eee Siete le eee ase < 4 y ) a ee ‘ aie ats) rh iat REPORT OF THE SIXTY-PIPTH MEETING OF THE BRITISH ASSOCIATION FOR THE ADVANCEMENT OF SCIENCE es HELD AT Polak Wairoa tia’ 4 on 5 i >» ne =% Ik -F ee IPSWICH IN SEPTEMBER 1895. LONDON: JOHN MURRAY, ALBEMARLE STREET. 1895. Office of the Association: Burlington House, London, W. i a fe r 4 E LONDON CONTENTS, en ee Page GHaners and ‘tules'of the Association v.........s.c.secnssedeerscvereessstetevecees XXVil Places and Times of Meeting, with Presidents, Vice-Presidents, and Local SSSCTSbARICS|TFOM-COMMENCEMEDE _es.ceceiae dois cui ov date ncessaunawndans ve dpyedessp XXXViil Trustees and General Officers, 1831-1895.............: Fh dss ginal Vea hSs <0 ict ty ] Presidents and Secretaries of the Sections of the Association from 1832... li MS IOEMEMenINg Wectiresns LER iio. c25h 5. Sees asars sceck Seened ee enc hou de cleeeeee Ixix Heeetures:to the Operativei@lasses. $v ..26) 1... flush eh edcte eee asblope ed eadedebeste Ixxi ~ Officers of Sectional Committees present at the Ipswich Meeting ..........., Ixxiii MMPeE A AAC OUNCHL WL BID—OG Jo. Jccke vas .ve se saeaea cect cseeoudnsdees ae L asaaes Coats Ixxv PASSE OSE NCCOUUU Ieee ery). ccacd nase sepocecneccredsycsnsshteeces aang ROne emda toes Ixxvi Table showing the Attendance and Receipts at the Annual Meetings ...... Ixxviii Report of the Council to the General Committee ..............scceeeeseereeeeeees box Committees appointed by the General Committee at the Ipswich Meet- eee bs CPARICTE ROU E23. s.csing't ja ceased «vndetexdius + 131 (a) MB TeMOL eh. ote cis. cecees ute dsecenetes «wade ste anerieeses qh seetles'a it ict s 139 (i) Meteorological Tables for Tokio............... ceeceecneeeceneeeeeeens 148 III. (7) Earthquakes recorded by Horizontal Pendulums in Tokio ..... 147 Description of a Catalogue of 8,33] Earthquakes recorded in Japan between January 1885 and December 1892..................4+ 149 (a) History of the Catalogues ...............ce.sccecesceerseecseens sears 149 (6) Explanation of the Catalogues .............c:cceceseeeeceeneneenee ees 151 vi REPORT—1895. Page (c) Object of the Catalogues .......:...ssseeeeceeeeseneseneseeeeneeeeeees 153 (d) Results already obtained or shown by the Catalogue and Map Ot! COMENER oes eo. coc esac ocean onnt ovistiels a oeoene nse a ties Sa ee mEnmrtte as 155 IV. On the Velocities with which Waves and Vibrations are propa- gated on the surface of and through Rock and Karth. (Compilation) 2.2. 0:.044iessres0ssncontenmace ne giee ee eee emmnee ay 158 Tntroduction le-.isccenacted5 ee salts eadfte kon pameemaaer eet mee eeemEE nea 158 (a) Observations on Artificially Produced Disturbances. Experi- ments of Manner, ApBot, Fovaut and Livy, Gray, and 1.) Rt pope MRE Seer Se terer ancre acisneeeer ho Mncanredtintccbacs..osootbnee 159 (6) Observations on Earthquakes. Where the wave paths have been short: (Mitnr and Omori). Where the wave paths have been long: (NrwcomsBe and Dutron, AGAMENNONE, Ricco, CancaNnt, von Respuur-PascHwitz, MILnp) ......... 163 (c) The Probable Nature and Velocity of Propagation of Harth- quake Motion. The suggestions of Dr. C. G. Knorr, Lord RAYLEIGH, Lord) KBE VIN yh cass a5 sensint ew saeee cater sttmes senses 170 (d) The Paths followed by Earthquake Motion. Hypotheses of Hopkins and SHesacu, Scumrpt, and a suggestion by the WELDED sos cfs c cae cased se acccen veaaualies veltace reset cperseenteueaseaeees 173 (2) Clone RODS 5. assgs cok emo vedo es nan gies na enes sone ra ane piace tees 178 V. Miscellaneous Notes relating to Large Earthquakes, &c...............- 179 ApprenDIx.—On Causes producing Movements which may be Mistaken for arth Dremoraict, ss gun’ dhiasp caine ee fale aeiielaa al alana alee 718 12. *On the Presence of Skeletal Elements between the Mandibular and Hyoid Arches of Hexacanthus and Lemargus. By Dr. Partie Ware, 719 © 13. *On the Presence of a Sternum in Hexanchus griseus. By Dr. PHILIP AVVIHIMISEINE sa cccccssawae eeoost rte anus teas eae ntameereen esse ck eamases cn ceraeny ces ae amma 719 14, On the Creodonta. By Professor W. B. Scorr .............ssscsscoscceseeenees 719 FRIDAY, SEPTEMBER 13. 1. On some Results of Scientific Investigation as applied to Fisheries. By Professor’ We Cy MSENTOSE, BUR Ss i220. tee beccs once cs coece enone sue ateanctmeaueee 720 . *On the Royal Dublin Society’s Fishery Survey. By Professor A. C. EVA DON cones hese ree edtoe nade bead Cee cece eee Leber s ob eniaseae ses tern se eaeeeetteetene 723 . *On the Fishery School at Ringsend, near Dublin. By Professor A. C. HEVATADION aoe voc dpcicea cenie ce dacs pp sence tenuateanceense sessed cab ve ana ieee eae 723 . Oyster Cultural Methods, Experiments and New Proposals. By BasHFORD DEAN, Assistant U.S. Fishery Commission ............ssessseeeees 723 . On Oysters and Typhoid: an experimental inquiry into the effect upon the Oyster of various external conditions, including pathogenic organisms. By Professor Rupert W. Boycs, M.B., M.R.C.S., and Professor W. A. ITERD MAN, DD)SC.,.BRSs covassvecoccsenshiees cade! sqiecaepseeceseventakass cena . 725 . *Onthe Oyster Culture in the Colne District. By Dr. H.C. Sorpy, F.R.S. 726 . *On Fish and Fishing Grounds in the North Sea. By J. T. Cunnine- HAM; BiAs,, acerca veaasnatenuats saensttvbay oxoshios sas devndenomees wean ddedcan ¢t tere eanEeee 726 . The Organisation of Zoological Bibliography. By Hrrserr Havitanp FPTEDD; BSD: cccsiescccencstadesteccse sens covebeseasSeuedesssces bon esen- theese aiaeerEe 726 . The ‘ Date of Publication’ of Zoological Memoirs. By Hrrpert HavILaAND Ber POD eer edt. . back dds cnn dese RUC ochatekp eve cuh Sec eak Caeser an (27 . On Economy of Labour in Zoology. By Tuomas R, R. Srepprne, M.A. 728 . On the Septal Organs of Owenia fusiformis. By Professor G. Ginson... 728 - *On a simple and efficient Collecting Reservoir for the Surface Tow-net. By: Wo GARSPAING. 55 020:4.5.>0.0-»»»07+enuspitemnlaasaas aallpenest ens paiiean eee eanne 729 . On the Statistics of Wasps. By Professor F, ¥, EDGEWORTH ...........0008 729 CONTENTS. xix MONDAY, SEPTEMBER 16. Page 1. *On Insect Transformations. By Professor L. C. Miatr, F.R.S. ......... 73 2. On Mounting Marine Animals as Transparent Lantern Slides. By H.C, SUED LLU SLD Ma O81 oS Be Seen Pare enn cnet ee ai ae neem 730 3. Description of Methods for Collecting and Estimating the number of Small Animals in Sea Water. By H.C. Sorsy, LL.D., F.R.S. ............0.000- 730 4, On the Conditions affecting Bacterial Life in River Water. By E. SER GAINACITAN Dy DD, Or Dits iE TRUS, ccs cc aces ciate cecsecateccsnaceastaeecspencocsssecte tes 731 5. *On the Exploration of the Islands of the Pacific. By Professor A. C. arias ken Th ease ran tron ads ba Qs ths wovtncae mh NS Belen geneen cansean handsbe 731 - 6. On the Coccidee of Ceylon. By E. E. Green .................cesececscenceeeeves 731 7. *Criticisms on some points in the Summary of the Results of the ‘Challenger’ Expedition. By Dr. H. O.-FORBES .........-...ssccesceseeescese 732 8. Observations on the Marine Fauna of Houtman’s Abrolhos Islands, Western Australia, By W. Savinun-Kent, F.L.S., F.Z.8. oo... eee 732 9. *On the Hereditary Polydactylism. By Dr. Greaa WILSON .......00....+8 733 10. *On the Reproduction of the Common Crab. By Dr. Greage Witson ... 733 TUESDAY, SEPTEMBER 17. 1. Observations on Instinct in Young Birds. By Professor Luoyp Morean, Be Se A BSOC EY SMa. cacanecalie- Yas deed gett se nee'd cojet’h «ges cesse peace saga eek lees 733 2. Notes on the Early Development of the Ganoids, Lepidosteus, Acipenser, andvAmia., By, BASHEORD DUAN ....0<....cscaunc-egencedssapeesgdecdes saatynaeeate 734 3. On some questions relating to the Morphology and Distribution of Mredseet. 9 ysl OMAR 25 io2.cktuacetees coats ecespstasedencesiedeccncasaceneass 734 4, On the Spermatogenesis in Birds. By J. E. S. Moort...........00.0....00 735 5. On the Development of the Teeth in Certain Insectivora. By M. F. ROM WARD. 00 oso tacatasenscnsneseneqencaecnuyunsecuacepadieesptbeete «eit veasacemediys 736 6. On the Mammalian Hyoid. By Professor G. B. How8s .................0006 736 7. On the Poison Apparatus of Certain Snakes. By G. S. Waser, , ES a ee ee eae ere tees 737 8. On the Value of Myology as an Aid in the Classification of Animals. By SMG PARAON Spy HUE, ©.9,. 0c 2ccecessagsesseysesntscciscsieotesncedecseses Sacssncheree sce 737 9. *On Ultimate Vital Units. By Miss Nana LAYARD............:.c.ceceeeeee ee 737 Section E.—GEOGRAPHY. THURSDAY, SEPTEMBER 12. Address by H. J. Macxrnper, M.A., F.R.G.S., President of the Section...... 738 1, On a Journey in Tarhuna and Gharian in Tripoli. By H. Swainson RPE WS. A725. 4Vds Tene svutectabs bededadee tus beherecncercoaseisnsecescoensencs 749 my *On Roeckalls By) MinLeriCHRisty) | 2... .concvete sine cevenieales on’ sieve cle seieee 749 3, *On Western Siberia and the Siberian Railway. By Dr. A. Marxorr... 749 a2 xx REPORT—1895. FRIDAY, SEPTEMBER 13. Page 1. A Voyage to the Antarctic Sea. By C. E. BoRCHGREVINE...............4+ 750 2. The Oceanography of the North Sea. By H. N. Dickson, F.R.S.E....... 752 3. *Oceanic Circulation. By Dr. Joun Murray, F.R.S.E, ..........:scceeeeees 752 . The Maps used by Herodotus. By J. L. Mypus, M.A.........::ceecenneeeees 752 . On the Sixth International Geographical Congress, London, 1895. By Major LEONARD DARWIN, Sec. R.GLS.......cc.s.sescnesseeennreeeconnsecsansecsees 753 . On the Cosmosphere: an instrument combining the Terrestrial and Celestial Globes for the purpose of demonstrating Astronomical-Geogra- phical Phenomena and Navigational Problems. By W.B. Brargre ...... 756 MONDAY, SEPTEMBER 16. 1, An Expedition to Ruwenzori. By G. F. Scorr Extior, M.A. .........06 756 2. Report on the Climate of Tropical Africa ...........s.sssccosessecnneenccencoens 758 3. Three Years’ Travelling and War in the Congo Free State. By Captain Brel ALTIN ID HEME Shas saNeds sate. « «cue eenamarabenele nace s® ef'hietelaaenis ersten ete ae tee sae ie 4, The Progress of the Jackson-Harmsworth Polar Expedition. By ARTHUR IMONEMETORE, EVG. SO.» Bick Ges cetessac cnsaeeenerens ssahes dnsen ce doses teed Deeeenee 759 5 *The Struggle for Existence under Arctic Conditions. By A. TREvor AMIE Sas anova noa sca ledeaioossonneconbeuRerthes rooed ey (Faken cu jars enes0Nescameenne 760 6. The Port of the Upper Nile in relation to the Highways of Foreign Trade. By. JAMES TURNBULL PLAYFAIR HBATLEY .......ccseccssereecenscetceeseaueenes 760 7. Exploration in the Japanese Alps, 1891-94. By the Rev. Watter WVESTON, MLA.) BIR. GRSS. vactcaceteasewemart MMos dumber ees Uulcthes Sante bie sane ramet 761 TUESDAY, SEPTEMBER 17. 1. Report on Explorations in South Arabia..............sscessseseescedccsenseseenes 762 2. Kormosa.: By JON DODD oe. oo. vcweeiete siee' sven vesivistines vesivots'e ste eoe th aaa 762 3. Russian Possessions in Central Asia. By Dr. A. MARKOFP...........00.000 762 4, The Towns of Northern Mongolia. By Dr. A. MARKOFF...............000005 763 5 . Notes on the Topography of Caria. By W.R. Paton and J. L. Myrns... 763 Section F.—ECONOMIC SCIENCE AND STATISTICS. THURSDAY, SEPTEMBER 12. Address by L, L. Pricz, M.A., F.S.8., President of the Section...............0+. 764 1. Comparison of the Rate of Increase of Wages in the United States and in Great Britain, 1860-1891. By A. L. Bow ny, M.A, ...........cseccneeeneee 775 2, *Bimetallism with a Climbing Ratio. By Henry Hices, LL.B............. 776 FRIDAY, SEPTEMBER 13. 1, The Normal Course of Prices. By Wiirt1am Smart, M.A., LL.D.......... 776 2. “A Proposal for a System of International Money. By W. A. SHAw. ... 777 _ CONTENTS. xxl Page "3 *The Gold Standard. By Hon. Guorer PEEL. ....c.ccccccscsessssseessereees 777 4. The Menace to English Industry from the Competition of Silver-using Gountries,. ) By LS. GUNDREssssecsscosccscdcdscorcedeedcendee sdacssbesusccvseeess 777 5, On the Preservation of the National Parochial Registers. By H. Paton, : SN cee esa oo anh ic pane scary ioamn anions dv's dann oVoticsaadanuncaniasynaerons 778 MONDAY, SEPTEMBER 16. 1. *Agriculture in Suffolk. By Captain E.G. Preryman, M.P................ 779 2. Agriculture of Suffolk from a Tenant’s Point of View. By Herman PRDOREE Baye k das ch ciaaid » oc WebGplaet Sula tA n te clleieohia vd a vtecle os nidclei sist Sad odislashiee bade dale 779 8. Co-operative Rural Banks. By Harozp E. Moors, FSI. ......... ees 779 4, Co-operation in the Service of Agriculture. By H. W. Worrr............. 780 TUESDAY, SEPTEMBER 17. 1. The Probability of a Cessation of the Growth of Population in England and Wales before 1951. By EDWIN CANNAN o.sesesseeseeeeeseeeeeeeeesesenes 780 2, On the Correlation of the Rate of General Pauperism with the Proportion of Out-relief given. By G. U. YULB ..........cccseecsesecsseneeseensenseenen cane 781 . *The State and Workers on the Land. By Rev. J. Frome Wixxrnson.... 781 . *The National Value of Organised Labour and Co-operation among ‘Women. By Mrs, Beprorp Fenwick 781 Seem e eee eee teeters eee eee eee eeseeeeee Section G.TMECHANICAL SCIENCE. THURSDAY, SEPTEMBER 12. Address by Professor L. F. Vernon Harcourt, M.A., M.Inst.C.E., President RNELLG SECHLON: raacvansseceddeorarensteeesaaadonesseucltts dec decent» done Weise deck elastance nct = 782 1, Light Railways as anJAssistance to Agriculture. By Major-General Wosper, ©.B., R.E., M. Inst. C.B. .......ccccecceeeeeeeeeeecnereeneeeeneeen enone 798 2, The Gobert Freezing Process for Shaft-sinking and Tunnelling under Rivers: By A. GOBERT .......cccccecccececconneecceeeesaneesceeadecenaeeseeeaensss 794. . *East Anglian Coal Exploration, Description of Machinery employed. By DTM RIRU TARTAN, «cen Tete clk wo ntaetee eaiviod om aceeNicesdeutnnaedeceriesesesessgedeseliocaseens 795 . The Effect of Wind and Atmospheric Pressure on the Tides. By W. H. WHEELER, M.Inst.C.B. ........0...ccsscsecsecsececneenecenceetensensessaseneeaeones 795 FRIDAY, SEPTEMBER 13. 1. *Notes on Autumn Floods of 1894. By G. J. Symons, F.R.S. .....eeeeee 796 2, *On Weirs in Rivers. By R. C. Napzur and F. G. M. Sronzy ......... 796 _ 8, An Experiment in Orgau-blowing. By W. Anperson, C.B., D.C.L., EUR Se cccecwe nec ewewesces de ciesencaceccecewsisests dedueiceeuedddeccesdeceesesevencererstccebes 796 . *The Growth of the Port of Harwich. By W. BIRt ........::::eeeeeeeeeees 796 xxii REPORT—1895. Page 5. The new Outlet of the River Maas at the Hook of Holland, and the Im- provement of the Scheur Branch up to Rotterdam. By L. F. VERNON Harcourt, M.A. M.Inst.0.E ........cccccccnseeenerseeeeeeneescunteceneseuneaaans . 796 6, The Snowdon Mountain Tramroad. By F. Oswxtt, Assoc.M.Inst.C.E, 798 SATURDAY, SEPTEMBER 14. 1, First Report on Standardising ..........::ssessessseeereeereeeeeeeeeereeseereeenens 799 2. Report on Coast Erosion ........eccccseseseeeceesessesaeeeeeterenneasecesennes .. 799 3, Dredging Operations on the Mersey Bar. By AnrHony GEORGE LysTER, IMT HHO OBI, cc. caves dockins cbsieevss on nbioenesss eso aatsoulsdainasenete «pg san ele eheneeans 799 4. *On Carbonic Anhydride Refrigerating Machinery. By E, Husker ... 799 5. On the Deodorising of Sewage by the Hermite Process. By J. Naprmr, F.C.S., Public Analyst for County of Suffollk...........ssseseesseeeereseeeeeeees 800 MONDAY, SEPTEMBER 16. 1. The Modern Application of Electricity to Traction Purposes. By [PETE DAWSON . O. J. Lodge, D. MacAlister. PRESIDENTS AND SECRETARIES OF THE SECTIONS, liii Date and Place Presidents Secretaries 1880. Swansea ...| Prof. W. Grylls Adams, M.A.,W. E. Ayrton, J. W. L. Glaisher, F.RB.S. Dr. O. J. Lodge, D. MacAlister. Maer, VOrkKs...c..0. Prof. Sir W. Thomson, M.A.,| Prof. W. E. Ayrton, Dr. O. J. Lodge, LL.D., D.C.L., F.R.S. D. MacAlister, Rev. W. Routh. 1882. Southamp- | Rt. Hon. Prof. Lord Baye W. M. Hicks, Dr. O. J. Lodge, D. ton. M.A., F.R.S. MacAlister, Rev. G. Richardson. 1883. Southport | Prof.0O. "Henrici, Ph.D., F. R.S.|W. M. Hicks, Prof. O. J. Lodge, D. MacAlister, Prof. R. C. Rowe. 1884. Montreal ...| Prof. Sir W. Thomson, M.A.,|C. Carpmael, W. M. Hicks, A. John- : LL.D., D.C.L., F.R.S. son, O. J. Lodge, D. MacAlister. 1885. Aberdeen...|Prof. G. Chrystal, M.A.,|R.E. Baynes, R. T. Glazebrook, Prof. F.R.S.E. W. M. Hicks, Prof. W. Ingram. 1886. Birmingham|Prof. G. H. Darwin, M.A.,|R. E. Baynes, R. T. Glazebrook, Prof. TED), Hees J. H. Poynting, W. N. Shaw. 1887. Manchester |Prof. Sir R. S. Ball, M.A.,|R. E. Baynes, R. T. Glazebrook, Prof. LL.D., F.R.S. H. Lamb, W. N. Shaw. 1g88: Bath........ Prof. G. F. Fitzgerald, M.A.,|R. E. Baynes, R. T. Glazebrook, A. F.R.S. Lodge, W. N. Shaw. 1889. Newcastle- |Capt. W. de W. Abney, C.B.,|R. E. Baynes, R. T. Glazebrook, A. upon-Tyne| R.E., F.R.S. Lodge, W. N. Shaw, H. Stroud. 1890. Leeds ...... J. W. L. Glaisher, Sc.D.,|/R. T. Glazebrook, Prof. A. Lodge, F.RB.S., V.P.R.A.S. W.N. Shaw, Prof. W. Stroud. 1891. Cardiff...... Prof. O. J. Lodge, D.Sc.,|R. E. Baynes, J. Larmor, Prof. A. nD... Hens: Lodge, Prof. A. L. Selby. 1892. Edinburgh /|Prof. A. Schuster, Ph.D.,|R. E. Baynes, J. Larmor, Prof. A. F.RB.S., F.R.A.S. Lodge, Dr. W. Peddie. 1893. Nottingham | R. T. Glazebrook, M.A., F.R.S.|W. T. A. Emtage, J. Larmor, Prof. A. Lodge, Dr. W. Peddie. 1894. Oxford...... Prof. A. W. Riicker, M.A.,|Prof. W. H. Heaton, Prof. A. Lodge, F.RB.S. J. Walker. 1895. Ipswich ...|Prof. W. M. Hicks, M.A.,|Prof. W. H. Heaton, Prof. A. Lodge F.R.S. G. T. Walker, W. Watson. CHEMICAL SCIENCE. COMMITTEE OF SCIENCES, II.—CHEMISTRY, MINERALOGY. £832. Oxford...... John Dalton, D.C.L., F.R.S. |James F. W. Johnston. 1833. Cambridge |John Dalton, D.C.L., F.R.S. | Prof. Miller. 1834. Edinburgh Dy LOD Care ceenptmncs sas aoa Mr. Johnston, Dr. Christison. SECTION B.—CHEMISTRY AND MINERALOGY. 1835. Dublin...... Dr. T. Thomson, F.R.S. ......|Dr. Apjohn, Prof. Johnston. 1836. Bristol...... Rey. Prof. Cumming ......... Dr. Apjohn, Dr. C. Henry, W. Hera- path. 1837. Liverpool...| Michael Faraday, F.R.S....... Prof. Johnston, Prof. Miller, Dr. Reynolds. 1838. Newcastle | Rev. William Whewell,F.R.S.)| Prof. Miller, H. L. Pattinson, Thomas Richardson. 1839. Birmingham | Prof. T. Graham, F.R.S. .|Dr. Golding Bird, Dr. J. B. Melson, 1840. Glasgow ...| Dr. Thomas Thomson, F, R.S.|Dr. R. D. Thomson, Dr. T. Clark, Dr. L. Playfair. 1841. Plymouth...|Dr. Daubeny, F.R.S. ......... J. Prideaux, Robert Hunt, W. M. Tweedy. 1842. Manchester |John Dalton, D.C.L., F.R.S. | Dr. L. Playfair, R. Hunt, J. Graham. 1843. Cork......... Prof. Apjohn, M.R.I.A......... R. Hunt, Dr. Sweeny. 1844. York......... Prof. T. Graham, F.R.S. ......| Dr. L. Playfair, E. Solly, T. H. Barker. 1845. Cambridge |Rev. Prof. Cumming ......... R. Hunt, J. P. Joule, Prof, Miller, E. Solly. liv REPORT—18908. ey Date and Place 1846. Southamp- ton. 1847, Oxford...... 1848. Swansea 1849. Birmingham 1850. Edinburgh 1851. Ipswich ... 1852. Belfast...... 1853. Hull......... 1854, Liverpool 1855. Glasgow ... 1856. Cheltenham 1857. Dublin...... 1858. 1859. Aberdeen... 1860. Oxford seeeee 1861. Manchester 1862. Cambridge 1863. Newcastle 1864. 1865. Birmingham 1866. Nottingham 1867. Dundee 1868. Norwich ... 1869. Exeter...... 1870. Liverpool... 1871. Edinburgh 1872. Brighton... 1873. Bradford... 1874. Belfast...... HS7o- Ee TIStoll :..c.. 1876. Glasgow 1877. Plymouth... 1878, Dublin Prot Presidents Michael Faraday, D.C.L., F.RB.S. Rev. W. V. Harcourt, M.A., F.R.S. ...|Richard Phillips, F.R.S. ...... John Percy, M.D., F.R.S....... Dr. Christison, V.P.R.S.E. Prof. Thomas Graham, F’.R.S. Thomas Andrews, M.D.,F.R.S. Prof. J. F. W. Johnston, M.A., mp DetueWDes Prof.W. A.Miller, M.D.,F.R.S. Dr. Lyon Playfair,C.B.,F.R.8. Prof. B. C. Brodie, F.R.S. ... Prof. Apjohn, M.D., F.R.S., M.R.I.A. Sir J. F. W. Herschel, Bart., D.C.L. Dr. Lyon Playfair, C.B.,F.R.8, Prof. B. C. Brodie, F.R.S...... Prof. W.A.Miller, M.D.,F.R.S. Prof. W.H. Miller, M.A.,F.R.S. Dr. Alex. W. Williamson, F.R.S. W. Odling, M.B., F.R.S. Prof. W. A. Miller, V.P.R.S. H. Bence Jones, M.D., F.R.S. M.D., T. Anderson, F.R.S.E. Prof. E. Frankland, F.R.S. M.D., Dr. Debus; HORS. eserecs Prof. H. E. Roscoe, B.A., F.R.S. Prof, T. Andrews, M.D., F.R.S. Dr. J. H. Gladstone, F.R.S.... Prof. W. J. Russell, F.R.S.... Prof. A. Crum Brown, M.D., F.R.S.E. A. G. Vernon Harcourt, M.A., E.RB.S. TW. Ho euking FBS. 22... HPPA DOL HS Ra Ste ereecencuecdes Prof. Maxwell Simpson, M.D., F.R.S, Secretaries Dr. Miller, R. Hunt, W. Randall, B. C. Brodie, R. Hunt, Prof. Solly. T. H. Henry, R. Hunt, T. Williams. R. Hunt, G. Shaw. Dr. Anderson, R. Hunt, Dr. Wilson. T. J. Pearsall, W. S. Ward. Dr. Gladstone, Prof. Hodges, Prof. Ronalds. H. S. Blundell, Prof. R. Hunt, T. J. Pearsall. Dr. Edwards, Dr. Gladstone, Dr. Price. Prof. Frankland, Dr. H. E. Roscoe. J. Horsley, P. J. Worsley, Prof. Voelcker. Dr. Davy, Dr. Gladstone, Prof. Sul- livan. Dr. Gladstone, W. Odling, R. Rey- nolds. J. 8. Brazier, Dr. Gladstone, G. D. Liveing, Dr. Odling. A. Vernon Harcourt, G. D. Liveing, A. B. Northcote. A. Vernon Harcourt, G. D. Liveing. H. W. Elphinstone, W. Odling, Prof. Roscoe. Prof. Liveing, H. L. Pattinson, J. C. Stevenson. A. V. Harcourt, Prof. Liveing, R. Biggs. A. V. Harcourt, H. Adkins, Prof, Wanklyn, A. Winkler Wills. J. H. Atherton, Prof. Liveing, W. J. Russell, J. White. A. Crum Brown, Prof. G. D. Liveing, W. J. Russell. Dr. A. Crum Brown, Dr. W. J. Rus- sell, F. Sutton. Prof. A. Crum Brown, Dr. W. Jd. Russell, Dr. Atkinson. Prof. A. Crum Brown, A. E. Fletcher, Dr. W. J. Russell. J.T. Buchanan, W. N. Hartley, T. E. Thorpe. Dr. Mills, W. Chandler Roberts, Dr. W. J. Russell, Dr. T. Wood. Dr. Armstrong, Dr. Mills, W. Chand- ler Roberts, Dr. Thorpe. Dr. T. Cranstoun Charles, W. Chand- ler Roberts, Prof. Thorpe. Dr. H. E. Armstrong, W. Chandler Roberts, W. A. Tilden. W. Dittmar, W. Chandler Roberts, J. M. Thomson, W. A. Tilden. Dr. Oxland, W. Chandler Roberts, J. M. Thomson. W. Chandler Roberts, J. M. Thom- son, Dr. C. R. Tichborne, T, Wills. PRESIDENTS AND SECRETARIES OF THE SECTIONS. lv : Date and Place : 1879. 1880. 1881. 1882. 1883. 1884. 1885. 1886 1887 1888. 1889 1890 Sheffield ... Swansea ... Southport Montreal ... Aberdeen... , Birmingham . Manchester . Newcastle- upon-Tyne . Leeds seeeee . Edinburgh 1893. Nottingham 1895. . Oxford Ipswich Presidents Prof. Dewar, M.A., F.R.S. Joseph Henry Gilbert, Ph.D., F.R.S. Prof. A. W. Williamson, F.R.8. Prof. G. D. Liveing, M.A., F.RB.S. Dr. J. H. Gladstone, F.R.S... Prof. Sir H. E. Roscoe, Ph.D., LL.D., F.R.S. Prof. H. E. Armstrong, Ph.D., F.R.S., Sec. C.S. W. Crookes, F.R.S., V.P.C.S. Dr. E. Schunck, F.R.S. Prof. W. A. Tilden, F.R.S., V.P.C.S. Sir I. Lowthian Bell, Bart., D.C.L., F.R.S. Prof. T. E. Thorpe, B.Sc., Ph.D., F.R.S., Treas. C.8. Prof. W. C. Roberts-Austen, C.B., F.R.S. Prof. H. McLeod, F.R.S. D.S8ce., Prof. J. Emerson Reynolds, M.D., D.Sc., F.R.S. Prof. H. B. Dixon, M.A., F.R.S. Secretaries H. 8. Bell, W. Chandler Roberts, J. M. Thomson. |P. Phillips Bedson, H. B. Dixon, Dr. W. R. Eaton Hodgkinson, J. M. Thomson. |P. P. Bedson, H. B. Dixon, T. Gough. P. Phillips Bedson, H. B. Dixon, J. L. Notter. |Prof. P. Phillips Bedson, H. B. Dixon, H. Forster Morley. Prof. P. Phillips Bedson, H. B. Dixon, T. McFarlane, Prof. W. H. Pike. Prof. P. Phillips Bedson, H. B. Dixon, H.ForsterMorley,Dr.W.J.Simpson. Prof. P. Phillips Bedson, H. B. Dixon, H. Forster Morley, W. W. J. Nicol, C. J. Woodward. Prof. P. Phillips Bedson, H. Forster Morley, W. Thomson. | Prof. H. B. Dixon, H. Forster Morley, R. E. Moyle, W W.J. Nicol. H, Forster Morley, D. H. Nagel, W. W. J. Nicol, H. L. Pattinson, jun. |C. H. Bothamley, H. Forster Morley, D. H. Nagel, W. W. J. Nicol. C. H. Bothamley, H. Forster Morley, W. W. J. Nicol, G. 8. Turpin. J. Gibson, H. Forster Morley, D. H. Nagel, W. W. J. Nicol. J. B. Coleman, M. J. R. Dunstan, D. H. Nagel, W. W. J. Nicol. A. Colefax, W. W. Fisher, Arthur Harden, H. Forster Morley. SECTION B (continwed).—-CHEMISTRY. ...|Prof. R. Meldola, F.R.S. ......|E. H. Fison, Arthur Harden, C. A. Kohn, J. W. Rodger. GEOLOGICAL (ann, untm 1851, GEOGRAPHICAL) SCIENCE. COMMITTEE OF SCIENCES, III.—GEOLOGY AND GEOGRAPHY. 1832. 1833. Cambridge.|G. B. Greenough, F.R.S. pte 1834. Edinburgh .| Prof. Jameson 1835. 1836. 1837. 1838. 1839. Oxford seeeee Dublin Bristol Liverpool... Newcastle... Birmingham R. I. Murchison, F.R.S. ... .|John Taylor. W. Lonsdale, John Phillips. J. Phillips; T. J. Torrie. Rev. J. Yates, SECTION C.—GEOLOGY AND GEOGRAPHY. Bes Oe GTUb se csens.scsccseseess'e Rev. Dr. Buckland, F.R.S.— Geog.,R.I. Murchison, F.R.S8. Rev. Prof. Sedgwick, F.R.S.— Geog.,G.B.Greenough,F.R.S. C. Lyell, F.R.S., V.P.G.S.— Geography, Lord Prudhoe. Rey. Dr. Buckland, F.R.S.— Geog.,G.B.Greenough,F.R.S. Captain Portlock, T. J. Torrie. William Sanders, S. Stutchbury, T. J. Torrie. Captain Portlock, R. Hunter.— Geo- graphy, Capt. H. M. Denham, R.N. W.C. Trevelyan, Capt. Portlock.— Geography, Capt. Washington. George Lloyd, M.D., H. E. Strick- land, Charles Darwin. lvi Date and Place 1840. 1841. 1842, 1843. 1844. 1845. 1846. 1847. 1848. Glasgow ... Plymouth... Manchester Cambridge. Southamp- tor. Swansea ... 1849. Birmingham 1850. Edinburgh! . Hull . Liverpool.. Ipswich . Belfast...... ae eeneee . Glasgow ... . Cheltenham . Manchester . Cambridge . Newcastle REPORT—1895. Presidents Charles Lyell, F.R.S.— Geo- graphy, G. B. Greenough, F.R.S. H. T. De la Beche, F.R.S. ... R. I. Murchison, F.R.S. ...... Richard E. Griffith, F.R.8., M.R.LA. Henry Warburton, M.P., Pres. Geol. Soc. Rev. Prof. Sedgwick, M.A., F.R.S. Leonard Horner, F.R.S.— Geo- graphy, G. B. Greenough, F.K.S. Very Rev.Dr.Buckland,F.R.8. Sir H. T. De la Beche, C.B., F.R.S. Sir Charles Lyell, F.G.S. Sir Roderick I. Murchison, F.R.S. FBS: SECTION C (continued) -«.| WilliamHopkins, M.A.,F.R.S. Lieut.-Col. Portlock, R.E., F.R.S. Prof. Sedgwick, F.R.S......... Prof. Edward Forbes, F.R.S8. Sir R. I. Murchison, F.R.S.... Prof. A. C. Ramsay, F.R.S.... The Lord Talbot de Malahide William Hopkins,M.A.,LL.D., F.R.S. Sir Charles Lyell, D.C.L., F.R.S. Rev. Prof. Sedgwick, LL.D., F.R.S., F.G.S. Sir R. I. Murchison, D.C.L., LL.D., F.R.S. J. Beete Jukes, M.A., F.R.S. Lieb; Prof. Warington W. Smyth, F.R.S., F.G.8. Secretaries W. J. Hamilton, D. Milne, Hugh Murray, H. E. Strickland, John Scoular, M.D. W.J. Hamilton, Edward Moore, M.D., R. Hutton. £. W. Binney, R. Hutton, Dr. R. Lloyd, .H. E. Strickland. Francis M. Jennings, H. E. Strick- land. | Prof, Ansted, E. H. Bunbury. Rev. J. C. Cumming, A. C. Ramsay, Rev. W. Thorp. Robert A. Austen, Dr. J. H. Norton, Prof. Oldham.— Geography, Dr. C. T. Beke. Prof. Ansted, Prof. Oldham, A. C. Ramsay, J. Ruskin. Starling Benson, Prof. Prof, Ramsay. Oldham, J. Beete Jukes, Prof. Oldham, Prof. A. C. Ramsay. ‘A, Keith Johnston, Hugh Miller, Prof. Nicol. .— GEOLOGY. C. J. F. Bunbury, G. W. Ormerod, Searles Wood. James Bryce, James MacAdam, Prof. M‘Coy, Prof. Nicol. Prof. Harkness, William Lawton. John Cunningham, Prof. Harkness, G. W. Ormerod, J. W. Woodall. James Bryce, Prof. Harkness, Prof. Nicol. Rey. P. B. Brodie, Rev. R. Hep- worth, Edward Hull, J. Scougall, T. Wright. Prof. Harkness, Gilbert Sanders, Robert H. Scott. Prof. Nicol, H. \C. Sorby, E: W. Shaw. Prof. Harkness, Rev. J. Longmuir, H. C. Sorby. Prof. Harkness, Edward Hull, Capt. D. C. L. Woodall. Prof. Harkness, Edward Hull, T. Rupert Jones, G. W. Ormerod. Lucas Barrett, Prof. T. Rupert Jones, H. C. Sorby. E. F. Boyd, John Daglish, H. C. Sorby, Themas Sopwith. 1 At a meeting of the General Committee held in 1850, it was resolved ‘ That the subject of Geography be separated from Geology and combined with Ethnology, to constitute a separate Section, under the title of the ‘“‘ Geographical and Hthno- logical Section,” for Presidents and Secretaries of which see page 1xii. ‘Sea? ) all dite SS = PRESIDENTS AND SECRETARIES OF THE SECTIONS. lvii Date and Place 1864. 1865. 1866. 1867. 1868. 1869. 1870. 1871. 1872. 1873. 1874. 1875. 1876. 1877. 1878. 1879. 1880. 1881. 1882. 1883 1884. IS ES ee eeneene Birmingham Nottingham Dundee Norwich ... Exeter ...... Liverpool... Edinburgh Brighton... Bradford ... Belfast...... Bristol...... Glasgow ... Plymouth... Dublin Sheffield ... Swansea ... Southamp- ton. . Southport Montreal ... 1885. Aberdeen... 1886. Birmingham 1887. Manchester 1888. 1889 1890 1891. 1892 1893 1894 . Newcastle- upon-Tyne . Leeds . Edinburgh . Nottingham . Oxford seeeee 1895. Ipswich ... ..-|Archibald Geikie, Presidents Proted.s ebillips, LL.D, F.R.S., F.G.S. Sir R.°I. Murchison, Bart., K.C.B. Prof. A. C. Ramsay, LL.D., F.R.S. F.BS., F.G.S. R. A. C. Godwin-Austen, F.R.S., F.G.S. Prof. R. Harkness, F.R.S., F.G,8. Sir Philipde M.Grey Egerton, Bart., M.P., F.R.S. Prof. A. Geikie, F.R.S., F.G.S. R. A. C. Godwin-Austen, | F.R.S., F.G.S. Prof. J. Phillips, F.R.S., F.G.8. Prof, ull,*- Me A.;-9ESRsS5 F.G.S. Dr. T. Wright, F.R.S.E., F.G.8. Prof. John Young, M.D....... W. Pengelly, F.R.S., F.G.S. D.C.L., John Evans, D.C.L., F.R.S., F.S.A., F.G.S. Prof. P. M. Duncan, F.R.S. H. C. Sorby, F.RB.S., F.G.S.... A. C. Ramsay, LL.D., F.R.S:, F.G.S. R. Etheridge, F.R.S., F.G.S. Enola {Wi .C. LL.D., F.R.5. W.T. Blanford, F.RS., Sec. G.S. Prof. J. W. Judd, F.R.S., Sec. G.S. Prof. T. G. Bonney, D.Sc., LL.D., F.R.S., F.G.S. Henry Woodward, LL.D., E.R.S., F.G.S. Prof. W. Boyd Dawkins, M.A., F.RB.S., F.G.S. Prof. J. Geikie, LL.D., D.C.L., F.R.S., F.G.S. Prof. A. H. Green, F.R.S., F.G.8. Prof. T. Rupert Jones, F.R.S., F.G.S. Prof. C. Lapworth, LL.D., F.R.S., F.G.8. J. J. H. Teall, M.A., F.RB.S., F.G.S. L. Fletcher, M.A., F.B.S. Williamson, M.A., W. Whitaker, B.A., F.R.S. ... Secretaries W. B. Dawkins, J. Johnston, H. C. Sorby, W. Pengelly. Rey. P. B. Brodie, J. Jones, Rev. E. Myers, H. C. Sorby, W. Pengelly. R. Etheridge, W. Pengelly, T. Wil- son, G. H. Wright. Edward Hull, W. Pengelly, Henry Woodward. Rev. O. Fisher, Rev. J. Gunn, W. Pengelly, Rev. H. H. Winwood. W. Pengelly, W. Boyd Dawkins, Rev. H. H. Winwood. W. Pengeliy, Rev. H. H. Winwood, W. Boyd Dawkins, G. H. Morton. R. Etheridge, J. Geikie, T. McKenny Hughes, L. C. Miall. L. C. Miall, George Scott, William Topley, Henry Woodward. L. C. Miall, R. H. Tiddeman, W. Topley. F. Drew, L. C. Miall, R. G. Symes, R. H. Tiddeman. L. C. Miall, E. B. Tawney, W. Topley. J.Armstrong,F.W.Rudler,W.Topley. Dr. Le Neve Foster, R. H. Tidde- man, W. Topley. E. T. Hardman, Prof. J. O’Reilly, R. H. Tiddeman. W. Topley, G. Blake Walker. W. Topley, W. Whitaker. J. E. Clark, W. Keeping, W. Topley, W. Whitaker. T. W. Shore, W. Topley, E. West- lake, W. Whitaker. R. Betley, C. E. De Rance, W. Top- ley, W. Whitaker. F. Adams, Prof. E. W. Claypole, W. Topley, W. Whitaker. C. E. De Rance, J. Horne, J. J. H. Teall, W. Topley. W. J. Harrison, J. J. H. Teall, W. Topley, W. W. Watts. |\J. E. Marr, J. J. H. Teall, W. Top- ley, W. W. Watts. Prof. G. A. Lebour, W. Topley, W. W. Watts, H. B. Woodward. Prof. G. A. Lebour, J. E. Marr, W. W. Watts, H. B. Woodward. J. E. Bedford, Dr. F. H. Hatch, J. E. Marr, W. W. Watts. W. Galloway, J. E. Marr, Clement Reid, W. W. Watts. H. M. Cadell, J. E. Marr, Clement Reid, W. W. Watts. J. W. Carr, J. HE. Marr, Clement Reid, W. W. Watts. F. A. Bather, A. Harker, Clemen Reid, W. W. Watts. F, A. Bather, G. W. Lamplugh, H A. Miers, Clement Reid. lviii Date and Place 1832. 1833. Cambridge! 1834, Edinburgh. 1835. 1836 1837 - 1838 1839 1840. 1841, 1842. 1843. 1844, 1845. 1846. 1847. REPORT—1895. Presidents . Liverpool... . Newcastle . Birmingham Glasgow ... Plymouth... Manchester se eeeeeee Cambridge Southamp- ton. seeeee Secretaries BIOLOGICAL SCIENCES. COMMITTEE OF SCIENCES, IV.—ZOOLOGY, BOTANY, PHYSIOLOGY, ANATOMY. Rev. P. B. Duncan, F.G.S. ... | Prot, Gaba vececsscsccsessssee Rey. W. L. P. Garnons, F.L.S. | Bev. Prof, J. 8. Henslow. |C. C. Babington, D. Don. |W. Yarrell, Prof. Burnett. SECTION D.—ZOOLOGY AND BOTANY. seme een eter eeseeeseee aterm etenees Way stla CLGBy .....cerssscnene Sir W. Jardine, Bart. ......... PromsOxens daR.S. icccesces sa Sir W. J. Hooker, LL.D....... John Richardson, M.D.,F.R.S. Hon. and Very Rey. W. Her- bert, LL.D., F.L.S. William Thompson, F.L.S.... Very Rey. the Dean of Man- chester. Rev. Prof, Henslow, F.L.S.... Sir J. Richardson, M.D., F.R.S. H. E. Strickland, M.A., F.R.S. | \J. Curtis, Dr. Litton. J. Curtis, Prof. Don, Dr. Riley, 8. Rootsey. C. C. Babington, Rev. L. Jenyns, W. Swainson. J. E. Gray, Prof. Jones, R. Owen, Dr. Richardson, E. Forbes, W. Ick, R. Patterson. Prof. W. Couper, E. Forbes, R. Pat- terson. J. Couch, Dr. Lankester, R. Patterson. Dr. Lankester, R. Patterson, J. A. Turner. iG. J. Allman, Dr. Lankester, R. Patterson. Prof, Allman, H. Goodsir, Dr. King, Dr. Lankester. Dr. Lankester, T. V. Wollaston. Dr. Lankester, T, V. Wollaston, H. Wooldridge. Dr. Lankester, Dr. Melville, T. V. Wollaston. SECTION D (continued).—ZOOLOGY AND BOTANY, INCLUDING PHYSIOLOGY. [For the Presidents and Secretaries of the Anatomical and Physiological Sub- sections and the temporary Section E of Anatomy and Medicine, see p. Ixi.] 1848. Swansea ...,L. W. Dillwyn, F.R.S.......... 1849 1850. 1851. 1852. 1853. 1854. 1855. 1856. 1857. . Birmingham Edinburgh Ipswich Belfast Liverpool... Glasgow ... Cheltenham Dublin | William Spence, F.R.S. ...... Prof. Goodsir, F.R.S. L. & E. .../Rev. Prof. Henslow, M.A., F.R.S. Cee ee ewe ere eeeessewenee 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. F.R.S. Prof. W. H. Harvey, M.D.,| 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. 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. lxi. 2 E— —————————————————— ULL PRESIDENTS AND SECRETARIES OF THE SECTIONS. . lix eee Date and Place 1858. Leeds ...... 1859. Aberdeen... 1860. Oxford...... 1861. Manchester 1862. Cambridge 1863. Newcastle 1864, Bath......... 1865. Birmingham 1866. Nottingham 1867. Dundee 1868. Norwich ... 1869. Exeter 1870. Liverpool... 1871. Edinburgh. Presidents C. C. Babington, M.A., F.R.S. Sir W. Jardine, Bart., F.R.S.E. Rey. Prof. Henslow, F.L.S.... Prof. C. C. Babington, F.R.S. se eeeeeee Prof. Huxley, F.R.S. Prof. Balfour, M.D.. F.R.S.... Dr. John E. Gray, F.R.S. T. Thomson, M.D., F.R.S. ... SECTION D (continued) Secretaries ‘Henry Denny, Dr. Heaton, Dr. E. Lankester, Dr. E. Perceval Wright. Prof. Dickie, M.D., Dr. E. Lankester, Dr. Ogilvy. 'W.S. Church, Dr. E. Lankester, P. L. Sclater, Dr. E. Perceval Wright. Dr. T. Alcock, Dr. E. Lankester, Dr. P. L. Sclater, Dr. E. P. Wright. Alfred Newton, Dr. E. P. Wright. Dr. E. Charlton, A. Newton, Rev. H. B. Tristram, Dr. E. P. Wright. ...|H. B. Brady, C. E. Broom, H. T. Stainton, Dr. E. P. Wright. |Dr. J. Anthony, Rev. C. Clarke, Rev. H. B. Tristram, Dr. E. P. Wright. ,—BIOLoGy.! Prof. Huxley, LL.D., F.R.S.| Dr. J. Beddard, W. Felkin, Rev. H, —Physiological Dep., Prof. Humphry, M.D., F.R.S.— Anthropological Dep., Alf. R. Wallace, F.R.G.S. —Dep. of Zool. and Bot., George Busk, M.D., F.R.S. B. Tristram, W. Turner, HE. 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. Rey. M. J. Berkeley, F.L.S.| Dr. T. 8. Cobbold, G. W. Firth, Dr. —Dep. of Physiology, W. H. Flower, F.R.S. M. Foster, Prof. Lawson, H. T. Stainton, Rev. Dr. H. B. Tristram, Dr. E. P. Wright. George Busk, F.R.S., F.L.S.| Dr. T. 8. Cobbold, Prof. M. Foster, —Dep. of Bot. and Zool., C. Spence Bate, F.R.S.— Dep. of Ethno., EB. B. Tylor. E. Ray Lankester, Prof. Lawson, H. T, Stainton, Rev. H. B. Tris- tram. Prof. G. Rolleston, M.A., M.D.,|Dr. T. S. Cobbold, Sebastian Evans, F.R.S., F.L.S.— Dep. of| Prof. Lawson, Thos. J. Moore, H. Anat. and Physiol., Prof. M. Foster, M.D., F.L.S.—Dep. of Ethno., J. Evans, F.R.S. JT. Stainton, Rev. H. B. Tristram, C. Staniland Wake, E. Ray Lan- kester. Prof. Allen Thomson, M.D.,|Dr. T. R. Fraser, Dr. Arthur Gamgee, F.R.S.—Dep. of Bot. and Zool.,Prof.WyvilleThomson, F.R.S.—Dep. of Anthropol., Prof. W. Turner, M.D. E. Ray Lankester, Prof. Lawson, H. T. Stainton, C. Staniland Wake, Dr. W. Rutherford, Dr. Kelburne King. 1872. Brighton ..,|SirJ. Lubbock, Bart.,F.R.S.— | Prof. Thiselton- Dyer, H. T. Stainton, Dep. of Anat. and Physiol., Dr. Burdon Sanderson, F.R.S.— Dep. of Anthropol., Col. A. Lane Fox, F.G.S. Prof. Lawson, F. W. Rudler, J. H. Lamprey; Dr. Gamgee, E. Ray Lankester, Dr. Pye-Smith. 1873. Bradford ...| Prof. Allman, F.R.S.—Dep. of| Prof. Thiselton-Dyer, Prof. Lawson, Anat.and Physiol.,Prof. Ru- therford, M.D.— Dep. of An- thropol., Dr. Beddoe, F.R.S. R. M‘Lachlan, Dr. Pye-Smith, E. Ray Lankester, F. W. Rudler, J. H. Lamprey. 1 At a meeting of the General Committee in 1865, it was resolved ‘That the title of Section D be changed to Biology ; > and ‘That for the word “Subsection,” in the rules for conducting the business of the Sections, the word “Department be substituted.’ lx REPORT—1892, Date and Place | Presidents 1874. Belfast seenee 1875, Bristol 1876, Glasgow ... 1877. Plymouth... 1878, Dublin 1879. Sheffield ... 41880. Swansea ... 1881. York.. 1882. Southamp- ton.! 1883. Southport * 1884. Montreal ... 1885. Aberdeen... Prof. Redfern, M.D.—Dep. of Zool. and Bot., Dr. Hooker, C.B.,Pres.R.S.—Dep. of An- throp., Six W.R. Wilde, M.D. P. L. Sclater, F.R.S.— Dep. of Anat.and Physiol.,Prot.Cle- land, M.D., F.R.8.—Dep. of Anthropol., Prof. Rolleston, M.D., F.RB.S. A. Russel Wallace, F.R.G.S., F.L.S.—Dep. of Zool. and Bot., Prof. A. Newton, M.A., F.R.S.—Dep. of Anat. and Physiol., Dr. J. G. McKen- drick, F.R.8.E. J. GwynJeffreys, LL.D.,F.RB.S., F.L.S.—Dep. of ‘Anat. and. Physiol., Prof. Macalister, M.D.—Dep. of Anthropol., Francis Galton, M.A.,F.R.8. 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. Prof. St. George Mivart, F.R.S.— Dep. of Anthropol., E. B. Tylor, D.C.L., F.R.S. —Dep. of Anat. and Phy- siol., Dr. Pye-Smith. A. C. L. Giinther, M.D., F.R.S. —Dep. of Anat. and Phy- siol., F. M. Balfour, M.A., F.R.S.— Dep. of Anthropol., F. W. Rudler, F.G.S. Richard Owen, C.B., M.D., F.R.S.—Dep.of Anthropol., Prof. W. H. Flower, LL.D., F.R.S.—Dep. of Anat. and Physiol., Prof. J. S. Burdon Sanderson, M.D., F.R.S. Prof. A. Gamgee, M.D., F.R.S. — Dep. of Zool. and Bot., Prof. M. A. Lawson, M.A., F.L.S.—Dep. of Anthropol., Prof. W. Boyd Dawkins, M.A., F.R.S. Prof. E. Ray Lankester, M.A., F.R.S.— Dep. of Anthropal., W. Pengelly, F.R.S. Prof. H. N. Moseley, M.A., F.B.S. Prof. W. C. McIntosh, M.D., LL.D., F.R.S. F.R.S.E. Secretaries W.T. Thiselton- Dyer, R. O. 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. Schifer. 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. E. Spencer. G.- Nias, Howard Saunders, wick, T. W. Shore, jun. Bloxam, W. Heape, J. B. A. Sedg- es 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. 1 The Departments of Zoology and Botany and of Anatomy and Physiology were amalgamated. ce ‘Anthropology was made a separate Section, see p. Ixviii. PRESIDENTS AND SECRETARIES OF THE SECTIONS. Date and Place Presidents lxi Secretaries 1886. Birmingham 1887. Manchester 1888. Bath eee eeeaee 1889, Newcastle - upon-Tyne 1890. Leeds 1891.” Cardiff eee 1892. Edinburgh 1893. Nottingham! 1894, Oxford? ... 1895. Ipswich ... W. Carruthers, Pres. L.S., F.R.S., F.G.S. Prof. A. Newton, M.A., F.B.S., F.L.S., V.P.Z.S. W. T. Thiselton-Dyer, C.M.G., F.R.S., F.L.S8. Prof. J. S. 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.RS., F.L.S. Prof. W. Rutherford, M.D., F.R.S., F.R.S.E. Rey. Canon H. B. Tristram, M.A., LL.D., F.R.S. Prof. I. Bayley Balfour, M.A., F.R.S. 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, Prof. H. Marshall Ward. KF. E. Beddard, 8. F. Harmer, Prof. H. Marshall Ward, W. Gardiner, Prof. W. D. Halliburton. C. Bailey, F. E. Beddard, 8. F. Har- mer, Prof. T. Oliver, Prof. H. Mar- shall Ward. S. F. Harmer, Prof. W. A. Herdman, Dr. §. J. Hickson, Prof. F. W. Oliver, H. Wager, Prof. H. Mar- shall Ward. F. E. Beddard, Prof. W.A. Herdman, Dr. S. 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, 8. 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. SECTION D (continwed).—ZOOLOGY. | Prof. W. A. Herdman, F.R.S.(G. C. Bourne, H. Brown, W. EH. Hoyle, W. L. Sclater. ANATOMICAL AND PHYSIOLOGICAL SCIENCES. COMMITTEE OF SCIENCES, V.—ANATOMY AND PHYSIOLOGY. 1833. Cambridge 1834, Edinburgh Dr. J. Haviland Dr. Abercrombie Dr. H. J. H. Bond, Mr. G. E. Paget. Dr. Roget, Dr. William Thomson. SECTION E (UNTIL 1847).—ANATOMY AND MEDICINE. 1835. Dublin 1836. Bristol 1837. Liverpool... seseee 1838. Newcastle 1839. Birmingham 1840. Glasgow 1841, Plymouth... 1842. Manchester .../James Watson, M.D. Dr. J. C. Pritchard Dr. P. M. Roget, F.R.S. ... Dr. Harrison, Dr. Hart. ...| Dr. Symonds. Prof. W. Clark, M.D. ......... Dr. J. Carson, jun., James Long, Dr. J. R. W. Vose. T. E. Headlam, M.D. ......... T. M. Greenhow, Dr. J. R. W. Vose. John Yelloly, M.D., F.R.S8....| Dr. G. O. Rees, F. Ryland. Dr.J.Brown, Prof, Couper, Prof. Reid. SECTION E.—PHYSIOLOGY. P. M. Roget, M.D., Sec. B.S. |Dr. J. Butter, J. Fuge, Dr. R. S. Sargent. Edward Holme, M.D., F.L.S.|Dr. Chaytor, Dr. R. 8. Sargent. 1843. Cork ......... Sir James Pitcairn, M.D. ...|Dr. John Popham, Dr. R. 8. Sargent. 1844. York......... |J. ©. Pritchard, M.D. .......-. 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. ]xviii. 2 The title of Section D was changed to Zoology. Ixii REPORT—1895. Date and Place 1846 . Southamp- ton. Presidents Secretaries Prof. Owen, M.D., F.R.S. | i C. P. Keele, Dr. Laycock, Dr. Sar gent. 1847. Oxford! .,.|Prof. Ogle, M.D., F.R.S. ......;Dr. Thomas 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 Benjamin Brodie, Bart.,|C. G. Wheelhouse. F.R.S. 1859. Aberdeen... | Prof. Sharpey, M.D., Sec.R.S.|Prof. Bennett, Prof. Redfern. 1860. Oxford...... Prof.G.Roleston,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................ G, F. Helm, Dr. Edward Smith. 1863. Newcastle |Prof. Rolleston, M.D., F.R.S.|Dr. D. Embleton, Dr. W. Turrer. 1864. Bathei:.! Dr. Edward Smith, LL.D.,|J.S. Bartrum, Dr. W. Turner. F.B.S. 1865. Birming- Prof. Acland, M.D., LL.D.,/Dr. A. Fleming, Dr. P. Heslop, ham.” F.R.S. Oliver Pembleton, Dr. W. Turner. p. lv GEOGRAPHICAL AND ETHNOLOGICAL SCIENCES. [For Presidents and Secretaries for Geography previous to 1851, see Section C, - ETHNOLOGICAL SUBSECTIONS OF SECTION 1846.Southampton|Dr. J. C. Pritchard D. Dr. King. 1847. Oxford ...... Prof. H. H. Wilson, M.A. ...|Prof. Buckley. 1848. SWANSED “°5.0].55 ccoossescssdecesnavcsvcsecenodssvasse G. Grant Francis, A849) DITMINe NAM |< sancsapssaeeudusepeesaeneross anes. 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.S.,|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. HSb35: Hull ..... 0a 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.R.S. Ihne, Dr. Norton Shaw, 1855. Glasgow ...|Sir J. Richardson, M.D.,;Dr. W. G. Blackie, R. Cull, Dr, F.R.S. 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, 8S. Ferguson, Dr. R. R. 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. lviii.). Section E, being then vacant, was assigned in 1851 to Geography. 2 Vide note on page lix. PRESIDENTS AND SECRETARIES OF THE SECTIONS. Date and Place xiii Presidents Secretaries 1858. Leeds eeeeee 1859. Aberdeen... 1860. Oxford...... 1861. Manchester 1862. Cambridge 1863. Newcastle 1864, Bath......... 1865. Birmingham 1866. Nottingham 1867. Dundee 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......... 1882. Southamp- ton. 1883. Southport Sir R. I. Murchison, G.C.S8t.S., F.R.S. Rear - Admiral Sir James Clerk Ross, D.C.L., F.R.S. Sir R. I. Murchison, D.C.L., FE.R.S. John Crawfurd, F.R.S.......... Francis Galton, F.R.S.......... Sir R. I. Murchison, K.C.B., F.RB.S. Sir R. I. Murchison, K.C.B., F.RB.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.S. Capt. G. H. Richards, R.N., F.R.S. R. Cull, Francis Galton, P. O’Cal- laghan, Dr. Norton Shaw, Thomas 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. E. T. Cusins, R. H. Major, Clements R. Markham, D. W. Nash, T. Wright. H. W. Bates, Cyril Graham, Clements R. Markham, S. J. Mackie, R. Sturrock. T. Baines, H. W. Bates, Clements R. Markham, T. Wright. SECTION E (continued).—GEOGRAPEHY. Sir Bartle Frere, LL.D., F.R.G.S. Sir R. I. Murchison, Bt.,K.C.B., LL.D., D.C.L., F.R.S., F.G.S. Colonel Yule, C.B., F.R.G.S. K.C.B., Francis Galton, F.R.S.......... Sir Rutherford Alcock, K.C.B. Major Wilson, R.E., F.R.S., F.R.G.S. Lieut. - General Strachey, R.E.,C.S.1.,F.R.S., F.R.G.S., F.L.S., F.G.S. Capt. Evans, C.B., F.R.S....... Adm. Sir E. Ommanney, C.B., E.RB.S., F.R.G.S., F.R.A.S. Prof. Sir C. Wyville Thom- son, LL.D.,F.R.S., F.R.S.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.B.S., ¥.R.G.S. Sir J. D. Hooker, K.C.S.L., C.B., F.R.S. Sir R. Temple, Bart., G.C.S.1., F.R.G.S. Ticot Col! He Ho Godwin: Austen, F.R.S. H. W. Bates, Clements R. Markham, 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. \H. W. Bates, E. C. Rye, F. F. Tuckett. H. W. Bates, E. C. Rye, R. Oliphant Wood. H. W. Bates, F. E. Fox, EH. C. Rye. John Coles, HE. C. Rye. H. W. Bates, C. E. D. Black, E. C. ye. H. W. Bates, E. C. Rye. J. W. Barry, H. W. Bates, E. G. Ravenstein, E. C. Rye John Coles, E. G. Ravenstein, E. C. Rye. lxiv REPORT—1895. Date and Place Presidents Secretaries 1884. 1885. 1886. Birmingham 1887. 1888. 1889. 1890. 1891. 1892. 1893. 1894. 1895. 1833. 1834. 1835. 1836. 1837. 1838. 1839. Birmingham 1840. 1841. 1842. 1843. 1844. 1845. 1846. 1847. 1848. 1849. Birmingham Montreal ... Aberdeen... Manchester Newcastle- upon-Tyne Leeds Carditi sc...» Edinburgh Nottingham Oxford...... Ipswich ...| Edinburgh Dublin Bristol aeneee Liverpool... Newcastle Glasgow ... Plymouth... Manchester Cambridge Southamp- ton. Oxford Swansea ... Gen. Sir J. H. Lefroy, C.B., K.C.M.G., F.R.S.,V.P.8.G.8. Gen. J. T. Walker, C.B., R.E., LL.D., F.B.S. Maj.-Gen. Sir. F. J. Goldsmid, KGS oly, Cab. pictus. Col. Sir C. Warren, R.E., G.C.M.G., F.RB.S., F.R.G.S. Col. Sir C. W. Wilson, R.E., K.C.B., F.B.S., F.R.G.S. Col. Sir F. de Winton, K.C.M G., C.B., F.B.G.S. Lieut.-Col. Sir R. Lambert Playfair, K.C.M.G., F.R.G.S, E. G. Ravenstein, F.R.G.S., F.8.8. Prof. J. Geikie, D.C.L., F.B.S., V.P.R.Scot.G.8. H. Seebohm, Sec. B.S8., F.L.S., ¥.ZS. Rev. Abbé Laflamme, J.S. O'Halloran, E. G. Ravenstein, J. F. Torrance. J.S. Keltie, J. S. O'Halloran, E. G. Ravenstein, Rev. G. A. Smith. F. T. §. Houghton, J. 8S. Keltie, KE. G. Ravenstein. 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. Capt. W.J. L. Wharton, R.N., \John Coles, W. S. Dalgleish, H. N. TMS J. Mackinder, F.R.G.S. H. M.A., Dickson, Dr. H. R. Mill. John Coles, H. N. Dickson, Dr. H. R. Mill, W. A. Taylor. STATISTICAL SCIENCE. COMMITTEE OF SCIENCES, VI.—STATISTICS. Cambridge | Prof. Babbage, F.R.S. ........./J. E. Drinkwater. Sir Charles Lemon, Bart....... Dr. Cleland, C. Hope Maclean. SECTION F.—STATISTICS. Charles Babbage, F.R.S. ...... Sir Chas. Lemon, Bart., F.R.5. Rt. Hon. Lord Sandon Colonel Sykes, F.R.S. ......... Henry Hallam, F.R.S.......... Rt. Hon. Lord Sandon, M.P., E.R.S. Lieut.-Col. Sykes, F.R.S....... G. W. Wood, M.P., F.L.S. ... Sir C. Lemon, Bart., M.P. .. Lieut.-Col. Sykes, F-.R.S., F.L.S. Rt. Hon. the Earl Fitzwilliam Gp shOTcer dE Ds sccacasststts Travers Twiss, D.C.L., F.R.S. J. H. Vivian, M.P., F.R.S. ... Rt. Hon. Lord Lyttelton...... 1850. Edinburgh |Very Rev. Dr. John Lee, i V.P.R.S.E. } W. Greg, Prof. Longfield. Rev. J. E. Bromby, C. B. Fripp, James Heywood. W. R. 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. Rev. 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. Prof. Hancock, J. Fletcher, Dr. J. Stark. 1855. Glasgow es) PRESIDENTS AND SECRETARIES OF THE SECTIONS. lxv Date and Place Presidents 1851. Ipswich 1852. Belfast...... 1853. Hull 1854. Liverpool...) Thomas Tooke, F.R.S. ......... ...|Sir John P. Boileau, Bart. ... His Grace the Archbishop of Dublin. James Heywood, M.P., F.R.S. R. Monckton Milnes, M.P.... Secretaries J. Fletcher, Prof. Hancock. Prof. Hancock, Prof. Ingram, James MacAdam, jun. Edward Cheshire, W. Newmarch. E. Cheshire, J. T. Danson, Dr. W. H. Duncan, W. Newmarch. J. A. Campbell, E. Cheshire, W. New- march, Prof. R. H. Walsh, SECTION F (continued ).—ECONOMIC SCIENCE AND STATISTICS. 1856. Cheltenham/ Rt. Hon. Lord Stanley, M.P. 1857. Dublin 1858. Leeds ....... 1859. Aberdeen... 1867. Dundee . $ 1860. Oxford 1861. Manchester 1862. Cambridge 1863. Newcastle . 1864. Bath 1865. Birmingham 1866. Nottingham 1868. Norwich.... 1869. Exeter 1870. Liverpool... 1871. Edinburgh 1872. Brighton... 1873. Bradford ... 1874. Belfast ee eeee 1875. Bristol...... 1876. Glasgow 1877. Plymouth... 1878. Dublin 1879. Sheffield ... 1880. Swansea ... Peel. York.....:... 1882. Southamp- ton, 1895. His Grace the Archbishop of Dublin, M.R.LA. Edward Baines Col. Sykes, M.P., F.R.S. ...... Nassau W. Senior, M.A. ...... William Newmarch, F.R.S.... Edwin Chadwick, C.B. ........ William Tite, M.P., F.R.S.... William Farr, M.D., D.C.L., E.R.S. Rt. Hon. Lord Stanley, LL.D., M.P. Prof. J. E. T. Rogers see eweerseee M. E. Grant-Duff, M.P. ....... Samuel*Brownl tt siz. 29.60.35 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.| ond) OFM a cami... cwees dees se James Heywood, M.A.,F.R.S., Pres. 8.5. ... | Sir George Campbell, K.C.S.L, M.P. Rt. Hon. the Earl Fortescue Prof. J. K. Ingram, LL.D..,| M.R.LA. G. Shaw Lefevre, M.P., Pres. 8.8. Goa Wing blastin os siVi IPs so52 sa. ant Rt. Hon. M. E. Grant-Duff, | _ M.A., F.R.S. Rt. Hon. G. Sclater-Booth, M.P., F.BR.S. Rey. 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, HE. Macrory, Prof. J. E. T. Rogers. H. D. Macleod, Hdmund Macrory. T. Doubleday, Edmund Macrory, Frederick Purdy, James Potts. E. Macrory, H. T. Payne, F. Purdy. G. J. D. Goodman, G. J. Johnston, EK. Macrory. |R. Birkin, jun., Prof. Leone Levi, E. Macrory. Prof, Leone Levi, E. Macrory, A. J. Warden. Rey. 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. A. M'‘Neel Caird, T.G. P. Hallett, Dr. W. Neilson Hancock, Dr. W. Jack. W. F. Collier, P. Hallett, J. T. Pim. W. J. Hancock, C. Molloy, J. T. Pim. Prof. Adamson, R. E. Leader, C. Molloy. N. A. Humphreys, C. Molloy. C. Molloy, W. W. Morrell, J. F. Moss. G. Baden-Powell, Prof. H. 8. Fox- well, A. Milnes, C. Molloy. Ixvi Date and Place 1883. 1884. 1885. 1886. 1887. 1888. 1889. 1890. 1891. 1892. 1893. 1894, 1895. 1836. 1837. 1838. 1839. 1840. 1841. 1842. 1843. 1844. 1845. 1846. 1847. 1848. 1849. 1850. 1851, Southport Montreal ... Aberdeen... Birmingham Manchester Newcastle- upon-Tyne Leeds seeeee Cardiff Edinburgh Nottingham Oxford Ipswich pam MENICe. eM CAs teosacn Bristol .....- Liverpool... Newcastle Birmingham Glasgow ... Plymouth Manchester Cambridge South’mpt’n Oxford...... Swansea ... Birmingh’m Edinburgh Ipawich ..... .|Sir John Robinson REPORT—1895. Presidents R. H. Inglis Palgrave, F.R.S. Sir Richard Temple, Bart., G.C.S.I., C.LE., F.R.G.S. Prof. H. Sidgwick, LL.D., Litt.D. J. B. Martin, M.A., F.S.S. Robert Giffen, LL.D.,V.P.S.8. Rt. Hon, Lord Bramvell, LL.D., F.R.S. Prof. F. Y. Edgeworth, M.A., F.S.S. Prof, A. Marshall, M.A., F..S. Prof. W. Cunningham, D.D., D.Sc., F.8.8. Hon. Sir C. W. Fremantle, K.C.B. Prof. J. 8. Nicholson, D.Sc., FE.S.S8. Prof. C. F. Bastable, M.A., F.S.S. .|E. Cannan, Prof. E. C. Secretaries Rev. W. Cunningham, Prof. H. S. Foxwell, J. N. Keynes, C. Molloy. Prof. H. 8S. Foxwell, J.S. McLennan, Prof. J. Watson. Rev. W. Cunningham, Prof. H. 8. Foxwell, C. McCombie, J. F. Moss. F. F. Barham, Rev. W. Cunningham, Prof. H. 8. Foxwell, J. F. Moss. Rev. W. Cunningham, F. Y. Edge- worth, T. H. Elliott, C. Hughes, J. E. C. Munro, G. H. Sargant. Prof. F. Y. Edgeworth, T. H. Elliott, H. §. 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. R. Price. Prof. J. Brough, E. Cannan, Prof. E. C. K. Gonner, H. Ll. Smith, Prof. W. R. Sorley. Prof. J. Brough, J. R. Findlay, Prof. E. C. K. Gonner, H. Higgs, L. L. F. R. Price. Prof. E. C. K. Gonner, H. de B. Gibbins, J. A. H. Green, H. Higgs, 1) Geen. serice: E. Cannan, Prof. E. C. K. Gonner, W. A. 5S. Hewins, H. Higgs. K. Gonner, H, Higgs. MECHANICAL SCIENCE. SECTION G.—MECHANICAL SCIENCE. Davies Gilbert, D.C.L., F.R.S Rev. Dr. Robinsor ............ Charles Babbage, F.R.S....... Prof. Willis, F.R.S., and Robt. Stephenson. Pee eeeweeesee John Taylor, F.R.S. ......e00 Rev. Prof. Willis, F.R.S ...... Prof. J. Macneill, M.R.J.A.... DOHnNaylorel. Raw. -cacccsetsne George Rennie, F.R.S.. Rev. Prof. Willis, M.A., F. R. s. Rev. Prof.Walker, M. Ne F.a.S. Rev. Prof.Walker, M.A.,F.8.S. Robt. Stephenson, M.P., F.R.S Reve ive WODINSORF s+. ce. scar ene William Cubitt, F.R.S.. .{T. G. Bunt, G. T. Clark, W. West. Charles Vignoles, Thomas Webster. R. Hawthorn, C. Vignoles, T. Webster. W. Carpmael, William Hawkes, T-. Webster. J. Scott Russell, J. Thomson, J. Tod, C. Vignoles. .|Henry Chatfield, Thomas Webster. J. F. Bateman, J. Scott Russell, J. Thomson, Charles Vignoles. James Thomson, Robert Mallet. Charles Vignoles, Thomas Webster. .|Rev. W. T. Kingsley. .| William Betts, jun., Charles Manby, J. Glynn, R. A. Le Mesurier. R. A. Le Mesurier, W. P. Struvé. .|Charles Manby, W. P. Marshall. Dr. Lees, David Stephenson. .!John Head, Charles Manby 1869. Exeter 1870. Liverpool... PRESIDENTS AND SECRETARIES OF THE SECTIONS. Date and Place 1853. 1854. 1855. Liverpool... Glasgow ... Cheltenham Dublin 1856. 1857. Dublin...... Leeds ...... Aberdeen... 1858. 1859. 1860. Oxford 1861. Manchester 1862. 1863. Cambridge Newcastle 1864. Bath 1865. Birmingham ae eeeeeee 1866. Nottingham 1867. Dundee...... 1868. Norwich 1871. Edinburgh 1872. Brighton ... 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... Ixvii Presidents John Walker, C.E., LL.D., F.R.S. William Fairbairn, E.R.S. John Scott Russell, F.R.S. ... W. J. Macquorn Rankine, F.R.S. George Rennie, F.R.S. ...... Rt. Hon. the Earl of Rosse, E.R.S. William Fairbairn, F.R.S.... Rev. Prof. Willis, M.A., F.R.S. C.E., Prof.W.J.Macquorn Rankine, LL.D., F.RB.S. J. F. Bateman, C.E., F.R.S.... William Fairbairn, F.R.S. Rev. Prof. Willis, M.A., F.R.S. J. Hawkshaw, F.R.S. Sir W. G. Armstrong, cae D., F.R.S. Thomas Hawksley, V.P. Inst. C.E., F.G.S. Prof.W.J. Macquorn Rankine, | LL.D., F.B.S. ... |G. P. Bidder, C.H., F.R.G.S. C. W. Siemens, F.R.S..........| Chas. B. Vignoles, C.E., F.R.S. | Prof. Fleeming Jenkin, F.R.S.. F. J. Bramwell, C.E. W. H. Barlow, F.R.S. ......... Prof. James Thomson, LL.D., C.E., F.R.S.E. W. Froude, C.E., M.A., F.R.S. C. W. Merrifield, F.R.S. ...... Edward Woods, C.E. eee eeeene Edward Easton, C.E. J. Robinson, Pres. Inst. Mech. Eng. .../James Abernethy, V.P. Inst. C.E., F.R.S.E. Sir W. G. Armstrong, LL.D., D.C.L., F.R.S. John Fowler, C.E., F.G.S. ... C.B., J. Brunlees, Pres. Inst.C.E. Sir F. J. Bramwell, F.R.S., V.P.Inst.C.E. Secretaries John F. Bateman, C. B. Hancock, Charles Manby, James Thomson. James Oldham, J. Thomson, W. Sykes Ward. J. Grantham, J. Oldham, J. Thomson, L. Hill, W. Ramsay, J. Thomson. ...|C. Atherton, B. Jones, H. M. Jeffery. Prof. Downing, W.T. Doyne, A. Tate, James Thomson, Henry Wright. J. CO. Dennis, J. Dixon, H. Wright. R. Abernethy, P. Le Neve Foster, H. Wright. P. Le Neve Foster, Rev. F'. Harrison, Henry Wright. P. Le Neve Foster, John Robinson H. Wright. W. M. Fawcett, P. Le Neve Foster. P. Le Neve Foster, P. Westmacotr. J. F. Spencer. ..|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, C. Manby, W. Smith. P. Le Neve Foster, H. Bauerman. H. Bauerman, P. Le Neve Foster, T. King, J. N. Shoolbred. 'H. Bauerman, Alexander Leslie, J. P. Smith. 'H. M. Brunel, P. Le Neve Foster, J. G. Gamble, J. N. Shoolbred. Crawford 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. IT. 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. 9 = ad Uxvi i Date and Place 4885. Aberdeen... REPORT—1895. Presidents Secretaries B. Baker, M.Inst.C.E. ......... A. T. Atchison, F. G. Ogilvie, E. Rigg, J. N. Shoolbred. C. W. Cooke, J. Kenward, W. B. Marshall, E. Rigg. C. F. Budenberg, W. B. Marshall, BE. Rigg. C. W. Cooke, W. LB. Marshall, E. Rigg, P. K. Stothert. C. W. Cooke, W. LB. Marshall, Hon. | OO, A. Parsons, E. Rigg. E. K. Clark, C. W. Cooke, W. B. Marshall, E. Rigg. |\C. 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. ROPOLOGY. E. B. Tylor, D.C.L., F.R.S....|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. iG. 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, Jeyons, J. L. Myres. H. Baifour, Dr. J. G.Garson, H. Ling Roth. J. L. Myres, Rey. J. J. Raven, H. Ling Roth. SECTION I.—PHYSIOLOGY (including Experimenta |Prof F. Gotch, Dr. J. S. Haldane, M. 8. Pembrey. 1886. Birmingham Sir J. N. Douglass, M.Inst. C.E. 1887. Manchester | Prof. Osborne Reynolds, M.A., LL.D., F.B.S. 1888. Bath......... W. oH. Preece, F.RBS., M.Inst.C.E. 1889. Newcastle- | W. Anderson, M.Inst.C.E. ... upon-Tyne 1890. Leeds ...... ‘Capt. A. Noble, C.B., F.B.S., F.R.A.S. 1891, Cardiff...,,./T. Forster Brown, M.Inst.C.E., 1892. Edinburgh |Prof. W. C. Unwin, F.RS., M.Inst.C.E. #893. Nottingham Jeremiah Head, M.Inst.C.E., F.C.S. 1894. Oxford...... Prof. A. B. W. Kennedy, F.R.S., M.Inst.C.E. 1895. Ipswich ...|Prof. L. F. Vernon-Harcourt, M.A., M.Inst.C.E. SECTION H.—ANTH 1884. Montreal... 1885. Aberdeen...| Francis Galton, M.A., F.R.S. 1886. Birmingham |Sir G. Campbell, K.C.S.L, M.P., D.C.L., F.R.G.S. 1887. Manchester | Prof. A. H. Sayce, M.A. ...... 1888. Bath......... Lieut.-General _ Pitt-Rivers, D.C.L., F.R.S. 1889. Newcastle- |Prof. Sir W. Turner, M.B., upon-Tyne}| LL.D., F.R.S. 1890. Leeds ...... Dr. J. Evans, Treas. RS, F.S.A., F.L.S., F.G.S. 1891. Cardiff...... Prof. F. Max Miiller, M.A. ... 1892. Edinburgh | Prof. A. Macalister, M.A., M.D., F.R.S. ¥893. Nottingham) Dr. R. Munro, M.A., F.R.S.E. 1894. Oxford...... Sir W. H. Flower, K.C.B., E.R.S. 1895. Ipswich ...|Prof. W. M. Flinders Petrie, D.C.L. PATHOLOGY AND EXPERIMENTAL PsyCHOLOGY). 4894. Oxford...... Prof. E. A. Schifer, F.R.S., M.R.C.S. SECTION K.—BOTANY. 1895. Ipswich ... | W. T. Thiselton-Dyer, F.RB.S. | Prof. F. E. Weiss, A. C. Seward. a we 1849. 1852. LIST OF EVENING LECTURES. LIST OF EVENING lxix LECTURES. Date and Place 1842. Manchester 1843. Cork 1845. Cambridge 1846. Southamp- ton, ; 1847. 1848. Swansea Birmingham 1850. Edinburgh 1851. Ipswich ... Belfast...... 1863. Hull..,...... 1854. Liverpool... 1855. Glasgow ... 1856. Cheltenham Lecturer Charles Vignoles, F.R.S.... Sir M. J. Brunel Ltr eV CHI SOMs, ce wslvcsces sana Prof. Owen, M:D., F.R.S....... Prof. E. Forbes, F'.R.S.......... seca weer eee eree DO LNSOM esse eres code eets Charles Lyell, F.R.S. ........ Dr. Falconer, F.R.S............. G.B.Airy,F.R.S.,Astron.Royal R. I. Murchison, F.R.S. ...... Prof. Owen, M.D., F.R.S. Charles Lyell, F.R.S. ......... Wrarrkts Groves HUN Sac, .saccsacee Rey. Prof. B. Powell, F.R.S. Prof. M. Faraday, F.R.S....... Hugh E. Strickland, F.G.S.... ---(John Percy, M.D., F.R.S....... W. Carpenter, M.D., F.R.S.... Hata aye His Hua -Avese vaca 5 Rev. Prof. Willis, M.A., F.R.S. Prof. J. H. Bennett, M.D., F.R.S.E. Dr. Mantell, F.R.S. Prof. R. Owen, M.D., F.R.S. eee eeeeeeeee G.B.Airy,F.R.S.,Astron. Royal Prof. G. G. Stokes, D.C.L., F.R.S. Colonel Portlock, R.E., F.R.S. < Prof. J. Phillips, LL.D., F.B.S., F.G.S. Robert Hunt, F.R.S... Prof. R. Owen, M.D., F, R. Ss. Col. E. Sabine, V.P. R. Ss. Dr. W. B. Carpenter, F.R.S. Lieut.-Col. H. Rawlinson Col. Sir H, Rawlinson ........ W. R. Grove, F’.RB.S.......... Subject of Discourse The Principles and Construction of Atmospheric Railways. The Thames Tunnel. The Geology of Russia. The Dinornis of New Zealand. The Distribution of Animal Life in the Aigean Sea. The Earl of Rosse’s Telescope. -|Geology of North America. The Gigantic Tortoise of the Siwali& Hills in India. Progress of Terrestrial Magnetism. Geology of Russia. ...| Fossil Mammaliaof the British Isles. Valley and Delta of the Mississippi. Properties of the ExplosiveSubstance discovered by Dr. Schénbein; alse some Researches of his own on the Decomposition of Water by Heat. Shooting Stars. Magnetic and Diamagnetic Pheno- mena. The Dodo (Didus ineptus). Metallurgical Operations of Swansea and its Neighbourhood. Recent Microscopical Discoveries. Mr. Gassiot’s Battery. Transit of different Weights with varying Velocities on Railways. Passage of the Blood through the minute vessels of Animals in con- nection with Nutrition. Extinct Birds of New Zealand. Distinction between Plants and Ani- mals, and their changes of Form. Total Solar Eclipse of July 28, 1851. Recent Discoveries in the properties of Light. Recent Discovery of Rock-salt at Carrickfergus, and geological and practical considerations connected with it. Some peculiar Phenomena in the Geology and Physical Geography of Yorkshire. .|The present state of Photography. Anthropomorphous Apes.. ..| Progress of Researches in Terrestrial Magnetism. Characters of Species. ..| Assyrian and Babylonian Antiquities and Ethnology. -|Recent Discoveries in Assyria and Babylonia, with the results of Cuneiform Research up to the present time. .. (Correlation of Physical Forces, lxx REPORT—1895. Date and Place Lecturer Subject of Discourse 1864. 1865. 1866. 1867. 1871. 73. Bradford . . Oxford . Belfast . Bristol seeeee . Aberdeen... . Manchester 2 Cambridge . Newcastle Birmingham Nottingham Dundee...... . Norwich ... . Liverpool... Edinburgh . Brighton ... carro . Glasgow .., | Rev. Dr. Robinson, F.R.S. ... Prof. J. Phillips, LL.D.,F.R.S. i Prof.W.J. Macquorn Rankine, ..| Prof. W. C.Williamson, Prof. W. Thomson, F.R.S. ... Rev. Dr. Livingstone, D.O-L, Prof. J. Phillips, LL.D.,F.R.S. Prof. R. Owen, M.D., F.R.S. Sir R. I. Murchison, D.C.L.... Rev. Prof. Walker, F.R.S. Prof.W.A. Miller, M.A., F.B.S. G. B. Airy, F.R.S., Astron. Royal. Prof. Tyndall, LL.D., ¥.R.S. rota OGM TH BS. vc esee cess Prof. Williamson, F.R.6....... James Glaisher, F.R.S......... ENOtWOSCOCs Hh Ou scr sccsure Dr. Livingstone, F.R.S. ...... J. Beete Jukes, F.R.S.......... William Huggins, F.R.S....... Dr. J. D. Hooker, F.R.S....... Archibald Geikie, F.R.S....... Alexander Herschel, F.R.A.S. | J. Fergusson, F.R.S............. Drs Win Odline. HORS: csc. J. Norman Lockyer, F.R.S.... Prof. J. Tyndall, LL.D., .R.S. LL.D., F.R.S. AA ADE]. FN HDss0sesu vecesess EBs DyloruhsR.S. sc. Prof. P. Martin Duncan, M.B., F.R.S. Prof. W. K. Clifford tee we eneeee ™ igs Prof. Clerk Maxwell, F. Sir John Lubbock, Bart. M. P. ; F.R.S. Prof. Huxley, F.R.S. ......... W.Spottiswoode,LL.D.,F.R.S. F. J. Bramwell, F.R.S.......... Prof. Tait, F.R. 's. E. The Atlantic Telegraph. Recent Discoveries in Africa. The Ironstones of Yorkshire. The Fossil Mammalia of Australia. Geology of the Northern Highlands. Electrical Discharges in highly rarefied Media. ...| Physical Constitution of the Sun, Captain Sherard Osborn, R.N. Arctic Discovery. Spectrum Analysis. The late Eclipse of the Sun. The Forms and Action of Water. Organic Chemistry. The Chemistry of the Galvanic Bat- tery considered in relation to Dynamics. The Balloon Ascents made for the British Association. ..|The Chemical Action of Light. Recent Travels in Africa. Probabilities as to the position and extent of the Coal-measures be- neath the red rocks of the Mid- land Counties. The results of Spectrum Analysis applied to Heavenly Bodies. Insular Floras. The Geological Origin of the present Scenery of Scotland. The present state of Knowledge re- garding Meteors and Meteorites. Archeology of the early Buddhist Monuments. Reverse Chemical Actions. Vesuvius. The Physical Constitution of the Stars and Nebulz. The Scientific Use of the Imagina- tion. Stream-lines and Waves, in connec- tion with Naval Architecture. Some Reeent Investigations and Ap- plications of Explosive Agents. ..| The Relation of Primitive to Modern Civilisation. Insect Metamorphosis. The Aims and Instruments of Scien- tific Thought. .|Coal and Coal Plants. Molecules. Common Wild Flowers considered in relation to Insects. The Hypothesis that Animals are Automata, and its History. The Colours of Polarised Light. Railway Safety Appliances, .| Force. Sir Wyville Thomson, F. R. 8. The Challenger Expedition. a * Da 1877. 1878. 1879. 1880. 1881. 1882. 1883. 1884. 1885 1886. 1887. 1888. 1889. 1890. 1891. 1892. 1893. 1894. 1895. te and Place Plymouth... Dublin Sheffield ... Swansea Southamp- ton. Southport Montreal... . Aberdeen... Birmingham Manchester Newcastle- upon-Tyne aeeeee Edinburgh Nottingham Oxford...... Ipswich LIST OF EVENING LECTURES. lxxi Lecturer W. Warington Smyth, M.A., F.R.S. Prof. Odling, F.R.S...........06 G. J. Romanes, F.L.S.......... Prof. Dewar, F.R.S, .:.........- W. Crookes, F.R.S. .........008 Prof. E. Ray Lankester, F.R.S. ... | Prof.W.Boyd Dawkins, F.R.8. Francis Galton, F.H.S.......... Prof. Huxley, Sec. B.S. W. Spottiswoode, Pres. R.S.... Prof. Sir Wm. Thomsen, F.R.S. Prof. H. N. Moseley, F.R.S. Veron toy Gets el 621) OS) GAS eee Prof. J. G@. McKendrick, F.R.S.E. Prof. O. J. Lodge, D.Sc. ...... Rev. W. H. Dallinger, F.R.8. Prof. W. G. Adams, F.R.S. ... John Murray, F.R.S.E.......... A. W. Riicker, M.A., F.RB.S. Prof. W. Rutherford, M.D.... Prof. H. B. Dixon, F.R.S. .. Col. Sir F. de Winton, K.C.M.G. Prof. W. E. Ayrton, F.R.S.... Prof. T. G. Bonney, D.Sc., F.R.S. Prof. W. C. Roberts-Austen, F.R.S. Walter Gardiner, M.A......... E. B. Poulton, M.A., F.R.S.... Prof. C. Vernon Boys, F.R.S8. Prof. L. C. Miall, ¥.L.8., F.G.S8. Prof. A.W. Riicker, M.A.,F.BR.8. Prof. A. Milnes Marshall, D.Sc., F.RB.S. Prof. J.A. Ewing, M.A., F.R.S., F.R.S.E. Prof. A. Smithells, B.Sc. Prof. Victor Horsley, F.R.S. J. W. Gregory, D.Sc., F.G.S. Prof. J.Shield Nicholson, M.A. ... | Prof. 8. P. Thompson, F.R.5., Prof. Perey F. Frankland, E.R.S. Subject of Discourse The Physical Phenomena connected with the Mines of Cornwall and Devon. The New Element, Gallium. Animal Intelligence. Dissociation, or Modern Ideas of Chemical Action. Radiant Matter. Degeneration. Primeval Man. Mental Imagery. The Rise and Progress of Palzon- tology. The Electric Discharge, its Forms and its Functions. Tides. Pelagic Life. Recent Researches on the Distance of the Sun. Galvanic and Animal Electricity. Dust. The Modern Microscope in Re- searches on the Least and Lowest Forms of Life. The Electric Light and Atmospheric Absorption. The Great Ocean Basins. Soap Bubbles. The Sense of Hearing. .|The Rate of Explosions in Gases, Explorations in Central Africa. The Electrical Transmission of Power. The Foundation Stones of the Earth’s Crust. The Hardening and Tempering of Steel. How Plants maintain themselves in the Struggle for Existence. Mimicry. Quartz Fibres and their Applications, Some Difficulties in the Life of Aquatic Insects. Electrical Stress. Pedigrees. Magnetic Induction. Flame. The Discovery of the Physiology of the Nervous System. Experiences and Prospects of African Exploration. Historical Progress and Ideal So- cialism. Magnetism in Rotation. The Work of Pasteur and its various Developments. —— lxxii REPORT—1895. LECTURES TO THE OPERATIVE CLASSES. Subject of Discourse Date and Place Lecturer 1867. Dundee...... Prof. J. Tyndall, LL.D., F.R.S. 1868. Norwich ...|Prof. Huxley, LL.D., F. B.S. 1869. Exeter ...... Prof, Miller, M.D., F.R.S. 1870. Liverpool... |Sir John Lubbock, Bart.,M.P., F.B.S. 1872. Brighton ...| W.Spottiswoode,LL.D.,F.R.S. 1873. Bradford ...|C. W. Siemens, D.C.L., F.R.S. 1874, Belfast...... Prot jOdling SH sh-Sissdcaes sey 1875. Bristol ...... Dr. W. B. Carpenter, F.R.S. 1876. Glasgow ...|Commander Cameron, C.B., RN. 1877. Plymouth ...|\W. Ele PLe@Ce....ccccssscosscsceves 1879: Sheffield ....| Wi. He Ayrton. seccscccecesssereee 1880. Swansea ...|H. Seebohm, F.Z.S. ..........0. ES PYVOLK: «.c5scn0 Prof. Osborne Reynolds, F.R.S. 1882. Southamp- |John Evans, D.C.L.,Treas. B.S. ton. 1883. Southport |Sir F. J. Bramwell, F.RB.S. ... 1884. Montreal ...| Prof. R. 8. Ball, F.R.S......... 1885. Aberdeen ...|H. B. Dixon, M.A. ............ 1886. Birmingham|Prof. W. C. Roberts-Austen, F.R.S. 1887. Manchester | Prof. G. Forbes, F.R.S. ...... 1888. Bath......... Sir John Lubbock, Bart., M.P., F.B.S. 1889. Newcastle- |B. Baker, M.Inst.C.E. ......... upon-Tyne 1890. Leeds ...... Prof. J. Perry, D.Sc., F.R.S. 1891. Cardiff ...... Prof. 8. P. Thompson, F.R.S8. 1892. Edinburgh | Prof. C. Vernon Boys, F.R.S. 1893. Nottingham | Prof. Vivian B. Lewes......... 1894. Oxford...... Prof. W. J. Sollas, F.R.S. W895. Ipswich, ...| Dr. A... Hison)......:cs<:s rine Matter and Force. A Piece of Chalk. .|Experimental Illustrations of the modes of detecting the Composi- tion of the Sun and other Heavenly Bodies by the Spectrum, Savages. Sunshine, Sea, and Sk Fuel. The Discovery of Oxygen. A Piece of Limestone. A Journey through Africa. Telegraphy and the Telephone. Electricity as a Motive Power. The North-East Passage. Raindrops, Hailstones, and Snow- flakes. Unwritten History, and how to read it. Talking by Electricity—Telephones. .|Comets. The Nature of Explosions. The Colours of Metals and their Alloys. Electric Lighting. The Customs of Savage Races. The Forth Bridge. Spinning Tops. Electricity in Mining. Electric Spark Photographs, Spontaneous Combustion. .|Geologies and Deluges. Colour. oe" a aS : lxxili OFFICERS OF SECTIONAL COMMITTEES PRESENT AT THE IPSWICH MEETING. SECTION A.—MATHEMATICAL AND PHYSICAL SCIENCE. President.—Professor W. M. Hicks, M.A., D.Sc., F.B.S. Vice-Presidents.—Prof. W. E. Ayrton, F.R.S. ; Prof. O. Henrici, F.R.S. ; Lord Kelvin, Pres.R.S.; Lord Rayleigh, Sec.R.S.; Prof. A. W. Ricker, F.R.S. Secretaries.—Professor W. H. Heaton, M.A.; Professor A. Lodge, M.A. (Recorder); G. T. Walker, M.A. ; W. Watson, B.Sc. SECTION B.—-CHEMISTRY, President.—Professor R. Meldola, F.R.S8., For.Sec.C.8. Vice Presidents.—Prof. P. P. Bedson, D.Sc. ; Prof. H. B. Dixon, F.R.S. ; Professor E. Frankland, D.C.L., F.R.S.; J. H. Gladstone, Ph.D., F.R.S. ; Professor Ira Remsen, Ph.D. ; Sir Henry E. Roscoe, D.C.L., F.RS. Secretaries.—E. H. Fison; C. A. Kohn, Ph.D., B.Sc. ; Arthur Harden, M.S8c., Ph.D. (Recorder) ; J. W. Rodger. SECTION C.— GEOLOGY. President.—W. Whitaker, B.A., F.R.S. Vice-Presidents—Gustave Dollfus; L. Fletcher, M.A., F.R.S.; F. W- Harmer ; Rev. E. Hill, M.A.; J. E. Marr, M.A., F.R.S. ; E. van den Broek. Secretaries.—F. A. Bather, M.A.; G. W. Lamplugh; Alfred Harker, M.A. ; Clement Reid, F.L.S. (Recorder). SECTION D.—BIOLOGY. President.—Professor W. A. Herdman, D.Sc., F.R.S., F.R.S.E. Vice-Presidents.—Prof. L. C. Miall, F.R.S. ; P. L. Sclater, Ph.D., F.R.S. ; Secretaries—G. C. Bourne, M.A. (Recorder) ; Herbert Brown, M.D. ; W. E. Hoyle, M.A.; W. L. Sclater, M.A. SECTION E.—GEOGRAPHY. President.—H. J. Mackinder, M.A., F.R.G.S. lxxiv REPORT—1895. Vice-Presidents.—Major L. Darwin ; Col. H. H. Godwin Austen, F.R.S. Sir Joseph Hooker, F.R.S. ; J. ’ Scott Keltie ; John Murray, D.Sc. E. G. Ravenstein ; Cal Sir C. Warren, F.RS. Secretaries.—J, Coles, F.R.A.S.; H. N. Dickson, F.R.S.E. ; Hugh Robert Mill, D.Sc., F.R.S.E. (Recorder) ; ee Taylor, F.RS.E. . > > SECTION F,—ECONOMIC SCIENCE AND STATISTICS, President.—L. L. Price, M.A., Vice-Presidents.—Professor F. Y. Edgeworth, M.A., D.C.L., F.S.S. ; The Hon. Sir Charles Fremantle, K.C.B.; J. B. Martin; J. E. C. Munro ; R. H. Inglis Palgrave, F.R.S. é Secretaries.— KE. Cannan, M.A., F.8.8. ; Professor E. C. K. Gonner, M.A., F.S.8. (Recorder); H. Higgs, LL.B. SECTION G.—MECHANICAL SCIENCE. President.—Professor L. F. Vernon Harcourt, M.A., M.Inst.C.E.. Vice-Presidents.—Professor A. B. W. Kennedy, F.R.S., M.Inst.C.E. ; E. Rigg, M.A.; Professor Silvanus P. Thompson, F.R.8.; W. H. Wheeler, M.Inst.C.G. Secretaries.—Professor T. Hudson Beare, F.R.S.E. (Recorder) ; Conrad W. Cooke; W. Bayley Marshall, M.Inst.C.E. ; F. G. M. Stoney, M.Inst.C.E. SECTION H.—ANTHROPOLOGY. President. —Professor W. M. Flinders Petrie, D.C.L. Vice-Presidents.—Sir John Evans, K.C.B., F.R.S.; Sir W. H. Flower, K.C.B., F.R.S. ; R. Munro, M.D., F.R.S.E. Secretaries.—J. L. Myres, M.A.; Rev. J. J. Raven, D.D. ; H. Ling Roth (Recorder). SECTION K,—BOTANY. President.—W. T. Thiselton-Dyer, C.M.G., C.LE., F.R.S. Vice-Presidents.—Professor Bayley Balfour, M.A., F.R.S.; Professor F. O. Bower, F.R.S.; F. Darwin, F.R.S.; Sir Joseph Hooker, F.R.S. Secretaries.—Professor F. E. Weiss (Recorder) ; A. C. Seward, M.A. OFFICERS AND COUNCIL, 1895-96. PRESIDENT. Captain SIR DOUGLAS GALTON, K.C.B., D.C.L,, LL.D., F.R.S., F.R.G.S., F.G.S. VICE-PRESIDENTS. The Most Hon, the Marquis or Briston, M.A., The Right Hon. Lorp HENNIKER, F.S.A. Lord-Lieutenant of the County of Suffolk. The Right Hon, LorpD RENDLESHAM. The Right Hon. Lorp WarsineHAM, UL.D., F.R.S., | J. H. BARTLEeT, Esq., MAYOR OF IpswicH. High Steward of the University of Cambridge. Sir G. G. SroxEs, Bart., D.C.L., F.R.S. The Right Hon. Lorp RayuricH, D.C.L., Sec.R.S., | Dr. E. FRANKLAND, D.C.L., F.R.S. Lord-Lieutenant of the County of Essex. Professor G. H. DARWIN, M.A., LL.D., F.R.S. The Right Hon. LorpD Gwypyr, M.A., High | Friix T. Coppoxp, Esq., M.A. Steward of the Borough of Ipswich. PRESIDENT ELECT. SIR JOSEPH LISTER, Barr., D.C.L., LL.D., Pres.R.S. VICE-PRESIDENTS ELECT. The Right Hon, the EArt or Dunsy,G.C.B., Lord | THE Principat of University College, Liverpool. Mayor of Liverpool. W. RatHeone, Esq., LL D. The Right Hon. the Eart or Serron, K.G., Lord- W. Crookgs, Esq., F.R.S. Lieutenant of Lancashire. GrorGE HOLT, Esy., J.P. Sir W. B. Forwoop. T. H. Ismay, Esq., J.P., D.L. Sir Henry E. Roscor, D.C.L., F.R.S. GENERAL SECRETARIES. A. G. VeErnNoN Harcourt, Esq., M.A., D.C.L., LL.D., F.R.S., Pres.C.S., Cowley Grange, Oxford. Professor E. A. SCHAFER, F.R.S., University College, London, W.C. ASSISTANT GENERAL SECRETARY. G. GRIFFITH, Esq., M.A., College Road, Harrow, Middlesex. GENERAL TREASURER. Professor ARTHUR W. RtckeEr, M.A., D.Sc., F.R.S., Burlington House, London, W. LOCAL SECRETARIES FOR THE MEETING AT LIVERPOOL. Professor W. A. HERDMAN, F.R.S. | Isaac C. THompson, Esq., F.L.S. | W. E. Witnink, Esq. LOCAL TREASURER FOR THE MEETING AT LIVERPOOL. REGINALD BUSHELL, Esq. ORDINARY MEMBERS OF THE COUNCIL. AnpeErson, Dr. W. C. B., F.R.S. Poutron, Professor E, B., F.R.S. AYRTON, Professor W. E., F.R.S. RaAmMsAyY, Professor W., F.R.S. BakeER, Sir B., K.C.M.G., F.R.S. REYNOLDS, Professor J. Emmrson, M.D., Boys, Professor C. VERNON, F.R.S. F.R.S. EDGEWORTH, Professor F. Y., M.A. SHAw, W.N., Esq., F.R.S. EVANS, Sir J., K.C.B., F.R.S. Symons, G. J., Esq., F.R.S. FOXWELL, Professor H.S., M.A. TEALL, J. J. H., Be, F.R.S. Harcourt, Professor L. F, VERN ON, M.A. THISELTON-DykErR, W.T., area. . C.M.G., F.R.Sz HERDMAN, Professor W. A., F.R.S. THOMSON, Professor 3.M . F.R.S.E. HORSLEY, Professor Vic TOR, F.R.S. Unwin, Professor W.C., EF, RS. LODGE, Professor OLIVER J., F.R.S. VINES, Professor Sie; ERS. MARKHAM, CLEMENTS R., Esq., C.B., F.R.S. WARD, Professor MARSHALL, F.R.S. MELDOLA, Professor R., ERS. WHITAKER, W., Esq., F.R.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. Sir Jonn Lussock, Bart., M.P., D.C.L., LL.D., F.R. The Right Hon. Lord RayLrieu, M. -A., D. C. L. nite Ds; Sec. R.S., E.R, The Right Hon. Lord PLayFratr, K.C Be Ph. D., LL. D,» F.R.S. PRESIDENTS OF FORMER YEARS. Prof. Allman, M.D., F.R.S. Sir W. H. Flower, K.C.B., I’.R.S. Sir John Lubbock, Bart., F.R.S. | Sir Frederick Abel, Bart., F.R. S. Lord Rayleigh, D.C.L., Sec.R.S. Dr. Wm. Huggins, D.C. Te F.R | Lord Playfair, K.C.B., F.R.S. Sir Archibald Geikie, LL.D., nae | Sir Wm. Dawson, C.M.G., F.R.S. | Prof.J.S.Burdon Sanderson,F.R.S. Lord Kelvin, LL.D., Pres.R.s. Sir H. E. Roscoe, D.C.L., F.R.8, The Marquis of Salisbury, K.G., Prof. A. W. Williamson, F.R.S. Sir F. J. Bramwell, Bart., F.R.S. F.R.S. GENERAL OFFICERS OF FORMER YEARS. The Duke of Argyll, K.G., K.T. Lord Armstrong, C.B., LL.D. The Rt.Hon. Sir W.R.Grove,F.R.S. Sir Joseph D. Hooker, K.C.S.1. Sir G. G. Stokes, Bart., F.R.S, F. Galton, Esq., F.R.S G. Griffith, Esq., M.A. Prof. T. G. Bonney, D.Sc., F.R.S. Prof, Michael Foster, Sec.R. Ss. P. L. Sclater, Esq., Ph.D., F.R.S. | Prof. Williamson, Ph.D., F.R.S. Sir Douglas Galton, K.C.B. F.R.S AUDITORS. Dr. T. E. Thorpe, F.R.S. | Ludwig Mond, Esq., F.R.S. | Jeremiah Head, Esq., M.Inst.C.E. REPORT—1895. THE GENERAL TREASURER’S ACCOUNT, RECEIPTS, & 8s dad Balance broupht!forwardy......scsscssccccccocenvenesterteasterenen ee 1094 2 6 Tate Compositions) ys. was dessaris-css sre omeaess aes eines Heeiees yaataeiees 15 0 0 *Herdman, Professor W. A.—Zoology, Botany, and Geology Ghathenlrish Sea. \. << was ites Re ee ete ec ose oes ceee 50 0 0 *Sclater, Dr. P. L.—Zoology of the Sandwich Islands ......... 100 0 0 Sclater, Dr. P. L.—African Lake Fauna............ 0.0... .00000 00: 100 0 O Herdman, Professor W. A.—Oysters under normal and abnormal environment sy iescctea-ceahiassoies vibe ses oa eyoaia secon 40 0 0 Geography. *Ravenstein, Mr. E. G.—Climatology of Tropical Africa ...... 10 0 0 Mechanical Science. Kennedy, Professor A. B. W.—Calibration and Comparison of Measuring Instruments (251. renewed) .......-.... 042045 30 0 0 *Preece, Mr. W. H.—Small Screw Gauge ............... 0.00000 10 0 0 Anthropology. *Tylor, Professor E. B.—North-Western Tribes of Canada (761. 15s. renewed) i.e eae tate ces LOO OD *Munro, Dr. R.—Lake Village at Glastonbury (5/. renewed) 30 0 0 *Evans, Sir J.—Exploration of a Kitchen-midden at Hastings (Unexpended balance 21. 6s. 6d.) ..........0cssseeeeereeeee oe ~— *Brabrook, Mr. E. W.—Ethnographical Survey (20/. renewed) 40 0 0 *Galton, Sir Douglas—Mental and Physical Condition of Ghildrert’4..0:22.. 22... Woe eso. 2s, Pee LOO *Flower, Sir W. H.—Anthropometric Measurements in Schools (Unexpended balance, 20. 148.) .....-...-..cesereceeeeecreseenes — Physiology. *McKendrick, Professor J. G.—Physiological Applications of ake PHonosraph: «1:17.20 eegee cence mecegeens yak ehasr mene seeps 20° 0" 0 Corresponding Societies. *Meldola, Professor R.—Preparation of Report .................5 30 0 0 £1,160 0 0 * Reappointed. The Annual Meeting in 1896. The Meeting at Liverpool will commence on Wednesday, Sep- tember 16. The Annual Meeting in 1897. The Annual Meeting of the Association in 1897 will be held at Toronto, Canada. lV. xevil General Statement of Sums which have been paid on account of Grants for Scientific Purposes. 1834. £3. d Tide Discussions .......0c..+60 20 0 0 1835. : Tide Discussions ...........0+6+ 62 0 0 British Fossil Ichthyology ... 105 0 0 £167 O O 1836. Tide Discussions ..,..........+. 163 0 0 British Fossil Ichthyology ... 105 0 0 Thermometric Observations, AMMA raeialechine vclesivow are ocave ses 50 0 0 Experiments on Long-con- tintied Heat .......s.c0cscoees ilgeice (0) Rain-gauges .......ec..ece0e oc eG 0) Refraction Experiments ...... 1b 0) 0 Lunar Nutation.................. 60 0 0 PEBETINOMELCTS \......0c0cces0s000 15 6 0 £435 0 0 1837. Tide Discussions ...........0.08 284 1 0 Chemical Constants ............ 2413 6 Lunar Nutation...........ccc0008+ 70 0 O Observations on Waves ...... 100 12 0 Wides ati Bristol ..,.....ccse.cesss 150 0 O Meteorology and Subterra- nean Temperature............ 93 3 0 Vitrification Experiments 150 0 0 Heart Experiments ............ 8 4 6 Barometric Observations ...... 30 0 0 [SAEOTHELETS 5.,.05.ccceceorscecosess 1118 6 £922 12 6 1838. Tide Discussions ............... 29 0 0 British Fossil Fishes............ 100 0 0 Meteorological Observations and Anemometer (construc- OTM eseceser dat ses cece onccscs ss 100 0 0 Cast Iron (Strength of) ...... 60 0 0 Animal and Vegetable Sub- stances (Preservation of)... 19 1 10 Railway Constants ............ 41 12 10 ISCO! TICES *.,.......c0ccceeseees 50 0 O Growth of Plants ............... 75 0 0 MiG in Rivers ...........sseee0s 3.6 6 Education Committee ......... 50 0 O Heart Experiments ............ 5 3 0 Land and Sea Level............ 267 8 7 Steam-vessels...............cc0008 100 0 0 Meteorological Committee 31 9 5 £932 2 2 1895. 1839. eas es Fossil Ichthyology ............ 110 0 0 Meteorological Observations at: Plymouth, &c. .........00. 63 10 0 Mechanism of Waves ......... 144 2 0 Bristol! Tides’... ..cccecserovcease 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 ............... 11 0 6 Stars in R.A.S. Catalogue 166 16 0 Animal Secretions............. . 1010 6 Steam Engines in Cornwall... 50 0 O Atmospheric Air ...........e006 146 $1 0 Cast and Wrought Iron ...... 40 0 0 Heat on Organic Bodies ...... 3.0 0 Gases on Solar Spectrum...... 22 0 0 Hourly Meteorological Ob- servations, Inverness and IKGINETISSIO! aces ceersssevcecsdsees 49 7 8 Fossil Reptiles ......,..cececeeee 118 2 9 Mining Statistics ............... 50 0 0 £1595 11 0 SSS 1840. Baistol MMS ees neem «-oscne=% ss 100 0 0 Subterranean Temperature... 13 13 6 Heart Experiments ............ 18 19 0 Lungs Experiments ............ 813 0 Tide Discussions .............0+ 50 0 0 Land and Sea Level...... feeOr Lie E Stars (Histoire Céleste) ...... 242 10 0 Stars (Lacaille) ...............008 415 0 Stars (Catalogue) .............85 264 0 0 Atmospheric Air ..........0.608 15 15 0 Waterion Irom ssep oo, LOWMOYEO £1608 3 10 1864. Maintaining the Establish- ment at Kew Observatory.. 600 0 0O I@oa ROSSI ys recs aeseannseerrs 20, (0820) | Vertical Atmospheric Move- METIUS) cece sesso seasiaseenee maces 20 0 0 Dredging, Shetland ............ 75 0 0 Dredging, Northumberland... 25 0 0 | Balloon Committee ............ 200 0 0 Carbon under pressure ...... LOVOFO Standards of Electric Re- SISUAMLCES .teneoet ree er eibeas sce 100 0 O Analysis of Rocks ............ 10 0 0 Ty MOL at veaseeaeenacenewese soars LOUOAO Askham's Gites. sc tecancceseere 50 0 O Nitrite of ‘Amiyle 2. c..cn-cesee 10 0 0 Nomenclature Committee ... 5 0 9 RAI CAUSES ses ecseseeseseceaces 19 15 8 Cast-iron Investigation .....- 20 0 0 Tidal Observations in the 18 hyve 0) sya eer nncricoarrorrccaeen a7 50 0 O pectral Raystocessss-ravesseaasee 45 0 0 Luminous Meteors ............ 20° '0"°0 £1289 15 8 1865. Maintaining the Establish- ment at Kew Observatory.. 600 0 0 Balloon Committee ............ 100 0 O Tehygeligortobrypanme visscc ont: 2850350007 13 0 0 Haln=Cauees " orescces cena aescets 30 0 0 Tidal Observations in the La R bh en ele RR onoctnendeite donot Gao Hexylic Compounds ............ 20 0 0 Amyl Compounds ............... 20 0 0 Prigh WO 1OTa .. sexsnescaee seers 25 0 0 American Mollusca ............ 3 OO | Orcanic Acids! Vieeseseeees eee 20°00 Lingula Flags Excavation ... 10 0 0 HUry PLerusy. 2cssseseeeeenheenecass 50 0 0 Electrical Standards............ 100 0 0 Malta Caves Researches ...... 30 0 0 Oyster Breeding .............0. 25.00 Gibraltar Caves Researches... 150 0 0O Kent’s Hole Excavations...... 100 0 0 Moon’s Surface Observations 35 0 0 Marine Hanna feestsseeessces 25 0 0 Dredging Aberdeenshire ...... 25 0 0 Dredging Channel Islands ... 50 0 0 Zoological Nomenclature...... 5 0 0 Resistance of Floating Bodies in) Waiter ts...cctgusshesetrscss< 100 0 0 Bath Waters Analysis ......... 8 10 10 Luminous Meteors ....... svc £0) ORO £1591 7 10 GENERAL STATEMENT. 1866. Coit: Maintaining the Establish- ment at Kew Observatory.. 600 0 Lunar Committee............... 64 13 Balloon Committee ............ 50 0 Metrical Committee............ 50 0 PIGISM MAIN TAL)... ..scncoeeces 50 0 Kilkenny Coal Fields ......... 16 0 Alum Bay Fossil Leaf-bed ... 15 0 Luminous Meteors ............ 50 0 Lingula Flags Excavation ... 20 0 Chemical Constitution of IOAAUBEEOWS oe -s50esoqenniova acess 50 0 Amyl Compounds ............... 25 0 Electrical Standards............ 100 0 Malta CavesExploration ...... 30 0 Kent’s Hole Exploration ...... 200 0 Marine Fauna, &c., Devon and Cornwall ............-s-e00 25 0 Dredging Aberdeenshire Coast 25 0 Dredging Hebrides Coast ... 50 0 Dredging the Mersey ......... 5 0 Resistance of Floating Bodies PNVVILEL vecen crease sossonsccsece 50 0 Polycyanides of Organic Radi- ReOa genie ce cccos vase faeces oss Ss 29 0 AO MLOTULS....-...c00eseceo ens 10 0 BPISM AMNeIda .........:022-.606 15 0 Catalogue of Crania............ 50 0 Didine Birds of Mascarene EATS ence sish-h odelaasinee's)-qet'e 50 0 Typical Crania Researches ... 30 0 Palestine Exploration Fund... 100 0 £1750 13 1867. Maintaining the Establish- ment at Kew Observatory.. 600 0 Meteorological Instruments, DME GING, ceancscaeevtntecessccee 50 0 Lunar Committee ............... 120 0 Metrical Committee ............ 30 0 Kent’s Hole Explorations ... 100 0 Palestine Explorations......... 50 0 Insect Fauna, Palestine ...... 30 0 ripisheRaintall. . .ccdecesssb «ane 50 O Kilkenny Coal Fields ......... 25 0 Alum Bay Fossil Leaf-bed ... 25 0 Luminous Meteors ............. Oa) Bournemouth, &c., Leaf-beds 30 0 Dredging Shetland ............ 75 0 Steamship Reports Condensa- tion ...... oc cpa Serbencetamutt ozs 100 0 Electrical Standards............ 100 0 Ethyl and Methyl Series...... 25 0 Fossil Crustacea ..........0s.+ 25 0 Sound under Water ............ 24 4 North Greenland Fauna ....... 15 0 Do. Plant Beds 100 0 Tron and Steel Manufacture... 25 0 IBAbEOG LAWS ....20cccaseees eee OOseO #1739 4 coloooooocoososo ocoocooooeocoocoeo (=) SCSCloO Oo Cot 0O Coo ooO SoSocCooCCoKRSO ®& ee) 1868. £ Maintaining the Establish- ment at Kew Observatory.. 600 Lunar Committee ............... 120 Metrical Committee............ 50 Zoological Record............+0+ 100 Kent’s Hole Explorations ... 150 Steamship Performances ...... 100 British Rainfall....... “PCOCTEP EOE 50 Luminous Meteors............... 50 OrganicvAcids: | waestceg.s0cses< 60 Fossil Crustacea.........0-sseeees 25 Methyl Series: 20. scsssats4-encsie 25 Mercury and Bile ..............- 25 Organic Remains in Lime- SLONESHOCKS vacsnanmnedes ess 25 Scottish Harthquakes ......... 20 Fauna, Devon and Cornwall.. 30 British Fossil Corals ......... 50 Bagshot Leaf-beds .......-...: 50 Greenland Explorations ...... 100 HOSSUGH OVA. tas. cssceaneaee doses 2 Tidal Observations ............ 190 Underground Temperature.., 50 | Spectroscopic Investigations cili oa . colo co coscocoscoooo cooocooooeoesesooe co|'o coo ooooooooo oscoecsescoooeseso & of Animal Substances ...... 5 Secondary Reptiles, kc. ...... 30 | British Marine Invertebrate HAG cacttheacits ceca tecesseceaae 100 £1940 1869. Maintaining the Establish- ment at Kew Observatory.. 600 Lunar Committee........... Seana a Metrical Committee.............++ 25 Zoological Record .............+5 100 | Committee on Gases in Deep- Well! Waters: cnrsncaneeosastees 25 |) SBxLibisheRalmrallle co. ceccscussecs 50 Thermal Conductivity of Iron, GEC rerteilals siaseetate eee ate Merc 30 Kent’s Hole Explorations...... 150 Steamship Performances ...... 30 Chemical Constitution of CaStwlnONsces. «i. civ £ 3. d. Chemical Constitution and Physiological Action Rela- CONS rw ccsgapeasceeucpesedase vey 15 0 0 Mountain Limestone Fossils 25 0 0 Utilisation of Sewage ......... 10 0 0 Products of Digestion ......... 10 0 0 £1622 0 0 1870. Maintaining the Establish- ment at Kew Observatory 600 Metrical Committee............ 25 Zoological Record............... 100 Committee on Marine Fauna 20 Mars in Wishes ..............0.9 10 Chemical Nature of Cast Ngee tec ceecoce es tor eoeens 80 Luminous Meteors ............ 30 Heat in the Blood............... 15 British Ranta. .cccesccesve ote 100 Thermal Conductivity of Iii (ORO ER Ret See eo ace 20 British Fossil Corals............ 50 Kent’s Hole Explorations 150 Scottish Earthquakes ......... 4 Bagshot Leaf-beds ............ 15 MUCOUS LON terse eit cace ee cae 25 Tidal Observations .....-....., 100 Underground Temperature... 50 Kiltorcan Quarries Fossils ... 20 Mountain Limestone Fossils 25 Utilisation of Sewage ......... Organic Chemical Compounds Onny River Sediment Mechanical Equivalent of eceooooooo eosoocso ooooo — Son Soto) ole ooooooooocoooo oocco ooooo 1871. Maintaining the Establish- ment at Kew Observatory 600 Monthly Reports of Progress aniChemistryievesscstc. ooo oS (So oc coe .coo ¢) 2 rOoOCcooc coo co oc GFoOC0oo evil 1885. £ Synoptic Chart of Indian OCGA. ctonscennen cepen ore meee 50 Reduction of Tidal Observa- IONS ceases collsnoheal etme enone rik 10 Calculating Tables in Theory Of Numberss.sceassen-eeaneausne 100 Meteorological Observations lon Bene Nevisiscnscesesceiere ves 50 Meteoric Dust ..........densce-s 70 Vapour Pressures, &c., of Salt Solutions........... orion oaaponod 25 Physical Constants of Solu- PONS? .-. snow een setincteseaeeas ere 20 Volcanic Phenomena of Vesu- WIUS2 cease wcieatcasvaneescsaeetveces 25 Raygill Fissure ...............00. 15 Earthquake Phenomena of SIAPAM™ acswessnessscsevsesss sass 70 Fossil Phyllopoda of Palaeozoic ROCKStt ac ccoeratacsceveose tees 25 Fossil Plants of British Ter- tiary and Secondary Beds. 50 Geological Record ..............+ 50 Circulation of Underground INV AUCIS 3. oc nscvsstecressteroch ccs 10 Naples Zoological Station ... 100 Zoological Literature Record. 100 Migration of Birds ............ 30 Exploration of Mount Kilima- HEL] AO Meteieeais vs cessebaccadersy sere 25 Recent Poly z0a......sssce.ccsecsse 10 Granton Biological Station ... 100 Biological Stations on Coasts of United Kingdom ......... 150 Exploration of New Guinea... 200 Exploration of Mount Roraima 100 £1385 1886. Electrical Standards............ 40 SOAR ACTALION sss atw ase teste cs 9 Tidal Observations ............ 50 Magnetic Observations......... 10 Observations on Ben Nevis... 100 Physical and Chemical Bear- ings of Electrolysis ......... 20 Chemical Nomenclature ...... 5 Fossil Plants of British Ter- tiary and Secondary Beds... 2 Caves in North Wales ......... 25 Volcanic Phenomena of Vesu- MMOS neue ctoreteiatissccesseete 30 Geological Record............... 100 Paleozoic Phyllopoda ......... 15 Zoological Literature Record. 100 Granton Biological Station... 75 Naples Zoological Station...... 50 Researches in Food-Fishes and Invertebrata at St. Andrews CE = (=f) ooo oococo oo o (>) =e} o fo) oo o (>) oO i — i=) oooocoe oo oo ooococo NSIS COR OS'S SOS SS OSS GS OC 1S SO Romomoues i) ooococo°o oo oo oooafo REPORT—1895. £ Migration of Birds ............ 30 Secretion of Urine.............0+ 10 Exploration of New Guinea... 150 Regulation of Wages under sliding) Scales, sqse.cse/as 10 Prehistoric Race in Greek Tslands:....psensreroscoweereeeeeey 20 North-Western Tribes of Ca- MAGA. 65 do sevnnsilswchne chee eeeeeee 50 £995 1887. Solar Radiation .............00s.- 18 Hlectroly sis... sonsces-=sseessn ts 30 Ben Nevis Observatory......... 75 Standards of Light (1886 feartebaue)) ionsoaonntoece en ona 20 Standards of Light (1887 TAME) trensspesrcaoacatnsea cows 10 Harmonic Analysis of Tidal Observations ...............006 15 Magnetic Observations......... 26 Electrical Standards ............ 50 Silent Discharge of Electricity 20 Absorption Spectra ............ 40 Nature of Solution ............ 20 Influence of Silicon on Steel 30 Volcanic Phenomena of Vesu- IVALLIS (ciheas "0"..0 Fossil Phyllopoda ...........++++ 5 0 0 Shell-bearing Deposits at ROIAMASICES Verenccccsstctecsessss 20 0 0 Eurypterids of the Pentland ETE, Set iold- wcekcicss «, . Tt wor oe ee 17-NAR GG i / . ~ _ PRESIDENT’S ADDRESS. P : ‘ ’ 4 1 1 at — ae ry, ‘ B Z ADDRESS BY SIR DOUGLAS GALTON, K.C.B., D.C.L, F.BS., PRESIDENT. b My first duty is to convey to you, Mr. Mayor, and to the inhabitants of _ Ipswich, the thanks of the British Association for your hospitable invita- : tion to hold our sixty- -fifth meeting in your ancient town, and thus to recall _.the agreeable memories of the similar favour which your predecessors con- farce on the Association forty-four years ago. | In the next place I feel it my ahibge to say a few words on the great loss which science has recently sustained—the death of the Right f Hon. Thomas Henry Huxley. It is unnecessary for me to enlarge, _ in the presence of so many to whom his personality was known, upon his charm in social and domestic life; but upon the debt which the . Association owes to him for the assistance which he rendered in the _ promotion of science I cannot well be silent. Huxley was preeminently " qualified to assist in sweeping away the obstruction by dogmatic au- "thority, which in the early days of the Association fettered progress in certain branches of science. For, whilst he was an eminent leader in . biological research, his bcitelleatustl power, his original and intrepid mind, his vigorous and masculine English, made him a writer who explained the Bdcepest subject with transparent clearness. And as a speaker his lucid and forcible style was adorned with ample and effective illustration in the lecture-room ; and his energy and wealth of argument in a more public arena exeoly: helped to win the battle of evolution, and to secure for us the right to discuss questions of religion and science without fear and without favour. _ It may, I think, interest you to learn that Huxley first made the B2 ~ ‘ Be 4 REPORT—1895. acquaintance of Tyndall at the meeting of the Association held in this town in 1851. About forty-six years ago I first began to attend the meetings of the British Association ; and I was elected one of your general secretaries about twenty-five years ago. It is not unfitting, therefore, that I should recall to your minds the conditions under which science was pursued at the formation of the Asso- ciation, as well as the very remarkable position which the Association has occupied in relation to science in this country. Between the end of the sixteenth century and the early part of the present century several societies had been created to develop various branches of science. Some of these societies were established in London, and others in important provincial centres. In 1831, in the absence of railways, communication between different parts of the country was slow and difficult. Science was therefore local- ised ; and in addition to the universities in England, Scotland, and Ire- land, the towns of Birmingham, Manchester, Plymouth and York each maintained an important nucleus of scientific research. ORIGIN OF THE BritisH ASSOCIATION. Under these social conditions the British Association was founded in September 1831. The general idea of its formation was derived from a migratory society which had been previously formed in Germany ; but whilst the German society met for the special occasion on which it was summoned, and then dissolved, the basis of the British Association was continuity. The objects of the founders of the British Association were enunciated in their earliest rules to be : ‘To give a stronger impuise and a more systematic direction to scien- tific inquiry ; to promote the intercourse of those who cultivated science in different parts of the British Empire with one another, and with foreign philosophers ; to obtain a more general attention to the objects of science, and a removal of any disadvantages of a public kind which im- pede its progress.’ Thus the British Association for the Advancement of Science based its utility upon the opportunity it afforded for combination. The first meeting of the Association was held at York with 353 members. As an evidence of the want which the Association supplied, it may be mentioned that at the second meeting, which was held at Oxford, the number of members was 435. The third meeting, at Cambridge, numbered over 900 members, and at the meeting at Edinburgh in 1834 there were present 1,298 members. At its third meeting, which was held at Cambridge in 1833, the Association, through the influence it had already acquired, induced the ADDRESS. 5 Government to grant a sum of 500/. for the reduction of the astronomical observations of Baily. And at the same meeting the General Committee commenced to appropriate to scientific research the surplus from the sub- scriptions of its members. The committees on each branch of science were desired ‘to select definite and important objects of science, which they may think most fit to be advanced by an application of the funds of the society, either in compensation for labour, or in defraying the expense of apparatus, or otherwise, stating their reasons for their selection, and, when they may think proper, designating individuals to undertake the desired investigations.’ The several proposals were submitted to the Committee of Recommen- dations, whose approval was necessary before they could be passed by the General Committee. The regulations then laid down still guide the Association in the distribution of its grants. At that early meeting the Association was enabled to apply 6007. to these objects. I have always wondered at the foresight of the framers of the constitution of the British Association, the most remarkable feature of which is the lightness of the tie which holds it together. It is not bound by any complex central organisation. It consists of a federation of Sections, whose youth and energy are yearly renewed by a succession of presidents and vice-presidents, whilst in each Section some continuity _ of action is secured by the less movable secretaries. The governing body is the General Committee, the members of which are selected for their scientific work ; but their controlling power is tempered by the law that all changes of rules, or of constitution, should be submitted to, and receive the approval of, the Committee of Recommendations. This committee may be described as an ideal Second Chamber. It consists of the most experienced members of the Association. The administration of the Association in the interval between annual meetings is carried on by the Council, an executive body, whose duty it is to complete the work of the annual meeting (a) by the publication of its proceedings ; (b) by giving effect to resolutions passed by the General Committee ; (c) it also appoints the Local Committee and organises the personnel of each Section for the next meeting. I believe that one of the secrets of the long-continued success and vitality of the British Association lies in this purely democratic constitu- tion, combined with the compulsory careful consideration which must be given to suggested organic changes. The Association is now in the sixty-fifth year of its existence. In its origin it invited the philosophical societies dispersed throughout Great Britain to unite in a co-operative union. Within recent years it has endeavoured to consolidate that union. At the present time almost all important local scientific societies scattered throughout the country, some sixty-six in number, are in corre- spondence with the Association. Their delegates hold annual conferences at our meetings. The Association has thus extended the sphere of its action: 6 REPORT—1895. it places the members of the local societies engaged in scientific work in relation with each other, and brings them into co-operation with members of the Association and with others engaged in original investi- gations, and the papers which the individual societies publish annually are catalogued in our Report. Thus by degrees a national catalogue will be formed of the scientific work of these societies. The Association has, moreover, shown that its scope is coterminous with the British Empire by holding one of its annual meetings at Montreal, and we are likely soon to hold a meeting in Toronto. CONDITION OF CERTAIN SCIENCES AT THE FORMATION OF THE British ASSOCIATION. The Association, at its first meeting, began its work by initiating a series of reports upon the then condition of the several sciences. A rapid glance at some of these reports will not only show the enor- mous strides which have been made since 1831 in the investigation of facts to elucidate the laws of Nature, but it may afford a slight insight into the impediments offered to the progress of investigation by the mental condition of the community, which had been for so long satisfied to accept assumptions without undergoing the labour of testing their truth by ascertaining the real facts. This habit of mind may be illustrated by two instances selected from the early reports made to the Associa- tion. The first is afforded by the report made in 1832, by Mr. Lubbock, on ‘ Tides,’ This was a subject necessarily of importance to England as a dominant power at sea. But in England records of the tides had only recently been commenced at the dockyards of Woolwich, Sheerness, Portsmouth, and Plymouth, on the request of the Royal Society, and no information had been collected upon the tides on the coasts of Scotland and Ireland. The British Association may feel pride in the fact that within three years of its inception, viz. by 1834, it had induced the Corporation of Liverpool to establish two tide gauges, and the Government to undertake tidal observations at 500 stations on the coasts of Britain. Another cognate instance is exemplified by a paper read at the second meeting, in 1832, upon the State of Naval Architecture in Great Britain. The author contrasts the extreme perfection of the carpentry of the internal fittings of the vessels with the remarkable deficiency of mathematical, theory in the adjustment of the external form of vessels, and suggests the benefit of the application of refined analysis to the various practical problems which ought to interest shipbuilders—problems of capacity, of displacement, of stowage, of velocity, of pitching and rolling, of masting, of the effects of sails and of the resistance of fluids ; and, moreover, sug- gests that large-scale experiments should be made by Government, to afford the necessary data for calculation. Indeed, when we consider how completely the whole habit of mind of the populations of the Western world has been changed, since the beginning ADDRESS. 7 of the century, from willing acceptance of authority as a rule of life to a — f universal spirit of inquiry and experimental investigation, is it not pro- bable that this rapid change has arisen from society having been stirred to its foundations by the causes and consequences of the French Revolu- tion ? One of the earliest practical results of this awakening in France was the conviction that the basis of scientific research lay in the accuracy of the standards by which observations could be compared ; and the follow- ing principles were laid down as a basis for their measurements of length, weight, and capacity: viz. (1) that the unit of linear measure applied to matter in its three forms of extension, viz., length, breadth, and thickness, should be the standard of measures of length, surface, and solidity ; (2) that the cubic contents of the linear measure in decimetres of pure water at the temperature of its greatest density should furnish at once the standard weight and the measure of capacity.'_ The metric sys- tem did not come into full operation in France till 1840 ; and it is now adopted by all countries on the continent of Europe except Russia. The standards of length which were accessible in Great Britain at the formation of the Association were the Parliamentary standard yard lodged in the Houses of Parliament (which was destroyed in 1834 in the fire which burned the Houses of Parliament); the Royal Astronomical Society’s standard ; and the 10-foot bar of the Ordnance Survey. The first two were assumed to afford exact measurements at a given temperature. The Ordnance bar was formed of two bars on the principle of a compensating pendulum, and afforded measurements independent of temperature. Standard bars were also disseminated throughout the country, in possession of the corporations of various towns, The British Association early recognised the importance of uniformity in the record of scientific facts, as well as the necessity for an easy method of comparing standards and for verifying differences between instruments and apparatus required by various observers pursuing similar lines of investigation. At its meeting at Edinburgh in 1834 it caused a com- parison to be made between the standard bar at Aberdeen, constructed by Troughton, and the standard of the Royal Astronomical Society, and reported that the scale ‘was exceedingly well finished ; it was about shoth of an inch shorter than the 5-feet of the Royal Astronomical Society’s scale, but it was evident that a great number of minute, yet important, circumstances have hitherto been neglected in the formation of such scales, without an attention to which they cannot be expected to accord with that degree of accuracy which the present state of science demands.’ Subsequently, at the meeting at Newcastle in 1863, the Association appointed a committee to report on the best means of providing for a uniformity of weights and measures with reference to the 1 The litre is the volume of a kilogramme of pure water at its maximum density, and is slightly less than the litre was intended to be, viz., one cubic decimetre. The weight of a cubic decimetre of pure water is 1000013 kilogrammes. 8 REPORT—1895. interests of science. This committee recommended the metric decimal system—a recommendation which has been endorsed by a committee of the House of Commons in the last session of Parliament. British instrument-makers had been long conspicuous for accuracy of workmanship. Indeed, in the eighteenth century practical astronomy had been mainly in the hands of British observers ; for although the mathe- maticians of France and other countries on the continent of Europe were occupying the foremost place in mathematical investigation, means of astronomical observation had been furnished almost exclusively by English artisans. The sectors, quadrants, and circles of Ramsden, Bird, and Cary were inimitable by Continental workmen. But the accuracy of the mathematical-instrument maker had not penetrated into the engineer’s workshop. And the foundation of the British Association was coincident with a rapid development of mechanical . appliances. At that time a good workman had done well if the shaft he was turn- ing, or the cylinder he was boring, ‘was right to the =,nd of an inch,’ This was, in fact, a degree of accuracy as fine as the eye could usually distinguish. Few mechanics had any distinct knowledge of the method to be pur- sued for obtaining accuracy ; nor, indeed, had practical men sufficiently appreciated either the immense importance or the comparative facility of its acquisition. The accuracy of workmanship essential to this development of me- chanical progress required very precise measurements of length, to which reference could be easily made. No such standards were then available for the workshops. But a little before 1830 a young workman named Joseph Whitworth realised that the basis of accuracy in machinery was the making of a true plane. The idea occurred to him that this could only be secured by making three independent plane surfaces ; if each of these would lift the other, they must be planes, and they must be true. The true plane rendered possible a degree of accuracy beyond the wildest dreams of his contemporaries in the construction of the lathe and the planing machine, which are used in the manufacture of all tools. His next step was to introduce an exact system of measurement, generally applicable in the workshop. Whitworth felt that the eye was altogether inadequate to secure this, and appealed to the sense of touch for affording a means of comparison. If two plugs be made to fit into a round hole, they may differ in size by a quantity imperceptible to the eye, or to any ordinary process of measure- ment, but in fitting them into the hole the difference between the larger and the smaller is felt immediately by the greater ease with which the smaller one fits. In this way a child can tell which is the larger of two cylinders differing in thickness by no more than ;,),,th of an inch. Standard gauges, consisting of hollow cylinders with plugs to fit, but ADDRESS. 9 differing in diameter by the y,);5th or the +,},;oth of an inch, were given to his workmen, with the result that a degree of accuracy inconceivable to the ordinary mind became the rule of the shop. To render the construction of accurate gauges possible Whitworth devised his measuring machine, in which the movement was effected by a screw ; by this means the distance between two true planes might be measured to the one-millionth of an inch. These advances in precision of measurement have enabled the degree of accuracy which was formerly limited to the mathematical-instrument maker to become the common property of every machine shop. And not only is the latest form of steam-engine, in the accuracy of its workman- ship, little behind the chronometer of the early part of the century, but the accuracy in the construction of experimental apparatus which has thus been introduced has rendered possible recent advances in many lines of research. Lord Kelvin said in his Presidential Address at Edinburgh, ‘ Nearly all the grandest discoveries of science have been but the rewards of accu- rate measurement and patient, long-continued labour in the sifting of numerical results.’ The discovery of argon, for which Lord Rayleigh and Professor Ramsay have been awarded the Hodgkin prize by the Smithsonian Institution, affords a remarkable illustration of the truth of this remark. Indeed, the provision of accurate standards not only of length, but of weight, capacity, temperature, force, and energy, are amongst the founda- tions of scientific investigation. In 1842 the British Association obtained the opportunity of extending its usefulness in this direction. In that year the Government gave up the Royal Observatory at Kew, and offered it to the Royal Society, who declined it. But the British Association accepted the charge. Their first object was to continue Sabine’s valuable observations upon the vibrations of a pendulum in various gases, and to promote pendulum observations in various parts of the world. They subsequently extended it into an observatory for com- paring and verifying the various instruments which recent discoveries in physical science had suggested for continuous meteorological and magnetic observations, for observations and experiments on atmospheric electricity, and for the study of solar physics. This new departure afforded a means for ascertaining the advantages and disadvantages of the several varieties of scientific instruments ; as well as for standardising and testing instruments, not only for instrument- makers, but especially for observers by whom simultaneous observations were then being carried on in different parts of the world; and also for training observers proceeding abroad on scientific expeditions. Its special object was to promote original research, and expenditure was not to be incurred on apparatus merely intended to exhibit the necessary consequences of known laws. The rapid strides in electrical science had attracted attention to the 10 REPORT—1895. measurement of electrical resistances, and in 1859 the British Association appointed a special committee to devise a standard. The standard of resistance proposed by that committee became the generally accepted standard, until the requirements of that advancing science led to the adoption of an international standard. In 1866 the Meteorological Department of the Board of Trade entered into close relations with the Kew Observatory. And in 1871 Mr. Gassiot transferred 10,0007. upon trust to the Royal Society for the maintenance of the Kew Observatory, for the purpose of assisting in carrying on magnetical, meteorological, and other physical observations. The British Association thereupon, after having maintained this Observatory for nearly thirty years, at a total expenditure of about 12,000/., handed the Observatory over to the Royal Society. The ‘Transactions’ of the British Association are a catalogue of its efforts in every branch of science, both to promote experimental research and to facilitate the application of the results to the practical uses of - life. But probably the marvellous development in science which has accompanied the life-history of the Association will be best appreciated by a brief allusion to the condition of some of the branches of science in 1831 as compared with their present state. GEOLOGICAL AND GEOGRAPHICAL SCIENCE. Geology. At the foundation of the Association geology was assuming a promi- nent position in science. The main features of English geology had been illustrated as far back as 1821, and, among the founders of the British Association, Murchison and Phillips, Buckland, Sedgwick and Cony- beare, Lyell and De la Beche, were occupied in investigating the data necessary for perfecting a geological chronology by the detailed observa- tions of the various British deposits, and by their co-relation with the Continental strata. They were thus preparing the way for those large generalisations which have raised geology to the rank of an inductive science. : In 1831 the Ordnance maps published for the southern counties had enabled the Government to recognise the importance of a geological survey by the appointment of Mr. De la Beche to aflix geological colours to the maps of Devonshire and portions of Somerset, Dorset and Cornwall ; and in 1835 Lyell, Buckland and Sedgwick induced the Government to establish the Geological Survey Department, not only for promoting geological science, but on account of its practical bearing on agriculture, mining, the making of roads, railways and canals, and on other branches of national industry. es ADDRESS. 11 Geography. The Ordnance Survey appears to have had its origin in a proposal of the French Government to make a joint-measurement of an are of the meridian. This proposal fell through at the outbreak of the Revolution ; but the measurement of the base for that object was taken as a founda- tion for a national survey. In 1831, however, the Ordnance Survey had only published the l-inch map for the southern portion of England, and the great triangulation of the kingdom was still incomplete. In 1834 the British Association urged upon the Government that the advancement of various branches of science was greatly retarded by the want of an accurate map of the whole of the British Isles ; and that, consequently, the engineer and the meteorologist, the agriculturist and the geologist, were each fettered in their scientific investigations by the absence of those accurate data which now lie ready to his hand for the measurement of length, of surface, and of altitude. Yet the first decade of the British Association was coincident with a considerable development of geographical research. The Association was persistent in pressing on the Government the scientific importance of sending the expedition of Ross to the Antarctic and of Franklin to the Arctic regions. We may trust that we are approaching a solution of the geography of the North Pole ; but the Antarctic regions still present a field for the researches of the meteorologist, the geologist, the biologist, and the magnetic observer, which the recent voyage of M. Borchgrevink leads us to hope may not long remain unexplored. In the same decade the question of an alternative route to India by means of a communication between the Mediterranean and the Persian Gulf was also receiving attention, and in 1835 the Government employed Colonel Chesney to make a survey of the Euphrates valley in order to ascertain whether that river would enable a practicable route to be formed from Iskanderoon, or Tripoli, opposite Cyprus, to the Persian Gulf. His valuable surveys are not, however, on a sufficiently extensive scale to enable an opinion to be formed as to whether a navigable waterway through Asia Minor is physically practicable, or whether the cost of establishing it might not be prohibitive. The advances of Russia in Central Asia have made it imperative to provide an easy, rapid, and alternative line of communication with our Eastern possessions, so as not to be dependent upon the Suez Canal in time of war. If a navigation cannot be established, a railway between the Mediterranean and the Persian Gulf has been shown by the recent investigations of Messrs. Hawkshaw and Hayter, following on those of others, to be perfectly practicable and easy of accomplishment ; such an undertaking would not only be of strategical value, but it is believed it would be commercially remunerative. Speke and Grant brought before the Association, at its meeting at Newcastle in 1863, their solution of the mystery of the Nile basin, which 12 REPORT—1895. had puzzled geographers from the days of Herodotus ; and the efforts of Livingstone and Stanley and others have opened out to us the interior of Africa. I cannot refrain here from expressing the deep regret which geologists and geographers, and indeed all who are interested in the pro- gress of discovery, feel at the recent death of Joseph Thomson. His extensive, accurate, and trustworthy observations added much to our knowledge of Africa, and by his premature death we have lost one of its most competent explorers. CHEMICAL, ASTRONOMICAL AND PHysICAL SCIENCE. Chemistry. The report made to the Association on the state of the chemical sciences in 1832, says that the efforts of investigators were then being directed to determining with accuracy the true nature of the substances which compose the various products of the organic and inorganic king- - doms, and the exact ratios by weight which the different constituents of these substances bear to each other. But since that day the science of chemistry has far extended its boundaries. The barrier has vanished which was supposed to separate the products of living organisms from the substances of which minerals consist, or which could be formed in the laboratory. The number of dis- tinct carbon compounds obtainable from organisms has greatly increased ; but it is small when compared with the number of such compounds which have been artificially formed. The methods of analysis have been per- fected. The physical, and especially the optical, properties of the various forms of matter have been closely studied, and many fruitful generalisa- tions have been made. The form in which these generalisations would now be stated may probably change, some, perhaps, by the overthrow or disuse of an ingenious guess at Nature’s workings, but more by that change which is the ordinary growth of science—namely, inclusion in some simpler and more general view. In these advances the chemist has called the spectroscope to his aid. Indeed, the existence of the British Association has been practically coter- minous with the comparatively newly developed science of spectrum analysis, for though Newton,! Wollaston, Fraunhofer, and Fox Talbot had worked at the subject long ago, it was not till Kirchhoff and Bunsen set a seal on the prior labours of Stokes, Angstrém, and Balfour Stewart that the spectra of terrestrial elements have been mapped out and grouped ; that by its help new elements have been discovered, and that the idea has been suggested that the various orders of spectra of the same ‘ Joannes Marcus Marci, of Kroniand in Bohemia, was the only predecessor of Newton who had any knowledge of the formation of a spectrum bya prism. He not only observed that the coloured rays diverged as they left the prism, but that a coloured ray did not change in colour after transmission through a prism. His book, Thaumantias, liber de arcu calesti deque colerum apparentium natura, Prag, 1648, was, however, not known to Newton, and had no influence upon future discoveries. — >. a ADDRESS. ko element are due to the existence of the element in different molecular forms—allotropic or otherwise—at different temperatures. But great as have been the advances of terrestrial chemistry through its assistance, the most stupendous advance which we owe to the spectro- scope lies in the celestial direction. Astronomy. At the third meeting of the Association, at Cambridge, in 1833, Dr. Whewell said that astronomy is not only the queen of science, but the only perfect science, which was ‘in so elevated a state of flourishing maturity that all that remained was to determine with the extreme of accuracy the consequences of its rules by the profoundest combinations of mathematics ; the magnitude of its data by the minutest scrupulousness of observation.’ But in the previous year, Airy, in his report to the Association on the progress of Astronomy, had pointed out that the observations of the planet Uranus could not be united in one elliptic orbit ; a remark which turned the attention of Adams to the discovery of Neptune. In his report on the recent progress of Optics, Brewster in 1832 suggested that with the assistance of adequate instruments ‘it would be possible to study the action of the elements of material bodies upon rays of artificial light, and thereby to discover the analogies between their affinities and those which produce the fixed lines in the spectra of the stars ; and thus to study the effects of the combustions which light up the suns of other systems.’ This idea has now been realised. All the stars which shine brightly enough to impress an image of the spectrum upon a photographie plate have been classified on a chemical basis. The close connection between stars and nebule has been demonstrated ; and while the modern science of thermodynamics has shown that the hypothesis of Kant and Laplace on stellar formation, so far as it assumed a fiery cloud for the beginning, is no longer tenable, but that in all probability it gives the true explana tion of stellar evolution, if for the fiery cloud we substitute cold meteoric particles, as suggested by Waterston! and by Lord Kelvin? at the Liverpool meeting of the British Association in 1854. We now know that the spectra of many of the terrestrial elements in the chromosphere of the sun differ from those familiar to us in our labora- tories. We begin to glean the fact that; the chromospheric spectra are similar to those indicated by the absorption going on in the hottest stars, and Lockyer has not hesitated to affirm that these facts would indicate that in those localities we are in the presence of the actions of temperatures sufti- ' In Note Lona paper on ‘The Physics of Media,’ communicated to the Royal Society, December 11, 1845, read March 5, 1846, and published, in 1892, in the Transactions, with an introduction by Lord Rayleigh. * Brit. Assoc. Report, 1854, Pt. I1., pp. 59-63; Mathematical and Physical Papers, vol, ii., art. lxix., p. 40. ' 14 REPORT—1895. ciently high to break up our chemical elements into finer forms. Other students of these phenomena may not agree in this view, and _pos- sibiy the discrepancies may be due to default in our terrestrial chemistry. Still, I would recall to you that Dr. Carpenter, in his Presi- dential Address at Brighton in 1872, almost censured the speculations of Frankland and Lockyer in 1868 for attributing a certain bright line in the spectrum of solar prominences (which was not identifiable with that of any known terrestrial source of light) to a hypothetical new substance which they proposed to call ‘helium,’ because ‘it had not received that verification which, in the case of Crookes’ search for thallium, was afforded by the actual discovery of the new metal.’ Ramsay has now shown that this gas is present in dense minerals on earth ; but we have now also learned from Lockyer that it and other associated gases are not only found with hydrogen in the solar chromosphere, but that these gases, with hydrogen, form a large percentage of the atmospheric constituents of some of the hottest stars in the heavens. The spectroscope has also made us acquainted with the motions and even the velocities of those distant orbs which make up the sidereal uni- verse. It has enabled us to determine that many stars, single to the eye, are really double, and many of the conditions of these strange systems have been revealed. The rate at which matter is moving in solar cyclones and winds is now familiar to us. And I may also add that quite recently this wonderful instrument has enabled Professor Keeler to verify Clerk- Maxwell’s theory that the rings of Saturn consist of a marvellous com- pany of separate moons—as it were, a cohort of courtiers revolving round their queen—with velocities proportioned to their distances from the planet. Physics If we turn to the sciences which are included under physics, the pro- gress has been equally marked. In optical science, in 1831 the theory of emission as contrasted with the undulatory theory of light was still under discussion. Young, who was the first to explain the phenomena due to the inter- ference of the rays of light as a consequence of the theory of waves, and Fresnel, who showed the intensity of light for any relative position of the interference-waves, both had only recently passed away. The investigations into the laws which regulate the conduction and radiation of heat, together with the doctrine of latent and of specific heat, and the relations of vapour to air, had all tended to the conception of a material heat, or caloric, communicated by an actual flow and emission. It was not till 1834 that improved thermometrical appliances had enabled Forbes and Melloni to establish the polarisation of heat, and thus to lay the foundation of an undulatory theory for heat similar to that which was in progress of acceptation for light. Whewell’s report, in 1832, on magnetism and electricity shows that ADDRESS. 