,670 fathoms) the insulation was perfect. On August 11 a sample was taken from 3,000 metres, and when it came up the thermometer read: 1°-285 C., after five minutes 1°283, after nine minutes 1°-270, and after eleven minutes 1°210. On August 13 in a sample from 2,000 metres the thermometer showed 1°-135, after five minutes 1°-135, after six minutes 1°-180, and after eight minutes 1°-110. Professor Nansen considers it essential to use an included thermometer. ‘Published in full in the Geographical Journal, vol. xvi. (1900), pp. 469-471. 820 REPORT—1900. Srction F.—ECONOMIC !SCIENCE AND STATISTICS. PRESIDENT OF THE SEcTION—Major P. G. CratciE, V.P.S.S. THURSDAY, SEPTEMBER 6. The President delivered the following Address :— Tun ‘ Advancement of Science’ is the motive wherewith the British Association brings annually together, in autumnal conclave, a gathering of those who desire to tell and those who wish to hear something of the most recent developments of scientific labour. Entrusted for the session with the high honour of presiding over a Section where the chair has from time to time been occupied by a long roll of distinguished men, whose qualifications for the task necessarily far outstrip any I could pretend to claim, I may yet follow the example set by such authorities in maintaining on your behalf, and on my own, that the right production, the proper treatment, and the wise grouping of garnered facts concerning man and his relations to the State as a member of society constitute a study second in importance to no other form of research. Moreover, such expert discussion of statistical methods and statistical results as ought to be possible in this Section should, I think, prove a factor of no small moment in its bearing on the true advancement of Science in its broadest sense, whether physical, economic, or political. Without the claim to speak to you on the lines which could be appropriately adopted by some former Presidents, who have held positions of eminence, won either in the highest fields of politics or earned by patient work in the cloistered retreats of academic study, I come here rather to represent those who form, as it were, the hewers of wood and drawers of water for the economic controversialists of the day. As such we are concerned in the daily outturn of raw statistical material, and we are naturally jealous as to the use to be made of our figures by those who employ them in the process of scientific deduction, in the business of practical administration, or in the efforts of philosophic teaching. Whatever be the precise meaning we are willing to accord to the term of ‘ statisties’—and both the primary interpretation and the proper scope of the expression have been differently construed—I believe you will agree with me in echoing the opinion expressed, I think, by a very distinguished past President of this Association, that nearly all the grandest discoveries in science have been but the rewards of accurate measurement and patient long-continued labour in the sifting of numerical results. Not only thus may we claim for what is sometimes looked upon as the merely mechanical part of statistical work a directly educational effect on the honest workers themselves, in the training and discipline of mind which are required for the handling and weighing, the balancing and comparing of numerically arranged facts; we may go further and assert that every science in its turn has occasion to TRANSACTIONS OF SECTION F. 821 rely on the statistician’s art, and that the true advancement of knowledge in what- ever path we take depends quite as much on the avoidance of rash conclusions as on the faculty of quick perception of apparent results, There is then this lesson to be learned in the discussions to be held in this Section, and it is one on which, in opening our deliberations, I think I am fairly entitled to insist. Since accurate statistical data are fundamental to sound areu- ment and correct deductions in any sphere of science, too great care cannot be expended in the task of making sure that figures given to the public are really what they claim to be. Where a comparison is to be made it is our business to see a practical identity in the character of the facts to be observed, and to give such warning as is requisite to guard against the possibility of over-strained and illegitimate use of the data by those into whose hands they may ultimately come. Where a deduction is to be made or a conclusion is to be announced by the original compiler himself, it is well, too, he should remember that a statistical decision should have in it something of judicial deliberation and gravity, and should be given to the world only after the application of a chastened scepticism and distrust to the testing of the first impressions to which the bare numbers that appear on the surface of any calculation seem to point. Lastly, let us not overlook the prescriptive cautions of many past masters in statistical work to distrust big totals and dissect general averages. We are all of us familiar with the vastly larger space accorded to statistics in debate in the second half of the dying century, how readily the arbitrament of figures is now appealed to by the politician or the journalist, by the man of science or the philosopher. This very fact, however, constitutes in itself a danger, and I trust, therefore,I may be forgiven if I interpose between the Section and its prepared work by preaching from the Chair with some insist- ence the somewhat trite doctrine that statistical and economic science has few greater enemies than those who fail to apply the most rigid tests to the sufficiency of the elementary figures on which a theory is to be formed or an administrative act accomplished. Nor, indeed, is a much smaller offence involved in the over- confident use, whether for international comparisons or for those flights of prophecy in which we all like from time to time to indulge, of figures not in their immediate connection themselves erroneous, but which are, nevertheless, not quite strong enough to bear the strain of the superstructure to be reared, or which are devoid of the essential elements of true comparability of condition. It is then alike for the makers and the users of statistics to observe much caution in their own utterances and in the manufacture of those missiles of con- troversy which every table furnishes, and which in the hasty discussions of our day, when mere rapidity is exalted almost to the place of a virtue, are apt at times to prove dangerous to those who wield them, whether in the press, the lecture- room, or the senate. Most of all is it incumbent on one who ventures on the duties of this Chair with none of the opportunities of reflection which many professorial predecessors must have enjoyed, and who comes straight from the daily turmoil of executive work and the discharge of continuous official service, to exercise some reticence in venturing on expressions of individual opinion. In what I may say, therefore, by way of preface to your discussions I would endeavour to confine my remarks to a notice of some of the chief statistical investigations now impending and an account of the difficulties to be encountered by the statistician in his work, illustrating, from the class of subjects with which my work has made me familiar, the sorts of obstacles which hinder the accurate presentation of international comparisons of agricultural conditions. The entire omission cf a sectional address—for which there is, I believe, pre- cedent in your records—or the substitution of a simple speech for a reasoned paper, as was allowed to the distinguished statesman who presided at the last Bradford meeting, on the score of the demands of the State on the services of its servants, might, perhaps, have met my case and relieved me of a duty to which I feel far from equal, and you of listening to my crude remarks, This indulgence has not, however, been accorded, and I must, therefore, crave the pardon of the Section I can 822 REPORT—-1900. only serve so badly, and urge its members, in the later discussions, to supply the shortcomings of the occupant of the Chair. Of all statistical work the enumeration of the units of population must ever take the foremost place, and on the eve of the census to be taken before man more months have passed a reference to that great impending task could hardly be omitted on this occasion. In common with all students of the machinery of census-taking I am sure I echo the feelings of the Section—as I do those of the Royal Statistical Society, who have long laboured in this direction—in deeply regretting that the first census of the twentieth century is not to possess the distinction many had hoped to see conferred upon it of being by preliminary announcement—as I hope it may prove to be in ultimate fact—the first of a series not of decennial but of quinquennial countings of the people. The growing complexity of social conditions and speed of life in all its functions at the present date, contrasted with the leisurely movements of a hundred years ago, would alone and amply justify a more frequent stock-taking of the inhabitants of Great Britain than has been the practice in the past. The practical wants of our much-multiplied system of local government cannot fail, I believe, ere long to bring about the granting of an intermediate numbering, even if for the moment other considerations overrule the more academic pleas of statisticians for this reform, or the arguments, sound as I believe them to be, for a permanent Census Office, a permanent Census Act, and a trained and continuous Census Staff, to whom preparation of the machinery beforehand and detailed elaboration of the results after the actual census year might with real economy be entrusted. Like probably many another student of practical statistical organisation, I have to own to some modification of the demands for enquiry into the condition as well as the numbers of the people, which I once believed might be properly combined with the actual operations of enumeration. Some little experience in measuring the extent and the value of the answers elicited by question and by schedule have shown me that with due regard to the quality, if not even to the quantity, of the replies extracted from the least instructed section of the popu- lation, you must limit your curiosity unless you are to be landed in doubt, in difficulty, and in misconception. Specific and parallel enquiries in point of time by one or another central body may no doubt be devised and directed so as to bring out a definite and limited series of facts, affording matter to be compared with population totals. But to load the census proper with side issues is not to help forward the best type of statistical knowledge, and the attempt may well be pushed too far. I fancy there is now some reason to believe that ten years ago we erred in this respect. For these reasons I have never in recent years been able to go along with many active and highly intelligent foreign colleagues, whose more sanguine aspirations as to possibilities of what a census can tell it is always pleasing to witness, even if the feasibility of their suggested developments may be questioned. Sound and reasonable advice on such a subject may be found in the timely remarks of my colleague Mr. J. A. Baines, in his paper to the Royal Statistical Society in February last on the ‘limitations’ of census-taking. From no better or more practical source could we hope to be instructed on what can and what can not with advantage be got than from the able officer whose superintendence of the vast Indian Census of 1891 brought him such widespread recognition. The mention J haye made of the suggestions of foreign statisticians on census- taking reminds me that although the proposal which has been before the Inter- national Statistical Institute in one form or another for a synchronous ‘ world’s census,’ at the moment of passing from one century to another, is hardly likely, for administrative reasons and in view of the previous fixtures of the great census- taking Governments of the earth, to be literally realised, the dates of the great countings of the nations will nevertheless come sufficiently close for all practical comparisons. The great Russian enumeration, on the success of which M. Troinitsky is so heartily to be congratulated, is not yet long accomplished. The twelfth census of the United States is now being taken. The Scandinavian enquiry TRANSACTIONS OF SECTION F, 823 coincides with the century’s end, the Italian and the Spanish censuses are already overdue, and both France and England take their count within a few months alter the twentieth century has begun. Not persons only, but their conditions, their possessions, their trade, and their burdens are all subjects of perennial statistical enquiry, and in connection with the last of these groups in the near future the attention of statistical critics will no doubt be drawn again to the massive collection of materials respecting local taxes, their growth and pressure, which may be looked for from the final report of the Royal Commission on Local Taxation. How many times in the last half of this century this section of our finance has been debated here I have not been able to ascertain. In one form or another it has exercised a fascination on the minds of some of our most active economists. Personally I confess the field was one of the first in which I ventured to make some enquiry and draw tabular comparisons. To this I was incited by the study, not at first of the second-hand stores of the many blue-books which have seen the light on this matter, but rather by the peculiar circumstances of my local residence in a Yorkshire township four-and- thirty years ago, when local government and local rates of necessity came home with primary concern to one who happened, like myself, to be the sole inhabitant householder of an area constituting for several purposes a unit of local administration. I cannot pretend to have followed through the later years of the century the wider developments of these controversies, which were far from simple even in the days when the issue was limited to a question of pressure of the ratal system on agricultural land. Now, when the vast and complicated outlay of the great urban centres on matters which, in time past, we were not disposed to regard as subjects of taxation at all, but rather of directly remunerative outlay, has to be brought into the survey, it may well tax the ingenuity of our younger statisticians to unravel the facts, and it may try the courage and the skill of the economists to pronounce, as this Section may be expected to do before its sittings close, as to the orthodox limits and sphere of ever-extending municipal expenditure and municipal trade. The statistical part of such enquiries as these will abound with problems in the working out of which it will be well to recall the warnings I have indicated as to the danger attending the use of non-comparative or defective data. Pitfalls innumerable await the less wary controversialist in such questions as these, which seem near at hand, while yet wider discussion on the relative pressure and com- parative growth of taxes generally may erelong attract renewed attention, as well as the subjects of statistical debate which centre round the records of crime and its punishment, of educational facilities and the economic results of their super- vision by the State, or, again, of excursions into the intricate region of labour and wages, wherein some of our section have already pursued useful investigations. In all and every one of these topics the scientific statistician will have to re- member that his profession does not allow him to be a partisan advocate of one or the other view, in search of some figures to illustrate or decorate a predetermined theory. On the contrary, his function is to work in the cold, clear light of pure scientific research, and with a single aim to free the facts of each case from obscurity and place the data before the world in such shape as to allow a true judgment to be recorded. Quite as full of difficult problems and obstinately non-comparable figures will be found to be the use of statistics of production and of trade. The varying and scanty records of one period may have to be viewed in connection with and inter- preted by the better and fuller data of the day, and the conditions of one country may have to be contrasted with those of another, while the puzzling variations in the system employed have to be allowed for and discounted in the conclusions. Perhaps the difficulties of just comparison between the records of one time and another, or one State and its neighbour, come home to me with peculiar emphasis when the statistics dealt with relate to agricultural conditions. With ourselves 824 REPORT—1900,. and still more in certain quarters abroad regular agricultural statistics are of quite recent birth. It is difficult, perhaps, for us now to recall the comparatively recent origin of comprehensive statistics of agriculture in Great Britain. Writers of note, economists, and philosophers had no doubt from early times ventured to make estimates of more or less individual authority on the probable magnitude of our agricultural resources, Expert witnesses, with more or less opportunities of indi- vidual observations, came before Parliamentary Committees with rough impressions of the extent of our cultivated area and the distribution of the crops which it bore. The labours of the old Board of Agriculture, which existed at the end of the last and for a few years at the beginning of this century, amassed, no doubt, much valuable though scattered local information and many details of farming practice, but they completed no such exact survey as would have proved invaluable now to the statisticians of 1900 respecting the use made of the soil of our country a hundred years ago, The erroneous estimate of 47,000,000 acres of total area assigned to Eng- land by the Chairman of that Board, when later data proved the measurements to yield 10,000,000 acres less, is a warning of the care which is needed in the use of such figures as were available in those distant days After efforts more or less spasmodic in 1831, again in 1845, and yet again in the more complete work of the Highland and Agricultural Society of Scotland in 1854— 7, encouraged by the verdict of the House of Lords’ Committee of 1855, and fortified by the repeated recommendations of International Statistical Congresses, the House of Commons was, in 1864, persuaded by Sir James Caird to pass a resolution for the establishment of annual agricultural returns. These were first collected in 1866, and one year later they took the more complete form which gave us the continuous records Great Britain now possesses for tracing the development or retrogression of our country in agricultural conditions throughout the last third of the nineteenth century. ‘The data thus obtained must, of course, be read with full allowance for some minute but inevitable variations of definition due to the gradual improvement and growing completeness of the returns themselves, first under the Board of Trade, then under the care of the Privy Council, and now under the Board of Agriculture. Agricultural statistics, whether in this or other countries, are assuredly not exempt from the need of careful and intelligent handling and of caution in drawing comparisons, The leading features to which any agricultural enquiry is directed are naturally the extent and characteristic modes of the occupation of the surface, the number of persons engayed and the size of their holdings, the area and yield of the distinctive crops, and the numbers and classes of live stock. Some of these points can, and others with advantage cannot, be made the subject of direct annual enquiry and compilation. But in all cases questions as to precision of definition arise when the careful investigator looks below the surface to see what the figures really mean. The total measured areas of the countries we desire to contrast may, it is true, be fairly accurately given, though even here there is room for error, in regard to the practice of including or excluding areas covered by inland and tidal waters, lakes, and rivers. When the next step is taken, and it is desired to contrast the respective areas actually made use of for productive purposes, difficulties of com- parison at once present themselves. The phrase ‘ cultivated’ area in our country Is one to which, at least in unofficial if not in Government publications, two distinct meanings are often attached. The term is sometimes used as if in some sense synonymous with the arable surface, whereas in the other, and with us by long tradition the official sense, the term covers all land, other than woodlands or rough wastes and mountain grazings, utilised for agriculture, whether under the category of permanent grass or under yearly varying crops. Nor is uniformity of practice much greater as regards the methods of returning the actual agricultural population. The number of persons actually employed, male and female, may as a rule be distinguished, but all countries are not agreed as to what employment means. The practice as to who are and who are not to be regarded as dependents, or as occasional and casual workers, may vary greatly, In all countries, and perhaps rather more abroad than here, there are aT TRANSACTIONS OF SECTION F, 825 many persons who combine an agricultural with some other calling, and this in an infinitely varying degree. The German and some other statistics endeavour laboriously to give tables which take account of these persons with double occupations and allot to them a place under more than one head. In England we have no provision in our census for these cases, and a farmer and brewer or a labourer engaged sometimes on a farm and at other times at other work may be classed by the accident of the first entry in one or other category at random. By what is nearly a common consent, the attempted enumeration of the agriculturally occupied population is connected rather with the general enquiries of the census than with the crop returns of each year. Its value of necessity depends on the coincident and relative record of the occupations, other than agricultural, in which the inhabitants of any country are engaged. Such con- siderations supply the answer to some of our less reflective writers on this question, who would have a perennial investigation going on into the available supply of agricultural labour—year by year, if not month by month. The move- ment in the direction of concentration of growing numbers of the workers of a nation in the urban districts, which is apparent in so many countries besides our own, and under the most opposite conditions of Governmental polity or agri- cultural organisation, will no doubt form in a short time a very interesting topic of statistical discussion. But the general figures cannot be handled with very great advantage now at the distance of wellnigh a decade from the last enumera- tions and at the moment when the taking of a new census is at hand. Until that enquiry reveals its facts, the student of questions of relative rural population may be referred to the mine of information collected by the Royal Commission on Labour, and the late Mr. W. OC. Little’s admirable and exhaustive analysis, and to the most valuable statistical buff-book which the Board of Trade have just issued from the pen of Mr. Wilson Fox. Equally or even more full of pitfalls for comparison are statistics of the size of holdings, whether the comparison be made between one date and another in a country like our own, or between one country and another. Not only will the grades employed necessarily vary between country and country, but the starting- point and definition of what is a ‘ holding’ is usually entirely different. In one of the earliest meetings of the International Statistical Institute at Rome I drew attention to the barrier thus offered to international comparisons on the latter point. I then showed how occasionally it may happen that the recog- nised ‘ boldings’ seem to have included every plot, however minute. Germany and Belgium, and I may add Ireland, apparently made a beginning at zero. Great Britain at one time regarded a quarter of an acre as a limit of statistical enquiry, although since 1892 restricting the term ‘agricultural holding’ to something over an acre of land. Elsewhere, as in Holland and in the United States, refusals, except under specially defined conditions, to take anything less than a plot of two and a half or three acres in extent as a starting-point in the agricultural enumerations are encountered. It is not always remembered that we ourselves have, even within the com- paratively brief course of our official agricultural returns in Great Britain, held more than one opinion as to what the siarting-point should be. At the first collection of these statistics nothing under five acres was taken account of as agri- cultural, ‘lhe scope of the annual enquiry was subsequently extended to plots of a quarter of an acre, and the limit was raised again eight years ago to the present requirement, which refrains from requesting annual details of the acreage of their crops from the occupiers of holdings of a single acre or less. As a matter of administrative convenience there is very considerable advantage in the course now pursued, and no real statistical loss is involved, for the land occupied by the various petty crofts or gardens which escape annual record was found not to reach one-tenth of one per cent. of the cultivated area, and such rare changes as might occur in the crops raised on these minute sections of territory could in no perceptible degree affect the value of the returns as affording a general view of the current change of agricultural practice, Changes, however, in the unit of 826 REPORT—1900. area, as well as changes even in the direction of improvement in the machinery of collection, are all hindrances to very close and accurate comparisons. Attempts have no doubt been made to enumerate separately the strips of land held as gardens or allotments, at different dates, in England, but considerations such as I have above indicated have rendered the results of much less statistical value than can be claimed for the yearly returns, and the failures of some of these repeated attempts furnish a conspicuous warning against overloading the never very simple task of rural stock-taking by too frequent and necessarily costly enquiries into very minute points of agricultural condition. Even in records of the numbers of animals there is room for much misunder- standing. ‘Horses’ are defined differently in the returns of different countries, at one place the numbers including trade and private horses, in another only those engaged in agriculture. The ages and the classes of the animals, and the dates of the collection again, may and do vary considerably, and this may bring in lambs in one country and omit some portions of this group in another. Even cows, it is found, may mean one thing in one country and another in another, and may be returned with other cattle in a single class or shown separately from other horned stock. Oxen are shown in some countries with no distinction of class or age ; in others those still used for working the farm may be distinguished from those reared for purposes of meat production only, All these cautions are only examples of the danger of venturing on too close reliance on data of this kind in interna- tional comparisons. Over and above all difficulties due to difference of agricultural practice and local definitions, the most serious bar to exact comparison of the course of agriculture in different countries is the widely varying practice as to the intervals at which statistics are collected. Live stock may be enumerated, as with ourselves, in France, or in the United States, annually, while wide gaps occur between the years of stock-taking elsewhere. The acreage of each crop in each season may be recorded in one country ; in another five or ten years, in some cases even fifteen, may elapse between the enquiries on this essential point, and estimates of produce checked by no local examination of the surface occupied too often prove delusive guides to the results of particular years. These gaps are the dread of any one who sets himself seriously to examine what has been the general movement either in the changing areas of crop distribution or in the relative growth or decline of agricultural production abroad. Continuous annual data of acreage, production, and live stock ought, however, to be within the reach of most fully equipped Governments of modern times. The method of the collection will necessarily differ. Information obtained direct from the immediate producer by written schedule is perhaps available nowhere but in ourown land. ‘The fact is one which says something for progressive intelligence and the general support which the State receives from the great bulk of farmers of Great Britain, and the working of our system has attracted much attention of late from those responsible for the conduct and development of agricultural statistics in foreign countries, We may pardonably view our position in this country with satisfaction when it-is recognised how largely foreign correspondents are yearly seeking for more and more information as to how so big a statistical operation is annually accomplished here between June 4 and August 28 in the time and with the machinery at our command, To the statisticians of Russia, Spain, Italy, Germany, Denmark, and even of Japan we have had lately to explain our process. Could some approach to this system be obtained, the means for accurate measure- ment of the world’s agricultural movements would be greatly helped, and it may at least be hoped that a generation hence facilities will abound for a closer review of the position of food supply and production than is now feasible. But it is not necessary to wait quite so long for some general glimpse of the facts. Already in France, Germany, Austria, Hungary, Roumania, Russia, and the United States among foreign countries, in our Indian possessions, and in our Australasian colonies, we find indeed annual statements—not all, however, collected similarly—of the area under the principal grain crops. Two only of the provinces of the Canadian Bat' TRANSACTIONS OF SECTION F. 827 Dominion venture on annual returns. Annual, if later, figures reach us from the smaller States of Holland and Sweden, and from Algeria and Japan. It is not for us here, like amateur war-critics distributing praise and blame from our armchairs on statisticians engaged in local conflict with the difficulty of crop- collection abroad, to forget the relative compactness of the area of these islands and the relatively developed intelligence of an agricultural population farming, on the average, larger holdings than most of our continental neighbours. We ought not, therefore, to refuse to appreciate the difficulties, administrative and financial, which a close adoption of anything like the British system would involve, either where the peasant population is predominant or where the areas to be accounted for are vast, as in the United States or in Russia. It is, I think, in the circumstances not illegitimate to use, at all events for comparison of the state of matters within the same country, the data which are now available from year to year. With less confidence we may even quote, as presumptive indications of the directions of movements, the isolated returns of acreage for particular years which alone some States supply. That there is peril, however, in such a course may be seen by what is proved to have happened in a country like France, whence we do receive continuous data. For the past quarter of a century the acres devoted to wheat in France have been practically the same, 17,000,000 acres. One single exception appears, however, in the season of 1891, when under exceptional climatic conditions an area of only 14,000,000 acres was reported. Now, had France rendered only occasional acreage records, like her Belgian neighbour, like Denmark, or like Argentina, and had the year 1891 chanced to be the date of the enquiry, an investigation of the rise or fall of wheat culture in Europe might have been deflected from a true conclusion by the deceptive record of a state of matters occurring only once in a single exceptional season, and immediately recovered from. In any attempts which may be made, even within the period of fairly reliable agricultural statistics, to trace the features of the changes of the past twenty or thirty years, it is necessary to remember that, as between one country and another, the data can be received only with much reserve, and as strictly comparative, if even that, only within the respective States compared at different dates. Attempts to utilise statistical data, to determine the relative development of agriculture in different parts of the world and at different periods of time, are sometimes made with regard solely to what is described as the world’s aggregate of one or two leading individual products as typical as the rest; or, again, one or two typical countries, or at least countries where the available information is more complete than elsewhere, are chosen, and the course of development or decline of their crop areas or the several descriptions of their animal produce is traced and compared. Certain obvious objections, which it is well to recognise, impede the student of figures who resolves to proceed on the first of these methods. At the outset he is arrested by embarrassment attending the choice of what single products are to be held as representative of agricultural outturn. The most usual of all selec- tions is that which restricts enquiries to the case of wheat. This course appears to be rendered, comparatively speaking, easy, as more has probably been written and more statistics, official or unofficial, theoretical or commercial, actual or imaginary, have been compiled, with regard to this bread grain than for any other crop. But it is time we recognised that wheat has had too much and too exclu- sive attention directed to it as a type of agricultural production. Very widely as it is undoubtedly used in the form of bread, even as food its place is occupied at one time or another, and in one country or another, by other substitutes, and its cultivation is, after all, not the employment which demands the most attention and most skill at the hands of the agriculturist. Not only do rye and even maize serve as substitutes or supplements in feeding man, but other crops, such as oats, barley, millet, rice, and so on, have claims to greater notice than they receive, and play a direct as well as indirect part in providing food. Cotton, flax, and wool are other typical products, the use of which for clothing is all-important 828 REPORT—1900, to an enormous population, and the extension or retrogression of such crops deserves some of the attention of the agricultural statistician. Tea, coffee, wine, spirits, and beer are, it is not to be forgotten, agricultural products in one clime or another, either directly or indirectly ; and crops so important as sugar or tobacco are almost to be classed as necessaries of existence. Of yearly growing importance is it also, in these days, when the animal portion of our food supply bulks so much more fully than before in the daily rations of populations as they grow in wealth and increase in consumptive power, that we should closely follow the fluctuations in the live stock maintained for food and learn the teaching of the agricultural returns on the manufacture of beef, of mutton, of pig meat, or of milk. The growing requirements of our 40,000,000 of population in this country— dependent for a large proportion of their meat on cattle, sheep, and swine fed in other lands and in some of the most distant countries of the globe—have pro- voked a series of enquiries into the extent of our domestic production and the density of the herds and flocks maintained on like areas of the surface of the other and different regions. It is half a century since Sir James Caird, in calling the attention of farmers to what he foresaw was the certain growth of the demand for butcher’s meat, for milk, and for butter in the United Kingdom, argued that as the expenditure of the lower classes increased the development of household outlay with increasing means would necessarily take this direction. Venturing a little beyond the safe ground of statistical deduction as to what was forthcoming from our own stock, it is true he prophesied that it would not be found practicable to import fresh provisions coming from distant countries, and he therefore suggested that the enterprising home producer would have the full market here practically at his own vommand, The same authority repeated in 1868 his advice as to the direction the development of agriculture here might take, placing the extent of the reliance of the British consumer on the foreigner at only one-ninth part of his supply of meat, and one-fifth of his consumption of butter and of cheese. That these ratios have altered since, to the detriment of the producer, if to the benefit of the con- sumer, assuredly does not render the need of statistical enquiry into meat and milk production less urgent than it was as a most important factor in the nation’s food supply. Sixteen years ago, when this Association met at Montreal, I ventured to lay before this Section some data on the nature and extent of our meat supplies and the scale of our production, based in the latter case mainly on the very practical investigation of a former President of the Royal Agricultural Society—Sir H. M. Thompson—but adapted to the data of the current agricultural returns of live stock. For numerous purposes the formula I then employed has since been followed as convenient for serial comparisons of annual results in the statistics founded on reports by Royal Commissions and Parliamentary Committees. But no student of statistics will contend that the conditions of agricultural production are ever absolutely permanent, and I have seen there are not wanting opinions that it may be needful, from one cause or another, to revise the scales of the calcu- lation, and to compare the most recent rate of meat production in this country with that of other lands. Few subjects seem to me to possess more practical interest for those willing to aid in statistical research, competent to apply to the numerical data a cor- responding knowledge of the development of stock-feeding in recent years and in different countries. I commend a re-investigation of this subject—and the kin- dred one of milk production and the manufacture of dairy produce in this country and abroad—on the lines in the one case of the inquiry of 1871, and in the other on the lines which Mr. Rew suggested in a paper in 1892 to the Royal Statistical Society—to the best attention of a younger generation of estimators. Whether and how far the earlier maturity of our present breeds of sheep and cattle and swine has resulted in the production of a larger annual volume of meat is a factor which should have careful consideration, and if a careful inquiry should suggest the time for revision has arrived respecting the 67 tons of beef, the 124 tons of mutton, or the 694 tons of pig meat I and others haye hitherto used as the equi- TRANSACTIONS OF SECTION F. 829 valent of the annual production of 1,000 animals of each type respectively I should not be unprepared to make whatever change is proved needful, despite the re- luctance with which every statistician forsakes, even on good grounds, a basis of conversion which has served without break of continuity for the comparison of more than thirty years. How largely the demands of a population like our own have upset the old pro- portions of our reliance on imported meat and imported milk products may be learned from the fact that the latest calculation which I have made suggests a meat consumption of no less than 132 lbs. per head in the United Kingdom, against a little over 100 lbs. thirty years ago, more than two-fifths of the whole now reaching us from foreign countries or British possessions, against the ninth part at which Sir James Caird estimated the foreign quota. The mention of these meat estimates suggests a reference, by way of illustration, to the extremely interesting and legitimate application of the important deductions . from purely agricultural statistics possible when once the temptation to narrow the question to one of wheat production and wheat supply is resisted, which was made by my colleague, Mr. Crawford, in a paper read to the Royal Statistical Society last winter. The calculations made dealt with the relative dimensions and sources of the food supply of the United Kingdom, France, Germany, and Belgium. The deductions made from the data available, and the useful discus- sions thus provoked—including a supplementary memorandum by Mr. Hooker on the relative forces occupied in production under the differing conditions of British and Continental farming—are replete with interest to the future investigator who is willing to face the labour of looking below the surface either of agricultural statistics or of import or export returns into the economic meaning of the situa- tion thus disclosed. No lesson, perhaps, of this paper is more worthy to be remembered than the warning which it gives to the class of writers who, without a due appreciation of the facts, are as ready, from the vantage-ground of the editorial chair, to fight the battle of the agriculturist for him on paper, as to teach our generals how to handle a British army in the field. But for considerations often overlooked, which were on this occasion put forward, the abolition of our dependence on sea-borne produce, it is sometimes argued, could be procured by a simple extension of our own agricultural area. What that extension would have to be it is now shown is something much more serious than many imagine. It is not alone that to fill the gap of our imports of wheat and flour would take another 6,000,000 acres of the prolific quality of our own, but the direct production of the imported meat and dairy produce and of the numerous feeding stuffs required for the manufacture of our present quota of animal food raised at home would at the most modest computation necessitate 17,000,000 acres more to be added to our productive area, and that, be it remembered, without withdrawing any portion whatever of our present surface, which, whether under crop or grass, helps to sustain our outturn at the present level. The prospects of a practical annexation of this aggregate of 23,000,000 acres to those now under cultivation at home I confess do not seem to me great. Although the attempt to grasp the relative magnitude of the agricultural production of one State as compared with another;‘or to note the growth or decline of its prominence in the cultivation of particular staples, or the manufacture of particular kinds of human food, is always an enterprise of difficulty in existing statistical conditions, it is one which has fascination for many classes of economists and politicians. If attempted at all it is well to recognise that there are inevitable dangers in tke task, and that if any figures are relied on as conclusive their meaning must be interpreted by some knowledge of the demographic conditions of each State and its geographical, climatic, and agricultural circumstances. Taking a few of the most conspicuous products of the soil, it will generally be found that a very few leading States are so particularly identified with one or other type of production that the examination of their records is therefore available as a guide to the course of a single crop. 830 REPORT—1900, Probably quite two-thirds of the cotton of the world is g¥own in the United States alone, where the surface so employed reaches 25,000,000 acres as compared with under 9,000,000 acres in British India, the next largest cotton-growing region of which statistical record exists. In wool the produce of the Australasian Colonies of Great Britain—with flocks which still exceed 100,000,000 head—makes much the largest contribution to the total. In rice, so far as statistics carry us, our Indian possessions head the list of producers. In hops the English crop still probably exceeds the German in production, although the latter with larger area closely contests the place. In tobacco, while the acreage apparently employed in British India is nearly double the 595,000 acres in the United States, no other country in our statistical records comes within one-seventh of the American area. The vineyards of Italy are returned as covering 8,500,000 acres, and those of France 4,300,000 acres, while those of Austria and Hungary, next in magnitude, cover but a seventh part of the last-mentioned figure. Russia bulks largely as a grower of flax, and alone shows a whole third of the area of barley recorded in all the countries which supply returns, and if in the case of potatoes the Russian acreage is not very different from that of Germany the total produc- tion of the latter empire reaches the largest aggregate of any single country. If the subject of enquiry be the place of wheut-growing in the world at one date or another, it would not be to the older European countries, other than Russia at all events, we should turn to see where the surface so utilised was extending, Reckoned by the percentage of her cereal area which she still devotes to wheat, France, with 47 per cent. under the crop, or Italy, with 55 per cent., would naturally be selected as typical wheat-growers; but both are practically in a stationary or, collectively, even in a. slightly retrograding position. It is on the other side of the Atlantic where the most noteworthy movements have occurred. In comparatively new exporting countries, such as Argentina and Canada, though the statistics from neither are complete, wheat areas still extend, and that of the United States, though fluctuating with great sensitiveness under vary- ing price conditions, and moving from one centre to another westward or north- westward across the American continent, is now reported as covering 44,600,000 acres. This total, it must be allowed, whatever views may be held as to future progress, makes the United States a typical grower of this particular cereal, to which it gives an importance second only to the still more extensive product of American soil, to which we give the name of maize, but to which alone in Ameri- can parlance is allowed the title of corn, The leading changes in the production of typical crops as measured by the acreage, and the stock of cattle, sheep, and swine recorded at or near the com- mencement, the middle, and the close of the past thirty years, may be contrasted for exporting countries with expanding populations and growing agriculture, and in countries where these conditions are absent, or in a typical consuming centre like our own country. Relying on the agricultural returns of the United States, a table could be constructed, as under, for three dates within the past thirty years which furnish the following indication of agricultural changes :— United States 1870 1885 1899 Population, in million persons . 5 : : 38°6 56"1 76:0 Area under maize, in millionacres . : : 38'6 731 82-1 Area under wheat A - a 4 19:0 34:2 44:6 Area under oats “e ‘ 88 22°8 26°3 Area under cotton a ; . 99 18:3 25:0 Cattle (million head) ‘J . 25°5 43°'8 43°9 Sheep z paeieg th ae ae 40:9 50-4 41-9 Swine " 5 E ¢ : 26'8 45-1 38°7 In 1870 the United States held, it would thus appear, a population of are TRANSACTIONS OF SECIION F, 851 38,600,000, and grew an acre of maize for each unit of the population, and an acre of wheat for every two persons, and somewhat more than an acre of cotton for every four. At this period the surplus exported to other nations, it may be added, represented two-thirds of the cotton, rather more than one-fifth of the wheat, but less thau one per cent. of the maize. In 1886 the population had augmented to an estimated total of 56,000,000, or by 45 per cent. The area under the crops above quoted had meantime been ex~ tended in nearly twice this ratio. The United States exported still about two- thirds of the cotton grown; the wheat export was slightly greater in proportion to the product than before, or 26 per cent., while nearly 3 per cent of the maize crop found a market abroad. The population of the States is now estimated to have risen to 76,000,000, or twice what it was thirty years ago, although the census has yet to say if this calculation has been realised. The cultivation of maize had meantime reached 82,000,000 acres, wheat was reported to cover 44,000,000 acres, and cotton 25,000,000 acres, while the foreign market received 65 per cent. of the cotton, 35 per cent. of the wheat, and now as much as 9 per cent. of the maize grown on these areas. In none of these cases, it will be noted, has the area under crop failed to increase, but in all the rate of increase was distinctly slower in the second than in the first half of the period. If time sufficed to trace the annual course of move- ment between the contrasted dates, it might be well remembered that from 1871 onward to 1889, with only a single slight check in 1887, the growth of the maize acreage has been continuous. From 1889 to 1894 fluctuations were reported yearly, ending in the latter year at a total acreage no higher than that of 1880, but returning again in a single year, if the record can be trusted, to, the highest point reached. The wheat acreage movement has been more irregular, and the latest figures are complicated by the admitted corrections which were made to an amount of 5,000,000 acres for too low previous estimates in 1897. Allowing for this, the regular upward movement of the wheat acreage was apparently checked in 1880, and has only begun again since 1898 under the stimulus of higher prices in that year. In live stock the development would seem to have been arrested altogether between 1885 and the end of the century in the case of cattle, and turned into an absolute decline in the number of sheep and swine, although in the fifteen years before 1885 cattle had increased more than 71 per cent., swine 74 per cent., and sheep 26 per cent. As a matter of fact the maximum number of cattle was reached in 1892, when the numbers were 54,000,000, or ten millions more than at present, the stock of swine declining in a still greater ratio from the same year. and sheep declining and rising again in the separate periods between 1883 and 1889, and between 1893 and 1897. If the ratio under each head to population is considered, it would appear that the United States possessed 661 cattle for every 1,000 of her citizens in 1870. This was raised to 829 per 1,000 persons in 1885, while the ratio now has fallen again below the starting-point, or to 604 per 1,000 persons, Sheep have fallen in the thirty years from 1,060 in 1870 to 880, and now to 537 head only per 1,000 inhabitants. These remarkable changes are worthy of note in connection with the exports of living animals and animal products, which last have been maintained at a still higher level than before. Turning to a country of nearly stationary population, provided for in the main from its own agricultural produce with only slight assistance from abroad, a like con- trast for the beginning, the middle, and the end of the period under review will give roughly the results shown below. Here, although we are provided with an annual figure, the start has to be made after the Franco-German war with the data two years later, or in 1872. (For table see p. 832.) ThusinFrance, where wheat-growing has always had such a predominance amon the cereals, the area is neither increasing nor diminishing. The total of 17,000,000 acres falls, however, somewhat short of the provision of an acre to two persons, 832 REPORT—1900. which held good in the United States; but this is more than corrected by tlie higher average yield, which is nearly 5 bushels per acre greater in France than in America. Taking wheat and rye together, there are a million acres less of bread corn grown in France than there was when her slow-moving population was two millions smaller, or less than 58 acres to 100 persons now as against 60 acres to the 100 twenty-eight years ago. France 1872 1885 1899 Population, in million persons . . . 36:1 38:2 38°5 Area under wheat, in million acres i 17:1 17-2 171 Area under oats Ss P je 14) 9:1 ADEE Area under rye =F : 4:7 41 3°6 Area in vineyards 5; 65 4:9 4:3! Cattle (million head) ‘ 11:3 131 13°41 Sheep ” . : P : F 24:6 22°6 21:3! Swine ff : : oy ee : 54 58 6-2! The changes which the last quarter of the nineteenth century has seen in the leading features of French agriculture may be easily summarised, The popu- lation of 1872 but little exceeded 36,000,000, that of 1885 reached 38,000,000, and the latest data only bring it up to little over 38,500,000. The wheat-growing area remains, it would appear, under all conditions practically at 17,000,000 acres, the only break to the general uniformity of the cultivation of this cereal (with which the returns include spelt) occurring in the season of 1891, when, under ‘exceptional climatic conditions, only 14,000,000 acres were harvested. There is one typical French agricultural product—wine—which has materially declined under circumstances which are well known. The vineyards of 1872, which were reported as covering 6,500,000 acres, are now returned as less by a third cf that area, and covering 4,300,000 acres only. In cattle a material growth up to 1885, but a very small increase since that year, is reported ; while if sheep, asin all European countries, are fewer, the fall is less than in Germany, and it is most marked in the first half of the period. Swine in France have steadily increased. As regards the cattle, it may be noted that France had 313 cattle to each 1,000 of her people in 1872, 345 in 1885, and 352 per 1,000 now. Of sheep the number per 1,000 is 560, against 681 at the earlier date. Treating a few of the distinctive points of our own agriculture in the same way at the beginning, middle, and end of the past thirty years, the statistics of the United Kingdom would give these results :— United Kingdom 1870 1885 1899 | Population, in million persons . 31:2 36:0 40°7 Area under wheat, in million acres . 3°8 2°6 21 Area under oats Fr 4:4 4:3 4-1 Area under other corn crops _,, ° : 3°6 3:1 26 Cattle (million head) . . . . 9°2 10-9 11:3 Sheep ” . a 32°8 30:1 al Swine os 37 37 4:0 Here the most striking contrast with France is in the growth of population. From being a country with 5,000,000 fewer inhabitants the United Kingdom is now one actually greater by 2,000,000 persons than is France. This isan increase of more than 80 per cent., while the surface under wheat has heavily fallen, the main loss occurring under circumstances which have been amply discussed between 1 In 1898 TRANSACTIONS OF SECTION F, 833 1875 and 1895, With some revival, as in America, consequent on an improve- ment of price in recent years, the slight apparent decline I have shown in the cultivation of oats is in fact confined to Ireland, the area in Great Britain being greater than at the beginning of the period. The cattle stock of the United Kingdom is increased by some 23 per cent., and the swine by about 8 per cent., while our flocks of sheep have been maintained at a level far exceeding that of other European States, and distinctive in a peculiar manner of the agriculture of Great Britain, for they still represent, as it appears, on the average 400 sheep to every 1,000 acres of land, against 164 in France, 81 in Germany, 32 in Belgium, and 17 in the United States. Passing to a comparison with another great country, which, like the United States, is a typical exporter of more than one form of agricultural produce, it may be asked how far the available statistics of Russia allow such information to be furnished. For the earliest of the three years contrasted the dates for the Russian empire are meagre and unsatisfactory. Poland must be excluded as blank in our statistics at that time, while as regards animals no figures at all would appear to have been made public for any of the last twelve years. With such qualifications as these, the available data for the nearest year in the larger crops stood as under :— Russia in Europe (ea Poland) 1870 1885 1899 | J aes Population in million persons . 65°7 81:7 9423 | Area of rye in million acres 66°4} 64:6 634 | Area of wheat * 28:7} 28:9 38:0 Area of oats “4 , 3 32°8! 34:9 36'1 Area of other cereals in million acres 2 31:4 34:2 Cattle in million head 22:8 23°6 ? (246) # Sheep ” 48:1 46°7 2 (44:5) # Swine 9% 9-1 9-42 (9:2) 4 . . . . . oe - O OOOO ee Thirty years ago the population of European Russia, ex Poland, would appear from such data as we possess to have been estimated in round numbers at under sixty-six million persons. It is given as somewhere about eighty-two millions in 1885, and according to the recent census it is ninety-four millions now. The bread corn of the country continues to be much more largely rye than wheat, and the area in the year 1872, for which statistics are available, occupied by the former crop was practically an acre to the person, or in all 66,400,000 acres, less than half an acre per inhabitant, or 29,000,000 acres, being under wheat. The combined surface devoted to these two bread grains together was thus 95,000,U00 acres in the aggregate, or 145 acres to every 100 persons. Fifteen years later, when the population was apparently greater by 16,000,000 persons, or 24 per cent., the statistics of rye acreage indicate 2,000,000 acres less than before, or 64,600,000 acres. The wheat acreage, if the official data be accepted, was little if at all in excess of the 1872 figure, the rye and wheat together roughly giviug 115 acres to 100 persons. The suggestion of this decline, while the exports of both grains were maintained or extended, affords an opportunity for closer enquiry into the basis of the published returns which are received from that country. But carrying the review of the official figures further, the very latest data for this section of the Russian territory would appear to indicate a yet further shrink- age in the acreage of rye, but accompanied now, as was apparently not the case until lately, by a considerable increase in land under wheat. The total of this cereal is now put as high as 38,000,000 acres, but the net available area of bread- stuffs, although brought up to 101,000,000 acres, represents a still diminishing ratio to population, or 107 acres to every 100 persons. Moreover, as Russia must 1 In 1872. 