15 these branches of science were looked upon as cognate, and that the theory of two opposite electric fluids was generally accepted. In magnetism, the investigations of Hansteen, Gauss, and Weber in Europe, and the observations made under the Imperial Academy of Russia over the vast extent of that empire, had established the existence of mag- netic poles, and had shown that magnetic disturbances were simultaneous at all the stations of observation. At their third meeting the Association urged the Government to establish magnetic and meteorological observatories in Great Britain and her colonies and dependencies in different parts of the earth, furnished with proper instruments, constructed on uniform principles, and with provisions for continued observations at those places. In 1839 the British Association had a large share in inducing the Government to initiate the valuable series of experiments for determining the intensity, the declination, the dip, and the periodical variations of the magnetic needle which were carried on for several years, at numerous selected stations over the surface of the globe, under the directions of Sabine and Lefroy. In England systematic and regular observations are still made at Greenwich, Kew, and Stonyhurst. For some years past similar observa- tions by both absolute and self-recording instruments have also been made at Falmouth—close to the home of Robert Were Fox, whose name is in- separably connected with the early history of terrestrial magnetism in this country—but under such great financial difficulties that the continu- ance of the work is seriously jeopardised. It is to be hoped that means may be forthcoming to carry it on. Cornishmen, indeed, could found no more fitting memorial of their distinguished countryman, John Couch Adams, than by suitably endowing the magnetic observatory in which he took so lively an interest. Far more extended observation will be needed before we can hope to have an established theory as to the magnetism of the earth. We are without magnetic observations over a large part of the Southern Hemisphere. And Professor Riicker’s recent investigations tell us that the earth seems as it were alive with magnetic forces, be they due to elec- tric currents or to variations in the state of magnetised matter ; that the disturbances affect not only the diurnal movement of the magnet, but that even the small part of the secular change which has been observed, and which has taken centuries to accomplish, is interfered with by some slower agency. And, what is more important, he tells us that none of these observations stand as yet upon a firm basis, because standard instru- ments have not been in accord ; and much labour, beyond the power of individual effort, has hitherto been required to ascertain whether the relations between them are constant or variable. In electricity, in 1831, just at the time when the British Association was founded, Faraday’s splendid researches in electricity and magnetism at the Royal Institution had begun with his discovery of magneto- 16 REPORT—1895. electric induction, his investigation of the laws of electro-chemical decom- position, and of the mode of electrolytical action. But, the practical application of our electrical knowledge was then limited to the use of lightning-conductors for buildings and _ ships. Indeed, it may be said that the applications of electricity to the use of man have grown up side by side with the British Association. One of the first practical applications of Faraday’s discoveries was in the deposition of metals and electro-plating, which has developed into a large branch of national industry ; and the dissociating effect of the electric arc, for the reduction of ores, and in other processes, is daily obtaining a wider extension. But probably the application of electricity which is tending to pro- duce the greatest change in our mental, and even material condition, is the electric telegraph and its sister, the telephone. By their agency not only do we learn, almost at the time of their occurrence, the events which are happening in distant paris of the world, but they are establishing a community of thought and feeling between all the nations of the world which is influencing their attitude towards each other, and, we may hope, may tend to weld them mcre and more into one family. The electric telegraph was introduced experimentally in Germany in 1833, two years after the formation of the Association. It was made a commercial success by Cooke and Wheatstone in England, whose first attempts at telegraphy were made on the line from Euston to Camden Town in 1837, and on the line from Paddington to West Drayton in 1838. The submarine telegraph to America, conceived in ]856, became a practical reality in 1861 through the commercial energy of Cyrus Field and Pender, aided by the mechanical skill of Latimer Clark, Gooch, and others, and the scientific genius of Lord Kelvin. The knowledge of electricity gained by means of its application to the telegraph largely assisted the extension of its utility in other directions. The electric light gives, in its incandescent form, a very perfect hygienic light. Where rivers are at hand the electrical transmission of power will drive railway trains and factories economically, and might enable each artisan to convert his room into a workshop, and thus assist in restoring to the labouring man some of the individuality which the factory has tended to destroy. In 1843 Joule described his experiments for determining the mechani- cal equivalent of heat. But it was not until the meeting at Oxford, in 1847, that he fully developed the law of the conservation of energy, which, in conjunction with Newton’s law of the conservation of momentum, and Dalton’s law of the conservation of chemical elements, constitutes a complete mechanical foundation for physical science. Who, at the foundation of the Association, would have believed some far-seeing philosopher if he had foretold that the spectroscope would analyse the constituents of the sun and measure the motions of the stars ; that we should liquefy air and utilise temperatures approaching to the ADDRESS. 17/ absolute zero for experimental research ; that, like the magician in the ‘Arabian Nights,’ we should annihilate distance by means of the electric telegraph and the telephone ; that we should illuminate our largest build- ings instantaneously, with the clearness of day, by means of the electric current ; that by the electric transmission of power we should be able to utilise the Falls of Niagara to work factories at distant places ; that we should extract metals from the crust of the earth by the same electrical agency to which, in some cases, their deposition has been attributed % These discoveries and their applications have been brought to their present condition by the researches of a long line of scientific explorers, such as Dalton, Joule, Maxwell, Helmholtz, Herz, Kelvin, and Rayleigh, aided by vast strides made in mechanical skill. But what will our successors be discussing sixty years hence? How little do we yet know of the vibrations which communicate light and heat! Far as we have ad- vanced in the application of electricity to the uses of life, we know but little even yet of its real nature. We are only on the threshold of the knowledge of molecular action, or of the constitution of the all-pervading zther. Newton, at the end of the seventeenth century, in his preface to the ‘Principia,’ says: ‘I have deduced the motions of the planets by mathematical reasoning from forces ; and I would that we could derive the other phenomena of Nature from mechanical principles by the same mode of reasoning. For many things move me, so that I somewhat sus- pect that all such may depend on certain forces by which the particles of bodies, through causes not yet known, are either urged towards each other according to regular figures, or are repelled and recede from each other ; and these forces being unknown, philosophers have hitherto made their attempts on Nature in vain.’ In 1848 Faraday remarked : ‘ How rapidly the knowledge of molecular forces grows upon us, and how strikingly every investigation tends to develop more and more their importance ! ‘A few years ago magnetism was an occult force, affecting only a few bodies ; now it is found to influence all bodies, and to possess the most intimate relation with electricity, heat, chemical action, light, crystallisa- tion ; and through it the forces concerned in cohesion. We may feel encouraged to continuous labours, hoping to bring it into a bond of union with gravity itself.’ But it is only within the last few years that we have begun to realise that electricity is closely connected with the vibrations which cause heat and light, and which seem to pervade all space—vibrations which may be termed the voice of the Creator calling to each atom and to each cell of protoplasm to fall into its ordained position, each, as it were, a musical note in the harmonious symphony which we call the universe. 1895. ‘ 18 REPORT—1895. Meteorology. At the first meeting, in 1831, Professor James D. Forbes was requested to draw up a report on the State of Meteorological Science, on the ground that this science is more in want than any other of that systematic direc- tion which it is one great object of the Association to give. Professor Forbes made his first report in 1832, and a subsequent report in 1840. The systematic records now kept in various parts of the world of barometric pressure, of solar heat, of the temperature and physi- cal conditions of the atmosphere at various altitudes, of the heat of the ground at various depths, of the rainfall, of the prevalence of winds, and the gradual elucidation not only of the laws which regulate the movements of cyclones and storms, but of the influences which are exercised by the sun and by electricity and magnetism, not only upon atmospheric condi- tions, but upon health and vitality, are gradually approximating meteor- ology to the position of an exact science. England took the lead in rainfall observations. Mr. G. J. Symons organised the British Rainfall System in 1860 with 178 observers, a system which until 1876 received the help of the British Association. Now Mr. Symons himself conducts it, assisted by more than 3,000 observers, and these volunteers not only make the observations, but defray the ex- pense of their reduction and publication. In foreign countries this work is done by Government officers at the public cost. At the present time a very large number of rain gauges are in daily use throughout the world. The British Islands have more than 3,000, and India and the United States have nearly as many; France and Germany are not far behind ; Australia probably has more—indeed, one colony alone, New South Wales, has more than 1,100. The storm warnings now issued under the excellent systematic organi- sation of the Meteorological Committee may be said to have had their origin in the terrible storm which broke over the Black Sea during the Crimean War, on November 27, 1855. Leverrier traced the progress of that storm, and seeing how its path could have been reported in advance by the electric telegraph, he proposed to establish observing stations which should report to the coasts the probability of the occurrence of a storm. Leverrier communicated with Airy, and the Government authorised Ad- miral FitzRoy to make tentative arrangements in this country. The idea was also adopted on the Continent, and now there are few civilised coun- tries north or south of the equator without a system of storm warning.' ' It has often been supposed that Leverrier was also the first to issue a daily weather map, but that was not the case, for in the Great Exhibition of 1851 the Electric Telegraph Company sold daily weather maps, copies of which are still in existence, and the data for them were, it is believed, obtained by Mr. James Glaisher, F.R.S., at that time Superintendent of the Meteorological Department at Greenwich. ae ADDRESS. 19 BIoLoGicaL ScIENcE. Botany. The earliest Reports of the Association which bear on the biological sciences were those relating to botany. In 1831 the controversy was yet unsettled between the advantages of the Linnean, or Artificial system, as contrasted with the Natural system of classification. Histology, morphology, and physiological botany, even if born, were in their early infancy. Our records show that von Mohl noted cell division in 1835, the presence of chlorophyll corpuscles in 1837; and he first described protoplasm in 1846. Vast as have been the advances of physiological botany since that time, much of its fundamental principles remain to be worked out, and I trust that the establishment, for the first time, of a permanent Section for botany at the present meeting will lead the Association to take a more prominent part than it has hitherto done in the further development of this branch of biological science. Animal Physiology. In 1831 Cuvier, who during the previous generation had, by the colla- tion of facts followed by careful inductive reasoning, established the plan on which each animal is constructed, was approaching the termina- tion of his long and useful life. He died in 1832; but in 1831 Richard Owen was just commencing his anatomical investigations and his brilliant contributions to paleontology. The impulse which their labours gave to biological science was reflected in numerous reports and communications, by Owen and others, throughout the early decades of the British Association, until Darwin propounded a theory of evolution which commanded the general assent of the scientific world. For this theory was not absolutely new. But just as Cuvier had shown that each bone in the fabric of an animal affords a clue to the shape and structure of the animal, so Darwin brought harmony into scattered facts, and led us to perceive that the moulding hand of the Creator may have evolved the complicated structures of the organic world from one or more primeval cells. Richard Owen did not accept Darwin’s theory of evolution, and a large section of the public contested it. I well remember the storm it produced—a storm of praise by my geological colleagues, who accepted the result of investigated facts ; a storm of indignation such as that which would have burned Galileo at the stake from those who were not yet - prepared to question the old authorities ; but they diminish daily. We are, however, as yet only on the threshold of the doctrine of evolution. Does not each fresh investigation, even into the embryonic stage of the simpler forms of life, suggest fresh problems ? v2 20 REPORT—1895. Anthropology. The impulse given by Darwin has been fruitful in leading others to consider whether the same principle of evolution may not have governed the moral as well as the material progress of the human race. Mr. Kidd tells us that nature as interpreted by the struggle for life contains no sanction for the moral progress of the individual, and points out that if each of us were allowed by the conditions of life to follow his own inclina- tion, the average of each generation would distinctly deteriorate from that of the preceding one ; but because the law of life is ceaseless and inevit- able struggle and competition, ceaseless and inevitable selection and re- jection, the result is necessarily ceaseless and inevitable progress. Evolu- tion, as Sir William Flower said, is the message which biology has sent to help us on with some of the problems of human life, and Francis Galton urges that man, the foremost outcome of the awful mystery of evolution, should realise that he has the power of shaping the course of future humanity by using his intelligence to discover and expedite the changes which are necessary to adapt circumstances to man, and man to cireumstances, In considering the evolution of the human race, the science of pre- ventive medicine may afford us some indication of the direction in which to seek for social improvement. One of the early steps towards establish- ing that science upon a secure basis was taken in 1835 by the British Association, who urged upon the Government the necessity of establishing registers of mortality showing the causes of death ‘on one uniform plan in all parts of the King’s dominions, as the only means by which general laws touching the influence of causes of disease and death could be satisfactorily deduced.’ The general registration of births and deaths was commenced in 1838. But a mere record of death and its proximate cause is insuffi- cient. Preventive medicine requires a knowledge of the details of the previous conditions of life and of occupation. Moreover, death is not our only or most dangerous enemy, and the main object of preventive nedicine is to ward off disease. Disease of body lowers our useful energy. Disease of body or of mind may stamp its curse on succeeding generations. The anthropometric laboratory affords to the student of anthropo- logy a means of analysing the causes of weakness, not only in bodily, but also in mental life. Mental actions are indicated by movements and their results. Such signs are capable of record, and modern physiology has shown that bodily movements correspond to action in nerve-centres, as surely as the motions of the telegraph-indicator express the movements of the operator’s hands in the distant office. Thus there is a relation between a defective status in brain power and defects in the proportioning of the body. Defects in physiognomical details, too finely graded to be measured with instruments, may be appreciated with accuracy by the senses of the observer ; and the records ADDRESS. 21 show that these defects are, in a large degree, associated with a brain status lower than the average in mental power. A report presented by one of your committees gives the results of observations made on 100,000 school-children examined individually in order to determine their mental and physical condition for the purpose of classification. This shows that about 16 per 1,000 of the elementary school population appear to be so far defective in their bodily or brain condition as to need special training to enable them to undertake the duties of life, and to keep them from pauperism or crime. Many of our feeble-minded children, and much disease and vice, are the outcome of inherited proclivities. Francis Galton has shown us that types of criminals which have been bred true to their kind are one of the saddest disfigurements of modern civilisation ; and he says that few deserve better of their country than those who determine to lead celibate lives through a reasonable conviction that their issue would probably be less fitted than the generality to play their part as citizens. These considerations point to the importance of preventing those suffering from transmissible disease, or the criminal, or the lunatic, from adding fresh sufferers to the teeming misery in our large towns. And in any case, knowing as we do the influence of environment on the develop- ment of individuals, they point to the necessity of removing those who are born with feeble minds, or under conditions of moral danger, from sur- rounding deteriorating influences. These are problems which materially affect the progress of the human race, and we may feel sure that, as we gradually approach their solution, we shall more certainly realise that the theory of evolution, which the genius of Darwin impressed on this century, is but the first step on a biological ladder which may possibly eventually lead us to understand how in the drama of creation man has been evolved as the highest work of the Creator. Bacteriology. The sciences of medicine and surgery were largely represented in the earlier meetings of the Association, before the creation of the British Medical Association afforded a field for their more intimate discussion. The close connection between the different branches of science is causing a revival in our proceedings of discussions on some of the highest medical problems, especially those relating to the spread of infectious and epidemic disease. It is interesting to contrast the opinion prevalent at the foundation of the Association with the present position of the question. A report to the Association in 1834, by Professor Henry, on contagion, says :— ‘The notion that contagious emanations are at all connected with the diffusion of animalcule through the atmosphere is at variance with all that is known of the diffusion af volatile contagion.’ Whilst it had long been known that filthy Connie in air, earth 22 REPORT—1895. and water fostered fever, cholera, and many other forms of disease, and that the disease ceased to spread on the removal of these con- ditions, yet the reason for their propagation or diminution remained under a veil. Leeuwenhoek in 1680 described the yeast-cells, but Schwann in 1837 first showed clearly that fermentation was due to the activity of the yeast- cells ; and, although vague ideas of fermentation had been current during the past century, he laid the foundation of our exact knowledge of the nature of the action of ferments, both organised and unorganised. It was not until 1860, after the prize of the Academy of Sciences had been awarded to Pasteur for his essay against the theory of spon- taneous generation, that his investigations into the action of ferments? enabled him to show that the effects of the yeast-cell are indissolubly bound up with the activities of the celi as a living organism, and that certain diseases, at least, are due to the action of ferments in the living being. In 1865 he showed that the disease of silkworms, which was then undermining the silk industry in France, could be successfully combated. His further researches into anthrax, fowl cholera, swine fever, rabies, and other diseases proved the theory that those diseases are con- nected in some way with the introduction of a microbe into the body of an animal ; that the virulence of the poison can be diminished by culti- vating the microbes in an appropriate manner ; and that when the virulence has been thus diminished their inoculation will afford a protection against the disease. Meanwhile it had often been observed in hospital practice that a patient with a simple-fractured limb was easily cured, whilst a patient with a compound fracture often died from the wound. Lister was thence led, in 1865, to adopt his antiseptic treatment, by which the wound is protected from hostile microbes. These investigations, followed by the discovery of the existence of a multitude of micro-organisms and the recognition of some of them— such as the bacillus of tubercle and the comma bacillus of cholera—as essential factors of disease ; and by the elaboration by Koch and others of methods by which the several organisms might be isolated, cultivated, and their histories studied, have gradually built up the science of bac- teriology. Amongst later developments are the discovery of various so-called antitoxins, such as those of diphtheria and tetanus, and the utilisation of these for the cure of disease. Lister’s treatinent formed a landmark in the science of surgery, and enabled our surgeons to perform operations never before dreamed of ; whilst later discoveries are tending to place the practice of medicine on a firm scientific basis. And the science of bacteriology is leading us to recur to stringent rules for the } In speaking of ferments one must bear in mind that there are two classes of ferments: one, living beings, such as yeast—‘ organised’ ferments, as they are sometimes called—the other the products of living beings themselves, such as pepsin, &c.—‘ unorganised’ ferments. Pasteur worked with the former, very little with the latter ADDRESS. 23 isolation of infectious disease, and to the disinfection (by superheated steam) of materials which have been in contact with the sufferer. These microbes, whether friendly or hostile, are all capable of multi- plying at an enormous rate under favourable conditions. They are found in the air, in water, in the soil ; but, fortunately, the presence of one species appears to be detrimental to other species, and sunshine, or even light from the sky, is prejudicial to most of them. Our bodies, when in health, appear to be furnished with special means of resisting attacks, and, so far as regards their influence in causing disease, the success of the attack of a pathogenic organism upon an individual depends, as a rule, in part at least, upon the power of resistance of the individual. But notwithstanding our knowledge of the danger arising from a state of low health in individuals, and of the universal prevalence of these micro-organisms, how careless we are in guarding the health conditions of everyday life! We have ascertained that pathogenic organisms pervade the air. Why, therefore, do we allow our meat, our fish, our vegetables, our easily contaminated milk, to be exposed to their inroads, often in the foulest localities? We have ascertained that they pervade the water we drink, yet we allow foul water from our dwellings, our pigsties, our farmyards, to pass into ditches without previous clarification, whence it flows into our streams and pollutes our rivers. We know the conditions of occupation which foster ill-health. Why, whilst we remove outside sources of impure air, do we permit the occupation of foul and unhealthy dwellings ? The study of bacteriology has shown us that although some of these organisms may be the accompaniments of disease, yet we owe it to the operation of others that the refuse caused by the cessation of animal and vegetable life is reconverted into food for fresh generations of plants and animals. These considerations have formed a point of meeting where the biologist, the chemist, the physicist, and the statistician unite with the sanitary engineer in the application of the science of preventive medicine. o 5 ENGINEERING. Sewage Purification. The early reports to the Association show that the laws of hydro- statics, hydrodynamics, and hydraulics necessary to the supply and removal of water through pipes and conduits had long been investigated by the mathematician. But the modern sanitary engineer has been driven by the needs of an increasing population to call in the chemist and the biologist to help him to provide pure water and pure air. The purification and the utilisation of sewage occupied the attention of the British Association as early as 1864, and between 1869 and 1876 a committee of the Association made a series of valuable reports on the subject. The direct application of sewage to land, though effective as a 24 REPORT—1895. means of purification, entailed difficulties in thickly settled districts, owing to the extent of land required. The chemical treatment of sewage produced an effluent harmless only after having been passed over land, or if turned into a large and rapid stream, or into a tidal estuary; and it left behind a large amount of sludge to be dealt with. Hence it was long contended that the simplest plan in favourable localities was to turn the sewage into the sea, and that the consequent loss to the land of the manurial value in the sewage would be recouped by the increase in fish-life. It was not till the chemist called to his aid the biologist, and came to the help of the engineer, that a scientific system of sewage purification was evolved. Dr. Frankland many years ago suggested the intermittent filtration of sewage ; and Mr. Bailey Denton and Mr. Baldwin Latham were the first engineers to adopt it. But the valuable experiments made in recent years by the State Board of Health in Massachusetts have more clearly explained to us how by this system we may utilise micro-organisms to con- vert organic impurity in sewage into food fitted for higher forms of life. To effect this we require, in the first place, a filter about five feet thick of sand and gravel, or, indeed, of any material which affords numerous surfaces or open pores. Secondly, that after a volume of sewage has passed through the filter, an interval of time be allowed, in which the air necessary to support the life of the micro-organisms is enabled to enter the pores of the filter. Thus this system is dependent upon oxygen and time. Under such conditions the organisms necessary for purification are sure to establish themselves in the filter before it has been long in use. Temperature is a secondary consideration. Imperfect purification can invariably be traced either to a lack of oxygen in the pores of the filter, or to the sewage passing through so quickly that there is not sufficient time for the necessary processes to take place. And the power of any material to purify either sewage or water depends almost entirely upon its ability to hold a sufficient propor- tion of either sewage or water in contact with a proper amount of air. Smoke Abatement. Whilst the sanitary engineer has done much to improve the surface conditions of our towns, to furnish clean water, and to remove our sewage, he has as yet done little to purify town air. Fog is caused by the floating particles of matter in the air becoming weighted with aqueous vapour ; some particles, such as salts of ammonia or chloride of sodium, have a greater affinity for moisture than others. You will suffer from fog so long as you keep refuse stored in your towns to furnish ammonia, or so long as you allow your street surfaces to supply dust, of which much consists of powdered horse manure, or so long as you send the products of hin ADDRESS. 25 combustion into the atmosphere. Therefore, when you have adopted mechanical traction for your vehicles in towns you may largely reduce one cause of fog. And if you diminish your black smoke, you will diminish black fogs. In manufactories you may prevent smoke either by care in firing, by using smokeless coal, or by washing the soot out of the products of consumption in its passage along the flue leading to the main chimney- shaft. The black smoke from your kitchen may be avoided by the use of coke or of gas. But so long as we retain the hygienic arrangement of the open fire in our living-rooms I despair of finding a fireplace, however well constructed, which will not be used in such a manner as to cause smoke, unless, indeed, the chimneys were reversed and the fumes drawn into some central shaft, where they might be washed before being passed into the atmosphere. Electricity as a warming and cooking agent would be convenient, cleanly, and economical when generated by water power, or possibly wind power, but it is at present too dear when it has to be generated by means of coal. I can conceive, however, that our descendants may learn so to utilise electricity that they in some future century may be enabled by its means to avoid the smoke in their towns. Mechanical Engineering. In other branches of civil and mechanical engineering, the reports in 1831 and 1832 on the state of this science show that the theoretical and practical knowledge of the strength of timber had obtained considerable development. But in 1830, before the introduction of railways, cast iron had been sparingly used in arched bridges for spans of from 160 to 200 feet, and wrought iron had only been applied to large-span iron bridges on the suspension principle, the most notable instance of which was the Menai Suspension Bridge, by Telford. Indeed, whilst the strength of timber had been patiently investigated by engineers, the best form for the use of iron girders and struts was only beginning to attract attention, and the earlier volumes of our Proceedings contained numerous records of the researches of Eaton Hodgkinson, Barlow, Rennie, and others. It was not until twenty years later that Robert Stephenson and William Fairbairn erected the tubular bridge at Menai, followed by the more scientific bridge erected by Brunel at Saltash. These have now been entirely eclipsed by the skill with which the estuary of the Forth has been bridged with a span of 1,700 feet by Sir John Fowler and Sir Benjamin Baker. The development of the iron industry is due to the association of the chemist with the engineer. The introduction of the hot blast by Neilson, in 1829, in the manufacture of cast iron had effected a large saving of fuel. But the chemical conditions which affect the strength and other qualities of iron, ard its combinations with carbon, silicon, phosphorus, and other substances, had at that time scarcely been investigated. 26 REPORT—1895. In 1856 Bessemer brought before the British Association at Cheltenham his brilliant discovery for making steel direct from the blast furnace, by which he dispensed with the laborious process of first removing the carbon from pig-iron by puddling, and then adding by cementation the required proportion of carbon to make steel. This discovery, followed by Siemens’s regenerative furnace, by Whitworth’s compressed steel, and by the use of alloys and by other improvements too numerous to mention here, have revolutionised the conditions under which metals are applied to engineering purposes. Indeed, few questions are of greater interest, or possess more industrial importance, than those connected with metallic alloys. This is especially true of those alloys which contain the rarer metals; and the extraordinary effects of small quantities of chromium, nickel, tungsten and titanium on certain varieties of steel have exerted profound influence on the manu- facture of projectiles and on the construction of our armoured ships. Of late years, investigations on the properties and structure of alloys have been numerous, and among the more noteworthy researches may be men- tioned those of Dewar and Fleming on the distinctive behaviour, as regards the thermo-electric powers and electrical resistance, of metals and alloys at the very low temperatures which may be obtained by the use of liquid air. Professor Roberts-Austen, on the other hand, has carefully studied the behaviour of alloys at very high temperatures, and by employing his delicate pyrometer has obtained photographic curves which afford addi- tional evidence as to the existence of allotropic modifications of metals, and which have materially strengthened the view that alloys are closely analogous to saline solutions. In this connection it may be stated that the very accurate work of Heycock and Neville on the lowering of the solidifying points of molten metals, which is caused by the presence of other metals, affords a valuable contribution to our knowledge. Professor Roberts-Austen has, moreover, shown that the effect of any one constituent of an alloy upon the properties of the principal metal has a direct relation to the atomic volumes, and that it is consequently possible to foretell, in a great measure, the effect of any given combination. A new branch of investigation, which deals with the micro-structure of metals and alloys, is rapidly assuming much importance. It was instituted by Sorby in a communication which he made to the British Association in 1864, and its development is due to many patient workers, among whom M. Osmond occupies a prominent place. Metallurgical science has brought aluminium into use by cheapening the process of its extraction ; and if by means of the wasted forces in our rivers, or possibly of the wind, the extraction be still further cheapened by the aid of electricity, we may not only utilise the metal or its alloys in increasing the spans of our bridges, and in affording strength and lightness in the construction of our ships, but we may hope to obtain a material which may render practicable the dreams of Icarus and of Maxim, and for purposes of rapid transit enable us to navigate the air. _ ona ere ADDRESS. 27 Long before 1831 the steam-engine had been largely used on rivers and lakes, and for short sea passages, although the first Atlantic steam-service was not established till 1838. As early as 1820 the steam-engine had been applied by Gurney, Han- cock, and others to road traction. The absurd impediments placed in their way by road trustees, which, indeed, are still enforced, checked any progress. But the question of mechanical traction on ordinary roads was practically shelved in 1830, at the time of the formation of the British Association, when the locomotive engine was combined with a tubular boiler and an iron road on the Liverpool and Manchester Railway. Great, however, as was the advance made by the locomotive engine of Robert Stephenson, these earlier engines were only toys compared with the compound engines of to-day which are used for railways, for ships, or for the manufacture of electricity. Indeed, it may be said that the study of the laws of heat, which have led to the introduction of various forms of motive power, are gradually revolutionising all our habits of life. The improvements in the production of iron, combined with the de- veloped steam-engine, have completely altered the conditions of our com- mercial intercourse on land ; whilst the changes caused by the effects of these improvements in shipbuilding, and on the ocean carrying trade, have been, if anything, still more marked. At the foundation of the Association all ocean ships were built by hand, of wood, propelled by sails and maneuvred by manual labour ; the material limited their length, which did not often exceed 100 feet, and the number of English ships of over 500 tons burden was comparatively small. In the modern ships steam power takes the place of manual labour. It rolls the plates of which the ship is constructed, bends them to the required shape, cuts, drills and rivets them in their place. It weighs the anchor ; it propels the ship in spite of winds or currents ; it steers, venti- lates, and lights the ship when on the ocean. It takes the cargo on board and discharges it on arrival. The use of iron favours the construction of ships of a large size, of forms which afford small resistance to the water, and with compartments which make the ships practically unsinkable in heavy seas, or by collision. Their size, the economy with which they are propelled, and the certainty of their arrival, cheapen the cost of transport. The steam-engine, by compressing air, gives us control over the tem- perature of cool chambers. In these not only fresh meat, but the delicate produce of the Antipodes, is brought across the ocean to our doors without deterioration. Whilst railways have done much to alter the social conditions of each individual nation, the application of iron and steam to our ships is revolu- tionising the international commercial conditions of the world ; and it is gradually changing the course of our agriculture, as well as of our do- mestic life. 28 REPORT—1895. But great as have been the developments of science in promoting the commerce of the world, science is asserting its supremacy even to a greater extent in every department of war. And perhaps this application of science affords at a glance, better than almost any other, a convenient illustration of the assistance which the chemical, physical, and electrical sciences are affording to the engineer. The reception of warlike stores is not now left to the uncertain judgment of ‘ practical men,’ but is confided to officers who have received a special training in chemical analysis, and in the application of physical and electrical science to the tests by which the qualities of explosives, of guns, and of projectiles can be ascertained. For instance, take explosives. Till quite recently black and brown powders alone were used, the former as old as civilisation, the latter but a small modern improvement adapted to the increased size of guns. But now the whole family of nitro-explosives are rapidly superseding the old powder. These are the direct outcome of chemical knowledge ; they are not mere chance inventions, for every improvement is based on chemical theories, and not on random experiment. The construction of guns is no longer a haphazard operation. In spite of the enormous forces to be controlled and the sudden violence of their action, the researches of the mathematician have enabled the just propor- tions to be determined with accuracy ; the labours of the physicist have revealed the internal conditions of the materials employed, and the best means of their favourable employment. Take, for example, Longridge’s coiled-wire system, in which each successive layer of which the gun is formed receives the exact proportion of tension which enables all the layers to act in unison. The chemist bas rendered it clear that even the smallest quantities of certain ingredients are of supreme importance in affecting the tenacity and trustworthiness of the materials. The treatment of steel to adapt it to the vast range of duties it has to perform is thus the outcome of patient research. And the use of the metals—manganese, chromium, nickel, molybdenum—as alloys with iron has resulted in the production of steels possessing varied and extra- ofdinary properties. The steel required to resist the conjugate stresses developed, lightning fashion, in a gun necessitates qualities that would not be suitable in the projectile which that gun hurls with a velocity of some 2,500 feet per second against the armoured side of a ship. The armour, again, has to combine extreme superficial hardness with great toughness, and during the last few years these qualities are sought to be attained by the application of the cementation process for adding carbon to one face of the plate, and hardening that face alone by rapid refrigeration. The introduction of quick-firing guns from ‘303 (i.c. about one-third) of an inch to 6-inch calibre has rendered necessary the production of metal cartridge-cases of complex forms drawn cold out of solid blocks or plate of the material ; this again has taxed the ingenuity of the mechanic in the device of machinery, and of the metallurgist in producing a metal possessed ee ADDRESS. 29 of the necessary ductility and toughness. The cases have to stand a pressure at the moment of firing of as much as twenty-five tons to the square inch—a pressure which exceeds the ordinary elastic limits of the steel of which the gun itself is composed. There is nothing more wonderful in practical mechanics than the closing of the breech openings of guns, for not only must they be gas- tight at these tremendous pressures, but the mechanism must be such that one man by a single continuous movement shall be able to open or close the breech of the largest gun in some ten or fifteen seconds. The perfect knowledge of the recoil of guns has enabled the reaction of the discharge to be utilised in compressing air or springs by which guns can be raised from concealed positions in order to deliver their fire, and then made to disappear again for loading ; or the same force has been used to run up the guns automatically immediately after firing, or, as in the case of the Maxim gun, to deliver in the same way a continuous stream of bullets at the rate of ten in one second. In the manufacture of shot and shell cast iron has been almost super- seded by cast and wrought steel, though the hardened Palliser projectiles still hold their place. The forged-steel projectiles are produced by methods very similar to those used in the manufacture of metal cartridge-cases, though the process is carried on at a red heat and by machines much more powerful. In every department concerned in the production of warlike stores electricity is playing a more and more important part. It has enabled the passage of a shot to be followed from its seat in the gun to its destination. In the gun, by means of electrical contacts arranged in the bore, a time- curve of the passage of the shot can be determined. From this the mathematician constructs the velocity-curve, and from this, again, the pressures producing the velocity are estimated, and used to check the same indications obtained by other means. The velocity of the shot after it has left the gun is easily ascertained by the Boulangé apparatus. Electricity and photography have been laid under contribution for obtaining records of the flight of projectiles and the effects of explosions at the moment of their occurrence. Many of you will recollect Mr. Vernon Boys’ marvellous photographs showing the progress of the shot driving before it waves of air in its course. Electricity and photography also record the properties of metals and their alloys as determined by curves of cooling. The readiness with which electrical energy can be converted into heat or light has been taken advantage of for the firing of guns, which in their turn can, by the same agency, be laid on the object by means of range- finders placed at a distance and in advantageous and safe positions ; while the electric light is utilised to illumine the sights at night, as well as to search out the objects of attack. 30 REPORT—1895. The compact nature of the glow-lamp, the brightness of the light, the circumstance that the light is not due to combustion, and therefore inde- pendent of air, facilitates the examination of the bore of guns, the insides of shells, and other similar uses—just as it is used by a doctor to examine the throat of a patient. INFLUENCE OF INTERCOMMUNICATION AFFORDED BY BrivrisH ASSOCIATION ON ScieNcE ProGRress. The advances in engineering which have produced the steam-engine, the railway, the telegraph, as well as our engines of war, may be said to be the result of commercial enterprise rendered possible only by the advances which have taken place in the several branches of science since 1831. Having regard to the intimate relations which the several sciences bear to each other, it is abundantly clear that much of this pro- gress could not have taken place in the past, nor could further progress take place in the future, without intercommunication between the students of different branches of science. The founders of the British Association based its claims to utility upon the power it afforded for this intercommunication. Mr. Vernon Harcourt (the uncle of your present General Secretary), in the address he delivered in 1832, said : ‘How feeble is man for any purpose when he stands alone—how strong when united with other men ! ‘It may be true that the greatest philosophical works have been achieved in privacy, but it is no less true that these works would never have been accomplished had the authors not mingled with men of corre- sponding pursuits, and from the commerce of ideas often gathered germs of apparently insulated discoveries, and without such material aid would seldom have carried their investigations to a valuable conclusion,’ I claim for the British Association that it has fulfilled the objects of its founders, that it has had a large share in promoting intercommunication and combination. Our meetings have been successful because they have maintained the true principles of scientific investigation. We have been able to secure the continued presence and concurrence of the master-spirits of science. They have been willing to sacrifice their leisure, and to promote the welfare of the Association, because the meetings have afforded them the means of advancing the sciences to which they are attached. The Association has, moreover, justified the views of its founders in promoting intercourse between the pursuers of science, both at home and abroad, in a manner which is afforded by no other agency. The weekly and sessional reunions of the Royal Society, and the annual sowrées of other scientific societies, promote this intercourse to some extent, but the British Association presents to the young student during its week of meetings easy and continuous social opportunities for ADDRESS. 31 making the acquaintance of leaders in science, and thereby obtaining their directing influence. It thus encourages, in the first place, opportunities of combination, but, what is equally important, it gives at the same time material assist- ance to the investigators whom it thus brings together. The reports on the state of science at the present time, as they appear in the last volume of our Proceedings, occupy the same important position, as records of science progress, as that occupied by those Reports in our earlier years. We exhibit no symptom of decay. ScrencE IN GERMANY FOSTERED BY THE STATE AND MUNICIPALITIES. Our neighbours and rivals rely largely upon the guidance of the State for the promotion of both science teaching and of research. In Germany the foundations of technical and industrial training are laid in the Real- schulen, and supplemented by the Higher Technical Schools. In Berlin that splendid institution, the Royal Technical High School, casts into the shade the facilities for education in the various Polytechnics which we are now establishing in London. Moreover, it assists the practical work- man by a branch department, which is available to the public for testing building materials, metals, paper, oil, and other matters. The standards of all weights and measures used in trade can be purchased from or tested by the Government Department for Weights and Measures. For developing pure scientific research and for promoting new applica- tions of science to industrial purposes the German Government, at the _ instance of von Helmholtz, and aided by the munificence of Werner von Siemens, created the Physikalische Technische Reichsanstalt at Charlottenburg. This establishment consists of two divisions. The first is charged with pure research, and is at the present time engaged in various thermal, optical, and electrical and other physical investigations. The second branch is employed in operations of delicate standardising to assist the wants of research students—for instance, dilatation, electrical resistances, electric and other forms of light, pressure gauges, recording instruments, thermometers, pyrometers, tuning forks, glass, oil-testing apparatus, viscosity of glycerine, &c. Dr. Kohlrausch succeeded Helmholtz as president, and takes charge of the first division. Professor Hagen, the director under him, has charge of the second division. A professor is in charge of each of the several sub-departments. Under these are various subordinate posts, held by younger men, selected for previous valuable work, and usually for a limited time. The general supervision is under a Council consisting of a president, who is a Privy Councillor, and twenty-four members, including the president and director of the Reichsanstalt ; of the other members, about ten are professors or heads of physical and astronomical observatories 82 REPORT—1895. connected with the principal universities in Germany. Three are selected from leading firms in Germany representing mechanical, optical, and electric science, and the remainder are principal scientific officials con- nected with the Departments of War and Marine, the Royal Observatory at Potsdam, and the Royal Commission for Weights and Measures. This Council meets in the winter, for such time as may be necessary, for examining the research work done in the first division during the previous year, and for laying down the scheme for research for the ensuing year ; as well as for suggesting any requisite improvements in the second division, As a consequence of the position which science occupies in connection with the State in Continental countries, the services of those who have distinguished themselves either in the advancement or in the application of science are recognised by the award of honours; and thus the feeling for science is encouraged throughout the nation. ASSISTANCE TO SciENTIFIC RESEARCH IN GREAT BRITAIN. Great Britain maintained for a long time a leading position among the nations of the world by virtue of the excellence and accuracy of its workmanship, the result of individual energy ; but the progress of mechanical science has made accuracy of workmanship the common property of all nations of the world. Our records show that hitherto, in its efforts to maintain its position by the application of science and the prosecution of research, England has made marvellous advances by means of voluntary effort, illustrated by the splendid munificence of such men as Gassiot, Joseph Whitworth, James Mason, and Ludwig Mond ; and, whilst the increasing field of scientific research compels us occasionally to seek for Government assistance, it would be unfortunate if by any change voluntary effort were fettered by State control. The following are the principal voluntary agencies which help forward scientific research in this country :—The Donation Fund of the Royal Society, derived from its surplusincome. The British Association has contri- buted 60,000/. to aid research since its formation. The Royal Institution, founded in the last century, by Count Rumford, for the promotion of research, has assisted the investigations of Davy, of Young, of Faraday, of Frankland, of Tyndall], of Dewar, and of Rayleigh. The City Com- panies assist scientific research and foster scientific education both by direct contributions and through the City and Guilds Institute. The Commis- sioners of the Exhibition of 1851 devote 6,000/. annually to science research scholarships, to enable students who have passed through a college curriculum and have given evidence of capacity for original research to continue the prosecution of science, with a view to its advance or to its application to the industries of the country. Several scientific societies, as, for instance, the Geographical Society and the Mechanical Engineers, have promoted direct research, each in their own branch of science, out of their surplus income ; and every scientific society largely assists research by the publication, not only of its own proceedings, but ADDRESS. 33 often of the work going on abroad in the brinch of science which it represents. The growing abundance of matter year by year increases the burden thus thrown on their finances, and the Treasury has recently granted to the Royal Society 1,000/. a year, to be spent in aid of the publication of scientific papers not necessarily limited to those of that Society. The Royal Society has long felt the importance to scientific research of a catalogue of all papers and publications relating to pure and applied science, arranged systematically both as to authors’ names and as to sub- ject treated, and the Society has been engaged for some time upon a catalogue of that nature. But the daily increasing magnitude of these publications, coupled with the necessity of issuing the catalogue with adequate promptitude, and at appropriate intervals, renders it a task which could only be performed under International co-operation. The officers of the Royal Society have therefore appealed to the Govern- ment to urge Foreign Governments to send delegates to a Conference to be held next July to discuss the desirability and the scope of such a cata- logue, and the possibility of preparing it. The universities and colleges distributed over the country, besides their function of teaching, are large promoters of research, and their voluntary exertions are aided in some cases by contributions from Parliament in alleviation of their expenses. Certain executive departments of the Government carry on research for their own purposes, which in that respect may be classed as voluntary. The Admiralty maintains the Greenwich Observatory, the Hydrographical Department, and various experimental services ; and the War Office maintains its numerous scientific departments. The Treasury maintains a valuable chemical laboratory for Inland Revenue, Customs, and agri- cultural purposes. The Science and Art Department maintains the Royal College of Science, for the education of teachers and students from ele- mentary schools. It allows the scientific apparatus in the national museum to be used for research purposes by the professors. The Solar Physics Committee, which has carried on numerous researches in solar physics, was appointed by and is responsible to this Department. The Department also administers the Sir Joseph Whitworth engineering re- search scholarships. Other scientific departments of the Government are aids to research, as, for instance, the Ordnance and the Geological Surveys, the Royal Mint, the Natural History Museum, Kew Gardens, and other lesser establishments in Scotland and Ireland ; to which may be added, to some extent, the Standards Department of the Board of Trade, as well as municipal museums, which are gradually spreading over the country. For direct assistance to voluntary effort the Treasury contritutes 4,000/. a year to the Royal Society for the promotion of research, which is administered under a board whose members represent all branches of Science. The Treasury, moreover, contributes to marine biological ob- servatories, and in recent years has defrayed the cost of various expedi- 1895. D 34 REPORT—1895. tions for biological and astronomical research, which in the case of the ‘Challenger’ expedition involved very large sums of money. In addition to these direct aids to science, Parliament, under the Local Taxation Act, handed over to the County Councils a sum, which amounted in the year 1893 to 615,000/., to be expended on technical educa- tion. In many country districts, so far as the advancement of real scien- tific technical progress in the nation is concerned, much of this money has been wasted for want of knowledge. And whilst it cannot be said that the Government or Parliament have been indifferent to the promotion of scientific education and research, it is a source of regret that the Govern- ment did not devote some small portion of this magnificent gift to afford- ing an object-lesson to County Councils in the application of science to technical instruction, which would have suggested the principles which would most usefully guide them in the expenditure of this public money. Government assistance to science has been based mainly on the principle of helping voluntary effort. The Kew Observatory was initiated as a scientific observatory by the British Association. It is now supported by the Gassiot trust fund, and managed by the Kew Observatory Com- mittee of the Royal Society. Observations on magnetism, on meteorology, and the record of sun-spots, as well as experiments upon new instruments for assisting meteorological, thermometrical, and photographic purposes, are being carried on there. The Committee has also arranged for the verification of scientific measuring instruments, the rating of chrono- meters, the testing of lenses and of other scientific apparatus. This institution carries on to a limited extent some small portion of the class of work done in Germany by that magnificent institution, the Reichsanstalt at Charlottenburg, but its development is fettered by want of funds. British students of science are compelled to resort to Berlin and Paris when they require to compare their more delicate instruments and ap- paratus with recognised standards. There could scarcely bea more advan- tageous addition to the assistance which Government now gives to science than for it to allot a substantial annual sum to the extension of the Kew Observatory, in order to develop it on the model of the Reichsanstalt. It might advantageously retain its connection with the Royal Society, under a Committee of Management representative of the various branches of science concerned, and of all parts of Great Britain. ConcLusIoNn. The various agencies for scientific education have produced numerous students admirably qualified to pursue research ; and at the same time almost every field of industry presents openings for improvement through the development of scientific methods. For instance, agricultural opera- tions alone offer openings for research to the biologist, the chemist, the physicist, the geologist, the engineer, which have hitherto been largely a ADDRESS. 30 overlooked. If students do not easily find employment, it is chiefly at- tributable to a want of appreciation for science in the nation at large. This want of appreciation appears to arise from the fact that those who nearly half a century ago directed the movement of national education were trained in early life in the universities, in which the value of scientific methods was not at that time fully recognised. Hence our elementary, and even our secondary and great public schools, neglected for a long time to encourage the spirit of investigation which develops originality. This defect is diminishing daily. There is, however, a more intangible cause which may have had influence on the want of appreciation of science by the nation. The Government, which largely profits by science, aids it with money, but it has done very little to develop the national appreciation for science by recognising that its leaders are worthy of honours conferred by the State. Science is not fashionable, and science students—upon whose efforts our progress as a nation so largely depends—have not received the same measure of recog- nition which the State awards to services rendered by its own officials, by politicians, and by the Army and by the Navy, whose success in future wars will largely depend on the effective applications of science. The Reports of the British Association afford a complete chronicle of the gradual growth of scientific knowledge since 1831. They show that the Association has fulfilled the objects of its founders in promoting and disseminating a knowledge of science throughout the nation. The growing connection between the sciences places our annual meeting in the position of an arena where representatives of the different sciences have the opportunity of criticising new discoveries and testing the value of fresh proposals, and the Presidential and Sectional Addresses operate as an annual stock-taking of progress in the several branches of science represented in the Sections. Every year the field of usefulness of the Association is widening. For, whether with the geologist we seek to write the history of the crust of the earth, or with the biologist to trace out the evolution of its inhabitants, or whether with the astronomer, the chemist, and the physicist we endeavour to unravel the constitution of the sun and the planets or the genesis of the nebule and stars which make up the universe, on every side we find ourselves surrounded by mysteries which await solution. We are only at the beginning of work. I have, therefore, full confidence that the future records of the British Association will chronicle a still greater progress than that already achieved, and that the British nation will maintain its leading position amongst the nations of the world, if it will energetically continue its voluntary efforts to promote research, supplemented by that additional help from the Government which ought never to be withheld when a clear case of scientific utility has been established. 0 ie aft Y om TYEE pers 7y. iis a net 5p i F} 2 ui Ae Nie lee a Bal te mya, ett Yeh lai REPORTS ON THE STATE OF SCIENCE. P " v "* la REPORTS ON THE STATE OF SCIENCE. Corresponding Societies.— Report of the Cominrittee, consisting of Professor R. MELpoLa (Chairman), Mr. T. V. HotmEs (Secretary), Mr. FrANcIS GALTON, Sir DotGLas GALTON, Sir Rawson Rawson, Mr. G. J. Symons, Dr. J. G. Garson, Sir Jonn Evans, Mr. J. Hopkinson, Professor T. G. Bonney, Mr. W. WHITAKER, Professor E. B. Poutron, Mr. CurHpert PEEK, and Rev. Canon H. B. TRISTRAM. Tue Corresponding Societies Committee of the British Association beg leave to submit to the General Committee the following Report of the proceedings of the Conference held at Ipswich. The Council nominated Mr. G. J. Symons, F.R.S., Chairman, Dr. J.G. Garson, Vice-Chairman, and Mr. T. V. Holmes, Secretary to the Ipswich Conference. These nominations were confirmed by the General Committee at the meeting held at Ipswich on Wednesday, September 11. The meetings of the Conference were held at the Co- -operative Hall, Ipswich, on Thursday, September 12, and Tuesday, September 17, at 3.30 p.m. The following Corresponding Societies nominated as delegates to represent them at the Ipswich meeting :— Belfast Natural History and Philosophi- Alexander Tate, M.Inst.C.E. cal Society. Berwickshire Naturalists’ Club : . G. P. Hughes. Birmingham Natural History and Philo- J. Kenward, F.S.A., Assoc.M.Inst. sophical Society. C.E. Buchan Field Club . ; John Gray, B.Sc. Burton-on-Trent Natural History and James G. Wells. Archzological Society. Caradoc and Severn Valley Field Club . W. W. Watts, F.G.S. Chester Society of Natural Science and Osmund W. Jeffs. Literature. Chesterfield and Midland Counties Insti- WM. H. Mills, F.G.S., M.Inst.C.E, tution of Engineers. Croydon Microscopical and Natural His- W. F. Stanley, F.R.A.S. tory Club. Dorset Natural History and Antiquarian Capt. G. R. Elwes. Field Club. East Kent Natural History Society A. S. Reid, M.A., F.G.S. East of Scotland Union of Naturalists’ Prof. D’Arcy W. Thompson, M.A. Societies. Essex Field .Club . 2 T. V. Holmes, F.G.S. 40 REPORT—1895. Federated Institution of Mining Engi- neers. Glasgow Geological Society Glasgow Philosophical Society Hertfordshire Natural History Society . Ireland, Statistical and Social Inquiry, Society of. Isle of Man Natural History and Anti- quarian Society. Liverpool Geological Society . Malton Field Naturalists’ and Scientific Society. Manchester Geographical Society North Staffordshire Naturalists’ Club. Norfolk and Norwich Naturalists’ Society North of England Institute of Mining Engineers. Northamptonshire Natural History So- ciety and Field Club. Perthshire Society of Natural Science Rochdale Literary and Scientific Society Royal Cornwall Geological Society . Somersetshire Archeological and Natu- ral History Society. Warwickshire Naturalists’ and Archeolo- gists’ Field Club. Woolbope Naturalists’ Field Club . Yorkshire Naturalists’ Union . Field M. H. Mills, F.G.S., M.Inst.C.E- J. Barclay Murdoch. Robert Gow. John Hopkinson, F.L.S. R. M. Barrington, LL.B. His Honour Deemster Gill. E. Dickson, F.G.S. Dr. E. Colby. Eli Sowerbutts, F.R.G.S. C. E. De Rance, F.G.S. H. B. Woodward, F.G.S. Prof, J. H. Merivale, M.A. C. A. Markham, F.R.Met.Soc. A.S. Reid, M.A., F.G.S. J. Reginald Ashworth, B.Sc. T. R. Polwhele. F. T. Elworthy. W. Andrews, F.G.S. Rev. J. O. Bevan, M.A. M. B. Slater, F.L.S. Ipswicu, First CoNFERENCE, SEPTEMBER 12, 1895. The Corresponding Societies Committee were represented by Professor R. Meldola, Mr. G. J. Symons, Mr. Hopkinson, and Mr. T. V. Holmes (Secretary). The Chairman of the Conference opened the proceedings with the following address :— Address of the Chairman, G. J. Symons, F.R.S. Just as with the great Association under whose auspices we meet, so with the numerous and intellectual bodies which you represent—each has a double duty. The duty to humanity of doing its best to in- terpret truthfully the lessons of the world in which we live, so that by increasing knowledge future generations may learn to make better use of its marvellous stores, and perchance repair some of the waste which has gone on in the past, and which is still going on. Our other duty is to advance the cause of the various bodies with which we are connected. Of course you know this as well as I do, but in these days when a universal genius has become an impossibility, and progress can be effected only by limiting one’s work to some corner of the field of science, there is great: danger Tot specialisation leading to forgetfulness of generalisation, and of what is the end of all research. You all know the necessity for inter- communication, which in the early years of this century rendered the formation of the British Association imperative, and you know how that need was met. I hold that this Conference and the work which it is doing are an equal necessity of the present time. How could workers in any branch of science know all that was being done by local effort without our index to your proceedings! The world is the better for the knowledge which you gain being rendered generally accessible, and both the British CORRESPONDING SOCIETIES, 4) Association and the local societies gain the strength which arises from federation. The Council having nominated me to the honourable office of Chair- man, my first and most pleasant duty is to offer you a hearty welcome ; and my second, which is a somewhat personal one, is to ask you to remember that it is not given to every chairman mentally to photograph every one present, and to remember not merely every face, but the name of its owner ; it is one thing to be Chairman whom every one can see and recognise, it is quite another thing for the Chairman to remember all the faces before him. It is therefore from no lack of courtesy, but from the physiological necessity, that I request that each delegate will preface his re- marks by mentioning his name, and that of the Society which he represents. I have already intimated my opinion that if a man wishes to do good work for science he must take some field, or corner of a field, and labour there. I have only a corner—rainfall, but I think that I know enough about some other parts of the field of meteorology to point out spots where good work could be done—and work precisely suitable for the members of your societies. Of course in the few minutes during which I may detain you I cannot enter into details, but there is such an organisa- tion as the Post Office. I do answer as many letters as I can, and an extra twenty or thirty will make no appreciable difference. Now, to take up the syllabus :— 1. Meteorological observations in general.—Do not encourage the keeping of records from any but good instruments, properly placed. A hard frost occurs, and forthwith there is a crop of wonderful records, some from thermometers badly placed, some from thermometers which never were good, some from good thermometers allowed to go wrong. An incorrect statement is much worse than none at all; see to it then that such records as you publish are worthy of your Society. I say no more on this head because the Royal Meteorological Society has published, almost at cost price (ls.), an amply illustrated pamphlet, ‘Hints to Observers,’ which will show any one what, and when, and how, observations ought to be made. It is by no means necessary to start with an elaborate and costly set of instruments ; but see to it that the instruments which you do have are good, and that no records except from good and tested instruments, properly placed, ever appear in your volumes. 2. Sea and river temperature.—I have interpolated the words ‘and river’ because I ought to have put them in the syllabus originally, and because my attention has been drawn to the subject by an excellent summary of Dr. Adolf Forster’s work upon the temperatures of European rivers, by Mr. H. N. Dickson, given in the September number of ‘The Geographical Journal.’ You will remember that for a few years there was a Committee of the British Association studying river temperature ; and I am sure that if your societies took up the investigation, a fresh committee could be appointed, so that we should not need to go to a German book to learn the details of the temperature of the Thames. The work is easy, healthy, and inexpensive. Easy, because it merely involves a walk to a bridge, a jetty, or a p‘er-head, the lowering of the thermometer into the water, entering the reading, and carrying it home again ; healthy, from the regularity of the walk ; and inexpensive, because the verified K. O. thermometer and its copper case, cord, and everything, could be sent to - any part of the country complete for a sovereign. 42 REPORT—1895. 3. Harth temperature at shallow and at great depths. —The second half of this subject has often been brought before you, because the Underground Temperature Committee is the oldest one of the British Association. It, as you know, deals chiefly with the temperature in mines and in deep shafts and wells. Any one who can obtain good records at depths of, or exceeding, 1,000 feet can do useful work, but I am doubtful whether much more can be learned in this country by observations at depths between 10 feet and 1,000 feet than we already know. I insert the words, ‘in this country,’ because I do not think that the law of decrease for tropical and for arctic localities is known. Unfortunately we have no representa- tives of such localities here, or we might sow: a productive seed. Obser- vations at shallow depths—say 3 inches to 10 feet—are becoming less rare than they were, and the time is not distant when the law of temperature variation for shallow depths will be known with sufficient accuracy. That much has yet to be ascertained, many persons learned by burst water- pipes last winter. I mention this as an illustration of the application of scientific records to the welfare of mankind, not as an indication that I consider the mischief to have been wholly produced by soil temperature ; but I must not digress. 4. Phenological work.—I am afraid that this word ‘phenological’ has not proved very acceptable. I once heard an inquiry what meteorology had to do with prisons—and it turned out that the querist had overlooked the ‘h,’ and reading it as ‘ penological’ thought that it must have something to do with punishment. However, I need not tell you that it means the laws of the life history of plants and animals ; in fact, an endeavour to record the progress of the seasons not by thermometers or by rain-gauges, but by plants, trees, insects, and birds, and the study of the relations between the indications of the natural history phenomena and those of the instru- ments and efforts to separate cause and effect. It has always seemed to me a class of work peculiarly adapted for the local scientific societies, for their Botanical and Entomological Sections. The Royal Meteorological Society has spent a considerable sum in promoting this work, and in the hands of Mr. E. Mawley it is progressing. Personally, I am not competent to pronounce any criticism upon the work beyond this, that Mr. Mawley has devoted himself to it, and has produced tables and diagrams of great interest. But I do say this, that I think that the naturalists should either co-operate heartily with the meteorologists, or else should show that the meteorologists are attempting the impossible or the undesirable. 5, Early meteorological records.—lt is a prevalent idea (especially with executors) that old manuscript books of observations are useless. I have every reason to believe that a long deceased relative of my own assisted in burning part of the oldest record of the rainfall in this country—that begun at Townley in Lancashire in 1677; and what she did at the beginning of this century has been done by scores of others, and will be until mankind are much more thoughtful and much better informed than they yet are. But I am not addressing you in the capacity of executors, but as representatives of large local bodies, many of them with museums and libraries ; and I invite you to see to it that any such records that you have are properly cared for. Another suggestion—the practice is fortunately rapidly spreading of publishing the early parochial registers. If each society represented here would make it a rule to go through all such publications as have been issued within its area, and print in chronological order all the notes on —————=—s rh ee) an pa CORRESPONDING SOCIETIES. 43 earthquakes, storms, frosts, floods, &e., which can be collected, much good would be done. Of course this can be done for unpublished as well as for published records. 6. Records of river and well levels.—The second half of this subject has so often been brought before you by Mr. De Rance, the Secretary of the British Association Committee on Underground Water, that I need merely mention it. The first part refers to a subject involved in my next _ and last heading, and to which, therefore, I will at once proceed. 7. Records of floods and the placing of flood-marks.—It is very strange that Englishmen (Britons I had better say, for our Irish and Scotch friends are equally bad) are so nearly the worst nation in Europe for looking after their rivers. J do not refer to fouling by sewage and by manufacturing refuse, or to defective engineering—I do not know where we stand in those respects—but I refer to records of river levels, to scale marks on the bridges, to automatic recorders of their rise and fall, to arrangements for warning the owners of low-lying property when floods are probable, and to the classification, levelling, and publication in full, of particulars as to old flood-level marks, and the due marking of new ones _ when floods occur. I do not suggest that your societies should themselves do all this, but that they should bring it before their Parish and County _ Councils, and couple their request with the offer of any assistance in their _ power. Of course the suggestion will be received politely, the great cost _ will be urged,and in many cases nothing will be done. Forgive my detaining you to hear a little true story. Years ago I suggested such arrangements to an influential man in York—nothing was done. In 1892 York had a flood, not so bad as some on record, but one which cost the Corporation a very large sum ; they paid it, and that steed having _been stolen they have figuratively locked the stable door by adopting all the arrangements suggested above. If the Councils do not take your advice, they must remember that your attendance will be on their minutes, to be referred to when their town or district suffers as York did. The Chairman then read a letter which he had received from Mr. R. Ashworth, of the Rochdale Literary and Scientific Society, who regretted his inability to attend and sent some notes showing what meteorological work was being done in his district. Mr. T. V. Holmes (Secretary) wished to make a few remarks with regard to the list of papers read before the Corresponding Societies and appended to the Report of the Corresponding Societies Committee. He hoped that the secretaries of the various local societies, in sending in their lists, would be very careful where the paper, from its title, might belong _ to either of two sections, to group it with that section to which it had most affinity. Examination had in some cases caused a paper to be classed with another section than that originally given. It was very necessary also that the names of papers sent in should not be those of “mere popular lectures, but of investigations of a more or less original - character. It had occasionally happened that when reference had to be _ made to some paper on the list in order to ascertain its true nature it had been found that the paper in question had not been sent to Burlington House. No paper would in future be placed on the list published by the British Association unless it could be consulted at the Office. The Chairman then invited discussion on the subjects mentioned in his address. AA, REPORT—1835. Captain G. R. Elwes (Dorset) laid upon the table a paper on the rain- fall in Dorset, which had been compiled by a member of the Dorset Natural History and Antiquarian Field Club, Mr. Eaton, from records kept in the county of Dorset during the last forty years. It was a most careful and exhaustive piece of work, and was illustrated by maps and diagrams. Mr. Eaton wished to have the paper submitted to that conference of delegates with the view of eliciting remarks upon it. The Chairman said that Mr. Eaton was an old friend of his, and he had much pleasure in testifying to the excellence of his work. One of the maps of Dorset was shaded so as to show the proportionate amount of the rainfall, the other the varying elevation of the land, and, as might have been expected, there was a fair amount of parallelism between the two. Mr. Eaton’s work was an admirable example of the way in which the rainfall of a county should be worked out, a labour especially requiring much patience and perseverance. He wished they could have such memoirs for every county. Mr. Sowerbutts remarked upon the difficulty of discussing Mr. Eaton’s paper in the absence of copies of it, and Professor Meldola said that there was not much to discuss, as the paper had been brought forward simply as an example of the way in which such work should be done. Professor Merivale asked whether it would be possible to obtain copies of Mr. Eaton’s paper, and Captain Elwes said that he would do his best to get copies for any gentlemen who would give in their names. Mr. Hopkinson stated that twenty years ago he began to record the rainfall of Hertfordshire with about twenty observers, and he had since done his best to add to their number, with the result that there were now about forty. The report which he had published last year contained the monthly returns from forty observers in Hertfordshire. He had obtained about thirty daily records, which were worked up and analysed but not published. In the Transactions of the Hertfordshire Natural History Society much space was devoted to meteorological work and to phenology, and he hoped that the Sccieties in other counties would work similarly at these subjects. He trusted also that delegates would preserve any early meteorological records they might discover. Mr. De Rance, in illustration of the increasing usefulness of local societies, mentioned the fact that two Committees of the British Asso- ciation, of which for many years he had been secretary—that on Coast Erosion, and that investigating the Circulation of Underground Waters— had just ceased to exist in consequence of the admirable way in which their work had been taken up by the Corresponding Societies. His Honour Deemster Gill mentioned that the subject of Coast Erosion had been taken up by a Committee of the Legislature of the Isle of Man, of which he was a member, but their investigations were not yet complete. But they had found that for some twenty miles on the west, the north- west, and the north, erosion had been going on to a very large extent, the evidence showing a destruction of land of about twenty acres to the mile within the last fifty or sixty years. The whole of the information would be sent to the proper Department when the investigation was concluded. Deemster Gill added, in reply to a question, that the portion of the coast mentioned was not rocky but sandy. The Chairman remarked that the meteorology of the Isle of Man was being looked after by Mr. A. W. Moore, and Deemster Gill added thai all that was necessary was being done there in that department. CORRESPONDING SOCIETIES. 4S Mr. Sowerbutts asked whether it was desirable that the Manchester Society should collect the results of observations at the observatories, and forward them to the Meteorological Society, and the Chairman replied that it was just one of the things wanted. Mr. Sowerbutts added that, though there were several observatories whose observations were hardly worth having, there was a thoroughly efficient one in the Park, under the Whitworth Trustees, another at St. Bede’s, and a third at the Manchester Waterworks. Captain Elwes hoped that it might be possible to induce local scientific societies to co-operate for the discovery of flint implements, and the for- mulation of results. He wished that they would make this branch of investigation a more special feature of their work than it was at present. Mr. Osmund W. Jeffs, Secretary to the British Association Committee for the Collection and Preservation of Geological Photographs, stated that it had been proposed by the Committee, and adopted by the Council of the British Association, that the photographs collected, should be placed in the Museum of Practical Geology, Jermyn Street. The first part of the collec- tion, consisting of 800 photographs, had already been deposited there, and the rest would be handed over as soon as possible. As, however, a great many parts of the British Isles were still unrepresented, it was proposed that they should go on collecting. From some of the eastern counties no pho- tographs whatever had been sent, and on that very day he had been pro- mised some from that neighbourhood. He hoped, therefore, that the _ delegates would remember that they were still collecting, and would men- tion the fact to their respective societies. Mr. De Rance, after complimenting Mr. Jeffs on the results he had achieved, remarked that it would be a good thing if each society would _ issue a circular, and send it to other local societies, so that all might know what photographs had been taken in each locality, and were available, and, on the other hand, in what districts photographers were most needed. Mr. Sowerbutts dwelt on the very valuable results already attained by Mr. Jeffs, and proposed a hearty vote of thanks to him for his exertions. This vote was seconded by His Honour Deemster Gill. After a few words in support of it from the Chairman it was carried unanimously Mr. Jefts, in acknowledgment of the vote of thanks, said that they were due rather to the Geological Photographs Committee than to himself personally, and that the work could not have been carried out as it had been but for the active co-operation of a great number of the local societies. Mr. J. B. Murdoch (Glasgow) thought that in too many of their investigations Scotland was excluded. He might mention as an example the British Association Committee for recording the position, &c., of the Erratic Blocks of England, Wales, and Ireland. Mr. De Rance stated that the Erratic Blocks Committee was formed many years before the meetings of the delegates of the Corresponding Societies began to take place. Any Scottish member of the British Association might have brought the matter before the General Committee and proposed the extension of the work to Scotland. Some remarks were made by Mr. Sowerbutts and Mr. G. P. Hughes on Scotland as a nursery of boulders, and the Chairman said that his impression was that many years ago some one suggested the inclusion of Scotland in the labours of the Erratic Blocks Committee, and was answered by a speaker who stated that the Royal Society of Edinburgh was already at work on the subject, and that it would be unwise to 46 REPORT—1895, trespass upon its territory. For his own part he was always pleased to co-operate with his Scottish friends, and had done so on the question of rainfall, and it would appear that in this Erratic Blocks Committee the exclusion of Scotland was the result of deference to her susceptibilities. Mr. Murdoch replied that it was quite true that for many years a Boulder Committee had existed in Scotland, but the work had been entirely under the control and direction of Mr. Milne Home, who was now dead, and who, for some time before his death, had been unable to get about the country. Mr. Milne Home’s Committee had issued eight yearly reports, which were very valuable, as many of the boulders were not only tabulated, but figured. But for some time the work had been practically at a standstill. The Chairman remarked that in that case it was certainly desirable that steps should be taken to have Scotland included. Deemster Gill said that the boulders of the Isle of Man were being noted by the Society to which he belonged, but not, he thought, by any extraneous body. Professor Merivale remarked that for some time they had been dis- cussing matters connected with Section C. He wished, before the meeting ended, to say a few words on Flameless Explosives (Section G). The North of England Institute of Mining Engineers had been continuing their experiments, and had published one report. They were still going on with their labours, and another report would be published shortly. He had nothing to say then as to the results of their experiments. The Chairman supposed that the Conference was, as usual, in favour of an application to the General Committee for a grant of 30/. to enable the Corresponding Societies Committee to carry on its work. Professor Meldola moved that an application for a grant of 30/. should be made, remarking that the amount named was only just sufficient to cover their expenses. The proposition was seconded by Mr. Hopkinson and carried unanimously. Srconp CONFERENCE, SEPTEMBER 17, 1895. The Corresponding Societies Committee was represented by Dr, Garson (in the chair), Mr. Hopkinson, Mr. Symons, and Mr. T. V. Holmes (Secretary). Dr. Garson said that Mr. Symons could not take the chair, as he was then at the meeting of the Committee of Recommendations. It was usual at their Second Conference to consider the recommendations from the various Sections respecting work in which it was thought the Corre- sponding Societies might usefully co-operate. He would therefore, in the first place, call upon the representative of Section A. 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k es * "00G "[09H “Y “Mutoh ; * soyoveg pesiey ug |* “VV ‘Mf ‘GOsUnAL g68T| ¢€e ‘XI i y * "SUDA, | * “OOSSY “[094) Spoo'T | * : * sourpy teddop ogury, ory oxy, |‘ "H MT ‘POOAL oy S61 Pr “"PSUT “pag “SUvLT, | * i * sul “sug “N | * f : : * SPLPUPION PuRIny ys | ° ‘d “ “poom 928 N-9Y}-U0 6 09T ce * ISUYDINIDNT assy : * 'O "\ xXossi “TOTEM WOIF VOSNT]OWL SUE -UON OUBOISTIOTT | “WM POITTAL ‘qq2M te 69 ‘TITA : g qwusnor | * * "009 "Hl "N ‘007,.N 2 S9JON TVOIsofoex | Aqoog ‘uosdmoyy AIOM SIvaX WIGS F68T| L6G | FEST AON | * MyDUNngnAT ay T | ° * UOTUYS) “JEN “SHIOX | SH puw soqqwmM0H Jepnog s11YysyIOX oyL |° semoyy, ‘278,], Yiprep ‘yoorg Suryi0M ‘Aramoig XIMOYT oY} Je TAM UeIsoIy ue jo Sutog oy} SuLNp vyzvIAG [AV] Pey MeN oyy UI ploy ~ LOT Wy Y § “a 3 : “ S OAYVN JO SUIBIQH JO 9DUAIINIDG 24} WO S2aj0ON | * $e St * ‘ JOOUIDAVT | ae ae | - Ya ic * 5. aa t if { s > J — ~ x $ Sho | REPORT—1895. 62 €6°G68 [10.7 ‘Til aN ‘II ‘TAXX ‘Til OL POST LON S681 107 PEST 107 6 ON 'T ale THA “re “AX FEST 10.7 €6-G681100 ‘AT “A “AI Ti iv q 10 ouNnyO A ‘SUDLT, 001 ‘SUDA, “"D0bq PUD ‘SUDLT . . . “ . “cc “cc * 981 DLNQONT IYT : : * “SUDLT *"00lq PUD ‘SUD, * SYDINIDAT LASS . . . “a . . © "90. “ SUDANION OUT . . * “SWOT, uoryworqNg JO OTT, ' ‘OH 'N 'W uopfory ‘O ‘a squey * "909 "FEN “AION *JAION ‘Tog "N ‘00g ‘syyOg * + ‘90g "FEN BIpseg "1009 "Tid “WT 10380010] "008 °V "H 'N ‘Tey ‘ung . . “ce “ . . “cs cc : * MOTUAQ “YN ‘SyIOX * “OH TBA “AOS 27 “TRO "TOS *N 009 WHO . : = ‘DO ‘A Xossy ‘ ‘0° ‘V‘H'N 20s10q * + WOTUA “eX ‘syIOX ’ ‘0 'H‘N ‘W uopforp : ‘009 "A ‘N Mossepy * "009 "JBN “AMON "JION : ‘009 ‘H ‘N MoOSsely ‘009 "[IYq “41'T Jaqse0re'] Ayato0g JO OTFTL Pozeraciqqy uoly -U9ADT J PUB OSNLD S}I : OSvISIG’ UIOMIIG OYJ, syuey YON JO Vosn[poyYy ey} Wo sazoN J9yIAN AT (qsvT pIIyL) vxoydimaey : YLOJAON Jo vxioy,q pue vanvq : UdAVIY OY} JO JUNeY-Surpserg ureyunoW_ V : * UWpOYssviyH UWLOIy soION AIO4SIP TRANQeNT : ; t eroydopidery- OXI YStJIG oy} UO Spllq U0 aJ0N V qseoQ ailysupooury ay} WO ITRITAA pexoeq-duny 9q4 Jo soueIIn00Q C6-FE8T FO 10FUTM OY} Ul JOLYSIq: JOqUINF, oy} Woz sojON pig ; F68T FO UUINNY oy} UL JOLYSI Joquiny ey} Wosy SO}ON PIT ‘ —- gold}SIG, IoquIN;T 94} WoIy saqON prlg says JO taysdg yeuep A1osueg oxy, (stunosuyy uo) ssarppy Sutuedg XOSSH UI Jeg ouljoIeg OU, suufuoukg JO UOTZVOgTWOOY YIM ‘EGRT UI puNoF siopidg YS ore pue MaN UO . . . . : : ¢ : p * gasioq jo sopiqyday E681 1OF SION YON WorZ sojON [BOLsoTOyITAIO ‘ — svlnu siuiagy JO yuowdopeasq 94} WO sajJON suvod -O}OAQ FO DOUVOYIUSIG 94} UO syIVUO YIM ‘awadorosp jo uo, @ Jo AMOYeUY oY} UO SazONT * —- SUOTINEUYOT : H[OJION Jo vunvT * spiig WouUOD smIOS Fo syIqey OY} WO SOIONT sjooyy puv sosneg S}I : warery snosoydopidey urez1e0 Ut UOT}eOTIIQ tadvg Jo apjty, *(panwquor) XNOTOOZ— Gg wWoroagl . . ‘g ‘Vv ‘UIe yy "MTA ‘A0y ‘ord * somes ‘spieapy ‘WH 'M ‘T00" qnary ‘a1yyng * "7 ‘euviqg LO ‘Aoy ‘[]94499NID uyor ‘et110p * ugor ‘xnvapz0p * “HAA ‘e8arT[09 * Arua ‘sazvo0p * Je ‘49sryO 6é “ ‘IO ‘aay «‘asprquep pievuoe7] ‘ssergng uvuUpooy "A ‘O pue “AA ‘uaspng . + “7 ooIg * ‘qf ‘ueumspig . . ‘Vv ‘a ‘phog ‘I TTexHsnog IoyNY Jo awey 63 CORRESPONDING SOCIETIES. “ “ bE9 66 83 ‘61 “ ‘TIA ‘AI ‘Il ‘I S681 100 ity FEST 107 6 ON I “ce ‘TIIA ‘TI ‘3d “TX THATX 6 ‘ON ‘I * "SUDA jouimor . . . é "SUDLT, " $SUDINIOAT “YOON : qoucnor . “cc ity . “ec “e . “ “ * gSyDUngON 9UT, . . iT7 ‘SUDLT qouinor . . . “cs . . . “ce ‘000 JEN ‘AION ‘JION * *00$ "H ‘N ‘00},.N * ‘000 ‘H 'N sqey{ ‘009 ‘H ‘N Mossepy * *d ‘NT Joysoqooy ‘008 ‘IMd “HN “Wr . a6 “ . “e “ce . “ 6s * UOIUQ “JUN ‘SYIOX ‘DO “H TIAA “A05 27 “teD ‘009 “4eN ‘MION “JION * ‘009 "H ‘N 'U04,N ‘009 "H 'N “V ‘Us}es,u10g ‘009 ‘Td “WT 100d,4r] . “ iT3 * "009 'H 'N 80H 0909 ‘JEN ‘AION “JON “ “ec “é “ ‘SOUSly :YLOJION Jo vuneg E681 10} pooymmogysieN pue artysuoydmeyyIoN Jo ADoTOYAIUIO et} UO soJON S681 teed 04} SULINP OILYSpIOFIALO]I Ul pOAIASqoO spAlg UO SojON auTysaTVg JO VOSsNT[OJ[ IO}VM-YSo1] PU PUBT IY} JO MOS TO syIvULEY ; sous LH oy} UT sok 94} JO UOIQVISIPY, OU, eB1a00pe[O YS ay} Jo stsdousg ysnoroqivog ‘uoydy rv93U ueyey sopoog TOYeM JO 4SI'T 94} 0} SUOTZIPPY d Apasety, pUrx[pooM V * ySsnoicqieog ‘uoyAY IveU WAHL} Sopjoog TOV A, “Oo ‘aILysu[OOUr'T Bsc fs 2 ‘QllysyIOK ut “ox ‘vynrasnf ‘~anL0ga mpoupod ‘soroHe A Sit pue mpedrorwgn) vuLosoprdgy SYMVPT YSN * Spllg :Y[OJION JO BAO[T puv vuneg (sn022 -sauop ‘q pure snuvjzuow “assvq) morredg prrqsy purlsag a pad o1do1y, ay} JO sduUeIINIIO splig yooy Ysiy MIOJION Ul (vpn2 SUQ) preysug yeery ey} JO 9OUEIINIDO yUsDOY sooeTEVIG TOY} PUL SoTpIE[IUMIG Mey :sfoyuoT pur us . . ; JOSIOWOG JO SpAl_ FO 4SvT OY} 0} VpUeppV s}Uy ULoLIEMLY YNOG ey} JO speg Woorgsny 9YL €68T re94 0y} Sutmnp eITysp10j10H Uy pearesqo vioydopide'y uo soqoN, : * S681 JO uorzeysozuy dseMy oy, (ouingoou) srurmoy srumbuns DwopyT WO S24ON ; ‘aJ'T puog Jo spearv oT, * sssq pur syseN Spud WN Ci * uyor ‘iq ‘eMoy i PIOT “plozqyy : Arueyy ‘story ‘TVD “Gus ‘ ‘HOM ‘soysnqq ‘ ‘A ‘y, ‘Wosspoy . 6c “ec . ac oy "OM ‘aay ‘MoH * WRITTLA “979M0H "HOW ‘sotsie yy TIOMYINOS “VY, pure “yy ‘¢ ‘Aourny : "Hf ‘foumy . . ace “hi ‘uuny * preipory ‘ausetH ‘ad ‘48 “H “qurmsploy eet k ‘Ford ‘wosqip j ‘a “Vv ‘sqqry . ‘ad ‘H eB IES) . “ce “c 1895. REPORT =x © “ F681 9681 F68T S68T “ “ F68T “ “ec S68T peyst] -qng g0€ 116 LLI €8 68 18 08 6L S6T G68T 10 “ce F681 104 “ “cc sc ‘AI “ce “AX G68T 107 EA &F ‘III “A ‘TITA ‘II “AI yavgq Io on [OA “ “ eC 8 “ . “ “ . “ “ + gsyangoNy ay], . . . a“ . . . sé “SUDA, 201 * 48YVUNIONT OUT, * ‘SUDLT, * 2.todaay . . . “cc . . . ts ‘SUDA, . “ “ * 00d PUD “SUDA, * PBYVINION “A'S! uorzworgnd JO OhL “ “ . . “cc oe “oe “ce : * UOIUQ “YN ‘SyIOX “ “ee . . “ “ec . . “ “cc . . “ce oe : 009 “FT "N MOSsepy - “OV HN Josi0q : * UOIUQ ‘JVN ‘SyIOX * "009 ‘9@N “AION "JION * 008 “H “N ‘1190 “41721 “0 ‘ay Ueyong * "009 "JBN “AION “JON 009 “HH 'N soy “ “ec “ O08 VY HEN ED ae "TOY *N 00g “syWEg ‘009 "H 'N 9093 “GT Ayato0g JO OPEL PopBraosiqqy G68T OF FB8T VOZ0,OIg * 6681 OF F881 “eqeurapoulyoy IGST ‘eroqdopidary G68T OF F881 ‘ea0vysniy 1681 ‘spug : Aydeasorqrg uury Sunpphydowhyy vuaydonjbhy NSVIUOT[ ‘SIw7/Le HUW snavUy “UULT ‘ungnpun UNULIONT sprvapy ou ‘srzpayoynd snuopoped pur ‘oxygery ‘saprowsoopod aoypzayduy uosdwoy yy, ‘2auvy vuynoovy E68T ‘SPURT jo SumeMo,q oy} pue “ow ‘syoesuy ‘spit jo soouviveddy ey} Uo suoT}VAIesqQ uo y10day muospie “YOu ‘wyyaisayung wrwuyosrdg JO Bare'y ayy JO wordiroseq] YIM “E6-ZGST Ul vioqydoprdeT yos10q JOIt4sT( OBIT oY} pu puLpiaquing Jo vaprourry ey JO 4ST] VW HLOFION UI09S9. M-UINOS UT EF Ss8T JO POOT,T FeA.LH 94} UO : * SOJON Tsorsofomoguy SOJON WGIM ‘ysvo— peoyrojed JO soustad ey} JO 4SIT sjouygnqry * SUMOMYJILT A[OJION WO SojyoN GST teak ay} SutInp s1ysps10j410F UI peatesqo vuomoueyg jedisojouayg uo 41odaxy wanasn AL aya! IqpnoyITYOy} 04 SUOT}IPPY[BOLso[ooz queda * €68T IO} SOION [BOLSOTOYITUIO ASopowmoyuy s1ysyyleg aILYsyy1eg Ul SuL1m900 so1oedg jo 4sIy v YQIM 1at30003 ‘v1a\domoH ~exoyd m0 puc ‘ereqdor9}0H- -eioydimey au, : : * sapIpooo1n o . . “cc “ . . . . . . jadvg jo at *(panwju0?) KNOTOOZ—q uUon0ag “ce oe “ce “ec “ “a aC ‘Mh xenaeoe . “ee “ . “e sé ° “ “ee ‘uos}19qQ Or “a “6 ‘WN ‘dospreyony ‘OW 409 ‘OSpruiq “MB - PIVAdIG “WV "Jorg ‘Uoj MeN "+g yore " t xXeTY Aeeq "sy ‘presen * prvapy ‘AolMvyy : uUyor ‘aT yoW * ysny Avyovyy “ “cc ‘WL ‘toseryoyq . “‘) ‘ULyeq ol loyyNY Jo eure yy 65 CORRESPONDING SOCIETIES. FEST S68T IT &F IT “ ‘TIL joUusnor * ‘SUDLT qousnor ‘00Q “S005 aptsoucy, * 00g "yory “HN ‘qang ‘00g ‘s004H apisoudy, S68T F681 S68T FEST S681 “ “cc €Il TTA £68T 104 F8T 10g S68 T IO FG8T OT “ “ “ : q860) UvIZeM[VG IY) O} JISTA JUDAT W asouvdyr oy} pue uvder ‘ — - BIIOY UL suMoPY Oy, "ydep pt Gendly Vy ‘qstpusaty ‘LH ‘aMorg ‘gq ‘Aopreorg Fy "“AHAVUDOINH—'"W woyoag “ “ce “cc “ec 1vuinor . "20h “ “ “ a BY DINION OY, * "SUDLT “ “ * "909 ‘H ‘N ‘007, 0 eV) "HON Weg . “ee “ * UOIUQ IVN ‘SxIOX “ “6 “ “ee “ce ae “ce “ a“ “ee “6 “cc * ‘O09 "JUN ‘ANION “JION ‘009 "H 'N Mossepy S Wd aT 10480010] * "009 "H 'N S}19H{ . “ “ . “cc “ (wading vrusng -0Y) YJOW IoIodmy oy} Jo AIOWSIPT ofr oy, | qn{O 943 Jo UapisaTg puv teapuno7 ‘pleyemorg “TI ‘Aey o4¥’] eq} Jo saousosturmay FOBT 10F AoC A WORE BEAL OUd Wine Be oN Pate 3 [IBPOVAM MOT[OX IY} JO uoT|eLSIPL OU, * OATYSYIOX JSCA-YIION Ur vraydoajop AQUTM YO ysty ourt{py FEST-ZEST ‘AqqIT AA Wosz sajON AIOYST [BINIEN Cuury ‘snbuasvy vadnzg ) SUING oy} JO uUoTyNqIysIq pue soyewe, QsvT PINGZL) BlVUWUL]Y : Y[OJION Jo vO, pue vuney EGS wok ay UL TANasNTY YOIMION pue Y[OJION oy} 0} suUOTJIPpy stI0g P * SGST Jo Ataysty Suttwoep oq} uo sazoN 4S¥OQ Y[OJION Oy} uO (H209.L0q DIOYT ) [WIG paprvag vy} JO souaIIN00Q 9} UC ¢ " WOWOEg YNoMIVA wary oY} 07 SSeIPPV * ssoippy [eIyUapIselg Ja1log @ sev “uuary ‘nznds109 svjpoyg emysify ul (‘qua ‘vsnpa svy07 ) Apieyyng 9 Moyjed-popno[g ey} jo 90ue7IN009 UdLS.19 4 NI Iwo ‘H[IMsTJsVQ WO, VORIJSOMOZUM VMWOS uO eprjeu . . . . . . . =12905 ystyig 94} JO satjotivA 9a} UO saqjoN a * uotyeg 949 JO ALOJSIP] [VINJLNY 9, ss O68T, 01 FSET “VIVIIyUaTDMD : Aydeasor ad uo Iz UO ‘H ‘A ‘AeY “poom “HH Aaqy‘poomuryy "EW “HOOT A ‘Ty ‘Wy ‘aosduoyy, ‘soy, ‘ucsuaydaqg “*¢ ‘aosyvAy-fovqg . “ “ . “ ae e “ “ee ‘ LT ‘TRANG \ “ugor “qgrmag * semoqy, {49009 9) g AY * ast0an ‘1adooy Six 1895, 1895. REPORT 66 “ “ “ss “ “ S68T F68T «“ “ec £681 F681 a7 $681 F681 “ S68T F681 S68T paqst] “qud Lol €&1 69T Stl F&I 896 iti “cc “cc “ce “ qouinor * SUDLT “ce “c “cc “ 7 “ “cc “ce 1DULnNOL * SUDA], a “ec “oe “ “ «“ qouLnor III : . YX 5 - ‘XT 5 . €6-G68TION) * : “ . . 6 . . xX , , Tl : ; ‘XI . : Bede. YX . : “ . . ‘Til 3 ) T : : ‘TIL . . “ . . Sd ; : 418g 10 eUIN[OA worwo![GN JO HITT, . ‘009 “S004 apisousy, . “ “ . “ec “ce . cc “ "909 “5004 "YOURTT ‘0 ‘H ‘NW uopdsorp . “cc “ "009 “50a "YOURTT 009 "5004 aptseucy, * 20g “S0a4 ‘qouryy 008 ‘Td “H ‘N ‘wig * "00g ‘s0aH ‘WouLyy ‘00g ‘.d0a4) optsoudy, ‘009 “UDIY “HN “ang ‘009 *50904) aptsoudy, “00g ‘Soay “qouryy 008 ‘Td “H 'N “Warg “00g ‘SoayH “qouvyy ‘00g “30a aptsausy, “ec “ "00g “S004 ‘Wouryy Ayatoog JO ORL poyeraaiqqy aidoag ay9 pue s1yun09 94} ‘eruomIy * svdkeyeuly oy} Jo worsay ony, ‘ : . * IOPVSTABN oy} ATUaTT oouTIg saoseul “eq 0} (a10y) Vyyy worz Aeaprey posodorg : ¥6- e681 UL AIOAA ‘AJorOog aamgoarT UBLIOJOTA a * Weer}g FINH sy} pur oyeum1[g : 5 : : * souuspry 94} WOLF SajoNy €68T UI [USOT 09 419seq URTIfY ayy ysnoryy ournor PEST “ItysytoX JO Aydersoap ay} UO UOTVUTMEX 944 UO 410dexT : : uoryrpedxg welod ysisug ouL . . “ E681 UL [Vonqiog ur Aaumor v Jo saqoNy BUOZIIW Gok Opwrofo ey} JO UoURD puvIQ oYy, : : * sojnoy epray, uvdvpewry * ; : : : * ummbuoy, pue wrig AVMTIeY Uewaqig yvery oy, yuvadoTy ot} ur ummolog vB uo sojJON OMe], OATS ey} WO szNsaYy queoyousg sqr puv ‘vorayy Temmap go quammdoraxsiy [eLorema04 our " uvysluey.ssy SUBPITY “IS ay} puv vplry “99 aay rene bue SITmvg oy} UL ssutsauimor : : aidoag sit puv euryg saqUIMOH [eJUeINAAIeda ayy Fo410daxy ay] 07 i 1 Aoaing dUBUPIO IY} JO YIOA\ OU, puvleuoyseyy Jo oingng oy, aodvg Jo opty, ‘seu “UL ‘FOIG “Zvraqoy, ‘a ‘OH ‘100 ‘1euuey, ny "g ‘Aoy ‘TeqqzUTE7g gC “WT ‘S}gnqiaMog * preamoy ‘¢ “paey * "Mf Sem pory ‘A ‘H ‘Iq ‘suosieg UWOA uoieg ‘wrayueddg SPIE CE paw? ‘X‘H ‘weyplo Vi STOTOMION, - “M “H “OTT * "a AA TeYsre yy * YO ‘mreyyreyy * pxory ‘Woy suTmET aoung ‘uryedory : “'y, ‘sey Mouy * “HH ‘wojsayor : ‘vy uyor ‘ABrDy | * 919998 “f ‘JIONTEL jo [ley ‘a1omung WU Jorg ‘sepsnog : ‘LH ‘yoor9 ‘Jy ‘y ‘unoynbrop Joy jo ouuy | —. er SS ee eee *(panuiquod) XHAVADOEH—‘T woroagy 67 SOCIETIES. CORRESPONDING e681 “ F681 f68T F681 S681 “ee “cr “ “ “ F68T “ec S681 “ F68T a Ee ae a ee ees eh A ee ee oe Bee 88 get OLT 63 £6 igg¢ FG-SG681I10g| * 9047 pun quoday S6-F68T | ° : * “SUDLT, “AXX |” : * "90 IX : . C6-FU8T | ° : ‘TIA . . . “ce qvuLnor . “ S6-F68T | ° ; * “SUDA, SORES : : e TLL! Oe ‘IX i C qwuLnor “AXX 5 i + “20. THA “"WSUT pag “SUDLT, "AXX : 20a ‘IIA . . “ "1X . . “ “ . . “ S6-F68T | ~ i * SUDAT ‘IX aS qouinor ‘AXX : 5 * 20d IX s : 1VUsNor 008 ‘Md “H 'N 9sej[9g * "00g “4RIg "Yours “00g "IY Mossely * puvlaly “00g “423g * "009 “RIG ‘YourTT ‘SUG “UTPY “SUT “pat * “905 "424g "Youryy "009 [IY Mossel * purypory ‘00g “4x49 . ‘009 ‘“TIGd Mossvyy . . “qsuy “SUnT "N "004 "TI Gd MOSSUpy ‘Bug “UI “sul "pag "009 "OAH "YW "AUIOD * "009 "379 ‘Woueyy * purely ‘00g ‘7249 "00g "[I[d MOssepy " purpary ‘00g “yeyg UIMIOA, JO UOT}VONpT YStpT OY, AUMIOUODT [LIOOY v uOTyRISTUIG, aTIUeANe 2 : 2 : * wolysont) soquerddy oxy, ,41ddng 1078 \4 omgnyy puv quasorg Ing, ‘iadug s.zoye A, “ap 0} ATdary : ; : ‘ : : * UOTJVXBT, [BOOT eIj00g VAON Jo quaumdoyaaoq [erouly OU, ‘puvlsugq jo Yueg oy} Jo syunoooy savaxX ATT SOIJOINOOY OYTFUeTOG ToyZO puv [vorydosoytyg ay} Jo AIOA\ oy} uO S]}Ud [VIOIpuLr JO WOISTAaIT ey} TOF OIN4yYsSqng vw sv asvyoang Asrospndmop qoodsorg & pue yoadsoajoyy & : puvyyoog Jo 4SOA\ OT} PUB MOSSLTD UL UOTJwONpH Tworuyoay, : : : : : * ssolppy [enuepiserg * smlotqorg Arequeg yuez10odmy aurog . . . . ° . ‘Soul JO Suryery UWOT}VO “py [worayoay, Jo sjusuidoyaaaqy yuaoey owog * S}UAWAAOT[ Joyreyy A[IvaxX oy} Fo A1oOayy, oyy, ‘ : ; : : ¥ * S19UI0M 00}409 ' F6-€681 SoyeIS Poul, OF UL sis [elouvurg oy, * G68 ‘PV suoyLnsoy Supring MossepH oy, s}oy pue’y oy} lepun uotsog pur ‘sorstiojovreyO ‘UISNO S}T :WOJsSND qYSII-JuvUey, 104s[Q UU, ‘SOLISILYLG GNV GONAING OINONOOY—q uoyoag . . “ce jousnor * ag, boa “ its ‘009 ‘S004 optsoucy, . “ec “ee * "00g *“B0aH ‘qouryy "900 "T1uUg MOSsepo . . qs0y Npurp oy} pue ‘ezuny ‘pear of) ie ULpng 94} 07 oynoY Joqrog-uryeng oy, | *O ‘[oO-"y] ‘Wosze Ay HA JOT YC | "aD ‘Monty : * uyor ‘stIjsuy * qaouadg ‘Aqaey * UTApHT ‘aruyny © cunt “op ‘urdyr) : “MCV ‘SOL ‘e ‘Jorg ‘wosns10,7 ' "A uyor ‘espa ; * {ruazy ‘19 * semmoyy, ‘sepsnoqg * somvp ‘s1oul[VyO . . ate “1 ‘apqysvp é "C ‘soTMog : Araay ‘suurg "M “AL TOD ‘sssig ‘AS 1, ‘Aqsreqqegq. “AA 851004) ‘SBE g : “A AM ‘ Aoqieg ‘a “a advo ‘pueqsnysuno x ‘UOTJESIABN vag vivy |p ydep ‘SsUISSIA, W 1895. REPORT 68 . ‘ . . FO81| 82T IITA : : “suply | * = ‘ou “Uy “4SUT “pad sjonpelA puL sesplig Joquiry, | *A\ Wesz0]q ‘soraeq G68l| Fg x1 2 i ears ge ieee 5: , " * * * WaAQ ax00 Avafog-yomeg ey, |* “H uyor ‘Aqueqg Ss LI TIA ASUT PE SULT, 5| ~ : * “qsuy “ouy “N | * 3 : ; * S[TMp-3Ooy YIM Suryurg | * yavrq ‘woysnop oe TLT ‘TIT : s eg : 009 ‘VY ‘H'N ‘zueg | * Suruiyy ystur0g jo Ar09stF] VY} UT Ia4¥dvyH ¥ | * ‘gd ‘f ‘ystur09 quasolg puv yseg FIOM Surmaeursuy F681| 99 ‘AX - : “"SUDLy, | ° * 909 "W Tood. Ary | 03 doUDTEJoI YIM “VoLIJy YINOG UI ANOJ, y | * "Ty ‘) ‘aoqing syonpoid-akg jo A1aaooary C68T| LF Cae ‘W8uy “pag ‘supe | * : ‘qsuy ‘Sug 'N | 9y} OZ woyskg puv UaAG 9yYOD Yyounrg oyy, | * * “7 ‘younrg SPMOIIN FYSVT O1ty ‘f col fi : g : as ‘ ‘ a! ss -09|] Ul dMsserg Suryelnsey Jo spoyyeyy omog | ° ‘SM “QInNOg sé I "AX : 5 * “SUD | * * ‘90g 'g Jood.ary | * suteautsug [edrorunyy :Sserppy Temoneuy |* “g ‘Y ‘sloujnog a[epi1eqyeg ‘oul, pray F68T| 9 TIA ““PSUT “Pay “SUDLT | * : ‘ qsuy ‘Sug ‘N | -TOATIg eprsucery ayy Jo uolydrtoseq pue A10ys1H | * = “HAA ‘osepIog UMOT, 943 Ut ATddng 19}BA\ 949 JO ssorsoI1g S68T! TéT Or : ; ‘‘supuy, | ‘009 “V "HN ‘Tey “wing | ey} pur ‘somjunq jo AJddng 193e\\ PIO o4y,|* some ‘noqieg ‘DONGIOG 'IVOINVHOSIY—' 9 worjoag c6st| T GG-F6ST | * : "*SQU0iUT, jae * 00g "9Bqg9 "Goury | ° quomdnoooy pur ‘yuottasro Ay ‘uoutIeyIog |* “S “FE “AN ‘SIIVAA a rad IX : : qvuinor | * * puvyery 00g "4R4g | * * 4iddng IoyVA\ VIN4N WT pure quasi nO “Vy UYOL axle os SOF ‘TIA : : “supe, | * “Bug “UT “ysu] ‘poy | ° : : " SseIPPY [eHuSprserd | * ‘vy ‘qatmdog I68I| ZS “AXX : : Ne I "009 "[Iq MOSSeTH | * : UY : " , *OSUA\ SULAIT VY |* “UA, “Iq ‘quvUIg C68l| 99 |FE-E6RT10q) ‘9047 puv quoday | * "90g "T1Yd “H ‘N IS¥jI9M | * ‘ f : ‘ ‘ uae Teuoyen |* Avmuop ‘goog yoodiaary IVwau s cé6I ce : 2 Smee s de ce ‘samioyy o8vjj0p AojIoyezey oy} Jo yunoooy |* “g ‘f “Iq ‘SUTAON parjeaz Mon st LOI ‘TITATX : * ‘004g | * ‘00g ‘TIT “gITT [ood ary | ul uoyxsisaT IMoqeyT pur orsielo0g yuoosy | * ‘WW “fC “Aq ‘a100Ty ss 9FS TIA ° “supe | °° “Sug UTP “gSUy “pay 4 * snswayyoreg jo Arjsnpuy g[tg egg, |* “VW ‘Taqdmvosiqy | Aouslmmy uerpuy uo as TL ‘AX X : : SN py) “909 "[Iqq MOSsepy | soqqQ1MIUIOD s]TOYOsITT ploy jo yzoday oy} uO *xolV ‘oopuroryy eiyRagsuy | #680 LOF ‘TIA E : * ‘SUDAT, | ‘ Sul ‘UT “SUT ‘pay | U9jsaA, JO soomosoy [e1euTy Jaeqjo pur poy |* “Ff ‘y ‘eoudery ‘poysty ese RH UOTPOITGN JO ITI, jo anit a rode g Jo opty, IOYINY JO ouvyy -qagd *(panuqjuod) SOILSILVLG GNV WONAIOG OIWONCOY-— yy ver p00g 69 CORRESPONDING SOCIETIES. ‘ILIA F6-E68 1107 TIA TIA eAuX TIA o “ TITA ‘AX “XI “AX “AXX ‘TIA ‘XI . . . “ * 'SUDLT “ec . “ “ ‘SUT “Pag “SUDLT . . “a : y * “SUDLT ““9suy “pag ‘Suna, ‘alg pup 2Lodary “PUL “Pad *SUDLT, ‘SUDLG : ; * "SUDL], “ “oc 98Uy “pag “SUDLT, . . . se . . . “ . . . “a ‘SUDAT, "UT “pay “SUDLT : ‘SUDLT, "204. “ “ “PUT “pag ‘8UDdT * “Bug “UNA “SUT “pag | : * 009 “Hf [ood ary . . . . “ “cc *qsuy “sug ‘*N 009 [OOH “Your "Bu “UT, “4sUl “pay * -qsuy “Sug "N "009 ‘Id “H ‘N S®jld "SUR UL “3sUT “ped ; * qsay “Sug ‘N ‘00g “a [ood Avy “ “ec “ “4SU FUND “PITT FOWayO * “BUG UIP “SUT “pay "00g "H [ood avy * -qsuq Bag ‘NI ‘00g “a [ood ary * "00g “TI MosseTH “ce ee “ “q8aJ quNOD "pI J109894) _Proyeos Aemoypey out ata A[snoaueyfamg SULYUIG pue Sure AL * —- syuameaRg 4oo1}9 SU[LY-POUg ur yuemasaoidmy SOLITON UWoAeTE}IT A, Bq JO YoIOAG TBOLL09ST HT . ssoUIN,T JO $21 10IJOS OY9 JO SUIUI, aL : : * —- soupy ur ysuq Surdmeg ug syuoutaAoiduy yuadaxT 0} 200 -Iajal Iv[NoyIed YYIA ‘doNesIAeN UIBAIg sq, qOLIystq TOABqoHTM OG} UT oyyerIaAY JO SUIYIOM IY, + SuOolqUaAUy [BOIIOIT| uULapoy : : : * —- auTaYyoY Taye, oUMO]Y oT, jeuep pur Avmyrey Aq 410dsuvzy, JO sysop pue suoljipuog satereduo0g ey, : * SOLIOT[OD WaAVYozI AA IY} Jo uoTydroseq aol pur ysop :Ao1oUq [woroepy jo Ajddng orqnug oy, Ioysoyouryy ‘M11 [0D UWO}SOPT OY} JV odoy sso[puy punoisiopuq uy [eop jo sat “YOU pUv SUTJIOg yOIIG IOF syUsMOSULIIY [eoruvyoeay «puke ‘Suiueer0g § ‘“qno - Suryueg qoIysiq Weysurmirg ay} 0} doUAIejer TeIoads IIA ‘UOTyVSIAVN purlUy ° * SOUl{ [VOD URI}OOY BAON Ut suOTsO[dxT 10}jyR[ oY} Jo yuourdoreaep peysoiie ay} Suryoutoid 10; uo1yeIapIsuoo sjt Aq pajsessns spoyjyout oy} pue ‘s{vm gt A pe skVMpIey Jo ssorsorg saTyepay ou * AIOUTPORIY SUTAVS-19}V A, UC oul @ FO AVMITY IY} UL UOTONIYsqQ Ue Jo Joo IY, * sa.tddng 10z@A\ JO UOTyNqII4SIG 944 UO SOJON ayarouoD YIM Surpting jo mays{g ,uvseystvg, oy} uO soursuq AIITIOD 03 potjdde se rey uorsuvdxq jo osq ouy, f S1OJO]T pue somvudg yuerimg snonuryu0p sy * ulor ‘UOSTLO,y Y Aa ‘UBsLOT ; “AA "YL ‘ATOOTT "1 1H “tonen ‘EH 'd ‘smouieyy : ‘CH ‘Urey " *W'f “aren UMA “199.11 AA ORT + ry ry ‘Aassvoeyy . * “ae ‘saver . “W ‘HH ‘souls E ‘gd “¥ ‘somyoyy * MH Gqteq7 * umenTTM ‘fey mould A ‘a ‘JT “ganooreyy * cunt “op ‘urdyr9 . ‘Vv wal ‘soqi0j, * ‘Wf ‘uosuvag . "7 if ‘OMT ‘soy, ‘uosuvound - -ugor ‘aesnog * a0lIneyy ‘aooved "M “T ‘OAvLy od 1895, REPORT 70 See = = = ss S681 F681 g681 “ “i F681 S681 ‘Ts “ee F68T “ cc“ ae S681 peqsty “ang €F9 961 FI L9F oO ag 6 nN &6 L9 asd “ec “cc ‘IITA ce “ TUIKX TITA ‘TWIXX F6-S68 1104 4ivgq 10 auIn[oA ‘qsuy “pay “SUDLT, . . . “ . . . “ . . . ‘ec . . . oc * ‘SUDLT, . “ 7 ""98Uuy "pag ‘SUDL, ; : * SUWDLT “"WSUT “Pay ‘SUDLT : : * “SUDA, . “ “ : ‘Ul Pag sunLy, *SUOLT, ‘204q pun 2Loday WOIBOITAN JO OGL, ’ * -qsuy ‘Sug ‘N “ “c oe “ ‘Bug “UN “4sUy “pag “ce iT . te “ * "90g *[oa!) "ToURTY . . se “ : * 4suy “Sug 'N ‘SUM “ULL “SUL “pag “gSUT FUND "PI J49489 49 ‘sug “UN “98UT ‘pad ‘ L-qsuy “sum "No "008 “[TYq Mosse * "909 ‘@ [ood Ary ‘Sug “UNL “ysuy “pag * ‘00g ‘[Oey ‘ours 00S ‘ld "HN 3e?j19d g S * JOYSPM-[VOH UOJN] oq, soulyy Teop ut daep -eyoyQ pure dmep-aitg jo esvyueolsg pue aoUdSaLI OY} SUIJOIJOp IOF 19}s94-sey MVYY oq, sj1odeag omy WaT suOTOOMUOL) Teuep sy puw Leadeiepolegaarnace : speury duwy Agozeg WS] quae OL, 9ja1NU0H UO SoJON, YIOMAOIG puv AIMosey[ UL 4nOIH puUe IVIIOTT JO O3Q VY} UO sojoN s}u9uI -YULQ UIT, SUIMMIOZ UL YIOMTIEG puv ojorou0g JO OS 94} pue WoYONI}sUOH SYIOAIOZVA\L UO SSUIMVI(] SuULIBOULSUT Jo Sutddog guid-ung oy} 10 ‘fydvisorpey Surooursug SOUL] UL sou x0 ‘exoulg ‘durep- IoyZy WoIy ory Jo Sutavg * govuINy IpPTeJeIwyG oy, ssoippy [ZyuepIsarg SSF S}I pue ou0jg o1gdercoyqy JoMog JO WOSss USUI, O119007T u0}0Ur “FIONA * AIOYTON SMITH “39 sy} Jo worydt10seq : ALouIyoORYY ILO y- omevus uo sLeAIO72 M ysipoug, euo0g sjeurg apr wey “SUING pur uopuoTy ay} 0} Surk{dde ApreT -norjied alow ‘sjuamesordmMy Iteyy puv steurg Sourpy ur gsnqg Suidmeq Joy smvereddy Sur (erds-1078\\ UL syuemaAordwy BOTANY [IV] UOLIaWy oy, . . . . . . . . . . . . . . ‘O “mM “pooM ‘sy ydasor ‘ost "HEM “19T90T AL * "q TOUOYT ‘STIOA . . ‘Vv ‘A919. * THRITITAA ‘S99 AV . aE “7 ‘OUIVMYT, : * UOUNTY ‘av, * “¥ ‘OD ‘Spreyeyeig : “TIAA ‘taouedy * punupy ‘osiedg * “‘xopy ‘suomaig * as10axy ‘re]Nodg G "dM ‘siodvg s ‘V7 ‘pe “Ieurg . . “MA “91BS "WRITE “ures * — g510axy ‘ayoory Ayaro0g JO SALT, Popelaaiqq vy sade Jo oJ, *(panwequod) AONTIOG IVOINVHOSW—'Y wo2vI9' IoyNyY Jo ouvN CORRESPONDING SOCIETIES. “ “ F681 S681 F681 S68T F681 ot ‘TI ‘TL “9d “TX F6-E68 1104 £7 €6-Z68T €6-G68 1107 F6-€68 1104 €6-G68T ‘Til “ €6-G68T “AX “ * SUD, . . P 204g "00k prio quodayy : * aodeaey hioqsrzy * ‘SUDAT, ‘004g puv .Lodayy hLogs uy . . . “ce : 3 * ‘SUD, . . . “ hopseyT J . 20 . . . “ce : ‘ * “SUDL 66 . . 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"i "mM UIE” * + mopSutTTUND "UL a ‘S2T09 ‘Vv ‘prerind * 7, ‘aay ‘uepny ‘190 1OAOUHINY—' FT W09aG) 1895. REPORT “ce 17 U0} “BIA pue ‘yy StqpnoyIry ‘sorjunq 07 sprva -JION WOIsusyXY ITY} 0} WOTILlAI UT ‘MAeYyAN(T ZEl ° s ‘ pare PUP se ON. 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REPORT 74 S68T “ “e F681 6st F681 S68T “cc ‘“ “ “ 681 oe 6st Fo8T 681 F68T peqst] “qn Se eee eee ——————e—e————eEeEEEEeeeE 96 LEE ‘19 ‘SIS {86 896 £0F one S68T 107 FST 10: FG8T 100 §6-Z68T POST 10 “AI ‘Il yt TAXX TI F68T 107 “THTA €6-G68T ‘TIA €6-G68T S681 107 Til 6 ON 'T T ‘ON I S68T IOW F681 107 4avgq 10 euIn[oOA . “ce “ * — QSUYDINIDAT PT, hsopsuy qLodaey * “SUDLT, *"006q PUD 'SUDALT, qLodary * ‘SUD BYDINION OUD, * g8UDLNIDAT LISS : hLogsruyy : : * SUDLT . . “ * gSyVENqON 2UT, . . “ce . . . “ce ' “SUD T h.ojsrzy | SYDINION OT, “a “ “ec “ * UOIUQ ‘JEN ‘SHIOX QUID ‘JN “YsHOrAIog * "008 ‘ld “S410. ‘003 “H ‘N Mossepy "OY “N ‘00g ‘SUyI9g 008 “Gory “HUN “HN * "00g "JBN HIprey ‘009 ‘VW ‘H ‘N ‘2U0q * UOlUA "IVN ‘S¥IO : * "9 "WW xassoy QuID “FEN “YsxorM tog * 909 "HT ‘N 8110 quiO “FEN "SPOT | * UOIUQ “FEN ‘SyY1OX 0G “Yd “WT 103s0010T ‘OH TIBA “A9S 29 “TBO * UOIU) ‘F@N ‘SHIOX woryworTqnd JO OL Ayo100g JO FTL poyeraciqqy + squelg eITysupooury fo onsopeyvy [VOD V {" erepyjorjsdawy WOIF SOJON TBOTURIOT j ; * — goy,Od & Jo VIOTH OL UO UOJMIN FO spULT MoovlIeUINn,T OF Woov[nounuey "T yvg : Ayoro -o9 jeorydosopiyg atysyIoX ey} jo wnUEq “19H OY} UL SyULT YsHMG oy} Jo ansoreie9 uorjyeja50A wodn syoaym [e1ouey S}I WIM “GEST IaX oY} SulIMp Joy} ayy uodn syremey pue sajoN [eoLsopo1094o]V E68 JO SUOISINOX| IewUIMg UO SeyoN &6-Z68T “WOT}O9g Teojdoosoxr0T HW pue jeoruvjog oy} jo yrodaxy * — owauag Jo saroadg [nJIQnoq ¥B UO 940N soTe@A\ WyNog jo We8YO4DAT on} jo yunoooy uB SpIVMO} WOTINGIIZWOD, 3 * 18Un JT snoLinyg euog episury jnoqe sopquieyy [Bolueyog : : ‘ * —- OSS UL OOLT, YRO VL SJULT I OILYSHOAMIa_ Joey IulOs Jo 4svT syong pur ‘spog ‘s}1ay{ Wory satoadg Jo 4sVT 3 qT ‘gozoqyooA OY} UO SOION JOYIAN,T : * ‘o3p QILYSYILY[IG UT sasoyy + JeoISOIYSV Jv IOATY 949 apisoq YO oy, 668T 0} SSSI ‘ws[y Ioyemysorg : Aydvrsorqig ; TIOAIOSOY enoysdoay ay} JO VIOT A II, e C : * pun * sJIOMIOppel_ UO pIOA\ VW €681-() LEST ‘eO],T OITYSVOURT YJION OY} JO SyuoNgTysuOH oq, . . . . . . VW Any ‘31900 -vaq - OYNIpOOM “ “6 ‘EH 'O ‘PpooM ULBITTIM “POO M ‘fH ‘aosunyiiM soup ‘1099 MA ‘dW Id ‘OVO poe ee ‘LO Id TNeqseA ‘Hy ‘ousvoy, “LH ‘371ddog ‘¢d ‘f¢ ‘emoysueyg WIRITIM ‘Aeys soumvp ‘stapuneyg a“ “ce SSI ‘Tssny ‘dM Snqooy "VY OL ‘Aoy ‘u0}Serg “ce “ce | “om Ssdrtd rzoqsyy ‘A}900 | | jaded Jo op1y, *(panuyuos) XNYLOG—‘y wor0ag) IOyyNY JO eweNy ON UNDERGROUND TEMPERATURE. 75 Underground Temperature — Twenty-first Report of the Commuttee, consisting of Professor J. D, EVERETT (Chairman and Secretary), Lorp Ketvin, Mr. G. J. Symons, Sir A. GEIKIE, Mr. J. GLAISHER, Professor E. Hunu, Professor J. Prestwicu, Dr. C. Le NEvE- Foster, Professor A. S. HERSCHEL, Professor G. A. LEBouR, Mr. A. B. Wynne, Mr. W. Gattoway, Mr. JosEpH DICKINSON, Mr. G. F. Deacon, Mr. E. WETHERED, Mr. A. STRAHAN, and Professor Micuie Smitu. (Drawn up by Professor EVERETT.) INFORMATION as to underground temperature in the southern hemisphere has hitherto been very scanty. Importance therefore attaches to observa- tions which have recently been taken in a deep bore in New South Wales by T. W. Edgeworth David, Professor of Geology in Sydney University, and E. F. Pittman, Government Geologist. The following account is derived from a paper by these gentlemen to the Royal Society of N.S.W., read December 6, 1893, supplemented by letters from Professor David to the Secretary of the Committee. The bore is 2,929 ft. deep, and is the second of two which have been sunk at Cremorne on the shores of Port Jackson. _ A protected maximum thermometer had been furnished by the sec- “retary to Professor David when he went out to Sydney in 1882 ; but it ‘had passed through several hands, and was not forthcoming when the opportunity for observation occurred. Professor David had accordingly to avail himself of such instruments as were accessible, and he borrowed four maximum thermometers, including two inverted Negretti’s belonging to Mr. H. C. Russell, the Government Astronomer, which had Kew certi- ficates. They were similar in pattern to those adopted by the Committee, except that there was no outer glass-case. In place of this, ‘a strong piece of wrought iron water-pipe, about two feet three inches in length,’ wasemployed. ‘A cap-piece was sweated on to the lower end of this tube, the threads of the screw in the cap-piece and pipe being filled with molten solder, and the cap:piece being screwed on while the solder was still molten.’ ‘The lower end of the pipe was then filled to a depth of about wo inches with prass turnings. The thermometers were next carefully lowered into the tube.’ They had their bulbs uppermost, as usual. ‘ Brass turnings were then packed around them in order that the heat might be conducted rapidly to their bulbs from the water in the bore. Strings were fastened to the bulbs to facilitate the withdrawal of the thermo- eters from the tube after the experiment of taking the temperature had een completed. The ends of these strings were carried close up to the p of the pipe, the brass turnings being packed around them like tamping ound a fuse in a shot-hole. A few cardboard wads and a layer of loose per two inches in thickness were inserted in the upper portion of the tube, to prevent the conduction downwards of the artificial heat, which would otherwise travel down to the thermometers from the upper end of he tube when it was dipped in the molten solder, previous to the upper “€ap-piece being sweated on. A ring-bolt for attaching the lowering cord was screwed into the upper cap-piece, with molten solder sweated into it ; and the whole cap-piece was then screwed and sweated on to the upper end of the tube in the same manner as the lower cap-piece.’ 76 REPORT—1895. The first experiment was a failure, the thermometers, though left for about an hour near the bottom of the bore, indicating about the same temperature that they had before lowering. This failure is attributed either to the non-conducting action of a few thicknesses of soft paper in which the bulbs were wrapped, or to the mercury which had left the bulbs having returned to them again while the tube was being conveyed from the bore to the plumber’s shop, where the cap-piece was removed. In the second experiment ‘no paper was wrapped round the bulbs, but the brass dust was continuous from the bulbs to the sides of the iron pipe. At the depth of 2,733 ft. an obstruction was encountered which prevented the tube from going lower, and which also caused the suspend- ing wire to kink and break. After an immersion of about twenty-seven hours, the wire was successfully grappled, and the tube brought to the sur- face. ‘The upper cap-piece was then rapidly heated in a chafing dish of charcoal made of an old nail-can, with a hole cut out of the bottom just sufficiently large to admit of the upper end of the tube being passed up it, and oxygen gas from a compressed cylinder was blown through a Fletcher’s blowpipe on to the charcoal, so that in less than half a minute the solder in the threads of the cap-piece was melted ; the lower portion of the tube containing the thermometers being meanwhile wrapped in wet cloths to prevent the heat travelling downwards. The cap-piece having been unscrewed and the thermometers withdrawn, the highest temperature registered was found to be 97° F. ‘ Not a drop of water had found its way into the tube.’ On the following day the experiment was repeated, no wire being used for lowering, but only tarred rope; and sheet lead was wrapped round the tube to increase the weight. The tube was left down for one hour, and the maximum temperature registered was 96° F. The difference of 1° below the former observation is what might fairly be expected from the stirring of the water and the thermal capacity of the sheet lead which, with the tube, weighed 30 1b, The first result, 97° F., is therefore adopted as the true temperature at the depth of 2,733 ft. The mean sur- face temperature, as determined by Mr. H. C. Russell, is 63° F., giving an increase of 34° in 2,733 ft., which is at the rate of 1° F. for 80 ft. As regards the possibility of disturbance of temperature by convection, Professor David mentions in a letter to the Secretary that the bore was only four inches in diameter. He also says, ‘ You understand, of course, that we can do nothing in the way of taking temperatures in a diamond- drill bore until the bore is quite completed, owing to the chilling of the rock at the sides of the borehole by the cold water which is being con- stantly forced to circulate under pressure through the bore.’ The temperature of the water of Port Jackson at the greatest depths near Cremorne, varying from 45 to 63 ft., was found (on December 6, 1893) to be uniform at 68° F. As this temperature is higher than that of the ground at the same level, no cooling effect can be attributed to the water. The slow rate of 1° F. per 80 ft., deduced from the observations, _ would therefore appear to be a good approximation to the truth. It is expected that shafts will shortly be sunk at Cremorne, and will afford opportunity for the systematic observation of rock temperatures from the surface to a depth of nearly 3,000 ft. ‘The first 1,000 ft. will be in horizontally bedded sandstone, and the remainder chiefly in clay shales, with interstratified sandstones and conglomerates.’ The observa- tions will be taken by Professor David and Mr. Pittman, with the— = - ¢ : . Fe - 8 a ae Le . 4 _ 7 sd — . " 1 ~ - x ey ~ ii ’ ty . - ae ee ? Pied sa a —e 7” - 1 SY \ . ‘ \ . , y wy. - iunal ‘ ‘ . rape: \ f - a , _ _ ‘ { ; . < \ _ ;' } an p. ~ ne = He G x ' ‘ , = = 4 = » re * , ; ' - oe = a =f e —— es * *€ v4 ae * s wD 7 7 - \ a = + enc t i} “Te iii . : -— , = * - i a sai Tx ee i it, F = ~ ¥ ‘ ie j : . * ‘ te . ‘ . ~ * \ ’ : “ = - Tse *% © <--> =e { 7 Pe -_ 7 =“ 65% Report Brit. Assoc, 1595, wrcnes Letterpress Mi The heayy lines show standart andi tinating dimensions | “Bead oF Book _b cenriarrnes ale eas 7 Cer ace! =: => —* Sraritaeraa = Tlustrating the Report on the Uniformity of Size of Pages of Scientific Socteties' Publications, — es Committee's slow-action shafts. 3 The Committee desi valuable member, Mr. P The Uniformity of Size Report of tha Com’ (Ohairman), Mr. | GLazeBRook, Dr. | (Secretary). ‘Tur importance of ad pages of scientific publ collected reprints of p: deayoured to have the more than passing in| cases, be handed down subject, and it is, there iy the omission of on Yeing bound up with t he Committee hay their attention chiefly mathematical and phy recommend as standa guided by the consid extent attained, and t accomplished without ‘principal journals, anc Tn deciding wheth size of the margin is ‘Thus the ‘ Bulletin of 4 centimetre wider a British Association,’ « till have exactly the “at the top and botts Physical Rocicty’ an “Magazine” although “arises the necessity 0} pied hy the letterpres tance from the ou stance from the to n of the last lir the margin: 1 in at the top ar (6=d). y adopting a m and a Banceh rrr. £ ON UNDERGROUND TEMPERATURE, vr ~ Gommittee’s slow-action thermometers, in holes bored in the sides of the shafts. The Committee desire to express their regret at the loss of their valuable member, Mr. Pengelly. The Uniformity of Size of Pages of Scientific Societies’ Publications.— Report of the Committee, consisting of Professor 8. P. THompson (Chairman), Mr. G. I. Bryan, Dr. C. V. Burton, Mr. R. T. GLAZEBROOK, Dr. G. JOHNSTONE STONEY, and Mr. J. SWINBURNE (Secretary). rs oe bia a re eee wee. a . [PLATE I] ‘Tue importance of adopting one or two uniform standard sizes for the ‘pages of scientific publications will be evident to all specialists who have collected reprints of papers on any branch of science, and who have en- _deavoured to have them bound into volumes. Such collections are of more than passing interest, and they might, with advantage in many cases, be handed down to posterity as records of work in any particular subject, and it is, therefore, of importance that they should not be spoiled by the omission of one or two papers whose size precludes them from being bound up with the rest. The Committee have thought it advisable in their first year to confine their attention chiefly to reporting on the size of the pages of existing mathematical and physical publications, and to deciding on what sizes to recommend as standards. In the latter matter they have been largely guided by the consideration that uniformity has been already to some extent attained, and this report will show that the desired results can be accomplished without making any radical changes in the sizes of the principal journals, and, indeed, without altering most of them at all. In deciding whether two papers can or cannot be bound together, the size of the margin is quite as important a factor as the size of “the paper. ‘Thus the ‘Bulletin of the New York Mathematical Society’ is more than a centimetre wider and two centimetres higher than the ‘ Report of the British Association,’ and yet if it were cut down to the same size it would still have exactly the same margin at the sides, and 6 mm. more margin at the top and bottom of the pages. Again, the ‘Proceedings of the Physical Society’ are printed with the same type as the ‘ Philosophical Magazine,’ although one is medium and the other demy octavo. Hence arises the necessity of taking an internal measurement of the space occu- pied by the letterpress, as well as an external measurement of the size of the paper page. __ This may be estimated as in fig. 1, which represents the opened pages of a book. a, b denote the width and depth of a paper page, ¢ is the distance from the outside edge of the letterpress to the back, and d is the tance from the top of the running headline or number of the page to the bottom of the last line of letterpress, exclusive of the ‘ signature.’ Hence a—cis the margin at the side of the page, and 6—d is the sum of the en at the top and bottom, so that if these are equal each is equal + (b—d). “By adopting a minimum limit for the size of the pages (measured by a, b), and a somewhat smaller maximum limit for the internal measure- U al! 78 REpoRT-—1894, ments c, d, we shall secure that all papers can be bound together without cutting the margin down below a certain limit. In fixing the limits we must allow for a little of the margin being cut away in binding. Octavo Pusiications.—In the octavo sizes, the diagram, Plate I., shows an overwhelming preponderance of medium and demy octavo, the demy size being not only in the majority in point of number, but also in- cluding many of the'most impor- tant publications. The royal octavo size recently proposed by the Royal Society is only repre- sented by about two journals, of which the ‘Proceedings of the Royal Artillery Institution’ is one. On the other hand, the space occupied by the letterpress, as shown by the measurements c, d, is no greater in several of the medium size than in the majority of demy octavo, and there would, therefore, be no difficulty in cutting these down in binding. The Com- mittee, therefore, recommend the following sizes :— Standard Octavo Size.—-Paper demy, the pages measuring 14cm. x 22cm., or, when uncut, 53 in. x 83 in. The width c, measured from the stitching to the edge of the printed matter to be 12 cm., or 45 in., and the height, d, of the printed portion including the running headline, to be 18 cm.,or 7 in. Limit of Octavo Size.—The paper page not to be less than 14 cm. x 21°5 em., or 54 in. x 8} in., and the letterpress not to exceed the measurements c=12'5 em., or 42 in., d=18°5 cm., or 74 in. Reprints and unbound numbers of journals to be issued with their edges uncut, or cut not more than 0:25 cm.,.or }in., all round. The use of standard as well as limiting sizes will easily be understood. Where publications fall within the limiting size there is little or no need for the size of the pages to be altered at present ; but when any alteration is made in the size, or in the case of new journals or papers printed by their authors for private circulation, it would be desirable to conform exactly to the standard size, which would ultimately become general. Taking, first, the limiting sizes, and allowing for 0°25 em., or } in., being cut off the margins in binding into volumes, the pages of these would measure 13°5 cm. x 21 cm., or 53 in. x 81 in., and this would allow of a margin of not less than 1 cm., or 3 in., all round, which is quite enough. Tf the standard sizes should become generally adopted the bound and cut volumes would measure the same, and the margin would be 2 em., or + in., at the sides, and 1°6 cm., or 2 in., at the top and bottom. In the diagram it will be seen that there are journals which do not fall within the limiting dimensions. Where @ and 6 fall short of the limits this could be remedied in some cases by leaving the edges uncut. Where c is too large, the letterpress could be brought a little nearer the stitching in imposing for press ; where d is too great, the pages could be shortened by a line or two. ; : Quarto PusiicaTions.—The corresponding dimensions for the prin- cipal quarto publications are given in the same diagram. Here, again, we find medium quarto (24cm. x 30cm., or 95 in. x 12in.) and demy quarto Fig. 1. ; UNIFORMITY OF SIZE OF PAGES OF SOCIETIES’ PUBLICATIONS. 79 (22 cm. x 28°5 cm., or 8? in. x 11} in.) almost universal, but the pre- ponderating sizes approach most nearly to demy, and on account of the large margins of many journals this is the most convenient size of the two, besides making the volumes less unwieldy. The Committee, there- fore, recommend, in cases where it is desired to retain the quarto size, the following measurements :— Standard Quarto Size.—Paper demy, the pages measuring, when uncut, 22 cm. x 28°5 em., or 8? in. wide x11} in. high. Reprints and unbound numbers of this size to be uncut, or cut 0°25 cm., or }in. Measurements of letterpress to be c=18°5 cm., or 74 in., d=21°5 cm., or 84 in. Limits of Quarto Size—Paper pages not to measure less than 21:5 cm., or 83 in., wide x 28 cm., or 11 in., high. Letterpress not to exceed the measurements c=19 cm., or 7} in., d2=23 cm., or 9 in. The same remarks as to the advantage of standard and limiting sizes apply as in the case of the octavo. Allowing for 0-25 em., or } in., being cut offin binding, the limiting sizes will allow of a margin of not less than 2 em., or 4 in,, all round, while the standard size will give a margin of 3-25 em., or 1} in., at the sides, and 2°5 cm., or 1 in., at the top and bottom. Puates often get sadly mutilated when different papers are bound together, and sometimes this even happens when a volume of any periodi- calis bound up. Where they are folded over they not infrequently get cut in two by the guillotine. To avoid this the Committee recommend that the dimensions of the illustrations should never exceed 13 cm. x 20 cm., or 5} in. x 74 in., for octavo plates, and 21 cm. x 25 em., or 8} in. x10 in., for quarto, the width being measured from the back of the book. Where plates have to be folded, the fold should be 12°5 cm., or 5 in., from the stitching in octavo, and 20-5 em., or 8} in., in quarto papers. Any folding plate should, when referred to elsewhere than in the opposite page of letterpress, have a blank space equal to the breadth of the paper page at the left hand, so that when open it can be referred to without closing the portion of the book being read that refers to it. This should be carried out even when the diagram or plate would not otherwise have to be folded, in order to reduce the trouble of reference. Each article should begin a page. If possible it should begin a right- hand page. It is then possible to bind up any article with others on the Same subject without having also to bind up the last half page of another paper. This difficulty can be overcome to some extent by splitting the paper. The pages of some of the journals abstracted in the ‘ Proceedings of the Physical Society’ are split, one side being sent to each abstractor. Comparison of Magnetic Standards.—Interim Report of the Commit- tee, consisting of Professor A. W. Ricker (Chairman), Mr. W. Watson (Secretary), Professor A. ScHuUSTER, and Professor H. H. TURNER, appointed to confer with the Astronomer Royal and the Superintendents of other Observatories with reference to the Com- parison of Magnetic Standards. with a view of carrying out such Comparison. Proressor Ricker and Mr. Watson have carefully compared three Kew- pattern magnetometers in order to investigate the causes of the discre- pancies between the measurements of declination made with them. They 80 REPORT—1895. find that if the greatest care be taken in the manufacture of the wooden box and the metallic adjuncts which are close to the magnet the discre- pancies disappear. In other words, the cause of the difficulty, in these three instruments at all events, is, not the metal base, but the much smaller masses of metal which are nearer to the magnet. The three magnetometers are now in good accord. A week has been spent at each of four observatories for the purpose of comparing one of these magnetometers and a dip-circle with the obser- vatory instruments. Professor Riicker made the observations at Kew and Falmouth ; Mr. Watson, those at Stonyhurst and Valentia. The greater part of the work which the Committee undertook has thus been accomplished. It is still necessary to compare the instruments again with the instru- ments at Kew to ascertain that they are unaltered by transfer from one place to another; and as a new magnet-house is about to be built at Greenwich, it has been thought better to postpone the comparisons at that observatory until the house is ready for use. The reductions of the observations which have been made are not yet finished. A full report will be made when the work is completed. The Committee therefore ask to be reappointed, but no further grant is required. The Application of Photography to the Elucidation of Meteorological Phenomena.—Fifth Report of the Commnuttee, consisting of Mr. G. J. Symons (Ohairmaw), Professor R. Metpoia, Mr. J. Hopkinson, and Mr. A. W. CLAYDEN (Secretary). (Drawn wp by the Secretary.) In the report which the Committee presented last year, it was proposed that an agreement should be entered into with the London and South- Western Railway Company for the use of a site on their land, in order to carry out some measurements of cloud altitudes by means of photography. This has been done. The cameras have been placed in position, and almost the whole time at the disposal of the secretary for such purposes has been spent in perfecting the electrical connection for releasing the two shutters simultaneously. Considerable trouble has been experienced in doing this. The apparatus, which worked admirably over a short dis- tance, proved unreliable over the greater distance (200 yards) at present adopted. The agreement with the railway company provides that the connecting wire shall be removed when not in actual use, thereby necessitating as light a wire as can be made to suffice, which of course implies a considerable resistance. The result is that a more sensitive electric detent is required for the shutters, especially as it seems not unlikely that the distance may have to be increased by another 100 yards when the measurement of the highest varieties of cloud is attempted. This is still engaging the attention of the secretary to the Committee. Some observations have been made, but although they confirm the belief that the method will prove valuable they have not yet been reduced to actual measurements. It should be remembered that the method is only applicable to those varieties of cloud which are visible at the same time as the sun, and that the opportunities of making observations cannot 65% Report Brit Yokohana On Fig, 1—Line from two «clits Tho gap is an interval of one hour. 30am TKS com On Rook | | Fig, 2.—Lino from broad slits, shows the unfelt earthquakes on Feb. 3 ‘An earthquake which was felt ought to be at A. 6pm 6am Feb LIE 6am Fa7e Ipn Fig. 8.—Daily curves on surfaco. Instrument A Tokzo. jz ok Ip 6pm Feb Pp. ince pe Oe PEM? OF 6pm. mr 6am. Feb. 5H Fia, 4.—Daily curyes underground (E) correspond to fig. 8 Toko ame 6am, Sen26 reg, 6pm Jan27 Gam Fo, 6—Underground tremors—dally curves—wandering of pendulam jarfaco tremors, dying ont and recommencing, Tekvo A May 2p e i mi f Ce Team ae oe a Tekuo. Fig. 7.—Curvo and tromors produced et the time a well was ompticd. *.* All gaps at or ncar noon represent an interval of ona huur. EXAMPLES OF RECORDS PROM HORIZONTAL PENDULUMS, Ilustrating the Fourteonth Report of the Committee on the Bartlquake and Voleanie Phenomena of Japan. — ON THE ELUCI coineide with the pos course of a short time have been finished Committee, ti that, they may carry ask for a further grant Solar Radiation. —E Sir G. C. Stoke JOHNSTONE STONE Mr, 0. Curee, M H. McLeo ding tha Dire Tie Committee regret Sxperiments have been the last’ meeting of the ntinue the experime the tnexpended balanc Tiveitigation of the Fourteenth Repor Lord KEtyiy, Pri ). Borroytey, F 0. G. Kyorr, ecretary). (Dri L The Gray-aitne UL Oe (0) The Diagriors (@) Tie Morcments i ieee? (6) Earthquakes W) The Ubserrations ) Senniticencss of t) Rents G) Daity Tring ( Petmet’ Seva J Records sbiained vs IT in fist of this form « jafeite of the British A wumment. at the Centr Sm indebted to M, fr L Heap olowing table ON THE ELUCIDATION OF METEOROLOGICAL PHENOMENA. 81 coincide with the possibility of making them, very frequently in the course of a short time such as that which has elapsed since the cameras _have been finished. Your Committee, therefore, ask to be reappointed for another year, so that they may carry out the work in hand, and with that object in view ask for a further grant of 15/. Solar Radiation.—LHleventh Report of the Committee, consisting of Sir G. C. Stokes (Chairman), Professor A. ScHuster, Mr. G. JOHNSTONE STONEY, Sir H. E. Roscoe, Captain W. DE W. ABNEY, Mr. C. Cures, Mr. G. J. Symons, Mr. W. E. WILson, and Pro- fessor H. McLEop, appointed to consider the best Methods of Recording the Direct Intensity of Solar Radiation. THE Committee regret to have to report that for various reasons no experiments have been made with the Balfour Stewart actinometer since the last meeting of the Association. As Mr. Wilson has undertaken to continue the experiments, the Committee ask for reappointment and for ‘the unexpended balance of the previousie grant. Investigation of the Earthquake and Volcanic Phenomena of Japan. Fourteenth Report of the Commvittee, consisting of the Rt. Hon. Lord Ketvin, Pres. 2.S., Professor W. G. Apams, F.R.S., Mr. J. T. Borromuey, F.R.S., Professor A. H. GREEN, I’.R.S., Professor C. G. Kwotr, F.R.S.L., and Professor JoHn MILNE, F.B.S. (Secretary). (Drawn up by the Secretary.) [PLATES ILIV.) CONTENTS. I. The Gray-Milne Seismograph . 81 (j) The Wandering of the Pen- Il. Observations with Horizontal dulums . ; “eco Pendulums . } 84 (k) Movements of Water in @ (a) The Instruments D 85 Well . 104 (b) Observations at Kamakura 88 (2) An Exper iment on Ev apo- (ce) The Diagrams . uO ration . . 106 (d) The Movements of the Pen- (m) Effects pr oduced are ec mpty- dulums . : : 90 inga Well . LOW (e) Earthquakes. 91 (n) Earthquakes. : . 108 (f) The Observations in Tokio. 94 (0) Tremors. - . 109 (g) Sensitiveness of the Instru- (p) Observations at Yokohama ments . 3 ; >. 94 and Kanagana . ‘ . 109 (h) Daily Tilting : : 95 (q) Conclusions ‘ 110: (@) E£etract from Journal if Ill. The Tokio Earthquakes of June Records obtained in 1894 . 96 20, 1894 : J ; oy Se IV. Miscellaneous . : : 2 te I. Toe Gray-MILne SEISMOGRAPH. Tux first of this form of seismograph, constructed in 1883, partly at the expense of the British Association, still continues to be used as the standard instrument at the Central Observatory in Tokio. I am indebted to Mr. K. Kobayashi, the Director of the Observatory ae following table of its records :— G 82 REPORT—1895. Catalogue of Earthquakes recorded at the Central Meteorological Observatory in Tokio between April 19, 1893, and May 17, 1894 Maximum Period and Amplitude of Amplitude of Maximum Period and = i f Horizontal Vertical | Nature No. | Month | Day Time Duration Direction Motion Motion G) Shock secs. | mm, | secs. | mm, 1893. H. M.S. M. S. 1322 Iv, 19 | 11 25 25 p.m. = = slight i = 1,323 * 21 7 10 57 P.M. 70 _ 2 2 — — | quick 1,324 ie 26 10 0 46 A.M. — — — — _ — -- 1,325 a 30 11 32 19 a.m. — E-W. = we = = = 1,326 Wu 1 2 5 6AM. _ _- — — —- — — 1,327 a 11 4 52 33 A.M. — E.-W. — — - — | quick 1,328 o a4 8 57 14 A.M. —_ — _— — —_ — —_ 1,329 ‘ 17 9 56 44 A.M. _— _ _- — — — -- 1,330 ts 18 3 32 38 P.M. — —_ — = — — — 1,331 a 21 9 10 40 A.M. — — — = — — — 1,332 as 24 7 0 32 am. — — — = —_ — — 1,333 a 8 58 57 P.M. 1 30 E.-W. — — —_— — slow 1,334 3 28 7 24 55 P.M. — = = Be — _ = 1,335 Sy 30 010 2AM. — — — — —_ -- — 1,335} VI. 4 227° 17 a.m. 0 3 E.-W. — — — — slow 1,337 oy By 9 7 38 a.m. — — — z= — — — 1,338 a rH 11 2 31aA™M. 01 N.N.W.-S.5.E Or4 06 _— _ quick 1,339 * 9 2 53 27 a.M. — — — — = —— 1,340 7 FF 4 48 41 pM. — =: 33 = so == Ben 1,341 os 10 8 6 44 A.M. _ — _ _— —_ _— _ 1,342 a 12 4 8 0AM. 1 50 W.N.W.-E.S.E. 05] 08 _— = qnick 1,343 es 13 7 44 16 P.M. 3 50 N.-S. 1:2 50 = — slow 1,344 “5 18 7 19 10 P.M. + _— — = _ _ 1,345 4 21 0 35 21 a.m. _ — — a= =~ — — 1,346} VII. 5 9 52 42 P.M. — — — — ue = — 1,347 “5 6 8 9 52 PM. _ — — = hs ay == 1,348 s 18 545 6 AM. a — = = = — a 1,349 os 19 8 38 23 P.M. 2 30 E.-W. 0-9 4 — _— slow 1,350] VILL. 2 6 25 54 A.M. — —_— — — — — — 1,351 ; 20 0 28 27 P.M. 0 4 N.N.W.-S.S.E. 0°5 36 0°3 1 quick 1,352 . 22 9 37 55 A.M. 2 30 _— V1 0-7 _ — slow 1,353 IX. 4 5 7 30 4.M. 2 30 N.N.E.-S.S.W. 1-0 07 — = ” 1,354 10 5 0 22 a.m. — — — = — — — 1,355 ~ 15 9 38 47 A.M. — — = aos ee ax =. 1,356 ¥ 5 6 28 22 p.m. = = a a4 —_ = 1,357 IX. 17 9 56 41 AM. — — — = es == == 1,358 “4 - 1 39 31 P.M. — — — = eS = = 1,359 >. 6 Tou), But — =. = = = = =s 1,360 os 10 8 27 21 pM. — — — = = = = 1,361 BY 19 0 57 17 AM. os — = fa a — = 1,362 XI, 13 10 52 55 p.m. — oo = = = = = 1,363 15 9 41 23 4.M. L 4 E.-W. 0-9 03 = — | quick 1,364 y 28 1 15 29 a.m. = — = ae = = — 1,365{ XII 29 11 33 57 a.m. L's N.E-S.W. 05 09 — — | quick 1894. 1,366 iT. 4 1 37 20 P.M. 0 55 E.-W. Os 05 slight quick 1,367 “ 10 6 56 4PM — — — — —_— — — 1,368 “a Ke 6 46 23 P.M 3 15 E.-W. _ —_— — —_ slow | 1,369 s 12 2 50 33 a.m — — = = a = se ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN, CATALOGUE OF EARTHQUAKES No. | Month | Day Time | Duration | H. M. S. M.S 1,370 im 16 5 29 40 A.M. — 1,371 * 18 3 45 21 P.M. 0 48 1,372 ce 25 10 48 11 A.M. _— 1,373 EL 2 7 114 PM. — 1,374 .. 16 2 0 53 P.M. —_— 1,375 ry 18 11 36 40 P.M. —_ 1,376 ‘ 20 829 3 A.M. 4 20 1,377 rc 24 9 33 54 P.M. 0 55 1,378 on 25 417 42 a.M. 3 40 1,379 _ 27 053 OM. 2 21 i: en » | 10 51 39 pM. = 1,381} IIT. 3 10 20 9 P.M. ain) 1,382} 4, 5 | 11 0 38a.x. | 0 1383) 45 6 | 8 29 30a.m. | 1,384 a 10 8 38 53 P.M. a 1,385 Pe 12 4 8 LPM. — 1,386 rs 13 7 28 38 P.M. — 1,387 a 14 8 59 57 A.M. — 1,388 ” ” 6 18 11 yo, —_ 1,389 ” 16 2 54 18 A.M. — 1,390 ER 20 | 11 33 53 P.M. = 1,391 ” 21 3 9 10 PM. | — 1,392 a 22 229 9PM. — 1,393 ” ” 2 38 42 P.M. = 1,394 2” » wt 39-PM. — 1,395| ., 3 7 27 49 pM. 0 10 1,396 i 93 7 48 53 pM. eo) 1,397 ” ” 10 6 16 P.M. — 1,398 ” ” 11 58 45 p.m. —_— 1,399 ri 23 0 45 54 A.M. _— 1400! ,, pe) 7 3i5'39 ae | | 1,401}, 26 2 36 12 a.m. = 1,402 ” ” 412 12 a.m. =* 1,403 = 29 6 0 27 P.M. — 1,404| IV. 1 11 29 38 a.m. ~- 1,405 a 2 56 31 3 aM _ 1,406] ,, 4 8 57 25 P.M. = 1,407 93 7 77 10’ P.M. — 1,408 % 12 10 13 40 p.m. — 1,409 mA 14 2 39 30 A.M. — 1,410 bs 4 3 34 32 A.M. 2 40 1,411 = 15 151 5 a.m, — 1,412 Br 17 3 54 52 PM. — 1,413 3 25 9 21 57 A.M. 218 1,414 AY 28 1 23 49 aM. —_— 1,415| V. 2 11 26 39 P.M. -- 1,416 5 4 | 10 51 55 a.m. _ 1,417 a 6 6 3 22 pM. — 1,418 ‘* 10 411 39 aM. 2 50 1,419 if 16 5 52 45 P.M. —_— 1,420 ” 17 6 129 a.m. _— 9 85 continued. Maximum Maximum Period and | Period and Amplitude of |Amplitude of bots Horizontal Vertical | Nature Direction Motion Motion of Shock i] secs. | mm. secs.| mm. | E-W. 10 04 — —_— slow E-W. — _— — — — rE-W. 16 51 slight slow N.N.W.-S.S.E. | 07 07 = — ee N.-S. ote} 68 — — = E.-W. 14 24 slight quick N.N.E.-S.2.W. | 11 3 | — — slow N.E.-S.W. 07 03 slight 5 liege oe | aces 7 ¥ -- he = ens, ) = == = red — ne ee oe: pe _ 36 53 slight slow N.-S. — _ —_— = P ES.E-W.N.W.| 06 | 1:3 04 | 10 | quick E.-W. 1:2 0°5 — —_ slow N.N.E.-S.S.W. | 0:7 05 — “= 84 REPORT—1895. Remarks. Shock 1,351.—Commenced very gently for about 36 seconds, when a violent shaking, lasting 16 seconds, took place. It then died out. Shock 1,352.—This commenced gently for 32 seconds, after which, for 9 seconds, the motion was strong. Then it died out. Shock 1,366.—Strong motion, lasting 15 seconds, commenced after 9 seconds of pre- liminary motion. Shock 1,368.—Was very slow and gentle. After one minute the horizontal motion was marked for about 13 seconds. During 26 seconds it showed nineteen large waves. Shock 1,376.—At first this was slow, but became stronger after 3 minutes 12 seconds, when for the next 30 seconds it was pronounced. II. OBSERVATIONS wiITH HorizontaL PENDULUMS. In the years 1883, 1884, 1885, 1887, 1888, 1892, and 1893 I embodied in Reports to the Association some account of work which had been carried out in Japan in the investigation of earth tremors or pulsations and earth tilting. The Twelfth Report (1892) describes a pair of extremely light horizontal pendulums the movements of which were recorded on photographic plates or films, and gives some account of the analysis of the resulting records. The observations were continued during the following year, and, as stated in the Thirteenth Report (1893), it was observed that the direction of earth-tilting movement and also of earth- quake movement in the majority of cases coincided with the direction in which strata have been folded to form mountain ranges bordering the Tokio plain. Another observation was that certain earthquakes had been preceded by an abnormal amount of tilting. In consequence of the liberality of the Royal Society of London dur- ing the last year I have been enabled to extend these observations, using six horizontal pendulums, each provided with photographie recording apparatus. The places of observation have been in Tokio, at my house, on a massive stone column, and at a place about 1,000 feet distant in an underground chamber ona concrete bed ; at Kanagawa, in an artificial cave driven in a soft tuff rock at a depth of 50 feet below its junction with 50 feet of over- lying alluvium ; at Yokohama, in a cave driven at the junction of the tuff and alluvium ; and at Kamakura, in a cave in the tuff which at this place is hard and dips at an angle of 80° N.E. All these places lie from Tokio ona §.S.E. line, and are respectively 20, 25, and 38 miles distant from my house. At Kanagawa and at my house there is only one instrument, and the booms of these pendulums point N.W. At the other stations two instruments have been or are now being used, and these are placed at right angles to each other, one pointing N.W., or parallel to the strike of the rocks, and the other N.E., or parallel to the dip. At Kamakura observations were made for two and a half months, when the instruments were brought to Yokohama. At this latter place, owing toa series of accidents, one of which was the collapse of the roof of the cave, up to the present the observations have been extremely few. At Kanagawa, although the cave is wet, the observations have been fairly continuous. In Tokio, where I am able to see the instruments every day, but few inter- ruptions have occurred. The chief part of this report, therefore, refers te Kamakura and Tokio. — sh ae ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 85 (a) The Instruments. Although pendulums made of pieces of aluminium wire and held up with quartz fibres with their mirrors and lenses have given excellent results, the apparatus required good installation and careful manipulation. As these requirements were not obtainable, excepting in Tokio, before commencing observations in the country my first task was to design an instrument of a simple character, not easily put out of order, and which would give continuous records for at least one week. This was done, and as the six instruments which have been made have worked satisfactorily I give the following description of one of them. Fig, 1 The pendulum stand A, fig. 1, with its upright, which is 50 cm. high, is of one piece of cast iron.! ‘The distance between the levelling screws work- ing in brass sockets is 23cm. The back screw tilts the upright and gives the required degree of stability to the pendulum ; one of the lateral screws is used in adjusting and calibrating the pendulum. It carries a pointer moving over a graduated arc. By turning it, for ae one degree, which means raising “this corner of the instrument sky of a millimetre (the 1 The form of the bed-plete is that of a right-angled triangle with the right angle near A. 86 REPORT—1895. serews having a millimetre pitch), the corresponding deflection of the pen- dulum maybe noted. The turning is done by a lever projecting from the head of the screw. The boom of the pendulum is an aluminium tube 4 feet (120 cm.) in length, carrying a sliding weight, W, and a movable point to which the supporting tie can be attached. This tie, which is of thin brass wire, at its upper end terminates with about an inch of untwisted silk. On the inner end of the boom tkere is a quartz cup which bears on a steel needle projecting slightly upwards from the base of the cast-iron stand. The suggestion that the needle should project from the stand rather than from the boom is due to Dr. von Rebeur-Paschwitz. It gets over the difficulty of having anything which may be markedly magnetic in motion ; and secondly, in case of violent disturbance, the relative verticality of the points of support is less liable to alteration. The instrument is adjusted so that the needle bears normally on the centre of the quartz cup, or so that the centre of gravity of the system falls about G. At the outer end of the boom a stiff wire rises vertically upwards. Clamped to this at the required height is a horizontal wire 15 em. long, carryipg a thin zinc plate p, measuring 6 cm. by 10 cm. In the centre of this, and parallel to the length of the boom, there is a slit about 0°5 mm. broad and 2 cm. long. As the boom moves to the right and left, this slit floats over a second slit about 5 em. long in the lid of the box covering the drum which carries the recording paper. These two slits are at right angles to each other, so that the light from a lamp reflected downwards by a plane mirror only reaches the drum as a spot. A. well-defined spot, which means a clear, sharp line on the photo- graphic film, can be obtained without fine adjustment. That is to say, the distance between the film and the slit, or between the stationary and moving slits, may be anything between 1 and 5 mm. _ Projecting an inch or so beyond the moving plate and attached to it is a pointer moving over a scale fixed on the cover of the box containing the clock of the recording drum. This can be inspected and the position of the boom at any time noted by looking through the glass plate at m. The recording drum, on which the photograph-paper is fixed with a spring clamp, as in a recording barometer, is of thin sheet brass 5 cm. wide and 105 cm. in circumference (some are much less). It is turned at the rate of 15 cm. per 24 hours, and a film therefore lasts one week. The clocks, which are an American type intended to run 8 days, have fitted to the slowest moving arbour four wheels, the last of which turns a disc with slots round its edges once a week. The recording drum, which can be dropped into its bearings, carries a large crank. When in position the clock is slid in a groove until one of the slots catches the outer end of the crank arm ; after this the cover is put over the clock and drum, and the whole is pushed on grooves into the end of the case covering the pendulum. Hollow wooden drums, which are easily driven by the clock-work, have a tendency to warp, and this may result in a want of uniformity in the motion. Brass drums in the damp atmosphere of a cave in a month or so tend to rust, and this rust may act upon the photographic film to such an extent as to render it illegible. Up to the present time ordinary kerosene lamps have been used, but OO ————— ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 87 as they require attention at intervals of from 8 to 12 hours they are being replaced by lamps such as are used in magnetic observations burning benzine. Every day from 12 noon to 1 p.m. the lamps are removed and a reading is taken, so that time intervals are marked on the photographs and scale values are obtained. It does not seem necessary that the boom should be made of alumi- nium, as I obtain what appear to be equally satisfactory records with booms of brass oreven wood. The most delicate pendulum I have has a boom made of varnished bamboo with brass fittings. It is about 5 feet in length, and when last rated had a period of 55 seconds. I say last rated because I find that this pendulum, like all others I work with, changes its period, and therefore its sensitiveness, from week to week. I notice that this source of error when computing results is also found in the infinitely better con- structed and better installed apparatus used by Dr. von Rebeur-Paschwitz. When the pendulum has its 55-second period one millimetre deflec- tion on the photographic plate is equivalent to a tilt of 0-08 second of are. With this degree of sensitiveness a 141b. weight placed on the column, which is old and massive, at a distance of 2 feet from the instrument causes a deflection of 0-5 mm. My weight on the floor at the outer end of the boom produces no visible effect. In this condition the pendulum is, however, often too sensitive, as it will, from time to time, wander an inch or so to the right or left of its mean position, and the spot of light fall outside the film. A sensitiveness of 1 mm. motion per 05 are is usually quite sufficient, and I do not think that apparatus like those of Wolf, d’Abbadie, Darwin, or von Rebeur- Paschwitz capable of recording tilting of from 4}, to 3}, of a second could be used on the alluvium of Tokio even when installed on a con- crete bed underground. Such apparatus might, however, be used on the solid rock which crops out round the Tokio plain. An attempt to test the accuracy of one of the horizontal pendulums was made by placing it on an iron plate resting on a plank 18 in. broad, 13 in. thick, which in turn rested on supports near its end 6 feet apart. It was then adjusted, so that trials with the test screw indicated that turns of 10° gave an average deflection of 11-5 mm. Side by side with the pendulum a transit instrument having a good telescope was placed, and this read on a scale fixed ona brick wall at a distance of 720 feet. The supporting plank was then loaded at its middle until the telescope showed a deflection of 14 in. on the scale and the pointer of the pendulum moved 93 mm. From this it seems that the pendulum indicated a tilt of 1 in 562, while the angular tilt of the telescope was 1 in 616. These are the means of a series of experiments, and assuming that the readings through the telescope were correct, then the pendulum indications are about 10 per cent. below their true values. On the other hand, assuming that the readings through the telescope were one inch too small, and it was difficult to read within that quantity, then the pendulum indications are 2°3 per cent. short of their true value. A great source of error no dovbt resides in the test screw of the pendulum. The instrument described will be recognised by those engaged in similar investigations as coarse in construction, roughly approximate in its records, and because it is large as being in all probability subject to 88 REPORT—1895. convection currents, unequal heating in its parts, and other interferences. In spite of these objections, I find it satisfactory. It is cheap, easily put up to read from 1” to 0’"5, easily worked, while the light is near the film, and therefore in the best position to use with ordinary bromide paper. With more delicate apparatus, on the Tokio plain at least, no matter what the size of the foundations might be, the results of my experiments show that such instruments continually require readjustment in order to keep the light on a film of manageable breadth, while if installed on the rocks in the mountains I fancy that, owing to earthquakes or the gradual yielding of the column, there would be a constant change in the mean- ing of the deflections. In two of my pendulums I notice that sometimes they gradually become more sensitive and sometimes less sensitive. The columns I am using underground are of brick, 2 ft. high and 2 ft. square, put together with pure cement. On the top of these, at first, I placed a slab of marble ; but because I noticed that in a damp atino- sphere there was a marked chemical action taking place between the brass screws and the stone on which they rested, the marble has been replaced by slate. (b) Observations at Kamakura. Kamakura, one of the ancient capitals of Japan, lies on the western side of the Miura Peninsula, facing the Pacific Ocean. On account of its ancient temples and its enormous bronze Buddha it is visited by almost all travellers to Japan. The geologist has an interest in visiting this place, as it has been the site of a series of earthquakes, which, with their accompanying sea waves on more than one occasion, are said to have laid waste a city of a million people. The place is prettily situated amongst Tertiary hills which rise to heights of from 100 to 600 feet around the plain on which the ancient capital stood. The cliff-like faces of these hills show a series of conformable beds dipping about 30° N.E. These beds, which are soft grey coloured clay stones or beds of consolidated ashes, are from a few inches to a few feet in thickness, and are traversed by numerous small faults the throw of which, so far as I have observed, does not exceed six feet. Near to the temples, caves have been excavated, which are used as shrines; while similar but smaller caves have been made by farmers, and are used as storehouses. The general relationship of the strata at Kamakura to the alluvium and diluvium overlying tuff at Yokohama and Tokio is shown in the ac- companying section. At Kamakura the tuffs are crushed and faulted, but before reaching Yokohama they pass into gentle folds, and then become horizontal and are capped with some fifty feet of reddish earth and gravel. This condition, with the exception that the overburden is perhaps 100 feet in thickness, continues up to Tokio. ~ At Yokohama the tuffs, which almost entirely consist of a light grey ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 89 coloured clay rock, are visible as cliffs from 50 to 80 feet in height. In Tokio, however, they only crop out at one or two places at the bottom of deep cuttings. The depressions in the section represent the flood plains of rivers which are filled with soft alluvium. Rather than working on strata which had been so far crushed and crumpled that further yielding is hardly to be expected, I should have preferred a site gn the strata which are gently folded, and where a measurable amount of yielding may yet be in operation. Although I had the choice of several caves as Kamakura, all of them were situated at some distance from the railway. To go and return from the one I selected took six hours, and it was therefore seldom that it was visited more than once a week. Very fortunately I received assistance from Mr. P. E. Heerman, a gentleman who happened to be staying in the neighbourhood, while one of the officials from the railway station kept the lamps burning, and three times a day took readings of the instruments. That the latter was attended to regularly was shown by a slight change in the intensity of the photographic trace at the times when the lamps were adjusted, a gap when they were removed to be refilled and a slight notch in the diagram from a self-recording thermometer at the times when the doors of the cave were opened, and the times at which these various marks were made coincided with the times at which the readings were noted as having been made. The cave seems to have been excavated on the line of a fault which, curiously enough, is with difficulty recognisable on the face of the cliff itself, but which is quite apparent in a photograph. The entrance to the cave, which faces 8.E., was, with the exception of the door, blocked up with a wooden wall faced on the outside with a bank of earth and rubble work 4 feet in thickness. The dimensions of the cave were 20 feet by 20 feet, with a height of from 7 to 10 feet. One corner of this was partitioned off with wooden walls to form a room 10 feet square, and from this the débris was cleared out to reach the solid rock on which two brick platforms were built. These were one brick thick and laid with pure cement. On the end of each of these platforms, which were at right angles to each other—one running N.W. and the other N.E.—a small pillar three bricks high and one brick square was built and capped with a slab of marble. These were finished on January 7, and the cave was left open for one week to facilitate the drying. At the end of that time, on January 14, as the cement appeared to haye set, the instruments were placed on the slabs and the records commenced. From that date, with but few interruptions continuous photographic traces were obtained until March 18. These machines I have called C and D. Machine C recorded tilting parallel to the strike, while D recorded movements parallel to the dip. By a lifting on the S.E. side the readings of the index attached to C increased in value, while the readings of D increased with a lifting on the 8.W. side. At the end of each week, when a photographic film was renewed, the sensitiveness of the instrument was determined, after which it was re- adjusted. These determinations are given in the following table. The ratio of unity to the numbers in the first two columns is the tangent of the angle through which the instrument would have to be tilted to produce a deflection on the photographic trace of one millimetre ; the corresponding angles in seconds of arc are given in the third and fourth columns. At the commencement it will be observed that to produce a deflection of one 90 REPORT—1895. millimetre in C a tilt of about 2’’ would be required. Between February 18 and 25 the same deflection was obtained by a tilt of about 0/’-27. Because D recorded more motion than C, it is important to notice that this occurred notwithstanding the fact that on all occasions, excepting between February 4 and February 11, C was very much more sensitive than D. Sensitiveness of Cand D. Date C D Cc D Jan. 14-21 | 115,776 86,400 UTS AED | PRPAIEP AS} 313,560 250,560 0’ 66 0'"-82 3. 2Oe 434,160 280,800 | 0-48 0'-73 Feb. 4-11 313,560 355,600 0-66 O'-58 Swiss 578,880 280,800 0:35 0'"73 53-9 BB8=25 771,840 280,800 | 0":27 0'° 73 » 2-4 675,360 302,400 0'"30 0'"68 March 4-11 627,120 216 000 | O32 0'-95 ey, nbd Eales} 482,400 259,200 0-42 0'-79 The temperature variations in the cave during 24 hours never exceeded eee 6s (c) The Diagrams. At first sight, with the exception of places where earthquakes have been recorded, the photographic traces appear to be a series of long straight lines, and the fact that movements have taken place to the right and left of a normal position can in most cases only be seen by looking along their length (see fig. 2, Plate JI.). The curves which are thus seen are too long and flat to admit of accurate measurement, and although the films had only moved at a rate of about 6 mm. per hour there is great uncertainty in determining points of inflection. For these reasons both the angular deflections and the periods occupied in describing them are only rough approximations. In the diagrams, Plate ITI., the observations extending over nine weeks are plotted as a series of curves. The vertical lines indicate noon and midnight of successive days, which are marked with their dates. The horizontal lines, which are 10 mm. apart, indicate seconds of arc. Ifthe curve for C goes downwards from its starting point the movement is equivalent to a rising on the 8.E. side, while if the D curve descends this means that the S.W. rises. The angular values for the various deflections are marked on the diagrams, while earthquakes recorded by seismographs but not by the pendulums are indicated by dots. Earth- quakes recorded by the pendulums but not by seismographs are shown by short straight lines. (d) The Movements of the Pendulums. From the diagrams it is clearly seen that during any week the pendulums have once or twice wandered away from and then returned to their starting point. Because the movements or periods of comparative rest of the two instruments approximately coincide in time, as, for example, during the fifth week, I take it that the cause of these movements is something more general than a warping of the supporting columns. The movement of D or that which is parallel to the dip has usually been greater than that indicated by C or parallel to the strike. For example, it may he 65% Report Brit. Assoc., 1895. Plate III Movement of horizontal pendulums at Kamakura. ez 7°92 aS ‘ \I | SCE “fe 3 Illustrating the Fourteenth Report of the Committee on the Earthquake and Volcanic Phenomena of Japan. ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 91 imagined that between February 28 and March 3 the dip of the rocks increased and then decreased through an angle of 4-08. About the same time the movement at right angles to this was 2/88. With the exception of a wave indicated by C between February 6 and 7, which had a period of 24 hours, all the other movements have had periods of from 48 to 70 hours. In this respect the movements are strikingly different from those recorded in Tokio, where diurnal waves are very frequent. Another remarkable feature in the records is the entire absence of tremors, which in Tokio on the alluvium often result in producing a photographic trace from 5 to 10 millimetres, and sometimes even more than this, in breadth (Plate IL, figs. 5 and 6). Although it is premature to offer an explanation for the Kamakura movements the following statement may be made. As the changes in temperature in the cave were usually too small to be measur- able itis not likely that the wandering of the pendulums can be attributed to such a cause. Any effect that the heat of the sun may have had upon the face of the cliff in which the cave is situated, in raising its tempera- ture or by withdrawing moisture from its surface, would probably be diurnal in its character. The only sunshine records which I have taken commence on February 25. From that day to February 28 there were 28 hours of sunshine which was followed by dull weather until March 11. Although the end of the period of sunshine was followed by a great move- ment, considerable movements occurred during the comparatively cloudy weather. Because the records are few this observation, however, carries but little weight. Rain, which only fell between February 8 and 9, and again between March 5 and 6, does not show any connection with the movements. Notwithstanding these observations, since the wandering of pendulums in Tokio, as will be shown later, is apparently connected with the movement of subterranean water, which in turn is related to percolation from the surface, it does not seem unlikely that the movements at Kamakura may also find a partial explanation in a somewhat similar cause. The only other explanation, which, however, has not yet been verified, is that they result from rock crumpling which is still in progress, and for this reason the greatest motion is parallel to the dip. Conclusions of practical importance which I arrive at are that although pendulums which will record a tilting of 0'’"3 are sufficiently sensitive to be used on the Tokio plain, an instrument of much greater sensibility is required to study movements on the rock, and, further, that all who have to carry out physical investigations requiring a steady platform will gain great advantage by installations on the rock where tilting is small and diurnal movements and tremors are not appreciable to instruments such as I have employed. (e) Earthquakes. The earthquakes which have been recorded by the Kamakura instru- ments in 1893 are as follows :— The following 26 disturbances are clearly shown upon the photographic traces. In addition to these there area number of slight irregularities with amplitudes of 1 mm., or under, which have been omitted, first, because they are very small, and secondly, because they might or might not be due to earth disturbances. While the observations were going on, that is, between January 14 and March 18, by means of seismographs in Tokio, 21 shocks were recorded. These were disturbances that were felt in Tokio, and itis known that several of them were also felt in Kamakura. It is probable 92 REPORT—1895. | | Range of. . | Instrument Month} Day Time motion ieee: Duration on which Remarks in mm. | = | recorded hr. min. | secs, hr. min. I 18 8 46 P 15 80'-00 2] 2-10 | Recorded in Tokio! 25 841A 14° | 11-48 |} 0 10 | D C not working | 25 9 21A 8 6.56 |.0 20 | D :. as 26 fils ye: Ala oes | II. | 1-2 | Six slight disturbances 3 8 380A) 12 5'-76 | 0 45) Cand D | D gives 8'"76 | 10 OOA | 6 ZS? 1O' Se1'8'| "CO aid 0) Sette OR SORAG Nieatdis st 90527601170): 2186) ieCland D de Sie ie Sie 7G6 4 | 7 OA} Slight | 5 | 718A? Fh CN LE | 3 54P Sioa VSS TO CO ams) C TOUS aemeaoe 2 | vo" | C 6 454A Dre Wan 2 APES C Si e250 Ac 2 6°96 | 0 30 D | 6 304 | 3 UGA Orta Ou D | 6 50A | -f Dao Ou lO D 19 | 7 31A | 6 41°38 | D | 8 OOA | Oo) eS | D 8 264 | 6 4''-38 | D 20 8 B0A 5 135 C On D438 Re-| | corded in Tokio) 27 12 50A 1 ome eee) C On D 4''-38. Re-| | corded in Tokio) that had a seismograph been placed in Kamakura all these shocks and possibly a few others would have been recorded. The horizontal pendulums, however, have only recorded three of the Tokio series, and to the remaining 18 they have been insensible. On the other hand, they have recorded 23 disturbances which the Tokio seismographs have failed to record. Although Ihave not yet had time to fully analyse the records of earthquakes given by the Tokio pendulums, from what I have seen of them I know that the results will be similar. On many occasions I have watched a horizontal pendulum while a sharp disturbance lasting from 15 to 30 seconds has been taking place. All that happens is that there is a slight elastic switching in a vertical direction of the pointer at the end of the boom. The boom does not swing, and I have not observed a blurr in the photographic trace. (Plate II. fig. 2.) On the other hand, whenever an earthquake instead of simply producing elastic vibrations throws the surface of the ground into undulations, the pendulums behave most erratically. They do not swing but they are forced first to one position and then to another. Now and then they may pause for two or three seconds, but only to start, perhaps, more vigorously than before. It is interesting to watch a seismograph writing an earthquake, but a horizontal pendulum actuated by earth waves is one of the most attractivesights that a seismologist can witness. When a seismo- graph is disturbed you feel the motion that causes it to move, and in two or three minutes all is ended ; but when a horizontal pendulum is disturbed nothing is felt, and its spasmodic movements may continue for one or two hours. Fig. 3, p. 109, shows what is almost continuous motion for 5 hours 24 minutes. Already I have had the ae fortune to see this phenomenon five times. On the last occasion, Mar ch 2 22, at 7.27 p.m., I sent a messenger to call my colleague, Mr. C. D. West, who arr ived some 15 minutes later, when we watched the big boom stopping and starting from various positions for 1 ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 993 hour 47 minutes. These waves had a submarine origin about 40 miles off the N.E. corner of Yezo, in about 43° N. lat. and 146° E long., and to reach Tokio had travelled some 570 miles. I think that they have been recorded in Rome, and I have written to Dr. E. von Rebeur-Paschwitz to learn whether they were noted at Potsdam, Wilhelmshaven, and Strassburg. They ought to have reached the Birmingham instrument about midday on March 22. While I am writing in Sapporo (Yezo), on June 20, at 2.32 P.m., a terrible earthquake has happened in Yokohama and Tokio. As we are 9 hours E. of Greenwich this should be recorded at the above stations and those in Russia at about 6.30 a.m. on the same day. From the manner a pendulum behaves I infer that its movements are due to the fact that itis being tilted, and because the photographic records are always less than the distances through which I have seen it move, the values given for the tilting are less than those which actually happened. Ti a pendulum is set swinging, for example, by standing near its column, through a distance of, say, 5 mm., it will come to rest in about 5 minutes. In calculating the duration of a disturbance allowance has been made for this factor. The point of greatest importance in connection with the foregoing remarks is the inference that the catalogue of Kamakura earthquakes represents a series of large disturbances which have travelled very great distances. Had there been any local disturbances sufficiently great to produce earth-waves, then the pendulums must have recorded the same, but no such disturbances occurred. As it is not likely that earthquakes originating at a distance could in any way he connected with local tilting, if earthquakes and tilting have any connection those which might be compared with the curves already given are those of local origin which have been recorded by seismographs in the vicinity, and not those which are shown on the photographic films. Between January 24and March 18 fifteen shocks were noted in Tokio, which cannot be seen on the photo- graphic traces. Because nearly all these were of the nature of elastic vibrations it is probable that they were for the most part of local origin. This is a point which can only be definitely settled by analysing the reports accumulated at the Meteorological Bureau, which for various reasons’ cannot be done in time for the present report. These 15 shocks are indicated on the curves as black dots, and it is certainly worth observing that they chiefly occur during the seventh, eighth, and ninth weeks when tilting was marked. Because the observations are few and because I am not yet ina position to analyse all the materials which have been accumulated, too great: stress should not be laid upon this last observation. It only indicates the nature of an inquiry that is being made. The Jast point to which attention must be called in connection with the Kamakura disturbances is that the greatest motion has nearly always been in the direction of the dip, that apparently being the direction of least resistance to yielding. By reference to the catalogue it will be seen that there are three instances where small disturbances have only been recorded by C, but in ali other cases the records are given by both instru- ments, the dip record being much the larger, or the record has been given by D alone. For example on February 8 D was tilted for 30 minutes through an angle of nearly 7”, while C did not show that any motion had taken place. 94 REPORT—1895. (f) The Observations in Tokio. Although the observations made in Tokio were carried on at two stations, because these stations were only 1,000 feet apart, and because both were on the alluvium which here forms a layer perhaps 100 feet in thickness above the tuff rock, it was anticipated that the records would to some extent be similar in character. For this reason they are described together. Machine A, which is similar to those used at Kamakura, is installed on a table-like stone column in my house. The column is 4 feet square and rises clear of the floor from a concrete bed. For a few hours in the morning and in the afternoon the sun produced a marked tilting as it shone upon the column through a window on the south side ; on closing this window by a shutter on the outside and by a curtain on the inside, this effect disappeared, while the diagram from a self-record- ing thermometer occasionally showed during 24 hours a steady rise or a steady fall of 1° or 2° C. More usually, however, the diagram showed that from 9 or 10 a.m. until 5 or 6 p.m. there had been a rise of 4° or 5° C., after which the temperature fell until next morning. This is a point to be noted, because it will be shown that the daily tilting and, in a less marked degree, the intensity of a tremor storm have a similar periodicity. The water level beneath my house oscillates above and below 36 feet. Machines E and F, which are underground, only differ from A in the fact that their booms are brass tubes. Machines A and F are parallel to each other, and point N.W. Machine E is at right angles to A and F. With an increase in the readings of A or F the movement corresponds to a lifting of the ground on the N.E. side of these instruments. An increase in the scale readings of E corresponds to a tilting on the 8.E. side. The underground chamber is excavated on a flat piece of ground about 20 feet below the site of my house. It is 13 feet deep and 20 feet square. The floor is covered with } in. of asphalt, which rests on a bed of concrete 6 in. thick, which in turn rests on a bed of well-rammed gravel. The walls and ceiling are brick with clay puddle on the outside. Above the chamber a wooden house has been built ; the entrance is by double doors, and it is fairly well ventilated by gratings for the admission of air and a short iron chimney for its exit. The daily fluctuations in temperature in this underground room are practically zero, the diagram from a self- recording thermometer showing a straight line which at present indicates a steady rising of 1° C. per week. The water level in a well about 80 yards distant, where I have established a tide gauge, is about 25 feet below the surface. The floor of the chamber is therefore about 12 feet above water level, but it must be remembered that this level may rise and fall through 2 or 3 feet. (g) Sensitiveness of the Instruments. From time to time the sensitiveness of the instruments was determined, and if necessary they were readjusted. The first column in the accompanying table indicates the number of millimetres through which the end of the boom travelled by a 1° turn of ' ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 95 the sensitising screw in the bed plate, the pitch of the screw being 1 mm. One complete turn of the screw attached to A tilted the bed plate of this instrument through an angle of | in 228. For E and F one complete turn represented an angle of 1 in 222. The ratio of unity to the numbers in the second and fourth columns is the tangent of the angle corresponding to a deflection of the boom through a distance of 1 mm., the values of these angles expressed in seconds of are being given in the third and fifth columns. A E and F Ee — eo 25 199,800 1-03 | 5 | 399,600 O'-51 6 479,520 0-43 6-5 519,480 0'-39 10 820,800 0/25 799,200 0'-26 10°5 861,840 0'-23 11 902,880 o”-22 | 879,120 0-23 12 984,960. 0/20 13 1,038,960 0-19 14 | 1,118,880 0-18 To bring the points of E or F to the centre of the scale, a rough adjustment is made with the sensitising screw, after which the boom may be slightly moved to the right or left by means of a stone about 40 Jb. in _ weight which I shift on the Hoor of the chamber towards or away from the instrument. (h) Daily Tilting. The approximate times at which the diurnal wave reached its maxi- mum and minimum, and the amplitudes of these waves for dates between January 24 and March 1, 1894, are given in the table, p. 97. Should it be necessary the table may be completed from December 9, 1893, up to the middle of June 1894. With but few interruptions the records have been continuous. It will be observed that the records for F, which is parallel to A, are only one or two in number. The letter s means that the diurnal wave is too small to be measurable, while blank spaces indicate that it was not visible, the photographic trace being a straight line. Had greater sensi- bility been given to F it is quite possible that the daily wave would have been recorded ; but this could not be done because, even with the stability it _ had during three days, the end of the boom often wandered through a dis- tance greater than 1 inch, and the spot of light left the film. This wander- ing of the pendulums has been already referred to. On two occasions when _F gave measurable waves (January 31 and February 2) the times of their occurrence approximately coincided with the movements of E and A—that is, the movement of the pendulums in one direction was reached in the evening, after which'they gradually returned to reach their norma! position _in the morning. The pendulums E and A, although at right angles to each other, have shown a marked synchronism in their movements. It would seem that these two instruments have either been simultaneously acted upon by independent forces, or that they have recorded components of a common force, which has acted in different directions at the two ' stations. The latter explanation appears to be the more satisfactory, because 96 REPORT—1895. periods of steadiness when the diagrams were practically straight lines happened at the same time, and because the large or small movements of A have agreed in time with the large or small movements recorded by E. As illustrative of this synchronism, the movements of these instruments between February 15 and February 25 have been plotted as curves (see Plate IV.). Once or twice it will be observed that crests of waves have been reached after midnight or in the morning, which agrees with the results published in 1893 (Thirteenth Report). In the majority of instances, however, this has been reversed, and the movement of the pendulum in one direction has been completed at any time between 4 p.m. and 10 p.M., and it has returned to its original position between 5 a.m. and 10 a.m. Because the waves on the original diagrains are long and flat it is usually difficult to determine with any accuracy the exact time at which an excursion in any one direction has been completed. Sometimes the boom has remained at rest at one of its limits for five or six hours before the return journey has been commenced. The movement from 5 or 10 a.m. until 4 or 10 p.m. has nearly always been quicker than the return motion during the night. The amplitude of motion does not seem ever to have exceeded 3’’:00. In 1893 I described movements of from 2’-00 to 10:00 ; but these which I now discuss are the result of observations with several instruments, although I cannot answer for any great degree of accuracy, I am inclined to consider the new determinations as being nearer the truth. The move- ments of KE, which is underground, have usually been greater than those recorded by A in my house. In a few instances, however, the deflections of A have been the greater. As an appendix to the table on p. 97 short abstracts from my journal are added :— (t) Extract from Journal of Records obtained in 1894. In the following extracts the sensitiveness of the instruments means the angular tilting required to produce a deflection of one millimetre of the points at the end of the booms. These degrees of sensitiveness for the instruments E, A, and F are given in fractions of seconds of are immediately after the date. January 24-27 (018, 0/23, 0”:43).—From the 24th to the 25th E showed a rapid 8.E. lifting of 3’ when the light spot left the film. A small earthquake occurred at 10.48 a.m. onthe 25th. From the 25th tothe 27th there was a 8.E. lifting of 1-62. Daily waves of 1/44 and 1/26 are well marked. All instruments showed tremors, but they are most marked underground on E, where they reach 12 mm. On A and F the daily waves are hardly visible. January 27-30 (0':19, 0'-23, 0’-18).—E moved 5’32, and the light spot left the film. It shows tremors reaching 14 mm. A and F agree in showing a N.E. lifting, but the daily wave is only seen on A when the tremors reach 10 mm. The tremors are most pronounced under- ground. January 30-February 2 (0°43, 0:23, 0'18).—E shows similar characters to A and F, that is, the trace is at first straight, and then two daily waves and three small earthquakes. For the first day A and F are straight, but for the other two days there are daily waves. F shows a 65% Report Brit. Assoc., 1895. ‘undye fo Duamousyd ovuwo0 4 pun aynnbypwwny ayy uo aajnumon ayy fo yoda yyuaninog oy buyvusnyy ‘]]eM & UL IojyeM Jo (gq) punoisiepun pue 9oRyan uorjom A[rep Surmoys ssatovry, uo stunjnpued jo min nab ae RIEuOTS aOR ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 97 E A F | | A —_.""“_ —————_—————o~ | SS A ae +a | Timeof | Timeof | =| Timeof | Timeof | Re ; ea an i) ime o ime 0 Bo ime 0: ime o “qo |} Timeof | 4 ag B= | Sinusof | Crestof | 25 | Sinusof | Crestof | 2% | Sinusof | 5 ay Wave Wave iP Wave Wave 3 » Wave | 3 | 189t Mh " u” Jan. 24-25 3.30-9.30 P 2°70 — s — — s = = (= » 20-26 | 11.30 P-1.30 A | 144 — LOA _ — s _— — 16 » 26-27 | 11.0P-12.0 | 1:26 9.0.4 8 = = 5 = 25 ms » 3l-1 6.0 P-8.0 P 0°86 9.0 A 6P 0°69 7.0 A 9.0 P-10.0 P| 0°36 4.04 — Feb. 1- 2 7.0 P-9.0 P 0°60 | 5.0-9.0 A 5 P-6 P O92 6.0A 8.0 P-9.0 P | 0°36 | — = eae 6.0 P 0°80 TOA - _ — — hear = ate ~ ee 6.0P 0°80 7.0.4 = = = a) get wa = aed 5 1.0P 0°80 7.04 a= = = a tyes = Ee 2 §6RG = — 6.0A 8P-9P = = s SS = » 6-7| 5.0P-10.0P | 1:29 8.04 5P-6P | 161 9.0.4 5 —t us a » 8 5.0 P-10.0 P 0°85 6.0 A 5 P-6 P 115 8:30 A s | 0°46 — — a, 8=0 = 086 | 7.0A = = = rol dy Vea af 27 » 210 4.0 P-4.0 A s 10.0 A 4P O78 — 8 ge a = = ahem 7.0P 0:86 3.0.4 3P-5P | 0-78 aa 5 pe a = » 11-12 7.0P 0°86 = = — — s bse = = > 12-13 10.0 P 0°86 6.0 A _— — — Large and irregular —_ » 12-14 3.0 A 0°86 7.380 A _— = = $s —_— — —_ » 14-15 9.0 P 1:29 7.30 A a —_— —_— s = = eae s 15-16 12.0PM 043 10.0 A _ O1 6.0A —_— — — == s, 16-17 | 10.0 P-12.0P | 1:29 8.0A 6 P-8P 0) 9.0 A » 17-18 | 10.0P-12.0P | 1°72 9.0 A. 6P 175 TOA — — = = » 18-19 9.0 P 2°58 10.0A 10P 2°50 0A s — — — » 19-20 6.0P 1:29 6.0.4 6P 1:25 | 1A-GA 5 = = ae » 20-21 6.0 P 215 6.0A 7.0 P 2°25 2A-6A — s — 1 21-22 = = = = =: = = 25 - 2 9 22-23 6.0 P 1:72 6.0A 4.0 P O75 TOA a s — pe 3) 23-24 4.0 P-6.0 P 1:29 | 6A-7A 6.0 P 0-75 6.0 A = 3 — _ sy 24-25 6.0 P 1°72 GA | 5.30 P O75 —_— — s — — » 25-26 6.0 P-7.0 P 172 6A 4.0 P _ — - s = = y 26-27 10.0A 2°58 6A | — s — | = s = Sa Mar. 1- 2 11.0P 301 9.0 A — 05 —_— — = — a s 238 6.0 P-1.0 A | 2°15 5.0.A — 0-5 — = = = 2 » 38-4] 6.0 P-12.0P | 0°86 2.0A — — — = = = 2 » 5-6 7.0P 1:29 10.0 A — s — = s = = Be ag 8.0 P 215 | 10.04 = s = - $ ey = ae oe 9.0P 1:72 9.0 A — s — = $ = = ” 8- 9 — s => —_ 8 _— — —— —— 112 » 9-10 _ $s _ —_— s — — = — | 3 » 10-11 _ 8 _— — — _— = = az | 19 _abae es 3 ze 2.0 P 1-0 6A 26 pa i Eee >», 13-14 — s —_ Irregular = a= ds = » 15-16 Clock repairing — — — = ees =e 8 in leotr ba a 8.0 P 25 WA a. — ee 35 eagle 2 ¥ 7.0 P 25 12.4 us Le =e Eas 23-24 - 2 6.0 P 1:60 104 2 ae #4 se ss 24-25 id - 6.0 P 1:40 104 a = an 5 » 26-27 ”» ” 10P 1:60 WA — — — 4 » 30-31 » ” 10.0 A 10 6A — = = 20 steady N.E. rising of 2/70 until February 2, when at 7 p.m. there was an earthquake. Tremors are slight. Pebruary 2-5 (0!:43, 0-23, 0”-23).—E shows the usual daily tilting with small trémors. . After the earthquake of the 2nd F continued to rise until the 3rd, when at 8 p.m. the light left the film. February 5-7 (0:43, 0/23, 0'-23).—The daily waves in E and A are pronounced, and when one is large the other is large also, and vice versd. In F the waves are not so marked. Tremors are slight on A, but under- ground in E and F they reach 3 mm. February 8-12 (0-43, 0'-26, 0'-23).—E daily deflection (9-10) slight, but from 10-11 like A. On A the daily deflections are well marked, but on F they are very slight. F, however, falls from 84-67 (3-91). Tremors are greater on the surface, reaching 6 mm., than they are under- ground, 1895. Ht 98 REPORT—1895. February 12-15 (0'"43, 0-25, 0'39).—E shows well-marked daily curves. A outof order, and therefore no record. F found to have changed its sensitiveness ; therefore reset, so that 1°=0'"23. From 12-13 F wandered from 75:5 to 52 (8/’-97), and again from the 14—15 it crept from 72 to 62 (230). These movements, which so often occur with F, meana change in sensibility. Both instruments show tremors of 3 mm. February 15-19 (0/48, 0:25, 0’:26).—On E and A the daily waves are seen as a succession of symmetrical waves, gradually increasing in height and in length. Close upon the crest of the last and largest of these waves an earthquake occurs. F only shows the last of these daily waves, the remainder of the trace being a straight line, indicating a slight N.E. sinking (1/30). Tremors on all three instruments are slight. February 19-22 (0/43, 0'25, 0-25).—E and A show a continuation of the daily waves. Between the 21st and 22nd both instruments gave a straight line. F only shows the wave of 20-21, but it shows a N.E. sinking from 76 to 40 (8-00). On the 20th, at 9.30, there was a strong shock. A shows two series of strong tremors, which are only faintly indicated by the underground instruments. February 22-26 (0':43, 0:25 0'26).—E and A show well-defined daily waves. F is nearly astraight line, but wandered about 30 mm., as if N.E. had sunk. Tremors are seen from 6 A.M. until noon on the 23rd, and again from 6 p.m. on the 24th to 4 p.m. on the 25th: on A and F they reach about 5 mm. The earthquake of the 24th is not shown. February 26—March 1 (0:43, 0/25, 0'26). The daily curves on E are marked, but they are irregular. The shock of the 27th occurs just over the crown of the daily wave, which was at 10p.m. The crest of this tilting, both in time and amplitude, was unusual. On A and F the daily curves are slight ; on A, like E, they are irregular. Tremors of 2 or 3mm. are shown on A and F onthe 26th, 6 to7 P.M.; 27th, 6 a. to 4 P.; and on the 28th, 6a. to 1 p. The last are visible on E. F wanders by a N.E. sinking through 10 mm. On March 1 the direction of motion commenced to change, that is, there was a N.E. lifting. March 1-5 (0/43, 0'-25, 0'-26).—On E the daily curves are large, but at unusual times. A shows slight daily curves, but a N.E. lifting of 10 mm. F shows a N.E. lifting of 22 mm. 2 Tremors are seen on A on the 2nd, 2 A. to 11 A. ; and this agrees with E, but not with F, which shows slight tremors, March 1, from 9.30 a. to midnight. March 5-8 (0/43, 0'°25, 0'25).—E shows a well-marked series of daily curves, and wanders 8 mm., as if the S.E. was rising. The daily curves on A are slight, but the trace is faint. F wanders 40 mm. as if the N.E. was rising. On March 6 small tremors are recorded, but only on A. March 8-12 (0':48, 0-25, 0':26).—E shows slight daily curves on the Sth, 1 p. to10 pr. Asinks on N.E. side 4 mm., showing tremors of 6mm. It then rises to the 10th, 8.30 p. 12 mm. At 8.40 an earth- quake. ON THE EARTHQUAKE-AND VOLCANIC PHENOMENA IN JAPAN. 99 F rises on N.E. side 40 mm. Tremors on E and F are slight. March 12-15. (0/43, 0/25, 07-26). The daily curve is barely visible on E, which shows small tremors. A shows curves, but they are irregular, and the N.E. sinks 15 mm. F rises 23 mm., that is, the direction of motion is contrary to A. Both A and F show small tremors. March 15-19 (043, 0:25, 0’:26).—E clock stopped, and therefore no records until end of month. From the 15th to 16th A was steady, but from this date onwards it gave large daily curves. On the 15th, and at 3 a.m. on the 18th, there were earthquakes. During the three days A rose 9mm. _ F does not show daily curves, but it rose 39 mm. The conclusions I arrive at respecting this section of the report is, that instruments on the surface and underground show diurnal move- ments, which closely agree in the times at which they occur. These move- ments are most pronounced underground by pendulum E, the excursions of which have in nearly all instances been greater than those shown by pendulum A in my house. The crest of a wave which corresponds to a N.E. lifting on A and a 8.£. lifting on E has usually been reached between 4 p.m. and 10 p.m., the movement in the opposite direction being completed between 5 4.m.and 10 a.m. It does not seem that air temperature has had any measurable effect in the production of these movements, because they have been most marked beneath the surface, where the change in temperature during twenty-four hours has practically been zero. The opportunities for observing whether they hold any relationship with rain- fall have been few. It is possible that the rainfali of March 16 and 17 may have been connected with the large motions of A between March 16 and 18, but the largest motions of E on March 1 and 2 occurred during a dry period. After the rainfall of January 25 and 26, and again after that of February 8 and 9, it may be noticed that the time at which E completed its N.W. excursion was delayed, while after that of March 16 and 17 pendulum A was delayed in its N.E. movement, and these are the only occasions on which rain fell in any quantity. (j) The Wandering of the Pendulums. The following table shows the daily change which has taken place in the position of the pointer of pendulum A, and for a few days that which has taken place with pendulums F and E. The numbers indicate so many millimetres of motion. The sign + prefixed indicates that the scale readings were increasing, while the sign — indicates that they were becoming smaller. When the signs for A and F are similar, then these two pendulums were moving in the same direction. The difference between the readings of an instrument when a new film was put on and when it was taken off gives the distance through which a boom has been displaced during periods of three or four days: this quantity is also ex- pressed in seconds of arc. The fifth column gives the rainfall in milli- metres, and the sixth the number of hours of sunshine, but only between February 25 and April 30. These latter records were taken for me by my colleague, Prof. W. K. Burton. H2 100 REPORT—1895. seismographs Z| Seaimeae Date A F E ue ea | gs a |me] 88 :| BA Jan. 24-25 al Sil =) 1 » 625-26 sai] +4 =15 16 + M6227 etl +1 +15 { —1 +4 +7 | 0"23 | +129 | +1:26 » 228 +2 +12 +26 ” 28-29 +3 » 29-30 +3 +5 +8 +13 =2 + 1” 84 + 2!'-34 —0'":57 » 30-31 —! eral +3 a Bi Lhep,.)) 2 +6 Feb. 1-2 iy 44 <7 a | +2 —0"-46 +2'-70 +086 paeteZ8 —4 » 3d4 +3 a 4-9 0 == ass 0 = 0-23 — 1-78 0 ” 5-6 +12 » 6-7 +1 » 1-8 +1 =8 | { | pt 5 +2 | +3/-29 Sarit +0'"86 | rh 9 —6 Lig | et) ei S020 0 spelled at) ) j, —8 ay +2 ||. -2'"08 391 | +0'"86 (eee a Sa fetes | nee L253 —2 —23 —3 . ss +4 +22 0 | » okdedb 0 ~10 +5 | | | +2 S13! +2 iWedeners” 15) Opal OLA Bee 1s Ayr ot LEEG: +8 ah es +5 ON THE EARTHQUAKE AND VOLCANIC PHENOMENA IN JAPAN. 101 A se | £26 Date A F E é e eke Es 2 'S Oh |) Bis 8 fo] oa pay o-3 +1 —5 +3 +025 | —1''30 | 41/29 Feb. 19-20 +10 1 . PDEA 212 1 oy PU =i 2 bts —94 =o | S0!-75 Ie 60 —1'"-29 =) 22-23 +3 0 » 2a-24 229) » 24-25 +3 8 2 »» 25-26 +1 5 +5 +3 0 +125 | 0-78 0 u] 7 — 9) 26-27 29 7 1 3 21-28 +2 9 1 » 28-1 (Mar.) =iK0 a1 =4 0 O25) | — eo" 0 March 1-2 +4 +4 £39) ” 2-3 +4 2 2 ‘a 3-4 +1 +30 —3 2 1 » 45 1 +9 +32 =i +995 | +8''32 | —0''-43 a 5-6 +1 +27 +6 6 1 a 6-7 +2 +15 » 7-8 —4 +15 +4 —1 +15 +8 —0!''-25 + 31-75 + 3/44 ~ ~ ! re 8-9 + 1 12 BS OETO +6 3 ee Olt 0 12 1 Pier =6 2 9 i a +34 ai l beO'T25 | eree Negras ee 11s =6 9 1 5 Re =6 4 2 14-15 =8 6 5 1 eal +23 = —3''-25 | +598 | —O0'-86 102 REPORT—1895. nan n | 7 ae | 2f| gee Date A F E 22/44 aS t 25 68 see = ae Bes =] 3 23 | March 15-16 | +8 8 6 1 a) eee +6 35 6 5 Mis —3 9 eho) | —2 3 Pasi i, ie 39 +8 | +2'7-25 + 10/714 43°44 | ay 6L9=20 ok 3 20-21 —4 4 1 5 alee -2 9 ri (Heesig: 2 | | —2''50 meee —7 | 9 9 » 2e-2t —6 | ” —25 +18 [ +5 +4 | +1125 | 411-04 ” 25-26 +9 Dd 2 b= —4 = 3 4 2 » 27-28 0 20 Sie ce) —6 ah 8 | -1 —10 | | 0-20 | —2'-60 HES tO) Fehrs. i i 6 1 ay ot Weonl +1 | 5 » 91-1 (Apr.)| +1 | 8g 1 | a oe | { aril —18 | + 0'"-20 —4''68 April 1-2 A 10 1 ” 2-3 +2 8 ” 3-4 +6 8 [ +2 = FA | | 0'"-40 —1'"-04 / fake, | | ” 4-5 18) ] 1 1 ” 5-6 +5 7. ” 6-7 0 6 » 7-8 all 5 1 [ +4 an) [| +080 | +-0'52 | _— ON THE EARTHQUAKE AND VOLCANIC PHENOMENA IN JAPAN. 103 a A & 2 gre @ale2i| sE6 Date A F E ch ee ge 3s > SS April 8-9 +1 8 vait9210 —2 14 boty LOL: +1 eul=12 —5 4 —5 +2 +8 —1'"00 | +0''52 | +4'°08 » 12-13 +6 1 » 13-14 +30 23 10 2 ey lASLb —6 8 8 | 1 » 15-16 —6 Sia} {| 424 fg -8 | 480 | +130) S4rrog £22293 9 » «623-24 +2 8 » 24-25 a1 23 1 jl ced +2 ih | — 22 +206 See een 26 ks um PSGLD 7 ae A W798 +10 56 1 » 28-29 —2 {| +10 0 0 | + 2'-30 0 0 » 29-30 ase +3 —11 » 30-1 (Ma 0 May at 7 0 al —10 3 gee rs) —21 | 0'':92 +0'°3 + Q2''-32 a f +1 38 26 | +0'-23 | —0'"96 iibies f +1 —1 ili 17 | + 0/193 —0'"12 1'"-39 iY (aera mtg +19 16 || 092 | +2'"0 —1''-60 3-16 [| , Pres Toa An examination of the above table leads to several important results. In twenty-four cases the motion underground has been greater than that 104 REPORT—1895. on the surface, while in six cases it has been less than that on the surface. These instances are taken from the three or four day periods. If the analysis was made for daily periods, the difference between the amount of motion recorded underground and that recorded on the surface would be yet more marked. Whenever the movements of the surface instrument A have been great, exceeding 1’ in seven instances, its direction of motion has corresponded with the direction of movement of the instru- ment which is placed in a parallel direction F. In two cases the directions. of movement between A and F have been opposite to each other. ‘When, however, the movements of A have been small or less than 1’’ the cases of agreement and of disagreement in direction of motion are practically equal, there being 6 of one and 11 of the other. For January, February,. and March rainfall seems to have been followed by considerable dis- turbances underground, the movements during dry periods being compara- tively small. The instrument on the surface has, however, shown several marked exceptions to the latter rule, its pointer having moved from 8 to 12 mm. (2” to 3”) at least five times when the displacement could not be attributed to the saturation of the soil. During April and May, although a considerable amount of rain fell, the movements of the underground instruments were small, but it must be remembered that during these months percolation was in all probability very small as compared with that of January, February, and March. Instrument A, on the contrary, showed on several occasions very large movements between April 13 and 14, moving as much as 30 mm. or 6”, and from what has gone before it is not necessary to assume that these dis- turbances were directly connected with rainfall. Up to the date of writing this report I have not been able to obtain from the Meteorological Department factors which enable me to make any accurate estimate of the ratio of percolation to evaporation, but it may be taken, as a general rule, that percolation and the fluctuations in height of subterranean water are greater during the winter months than they are during the summer, and if the instruments partly owe their move- ments to movements of underground water, these movements ought to be most pronounced in winter, and this seems to have been the case. Since the commencement of May, up to June 6, E and F have wandered but little, the diagrams being fine straight lines like fig. 1, Plate II., and without tremors. It must also be observed that it has been the instruments in the under- ground chambers within 12 feet of water level which have moved the most.. To throw additional light upon the part that subterranean water may have played in influencing the motion of the pendulums the following experiments were made :— 1. The movements of water in an unused well were recorded. 2. A rough measurement of the rate at which moisture was evaporated from ground near to one of the instruments was made. 3. A well near to'one of the instruments was twice emptied of its water. (k) Movements of Water in a Well. From April 18 until June 8, I established a tide gauge in an unused well 80 yards to the east of the underground chamber. It consisted of a large wooden float carrying a bamboo mast 30 feet in length, the top of which projected through a hole in a lid which covered the top of the well. As the mast rose and fell a pencil in contact with a sheet of paper on a drum ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 105 recorded the motion. The diagrams obtained indicate the following facts. Very shortly after heavy rain the well commences to rise, and the rising continues for three or four days after the rain has ceased. The upward motion, which at times has been as much as7 or 8 inches in 24 hours, even- tually becomes slower for about two days, after which the water falls slowly. A more important observation, however, is that during any 24 hours there are fluctuations in the rate of rising or falling which when the well is nearly steady are distinct, but when the coming up or going down of the water is rapid they are barely visible. A number of these daily fluctuations are shown on Plate IV. About midnight and for some hours afterwards the water is at its highest, and it is again high during the middle of the day. It is lowest in the evening and the early morning, which is the time when the greatest quantity of water is being drawn from wells throughout the city. The nearest well from which water is drawn to the one in which the gauge is established is on the east side, about 60 yards distant. In the following table the dates refer to the interval between noon of one day to noon of the succeeding day. The figures in the columns indicate the hours at which the well commenced to sink and then to rise in the afternoon and evening, and when it again commenced to sink and to rise in the morning. The time midway between the rising in the evening and the sinking in the morning may be taken as the crest of the night wave, the crest of the midday wave being halfway between the A.M. rising and the p.m. sinking of the next day. The omission of dates or hours indicates that the inflections on the diagram were indistinct or absent. The letters R, F, or S in the sixth column indicate whether the well was rising, falling, or steady. The time at which the well commences to rise in the evening is fairly constant, about 8 p.m. This precludes the idea that the diurnal motion may be dependent upon the tides in the neighbouring bay, which is some two miles distant. The most irregular figures are those indicating the time at which the well commences to sink in the morning, which as summer approaches, when the city rises at an earlier hour, also tends to become earlier, and therefore assist in confirming the suggestion, that the rising and falling of the water are due to the facts that larger quantities of water are being used in the morning and evening than are being used during the middle of the day and the middle of the night. The amount of these fluctuations has seldom exceeded 5 mm., and the day and night waves have about the same amplitudes. Professor Franklin H. King found that a heavily loaded train moving slowly past a well at a distance of 140 feet caused the water in the well to slightly rise, from which it might be inferred that the rising and falling of water in a well might be accompanied by a rising and sinking of the surrounding surface. If this were the case then during a day and night the horizontal pendulums in Tokio ought to show a double curve. In some few instances there is a tendency to show such a double motion, as, for example, in fig. 5, Plate II. But because one of the curves is faint and because it is of rare occurrence, the 12-hour movement in the well is by no means sufficient to explain the daily wave indicated by the pendulums. It must, however, be remarked that the period of well observations coin- cides with a period when daily curves were not well marked, and what happened in the well when they were distinctly marked I have at present no means of ascertaining. 106 REPORT—1895. P.M. A.M. General Date SS | behaviour Sinking Rising Sinking Rising of well April 18-19 20-21 21-22 22-23 3, 23-24 an BABB 5, 30-1 (March) March 2-3 627 7-8 - 9-10 >, LO-11 11-12 12-13 14-15 15-16 18-19 19-20 20-21 21-22 25-26 26-27 Peters ail tt lel | o| it — wie | ane | vo | ea ae acy om oo oo oo | aa roo | | o | | | WOUONNTONOABANOBDOOS (1) An Experiment on Evaporation. Because it was found that a load of about 1,000 1b., made up of men and boys standing outside my observatory wall at a distance of 15 feet from pendulum A, would deflect it 2 mm., the following experiment was made. In my garden a strong beam was rested on knife edges on the top of a stake driven into the ground. On one end of this a box 1 foot 6 inches square, and 6 inches deep, was hung, so that it could swing freely in a hole cut in the ground. The box was filled with earth which came from the hole, and was covered with turf like the surrounding lawn. This load was balanced by weights suspended at the other end of the beam attached to which there was a pointer moving over a scale. During three fine days it was found that the box lost weight at the rate of about 4 lb. per day per square foot of surface, and as the surface of the material “in the box was similar to that of the surrounding ground with which it was level, it was concluded that similar ground in the neighbourhood lost weight at about the same rate. During a night the gain by precipitation of dew was sometimes as much as 1:2 oz. per square foot. No doubt many accurate observations have been made on the variation in the rate of evaporation and condensa- 1 ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 107 tion of moisture from and upon various natural surfaces, but I have not been able to consult them. In open ground 30 per cent. of the rainfall may percolate, but in a forest as much as 80 per cent. may find its way downwards, the difference being due to evaporation ; but as evaporation may cease or even be re- presented by condensation during the night, it would seem that the volume of water in surface wells especially on hot days following rainy weather might have a daily fluctuation. Such a fluctuation would, however, only account for the rising of water during the night and for an additional rise about midday. Another point to be noted is the fact that the alternations of evapora- tion and condensation mean that neighbouring areas, some of which are open and others covered with forest every 12 hours, are wnequally relieved of considerable loads. For example, from an area of about 140 feet square in front of my house, which faces south, every day during fine weather about 5 tons of moisture are removed. From the back of the house, which is sheltered from the sun, and where the ground is always damp, compara- tively but little is evaporated. The underground chamber is sheltered by a grove of trees on its south and west sides, and on the east side it is open, and pendulum E behaves as if a load were removed from the east side during the morning and afternoon, and that side of the ground had con- sequently risen. Pendulum A in my house, where there is an evaporation area on the east, south, and partly on the west side, usually behaves like E, to which, however, it is at right angles. By comparing the table of daily waves with the rainy days when there was no sunshine, when it may be assumed that evaporation was small, as, for example, between March 8 and 11, it will be observed that the daily curves for A and E were not measurable. On sunny days, even if it rained, the curves were pronounced, but they were also large on other days, when, however, evaporation may possibly have been great. To settle this question future diagrams must be compared with the records obtained from a hygrometer exposed to the open or by two pen- dulums in parallel positions, but on the opposite sides of a piece of forest land. Two pendulums thus placed ought at the same time to move in Opposite directions, that is, during the day each boom ought to move towards the forest. An observation entirely opposed to what is here suggested is that made by Professor Kortazzi at Nicolaiew, who placed a hydrograph in the cellar where a horizontal pendulum was established, and found that the diagrams given by the two instruments were very similar. This he attributed to the stone column carrying the pendulum behaving like a sponge and absorbing moisture. When the openings to the cellar were closed and the pillar covered with a waterproof material the effect of moisture almost entirely disappeared. (m) Effects produced by emptying a Weill. To determine what effect a slight disturbance of subterranean water _ would produce on a horizontal pendulum, on May 21 I employed men to rapidly empty a well which is 104 feet distant in an E.N.E. direction from pendulum A. The well is 42 feet 7 inches deep, 2 feet 7inches in diameter, and on this particular day it contained 13 feet 1 inch, or about 2 tons of water. 108 REPORT—1895. For several days the pointer of the pendulum had been fairly steady, pointing at division 70 on the scale of millimetres. What happened when the well was emptied is given in the table below. The photographic trace with interruptions in it when the light was removed is shown in fig. 7, Plate II. The movement of the pointer from 70 to 79 indicates a tilt of 1/36 and the direction of motion was as if a. load had been taken away on the well side, and the ground on that side had therefore risen. This may be explained by the fact that as the water came to the surface it was run into a gutter to flow away quickly down a hill. The pendulum remained between 77 and 82 until May 27, when the experiment was repeated. It started at 80, and in 6 hours and 40 minutes it reached 86, and here it has remained with a tendency to get higher but not to return. 3 Position of | Distance ; aay Time pendulum | to water ee ft. in. 21st 8.30 A.M. 70 36 6 | Taking out water for house S40 72 8.50 ,, Commence to empty well 9 Binion: 72 | 9.30 ,, 73 9.45 ,, 73 48 11 | Well empty excepting 8 inches. Water bubbling in OO 75 40 7 | Water rising 12.00 ,, 76 12.30 P.M. 37 8 ‘, i 4.00 ,, 79 Maximum deflection reached 5.25 ,, 79 36 0 | Water higher than at the commence- 7.10 4h ment 22nd | 7.30 A.M. (ae ap * 10 a i ‘ Not only was tilting produced by these operations, but as seen in the photograph tremors were induced. It might have been anticipated that by emptying the well and the subsequent inflow of water to refill the same—if in consequence of this operation a superficial movement took place—this would have assumed the form of a quaquaversal dip towards the well. What happened was exactly the reverse, from which it may be inferred that the motion of the pendulum was due to the removal of a weight rather than to the movement of the subterranean water. (n) Barthquakes. In the last column of the table showing the wandering of pendulums, the number of earthquakes which occurred on various days is given. These are the earthquakes which were recorded by seismographs in Tokio, and it is only one or two of these like the disturbances of March 22, when earth waves were produced, that are recorded by the pendulums. As already stated when speaking of the Kamakura records, although it is probable that most of these shocks were of local origin, this fact cannot be ascertained until the records accumulated at the Meteorological Department have been analysed. Two things, however, are very remark- able, the first being that at about the time of nearly all the shocks, pendulum A has shown abnormally large movements, and secondly there are only three occasions when the movements of A have been moderately ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 109 large that earthquakes have not occurred.. The tremor storms which were numerous in the early part of the year have no doubt obliterated many of the unfelt earthquakes to which the pendulums were sensitive. Notwith- standing this, there are a considerable number of disturbances on the traces, the record of which must be left for a future report. The most remarkable of these was recorded by pendulum F, which at the time was steady and producing a clear sharp straight line (see fig. 3). This was on June 3, when at 4.36 p.m. the pendulum commenced to move from side to side, and, with the exception of two or three intervals of about five winutes, it continued to move until 10 p.m. Although 14 points of maximum may be counted, the photograph represents what is practically a continuous earthquake of 5 hours 24 minutes’ duration. The picture is that of a series of small flat cones, each inverted, with their axes in one straight line. No displacement of the pendulum took place, and after the Fig. 3. About half actual size. The gap at or near noon represents an interval of one hour. disturbance it continued to draw the same thin line. I do not know where this or the other unfelt earthquakes originated. The rate at which the decided movements are propagated is from 2°5 to 4 kilometres per second, and there are reasons for believing that many of them, like that of March 22, originated beneath the bed of the ocean. (0) Tremors. In the extracts from the Journal (pp. 96 to 99) it will be seen that tremors or earth pulsations have often been recorded, and that some- times these were greater underground than on the surface. During the last two months they have been greater on the surface. Previous analyses have shown that they nearly always accompany a steep barometric gradient. They are sometimes marked when the daily curve is barely visible, but small tremors at least usually accompany these waves, and'they are more pronounced during the night and early morning, when the rate at which a pendulum is being displaced is relatively slow. The fact that small tremors were produced at the time the well was emptied is a fact not to be overlooked when considering their origin. I regret to say that a more careful examination of the tremor records must be left for a future report. (p) Observations at Yokohama and Kanagawa. As already stated, the instruments at Kanagawa (1) and (G and n) at Yokohama are underground, and stand on short brick columns rising from soft tuffrock. The softness of this rock may be judged of from the fact that _ when a person stands near one of the columns, the boom of the pendulum is deflected from 5 to 17 mm., from which it appears that, as a foundation to resist loading effects, the tuff rock is no better than a slab of concrete on the alluvium in Tokio. Owing to the collapse of the roof of the Yoko- hama cave, which caused a delay of two weeks, and owing to the fact that the clocks have been continually stopping, and good clocks cannot be found 110 REPORT—1895. in Tokio or Yokohama, the records from this place are extremely few. Those which have been obtained, extending over two or three days, show straight lines likefig.1, Plate II. There are neither daily curves nor tremors. From Kanagawa, although the cave is very wet and the conditions for observing very unfavourable, for about two months everything has worked satisfactorily. Like the Kamakura records they do not show tremors or daily waves, but they do show unfelt earthquakes and wandering. For example, on May 5 the boom moved as if by a N.E. tilting as much as 14’. This it reached on May 7. From this date it slowly returned to its starting point, which it reached on May 12. Small shocks occurred on the 2nd, 4th, and 6th. (q) Conclusions. Tnasmuch as the analysis of materials already accumulated is not yet completed, and as certain experiments require to be repeated or amplified, it is premature to formulate definite conclusions. All that can therefore be done is to outline the form which conclusions may possibly assume. Although I understand that Italian observers have found that tremors are as marked underground, even on the rock, as they are on the surface in Japan, this seems to be only true for the alluvium. Underground on the rock at three stations, with such instruments as I have employed, there has not been even an indication of tremors. Neither have daily waves been observed. All the pendulums, whether on the rock or on the alluvium, from time to time leave their normal position, moving for two or three days in one direction and then slowly returning. These movements, which have been called wanderings, sometimes indicate a tilting of as muchas 14”, Because these movements have often been accompanied by local earthquakes, it seems possible that they may actually represent rock bending, the earthquakes announcing the fact that resistances to the process are being overcome. Some of the wanderings noted on the alluvium may possibly be attributed to disturbances in the subterranean circulation of water after rainfall. Although the daily movement of the pendulums has been most marked by those which are nearest to water level, because they only show a single wave during the day, while the water in a neighbouring well rises and falls twice during the 24 hours, the daily wave cannot altogether be attributed to the movement of subterranean water. Because certain diagrams have shown a superimposed wave, it is possible that the cha- racter of the daily wave may now and then be influenced by subterranean water. Because a wave may be produced by relieving an area in the vicinity of a pendulum of a load, as, for example, by taking 2 tons of water out of a well which is 104 feet distant from pendulum A, and pouring the water away down a slope, it seems likely that the daily wave is produced by an action of this description. The action suggested is that which takes place every day when the sun shines or the wind blows across ground which is open and that which is covered, for example, by forests or buildings. By evaporation one area is rapidly relieved of a load, while the adjacent area loses but little. For example, experiment shows that on fine days an open grass-covered area 140 feet square in front of my house, which is 120 feet long and runs E. and W., loses in 12 hours about 5 tons of moisture. At the back of the house, where the ground is sheltered from the sun, evaporation is small. As confirming this view it . ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 111 is observed that pendulum A is steady on dull wet days, but on warm days the daily curves are well defined. Farther, although A and E move at the same time, they move in opposite directions, but each usually moves towards the side from which the greatest load is being removed by evaporation. III. Tue Toxio EartHquakeE oF JuNE 20, 1894, On June 20, at a few minutes past two in the afternoon, Tokio, Yokohama, and the surrounding districts were shaken by an earthquake which was more violent than any which has been recorded since 1855. On June 25 it was reported that in Tokio alone 33,940 buildings had suffered damage, some being entirely ruined, 140 persons had been wounded, and that 26 had been killed. In Yokohama, where many chimneys fell and houses were unroofed, 6 people were killed. When statistics are completed and it is known what has happened in other places these numbers will be increased. Small fissures were formed in the ground at Tokio in 96 places, many walls were shattered, while stone lanterns and tombstones were overthrown, twisted, or deranged. The following facts are taken or deduced from the records obtained at the Central Observatory and the University Laboratory, both of which are in Tokio, at a distance of about 1} mile from each other. To these are added observations from the Hitotsubashi Observatory, which is situated on soft ground lying between the Central Observatory and the University, at which places the ground is comparatively hard. Hitotsu- — Central Observatory |University Laboratory| bashi Ob- servatory Time . a F s .| 2b.4m.10s.P.M.| 2h. 2m. 30s. P.M. Duration 5 . P a 4h. 4m. 48s, 4 mins. 30 secs. 5 mins. Direction . N.E-S.W. N.E.-S.W. Maximum horizontal motion 76 mm. or 59 mm. 80 mm. 130 mm. Period of $3 1:3 sec. 2 secs. 1'5 sec. Maximum vertical motion 5 18 mm. 10 mm. 45 mm. Period of . 5 ‘ 1:0 sec. At the University for the first 10 seconds the horizontal motion was slight, when it suddenly became severe, reaching 80 millimetres. The severe motion continued for about a minute, during which time there were more than 10 pronounced movements. As the range of motion was outside the limits of seismographs with multiplying indices these were deranged or broken, and complete diagrams were only obtained at the University and Hitotsubashi, where there are seismographs without such indices, the recording surfaces for which are only set in motion at the time of violent disturbances. Until the diagrams have been carefully analysed I am inclined to think that the recorded horizontal motions may represent the angles through which the seismographs have been tilted, rather than the range through which a given point suffered horizontal displacement. Assuming for the present that these quantities are what they are represented as being, then at the University and at Hitotsubashi the maximum accelerations were respectively 400 and 1,000 millimetres per sec. per sec. Inthe Nagoya-Gifu earthquake of 1891, when nearly 10,000 112 REPORT—1895. lives were lost, the maximum accelerations, calculated on more certain data, varied between 3,000 and 8,000 millimetres per sec. per sec. At the University there is a seismometer, consisting of a number of iron shot, arranged on a ledge round the top of a strong post, beneath which there isa bed ofsand. These shot were not projected, but all of them, excepting one on the N.E. side, simply fell. The duration of the disturbance is of course that given by seismographs. Horizontal pendulums may have been tilted backwards and forwards for one or two hours. For some time after the shock it was observed that the Sunida River, which runs through Tokio, rose and fell as if its bed continued to be agitated. The direction of motion, as with nearly all earthquakes, was varied, and the direction given is that which was most pronounced. The times at which the commencement of the disturbance was recorded at places some distance from Tokio are as follows :— District Time. P.M. Tutensity Be Mores Yokosuka . Dek O20 Strong Numazu 23? 2b || 4 Utsunomiya 2 4 16 z Mayebashi ete 3G) » clocks stopped Kofu. 2/300 | 5 = Choshi Zueey 6009) Weal Nagoya 2 4 44 5 Gifu . 2) 4°28 kr Osaka 2 4 0 ” ” ” Hikone 2° oF te Fukushima Dede) 2H _ Aomori 256 40 Feeble Sakaye 2-10 ra From these times and the distribution of destruction it may be assumed that Tokio was well within the epicentral area. A remarkable feature distinguishing this earthquake from most others is that during the next three days instead of a long series of after shocks only three disturbances were recorded, The primary shock does not appear to have been accompanied by any sound, while one of the secondary shocks, at 4.25 p.m., on the 20th was preceded by a roaring sound. At many places telegraph and telephone wires were broken. Under- ground the pipes of the Yokohama Waterworks were caused to leak, drains were deranged, and there was a falling in of material in a railway tunnel. A curious fact communicated to me by my colleague Professor W. K. Burton is that in his house, where he was barely able to keep his feet while the shaking was going on, several decanters were not upset, but their stoppers were shot out. This is similar to what has occurred on more than one occasion with the lamp glasses at the Kannonsaki light- house in Tokio Bay. TV. MisceLLANeEous. In addition to the foregoing work two numbers of the ‘Seismological Journal’ have been issued and the manuscript of a catalogue of Japanese earthquakes between 1885 and 1892 has been completed. This catalogue gives the date, the time, the area shaken, and the position of the origin for 8,337 shocks. Appended to each shock are a series of numbers, and ‘ ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 113 a line traced through these, as shown on a key map, is an outline of the Jand area which was disturbed. The object of this catalogue, which is different from previous publications of the same description, was stated in the last report. Investigation of the Earthquake and Volcanic Phenomena of Japan.— Fifteenth Report of the Commuttee, consisting of the Right Hon. Lord Ketvin, Professor W. G. Apams, Mr. J. T. Borromtey, Professor A.H. GREEN, Professor C. G. Knott, and Professor JOHN MILNE (Secretary). (Drawn up by the Secretary.) ConreENTS. AGE I. The Gray-Milne Seismograph . - - ; ’ . . . . 118 Il. Observations with Horizontal Pendulums bs . - Sooeglal (a) The Instruments, Installation, Character of Movements 4 - idle (b) Daily Wave Records . : 5 : - 122 (ec) Tremors, Microseismic Disturbances, or Earth Pulsations : : 26 128 (d) The Slow Displacement of Pendulums.. (e) Periodic movements of several days’ duration, and wandering of 129 the pendulums. (7) The daily change in the epee o the uae ‘ ? ; . 130 (gq) The Diurnal Wave. ! H z Seal Hh (h) Tremors . : : : : : - : . | 139 (i) Meteorological Tables for Tokio. : A . 143 (j) Earthquakes recorded by Horizontal Pendulums in Tokio : : 147 III. Description of a Catalogue of 8,331 Earthquakes recorded in res 149 between January 1885 and December 1892. (a) History of the Catalogues . : “ : ° 5 : 5 . 149 (b) Explanation of the Catalogues . c : é Fi ; : . 151 (ec) Object of the Catalogues. 153 (a) Results already obtained or shown By y the Catalogue and Map of 155 Centres. IV. On the Velocities mith which Waves and Vibrations are propagated on 158 the Surface of and through Rock and Earth. (Compilation). Introduction. (a) Observations on Artificially Produced Disturbances. Experiments 159 of MALLET, ABBOT, FOUQUE and Livy, GRAY and MILNE. (4) Observations on Earthquakes. Where the nave paths have been 163 short: (MILNE and OMOoRI). Where the ware paths have been long: (NEWCoMB and DUTTON, AGAMENNONE, Ricco, CANCANI, Von REBERUR-PASCHWITZ. MILNE). (e) The Probable Nuture and Velocity of Propagation of Earthquake 170 Motion. The suggestions of Dr. C. G. KNoTT, LORD RAYLEIGH LorpD KELVIN. (d) The Paths Followed hy Earthquake Motion. Hypotheses of HOPKINS 173 and SEEBACH, SCHMIDT, and a sugaentien YY the writer. (e) Conclusions . : F 1 V. Miscellaneous Notes elacis to pee hathouiba, Se... 5 : 1 APPENDIX.—On Causes producing Movements which may be Mistaken foe 182 Earth Tremors. I. Tue Gray-MILNnE Seismocrapu. The first of the above seismographs, constructed in 1883, partly at the _ expense of the British Association, still continues to be used as the _ _ standard instrument at the Central Observatory i in Tokio. T am indebted to Mr. K. Kobayashi, the Director of the Observatory for the following table of its records :— 1895. I 114 REPORT—1895, | Catalogue of Earthquakes recorded at the Central Meteorological Observatory in Tokio between May 1893 and February 1894. | Maximum Maximum Period and | Period and Amplitude of |Amplitude of f a irec- | Horizontal Vertical at: No. | Month} Day Time Duration Fees Motion Motion ane of secs. | mm. | secs. | mm. 1894. H. M. S. M.S. | 1,421 ‘Vie 22 11 51 48 p.m. 0 30 Ew. slight slight | slow, weak 1,422! ,, 28 8 13 02 A.M. =u = = = =) | = slight 1,423 by 29 6 45 56 A.M. 5 1,424] Vis 5 | © 28 05 P.M. “3 1,425 9 14 4 59 52 P.M. -- i 1,426 a 20 5 16 52 A.M. 0 | — 03 0°35 — _ slow 1,427 2 Pa 2 410 PM. 4 48 S.W. | 13 76 | 1:0 18 | quick, strong 1,428 > ss 4 22 44 P.M. 1 45 W.N.W.| 1:2 0°6 _ — slow, weak ago}, A 93451 pMm.| 043 |W.N.W.| 0-7 | 06 slight J 1,430 a 25 5 15 36 P.M. 1 45 W.S.W.| 0°8 4:8 “4 : quick, weak 1,431 » 27 4 23 59 A.M. _ _— — _ - — slight 82 le iy 30 | 10 56 28 pM. = = = = See = 1,433] VII. 9 9 41 19 pM. — — — — — — i 1,434| ,, 10 | 433 Oam.| 045 E.-W. | 05 | 06 |e slow | 1,435| —,, 5 81328 am.| 1 34 E-W. | 06 | 0:6 = = } 1,436]; ,, 12 0 54 28 A.M. = = = = she slight : 1,437 5 17 | 11 121 pM. SHG N.W. | 07 17 05 0-6 quick, weak 1,438 5 25 10 24 2 A.M. 0 56 N.W. 06 08 05 0-2 slow, weak 1,439) VIII. 1 8 44 35 A.M. —_ E.-W slight — —_ weak 1,440 5 “4 4 013 P.M. — — — = —_— — slight 1,441 ” 29 7 55 18 pM, 6 1 N.N.E. | 1:8 1:8 _ — slow, weak | 1,442 IX. 12 9 015 PM 0 57 N.W. 06 O7 slight FS 1,443], 13 | 340 3 PM = et een eee slight : 1,444 = 17 8 53 56 P.M 1 25 S.S.W. | 1:2 05 — —_ slow, weak 1,445 * 21 8 2 36 AM _— — — — — = slight 1,446] ,, » | 75816 an = eee) ee Ny ae 4 1,447 = aS 10 25 41 pM tee — —_ — — — s 1,448 99 24 4 32 28 P.M — — _ -— — — i } 1,449 sa 29 7 24 43 A.M = — — — — — a ; 1,450 X. 7 830 3 PM 8 0 N.W.| 2°3 43°7 17 2°4 quick, strong 1,451 5 8 9 48 28 AM == —— a — == slight 1,452 22 5 36 31 P.M — E-W. — —_ — — slow, quick 1,453 XI. 11 8 54 4 P.M — — —_ — — = slight 1,454| ,, 15 | 9 42 39 pm = = = = = i 7 1,455 5 18 1 813 PM 1 38 N.-S. 13 0-2 — — slow, weak 1,456 ia 21 10 42 14 pM —— — — — = Ss slight 1,457 # 22 8 13 53 AM — = — = = = eS 1,458 3 28 1 5 22 aM 3 56 E.-W. | 30 15 -- _ slow, weak 1,459 a a9 6 44 51 A.M = — — — == — slight 1,460 an 30 8 30 57 pM hey é W.N.W.| 0°6 5°09 0-2 old quick, strong 1,461) XII. 1 6 36 59 pM 0 49 N.W. | 08 0-7 — -- quick, weak 1,462 ay 16 17 0PM — — _ — = Ee slight 1,463 iy 23 3 5 1PM — —_ — — = bos F 1,464 sk 28 1 430 am — — — — = = ef 1,465 “ 31 10 7 42 AM 3 5 W.N.W.| 1°6 1:8 — _ slow, weak 1895. 1,466 ne, 6 tA ei: _ — — — —_— — slight 1,467 5 10 343 5 AM. _ — —_ — f< = E 1,468 Es a 617 5 AM. — — — = = a es 1,469 Ss ht 5 53 30 P.M. — — — 15 = = is 1,470 55 14 1 9 .9 AM, — = —_ = ,%, <— = 1,471 53 18 914 3AM 315 |W.N.W.} 0:9 14 0:3 0-2 quick, weak 1,472 ay i 2 54 35 AM — =, —_— —= = _— slight 1,473 My ‘ 10 48 24 P.M. 4 4 |N.N.W,| 0:9 41 0-7 |11-0 quick, strong 1,474 a 5 1117 4PM a == se = = a slight 1,475| ,, 19 | 020 44 aM. -- = aie | pees | ee - 1,476], 7 327 7AM. es = = = = fee i Arti cs 9 43 55 PM. = — 2s a SAB ng Ry a 1,478 > 21 4 52 47 aM. — — A. = =. oe 1,479 ” » 8 29 22 a.m. 0 10 N.S | 0-7 0-2 slight quick, weak 1,480 5 s 7 31 22 P.M. — — = a — =: slight 1,481 + m5 919 28 PM. _— = = — +25 = > 1,482 » 23 8 56 10 A.M. ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 115 ae ae ae OF RABBAQU ARES —-ompionuad,2 Maximum Maximum | Period and | Period and | Amplitude of |Amplitude of) | . irec- | Horizontal Vertical | Tat off No. | Month | Day Time Duration puree Motion Motion N ed aH secs. | mm. | secs.) mm. | ! | 13895. H. M.S. M.S | 1,483 1G 23 2 12 30 PM. 210 N.-S 0-7 2-4 06 | 06 quick, weak |} 1484) ,, 24 830 9 AM. == = slight | i5| |, «| 25 | 11 4442 ae | — aie eee dient ES NE = 1,486 ine 3 1 49 15 P.M. — — — = — — 5 | | 1,487 a 4 6 30 25 A.M. = — = — = — Pe + 1,488 pa 5 | 1 46 36 P.M. — -- _ — = — f { 1,489 “ 17 5 37 10 A.M. — — = a= -= = Fs | 1,450 as 18 052 O AM. — —_ = — == — ¢ | 1,491 » » 8 37 33 A.M. — — — — — — rn 3,492) 23 | 11 326 aM. _ = = = = ees = 1,493 3 BS 1114 8 A.M. 0 12 E.-W. | 0°9 0-2 — _- slow, weak } 1,494 is 28 | 10 39 28 a.M. — — = = — — slight ' 1,495 IIf. 1 5 33 48 P.M —- os | 1,496 5 3 4 14 50 P.M = ~ ES. = = ar i 1,497 Ff 9 0 28 19 pw =e ae ws nE ~~ =, a i 1,498] ,, 15 7 19 52 pM = = = a Ey. As 1,499 - 16 0 423 PM 0 58 E.-W. | 0:8 Or4 aa —_— —_ \ 1,500} ,, 20 1 5 26 pM 0 42 E-W.| 07 | 05 a = | 1,501 » 27 2 8 OPM ” | 1,502 ” 30 3.35 39 AM _ _ — — — — 9 | “| 1,503 + 31 8 53 41 A.M.? — — — — — — | perhaps due to | } wind 1,504; IV. 2 3 12 34 P.M — -- — — — — — 5} 1,505), 3 853 19 AM mf 2 = = a | ee a | 1,508} 3 | 74944 pMm.| 158 N.W. | 07 | 1:3 | 06 | 0°3 = 1,507| ,, 4 | 14132pm.] 1 0 |N.N.W.| 1:2 (igen |) ee ea 1,508 5 5 310 O A.M. 1 8 N.-S. | 0:7 03 — — — 1509 ” 5 915 39 AM. => —_— _— — — slight | 1,510 ” 5 [:11 24 3 aM. -- — = — _— — pA ; 1511 A 6 4 32 36 P.M. — — = = a x | 1,512 Ry 9 312 7 AM. 1 8 N.W. 0-7 1:2 —|/—- _— 1,513 a 12 3 7 28 AM. 0 52 WN.W.| 0:3 0°3 _— = = | 1,514 35 12 10 21 29 P.M. _ _ a —_ —|—- 3 1,515 = 13 10 41 46 A.M. - _ — — — — a 1516) 17 1 53 38 P.M. = = as =e ie é. 1,517 ” 22 7 9 3 AM. _ —_— — — es —, et SIS | 4 93 | 3 21 59 aM. = = = = as |} ft »} 1,519) ,, 25 016 19 A.M. = = = 2s = |= 5 | 1,520 ” 27 358 5 P.M. — = _— — — _ 7 ) 1,521|- V. 1 | 225 1am. = = a ee a is 1,522 3) 2 415 7 AM. _ —_— — — — — 35 II. OBSERVATIONS WITH HorIzoNTAL PENDULUMS. (a) The Instruments, Installation, Character of Movements. Since 1893 nineteen sets of records have been obtained from horizontal pendulums installed either in Tokio or its vicinity. In the following description the different installations or sets of instruments are indicated by letters of the alphabet. The instrument at A, which was in my house, occupied the same position from the commencement of the observations until February 17, 1895, when it was destroyed by fire. The instruments at other stations were kept in position until they had given continuous records for a period of from one to four months, when they were moved to a new locality. Although these periods may appear short, they seem to have been amply long to determine the general character of the move- ments to be expected at any given station. Instruments within a mile of 12 116 REPORT—1895. my house were visited every day, while those at a distance—as, for ex- ample, at Kamakura (C and D)—were visited at least once a week. Not- withstanding the time taken in making journeys to the more distant stations, one of which occupied from ten to twelve hours, because the clockwork kept going for a week and the lamps burned for two or three days, it was often possible to keep six instruments working simultaneously. The notes and photograms for 1893 and 1894 obtained from stations A, Fie. 1.—Map showing Positions of Pendulums. Scale about wlio LDistarues uv yards trom J-H6 R-3500 N-/200 @dI5UU E, F, C, D, G, H, and I, which were destroyed by fire, are fortunately described in the fourteenth report to this Association. In order to show the relationship of these observations to those made during the past year at A, H, I, and the remaining eleven stations, they are briefly referred to in the following notes. The sensibilities of the different instruments which are described in the Report for 1894 are indicated by the number of millimetres the end of the boom was deflected by turning one of the screws in the bed plate ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 117 one degree. The pitch of a screw was one millimetre, and its distance from the axis on which the bed plate was tilted may be taken at 220 millimetres. All the instruments excepting A had usually a sensibility of 1° for 3 mm., which is approximately equal to a tilting of 1” for each millimetre of deflection. Occasionally the sensibility was increased two- fold or threefold. The reason for this indefiniteness respecting sensibility is that the notes relating to the calibration of the instruments were burned. The chief value of these determinations is to give angular values for the diurnal wave, and because it will be shown that this is a quantity with large variations depending upon locality and weather, the necessity of accurate measurements becomes more apparent than real. The Pendulum at A.—Sensibility, September 26, 1894. 1°=12 mm. or 1 mm.=0'20. This instrument, which was adjusted to have a sensi- bility twice or six times greater than the other instruments, was installed in my private observatory on a massive well-built stone column resting upon a bed of concrete. ‘Towards the east and west it was protected by 60 feet of building, but to the north and south by only about 10. feet. The only window in the room, which was on the south side, was always closed by a curtain on the inside anda solid shutter upon the outside. The reason that it was oriented to record N.E. and 8.W. motions was because, as was explained in the last Report, there were reasons for believing that in such a direction earthquake and other motion had a maximum. The daily movements were often eclipsed or made indefinite by the occurrence of tremors. When they were visible, although on one occasion they were represented by deviations of 8 mm., it was rarely that they exceeded 2 or 3mm. In many instances it seems that a second wave was superimposed upon the ordinary diurnal disturbance. Excursions towards the N.E. were usually completed between 5 and 15 hours, while the 8.W. motion ended between 0 and 3 hours (fig. 6, p. 134). Pendulums at C and D.—These were installed upon rock in a cave at Kamakura, about 27 miles distant from the pendulums in Tokio. One of these recorded motion in the direction of the dip of the strata, and the other in a direction at right angles to this. Their records are described in the Report for 1893-94. Pendulums at E and F.—These pendulums were in directions N.E. and N.W. or parallel to C and D. The N.W. booms were parallel to A. The installation was in an underground chamber, where as at Kamakura the daily change in temperature was practically unappreciable. These records are described in the Report for 1893-94. Pendulums at G and H.—The pendulums G and H were placed on the rock in a cave at the Yokohama Brewery. Their orientation corresponded to that of C and D or E and F, and their records are referred to in the above-mentioned Report. Pendulum at I.—This pendulum was in an exceedingly damp cave at Kanagawa, about three miles distant from G and H. Its boom, like that of A, pointed towards the north-west. The few records obtained from this station are described with those of the above-mentioned three stations. The Pendulum at J.—Sensibility, August 18, 1894, 1°=6°5 mm., or 1 mm.=0/"39. January 5, 1895, 1°=3 mm., or 1 mm.=0'"80. This was an aluminium boom which, with its plate and index, had a total length of about 4 feet 9 inches. Its cast-iron stand rested upon a slab of slate upon the top of a short brick column, which rose from a layer 118 REPORT—1895. of concrete covering a bed of gravel rammed into the natural earth. It was covered by a coarse wooden case. The whole arrangement was shel- tered by a small wooden hut, 9 feet long and 7 feet broad, and up to the eaves 6 feet in height. This hut, like all the other huts, admitted so much light that the photographic films had to be changed at night. Currents of air came in freely, and, as might be expected, there were considerable fluctuations in temperature. On the west side the ground was flat and open, and it was also fairly open towards the north and south. On the east side, however, it was sheltered by a small hill and trees, behind which came a pond, more trees, and then instrument K, which had a small tract of open ground upon its eastern side. The westerly motion, which varied from 5 to 40 mm., usually took place between 18 or 21 hours and 6 or 9 hours, that is to say, the pendulum commenced to move towards the west at about 6 or 9 a.m., and continued this motion until 6 or 9 p.m. (fig. 7). During the night the easterly or return motion was gentle, and usually less than the motion towards the west. On wet cloudy days no curves were visible. Tremors were not marked at this station. Comparing the N.E. and8.W. motions of A with the E. and W. motions at J in 24 instances these movements were completed at about the same hour. In 21 instances, however, there is a difference between them of from 5 to 10 hours. An experiment which was made at this station was to dig a trench round the hut on its south and west sides. This was 5 feet in depth, while its distance from the column was about 10 feet. The only effect that this produced upon the daily diagrain seems to have been that the points of inflection in the curve became somewhat sharper, the range of motion of the pendulum remaining constant. Pendulum at K.—Sensibility, September 20, 1894, 1°=4:5 mm., or 1 mm.=07:50. November 21, 1894, 19=3 mm. The installation of this instrument, excepting the fact that it was exposed to open ground towards the east and north, and sheltered by a grove of trees upon the south and west, was similar to that at J. The instrument itself was like that at J. The diurnal movements had a range of from 4 to 40mm. The westerly excursion usually commenced at 5 or 6 a.M., and continued until about 4 or 6 p.m. (fig. 8). The motion was therefore about one hour in advance of that at J, which roughly corresponds to the difference in time at which ‘the ground in their respective vicinities were exposed to the morning sun. Comparing the hours at which the easterly and westerly motions of J and K were completed in fifteen cases, they closely agree. When these hours do not agree, K has usually reached its western limit from one to four hours before J. In two instances it completed this movement seven hours after J, while in two other cases one pendulum has been near its western limit, while the other has practically completed its movement in an opposite direction. Tremors were not marked. The object in placing J and K, which were 275 yards distant from each other, on opposite sides of a small grove of trees, was with the expectation of finding that at the same time they moved in opposite direction. It is seen that the expectation was not realised. Pendulum at L.—This instrument, which in construction is very like ee a ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 119 that at A, and is similarly oriented, stands beneath a wooden case on the concrete floor of a cellar in the north-western corner of the Engineering College at the Imperial University. It is without recording apparatus. Its pointer floats over a scale, and its position is noted every day about noon. When first set up on September 19, 1894, it had a period of 28 seconds. Its movements, which are indicated in millimetres, the sign + meaning displacement towards the west and — towards the north and east, have been gradual. They were as follows :—- 1894, During September —lor2 October 1-October 21 —2 October 21—October 31 +2 November 1—November 24 —7 November 24-December 3 +7 December 3—December 20 —2 Pendulum at M.—The object of this pendulum, which was installed upon the same column as A, was somewhat different from that of the others described in this series. It consisted of an aluminium boom loaded at its outer end with a weight of about 300 grms. In addition to this it carried a small vessel of ink from which a capillary tube projected, making the total length of the boom about 4 feet 6 inches. This tube was balanced, so that it barely touched the surface of a band of paper moving at the rate of about 8 inches per hour. The force required to deflect the boom one millimetre when applied at a distance of 4 feet from the agate pivot was approximately one milligramme. Before it was destroyed by fire it recorded the occurrence of several local earthquakes, and, considering its sensibility to tilting, it is probable that it would have recorded the gravi- tational elastic waves of disturbances originating at great distances. A necessary adjunct to such an apparatus in order to obtain an open diagram is the addition of a quick speed feed for the paper, which must come into action directly the pendulum commences to be deflected to the right and left of its normal position, Such a device was designed for me by my colleague, Mr. C. D. West, and it apparently works more satisfactorily than the original form of this kind of apparatus which is found in the Gray-Milne seismograph. Pendulum at N.—Sensibility, January 5, 1895, 1°=3 mm. January 25, 1895, 1°=2°5 mm., or 1 mm.=1-03. The pendulum used at this station was originally at K. The hut was situated on the western side of Uyeno Park, near to its southern extremity. It was sheltered by trees on its eastern and southern sides. On its western side, where it was open, there was a steep scarp leading down to the Shinobadzu Pond, which lies ‘in the bottom of a flat open valley. A, J, and K were on the plateau on the opposite side of this valley, the heights of these stations being about 50 feet above the flat plain on which the greater portion of Tokio is situated., The movements were usually small, seldom exceeding 7 mm. The westerly movement commenced from about 6 or 9 P.M., and con- tinued until about noon next day ; that is to say, that about the tume when the instruments wpon the opposite hill or plateau were going eastwards, the instrument at Uyeno went towards the west, and vice versa (fig. 10, p. 136). Pendulum at O.-—Sensibility, January 12, 1895, 1°=1:°5 mm. January 22, 1805, 1°=1:5 mm. Station O was situated at a place about 20 yards to the south of J. It only differed from the instrument at this latter station in the fact that the boom of the pendulum pointed from west towards the east, and it therefore recorded north and south motion. 120 REPORT—1895. During the few weeks it was used, it showed a small but regular diurnal fluctuation, being farthest north about 3 or 5 p.m., and farthest south between 9 a.m. and noon (fig. 12, p. 137). Pendulum at P.—Sensibility about the same as N. The instrument used at this station was the same as that used at N and K. The hut faced an open space about 70 yards square on its northern side, but on all other sides it was shaded by high trees. For one or two hours about mid-day a few rays of sunshine reached the roof of the hut and the northern side of the open space. That the ground within 20 or 30 yards of the hut had but little sunshine may be inferred from the fact that after a fall of snow this remained upon the ground for ten or fifteen days. On open ground the snow disappeared in two or three days. During the day this would slightly thaw upon its surface, and at night it would freeze. About 50 yards to the east, a bluff sloped down to the Tokio plain. Observations were only made between January 14 and February 4. The movements were extremely irregular, the most peculiar happening between January 14 and January 26. On these days, excepting the 23rd * and 25th, during the night the pendulum made a rapid excursion towards the east, returning to its normal position some time about noon on the following day. These abnormal movements took place upon nights when Fig. 2. 2.20 Liv 2.50pm Jar l5 1215 2 ee gee ’ Tan. 13 (895 : ere Lastwardsis unknown it was unusually cold, and therefore they may have been due to the freez- ing of moisture beneath or in the vicinity of the column (fig. 2). Pendulum at @.—This instrument, which is in charge of the Meteoro- logical Department, is as well installed as the pendulum at A. Jt stands. on a stone column in a dark room in the same building with a self- recording electrometer. The boom, which at first was partly made of lacquered bamboo, but which has been replaced by one of aluminium, points from north to south. Immediately outside the room there is one of the castle walls sloping down to a deep moat, beyond which comes the plain of Tokio. The diurnal movements are slight, but decided, the westerly excur- sion being completed at from 3 to 6 p.m., and the easterly at about 6 A.M., which corresponds to the motions at J and K. Tremors are slight. Pendulwm at R.—This pendulum was set up in a hut in the garden at No. 17, Kaga Yashiki, Tokio. At a distance of about 5 yards on its western side a steep bank leads down to a road, which joins a second road at right angles on the north side of the hut, about 30 feet below the level of the garden. The instrument is intended to act as a seismograph, sensitive to slight vibratory motions, while from the length of its boom, which is about 3 feet, it is also able to record slight changes in level. The first 2 inches of the boom is a small metal tube, at one end of which there is an agate cup. This boom is continued by a reed, at the end of which there is a ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 12] black filament of straw. To balance the weight of the reed and straw a light arm, resting upon a pivot on the underside of the brass tube, carries. at its extremities two smal] weights. Assuming the pivoted mass, which has a considerable moment of inertia and but little weight, to be the centre of oscillation of the system, which is held in a horizontal position by 2 thin wire tie, then the arrangement is that of a conical pendulum seismo- graph, having a multiplication of about twenty, and without the friction of a writing pointer. The black hair at the extremity of the boom floats above the slit in the box containing the drum, carrying the photographie film, which moves at a rate of 2 inches per hour. The resulting diagram is a white line showing the position of the shadow of the hair-like filament. A modification of this instrument was to reduce the length of the boom to 2 feet, and because the trace given by the shadow of the filament at the end of the boom was wanting in sharpness, the filament was re- placed by a thin plate of mica about half an inch square, with a small slit in its centre, similar to that used in the larger apparatus. Because the floating plate attached to the boom does not cover the whole of the slit im the box above the drum carrying the photographic film, the diagram is a black line given by the spot of light from the crossed slits, bounded on the right and left by a black band, the irregularities on the inside edges of which correspond with the irregularities on the central line. Every hour a separate clock depresses on one end of a balanced lever, at the other end of which there is a light vane which rises in front of the lamp, and cuts the light off for one minute. The result is that the central line (when there are no tremors), and the two bands at all times, are transversely marked by a distinct white line. Not only do the bands indicate time, and repeat the sinuosities and other movements shown on the central line, but by the presence or absence of striations they immediately show whether the clock driving the drum has been working regularly. Instead of cutting off the light from the lamp, the light is now cut off the edge of the fixed slit by the hour hand of a watch moving horizontally across the same (fig. 3). Fie. 3. An experiment made at this station was to obtain diagrams on films, which only moved at the rate of 75 mm. in twenty-four hours, or 3 mm. : per hour, which, from the results obtained, appears to be a suitable speed for recording diurnal waves and earth tremors (fig. 9). The western elonga- tion is completed rather suddenly between 7 and 8 a.m. (nineteen and twenty hours). The eastern movement, which is performed with extreme irregu- larity, is ended about 4 p.m. The amplitude of this wave is about 30 mm. 122 REPORT—1895. During the day, or from 7 a.m. until about 9 p.m., tremors are absent, but they occur in a very marked manner between 9 p.m. and 7 A.m., when they suddenly cease (fig. 9). The central part of fig. 3 shows a white band the width of a small plate of blackened mica at the end of a reed boom. In the mica there is a broad and a narrow slit,which correspond to the broad and thin lines in the diagram. The object of the broad line is to obtain a photogram, when the boom and its plate of mica are displaced rapidly, at which times sufficient light may not pass through the narrow slit to affect the bromide paper. When the motion is slow the fine slit gives the best definition. The vertical white marks at distances of 41 mm. apart are made by the pro- longation of the minute hand of a watch crossing one end of the fixed slit every hour. If the instrument be disturbed at known times, and the times at which these disturbances took place be determined by the irregularities produced on the broad and thin bands, the errors in these readings vary between three and twenty seconds. Should the paper move irregularly, this is shown by differences in the length of the spaces representing hours, while the times at which retardation or acceleration took place are shown by vertical striations in the broad black bands. This is the form of recording surface which I am using to obtain photo- grams of movements due to earthquakes. It is not suitable for tremors or daily waves. Pendulum at S.—This pendulum, originally at N, commenced its records on April 24, 1895, at the Agricultural School at Komaba, which is five and a half miles distant in a 8.W. direction from the University. Komaba is situated on a flat plateau, and the nearest irregularity in the contour of the ground from the instrument which stands in the middle of a field partly covered with corn is at a distance of about half a mile, where there is a small valley. The soil is so light and dusty that a walking- stick may be pushed into it for a depth of two or three feet. Beneath this comes a red earth. The records show tremors, but they are small. A westerly motion of about 5 mm. is completed at about eighteen hours, or 6 A.M., and an easterly movement of equal amount at about three hours, or 3 p.m. (fig. 11, p. 137). On the 8.E. side of the instrument the ground is bare, and during the day the pendulum moves to this side. (b) Daily Wave Records. In the following tables the localities or instruments are indicated by capital letters. The times at which an instrument completed its N.E., S.W., E., or W. excursion are indicated by hours, 0 or 24, corresponding to mid-day, and 12 to midnight. The figures in brackets give in milli- metres the amplitude of the displacements. When a dash takes the place of hours it means that the displacements were too small to be measured, or that the diagram was a straight line. When the space for hours is left blank, it signifies that for some reason or other, either that no diagram was taken or that it has been lost. A record like 9-15 on October 15 means that the S.W. motion of A was completed between nine and fifteen © hours. ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 125 Daily Waves. ! | . 1 | J ! K 1 | | } vi i | Remarks i | B | w. } E. | W. | + | | } :i f 1894. } October 13 .