2 In 1883, * Census of 1897. ‘ In 1888. 190 0, 3H 834 P REPORT—1900. be regarded as growing both wheat and rye for export as well as consumption, the larger proportions of her acreage which is employed in feeding a non-Russian population deserve to be specially marked in this connection, when the low yields of both cereals are remembered. Whether the foregoing figures do indeed represent the facts of each period is, I think, a worthy object of enquiry for some of our younger statisticians, and it is a problem one would like to see solved as regards this particular country before venturing on any too confident conclusion as to what is the real meaning of the changes of the past, and what may be the future position in regard to the growth of breadstuffs and the growth of population in the world as a whole. Calculations, however, such as those just quoted cannot fail to remind the student how very different in productive power the ‘ acre’ of wheat may be, and is, in different countries. Assuming that we take the existence of 38,000,000 acres as reported of wheat land in Russia in Europe (ev Poland) to be proved, a com- parison of the estimated yields shows that such an area represents less than 12,000,000 acres of the productive power we are accustomed to in Great Britain. So, too, for the vast wheat area of the United States, it takes two and a third acres to produce what is now our average yield in this country. Three Indian or three Italian acres of wheat of the calibre now in use would in the same way be required to supply the number of bushels that a single acre of our soil in the climate we enjoy, and worked under the system of farming that we practise here, would in ordinary seasons produce. In other extensive areas of wheat-growing the yields, though greater than the above, are very considerably below our own, the Austrian, Hungarian, and French yields standing at 16,17, and 18 bushels respectively, against the 30 bushels which is apparently the average yield of the last five years in the United Kingdom. Only when we come to very small total areas do we find instances where the average wheat yields approach or over any consideyr- able periods exceed our own. When Denmark, for example, is referred to as reaching 42 bushels per acre in the season of 1896, it is not to be forgotten that only a minute area of selected land, in this case only 84,000 acres, is devoted to this cereal. Results realised on this small scale can hardly be spoken of as an average in contrast with those of countries where millions of acres are grown, and can usually be paralleled in some sections of the bigger country. Nor should it be forgotten, if the agricultural position of one State be com- pared with another, how widely the conditions of different parts vary from the picture presented by the average figures credited to the State as a unit, and how often sections of one country differ more from each other agriculturally than from the country with which they are contrasted. Within the United Kingdom alone we are, or ought to be, familiar with essential local differences of this type, which have to be kept in mind. Even in respect of the relative density of population and the number of mouths to be sustained in a given area, it may be quite correct to describe every 1,000 acres in the United Kingdom as carrying on their surface on the average 519 persons, but it may be remembered with advantage that, considered geographically apart, Scotland, for example, is a country of but 220 persons, and Ireland of but 219, to the 1,000 acres of area. Such a position suggests that it might be fair to draw our agricultural com- parisons between Scotland or Ireland as units of area, and such a country as Denmark, where the population is 248 to the 1,000 acres. Thus one-third of the cereal area of England is still devoted to the growth of wheat, while Denmark has but 8 per cent. so occupied, thereby resembling Scotland or Ireland, where some 4 per cent. only of the corn is wheat. Similarly, on this population basis, Austria with 320 persons, or Switzerland with 311, to the 1,000 acres may be not inappropriately classed with Wales, where the density is $45. In particular an examination of the live stock maintained by each 1,000 acres of the surface in all these cases affords parallels and contrasts which are both interesting and instruc- tive. (For table, see p. 835.) Thus Wales bears easily the palm as regards the total stock of sheep carried, while Ireland, with a population practically bearing a similar ratio to that of TRANSACTIONS OF SECTION F. 835 Scotland to her surface, has more than three times as dense a stock of cattle and more than eight times as many pigs, although not much more than half as many sheep to the 1,000 acres. Although beaten as regards the number of pigs maintained on a given area by Denmark and by Hungary, Ireland’s cattle are more than twice as numerous relatively as those of France, where the population is not so very different in proportion to the soil. Per 1,000 Acres of Total Area Country Persons Cattle Sheep Swine Treland . : f é 219 217 207 61 Scotland. E A : 220 64 390 7 Hungary. 3 : ; 232 85 102 92 Denmark . = 5 248 186 115 88 France . 2 ‘é 293 103 164 48 Switzerland . 5 ‘ 311 132 27 57 Austria . F - ; 320 117 43 48 Wales . : “ ‘ 345 147 685 50 ———e Among countries where the areas are still greater in proportion to the resident population it may not be without interest to group together—as regards their present density—persons, cattle, sheep, and swine. Per 1,000 Acres of Total Area Countries Persons Cattle Sheep Swine New South Wales . : 7 10 221 il New Zealand . 3 d 11 18 294 3 Victoria. . A : 21 32 234 6 Norway . f : F 26 13! 18} 2 United States . : F 32 19 17 17 “Sweden. . : : 49 25 13 | 8 Russia (ex Poland) . 4 66 20? 36? WE ST Such figures serve to emphasise the vast difference between the flocks main- tained in our Australasian colonies and the other countries in this group. The animal wealth of England by herself, omitting the Celtic fringes above quoted, may be compared with a nearer competitor. Belgium has 893 persons to 1,000 acres, England 925; and Belgium has 195 head of cattle and 160 head of swine, but only 32 sheep, on an average area of this size in her little kingdom, against 144 cattle, 64 pigs, and as many as 488 sheep in England. Were the comparison to be made more closely yet, the cattle stock of Belgium agrees closely in point of density with, say, the particular division of our area com- prising the north-western counties of England, which have 194 cattle to 1,000 acres, or considerably more than the great butter-exporting country of Denmark, and at least a very close approach to the 197 head per 1,000 acres which are to be found in the fat pastures of the Netherlands. These limited comparisons on single points of agricultural production in single countries do not, I know, satisfy the demands which are often made for world-wide surveys and comparisons on a larger scale. I confess I somewhat distrust the streneth and due coherence of tke statistical bricks on which these heroic conclusions are built up. It is most usual in corn trade journals, and the practice is sometimes followed in serious debate and repro- duced in the year-books of the United States Government, to give a yearly 1 In 1890, ® In 1888. 836 REPORT—1900. picture of at least the world’s wheat crop. For the close comparison of one season with another much must depend on the sufficiency of the weakest item in the account, and weakness is sure to creep in somewhere when crops are estimated on varying systems, at different dates, and on authorities of unequal value. The definitions adopted by one calculator as to the limits of the ‘world’ vary from those of another, and commercial estimates, as they are called, may be, at the discretion of the computer, substituted for or adopted in the absence of official data, so that the guesses at a single country’s harvest may differ more widely from each other than wouldaccount for the total margin between one year’s aggregate supply and another, to the confounding of satisfactory conclusions as to what is really happening. Last but not least of the obstacles to uniform grouping of harvests in complete years—ending as these years do at different periods—is the fact, not to be overlooked, that wheat harvests are being gathered somewhere in every month in twelve. One is driven back then to the attempt to rest opinions on the growth of one form of culture or another on recorded acreage, rather than assumed production. Yet even here a good illustration of the difficulty of any extensive compilation may be found in the tentative memorandum Sir Robert Giffen put before the last Royal Commission on Agriculture as indicating, with many necessary reservations and qualifications, the relative movements of grain area, live stock, and population in the twenty years before 1893. Briefly, the earlier totals brought into conjunction for this purpose were made up, as regards the population figures taken to represent the starting-point of 18738, from the statistics of groups of countries and colonies at dates for the most part about 1871-3, but in some instances ranging back to 1866 and on to 1881, and aggregating 365,800,000 persons, Against these were set a total of 461,800,000 persons, enumerated, for the most part, about 1890-93, but in a few instances, where later data were wanting, going back to 1880-88, the growth of population between the totals being 26 per cent. The acreage about 1873 and about 1893, contrasted with these figures, included wheat, rye, barley, and oats, but not maize—a larger crop than any of the last three. ‘The countries contrasted were limited necessarily by the extent of information, and the list did not include all of which the population was accounted for, the increases per cent. being 28 per cent. in the case of oats, 19 per cent. in the case of wheat, 5 per cent. in the case of barley, with a decrease of 5 per cent. in rye. It should be observed, however, that the calculation as to the increase of wheat would have been much closer to that of population had not a very large area, nearly stationary in amount, been credited to India and Japan at both dates; the local population of these Asiatic countries being disregarded as, generally speaking, non-wheat-eating. It was only as an outline pointing the direction in which enquiry might be useful that Sir Robert Giffen called attention to these figures, which, as he acknow- ledged, were of the roughest possible description, and rather suggestive of a closer enquiry, which should take account of the difference between the consumptive power of the countries aggregated, the varying productive power of nominally equal areas of surface, and the varying type of live stock maintained. If the wheat acreage table, in the memorandum referred to, is examined in detail, a very effective picture of the difficulty of exact comparison as between any two given dates is incidentally presented. Out of twenty-four countries enumerated (including Canada and Australasia as units) a twenty or twenty-one years’ coraparison is only really effected in five cases—Russia, the United States, France, United Kingdom, and Australasia. In five other instances the period dealt with is only from seventeen to eighteen years; in three other casas only fourteen or fifteen years. In Canada, Egypt, and Denmark, the comparison will be found to be more limited still, and only to cover eleven or twelve years ; while in the Argentine Republic, where the recent expansion of wheat-growing has been prominent, the available statistics allowed only of a comparison of two periods, no more than nine years apart. For seven other countries the wheat acreage was necessarily either omitted or inserted as presumably the same at both the earlier and the later date, Had the retrospect been confined to the cases where a twenty =—s os ao TRANSACTIONS OF SECTION F. 837 or twenty-one year's’ comparison was possible—and these, after all, included the most important and typical wheat-growing communities—the increase would have stood, not at 19, but at 24 per cent., or scarcely below that of the growth of population generally. This result is reached without taking account of any South American figures, where the increase of area is relatively much greater, or of those of India, where the comparison is difficult and the acreage growing but slightly. But, further, it is to be remembered that if the comparison of the memorandum were to be continued up to 1899, instead of stopping at 1893, the figures would have shown that wheat-growing had apparently made a new start in the five important countries for which the lone comparison was possible, as many million acres having been added in the past six years as in the whole pre- ceding twenty—a result which may afford much occasion for suspending our final judgment and no little warning of the danger of single-year contrasts. Since the above calculations were before the Commission there has been an extension of 10,000,000 acres in the official estimates of wheat areas in the United States, and 5,400,000 acres in Russia, while, although official details are still wanting beyond 1895 for Argentina, nearly 3,000,000 acres more were in that year accounted for in that republic; and there is an impression, apparently well founded, that by the present time the total may have reached 8,000,000 acres, or nearly five million acres more than the final figure in Sir Robert Giffen’s calcula- tion. If anything like 20,000,000 acres have thus been added to the wheat- growing surface of the globe in the last five or six years, which these further figures suggest, even if no correction be made for the Indian quota, there may be much less difference than was suggested in the memorandum between the growth of population and wheat-growing. : Without attempting in any way to controvert what was one of the lessons of the memorandum f{ have been examining, as to the tendency to increase the numbers of cattle at a ratio above that of population, it has also to be remembered that the apparent 37 per cent. increase there shown between 1873 and 1893 may have to be discounted by subsequent deductions in the United States, in Aus- tralasia, and at the Cape in recent years; while it is one of the problems I have never yet seen satisfactorily answered, why in almost all old countries except our own the diminution of the stock of sheep seems continuous and remarkable. I mention these matters only, however, to suggest the amount of uncertainty which must attend the efforts to arrive at conclusions, made even by the highest authori- ties, on the only data which exist. If there is, as I have shown, such uncertainty still in the facts on which a conclusion could be built as to the past history of the relative growth of live stock, or of cereal culture and the supply of bread-stuffs, how much greater must the difficulty be of those who attempt, on the basis of such data, to forecast the course of events for a generation yet tocome! I confess I am not intrepid enough to follow some of the conjectures which have been hazarded on this point, and can only, in concluding this address, recur once more to the prime qualifications for safe statistical deductions with which I opened my remarks—redoubled caution in handling calculations, a very guarded use of data giving records of single and isolated years, and a wise reservation in any prophetic pictures of the future of agricultural production, whether of wheat or cotton, in meat or in wool, of the contingency, always present, of altered con- ditions which ever and anon in the past have altered and falsitied the predictions of earlier observers, The following Reports and Paper were read :— 1. Report on Future Dealings in Raw Produce.—See Reports, p. 421. 2. Report on State Monopolies in other Cowntries.—See Reports, p. 436. 838 REPORT—1900, 3. Population and Birth-rate, viewed from the historico-statistical standpoint. By Marcus Rusty, Director of the Royal Danish Bureau of Statistics. As is well known, it has become more common than furmerly for historians to seek the help of statistics to support, as far as may be, with observations of groups, those scattered records which frequently give misleading results, A not un- important part of the investigations undertaken, and of the tracts, &c., published by the author outside his official reports, have been coneerned with kistorico-statis- tical investigations. One of the earliest of them—published in 1882—was con- cerned with the question of the number of the inhabitants of Copenhagen in the seventeenth century, an inquiry based on the records of baptisms in the church registers for that century. The paper offers an extension of the discussions of principle to which that inquiry gave rise. The chief question to be answered is the following: Assuming that the number of baptisms at some period in the past can be ascertained for a town or a country, how can its population be deduced from that number? As a rule the registers give information only of baptisms, not of still-births. In general, at any rate in Denmark, children were baptised as soon as possible after birth, so that the numbers not baptised may rather be compared with the still-born of later times. Given the number of baptisms at some period in tke past, this number must first be subjected to an addition before it can be compared with the record of births of recent times (living births and still-births), At the beginning of the present cen- tury the still-births were some 8 per cent. of those born alive. Thus to find the number of births of the earlier times at least 8 per cent. must be added to the number of baptisms. Having obtained this datum, what multiplier will yield the total of the population? This is dependent on whether people in former times married earlier than now; further, on whether marriages were more fruitful ; and, finally, on whether the number of illegitimate births was greater. It is quite clear that if, in comparison with the population, more children were born in preceding centuries than nowadays, the multiplier must be made less than would serve now to deduce population from births, and vice versa. Unfortunately, the old Danish church registers contain no record of the ages at marriage, but one may assume that people married earlier than at present, because such a course was in agreement with the needs and wishes of the time, whether considered from the point of view of State, of Church, or of public opinion. I have secured information on this point from the records of a census of Den- mark in the year 1787, which exist in the Danish Statistical Bureau, but have not been published hitherto. This census proves the following both for town and country :—In former times the well-to-do and independent section of the population married earlier than now, while the masses married later. This is a consequence of the fact that the labouring classes were not then free as now, but boarded in their master’s house, and for this and other cognate reasons were obliged to delay marriage; whereas nowadays they need not wait; indeed they often find advan- tage in marrying young. The more well-to-do, on the other hand, married as soon as they could, since in old days people did not take our modern views in social matters, but regarded it as both the right and the duty of men (and of women) to marry as soon as law and custom made it possible. But, further, not merely did all marry as soon as they might, but they married as often as might be, 2.é., there were fewer widows and widowers than in our time, since none who could marry remained unmarried. To sum up, on the average the age of marriage was higher than in our time, because the masses were compelled to postpone marriage, but in spite of this the number of marriages was greater, partly because the well-to-do married earlier than now, partly because the masses married, almost without exception, as soon as they could, and, further, partly because the widowed remarried in far greater proportion than now. ‘The statistical proof of the fact is given in the paper, where it is also shown that precisely the opposite happens nowadays to that which occurred formerly. Now the well-to-do marry late, the masses early} Although, on the average, marriages were later than now, yet the number 1 See Table I. TRANSACTIONS OF SECTION F, 839 of children to a marriage was at least as great as in our time. In our time the fertility of marriage is determined partly by physical, partly by social causes. Formerly the fertility of marriage was as great as nature permitted, just as marriage was undertaken as freely as the law and the economic development of the community permitted, not as nowadays, when people remain unmarried though not restrained by the fact of being unable to afford it. In spite of the marriages taking place later on the average, the fertility of marriage was not less than now. This position is established in the paper by means of statistics. Finally comes the question of illegitimacy. A result of the masses being com- pelled to defer wedlock to a later age than now was that the number of illegitimate births was greater than in our time. This cannot be proved directly, but the paper shows, by the use of modern statistics, how the number of illegitimate children increases as the age of marriage among the masses increases. I am confident that the rule can be laid down for Denmark that in former times, both within and without the bonds of wedlock, more children were born relatively to the population than in our own time. The tendency towards a diminished birth- rate which can be shown for our time (and is demonstrated in the paper) did not exist of old. That the population did not increase was due, not to a small natality, but to a great mortality, as is also shown in the paper. When the number of the baptised in former centuries is determined, a smaller factor must be used with which to multiply it, in order to deduce the population, than would be appropriate for our time. If the number of baptisms in former times be multiplied by 30, the numbers of the population will probably be determined to within 10 per cent. of excess or defect. The following tables illustrate some of the more important facts to which allusion is made :— TastE I.—Change in the Ratio of Civil Conditions at each Age-group in Denmark. ; 100 in each Age-group and for each of the Sexes. Males Females Ages Unmarried | Married | Widowed | Unmarried] Married | Widowed (a) Census of 1787. 20~40 56°6 426 0:8 44-9 53'0 21 40-60 88 86°9 4:3 8:0 176 14-4 60 and over 3°8 75:5 20°7 6:0 46:0 48:0 20 and over B31 62:2 AT 26:6 60°1 133 (b) Census of 1890. 20-40 48'8 50:1 11 43:5 54:4 21 40-60 8:8 85:0 6:2 12:0 734 14:6 60 and over 6:4 67:0 26°8 96 42-2 48-2 20 and over | 28:2 64°6 72 27:1 58:2 14:7 Taste II.—Change in Numbers in different Age-groups. Of every 1,000 Males Of every 1,000 Females Ages 1787 | 1801 1880 1890 1787 1801 1880 1890 0-20 408 | 409 440 454 401 403 416 423 20-60 512 503 471 450 506 498 482 469 60 and over 80 88 89 96 93 99 102 108 1,000 {1,000 |1,000 j1,000 |1,000 |1,000 {1,000 | 1,000 ee Se ee ee ee a ee 840 REPORT—1900, FRIDAY, SEPTEMBER 7. The following Papers were read :— 1. Results of Experimental Work in Agriculture in Canada under Govern- ment Organisation, By Wiuitam Saunpers, LL.D., Director of Canadian Experimental Farms. For some years prior to 1884 agriculture in Canada was in a depressed condition, and during that year a Select Committee was appointed by the House of Commons to inquire into the best means of encouraging and developing the agricultural in- dustries of Canada. From the investigations of this Committee it was shown that farming in Canada was at that time in a very defective condition, that there was a lack of thorough tillage, that no sufficient measures were taken to maintain the fertility of the soil, that there was a want of knowledge in regard to rotation of crops, and of the selection of improved varieties of seed; that lack of information existed also in reference to many of the principles underlying the successful rearing of stock, the manufacture of dairy products, and the growing of fruit. This Committee recommended that the Government establish an Experimental Farm where experiments might be carried on in connection with all branches of agriculture, horticulture, and arboriculture, and that the results of these experi- ments be published from time to time and disseminated freely among the farmers of the Dominion. In 1886 an Act was passed by the Parliament of Canada authorising the Government to establish a Central Experimental Farm and four Branch Experi- mental Farms in different parts of the Dominion, and during the two years following these farms were established and set in operation. The results of twelve years’ experience have shown that these institutions have been highly beneficial to the farming community. Experimental research has been carried on along the lines prescribed by the Act by which these farms were established, and much information has been accumulated and distributed freely to the farmers of Canada in reports and bulletins. Benefits have thus been con- ferred on Canadian farmers in connection with all the more important farm crops, in the development of the stock and dairy industries, in the production of fruits, in the growing of trees for shelter and timber, and in the advancement of other - branches of arboriculture. Much attention has been given to experiments relating to the maintenance of the fertility of the land, to the best methods of cultivating the soil, to a proper rotation of crops, to the best time for sowing, and the selection of the best and most productive varieties for seed. By freely spreading the information gained, supplemented by a liberal distri- bution of samples of the best and most productive cereals, crops have been im- proved, and the attention of farmers generally awakened to the importance of adopting such measures as will result in increased crops. The steady advance- ment which has taken place within recent years in Canada, and the increasing prosperity of agricultural industries, may in large measure be attributed to the useful work of these Experimental Farms established and maintained by the Government in different parts of Canada. 2. The Economic Possibilities of the Growth of Sugar Beet in England. By A. D. Hati, WA., Principal of the South-Eastern Agricultural Col- lege, Wye. The sugar beet can be grown successfully in the south and east of England ; the yield of sugar per acre is equal, if not superior, to the yield in other countries, where the industry is conducted on a large scale. The economic question of the value of the industry is confused by bounties and TRANSACTIONS OF SECTION F, 841 duties; it is therefore necessary to ascertain the possible profit of the crop at the price of sugar which prevails in the open British market. Itis also desirable to find the value of the crop for consumption on the farm, pending the general establish- ment of factories to deal with the roots grown in each district. In 1898 a series of trials was carried out on farms in various parts of the country ; the average yield per acre was 15} tons of unwashed roots. This figure is probably too high, if roots with a high sugar content are grown; in the same year the average yield of six German estates, where an intensive system cf cultiva- tion is practised, was only 10:7 tons of washed roots per acre. In 1898 six different kinds of sugar beet were grown upon the farm of the South-Eastern Agricultural College at Wye, Kent, the crop being managed in the same manner as the adjacent mangold break; the average yield per acre was 14 tons of unwashed roots, as against 29 tons of mangolds. The sugar content was highly satisfactory, the season being one of prolonged warmth: it is calcu- lated that about 1} ton of sugar per acre could have been extracted, representing a gross return of 18Z. 10s. In several respects the crop is more expensive to grow than mangolds; manure and cultivation were found to cost 10/. 8s. per acre, to which rent, supervision, and all incidental charges must be added. The roots grown were stored with the mangolds until spring, and given, together with cake and corn, to two selected lots of sheep, with the general result that each sheep consumed 63 lb. of sugar beet per week, against 146 Ib. of mangolds, and that the increase in live weight was 30°6 per cent. with beet and 37°2 per cent. with mangolds. Recalculating on a basis of acreage required: ten- elevenths of an acre of sugar beet will provide the same amount of succulent food for sheep as an acre of mangolds, and will supply 38 sheep for 12 weeks; the sheep on mangolds will, however, make 293 lb. greater increase in live weight. The experiment showed that the beet forms an indifferent fodder for sheep. Turning to the general question of the return to the farmer, the average price paid in 1898 in the six selected German cases mentioned above was 19s. 6d. per ton for roots delivered at the factory. Assuming from the 1898 experiments an average English production of 14 tons of dressed roots per acre, the gross return to the farmer at the above price would be 187. 18s. The cost of cartage from the factory to the farm must be taken into account: it is estimated that the 3,000 acres of sugar beet which Lawes and Gilbert specify as required to maintain a factory would mean an average distance from farm to factory of four miles, the cartage over which distance would cost about 30s, per acre for the 14-ton crop. When this is added to the cost of cultivation and an allowance made for rent, &c., there is no margin left for the farmer from the gross return of 131. 13s. per acre set out above. The 19s. 6d. per ton for roots is a price that is not possible in this country, the price payable for the raw material being dependent on the price of sugar. Taking similar grades of sugar, the return received by the German manufacturer was in January 1900 13s. per ewt., while the price in England was 11s. 3d. per ewt. ; a difference of 35s. per ton of sugar. As 7} tons of beet are required to produce a ton of sugar, this difference in the price of the finished product is equivalent to a reduction of 4s. 8d. per ton in the price payable for roots. The English figures, then, become: Average yield per acre, 14 tons; price at the factory, 14s. 10d. per ton; gross return to the farmer, 10/. 8s. per acre ; against an expenditure which has been set at 11/. 18s. per acre, without including rent. The success of the sugar beet industry depends upon several factors :— (1) Cheap technical skill in the factories. (2) A farming community working for smaller returns than prevail in Britain. (8) A system of bounties and countervailing duties. For further details see the Jowrnal of the South-Eastern Agricultural College. 842 ‘ REPORT—1900. 3. The Economical Position of the Agricultural Labourer considered historically. By Frank P. Waker, B.Sc. 1. Historical sketch of the chief phases in the history of agricultural labour, noting— The Black Death, some of its results. The depreciation of the coinage under Henry VIII. and its effects. Poor relief and the settlement and allowance systems. Competition the farmer has now to maintain (i.) in the market for labour with manufacturing operations, and (ii.) in the produce market with foreign supplies of food. 2. Three tables derived from replies to a form of questions attached to the paper and sent to certain farmers of my acquaintance. These show :— (a) An increase in the amount of land laid down to permanent pasture. (6) An increase in the wages paid for the several kinds of piecework concomitant with (c) An increase in the weekly wages paid for all kinds of agricultural labour, 3. Notes on these replies, and conclusion. 4. Trade Fluctuations. By Joun B. C. Kersuaw, F.S.8. The author stated that this subject had attracted in the past the attention of many minds, especially in times of commercial depression, and that the records of the Royal Statistical Society and of the Economic Section of the British Association proved that the members of these two learned bodies had not neglected to under- take their share in this investigation. But though some of the keenest minds in the realm of economic science had attempted to discover the laws which govern trade fluctuations, these phenomena of the industrial and financial world were still largely unexplained. The currency, protection, free trade, war, famines, labour disputes, trade unionism, radical governments, and sun-spots had been advanced at one time or another as chief causes of the periodic depressions from which British trade suffers. Each of these explanations had, however, on examination proved unsatisfactory and insufficient to account for the fluctuations revealed when the trade figures over along period of years were subjected to scrutiny in the light of the particular theory. One theory, however, had seemed to the author worthy of further examination and inquiry, and for some months he had been collecting statistics bearing upon it. The theory was that first advanced by Sir William Herschel, and supported in a qualified manner at a later date by Giffen,! Jevons,” and Binns.’ Briefly summarised it was as follows:— Normal trade between any two countries when reduced to its ultimate compo- nents was seen to be simply an exchange between the commodities which they pro- duced. The countries of the world might be roughly classified as those in which the produce is chiefly that of the soil, or in which it is chiefly that of the hand and brain. The agricultural labourer and the skilled mechanic were therefore the repre- sentative human units of the two great divisions of employment, and all commerce was merely the exchange or barter of the products of their activities. The volume of trade must consequently be dependent upon the volume of crops if this theory of commerce be correct; and a series of bad harvests, using that term to cover every 1 Journal Royal Statistical Society, vol. xlii. p. 36. 2 Currency and Finance, chap. 1x. % Journal Manchester Philosophical Society, December 1894. ae TRANSACTIONS OF SECTION F. 843 product of the soil, must sooner or later have their effect upon the trade in manu- factured goods. The trade statistics dealt with related to the value and volume of the exports of the United Kingdom for a period of forty-three years; and statistics relating to the total world crops of cotton, wheat, and sugar had been sought, with only par- tial success, for the same period. These three agricultural products were selected because they are those upon the ample provision of which British industrial activity and prosperity appeared most largely to depend. ‘The period 1856-1898 was selected because during these years British export trade had experienced most severe fluctuations, and also because the nearer one approached to the end of the century, the more reliable and complete were the statistics relating to trade and crops. The figures collected by the author in the course of his inquiry, with full infor- mation as to their source, were given in an appendix to the paper; and for the pur- poses of comparison they had been thrown into diagrammatic form, which was distributed at the meeting. * The curve showing the volume of our export trade year by year since 1857 was marked by dips in 1860-62, 1873, 1876, 1835, 1831-93, and in 1897-98. The curve showing the volume of the sugar crop of the world was marked by dips in 1861, 1864, 1868, 1872, 1875-77, 1880, 1886, 1888, 1896, and in 1898. The curve showing the volume of the cotton crops of the four leading producing countries since 1870 was marked by dips in 1872-738, 1877-79, 1882, 1884-85, 1889, 1893, and in 1896, The curve showing the volume of the wheat crops of the world since 1876 was marked by dips in 1879, 1883, 1885, 1888-89, and in 1895-97. Finally a compounded curve showing the total crops of cotton, wheat, and sugar since 1876 was marked by dips in 1879, 1885, 1888-89, 1893, and in 1896-97. In conclusion the author claimed that the theory of a connection between trade fluctuations and agricultural prosperity found support in the figures he had pre- sented. Many causes no doubt combined to produce trade depressions, the mental mood of bankers and capitalists—so ably discussed by Mr. John Mills before the Manchester Philosophical Society in 1867—being one of these, and sudden change in foreign tariffs another. But the cause discussed in the author's paper was not less important, and when fuller statistics relating to wheat were available he hoped to continue his investigations. SATURDAY, SEPTEMBER 8. The Section did not meet. MONDAY, SEPTEMBER 10. The following Papers were read :— 1. Municipal Trading. By ARTHUR PRIESTMAN. _ The recent action of the London Chamber of Commerce and the Royal Com- mission. _ The commercial world does not object when the trading helps them in their private undertakings. The increase and extent of municipal trading in U.S.A and other countries. Sir Henry Fowler's figures and the Blue-book returns. Comparison with capital invested in co-operative societies, Reasons urging still 1 The Paper will be published in the Journal of the ‘British Economic Association.’ 844 REPORT—1900. further municipal enterprise: (a) health and housing; () milk supply; (c) tele= phones; (d) fire insurance; (e) savings banks; (f/f) drink; (gy) combinations amongst traders. Monopoly by combination of private traders in comparison with a municipal monopoly. ‘General user’ theory. Artificial raising of wages by municipal standard rate of wages. Can a city councillor undertake so many and increasing duties? Possibility of reintroduction of cottage industries by cheap municipal electric power supply. Conclusion. : 2. Municipal Building for the Overcrowded. By AUBERON HERBERT. We can supply this want either by the system of free trade, which has dore so much for us, or by enlarging once more the area of compulsion. The real question is then: Is compulsion a good or a bad thing? Undoubtedly it is easy and con- venient ; but does it not tend to bring serious evils with it—disagreement, care- less and expensive management, corruption? does it not make children of us, spoiling the temper of compeller and compelled ? Let us see how the land lies. Looking round at Europe to-day we see a general failure of highly organised systems of compulsion. Writers of different schools complain that parliamentary institutions are breaking down. Almost everywhere minorities are in revolt against majorities. They obstruct, prevent discussion, and lock the machine. Once we hoped great things from the system of majorities and minorities. The sting was to be extracted from human disagree- ments, and we were to live side by side in a happy family. Unfortunately men have discovered that majorities are very keen to pursue their own particular interests; that to be in a minority means to lose all control, perhaps for many years, over one’s own mind, body, and property, and that the ingenious precept that it is the duty of minorities to turn themselves into majorities, and so to possess the promised land, is rather like the nursery maxim—jam yesterday, jam to-morrow, but never to-day. Why has the governing machine failed? Partly because men are not scrupulous enough to possess this power over each other, and spend the money of others on their own pet projects; partly because the game of politics accustoms us to the use of crooked weapons; partly because compulsion destroys competition » and disfavours difference—‘ Progress is difference,’ said Spencer, condensing a whole philosophy of life into that short sentence, and packing enough moral dynamite into it to upset a good many comfortable armchairs—and partly because the human race, keen to get its business done for it on such easy terms, and entirely forgetting the narrow limits of brain-power in these days of accumulated knowledge, has piled such a monstrous amount of work on the governing machines. The consequence is that Governments, overpowered by details and lost in a flood of useless paper-work, cannot control their own work; and the people cannot control their Governments, or even understand what is done in their name. The vastness, the multifarious character, the ever-extending range of what is undertaken, render ignorance compulsory on all of us, and we all, representatives and represented, go stumbling and blundering on together, attempting to do the impossible. Just as it is with the big central machine, so it is with the smaller local machines. The same ambition to undertake everything and to play the part of earthly Providence, to be all-wise and all-directing ; the same strife between parties, with the same handing over of the minds, the bodies, and the property of all to the victorious section—are producing the same results. What a chronicle of ex- travagance and corruption has met our eyes in many cities of other countries! what violent partisanship in the Paris and Vienna of the present hour! what organised illegality in New York! what desperate remedies in the suspensions of the right to govern themselves in the cities of America ! What is the remedy? Let our municipal bodies develop a voluntaryist side to their work. Instead of always compelling, let them sometimes persuade us to help them in some of their many duties. In this very matter let them appeal to us to TRANSACTIONS OF SECTION F. 845 form building companies, with shares placed at a low amount, so that all may join. We cannot go on for ever slipping and sliding against our will into Socialism; we must learn to meet great wants in better fashion—the fashion of men who are not compelled. Then the new wants of civilisation will prove to be our best educa- tors—developing energy and friendliness, and the power to work together. So long as we satisty every new want by the easy and idle methods of compulsion, we learn nothing, for compulsion leaves all faculties undeveloped and only deepens the causes of strife. 3. Recent Changes affecting the Legal and Financial Position of Local Authorities in England. By F, W. Hirst, B.A. Changes in our Local Government Law may be produced in four distinct ways :—- 1. By Act of Parliament, private or public. 2. By decisions of the Courts, z.e. changes of interpretation. 3. By orders and regulations, 4, By bye-laws. With regard to the third heading it may be pointed out that there are draw- backs as well as advantages in connection with the central control exercised by departments like the Local Government Board, Home Office, and Board of Trade over the Local Authorities. The system of auditors is a good example of a form of administrative control which is wholly advantageous. But other forms of control involve administrative law, and both Parliament and the Courts are justly jealous of interference by bureaucratic boards which sit in London with the tree play of representative local councils. In the case of Kreese v. Johnson, the late ord Chief Justice held that Justices should be slow to invalidate a bye-law made by a local representative body. On the other hand the Private Street Works Act of 1892 substitutes Magistrates for the Local Government Board in appeals against apportionment. Perhaps the development of Local Government by judicial decisions has been most marked of late years in the spheres of rating and drainage law. In the first, the recent case of Cartwright v. Sculeoates Union deserves particular attention. It follows, I think, from the important decision of the House of Lords in that case that the rent of a tied public-house is legally worthless as evidence of its rateable value, and that evidence of the business actually done on the premises not only may be, but ought, in such cases, to be obtained. As regards public bill legislation there is no more interesting study than the rules by which Parliamentary Committees are, or ought to be, guided in dealing | with applications for borough extension. This is a subject well understood and practised by Bradford, which is also a pioneer municipality in consolidating rating areas and placing the levying and collection of rates under the control of the Urban Authority—a reform much to be desired in the interests of good govern- ment and public economy. Another kindred subject is the extension of municipal industry by Private Acts. Lastly,it may be well to pass in review some of the more important measures which have been placed on the Statute-book during the last ten years, including, besides those already mentioned, the Light Railways Act of 1897, the Highways and Locomotives Amendment Act of 1898, the Isolation Hospitals Act of 1893, the Parish Councils Act of 1894, the Agricul- tural Rates Act of 1896, and the London Government Act of 1899. 4. The Local Incidence of Disease in Bradford : a Comparison between the Rates and Causes of Mortality in Bradford and those of England generally. By A. Rapaeuiati, ID. _ The period dealt with is from 1874, when a Medical Officer of Health was ap- pointed in Bradford, to 1895, The woollen industry as a whole not unhealthy, al- 846 REPORT—1900. though, in some details, as ‘gassing’ and the large amount of moisture present in the air in some of the dyeing processes, it might be improved. The birth-rate in Bradford exceedingly low. This largely accounts for’a low death-rate and a low zymotic death-rate. The Bradford marriage-rate exceedingly low, and yet infant mortality very high; an unsatisfactory combination. Connection between the state of trade and the marriage-rate. Why the zymotic death-rate has not diminished in the last ten years. Has any part of the causes of zymotic disease been over- looked? Why has influenza come apparently to stay? Increase in cancer. Diminution in consumption. Comparison of mortality in Bradford from con- vulsions, diarrhcea, and the respiratory diseases, with that of England generally. General conclusions. TUESDAY, SEPTEMBER 11. The following Papers were read :— 1. American Currency Difficulties in the Eighteenth Century. By W. Cunnineuam, D.D. To many Englishmen it is a matter of surprise that currency questions should be such prominent political issues in the United States at the present time, and it is instructive to remember that debates about the circulating medium were as common there in the eighteenth century as they are to-day. There has always been, as it seems, a considerable body of colonists or citizens who have believed that existing monetary conditions had been devised in the interest of some par- ticular class, and that it was right and fair to manipulate the currency so that it should be more favourable to the interests of their own class or district. These efforts have generally resulted in depreciation of some kind. 1. The American Colonies in the seventeenth and eighteenth centuries had practically no coinage of their own, and there was great difficulty in maintaining the right standard of weight among the Spanish coins which formed the ordinary currency. The clipping and sweating of the coin was very common, and was even connived at by the authorities. In 1782, when Congress obtained a loan from France, it seemed absurd to let the heavy coins get into circulation, and Mr. Timothy Pickering was ordered, much against his will, to get ‘a pair of good shears, a couple of punches, and a Jeaden anvil’ for the work. If he had difficulty in the business he was referred to the Paymaster-General of the Forces, who was supposed to know all about it. 2. There have of course been various examples of the depreciation of the currency by the oyer-issue of paper in Massachusetts in 1740, in 1779, when a suit of clothes cost $2,000 in Continevtal paper, and in 1786, when attempts to circulate the bills of Massachusetts, Rhode Island, and New Jersey gave rise to much trouble. 3. There were few facilities for mining in America, and the issue of debased coin was impracticable; but the separate colonies, both on the mainland and the islands, had recourse to the expedient of raising the rating at which the coins in circulation should be accepted, so as to give each piece of money a greater nominal value, and temporarily at least a greater purchasing power. This can apparently be practised with success in a country where business is practically done by barter, or with commodity money, or where prices are the subject of authoritative assess- ment, All these conditions were largely present in the colonies in the seventeenth and eighteenth centuries. The object of a colony in enhancing the coinage and thus lowering all prices, was to attract silver from its neighbours, so that there might be more currency within its own area, and some relief from the inconyeni- ences of barter. In 1698 Pieces of Eight were suddenly raised in Pennsylvania from six shillings to pass for seven shillings and eightpence. This involved a loss of nearly 30 per cent. on the tobacco duty when the cost of collection was defrayed. The variations were frequent and considerable, and were said to be due to ‘the contrivance of some designing men in those countries who engross it when at the TRANSACTIONS OF SECTION F. 847 lowest, and so make merchandise of it and export it into foreign parts,’ At all events it gave rise to a sort of currency war between the colonies, each trying to draw away the circulating medium from others to itself. Thus about 1740 Virginia was attracting money from Maryland, and in 1798 the West Indian Islands set about establishing what Mr. Chalmers calls‘ retaliatory ratings ’ against each other on a considerable scale. It would be interesting to follow out the probable resuits of this method of manipulating the currency; immediately they would he precisely opposite to the consequences of debasing the issues from the mint. Debasing the coinage means a rise of prices; enhancing the coin is a lowering of prices all round; it does not increase the quantity of money in circulation; and while debasing the currency renders the exchanges unfavourable, the object of enhancing the coin is to attract bullion to the country. In so far as quantities of bullion were secured, there would of course be subsequent readjustments, but the immediate results would be very different from those of debasing the currency, except in one particular. Both methods of manipulating the currency would mean that creditors must accept smaller quantities of silver in satisfaction for existing debts. This last does not appear to have been the motive of the Governments at the time; they seem to have been actuated by a reasonable desire to attract currency or prevent a drain of coinage, and to have pursued their aim by a method of very questionable honesty, but well calculated, under the circumstances, to attain the wished-for result. The conditions under which ‘enhancing the coinage’ can be successfully practised so as to influence internal prices are unlikely to recur in the business communities of the world; and there is little motive to have recourse to it, since it yields no immediate gain to a Government; but there is at least a scientific interest in noting how this method of manipulating the currency worked in a state of business relations with which many of us are unfamiliar, 2. Some Heconomic Consequences of the South African War. By L. L. Price. There is a tendency to attach an unreal importance to divisions of time like those parting one century from another; but the end of the nineteenth century is accompanied by a series of remarkable events. At the beginning of the century England was engaged in the Great War with Napoleon, which, in addition to direct influence on the finances of the country, postponed the progress of fiscal reform, caused the suspension of cash payments, assisted the alarming growth of pauperism, aggravated the evils of the early Factory System, and was followed by prolonged depression. The South African War, with which we have been occu- pied at the close of the century, is not, so far as its direct financial consequences are concerned, an economic event of the same magnitude. War is indeed more costly now, but the duration of the war with the Boers will bear no comparison with the twenty years of the Napoleonic contest. It may occasion a considerable permanent increase in military expenditure ; but the sums involved in the two cases, taken absolutely, are very different, and, measured by the material resources of the nation, the earlier figure was enormous, while the later is trifling. The increased military expenditure may be accounted, on a strict interpretation of the term, ‘unproductive,’ and the growing pressure of foreign competition in our own manu- factures and trade, coupled with the increasing cost of obtaining the coal which is still the source of much motive power, and the large additions made to local and municipal indebtedness, may render it desirable to husband resources and avoid augmentation of the National Debt. ‘The Transvaal, however, will bear part of the direct expenditure of the war, and, even when the indirect burden is brought into the account, the total weight may be described as inappreciable, contrasted with the strain imposed by the Great War. But some of the possible economic effects of the later contest deserve attention; for it has been a disturbing factor, which may supply the force needed to move the currents of action from a groove in which they had settled. Passing by some obvious immediate consequences to the labour market and to trade, three points demand especial notice. (1) In the first place, the influence of an increased output from the mines of 848 REPORT—1900. the Rand should be seen in a rise of gold prices. This is difficult to bring to quantitative measure, and prediction may prove deceptive. Sir Robert Giffen foretold, in 1894, that the fall of gold prices was ended; but in 1897 he confessed that his expectations were not yet realised. By the present time, however, the evidence of index-numbers, such as that of Mr. Sauerbeck, seems to show a rise beyond any movement due to credit, in spite of the temporary cessation of supplies from the ‘I'ransyaal. But past experience enjoins caution in any estimate. The percentage of increase in the output is at present much less than it was at the Australian and Californian discoveries in the middle of the century. Predictions made at that time, even by a competent scientific observer like Jevons, were dis- appointed; and, although the ‘compensatory action’ of the bimetallic mint at Paris, which then acted as a ‘ parachute’ to break the fall in the value of gold, is now absent, yet the normal counteracting causes, such as the increased use of the metal in the currencies of the world (apart from any special new demands), the great growth of trade and industry, and the influence of credit, have become more powerful. A rise of gold prices may be expected; but it is impossible to fix the point which it will reach. Its consequences will be beneficial, and may assist in solving unsettled monetary questions. (2) The aid rendered by the colonies to the mother country in the war is likely, in the second place, to increase the momentum behind the conception of an Imperial Zollverein. There are special difficulties attending a Customs Union of the British Empire, arising from the separate situation of its component parts, which have not presented themselves in the case of Germany or the United States. These difficulties may, or may not, be eventually overcome; but some general con- siderations, apposite to the question, may be submitted to a scientific gathering like the British Association. Such a Customs Union, while it may conceivably result in an increase of internal free trade within the limits of the Empire, must, in all likelihood, involve some differential treatment of foreign goods. It must, so far, infringe the principles of Free Trade strictly interpreted. Recent theoretical discussion, especially of the incidence of taxation, has weakened some arguments for Free Trade, but the practical difficulty of limiting your action to what you really intend, and the great advantage of an attitude of neutrality on the part of Government in matters of trade, have not been diminished by recent experience. Yet an economic sacrifice may be incurred to secure a political end, or a temporary loss may be risked in the hope of an ultimate gain. The economist will urge that the step should be taken knowingly, and that its consequences should he seen and realised. On this ground the more obvious and open action of bounties is to be preferred to the obscure indirect influence of import duties. Lastly, the economist, while noting the crude fallaciousness of not a little reasoning, may admit the weight of some arguments employed against Free Trade. He may reach the con- clusion that the matter must be decided mainly on practical grounds, and that theory ends with opening men’s eyes to the results of their action. A non possumus attitude towards a Customs Union is no longer possible. (8) A third and last consequence of the South African War, which must be briefly noted, is its effect on Socialism. The unity of classes at home, which has resulted from common interest, is not favourable to class dissension. The increased military expenditure is calculated to prevent or delay the execution of costly social experiments, although Chancellors of the Exchequer, seeking to broaden the bases of revenue, may possibly, if improbably, give effect to some socialistic aspirations of mulcting ‘ unearned increments.’ Yet it may be a sound instinct which draws a distinction between socialism and militarism. Finally, it may be remarked that the consequences of the war thus noted are certainly not unimportant, if they may seem problematic. 