} 9(3] | 19(3) || 12¢7] | 23071 || ay, 14. 6 [3] 19[3] || 6 [5] 23 [5] 5 es 15 3 9-15 [3] || irregular 6 \ Pde 2.) 15 [8] » FA ely. 21 [8] / | me 18. | 3-6'(5] 15=91 18 [35] gs very | slight 5-12 [35] | 3-6 | 19 [15] 18 [25] | » 20. ” » | 6 [15] 3-6 19 [8] + Coal hal 6 [8] |! 9 13 18 [18] 18 [12] Wa kee: 9 13 | 6 [18] || 6 [12] 18 24 23 [14] 0 | 23 [18] Mw ..23 . 5 11 0 6 [14] | 4[8] | 16 24 21 [5] || 18 [12] pect . | 15 [5] 25 [5] 6 [5] Irregular and || | broken | ’ 21 [18] vel ebb 9 15 6-15 [18] i 18 24 23 [6] | 26 6 6 [6] 6 21 [6] 21 [4] ae | 6 [6] slight | | November 4 18 [15] 21 [40] | The deflections for A a, 5 4 4[15] || 4 | are too small and ir- ‘ 15 21 [18] | 18 [40 2] regular to be relied oH 6 6 | upon. : 18 15-21 [14] | J does not change much as 7 6-9 || between 2 and 10, and 18 21 [14] again from 15 to 16 a 8 6-12 || hours. 22 [14] N The motion of K is more ay 9 6-12 uniform without 21 [10] periods of rest. BS 10 6-9 | 15-21 [18] a 11 small ch 12 21 , J no wave, but tremors x, 13 10 24 6-9 at 21 and a westerly 21 [20] tendency. a 14 12 21 6-9 21 [19] 4 15 6 21 [19] » 16 6-9 18 [15] “4 17 6 ” 18 6 From 20th to 21st and 18 [20] 24th to 25th were on 19 4 9 5 [5] times of rain, and J 12 24 [15] 12 to does not show a daily > 20 7 0 22 wave. 12 0 With K from the 19th ” 21 3 and 7 6 to the 20th at 22 hours 6,14 || 19 [28] 18 [40] where there was rain, hiss 22 3 6 the daily curve is q 17 19 [23] 15 [40] absent or small. o> 23 9 i 21 15 [40] van 24 0 0 no diagram 0 ) Machine K was moved toN. 124. REPORT—1895. DAILY WAVES—continued. | A J | N | — | Remarks N.E. S.W. E. | W. | E W. | 1 1894 November 25 22 ¥ 26 5 9 [30] 12-15 18 22 24 ” 27 9 [30] 15 21 24 = 28 5 6, 12 [20] | 18 9 [5], 21 9 29 6 9 [20] 15-18 12 24 24 The diagrams are fairly ” 30 4 [12] straight during a 12 heavy tremor storm. December 2 4 [4] With J no motion from 24 21 10 to 21 hours or | 3 3 9 [15] 9 during the night. The 15 [5] 21 24 daily wave occurs ‘5 4 5 [10] 8 or 9 during the time that 15 [2] 12-20 24 the ground is un- = 5 19 5 [10] 6 equally heated on the 15 12-20 24? two sides of the hut. - 6 7 5[10] || 4-15 14 19 10-21 24 5 7 0 5 [10] 6 12 12-23 “s 8 0 0 24 0 0 Ps 9 11 0 18-24 24 0 4 10 12 0 9-12 21 21 | For J no daily wave os ll 5 6 [20] | from the 8th to the 18 19 10th at 21 hours when + 12 6 [20] there was rain. Very 18 little motion between *3 13 5 5 [15] | 15 and 21 hours. ” 14 ? 8 [15] | én 16 6-12 straight 24 A 17 18 6 [12] 6-9 24 21 21-24 [3] “5 18 9 18-21 6 [10] 5 18-24 [5] on 19 21 6 [10] 6-9 18-21 [4] | » 20 off the film 9 | » 21 [4] 3 21 21 a 9 » 23 [4] 3 22 6-9 a 6-9 23 [4] * 23 mp 6 [20] 15 23 [5] 5 24 6 [20] 6 24 23 [4] 2 25 7 5 [12] 6 9-24 15-24 [7] | = 26 5 [12] 7 9-23 18-24 [7] | . 27 12-16 [21]| 12-18 . 23 24 [3] 28 6 7 [3] 15-21 [5] 18-21 24 24 [5] | a 29 6 ” 30 small | ] 12 \ 12-15 For J from 15 to 24 |) 24 | hours not much mo- | os 31 | 1 8[12] | 6-9 tion. The daily curves | | { are sudden. | 15 18-21 N gives smooth flat } waves: | ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 125 DAILY WAVES—continued. A J j N = NE. | SW. Deeg bee es aaa Remarks | 1895. January 1. 23 1 7 (10) 6 15 18-21 m3. 9-12 5 24 23 21 x ae 5 || 6 [15] 6 | 18 1 18-21 » 4. 5 J | 12 | 18-21 | ” 5 ‘-\ - i. 6? 21 : 7. 6 15-21 ; 3. Sic |) 18 4 9. straight H oD: | A dz Oo | NE. | S.W. Ber] in We a aes Beatie 6 |; On 13th at 14h, 20m, 18-21 The curious movements 15 18 moved quickly east- 2-6 | of P which are large 0 5 wards off the scale. 0-3 18-24 | displacements, taking 14 19 It returned on the! 30 minutes or 1 hour 0 6 14th at 3h. but! 24 for their completion, 14 went off again at 18 appear to have taken 0 8 12h. 15m. to return place on frosty nights. 16 24 again next day at O gives a smooth curve 2h. 30m. It left the with an amplitude of scale again at 1Lh. 4or 5 mm. 30m., and move-| ments seem to have continued during | the week, the pen- dulum being steady | and on the scale from about 3 to 12 hours Up to the 20th the}! On the 20th it went 5 19 trace is practically|| quickly eastward a straight line at 7h. and returned to go westwards at bo 18h. 30m. Passed to the east on the 21st at 12h. 30m., and returned onthe 22nd at 2h. 18m., when it was steady until 15h. 34m,, when it went east- | wards. It was | steady from the 23rd to the 25th, | when at 15h. it went | again eastwards. Returned at 3h, on | the 26th and re- mained steady | 0 cv) 0 21 The wayes on O are de- 23 || cided and regular. It 18 24 8 3 1Z is difficult to determine 12 19 the hour for the south- 6 12 0 4 18 ern elongation, 18 24 18 24 9 18-21 0 3 21 15°5 off film } _ — 23 4 15-18 _ — = = Rain. 15 no curves 12°15 off film towards diagram bad east returned at 23 hours irregular and then no diagram 126 REPORT—1895. (c) Tremors, Microseismic Disturbances, or Earth Pulsations. In these tables the instruments or localities are indicated according to the letters of the alphabet. The hours between which tremors were marked are, for example, given thus, Oct. 13, 3 to 24. The times at which they attained a maximum range are given thus, max. 15 to 18. 0 or 24 indicates mid-day. The small tigures in brackets give in millimetres the range of motion of the pendulum, as shown upon the photograms. Date A J K Remarks 1894. Oct. 13 | 3 to 24, max. 15 to 18 (5) From the 13th to the Slight tremors be- | With the ex- 14 | 0 to 6 (2), 15 to 24 (2) 21st very slight tremors, | tween the 18th and | ception of the 15 | 0 to 6 (1), 12 to 24, max. 19 (3) but there are three | 19th only, and the | 13th when there 16 | 0 to 3 (2), 18 to 24 (2) decided diurnal waves | easterly sinus of | was rain the 17 | 0 to 6 (2), 15 to 24, max. 19 (4) | the easterly sinuses of | this day agrees |large tremors 18 | 0 to 6 (2), 12 to 24, max. 19 (6) | which on the 17th, 18th | with the records of | andlarge waves 19 | Oto 1 (1), 12 to 24, max. 22 (4) | and 19th coincide with | J and thelargetre- | occur on the | 20 | 0 to 24, max. 18 (4) the maximaof tremors. | mors of A on the | fine days. The largest wave co- | 18th incides with the most pronounced tremors on the 18th 21 | Oto 6 (0), 9 to 21, max. about | 15 to 21, max. 19 (3) 14 to 17 (3) On the 26th, 18 (5) 27th, and 28th, J 22 | 12 to 24, max. 18 to 21 (10) 20 to 24 (2) 0 when there 23 | 0 to 3 (5), 8 to 24, max. 18 to 21 | 15 to 18 (2) 0 were no. tre- 10 mors, the daily 24 | 0 to 4 (5), 6 to 24, max. 15 to 21 | 6 to 21, max. 18 (3) Off scale curves of J and (15) K are feeble. 25 | 12 to 24, max. 18 to 21 (10) 12 to 18 (2) * _ 26 | 0 to 6, trace of trems. about 18 0 0 _ 27 | About 21 a trace 0 0 _ Noy. 4 | 7to10(4) ~- — — 5 | 15 to 24, max. 15 to 21 (9) 9 to 18 and 21 to 23, | About 18 slight = | slight 6 | Oto 3 and 9 te 24, max. 18 to 21 — Diagram ceases _ (12) after 6th 7 | 13 to 24, max. 18 to 21 (7) 12 to 21 (2) — _ 8 | 15 to 18, max. 18 (3) 18 slight — — 9 | 18 to 23, max. 21 (3) — — _ 10 | 12 to 21, max. 18 (10) -= —_— — 11 | 12 to 24 small 9 to 21, max. 19 (2) Slight llth to noon 12 | 0 to 22, max. 18 (10) 12 to 21, max. 18 (3) No diagram of the 13th 13 |} 12 to 22, wax. 18 to 21 (8) 9 to 21, max. 19 (3) —_ clouds and rain. 14 | 12 to 21, max. 18 to 21 (6) 12 to 19, max. 17 (2) _ Although there 15 | 13 to 22, max. 18 to 21 (5) 6 to 21, max. 18 (2) — are no daily 16 | 15 to 24, max. 18 to 21 (6) 6 to 16, also 21 to 24, _ curves, tremors | max. 15 (2) oecur with the morning _fre- quency. Tre- | mors are marked . while the pen- dulum is moy- ing eastward and during its comparative rest of 15 to 21 hours. 17 | 0to6 0 to 6 -— Windy morning. 18 | 11 to 23, max. 16 to 21 (9) 6 to 18, max. 12 (2) No record — 19 | 17 to 22, max. 19 (4) 12 to 16, max, 14 (2) 12to16,max.14(2) | J and K for 20 | 8 to 11 (2), 18 to 21, max. 19 (3) | 9 to 11 and 13 to 18, | 6 to 9and 16 to 17, | 19th to 20th no max. 17 (1) max. 15 (2) © curve, but there are tremors, 21 | 18 to 21, max. 19 (2) 15 to 19, max. 18 (2) 0 For 20th to| © 22 | 15 to 23, max. 21 (2) 0 0 2ilst on J no curve, but tre- mors. 23 | 18 to 23, max. 21 (4) 0 0 — 24 | 12 to 24, max. 18 and 24 (5) 0 0 — oe ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 127 TREMORS, MICROSEISMIC DISTURBANCES, OR EARTH PULSATIONS—continued. Date 0 to 21, max. 12 (4) 16 to 22, max. 19 (5) No diagram A J 1894, 0 max. 18 (3) Off film max. 18 (3) 16 to 22, max. 19 (4) 18 to 24 0 to 24, max. 15 to 21 (15) 0 to 24, max. 16 to 21 (10) 0 to 22, max. 0 to 18 (10) 8 to 24, max. 18 to 21 (8) 12 to 24, max. 15 to 23 (8) 0 to 4 and 7 to 24, max. 17 to 21 (10) 12 to 24, max. 12 to 24, max. 13 to 24, max. 11 to 24, max. 18 to 21 (8) 18 to 20 (8) 18 to 21 (4) 22 (6) 0 to 18 and 22 to 24, max. 12 (5) 0 to 6 (5) and 22 to 24 (5) 0 to 5, 9 to 23, max. 18 to 21 (5) 15 to 23, max. 21 (6) 0 to 8 (3) and 18 to 24 (4) 0 to 24, max. 9 to 18 (10) 0 to 3 and 2 to 24, max. 18 (8) 0 to 3 and 9 to 23, max. 15 to 21 (8) 12 to 22, max. 18 (7) 15 to 22, max. 20 (6) 16 to 22, max. 18 to 21 (5) 15 to 21, max, 21 (4) 18 to 21 (2) 0 ie 5 (4) and — to 23, max, 19 4 — to 23, max. 20 (10) to 24, max. 18 to 21 (10) to 5 (5), 7 to 12(8), 15 to 24 (8) to 24, max. 12 to 18 (10) 2? to 24, max. 20 (8) to 24 (6) to 24 (6) aroo- 12 to 24, max. 18 (5) 0 to 4 (3), 12 to 22, max. 18 and 21 (6) 15 to 24, max. 21 6 to 24 (6) 0 to 24, max, 19 (9) 12 to 18 (6) 0 to 3 (2), 21 to 24 (1) 0 to 3 (2), 10 to 24 (2) 0 to 12 (1), 10 to 24 (1) 0 to 3 (1), 15 to 24, max. 21 (5) 18 to 22, max. 21, (3) 0 to 24, max. 18 to 23 (3) 0 to 2 and 9 to 24, max. 2 (2) 0 to 20, max. 20 (2) 15 to 22, max. 19 (2) b 15 to 20, max. 19 (2) Slight 15 to 20, max. 18 (3) 7 to 21, max. 14 to 18 (2) 9 to 24 slight 0 to 18 slight, max. 18 (3) 12 to 24 slight 0 to 24 slight, max. 12 (2) and 18 (2) 12 to 15 slight Slight Slight 9 to 18 (2) 0 to 21 slight 12 to 20, max, 16 (2) Off the film tal aitalicd Slight up to 21 Slight 12 to 23 1895. Slight 9 to 23 9 to 21 (2) Slight 12 to 21 till feat St ct N Remarks 0 0 0 18 to 22, max. 21 (3) 2 to 4and 10 to 24, max. 18 (3), 22(4) max. 18 (5) 0 to 3 (1) and 15 to 21 (1) 6 to 18 slight 8 to 24, max. 12 (5) and 18 (5) 0 to 4and 21 to 24 0 to 6 (3) and 21 to 24 (3) 15 to 24 (1) 0 to 3 0 Slight at 23 (3) Oto 24intermittent up to 4 0 to 17 (5) and boom held by a spider’s thread 21 to 24 (4) 0 to 4 (2) 18 to 21 (1) 23 (1) 0 to 4 (4) —to7 15 to 23, max. 21 (3) | 15 to 21 slight W2to1ls ,, 12to21 ,, 3to2l 7 to 24 (1) 10 to 24 (1) 12 to 24 (1) 18 to 24 (1) 0 to 24 (1) eb TA | Midday tremors at N might be due to traffic, but not those on the 3rd. On the 9th up to midnight very many thou- sands of people were in the park and round the pond near N celebrating the capture of Port Arthur and the naval battle at Yaloo. Tremors of N about midday may be due to traffic. Htaltalheatee ate fi tt ea ste ae) The diagrams for N between the 6th and 13th ‘| were destroyed, and these re- eords are from notes. 128 REPORT—1895, TREMORS, MICROSEISMIC DISTURBANCES, OR EARTH PULSATIONS—continued. \Date A 12 (@) Remarks 1895. Jan | 14 | 0 to 3,7 to 24, max. 18 (10) Trems. during day of | Very slight tre- 15 | 10 to 24, max. 18 (8) (2), but during the | mors on nearly all 16 | 13 to 23, max. 18 to 21 (5) nights of the 13th, 14th | days 17 | 9 to 21 (2) and 15th. the light spot | 18 | 7 to 23, max. 19 (4) off the film | 19 | 15 to 23, max. 20 (4) — | 20 | 14 to 19, max. 18 (3) Slight | 21 | 12 to 24, max. 18 (4) tel ted Tat hea Pili, al oll SA) a) Saas 22 | 16 to 21, max, 19 (3) — 23 | 0 —_ 24 | 18 to 24, max. 21 (3) —- 25 | 0 to 4, 9 to 24, max. 18 (5) — 27 | Bto 7 (1) 0 to 9 (5), 18 to 24 (5) 15 to 18 slight 28 | 8 to G (1), 15 to 23, max. 20 (2) | 3 to 21 (2) 6 to 12 at 18 (2) 29 15 to 21, max. 19 (2) | 12 to 21, max. 18 (2) 9 to 18 (1) 30 | 2 to 6,11 to 22, max. 16 (5) 3 to 15 (2) then off the | — to 18 (1) film es No record, 18 to 22, max. 21 (2) | 15 to 18 (1) 6 to 10 (1) — feb. 1 | 3 to 6, 18 to 23, max. 18 (3) 3 to 6 (2), 12 to 24 (2) ae ss 2 | 0 to 24 (3) 6 to 12 (2), then off the | Slight tremors, but —_ film the diagram is bad 3 | 0 to 4(2), 15 to 21, max.18(5) | 0 to 24 (2) — — 4 | 15 to 21, max. 18 (5) No diagram — = 5 | 14 to 20, max. 18 (3) “ = — 6 | 18 to 20, max. 19 (2) as = = 7 | 18 to 24 (3) i = = 8 | 0 to 4 (3), 15 to 21, max. 19 (3) % _ = (d) The Slow Displacement of Pendulums. All my horizontal pendulums, whether they were situated upon the rock or upon the alluvium, have crept away from their normal position. While some of them have moved towards the east, others have moved towards the west. Irregularities like these have been noticeable upon newly built light foundations. Pendulums like those at A and L, where the foundations were massive and old, during the time that they were ebserved, had a general tendency to creep towards the west or south- west. These movements, which were often interfered with by permanent displacements caused by earthquakes, closely resembled the gradual dis- placements observed at stations upon the rock, where, for earthquakes at least, the yielding parallel to the dip of the strata was greater than it was in a direction at right angles to the same. Although my intention when installing the instruments parallel and at right angles to the dip was to determine in which of these two direc- tions yielding was the most pronounced, the observations were not con- tinued sufficiently long to determine whether such changes as were observed had any connection with the secular movements which around Yokohama are apparently proceeding with unusual rapidity. To carry out this investigation, which would not be difficult for a resident at Kamakura, where caves are numerous, at least two installations would be required, and it is not unlikely that within a period of two or three years some measurement of geological changes would be obtained. I also regret to say that the duration of the observations was not sufficiently long to determine whether the wandering of the pendulums had an annual periodicity such as might be expected from the results obtained by observers in Europe. ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 129 (e) Periodic movements of several days’ duration, and wandering of the pendulums. In order to determine the existence or non-existence of periodical movements greater than twenty-four hours, the mid-day position of instruments A and J were plotted on squared paper. This was done for dates between October 13 and December 4, 1894. Because the instrument at K during the period wandered so rapidly towards the east, Fiaq. 4. OctiS _18 23. 28 Nee 7 72.77 28 .27 Ded? ANE NOY nial Bar >A AN re aS I sl olf fons fh ool laetieadgtgeeh li hi RAL Leb. MNOS “i a i da ro LAL AY YM alt Abed but ul siya A S S S and had in consequence to be repeatedly re-adjusted, its records have not been considered. Whether the mid-day reading is the best one to represent the mean daily position of the instruments must for the present be left until a second examination of the diagrams has been made, when the analysis may be continued up to the end of the first week in February 1895 (fig. 4). ; Fig. 5. O73 177 214 25 29Nor2e2 C 10 14 18 22 26 30 1834. By drawing a free curve through the diagrams of mid-day positions of A and J, and reducing this horizontally and vertically one-fourth, the two curves shown in the accompanying figure are obtained (fig. 5). During the complete period considered neither of the pendulums hhas changed much in its mean position. Whatever slight changes have 1895. K 130 REPORT—1895. taken place may be due to the direction in which the instruments or their foundations have warped, or, what is equally probable, they may each have moved away from an exposed area which, in consequence of evapora- tion, may have been rising. About this general movement of the pendulums which might be included in the previous section of this report, because it only refers to observations extending over fifty-two days with pendulums, one of which had a light foundation, no definite conclusions can be stated. One thing, however, which is clear, and which can hardly be attributed to the warping of instruments or their foundations, is that the pendulums wandered at the same time in the same directions. For the first four days the pendulums at A and J moved westwards, for the next twelve days they moved eastwards, after which there was a slight westerly and then an easterly motion up to the fortieth day, when they both turned quickly westwards. This synchronism in direction of motion is evidently due to some general cause, which may act on the surface of the earth or within its interior. A barometric curve determined in a manner similar to that in which the curves for A and J were deter- mined shows that atmospheric pressure was near its maximum when the pendulums were at their western limits, but the relationship between this curve and those of the pendulums is not sufficiently clear to conclude that the movements of the pendulums have been altogether due to fluctuation in atmospheric pressure. Possibly the movements may have been due to evaporation and precipitation lightening or loading some particular area in the vicinity of the pendulums. The earthquakes of local origin indicated by circles on the curve for A, which occurred during the time that there was a rapid westerly motion, suggest the idea that the movements may have a hypogenic — origin. (f) On the daily change in the position of the pendulums. The table below gives in millimetres the difference in the mid-day read- — ings of the positions of the pendulums A and J. The sign + indicates — that during the past twenty-four hours the pendulum has moved so many ~ millimetres towards the west, while the sign — indicates a displacement — towards the east. The sign ? means that no reading had been taken or that no displacement was observed. 1894 A J | 1894 A J ———|- —|— -|@ October 14 . -— 1 — 5 | October 31 . i — 2 peat + 15. + 5 + 20 November 1. : - 3 + 6 | ‘. 16. -— 1 + 8 | ise — 2 — 6 of ts + 3 +12 ‘y Bile +1 se, al | eal Si:6 — 6 +3 " 4. ? + 8 Fr 19). — 4 -— 3 | a 5... + 1 mss A 00) 05 =4 Nats | - 6. asf ~10 % Dire — 38 ade i ry fe + 4 = 1 5 Eze — 3 |) —17 | 3 8. =a + 6.5 3 23. - 8 — 7 a 9). 2 SU Ge | 8 24. + 5 + 7 | 3 LOM. ? ao * 25. — 8 — 3 Lies +3 ee See — 6 +5 ro ee ate an 7 Fh at +7 + 7 oP ark ? eh Fr 28 . + 4 + 3 3 14. — 4. aay * 2003 — 6 —13 . Uses — 3 +10 5 30. ? — 4 5 16. + 2 #393) ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 131 1894 A J 1894 A J November 17 . - + 2 — 1 December 3 + 6 +12 a 18 . : 2 — 4 = 4 = 5 sli 7 LO. F — | Sits) ‘a 5. + 1 — 2 lo oe eae Hage cea en is 6. am ea * Vik - + 7 sedis 1 “3 7 + 2 2 PUSS 99 aS +34 f ant ao — 3 PP 23 + 2 2 _ On ? 10 Bl 24 — 1 + 3 se 10. ? | ? ba 25 ee = #1 * Tile eh SSA) ta DG +12 +16 cee dae. =e = 4 dant 9 eg Seems te ig ? As 28°. + 2 + 9 sy 4. es ek) — 6 Ns 29% ? ? 4: ls +e | ? + 4 eae ar 5 15 eat 16) al + 4 December 1. ae, Sie | F 1 ae ? — 7 ae ; : = fi sendy | An inspection of this table shows that, although the pendulums A and J were separated by a distance of about 270 yards, and were differently installed, there has been a general agreement in the direction of their displacements, and that this is particularly marked when the movements of A were decided. When there has been disagreement in the direction of motion, the movements of A have usually been small, and it is not unlikely that such discrepancies would disappear if a time had been taken to represent the daily mean position farther removed from the hour at which the western movement of the diurnal wave commences. The changes indicated in the table are also shown diagrammatically in con- junction with a curve showing the fluctuations of the barometer (p. 129). What is true for A and J is generally true for J and K. Although between October 13 and November 20 there are six decided barometrical fluctuations, and during the same interval there are six decided westerly movements of J, the crests and depressions of these diagrams do not retain the same relative position. For example, on October 17 the barometrical crest corresponds to the westerly extension of J, while an November 5 a similar movement of J corresponds to a barometrical depression. Although at times it appears as if there were a close relation- ship between barometrical fluctuation and the movements of the pen- dulums, the diagram (fig. 4) indicates that, although both phenomena are nearly identical in having a periodicity of between two and seven days, it _ does not show that they are absolutely synchronous. It seems that the instruments at J and K, which were within six feet of exposed ground, with or after rain moved westwards, but equally large westerly motions _ have occurred without rain. g. On the Diurnal Wave. In considering the results towards which the observations of the daily wave point, it is necessary to consider the observations made during _ the past year in conjunction with those described in the Report for 1893-94. When instruments were installed upon the rock in caves as at Kama- kura (C and D), at Kanagawa (I), and in Yokohama (G and H) the daily wave was not perceptible. This by no means precludes the possibility of K 2 132 REPORT—1895. its existence in such places, and had instruments of greater sensibility been employed it is likely that it might have been detected. It was perceptible and often measurable, but by no means pronounced in the records from my house (A), where the instrument was well founded and in an east and a west direction, well protected trom temperature effects upon the sur- rounding soil. It must not be forgotten that this instrument was the most sensitive, being capable of recording changes of 0-1. Had the sensibility of this instrument not exceeded that of other instruments less favourably installed, it is doubtful whether it would have shown any marked trace of the daily wave. Two instruments in an underground chamber (E and F), whereas in the caves the daily change in temperature did not exceed 1° C., often showed the daily wave in a marked manner, but it was not so great as it was at stations J and K upon the surface. The conclusion to which these observations lead is that the daily wave is not due to fluctuations in tem- perature immediately near to the instruments, but that it is a surface phenomenon which penetrates to a depth of at least 12 feet in the alluvium. An instrument upon the surface (J) the ground round which was — exposed to the sun upon all sides excepting the east, and another (K) which was exposed on all sides excepting the west, showed large diurnal waves, and notwithstanding the fact that between these two stations there was a pond and a grove of tall trees, the pendulums usually moved in the same direction at about the same time. The magnitude of the movements was different, but with this exception the only other difference was that J, the open ground round which was exposed to the afternoon sun for one or two hours longer than the open ground round K, continued its westerly motion for one or two hours longer than K (figs. 7 and 8). An experiment made at J was to dig a trench 5 feet in depth round the south and west sides of the hut. This did not appear in any way to affect the amplitude of the daily wave, but it seemed to increase the suddenness with which the westerly displacement commenced, and at the same time the number of hours occupied in making a complete wave was reduced. With an instrument at O, a few yards from J, which recorded north and south motions, the wave was regular but of small amplitude, the northern movement coinciding with the western motion of J and K. The direction of maximum tilting may therefore have approxi- mately been W.N.W. and E.S.E. On the western side of a plateau facing the eastern slope of the plateau on which A, J, K, and O were situated, an instrument N showed a daily wave, but the westerly excursion of the pendulum was completed only a few hours later than the easterly excursion was completed by those upon the opposite hill. It appeared as if the two bluffs, or at least the trees upon them, inclined towards each other, and then away from each other once in twenty-four hours. Between the two bluffs there is an open valley, in which there"is a lake or pond nearly half a mile in breadth. That the records at N were small may be attributed partly to the fact that the instrument never had given to it any great degree of sensitive- ness, and partly to the fact that on all sides excepting the west the ground immediately round the instrument was well shaded by tall trees. There is, however, a large open space about 100 yards to the east of this station. At another station P, on the eastern side of the plateau, on which N was situated, and at a distance from it of about 200 yards, the movements, ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 133 especially upon frosty nights, were extremely erratic, and they ma probably have been produced by the freezing of the ground. When the cold was not great the movements were small, and here, again, the ground around the instrument was so well shaded by trees that after a snow- _ storm it would take from ten to fifteen days to melt away the snow, which at other places disappeared in one or two days. At Q, R, 8S, and O the movement during the day was towards the side on which the ground _ near to the instruments was most exposed to the sun. One very important observation especially marked at stations where _ large diurnal waves were recorded was that on rainy or cloudy days these instruments were steady, and no diurnal wave was recorded. The general conclusion to which these observations on the diurnal wave _ point is that on the alluvium on open ground, the daily wave is most pronounced on the surface, it is less in amplitude, but it may be decided at a depth of 12 feet ; while ona massive foundation the ground round which is well protected by a building or trees the wave is slight. Deep under- _ ground on a rock foundation with instruments such as I have had at my disposal it is not perceptible, but it is not improbable that a residual effect of the surface motion might be detected with more delicate apparatus. The cause of the motion is not any immediate effect of temperature upon the instruments, nor if we except the case where actual freezing of moisture in the ground round and possibly inside one of the huts took place does it appear to be due to expansion or contraction in or near the foundations “accompanying the acquisition or withdrawal of heat. The most active cause producing the movement which takes place during the day may be the fact that the ground on different sides of an “instrument is unequally exposed to effects producing evaporation. The retrograde motion during the night, which is smaller and more gentle than at which has happened during the day, may be due to the unequal condensation of moisture on two sides of a station. 1. Hifects accompanying Evaporation (Daylight Hffect).—As the side of a station from which most moisture is withdrawn to be dissipated in the atmosphere has been relieved of a load, we should expect it to rise, and this effect ought, in alluvium, to be perceptible to some depth. The Same area, because it is contracting like a drying sponge, may sink, but this would be a superficial action. On open ground, under favourable circumstances, the load taken away “from a surface of earth by evaporation may amount to 4 or 5 lb. per Square yard, or from an area 20 yards square, about 1 ton. Experiment e has shown that 2 tons of water taken out of a well and run off down a hill will cause a pendulum at a distance of 20 or 30 yards to behave as if the ground upon the well side had risen. If these premises are correct, then an instrument well surrounded by trees or buildings, because the evaporation is slight and is not likely to be much more marked upon one _ Side than it is upon another, should show but little motion. A pendulum at a station freely and uniformly exposed upon all sides should also show but little change. During the morning a north-south pendulum would be expected to move slightly towards the west. For some hours after the sun’s meridian passage there would be a pause in such displace- Ment, after which a retrograde motion would set in. An instrument ‘with open ground upon its eastern side would, during the morning, be expected to move westwards ; while at the same time another instrument, with the western side as an evaporation area, would move eastwards. It , Fig. 6. A.—Moves west from 3 A.M or 6 A.M. to 3 P.M., or from noon to 9 P.M., or midnight. STIG 3 Noon 21 é 0 TGS 7, ™ rn ~ t vs) Dd &> = a & ~ 18 13. ote 9 6 3 0 | T | Moun Westward. es Diagrams of Diwrnal Waves are reduced about one-half. ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 135 is not likely that pronounced movements would be recorded upon rock, neither should there be an appreciable trace of diurnal waves on days when it was wet or cloudy. 2. Contraction due to Desiceation.—If the desiccation due to heating by the sun is followed by contraction, we should expect that during the day a pendulum would move towards the side losing the greatest amount of moisture ; that is to say, its movement would be in a direction opposite to that accompanying the removal of a load due to evaporation. On ground covered by trees or buildings, or on ground uniformly open all round, but little motion should be expected. Whatever effect was observed it is not likely that it would penetrate many inches beneath the suriace. The following is a comparison of these considerations, with the observed movements of the various pendulums and the character of the surrounding ground. For 100 yards to the east and west of A the ground is equally open. The most open ground, however, lies to the east. It would therefore be expected that movement during the day due to unloading would be west- wards. The observed movements, however, although generally westwards, showed too many irregularities, and were too feeble to justify a conclusion that they were due to such an influence (fig. 6). For 100 yards round station J the ground is more open upon the western side than upon the eastern side, and the westerly motion might therefore be attributed to desiccation and contraction upon this side. Beyond this limit, however, the ground is most open upon the eastern side, which might therefore, by evaporation, rise. This would give a westerly motion (fig. 7). Fie. 8. K.—Moves west from 6 A.M. to 8 or 6 P.M. Nom ti 18 Gow 9 6 3 0 For 100 yards round K the ground is most open upon the eastern side, and desiccation would result in an eastern displacement. The westerly motion recorded seems to find its only explanation in the fact that the eastern side of the instrument is more open than the western side, but the reason that these movements were greater than those at J is not clear (fig. 8). Immediately to the west of R there are tall trees and a deep cutting. So long as the sun shines over these trees upon an area 50 or 190 yards long to the east of the instrument, the pendulum moves towards the area 136 REPORT—1895. which is drying. Beyond this limit, however, there is far more open ground on the N.W., W., and 8.W. sides of the station than there is in opposite directions, and the pronounced easterly motion may therefore be due to the unloading on the western side (fig. 9). Fig. 9. R.—Moves east from 8 A.M. to 3 or 4 P.M. lz 9 6 3 Noon 21 18 15 12 1 Afternoon peti ate 4 Wh | hin ii, lan. All round station N for a distance of at least fifty yards there are either high trees or shrubs. Beyond this limit in a westerly direction but at a lower level there are a pond and flat ground. In an opposite direction Fic. 10. N.—Moves east from 9 A.M, to 6 or 9 P.M. Cho THRE BBB NODDY 21 UN TE IN OD 6 alk ein Westwards \_, on the same level there is at a distance of about one hundred yards a smaller area of open ground facing the Exhibition buildings. The move- ment is therefore as if the ground on the side of the largest evaporation area had arisen. But the movement is small (fig. 10). ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN, 137 Near to the instrument at S on the west side the ground is covered with green corn about one foot in height, while towards the S.E. there is a strip of bare ground perhaps fifty yards wide and one hundred yards in length. The movement, which, however, is slight, is towards the area most open to the sun. Neglecting this strip, then, there is very much more open ground on the western than upon the eastern side of the station, and the movement may be explained on the assumption that this side, because it loses the most weight, rises relatively to the other (fig. 11). E Fig. 11. S.— Moves east from 6 A.M. to 3 P.M. Tiomaba. § Bt On Bas 3s MOM ay 21 RO ACL Ap26 3 ' Near to O the ground is somewhat more open on the north side, and it would appear that the motion was towards this side. Because the movements are slight, they might equally well be explained as a com- ponent of a south-eastern tilting due to greater relief of load upon the §.E. side, which is more exposed than that in the opposite direction. Although a diagram may be modified by contraction following desic- cation in the immediate vicinity of an instrument, this detailed examina- tion of the observations in relation to the localities at which they were Fig. 12. O.—Moves north from 9 A.M, to 5 P.M. North, Motion made tends to the conclusion that diurnal waves are in part distortional effects of the earth’s surface due to unequal relief of load from various areas by evaporation. When the movements have been absent or small, the instruments have been, at stations on the solid rock, well protected by trees or on an open plain. Many anomalies occur which still require an explanation, the most remarkable perhaps being the smallness of the motions at A, where the hypothesis requires that they should have been pronounced. The intermittent character in the movement at R may pos- sibly be connected with the deep cutting on its western side, which breaks 138 REPORT—1895. the continuity of the ground upon that side, which it is assumed in order to produce the easterly deflection must rise. I put forward these conclusions simply as being, for the present at least, the best that Iam able to arrive at as explanatory of my own observa- tions. The conclusions reached by Dr. E. von Rebeur-Paschwitz only partly confirm my results. In the British Association Report for 1893, on p. 316, he says that ‘the range of motion is on an average very nearly proportional to either the quantity of sunshine or the maximum oscillation of temperature during the day.’ This and the fact that the movements at Teneriffe, where the observatory appears to have been founded on and surrounded by soil and rock, were very much more pronounced than they were at Potsdam and Wilhelmshaven, where the soil was comparatively soft, apparently support the view that the diurnal wave may be a distor- tional effect due to evaporation. On p. 320 of the same report, however, he says that ‘at Potsdam as well as Orotava the average range of daily motion agrees most remarkably with those meteorological elements which we may consider as a measure of the intensity of solar radiation. But I must not omit to remark that the single days do not show this coincidence equally well. For cloudy days occur with a large range of oscillation, and clear days with a small range.’ Although my observations in Japan have shown that when it was cloudy and wet the diurnal wave has been absent, it is not impossible that there may be cloudy days when, in consequence of wind, evaporation may occur, and in consequence the daylight distortion may be marked. 3. Hffects due to Condensation (Night Hffect).—It has been shown that at a favourably situated station the evaporation effect which has been marked during the morning may late in the afternoon be the means of starting a retrograde movement. It, however, remains to be explained why a motion possibly commenced in this manner continues slowly during the night until about 6 a.m. upon the following morning. Because this movement is comparatively small it may be produced by the addition or removal of a comparatively small load. The precipitation of dew, which on a uniform area like evaporation follows in the wake of the sun, represents a feeble load, but the retrograde motion continues when dew is not visible. But although dew may not be visible, if we look beneath a board which has been lying on the ground all night it is usually found to be very wet. This observation suggested the idea that just as moisture is condensed beneath a board, so it may be condensed in the ground within one or two inches of the actual surface. During a hot day moisture is evaporated from the soil, which is per- ceptibly heated to a depth of about one foot. Shortly after sunset the surface to a depth of one or two inches is chilled or in winter it is frozen. The result of this is, that moisture rising as vapour and by capillarity from water-bearing strata is condensed on the underside of the chilled sur- face. Like the dew we see ona uniformly covered surface the underground dew should be first precipitated on the eastern side of a station and sub- sequently upon the western side, and therefore during the night the surface on the former side gains weight at an earlier hour than the latter. To determine how far superficial soils gain in weight by an action of this description, independently of moisture precipitated from the atmo- sphere or condensed as it rises out of the ground, the following experi- ments were made. Two boxes each 1 ft. 6 in. square and 2 in. deep were ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 139 balanced on the extremities of beams carried upon knife edges. One box had a bottom made of tin and the other of fine wire netting, and each was filled with earth. Excepting when they were weighed, by placing weights at the other ends of the beams, they were allowed to rest on the soft earth of my garden. Sometimes it was found that during a night both boxes would lose weight, but at other times it was found that the weight of the box with the tin bottom had not changed, whilst the one with the wire netting had gained from 2 to 2-5 ounces, which apparently showed that there had been a condensation of moisture coming up from beneath of 10 ounces per square yard, or about one-eighth of that which might have been removed during a day by evaporation. As my notes upon these experiments were destroyed by fire, what is here said can only be taken as indicating the character of a phenomenon which hitherto has not received attention. Whether the causes which have been described are sufficient to account for the diurnal movements of a horizontal pendulum remains for future investigators to decide. The gradual taking away of weight, followed by a gradual addition of weight unequally on the two sides of a pendulum during each period of 24 hours, will account for the observed movements, and in the evapora- tion of moisture during the day and the precipitation of moisture on the surface, together with its condensation beneath the surface during the night, we have phenomena which relieve or load surfaces in the required manner. (h) Tremors. In the third Report to the British Association, 1883, after observing tremors with the ordinary Italian form of tromometer, I attributed their origin either to the effects of high winds or to small but rapidly recurring variations in atmospheric pressure, such as may be observed during a typhoon. After analysing a long series of records of these movements, which were obtained from an automatic tremor recorder, and comparing the results with observations made in Italy, the conclusion arrived at was that tremors were at a maximum when the barometrical gradient was steep, no matter whether at the place where the tremors were observed the barometer was high or whether it was low. This relationship between tremors and the state of the barometric gradient, although it did not explain the origin of tremors, tended to destroy the distinction between tremors which occur with a low barometer, and are called baro-seismic motions, and those which appear during periods of high pressure, which are called volcano-seismic disturbances. An examination of the photograms obtained from the horizontal pendulums, which permit of more accurate analysis than those previously obtained, although it does not show that tremors only occur at the times when the barometric gradient is steep, shows that at such times tremor storms are marked. These same diagrams, however, on account of the relationship they show between tremors, the changes in the position of a horizontal pendulum, barometrical pressure, and the diurnal wave, lead me to withdraw the suggestion that, because steep gradients are usually accompanied by wind, such winds, whether they are local or distant, may be the immediate cause of tremors. In their times of occurrence winds 140 REPORT—1895. and tremors undoubtedly show a close relationship, and therefore the former may, by its mechanical action upon buildings, trees, and the surface of a country, produce slight tremors, and influence the character of a record. The points which are marked in connection with the recent observations are as follows :— 1. Relationship of Tremors to Localities and Instruments. Tremors have been pronounced at Station A, the instrument at which station, however, was the one most sensible to changes of level. At stations on the surface in Tokio they have been feeble, but have varied in their intensity. Underground upon the rock they have never been observed. This latter observation, which is based upon records obtained from five instruments, is in direct opposition to the observations made at Rocca di Papa in Italy, where, I understand, tremors are as pronounced underground as they are upon the surface. At Station A, an instrument which showed tremors even in a more marked manner than the large horizontal pendulum, was a similar instru- ment made of a few millimetres of aluminium wire, a small mirror, and a needle point, weighing only a few grammes, a comparatively large form of which is described in the Report for 1892. On account of the manner in which the spots of light reflected from the mirrors of a pair of these instruments placed side by side would come to rest, and then start suddenly to move in the same direction, I was led to the conclusion that they were actuated by an intermittent tilting, and therefore that tremors, rather than being elastic vibrations, had the character of wave-like undulations.! The fact that the instrument most sensitive to changes of level gave the most pronounced records appeared to strengthen this sup- position, and I was led to call these movements earth pulsations. The only effect produced by heavy gusts of wind striking the building, or the beating of a steam hammer at a distance of fifty yards, is to pro- duce a temporary vibration in the pointers of an instrument ; but there is no angular displacement, and consequent swing, which characterises the movements during a tremor storm. An important observation made at Station A was that tremors were produced when two tons of water were taken out of a well distant about thirty yards. The operation caused the ground upon the well side to rise, and the horizontal pendulum was gradually displaced in an opposite direction. From this it may be inferred that either the pendulum took up its new position intermittently, or that the level of the ground changed intermittently. Whichever it may have been, it may be concluded that whenever a rapid change in the inclination of the ground takes place, horizontal and probably other pendulums may be caused to swing, and, as will be seen in the next section, at least a portion of the tremor records may be explained on the supposition that they are due to such causes. 2. Relationship of Tremors to the Diurnal Wave. (1) Even when a horizontal pendulum is steadily following the diurnal wave and no tremors are visible, slight tremors nearly always appear about 6 or 9 A.M., just at the time when its easterly excursion has been completed and it turns to commence a relatively rapid motion towards the west (figs. 9 and 13). ) The instruments were under the same cover. See Appendix. ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 141 (2) Should there be a tremor storm extending over one or two days there is a maximum motion at about 6 or 9 a.m. (figs. 9 and 13). (3) Large daily waves nearly always correspond with pronounced tremors (47 cases). (4) When no daily wave appears, or when it is feeble, which usually happens when the weather is dull or wet, there have been eight cases of feeble tremors, and nine cases where tremors have been practically absent. (5) The greatest motion is experienced, or motion is most frequent, while the pendulum is moving eastwards—an observation which is connected with the remarks in the next section. 3, Relationship of Tremors to the Hours of Day and Night. (1) It has been shown that tremors are most frequent or at their maximum at about 6 or 9 a.m. (figs. 9 and 13). (2) The hours during which storms are the most frequent are from 9 P.M. or midnight until mid day. During the afternoon and evening, therefore, tremors are not so frequent. (3) The tremors at 6 or 9 a.m. may be attributed to irregular move- ments accompanying the reversal in the inclination of the ground which Fig. 13. oO i=] oat 2 18 15 2 9 6 4i[Nya ) va ih CDi ac ‘Niu Mabe AH LN AY ALR TIND HPAee e Pe Th Aida iit MANNE Kb wid Au ay ae be attributed to an intermittent change in level, it then becomes neces- sary to explain why the smallest changes in level are most intermittent in their character, which supposition’ is improbable. The accompanying figure shows how a tremor storm which may continue over several days has a maximum at 6 or 9 A.m., and also, as it dies out, that it terminates with slight tremors at these particular hours. It is taken from instru- ment A. takes place at these hours, but if the tremors which occur at night are to 142 REPORT—1895. 4, Relationship of Tremors to Barometrical Conditions. (1) Tremors are apparently as marked with a high barometer as with a low barometer. (2) Tremors chiefly occur with steep barometric gradients. (3) They are marked when barometric changes are rapid, whether the barometer is rising or whether it is falling. (4) Although it is not likely that the daily fluctuation of the barometer should have any marked effect upon the production of tremors, it may be noted that the maximum of tremors occurs when the barometer is at its greatest height and about to fall rapidly to its daily mimimum. Mr. T. Wada, of the Meteorological Observatory, has kindly given me the follow- ing table showing the daily barometrical maxima and minima deduced from eight years’ observations :— | | — | Fluctuation Maxima | Minima BS yt gE 4 Fuse TE as | mm. Hour | Hour Winter . A ; ed 2°23 9 A.M. 2 P.M. Spring . 19 eee rer Summer 1°35 ae | 4 ,, Autumn | 174 + ey, | Sine For the year 760°00— 758 30=1'70 mm., at 9 A.M. 5. Relationship of Tremors to Wind, Temperature and sub-Surface Condensation. Although tremors have occurred when a heavy wind was blowing in Tokio, as, for example, on October 26, tremors have been marked when wind was practically absent. Neither does there appear to have been any marked connection between the occurrence of tremors in Tokio and the wind at Choshi, which is situated on the coast about 50 miles west from Tokio. Although the morning breeze is apparently stronger than that in the evening, it does not seem to be connected with the morning frequency of tremors. Tremors are most frequent at the hours when the temperature is lowest, or during the time that sub-surface condensation is taking place. Tremors are at a mimimum during the time that the ground is becoming heated, and there is a free flow of moisture in the form of vapour from the earth to the atmosphere. Tremors and Waves on the Coast.—At the various lighthouses round the coast of Japan at 2, 6, and 10 a.m. and p.m., records are made of the force of the waves. In these records 0 = calm and 6 = waves, which are unusually large. JI have compared the records from Jogashima, 33 miles south of Tokio, and Inuboye, 53 miles west of Tokio, with the records of tremors, but I do not observe any connection between them (see Tables). i Occurrence of Tremors in Manila.—A. set of diagrams which clearly show the relationship between various atmospheric phenomena and the occurrence of tremors are the monthly sheets of the Meteorological Obser- vatory in Manila, where from some date prior to 1883 observations have been made with Bertelli’s tromometer. Tremor storms are apparently —_——-- - —— SS — ” ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 143 frequent from the end of June until the end of November, and accompany winds having a velocity of from 50 to 100 km. per hour, the barometer being Jow. During the remaining months of the year although slight tremors are frequent it is seldom that they are pronounced. When winds are fairly strong, reaching 30 or 40 km., unless these are continuous over: several days the tremors are slight. Cases occur when tremors are fairly frequent with a low barometer (757 mm.) whilst there was but little wind. On the other hand, with a wind not exceeding 30 km., there have been decided tremors with a high barometer (763 mm.). The conclusion to be derived froin these records, which, however, do not show the state of the barometric gradient, is that tremors are frequent with high winds, with winds of moderate intensity if these are continuous over several days, and at times when the barometer is low. Because they are sometimes absent when a wind of moderate intensity is blowing, it would seem that their appearance may be more closely connected with changes in barometrical pressure than with the mechanical effects of wind upon surface irregulari- ties. They do not appear to be connected with daily changes in tempera- ture, the hygrometric state of the atmosphere, or with the occurrence of earthquakes. Since writing the above Father M. Saderra, 8.J., Director of the Obser- vatory at Manila, writes me as follows: ‘Evidently the results are influenced by atmospheric currents, but in an indirect manner, as is proved by the fact that the hours of greatest wind force an@® greatest movements of the tromometer do not always coincide. The influence is verified by means of the vibratory motion which the wind produces in the earth itself by impinging against mountains. It now remains to observe and study this influence and endeavour to ascertain which wind exerts most influence. Hitherto this has not been feasible, but now, God helping, I will set about doing it.’ Although these observations throw a certain amount of new light upon the occurrence of tremors, and possibly explain their morning frequency, the causes producing tremor storms are yet obscure In Japan, at least, they appear to be a surface phenomenon which exhibits itself in different degrees in different localities. Although the longer period motions of hori- zontal pendulums show that changes in barometrical pressure may be suf- ficient to produce changes in level, it does not seem unlikely that rapid alterations in barometrical pressure over an area, the yielding of different portions of which are unequal, may be sufficient to create irregular mechanical disturbances in such a district, and the motion once started as with s severe earthquake may continue for several hours after the initiat- ing weuse has ceased. Whatever may be the cause of these ubiquitous phenomena, because they interfere with so many delicate physical opera- tions, they certainly demand serious attention. For the assistance of those who desire to scrutinise the analyses of which I have only given the results or to make new investigations, the following list of meteoro- logical conditions during the period which has been considered is here appended. (See Appendix, p. 182.) (i) Meteorological Tables for Tokio, October 13, 1894, to January 1895. The following tables have been extracted or computed from informa- tion given in the weather maps which are issued three times per day by the Central Meteorological Office in Tokio :— 1895. REPORT 144 GL, 0-3 68 | 68° | T6 | TL OT| OT) FL | FL | TL | og OT] OT) 19 | #9 | 99 | L+ 8L| 1) 28 | OF | FF | 0G OL) ET|/ GL | 88 | 82 | 69 G1] OL) TL | &L | FO | 09 GL] ST} 99 | FL | 02 | OF 2) 81) 9F | 26 | LL | #9 Z| 06|F8 | 98 | 88 | ¢8 LT} LT) 28 | 16 | 68 | %9 LI) @1| 6S |%¢ | 92 | Le 0-T| G1} LOL | @1L | T-0L | 28 GI] OL) 16 | G6 | 28 | GL OT! OT; 82 | 96 | 82 | 2-9 BI} @1|99 | 12 | e¢ | 09 0:3) GG) PL | $6 SOL | €-6T 0%) SL) GIL | OL | LOT | 6-6 0-3) 01/6 | 28 | #8 | Ld 0-2| 01/98 | 06 | &2 | 0-9 0610-6) 62 | 0.6 | 22 | FL 0-8) GT) 21 | IL | FIT | GOT 0%! @T) 90L OL | 9-01 | $6 06) OL) $6 | 00T | 0-6 | 0:8 L1) Ot) £8 | 90T | TOL | 6-6 OG) @L) GEL FEL | GEL | GIT G| 81) LIL | FIT | $0T | F-6 O01) ¢6 | G8 | &8 | 18 61/08 | T6 | 06 | $6 1036/98 | 06 | G8 GL |@1/ G2 | 96 | #8 | 98 ST) 16 G8 | OL | £6 | 2-1) @6 | 00T | #6 | TOT | SL) &IL | $-0T | SOL | 26 | OT! GOL |} 66 | T6 | £6 OL) TET | GE | MBL | BBL (OT) SEL | REL | HEL | LEE | O-T| 220 | LET | @EL | F-6L | 80| L&T | el | 98L | 6-30 Ie OGL | SL | OLE | 0-01 oH eS iS e\8S dor| d9 | dg | vor ro cot Tosuay, mode A On nnootronr Mmevvvoeonern RE HHOoOHHHH HHS Or~vdoryttoarn OdDaSH6 SeGr-arntH- anne = Aer NMAI HS ee HORDE UONAR HM MAME AN RMaAANDYh ReOHSSL HR HOLE HHSSOUWHS +x = = 7 O10 CD i> aA = SHASCDARMANDAGHS 7 I Ayrpram yy 0ATyepOYy I ! 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Aqrpruin yy aatgvpayy OT]7B9 AY Wey arnqeszodmeaL, oases p++++ | i+++1 NSANSCOHORADMHONOOMWS FAI BWHAOSBWINMINAMNTDONME-EHOUNG [+1 +++44] DOME OA assay OLIQIULOLE ET GE9 | Leo | 3-¢9 €-99 | #69 | T-L9 ¥-99 | 9-F9 | ¥-F9 G19 | ¢-99 | 3-€¢ 869 | GES | Gg 9-66 | 8-69 | 6-09 0-69 | #19 | 8-09 £29 | 6-9 | 8-29 F-G9 | G19 | 6-89 “ure Jojyotmoreg S68T ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 147 The barometer readings are given as the number of millimetres above 700. The barometrical change is the difference in the readings on successive days taken at 2 p.m. The numbers representing barometric gradient are the number of millimetres on the weather map (where 1 mm.=6 geo. miles), which cor- respond to a difference in pressure of 5mm. Where a number is omitted it means that the barometrical pressure has been fairly uniform over Central Japan. Temperature is indicated in the Centigrade scale and rain in milli- metres. To show the state of the weather the following signs have been used— cl=cloudy, c=clear, r=rain, f=fine, fy=fog, and s=snow. The relative humidity is in percentages, 100 being saturation. Tension is expressed in millimetres of mercury. _ The force of waves is recorded at 2, 6, and 10 a.m., and at 2,6, and 10 p.m. at the various lighthouses round the coast. The scale employed is as follows :—O=calm, 1=smooth, 2=moderate, 3=rough, 4=high, 5=very high, 6=tremendous. In the tables the mean value for the above hours is given for Jogashima, 3:3 miles south from Tokio, and for Inuboye, 53 miles east of Tokio. (j) Earthquakes recorded by Horizontal Pendulums in Tokio, October 31, 1894, to February 7, 1895. To obtain Greenwich mean time, subtract nine hours. The instrument which recorded a given shock is indicated by its letter. The numbers in brackets indicate the width in millimetres of the displacement as shown upon the photographic trace. The times given are obtained by a rough measurement of the diagrams. For several of these disturb- ances it would have been desirable to have made the time observations more accurate, but owing to the loss of my notebooks by fire, this is now impossible. 1894 Oct. 13 8.59 (5), A. Sudden commencement. 21.27. J. 15 7.0 (2), A. Sudden commencement. 7.80 (2) ,, > re OAS EG) a ww <5 18 1.20(6) ,, Gradual » ES KOR @) ae 4.33 (2), J 7.88-(h), ,, TOT CL, 5 26 9.0, K. Three slight disturbances. 27 2.10 (10). A. 18.0 (10), A. Commenced gently; duration 1 hr. 45 min. 18:5. J. : 3 of 3 hrs. 0 min. Ui Se oy 6 i 2 brs. 25 min. 28 4.20 (3), A 29 11.9 (6), ,, 31 8.0 » Slight. 9.30 5 7 10.0 (5), ,, ' Time evidently wrong, 148 Nov. 2 REPORT—1895. 1.30. J. Commenced gently, duration 30 min. 16.30. J, + lhr.30 min. Three shocks. 20.0 (10), A. Commenced gently. 21.0. J. Slight. 5.30 to 6.30. A. Two shocks of (38) and (8.) 7.00? A. Slight. 10:07 ,, % 4.0 22 ” 7.30 5, 5 9.02 4.302 (10), A 0.0to9. A. About seven disturbances. 2.0, A. Slight. 5.0 (5), A. Commenced gently, duration 3 hrs. 2.0 to 2.30 (10), A 4.0to7.0(5) ,, 10 0 (5) 9.0, about J. Strong. Local origin. 12.0. J. 22.0 to 24.0. A. Several small disturbances. 1.0, 3.0, 4.30 to 6.0, 7.0 and 8.0, each about (5). A. 2.0, several ; 2.45, 4.0, 4.30 and 9.0, each (2) to (4). A. 1.0. 2.0, 4.0 and 5.0. A. AJ] doubtful. 3.0 (15). local origin ; and up to 9.0, four shocks each (2). A. 18.0 (20). 19.0 (5). 9.0 and 11.0 (8) or (4)? A. 2.0 to 3.0(5)? A. 3.0 and 6.30 Es 6.15 and 7.15 (5). J 7.30 (2). A 9.0 and 11.0(1). A. 3.15 and 4.0 (1). _ ,, (local origin). 7.0 and 2.0, and 23.45 (1). A. 3.0 to 5.0. A. May be tremors. 2.0 and 7.30 (5). A. 3.0 and 7.0 (27). 9.30 (2). A. ROG. 21.0 (4). Earthquake. A. 21.0 (2). 3.0 and 6.0 (3), introduction to a tremor storm. (Local origir..) 11.0, large earthquake. A. (Local origin.) 11.0. 3.0 and 4.30 (2). A. Local origin. 9.0. A. Slight. Local origin. 7.80, 10.0 and 11.0. Slight. A. (kOe HAS 6.0 to 8.0. O. Perhaps tremors or three quakes. SO), A. PRON GL) Ne 10.0. A. 10.0, A. 1.30 and 8.30 A. 8.0. A. a oe ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN, 149 One of the most interesting of these disturbances is that which was recorded at three stations, at about 18 hours, on October 27. The origin of this was near to the Antipodes of Japan, in the Argentine Republic. In the shaken district Dr. E. von Rebeur-Paschwitz tells me that the mean velocity of progagation was about 1:2 km. per sec. Mr. C. Davison tells me that it reached Europe to be recorded at Rome with a mean velocity for the large motion, of 3:17 km. per sec., the preliminary vibrations having a velocity of 10°38 km. per. sec. These latter movements reached Charkow and Nicolaiew with velocities of 11:47 and 9:47 km. per sec. If the record J for Japan can be assumed to be approximately correct, then the movements recorded in Japan, if they were propagated over the surface of the earth, reached that country with a mean velocity of 19 km. per sec.! The figure is reduced from the record of K. Fig. 14. : Oct. 27th | | 1894 H » III.—Description oF A CaTanocuet oF 8,331 EARTHQUAKES RECORDED IN JAPAN BETWEEN JANUARY 1885 AND DecremBer 1892. (a) History of the Catalogues. In order to determine the number of shocks which are felt per year in Japan, and to obtain some general idea as to their distribution, in 1880, with the assistance of Mr. Toshiwo Nakano, the present writer communi- cated with residents in all the principal towns of the Empire, asking them to furnish information about the seismic activity, both past and present, of the districts in which they resided. An examination of the replies which were received led to the conclusion that on the average there were three or four shocks per day, or for Japan alone there were as many shocks per year as Professor Heim had calculated for the whole globe (‘ Trans. Seis. Society,’ vol. iv. p. 30). In the following year, in order to determine the extent of country which was shaken by a given shock, bundles of post- cards were sent to very many towns and villages within a range of about 100 miles of Tokio, with a request that every week one of these cards should be returned with a statement of the earthquakes which had been felt. The result of these communications showed that nearly all the shakings which disturbed Tokio came from the east and north, and seldom passed beyond the mountain ranges to the west and south. These facts having been established, the barricade of postcards was extended north- wards until it reached Sapporo, which is about 450 miles north from Tokio. With this system, between October 1881 and October 1883, 387 earthquakes were recorded, for each of which a map was drawn showing ‘ They may have passed through the earth with a velocity of 13 km. per second. 150 REPORT—1895, the area which had been shaken and the approximate centre from which each disturbance had originated. To render the observations more com- plete, one or two watches were given to telegraph operators (a few of the more enthusiastic observers provided themselves with good time-keepers), and seismographs were sent to the following stations :— Geo. Mile. J'rom Tokio. Nagasaki. : - 3 : . 550 W.S.W. Kobe . : ; ; : 4 2 ZO W. by 8. Yokokama . : : . : Seas: S.W. by S. Chiba . : : : : ‘ ao ait K. by 8. Kisaradzu. : 5 3 ; ae pel 8.E. by §. Kamaishi : : : : leo N.N.E. Hakodate. : : : : te N. by KE. Sapporo ‘ ] : - : . 450 N. by EH. From these observations it was definitely shown that the greater number of earthquakes had their origin along the seaboard or beneath the ocean, that the volcanic and mountainous regions of Japan are singularly free from shakings, and that the country might be divided into seismic regions (‘ Trans. Seis. Soe.,’ vol. vii. Part II.). The establishment of these and other important results in 1884 led the Imperial Meteorological Department, then under the direction of Mr, Arai Ikunosuke, to under- take the continuation and extension of investigations, the labour and expense attending which were altogether too great to be borne by an individual. On the retirement of Mr. Arai the work was continued by Mr. K. Kobayashi, the present Director of the Bureau, and it is to his kindness that I am indebted for access to the vast amount of material that has beenaccumulated. The observing stations from which this mate- rial is being derived, and which for the last two years has been pouring in at a rate too fast for analysis, are as follows :— Gunyakusho (district offices). (As several of the smaller of these are controlled by their larger neighbours, postcards and letters are only forwarded from 527) 804 Kencho (offices at the capitals of provinces) . 43 Fu (arge cities), Tokio, Kyoto, and Osaka ; , 3 Light-houses . ; ; : ; : F ; 4 7) NGS Light-ships . F 5 : : : : ‘ 4 : 3 Meteorological Observatories (of these 39 have instruments). 52 Total number of reporting stations - . 968 The information derived from these stations, which are distributed over the Empire, an area of 140,000 square miles, is from time to time supplemented by records obtained from stations under the control of the Imperial University and those of private observers. When an earthquake is felt, according to the area over which it has extended, the number of postcards, letters, and diagrams which may be received at the central station vary between three or four and several hundreds. From the catalogue it will be seen that between 1885 and 1892 more than 8,331 shocks have been recorded, and for each of these a separate map has been drawn. To draw these maps, which has been entirely the work of the Meteorological Department, it is possible that 80,000 to 100,000 documents were examined. For reducing this bulky mass of matter into the comparatively small and accessible form in which it has been published, my thanks are due to Mr. M. Suzuki, a former ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 151 assistant of the Meteorological Bureau, who has worked with me, pointing out doubtful information, translating papers, calculating areas, determining centres, filling in maps, and in carrying out other tedious operations for the last twelve months. The chief reason for terminating the catalogues at the end of 1892 is because the material subsequent to that date has not yet been reduced to the map form, and to examine all the documents necessary to accomplish this would have occupied at least another year ; also it may be added that what has been done is in all probability sufficient to determine whether work of this description is likely to lead to results of sufficient importance to guarantee its continuance. (b) Explanation of the Catalogues. In the first catalogue the shocks are placed in chronological order from 1 to 8,331. When disturbances have apparently been simultaneous in two distant localities, they are included under a single number. In the second and third columns the date and time for each disturbance are given. When the latter is noted to seconds, the record refers to the commencement of motion at an observatory, like that in Tokio, which is provided with automatic chronographs. Until the end of 1887, these records, which are practically correct, refer to Tokio mean time, or 9 hr. 19 min. 1 sec. before Greenwich mean time. Subsequently to this date the times given are those of Long. 135° E., or nine hours before Greenwich mean time. The other time records are only approximately correct, and eannot be used in any investigation relating to the velocity with which earthquake motion is propagated. The fourth column gives in square ri (1 square 7i=5'96 square miles) the land area which was shaken. For small shocks which were only felt at one or two stations the determination of this quantity has largely depended upon the judgment of the observer. The figures given are those obtained from the maps by means of a planimeter and entered in the records of the Meteorological Department. In the second catalogue, based upon a second inspection of the maps, it will be noticed that many mate- rial alterations have been made in these quantities. Im many instances the land areas of the first catalogue are total areas, but in others they only represent an insignificant portion of a disturbed tract, the centre of which was beneath the bed of the ocean. The limits of the areas given are those places round an origin up to which the movement was perceptible to people or sufficiently strong to have been recorded by ordinary seismo- graphs. With instruments like delicately adjusted horizontal pendulums, there is no doubt that movements might have been detected far beyond these arbitrary limits. For example, shock number 4,145 has assigned to it a land area of 15,750 sq. 72, when we have good reasons for believing that with suitable instruments it might have been noted at any point upon the surface of our globe. The number in the fifth column approximately indicates, as shown upon the key map, the epicentre of a disturbance, or a number on the coast line nearest to a submarine origin. In the second catalogue, the position of a submarine origin, by means of a distance in tens of miles and the direction in which it is to be measured from a central number, is defined more closely. On the key map the numbers referring to squares, 152 REPORT—1895. each 10 miles by 10 miles, commence at the top and run from left to right down to the bottom of the same. A line drawn on the key map through the numbers in the sixth column gives the boundary of the land surface which was shaken. The area of this should be equal to the quantity in the second column. By com- pleting, when it may be necessary, this outline seawards, a total area is obtained, which is indicated by its major and minor axes in the second catalogue. ! In the small map, which is a photographic reproduction of a map the same size as the key map, the small dots indicate the position of all the epicentral numbers, and the large numerals ranging from | to 15, districts in which earthquakes are frequent. Districts 6 and 7 are bounded by straight lines because there was not sufficient space in which to place all the dots. For example, in District 7 all the dots indicate earthquakes which originated about the centre of this district. Until October 28, 1891, the disturbances in this district were not more numerous than they are in District 8. When an earthquake has been felt at the extremities of the Empire, and at the same time not along a great length of coast line, as in Districts 1 and 10, it is often difficult to determine the direction or distance from ‘ the coast line of its origin. In these cases the assumption made has been that the shocks just reaching the coast have originated from about the same locality as the larger shocks which have spread some distance along the shore line, these stronger disturbances being severe at places just reached by their feebler successors. The signs + and — along the coast line indicate that near these places there are evidences of secular elevation or depression. This information was obtained by the help of Professor D. Kikuchi, who kindly assisted in the distribution of a circular to various towns and villages round the coast of the Empire inquiring whether from maps, traditions, or observations there were reasons to believe that changes had taken place in the relative position of the land and water. The large black dots on the map indicate the positions of more or less active volanic cones, in the neighbourhood of which there are huge bosses of voleanic rocks and many ancient craters. The dotted lines show the boundaries of provinces, which are usually the ridges of high mountains dividing one seismic region from another. If analyses of this catalogue show that it is of any value, it is clear that several advantageous changes may be made in a system for its con- tinuation. As it stands it is only a tentative effort to provide investi- gators with a new kind of data, which may lead to investigations not hitherto possible. None of the facts, excepting a few of the time obser- vations, claim any great degree of accuracy. The object of the list drawn up for me by Dr. E. von Rebeur-Paschwitz is explained in the next section. The long list of corrections, additions, and suggestions at the end of the volume, inasmuch as they have, so far as possible, been inserted in the second catalogue, almost entirely refers to the first catalogue. Although they show that actual errors occur in work of this description, they also show that from given data different persons may arrive at different results. 1 The unit is 10 geographical miles. a a re ee ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 153 (ec) Object of the Catalogues. The principal object of the catalogues, as we have indicated, is to furnish investigators with a certain quantity of material relating to the occurrence of earthquakes, different from that which has hitherto been at their disposal, on account of the want of which it has been impossible to make many desirable inquiries. Many catalogues exist, like those of Perrey, Mallet, Kluge, de Bal- lore, and Fuchs, in which the actual number of records are equal to, or greater than, the number of earthquakes now noted, and which are equally good as foundations for a particular class of investigations. The incompleteness of these catalogues, however, is seen in the fact that they give for the whole world a frequency less than the present list gives for a small portion of it like Japan. If, for example, we take Dr. C. W. C. Fuchs’ ‘Statistik der Erdbeben,’ 1865 to 1885, giving a list of some 8,000 disturbances, out of these Japan is credited with from three to thirty shocks per year, while a truer estimate would have been from 500 to 1,000. Again, it is often difficult to distinguish between shocks which have shaken a few square miles and those which have disturbed an empire. Large shocks and small shocks, primary shocks and after shocks, are with difficulty separable, and no data have been available enabling an investi- gator to separate disturbances arising from the yielding of strata in one area from those due to fracturing which might take place in a neighbour- ing region. Even when the lists of a particular observatory have been examined by themselves, inasmuch as its records are those of shocks of local orgin combined with those of shakings which originated at distances of several hundreds of miles, all that we can expect to find is a relation- ship between earthquake occurrence and influences of a widespread character. Such investigations have been made for the records of obser- vatories, countries, and the world, with the result that a more or less pronounced annual and semi-annual periodicity and traces of what is apparently a lunar influence have been discovered. No doubt many and very just objections may be made as to the aceuracy of much of the material in the present list; but because it enables us to give approximate weights to the different shocks, to dis- tinguish between primary and secondary disturbances, and to divide the country to which it refers into distinct seismic or natural districts, it is to be hoped that it will open the way for investigations along new lines. Although the catalogues suggest several investigations hitherto impos- sible, inasmuch as it so often happens that one inquiry becomes the parent of another, it is impossible to indicate all the paths which may be followed. A suggestion given by the list, which shows that shocks originating in Japan have travelled to Europe, is that a ring of twelve or twenty-four stations situated round our globe would in a very short time give us valuable information, not simply about its crust, but possibly also about its interior. One set of investigations which may possibly lead to interesting results will be those relating to the frequency and periodicity of earth- quake shocks which may be considered as having equal values, or receive values relative to the area they have disturbed. Each of these analyses may be made for Japan as a whole, or for special seismic districts ; in the former case the object being to determine whether the occurrence of 154 REPORT—1895. earthquakes is dependent upon influences which simultaneously affect Japan as a whole, and in the latter case to determine how far their frequency may be related to phenomena of a more local character. As an example of an influence which affects Japan as a whole, the difference in the summer and winter barometrical gradients crossing the country may be taken, while tidal loads along the coast would be expected to produce effects in different districts at different times. Not only is it open for us to determine effects due to external influences, but these, so far as possible, must be distinguished from effects resulting from internal conditions. The great frequency in District 7 was entirely due to the shocks succeeding a terrible disturbance which took place on October 28, 1891; and if these after shocks, which at first occurred at the rate of 1,700 per month, and which apparently result from the settlement of disjointed strata, are included in any general list, it is clear that they might accentuate or destroy any law respecting a long period frequency. What is true for District 7 is also true for District 11. By themselves they yield information about the rate at which an enormous quantity of broken-up strata settles to a state of equilibrium, and because the district around the epicentrum is for some time after the primary . disturbance in an extreme state of seismic sensibility, it is quite possible that there may be fluctuations in the rate at which quiescence is ap- proached, due to external influences. Other problems which suggest themselves are the possible relationships between the seismic activity of the various districts, the times taken for different areas under the influence of secular movement to attain varying degrees of seismic sensi- bility, and the connection between earthquake occurrence and the geotectonic character of the country. If the object of an analysis is to discover a relationship between earthquake frequency and exogenous phenomena which recur at long intervals, it would seem advisable to omit long lists of after shocks, and only to take into consideration disturbances which occur in districts where seismic activity is in a normal state. On the contrary, should we seek a relationship between the occurrence of earthquakes and phenomena which recur at intervals of not more than a few days, as, for example, barometrical fluctuations or the rising and falling of the tide, this precaution is hardly necessary. Rinse District High Water, Full ; | 7 end Change | h, Nemuro : 1 4. 299 Tsugaru Strait . 2 | Siren Hachinohé 3 4 40 Yamada 4 4 15 Kinkasan 5 4+ 30 Tnuboye-saki 6 5 45 Yedo Bay . | 6 5-45 Mia-ura ) 7 6 00 Kii Channel 8 6 00 Bungo Channel : ‘ : : ; ail 9 6 00 Kagoshima Bay : 2 : ; A al 10 6 50 Shimabara Gulf ; 5 ; , : 5 14 Co aye | Idzumo Coast . , . : . a 12 1°20 Echizen Coast . ; , ‘ ; ‘ D4 13 2 00 Toyama Bay. ; : é ; ‘ ; 14 3 06 Off Niigata : ; : . . ‘ , i} 2), bp ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 155 For the latter investigation, the most desirable lists to use would be those referring to shocks originating beneath the ocean or along the sea- board, and as an assistance to this I give the preceding table, showing the times of high water at full and new moon on the coasts for the fifteen seismic districts shown in the small map. Nothing has been said about the possible relationship between earth- quakes and volcanic eruptions, first, because we have no reason to believe that, with the exception of a few feeble shocks which may precede or accompany an eruption, there is any marked direct connection between these two phenomena, and secondly, because the present catalogue does not extend over a sufficiently long period of years to lend itself to such an investigation. Although one or two new investigations have been here suggested, the principal work will be a repetition of old analyses, taking advantage of the fact that we are now able to deal with natural districts, to give carthquakes, where required, relative weights, and to distinguish between after shocks, the occurrence of which is but little influenced by epigenic actions of long periodicity, and those of a district where seismic strain is in a normal condition. As to whether seismology will be advanced by carrying out these and other inquiries which may present themselves is a question which cannot yet be answered. It may be or it may not be, but the catalogue, which could not have been compiled without the generous assistance of the Royal Society of London and the kindness of the director and officers of the Imperial Meteorological Department of Japan, by allowing access to their unequalled store of valuable facts, will, it is hoped, settle the question as to whether it is desirable to continue in its present form the largest and probably the most perfect seismic survey which has hitherto been attempted. I am glad to say that some of the features presented by the catalogues are now being analysed by Dr. C. G. Knott, of Edinburgh. (d) Results already obtained or shown by the Catalogue and Map of Centres. After Shocks.—About the time that the catalogue was commenced, Mr. F. Omori undertook an examination of the shocks succeeding the great earthquake of October 28, 1891. which are now indicated upon the map in District No. 7. This he did, following up the in- vestigation oy an analysis of the disturbances since 1889 in District 11, a series which recently occurred in District 10, and another series belonging to a region lying between 8 and 9, which, although now quiescent, about forty years ago was unusually active. As an outline of Mr. Omori’s investigations is published in the ‘Seismological Journal,’ vol. iii. p. 71, and in greater detail in the ‘Journal of the College of Science,’ vol. vii. Part II., it would be out of place to give any detailed reference to them here. Briefly, it seems that when a large disturbance is followed by a long series of after shocks the number of these is roughly proportional to the area first shaken, or what may provisionally be called the intensity of the initial impulse. The character of the curves which represent the frequency of the after shocks in relation to time is remarkably similar, and having determined by observation the form of the earlier portions of a frequency curve, it seems possible to roughly 156 REPORT—1895. calculate, not only the number of shocks which will be experienced before the district settles to its normal state of seismic activity, but also the interval of time that will be involved in such an operation. For the earthquakes considered by Mr. Omori it may be concluded that the earth’s crust had been so far fractured that there was an approximate similarity in the heterogeneity of the disjointed material, which there- fore, as it settled, gave rise to after shocks following a somewhat similar law. Another observation was that the larger of the after shocks travelled to greater distances than their smaller companions, and in con- sequence there was a marked difference in frequency at places situated at different distances from the primitive origin. If there is any law in this decrease in frequency with distance, then the frequency of what are evidently after shocks observed upon a coast line, as in Districts 1 and 10, might enable an observer to make a rough estimate of the distance of an inaccessible submarine origin. That satisfactory results would be obtained from such an investigation is, however, doubtful. Distribution of EHarthquakes.—An inspection of the map of earth- quake origins or centres shows that the central portions of Japan, which are the mountainous districts where active volcanoes are numerous, are singularly free from earthquakes. The greater number of disturbances originate along the eastern coast of the Empire, and many of these have a submarine origin. That very few earthquakes are shown on the coast line between Districts 1 and 2 isin a great measure due to the fact that in this region there are but few observing stations, the island of Yezo in which these districts are situated being sparsely populated. A line drawn from N.N.W. to 8.S.E., or from numbers 7 to 557, is the chief anticlinal axis of the northern island, and from the southerly prolonga- tion of this beneath the ocean, earthquakes from time to time originate, which shake, not only the eastern coast of Yezo, but also many of the districts on the main island. Although districts like 11, 9, 8, and then through 7, suddenly northwards up to 13 or 14, lie along the strike line of the southern portion of the Empire, a greater number of earthquakes seem to originate from the face of the steep monoclinal slope which Japan presents towards the Pacific Ovean. Lines, 120 geographical miles in length, running in an easterly or ssouth-easterly direction from the highlands of Japan into the Pacific Ocean, like similar lines drawn from the Andes westwards into the same ‘ocean, have a slope of 1 in 20 to 1 in 30, and in both of these districts earthquakes are frequent. On the contrary, along the face of flexures which are comparatively gentle, being less than half these amounts, which may he seen along the borders of most of the continents and islands of the world, earthquakes are comparatively rare. The inference from this is that, where there is the greatest bending, it is there that sudden yielding is the most frequent. In the case of many of the Japanese earthquakes, this takes place along the face of a monoclinal feature of the world’s surface, and the intimate relationship between monoclines and faults is known to all geologists, the former being, in the words of Sir Archibald Geikie, an incipient stage of the latter. Earthquakes and Secular Movements.—Another feature indicated by the map or known to the writer from personal observation is that earth- quakes are frequent in those districts where there are evidences of secular elevation or depression, that is to say, in those districts where movement “of the earth’s crust is yet slowly taking place. lt tle ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN, Toa Tn Districts 1, 2, 5, 6, and 7 the writer knows from repeated observa- tion that there are evidences of very recent elevation, and certainly in these districts earthquakes are extremely frequent. The signs + and — in the neighbourhood of Districts 8, 9, 11, 12, and 13, and along the Inland Sea, lying to the north of 8 and 9, but to the south of 12, also show a like relationship. The only exceptions to the general rule appear to be the westerly portion of the district between 12 and 13, where there are evidences of secular movement, and earthquakes are of rare occurrence, and 1 in 5 cases where these conditions are reversed. The district No. 14 presents a series of earthquakes originating along the line of a valley between high mountains running from N.N.E. to 8.S.W. Another good example of earthquake fracturing following a line of weakness down a valley between high mountains until it reached the plain was the disturbance of October 28, 1891, which, as has been explained, resulted in the abnor- mal conditions shown in District 7. In Japan, therefore, earthquakes have been frequent along the steep monoclinal face of the country, in the synclinal trough of deep valleys, possibly along the continuaticn of the Yezo anticlinal, and in districts where secular movement is in progress. In Italy earthquakes originate along tiie anticlinal of the Apennines, and from what we know of the geological history of the country, which had its greatest growth in Tertiary times, and from the bradyseismic movements on the coast, it is not unlikely that the shakings it experiences announce the fact that secular yielding is yet in progress. The earthquakes of Switzerland and those which shake the Himalayas, and the younger mountains of the world, may also be taken as due to orogenic causes which seem to be so actively in operation in Japan. ‘ Earthquake Sownds.—A. map which has been prepared, but which has not been reproduced with the catalogue, shows the distribution of earth- quakes accompanied by sound phenomena, ‘To indicate that a sound was heard, a dot is used, for a sound with a shock the sign +, for a sound before a shock the sign—, while for a sound after a shock the sign | . After a volcanic explosion it might be expected that a sound wave propagated through the atmosphere would succeed a trembling of the ground. As the latter sign occurs but seldom, although there are one or two cases of its occurrence in Districts 6, 7,12, and 14, generally near active or old volcanoes, and about two cases in District 8, it may be assumed that earthquake sounds, rather than representing atmospheric waves radiating from an epifocal area, represent elastic vibrations transmitted cenaee the ground, and therefore arrive at a given station in advance of any quasi-elastic surface undulation. Inasmuch as earthquake sounds only travel a few miles from their origin, the intervals between them and an earth movement which can be felt are very small. The result of this is that it often appears that the two phenomena are simultaneous, and therefore on the map we find nearly as many signs indicating ‘sound with shock’ as those which indicate ‘sound before shock.’ Sounds are often. \izard which cause people to run from their houses, expecting a shock which does not come. The dots on the map represent sounds which have been to ordinary observers simultaneous with an actual shaking of the ground. Taking the districts in order, we find tke sound phenomena distributed as follows :— 158 REPORT—1895. 1. Sounds fairly frequent on the coast at the most easterly and most southerly portions of the district. Iniand and on the northern coast they are rare. This may indicate that the majority of earthquake origins le to the 8.E. and are submarine. 2 and 3. Sounds are rare. Many of the origins of these shocks are submarine. The coast between 2 and 3 is composed of soft materials. 4 and most easterly part of 5. Here the coast is rocky, built up of Paleozoic strata. Sounds are fairly frequent. In the southern part of 5, where there is much soft Tertiary material, sounds are rare. 6. Sounds are frequent in the northern part of the district, which is mountainous, while in the plain of Musashi, constituting the southern part, they are rarely heard. 7. Amongst the Paleozoic hills of the district, and extending down into the plain, sound phenomena accompany about 30 per cent. of the disturbances. 8 and 9. Although the districts are mountainous, sounds are rarely heard. Possibly the shocks originate beneath the ocean. 10, 11, and 12. Sounds are fairly frequent. 13. Here, which is another mountainous region, sound phenomena _are common. 14. Sound is occasionally heard. 15. Along a sandy coast bordering a plain, sound phenomena seem never to be heard Generally sound is heard in rocky mountainous districts, while on the alluvial plains it is but very rarely observed. Earthquakes which have been propagated to Europe.—The object in appending to the catalogue‘a list of earthquakes which was kindly drawn up for me by Dr. E. von Rebeur-Paschwitz is to show that some of the Japanese disturbances have travelled as far as Europe, where for minutes or hours, although they were unfelt by persons, they caused movements in delicately adjusted horizontal pendulums. A similar series of unfelt disturbances originating in distant countries or beneath the oceans have been recorded in Japan. TV. ON THE VELOCITIES WITH WHICH WAVES AND VIBRATIONS ARE PROPAGATED ON THE SURFACE OF AND THROUGH Rock AND Eartu. (A Compiation.) Introduction. Because the observations which have been made upon the rate at which waves and vibrations are transmitted through rock and earth are so varied and oftenapparently contradictory, it has been thought advisable to select from the vast amount of material which is at our command a series of illustrations from experiments upon artificially produced disturb- ances, and from the records of actual earthquakes in which personal and instrumental errors have been small. Amongst the real or apparent difficulties are the following :— 1, Along the same path, earth waves, originating from a powerful ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 159 impulse, travel at a higher rate than those resulting from an effort of lower intensity. 2. Near toan origin, the velocity of propagation is greater than it is between points at a distance. 3. After a disturbance has decreased in its speed of transmission it may be accelerated, and this acceleration cannot be with certainty attributed to its having entered a more elastic medium. 4. As an earthquake radiates, it is preceded by a series of minute tremors, the velocity of propagation of which is certainly very much higher than that of the main disturbance. (a) Artificially produced disturbances. 1, Experiments of Mr. R. Matter, In the experiments of the late Robert Mallet conducted at Killiney Bay, Dalkey, and Holyhead (‘ British Association Report,’ 1861) the initial impulse was caused by the explosion of charges of gunpowder. The electrical contact which caused the explosion released a chronograph which was stopped by an observer directly he saw, by means of a microscope magnifying 11°39 times, an agitation caused by the resulting wayes ina dish of mercury. After corrections for the intervals of time thus noted, in round numbers the results obtained were as follows :— In wet sand , . : : 5 . 0°251 km. per. sec. In discontinuous granite . 5 . « SOBOS 5 Saas In more solid granite : 3 ; « “ODD: = Spares id In granite at Holyhead (mean). d oh) ORE, ee aS The charges of powder employed varied between 25 lb. and 12,000 Ib., and with but one exception it was clearly shown that the velocity of wave propagation increased with the force of the initial impulse. For example, at Holyhead the relationship between the quantity of explosive and the _ resulting velocities was as follows :— 12000 Powder in lb. . | ) 2100 2600 | £200 | 4400 | 6200 2. Lxperiments by General HW. L. Anzor. In 1885 when Flood Rock was destroyed by the explosion of 240,597 lb. of rack-a-rock and 48,537 lb. of dynamite, the most distant observing station was 182-68 miles off. The instant of the explosion was noted at all the points of observation by means of electrical connections and chronographs, while the arrival of the first tremors and their duration ‘was recorded by observers who watched the disturbance of an image reflected from the surface of mercury. The Hallet’s Point observations, where the initial impulse was due to the explosion of 50,000 lb. of dynamite, and others made in connection with subaqueous explosions at the school of submarine mining at Willet’s Point, were conducted in a somewhat similar manner. In the following table, which has been drawn up from the scattered writings of General Abbot, the velocities have been reduced to uniform units :— 160 REPORT—1895. - «| Magnifying | Mercury in Pr +e Diane in power of | agitation velorke ees telescopes sec P v 1 Flood Rock ex. 288,934 Ib. aft Ss 4 80 11,577 m. eet ee explosive. ; 2 ; . 16:78 14 104 4,086 m. H 2. 3 E: * 36°65 18 35? | 4,537 m. $ i 4 “ e 48-52 Cr ie 5,068 m. i 3 5 i: » | 14489 154 | 74 |3,958 mn. - ‘ 6 s 5 | 182-68 750) | 95+ | 1,335 m. is * 31 76 ~=—-| 5,008 m. ( x ‘ i: 7 ’ » | 48t |) 16 | 70 | 6,248 m. { eee DNEE rictag: pe) | eae 6,243 m. | aS 8 Ks i. eae OA A OE meee alice s 3 Hallet’s Pt. ex.) | . : 9 50,500 Ib. dy- | 513 6 och LeGSiqe \t,180m: 1 Rbraueh lay ans) namite. ) | : | S Through water & 10 + 3 8°33 12 | 72 | 2,530 m. shore of East | | river. i F 4 0-33 6 231,378 m. { i oak a 12 uf eg erasers 12 19 1,618 m. e $ 13 400 lb.dynamite.| 1:17 6 8 1,045 m. ey ss iain S. " 1:17 12 18 | 2,686 m. “ 2 115 200 ,, B 1:34 6 9 | 2,051 m. sf ’ 16 4, 55 ¥ Tea Nate alle 17> |/2:669 ms ¥ s yt ere: ‘, 5a 12 1,609 m. ‘ “s 18 701b. powder. | 140 | 6 inst. | 878 m. | Hae g 3 a gma aber 6 6 | 1,694 m. | aed Aa hi . 1°34 12 15 2,565 m.| Vater From the above data it is clear, as Abbot shows, that the rate at which a shock is transmitted increases with the intensity of the initial explosion ; that when a high magnifying power has been used, tremors in advance of those revealed by a low power have been noticed, with the result that the apparent velocity in the former case is greater than in the latter ; and that the velocity of propagation has been higher through rock than through soft material like drift. A query put forward by General Abbot is whether still higher velocities would have been recorded had telescopes with a greater magnifying power been used. The answer is apparently in the afliirmative, and therefore if we wish to compare the observations amongst themselves, not only must we choose those in which the initial impulse has been the same, but where the observers have employed similar instruments. Comparing observations 10 and 12, but not overlooking the fact that No. 10 was largely transmitted through water, and again 16 and 17, it might be concluded that as a wave advances its velocity is diminished ; but from the first five observa- tions it would seem that there is at the commencement an increase in the initial velocity until it reaches a maximum, after which there is a diminution. This increase in the rate of transmission at the outset of a wave from its origin is again seen in experiments 9and 11. The difference in the velocities recorded for experiments 18 and 19 may be due to the fact that in the case of the shallow torpedo much of the initial energy was ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 161 expended in throwing up a jet of water 330 feet in height into the air. A point well worthy of notice is the fact that the gunpowder waves had a more gradual increase than those observed in shocks produced by dynamite ; in other words, the former had a closer relationship to what is so often observed in the records of actual earthquakes than the latter had. 3. Experiments of MM. Fovaut and Livy. In the experiments of MM. Fouqué and Lévy the velocity of vibrations on the surface and underground was determined by recording the intervals between the shock which was usually produced by the explosion of from 4 to 8 kilos. of dynamite, and the displacement of an image produced by a ray of light on a photographic plate moving with uniform motion. The ray of light was reflected from a surface of mercury at the receiving station. The highest velocity was obtained between a point underground and the surface, along a line of 383 metres in length, which gave a velocity of 2,526 metres. In this case the shock was due to an explosion of 8 kilos. of dynamite. The general results obtained were as follows :— Character of Ground | x et et edn ea ae ee m. m. m. m 1. In granite on the surface . , ; wh 2.450 tors. 141 | 219 — 108 _ | 2. Underground to surface and underground | to a greater depth. : : é 2 2,000 to 2,526 || 1,212 — 440 3. In grés permiens not so compact ; Sh 0: | = 4, In limestone from surface to underground | 632 | = f 5. In sable de Fontainebleau . . : d | 300 — The velocity evidently increased with an increase in the amount of explosive employed, and it was greatest in the more elastic rocks. _ The discrepancy which exists between the above and Mallet’s deter- mination for granite (507 m.) only disappears if we compare it with the second maximum in the photographic record (325 m. to 543 m.). _ The second set of experiments, considering the nature of the material in which they were obtained and the smallness of the charges employed, ive remarkably high results, the velocity for the first maximum exceeding that obtained by firing a larger charge of dynamite in granite on the surface. In a single experiment to determine the velocity between a lower and a higher level underground, the direction of the wave path is unfortunately not very different from that of the stratification, and there- fore is not comparable with those velocities along paths from the upper level nearly transverse to the stratification between it and the surface, If we are allowed to accept the results of Mallet’s experiments, which show that the velocities in these two directions are in round numbers as 18: 1-0, then we may conclude that the velocity between the lower level and an upper level was markedly greater than it was from the latter upwards to the surface. These experiments show that the velocity between two points on the surface is less than it is between the surface and a point underground. They also indicate that the velocity with which vibrations are transmitted may vary with the depth of the wave path. 1895, M 162 REPORT—1895. 4. Observations of Prof. J. Mitne and Prof. T. Gray. In the author’s experiments, which were commenced in conjunction with Professor Thomas Gray in 1881, and continued at various times during the next four years, the object was not simply to determine the rate of transmission of earth waves, but also to determine their general character. Usually the movements resulting from the fall of a heavy weight, or the explosion of dynamite or gunpowder, were recorded by seismographs. The weights employed varied from 1,710 Ib. to 2,000 Ib., while the charges of dynamite, which were exploded in holes 8 or 10 feet in depth, seldom exceeded 2 1b. Although the ground in all cases excepting one was soft, the resultant vibrations up to distances of about 600 feet were sufficiently large to be recorded as clear diagrams by bracket and other seismographs. At various stations usually in a straight line joining them with the focus of the explosion, seismographs were installed, which wrote their movements on the smoked surface of a long plate of glass, the motion of which was controlled by clockwork. One seismograph was placed so that it wrote the movements parallel to the line of installation. These are called normal vibrations. A second seismograph was arranged to record the movements at right angles to such a direction. These are called transverse vibrations. A vertical lever seismograph was occasionally employed to give the vertical motion. A fourth pointer actuated by an electromagnet in connection with a short pendulum swinging across mercury gave a broken line marking small but equal intervals of time. By the depression of a contact key, the receiving plates at all the stations were set in motion, the pointers of the seismographs drew fine straight lines on the smoked surfaces, while the pendulum indicated intervals of time. A few seconds later a second contact was made and the charge exploded, and the seismographs gave open diagrams of the resulting vibrations. When the earth motion had ceased, all the plates were stopped and were ready to receive a second diagram without any readjustments. One observer controlled all the stations, and the only errors due to human interference may have arisen from slight differences in the sensibilities given to the recording instruments. This, however, disappears when velocities were determined, not from the commencement of a disturbance, but from the sharp commencement of the violent vibra- tions or from the intervals of time between the appearance of particular waves at the different stations. Observations were also made with seismographs having single indices by observing the disturbance created in similar dishes of mercury, and with other arrangements. The results of observations made respecting velocity of propagation were as follows :— 1. The velocity of transit of vertical vibrations near to an origin decreases as a disturbance radiates. Normal vibrations, although they have shown a decrease in velocity between the second and third stations, have also shown a decided increase. This latter observation has been marked with the transverse motions. 2. Near to an origin the velocity of transit varies with the intensity of the initial disturbance. 3. In different kinds of grounds, with different intensities of initial ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 163 disturbance, and with different systems of observation, I determined velocities lying between 630 (192 m.) and about 200 (61 m.) feet per second. 4, In my experiments the vertical free surface wave had the quickest rate of transit, the normal being next, and the transverse motion being the slowest. 5. The rate at which the normal motion outraces the transverse motion is not constant. 6. As the amplitude and period of the normal motion approach in value to those of the transverse motion, so do the velocities of transit of these motions approach each other. (6) Observations on Earthquakes. The observations quoted in this section commence with those where the wave paths have not been more than a few hundred feet from station to station. These are followed by the results obtained from instruments separated from each other by distances of from three to six miles, a few hundred miles and so on up to velocities determined over paths equal to a quarter of the earth’s circumference. 1, Observations in Japan. i For several years the author took diagrams of earthquakes at seven stations, each about 900 feet apart. These stations were in electrical connection, so that one pendulum marked time intervals upon each of the moving surfaces upon which diagrams were being drawn. From fifty sets of diagrams, representing fifty different earthquakes, it was only in five nstances that the same wave could be identified at the different stations. The result of these identifications led to calculation of velocities of 1,787, 1,302, 1,825, 869, and 501 metres per second. _ Even these determinations cannot be accepted without reserve, because it is found that waves may spread out as they pass from station to station, a given wave splitting up into two waves, &c. Hence «@ velocity calculated from a wave (a) may be different from a velocity of a wave (b), and yet both are part of the same disturbance. In the diagram from one station a large wave may have a slight notch _upon its cr est, at rd station it is so large that the single wave appears as two waves. As in the artificially produced disturbances, although an earthquake becomes feebler as it radiates, it apparently increases in its duration. _ The same system of observation has recently been elaborated in Japan, but the distances between stations have been increased to several Riles. Because the commencement of a disturbance at a given station ‘varies with the sensibility given to the seismograph, the determinations of velocity depend upon the identification of particular waves upon the diagrams obtained from at least three stations. Up to the present this has only been possible on one or two occasions. On November 30, 1894, at 8.30 p.m., a velocity of 5 km. per second was obtained, other dis- _ turbances giving from 2-4 to 36 km. per second. The following are examples of velocity determinations made in Japan Berean stations which have access to the telegraphic system of -the country, and which are provided with seismographs and clocks which M2 164 REPORT—1895. automatically record the time at which a particular vibration was drawn. At each of the observatories it is therefore possible to calculate the instant at which a given instrument commenced to write its record. In 1891, on December 9 and 11, strong shocks originated in the province of Noto on the west coast, which were observed in Gifu, Nagoya, and Tokio, The mean velocity determined from these records was 2°31 km. per second. The destructive disturbance of October 28, 1891, which was recorded in Europe, was followed by many after shocks, the times of arrival of seventeen of which were accurately noted at Osaka, Nagoya, Gifu, and Tokio. The origin of the main shock was about five miles to the west of Gifu. To reach Tokio, a distance of 151 miles, took 120 seconds. The average time taken for all eighteen shocks was 118 seconds, and the average velocity was 2:40 km. per second, the rate of transmission to Osaka being the same as it was over the much longer path to Tokio. The primary disturbance seems to have reached Shanghai at a rate of about 1°61 km. per second, and Berlin at about 2°98 km. per second. For the Shonai shock on October 22, 1894, as a mean obtained by the method of least squares from observations at ten stations from 60 to 300 miles distant from the origin, a velocity of about 1:95 km. per second was obtained. Giving these last determinations, all of which were computed by Mr. F. Omori, weights proportional to the number of observations each represents, the average rate at which disturbances are propagated over long distances in Japan is 7,560 feet, or 2°3 km. per second, a rate which fairly well agrees with that at which the large waves of similar dis- turbances travel from Japan to Europe. 2. Observations along Wave Paths of Great Length. Next we will turn to earthquakes which have been noted at distances from their origins greater than those at which it has been possible to observe in Japan—a notable example of which are the observations made at the time of the Charleston Earthquake on August 31, 1886. Over 400 observations were made. A number of these were obtained from clocks which had been stopped, and as many of these were regulators which had daily been compared with a time signal, there is no reason to doubt their accuracy. All these observations, which were made on wave paths between 300 and 924 miles in length, were subjected to a rigorous analysis by Professor Simon Newcomb and Captain Charles Dutton, with the result that an average velocity of 5,184 m. was determined, and there was no indication of any sensible variation in speed. Considering the phase of motion which in the majority of instances was in all probability observed, this result 1s remarkably high. A valuable study of the rate at which vibrations may be propagated through the earth’s crust is one made by Dr. G. Agamennone of a series of shocks which in 1893 had their origin near to the island of Zante. These were recorded at the various stations mentioned along the foot of the diagram Fig. 15, the one farthest from the origin being Potsdam. The lengths of the various wave paths are indicated in kilometres. The time intervals measured vertically are on a scale of 20 seconds per millimetre. For five shocks straight lines connect a series of points indicating the differences in time between the occurrence of the shock near to its origin f ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN, 165 Sand the time at which maximum motion was experienced at the various _ stations. The dotted lines connect similar points for the commencement of the disturbance. The time of these commencements undoubtedly varied with the sensibilities of the recording instruments, and therefore it will be noticed that they have only been taken into account for Rome, Nicolaiew, Fig. 15. Ewe El ae as ‘OT Pe ee | ae Bis Ee ees NES Pee AS 3 ~ S ~ Ss waiag we ied waa ae Zant ot pt Renee CALTASSO . ES ey ane . IN Ss 8 & erie) Catlama in eel LAE \ Corfia Moneo Denevento Roma Fadova = Mota SG. PUTO Lotsdainr Strassburg, where records were obtained from the great pendulum of Collegio Romano, or from the horizontal pendulums of Dr. E. von eur-Paschwitz. __ The principal object in reproducing this series of observations is to see _ if there is any reason for believing that there is any variation in the velocity with which a given disturbance is propagated. 166 REPORT—1895. In examining this diagram it must be remembered that near to an origin the difference in time between the maximum phases of an earth- quake and its actual commencement may be only a few seconds, while at a great distance the records of sensitive instruments show that the same interval may be many minutes. When instruments of such sensibility are near to an origin, my own observations seem to show that they are not set into any sensible amount of motion before the ordinary seismo- scopes or seismographs, and therefore for places comparatively near to the origin of a disturbance, when observations were made with the latter type of instrument, I should be inclined to think that the phases of maximum motion might be approximately coincident with the times of commencement of movement. An inspection of the diagram pomts towards the following results :— No. 1. The velocity for the first 550 km. is greater than it is toa point which is more remote. No. 2. This is the only disturbance for which observations are made at points comparatively near to the epicentre, for which they show a very high velocity. Between stations distant 300 and 1,100 km. from the origin the velocity decreases, but beyond this limit it apparently increases. No. 3. The chief difference between this and No. 2 is that the point of inflexion of a free curve drawn between the points of observation, instead of being at a distance of 1,100 km. from the epicentre, is at about 1,500 km. from that point. No. 4. The velocity is apparently greater at a distance from the epi- centre than near to it. No. 5. This resembles No. 4. If we omit the one case which shows a high velocity in the immediate neighbourhood of the origin—which, however, is in perfect accordance with results obtained with artificially produced disturbances—there remains the clearly marked observation that to Catania and Mineo the velocities are, as compared with the rate of propagation to more distant stations, relatively low. Professor A. Ricco, who discusses these observa- tions, gives us every reason to believe that the time observations at Catania are correct, while those at Mineo may be in error, owing to the manner in which it receives the time signals from Rome, which finally reach the observatory by circolare. Professor Ricco concludes that the low velocity between Zante and Catania may be accounted for by the fact that the motion was entirely transmitted through water, because the velocity recorded of 1,439 km. per second practically coincides with that of 2 sound wave in water. Professor Ricco adds that Bertelli has shown that the shocks of earthquakes felt on shipboard and the sound waves have been simultaneous. From one of Abbot’s experiments, however, we have seen that a wave velocity obtained from a water path was greatly increased. The following is Agamennone’s table of velocities, which, although they represent averages, show that the lowest is the one on August 4, which had the shortest range :— a tee lh i ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 167 Velocity of Velocity of No. of af clots oh) No. of | Max. Motion No. of Commence- Date Stations Waaed out wh Stat ons based on cer- | Stations | ment of Motion con- Pishndatlons con- tain Obser- | con- at Certain sidered or ‘| sidered vations. | sidered Stations. Km. | Km. | | Jan. 3L ‘ 7 4:04 4 | 2°86 4 3°08 Feb. 1 6 3°28 4 2°42 4 3:92 March 20 . 5 2°33 3 | 2°82 3 Cle0, April 17 10 2°55 5 | 2°59 5 3°16 August 4 3 2°12 2 | 2°36 2 2°83 Mean t — 2-40 Seis | 2°45 — 2:34 | The averages of velocities to the Italian stations and the actual veloci- ties to Mineo and Catania, which may be compared with the first deter- mination in the preceding table, clearly show that the apparent velocity to the nearer stations was lower than it was to stations which were more distant, :— Italian Stations. Mineo. | Catania. a Kn. ims | Km. January 31 5°76 83 114 February 1 4-26 2-04 1:43 March 20 : : : : Es) 1°86 Wr 1°98 ee i oF 2-09 ‘96 1:20 August 4. 212 3°05 — Dr. A. Cancani, who has devoted much attention to the velocities with _ which earth disturbances are transmitted, is apparently inclined to attri- bute the high velocities sometimes observed near to an epicentre—which, however, is not the case with those just quoted—to the more rapid transit of a longitudinal wave. He, however, adds that at such places, and even at distant places, the normal and transversal waves may occur together, and the velocities determined on such occasions will have intermediate values. In fairly homogeneous earth it has been shown that, within 100 feet or so from the origin of an artificia! disturbance, a normal move- ment outraces the transversal disturbance, but such a separation is not observed, nor should we expect it to be observed, at distant stations (see pages 162 and 163). When Dr. Cancani quotes my opinions that ‘velocities of 2 or 3 km. per second refer to the propagation of a motion not unlike the swell upon an ocean’ as not being contrary to his ideas, it must be clearly under- stood that I do not refer such movements to the purely distortionai elastic waves of an isotropic solid.! Amongst other observations quoted by Dr. Cancani to show that the velocity with which earthquake waves are propagated is higher nearer to an epicentre than at a distance, I select the four following, which have reference to the Andalusian disturbance of December 25,1894 :— To Lisbon, distance 530 km. velocity in km. per sec. 4:2 ;, Pare St. Maus, Pe 1.350 3 os pa 3:2 4, Greenwich, Fe. 1,620 ae a * 3°6 3, Wilhelmshaven, 5 2,000 ix a a 28 1 R. Accad. dei Lincet, vol. iii. 1894, p. 410 168 REPORT—1895., Dr. Agamennone, after examining the data on which these tables are founded, shows that the conclusion to which they point disappears if the time taken at Cadiz by the stopping of two clocks was a minute too late, while the times at Greenwich and other observatories correspond to the beginning of the motion. From the calculations of Offret relating to the Ligurian earthquake of February 23, 1887, it would appear that the velocity of propagation increased as a disturbance radiated, but such anomalies may aiso be explained by the assumption that there were errors in the time observations near to the epicentre. As another indication of what is apparently the reverse of the results adduced by Dr. Cancani, we may take either the earthquakes of Zante or the following Japanese earthquakes, observed in Europe by Dr. E. von Rebeur-Paschwitz :— Spherics1 Ve'ocity Date Locality Distance. BMA ERD) : rea. in km. per sec. 1889, April 17 . ; ; ol eeotsdamll ase . 8,950 S20 5 Ue \s : is 2°79 Wilhe]mshaven : 9,070 | 350 1889, July 28 . ‘ é . | Potsdam . M : 8,810 2-98 : Wilhelmshaven 5 8,940 a31 1892, May 11 . ‘ . , | Strassburg - ; 9 520 3°07 Nicolaiew, I. . : 7,910 2°75 7 as : 45 2-41 1892, October18 5 . | Strassburg’ : ; 9,520 3°83 Nicolaiew. I. . ¢ 7,910 | 2°55 HF 1 ae 5 + 2°24 1892, November 4 . 4 . | Strassburg, I. . ‘ 9,520 3:15 PA I. 3 - 2°64 Nicolaiew ; 54 7,910 Pr (6 | 1893, March 23 : , . | Strassburg, I. . : 9,520 4:13 | ie II. 4 3 3°62 Nicolaiew ; A 7,910 3°72 Average . 3 : ; : . ; : : ; ‘ . 3:10 The centre of the second disturbance is taken near to Kumamoto, while that of the others as being near to Tokio. Arranging the above according to distance, we find :— 6 observations for 7,910 km. give a velocity of 2°73 5 a 8,900 rn “4 3°16 6 7 9,520 on ~ 3°41 The numeral I. refers to the greatest increase in motion, while IT. refers to the maximum itself, and it will be observed that the value for TJ. is always less than it is for I. A good series, showing the widely different results which may be obtained as to the velocities with which given disturbances are propagated, may be found in the British Association Report of the Committee on Earth Tremors for 1894. The earthquakes to which these refer are those of April 20 and 24 of 1894, which originated in North-east Greece, and which were recorded by different types of instruments at 41 different stations in Europe, the length of the wave paths being from 701 to 2,455 km. The velocities obtained vary between 1:29 and 11-71 km. per second. The high velocities are those obtained from records of the com- ON THE EARTHQUAKE AND YOLCANIC PHENOMENA OF JAPAN. 169 mencement of movement by the more sensitive classes of instrument, the records from which also give the lower values, if the arrival of the dis- turbances is taken as being the time when they recorded maximum phases of motion. As a last example of the different results which may be obtained from the same record, I take that observed at Rocca di Papa on March 23, 1894. The shock originated beneath the ocean about 70 miles S.E. of Nemuro, on the north-east coast of Yezo (Lat. 42° N., Long. 146° E.). It was observed at Nemuro in Greenwich mean time at 10.20.45 a.m. The times at Rocca di Papa and the resulting velocities were as follows :— First tremors, 10.36.0 G.M.T. 11:35 km. per sec. Decided motion, 1 Un I OS 3-06 Re Maximum motion, 11.19.0 ,, 2°69 y In Tokio it was observed at 10.27.40 G.M.T., after which four after- shocks were noted. The average time difference between the observations at Tokio and Nemuro was 6 min. 43 sec., and the difference in their distances from the origin is about 600 miles, from which an average velocity of about 2°3 km. per second is calculated. If it is assumed that the first tremors reached Rocca di Papa by direct radiation along a chord or through the earth, then their velocity may be reduced to 8 or 10 km. per second (see example on p. 149). 3. Conclusions. Very many records might be added to those which have been given, but it does not seem likely that, until we are in possession of a series of records taken at long distances apart on the surface of our globe by means of instruments which are similar, which have sufficient sensibility to record preliminary tremors, and which record upon surfaces moving sufficiently quickly to allow of accurate time determinations, that our present know- ledge will be greatly increased. Because the waves of a disturbance change in period as they travel, while one wave breaks up to form two or more waves, and this even in ground which is apparently homogeneous, a given earthquake may show as many velocities as there are waves between which we choose to make measurements. What weknow from experiments, and what we should expect from & priori reasoning, is that the rate at which a disturbance is propagated varies with the nature of the medium through which it is transmitted. Experiments have shown that the vibrations fol- lowing an artificial disturbance, where the initial impulse has been strong, travel more quickly than those where the originating cause has been feeble f also that there is apparently a higher velocity very near to an origin than at a distance. The latter phenomenon seems to find confirmation in the records of certain earthquakes. Although it may be difficult to interpret the meaning of these latter observations, when we endeavour to find an explanation for the existence of the long series of preliminary tremors which are recorded at places nearly a quarter of the earth’s circumference from an origin, and which have apparently reached these places by travel- ling at rates of 9 to 12 km. per second, the difficulties which confront us are still greater. The next section is an attempt to explain these phenomena. 170 REPORT—1895. (c) On the Probable Nature and Velocity of Propagation of the Movements resulting from an Larthquake Disturbance. If it is assumed that the crust of the earth has the character of an isotropic elastic solid, then from an earthquake centrum two types of waves may emanate. In one of these the direction of vibration of a particle is parallel to the direction of propagation of the wave or normal to its front, as in a sound wave, whilst in the other it is transverse to such a direction, or, so far as this character is concerned, it is like the move- ments in a ray of light. These two types of movements, which are respectively known as condensational and distortional waves, are propagated with different velocities, which depend upon certain clastic moduli and the density of the material. These velocities may be respectively expressed by the quantities mip aud /n/p, where p is the density of the material, 2 the modulus of rigidity or resistance to distortion, and m a modulus depending upon the modulus of rigidity and the bulk modulus or resistance to compression k, which is equal to £+3n. The first conclusion to which the theory leads is that the condensa- tional wave has a higher velocity than the distortional wave, and therefore the first ought to outrace the latter. With artificially produced disturb- ances at points near to origins in fairly homogeneous earth, a phenomenon similar to this has been observed, but whether the preliminary tremors preceding more decided movements observed at great distances represent condensational waves propagated from an origin is yet uncertain. From experiments made in conjunction with Professor T. Gray to determine the elastic moduli of granite, marble, tuff, clay rock, and slate, and the veloci- ties with which normal and transverse movements have been propagated in alluvium, Dr. C. G. Knott drew up the following table as representing average constants involved when determining the velocities with which disturbances may be propagated through fairly solid rocks :— Density " : - p=3 Rigidity : ‘A : - m=1°5x10"' C.G.S. units Ratio of the wave moduli : . » minr=3 With the above numbers the velocity of a distortional wave would be 2-235 km. per second, while the condensational wave would have a value about double this quantity. Should we accept the records made of decided movements which had their origin in Japan, but which have been recorded in Europe as representing distortional waves, then our expecta- tions based upon theory closely accord with what has been observed. On the other hand, because it has been shown that small vibrations have been noted which have travelled at rates of from 9 to 12 km. per second, the fact must not be overlooked that we are not yet in possession of sufficient constants to apply the theory to all the cases which have been observed. Even if we had the constants referring to the elasticity and density of material in the interior of our earth, when we consider the heterogeneity of the materials through which a disturbance probably passes, as Dr. C. G. Knott and other writers point out, there are serious objections to the assumption that waves with a high velocity are due to the transmission of normal motions, while those with a lower velo- city represent the less rapid transversal vibrations, At every boundary ON THE EARTHQUAKE AND VOLCANIC PHENOMENA OF JAPAN. 171 between two media different in their elasticity, either a condensational or a distortional wave is broken up into reflected and refracted distortional waves as well as reflected and refractecdl condensational waves, and there- fore as a disturbance travels through the heterogeneous mass of materials constituting the earth’s crust there is, in every probability, a continual change in the character of the motion. Not only does this consideration make it appear unlikely that the tremors which have been observed at stations far removed from an origin if they were propagated on or near to the swrface of the earth are due to condensational waves, while the more pronounced movements which succeed them represent the distortional waves, but it also indicates that at a given station there should be no definite relationship between the motion of an earth particle and the direction of propagation of an earth- quake. For feeble earthquakes, and for those recorded at points outside a megistoseismic area, this latter conclusion is remarkably concordant with observation. On the other hand, however, if preliminary tremors are movements which have been transmitted at great depths through a medium where V