3. Colonial Governments as Money-lenders. By Hon. W. P. REEvEs. For many years high rates of interest have been almost as much complained of by farmers and graziers in Australia and New Zealand as in the Western States of {TRANSACTIONS OF SECTION F. 849 America, Forty years ago 15 per cent. was commonly paid in the year in interest and commissions by this class of borrowers. By 1898 this had fallen to from 6 to 8} per cent., but the prices of produce had fallen in proportion. In the years 1894-96, the Governments of four colonies—New Zealand, South Australia, Western Australia, and Victoria—established monev-lending departments for making ad- vances on mortgage to the smaller class of farmers. In this way over 4,000,000/. has already beenlent out. Details are givenin the paper of 3,600,000/., of which about 2,200,0002. has been lent in New Zealand, 790,000/. in Victoria, 530,000/. in South Australia, and 100,000/. in Western Australia. About 450,000/. has already been repaid. The New Zealand Government raises its loan capital by issuing stock in London; the others by selling mortgage bonds from time to time locally. In Victoria, this capital has been obtained at 3 per cent. (from the State Savings Bank) ; in New Zealand it has cost 3; per cent., and in South Australia 34 per cent. The rates charged to farmers are in New Zealand 5 per cent.; in the Australian colonies 43 per cent. The fees charged by all the State lending offices are very low—lowest of all in South Australia, The management expenses, are, however, small also, and the lending would seem at present to have been done prudently, At any rate, balance-sheets to the end of June 1899 and March 1900 show no losses, while of arrears of interest there were none in New Zealand, and but a few hundreds in Australia. The lending is done by way of first mortgage on freehold, or on leasehold held from the Crown. The loans are devoted to improving settlers’ holdings, or to paying off existing mortgages bearing a higher rate of interest. In Western Australia they are restricted to the former purpose; else- where more than half the money is applied to the latter. The highest sum which may be lent to one borrower is 3,000/. The proportion of loan to security must not exceed 60 per cent. of a freehold, or half the selling value in case of a lease. An interesting feature is the system of repayment of loans by instalment. Under this the borrower pays 6 or 7 per cent. annually, of which 44 or 5 represents interest, and the remainder goes to form a sinking fund to extinguish the debt. In New Zealand every loan must thus be repaid by seventy-three half-yearly instalments. The mortgagee may, however, hasten the process by depositing additional sums or paying off the whole principal whenever he chooses. In 1899 the Government of New South Wales followed the example of the neighbour colonies and passed an Advances to Settlers Act. As an example of the effect of these Acts in reducing rates of interest, it may be remarked that in 1894 almost two-thirds of the money of registered mortgages in New Zealand bore from 6} per cent. upwards. In 1898 six-sevenths of the mort- gage money was yielding less than 64 per cent. 4, Variations of Wages in some Co-partnership Workshops, with some Comparisons with Non-Co-operative Industries. By Ropert HatstEap, Secretary of the Lancashire and Yorkshire Centre of the Labour Association. The difficulty of securing suitable data for the purpose of the paper was con- siderable, owing to the fact that the kind of information required was very local and very special. The officials of thirty-four co-operative productive societies furnished information respecting 4,012 co-operative workers with a total wage of 209,5210. for the year 1899. Fourteen societies sent replies, the total wages of which amounted for that year to 122,313/. The average increase of wages in these co-partnership workshops since 1891 was 9 per cent. Means for comparison with non-co-operative wages are available for 1899 only, which shows a result in favour of co-operation of 7 per cent. Co-operative workers also have two hours a week less than non-co-operative workers. The figures also reveal that a large number of co-partnership workers were connected with their own trade unions. Particulars were supplied by ten societies, in which 246 workers were concerned, and in which last year the total wages were 9,486/. These showed that the workers had wages in excess of non-co-operative ones in the same trade and district by 11 per cent., 1900. 31 850 REPORT—1900, and that they worled one and a half hour a week less, Moreover, the loyalty of these workers to trade unionism was shown by a high percentage of them being members of their own trade and district branches. Five co-partnership societies with a total number of workers of 501, and wages for 1899 of 23,557/., show an average increase in wages of 17 per cent. since 1891; but there is no means of comparing this with the wages of non-co-operative workers. With regard to the five remaining societies little more can be said than that they paid more than standard or trade union rate of wages in addition to a share of the profit, and that in some cases they worked fewer hours than non-co-operative concerns, The returns also show that in nineteen cases concerned there was an average increase of 11 per cent. from 1891 to 1899, and that in fourteen cases there was an average difference in favour of co-operative as against non-co-operative wages of 9 per cent. This result in favour of co-operation is argued to be due partly to the sources from which the facts are obtained, but mainly to the high relative efficiency of co- partnership industries. The causes of this efficiency are held to reside in the fact that co-partnership brings the workers to more points of contact with the profit- making aspect of an industry than ordinary forms of production. Workers in co-partnership concerns have a special incentive to obtain higher wages, because they share in profits in proportion to their wages, thus absorbing as much as possible of the results of the extra efficiency due to their special form of enterprise. The large proportion of the worker being trade unionist is held to increase in force, inducing co-partnership societies to take the lead in the matter of wages. 5. Labour Legislation for Women. By Marcaret E, MacDonato. Certain fundamental differences between men and women engaged in industry affect the question of legal regulation, (a) Physical differences, e.g., young mothers need special protection from un- healthy conditions. (6) Differences in economic position. Even those women who do not marry are influenced by the fact that marriage is an event which revolutionises the economic condition and the industrial outlook of the great majority of women. As the result, women have a lower standard of pay and work than men. In a large pro- portion of cases they only need their wages as pocket money, or at most only to keep themselves, and where they are the breadwinners of the family they are usually overburdened with household cares and unable to stand out for better con- ditions. They are comparatively unorganised, e.g., only 116,016 women are re- turned as members of trade unions, and of these 116,470 are in the textile trades. They are less ready to complain than men; ¢.g., in the Post Office women only get half, or less than half, as much pay as men for the same amount and quality of work ; yet the Tweedmouth Commission, while devoting great attention to the grievances of the men, made no recommendations with regard to women, naively explaining that ‘there is a general absence of complaint from them,’ The comparatively low standard of women’s work and pay has an injurious effect upon men’s labour wherever it comes into competition with it; e.g., the introduction of light machinery is constantly made the excuse for substituting women for men workers at lower rates. By setting a legal standard the State compensates to some extent for the lack of organisation and of a high standard amongst the women. We have experience of labour legislation for women in certain classes of em- ployment from 1842 onwards. By comparing the conditions of workers in these trades before and after regulation, and also comparing their conditions at the present time in regulated and unregulated trades, we find that in regulated trades: TRANSACTIONS OF SECTION F, 851 (1) Sanitary conditions have improved relatively. (2) Wages have risen relatively. (3) The number of women employed have increased relatively, (4) Organisation amongst the workers is more general. This study encourages the further extension of legal regulation. In discussing the details of fresh legislation the following points are to be considered :— (1) Classes of workers at present unregulated, or very partially regulated, e.g., home-workers, shop-assistants, laundry workers, clerks, &c.! (2) Matters for legislation—e.g., hours of work, sanitation, dangerous pro- cesses, wages. (3) Administration, central v. local authorities, women inspectors, (4) Codification of present law, accompanied by differentiation to meet special requirements of special trades. 6. The Treatment of the Tramp and the Loafer, By Witriam Harsurr Dawson. No time can be more fitting than the present for filling up an important gap in our penal system and for introducing a reform which became a logical and social necessity when the Poor Law was placed on its existing basis. The time has come for transferring the habitual vagrant and the loafer generally from the province of the Poor Law to that of the Penal Law. To the former they do not in any sense belong. The failure of centuries of reformers and legislatures to make the slightest impression upon the tramp population is largely due to the persistent mistake of treating his case as coming under the law of public charity. What society is bound to do, as far as possible, is to exterminate the social parasite of every kind. His existence is a positive injury to the State in every way. He robs the State not only of the industry which he owes it, but he consumes the produce of other people’s labour and renders it nugatory, abstracting from the wealth of society without adding to it. His example scandalises honest workers ; he is a standing menace to public peace and safety; and for society to tolerate him is not merely to condone injury done to itself, but absolutely to place a premium upon social treason of the most insidious and most vicious kind. Think what we do for the professional idlers!] Take the urban loafer. While honest men are working we give him the free run of our thoroughfares and set apart for him the best of our street corners. Should he be a vagrant loafer we make it possible for him to travel through England from the Tweed to the Channel with- out doing one hour's serious work, save for the labour tests which are imposed by some—and only some—of the workhouses at which he may call. Who should wonder that our past indulgent treatment of the vagrant has had the effect of eee tuating and multiplying this class of social parasite? The dictum of wise ir Matthew Hale is still irrefutably true: ‘A man that has been bred up in the trade of begging will never, unless compelled, fall to industry.’ But that is not the whole of the truth. Every one of these men creates imitators. On the highways he is a walking advertisement of the advantages of idleness, while in the model lodging-house, or wherever else the workhouse-shunning tramp seeks nightly shelter, he acts the part of recruiting sergeant for the great army of sloth and vice. What we should do, and shall have to do sooner or later, is to collect the tramps from the four winds of heaven and try to discipline the idleness out of their natures. For it is not, in the main at any rate, a dangerous criminal class with which we have here to do, but for the most part the weak and aimless characters whose great need is the moral tonic of discipline and compul- sion. No faith should be placed in any cobbling of the existing Poor Law. No doubt a good deal more could be done to discourage vagrancy if the separate cell system were made universal, and if taskwork were rationally imposed ; in a word, if the régime of the casual ward were made sufficiently rigorous to be deterrent, and - |! See Factory Inspector's Report, 1899, p. 254. 312 852 REPORT—1900. if such rigorous action were made uniform throughout the country ; and finally if magistrates more consistently enforced the laws against begging, sleeping out, and similar tramp offences. But this would only be a temporary makeshift, and the true remedy is to hand these parasites over to the Penal Law. In the first place, vagrancy and loafing generally should be made indictable offences. The right of free migration in the case of the destitute should be restricted to the extent of making it dependent on police permission to travel in search of work, after the principle of the police pedlar’s licence. But, further, the casual ward must be abolished. This might seem a strong measure, but it is really the fulerum on which the lever of reformation must rest. If loafing is to be regarded as an offence to be punished, instead of an innocent weakness to be humoured, the loafer’s free lodging-house must disappear. The casual ward is entirely incom- patible with the laws which already exist for the repression of vagrancy. It is illegal to beg ; it is illegal to wander about without means of subsistence; but there is no habitual vagrant living who is not guilty of this compound fracture of the law, and few who have not been punished for it. Nevertheless, we wink at these misdemeanours, and in housing 10,000 vagrants every night in the casual wards—which, of course, is but a fraction of the total highway population—we offer direct encouragement to known law-breakers to persist in breaking the law. It would, of course, be necessary to meet the case of genuine seekers of work, and we should meet it considerately and indulgently. They would be expected to legitimise themselves by means of a police or properly attested private certificate, asserting their dona fides and destination, and this labour passport should secure the free right of lodging and food on the way. For them housing might be found in proper quarters, the workhouse, or any decent house of call, or in night shelters such as exist in Germany and Switzerland. But the crucial point is, ‘ How to deal with the vagrants and loafers who do not abandon their idle ways and ‘seek work? After a first warning these should be detained—for a period sufficiently long for disciplinary purposes—in correctional institutions; the hardened cases in penitentiaries to be specially provided for in existing houses of correction whose régime should be modified to their needs, and the more hopeful ones in some form of labour colony which, besides receiving vagrants who hed passed under magisterial jurisdiction, should also, as in Germany, Holland, and Switzerland, offer a temporary home to work-seekers of all kinds. It might be said that that was to admit the principle of the right to work. Even if that were so, the right to work is an infinitely better and wiser and safer principle to concede to the masses than the right to be idle. Early English laws really proposed in a crude fashion this very treatment of habitual vagrants and idlers, and Germany and Switzerland—the one aconservative and the other a democratic country—are treating the problem on these lines. WEDNESDAY, SEPTEMBER 12. The following Papers were read :-— 1. The Relation between Spinners and Piecers in the Cotton Industry, By 8. J. Cuapmay, ILA. When spinning first became a separate industry for men at the beginning of this eentury the spinners successfully enforced apprenticeship rules ; and even after the ‘mules’ and ‘jennies’ became longer, cartying more spindles—especially after power was used for driving the carriage backwards and forwards—and when con- sequently more piecers were required on some ‘ wheels,’ the old apprenticeship rules were still enforced, and a distinction was drawn between those piecers who were ‘learners’ and those who were not. When, however, it became the rule to have on each machine piecers who were not learners, and when, moreover, im- Proved machinery was rendering the learning of spinning an easy task, the distinc- TRANSACTIONS OF SECTION F, 853 tion between piecers and ‘learners’ broke down, and the apprenticeship rules could no longer be maintained. Then the spinners adopted a new policy. They merely insisted on their existing large share of the total wage paid on the ‘mules,’ op- posed all increases in piecers’ wages, which they knew would be at their expense, and limited the quantity of machinery to each spinner. The result is that there are to-day from two to three times as many piecers as spinners, and that a great number of the former have been for years as fully qualified as the latter, though they receive at most only about half a spinner’s wage. Both masters and piecers have attempted to do away with this arrangement, which is by no means economical, and which benefits only existing spinners at the expense of the piecers and all future workers in the industry. But the opposition of the piecers is weak because they are badly paid, and are ever hoping to become soon highly paid spinners or something else; and, on the whole, the men have been successful in resisting the masters’ attempts to introduce the ‘joining,’ ‘ dofling,’ and ‘ appren- ticeship ’ systems, and the ‘ coupling of wheels’ (double- and treble-decking), which were all directed against the existing arrangement of hands on the ‘ mules,’ 2. Indian Guaranteed Railways ; an Illustration of Laisser Faire Theory and Practice. By Eruen R. Farapay, M.A. The dogmatic rigidity of the laisser faire school, and their refusal to recognise the principle of development in economics, have produced the characteristic weak- nesses of their policy, its carelessness of detail, its sacrifice of actual to nominal freedom, its neglect to provide for future possibilities, and its attempt to apply the same reasoning to different circumstances; all cf which are illustrated in the later history of the Indian guaranteed railways. The guarantee system, in origin a purely practical expedient, had outlived its utility before it was revived by the English Government of 1868-74, apparently as being preferable, from the daisser faire point of view, to the direct State ownership which was considered by Lord Lawrence, as by Roscher, advisable in India. In the contracts renewed with three railways—the Great Indian Peninsula, Bombay, Baroda, and Central India, and Madras lines—it was agreed that the companies should receive interest at the guaranteed rate of 5 per cent. and half the surplus profits, no account being taken of deficits ; that remittances to England should be converted at the rate of 1s. 10d. the rupee; and that calculations should be made on a half-yearly basis. The result was that the Indian Government bore all the loss of the unprofitable half- years and, after 1875, never received its full share of gain in the profitable ones, since, as the exchange value of the rupee fell below Is. 10d., the shareholders received a gradually increasing proportion of the surplus profits, while the contract obligation to pay interest at 5 per cent. deprived the State of advantage from cheaper money and improved credit, which would lately have enabled it to raise money at 23 or 3 per cent. to pay off loans advanced at a higher rate of interest. On the three lines in question, taken together, the average proportion of earnings yearly remitted to England, 1892-7, was 99°70 per cent., and the net annual Joss to Government amounted to 13,000,000Rs., a tax imposed on the Indian public, for the benefit of the British shareholder, by that Jaisser faire school which objects to State railways as taxing one part of the community for the benefit of the other. Statistics showing the working expenses of railways formerly guaranteed, before and after their acquisition by the State, indicate that the guarantee system was uneconomical ; but the fault is less with the companies than with the Jaisser faire English Government, which gave them the material advantages of liberty, and freed them from its responsibilities. 3. Price-changes in the Foreign Trade of France. By Professor A. W. Fiux, IZA. Some twenty years ago, M. de Foville traced the variations of price-level in French trade by using for the years 1827 and 1847 to 1862 the values of the 854 REPORT—1900. trade of each year as ascertained and comparing it with the Official Value, which expressed its value at the prices fixed for the year 1827. From 1862 onwards these Official Values are not recorded, but in each year the trade is first valued at the prices of the preceding year, and, later, a revised valuation, at the prices of the year itself, is supplied. Thus the price-movements were traced from 1847 to 1878.1 he paper continues the latter series of comparisons to 1898. Taking the price- level of 1862 as 100, the lowest level subsequently reached was in 1897, when imports reached 57°2 and exports 57°6. In 1898, neglecting fractions, the level of price for both imports and exports was 58, In the interval the fall of price- level for exports was almost unbroken, the elevations of 1864, 1872, 1880, and 1890 being comparatively slight. In the case of imports there was a considerable and sharp rise from 1869 to 1872, after which the course of the movement has been similar to that of exports, but so much more rapid has been the decline as to bring the figures for both sections of trade to approximately the same level in the last few years. The piecing together of a record of price-movement before and after 1862 as ascertained by two different methods gives interest to the comparison of the measures of the movement from 1887 to 1896 by each of these two methods. ‘The Tableau Décennal for 1887 to 1896 supplies a valuation of the trade of each year at 1896 prices. The two measures of price-movement give substantially the same results except in the years most removed from the year with which comparison is made. The fall of price is greater for exports, less for imports, from 1887 to 1896 as measured by direct evaluation of the trade of each year at the prices of 1896 than as measured by the index of price-movement previously obtained. The greatest difference shown falls short of 3 per cent. It is possible that, just as a divergence between the course of price-movement of imports and exports up to 1872 did not prevent the substantial identity of price-change in both over the period 1862 to 1898, so the divergence shown over a ten-year period, in the two measures of price-movement, is no proof that, could the same method have been used for tracing price-change from 1827 to 1898, instead of two methods linked together at the date of passing from one to the other, the indication of change of price-level over the whole period would have differed substantially from that actually obtained. It is interesting to note that the difference of price-level in the early sixties and the late nineties as shown by Sauerbeck'’s Index Number is not far from the same as that ascertained by the methods used in the paper for French foreign trade. 1 Cf. Journal of the Royal Statistical Society, December 1879. TRANSACTIONS OF SECTION G, " §6a Section G.—_MECHANICAL SCIENCE. PRESIDENT OF THE SEcTION—Sir ALEXANDER Binnie, M.Inst.C.E., F.G.S. THURSDAY, SEPTEMBER 6. The President delivered the following Address :— Looxine back at the Addresses of my many distinguished predecessors in this chair, I find that, devoting their attention as they have done either to the general progress of engineering knowledge or to those particular parts of it that have engaged their personal study, the possible field of observation has become some- what circumscribed. Every one, I think, must by this time be fairly well acquainted with the progress made in our.work during the present century or during the reign of Her Majesty the Queen. But although this detailed examination of progressive advancement may appear at first sight to be exhausted, yet it may be not altogether unprofitable if we endeavour for a few minutes to consider how, and under what circumstances, that advancement has alone become possible. Living as we do at the end of the nineteenth century, and surrounded as we have all of us been from our earliest years with a march of progress unequalled in the world’s annals, we are apt to assume that the circumstances which surround us, the general attitude of the scientific mind, and our conception of nature and its phenomena, are things which come to us by nature as our birthright, forgetting that they are the result of thousands of years of work and thought among some of the greatest minds that the world has ever produced. It may not therefore be displeasing to the audience which I see before me if in an imperfect way I attempt to lay before them some, at all events, of the salient facts which lead up to our present outlook on the scientific matters with which our profession deals, We as civil engineers define our profession as being ‘the art of directing the great sources of power in nature for the use and convenience of man.’ Conse- quently our success or otherwise will depend on the estimate we may form of nature as a whole, and of those great sources of power which it places at our disposal. Undoubtedly in the history of the world there has never been a period when the study of nature has been so open and free from all prejudices of any kind whatever as it has been during the present century; nor, perhaps, with but few exceptions, has there ever been in any age or country atime when nature and her laws have been investigated with so pure and steadfast an aim after actual truth without the mind being prejudiced by authority or preconceived ideas derived from those great departments of human thought which deal more particularly with matters of faith, morals, and religion. _ This equanimity of mind in which we now approach all subjects relating to science has not, J need hardly say, been the case in the past. Some persons may 856 REPORT—1900. ascribe it entirely to the inductive method introduced by Bacon, as opposed to the too exclusive confinement of the mind to the deductive systems of the older scholastic philosophy which preceded his time, and to which in a large measure he was undoubtedly instrumental in giving the death-blow. This view, however, is not altogether correct, for in the teaching of Socrates and Aristotle we find continued reference to the impor ance of inquiry, observation, and induction. And in the cases of Hipparchus and Ptolemy in the best days of the Alexandrian school of astronomy we find the most laborious observations carried on for hundreds of years under circumstances and with instruments which we should now consider totally inadequate; and by their means discoveries were then made with an accuracy which surprises us; and from these discoveries conclusions were drawn which for more than a thousand years stood the test and satisfied the requirements of some of the most acute thinkers of the world. We should, I think, in the first instance inquire how it came about that the great mental energies of philosophers of-the ancient world failed to produce that fruit which we in later ages are gathering in such rich abundance. To arrive at some idea on this question we must endeavour to picture to our- selves the inner consciousness of the great minds of antiquity when they first began to contemplate the circumstances by which they were surrounded, and were called upon by that inexorable and mysterious longing of the human mind to answer those great questions of the whence and the whither which are so strangely rooted in the hearts of all deep-thinking people. To them were presented for the first time those great phenomena of nature by which we are always surrounded, many of these being of a character at once to charm and at other times to terrify the beholder, And in what I may call the childhood of the human mind, they, like children of a later age, were prone to ascribe to what they saw around them qualities and properties to which the phenomena in themselves had no relation. What I may call the nascent deductive principle, so strong in all our minds, had given to it by these ancient philosophers the free play of fancy and imagina- tion which led them to conclusions based on their own ideas and not upon the facts of unerring nature. Consequently we see in the early age of Greek thought the natural laws of the universe in smiling morn or darkening night, in raging sea or the thunderbolts of heaven, ascribed to the immediate action of benevolent or malevolent powers in the celestial world; and as a consequence the Greek mind from its earliest period became saturated with the beautiful conceptions of her poets, and following from this when philosophy first approached the subject, theories were broached and conclusions were adopted, many of them on an utterly erroneous basis. Steeped as the Greek mind was in its lovely ideals of nature, it is not sur- prising to find that, when their philosophers began to formulate their theories, these deductions took the place of fact; and celestial observations, when they made them, as they undoubtedly did, were used, not for the purpose of illustrating the laws of nature as we interpret them, but as a means, partly religious and partly philosophical, in support of their preconceived ideas of the universe, the foundations of which, having been laid in poetry, became crystallised in the wonderful con- ceptions of the great men who directed their country’s mind. In looking, therefore, at nature in the earlier ages of scientific thought, we find that the standpoint from which everything was viewed was narrowed down to a universe constructed for man alone, the powers of which were governed by the caprice and whim of the great gods of Olympus, and yet even in this period- we notice true opinions arising with regard to the structure of the universe. For instance, Pythagoras—and Aristarchus—conceived the idea that the sun was the centre of the universe, and that the planets revolved around him. _ This correct deduction was to a large extent vitiated by bringing it into rela- tion with another conception, that of harmonics. Hence we find the true ideas of Pythagoras mixed up, and in a sense confused, by this theory of the harmony of the spheres. And even when at a later period, more accurate observation gave the ancients TRANSACTIONS OF SECTION G. 857 still better data on which to reason, they yet continued to ascribe, as the very names of the planets indicate, connections between them and the gods. The outcome, however, of the teaching of the Greek schools, culminating as it did in the splendid work of the Alexandrian philosophers, resulted in the mistaken formula that the earth was the centre around which all the phenomena of nature were carried on. It must not be imagined for one moment that Hipparchus and Ptolemy were not acute and accurate observers. They at an early period detected some of those inequalities in the moon’s motion which require all the force of the gravitation theory to explain. They defined, by patient observation, the irregular motions of the planets, sometimes progressing, sometimes retrograding, and with wonderful accuracy they were able to measure the precession of the equinoxes which carries the equinoctial points backwards along the line of the ecliptic. They had a very clear conception of the rotundity of the earth, as we know from the fact that they made attempts to measure an arc of meridian. All this wonderful mass of observation and discovery, when taking into con- sideration the imperfect means at their dispcsal, will ever remain throughout all ages one of the greatest monuments to perpetuate the fame of the men who pro- uced it. The question at once arises, How was it that with their wonderfully accurate observations and their perfect knowledge of the movements of the heavenly bodies they did not arrive at some of those revelations which later ages have brought to light ? It is difficult to answer this question with any degree of precision, but one can see clearly that their minds were governed, and the results of their inductions vitiated, by conceptions such as those of which I have above spoken. These conceptions were that, seeing that the sun, moon, and planets appeared to revolve around the earth and return at different. periods into closed orbits, therefore, as a circle was the most perfect of all figures, they must necessarily revolve in circular orbits, and that as celestial bodies this motion must be uniform Consequently, to unite together the accurate observations that they had made of all the varying motions of the heavenly bodies, they had to invent circular orbits and smaller orbits carried by these in which the sun and planets revolved, and so gradually built up that wonderful and complex system, to which the name of Ptolemy is always attached, of cycles, epicycles, and deferents, by which in a most complicated manner they were able at length to reconcile their accurate observations with their preconceived idea of circular motion. The Ptolemaic system will always remain a wonderful monument to the skill of the observers and the acuteness of the thinkers in the ancient world. Turning now to the domain of mechanics, with which were intimately bound up their ideas of geometry, we find, as our old friend Euclid has long since taught us, not only that they were among the most acute reasoners, but that they possessed logic, which, when applied to such conceptions as these, has remained after 2,000 years the text-book in our schools. But in their estimate of the uses of geometry and the functions of the conic sections, the philosophers cf old regarded them mainly as a species of intellectual athletics by which the mind was trained and perfected, and they believéd that it was degradation to apply that knowledge to the affairs of mundane life. In the case of Archimedes we see the master-mind grappling for the first time with some of the great problems of mass and of force, and solving to a large exten some of the principal problems placed before him. But here also Greek notions of mass and of force were mixed up with others, which ascribe to them properties perfectly ideal, and it was considered, in the words of our great poet, that the application of these wonderful discoveries to the affairs of life was ‘ base mechanical.’ No doubt much of this was due to the fact that the teachings of the old Greeks were held to be exclusively the property of certain schools and academies, and that 858 REPORT—1900. the culture of the mind was the object in view. On the other hand, all the affairs of life connected with the mechanical arts were confined for the most part to a large section of the people who were held in slavery, and who, with but few exceptions, never rose to intellectual pursuits. But, above all, as their ideas crystallixed into the form of concrete theories nearly allied to many supernatural conceptions, these were gradually absorbed by the priesthood and mingled with the national faith, to differ from which, as in the case of Socrates, meant recantation or death. Reviewing, therefore, the above impressions of the ancient world, we find the most accurate observations combined with the most fanciful theories, worked out with a logical and a mathematical skill which all the world admires, yet vitiated by conceptions or theories based on fanciful resemblances, and the whole gradually consolidated by priestcraft into a mass of superstitious dogma, to differ from which was to incur the odium of heresy. We shall see as we proceed that this palsy of the mind was again repeated after a lapse of 1,500 years. But even in the century which immediately preceded our era, we have indica- tions that there were clear theories which had they been followed out to the full might have led to an earlier gathering in of the fruits of science. At this point I may perhaps be permitted to read a few passages from the great Latin poet Lucretius, who in his sweet Pyrrhean verses attempts to lay before his beloved Memmius, the Roman soldier, the learning of tle Greeks. T shall use Munro’s translation. The entire six books are taken up by an attempt on the part of Lucretius to explain to Memmius the whole realm of nature, starting from the atomic stand- point of Democritus and Epicurus. I should explain that in the following passages Lucretius calls the atoms the first-beginnings of things. This poem was written in the first century before our era, and gives a good idea of the attitude of the Roman mind in its admiration of Greek philosophy, while at the same time attacking the gross superstition of the priests. ‘ When human life to view lay foully prostrate upon earth crushed down under the weight of religion, who showed her head from the quarters of heaven with hideous aspect lowering upon mortals, a man of Greece ventured first to lift up his mortal eyes to her face and first to withstand her to her face. Him neither story of gods nor thunderbolts nor heaven with threatening roar could quell: they only chafed the more the eager courage of his soul, filling him with desire to be the first to burst the fast bars of nature’s portals. Therefore the living force of his soul gained the day: on he passed far beyond the flaming walls of the world and traversed throughout in mind and spirit the immeasurable universe; whence he returns a conqueror to tell us what can, what cannot come into being; in short on what principle each thing has its powers defined, its deep-set boundary mark. Therefore religion is put under foot and trampled upon in turn; us his victory brings level with heaven.’ } ‘This terror then and darkness of mind must be dispelled not by the rays of the sun and glittering shafts of day, but by the aspect and the law of nature ; the warp of whose design we shall begin with this first principle, nothing is ever gotten out of nothing by divine power.’ * ‘We must admit therefore that nothing can come from nothing, since things require seed before they can severally be born and be brought out into the buxom fields of air.’$ ‘ Moreover nature dissolves everything back into its first bodies and does not annihilate things.’ * ‘And yet all things are not on all sides jammed together and kept in by body: there is also void in things.® ‘Time also exists not by itself, but simply from the things which happen the sense apprehends what has been done in time past, as well as what is present and } Book I, p, 2, 2 Tbid, p, 4. 3 Ibid. p. 5 4 Thid. p, 6, 5 Thid, p, 8 TRANSACTIONS OF SECTION G. 859 what is to follow after. And we must admit that no one feels time by itself abstracted from the motion and calm rest of things.’ ! Lucretius, speaking as in the following lines of atoms as the first-beginnings, appears to have the conception, not only of atoms, but also of molecules; for instance :— ‘Bodies again are partly first-beginnings of things, partly those which are formed of a union of first-beginnings.’ * ‘ But since I have proved above that nothing can be produced from nothing, and that what is begotten cannot be recalled to nothing, first-beginnings must be of an imperishable body, into which all things can be dissolved at their last hour, that there may be a supply of matter for the reproduction of things.’ ® From the following quotations it will be seen that Lucretius had a very good idea of the struggle for existence and the survival of the fittest. ‘That also which before was from the earth passes back into the earth, and that which was sent from the borders of ether is carried back and taken in again by the quarters of heaven.’ 4 ‘ Thus one thing will never cease to rise out of another, and life is granted to none in fee-simple, to all in usufruct,’ ° ‘ And many races of living things must then have died out and been unable to beget and continue their breed. For in the case of all things which you see breathing the breath of life, either craft or courage or else speed has from the beginning of its existence protected and preserved each particular race. And there are many things which, recommended to us by their useful services, continue to exist consigned to our protection. In the first place the fierce breed of lions and the savage races their courage has protected, foxes their craft, and stags their proneness to flight. But light-sleeping dogs with faithful heart in breast and every kind which is born of the seed of beasts of burden, and at the same time the woolly flocks and the horned herds, are all consigned, Memmius, to the protection of man. For they have ever fled with eagerness from wild beasts, and have ensued peace and plenty of food obtained without their own labour, as we give it in requital of their useful services. But those to whom Nature has granted none of these qualities, so that they could neither live by their own means nor perform for us any useful service in return for which we should suffer their kind to feed and be safe under our protection, those, you are to know, would lie exposed as a prey and booty of others, hampered all in their own death-bringing shackles, until ature brought that kind to utter destruction.’ ® I must conclude my quotations from Lucretius with his splendid exordium to Memmius in the second book. ‘Apply now, we entreat, your mind to true reason. For a new question struggles earnestly to gain your ears, a new aspect of things to display itself. But there is nothing so easy as not to be at first more difficult to believe than afterwards ; and nothing too so great, so marvellous, that all do not gradually abate their admiration of it. Look up at the bright and unsullied hue of heaven and the stars which it holds within it, wandering all about, and the moon and the sun’s light of dazzling brilliancy: if all these things were now for the first time, if I say they were now suddenly presented to mortals beyond all expectation, what could have been named that would be more marvellous than these things, or that nations beforehand would less venture to believe could be? nothing, methinks: so wondrous strange had heen tnis sight. Yet how little, you know, wearied as all are to satiety with seeing, any one now cares to look up into heaven’s glittering quarters! Cease therefore to be dismayed by the mere novelty and so to reject reason from your mind with loathing: weigh the questions rather with keen judgment, and if they seem to you to be true, surrender, or if they are a falsehood, gird yourself to the encounter. For since the sum of space is unlimited outside beyond these walls of the world, the mind seeks to apprehend what there is yonder there, to which the spirit ever yearns to look forward, and to which the mind’s immission reaches in free and unembarrassed flight,’ 7 > Book I., p. 11. 2 Thid. p. 12. 8 Ibid. p. 13. * Book IL., p. 52. > Book III., p. 80, * Book V., p, 136, 7 Book IL, pp. 52, 6%, 860 ; - REPORT—1900. In the early centuries of our era, however, a great change was coming over the human mind. We have seen from the above quotations that, even before the advent of Christianity, thinking men were beginning to revolt against the super- stition of the old mythology. Soon after there arose the Neoplatonic school at Alexandria, which mixed up, in a way difficult to describe, beautiful conceptions of moral and religious training through astronomy and the sciences in an inexplicable tangle of pseudo- Greek philosophy. At the same time there was gradually stealing over the minds of men an entirely new feeling, born of a new faith, which taught that things earthly and appertaining to the earth were of slight importance, and that all the splendid learning of the Greeks was but vain philosophy, and that the thoughts of man must be directed, not to the present, but to the future. Among these conflicting ideas, there was intruded the outer barbaric power which knew nothing of science or of philosophy, but which, by its virile force and austere tenacity of moral worth, overran and conquered the Roman Empire. These untutored peoples were soon attracted by the beautiful simplicity of the new religion, and were gradually absorbed into the Christian Church. In the year A.D. 640 a serious blow was struck to advancing science, and for a thousand years we are parted from all the learning of the ancient world by the destruction of the Alexandrian Library by the Saracens. Then followed for nearly a thousand years that period of intellectual torpor which we generally denominate ‘the dark ages.” To a large extent natural science became unknown, the astronomy of the Greeks degenerated into astrology, and when occasional thinkers did inquire into nature’s secrets, it took the form of alchemy, and a desire to discover the philosopher’s stone, and the transmutation of metals. Mixed up with these were also a school of magicians, individuals who revelled in mysteries—always an indication of ignorant superstition. During this period the ideas of the universe were taught from the books of Moses; even the learned lost all conception of the rotundity of the earth, and indeed we have treatises written to prove that we live on a flat world. Of course, during the period I am speaking of there were some minds, in isolated cases, which still believed in the teaching of the Ptolemaic system. But the overruling authority of the Church crushed out all inquiry into the nature of things, deeming it sufficient that men should either remain ignorant, or devote their attention to a future existence. At length, however, after the conquest of Constantinople, in 1453, there came a period when the literature of the ancient world again claimed attention, and the logic of Aristotle became the dominant factor in the teaching of the Church. 7 Another element was also contributing to the revival of the human in- tellect. The Saracens, after their conquest of Alexandria, had preserved in the univer- sities of Bagdad and Damascus much of the learning of the philosophers of the ancient world. This in the course of time followed their conquests along the northern coast of Africa, and was gradually grafted into the European mind by the teaching of the doctrines of the school at Salamanca; and it is to this channel, strange to say, that we are indebted for what we know of the tenets of Hippar- chus and Ptolemy, as well as to many of the alchemistic sciences which they them- selves assiduously cultivated. Thus gradually we see dawning upon the benighted minds of the middle ages a revival of the learning of the ancient world. The invention of printing and the lessons of the Reformation at once threw open the whole question to independent thought, and at the same time afforded a means of free interchange of opinions throughout the whole world. About this same time the vexed question of the earth’s rotundity was for ever set at rest by the discoveries of Columbus in 1492, and the circumnavigation of the globe in 1522. I now approach a period when it becomes necessary to show, with somewhat, more exactitude than that with which I have hitherto treated the subject, how TRANSACTIONS OF SECTION G. 861 gradually there grew up in the minds of men those modern truths to which I have alluded in the opening passages of my remarks, To attempt to do justice to this theme in the few minutes at my disposal would be indeed a vain endeavour ; but for the purpose of showing the lines along which they ran, and to enable you to carry away with you the sequence of events to which I am about to allude, I have prepared a chronological chart. This chart extends from the time of Edward VL, in 1550, to the present year. Horizontally it is divided, as you will notice, into years, and to the same scale vertically into years also. Immediately below are marked off the reigns of the various English sovereigns, under which are recorded, against their proper dates, some of the principal political events of the period. At the top of the chart will also be found, against their appropriate dates, a record of some of the principal social events, voyages, dis- coveries, inventions, and other data which indicate the progress of science and the arts, as well as of those social events which mark the increase of civilisation and the growth of kindlier feelings in the human race. A few statistics are also given of population, the output of coal and iron, and the progress of railway develop- ment, to show how rapid has been the advance during the present century. In the body of the chart are marked off by diagonal lines, commencing at their births and terminating at their deaths, the names of the great thinkers and workers, scientific and otherwise, who have done so much for the advancement of the human mind ; and coming later in the field, and marked in red, are noted those engineers whose work alone became possible as the study of nature broadened out and bore fruit. Consequently, by running the eye vertically upwards at any particular period, it will at once be seen who were the great contemporaries of that period, to what predecessors they were indebted, and what was the state of science during their lifetime, and among what political events they carried on their work. A very brief inspection of this chart will show that to no one man or country can be ascribed the sole merit of advancement. Advancement depends on the knowledge we have inherited from our ancestors, and the opinions of our contemporaries acting on and reacting upon each other, and together forming what we may call the drift of opinion of any age or period which we may examine. At the stage at which we have now arrived it is as well to conceive what must have been the feelings of men, especially of Englishmen, in the middle part of the sixteenth century. By the Reformation their minds had been opened to the exercise of private judgment, and there was presented before them a circumstance never before experienced, nor which can ever again appeal to the human mind. By the discovery of the new world the earth space had been practically doubled. These two great factors, freedom of thought and the enlargement of the world, aided by printed books, produced fresh fruit in literature and science, and an enthusiasm, almost amounting to the romantic, which carried men on to enter- prises of the most daring kind, and filled them with the confidence that a great and brilliant future was in store for the human race. The poetry and literature of the Elizabethan period teem with these senti- ments, and these feelings sank deep into the minds of thinking men when they contemplated more serious subjects. Peter Ramus (1515-1572) attacked the Aristotelian philosophy. Copernicus (1473-1543) revived the idea of Pythagoras and Aristarchus, that the sun, and not the earth, was the centre around which it revolved in company with the other planets. He, however, still retained the notion that they revolved in circles, and had, of course, to resort to epicycles, deferents, and the like, to account for their apparent irregular motions. At a little later period, Tycho Brahe (1546-1601) was carrying on a series of astronomical observations of an accuracy never before attempted; and although he did not accept the Copernican theory, yet he so far began to lose faith in that of Ptolemy as to propound a theory of his own to reconcile his more accurate observations. About the same time, William Gilbert (1540-1603) published his work on the 862 REPoRT—1900. magnet, and Sir Francis Drake, led away by that enthusiasm of which I have already spoken, in his great voyage round the world added new glories to English navigation. As conceptions more exact and observations more accurate were made, it became necessary in some way to shorten the laborious calculations previously carried on. Hence we get about this time the invention of logarithms by Napier of Merchiston. But this evident advancement of the mind was opposed fiercely by the powers of the Church, resulting in the burning of Giordano Bruno at Venice, in the year 1600, for upholding the Copernican theory. There now came upon the scene one of the greatest thinkers of our country, to whom all Englishmen, if not all Europeans, should feel the deepest gratitude, the great thinker, Francis Bacon, who, in his various works which he has left behind him, bequeathed to future ages that system of inductive philosophy which has done so much for the advancement of learning. As you will remember, his first doctrine is that we must avoid the errors which are inherent in the human race, and which he classes under the four heads of ‘Idols of the tribe,’ ‘Idols of the den,’ ‘ Idols of the forum or market,’ and ‘ Idols of the theatre.’ Having vot rid of erroneous and preconceived opinions, he lays down rules of right thinking, afforded by scientific facts which have been invaluable in the investigation of science. He does not touch upon religious and controversial subjects which engaged the attention of so large a proportion of his contemporaries, but directs the whole force of his philosophy to the acquisition of what he calls ‘fruits,’ that is to say, the pursuit of truth for its own sake. And as Macaulay says of him, although he is best known by his essays, yet of his more philosophical works he remarks that ‘they have moved the intellects which have moved the world.’ We now have to consider for a moment a name which should be highly honoured among all men of science, but especially among engineers, for to Galileo we are indebted for the first principles of mechanics. He invented the thermo- meter about 1602, and the telescope which bears his name in 1609. In 1586 he composed his first essay on the hydrostatic balance, and his observa- tions on the swinging of the great bronze lamp in the Cathedral of Pisa, as well as his experiments on the centre of gravity, and on falling bodies from the leaning tower, laid the foundation of the exact determination of some of our simplest mechanical conceptions. His astronomical observations of the moon, his discovery of Jupiter’s satellites in 1610, as well as the rings of Saturn and the phases of Venus, gave to the Copernican theory the basis of fact which was before wanting. It is needless to say that Galileo advocated most strongly the theory of his predecessor Copernicus, and for the doctrines which he so taught he was brought before the Inquisition, imprisoned, and his Jatter days rendered miserable by the persecution of the Church. Contemporary with Galileo was his illustrious correspondent Kepler, who in the most laborious manner, from the observations of Tycho Brahe and other accurate astronomers, gradually gave to the world thosé laws which bear his name, and fixed for all time the fact that the planets revolved around the gun, not in circular, but in elliptical orbits. These teachings, assisted by the illustrious Gassendi, were gradually forming tS the minds of men a somewhat more accurate idea of the universe in which we ive. We now come to one of those great minds, who, in the realm of philosophy, had a vast influence in turning the thoughts of men into direct channels. I allude to that distinguished Frenchman, René Descartes, I do not propose to inquire into his axiom, ‘I think, therefore I am;’ into his conception of innate ideas, nor into his theory of vortices, but would merely point out what may be almost called his great discovery, namely, the application of TRANSACTIONS OF SECTION G. 863 algebraical veasOning to geometrical conceptions and astronomical observa- tions. Of course his freedom of thought offended many, both the Jesuits, in whose school he had been educated, and the pastors of the Reformed Church, among whom he lived in Holland. And it is well known that he delayed to give to the world some of his best ideas owing to the way in which Galileo had been treated by the Church. The English philosophical writer, Thomas Hobbes, by the publication of his work called ‘The Leviathan,’ was also educating the minds of Englishmen in the direction of sound knowledge. It is interesting, however, to note that the new ideas had not as yet sunk deeply into the minds of the English people. Shakespeare remarks: ‘He that is giddy thinks the world turns round’ (‘Taming of the Shrew’). Bacon also naver accepted the Copernican theory, and if we turn to the eighth book of ‘ Paradise Lost’ we find that although Milton, who had visited Galileo in Italy, and who was well acquainted with the theory of Copernicus, founds his whole poem on a Ptolemaic basis, yet he was, apparently from the words which he puts into the mouth of the archangel Raphael, halting between two opinions. We now have to note another of the experimental philosophers in Christian uygens. Up to his time, the means of making accurate observations in which time was concerned wasa most difficult, nay almost an impossible, matter, By his introduction of the pendulum, as a regulator of clocks, he at once placed in the hands of men of science one of its most valuable instruments. His work on the centre of oscillation and the cycloidal curve shows how deeply he worked out the theory. His observations on double refraction, and his promulgation of the theory of an elastic ethereal medium in which the vibrations of light are carried on, place him in the forefront of the observers of his time. The sagacious Hooke, Wren, Wallis, and Newton’s great master Barrow, as well as the distinguished Boyle and the indefatigable Oldenburgh, were all carrying forward the work which distinguishes this period; and when we look back to those pleasant meetings at Wadham College, Oxford, during the Commonwealth ‘we contemplate a body of men working for true science who were to be the founders of that Royal Society which has done so much for the advancement of science throughout the world. The labours of all the great men of whom I have yet spoken were at this period gradually drawing together a vast mass of facts which required some com- mon explanation. The rudiments of mechanical science were beginning to teach the truth as to the laws of falling and oscillating bodies. The Ptolemaic system, with its complex theories, was gradually yielding to the accumulated evidence in favour of the Copernican system. The erroneous idea of circular motion had yielded, as the fruit of Kepler's per- severing work, to the law of elliptical orbits. But yet the minds of many men were still directed by the idea that the planets were carried round the sun by some inherent force in themselves, and in the same very imperfect way they were beginning gradually to think that this force, be it what it might, acted in inverse ratio to the square of the distance. Matters were in this state when there arose the greatest genius that the Knglish race has yet produced, the retiring, the sensitive, and the devout Isaac Newton, who, acting like an electric spark in a mixed and chaotic mass of vapour, at once recipitated, as it were, the confusion, and brought to light, with a dazzling bril- iancy, the gravitation theory, which not only accounted for all the difficulties which his contemporaries were struggling with, but at one bound elucidated those many and confusing motions of the heavenly bodies which had hitherto been the stum- bling block of observers. By his discoveries, for the first time an accurate scale was given to the universe, ‘and in his statement that every particle of matter in the universe is attracted 864 REPORT—1900. directly as the mass, and inversely as the square of the distatice, we have laid before the world once and for all time a sure and certain guide to all the phenomena of nature. He reveals to us distances incomprehensible, and magnitudes which transcend the most fanciful ideas of his predecessors, and flowing from this we have esta- blished the important conclusion that as far as matter is concerned, whether in the case of our own planet, in the sun, in the mighty orbs of Jupiter and Saturn, or in the distant nebule and stellar masses, the whole is governed by exact law, and is not a fortuitous concourse of atoms, or the result of some unexplained and inex~- plicable vortex motion. We may say of him in the words which I have above quoted from Lucretius, ‘the living force of his soul gained the day : on he passed far beyond the flaming walls of the world and traversed throughout in mind and spirit the immeasurable universe ; whence he returns a conqueror to tell us what can, what cannot come into being; in short on what principle each thing has its powers defined, its deep- set boundary mark.’ We must now turn to the contemplation of a great thinker who, although not a scientific man, has yet had the most profound influence in the direction of clear reasoning of perhaps any man in England since the time of Bacon. Lallude to the illustrious John Locke, the friend of Newton, of Boyle, of Monmouth, of Somers, of Clarke, of Montagu, of Pembroke, and of Shaftesbury, admired alike by Horace Walpole and by Voltaire, and the trusted friend and councillorof William of Orange. Intimately connected with the freedom of the press and the currency of this country, one of the first commissioners for trade and the colonies, he is princi- pally distinguished by his charming essay on ‘The Human Understanding.’ Putting aside the metaphysical conception of Descartes, he lays down the law that all our knowledge must be founded on two principles, experience of the outer world through our senses, which he calls ‘ sensation,’ and the inner working of the mind on the experience so gained, which he calls ‘ reflection.’ To his clear and lucid English which appeals to every reader, taken in conjunc- tion with the simple facts which he enunciates, the English nation is indebted for much of that common sense and freedom from fanciful speculation for which we are distinguished among the nations of the world. aa At the end of the seventeenth century Boyle, Hooke, and many others of their illustrious contemporaries were, in the early days of the Royal Society, founding that school of physics and chemistry which, taking the place of the alchemy and the magic of the middle ages, was being gradually moulded into shape in accord- ance with true induction and ina scientific spirit. But little had yet been done in the study of the earth itself. Pliny mentions the fact that fossil shells had been found; and Leonardo da Vinci, about the beginning of the sixteenth century, had argued that these fossils were the remains of extinct beings, and not Zusus natw'e formed by the action of the stars on the plastic substance of the earth; nor, as taught by the Church, shells dropped from the hats of pilgrims on their way from the Holy Land. And even at the end of the eighteenth century Johnson spoke, as it will be remembered, of people engaged in such a study as ‘ fossilists.’ We are indebted, however, for right thinking on truly scientific lines to Hutton, to Playfair, to Werner, and to Cuvier, who about the end of the Signe century began to formulate distinct and clear conceptions on the subject. The rocks of which the earth’s crust was composed were gradually being divided into aqueous, plutonic, and metamorphic. It was clearly established that among the aqueous deposits the various strata contained fossils different both in kind and in species from those of living beings. To our illustrious countryman William Smith we are indebted for the first geological map of Central and Northern England. Controversies arose as to how the great succession of events which accurate inquiry was unfolding to our knowledge was produced: whether upheavals and depressions in the earth’s crust were due to sudden cataclysms, dividing and TRANSACTIONS OF SECTION G. 865 shutting off, as it were, each successive period from those which preceded or succeeded it; or whether, as some imagined, they were the result of the Noachian deluge. And in the beginning of this century fierce discussions arose as to whether or not the whole tendency of these investigations was not intensely irreligious, as it appeared to be at variance with the account of the creation as given by Moses. In 1830 to 1833, however, by the publication of his ‘Principles of Geology, or the Modern Changes of the Earth and its Inhabitants,’ Sir Charles Lyell, following on the lines laid down by Hutton and Playfair, in the most philosophic spirit proved beyond a doubt that all the great changes which geology disclosed were the outcome of the action of those forces of nature which we see around us, operating with greater or less energy throughout long ages. Lyell did not attempt to theorise on how or why the remains of extinct animals and plants succeeded each other in the rocks, but he pointed out in the most precise manner that, whether we take the primary, the secondary, or the tertiary periods, the different series of organisms, of which we find the remains, were each distinctive of its particular zone; and that as we examine the tertiary strata their characteristics become more and more similar to the animals and plants which we see around us at the present day. Newton had taught us that the sum of space throughout the universe is prac- tically unlimited, and that the whole is governed by law and not caprice. The teaching of geology has instructed us in a somewhat similar way that the time over which the present forces of nature that have tended to form the earth, as we now see it, have operated, is to be measured, not by 6,000 years, but by many millions of years. I do not pretend to enter upon the vexed question of how many millions of years, but what I wish to direct your attention to is that, as astronomy teaches an almost infinite space, geology teaches not perhaps an infinite but a vastly extended period of operation almost beyond the grasp of the human mind. '_ Ihave spoken above of the action and interaction of the thoughts of our pre- decessors and our contemporaries in forming and originating new scientific conceptions in different periods. A curious example of this is to be found in modern science. Malthus published his essay on population in 1798, Sir Charles Lyell his £ Principles of Geology’ in 1830 to 1833. The great Charles Darwin has told us that it was by the study of these two books that he was first led to contemplate those changes in nature, and to amass that vast collection of scientific thought, which resulted in ‘ The Origin of Species,’ published in 1859, coincidently corroborated by the illustrious Wallace. The co-operation of these two great thinkers, the graceful way in which the younger gave place to the older observer, marks an advance in the kindlier feelings of contemporaneous scientific workers, in marked contrast to the virulent and often acrimonious controversies which characterised the period of Descartes and Newton. _ 1am not going to enter into a description of the Darwinian hypothesis, but it is sufficient to say that putting on one side for a moment the details with which it deals, the teaching of Darwin has produced during the last thirty years an entire revolution in our ideas, whether we look at them in literature or in science, by which we begin to understand how, in the long series of past ages, the various organisms which we find in the fossil state have passed gradually and almost imperceptibly from a lower to a higher state of organisation. And possibly in the teachings of our great countryman we see, for the first time, perhaps, in a some- what dim and distant way, a scientific reason for the origin of those innate ideas which formed so large a portion of the teaching of that great Frenchman René Descartes. And, again, we see in the teachings of science the reiterated lesson that nature works by slow decrees in an orderly and regular succession, ever advancing, ever improving, and not by spasmodic jerks; and the train of such ideas naturally leads the mind to the contemplation of a future more perfect and more beautiful in all that is good and true. 1900, 3K 866 REPORT—1900. And in the words of Tennyson we may say— Yet I doubt not, through the ages one increasing purpose runs, And the thoughts of men are widened with the process of the suns. It is not my object to trace the advance of science in all its branches down to the present time. I have above indicated the general lines along which the human mind has advanced in laying the foundations of our modern views; but so intimately are we, as engineers, connected with all the sciences that I must just refer in the briefest manner to the development of chemical science as it grew out of the teaching of Aristotle and Galen, that there were four elements, to the acid and alkaline dis- coveries of Sylvius, through the teaching of Geoffrey and Stahl of the phlogistic theory. We then have the discovery of oxygen by Priestley, and fixed air by Black and Cavendish, composition of water by Cavendish, Watt, and Lavoisier, followed by Davy and Dalton, the latter of whom formed our present conception of the atomic theory and the combination of the elements in their true proportions. Through Davy, Faraday, and Tyndall we gradually arrive at our electro- chemical ideas of the present day. We last year had so lucid an exposition from Professor Fleming, at Dover, of the march of progress in electrical science during the past century that it would be presumption on my part to attempt to recapitulate even the names which extend from William Gilbert, in the sixteenth century, down to the discoveries of Hertz of the present day. But I may be permitted to point out that from the time of Volta, Ampére, and Oersted the rapid progress which electrical science has made has been due in no small measure to the manner in which its experiments have been treated, on strictly mathematical lines, by the master minds of such men as Maxwell and Kelvin, until at last we arrive at the demonstration, long foretold, of the wave theory, which renders wireless telegraphy an accomplished fact. Light to the engineer has at all times been of supreme importance, and on the chart we may scan the names of those who have advanced our scientific knowledge of it from Galileo, Descartes, Huygens, Gregory, Newton, up to Roemer who dis- covered its velocity, then Halley, Herschel, and the illustrious Thomas Young who revived and Fresnel who perfected the undulatory theory, until at last we come to those mysterious Fraunhofer lines, previously noticed by Wollaston, interpreted by Bunsen and Kirchhoff in 1860, and applied as an aid to chemistry in the analyses of terrestrial and celestial bodies. In the theory of heat we have the experiments of Cavendish and Priestley investigated by Count Rumford, illustrated by Tyndall, and bearing fruit in Joule’s mechanical equivalent. Perhaps none of the allied sciences appears so distant from our own profession as that of physiology, The discovery of Harvey gives us, however, a beautiful insight into animal mechanics; and the observations of Leeuwenhoek about the year 1700 first bring us into contact with those minute organisms which he discovered by means of the microscope, and which are now found to play so large a part in the economy of nature. Up to within the last twenty years it was generally held that dead organic matter, anima! and vegetable, could but, in the words of Shakespeare, ‘lie in cold obstruction and rot,’ this process being assisted, it was assumed, by chemical oxidation; and, until the researches of Pasteur and Koch, we were entirely ignorant of the fact that nature had at her command countless millions of organisms, always reducing the effete products of animal and vegetable life back into simpler elements. The tendency of later years has clearly been, whether we look at the links which unite heat and work, chemistry with electricity and magnetism, and light with both, or physiology with chemistry, to obliterate those boundary lines which we have been accustomed to regard as fixed, and from the time of the publication TRANSACTIONS OF SECTION G. 867 of Sir W. Grove’s correlation of the physical forces in 1846 we have made con- tinued advances in the same direction. What the future may have in store for us we cannot imagine, but clearly if we compare the facts known at the commencement of the nineteenth century with those in our possession at the beginning of the twentieth century, we may look forward to a still richer harvest of what Bacon calls ‘fruits.’ Looking back upon the facts that I have been enabled, and I feel so imperfectly, to bring before you, I have ‘ to answer’ the question with which we set out. Modern scientific thought is due to an inquiry into Nature and her works, irrespective of all preconceived theories, and the breaking away from the authority which other departments of human thought and faith have in former ages imposed upon some of the earlier inquirers into science. Faith in religion has been defined as ‘the substance of things hoped for, the evidence of things not seen,’ which is altogether apart from the other and wider faith with which the scientific inquirer contemplates that vast, that stupendous, that beautiful universe which has been revealed to him by the teaching of his pre- decessors, and which inspires him with those hopes to which I have just alluded. On the teaching of the ancients Bacon remarks: ‘The opinion which men entertain of antiquity is a very idle thing, and almost incongruous to the world ; for the old age and length of days of the world should in reality be accounted anti- quity, and ought to be attributed to our own times, not to the youth of the world which is enjoyed among the ancients, for that age, though with respect to us it be ancient and greater, yet with regard to the world it was new and less.’ This idea is perhaps more and more beautifully expressed by Tennyson in the words ‘I, the heir of all the ages in the foremost files of time.’ And in another respect, taking Bacon’s teaching which he so often reiterates, as being a search after fruits, we must not imagine that the fruits of which he speaks are necessarily to be gathered in by the worker himself. For the pursuit of true science is often hindered by the too greedy effort to grasp the sordid rewards of the present, and, alas! Bacon himself will ever stand as a most painful example of the depth of degradation to which even the highest minds may fall. We must learn from Nature what she is continually teaching, that her efforts are directed, not solely for the benefit of the individual, but for the welfare and the advancement of the race. The fruits and the rewards which grow from a study of Nature, and a truly scientific effort to expound her laws, are of a higher and a wider scope. And in contemplating the work of the great men of the past with whose names we have been so freely dealing, looking at the present attitude of the scientific mind, and our share in the application and directing of those great sources of power in Nature, we may say : “No more a wind-borne leaf upon the waves Of time and chauce, but one to whom is given, To help the mighty purpose of the world, To straighten crooked paths, to smooth the hills Of sin and sorrow, that on some bright day The great wheels of the world may run their course Without one jar or check.’ The following Papers were read :— 1. Water Supply, with a Description of the Bradford Waterworks. By J. Watson, M.Jnst.C.B.+ _ 2. The Disposal of HouseRefuse inBradford. By J.McTaceart,A. MIME. The author gave particulars as to the quantity of refuse collected, the quantity destroyed by the destructors, and of the quantity tipped or sold. 1 Published in exténso, Bradford, 1900. 3K 2 : : ) &68 REPORT—1900. Particulars were given as to the number and capacity of refuse destructors in Bradford, and a complete description of the Hammerton Street destructor, and the results of a seven days’ test on this destructor were supplied. The utilisation of the residuum or clinker from the destructors, its use in mortar making, and the clinker-crushing and screening machinery were described. A short account was also given of the utilisation of the steam produced by the destructors, and a description of a new destructor in course of erection at Southtield Lane. FRIDAY, SEPTEMBER 7. The following Papers were read :— 1. Resistance of Road Vehicles to Traction. By Professor Hee Suaw, LL.D., FR.S. About the time of the general introduction of railways considerable attention was directed to the nature of the resistances encountered by vehicles upon the common road, and the researches of Correze, Edgeworth, Coriolis, Morin, Tredgold, Dupuit, and others must be regarded as having thrown considerable light upon the subject. From time to time recently others have done work in this direction, but there is no doubt that the attention directed to traction on railways has thrown the scientific investigation of the subject of common roads almost entirely into the background. During the last few years, however, it has been realised that there was a great field for the development of traction, and particularly by mechanical means upon the common roads, and the improvement which has been quietly taking place in the construction and maintenance of roads is a feature of national importance. Not only is the condition of the pavements in the cities and towns much improved, but in out-of-the-way districts, such as in the hilly parts of Cumberland and Westmorland, the use of steam rollers by the County Councils has effected vast improvement in the state of the roads. Various causes have contributed to this result, but it is worthy of notice that whereas when the coaching days became comparatively a thing of the past the roads fell into neglect, so now the increasing number of cyclists and tourists who visit country places are an appreciable factor worthy of consideration and encouragement by the local authorities. The recent remarkable and growing development of motor vehicles with a legal limit of speed as high as twelve miles an hour, and the generally increased speeds of tram-cars in cities owing to the introduction of electricity and steam, give some reason for thinking the general rate of speed on common roads may reach, or even exceed, the present legal limit applying to motor vehicles. As showing the mechanical possibilities in this direction, it may be poe out that quite recently in France between forty and fifty miles an hour ias been safely maintained for more than 300 miles upon the common road. Such a speed—or anything approaching to it—would not be allowed in this country, but the fact remains that it is possible with safety. With heavy traffic the legal limit for a self-propelled waggon of about two tons tare, capable of carry- ing several tons, is no less than eight miles an hour, and the heaviest traffic with a tare limit of vehicle of three tons, probably carrying a load of eight or ten more, is as high as five miles an hour. These facts, and the introduction generally of mechanical propulsion, point to the necessity of having a fairly complete knowledge’ of the resistance of common roads of various kinds upon different classes of vehicies moving at different speeds. In the brief historical account given by the author of what has hitherto heen done in this direction it will be seen that the experimental means of traction has without exception—as far as the author is aware—been limited to traction by horses ; ard as at any rate the earlier experiments were made with the view of horse traction, only two speeds were taken into account, viz., walking and trotting. Considering the variation in speed of horses under these two conditions, these terms TRANSACTIONS OF ‘SECTION G. 869 cannot be said to express anything very definite, and certainly afford no guidance whatever as to the resistance of self-propelled vehicles at various speeds, Again in recent years large sections of cities have been paved with asphalte and wood, while the laying of setts or stone pavements has undergone considerable modi- fication, which is readily seen by an examination of a modern street and one of ten or fifteen years ago. Another modern development is the introduction of solid indiarubber and pneumatic tyres, which were at first regarded merely as a luxury, but have now proved to be an important factor in the life of the vehicle, as well as of its resistance, this being so much the case that efforts have from time to time been made to introduce the use of indiarubber tyres upon traction engines. Beyond the foregoing points, which have not been brought under investigation in connection with the resistance of vehicles, no attempt appears to have been made to ascertain the extent to which the various factors of resistance relatively affect the whole result. Now it is evident that as the higher speeds are used, and the weights are increased, vibration and shock become more and more important ; thus the resistance due to the rim of the wheel, and the ways in which it can be met by mechanical contrivances, must be regarded as quite a different problem from that of the springs attached to the body of vehicles, and some distinction must be made between the resistances as affected by each of the foregoing. Enough has been said to show that there is not only matter for an inquiry which would be welcomed by makers of road vehicles, especially of self-propelled road vehicles, but that such an investigation, if it is to be of any real value, must be thorough, and requires not only some expenditure of money, but cannot well be undertaken by any single individual. The great interest which was excited by the paper read by Mr. Thorneycroft at the last meeting at Dover of the British Association, and the previous communications which have passed between the author and the President of this Section, who is himself a high authority upon the question of roads, have led to this matter being brought forward with the idea of forming a committee of the British Association for the investigation of road resistance. In order to facilitate the work of the Committee, a summary of previous investi- gations in this subject has been prepared, which can be laid before the members, if it is formed. Some preliminary experiments have also been made with a view to obtaining some idea of the nature of the apparatus required, and the amount of expense likely to be entailed. Preliminary Experiments. Allusion has been made to the fact that all the previous experiments have been performed by means of the traction of horses: it seemed with the introduction of powerful motor cars it might be able to pull steadily any vehicle at any required speed. This idea really forms the chief feature of the proposed experiments, as it is evident that if one motor car is not suflicient two or more could be harnessed to the vehicle which is to be drawn. In order to ascertain how far this idea was practicable, Mr. J. A. Holder, of Birmingham, who owns a 12 h.p. Daimler car, was kind enough to visit Liverpool, and on Tuesday, Wednesday, and Thursday, July 17, 18, and 19, a series of experiments, in which the author was assisted by two former students, Mr. Humfrey, B.Sc., and Mr. Cormack, B.Sc., were made, Mr. Holder's autocar towing the author's New Orleans Voiturette. These experiments took place over roads of asphalte, wood, setts, and macadam in the neighbourhood of Liverpool, both level and up the steepest gradients which could be found, viz., Everton Brow, the details of which were given in a wall diagram. It will not serve any useful purpose at present to give the detailed results of these experiments, as they were obviously incomplete, and pointed to the absolute necessity of more elaborate apparatus of a self-recording nature ; but it may be of interest to explain the apparatus actually employed, so as to indicate what wiil be required to insure satisfactory results. The apparatus consists of two parts, which were illustrated by wall diagrams (1) a dynamometer, and (2) a speed indicator: Dynamometer—This consisted of an ordinary spring balance, the back of 870 REPoRT—1900. ‘which was riveted to a cylinder of a small steam engine which acted as 4 dasha pot. The ports of the steam cylinder were closed up, and a small hole drilled into the piston was found quite sufficient when the cylinder was filled with oil to check the free oscillations of the spring. Speed Indicator.—The speed indicator was a Schaffer and Budenburg tacho- meter to which a temporary wooden wheel was attached, and a special dial was made, so that instead of indicating revolutions per minute the miles per hour at which the vehicle was travelling were at once made visible. The mode of con- ducting the experiments is shown by a photograph. A rope about 20 feet long was attached to the Voiturette and connected with the dynamometer, the dial of which an observer was able to read. At the same time a second observer called out the actual speed of the vehicle at that instant and the nature of the road which was being passed over, which were recorded by the first observer in his notebook, together with the pull on the dynamometer. The net result of the experiments showed that, even on apparently the smoothest road, the variation in the pull was so considerable that nothing but appliances which would record autographically both the pull and yelocity at the same instant and indicate also the distance travelled, so as to identify the exact piece of road corresponding to the record, would be of any value. Moreover, it was evident that some autographic record of the nature of the road, as well as some instrument for recording the vibration of the vehicle which was being towed, was necessary in order to form some estimate of the effect of vibration upon the resist- ance. With such appliances the pull on waggons, lorries, ordinary vehicles with iron rims, pneumatic and indiarubber tyres, could be investigated for any speed, and it is not too much to hope that some definite idea of the laws concerning traction might be found, with the effect of springs, tyres, and the surface of the road taken into account. 2. The Viagraph. By J. Brown. The viagraph is an instrument for indicating the degree of unevenness of road surfaces, and consists in principle of a straight edge to be drawn along the road surface and provided with a profiling wheel running on the surface, the vertical motions of which are transmitted to a pencil marking on a paper band, drawn under its point by a drum revolved by gear connected to the profiling wheel. The result is a profile of the road surface full size vertically, and 4 inch to 1 foot horizontally. Means are provided for indicating the sum of the vertical motions of the profiling wheel, which sum represents numerically the relative unevenness of the road, and is called the index of unevenness when taken for a unit length of 88 yards of road. This leneth is automatically measured by the iustrument, and an alarm bell rung when it has been traversed. Speculations as to the causes of unevenness, the proper make of wheels and springs for a given unevenness, and calculations of the horse-power absorbed in traction due to unevenness may be founded on the indications of the instrument. 3. A Self-registering Rain-gauge. By W. J. E. Binnie. This rain-gauge is constructed so as to register the rate of rainfall at any moment by means of the drops falling into the interior of the gauge from the orifice of the collecting funnel. The weight of each drop depends upon— 1. The surface tension between air and water. 2. The dimensions of the orifice. 3. The interval which separates the fall of the drops. 1. The surface tension varies with the temperature, amounting to about rz per degree Fahr , giving a probable maximum error of 2} per cent. 3. The influence on the size of the drops of the interval between the fall of TRANSACTIONS Of SECTION G. 71 each is very tnarked when that interval is less than five seconds; biit the telative dimensions of the funnel and the orifice are so chosen that sufficient interval for the formation of the drop is allowed even with very heavy rainfalls. The funnel is so arranged as to discharge into a tube containing the drop former. From the orifice of the drop former each drop falls and impinges on a pan carried at one end of a counter-balanced lever. The momentum of the drop striking the pan causes that end of the lever to be depressed, so that a small pointer rigidly attached to the lever dips into a cup of mercury, closing the electric circuit to the receiver. The counter-balance then brings the lever back to its original position in which the circuit is broken. The rain, after falling from the pan, passes into a collecting vessel by means of which the readings can be checked, and which would also obviate the loss of a record in case of anything going wrong with the instrument, In this way each drop as it falls sends a current through to the receiver, which may be placed anywhere. The receiver consists of a drum driven by clockwork, to which is attached a diagram in the usual manner. This diagram is divided vertically into time intervals, and horizontally sv as to read in inches of ‘rainfall,’ the scale being dependent on the relative dimensions of the collecting funnel and drop former. Each current transmitted to the receiver works an electro-magnetic escapement in such a manner as to move a pen on the diagram through a certain space vertically. By this means the total rainfall and the variations of rate of rainfall are registered on the drum. 4, The Coal Fields and Iron Ore Deposits of the Provinces of Shansi and Honan and Propose’ Railway Construction in China, By J. G. H. Guass, C.L7. The general object of this paper was to furnish information respecting the opening up by British capital of the two large provinces of Shansi and Honan, and developing the vast and practically unparalleled mineral wealth they contain, by the construction of a system of railways, starting from the coal-fields of Shansi and connecting with the Yangtzi River opposite Nanking on the south-east and the Wei River on the east, at a place called Taokou. At the proposed terminus pe Nanking, the Yangtzi River is open to sea-going vessels, and at Taokou, the other terminus, the Wei River is now navigable for barges having a capacity of from twenty-five to thirty tons as a maximum, and by the expenditure of a moderate sum in deepening and widening certain parts, navigation would be eatly improved. The large and commercial town of Tientsin is reached from aokou by means of the Wei River and the Grand Canal, on both of which there is free navigation throughout the year, excepting for a short period in the winter of varying duration, when it is closed by ice. The coal-fields will thus be brought into communication with the seaboard at Nanking in the south and Tientsin in the north. The railways will besides connect with numerous waterways inter- secting the country traversed, most of which are navigable, affording a cheap and convenient means of conyeying ccal, &c., to the dense population inhabiting the Great Plain of China. The paper gave a description of the bituminous and anthracite coal-fields of Shansi and Honan, visited either by the author or by members of his expedition last year, and the approximate area of the coal-measures and contents available. Analyses of specimens of the coal, brought to England for that purpose, were furnished, and information given on the methods of mining adopted by the Chinese, the output at the mines visited, and the cost at pit-head. Photographs of a typical coal-mine, showing the workmen, coal-stacks, and the vehicles used for transporting the coal, were shown to illustrate the paper, and maps of the country, showing the proposed railway routes. The paper described the great deposits of iron ores associated with the coal-fields of Shansi, and the‘r general Ny 872 REPORT—1900. distribution and occurrence ; analyses of them were given, and the methods fol- lowed by the Chinese in their reduction described. Sketches were given of the furnace employed, the manner of loading it was explained, and details were given of the results obtained, and an estimate was furnished of the yearly output gathered from reliable sources, and the cost of production. The description was illustrated by photographs, The existing means of communication by land and water was referred to, and information collected by the writer furnished in respect to the vehicles and pack animals used for carriage on roads, and the cost of trans- porting the products of the mines under present conditions, A description, accompanied by photographs, was given of one of the great high roads of China, the methods of its construction and alignment, and the difficulties which it presents to vehicular traffic briefly alluded to. Some information was also furnished regarding wages of skilled and unskilled labour, the general condition of the people, their food and habits, the effects of the last great famine on them, their demeanour towards foreigners as experienced by the writer and his staff, and as gathered from statements received personally from missionaries who have long resided in the country, and the desire evinced, not only by the workmen them- selves, but also by officials, to see the natural industries developed whereby regular employment and good wages would be obtained. The implements used by the Chinese in mining and other industries, and their methods of agriculture were alluded to. A general description of the country to be traversed by the proposed railways, its physical aspects, population, and trade, was given, and also an account of the rivers and waterways encountered, with special reference to the Yellow tiver, and the measures to be adopted for bridging it, The gauge on which the railways are to be built, and the nature of the permanent way and rolling stock were referred to, and also other matters of interest in connection with construction. The paper also contained some remarks on existing and projected railways in China. It concluded with some general remarks on the cost of the lines of railway referred to, and haulage rates. 5. The Use of Expanded Metal wm Concrete. Ly Artuur T. Watmistey, I. Jnst.C.£. The author’s paper began by stating that the subject of the judicious intro- duction of iron and steel sections into concrete was a leading topic of discussion at the present time among engineers, and he referred to the paper read at the Liverpool meeting of the British Association descriptive of the manufacture of expanded metal by Mr. J. F, Golding, the inventor of the machinery for its production, and then dealt with its development, with special application to its introduction into concrete for supplying that tensile element which concrete without metal lacks. The present machinery is limited to sheets eight feet in length, but larger machines are in contemplation for the Expanded Metal Company’s works at West Hartle- pool, to enable sheets of metal long and strong enough for spans of 16-foot slabs to be supplied. The author assumed that the safe-working unit stress for concrete in compression is ten times the safe-working unit stress for concrete in tension, and pointed out that, under these circumstances, with a homogeneous section of pure concrete having parallel sides the neutral axis must be above the level of the centre of gravity of a slab laid horizontally or vertically; and that, assuming—as in the case of a slab supported at the edges—that it is laid flat, the neutral axis of a section divided the depth into the proportions of 24 and ‘76 re- spectively in order to create a result equal to a couple in which the compressive and tensile elements unaided by metal would be in equilibrium. The author then gave calculations showing the effect of introducing metal into the tensile portion of the section, whereby the neutral axis under the above conditions of equilibrium is lowered, the compressive portion is increased, and the neutral axis made to approach nearer the centre of gravity of the section. Examples were given of a section containing wires or rods, plates, and inverted tee sections, together with a comparison of a section containing expanded metal; and the author pointed out - that the latter provides a uniform distribution of tensile strength in all directions, TRANSACTIONS OF SECTION G. 873 ‘ample in amount without extravagance, and easily laid without the responsibility of supervision in placing the material transversely at the specified distances apart, as would be necessary in the case of separate pieces. The insertion of wires or individual sections gives strength in the direction of their length, leaving the inter- mediate concrete comparatively weak. Expanded metal contributes strength laterally both in the direction ot width and length, as well as giving an effective keyage in its depth. The coefficients of expansion of the two constituents, iron or steel and concrete, are considered for all practical purposes to be identical. Results of experiments made on various-size slabs were next given, the longest span without intermediate joists being on a slab 12 ft. Gin. by 11 ft. clear span, which was loaded to 53 ewt. to the foot super, and bore this load for 14 hour before it collapsed, the fractures occurring at each of the four corners. The gradual increase of the load and progress of deflection of the slab were related in detail. The adhesion of iron and concrete was found by Professor Bauschinger, of Munich, to be about 569 to 668 pounds per square inch, but a case was quoted, experimenting upon 2 in. diameter anchor bolts set 11} in. in a masonry block, with lead, sulphur, and cement, from which it was inferred that in suitable setting the cement joint on a smooth rod might be made to fracture the rod before the adhesion of the connection failed. The author described the introduction of the aid of channel arches by the Expanded Metal Company. The spans were enabled to be increased thereby, the only objection being, in the author’s opinion, the exposure of the under surface of the channel metal rib; but the surface so exposed is com- paratively small compared with the various systems of trough flooring that have been patented. The result of experiments was stated in the paper, the channel ' metal flat arches being firmly held between longitudinal joists spaced at specified intervals. The author considered that, in order to keep the portion of a slab containing metal in tension below the neutral axis, the slab should not be fixed at its bearings ; but he pointed out that probably there is a tendency to form a flat arch within a concrete beam, which converts a large part of the vertical pressure into lateral thrust, which in the case of an expanded metal section becomes a tied arch, and that, in his opinion, a concrete beam should be viewed as a bar, with a hollow curved soffit. Further developments of the system were reviewed, and diagrams illustrative of the arguments propounded were exhibited, with a view to elicit suggestions as to any desired improvement in the size of the meshes employed or to further experiments needed. 6. Power Generation.—Comparative Cost by the Steam Engine, Water Turbine, and Gas Engine. By Joun B. C. Kersuaw, £.L.C. There is no question of greater importance at the present moment to those engaged in the management of our manufacturing industries than that of power generation. The supremacy which the steam engine has so long enjoyed is now assailed from two sides. The water turbine and the gas engine have become dangerous rivals. During the past ten years a most remarkable development of hydraulic power has been taking place on the continent of Europe in France and Germany, and in America at Niagara. The aggregate amount of power at the present date generated from falling water forms no inconsiderable portion of the total power utilised in manufacturing industries; and two years ago it was estimated by the author to be between 236,000 and 350,000 horse-power. On the other hand gas engineers have been busily engaged in working out the problems presented by large gas engines and by the utilisation of the waste gases of blast furnaces. Gas engines up to 650 horse-power have been built, and have worked smoothly and economically ; while at Seraing in Belgium and at other places the blast furnace gases have been utilised for driving the engines which supply the blast. The question, therefore, which the engineer now has to settle when deciding upon the site and locality for a new factory, or when deciding upon the system of 874 REPORT—1900. power generation to adopt for extensions of the old, is no longer so simple as when only one method of power generation in large units was open to him. It is no doubt true that the choice between the three possible sources of power is one which in many cases will be settled purely by local considerations ; and the proximity of a large waterfall or of an extensive coalfield to the factory, will be held to point to the turbine or to the steam engine as the most economical power generator. Ina great number of cases, however, especially when the decision of the engineer covers the choice of a site for the factory, the problem is capable of no such easy solution; and the most economical source of power can only be determined after an exhaustive study of comparative costs data. The aim of the writer in the present paper has been to collect and arrange in comparable form some of the more important figures bearing on the cost of power generation. Full references are given to all the original articles from which these figures are drawn.’ Taking the best figures for each of the three sources of power dealt with above, and bringing them all to a common basis of comparison, namely, the cost of the E.H.P. year of 8,760 hours, the authcr obtained the figures given below, Taste VII.—Comparative Costs of Electrical Power. Lowest Cost per E.H.P. year of 8,760 hours Source of Power Estimated Locality | Actual Locality 4s. Sd. le 8. d. Water. 1 5 5 | Canada | 119 0| Switzerland Steam . ‘ 418 8 | North England |4 9 7| United States Gas (Producer) . 56 O O | England — — Gas(Blast Furnace). | 4 1 7 | Germany | — — The figures in the table support the opinion, now generally held, that water when developed without excessive capital expenditure is the cheapest source of mechanical or electrical energy. When, however, the hydraulic engineering expenditure has been heavy, or when the power after generation has required to be transmitted over long distances, the margin between the relative costs of water and steam power is greatly narrowed, and in some Cases disappears. Electrical energy generated by falling water is costing more at Rheinfelden, at Zurich, and at Buffalo than it would cost in South Lancashire if generated by steam power in large units ; and the margin between the actual charge for power | . Niagara and the estimated cost of steam power in large generating stations in ‘outh Lancashire is only 12s. 1d. per E.H.P. year. In this connection it is interesting to note that the charge for electric power in Buffalo is 13s. 6d. per E.H.P. year higher than at Niagara; and the excessive charge to small consumers in the same city (25/. 11s. per K.H.P. year) would seem to indicate that the cost of transmission between Niagara and Butfalo represents at least 20s. per E.H.P. year on the power sent into that city. Turning now to a consideration of the relative position of gas power, the ques- tion of the practicability of large engines may be taken as settled. If they do not cost excessive sums for maintenance and repairs, large gas engines, in conjunction with coke ovens and blast furnaces, may entirely alter the present position of affairs; and the new industries which at present are being established in the neighbourhood of water-power stations may find themselves in severe competition with similar manufactures carried on in the coal and iron districts of the older manufacturing countries, _ It has been calculated that 2,000,000 H.P. is annually wasted in the gases issuing from the blast furnaces of the United Kingdom. If these waste gases 1 Tables I. to VI. contain details of sixty-five actual or estimated costs of steam, water, or gas power per H.P. year of 8,760 hours, TRANSACTIONS OF SECTION G. 875 Could be industrially utilised in the manner suggested, we should to a large extent be compensated for our lack of natural water power. But blast furnaces demand coke, and coal beds are exhaustible, so that even if this source of mechanical and electrical energy be tapped it can only postpone, but not avert, the final triumph of the waterfall and of the turbine. SATURDAY, SEPTEMBER 8. The Section did not meet. MONDAY, SEPTEMBER 10. The following Papers were read :— 1. The Automobile for Electric Street Traction, By J.G. W. ALDRIDGE. 2. The Manchester and Liverpool Express Railway. By Sir W. H. Prrece, /L.S. A monorail line has been projected by Mr. Behr between Manchester and Liverpool to accommodate express passenger traffic alone between those two cities. It is to be worked by electric traction and to attain very high speeds. The train ‘is to consist of only one coach, weighing forty-five tons and seating sixty-four passengers. Starting at every ten minutes, and travelling at the mean rate of 110 miles an hour, it will do the distance of 34} miles in twenty minutes. The fares will be slightly lower than those charged at present. There will be no inter- mediate stations, no points or crossings. There will thus be no necessity for signals to protect the line during other operations. Signals would be needed only to secure a perfect block system of working the line. The monorail railway was projected by Lartigue in 1882. We have only one example of this system of railway in the United Kingdom, viz., between Listowel and Ballybunion, in County Kerry, Ireland. This line was designed and engineered by Mr, Behr. The Act was obtained in 1887, and the line was opened for traffic in February, 1888, and it has been running ever since. The line is 94 miles long. It has one intermediate station, Liselton. There are forty-two level and farm crossings, It is worked by steam. The train consists of a locomotive and four coaches. It cost 33,000/. to build, or 3,060. per mile. When I inspected the line in the early part of this year there had never been a Board of Trade inquiry into any accident. The maintenance of the structure had been effective. No rail had ever been turned. The mechanical structure had exhibited no defects, but several breakdowns had occurred in the locomotive and rolling stock. ‘There are three locomotives, eleven passenger coaches, and two brake vans. They had, however, continued to work the line uninterruptedly for twelve years, and there had been no renewals or new stock, Its main principle is the suspension of the coaches on a single elevated rail so that their centres of gravity are below the rail. Hach coach sits the rail like a saddle. The rail is fixed on trestles; which are tied and braced together, the tie bars being light rails against which guide wheels roll. The Manchester and Liverpool Express is intended to be more massively and rigidly built. Derailment on such a structure is impossible, and curves of com- paratively small radius can be passed with safety at high speeds. Vibrations and noise will be reduced, and travelling will be conducted with greater comfort than at present. It is proposed to fix the generating station midway at Warrington, and to transmit the electric energy at high pressure (10,000 volts) to each terminal 876 REPORT—1900. station. There would be sub-stations along the line, at distances apart of four miles, where the 10,000 volts would be brought down to 1,V00, at which pressure it would be picked up by the motors on the coach. The speed which a train can acquire on a railway depends on the power that can be continuously applied at the thread of the driving wheel. Electricity enables the engineer to apply instantaneously to light loads a power which steam cannot supply. Hence speeds are possible with electricity which are unattainable with steam. A coach weighing forty-five tons can easily and quickly attain 110 miles an hour. 1,600 horse-power will accelerate the coach so as to attain this speed in 110 seconds, and 500 horse-power will maintain this speed on the level. Electricity has two advantages over steam. It enables us to obtain an accelera- tion of 13 feet per second, which is virtually the limit that can be obtained without causing discomfort to the passengers; and, secondly, it applies a continuous and constant torque instead of the variable one due to the reciprocating action of the ordinary steam locomotive. Hence it not only enables us to maintain high speeds on long through lines like the proposed Manchester and Liverpool Express, but it enables us to attain high speeds with greater rapidity on short lines having frequent stoppages, like the Metropolitan railways of London, and thus increase the capacity of the line for traffic. The chief causes of accident on ordinary railways, viz., collision, derailment, points, and the human error of the signalman, will be removed from lines. Hence travelling will be much safer. 3. Manchester and Liverpool Electrical Lxpress Railway : Brakes and Signals. By F. B. Brnr. The questions of brakes and signals are so intimately connected that the one cannot be treated separately from the other, The most perfect condition under which a railway could be worked would be that in which both brakesand signals could be dispensed with ; therefore it follows that the fewer the occasions for using either, the better. Now as to brakes, there is a limitation of their application, which depends not so much on the mechanical appliances themselves as on the endurance of the passengers. It was stated by an eminent railway official to the Select Committee of the House of Commons that with the Westinghouse brake a train travelling at 60 miles an hour could be stopped at an emergency, within 360 yards, without inflicting too great a shock on the passengers. In the same way the proposed train travelling at 110 miles an hour could be stopped within 500 yards, and probably in a shorter distance, as in this case electrical means would be at hand, such as the reversal of the motors, so as to turn them into dynamos. More rapid stoppages could only be made with great discomfort to the passengers. Now in the ordinary way of working our railways at present there are many occasions in which it might be important to stop the train as rapidly as possible; for instance, if a train should be seen in front, or some shunting operations were not com- pleted, or in some other cases too many to enumerate. But no brake, however powerful, would be of the slightest use to-day for avoiding a sudden obstacle, such as a stone placed on the rail, or a broken rail, for it is impossible for the driver to be aware of such obstacles until he is practically upon them. In these a therefore, the power of stopping at 300, or 200, or even 100 yards is quite useless, The author then stated that on the proposed high-speed electrical railways, though it is quite possible to stop the train within less than 500 yards, it never can be necessary to bring it to a standstill at even a much longer distance. On the proposed railway there will be no level crossings, no switches, no shunting operations, and in fact nothing that will require the*train to be brought to a standstill unless a preceding train should break down. Besides this. one case, the brakes can only be used for stopping as you approach the stations. A broken rail produces no danger whatever, for the train would run over it without any risk or difficulty. ‘This can easily be shown by carefully TRANSACTIONS OF SECTION G. 877 considering the relative position of the wheels of the carriages to the rails over which they travel. It remained, therefore, only to explain the manner in which it is arranged that the driver of each train shall be informed of the possible stoppage of the train in front of him. Under normal conditions no second train will leave the station at Manchester or Liverpool until the first has reached Warrington, a distance of over 17 miles. The line will be subdivided for the purpose of signalling into eight sections of 4:3 miles each. As a train leaves Manchester or Liverpool a danger signal is put up automatically at that station, and a second similar danger signal is put up in the same way at 4°3 miles off, the first remaining at danger. The train travels on until it reaches 8°6 miles, when it puts up a third danger signal, and simul- taneously the signal is lowered at Manchester or Liverpool, so that the second train can now leave. Assuming that the first train has met with an accident after passing the point distant 86 miles, the second train would travel at full speed until it passes point ‘38 miles. The danger signal at that point not having been removed by the first train, as it never reached point 13 miles, the driver of the second train would be informed that the first train had met with an accident between 8°6 miles and 13 miles, and therefore that he has to slow down, but that for such lowering of his speed he has a clear run of over four miles. Therefore, there could be no difficulty in stopping without using the brake at all by simply cutting off the current. Whenever a train passes over a point where the danger signal is put up this is reproduced, either electrically or mechanically, by a very simple and inexpensive contrivance in the cabin of the driver, so that he would be perfectly able to see it without difficulty even if there was a thick fog. Under these conditions of travelling it seems, therefore, superfluous to have any emergency brakes; and though it will be possible to stop the trains within 500 yards, no ease can be imagined in which it would be useful or necessary to resort to such a stoppage. A six minutes’ service of trains could be established without any alteration in the proposed arrangement, and if a three minutes’ service was required the blocks would have to be reduced to two-mile sections, giving a clear run of two miles in case of a breakdown. 4, The Construction of Large Dynamos, as exemplified at the Paris Exhibition. By Professor 8. P. Toompson, F.R.S. B. Recent Tramway Construction. By W. Dawson. 6. Measurement of the Tractive Force, Resistance, and Acceleration of Trains. By A. Mattock. The author described in the paper some experiments recently made on electric and other railways, the object of the experiments being to determine the accelera- tion, tractive force, and running resistance to which the trains are subject. The appliance used was a short pendulum whose free vibrations are adequately damped. If this is snspended on the moving body it will hang in the direction which is the resultant of gravity and the acceleration which the body at the time experiences; hence the angle which such a pendulum makes with the vertical gives the measure of the accelerations at each instant. In the experiments the pendulum was arranged so as to record its position on uniformly moving paper, on which at the same time seconds were marked by an electyic clock, and a contact marker, worked from one of the wheels of the carriage, caused a second pen to record each revolution performed by the wheel, The 878 ‘ REPORT—1900. diagram thus obtained gives a direct measure of the speed and acceleration of the carriage. The author showed that pendulum observations, combined with a record of speed and power supplied, offer a simple and effective means of determining the resistance to, and efficiency of, electric or other kinds of motor vehicles. 