) The pendulums of Hengeller, Perrot, and Zéllner, in which it lies outside them. 2. The pendulums of Gerard and Milne, on which the rod is supported by one wire and on one steel point. 3. The pendulum of von Rebeur-Paschwitz, which is supported on two steel points.’ ' In this class should be included Professcr Ewing’s borizontal pendulum seis- mograph, which, though designed for a different purpose, also records slow tilts of the ground (Zneyel. Brit. vol. xxi. p. 628). 186 REPORT—1895, Meteorological Observations on Ben Nevis.—Report of the Committee, consisting of Lord McLaren (Chairman), Professor A. CRruM Brown (Secretary), Dr. JouN Murray, Dr. ALEXANDER BucHan, Hon. RatrpH ABERCROMBIE, and Professor R. CopELAND. (Drawn up by Dr. Bucnan.) Tue Committee was appointed, as in former years, for the purpose of co-operating with the Scottish Meteorological Society in making Meteoro- logical Observations on Ben Nevis. The hourly eye observations by night as well as by day have been made uninterruptedly by Mr. Omond and his assistants during the year at the Ben Nevis Observatory ; and the continuous registrations and other observations have been carried on at the Low Level Observatory at Fort William with the same fulness of detail as during the previous four years. The Directors of the Observatories tender their cordial thanks to Messrs. C. M. Stewart, B.Sc., A. D. Russell, and C. T. R. Wilson for valuable assistance rendered as volunteer observers during the summer months for about six weeks each, thus giving greater relief to the members of the regular observing staff. For the year 1894, Table I. shows the monthly mean and extreme ‘ pressures and temperatures, hours of sunshine, amounts of rainfall, number of fair days and of days when the amount exceeded one inch, the number of hours of bright sunshine ; and this year for the first time the mean rainband (scale 0-8) at both Observatories, and the mean hourly velocity of the wind in miles at the top of the mountain. The mean barometric pressures at the Low Level Observatory are reduced to 32° and sea level, while those at the top of the Ben are reduced to 32° only. TABLE I. 1894 | Jan. | Feb. 'March April May | June | July | Aug. | Sept. | Oct. | Nov. | Dec. | Year Mean Pressure in Inches. | Ben Nevis Ob- | 24°980) 25°086, 25°192) 25286) 25°357! 25°450) 25°369! cls gt 25°665! 25°357! 25°181! aba 25°291 servatory | | | Fort Wiliam | 29°595 29°697, 29°764 29-844) 29°951, 29:960' 29-220) 29°823) 30°232) 29°915| 39°716 29°828) 29°845 Differences .| 4:615| 4°61], 4°572| 4:558, 4°594| 4°510| 4-451, 4-484) 4067) 4°558| 4°535| 4:596| 4°354 Mean Temperatures. } } | | | | ° | ° | (9) | ° } BenNevisOb-| 21-7 | 240 | 282 | ait) 24 | 382 | 433 | ab2| sf | 387) sla | 276 | sto servatory | / | . | | fae Fort William | 39°3 | 40:3 | 42:9! 484 46-9 | 54°S | 58:9 | 55-2 | 510) 456 | 46-7 | 411) 47-6 Differences . | 17:6 | 16:3 | 14:7 | 17°3.| 178] 166 | 15°6 | 160 | 13°77 | 12°9 | 15°4 | 13°5 | 15°6 Extremes of Temperature, Maxima. | \ \ / i | ° ' ° BenNevisOb-| 25-4) 362 41-2 40:3 451) 635 | 62:9) 53:9 S51 | 55:5 436 41-0) 635 servatory | | . | . ) 62°6 611 Fort William | 535 | 52:0 63-1 7 21:9 | 218) 160) 14 Differences .| 181 | 15°8 Extremes of Temperature, Minima. ° °o ° ° ° ° | ° | ° ° °o ° ° Ben NevisOb-) 0:7 | 12°3 | 17°6 | 22'8 | 1671 | 283 | 32:6 | 310 | 26-4 | 171 | 20:3 | 11-2 | O7 servatory | | | | Fort William | 20°8 | 21:5 | 287 | 33:9 | 81:7 380 | 47°38 | 42°6 | 37°3 | 245 | 31:7 | 244) 20°8 Differences .| 20°71 |° 92 111 | lll | 15°6 971 14:7 | 116 | 10:9 7-4] 114 |} 13:2 | 201 METEOROLOGICAL OBSERVATIONS ON BEN NEVIS. 187 TABLE I.—continued. 1894 | Jan. | Feb. |March| April May | June | July | Aug. | Sept. | Oct. | Nov. | Dec. | ea Rainfall in Inches. | 17-70! 1:32| 4:68) 17-40) 14:93 149-96 | ‘|Ben NevisOb- | 15°96 | 33°55 | 1458 3°50! 6°66) 833] 11°35 servatory | | | | | | | | | Fort William 11°79) 13°62 9°36 | 1:37 | 3°78} 313) 5:70) 7:72) 0:24) 2°06) 11°62) 878 79°17 | | Differences .| 4:17| 19°84] 5-221 2-13) 2°88) 5-20| 565) 9°98) 1-08| 2°62, 578) 615| 70:79 | Number of Days 1 in. or more fell. . Ben Nevis Ob- 4 11 6 1 0 3 4 6 0 1 5 oh, Oy, |S A0er servatory | Fort: William 3 3 3 0 0 1 1 1 0 0 2 2 16 Differences . 1 8 3 1 0 2 3 5 0 1 Sali 8 30 Number of Days of no Rain. Ben NevisOb- 4 2 Tay eel8 2) 10 12 |e fF | | 13 3 6 , 119 servatory | | j | | | Fort William 6 8 14,920 | 12 i9 | 12; rks 25 21 BP e it 157 | Differences .| 2 1 OF seule? 7 3 | 6 rh 2 % 1138 Mean Rainband (scale 0-8). BenNevisOb-; 2:0 27 19 | 1:9 1'8 be ed ee el a ee py eae 14 | 20 servatory | | | Fort William | 3:0 44 33 36 38 48 | 53 5-2 36 | 3°6 4-4 30 | 40 Meeteronces ©}! 1:0 | 1-70pC4 | 17.| 20] 241 28 | ay | 21 | 7 [SSP t)e | 20 Number of Hours of Bright Sunshine. |BenNevisOb-} 3 9/101 y e) 78) 117) 115 | 45 | 126 | 91 15} 28 | 810 | | _ servatory | } | } Fort William 16 2u | 132 165 ; 171 170 | 143 | 76 147 | 91 13} 16 | 1,160 | Differences . 13 11 31 | 83] 93] 53 28} al | 2k 0 —2|-12 350 Mean Hourly Velocity of Wind in Wiles. | ‘BenNevisOb-| 26 ; 19 | 18 | 19 | 11 | 10 | 12 He ede bea ate en seul bez) | servatory | | | | | | Percentage of Cloud. Nevis Ob-| 95 96 | 69 80 85 77 80 89 | 58 | 69 91 84 81 | oS | | 75 80 54 60 76 73 73 72 56 66 84 79 71 20 16 15 20 9 4 7 17 2 3 7 5 10 or 0°'8 greater than the mean of previous years, being the excess above mean at western stations in Scotland from Ayrshire to Ross-shire. ‘The mean temperature at the top of Ben Nevis was 32°:0, or 0°-9 above the mean for the same years, being thus nearly the same excess as at the wer Observatory. _ The lowest mean monthly temperature at Fort William was 39°°3 in anuary, being 0°-7 above the mean ; and at the top of the Ben 21°-7 in January, which is 2°] under the mean. This gives an unwonted large | difference of temperature between the Observatories for January, which _ Was occasioned by a comparative absence of anticyclonic weather and the relatively low temperature accompanying at the upper station, and the singular want of sunshine, there being registered for the whole month _ At Fort William the mean temperature of the whole year was 47°°6, | . 188 REPORT—1895. only three hours of sunshine. On the other hand, anticyclonic weather was of frequent occurrence in September, October, and December ; and accordingly in these months sunshine was large, being absolutely the highest hitherto recorded in September and October, and having been only exceeded in December. It will be also observed that during these months the difference of temperature between the two Observatories was much less than usual, owing to the higher temperature of the auticyclones at the top of the Ben. The highest monthly mean temperature at Fort William was 58°-9 in July, or 2°-2 above the mean ; and at the top 43°-3 in the same month, or 3°°0 above the mean. The month of greatest excess above the average was November, whose mean temperature at Fort William was 46°:7, or 4°-1 above the mean, while at the top it was 31°°3 or 3°'2 above the mean. This great excess of temperature was about the same in all parts of Scotland, and was occasioned by an extraordinary predominance of south-westerly wind, which exceeded any observed in November during the past forty years. The sunshine was markedly deficient, and hence temperature at the top was relatively lower than at Fort William. The following show the deviations of the monthly results from their respective means :— TasLeE IT. Top ot Fort Ben Neyis William fo} fe) January ‘ : : : F j : . —2°0 O7 February. ss 40 5 ean! Pi teed| May. + 65 a O “2 LO 4 1 0 June. — 65 DEMIR TS .I| , 35 3 betta July . —11:0 Zit Owr visi 5 50 Bipie a0 August — 75 Wiihend h : 115 de Or 0 September + 40 3. 0 2 a 85 Dy Oe 20 October + 35 SS ae aD Ei yplohenl iota) November. + 65 led ul ol | pee 2180) 5 0 0 December . 4 — 30 PS eo 43 | “7 30 4 0 1 Totals . 5 +29'0 3L 5 24 || +10~> x 1040 zs a (Re: in 300 days | in 300 days According to Table IT. if every day behaved like a ‘quiet’ day there would be an annual increase of 35’ in westerly declination, instead of the actually existing decrease of 7’, and an increase of 1265x10~° C.G.S. units in H.F., instead of the actually observed 20 x 10~°. Taking the figures as they stand, the evidence in favour of a general tendency to a non-cyclic variation in the direction of increasing westerly declination during ‘quiet’ days is perhaps not conclusive. Of the indivi- dual months’ records twenty-four show a decrease, and the balance the other way might be pure chance. The figures relating to the horizontal force, however, unless ascribable to error, prove conclusively that during the five years in question the force increased at a wholly abnormal rate on ‘ quiet’ days. It is difficult to imagine any cause of error working so uniformly throughout the year. Supposing uncompensated temperature effect to exist, for instance, the phenomenon should tend one way during one season, the opposite during another. The interval between successive r 2 212 REPORT—1895. ‘quiet’ days varied arbitrarily, so that the positions of the two midnights of a ‘quiet’ day on the photographic sheets were constantly being inter- changed. It may also be added that the phenomenon is not peculiar to Kew, but may be seen in the published Greenwich and Falmouth results for the same epoch. § 5. The phenomena seem not unlikely to be only another phase of phenomena observed many years ago by General Sabine and Dr. Lloyd. The former from a careful study of what he termed ‘disturbances’ con- cluded that the aggregates of easterly and westerly declination disturbances at Kew during 1858-62 nearly balanced, ‘there being in some years a slight preponderance of westerly, and in other years of easterly deflection ;’! at the same time he found ? ‘a slight preponderance of easterly values on the average of the four years (1858-61).’ As regards the horizontal force he deduced * from 5,932 disturbed observations at Kew during 1858-64 that ‘the ratio of the value of the disturbances decreasing the (horizontal) force to those which increased it was nearly as 3:23 to 1.’ In agreement with this last result Dr. Lloyd found‘ from an examination of the 335 (?) most disturbed days at Dublin during the ten years 1841-50 that ‘the mean effect of disturbances is to diminish that (the horizontal) force.’ The significance of these results, when taken along with the tendency suggested by Table II. to a slight abnormal increase of westerly declina- tion on quiet days, and the clear evidence of an abnormal increase of horizontal force on these days, need not be dwelt on. Although the vertical force lies outside our present inquiry, it may not be amiss to mention that evidence of a connection of the kind foreshadowed above is also supplied by it. The results, in fact, from the last five years at Kew show a distinct abnormal decrease of vertical force on ‘ quiet’ days, while General Sabine observed a very decided preponderance of disturbances to be associated with increasing vertical force. Whether the species of opposition in the phenomena exhibited by the horizontal and vertical forces is to be associated with the fact that at pre- sent the former element is increasing the latter decreasing seems an inter- esting speculation, but it lies outside our present inquiry. Method of Treating the Non-cyclic Diurnal Element. § 6. General Sabine got out tables according to which ‘ disturbances ’ at Kew were by no means uniformly distributed over the twenty-four hours ; further he found that disturbances associated with easterly deflections had different hours for maxima and minima from disturbances associated with westerly deflections, and a like difference appeared between disturb- ances associated with increasing and those associated with decreasing horizontal force. If this be so, and if the non-cyclic phenomena observed on ‘quiet’ days be in any way complementary to the disturbed phenomena, then there is certainly ground for suspecting that the abnormal increase, say, of H.F. observed in the mean ‘ quiet’ day of a certain month is not uniformly distributed over the twenty-four hours. While fully recognising the uncertainty of the hypothesis of uniform distribution of the non-cyclic element, I have unhesitatingly adopted it provisionally. What General * Phil. Trans. for 1863, p. 282. ? Proc. Roy. Soe., vol. xi. p. 590. # Phil. Trans. for 1871, p. 310. * 1 Treatise on Magnetism, p. 211. DIURNAL INEQUALITY. ination, Horizontal Force. Declination 05 becca / ee Se ee L Sed bride a KANN Lee eH ‘ 6 4 3! 2 1 ar -2' £9! -¥g’ & Abscisse time in hours from midnight. Illustrating the Report on Comparison and Reduction of Magnetic Observations. ON COMPARISON AND REDUCTION OF MAGNETIC OBSERVATIONS. 213 Sabine termed ‘disturbed’ observations included only some 10 per cent. of the entire number; so that, even supposing the years to which his results and the present results applied had been the same, it would hardly have been possible to utilise his results in framing a better hypothesis. Some light might have been thrown on the subject by taking measure- ments at each hour of every day immediately preceding or succeeding a ‘quiet’ day, and examining the magnitude of the non-cyclic element for each combination of twenty-four consecutive hours. The fact that this would have entailed some 12,000 additional measurements put it out of court so far as the present inquiry was concerned. I have thus decided to regard the variation of an element throughout the typical ‘ quiet’ day of a given month as composed of first a non-cyclic part, consisting in a uniform increase or decrease throughout the twenty- four hours, second a truly cyclic part spoken of as the diurnal inequality. Thus suppose an increment 24 I to occur during the twenty-four hours ; then the diurnal inequality is what remains of the observed hourly departures from the mean for the day after the correction (12—#)I has been applied, ¢ denoting the number of hours elapsed since midnight. This correction raises the values throughout one half of the day and depresses them throughout the other. It of course leaves unchanged the mean value {3((0]+[24])+[1]+ .. . +[23]} /24, and after its application [o]=[241. The size of the correction applied to each month’s results for declination and horizontal force is obvious from Table II., so that the uncorrected values can easily be reproduced from the corrected ones recorded pre- sently. Tables of Diurnal Inequality and their Discussion. § 7. The following tables, III. and IV., give the diurnal inequality in the several months and quarters of the year, as well as for winter, summer, and the entire year. The values given under each month are the arithmetic means from the data of the five years. The numerically largest maxima and minima are distinguished by heavy type. The hours are numbered continuously from midnight, so that 13 and higher numbers refer to the afternoon. The results for hour 24, being the same as for hour 0, are omitted. A graphical illustration of the diurnal inequality for the year; for winter, for summer, for midwinter (December and January), and for midsummer (June and July), is afforded in Plate V. by the curves 1, 2, 3, 4, 5 for the declination, and by the curves 6, 7, 8, 9, 10 for the horizontal force. The curves will facilitate the comprehension of the principal phenomena. A comparison of the declination table and curves with the corresponding results at Kew during the epoch 1858-62, as given by General Sabine in the ‘Phil. Trans.’ for 1863, will be found of interest. § 8. In both tables the results proceed one figure further than the actual measurements, the extra figure arising in the process of taking the means. No smoothing process has been applied to the original data, and no correction other than the elimination of the non-cyclic element. That the results are trustworthy, as measurements of magnetic variation, to 214 REPORT—1895. Taste III.—Diurnal Inequality of Declination (aft ! Hour. “sf a 0 1 2 3 4 5 6 7 8 9 { ‘ / / i 1] < ‘ / / ‘ January .« . | —1°36 | —1:17 | —0:86 | —0°68 | —0°69 | —O:80 | —0:84 | —0°97 | —1°34 | —148 February . . | —1:40 | —1°45 | —1°31 | —1°15 | —1°00 | —1:14 | —1-15 | —1°43 | —1°85 | —1°86 March 5 . | —1:°07 | —0:92 | —0°89 | —1°08 | —1°39 | —1°32 | —1:77 | —2°63 | —3°74 | —3*43 April. i . | —0°71 | —0-74 | —0°92 | —1:07 | —1°36 | —1'73 | —2'51 | —3-84 | —4°91 | —4°48 May. = . | —0°83 | —0°86 | —1-09 | —1°34 | —2°07 | —3°38 | —4:29 | —5°08 | —4°75 | —3°26 June. ° . | —0°45 | —0°76 | —0:90 | —1:27 | —2°10 | —3°57 | —484 | —5:29 | —5°12 | —3°79 July . O . | —0°66 | —0-'80 | —1°10 | —1:24 | —1:99 | —3°53 | —4:-49 | —4:73 | —4-77 | —3°65 August . . | —0°94 | —1°10 | —1°35 | —1°80 | —2°17 | —3°03 | —4:20 | —5°01 | —4:70 | —3°06 September . | —138 | —1:°43 | —1°58 | —1:°96 | —2°39 —2°56 —316 —3'85 | —396 | —2°40 October . . | —1°48 | —1:13 | —1:03 | —0:96 | —1:10 | —1:07 | —1°50 | —2°04 | —3°05 | —3:23 November . . | —1:15 | —0:82 | —0:79 | —0:74 | —0-75 | —0°95 | —114 | —1:33 | —1°84 | —1:93 December . . | —115 | —0°77 | —0-46 | —0°38 | —0°39 | —0°47 | —0°74 | —0°86 | —1:03 | —1°17 First Quarter . | —1:28 | —118 | —1:02 | —0°97 | —1:03 | —1:09 | —1:26 | —1°67 —2:31 | —2:26 Second Quarter | —0°66 | —0°78 | —0°97 | —1°23 | —1°84 | —2°89 —3°88 | —4:74 | —4°93 | —3°84 Third Quarter . | —0°99 | —111 | —1°34 | —1°67 | —2°18 | —3°04 | —3°95 —453 | —4'48 —3°04 Fourth Quarter | —1'26 | —0:90 | —6:76 | —0°69 | —0'75 | —0°83 | —1:12 | —141 | —L:97 | —2:11 Winter . . | —1:27 | —1:04 | —0°89 | —0°83 | —O:89 | —0°96 | —1°19 | —1°54 | —2°14 | —2:18 Summer . . | —O°83 | —0°95 | —1:16 | —1°45 | —2°01 | —2°97 —3°92 | —4°63 | —470 | —3-44 Year. ‘ . | —1:05 | —1-00 | —1:02 | —1'14 | —1°45 | —1:°96 | —2°55 | —3:09 | -—3°42 | —2°81 10 t —0'33 —0°68 —158 —2:18 —0°31 —1°26 —136 —0-01 +0°49 —162 —0°82 —0:14 —0°86 —1:25 —0:29 — 0°86 —0°86 —077 —0°82 Hour. ‘ < 0 al 2 3 4 5 6 7 8 9 10 | January . .|+7/4+7/)] +7 +19 +43 +60 +58 | + 64 | + 32 | — 26 | — 76 February . - | +37 | +23 | +424 +18 +24 +44 +47 | + 63 | + 35 | — 43 | —110 March. +57 | +50 | 445 +42 +41 +64 +71 | + 38 | — 31 | —126 | —195 April. - -| +79 | +74 +64 +65 +62 +66 +63 + 34 — 56 —163 —256 May . . «| +79 | +75 +51 +49 +31 +19 —24 — 90 —178 —244 —260 June. * - | +65 | +49 +44 +42 +37 +18 —40 —113 —183 —240 —259 July . sy . | +62 | +59 +38 4-46 +31 +16 —33 — 90 —155 —228 —272 August . - | +75 | +81 +69 +69 +62 +34 —10 — 94 —188 —268 —294 September - | +88) +82] +71 +55 +54 +40 +1 | — 62 | —156 | —231 | —265 October . - | +67 | +57 +59 +77 +68 +82 +82 + 50 — 20 —130 —218 November. . | +36 | +36 +38 +42 +63 +79 +85 + 65 + 15 — 75 —154 December. .| —16|—8]| —7 +3 +26 +42 +53 | +57 | + 36 | — 4 | — 68 First Quarter . | +34 | +26 +25 +26 +36 +56 +59 + 55 + 12 — 65 —127 Second Quarter. | +74 | +66 +53 +52 +43 +34 — 1 — 56 —139 | —216 —258 Third Quarter .| +75 | +74 +59 +457 +49 +30 —14 — 82 —166 —242 —277 Fourth Quarter | +29 | +28 +30 +40 +53 +68 +74 + 57 + 10 — 70 —145 Winter . -| +3 +27 +28 +33 +44 +62 +66 | + 56 +11 | — 67 | —136 Summer . SETS) +70 +56 +54 +46 +32 —7 | — 69 | —153 | —229 | —268 Year. . . | +53 | +49 +42 +44 +45 +47 +29 — 6 — 71 —148 —202 units in the last place cannot, I think, be maintained for a moment ; but the omission of the last figure would render it impossible to give an adequate idea of the extreme smallness of the variation during many hours of the night. The most conspicuous feature of the declination diurnal inequality, especially in summer, is the rapid change from a maximum easterly declination, occurring from 7 to 9 a.m., to a maximum westerly declination about 1 p.m. In winter, as is apparent on inspection of the winter and midwinter curves, there is a subsidiary westerly movement during the ON COMPARISON AND REDUCTION OF MAGNETIC OBSERVATIONS. 215 nination of non-cyclic element), + being to west of mean. 14 15 16 17 18 19 20 21 22 23 / / 4351 | +3°02 | +1'98 | 41°37 | +0'82 | +0'36 | —o'03 | —o'54 | —1'02 | —1'23 | —1"49 +3:76 | +3°78 | +3:02 | +1°53 | +0°83 | +062 | +026 | —0:36 | —0°77 | —1:07 | —1:36 +599 | +5°50 | +3°91 | +1:70 | +035 | —0'10 | —0-48 | —0°55 | —0°88 | —1°01 | —0-96 +635 | +5°87 | +412 | +2:39 | +1:00 | 40°14 | —0-25 | —0:22 | —013 | —0:25 | —0-44 +685 | +616 | +449 | +242 | 40°89 | —0-:08 | —0-43 | —060 | —0-43 | —0:38 | —0:47 +595 | +579 | +466 | +3:25 | 41°84 | +0°93 | +034 | +027 | +018 | +0°3L | —0-28 "12 | +652 | +5°37 | +3:23 | +133 | +023 | —0:09 | —0:09 | +0°02 | —0°02 | —0-20 +723 | +628 | +449 | +214 | +030 | —0°45 | —0°30 | —0°33 | —0°31 | —0°60 | —O-71 +3" +651 | +540 | +336 | +165 | +050 | —0:00 | —017 | —0:50 | —0°56 | —O'61 | —1-02 +140 | +413 | +528 | 44°84 | +359 | 41:93 | +112 | 40°45 | —0°03 | —O'44 | —1°14 | —1°41 | —1°51 -143 | +318 | +3°95 | +326 | +221 | +140 | +062 | +0:25 | —0°04 | —0°59 | —1:0) | —1:23 | —1:18 106 | +1°99 | +2°65 | +244 | 41°90 | +115 | +051 | +0°30 | —0°12 | —0°65 | —111l | —1:28 | —1°32 41°29 | +3:45 +442 | +410 | +2°97 | +153 | +067 | +0:29 | —0:08 | —0-48 | —0°89 | —1:10 | —1:25 4195 | +499 | +639 | +5°94 | +442 | +269 | +124 | +033 | —O11 | —0718 | —0°13 | —O11 | —0-40 +5°54 | +662 | +6°07 | +441 | +2°34 | +071 | —0:07 | —0°19 | —O0°31 | —0-28 | —O-41 | —0°64 4130 | +310 | +396 | +351 | +257 | +149 | +075 | +034 | —0:06 | —0°56 | —1-:08 | —1:31 | —1°34 v 130 | +3°27 | +4:19 | +3°81 | +2°77 | +151 | +071 | +0°31 | —0°07 | —0°52 | —0-°99 | —1:20 | —1-29 2:39 | 45:27 |} +650 | +600 | +442 | +251 | +0°98 | +013 | —0°15 | —0'24 | —0:20 | —0:26 | —0'52 1°84 | +427 |} 45°35; +490 | +359 | +201 | +084 | +022 | —O-11 | —0°38 | —0°60 | —073 | —0°91 12 13 | 14 15 16 17 18 19 20 21 | 22 23 ll | — 94 — 46 —22 |) —18 | — 12 + 3 + 29 + 35 + 23 + 15 + 3 + 5 —126 — 84 —41 | -15}—- 5 + 9 + 32 + 38 + 52 + 50 ee 37 + 33 —163 — 92 —31 | +20 | + 23 + 14 + 43 + 76 + 73 + 62 + 59 + 68 —223 —144 —68/} +1] + 38 + 70 + 83 +106 +105 + 97 + 92 + 88 —155 — 87 —21L | +33 | + 83 +127 +144 +152 +128 +120 +102 + 92 —150 | — 82 | —7]} +63] + 86 | +119 | +161 | +170 | +146 {| +125 | +102 | + 78 —188 —113 —18 | +68 | +105 +138 +157 +164 +145 +127 +104 + 85 —152 — 64 +2| +42] + 77 + 95 +129 +139 +129 +129 + 87 + 97 —105 — 21 +24) +18] + 11 + 35 + 70 + 99 +105 +108 + 92 +103 —186 | —106 | —52} —22} —13 | + 31 | + 59 | + 67 | + 67 | + 75 | + 67 | + 73 —146 —112 —60 | —22|}— 5 + 29 + 43 + 57 + 47 + 37 + 34 + 28 — 78 — 44 -21);-—7/+ 4 + 22 + 26 + 33 + 20 + 4 -—- il + 5 —128 | — 74 | —31}—4]+ 2 | + 9 | 4+ 35 | + 50 | + 49 | + 42 | + 33 | + 35 —176 —104 —32 | +32 | + 69 +105 +129 +143 +126 +114 + 99 + 86 —148 — 66 + 3) +43 | + 64 + 89 +119 +134 +126 +121 + 94 + 95° —137 — 87 —44) -17 | -— 4 + 28 + 43 + 52 + 45 + 39 + 34 + 35 —lo2 | — 81 —38 | —1l1/}—- 1 + 18 + 39 + 51 + 47 + 40 + 33 + 35 —162 | — 85 | —i5 | +37 | + 67 | + 97 | +124 | +138 | +126 | +118 | + 97 | + 90 } | | —147 | — 83 —26 | +13 | + 33 + 58 + 81 + 95 + 87 | +79 | + 65 + 63 night, entailing two unmistakable maxima of westerly declination and two of easterly in the twenty-four hours. This accords generaily with conclu- sions I., 1I., III. for Dublin on pp. 175, 176 of Dr. Lloyd’s ‘ Treatise.’ His further conclusion, IV., that ‘in summer the westerly movement during the night disappears,’ is in more doubtful accord with the present results, The variation during the night in summer is so very slow that a definite conclusion would require the warrant of more data than are here avail- able ; but according to Table III. there is, to say the least of it, the suspicion of a slight secondary westerly movement in most of the summer 216 REPORT—1895. months a few hours before midnight. To attain certainty in such a case . one would require a very large number of observations for each month in the year. When the results of several months are grouped together, secondary maxima, unless occurring very nearly at the same hour in each month, are apt to disappear. The smoothness of the mean curve for a year or a half-year is doubtless in part due to the elimination of observa- tional errors by means of the large number of observations included ; but in some cases at least it arises from what may be termed the swicide of secondary phenomena. Mutual extermination of very delicate phenomena may even arise when so short a period as a month is dealt with as a unit. If, instead of the inequality of declination, the inequality of the disturbing force perpendicular to the magnetic meridian be desired, then the results of Table III. may be converted into C.G.S. measure of force at the rate of 1’ to 53 x 10-° C.G.S. units. In the horizontal force inequality the most conspicuous feature is the minimum occurring from 10 to 11 a.m. In every month there is an unmistakable maximum—especially conspicuous in summer—about 4 P.M. In winter there is distinct evidence of a second minimum and maximum during the night and early morning, the maximum being usually the largest in the twenty-four hours. In summer the evidence in favour of a second maximum and minimum appears somewhat uncertain. The results are in general accord with the conclusions for Dublin on p. 184 of Dr. Lloyd’s ‘ Treatise.’ Harmonic Analysis of Diurnal Inequality. § 9. The diurnal inequality of one of the elements, say the declina- tion, D, can be analysed into a series such as Qrt st Te Qrnt - Inrnt 2D=a, cos = 40, fie + a cbs bei ee ie oer eae ag. | or 9 9 ¢D=c, cos = (t—r,)+ . +c, cos or (t—t,)+..... (16) Here ¢ is the time in hours measured from the first midnight ; » is an integer ; @,, 6,, C,, T, are constants, connected by the equations C.=Va,2+6,2 - : . ; : - (2) = 74 tan-1 (6 3 fe an—!(b,/a,) . ; , ‘ . (3) In what follows it is arranged that c, shall always be positive, and so 7, is the time of the first maximum, in an algebraic sense, subsequent to midnight. Supposing hourly values of the element known, one has twenty-three constants at one’s disposal ; but here I have contented myself with deter- mining the coefficients of the terms whose periods are respectively 24, 12, 8, and 6 hours. The subsequent terms appear in reality to be very small, and any numerical results one might reach in connection with them would be of doubtful accuracy. The following table, V., gives the values of the a, 6, ¢ coefficients ow .. “ON COMPARISON AND REDUCTION OF MAGNETIC OBSERVATIONS, 217 for the mean diurnal inequalities of winter, summer, and the whole year. : : The a, 6 coefficients for the ‘ year’ are the arithmetic means of those for ‘ winter’ and ‘summer’; but as a check on the accuracy of the work they were calculated independently. Variation to the west in the declination is regarded as positive. TABLE VY. a, b, CF | a, b, Cy as b, CH a, b, €, | / / 1 / Winter . |=1'55|—1'17| 1°94 | +0'72|+1/21| 1°41 |—0-62 |—0'49| 0-79 |4+0°30| +0:25. | o-39 8D {Summer — 197 —2:59| 3-96 |42:05|41-64] 263 |—0-99|—0-61| 1:16 |+0-16| 40-095 | O-19 Year —1°76 |—1°88| 2°58 |41°39|}41:42| 1:99 |—0°81|—0°55| 0°98 |+0:23| +017 0:29 Winter.!+ 68 | — 3 68 —52} +11 53 +13 | —22 26 +2 +15 15 torent | Suumer }4+125 | —89 | 153 —52 |) +50} 73 | —3]| —27 27 +7 +10 13 Year .|+ 96 | —46 | 107 —52 | +31 61 +5) —25 | 25 +4 +13 13 The only change required in Table V. if time were measured from noon, instead of as throughout the present paper from midnight, would be the alteration of the signs of the entries referring to a,, 6), a3, and b3. It should be explained that the calculations on which Table V. is based proceeded in every case to at least one decimal place, usually two, beyond that shown. The table shows that in the case both of the declination and the horizontal force, the terms whose period is twenty-four hours are very much greater in summer than in winter, and the same phenomenon shows itself in the terms in the declination whose period is twelve hours. On the other hand the terms in the declination whose period is six hours appear relatively much larger in winter than in summer. It would hardly be prudent to attach too much weight to this last conclusion, in view of the extreme smallness of the quantities involved ; but it is in accordance with Tables XV. and XVI. of the ‘Greenwich Magnetical and Meteoro- logical Observations’ for the two years 1890 and 1891. A comparison of the other features common to these two Greenwich tables and to Table V. will be found of interest. The Greenwich tables, it should be noticed, are not confined to ‘quiet’ days, and in treating the horizontal force they take as unit the (1/100000) of this force at Greenwich, or, say, 10-8 x 182 C.G.S. unit. § 10. The number of degrees in the angles 27n7,,/24 is easily obtained from Table V. by means of the formula (3). Instead of giving these angles explicitly I have preferred to give the times 7,, answering to the earliest maxima in the day of the Westerly declination and the hori- zontal force. These times are included in Table VI., along with the earliest times in the day when the several terms of the types appearing in (1,) vanish and have their minima. The interval between successive maxima or successive minima is double that between successive zero- points, and equals the periodic time, é.¢., is 24, 12, 8, or 6 hours, as the case may be. With one important exception—that of the harmonic term in the declination whose period is twenty-four hours—the first maximum of every term appears earlier in the day in summer than in winter. The difference between the corresponding times in winter and summer is 218 REPORT—1895. TABLE VI. Peridot term Winter Summer Year i | hone Max. | Zero | Min. | Max. Zero | Min. | Max. | Zero | Min h.m.| h.m.| h.m.| bhem.| be. m.|h.m.| b.m.| b.em.} b. m. 94 ee 1429) 829| 229/)1531|) 931] 331/15 8| 9 8] 3 8 ee H.F. 23 52| 552)1152/21 38) 338] 9388]2218) 418]1018 12 Decln Tesi 4.58 | eueosi| LT | 41 |) Tie oie aol eo H.F 5 36| 236|1136] 432] 132)1032) 459) 159/1059 i 8 Decln .| 451) 251) O51| 442) 242) 042) 446) 246] 0 46 H.F 641| 041) 241] 552) 352) 152} 616) 016); 216 6 Decln 040] 210} 340) 030] 2 0} 3830| 0387) 2 7] 337 H.F 124) 254] 424) 055] 225} 355] 111) 241] 411 conspicuously greater in the case of the horizontal force than in that of the declination. There is, it will be noticed, a close coincidence between the time, 9 hr. 38 min., of the minimum in summer of the horizontal force term whose period is twenty-four hours and the time, 9 hr. 31 min., of the first zero in summer of the corresponding declination term. ‘The fact, however, that no such coincidence presents itself between the correspond- ing times in winter would suggest the phenomenon was in part at least accidental. It can hardly be connected with the fact—shown conspicu- ously by Tables III. and IV., or still better by curves 1 to 10—that the time of the principal minimum of the total horizontal force inequality, from 10 to 11 A.m., is nearly coincident with a time at which the total declination inequality vanishes. Papers dealing with a theoretical con- nection of the sort, by Professor A. Schuster and Mr. C. Chambers, will be found in the ‘ Phil. Mag, for April and May 1886, and in ‘ Proce. Lit. and Phil. Soe.,’ Manchester, Session 1886-87, pp. 23-46. Resultant of Cyclic Horizontal Disturbing Forces producing the Diurnal Inequality. § 11. The importance attaching to variations in declination suggests most naturally the resolution of the horizontal disturbing force, to which the diurnal inequalities just considered are due, into components ¢X and eY respectively in and perpendicular to the magnetic meridian. The preceding results show that, H denoting as usual the total horizontal force, €X/H and éY/H are at most small quantities of the order 1/500. Thus to a very close approximation we have WonDs: a ee Cee where 6H and éD are the inequalities of horizontal force and declina- tion, while H is the mean value of the horizontal force for the time under consideration. ON COMPARISON AND REDUCTION OF MAGNETIC OBSERVATIONS. 219 For the mean of the years 1890-94 we have H='18211 C.G.8. units ; whence cY =530x 107-7 x 6D 5 e . e ry Py ‘ » (5) where ¢D is supposed to be given in minutes of arc. Resolution in and perpendicular to the magnetic meridian is some- what inconvenient when the general features of terrestrial magnetism are being considered, owing to the complicated relationships between the magnetic meridians at different stations. Even in dealing with the phenomena extending over a long interval of time at a single station, the reference to a set of axes whose position is continually altering has its disadvantages. When, however, the components of a force along two rectangular axes are known, the components along any other pair in the same plane are easily deduced when the inclination of the old to the new axes is given. It will thus suffice to state that for the epoch 1890-94 the mean magnetic meridian at Kew lay at 17° 36'-2 to the west of the astronomical meridian. § 12. Instead of giving explicitly the components in and perpendicular to the astronomical meridian I propose to consider the magnitude and direction of the resultant horizontal disturbing force itself. Denoting its intensity by », its inclination to the east of magnetic north by J, we have to a sufficiently close degree of approximation p=v (¢X)2-+(0Y)?=cH sec . . . : (6) YStan"! (—dY /¢X)= fant) ( 20% H/2H) ° “ : (7) Remembering that the inclination of p to the astronomical north is —(17° 36’:2), it would be found a simple matter to deduce the com- ponents of the disturbing force along and perpendicular to the astro- nomical meridian from the calculated values of » and w. The following table, VII., gives the values of » and y for the mean of December and i anuary, or cand inter, the mean of June and July, or midsummer, and the mean for the year at each hour. The greatest and least values of p in each case are in heavy type. In comparing Tables IV. and VII. the reader will require to notice that the former refers to 10° cH, the latter to 10%». Table VII. was got out from arithmetical means proceeding to two places beyond those retained in Table IV., and an extra figure was retained in p», so that the arith- metical accuracy of any resolution of p into orthogonal coordinates should be as trustworthy as its previous resolution into éX and oY, 2.¢., into 6H and HcD. The angle 360° is to be added to the values of / under the hour 23 for ‘midsummer,’ and for hours subsequent to 18 in ‘midwinter’ and ‘ year,’ - it is desired to make out the true increase of y relative toa previous our. In the case of the yearly mean the vector p has a continuously pro- gressive rotation from east to west through south, like the sun as seen from the earth. This is the general character of the rotation at any season ; but at midwinter there i is an unmistakable retrograde motion in the early morning for several hours, and at midsummer there i is at least @ suspicion of a retrograde motion from 8 to 10 p.m. From 10 a.m. to 1895. REPORT 220 ‘06E'T Suteq ava 94} 10J UvoUt ay} ‘sOMUINSprIUt ut gz¢E‘T 04 IOJUIMPIOL UI ZZ) WOL} SOtIVA SINOY FZ OY} 4Hoysnorq} d,OT Jo on[va uvatt OUT, ~ | BT cLE | LF 008 | LFolS | woSl | Go | TS olSE| ST oBSE| SolBS | oFL] | FI oFNZ| OF ofSZ | 19 o98@| ° : au : * WeaX I6L LG) 0&8 068 6T6 | 1Z8 0gL 9IT'T | tO06LT | ST9'S | TS6'% | GEY'S | ° *dx .0T SF o8 | OF 898 | TE oLGE | 16 BSE | Lh oLLE| JF oGFE | ZS o9BE| 1B 0668 | SF o€86| TS oL9G| 1B ofSS | 0G oF SB) * ; “| JOUIUINSPIP, $38 FE0'L 6S4'L cop] EL9'L 8I9‘T 98¢'T F9G'L 9EL‘S T1a'e | eves | 968's | ° ‘dx or E 19.098 | 122088 | 06008 | 91099 | 8% 09 | 12 oLZE| ZF 068 | ,FE 099Z | 199 0B9B | FE o19B | KE oF G2 | EI o88S, * : a JaqUIAMp UY 96L 999 @Lg €8¢ €he= In. Fee 9L¢ 019 SEO'T GOF'T b69'T PEPT | ° ‘dx .0 ete ale : - ¢ * &Z GS 1Z 0Z Gime de Si 1T 91 co FI ra ZI Inox] U1 090 | FY oL9T| TE oF ST | 0G ol TT | ,9T 066 | SF oLL | 88099 | 8069 | oF | 6T 069 | LT oLF | s16 09F | * : he : - eax $13 90'S | ZOT'G OFG6'T 1f9'T | #88'T IFT 168 9FL fefefe) LIL LOL : ‘dX OT 16 o661 | /€6 G91 TG oBEL | 67 oGGL | ES OTL} :8% o86 | SF ofS | OF oGL | 189099 | ET 06S | FS oLG | EF ofS | : *h } JOUIMINSpIP GE'S SEL‘S 8g0'¢ 6IL'S SESS | «(00S'S L88'T géI'T L6L €L9 619 ToL : “dx ,01 : (SF 090G | BF o69T| 8 oGOL | GT o19 | 9E o8E | FI o9E | OT ofE | ZF GE | 0069 | 1G006 | SF 006 | FF of6 | * : ah J9)ULM PIN Stl‘ FOL SIL GIL GL) 669 TI9 StF 008 Fe =| «BIS 899 i x9 X01 se II or 6 8 L 9 ¢ P ¢ z I 0 Inoy ‘TIA YIdV bb oo eek a) Plate Vi f SS Abscisse time in hours from midnight. Tllustrating the Report on Comparison and Reduction of Magnetic Observations. ON COMPARISON AND REDUCTION OF MAGNETIC OBSERVATIONS. 221 2 p.m., the time of the day when the diurnal inequality is most in evidence, the value of i) seems to vary very little with the season. Curves whose radius vector is p, and vectorial angle J, illustrate the variations of diurnal inequality in a conspicuous way. Numerous curves of this kind, illustrating the results obtained at Greenwich for the years 1841-57, were given by Sir G. B. Airy in the ‘Phil. Trans.’ for 1863, ‘and a smaller number, referring apparently to the years 1873-75, were also iven by Airy in the ‘Phil. Trans.’ for 1885. Several applications of these curves to Dublin results appear in Dr. Lloyd’s ‘ Treatise.’ Following ‘these examples I have drawn curves 11, 12, and 13, Plate VI., based on he results in Table VIT., for midwinter, midsummer, and the whole year. The hours are stated beside the points on the curves to which they refer. The prominent loop on the midwinter curve should be noticed. The existence of a loop on the mean winter curve and its absence in the mean _ summer curve for Dublin are referred to by Lloyd (loc. cit., p. 187). The tendency to loops in winter months is conspicuous in Airy’s Greenwich “curves. Relative Intensity of the Forces to which the Diurnal Inequality 1s due throughout the year. § 13. Without knowing the true nature of the disturbing force or forces to which the diurnal inequality is due, it is difficult to suggest any wholly satisfactory measure of intensity. Assuming the inequality to be aha composite phenomenon, the counteraction of opposing forces may produce _ the same effect at one hour as the absence of forces at another. All the _ phenomena seem, however, to point to greatly increased activity of dis- _ turbing forces in summer. The data given above as to the mean values of p throughout the day at midwinter and midsummer make the former _ mean only -374 of the latter. Evidence in the same direction is supplied by the following table VIII., which gives for each month, each quarter and half-year, and for the whole year, the sum of the hourly departures from the mean for the day, irrespective of sign, along with the range, or algebrai- cal difference between the extremes. To show how comparatively little _ depends on how the non-cyclic element is dealt with, the table, in addition to the results obtained after the non-cyclic element has been eliminated, gives likewise the range deduced from the uncorrected data for each month. The fractions, which the table records, refer exclusively to the | corrected data. _ The range and the sum of the inequalities in both declination and horizontal force show a distinct minimum in December. In the declina- _ tion both the range and the sum of the inequalities present an absolute “maximum in August, with apparently a second, only slightly smaller maximum, in May. The variation, however, especially of the range, is so small from April to August that it would hardly be safe to conclude this was the normal phenomenon in a year of ‘quiet’ days. In the horizontal _ force there would appear to be a single maximum, whether for range or sum of inequalities, in July ; but the difference between the results and those for May, June, and August is extremely small. $14. These conclusions are only partly in accord with those got out by Dr. Balfour Stewart! for a long series of years, 1858-73, at Kew, and by Mr. W. Ellis,? for a still longer series of years, 1841-77, at Greenwich. 1 Proc, Roy. Soc., vol. xxvi. 1877, p. 103. 2 Phil. Trans. for 1880, p. 544. 222 REPORT—1895. Taste VIII. Declination | Horizontal Force in C.G.S. measure Sum of Sum of In- 's Inequalities Range equalities x 10° Range x10 Month | Hw oso mn i co H 5 ss | 3 tee eS s3 | 2 | o |S so mee io] 3S co eo lee 3 2 Siar =e 2s E g 28 a8 23 E 3 2s Sa BA ° 4 24 Sa | $8 3S o BA ae |) ee |) 2 Be a ee ee eee see to Be) 8 |S | 8s | A EE Sr) ks e A er lea 4 FI January . - | 29/52 0°635 522 4°99 07559 823 0434 172 180 | 0°567 February . - | 35/95 0-773 5/72 564 0°632 1,132 0:598 214 205 0642 March. e 4758 1:024 9°78 9°73 1-089 1,689 0°892 290 282 0°883 April . . | 5145 1107 11°30 | 11/26 1261 2,371 1-252 386 381 1192 May e e | 59/32 1:276 12/00 | 11/93 1:337 2,571 1°358 428 | 411 1:288 June . e - | 59/26 1:275 11/18 | 11/25 1:259 2,610 1:378 434 429 1342 July . 4 «| 57°46 1:236 11-18 | 1129 1264 2,686 1-419 444 | 436 1:366 August . | 60°14 1:294 12/16 12/23 1:370 2,632 1390 450 | 433 1:355 September . | 55/04 1184 1050 | 10/47 1172 2,113 1116 386 372 1166 October 2 | 45°48 0-978 8°54 8'°52 0'954 1,964 1:037 332 317 0-991 November . | 32/59 0-701 5/92 5”°88 0-658 1,468 0°75 234 245 0°765 December . 2 | 24°03 0517 4/02 3/97 0°445 664 0°351 140 142 0 445 Means: 1st Quarter. - | 37°68 —_ _ 6"79 — 1,215 —_— _— 222 -~ 7G Lae ea .- | 56°68 _ — 1148 — 2,517 —- — 407 —_— 8rd yg fw | STDS == = 11:33 = 2,477 = ry hei = athe ee hk. SAS — = eg | — 1,365 = — |) 234 a Winter A . | 35/86 _— _ 6°45 — 1,290 - — 228 — Summer . 57/11 _— _— 1141 _ 2,497 — — 410 — Year e 46'49 _ _ 8°93 _— 1,893 oa - 319 —_ The tables by Dr. Stewart and Mr. Ellis both give April as the month in which occurs the largest maximum in the declination range. Dr. Stewart’s table gives slightly smaller, and nearly equal, maxima in June and August. In Mr. Ellis’s table the mean range for August is decidedly higher than the mean for June, which latter, however, is a shade higher than the mean for May and decidedly higher than the mean for July. Again, the difference between the maximum and minimum ranges of declination in Table VIII. is much greater than in either of the other tables referred to. Thus, by Table VIII., the corrected range varies from 12'-23 to 3/-97, while in the general mean of the monthly results from the thirty-seven years included in Mr. Ellis’s table the extremes are 11'-96 and 5'*78, and in Dr. Stewart’s table the ratio of the maximum to the minimum monthly range is only 2: 1. Dr. Stewart’s table is confined to declination, but Mr. Ellis gives results for the range of horizontal force as well. The general means he gives for the four months, April to July, are very nearly equal ; the greatest value, that for April, being about 2 per cent. only in excess of the least of the four, that for May. The difference between the greatest and least of the mean monthly ranges of horizontal force in Mr. Ellis’s table is again much less than the corresponding difference in Table VIIL., the minimum, appearing in December, bearing to the April maximum the ratio 42 : 100. The mest conspicuous difference between Table VIII. and the results of Dr. Stewart and Mr. Ellis is that it shows no trace of a maximum of activity in April, and indicates markedly increased activity in August. It would, however, be precipitate to assume that the time of maximum ON COMPARISON AND REDUCTION OF MAGNETIC OBSERVATIONS. 223 activity falls later in the year now than in the epochs dealt with by Dr. Stewart and Mr. Ellis. The different character of the materials employed in the several cases must be borne in mind. Dr. Stewart took into account all observations except the comparatively small percentage falling under General Sabine’s definition of disturbed, and Mr. Ellis took all but days of considerable magnetic disturbance ; thus the material ‘dealt with by both possessed presumably much eveater heterogeneousness than that dealt with in Table VIII. Again, ' the mode in which the results were treated was different. Dr. Stewart, it is true, apparently took the means from groups of four successive years, but Mr. Ellis took ‘the mean of the ranges deduced from each single year’s records. The taking a group of years probably depresses the mean range most in those ‘months in which the progress of the diurnal inequality is least regular. Harmonic Analysis of Monthly Ranges. § 15. I have analysed into harmonic terms the quantities measuring mean range for month _ the departures from unity of the fractions — for both mean range for year declination and H.F. Putting for ee ; SI LN ad nema: Se tem alter sonics perils) where ¢ is time in months from the middle of January, I find for the declination mean range for month T mean range for year +:08 sin 27%+-01 cos 3a—°04 sin3z%+°01 cos 47+:-00 sin 4x +04 cos 5a—:03 sin 5a+'03 cos 6a . : : Z (9) for the Horizontal Force mean range for month eal mean range for year +:03 sin 2x+:00 cos 3a—:‘00 sin 3x+°03 cos ri ‘03 sin 4a +:03 cos 5a+°01 sin 5a2+:01 cos 6x . 5 tO) In both cases the terms whose period is the full year are , greatly pre- dominant. There appears also in both cases an appreciable semi-annual variation ; but the terms with shorter periods are very small, and little weight can be attached to their numerical measure. = —40 cos «+14 sin x—°'1] cos 2a = —°43 cos x+:'08 sin x—:07 cos 2x Annual Variation. $16. The variation of a magnetic element throughout the year, like variation throughout a quiet day, i is most simply regarded as composed f two parts, a uniform drift or secular var vation, and a eyclic portion, which may be called the annual inequality. This is a somewhat arbi- trary separation. The increase of the horizontal force, for instance, from year to year, got out from the observations of most observatories, is far from uniform ; and if this be a true phenomenon the hypothesis that the secular drift is uniform throughout the whole of one year can hardly claim a physical basis. It is, however, at any rate a conyenient mathe- matical fiction whose adoption can do no harm when its true character is explicitly recognised. 294 REPORT—1895. The following data are extracted from the annual Kew ‘Reports :— TasLe LX. | Year | 1890 | 1891 1892 1893 | 1894 | Mean Declination . .| 17° 50'6 V7 To S6l7 WELZ DEGRA aT Oe a ri Fc Ie, 18173 "18193 ‘18202 “18238 “18251 The mean values thence deduced for the secular variation are a decrease annually of 6'9 in declination, and an increase annually of 10-6 x 195 C.G.S. units in horizontal force. It will be assumed that these secular variations proceed uniformly throughout the mean year, got by combining the five years 1890-94. To eliminate the secular variation one adds to the observed values +0':575t¢ in the case of the declination, and —10-® x 1°625¢ in the case of the horizontal force, ¢ being the time elapsed in months from the middle of the mean year. Subtracting the mean value for the year from the monthly means thus corrected, one obtains the annual inequality. § 17. To make the true position of affairs clear, a brief explanation is necessary of how the magnetic curves are standardised at Kew. Of late years the practice has been to determine the value of the zero line for each month’s curves by reference solely to the absolute observations of that month. The same instruments are used for each observation of an element, and every observation is independent of the others, except that the constant usually called P in the formula for the horizontal foree— i.e., the coefficient of the secondary term in the expression for the deflect- ing foree—is determined from a whole year’s observations. One of the most probable and subtle causes of error one has to provide against in getting out an annual variation of any physical phenomenon is a possible secular or annual variation in the measuring instruments. This is especially the case with apparatus sensitive to changes of temper- ature. Now it is unquestionably true that the horizontal force magneto- graph is affected by changes of temperature, and though the underground chamber it is worked in at Kew has a very small diurnal variation of temperature, it has a considerable annual fluctuation. Thus, however carefully temperature corrections might be determined and applied, the suspicion of an ‘annual inequality’ being far other than it seemed might not unreasonably be entertained, if the ultimate reference were to the mag- netograph curves, either unstandardised, or standardised by reference to the mean of a year’s absolute observations. It is partly to provide against this that each month’s curves are referred to that one month’s absolute observations. These observations are taken about once a week and scattered over tthe month, so that any secular or annual variation in the magnetographs themselves must be very nearly eliminated. As regards the absolute instruments there is, so to speak, no higher court of appeal. There is no obvious ground for suspicion. The hori- zontal force magnet has a temperature correction to apply, but this is only to allow for the difference in its temperatures at the times of the vibra- tion and deflection experiments in the same observation. This difference in temperature is very small and very irregular, and even if the tempera- ON COMPARISON AND REDUCTION OF MAGNETIC OBSERVATIONS. 225 ture correction were considerably in error the consequence could hardly be a regular annual variation, but merely an increased probable error in each individual observation. _ A second source of uncertainty is that the probable error in an abso- lute observation and its comparison with the corresponding curve value is somewhat large compared to the annual inequality it is desired to “measure. The number of observations, some twenty, on which the mean for each month of the mean year depends may seem sufficiently large to render ‘any mere observational error insignificant. It must be remembered, however, that on a considerable number of the days of absolute observa- tion there proves to have been a good deal of magnetic movement. Some- times the disturbance has been such as to render it necessary to discard the observation entirely, and in other cases there is appreciable uncer- tainty as to what is the true length of the curve ordinate to be taken as answering to the observed absolute value. This will be readily under- stood of the horizontal force, an absolute observation of which lasts usually over an hour. The result of the absolute observation is a species of mean value, to which some portions of the time occupied by the obser- _yation contribute more than others. The determinations of the declination are less subject to uncertainties of this sort ; but on the other hand the ‘range of its annual inequality seems to bear a much smaller ratio to the secular variation than in the case of the horizontal force. ~ §18. The natural outcome of the second class of errors would obviously be a series of fictitious discontinuities in passing from one month to another of a year. Asa matter of fact there did appear an unnatural amount of fluctuation in the figures obtained for the annual inequalities from the mean values answering to the middle of the months. To get rid of this I have deduced the annual inequalities in the following table, X., from a series of values, each of which is the arithmetic mean of the actually observed means of two consecutive months. These arithmetic eans are attributed to the first day of the second month of the two. The first two columns of the table give the departures from the mean for the year of the actually observed means for the individual months ; so that anyone who prefers to deduce the annual inequalities from these an easily do so. I ought to explain that in calculating Table X. some slight differences ‘were introduced from the declination results for 1890 published in the Kew ‘Report.’ The declination curves for that year had been standardised by treating as a whole the absolute observations and corresponding curve easurements throughout the year, instead of taking each month sepa- rately. I have thought it best to remove this peculiarity of treatment, referring for the purpose to the absolute observations for the year, of which, of course, the record remained. The numerically greatest and least values in the annual inequality columns are in heavy type. The ranges given by Table X. for the annual inequalities, viz., 1/"22 for the declination and 10-°x129 for the horizontal force, would be - imereased to 1/52 and 10-§x141 respectively if the monthly means, for _ the middle of each month, were taken and corrected for secular variation. § 19. The results obtained for the annual inequalities are much smoother and more consistent than might have been expected ; but taking _ the smallness of the apparent ranges, and the fact that the - 1895. Q f 226 REPORT—1895. Taste X.—Dzifferences from Mean for Year commencing on January 1. Monthly means, for middle Results answering to first of month, uncorrected for d y of month after secular Month secular variation correction applied Dec'ination H.F. x 106 Declination HF.x10 i i January . - - . + 3°32 —117 + 0°48 —13 February . ; : +315 — 73 + 0°36 -—14 March. : : : +168 — 86 + O11 —15 April : 3 : : + 0°83 — 22 —O0-47 — 5 May. : : : 5 +0°31 + 48 —0°58 +46 June : ‘ F : — 0°43 + 66 —0°63 +74 July. : : : é —0°70 + 27 —057 +47 August . . ; ; —0-70 + 55 —0'12 +24 September : : é —0'88 — 26 + 0°36 —18 October . : : - —2-01 | + 13 + 0°28 —55 November - : : — 2°22 + 25 +0:18 — 46 D: ember ; ‘ ‘ — 2°35 + 90 | +0759 —24 measurement of the curves proceeds only to the nearest 0'-1 in the case of the declination, and to the nearest 1 x10~-° in the case of the horizontal force, I do not think too much confidence should be placed upon details. The results for the annual inequality of declination show unques- tionably a good general agreement with those deduced by General Sabine ! from the undisturbed readings of the Kew magnetograph during the five years 1858-62. General Sabine’s own paper treated each week of the mean year separately ; but a summary giving mean results for the several months appears on p. 76 of Walker’s ‘ Terrestrial and Cosmical Magnetism,’ where there is an interesting discussion of the question. According to the summary, General Sabine’s results made the annual inequality negative from May to August inclusive, and positive throughout the rest of the year, the range amounting to almost exactly 2’. From General Sabine’s own table one would deduce a principal maximum of westerly declination in the latter half of October, with a second and only slightly smaller maximum early in December, whilst the easterly movement was conspicuously largest about the middle of July. The times at which General Sabine observed the inequality to change sign are substantially in accord with Table X.; and if the range he observed was decidedly larger, this might be associated with the fact that the secular variation during the epoch he dealt with was greater than during 1890-94. In case this agreement should be referred to identity of apparatus, it may be as well to mention that the declination magnet employed for the absolute observations at Kew of late years came into use only in the beginning of 1890. A comparison of the declination results with those at other British stations is unfortunately by no means so reassuring. For Dublin the annual inequality got out from the mean of the years 1842-50 by Dr. Lloyd ? makes the westerly declination below the mean from December to June, and gives a range exceeding 4’, There are also conspicuous differences between Table X. and the Greenwich results obtained by Sir ' Phil. Trans. for 1863, p. 292. 2 Treatise on Magnetism, p. 162. ON COMPARISON AND REDUCTION OF MAGNETIC OBSERVATIONS. 227 G. B. Airy | from the two periods 1841-47 and 1848-57. The results for these two periods, however, it must be said, differ widely between them- selves, the range deduced from the first being nearly thrice that deduced _ from the second period. Thinking more light desirable in the face of these discordances, I got out the annual inequality for the mean of the five years 1887—91 from the results published annually in Table XI. of the Greenwich ‘ Magnetical and Meteorological Observations.’ Proceeding as in Table X., 2.e. taking means for the first of each month, and applying the secular correction 6':4 deduced from the Greenwich tables, I obtain an inequality whose resemblances to that shown in Table X. are not more conspicuous than the divergences. The largest easterly declination appears in April-May, the largest westerly declination in September-October, and the range, 0'°6, is even smaller than in Table X. Against these comparative agreements must, however, be set the fact that the first three months of the year show an easterly departure from the mean. The divergences in the results obtained for the annual inequality of declination do not, of course, necessarily imply that any of them are erro- neous. The phenomena at any one station might not unnaturally present considerable variations—at least in range—from year to year; and it is conceivable that local influences may be more effective in this than in other phenomena. It has also to be borne in mind that the data em- _ ployed at the several stations were selected on different principles. Still, 1 am doubtful whether any more definite conclusion should be drawn _ than that the annual inequality of declination near London is at present a very small quantity. § 20. The annual inequality of horizontal force shown in Table X. is, comparatively speaking, large and unmistakable ; its range is a large fraction of the secular variation. In this instance there is a very fair agreement with the results given on pp. 166, 167 of Lloyd’s ‘ Treatise ’ for Dublin on the mean of the years 1841-50, the most conspicuous differ- ence being that the Dublin range was some 50 per cent. in excess of that given by Table X. The only previous determinations, so far as I know, of the annual variation of the horizontal force at Kew are those of General Sabine? and ‘Dr. Balfour Stewart,’ for the epochs 1857-62 and 1863-68 respectively. The former found the horizontal force, corrected for secular change, to be on an average about ‘00012 C.G.S. units higher in summer than in winter, while the latter found no difference. This divergence might be attributed to the epochs considered being different ; but I feel consider- able doubt as to the data employed having being adequate. They appear to have been in both cases simply the results of the absolute observations, _ ungorrected by reference either to the magnetograph curves or to the diurnal variation. In conclusion, I have much pleasure in acknowledging my mdebted- ness to Mr. T. W. Baker, chief assistant, and Mr. R.S. Whipple, librarian at Kew Observatory, for explanations as to the methods of standardising the magnetic curves at Kew, and for other valuable information and assistance. Phil. Trans. for 1863, p. 314. 2 Phil. Trans. for 1863, pp. 298, 299. 3 Proce. Roy. Soc., vol. xviii. 1870, pp. 238, 239. Q 2 228 REPORT—1895. The Teaching of Science in Elementary Schools.—Report of the Com- mittee, consisting of Dr. J. H. GLADSTONE (Chairman), Professor H. E. Armstrone (Secretary), Professor W. R. Dunstan, Mr. GEORGE GLADSTONE, Sir Joan Lussock, Sir Partie Maanus, Sir H. E. Roscoxr, and Professor S. P. THompson. At the meeting of the British Association for the Advancement of Science, held at Sheffield in 1879, a Committee was appointed with reference to the examination in the scientific specific subjects of the Code in Elementary Schools. Mr. Mundella was the first Chairman, but he was unable to continue such, as he shortly afterwards became Vice-President of the Committee of Council on Education. The Committee was re- appointed next year, with the object of reporting on the manner in which rudimentary science should be taught, as well as examined. In 1881 the Committee was again reappointed to watch and report on the working of the proposed Revised New Code, and of other legislation affecting the teaching of science in Elementary Schools. In November of that year the Committee agreed upon certain recommendations, which were adopted by the Council of the Association and transmitted to the Education Department. The Government adopted some of these recommendations in whole or in part. Since that date the Committee has been continued annually, and has regularly reported on the progress of the teaching of natural science in Elementary Schools. It has also used its influence in respect of the great question of technical instruction, the formation of school museums, Evening Continuation Schools, and other matters that have come before the Legislature. When the Royal Commission on Elementary Education was sitting, the Council of the British Association adopted a Resolution of this Committee, authorising one of its members to give evidence before the Commission, which was done accordingly. The question of the method of teaching science to classes of young children has also been considered recently, and formed part of the Report of the Committee. As the object of this Committee more directly affects those sections which deal with natural science, it was reappvinted last year under the auspices of Section B. With regard to the progress of scientific instruction in Elementary Schools, the number of departments of schools in which the following class subjects were examined by Her Majesty’s Inspector during the eight years 1882 to 1890, when English was obligatory, were as follows :— | | | Class Subjects.—Departments | 1882-83 | | 1883-84 1884-85, 1885-86 | 1886-87 | 1887-88 1888-89 1800 1889--90 Enelislt, ¢) ey wavy wales ices] 028,868 5 ,080 | 19,431 | 19,608 | 19,917 "2 20,041 ou 20,153 | 20,304 Geography . . « .| 12,828 | 12,775 12,336 | 12,055 | 12,035 | 12,058 | 12,171 | 12,367 Elementary Science i 48 5L 45 43 | 39 | 36 | 36 32 The numbers during the last four years, when managers and teachers have had full liberty of choice, have been as follows :— ON THE TEACHING OF SCIENCE IN ELEMENTARY SCHOOLS, 229 Class Subjects Departments 1890-91 1891-92 | 1892-93 | 1893-94 Sereeh. ss | | 19,825 18175 | 17,894 | 17,082 | Geography . : a) 12,806 13,485 | 14,256 15,250 Elementary Science =| 173 788 LOT3 _ | 1,215 It will be noticed that during the former period, while the study of English Grammar increased with the natural increase of schools, the study of scientific subjects positively decreased ; but since that time, while Grammar has steadily declined, Geography and Elementary Science have increased. The number of departments in ‘schools for older scholars’ for the year 1893-94 was 22,779, of which 111 did not take any class subject, leaving 22,668 as the number of departments with which the foregoing table has to deal. But it must be borne in mind that History is taken in 2,972, and Needlework (for girls) in 7,675 departments, making, with the other three subjects in the table, 44,144 in all. This shows an average of nearly two class subjects to each department. As, however, there were no less than 5,975 departments in which only one class subject was taken, it is evident that the plan of teaching one subject in the lower division of a school and another subject in the upper division, thus counting twice over - in the statistical table, is largely adopted. This is further borne out by the fact that, while only two class subjects are allowed to be taken by any individual scholar, there are 4,388 departments in which three, and 197 in which four or five, of these class subjects are taught. That Elementary Science is taught in 1,215 departments must, therefore, be accepted with the reservation that, in many cases perhaps, it is only a portion of the school that gets the benefit of this instruction. The number of scholars examined in the scientific specific subjects — during the eight years 1882-90 has been as follows :— 1 ; Specific Subjects——Children | 1882-83 1883-84 1884-85 | 1885-86 | 1886-87 | 1887-88 | 1888-89 | 1889-90 Algebra . . . «| 26,547 | 24,787 | 25,347 | 25,393 | 25,103 | 26,448 | 27,465 | 30,035 -} Buclidand Mensuration . - 1,942 2,010 | 1,269 1,247 995 1,006 928 977 Mechanics,A. . «. «| 2,042| 3,174) 3,527] 4844] 6,315 | 6,961 | 9,524 | 11,453 is IBY 7 - - —_— 206 239 128 33 331 127 209 Animal Physiology. é . | 22,759 | 22,857 | 20,869 | 18,523 | 17,338 | 16,940 | 15,893 | 15,842 Botany . . . - «| 3,280| 2604] 2,415| 1,992] 1,589] 1,598} 1,944] 1,830 Principles of Agriculture .| 1,357 | 1,859 | 1,481 | 1,351] 1,137] 1,151] 1,199 | 1,228 Chemistry . . .| 1,183} 1,047] 1,095] 1,158] 1,488 | 1,808] 1,531 | 2,007 Sound, Light,and Heat. . 630 | 1,253] 1,231] 1,334] 1,158 978 | 1,076 | 1,183 | Magnetism and Electricity . 3,643 3,244 2,864 2,951 2,250 1,977 1,669 2,293 Domestic Economy. . .| 19,582) 21,458 | 19,437 | 19,556 | 20,716 | 20,787 | 22,064 | 23,094 Total . . . «| 82,965 | 84,499 | 79,774 | 78,477 | 78,122 | 79,985 | 83,420 | 90,151 Number of scholars in Stan- ). . a j dards V., VI., and VII. } 286,355 | 325,205 | 352,860 | 393,289 | 432,097 | 472,770 | 490,590 495,164 The numbers in the last column of table on p. 230 reveal a general advance ; but the most marked proportional increase is to be found in the number of scholars taking Chemistry and Magnetism and Electricity. The num- bers during the last four years are :— 230 REPORT—1895. Specific Subjects.—Children 1890-91 1891-92 1892-93 1893-94 Algebra. ; i : 31,349 28,542 |. 31,487 33,612 Euclid c ; 2 : 870 927 1,279 1,399 Mensuration . ; : 1,489 2,802 3,762 4.018 Mechanics . ; : : 15,559 18,000 20,023 | 21,532 Animal Physiology . : 15,050 13,622 14,060 To;20 Botany : : : 2,115 1,845 1,968 2,052 Principles of Agriculture . 1,231 1,085 909 1,231 Chemistry . F : P 1,847 1,935 2,387 3,043 Sound, Light, and Heat _. | 1,085 1,163 1,168 1,175 Magnetism and Electricity | 2,554 2,338 2,181 3,040 Domestic Economy . 7 27,475 26,447 29,210 | 32,922 | Total ; 3 - | 100,624 | 98,706 108,434 119/295 With regard to the teaching of Mechanics, which has attained a development, within the last few years, far greater in proportion than any other of the scientific subjects, it is very satisfactory to note that of the 21,532 scholars above enumerated, no less than 3,407 had reached the third stage of the syllabus, while 7,296 were examined in the second stage. Considering how rapidly the elder children drop out of school after they have passed the legal Standard of exemption, these figures augur well for the value placed upon the instruction in this subject, which has become almost a speciality of the London, Liverpool, Birmingham, and some of the other large School Boards, and which is almost entirely carried on by special instructors on the peripatetic system. The sudden rise of more than 50 per cent. in the last two years in the number of students in Chemistry does not admit of any such proportion being found in the laver stages ; but considerably over one-fourth of the whole were examined in the second and third stages. The recognition of the importance of experimental teaching is leading to the establishment. of well-appointed laboratories by some of the School Boards, such as those of Hove and Handsworth, which can be made to serve also for the teaching of this science in the Evening Continuation Schools. Estimating the number of scholars in Standards V., VI., and VII. at 570,000, the percentage of the number examined in these specific subjects as compared with the number of children qualified to take them is 20°9 ; but it should be remembered that many of the children take more than one subject for examination. The following table gives the percentage for each year since 1882 :— In 1882-83 eet: moeat OO 8. Cee »» 1883-84 » 1884-85 » 1885-86 eas eee ee ,, 1886-87 sends -chnabik diiniewt Sa », 1887-88 ARE Ones VEER: », 1888-89 ne lee tierra ites = <, , 1889-90 Bl nt cee ee 1890-91 Bt 7 40 oligt fo were 1891-92 , 1892-93 Lmeiternd bay ee Sy ee Oo per cent. DWH DOH HH Hebb bp SSOSHABPOWSS ONWIW KOSH ORDS ON THE TEACHING OF SCIENCE IN ELEMENTARY SCHOOLS. 231 The returns of the Education Department given above refer to the whole of England and Wales, and are for the school years ending with August 31. The statistics of the London School Board are brought up to the year ending with Lady Day, 1895. They also illustrate the great ~ advance that has been made in the teaching of Elementary Science as a class subject, and they give the number of children as well as the number _ of departments. Years Departments Children 1890-91 11 2,293 1891-92 113 26,674 1892-93 156 40,208 1893-94 183 49,367 1894-95 208 52,982 The total number of departments for ‘older scholars’ under the London School Board at the last-named date was 820, so that in just over one- fourth of the whole the teaching of Elementary Science has been introduced into the curriculum. The number of schools under the London School Board that are now working in accordance with the syllabus of Elementary Physics and Chemistry given in the day and evening schools Codes is steadily increasing, and the work as it becomes better understood by the teachers is naturally being better taught. About thirty schools under the Board will be engaged in this work after the summer vacation, all of which are supplied _ with the necessary apparatus. The old system of peripatetic experimental lectures by a demonstrator has been practically superseded in the divisions of Tower Hamlets and Hackney. The scholars are not now dependent on a brief inspection of apparatus once a fortnight or three weeks, but can use it at any opportunity given by the master of the class. The enormous size of the classes—often 120—is, however, a serious obstacle to the success of a scheme designed to cultivate the reasoning faculties rather than the acquirement of knowledge of scientific facts and _ theories ; in this sense it cannot be said that the scheme has yet had a fair trial. Very much depends on the individual ability and enthusiasm of the teacher, much more so than under the old system ; so that in most eases the work is not satisfactorily carried on if the teacher himself has not been through the whole course practically before he begins to teach ‘it ; in fact, the Science and Art system has left its mark so deeply engraved _ on many teachers’ minds that it takes some time to instil more modern notions into them. The alteration in the system of inspection, though beneficial in all subjects of school curriculum, will have an especially useful effect in the teaching of science. Under the new conditions the work must be done more thoroughly, and the subjects of the syllabus evenly distributed over the year, thus preventing the rush and cram of revision in the period im- mediately preceding the annual examination. The training of teachers being, as above stated, the all-important factor in securing the success of this scheme, more facilities are required for bringing together the older teachers to form normal practical classes. Tn considering the establishment of such classes it must be remembered that teachers, already out of their training course, give their time volun- 232 REPORT—1 895. tarily after a hard day’s work in school ; the conditions under which such classes are held must therefore be made as easy as possible if they are to be successful, and the sympathy and enthusiasm of the teacher are to be aroused. During the last year some fifty or sixty teachers under the London Board went through practical courses at the demonstrator’s laboratory in Whitechapel, where the accommodation will soon be quite insufficient to meet the requirements of the district. Full and complete notes and sug- gestions were issued to all teachers attending the courses, which were much appreciated. The development of the work is largely due to the establishment of this system of normal classes. In the meantime the question of science teaching in girls’ schools has not been left unattacked. Two schools have now adopted a course of domestic science in lieu of domestic economy. A syllabus has been devised to deal as far as possible with the nature of the processes and the materials employed in the household. A short course of measurement and weighing has been introduced with the double object of familiarising the scholars with the decimal system and making them acquainted with the instruments they will have to use in accurate experimental work. The general effects of heat on matter, and their application to the work of the laundry and kitchen, are then studied ; the modes of cooking and some of the simpler changes involved, chemistry of air and water, combustion, fuel, soap, hardness of water, and finally a few lessons are given on the mechanics of the household, such as the structure of taps, locks, gas fit- tings, hot-water boilers, flushing tanks, &e. Classes have been held for the mistresses in this subject at the laboratory, and it is generally considered by those who have been through the course to combine mental training with the acquirement of valuable information, Except that the physiological part of the Domestic Economy is not touched, most of the important work in that syllabus which can be dealt with by scientific methods has been considered. During the coming winter classes will be held at Berner-street Laboratory, London, E., in all stages of Elementary Natural Philosophy and Domestic Science syllabuses, but it is only too clear that this course involves commencing at the wrong end. Before any great headway is made, work of this nature must be introduced into the teachers’ course of training, and to this end it is essential that teaching on the lines of the new syllabuses must be started in the Pupil Teachers’ and Training Colleges. Jn many parts of the country School Boards and County Councils are beginning to follow in the wake of the London Board ; the subject is becoming a popular one in Evening Continuation Schools, and is often adopted as part of the elementary course for organised science schools. The great obstacles to good science teaching at the present time in Elementary Schools are— . Large classes. 2. Multitude of subjects. 3. Insufficiency of the training course for teachers in science sub- 4 bt jects. . Effects of the old Science and Art system, which is clearly far too formal, and pays far too little attention to ordinary requirements. The return of the work of the Evening Continuation Schools under — = ON THE TEACHING OF SCIENCE IN ELEMENTARY SCHOOLS. 233 the Code of 1893 furnishes interesting data as to the instruction in scientific subjects in these schools. Your Committee drew attention in their Report for 1893 to the development which was taking place at that time in this direction ; but pointed out that the Government return of that year did not furnish precise information on the point. A new table has been introduced this year, which gives the information desired. In the following table your Committee give the number of ‘units for payment’ of the grant by the Education Department for the several scientific sub- jects taken throughout England and Wales during the session 1893-94, to which is appended a similar return for the schools under the London School Board, extracted from the Board’s Annual Report upon their Evening Continuation Schools. It may be necessary to explain that the ‘unit’ means a complete twelve hours of instruction received by each scholar, fractions of twelve hours not counting. Units for payment Sta SUIS | England and London School | Wales Board re FT ORE RO nee 595 10 Algebra . ’ - ; : : : : 3,940 316 Mensuration . \ 4 ‘ i : : 14,521 279 Elementary Physiography : 3 ; 2,554 37 Elementary Physics and Chemistry . 4 6,500 79 Science of Common Things . s : 5 6,223 231 Chemistry . : : : : : Ht 3,484 212 Mechanics. ‘ : : : ‘ : 841 230 Sound, Light, and Heat ; 4 ; F 500 = Magnetism and Electricity , a 2,359 | 662 Human Physiology . | 5,695 91 Botany . : 2 - | 336 5 Agriculture =| 3,579 — Horticulture . | 438 — Navigation ? | 42 = The total number of units is (for England and Wales) 51,607, whereas the number of scholars is 41,960, indicating that about one-fourth of them must have received at least twenty-four hours of instruction. It is evident that London is far behind the country in general in the teaching of these science subjects in their Evening Continuation Schools, excepting in the matter of Mechanics and Magnetism and Electricity. The stronghold of this instruction is in Manchester and the other manufacturing districts. It is especially interesting to note that 3,696 students took up Chemis- try, and that a much larger number took the comparatively new subjects of Elementary Physics and Chemistry, and the Science of Common Things. Your Committee has already on a former occasion (1893) expressed approval of the course on Elementary Physics and Chemistry in the Evening School Code, which is a practical course intended to be carried out experimentally by the scholars themselves, and deals, not with defini- tions or descriptions, but with actual facts. The course on the Science of Common Things is ‘a brief survey of the physical properties of bodies, serving to determine their uses and relative value.’ It may be looked upon as an introduction to physical and biological science in general, and to its application to ordinary and domestic life. In their last Report your Committee referred to the difficulties inter- 284: REPORT—1895. posed by the regulations of the Code in making visits for the purposes of education to such places as Kew Gardens, the South Kensington Museum, &c., although the Science and Art Department have recognised the educa- tional value of such attendances; and stated that Mr. Acland had favour- ably received a deputation on the subject, and promised increased facilities. This promise has been fulfilled ; and the Code of this year provides that the time spent during school-hours in visiting museums, art galleries, and other institutions of educational value may count towards the time re- quired for an attendance at school. Her Majesty’s Inspectors are more- over instructed to encourage these visits wherever such institutions exist. It is stipulated that the teacher in charge should not have, as a rule, more than fifteen scholars with him, and that no visits should be paid unless some person competent to give information of a kind interesting to young children is present. All these regulations appear wise and proper, so that the real object of visits to these institutions may be attained ; and the limitation of them to twenty in the course of the school year is not unreasonable, as, with all the other matters that demand attention, more time certainly could not well be spared. The only other alteration of importance in the Code that concerns your Committee is the new stipulation that object lessons must be given in all schools to the children in Standards I., II., and IIT., and an excellent circu- lar to Her Majesty’s Inspectors has recently been issued, pointing out the true aim and nature of object teaching. It commences by drawing attention to the two kinds of instruction which are often confused : (1) observation of the object itself, and (2) giving information about the object. It dwells upon the importance of the distinction, adding, ‘Object teaching leads the scholar to acquire knowledge by observation and experiment ; and no instruction is properly so called unless an object is presented to the learner, so that the addition to his knowledge may be made through the senses.’ It enforces the selection of subjects which can appeal to the hands and eyes of the scholars, stating that ‘however well the lesson may be illustrated by diagrams, pictures, models, or lantern slides, if the chil- dren have no opportunity of handling or watching the actual object which is being dealt with, the teacher will be giving an information lesson rather than an object lesson.’. . . ‘It is Elementary Science only in so far as it aids the child to observe some of the facts of nature upon which natural science is founded; but as it deals with such topics without formal arrangement, it differs widely from the systematic study of a particular science.’ The circular contains many suggestions on the choice of objects ; the avoidance of what is purely technical; the making of drawings or models both by teacher and children; the relation of the parts of the object to the whole; and the leading the children to describe accurately what they have seen. Several complete schemes are given for guidance in the appendix to the circular. The Parliamentary Committee which has been considering the question of decimal weights and measures, under the chairmanship of one of your Committee, Sir Henry E. Roscoe, has just reported in favour of the per- missive use of the metric system for all purposes for the next two years, after which that system should become obligatory. It recommends that it should be taught in all public schools as a necessary and integral part of Arithmetic. The Elementary School Code has, for some years past, contained a note to the effect that ‘the scholars in Standards V., VI., and VII. should know the principles of the metric system,’ but it has not ON THE TEACHING OF SCIENCE IN ELEMENTARY SCHOOLS. 235 received much attention while so much time had to be spent upon the tables of weights and measures in ordinary use. When these cease to be legal, not only will the teaching of Arithmetic be rendered more rational, but a large amount of time will be set free which can be applied to the promotion of science teaching. Looking back over the years that have elapsed since the passing of the first Elementary Education Act, it is evident that the constant tendency has been to add to the curriculum of the schools ; and some of the most recently recommended additions to the time-table include manual instruc- tion and physical exercises. The difficulty of finding time for these has led to the suggestion that the generally recognised hours of schooling might be extended in the case of the elder scholars. This course would involve some practical inconveniences ; and in view of the fact that the children pass their Standards now at an earlier and more immature age than they did some years ago, it is a question worth consideration whether the time has not arrived when the recognised school age should be raised from thirteen to fourteen, and the work of the Standards made to spread over this extended period. Such an arrangement would have the manifest advantage of affording a broader and more practical education, without over-pressure to either the teachers or the taught. Quantitative Analysis by means of Electrolysis.—Second Report of the Committee, consisting of Professor J. EMERSON REYNOLDS (Chair- man), Dr. C. A. Koun (Secretary), Professor P, FRANKLAND, Pro- fessor F. Clowes, Dr. Huan Marswatyi, Mr. A. E. FLETCHER, Mr. D. H. Nace, Mr. T. Turner, and Mr. J. B. CoLEMAn. A PRELIMINARY report was furnished by the Committee last year in which the contemplated plan of work was outlined. The bibliography of the subject has been completed and is ap- pended. The experimental work has been carefully organised, and the results on the determination of bismuth and of tin are nearly complete. Other work is in progress, but the Committee prefer to hold over these results until next year in order that they may be added to and may include methods of separation of some of the metals. Considerable attention has been given to the choice and arrangement _ of the special apparatus required. A detailed description of the arrange- ments adopted will be given in the next report. As the bibliography is completed, the Committee propose to devote their attention during the coming year exclusively to experimental inquiries. Bibliography on Methods of Quantitative Analysis by means of Electrolysis. The bibliography has been compiled from the following journals, and is complete up to the end of 1894 :— 236 REPORT—1895. Journal | pees a Abbreviation 1 | Journal of the Chemical Society . | 1847-1894 J. Chem. Soc. 2 | Journal of the Society of Chemical | 1882-1894) J. Soc. Chem. Ind. Industry 3 | Chemical News . : j - | 1860-1894 Chem. News. 4 American Chemical Journal - - | 1878-1894} Amer. Chem. J. 5 | Journal of Analytical and Applied | 1887-1894| J. Analyt. & App. Chem. Chemistry | 6 | Journal of the American Chemical | 1879-1894| J. Amer. Chem. Soc. Society | 7 | Zeitschrift fiir analytische Chemie . | 1862-1894) Zeits. anal. Chem. 8 | Berichte der deutschen chemischen | 1868-1894 Ber. Gesellschaft 9 | Zeitschrift fiir anorganische Chemie . | 1892-1894] Zeits. anorg. Chem. 10 | Zeitschrift fiir physikalische Chemie | 1887-1894} Zeits. phys. Chem. 11 | Zeitschrift fir Electrochemie . : 1894 Zeits. Electrochem. (Organ der deutschen electroche- | mischen Gesellschaft) References to papers of importance published in journals other than the above are also included, viz, :— Journal Abbreviation American Chemist. F : . | Amer. Chem. Annales de Chimie et Physique ‘ ‘ . | Annales Chim. et Phys. Berg- u. hiittenminnische Zeitung. ; 8 : . | Berg- u, hiitten. Zeit. Bulletin de la Société Chimique . : 5 ; , Bull. Soc. Chim. Chemiker-Zeitung . : d : < : ; . | Chem.-Zeit. Comptes Rendus . j 3 ; : ‘ : . | Compt. Rend. Dingler’s Polytechnisches Journal . 3 ‘ . . | Dingler Polyt. J. Jahresbericht der Chemie . : ; . : . | Jahresber. Chem. Journal of the Franklin Institute . : , : . | J. Franklin Inst. Journal fiir praktische Chemie : : : - . | J. prakt. Chem. Monatshefte fiir Chemie : ; : : : . | Monatsh. Chem. Pharmaceutische Central-Halle . : : : . | Pharm. Central-Halle. Repertorium der analytischen Chemie . : ‘ . | Rep. anal. Chem. Zeitschrift fiir angewandte Chemie | Zeits. angew. Chem. Books of Reference. 1. ‘Quantitative Analyse durch Electrolyse.’ A. Classen. 3rd edit., 1892. Published by J. Springer, Berlin. Translation, by W. H. Herrick, of 2nd edition, 1887, ‘Quantitative Chemical Analysis by Electrolysis.’ Published by I. Wiley, New York. 2. ‘Electro-chemical Analysis.’ Edgar F. Smith. 1890. Published by P. Blakiston, Philadelphia. Arrangement of Bibliography. The bibliography is divided into the following sections :— I. General conditions for electrolytic analysis. IT. Special apparatus employed. III. Quantitative methods, for the determination of metals by means of electrolysis. IV. Quantitative methods, for the separation of metals by means of electrolysis. V. Special applications of electrolysis in quantitative analysis. VI. 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SEER Gyo ppt . can, ‘TUeUyIO A "may ‘Masue ‘sie |* * * —* q ‘Bropny “y ‘rulZ ‘MOY ‘[VUr ‘s}loz | -zeoseyY pure “Hy ‘tporyg ‘mY ‘[TeuV ‘sjlez | * : : ‘9 ‘moxon'y - ‘yrz-meyg|* ‘ ° ‘Wy ‘seruasoey , L ‘9323 *puy “WAaYyO 009 "fF | -pcoA, pus “y ‘O ‘uqoy . . * leg e . . . ‘YY ‘massulO : * ‘leg | ‘Y ‘otapry pure “y ‘aassefp y < a (20 (a C ° "vy ‘dasseipQ a ‘ vag | ‘VJ ‘sly pue “y ‘uasse[o ‘mayo ‘Teuv ‘s}10Z | . . ° . ‘v ‘puvig euinor 1oyjny ‘(sappy U2) poyeys OSIMIOY}O BOY ydaoxo ‘qons sv payisodap st [vJoUl eYT— I] ALON *‘popnypout ore 0} pediejar [@}0U OY} JO ATES B JO UOTqNIOS [vIyNAU v 0} pappe sooWLASqNsS JO soURIsqns aq} ,‘o4A4JoI]Da[q JO UoryIsodmog , Surpesy oy} Jepuy-—"] ALON QUANTITATIVE ANALYSIS BY MEANS OF ELECTROLYSIS. ‘OUT, “FG “UNTINTTAT, “0% ‘NUT, “OT “SINDION “GT ‘unIpay “8 “UUNITPED “F “TINIUBIY) “EZ “IOATIN ‘61 ‘MUNIPEled “GT ‘asouvsUv “TT ‘PION “2 ‘TIQNUISIg “¢ “UL, ‘GS ‘UINTUITAS “ST ‘OXON “FT ‘pee ‘OL ‘raddog ‘9 ‘OIUBSIV ‘GZ “TUNTTVYL “1G “manIpoyy “LT ‘umagepqAToN “eT ‘UOIyT *6 “W1BQ90 “Gg ‘AuowTyUY *T — USAID Ol S[RIIUT SUTMOT[OJ 9Y}.10J spoyjout ayy, - ‘seshjoupapy fo sunau hg spojayy fo woywurwopag 24} Hof spoyjayy aarjgozyunn?) TIT 4 1895. REPORT 240 Ne } ra eee a EES ae St MOR |e pees ae eIOe ‘mpbypun so “rag ‘10g * "THAYD ‘[RUB ‘s}187, * “WAY ‘TeUR *sy1a7 ‘-Iog : “pp wWoYyO ‘eMy ‘moyD ‘ddy x -44,euy “¢ * “MAYO “AMISUB *SqIO7 * “WIOYQ ‘TBUR “Sq197 | * -maeyO ‘shud *s}107 : “qsuy Ulyue YL ) "TOYO ‘[BUL ‘s}1907 “ “pur "mayy ‘00g “¢ * -“MmeYyO ‘S1ouv *sy107 * "tay *[vue *s}187 * “MAYyOOIOETT *S}197, 9} {Toaqoayy JO woiztsodur0g | aded | awnyog | vax | *pa7yeSpoo MM puey ‘p‘uyoy . . . . "M ‘sqquy ‘vy ‘uassv[p “VW ‘stoy puv “y ‘uasse[p . . ‘ . ‘Vv ‘pueig . . . "TI “‘gyonyog . “A a ‘QyIUIg “aA a ‘qQrUIg “a ‘qyIMg ‘a ‘Hropny “*¢ ‘MoxON'T "YH ‘sioquepnory “MT Toque “A ‘WOSPYSIT AA "e ‘puvjetowysa A, "SH “SOE A, . . . . 70) ‘UdIFTI ' "H ‘uerpmoyy [euinor qoyyny ‘penulju00—seshjougoang fo suvaw hg spvqazy fo uorynuruuagag ay? wof spoyjapy aayupyquon’y 245 QUANTITATIVE ANALYSIS BY MEANS OF ELECTROLYSIS. ‘apizo sp Sayerjyta 1eddoo puv prior o1}INN ‘apwwo Sp £ plow OIIJIN ‘apne SD § plow OIIZIN yojaU sp S ayerpAY VANTpog ‘aprxo sp § * oyBITU raddoo puv prov o114yIN ‘)pyaU Sv i sploe ae pure OLIN | ‘OPUeo 8D ‘ prow OW4IN J ‘aprLo SD $ plow OWIGINE yojau sp SayerIpAY untuomme pur ‘ayeipAq wntIpos ‘aze1j1~3 wNTIpog (pau sp t ayeqjooe I[ey[e pue azvijtey, ‘apie §p {plow LI} pur o}euoqiey ‘IPULO $Y * plow OLYIN ‘APO SY ILO OITJIN ‘apiwo SP {PINS OLIJIN } “DIA SY Sayeyooe [V.1}NIN ‘apiwo sp S$ pioe o1myding ‘apiwo SV $ plow OIIJIN [Dyas 8M Saplqo[go vANIpog | DIU SY * aYyeYooR [BIJVIN } ‘IPO 8) < plo’ OLIN, ‘apiwo SD {plow OLIGIN ‘apuxo sp {plow OIIYIN } yojIwW se {ayerexo tTantuomMUTy "(Djau $p * plow o11e,1%} pue azeydsoydorkd wnipog \ ‘(pjaw §p $ plow O1IyIU pue ayeydsoydordd wurpog | N“ ‘ayeipAT UINIpos pue 97eI171e} TINIssejod TNIpOYg ‘ayerpAy WUNTUOMIMe puL plow OLIe}IVY, ‘aye1}10 TanIpog ‘oye[exo WNnTUOMUMy ‘oqe[exo WNIUOMUMYy ‘aye[exXO WUNIUOMIMIY ploy ‘plow o110ydsoyg *ploe O11z10 pue 97e1710 WNTUOMMYy = T F681 g €8st GG ssl OL LL8T = G68L 1 6S8I 8 LL8I RT 6L8T 9T LL8T 6 C681 FI SYST TI GL8T 6 O88T BLT FORT LG F68T GF €SsT L1G F681 LG F68T FI T8s8I 86 688T ‘ava'T “OL FI S681 G T68L OL 8881 T F68I ar G68L 81 6181 €g¢ 988T O8sT * “Ws T901}N9[F *S}19Z i * “Pp -wWeYyD ‘Ieuy : Be cu9) ‘[eue ‘sq}1907 ; * “19g * ‘MOYO “MaSue 's}107 | ‘sf q 30 ‘WIYO sepeuuy ; * “puayy ‘ydurop * “Ue YH *eue *sq187 ‘ OH), ‘TRU ‘Sq107 " WyaYD :TeuR *s}197 "TOL * ‘UaYyO ‘Teue ‘sy107Z | ' “MOYO ‘Teue ‘sz107 : ag ‘lod Jap Sury : * Jog ‘qOZ “Uaqqny "n -S1og ‘leg “19g *"Iag . . . . . . . . * “Ma ‘[eue ‘s}197 "Urey "Ys}eTOy ‘mayy ‘ddy 7 “y4;euy ‘f° . ‘Pp WEYyO ‘IoUy * “UIaT{90I499[] *S}197, * ‘meYyO “MaSuv *sz197 * ‘UA “[eUe "84197 : ‘ —- SMON “TIED * WeyD ‘Teue *s}1907 “+ “A ‘uapeuroyy, * gy ‘Seuuey, Ty ‘sqonqog H ‘BIq99 "A Bropny . . . . ‘Vv ‘QYOny "y ‘QTONy *y ‘TUIZzeoseyy puw Sa) epeted ‘¢ ‘folzHOse Hy pue ‘4 ‘tporvg "T ‘snorpeyl OM ‘AU WOTJOIIL, playsur][ ‘2 ‘Moxyon'T *¢)) ‘Moxon'T "y ‘lonesqowry ‘WW ‘PaenTy “vy ‘uasse[D “vy ‘dasse[pD ‘VWI ‘Sloy pur “y ‘dassetp ‘Vv ‘purig 9) Be A A “Tq pue “yf “OL “atu ; ‘a ‘a “uyTUg ‘H ‘uepemoyy “A ‘BIOpn WV spuazeos WL Bue Ipoleg * «yZ, ‘e100 ‘0 ‘moyonT . . . 1895. REPORT 246 ‘prow olmnyd[ng | ‘ayerpAy uNUOTMUTE pur oyeydsoydor4d mantpog | ‘apweo sp {ptoe oLmnygdyug \ ‘apo sp S ayeyexo TUNTUOTUULY ‘apwo SY plow OLWIOF PUL 9}VUIIOT ‘apuco sp < prow oLmydjng ‘aprvo sp {plow OIAJIN ‘apweo sp §proe o1myding | ‘apivo sp {proe o1myding | ‘apo sp {prow OYIN } | ‘aprxo sp $ prow o1mmydyng | | ‘yojyau so SayeueXoorqy wuMtuouIUy | | ‘aprvo SD LpPlOw OWYIN J | ‘apivo sp $ plow olyIN | ‘apivo sp * * to “qarmg ‘PIOB ONIN | UZ IN “SH ‘dd “OD “PO | 29% 0 6st | * ‘wey ‘ddy » adyeuy ‘¢ | ‘af ‘weko 9 a“ “Tayag ‘plov OLIN | * dd | 831 L | 8681 | * “wraq “ddy 2 94feuy -¢ | ‘0 “f ‘reaTeg 2 “a “a ‘GaTOg “plov o119719 puvapraedéo urnisse30q "7 mo | 88h BE O6BT fe AYO Tomy | “MT ‘equenT 9A" “Uatag ‘provonngding uz‘ IN‘ ed‘oo'po | 906 8 | S88 °° "Rk WaYyQ Youy | ‘gy ‘ueUy yy gy “qIMg “prior | | | . o1ej1e} pur oyeipdy WNIUOMMy* ; sng fey ‘qaleal ‘ceil ei oT -) eer a: ‘909 "MaYyO ‘Iemy cf - ; ‘9 ‘Ss ‘“Iayonmyog *plovoliz10 puvapiuvdéounissejog | * e? SLO Me 2G 20 {S68 * carayg ‘sfyd ‘sytez | * : ‘yy ‘S1aquepnoary *SO4U[ | | -exO UIssvjod pue wntuomMmy | ° PSC ZAMRINS On Ss ege! |) 61 | 9gsl | ° ? 5 : * ‘nog | ‘yy ‘stupnyT pue “vy ‘aasse[p "SOY | -exXO UnIssejod puv uNnIueMUTy | * 4 : “ay | te! oan | Teer i: 3 : : Seer ye : : * “y ‘uasse[p “HLOWSIG, ‘ayerpq pue apiydins untpog | * * + ug ‘sy | gem | § | 6881'* ° ‘pur "HED "008 “f | “f ‘a7eSpOoA, ¥ “VW “O ‘UGOY ‘ayeipAy pue oprydins umtpog ug sy | 0906 | «26, | HOSE "reg |" "V ‘uasse[p ‘ayerpdy pur eprydins wurpog : : . us 2686 | 16 SssL °- i 3 ‘ * weg | “W ‘STI249S pue “vy ‘uasseip ‘overpay pue aprydins umtpog | * = * ug'sy | ese | 6E | 98st °° °° * ‘reg | “Y ‘Stapwy pur ‘ "y. WossEIQ ‘oyerpAy puv eprydins umipog * ty sy | FOIL | SE ] 8st; tog | “Y “BrapnyyT pue “Vy ‘uasse[9 ‘ANONILNY “T ay ATo1300/q JO uot odmog woz pavesudas 189° | ebeg | TOA. | Iva Xt | yRuinoe ioqiny ‘s]BJOUL 9T]} JO JapAO [wotyoqeYydye oatyepol OY} UT UBAIS ST doUEAoJor 94} ATTVOTZA]O.LJOoTO pouTUIeyep ore sTeyoUt 910 10 OM} Ue “AT[VOIQATOAJOOTA POUIULIOJOp ST YOIYA [eIOUL 9eYy9 JO pvoy oy} JepuN posuezIe ore suotRaedes 3 UM eo aT [eeebeut P SP qorqas | HF Jo Pvey, of}, AQpUrt | - UL “UUNUTYLLT ‘ZT ‘AINDIII “6 ‘sraddog ‘9 ‘unIMIpRD “¢ ‘OULZ “FT “wnTpelled “TT ‘UoIT “8 “HBQOD °¢ “YINUISI_ *G “MOATIS “ET ‘TPX9IN “OT “PION *L “UUNTULOIY) “F “‘AuOWIyUY *T —! S[ejoUL SUIMOT[OJ oYY JO Spvoy oY} JopuN poduvare ore uorTyeiedes Jo spoyyott oY, ‘sishjoupoarg fo sunau hg spojapy fo uoynunday ay) wof spoyrazy aarjoquywond) ‘AT 253 QUANTITATIVE ANALYSIS BY MEANS OF ELECTROLYSIS. ‘aqe[Vxo WNIuOMMY | * : 0 : "plow o1ja0v puv 940490" wUNIpog ‘plow O1UIIOJ pue soqyvuI0,T ‘aprueéd uintssejog ‘prov o10yd -soyd pue ayeydsoyd wmipog ‘apruvdd tnIssejog *proe o10yd -sogd pue oyeydsoyd wumrpog ‘opruevéd UINISseyOg ‘epruvdd wnisseyog ‘aptuedo winIssejog *ploe O11e}1e} pue soqviqiey, } *ploe o1j00e pur soqvjooy “‘proe O11e}1e} pue s}eipAy winiuoMMy *plov o1toqdsoyg *ploe oumyd -INs pue ojeydins wnimommy ‘eprueéd wnissejog *SOqR] | -exo Unissejod pur mntuomMmy *ploe 014008 pure 93v390" TuNIpog | *SO4R] “exo unissyjod pure wniuomUy ‘aqgeipsy wniuomMe IO poe o1myd [nus puev eyvydsoydoisd wmntpog “poe ormmyding | far uz * UZ IN ‘UW ‘Og ‘00 { ce iy ae ee tay te "M ‘OW ‘sv UZ “IN ‘eq ‘ID ‘IV ES LAN 00) uz - 19 > ap . ‘ug ‘sy ‘qg ‘aaare “uz ‘ag ‘op | uz ‘no ‘09 ‘sv S UZ ull . . a UZ ‘IN 8g ‘09 | 194% | Zt | ¥gs8t |° ‘NOINOUH() ‘f 8T $a G86 6LL O88I 668T 6681 6681 906 86P T68T 0681 66E POT 696 £8¢ 906 O68T O68T 688T 6881 G8s8T C61 606 S681 988T L6 €68T 8F¢ S881 TLLG | FL | I88T 18g 86 | 688T "WOINGYY) “¢ “IYO 90g “TIME * SMONT eet : "maqD “BIOUL ‘S}197, “‘msyD Log ‘f ‘WayD. Ieuy ‘f ‘WeYD ‘1Ieuy * +p Mey ‘lemy ‘"p WeYyD ‘oul “Pf UleyH ‘iemy ‘ddy 7 A,euy “¢ ‘Pp ‘WeYyD ‘IeMy ‘00g ‘WaYH ‘Iowy “f * —- SANON “TOYO ‘wayO ‘sfyd ‘sq107 ‘MAYO "[eae ‘sz197, * “reg WOH ‘[euv ‘sz107 ‘rag |° * "Wy ‘dasseIQ *V ‘IOAX ‘SH ‘Norse Ay, T'C ‘O0RTe A 9 “A “WAIHI . . . a“ “qgrag MT Pye Yao WUT ek gO MT eyo 9A TTS ET Tomer 9“ “ua MC MC MRLC LILACS ‘a ‘ ‘Teuy 3 “Wy ‘yyIUg Jo *g ‘Iayonmyog * +y, ‘emo00yT ‘HT ‘s1aquopnor, ‘§ ‘Broqserrg * *y ‘uassetO “y ‘purig 1895. REPORT 254 “pe ON}N ‘prov o1mmydyng O48 eXO UNTUOTIUTYy *SO}] -eXO WINIUOTIMIY pu UINISseJOg ‘plow’ O111U 10 ‘plow olmnyd{ns 10 ‘ayeapéy uMmou -mv pure oyeqdsoydordd wmipog “plo o1mmydyng “Oprpor tauissvjod pue oqeijie} 1[ex[V ‘ayeapay pur ayeydyns wntuowmy ‘ayeuoq.eo wnIMoMUIe pues ploe o1oydsoyg ‘oyerpAy pue ‘ayeydins umiuowmte ‘prow onmyto ‘aqyeexo WHnTUOTIULy *SO4rT .-@xO wuniIssvjod pue wuntuowUy ‘a]e]eXO WUNTUOTIMLy "SOqeT -exO TinTIssejod pue wntuomMy ‘a]R]eXO TINTUOUL -me pue ojyvydsoydorfd umtpog ‘ayeydsoydoidd winrpog ayApor}0a]q JO UorzIsodur0y e * e . po Me mere | | poe | 197 | LT | PSST otioydsoyg ‘az ‘IN | ‘UW “SW “ed 10 ‘00 ‘TV | | ; : : SUE Te pe Ieser / ; UW | 189 | 8Z | 6ST . ot | GOI 6 | OLSI ‘udddo9N °9 a re | A ae oe ons 988 FI | S68T ° UAL “ID “TY “608 ¢g | 9881 UW ‘Of | BBL ZIT | GST ' of | 090 | 26 | F68T | : "onl | eo A - uppgs| 4976 | 2T | F887 eet oan Cue | Name pil 1881 | ret oe | aid 3 / ‘a ‘2m ‘ty J | 182 88 | 68ST | Wo. pozeredes spejapy “LIVAOD “G | asvg | [OA | qwox | ‘HAY “[eUv ‘S107 “WAYO [eur ‘s}197, ‘MOYO ‘s}RUOTL sMoN “WAayO “puayy “ydut0og | * lag ‘UIYO ‘]BUe ‘S}19Z * *y SuessrIp * *y ‘Udassetp : ‘ * yw ‘puvig ap bovey ‘uorpneqstog “ny ‘UURU4IO A “J, ‘2100, ‘Vv “x ‘Soy ory * *y ‘uasse[pD "Ww ‘Uasse[p * -y ‘uassr[O *y ‘pueig jeutnor qoyyny ‘panutzu0e— srshzouzoayy Jo sunaw hq syojayy fo uorgvendag ay) sof spoypryy aarzoprzumng) “AT pie) 2 iS) F ELECTROLYSI QUANTITATIVE ANALYSIS BY MEANS O “plow ONIN, (Plee ONIN, “ple ONFIN “Plow ONIN ‘poe ormydng Pree onary “plow OLIN ‘oyerpdAy tantuowULy : ‘ppe eek *‘ploe o1myding ‘plow OLQIN, ‘ploe ormyding plo’ OLIN, “prow OLIN, ‘aqeap og . . . BY ‘SH : ey Ber * uz ‘IN ‘aq ‘09 ‘po ‘ ‘ "ag t qd ‘a uz ‘IN ‘OH “ID ‘09 ‘po , - sy PO ; 5 149) ‘CW ug ey ‘AS IN *3V oN oe PO sptoe o1toydsoyd pue ‘o1eqiey forjooe ‘sT[ey[e pue syjiva oulyeyye ‘uz “py “IN ‘UN ‘dd ‘a ‘PO ‘IV WOJ} poyeuvdos s[eqoyy L6G ST | 9L8T $86 T 6681 9€¢ FI | S681 SIP g E881 L116 696 | 988T | OGF 9T | F68T | L6T g €68T 696 L €68T 681 L §68T 861 L €68T 63E GI | O68T 83F GI | O68T FOL GT | O68T | If G O8sT S6I ST | S68I FTE 9T | LL8T OSF — | 868T } £69 — | 6681 809 €L | G88T *panuzjuogI—AtddON 9 Bug | ‘JOA | Iw9X * -"UIAYO ‘Teue 'sz107 * ‘MeYO “sLOUv *sq107 : * “MeO ‘syeuU0yY : ‘"p ‘WeYD ‘IeuIy ; ‘f ‘94Jog aap surg * 00g, "MeYH ‘Iamy “¢ * "mayO ‘s10uR ‘sz107 ‘moyD ‘Udy » 44[puy “¢ ‘moyD ‘ddy x -44[euy “P ‘mayD ‘ddy 2 “44,euy “¢ “"p TeYO ‘IEWy ; ‘Pp MOYO ‘IeUy ‘Pp ‘mMIYO “IeUy “Pp "WMIYO ‘1emMy * ‘00g "MAYO ‘IomMy “fC * "MAYD ‘Teue ‘sy1e7, * ‘May D ‘MesuR ‘sq107, ‘MOYO “MosuR ‘s}197 ‘shy 32 ‘WIYO sopeuny [vuinoe “A ‘Wosyy StI A, 'S “H “SOrre | “W) ‘WUPUI}IO A . . ait cw a ‘ fouuey, “AA ‘TURaS ‘a H ‘teouedg 79° Wa ‘ygtug ‘AH “yWIUIg ‘a ‘f ‘xakoy 3 “A “aw ‘yyTUIg Td Sovrrem 3 “Wg ‘GAIA Of ‘teqTeg 2 WT “a ‘YgTUIYg ‘TH ‘Wyrag MT PyueT yg ‘yz “MT Toque a gS ‘a ‘qyIWg ‘9 *§ “layonumyog j ‘d ‘lapemyog A PrIopnyr * “a ‘propny Vy ‘amon 1loyyny ‘ponutyu0o—srshpoujzoy gy fo suvow hq spnjapy fo uouvunday ay2 wof spoyrapy aargopyumn® * Ay 257 ELECTROLYSIS. QUANTITATIVE ANALYSIS BY MEANS OF raqerpdéy unimowme pue plow o1reqIey, ‘ayery1o tanTpog ‘ayeuoqieo tuntuoTUUe pue prov o110ydsoy,g "SOqRl “exo WnIssejod pur wntuoWMYy ‘wnhoup so i soyeyding *SOqU] -exO Wnissejod pue wniu0owMy ‘oJv[eXO TINTUOTWIUYy *o}B[VXO WNTUOTIMYy "SO]P -exO tnissejod pue wntuomULy ‘aqe[exo TUNTUOMIIUY SO} PL -exO uUInIssvjod pue umntuowuUy "$948 -exO UInIssvjod pue uwmtuomUy ‘ayeyexo TWNTUOMIMYy *Sq9e] “CxO UWnissejod puv wntuomMmy ‘ayelexo UnTUOTUUTy ‘aye[exo UUNTUOTIUTy ‘oqe[exO TUNIMOUL “we puv ayeqdsoydorfd tuntpog ‘ayeqdsoydorkd wmipog ‘apruefo wmntissej0g ‘oyerpAy pure oprydins wntpog ‘apruevdd unIssejog *pioe or10oyd -soyd pue ojeyqdsoyd umrpog ‘apruedo uinissejog : . - o. ‘ : "i ‘oo : ; ult “10 ‘IV ey, ‘aW ID ‘IV ‘ “Sol L¥i } "IN ‘09 ‘ull ‘IV uit} ~ «lV * uz ‘pn ‘IN ‘09 ult : : é 6 ay proe onoddhoud | ‘plow Onn ing ‘Ol 1Z ‘A “ID ‘og wv | ‘UW ‘TV ERE ee ' -* 9 “Sit ‘TY . AK ‘SO ‘OW ‘sy . A *M ‘ag ‘ow ‘Sy UZ “Id “Pd “IN ‘ND ‘op . . . uz ‘09 “4d ‘ND ‘sy OT €¢ 8T LT ‘meq ‘ddy puv ‘y4;euy “pc *"p WaYyO “Iemy SMON “WOO ‘ BET Met AO 7k : ‘Pp ‘WayD ‘10uly fia ¢ og : . : log 2 : “9g : ; ; ‘10g ; ; : Jog : ' Jog : : ; "reg * ‘ureqg ‘skyd ‘sq107 8 gage “WIS addy 3 ‘y4Teuy “f ‘f “WeYyD ‘lsmy “"p WaYyD ‘Iouy Riker } a qn pase “yom ‘yqrorg 7 ‘Wa “qtg L ‘e100yy ‘£ eye3poom 39‘ V “0 ‘WON “AN ‘SqqT) a * "vy ‘dosseip ‘ : * "YW ‘UassR[O * y ‘uassR[DQ . . . *y ‘uasse[pD . 2 . “y ‘aasseip *y ‘uassrlp ‘V WN ‘sloy pure “y ‘uassetp . . . ‘'y ‘puvig ‘I'd "OORITEM 29 aa “qatug p A ‘YytUIg “A AOL 3 “wy SOgTMg “Aa “TOS siete Sieues’ are: | ‘Broquepnels ‘apruvdsd UINISSeIOg ‘apiqdqus tantpog ‘aptuvdd UWINISstyog ‘apruvdso UINIsseyog ‘apluvdéd UINISse}0g ‘apruv{o TUnIsse}Og “prow OLIe}IV} pus ayerpAy wWintuomMUTy ‘aqerp dy TINIUOTIM puv ayeydins wurpog ‘Phe OLIN “prow olmmydyng ‘prow olreyie} pus ayvipsy WntIuoMmMy 8 ‘plo’ OLIN oO ‘apruvdo wanIsseyog | — | | *proe ONIN, es l| o) ‘plo’ O11g1U 10 | a oMnydus 10 oyvIpAY WTO | (ex) -ue pues oyeydsoydordd wmipog | *SOqUT | -exo UWNIssejod puy uINIUOMIUTy ‘ayeyexo TIMTUOTIM\y “OpIpor wuissvjod pue ayers, YeyLy { UIT ; uz ‘IN ‘NO . . ug ‘sy * AM ‘Pd ‘OW ‘sv t uz ‘IN ‘09 at oe S¥ BO Led 19 2 ug “qg ‘SV e ; Se ON Po "UZ ‘IN ‘UW ‘Od . . . sy ‘ag ‘ig ‘sy np ‘po : O “Ig ‘IN ‘OW ‘Ot “ID ha) "joy “Cyoy a1 Sin ng UyL | J 16 18g 86 T68T T681 T681 O68T O68T 688T 6881 €68T F68T S68T 988T 6881 ‘AUNOUTT “6 |. T&6G | TT9T ES val | fat | F88T COST “ponurzuodI— NOUT * og } * uray D Co) ‘yAyeuy “cf * -moyg ‘ddy 2 y4yeuy “¢ ‘Pp UIEyD “Iauy ‘Pp UEYDO “auy ‘pul O ‘IouUy * mayo ‘ddy 2 ‘g4yeuy “¢ . . ‘00g “WsyD ‘IoUy ‘“f ‘TUaYO “MISUe ‘s}107 0 * -‘tmmaqg ‘shyd ‘sy1907 . . . . . “19g : * “THO YD [BUY ‘S197 | Og ULOY) “S}LUOTT | * VM *£oToe OW, pure “7 “q ‘qyITIg : ‘A “gatas "WT oyury ya ‘qyaIg WT eoyaen ya a “gag “YO oyuer yy a TUL WT Pyar “Gag ‘9 'g “IayonuyO, * a Briopny * yy ‘Sroquopneig Qy ‘SIMpuy pure “y ‘uesse[p "y ‘pueig “£ ‘PULL AY 4 ‘UUBUIO A 9} {orjo1]4y JO doryrsodwog | Woy paqe nds STPEJITT ane, | gl OUN Iva [euinor Ioqny 258 ‘panutquoo—sishpougoarg fo sunau hq synjazy fv uoizounday ayp sof spoyzeyy aa yo pquane?) NN QUANTITATIVE ANALYSIS BY MEANS OF ELECTROLYSIS. ‘plow o1moyd -soyd pue ojeydsoyd umtpog *ploe O10 oorpAPT ‘apruvdo wunissej0g ‘plow onoyd -soyd pue ojvydsoyd wmrpog “Oprpor tuimissejod pue oyvIyIe, 1[eyxLV ‘ayerpAy pure ayeydins wntuowmuy ‘aqyerpAy pur oyeydyns wunraowuy ‘plow ormydyng ‘oqeipAY TnTMOWIULy ‘ayeumoqivo TINTUOMIMIY pue plow oLoydsoyg ‘aqerpAy pur oyeyqdins wmtuowmy ‘oploryo puv oyerpAéy wantuouUry ‘oJR[VXO TUNTMOTIULy *SOqRT -BxO WnIssvjod pue untuomUy *(aqeydsoyd se uoezidierd 10938) o4vIp -Ay pue ozeydius wntuowmmy ‘ayerpsy tuMm0UL -mie puev ajeydsoydoidd wmrpog ‘oyeydsoydordd tintpog "plow OILIINN "plow OLIN “opymedo sHADESSEIOT - A vy | CéP FI ug ‘sv ll ,, SV ‘OH ‘ny J 16 él “WONILV TG qT CEP | tI “‘WOIGVTIVq uz | Iv J 9&9 FI * Of | PPE 9T UW “SIT | 80g SI ' SIN | 93% G8 uy “0 ‘LV | 60 eg UN ‘Od | BBL raat 7 Um | 22 96 UML | 9&3 8 UM | TLl6 | FT 7 faa t | -816 || TR 189 86 668I &68T ‘EL 681 ab €68T LL8T 6881 LLST 988T T68T L881 6881 {88T 8L8T 6881 “IMMOINT “OT €68T ‘mayO “‘ddy x ‘q4;euy “¢ ‘uioyD ‘ddy 7 y4yeuy “¢ fs *"e ‘WeYyD ‘1eury * ‘may ‘sfyd ‘sq1az, : 5 ‘"p ‘MoyQ ‘IoWy , * ‘Ue OQ ‘syeUOPL “ “MISO “Teue ‘sz07 ca) j0 “WIIYD sapeuuy “puoy “ydut0p : " SMON ‘UIAYD 2 “puayy ‘ydm0p ‘MIAO [BUR ‘sq107 * “puy ‘WayO “dog “P¢ . . . . ‘Iog * ULaYD *[eue *syz107 * MHAYQ, ‘TRUE ‘Sz187, ati toes . “og : es : ‘AT 'a ‘yg ; 4 ; ‘a ‘HU - * uy ‘umeT4I0 A, 3 . ’ ‘gq “SIapametog pemmmmreserr 8 Oe| . . . . ‘Vv ‘Qyony . . . . “Ak ‘A100] RE heat 4 Ware Gal au . 2 ; * uUlequuy "f ‘oyespooy ¥ “VW ‘O ‘UYOY . . * “vy ‘uassetg ‘$a ‘spreyory pur’ ‘yy ‘Aouayo cr a) OU CS | ‘af ako 3% “A “YT ‘ae ‘oko FA “A ‘UNUIg id ‘aoe PAL puv “a “H ‘aqWg ma : *"Y ‘siaquopnarg | , 1895. REPORT: 260 *pyov ortnydyng ) poe omy f| @N ea ‘BW ‘dd | 80G | et | Z8sT ‘ayeuoqieo wntuoulUe pue poe o1oydsoyg | * G UW “0 ‘IV | 606 9 | 988T ‘unhpuDv sv ‘prov o1mydins 10 omor,yoorpAy | * 4d. WN ‘OW ‘an ‘09 | 8g 6 S881 ‘ayerpéy pure oyeydins wntuowmy le " UM | 992 8 6881 ‘oye[VxO VINTUOWMLY Se OS | 2aRe HO PeeL | *SOqRT -ex0 Wnissejod puv ummowumy * Ul TLL16 tI 1881 ‘ageapAY TantuoUt “we pue oeyeydsoydordd wnmpog | - ; : ‘ UI ‘ayeydsoydorsd eatrece i "9 SSI a} Ts9 86 | Gust ‘ONIZ “FI ‘aptuvdo tanissey}0g PO | 0GF 9T | F681 plo’ OLIN “ ad | 696 Z S68T ‘opruvéd UINIsseyIOg “ so | 6LL GZ | G68T ‘apruvdd UWMNISseIOg . Id | LIP €T | T68I ‘apruedo tunIsse{0q A oe ‘Sy | 83F GL | O68T ‘apruvdo tanisseyog EN aL POL oI | O68T ‘apruvéd wnIssej}og ; * nO | $96 g 688T ‘poe o1myd “Ins pue ojeydins wnwowmy * uz) Ree wT cared - arf| 809 | st | eset *Splov OT[VXO puv OITJIN : : * 4d | Qt§ — | 068T ‘oqyedy “TU WINTUOWUe puv pIOv OLIN : : 2a ‘pore oryiey pue epruvfo umisseyog }| - ‘ : . : *sproe ee pure OLIN "8 | 26 GE | S681 ‘ayerpfy pur oyeydius untuowuy | « : ‘po ‘sv 3g oe ‘apruvéo untssejog | IN ‘ng ‘09 “po ‘sy ‘UHATIC “ET ayATOsqoaTY JO UoT}{[sodu09 Woly peqwaudas spezoyy asvg | ‘JOA | avox | ‘shad 99 ‘wIqO soyeuuy z * — SMONT ‘TAT, : : “qloz-" ms : "PUT “WYN “90g “C : + og : F . og | * "MHD ‘Teur ‘sz197 | * ‘009 ‘MeO ‘1dmy ‘f "meyg ‘ddy 2 “y4reay “¢ Jog 7 ‘+p ‘may ‘iu : - Pp -wayD ‘EMy “*p ‘MIEYO ‘IoWy ‘moyD “ddy 2 -44,eay “¢ ‘shy g jo ‘WIYD soyeuuy * "MOYO “MosUP “s}I07 * ‘tayo ‘sfyd ‘sq107 [eu.tnoe “'V ‘QUONy * +y, ‘aLooyT sy s =) jah aoe At ‘oye ouneny 9" ‘VO ‘aqoy 5 "Vy ‘uassviD "sv “UaSSPTO *y ‘pueig ‘aE HH ‘toouedy » “qq ‘ygTUg df ‘oO 3 “wT “O ‘UGTIUG TC ‘OOUlleM 9 “EaTUg ‘A TUNA 29 “A o “UyTUUg WT Tear 9 Wg yyrag WT Pee yw of yt MT PyUeL 8 a “yy "oy QTOry *"?— ‘moxyon'y yA ‘Sroquepnory ioyyny ‘ponuyyuoo—sishzoujoayy fo suvow hq synjapy fo uoyuundag ay2 sof spoyzary angozyguond “AT 261 VE ANALYSIS BY MEANS OF ELECTROLYSIS QUANTITATI “TaNTMAI pep SOIOIPE Lech “YG MUsteg “UNL ‘roddog ‘seshjouqoany fo supa *sq]@S IOATIS Itoyy Jo siskporjooya oy} Aq ouTpor | pue ‘aurmoiq ‘eulIo[yo Jo uORULUMIOJep yoorrpuy J ‘UOIT UL WOgI¥vO JO UOTZVUTUMIEJO, ‘sueSoeg Jo WoTyeUuTUMIaJep O19A[01}09[ ‘sisfjoryoa[e Aq plow OlI}IU JO UOTZVULMIEYOp OTL], “quad 1140979 94} Aq 971000TeTD JO UOT}epIxO ‘quarmMo O1mqoeTa OY} Aq yTUTOIYD Jo MoOTzIsoduIO0DaqT *quarIMd O1140919 943 Aq soptydyus Jo uoTeprxO *‘SUOTJVULULIOJOp 1eSns-J19AUT 04 perdde se zeddoo zo uoryempysa o1ATo1}0e79 OUT, ‘J90}S UL WOgIvo Jo MOTYQeUITIE\Oq *£Teo1yApo1y09T9 SUIMIOIA PUR SULIOTYD JO UOVUIULIE}ep yoOoILpUT “quar -M9O O11qO9T9 BY} Aq SsoprluasIe OTT[VJOUL JO UOTyepIxO ‘uesor}IU pur ‘mntuoume ‘mmnissejod Jo UoyeUTMIOjep yooIIpUy qoatqng F9E €GP 8&6 0066 GSE IGP GIL 086 8616 O6F 8E66 TIF 6816 SIé 9166 6101 LOFG T tI &G 1G &I S681 6681 O68T 888T FL81 988T 6981 F681 O68T 168T 1681 T68L T681 6881 0681 688T 6681 F98L 6881 G68T F88t anv amino A IeoX Bo: (@ ‘SIOUL *S4197Z, “gk CUO ROuay, * “Iag , 8 8 9g "MHAYO ‘[BVUe *sz107 hq suoyvunuagag wy brau-onu0py “Pp ‘UsYO ‘IeuUry ‘Moy ‘[eue "sq107 : a “Ssqyeuoy * “Taq "meg, ‘day ay “qdyeuy ‘¢ | . . ‘rag f fee ris Oren * Jog ff HEE UlLyUVIA LC | M * "leg raed ‘may ‘ddy ay “y4yeuy ‘¢ ‘ “Mey D ‘[TBue *sz197 ‘*p uayO ‘TaUry SMON ‘TOTO “10g “AH UITOIg 79 “SAA TOUTIOT ‘A ‘of Ba el 9H “1eT1eM **y ‘uasse[p Vv, WSBSELS xy “P ‘zq1esu0g *M ‘odury Hf “PIeUITTM * *'M ‘TOM “) SUULTO4.I0 A “wy SUUPUZIO A ‘T'd ‘OORTTEAL PUr “WT “A “UWUIG . : AW ‘WMG ‘a ‘a ‘WU *d ‘d ‘ssoy Oo SURMUIYy ‘qT quoraury . SST Ty ‘Toyuely “+y ‘uassR[O [eurnoe soqyny ‘sishpouy aayniyunnty wr sishpoyoayy fo suornayddy yoroody * A “PPS ormI0} PUY sayeULio,T ein ee “UldYO *S10U8 *s}107 ‘SH SORA . ) ‘aaeorp BUT}IO A 1895. REPORT 262 LUdbue& *AIMOIOUL F ‘OIUaSIV FO WOT}D940q ‘AMOIOUI JO WOTW0940qq “UNIpeUvA pue o L [etpud) GU d * “Ua O “MISUB “S}IOZ ITeH [eIyuep ‘wey : ‘mayO ‘jeue ‘dayy ‘aoyssunq ‘amrmdprp ‘canted Jo sj[vs Fo siskpomj09[ ISL €I OSS : o - Se rog j|° "OL ‘AL ‘SV ‘99 IN ‘uN ‘qq ‘09 ‘tq Jo suONTOoS TOIT stskfoI14 -09[9 SULINP PoeUIOF SaptxO YOIYAr apun suoTyIpuog COP ad 8ST : ' "THAT, ‘"yeue ‘sq1ez | * “IOATIS FO WOM9949(T FIT G 2981 “ “Ua *[eUB "s}O7Z | * ‘pos JO woT}0930q] 9€8 9 L88T ; * “pul “Met "008 *f | * ‘sprov snommyd [ns pue ‘ormydms ‘orngia ‘aprueso umisseyod ‘soprydins 1eyye ‘umrmo1go Jo sys jo stsAjoryoapT T 6I OSST c * ‘Ue ‘[eueB *s}187Z | * ‘OSOUR.SULU PUY PRET JO UOMIaIE(T T&S LLI FIST "pe -ydjog Jepsurq | ° “AINOIOU FO WOTJOaqIaq. O&Z 61 OS8T ‘IYO [BUR *Sz187, ‘StJIve dIVI 9Y} JO sz[es Jo stskporqoO9 [HT 09 z Z6ST_ | * ‘WayO “s10ue ‘sqy1eZ | * ‘autin ut Ammoseut pue ‘pret ‘1taddoo ‘Kuowjue Jo pue suostod orpejyeut jo uooojoq L1ze Or IG8L : * "pay “WaT ‘90g "fC * ‘peel Ul YANUISIG Jo UOTZOa40q . r : ie ‘so10 OUIZ PU OUIzZ UL osouvsUeUT Es 0140930] | 629 16 E881 | pued acura | Bi 5 E [| S6T €9 I68. | b * sMON “UTED - soqeuesd0ryy O1peqout Fo stsfpo1400[ 7] VW tt TOT 181 - -qsuy uIpquRng *f “OIUNSIB JO WOT}OI3aqT COL 6 Olen i" * ‘may O ‘yeuR ‘sqylez | * ‘(ourz ‘t9ddoo) suostod orpezour Jo uooa30q B09 e OSs. ° 3 ‘mmAYyO “Teqsoryer | * | youuoy Aq y Leman an *steqq ‘stsATo130901q Aq SISAT UL puv 10498UI OIUBsI0 ur AUOTITZUe Jo m0140940(q g ca. L88T | oy, ee | == 8 — | "proy ynoyoouu0g ‘o01g “OIUOSIV LOF 4804 O14A[OIZOOTT 8&E &1 T98T ; " * "909 "UIT *f , ‘(oq ‘ng ‘Ig ‘sy ‘qg) s1093eUI oTURSIO Sut -UIVJUOD SOIN}XIUL UT S[RJet snotostod Fo uOTJO930q aI el TOSI : . * ‘90g ‘mAeyTO Lf ‘sTeJeu 1eqj30 pue | | UOIL JO souasoid UT osoUVsULIT PUL PROT JO UOTDaIaqq ose GF oss | * ‘sAY[J 70 “WIYO seTeuay | ; yoatqng astg | omnjo, ava | yeuinor | "HO ‘BIOM: ‘HO ‘BIOM ‘HO ‘FIOM ‘AH “qyTuIg ' "JT Gyonqog "°° ‘S9PLOIN Q * uoduakeyy : ‘Cd ‘moyon'T, : ‘9 ‘MoxON'T 9 * OTAoIeze'T “o ‘ssniy . ‘Vv 70) ‘UyoOy : *-y ‘predny EET ‘Toque youcsT pue 12. Mang-kudu (Al.) (Sn.). Root of Morinda umbellata. i 7. Lac-dye (Sn.). 9 8. Cochineal (Sn.). Notes.—This class includes several colours of the alizarin group, so well known for their general fastness to light, washing, milling, &c. The superior fastness of the red given by Chay-root, as compared with that obtained from Madder, is no doubt due to the absence of Purpurin in the former. The colours given by Lac-dye and Cochineal with tin mordant are dis- tinctly faster than those with alumina. Most noteworthy is the remarkable fastness of Diamine Fast Red, since it belongs to the so-called ‘Congo Colours,’ a group which, as already stated, usually supplies only such red dyes as possess at most a moderate fastness to light. ORANGE AND YELLOW COLOURING MATTERS. Cuass I. Very Fucitive Conours. (Wo00tr.) Azo Colour. Wool Book VIII. Developed Colour. Primuline Orange. From primuline and resorcinol. ON THE ACTION OF LIGHT UPON DYED COLOURS. 269 Natural Colouring Matters. Wool Book VIII. Non-mordant Colours. 3. Gardenia florida (fruit). 4. Coscinium fenestratum (root). » 5. Evodia melizfolia (bark). Norz.—tThe fugitive character of the dyes given by Coscinium fenes- tratum and Evodia melicfolia, the colouring principle of which is the base Berberine, is quite in accordance with the similar result obtained with all other ‘basic colours.’ ” Cuass II. Fuarrive Contours. (Wo0t.) zo Colours. Wool Book VIII. Acid Colour. 1. Metanil Orange 1. From m-diazo-benzene-sulphonic acid and a-naphthol. §. and J. 77. Basic Colours. 1. Tannin Orange R. From p-amido-benzyl-dimethyl-amine and B-naphthol. 2. New Phosphine G. From, p-amido-benzyl-dimethyl-amine and resorcinol. ” Wool Book VII. Direct Cotton 2. Toluylene Brown G. Colours. 18. Nitrophenine. From p-nitraniline and dehydro-thio-p-toluidine. Mordant Colours. 1. Cloth Brown R (Cr.) (Al.) (Sn.). From benzidine, salicyclic acid, and 8-naphthol-sulphonic-acid. S. and J. 171. 3 4. Cloth Orange (Cr.) (Al.) (Sn.). From benzidine, salicylic acid, and resorcinol. S. and J. 170. 13. Congo Brown R (Cr.) (Al.) (Sn.). From naphthionic acid and Cloth Orange. S. and J. 216. i 14. Congo Brown G (Cr.) (Al.) (Sn.). From sulphanilic acid and Cloth Orange. S. and J. 217. " 15. Cloth Brown G (Cr.). From benzidine, salicylic acid, and dioxy-naphthalene (2: 7). 8S. and J, 172. Natural Colouring Matters. Wool Book VIII. Mordant Colours. Jack-wood (Al.) (Sn.). Wood of Artocarpus integrifolia. Kamila (Al.). Fruit glands of Mallotus philippinensis. » Nores.—Tannin Orange R deserves special notice since it is superior in fastness to all other basic yellows hitherto examined. The Indian dyestuff Kamala has been regarded by some as a fast dye- stuff, but as applied to wool it cannot be so regarded ; applied to silk, however, it is very much faster. Crass III. Mopsratety Fast Contours. (WOoL.) Azo Colowrs. Wool Book VII. Direct Cotton 5. Brilliant Orange G. Constitution not published. Colours. 6. Toluylene Orange G (O.) (Cr.) (Al.) (Sn.). From tolidine, o-creso- tinic acid and m-toluylene-diamine-sulphonic acid. 8. andJ.196. 7. Cotton Orange R. From m-sulphanilic acid and Cotton Orange G. n 8. Cotton Orange G. From primuline and m-pheny lene-diamine- disulphonic acid. 2, Benzo Orange R (Cr.) (Al.) (Sn.). From benzidine, salicylic acid, and naphthionic acid. 8. and J. 173. Cotton Yellow G (Cr.) (AL) (Sn.). From p-amido-acetanilide and salicylic acid, &c. S. and J, 144. 270 REPORT—1895. Wool Book VIII. Primuline Yellow. From primuline and phenol. Wool Book VII. Acid Colour. 2. Metanil Orange 2. From m-sulphanilic acid and f-naphthol. S. and J. 77. Unclassified. Wool Book VIII. Acid Colour. Xanthoproteic acid. Produced by the action of nitric acid on wool, Natural Colouring Matters. Wool Book VIII. Mordant Colours. Jack-wood (Cr.). Wood of Artocarpus integrifolia. 35 Morinda-root (dyed without mordant). Root of Morinda citrifolia. Norers.—-Benzo Orange R becomes yellower during fading ; at the end of a year’s exposure there remains an olive-yellow of medium intensity. With aluminium and tin mordants the fastness is about the same as with chromium. Toluylene Orange G and Cotton Yellow G, dyed as acid-colours, were exposed last year and placed in this same class. The fastness of the former is the same with chromium, aluminium, and tin mordants; the fastness of the latter is greatest with chromium. The comparative fastness of the colour given by Morinda-root without the use of any mordant is somewhat interesting. The bright orange-yellow colour produced by the action of commercial nitric acid on wool, now known as Xanthoproteic Acid, was at one time supposed to be identical with Picric Acid. Apart from the very decided difference in shade of the two dyes, these exposure experiments confirm most conclusively the present view that they are distinct colouring matters. Picric Acid yellow rapidly changes from a pure lemon-yellow to orange on exposure to light, whereas the orange-yellow colour due to Xanthoproteic Acid undergoes no such change ; it merely becomes in the early stages of fading a little duller and apparently slightly darker. Its behaviour under the influence of light is very similar to that of such colours as Curcumein and Azoflavin (reported upon last year), and may possibly indicate that Xanthoproteic Acid belongs to the class of Nitro- azo colours ; at present its constitution is entirely unknown. Crass IV. Fast Contours. (Woot.) The colours of this class show comparatively little fading during the first, second, and third periods. At the end of the fourth ‘period of ex- posure’ a pale shade remains, which at the end of the year’s exposure still leaves a pale tint. zoxy Colowrs. Wool Book VII. Direct Cotton 1. Chloramine Orange. Constitution not published. Colours. 3. Diamine Orange D. Constitution not published. * 4, Direct Orange 2R. Sodium salt of azo-stilbene-disulphonic acid. Azo Colours. Wool Book VII. Direct Cotton 9. Cresotin Yellow R (Cr.). From o-tolidine and o-cresol-carboxylic Colours. acid, ; < 10. Diamine Yellow N (Cr.). From ethoxy-benzidine, phenol, and salicylic acid (ethylated). 8. and J. 204. a ON THE ACTION OF LIGHT UPON DYED COLOURS. 271 Nores.—The fastness to light of all the azoxy colours here mentioned is so good that they might be almost equally well placed among the ‘very fast’ colours. The Direct Orange 2R here referred to is quite distinct from the colouring matter of the same name mentioned in last year’s Report, and there classed as a ‘ very fugitive’ colour. Cresotin Yellow R and Diamine Yellow N were exposed last year, applied as acid-colours. Here, where they are applied on chromium mordant, they appear to be little or no faster to light; applied on aluminium and tin mordants they are distinctly more fugitive. Cuass V. Very Fast. (WOoz.) The colours of this class show a very gradual fading during the different periods, and even after a year’s exposure a moderately good colour remains. Azoxy Colours. Wool Book VIT. Direct Cotton 10. Mikado Gold Yellow 2G. Constitution not published. Colours. 11. Mikado Yellow, Constitution not published, 4 13. Direct Yellow G. Sodium salt of di-nitroso-stilbene-disul- phonic-acid. A 14. Diamine Fast Yellow A. Constitution not published. AA 15. Mikado Gold Yellow 4G. Constitution not published. A 16. Mikado Gold Yellow 6G. Constitution not published. 8 17. Direct Yellow 3G. Oxidation product of Direct Yellow G. Azo Colours. Wool Book VII. Direct Cotton 9. Terra Cotta R. From aniline and salicylic acid (nitrated). Colours. 12. Diamine Gold. From di-amido-naphthalene-disulphonic acid (1: 5:3: 7) and phenol (ethylated), os 5. Hessian Yellow (Cr.). From diamido-stilbene-disulphonic acid and salicylic acid. S. and J. 154. $ 6. Chrysamine R (Cr.). From o-tolidine and salicylic acid. 8S. and J. 195. 6 7. Chrysamine G (Cr.). From benzidine and salicylic acid. S.and J. 166 A 8. Cresotin Yellow G (Cr.). From benzidine and o-cresol-car- boxylic acid. x 11. Carbazol Yellow (Cr.). From diamido-carbazol and salicylic acid. §. and J. 131. Oxyketone Colours. Wool Book VIIT. Mordant Colours. ” . Purpurin (Al.) (Sn.). . Alizarin (Al.) (Sn.). Anthrapurpurin (Sn.). . Flavopurpurin (Sn.). . Alizarin § (Al.) (Sn.). Sulphonic acid of alizarin. . Alizarin 8S (Al.) (Sn.). Sulphonic acid of anthrapurpurin. - Alizarin SSS(Al.) (Sn.). Sulphonic acid of flavopurpurin. ” AOA Wr Natural Colouring Matters. 1. Sophora japonica (Cr.) (Sn.), 3. Munjeet (Sn.). Ss 4. Morinda-root (Sn.). 5. Madder (Sn.). §. Chay-root (Sn.). 272 REPORT—1 895. Nortss.—-The following Azo colours, reported upon last year, were ex- posed after having been applied as acid-colours : Hessian Yellow, Chrys- amine R and G, Cresotin Yellow G, and Carbazol Yellow. Those exposed during the past year, and reported upon now, were applied upon chromium mordant. The results now obtained show that all these colours when dyed on chromium mordant are distinctly faster to light than when dyed as acid-colours. An important additional advantage of the chromium colours is that even after a year’s exposure the faded colours appear level, showing none of the speckled appearance so frequently noticed with the faded colours dyed by the acid method. When these colours are applied on aluminium and tin mordants they are more fugitive, and may then be classed as ‘fast’ or ‘moderately fast.’ It may be noticed that Madder, Munjeet, and Purpurin give faster colours with tin than with aluminium mordant. SILK PATTERNS. All the foregoing colours were also dyed on silk, and the patterns were exposed to light, along with those on wool, with the result that the rela- tive fastness of the various colours was practically the same as on wool. The only exceptions were the colours obtained from Morinda-root and from Kamala. Morinda yellow, dyed without the aid of any mordant, is much faster on silk than on wool, and although the colour becomes brownish during exposure, it may be classed as ‘fast’ on silk. The Indian dyestuff Kamala was reported upon last year and classed as a ‘fugitive’ colour. This year the orange-yellow colour exposed was obtained by applying it in conjunction with alum, and found to be much faster than the colour obtained by dyeing in a simple alkaline bath (Na,,CO,). A sample of the rich red-orange colour dyed in India was also exposed. Both dyes examined this year may be classed as ‘ moderately fast.’ Tsomeric Naphthalene Derivatives—Ninth Report of the Committee, consisting of Professor W. A. TILDEN and Professor H. HE. ArM- stronG. (Drawn up by Professor ARMSTRONG.) In previous reports reference has frequently been made to the trichloro- naphthalenes : during the past year Dr. Wynne and the writer have at length completed their examination of this series, and have satisfied them- selves of the existence of 14, but only 14, such compounds, which is in accordance with theory. A complete table of the 14 trichloronaphtha- lenes having been published in the ‘Chemical Society’s Proceedings,’ No. 151, 1895, p. 85, it is unnecessary here to further refer to them. It may be mentioned that the series is the largest hitherto known isomeric series. Tn completing the work on this subject not only have numerous pre- parations been required, but it has been necessary also to make many chlorine determinations, and the grant has been expended chiefly on these latter. I am specially indebted to Mr. R. L. Jenks for his assistance in the analytical work. ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 273 Wawe-length Tables of the Spectra of the Elements and Compounds.— Report of the Committee, consisting of Sir H. KE. Roscoe (Chairmyn), Dr. MarsHaLL Warts (Secretary), Mr. J. N. Lockyer, Professors Dewar, G. D. Livernc, A. ScHusterR, W. N. Harrey, and Wotcotr Grisps, and Captain ABNEY. (Drawn up by Dr. WarTTSs.) TABLE OF STANDARD WAVE-LENGTHS (in air at 20° C. and 760 mm.). [See Explanatory Note, p. 294.] Rowland: ‘ Astronomy’ and ‘ Astro-Physics,’ 1893, xii. 321. | Intensity Re iue ton aud Weight Wave-lengths to. | 525 Character) Kind of Vacn» | S99 Element |____| Standard —____ I In | Jno In| Io | In Are In Sun es ee Are | Suo Are | Sun (@) (b) aul ¥ | 4 1 7714-686 | 2:09 3-5 | 12958°8 7 1 7699:374 |2-08) ;, | 12984:6 PAs] so 7 3 7671-994 | ,, 5, | 180380°9 0710 7 3 7670°993 | ,, », | 180326 [Arc] {6 8 3 7666°239 | ,, » | 18040°7 ne. O 8 3 7665:265 | ,, 3, | 18042°4 oO. 14 III. 3 7660778 | 2:07) ,, | 1380500 {6 . 14 III. 3 7659°658 | ,, 3, | 18051°9 « O 14 1G 3 7628585 | ,, | 131051 {0 14 Ill. 3 | 7627232 | ,, + | LBLOT-4 O 12 III. { | 7624853 | 2:06) ,. | 131115 { oO 12 Il. 4 7623°526 | ,, | 3°6 | 13113:7 ] oO 10 II. 5 TG21:20T 10", VLSI. [A*] 0 4 7594-059 | ,, » | 131646 2 3 1 7545°921 | 2°04) ,, | 13249°2 6 3 7511-286 | 2:03) ,, | 13309°7 6 3 7495'351 | ,, » | 133380 6 2 7462°609 | 2:02) ,, | 13396°5 6 3 7446038 | ,, », | 18426°4 6 2 .7409°554 | 2°01) ,, | 13492°5 7 2 7389°696 | 2:00) 3:7 | 13528-7 2 3 7331-206 |1-99) ,, | 13636°6 2 3 7321-056 |1°98) ,, | 13655°5 aha 4 7318°818 | ,, » | 138659-7 a 4 7304475 | ,, » | 18686°5 4 3 7300°056 | ,, » | 13694°8 10” 3 7290°714 | ,, » | 187124 6 3 7287-689 | ,, » | 187181 8 4 7273°256 | 1:97] ,, | 18745°3 3 2 7270°205 | ,, | ,, |.13876L1 8 3 4265833 | 5, | ,, | 138759'3 8 3 7264-851 | ,, » | 18761:2 4 2 7247-461 |1:96) ,, | 137942 15 TUT: 4 7243904 | ,, », |13801°0 4 5 7240:972 | ,, », | 18806°6 8 II. + 7233171 | ,, » | 13821°5 3 3 7232°509 | ,, », | 18822°8 6 4 7227-765 | ,, » | 13831°8 8 DET. 5 71223°930 | ,, » | 138839-2 wv? 6 4 7216°812 | ,, » | 13852°8 . -* Beginning of head of A, outside edge. + Single line at the beginning of the tail of A. 1895. T REPORT—1895. TABLE OF STANDARD WAVE-LENGTHS—continued. Inteneity | Reduction and Weight Waye-lengths to Character, Kind of Vacuo Element Standard In | In In| In In Are In Sun 3 Are | San Arc | Sun (a) (b) ss | wy 10 Wie 5 7201°468 | 1:95) 3°8 wv 10 ep. 5 7200°753 | ,, oO wv 7 3 4193°921 | ,, op wv? ot 6 7186°552 | ,, +“ wv? 4 fa 7184-781 | ,, 5 wv? 3 6 7176°347 | ,, 6 ? 3 5 7168°191 | 1:94] ,, ? 7 168 4 7148:427 | ,, "B 2 1 4 7147942 | ,, 6 ? 6 iT. 5 712249); | 1-981 5, ? 4 Ii. 5 7090°645 | 1:92) ,, 2 4 ET 10 7040°058 | 1:91) ,, 2? 2 6 7038°470 | ,, ay 2 6 II. 8 70357159 | ,, “5 2 3 7 4027°(26 | ,, “4 1 1 1 7027-199 |) 5, ” ? SASL. 2 7024-988 | 1:90] ,, 2 3 LV; ff COZ3 TATE Nt yy a Hf 4 IV. 1 7023:225 | ,, ” wv? 6 IV. 9 7016690 | ,, |3°9 wv? 3 IV. 5 GOLG2IDs| ss eas ij 3 ELT; 6 7011-585; |_,, ” 1 Be ol. 5 7006160 | ,, | 4, ? 4 EET. 3 7000143 | ,, 3 wv? bw aLVe 6 6999°174 | ,, | 45 wv? 5 II. 7 6989240 | ,, “A wy 5 yi, 10 6986°832 | 1°89] ,, 1 2 5 6978°655 | ,, f wv? 6 Ill. 12 6961°518 | ,, > wvl 3 III. 10 6959°708 | ,, - wv 8 I. 12 6956°700 | ,, a bani: ) >| tid Meley 4 6953-838 wv? ; 2s : Er wv? : 8 ie 10 6947:781 | 1:88) ,, B,J f0: Bie ca 5 6935°530 | » | 4, WYO. 1 III. 4 6934-646 | ,, xn [B ino ; 2 II. 8 6929 838 | ,, “f ntio, 2 1 5 6928:992 | ,, a (B12: SF ern ll 6924-420 |» | 3 10 to ‘ on) als 8 6923-557 | ,, | Fox: 4 T: 9 6919-245 | ,, ‘ [By] 10 ate. oF, 5 6918-363 | \,.| a 2? ; 2 It. 5 6916957 | ,, + IND tire : 5 3 Vile 4 6914°819 | ,, np [B,] Oo. 5 ie 4 6914:328 | ,, “f 8. oO. 5 Ti 5 6913°454 | ,, + B (Oe. 6 I. 9 6909°675 | 1°87] ,, Bo" Baloo ale 5 6908-785 | ,, | , [B,J { O. 6 I, 5 6905263 | ,, 5 110, 6b. — ae 5 6904358 | ,, |, B On; 6 Ts 8 6901-113 | ,, as BBall Oo" Gels re 6 6900199 | ., | ,, BJ Eo 6 1 8 6897:195 | ,, 7 | [Bs 10 ee 7 6896-292 | ,, |, Osci'lation Fiequency in Vacuo 138823 13883°6 13896°8 139111 139145 13930°9 13946°7 13985°3 13986°2 140362 14099°3 14200°6 14203'8 142105 14225°6 14226°6 14231°1 14233°6 142345 142478 14248°7 14258°2 14269°3 14281°5 14283°5 14303°8 14308°7 14325°5 14360°8 143645 14370°7 14376°6 143892 144146 14416°4 14426°4 14428°2 14437-7 14439°5 14448°5 14450°4 14453°3 14457'8 14458°8 14460°6 14468°6 14470°4 14477°8 14479°7 14486°5 144884 14494-7 14496°6 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 275 Element lt TABLE OF STANDARD WAVE-LENGTHS—continued. Intensity and Character In Are —s = — OWOW PN EWR DWH NWH WWW OR WP EPROM NOIIwe He haa aan > = ead Ss orb 3 2 —— Kind of Standard ala al alls Il. Ill. = alt al mal al al al sal cl call cll jW II. Weight In Sun In Are — em o1ror ow e fod e enmbd &w om bw AOOQarkoanwondnae ll aor — ANNO SCUAeCANAAH _ Wave-lengths In Are (a) 6708-070 In Sun (b) 6893°559 6892°614 6890°149 6889-194 6886°987 6886:008 6884:083 6883°318 6882-772 6881:970 6880°176 6879294 6877:878 6876°957 6875°826 6874:884 €874:039 6873076 6872-493 6871°527 6871-179 68707186 6869-347 6869-141 6868:779 6868°393 6868-124 6867:800 6867-461 6855°425 6843°908 6841°591 6828°850 6820°614 6810°519 6807:100 6787:137 6772°565 6768°044 6752°962 6750°412 6726'923 6722-095 6717:934 6705353 6703813 _* The principal line in the head of B, a difficult double. __ + These two lines are at the beginning of the head of B. There isa fine line midway between them. ' ¥ A difficult triplet. Reduction to Vacuo O cillati n Viequency in Vacuo 145024 14504°4 14509°6 14511°6 14516:2 14518°3 14522°4 145240 14525:1 14526°8 14530°6 14532°5 14535°5 14537°4 14539°8 14541°8 14543'6 14545°6 14546°9 14548°9 14549°6 14551°7 14553°5 14554°0 145547 14555°5 145561 14556°8 14557°5 14583°1 146076 14612°6 14639°7 14657°4 14679°2 14686°5 14729°7 147615 147713 14804°3 14809°9 148616 148723 148515 14903 4 14909°5 149129 T2 276 REPORT—1895. TABLE OF STANDARD WAVE-LENGTHS—continued. Intensity Reduction aq and ore Weight Wave-lengths to aoe Character | Kind Vacuo | 239 Element of aa 8 In In ae In | In | In Are In Sun me ee & s” Arc} Sun Are| Sun} (a) (b) A i) Fe . 5 I 10 6678°232 |1°81 | 4:0 | 149700 Fe 4 } ae 6 6663°696 | ,, | 4:1 |15002°6 2 1 iT. 4 6663'525 | ,, | ,, | 150030 Ni 5 5 i. 10 6643°882 {1°80} ,, | 15047°3 Fe 3 III. 7 6633992 | ,, | ,, | 15069°8 Fe ; 4 I 9 6609°345 | ,, | ,, | 151260 Fe 4 I. 12 6594115 |1:79)} ,, | 15160°9 Fe 5 if 11 6593161 | ,, | ,, | 151631 Fe 4 IV. 7 6G575:179.