7. On a Combination integrating Wattmeter and Maximum Demand Indicator. By T. Barker. The paper fully sets forth the advantages of the maximum demand system of charging for the supply of electricity, and describes a new meter—the invention of Messrs. Barker and Ewing--to be used for this purpose. The paper was illus- trated by diagrams, and examples of the meter were exhibited. In charging for the supply of electricity it has become usual to make a dis- tinction in the prices charged to those consumers who use a few lights for many hours per day and those who use many lights for an hour or less; for, although at the end of the year the number of units consumed may be the same in both cases, the cost to the company or corporation in machinery, mains, and every other charge will be in the ratio of the number of lamps lighted at one time. The consumer who uses a few lamps for many hours should be charged at a less rate per unit in view of the smaller capital expenditure which his supply involves. The late Dr. Hopkinson advocated a system which takes account of this con- sideration in arriving at the fair price to be charged for current. In the system in question, now known as the ‘ Maximum Demand System,’ the total quantity of electricity consumed in six months is measured in the usual way, and the greatest rate at which the consumer has been taking current is also recorded. If the con- sumer in the six months’ period takes a smaller total than would correspond to one hour a day at the greatest rate of demand, he is charged the full price per unit, but if the total consumption exceeds this he is charged a reduced rate for each unit in excess. The system has been used with marked success in some seventy-two towns, It has improved the load factor, and has enabled a large number of additional units to be sold without increase of station plant or mains. Until the introduc- tion of Barker and Ewing’s Demand Indicator it was necessary to use two meters —one to record the total number of units taken by the consumer and the other to show his maximum rate of demand. The Barker and Ewing Indicator forms an integral part of the ordinary meter, and absorbs no energy; it further records watts and not amperes. With an alter- nating supply it shows actual watts and not apparent watts, an important difference in the case of motors andarc-lamps. It is not affected by any ordinary short circuit, its time lag being sufficient to prevent 1t coming into action. The Indicator may be used to show the actual rate of demand at any instant in place of recording the maximum rate of demand. In this form it is specially useful in switchboard instruments, showing the attendant the rate at which electric energy is passing through a feeder or is supplied from a dynamo at any instant. The meter also serves at the same time to integrate the total amount which has passed through that particular feeder or machine. 8. The Design and Location of Electric Generating Stations. By Aurrep H. Grssines, I Inst.£L. The term ‘central station’ is gradually being supplanted by more comprehen sive designations, All design and arrangement in regard to electric works must be with a view to securing the highest average efficiency together with reliability in operation. Electric works at present do not fulfil these conditions, but that may excusably be accounted for because it was impossible to foresee modern’ developments. Electricity, at first used for lighting only, has now come to be used in the form TRANSACTIONS OF SECTION G. 879 of electric motive power and electric traction. The attempt to supply all these from one generating station has led to the use of unsuitable plant, to confusion in the station itself, but at the same time to a reduction in prices charged. It has also resulted in a large variation in capital cost per kilowatt of plant. Small and isolated undertakings try to attain equally successful results by other experiments, but fail. Economical production is only possible where both the generating costs and the standing charges are reduced together as the load increases and the system extends. To effect this generating works must in future be constructed and located with a view to include the supply of energy for motive power, tramways, and electro-chemical purposes. Details of such construction and location should embody the following points :— (1) The machinery must be designed to generate at high voltage, differing according to the extent of the area and the nature of the system, but it must be suitable for transformation at sub-stations to meet all possible requirements. (2) The type of all boilers, engines, electric generators, switchboards, &c., must be simple and mechanically reliable, even at the sacrifice of some slight maximum economy. (3) All complicated gear and fanciful combinations, such as might lead to possible breakdown, must be avoided throughout the entire arrangement. (4) As far as possible the different units of the respective types of plant should be uniform in design and arrangement and made to one standard size, thus econo- mising in Jabour, avoiding large ‘ stand-by’ plant and spare gear, (5) The buildings should be devoid of all unnecessary embellishments, nor should an attempt be made to confine too many departments under one roof. (6) The location should be such as to ensure a cheap and ready supply and delivery of fuel, and where condensing can be accomplished efficiently and inexpensively. TUESDAY, SEPTEMBER 11, The following Report and Papers were read :— 1. Report on Small Screw Gauges. See Reports, p. 436. 2. On Screw Threads used in Cycle Construction, and for Screws subject to Vibration. By O. P. CLements. The Chairman of the Screw Gauge Committee of this Association has honoured me by the request that I would contribute a short paper on screw threads which, in my experience, have proved to be the most suitable for use in cycle construction and for screws that are subject to vibration. In complying with this request I propose to confine myself chiefly to the consideration of what is of most importance in this connection, namely. the shape of the threads. The time limit allowed for this paper would be inadequate for dealing exhaustively with such matters as pitch in relation to diameters, interchangeability, and gauging. In my opinion it would be impossible to devise a standard thread suitable for all classes of work and the various conditions of use. At present there are not only standard threads differing so much in shape as the Whitworth and the American, but also a large number of bastard threads, differing in shape from either of these, and which have been adopted in most instances as a matter of expediency and necessity. A too slavish use of a standard thread has no doubt often been the cause of much mischief and inconvenience in its adaptation to purposes jor which it was unsuitable. » When Sir Joseph Whitworth framed his system of threads and pitches he had not at his command the superior quality of steel for the manufacture of screws which we have in the present day. If he had, I venture to think that his system would have been somewhat modified both in shape of thread and in pitch. 880 REPORT—1900, I think that the correctness of these views cannot be better demonstrated than by showing what is the general practice and experience with regard to screws used in the gun trade. In both sporting guns and military rifles the screws are subject to severe vibration as well as sudden strains, and ure therefore extremely liable to work loose. To obviate this the gunmaker uses a thread with a well rounded top, and care is taken that the whole of the thread fits well, but more especially the top of the thread, where the frictional contact on the greatest circumferential portion of the screw will prevent loosening. We have thus a thread that differs from any recognised standard. It is shallow, with a large angle of the sides generally about 60°, and is admirably suited for the purpose of resisting vibration. I will now refer toa shape of thread which merits consideration, namely, flat- topped threads, which are very suitable for many purposes. It is also a shape of thread to which most accurate gauges can be made ; but while admitting their un- doubted suitability for gauge making, I must remark that gauges for threads with rounded tops can also be made satisfactorily, for all practical purposes, both as regards size and form, and so as to be perfectly reversible. Such gauge making, however, certainly requires a skill and experience which can be attained in but few tool shops. The flat-topped thread can be most accurately formed with a single tool on the ordinary screw-cutting lathes, or on machines having a leading screw or former. The tool can be easily ground to correct shape, and so as to have the cutting clearance which is necessary for the durability of the tool and for the production of clean and accurate work. There are, however, serious objections to the adoption of suck a thread for screws used in cycle work, and for screws subject to vibration. It is certain that the flat-topped thread cannot give the frictional resistance to vibration which is the case with the round top; and in the economical production of such work it would be very difficult to maintain the correct shape of the thread. In this production, screwing dies are chiefly used, and these tools show the first and most rapid wear on the parts forming the sharp edges or corners of the thread. For this reason it will be found a serious matter to keep up the screwing tackle, male and female, in the proper working condition necessary to produce flat-topped threads, especially if they should have a small angle of the sides. I am regarding this matter from the commercial point of view, that is, the production of work in quantities to be profitable and accurate, so far as . accuracy is commercially possible. In my experience the most favourable shape of thread for production with screwing dies and taps is a shallow thread with a large angle of the sides. This will give the best cutting clearance in the screwing tools. All the faults and errors in screw threads, and the difficulties in manufacture, can generally be traced to the bad cutting clearance in screwing dies and taps for high threads with small angles of the sides. Thus, through the strain put on the sides of such threads, there is a liability to breakage of the threads on the screwing dies and taps, and it also causes the screw to elongate and produces a fewer number of threads to the inch than standard pitch requires. This pitch error is a most serious fault, as the strain which should be distributed over all the threads is often taken by only one or two of them. Owing to the rapid wear of dies and taps with a bad cutting clearance, a faulty shape of thread is produced, especialiy at the sides of the thread. The angle of the male thread is often different from that of the female thread, and, in such case, the bearing surface at the sides of the thread is, of course, con- siderably reduced. This fault is especially serious in long-sided threads. The spreading or elongation of the thread is another matter which I may here refer to, [t is found necessary in tapping holes to drill or reamev the hole larger “than the bottom of the thread on the male screw. In the process of tapping, the thread elongates so as to fill the cavities between the threads and the tap, and upon the completion of the operation the hole will be found to be considerably smaller than when the tap was first inserted. This elongation also occurs in the male thread, but to a less degree, and if proper allowance for it is neglected, TRANSACTIONS OF SECTION G. 881 ripping of the threads will be caused. Much depends, also, on the material to be operated upon. In mild steel the elongation is more than in hard steel ; in brass and gun metal rather more than in mild steel; and in cast iron it is considerably less than in either of the other metals mentioned. Further, in threads with a small angle of the sides it is considerably more than in those having a large angle. The screws used in cycle construction are subject to even more continuous vibration than gun screws, but owing also to the low margin of safety in cycle work, it has been found necessary to use shallow threads, so as to give the greatest possible strength to the core, and to obtain a large angle of the sides of thread, which especially is important, as a large number of parts are har- dened, and therefore the greatest possible strength of thread is necessary. While a few firms use the Whitworth thread exclusively, others use a shallow thread, as before described, in a portion of their component parts, with Whitworth ‘threads in the remainder. With the exception of two instances, as will be seen from the attached list, the shallow thread is adopted throughout for B.S.A. cycle components. Time, however, will not permit me to give the reasons why a different thread is used in the two exceptions, but they illustrate the necessity which sometimes arises for the adoption of a different thread to suit altered conditions. The ‘B.S.A.’ thread is now extensively adopted as a standard in the cycle trade, and although the B.S.A. Company make all their own screws, the screw manufacturers to the trade have found it necessary to make the ‘B.S.A.’ standard a staple article of their trade, and tool makers have also now a marketable article in taps, dies, and chasers for the ‘B.S.A.’ thread. The illustration which was exhibited gave the section of the ‘ B.S.A.’ thread,and for comparison also sections of the British Association, the Whitworth, and the Seller threads. A list of the diameters, pitches, &c., of the screws used in the ‘BS.A? cycle components was also given. It is to be noted that the angle of the ‘B.S A’ thread is 60°, with tops and bottoms rounded to a radius of one-sixth of the pitch, and this is practically the shape of the thread used for the screws of the Lee-Enfield Magazine Rifle, which is manufactured for Her Majesty’s Government by the B.S.A. Company. 3. Lhe Photographic Method of preparing Teatile Designs. By Professor Roperts Beaumont, II.Mech.E., Yorkshire College, Leeds. The preparation of designs for the loom has, throughout the history of weaving, been regarded as a purely manual process controlled by the intelligence, ingenuity, and skill of the craftsman. It is only natural, therefore, that the invention of apparatus for this specific purpose should have created much interest amongst both British and foreign textile experts. Photography, as understood and practised, appeared as incapable of aiding the artist in the actual painting of his picture as the designer in the transference and execution of the plain sketch of the pattern on to the ‘scale’ paper for the loom. Within the wide range of technical and scientific data in the construction and embellishment of woven fabrics there is, perhaps, no phase of the work more difficult to assail, by mechanical devices, than the application and adjustment of the manifold ‘ weave’ units which compose all figured textiles. Design acquired in the loom is a distinct type of ornamentation involved in. varied technicalities, It is not the result. of one but of a number of processes, over- lapping each other, and yet uniting to construct and perfect the same woven effect. Fabric and design have to be simultaneously obtained. These can only be divorced by resorting to the arts of printing, embroidery, and painting. Obviously, in the preparation of the‘ design ’ sketch for weaving, numerous limitations have to be encountered, whicb, on a first consideration. seem liuble to be increased rather than diminished by a photographic process of design-development. Much ingenuity has been exercised by Szczepanik in his solution of these ‘weave’ problems. Szezepanik’s apparatus is not for the origination of designs either in the 1900, ; 3L §82 REPORT—1 900. theoretical or technical form, for in both processes the knowledge of the expert is demanded ; but its province is to lessen, and, in some instances, dispense with, the monotonous manual labour necessitated by the present system. There are large areas of point paper in elaborate designs to which the same weave effect has to be applied, and where some labour-saving device is much needed, Further, in the enlargement of the artist’s sketch to scale there is much mechanical work that it ought to be possible to reduce. The photographic inventions of Szczepanik profess to accomplish these objects, and the designs submitted prove that there are possibilities of success in certain styles of pattern. A new field for experiment has been discovered, the extent of which it is not possible to forecast, but it may reasonably be anticipated that the genius and temerity of the discoverer will prove equal to its more complete exploration. The essential purpose of Szczepanik’s invention is to develop from the ordinary sketch and enlarge to a prescribed scale the technically prepared design, marked with the thousands, or may be millions, of dots grouped in different orders and so fitted together as to impart precise definition to the several portions of the woven figure or design. ‘The process is threefold, consisting (1) of the preparation of the ruled paper; (2) the development of the design from an ordinary photographic negative ; and (3) the application of the weave units to the several parts of the figure. Primarily the apparatus consists of an optical lantern with a suitable arrangement of lenses. One important factor is the ‘raster’ or multiplying plate, containing some 435,600 perforations, through each of which the weave type passes, and is printed on the enlarged design. In addition there are weave-plates for determin- ing the details of the pattern, and small metal slides for producing particular sections in distinct forms of type, so that they may be as readily distinguished from each other as if sketched in various colours. The light from the lantern passes through the negative of the design, entering a pair of lenses between which is fixed the small metal plate of the proper shape for developing the marks on the sensitised paper. The process consists in dividing and subdividing the ‘scale’ pattern into rectangular spaces, and of marking each with the correct weave type. When there is no negative in the lantern this type is repeated as many times as there are holes in the ‘raster, showing the feasibility of marking every square photographically on any kind of weaver’s paper. Tn the first place, the negative is made of the complete design, and all parts erased but the ground sections, allowing of these being printed with their supple- mentary weave elements. Negatives of every part of the pattern are similarly printed in succession until the entire design has been obtained. For the production of shaded work, e.g. portraits and pictorial subjects, selecting plates are employed. These secure an accurate graduation of tones perfectly in harmony with the photograph from which they are derived. Provision is made for the execution of patterns in compound as well as in single structure fabrics ; but it follows, the more complex the build of the texture, the more intricate the process of design produc- tion. Certain textile designs may evidently be produced photographically by the Szezepanik system, so that it is now a question for demonstration whether designs so produced are comparable in legibility and equal for all practical purposes—as forcible in detail, as vital in execution—to those prepared by the much slower hand method, 4. Shop Buildings. By E. R, Cuarx, M.Lnst.C.£. 5. The Internal Architecture of Steel. By Professor ARNOLD. 6. A New Form of Calorimeter for measuring the Wetness of Steam. By Professor J. GOODMAN. TRANSACTIONS OF SECTION G, 883 7. On the Reheating of Compressed Air. By Wituiam Georce Waker, 4.IL00.£., MIME. Considerable economy can be obtained by reheating compressed air before admitting it to the engine. Reheating is accomplished by two methods :— 1. By passing the air through hot pipes heated by a furnace fire. 2. By pasaing the compressed air through water in a boiler at a temperature depending on the pressure in the boiler. The author and Mr. P. Y. Alexander have investigated these methods. Generally speaking, the results show that an additional horse-power can be obtained with an expenditure of one pound of coal, which is more efficient than the most economical engine and boiler using steam. The experiments show that in many cases it would prove advantageous to use compressed air in conjunction with steam in an ordinary engine. 312 884 REPORT—1900. Section H.—ANTHROPOLOGY. PRESIDENT OF THE SECTION—Professor Joun Ruys, M,.A,, LL.D. THURSDAY, SEPTEMBER 6. The President delivered the following Address:— Prruars I ought to begin by apologising for my conspicuous lack of qualifica- tion to fill this ckair, but I prefer, with your permission, to dismiss that as a subject far too large for me to dispose of this morning. So I would beg to call your attention back fora moment to the excellent address given to this Section Jast year. It was full of practical suggestions which are well worth recalling: one was as to the project of a Bureau of Ethnology for Greater Britain, and the other turned on the desirability of founding an Imperial Institution to represent our vast Colonial Empire. I mention these things in the hope that we shall not leave the Government and others concerned any peace till we have realised those modest dreams of enlightenment. People’s minds are just now so full of other things that the interests of knowledge and science are in no little danger of being overlooked. So it is all the more desirable that the British Association, as our great parliament of science, should take the necessary steps to prevent that happening, and to keep steadily before the public the duties which a great and composite nation like ours owes to the world and to humanity, whether civilised or savage. The difficulties of the position of the president of this Section arise in a great measure from the vastness of the field of research which the Science of Man covers. He is, therefore, constrained to limit his attention as a rule to some small corner of it; and, with the audacity of ignorance, I have selected that which might be labelled the early ethnology of the British Isles, but I propose to approach it only along the precarious paths of folklore and philology, because I know no other. Here, however, comes a personal difficulty: at any rate I suppose I ought to pretend that I feel it a difficulty, namely, that I have committed myself to publicity on that subject already. But as a matter of fact, 1 can hardly bring myself to confess to any such feeling; and this leads me to mention in passing the change of attitude which I have lived to notice in the ease of students in my position. Most of us here present have known men who, when they had once printed their views on their favourite subjects of study, stuck to those views through thick and thin, or at most limited themselves to changing the place of a comma here and there, or replacing an occasional and by a but. The work had then been made perfect, and not a few great questions affecting no inconsiderable portions of the universe had been for ever set at rest. That was briefly the process of getting ready for posterity, but one of its disadvantages was that those who adopted it had to waste a good deal of time in the daily practice of the art of fencing and winning verbal victories ; for, metaphorically speaking, ‘With many a whack and many a bang Rough crabtree and old iron rane. TRANSACTIONS OF SECTION H. 885 Now all that, however amusing it may have been, has been changed, and what now happens is somewhat as follows: AB makes an experiment or propounds what he calls a working hypothesis; but no sooner has AB done so than CD, who is engaged in the same sort of research, proceeds to improve on AB. This, instead of impelling AB to rush after CD with all kinds of epithets, and insinuating that his character is deficient in all the ordinary virtues of a man and a brother, only makes him go to work again and see whether he cannot improve on CD's results; and most likely he succeeds, for one discovery leads to another. So we have the spectacle not infrequently of a man illustrating the truth of the poet’s belief, ‘That men may rise on stepping-stones Of their dead selves to higher things.’ It is a severe discipline in which all display of feeling is considered bad form. Of course every now and then a spirit of the ruder kind discards the rules of the game and attracts attention by having public fits of bad temper ; but generally speaking the rivalry goes on quietly enough to the verge of monotony, with the net result that the stock of knowledge is increased. I may be told, however, that while this kind of exercise may be agreeable to the ass who writes, it is not conducive to the safety of the publisher’s chickens. To that it might suffice to answer that the publisher is usually one who is well able to take good care of his chickens; but, seriously, what it would probably mean is, that in the matter of the more pro- gressive branches of study, smaller editions of the books dealing with them would be required, but a more frequent issue of improved editions of them or else new books altogether, a state of things to which the publisher would probably find ways of adapting himself without loss of profit, And after all, the interests of know- ledge must be reckoned uppermost. It is needless to say that I have in view only a class of books which literary men proper do not admit to be literature at all; and the book trade has one of its mainstays, beyond all doubt, in books of pure litera- ture, which are like the angels that neither marry nor give in marriage: they go on for ever in their serene singleness of purpose to charm and chasten the reader's mind, My predecessor last year alluded to an Oxford don said to have given it as his conviction, that anthropology rests on a foundation of romance. I have no notion who that Oxford don may have been, but I am well aware that Oxford dons have sometimes a knack of using very striking language. In this case, however, I should be inclined to share to a certain extent that Oxford don’s regard for romance, holding as I do that the facts of history are not the only facts deserving of careful study by the anthropologist. There are also the facts of fiction, and to some of those I would now call your attention. Recently, in putting together a volume on Welsh folklore, I had to try to classify and analyse in my mind the stories which have been current in Wales about the fairies. Now the mass of folklore about the fairies is of various origins. Thus with them have been more or less inseparably confounded certain divinities or demons, especially various kinds of beings associated with the rivers and lakes of the country. They are creations introduced from the workshop of the imagination; then there is the dead ancestor, who also seems to have contributed his share to the sum total of our notions about the Little People. In far the greater number of cases, however, we seem to have something historical, or, at any rate, something which may be contemplated as historical, The key to the fairy idea is that there once was a real race of people to whom all kinds of attributes, possible and impossible, have been given in the course of uncounted centuries of story-telling by races endowed with a lively imagination. When the mortal midwife has been fetched to attend on a fairy mother in a fairy palace, she is handed an ointment which she is to apply to the fairy baby’s eyes, at the same time that she is gravely warned not to touch her own eyes with it. Of course any one can foresee that when she is engaged in applying the ointment to the young fairy’s eyes one of her own eyes is certain to itch and have the benefit of the forbidden salve. When this happens the midwife has two very 886 REPORT—1900, different views of her surroundings: with the untouched eye she sees that she is in the finest and grandest place that she has ever beheld in her life, and there she can see the lady on whom she is attending reposing on a bed, while with the anointed eye she perceives how she is lying on a bundle of rushes and withered ferns in a large cave, with big stones all round her and a little fire in one corner, and she also discovers that the woman is a girl who has once been her servant. Like the midwife we have also to exercise a sort of double vision, if we are to understand the fairies and see through the stories about them. An instance will explain what I mean: Fairy women are pretty generally represented as fascinating to the last degree and gorgeously dressed: that is how they appear through the glamour in which they move and have their being. On the other hand, not only are some tribes of some fairies described as ugly, but fairy children when left as changelings are pictured invariably as repulsive urchins of a sallow complexion and mostly deformed about the feet and legs: there we have the real fairy with the glamour taken off and a certain amount of depreciatory exaggeration put on. Now when one approaches the fairy question in this kind of way, one is forced, it strikes me, to conclude that the fairies, as a real people, consisted of a short, stumpy, swarthy race, which made its habitations underground or otherwise cunningly concealed. They were hunters, probably, and fishermen; at any rate they were not tillers of the ground or eaters of bread. Most likely they had some of the domestic animals and lived mainly on milk and the produce of the chase, together with what they got by stealing. They seem to have practised the art of spinning, though they do not appear to have thought much of clothing. They had no tools or implements made of metal. They had probably a language of their own, which would imply a time when they understood no other and explain why, when they came to a town to do their marketing, they laid down the exact money without uttering a syllable to anybody by way of bargaining for their purchases. They counted by fives and only dealt in the simplest of numbers. They were inordinately fond of music and dancing. They had a marvellously quick sense of hearing, and they were consummate thieves: but their thieving was not systematically resented, as their visits were held to bring luck and prosperity. More powerful races generally feared them as formidable magicians who knew the future and could cause or cure disease as they pleased. The fairies took pains to conceal their names no less than their abodes, and when the name happened to be Giscovered by strangers the bearer of it usually lost heart and considered himself beaten. Their family relations were of the lowest order: they not only reckoned no fathers, but it may be that, like certain Australian savages recently described by Spencer and Gillen, they had no notion of paternity at all. The stage of civilisation in which fatherhood is of little or no account has left evidence of itself in Celtic literature, as I shall show presently; but the other and lower stage anterior to the idea of fatherhood at all comes into sight only in certain bits of folklore, both Welsh and Irish, to the effect that the fairies were all women and girls. Where could such an idea have originated? Only, it seems to me, among @ race once on a level with the native Australians to whom I have alluded, and of whom Frazer of ‘the Golden Bough’ wrote as follows in last year’s ‘ Fort- nightly Review:’ ‘Thus, in the opinion of these savages, every conception is what we are wont to call an immaculate conception, being brought about by the entrance into the mother of a spirit, apart from any contact with the other sex. Students of folklore have long been familiar with the notions of this sort occurring in the stories of the birth of miraculous personages, but this is the first case on record of a tribe who believe in immaculate conception as the sole cause of the birth of every human being who comes into the world. A people so ignorant of the most elementary of natural processes may well rank at the very bottom of the savage scale.’ Those are Dr. Frazer’s words, and for a people in that stage of ignorance to have imagined a race all women seems logical and natural enough— but for no other, The direct conclusion, however, to be drawn from this argu- ment is that some race—possibly more than one—which has contributed to the folklore about our fairies, has passed through the stage of ignorance just indicated ; TRANSACTIONS OF SECTION H. 887 but as an indirect inference one would probably be right in supposing this race to bave been no other than the very primitive one which has been exaggerated into fairies. At the same time it must be admitted that they could not have been singular always in this respect among the nations of antiquity, as is amply proved by the prevalence of legends about virgin mothers, to whom Frazer alludes, not to mention certain wild stories such as some of those recorded by the naturalist Pliny concerning certain kinds of animals. Some help to make out the real history of the Little People may be derived from the names given them, of which the most common in Welsh is that of y Tylwyth Teg or the Fair Family. But the word cor, ‘a dwarf, feminine corres, is also applied to them ; and in Breton we have the same word with such deriva. tives as horrik, ‘a fairy, a wee little wizard or sorcerer,’ with a feminine korrigan or korrigez, analogously meaning a she-fairy or a diminutive witch. From cor we have in Welsh the name of a people called the Corannians figuring in a story in the fourteenth-century manuscript of the Red Book of Hergest. There one learns that the Corannians were such consummate magicians that they could hear every word that reached the wind, as it is put; so they could not be harmed. ‘The name Corannians of those fairies has suggested to Welsh writers a similar explanation of the name of a real people of ancient Britain. I refer to the Coritani, whom Ptolemy located, roughly speaking, between the river Trent and Norfolk, assigning to them the two towns of Lindum, Lincoln, and Rate, supposed to have been approximately where Leicester now stands. It looks as if all invaders from the Continent had avoided the coast from Norfolk up to the neighbourhood of the Humber, for the good reason, probably, that it afforded very few inviting landing- places. So here presumably the ancient inhabitants may have survived in suffi- cient numbers to have been called by their neighbours of a different race ‘the dwarls’ or Coritani, as late as Ptolemy’s time in the second century. This harmonises with the fact that the Coritani are not mentioned as doing anything, all political initiative having long before probably passed out of their hands into those of a more powerful race. How far inland the Coritanian territory extended it is impossible to say, but it may have embraced the northern half of North- amptonshire, where we have a place-name Pytchley, from an earlier Pihtes léa, meaning ‘ The Pict’s Meadow,’ or else the meadow of a man called Pict. At all events, their country took in the fen district containing Croyland, where towards the end of the seventh century St. Guthlac set up his cell on the side of an ancient tumulus and was disturbed by demons that talked Welsh. Certain portions of the Coritanian country offered, as one may infer, special advantages as a home for retreating nationalities: witness as late as the eleventh century the resistance offered by Hereward in the Isle of Ely to the Norman Conqueror and his mail- clad warriors. In reasoning backwards from the stories about the Little People to a race in somé respects on a level with Australian savages, we come probably in contact with one of the very earliest populations of these islands, It is needless to say that we have no data to ascertain how long that occupation may have been uncontested, if at all, or what progress was made in the course of it: perhaps archeology will be able some day to help us to form a guess on that subject. But the question more immediately pressing for answer is, with what race outside Wales may one compare or identify the ancient stock caricatured in Welsh fairy tales? Now, in the lowlands of Scotland, together with the Orkneys and Shet- lands, the place of our fairies is to some extent taken by the Picts, or, as they are there colloquially called, ‘the Pechts.’ My information about the Pechts comes mostly from recent writings on the subject by Mr. David MacRitchie, of Edinburgh, from whom one learns, among other things, that certain underground— or partially underground—habitations in Scotland are ascribed to the Pechts. Now one kind of these Pechts’ dwellings appear from the outside like hillocks covered with grass, so as presumably not to attract attention, an object which was further helped by making the entrance very low and as inconspicuous as possible. But one of the most remarkable things about them is the fact that the cells or apartments into which they are divided are frequently so small that their inmates 888 REPORT—1900. must have been of very short stature, like our Welsh fairies. Thus, though there appears to be no reason for regarding the northern Picts themselves as an under- sized race, there must have been a people of that description in their country. Perhaps archeologists may succeed in classifying the ancient habitatious in the WWorth accordingly: that is, to tell us what class of them were built by the Picts aod what by the Little People whom they may be supposed to have found in posses- sion of that part of our island. In Ireland and the Highlands of Scotland the fairies derive their more usual appellations from a word sid or sith (genitive side), which may perhaps be akin to the Latin sédes and have meant a seat, settlement, or station; but whatever its exact meaning may have originally been, it came to be applied to the hillocks or mounds within which the Little People made their abodes. Thus des Side as a name for the fairies may be rendered by mound people or hill folk; fer side, ‘a fairy man,’ by a mound man; and den side by a mound woman or banshee. They were also called simply sfde, which would seem to be an adjective closely allied with the simpler word sid. But to leave this question of their names, let me direct your attention for a moment to one of the most famous kings of the fairies of ancient Erin: he was called Mider of Bri Léith, said to be a hill to the west of Ardagh, in the present county of Longford. There he had his mound, to which he once carried the queen of Eochaid Airem, monarch of Ireland. It was some time before Eochaid could discover what had become of her, and he ordered Dalan, his druid, to find it out. So the druid, when he had been unsuccessiul for a whole year, prepared four twigs of yew and wrote on them in Ogam. Then it was revealed to him through his keys of seership and through the Ogam writing, that the queen was in the sid of Bri Léith, having been taken thither by Mider. By this we are probably to understand that the druid sent forth the Ogam twigs as letters of enquiry to other druids in different parts of the country ; but in any case he was at last successful, and his king hurried at the head of an army to Bri Léith, where they began in earnest to demolish Mider’s mound. At this Mider was so frightened that he sent the queen forth to her husband, who then departed, leaving the fairies to digest their wrath; for it is characteristic cf them that they did not fight, but bided their time for revenge, which in this case did not come till long after Eochaid’s day. Now, with regard to the fairy king, one is not told, so far as I can call to mind, that he was a dwarf, but the dwarfs were not far off; for we read of an Irish satirist who is represented as notorious for his stinginess, and who, to emphasise the description of his inhospitable habits, is said to have taken from Mider three of his dwarfs and stationed them around his own house, in order that their truculent looks and rude words might repel any of the men of Erin who might come seeking hospita- lity or bringing any other inconvenient request. The word used for dwarf in this story is corr, which is usually the Irish for a crane or heron, but here, and in some other instances, which I cannot now discuss, it seems to have been identical with the Brythonic cor, ‘a dwarf.’ It is remarkable, moreover, that the réle assigned to the three Irish corrs is much the same as that of the dwarf of Edern son of Nudd, in the Welsh story of Geraint and Enid and Chrétien de Troies’ Erec, which characterises him as fel et de put’eire, ‘treacherous and of an evil kind.’ By way of summarising these notes on the Mound Folk I may say that I should regard them as isolated and wretched remnants of a widely spread race possessing no political significance whatsoever. But, with the inconsistency characteristic of everything connected with the fairies, one has on the other hand to admit, that this strange people seems to have exercised on the Celts—probably on other races as well—a sort of permanent spell of mysteriousness and awe stretching to the verge of adoration. In fact, Irish literature states that the pagan tribes of Erin before the advent of St. Patrick used to worship the séde or the fairies. Lastly the Celt’s faculty of exaggeration, combined with his incapacity to comprehend the weird and uncanny population of the mounds and caves of his country, has enabled him, in one way or another, to bequeath to the great litera~ tures of Western Europe a motley train of dwarfs and little people, a whole world of wizardry, and a vast wealth of utopianism, If you subtracted from English TRANSACTIONS OF SECTION H. 889 literature, for example, all that has been contributed to its vast stores from this native source, you would find that you left a wide and unwelcome void. But the question must present itself sooner or later, with what race outside these islands we are to compare or identify our mound-dwellers. Iam not pre- pared to answer, and I am disposed to ask our archzeologists what they think. In the meantime, however, I may say that there are several considerations which would impel me to think of the Lapps of the North of Europe. But even supposing an identity of origin could be made out as between our ancient mound-inhabiting race and the Lapps, which, I am told, is craniologically impossible, it would remain still doubtful whether we could expect any linguistic help from Lapland, The Lapps now speak a language belonging to the Ugro-Finnic family, but the Lapps are not of the same race as the Finns; so it is possible that the Lapps have adopted a Finnish language and that they did so too late for their present language to help us with regard to any of our linguistic difficulties. One of these lies in our topography: take for instance only the names of our rivers and brooks—there is probably no county in the kingdom that would be too small to supply a dozen or two which would baffle the cleverest Aryan etymologist you could invite to explain them; and why? Because they belong in all probability to a non-Celtic, non-Aryan language of some race that had early possession of our islands. Never- theless it is very desirable that we should have full lists of such names, so as to see which of them recur and where. It is a subject deserving the attention of this Section of the British Association, We have now loitered long enough in the gloom of the Pecht’s house: let us leave the glamour of the fairies and see whether any other race has had a footing in these islands before the coming of the Celts. In August 1891 Professor Sayce and I spent some fine days together in Kerry and other parts of the south-west of Treland. He was then full of his visits to North Africa, and he repeatedly assured me that, if a number of Berbers from the mountains had been transferred to a village in Kerry and clad as Irishmen, he would not have been able to tell them by their looks from native Irishmen such as we saw in the course of our excursions. This seemed to me at the time all the more remarkable as his reference was to fairly tall, blue-eyed persons whose hair was rather brown than black. Evidence to the same effect might now be cited in detail from Professor Haddon and his friends’ researches among the population of the Arran Islands in Galway Bay. Such is one side of the question which I have in my mind: the other side consists of the fact that the Celtic languages of to-day have been subjected to some dis- turbing influence which has made their syntax unlike that of the other Aryan languages. I have long been of opinion that the racial interpretation of that fact must be, that the Celts of our islands have assimilated another race using a language of its own in which the syntactical peculiarities of Neo-Celtic had their origin: in fact that some such race clothed its idioms in the vocabulary which it acquired from the Celts. The problem then was to correlate those two facts. I am happy to say this has now been undertaken from the language point of view by Professor J. Morris Jones, of the University College of North Wales. The results have been made public in a book on The Welsh People recently published by Mr. Fisher Unwin. The paper is entitled ‘Pre-Celtic Syntax in Insular Celtic,’ and the languages which have therein been compared with Celtic are old Egyptian and certain dialects of Berber. It is all so recent that we have as yet had no criticism, but the reasoning is so sound and the arguments are of so cumulative a nature, that I see no reason to anticipate that the professor’s conclusions are in any danger of being overthrown. At the close of his linguistic argument, Professor Morris Jones quotes a French authority to the effect, that, when a Berber king dies or is deposed, which seems to happen often enough, it is not his son that is called to succeed him, but the son of his sister, as appears to have been usual among certain ancient peoples of this country; but of this more anon. In the next place my attention has been called by Professor Sayce to the fact that ancient Egyptian monuments represent the Libyans of North Africa with their bodies tattooed, and that even now some of the Touaregs and Kabyles do the same, These indications help one to group 890 REPORT—1900. the ancient peoples of the British Isles to whose influence we are to ascribe the non-Aryan features of Neo-Celtic. In the first place one cannot avoid fixing on the Picts, who were so called because of their habit of tattooing themselves. For as to that fact there seems to be no room for doubt, and Mr. Nicholson justly lays stress on the testimony of the Greek historian Herodian, who lived in the time of Severus, and wrote about the latter’s expedition against the natives of North Britain a long time before the term Picti appears in literature. For Herodian, after saying that they went naked, writes about them to the following effect : ‘They puncture their bodies with coloured designs and the figures of ani- mals of all kinds, and it is for this reason that they do not wear clothes, lest one should not behold the designs on their bodies,’ This is borne out by the names by which the Picts have been known to the Celts. That of Pict is itself in point, and I shall have something to say of it presently ; but one of the other names was in Irish Cruzthni, and in Welsh we have its etymological equivalent in Prydyn or Prydain. These vocables are derived respectively from Irish eruwth and Welsh pryd, both meaning shape, form, or figure, and it is an old surmise that the Picts were called by those names in allusion to the animal forms pricked on their bodies, as described by Herodian and others. The earlier attested of these two names may be said to be Prydyn or Prydain, which the Welsh used to give in the Middle Ages to the Picts and the Pictland of the North, while the term Ynys Prydain was retained for Great Britain as a whole, the literal meaning being the Island of the Picts: that is the only name which we have in Welsh to this day for this island in which we live— Ynys Prydain, ‘The Picts’ Island.’ Now one detects this word Prydain in effect in the Greek Hperamxal Njoo given collectively to all the British Isles by ancient authors. it may be rendered the Pictish Islands, but a confusion seems to have set in pretty early with the name of the Brittanni or Brittones of South Britain: that is to say, Pretanic, ‘ Pictish,’ became Brittannic or British ; and this is, historically speaking, the only known justification we have for includ- ing Ireland in the comprehensive term ‘The British Isles,’ to which Irishmen are sometimes found jocularly to object. In the next place may be mentioned the Tuatha Dé Danann of Irish legend, who cannot always be distinguished from the Picts, as pointed out by Mr. MacRitchie. The tradition about them is, that, when they were overcome in war by Mil and his Milesians, they gave up their life above ground and retired into the hills like the fairies, a story of little more value than that of the extermination of the Picts of Scotland. In both countries doubtless the more ancient race survived to amalgamate with its conquerors. There was probably some amount of amalgamation between the Tuatha Dé Danann or the Picts and the Little Moundsmen; but it is necessary not to confound them. The Tuatha shared with the Little People a great reputation for magic; but they differed from them in not being dwarfs or of a swarthy complexion: they are usually represented as fair. In the case of Mider, the fairy king, who comes in some respects near the description of the heroes of the Tuatha Dé Danann, it is to be noticed that he was & wizard, not a warrior. Guided by the kinship of the name of the Tuatha Dé Danann on the Irish side of the sea and that of the Sons of Dén on this side, 1 may mention that the Mabinogion place the Sons of Dén on the seaboard of North Wales, in what is now Carnarvonshire: more precisely their country was the region extending from the mountains to the sea, especially opposite Anglesey. In that district we have at least three great prehistoric sites all on the coast. First comes the great stronghold on the top of Penmaen Mawr; then we have the huge mound of Dinas Dinlle, eaten into at present by the sea south-west of the western mouth of the Menai Straits; and lastly there is the extensive fortification of Tre’r Ceiri, over- looking Dinlle from the heights of the Eifl. By its position Tre’r Ceiri belonged to the Sons of Dén, and by its name it seems to me to belong to the Picts, which comes, I believe, to the same thing. Now the name ‘lre’r Ceiri means the town of the Keiri, and the Welsh word ceirz is used in the district in the sense of persons who are boastful and ostentatious, especially in the matter of personal appearance and fine clothing. It is sometimes also confounded with cewri, TRANSACTIONS OF SECTION #. 891 ' piants,’ but in the name of Tre’r Ceiri it doubtless wafts down to us an echo of the personal conceit of the ancient Picts with their skins tattooed with decorative Pictures ; and Welsh literature supplies a parallel to the name Ynys Prydain in one which is found written Ynys y Ceti, both of which may be rendered equally the Island of the Picts, but more literally perhaps some such rendering as ‘ the Island. of the Fine Men’ would more nearly hit the mark. Lastly, with the Sons of Don must probably be classed the other peoples of the Mabinogion, such as the families of Llyr, and of Pwyll and Rhiannon. All these peoples of Britain and Ireland were warlike, and such, so far as one can see, that the Celts, who arrived later, might with them form one mixed people with a mixed language, such as Professor Morris Jones has been helping to account for. Let us now see for a moment how what we read of the state of society implied in the stories of the Mabinogion will fit into the hypothesis which I have roughly sketched. In the first place I ought to explain that the four stories of the Mabinogion were probably put together originally in the Goidelic of Wales, before they assumed a Brythonic dress. Further, in the form in which we know them, they have passed through the hands of a scribe or editor living in Norman times, who does not always appear to have understood the text on which he was operating. To make out, therefore, what the original Mabinogion meant, one has every now and then to read, so to say, between the lines. Let us take for example the Mabinogi called after Branwen, daughter of Llyr. She was sister to Bran, king of Prydain, and to Manawyddan, his brother: she was given to wife to an Irish king named Matholwch, by whom she had a son called Gwern. In Ireland, however, she was, after a time disgraced, and served in somewhat the same way as the heroine of the Gudrun Lay; but in the course of the time which she spent in a menial position, doing the baking for the Court and having a box on the ear administered to her daily by the cook, she succeeded in rearing a starling, which one day carried a letter from her to her brother Bran at Harlech. When the latter realised his sister’s position of disgrace, he headed an expedition to Ireland, whereupon Matholwch tried to appease him by making a concession, which was, that he should deliver his kingdom to the boy Gwern. Now the question is, wherein did the concession consist ? The redactor of the Mabinogi could, seemingly, not have answered, and he has not made it the easier for any one else to answer. In the first place, instead of calling Gwern son of Matholwch, he should have called him Gwern son of Branwen, after his mother, for the key to the sense is, that, in a society which reckoned birth alone, Gwern was not recog- nised as any relation to Matholwch at all, whereas, being Bran’s sister’s son, he was Bran’s rightful heir. No such idea, however, was present to the mind of a twelfth-century scribe, nor could it be expected. Let us now turn to Irish literature, to wit, to one of the many stories associated with the hero Ciichulainn. He belonged to Ulster, and whatever other race may have been in that part of Ireland, there were Picts there : as a matter of fact Pictish communities survived there in historical times. Now Citichulainn was not wholly of the same race as the Ultonians around him, for he and his father are sharply marked off from all the other Ultonians as being free from the periodical illness connected with what has been called the couvade, to which the other adult braves of Ulster succumbed for a time every year. Then I may mention that Ctichulainn’s baby name was Setanta Beg, or the Little Setantian, which points to the country whence Ctichulainn’s father had probably come, namely the district where Ptolemy mentions a harbour of the Setantii, somewhere near the mouth of the Ribble, in what is now Lancashire. At the time alluded to in the story I have in view, Ctichulainn was young and single, but he was even then a great warrior, and the ladies of Ulster readily fell in love with him; so one day the nobles of that country met to consider what was to be done, and they agreed that Cuchulainn would cause them less anxiety if they could find him a woman who should be his fitting and special consort. At the same time also that they feared he might die young, they were desirous that he should leave an heir, ‘ for,’ as it is put in the story, ‘ they knew that it was from himself his rebirth would be,’ 892 REPoRT 1900. The Ulster men had a belief, you see, in the return of the heroes of previous generations to be born again ; but we have here also two social systems face to face. According to the one to which Ctchulainn as a Celt belonged, it was requisite that he should be the father of recognised offspring, for it was only in the person of one of them or of their descendants that he was to be expected back. The story reads as if the distinction was exceptional, and as if the prevailing state of things was wives more or less in common, with descent reckoned according to birth alone. Such is my impression of the picture of the society forming the background to the state of things implied by the conversation attributed to the noblemen of Ulster. Here again one experiences difficulties arising from the fact, that the stories have been built up in the form in which we know them by men who worked from the Christian point of view; and it is only by scrutinising, as it were, the chinks and cracks that you can faintly realise what the original structure was like. Among other aids to that end one must reckon the instances of men being designated with the help of the mother’s name, not the father’s: witness that of the king of Ulster in Ctichulainn’s time, namely Conchobar mac Nessa, that is to say, Conor, son of a mother named Nessa; similarly in Wales with Gwydion son of Dén. Further we have the help of a considerable number of ancient inscrip- tions, roughly guessed to date from the fifth or the sixth century of our era, and commemorating persons traced back to a family group of the kind, perhaps, which Ceesar mentions in the fourteenth chapter of his fifth book. Within these groups the wives were, according to him, in common (7nter se communes). Take for instance an inscription from the barony of Corcaguiny in Kerry, whick com- memorates a man described as ‘ Mac. Erce, son of Muco Dovvinias, where Muco Dovvinias meaus the clan or family group of Dovvinis or Dubin (genitive Ducbne), the ancestress after whom Corcaguiny is called Corco-Duibne in Medieval Irish. We have the same formula in the rest of Ireland, including Ulster, where as yet very few Ogams have been found at all. It occurs in South Wales and in Devonshire, and also on the Ogam stone found at Silchester in Hampshire. The same kind of family group is evidenced also by an inscription at St. Ninian’s, in Galloway; and, to go further back—perhaps a good deal further back—we come to the bronze discovered not long ago at Colchester, and dating from the time of the Emperor Alexander Severus, who reigned from 222 to 235, This is a votive tablet to a god Mars Medocius, by a Caledonian Pict, who gives his name as Lossio Veda, and describes himself further as Nepos Vepogeni Caledc. He alludes to no father, and Nepos Vepogeni is probably to be rendered Vepogen’s sister’s son, At any rate, the Irish word corresponding etymologically to the Latin nepos has that sense in Irish; and, so far as I know, it has never been found meaning a nephew in the sense of brother’s son. That may serve as an instance how the ideas of another race penetrated the fabric of Goidelic society ; for here we must suppose a time to have come when there was no longer any occasion for a word meaning & brother’s son, which, of course, there never was in the non-Celtic society which ranked men and women according to their birth alone. Now this Caledonian Pict was not exceptional among his kinsmen, for they suc- ceeded in observing a good deal of silence concerning their fathers down, one may say, to the 12th century. It is historical that the king of the northern Picts was not wont to be the son of the previous king, In short, when the Celtic elements there proved strong enough to ensure that the son of a previous king should succeed, a split usually took place, the purer Picts being led by the rule of succession by birth to set up a king of their own. The fact is not so well known that the same succession prevailed also some time or other at Tara in Ireland; it is proved by a singular piece of indirect evidence, the existence of a tragic story to explain why ‘no son should ever take the lordship of Tara after his father, unless some one came between them.’ The last clause is due, I should say, to somebody who could not understand such a prohibition based on the ancient rule that a man’s heir was his sister’s son, This would be, according to Irish legend, in the lifetime of Conor mac Nessa. It is curious to notice hew the stories about the Pictish ménage seem to have TRANSACTIONS OF SECTION H, 898 puzzled ancient authors. I will cite only one instance, to wit, from Golding’s 16th century translation of what then passed as the production of Solinus, and what may pass now, even according to Mommsen, as quite old enough for my present purpose. It runs thus: ‘ Next come the [les called Hebudes, five in number, the inhabiters whereof know not what corne meaneth, but liue onely by fishe and milke. They are all vnder the gouernment of one King, For as manie of them as bee, they are seuered but with a narrowe groope one from another. The King hath nothing of hys own, but taketh of euery mans. He is bounde to equitie by certaine lawes: and least he may start from right through couetousnesse, he learneth Justice by pouertie, as who may have nothing proper or peculiar to himselfe, but is found at the charges of the Realme. Hee is not suffered to haue anie woman to himselfe, but whomsoeuer he hath minde ynto, he borroweth her for a tyme, and so others by turnes, Wherby it commeth to passe that he hath neither desire nor hope of issue.’ The man who wrote in that way presumably failed to see that the king was not subject to any special hardship as compared with the other men in his kingdom, where none of them had any offspring that he could individually call his own. This, be it noticed, refers to the Hebrides, not, as sometimes happens with such references, to the more distant island of Thule, where there was also a king, as any reader of Faust will tell us. We now come to the Celts, and begin with Pliny’s version of Czsar's words about the division of Gaul into three parts, as follows: Gallia omnis Comata uno nomine appellata in tria populorum genera dividitur, amnibus maaxime distincta. A Scalde ad Sequanam Belgica, ab coad Garunnam Celtica eademque Lugdunensis, inde ad Pyrenei montis excursum Aquitanica, Aremorica antea dicta. We may for the present dismiss the third or Aquitanic Gaul from our minds; but Belgic and Celtican Gaul may be taken as representing the two sets of Celts of our own islands. The Belgic Gauls began last to come to this country, and their advent seems to fall between the visits of Pytheas and Julius Cxsar: that is, roughly speaking, between the middle of the fourth century and that of the first century B.c. In this country they came to be known collectively as Brittanni or Brittones, the linguistic ancestors of the peoples who have spoken Brythonic or the Lingua Brittannica, such as the Welsh, the Cornish, and the Strathclyde Britons. As to the other Celts, it is much harder to say when or whence exactly they came—lI mean the linguistic ancestors of the Gaels of Ireland, Man, and Scotland, that is to say, the peoples whose language has been Goidelic. Some scholars are of opinion that there were no Goidelic-speaking peoples in Britain till some such came here from Ireland on sundry occasions, beginning with the second century, in the time of the Roman occupation ; but how the Goidels would be supposed by them to have reached Ireland I do not exactly know. My own notion is that the bulk of them reached that country by way of Britain, and that they arrived in Britain, like the Belgic Gauls later, from the nearest parts of the Continent; for this would be previous to the appearance of the Belgic Gauls on the western sea- board of Europe: that is to say, at a time when Celtica extended not merely to the Seine, but to the Scheldt or to the Rhine, if not even further. Then as to the time of the coming of the ancestors of the Goidels, it has been supposed coincident with a period of great movements among the Celts of the Continent, in particular the movements which resulted, among other things, in some of them reaching the shores of the Mediterranean and penetrating to the heart of the Iberic peninsula. Perhaps one would not be far wrong in fixing on the seventh and the sixth seniuries B.C. as covering the time of the coming of the earlier Celts to our ores. In Britain I should suppose these earlier hordes of Celts to have conquered most of the southern half of the island; and the Brythonic Celts, when they arrived, may have overrun much the same area, pushing the Goidelic Celts more and more towaids the west. Under that pressure it is natural to suppose that some of the latter made their way to Ireland, but it is quite possible that their emigration thither had begun before. Some time or other previous to the Roman occupation the Brythonic people of the Ordovices seem to have penetrated to the 894 REPORT—1900. sea between the rivers Dovey and Mawddach, displacing probably some Goidels who may have gone to the opposite coasts of Ireland; but in Ivish story more traces appear of invasions on the part of the Dumnonii, who possessed the coast between Galloway and Argyle. These were so situated as to be able to assail Treland both in front and from behind, and this is countenanced to some extent by Irish topography, not to mention the long legends extant as to great wars in the west of Ireland between the Tuatha Dé Danann and invaders including the Fir Womnann. I suspect also that it was the country of these northern Dumnonians which was originally meant by Lochlinn, a name interpreted later to mean Norway. Such are some of the faint traces of the Goidelic invasions of Ireland from Britain, but it is possible—perhaps probable—that Ireland received settlers on its southern coast from the north-west of Gaul at a comparatively late period, at the time, let us say, when Czesar was engaged in crushing the Veneti and the Aremoric League. This has been suggested to me by the name of the Usdie, which probably survives in the first syllable of Ossory, denoting a tract of country now, roughly speaking, covered by the county of Kilkenny, but which may have been considerably larger before the Déisi took possession of the baronies of the two Decies and other districts now constituting the county of Waterford, not to mention possible encroachments on the part of Munster on a boundary which seems to have been sometimes contested. Now the Continental name which invites comparison with that of the Usdiz is that of the Ostizi, who in the time of Pytheas appear to have occupied the north-western end of what afterwards came to be called Brittany; they were also called Ostiones, and more commonly Osismi, I see no reason to suppose that the ships of the Aremoric League could not make the voyage from Brittany to the principal landing-places on the south of Tveland from the Harbour of Cork to that of Waterford, and I gather from Ptolemy’s Geography that Ireland was relatively better known on the Continent than Britain, although the latter had in a manner been long connected with the Roman world. This I should explain somewhat as follows:—Czsar, who knew very little about the west of Britain and less about Ireland, says that in his time the great druidic centre of Gaul was in the country of the Carnutes, somewhere, let us say, near the site of the present town of Chartres, that druidism had been introduced from Britain to Gaul, and that those who wished to understand it had to go to Britain to study. The authors of antiquity tell us otherwise nothing about druids in Britain except that Tacitus speaks of such in the Annals, in his well-known passage as to Suetonius Paulinus landing with his troops in Anglesey and the scene of slaughter which ensued. Indeed, one may go further and say that there is no proof that any Belgic or Brythonic people ever had druids: they belonged to the Celtican Gauls and the Goidelicising Celts of Britain and Ireland, who had probably accepted the institution from the Pictish race. At any rate it is significant that the Life of St. Columba intro- duces the reader to a genuine druid at the court of the Pictish king, near Inver- ness, where, as well as on Loch Ness, the sainthad to contend with him. In any case, it is highly probable that druidism was no less a living institution in Ireland than in the Goidelic and Pictish parts of Britain. Presumably it was more so, and it may be conjectured that Gaulish students of druidism visited Ireland no less than Britain; also, vice versa, that Irish druids paid visits to the Celtican part of Gaul where druidism flourished on the Continent, and in a word that there was regular intercourse between Gaul and the south of Treland. If the druids of Ireland, who, among other roles, played that of schoolmasters and teachers in that country, travelled to Celtica, they must have spread on the Continent some information about their native country, while generations of them cannot have returned to Ireland, with their druidic pupils, without bringing with them some of the arts of civilised life as understood in Gaul: among these one must rank very decidedly the art of writing, which the druids practised. Now you know the usual account given of the ordinary Latin for Ireland, namely Hibernia—to wit, that it was suggested by such native names as that of one of the greatest tribes of that country, namely the “Iovepvoe TRANSACTIONS OF SECTION H. 895 or Iverni, and that it had its v ousted when Latin began about the 4th century to write 6 for v, and that an % was then prefixed to make the word Hibernia properly connote the wintry climate which our sister island had always been supposed to enjoy. But now comes the question, where did Pom- ponius Mela, who flourished about the middle of the first century, get his Luverna, which Juvenal also used? Doubtless from a druid like Dalan, or some other educated native of Ireland; for what the editors print as Iuverna, Luuerna, or Juverna, would appear in ancient manuscripts as IVVERNA or duuerna, in which the first two syllables are spelt correctly with vv according to a system of spelling well known in Ogmic writing centuries later. But a parti- cular system of spelling seems to me to imply writing, and thus one is encouraged to think that the Ogam alphabet may have been invented no later than the first century, in the intercourse I have conjectured to have been going on between the north-west of Gaul and the south of Ireland, where the majority of Ogam inscriptions are now found. But what has archzology to say on the question of such intercourse ? After this digression I come back to the two main streams of Ceitie immigra- tion, from the same parts of the Continent in two different periods of time. he later of these introduced the Lingua Brittannica, which was practically a dialect of old Gaulish ; but the affinities of the other Celtic language of these islands, the Goidelic, are not so easy to determine. I have long thought that I can identify traces of it on the Continent, and that its principal home was in the region which Pliny called Celtica, between the Garonne and the Seine. I ven- tured accordingly to call it Celtican, asthe simpler word Celtic had already been wedded to a wider signification. Since I did so the existence of that language has been placed beyond doubt by the discovery of fragments of a calendar engraved on bronze tablets. This find was made about the end of 1897 at a place called Coligny, in the department of the Ain, and the pieces are now in the museum at Lyons. It is difficult to say for certain whether Coligny is within the territory once occupied by the Sequani, or else by the Ambarri, a people subject to the Mdui, who were the rivals of the Sequani and Arverni. The name of the Sequani would seem to have belonged to the Celtican language, and Mr. Nicholson, in his interpretation of the calendar, has ventured in this instance to call it Sequanian. But two inscriptions in what appears to be the same language have come to light also at a place called Rom,in the Deux Sévres and on the Roman road from Poitiers to Saintes. This Celtican language is to be carefully distinguished from Gaulish, but it is not exactly what I expected it to be: it is better. For several of the phonetic changes characteristic of Goidelic had not taken place in Celtican. Among other things it preserves intact the Aryan consonant p, which has since mostly disappeared in Goidelic, as it had even then in Gaulish. This greater conservatism of Celtican enables one to refer to it the national appellation of the people of the region in question, namely that of the Pictones, from which it is impossible to sever the name of the Picts of Britain and Ireland, who are found also called Pictones and Pictanez. Here I may mention that Mr. Nicholson calls attention to instances of tattooing on some of the faces on ancient coins belonging to Poitou and other parts of western France. In the light of the names here in question one sees that pictos was a Celtican word of the same etymology, and approximately, doubtless, of the same meaning, as the Latin word pictus, that the Celticans had applied it at an early date to the Picts on account of their habit of tattooing themselves, and that the Picts had accepted it (with its derivative Pictones) so generally that by the time when the Norsemen arrived in the North of Scotland, it was the name which the natives gave them as that by which they called themselves. That is practically proved by the Norsemen calling Caithness and Sutherland Petta-land or the Land of the Picts, and the sea washing its northern shore Pettalunds fiorth, which survives modified into Pentland Firth. Another Celtican word of great interest here has by a mere chance come down in a High German manuscript written before the year 814: itis Chortonicum, and it occurs among a number of geographical names, several of which refer to Gaul, 896 REPORT—1900. so that Chortonicum may very well have meant the country of the Pictones. At all events, the great German philologist Pott at once saw that it was to be ex- plained by reference to the word Cruithne, ‘a Pict,’ with which it decidedly goes as distinguished from its Brythonic equivalent Prydyn (or the older Priten) with an initial p. The Celtican form originally meant was some such vocable as Qurtonico-n, with the gu which was usual in Celtican and early Goidelic, where it formed, in fact, one of the most conspicuous distinctions between those languages and Brythonic or Gaulish, in which gu had been changed into p. My remarks have again run into tiresome details, but it is only by attending to such small points that one can hope to force language to yield us any information in the matter of ethnology. It may perhaps help in some measure if I sum up what I have been trying to say, thus: The first race we have found in possession of the British Isles consisted of a small swarthy population of mound-dwellers, of an unwarlike disposition, much given to magic and wizardry, and living underground: its attributes have been exaggerated or otherwise distorted in the evolution of the Little People of our fairy tales. The next race consisted of a blue-eyed people, taller and blonder, who tattooed themselves and fought battles. These tattooed or Pictish people made the Mound Folk their slaves, and in the long run their language may be supposed to have been modified by habits of speech introduced by those slaves of theirs from their own idiom. ‘The affinities of these Picts may he called Libyan, and possibly Iberian. Next came the Celts in two great waves of immigration, the first of which may have arrived as early as the 7th century before our era, and consisted of the real ancestors of some of our Goidels of the Milesian stock, and the linguistic ancestors of all the peoples who have spoken Goidelic. That language may be defined as Celtican so modified by the idioms of the population, which the earlier Celts found in possession, that its syntax is no longer Aryan. Then, about the third century B.c., came from Belgica the linguistic ancestors of the peoples who have spoken Brythonic; but most of our modern Brythons are to be regarded as descended from Goidels who adopted Brythonic speech, and in so doing brought into that language their Goidelic idioms, with the result that the syntax of insular Brythonic is no less non-Aryan than that of Goidelic, as may be readily seen by comparing the thoroughly Aryan structure of the few sentences of old Gaulish extant. Those are the races which have been inferred in the course of these remarks, in which I have proceeded on the principle that each successive band of conquerors has its race, language, and institutions eventually more or less modified by contact with the race, language, and institutions of those whom it has conquered. That looks simple enough when stated so, but the result which we get proves com- plicate. At all events I have endeavoured to substitute for the rabble of divinities and demons, of fairies and phantoms that disport themselves at large in Celtic legend, a possible succession of peoples, to each of which should be ascribed its own proper attributes. But that will only be possible if we can enlist the kindly aid of the Muse of Archeology. The following Papers and Reports were read :— 1. Some Implements of the Natives of Tasmania. By J. Paxton Morr. The author gives an account of diggings in native camping grounds in Tasmania, and of the rude underground stone implements found there, comprising hand-axes, skinning knives, &c., and especially certain tools of finer make, concave scrapers, and groovers. TRANSACTIONS OF SECTION H. 897 2. The Stone Age in Tasmania as related to the History of Civilisation. By E. B. Tytor, /.RS. This paper, with special reference to the previous one, discussed the Paleolithic, or unground Stone Age in Tasmania, which lasted till superseded by the English colonisation early in this century, passing directly into the Iron Age without the intervention of a Neolithic, or ground Stone Age, 3, Report on Mental and Physical Deviations of Children in Schools, See Reports, p. 461, 4, Report on the Sulchester Hxcavation.—See Reports, p. 466, 5. Writing in Prehistoric Greece. By Antuur J. Evans, U.4., F.S.A (1) Clay Documents with Hieroglyphic or Conventionalised Pictographie Script from the Palace of Knossos. The discovery originally announced by the author in 1894, in this Section,’ of the existence in prehistoric Crete of a system of conventionalised pictographic or hieroglyphic writing had received an extraordinary corroboration and supplement from his recent excavations in the Mycenzan Palace of Knossos. ‘The first indica- tions had been supplied by groups of signs engraved on early seal-stones, and by its nature the evidence was limited. But in the great prehistoric building now par- tially explored at Knossos, the latest elements of which can hardly be brought down later than the thirteenth century 3B.c., there came to light a series of deposits of clay archives inscribed both with hieroglyphic and a new system of linear writing. Those of the hieroglyphic class, though apparently contemporary with the other, were less numerous and were found in a separate magazine. They were in the form of square and three-sided bars, perforated at the end, clay ‘labels’ also perforated, in shape like bivalve shells, and sealings of clay which also presented impressions of signets with characters of the same conventionalised pictographic class. The graflito characters of the clay bars, &c., gave more linearised versions of the fuller representations of the engraved seals, and thus illustrated a step in the formation of letters. The tablets showed various new forms of hieroglyphs not as yet found on the signets, raising the Cretan series to over a hundred. ‘The picto- graphic signs might be said to form an illustrated history of Oretan culture in Mycenzan times. Among new characters might be mentioned an eight-stringed lyre, carpenter's tools such as a kind of plane and perhaps a level, dogs’ heads, bees, a glove-like object perhaps not unconnected with bee-keeping, and appa- rently olive sprays. The obviously ‘ ideographic’ or ‘determinative’ character of some of the hieroglyphs gives a clue to the meaning of many of the tablets. Ships, ploughs and ox-heads, vessels filled with grain, and the Egyptian palace sign speak for themselves. A boustrophédon arrangement of the characters is often traceable. Many of these clay records are accounts, as is shown by the presence of various numeral signs, the ciphers never exceeding eight in a group. But the form of numeration still presents points of obscurity. The hieroglyphic script itself shows a certain parallelism with the ‘ Hittite? inscriptions of Anatolia and Northern Syria. Its beginnings can, however, be traced very far back on Cretan soil, and it unquestionably represents the writing of the indigenous Cretan stock, the Eteocretans of the ‘ Odyssey,’ 1 Report Brit. Assoc. (Oxford), 1894, p. 776. 1900, OM 898 REPORT—1900, (2) Clay Documents inscribed with Linear Script from the Palace of Knossos. The great bulk of the clay records discovered in the Palace of Knossos exhibited a linear style of writing fundamentally different from that of the hieroglyphic class, and far ahead of it in development. The tablets are for the most part elongated slips of hand-moulded clay, from two to about seven inches in length, and from half an inch to three inches broad ; others, however, are of a squarer form. They present some distant analogy to the Babylonian tablets, and the inscription is divided by horizontal lines. The letters themselves, however, are of a free, upright European character. Some seventy characters seem to have been in common use, and of them about ten show resemblances to the later Greek and the same number to the Cypriote syllabary. About the same number of forms are also common to the hieroglyphic Cretan series. The letters seem to have been for the most part syllabic ; lines of division appear between the words, and the writing runs consist- ently from left to right. The pictorial origin of these letters may be traced in some cases. Thus, we have the human head and neck, the hand, the crossed arms, a bird flying, three or four barred gates, a fence, a high-backed throne, a tree, and a leaf. A certain number are unquestionably ideographic or determinative. Others represent measures and quantities, and are always associated with numerals. A good many of these documents evidently refer to Palace accounts, and a clue to the general purport of the tablet is often supplied by the introduction of a pictorial figure. We thus find chariots and horses, human figures, perhaps slaves, axes, ingots, vases of precious metals, others of clay for various liquids, houses or barns, swine, ears of corn, various kinds of trees and a crocus-like flower, perhaps used for a dye or perfume. A decimal system of numeration was employed, somewhat resembling the Egyptian, The value theoretically arrived at by the author for the numerals was Bere by an addition sum presented by one tablet, the total of which worked out correctly, The ingots depicted on the tablets resembled a Mycenzean copper ingot from Cyprus and others from Sardinia, They were followed by a balance (the Greek talanton) and numerals apparently indicating their value in Mycenzan gold talents. It has thus been possible to make an approximate calculation of their weight. Objects in precious metals represented were identical with some typical tributary offerings of the Keft chieftains on the Theban monuments of Thothmes IIT.’s time, and tended to show that some of these clay documents went back to the first half of the fifteenth century B.c. Other tablets, without ciphers or pictorial figures, perhaps refer to contracts or correspondence, such as the contemporary records of Syria and Babylonia. The tablets had been originally contained in coffers of wood, clay, and gypsum, and these in turn secured by clay seals bearing impressions of Mycenzean engraved gems of the finest style. These impressions had in many cases been countermarked with a graffito sign by the controlling official while the clay was still wet, and the back of the clay seal was at the same time endorsed and countersigned with short inscriptions in the same script as that of the tablets. Such legal precautions were quite worthy of the ‘Palace of Minos.’ These discoveries not only carry back the existence of written documents on Greek soil some seven centuries before the first known monuments of Greek writing, and five before the earliest Phoenician, but they afford a wholly new standpoint for investigating the origin of the alphabet. The letter-forms borrowed by the Greeks from the Phcenicians seem to have been influenced by these pre-existing Aigean scripts. The common elements existing in the Phoenician alphabet itself are very noteworthy. Out of twenty-two original letters, some twelve present obvious points of comparison with characters belonging to one or other of the two Cretan scripts, and to these at least four may be added as showing possible affinities. In view of such parallelism, which extends to the meaning as well as the form of the signs, De Rougé’s theory of the derivation of the Phoenician letters from remote hieratic Egyptian prototypes must be definitely abandoned, The Phcenician, and with it the Greek, alphabet must ‘TRANSACTIONS OF SEOTION H. 899 be regarded as a selection from a syllabary belonging to the same generic group as the Cretan. Such a phenomenon on the Syrian coast is perhaps explained by the settlement there in Mycenzean times of an A‘gean island race, the Philistines, whose name survives in that of Palestine. Though later Semitised, their biblical names of Kaphtorim and Kerethim, or Cretans, sufficiently record their Algean origin, 6. On the System of Writing in Ancient Egypt. By F. Lt. Grirvitd, Egyptology has now reached a position among the sciences from which it may contribute trustworthy information for the benefit of kindred researches. Egyptian writing consists of Ideographic and Phonetic Elements, the signs serving as —1, Word-signs ; 2, Phonograms; 3, Determinatives. The highest development shown is an alphabet, which, however, is never used independently of other signs: it is apparently not acrophonic in origin; it represents consonants and semi- consonants only, vocalisation not being recorded by Egyptian writing. No advance can be detected in the system from the beginning of the historic period to the end, notwithstanding some improvements in practical working which facilitated the uss of cursive writing. Phonograms derived from word-signs. The end of the native system was brought about by the gradual adoption of the Greek character —heginning, perhaps, in the second century a.p. If any radical improvement was ever made in the Egyptian form of writing that improvement must have taken place at or after adoption by another people: eg., some have supposed that our alphabet was derived by the Phoenicians from Egypt; but any such derivations are at present entirely hypothetical. Although the Egyptian system of writing may not be actually a stage in the history of our alphabet, it throws a strong light on the development of the alphabetic system; and the survival of its pictorial form (for decorative purposes) enables us to recognise the highly ramified connections between the forms and meanings of characters to an extent which is impossible at present in any other system, whether in Mesopotamia, China, or elsewhere. Results of recent Egyptian philology : Egyptian originally a Semitic language, though its character changed early. The main lines of the grammar being at length established, the materials for a complete dictionary are now being collected and classified. 7. Interim Report on Anthropological Teaching. 8. Report on Anthropological Photographe.—See Reports, p. 568, PRIDAY, SHPTEMBER 7, The following Papet's were rend: — 1. The Cave of Psychro in Crete. By D. G. Hocarri. It has been known for some years that @ large cave above the village cf Psychré, in the Lasithi district of Crete, was a repository of primitive votive objects in bronze, terra-cotta, &c. As this cave is situated in the eastern flank of the mountain which dominates the site of ancient Lyttos, and is the only import- ant cave known in the neighbourhood, it was conjectured that it was the Lyttian grotto connected with the story of the birth of Zeus in the legend, whose earliest 3M 2 900 REPORT—1900, version is preser'ved by Hesiod. A thorough exploration of it, undertaken in May and June of the current year, by Mr. D. G. Hogarth, on behalf of the British School at Athens, aided by the Cretan Exploration Fund, has served fully to con- firm this view. ‘The cave is double. On the north is a shallow grotto, the upper part of which was cumbered with immense fallen frazments of the roof. The lower part contained deep black earth, partly ransacked by previous diggers. This was thoroughly dug out this year, and when the great blocks had been broken up with blasting powder and removed, the deposit on the higher slope was also searched. ‘The result was the discovery of a rude altar in the middle of the grotto, surrounded by strata of ashes, pottery, and other refuse, among which many votive objects in bronze, terra-cotta, iron, and bone were found, together with fragments of some thirty libation tables in stone, and an immense number of earthenware cups used for depositing offerings. The lowest part of the Upper Grotto was found to be enclosed by a wall partly of rude Cyclopean character, and partly rock-cut ; and within this Temenos the untouched strata of deposit ranged from the early Mycenzan Age up to the Geometric period of the ninth cen- tury B.c. or thereabout. Only very slight traces were found of later offerings. The earliest votive stratum belongs to the latest period of the pre-Mycenean Age, that marked by the transition between the ‘Kamaraes’ fabric of pottery and the earliest Mycensean lustre-painted ware. But below all isa thick bed of yellow clay, containing scraps of primitive hand-burnished black and brown pottery, mixed with bones of animals. This bed seems to be water-laid, and to be prior to the use of the cave as a sanctuary. Probably, when it was in process of formation, the cave was still a swallow-hole of the lake which once occupied the closed Lasithi basin; but before the Mycenzean period the present outlet had opened, and the plain was dry. The southern or Lower Grotto falls steeply for some 200 feet to a subterranean pool, out of which rises a forest of stalactite pillars. Traces of a rock-cut stairway remain. Much earth had been thrown down by the diggers of the Upper Grotto, and this was found full of small bronze objects. But chance revealed a more fruitful field, namely, the vertical chinks in the lowest stalactite pillars, a great many of which were found still to contain toy double axes, knife-blades, needles, and other objects in bronze, placed there by dedicators, as in niches. The mud also at the edge of the subterranean pool was rich in similar things, and in statu- ettes of two types, male and female, and engraved gems. These had probably been washed out of the niches. The knife-blades and simudacra of weapons are probably the offerings of men; the needles and depilatory tweezers of women. The frequent occurrence of the double axe, not only in bronze, but moulded or painted on pottery, found in the cave, leaves no doubt that its patron god was the ‘Carian’ Zeus of Labranda, or the Labyrinth, with whom perhaps his mother, the Nature goddess, was associated, and the statuettes probably represent the two deities. Here was the primitive scene of their legend, transferred in classical times to a cave on Mount Ida, 2. On the Japanese Gohei and the Ainw Inao. By W. G. Aston. The paper illustrates a principle in the history of religion by which the object which is at first simply an offering has a tendency to become conceived of as the embodiment of the God, or even as a distinct and independent deity. : In ancient Japan the offerings to the gods were of the most varied description. Among them were included hemp and bark fibre, together with cloth made from these materials. In later times there was substituted a small quantity of paper made of the same bark fibre and attached to a wand in the form known to us as gohei, With the change of form the original character of the gohei as offerings was forgotten. They were looked upon as receptacles or embodiments of the God, and honour was paid to them accordingly. At festivals the God descended into the gohet on a certain formula being pronounced by the priest. Hypnotic prac- titioners also used these objects in their séances, the deity who inspired them in TRANSACTIONS OF SECTION 4. 901 their trances being supposed to enter their body by this channel. There are cases in Japan in which the devotee has gone a step further, and has constituted the object, which was originally an offering, a distinct and independent deity. _ The Ainus of Yezo use in their worship whittled sticks called cnao, which have a general resemblance to an old form of the gohez, and are no doubt a cheaper substi- tute for them. The znao, like the gohet, are primarily offerings, but in certain cases they receive direct worship as gods, having become in short genuine fetishes. Another link between the inao and the gohei is provided by certain whittled sticks closely resembling znao which were in use in Northern Japan a century ago for striking women with in order to ensure fertility, as in the Roman Lupercalia. Similar sticks after consecration by the Shuite priests were formerly used at Kioto to kindle the household fire afresh on the new year, and so avert possible pestilence. 3. The Textile Patterns of the Sea-Dayaks. By Dr. A. C. Havpon, F.R.S. The Sea-Dayak women weave short cotton rep petticoats and cotton sleeping wraps which are covered with beautiful and oftenintricate patterns. The patterns are made in the following manner: the warp is stretched on a frame, the woman takes the first fifteen to thirty strands and ties them tightly with strips of leaves at irregular intervals, according to the design, which she carries in her memory. The next fifteen to thirty strands are similarly tied, and this process is repeated until all the threads have been utilised. The warp is then removed from the frame and dipped in a reddish dye, which colours the free portions of the warp, but the tied-up portions remain undyed ; thus a light pattern is left on a coloured back- ground, when the lashing is untied. Ifa three-colour design is required, as is usually the case, the first lashing is retained, and various portions of the previously dyed warp are tied up; the whole is immersed in a black dye, and then both sets of lashing are untied. The pattern is thus entirely produced in the warp, the woof is self-coloured, and does not obtrude itself in the material. There are a very large number of designs and patterns, which are remembered by the women and handed down from mother to daughter. By far the greater number of these designs are based upon animals, whereas most of the patterns carved by the men on wooden and bamboo objects are derived from plant motives. The designs embroidered by the women on jackets and loin-cloths are usually zoomorphic in character, but the treatment of the motives is quite different from the decoration of previously described fabrics. The decorative art of the Sea-~Dayaks of Sarawak differs in character from that of the Kayans, Kenyahs, and other inland tribes. 4, Relics of the Stone Age of Borneo. By Dr. A. C. Havpon, F.R.S. Until about eighteen months ago the only authentic example known in this country of a stone implement from Sarawak was the specimen collected by A. Hart Everett, which is now in the Pitt Rivers Collection at Oxford. In December, 1898, the Sarawak Museum obtained a specimen of a different type. I discovered a third type in a Sibop house on the Tinjar River in the Baram District of Sarawak ; later Dr. C. Hose, the Resident of the Baram District, obtained numerous examples from various interior tribes in his district; these he has generously presented to the University of Cambridge. The occurrence of stone implements in Borneo has been previously noted. _ The implements are made of various rocks, including fibrolite, impure sand- stone, arkose, silicified limestone, shale, andesite, and chalcedony. The form, too, varies greatly ; some are obviously axe heads, others adze blades, while certain cylindrical forms, with a more or less cup-shaped cutting end, were probably used to extract the pith from the sago palm. In the collection are several stones of irregular form; the former use of some of them is problematical, but they have recently been used as touchstones, 902 REPORT----1900. The natives have a high regard for these stone implements, which have in their eyes a sacred character, and it is very difficult to persuade their owners to part with them. In all cases fowls had to be sacrificed to appease the spirits. The implements are stored with other sacred objects, and most of them are believed ta be teeth, or toe-nails, of Baling Go, the Thunder God, 5. Houses and Family Life in Sarawak. By A. C. Hanpon, Se.D., PRS. The author exhibited a series of nearly fifty lantern slides taken during his recent expedition to Sarawak, which were selected to illustrate the type of house that is common among the settled inland tribes of Borneo and the every-day life of the people. No attempt was made to distinguish between the various tribes, as their mode of life is very similar in its main features. The villages are all situated on or close by the banks of rivers; most of the houses are of large size, and may con-' tain from half-a-dozen to sixty families. Sometimes a village consists of a single house or of a string of houses placed endwise to each other. A house is built on piles some ten to twenty feet from the ground. Along the side facing the river is a wide verandah, which stretches down the whole length of the house. Here many of the domestic industries are carried on, and all social and public business is transacted. The dwelling-rooms of each family open by a single door on to the verandah. While the common verandah affords every facility for social intercourse the privacy of the home is thoroughly respected. In the verandab of nearly every house is at Jeast one trophy of the skulls of enemies, which are supposed to bring good luck and plenteous harvests. Food is occasionally offered tc them, and a fire has to be kept burning beneath them, other- wise the skulls would be uncomfortable and bring misfortunes to the house. Various industries were illustrated by slides, such as the husking and winnowing of rice by the women. The houses are often ornamented with carvings or paintings of a conventional character, the style of decoration varying according to the tribe. SATURDAY, SEPTEMBER 8. The following Papers were read :— 1. On the Anthropology of West Yorkshire. By Joun Bepvor, JLD., LLD., F.R.S. The author discussed the question whether any considerable British or pre- Anglian element remained in the country around Bradford. Without coming to any positive conclusion, he was disposed to consider the inhabitants of these parts as mainly Anglian in type. More British blood remained further north, in Craven. A prevalent type about Leeds seemed to him to resemble the Burgundian Belair type of His and Riitimeyer. 2. On the Vagaries of the Kephalic Index. By Joun Beppog, MD, LL.D, FAS: Lhe communication is based on a description of two heads, both dolichoid in pattern, but of which the one, which was most distinctly so, gave a latitudinal index (living) of 82:3, owing to retarded ossification of the posterior part of the temporo-parietal suture. But for this the author thought the index would nog have exceeded 77 TRANSACTIONS OF SECTION H. 9038 3. On certain Markings on the Frontal Part of the Human Cranium, and their Significance. By A. Francis Dixon. An examination of the frontal region of the cranium shows that, in many cases, grooves or channels are present on the bone, corresponding to the branches of the supra-orbital nerves. These grooves vary very much in appearance, as they may be simple or branched, shallow or deeply cut. They are not infrequently converted in parts of their course into little tunnels. In some cases they are found on one side of the cranium only, in others they occur on both sides; their distribution is very rarely quite symmetrical. Most frequently the grooves occur beneath the outer branches of the supra-orbital nerve, but in many cases they are found beneath the inner branches. The grooves never pass from the frontal on to the parietal bone—across the coronal suture. They often extend upwards from the supra-orbital notch, or foramen, as far as the coronal suture; in other cases they begin inferiorly at a little foramen where some branch of the nerve enters the bone. The openings of these little foramina are directed upwards towards the coronal suture, just as the openings of the nutrient foramina in the long bones are directed towards the end of the bone where growth is most active and goes on longest. The presence of these grooves indicates a want in proportion between the growth in length of the nerves and the amount of expansion of the underlying part of the cranium. The nerves might be looked upon as constricting cords which become depressed in the developing bone as the cranium expands. The constricting portions of the nerves are often limited inferiorly at a point where some little branch enters the bone, and superiorly at the coronal suture, where the deep layers of scalp are firmly bound down to the cranium. Hence the grooves for the nerves do not cross the coronal suture and often begin inferiorly at little foramina whose openings are directed upwards. The grooves appear to indicate in the skulls in which they occur an excessive development of the frontal part of the cranial wall. In races in whom the grooves are common, and strongly marked, we would expect the presence of a tendency towards increased development and capacity of the frontal part of the cranium; while,on the other hand, in races in whom the grooves do not occur, or are rare, and but feebly marked, we would expect to find much uniformity in the shape and size of the cranium, indicating that none of its various parts are tending towards an increased develop- ment, In the purer races of mankind, with marked uniformity in the size and shape of their crania, we would look for the greatest harmony between the growth in length of the overlying structures and the amount of expansion of the various parts of the cranial wall; on the other hand, in mixed races we would be more likely to find individuals exhibiting a want of such correspondence in the amount of growth of the superficial and deeper structures. In this connection it is interesting to note that the frontal grooves are almost never found in Australian and Tasmanian skulls, that they are rare among Melanesians, slightly more common among Polynesians, while among Bushmen and Negroes, especially in Zulus and Kaffirs, they are very common, and often extraordinarily well marked. Among Negroes they are present in over 50 per cent. of the skulls examined. In the skulls obtained in the dissecting room they are present in about 41 per cent, of all cases. 4. On the Sacral Index. By Professor D, J. Cunnincuam, I/.D., F.R.S. Inasmuch as the true length of the sacral portion of the vertebral column is not indicated by the shortest distance between the apex and base of the sacrum, but rather by the length of the curve formed by the sacral vertebre, it is proposed that, in making measurements for the determination of a sacral index, ‘length’ should be measured by using a tape along the concavity of the sacral curve, and not by calipers, one limb of which is placed upon the base and the other on the apex of the sacrum, Breadth (measured by calipers in the ordinary manner) 904 REPORT—1900, multiplied by 100 and divided by length, measured in the manner indicated, gives the true sacral index. The curvature of the sacrum may be conveniently plotted by taking a tracing from a strip of soft metal which has been previously adapted by pressure to the front of the sacrum along its middle line. The index of curvature may he ex- pressed by the number derived by multiplying the height of this plotted curve by 100 and dividing by the number corresponding to the true length of the sacrum. 5. On the Microcephalic Brain. By Professor D. J. Cunnineuam, ILD., F.R.S. The brain of the microcephalic idiot may exhibit features which do not merely represent a ‘fixed’ embryonic condition. In one specimen the arrangement of the fissures and sulci is found to approach more closely the ape than the human type, and in almost every furrow some simian character can be detected. These simian characters must not be considered mere foetal conditions rendered per- manent. ‘The ape-like condition existing in this brain does not as a whole correspond to that of any one ape, or group of apes, but there is a complicated mixture of features some of which are characteristic of high apes, while others find a parallel in the brain of low apes. The microcephalic brain may be regarded as a partial ‘atavism.’ So far as its surface markings are concerned the specimen noted has reverted in part, or wholly, to an arrangement which, in all probability, existed in some early stem-form of man. 6. Developmental Changes in the Human Skeletcn from the Point of View of Anthropology. By Davip Waterston, I.D., PR.CSL. A series of specimens of the long bones of the extremities at different ages of embryonic and infantile life has been collected and examined. The methods employed in the examination were those of anthropometry, namely, osteometry and osteoscopy. By the former, the relative lengths of the bones of the limbs at different ages have been ascertained and compared one with another, and by the latter it has been found that these bones present some definite and interesting characters. Without going minutely into the rate of growth of each segment of the upper and lower limbs, the general character was shown, and the special features of the bones at different ages were demonstrated by means of lantern slides taken from photographs of the objects. An attempt has also been made to ascertain the cause of the special characters found in the bones by investigating the time of their appearance and of their replacement by adult characters. A comparison has also been instituted between the bones of the embryo and those of the lower races of mankind and of the higher apes, both as regards their relative length and their characters. ‘ As it has been shown that the curvature of the spine in the lumbar region is a post-natal development, and one adapted to the assumption of the erect attitude by the infant, it was shown that in a similar way the configuration of the bones of the lower extremity alters after birth, before the infant can stand erect. MONDAY, SEPTEMBER 10. The following Papers and Report were read :— 1. On the Imperfection of our Knowledge of the Black Races of the Trans- vaal and the Orange River Colony. By E. S. Harruann, £.S.A. Our information on the customs, institutions, and beliefs of the native races of the Transvaal and the Orange River Oolony is derived chiefly from fragmentary TRANSACTIONS OF SECTION H. 905 notices by missionaries, an! these are not to be implicitly trusted. The black peoples of South Africa are Bantus and Bushmen-Hottentots. Though there is a general similarity of custom among them all, there are also important differences, of which some examples are given. Inquiries made by the Cape Government. The difficulty experienced by Europeans, even when long resident among the natives and intimately acquainted with them, of understanding the real meaning of their institutions. The practice of dobola supplies a striking example of this difficulty. An accurate study of the native customs, institutions, and beliefs is an urgent necessity both for missionaries and for purposes of government. 2. On a Mould showing the Finger-prints of a Roman Sculptor of probably the Third Century. By Sir Witi1aM Turver, JLB., FBS. Sir Wm. Turner exhibited a plaster mould of a head, which had been modelled by a Roman sculptor in probably the third century A.D., on which the prints of the lines on the skin of the sculptor’s fingers had been preserved. The mould belonged to Mr. G. Allis, of the Roman House, Lincoln, who had obtained it during the excavation of the foundations of his house a few years ago, the site of which is within the area of a large building of Roman times, several of the columns of which are preserved in the basement of his house, 3. Report on the Canadian Ethnographic Survey.—See Reports, p. 468. 4. The Paganism of the Civilised Iroquois. By Davip Bortz, Curator of the Musewm, Toronto. Notwithstanding the contact of the Iroquois, or Six Nation Indians, with white people for more than three hundred years, a very considerable number of the former have retained many of their old-time beliefs, with the forms and ceremonies appertaining thereto. Of four thousand Caniengas (Mohawks), Senecas, Cayugas, Onondagas, Oneidas, and Tuscaroras now residing on the Grand Reserve, within sixty miles of Toronto, Ontario, fully one-fourth continue to observe the ancient feasts or dances connected with the growth and ingathering of corn and fruits, and for desired changes in weather, as well as for the cure of disease. Some modification in the ceremonies was made about a century ago by an Onondaga named Ska-ne-o-dy’-o, who announced himself as a prophet who had paid a visit to the abode of the Great Spirit. The changes introduced by him, however, have not by any means removed the pagan character of the native beliefs, although he certainly did attempt to imitate some Christian observances. Still, the addresses of the medicine men retain most of the old-time forms, although their significance in many cases is lost, and even the meaning of numerous words is no longer known. The leading idea in the present form of worship is that of a Great Spirit, but this has been acquired from missionary sources; and although the Indians have adopted the idea of a heaven, they do not believe in any hell. The quoted examples of petitions addressed to Rawen Niyoh (the Creator) illustrate the lack of assimilation of the old and néw forms. One of the most characteristic ceremonies connected with Iroquois paganism is that of the sacrifice or burning of the White Dog at the new year feast during the February moon, when the spirit of the dog, accompanied by offerings of tobacco, conveys to Niyoh information respecting the condition of his ‘own people’ on the Grand River Reserve. 906 REPORT—1900. 5, Notes on Malay Metal-work. By Water Rosennaln, B.A., St. John’s College, Cambridge ; 1851 Exhibition Commissioners’ Research Scholar, University of Melbourne. The paper dealt with some specimens of Malay metal-work submitted to the author for microscopic and other examination by Mr. W. W. Skeat. Some Malay processes actually witnessed by Mr. Skeat were described. and the bearings of the microscopic examination on the explanations of these processes are discussed. The first question dealt with is the production of the ‘damask’ pattern on a Malay kris. Mucrophotographs were given showing that the ‘damask iron’ really consists of layers of locsely welded’ wrought iron, the only other metal used being tool steel. ‘The body of the blade is made of steel, and a layer of laminated ‘damask iron’ is welded upon either side of the central layer of steel; a thin layer of steel is welded on outside the ‘damask iron.’ The author believes that the striated ‘damask’ effect is due to the opening of the loose welds in the damask iron during the forging of the blade, steel being driven between the lamine. The outside layer of steel is entirely ground away, and when the compound surface so produced is ‘etched’ by the pickling process employed, the more readily corroded steel is attacked, leaving the edges of the layers of iron as a series of narrow projecting ridges. The tools of the Malay goldsmith were next described, and the micro-structure and composition of Malay bronzes and ‘ white metal’ were described and discussed. The final section of the paper dealt with the Malay method of producing chains by casting. 6. Note on the ‘ Kingfisher’ Kriss. By Professor Henry Louis, JA. This note describes a peculiar pattern of kriss used in a limited area in the north-east of the Malay Peninsula. The Malay legend of its origin is that a party of Malays from the Bugis islands invaded this portion of the peninsula many centuries ago; one of their leaders was known as ‘the Kingfisher’ (pre- sumably on account of his rapid movements). The invasion was successful, but the leader fell in one of the last engagements. After his death his followers carved their kriss handles into shapes resembling the kingfisher’s head and beak. Under Chinese influence the pattern became more ornate, until it reached the present fixed type. The writer discovered in a pawnshop in Bangkok an earlier form of this type (possibly the only one extant): this kriss seems to have been sold by a Malay from this region, many of whom are well known to have been deported by the Siamese between the years 1790 and 1820. Colonies of their descendants still exist in Siam, and have been visited by the writer. The early type of ‘ King- fisher’ kriss is much more like the bird’s head than the modern pattern, which is, however, now the only one seen among or known to the Malays. The region in question has rarely been visited by Europeans. 7. On some Buddhist Sites. By W. Law Bros. The author exhibited a photograph of the temple erected on the spot where Buddha ‘ meditated’ A sample of the sacred ‘Bo’ tree was also shown. The delicate carvings in these temples were exhibited and explained. What was described as the ‘Tope’ was a characteristic development in Buddhist sacred buildings, and sometimes these ‘were treated with elaborate ornamentation. In addition to the sites a series of views showing the rock-caverns which enter so largely into Buddhist religious life were exhibited. These rock-caves contain specimens of the earliest Buddhist sculptures known. The author also showed views of a number of Jain temples which were among the most richly elaborate in ornamentation of all Indian sanctuaries, and also views of side-chapels and cloisters belonging to these temples, in nearly all of which the cross-legged figure of the Buddha was found, ‘ TRANSACTIONS OF SECTION H. 907 TUESDAY, SEPTEMBER 11, The following Papers and Report were read :— 1. On Permanent Skin-marks, Tattooing, Scarification, &c. By H. Line Ror. The author enumerated the various purposes for which these disfigurements were made. ‘T'hey were connected among other things with beliefs in the future life, it being supposed that without them one could not find his way about in the next world. They also served as charms for women at childbirth. The institution was really divisible into four divisions. The Tahitian method was the one commonly seen on our sailors. The New Zealand method, which was performed _ by a pricker, left behind a very deep mark in the skin, and was often performed so freely as to cover the whole skin. The West African and the Tasmanian methods differed from the preceding ones, and in the case of the last of these the marks develop into large continuous scars. They were all variations of skin deformations, but rubbed in, and they leave a permanent mark The author exhibited pictures of the various specimens of; hese different methods of tattooing, and accompanied them with pictures of the different instruments employed. The wounds made were frequently reopened in order to put in colouring juices, and owing to this they were a long time in healing, and left behind them permanent scars. 2. Some Peculiar Features of the Animal-cults of the Natives of Sarawak, and their Bearing on the Problems of Totemism. by Cuaries Hoss, D.Sc., Resident of the Baram District, and W. McDovueat., IA. We had observed customs that seemed to indicate the existence of a well- developed totemism, either at the present time or in recent times, among the natives of Sarawak. We have therefore collected information bearing on this subject as diligently as possible, from all the tribes with whom we have come into intimate contact. We found a great number and variety of peculiar rites and customs observed by the people of the different tribes in their dealings with animals and plants. We confine ourselves in this short paper (1) to giving a general account of the customs of one of the inland tribes, the Kenyahs; (2) to describing the ‘ Nyarong,’ or spirit-helper of the Sea-Dayaks, and some similar institutions among the other en and (8) to pointing out the bearing of our observations on the totem roblem. + The Kenyahs are a warlike agricultural people, living as isolated communi- ties of twenty to fifty or more families, each community inhabiting a single long house built on the river-bank. Their religion is peculiar, in that they helieve in a beneficent Supreme Being and a group of departmental deities, while they attri- bute to every agent that affects their lives a spirit that must be properly respected and, if necessary, propitiated. Most important to them of all the animals is the common white-headed hawk. He brings messages of warning and advice from the Supreme Being to those who know how to read the signs he gives, and he is consulted before every under- taking of importance, and sacrifices of fowls and pigs are made to him. A wooden image of the hawk stands before every house. Several other birds give them omens of lesser importance, and none of these may be killed or eaten. The domestic fowl is killed as a sacrifice to the hawk or other powers, and its blood is sprinkled on the altar-posts of the gods and on the persons taking part in various ceremonies, especially peace-making ceremonies. The domestic pig is sacrificed in much the same way. ‘The spirit of a pig is always charged with some prayer to be carried to the Supreme Being, and the answer is read from the markings of its liver. The crocodiles are regarded as a friendly and allied tribe, aad may be killed in 908 REPORT—1900. retaliation only, No Kenyah will kill a dog, and the dead body of a dog is re- garded with fear. Kenyahs will not eat the flesh of deer or horned cattle, and there are many restrictions on touching or using any parts of them. Only old or renowned warriors will wear or touch the skin of a tiger. One house is decorated with carvings of the gibbon on every large beam, and all Kenyahs have a dread of the Maias and the long-nosed monkey. There thus seems to be every degree of regard paid to the different beasts, from the mere uneasy feeling in the presence of the uncanny long-nosed monkey to the elaborate cult of the hawk, and the nature of the respect paid to any species seems in nearly every case to be the direct expression of the impression made on the barbarian’s mind by the behaviour of the beasts. The Spirit-Helper.