| 4, | 55 | 15204:6 2 2 III. 5 6574477 | ,, | 5, | 15206:2 wv 1 III. 6 6572°312 | ,, |, | 15211:2 Fe . 6 I; 13 6569°461 |1:78| ,, | 15217°8 [C]H 30 I. 13 6563:054 | ,, |, | 15232-7 wy. 2 III. 6 6552°840 | ,, | ,, | 15256°5 nS : \s L. 1 6546-486 | ,, | 4, |15271-3 2 3 I. 12 6534173 | ,, | ,, | 153001 wv 1 III. 7 6532°546 |1:77| ,, | 15303-9 Fe . 4 ine 10 6518°594 | ,, | ,, | 153366 (fat Es 6] 4 III. 7 6516°315 | ,, |, | 15342-0 Ca. Bul eb Ip 10 6499871 | ,, | 4:2 | 15380-7 Fe . 7 I. 9 6495:209 | ,, | ,, | 15391°8 Ca . 8] 6 I. 10 6494-001 |1'76| ,, | 15394-6 2 4 I. 8 6482:099 | ,, | ,, | 154229 wy. 4 1 ino 6 6480°264 | ,, | 5, |15427-3 Ca . 5] 5 7 1¢ 7 6471°881 | ,, | 5, | 15447-2 ne io) tae } I. 9 6462'835 | ,, | ,, | 154689 Ca. 5] 6 I. 6 6450:029 |1'75| ,, | 15499-6 Ca 10r| 7 I. 11 6439298 | ,, | ,, | 15525-4 Cd M. 1 6438680 ” ” 15526°9 Fe 6 I. 10 6431:063 | ,, | ,, | 15545°3 Fe 6 III. 10 6421°569 | ,, | | 155683 Fe 5 1B 8 6420°171 ” ” 15571'°7 Fe 7 I. 10 6411-°864 |1'74| ,, | 15591°9 Fe 6 I. 8 6408:231 | ,, | 5, | 15600-7 Fe . 5 3 IV. 6 6400°509 | ,, | ,, | 15619°6 Fe x 8 IV. 5 6400°200 | ,, | ,, | 15620°3 Fe 7 1g 9 6393°818 | ,, | ,, |15635°9 Fe t I. 6 6380:951 |1'73| ,, | 15667-4 Ni 5] 2 IV. 2 6378461 | ,, | » | 15673°6 Fe 6 I. 8 6358:902 | ,, | 4°3 | 15721°7 Fe 5 III. 8 6355'259 | ,, | 5, |15730:7 Fe . 5 16 6 6344°370 | ,, | 5 | 157577 Fe . ; 6 if 12 6337-042 |1:72] ,, |15775°9 Fe . & 6 16 12 6335:550)| |y50) ose | one Fe . Fs 5 I. 13 6322:912 | ,, | ,, | 15811°2 Fe-(Ca) . 6 I. 14 6318'242 | ,, | ,, |15822°9 Fe . : 3 LV; 5 6315541 | ,, | 5, | 16829R7 Ni’. 6) 4 I. if 6314:874 | ,, | ,, | 15831°3 Fe fi i, 7 6301'719 |1'71| ,, | 15864-4 OL 3 I. di 6296'144 | ,, | ,, | 15878-4 O* 3 III. 6 6293152 | ,, |,, | 15886:0 * Second line in the second pair of tail of a. ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS, 277 TABLE OF STANDARD WAVE-LENGTHS—continued. Intensity Reduction A and Kina | Weight Wave-lengths to She Character of Vacuo oa FI ie ee en (SLANGSTO tan) eoia|t me ava wale |. an a ee In | In , In| In| In Are In Sun }a4 1 é o Are | Sun Are | Sun (a) (b) Jone = 2 II. 5 6289°608 |1°71)| 4:3 | 158949 2 Il. 7 6281°374 » | 9 | LOgLo:8 4” I, 9 6278°289 » |» | 169236 3 a 10 6270°439 » | >, | 15943°5 a I. 11 6265°347 |1'70| ,, | 15956°5 5 2 I. 9 6261:316 pre gy) |ogeGra hep x 8 6256574 | » | » |15978-9 7 Te 9 6254-454 > |» | 15983°8 (a I, 9 6252°776 » |» | 15988°6 7 I. 9 6246°530 » |, | 16004°6 4 ie 8 6237529 | » |» |16027°7 2-6 7 I. 12 6230:946 |1°69| ,, | 16044°6 6 q. 10 6219-493 » | 44 | 160741 6 13 9 6213°646 eli | | LEOSS:2 6 i 10 6200°533 we list (hobeorZ 8 is 10 6191:770 {1°68} ,, | 161461 4 6 il 9 6§191°397 » | 9 |16147°0 6 Le 8 6180°419 sy Waw) PLOLT beg 5 6 if 8 6177:028 » |» | 16184°6 6 Ty 8 6173°554 lee LOEB ri 7 7 Te 8 6169-775 » | 9 | 16203°6 Gil Gekt nk 4 6169-260 | 5, | ,, | 16205-0 1dr] 10 | i. 9 6162383 | ,, |,, | 16223-1 5 ite 4 6160-970 » | | 162268 3 ae 5 6154:431 |1°67] ,, | 16244°0 LS de 9 6141934 dye [ste REZTT 8 IL. 9 6136°834 » | 5, | 16290°6 Pdr) +9) Ts it 61227428 » | 5). | 163290 5 6 1 8 6116415 |1°66| ,, | 16345-0 4 3 ie 8 6111°287 yltin | L6358:8 5 6 I. 8 6108°3388 » | | 16366°7 20 M. 4 6103'812 » | 99 | 163788 zs \ IV. 8 6103-449 | ,, | |16379°8 10r| 6 I. 9 61027941 » | | 163811 4 II. 4 6102°408 » | 9 | 16382°6 3 1s 12 6079°223 |1:°65/4°5 | 16445-0 Bal ok 13 6078-709 | ,, | ,, | 16446-4 a 13 6065-708 | ,, | ,, | 16481°6 5 is 9 6056:232 | ay | 265074 ry oe 2 8 6042316 |1°64| ,, | 16545-4 dalbe-o: 7 6027-265 | ,, | y | 16586:8 Gale ake 8 6024-280 | ,, | ,, | 16595-0 10 5 is 6 6022:017 | a) 1) LEGON “ \ IV. 6 6020-347 | ,, | 5 | 16605'8 10 6 I. 8 6016°856 » | ey | 16615°5 10 6 ie 5 6013°717 lon pleG2ace 6 I. 6 6008°782 st | 59) | 2663758 First line of first pair in the tail of a. * + Chief line in the a group, a very close doub!s, } A difficult double. 978 REPORT—1895. TABLE OF STANDARD WAVE-LENGTHS—continued. - Reduction ena 5 Weight Wave-lengths to Character! ind Vacuo Element ot 7a 7) Sen Shandard In | In In | In In Are In Sun Pea (ote Arc} Sun Are | Sun (a) (b) A Fe 4 BE 3) | 6008'196 |1°64 | 4°5 Fe 6 i 7 6003°245 {1°63} ,, Fe 6 If if 5OSTH2SGUt sy) ||| gs Fe 6 ik 6 5985-044 | » |» wy 2 IV. 1 | BONT-2549|' fy iss Fe 5 DUT: 13 5977 -005=|| Gar la Fe 4 T; 12 5975:O 065) > 55" ss Fe 5 if 12 5956°925 |1°62/4°6 Si 6 i 14 59487G1E|) $5 oles Fe 6 Te 13 5934°883 | 4, | 55 Fe 6 ike 14 5980°410'| 55 | 5 wv 6 ile 12 5919-855 |1°61] ,, Fe . 5 i: 16 SOWG ATS") 3,455 2wv. 5 a ; } I. 17 59143841 ,, | ,, Fe . 5 I. 15 BSOD*8956) 55 alas Fe? 1 ; eet 4 } IV. 13 5901681 | 5, | » Fe? \ i Par ze i } IV. 10 5898395 | » | 9» [D,]Na 10 1s 20 5896154 | 5, | » Niv: ai 4: Iil. 14 5893°098 | ,, | 3 [D,]Na 15 II. 20 5890-182 |1°60} ,, WV 3 IV. 8 5889°854 | 4, | » wy 4 Ags } IV. 11 5884-048 |», |» [D,]He 5875°982 | ,, | 3 Fe . 6 ie 16 5862-580 | ,, | » Fe . 6 118 15 5859°810'| 4» | »» Ca 10 ef AT, 14 bSaTOe2e|) all as Ba 10} 5 I, 14 5853-903 |1°59] ,, Ni S| ie 10 6 5831-832 | ,, | 4:7 Fe 6 IV. 14 5816'594 | ,, | 4; Fe 5 I. 14 5809°437 | ,, | ,, Fe 5 i 7 5806°954 | ,, | Ni 7 5 I, 8 5805-448 | 1°58) ,, Fe 5 I: 9 5984000) sy | ss 2 4 I, 10 5798:0871 5, | 4s Fe = ; Cr J 10 7 E, 16 OTILZOT | sy | as Cre i. 5 E. 13 5788136 35 | as (Gai . 6 4 Me 9 5784081 | ,, | Cu? Co?. if I. 9 5782°346 | ,, | 5» Fe . 5 I. 9 5775°304 |1°67] ,, Si 5 De 6 BTT2Z:360| 45, “| 55 Fe 7 IV. 8 BGs Zao “5 |) 4, 2 By Ni 5 Ts 9 5754884 | ,, | 4, Fe 5 Ti 10 ray E3313: 2g Up Me Fe 4 iT 10 SIUB2Z250 1,5 ||\55 Fe 3 JHU 10 5742°066 | ,, | ,, Fe 5 le 10 5731-973 |1:56! ,, * An exceedingly close double. Oscillation Fiequency io Vacuo 16639-4 16653°2 16697°6 16703°8 16725°6 16726:2 16730°3 16782°6 16805°6 168449 16857°6 168877 168974 16903°3 16927°6 16939°7 16949°2 16955°6 169644 16972°8 16973°7 16990°5 17013°8 17052°7 17060°8 17067:0 17077°9 17142°6 171875 17208°7 17216°0 17220°5 172414 17242°4 17262°8 172720 172841 17289°3 173104 17319-2 17346°7 173718 17376°5 17379°8 17410°6 17441°3 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 279 Element TABLE OF STANDARD WAVE-LENGTHS—continued. Intensity and Character In | In Arc | Sun 3 5 | o 6 5 5 6 5 4 5 6 4 2 3 a 2 a 5 il 4 2 4 2 Z 3 2 3 5,2) 4 2 2 2 6 2 2 5 5 6 3 2 2 5 4 fii 4 3 2 Tr) 6 5 4 10r} 6 6 4 5 4 6 5 4 3 3 2 3 2 2 10 7 5 3 5 4 5 4 3 4 2 3 l5r| 4 3 3 3 4 3 4 Kind of Standard M. Ill. 7 HH | oon I aoe fl cn Be anit = in | on er ne ee He SR latte at M.I. _ SHH Ft et ete lama! _— Be et te Weight In Sun In Arc 10 bw phew to as MOM DMODNMDDDDOHMDNIDOMNANPEE Wave-lengths In Are (a) 5711°374 5601°502 5598712 5598.563 5594689 5590°352 5588-977 5582°204 5528-672 5513:127 * Not recommended as a standard in the are. + Fe 5603-180 Ca 5603-080 Fe 5602:995 |} { In the arc this line is diffuse on one side. edge of the band-like line. In Sun (b) 5715°309 5711°318 5709°760 5709°616 5708620 5701769 5688-434 5682861 5679°249 5675°648 5662°745 5658'096 5655°707 5645°835 5641°661 5634167 5624-768 5624-253 5615°879 5615°526 5603-097 5601°501 5598-715 5598°555 5594-695 5590°342 5588-980 5582-195 5576°319 5569848 5555°113 5544158 5543°418 5535073 5528°636 5513-207 5507-000 5501-685 5497-731 5487-968 5477-128 5466°608 5463-493 5463:174 Reduction to Vacuo Oscillation Frequency in Vacuo 1749271 1750430 175091 17509°5 175126 17533°6 175747 17592-0 17603°2 176143 17654°5 17669'0 176765 177074 17720°5 17744:0 17773°7 177753 17801°8 178030 17842°4 17847°50 17856°3d 17856°8d 17869°2 1788316 17887°45 17909°2b .| 179281 179489 17996°5 18032°1 18034°5 18061°7 18082°7 18133°48, 18153°8 18171°2 181843 18216°7 18252°7 182879 18298°3 18299°4 The solar line corresponds to the 280 REPORT—1895. TABLE OF STANDARD WAVH-LENGTHS—continued. aa Fanny EERE 7 Intensity and Element es =| Q © 5 Oar x ra —— “© = ROS CSE A SEO SO SOU Sy POH WRAANNWARTAAIAT A AONw oH gy ? oO rn 4226 ° Ne —— w — bo OWA, oo TPP iro ad WNNETONF WHER OWOrO ey © 209 Cs GO > Or CD HE OTD OOD He LO ey © an, es ee, isl eo! oO * ao 8 * A difficult double. + The red component, a difficult double. Character Kind of Standard Weight In | In Arc | Sun ae m7 re iy — NOOK NRE OO CONCH DO © 12 3 16 bo Wave-lengths Reduction to Vacuo In Are (a) 5447°116 5434:725 5405979 5397°319 5350 670 5349-599 5270-445 5269°714 In Sun (b) 5462°732 5455°826 5455-759 5455°666 5447-130 5434°742 5424°284 5415421 5410-000 5405°987 5397°346 5393378 5389-683 5383°576 5379°776 5371-686 53707165 5367°670 5363:056 5363°011 5361°813 5353592 5349-623 5333-092 5324'373 5316°950 5316°870 5316°790 5307-546 5300918 5296'873 5288°708 5283 803 5281-968 5276:205 5273554 5273443 5273°344 5270533 5270°4.95 5270448 5269°722 { A difficult triplet. | 18583-0 Oscillation Frequency in Vacuo 18300'9 18324:0 183243 18324°6 18353°3d | 18395:10 | 18430°6 18460°8 18479'3 1849300 18522°5d 18536°2 18548°9 18569°9 18611-°0 18616°3 18625-0 186410 186411 18645°3 18673 9 18684-1 18687°8b 18745°7 187764 18802°7 18803:0 188032 18836:0 18859°5 18873°9 18903-0 18920°6 18927'1 18947'8 18957°3 18957°7 18958°1 189682 18968°3 18968°5d 18971-10 § The 1474 lines is a triplet, or rather a double, the red component of which has a:weak side-line to the violet ; probably the violet component is due to iron, and the weak line to cobalt, but the red is unknown. ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 281 Element TABLE OF STANDARD WAVE-LENGTHS— continued. Intensi'y and Character In | In Are} Sun 6 6 4r ja 5 8 3 (ii: a 4r| 3 f 6} 2 \ 1 2 6 }s 2 1 2 3 3 3 2 2 3) 3 iq 8 4 4 2 2 Bs 4 3 4 10r} 3 3 3 8r| 4 4 3 2 2 3 4 8 3 6 4 2 4 40r| 20 10r| 3 35r| 10 5 5 3 4 3 4 6 6 20r) § 2 2 1 4 4 2 6 2 2 2 1 4 3 ? 3 5 Kind of Standard I. ed Fe ed) eed co ea Sietatalalatalltalala ire re _ Reduction Weight Wave-lengths to Vasio |. 2 S 2 a3 Ail eee In| In In Are In Sun Soe) es Arc} Sun (a) (b) cats es 1 8 | 5266-733 | 5266°729 | 1:44) 5-2) 18981:95 1 5265°884 | ,, » | 18985:0 2 5265°789 | ,, » -| 18985'3 1 2 | 5265°725 | 5265°727 | ,, » | 189855 2 3 | 5264408 | 5264:395 | ,, »» -| 18990°3d 3 5264°327 ” ” 18990°6 2 5 | 5262-408 | 5262°391 | ,, » | 18997°6b 1 5262°341 | ,, 3 | 189977 1 | 12 5261°880 | ,, » | 18999°4 1 5 | 5260°556 | 5260°557 | ,, », | 19004:20 12 5253°649 | ,, » -| 19029°2 11 5250°825 | 1:43) ,, | 19039°4 iat 5250°391 | ,, », | L9041:0 10 5242°662 | ,, « | 19069°1 9 5233°124 | ,, » -| 19103°8 8 5230°014 | ,, » | 19115:2 10 5225°690 | ,, 3) | L930 10 6217°559 | ,, », | 19160°8 10 5215°352.| 5» » | 19169:0 2] 12 | 5210-549 | 5210556 | 1-42) ,, | 19186-6d 10 5204°708 | 5, | 5:3 | 19208'1 : 11 5202°483 ” ” 19216°3 10 5198°885 | ,, », -| 19229°6 2 8 | 5193°134 | 5193°139 | ,, » | 19250°90 1 3 |} 5189-019 | 5189°020) ,, », | 1926626 7 5188°948 ” ” 19266°4 2/11 | 5183-791 | 5183:792 | ,, », | 1928568 1h) 5173'912 |1°41) ,, | 19322-4 2 9 | 5172°866 | 5172°871 | ,, 1, | 1932636 11 5171°783 | ,, » | 19330°4 33 5169°218 | ,, » | 19340°0 5 5169°161 | ,, », | 19340°2 3 | 5169066 | ,, » | 19340°5 2 3 | 5167-664 | 5167°686 | ,, », | 19345°76 1 5167°572 | ,, » | 193461 2 3 | 5167-488 | 5167-501 | ,, », | 19346°40 10 5165°588 | ,, | ,, -|19353°6 2 1 | 5165-241 | 5165:190} ,, » | 19354-9a 13 5162°448 | ,, » | 19365°4 11 5159°240 | ,, », | 193774 10 5155°937 | ,, » |19389°8 10 5154:237 | ,, » | 19396:2 9 5151:026 | ,, », | 19408°3 10 5146°664 | ,, » | 194248 the arc the first line of the first head of the green carbon band. 282 Element Fe . ‘ Fe(Cu) . Fe . . Fe . Cd . Fe P50 ~ REPORT—1895. TABLE OF STANDARD WAVE-LENGTHS—continued. Intensity and Character| Kind of Standard In | In Arc | Sun IV. 3 4 iW. 5 2 IV. ANS) 1 ( III. 5 6 Ta: 4 6 | III. 2 6 : \ I. 4 4 I. 3 2 ip 3 Bll 2} iis IV. 5 2 Ie 4 3 aoe } Il. 3 2 ls BM 83 I. 33 2 LV: Chee it 2 M. 4 3 if 4 4 i 10 3 IT. 2 2 Il. Be 66 t., 3 2 M. 33 2 a 2 \ IL. a 3 II. 5 4 ie: |e. II M. 3 3 tor Wele-e 2) 6 Up 33 4 II. M. 10x i }4 M. II 3 4 if 10 4 RT, 2 1 as } i. 3 3 : } IL. 3 ; }s I. 8 | M. IV 6 | M. IV Reduction Weight Wave Lengths to Vacuo In | In In Are In Sun |, ay. Arc | Suo (a) (b) A 2 5143-106 | 1°41) 5:3 5 5143°042 | ,, is ] 5142°967 | ,, se 5 5141:916 | ,, ay 4 5139°645 | ,, i 4 5139°539 | ,, FP) 4 5139°437 | ,, - 12 5133-871 | 1:40) ,, 9 5127°530) 1 |: a 9 5126°369 | ,, ss 9 WEY 4p 9 5115°558 | ,, | 5-4 11 SITO STON, Ss rf 11 5109°825 | ,, Aa 12 5105°719 | ,, yr 7 5097°176 | 1°39) ,, 9 5090959 | ,, . 1 5086001 ” ” 9 5083°525 | ,, mI 14 5068946 | ,, ; 12 5064°833 | ,, a as) 56060252 | 1-38) ,, 12 5050-008 ” ” 2 1 | 5041-867 | 5041°795 | ,, Pr) 8 50367113 | ,, Ay 8 5020°210 | 1°37) 5:5 10 | 65014:412 | 5014422 | ,, a3 3 | 10) 5007-473 ” ” 5007°05 ” ” 10 5007°431 ” ” 8 5006°303 | ,, ” 10 5005°904 ” ” 5 5005-634 » ” 8 | 4999°668 | 4999-693 | ,, 7 7 4994°316 ” ” 1} 10] 4981°893 | 4981°915 | 1:36) ,, 5 4980°362 | ,, ” 8 4978-782 ” ” 10 4973:274 | ,, ” 4959°02 ” ” 3 4957-786 | ,, > 3 4957-482 | ,, A * Commencement of the head of Mg band. Oscillation Frequency in Vacuo 19438:2 19438°4 19438°7 19442°7 19451°3 19451°7 194521 194732 19497°3 19501°7 19519°1 19542°8 19561°9 195647 19580°5 19613°3 19637°3 19656-4 196660 19722°6 19738°6 19756°5 19796°5 19828 5a 19851-2 19914:0 19937°50 19964°6 199663 19964°8 19969°3 199709 19972:0 199957 20017'3 20067°10 20073°4 20079°7 201020 20159°8 201648 20166:0 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 283 TABLE OF STANDARD WAVE-LENGTHS—continued. Intensity Reduction » and it Weight Wave-lengths to aes Character) Kind Vacuo | £98 Element __ of re =e In| In plandard n| In In Are In Sun il & oF Arc} Sun Arc} Sun (a) (b) iil a i= Ba* , 60 | 7| M.II.| 1| 10 | 4934-237 | 4934-247 | 1-35! 5-6 | 20260-95 Fe |. phy ete 12 4924-955 | ,, | ,, | 202992 Fe 2) 4| 1. 13 4924-109 | | | ») | 203026 Fe 9| 9| m.r. | 1] 7| 4920-676 | 4920-682 » | ;. | 2031685 Fe ein) k 4 4919183 |, | ;, | 20323-0 Pb Th. ile 4905-634 134] ,, | 20379.1 Fe 5 L. 14 ag Bile te } 4903-488 | ,, | ,, | 20388-0 Yt. 2| IL 11 4900:306 | ,, | ,, |20401:3 iy, 4.) 2s] oaks 1 4900098 | ;. | ,, | 204021 Fe . 7.) Miho. 11 4890945 |» | >. | 20440°3 [F] H 15| IL. 5 4861-496 | 1°33] 5-7 | 205641 Fe . dhs BREE Tg, 14 4859:934 | ,, | ,, | 205708 Fe? a4 re _ | 4824-325 |1:32| ;. | 20722°6 Mn 10| 6| M.L | 1/12] 4823-715 | 4823-697] ,, | ,, |20725°36 zn 3/ MI. | 1] 1] 4810-725 | 4810-723 | . | ,, |20781-20 sat a ee ee 3 4805-253 20804°8 2s ? 1 J 2 ” ”> Cd . Mews. | |o08 4800-097 131] ,, | 20827-2 Mn . 10r| 6| M.I. | 1] 11 4783-607 | 4783601 | ,, | 5-8 | 20898-95 Mn . 15r|' 6 |. I. ret 4754-226 |1°30| ,, | 21028-1 Mn ff 3 re } ality \ um. 11 4727-628 |1-29 ,, | 211465 Zn. 4| 4| MI. | 2] 2| 4722339! 4729349] ,, | ,, |2117015 Ni. or} 6”) M.1I.| 1| 1 4714598 | 4714599 | |, | ., |21204-90 Ni 3.) apis) ide 13 4703-986 | | | 5-9|21252-7 Mg Bl ul ok: 1 | 11 | 4703-249 | 4703180 | ;, | ,, |21256-3b Fe | 3) 4 ; j : Ti } | oe hi 11 4691°581 | 1-28) ,, | 213089 2 dpdit oT. 14 4690°324 | ,, | ,, {213146 Ni 4) heim 12 4686395 |; | ., | 21332 Fe eae Ce ee 13 4683:743 | ,, | ,, | 218445 zn 2] M. 1 4680:319 » | | 21360-2 Fe s)4@| I 12 4679028 | |, | ,, |21366-1 Ca 42| M. | 3] 3| 4678-339] 4678353 | ; | |, |21369-15 4 ARS \ 1. re 4668-303 | ,, | ,, | 214152 Ni ér} 3| M.Ur.| 1] 1] 4648-833} 4648-835 |1-27| ,, |21504-90 Fe 2|4|/ 1 17 4643°645 | ,, | , | 215289 Fe 3| 4] IL 14 4638-194 | |. | 3, | 215542 Fe S71) 14h ho alle 14 4637°683 | ,, | ,, | 215566 Co 5 KLE ‘ 4 . : \s Il. 13 4629°515 | ,, | 6-0) 215945 mg ai Bae 11 4611-453 |1-26 ,, | 21679-1 Sr bor) 2| M.II. | 5] 4| 4607-606] 4607-509] ,, | ,, |21697-7a Ct 46066 , | a | 217020 Li 50r M. 1 460225 | oy | 217225 Fe sl ec lewis 20 4602183 | ,, | ,, |21722°8 Ti? anh s-eils 15 4590129 | ,, |, |21779-9 Cr? dalek i 14 4588384 | ,, | ,, | 21788-2 Ca Ti BL) phe i 1 | 14 | 4578-807 | 4578-731 [1-25] ,, | 2183410 * A difficult double. } First line in first head of blue cyanogen band (¢). 284 eee ee EE — Element REPORT—1895. TABLE OF STANDARD WAVE-LENGTHS—continued. Intensity and Character In | In Arc | Sun 5 6 3 5 4 6 70r| 7 4 6 5 1 2 2 1 5 4 5 a| 1 3r] 2 6r| 6 8 5 4r} 3 Sr} 4 5r| 4 4r} 4 6 6 9r| 2 10r;} 8 1 1 2 3 15r| 10 5 5 4 5 5 1 oA 3 3 1 4 3 2 2 2 1 10r} 8 4r| 3 P(e) ee 4r| 2 10r| 4 8 2 6r| 4 aL) wz 4 10r} 4 4r| 3 5r| 3 L5r) 1b 8 2 1 Kind of Standard Weight Wave-lengths In | In In Are In Sun Arc | Sun (a) (b) 14 4572157 1 | 14 | 4571:281 | 4571:277 118} 4563939 6 8 | 4554-212 | 4554-213 3) 4513°883 4 4511474 ile 4508°456 4502°6 18 4501°444 { 4499°315 8 4499:070 I 14 4497:041 2118 | 4494:756 | 4494°735 5 2 | 4456°791 | 4456°793 6 3 | 4456:055 | 4456°047 2 6 | 4454-949 | 4454-950 5 | 18 | 4447'912 | 4447-899 5 6 | 4435°856 | 4435°852 5 5 | 4435°133 | 4435°132 9 7 | 4425°616 | 4425-609 3 7 | 4415°298 | 4415-299 4413181 19 4407850 10 | 11 | 4404°928 | 4404-927 14 4391:149 10 | 11 | 4383°721 | 4383:721 1 | 17} 4876108 | 4376:103 1 | 14 | 4869:948 | 4369-943 10 4359°778 1 | 17 | 43&2°908 | 4352-903 11 4343°387 8 | 15 | 4825°932 | 4325:940 3 | 16 | 4318°816 | 4318°818 8 | 10 | 4808°072 | 4308:071 3 4308:034 3 3 | 4307-906 | 4307:904 4 4 | 4306:071 | 4306:071 1 4305°636 5 7 | 4302-690 | 4302°689 3 5 | 4299°153 | 4299°152 14 4293°249 2 2 | 4289°884 | 4289-881 3 5 | 4289°527 | 4289°523 2 4 | 4283:175 | 4283:170 1 2 | 4274-954 | 4274-958 8 9 | 4271:920 | 4271:924 12 4267958 Reduc- tion to vacuo A+ y in Oscillation Vacuo Frequenc 21865'5 21869'70 21904'8 21951°60 22147'8 22159°6 22174:4 22203°3 22909°0 22219°5 22220°7 22230°7 222420 22431°5 2243524 22440°7b 224.76°3D 2253740 22541-0D 22589°5d 22642°2a) 22653°1 22680°5 22695°6d 22766°8 22805-4 22845°1b 22877°3d 22930°5 22966°8D 23017'1 23110-00 23148710 23205°7b 23205:°9b 23206°60 23216°5 23218-9 23234°8b 23253°9b 23285°9 23304:2b 23306°16 23340°7b 23385°5d «| 23402°26 234239 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE: ELEMENTS. Element Fe-1§ Ce-Fe-Ti TABLE OF STANDARD WAVE-LENGTHS—continued. Intensity and Character In | In Arc} Sun 6r 20r | a Se Le} = Re POONA 40r — ~ bo 0100 bo eee ~ ia Senet or wm ee iad ee AaAnInoroOnrFNNH DM ORR Www we oo ore —HOmNONMTORON ANN WRAWRHO,- 6 40r} 1? 20r, 20 50r 7 20r 10} 1 4 1, 2 285 Kind of Standard _* First line in first head of cyanogen band (6). ¢ First line in second head of cyanogen band (6). Reduction Weight Wave-lengths to Ee Vacuo | S58 ia In | In In Ate In Sun u EES Arc|Sun| (a) Gb) | = Pee. | 4| 3 | 4260-647 | 4260-638 | 1:17) 6-5 | 23464-12| 2/15 | 4264-494 | 4254-502 | ,, | ., | 23498-05) 4} 3] 4250°949 | 4250:956 | ,, | 66| 23517-6a 1] 1 4250-300 | 4250:290| ,, | 4 | 23521-20 9| 10] 4226898 | 4226-892 | 1:16) ,, | 23651-42 1 | 22 | 4229:396 | 4229-381 | ,, | » | 23676-70) 4| 2] 4216133 | 4216137] ,, | ,, | 23711-8a 6| 3 | 4215-688 | 4215-687] ,, | ,, | 23714:3a 2 4215-616 |. | » | 23714-7 | 2| 41] 4202-187 | 4202:188 | 1:15) ,, | 23790-52 2 | 22 | 4199-257 | 4199-263 | ,, | 6°7| 23807-0 5 | 6| 4197-256 | 4197-251 | ,, | ,, |23818-40) 20 4185-063 | 4 | » | 238878 | 41582 Ll4) ,, | 24042-2 | 17 4157-948 | 4, | 5, | 24043°6 | 13 4121-968 | 1:13) 6°8 | 24953-5 | 1| 12] 4121-476 | 4121-481 | ,, | ,, | 2428682) 14 4114-600 | ,, | » | 24296:9 | 12 4107°646 | ,, | ,, | 243380 10 4103101 | ,, | ” |24365-0 | 8 4088-716 | 1:12) 6:9) 24450:7 | 7 4083:928 | ,, | ,, | 24479:3 | 7 4083:767 | ,, | ,, | 244803 | 5 | 6 | 4077°876 | 4077:883 |] ,, | ,, | 24515-6d 14 4073920 | ,, | , | 245395 7| 9| 4071-903 | 4071-904 | ,, | ,, | 24551-6d 7| 7 | 4063755 | 4063-756 | ., | ., | 24600-90 8 4062602 | ,, | ,, | 24607:9 13 4055°701 | ,, | ,, | 24649°7 13 4048-893 | 1:11) 7-:0| 246911 “9 4047-373 » | oy | 247004 | 7| 7 | 4045975 | 4045-975 | ,, | ,, | 247089 2} 2] 4044-301 | 4044-293] ,, | ,, | 24719-20 4035°88 | 4035°38 | ,, | ,, | 24770°7 | 3| 4] 4034-642 | 4034-641 | ,, | ,, | 24778-20) 3] 4 | 4033-230} 4033-225 | ,, | ,, | 24787-10 3} 4] 4030919 | 4030-914 | ,, | ,, |24801-30' 10 4029:796 | ,, | ,, | 248081 a 4016578 | ,, | ,, | 24889:8 | 3 4005°305 |1:10| ,, | 24959-9 9 4003:916 | ,, | ,, | 249685 } Cobalt line measured. § Seven or éight lines, the brightest and most of the others due to Fe. 286 REPORT—1895. TABLE OF STANDARD WAVE-LENGTHS—continued. Intensity Reduction g and dj Weight Wave-lengths to Sie Character| Bind Vacuo | 33% Element of | aos 3 Standard | ‘oot In | In In | In In Are In Sin | eae Are | Sun Arc | Sun (a) (b) Carel ire i) Co 1] 2 Mn 4 to II. 4 3987-216 | 1-10] 7-1 | 25073-0 ? aay & z \ mm 9 3986-903 | ,, | » | 250750 a 2 lo { Ill. 9 3984-078 | ,, | 5, | 250928 Fe-Ti 62) 4| IIL 14 3981-914 | ,, | 4, | 25106-4 Fe 6, |) 2eha tt 15 3977891 |” | ., | 95131-8 Ca* 5| 3} mM. | 1] 2| 3973-881 | 3973-835 |1:09] ,, |25157°5 Rupees ..| 0 | 4el-calh uu 3971-478 | ,, | » | 251724 7 oe M. 3970-05 "| 4 | 231815 [H] Cat .| 70r200) Mm. | 7| 6 | 3968-617 | 3968-620 | > | ,, |25190-6a AD 8 30r| 15 | M.Iv.| 7| 8 | 3961-680 | 3961-676 | » | ., |25234-75 Fe . 3,|) Socal ul 3960-429 | ,, | » | 25242-7 Fe-Ca 5,6| 6| mm. | 1] 2] 3957-228| 3987-180] * | ., |25263-40 Fe . 2} 2] IL 13 3954-001 |» | 7:2| 252836 Yt 10| 2| IL 13 3950-497 | |. | ,, | 253061 Fe | aah Fal ape 15 3950101 | ,, | 5, | 253086 Ca! 4| 2} Mm. | 1] 2| 3919-070] 3949-034 | ” | |, | 2581540 Alt . 20r} 10 | M.Iv.| 7| 7| 3944165 | 3944159 | ” | |) |95346-7 ‘Aes sap be \ mr. 15 3942-559 | ,, | ,, |25357-0 Fe-Co 4,4| 5] m0. | 1| 15] 3941-034] 3941-021 | ,, | ,, | 2536695 Fe . 8-|. 4) -eat: 8 3937-474 |” |” |95389:8 [K} Cat .| 75r\300| M. | 6] 6 | 3933-809 | 3933-809 |1°08| | |25413-4 Fe 10r| 8} M. | 1| 3] 3998-060] 3928-071 | ,, | ,, | 2545060 ? pelid wey ts } IL 12 3926123 | ,, | y | 254632 Fe . 8.|1 shnttt, 13 3925-792 | ,, | ,, | 25465-4 a - }4 Il. 15 3925345 | ,, | ,, | 254683 Ti G,| | Saeents 15 3924-669 | ,, | 5 | 254727 Fe 3| 3] IL | 11/12] 3916886] 3916-875 |» | 7 | 25528-40 Si 10r}10} M. | 4| 4| 3908-670 | 3905-666 | ., | 7°3| 25596-55 Fe sb adaamt 12 3897599 |» | ,, | 25649°5 Fe usr| 9|M.Iv.| 7] 6 | 3886-421 | 3886-427 |1:07| ., | 25723-3a eorie |: d[e TET, 12 3883-773 | ,, | ., |23740°9 peutic! . M. IV. 8 | 3883:523 | 3883548 | ” | ; | 25742-3h Cj 7|M.iv. | 5| 3] 3883-479 | 3883472 | > | ,, |25742:8a rhe I a |=. 15 3875204 | ,, | ,, |25797-7 cq 4| m. | 4| 4] 3871-527| 3871-528] ,, | ,, |25822-30 cr 3.(\) lili 8 3864-441 | | ” | 958697 Fe 10r} 10 | Mm. Iv. | 2| 3] 3860-050] 3860-048 | ” | ” |25899-10 He) 9] Teel 7a) Sar ily 3856°517 |1:06) |, | 259228 Sate | | A slop BROT OE, 8 3843-406 | ,, | ., |26011°3 Fe. .| a| 7| M. | 1{| 2] 3840589] 3840584 | » | ;. |26030-40 Mg. .[40r|/ 20] M. 2 3838-430 |» |. | 26045-0 * Red component of double ; the violet component is due to Fe. + Solar line doubly reversed. { Red component of triplet. § Edge of first head of cyanogen band (7). || First line of first head of cyanogen band (7). { Second head of cyanogen band (7). . ** One of the lines in cyanogen band. ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 287 TABLE OF STANDARD WAVE-LENGTHS—continued. * Central line of symmetrical group. Intensity and Weight Wave-lengths Character} Kind of Element Stavdard ; In | In In | In In Arc In Sun Are | Sun Arc | Sun (a) (b) OF. 5 | M.IV. 1 1 | 3836°638 | 3836°652 27-C . 4 III. 8 3836226 Mg. 30r| 10 M. 2 3832°446 Mg. 20r] 8 M. 2 3829°505 Fe . 8r| 8 M. 1 | 1 | 3827:973 | 3827-973 Fe . 20r| 20 |} M. III 4 4 | 3826°024 | 3826-024 Mn (Cr) 5,lr| 5 IL. 10 3823°651 Fe . 5 | 6 Il. 10 3821°318 Fe . 30r} 30 | M. IIT 4 | 41] 3820°566 | 3820°567 Fe 20r} 20 | M. III 4} 3 | 3815-984 | 3815-985 Fe-Di 4,71 6 I. 15 3805°487 Fe 2) 3 I. 15 3804153 Fe 8/ 8 Ill. 2 3799-698 Fe 7| 7 III. 2 3798°662 Fe 8| 8 M. 3 | 4] 3795:148 | 3795°150 Fe-Cr ye III. 15 3794014 Fe 7r| 8 | M.III. | 3} 3 | 8788-029 | 3788-032 Ni 10r| 6 III. 15 3783°674 Fe ale IL. 15 3781°330 ? 4 II. 15 3780°846 Th 40r M. 1 37765 :°869 Yt? 6 | 3|M.III 1| 1 | 3774478 | 3774-480 Fe 3] 4 III. 12 37707130 Fe 7r} 8 | M. III 9 | 8 | 3767:342 | 3767-344 Fe 9r| 10 M. 9 | 8 | 3763-939 | 3763-942 Fe l5r| 15 | M. IIL 8 | 7 | 3758°380 | 3758-379 Fe 2] 2 II. 12 3756°211 ; I aaa 12 3754664 Fe . 20r| 20 | M. III. 7| 8 | 8749°633 | 3749-633 Fe . 10r} 10 | M. III 7/1 8 | 3748410 | 3748-409 Mg ai }7| I | 1] 9] s7erose | 3747-095 Fe Onn M. 6 | 5 | 3746:048 | 3746-054 Fe . 10 | 10 M. 8 | 6 | 3745:708 | 3745-701 Cr 3 | 2 | Fe ¥ 5] 6 | M.IIL) 4) 2 | 3743506 | 3743-502 Ti Se] 2h! Fe . 25r| 30 | M. III. | 7 | 8 | 3737-280 | 3737-282 Ca 4r M.IV. | 2} 3 | 8737:081 | 3737-075 = alate 2 3736-969 Fe . 40r| 50 | M. III 8 | 7 | 3735:012 | 3735-014 Fe . 6r} 7 | M. III 5 | 3 | 3733:-467 | 3733-467 Fe . 5 5 I. 1 | 15 | 3732°549 | 3732°542 Fe . aril 7 M. 5 | 3 | 3727-768 | 3727-763 | t a 10] M. IIT. | 7] 5 | 3722°712 | 3722-691 Fe . 40r| 50 | M. III. | 11 | 10 | 3720:082 | 3720-086 Fe . a i 1 | 12 | 3716601 | 3716°585 Yt 10r} 3 | M.III. 1] 11] 3710-442 | 3710438 Reduction to Vacuo fe. A+ A 1:06} 7°3 Oscillation Frequency in Vacuo 26057°10 26060:0 26085°7 26105°7 261162 26129-4 26145°7 26161°7 26166°85 26198-2a 26270°4 26279°7 26310°5 263177 26342:0b 26349°9 26391°50 26421-9 26438°3 26441°7 264766 26486°30 26516'8 26536:4a 26560-4a 26599°7a 26615°1 26626:0 26661°8 2667050 26679°86 26687-3a 26689°7a 26705:4a 26749-9b 26751:40 26752:2 26766-la 26777°3 26783°9b 26818'la 26854:5a 26873°5a 26898'8b 26943°46 } Iron line measured. 288 REPORT—1895. TABLE oF STANDARD WAVE-LENGTHS—continued. |Intensity | |Reduction A aud Weight Wave-lengths to 5 (x Character! Kind of Vacuoo | $eg Element |__| Standard = G6 | | xs) ahs: In | In In | In In Are In Sun |, 1_i6s are Sun) Are | Sun (a) (b) A ool | | | | | Fe 10r} 10 | M. IV. 6 | 4 | 3709395 | 3709-397 | 1-03) 7-6 | 26951-0a Fe 5 | 5 i 1 | 11 | 3707-201 | 3707:186 | ,, | ,, |26967-00 Fe* 72) el MeL, 7 | 5 | 3705°715 | 3705-711 | ,, | », | 26977-7a Fe 5 |)-5 if 1 | 11 | 3695-208 | 3695°194 | 1:2) ,, | 27054-6d Yt 3] M. IIT 1 | 1 | 3694-351 | 3694-349 | ,, | ,, |27060°80 Fe 10r} 8 | M.III.} 8 6 | 3687-609 | 3687607 | ,, » |271102¢ Fe 5 | 6 ig 1 | 14 | 3684-268 | 3684259 | ,, | ,, | 2713495 Pb Or) a AEF eS 3683°622 » | (7 | 2713895 Va 4 Fe t 3 | 6 I. | 1] 13] 3683-209 | 3683202 | , | . | 2714265 Co J 9 Fe . 8r| 8} M.III.| 8 | 7] 3680-064 | 3680-064 | ,, | ,, | 27165:7 Fe 4 5 3 I. | 13 3667°397 ” ” 27259°6 és | a} Sl iapebect wrecks 3658688 | ., | ,, | 273245 meh; lor] 4] M.II. | 2/ 7 | 3653-639 | 3653-639 | 1:01) ,, | 273623 Co 5 3 I. 5 3652-692 | ,, » | 27369°4 Heys, 10r} 10 | M. III. | 10 | 11 | 3647-995 | 3647-995 | ,, | » | 274046 23 } male |s M.I. | 1] 14| 3640545 | 3640-536 | ,, | ,, | 2746085 Pbt . a) Oo le M. 4 3639°728 » | » | 274669 Fe -| 5] 5] M.IV. | 1] 1 | 3638-454 | 3638-435 | ,, | 7:8 | 27476:65 Ti 1dr} 3) M. II 3 1 | 3635°615 | 3635°616 | ,, », | 27497-9a Vitis 5 3 M. 1 1 | 3633-277 | 3633-259 | ,, » | 2751575 Fe . 20r| 20 | M. IV. | 11 | 10 | 3631-616 | 3631-619 | ,, | », |27528.2a Yt 3 2 | M. III 1 1 | 3628°853 | 3628°853 | ,, » | 27549°1 Fe 2\"3 I 10 3623-603 | ,, | 5, | 27589°1 Fe 4 4 M.J. | 11] 14] 3623-338 | 3623-332 | ,, » | 275911 Fe 4) 4] M.IV.| 2); 3 3622-161 | 3622-147 | ,, | ,, | 2760016 Fe 4 4M. III 2 2 | 3621:616 | 3621°606 | ,, » | 27604°3 Yt. 3 1 M. 1 1 | 3621:096 | 3621-122 | ,, », | 2760800 Fe . 20r) 20 | M. IV. | 11 | 10 | 3618-922 | 3618:924| ,, | ,, | 27624-7a ae A *| 3) tury.) 1} 1] 3617-939 | 3617-920 |1-00| ,, | 2763240 Fe Aik IV. 1 | 15 | 3612-237 | 3612:217 | ,, | ,, | 27676:0d Yt Teed i 1} 1] 3611:196 | 3611:193 | ,, | ,, | 27683°90 Fe 15r| 15 | M. III. | 11 | 10 | 3609-015 | 3609-015 | ,, » | 27700°6 Fe§ 4 6 M. 2 2 | 3606°836 | 3606°831 | ,, » | 27717-46 Fe 56] 7] M.IV. | 2] 2] 3605:621 | 3605635 | ,, | ,, .| 2772665 Cr. 1dr} 4 | M.IV 1} 2] 3605-497 | 3605-483 | ,, | ,, | 27727-76 Witer: 6 2 | M. IIL 1 1 | 3602-065 | 3602-061 | ,, » | 2775410 Yt (Fe) 102} 4) M.I. 1{ 1] 3600-884 | 3600-880 | ,, | ,, | 27763°2b Ree 5| 4 ole 12 SHIT 92 Fle sy cea C|l 3 M. 7 3590°523 » | 7:9 | 278432 Ore es : 2 M. 2 3686°041 » | 9» | 278780 Cq . leh ae M. 8 3585-992 330 || bau eomeny Nits ae Pay |h ee M. 1| 11 3584-662 | 3584:662! ,, | ,, | 278887 * Violet component of double. fj Iron line measured. ~ Red component of double. § The solar line is a group of four; the second from the red is the brightest, and due to Fe. || First line in first head of cyanogen band. @ First line in second head of cyanogen band. ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 289 TABLE OF STANDARD WAVE-LENGTHS—continued. Wave-lengths Intensity and Weight Character| Kind of Element | Standard In | In In s, In Arc Arc} Sun Arc | Sun (a) teeta) .2.| 4 L 12 Fe . .| 30r| 40| M.IV.| 9| 6] 3581-344 Fe . 10/10| M. 1| 11 3570-412 Fe* . 20r| 20 | M. 8 | 4 3570-253 Fe 10r} 12] M. 6 | 4| 3565530 Fe} 1/1) a oly! I. 12 Fe . 9r| 8 | M.III.| 3| 4| 3558-674 Fe . 2 3 I. 7 xt... ol? ooh eed. 1| 1] 3549-147 il 4 7 6 Fe . 3 | 5 Tt: 10 Th . 20r M. 1 3529°547 Fe . br| 7] M. 6| 5 | 3521-409 7h... 40r M. 1 3519342 ea... 6r| 5 I. 10 Fet . eG) a 2| 31] 3513-981 Tis We shire id 8 ma. 71 7 il3 4 Fe . 2 3 I. 4 2 e a V4 Al bs \ mM. | 5| 4] 3497-991 Fe* . ? 5| M. 1! 1] 3497-266 ie \ fd } al pap ee 8 Fe . 10r} 10} M. 7| 3 | 3420-724 Ni. ar VB.) I n) Ni | 2 | Fe ae T 10 Co j 2 J Fe} . orl 6 Mr 5 | 2] 2476848 Fet. 10r} 10 | M. 7| 3] 3475-602 ots var it } mM. | 7/| 3| 3466-010 Sr?. 8| 3 ie 8 Co 6r| 4 2 | 10 re. Sr} 8|M.IV.| 6| 4] 3444-024 Fe . 10| 10] M.IV.| 6] 4] 3441-135 Fe 15r| 15 | M.IV. | 7| 4] 3440756 Fe*. €| 6] M. 2| 1 | 3427-279 a... 2 I. 15 Fe . ae wr |. |” 1) te: 9406-065 Fe . 4 ai 11. 1/18 | 3406-602 Gt ane 1 I. | 1| 12 | 3405255 ee : A) ie 1 | 12} 3389-913 i 5 3 | mi | 5| 3 } Zr 4 1 I. 8 | - ll ae 9 e 3 eS | crt eee } I, 9 * Red component of double. ‘peti line of a group of six. In Sun (b) 3583°483 3581344 3570°402 3570°225 3565°528 3564°680 3558°670 3550-006 3549°145 3545°333 3540°266 3521-404 3518°487 3513-947 3510-987 3500 993 3500721 3197-991 3497:264 3491-464 3490°721 3486°036 3478-001 3476°831 3475594 3465°991 3464°609 3455384 3444-032 3441135 3410°759 3427°282 3425721 3406-955 3406°581 3405272 3389°887 3377667 3356°222 3351 877 3348-011 Reduction Oscillation Frequercy in Vacuo 27897°9 27914°6 28000:26 28001-3a 28038"4a 28045°1 28092°5d 28161:0 28167°8b 281981 28238°5 28324:3 28389'7a 28406°4 28413:3 28450:0b 28474:0 28555°2 28557°5 28579°7 28585:7b 28633°2 28639'3a 28677'8 287441 28753-6a 287639a 28843-4a 28855°1 28932:1 29027-6a 29052:0 29055 2a 29169:4a 29182°6 29343-40 29346°6D 29357°9b 29491:10 29597°8 29786°9 29825°5 29860°0 + Violet component of double. § Iron line measured, 1) 290 Element REPORT —1895. TABLH OF STANDARD WAVE-LENGTHS—continued. Intensity and Character! Kind of ' Standard In | In Arc} Sun 2 2 JUG 5 5 r. 3,6) 4 3 1 I. 10 70) we (el 10 ia NEAL 3 3 II. 10r} 5 |} M.IV. or Poo Ni 1. 3,2) 4 lip 4,7 A bs I. 6 5 I. a0rl PGi Dla. 10 4 | i 1 3 Gu | 4|J 40r} 9 | M.IV. 6 re l1or| 8 M. 6 4 Ill. : }s I. 8 8 M. 6 4 I. ? th 6 5 M. III.! 6 } IT; 6 Ta; 4 3 if. 5 5 M. LOx|. v4) MST. 3 3 M. 4 4 TI. 1 1 ie 5 Te ik dul 8 M. 2 II. 3 TI. 4 2 UE 10r} 8 M. 3 1 ile 7 5 iis 2 T. 3 II. 2 ILL. 10r! 6 M. Weight In | In Arc} 8un 8 10 10 1 5 ii 5 10 | it 6 1 6 9 10 9 | 15 5 10 10 U5) 5 12 i i ue | 12 1 3) 1 3 3 1 1 | 1| 6 | 1 1 5 1 1 5 5 1 5 1 1 3) 5 3 1 5 9 3 real u 3 Wave-lengths In Arc (a) In Sun (») Reduction to Vacuo ES A 3306°481 3306:119 3303°119 33027504 3274-090 | 3247-671 3236°696 3225°907 3222°197 3214152 3200:040 3195°729 3158-994 3134:223 3101:994 | 3331-741 33187163 3308-928 3306471 3306 117 3303-648 3303°107 3302501 3295°957 3292°174 3287-791 3274-002 3267°839 3260-384 3247-680 3246°124 3236°697 3232-404 3231-421 3225923 3224°368 3222-203 3219-909 3219-697 3218390 3200-032 3195-702 3188164 3176104 3172175 3167290 3158:988 3153°870 3140°869 3137-441 3129-882 3191-275 3115°160 | 8109-434 3106677 0°93) 8°5 » | 86 ” |o-87| * Second line from violet side of a group of four. + Second line from red side of a group of five. Oscillation uency in acuo ct 30005:8 30128°6 302127 30235°1d 30238°4d 30261:0 30265:9u 30271°56 30331°6 30366°5 304069 30534:la 30592°6 30662°5 30782°5a 30797 2 30886:°9d 30927'9 30937°3 30990:2a 31005:2 31025-9a 31048-0 31050:0 31062°6 31103°5 31240°83 31283:18 31357°1 3147671 3151571 31563°7 31646°70 31698°1 31829 2 318640 31896°7 319410 320291 32092:0 321510 32180°5 322281 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Element TABLE OF STANDARD WAVE-LENGTHS—continued. 291 Intensity Reduction q and Weight Wave-lengths to Bice ll Character} Kind of Vacuo s S a | Standard eis In | In In | In In Are In Sun | qa ia 2s” Are | Sun Are | Sun (a) (b) nN oa) 20r| 8 M. 3 3101:673 0:87! 9:2 | 32931°5 6] 6 M. 3 3100:779 » | 99 | 32240°8 42 | 4 M. 3 3100-415 | oy | 322445 a 7 M. 3 3100:064 Shan lpeesoes pe) Sql ORE 9 3095-003 | ,, | 5» | 3280079 } 2 ie 9 3094-739 | 4, | 5» | 323037 4 2 M. 8 30927962 ” ” 32322°3 | 20r| 10 M. 15 3092°824 |) | Seb eaed Sr} 8 M. 1 3088-137 spall 52372'8 | 4 1s 1 3086891 | ,, | 4, | 32385°9 6r| 7 M. 5 3083°849 yy | 9:3 | B2417°7 | 20r| 7 M. 17 3082272 tulle 32434°3 | 5 I. 1 3080:863 | ,, | 4, | 32449-1 Til 2 I. 1 3079°724 | ,,| 4, | 324611 4 6 M. 3 3078°759 ” ” 32471°3 4 I. 6 3078148 | ,, | ,, | 32477°8 4| IIL. 6 3077'303 | ,, | ,, | 32486°7 2 M. 1 3077°216 | 99 | 32487°6 10r| 10 M. 4 3075°849 » | 9 | 82502-0 6 | 8 M. 3 3075°339 » | 3 | 32507-4 10r| 10 M. 10 3067:363 » | as | 32592°0 sr} 3] M.L. 1! 5 | 3061-932 | 3061:930 | 0:86] ,, | 32649°8b 3 II. 1 3061:098 | ,, | ,, | 32658°7 10r| 10 M. 15 3059-200 » | | 326790 10r| 10 M. 8 3057°557 » | 9 | B2696°6 5 I. 5 3055°821 | ,, | 4, | 32715-1 : } II. 1 3053'527 | ,, | 94|32739°6 | 3 Til 5 3053173 | ,, | 4, | 327434 | } I. 5 3050:212 | | » | 327752 | | 20r} 20 M. 13 3047-720 » | 9» | 32802-0 IL. 1 3046:778 | ,, | yy | 328122 | | 10r| 3 II. 5 3044:683 | ,, | ,, | 328347 lier} 4|/ M.Iv.|] 3| 2| 3044114] 3044119 | ,, | ,, | 32840-9a lar] 15 M. 10 | 2 3037°505 | 2037-492 | ,, | ,, | 32912-4a | Bel Tie 7 3035°850 | ,, | 4, | 82930°3 | M. 1 3027-245 » | ay | B3023:9 | 10r| 10 M. 7 3025-958 yy | ay | 330380 4 Il. a hes 3025°394 | ,, |, | 3304471 5 IL. T 3024-475 | ,, | 9°5| 330541 aes b M. % 3024:154 ” ” 33057°6 15r M. 18 3021°191 0°85} ,, | 33090-0 25r | M. 18 3020°759 | a | 330948 lor! M. 15 3020°611 » | 9) | 83096'4 M. 1 3019-752 oy |g | BBLOBB 5 | M. 1 3019108 S| yy | BBLL29 5 M. 1 3017-747 4 | Seu 3 M. 1 3016:296 » | oy | BB1437 6 IV. 4 3014-274 | ,, | ,, | 33166°0 Ae) TV. 5 3012°557 | ,,| ,, 331849 4r M. 3 3009°696 pol | 3216-4 Tr M. 3 3009-327 | » |» | 882205 6r M. 15 3008-255 | ‘yll> ap baawag:4 U2 292 REPORT— 1895. TABLE OF STANDARD WAVE-LENGTHS—continued. Intensity and Weight Wave lengtts Character) Kind of Element | Standard | = = zee In | Io In | In In Are In Sun Arc| San Are | Sun (a) (b) Fe 1 M. 3 3007-408 Fe 2 M. 1 3007°260 Ca 15r M. 3 3006978 2 4 IIT. 1 3005°404 ? 3 7) + a 3005°160 Fe 8r M. | 15 3001-070 Ca 8r 1 ey 83 3000°976 Ca 6r M. 3 2999-767 Fe 4r M. 5 2999-632 Ca 10r M. 3 2997:°430 Ca Tr M. 3 2995074 Fe &r M. 18 2994°547 Si 4 M. 5 2987°766 Fe M. 1 2987°410 Fe 10r M. | 15 2983°689 Fe 2 Me t) 6 2981°570 Fe 12r M. | 15 2973°358 Fe 6r M. % 2973°254 Fe 4r M.~ FlGRa 2970°223 Fe 8r M. | 12 2967:016 Fe M. 1 2966°985 Fe 5 M. 3 2965°381 Fe 5 M. 3 2957°485 Fe Tr M. 4 2954:058 Fe 8r M. 4 2947:993 Fe 10r M. 4 2937:020 Fe 8r M. 3 2929°127 Fe 7r Met! 63 2912°275 Si 15 M. 12 2881°695 Mg 100r M. | 15 2852°239 Fe 6 iM. 41 6 2851°904 Fe 5 M. i 2844-085 Fe 3 M. 1 2843°744 Fe 3 M. 1 2838°226 Fe 4 Mis Liped 2832°545 Fe 5 M. 1 2825°667 Fe 3 M. 1 2823-389 Fe 5 M. 3 2813°388 Mg 20r M. 10 2802°805 Mn M. 3 2801°183 Mn M. 3 2798°369 Mg | 20r M. 12 2795°632 Mn M. 3 2794911 Fe M. 3 2788°201 Mg* Sr M. 5 2783:077 Fe M. 1 2781°945 Meg* br M. 5 2781°521 Meg* 8r M. 5 2779°935 Mg* 5r M. 3 2778381 Fe M. 2 2778340 Mg* 5r M. 5 2776:798 Fe M. 2 2772:206 Reduce ion to | Vacuo Oscillation Frequency in Vacuo | | —9°5| 332417 » | oo 33243°4 | 33246°5 332639 33266°6 33312°0 33313°0 33326°4 » | 333279 3 | 33352°3 » | 33378°6 333844 »y | 83460°2 33464:2 »» | 33506:0 33529°8 33622°4 33623°6 33657°8 33694°2 33694°6 337128 33802°8 33842-0 » | Bool l7 34038°3 341301 343275 34691°8 35050°1 350542 351505 35154:7 ” ” 35223°1 35293°7 35408'1 355340 35668'2 35688'9 357247 857597 35768'9 358550 35921°1 35935°7 I » | 35941°2 359617 35981'8 35982'3 | 7 | 360023 '10°5 | 36061°9 | S3ge)) 99 \ 5 * A remarkable symmetrical group of five Mg. lines. a? ON WAVE LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS, 293 TABLE OF STANDARD WAVE-LENGTHS—continued. Element 2 1/10 .} 10 Intensity and Character In | In Are Sun) or cr 10 Reduction Weight Wave-lengths to = B32 Kind of | Vacuo | $89 Standard | - seb | | oo In| In| In Are InSun |,,/1_| 528 Are | Sun (a) (b) A M. 2 2767-630 0°79,10°5 | 361215 M. 2 2762110 » | a | 361937 M. 2 2761876 » | x» | 3861968 M. 3 2756°427 » | 99 | 86268-4 M. 2 2755'837 || pao Boz Reel M. 3 2750:237 »» 10°6 | 36349:9 M. 3 2742485 » |» | 36452°7 M. 3 2737°405 0:78} ,, | 36520°3 M. 3 2733673 » | + | 365702 M. 3 2723:668 » |L0°7 | 36704:5 M. 1 2721-762 » | x9 | 36730:2 M. 3 2720°989 » | 9 | 36740°6 M. 3 2719119 |) ae | 86765°9 M. 2 2706°684 » | sy | 369349 M. 3 2679148 0:7710°9 | 373144 M. 7 2631:392 0°76 11:1 | 37991°6 M. 3 2631125 » |» | BT995'S M. 2 2611-965 a | sy | 382743 M. 3 2599:494 | 0°75 11-2 | 38457°8 M. 2 2598-460 lL, a> [eess | BOATSEL M. 2 | 2593:810 te So fh fteat | BB oaeel M. 2 2585963 | ,, |11:3 | 38659°0 M. p 2584-629 » | 9) | 38679°0 M. 2 2576-195 ys |» | 88805°6 M. 5 2575198 fe 1) sy | BSB2O7 M. 5 2568-085 ., 11-4 | 389281 M. 2 2549°704 0-74} ,, | 39208-8 M. 3 2546-068 | |, (11-5 | 39264-8 M. 3 2541 058 ” ” 39342°2 M. 2 2536°648 » | 9 | 39410°6 M. 3 2535-699 » | oy | 394254 M. 5 2528'599 », 11'6 | 39536-0° M. 3 2527-530 1 Awl Gr PROBB2 7 M. | 10 2524-206 | | a» |89604:8 M. 3 2522-948 | 1. | yy | 396246 M. | 10 2519:297 | 4, | 9» | 39682°0 M. 3 2518'188 |, | 4, | 39699°5 M. 7 2516210 10:73! ,, | 39730°7 M. | 10 2514-417 | 4. | 9 | 897591 M. 3 2510°934 | » (11-7 | 39814-1 M. | 15 2506°994 » | » | 398767 M. 3 2501-223 | |, | a | 39968-7 M. | 20 2497°821 | sy |» |40028-2 M. | 20 2496:867 het. | 40088*5 M. 3 2491244 | ,, {11-8 | 40128:8 M. 3 2490°723 Yt ys | 401872 M. 3 2489-838 » | gy | 401515 M. 3 2488-238 . | Paola M. 3 2484-283 » | gy | 40241°3 M. 3 2483359 » | 9 | 40256:2 M. 3 2479°871 | 4, |» | 40812°9 M. | 15 2478:661 » | ss | 40332°6 M. 3 2472974 ». |11°9 | 40425-2 M. 3 2462-743 0:72| ,, | 405932 294. REPORT—1895, TABLE OF STANDARD WAVE-LENGTHS—continued. Intensity Reduction q 2 and Weight Wayve-lengths to Se, Character | Kind of Vacuo | 2&3 LBV op S| Serie il ee & eR In, In In | In In Arc In Sun At tS = Are | Sun Arc! Sun (a) (b) r al eos M. 3M 2457°680 0:72\12'0 | 40676'8 | Si. 3 M. | 10 2452°219 » | 1 | 407674 Fel. M. 3 | 2447-785 » | a | 408413 Siu 3 M. 10 2443°460 » |12°1 | 40913°5 Si 3) M. 10 2438°864 on » | 40990°6 Slice 8 M. 15 2435°247 » »» | 41051°5 Fe . M 2 2410°604 0°71)12°3 | 414711 | Fe . 4 M. 2 2406°743 AA » | 41537°6 Fe . 4 M. 2 2404-971 #5 », | 41568°2 Fe M. 2 Ppt spe} “a », | 41666°0 Gar >; 25r| M. 5 2398-667 2 », | 416775 Fe?. M. 3 2395-715 » (12-4| 41728°8 Fe . M. 2 2388:710 * » | 41851:2 Fe?. M. 3 2382°122 ,», |12°5 | 41966'9 Fe . . M. 2 2373771 0-70) ,, |42114°6 OA Niece 5 7 M. 3 2373°213 ., », | 42124°5 PATiay= : 6 M. 3 2367:144 » |12°6 | 42232°4 Fe M. 2 2364897 i »y | 422726 Fe M. 2 2348°385 », |12°7 | 42569'8 ile); ; M. 2 2343°571 ” », | 426564 Ba. . | 20r M. 1 2335°267 y» |12°8 | 428089 ane Pi 20r M. 1 2304364 0°69)13:0 | 48382°9 Fe?. : M. 2 2298-246 » |13°1 | 43498°3 Caves . | 20r M. 3 2275°602 0°68.13°3 | 48931:1 Sr 10r M. 1 2275'376 |» | 439855 Al 4 M. 2 2269-7161 * » | 44055'8 Al 3 M. 2 2263-507 “4 » | 44165°9 Si 2 M. 2 2218:146 0:67/13°7 | 45069:0 Si 4 M. 2 2216°760 . » | 45097:2 Si 2 M. 2 2211-759 », |18°8 | 45199-1 Si 3 M. 2 2210939 | ap | SO2 Los Si 2 M. 2 2208-060 - » | 452748 | [Sion rae ; 3 M. 1 2165'990 0°66 14:2 | 46154°1 Siti. 3 2 M. 1 2152°912 yy [14:3 | 46434-4 EXPLANATORY Notre.—The first column gives the symbol of the element whose wave-length has been measured, e.g. O signifies oxygen, wv water-vapour, &c. If a letter stands at the left within brackets: thus, [A] [C], it is the ‘name’ of the line in the solar spectrum. A mark of interrogation after the symbol means that it is doubtful if the line is really due to that element. Two symbols on the same line (e.g. Mn Di, 3295-957) signify that these two elements have apparently coincident Mn lines as their wave-length. Two or more symbols bracketed (e.g. Si } s260a Fe mean that the first has a line coinciding with one side of the corresponding solar line, the second with the middle, &c. A mark of interrogation alone signifies that the chemical origin of the line is unknown. ‘The fifth and sixth columns give the ‘weights’ to be attached to the lines as standards in the arc and solar spectrum respectively. The fourth column gives the character of the standard. M. meansa standard in the arc spectrum; I. a remarkably good standard in the solar spectrum ; II. a good solar standard ; III. an ordinary solar standard; and IV. a rather poor solar standard. Columns 7 and 8 give the wave-lengths in air at about 20° C. and 760 mm. Lines marked with two dashes are double: thus 6’’, r signifies reversed. ON WAVE-LENGTH TABLES.OF THE SPECTRA OF THE ELEMENTS. 295 Wave- length T6161-2 6154-6 *+5896-2 *+5890°2 $5688°3 +5682°9 +5675°9 5670'4 $5153-7 5149-2 $4983'5 $4979°3 4752-2 47484 +4669-4 +4665°2 4581-7 4573°6 4570°4 4565-2 4555°7 4546-0 $4542'8 4539°0 +4500-0 444943 4393-7 4390-7 3533°8 $3303-1 *+3302°5 Soprum (Spark SPECTRUM). Eder and Valenta: ‘Denkschr., Wien,’ Bd. Ixi. 1894. Reduction] s {iu | 247192 | #432175 2§ wo | ae | are 4040°2 1 » | 9» | 24744:2]] 3209-0 Is » | 89) 31153°5 4026-0 1 » | » | 24881°6|| 320271 Is ot: su eple20:6 4018'8 In » | » | 248760] 31902 | 2n Pipes eye 40123 2 1:10] ,, | 24916:4|| 3169-2 Is 0°89 | 9:0} 31544-7 4001-2 6s » | 71] 24985:4|| 81575 | | Is » | » | 81661-6 3995-0 Is » | 9 | 25024°2|| 3143-7 3s » | 9'1| 31800°6 3972°6 3s 1:09| ,, | 26165:3|| 3129°3 4s | 0'88| ,, | 31946°9 39667 4s » | + | 25202°8|) 3104-5 5n » | 92| 32202-1 3955°3 4s » | 72) 25275°3 || 431023 In jo | Gayl Be Beeae 3943°3 2s 9 ole avy (28352°3 || 20746 In | 0:87) 9:3] 32515:3 3984-7 Is 1-08| ,, | 25407-7 |) 30673 | In a. | 5s | OT 3927-0 1s » | 9 | 25457°5 || 3062-4 6s | 0-86) ,, | 32644-8| 3923°8 Is ae asl 25478'3) | S056 Lie In a 1 35 3898-1 8s » | 73| 25646-2|| 3051-5 | In » | 94| 827614 3884-2 Is DOF 55 | 2573870)! = 3030:0mu en ia oe he 4g eSB -9 3879-2 1s si. |) s9° DST TB S0R8O In | 0:85| 95} 330702! 3874-1 2s a» | a | 258051) 42992:3 4s » | 9°6| 33409°5 3862°3 Is » | » | 2588401] 29860 | | Im | | -,, |44,0ltads00 3818-5 In 106] ,, | 26181:0|] 2938-7 In | 0:83] 98] 34018:8 3800-8 1s 1:05 | 7-4} 263028 || 2853-5 In 0°81 10-1 | 35034-6: 3783-2 338 » | » | -26425:2)) 2833:0 |. 2n | ,, {10:2 852881 3767-1 Is 1:04| 7°5| 26538-1|| 28190 | 1 | 080j\10°3| 35463:3 3757-4 1s » | » | 266066|| 27805 | J 0-79 10-4) 359544 8749) Is » | » | 26665°6|| 27362 In | 0-78 10°6 | 36536-4 37445 1 » | 9 | 266983 || 2690-4 ia || 077 {108 37158°4 3739-2 In Petia, HasOTaGs2i| EGR". Ale a » |10°9| 37547°8 3727°5 In | 1:03] 76! 26820':0|| 26353 | 1 | 0°76 /11°0| 379353 \ § Probably double. ——— S CUT ll ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 297 POTASSIUM (SPARK SPHCTRUM)—continued. t Occurs also in the Arc Spectrum. See Report 1892. Reduction Eb Reduction E bo Wave. _ | Intensity to Vacuum a 5 S see: Intensity to Vacuum = g 3 length ani = ce || length an Boe s Character) 4 + <- Gna Character| ) + i= ae eS 2614:0 1 0:76 |11-1| 38244-4 2274°4 In 0°68 |13°3 | 43954°3 2549-4 2s 0°74 |11-4| 39213°5 || 2268-1 In rs », | 44076°5 2440°9 1 0:72 |12:1| 40956°4 || 2261°8 1 yy \13°4] 44199°2 2379°5 1 0°71 |12°5 | 4201371 || 2258°3 1 3 » | 4£4267°7 2358-9 In 0°70 |126 | 42380-0 22549 1 “y » | 44334°5 23504 In yy {12-7} 42533°2 2248-4 1 », |13°5| 44462°6 2344-7 In ‘A », | 42636°7 2243°5 1 " » | 44559°7 2341-7 In i » | 42691°3 2203°9 1 0°67 |13°8 | 45360°3 CapMium (SPARK SPECTRUM). Eder and Valenta: ‘ Denkschr., Wien.’ Bd. Ixi. 1894. =. | Reduction =) Reduction q S |to Vacuum 8 S 3 s $ | to Vacuum 8 eg No.| Wave | 23 e222 |. | Wave- | 28 eo . A = 5 | No. “rt By os length as 1 3 oe | length aS 1 a2 Je . 4 pies Eres 64674] 2s | 1:76) 4:2) 154580) 4693:'7| 2s | 1:29] 5:9} 21299-2 1 6439°3| 10s | 1:75) ,, | 15525:-4| 6 | t4678:-4| 10s | 1:28] ,, | 21368-9 6057'7| 2s | 165} 45) 16503°4 $4662'7| 3s » | oy | 21440°9 6004-7} 2s | 1:63] ,, | 16649-1 | 46465} Is | 1:27) ,, | 21515:7 5958°7) 2s | 1:62] 4:6} 167776 46348] Is » | 60] 21569°9 5914-1} 2s | 161) ,, | 169041) 4631°3} Is # » | 21586°2 5791-1) 2s | 1°58) 4:7) 17263:2 4600'0| In | 1:26] ,, | 21733:1 5688:2| 4s | 1:55) 4:8) 17575-4 || 4581:9| Is ” », | 21819:0 5663°6| Is | 1:54] ,, | 17651°8 || 4541°6| Is | 1:24) 61} 220126 5640°6| Is rs » | 177238 | 4521:4| Is a +» | 221109 56116; Is | 153] ,, | 17815-4)}) 44913} Is | 1:23] 6:2} 222591 6490°'2| 6s | 1:50} 5:0} 18209°3 || 4487°8| 1s + » | 222764 5472°5| 6s | 1:49] ,, | 18268-2 44434] 2s | 1:22] ,, | 22499-1 53911) 2s | 1:47) 5:1) 18544:0|| 7 | f4415°9} 10s | 1:21] 6:3} 226891 2 5379°3| 10s x » | 18584:7 $4413:2| 2 ny » | 22653:0: 3 53386] 10s | 1:46] ,, | 18726:4)) 4403°5| 1 # »» | 22702:9) 5308'2| 1s | 1:45] ,, | 18833°7 | 4393°5| 1 1:20] ,, | 227546 5305°1| 3s - », | 18844°7 42939} 2s | 1:18] ,, | 22752°5 5203'9| Is » | 53} 1921-1 || 4272°9| 3s | 1:17] 6:5) 233968, 5174:3) 38s | 1:41] ,, | 19321:0 4271:2| 3s zs » | 2840671 61552} Is - » | 19392°6 | 4245°8| 4s » | 66] 23546:1 4 | +5086:1| 10s | 1:39] 5:4} 19656-0 | 42266} In | 1:16] ,, | 23653-1 5026°5| 1s | 1:37] 5°5| 19889-1 | 42171] 6s # » | 23706°4 4854°7| 2s. | 1:33) 5:7} 20592°9 | 4214:0} 2s ¢ » | 237238 5 | $4800-1] 10s | 1:31] ,, | 20827-2| 4191°8| 4s | 1:15}| 6:7) 23849°4 47836) Is » | 58] 20899-0 | 4177'5| 2s - » | 23931°1 4707°3| 2s | 1:29] 6:9| 21237-7| 4171'6| 2s 23964°9 298 CADMIUM (SPARK SPECTRUM)—continued. No. 8d REPORT—1895. r= Reduction & 5 |to Vacuum s eg Wave- | BS weg N Wave- length | 2¢ | 1 3 Sr | length £5 [pat |=-| 64 z AT de 4163-9} 2s | 1:14) 6:7| 24009-2 | 3840°6 | 41581] 5s 7 » | 24042°7 | 3837°9 4142-1} 4s » | 68} 24135°5 3808-2 4139°8| 2s ” », | 24149-0 $3614-6 4136:9} In x », | 24165°9 || 9a! +3613-0 41343] In ” », | 2418171 || 95] 43610°7 4130°9| In | 1:13) ,, | 24201-0) 3535°8 41271) 6s 53 », | 24223°3 $3501-2 41168} 3s = » | 24283°9 3499°3 4114-7) 5s + » | 24296°3 || 10a) 43467°8 4112°8|} 1 ” » | 24307°5 || 100 | +3466:3 41026} 1 5 » | 24368°9 |) 11 | 34037 4095:0| 7s » | 69) 24413°1 T3299'1 4092°5] 3s | 1:12] ,, | 24428:0||12@| 3285°8 4083°9] 1 £ » | 24479°5|1126| 3283°6 4077-4] 1 ce » | 245185 3276°9 40758; 1 s » | 24528°-2 3264-2 40721} 1 ry » | 24550°5 $3261°2 40688; 1 ss » | 24570°4 $3252°6 4066°3| 1 se » | 24585°5 3250°5 40641] 1 i » | 24598°8 3236°4 40577} ‘5s - » | 24637°6 3221°3 40540} In | 1-11] ,, | 2466071 3217°8 40491} 3s » | 10} 24689°8 3212-0 4044-7] 3s f- » | 24716°7 3209°9 4038-6} In : » | 247541 3201°8 40351] 3s : » | 24775°5 3197°5 4029:2|} 1 at » | 24811°8 3196-2 4023°3] 1 % » | 24848-2 31854 40185} 2n + 9 | 24877-9 3182°8 40148; In | 1:10} ,, | 24900°8 31785 4009:2|} 1n F » | 24935°6 31767 40060} In £ », | 249556 §3173°8 39941] 3s » | @1| 250298 3161°6 3992-0! 4s # » | 25043-0 3157-1 39884] 5s », | 250656 3153°6 39847} 3s Fs » | 250889 3141-2 3977°8} 6s 5 » | 25182°4]/13 | F3133°3 3976°8} 6s ” », | 25138°7 3129°5 39589} Ts | 1:09] ,, | 25252°4 31248 39510} 3s » | 72] 25302°8 3122°2 3945°7| 1 + » | 253368 3119-2 3940°4| 8s RS » | 25370°9 3113°5 3935°7| 38s | 1:08] ,, | 25401-2 30959 3919°6| 4s + » | 255056 3093:0 3910°5} In 3 » | 255650 3089°3 39029] In » | 73] 256147 || 14a) 3085-4 3899-4] 2s ff » | 25637°7 ||14b | +3081-0 3889'8| 1 107] ,, | 25701:0 3077°3 3865'4| 2s ” » | 25863°2 30689 3852°3|} 4s | 1:06] ,, | 25951:2 3065°0 38482] 2s a », | 259789 3059°5 8843°8| 2s + » | 26008°6 3053-2 § Probably double. Intensity and Character Reduction | to Vacuum 1 A+ me Oscillation Frequency in Vacuo 26030°3 26048°6 26251'7 27657°8 27670:0 27687'7 282741 28553°5 28569:0 28828°5 28841:0 29371°5 30302°7 30426°3 30445°7 30507°9 30626°7 30654°9 30735°8 30755°7 30889'7 31034°6 31068°3 31124:3 311447 31223°5 31265°5 31278°2 31384°3 31410°0 314524 31470°2 31499-0 31620°5 31665°6 317008 31825°9 31906°1 31944°9 31992°9 32019°6 32050°4 32109°0 32291°6 32321°9 32360°6 32401°5 32447°7 32486°7 32575°7 32617:1 32675'8 32743°1 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 299: CapMIUM (SPARK SPECTRUM)—continued. eee B. | Redaction) >, |. | Reduction | 4 aa | £2 ito Vacuum) .2 8 3 == |to Vacuum] .- 35 | No. Wave- | £3 i 332 Il No. Wave- 2s | Bega . length _ gs ly 5 SF | length hg 1 I o r De on; PS n= ‘ 4 ey A+ re on a | i: (S) | At x Om = J | — . 3048-9, 3 | 08°6| 9-4} 32789°3 | $2633:1; In | 0°76 \11-0| 37967-0 30358) 1 es | 3203078) 2629:7| 1 » {Ll1l-1} 38016-0 30248 In »» | 9°5| 33050°5 || 26191} 2 ” » | 38169°9 3017-2) 3 0°85| ,, | 33133°8 | +2602°0| In | 0°75 )j11-2| 38420°8 . 30141; 1 » | 9 | 331679 | $2592:3| 1 9 » | 38564°6 . 3011-4) In » | » | 338197°6 25805} 1 » |11:3| 38740°9 3008'7} In 3 | 4 | 38227-4/118 | ¢2573°1} 10s ” » | 38852°3 3007°2| In » | 3 | sozde-0 72552'2| 5 O74 |11°4} 39170°5 30038; In 3 . | 33281°7 2546'5| 1 », |11°5| 39258°1 : 29962) 5n » | 9°6| 33366:0 $25449; 1 | ,, » | 39282°8 4 2987°3| 2n ” », | 38465-4 || 19 2499'9} 3 0:73 |11-7 | 39989-9 |15 | F2980°8| 10s | O84) ,, | 33538°4 2495:5| 1 ” » | 40060°4 . 29718) 2 » | 33640°0 2487:9| 3 » {11°8| 40182-7 29646) In » | 97) 33721°7 | 2478°7 |2(Cd?) sy » | 40331°9 12961°8| 2b’| ,, » | 33753°5 || 20 24700} 4 0°72 |11:9} 40473°9 29524) 2 ” » | 338610 | 24461) 2 » |12°0| 40869-4 2948'9| 4 ” » | 33901°2 | 2433°8| 1 5, {12-1} 410759 29266) J 0°83) 9°8 | 34159°5 24266) 1 » [12-2] 41197-7 2 29109) 4 » | 9:9) 34343°7 2423°9} In ” » | 41243°6 | 28937) 1 0°82 |10°0 | 34547°8 || 21 24189) 4 O71) ,, | 41328-9 $2880:'9 | 10b 3 »» | 34701°4 || 24186) 1 ” » | 41334-0 428684.) 5b | ,, |10°1| 34852:5| 2411'2| 1 »» [12:3] 41460°8 728620) 2b | O81) ,, | 349305 | 2377:0| 2 », |12°5| 42057°3 $2837-:0| 8b » |10°2| 35238°3 | 2375:0| 1 ” » | 42092°8 2834°4| 3b ‘ », | 309270°6 | 2355°4| 1 0°70 |12°6 | 42443-0 28239; 1 0°80 |10°3 | 35401-7 | 23505} 1 9 [12-7] 425314 28185) 1 i » | 35469°6 | 23435} 1 ” » | 42658°5 28055 | 2 o » | 35634-0 2333'2| 1 » |12°8| 428468 2802°7| 1 nc » | 396696 $2329'4| 7s » » | 42916°7 2795°7| 2 » |10°-4| 35758°8 || 22 | 2321-2) 8s | 0°69 /12°9| 43068°3 2780°1) 1 0:79| ,, | 35959°5 || 23 | ¢2313:0| 10b » {13:0} 43220°9 27751) 6s » {105} 36024-2 72306°7| 5s ” » | 43339-0 2773:1| In ” », | 36050°2 | $2288'1| 10sv| ,, |13°2| 43691-2 2767°2| 2 ” » | 36127-1 422675) 38s | 0°68 ]13°3| 44088:1 2764:3| 4s + » | 36165:0 || 24 | 2265-1} 10sv|_,, », | 44134°9 f2757:1; 1 » » | 36259°5 2248°7| 1 » |13°5) 44456°6 $2748°7 | 10s » {106} 36370°2 | $2239'9| 3 5 » | 44631°3 727340) 3 078} ,, | 36565°8 | 2228:1| In | 0°67 13:6) 44867-7 2726°9| 2 » |10°7| 36661:0) 22243) 3n » {13:7 | 44944°3 $2712-0 ne » | 36862°5 | 22040) Inv} ,, |13°8| 45358-2 27069} 2 BS », | 36931'9 || 25 | 72194-7| 5s », j13°9| 45550-4 {2677-7| 8 0°77 |10'9 | 37334°6 2187'9| 1 » {14:0} 45691-9 26710; 2 » | 37428%3 | 21831) 1 i » | 45792°4 26683) 2 oe » | 374661 72168°8| In | 0°66 |14:2| 46094-2 72660°5| 7 ” » | 375760 | $2144:5) Ssv} ,, |14-4| 46616°5 12639°8| 3b | 0°76 11:0, 37870-0 | 2111°6| 2sv} 0°65 j14°7 | 47342°7 Compare Hartley and Adeney’s list of Cadmium Spark Lines. Report, 1884 300 REPORT—1895. Mercury (Line Spectrum). Eder and Valenta: ‘ Denkschr., Wien,’ Bd. lxi. 1894. The lines given below all occur in the spectrum of a mercury vacuum-tube strongly heated and excited by a powerful condensed spark. Those marked * occur also on a tube on higher pressure (10 mm. to 1,000 mm.) between 180° C. and 1,00U° C. with the condensed spark. Those marked f+ occur in a highly exhausted tube between 15° C. and 80° C., with the spark without condenser. ‘Those marked § occur in the condensed spark between mercury electrodes at atmospheric pressure, and those marked || occur in the arc-spectrum. ** Probably double. @ Observed also by Vogel, Wied. Ann. v. 500. Reduction to ’ : Vacuum ne ica me ty Previous Measurements | —____ Pa (Rowland) | Character (Angstrom) ae ie in Vacuo A 6363°5 2*§ 6360 Huggins 173 | 4:3 157103 6152°3 9*S 6151-2 Thalén 167 | 44 16249°7 5889°1 8*§ DSsoa Fe,, 160 | 46 16975°9 5880°5 2 5 s 17000°8 5872°1 8*S Bolt) " a 1702571 5864-4 2 Se lp bards 170474 5854°5 1b | 1:59 ss 17076°3 5840°6 1 ees " 171169 5834-0 3 » AT | 17136°2 5819°1 4*§]| 56817 Huggins Ngee eran | 17180:1 5804°3 10*f|| 5800 iD 1358 |) 6) 17223°9 5790°5 2*t§ || 5789°6 Thalén 9» . 17265-0 5781°9 1 x 3 172906 5769°5 10*f§|| 57681, 157 a 17327'8 57466 3 to 3 wi 17396°9 5727-7 5 1:56 Bs 17454:3 5717-0 1 5 4:8 174869 5713-4 2 | - i 17497°9 5699-0 3 1:55 a 17542°1 5695°7 1 4 a 175523 5679-1 10*§ pGTSel 7; ra 17603°6 5665'8 3 154 53 176450 5662°5 3 : i 17655:2 5637°8 7* i if 177326 5596-0 8*S Boo Serle 153 | 49 178650 55879 2 1:52 a || 17890°9 5576°2 3 ” ” 17928 5 6571:2 8 ‘5 - 17944°6 5553°6 4*b Rt 18001:4 5541°0 6* Teo . 180424 5513-4 3b 1:50 | 18132°7 5501-4 2 a 50 | 181722 5490:0 3 4 ; 18209°9 **5 484-6 4 aa ae | 18227°9 5476°3 4 1:49 ) 18255°5 5461-0 10*t§||b 54606 FA A a 183067 5455-0 3 ase e 183268 5449°9 3 cab te 183440 5443-2 3 ile Sn 18366°5 5426°5 10*§b 42671, Viale Val epee) 184231 5416°9 3 hy wiles. A 18455°7 5398-5 2. | Leste WP 6pl | 18518°6 5393-4 eee A is 18536'1 6384-9 1 Ms os 18565°3 ON WAVE-LENGTH TABLFS OF THE SPECTRA OF THE ELEMENTS. 301 MeRcuRY (LINE SPECTRUM)— continued. Reduction to Wave- Intensity | Previous Measurements hit sa Oseil'ation length and (Angstrém ) aa. ear Frequency (Rowland) | Character Aes ns in Vacuo a 5373°2 3 1.47 51 18605°8 5365°5 2*§]| 364:6 Thalén ae ys 18632°5 5360°6 In 1:46 5S 18649°5 5355°5 1 Pan itoare 18667°3 5352°4 1 onl ess 186781 5346°3 3 % 5 18699°4 5334'3 2b ” ” 18741°5 5311°7 4 1:45 +4 18821°3 5308-0 1 35 = 18834°4 5294-7 2 7. 5-2 188816 5288°7 6* 1-44 3 18903:0 5284°2 3 % % 18919°1 5281°5 5 pets re 18928°8 5279'3 4*§ 52786 i, “ 7 18936°7 5275°5 1 3 in 18950°3 5273°7 4 as co 189568 5254:0 2 “ ” 19027'9 52428 ae 1:43 3 190686 5233°8 4* # 8 19101°4 5218-0 T*S baLy2 5 Wai 53 4 19159°2 52112 4 | 1:42 38 19184-2 5207:0 T*S 52062 _—s«, ess 5:3 19199°6 5196°6 4 * Py 19238'0 5190°7 1 Fa 19259°9 5187-5 2 ii is 192718 5172-4 2n 1-41 3 19328°1 5163:2 4* pe ers 19362°5 5149-2 4* a 5 19415°2 5141°5 1 ss 5 19444°3 51356 5 1-40 7 19466°6 5132-0 7§ 51312 —S,, % 19480°3 5113°7 1 54 19549'9 5107°3 3 f e 19574°4 51029 3 | * - in 19591°3 51005 1 1:39 % 196005 5098°4 2 = + 196086 50863 1 3 As 19655:3 5083-0 2 oe . 19668:0 50736 2 93 i 19704°5 5068-2 7 rs is 19725°5 5062°6 4 1:38 is 197473 5058°4 1 5 - 19763:7 5051-8 1 3 = 19789°5 5048-4 ZN 35 aa 19802°9 5045°7 4 | = i 198135 5042°4 2 a i 19826°4 5038°3 2 ‘ - 19842°6 5027-1 1 ss 55 19886°7 5020°9 2 137, ni 19911:2 5018°4 2 ¥ - 19921°2 5008°6 2b ee - 199602 4992°5 5 es x 20024°5 4986:7 3 1:36 i 20047°8 4981-3 3 Me 20069°6 4974-0 6* a 20099-0 302 REPORT—1895. Mercury (LINE SPHCTRUM)—continued. Reduction to Wave- Intensity | Previous Measurements St ae Oscillation length and (Angstrém ) ce ple Frequency (Rowland) | Character u in Vacuo At Re 4970°0 1 1:36 | 55 | 20115°2 4965-4 1 “ 20133°9 4959°7 4*§]|b 49581 Thalén : > 20157-0 4949-4 3 Doel A 20199-0 4943°4 1b » | 86 20223-4 4933-0 2 » x a 20266-0 4917-9 2 % a 20328'3 4916-4 4*+§]| 49161 ,, Loa oe 20334°5 4913-0 2 PM errr 5 203486 4902°1 4* 5 lS Se 203938 4898°3 i a - | 20409°6 4895°8 2 : Pe 204201 4880°2 1 * ei} 204854 4869°9 3)) » 1:33 3 an 20528'7 4867°3 4f ” aii 20539°7 4864'8 3 i * 20550°2 4856°6 3 S 57 20584:8 4849-4 1 7 ‘ont 20615°4 48446 9s 3 5 206358 4841°3 4* 132)! »,, 20649°9 4826-0 8*§ ad ae 20715°4 4813-0 4* ae | les 20771°4 4797-4 8* Pat ie 20838°9 AT73°7 1 th aesal BB: 20942°3 47681 6 | Nn a 20966°9 4753°4 3* (30 Ey 21031:8 ATALT 6* A OEY ae 21070°3 4740°3 1 aN aes 21089°9 4729°9 8 1:29) ae | 211363 4697-9 1 soe] Bala} 21280°2 4689°1 1 1:28 roe 21320°1 4687-0 1 5 eo 21329°7 4681-6 2n ee 21354:3 4667°5 2 . a 21418°8 4664-2 1 e i, 21434:0 4661:0 7* a ¥ 21448°7 4651-7 5 127 bl) ee 21491°6 4647°8 2 me ae fe 21509°7 4639'3 1 ae ee 2154971 4637-0 2 a Eh is 21559'8 4635°9 1* .; » | 21564:9 4634-2 1 ee 6-0 | 21572°7 4630°5 1 tl es 21589:9 4626-2 2b ale Pos 21610-0 4620°5 1 ee 21636°7 4616-5 1 126 Sh xs. 3 21655°4 46048 2 a a4 21710°5 4602-9 2 a 21719°4 4600°7 2 » |» 21729°8 4598:2 5* SS ae: 21741°6 4593°5 1 ah Bee - Ot 21763:9 4587-1 2 fe a 4 217943 4580°1 In 1:25 Hits, | 21827°6 4578°2 1 Seg te 21836°6 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 308 MEROURY (LINE SPECTRUM) —continued. Reduction to Wave- Intensity | Previous Measurements , aia Oscillation length and (Angstrém) a Freouency | (Rowland) | Character we ilps in Vacuo a A 45715 1 1°25 6:0 21868°6 4568°8 2b » ” 21881°6 4562°3 21 « “p 61 21912°7 45538 6s ” ” 21953°6 4547°0 2 ”» ” 219864 4544-2 4 eae oes 2000-0 4541°7 1 | 1:24 ” 22012°1 4539°9 in oF ” 22020°8 4537°7 2n ” ” 22031°5 45349 1 ” ” 22045'1 4532°7 2 “4 ms 22055:8 4530°3 1 ” Pa 22067°5 4525°1 1 ” ” 22092°9 4522°9 6*3 HH ” 22103°6 45189 1 AY ” 22123°2 4516-4 4 ” ” 22135°4 4511°5 2 ” ” 22159°5 4507:2 2 5 ” 22180°6 4505-0 1b | | 1:23 ” 22191°5 44199°8 1 | ” ” 22217°1 4498-0 1 ” ” 22226°0 44950 1s os 6:2 22240°7 4493°2 1s | ” ” 22249°6 4491-9 1 ” ” 22256°1 4490°3 3 0 FA 22264:0 4486'8 8*b Se nie ass 22281-4 | 4483-7 3 “ 9 22296°8 _ 4480°7 1 S Ph 22311°7 4470°5 5* ” ” 22362°7 4466°7 2n 1:22 of 22381:7 4464°2 3 ~ ag 22394:2 4461-5 1 oss eo sedges ' 4459°3 3 ” ” 22418'8 | 4454-1 2n ss a 224450 | 4450-7 1* a, a 22462:2 «44464 3 ” ” 22483-9 4435'8 3: ” ” 22537°6 4434-2 2 ” y 22545'8 4431°6 2 7 63 22558°9 4425°9 8b 1:21 & 22588:0 j 4422:2 2 ” ” 22606'9 } ‘ 4420°6 2 ” ” 226151 4416-0 1 ” ” 22638°6 4415-4 3 os iy 226417 4414-0 3 aS 22648°9 44121 3 4 oy 22658°6 4408°4 i ! ” 22677-T 44015 10*b 9 ” 227132 4391-9 10*b | 1-20 a 22762°9 4385°7 8 “s ay db 227951 4382:9 8 mo a 22809°6 4378'7 8* ih tore Ble css 22831°5 4376-1 10* “A 35 22845:1 4372°6 2t | ” ” 228634 4369°6 1 To rae 22879'1 304 REPORT—1895. MeERcuRY (LINE SPECTRUM)—continued. Reduction to . Vucuum sy oye Wave- eee Previous Measurements | nines length Character (Angstrom) | ae eles in Vacuo A 4358°6 10*f§]| 4358°0 H.& A.,4358 1T.| 1:20 64 22936°7 4347-7 10*F§}| 4348-0 H. & A. 119 7 229943 4344-2 2 43410, cae et te 23012°8 4339-5 6*f§ || a3 aly ta 23037:7 4336°9 8 36 6 23051°5 4333°4 3 53 5) 23070°2 4329°1 1 + os 23093°1L 4327:2 5 6 nf 23103°2 4324-7 5 = 7 231166 4320°4 8 in ; 23139°6 4318°3 1 | 1-18 * 231509 4315°8 1 Ne gs of 23164°3 4314:2 \ 4 ” ” 23172°9 431279 ab a = 23179°9 4310°3 2 ree leer 23193°8 4308°6 1 », | 6:5 23202°9 4306°6 4 Sells bias 23213°7 4305°5 4 rm F 23219°6 4304:0 1 ” ” 23227°7 4301°7 2b ” ” 232401 4300°0 1 by os a 23249°3 4297°6 5 \ ¥ “r + 23262°3 4292°3 5 a 23291°0 42901 3 ” ” 23303°0 4288°2 2 5 23313°3 **4285°1 6 ” ” 23330°2 4282-7 6* - 2 23343°2 4276°7 3b Le es 23376°0 42701 3 % 4 234121 42642 8*b ” ” 23444°6 4261°6 8*b rr 4 23458°9 4259°0 2 * on 23473°2 4257°6 3 - ¥ 23480°9 42564 4 ” ” 23487°5 4255°2 2 A on 234942 4252-7 4 : 66 23507°9 4249-2 2b + A 23527°2 4248-9 5 ee + 235289 4237-7 5 1:16 +n 2359L1 4234°5 6* oF 6 23608°9 4232°8 4 A £ 23618-4 4230°1 ti = A 23633°5 4227-4 8* is as 236486 4225°4 2 _ es 23659°8 4221°6 6* ay ay 23681-1 4219°4 1 > e 23693-4 42186 2 ase | Ay 23697°9 4216°8 10*$b ree | ee 237081 42118 6* oP alaes: 23736°2 4206°6 5 5 - 23765°6 4200°8 1 15 5 23798-4 4199°1 1 3 6:7 23807°9 4196°8 6 x : 23821:0 4192-4 5* 3 +s 23846:0 41860 7 23882°4 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 305 Mercury (LINE SPECTRUM)—continued. ge Ua to . acuum eame Wave- ss er Previous Measurements Peron length Shaniee (Angstrém) 1 in see A+ ye 4183°0 i 1.15 | 67 23899°6 4181°5 1 ” ” 23908°2 41785 8* ” oA 239253 41759 6 or 1 23940°2 4169:0 Oe 1-14 F, 23979°9 4167°8 1 ” ” 23986°8 4165°7 1 ” ” 23998'9 41646 1 Af 7 24005-2 4162:0 8* 99 + 24020°2 4157-1 4 “r * 24048-5 4155-1 a “ A 24060°1 4149°5 3 s ot 240926 4148°6 1 * 6°8 24097°7 4145:0 2 = oh 24118°6 4143°7 1 * A 24126°2 41405 1 | + 3 24144:9 41349 2* 9 7 24177°6 4132-7 1 9 5 24190°5 41243 2 ; 1:18 i 24239°7 41230 1 ” ” 24247°4 4120°9 8*Sb ” ” 24259°7 4117°5 3 ” ” 24279°8 4115°3 8*§ es Fh 24292°8 4109-1 6*§ FA s 24329°4 4106°9 6* oe + 24342°5 41041 8* 3 Ft 243591 4098:0 3 3 69 24395:2 4096'5 1 ” ” 24404:2 4093-1 2 Pp 1:12 “5 24424°5 4091°8 2 Pe # 24432-2 4088-4 2 a cf 244525 4086:9 i rf - 244615 4084°6 1 5 1 244753 4083:1 ae 3 i 24484°3 4080°7 1 EA oF 24498-7 4078:1 10*f§||b ” ” 24514°3 4077:0' 5 40775 H.& A. be Ps 8 24520°9 4073°6 4 eee fF 24541°4 4069°8 3 “5 ii 24564°3 4066:7 2 Fs i 24583°1 40625 2 ” ” 24608°5 4061°8 1 i ‘5 24612°7 4061:0 4 ” ” 24617°6 4057°9 4*t An 3 2463264 4056-0 1 $i 3 24647°9 4054°5 1 siti a 246570 4053°5 4 r 3 24663°1 4046°84 10*+§|| 4046-5 H & A. * 7:0 24703'9 4040°7 5*§ | ss 3 24741:2 4037°5 4 55 8 24760°8 4035°3 5 ss 3 247743 4033-0 Tb ” » 24788°4 4030°9 1*§ ee re 24801°4 4029-9 3 es is 24807°5 4024-4 8*§b 3 Ps 24841-4. | 1895. x 306 REPORT—1895. Murcury (LiInE SPECTRUM)—continued. Reduction Wave- Intensity | Previous Measurements to Vaenum Oscillation length and (Angstrém) Frequency (Rowland) | Character re ting in Vacuo A 4022-0 1 1:11 7-0 248562 4021:0 2 on ee 24862°4 402071 4 5 a 24868:0 4014'8 iE 1:10 et 24900°'8 4011:0 2 ” ” 24924-4 4010-0 1 5 39 24930°7 4006'0 8*b ” ” 24955°6 4003°5 4 a 71 24971°0 4001°8 3 és is 24981°6 3999°9 if ” ” 249935 3999-2 2 s oe 24997°9 3998-2 1 99 5 25004'2 3996°8 1 * = 25012°9 3995'8 1 5 i 25019°2 39938 6 a > 25031°7 3989 8 2 * 4 25056'8 39688 | 1 a ‘ 25063'1 39841 | 10*§||b 3984-0 H. & A. y > 25092°7 39788 4 as “ 2512671 3976°5 6 ] »” ” 25140°6 3971°6 1 ” ” 25171°7 39703 1 | ” 25 25179°9 3967°9 8*b a a 25195°1 39649 4* = 3 25214°2 3962-9 Bl x ” , 25226'9 3960°2 5s 3 :. 25244-1 3954-7 6 by 7:2 25279°2 395171 2 - 25302°2 3950°2 3 ee 25308'0 3948°3 Tb ” ? 25320°2 3945-2 6* ns = 25340°1 3942-3 3 - 7 253587 3939-6 3 35 . 2537671 3936-7 5 | 1:08 = 25394'8 3931-7 2 Se ss 254271 3930°3 2 s 4 2543671 3928°1 6 i 3 254504 | 3925-5 $b | 4 : 25467°3 3922-0 if | a ES 254900 3918-9 7 | if zs 25510°2 3916-4 5 ; ~ 255264 3914-5 5*§ | Al = 25538'8 3911-1 1 \ * gens 25561°] 3909-7 ] | e ie 25570°2 3908-9 2 “ 73 265753 3906-6 4*t¢$|[b 3 : 25590°4 3904-4 2 | ‘ bs 25604:'8 3903-7 3 ; :; 25609°4 3902.1 ies a 3 2561979 3901-6 ] - = 25623°2 3900°1 5 Ae 3 256331 | 3899-0 4 A 2 25640°3 3897°5 1 * 25650°2 389673 1 1:07 os 25658°1 ——— ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 307 Wave- length (Rowland) 3895-6 F 3887°3 : 3883-9 3882:0 38811 3878-0 3875°2 3874:3 3873°6 3870°3 3869°3 q 3864-0 3863°4 3860-4 3857°5 3856°6 3851:2 3845:1 3843:2 3842:0 3840°5 3839°49, **3837°8 3835-9 3834-6 3833°6 3832-6 3829°6 3829-4 3826°8 3822°7 3820°69 3817-7 3816°3 3814-2 3812-7 38115 ; 38111 } 3810-4 3809-0 ¢ 3807°6 “Te 3803°6 : 3801°5 : 3797-6 “ 3795'8 * 3792-7 379049 3788°0 3787-2 37863 3784-6 3783:8 3782°5 3780°8 3779-7 C—O ee OO MERCURY (LINE SPECTRUM) —continued. Intensity and Character Ot et OD i=] * at * 77) Bea ees BENS CERO ras 02 Ol ats * 770) o 5 —~ % ayn en ree abo Ss RA CTA BOARS BO Pets CAA 77) aR 5 o woe * * ou o % 7) lo” RP NN RR Re ewe we Previous Measurements (Angstrom) 3859:0 H. & A. 38200 ,, 3807-0 3800°0 ,, 3790°0 ,, Reduction to Oscillation Frequency in Vacuo Vacuum eg 1 | + sree A | * LO7 + | 7:3 ” | ” | ” ” ” 3 ” ” ” ” ” ” 2” ” | | ” ” | | ” ” | ” ” | ”? ” ” ? ? 29 ” ” 1:06 9 ” ” ” ’ ” ” | ” ’ | ” ” 2 ’ j ” , 7 ] | ” i ] ” ’ | | LY 9 3? ” ” ” ” 39 ” ” ” ” = - 74 1:05 ) 105 | ss S ~ 25662°7 25717°5 25740:0 25752'6 25758°6 25779°2 257978 25803'8 25808°5 25830'5 25837°2 25872°6 25876'6 25896°8 25916°2 25922°3 25958°6 25999'8 26012'7 26020°8 26031:0 26038°4 26049°3 26062-2 26071:0 26077 8 26084°6 26105°1 26106°4 26124°2 26152-2 26166°6 26186°4 26196:0 26210°4 26220°7 262290 26231:7 26236°6 26246°2 26255:°9 26283°5 26298:0 263250 26337'5 26359°0 26375:0 26391'8 26397°3 26403-°6 26415°5 26421°1 264301 26442:0 26449-7 x 2 308 REPORT—1895. Mercury (LINE SPECTRUM)—continued. Wave- length (Rowland) Intensity and Character 3776°5 3774-39 3770°7 3762'2 3759°9 37573 3756°6 3T555Y 3752'5 3751'8 3750°9 3747°5 3743°9 3742'6 3741°7 3740°7 37389 3735:0 3729°5 3726'9 37263 | 3724°7 | 37180 3715°5 3712:9 3711-2 3709°6 3708'2 3707°6 3707°0 3705°7 37049 3704-6 | 3703-4 3702'4 3701°4 3698'6 3695'6 3691'8 3690:0 3689:2 3688°5 3685°2 3680°7 3665°4 3663'3 3661°4 3659°4 3656-4 3654-9 3651-9 3650°3 3644-5 3642:5 2638-5 3n 8*b 5*§||b *§ (br 1O*tS |b 3 i 1 8*f$ | 3 10*f$|| 5 WODR RK RPWH NRF WORK WN RWW RE RW RE RE Ob eee br bw or Reduction to Vacuum Previous Measurements |__ (Angstrém) | 4 A+ | ae 1-04 TA ” ” 3770-0H. & A. wh Ce ” ” ” ” ” ” , ” ” ” ” ” 3751:0 ” ” ” ” ” ” ” ” ” ” ” » ” ” ” ” ” 1:03 ay ”» ” s 76 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” 1:02 5 ” ” ” ” be ” ” ” ” ” SOoL9) es ae ” ” ‘Sg » i » ” ” | ” ” 1:01 oF 36544, ” ” ” %” 3650-09 5 4 ” %” ay »” A 78 Oscillation Frequency in Vacuo 26472°1 26487°6 26512°8 26572°7 265889 26607°4 26612°3 26620°1 26641°4 26646°4 26652'8 266770 26702°6 26711°9 267183 26726'5 26738°3 26766'3 268057 26824'3 26828-7 26840°2 26888°6 269067 26925°5 26937°9 26949°5 26959°7 26964:0 26968°4 26977°8 26983°7 26985'9 26994°6 27001'9 27009°2 27029°6 27051°6 27079°5 27092:7 27098°5 27103°7 271280 27161:0 27274°4 27290°1 273043 27319°2 27341°6 27352°8 27375°3 27387°3 274309 27446-0 27476°0 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 309 MERcuRY (LINE SPECTRUM)—continued. Reduction to Wave- | Intensity | previoys Measurements |__~"™ Oscillation length and = ° (Angstrém) Frequency (Rowland) | Character ee at in Vacuo A 3633°5 3* 1:01 78 27513'9 3632°5 1 ” ” 27521-4 3630°3 5 9 oF 27538-1 3627°6 1 ” ” 27558°6 3623-4 Is ” ” 27590°6 3620°0 1 ” ” 27616°5 36186 5S ” ” 27627°2 3616°0 2 1:00 » 27647°1 3613°7 4S ” ” 27664:7 3610°7 1 ” x 27687-7 3609°1 1 ” | ” 27699°9 3607-6 5§ 3 5 27711:5 3604-2 28 ” “, 277376 3594-7 3§ 3 79 27810°8 3593-2 3§ 9 + 27822°4 3590°9 1§ A 278403 35777 28 0:99 x 27943-0 3561°5 5*t§||b 356071 H. & A. ” ” 28070°2 3549°6 1 ” 8:0 281642 3543-7 5*f§||b 3542°3—,, i ” 282111 3533'5 2 0:98 5 28292°6 3518°0 1 ” = 28417-2 35001 1 ” 81 28562°5 3494°5 1§ 34926 ,, 0:97 + 28608°3 3473°6 1§ 34734, ” » 28780°5 3456'3 1 0-96 | 82 28924°5 3451°8 2§ 34514, - 7 28962-2 3440°6 1 = -, 29056°5 3437°1 i ” of 29086°1 3434-7 1 29 5 29106°4 3431°7 2b y 8:3 291318 3423°5 1 2 4) 29201°6 34149 1 0°95 “5 29275:1 3410:0 1 5 a 29317°2 3407'1 1 ’ ” 293422 339671 if 9 8-4 29437°1 3390°5 5t§||b 3389°5 ‘ cf 29485°8 3386°6 s = nF 29519-7 3366°7 2t§||[n 3365°5 i, 0:94 + 29694:'3 3351°5 4t§|| 33512 ~—C, " 85 29828-9 33417 6t§|| 33412 Sy, fe Si 29916°4 3320°5 1 33264 =, 0:93 | 86 30107°3 3305°2 1$|| » is 30246°8 3278'5 2t§ 0:92 | &7 30493'1 3264:3 2tS || ” ” 30625°7 3227°5 2§ 0-91 | 88 309749 3208-7 3t§ a207- ss 0:90 | 8&9 311564 3207-7 1 ay a 31166". 3144°6 3$||b 0°89 | 91 31791-4 3135-9 1||/n 0:88 - 31879-7 31318 5t§|| 3130-4 » |» 31921-4 3125°8 5t§|| 31248 ry 5S 31982°7 8116°5 1 3 a9 32078°2 3107°7 1 or 9-2 32168:9 3096-0 2 || 3094:0 H. & A. 0:87 + 32290°5 310 REPORT—1895. MERCURY (LINE SPECTRUM)—continued. | Reduction to Wave- Intensity : Me a Oscillation length and Previous Measurements }——{_—_—_ Frequency (Rowland) | Character | (Angstrom) ee ay in Vacuo A 3093°3 1 0:87 | 9:2 32318-7 3090°6 1 bs 3 32347-0 3085°4 1§|n » ” 32401°5 3051-0 25 || 0:86 | 9-4 327667 3038°7 2i|s * ; 32899°4 3027°6 2Fll ” ” 33020°1 3023°7 2tll ” 9°5 33062°6 3021-6 3T$|| 3021-0 H. & A. 0:85 J 33085°5 3011-2 1jn s- 4 33199°8 3007'0 2§|[n * 5: 33246:2 2972°8 1s 084 | 96 33628°7 2967°4 St§|| 29664 4, + 97 33689'8 2955°3 1 - 5 33827°8 2953 3 m9 9 | ‘Nm ier 33850°7 2947°5 3t§ 29466, 7 - 339174 2942°6 ln / 0:83 | 9°8 33973'8 2941°3 ln it 7 33988'8 29398 1§ 35 ” 34006:1 2935°8 28 29355, . is 34052'5 2925°5 7t§ || 2925-2 » al | 34172°4 2916-4 3t$ | 2915-3 4, % 99 | 342789 2915°5 1 3 ‘ 34289'5 2893°7 =| ss 7F$ll 28929, 0:82 | 10-0 34547'8 28868 | 1§ § 5 34630°4 28822 =| 1f § . 34685°7 28733 | «28s * ‘ 34793-2 28651 | 28||b 5° 1104 34892-7 28571 | 4t§|| 0:81 » | 34990°4 23620 = | 1 ‘s an 35053-0 28479 | 8t§| | 28468 ,, i." HI 35103-4 28420 | In | i, si 351763 Ac! aca is x 35263-2 28335 | 26§|| 57) ee - 35281°8 28200 | 4t§ilb | 2819-7 0:80 | 10:3 354507 28065 | 1f§ | 2810-0 H. & A. * x 35621°3 23044 | 14§ 28045 - " 356479 2803°7 3t§ || | i. i 356569 27998 1§ | 27985 ,, - a. 35706'5 27912 =| «38 27900 si, eee! 358165 27891 =| 1 i, an 35843°5 27846 | 1 % ond 35901°4 2781-0 1 | 0-79 ah 35947°9 2774-7 25 | | 27732 ,, nt 10 36029°4 2767°6 1 ‘ _ 361219 27622. | 2 . ¥ 36192°5 27593 =| -2t§| D1608 5 é 36224-0 2752°9 6tS|| 2751-5 ie 363148 2741:3- | In 0:78 | 10-6 36468'4 27265 ~* | --1§ ss 4 Or 366664 27242 | 18 = ‘ 36697°3 2710°4 1§ § a 36884-2 2705°5 1§ te “ 36951-0 2702-7 25 27020 H. & A. » 1208 36989-2 2699°5 3tll “= i 37033'1 2686-7 28 |b | 0-77 ‘4 372096 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 311 Mercury (LINE SPECTRUM)—continued. Reduction to Jae . . Wave- Intensity | Previous Measurements Ypcuam Oscillation length and make [an a Frequency (Rowland) Character Capertnim) Pees eo in Woe A 2675°2 1|| 0:77 | 10:9 37369'5 2672'8 1§]| eee ara 374030 26645 1 fhe sca | ae 37519°6 2660°6 1§]| § | 375746 2658°6 In 2657°6 H. & A. = ae | 37602°9 2655°3 2t§ || s — 37649°6 : 26539 2t§ |] 0-76 |11:0 37669°4 2652°2 3t§|| 26522 = 5, = 5 37693°5 2648°3 18} 9» - 377491 2642°7 28 |b 26446 5, ; : 37829°1 2640°5 1t 26406 ,, - * 37860°6 ; 2629-0 In ese | LIL 380262 | 26257 ~-| 1 pi o 38074:0 | 2614°8 1 ” ” 38232°7 | 2609°7 28 | 0-75 | ,, 38307°5 2605°3 28 | LL 38372°1 2603-1 3t§ 26023, “ ne 384045 2598°3 1 = i 38475°5 7 2584:7 25 2584-2 ,, be LS 38677°9 | 2576°3 3t§|| nat: 5 388041 2575°2 25 25753. ay #5 = 38820°6 2564-1 1t$|| 0-74 | 11-4 38988°6 2561-4 1 i er 39029°7 ‘| 2558-0 1§ z i 390816 2540°4 28 || Seagal 39352°4 2536-7 6tS || 25358 #8 eal 39409°8 2534-9 3t§]| 2533'8 % 33 39437°8 2524'8 28 |b 2522°7 sp Le 39595°5 2515-2 2§ 2514-3 O7ZBealonss 397467 2507-2 1 ater | 398734 2505-0 18} $ RS cath 39908°5 2499-4 1 ” ” 39997°9 2492°2 3t§s 2491-4 ee Gh ae 40113°4 | 24902 1§ a x 40145°6 2483-9 1t$ 2484-2 aed 9 402475 ‘ zisoa | 1+ ss i. 40263°7 | 2482-1 2t5 || : 7 40276°7 : 2478°8 1¢§||n 2477-7 - i 40330°3 2478-2 1+ b = 40340°1 | 2469-5 18 072 |11:9 | 4048-1 2468°1 28 24680 H. & A. ‘s oH 40505:1 | 2464-2 44§]|| 2463-7, i mgt: 405692 2459°6 1§ 24593, e320 406450 | 2447-0 2+ || ¥ + 408544 f 2414:3 ATS 2414-3 0-71 | 12-2 41407-7 | 2412°3 1t$|| nT tas 41441-9 | 2407-6 4t§ 2407°3 . ts _ 41522°8 23996 86; 2i| ees 3 41661°3 93903 | 1§ 2390-0 i, Ae! | 418233 2380°1 In | tes 42002'5 2378'4 3t$|| Fs 42032°6 2374-1 1\jn - _ 42108°7 2369-3 2§ 0-70 | ,, 421941 2354°3 1§ 2355°2 H. & A. PT, 42462'8 2353°6 1} 4 2 424754 312 REPORT—1895. MeERcuRY (LINE SPECTRUM)—continued. Reduction to ee eed Previous Measurements ore ered Oscillation en on Oo . (Sonlaad) Character aac ut py cee ee ed ae 2352°6 1fn 0-70 | 12-7 42493°5 2345-4 248] = és 42623°9 2341°9 1§ 2342-2 H. & A. Fr sh 42687°7 2340°5 1§ 2340°0 a 12°8 427131 2339°3 3§ 5 is 42735-0 2335'1 1§n P: 5 428119 2327°5 In 7 139 42951°7 2323°1 ln | 0°69 FF, 43033°0 2321:0 1§n Res 3 430720 2315-0 1§b 2315-2 3255 ne 43183°6 2301-6 1} \|b | ,, {18-0 43435:0 22964 1§b 2296°5 os 13:1 43533°3 22920 2$n 2292°6 Me a 43616°9 2284-0 1 oneal Be: 43769°6 2264:0 2t§b 2264:2 0°68 | 13:3 441563 saan | 24$]| 2263°3 » | 134 44191-4 2260:4 27§]|| 2261-4 + » 44226°6 2258°6 In a a3 44261°8 22529 2§|l 2254-0 By 7 44373°8 2244-1 1§ "3 13°5 44547°8 2230:0 2§ 2231:0 0°67 |13°6 44829°4 2224°7 21§||b 2225°7 PA 13°7 44936°2 2191°3 1§ 2190°9 antes 14:0 45621-0 2150°6 1§ 21480 0°66 | 14:3 46484°3 Mercury (Banp SpecTRUM—SparK IN Vacuum TusBE witnout LryDEN JAR). Eder and Valenta, ‘ Denkschr. Wien,’ Bd. 1xi., 1894. Reduction Reduction Bo Bho Wave: pee bo Vespan EEE Wave. iraty to Vacuum ese length Character rae eee length Character 1|3e> A+] =-| SES A+ |---| BES ‘tae? i oi os | @45171 | 2s) S| 1-24| 61/22132-0 4477-0 | 3 1:23 | 6-2 | 22330-2 B45143 | 2s} s| ,, | » | 221457 4474-6 | 1 » | 9 | 22342-2 A530.) T \br5| .,,, |», | 22152 4465°5 | 3 1:22| ,, | 22387°7 45105 | ea ae. Mueeral ee laded: 4462°6 | 1 a. eee ODS 45087 2) | ,, | », | 221732 4451°4 | 2 f », | 22458°6 45052 | 2 1:23] ,, |22190°5 *4448'8 | 1 » | se | 22a718 *45025 | 2 a »» | 22203°8 4434-8 | 1 as | gg | 22542-7 44979 | 2 - », | 22226°5 4433-4 | 1 il y, | 22549°8 44954 | 1 », | 6:2 | 22238'8 43963 | 38s, |] 121 63) 227401 44934 | 1 . »» | 22248°7 a{ 43950 3s} 8! ,, | ,, | 227468 44893 | 3 id » | 22269:0 4393°2 | 4s = 1:20! ,, | 227561 44872 | 3 a », |22279°4 a s5020 3s(P"E} .. |, | 22759°3 4484-9 | 1 - 5 | 22290°8 4391°5 | ie | » | 227650 4478'8 | 3 a » | 22321-2 43904|3)] wl ,, », | 22770°7 * Perhaps double. ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 313 MERcURY (BAND SPECTRUM)—continued. Wave- length 4389°4 43881 4386°5 4385°2 4384-4 4382°8 4389-0 4381:3 4380-0 4378°3 4378-0 4376:2 4374-9 4374-5 [4372-6 4370°6 4369-4 4369'1 4368°3 436671 4364-0 [4358-6 4353-2 4352°6 4350-0 [4347°7 4344-0 43431 43406 [4339-5 *4338'4 4336°8 4332'8 4332°0 4330°6 4330°1 4328°7 4326-4 4321-1 4319-6 4318-0 4317°6 4315-2 4308°3 4307°3 4305°6 4303-2 Reduction i | B Lie. | ta § Reo Intensity °° ecu BS 3 | Wave- | intensity po penum = 8 3 ot Ra as | =a eee and Rey \Character Ae pe S| = Character es | Se ene | ke i Ae | | | | | 3 1:20} 6:3 | 22775°8 42948 | 2 118 | 6°5| 232775 3 » | 95) | 220026 4292°4 | 2 9 «| gy =| BaZ90°5 4 > | 9» | 22790°9 | 4991:2 | 2 7 », | 23297:0 3 te || Sige abeeionicd: | 4289°8 | 1 | os ee a04-6 3 5 +, | 22801°8 42823 | 1 » | 9, | 23345-4 2 o », | 228102 | 42781 | 2 117! ,, | 23368-4 2 6 » | 22814°3 4275°3 | 1 3 » |zeeso't 3 “e », | 22818-0 | 42665 | 1 es » | 23431°9 2 6 » | 22824:7 42629 | 1 a » | 23451°7 2 a », | 22833°6 4260°6 | 1 Ry » | 23464-4 2 ue » | 22835°2 4250°7 | 1 =5 66 | 23518'9 2 nd », | 22844°6 42461 1 FS » | 235444 1 “A » | 22851°4 4243°6 | 1 1:16] ,, | 235583 1 », | 22853°4 4233°8 | 1 5) Roe BOLe:s 3, line 22863°4 &e,&e. | Numer- | spec- | ,, - | ous very | | trum] faint 2 * » | 228739 | lines 1 *. + | 22880°1 4218-9 | 3s | 4, | | 236963 1 | 2 lpeser-7 || *laoi83 (331 SS) a | decnh Begg 1 Fe 6-4 | 22885°8 42180 | 1 Ci rr » | 23701°3 3 ee 3 | 22827°3 42176 | 2 rb 5) 3 » | 23703°6 3 Fi », | 229084 2906°8:)1 | Sb 5 |os5 BaTOsd 10b, line 22936-7 42159 |1]) | , | » | 2387131 spec- s P 4215:0 | 1 PA +» | 23718°2 trum] 4214-1 | 4s » | 9 | 28723°3 2 119) ,, |} 22965 2 B 1 4913:8 4s Fe » | 287249 2 is », | 22968 4 4212°9 | 5 » | 3: | 237300 3 « »» | 229821 42121 | 1 » | gp | 287845 10b, line 22994:3 || *4211-2 | 4 » | | 23739°6 spec- ” 3 4210-2 | 1 » | | 23745°2 trum] : 4209-1 | 3 ., a eT DLA. 2 a! », | 230139 4208°7 | 2 re » | 23753°7 2 » | 49 | 280186 4207°6 | 2 » | yy | 28759°9 3 3 » | 23031°9 4207:2 | 2 55 3 | 23762-2 10b, line 23037°7 42067 | 1 oF » | 23765°0 spec- cs Ps 42063 | 3 5 » | 23767°3 trum] *4205'5 | 2 1:15] ,, | 23771°8 1 +s 3» | 23043°6 4204-7 | 2 * », | 23776°3 5 o » | 28052°1 4203°5 | 1 ae 3 | 287831 1 » | 99 | 23073°4 42028 | 1 | is [age eBBVOT1 1 i , | 23077°6 4201°9 | 2 | ie We sen hemBraa2 2 rs », | 23085°1 | 4201°3 | 2 eee » | 28795°6 2 E ,, | 23087°8 41998 | 1 | ,, | 67] 288039 3 : », | 23095°2 4198°6 | 1 | os Phy. t 8820-8 1 99 », | 23107°5 4197°6 | 1 eaream eames Ki 1 33 », | 23135°9 41970 | 3 p. [8s5 1 SEBESS 1 » | ». (231489 | 4195-2 11 | a | o | 238301 a 1:18] ,, |231525 | 4194-4 | 2 | 4, | 9 | 23884°6 2 as », | 23154°6 | 4192°8 | 1 “4 » | 23843°7 1 Opa ee 231675 | 41923 | 1 » | 99 | 23846°5 1 5 6°5 | 232045 4191°6 | 2 A » | 238850°5 1 | 9 | 23209-9 4190°3 | 1 y» | 93 | 28857-9 3 | gp | 232191 41891 | 2 » | 9 | 23864:8 1 23232:0 4187-1 | 4 238762 314 REPORT—1895. MeERcuRY (BAND SPECTRUM)—continued Reduction) gg, | Reduction} ¢ 5, Intensity | to Vacuum | 8 2 Intensity | t© Vacuum} -& 25 euED Character 1 3 5 z | eng Character 1 So =| At x On | At AE Ons 4185-9 | 2 1:15] 6°7| 23883:0|| 4101-6 | 2 1.13,, 6-8 | 243739 41851 | 2 yy | Ua 2S887-6 || 6 ALONG | 2 » | on poses 41836 | 3 - » | 23896-2 | 4097°8 | 1 » | 69) 24396-4 4181-3 | 38 » | 9 | 289093 4096°7 | 1 »» | o» | 24403°0 4181:0 1 ” ” 23911-0 | 4096°2 1 ” ” 24406:0 4180-2 | 1 » | » | 23915°6)} 4091°8 | 1 1:12] ,, | 244322 4179-7 | 2 59 | hes. RBOLS'S 4089°9 | 3 » | 9 | 244436 4178'8 | 2 » | > | 289236 || 4087°3 | 2 » | ose | 2445971 4177-2 | 3 » | » | 28982°8 || © 4085:5 | 2 » | 9 | 24469°9 4175°0 | 4 » | 9 | 23945-4/| 40845 | 2 » 10x) |) 248759 41739 | 2 » | » | 23951°7 4079°5 | 1 o> [aay eeeO5'9 41725. | 3 » | 9 | 23959-7 40790 | 2 » | x» | 24508°9 4172-0 | 2 3 » | 23962:6|| [40781 | 8b,line| ,, »» | 245143 41700 | 3 » |'a | 2389741 || spec- 416971 | 1 5 BESS trum] 4167-8 | 3 1°14|>,, | 239868 || 4077-1 | 3 » 1 5 | 245208 4167:2 | 1 3» | x | 239902 40766 | 2 | » | o» | 245233 4166-2 | 2 3; »» | 23996-0 4075°5 | 1 » | 9» | 24530°0 *4164:8 | 3b » | 5, | 240040] 4073-0 | 2 | op 4%, | BHS450 41641 | 1 ob (ys, 4008-4 40717 | 2 » | 9 | 24552°9 41621 | 3 » | 9 | 24019°6 4063-9 | 2 » | » | 24600°0 41600 3 (a | Sy” We SAO81-8 40620 | 1 53 , | 24611°5 4157'9 | 2 1 ees », | 24043-9 4059°6 | 1 ) » | 24626-1 4156-7 4 | 5, | » | 24050°8|/ 4058-4 | 2 » | 24633°3 4155-0 | 1 » | + | 24060-7|| [4057-9 | 3s,line | ,, | ,, | 246364 4153-9 | 3 | 4, |g | 24067-1 spec- | 41520 | 4 | 3 (ees Pedorert| trum] 41490 1 , | 68) 24095-4 4050°7 | 1 1-11) 7:0 24680-1 4148-4 | 3 » |» | 24098-9]) 4049°8 | 2 » | 9» | 24685°6 41452 | 1 . lace | BaLLT-6 40490 | 1 7 » | 24690°5 41446 1 a. [tay 1 BELLO 40481 | 1 » | 9 | 24695-9 4143-3 | 4 | ee Ae aa as 4047°6 | 3 » | 9: | 24699°0 4142-4 | 1 | ., | y | 24133°8]} [40468 | 10b,line ,, | ,, | 24703°9 4139-4 | 4 bk hi Iemma TS spec- | | 41391 | 3 m » | 24153-0} trum] 4138-4 | 1 bose.) Lae 40445 | 3 loys’ dogy: IeaeaeS 4134-6 | 3 lo 1 Oey Ieee OS 40420 | 1 3 | 9 | 247882 4133°7 | 3 |’, [. (eases 4040°6 | 1 » | » | 24741°8 4129-9 | 2 | 1:13] ,, | 242069] 4038-7 | 1 » | sy (eReTSe4 41295 | 2 | 5 | oy | 24209:2 40371 | 1 oi | tape HBS 3 4128°8 | 2 » [%5. | 242433 4035°1 | 2 | os | sp HAIRS 'S 4124-0 | 2 [hay Paes 40346 | 1 | so | Pere SS 4123°8 | 2 Lge | Sag, Gee |) eeog4eee » | Carel, 41233 | 2 | sy | sp | 242456 40328 | 1 » oon IRBOT 4121:7 | 1 » | 9 | 24255°0') 4031-6 | 1 » | 9 | 24797-0 4119-6 | 2 » | 9 | 24267-4|| 4030°8 | 1 | ss Toop 4 @8B02-0 4118-9 | 2 5s [op | 242715 |) 4029-8 | 2 la [ae DRT 4117-5 | 1 | fap) B4279°8 4027°8 | 1 | ay | age SBO# 4113°3 | 2 » | x | 24304:6 40268 | 1 » |» | 248266 41128 | 1 » | 9 | 243075 4026-2 | 1 as | oy | 24830°3 4109°8 | 1 » | 9 | 248253) 4025-4 | 1 » | oo P 248352 41090 | 1 » |» | 24330°0|| 4024-2 | 1 » lia meee? 4108-2 | 4 o> hg, 4) 24384-8 | » 0222 | 4 » | 2 | 24855-0 4105°2 | 1 ss | » | 248525]; 4020-4 | 1 » | oy || 2486671 41019 | 3 24372'1|| © 4020:2 | 1 oy las (eaaeeT4 sl ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 312 MERCURY (BAND SPECTRUM)—continued. ; Reduction | gp. Reduction! gp, a Intensity to Vacuum s = =] Intensity to Vacuum | ae A = Wave- and 3 2 g Wave- and ee AC e| = oR: length (oharacter 1 = oe length =| Character 1 3 2. Gieoival || Cece At 157 | Ope 4018°8 | 1 1-11/ 7:0} 248760 3970-7 | 1 1:09 | 7-1; 25177°4 fa4017°5 | 4 ” » | 248841 397071 | 1 FA » | 25181°2 | 44017°5 | 4s re, op 3969°7 | 3 of » | 25183°7 a401771 | 4s 7 » | 24886°6 | 396971 | 2 a » | 25187°5 *4016°2 | 2 ro} oy » | 24892°2 | 3967°8 | 3 ” » | 25195°8 40151 | 3 8) 1:10) ,, | 24899-0| 3965°7 | 4 ) » | 25209°1 ; 40149 | 1 oa eS » | 24900°2 | 3965°4 | 4 ” » | 252110 4013°5 | 2 brig a » | 24908°9 3963°8 | 3 ” », | 26221°2 | 4013-2 | 1 si! 5 + | 24910°8 || 3962°8 | 2 “p » | 25227°6 8 f 4012-0 | 4s = » » | 24918°2 || 3962-0 | 2 ” » | 25232°7 14011-6 | 4s ” , | 24920°7 3960°9 | 1 3 » | 25239°7 , 4010°8 | 3 o6 » | 24925°7 || 3959°6 | 4 “5 » | 25248°0 | 4010°6 | 3 » | 24926°9 || 39589 | 3 ” » | 25252°4 J 4009°8 | 3 x » | 24931°9 || 3957-4 | 3 “1 » | 25262°0 | 4009°2 | 1 ” » | 24935°6 || 395671 | 1 ” 7:2 | 25270°2 4008°6 | 3 ne »» | 249394 || 39557 | 2 rr » | 25272°8 4008°0 | 2 + > | 24943°1 || 3953°5 | 4 99 » | 25286°8 4007-1 | 3 x » | 24948°7 3952°3 | 2 -r » | 25294°5 400673 | 1 Fy » | 24953°7 3950°6 | 2 a s, | 25305°4 40061 | 2 3 » | 24954:°9 3949:0 | 3 es », | 253157 4005°2 | 6 + » | 24960°5 3946°7 | 3 “6 » | 253304 40044 | 2 “ » | 24965°5 3945-2 | 3 7 » | 2538401 4003°9 | 2 “ » | 24968°6 3943°0 | 2 ” » | 253542 4003'1 | 7 5 71| 24973°5 394171 | 2 +f » | 253664 4001°8 | 3 FA » | 24981°6 3941-0 | 1 An 3, | 2536771 4000°9 | 2 eh s, | 24987°3 3939°6 | 3 rh, » | 25376°1 4000°4 | 4 a » | 24990°4 3938°5 | 2 7 » | 25383°2 3999°7 | 2 » | | 24994°8 39367 | 1 1:0 », | 25394:8 3998°9 | 2 » | 9 | 24999°8 3935:1 | 2 aa » | 25405°1 *3997°3 | 5 » | 9 | 25009°8 39346 | 2 ie » | 25408°3 3996°1 | 1 a » | 25017°3 3932°7 | 1 oF » | 25420°6 3995'6 | 3 FY 5 | 250204 3931-9 | 3 = » | 25425°8 3994:0 | 4 Pe » | 25030°5 3929°9 | 2 a » | 25438°7 , 3993-9 | 4 oy | 93 | 200311 3926°9 | 2 + » | 25458°2 : 3991°8 | 5 » | 9» | 250443 3923°9 | 3 Pr » | 254776 : 3990°9 | 1 FE » | 25049°9 || 39218 | 3 a » | 25491°3 : 399071 | ? a s, | 250549 39189 | 2 re » | 25510°2 ¥ 3989°9 4 ” ” 25056°2 3918°1 2 ” ” 25515°4 f 3987°6 | 3 + » | 25070°6 39176 | 1 % » | 25518°6 ‘| 3987°3 | 3 » | 9 | 28072°5 39158 | 3 » | 99 | 555304 7 3986:0 | 4 » | a | 25080°7 3914°6 | 1 : » | 205382 4 39854 | 4 a » | 25084°5 39132 | 2 a » | 25547°3 ; 39833 | 3 2 » | 25097°7 3910°3 | 2 “i » | 255663 ' 3982°4 | 3 “y » | 251038°4 3908°4 | 1 rf 73) 25578°6 } 8981°5 | 4 ce » | 25109°1 39067 | 3 = » | 25589°8 3980°6 | 3 ry ».| 251147] [8906-6 | 5s, line * » | 25590°4 39803 | 3 » » | 251166) spec- 39784 | 3 ‘5 » | 25128°6 | trum] ‘ 39769 | 2 5 > | 25138°1 |] 39043 | 1 fs » | 2560575 39766 | 3 i. 3, | 25140-:0 | 3902°2 | 1 + » | 25619°3 39754 | 2 1:09; ,, | 25147°6 3901°5 | 2 a 3 | 25623°9 39750 | 2 2, » | 25150°1 38985 | 1 os » | 25643°6 32742 | 1 = » | 26156°2 | 3897°7 | 3 a » | 25648°8 39731 | 4 » | 25162°2 38950 | 2 1:07| 7:3! 25666°6 3971:2 | 5 a » | 251742 38940 | 1 — » | 20673°6 316 REPORT—1895. MERCURY (BAND SPECTRUM)—continued. Reduction | gy, . | Reduction | ¢ p,. | Wass Ee to Vacuum - g g aot ashen! to Vacuum a 5 | pe Et Character 1 5 a” aie Character 1 5 cid 3892°1 | 2 1:07 | 7°3| 25685°8 || 37084 | 1 1:03 | 7:6} 26958°2 ! 38881 | 3 » » | 25712°2 || 3706°9 | 1 3 || 26969 3887'8 | J ” » | 25714-2 | 37064 | 1 5 » | 26972°8 38851 | 1 » | 25732°1 | 37060 | 1 ” » | 26975°7 | 38824 | 2 ” » | 25750:0 | 37055 | 1 ” » | 26979°3 3878:0 | 2 3 3 | 200092 37031 | 1 sy) » | 26996°8 3876°6 | 1 99 » | 25788°5 3702°6 | 1 4 » | 270004 387571 | 2 3 » | 25798°5 | 3700°6 | 1 a » | 27015:0 3872-4 | 2 a5 9 |) 25816'5 3699°7 | 1 i » | 27021°6 3870°7 | 1 > » | 25827°8 | 3698°8 | 1 ” » | 27028-2 3867°6 | 3 ” » | 25848°5 | 36971 | 1 1:02} ,, | 27040°6 3864°7 | 2 ” » | 25867°9 3696°1 | 1 5S » | 27047°9 38617 | 1 ” » | 25888-0 3695°3 | 1 ¥ » | 270538 3856°6 | 2 1:06) 4, |) 25922°3 3694°8 | 1 ” » | 27057°5 3853°8 | 1 ” » | 20941°1 3694°5 | 1 4 » | 27059°7 8852°2 | 1 os » | 25951°9 3693:2 | 1 3 » | 27069:2 3850°9 | 1 e » | 25960°7 3692°3 | 1 » » | 270758 38452 | 1 # » | 25999°1 3690°7 | 1 + » | 270875 3833-2 | 1 “ », | 26080°6 | 3689°2 | 1 ae » | 27098°5 3830°7 | 1 ” » | 26097°6 | 3688°2 | 1 ” » | 27105°9 3820°6 | 1 ” » | 26166°6 3686°3 | 1 ” » | 27119°9 3807°3 | 1 1:05 | 7-4) 26257°9 36861 | 1 ” x | 27121°3 &e. &c. | numer- 36841 | 1 *” » | 271361 ous faint 3681°6 | 1 “f TT) 271544 lines 3680°7 | 1 » » | 27161:0 z 37286 | 2s, _,| 1°03] 7-6} 26812:2 3679°8 | 1 ” » | 271677 { 3728:0 | 1s a| » | 7:6) 26816-4 3676°6 | 1 » » | 27919°3 3726-2 | 3 |byS| ,, » | 26829°4 36760 | 1 + an | 2095's 37251 | 1 A} » » | 26837°3 3675'1 | 1 ” » | 27202°4 3723°6 | 1 seal) 95 » | 26848°1 36711 | 1 ” » | 27232°1 3722°6 | 2 ci Rees », | 26855°3 3670°6 | 1 ” 9» | 272385°8 3722°3 | 1 ” » | 26857°5 3669°9 | 1 ” » | 27241:0 B3721°4 | 3 a » | 268640] &c. &c. | numer- Sith | 1 % », | 26866:2 ious faint *3720°4 | 1 % » | 26871°2 || lines 3719°6 | 3 s » | 26877-0 || © 37183 | 3 ” » | 26886°4 a3500°1 | 1 } brs | 0°98) 8:1) 28562°5 37170 | 3 ” » | 26895°8 B3495'0 | 1 iq | 0:97] ,, | 28604°2 | Foro |) J as », | 26903°8 5 | 37152 | 3 5 » | 26908°8 Le) | 37142 | 1 ” » | 2691671 a3274°5 | 1 \ brs | 0°92] 87] 305303. 3713:2 | 3 » | s | 26923°3| 632681) Tf | » | | 305902) 3712:0 | 2 or +» | 26932°1 eS 3711°0 | 3 rn » | 26939°3|| &c. &c. | numer- 3709°4 | 1 (4 » | 26950°9 ous faint 370877 | 1 5 » | 26956-0 lines ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 317 OxycEn Coat-Gas (FLAME SPECTRUM). costae ‘Phil. Trans.’ clxxxv. 162 (1894). Wave. Lae ‘ Oscillation ] leneth _ and Previous Measurements Frequency s Character | in Vacuo ee \ | winst edge 56347 Watts 5635-43 K. & BR. } i{ 176064 Bey | Second edge | © | 55853 558550, | { es aor sty, | eee ae | 17988-7 5520 J | Third “A : 5542°3., ~=— 5540°86 he 1} 181143 5492 | Fourth ,, Ss | 55035 ., 5492°8 PiazziSmyth | 18202 5473 Fifth ,, )&| 54784 ., 5473-0 % id 18267 5446 Sixth , | 4 | 5440 ,, 54488 ss » | 18355°5 | pie2 | Seventh, |B] 525, (| || Std 5399 Kighth , | 6 18516 5872 Ninth ,, | 18609 5193 Tenth a | 19252-2 5170 First 2, 1 5165 » 9165:241 Rowland | 19336-2 5138 Second ,,) 9 5130-4 ,, 5129°8 Piazzi Smyth | 19457-9 5098 | Third 4) h. | 51000 ,, 5097-9 Fievez 19608 6086 | Fourth ,\ 171410 || 4044-29 8s 24718°8 172303 || (3447-49 | 6s 28997°8 17288:0 | { 3446°49 8s 29006°2 186516 | { 3217°76 4s 31068:0 18720'7 || | 3217-27 6s 31072°7 24700°1 | | | A strong continuous spectrum from 4610 to 3440. Cadmium yields one line only (the least refrangible of the triplets at cadmium 17) 326117. Oscillation frequency 30654-4. Zinc and zinc oxide give nothing but a continuous spectrum. Catctum FLUORIDE. OXYHYDROGEN (FLAME SPECTRUM). | Hartley : ‘Phil. Trans.’ clxxxv. 179 (1894). | : Oscillation : Oscillation Intensity and} 7, | as Intensity and | Wave-length | Gharaccer aoe cad | Wave-length ira tte pieces |, 62158 eb 16090 | 5352°5 | 4 18678 | 6009 1 | 16638 || 6316 | f 1 18807 | 5739 lactis | { 17420 | 5316 | a 18807 55835 J {17905 | 5303°5 | eet 5583°5 os f17905 || 4231* ds 23630 5503 | 18166 | * Probably Kayser and Runge’s Calcium line 4226-91. _ ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 321 2 SrrRoNTIUM OXIDE. OXYHYDROGEN (FLAME SPECTRUM). Hartley: ‘ Phil. Trans.’ clxxxv. 179 (1894). . _ =— 3 Oscillation : Oscillation Intensity and Intensity and Wave-length 2 Frequency || Wave-length ‘ 7 Frequenc Character ma Vanna g Character a Vacn aS | 6085 } b 16430 4591 sv? 21774 6053 16515 *4228 1 23644 5870? line 2s 17032 4216°5 1 23693 *5547 2n 18023 *4079 1 24510 *4609 4s 21691 : * Kayser and Runge record lines in the are-spectrum of strontium at 5543-49, — 4607°52, 4226°91, and 4077°88. Barium OXIbE. E OXYHYDROGEN (FLAME SPECTRUM). ; Hartley: ‘ Phil. Trans.’ clxxxv. 180 (1894). ; é Oscillation : Oscillation Intensity and 2 Intensity and Wave-length Frequency Wave-length Frequenc 8 Character Sony Ut 5 Character ce 2 ed 5720 17478 5384 = J 18567 5712 2b 17503 || —~«6356 18665 5697 | 17546 5322) a 18784 5690 7 strong band 17570 5221 ¢ 19149 5660 (overlap- 17662 5162 b { 19368 5619°5 ping a weak 17790 | 30895 s | 19642 | one) 4932 20269 5587 17895 4887} b 20456 5555 17997 4862'5 | | \ 20559 5499 br 18178 4833 20684 } 5544 18032 4715 : 21202 | 5503 18163 || 4602} | Pvery faint, | 31506 MaGnesium OXIDE. OXYHYDROGEN (FLAME SPECTRUM). Hartley : ‘ Phil. Trans.’ clxxxv. 181 (1894). A 38 > Ae Po 4 Intensity and : aes | Wave-length Gharkcter Previous Measurements B 3 2 és 3) 3929 25447 3885 | br 25752 3874 25805 3856 ) 4b° 25929 3852 43 25955 3834 br 26074 3805 6b* 26269 3805 1b 26269 3739 2b 26734 9 seg re bY aac near M and cag eid: Sie 3709 Bb ciated bands. 26950 3682 6bY 27151 3852 8s Mg. 2852:22 K. & R. 35050 1895. y on REPORT—1895. CALCIUM OXIDE. OXYHYDROGEN (FLAME SPECTRUM) Hartley : ‘ Phil. Trans.’ clxxxv. 182 (1894). r Intensity and - Oxciliation, Wave-length Ghar Previous Measurements Frequency in aracter Wace 6253 | 4b’ 15988 6116 | 16351 6075 \ 2br | 16463 5895 | ‘ 16964 5739 4b* 17424 5598 8b* | Ca 5594-64 K. & R. 17862 5485 } 18233 5445 2b¥ 18363 5493 | 18440 5390 L | 18545 5359 ~b | 18660 5341 18724 5322 18791 5304 2b’ 18852 4222 | 8br Ca 422691 K. & R. | 23681 4215 | | 23717 PuHosPHoRUS PENTOXIDE. OXYHYDROGEN (FLAME SPECTRUM). Hartley: ‘ Phil. Trans.’ clxxxv. 183 (1894). [ Oscillation Wave-length Intensity and | Previous Measurements Frequency in Character | Vacuo 3279 Is | 30488 3274 Is | 30535 3271 1s | | 30563 3268 Is 30591 3255 1s 30713 3245 Is / | * 30808 ARSENIC. OXYHYDROGEN (FLAME SPECTRUM). Hartley : ‘ Phil. Trans.’ clxxxv. 183 (1894). Intute and | Oscillation Wave-length EDS yon Previous Measuremcnts Frequency in Character | Vacate | ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 323 SELENIUM. OXYHYDROGEN (FLAME SPECTRUM). Hartley : ‘ Phil. Trans.’ clxxxv. 184 (1894). Intensity and . as Wave-length Char y Previous Measurements Frequeney in haracter Vann 4890 } 204439 4816 | by 20757°8 4804 } 20811 4746 br 4745 Salet | 21064°7 4720 \ | 21180 4676. br 4675 Pliicker & Hittorf 21381 4643 | 21529 4599 | br 21738 4569°5 21878°6 4491°5 \ br 22258°2 4407°5 br 22682 4339 br 23042 4299 br 23253:0 4222 by 236769 4170°5 by 23969'8 4124 br | 24242-4 4093 by | 24426 4041 br 24738 3976°5 br | 25141°1 3941°5 br 1 25364:3 3921°5 br 25500°3 3883 br | 25744:2 3851 by 25958 3827 br 26122°2 3796 br 26335°4 3749 by 26664 3733 br 26780 3707 by 26994 TELLURIUM. OXYHYDROGEN (FLAME SPECTRUM). Hartley : ‘ Phil. Trans.’ clxxxv. 185 (1894). Intensity and . Oseienos Wave-length Ch. y Previous Measurements Frequency in aracter Vacho 4818 2b 4820 Salet 20749 4760 4b 4767 21001 4702°5 b 21258°6 4668°5 b 4670 21414°6 4648 b 21510 4620°5 b 21635 4593 b : 21765 4580 b 21829 4532 b 220484 4495 b 22240 4470 b 4470 22365 4426 br 22589 4397 br 4400 22735 4379 br | 4378 22831 Pars 324 REPORT—1895. TELLURIUM —continued. - Oscillation Wave-length mi teow! and Previous Measurements Frequency AE in Vacuo 4335 2by 230641 4325 1b’ 4324°6 23206 4211 3bv 23740°9 4201 4200 23802°8 4179) {| i 41807 H.& A. 23923 4163 f ; 4170°3 H.& A. 24012'8 4151°5 by 24080'8 4130°5 br 24202'9 4120 4109-7 H.& A. 24265 4107 } 24340 4098 2 b 24393°6 4085 | 24471 4072°5 br 4072°7 H. & A. 24548°7 4025°6 | 24835°5 3999 by 24997°4 3937 by 25391°3 3880 br 25768 3769 by 265260 3708°5 by 26956'9 3661 by 23710°0 3604 by 27736 3560 lb 28083°6 3383°5 | 48 3382°4 H. & A. 29547 3281 4s 32800 __—,, 30469°S 3273 4s 32734, 30541 3248 4s 32468, 30781°9 ANTIMONY. OXYHYDROGEN (FLAME SPECTRUM). Hartley : ‘ Phil. Trans.’ clxxxv. 187 (1894). Rear lcrctli Intensity and Praviouaill : t Be ave-lengt Character revious Measurements nequenny in 6511 by 18139 4675°5 | 21834 4503 J by 22203°4 4399°6 2br 22740 4273 2bY 23398 4132 2bv 24195°7 4079 2by 24511 4051 2b" 24676 4038°5 1br 24754°5 3990 lbY 25056 3949°8 by 25304 39365 br 25403 3913 by 25550 3910 by 25571 3890 by 25700 3853 br 25947 3813°5 by 26215 3778 by 26462°1 3751-9 by 26646 —— ee a ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ANTIMONY— continued. ELEMENTS. 325 Taorecbouand : Oscillation Wave-length Cares tér Previous Measurements Frequency in Vacuo 3748°5 br 26757 3700 br 27019 3686°5 Is 271179 { 3676 Is 271958 3661 2br 27306 3664 2bY 27434 3626 2br 27571 3602 2b’ 27752 3573 2b* 27981 BIsMUTH. OXYHYDROGEN (FLAME SPECTRUM). Hartley : ‘ Phil. Trans.,’ clxxxv. 188 (1894). Hitensit a : Oscillation Wave-length reise y au Previous Measurements Frequency in aracter Varco 5805°5 17220 5714°2 | s | by 17495 5215°7 bY; 17802°4 5549 lb 18005°8 5422 1b’ 18438 5333 1b’ 18745 5310-1 | 1b 18827 5292 | 1b 18890°3 4850°5 | 1b’ 20609 47245 | lb 21159 47145 8b 21205 4707 s 21241 4691 br 21309°6 4672°8 br 21394 4632 br 21584°5 4582 br 21820 4544 by 220014 4516°5 by 22135 4484 br 22295 4441°5 by 22508 4420 by 22619 4399 by 22727 4382°5 br 22811 71373°5 1 22859 4353°5 22964 4366 by 22898'1 43212 s 23134 4256°5 py 23492 3872°5 by 25816-2 3845 br 26001 3752 by 26646 3652 br 273348 3527-9 2s 28342 35179 2s 28409 3510 5 2s 28467 3067 4s Water 3067-2 L. & D. 32592 326 REPORT—1895. BISMUTH—continued. Oscillation Wave-length ert gens Previous Measurements i in acuo 3023'8 2s Bi 3023°8 H. & A. 33061 2992-2 2s Bi 2992'2 sé, 33376 2983°1 2s Bi 29829 __s, 33431 2937°5 2s Bi 2937°5 ,, 34021 2900:2 2s Ag 29016, 34473 2897°2 | 2s BU23897-2, “4,s 34501 Leap. OXYHYDROGEN (FLAME SPECTRUM). Hartley: ‘Phil. Trans.’ clxxxv. 190 (1894). Intensity and P Cees Wave-length Ch ya Previous Measurements Frequency in aracter Weve 5675 by 17616 5620°5 by PbO 5615 Mitscherlich 17786 5585 17898°6 5460 | b PbO 5460 3 18301 5400 br 18512°4 5340 by PbO 5328 . 18721°4 5241 | 19074 | 52105 by | PbO 5220 5 19188 5194 19247 slut by | PbO 5144 = 194512 5051 by 19792 4980°5 br PbO 4993 is 20073 4961 2b 20152 4955 2b 20175 4925°5 2b 20296 4914°5 2b | PbO 4913 5, 20342 4901°5 2b 20396°9 4896 2b | PbO 4880 5 20418 4858 2b | PbO 4852 53 20579 4824 by PbO 4825 ay 20722°8 4748 by 21054:7 4707 by 21237°6 4657 br | PbO 4664 ts 21468 4608 pY | 21696°5 4597-5 by | PhO 4593 5 21745 4508°5 by 22173 4455 s PbO 4468 7s 22440 4370°5 by PbO 4381 3 22875 | 4314-5 Rs 23171 4225°5 | br 23659 4163 bY 24015 4140°5 Abe 24145°7 rR 4062°5 Liveing and p Sn 4059 6s Pb { pir Resets 246316 4028 by 24819 3985 by 25070 3954 by 25283 3913 br 255473 3880 by 25766 > ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 327 LEap—continued. 1 Ww feneth Intensity and Previ M t ES ito nade q ave-lengt Character _ Previous Measurements wy vent in 3839 by 26043 83805 bY 26275 3783 br 26431 3740°5 bY 26727 371575 by 26906 3684 8s 27138 36715 1bY 27229 3655 1b’ 27349 3639°5 8s 27469 3610 by 27691 3594 bY 27817 3592-5 bY 27828°6 3571 by 279936 3555 by 28119 3501-5 bY 28552 3486 ay! 28677 3447 2b’ 29004 34315 2b’ ’ 29133 3405 bY 29359 3368 1bY 29686 3352°5 1b’ 29820 8845 1b’ 29890 | 3320 1bY 80111 i 3a0T ips 30226 3304 by 30260°9 3264 ‘bY 30626 » 3209°5 2by 31148 (2832°2) 2s 35284 TIN. OXYHYDROGEN (FLAME SPECTRUM). Hartley: ‘Phil. Trans.’ clxxxvi. 193 (1894). Intensity and . | Gecillation Piieactae Previous Measurements Freguens in bY , 21416 bY ; 21472 2br 4600 Salet 21689°5 2bv 21939 2b’ . 22062 2by | 22189 by / 22545 by | 22444-3 2b” 22882 2b’ i 22997 -4 bY 23222 by y 23439 bY : 4240 Salet j 23562°9 bY 23681 bY 24220 bY 24271 by 4080 Salet 24448°6 398 REPORT—1895. TIN—continued. Oscillation sity ¢ ¥ Frequency in Boeelenoas Intensity. and Previcus Measurements Ea ; 247865 4033 by 25113 3981 br 25278 3955 br 25588 3907 by 25828 3871 br 26048 3841 b® 26125 3827 br 26237 3810 by 26416 3787 2b 26581 3761 2b” 26822 3727 8bv 27046 3696 8bv 27632 3618 2b* 27849 3590 6bY 28182 3547 2br 28645 3490 6by 28969:3 3451 2b 29220 3421 4b 29454-1 3394 4b 30028-0 3329-5 8br 30307 3298°5 2b 30593 3268 6br 30906 3234-5 4b 31181°6 3206 5by 31452 3179 6br 32301 3095 4b 32573 3068-6 4br 32998 3038°8 lb 33177:0 3031 lbv 33444 2989 lb ub be SILVER. OXYHYDROGEN (FLAME SPECTRUM). Hartley: ‘ Phil. Trans.’ clxxxv. 195 (1894). - Oscillation ; Bled Frequency in Wave-length atch 2 E eyes aa Vacuo | | : 17791:7 5556'7 | 1s 55566 Thalén ] (ascatten) 181276 5515:0 Is n4ae-6 J 18231 5483°7 | Is 5465°66 K.& BR 18298°6 5463°4 | Is 2 : ‘ 21288 4696-0 Wistiband 4669 L. de B. 214964 pe ita a 21657 46165 | band 4622 L. de B. 217756 4591-onfus | ae ban r 21907°3 45634} | 3.4 bend 4570 L. de B. }(Angstrém) 22050°7 4533-4 f | z 221231 45190) | band 4518 L. de B. 22262:0 44909)f | Pe 22361°3 4470°9 \ Benen 4475:1 Thalén 22467 suo sie | Pa Tae 22594 4424-8 | | Gil hand 22677-0 4408-6 CN WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 329 SILVER—continued. Oscillation Wave length Tei en Previous Measurements Heaney in 43962 22741 4373°5 7th band 4396 L. de B. 92859 4360°7 0 22926 4347-0} | Sth band 22998-2 43309 23084 4300°5 9th band 23246-0 4294-7 23278°1 4283-2 \ 10th band 23341 4273-9 93392 4258-0 11th band 23478-3 4944-9 23529 4938-2 ; b 23588 4231-0 23628 4176-4 239375 4156-4 b 4052-7 4147-4 24105 4102-0 2s 24372 4091-0 9s 24437°6 4088-0 Qs 24455 4030°3 3 24810 3795-4 re 26340 3775-2 Is 26481 37127 Te 26926 3672-0 1s 27294 3631°5 Qs 27529-4 35765 2s 27952 3539°5 2s 3541°3 H. & A. 28245-4 3518-4 2s 284135 3510-0 } 2s 28481-3 289523 28971-1 br Ist group* ae 29019 29052°5 29090°4. 29127 3431-8 s | 29131 3421°8 s 29216 3418°5 s 29244-2 s s 3418-1 29248 3415-1 by 2nd group 29274 34105 4s 29313 3407-0 5s 29343-5 3403-2 6s 29375°4 3401-0 | Ts 29394-9 3397°8 | 8s 29423-1 3395-0 29447 29469 29496 29523°9 33830 K. & R. re: 295922 2962571 br 3rd group Bre 29735°1 3362°2 | 330 . REPORT—1895. SILVER—continued. Oscillation Wave-length ae Previous Measurements | wes ten in == | and § SESE RS eet anes fe 3359°5 | s | 29758 33582 | os | 29770 3357-7 | s 29775 33548 | s | Third group 29809°7 33500 | 3s | (of 19 lines) . 29843 3347-2 | 4s | 29877:2 a 5s | 29879-0 3341-6 6s 2991 7-1 3336-4 | In 29964°7 33338 | In 29987 3331°7 In Fourth group 30007 33304 In; (of 6 lines) 30019 al | in| 30036 0 3327-4 in | | 30043-0 3319-9\ by 30112 3315-3 by | 30154 3309°2 by 30209:7 3305°5 br| Group of | | 302436 3297°3 \ by} 9 narrow | 30319°9 3293°5 br bands | 303449 3289-2 by 30393°9 3285°5 by ‘ 30428 32821 | ‘bv 30459 3276°4 / | Sbr 328080 K. & R. 30512 3271°3 2s 30560°5 3269°3 s | 30579 Tron. OXYHYDROGEN (FLAME SPECTRUM). Hartley: ‘ Phil. Trans.’ clxxxv. 199 (1894). * Double. + Present also in the spectrum of ferric oxide. I : a Oscilla ion Wave-length pee! an Previous Measurements | Frequency in aracter | SWiata feat acne 59277 | 593025 K. & R. |: 16865 57385 lb 17421 56898 | 17570 5689°8 ) b 17570 5619-4 | b | 17790 55943 b | 17870 5537°1 b | 18055 5385 b 18565 53248 5324°31 + ; 18775 5266°5 5266-72 ~—,, 18983°3 4479°3 4479-73 5, 22319 4459°7 | 4469-24 22417 4426-7 | 4427-44 ,, 22584 4405°7 | 440488 _,, 22692 4384-0 4383-70 Ss | 22804 43768 R437604 —,,, | 22842 4326°2 R4325:92 23109 ' G4308°5 R4307°96 23204 *4272°4 4271:93 3 23400 || Due to Manganese. _ R. A line marked R is one of Rowland’s ‘normal’ lines, ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 331 ITRON—continued. Intensity and Oscillation Wave-length Character Previous Measurements me in 4266'9 R4267:97 K. & R. 23430 4071°5 4071:99° +) ., 24555 4058°3 405830, 24633°6 4052-4 505275, 24669°8 4047°5 404590, 24700 4031-7 403084, 24796 4019°8 Mn 248695 4002°9 400533, 24975 3998-16, 3996°8 }399749 25013 $3980°6 398187, 25115 +3926°6 3928-05, 254583 $3921-1 3923-00 __,, 25496 3915-7 R3916-82 i, 25531 (390400, 3904-2 { ee 25606 $3900-4 _ 389980. 25631-2 3897'S 3898-05, 25648 $3896°5 389575, 25657 3894°6 3894-09 _, 25669 : (389202 _,, ADR 3891-5 389096 256902 3888-2 388863, 25711 388638, 3885:1 388561 25732 3880-2 25765 13877-6 387832 i, 25782°4 3874:3 387388 _,, 25804 $3860°5 386003, 25896 $3858-9 3859-49, 25907 3853°7 3854-51 25941 3845-4 384696 ,, 25998 3841-4 3841-19 26025 3839°1 384058, 26040 4 (383648, 3835°2 1383437 26067 $3825°9 3826-04, 26130 3821°5 leserr 26159 438212 pease er eat: 26163 13819°7 382056 _,, 26172°2 3810-6 3810°89 26235°1 380871 | 380886, 26252 | 3796-1 379513, 2633571 | 8785-2 3786-07, 26410-9 3772°6 37738418), 26497°3 3765°3 STERB0- 1 **, 26548 3763°3 376390 _,, 26565 | +8757-9 375836, 26599 | 3751-9 | 375197, 26645°0 | 3749-4 374961, 26668 3748-1 374839, 26672 3747-6 R3747:09 i, 26676 ; : (374567, : | 3743°5 [374345 26705:0 | 187369 a787-37O",, 26748 | 8735:5 373500, 26763 a peel 3727°78° |, 26815 Bp) 3727-9 3727-18 ,, 26817 332 REPORT—1895. TRoN—continued. : Oscillation Intensity and : . : Wave-length Charzie Previous Measurements ee. in 37223 372269 K. & R, 26857 $3720°2 3720°07 9 26872 3705'5 370570 i, 26969 3688°5 368777 i, 27095 3685'8 3687°58 27134 36816 | 368043 _,, 27154 3648°6 | 3647:99 _,, 27399 3631-0 363162, 27542 36092 360899 27692 N73581°1 358132 si, 27909 3569°6 357023, 27997 3565-0 356550 i, 28020 3531-2 28320 3501°8 350064 28559 13492°3 3490°65 + 28622 3475:5 | eeRaeu” 28752 3460°9 346002, 28827 03440°8 344107 ___s—,, 29045 $3400°2 3440°69 33 29060 3059°1 3059°19 65 32680 $3047-4 3047-71 " 32806 3039°1 304054 32896 : ( 8021°15 i Tt3021°1 | 3020-70 if 33091 NICKEL. OXYHYDROGEN (FLAME SPECTRUM). Hartley: ‘ Phil. Trans.’ clxxxy. 203 (1894). * Also in the spectrum of the flame of nickel tetra-carbony]l. ——— Wave-length Intensity and Previous Measurements (Rowland) Character (Angstrém) *3859 3857°8 L. & D. *3809 38066, *3784 37830, *3776 37750, *3619 36188, *3611 36098, 3599 3597 as *3574 3572 Cornu *3569 3570°8 ,, 3527 35271 L. &. D. 3518 35191, 3613 3514-4, 3503 3501'8 i, 3496 34923 is, 3487 34852, 3475 3470:8) a; 3462 OSOL I es, *3460 3457°9 5, 3453 34529, *3445 3445°7 i, Oscillation Frequency in Vacuo 25893 26248 26419 26478 27620 27687 27777 27972 28012 28339 28417 28459 28539 28599 28667 28769 28870 28892 28954 29017 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 333 NickEL—continucd. Wave-length rey Peat Previous Measurements om haracter Vacuo #3436 | 3487-7 L. & D. 29097 *3433 34330 _,, 29123 *3423 Sao) Lanes; 29205 *3415 34138, 29276 *3392 BEE RES Aer 29469 *3391 33904 =, 29484 *3381 33800 29565 f*33713 ,, *3370 | 33689 29665 *3316 SEG a 30148 ¥3233 Bean Oi ss 30925 CoBALT. OXYHYDROGEN (FLAME SPECTRUM). Hartley : ‘ Phil. Trans.’ clxxxv. 204 (1894). ; : Oscillation Wave-length Intensity and Previous Measurements : (Rowland) Character (Angstrém) sc ca 7: 4119 4120 Huggins 24270 3996 3397°3 L. & D. 25019 3899 39052 ss; 25633 3875 38732, 25797 3847°5 | 38448 ,, 25983 3819°5 27620 3612 36113 SC, 27680 3603 36016 27747 3596 35944, 27797 3578 35749, 27942 3571 35689, 27992 3536 3532°8 i, 28272 3531 35293, 28312 oe 35284, 28327 3527 28344 3517 35177, 28429 3513 35120 _—s, 28459 : 35097 i, 3509°5 35093. 28487 3504 35020 _ sy, 28529 3496 3495°1 28599 3483 34827, 28702 3468 34652, 28827 3463 34622 28870 3461 34606 ,, 28887 3454 34529, 28945 s344g9 i, 3449 (34486 28987 3443 34430, 29037 3432 Spree ae 29129 3415 | 34142, 29277 3413 1 oati7 " 29292 ” 3409 34086, 29328 3405 ; 34085, 29357 334 REPORT—1895. CHROMIUM. OXYHYDROGEN (FLAME SPECTRUM). Hartley : ‘ Phil. Trans.’ clxxxv. 205 (1894). Wave-length Intensity and Previous Measurements Teme (Rowland) Character (Rowland) aati 4290) . s 4289°87 Hasselberg 2330 4277 8 4274-91 ‘ 2337 4255 s 4254-49 + 2349 3607 s 3605-46 . 27716 3595 s 3593°57 oe 27802 3580 | 8 357881 + 27927 ALUMINIUM. OXYHYDROGEN (FLAME SPECTRUM). Hartley: ‘ Phil. Trans.’ clxxxv. 207 (1894). ee ; | . Oscillation Wave-length | specs and | Previous Measurements Frequency in | aracter | Warne 4042 s 24733 3968°3 8 25193 3953°5 s 25287 CoppPER. OXYHYDROGEN (FLAME SPECTRUM). Hartley: ‘ Phil. Trans.’ clxxxv. 207 (1894). Wave-length Intensity and Previous Measurements pettiness Character (Angstrém) acne 5506°5 b 18155 5080 2s 19679 3290 b 3289°9 H. & A, 30389 : 32652 . : 3262°5 b { tice 30643 Copper OXIDE. OXYHYDROGEN (FLAME SPECTRUM). Hartley: ‘ Phil. Trans.’ clxxxv. 208 (1894). ‘ : Oscillation Intensity and Previous Measurements , =r Liao Character (Angstrém) — o 5840 In 17120 5790 2n 17267 5747 4br 17397 5577 Bb 5563 L. de B. 17934 5356 5355 tp 18667 5296 br 5300 + 18875 5241 br 5239 7" 19077 5183 by 5150 3 19293°2 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 335 COPPER OXIDE— continued. Oscillation Intensity and Previous Measurements Th. . paretength Character (ingetiinn) Brees = S 5107 by 5106 L de B. 19582 4957 by 4945 + 20167 4849 be | 4847 3 20616 4777 by 4757 ; 20926 4712 jane 4704 . ‘ 21219°7 4688 br 21324 4644 by 4659 cA 21525°6 4518 br 4522 os 22128 4456 Toe 4436 + 22438 4379 br -| 4353 “3 22833 4328 br 4331 - 23099 4280 br 4281 A 23355:0 4228 br 4217 +4 23643 4096 Is 24405 4080 1s 24507°6 4069 Is | 24569 4053 Is 24664 4040 1s | 24743 4031 1s 24802 4017 Is 24888 3282 4b 30452°8 3256 4b | 30697 MANGANESE. OXYHYDROGEN (KLAME SPECTRUM). Hartley: ‘Phil. Trans.’ clxxxv. 1029 (1895). * Seen also in the spectrum of manganese oxide. aye i Previous Measurements 3 s 3 tl 5 Intensity and revious Beereleneth Character (Rowland) a 3.2 Te *5855 2b Fe 5856:24 Kayser & Runge 17073 5813 s 17197 5800 s Fe 5800:21 rs . 17237 5764 1b* | 17345 5730 1b‘ 17446 5712 1b’ very weak 17503 5692 by 17563 #5AQ2 br Fe 5624-70 5 ch 17781 5598 3b 17858 | *5591 br Fe 5592°6 & ce 17881 | *5571 s Fe 5573:05 x . 17945 5556 br 17995 5532 8 18072 5500 s 18175 | *5478 s Fe 6476°82 o + 18250 — «6465 br 18293 — -*5445 s Fe 544705 —,, % 18360 — -*5438 s 18385 — *5402 4b* 13505 ia #539] b Fe 5393°30 a ” 18543 336 REPORT—1895. MANGANESE—continued. Wave length Intensity and Character Previous Measurements *5370'5 5364 *5347 *5315 *5270 *5235 *5199 *5166 *4830 *4791°5 *4762 *4064 *4056 *4049°5 *4041°3 *4036°5 *4029°5 *3894 7 *3874 *3860 *3847 *3835 3827 *3824 *3808 *3803 3764 *3621 *3612 *3607'5 *3604 *3600 *3589 *3587 *3578 *3576 *3571 *3568 *3566 *3562 *3549 *3543 *3536 *3554 *3533 *3530°5 *3529°5 3528 *3525 *3524 3515°5 3514°5 *3513 *3511 bY weak ” S weak s doubtful s ” DNENDMDMNANMNANDUAWDBMNM Fe 5371-62 Kayser & Runge Fe 5316°85 5 2 Fe 527004 ” 3 Fe 5233-05 3) + Fe 5198-82 + + Fe 5167°50 - ” Fe 4832°84 5 F Mn 4762:2 Thalén Mn 4063°6 Thalén, Fe 406363 K. & R. Mn 4055'5 Thalén Mn 4049-0 Thalén Mn 4041°6 Thalén Mn 4035°6 Cornu Mn 40306 _,, Fe 3895'75 K. & R. 403316 ,, 4035°76 K.&R. | Fe 4030°84_ _,, Fe 386003 __,, Fe 383437 __,, Fe 382458 ss, Fe 380547 ss, Fe 362161 Fe 3608:99 _,, Fe 3570°23 Fe | | \ Oscillation requency io Vacuo i ioe) lor) rm or 18637 18698 18810 18968 19095 19230 20696 20864 20992 24598 24649 24687 24735 | 24766 24810 25676 25808 25898 25985 | 26070 | 26125 26143 26255 26289 27607 27677 27712 27737 27792 27852 27870 27937 27954 28000 28020 28037 28067 28167 28217 28274 28288 28299 28317 28322 28342 28358 28367 28437 28447 28454 28475 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 337 MANGANESE—continued. ee a Oscillation Wave-length sada rat Previous Measurements Frequency in aracter Vacuo #3507 s doubtful 28504 ¥*3503 s 4 Fe 3500°64 K. & R. 28537 *3498 8 i 28577 *3497 8 i Fe 3497:92 __,, 28587 *3493°5 s op 28617 *3185 s as 28685 *3476 s + Fe 3476°75 5: 28762 *3473'5 s z 28782 *3472 s a 28792 *3470°5 8 x Fe 347140 ——,, 28806 #3168 s $ Fe 3468-92, 28824 *3467 8 or) 28834 _ *3465 s is Fe 346595, 28852 *3464°5 s A} 28885 *3461 s f Fe 346002 __,, 28884 *3457 8 a Fe 3458:39 28921 ¥*3453 s “5 Fe 3453:10 _,, 28954 *3448 s 3 28999 *3442 8 = Fe 3441:07 so, 29047 *3437 \ be 29085 #3434 | 29110 *3431 by 29140 *3419 br 29237 *3418 by 29250 *3415 by Fe 341792, 29272 *3413 by 29290 *3410 by 29318 3406 bY 29354 MANGANESE OXIDE. OXYHYDROGEN (FLAME SPECTRUM). Hartley : ‘ Phil. Trans.’ clxxxv. 1033 (1895). * Seen also in the spectrum of the metal manganese. + Bands peculiar to the owide of manganese - Wave-length Intensity and Previons Measurements Be va (Rowland) Character (Angstrém) i He f 5873 by \85 *5856 by 5858 Lecoq de Boisbaudran 17023 L Fe 58562 K. & R. (Rowland) 17071 5827 b 17155 5800 2b { 5807 L. de B. | Fe 5800-21 K. & R. (Rowland) 17235 5752 3bY 5759 L. de B. 17380 5717 3bY 5719 oy 17485 a@\ 5681 3bY 5683 5 17598 | 5645 bY indistinct 5644 Watts 17700 *5622 s Fe 5624-70 K. & R. (Rowland) 17782 5607 by 5607 Watts 17830 *5591 bY Fe 5591 17880 5586 by 5587 L. de B. 17897 1895. Zz 338 MANGANESE OXIDE—continued. REPORT—1895. Wave length ' Intensity and Previous Measurements Character (Angstrém) *5575 2by Fe 5573:05 K. & R. (Rowland). *5474 5473 L. de B. *5443°5 n Mn 5543°1 Thalén *5438 n 5432 by 5433 Watts, 5432 Huggins 5427 by 5427 L. de B. *5405 4s Mn 5406°6 Thalén *5400 4by Mn 5399'9 Thalén, 5398 L. de B. *5368°5 br 5367 L. de B. *5347 lb’ Mn 5348 Huggins *5318 lbr Fe 5316°85 K. & R. (Rowland). *5271 2b’ (E,) Fe 5270°43 K. & R. (Rowland) *5234 3b” Mn. 5233°8 Thalén, (E,) Fe 5269°65 K. & R. (Rowland). *5197 4bv Fe 5198'82 K. & R. *5163 2br 5055 2bv 5018 2br 4976 2bY 4935 s 4896 | Edge of band 4853 Edge of ane} doukbfol *4828 n Fe 4832°84 K. & R. (Rowland). *4790 n arms) | *4762 s Mn 4761-3 Thalén 4749°5 ) 2br 4696 lby 4656 }t | 1b’ 4600 Doubiful 4575 4s SAO UP ae) Libr f Mn 4491-1 Thalén 4457 ff | Mn 44576 ,, 4403 ioe 4293 py 4273 r bY Mn 4271°6 Thalén 4252 &e. &e. Imperfect edges as far as 4226 4226 \ Mn 4227-0 Thalén 4135 by 4133 \ by br Fe 4132°15 K. & R. (Rowland). 4130 J bY 4125°5 | by 4121 3n 4079 4n Mn 40796 Angstrém 4075 2n 4065 In *4062 In Fe 406363 K. & R. (Rowland). *4054 5 4s Mn 4054°3 Thalén *4049F 4s Mn 4048:7 Cornu *4040 4s Mn 40iu'0 ——=», 4b* 4by 4g acuo Vv; Oscillation Frequency in ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 339 Wave-length 3991 3988 #3894 3886 3882 3878 #3873 3869 3866 *3860 #3846 3842 #3833 5 #3894 #3809 3806-5 3752 | 3728 | 3721 i 3715 3670 | 3661 jt 3623 #3621 t #3612 #3609 *3603 #3600 #3588 #3587 #3578 #3576 #3570 43564 #3561-5 #3559°5 } 3553 #3548 #35415 #3539 #3533 #3539 3530 43598-5 #3526 #3524 3523 3521 3520 3518 3513°5 #3513 #3510 #3506 #3502 MANGANESE OXxIDE—continued. Intensity and Character 2s double 4s 8s Previous Measurements (Rowland) Mn 3989:2 ” Mn 3991-7 Lockyer (Angstrém). Fe 3895°75 K. & R. Fe 3886°38 Fe 3878°82 Fe 3860°3 | Fe 3841-19 | Fe 383437 | Fe 382458 ” ” 3806-4 Cornu (Angstriém). Fe 3727°78 E &. Ye 3621:°6L Fe 3608 99 Fe 3605°62 Fe 3570°23 Fe 356550 Fe 3526°51 Fe 3500°64 ” NR. Oscillation Frequency in Vacuo 340 REPORT—1895. MANGANESE OXIDE—continued. | gee Bey, Intensity and Previous Measurements BES Wave-length Chashiner (Rowland) & mie 5a i] *3498 In 28582 ¥*3496'5 In Fe 3497:92 K. & R. 28592 3494 In 28614 8492°5 In 28624 3490°5 In Fe 3490°65 28642 3488°5 In 28657 3487 In 28670 *3485 In 28686 3484 In 28695 3482°5 In 28707 3481 In 28722 34785 In 28741 3477 In Fe 347675 —,, 28754 *3475 } re Fe 3475°52 —,, 28766 *3474 28779 *3471 2s 28799 *3470 2s Fe 3471-40 __,, 28812 *3468 4s Fe 3468:92 __,, 28830 *3466 Is 28841 *3465 2s Fe 3465°95 _s,, 28852 *3463°5 23 28864 *3462 1s Fe 3460-02, 28875 3460°5 2s 28889 *3456 8s Fe 345839 __,, 28927 *345) Is Fe 3453°10 _,, 28970 *3449 28986 3447 br 29005 3445 2b” 29020 3444 2s 29030 *3441 2s Fe 344107 __,, 29051 3439 2s 29070 *3437 a 29088 *3433°5 29117 *3430 br 29148 *3417'5 Is 29252 *3415 s Fe 3415°61 ,, 29277 *3413 8s 29294 *3410 Is 29315 3409 1s 29324 3405 8s 29360 3406 8s 29402 3395 8s 29446 3391 8s 29484 3388 8s 29508 NotTE.—Unless otherwise stated, all wave-lengths are upon Rowland’s scale in air at about 20° C. and 760 mm. pressure. All oscillation frequencies are in vacuo. THE PRODUCTION OF HALOIDS FROM PURE MATERIALS, 34] The Production of Haloids from Pure Materials.—Report of a Com- mittee, consisting of Professor H. E. ArmsrronG, I’.R.S., Professor Wrynpuam R. Dunstan, F.R.S., Mr. C. H. BoTHaMuey, and Mr, W. A. SHENSTONE (Secretary). Tur work of the Committee has been actively continued during a con- siderable part of the past year. The various preliminary difficulties involved in the preparation of pure materials, and especially of chlorine, have now been largely over- come, and it is anticipated that considerable progress will be made during the coming year in investigating the behaviour of highly purified chlorine, and the Committee ask to be reappointed for this purpose. A considerable part of the grant made to meet expenses already incurred in 1894 remains in hand, and therefore it is not necessary to ask for a further grant this year. How shall Agriculture best obtain the Help of Science? By R, Warincton, M.A., F.R.S., Professor of Rural Economy, Oxford. [Ordered by the General Committee to be printed in ewtenso. | Our discussion to-day will, I trust, have practical results. The time is certainly ripe for decided steps being taken. No doubt exists in the mind of any one that British agriculture is in great need of some powerful helping hand, which, in popular phraseology, shall ‘put it on its legs again.’ There is probably also no doubt in the mind of any person in this room that, if the farmer is to be enabled to do his best, agriculture must be advanced from its original condition as an art, and that in future its operations must be conducted with the full assistance of natural science. The so-called ‘practical man’ may indeed believe that the question we have met to discuss will be at once set aside as profitless if we raise the preliminary question, Do you believe that the assistance of natural science will remove agricultural depression ? I answer at once that I do not know that it will, but that this is no reason for declining the aid which science offers. When a sick man calls in a physician he does not ask the preliminary question, Do you promise to restore me to full health ? If the question were asked, the physician would positively decline to make any such promise ; and yet the sick man would place himself unreservedly in the physician’s hands, feeling that he could not do better than make use of the best knowledge of the day on the subject of his complaint. Now agricultural science should mean the best knowledge of the day on the subject of agriculture, and a farmer will surely do wisely to obtain the aid of this knowledge in all his operations. We have now to consider in what manner, by what methods, agricul- ture may best obtain the aid of science. We might divide our answer to this question into two parts. We might say, in the first place, that the science of agriculture is still only in its infancy, and that if agriculture is 342 REPORT—1895. to be effectively aided by science it is necessary that there should be a great increase in the number of practical investigations of agricultural questions. In the second place, we should add, that all the investigations already made, or to be carried out, will fail of practical utility if the farmer remains uninformed of the knowledge thus acquired. Our answer would thus be, that we require, firstly, an extended system of practical investiga- tions; and, secondly, an effective scheme of agricultural education. A]] that. will be said to-day could probably be classed under one or other of these two heads. I propose, however, in these opening remarks to adopt a less. logical division of the subject. In order that our discussion may not assume an academic character, but may, if possible, lead to some practica} result, I will at once descend into the region of practical politics, and endeavour to answer the question by pointing out what can most usefully be done by (1) a Board of Agriculture, and (2) by County Councils, to accomplish the objects of agricultural investigation and agricultural edu- cation, which we believe to be so important. There are certain kinds of work which can be accomplished best by a central organisation ; work which is of general, national importance ; work which is necessary to form the basis of future developments. Such work should be at once undertaken by the Government, through a Depart- ment of Agriculture. We need a really complete agricultural and horticultural library, freely open to the public. The literature of the subject is extremely large and rapidly increasing ; much of it is quite beyond the reach of a private individual, while it is of too special a character to be found in our ordinary public libraries. To give one illustration. There are at the present time about 300 fully equipped experiment stations in Europe and America, besides many smailer institutions. The results of their in- vestigations are published in numerous reports and journals in many janguages. No person is able at present to refer to more than a small part of this literature. Instead of consulting the original papers, one is generally obliged to be content with the meagre abstracts furnished by a German Jahresbericht or Centralblatt, and whatever does not find entrance into these periodicals is lost to the general public. As an illustration of what may be done in this direction by an energetic Board of Agriculture, I may mention that the Department of Agriculture in the United States compiles a card catalogue of all the published work of the fifty-five American experiment stations, and supplies a copy of this catalogue to each station. We need also an English journal published monthly, in which the results of the most important agricultural investigations should be made accessible to the general scientific public. The advantage of this to teachers and investigators would be very great. As such a journal could not be expected to pay its expenses, it should be published for the benefit of the country by the Government. The American ‘Experiment Station Record’ is an example of work done in this direction: it is chiefly, but not exclusively, concerned with the investigations made at the American stations. Another piece of work which belongs peculiarly to a central department is the collection and preparation of national statistics. Statistics of acreage under different crops, with the annual and average produce per acre, and the number of live stock in the United Kingdom, are collected and published by the present Board. The Board that we desire would go much further = HOW SHALL AGRICULTURE BEST OBTAIN THE HELP OF SCIENCE? 343 in this direction. We have at the present time no accurate idea of what is the average composition of any portion of our agricultural produce, for the simple reason that the collection of the scattered analyses, the rejection of imperfect work, and the averaging of the remainder is so large an under- taking that no private individual has had the courage to attempt the task. The results of this present lack of national information are not unimport- ant. We are obliged at the present time to employ German averages for all purposes of teaching or calculation. These averages are in the main prepared from German analyses, and relate to crops and foods grown in a different climate, and under different conditions, to our own. In the United States, the want of national statistics respecting the composition of foods and crops has been supplied by their Department of Agriculture, which has published in one volume more than 3,000 analyses of American- grown foods, all properly classified and averaged. In the same way the results of American digestion experiments, made exclusively with American foods and American animals, have been collected and pub- lished, thus again obviating the necessity for relying solely on German figures. An efficient Department of Agriculture should be provided with a staff of officers representing all the sciences connected with agriculture ; these officers should be furnished with suitable laboratories, and all the machinery required for carrying out investigations and making reports. Thus equipped the department would be able to attempt the solution of agricultural problems of pressing importance. The work done at this Government institution would also serve as a model for the investigations carried on at the smaller experiment stations. The investigations thus conducted with public money should be of a thoroughly practical character, the results of which would have a direct bearing on the farmer’s work. Let me venture on a single illustration. Persian barley has lately been imported into England in considerable quantity ; its price has been lower than that of any other kind of barley in the market. A question at once arises in the mind of the cattle-feeder, Is it really cheap? Will asovereign expended on these thin, shrivelled grains purchase a greater weight of food substance, and fatten an animal better, than the same money spent on English barley? The farmer can neither make a chemical analysis nor carry out an accurate feeding experiment, but a properly equipped Department of Agriculture could do both, and in a few weeks issue a report which would be of substantial benefit to the farmers of this country. Before leaving this part of the subject let us note what our brethren across the water are doing in this matter. Canada, though a poor country, and with a population of only five millions, has its central agri- cultural laboratories, and its chemists and botanists employed under its Department of Agriculture, and spends 15,000/. a year on the agricultural investigations conducted at the central station at Ottawa and at the four provincial stations. In the United States the annual cost of the in- vestigations carried out by the Central Department of Agriculture at Washington cannot be less than 60,000/., and this is exclusive of the cost of the work done at the fifty-five experiment stations in the various States, towards which 150,000/. is annually contributed by the National Government. ! The figures quoted, both for Canada and the United States, do not include the very considerable sums spent for the same objects by the local governments in these countries, 3844 REPORT—1895. We may certainly congratulate ourselves that we have at last a Board of Agriculture, presided over by a Minister having a seat in the Cabinet. The work done by the Board has already been of considerable benefit to the country. What we desire is that far larger means should be placed at its disposal; that the scope of its work should be enlarged ; and that, especially, it should acquire a distinctly scientific character, which, as we have already remarked, simply means that the best knowledge of the day should be enlisted in the service of agriculture. We shall feel ashamed, I think, when I mention the sum at present devoted by the Board to the purpose of investigation. The grants made for education and investiga- tion in the year 1894-95 may be summarised as follows :— Collegiate centres . : s : 2 EL . £5,550 Dairy institutes . : c - n : 950 Instruction in forestry . : . : 250 Investigations by various associations : ° a 650 7,400 Thus 650/. is the whole sum directly devoted by the Board to the _ purpose of investigation : some portion of the sums contributed to colle- giate centres may, however, be employed for this purpose, as experiments are conducted by some of the colleges thus assisted. The 6,750/. distributed by the Board to educational institutions is very wisely allotted to those giving a complete course of instruction. The provision of a full course of training for teachers should always have the first consideration in any educational movement. In referring to the present national expenditure on agricultural educa- tion we must not omit the grants made by the Department of Science and Art to science schools and classes teaching the principles of agriculture. The total grant amounted in 1893-94 to the sum of 2,937/. The Depart- ment has recently attempted to improve the instruction given in these classes. A new syllabus of the subject has been prepared for the use of the teachers, with suggested experiments, and a few necessary diagrams, The Honours examination has also been made much more thorough. We next turn to the work done in this country by local authorities. This is a very wide subject, and I can only glance at a few points. We all know that a really large sum of national money has been placed in the hands of the local authorities during the last few years, which they can use at their discretion for the purposes of technical and secondary educa- tion. The sum thus placed at the disposal of the local authorities in England for the year 1894-95 amounted to about 744,000/., of which about 600,000/. was actually spent on education. The particular educa- tional objects aided vary, of course, very much in different localities, and it is only in the counties that we can expect to find the teaching of agriculture occupying an important place. The annual grant at the disposal of the English counties somewhat exceeds 400,000/. It is very difficult to tell how much of this is devoted to agricultural purposes. In the case of a few counties, as Kent, Bedfordshire, and Berkshire, it would appear from the figures published in the ‘ Record of Technical and Secondary Education ’! that about one-third of the total grant is 1 T am indebted to the reports in this valuable periodical for much of the informa- tion here given respecting the agricultural work of County Councils. {/* HOW SHALL AGRICULTURE BEST OBTAIN THE HELP OF SCIENCE? 345 allotted to agriculture, but in most counties the proportion is very much less. The mode in which this agricultural education is carried out is, of course, very varied. It may consist simply in money aid to classes under the Department of Science and Art; or the county may have its own travelling lecturers, who deliver short courses on agriculture, horticul- ture, dairy-work, poultry, bee-keeping, and the diseases of animals. Purely technical classes on horse-shoeing, ploughing, hedging, draining, are also common. The most popular, and certainly one of the most useful, of these technical schools is the travelling dairy, by which practical in- struction in butter-making is given at many centres throughout the county. Asa help toa higher grade of instruction than is furnished by these popular classes, the County Councils grant agricultural scholarships available for the courses of instruction at agricultural schools and col- leges, and in some instances at institutions of university rank. In a few cases dairy institutes and agricultural colleges have been established by County Councils, usually by the united action of two or three counties, and in these cases considerable sums are annually set aside for their support. The sketch we have given of County Council work will, how- ever, leave a far too favourable impression if we do not bear in mind that only a portion of the schemes mentioned are generally in use in any one county. As it is clearly most important that these new schemes of agricultural education should be wisely and efficiently carried out, we may profitably devote a few minutes to the consideration of some important points upon attention to which any real success will largely depend. With lads of the age at which they are usually in attendance at elementary schools little can be done in teaching the scientific principles of agriculture ; such lads have not acquired the previous scientific know- ledge necessary for understanding what is to be taught. They may indeed learn off answers to questions either from the blackboard or from a printed text-book, and thus furnished they may pass examinations ; but the know- ledge they have acquired is merely a knowledge of words, and will be of no value to them in after-life. The foundation of habits of observation and logical reasoning must, however, be laid in the elementary school if higher instruction is hereafter to be given. This elementary training may easily be made to have an agricultural bias. No better means of educating a boy’s powers of observation can be found than a study of the individual characters and modes of development of the various crops, weeds, and insects of the farm. When lads have passed through the elementary school their special training should immediately commence ; any delay is most unfavourable to the boy’s development. The time has now come when a distinction has to be made between the students ; some are to be labourers, some are to be farmers. For both technical instruction is required: the arts of agricul- ture have to be mastered.!. The farmer's son, however, requires besides this a higher course of study if scientific principles are to be introduced into his future practice. One great need of the present day is the esta- blishment of secondary agricultural schools, which shall be centres both for ° 1 In some countries, as Ireland and France, instruction in the art of agriculture is given in connection with the elementary schools: this is, of course, possible if the school engagements admit of time being thus spent, and there is convenient land adjoining. 