—Every Sea-Dayak hopes to be guided and helped all through his life by a spirit which announces itself to him in dreams and takes up its abode in some peculiar natural object or in some animal. In the latter case the Dayak will never kill or eat one of the same species of animal, and will lay the same prohibition on all his descendants, so that a whole family may come to pay especial regard to one species of animal for many generations, A similar institution occurs, though less commonly, among the other tribes. In such cases we seem to be able to trace sometimes the actual origin and growth of a totem. 3, Report on the Ethnography of the Malay Peninsula. See Reports, p. 393. 4, On the Present State of our Knowledge of the Modern Population of Egypt. By D. Ranpari Mactver, JA. 5. Perforate Humeri in Ancient Egyptian Skeletons, By Professor A. Macauister, 2.8. In sorting out our Cambridge collection of Egyptian bones I have noted the frequency of supra-articular perforation of the humerus, especially in the bones from Libyan graves. I did not begin to count the number of examples until more than three-fourths of the series had been put away in store-cases, but out of the last twenty boxes opened I found that out of 682 humeri 390 were perforate and 292 imperforate. The percentage of perforation is therefore 57:2. This exceeds anything hitherto published. Of ancient North Americans the percentage of perforate bones out of 300 specimens is 40 percent. In one collection from the Gila Valley, in Arizona, 48 perforate bones were found out of 89, a per- centage of 53°9; but this is exceptionally high, and the number of bones is not large. In our Cambridge collection when I began to count I found out of the first 115 bones that 65 were perforated ; so, had I none but this series, the pereent- age would have come out 56°65. The Libyans may therefore, I think, claim to hold the record. In our dissect- ing-room there were three instances out of the last hundred bodies examined. te statistics will be found in Messrs. Matthews and Lamb’s article on the subject. The authors just quoted are most probably correct in considering this as an acquired character. The youngest specimen obtained was in a humerus of a child probably six yearsold. I have not seen any genuine approach to this condition among 100 foetal humeri examined for the purpose. As far as I know, it has never been found in a foetal bone. It is a perforation of the shaft well above the epiphysial junction line, The 1 Mem, Amer, National Acad, Sci., vi, 217, TRANSACTIONS OF SECTION H, 909 distal extremity of the diaphysis thickens below the hole down to the place where the epiphysis is set upon it. ‘ It is always in the intra-articular part of the olecranon fossa, below the line of reflexion of the synovial membrane that crosses the middle of the fossa. It is therefore quite distinct from the vascular holes with which Topinard associates it, as these are always extra-articular [the vessels are chiefly derived from the inferior profunda], ‘ Of these perforate humeri 172 were right and 218 were left. As far as could be determined from size, shape, and from the accompanying pelvic bones, 192 were male and 198 were female. There is thus the same preponderance of left and female over right and male bones which was noticed by the describers of the Hemenway Collection, leading one to speculate as to the nature of the work which predisposed to the perforation—the mill, the shadoof, or the mattock. As to the sizes of the holes, they were mostly oval or elliptical, with the long axis transverse or nearly so, and the distribution of their sizes is shown in the accompanying table :— Length of Mate. FEMALE. Long Axis 7 ia in mm, Right. Left. Right. Left. 1.4 17 9 12 10 5-9 54 58 52 63 10-12 14 37 22 39 Over 12 1 2 0 0 Total ; : 86 106 86 112 In the few recent examples, which were large, the hole was actually open in the recent state ; when small it is usually closed by membrane ; 27 were young bones with un-united upper epiphysis, 5 coexisted with the supracondylar process. The opening is reniform or bilobed in 33. This note is only preliminary, as the subject is sufficiently important to require still further study. I have, however, been able to determine that while in ordinary extension and flexion the tips of the processes do not press on the humerus, yet by forced extension and forced flexion contact can be made to take place, especially when the elbow is forcibly extended, with the hand in the position of pronation, 6. On Anthropological Observations made by Mr. F. Laidlaw in the Malay Peninsula (Skeat Expedition). By W. L. H. Duckworrs. The anthropological results of the Skeat Expedition comprise museum specimens in the form of a skeleton of a native of the Pangan tribe (Kedah), of samples of native hair, and also a collection of measurements by Mr. Laidlaw. The skeleton is that of an adult male, whose stature was distinctly small (about 5 feet). The skull presents a combination of features commonly found in the skulls of negroes with those which characterise the crania of infants, the whole constituting evidence of the lowly physical type of the individual. The bones of the skeleton show signs of widespread disease, possibly of a congenital nature. Mr. Laidlaw’s measurements and observations relate to members of the same tribe, and are to be welcomed as affording precise information about a race of Malayan aborigines hitherto little investigated. Perhaps the most interesting point to notice is the small average stature of the Pangans (about 5 feet for adult men). Though dwarfish, they are, however, markedly taller than the African dwarfs. It is also noteworthy that differences in the colour of the skin (varying shades of dark brown) and in the character of the hair occur in the different tribes. It is important to notice that they present comparatively few anatomical features which can be claimed as evidence of an approximation tu the ape. How- 910 . REPORT—1900 ever primitive in their mode of life, they are anatomically truly terrestrial anid human. The present communication is only a preliminary account of Mr, Laidlaw’s results; moreover, there is much information available through the etforts of the Skeat Expedition regarding the mode of life, language, customs, and religious belief of these fast-disappearing aborigines. The Association is therefore to be congratulated on having, by contributing to the Skeat Expedition, assisted materially in rescuing these records of the Pangan tribe of the Malay Peninsula. 7. On Crania collected by Mr. J. Stanley Gardiner in his Expedition to Rotuma. By W. lL. H. Duckworrtu. The subject of this communication is a collection of nine crania from the above- mentioned locality. The results of a craniological investigation show that while considerable individual differences exist, there are at least two types of skull to be met with in the island of Rotuma. These are in the first place a variety of the form of cranium usually found among Polynesian natives, though possessing certain characteristics which may almost be described as Mongolian; and in the second place the type of cranium characteristic of Melanesians occurs in Mr, Gardiner’s collection. That such different types should be met with in one small island is in accordance with what would be expected on @ priori grounds when it is considered that Rotuma is situated at the centre of contact of three important ethnical areas, viz., the Polynesian to the east, the Melanesian to the south-west, and the Micronesian (where Mongolian elements are discernible among the natives) to the north-west. 8. A System of Classification of Finger Impressions. By J. G. Garson, U.D., Expert Adviser and Instructor on Identification, Home Office. This system of classification of finger impressions has been devised to be worked in conjunction with classification of records by measurements of the head and limbs for the purpose of facilitating search for previous records of criminals. It is also applicable for the classification of small collections of records without the concurrent use of measurements. The objects aimed at in preparing this classification have been to get a moderate number of divisions under which the various patterns and combinations of patterns occurring inthe arrangement of the ridges of the skin on the palmar surface of the terminal phalanges of the digits of the hand may be classified, so that each divi- sion shall contain approximately an equal percentage of the total number of records dealt with, using for the purpose the fewest number of digits that will suftice to get such a distribution, and including only the impressions of those digits which are taken in all countries where the Bertillon system of identification has been adopted—namely, the first four digits of the right hand, The patterns which the ridges form are four in number, and are graphically indicated by the use of the following signs :— An arch thus . . < ; ° . puGyoN A loop which opens on the left . : : ere 4 A loop opening to the right : ; 5 : N A whorl of any kind . : : : ; O The representations of the ridge-patterns depicted by these signs from the im- pressions of the several digits in order of succession constitute the finger formula of an individual, which should be noted on a prominent part of each record so as to be readily seen. It has been found that the patterns and their combinations on the thumb and three following fingers may be conveniently arranged in ten divisions, The thumb and forefinger are always required in the classification, but when the divisions given by these digits are large, the middle finger or the middle and ring finger TRANSACTIONS Of SECTION H. 911 inipréssions aie also iiedded to equalise the size of each division to as nearly as possible 10 per cent. of the total number of records. In the first instance the records are classified into two divisions by the ridge» pattern on the thumb, according as this happens to be A, an arch or either form of loop; B, a whorl. Each of these two groups is broken up into four smaller divisions by the pattern on the forefinger according as it is (a) an arch; (6) a loop with the mouth opening to the left; (¢) a loop with the opening to the right ; (d) a whorl. Of the eight divisions thus obtained no further subdivision is necessary of six groups—namely, of a,b, and d of the A division, and of a, b, and ¢ of the B division. In the A division, further subdivision of the ¢ group by the middle and ring fingers is necessary. This is done by separating the cases where there are loops on each of the four digits from those in which there is any other combination of patterns on the thumb, mid, and ring fingers. Thus we obtain five groups in this first: division. Again, in the B division—namely, the cases in which there is a whorl on the thumb—subdivision has to be resorted to in the d group when there is a whorl on the forefinger as well as on the thumb. This is done by separating the cases where the middle finger bears a whorl from those in which there is an arch or either form of loop. Thus we obtain five groups in this second division. We have now got ten groups, which are of approximately equal size, except the @ group of the B division—that in which the thumb bears a whorl and the forefinger an arch, which is considerably smaller than the others, but this cannot be obviated. In any given number of individuals there will always be some in whom one or more of the four fingers used in classification have been damaged from some cause or other, so that the pattern of the ridges is undecipherable, or one or more fingers of either hand have been lost partially or completely ; espe- cially is this the case amongst the labouring classes in manufacturing districts or towns. In adult criminals such cases amount to about 5°5 per cent. In any system of classification it is necessary to provide for such cases either by making a separate group of them or by placing them with some other group as may be found more con- venient. If the latter course be adopted, and they are added to a of the B group, it will be brought up to the level of several of the other groups. The following is the scheme of classification reduced to tabular form, and the approximate percentage of the records in each of the ten divisions is indicated by the figures given in the lowest line :— . A. B. Right Thumb SRE } O Right Forefinges “\ y | ba | O | aN |Z | rh O 9-3 13-5 NANSI A109. 33 | | . Damaged | | 12*1 Ca | ‘5 STS) ZN 7 N@ =88 10:7 9-4 With the above ten divisions of the finger impressions worked in conjunction with and secondary to classification by measurements, sufficient power is available to enable the records of a large number of criminals to be easi!y manipulated. For example, if only four measurements be used in the tripartite classification, which is universally followed, we have 81 divisions; by the employment of this decimal division by finger-prints, a total of 810 divisions are obtained; while if five measurements be taken, as adopted in England, which gives 243 divisions, by the 912 REPORT—1900, combined system, we increase the power of effective classification tenfold, and obtain no less than 2,430 divisions, and that without straining either source of classification, WEDNESDAY, SEPTEMBER 12. The following Papers and Report were read :— 1. The Sense of Effort and the Perception of Force. By Professor G, J. Stokes, J/.A. According to the most generally accepted view the idea of force is obtained from the muscular sense. It has also been attributed to touch. The most important question is whether the perception is connected with the motor or sensory nerves. If the latter view be adopted, it has been thought that this sensa- tion can reveal nothing of the nature of the objective cause. As recent investiga- tion seems to compel the adoption of the latter view, the objective character of the perception can only be saved if we admit the presence of an objective character in all sensation. If Wundt’s theory of the original functional indifference of the nerves be accepted, we may yet be enabled to remove the difficulties in the way of admitting such an objective character. The true difference between the perception of force and other sensations will then lie, not in the process by which the pheno- menon is apprehended, but in the nature of the phenomenon apprehended. We may thus have an apprehension of an objective external reality—the same reality which underlies the phenomena of dynamics. The principle of Least Action may perhaps explain the directive character of vital and voluntary processes. 2. On Interpolation in Memory.' By Professor Marcus Hartoe, J.A., D.Se. Many educational syllabuses that profess to rest on a psychological base assume that the only guidance for action is a sensation which has been memorised by frequent repetition. The mind, however, seems to have the power of classifying the memories of each category apart and in order of magnitude and direction, completing the records of single memories with what may be compared with an interpolation-curve, and even extrapolating on either side; so that, if a suitable response have been learned to a limited number of sensations, a new sensation of the same category will produce a new appropriate response. This capacity for in- terpolating has been long recognised in various arts, and is known as ‘ faculty,’ ‘feeling,’ &e. It has not, however, been definitely recognised hy the psychologist, who has asked whether the conseiows memory and judgment can construct inter- mediate sensations between those he has learned from experience, rather than whether there is a power in virtue of which it can recognise the appropriate position of new sensations, or appropriately act on the stimulus of new sensations when they occur. Similarly with combinations of intermediate sensations, the mind can simulta- neously act on them and execute the combined appropriate response in much the same way as the pencil of a tide-predicting machine is simultaneously acted upon by the independent wheels. This is shown by the now received fact (finally proved by Richet) that each mental act takes about the tenth of a second, and any act of conscious (sit venia verbo) combination and judgment is usually out of the question from a lack of adequate time. Illustrations of these views were quoted from the domains of housekeeping, the plastic arts, cards, billiards, and language. It was urged that @ prior? methods of instruction based on incomplete premises must be regarded with extreme caution. 1 Published in the Contemporary Review for October 1900. TRANSACTIONS OF SECTION 8. 913 3. The Defensive Earthworks of Yorkshire. By Mrs. Armirace. The author describes the various types of earthworks in Yorkshire—Roman camps, hill forts, and boundary earthworks—and gives a summary of the results of recent researches regarding these three classes of earthworks. A fourth class very frequent in Yorkshire is the moated hillock, with moated court attached. It has been assigned in turn to the Britons, Romans, Saxons, and Danes. The author gives reasons why none of these views is probable, and shows the erroneousness of the theory of Mr. G. T. Clark, now so widely accepted, that the Anglo-Saxon burh was a hillock of this kind, its meaning in Anglo-Saxon literature being clearly a fortified town. The author produces the following arguments for the Norman origin of these hillocks (called by the Normans mottes): (a) the Normans are known to have built such earthworks in Normandy and Ireland, and are represented in the Bayeux tapestry as throwing up a similar work at Hastings; (8) the type belongs to the age of feudalism, and answers to the needs of the Normans in the United Kingdom ; (y) the Norman castles mentioned by the contemporary chroniclers or by Domesday Book as constructed by the Conqueror or his followers have nearly all of them mottes. The evolution of the Castle, the personal fortification of the feudal chieftain, accompanied the evolution of society from the tribal to the feudal type. 4. On the Prehistoric Antiquities of Rumbald’s Moor. By Butter Woop. 5. On the Occurrence of Flint Implements of Paleolithic Type on an old Land-surface in Oxfordshire, near Wolvercote and Pear Tree Hill, together with a few Implements of various Plateaw Types. By A. M. Bett, J/.A. At Wolvercote, near Oxford, there is a large section of a quaternary river-gravel which has produced the usual fauna, Elephas primigenius &c., and many fine implements of human workmanship. This gravel cuts into and is consequently newer than a previous land-surface. A portion of this surface is found at Wolvercote and another portion at Pear Tree Hill, about half a mile distant. In both places flint implements of paleolithic type, together with bulbed flakes and a few implements of plateau type, have been found. In every case the flints are ochreous, which distinguishes them from those which belong to the river- gravel at Wolvercote. The older surface has been previously described as Northern Drift. It is sup- posed by the author to be a remaniement of the true Northern Drift, but to have been deposited under semi-frozen conditions. It must be anterior to the river- valley, and consequently its relics of man are the oldest as yet obtained from the Thames Valley. The drift in question most resembles the drifts of Caddington, described by Mr. G. Worthington Smith, and some sections of the Lower Greensand near Limpsfield. Both of these drifts are implementiferous, and the author would correlate the Wolvercote and Pear Tree Hill surface with these drifts. 6. On the Physical Characteristics of the Population of Aberdeenshire. By J. Gray, B.Sc., and J. F. Tocusr, F.C. These observations were taken at the Lonach gathering in Strathdon, a district lying right at the head of the valley of the Don. The district is comparatively isolated, the nearest railway station being over twelve miles distant. Our principal object was to ascertain what difference if any existed between the people in the upper ends of the river valleys and the people on the eastern sea- 1900, 3N 914 REPORT—1900, board, the anthropological statistics of which have been recently ascertained. The following results show that a very considerable difference exists; and it being highly probable that a more primitive stratum of the population is always to be found in the upper ends of river valleys, the results are of great interest from this point of view. } The pigmentation and nose statistics of the whole of the people attending the gathering, namely, 361 males and 243 females, were taken at the gate by two observers. Later on the same statistics, with the addition of measurements of the head and of stature, were taken in a tent in the grounds, about ninety adult males, natives of the district, being measured. The people observed at the gate contained a small percentage of visitors from a distance, which may account for the difference in the results obtained at the gate and in the tent. Hair Tyes Types of Noses | | \Fair,Red iste Dark | Light tea Dark Straight, Roman Wavy Concave! Jew } f ‘aes | = Males : | W. Aberdeenshire | 10 8 | 42 |. 40 57 48.j.. 14 79 15 3 2 i (gate) | | | | | W. Aberdeenshire | 5| 8 40 | 47 38 =| 45) 17 56 | «22 13 6 3 (tent) | E. Aberdeenshire | 9}| 6| 66 | 19 26 51 | 23 | ey ee rt cy ae od) (gate) M jerks | | | | | E. Aberdeenshire | 18 | 2 | 40 40 35 | 46 | 19 66.5020 meee | “ : : - 2 : di . 444 Second Interim Report on the Working out of the Details of the Observations of the Migration of Birds at Lighthouses and Lightships, 1880-87 . - 447 Eighth Report on the Climatology of Africa : c ‘ : “ ‘ . 448 Report on the Exploration of the Island of Sokotra- . . . . 3 . 460 Report on the Means by which Practical Effect can be given to the Intro- duction of the Screw Gauge proposed by the Association in 1884 ; . 464 On the Erection of Alexander III. Bridge in Paris. By M.AMEDBEALBY . 469 Dover Harbour Works. By J. C. CoopE and W. 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Proressor SIR WILLIAM TURNER, K.C.B., M.B., D.Sc., D.0.L., LL.D., F.B.S. VICE-PRESIDENTS. The Right Hon. the Hart or ScArBROUGH, Lord- Lieutenant of the West Riding of Yorkshire. His Grace the DUKE OF DEVoNsHIRE, K.G., D.C.L., LL.D., F.R.S. The Most Hon. the Marquis or Ripon, K.G., G.O.S.1., D.O.L., F.R.S. ‘The Right Rev. the LorpD Bisnop or Ripon, D.D. ‘The Right Hon. Lornp Masham. His Worship the Mayor or BRADFoRD. The tat’ H.E. Boturn, Lord of the Manor, Brad- ora, Sir ALEXANDER BINNIF, M.Inst.0.E., F.G.S, Professor A. W. Ricker, M.A., D.Sc., Sec.R.S. Dr. T. E. THoRPS, Sce.D., F.R.S., Pres.C.S. Principal N. BopinG'ron, Litt.D., Vice-Chancellor of tbe Victoria University. Professor L. C. MIALL, F.R.S. PRESIDENT ELECT. Professor A. W. Ricker, M.A., D.Sc., Sec.R.S. VICE-PRESIDENTS ELECT. The Right Hon. the EARL or GLAscow, K.0.M.G. ‘The Right Hon. the Lorp BLyTHswoop. The Right Hon. the Lorp KEtvin, G.C.V.0O., D.O.L., LL.D., F.B.S. ‘The Hon, the Lorp Provost or GLASGOW. ‘The Principat of the University of Glasgow. Sir JOHN MAXWELL STIRLING-MAXWELL,Bart., M.P. Sir ANDREW NoBLgE, K.O.B., D.C.L., F.R.¢. S r ARCHIBALD GRIKIE, D.C.L., LL.D., F.RS. Sir W. T. THISELTON-DyeEr, K.C.M.G., C.1.E., F.R.S, JAMES PARKER SMITH, Esq., M.P, JOHN INGLIS, Esq., LL.D. ANDREW STEWART, Esq., LL.D. GENERAL SECRETARIES. Professor Sir William 0. Roperts-AUSTEN, K.C.B., D.C.L., F.R.S. Dr. D. H. Scorr, F.R.S. ASSISTANT GENERAL SECRETARY. G. GrirrirH, Esq., M.A., Harrow, Middlesex, GENERAL TREASURER. Professor G, Caney Foster, B.A., F.R.S., Burlington House, London, W. LOCAL SECRETARIES FOR THE MEETING AT GLASGOW, Sir J. D. Marwick, LL.D.,F.RS.E. | Prof. JOHN YouNG, M.D. | Prof. Magnus MAcLEAN, D.Se LOCAL TREASURERS FOR THE MEETING AT GLASGOW. ROBERT GOURLAY, Esq. | JAMES NICOL, Esq., City Chamberlain, ORDINARY MEMBERS OF THE COUNCIL. ARMSTRONG, Professor H. E., F.R.S. Bonar, J., Esq., LL.D. Bowen, Professor F. O., F.R.S. OALLENDAR, Professor H.L, FR.S, CrEAK, Captain E. W., R.N., F.R.S. DARWIN, F., Esq., F.R.S. Darwin, Major L., Sec.R.G.S. FREMANTLE, Hon. Sir OC, W., K.C.B. GASKELL, Dr. W. H., F.R.S. HALLIBURTON, Professor W. D., F.R.S. Harcourt, Professor L. F. VERNON, M.A. Kettim, J. Scorr, Esq., LL.D. LANKESTER, Professor E. Ray, F.R.S. Lockyer, Sir J. NorMAN, K.C.B., F.R.S. Loner, Professor O. J., F.R.S. MAcMAHON, Major P. A., F.R.S. Marr, J. E., Esq., F.R.S. Poutton, Professor E. B., F R.S. PREECE, Sir W. H., K.C.B., F.RS. | Price,. L. L., Esq., M.A. | SOLAS, Professor W. J.. F.R.S. THOMSON, Professor J. M., F.R.S. TILDEN, Professor W. A., F.R.S. Ty Lor, Professor E. B., F.R.S. WoLre-Barky, Sir J., K.C.B., F.B.S. EX-OFFICIO MEMBERS OF THE COUNCIL, The Trustees, the President and President Elect, the Presidents of former years, the Vice-Presidents and Vice-Presidents Elect, the General and Assistant General Secretaries for the present and former years, the Secretary, the General Treasurers for the present and former years, and the Local Treasurer and Secretaries for the ensuing Meeting. TRUSTEES (PERMANENT). The Right Hon. Lord AveBoury, D.C.L., LL.D., F.R.S., F.L.S. The Right Hon. Lord RayirieH. M.A., D.C.L., LL.D., F.R.S., F.R.A.S, Professor A. W. RijckER, M.A., D.Sc., Sec. R.S. PRESIDENTS OF FORMER YEARS. Sir Joseph D. Hooker, K.C.S.1., | Sir H. E. Roscoe, D.C.L., F.R.S. | The Marquis of Salisbury, K.G. PRS. ar Sir F. J. Bramwell, Bart., F.R.S. ¥.R.S. , Sir F. A. Abel, Bart., K.0.B., P.R.S. | Lord Lister, D.C.L., F.R.S. Sir Wm. Huggins, K.0.B., P.R.S. | Sir John Evans, K.C SirArchibald Geikie, LL.D..F.R.8. | Sir William Crookes Lord Avebury, F.R.S. Prof. Sir J.S. Burdon Sanderson, | Sir Michael Lord Rayleigh, D.C.L., F.R.S. Bart., F.R.S. M.P., Sec.R.S. GENERAL OFFICERS OF FORMER YEARS, F. Galton, Esq., D.C.L., F.R.S. P. L. Sclater, Esq., Ph.D., F-R.S. | Prof. A. W. Riicker, D.Sc. See R.Se Prof. Sir Michael Foster, K.C.B., | Prof. T.G. Bonney, D.Se., F.R.S. | Prof. E. A. Schiifer, F.R.S, M.P., Sec. R.S. Prof. A. W. Williamson, #.R.S. G. Griffith, Esq., M.A. A. Vernon Harcourt, Esq., F.R.S, AUDITORS. Dr. Horace Brown, F.R.S. | A 2 Sir G. G. Stokes, Bart., F.R.S. Lord Kelvin, G.0.V.0., F.R.S. Prof. A. W. Williamson, F.R.S. E. W. Brabrook, E:q., C.B, ie ee ‘4 Wik Sart, $- ri at SP oo LIST OF MEMBERS OF THE BRITISH ASSOCIATION FOR THE ADVANCEMENT OF SCIENCE. 1900. * indicates Life Members entitled to the Annual Report. § indicates Annual Subscribers entitled to the Annual Report, §s indicates Annual Subscribers who will be entitled to the Annual Report if their Subscriptions are paid by December 31, 1900. { indicates Subscribers not entitled to the Annual Report. Names without any mark before them are Life Members, elected before 1845, not entitled to the Annual Report. Names of Members of the GENERAL CoMMI?TrEE are printed in SMALL CAPITALS. Names of Members whose addresses are incomplete or not known are in italics. Notice of changes of residence should be sent to the Assistant General Secretary, G. Griffith, Esq., Burlington House, W. Year of Glection. 1887. *AnBE, Professor CLrveranp. Weather Bureau, Department of Agri- culture, Washington, U.S.A. 1897. t{Abbott, A. H. Brockville, Ontario, Canada. 1898. §Abbott, George, M.R.C.S. 33 Upper Grosvenor-road, Tunbridge Wells. Fe 1881. *Abbott, R. T. G. Whitley House, Malton. 1887, tAbbott,T.C. Eastleigh, Queen’s-road, Bowdon, Cheshire, 1863. *AseEL, Sir Freprrick Aveustus, Bart., K.0.B., D.C.L., D.Se., F.R.S., V.P.C.S., President of the Government Committee on Explosives. The Imperial Institute, Imperial Institute-road, and 2 Whitehall-court, S.W. 1885, *AnERDEEN, The Right Hon. the Earl of, G.C.M.G., LL.D. Haddo House, Aberdeen. 1885. tAberdeen, The Countess of. Haddo House, Aberdeen. 1885. { Abernethy, David W. Ferryhill Cottage, Aberdeen. 1885, tAbernethy, James W. 2 Rubislaw-place, Aberdeen. 1873, *Asney, Captain Sir W. pz W., K.C.B., D.C.L., F.R.S., FLR.A.S Rathmore Lodge, Bolton-gardens Sevth, Earl’s Court, S.W. 6 LIST OF MEMBERS. Year of Election. 1886, 1884. 1875. 1900. 1882. 1869. 1877. 1873. 1894, 1877, 1898. 1887, 1892. 1884. 1871. 1879. 1869. 1879. 1896. 1898. 1890. 1890. 1899. 1883. 1896. 1884. 1887. 1864. 1871. 1871. 1895. 1891. 1871. 1898. 1884. 1886. 1900. 1896. 1894, 1891. 1883. 1858. 1896. 1891. 1883. 1883. 1883. 1867, fAbraham, Harry. 147 High-street, Southampton. tAcheson, George. Collegiate Institute, Toronto, Canada. tAckroyd, Samuel. Greaves-street, Little Horton, Bradford, Yorkshire. §Ackroyd, William, Borough Laboratory, Crossley Street, Halifax. *Acland, Alfred Dyke. 38 Pont-street, Chelsea, S.W. tAcland, Sir C. T. Dyke, Bart., M.A. Killerton, Exeter. *Acland, Captain Francis E. Dyke, R.A. Woodmansterne Rectory, Banstead, Surrey. *Acland, Rey. H. D., M.A. Luccombe Rectory, Taunton. *Acland, Henry Dyke, F.G.S. The Old Bank, Great Malvern. *Acland, Theodore Dyke, M.A. 74 Brook-street, W. tAcworth, W.M. 47 St. George’s-square, 8. W. tAvaaa, J. G., M.A., M.D., Professor of Pathology in the University, Montreal, Canada. tAdams, David. Rockville, North Queensferry. tAdams, Frank Donovan. Geological Survey, Ottawa, Canada. §Adams, John R. 2 Nutley-terrace, Hampstead, N.W. *Apams, Rev. THomas, M.A., D.C.L., Paignton, South Devon. *Apams, WILLIAM GryLts, M.A., D.Sc., F.R.S., F.G.S., F.C.P.S., Pro- fessor of Natural Philosophy and Astronomy in King’s College, London. 43 Campden Hill-square, W. tAdamson, Robert, M.A., LL.D., Professor of Logic in the Uni- versity of Glasgow. tAdamson, W. Sunnyside House, Prince’s Park, Liverpool. §Addison, William L. T. Byng Inlet, Ontario, Canada. t{Addyman, James Wilson, B.A. Belmont, Starbeck, Harrogate. tApengy, W. E., F.C.S. Royal University of Ireland, Earlsfort- terrace, Dublin. §Adie, R. H., M.A., B.Sc. 8 Richmond-road, Cambridge, tAdshead, Samuel. School of Science, Macclesfield. tAffieck, W. H. 28 Onslow Road, Fairfield, Liverpool. tAgnew, Cornelius R. 266 Maddison-avenue, New York, U.S.A. tAgnew, William. Summer Hill, Pendleton, Manchester. *Ainsworth, David. The Flosh, Cleator, Carnforth. * Ainsworth, John Stirling. Harecroft, Gosforth, Cumberland. t{Ainsworth, William M. The Flosh, Cleator, Carnforth. *Airy, Hubert, M.D. Stoke House, Woodbridge, Suffolk. *Aisbitt, M. W. Mountstuart-square, Cardiff. §AITKEN, JOHN, F.R.S., F.R.S.E. Ardenlea, Falkirk, N.B. {Axnrs-Dovetas, Right Hon. A., M.P. 106 Mount-street, W. *Alabaster, H. Lytton, Mulgrave-road, Sutton, Surrey. *Albright, G.S. The Elms, Edgbaston, Birmingham. § Aldred, Francis J.. M.A. The Lizans, Malvern Link. §Aldridge, J. G. W., Assoc.M.Inst.C.k. 9 Victoria-street, West- minster, S.W. tAlexander, A. W. Blackwall Lodge, Halifax. tAlexander, D.'T. Dynas Powis, Cardiff. tAlexander, George. JKildare-street Club, Dublin. *Alexander, Patrick Y. Experimental Works, Bath. tAlexander, William. 45 Highfield South, Rockferry, Cheshire. *Alford, Charles J., £.G.S. 15 Great St. Helens, E.C. tAlger, Miss Ethel. The Manor House, Stoke Damerel, South Devon. tAlger, W. H. The Manor House, Stoke Damerel, South Devon. tAlger, Mrs. W. H. The Manor House, Stoke Damerel, South Devon. tAlison, George L. C. Dundee. LIST OF MEMBERS, 7 Year of Election. 1885, {Allan, David. West Cults, near Aberdeen. 1871. {Allan, G., M.Inst.C.E. 10 Austin Friars, E.O. 1871. {Axten, Atrrep H.,F.C.S. 67 Surrey-street, Sheffield. 1879, *Allen, Rev. A. J.C. The Librarian, Peterhouse, Cambridge. 1898. §Allen, E. J. The Laboratory, Citadel Hill, Plymouth. 1888. 1884. 1891. 1887. 1878. 1891. 1889. 1889. 1886. 1896. 1882. 1887. 1873. 1891. 1883. 1883. 1884. 1883, 1885. 1874. 1892. 1899, 1888. 1887. 1889. 1880. 1883, 1895. 1891. 1880. 1886. 1883. 1877. 1886. 1900. 1896. 1886. 1878. 1890. . §Arber, E. A. N., B.A. Trinity College, Cambridge. . {Archer,G, W. 11 All Saints’-road, Clifton, Bristol. . §Archibald, A. The Bank House, Ventnor, . “Archibald, E. Douglas. Constitutional Club, Northumberland tAxten, F. J.,M.A., M.D., Professor of Physiology, Mason University College, Birmingham. fAllen, Rev. George. Shaw Vicarage, Oldham, fAllen, Henry A., F.G.S. Geological Museum, Jermyn-street, S.W. fAllen, John. Kilgrimol School, St. Anne’s-on-the-Sea, via. Preston. tAllen, John Romilly. 28 Great Ormond-street, W.C. tAllen, W. H. 24 Glenroy Street, Roath, Cardiff. tAllhusen, Alfred. Low Fell, Gateshead. tAllhusen, Frank E. The School, Harrow. tAllport, Samuel, F.G.S. Mason University College, Birmingham, TAlsop, J. W. 16 Bidston-road, Oxton. *Alverstone, The Right Hon. Lord, G.C.M.G., LL.D. Hornton Lodge, Hornton Street, Kensington, S.W. fAlward, G. L. 11 Hamilton-street, Grimsby, Yorkshire, tAmbler, John. North Park-road, Bradford, Yorkshire. fAmbrose, D. R. Care of Messrs. J. Evans & Co., Bute Docks, Cardiff. §Amery, John Sparke. Druid, Ashburton, Devon. §Amery, Peter Fabyan Sparke. Druid, Ashburton, Devon. tAmi, Henry, M.A., F.G.S. Geological Survey, Ottawa, Canada. tAnderson, Miss Constance. 17 Stonegate, York. *ANnDERSON, HucH Kerr. Caius College, Cambridge. tAnderson, John, J.P., F.G.S. Holywood, Belfast. fAnderson, Joseph, LL.D. 8 Great King-street, Edinburgh. *Anderson, Miss Mary K. 13 Napier-road, Edinburgh. *Anderson, R. Bruce. 354 Great George-street, S.W. fAnderson, Professor R. J.. M.D. Queen’s College, and Atlantic Lodge, Salthill, Galway. tAnderson, R. Simpson. Elswick Collieries, Newcastle-upon-Tyne. *ANDERSON, TempEst, M.D., B.Sc., F.G.S. 17 Stonegate, York. tAndrew, Thomas, F.G.S. 18 Southernhay, Exeter. tAndrews, Charles W. British Museum (Natural History), S.W, tAndrews, Thomas, 163 Newport-road, Cardiff. *Andrews, Thornton, M.Inst.C.E. Cefn Eithen, Swansea, §Andrews, William, F.G.S. Steeple Croft, Coventry. fAnelay, Miss M. Mabel. Girton College, Cambridge. §AneELL, Jonny, F.C.S., FIC. 6 SBeacons-field, Derby-road, Withington, Manchester, tAnnan, John, J.P. Whitmore Reans, Wolverhampton. §Annandale, Nelson. 84 Charlotte Square, Edinburgh. fAnnett, R. C.F. 11 Greenhey-road, Liverpool. fAnsell, Joseph. 38 Waterloo-street, Birmingham. tAnson, Frederick H. 15 Dean’s-yard, Westminster, S.W. §Antrobus, J. Coutts. Eaton Hall, Congleton. Avenue, W.C. . §Armistead, Richard. Chambres House, Southport. *Armistead, William. Hillcrest, Oaken, Wolverhampton, . Armitage, Benjamin. Chomlea, Pendleton, Manchester. 8 LIST OF MEMBERS. Election. 1857. *Anmstronc, The Right Hon. Lord, C.B., LL.D., D.C.L., F.R.S., Cragside, Rothbury. 1873. *Armstronc, Henry E., Ph.D., LL.D., F.R.S., Professor of Chemis- try in the City and Guilds of London Institute, Central Institution, Exhibition-road, S.W. 55 Granville Park, Lewisham, S.E. 1876. {Armstrong, James. Bay Ridge, Long Island, New York, U.S.A. 1889. t Armstrong, John A, 32 Eldon-street, Newcastle-upon-Tyne. 1889. +O EERE) Thomas John. 14 Hawthorn-terrace, Newcastle-upon- ne, 1893. eae oem H., M.A., F.G.8. 56 Friar-gate, Derby. 1870. *Ash, Dr. T. Linnington. Penroses, Holsworthy, North Devon. 1874. tAshe, Isaac, M.3. Dundrum, Co. Dublin. 1889, tAshley, Howard M. Airedale, Ferrybridge, Yorkshire. 1887. tAshton, Thomas Gair, M.A. 36 Charlotte-street, Manchester. *Ashworth, Edmund. Egerton Hall, Bolton-le-Moors, Ashworth, Henry. Turton, near Bolton. 1888. *Ashworth, J. Jackson. Haslen House, Handforth, Cheshire. 1890. {Ashworth, J. Reginald, B.Sc. 105 Freehold-street, Rochdale, 1887. tAshworth, John Wallwork, F.G.8. Thorne Bank, Heaton Moor, Stockport. 1887. tAshworth, Mrs. J. W. Thorne Bank, Heaton Moor, Stockport. 1887. tAspland, Arthur P. Werneth Lodge, Gee Cross, near Manchester. 1875. *Aspland, W. Gaskell. Tuplins, Newton Abbot. 1861. {Asquith, J. R. Infirmary-street, Leeds. 1896. *Assheton, Richard. Grantchester, Cambridge. 1861. {Aston, Theodore. 11 New-square, Lincoln’s Inn, W.C. 1896. §Atkin, George, J.P. Egerton Park, Birkenhead. 1887. §Atkinson, Rev. C. Chetwynd, D.D. Ingestre, Ashton-on-Mersey. 1884. ae Edward, PhD., LL.D. Brookline, Massachusetts, S.A 1898. *Atkinson, E. Cuthbert. Temple Observatory, Rugby. 1894, tAtkinson, George M. 28 St. Oswald’s-road, 8. W. 1894, *Atkinson, Harold W. Rossall School, Fleetwood, Lancashire, 1861. {Athinson, Rev. J. A. The Vicarage, Bolton. 1881. {Atkinson, J. T. The Quay, Selby, Yorkshire. 1881. tArxinson, Ropert WittiAM, F.C.S. 44 Loudoun-square, Cardiff. 1894, §Atkinson, William. Erwood, Beckenham, Kent. 1863. *ArrriIELD, J., M.A., Ph.D., F.R.S., F.C.S. 111 Temple-chambers, K.C. 1884, tAuchincloss, W.S. 209 Church-street, Philadelphia, U.S.A. 1853. *AveBuRY, The Right Hon. Lord, D.C.L, F.R.S. High Elms, Farnborough, Kent. 1877, *Ayrton, W. E., F.R.S., Professor of Applied Physics in the City and Guilds of London Institute, Central Institution, Exhibition- road, S.W. 41 Kensington Park-gardens, W. 1884. {Baby, The Hon. G. Montreal, Canada. 1900. §Baccuvus, RamspEN. 15 Welbury Drive, Bradford. 1883. *Bach, Madame Henri. 12 Rue Fénélon, Lyons, Backhouse, Edmund. Darlington. 1863. {Backhouse, T. W. West Hendon House, Sunderland. 1883. *Backhouse, W. A. St. John’s, Wolsingham, R.S.0., Durham. 1387. *Bacon, Thomas Walter. Ramsden Hall, Billericay, Essex. 1887. {Baddeley, John. 1 Charlotte-street, Manchester. 1883. {Baildon, Dr. 65 Manchester-road, Southport. 1892. {Baildon, H. Bellyse. Duncliffe, Murrayfield, Edinburgh. Year of Election 1883. 1895. 1870. 1887, 1865. LIST OF MEMBERS. 9 *Bailey, Charles, F.L.S, Ashfield, Cullege-road, Whalley Range, Manchester. §Bartey, Colonel F., Sec. R.Scot.G.8., F.R.G.S. 7 Drummond-place, Edinburgh. {Bailey, Dr. Francis J. 51 Grove-street, Liverpool. *Bailey, G. H., D.Sc., Ph.D. Marple Cottage, Marple, Cheshire. tBailey, Samuel, F.G.S. Ashley House, Calthorpe-road, Edgbaston, Birmingham. 1899.§§ Bailey, T. Lewis. 85 Wawarden-avenue, Liverpool. 1855. 1887. 1894. 1878. 1885. 1897. 1885. 1882. 1898. 1898. 1891. 1881. 1875. 1881. 1884. 1871. 1894. 1875. 1885. 1878. 1866. 1885. 1886. 1869. 1890, 1899. {Bailey, W. Horseley Fields Chemical Works, Wolverhampton. tBailey, W. H. Summerfield, Eccles Old-road, Manchester. *Baily, Francis Gibson, M.A. 11 Ramsay-garden, Edinburgh. {Baity, Watrpr. 4 Roslyn-hill, Hampstead, N.W. {Bary, Atexanprr, M.A., LL.D. Ferryhill Lodge, Aberdeen. §Bain, Jamas, jun. Toronto. {Bain, William N. Collingwood, Pollokshields, Glascow. *Baker, Sir Bensamrn, K.C.M.G., LL.D., D.Sc., F.R.S., M.Inst.C.E. 2 Queen Square-place, Westminster, S.W. {Baker, Herbert M. Wallcroft, Durdham Park, Clifton, Bristol, {Baker, Hiatt C. Mary-le-Port-street, Bristol. {Baker, J. W. 50 Stacey-road, Cardiff. {Baker, Robert, M.D. The Retreat, York. {Baxer, W. Proctor. Bristol. {Baldwin, Rev. G. W. de Courcy, M.A. Lord Mayor’s Walk, York. {Balete, Professor E. Polytechnic School, Montreal, Canada. {Balfour, The Right Hon. G. W., M.P. 24 Addison-road, Ken- sington, W. §Balfour, Henry, M.A. 11 Norham-gardens, Oxford. {Batrovr, Isaac Baytry,M.A.,D.S8c.,M.D., F.R.S.,F.R.S.E., F.L.S., Professor of Botany in the University of Edinburgh. Inverleith House, Edinburgh. tBalfour, Mrs. I. Bayley. Inverleith House, Edinburgh. *Ball, Charles Bent, M.D., Regius Professor of Surgery in the University of Dublin. 24 Merrion-square, Dublin. *Batz, Sir Ropert Srawert, LL.D., F.R.S., F.R.A.S., Lowndean Professor of Astronomy and Geometry in the University of Cambridge. The Observatory, Uambridge. ; *Ball, W. W. Rouse, M.A, Trinity College, Cambridge. {Ballantyne, J. W., M.B. 24 Melville-street, Edinburgh. {Bamber, Henry K., F.0.S. 5 Westminster-chambers, Victoria- street, Westminster, S. W. Bamford, Professor Harry, B.Sc. McGill University, Montreal, Canada. §Bampton, Mrs. 42 Marine-parade, Dover. 1882. {Bance, Colonel Edward, J.P. Oak Mount, Highfield, Southampton. 1898.§§Bannerman, W. Bruce, F.R.G.S., F.G.S. The Lindens, Sydenham- 1884, 1866, 1884. 1890. 1861. 1894.§ 1871. road, Croydon, {Barbeau, EK. J. Montreal, Canada. {Barber, John. Long-row, Nottingham. tBarber, Rev. 8. F. West Raynham Rectory, Swaffham, Norfolk. *Barber-Starkey, W. J.S. Aldenham Park, Bridgnorth, Salop. *Barbour, George. Bolesworth Castle, Tattenhall, Chester. §Barclay, Arthur. 29 Gloucester-road, South Kensington, S.W. {Barclay, George. 17 Coates-crescent, Edinburgh. 1860. *Barclay, Robert. High Leigh, Hoddesden, Herts. 1887. *Barclay, Robert. Sedgley New Hall, Prestwich, Manchester. 1886. {Barclay, Thomas. 17 Bull-street, Birmingham, 10 LIST OF MEMBERS. Year of Election. 1881. {Barfoot, William, J.P. Whelford-place, Leicester. 1882. {Barford, J. D. Above Bar, Southampton. 1886. {Barham, F. F. Bank of England, Birmingham. 1890. {Barker, Alfred, M.A., B.Sc. Aske’s Hatcham School, New Cross, S.E, 1899. §Barker, John H. 26 Park-parade, Cambridge. 1882. *Barker, Miss J. M. Hexham House, Hexham. 1879. *Barker, Rey. Philip C., M.A., LL.B. Priddy Vicarage, Wells, Somerset. 1898. §Barker, W. R. 106 Redland-road, Bristol. 1886. {Barling, Gilbert. 85 Edmund-street, Edgbaston, Birmingham. 1873. {Barlow, Crawford, B.A., M.Inst.C.E. Deene, Tooting Bec-road, Streatham, S.W. 1889. §Barlow, H. W. L., M.A., M.B., F.C.S. Holly Bank, Croftstank- road, Urmston, near Manchester. 1883. {Barlow, J. J. 37 Park-street, Southport. 1878. {Barlow, John, M.D., Professor of Physiology in Anderson’s Col- lege, Glasgow. 1883. {Barlow, John R. Greenthorne, near Bolton. 1885. *Bartow, WitiiAM, F.G.8. The Red House, Great Stanmore. 1873. {Bartow, Wixi1am Henry, F.R.S., M.inst.C.E. High Combe, Old Charlton, Kent. 1861. *Barnard, Major R. Cary, F.L.S. Bartlow, Leckhampton, Cheltenham, 1881. {Barnard, William, LL.B. 38 New-court, Lincoln’s Inn, W.C. 1889. {Barnes, J. W. Bank, Durham. 1868. §Barnes, Richard H. Heatherlands, Parkstone, Dorset. 1899.§§Barnes, Robert. 9 Kildare Gardens, Bayswater, W. 1884. {Barnett, J. D. Port Hope, Ontario, Canada. 1899.§§Barnett, W. D. 41 Threadneedle-street, H.C. 1881. {Barr, ARCHIBALD, D.Sc., M.Inst.C.E. The University, Glasgow. 1890. {Barr, Frederick H. 4 South-parade, Leeds. 1859. {Barr, Lieut.-General. Apsleytoun, East Grinstead, Sussex. 1891. §Barrell, Frank R., M.A., Professor of Mathematics in University College, Bristol. 1883. {Barrett, John Chalk. Errismore, Birkdale, Southport. 1883. {Barrett, Mrs. J. C. Errismore, Birkdale, Southport. 1872. *Barrert, W. F., F.R.S., F.R.S.E., M.R.1.A., Professor of Physics in the Royal College of Science, Dublin. 1883. {Barrett, William Scott. Abbotsgate, Huyton, near Liverpool. 1899. §Barrert-Hamitton, Capt. G. E. H. Kilmarnock, Arthurstown, Waterford, Ireland. 1887. {Barrington, Miss Amy. Fassaroe, Bray, Co. Wicklow. 1874. *Barrineton, R. M., M.A., LL.B., F.L.S. Fassaroe, Bray, Co. Wicklow. 1874. *Barrington-Ward, Mark J., M.A., F.L.S., F.R.G.S., H.M. Inspector of Schools. Thorneloe Lodge, Worcester. 1885. *Barron, Frederick Cadogan, M.Inst.C.E. Nervion, Beckenham- erove, Shortlands, Kent. 1866. {Barron, William. Elvaston Nurseries, Borrowash, Derby. 1898, *Barrow, GuoreE, F.G.S. ‘Geological Survey Office, 28 Jermyn- street, S.W. 1886. {Barrow, George William. Baldraud, Lancaster. 1886, {Barrow, Richard Bradbury. Lawn House, 13 Ampton-road, Edg- baston, Birmingham. 1896. §Barrowman, James. Staneacre, Hamilton, N.B. 1886. {Barrows, Joseph. The Poplars, Yardley, near Birmingham. 1886. {Barrows, Joseph, jun. Ferndale, Harborne-road, Edgbaston, Bir- mingham, Year of LIST OF MEMBERS. 11 Election. 1858. 1883. 1881. 1884, 1890. 1890. 1892. 1858. 1884. 1873. 1892. 1893. 1884. 1852. 1899. 1892. 1887. 1898. 1876. 1876. 1888. 1891. 1866. 1889. 1869. 1871. 1889. 1883. 1868. 1889. 1884. 1881. 1863. 1867. 1892, 1875. 1876. 1887. 1883. 1886. 1886, 1860. 1882. 1884. 1872. tBarry, Right Rev. Atrrep, D.D., D.C.L. The Cloisters, Windsor. {Barry, Charles E. 1 Victoria-street, 8. W. {Barry, J. W. Duncombe-place, York. *Barstow, Miss Frances A. Garrow Hill, near York. *Barstow, J. J. Jackson. The Lodge, Weston-super-Mare. *Barstow, Mrs. The Lodge, Weston-super-Mare. tBartholomew, John George, F.R.S.E., F.R.G.S. 12 Blacket-place, Edinburgh. *Bartholomew, William Hamond, M.Inst.C.E. Ridgeway House, Cumberland-road, Hyde Park, Leeds. {Bartlett, James Herbert. 148 Mansfield-street, Montreal, Canada. {Bartley,G.C.T.,M.P. St. Margaret’s House, Victoria-street, S.W. tBarton, Miss. 4 Glenorchy-terrace, Mayfield, Edinburgh. {Barton, Edwin H., B.Sc. University College, Nottingham. {Barton, H. M. Foster-place, Dublin. tBarton, James. Farndree, Dundalk. *Barton, Miss Ethel 8. 7 Brechin Place, South Kensington, 8.W. tBarton, William. 4 Glenorchy-terrace, Mayfield, Edinburgh. {Bartrum, John 8S. 13 Gay-street, Bath. *Bashforth, Rey. Francis, B.D. Minting Vicarage, near Horncastle. tBason, Vernon Millward. 7 Princess-buildings, Clifton, Bristol. {Bassano, Alexander. 12 Montagu-place, W. {Bassano, Clement. Jesus College, Cambridge. *Basser, A. B., M.A., F.R.S. Fledborough Hall, Holyport, Berkshire. {Bassett, A. B. Cheverell, Llandaff. *BassErt, Henry. 26 Belitha-villas, Barnsbury, N. {BasrasiE, Professor C. F., M.A., F.S.S. 6 Treyelyan-terrace, Rathgar, Co. Dublin. {Bastard, 8.8. Summerland-place, Exeter. {Bastran, H. Cuarzuron, M.A., M.D., F.R.S., F.L.S., Professor of the Principles and Practice of Medicine in University College, London. 84 Manchester-square, W. {Batalha-Reis, J. Portuguese Consulate, Newcastle-upon-Tyne. {Barrman, Sir A. E., K.C.M.G., Gontroller General, Statistical Department. Board of Trade, 7 Whitehall Gardens, S.W. tBateman, Sir F., M.D., LL.D. Upper St. Giles’s-street, Norwich. {Bates, C. J. Heddon, Wylam, Northumberland. tBareson, Witt1am, M.A., F.R.S. St. John’s College, Cambridge. *BaTHER, Francis ARtHuR, M.A., D.Sc., F.G.S. British Museum (Natural History), S.W. §BavERMAN, H., F.G.S. 14 Cavendish-road, Balham, 8. W. {Baxter, Edward. Hazel Hall, Dundee. §Bayly, F. W. 8 Royal Mint, E. *Bayly, Robert. Torr-grove, near Plymouth. *Baynus, Rospert K., M.A. Christ Church, Oxford. *Baynes, Mrs. R. E. 2 Norham-gardens, Oxford. *Bazley, Gardner 8. Hatherop Castle, Fairford, Gloucestershire. _ Bazley, Sir Thomas Sebastian, Bart., M.A. Winterdyne, Chine Crescent-road, Bournemouth. {Beale, C. Calle Progress No. 83, Rosario de Santa Fé, Argentine Republic. {Beale, Charles G. Maple Bank, Edgbaston, Birmingham. *Bratz, Lionet S., M.B., F.R.S. 61 Grosvenor-street, W. §Beamish, Lieut.-Colonel A. W., R.E. 27 Philbeach-gardens, S.W. {tBeamish, G. H. M. Prison, Liverpool. ee Edward, F C.S. Moatlands, Paddock Wood, Brenchley, Kent. 12 LIST OF MEMBERS, Year of Election. 1883. t{Beard, Mrs. Oxford. + 1889. §Buarn, Prof. T. Hupson, B.Sc., F.R.S.E., M.Inst.C.E. University College, W.C., and Park House, King’s Road, Richmond. 1842. *Beatson, William. 2 Ash Mount, Rotherham. 1889. {Beattie, John. 5 Summerhill-grove, Newcastle-upon-Tyne. 1855. *Beaufort, W. Morris, F.R.A.S., F.R.G.S., F.R.M.S., F.S.S. 18 Picea- dilly, W. 1886. {Beaugrand, M.H. Montreal. } 1900. §Beaumont, Prof. Roberts, M.I.Mech.E. Yorkshire College, Leeds. 1861. *Beaumont, Rev. Thomas George. Oakley Lodge, Leamington. 1887. *Beaumont, W. J. The Laboratory, Citadel Hill, Plymouth. 1885. *Beaumont, W. W., M.Inst.C.E., F.G.S. Outer Temple, 222 Strand, W.C. 1896. {Beazer, C. Hindley, near Wigan. 1887. *Brcxerr, Joan Hamppen. Corbar Hall. Buxton, Derbyshire. 1885, {Bepparp, Frank E., M.A, F.RS., F.Z.S., Prosector to the Zoo= logical Society of London, Regent’s Park, N.W. 1870. §Beppoz, Jonny, M.D., F.R.S. The Chantry, Bradford-on-Avon. 1896, §Bedford, F. P. 326 Camden Road, N. 1858. §Bedford, James. Woodhouse Cliff, near Leeds. 1890. {Bedford, James E., F.G.S. Shireoak-road, Leeds. 1891, §Bedlington, Richard. Gadlys House, Aberdare. 1878. {Brpson, P. Puitiies, D.Sc., F.C.S., Professor of Chemistry in the College of Physical Science, Newcastle-upon-Tyne. 1884. {Beers, W.G., M.D. 84 Beaver Hull-terrace, Montreal, Canada, 1873. {Behrens, Jacob. Springfield House, North-parade, Bradford, York- shire. 1874. {Belcher, Richard Boswell. Blockley, Worcestershire. 1891. *Belinfante, L. L., M.Se., Assist.-Sec. G.S. Burlington House, W. 1892. {Bell, A. Beatson. 143 Princes-street, Edinburgh. 1871. {Bell, Charles B. 6 Spring-bank, Hull. 1884. {Bell, Charles Napier. Winnipeg, Canada. 1894, {Bynt, F. Jerrrey, M.A., F.Z.S. 35 Cambridge-street, Hyde Park, W. : Bell, Frederick John. Woodlands, near Maldon, Tssex. 1860. {Bell, Rev. George Charles, M.A. Marlborough College, Wilts. 1900. *Bell, H. Wilkinson. Holmehurst, Rawdon, near Leeds. 1862. *BxExt, Sir Issac Lowrmran, Bart., LL.D., F.R.S., F.C.S., M.Inst.0.E. Rountou Grange, Northallerton. 1875, {Brtt, Jamrs, C.B., D.Sc., Ph.D., F.R.S. Howell Hill Lodge, Ewell, Surrey. 1896. {Bell, James. Care of the Liverpool Steam Tug Co., Limited, Chapel-chambers, 28 Chapel-street, Liverpool. 1891. {Bell, James. Bangor Villa, Clive-road, Cardiff. 1871. *Brrt, J. Carrer, F.C.S, Bankfield, The Clitf, Higher Broughton, Manchester. 1883. *Bell, John Henry. 100 Leyland-road, Southport. 1864. {Bell, R. Queen’s College, Kingston, Canada. 1888, *Bell, Walter George, M.A. ‘Trinity Hall, Cambridge. 1893. {BEnpEr, The Right Hon. Lord, LL.M. Kingston, Nottinghamshire. 1884. {Bemrose, Joseph. 15 Plateau-street, Montreal, Canada. 1886. §Benger, Frederick Baden, F.LC., F.C.S. The Grange, Knutsford. 1885, {BenHam, WiLLIAM Braxtanp, D.Sc., Professor of Biology in the University of Otago, New Zealand. 1891. {Bennett, Alfred Rosling. 44 Manor Park-road, Harlesden, N.W. 1870. {Bennert, Atrrep W., M.A., B.Sc., F.L.S. 6 Park Village East, Regent’s Park, N.W. LIST OF MEMBERS. 18 Year of Election. 1896. §Bennett, George W. West Ridge, Oxton, Cheshire. 1881. §Bennett, John Ryan. 5 Upper Belgrave-road, Clifton, Bristol. 1883. *Bennett, Laurence Henry. The Elms, Paignton, South Devon, 1896. {Bennett, Richard. 19 Brunswicl-street, Liverpool. 1881. {Bennett, Rev. 8S. H., M.A. St. Mary’s Vicarage, Bishopshill Junior, York. 1889. {Benson, John G. 12 Grey-street, Newcastle-upon-Tyne. 1887. *Benson, Mrs. W. J. Care of Standard Bank of South Africa, Stel- lenbosch, South Africa. 1863. {Benson, William. Fourstones Court, Newcastle-upon-Tyne. 1898. *Bent, Mrs. Theodore. 13 Great Cumberland-place, W. 1884. {Bentham, William. 724 Sherbrooke-street, Montreal, Canada. 1897. {Bently, R. R. 97 Dowling-avenue, Toronto, Canada. 1896. *Bergin, William, M.A., Professor of Natural Philosophy in Queen’s College, Cork. 1894. §Berkeley, The Right Hon. the Earl of. Foxcombe, Boarshill, near Abingdon. 1863. {Berkley,C. Marley Hill, Gateshead, Durham. 1886. {Bernard, W. Leigh. Calgary, Canada. 1898. §Berridge, Miss C. EK. Wellscot, Hayward’s Lane, Cheltenham. 1894. §Berridge, Douglas, M.A., F.C.S. The College, Malvern. 1862. {Busant, WittrAM Heyry, M.A., D.Sc., F.R.S. St. John’s College, Cambridge. 1882. *Bessemer, Henry. Town Hill Park,West End, Southampton. 1890. {Best, William Woodham, 31 Lyddon-terrace, Leeds. 1880. *Brvan, Rev. James Ortver, M.A.,F.G.S. 55 Gunterstone-road, W. 1885. {Beveridge, R. Beath Villa, Ferryhill, Aberdeen. 1884. *Beverley, Michael, M.D. 54 Prince of Wales-road, Norwich. 1870. {Bickerton, A.W. Newland Terrace, Queen’s Road, Battersea, S.W. 1888. *Bidder, George Parker. Savile Club, Piccadilly, W. 1885. *BripwELL, SHELForD, Sc.D., LL.B., F.R.S. Riverstone Lodge, . Southfields, Wandsworth, Surrey, 8.W. 1882. §Biges, C. H. W., F.C.S. Glebe Lodge, Champion Hill, S.E. 1898. §Billington, Charles. Studleigh, Longport, Staffordshire. 1886. {Bindloss, G.F. Carnforth, Brondesbury Park, N.W. 1887. *Bindloss, James B. Elm Bank, Eccles, Manchester. 1884, *Bingham, Lieut.-Colonel John E., J.P. West Lea, Ranmoor, Sheffield. 1881. {Brnnie, Sir ALExanpER R., M.Inst.C.E., F.G.S. London County Council, Spring-gardens, 8. W. 1873. {Binns, J. Arthur. 31 Manor Row, Manningham, Bradford, York- shire. 1899. §Bird, F. J. Norton House, Midsomer Norton, Bath. 1880. {Bird, Henry, F.C.S. South Down House, Millbrook, near Devonport. 1888. *Birley, Miss Caroline. 14 Brunswick-gardens, Kensington, W. 1887. *Birley, H. K. Hospital, Chorley, Lancashire. 1871. *Biscnor, Gustav. 19 Ladbroke-gardens, W. 1894, {Bisset, James. 5 East India-avenue, F.C, 1885. {Bissett, J. P. Wyndem, Banchory, N.B. 1886, *Bixby, Major W. H. Engineer's Office, Cincinnati, Ohio, U.S.A. 1889. {Black, W. 1 Lovaine-place, Newcastle-upon-Tyne. 1889. { Black, William. 12 Romulus-terrace, Gateshead. 1881. {Black, Surgeon-Major William Galt, F.R.C.S.E. Caledonian United Service Club, Edinburgh. 1869. { Blackall, Thomas. 13 Southernhay, Eveter. 1876, {Blackburn, Hugh, M.A. Roshyen, Fort William, N.B, 14 LIST OF MEMBERS. Year of Election. 1884, {Blackburn, Robert. New Edinburgh, Ontario, Canada. 1900. §Blackburn, W. Owen. 3 Mount Royd, Bradford. 1877. {Blackie, J. Alexander. 17 Stanhope-street, Glasgow. 1855. 1896. 1884, 1883. 1896. 1886. 1895. 1883. 1892. 1892. 1883. 1846. 1891. 1894. 1900. 1881. 1895. 1884. 1869, 1887. 1887. 1887. 1884, 1880. 1888. 1870. 1859. 1885. 1867. 1887. 1870. 1887. 1900. 1889. 1884. 1887. 1898. 1876. 1894. 1898. 1898. 1883. 1871. 1888, 1893. *Brackre, W. G., Ph.D., F.R.G.S. 1 Belhaven-terrace, Kelvinside, Glasgow. §Blackie, Walter W., B.Sc. 17 Stanhope-street, Glasgow. +Blacklock, Frederick W. 25 St. Famille-street, Montreal, Canada. {Blacklock, Mrs. Sea View, Lord-street, Southport. {Blackwood, J. M. 16 Oil-street, Liverpool. ae John, F.L.S. The Bridge House, Newcastle, Stafford- shire. {Blaikie, W. B. 6 Belgrave-crescent, Edinburgh. {Blair, Mrs. Oakshaw, Paisley. {Blair, Alexander. 35 Moray-place, Edinburgh. {Blair, John. 9 Ettrick-road, Edinburgh. *Brake, Rev. J. F., M.A., F.G.8._ 69 Comeragh-road, W. *Blake, William. Bridge, South Petherton, Somerset. {BraxesLpy, THomas H., M.A., M.Inst.C.E. Royal Naval College Greenwich, 8.E. — {Blakiston, Rev. C.D. Exwick Vicarage, Exeter. *Blamires, Joseph. Bradley Lodge, Huddersfield. {Blamires, Thomas H. Close Hill, Lockwood, near Huddersfield. {Blamires, William. Oak House, Taylor Hill, Huddersfield. *Blandy, William Charles, M.A. 1 Friar-street, Reading. tBranrorp, W. T., LL.D., F.R.S., F.G.8., F.R.G.S. 72 Bedford- ardens, Campden Hill, W. *Bles, Be J. S. Palm House, Park-lane, Higher Broughton, Man- chester. *Bles, Edward J., B.Sc. Newnham Lea, Grange-road, Cambridge. {Bles, Marcus S. The Beeches, Broughton Park, Manchester. i *Blish, William G. Niles, Michigan, U.S.A. {Bloxram, G. W., M.A. 11 Presburg Street, Clapton, N.E. §Bloxsom, Martin, B.A., Assoc.M.Inst.C.E. Hazelwood, Crumpsall Green, Manchester. {Blundell, Thomas Weld. Ince Blundell Hall, Great Crosby, t{Blunt, Captain Richard, Bretlands, Chertsey, Surrey. Blyth, B. Hall. 135 George-street, Edinburgh. {Buyta, James, M.A., F.R.S.E., Professor of Natural Philosophy in Anderson’s College, Glasgow. *Blyth-Martin, W. Y. Blyth House, Newport, Fife. {Blythe, William S. 65 Mosley-street, Manchester. tBoardman, Edward. Oak House, Eaton, Norwich. *Boddingtcn, Henry. Pownall Hall, Wilmslow, Manchester. §BoprneTon, Principal N., M.A. Yorkshire College, Leeds. +Bodmer, G. R., Assoc.M.Inst.C.E. 80 Walbrook, E.C. {Body, Rey. OC. W. E.,M.A. Trinity College, Toronto, Canada. *Boissevain, Gideon Maria. 4 Tesselschade-straat, Amsterdam. §Bolton, H. The Museum, Queen’s-road, Bristol. tBolton, J. C. Carbrook, Stirling. §Bolton, John. 15 Clifton-road, Crouch End, N. tBolton, J. W. Baldwin-street, Bristol. §Bonar, J., M.A., LL.D. 1 Redington-road, Hampstead, N.W. tBonney, Frederic, F.R.G.S. Colton House, Rugeley, Staffordshire. *Bonney, Rev. Tuomas Guroren, D.Se., LL.D., F.R.S., F.S.A. F.G.S. 23 Denning-road, Hampstead, N.W, tBoon, William. Coventry. {Boot, Jesse. Carlyle House, 18 Burns-street, Nottingham, LIST OF MEMBERS. 15 Year of Election. 1890, 1883. 1883. 1876. 1883. 1900. 1876. 1882. 1876. 1896, *Bootu, Cuartus, D.Sc., F.RS., F.S.S. 24 Great Cumberland Place, W. {Booth, James. Hazelhurst, Turton. {Booth, Richard. 4 Stone-buildings, Lincoln’s Inn, W.C. {Booth, Rev. William H. Mount Nod-road, Streatham, S.W. {Boothroyd, Benjamin. Solihull, Birmingham. §Borchgrevinck, C, E. Douglas Lodge, Bromley, Kent. *Borland, William. 260 West George-street, Glasgow. ee Henry, Ph.D., F.C.S. 19 Alexandra-road, Wimbledon, urrey. *Bosanquet, R. H. M., M.A., F.R.S., F.R.A.S. Castillo Zamora, Realejo-Alto, Tenerife. tBose, Dr. J. C. Calcutta, India. *Bossey, Francis, M.D, Mayfield, Oxford-road, Redhill, Surrey. 1881. §BotHaminy, Cuartes H., F.1C., F.C.S., Director of Technical Instruction, Somerset County Education Committee, Otter- wood, Beaconsfield-road, Weston-super-Mare. 1887. {Bott, Dr. Owens College, Manchester. 1872. {Bottle, Alexander. 4 Godwyne-road, Dover. 1868. {Bottle, J.T. 28 Nelson-road, Great Yarmouth. 1887. ney, James, D.Se., B.A. 220 Lower Broughton-road, Man- chester. 1871. *Borrominy, James Tuomson, M.A., D.Sc., F.R.S., F.R.S.E., F.C.S. 13 University-gardens, Glasgow. 1884, *Bottomley, Mrs. 13 University-gardens, Glasgow. 1892. {Bottomley, W. B., B.A., Professor of Botany, King’s College, W.C. 1876. {Bottomley, William, jun. 15 University-gardens, Glasgow. 1890. {Boulnois, Henry Percy, M.Inst.C.E. 44 Campden House Court Kensington, W. : 1883. {Bourdas, Isaiah. Dunoon House, Clapham Common, S8.W. 1883, {Bourns, A. G., D.Sc., F.R.S., F.L.S., Professor of Biology in the Presidency College, Madras. ; 1893. *Bourne, G. C., M.A., F.L.S. Savile House, Mansfield-road, Oxford. 1889. {Bourne, R. H. Fox. 41 Priory-road, Bedford Park, Chiswick. 1866. §BouRNE, StepHEN. 5 Lansdown-road, Lee, S.E. 1890. {Bousfield, C. E. 55 Clarendon-road, Leeds, 1898.§§Bovey, Edward P., jun. Clifton Grove, Torquay. 1884, {Bovey, Henry T., M.A., M.Inst.C.E., Professor of Civil Engineer- 1888. 