346 REPORT—1895. purely technical and for scientific instruction. The farmer’s son on entering such a school would commence at once his technical training, and he would at the same time commence the study of elementary chemistry and elementary biology and geology. Not till he had gone through elementary courses on these subjects would he be prepared for instruction in the scientific principles of agriculture. It is from well-arranged schemes, in which the instruction proceeds from first to last in a proper order, that the best results are to be expected ; such schemes should gradually be made to take the place of the short mis- cellaneous courses of instruction, imperfect in themselves, and given to an audience unprepared for them. The principal use of popular lectures is undoubtedly to arouse a general interest in the subject, and to show how much there is to be learnt on agricultural matters. Miscellaneous lectures have thus a great value in pioneer work, but it must never be supposed that they can take the place of solid, systematic instruction. Lectures to farmers are undoubtedly of very considerable importance, as they are one of the few means of improving the practice of the present generation, but they are the most difficult of all lectures to carry on efficiently. The lecturer must be thoroughly acquainted with farming practice, and with the conditions which determine profit and loss, or he will bring his science into contempt. The teaching of science as science to an audience of farmers will soon result in an empty room; but keen, practical men will listen carefully to the conclusions drawn from scientific investiga- tions when these can be shown to have a direct bearing upon their daily work. One of the greatest obstacles to the teaching of scientific agriculture in the present day, whether in schools or in evening classes or lectures, is the great lack of competent teachers. The best qualification which a teacher can offer is that of graduate of one of the larger agricultural colleges, but the supply of such men is extremely small. The qualification sufficing for teaching the principles of agriculture under the Department. of Science and Art is an extremely low one,! and should never in itself be accepted as sufficient. A poorly qualified teacher solves all his difficulties by adopting a popular text-book, and teaching this in a literal manner. Unfortunately some of the text-books most largely used entirely fail to represent the present condition of agricultural science, and persistently teach a whole series of exploded errors. Technical committees should not sanction the use of text-books of scientific agriculture which are mere reprints of works written many years ago. County Councils should recollect that all educational machinery re- quires inspection. They act unadvisedly when they try to rid themselves of trouble and responsibility by making grants to Parish Councils for tech- nical education, and then leaving them to direct the work. It is necessary always to ascertain how a teacher does his work. Does he illustrate his lessons by specimens, diagrams, and experiments; or is his object simply to cram for a written examination? Opportunity should be given to teachers to improve themselves by further study. Schemes for Saturday 1 A person becomes qualified to conduct a class under the Department by answering successfully six or seven questions, selected by himself out of twelve or fourteen, from a paper drawn up to suit the capacity of lads of fifteen. ‘The new regulations for the Honours examination, which come into force next year, will provide a much higher qualification, as the successful candidates will in this case have passed two examinations subsequent to the one just named. HOW SHALL AGRICULTURE BEST OBTAIN THE HELP OF SCIENCE? 347 lectures to teachers, or classes for teachers held in the vacation months, are of the greatest use if good men can be secured as instructors. We must now speak of the relations of County Councils to agricultural investigation. This kind of work has been undertaken at present by only a few counties, and by them to a very limited extent: public opinion is, indeed, not nearly so developed upon the subject of investigation as it is on that of education. Practical investigations are, however, urgently required if the operations of agriculture are to be carried out in a scientific manner. The science of agriculture is, in fact, as yet in its infancy, and can be perfected only by well-arranged experiment. There is room for an immense variety of work. Every substance which the farmer uses, every living organism (plant or animal) with which he is concerned, every operation he conducts, must be thoroughly understood if it is to be employed to the best advantage. Great Britain is singularly behind other civilised countries in the work of agricultural investigation. The reason has apparently been very simple. In most European countries, and in the United States and Canada, the initiative has been taken by the Government. Ministers, having a just idea of the conditions on which national prosperity depends, have succeeded in obtaining public funds for the support of experiment stations, institutions provided with laboratories and skilled workers, and devoted to the elucidation of agricultural problems. The German Empire alone has about fifty-four Versuchs- Stationen, without reckoning the public laboratories occupied chiefly with the analysis of manures and seed-testing. In England agricultural investigation has been left to private enterprise, which during the present century has produced one first-class experiment station—that of Rothamsted—of which we are all rightly proud, but which is wholly inadequate for the growing needs of the country. I am not at this moment advocating the immediate creation of many first-class experiment stations, though there is ample scope for such in the hands of competent workers. One first-class station should certainly be at once started under the immediate control of a reorganised Department. of Agriculture, as without this the national investigations, which would become one of the functions of this department, could not be carried out. The great need at the present time is the creation of numerous. local stations, to work upon the practical problems of each locality, and so become centres of scientific teaching and scientific demonstra- tion. If Parliament were to offer to give 1,000/. a year! towards the support of a county experiment station, erected and maintained by the: _ County Council, and subject to the inspection and approval of the De- partment of Agriculture, a great start would be at once made in the right. direction. A few words may be said as to the kind of investigations to be undertaken by a local experiment station. The subjects taken up will of course depend upon the style of farming in the neighbourhood, the object being in every case to bring scientific knowledge and methods into actual touch with the farmer’s work. Some of the experiments would be carried out on selected farms, possessing soils and climates typical of considerable areas in the county. Comparative trials of different Ee ee ee ee eer 1 This should be regarded as a minimum sum. In the United States each State receives 3,000/. annually from the National Exchequer towards the maintenance of __ its experiment station. . 3848 REPORT—1895. varieties of grain, root, or fodder crops upon the various soils of the locality would be most useful.! Farmers usually go on sowing the same kind of seed, or make a change only to something that is well advertised, without ever ascertaining by actual experiment which of the manifold varieties in the market is best fitted for the conditions of their own soil and climate. Other experiments could only be conducted at the experi- ment station. It is to be hoped that comparative trials of the nutritive value of different foods would in all cases be undertaken : on this point our knowledge is sadly deficient.2 The chemical analysis of foods, as conducted at the present day, is no sufficient guide to their feeding value. We need facts as to the actual effect of different foods upon the animal, and we must then seek to bring our methods of analysis into consonance with these facts. Besides actual investigations these local agricultural stations might be made to supply demonstrations which would be invaluable for teaching purposes. If, however, agricultural secondary schools are established, such demonstrations would find their most suitable home in these esta- blishments. It will probably be desired in some cases to make the experi- _ment station a place for the analysis of manures and feeding stuffs for the farmers round. Ifa special assistant is allotted to this kind of work there can be no objection to it ; but it would be folly to allow investi- gations to be interrupted by attention to such matters. At the present time the majority of the County Councils have not made any commencement in agricultural investigations. Those councils which have taken up the subject appear generally to have avoided any responsibility of their own in the matter. The usual course has been to make a grant to some agricultural college, or to some local Chamber of Agriculture, on the understanding that they will carry on experiments in the county. There is surely, however, no reason why a strong agri- cultural committee should not be formed in every county by the addition to their number of experts residing in the county. The experiments at present carried on through the medium of agricultural colleges and Chambers of Agriculture are almost all of one type: they consist of the comparative trials of manures. This style of experiment is indeed the only one which has found general favour in this country. The fact is certainly regrettable, as it exhibits a poverty of idea on the part of the experimenter, and a lack of apprehension of the many serious problems which are awaiting solution. Many important topics have been left unmentioned which will doubt- ~ less be taken up during the discussion which is to follow. My object has been merely to give a brief sketch of the kind of national and local work required if a real effort is to be made to give agriculture the aid of science. ' In Essex and Nottinghamshire a commencement has been made of work of this kind. * In Norfolk valuable experiments have been made on the feeding value of oil- cake containing different percentages of oil. ON THE HIGH-LEVEL FLINT-DRIFT OF THE CHALK. 3849 High-level Flint-drift of the Chalk.—Report of the Committee, consisting of Sir Jonny Evans (Chairman), Mr. B. Harrison (Secretary), Professor J. PrestwicH, and Professor H. G. SEELEY. Drawn up by Mr. B. Harrison. Tur Committee were appointed to investigate the nature and probable age of the High-level Flint-drift in the face of the chalk escarpment near Ightham, which appears to be productive of flakes and other forms of flint probably wrought by the hand of man. This patch of gravel has been preserved upon a promontory of the chalk escarpment, at an altitude of 658 feet. It extends for some 70 yards, and attains a maximum thickness of 5} feet. It is composed chiefly of sharp angular flint, varying in colour from bluish-white to bleached-white. Accompanying this is a quantity of deeply-stained ochreous flints, with here and there pieces of chert, Oldbury stone, and rag. Flakes made by man exist in thousands, and they preponderate over the more elaborately worked specimens. Numerous scrapers, hollow- notched and of horse-shoe shape, were obtained, as well as partially finished implements ; but no perfect large tools, and none with any sign of polishing. The worked-flint material is similar to that spread out in the Holmes- dale valley, where it is accompanied by large somewhat rude implements. Amongst the deep ochreous flints some bear the look characteristic of the plateau specimens. The matrix is usually clayey, of a dark red colour, but in places it is quite chalky, and unstratified. A large quantity of the flints are encrusted with carbonate of lime. With the view of tracing the origin of this bed attention was directed to the ground above, in hope of finding either a Neolithic settlement, or plateau implements am sita. The latter having been traced to a position where an excavation had brought them from a depth of six or seven feet (Pit A), it was decided to dig a pit to obtain a section upon Parsonage Farm, Stanstead, by the kind permission of the owner, Mr. Pink. The excavation was closely watched by Mr. W. J. Lewis Abbott, F.G.S., and myself, and occasional visits were made by the Rev. R. Ashington Bullen, F.G.S , acting under direction of Professor Prestwich, Mr. F. J. C. Spurrel, Mr. Corner, F.G.S., and others interested in the subject. The following is the section (see p. 350). f Work was commenced on October 19, 1894, by digging a pit 12 feet by 6 across. At the top, 2} feet consisted of a stony loam, with a large percentage of ochreous flint, much worn, angular white flint, Tertiary pebbles, and some evidence of southern drift. With a fairly even line of demarcation came a grey Joam containing some small fragments of flint, a few small Tertiary pebbles, and small rudely worked stones scattered throughout at places. At about 5} feet this loam became more clayey, and of a deep rich ochreous colour, overlying a gravel, about 12 inches in thickness, composed of much-worn ochreous flints, some very large, and many Tertiary pebbles. This gravel was hard and compact. From it I secured very many worked implements. Heavy rain now hindered work by filling the pit. Measuring off 12 feet in line we began to dig another pit. 350 REPORT—1895. Pit 1. Parsonaze-farm, near Ash, Kent. umus and drifted material, white flints, pebbles, and many ochreous flints worn and worked. Grey loam, with scattered small pebbles, and a few small worked ochreous flints throughout; the lower part of this deposit was more clayey and deeply ochreous. Gravel, about J2 inches thick, varying, confu- sedly laid, very hard and compact; pebbles, large flints, and many bearing work. Pit 2. Parsonage-farm, near Ash, Kent. Humus and drifted material, white flints, pebbles, and many ochreous flints, worn and * worked ; one piece of Oldbury stone. ‘Grey loam, with scattered small pebbles, and a few small worked ochreous flints throughout ; the lower part of this deposit was more clayey and deeply ochreous. Gravel, about 12 inches, varying, confusedly laid, hard and compact; pebbles, large flints, many bearing work. A few worked flints were found, at 8 feet, in one spot. This pit dug to a depth of 26 ft. passing through sandy loams obliquely bedded; lower Tertiary pebble-. One foot tested by a hop-pitcher (iron bar) ; no sign of chalk, —: . A. Pit dug by the owner in the spring of 1894, to about 10 ft. [Worked flints were found, ani Pit B was sunk immediately adjoining it. ] B. Pit 1. Sunk to the level of the gravel, about 7 ft.; work interrupted by heavy rain. C. Pit 2. Sunk at 12 ft. off toS.W. Gravel found at the same level, 6 to 7 ft. Tertiary loams and sands, sunk through to a depth of 26 ft. Pit No. 2 presented precisely similar conditions, 2} feet of surface drift, the grey loam, with its weathered pebbles and few small worked stones, continuing until the ochreous clayey deposit was reached which _ overlay a continuation of the gravel. In this pit, however, the gravel was much stained at places and hardened throughout by manganese. The seam of gravel proved to be about 12 inches in thickness, varying at places. At one spot in this pit, at a depth of 8 feet, a few worked stones were found lying in a sandy matrix ; but below this, although a depth of 26 feet was pierced, no further evidence of worked tools was found. _ As the object was to investigate the nature of the deposits and to reach the Chalk if possible, the work was continued until a depth of 26 feet was reached when, owing to the men working in danger of a slip, and being so well in the Tertiaries, orders were given to fill in. At 26 _ feet a hop-pitcher (iron bar) was used to pierce about a foot more, but no _ evidence of the chalk was forthcoming. The Volcanic Phenomena of Vesuvius.—Final Report of the Committee, consisting of Mr. H. Baverman (Chairman), Dr. H. J. Jounston Lavis (Secretary), Mr. F. W. Rupier, and Mr. J. J. H. TEAL, appointed for the purpose of Investigating the Volcanic Phenomena of Vesuvius and its Neighbourhood. Tue reporter having since the last meeting of the Association terminated his residence in Naples, the continuous observations of the volcanic phenomena of the district which he has carried on during the last sixteen years have naturally come to an end. It is therefore not considered advisable to ask for the reappointment of the Committee. In closing the work of the Committee the reporter wishes to express his sincere thanks for the valuable aid he has received. An account of the eruption during the early months of this year was published by the reporter in ‘ Nature’ of August 8, 1895. 352 REPORT—1895. The Rute of Erosion of the Sea-coasts of England and Wales, and the Influence of the Artificial Abstraction of Shingle or other Material in that Action.—Fourth Report of the Committee, consisting of Mr. W. Warraker (Chairman), Messrs. J. B. RepMan and J. W. WoopaLL, Major-General Sir A. CuarKke, Admiral Sir E. OmmaNNEY, Admiral Sir GEorGE Nares, Captain J. Parsons, Admiral W. J. L. Waarton, Professor J. Prestwicu, Mr. Epwarp Easton, Mr. J. S. VALENTINE, Professor L. F. VERNON Harcourt, and the late Mr. W. Toptey. and Mr. C. E. Dr Rance (Secretaries). (Drawn up by C. E. DE Rance.) APPENDIX PAGE I.—Summary of Previous Reports ‘ : : 4 : . 854 1s —Information received and collected since 1888 . ‘ 359 Ill.— Various Scheduled Returns: Replies to Printed Queries circulated by the Committee. 372 IV.—Second Chronological L ist of W ‘orks on , the " Coast- changes and Shore- Deposits of England and Wales. By W. WHITAKER, B.A, F.B.S., F.GS., Assoc. Inst. C.E. = : , ; : f : 3 . 388 THE seaboard counties of England and Wales are twenty-nine in number : of these Cornwall has the largest amount of coast, with a curiously indented outline of hard Paleozoic rocks ; the county of Devon stands next with similar rocks, except on the south-eastern const, where Secondary rocks form the coast-line, and the rate of waste is considerable. The counties of Lancashire and Yorkshire stand next, and are margined by Secondary rocks and Drift, and the rate of erosion is excessive. Sussex and Kent stand next as regards length of coast-line, and are wholly composed of more or less soft Secondary and Tertiary deposits, offering a ready prey to the devouring waves, often increased by badly designed works of so-called protection. The last remarks apply to the coasts of the whole of the remaining counties of England, except Northumberland, where Upper Paleozoic Coal-Measures and Permians are being moderately wasted by coast erosion, and Cumberland, where also, through the ancient hard rocks of the Lake District being sea-margined by Coal-Measures and Glacial Drift, very considerable coast erosion is taking place. Similarly in Wales the hard rocks of the Cambrian Mountains are, or were, margined by terraces of soft Coal-Measures and red rocks in Flintshire, Glamorgan- shire, and Pembrokeshire ; and even in the western coast the sites of terraces of Drift once present now underlie high-water mark ; a process which would have been still more marked in North Wales had not the London and North-Western Railway run for so many miles along its base, necessitating that company keeping out the inroads of the sea. Your Committee was appointed in 1881, at York, at the suggestion of the surviving Secretary, who acted as Chairman in that year, his place being taken by Sir John Hawkshaw in 1882, who was succeeded by Mr. R. B. Grantham between 1883 and 1889. Since 1890 Mr. W. Whitaker has been Chairman. 1171, 1172 * Portnabo . . . a . Dolerite dyke 1173, 1174 a5 Benanouran Head 4 : ; | Basalt Co. DoNnEGAL 1175, 1177 Killybegs 5 2 . General view 1176 Donegal. 5 4 zi ” ” Microscopic Rock Srctrions.— Photographed by W. W. Warts, 28 Jermyn Street, S.W. Size 44 x 3} inches. 1194-1205 Tardree, Sandy Braes, | Perlitic cracks in the quartz and matrix and Templepatrick \ of a rhyolite Size 7 x5 inches. 12206-1216 Sulby Glen, &c., Isle of Man . Sections of the ‘ Crush Conglomerates ’ and associated rocks ON PHOTOGRAPHS OF GEOLOGICAL INTEREST. 411 APPENDIX I. Schedule of the collection of Photographs of Geological Interest, as arranged by the Committee appointed by the British Association, forwarded (in accordance with a resolution of the Council) to the Director-General of the Geological Survey, to be deposited in the Museum of Practical Geology, 28 Jermyn Street, London. ARRANGEMENT OF THE COLLECTION OF GEOLOGICAL PHOTOGRAPHS. Nore.—The Committee appointed to undertake the ‘collection, pre- servation, and systematic registration of photographs of geological interest in the United Kingdom’ began its operations in 1889. During the first two years prints were received mounted on cards without restriction as to size. Afterwards, to secure uniformity, a standard mount was adopted, with perforated edges for binding in cases (size 155 x 12 inches). It was not found practicable to transfer the early portion of the collection to the standard-sized mounts in cases. The arrangement of this portion has therefore had te be made in portfolios, boxes and cases of various sizes. When the size is not stated it will be understood that the cases consist of the standard-sized mounts, measuring 155 x 12 inches. Inventory.—-The following are on irregular sized mounts, dimen- sions of the /argest mounts being given below :— CONTENTS. Miscettaneous (I.) Size wp to 21 x 18 inches. No. of Description of Photographs Case, &e. : in Case, &e. Part 1. (a) Series of Mr. G. H. Morton, illustrating the Carboniferous (Cloth Case.) limestone of Llangollen. (b) Series of the Yorkshire Geological and Polytechnic Society. (ce) Series of the Leicester Literary and Philosophicai Society (2). (d) Series of Mr. Ussher, illustrating the granite structures of Dartmoor, &c. (e) Chalk, Co. Antrim (enlargements), by Miss M. K. Andrews * 38 NorTHUMBERLAND AND Duruam (I.) Size wp to 14x10 inches. Part 2. Mr. E. J. Garwood’s (First) Series, illustrating Sections in Coal (Cloth Case.) Measures, &c. . : : : 5 . 5 5 : 14 LANCASHIRE AND Cursutre. Size 14x11 inches. Part 3. Series cf the Liverpool Geological Society and the Leeds Geo- (Cloth Case.) logical Association, kc. . : : : 5 5 : 44 Norra Wates anpD IsLE oF Man (I.) Size 14 x12 inches. Part 4. Series of the Liverpool Geological Society, Leeds Geological (Portfolio.) Association, and Mr. A. O. Walker . ; - 36 TreEvanp (I.) Size 12 x10 inches Part 5. (a) Series of Professor V. Ball, illustrating the Cambrian quartz- (Portfolio.) ites and Boulder beds, drift on Cambrian rocks of Howth, Carboniferous Limestone, &c. (6) Series of Miss Andrews, illustrating Chalk at Kenbane Point, . Antrim basalts and granite boulders, Newcastle . . 25 412 REPORT—1895. YorKSHIRE (I.) Size 13 x10 inches. No. of Description of Photographs Case, &c. in Case, &c. Part 6. (a) Series of the Leeds Geological Association. (Portfolio.) (0) Series of Mr. J. W. Woodall, illustrating effects of recent floods on Chalk : 4 : 4 - : : 60 Misce,Laneous (II.)—Soutuern Counties. Size 17 x12 inches. Part 7. (a) Series of East Kent Natural History Society, illustrating (Portfolio.) Thanet beds and Chalk of the Elham Valley. (b) Views and Sections in Devon, Surrey, Somerset, Berks, and Wilts . : ; : - : : ‘ ‘ 4 24 ScorntanD (I.) Size 13 x 10 inches. Part 8. (a) Series of Professor Heddle and J. A. Harvie Brown, illus- (Portfolio.) trating Caithness, Island of Mull, &c. (4) St. Kilda: Weathering of volcanic rocks (c) Stigmarian roots at Partick . < 5 ° e . . 32 Misceittaneous (III.) Size 16 x 14 inches. Part 9. Series of Mr. J. J. Cole, F.R.A.S., illustrating sections in Dorset, (Box.) Devon, Cornwall, and the Snowdonian region, North Wales : ‘ 5 ‘ ‘ - : 4 - : 18 MIscELLANEOUS (IV.) }-PLATE AND }3-PLATE PuHomos. Size 9x 5 inches. Part 10. (a) Microscopic Sections of Phosphatic Chalk, Taplow. (Case.) (6) Saurian footprints from the Cheshire Trias. (c) Sections in vicinity of the Manchester Ship Canal. (ad) Views in Dorset. (e) Views in Nottingham and Derbyshire . . : : 4 41 The following are all on standard-sized mounts :— NORTHUMBERLAND AND Duruam (II.) Part 11. (a) Mr. Garwood’s Second Series, illustrating Whin Sill, Tees- (Case. ) dale, &c. (0) Mr. G. Hingley’s Series, Marsden Bay, &c. . - 5 : 34 YORKSHIRE (II.) Part 12. (Case.) Series of the Leeds Geological Association and others 5 oe cel Trevanp (II.)—Co. Anrrm. Part 13. Series of Dr. Tempest Anderson, Mr. W. Gray, the Belfast (Case.) Naturalists’ Field Club, Miss M. K. Fae le and Mr. R. Welch A Ec - : 5 84 IRELAND (III.) Part 14. Series of Miss Andrews, Mr. W. Gray, Belfast Naturalists’ Field (Case.) Club, &c., illustrating counties Londonderry, Down, Done- gal, Fermanagh, Clare,and Cork . : : 4 : 67 ON PHOTOGRAPHS OF GEOLOGICAL INTEREST. 413 Scorianp (II.) No. of Description of Photographs Case, &c. in Case, &c, Part 15. Series of Messrs. Valentine, illustrating Staffa and Skye. (Case.) Series of Mr. W. Lamont Howie, illustrating Pillars of Old Red Conglomerate, Morayshire (and Earth Pillars of the Tyrol), the Scottish Highlands Series of the Perthshire Society of Natural Science. Series of Mr. Wilbert Goodchild, arcane ip Sections in the vicinity of Edinburgh, &c. : - 54 Nortu anp Sourn WALEs AnD IsLE or Maw (II.) Part 16. Series of Mr. W. W. Watts, Mr. C. J. Alford, the Manchester (Case.) Geographical aes &c., and of Mr. F. J. Eaton Cre of Man). CHESHIRE, DERBYSHIRE, SHROPSHIRE, AND Monmouta. Part 17. Seriesof Mr. W. W. Watts, Manchester arent eve and (Case.) others c - : 54 Mippiesex, Berks, Herts, Starrorp, WARWICK, AND WORCESTER. Part 18. Illustrating various Sections at Tewkesbury, St. Albans, Nun- (Case.) eaton, &c. . : : : A : : : ; : 26 Dorset, Kent, Hants, CoRNWALL, AND SURREY. Part 19. Series of East Kent and Dover Natural History Society and (Case.) others, illustrating various Sections, &c., and groups of bone and flint implements and teeth, from Kent’s Cavern, Torquay (Mr. A. R. Hunt) é : : e 2 - 81 Total . ‘ ° . - F . 886 APPENDIX II. REFERENCE List oF PHOTOGRAPHS ILLUSTRATING GEOLOGICAL Papers AND MeEmnorrs. Geologists’ Association. ‘ Proceedings.’ Vol. XIII., Part 9. August, 1894. Illustrating Paper on ‘The Geology of South Shropshire,’ by Professor C. Lapworrn, LL.D., F.R.S., and W. W. Warts, M.A., F.G.S. (From Negative by Rev. J. MacLzon, of Hope.) Regd. No. View of Roundtain,looking Arenig Lava. (From Negatives by W. W. North WATTS, M.A.) 87 E. Crags, of Todleth . - Columnar Andesite 84 Quarry at Tasgar. . Upper Arenig ash-bed, with fossiliferous shales at base #35 Section at Hope Rectory . Contorted ash-bed in Middle Arenig shales 80 Section at Hope Dingle . Hope shales and ash-beds; Llandovery shales 436 Road cutting, Wenlock Wenlock Limestone Edge Geological Magazine, Dec. 10, Vol. II., 1894. Plate XL. (From Nega- tives by C. C. Howarth.) 1179-1182 Cannock Chase . : . ‘Pitted’ pebbles from Bunter Con- glomerates 414 REPORT—1895. Geological Society. ‘Quarterly Journal.’ Vol. L., 1894. Plate XVIII. and page 371. Figs. 1-6. (From Negatives by W. W. Warts.) 1194-1205 Tardree, Sandy Braes, &c. . Perlitic cracks in Quartz Geological Society. ‘Quarterly Journal.’ Vol. LI., 1895. Plates XX. and XXI. (From Negatives by W. W. Warts.) 1206-1215 Sulby Glen, &c., Isle of Microscopic sections of ‘Crush Conglome- Man rates’ Hertfordshire Natural History Society. ‘Transactions.’ Vol. VII., Part 8. February 1894. Illustrating Report on Field Meetings of the Society, by Jonn Hopxinsoy, F.G.S. Photographed by Mr. Horxtnson. 733 St. Albans—Section on) ee ; Midland Railway J Chalk, Tertiaries, and Drift 734 St. Albans : : . Section of Hertfordshire Conglomerate ‘Liverpool Geological Association. ‘Journal.’ Vol. XIV., 1893-94. Tllus- trating Paper on ‘The Fossil Footprints of Storeton,’ by Osmunp W. Jerrs. (From Negatives by F. N. Eaton.) 741-746 Slabs of sandstone, from the Keuper of Storeton, Cheshire, showing various types of saurian footprints (3 plates, 6 photographs). Stonesfield Slate——Second Report of the Committee, consisting of Mr. H. B. Woopwarp (Chairman), Mr. EH. A. Watrorp (Secretary), Professor A. H. GREEN, Dr. H. Woopwarp, and Mr. J. WINDOES, appointed to open further sections in the neighbourhood of Stonesfield in order to show the relationship of the Stonesfield slate to the wnder- lying and overlying strata. (Drawn up by Mr. Epwin A. WaLForD, Secretary.) TuE shaft sunk by the Committee in 1894 was reported by the work- men to be unsafe, and an unsuccessful attempt was made to find the old sinking of 1830 at Reed Hill, near Stonesfield, reported upon by Professor Ed. Hull. The work was ultimately continued upon the Stocky Bank shaft to a depth of 60 feet. At that depth it had penetrated 13 feet into one of the highest beds of the Inferior Oolite—the Clypeus-Grit (zone Ammonites Parkinsoni). It has proved the continuance not only of the compact barren limestones (sub-Bathonian) so well developed’ around Chipping Norton, but also of the sandy limestone beds between them and the Glypeus-Grit. The section, as before stated, has been made by scarping a bank for about 30 feet, and by sinking a shaft to a depth of 60 feet on the step of the bank. It is practically a continuous section, only 2 or 3 feet intervening, laterally, between the ending of the one cut and the beginning of the other. STONESFIELD SLATE. 415 Section at Stocky Bank, Stonesfield, from the Great Oolite coral beds to the Inferior Oolite, showing position of Stonesfield Slate series and Chipping Norton limestones. Ft. in. 1. Surface soil with Limestone fragments. Nerinea, Corals, Thamnastrea Lyellit, Isastrea limitata, Cryptocenia Prattii, &c. ‘Rift Bed’. 2,3. Marls and Limestone, with Oysters and Rhynchonella concinna 4. Limestone, cream colour, shelly and compact ° 5-9. Marls and Limestone, five beds with Oysters and Rhynchonella 10-13. Stonesfield Slate beds :— Roof-shelly Limestone . Top hard-shelly Limestone Pendle-Sandstone Floor-fissile Limestone 14, 15. Limestone, with thin Marl parting a top 16. Fissile Sandstone : : 2 : : ; 17,18. Fawn colour, sandy, and ‘oolitic Limestone 7 5 : 5 , ad: 19. Clay. 20. Limestone, buff colour : 21, 22. Limestone, with Marl parting atop, Mytilus Sowerby yanus, Rhy ynehonella concinna, Ostrea Sowerbyi . 23. Black Clay, crowded with Placunopsis and with Perna, Nucula, and Ostrea . ; 24. Shelly Limestone made up of fragments of Ostr ed, passing into a brown Limestone, blue hearted, crowded with shells, Perna quadrata, Cy- prina, Corbula, Macrodon, &c. F - ‘ 25. Black Clay 26. Roe stone, an oolitic stone, blue hearted, made up of “whitish oolites ; in blue or brown base (like the blue oolitic slate) . . Siyto 27. ‘Callous’ Limestone—stone in fragments cemented together 28. Bastard Freestone, fine grained, oolitic, with masses of fossil wood 29. Buff and brown Marly Rubble, with carbonaceous Sener and remains of shells, Cyprina, &c. : _ 30. Bastard Freestone, cream coloured, without plant remains . 31. Bastard Freestone, with black dendritic markings : 32. Freestone of poor quality, splintery, more distinctly oolitic than beds 7 30 and 31 33. Sandy Limestone, fine- -grained, blue-hearted, ‘oolitic 34. Grey, blue and brown Marls, with Oysters and fossil wood in ‘lower part 35. Limestone, shelly, oolitic, cream-coloured and fine-grained, pale blue centres, and with brown vertical markings : 36. Rubble with ochreous patches and carbonaceous markings 2 37. Clypeus-grit ; a coarsely oolitic gn Limestone with ae iain: Plotii, pinkish in upper part . : (About 12 feet of stone can be made out below.) Neo COND NARS woos NOewonn _ 1 | | DROAR Ww ob led — i) orf OO He He Npwo Ll road So} o oo ooo oow woo- e oo Whether beds 16 to 26 are in their proper place is open to doubt. They contain fossils (excepting corals) similar to those found in the railway cutting at Ashford Bridge, barely a mile distant, and the clay courses are alike. Many authors report the slate to underlie the carbo- naceous clays and coral bed in the Ashford Bridge cutting. The Stocky Bank is much faulted. In the open section at Reed Hill, as described by Mr. H. B. Woodward, the slate is covered by 5 feet of marls with Modiola gibbosa, Rhy iynchonella concinna, and Ostrea Sowerbyi. In the Stocky Bank section, in the near shafts, and in other open workings, the succession of strata is the same. In order to consider more fully the true position of the beds 16 to 26 and to study relative sections and their fossil contents, your Committee would defer the final report until 1896. 416 REPORT—1895. The Fossil Phyllopoda of the Palceozoic Rocks.—Twelfth Report of the Committee, consisting of Professor T. WILTSHIRE (Chairman), Dr. H. Woopwarp, and Professor T. Rupert JONES (Secretary). (Drawn up by Professor T. RuPERT JONES.) 1§. A sHort provisional list of the Silurian Peltate Phyllopods was appended to our Report (the Tenth) for 1893 ; but since then a complete catalogue of the Lower Paleozoic Phyllopoda (Phyllocarida), with their geological horizons, their range and localities, has been made with the obliging ‘help of Dr. C. Lapworth, F.R.S. This is now produced in four tables, as it greatly enhances the value of our Reports on these fossils, and will be of considerable use to paleontologists both at home and abroad. TABLE I.—List of the Genera and Species of the Lower Paleozoic Phyllopoda referred to by T. Rupert Jones and H. Woop- WARD 27 their Reports tc the British Association, 1883-94. (The figures at end of lines refer to pages in the ‘ Monogr. British Palaozoic Phyllopoda,’ Paleont. Soc., Part II., 1892.) Hymenocaris vermicauda, Salter . : : 3 $ 74-79 Lower Lingula-flags. — Pentre’r felin, west of Penmoria 3 z d ay (if a: F Gareg-felen . : . : : oe RTD 5 3 Bryntwr Summerhouse ; 77 os - Moel-y-gest, hill behind Portmadoc Q Tremadoe) 7 717, 79 3 - Wern, near Penmorfa, near Tremadoc 4 77 - », (Upper part of).—Cae’n-y-coed, near ee eae) . sky Gwern-y-barcud , ; palit hcl Middle Lingula-flags. —Borth, Portmadoc , : : - 4 > . 78 - is Ffestiniog : 5 did, Wern, cutting n near. en J. Williams. Upper Lingula-flags. _— Moel-hafod- Owen, near Dolgelly . ; 5 Ss wenifAls Upper Tremadoc-flags.—Garth Hill, near Portmadoc . : : 4 capa ir Pont Seiont Shales.—Pont Seiont, Caernarvon Z : : : é Saf H. lata, Salter F 5 - ; : 4 79, 80 Upper Tremadoc Group. —Garth, Portmadoc. | Lingulocaris lingulecomes, Salter . a 5 . . ee | Upper Tremadoc Slates.—Garth, Portmadoc. | Upper Llandeilo Beds, near Builth. L. siliquiformis, Jones . : : : ; “ = 182 Upper Tremadoc Series. —Garth, Portmadoc. Bala Rocks.—Bwlch-y-gaseg, near Cynwyd, Corwen. L. Salteriana, T. R. Jones and H. Woodward : ons, Sa8e Lower Lingula-flags (upper part).—Cae’n-y-coed, near Maentwrog. Lower Tremadoc Slate Series.—Tu-hwant-i ’r-bwich Quarry, Portmadoc. 1 Brathay Flags.—E. side of Long Skeddale sp. . 5 ; ; . : : 3 : ; : Schiste Ardoisier inférieur (Faune 2°4*),—Maine-et-Loire. THE FOSSIL PHYLLOPODA OF THE PALZOZOIC ROCKS. 417 Saccocaris major, Salter : » 84,85 Lower Lingula—flags (upper part). Cae’ n- y-coed, near Maentwrog. Upper Tremadoc Slates (small individual)—Tu-hwnt-i’r-bwlch, S. minor, T. R. J. and H. W.. : ‘ ° . . + 86-88 2 Lower Lingula—flags. ‘“wern, near Portmadoc. Upper Arenig Slates (Daear- fawr Shale).—Craig-yr-hyrddod, Arenig. Caryocaris Wrightii, Salter . é - < 2 ‘ : ‘ ‘ . 89-91 Skiddaw Slates.— Near Keswick. Graptolitic Shalés of the Ballantrae Rocks.—Bennane Head, Ayrshire. Pont Seiont Shales.—Nantlle Tramway, near Pont Seiont, one mile south-east of Caernarvon. “Arenig Series’ of Huy and Nahnine, Belgium. C. Marrii, Hicks . Spe te ‘ ; ‘ . ‘ » 92,93 Skiddaw Slates. *_ Near Keswick. Pont Seiont Shales.—Nantlle Tramway, Pont Seiont, one mile S.E. of Caernarvon. C. Salteri (M‘Coy). (See also the Tenth Report, 1893) ° ‘ < ° « 93 Llandeilo Series.—Redesdale, Victoria. Aptychopsis prima, Barrande . - . . 100 Etage E (obovate ‘ prima’; var. ‘longa’; oval ' Wilsoni °) Limestone. — Bubowitz, Slawick, Wohrada, and Kozel . 3 - 100,101 Bohemia (circular ‘ secunda’) Schistose mudstone. —Borek, ‘Litohlow, and Kozel... 2 5 : . 5 ‘ i > . - 101,104 A. Barvandeana,T.R.J.and H.W. . d 4 ‘ ’ . 161 Birkhill Shales.—Dobbs Linn, Moffat, Dumfriesshire. Var. brevior, T. R. J. and H. W.—? Birkhill Shales,?Loc. . ‘ é . 102 A, anatina (Salter). (See the Tenth Report, 1893) . j ‘ i - 103 Lower Wenlock Beds.—Rebecca Hill, Ulverston, Lancashire. A. lata,T. R. i andH.W. . : . 104 Gala Group.—From a stream east of Nether Stennies Water, 64 miles N.N.W. of Langholm, Dumfriesshire. _ A. glabra, H. Woodw. . . 104, 105 Gala Group. —Clovenford, near i (W. of) Melrose, Roxburghshire. * Col- lection of the Museum of the Geol. Survey of Scotland. Buckholm Beds of the Gala Series.—Meigle [hill]; Galashiels, Sel- kirkshire. A. Wilsonit, H. Woodward . . 105,106 Riccarton Beds.—Shankend, Slitrig Water, near Hawick, ‘Dumfriesshire; Yads Linn, near Hawick ; Elliottsfield, near Hawick ; Longside Burn, Shankend, Roxburghshire. Riccarton Graptolite Shales._Stennies Water, near Langholm, M.G.8.Sc.; Streamlet E. of Nether-Stennies Water, near Lang- holm, Dumfriesshire, M.G.S.Sc.; Millstone Edge, Teviot Head, Roxburghshire, mM. G.S. ae A, port, H. Woodward . . - 106-108 Skelgill Beds, or Coniston Mudstones. —Skelgill Beck, near Ambleside, Westntforeland. ; Birkhill Shales,—Eldinhope, on the Eldinburn, on the Yarrow, Selkirk- shire 1895. EE 418 : REPORT—1895. Birkhill Shales.—Sundhope Burn, on the Yarrow, Selkirkshire. 5 Dobbs Linn, near Moffat. Red Shale. —Moffat, Dumfriesshire. Grieston Shales of the Gala Group.—Innerleithen, Peeblesshire, and Selkirkshire. A. ovata, T. R. J. and H. W.. , - 108, 109 Gala Group.—Stennies Water, 63 miles N. W. of Langholm, ‘Dumfries- shire. A. Salteri, H. Woodward : - > “ ° « 109 Wenlock Shale.—Pencarreg, Caermarthenshire. A. subquadrata, T. R. J. and H. W. 5 FI = . A 5 ; - 110 Silurian Beds.—Cloncannon, Tipperary. . A. angulata (Baily) A ° 2 * . : é . 110,111 Silurian Beds. “ Cloncannon, Tipperary. Birkhill Shales —Streamlet, Craigdasher Hill, 4 miles W. by S. of Dunscore, Dumfriesshire, Brathay Flags.—Nanny Lane, Troutbeck, Windermere, Westmoreland. A. oblata, T. R. J. and H. W. ; - 111,112 Riccarton Beds.— Balmangan Bay, west side of Kirkcudbright ‘Bay, Kirkcudbrightshire. Birkhill Shales.—Dobbs Linn, Moffat. Gala Group.-—Gala Hill, Galashiels, Selkirkshire and Roxburghshire. Peltocaris aptychoides, Salter 3 : 4 . 113,114 Birkhill Shales.—KEdinhope, on the Yarrow, Selkirkshire. Grieston Beds, Gala Group.—Rotten Gair, Innerleithen. Birkhill Shales.—Duffkennel, Dumfriesshire. - » (Young specimen).—Polmoody, at the top of the Moffat Water, about 13 miles from Moffat, on the road to Dobbs Linn. + », Dobbs Linn, Moffat, Mus. Geol. Surv. Scotl. P. Marrii, T. R. and H. W.—See the Tenth Report, 1893. F = - 114,115 Skelgill Beds.— West side of Long Sleddale. Shales (? Birkhill Shales).—? Moffat. Birkhill Shales.—Whitehope Burn, St. Mary’s Loch, Selkirkshire. Birkhill Group.—Streamlet, Craigdasher Hill, 4 miles W. by S. of Dunscore, Dumfriesshire. Birkhill Shales.—Garple Glen, 4 miles W. of Moffat. P. patula, T. R. J. and H. W. 3 3 5 A . : - : . 116 Birkhill Shales.—Belcraig, Annandale. Skelgill Beds.—Skelgill Beck, near Ambleside, Westmoreland. P. Carruthersii, T. R.J.and H.W. , - ° “ = - ‘ . 116,117 ? Birkhill Shales.— ? Near Moffat. Llandovery Beds.—Tieveshilly, near Portaferry, and Coalpit Bay, Co. Down, N.E. Ireland. Birkhill Shales.— Dobbs Linn, Moffat. ? P. Harknessi, Salter . ‘3 i “ . ‘ i . 117 Moffat Shales (? Birkhill). —Dunfriesshire. Pinnocaris Lapworthi, R. Etheridge, jun. . Balclatchie Beds.—Balclatchie, Girvan, ‘Ayrshire. - Upper Silurian Rocks.—Kendal, Westmoreland. THE FOSSIL PHYLLOPODA OF THE PALAHOZOIC ROCKS. 419 Discinocaris Browniana, H. Woodward 2 5 3 2 : onl 19=121 ? Birkhill Shales.—Dumfriesshire. Birkhill Shales.—Garple Linn, Moffat. - ; Dobbs Linn, Moffat. Argenteus-Zone, Skelgill Beds.—Lower footbridge, Skelgill Beck, near Ambleside, Westmoreland. Birkhill Shales.—Dobbs Linn, Moffat. 5 5 Polmoody, Moffat. D. ovalis, T. R. J. and H. W.. F E + 21, 1223 Birkhill Beds.—Dobbs Linn, Moffat. D. undulata, T.R.J.and H.W... Tee Birkhill Beds.—Garple Burn, Moffat. D. gigas, H. Woodward . : : : : : ; : 4 Argenteus-Zone, Skelgill Beds.—Skelgill Beck, Ambleside. Birkhill Shales.—Dobbs Linn, Moffat. . - 122,123 D. Dusliana, Novak. itage H-e, 1.—Gross-chucle, 8. of Prague, Bohemia.—‘ Geol. Mag.,’ 1892, p. 148. Caudal Appendages : . ; : : : 5 - Riccarton. beds, pl. xvii. f. 8—Shankend, Hawick . : : : rt Buckholm beds of the Gala group, pl. xvii. f. 13.—Meigle Hill, Gala- skiels.—‘ Monogr. Pal. Soc.,’ 1888, Part I. p. 45, Mudstone of the ‘ Barren Band,’ Skelgill Beds, pl. xvii. f. 12.—Skelgill, Westmoreland . : , : : : - : bee be é Pont Seiont Beds, pl. xvii. f. 9-11.--Nantlle Tramway, near Seiont, Caernarvon - . } : : - “ . 124 . 124 Note by Professor C. Lapworty, LL.D., F.R.S., F.GS. The fossils named in the preceding list are confined to the so-called Lower Patmozoic Rocks, constituting the original ‘Silurian System’ of Murchison and Barrande, and variously classified by geologists at the present day. All are agreed, however, that they contain three distinct faunas, namely, the ‘ First, Second, and Third Faunas’ of Barrande ; but the three distinct series of strata containing these three faunas are vari- ously grouped by different authorities. The French geologists still retain in principle the nomenclature of Barrande, and regard these three rock groups as the three component divisions of the Silurian system, namely, Silurien Inférieur or Primordial, Silurien Moyen, and Silurien Supérieur. The plan adopted in the present notice is to regard each of these three rock series as constituting in itself a distinct system, namely, (A) Cam- brian, or the System of the First Fauna; (B) Ordovician, or the System of the Second Fauna ; and (C) Silurian (or Salopian), or the System of the Third Fauna. 1 In the following table the various schemes of nomenclature lying between the two extreme types are given for the sake of reference and comparison, and the several formations which have hitherto yielded fossil Phyllopoda (Phyllocarida) are arranged in their natural positions in the general scale of sequence. EE2 420 REPORT—1895. TABLE II.—Showing the Geological Distribution and Vertical Range By Professor C. Lapwortu, Comparative Nomenclature C. STRATA OF THE THIRD FAUNA. ‘ Silurian’ of Sedgwick (Salopian). (c’) Ludlow Series (Upper Salopian) . 5 (c) Upper Ludlow and Passage-Beds . c ; (6) Aymestry Limestone . _. - : 2 ; (a) Lower Ludlow Shales . 8 5 ; : (c?) Wenlock Series (Middle alepiaw) (c) Wenlock Limestone (b) Wenlock Shales . : ; (a) Woolhope Beds . : 5 Geological Survey. Silurien supérieur Half only). Upper Silurian of Murchison and Silurian of Sedgwick. Upper Silurian of Lyell. (c}) Llandovery Series (Lower geen (ce) Tarannon Shales . : (b) Mayhill or Upper Llandovery : 5 : (a) Lower Llandovery 4 5 P 3 : / Upper Silurian of Barrande (Lower (8°) Bala or Caradoc Series (Upper Ordovician) | (b) Upper Bala, with Dicellograptus . | (a) Lower Bala, with Dicranograptus Survey. (B*) Llandeilo Series (Middle Ordovician) (bo) Upper Llandeilo, with Canograptus gracilis (a) Lower Llandeilo, with Didymograptus Murchisoni Murchison). (B!) Arenig Series (Lower Ordovician) (6) Upper Division, with Placoparia (a) Lower Division, with Phyllograptus Lower Silurian of Lyell (not of Lower Silurian of Barrande. Upper Cambrian of Sedgwick. | B, STRATA OF THE SECOND FAUNA. ‘ Ordovician’ of Lapworth, Se. _ Silurien moyen of the French authors. A. STRATA OF THE First FAuNA. ‘ Cambrian’ of Lyell. (A$) Olenidian or Upper Cambrian . : (b) Tremadoe Beds with Dictyonema and Olenus (@) Lingula Flags (of Belt) F Upper or Dolgelly Beds with Spherophthalmus ; Middle or Ffestiniog with Hymenocaris Lower or Maentwrog with Olenellus truncatus (A*) Paradoxidian, or Menevian Series, or Middle Cam- brian, nith Paradoxides Davidis, Sc. Lower Silurian of Murchison and the Geological Cambrian of Lyell. Silurien inférieur or primordial. Primordial Silurian of Barrande. Middle Cambrian of Sedgwick. (A!) Laconian, or Olenellus Zone, or Loner Cambrian, with Olenellus, Kutorgina, Se. a —— THE FOSSIL PHYLLOPODA OF THE PALAOZOIC ROCKS. 421 * the Lower Paleozoic Formations yielding Fossil Phyllopoda. LD. F.RS., F.GS. Horizons yielding Fursil Phyllopoda Lake District Scotland Treland Bohemia Other Localities nlock Shales. Ri art Brathay Graptolitic Cloncannon || E 1 Etage, Flags. Shales: (Tipperary) || Bohemia. | Bukowitz Grieston Shales} Treveshilly and and Gala _/Beds (County||Gross Kuchel, Skelgill Group. Down) &e. Beds. Balclatchie Redesdale Beds. (Victoria). Skiddaw Schiste Slates, &c. = Ardoisier (France). Bennane Head : z Shales. Arenig Series (Belgium). 1895. REPORT ‘(Bq10jOIA) OTEpsopoy a gl | | " * + (40p,W) wonng = ‘quoIag UO ‘aqBIg Aeppryg ' al ) os OP srory aamoge i ‘(unsjoq) Anz ‘yuo1sg yuog | ‘peop oueunog. | ‘ovLzULT[e ‘“Soye[G AULPPIAS x ot gaqpeg 229y bug, suevoohun9 ‘SIUILY PU So}VIQ DOpLUtIy, " % * AA EL pue pe ay oy, Scour Ht ‘OOpLUlAL], PUL SoLpT BASU] ) 2 : : ¢ * raqyeg ‘volpw s~wvo000n5 ‘(OUIvIT) IOISIOpIy 4ST | | ars | fe . “ : : nae “ | | | : | | prvMpooA, “FL ‘ssurq Avyyeag ‘sovpq vlncary ie | / re | pue sour yy ‘yy, ‘wwnragpng ‘syooy veg “spog oopeumary, | | a fr la * samp ‘sxucofimbyis H “oTLop | | | | -uvpy aeddg ‘oopruoazy, toddy | ‘ r pe * qoqyeg ‘sauoanpnbuy srewoojnbury | | | ‘souoz toddq ooprvuta.y, 5 ies 0 ; Jaqeg ‘790) Mu | ‘NOpVUlely, puv ssvpT vpusarvy | . * 1ay[eVg ‘wpnvovutaa srevoouarulizy | 0) FA@) tO i> stl al 1 cV aV ay Te FS ee me eae 8S | 28/8] -3 | ee!] 2 | 23 | se] Se) Ea) eres (see a) mer ee | Bal ee | ese | B90 )/e&/ se |] Bo | Be] § | Bo | se] Bs S 3. ae Se eee erste > en seel) aes we 7 “ bie we el ee g SUOZIIO FT x S 3 pe || ea) ape.) (ce saroodg pus wieuay eS eee =) a ae ee Ber ee vuney pag y, vuney puoveg | Boney Isat 10 10 | 10 ‘Cueidoysq) uvranqig ‘UBIDIAOpPIC) | ‘uBliquied SOU SH CTT ‘wtaomavy ‘0 “Jorg hig ‘(oprimoophyg) npodoyhyg nozoang wanoy oy) fo saody puv vuauey ay) fo obumy poorbojoay ay) buimoyy— IT] Wavy, 423 THE FOSSIL PHYLLOPODA OF THE PALHZOZOIC ROCKS. ‘quoleg yuog ‘THSPAS ‘spTyserey “Yor Mey TIESTOAS sj | “c “ EGS “ATILYSOASTT, 3 iid ‘TIS EAS $ a 239) “ “moOJIBOOTY “elex) ad ‘Aeyyeag ‘Arvsoddry, ‘(pyar -Areraddty, *‘SoTeM Yynog ‘sar1eodeg ‘dnory vey "HOWSOIIH “TSTEAS “WALA ‘spog M0WBOOTYT 66 “ec ‘dnory vey “qOLIAsIC OHV “YOOTUSM, “sores Tata “elmoyog ‘gq eseig . “BUIOyog [‘e-q o8R1g | ‘jepusy ‘ayoyeporeg | * * eee E * KX & * *e sabopuaddy yopny7 : *MBAON ‘vuvysnqy 4 : * prvapooM ‘E ‘svhib » ‘M‘H pue pe yy ‘vzpynpun 43 ‘MH pur “ft uL ‘82700 s * PIVAPOOAA “FT ‘VUunrwl0LT s.wva0UrL0suT ‘ant ‘espuoyya 'Y ‘2yz,lomdyyT siwvo0uurg St Joq[Rg ‘wssauywopy (j) “ ‘M‘H pue "fe “YL ‘eswayznsoyg . “M ‘H pues ‘e “iy a ‘myngod “ “AA H PUR CL Snemyy * 2 Iayeg ‘saproyohydy 1.00907). ACE Dae AE le aie ie : * (Ayregq) vzopnbuv sf “MH pue ‘pe "y ‘y ‘vzvuponbqns se ; * pIeMpooM\ “H “2.097] 06) “y . “Mm ‘A pue ‘L “a Pay ‘27000 “ee * prvapoon “H ‘27200udvT ye PIVMPOOM “FL ‘220087044 . 4 * prvmpoor “A ‘v.0gn7b ‘ty . "mM ‘H pue ‘Lf a “I; ‘090) “ce "8 * Goaqeg) vurxzoun 4 ae a “s PRY Cea : OT, ene: spas ‘nud sisdoyohiay 42.4: REPORT—1895. TABLE IV.—G@eological Order of the Species. (C%) Ludlow . Local Formation Kendal Beds of the Lake District Species Third Fauna (Silurian, or Salopian). Pinnocaris Lapworthi. (C*) Wenlock . Riccarton Beds of South) Scotland i Wenlock Beds of South Wales Wenlock Beds of Rebecca Hill, Lake District Wenlock Beds, Brathay Flags of the Lake Dis- trict Wenlock Beds of Tippe- rary Aptychopsis Wilsoni. a oblata. 9 Salteri. ns anatina. 5s angulata (?). Lingulocaris Sa]teriana(?) { Aptychopsis angulata. oh subquadrata (C1) Llandovery, Sc. - | Gala Group of South Scot- land (Tarannon, &c.) | Birkhill Shales, Moffat, &c. (including all Llando- very, and locally the Tarannon) Skelgill Beds (or Coniston mudstones), Llandovery Aptychopsis lata. . glabra. a Lapworthi. #5 ovata. Be oblata. Peltocaris aptychoides. Aptychopsis Barrandea. ” ” + var. brevior. on Lapworthi. 5 angulata. oblata. Peltocaris aptychoides. a» Mairi » patula. » Carruthersii (andat Tive- shilly, &c., Treland). Discinocaris Browniana. 5 ovalis. “a undulata. as gigas. Aptychopsis anatina. Lapworthi. Peltocaris patula, Discinocaris Browniana,. gigas, ” —— . THE FOSSIL PHYLLOPODA OF THE PALZOZOIC ROCKS. Taste LV.—Geological Order of Species—continued. Local Formation | 425 Species Second Fauna (' Ordovician’ of Lapworth, §:c.). (B*) Bala or Caradoc Bala Beds of Corwen Lingulocaris mis. siliquifor- (B*) Llandeilo (B') Arenig Balclatchie Beds, Girvan Probably highest Llan- deilo Beds } Upper Llandeilo Beds | (near Builth) J Llandeilo (?) Beds of Aus- tralia Pinnocaris Lapworthi. Lingulocaris lingulzco- mes Caryocaris Salteri. Upper Arenig Beds of Caer- narvonshire (Pont Seiont) Hymenocaris vermicauda. Saccocaris minor. Caryocaris Wrightii. nn Marrii. Skiddaw Slates Arenig) Bennane Head Shales of South Scotland Arenig (mainly Caryocaris Wrightii. First Fauna (§ Cambrian’ of Lycil). (AS) Olenidian, or Upper Cambrian. Upper Tremadoc Slates Hymenocaris vermicauda. A lata. Lingulocaris linguleeco- mes. Lingulocaris mis. Saccocaris major. Siliquifor- Lower Tremadoc Slates Upper Lingula Flags. Middle Lingula Flags Lower Lingula Flags Lingulocaris Salteriana. Hymenocaris vermicauda. Hymenocarisvermicauda. Hymenocaris vermicauda. Lingulocaris Salteriana. Saccocaris major. ? Saccocaris minor. 2§. Latest Additions to owr Knowledge of the Lower Paleozoic Phyllopoda (Phyllocarida). There has not been much to notice additional in the study of Palzozoic Phyllopoda since the last (Eleventh) Report in 1894. 1. Professor Dr. Gustav Lindstrém, paleontologist in the State Museum of Sweden, has discovered and courteously sent to us specimens of a new Hmmelozoe, not far removed in shape and features from £. elliptica (M‘Coy). Several very definite individuals, with delicate, thin, shining carapace-valves, light brown, and somewhat iridescent, occur 4.26 REPORT—1895. in a bluish-grey marly shale from Lau in Gothland, corresponding with the Wenlock Shale of England. They will be figured and described in the ‘Geological Magazine’ before long as Hmmelozoe Lindstroemi. 2. In the ‘Sitzungsberichte kénig]. Bohmisch Gesellsch. Wiss., Math.- nat. Cl.’ for 1894, article xxxvi. (separate copy dated 1894), Professor Dr. Anton Fritsch, in a preliminary report on the Arthropoda and Mollusca of the Permian formation in Bohemia, enumerates five species of Lstheria, partly noticed in our Tenth Report, 1893, namely, (1) Bstheria triangularis, Fr. (=? E#. tenella in his ‘Fauna der Gaskohle,’ vol. i, p- 31), with remains of the animal, from the Gas-coal of Nyian ; (2) #. cyanea, Fr., from the Black-coal of Kounova; (3) #. paleo- niscorum, Fr., covering whole beds in the Brandschiefer (Carbonaceous Shale) of Kostialov; some individuals show the large antenne ; (4) £. calcarea, Fr., related to H. minuta ; rare, in the red Plattenkalk of the Braunau district ; (5) #. ultima, Fr., in the uppermost part of the limestone with Amblypterus Feistmanteli, near Vitouchov, not far from Lomnitz. There are also Candona elongata, Goldenberg, from the red limestone of KieGowic, near Rowensko (Turnau) ; and Carbonia Salteriana, Jones and Kirkby, in the red limestone of Stradonic, near . Peruc ; and Cythere, sp., in the red limestone of Klobuk, near Schlan. Erratic Blocks of England, Wales, and Ireland.—Twenty-second Report of the Committee, consisting of Professors EK. HuLu (Chair- man), J. Prestwich, W. Boyp Dawkins, T. McK. Huaues, T. G. Bonney, Messrs. C. E. DE Rance, P. F. KENDALL (Secre- tary), R. H. TrppEmMan, J. W. Woopat., and Prof. L. C. Mian. (Drawn up by the Secretary.) [Read at Oxford, 1894.] THE investigations of the Committee during the past year have yielded results of more than ordinary interest, though the amount of information to be embodied in their report is less than has been available during the previous two or three years. A hope was expressed in the twenty-first Report that, as the result of an appeal made to the Corresponding Societies, information would be forthcoming regarding the Erratic Blocks of districts from which hitherto no returns had been sent in. This expectation has been realised ; and the Committee, for the first time in their history, are now enabled to justify the reference to Ireland in the terms of their appointment. In response to the circular issued by this Committee to the Corresponding Societies, the Belfast Naturalists’ Field Club promptly organised a committee to inves- tigate the Erratic Blocks of the north-east of Ireland ; and the first report, drawn up by the Honorary Secretary, Miss Sydney M. Thompson, and printed in the Proceedings of the Club (1893-94), is a valuable record of minute painstaking and accurate investigation. The Com- mittee have not limited their work to merely recording the erratics, but have made a complete study of the Drift deposits, and their organic and other contents, at several selected exposures, and have trans- mitted to this Committee a series of twenty photographs illustrating the features described. Lincolnshire is also added to the list of English counties coming within the sphere of the actual operations of the Com- ON THE ERRATIC BLOCKS OF ENGLAND, WALES, AND IRELAND. 427 mittee, and it is matter for congratulation that two observers have under- taken the work of recording the erratics of that county Two very im- portant pieces cf work have been undertaken by the Yorkshire Boulder Committee, one in the western portion of the area coming within their purview, near Barnsley, and the other, by the aid of the East Riding Boulder Commiitee, organised under the secretaryship of Mr. J. W. Stather, F.G.S., by the Hull Geological Society, in the country round Hull. In the latter case an exhaustive survey has been undertaken of all the erratics at present visible in the area selected, the one-inch map being divided into squares, and each square allotted to a worker, who will record every erratic above ground. The value of such a survey, in the elucidation of the complex problems of glacial geology, can hardly be over-estimated. The Barnsley reports refer to a series of erratics, some of which were ob- served many years ago, but only a few of which were recorded. Fortunately, a local worker, Mr. W. Hemingway, preserved the information left in his hands by Professor A. H. Green, and supplemented it largely by his own observations. Mr. T. Tate, Secretary of the Yorkshire Boulder Committee, and the present writer, went over much of the ground under Mr. Heming- way’s guidance, and can thus corroborate his testimony on many important points ; though a very large proportion of the erratics, especially such as were of a hard nature, have disappeared under the hammer of the road- mender. (It would be well here to remark that a like fate is rapidly overtaking many of the most interesting and significant of the ice-borne boulders in the country, and to reiterate the oft-repeated appeal to local observers to take prompt measures to record—and, if possible, to preserve —the erratics which come under their notice.) The especial interest of the groups observed lies in the fact that they are quite detached from the main lines of transport, and are so placed that they conceivably may have come by either of three routes—viz : (1) with the train of erratics, exclusively from the Lake District, which is traceable down Calderdale to within a few miles of Royston and Barnsley ; (2) with the dispersion of Brockram, Shap granite, and other Lake District rocks, with a few Scottish rocks, which can be traced down Teesdale and the Vale of York ; or (3) with the coast dispersion characterised by a similar series to that of the Vale of York, with some Scandinavian and other crystalline rocks superadded. The abundance of rocks from the northern part of the _ Lake District is conclusive against (1), while the occurrence of crystalline rocks, red and grey granites, gneissose granites, and felspar porphyries, certainly coming from neither English nor South Scottish sources, seems equally against (2), leaving the third the probable direction of origin. Mr. Tate recognised a Norwegian aspect of the non-British rocks. Another important report is that by Mr. W. Andrews, giving details of the dispersion of boulders from six small bosses of syenite which crop out about Sapcote, near Leicester. CHESHIRE. Reported by Surgeon-Major W. R. Dampriwi-Davins, per Glacialists’ Association. Macclesfield— 2 Lake District andesites. 428 REPORT—1895. Alderley— 1 Eskdale granite; 1 L. D. andesite. Knutsford— 4 Eskdale granites; 2 L. D. andesites; 1 Buttermere granophyre; 1 Scottish granite. DERBYSHIRE. Reported by Miss Evizapetn Dats, per Glacialists’ Association. Buxton— Lake District andesite and ashes, Buttermere granophyre, Silurian grit, chert gannister, toadstone. DuruHAmM. Reported by Mr. P. F. KenDAtt. Beda Hills Carboniferous limestone, Carboniferous sandstone, clay ironstone, Lake Dis- trict andesites and ashes, red granite, and a rock something like the Armboth Dyke, but much decomposed. These occur in gravel forming the Beda Hills. Kip Hill— Carboniferous limestone, Carboniferous sandstone, many Lake District andesites, porphyrite. No granites were visible at this place. Durham (City)— Lake District andesites, and a red granite with much black mica (perhaps Scottish). LINCOLNSHIRE. Reported by Rev. W. TucKWELL. Grimsby— 2 grey granites (1 gneissose); 2 coarse red syenite, with some black mica. These rocks are probably non-British. 2 dolerites, probably Whin Sill. Reported by Mr. J. Lorper. Louth— 1 dolerite; 2 sandstones (? Jurassic); 1 red granite (scratched); 1 red granite (rudely foliated) ; 1 ? granite; red sandstone; ? blue granite. NORTHUMBERLAND. Reported by Mr. P. F. KENDALL. Litile Mili— Dolerite (? Whin Sill) ; sandstone ; Carboniferous limestone; red porphyrite ; jasper; red sandstone. These occurred in Boulder Clay, resting upon a surface cross-striated from three directions, viz. N., N. 4° E., and N. 40° E. WARWICKSHIRE. Reported by Mr. W. ANDREWS. Coventry and Neighbourhood— 15 examples of the syenite, which crops out in 6 small bosses near Sapcote, 23 miles 8.W. of Leicester ; 1 Mount Sorrel syenite. ON THE ERRATIC BLOCKS OF ENGLAND, WALES, AND IRELAND. 429 YORKSHIRE.! Communicated by the Yorkshire Boulder Committee. Reported by Mr. W. Hemineway. Barnsley— Shap granite. | Andesitic ash and breccia. Gneissose granite. Rhyolitic breccia. Grey + Diabase. Coarse 35 Magma basalt. Rhyolite. Olivine ,, Quartz porphyry ?(? Armboth Dyke). | Borrowdale plumbago. Ennerdale granophyre. Carboniferous limestone. Felspar porphyry. Magnesian s Porphyrite. Flints (from Yorkshire chalk). Andesite. Lias limestone, with Gryphaaineurva Reported by Mr. T. Tate. Royston— Volcanic ash ; felsites; chert; magnesian limestone; 2 quartz felsites, Threl- keld; diabase ; basalt. Reported by Mr. W. GREGsoN. Baldersby— 1 Shap granite. Kirklington— 1 basalt. Reported by Mr. J. W. 8. Starner, Secretary of the Hull Geological Society. Sheet 72 of 1-inch Map—Beverley. North Cave— 1 basalt. Market Weighton— Carboniferous sandstone with fossils. Banacks— Carboniferous sandstone with fossils, Chalk Villa— Garnetiferous; mica schist; granite; basalt. Reported by Dr. F. F. Wauton. Newbold Church— 1 red granite ; hard limestone. South Cave— Limestone. ‘ The detailed report of the Yorkshire Boulder Committee, drawn up by the secretary, Mr. T. Tate, F.G.S., is published in The Naturalist (No. 231, October, 1894, Pp. 297-303). 430 REPORT—1895/ Reported by Mr. T. THELWALL,. Skidby and Little Weighton— Basalt. Reported by Mr. W. N. Crorts. Cottingham— 4 basalts. Reported by Mr. J, Nicuouson. Swine— 4 basalts ; 1 Milistone Grit; 5 Carboniferous limestones. Reported by Mr. H. Rosinson. Sutton-on-Hull— 5 basalts; Carboniferous limestone ; Liassic limestone with Gryphea ; granite. Reported by Mr. P. F. KENDALL. Out Newton, near Withernsea— Elzolite syenite (7) ; Laurvigite (augite syenite of Laurvig) ; rhomb-porphyry. Erratic Blocks of England, Wales, and Ireland.—Twenty-third Report of the Committee, consisting of Professor E. Hun (Chairman), Professor J. Prestwich, Professor W. Boyp Dawxrys, Professor T. McK. Huaues, Professor T. G. Bonney, Mr. C. E. DE Rancg, Mr. P. F. Kenna (Secretary), Mr. R. H. Tippeman, Mr. J. W. WoonaLt, and Professor L. C. MiaLn. (Drawn up by the Secretary.) Tur Committee have again to report that the work of recording the ice- borne erratics of Great Britain and Ireland has made satisfactory progress, and that several districts, regarding which no information was previously obtainable, have been reported upon. The Yorkshire Boulder Committee, acting in conjunction with the sub-committee appointed by the Hull Geological Society, have presented another valuable report. Further details are furnished relating to the re- markable series of erratics found in the Yorkshire Calder ; but the most noteworthy contribution is a tabulated list of no less than 2,070 boulders, comprising the whole of those visible im sitw in the cliffs or lying on the shore ‘above ‘half-tide,’ along a length of fourteen miles of coast of Holderness from Withernsea to Hornsea—a truly admirable piece of ob- servation. Several records are given of the occurrence of Scandinavian erratics at inland stations in Holderness. Other reports received from the same source deal with sporadic boulders in other parts of Yorkshire. The Rev. W. Tuckwell, of Great Grimsby, has added to the list of erratics noted in Lincolnshire, and is taking active measures to secure the co-operation in the work of the clergy of the district. New ground has been broken in the county of Northumberland, with ON THE ERRATIC BLOCKS OF ENGLAND, WALES, AND IRELAND. 431 some observations upon the erratics of the upper part of the Tyne valley, near Haltwistle. Mr. Dwerryhouse furnishes a valuable and exhaustive series of reports upon the boulders of a portion of the Cheshire Wirral and the previously unrecorded district around the Wrekin in Shropshire. For the first time since the appointment of the Committee reports have been received from South Wales, where Mr. Storrie has done some _ excellent work in the neighbourhood of Cardiff. ; From Ireland a second report has been received from the Belfast Naturalists’ Field Club. ENGLAND. CHESHIRE. Reported by Mr. J. Lomas, A.R.C.8S., and Captain A. R. DwerryHoussE, per Glacialists’ Association. . Prenton Village, near Birkenhead— 5 L.D. andesites; 1 fine L.D. Ash; 3 Yewdale breccias; 1 Eskdale granite ; 1 Buttermere granophyre ; 1 Scottish granite ; 1 Criffel granite; 2 grits of undetermined origin. Roman Road, near Little Storeton— 1 L.D. andesite. Road behind Little Storeton— 2 L.D. andesites ; 1 basalt. Railway Cutting between Barnton and Neston— 1 limestone ; 1 diorite. Reported by Captain Dwerryuouse, per Glacialists’ Association. Sutton Weaver— 3 L.D. andesites ; 3 Eskdale granites. Preston Brook— 41L.D.andesites ; 2 Eskdale granites ; 1 Buttermere granophyre ; 1 Silurian grit. Preston-on-the-Hill— 3 L.D. andesites ; 3 Eskdale granites; 1 grit (? Silurian). Willaston and Burton, near Neston— ' 40 L.D. andesites; 10 L.D. ashes; 1 L.D. andesitic agglomerate; 6 Eskdale granites; 3 Buttermere granophyres; 3 diorites; 3 Galloway granites ; 6 Criffel granites; 1 felsite (reddish) ; 1 grit with numerous quartz-veins ; 5 grits; 11 Silurian grits; 2 basalts; 1 limestone. LINCOLNSHIRE. Reported by Rev. W. TuckweELt. Great Grimsby— Boulders of Whin Sill are common from Grimsby to Brigg. Several Scandi- navian rocks from the neighbourhood of Christiania were found at depths of 10 to 15 feet in the foundations of the new Union. 3 a > 432 REPORT—1895. NoRTHUMBERLAND. Reported by Mr. G. SiaTER. Haltwistle and Lambley— Boulders averaging a foot in diameter :— Haltwistle Lambley Limestone ; : , . 40percent. . ; . 3 percent. Millstone grit . . a ph ke a . ; - 20 a9 Sandstone ; : . eal b2 ae = Whin : : ; ; eg + ‘ : 2 PG = Silurian . : : : LO +) 5 A ; 120 53 Granite . - - ; 5 ly +: , : a ee - Grindstone sill : : =e! “ . : . 80 i Permian . F : — A 5 10 Ay N.B —The percentages are not to be relied on as correctly indicating the proportions at each place, but serve to show the contrast between the two localities in regard to the figures printed in heavy type. SHROPSHIRE. Reported by Captain A. R. Dwerrynouss, per Glacialists’ Association. Wrockwardine— 12 Arenig felsites ; 2 L.D. andesites; 1 Eskdale granite. Between Wrockwardine and Walcot Station— 1 Arenig felsite. Between Wrockwardine and Leaton— 1 Arenig felsite. Leaton— 1 Arenig felsite. Overley Hill '\— 1 Eskdale granite; 2 Galloway granites; 1 Buttermere granophyre ; 1 Triassic sandstone (local). Wellington '— 2 Eskdale granites; 1 L.D. andesite; 1 Arenig felsite. The Wrekin— In Forest Glen :—1 Eskdale granite; 1 Criffel granite; 2 Silurian grits. Wenlock Wood :—1 Eskdale granite; 1 Arenig felsite. Near Newhouse Farm :—1 Arenig felsite. Steeraway— 1 Eskdale granite. Little Wenlock— 3 Eskdale granites; i L.D. andesite; 1 Galloway granite; 1 Arenig felsite. Huntington— 4 Eskdale granites; 1 Galloway granite; 1 Criffel granite; 1 Silurian grit; 3 Arenig felsites; 1 Coal Measures sandstone (? local); 1 spherulitic rhyolite (Overley Hill) ; 1 basalt (? local). Road Huntington to the Hatch— 2 Eskdale granites; 1 Arenig felsite. Near Sapling Farm— 2 Arenig felsites. Buildwas— 1 Eskdale granite; 1 Arenig felsite. 1} Observed by Mr. Lomas and Capt, Dwerryhouse. | ON THE ERRATIC BLOCKS OF ENGLAND, WALES, AND I. ELAND. 433 YorKSHIRE.! Communicated by the Yorkshire Boulder Connittee. Reported by Mr. J. Burton. Millwood, T'ormorden— Buttermere granophyre; granites (L.D.); grits (Millstone Grit). The boulders here are much larger than those lower down the Calder Valley. Mirfield— Eskdale granites; L.D. andesites ; Mountain Limestone with Productus. Horbury— Granites occur in a ridge of clay. Reported by Mr. Rosert Law. Millwood— 1 grey quartz-felsite ; 6 Buttermere granophyres; 5 Eskdale granites; 2 L.D. andesites; 1 eurite; 1 mica trap. Reported by Mr. THomas SALTONSTALL. Luddenden Foot— 1 pink rhyolite ; 1 Eskdale granite. Sowerby— 1 pink rhyolite; 1 rhyolite; 2 Eskdale granites; 1 Buttermere granophyre ; 1 L.D. andesite; 1 quartz-felsite ; 1 porphyrite ; 1 quartzite. Reported by Mr. W. GREGSON. Rokeby Park— 1 Shap granite. Reported by Mr. T. Carter MiTcHeE.t. Baldersby— 3 Carboniferous limestones. Reported by Mr. E. HAwKEswortu. Saliburn— 3 Shap granites ; 1 basalt. Reported by Mr. T. SHEPPARD. Burstwick— Chalk and flint; lias limestone and marlstone with Ammonites communis and Gryphea incurva; rhyolites; Carboniferouslimestone; Brockram; Armboth quartz-felsite ; Whin Sill; Rhomb-porphyry ; red granite (? Scandinavian) ; gneiss. Reported by Mr. J. W. SraTueEr. Melton— Laurvigite (augite-syenite of Laurvig); Rhomb-porphyry; Armboth dyke quartz-felsite ; Brockram (Vale of Eden). Bessingby— Rhomb-porphyry. 1 This report will be published in eatenso in The Naturalist. 1895, FF 434 REPORT—1895. Reported by the Hull Geological Society. TasLE I.—Boulders noted on the Holderness Coast between Withernsea and Hornsea, 1895. A B Cc D E F G H I J FA) 5 a oe Bas mn . ay 3 gage 1S ole (E(B dre (eg she | Mri Fis a Lar} | aa = Ha |u| Cs |e f $3 |S | gt) S|] ee |e /e2)/ oq} 2 Belo ‘wh | SS |] 2S 118] 3% Stee |Fa) ee) en | ae aq | Boulders over 1 foot in Rest |) es | oe | oe) oe 2 | oS diameter aa | oe | 3s iuee | os ma on | oe ge | Boe Sa 5 A 8 a | te a Mites | Mite | 14 Mile |34 Miles} 4 Mile | 1 Mile | 2 Miles |23 Miles Guein Per |PRer Per Per Per Per Per Per 8 cent. | cent.| cent. cent. cent. cent. cent, cent. Carboniferous limestone, including possibly a few other Palzozoic sedimentary rocks . o -| 46:4] 37:6) 16°7 26°3 23°8 23°9 19°4 24 Sandstones, grits, &c., probably all from Carboniferous or other Palzozoic rocks . 5 A «| M6) 17°9) 182 13-7 71 10°3 177 20°9 Mesozoic rocks, Jurassic lime- stones and sandstones, chalk, &e. 5 ns 5 “i . ° 11 18°6 45°8 284 34:6 27°6 49°4 36 | Basaltic and other eruptive rocks | 195) 234) 21°5 26°4 30°8 34°6 12°4 16 Granite, schist, gneiss, &c. 85 2°5 2°38 52 37 3°6 11 31 100:0, 100:0; 100-0 100°0 | 100°0 | 100°0 100°0 | 100:0 oe ee ON THE ERRATIC BLOCKS OF ENGLAND, WALES, AND IRELAND. 435 I. The above is a rough classification of 2,070 boulders (above a foot in diameter) noted on the Holderness coast between Withernsea and Hornsea, a distance of 14 miles, during the summer of 1895. II. All the boulders tabulated in sections A, B, C, D, E, G, H in the above table were in sitw in the clay, or were close to the boulder clay cliff from which they were recently fallen. In section F, however, a large group of boulders occurred at about ‘half-tide,’ and these are in- cluded in the table. III. Table I. gives the actual number of boulders noted in the different sections of coast. Table II. gives the percentage of the different classes of the rocks. IV. The largest boulder seen was a block of Carboniferous limestone : on the beach near Mappleton (85 inches x 31 inches x 30 inches +). ee Many others approach this size. A block of garnetiferous schist was noted at base of cliff near Cowden, 22 inches x 30 inches x 13 inches. SOUTH WALES. GLAMORGANSHIRE. Communicated by the Cardiff Society of Naturalists. Reported by Mr. J. Storr. Pencoed, Bridgend— Fragments of indeterminable marine shells ; chert from Lias and Carboniferous limestone; no chalk flints; 4 or 5 Lower Lias limestone with Gryphea incurva ; 3 white cherty sandstone from U. Trias of St. Mary Hill; 7 or 8 Rhztic sandstones, with fossils from St. Mary Hill; 2 or 3 dolomitic breccia; Pennant Grit ; Cockshot rock; over 100 Millstone Grit; 40 to 50 Carboniferous limestone; 35 Old Red sandstone, besides pebbles ; 1 black micaceous flag (probably Llandeilo); 7 grits and yellow sandstones (pro- bably Silurian) ; 1 fossiliferous Wenlock limestone ; 2 granites (specimens mislaid) ; 3 ‘trap’; 1 brecciated ‘trap’; 3 basalts; 1 porphyritic diabase (amygdaloidal); 1 volcanic ash; 1 rhyolite, showing macroscopic flow structure ; 1 gabbro; 1 green rock with white chalcedony. Some of these have been sectioned and submitted to petrologists, who note the following facts :— One was identified with the gabbro of St. David’s Head; a felsite bore some resemblance to the pre-Cambrian rocks of Pembrokeshire; 2 or 3 acid rocks, brecciated felsites, and tuffs were very like Carnarvonshire rocks, especially those of the Lleyn promontory. None was recognised as belonging to the volcanic rocks of the neighbourhood of Fishguard, of Mid Wales, or of any place further north than Carnarvonshire. From these data it is concluded that the movement of transport was from the west or north-west. Some were of such a general character that it was impossible to locate them. IRELAND. Co. Down. Communicated by the Belfast Naturalists’ Field Club. Coast road between Ballymartin and Annalong— 1 Granite from Slievh Lawagan, Mourne Mountains, FR2 436 REPORT—1895. Holywood— Olivine gabbro, possibly from Slemish. The boulder was embedded in clay containing fragments of flint, chalk, basalt, and quartzite. Island Hill, Strangford Lough— 2 Ordovician grits. Rough Island, Strangford Lough— Boulder showing junction of granite and Ordovician grit with vein of eurite ; Ailsa Craig eurite; Antrim chalk and flint ; pitchstone. Co. ANTRIM. St. Nicholas, Carrickfergus— Large boulder of unidentified rock in fossiliferous Boulder Clay, containing a fragment of eurite from Tornamoney (coast of Antrim) St. John’s Whitehouse, on shore opposite Macedon— 1 fresh olivine dolerite, derived from one of the volcanic necks of Antrim. Blacklion— Co. Cavan. 1 Millstone Grit. The stone is perched on a pedestal of Carboniferous limestone. Its upper surface is sculptured with concentric circles like those on cover-slabs of Kist-vaens, Some Suffolk Well-sections. By W. Wuiraker, B.A., F.R.S., F.G.S., Assoc. Inst.C.E. [Ordered by the General Committee to be printed in full.] Accounts of seventeen wells having come to hand since the last Geological Survey Memoir that deals with Suffolk was issued, advantage is taken of the meeting of the British Association at Ipswich to make them public. A great number of well-sections in the county have been printed in the following Geological Survey Memoirs, to which inquirers are re- ferred :— 1878. The Geology of the N.W. Part of Essex . . . with Parts of... Suffolk, p. 84. ‘ 1881. The Geology of the Neighbourhood of Stowmarket, pp. 18-25. 1881 (or 2). The Geology of the Country around Norwich, pp. 156 (and diagram), 157, 158, 162, 166. 1884. The Geology of the Country around Diss, Eye, Botesdale, and Ixworth, pp. 29-41. 1885. The Geology of the Country around Ipswich, Hadleigh, and Felixstow, pp. 111-125. 1886. The Geology of the Country around Aldborough, Framlingham, Orford, and Woodbridge, pp. 50-57. 1886. The Geology of the Country between and south of Bury St. Edmunds and Newmarket, pp. 20-25. 1887. The Geology of Southwold, and of the Suffolk Coast from Dun- wich to Covehithe, pp. 78-80. [Words in square brackets have been added by the writer.] ON SOME SUFFOLK WELLS. 437 1887. The Geology of the Country around Halesworth and Harleston, pp. 36-39. 1890. The Geology of the Country near Yarmouth and Lowestoft, p. 83. 1890. The Pliocene Deposits of Britain, p. 110. 1891. The Geology of Parts of Cambridgeshire and of Suffolk, pp, 114— 119. 1893. The Geology of South-western Norfolk and of Northern Cambridgeshire, pp. 161-164. Cuare. Snow Hill (half a mile N. of the Church), by the roadside, 1894. About 1765 feet above Ordnance Datum. Made and communicated by Mr. G. INGOLD. Water rose to 153 feet from the surface. Thikness Depth iu Feet in Feet { White clay ; 7 7 [Glacial Drift] Boulder clay Brown clay; 62 132 Red and green sand . . ‘ 11s 25 Chalk, veryrotten, { Soft brown chalk ‘ ‘ : 35 60 and with very few | Soft white chalk ; c : 42 102 flints Harder white chalk . : : 38 140 Haveruitt. Waterworks, Camps Road, 1894. Nearly 297 feet above Ordnance Datum. Made and communicated by Mr. G. INGOLD. Shaft, 103 feet ; the rest bored. Water-level, 733 feet down. Yield exceeding 150 gallons a minute. Thickness Depth in Feet in Feet _ Mould . tn 3 3 , Brown sandy loam 25 z White boulder clay ils 17 [Drift] { Blue clay 6 23 Blue and brown clay . 2 25 Chalk and clay . 3 28 Upper Chalk, with flints ie gag from 130 to 1 230 feet down) ed hl aoe Hircuam. Communicated by the Rev. EH. Hitt, from infcrmation from Mr. COBBOLD, well-sinker. The Hall. About 175 feet above Ordnance Datum. Well 60 feet deep. “wet aso Blue clay. [Drift] } Brighter clay and marl. Sand and consolidated flint-pebble-bed, from which the water comes. The Rectory. About 235 feet above Ordnance Datum. Well 102 or 103 feet deep. At 100 feet a ‘fault’ (so-called) of hard sand, from which - the water comes. [Drift.] _ Squirrels Farm. Eastern end of parish. Well said to be 100 feet deep, all in [Boulder] clay. 438 REPORT—1895. Kerriesaston. High House Farm. About 230 feet above Ordnance Datum. Communicated by the Rev. E. HILu. Well 70 feet to water. Marker Weston. Small Farmhouse on the Bury Road, near Hopton Greyhound, 1889. Made and communicated by Messrs. GEDNEY (of Norwich). Shaft 35 feet, the rest driven tube. Thickness Depth in in Feet. Feet Made Soil . , ; : : ‘ 1 il Red sand , = 15 16 Grey sand . : 14 30 : Quick sand , F 5 35 eat Gravel. 5 12 47 Sharp red sand . 16 63 Grey sand . ; 38 101 Metron. Suffolk County Asylum (at a distance from the Asylum). From a Report by Mr. G. Hopson, 1894. Test boring, No. 1, 1891. Yield proved to 348,000 gallons a day. Water very hard. Thickness Depth in in Feet Feet Soil A : 5 : : . ° : 3 3 : Sand and gravel. . . 42 7% Deana Cree i { Sand Rs ik ae eta i eae 10! 18 Coloured [mottled] clay and drift-flints : . : : 2 20 (Red. 2 22 Mottled clay | ;. ‘ [Reading Beds “| Light blue 2 225 34 feet] > « Brown sandy clay 83 31 Green sandy clay 5 5 1 32 Brown running sand . : 12 44 Blue clay . 5 : 4 4 6 50 Green sand and flints , - 2 52 [Upper Chalk] Flints and chalk : ; : , 248 300 | Test boring, No. 2, 1891 (2). | Yield insuttlicient at the depth of 300 feet. Continued for another 50, in which a further supply was found. Yield proved to be 240,000 gallons in 24 hours, the water being lowered 14 feet. Thickness Depth in in Feet Feet Sekt 5. sacs Aaa ar 3 3 [Drift ?] Sand and gravel . d 5 : 14 17 Coloured [mottled] clay 5 22 Sand and clay . 2 24 F Brown clay . 8 32 pease Fe eT Running eid 12 44 eat Sand and clay : 3 AT Dark clay . ; é - | 4 51 Green sand . 1 52 [Upper Chalk] Flints and chalk 298 350 ON SOME SUFFOLK WELLS. 439 Naveuron. Rectory. About 282 feet above Ordnance Datum. Communicated by the Rey. E. Hrx1, from information from Mr. COBBOLD, well-sinker. Well in blue [Boulder] clay to the depth of 130 or 140 feet. SraNNINGFIELD. Half a mile N. 15° E. of the church, at the spot marked ‘Well’ on the 6-in. map (in error, as there was only a pit there). 1894. Communicated by the Rev. E. HILL, from information from the owner, Mr. CROSSFIELD, verified by inspection. 310 feet above Ordnance Datum. Sunk to the depth of 111 feet, when water rose to 56 feet from the surface. Wholly through grey chalky Boulder Clay, with chalk pebbles (some scratched), large flints, fragments of Kimeridge Clay and of Ammonzites. The flints and Kimeridge Clay occurred noticeably at the depth of 60 to 80 feet. STRADISHALL. Public Well. 1893. Made and communicated by Mr. G. INGOLD. Shaft. Water-level 35} feet down. | Thickness Depth in in Feet Feet Mould | 2 2 Loamy sand F ; Ea 2 4 White clay . | 5 9 [Boulder Drift] . } Brown clay. | 4 13 Blue clay | 47 60 Chalk . ‘ : | 9 69 Srutron. Zhe Hall. About 14 miles S. of W. from the Church. Communicated by Mr. G. F. MANSELL. | Thickness in Depth in Feet Feet Boil... ‘ 5 : : c : 3 : a 3 3 Gravel : : : é : : ; : 10 13 Mee Galonred(clay) =o) es het 4 17 eee The tae clay gabe’ 29 Sandy clay . 2 2 - 34 55 84 Mottled clay, with claystone (3 inches) 2 feet down . : 123 96+ : ; Stone . - : ; 2 - 1 97% | cy Seine rene - Green clay and sand . ; oo 243 122 | Dark clay . : ; ; mal 7 129 role and a little sand. 5 sat 7+ 136} Flint and pebbles : 137 Chalk and flint . 44.0 REPORT—1895. THorPE Morigeux. Chinery’s Farm, 270 feet above Ordnance Datum. Communicated by the Rey. E. H1ut, from information from Mr. COBBOLD, well-sinker. Well 120 feet deep. ‘Mostly blue clay ; sandy gall at bottom.’ TrimLey. Felixstow and Walton Waterworks, 1893. Communicated by Mr. H. MILLER, Sixty feet above Ordnance Datum. Iron cylinders 83 feet, the rest bored. Water rose to 55 feet from the surface. Supply good. Quality excellent. Thickness in Depth in Feet Feet Soiland Crag. / 8 8 [London Clay]. Clay ‘and “loam, with 7 inches of Septaria 883 feet down . ' é : 81 89 Mottled clay t : Bich 18 107 Pees Uilaalay sts. ee 9 116 J Greenish sand. 9 125 Chalk, Thin mest of flints 144, 161, 165, and 178 feet down ; 1163 2413 WartrisHAM. Opposite the gate to the Hall. Communicated by the Rev. E. HILL, from information from Mr. CoBBOLD, well-sinker. Road-level about 285 feet above Ordnance Datum. Well 80 feet deep, mostly through stiff blue [Boulder] clay. Woopsrivce. Zhe Thoroughfare. Mr. Carter's. 1895. Made and communicated by Mr. F. BENNETT. Good supply. Water stands about 26 feet down. Thickness in Depth in Feet Feet Well (? old), the rest bored : by pt SET ee == 28 [? Crag or Eocene] Running sand | 12 40 Mottled clay 10 50 [Green sand . 9 59 [Reading Beds, | Running sand 22 614 26 feet] Dark green sand and flints . 1 624 Mottled clay 2 645 Dark green clay . ; 13 66 Chalk, with flints nearly every foot 64 130 [Upper Chalk] Mottled clay [? a marl-bed in the | chalk, orpipe of Reading Beds?| | 3 1302 ee ie a . 7 } * ON THE DIP OF THE UNDERGROUND PALAOZOIC ROCKS. 4A] On the Dip of the Underground Paleozoic Rocks at Ware and Cheshunt. By JoserH Francis, M. Jnst., C.L. [Ordered by the General Committee to be printed in extenso. | Ir has come to my knowledge that some of the geologists specially interested in ascertaining the lie of the ancient rocks beneath the Eastern Counties of England, are doubtful whether any value is to be attached to statements that have been made with regard to the dip of these rocks at certain places. I refer especially to two instances in which borings were made into the strata underlying the Gault to the north of London, and where much time and money were spent in obtaining the true angles and directions of dip. It was in the year 1879 that these observations were made, but it does not appear that any description of the methods adopted has hitherto been published, and Mr. Whitaker has suggested that I should give a short account of the experiments that were carried out by me under the direction of the late Mr. James Muir, the former engineer to the New River Company. This I now propose to do, and hope to be able to show that the recorded results may be accepted as perfectly reliable. These borings were undertaken by the New River Company on the advice of geologists who were of opinion that the Lower Green Sand extended to the outskirts of London, and that when found, it could be relied upon to afford a plentiful supply of pure water for the use of the metropolis. The outcrop of the Lower Green Sand to the north of London extends from Leighton Buzzard to Ely, over an area of 166 square miles, and con- sequently must receive on its surface an immense quantity of rain water ; moreover, being extremely pervious, it must be capable of transmitting through its mass a large percentage of the rainfall. Nearly forty years before this, a good yield had been obtained from the same formation, at a depth of 1,800 feet, at Grenelle, near Paris, and later on at Passy, in the same neighbourhood. A deep bore at Kentish Town, made in the year 1855, had revealed the fact that a ridge, if nothing more, of ancient rocks protruded upwards to the Gault, and this discovery raised considerable doubt as to the extent of the sandy layer under ground. There was also a great amount of uncertainty as to whether this stratum, which is so prolific of water when tapped anywhere near its outcrop, would yield equally well where compressed by the weight of a thousand feet or more of superincumbent earth. On the other hand, the Royal Commission on Water Supply, which sat in 1869, had reported that ‘so far as this Green Sand continued, it would form a valuable and copious water-bearing bed,’ and it was felt that the problem was one of such extreme importance that it was of the utmost consequence it should be solved. The water supply, which there was a chance of so gaining, was so convenient and good as to justify some amount of speculation in endeavouring to obtain it, whilst there was, in any case, a certainty of a large accession of Chalk water from the upper part of the bore. J may here remark that, although several eminent men decidedly encouraged the venture, they can hardly be held responsible for the extravagant notions entertained by some persons, who assumed that this experiment was about to solve the whole question of the future supply of water to London. 44.2 REPORT—1895. One of the borings to which I wish to call attention was made at,Ware, and the other at Turnford, near Cheshunt, both in the county of Hertford. These particular places were chosen because they offered suitable sites for new Chalk wells, and because land alongside the channel of the New River was available for pumping stations. On reaching certain depths, the bore holes furnished conclusive evidence that it was quite hopeless to expect a supply of water from below the Gault, and orders were about to be given for a cessation of the work, when those geologists who had watched the progress of the enterprise, expressed a wish that endeavours might be made to learn the direction of the dip of the lowest stratum reached in each case. Instructions were thereupon given for the requisite investigation to be made, and when the inquiry was found to involve additional boring, the construction of special apparatus, and the devotion of much time and attention, these were liberally provided by the New River Company. A number of men of science formed themselves into a Committee to advise as to the best way of obtaining the desired informa- tion. This Committee consisted of Sir William Thomson, now Lord Kelvin, Dr. C. W. Siemens, Mr. Etheridge, Professors T. McK. Hughes, Maxwell, and Stokes, Mr. Mylne, and Mr. Muir. From time to time they discussed various modes of proceeding, and under their advice the several experiments were arranged. In carrying out their suggestions, every possible care was exercised to ensure correct results, and observations were repeated until there could be no reasonable doubt of the truth of the conclusions arrived at. Before describing in detail the appliances used, I may give a general outline of the circumstances preceding the discovery of Silurian Rock at the Ware boring, and of Devonian at Turnford. Before the year 1872, a well had been sunk into the Chalk at Turnford, and pumping engines erected. The shaft had a depth of 176 feet, with a bore hole 34 inches in diameter, extending to a depth of 362 feet from the surface of the ground. The bore was made of this large size in order to admit of its being continued downwards to a great depth without undue contraction of diameter, in case it should be afterwards decided to search for the Lower Green Sand ; but it was not until 1874 that it was resolved to follow up the question. Arrangements were then made for deepening the bore and for dealing with any water that might be obtained from the hoped-for deep source. ‘To convey the expected supply of water to the surface, a wrought iron tube of 24 inches internal diameter, and long enough to reach to the bottom of the hole, was provided. Its joints were made quite watertight throughout by calking, and all access of water from a higher level was to be shut off by sealing up an annular space to be left around the tube where it passed through the Gault clay. The sinking of this tube to a depth of 896 feet, was accom- plished by the old system of breaking up the material with chisels and bringing it to the surface by means of buckets with valves in the bottom. In the meantime, the more rapid method of rock-boring by means of diamonds had become a success, and, after due consideration, it was decided to put down a hole by this means at another spot in order to obtain an early solution of the question. A site near Ware, six miles north of Turnford, was selected, and in the beginning of the year 1878 a boring by the new process was commenced there. By this method, a number of black diamonds fixed in one end of a ring or short tube of steel, techni- cally called a ‘crown’ (fig. 1), are caused to rotate against the rock to be aaa a ON THE DIP OF THE UNDERGROUND PALZOZOIC ROCKS. 443 drilled, and the diamonds, being harder than any other known substance, eut their way through, forming an annular groove which becomes deeper and deeper as the crown is slowly lowered. A cylindrical core of un- detached rock is thus left standing in the middle (fig. 2), and is received in a long tube of a somewhat greater internal diameter than the crown which it surmounts. To the closed top of this core-tube is attached a column of tubular rods, by which a rapid rotary motion is transmitted from machinery above, and down which water is pumped, with the double purpose of keeping the drill cool and of bringing up the abraded material. To admit of the passage of the water from the inside to the outside of the crown, grooves are formed across the cutting face, and through these the water is forced, carrying with it the débris cut away by the diamonds. The water then passes upward outside the core-tube to the top of the hole, bringing with it the lighter of the particles. Above the core-tube, and enclosing the lower end of the suspending rods (fig. 3), there is an open topped tube of a few feet in length, into which the heavier matter falls, and this sediment tube is emptied when the crown is raised to the surface. Before the core can be brought up from the bottom it must be detached from its bed. This is usually effected by friction during the revolution of Fiq. 2. SSS MOMMY Scale, 1 in. to 1 ft. RALEAKE MAY Y Le Z Scale, 1 in. to 2 ft. the crown in boring, the inner surface grasping the core with sufficient force to break it off. The block then falls out of the perpendicular, and when the boring-rods are drawn up, it is generally found with its lower end resting on the internal shoulder of the crown. Most frequently, the fracture occurs at a bed or other joint in the rock. Should the pillar remain firmly fixed after it has attained the full height of the core-tube, one of the various appliances known as core-extractors is lowered. This firmly clips the core at the bottom, and on the application of adequate lifting power to the rods, the piece is broken off and can be withdrawn. In this way, solid columns, 30 feet in length, and 16 inches in diameter, were obtained. The great advantage of the system is, that substantial specimens of the materials bored through can be obtained, and their relative positions actually seen. No room is left for doubt as to the depths and thicknesses of the various strata, and since the hole is put down perfectly vertical, there is no difficulty in ascertaining the exact angle of the dip if it is steep enough to be appreciable in the core. On the other hand, the rota- tion of the apparatus precludes all knowledge of the direction of dip by mere inspection, and special means have to be devised for ascertaining this particular. 444, REPORT—1895. Returning now to my narrative of events. When it was decided, in 1878, to put down a test hole at Ware, it was anticipated that the Gault there would have been passed through before the Turnford boring had pro- | Fie. 3. «Lorug rods | Sedument tube Core ltbe + Crown Scale, 1 in. to 8 ft. gressed very much beyond its then depth of 836 feet, in which case the latter could have been dis- continued if the Ware site proved unfavourable ; for it was obvious that if the Lower Green Sand did not yield water at the more northerly of the two points, it would not do so at the other, which was so much farther from the outcrop. But delays occurred. Soon after starting, the boring-rods broke in consequence of a fall of gravel from above ; the core-tube and a core-extractor were dropped to the bottom, and the guide-pipe at the top was carried away. This necessitated the sinking of cast-iron cylinders, 6 feet in diameter, to a depth of 30 feet from the surface, by means of compressed air ; a work that occupied some time. Later on, a rod became bent near the bottom of the hole ata depth of 780 feet, and much time was lost in re- covering the crown and tubing which were set fast by this accident. Thus the work occupied much more time than had been expected, whilst at the Turnford boring, the contractors (Messrs. Docewra & Son), after reaching a depth of 896 feet, adopted the diamond drill, and in this way hastened the completion of their work. Whereas the boring by chisels had been proceeding through the Gault clay at an average rate of about 2 feet in depth per week, by the new process an advance of 18 feet or more was made in the same time. Thus it even- tually happened that the Gault was pierced through at both places at about the same time. Shortly before this, a boring made at Crossness for the late Metropolitan Board of Works had shown that there was no Lower Green Sand in that locality ; whilst at Tottenham Court Road, Messrs. Meux had bored through 64 feet of what was at the time erroneously supposed to be Lower Green Sand, and had found it to be a comparatively compact stone, containing but little water. These facts were discouraging, but they still left room for hope that the thinning-out of the water-bearing stratum was confined to the deepest part of the London basin. The results of the New River Company’s borings were, therefore, looked for with great interest, and when, in May i879, Silurian rock was struck at a depth of 7963 feet at Ware, and, a month later, Devonian was found at a depth of 9803 feet at Turnford, those who took a scientific interest in the question, naturally tried to secure all the information obtainable under these exceptionally favourable circumstances. Hence the demand for a special inquiry as to the direction of the dip of these rocks. ——— ON THE DIP OF THE UNDERGROUND PALAOZOIC ROCKS. 44.5 At neither place was there any Lower Green Sand, although in each case the occurrence of a dark-coloured sand, several inches in depth, above the Paleozoic Rocks gave rise to the belief that the stratum was repre- sented in an attenuated form. Recent investigation by Mr. W. Whitaker and Mr. A. J. Jukes-Browne has, however, shown that this was merely the basement bed of the Gault, whilst the 64 feet of rock occurring between the Gault and the Old Red Sandstone at Messrs. Meux’s well, has been declared by the same authorities to belong to the Jurassic system. I will now proceed to describe the various appliances, either suggested or used, for obtaining the desired information, and the manner in which the experiments were conducted. The first idea that occurred was, to make use of a magnetic needle. Fie. 4. Seale, 1 in. to 2 ft. Scale, 1 in. to 2 ft. Suitably mounted,{this would be lowered on to the top of a piece of core that was still affixed to its base, and when it had come to rest in its natural position, it would either be secured immovably to the core, or its impress stamped in some way upon the top. If a sufficiently long piece of core were then broken off and brought up, the angle between the line of dip and the magnetic meridian of the day could be directly read off _ the specimen by means of a protractor. For fixing the needle in position when arrived at the bottom, various devices were suggested, including, amongst others, its enclosure in a pressure-tight box, so arranged as to be capable of becoming firmly attached to the core when lowered over it. In 446 REPORT—1895. this box was to be a solution of gum mastic, from which the gum could be thrown down by the admixture of water that would be allowed to gain Wig. 6. Tubular boring Ber P| Scale, 1 in. to 8 ft. access by the opening of a stop- per manipulated from above. The whole could afterwards be lifted without altering the re- lative positions of the parts. Another proposal was, first, to grind the top of the core to a level surface (fig. 4), and then to let down a strong needle sup- ported on a spring centre, and having steel points affixed under- neath, two near its north end and one near its south end. By releasing a weight, or putting on the steady downward pres- sure of a screw, the points were to be forced into the rock, giving the line of meridian in the most direct manner. A plan was also suggested for lowering a mass of plastic material (fig. 5), such as wax, on to the roughly fractured top of the fixed core, and after an impression had been taken, the frame carrying the wax was, before withdrawal, to be marked by a magnetic needle suspended above its upper sur- face. This was to be accom- plished by having an annular groove, also filled in with wax, on the upper side of the carrier. The needle would be balanced on a spring point at the centre of this circle, and would have differently shaped points on its under side at either end just over the ring of wax. By press- ing these down when they had finally come to rest, the direc- tion would be given upon the carrier, ready for transference, first to the cast of the core, and afterwards to the core itself, when this was brought to the surface. But there were difficulties in arranging an instrument that would be likely to work satisfactorily on these lines. The risk of disturb- ing the needle during the descent of a weight or the inflow of a liquid was very great ; but the principal objection was, that the tubes to which the ON THE DIP OF THE UNDERGROUND PALAOZOIC ROCKS. 44.7 apparatus must be connected were bf steel, and would in all probability so disturb the movements of the magnet as to lead to erroneous conclu- sions. So also, masses of iron in the earth might cause deflection, whilst there would be nothing to indicate that such had occurred. The idea of attempting to trace the magnetic meridian on the rock was consequently abandoned, and it was next considered how the core, or a cast of it, could be marked with some other known line of direction. To do this, the carrier of the marking apparatus, or of the plastic material, must be placed over the centre of the hole, with a horizontal line, the bearing of which is known, marked upon it. It must then be lowered to the bottom and made to operate without receiving the slightest permanent twist during any part of the movement. This maintenance of a marked diameter always in the same azimuth was the most difficult requirement to fulfil. The earliest proposal was, to stretch a pair of fine steel wires verti- cally between a core tube (fig. 6), used as a marking frame, and the top of the boring stage, at 30 feet above ground. These wires were to be on opposite sides of the axis of the boring-rods and at equal distances there- from, but no nearer to each other than was necessary for clearing the sides of the bore-pipe all the way up. They were to be made fast at their lower ends to the core tube, but at the top were to be passed over pulleys, and attached to heavy counterbalance weights for keeping the lines tightly strained during the descent of the marker. There would thus be about 30 feet in height of each always visible, and by placing a theodolite on one side, in the plane of the wires, one of them could be kept under observation, and any deviation from the vertical that might be caused by unavoidable rotation seen, whereupon the marker would be at once restored to its correct position by moving the rods round at top. But the length of wire exposed would have been so small, compared with the full depth of the hole, that it was feared a considerable amount of twist might occur at bottom without detection by the instrument. That plan was consequently given up, and means were contrived for observing the boring rods themselves, and guiding them in such a manner as to prevent all possibility of twist. The details of this arrangement I will now explain. On the circumference of the crown or tube carrying the marker, the ends of a diameter were indicated by differently shaped notches. At the commencement of an experiment, the tube was suspended with these notches opposite to two sharp : pointers (fig. 7), which were Pia. 7. firmly fixed at the Yevel of the ground line on opposite sides of the hole, and at such a dis- tance from its axis as just to clear the crown. The pointers were hinged to fold back, so Z as to leave ample space for the Scale, 1 in, to 2 ft. core-tube to pass freely down. I should mention that the boring-rods at Ware were made of steel _ and were tubular, 14 inches inside and 25 inches outside diameter, and 5 feet in length, with screwed ends (fig. 8). They were coupled up by in- ternally screwed sockets, but when being lowered or raised they were connected or disconnected in 30 feet lengths. At about 6 feet from the _ axis of the hole, in a convenient direction, was hung a long fine plumb-line (fig. 9), towards which a horizontal radial arm, clamped on the boring-rods 448 REPORT—1895. at 30 feet above the ground, was directed. On the outer end of the radial arm was an adjustable pointer, the sharp edge of which was set to almost touch the plumb-line. The rods were slowly lowered for 30 feet, with every endeavour to avoid rotation, but if the radial pointer did deviate at all from the plumb-line, this was corrected by gently twisting the rods. A second radial arm, exactly similar to the first, was then clamped on at 30 feet higher up, and its pointer accurately set to the line, after which the lower one was removed. This was repeated until the marking tool reached the core, and in returning to the surface the cee of fixing and unfixing the radial arms was performed in reverse order. The form of apparatus to be used for establishing a connection between Fig. 8. Lorvg rod f Ly [ ] Socket Scale, 1 in. to 2 ft. the marked diameter on the crown or tube and the unbroken rock, next claimed attention. Whatever method might be adopted, it was obvious that it was only whilst the rock was in situ that this relation could be determined, and consequently the greatest care would be necessary to ensure that any core operated upon had not been broken off during the revo- lution of the boring crown. At Ware, the first trial was made in the follow- ingmanner. Three steel V-shaped cutters (fig. 10) were fixed on the inside surface of a boring crown, at a distance of 15 inches from its lower end, and with their cutting edges at such a distance from the axis of the crown as was about } of an inch less than the radius of the core, whose diameter was 13} inches. One of these cutters was set on the line of diameter indicated by the notches on the outside of the crown, and the other two cutters were placed at equal distances from the same line on the opposite ON THE DIP OF THE UNDERGROUND PALZOZOIC ROCKS. 449 side of the circle, thus marking distinctively the one end of the diameter from he other. Crown and cutters were carefully lowered into the bore hole and over the core at its bottom, with every precaution to maintain the aforesaid diameter in the same known direction. They were then brought up with the same care, and so successfully, that the crown returned to fhe ‘surface with its marked diameter exactly in the direction in which it began to be lowered. Fie. 9. As a check upon what had been done, a cast was then taken of the rough top of the stone. To do this, a tube of a size to encircle the core (fig. 11) was pre- ) pared by fixing a diaphragm in it at a distance of 9 inches above its lower end, and filling in beneath this diaphragm, to a depth of 6 inches, a mass of wax, softened with spirit of turpentine, and coloured with enetian red. A diameter was marked, as in the preceding case, by notches at either end, and the whole was lowered upon the core with the same care o keep the marked diameter in the proper azimuth. “Boring rods Just before making the imprint, water was pumped through a pipe, 15 inches in diameter, that passed i down the middle of both diaphragm and wax. There aes was thus removed from ine top the sediment that PURER would otherwise have prevented a true impression being obtained. The weight of the core-tube, rods, and boring head, was counterbalanced, so that a pres- sure of only 10 lbs. per square inch came upon the surface of the wax, but nevertheless, great difficulty Was experienced in arriving at the proper consistency for the plastic material. If too soft, it would not etain its place until it reached the bottom, and if too hard, a satisfactory print could not be obtained. After several failures, the right admixture was hit upon, and a cast secured. The tube, with its mould of wax, was then brought up, without having received the slightest twist from the time it began to descend to the time at which it again reached the surface. The core-extractor was afterwards sent down. to bring up the marked core for examination. On its arrival at the surface, the three cutter marks were seen in the form of vertical chases more than three feet each in length on the outside of the cylinder of rock, and the rregularities of the top face completely corresponded with those appearing on the wax cast. By tracing on the upper end of the core, the diameter marked on the wax carrier, it was found to coincide exactly with a line passing through the single chase and mid- Scale, 1 in. to 8 ft. way between the pair of “chases, affording a complete } roof of the accuracy with which the proper direction had been maintained bs ~The Committee being anxious to have full confirmation in every respect the results thus obtained, a further test was devised. The bottom of e hole was faced up quite ‘level by the revolution of suitable cutting | te and a groove about 6 inches deep was formed around the circum- , 3. GG 450 REPORT—1895. ference to receive sediment, thus forming a core to that height. The marked crown (fig. 12) was then prepared by fixing across it, near to the lower edge, a stout bar, un the under side of which were three strong steel points, arranged in a straight line on the marked diameter. One steel point was placed on either side of the centre, at a distance therefrom of 5 inches, the third being at 4 inches from the centre. This served to distinguish one end of the bar from the other. The crown was placed over the hole at the ground level, with the points of the three punches in a line between the two fixed pointers, Seale, 1 in. to 2 i. and was lowered without rotation. The weight of the rods was allowed to come on the points, forcing them a short distance into the stone, after which the crown was raised, again without twist, the proof of this being that it returned with its line of points exactly in their starting position. The core, when broken off and Fig. 10. ire. 11. i7ubular borug rod ") Y Y Y i Y Y q A | Counterbalance of weight H of waler pe Core Scale, 1 in. to 2 ft. Scale, 1 in. to 2 ft. brought up, exhibited distinctly the three punch marks, indicating the line whose bearing was known. The boring was then continued 2 feet deeper, and an attempt was made to take a wax impression of the mark- ings, but the attempt proved only, that the smooth surface, to which the ON THE DIP OF THE UNDERGROUND PALZOZOIC ROCKS. A451 stone had been planed off in order to its being marked with punches, pre- vented its yielding a proper recognisable impression, owing probably to adhesion between the two surfaces. The core was therefore detached and drawn up. It came to the surface in several pieces, but, as the lines of fracture extended below the bottom of the shallow groove which existed when the punch marks were made, it was evident that no fracture had taken place before the rock was marked. It then remained, in the first place, to measure the angle between the direction of dip and the diameter marked on the crown or tube; secondly, to ascertain, by a compass placed beyond the influence of the iron of the boring machinery, the angle between the direction of the fixed pointers to which the marked diameters were set and the magnet meridian ; and, thirdly, to learn from an authentic source, the angle then obtaining between the magnetic and the true meridian. By this process it was easily determined that the direction of the dip of the Silurian Rock at Ware, at a depth of 828 feet below the surface, and 31 feet below the top of the stratum, is about one degree west of true south. This is a mean between the angles derived from the two distinct experiments, the varia- tion between them having been 1° 12’.. The angle of dip is 41° from the horizon, as was clearly shown by layers of fossils, along which the stone easily fractured. At Turnford, the general arrangement of the boring apparatus was much the same as at Ware, the only difference of any consequence being, that the rods were connected up in 20 feet instead of in 30 feet lengths. The means employed in determining the direction of dip were somewhat similar to those already described, but greater difficulty was encountered in obtaining reliable results. The complete success that had attended the experiments at Ware warranted the belief that there would not be the same necessity for repetition as when the methods were first tried ; but at the same time it was recognised that every result must in some way be corroborated before it could be accepted as correct. In the first instance, three cutters, for making vertical lines on the outside of the core in the way I have already described, were used. The precautions which had been successfully adopted to guard against the angular motion of the marking tool in its descent and ascent were again employed. But while the said tool was being lowered, an inconsiderate handling of the apparatus by one of the workmen gave rise to the fear that some slight disturbance of the true adjustment of that apparatus had been thereby caused. The marker, on being raised to the surface, came up, not, as had hitherto happened, in the same position as that from which it went down, but showed a rotation of 12 of aninch at the circumference, equal to an angle of 5° 50’. Considering the circumstances attending the interference that had taken place during the lowering, it was con- sidered a fair inference that the core had been marked with the tool turned in the direction in which it came up, not in the position given to it before it was sent down. An endeavour was then made to obtain a cast in wax cement in much the same manner as at Ware, but this proved a failure owing to a piece that had broken away from the top of the core having fallen against the side of the hole, so that the tube carrying the wax could not be got down over it. Although no information was to be looked for in this instance, still, as a test of the accuracy of the operation, the rods were guided as usual during their ascent, and when they came up were found not to G@G2 A452 REPORT—1895. have twisted in the least. The ‘extractor’ was then lowered to break off and draw up the core. Studii anatomici sulla famiglia Ophrotrichidz del Golfo di Napoli. ‘Ricerche Lab. Anat. norm.,’ Roma, vol. 4, 1894. 9 Sull’ apparecchio genitale del Syndesmis <«chinorim, ‘Boll. soc. Nat. Napoli,’ vol. 8, 1894. Ph. Knoll s ° » Ueber die Blutkérperchen bei wirbellosen Tnieren. ‘ Sitz. Ber. Akad. Wiss. Wien,’ Math. Nat. Cl., B. 102, 1893! T. Groom ° . . On the Early Development of Cirripedia. ‘ Phil. Trans. Roy. Soc.,’ London, vol. 185, 1894. J. v. Uexkiill . . . Physiologische Untersuchungen an Eledone moschata, III. Fortpflanzungsgeschwindigkeit der Erregung in den Nerven. ‘Zeitschr. f. Biologie,’ B. 30, 1894. - Physiologische Untersuchungen an Eledone moschata. IV. Zur Analyse der Functionen des Centralnerven- systems. Jbid., B. 31, 1894. H. C, Bumpus. . - The Median Eye of Adult Crustacea. ‘Zool. Anz.,’ Jge. 17, 1894. W. Wheeler . ° . Protandric Hermaphroditism in Myzostoma. Jhbid. V. Willem La structure des palnons d’Apolemia uvaria, Fsch., et Jes phénoménes de l’absorption dans ces organes. ‘Bull. Acad. R. Belgique,’ t. 27, 1894, AT THE ZOOLOGICAL STATION AT NAPLES. 479 W. Nagel = ; - Beobachtungen iiber den Lichtsinn augenloser Muscheln, * Biol. Centralblatt,’ B. 14, 1894. is Vergleichend physiologische und anatomische Unter- suchungen tiber den Geruchs- und Geschmackssinn u. ihre Organe. ‘ Bibl. Z.,’ Heft 18, 1894. + Experimentelle sinnesphysiologische Untersuchungen an Coelenteraten. ‘ Arch. Phys. Pfliiger,’ B. 57, 1894. is Ein Beitrag zur Kenntniss des Lichtsinnes augenloser . Thiere. ‘ Biol. Centralblatt,’ B. 14, 1894. = ©. Lanz . : : . Zur Schilddriisenfrage. Leipzig, 1894 (partim). J. E. 8. Moore : . On the Germinal Blastema and the Nature of the so-called ‘Reduction Division’ in the cartilaginous Fishes, ‘Anatom, Anz.,’ B. 9, 1894. J. Gilchrist . : - Seitrige zur Kenntniss der Anordnung, Correlation und Function der Mantelorgane der Tectibranchiata, ‘Jen, Zeitschr. f. Naturw.,’ B. 28, 1894. N.Iwanzoff , - - Der mikroskop. Bau des elektrischen Organs bei Torpedo, Moskau, 1894. G. Mazzarelli . 4 « Intorno al rene dei Tectibranchi. ‘Monitore Zoologico Italiano,’ Anno 5, 1894. + Sull origine del simpatico nei Vertebrati. ‘Rendic. R. Accad. dei Lincei,’ vol. 3, 1894. A. Korotnefft . , . Tunicatenstudien. ‘ Mitth. Zool. Station, Neapel,’ B, 11, 1894, W. Salensky . F . Beitrige zur Entw.-Geschichte der Synascidien. 1. Ueber die Entwickelung von Diplosoma Listeri. bid. 8. Trinchese . . Protovo e globuli polari dell’ Amphorina caerulea, *‘ Me- morie R. Accad. Sc. Ist. Bologna,’ t. 4, 1894. G. W. Miiller . X - Ostracoden. 21. Monogr. ‘ Fauna u. Flora des Golfes von Neapel.’ Berlin, 1894. SE P.Samassa . : . Zur Kenntniss der Furchung bei den Ascidien. ‘Arch. f. mikrosk. Anat.,’ B. 44, 1894. L. Murbach . : . Beitrage zur Kenntniss der Anatomie und Entwickelung der Nesselorgane der Hydroiden. ‘Archiv f. Naturg.,’ 60 Jgg. I., 1894 ( partim). G. Gilson ° F . The Nephridial Duct of Owenia. ‘Anat. Anzeiger,’ B. 10, 1894, Th, Beer. 2 ‘ . Die Accommodation des Fischauges. ‘ Arch. f. d. ges, Physiologie, Pfliiger,’ B. 58, 1894. G.Formario . i . le degenerazioni dell’ encefalo e dei muscoli negli Scyl- lium. ‘Atti R. Accad. Med. Chir. Napoli,’ Anno 48, 1894, M. Golenkin . . . Apologische Notizen. ‘ Bull. Soc. Nat. Moscou,’t. 8, 1894. J. Hjort . 3 F . Beitrag zur Keimblitterlehre u. Entwickelungsmechanik der Ascidienknospung. ‘ Anat. Anz.,’ B. 10, 1894. B. Lwoft , * “ . Die Bildung der primaren Keimblitter u. die Entstehung der Chorda u. des Mesoderms bei den Wirbelthieren. ‘Bulli. Soc. Nat. Moscou,’ t. 8, 1894. 2 ———— <<“ --_ = —-_—_ = G.Tagliani . 5 . Ricerche anatomiche intorno alla midolla spinale dell’ Orthagoriscus mola. ‘Monitore Zoologico Italiano,’ Anno 5, 1894. ‘ _ ©.C.Schneider . . Mittheilungen tiber Siphonophoren. I. Nesselzellen. ‘Zool, : Anz.,’ Jgg. 17, 1894. _ 8. Fuchs. . - . Ueber den zeitlichen Verlauf des Erregungsvorganges in . marklosen Nerven. ‘Sitz. Ber. Akad. Wiss. Wien,” Math. Nat. Cl., B. 103, 1894. ; ” Einige Beobachtungen an den elektrischen Nerven von Torpedo ocellata. ‘Centralblatt f. Physiol.,’ B. 8, 1894. 4.80 REPORT—1895. The Climatology of Africa.—Tourth Report of «a Committee, consisting of Mr. E. G. RavensTeIn (Chairman), Mr. BALDwin LatHam, Mr. G. J. Symons, Mr. H. N. Dickson, and Dr. H. R. MILu (Secre- tary). (Drawn up by the Chairman.) Your Committee in the course of last year granted a complete set of instruments, including a mercurial barometer presented to them by the Meteorological Council, to the Scottish missionaries established at Kibwezi, on the road from Mombasa to Machako’s. They also supplied Mr. Hobley, now in Uganda, with one of Symons’s earth’ thefmometers. “Sets of instruments have now been supplied to the following stations :— ' Bolobo (Rev. R. Glennie).—Registers up to tie wane been regularly received since January 1891. The abstract for thé past year has been prepared by Mr. H. N. Dickson. Lauderdale, Nyasaland (Mr. J. W. Moir).—An abstract of one year’s observations has been sent home through Mr. Scott Elliott. Zombe, Nyasaland (Mr. J. Buchanan). —Registers of the observations made from June 1892 to March 1894 have been received. ‘The abstract published in the Appendix has been prepared by Mr. Dickson. Lambarene, Ogowe (Rev. C. Bonzon).—-Only one month’s observations have been received. Kibwezi, British Kast Africa (Scottish Mission).—The instruments were only granted this year. One year’s rainfall observations have been received. Warri, Benin (Capt. Gallwey).—The registers have been received up to the date. An abstract has been prepared by Mr. Dickson. The sets at all these stations, with the exception of Warti, include a mercurial barometer, four thermometers, and a rain-gauge. That at ‘Warri includes a black bulb thermometer. Meteorological reports from thirteen stations in British East Africa have been received. These stations lie on or near the coast, between Wasin and the Jub, and along the road connecting Mombasa with Fort Smith in Kikuyu, the climate of which is described as being exceptionally well suited to European residents. These observations were, in most instances, made by officials of the Imperial British East Afriea Company. The abstracts have been prepared by the Chairman. (See Map, p. 491.) Your Committee regret that the instructions laid down for the guid- ance of observers should, in many instances, have been set aside, and that observations should have been made at hours precluding the possibility of deducing trustworthy means. Where circumstances do not admit of the instruments being read thrice daily—at 7 a.m., 2 P.mM., and 9 p.m.—the thermometers should be read at 9 a.m., or twice daily, at an interval of twelve hours. The barometers, however, should be read at intervals of six hours—say at 9 A.M. and at 3 P.M. Your Committee have expended the 5/. granted. 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REPORT—1895. Rainfall—Amount in Inches. Station By Sloe | em |e) ete leer) Oe lesa) eee Seala| So te | s |e epee | gee Chuyu (4° 38 $, 39° | 1893 [4°51 [1-53| 6-74 | 25:30 | 10:80 |9-24 2°65 |9-9] (0-38 [0°68 | 10-94 |1-55 | 66-27 21 E.). 1894 | — |2:05| 2-12 | 2°63 | 10-87 |5-54 |4-19 |9-95 0-16 |O11 | 7°42 |4-94) — ACO (025 2°00 fe — | — | — | eee a Mombasa (4° 4’ S, 39° | 1875 |— |— | — | 12-20 | 74-73 |6-30 |9:22 |1-g9 [0-35 [4-60 0°35 |6s) — 42’ E,, 60 it.). 1876 |0-35 [0-18] 3°57 | 5-99 | 76-40 |3:16 |4°68 |9-79 |2-68 |1-00| 0°56 [0-60 | 41-89 1890 | — |— | — | 6-94 | 76-65 |1-59 |210 |1-36 (0-57 (015) 252 1-32) — 1891 |0-62 |0-02| 0-62 | 3:74 | 74-87 |5°63 [1-68 |.03 |2-46 [8-83 | 3°53 [2°56 | 46-56 1892 |0-11 [0-43 | 0-41 | 6-18 | 77-32 |1-43 |2-17 |]-96 |1°52 (0°35 | 1-26 (0°39 | 26°83 1893 |2-43 /1°85 | 4°68 | 12°51 | 74-29 |7-69 |2+15 [9-78 2-10 (2:27 | 10-91 0°51 | 64°17 1894 |0°16 |2:51 | 1°46 3°04 | 72°29 |4°27 |1°49 |1-33 [0:29 [0°65 | 7°59 [2:88 | 37-96 1895 |0-01 |0-34| 303 | — | — a 1 ah aid oz Mean /1:22|0-94| 2-16 | 7-67 | 13°47 |4°63 13-72 |2-7g [2°55 (3°50 | 5ST |1-73| 49°88 © 477g, 39° | 1892 |o-82|o26| — | 1-14 | 2407 |5-21|1-53 |1-21 12-70 |0-00| 2-77 \o00| — Tee Co pcorvers in | 1893 |1-50|0-57| 5-41 | 7-01 | 939 (7-87 l2-80|1-¢7 lorss (1-39 | 786 lores | 4066 1894 : J. Bell Smithand | 1894 |0-00 |0-00| 1-91 | 4:57 | 75:39 [5-46 [1-85 [0-49 [0-37 |0-17| 7-20 lo-¢o | 38:01 K, MacDougall. SLB 5 9 0200)) 0:08 Be 6 =) ea ica a a ia ee ae Mean |0°58 [0°23 | 4-14 | 4-24 | 12-93 [618/206 [1-12 {1-21 |0'52| 3°92 [0-41 | 87-54 Ce o | 1891 }— |— | — | 5-85 | 12-00 |4-26 |3-68 |o-08 [1-80 |3:31| 3-48 l#o2| — Mey, © 18S. 4° | re92 foe Jo-50| 0-49 | 5-97 | 24:90 [3°04 [i-e2 lo-zg (1-41 (orgs | 0715 lo-9 | 302 cs 1893 [0°75 0-12 | 2°38 | 18-50 | 7-83 |7°65 |2-26 |1-71 [1-05 [1-14| 5°77 |1-63 | 50-79 1894 |0-40|0°05 | 1-28 | 0-45 | 14:09 |5°21 1-76 '1-18 (0°00 0-07| 2:50 [1-96 | 28°95 L505 (10-08 0-10} a5 t4 — || = a eae of Rolie ole ae ee Mean 0-45 [0°19] 1-25 | 7-69 | 22-08 [5-26 2-38 1-31 |L-07 |1-22| 2-97 |1-95 | 37°82 ; © 10° s, 39° | 1893 [3-75 |2-24| 2-96 | o-77 | 402/362 1-14 \204l069 (009) #77/— | — ork si aaNet hE Erg? Recetas ra ota deb at PBS SO] = p9e a Ye I ee Se ae f al serail nine lay | iG sees Magarini (3° 5’ S,, 40° | 1893 {0°85 (0-37| 2-69 | 73-45 | 5:25 [5-61 2-65 |1-97 (0-72 [0-84 480 |1-00 | 40-20 fn, © > S» 40° | r894 Jo-00 |o-00| 3-38 | os | z0-32 [4-42 (1-69 = 0:07 |0-00| 756 4-48 | 33-28 AOS 10°O0 WaT B07 | — | Sn lah ee Lamu_ (2° 16’ $, 40° | 1890 |0-21|0-00| 1-50 | 1-95 | 78-06 |2:50 2-17 1-22 |1-20 |013| 0°04 0-00 | 28-98 54’ E.). 1893 |0-41 |1-04| 2-97 | 1550 | 16:35 2-93 |0-85 0-56 0-97 |1-70| 0°35 |o-91 | 44°54 1894 |0-00 |0-00 | 0-15 | 0-25 | 75:28 |215 /0-45 [0-22 0-00 |o-10| 1-60 (0-94 | 21-14 Mean |0°20 0°35 | 154 | 5-90 | 16-56 2°53 1-16 0-66 0-72 |0-64| 0-66 0-62 / 31-05. aes) sk ees Praeral Kisimayu (0° 22/ §,, 42° | 1893 |— |— | — | 4-491 5-63 jo-16 /000/— | — |— | — {|— | — 33/ E.). 1894 |— |— | — | 389) S24 |1-17 0°53 0°52 0°00 /029| 0-60 7-59 | 13-73 1895 (0-00 |0-00] G00 | | — |S tes Jem eo) |) eee eee Mbungn (3° 46’ §., 39° | 1891]— |— | — | — | 6-03 [2-25 '0-85|1-12\1-21 (0-70) 3-72 354) — 30’E.). Observer : Rey, | 1892 |1°52|1°49 | 2-37 D765), 12:69) 053 — | —— bo aes 1893 |4-47|113| 8-65 | 584) 3-78|— (0:49 /2-13|051|1-56| 507 |— | — 1894 |— |— | — | — | 7-30 0-64 /1-70 0-75 |0-03 0-04 5-64 2-08) — 1885 }0p0}109| 4-17 | — 3 > |odes fee tl 2 |) ene oe Nai (3° 20'S, 38° 29H, | 1894 |— |— | — | — | — | |— |_| |] 240 |se0| — 2,400 ft.). “Observer : | 1895 /110/2-22/ 501 | — | — dee | | a i Ch. Wise. Kibwezi (2° 25’ S,, 37° | 1893 | — |— | — | — | — |— |— |— |— |— | 1872 |7-80 Ee 55’ E., 3,000 ft.) : Ob- | 1894 [012/058 664 | 1-44 | 1-13 [0-05 [0-00 [0-00 |0-00 |0-00| 13°55 3-24 | 26-73 server : Rev. T. Watson, Machako’s (1° 31’ §,, 37° | 1893 | — | — | — — | — |—|— |— |0:00/1°37| 6-64 |6-34) — 18’ B., 5,400 ft.). 1894 |0°75 0°16] 5-48 | 9:33 1:93 |0°58 |0°09 |0:06 |0°02 |1:27 | 18°16 |4:13 | 41-96 1895 [0-00 [3:85 | 10-13 = =o ge cag, Fs Fort Smith, Kikuyu (1° | 1893 |— |— | 13°65 | 15-60| 854 0-28 1:01/— |263|061| 5:09 3:80) — 14’ S., 36° 44’ E., 6,400 | 1894 [112 |0-23| 5:33 | 7-23] S27 [3-46 213 [1-02 (2-22 /1-27| 668 932 | 48-12 tt.) 1895 1/0°00)/7-48 10-46} —= «| Eee) See eee ee ee * The means for Mombasa are deduced from n Frere Town, where 90:06 in, fell in 1877, 51°30 in. i early eleven years’ observations, including those made at n 1875, 45°57 in. in 1879, and 44-75 in. in 1880. THE CLIMATOLOGY OF AFRICA. 487 Heaviest Fall of Rain within 24 Hours. Station 2 2 c & 2 E | 2 2 & 2 } a “s= 05) we he = — ee — kver | 003 | 150 | 258 | 143 | 180} 117 | o16 | 09 | 1-43 | 162 | Mombasa . «-~z| 012 | 214 | o46 | 1-68 | se2 | 1-63°| 050| o40| o70| 027 | 118 | 153 ‘|Takaungn . . «| — | — | rai | 197 | #55 | 1-70'| 0-75 | 015 | o19 | 017 | 038 | 033 Malindi . . .| 035 | 0-05 | 0-85 | 0-20 | 3-25 | 1:30 | 0-44 | 019 | — | 0:07 | 250 | 0-95 Jilore . 0 a -| — _ 1:12 _— _— _ _ — — el 1:20 | 2°16 Magerint =. «2. ~.| — | — | 1:78 | 0-38 | 267 | 087 | 045 | — | 040| — | se7 | 2:56 Tom. . . .| 000| 000| 015 | 025 | 30 | 075 | 030| o12 | — | o10 | 140 | 0:5 Kisimayn . . «| — | — | — | 220] 240! 070 | 035 | 0-15 | 0-00 | 029 | 040 | 13 Mbungu. .. —_ = _— —_ 168 | 022 | 0-76 | 019 | 0-03 | 0-04 | 1°57 | 0:92 | | Kibwezi A . «| O12 | 0-33 | 2°90 | 1:04 | 067 | 005 | — _ _ _ | ood 1:18 Machako’s . .. . | 050 | 012 | 1:76 | 1:94 | 053 | 0-47 | 0:05 | 0:03 | 0°02} 0:70 | S18 | 1°25 Fort Smith . ° - 072 | 020 | 2:96 1-40 | 2:07 | 1:38 | 1:08 | 0:37 | 1:08 | 0°53 | 2-13 | 167 Number of Rainy Days. Only Days on which at least 0°01 in. of Rain fell are counted. " as = =| bm 2 > tb +s (Sewell + Yea: a 2 & 2 o a =o a 2 o XY Station ear | I 2 S & g 2 fe 2 3 / 8 ie a ear Sage) .|1s93| 5 |2 | 5 | 10 | 19 | 20 | 16 | 12 4 a \igp hae | Greg eee crigns || 3 | 7 Cue Ure aieuoe ul) a 3 i Paeeoe le lok cry |: ees eee i695) a |) vy) — Ce | eee | eee | enema ee ad SU trac |-190a-| 7 |~s | a0 | 19 |) 24-|-16 | 1 | 22 | 18-| 10-|.a5-|-6 | 164 Eo Mitigaw | 2) 83 | 06 8 | 18 | 11 7 9 8 9 | 19 ies * © lt FRET aM FeavTee he ey fe Pa amo SERS eta Al ee A 2 ee Takauneu .|1893|3|1| 7 | 12 | 2 | 18 | 1] 1 4 Sy MG 102 z eibisoi c= ||| 13. perder ae oe 8 3 1 9 4 tice clu Gi stop et ca ca (Pe eet rec eT ee ee [Malindi = = | — 65°2 = 735 | 845 | 758 —_— 711 =| 77-4 _ + 14th to 30th only. BoLoBo (CoNGO)—continued. oe ane. ae amit y Cloud—Amount Rain Weather Month 2 / 1 5 | dy 2 9 7\9 9 5 ge Hea- 2% Fe was Ree Pat Pat, Me Pat. see pM, eae “ie PM. aN Mean} iz ia ae a a2 ge 1894 See! ee) inceg any finn P.C.| p.C.| p.c.| 9 3 B ae pis | In January . 71:9 |76°2 72:7) -760 | -802 769 92 | 70 | 88 | 8-4 58 | 67 70 | 6°64 | 12 , 2°10 4/ 0] 2 February. 72°5 \72:73:2 776 |°828' ‘777, 92 | 69 | 86 | 7:8 6-0 61 6°6 10:59 | 11 6-44 2 I 2 March. . 724 (774 732 | 772 = |°810 Tis 92 | 63 | 85 | 82 65 6:0 6-9 3°75 | 10 | 2°38 ie | 0 April . . | 726 |76-9.726) 777 |-805|-762| 92 | 65 | 86| 7-7 | 64 | 61 | o7 | 767 | 11 i soo | 4] 0] 3 May. . .| 723 |77-1,73'5| -771 |-826|-787, 92 | 69| 86 | 78 | 68 | Go | co | @71|13) 283 | 3] 1] 2 Jie | 70°0 ss ian Gehan 698 aed 87 | 64 | 82 |-7:9 65 63 69 | 0.00 | 0 0°00 0; 0 1 July . .!