1881. 1898. 1856. 1898. 1880, 1887. 1865. 1899. 1899. 1887. 1895. 1871 ing and Applied Mechanics in McGill University, Montreal. Ontario-avenue, Montreal, Canada. {Bowden, Rey. G. New Kingswood School, Lansdown, Bath. *Bower, F. O., D.Sc., F.R.S., F.R.S.E., F.L.S., Regius Professor of Botany in the University of Glasgow. “Bowker, Arthur Frank, F.R.G.S., F.G.S. Royai Societies Club St. James’s-street, S.W. ; *Bowlby, Miss F. HE. 23 Lansdowne-parade, Cheltenham. §Bowley, A. L., M.A. Waldeck House, Southern Hill, Readine. tBowly, Christopher. Cirencester. 2 {Bowly, Mrs. Christopher. Cirencester. §Bowman, F., H., D.Sc., F.R.S.E. Mayfield, Knutsford, Cheshire. *Bowman, Herbert Lister, M.A. 13 Sheffield-gardens, Kensington We *Bowman, John Herbert. 13 Sheffield Gardens, Kensington, Ww. §Box, Alfred Marshall. Care of Cooper, Box & Co., 69 Alderman- bury, E.C. *Boycs, Rupert, M.B., Professor of Pathology, University College Liverpool. 4 » [Boyd, Thomas J. 41 Moray-place, Edinburgh, 16 Year of LIST OF MEMBERS. Election. 1865 1884, 1892. 1872. 1869. 1894. 1895. 1899. 1892. 1863. 1880. 1864. 1888. 1898. 1865. 1867. 1861. 1885. 1890. 1868. 1877. 1898. 1882. 1866. 1891. {Boytz, The Very Rev. G. D., M.A. The Deanery, Salisbury. *Boyle, R. Vicars, O.S.I. Care of Messrs. Grindlay & Co., 50 Parliament-street, 5. W. §Boys, CHaRLes VERNON, F.R.S. 27 The Grove, Boltons, S.W. *Braproox, E, W., C.B., F.S.A. 178 Bedford-hill, Balham, S.W. *Braby, Frederick, F.GS., F.C.S. Bushey Lodge, Teddington, Middlesex. *Braby, Ivon. Bushey Lodge, Teddington, Middlesex. §Bradley, F. L. Bel Air, Alderley Edge, Cheshire. *Bradley, J. W., Assoc.M.Inst.C.E, Town Hall, Wolverhampton. §Bradshaw, W. Carisbrooke House, The Park, Nottingham. {Brapy, Guorce S., M.D., LL.D., F.R.S., Professor of Natural History in the Durham College of Science, Newcastle-on-Tyne. 2 Mowbray-villas, Sunderland. *Brady, Rev. Nicholas, M.A. Rainham Hall, Rainham, 8.0., Essex. Braham, Philip. 3 Cobden-mansions, Stockwell-road, S.E. §Braikenridge, W. J., J.P. 16 Royal-crescent, Bath. §Bramble, James R. Seafield, Weston-super-Mare. §BRAMWELL, Sir FREDERICK J., Bart., D.C.L., LL.D. F.BS., M. Inst.C.E. 5 Great George-street, S.W. tBrand, William. Milnefield, Dundee. *Brandreth, Rev. Henry. 72 Hills Road, Cambridge. *Bratby, William, J.P. Alton Lodge, Hale, Bowdon, Cheshire. *Bray, George. Belmont, Headingley, Leeds. {Bremridge, Elias. 17 Bloomsbury-square, W.C. {Brent, Francis. 19 Clarendon-place, Plymouth. §Brereton, Cuthbert A., M.Inst.C.E. 21 Delahay-street, S.W. *Bretherton, C. E. 26 Old Broad Street, E.C. {Brettell, Thomas. Dudley. {Brice, Arthur Montefiore, F.G.S., F.R.G.S. 159 Strand, W.C. _ 1886.§§Briven, T. W., M.A,, D.Se., Professor of Zoology in the Mason 1870. 1887. 1870. 1886. 1879. 1870. 1890. 18938. 1868. 1893. 1884, 1898. 1879. 1878. 1884. University College, Birmingham. *Bridson, Joseph R. Bryerswood, Windermere. Brierley, John, J.P. The Clough, Whitefield, Manchester. {Brierley, Joseph. New Market-street, Blackburn. {Brierley, Leonard. Somerset-road, Edgbaston, Birmingham. tBrierley, Morgan. Denshaw House, Saddleworth. *Brice, Jonn, M.P. Kildwick Hall, Keighley, Yorkshire. {Brigg, W. A. Kildwick Hall, Keighley, Yorkshire. {Bright, Joseph. Western-terrace, The Park, Nottingham. {Brine, Admiral Lindesay, F.R.G.S. United Service Club, Pall Briscoe, Albert E., B.Sc. ,A.R.C.Se. Municipal Technical Tustitute, Romford-road, West Ham, E. {Brisette, M. H. 424 St. Paul-street, Montreal, Canada. {Bristox, the Right Rev. G. F. Browns, Lord Bishop of, D.D. 17 The Avenue, Clifton, Bristol. *Brirrain, W. H., J.P., FE.R.G.S. Storth Oaks, Sheffield. {Britten, James, F.L.S. Department of Botany, British Museum, S8.W “Brittle, John R., MInst.C.E., F.R.S.E. 9 Vanbrugh-hill, Black- heath, 8.E. 1899.§§ Broadwood, Miss Bertha M. Pleystowe, Capel, Surrey. 1899.§§ Broadwood, James H. E. Pleystowe, Capel, Surrey. 1897. {Brock, W. R. Toronto. 1896. 1883. *Brocklehurst, §. Olinda, Sefton Park, Liverpool. *Brodie, David, M.D. Care of Bernard Hollander, 61 Chancery-lane, WECE LIST OF MEMBERS. Uy Year of Election. 1884, ee William, M.D. 64 Lafayette-avenue, Detroit, Michigan, U.S.A 1883. *Brodie-Hall, Miss W.L. 5 Devonsbire-place, Eastbourne. 1881. Po, Robert G. Wolverhampton House, St. Helens, Lanca- shire. 1864, *Brooke, Ven. Archdeacon J. Ingham. The Vicarage, Halifax. 1887. §Brooks, James Howard. Elm Hirst, Wilmslow, near Man- chester. 1863. {Brooks, John Crosse. 14 Lovaine-place, Newcastle-on-Tyne. 1887. {Brooks,S. H. Slade House, Levenshulme, Manchester. 1883. *Brotherton, E. A. Arthington Hall, Wharfedale, vii Leeds. 1883. *Brough, Mrs. Charles 8. Rosendale Hall, West Dulwich, S.E. 1886. {Brough, Professor Joseph, LL.M., Professor of Logic and Philosophy in University College, Aberystwith. 1885. *Browett, Alfred. 29 Wheeley’s-road, Birmingham. 1863. *Brown, ALEXANDER ORvM, M.D., LL.D., F.R.S., F.R.S.E. , V.P.C.S., Professor of Chemistry in the University of Edinburgh. 8 Bel- grave-crescent, Edinburgh. 1892, {Brown, Andrew, M.Inst.C.E. Messrs. Wm. Simons & Co., Renfrew, near Glasgow. 1896. {Brown, A. T. The Nunnery, St. Michael’s Hamlet, Liverpool. 1867. {Brown, Sir Charles Gage, M.D., K.C.M.G. 88 Sloane-street, S.W. 1855. {Brown, Colin. 192 Hope-street, Glasgow. 1871. {Brown, David. Willowbrae House, Midlothian. 1863, *Brown, Rey. Dixon. Unthank Hall, Haltwhistle, Carlisle. 1883. tBrown, Mrs. Ellen F. Campbell. 27 Abercromby-square, Liverpool. 1881. {Brown, Frederick D. 26 St. Giles’s-street, Oxford. 1883. {Brown, George Dransfield. Henley Villa, Ealing, Middlesex, W. 1883. “Brown, Mrs. H. Bienz. Fochabers, Morayshire. 1883. {Brown, Mrs. Helen. Canaan-grove, Newbattle-terrace, Edinburgh. 1870. §Brown, Horace T., LL.D., F.R.S., F.G.S. 52 Nevern-square, S.W. Brown, Hugh. Broadstone, Ayrshire. 1883. {Brown, Miss Isabella Spring. Canaan-grove, Ni ewbattle-terrace, Edinburgh. 1895. {Brown, J. Auten, J.P., F.R.GS. FGS. 7 Kent-gardens, Ealing, W. 1870. *Brown, Professor J. Campsett, D.Sc., F.C.S. University College, Liverpool. 1876. §Brown, John. Longhurst, Dunmurry, Belfast. 1881. *Brown, John, M.D. Stockbridge House, Padisham, Lancashire, 1882. *Brown, John. 7 Second-avenue, Nottingham, 1895. *Brown, John Charles. 2 Baker-street, Nottingham. 1894, {Brown, J. H. 6 Cambridge-road, Brighton. 1882. *Brown, Mrs. Mary. Stockbridge House, Padisham, Lancashire. 1898. §Brown, Nicol, F.G.S. 4 The Grove, Highgate, N. 1897. {Brown, Price, M.B. 37 Carlton-street, Toronto, Canada. 1886, §Brown, R., R.N. Laurel Bank, Barnhill, Perth. 1863, {Brown, Ralph. Lambton’s Bank, Newcastle~upon-Tyne. 1897. {Brown, Richard. Jarvis-street, Toronto, Canada. 1896. {Brown, Stewart H. Quarry Bank, Allerton, Liverpool. 1891. §Brown, aie Forstar, M.Inst.C.E., F.G.S. Guild Hall Chambers, Cardiff. 1865. {Brown, William. 414 New-street, Birmingham. 1885. {Brown, W. A. The Court House, Aberdeen. 1884, {Brown, William George. Ivy, Albemarle Oo., Virginia, U.S.A. 1863. {Browne, Sir Benjamin Chapman, M.Inst.C.E. Westacres, New- castle-upon-Tyne. 1900, B 18 Year LIST OF MEMBERS. of Election. 1900. §Browne, Frank Balfour. Goldielea, Dumfries, Scotland. 1892. t Browne, Harold Crichton. Crindon, Dumfries. 1895. *Browne, H. T. Doughty. 10 Hyde Park-terrace, W. 1879, {Browne, Sir J. Cricuton, M.D.,LL.D., F.R.S.,F.R.S.E. 61 Carlisle- 1891. 1862. 1872. 1887. 1865. 1885. place-mansions, Victoria-street, S.W. {Browne, Monracu, F.G.S. Town Museum, Leicester. *Browne, Robert Clayton, M.A. Browne’s Hill, Carlow, Ireland. tBrowne, R. Mackley, F.G.S. Redcot, Bradbourne, Sevenoaks, Kent. tBrownell, T. W. 6 St. James’s-square, Manchester. {Browning, John, F.R.A.S. 63 Strand, W.C. t{Browning, Oscar, M.A. King’s College, Cambridge. 1855. { Brownlee, James, jun. 30 Burnbank-gardens, Glasgow. 1892. {Bruce, James. 10 Hill-street, Edinburgh. 1893. {Bruce, William S. 11 Mount Pleasant, Joppa, Edinburgh. 1900. *Brumm, Charles. Lismara, Grosvenor Road, Birkdale, Southport. 1863. *Brunel, H. M., M.Inst.C.E. 21 Delahay-street, Westminster, S.W. 1863. {Brunel, I. 15 Devonshire-terrace, W. 1875. {Brunlees, John, M.Inst.C.E. 12 Victoria-street, Westminster, S.W. 1896. *Brunner, Sir J.T., Bart., M.P. Druid’s Cross, Wavertree, Liverpool. 1868. {Brunton, Sir T. Lauper, M.D., D.Sc., F.R.S. 10 Stratford-place, Oxford-street, W. 1897. *Brush, Charles F. Cleveland, Ohio, U.S.A. 1878.§§Brutton, Joseph. Yeovil. 1886 1894, 1884. 1897. . *Bryan, G. HH D.Sc, F.R.S., Professor of Mathematics in University College, Bangor. {Bryan, Mrs. R. P. Plas Gwyn, Bangor. {Brycz, Rev. Professor GeorcE. Winnipeg, Canada. {Bryce, Right Hon. James, D.C.L., M.P., F.R.S. 54 Portland- place, 1894. {Brydone, R. M. Petworth, Sussex. 1890. 1871. 1867. 1881. 1871. 1884. 1883, 1886. 1865. 1886 1884 1851 1887. 1875. 1883. 1893. 1871. 1885. 1895. 1886. 1842. 1869, §Bubb, Henry. Ullenwood, near Cheltenham. §Bucwan, ALEXANDER, M.A., LL.D., F.R.S., F.R.S.E., Sec. Scottish Meteorological Society. 42 Heriot-row, Edinburgh. {Buchan, Thomas. Strawberry Bank, Dundee. *Buchanan, John H., M.D. Sowerby, Thirsk. t{Bucwanan, Joun Youns, M.A., F.R.S., F.R.S.E., F.R.G.S., F.C.8, 10 Moray-place, Edinburgh. {Buchanan, W. Frederick. Winnipeg, Canada. {Buckland, Miss A. W. 5 Beaumont-crescent, West Kensington, W. *Buckle, Edmund W. 238 Bedford-row, W.C. * Buckley, Henry. 18 Princes-street, Cavendish-square, W. .§§Buckley, Samuel. Merlewood, Beaver Park, Didsbury. . *Buckmaster, Charles Alexander, M.A., F.0.8. 16 Heathfield-road, Mill Hill Park, W. . *Bucxron, Grorce Bowpter, F.R.S., F.L.S., F.C.S. Weycombe, Haslemere, Surrey. {Budenberg, C. F., B.Sc. Buckau Villa, Demesne-road, Whalley Range, Manchester. tBudgett, Samuel. Penryn, Beckenham, Kent. {Buick, Rev. George R., M.A. Cullybackey, Co. Antrim, Ireland, §BuLLerp, ARTHUR, F.S.A. Glastonbury. {Bulloch, Matthew. 48 Prince’s-gate, S.W {Bulpit, Rev. F. W. Crossens Rectory, Southport. {Bunte, Dr. Hans. Karlsruhe, Baden. §Bursury, 8. H., M.A., F.R.S. 1 New-square, Lincoln’s Inn, W.C. *Burd, John. Glen Lodge, Knocknerea, Sligo. {Burdett-Coutts, Baroness. 1 Stratton-street, Piccadilly, W. LIST OF MEMBERS. 19 Year of Election. 1881. {Burdett-Coutts, W.L.A.B., M.P. 1Stratton-street, Piccadilly, W. 1891. {Burge, Very Rev. T. A. Ampleforth Cottage, near York. 1894. {Burxn, Jonny, B. B. Trinity College, Cambridge. 1884. *Burland, Lieut.-Col. Jeffrey H. 824 Sherbrook-street, Montreal, Canada. 1899. §Burls, Herbert T. 206 Lewisham High-road, 8.E. 1888. {Burne, H. Holland. 28 Marlborough-buildings, Bath. 1883. *Burne, Major-General Sir Owen Tudor, G.C.LE., K.C.S8.L,F.R.G.S. 132 Sutherland-gardens, Maida Vale, W. 1876. {Burnet, John. 14 Victoria-crescent, Dowanhill, Glasgow. 1885. *Burnett, W. Kendall, M.A. 11 Belmont-street, Aberdeen. 1877. {Burns, David. Alston, Carlisle. 1884, {Burns, Professor James Austin. Southern Medical College, Atlanta, Georgia, U.S.A. 1899.§§Burr, Malcolm. Dorman’s Park, East Grinstead. 1887. {Burroughs, Eggleston, M.D. Snow Hill-buildings, E.C. 1883. *Burrows, Abraham. Russell House, Rhyl, North Wales. 1860, {Burrows, Montague, M.A., Professor of Modern History, Oxford, 1894. {Burstall, H. F. W. 76 King’s-road, Camden-road, N. W. 1891. tBurt, J. J. 103 Roath-road, Cardiff. 1888. {Burt, John Mowlem. 3St.John’s-gardens, Kensington, W. 1888. {Burt, Mrs. 3 St. John’s-gardens, Kensington, W. 1894. {Burton, Charles V. 24 Wimpole-street, W. 1866. *Burron, Frepericx M., F.L.S., F.G.S. Highfield, Gainsborough, 1889. ¢Burton, Rev. R. Lingen. Little Aston, Sutton Coldfield. 1897. {Burton, 8. H., M.B. 50 St. Giles’s-street, Norwich. 1892. {Burton-Brown, Colonel Alexander, R.A., F.R.A.S., F.G.S. 11 Union Crescent, Margate. 1897. {Burwash, Rev. N., LL.D., Principal of Victoria University, Toronto, Canada. 1887. *Bury, Henry. Trinity College, Cambridge. 1899. §Bush, Anthony. 48 Portland-road, Nottingham. 1895. §Bushe, Colonel C. K., F.G.S. 19 Cromwell-road, S. W. 1878. {Burcusr, J.G., M.A. 22 Collingham-place, 8. W. 1884. *Butcher, William Deane, M.R.C.S.Eng. Holyrood, 5 Cleveland- road, Ealing, W. 1884. {Butler, Matthew I. Napanee, Ontario, Canada. 1884, *Butterworth, W. Park Avenue, Temperley, near Manchester. 1872. {Buxton, Charles Louis. Cromer, Norfolk. 1883. {Buaxton, Miss F. M. Newnham College, Cambridge. 1887. *Buxton, J. H. Clumber Cottage, Montague-road, Felixstowe. 1881. {Buxton, Sydney. 15 Eaton-place, S.W. 1868. {Buxton, S. Gurney. Catton Hall, Norwich. 1872. {Buxton, Sir Thomas Fowell, Bart., G.C.M.G., F.R.G.S. Warlies, Waltham Abbey, Hssex. 1854, {ByErtey, Isaac, F.L.S. 22 Dingle-lane, Toxteth Park, Liverpool. 1899. §Byles, Arthur R. ‘Bradford Observer,’ Bradford, Yorkshire. 1885. {Byres, David. 63 North Bradford, Aberdeen. 1852. {Byrne, Very Rev. James. Ergenagh Rectory, Omagh. 1883. {Byrom, John R. Mere Bank, Fairfield, near Manchester. 1889. {Cackett, James Thoburn. 60 Larkspur-terrace, Newcastle-upon- 'yne. 1892. {Cadell, Henry M., B.Sc., F.R.S.E. Grange, Bo’ness, N.B. , 1894, {Caillard, Miss E. M. Wingfield House, near Trowbridge, Wilts. 1863, {Caird, Edward. Finnart, Dumbartonshire, B2 20 LIST OF MEMBERS. Year of Election. 1861. *Caird, James Key. 8 Roseangle, Dundee. 1886. *Caldwell, William Hay. Cambridge. 1868. {Caley, A. J. Norwich. 1887. {Cartaway, CuartEs, M.A., D.Se., F.G.S. 35 Huskisson-street, Liverpool. 1897. §CaLLENDAR, Prof. Hueu L.,M.A.,F.R.S. University College, Gower Street, W.C., and 2 Chester Place, Regent’s Park, N.W. 1892. {Calvert, A. F., F.R.G.S, Royston, Eton-avenue, N.W. 1884. {Cameron, Aineas. Yarmouth, Nova Scotia, Canada. 1876. {Cameron, Sir Charles, Bart., M.D., LL.D. 1 Huntly-gardens, Glasgow. 1857. Se Sir Cuarters A., C.B., M.D. 15 Pembroke-road, Dublin 1896. §Cameron, Irving H. 307 Sherbourne-street, Toronto, Canada. 1884. {Cameron, James C., M.D. 41 Belmont-park, Montreal, Canada. 1870. {Cameron, John, M.D. 17 Rodney-street, Liverpool. 1884, {Campbell, Archibald H. Toronto, Canada. 1876. oa Nich dre Hon. James A., LL.D., M.P. Stracathro House, rechin. Campbell, John Archibald, M.D., F.R.S.E. Albyn-place, Edinburgh. 1897. {Campbell, Major J. C. L. New Club, Edinburgh. 1898.§§Camphell, Mrs. Napier. 81 Ashley-gardens, S.W. 1897, {Campion, B. W. Queen’s College, Cambridge. 1882. {Candy, F. H. 71 High-street, Southampton. 1890. {Cannan, Epwin, M.A., F.S.8. 1 Wellington Square, Oxford. 1897. §Cannon, Herbert. Woodbank, Erith, Kent. 1898, {CawreRBuRY, Right Hon. and Most Rev. F. Tempre, Lord Archbishop of. Lambeth Palace, S.E. 1888. {Cappel, Sir Albert J. L., K.C.LE, 27 Kensington Court-gardens, London, W. 1894, §Capper, D. S., M.A., Professor of Mechanical Engineering in King’s College, W.C. 1883. {Capper, Mrs. R. 9 Bridge-street, Westminster, S.W. 1887. {Capstick, John Walton. University College, Dundee. 1873. *Carpurt, Sir Epwarp Hamer, Bart., M.Inst.C.E. 19 Hyde Park- gardens, W. 1896, *Carden, H. V. Balinveney, Bookham, Surrey. 1877. {Carkeet, John. 3 St. Andrew’s-place, Plymouth. 1898, {Carlile, George M. 7 Upper Belgrave-road, Bristol. 1867. {Carmichael, David (Engineer). Dundee. 1897, {Carmichael, Norman R. Queen’s University, Kingston, Ontario, Canada. 1884. {Carnegie, John. Peterborough, Ontario, Canada. 1884. Tiare Louis G. Agricultural College, Fort Collins, Colorado, USA 1897. {Carpenter, R. C. Cornell University, Ithaca, New York, U.S.A. 1889. {Carr, Cuthbert Ellison. Hedgeley, Alnwick. 1893. {Carr, J. Wustny, M.A., F.L.S., F.G.S., Professor of Biology in University College, Nottingham. 1889. {Carr-Ellison, John Ralph. Hedgeley, Alnwick. 1867. {CarrurHEeRs, WiutiraM, F.R.S., F.L.8., F.G.S. 14 Vermont- road, Norwood, 8.E. 1886. {CarstaKe, J. BarnaM. 3O Westfield-road, Birmingham. 1899. §Carslaw, H.8., D.Sc. The University, Glasgow. 1883. {Carson, John. 51 Royal-avenue, Belfast. 1868. *Carteiche, Michael, I°.C.S., F.L.C. 180 New Bond-street, W. a LIST OF MEMBERS. 21 Year of Election. 1897.§§Carter, E. Tremlett. ‘The Electrician, Salisbury Court, Fleet 1866. 1870. 1885. 1900, 1883. 1896. 1878. 1870, 1862. 1894. 1884. 1884. 1887. 1897. 1896. 1871. 1873. 1900. 1897. 1888. 1874, 1859. 1886, 1883. 1859. 1883. 1884. 1883. 1881. 1865. 1865. 1865. 1888, 1861. 1897. 1889. 1900. 1884. 1899. 1877. 1874. 1874, 1866. Street, E.C. {Oarter, H. H. The Park, Nottingham. {Carter, Dr. William. 78 Rodney Street, Liverpool. {Carter, W. C. Manchester and Salford Bank, Southport. *Carter, Rev. W. Lower, F.G.S. Hopton, Mirfield. tCarter, Mrs. Manchester and Salford Bank, Southport. §Cartwright, Miss Edith G. 21 York Street Chambers, Bryanston Square, W. *Cartwright, Ernest H., M.A., M.D. Bower Terrace, Maidstone. §Cartwright, Joshua, M.Inst.C.E., F.S.I., Borough and Water Engineer. Albion-place, Bury, Lancashire. tCarulla, F. J. R. 84 Argyll-terrace, Derby. {Carus, Paul. La Salle, Illinois, U.S.A. *Carver, Rey. Canon Alfred J., D.D.,F.R.G.S. Lynnhurst, Streatham Common, 8.W. {Carver, Mrs. Lynnhurst, Streatham Common, S.W. {Casartelli, Rev. L. C., M.A., Ph.D. St. Bede’s College, Manchester. *Case, Willard E. Auburn, New York, U.S,A. *Casey, James. 10 Philpot-lane, H.C. {Cash, Joseph. Bird-grove, Coventry. *Cash, William, F.G.S. 35 Commercial-street, Halifax. *Cassie, W., M.A. Professor of Physics in the Royal Holloway College, Brantwood, Englefield Green. {Caston, Harry Edmonds Featherston. 340 Brunswick-avenue, Toronto, Canada. { Cater, R. B. Avondale, Henrietta Park, Bath. {Caton, Richard, M.D. Lea Hall, Gateacre, Liverpool. tCatto, Robert. 44 Kine-street, Aberdeen. *Cave-Moyles, Mrs. Isabella. Lancaster House, 102 Palace-road, Tulse Hill, S.W. Cayley, Digby. Brompton, near Scarborouch. Cayley, Edward Stillingfleet. Weydale, Malton, Yorkshire. {Chadwick, James Percy. 51 Alexandra-road, Southport. tChalmers, John Inglis. Aldbar, Aberdeen. {Chamberlain, George, J.P. Helensholme, Birkdale Park, Southport. {Chamberlain, Montague. St. John, New Brunswick, Canada. {Chambers, Mrs. Bombay. *Champney, John EK. 27 Hans Place, S.W. {Chance, A. M. Edgbaston, Birmingham. *Chance, Sir James T., Bart. 1 Grand-avenue, Brighton. tChance, Robert Lucas. Chad Hill, Edgbaston, Birmingham. {Chandler, S. Whitty, B.A. Sherborne, Dorset. *Chapman, Edward, M.A., M.P., F.L.S., F.C.S. Hill End, Mottram, Manchester... {Chapman, Edward Henry. 17 St. Hilda’s-terrate, Whitby. JChapman, L. H. 147 Park-road, Newcastle-upon-Tyne. §Chapman, L. J. 79 St. Bees Street, Moss Lane East, Manchester. Chapman, Professor. University College, Toronto, Canada. §Chapman, Sydney John. University College, Cardiff. f{Chapman, T. Algernon, M.D. 17 Wesley-avenue, Liscard, Cheshire. tCharles, J. J.,. M.D., Professor of Anatomy and Physiology in Queen’s College, Cork. Newmarket, Co. Cork. {Charley, William. Seymour Hill, Dunmurry, Ireland. t Charnock, Richard Stephen, Ph.D., FSA. Crichton Club, Adelphi- terrace, W.C. 22 LIST OF MEMBERS, ‘Year of Election. 1886. {Chate, Robert W. Southfield, Edgbaston, Birmingham. 1884, *Chatterton, George, M.A., M.Inst.0.E. 6 The Sanctuary, West- minster, S. W. p. ahe) 1886. *Chattock, A. P., M.A., Professor of Experimental Physics in University College, Bristol. 1867. *Chatwood, Samuel, F.R.G.S. High Lawn, Broad Oak Park, Worsley, Manchester. 1884, {CHAuvEAv, The Hon. Dr. Montreal, Canada. 1883. {Chawner, W., M.A. Emmanuel College, Cambridge. 1864, {CHEaptE, W. B., M.A., M.D., F.R.G.S. 19 Portman-street, Portman-square, W. 1900. §Cheesman, W. Norwood. The Crescent, Selby. 1887. {Cheetham, I’, W. Limefield House, Hyde. 1887. {Cheetham, John. Limefield House, Hyde. 1896, tChenie, John. Charlotte-street, Edinburgh. 1874. *Chermside, Major-General Sir H. C., R.E., G.C.M.G.,0.B. Care of Messrs. Cox & Co., Craig’s-court, Charing Cross, 8. W. 1884, {Cherriman, Professor J. B. Ottawa, Canada. 1896. {Cherry, R. B. 92 Stephen’s Green, Dublin. 1879. *Chesterman, W. Belmayne, Sheffield. 1883. {Chinery, Edward F. Monmouth House, Lymington. 1884. {Chipman, W. W. L. 957 Dorchester-street, Montreal, Canada. 1889. {Chirney, J. W. Morpeth. 1894. {Chisholm, G. G., M.A., B.Sc, F.R.G.S. 59 Drakefield Road, Upper Tooting, 8. W. 1899. §Chitty, Edward. Suffolk House, London-road, Dover. 1899, §Chitty, Mrs. Edward. Suffolk House, London-road, Dover. 1899. §Chitty,G. W. Mildura, Park-avenue, Dover. 1882. {Chorley, George. Midhurst, Sussex. 1887. tChorlton, J. Clayton. New Holme, Withington, Manchester. 1895. *CurEn, Cuartns, D.Sc., F.R.S., Superintendent of the Kew Observatory, Richmond, Surrey. 1900. *Christie, R. J. Duke Street, Toronto, Canada. 1884, *Christie, William. 29 Queen’s Park, Toronto, Canada. 1875. *Christopher, George, F.C.S. May Villa, Lucien-road, Tooting Common, 8. W. 1876. *Curystat, Grorer, M.A., LL.D., F.R.S.E., Professor of Mathe- matics in the University of Edinburgh. 5 Belerave-crescent, Edinburgh, 1870, §Cauron, A. H., M.A., F.R.S., F.S.A., Professor of Chemistry in the Royal Academy of Arts. Shelsley, Hnnerdale-road, Kew. 1898. §CHuRcH, Colonel G. Eart, F.R.G.S. 216 Cromwell-road, 8. W. 1860. {CHuRcH, Sir WrrrraAm Supy, Bart., M.D. St. Bartholomew’s Hospital, E.C. 1896. §Clague, Daniel, F.G.S. 5 Sandstone-road, Stoneycroft, Liverpool. 1890. {Clark, E. K. 13 Wellclose-place, Leeds. 1877. *Clark, F. J., J.P., F.L.S. Netherleigh, Street, Somerset. Clark, George T. 44 Berkeley-square, W. 1876. {Clark, George W. 31 Waterloo-street, Glasgow. 1892. {Clark, James, M.A., Ph.D., Professor of Agriculture in the York- shire College, Leeds. 1892. {Clark, James. Chapel House, Paisley. 1876, {Clark, Dr. John. 138 Bath-street, Glaseow. 1881. {Clark, J. Edmund, B.A., B.Sc. 112 Wool Exchange, E.C. 1855, {Clark, Rev. William, M.A. Barrhead, near Glasgow. 1887. §Clarke, C. Goddard, J.P. Fairlawn, 157 Peckham-rye, S.E. 1875, {Clarke, Charles S. 4 Worcester-terrace, Clifton, Bristol. LIST OF MEMBERS, 23 f Hleotion. 1886. {Olarke, David. Langley-road, Small Heath, Birmingham. 1886. {Clarke, Rev. H. J. Great Barr Vicarage, Birmingham. 1875. {CxarKxn, Joun Henry. 4 Worcester-terrace, Clifton, Bristol. 1897. §Clarke, Colonel S. C., R.E. Parklands, Caversham, near Reading. 1883. {Clarke, W. P., J.P. 15 Hesketh-street, Southport. 1896, §Clarke, W. W. Albert Dock Office, Liverpool. 1884. {Claxton, T. James. 461 St. Urbain-street, Montreal, Canada, 1889. §CraypeEn, A. W., M.A., F.G.S. St. John’s, Polsloe-road, Exeter. 1866, {Clayden, P. W. 13 Tavistock-square, W.C. 1890, *Clayton, William Wikely. Gipton Lodge, Leeds. 1859. {Cleghorn, John. Wick. 1875. {Clegram, T. W. B. Saul Lodge, near Stonehouse, Gloucestershire. 1861. §CreLanp, Jonny, M.D., D.Sc., F.R.S., Professor of Anatomy in the University of Glasgow. 2 The University, Glasgow. 1861. *Oxrrron, R. Betamy, M.A., F.R.S., F.R.A.S., Professor of Experi- mental Philosophy in the University of Oxford. 3 Bardwell- road, Banbury-road, Oxford. 1898. {Clissold, H. 30 College-road, Clifton, Bristol. 1893. {Clofford, William. 36 Mansfield-road, Nottingham. Clonbrock, Lord Robert. Clonbrock, Galway. 1878. §Close, Rev. Maxwell H., F.G.S. 38 Lower Baggot-street, Dublin. 1873. {Clough, John. Bracken Bank, Keighley, Yorkshire. 1892. tClouston, T. S., M.D. Tipperlinn House, Edinburgh. 1883. *Crowns, Franx, D.Sc., F.C.S. London County Council, Spring- gardens, S.W., and 17 Bedford Court-mansions, W.C. 1863. *Clutterbuck, Thomas. Warkworth, Acklington. 1881. *Clutton, William James. The Mount, York. 1885. {Clyne, James. Rubislaw Den South, Aberdeen. 1891. *Coates, Henry. Pitcullen House, Perth. . 1897. {Coates, J., M.Inst.C.E. 99 Queen-street, Melbourne, Australia. 1884, §Cobb, John. Westfield, Ilkley, Yorkshire. 1895. *Cossorp, Fenix T., M.A. The Lodge, Felixstowe, Suffolk. 1889. {Cochrane, Cecil A. Oakfield House, Gosforth, Newcastle-upon-Tyne. 1864. *Cochrane, James Henry. Burston House, Pittville, Cheltenham. 1889. {Cochrane, William. Oakfield House, Gosforth, Newcastle-upon-Tyne. 1892. {Cockburn, John. Glencorse House, Milton Bridge, Edinburgh. 1883. {Cockshott, J. J. 24 Queen’s-road, Southport. 1861. *Coe, Rev. Charles C., F.R.G.S. Whinsbridge, Grosvenor-road, Bournemouth. 1898.§§Coffey, George. 5 Harcourt-terrace, Dublin. 1881. *Corrin, Watter Harris, F.C.8S. 94 Cornwall-gardens, South Kensington, 8.W. 1896. *Coghill, Perey de G. 4 Sunnyside, Prince’s Park, Liverpool. 1884. *Cohen, B. L., M.P. 30 Hyde Park-gardens, W 1887. tCohen, Julius B. Yorkshire College, Leeds. 1894. *Colby, Miss E. L., B.A. Carregwen, Aberystwyth. 1895. *Colby, James George Ernest, M.A., F.R.C.S, Malton, Yorkshire, 1895. *Colby William Henry. Carregwen, Aberystwyth. 1803. tCole, Prof. Grenville A. J., F.G.S. Royal College of Science, Dublin. 1879, {Cole, Skelton. 387 Glossop-road, Sheffield. 1864. {Colefax, H. Arthur, Ph.D., F.C.S. 14 Chester-terrace, Chester- square, S.W. 1897. §Coteman, Dr. A. P. 476 Huron-street, Toronto, Canada. 1893. tColeman, J. B., F.C.S., A.R.C.S. University College, Nottingham, 1899. §Coleman, William. The Shrubbery, Buckland, Dover. 1878. {Coles, John. 1 Savile-row, W. 1854. *Colfox, William, B,A. Westmead, Bridport, Dorsetshire. 24 Year LIST OF MEMBERS. of Election. 1899 . §Collard, George. The Gables, Canterbury. 1892. {Collet, Miss Clara E. 7 Coleridge-road, N. 1892. 1887. 1869. 1895. 1854. 1861. 1876. 1865. 1882. 1884, 1897, 1896. 1888. 1884. 1891. 1900. 1892. 1884. 1896. 1890. 1871. 1893. 1899. 1898. 1900. 1882. 1876. 1881. 1868. 1895. 1868. 1884. 1878. 1881. 1865. 1896. 1888. 1899, 1895, 1893. 1883. 1868. {Collie, Alexander. Harlaw House, Inverurie. {Cottre, J. Norman, Ph.D., F.R.S., Professor of Chemistry to the Pharmaceutical Society of Great Britain. 16 Campden-grove, W. {Collier, W. F. Woodtown, Horrabridge, South Devon. {Collinge, Walter E. Mason College, Birmingham. {Cottinewoop, Curuperr, M.A., M.B., F.L.S. 69 Great Russell- street, W.C. *Collingwood, J. Frederick, F.G.S. 5 Irene-road, Parson’s Green, tCottins, J. H., F.G.S. 162 Barry-road, S.E. *Collins, James Tertius. Churchfield, Edgbaston, Birmingham. {Colmer, Joseph G.,C.M.G. Office of the High Commissioner for Canada, 17 Victoria-street, S.W. t{Colomb, Sir J.C. R., M.P., F.R.G.S. Dromquinna, Kenmare, Kerry, Treland; and Junior United Service Club, S.W. {Colquhoun, A. H. U., B.A. 39 Borden-street, Toronto, Canada, *Comber, Thomas, F.L.S. Leighton, Parkgate, Chester. {Commans, R. D. Macaulay-buildings, Bath. tCommon, A. A., LL.D.,F.R.S., F.R.A.S. 63 Eaton-rise, Ealing, W. tCommon, J. F. F. 21 Park-place, Cardiff. §Common, T. A., B.A. 63 Eaton Rise, Ealing, W. t+Comyns, Frank, M.A., F.C.S. The Grammar School, Durham. {Conklin, Dr. William A. Central Park, New York, U.S.A. t{Connacher, W.S. Birkenhead Institute, Birkenhead. {Connon, J. W. Park-row, Leeds. *Connor, Charles C, 4 Queen’s Elms, Belfast. {Conway, Sir W. M., M.A., F.R.G.8S. The Red House, Hornton- street, W. §Coopz, J. Cuartes, M.Inst.C.E. Westminster-chambers, 9 Vic- toria-street, S. W. §Cook, Ernest H. 27 Berkeley-square, Clifton, Bristol. §Cook, Walter. 98 St. Mary’s Street, Cardiff. {Cooxr, Major-General A. C., R.E., O.B., F.R.G.S. Palace-chambers, Ryder-street, 8. W. *CooKE, ConrAD W. 28 Victoria-street, 8. W. {Cooke, F. Bishopshill, York. {Cooke, Rev. George H. Wanstead Vicarage, near Norwich. {Cooke, Miss Janette E. Holmwood, Thorpe, Norwich. tCooxn, M.C.,M.A. 53 Castle Road, Kentish Town, N.W. {Cooke, R. P. Brockville, Ontario, Canada. {Cooke, Samuel, M.A., F.G.S. Poona, Bombay. {Cooke, Thomas. Bishopshill, York. {Cooksey, Joseph. West Bromwich, Birmingham. t{Cookson, E. H. Kiln Hey, West Derby. TCooley, George Parkin. Cavendish Hill, Sherwood, Nottingham. *Coomara Swamy, A. K. Walden, Worplesdon, Guildford, tCooper, Charles Friend, M.I.E.E. 68 Victoria-street, Westminster, S.W {Cooper, F.W. 14 Hamilton-road, Sherwood Rise, Nottingham, {Cooper, George B. 67 Great Russell-street, W.C. tCooper, W. J. New Malden, Surrey. 1889. {Coote, Arthur. The Minories, Jesmond, Newcastle-upon-Tyne. 1878. 1871. tCope, Rev. 8. W. Bramley, Leeds. {CopeLann, Ratpn, Ph.D., F.R.A.S., Astronomer Royal for Scotland and Professor of Astronomy in the University of Edinburgh. — a LIST OF MEMBERS, 25 Year of Election. 1885. 1881. 1891. 1887. 1894. 1883. 1870. 1893. 1889. 1884. 1885. 1888. 1900. 1891. 1891, 1883. 1891. 1874. 1864, 1869. 1876. 1876. 1889. 1896. 1890. 1896, 1863. 1868. 1872. 1900. 1895. 1871. 1899. 1867. 1867. 1892. 1882. 1888. 1867. 1883. 1890. 1892. 1884, 1876. 1884, {Copland, W., M.A. Tortorston, Peterhead, N.B. {Copperthwaite, H. Holgate Villa, Holgate-lane, York. Corbett, E. W.M. Y Fron, Pwllypant, Cardiff. *Corcoran, Bryan. Fairlight, Oliver Grove, South Norwood, S.E. §Corcoran, Miss Jessie R. The Chestnuts, Mulgrave-road, Sutton, Surrey. *Core, Professor Thomas H., M.A. Fallowfield, Manchester. *CorrieLD, W. H., M.A., M.D., F.C.S., F.G.S., Professor of Hygiene and Public Health in University College, London. 19 Savile- row, W. *Corner, Samuel, B.A., B.Sc. 95 Forest-road West, Nottingham. {Cornish, Vaughan, M.Sc., F.R.G.S. Branksome Cliff, Branksome Park, Bournemouth. *Cornwallis, F. 8. W., M.P., F.L.S. Linton Park, Maidstone. tCorry, John. Rosenheim, Park Hill-road, Croydon. tCorser, Rey. Richard K. 57 Park Hill-road, Croydon. §Cortie, Rev. A. L., F.R.A.S. Stonyhurst College, Blackburn. tCory, John, J.P. Vaindre Hall, near Cardiff. tCory, Frain: Richard, J.P. Oscar House, Newport-road, Car- ‘ti iff, {Costelloe, B. F. C., M.A., B.Sc. 33 Chancery-lane, W.C. *Cotsworth, Haldane Gwilt. The Cedars, Cobham Road, Norbiton, S.W *Correritt, J.H., M.A., F.R.S. 15 St. Alban’s-mansions, Kensing- ton Court-gardens, W. {Corron, General FrepErick C., R.E., C.S.I. 13 Longridge-road, Earl’s Court-road, 8. W. tCorroy, Wiitram. Pennsylvania, Exeter. Couper, James. City Glass Works, Glasgow. {Couper, James, jun. City Glass Works, Glasgow. {Courtney, F. S. 77 Redcliffe-square, South Kensington, S.W. {Courtyey, Right Hon. Leonarp. 15 Cheyne Walk, Chelsea, S.W. tCousins, John James. Allerton Park, Chapel Allerton, Leeds. {Coventry, J. 19 Sweeting-street, Liverpool. Cowan, John. Valleyfield, Pennycuick, Edinburgh. {tCowan, John A. Blaydon Burn, Durham. {tCowan, Joseph, jun. Blaydon, Durham. *Cowan, Thomas William, F.L.S., F.G.8, 17 King William-street, Strand, W.C. §Cowburn, Henry. Dingle Head, Westleigh, Leigh, Lancashire. *CowE LL, Puitie H., M.A. Royal Observatory, Greenwich, S.E. {Cowper, C. E. 6 Great George-street, Westminster, S.W. §Cowper-Coles, Sherard. 82 Victoria-street, S.W. *Cox, Edward. Cardean, Meigle, N.B. *Cox, George Addison. Beechwood, Dundee. tCox, Robert. 84 Drumsheugh-gardens, Edinburgh. tCox, Thomas A., District Engineer of the S., P., and D. Railway Lahore, Punjab. Care of Messrs. Grindlay & Co., Parliament- street, S.W. tCox, Thomas W. B. The Chestnuts, Lansdowne, Bath. $Cox, William. JF oggley, Lochee, by Dundee. {Crabtree, William. 126 Manchester-road, Southport. tCradock, George. Wakefield. *Craig, George A. 66 Idge-lane, Liverpool. §Craicre, Major P. G.,F.S.S. 6 Lyndhurst-road, Hampstead, N.W. ${Cramb, John. Larch Villa, Helensburgh, N.B, {Crathern, James. Sherbrooke-street, Montreal, Canada. 26 LIST OF MEMBERS, Year of Election. 1887. 1887. 1871. 1871. 1846. 1890. 1883. 1870. 1885. 1896. 1879. 1876, 1887. 1896. 1880. 1890. 1878. 1857. 1885. 1885. 1885. 1887. 1898. » 1865. 1879. 1897. 1870. 1894. 1870. 1890. {Craven, John. Smedley Lodge, Cheetham, Manchester. *Craven, Thomas, J.P. Woodheyes Park, Ashton-upon-Mersey. *CRAWFORD AND BatcaRREs, The Right Hon. the Earl of, K.T., LL.D., F.R.S., F.R.A.S. Dun Echt, Aberdeen. *Crawford, William Caldwell, M.A. 1 Lockharton-gardens, Craig- lockhart, Edinburgh. *Crawshaw, The Right Hon. Lord. Whatton, Loughborough. §Crawshaw, Charles B. Rufford Lodge, Dewsbury. *Crawshaw, Edward, F.R.G.S. 25 Tollington-park, N, *Crawshay, Mrs. Robert. Caversham Park, Reading. §Creax, Captain E. W., R.N., F.R.S. 9 Hervey-road, Black- heath, S.E. {Cregeen, A.C. 21 Prince’s-avenue, Liverpool. {Creswick, Nathaniel. Chantry Grange, near Sheffield. *Crewdson, Rev. Canon George. St. Mary’s Vicarage, Windermere. *Crewdson, Theodore. Norcliffe Hall, Handforth, Manchester. §Crichton, Hugh. 6 Rockield-road, Anfield, Liverpool. *Orisp, Frank, B.A., LL.B., F.LS., F.G.8. 5 Lansdowne-road, Notting Hill, W. *Croft, W. B., M.A. Winchester College, Hampshire. {Croke, John O’Byrne, M.A. Clouneagh, Ballingarry-Lacy, co, Limerick. tOrolly, Rev. George. Maynooth College, Ireland. tCrombie, Charles W. 41 Carden-place, Aberdeen. {Cromsrg, J. W., M.A., M.P. Balgownie Lodge, Aberdeen. {Crombie, Theodore. 18 Albyn-place, Aberdeen. §Croox, Hnnry T. 9 Albert-square, Manchester. §Crooke, William. Langton House, Charlton Kings, Cheltenham. §Crooxss, Sir Wri1iam, F.R.S., V.P.C.S. 7 Kensington Park- gardens, W. {Crookes, Lady. 7 Kensington Park-gardens, W. *CrooxsHaNK, E. M., M.B., Professor of Bacteriology in King’s College, London, W.C. tCrosfield, C. J. Gledhill, Sefton Park, Liverpool. *Crosfield, Miss Margaret C, Undercroft, Reigate. *CROSFIELD, WitLIAM. Annesley, Aigburth, Liverpool. {Cross, E. Richard, LL.B. Harwood House, New Parks-crescent, Scarborough. 1887.§§Cross, John. Beaucliffe, Alderley Edge, Cheshire. 1861. 1853. 1887. 1894. 1897. 1894, 1883. 1882. 1890. 1863. 1885. 1888. 1898, 1888. 1883. tCross, Rev. John Edward, M.A., F.G.S. Halecote, Giange-over= Sands. tCrosskill, William. Beverley, Yorkshire. *Crossley, William J. Glenfield, Bowdon, Cheshire. *Crosweller, William Thomas, F.Z.S., F.L.Inst. Kent Lodge, Sidcup, Kent. *Crosweller, Mrs, W. T. Kent Lodge, Sidcup, Kent. {Crow, C. F. Home Lea, Woodstock Road, Oxford. {Crowder, Robert. Stanwix, Carlisle. §Crowley, Frederick. Ashdell, Alton, Hampshire. *Crowley, Ralph Henry, M.D. 116 Manningham Lane, Bradford. tCruddas, George. Elswick Engine Works, Newcastle-upon-Tyne. {Oruickshank, Alexander, LL.D. 20 Rose-street, Aberdeen. ie tas William J. London and Brazilian Bank, Rio de Janeiro, razil. {tCroUNDALL, Sir Wittiam H. Dover. {Culley, Robert. Bank of Ireland, Dublin. *CULVERWELL, EpwaRD P., M,A. 40 Trinity College, Dublin. LIST OF MEMBERS. 27 Year of Election. 1878. 1883. 1897, 1898. 1861. 1861. 1882. 1877. 1891. 1852. 1885. 1869. 1883, 1892. 1900. 1892. 1884, 1898. 1878. 1884, 1883. 1881. 1889. 1854. 1883. 1898. 1889. 1863. 1867. 1870, 1862. 1876. 1896, 1849, tCulverwell, Joseph Pope. St. Lawrence Lodge, Sutton, Dublin. {Culverwell, T. J. H. Litfield House, Clifton, Bristol. tCumberland, Barlow. Toronto, Canada. §Cundall, J. Tudor. 1 Dean Park-crescent, Edinburgh. *Cunliffe, Edward Thomas. The Parsonage, Handforth, Man- chester. *Ounliffe, Peter Gibson. Dunedin, Handforth, Manchester. *CuNNINGHAM, Lieut.-Colonel AntAN, R.E., A.LC.E. 20 Essex- villas, Kensington, W. *CunnineHAM, D. J., M.D., D.C.L., F.R.S., F.R.S.E., Professor of Anatomy in Trinity College, Dublin. tCunningham, J. H. 4 Magdala-crescent, Edinburgh. {Cunningham, John. Macedon, near Belfast. {Cunnivenam, J. T., B.A. Biological Laboratory, Plymouth. f¢CunnineHam, Rozserr O., M.D., F.L.S., F.G.S., Professor of Natural History in Queen’s College, Belfast. *Cunninenam, Rev. W., D.D., D.Sc. Trinity College, Cambridge. §Cunningham-Craig, E. H., B.A., F.G.S. Geological Survey Office, Sheriff Court-buildings, Edinburgh. *Cunnington, W. Alfred. 13 The Chase, Clapham Common, S.W. *Currie, James, jun, M.A., F.R.S.E. Larkfield, Golden Acre, Edinburgh. {Currier, John McNab. Newport, Vermont, U.S.A. {Curtis, John. 1 Christchurch-road, Clifton, Bristol. {Curtis, William. Caramore, Sutton, Co. Dublin. {Cushing, Frank Hamilton. Washington, U.S.A. TCushing, Mrs. M. Croydon, Surrey. §Cushing, Thomas, F.R.A.S. India Store Depdt, Belyedere-road, Lambeth, S.W. tDagger, John H., F.I.C. Victoria Villa, Lorne-street, Fairfield, Liverpool. {Daglish, Robert. Orrell Cottage, near Wigan. {Dihne, F'. W., Consul of the German Empire. 18 Somerset-place, Swansea. §Dalby, Prof. W. E. 6 Coleridge-road, Crouch End, N. *Dale, Miss Elizabeth. 2 Trumpington Street, Cambridge. {Dale, J. B. South Shields. {Dalgleish, W. Dundee. {Dattrnerr, Rev. W. H., D.D., LL.D., F.R.S., F.L.S. Ingleside, Newstead-road, Lee, S.E. Dalton, Edward, LL.D. Dunkirk House, Nailsworth. {Dansy, T. W., M.A., F.G.S. The Crouch, Seaford, Sussex. §Dansken, John, F.R.A.S. 2 Hillside Gardens, Partickhill, Glasgow. §Danson, F. C. Liverpool and London Chambers, Dale-street, Liverpool. *Danson, Joseph, F.C.S. Montreal, Canada. 1894, {Darbishire, B. V., M.A., F.R.G.S. 1 Savile-row, W. 1897. {Darbishire,C. W. Elm Lodge, Elm-row, Hampstead, N.W. 1897.§§Darbishire, F. V., Ph.D, Hopefield, Denison Road, Victoria Park, Manchester. 1861. *DarsisHirE, Ropert DuxinrrenD, B.A. 26 George-street, Man- chester. 1896. {Darbishire, W. A. Penybryn, Carnarvon, North Wales. 1899. 1882, *Darwin, Erasmus. The Orchard, Huntingdon-road, Cambridge. {Darwin, Francis, M.A., M.B., F.R.S., F.L.S. Wychfield, Hun- tingdon-road, Cambridge, 28 Year Electi 1881 1878. LIST OF MEMBERS, of on. . *Darwiy, Grorer Howarp, M.A., LL.D., F.R.S., F.R.A.S., Plumian Professor of Astronomy and Experimental Philosophy in the University of Cambridge. Newnham Grange, Cambridge. *Darwin, Horace. The Orchard, Huntingdon-road, Cambridge. 1894. *Darwin, Major Lzonarp, Hon. Sec. R.G.S. 12 Egerton-place, South 1882. 1888. 1872. 1880. 1898. 1884. 1870. 1885. 1891. 1870. 1887. 1896. 1893. 1898. 1887. 1878. 1870. 1864. 1882. 1896. 1885. 1891. 1886. 1886. 1864. 1857. 1869. 1869. Kensington, S.W. {Darwin, W. E., M.A., F.G.S. Bassett, Southampton. {Daubeny, William M. 11 St. James’s-square, Bath. {Davenport, John T. 64 Marine-parade, Brighton. *Davey, Henry, M.Inst.C.E., F.G.8. 3 Prince’s-street, West- minster, S.W. §Davey, William John. 6 Water-street, Liverpool. tDavid, A. J., B.A., LL.B. 4 Harcourt-buildings, Temple, E.C. {Davidson, Alexander, M.D. 2 Gambier-terrace, Liverpool. tDavidson, Charles B. Roundhay, Fonthill-road, Aberdeen. {Davies, Andrew, M.D. Cefn Parc, Newport, Monmouthshire. {Davies, Edward, F.C.S. Royal Institution, Liverpool. *Davies, H. Rees. Treborth, Bangor, North Wales. *Davies, Thomas Wilberforce, F.G.S. 41 Park-place, Cardiff. *Davies, Rev. T. Witton, B.A., Ph.D. Baptist College, Bangor. §Davies, Wm. Howell, J.P. Down House, Stoke Bishop, Bristol. {Davies-Colley, T. C. Hopedene, Kersal, Manchester. *Davis, Alfred. 37 Ladbroke Grove, W. *Davis, A. S. St. George’s School, Roundhay, near Leeds. tDavis, Cuartes E., F.S.A. 55 Pulteney-street, Bath. {Davis, Henry C. Berry Pomeroy, Springfield-road, Brighton. *Davis, John Henry Grant. Balcombe Road, Hayward’s Heath, Sussex. . *Davis, Rev. Rudolf. Hopefield, Evesham. tDavis, W. 48 Richmond-road, Cardiff. {Davis, W. H. Hazeldean, Pershore-road, Birmingham. {Davison, CHartEs, D.Sc. 16 Manor-road, Birmingham. *Davison, Richard. Beverley-road, Great Driffield, Yorkshire. {Davy, E. W., M.D. Kimmage Lodge, Roundtown, Dublin. tDaw, John. Mount Radford, Exeter. {Daw, R. R. M. Bedford-circus, Exeter. 1860. *Dawes, John T. The Lilacs, Prestatyn, North Wales. 1864. {Dawxrns, W. Boyn, D.Sc., F.R.S., F.S.A., F.G.S., Professor of Geology and Paleontology in the Victoria University, Owens College, Manchester. Woodhurst, Fallowfield, Manchester. 1886. {Dawson, Bernard, The Laurels, Malvern Link. 1891 . {Dawson, Edward. 2 Windsor-place, Cardiff. 1897.§§ Dawson, G. M., O.M.G., LL.D., F.R.S., Director of the Geological 1885. 1884, 1859. 1892. Survey of Canada. Ottawa, Canada. *Dawson, Lieut.-Colonel H. P., R.A. Hartlington, Burnsall, Skipton. {Dawson, Samuel. 258 University-street, Montreal, Canada. *Dawson, Captain William G. The Links, Plumstead Common, Kent. {Day, T.C., F.C.S. 36 Hillside-crescent, Edinburgh. 1870. *Dzacon, G. F., M.Inst.C.E. 19 Warwick-square, 8.W. 1900. §Deacon, M. Whittington House, near Chesterfield. 1887. 1861. {Deakin, H.T. Egremont House, Belmont, near Bolton. tDean, Henry. Colne, Lancashire. 1884. *Debenham, Frank, F.S.S. 1 Fitzjohn’s-ayenue, N.W. 1866. tDrsvus, Hetricu, Ph.D., F.R.S., F.C.S. 4 Schlangenweg, Cassel, Hessen. 1884, {Deck, Arthur, F.C.S. 9 King’s-parade, Cambridge. 1893. {Deeley, R. M. 38 Charnwood-street, Derby. LIST OF MEMBERS. 29 Year of Election. 1878, 1884. 1870. 1896. 1889. 1897. 1896. 1889. 1874, 1896. 1874. 1894, 1899. {Delany, Rev. William, St. Stanislaus College, Tullamore. *De Laune, C. De L. F. Sharsted Court, Sittingbourne. {De Meschin, Thomas, B.A., LL.D. 2 Dr. Johnson’s Buildings, Temple, E.C. §Dempster, John. Tynron, Noctorum, Birkenhead. fDendy, Frederick Walter. 3 Mardale-parade, Gateshead. §Denison, F. Napier. Meteorological Office, Victoria, B.C., Canada. {Denison, Miss Louisa E. 16 Chesham-place, S.W. §Drnny, ALFRED, F.L.S., Professor of Biology in University College, Sheffield. Dent, William Yerbury. 5 Caithness-road, Brook Green, W. {De Rance, Cuarres H., F.G.S. 33 Carshalton Road, Blackpool. {Dersy, The Right Hon. the Earl of, G.C.B. Knowsley, Prescot, Lancashire. *Derham, Walter, M.A., LL.M., F.G.S. 76 Lancaster-gate, W. *Deverell, F. H. 7 Grote’s-place, Blackheath, 8.E. {DrvonsuHrRE, The Duke of, K.G., D.C.L., F.R.S. 78 Piccadilly, W. 1899.§§Dewar, A. Redcote. Redcote, Leven, Fife. 1868. {DEewar, Jamus, M.A., LL.D., F.R.S., F.R.S.E., V.P.C.S., Fullerian 1881. 1883, 1884. 1872. 1887. 1884, 1873. 1896. 1897. 1889. 1863. 1887. 1884, 1881. 1887. 1885. 1883. 1862. 1877. 1869. 1900. 1898. 1899 1874, 1900. 1883. Professor of Chemistry in the Royal Institution, London, and Jacksonian Professor of Natural. and Experimental Philosophy in the University of Cambridge. 1 Scroope-terrace, Cam- bridge. {tDewar, Mrs. 1 Scroope-terrace, Cambridge. {Dewar, James, M.D., F.R.C.S.E, Drylaw House, Davidson’s Mains, Midlothian, N.B. *Dewar, William, M.A. Horton House, Rugby. {Dewick, Rev. E.S., M.A., F.G.S. 26 Oxford-square, W. {Dz Winton, Major-General Sir F., G.C.M.G., C.B., D.C.L., LL.D., F.R.G.S. United Service Club, Pall Mall, S.W. tDe Wolf, 0. C., M.D. Chicago, U.S.A. *Dew-SuitH, A. G., M.A. Chesterton Hall, Cambridge. tD’Hemry, P. 186 Prince’s-road, Liverpool. {Dick, D. B. Toronto, Canada. {Dickinson, A. H. The Wood, Maybury, Surrey. tDickinson, G. T. Lily-avenue, Jesmond, Newcastle-upon-Tyne. {Dickinson, Joseph, F.G.S. South Bank, Pendleton. tDickson, Charles R., M.D. Wolfe Island, Ontario, Canada. tDickson, Edmund, M.A., F.G.S. 2 Starkie-street, Preston. §Dicxson, H. N., B.Sc., F.RS.E., F.R.G.S. 2 St. Margaret’s-road, Oxford. {Dickson, Patrick. Laurencekirk, Aberdeen. {Dickson, T. A. West Cliff, Preston. *DitkE, The Right Hon. Sir Coartes WeEntwortu, Bart., M.P., F.R.G.S. 76 Sloane-street, S.W. {Dillon, James, M.Inst.C.E. 36 Dawson-street, Dublin. Dingle, Edward. 19 King-street, Tavistock. §Divers, Dr. Epwarp, F.R.S. 9 Rugby Mansions, Kensington, W. *Dix, John William 8. Hampton Lodge, Durdham Park, Clifton, Bristol. *Dixon, A. C., D.Sc., Professor of Mathematics in Queen’s College, Galway. *Dixoy, A. E., M.D., Professor of Chemistry in Queen’s College, Cork, Mentone Villa, Sunday’s Well, Cork. §Dixon, A. Francis, D.Sc., Professor of Anatomy in University College, Cardiff. tDixon, Miss E. 2 Cliff-terrace, Kendal. 30 LIST OF MEMBERS. Year of Blection. 1888. 1900. 1879. 1885. 1896. 1887. 1885, 1890. 1885. 1860. 1897. 1892. 1891. 1898. 1875. 1870. 1876. 1897. 1889. 1898. 1895. 1885. 1869. 1877. 1889. 1896. 1861. 1881. 1867. 1863. 1884. 1890. 1883. 1884. 1876. 1884. 1865. 1881. 1887. 1894. 1883. 1892. 1868. 1890. 1892. 18953. 1889. 1897. 1892, §Dixon, Edward T. Messrs. Lloyds, Barnetts, & Bosanquets’ Bank, 54 St. James’s-street, S. W. *Dixon, George, M.A. St. Bees, Cumberland. *Drxon, Harorp B., M.A., F.R.S., F.0.8., Professor of Chemistry in the Owens College, Manchester. {Dixon, John Henry. Inveran, Poolewe, Ross-shire, N.B. §Dixon-Nuttall, F. R. Ingleholme, Ecclestone Park, Prescot. {Dixon, Thomas. Buttershaw, near Bradford, Yorkshire. {Doak, Rev. A. 15 Queen’s-road, Aberdeen. tDobbie, James J., D.Sc. University College, Bangor, North Wales. §Dobbin, Leonard, Ph.D. The University, Edinburgh. *Dobbs, Archibald Edward, M.A. Hartley Manor, Longfield, Kent. {Doberck, William. The Observatory, Hong Kong. {Dobie, W. Fraser. 47 Grange-road, Edinburgh. {Dobson, G. Alkali and Ammonia Works, Cardiff. {Dobson, W. E., J.P. Lenton-road, The Park, Nottingham. *Docwra, George. 19 Clarence Street, Gloucester, *Dodd, John. Nunthorpe-avenue, York. {Dodds, J. M. St. Peter’s College, Cambridge, {Dodge, Richard E. Teachers’ College, Columbia University, New York, U.S.A. {Dodson, George, B.A. Downing College, Cambridge. tDole, James. Redland House, Bristol. {Donald, Charles W. Kinsgarth, Braid-road, Edinburgh. {Donaldson, James, M.A., LL.D., F.R.S.E., Senior Principal of the University of St. Andrews, N.B. {Donisthorpe,G. T. St. Dayid’s Hill, Exeter. *Donxin, Bryan, M.Inst.C.E. The Mount, Wray Park, Reigate. {Donkin, R. 8., M.P. Campville, North Shields. {Donnan, F. E. Ardenmore-terrace, Holywood, Ireland. {Donnelly, Major-General Sir J. F. D., R.E., K.C.B. 59 Onslow- gardens, S. W. {Dorrington, John Edward. Lypiatt Park, Stroud. {Dougall, Andrew Maitland, R.N. Scotscraig, Tayport, Fifeshire. *Doughty, Charles Montagu. Illawara House, Tunbridge Wells. tDouglass, William Alexander. Freehold Loan and Savings Com- pany, Church-street, Toronto, Canada. {Dovaston, John. West Felton, Oswestry. {Dove, Arthur. Crown Cottage, York. {Dove, Miss Frances. St. Leonard’s, St. Andrews, N.B. Dowie, Mrs. Muir. Golland, by Kinross, N.B. *Dowling, D. J. Bromley, Kent. *Dowson, E. Theodore, F.R.M.S. Geldeston, near Beccles, Suffolk, *Dowson, J. Emerson, M.Inst.C.E. 91 Cheyne-walk, S.W. {Doxey, R. A. Slade Honse, Levenshulme, Manchester. {Doyne, R. W., F.R.C.S. 28 Beaumont-street, Oxford, {Draper, William. De Grey House, St. Leonard’s, York. *Dreghorn, David, J.P. 188 Nethersdale Drive, Pollokshields, Glas- gow. {DrusseR, Henry E., F.Z.S. 110 Cannon-street, H.C. tDrew, John. 12 Harringay-park, Crouch End, Middlesex, N. {Dreyer, J ee L. E., M.A., Ph.D., F.R.A.S. The Observatory, Armagh. §Druce, G. Craripen, M.A., F.L.S. 118 High-street, Oxford. {Drummond, Dr. 6 Saville-place, Newcastle-upon-Tyne. {Drynan, Miss. Northwold, Queen’s Park, Toronto, Canada. {Du Bois, Dr. H. Mittelstrasse, 39, Berlin, LIST OF MEMBERS. 31 Year of Election. 1856. *Ducre, The Right. Hon. Henry Jomn Reyryotps Moreton, Earl of, F.R.S., F.G.S. 16 Portman-square, W.; and Tortworth Court, Falfield, Gloucestershire. 1870. {Duckworth, Henry, F.L.S., F.G.S8. Christchurch Vicarage, Chester. 1900. *Duckworth, W. L. H. Jesus College, Cambridge. 1895. *Duddell, William. 47 Hans-place, 8. W. 1867. *Durr, The Right Hon. Sir Mounrsruarr ExpHiystone GRANT-, G.C.8.L, F.R.S., F.R.G.S. 11 Chelsea-embankment, S.W. 1852. {DurreRin and Ava, The Most Hon. the Marquis of, K.P., G.C.B., G.C.M.G., G.C.8.L., D.C.L., LL.D., F.R.S., F.R.G.S. Clande- boye, near Belfast, Ireland. 1877. {Duffey, George F., M.D. 30 Fitzwilliam-place, Dublin. 1875. {Duffin, W. EH. L’Estrange. Waterford. 1890. {Dufton, 8. F. Trinity College, Cambridge. 1884, {Dugdale, James H. 9 Hyde Park-gardens, W. 1883. {Duke, Frederic. Conservative Club, Hastings. 1892. {Dulier, Colonel E.,C.B. 27 Sloane-gardens, 8. W. 1866. *Duncan, James. 9 Mincing-lane, E.C. 1891. *Duncan, John, J.P. ‘South Wales Daily News’ Office, Cardiff. 1880. {Duncan, William S. 143 Queen’s-road, Bayswater, W. 1896. {Duncanson, Thomas. 16 Deane-road, Liverpool. 1881. tDuncombe, The Hon. Cecil, F.G.S. Nawton Grange, York. 1893. *Dunell, George Robert. 7 Spencer-road, Grove Park, Chiswick, Middlesex. 1892, {Dunham, Miss Helen Bliss. Messrs. Morton, Rose, & Co., Bartholo- mew House, E.C. 1896. *DuNKERLEY, S., M.Sc., Professor of Applied Mechanics in the Royal Naval College, Greenwich, 8.E. 1865. {Dunn, David. Annet House, Skelmorlie, by Greenock, N.B. 1882. {Dunn, J. T., M.Se., F.C.S. Northern Polytechnic Institute Holloway-road, N. 1883. {Dunn, Mrs. Northern Polytechnic Institute, Holloway-road, N. 1876. {Dunnachie, James. 2 West Regent-street, Glasgow. 1878. {Dunne, D. B., M.A., Ph.D., Professor of Logie in the Catholic Uni- versity of Ireland. 4 Clanwilliam-place, Dublin. 1884. §Dunnington, Prof. F. P. University of Virginia, Charlottesville, Virginia, U.S.A. 1859. {Duns, Rev. John, D.D., F.R.S.E. New College, Edinburgh. 1893. *Dunstan, M. J. R. Newcastle-circus, Nottingham. 1891. {Dunstan, Mrs. Neweastle-circus, Nottingham. 1885. *Dunstan, WynpHAM R., M.A., F.R.S., Sec.C.S8., Director of the Scientific Department of the Imperial Institute, S.W. 1869. {D’Urban, W.S. M., F.L.S. Newport House, near Exeter. 1898.§§Durrant, R. G. Marlborough College, Wilts. 1895. *Dwerryhouse, Arthur R. 5 Oakfield-terrace, Headingley, Leeds. 1887. {Dyason, John Sanford. Outhbert Street, W. 1884, {Dyck, Professor Walter. The University, Munich. 1885. *Dyer, Henry, M.A., D.Sc. 8 Highburgh-terrace, Dowanhill, Glasgow. 1869. *Dymond, Edward E. Oaklands, Aspley Guise, Bletchley. 1895, §Dymond, Thos.S.,F.C.S. County Technical Laboratory, Chelmsford. 1868. {Eade, Sir Peter, M.D. Upper St. Giles’s-street, Norwich. 1895, {Harle, Hardman A. 29 Queen Anne’s-gate, Westminster, S,W. 1877. tHarle, Ven. Archdeacon, M.A, West Alvington, Deyon, 32 LIST OF MEMBERS. Year of Election. 1874. 1899. 1871. 1863. 1876. 1883. 1898. 1884. 1861. 1870. 1899. 1887. 1884. 1887. 1870. 1883. 1888. 1884. 1885. 1867. 1899. 1884. 1887. 1896. 1876, 1890. 1885. 1883. 1891. 1883. 1886. 1898. 1877. 1875. 1880. 1891. 1884. 1869. 1887. 1862. 1899. 1897. 18838, {Eason, Charles. 30 Kenilworth-square, Rathgar, Dublin. §East, W. H. Municipal School of Art, Science, and Technology, Dover. *Easton, Epwarp. 11 Delahay-street, Westminster, S.W. {Easton, James. Nest House, near Gateshead, Durham. {Easton, John. Durie House, Abercromby-street, Helensburgh, N.B. {Eastwood, Miss. Littleover Grange, Derby. *Ebbs, Alfred B. Northumberland-alley, Fenchurch-street, E.C. {Eckersley, W. T. Standish Hall, Wigan, Lancashire. tEcroyd, William Farrer. Spring Cottage, near Burnley. *Eddison, John Edwin, M.D., M.R.C.S. The Lodge, Adel, Leeds. tEddowes, Alfred, M.D. 28 Wimpole-street, W. *Eddy, James Ray, F.G.S._ The Grange, Carleton, Skipton. {Ede, Francis J., F.G.S. Silchar, Cachar, India. *Edgell, Rev. R. Arnold, M.A., F.C.S, The College House, Leamington. §EpeewortH, F. Y., M.A., D.C.L., F.S.8., Professor of Political Economy in the University of Oxford. All Souls College,Oxford. *Edmonds, F. B. 6 Clement’s Inn, W.C. {Edmonds, William. Wiscombe Park, Colyton, Devon. *Edmunds, Henry. Antron, 71 Upper Tulse-hill, S.W. *Edmunds, James, M.D. 26 Manchester-square, W, t{Edmunds, Lewis, D.Sc., LL.B., F.G.S. 1 Garden-court, Temple, E.C. *Edward, Allan. Farington Hall, Dundee. §Edwards, E. J. 33 Newland-terrace, Queen’s-road, Battersea, 8.W. t{Edwards, W. F. Niles, Michigan, U.S.A. *Egerton of Tatton, The Right Hon. Lord. Tatton Park, Knutsford. tEkkert, Miss Dorothea. 95 Upper Parliament-street, Liverpool. tElder, Mrs. 6 Claremont-terrace, Glasgow. §Elford, Percy. St. John’s College, Oxford. *Exear, Francis, UL.D., F.R.S., F.R.S.E., M.Inst.C.E. 113 Cannon- street, E.C. {Ellington, Edward Bayzand, M.Inst.C.E. Palace-chambers, Bridges street, Westminster, S.W. {Elliott, A. C.,D.Sec., Professor of Engineering in University College, Cardiff. 2 Plasturton-avenue, Cardiff, *Exziorr, Epwin Bartey, M.A., F.RS., F.R.A.S., Waynflete Professor of Pure Mathematics in the University of Oxford. 4 Bardwell-road, Oxford. Elliott, John Fogg. Elvet Hill, Durham. tEtnior, Tuomas Henry, C.B., F.S.S. Board of Agriculture, 4 Whitehall-place, S.W. tElliott, W. J. 14 Buckingham Place, Clifton, Bristol. {Ellis, Arthur Devonshire. Thurnscoe Hall, Rotherham, Yorkshire. *Ellis, H. D. 12 Gloucester-terrace, Hyde Park, W. *Exuis, Joan Henry. Woodhaye, Ivy Bridge, Devon, §Ellis, Miss M. A. 1] Canterbury-road, Oxford. Ellis, Professor W. Hodgson, M.A., M.B. 74 St. Alban’s-street, Toronto, Canada. {Ellis, William Horton. Hartwell House, Exeter. Ellman, Rey. E. B. Berwick Rectory, near Lewes, Sussex. tElmy, Ben. Oongleton, Cheshire. {Elphinstone, Sir H. W., Bart., M.A., F.L.S. 2 Stone-buildings, Lincoln’s Inn, W.C. *Elvery, Miss Amelia. The Cedars, Maison Dieu-road, Dover. §Elvery, Mrs. Elizabeth. The Cedars, Maison Dieu-road, Dover. {Elwes, Captain George Robert. Bossington, Bournemouth. LIS! OF MEMBERS. 33 Election. 1887. §EtwortHy, Freperick T. Foxdown, Wellington, Somerset. 1870. *Exy, The Right Rev. Lord Atwynr Compton, D.D., Lord Bishop of. ‘The Palace, Ely, Cambridgeshire. 1897.§§Ely, Robert E. 744 Massachusetts-avenue, Cambridge, Massa- . chusetts, U.S.A, 1891. {Emerton, Wolseley, D.C.L. Banwell Castle, Somerset, 1884, {Emery, Albert H. Stamford, Connecticut, U.S.A. 1863, {Emery, The Ven. Archdeacon, B.D. Ely, Cambridgeshire. 1890. {Emsley, Alderman W. Richmond House, Richmond-road, Head- ingley, Leeds. 1894. {Emtage, W. T. A. University College, Nottingham. 1866, {Enfield, Richard. Low Pavement, Nottingham. 1884, {England, Luther M. Knowlton, Quebec, Canada. 1853. {English, E. Wilkins. Yorkshire Banking Company, Lowgate, Hull. 1883. {Entwistle, James P. Beachfield, 2 Westclyffe-road, Southport. 1869, *Enys, John Davis. Enys, Penryn, Cornwall. 1894, {Erskine-Murray, James. Callander, Scotland. 1862. *Esson, WitiraM, M.A., F.R.S., F.R.A.S., Savilian Professor of Geometry in the University of Oxford. 183 Bradmore-road, Oxford. 1878. {Estcourt, Charles. 8 St. James’s-square, John Dalton-street, Man- chester. 1887. *Estcourt, Charles. Hayesleigh, Montague-road, Old Trafford, Man- chester. 1887. *Estcourt, P. A., F.C.S., F.1.C. Seymour House, Seymour Street, Manchester. 1869. {Eruerines, R., F.R.S., F.R.S.E., F.G.S. 14 Carlyle-square, S.W. 1888. {Etheridge, Mrs. 14 Carlyle-square, S.W. 1883, {Eunson, Henry J., F.G.S., Assoc.M.Inst.C.E, Vizianagram, Madras. 1881. {Evans, Alfred, M.A., M.B. Pontypridd. 1889. *Evans, A. H., M.A. 9 Harvey-road, Cambridge. 1887. *Evans, Mrs, Alfred W. A. Lyndhurst, Upper Chorlton-road, Whalley Range, Manchester. 1870, *Evans, Artuur Jouy, M.A., F.S.A. Youlbury, Abingdon. 1865. *Evans, Rev. Cuartes, M.A. 41 Lancaster-gate, W. 1896.§§Evans, Edward, jun. Spital Old Hall, Bromborough, Cheshire, 1891. {Hyvans, Franklen. Llwynarthen, Castleton, Cardiff, 1889. {Evans, Henry Jones, Greenhill, Whitchurch, Cardiff, 1883. *Evans, James C. 175 Lord-street, Southport. 1883. *Evans, Mrs. James C. 175 Lord-street, Southport. 1861, *Evans, Sir Jonny, K.C.B., D.C.L., LL.D., D.Se., F.R.S., F.S.A,, F.L.S., F.G.S, Nash Mills, Hemel Hempstead. 1897. *Evans, Lady. Nash Mills, Hemel Hempstead. 1898, {Evans, Jonathan L. 4 Litfield-place, Clifton, Bristol. 1881. {Evans, Lewis. Llanfyrnach, R.S.0., Pembrokeshize. 1885. *Evans, Percy Bagnall. The Spring, Kenilworth. 1865. {Evans, Srpastran, M.A., LL.D. 15 Waterloo-crescent, Dover. 1899.§§Evans, Mrs. 15 Waterloo-crescent, Dover. 1875. tEvans, Sparke. 3 Apsley-road, Clifton, Bristol. 1865, *Evans, William. The Spring, Kenilworth. 1891. tEvans, William Llewellin. Guildhall-chambers, Cardiff: 1891. {Evan-Thomas, C., J.P. The Gnoll, Neath, Glamorganshire, 1886, {Eve, A.S. Marlborough College, Wilts. 1871. {Eve, H. Weston, M.A. 37 Gordon Square, W.C. 1868, *Evernrr, J. D., M.A., D.C.L., F.B.S., FR.S.E. 11 Leopold Road, Ealing, W. et fiiverett, W. H., B.A. University College, Notlingham, 900. © 34 LIST OF MEMBERS, Year of Election. 1863. *Eyeritt, George Allen, F.R.G.S. Knowle Hall, Warwickshire. 1886. {Everitt, William H. Finstall Park, Bromsgrove. 1883. {Eves, Miss Florence. Uxbridge. ; . 1881, {Ewarr, J. Cossar, M.D., F.R.S., Professor of Natural History in the University of Edinburgh. 1874. {Ewarz, Sir W. Quartus, Bart. Glenmachan, Belfast. : 1876. *Ewine, Jamus Atrrep, M.A., B.Sc., F.R.S., F.R.S.E., M.Inst. C.E., Professor of Mechanism and Applied Mechanics in the University of Cambridge. Langdale Lodge, Cambridge. 1883. {Ewing, James L. 52 North Bridge, Edinburgh. 1884. *Eyerman, John, F.Z.8. Oakhurst, Easton, Pennsylvania, U.S.A. 1882, tEyre,G. E. Briscoe. Warrens, near Lyndhurst, Hants. Eyton, Charles. Hendred House, Abingdon. 1890. {Fanpr, MpMuND Beroxerr. Straylea, Harrogate. 1896. §Fairbrother, Thomas. 46 Lethbridge-road, Southport. 1865, *Farrtzy, Tuomas, I.R.S.E., F.C.S. 8 Newton-grove, Leeds, 1886. {Fairley, William. Beau Desert, Rugeley, Staffordshire. 1896. §Falk, Herman John, M.A. Thorshill, West Kirby, Liverpool. 1883. {Fallon, Rev. W. 8S. 9 St. James’s-square, Cheltenham. 1898. §Faraday, Miss Ethel R., M.A. Ramsay Lodge, Levenshulme, near Manchester. 1877. §Farapay, FP. J., F.L.S., F.S.S. College-chambers, 17 Brazenose- street, Manchester. 1891. {Fards, G. Penarth. 1892, *F'armer, J. Breriann, M.A., F.R.S., F.L.S., Professor of Botany, Royal College of Science, Exhibition-road, 8.W. 1886. {Farncombe, Joseph, J.P. Saltwood, Spencer-road, Hastbourne. 1897. *Farnworth, Ernest. Rosslyn, Goldthorn Hill, Wolverhampton. 1897. *Farnworth, Mrs. Ernest. Rosslyn, Goldthorn Hill, Wolverhampton. 1883. {Farnworth, Walter. 86 Preston New-road, Blackburn. 1883. {Farnworth, William. 86 Preston New-road, Blackburn. 1885, {Farquhar, Admiral. Carlogie, Aberdeen. 1886. {FarauuArson, Colonel Sir J., K.C.B., R.E. Corrachee, Tarland, Aberdeen. 1859. [Farquharson, Robert F.O. Haughton, Aberdeen. 1885. *Farquharson, Mrs. R. F.O. Haughton, Aberdeen. 1866. *Farrar, The Very Rev. Freperic Witiiam, D.D., F.R.S. The Deanery, Canterbury. 1883, {Farrell, John Arthur. Moynalty, Kells, North Ireland. 1897. {Farthing, Rey. J. C., M.A. The Rectory, Woodstock, Ontario, Canada. 1869. *Fauldine, Joseph. Boxley House, Tenterden, Kent. 1883. {Faulding, Mrs. Boxley House, Tenterden, Kent. 1887. §Faulkner, John. 15 Great Ducie-street, Strangeways, Manchester. 1890. *Faweett, f. B. University College, Bristol. 1900. §Fawenrg, J. E., J.P. Low Royd, Apperley Bridge, Bradford. 1886.§§Felkin, Robert W., M.D., F.R.G.S. 6 Crouch Hall-road, N, Fell, John B. Spark’s Bridge, Ulverstone, Lancashire. 1900. *Fennell, W. John. Kileoroon, Stockman’s Lane, Belfast. 1883. {Fenwick, E. H. 29 Harley-street, W. 1890, {Fenwick, T. Chapel Allerton, Leeds. 1876. {Ferguson, Alexander A. 11 Grosvenor-terrace, Glasgow. 1885, |{Ferguson, Mrs. A. A. 11 Grosvenor-terrace, Glasgow. 1871, *Furevson, Jonny, M.A., LL.D., F.R.S.E., F.S.A., F.C.8., Professor of Chemistry in the University of Glaseow. LIST OF MEMBERS. 35 Year of - Election. 1896, *Ferguson, John. Colombo, Ceylon. 1867. {Ferguson, Robert M., LL.D., Ph.D., F.R.S.E. 5 Learmouth-terrace Edinburgh. : 1883, {Fernald, H. P. Clarence House, Promenade, Cheltenham. 1883. *Fernie, John. Box No.2, Hutchinson, Kansas, U.S.A. 1862. {Ferrers, Rev. Norman Macrxop, D.D., F.R.S. Caius College Lodge, Cambridge. 1873. {Furrier, Davip, M.A., M.D., LL.D., F.R.S., Professor of Neuro- Pathology in King’s College, London, 34 Cavendish-square, W. 1892, {Ferrier, Robert M., B.Sc. College of Science, Newcastle-upon-Tyne, 1897. {Ferrier, W. F. Geological Survey, Ottawa, Canada. 1897.§§Fessenden, Reginald