| 68:4 (74:3 )71'7| °647 | °702; fo 83 | 58 | 82 | 7:2 8:2 76 T7 003 1 0°05 0 | 0 1 August . (69°5); — | — (680) | — | — (85))/ — | — | (86) | — | (68)| — | 385 7 | 1000) a] SORE September / 70-4 |75°2|722| 692 |-729|-732, 82 | 59 | 80 | (7-1) | (6-1) | (78) | (7-0) | 2692, 52, 1282 3] 0} 0 October | 714 |74:8/71°3| -741 |°767/-732| 90 | 71 | 88 | 8-6 69 54 70 431 | 9 | O64 0.) Ose November | 72:0 |75°3|72°1| °761 |-781|°755 92 | 71} 88} 8-2 67 75 i) 5°46 13} 1-20 2 0} 2 December. | 71:8 |76°0|73°0| -754 |-792|-775 91 | 68 | 87 | 87 | 5-4 | 52 | G4 [1103 13) 447 | 1] 2] 1 ear | 708) eT ea SON | — 18:0) — 6b i ear73410b) (6:4 lias | 5 | 15 In the hourly barometric observations considerable interruption, through illness of the observer and other causes, was unavoidable. The observations wanting on the term days during the first four months of 1895 have been inter- polated as far as possible by drawing the curve for each day and filling up by comparison with the curves for days immediately preceding and following it. It must be admitted that the method is liable to considerable error, but under the circumstances it is believed that the results may be useful. The barometer readings have in all cases been reduced to 32° F. and corrected for gravity. i . THE CLIMATOLOGY OF AFRICA. Bolobo Hourly Barometer Observations, 1894. 489 January February Hour =— . Ist 11th 21st 1st 11th 21st Midnight . | 28-802 28°897 28°878 28-808 28°S32 28°851 1 A.M. “798 S95 S76 "824 S38 835 2 5 797 S94 ‘873 “840 S44 ‘S35 See y5 ‘797 893 865 “S40 “S50 *835 ee, 795 ‘S91 ‘87 *839 S57 845 BL 4, TOL “890 $76 ‘S47 S65 S64 ee t, 836 920 881 ‘S60 872 890 ees; ‘ST7 “938 887 “S71 879 919 Psy “884 “939 901 875 886 925 9) 4, 893 “947 “912 ‘S78 ‘910 952 EOE, 883 934 “901 880 926 947 Me, 4 871 914 883 864 922 937 Noon al 821 “908 872 "834 “891 ‘906 1 P.M “805 878 *850 810 “848 858 al 55 | ‘770 *856 824 Sricell 825 830 2 att 755 849 786 “743 307 817 ok Daas “745 *858 ‘778 ‘726 ‘786 “T91 as H “+742 "855 ‘780 ‘715 ‘772 BOLTS Oy ss 753 *855 ‘786 722 ‘776 “782 Mes; 783 “866 ‘791 ‘740 “SOL 785 ee sy 815 “880 “819 ‘763 813 813 a 831 “911 *843 ‘781 842 829 iy 3; 837 ‘913 857 821 ‘S60 “851 1 837 ‘914 866 825 S65 863. March April Hour 1st 11th 21st Ast 11th 21st Midnight . 28-920 28°S90 28-764 — — _ | 1 A.M. S80 ‘S96 767 == = = Det. ‘S58 “899 770 Aa = = a AS | "S54 S98 778 - —— _- a a5 | "857 898 179 = = = (ae 889 905 785 — —_— — Bl a: | ‘910 "921 ‘793 28°853 28852 28°866 ta 3, "925 “936 “808 *865 858 886 ory, “939 946 834 “866 *870 903 ae, ‘937 “947 856 882 886 920 OF ;, 9B5 "946 "851 872 SSS ‘917 uy, | “906 933 844 845 873 889 oon . “883 OL 817 832 844 “871 Pol P.M, 862 *886 781 ‘790 “816 *850 mar 5 “S40 “860 “749 ao “804 “810 Bas 5, 807 “860 “690 13 ‘790 TTT eae 5, 795 “860 ‘707 726 ‘748 763 iD ,, 79 *858 725 724 740 “753 GF, SOT S59 ‘720 ‘746 766 783 ac, “816 867 ‘749 788 818 *818 ms). 5, “S31 873 ‘793 817 *830 852 aD 5s S61 “876 826 *856 826 *859 710 .,, *888 “887 834 *860 S23 *875 Ts “902 S94 S38 “860 S27 “891 1895. REPORT 490 “ROIIUIIE PUY VUIOTXLO LRIUT dy MOLY poonpop sB “T o[§ Sutaq Jo pvaqsur “FT 92 pasoxo Aqeqoad you soop ainqeV1dd M9} UBaTE aILT, *"pezSN.49 oq 07 JOU vAV SADQOTMOTLAA} WINTAIXLM PUL TINTTTIIUT 919 JO SSUIpe ot ay, ] | | | olo /s 2010. |-0 | 0.) 0 asl eu Ta: |e rr: g | (LT | FT /¥eS [oIbT | Tez | so | 66 es ou 318 92 |* * * Indy ot jo | | T{O}o}o}o jo jst}s |2 |e |& |e | wt | Frees |FtT | Tes | €9 | 86 joes [6-02 0.86) T-18 Gb. | * + ‘Moreyy o}o0 /e 0/0) 0/0) 0/0 jo j4rie |e jt 1 |e | goo | s |¢o0 jtoFr| Zee | co | 66 [Lee |e 996) G8 | OFZ |* Axnraod 0/0 |0 t}o|o|}/tlojo jo |tw/s jo |e |1 |e | sec] s jee |eorr| ete | 99 | 26 |ezelPTeit-eo| 818 | Lez |* * Sxunuee | aah i | S681 o{stjeer et ar} 2 | 2) ¢|2| 0 | st 96 | ov | 22 | te | og | $6 |) oe | ret\ce-rttosst | eet | co | cor |e-telz-12 | Lee [°° * avez o}o |o |1@/0 |o}o0]ojojo}r js yerjt jo fe je |* | ore |e |re9 joesr| tes | o: | 66 [ene er | Lez | * taqmeoaq 0]/0 jo |es\s |}o]o/o]o]o}F jo |i) t |o |e | t | t | ger | or leoe Jozor | 60s | co | 66 2-28 \e-c2 3-86) G62 | BFL | * JoqueAoN o/t |9°| or | + | t}o}ol]o;ojr |e jorjt js ja |t |e | t+ | et joer leser | er | 89 | 96 208012 |268| G2 | F-e2 | * * 40q0300 ojo |¢ |e}e |o}o}o]ol]ojo jz |a{t jo }o !o Jo | ont | te joer |rost | et | 29 | #6 |¥6z\2-12|T-28| 6-92 | 62 | * ToqMo;dog 0 {0 |&)8 jo |o}/0/0}0/0/]0 |e) 9 |e |o |o |o | | et | sx jzecr jeert | et | 29 | co lOoe ror |z28| tus | Les |* * gensny ojo jez |t |}o}o0};0/]0]o0)/0 |stjar{/t jo jo jo Jo | oo8 | rr] Fe-9 |2eor | sor | 29 | F6 |008\912|F88] 882 | 082 |* * * Arne Ot | 1/0/o0]o0/o0]o]o/t |tsl/e |% }o |& jo |i soe | Fz j1F9F |8crt | 9.01 | 69 | ce [608 |612|\9e8| o82 | er |* * * oung oie /9 jetjs }olo}rtjsljole le je le le le je |r || ogg | 52 josce lever | 02 | 69 | 66 le-celoce|rae| 202 | e472 |" * * Sem o}s |sij¢ |tjs}rtj}e|sejojr lo je je }s |r le |e | srt | sr iseo jeser| tre | 69 | co |res|zz2\1-F6/ 008 | #92 |* * * THdy 0}/s |sr)2 |o |r} s}oj;ojojr|s je js jo |F | |o | or | sr |es¢ |rosr | tte | 89 | 86 oes |s.c2/9-¢6| 08 | eox |* * *uoreH ojo /st}¢ jt |/a]/rjo;tilo|sjajs |e je js lo |g |lses}e |eoe |eser| oes | 69 | cor |F-F8loez\6-96] 9.28°| ors | *° *Sxunaqag O}2 j4t)t |o|t}]e}o)}s}o/s |st}s jo jo |e | | 8 | 000 |e |ee0 [Lert | 9.0¢ | 29 | 96 8-18\9.02/T-€6) F18 | &oL | * * Saunuee rag uy ° ° ° ° ° ° ° ° ° F681 } Pee rere ee a _ — -|- — | a | a b> a = p co ~ aa | | a ; | z z |e arae| aa aa BE es a = = = = - 7 ame We 8 He asuey = —= P< 2 a Nad 9 wy) fone Swed. HIUOTL Pate SS Urey [ee aee aanqerednoz, UoT{OaIIp payloads B MOAT MATG 41 YONA uTsABG Jo IOqUUNNT : PUTAA 99 Jo UOTOaAICT ‘CN VOUT HPO OTH SOU UO LAT 1840000890 “PALO AG o§ BUT “N18 oG “WT “Cupuag) punt THE CLIMATOLOGY OF AFRICA. 49] Lambarene, Ogowe, Lat. 0°40’ S., Long. 10°18’ E£. Observer: Rev. C. Bonzon. Result of observations made at 9 a.m. during November 1893. Barometer at 32° i . B . 29°864 in. Temperature : mean of maxima 5 wei? EB: PP > minima ‘ 40°-2 Extremes . 3 . 98°0 and 66°3 Dry bulb . : delat il haa 2) Wet bulb . F eo aSO Rain, 13:10 in. on 23 days. Heaviest fall, 164 in, Cloud, amount, 80. Meteorological Stations in East Africa. The Exploration of Southern Arabia.—Report of the Committee, consisting of Mr. H. SEEBoHM (Chairman), Mr. J. THEODORE BENT (Secretary), Mr. E. G. Ravensrein, Dr. J. G. Garson, and Mr. G. W. Broxam. (Drawn up by Mr. BENT.) Tus last winter, after leaving Muscat we proceeded along the coast for a distance of 640 miles, and applied ourselves to the exploration of a certain district known as Dhofar, with the Gara mountains. The results of this expedition, which lasted over several weeks, may be treated of under three different heads :— 1. The geographical results referring to the nature of the country, its configuration, and its productions. 2. The anthropological results, with an account of the inhabitants and a comparison of them with those of other parts of Arabia. 3. The archeological results of the study of the various ruins and identification of sites mentioned by ancient authors. (1) The district of Dhofar is for Arabia a most remarkable one, It constitutes a sort of oasis by the sea, and consists of a flat alluvial plain about 60 miles long and 9 miles at its widest point, very fertile, and with 492, REPORT—1895. abundance of water lying either in stagnant pools or procurable by sinking shallow wells. It is capable of producing almost anything : cocoanut palms grow in clusters along its whole length ; cotton, indigo, tobacco, plantains, jowari; and in the gardens papyas, mulberries, lemons, oranges, and chillis grow profusely. The inhabitants of the villages scattered along the coast are for Arabia particularly prosperous ; they are governed by a representative from the Sultan of Oman, who has of late years been successful in establishing peace. Behind this rich plain is a range of mountains, known as the Gara range, rising to about 3,000 feet above the sea level. In the valleys sloping towards the Indian Ocean on the south, and towards the desert of Nejd on the north, are found the various frankincense districts where the frankincense tree, Boswellia Carteri, is still found, and which constitutes an industry for the inhabitants, as it has done for thousands of years. There are three chief districts where the shrub grows, and the export of the gum is now about 9,000 cwt. per annum, which is sent to Bombay in dhows. Myrrh is also found in proximity to the frankincense tree, and in ancient days the commerce in these odoriferous drugs gained for this district a world-wide reputation. The Gara hills are rounded and undulating, except on the coast side, where the approach is precipitous and rugged; they are of limestone formation, and retain a surprising amount of moisture, which is at the same time the cause of their fertility and the fertility of the plain of Dhofar, which is an alluvial deposit from them. The valleys running into these hills from the coast are of great fertility, containing a dense mass of tropical vegetation, huge sycamores block up the valley, with cacti, acacias, and numerous creepers; in several places lodgments of water have formed themselves into little lakes or tarns, an altogether unknown condition of affairs in any other part of Arabia. The mountain sides are honeycombed with caves, in which the inhabitants dwell with their flocks and herds. Right up to the summits of the Gara mountains the same condition of fertility is observable—they are covered with grass all over, and clusters of sycamores grow right up at the summit, giving to them quite a parklike appearance ; and the flora of this district is very extensive. Although we were there during the dry season we collected 260 different specimens of plants, as against 150 collected during a much longer period and more extended area in the Hadramut last year. These plants have now been deposited at Kew, and though more numerous they do not contain so many new varieties as those from the Hadramut ; they establish an extension westwards of the Indian and Beloochistan flora, whereas those of the Hadramut are more African in their character, tending to prove by their geographical distribution that the floral line of demarcation between Asia and Africa takes place somewhere between the Hadramut and Dhofar. From the summit of the Gara range an interesting view over the frankincense country is obtained. To the north the hills slope down towards the desert of Nejd, which gradually destroys the vegetation, and ends in a long blue horizon like the sea. To the east and west the same characteristics are observable, and to the south the view is bounded by the sea. The district of Dhofar owes its peculiar fertility to the water- retaining qualities of its geological composition, and to the regularity of its rainfalls, which occur from July to September, when the valleys are turned into torrents, and even the Bedouins find it difficult to get about. On proceeding up a valley to the east of the Gara range we came ON THE EXPLORATION OF SOUTHERN ARABIA. 493 across a very curious natural phenomenon. The valley, which is here about. a mile and a half broad, with hills on either side reaching an elevation of about 2,000 feet, has been blocked up by a calcareous deposit, which has collected round an isolated hill in the centre of the valley, and has formed itself into a perfectly sheer and precipitous wall or abyss. To the east of this hill the abyss is 550 feet high and three-quarters of a mile in length. It is hung with white stalactites, and presents a whitish-grey colour ; over this abyss small waterfalls precipitate themselves, and the ground below is spongy and fertile, and all along the river bed the rocks are white with calcareous deposit. At the top of this abyss an exceedingly fertile flat meadow extends for several miles inland, richly wooded, and providing rich pasturage for the cattle of the Bedouins, who own it ; and about a mile and a half from the abyss are two lakes joined together by a meandering stream. They are long and narrow, but in places of consider- able depth, and it is the overflow from these lakes which falls over the abyss. Bulrushes, water plants, and water birds abound here, and the spot is marvellously fertile. (2) The inhabitants of the Dhofar district may be divided into two distinct groups, namely, the Arab inhabitants of the coast villages who cultivate the fertile plain, and occupy themselves in fishing, and the nomad Bedouins of the Gara tribe, who inhabit the mountains, and are purely pastoral. The coast Arabs are chiefly from Oman, and are of the Ibadiyeh sect, recognising the Sultan of Oman as the head of the church. This sect of Mohammedans is much less fanatical than the others in Arabia, probably from the long struggle they had with the Wahabis of Nejd at the com- mencement of this century. They offered no objection to our visiting their mosques, and we were subjected whilst amongst them to none of that fanati- eal hatred which caused us so much inconvenience during our sojourn in the Hadramut last year. The mosques of the Ibadiyeh are small and with- out minarets ; their heterodoxy consists in not accepting any of the Imams who succeeded Mohammed, but they consider that the Imam or head of the church is to be elected by the people as occasion requires. Eighteen years ago the Arabs in Dhofar were in a very sorry condition, and sent to the Sultan of Oman toask him for a governor : the blood feuds between the tribes and the hostile attitude of the Bedouins rendering existence almost intolerable. Sultan Tourki of Oman sent as Wali a trusted friend of his named Suleiman, who has been there nearly ever since. ‘and by his wise rule and administrative power peace and a measure of prosperity have been restored amongst the Gara tribe. The Arabs them- selves never penetrate into the interior, but are content to cultivate the fertile plain of Dhofar, and inhabit the prosperous villages by the coast. The Bedouins of the Gara tribe, who are perhaps the wildest and most uncivilised of any of the tribes of the South of Arabia, form a most inter- esting study for the anthropologist. They are clearly an aboriginal race, as distinct from the Arab as the Spaniard is from the American Indian. They are small of stature and of limb, but exceedingly lithe and well made. They go about naked, save for a loin cloth, and wear their long tangled locks bound together by a leather thong. There are hardly any firearms amongst them, but every man carries with him three indispensable weapons—his shield made of wood or sharkskin, with a knob at one end, which he turns round when tired, and uses as a stool ; his flat iron sword with a wooden handle; and his throw stick, a wooden weapon pointed 494: REPORT—1895. at both ends, which he uses with great skill both in war and in the chase. The Gara live chiefly, as stated above, in the deep caves of their limestone mountains, which provide accommodation for the family and many head of cattle. They have a large number of milch cows and goats, and make ghee in great quantities, which is exported from here. All their implements are of the most primitive description. The churn is a skin hung on three sticks which a woman shakes about until butter is formed ; to make their cows give milk freely they stretch a calf’s skin on two sticks, and give this to the cow to lick. The calves and kids are kept in the innermost recesses of the caves during the absence of the dams at the pasturage. ° Camel breeding is also a great industry among the Gara Bedouins, and the animals are remarkably fine and healthy ; they have but little use for these camels, but they take them to great fairs and recognised rendez- vous of the Bedouins of the interior, and sell them. The camels are curious feeders, bone being greatly appreciated by them, also small dried fish and sections of a cactus which grows in the mountains. Some of the richer Bedouins own as many as seventy camels and 500 head of cattle ; they ‘are, however, devoid of luxury, seldom constructing any habitation for themselves, and never using tents. In the wet season, when they come down to the plain of Dhofar for the pasturage, they erect as shelter for themselves round beehive huts of grass and reeds, but in the mountains they never require more than their ancestral caves, which are cool in the heat and dry in the rain, and the floors of which are springy and soft with the deposits of many generations of cattle. The Bedouins of the Gara mountains have many interesting customs : their greetings are very complicated and curious to watch. For an acquaint- ance they merely rub the palms of the hands when they meet, and then kiss the tips of their fingers ; for an intimate friend they join hands and kiss each other ; for a relative they join hands, then rub noses, and finally kiss on either cheek. The Gara are great believers in the existence of Jinnis, or spirits, in their mountains and streams. -As we passed by a great rock one day they all set to work to sing the words ‘ Alaik Soubera,’ which we were told was a request to the Jin to let us pass in safety. Again, at a lake we visited in the mountains they affirmed their belief in the existence of Jinnis, stating that it is dangerous to wet your feet in the lake, or you will catch a fever. The Jinnis inhabit the caves, the trees, and the streams; and at an annual festival and gathering of the various families into which the Gara tribe is divided, the great ceremony is the propitiating of the Jinni of the lake by a magician who sits on a rock, and performs his incantations whilst the people dance around. They believe that the Jinnis when propitiated are very helpful to mankind ; and inasmuch as they inhabit the lower heaven, they can overhear the conversation of the angels, and if disposed communicate their valuable secrets to man. This would seem to be aimost the only trace of religious observance amongst the Gara Bedouin ; they may have others which we were unable to ascertain, but one thing is certain, that though they may conform to the dictates of Islamism when visiting the Arab villages cn the coast, when up in the mountains they observe neither prayer nor ablu- tion, nor any of the ceremonies inculcated by that creed. The Arabs attribute to the Bedouins certain pagan rites, and they are probably cor- ON THE EXPLORATION OF SOUTHERN ARABIA. 495 rect ; as in many other parts of the Mohammedan world it would seem that certain ancient cults and ceremonies have been retained, which the Moslem has been unable to eradicate. The Gara tribe is divided into families, the chief of which is the Al Kahtan family, and the head of the Al Kahtan family is recognised as the Sheikh by all the Garas. These families have constant blood feuds amongst each other, which they make up when war is on with their neigh- bours, the Mahri tribe, or the Geneveh tribe. Wali Suleiman during late years has done much to heal these feuds, and it was through his instru- mentality that we were enabled to penetrate into the Gara mountains, with an escort of the heads of the chief families, with comparative safety. (3) The archeological interest in the plain of Dhofar centres chiefly in its connection with the frankincense trade and the towns established in ancient times along the coast by the merchants who provided the ancient world with the odoriferous drugs. We have several classical authorities who refer to this district, notably Claudius Ptolemy, the author of the ‘ Periplus of the Red Sea,’ Pliny, and a few others. From them we can gather certain definite points, that beyond Ras Fartak and the Sachalites Sinus there stretched a fertile coast line known as the Libaniferous coast. The capital of this district was accord- ing to Ptolemy called the oracle of Artemis (Marretor *Apréuucoc), and the city next in importance was called Abyssapolis, near which was the harbour, the portus nobilis, or Moscha of the Periplus, where the merchants on their way to and from India used to tarry during the violence of the monsoons. Along the whole line of the plain of Dhofar there are no less than seven spots where ruins occur, all indicating towns of considerable size ; but on close examination of all of them there can be no manner of doubt that at Al Balad and Robat—which are about two miles from one another and connected by a series of ruins—the capital stood. These places are close to the coast, and nearly in the centre of the line of plain, and consist of the remains of many temples, tombs, and public buildings. The acropolis is well marked with the débris of buildings ; there is also a tiny little harbour, evidently only for small craft, across which a chain was discovered, the _ Arabs say, a few years ago. Then there is a moat round the outer edge of this town, in which water is still found, and bulrushes. The columns still standing form an interesting link, which connects these ruins archi- _ tecturally with the other ruined sites of the Sabzean world ; they are square and fluted at each corner, and with step-like capitals. A further development of this is evidently of later origin, when they decorated the capitals with floral and geometric devices. The columns at Axsum in Abyssinia, at Koloé and Adulis on the coast of the Red Sea, and at Mariaba in Yemen, are all of the same character, and indubitably establish the Sabzean origin of the ruins. One column at Robat we found with a capital decorated on four sides, three sides with intricate geometric patterns, and the fourth with the Sabzan letters ein and 7' alternately. No other ruins either in size E architecture on the plains of Dhofar can compare with these, and we t can safely say that they formed the capital of the district, which Claudius Ptolemy calls the oracle of Artemis (Marreioy *Aoréudoc), and which in _ later times was known as Mansura, where dwelt, Yakout tells us, the _ Prince of Dhofar, who had a monopoly over the frankincense trade, and _ punished the infringement of it with death. In later times the Persians _ occupied this spot, in the fourteenth and fifteenth centuries of our era. To _ them we owe the fact of the disturbance of the old Saban columns, and 4.96 REPORT—1895. the utilising of them to erect mosques, many of which are now standing in a fair state of preservation. We tried to find the site of the oracle of which Ptolemy speaks, but could not come to a satisfactory spot until we visited the mountains, and in the Wadi Nehaz, about 9 miles from the capital, just at the foot of the mountains, we found a curious natural hole, about 150 feet deep and 50 feet in diameter. Around this there was a wall of Saban origin which had a massive gatepost, and in the immediate vicinity were traces of many ruins. For several reasons I am inclined to believe that this is the site of the oracle mentioned by Ptolemy. In the first place, the hole resembles in character the site chosen for an oracle in the ancient world, bearing a remarkable resemblance to the holes which existed in Cilicia, the oracles of the Corycian and Olbian Zeus, and several other spots in Greece. Secondly, Yakout tells us that the abode of the Adites was half a day’s journey from Mansura, the term Adites generally being given to the adherents of the ancient cult ; and, thirdly, because there is no other spot on the plain of Dhofar where one can say there is a probability of an oracle existing. Yakout further tells us that 20 parasangs from Mansura was the ex- cellent harbour, frequented by the crafts onthe way to and from India, and by merchants in search of frankincense. The author of the Periplus refers to this harbour, and calls it Moscha, and Ibn Khaldun also speaks of it as Merbat. As we journeyed along the coast we were constantly on the look out for this harbour, and on the second day, after leaving the ruins of the capital, we reached the village of Takha, in the vicinity of which are traces of many ruins scattered about, but inferior in architecture to those at Al Balad. Next morning we were conducted by the natives round a headland, and there saw a long sheet of water stretching inland, but silted up at the mouth by a sand belt, over which the sea flows at high tide. This same sand belt now separates from the shore a rocky island with traces of fortifications on it. There can be no doubt but that this is the harbour, and the island rock guarded the double entrance to it before the invasion of the sand. The harbour is deep, and extends inland about a mile and a half, and there are many ruins around it. Here we have the portus nobilis of the Periplus, the harbour to which the frankincense merchants came, and it is, as Yakout tells us, just 20 parasangs from the capital. The term Moscha, given to it in the Periplus, is a common term given to bays and inlets on the Arabian coast. Merbat, the name given it by Arabian writers, is still retained in the headland 12 miles east, where Arab dhows find a shelter during the north-east monsoons, but it affords no other harbourage, and Ptolemy’s name for this place is Abyssapolis, a name which I consider to be derived from the great abyss which I have already described as existing a few miles inland, and which must have been a conspicuous and well-known object to all merchants who frequented this port. Ptolemy, as it will be seen from the name given to the capital, gave Greek names, or equivalents, to the places on this coast, and in naming this place he evidently used the most con- spicuous object in its vicinity. Thus we were able to reconstruct on fairly probable lines the geographical features of this frankincense district, and fix the position of the sites of its towns. INSTRUMENTS USED IN ENGINEERING LABORATORIES, 4.97 Calibration of Instruments used in Engineering Laboratories.—Report of a Committee, consisting of Professor A. B. W. Kennepy, F.R.S. (Chairman), Professor J. A. Ewine, F.R.S., Professor D. 8S. Carrer, Professor T. H. BEaRE, and Professor W. C. UNWIN, ERS. (Secretary). (Drawn up by the Secretary.) At the first meeting of the Committee it was decided to investigate initially the accuracy of instruments for measuring the tension coefficient of elasticity, or Young’s Modulus. A general letter was addressed to various professors and others in charge of engineering laboratories inviting co-operation. Most of those written to agreed to make a series of measure- ments for discussion by the Committee. It was then decided'that sets of standard test bars should be prepared, to be subjected to tension and measurement. Figs. 1, 2 show the forms of test bar decided upon. Two of the standard bars of each set are cylin- drical bars, with screwed ends of about 1}-inch and }-inch diameter. _ These have gauge points for measuring instruments, suitable for extenso- meters of 8-inch, 10-inch, 16-inch, or 20-inch range. These bars are of a special steel of high tenacity, rolled specially for the Committee by the Blaenavon Company. The whole of the bars were cut from a single rolled bar about 20 feet in length, and were very accurately turned to the required dimensions by Mr. W. R. Munro. The third bar of each set was a flat bar, of section about 2 inches by 4 inch, of mild steel. All these bars were cut from a single plate, and they were prepared with gauge points at 8 inches and 10 inches. In order to obtain some preliminary information as to the mechanical properties of the standard bars, one round bar and one flat bar were tested in the testing machine at the Central Technical College. The. following table gives the results obtained :— Preliminary Tests of Materials used for Standard Bars. TENSION EXPERIMENTS. : ' Maximu m Breaking Yield Point Tad Tena Ps Mark Elonga-| Con- E. er Dimensions. | Area. tion on |traction| Tons Inches Sq. in. Tons Tons Tons 8in. |of Area per Bar Load. ; mane per | Tons} per |Tons} per |percent.|/percent.| sq. in. sq. in. sq. in. sq. in. D_ | 2:000x0°507| 1:014 |16°19 | 15°97 | 23-725) 23-40 | 19°75] 19°48 32 | 62 13,113 N 0°750 diam. | 0°4418 | 9°00 | 20°37 |15°725) 35°59 | 13:76| 3114 24:5 | 42 Bar D was exactly similar to the flat bars A, B, C. Bar N was of the same steel as standard bars marked E, F, K, L, &c. __ The Committee then drew up a test-sheet form to be issued with the bars, on which measurements were to be recorded. These sheets were so- arranged that two sets of measurements for each bar, and the mean of these, should be recorded ; also that the extensions for short and long ranges of stress should be recorded. It was hoped that in this way some measure of instrumental errors would be obtained. In January two sets of bars were sent out for measurement, to be ae eted amongst those who had consented to co-operate with the 1 5. K K REPORT—1895, Marked End 498 Kasees SS eke Sak 5 ee ca ae na a li Whuworth Uicad Fig. 2. INSTRUMENTS USED IN ENGINEERING LABORATORIES. 4.99 Committee. The measurements have taken much time, and the whole of the reports of observers have not yet been received. Some of those already sent reached the Committee too late for discussion this year. It appears, therefore, to the Committee that it is unavoidable that only an interim report can be presented this year. The Committee ask for re- appointment, in order that the results obtained may be discussed and presented. It may, however, be useful even at this stage, to give a very short summary of some of the results sent in. The following table gives a Measurements of Dimensions of Test Bars. summary of the measurements of the standard bars by different observers. It will he seen that there is an appreciable difference even in the measure- ment of the dimensions of the same bar. was machined on the edges only. The flat bar, it may be noted, was Dimensions. Area. Bar Observer Inches Sq. in. ( W. C. Unwin 1:999 x 0°509 1:0175 , |, A. B. W. Kennedy 1:998 x 0:509 1:0170 ow * | op. Hudson Beare 2-000 x 0:5095 10190 (| J. Goodman 1:999 x 0°509 1:0170 (| W. C. Unwin 1:9995 x 0:508 1:0157 Flat BarB . . ,| H.S. Hele Shaw 2-000 x 0°509 1:0180 { J. A. Ewing 2-000 x 0°506 1:0120 W. C. Unwin 1:248 diameter 1:2230 A. B. W. Kennedy 1-248 - 1-2230 ged Hor¥ - +| t Hudson Beare 12495 1-2262 J. Goodman 1:248 oy 1:2230 W. C. Unwin 1:249 diameter 1:2252 Round Bar E : H. S. Hele Shaw 1:247 rt 1-22125 J. A. Ewing 2 1:249 = 1:2250 ( W.C. Unwin. 0:7495 diameter 0:4412 A. B. W. Kennedy 0:748 a 0:-4394 Round Bar L * 1) T. Hudson Beare 0°750 0:4418 | J. Goodman = 0:748 2) se | gases —— a a ACMr A = Bas 4 2 SSv] : : — = 1 B alee = ao : ? = om fa ow stone > eS a a a eae : = = omer} : : 2 2S SSBID TeI90g Tadd H | eee i = Sx worpyD, ystsa , 318s . aru S.8 spooyo: Tsu Hi io) On wea = —— | :) = = An 1 aS ea] AQ 8 no, | & | g aaa es nr a aes : = : = 2 : : : ae [WROASRIAE callie ine Be site 2] _ B SS SStID TeIo0g raddq z ee om *o s[ooyo a “a Sa B —— Ss: pie Ss Hi G er ue es af tebe r x See ea eal =! Vesa to Vache ae ch) a S'S g [J se aubaliks sie eo “S 5 SrA EN a : ; | [= lheeoeeses - : = ss he Teoog asRI0A Vy 3 — : ' S IPD Ys e as = = 1 & a nig esa es 6 cas Ae Soret rset = Hr ero > ; f og Arquno ie ‘ . * owrysoy SI 6-LFL —) a = T = G € G i I = T I * ; ~ * ULES Or 9-FS1 T = T € = G G T = = ars ra, = a 4 . YOWVO FEN sasuy aSeroay | S91 | I9T | GST | LET | SGT | SOT | TST | GOT | LPT | QPL | EFT | THT | 6eT } Sa Ee JO toqunyy GOT | O9T | 8ST | 9ST | FST | SSL | OST | SFI | OFT PPL GFL OFT 8EI ‘(0A0 pure sivek 0%) NA JO MOV JO HLavaug 9€ LEgt G € ¥ g g g i) g T u ‘ * [ezoy, 06 SPST I z F € F Z S z = > e Z * OWITYSOS, 6 SoS T = a T I a § G T ¢ ; . * ULB yy L FET = T = IT Se € TI T = ‘ % : YO WVOTeN sosep 3 6E9T 619T 66ST 61ST 6991 6E¢T 61ST 66FT 6LFT } 5 5 5 A ne yoroquny | °P°V | —oggr | —oo9t | —osgt | —og9et | —oret | —ozert | —oogt | —osét | —09FT tai ‘(ese Jo sivak GG-)1) NHWOM JO TUALLY OF G F G F L 9 € 8 6 : * [®IOL 61 ar 6 T T € F G g “Ez ; ¥ : * ovllysoy €T —— T T G € T ae G G 7 ; e * urea y 8 G T od T T ! I I a r YOPVO, YVN sasep oSe10ay 6SLT 6ELT 6ILT 669T 6L9T 699T 6E9T 619T 6691 6LST Me 5 ; . WH JO TequInN —OPLT | —O3LT| — O0LT| —O89T | —O99T | — OF9T | —OZ9T | —O09T | —O8ST| —O9gT ‘(988 Jo steak 69-02) NA 10 TAALVIG “BRMyony ee REPORT—1895. 526 LE 8-161 She te ae 9 6 T f v P v € | T Co is—elheaEse ey ‘ * [Tej0y, Spe mc Pe per me er ae es Pam i tl Pe RU AES 03 L631 Bert. do) hale er clnket | Th eit) Select Thee See Ee ke * OUITYSOY 6 @-611 See eee ea a | lr Vee TD ate) Sat) | ae = ae ene * TFNIYRA 8 8-861 a eres | ee =| — A) ee VES SS alk 2 PN Ma | a Chg me oe ; : ; AOWVO YEN sasep aSeroay | 681 / LET| SET | SST} TeT| 6ST} L481 | 9ST | S2z | TL | GIT LTT gtr ett TIT | GOT} LOT a o cagley ay Rempasete, JO Toquun yy SEL | 981 | FEL] SST | O€L| 8ST | 931 | FST | SSL | OST | SIT 9TL FIL) SIL} OIL! 80L| 90T ‘(ase Jo sivok G¢-11) NUWOM HO TOV ao LHYIG FP L631 tH a € F P 9 g 8 F I G T G i 3 “ [eT FI i em S| | 06 F-86L <— — T I G t F F G ce a il - 1 ; * OWITYSOYy al P-8E1 T = if T G G I G 1h = I oa G 3 : : * NEVA 6 L-TE1 G = i! G > = = G I i! a = aa ; ; : YOWVO YBN | 4 : : sasup oSeroay | TPT | 6&1 | LEI | Get | eer | Tet | eat | zzz | get | est | tet | ett | 2TT if say tate fant FO toq uu Ny OFT 8éI 9&T PEL GET | OSL | 8ZI | 9ST | PSL | ZZE | OSL | SIT | OTT | ‘(e8e Jo srvak g9-0Z) NAT fo TOV AO LHYIa Iv L&?1 GG 8-ITFL OL F-8F1 6 L-9FT saseg jo zaquanyy asvIloAV | = T I SST 6ST IST OST T 6 6FT 8FT N20 LET 9FT age Reel | aa Ae pe aS a Th fll Sol de ee es lS cet ae) fn Ey, ll | he SFI | ShL | TFT | 6eI | Ler | ger | eet | PFI | OPI | OFT | SI | 9er | FET | ser ‘(toa0 puv steed JT) NAWOM JO GOVY ao HLavaug . . . TeqOT, * OUITYSOY ULBALy YOHBO YUN f *““Uay 527 ON THE NORTH-WESTERN TRIBES OF CANADA. 9€ 1/—|—|—/—|-]z|-|z2/e/e|—|slele|t)e|rlrlsirlele|r] - r 06 L-€¢ } Ome Vitae sea fm FU) Ht] oY OS acd st Vee aA at Od OBI 1 eet ome —aa ‘ 6 8-86 Se (od a 2 naar awed eet mame sel feed eel ME GI cate L LTg sau acme Pesala esa sm a ag A A Hee a et jes A = jo Feanie asvieay | 99/99/#9| 89) 29 T9 | 09) 69 | 89 | 12) 99] 99) $9 | 9} GG | TS | 09 | 6F gFLF 96 SF/FF eF ie of ‘(ase Jo sivak 69-1) NAWOM, JO ASON JO LHYIDH S&P L-Gg oN ieee a am 6 | 6 9 |; OL | § Y & 6 te) 6 Fe “= G 02 1.99 —|—|—jaisbere trate t thelr} —}]— it FI 8-F¢ Ss | SS ae te GAG G I I I 6 I TE a T : 6 0.18 Pie Sr She) Sf slo sel | Es Ce ae ete ee eee sosvy aay eae SES ls 1 Heras lk ck | tO Sem ewer [pene | eee [cna A yo xaquain asviaay | €9 | 29 | 19 | 09 | 6G | 8G | 29 | 99 | G9 | Fa | EG | oe} Tg | O89 6h 8F } ‘(ese Jo sivok 6G-0Z) NU] JO ASON AO LHDIGH 9€ 6-GE t € g G IL G S 6 1) il { 06 F-G§ & I € i 9 6 G I I = : i 6 6-6€ Ex T 7 I € am I I I I + L 0-G¢ I ji G ay A = = a: I = 3 sasey 2 : : Jo raquiny, joe mee eey 6& | 8€ | LE | 98 a€ ve && of Tg 0€ } ‘(a8ev jo sreok 69-11) NUWOA, JO ASON JO HiLavaug GT €-66 T = T g g IT 9 8 8 € va F P 3 06 G68 il = = = g = i g g IT I oo | oA J ial L-8¢ x a = § es = T I G i T t 3 8 9-0F = = et = a it T dj T a ee . es aa | ea eee RT | eee ee eseroay |. 9F | 9F | 3% | eh | oy | Ty | OF | Ge | 88 | 2e | 98°] 98 ie : * [eVOI, * owlysoy * Upeay * -YOVTeOTEN * UL * 1230 * OWLYSOY * UTE 7O}1L07eN : cent * [R40], * OWILYSOy * UTE * —-yoq7B0,72N 4 UY TROL * OUNTYSOS] * * yMETeALy * -¥Q}180,xUN “UY 528 REPORT— 1895. It appears that the three groups are quite uniform. Possibly the breadth of face of the most northern group, the Nak’oartdk, is a little larger than that of the others, but the number of cases is so small that it remains doubtful if there is any real difference between the types. It will be seen that the three tribes differ very considerably from the Nass River Indians, their faces being much higher and narrower. In order to prove properly the uniformity of the material collected among the Kwakiutl, it is necessary to take into consideration their habit of deforming the head by means of a pressure brought to bear upon the front and sides of the head. Possibly the practice might have an effect upon the development of the face, which differs much from the form found among all the neighbouring tribes. In order to decide if the artificial deformation has any influence upon the form of the face, I have divided the material into three groups :—Heads not deformed or slightly deformed only, moderately deformed heads, and strongly deformed heads. As will be seen from the tables showing the measurements of individuals, I made finer distinctions when recording the original observations, namely :—Not deformed, slightly deformed, moderately deformed, considerably deformed, strongly deformed, and very strongly deformed. The first two classes embrace children and young persons only, the practice of deformation ’ being gradually abandoned. Leaving these out of consideration, we find the following numbers of individuals in each class :— = Meno Women Men Women Moderately deformed F 25 9 59 % 32 % Considerably deformed . 8 7 191% 25 % Strongly deformed . : 9 9 22 % 82% Very strongly deformed . —_— 3 ae 11% This table shows that the heads of female children were much more strongly deformed than those of male children, and that the deformation represented in each group is stronger among women than among men. 5 Slightly Moderately Much Deformed Deformed Deformed Length of Head {Women! 1) 1863 tera | 1912 Bas ot ia (Me | aT | ae Bice ees VME | MR | ~ BRR |g Height of Face { Women’ || 1186 11947 1236 The differences exhibited in this table show clearly that a strong deformation of the kind practised by the Kwakiutl increases the length of head and diminishes the breadth of head ; but that moderate degrees of deformation do not influence materially the lower portion of the skull, in which the greatest breadth of the head is found. The table does not reveal any influence upon the dimensions of the face, so that, so far as the latter is concerned, we may consider all the measured individuals together, without regard to the degree of deformation of the head. While the preceding discussion has shown that the tribes of the [North-Western Tribes of Canada. 1 ® Son of No 41. Right ieg broken. 34 35 36 37 38 39 40 41 42 a | o ao o | 2 ‘s i 2 a | 4 ry See fee |e | Be | 8 BR g S ma = < s 2 BS & oS a BS - q = to} 5 E 3 g g B = # a a ee CS) ret o 2 Ca hay Ei ls =| 5 = a 42) bm & P| Ss ~ a SG |e |] 3 | = Oo; s | air k= a ! | Senor ee 3 | | | eS a ‘=| | 3 8 re r s | 8 = s ema frm) ee be |) ee | 7) | Oo aH FI | ; | 40 45 55 58 60 62 65 67 | 65-70 (1,677 | 1,625 | 1,644 | 1,645 1,627 1,623 1,633,573") —™ | | | i 1,373 | 1,328 | 1,333 | 1,332 | 1,871 | 1,342 |1,331 |1,282 |} — | wre FAG | 7T56°| F281) 779 | TERT TIS |! - 720 | | 1,798 | 1,730 | 1,761 | 1,740 | 1,810 | 1,735 | 1,685 | 1,647 | — | | 911 | 904] 890! 915 | 840: 865] 900] 846] 795 | 385 | 378 | 402/| 373| 400] 418] 400] 388| 357 195 | 205 | 204! 206] 1941 197] 199| 191| 194 | '159°5 | 158| 164} 162] 158] 163] 160] 161] 169 119 | 119 | 124] 123] 128] 125 | 120| 124] 113 158 |1525 | 159} 149| 161| 167] 155 | 156] 158 57 50 53 52 51 52 54 49 53. 41 39 46 42 47 49 43 41 41 81:8 | 77-1 | 80-4 | 786] 81:4 | 82:7 | 80-4] 843] 87-1 75°3 | 780 | 78:0 | 826} 795 | 749 | 77-4] 795 | 71:5 719 | 78:0 | 868 | 80:8 | 92:2 | 942 | 79:6 | 837] 77-4 461 | 45:7 | 46:1 | 44:1 | 47-8 | 47:0] 44-0 ie Be 1070 | 106-1 | 107-4 |105°5 | 111-1 |107°1 | 103-4 |1049 | — 542 | 55:5 | 64:3) 555 | 51:5 | 58-4 | 55-2 53-9 | a 22:9 | 23:2 | 24-5 | 226 | 245 | 258 | 24-5 | 247] — 65th Report, Brit. Assoc., 1895 p Brit. Assoc., 18: i] . [Worth- Western Tribes of Canada 1 1. Taietsalut, y Niska’ — Males = Y I. Males Number 2) 5 2 AAI ; : 7 = ae = 1 2 3 1 2 4 7 7 5 q 10 1 12 ww) 16 / 16 | 17 |) 18) )) 19 20 a1 | 23) | 23 | 2 Th we) 20 10 a1 a2 a 15 A7 48 39 | 40 | 41 42 | 7A 7 ey il | | | £ EI E g 3 A = z = | 4 Bali ) 2 \3 3g z z E 5 | Same Se luce lle is || il lik A 5 & | = 5 | | | z = 5: 4 . | 2 e | a 3 5 r) Fe = 3 S st | x | = | A 3 a Delle g E 8 FI | 3 DD} | 4 = E | | 2 2 | 4 | 2| 4 2 : 3 | 3 2 g | Sa Sales | 5 | z/8 eh a = 2 |e = | 5 =| | | s * a | : Bs Z El nals ey ile les , || > = e - z . = Tribe $ Z| & = Zz steed | [ie je Pe Sin | esl es ee sinesial (earind wari, | eee : ef og |S eres 2 =i |) I 2 3 2/2)5 2/2/23) g 2 s/2\3 3 e] s/s A 2|% % z |% | 2 la Fae | (Wee |) ¢ A Pa |ies || Pe z pe |e || z a i} | £ = ie i | | t of} i a Age % } 4 | an } 55) |} YO) } to} ay) 1s) me | as ea 1 | 16 | 16 | 17 | 17 | 20'| 20 | 20) | 97 | 2 28 80 2 | 38 5 | 85 38 | 40 sg | G0 | n2 | 6s | 67 | 65.70 | cua Sob) 1 be aie 3 mm. | mm, | mm. | mm, | mm. | mm, | me. | mm, | me mom, | mm. | me, | mm. | mom | om, | mm. | mm. | mm. | mm. | mm. | om | mm. | me. | mm. | mm, | mm, | mm. | mm. | mm, | mm, | mm. | mm. | mm. | mm. | mm. | mm. |/mm, (eight, standing 1,097 1; 20 |1)421 | 1.4884 1,578" 1,545 11,630 | 1,689" 1,634 | 1,608 | 1,643 | 1,605 1,620 }1,617 | 1,671 | 1) (00 | 1,680 1,712 | 1,632" 1 98 | 1,668 7 1,624 (1,039!) Height of shonlde 1,107 | 1,021 | 1,010 | 1,141 1,905 1,346 1,805 1,810 | 1,932 | 1,298 |1,878 | 1484 - 1,936 | 1,440 | 1,340 | 1,881 5 1,842 | 1,381 Length of aru 678 | soi] 684) cHy) 690 700 76 694 780 | 810 — | 784) 761) 784] 70} 742] b08| 7 Finger-reach + | 1691 1,834 1,500 1,468 1,047 1,694 1,680 | 1,691 593, }1,850 — | 1,841 | 1,880 | 1,827 | 1,803 | 1741 1,860 | 1,708 Height, sitting 808 401 | as 32 900 | 914 | 800 | 908 | 928 [1,615 | 880 | 954 931) 881] 878 | s9| #85 911 Width of shoulder 851) — 261 4) | s90| 384 395 | 402 | 678 | | 425) 985 | 85) 309] 408 3 Length of head wo} 191 | 183 | | 178 188) 186 | isp | 192 1a) 189 201 | 194 1926) 189 195 cos | lp 6 5 | | Breadth of be: 168 | 153 M4 1625 | 109 168 |1615 | 160] 155 160) 157| 164 1595 164 Height of face 110) 328 | 12 100) 110} 112 | 12, | ne} 194 133) 124] 126) 110 119 124 Breadth of face 6 46 161 1M 138 143 } 148 19 160, | 143 1675 | 167 | 160) 163 138 5 | 169 Helght ¢ 47) | 06 so] 36] 43] 40 oo} co) 6o| c4| 48) 48] 47 | 58) 49) 49) 49) or) 50] 68 Bresilth of nose a} on} 40 a5} | 38| 40) ao] a7] 41] 40] 43) 98] 35 43} 39] 37} a9] | 39| 40] | Length-breadth index 832) 601 | 88 | sd | 804) 879 801 | 609 | 812) soo 46 | 880 | 805 | H4| S10) ase) 580 784) 809 | 85 885 | 7-1 | sou) 70) 814 Facial index P 70a)| 677 | 808) 707) 768 | rhe 747] 797 | 768 86 | 591 147) 867 sea] 790) 788 768 | 661 | 763] 780) 780) B26) 706 Nasal index | 872 820) 768) 864] B24) sy4 | 805 | 884 780 | 740) 820! 744 | 896) 72) 745 Bll) 796 | 756 510 | za1| 769) 719 | 780| 868] S08) 922 Index of arm | 424 — | 407) 490] asa | 436 416) 448) 186 | 44) 480) 456) doa aya) 448) daa] 407) a7a) 447 | 452) 455 {58 | 461 467 470 | 401) 457) 401 | 442) 178 400 | 459 | Index of finger-reach 204 1059 | 1086 }1026 000 985 | 1084 }1040 1065 1011 | 1058 | 1015 | 1099 | 105-7 | 1057 1048 | 1044 | 107-1 |1087 | 107-0 | 1050 1054 | O84 | — |1077 1057 1058 |1075 | 105-0 1069 }1081 1070 | 1061 | 1074 Aide }1071 1034 | 1049 | — Indox of height, sitting s2'| — | 508 308 | 656 | 664 bd1| 639 | 580 Si | 689) 6h1| 552) O47 | oH 660) 51d 40) 588) 632 5L6 598) o5%) 088) ois | 526 | G45! srg G42! B55) O48) 655 584] 552) sv) — Tndex of width of should 219) — | 224 211] 921 | 210. 2y0 | 22a zea) 241] 299] 284) 294] 293° 204 | 248! 2n1| 225] 292! 218] x24! on4| 292! 201] 225] 2x5) 299| 200] a4 aga | 2465 258 | 5) 47) — * Son of No. “Brother ofNo.G. ' Son of Nos 40and 74. lind In consequence of an explosion of gunpowder. Hight leg broken. T Sou of Noa. 42nd 70. Biother of No. 49. 7 Son of No, of. Brother of Nos. 9,44, 65. * Brother of No. 18. _* Son of No, 67. Trother of Nos. 4, 44, 65: 3 " FatherofNo 10. '* Father of No. 18. Occlput rither Ral, Large exostosis on vortex. "Father of No. 1: Father of Nos, 3 aud 49, Much bent by age. | North-Western Tribes of Canada 2 nued). 24, Nisk-a' Half-bloods. | I. Males. II. Females. 58 75 (i ee 78 79 a ie | ie 3 2 | = | = < 2 ay | 2 a o 5 < z q = oe a 8 3 4 « 5 = {ets o | S 2 pi & S 2 & ‘ RD ra) re x S q eS 5 E ee ea [o} | a i=] ~ | g = a E> rs = | $8 a ca =| 2 A @)2 | ¢# @ = = Ay ss ie iz A Z £ 4 dia is! . ea s BA si a ee a Li a : =a Bit Si> = 3 aie: “ fi E 3 a @ 8 p & Bate |), a 3 Za | 3% 4 iz a dia S wm dia = S yi mM ipa | ale : = é; a] gs ; Be | & i a | i & | 20 3 5 | 16 29 6 25 32 mm. Es mm mm. mm. mm. mm. mm. 1,571 | Lisss — | 1,579 | 1,652 || 1,146%} 1,632 | 1,603 meee | 1) ey ele sOte S52) || sss. | 1.360 1-312 679 2 | ae 726 754 465 732 723 | | 1,605 | ligg9g | — 1,630 | 1,712 1,118 | 1,686 | 1,653 862 ls |} — | 834 872 | 635 822 874 318 201 oe, || eae 374 || 248 326 328 193°5 168 176 179 18s || 175 176 181 150 141 140 | 181°5 150 145 160 155 115 90 = 111 130 95 117 110 142°5 112 117 1405] 144 119 139 146 47 34 39 | 49 55 37 52 48 | 38 26 28 38 35 32 31 33 a | | 775 83:9 79:6 84-7 798 || 82:9 909 85°6 80:9 B0-4 = 78:9 90:3 798 84:2 754 80:9 76°5 71:8 176 63°6 86°5 59°6 68:8 43-2 = = 45:9 45:7 40-4 44-9 45:2 1022 | 1601-1 — 103°2 | 103:8 97-2 | 103-4 | 1033 54:9 56°8 = 52°8 52°8 55-3 50-4 546 20°3 22:6 wee 20°6 227 || O11 20:0 20°5 - 51. kk. 23 Daughter of No. 67. Sister of Nos. 4, 9, and 44. Nos. 4, 9, 44 No, 62. Sister of No. 76, Nisk-a' (contin Niska! Half-blood = If, Female. 1. sal II, Female ‘ u 45 6 rr i | 49 0 \ 2 iy )iiss te | oo | oo | ol ( Gin mec 66 o | 6 | 7 1 73 | 7 i e z 2 2 3 S | > z Zz z Zz zZ z Z z Zz z zZ |< z : | | |: ale 419 | 456 | — 3 A o17 | 1,003 | 1,050 1,65 se oe n = 2 a | a7 ‘ 20 26 us| 526 | 9a ri = - = | 168 | 170 | 177 wo | 116 iss | 184 1995 | 180 8 | ise5 | 1ag | 180 ; eae PETE Sci) TE | he Mi 137 148 15 151 ig 160 | 1685 167 156 166 | 1476 rw M0 | 18 150 1s } if 85 49 | 97 101 115 n 108 100 117 Ml r il 180 05 a 124 118 125, 194 10 “a5 148s 149 142 141 12) 171 M05) 14 no t 2 36 40 | a0 4 — 47 4 15 7 18 48 40 45 44 a4 a0 a 5 37 28 a 29 a a 4 = ag 33 38 45 3 38 7 35 19 1 49 26 28 38 42 41 33 ith index o7 | 806 Ao 858 gro} 601 | 793 | 704 | e539 | 776 | #57 | 872 | BoM | Siz sco | sso | 793 “9 $17 829 | Focial ind ea | 748 74 siz | — | 766 786 | aro | gon | 782 | zoe | 338 | 762 | 785 604 739 | 903 | | | e 3 | BLL 10.5 173 - | 881 703 | 809 8 875 | 848 | | si || tes | m3 | 776 | 36 | eos | oo | ose ola aan (vans ri is = is7 | 492 | 44 tio | as7 | asi [aso [seo | en | vee | ten [er 199 = | | Tedex o i 901 a! & 1008 114 | = | = | act 1083 | 1022 | 100 1057 | 1062 | 1006 | 1080 | 1048 | osx | ova jose Wan) || = Index of height, alttin ; re siz | 5 5 3 | sto | « res | Ines of} ri) 00 | = ra Were ican) == ll | igen oso | 040 ‘ si7 | soo | oor | ot | cro | so | oso | = eb width’ of ationlden 20 i a1 | ot | 3 | 204 = = 1 290 | 209 1 a 9g] sia | 258 } 289 | a4 | | a | | " Daughter of No. 65, " Daughter of No. 07, Slator of Now ® Daughter of No, 03. Sister of No. 48. ™ Hunobback Sistor of No, Daughter of No. 08. Sister of No. 48. © Danghtor of Nos. 42 and 70. > Sisto 4 Tdlotic Mothor of halfbreeds and 79, 2M Mother of No, 43 © Mother of 9, AA, and 65. * Mother of Nos. 8 and 49 > Mother of No, 18 ™ Son of No. 62, Consumptive jer of Nos, 45 nnd 48, | he ~ { [North-Western Tribes of Canada. 3 4. Heéiltsuk. II. Females | Female da) 19 |-20o/| a1 | 22 | 23 | 2 | 1 | | i | | | 3 | . 3 aa o || g| 4 8) SE al ae 0 ee eB 3 = 3 & a 5 id See | a te; & | bee Le I | a | s ig ov re 2 pan ey = 4 coh) ei ] py = Sia ge ia adie | a 3 ma ee oe | a oe. Bg = a | . js | 4 \ = ee | | i. ee ites | = i -s |) 4 | 28 BH =| “6s % % = | 8 =e § a BY | 6 8 s & 1D 3 3 & | Mz | 3 cs oS) 3 ae | ne 28 30 50 50 60 | 60 65 58 | .| mm.) mm.) mm. mm.| mm. mm.) mm.) mm | 1,486 |1,565'51,597 |1,522'7/1,532 1,542'9)1,5302%) 1,522 1,197 °|1,273 /1,322 1,243 [1,236 /1,250 |1,272 || 1,255 626 | 650 | 676 | 694 | 680 | 658 | 668 675 1,525 1,615 |1,645 |1,650 {1,660 (1,635 |1,570 || 1,618 ‘} 853 | 841 | 842 | 840 | 863.| 810 | 835 826 345 | 342 | 370 | 367 | 358 | 338 | 342 335 1921) 1944] 190%; 1864] 200%/ 1811 1904 182'° 1601} 163¢| 1564) 1554| 159°) 171° 1524! 162'° 117 | 193 | 123 | 128 | 134 | 129 | 195 || 116 1415) 150 | 146 | 147-5) 148 | 156 148 | 150 a it te | be | ba.) 68) 59-| ot || se. | 35 | 35 | 37 | 38 | 371 37 | 36 || 38 83°3! | 84-04) 82-14 83:34| 79-53) 94°41 80°04} 891 | 83:0 | 82:0 | 84:3 | 87:1 | 90:5 | 82:7 | 84:5 Tae 74-5 |} 62:5 | 71:2 | 70-4 | 63:8 | 62-7 | 63:1 || 73-1 | | | 420 | 404 | 423 | 4b7 | 444 | 427 | 43-7 || 444 | 1024 1029 1028 1086 1085 106-2 102-0 106°5 . | ) | | B72 | 536 | 526 55:3 564 526 | 546 543 23-2 | 218 | 23-1 | 23:5 | 23-4 | 22-0 | 22-4 22:0 ch deformed. 7 Son of No. 12, brother of No. 2. § Son ather of Nos. 1 and 2; son of Nos. 15 and 23; brother of No. 19. 1 Sister of No. 8. '§ Grandmother of Nos. 1 and 2, mother 65th Report, Brit. Assoc., 1895.) 8, Goasila and NaKoartok. [North-Western Tribes of Canada, 3 Keot/iealas HMad'tlelas Nemo'guls Kyili’tm Kvo'muut Si'with Ta'miait Malu'to Kot/kulagyila Kyvnidkyas ‘Te'umidaen uth Gonaila he |. Goasila Nakoartok Nakoartok Nakoartok Nak’oartOke Nakourt0k ¥. Goasila cone Nak’oartok F. Nakoartik ‘M. Gonsila ‘Nak’oartok Nak’onrtok : F, Nak’oartdk M = Awi'ky'cobx F. Nak’oartok P. } Goasilo, 4 Nak’oartOke = ¥, Gonsila, 4 Nak’oartOk 5 M. Height of eboalder 127s) [1,922 650 1015 1,615. Ba Es Width of shoulders 676 B42 870 1,272 668 1,570 845 42 4. Héiltsuk. II, Females || Female 19))|) 20) } (23))} F225] a) a i El i | ] 4 aig gi 5 G)2)a\3 ail a rial enn octet | 4 Sig leis | 3] ; Se pial hs q | Beil | Wer jh ase |p i Et | | 3 ai 22 | x S204 x s 43 S| 2 a4 Sle ae sialce kee sts il ints Sie, 28)2)28 et] alles Aa) See tori az z sq) = |= | z cz Et ‘wal Et \ | \ 30 | +50 50 | 60 65 i} mm.) om. mm.) mm.) mom. mm.| mm, | mm. 1,666'81,697 1,542'91,630") 1,522" 1,256 675 1,018 826 4i*| 190" 103) 1068 128 | 123 160 | 146 Length-brealth index . Index of finger-reach * Bllghtly deformed. 62 0) MOT 44 427 190¢ 1524 125, | 18 soo) 691! B45 767 O31 | 781 437) 4 1006 43 sy ae atid » 44. +8’ Father of No. 11. [North-Western Tribes of Canada. 4 . Koskimo, Tlask’é no | 21 2M PB} 1 42 43 44 45 46 47 | 48 49 in] ; at 2 / f= Ss 8 nm n ag ° . : sia FS s a} i 74 ees | = 4 | ae 3 a &B 2 = q 9 a a or) ay 3B a Ss | 3 b a 5 wa q A & a | 2 3 & ao =| be a rs cs s | 3 EB >) 2 ES 3 S ey = q = | g Z ! jo A g q 3S =! | & Cy S| a 1 a S| 4 ; & ‘4 a S =I 13 ee | i) a Hy ) 1,680 | 1,600 1488™) 1,8 1K) 9) 40 1,29: 0 | 1,863 1 1 Lal1 {1,024 994 |1,992 [i201 | 1,980 1,010 [1,171 1 ‘ 4 7a1 | 702 | 709 ¢ 741 724 | 700 | 762) 746 | 705| 732 8 f 5 1,740 (1,722 {1,708 11,626 {1,680 | 1,011 |1,742 |1,025 |1,765 | 1,708 {1,745 11,690 1,777 |1,728 | 1,660 1,670 |1,265 [1,470 07 n0 88 12| on | 998) 34 8 19 | 998 | si0 5 | 883 | 694 | 8 261) 95% 412 5 | 368 ) 19 7 2) a7 | 4 i 5 ) a34 | 16] 37) — 39 | 322 | — al i i 202") 105" ‘| 1924 1608] 109% 2005 17h 1 4165) 198% 1989| 208%) 2017| 208% 200 1 188!| 1909] 1944 1) 188¢| 1912 160!) 1485) 1592) 1624) y50'| 101% aays) 16 140-| 1564| 1434) 1613 144! 1599) 154*| 160% 153 152!) 150%) 150°) 145*| 148 1) 1464! 1452 ( 1 1 ios | 1 181 lio 135 | 1 132) 121 | 186] 14 8 130 | 119 | 129 iat} 130 | 117 g)] 124 UB | 16 153 152 149 lisss | 100) 1 Iol | 15a | 158) 164 146 145 | 42 | 7 0} 140 | 185 B) 4 6 H a7 a) c5| 55 67 8| 56} 67| 61) 63 | co] 69|| »| as | at 3] 03) 63) 5a} 50 1 ) 10} 38) 98} 39| 26 | 38 y| 40) 42 ‘ 9} ar] 42] a8) 41) go) 31] sa) 36) 38 30 | 35| 35 b 1 (| aom 4404 4) 6395 78 1 2 ) 705") 7060 | goa) ' i 763" 766% B20" 7 in 7 age a4) |\ god 709 70 791 | 861 836 867 | 806] 38 | sv3| 823] sca] 5 x 6) 69 G67 | ott | 67 | 684 | ors | 5 »| ¥a6 793 | 683} 694) 7068] 620| 660 704} Gli | 795 | 160) 660] cis It M7) #1 495) 446) 442 0 a} 41a} 404 | 401 46 478 43 ia 4a4| 492) 429 | 431 | 497 | f floger-reach 4) 980 1083 [1071 | 986 | 998 1010/1009 | 985 }1108 | 1018 | 1107 |1050 10 1010 100-0 984 104-0 |102-5 | 1018 |1024 | of height, sittin 568 | 558 oo | 648) nha 6o7 | 560 1] cia} ovo | 548 | 510 | 535) 5 586 5 18} 666) 528) 554 | f width of wt ra 20 : — | ops 5 | 298 231 | 280] 18] 299} 298} 227) 238) — 5 | 218 a4 | 226] — | ava] s13| are foformed Slightly deformed Much deformed. * Very much deformed. # Measured by Dr. G. M. West ‘Ono leg deformed. Son of No. 2 ™ Father of No. 30. » Drother of No. 44 = Father of No. 11 » [North-Western Tribes of Canada. 5 7A. Kwakwutl Half-bloods. 8. Sishiatl. | I. Males II. Female || I. Boy II. Girls 14 | | 1 2 3 1 BONS 3 | % | F ral i a4 . = oS I} a a BY n 2 = 3 ye! = % = S < ‘2 | s B a | § = I & | 3 o i) rey | se & 8 | o | 7 = = ES = 3 ra} ae Sh a Ss =| oS | A ——1 ie 2 3 = =) Ss © | hie] aE) ° Eg Se | 3s 28 Cs = 3 ao | 32 | Be a = 2 | & ae q4 | oB ES 3 2 | 4 ah a5 Ras i m # A i= A * rian Panes a) a Fe = aS a fe = 20 26 23 ll 5 11 mm. mm. mm, mm. mm, mm. 1716 | 1,662 1,510 1,307 || 1,066- | 1,350 1,410 | 1,390 1,201 1,035 820 | 1,102 790 760 627 573 432 580 1,968 | 1,824 1,560 1,338 || 1,050 | 1,340 895 874 858 704 576 728 400 494 358 282 239 307 183! 184} 187! 180 159 171 154" | 151! 154! 147 145 156 125 124 125 104 90 100 147 145 147 127 121 135 53 50 52 41 35 38 40 39 33 30 29 35 842: | gad} 82:4! 81°6 91-2 915 85:0 | 85:5 | 85:0 81:9 74:4 741 155 780 || 635 73:2 82:9 92-1 459 | 458 || 41:5 43-7 || 40-4 | 43-0 1144 | 1099 103°3 102'1 98-2 99-3 52:0 | 527 56'8 537 53'8 53-9 23.3 24-3 23-7 21-5 22:3 22-7 43 Sister of No. 20, * sister of No. 18 65th Report, Brit. Assoc, 1899. 7 6. Nootka Kwakiutl, Ma'malelek-ala, Ne’mk-ic (Worth- Western Tribes of Canada. 5 : ; TA, Kicakwutl Half-bloods 8, Sishiadl Women Males —- - = = = : LM. | II. Female I, Males IL. Fe L Boy |) i Gins | 3 | | 2 | 3 3 4 : | 2 |: : F 'g | | . | 3 Ele | | | S | | | 5 = | | = I e 2 | | | | | | =) | Jz eem| z | 2 za }2.| 2, | et eal | 4 Z = || gz | 23 | a) 3 Zo |e | 4 | Ze | \ a | = 34 |3 Er mer rea) | 2 el eS | a 2 | = a= i = = | q z ey es | fe | = Z =| It 3 1 || 3s 2 = is =| 22 | 25 | 3k 4 Be lee) || = EW Ne fa | leesual| 3 | #5 | Be ¢ | 3 Tribe Er a) es Pea 2a G | a2 S 3 4 | FI | ic us | 3 | 4 x za | 2s | #3 $ a | sf) 42 | 2= 5 q | ae | a@ | a a |e z | | 2 3 se | oo | ee Be Bet WSs Wigs ee We | 3 | a | me} cs | | z \ean| = | my | “2 2 ea | 5= eke ig | | | | Ba | 2 | | = a |e « 3 | os : Bi | | | | c | | | | | | rt || | | | | | | | = | | | ; = | | =| Are 40 18 18 | 236 Joan | ac | a3 | as 12 42 | oo | co | oo |} a | 8 ul ia | 38 | a | | 5) || 40 26 En | en a | Height, tanding 1,001 1,038 110 | 1,660 | ao05=) "990" 1353 | 1460"! 1,486 1,06: 1716 | 1,602 |) a,e07 |) 1,066 | Height of shou 1317 | 4 1,000 | 1,286 1100 | 1,183 | 1,234 | 1,868 | 1,292 | 1219} aio | 4,390 1,201 |) 1038 || s20 Length of arm 630 | 705 673 | gia | - = — || cu | «sr | | | 695 | 714 | 790 | 7H 627 673 || 432 | Finger reach 1682 | 1,650 1,950 | 1,615 | 1,782 1a 1,262 1,663 | 1,694 | 3,674 | 1,680 1,564 | 1,608 | 1,601 || 1,908 | 1,824 | || 1,888. |} 1,000 | Height, sitting | 50 #9 7 800 eH0 | 835 | 816 686 726 | | | ga. | g37 | 833 | | soz | 764 au | || 704 670 Width of sbonlders 383 | 366 ss | — 297 aca | 93 | — 353 | 267 | 309 | ais | | Si) = i) tea] uo | 318 | gos |) 400 | 401 |) 2x9 |) 259 Length of head 188! 182!) a7) 1998 a7?) IML weit | 1807) 198") yore) — Wo" !} so6"| ama") i79") azz* | ae48) 477 | 190] 180° igi? | 179* 18st) 1Ndt 187! 1s0 || 169 | amt | Bresdth of bead 161! | 146" 160! 458! 60" os? | 169%) 160 yoo'} 1612) 156") 163] 168 | 167° wo} 140") yaa") 147=| 160") i641 | }/ 1525) 165") 14s| 162°) 163") 145% | 154! Xi 164! |} 147 |} 45 | 166 | Height ot face | 118 tor | ue | 198 13 | as2 | i260 | air | am | in1 | 124 | 190 | 188 |] | io | as | 103 | an | | 193 | an | wo | uo | nia | us | 24) 195 wos |) 00 | 00 Breadth of face | 1465 126 40 ie | us | in | ase} 166 | a1 ) 103 | ir ue | 183 | 335) is2 | 140 | | 139 | 135 80 | 148 ) 5} 17 } 2 | 135 Height ot nose | 41 62 2} 45 | | 60 66 | 48 se | 58 66 | || ‘er | 2 |} | ss | 40 | 43 | 45 | 6 | 07 “ 46 45 | 68 60 |) | | 35 | 88 Breadth of nase u | 86 | 35 36 w | 43 | 43 sa |) 87) 87 | 13 | a1 | 43) |} 2 | 30 | 33 | as | a5 | st | as | 30 | a7 0} 39 ] oo — E i —— |. ——|--__| |—— — - —|-—_—. ——— a Leoitbbreadth index | 80a" a24)| eea'| agg? 08?) soa") BoUe so8*| s53*| — | g4o'|| gs7)| gvo'| saat] gaz “| 750?| soo") sci? s78*| 51 | s1' | | Paclal Index | soa | 849 | sl4 | 005 | BIL so | ao | aoa | axe | #50 | sve | 27 | 850 | 30 yee | ain | f asa | oa | ss | are | 86 855 Namal index | 723 | woz | ara | ora | oo | 033 | oo. | 771 73 | p90 | 708 2 | 79 | 603 | ste | 763 | 750 | 767 550 | 614 | 705 svc | 667 780 =e | | | | | a) OG Th | Ye) | OSE een is pes ASST OO! Tedex of arm | a2 | 43 |) 40s | pe) aan | vo | 44 | aco | ase | au | ace | — | 46 | 45 | ato | ave | axe | — || asa |) aco] — (ato |) sew | seul (a4 | ay | 438 450) 459 | 458 Index of fnger-reach . 1051 | 1057 || 1055 | 997 | 1074 1088 | 1100 | 1050 | 10¥6 | 1066 | 1094 | 1007 | 1082 | — | 1057 | 1004 || 985 | | 1000 | 1036 | 1057 | 1099 fauece SCN ta 1055 | 1028 | 1017 | 1027 1084 | 1144 1099 Iedex of : | 2 76 28 | sa7 | soz | ose | soo | soe 620 627 Vee t eight, sitting 625 | sod || o2 | ooo | ono | ore | cre | oid | 657 | B60 | 644 | oan ex Bese meee OH ein, bebe ee, ese | ees | eee hae | ae me | ga | stn Index of width of shoalders } 920} are | at | = \ ox = ais | avs | 297 | 6} — | — | 28 — || 20 204 | 220 | oo | gus | — _ ou5 | 240 | 2206 | SL | 20 a 2 3 © Sister of No. —— ~ —— = 5 = Hon OENo:IG0 7") Enthor o€ No: Wi Sister of No. © Sister of No. 20,“ sister of No.18 ‘Notdotormed. + Slightly deformed. _* Moderately deformed, Mother of No, 1, Son of No 1 Father of No. 1. ister of N er of No. F. NtlakyapamuqQ Christine Joseph | M. PEla’tlq [North-Western Tribes of Canada. 6 10. Tribes of Harrison River. 10a. Half-blood Stsré lis. I. Boys II. Girls Boy 4 5 6 qT 8 9 | 10 11 12 2, \ Fa nie Parla Seg. We >| E es eee as |) a | Ss 1s a 3 S = g g a Bs a M [S) =| “a Db cal — oS 2 Ss = a = is = 3 I a Fi s q s 8 5 a | a | fe = 2 4 4 id vd ad = +s A fe ae) n he & a ac — rr) = =o a) — a re! / Az 5 a 3 a 2 a = “| = 7 S = 3 a B S 8 S| g cis a a4 wm n 4 4 M4 . a R Mm R mM RQ as nic 5 geht | tall 46 9 1,200 | 1,366 | 1,197 1,468 | 1,198 958 | 1,094 | 1,213 | 1,198 | 984 517 | 609} 654 | 646 || 534 1,197 | 1,424 | 1,523 | 1,520 | 127 653 | 726] 796 | 785 || 646 253} 304] 318] 328 263 166 | 167 | 182! 162 171 143 | 146] 165] 153 | 153 94/ 105] 111] 102 95 1290) 1265) 141 |" 137 124 39 46 48 | 39 || 38 30 34 35 34 33 } 86:1 | 87:4 | 90:7 | 94-4 89°5 77-0 | 83:3 | 78:7 | 74:5 76°6 769 | 73:9 | 72:9 | 87-2 S66 431] 445 | 43-6| 43-9 44-5 99-8 | 103-9 | 101-5 | 103-4 101:4 54-4 | 526 | 53:1 | 53-4 | 53:9 21:1 | 22:2 | 21-2 | 99-3 236 Report, Brit, Assoc., 1895,] (North-Western Dribes of Canada. 6 9. Tribes of the Delta of Fraser River LOK Bar 94. Half-boods, Delta of Fraser River. Stare li = a 1 Boys M1, Girls L Boy 11 Girls i I. Girle Toy 3 1 2 $ 4 r 6 7 8 4 10 i 12 13 MW 15 16 17 18 19 20 21 22 2 pt 25 26 28 30 31 33 | 31 35 46 37 38 3 40 41 | 1 ae | ea) 4 i re Ma cy ll oy 10 il 12 | 7 | 7 Saal ~|I >| | 7 { £ S38 5 g | eee heel | } 5 2 = 8 5 a | | 4 | | gg | 2 st 2 PI 4 z E 3 2 5 Sailieg 2 WS 3 = £ = g 3 a 2 Ss 5 ET 2 5 5 | 2 e = $ z z= gs 4 | 3) 8 | 4 B 3s | T ) Et | | | z a a | 3 = = = : z £ & 6 | 4 : S | 2 ° 2 | \ 2) |= | = | a || | | Z | | Py “ 2 Vela acl — || R Wart Meee fe ee ; 5 3 Eta) é S35 | 2 | 23 || 3 3 |3 | Salea z g a > a 2/é Bu | q Jz |e 3 5 3 8a |, let | g|a & | 2 2 A ae Ale He ra a | a im | | | : as} i se = en |e | 4 | | 7 | 9 [90] 9 | a0) } x0 [aay] a | aagase|as fm) a) (Fo | so ban) a | in | | a2 | ia | a8 | aa 6 | ae | az | an as] area | | | ao | fa | oe fae fo [to any] a2 | as | as | aa nm | 1 | 16 ry ; om. | om.|mm.| mm | mm. mm.| mm, | om. | om. | mm. | om. m mm. | mm, | om. | mm. | om, | mm, | mm, | om, mm | mm. | mm. | wm mm. om, | mm, om. | mom mm. | mm | mm. | mm. | om mm. Ing «= 166 /1.180 | 1,286 | 1,208 |1,504 1,240 |1,870 | 1,992)] 1418 | 1426 [1.418 | 1/5034 1,978 1,501) 1,465 182 | 1404 17 1,061 | 1,198 | 1,295 |1,860 | 1,410 |1,856 | 1,898 14d | 160 |1,107 | 1468 1,108 f shoulder su | 942] 950] o44 1,123 |1,075 |1,173 | 1,164 | 1,162 1,122 | 1,107 1,108 1,176 {1,197 1,190 1,019 || 835) 925 |1,010 | 74 |1,122 |1,103 |1,120 1,188 | 1,140 | 1,004 |1,022 | 985 | 1,030 958 | 1,094 (1,218 | 1,108 98k | 505 | 508 | cio 615 | 610} ai) 22) 031 | 587 675 | 6x6 23 | 068 618 669) 436) 473) G10 | 587 627 | 60 600 | 654) o16 634 227 1,427 |1,426 | 1,470 | 1,470 | 1,468 1446 1,868 1,488 | 1,687 1,550 1,404 |) 1,053 |1,215 | iy 430 1,516 402 1,217 sitting 602 724| 096| 747| 766) 771 73a | 740 750 | s16| 761 710 | 800) 818 $00) 1 6a) o&t| Get) o93| oss | a76} 712 677 O15 { sboaldern 4 318 | 309 | 324 412 310 sos | 335 | 320] 44] giz) 935) sou 285 | 937| 969 | 401 248 263 wh of bend . 1705) 177 | 169 169) 174) 181 187 170 170) 471 174 | 171} 108] 180) 180) 178 | 181] 181 | 170 | 178 170 | 173 | 100 | 188 181 162) 102 71 neith of head 165 | 143| 152 156} 160} 163 | 1s0;| 148 | 364 | M48) 166 Ma) 149 11 | 152 145) Wi) 11) 18 | 360| 166] 147 | 349 | 140 150 M7 150} 162 167 165 | 168 153 At of fas + «| | 95) 100 102) 105) 96 tol || 92| 102 105 | 105 109) 103 | 12} 104} tor} 119] 12} 115] 110] 105 | 96) 97 1 110 | 103 | 7 | 103 Mt 11} 102 95 of face +} 327 | 125) 131 133) 158 136 | isi | 120} 191 | 120] 135 | 126137 | ago} 137) asi} 134 136 | | ner) evel seh | 118 129 | 134} 195| 198 | 190 | 152 36] 11 Mi} 137 4 eon - 85 | 37| 38 4o| 41| 36} 42 || 36 42 | | 44 43 is} 42] 41| 43 49| 48 | 37 43| 43| 47] 46] fo] 43 33) 49] 44 48) 39 38 pets ot nome 2) Ne) 88) | || a6| ae| 34 | as} a3] ssi) 28] at Pall 5 a | sc} s2| a1] 36 s| 3 aL 3o| 82] 80 35| sa| 39) 30) 30 at un —— ( | oS Be ES s We : pea Le = Zs ie |_| = “s eset = ibtraih index a2 | 08 ova | 923) 920| 845 | 931] s76| s11| 602) s40| 905] 84a | a71| ssc so4| 871) sos | ss9| so3| a9 | s91 | 86 | 882 | 850 850 | | 920 | ss | 46 | seu | 92 867) 861 | 874 | 907 Ge Wt 10 | 772 739 | 767) 761| 706) 711) 866 | 827) 764) 107) 779] 783] 914 | 778] 830 | 861) 805 | 752] B54 | 748] S62) 759] 771) B19 sea oro 701 | 71 | 816| 805 | ses | 772| 797] B02| 706 | sro} 758 | s24| 767) 770) 833 787 | m6 al inde 3 : lbs 3 a 5 0 872 | sea ae | 948 | 802 | 895 | 20] 900| 780) 914) s02| 675] 780 166 || 778 | 788 | ovo | 782 727) 820] 688 | 724 | 854| 760] 702 | 829] 83 ors | 720 721| sta} 724] oxo! sea cox | s00| s72| 921 | o75| 890 | 769] 750 | 872 | 0 ae 2 be ane 426 410) 425 | 424 | 453 151 | 462) 444 | 495 44 | 4a | 449 | | 4s3| 427| va) aia] ase | ava] 450 | 434 | ato | 445 | a) go7) 419} asa | 4 42 e7 | ano 4 | 491] 418 449 | 496) 431) 445 | 496) 499 FFG tof finger-reach . ie [ra | | = : alkern 99 0 }103 gerne 1000 |1001 | 1000 |10 |104'5 }106-2 |1080 | 1085 |10 28 | 1084 ||1027 | 1010 1018 | 998 |105 3000 | 1018 | 1047 }1027 |1049 | 1088 |1001 |106-5 |1027 | 1064 1008 | 1019 | 994 |1021 100°0 104.6 | 101-4 | 105-9 1006 |100 | 1026 | 1038 |1033 | 1017 |1002 |1048 |1046 | 998 | 103-9 | 1015 | 103-4 1014 Hof belght, a | ? a ; 5 ra lire roles) 21 . - sht sitting =.) 547 | Bit | 54-4 | 66: | 627 | o28| ce7| c26| 529 | 543] o24| ove | 655] 560) 632| o47| 638| 581 | Gi4| B31) 525 | 53:3] 553 | 560 51 || 554] 068 | 58-7) 646) 5s sos | Sie oo1) 695 | 087) 639 | ci4| 590) s21) 644 626) 631 | ood 539 ot width of shoulders, | 217 | 9 } | sare) |Nteat | 997 | 209 \ Eeraleroiltcetiits oc |) ors | 217] 2291 229! 201| 224 | 2x6) a11| 229] are] on 2a *idth of shoulders. | 217 | 25-4} 297 230 | #32 ac: |aial| cent hmrall salle 215 | 209) 290 | 201] 29 ave | 298 | 227 3| 268) 227 | 209 237! 216! 299) 2p8 295 | a4 28 | 217 | 229] 220) 201| 24 | 206] ai1| 22a 212] 228 6 = TGrotherofNo.28, ‘Slater of No. 2 * Sister of No. 16, «Sister of No. & [Worth- Western Tribes of Canada. é tlakya'pamua. 24 25 26 44 45 46 47 48 49 50 - pete b v <>) of qd vm 2 = A 3 A OT a On oS a a See esp ot s | a} x Siig cea = x SA aaa em at Zz B = ee re = = ——— es ee _ S ne} so rg z Me le le je lg 12 |e lt | 12 12 13 See ee ee Baim oe | Me | Me | Oe | Ay | Oe Ab $3 /29 1/88 | 28 | $438 / 38/38/38) 28/38) 58 | sa S£/ 58/58 / 5a] Sessa ]Be/ 5a |] Bal Be | Be |] Be |] Be Be 2s | ee [28 | 2849 [ae | 28 ag 28 | as | as | 28 SA | 28 | SA | Sa | false (ta | 38) | sh | ta | BS | ta BQ les les [az lesitelfulizeleeleulezvleu/es Ea | es aa Es a s!e & qi Ea g& as Ba Ea Bd J ~ Soa Ss ~ ~ Pee iP Fe IP i 16 16 |6 |5 16 16 [sé 6 9 9 9 9 [85 58 | 60 | 60 | 68 | 68 |70-75| 75 mm. | mm. | mm. : mm. | mm. | mm. | mm. | mm. | mm. | mm. 1,224 | 1,258°| 1,280 ‘ 1,555 | 1,622 | 1,566 | 1,538 | 1,620 |/1,572 | — 971 | 1,023 | 1,138 1,258 | 1,350 | 1,292 | 1,280 | 1,308 |1,313 | — 516 | 523 | 636? 682) 713 | 760) 672) ‘740 )) 7161) = 1,198 | 1,220 | 1,285 1,610 | 1,745 | 1,707 | 1,552 | — |1,672 | 1,558 644 | 633 | 698 830 | 816 | 808] 797] 843] 815} 793 246) 251 | 274 365 | 364/| 334] 354] 348] 361]! 348 168 | 1715) 176 195 | 188] 191] 182] 185] 176] 188 151 | 147 151 155 | 162] 160] 151] 154] 156] 160 101 | 101 96 130) |" 118") 124) 1217) (180 |. 130 | 17 128 | 127 128 149 | 153] 150] 148] 143] 146] 153 | 42 | 40 40 55 47 5b 51 56 62 57 35 | 31 35 40 41 43 38 40 38 43 wae | 89°9 | 86:0 | 85:8 79:5 | 86:2 | 83:8 | 83:0 | 83:2] 886} 85:1 — 789 | 79:5 | 75:0 87:3 | 77-1 | 82:7] 81:8 | 90:9 | 79:0 | 765 83:3 | 77:5 | 87-5 72-7 | 872) 782) 745 | 714] 61:3 | 75-4 | see | a le 42:3 | 41:5 | 49:7? 44-0 | 440] 48:4 | 43-7] 45-7] 456) — | 98°2 | 96°8 | 100-4 103-9 |107:7 |108:7 |100°8 | —- |1065) -— 528 | 55:0) 545 | 53:5} 50-4 | 51:5 | 51:8 | 52:0] 51:9! —-~ ' 199 | 21-4 23:5 | 22:5 | 21:3 | 23:0 | 21:5 | 230| — 13 8. ° Son of No. 10; brother bother of No. 28. 12 Father of No, 20. 10 Brother of Nu, St. rt, Brit, Assoc. 1895 : b. Wtamkt of Spussum a. Ulamkct of Spuzsum. and Upper Divisions mixed. c. Upper Utamkt of Boston Bar and North Bend 1. Males IL, Females | Males T, Males 1 Ha (0) [Un] [LCA PLEIN Pnccenll EDL ET Onn JSC) eG PDE YN puna ue im | 16 | 19 a1 Jeo [so Jan |) a2) say) sh) a6 7 We 2) 13. ‘5 Ls 47 | 48 | 49 | 60 | = ae =! = kK = = | | | = =e ia | 2 all S = | | & | i 2 & £ | 5 }g121¢ 1 see 4 2 2) | -5))) | |eale als s Ss 12 | 2 ¢ | = = s |p a |g | 3 | ee) 2 Pee leese act || ei zB 2,2) 4 zy || 5 g Bin lee Ela 2 |e | 2 | Bile |/se)eig)s ail & |< 4a B lca | 8 |} =k é 2 bP |e2) 8 | =e | 2 | a | a) = leh] |2 |= | oe | Fe 3 | | 2 |42| 2 a|2| 2 We =| z =} Bats E pee ay % | Veo | | 3 a We aa ail glue : B lz q z z | z Pal PlelELElElilele E ESeale a \fa|# |e : 23 |2a\ Elala|el|e)2)e)s)e)é : Be 5s | 5 EAEAIEGIEE E eIEE slelaletede ls | sl zs 23|28)22|28 28 | 22)|28 a 2g |28 Ss |S esales. ase |e ES alti | 33 S332 |/58|32 3 3a\s s =3/33 Pa es || 200 ie | 5 34/52/24 | 52) 3a | 28 =a 32/38 | = |38 | 38 eles ig = a3 ee ie 22 |a¢ & ig|is s| 8 H |e2|ge]e2|e2 | ea aa] ea |e 5 23 |a8 BS \5 ce é | EP jl 3 sia [Rs | )B |e 5 \5 = ii || 5 =P |=) mm, | mm. mm. | mm.) om. | mm.| mm! mm.) mm mm, | mm.) mm.) mm, | mm, | mm. | mm. mm. | mm.) mm. | mm. | mu. rom, | om, | mm. mm | mm. om. | mm. | mm, | mm. | mm: | mm, {1,630 | 1,601 1,611 )1,494 )1,863 1,670 1,624" 1,687 1,610 |1,507 | 1,45 | 1,654 1,492" 1,600% 1,664 | S0s* 24 1,453") 1,288 | — 1,642 1713 1,622 | 1,66 1,020 |1,672 | — der 1 1,246 !1\860 1,274 1 — |it87)1,010 | 1,205 |1,810) — | aoa 7 }1,180 | 1,028 1,820 | i407 | 1,360 |1, 108 |1,313 | — 685) 760) 702| G78! 701 24 || cor) ci) vis} — | 27 | — 516 | ost | 608 78 740 13 | 760 | aol) — 1 1,057 1,50 | 1,645 | 022 | a,007 |1,576 {1,690 | 1,700 | 728 1) 1432 |1 1,728 (1,796 17745 |1 829) 788) 700 7aa\| 7c} 868) sa1'| 823 | 858/480 | oie | mm | 897 | 862} 905 816 | 808 sia| 815} 798 dere 308) 74) 362 _ ay2 || 369 356 | 310 r 46 | 3T7 | Boa) a4 a48| 361) 318 | 192) 181) 183 189) 181) aK2| 186 ye6 | 181) 203 | 104 180 Tei) 188)) 18) 198| 191 | 162| 185) 176) 188 145 | 158) 172 155) Wer | 469) 104) aoa) 62) a7 Yor} ini) 154 161 | 150 153] 156) 148| 168} 159] 155) 165) 165] 157) 156) 164 | 161 155] 162] 160] 151] 154] 156] 160 | 110} 126] 115 | 100] 114) us| sna] st] 104! a2 wel rv | 7 101 108 tov) 112) 116) 117] 122) 120) 181) 140) 115) 120) 121 | 120 130] 118 124] 121] 180] 190) 117) 7 7 | 148 | 143 | 148 | 146 } 1} 42 m8) 141] a6 25 130 135} 133] 186] 142) 149] 148) 148| 161 | 150 ]i1s05| 148 | 164 wig} 163} 160) 148] 148) 140] 153 52] | 52) 55) 00} 60. | 4 45 61 | 60.) (2) 43) 45) 45] 47) 62] oa] 53 48| GL) c2) co} 65) 52) ot 55 se] 02) 57 40} 30} 48] 40| 44) 38} 40) 40) 42] 35 42] 98] 36 35 | 35} a4] 35] 93| 88) go}| a7] 38) 41) 31) 96 40 40 lth index | 882] - Boo | 928) By2) HOT | KOT | BAG) M15 | 815) BiG | 790) BRK 2 8o4 all 860] 855) 890) 303) Boo ore | srs | 873] 869 | 899) #51) S68) S10 95 832 | 707 | B57 | 782) 421 | 861) 774) B41 720 | 770) 815. 2) 7A | S84] 770) 858 739 750| 815 | 793) S17 842] B53 | 824] BLO] 811) Bba) 927) 773 873 900 Bex : sa | O90 | 750 100 | 70% | 800) 772 781 | #00) 0] Bra) aaa |) 977 706 sa | 775 | 875)|/ 933,/ aL 702 | 791) 786 804 | 548 | 720 727 m4 Ja 1 12 S u I" We NS | EE ed | | oe a ee fete Pe = e Mam, 449 | 499) 445 4648) 455 | 402 | 400) 405%) 467 | 4a | 409) — | 490 406) — || 407) — 423 497!) 418 | 424 | 402 Se ee 441 | sia | 41) 460 | doa 440 407 | a6) — Mf oyer-reac 10s | 1608 liox0 105% 1076 |1000 |1087 07/1055 |10h0 106% | tos 10 | ne | 1004 056 /1024 | 961) — |iova| 952 | 1004 |1016 | 994 | 988 1065 | 1050 { at beigbt, sliting GIN | o14) 540] cos | 548) o15| 526) c1G| 528) ote | 194) oai| ors | si) 522 S14 | 617 || 598 | 74) BB | 528 545 1 | 634 554 | - o6 | 629 ; | | tvidth of shoulders. | 222] 237 | 2r0| 230] 243 | a37 | 254 | 217 | 208) 200 Gy) —|-| 222) 205) — bay} s06 Aid|] 246 | 293 | 22-0 || 227° 4) 280 | | ¥ather of Nos. 16, 17,and18, * Mother of half-blooda Nes. 2, 4, and 18. * Son of No, 10; brother of Nos. 17 and 16. + Son of No. 10; brother of Nos. 10 and 18. Son of No, 69; brother of No. 61. 11 Father of No, 20. * Son of No, 10; brother of Nos. 16 and 17, 4} Father of No. 21. * Son of Nos, 39 and 0. * Son of No. 42, * Granilson of No. 42. * Irother of No, 28. li ienel r ei eee i ee Be ee ee ee * rat rt ne SSS See o | site Bo oo se ne onnlorwrrtkownl(HAOlh + +H @ 2 Seoryrocwtwaolowmntaynnmli tool H+ ob oW q#onNn Ey ROM lH Aa a noriwtouon eo Loma onl 4 BSth Report, Brit. Assoc Er) & [Worth Western Tribes of Canada. 8 11. Nuakya’pamua (continued). Dlank-t and Nllakyapamua’s'é mixed. ©, Ntlakyapamun'd'é. Fomales ©. Upper Utamkt of Boston Bar and North Bend (continued), I. Males ms] 09 | @ 2) 63 | 5 a 5 ] | = - —_— a | 59 | 60 | s | 62 | 63 | ot | 65 | e6 | ez | 68 | 69 | 70 is | 7 is | 77 | 78 | 79 || 80 | su |) 82 | 83 | et | 85 | a6 | 67 | 88) | 89 | 90 | 91 | om | 93 |\ 94 |) 95 || 96 || 97 | 98 | 99) | 100 | 101 | 102 | 103 |) x08 | i | | | i | 107 | 108 | 109 | 0 | 11 i | : | | | | 2 ep 2 |4 | 2 g |= E A = a ma| Ase Neha & 2 4 | BE e || 2 + 3 | & > | | ¥ Fie, |) fl z | eae ee: z z 2 ee Ee aie\als ale PES Ae Vale ete ele 2/24 4 2 Z| £/s/3/e |z a | S12 /s)/Elal eyelet ga/e]/2)21 3/28 3 Eee: Se We ee el 2) Be] £|/s |e F =| 5 | e @ | 2 \s Fe ealElale (|e) ela ea) a)8 |) 8] g PLS) e I/F lelaleia | se AL I | 2 & Pale i | | 2 ee ys é & | 2 | 2 | | 4 8 2 a) @ | & | | = a \ z . & is ik i | | | + iF | } | | Z Salle. | = ite lng og g| 2 | ] ] } re ee 213.123.133.123 13 a ai 3 2| Ela i || 22/2: | 8s y)23/4y)83|4yla5 (85 (25g |4y(83/42| 8) Sl. | &| ley] eis isisisielelels || le | sie é 2 < : 2244 =e 48 24 g4| 28 | 48 | 25 |24|a4 38 || | es |e | et] es # eelzgilzliziz\izei/3\/3|2)]2 1/3|3|3 3 S \% = Py = e Py PT e g eltea ey = eT Be || Sar = - alll 2 2 ie i g g Z 2 z Z g z z z g 3 Ss ls 5 Ss 5 S 5 s§ es = 3)\3 32 EF Gy € $23 23 z2 22 et ze |\z3)22|2¢|22/2¢ 2a | #4 | 24 2m 24|25/5. ia BE Bell gia) /e)a)2)2 |g | Fl | 2 2 2/58/38 |38 3a |sa/ea|sa|s8|s8/s8/s8 Sh tg |ta |b | 33 || gs [75 le leis a = }R| |e) & | & & = = 2) 23/23 a3 £3) 53) 23/23) 22 | 23) 29) 22 HERS RS CRS Re eo RS g\2\4 E| 3 ef et ete 4 2 2 2 2/42/43 42 49)92)92 ge | gs 2 qa q2 aa a| alm B\ ea) a Ble le le le 2 | s/2)2)/2 Fo = = 2 2 |3 3 2 \2 |g é a |g Soll) So | el A . a cal | ca | = {2 |> a 5/6 |3 Bre ee ie pe lipiiiie 5 All SI wi gle | Bay | 4 5 6 | 6 | 10 1 |} W iW 19 pz) 24 | 95 | 26 || 30 | 30 52 38 40 40 42 | 65 60 5 8 9 ga | 40 | 42 || 6 6 6 | 7-8 9 9 9 10 68 | BB} GO | 60 65 | 65 = —! a }) 3) | z = = ee =| aett mom. | mm. | mm. . | mm. | om | mm, | om. | mm. | mm. | mm. | mm. | mm. mm. | mm, | mm. | mm | 1080 [1,091,263 1,591" 0381103) 1,163 11,210,128") 1,805 |1,267 1,970 1,608 | 1,635 ia 11,641 BH) 853 11,013 1,313 B12 | 840 914 | 955 | 902 | 1,047 | 1,012 1,017 1812 | 1,341 | 1,273 1,826 47 | 441 | 526 683 | 444 | 472| 499 470 | co2 | 55) 478 | 462 ov) 71 701 704 1,063 1,068 [1,248 1,609 1,003 |1,103 | 1,168 |1,204 |1,160 |1,818 |1,266 | — 1,656 | 1,742 | 1,618 1713 580 | 627 | 683 861 612 | 610 G17 | 692 | 600 705 | 687) 618 B18 | 842} 813 870 246 | 140 | 268 836 | 225 | 249 | 258 | 200 | 268 | 285] 273 | 27a 165 | 364 | 168 | 169) 351) 172) 171) 164 360 | 171 | 174 | 467 | 180 | 178\|} 164 | 168] 472) a7a y v7 187 | 191| 196 | 197] 189 | 180| 183) 190 151 | 146 | 150 | 16g) 142} 144] 155 | I56 154! 160 | 140 168 | 163} 140 | 161) 163) 145 | 149 145 | 141 | 162 | 160 | 147 | 161) 150 | 161 | 155) 168 154 160} 148) 151] 16%] 163 | 146) 150) 146 | 1 | 97 | 93| 93} 98] 106) 112 is | 116 | 110 M0 | 109) 119 | 107) 110) 104} 108 o7 | 102 | 121 | 120 | 108 | 108|| 93 | ov | 95) 97 | 102 6} 117) 125] 128) 115 | 120) 120) 125 123) 119 | 326 | 128) 124 | 1985) 181 | 141 wi) 143 | 154 437 | 144] 134 | 135] 140) 196 | 196 Ya | 198 | 198 | 147 | 141 | 189) 120 | 128 | 127) 121 | ) au aig} 144) tas) a7 | 154 | 199] 148) 145 a5) 39) 40 | 37) 40) 41\) 48) 48 47) 48 | 4 48) 44) 44) 48) 62) 46) 40 go | 40} 47 | 45) 50} 6O\) S|} 87 |) 37) yA | 87 62} 63] co) ol) 48) 59) 62) 52 w | 29) s2| 28) og) a5| ss a4] 37] 92] 33] 34 | 87) 34 | a8] a6] 40] 42 um | au} sz] gi | 40} B4|| 28) 80) BL) sy | se 89) 37 a7 82 88 38 a a8 40 36 39 bo) — 85 40 89 39 42 38 AL 46 “493 | 905 haamiallt ali Pil i| itr a 27 | 7901 808) a7 r 4 Ml 915) HOO 493 | 905) 941 | BIT] O06 | ROL | | 860 S11 | 829] 864] 913) 860] 607 | BOX) B14) 792) BAT | 906 | 826 | 874) Bod | 778 | B48 | 916) 958 | 893) 919) 830) 870) 786 | 873) S47 | 864 866 | 623 895 | B42] S07] BL] 797) B98) 827) THO 802 775 | 170 820 as 0 717) 748 | 705 760 | $09) 795) 123 | 816 | B44) B11| 821) 847] 809) 75-7) B88) 799) 7o4| 705 | 794 r40| x64 | s77| sv0| 200] 277] 270) 768| 748] 740] r46| 101 | soa] 791] 880) e553 | s00| 271 | see 7w2| 803 | e68| so7| s91| eso | — | 738| 705) 812] Bos shi | 862 700 | 730] 914 | 769 | 780 | 814 | 773) 178) 726 | 724 | 771 | 727| 688) 708) #41 | 779 | c8H| o9g| BoD] O18 s72| 775 | 081 | 756] 800) 680) 757) 811 | 848 | 941 | SOO |1050| 717 | 721) 740] 771) GO| 760) 64-7 792 | 691 | 690) 056] 722| 750) — | 80] OTS) 755) ooo 788 | 866 ae irr XG anal near lage ay i mara irre i era PT rc pry i atlcanhl 4 405 | 417 | 481 | 423 | 499 | 443 | 426 | 428 | 490] 473) 418) 448) 448 | 43-7 483) 445) 431) 483) — ! 405 | 40-7] 404] 493 | 480) 426) 499 | M92) 429) 434) B94 | doa | 427) 421) BO4) 434] 447 | 492) 448 | 444 45 | 459 | 435 489) 460) 441 | 438) 492) 496) 452 456) 420 94 971 | 99-0 |1011 1010/1010 |1000 | gx | 1026 | 101-2 |102%5 |101-3 }105% }10%9 1026 |1007 1021 |1027 1079 | — 1026 | — |)1000| 976 | 986 | 1019 |103B | 990 }1019 | 1000 | 100-0 | 1000) 995 | 1018 |101-0 | 1000 | — |101°6 | 1058 | 1024 |108:8 | 1058 107 |1064 | — | 1007 [1017 10841 |1056 | 1082 ites 1069 | 1008 tes ee 7 675) os2| 692 ce | 527) oes ox | O12 | 42) 651| 669] 653] 647) G41 | 529] 643| 661) Goo] o18| 624) — |) 650) G4] G50) Ga) Gai) 686) GOT) 494) G55) 637) B72) Ba1| oe) B41) 483) Gos| 632) 525) BIn| OLS sat | 495 | G24) ons| 030) ox2) B02) tT B a Buz |/oxe| 6 eae | 28 | 20 | 218) 21a) 218] 290) 217 | 291) 219 | 214) 222] 224] 925) 199 | 293] 220] 228] 220] 21g | voo| ore] — || 201] 209] 291] 211] 227 | 216] 202)) 210} 226] 224] 216 | 287] 209) 210} 215 | sv5| 208] 285) 17 | 260 2o4| 220 | 228 | 202 220] 200] sio| 2va| Sint ara) aia | 297 | 294] 28: 1| 227 ‘ Danghi ister ‘ Nos. 7 80 and 111; sister of Nos. 76 and 78 —* Daughter of No, 140, sister of Xo. 31. ” ri 7 y ” " ” if No, 64. Sister of No. 62, © Davghter of No, 73, * Mother of Nos. 31 and 35. ® Mother of No, 67. * Daughter of Nos. 80 and 111; sister of Nos. 76 and 78. = Daughter of Nos. 3 er of Non. 60 ancl V1.1 alter of Hons 16 aod Toe AR BENE BO Oa oad 18, Cae et ReRUCTA et ot oe: To eae oe, Te und 101 (placed by mistake in this group). Son of No, 188. ™ Son ef No. 106; brother of No.2. \ +" Grandson of No. 140,» ™ Son of No. 106; brother of No. 86, ™ Father of No, 120. ™ Father of No, §3. _™ Brother of No. 108, ” Father of Nos. 82 and 180, Father of Nos. 86 nnd 92; brother of No. 102, ‘\ Father of Nos. 75, 76, and 78. © Fathor of No, 16%, j <— 2 = — _ sinc ——————————— ee = ll. Wilaky na ve wo tad = 1D 10 r) 2 o> o = a | d 3 s Q for) 3 x = BS iC a 5 | 2 Sa 32 35 . mm. mm. # |1,54855) 1,505 B |1,258 | 1,227 674 682 1,565 | 1,605 777 329 179 140 119 130 53 31 78°2 91-5 5E 45:2 106°3 522) 51-3 Inj21°8 91-8 [North-Western Tribes of Canada. 9 mua’o'é (contite’s'e and Upper Tribes mixed. II. Females 159 160 | 161 162 | 163 | 164 | 165 166 4 4 iF ql a0 = 3 —| Ss a. re} ee ees | 2 |) pe 3 | < I | 2 ane Romer |lesu || =: ||| o> | 2 | 2 | aj) 2 i) 5.15] [le | 2 | 3 3] | } | af S 3 | 3 | 3 $ $ S a I : E ES | 13)2 g Ble/e/e/2/2/8 |3/ 3% 3 l2]/2|¢ 2 2/3/32 3 PEPE allied Atlee clk © | Je | a Z e)/—a|ei|eée|é | 5 q | 8 B)/afe|ela z g |e | 8 F| | 35 |S—8| Seiise q2|23| 5 | $2) 5 = : z|3| Es e|a/ dfeleyelelelé Ea ee es ee ES ;2e}4)2)¢ 5 aa lage a5 (Be de |e | 3 |53| 3 | P| 2 BB |e ) & Bb |i B)e)b) eG) & & | Ble) & 2 ne eee §3 | 23 | \ 3 /n2| 2 | 4 2) sees a | 3 legals lose leaulisaullire 4 22 | 2 3 |#3 RS BF Fe al ental a (2 {| | 2% ea || fe | Meal tease tea jl eae: || as; ||) az \|% )4|% | a )a)z % 4 |% | % a I = i = = | S | | | | | Bel) | eel | a [ae a ia! A | PA! | Age 16 | 16 | 18 || 18 || 18) | 19 | ay | 28 |) 30°] go] a 40 | 40 | 45 | 52 |] 53 | 65 | 55 | 55 | 5B | GO | 6O | 60 18 | 40 | 42 | 70 | so | 40 —— oe ee al aes x cork ee eel = Esee = = = | | ae | moo. | mm. | mm. | mm. | mm. | mm. | mm. | mu. om. | mm. | mm, ram, mo, Sel | | standing. |1,607> 1.6485) 1,349"1,622™ 1,5 H1A90° 1.5668" 1, Lol 1,697 347 1,610 1,656 1\540")1,673" | Height of shoulder 1,286 |1,270 {1,266 |1,105 {1,247 |1,301 | 2 |1,298 1,902 |1, 1,220 [1,168 |1,907 1,298 1,270 [1,481 Length of arm 716 | 650 | oan | 562 | 647 | cor | 682 | 718 | Gio | oGi | 653! 39) 679 | 695) 034 | c20 | a3) oaa | noe 065 683 | 689 Finger-reach : 1,670 |1,518 |1,606 1,668 /1,619 11,628 |1,604 | — [1,665 }1,605 {1,655 {1,477 11,686 1,565 1,642 1,600 |1,612 |1487 {1,490 |1488 ideo | — 1,620 hi,oss.|hoas Height, sitting 405 | sox | 703 $10} su6| 701 | 827 | 793) siz | 777 | a6 | sos | soz | s30| 825 | sto | 761} sio| zor | 753) 736 | 798 520 saz | sso Width of shoulders 330 | 948 350] 367 | 33 | 362 | 931/ 940) 329) a45 | 301 | sac | 938) ag0| s48 | 923] soo | saa | as| axe | ser 928 | 391) 360 | ass || 836 343 | 71 Length of head, : 172] 179] 83 | 188 | agate | iva ize | ae | 189 | 170 “Twi 18 | 181} 161| 11 | 361] feo0| 179] 186 amo | 183 | 161 | 191 | 172 1)| a7 172| 180] ist | 178 } Breadth of head 161 | 144 | 148 151} 165 | 158 | 147 | wMtads | wo} 148 | a4 | ruc | 144 162 | uz} u3| 152] 148} 142] 162) 147) 149 149 | 162 | 168 | 160 |) 147 150 | 16 6} 149} 152 | 152 Height of face 107 | 105 | 105 us} io} 110 | 117 | 17} 108 | 119) 118 | 11s | 12 | 105 | ut} 14} 112} 110 | 108] 116 | 108} tin 102 | 108) 122 | 125 | 93 ut | 108 13} 122] 14 | 110 | Breadth of feo 185 | 134 | 183 185} 1G} 188 | 184 | 137] 137 | 130| 199 | 197 195} 141) 142 | 132] 138) 140} 136/ 185 | 134] 186 136 | 153) 145 | 149 | 121 18s | 133 133) 138} 143 | 144 Height of nows a0 ja} 40 62] 46) 45] 49 46) 42 68 ol 43) 60) 47 oo} 49) 49] G1] 62 47] 63 a6 48) 49 | 68 89 go} 47 49| 60) 46 | 45 Breadth of nose 87) 36] 85] 38} IL 85] 87] 33] BH] 36] 81) 31} 85] 35 a3] 86) 38] 37] 38] 40 33 | 37 ag} 38] so} 40] aL a] 36 35| s7| 36} ax Yevith- breadth index 403 | 898 | 817) #02) ayn | a52| B17 | 879) 867 | Go9| B88] B92) 881 | o04| BOG) S78| soG| B80) rH2| 707) HBB | 792 79 | so2| s47| 87-8 | 790) 777| S40] sox) 765 | SLT) s21| gor 32] 885 | era | ssa) o55 S43) 854 $49 | 828) 510) B54 ee Ao 74) 704] 770 | 789] 810 | 707| 709] 78a] 741] 81-7 | 703| 783 | 707] 742) 709) B37] BL5| 747] B73) 704| 788] OVG s90| 789} 778 | ao1| 762] so4| 912) sve! 794] 859] 206] seo 750| 706} s11| so9 | 750 805 | 12 850 | ss4| 791| 764 Nasal index . a | 704 z ; i “8 | 80 : 783| 73:6 | 5€ 6s | 700] 767] 720) 809] 740) 770] si6| 627) ora] soo} os 100-0 | 792) 796 | 690 | 79.5 8i6 | 766 a4) 740) 739] 739 —— : 16%) 703) ovo) 850) 756] 786] 783)| 783 | 867 | 800] 949] 833 | 701 948 | 705) ors! so4| 783) co4| 753 a} Bo i) [fe] es eae aes | eal liata 404)| 420\|/aaj| 409 |lacailevall-asa|| as0| aea|| asl avail avai|aao\| asa) ase 492 436 | 126| 423 | 420| 438| 461| 493 | 428] 431] 402] 449] Ao 440] 442) 434) — | — | qos] dea] a67| 425|/ — | ace 443 | 459 Kader ot ger-reac . | 994 |20¢0 | 1000 50-0 | 996 |1608 | 984 | 1022 |1034 1058 | 1018 |1057 |1006 |1002 | 970 | 1004 | 1049 | 1026 1022 991 |1016 | 101-6 | 108% | 1032 | 1088 | 991 |1028 |1o11 |1027 | — |rora 1050 | 1066 | 1054 | — | 1022 |yo11 )1036 |1097 | 1026 | 1027 }1088 | 1012 |10%4 | 1043 fedex of bgbt, ating BHO) B59) 40) 616 | 653 | 598) 546] 601] 586) 4182] 512] oL0| 542) O15) 590] 580} con) 620 627 589| 64} 699] oo4| o28| coo! cio) ors) 612) B14) cL! oxo tt) 62) ooo | — | — | grs| 527) sx8| sro} — | 626 ae us 554 lex of wid x “ 9 is ‘ ra | ob a} on E r v5 | 214 4] 284 934 e y 208} 248] 240] — | 208} 921] 917} 296] 21.1] e929] O15 | 294] 299] O86 poet tot aleatien = | 788} 243] 200] 291 | 202] 209] 294] 195] 205] 208] 290] 219] 220) 212] 920] 220] 226 251 ave | 2v3| 202] 214] 219 | 922] 295] 214] 20:4] 280] 230] 224] a18| ave 2 Granddaughter of No. 1067 % = © Sister of No. 198. Grand-davghter of No. 106; sister of No. 116; twin sister of No. 127." Grand-daughter of No, 149) sisterof No.129.__! Grapd-danghter of No. 106; sister OND AN; twine OE Neca NOG and AT, Sister of No IK. Sister of Now 117. s* Daughter of N TOUR ET SHS TONER PSN SoeIN EMRE Danghter of No. 148, ® Daoghter ofNo. 77. © Grandmother of Noa. 126 and 129. = Grandmother of No. 84; daoghtar of © Sister of No. 122, 4 Sister of No. 126, Daughter of Nos. 103 and 190 ™ Sliter ot reaae “ Mother of No. 19, ® Mother of No. 140; groatsgrandmothor of No, 51). Son of No, 166; brother of No. 160, * Bon of ™ Son of No. 156. Father of No, 165. * Daughter of No. 162, f 1 Sister of No. 165. 1 Daughter of No. 160; sister of No, 159, » Mother of No. 119, 1 Mother of No. 157. ™ Mother of Nos, 162 and 169, 65th Report, Brit. Assoc., 1895.) [Worth- Western Tribes of Canada, 10 11. Wilakya’pamus (continued). ——- 8: Vkamtci’nsmua. h. Vkamteinemua mixed with Shuswap and Okanagan = iB AES {Females a If, Females Number lot | 168 | 170) a7i) |) 172)|/ 178) | 17 [faze | ato | 178) | 179 | 180 | 181 | 188) || tes), 184 | 185) || 186) 487 | 88 | 180 || 100 | 191) 192) 199i 198) | 1951] 10m] a7 )va9m |vaen. | 203 201 | ¥05 | 206 | 207 os fee zi [laze a ell Hy t || | | | | | 4 en | | = = i} =a | | teal tim na { a | £ ga | 4] Beli ey | | @, || S eg Vie | le teal eed eee i leet | el G0 eee |e eel (cer cule a) 8 4|8 2 | 3] ale | EN cll Tey lla S|. 2S eee alee: Aalst apes = 8133/2 2 | g | # 2)e fe Is Siaien Sis )42] 4 ey i ject re Ca neni ey eye) ) |) EP Vee PEE NE iy aie ys 2\3 ales 3/4 see einen) = Weaules ales | S|) 3 | 8 | | 8 |e C| o. | F = E | 2s a EL |] | a | a d | | 2 | 3 5 | ce ch ety El IS z ies ee 2 }2l)e)g|2 Bla) 98 | gis aes 2/2 eae wie 8 iS | ants 2 E | | | | te eee | =| Pc | ae l — | (Ls 2 L | | | = | | I | } = i | | | | | | | | 2 2! g oF ol 2] ¢g 2 z1 2] ;Z/g]2]gle]e}2 BOW EWE Fe Mp ee A a | & z) 2) 2] 2/2] 2 leeelsg| 22 leacece| a4 | oa ezelece g | | I Z | 28 |eesees| ga 5 EEE! 1 2/2 Wench face line EPEAT ee EEE EE EEE IE fale]ai4 a) 2] 2/2] 2] 2 ese fe) a2 eee cas| ee | ae eke de ribe S GSE ect [cy |} ach || Eee each iece cn ewer |) Si}e |e ia s/s)/2]s]8 | 8 jeeal se) 2s joecisgs| £5 | Seals B13 Z/S/8)ala/3] 3 Bis) e)3ig)3 i]s 0 eval B|3|8]3] 8 | S lees so | 38 [Sesaas) 5s | os lessees | 3 z Je |e ig ania (3 \3 eye lglglalels Ene} i a Z| BEEN EE EE | 38 23 ERBEEE og |og BERIERE! A felzj2le)2i2 2 g)dielellala S)e)2)e]2)2l2|2) 2) 2] 2 jactian 22 eoeckelaz | a2 eee ees | ea | ena lfires || 8 |f Blalz|2a iz |) ea WW z|z2l|a2/2)2 | % IE Beg eAseeg “S/S BSG | | z 2l | 26 | 25 | 29 | 30 | 33 | a8 | 40 | 50 | co 65-70] 70 | 76 | 95 6 ie | 16 | 1 19 |e [35 | a7 | 40 | 48 | 52 | co | 68 | 70 || 48 63 | 65 BSphtssiailee om. | om.) mm.) mm | mm. | mm.| mm.| mm. | ma, | mm mm, | mm} mo.) mm. | mm.| mo.) mm. | mm. | mm i mm. | mm. ight, standing 1,860" )1,674 71,716" 1,655 1,600")1,6081,645™1,600" 1,618 | 1,610 1,602 | — |1,540°| — 11,016" 1,108™ 1,605") 1,642 |1,612 pW pee Height of shoulder 884 | 1,569 1,206 | 1,900 | 1,972 |1,048 | 1,228 | 1,350 1941) — }),246 =— 850 | 887 1,274 | 1,363 1,297 | 1,178 eee | 47) 836 TL} 707 | 749) 715) 689) 707 wor] — | 686 | — | 439 | ace | 683 578)))| (686 Ra ae 1145 | 1,855, — {1,660 | 1,708 | 1,685 | 1,601 | 1,062 1724) — jel — 1,032 (1,075 (1,565 1,875 | 1,490. re Ht, witting -| 600) 926 23 | 833 | 842] Bed) B10! B42 B27) — 773 — 593 | 619 | #19 840 726 een ede 265 | 408 363) 374] 382] B71 | 969| 343 862] — | 341 | — || 225 | 208 | 954 833 | 321 Length r = rae Ir = ere +] 178)) 202 186 | 190} 170) 187) 197) 181] 190| 181 | 187) 198] 186 161 | 162 | 184 | 185 M7) 178 Ree pea +| 1) 10 166) 161 158} 163) 158] 148) 130) 102 | 101] 161] 108 138) 161 | 154 | 149 152 | 150 ae te 2 90 | 145 110) 116} 120] 420) 126) 11) 198) 115 | 122] 118) 119 90 | 113 | 118 | 118 110 | 102 Sister on He 143] 144} 343) 147) 165 | 140") 8) 145 | 48} 145] 146 us | 126 | 136 | 140 M0) 143 Ree a8) 5. bo] 48] 52) oo) s2] 63| c2| 5, 19 | ot| 48) co st} 42 | 4a} 47 43) 48 oe he | 4 85] 40} ya} a5) a7] a1} 41| 36) so] a8] so] a8 ai} so} a5 | ss anil 37 Leogti-breadth lracalias ——— = — } - = | = eon ett Index . 890) 602 | B18 | #24 | H4a 833} 795) 86:5] 818) 802] 818| 789 B40 | B07) 763) BOF 860 | O82 | 887 | 805) S61 | asa 762) 850} 809 827 793 | 797 || 802 834 || 866 | 787) 770) 855) 859] 843 PAE : 726) 694) 761 | s70| 848] 700] #00] 902] #16) 806 | s54| 8n5| 793 | se4| B14] 15 770 | 697 | 868 881 | R21] 888] 769] 868] S20] 5:0] 8x1} 852] 710] 781 709 | 764| 890 | 806) 837| sve | 713 = = 868 | 746) 74:5 O70 | 70-0) BX | 7A) O25) Te) 774) 788 | 665 BIG | 704] 750] 683] 900} 727! 78% B98 | G4 | 77:3 766 | 830) SIG) 796) 645 | 800| 800] 783 | T41| 958) 792 769 || 763 | 787) 783) 667) 814 | 771 Thies of aor) _ 3 [= = pana! s — . ad Tacs cae s | NT) 469) 453 | ana} 407 | 445 ao4 | ana 461 | 450) 439) 457) 439 | 404] 42] 477) — | 4n5 |) — dw] grs| 498] dor 441 | 482) 45:0) 441 | 422] 455) 4093] dod]! 441 | doa | 45-0) 445] 495) 462] 497) 495 | dos Niles chien 101-1 1008 | 1059 | 1068 |1062 | — |4064 }1095 |1015 |1o1-0 |1032 |1070 1or'8 [1091 {106 |1078| — j1ors| — 96:3) 969 | 1000 | 1082 1016 | 1057 |105.5 | 1021 |1020 | 1069 | 1020 | 1048 | 1045 | 1052 | 103-0 | 101-2 |102-7 | 105-0 | 1016 | 101-0 | 1049 Inder of rh Hitting, SH1) col) oH} cee! oa2] ora] ox] ova} o20| 548] cea} oie! oro | cox) 527) or | — 58 | — | on) soe} 525} coe so8 | sa2| seo] o13| ors] ors | 484] 518) 623| 523] 620) B60} 524] o3a| 520) 638) 514 of width of shoulders. | 295 | 49 | 2 : 2 13 | 92: E E | 214 i : & = of ahoulders . 246 | 421) 291) 298) 2468) 297] o40) g2| ong Ad} 2H) 21 201 | 225) 229) 226) — | 222) — | 214 | oye) 227] 227] 204} 210) 222) 233) 222) 210) 226] 212] 221) 21-9]| 226) 21-9] 211 || 208) 214 | 222] 202) 418] oo9 of Nos, 179 and 207, nN ai 5 7 @ other of No, 170. __™ Son of No, 107; brothor of No. 176. © Brother of No. 1u8. " Hrother of No. 173, ” Brother of No, 172. Son of No. 198. “ Son of No 107; brother of No. 169. Father of No. 187. ™ Father of No, 167, ‘Father of No, 188. Daughter of No. 192" ™ Daughter o€ No, 18. ™ Daughter of No. Wh." Mother of No. 186, and of balkbiood No. 6. ether of Nox 169.and 118." ™'Mowher of No. 174, Mother se-Ne er, = SS = = — _ a 5 Ih 19 | 20 = a S| 8 ag i=] a | ig A ao > os Dn | < re iy re) om Bia 2 | = cc) as qs dq Ss S35 oR] S HE Bale os | aa - 3a 6 =| irs} Fs || 2 a Alm! § | BE a fe = <4 a iv) Ih}: 12 1,5 mm. mm, 1,376 | 1,340 1,112 | 1,092 628 | 612 1,466 | 1,409 752 | 747 315 | 305 179°) 176 148° 142 109 | 106 128 | 129 46 | 45 34|- 32 82:7 | 80-7 852 | 82-2 739 | 71-1 J45°5 | 45-7 {06-2 | 105-1 ]545 | 55-7 22'8 | 22:8 her of N« “6 Daughter of Julie Célestin | | SEQua’pamugq (Chukchukwulk) 34 84-4 88:1 77:3 42:7 103-1 5771 20°6 stern Tribes of Canada. it 13a. Half-blooa 13. Okanagan. Okanagan. II. Females | Males ae 2 2 I n fe) be vey = aie es epee So) ef. e ae) mS Gaye Male gs = ee ee) a | Mg 8 aa | & | ag s S| 4 lies: 3 xq 3 = ic3) i RMR hee es a | 8 a a F Se | Os ap toto) op ‘aos =| S | Ss s oot = x ; 8 = Beery os ex A ong oS iss] | Ss | Oo Ss o) a4 ~ i : a) fo) jo) jo) eee Me | = a= = ala eat }12 12 1s |, ay 1l mm mm. mm. mm. mm 352 1,354 | 1,552 || 1,355 1,270 103 | 1,103 | 1,284 1,087 999 111 99] 110 | 97 103 134 | 131] 140] 196 123 43 41| 43]) 41 44 32 | 29 ene 30 34 53°8 86:2 | 78:2 81:9 78°1 2°8 75°6 | 84:6 77-0 83°7 4-4 70°7 | 76:7 73°2 77:3 37 45:2 | 45-8 44-1 42:7 22 {103-4 | 104-7 || 100-7 99°4 4:3 64:8 | &2:9 64:3 55°8 20 224 | 226 21:2 22°1 = S = = = 2 = : R British Azsoc., 1895.) port, J , : (Worth- Western Tribes of Canada. 11 11, Nuakya'pamue (continued) 19A, Half Blooa i. Holfilood Nuakya'pamun. 12. Shuswap. 124. Shuswap Half-bloods. 13. Okanagan. Okanagaris 7 = =e = = = ; | I. Males | IL Females . I, Males | I, Females | 1. Males | I, Females || 1 Malo | 11, Femates | Males = T 7 7 = a } = h = Se /—_——] is 9 | 10 fa | a2 |) ae a ws | 16 [a7 |e | 39 [20 fa | BO) ee ea toh ay ae asp ae ashe) | ar [ae] to) | 20) an fea 23 | 2 | a cn ea) <<) ca ea 10 1 2 |v] } i | =; =| =| i } — | a S| 4 4 | 2 a | i | | i 5 Z 5 = 2\3 Bla g).i2/4 2 | [heel z } | |e) 3 a\2)32 cE et BE Bi|a/é 2/3 a eval al ela) ele | 2 | E 2) 2] | 2 Bs o/£/|alaie]} 5 settee ||) 2 lt capi a4 )e la ley eS) 2 la leia le | ee le Ween eel £ = ala SVE lel alaj2l|als (tle aes ha lg le le 212 lave le 4a) ee) 2 ia 2|4 le |2/2 a Fis Vee ETAL ELEIElElElSlelalelelelaleleley ale lalaielalelelt sig ielaielaieieiaié| : = — 3 |: = Eis 8/3 5 Zi3 |e I ch | q 2 5 | 2 gle = a i 3 4 EI | é|lg i 3 2|8 = Sie et Pe] lie} | a | 3 \ le pau | a} ai2|7 | 2/a 2/3) 8 Gye |4flelejaya PFla alae Se z = eae Lise [osl| | | a = 5 | = We] al eal eae ee a ea es =a eal a Tolar =I I = } i 2| ola lz | sli s e| 2| f BO | ease | pe | css | ee Dre z|2 z g/e | 2 J 2| el¢.\2 z| Sle_| 8] siz ayeleleleielalalalil EUW saben 2 |lesllee teed lean ealecates|loz 22 i es|_ce Fi 228 <2) 22) 53) cf l48 | 25)| oa a s | 2 = E E 2 | 8 EVM se UE 1 Et REP EAIEtEN | EL ed = | a= 28 Ale go lgeelgze ag |g £G2|22 2 jae |32| 22/28/22 |s4|22| & B)ej2)2/elalele/elaldlal2ie)aiala|ielie] 2 |ge) |S | ies gs|2 a> |e aeons 2] a | 22 | 82 5 | 33) \o— BE lERIEE fe = Be] g gigil¢gleilgieleleigielelels|2iele| es |S3|S2! 2 |£2|c/] ¢ lst iste 23| 2 39 [Esstes 2 | 2 28) 33 fg) 23 |e lad lag laa led led lec led lee & z pei ala i |) alga|/qalie)8i¢ia)é2)se|3e) 8 |28) 8 | 8 128 eee 23)" 28 >egiazg | 2] 2 |) Ss | go acd nd (ag|ag|ad ld led |ealedled| A/G E LR ETETELGILI ELA E/ ELI Ela la HIB) G/B i |i |2L Bech EE ai casege) 2/8 | 8 | ec | 82| “5 z Se | z| 2 z| zi i £ i é ¢ é ids & | ee | £2) 8 |eais2| £)8e| 2) s Eee Bla? ln? | | hea beast LA ie a) al SES lal SHS [is | Sareea Nissen tay [ere Ss Wailen | p )S SE | eS a ia) ieee A a ie ee Peale eo) al 2h = i ode a) a) 8 Ble |e |e) 8) eR) 8 | 2) 8) e12)e)2) 81 2) 2] 2 | | 2) 3) 2fa = | | ai = 4 = | He } I ojaja)ae!/a2};al/atoalelealala)a|"*ia)a/& o | 2 | A | a | a A + 5 8 8 li | a | 12 | 12 2) 16 3 32 6 a 9 12 16 20 20 | 32 6 i 12 12 16 22 23 py 25 80 30 36 36 37 40 | 9 10 tt 12 13 ot} 16 23) 86 | 9 LU 12 13 |8or9) 10 1s 16 18 22 —— Le P| = le | ae — eo om mo om) mm | om | mm | om.) mm | mm mm. mm, mm. |mm.|mm.| om.) mm.| mm. || mm. | mm. | mm. | mm. | mm . | mm. | mm. | mm. | mm. | {mm | om | mm.| mm.) mm. | mm.) mm. | mo. | mo. | mm, | mm. | mm, | mm. | mu, | mm. | mm, 956 1018 1230 1208 )1a2 143 | 1,387 1,916 1,362 1,645 1,694 11,210 1,901 | 1,188 | 1,643 | 1,684 | 1,572 |1,601 | 11431) 1,267 | 1,801 | 1,360 | 1,396 j2 1,867 | 1,716 | 1,677 1,609% 40 | 1437 | 1481 | 1,449 | 1,582, 1,650') 1.263% 1,218 | 1,390 127 || 1,218 | 1,341 | 1468 1,466% 1,688 | 1,584 = 953 1,089 | 1,102 | 1,046 | 1,058 1,100 1,366 1,384 944 1,039 | 970 | 1,867 | 1,284 | 1,808 | 1,800 884 | 1,003 | 1,045 | 1,077 | 1,121 11,873 | 1,408 | 1,867 | 1,911 1,092 | 1,168 | 1,212 | 1,174 | 1,278 v | 1,020. 980 | 1,105 | 1,187 963 | 1,064 1,183 | 1,180 1,297 | 1,293 = 517 604| 615) 571} 656| 601| 723| 767! 476| 544) s00| 743) 714] 658] 666 |] 469) 530] 57] 603) 638 | 287) 69 | 752) 705 ei2| 615] o77| 641| cov) — || 53a 490) 590| Gor |) 522] 5} Gos | 637] 710) ost | | I - 1,164 41,970 | 1,440 |1,893 | 1,446 | 1,393 |1,712 1,763 4,200 | 1,800 | 1,176 1,704 | 1,648 ) 1,644 /1,696 | 1,172 |1,208 /1,206 |1,368 | 1476 1,764 |1,818 |1,791 | 1,718 409 | 1,484 |1,580 |1,512 /1,688 | 1,628 | 1,280 |1,278 | 1,448 |1,428 | 1,288 | 1,408 | 1,647 |1,498 | 1,680 | 1,643 539 672 690} 690| 683} 698 | 728| S71 | 875 | 653 | 710) 631} 847) 842) B87) B61 638} 702 | 716) 760| 765 B41 | 902) 892) 865 717 | 822) 811) 798) 837] 825 693 | 666 | 736| 788 |) 664| 727{ 778] 769) 822) 810 257 | 268) 201) 266) 2068) 311) as7 | 05 268 | 281 | 267] 348| 826| 317] 332 || 253) 284 | 223) 986 | 312 365) 891) 410) 387 | 169) 17a | 108) 178} 175) 180) YL} A72) 179) 176) 188) 180) 14} 192) 192) 103| 201) 187] 181] 183) 200) 101] 198) azz a7] 170 | 176 | 170 175) 184| 189 | 142] 148 149 | 146) 149) 148) 148 |} 148) 151) 147) 168] 161) 161 164) 166) 160] 160] 168] 162) 166] 151, 11} 166) 14a] 40) 148 112] 161] 150) 156] 156! 160 | 92) 97) 4] 112) 110) 118] 109] 99} 105} 104) 109} 105] 108) 121) 191) 128) 191} 195) 129] 11] 120) 125) 120] 99] 106) 109| 106] 11s} 107] 110) 117) 120) 424) 131 | 122) 181) 187| 199) 185 |) 125) 127] 124] 198] 188) 134) 148) M4) 149) 152) 159/ 145] 140] 150] 152) 164 || 121| 196] 128) 120| 194] 184) 143] 140] 150 36 41| a] 44] 48] 47] 47]) 42] 45] 48| 48) 48] 48] G4) 63] Gi! co! co| c7| ce) o3| s6| 48]) 41] 44] 46| 45] 44| a6| 43] 40] 05 167 178 185 173 «176/ 178| 181) 178| 190 ai} 146 a2) 146/151] 100 145| 168] 164} 160] 166 #1 87 ot! 101) 100) 100) 100) 102) 107, 108) 116 us 419) 190-48 | eT 424 120) 196 | 331) 143) 142 2, 40) 35) 40) 41 40} 43) 46) 42) 46 a7) | a) s8) as | ao} #2) 35) a5] a0 45 20 Lepib-teradth des B44 ADS ATG BO ALB 467 KDA] O18 | 8B7| B09| HIG| HOO) H3G| HO, AGG| 627) He4| BO1| G22/ Bre! B60| 873 | a0 | e968) e99| e21| B64 s13/ 631| 796| GoH| 695) a52| 770| e49| 898 || Gow! aro| 627| so7| HL4| B67| Bs | 620 | A841 406 | 698 ga} ai] az| a4] 83) 86) 31j} 33) 81) 28] Bi) a5/ 86) 41) 88) 40) 49) 69) 40} 41) 48] 48} 41} a1] 50] ga] 32) 94) 838] 31) 37) 36) 840 | 857 | 871 | 860) 869 | 861 Facial index - - + NT Fl 700) 856 767 sya | 760) #17| 741) 610 73) 787) 742) 740) 770] 866 | 808) BIB) B07) 702) B27 | B30) Boe) 761) BOG) BIB) BLO) Ben | AED! B42) B11) O15 | S00] e22| 779) BLa| sii] a52| g22] 881) 799| 769/ 90] B00) 782) 742) 752 745) 782) Ble Saal iotez - «| HA) 0) 4a) 700 OS ro} s44| 761| #93 | 667| 702 | 875) 917, 756| o11| 773] 688| 746] 669] 788 | 660! 688) 70% | 720] 750) 750) 717) ™41| 700] 660} 702] 782| B11] 768 | 864) 756) 682] 799) m11| 779 | 717 | 721| 755] 679 829 | s20| 739) s60| 715 | 787 ieee - «| — #1 412) 431| 450| 459| aa | aga | 442 | 44a dda | eo) — | 394) a0 | 420] 45a| 452) 400/ 417] 411) 428 | 429] 439] 456] 458) 441] 450) 440) 434] 400] 499] 444] 417 | 405) 428] 495 | 622 | 455 | 457) 427) 457)| 442) 4] — | AL] 441] 406 | 483) 447) 487 Index of Seger-tesch i —_ 1000 | 90 947 1058 1072 | 969 |1020 |1024 |1044 1055 |1036 |) — | 992 |1000)| 988 | 1039 |1043 | 988 | 998 |/1028 | 1026 | 99-7 | 101-3 | 10-4 | 1076 | 106-0 | 1051 |107°6 | 1056 | 1087 | 1049 | 106:3 | 1057 | 106-6 | 106.4 |] 99-7 | 1040 | 1062 |105 | 103-1 | 1068 | L043 | 103-7 104-7 101°9 | 105:2 | 1052 | 1019 | 105-7 | 1040 Heder of hele, sitting. i 0 26 O| 23 ove! 496) 24| 5a5| ca) c18| saa) — | 560} s16| 90) 616) 683] 665] 688) coo) 657! 661 | O60) G47) 658) 629) 695) 528| G30 | O90) 627) 6o7| G24] G81) 587 || B56] G47 | oV5| 567] G71| 518| 550] G80] 531 |) 560) 698) 530 o 549) 543) 626) o10| oL7| o52 Aiter ch with cf stvresters. | 295 | v4 | 984) 214 | 208 217 | 191 | 224 | 290] 205] 284] 200] — | 32a ave | 24 | 212] 208)] 209] 208 292) 220) ars | aia) 228 | 227 22 | 295) 247] 230] 24-7] 297] 220] 227] 244 | 240|| 218 | 29-7| 228) 228 | 206) 290| 224] 230) 2097) 200) 218] 281) 318) 222) 29) aro) 236] 227) 227) 220 ————___—__ 1 ¥ Bon of Now. 11 and 25, ¥ Vather of No. 1. * ¥athior of half-bloods Nos, 1 and 8, * Mother of No. 1. * Son of Shuswap No. 16; brother of No. 8 “+ Daughter of Shuswap No, 16; sister of No, 1. I ON THE NORTH-WESTERN TRIBES OF CANADA, 529 Kwakiutl, so far as they are represented in my measurements, belong to one type, the tables reveal considerable differences among the subdivisions of the Ntlakya’pamug. Besides the groups named above, I subdivided the Uta’mk-t into two groups, that of Spuzzum and that of the villages higher up Fraser River. Unfortunately, in the limited time at my dis- _ posal, I was unable to obtain measurements of the Stlaga’yug of Fraser River and of the Cawa‘gamug of Nicola Valley. A study of the last- named group would be of interest on account of the admixture of Tinneh blood in this region. In the following pages the measurements and a few tables which show the principal results obtained by their means are given. It will be seen (pp. 530 and 531) that the statures of men and women of the different tribes are nearly arranged in the same order, differences ap- pearing only in cases where the number of observations is very small. I have given the averages of the various series, not because I consider the averages as the typical values of the tribes, but because they give a con- venient index for purposes of comparison. The table shows a gradual decrease in stature as we go southward along the coast from Alaska to Fraser River. In the series for men the stature decreases from 173 cm. among the Tlingit to 169 cm. among the Haida and Tsimshian ; while the Nass River tribes, who live farther inland, and who are probably mixed with Tinneh tribes of the interior, are only 167 cm. tall, the Tinneh of the interior being in their turn only 164 cm. tall. As we proceed southward, the stature decreases to 166 cm. among the Bilqula, 164 among the Kwakiutl, 162 in the Delta of Fraser River, and reaches its minimum of 158 cm. on the shores of Harrison Lake. As we go southward, the stature increases again, but its distribution becomes very irregular. The Salish tribes of Puget Sound and the Yakonan, Tinneh, and other tribes of Oregon have a stature of 165 cm. It seems that the Clallam and Nanaimo represent a taller people, but I am not quite certain of this, as some of the taller half-breeds may have been included in these series. On Columbia River the Chinook, who extend from Dalles to the coast, represent a taller type of a stature of 169 cm., which may be con- sidered as a continuation of the tall Sahaptin type, which has a stature of 170 cm. South of the Oregonian Tinneh the stature increases slightly, reaching 168 cm. among the Klamath, and sinking again to 166 among the Hoopa. The tribes of California, who lived north of San Francisco, and who are gathered on the Round Valley Reservation, near Cape Mendocino, represent a very short-type of 162 em. only, which is also distinguished by its elongated head. When we consider the stature of the inland tribes, we may say that the stature decreases north and south from Columbia River. The Sahaptin, a people of a stature of 170 cm., represent the tallest type ; northward we find the Spokane and Okanagan 168 em. tall, the Shuswap of South Thompson River of the same stature, while those of North Thompson River measure 167 cm. only. The Chil- cotin measure only 164 cm. Along Columbia River the tall stature extends to the sea. . In the part of Oregon east of the Cascade Range, and in western Nevada, we find statures of 168 em., while the Shoshone tribes of Idaho and Utah measure 166 em. only. I have added to these tribes the Eskimo of Alaska and those of Labrador. It will be seen that, while the latter are exceedingly short 1895. MM REPORT—1895, Ee ga eal a dl pa ae i i ee AVYG pus UoyOg TZT]| T-99T }—| 1 | 1 |}/—)\—) 8) T| 8] 9) St, St A FL) St) & | CEA bo ee a oa tn 3 oq puv ouoysoyg gouel | -Mery pus youqueperg 89 | 8.89T |—;—}T)—|T|/—|8]$)]6]It)/8 |sl)9 |F IT | F) TT); | tia) 7 + Bpraoyy ‘ant qnuseyD 0g | 8-T9t |—|—|—;—j—|—I—| TI TIL ss |—|9 19 |F cls | 85) | ea AaT[eA puny 4PTF -Buery pus yoouow og T99E pt a Ss | Slee SS Ss te LS) Diath S| — |S eS * edoozT yomouoy 0s | GLIT |—;—|—|—!|Ti—}T|F) 8/8 |F |S |S |e |T |} E/T). Se Me ag ee 2 YUU SOUOIMET ee OOS SOT be ee he | SS) EF 69 Re BY IGE be | Sie ie WOLaIO JO FSBO!) Tesutuat | | -ojg pus yomouow TL | L69T |—|—|—|/—|—]| 8/9] 6] 8/IT|IL}9 |IT)F |— Fe (Sal | eh oe ‘8 ugderrg seog pus {Ion.O 6 | Lé69t |—);—|—|—);—|T/8|e/T]o \F |S |T |t iT |G lige sa aa he , yoourgo stog pus doyone A 66 S790 ls el aos SLB MS 919 KOLMSLILE 8 FT) AL RCT ol) St | = yjareume te “pg qoang doysne\ pus uaorg gt | 7-691 |—/—|—|Tj—| EI} T | Ti=|s 18 It 18 |—|8 | |T ITI TI TI TIT. SUSIO Pee eto FANE BT JO 2801 Ps) Sle ale Eo) EE LT ee Doe fe ot | Eek pay Tt |S SHeRURS, eouoIMUT] pus 190T) 69 | L-89L |—|/—|—|/—\—|—| 4} F) 8 |stl/Orj sti |F JL || Bl—\—|—j_ I Y * " * uesvuUryO gem To | e991 |—|—|—|—|—|8|s,e/9\¢ {¢ |6 19 |9 |e | T|—| 8} S)/—|—I—|—)¢ 2" aeasnts orenTON 478M ‘e0ry ‘svog SF 6-291 | —|—|—;—),—|T|3] 8] %/T |9TI/9 |F% 1B 1G Tet te SS et : * sdoopurey ‘dvasnyg svog ST PE) el eT pf Pf A Pe ol al (Cc a 0 a Ble Sa \zé * OnNUIaU, 10J Ue NT Joon pas svog 77 | L291 |—|—|—!—|—|—|—|—|T|F {8 [8 [9 Je |f§ |8( sl FI Te) |i lee ‘a0, onummedeAyeyy N BMOT GL |= GOT ts) = | — ae ee to) oe a ee ee | ee Ey : bes sarorea Jeorn pus Seog Zo | $.09f | —|—|—|—|—|—|—|—|T|—|—]8 |§ |* |8 bee eee A ee ‘ ® wuzzndg svog IT O89 eS ah elie eee | me ee =| S+) E | eel [eet | 5 y ayer] UOSLAe Jeary pue svog og | 8-19 |—|—|—|—|—|—|—|—|/—|—|t |e 18 19 |4 | EI} LT] Ei|s) EIT El): + JOAN cosvay JO VILOC svog OF WEP OM th ee ia |i eee ras ena YF (flee N egestas 5 . Ue yy SHOR OG [2 G99T al =| — as VS leh RA Pe eee Pal ya at : 2 epnbyrg umorg 62 | $:69T |—|—|—|—|—| E|T/9/s8]/s |3 1% 18 |S |—|—|— | TI] I TI TIT : ; * URIYSUUSy, svog 0G OLE ae I ee SS SS SEIS ESS Sle Se i ‘ : erp aT IOAN SSUN, uamorg g¢ | G.69T |—|/—| 1) 1T}T)E)1/%)¢/8 |¢ fe }s |s j—|—-|—] PIT) IT] os 4" Spray uMoIg ‘gsnery ‘uosyotpucy Gt | O-GLT |—|—|—| @] TE} t/—|8|e|—l% |—|% |—|-iS IT ITI TI bo Seabee” SUSU: — +78) 9995 |—|—|—|/—|—|—|—| e|—-|F [2 19-18 |% |9 | Eye — "+s BYsBpTY JO OWMLSH zeBrequaog 93 | g.Lgt |—|—|—|—|—|—|—|—|—|—|—|8 |r 1s | |} 8)S}%)9\|—}—|—|—| °° sopeaqury Jo ommysat : | pegs 2) soSvr [ggTiLST\SST SST\IST SLL LLTSLTSLI TAT 691 LOT SIT SOT LOL 6ST LET SST Sst TST OPT LPL SPT © + 6 8 8 mg O53) Jed CAEN -2AV |ST\9ST|FST/G8T OSTISLT 9LT\FLT SLT OLT ees aca 8ST 9ST/FSTGST OST SFL OFT FFT | ee Se | ae ee a a a a SI SS AAI eA a i Se eee Se ysnog syfiong oyz fo seqi4y, fo vuayy fo aunjnjg 931 ON THE NORTH-WESTERN TRIBES OF CANADA. | uoqjog pus avery 08 6 29Ne fea = | | youqueperg FE | 0.SST aes == qyuussy Os I ail Te Ea qpleysuery AT | 6.S99T | — | —}|— | — HomouoH] $B | L6St | — | — | — | — svog pus souormey 9, | g.Fet | — | — | — | — seog ‘sn3itM \owouoyy ‘Tesurmo0ysg 9¢ | F.LeT | — | — | — | — svog pus Yorouoyy 2 GCIs lee — | eae a doysnem Gh | O.Fet | — | — | — | — uMoIg puv doysneM OL | F.9er | — | — | — | — Ped Leg BG ee) sets stog ; frad14 ‘eOUeTMETT GE G.9SsT | —|—|]—|— HYEM 83 CES Tee |e eS SBOoq PUv 190TH 0S PCIE ees ol ee [| svog ZL) LLST |— | —}|—|— svog pue io01y FL] 0.66. | — | —| — |] — svoq LT ree coo St See te | a sBog pus A904) cL L.GSTt —— — _ _ seogg | 6.08T | —|—|—|— W901) ZS | O-TST | — | — | —- |] — svoq 9& LENG Soa pel eel ee Ua svog 9 S990 | a Se | uMoIg ST | F.8ST | — )} —}—/]— BUC Sis! SS-FS0- |. =a. I | uMOLA 8 SLC tas) a | uosyopuer ¢ 0:9. Teo nee lt — 9% Lok SS [| qes1equiog 9f | O.8FLT | — | — | —}] — SI9AIOSqO sesvr | 6LT| LLT| SLT | SLT *S9SB\) JO JoquInN “OAV | SLT | 9LT| PLT | SLT TLT|69T OLT|S9T LOT 99T g9T S9T POT BOT [wo [~ | Or Oro aoe oye Em | awtl{[aflanco| | laataawt Hare [AM |ACAN | Hnaoaco~ TOT|6ST O9T 8ST {hesitate A Hino © di LST 9ST SrAnkews HOA A eH oD ~eoio nr rc oO MI b= 19 29 maaona nm rc MMM Ee OHAN IN MOO HAS He ~s ODP AGUA Had SH | 4 60 | A ciclcl | [Ewa aAeS [aaa iri ord | iets al[ | lal |[eannno [ran co | [ula a 21.) pues suoysoys . . . . . . ‘BpBAdy ‘eng AoT[VA punoy C * edooyyT : Ree Di U0SaIQ JO ySvOH * uydeyes * yoouryy qoreumyd “yeyxey “ps yosng WLIO puws weyoyraoy onured - PAYBIN . —— - * TOuULy, * wesvueyo demsnyg w1ey310 Ny sdoopuvy ‘deasnyg - 3 ONUIAU,10Z ULB NT 0 onurede Axe yy N F-3UL 290) * — umzzndg oye] UOsTIe yy * TOATY Taser JO Vqjoq * qMyeLyy ‘+ embirg * -WRIYSUIST, SUVIPUT TOATYT S88 * eprey ‘ * gary, ‘ wyseV JO OUNTYSHT IopRiqery Jo ow1ysa SSTISST|TST PST\SSTOST 6FT 8FT LOTSFL OFT|FFL T#T OFT ysn0y oyfrong oy2 fo saqruy, fo uamwoy fo aunjgnjy L&T \98T Mm 2 532 REPORT——1895. the stature of those of Alaska equals that of the Bilqula, reaching 166 cm. The measurements of the Alaskan Eskimo prove clearly that they are mixed to a considerable extent with Tinneh blood. I think the points of particular interest brought out by this statement are the gradual change of stature in British Columbia and the great irregularity of distribution in the southern: regions. There are no differ- ences of food supply or mode of life of the people which would have the effect that the stature should be lowest on Lower Fraser River, and in- crease in both directions along the coast, or that the same decrease should be found as we descend Fraser River. It seems that these phenomena can be explained only by a slow permeation of the tall tribes of the north and of the short tribes of Fraser River. It is curious to note that the distribution of stature shows regular changes, while all other features are distributed in quite a different manner, as will appear later on. It is of some interest to compare the stature of men and women. When we consider the tribes contained in the preceding list, we find the following result :— Stature of men Average stature of men Stature Pe Phi 28 bidicas | mm. mm. 1575-1627 1605 94:2 1637-1660 1650 94-4 1661-1681 1671 93°1 1683-1697 1692 92:7 The proportionate difference between the stature of men and women is the less the smaller the people. The same result appears from a study of the Indians of the whole of North America, as is shown in the following table :— Stature of women in per cent. Stature of men Average stature of men ot thatiomm an mm. mm. 1660 and less 1637 93°6 1660-1699 1684 92°9 1700 and more 1712 92:7 While for the middle group the values are almost the same as those found on the Pacific coast, the women of the short tribes of the Pacific coast seem to be taller than those of the short tribes of other regions. Before discussing the types found on the Pacific coast any further I shall give tabulations showing the principal results of the measurements. The proportions of the body are computed in such a manner that the stature is taken at the nearest centimetre, and divided in the other measurements. | ar 533 OF CANADA. TRIBES ON THE NORTH-WESTERN Fp ee Sate IE ER EI pe oh | OT ils &€ 61 g ae 8 Té sasep jo Joquinyy soseg jo 1aquinyy OSBIOAY 6-88T 8-I6T 6-881 6-98T L-98T L-98T 0-€8T §-16T $-S6T asRIOAy ao | AANA HARTA MMNAN mn | |manea lHaAaNdtaARn of | [aan | nl[alars | IT § & IT | Ja lanman I T * YouULy, WeIuoSeIQ onwaU,1OJ Mey Ny "9; o,onuredesye[yN q-40029) tanzzndg aye'y Uosueyy [OTe SUBIPUY 1A sseN bod L6T 96T G6T F6T S61 G61 I6T O6T 68T 88T L8T 98T 98T *81 €8T | 181 681 | O8T 6LT BLT LLI 9LT ‘wamoyy fo poazy fo ysbuarT 1 ~ nl bLT SLT SLT 69T 89T | . - TOY, T T I rd T 6 € wmeanaAlaAlA 106 006 661 | L6T 86T | 961 g6T F61 ast | a | om | co eocn | oD co oo €6T | T6T G6T | O6T al Ana ornn ‘way fo poazy fo ysbuaT Jwandaa | an * qouury, uvIuose19, demsnyg Onwmgu,10puIeyN a) 2 oumedesyeyy N YALL wauzzndg * aye] wost1eyy } * eabiig SULIPUY IOATY sseN £ 89qnaT, €8T 68T CIAL 1895. REPORT 584 "199TH “JW ‘(Sesvo OE) T-99T z “19014 ‘WW ‘(S88 8g) 0-Z9T 1 OL L-6F1 | eed |e I T T = z a § = —— —— “qouuny uelM0saIQ, 2¥ 8-FST oa a aa T rr 6 3 at FF TF T aa Wi = : demsnyg 9T O-LFT a | epieAlendy | Wi ar iz, 6 T a 6 F 6 aE * OnUIgU,1o}UIeyN facts L-L¥T =F = = = I 9 € 8 8 g S Z "8 oSnuvdesyeyyN 61 GIST eal ome dea T & I F if I F I a an ‘ 9-29) g 8-IST =m eee |e es = I g aa = T = — = : : tmnzzndg a 6-€9T a I S I = a g I = T a az * exer] WosTAe yy L §-F9T el eee a iF a if a 6 a = ie = a x * [gMTyBAs yy 16 9-691 =a neil 4 G 9 F af € IT IT 6 = = SUBIPUT IOATY SSBeN £9QUhT Sasep oSereay | S9T|S9T) TOT | GSE | LET | Set | eg | TST | GPE | LET | SPL | SPT | THT i ‘ : - Uy JO JoquIn NY F9L|G9L) O9T | BSL | OSL | FST | GST | OST | SFL | OFL | FRE | GFL | OFT ‘wamoy, fo poapyy fo yipoang “T90IN ‘W ‘(Sesvd 6E) 9-891 « “1901 ‘W “(seseo 18) 6-99T 1 61 0-891 Pea || ar x fa | a? | (a We oe No & G T ¥ T = a * qouUry, uelUosaIQ 201 L-09T Fre Neer ease ele aleMea nels slnale tligSr lamer g il 7 ms aa = : deasnyg IG 9-491 Didlees loneilsne lone iitar sels ee € G I i 9 T = * dnmau,toyurey N 196 L-€ST ed eee a dl On en, tee g 8 ve g F j 2,0, onuede Aye N 81 6-891 oe | a ape ea | aaah | eS a Ns 7 G ¥ G ze SG = ze : ; 4. UT,27 0) a 1-681 See (ede ea ee Tl a z € = I = aaa " * wanzzndg 91 G-P9T IT Goals leo aw IE, alee Nea. a: me 6 rei = = — © aye] uostaIeyy a 1-891 ete ee weed ae a al ee He 9 T 3 T I 5a a A kd G6 ¢-T9L he or ie Aa ¥ F g g F € mame = T =< = SUVIPUT IOATY sseNy TAA A sose) oSvroay GLT| S21} TLT| 691} 291) G99T|E9L}T9T) 6ST | 2Z9T | SST | Sot | TST | GFL | LFT } ; ( *-UNTY Jo coquunN PLL] SLL} OLT| 891/991; F9T|S9T)O9T|) SST | 9ST | FEL | SST | OST | BFL | OFT : ‘way Jo poazy fo yypoorg 5385 ON THE NORTH-WESTERN TRIBES OF CANADA. 6 L-STI sl | ss ep a Def =m el lame) Of el) S| Sy ta i fc a Fp) oa eeienetgy eheinetorsiay go: fel 9-FIT =|] —| —) — | — | — | =] — T}/3/6/1)/6)¢}] t)}—i—|/—|—|—|—] —| ° dnmmoromegy 63 G-ZIT TIA ITS lat HI el 8 1 e] et) 9) 81] el] Li] ti—| —| + 200nmedetyepn LI LSI S| a | SS | Gel S| Z {| TT) 8] Ss) tie ee 4-024) & 0-€1T ae | pe eee Ps a eS SFR lS ET taal pea lel . wanzzndg a €-60T —|—|—|—|— = TiS | Oe ee) S| DSi] — | | 2) 8 exam aos Lg 8-121 Ty] 08 PS 6 TR eae ae | PBT Dele | Sa el ee tan nee 9 CC Sala Mr ol) gel a irl pe i 4 9 Pc a st | eM mem ae Fe et) * Bub 6I PSI [||| |S l SIH] Ul ty eye) })] it) ))] oy) ¢|/—|—l—l—]| —] suerpuy seany sseny 2 Ques, sasep oSeivay |SET/LET SET SET TEI 6ST/LOTSST/ESI|IZI/6TL LTT SIT SIT TIT60T LOLOL SOT|I0T| 66/26) 96|). « . apy JO JaquinN SELIMET/FELISET/OSTISSLISLIFSLSST/OSI/STLOLLFIIIZLLOLL/S0T 901 FOTZOT00T/ 86 | 96| #6 f ‘uauoy, fo song fo yy brazy 0% $931 ST | SLPS SG LSP Neh Se | LPs deg ap | et — | —- oe” aeddi ys, UurosorG 8 9-F3L 1 VT t= 1 Beetles tte “Gry nas Nl ean |) Sey le fn ee iene cee nO OL 0-831 ed Hel [el Femelle (ee Fe) (| pe Pen te : deasnyg ST 9-131 Tet Vem | Ret pek |.oBe |! are] weer) ME) Set) cea) SE) eee) See aeee| 1) Sen Sek Gna tog, SI ¥-G1T TITITIThET IT] me] ty) e ] ee] 9] ee] ee] em] Tp | HH | =H] + 20 dnmededyeian rae Pavan Sel | san Wega NL | ml | mel | feces) de S| RR SD ps ve SA) ee el] MO 4-yUr 24) €I L611 ae Egle al Nh line rc Nr le | | tanzzndg IL ¢ SIL VICE ea a ae Se Se Se a te) SO “ee G F-931 ee a ee a Se ae ee ¢F T-681 SIH STF) FL 91 ee) Ee) So) Bl elope le al — lH = CO ee ira 6-LZI —|G@i[—|T]@]/ 6) 9) 8) L)e)e@)1—| bt) ¢l]—/—l—/—|—] * °) mS embag 03 G-0Z1 |e Re BL Be Bo Se sump senreean aque sasep oSvray IPI Ger Let GET/EST | TST | GSI | LOL | SSL} SS | ISL |GIL| LIL) GIL} SIt| TIT |60t]/20T;/Gor;\. . . . UyY JO 1oquINN, OFTSEL 9ETFEL EL | OFT | SEL] 9ZL| FEL | SBT | OSL | SIT | 9IT| FIT | SIT | OLE | SOT | 90T| FOL | J ; uagy fo aang fo sy bor REPORT—1895. 536 RI IIODIEED IIE IEEE es ‘19049 "WW ‘(sasvo 29) F.8eT + Or L-8&1 re ee Sa (a SSF SU eset I @€/—-}¢s/—-]ti—l— Youuly, uermosar (og) (9-61) a | TS SRR | an fete || Meee gr Drea mc ee a“ _ Saaatue I9a1r) 91 9-LET Teds TEC eT hele Te Sey eST WEP (S-[OGr ease He. PR [Se lod eee LSE) Onoree cope 166 8-981 Frakpyestereelt wee) eet ser Ee eet ee Vee Br ee | Lita eee Ses er 9,9, onoedysyeyy N 61 6-681 ea care | ice oN (ene Nm mere Fi - | - i | hS | ee " 4.qU0,290, g 9-PPL ee he | ll Wa es | | Te Sole == cael) : tanzzndg g _0-S9T T= wis oom (eee e IT ae a A Spe Ae US eae | oe * punog yosng al §-0FT ete | pe a a ee ee a ea ee a ee Se a enacekan 1G 2 L&Pl a I — ta G ts Sig) & 9 ¥ T a D1), emer linea | aoe 2 z TADIyVA 9 LOFT 4 se Pe mm ce | ee ce eae 16 GSP =, oe oats | I SS ae ey aS at T ise ip I |}—/|]—|=—| =| suermpuy zeanyz ssen “ £ 8aqQuey sOSt) aSexoay | S9T | LOT | 9S | SSL | IST | GFT] 2FT | OFT | ebT| FT| GET | LET | GET | eeI | TET | 62T | Lat |. forenyny delay jo zequinyy BST | 9ST | FOL | ZOE | OMT | SFT] OFT FFL ShT| OFT | SEL | 9ET | FEL | SET | OT | BzT | 9T Sa ‘uawuog fo ang fo yypoang ‘yorrouoyy ‘Iq ‘(sasvo F£) £-09T + ‘Taery) "W ‘(Sa8vo Bg) E.09T ¢ “I9OLN ‘W ‘(saseo Tf) L-SOFT « ‘Ta0IH ‘WW ‘(sesvo gg) 0-TST 1 al got f= |= 1—|— tall ba [tte | et eel ee cto 03 0-9F1 ull s Hal Seales Cee eller Cl se € F Te os —_ g Z I T youury, UVIUOSIIO +6 GIS S|] Tierra AE Tyrie ome eg) at ae * uydeyeg 2 OL G-6FL cael a aaa ee (cman (iats| iu beara ies G T G cm eo — T =o = 2 ‘ deasnyg 1Z LI ST eral Se | en pet aaa Ge rlosee ei q | F POI LOg T | — | — | * Snugu,toymeyN 29% 6-91 ICT See yeees Sey SSO thie 9 9 je ne ba if 0,0, nmedeaxrepN 8I L-S1 Se A Fate fe | li oR, a a, Br hh Sm yf a as * 4.30290 1 LSP er Oe salle eee PL fn Kc || 7 id eg eee Piety) eK me y 0-F91 Se ieee ea Nek ON Se | gL aN ee TE | ef | | | oo aren iL 6-691 Be rel ST) see pa | rth PT Sell co ne | eg | er ee TISeVl yy jO eyed ST G-19T Bad reall nd ease ta | Bite | al i ese] <8 pet xe LT | — | — | * 9yey uostaeH OF F-0ST Sasol cecal gp id Pee Pe Peel i L Gy EG) On eel t= I CLLS/ 2.0: | ¥ F251 aera ce po le ea ary eel al ie eg |e ie Tae pele eee) ar fe ¢-991 Bee: i at ie a8, eps eae aT @ le6s| >| we) S| | Baepoaenrg see $89QULT, sasuy) aBvroay [491/991 S9T/T9T | G91] 291 | SOT} E91 | TST | GFE | LOT | SFL | SFL | THT | Ger | LET i — jo JoquinN 99T|F9T Z9L|O9T| 821/991] FST] SST | OST | SFI | OFT | FFI | SFI | OFT | SET | 9EI m ‘wary fo aong fo yypooug ti = eed 6 Ah Zi 0 Fev Fa fe matt al al) LEST Gisela Th Ped ma a etl * ONUIAU,10, ey NT 61 G-GF Fe amet a a ee mad eda tae LT MST ere ICSI li lb le 0,0, onmedy dary Nn 66 ¥-LT a ie enfield ae ee LY MENS eet af lc : ‘4.3700, 249 ¥ o.LP 1 Se Ss ry ch i * wnzzndg Or t-6F se | fast eid AT cca lagen ES NS Kae TEEN PRD es fle * eyVy woswieyy 9¢ 8-19 ee De ms en 4 WA mf Scale flee ao cel fi 9 8-49 SF FI] 8 tb] 0) thle |-I ites ebytg a GI 3-9 TIFF IFFT IR Ii III] 1/313) t |) sleiglsijtj—ij-l tii] *. suerpuy saary sseyy z a A Oma (NO Oe PY RC St SF ed i Sb a 2p fe DPR | a eae Has o jo sein XN aBVIOAV 99 G9|F9'S9 Z9|T9109 69 /BG|Lg19¢ ¢| FSlEgizg TelOG|6F SF LF FoF FEET FIP OF|6E8E LE 9S ce . wy i e Q ‘uauos, fo asoxr fo qyhrazy | - 4 H Z a=] | & mM isu zi { = 61 0-99 Ep ee el Be a al oe ee) Ble ee eee 20] OL 9.9g Se dee tee ie Ge es a gee Sel coor eee fet | EC BI GT 6-29 SS | SI oe i a Ie ha cee Tie asl es erg les es fe) 8I G.8g see \ aac) ail ae ie haa ae lNeoell eran tere Papal: Gholi ges || he 2,0, onuedesyepN a ra 3-89 soot (emma SN (hum cham | Usman sal ‘ath ful “ng ed SP Sel Pe ey MPa CS Sa oy a él 6-89 SS SSS Sara ale a ee ee ee EB II 8-29 SS | ety ee a (ca (2 Ramee acl Ll Mell eel ms ' &F L-9¢ Fae dei Re ie ee PHO OTE Ty pl ae on aa neg ma are ree ae 3 G LLg Be |B ee Beh RS ies Ee BEN Be ae eR a ee en 5 ES res 02 8-05 fet he ES AL, et SF El Sa) So. 9) eh) Pig eS Samii, soar eel) e8uiaay | 49 | 9 | 29 | 19 | 09 | 69 |89| 29 |99| eo | 9 Jeg] oo | 19) 09) cel er lapis. ° °° my jo raquny ‘wapy fo asoyr fo qy bray REPORT—1895. 538 9% reg = |—|—|—|—-|—-|-|— —lelrtititieislale|siziti— t|— fee deasngg oF g-38 | ai] Vl eel | aml Waal Vs ie |” kal half Ne ell a ik SA * ONUIAU,1oyUIeyN 98 9-€8 —|—|T/—|—|+} 3%] ths} @) 99} often] sz/ Fi 2)o]/9]F |r )—]* 2edneededqepy 19 §-98 Se) op ear he | Geel 8 bee CaS | ete | Bal aad eee a 6T ¢-€8 SS fat Fal Cl ce ar ae ee eal en Sie sealleg eal eC ae EE ‘© “tanzzndg the 1-88 Three Lad ph eh | Bal Sede Fabs Bape | ea Rl oli ee ei ea * oYv'T UOsreyy gg 0-18 Teh De Sa Re PO BR Bell Pet ela ee re eel ee | aera ST ee Oeil 16 8-€8 in he Tet ele Gel pe Ton hr | ec | Deeg eDery Tau ese aL 6& F-48 Sl | (| Sastry pa tem fa Ch (Stel aan hl Ch st ig) i ete i el be F : vnbrg SL G-€8 Se eee Se Se | SES PIES eh Senet) Fell S-|=S = |<)" SUeMDUTe AT See IN: aSvi0Ay @8|}18|08|6L\g2| 22) 92) 92 "pe as "sarlag’ 1010, “xapuy yypne.rq-yjbuaT GI 1-98 = = & G iF T 6 T 6 =o slope cae eee * ONMUIAU/LOJUTB YN 6 L-FS ra ees T Ta 3 g g 9 3 S° alee ss 2,0, onuedudyean LT 0-9§ =H ae 6 = iz § I I 9 g (Spats ee ; * 4-UT/290 P &-8E T oS T = = = T T a eo hee — i a : * uimzzndg or 9-98 = te a I l Be T if (4 rin ee aol ae eae a * oye] wosteH 9§ GSE er a a t § g j IL G & G & Tamali ‘ TARA 9 8-FE —— — —- T = == G a a 6 IE ara Oi [A on” : . epnbiig 61 9:9§ = T i § F Se g — | 7G — | — | — |} °* suvtpuy roan sseny } | = Tt | & eee asvIoAy oF Tr | OF 6& 8& LE 96 GE FE |. GS 8e' | TR) Ose |= : : ‘ TIT ‘wawoy fo asoyy fo Yrpunang or 8-0F Se he oe Wi a eA we a Ol? | It 1¢ B= Vie ee a ee . * deasnyg + f 0-88 | A ate | ee | mang | Ft (Aa eel i 7 IT € A oe BR ae Ss * ONUITU, OyUMIVY NT LI sze | —|—|—|—|a—|—}eirilt)eded1 | B he Be el ape et 9,o,ouuedesyep Ny at 8-88 Bhar ea Ee NS thd ch Bt ae) of oferta 7 8 4.qUZ90 &1 8-6& FP sta ero cg A Late BP a ee Te Be ER I ee ee a * umzzndg ee que | —|—|—|—|—j—fel—ltalate)el—|}aets | —y-e}— * ayer] uosuaey | g 9-0F Ta aac am | lb cal ell eee pee heen I }—}—!] — | — | — | — |-° 4e0a4Ty sosery Jo vqjoq GF 6-66 S| fsa es) | em Wt fs TSP en) Cal 2 Ec ee oo Ce eee el a © [MEywAy 3 1-8 Lh Lr go at a] aba Ot ee |.” oe omega 06 1-0F 4 oes | | Soe | me emer FI yr |-8 I € 6 a I = | — |-— |.* sierpul toaTy ssen Jo aedathiy aseroay | SF | LF | OF | Sh | th | S&F | SF | IF | OF | GE | 8E | LE | 96 | VE | FE | S& | c& | ° ; IT ‘uapy fo asony fo yipoang > 4 Or €-€8 St (Bm ram | lf Ry € Te a tem treromery a &-F8 Mi bak ae ee oll meets iv T ra 4 ae I Te es he * OuuITU,LoyUTey NV 66 8-18 Saal cae War alt lee Pah ee! Ne rat] 5S g L € 6 | —~ |} — |] —!] — | * 0,0onuedysyepy LI 6-08 Iege (beeng ene (gee | 100 dt 8 A, En Se ee F 8-LL aaa Geers Gas SHE eet | coe | ae ce lt ee IT qT IT * T S| Sa (a : : umnzzndg 6 ¥-8L 3 | i eel a |e Lal oe & e G (CP sara il si, ol ' OYV'T Use xy fei pe Rallye area yy ¥G £-9F Tol ae ek th Bleed ealbee: wl £0 al Galle Vicente Ole oct a a an ee cc eT 61 PSF By | ST Ee a Se) a ae re ee ae a ree | Sep ce | $SIQULT, sesey aSeiaay | P84) 6-27, Flt 6-9F| F-9F| 6-9F| F-9F| 6-FF] F-FF| 6-EF| F-F 6-BF| F-Sh| 6-1F, F-1F| 6-OF F-OF| 6-68, 09] , 41190 19 | Jo taquinN 0:84] 9-LF] 0-LF) -94| 0-9F] 9-SF| 0-94] 9-FF] O-FF] G-EF] O-SF] S-BF| 0-BF 9-13 0-1F | 9-0F| 0-0F| ¢-6¢| Taorg J d ‘vary fo wiy fo ypbuaT fo wapu, 1895. REPORT 542 — == So ee ee ee et | | ee rrr, cre OS OIG) cae T:29 9} —| yee Sell Se lee lS es ee Bl Se ek Sale Eee gh Ba) pe] i Dam Tope 8 Leg f={ —| | —} | mp ahaa hr] oe] 9] 3] 9) ¢] 2e¢] ¢] 3] —| —| —| *2,0,dnuededqepy pa SST TO es My Vee | Weel Eats Esme A cal Seb lL: a eS Sc Sl Ss a ese Se I Sa ale P G.1g —/| —}; —| —}| —| —| — | oO | — | — (lh SS SB a | SS) a e 4 tanzzndg 8 EG aleee|: eth ee eel Sel Se Sl) ak oD eG etek ae pee ie oer €¢ og ee af eeal, a lore Le inlet lle ee le Sal aoa ee Ely eal eal le tt ae a ee 9 po ares |e mee ee le ol | 8 he oe ee el SL ella boa tse co LI iGO ae | ele — lel Te ah el we [Ge Stl cod eS ie i ea) SURI aeons 1 Qe], | | S988) | aBer9ay|6-09)/F-69)6-89 F-89|6-L9/F-29/6-99| F-99/6.¢ F-89.6-19 F-F9 6-68 F-89 6-9 F-Z9 6-19|F-TS 6.08 F.08 6-6F'F-6F| Ol. ‘499 Jog Jo qaquinN 9-69|0-6S;9-89/0-89 9-29|0-29)9-99,0-95|9-2¢|0-99 9-49,0-F9/9-89 0-89 6-89 0.69 -T2|0-18 9.09 0.09'9-6410-64 WOdy j ‘wawos, fo burps qybrazy fo xapuy | | | | | | s 9T Tce | —|—!| t|/—!|—|—|—|—] 2 | Ch “Gslaccalemle | cpcisameie le ee ee * qouury, WeTU0s019, Or CO NS ee Nea ae Pe ee PES AO ARE A: a eet DG eh PFS SLE at ST 0:69 hye loan oral) ar) are de 0 tele! Sled Sal Bt Fe bibale’ jee he Ge OnUIAT, toy UIE N 81 Tee | eles | ol! ech deers el ber leda sled verh 8 |: Steal 6 opty (Sk Te) *8,0.0nmedeGiepn 61 rcs CSP ie eee | ent) En ea fel ea JME SS es SS | Me |e a | SA NR Ws a (Rn ne | See 10720 &I CLEFT Sees ae Scale, ara eg ellie. rae secs ok ee) | ceed a a CA a * — wnzandg Or Ge eee se | ae ee ee ee eee Ee Se ae aye] WosTeyy 98 PsA ees ea ee am Ol Rs PG St ag ae a Wee ge ot og a I * UPR iia Omg teen gee | | eee a ee Gaal owe toe TE | tol ton "+ emnbrtg 03 geal) eset) ae Sa ae eae Ge Gel oe te te Ee ee |e | LEA A 8288) | aSeroay|6-65|F-69/6-89/F-89/6-L91F-L9)6-92]F-99/6-99 F-2916-F9)F-F9 6-€9 F-€9 6.09) 7-29)6-19) F-T9 | 6-09 | F-09 | 6-6F ol. 4190 10g JO Jaquinyy G-65}0-69|9-86|0-89)9-29/0-29)9-99/0-94|9-99)0-29/¢-F9 0-F9)9-89 0-€9)2-29/0-69)9- TS] 0-TS | 2-09 | 0-09 | $-6F | Moxy ‘wary fo burgs gybrazy fo xapuy an) Si ee | 1D 6 Eel |. — = = aK | I G | T i ae | Te) ote} 2— |= | — | * qauunypoerosar9 61 L-€0L | a ar = —. & = fe | pel we | Se 8S et ee onwmauU,10FWUIey NE 86 Loot | i Se SPSS Sh ac F g 9 | DASA] 8° |= | Ft — | — | ° 2 odnoredgsyeny 91 eG of = Nok at ae eee eee Sar | oo | Se Saas ee ee ed no = oe a ii 8-TOT i ee. Pee i Peel Se Skt | a St Sa esters: ge oes]. : * umzzndg : 8 Crier ea a eee 3 [> ST Ti otjmim—joj}o—lm—i ala + ¢ eyed uosurey A gé 9-Z0T — Le i) 26 6 T 9 T 8 i) COP 6 ama ee el Hea | =| PN ae i * [ULTRA | “1536 1543 153-9 1548 Height of face __,, z =|)” elise 1218 109°3 — Breadth of face ,, : , | 1432 143°1 140°3 143°5 Height of nose 45-2 51:8 49-4 == Breadth of nose _,, ‘ : c | 36:6 35-2 35:5 Et Facial index . : : ; 786 84:8 78:4 = | Nasalindex . ; : : , 81:8 68°6 726 — 1 Total series. Tt will be noticed that the series of men and women agree very closely. The types expressed by these figures may be described as follows, The Nass River Indians are of medium stature. Their arms are relatively long, their bodies are short. The head is very large, particularly its trans- versal diameter. The same may be said of the face, the breadth of which may be called enormous, as it exceeds the average breadth of face of the North American Indian by 6mm. The height of the face is moderate ; therefore its form appears decidedly low. The nose is very low as com- pared with the height of the face, and at the same time broad. Its elevation ON THE NORTH-WESTERN TRIBES OF CANADA. 045 over the face is also very slight only. The bridge is generally concave, and very flat between the eyes. The Kwakiutl are somewhat shorter, their bodies are relatively longer, their arms and legs shorter than those of the first group. The dimensions of the head are very nearly the same, but the face shows a remarkably different type, which distinguishes it fundamentally from the faces of all the other groups. The breadth of the face exceeds only slightly the average breadth of face of the Indian, but its height is enormous. The same may be said of the nose, which is very high and relatively narrow. Its elevation is also very great. The nasal bones are strongly developed, and form a steep arch, their lower end rising high above the face. This causes a very strongly hooked nose to be found frequently among the Kwakiutl, while that type of nose is almost absent in all other parts of the Pacific coast. This feature is so strongly marked that individuals of this group may be recognised with a con- siderable degree of certainty by the form of the face and of the nose alone. It will be noticed that in this group the facial and the nasal indices of the women indicate that their faces are more leptoprosopic, their noses more leptorrhinic, than those of the men, while among almost all races the reverse is the case. This fact led me first to suspect that the artificial deformation which is more strongly developed among women might be the cause of the peculiar form of the face of this tribe. I have shown, however, in the preceding pages that the observations give no countenance to this theory. Besides this the Bilqula show the same features and the same relation between the two sexes, although the heads of the men are not deformed, and those of the women are deformed in a different manner. The measurements of Bilqula women can, however, claim no great weight, as they are too few in number. The Harrison Lake type has a very short stature. The head is ex- ceedingly short and broad, surpassing in this respect all other forms known toexist in North America, The face is not very wide, but very low, thus producing a chameprosopic form the proportions of which resemble those of the Nass River face, while its dimensions are much smaller. In this small face we find a nose which is absolutely higher than that of the Nass River Indian with his huge face. It is, at the same time, rather narrow. The lower portion of the face appears very small, as may be seen by subtracting the height of the nose from that of the face, which gives an approximate measure of the distance from septum to chin. The values of this measurement for the four types are 69, 73, 62, and 67 mm. respectively. The Shuswap represent a type which is found all over the interior of British Columbia, Idaho, Washington, and Oregon, so far as they are in- habited by Salishan and Sahaptin tribes. Their stature is approximately 168 cm. The head is shorter than that of the tribes of Northern British Columbia or of the Indians of the plains. The face has the average height of the Indian face, being higher than that of the Nass River Indians, but lower than that of the Kwakiutl. The nose is high and wide, and has the characteristic Indian form, which is rare in most parts of the coast. The facial and nasal indices are intermediate between those of the Kwakiutl and of the Nass River tribes. I marked together with the measurements of the Indians certain descriptive features. I give here a tabulation of these observations, but only those taken during the journey of 1894, as I find that it is very difficult to compare descriptive features on account of the large personal 1895. NN 546 REPORT—1895. equation of the observers, and even of the same observer at different times. The type which is being described exerts a deep influence upon the form’ of description. Thus when first visiting the Indians there is a tendency to describe the lips as thick because they are compared with those of the whites, while later on they are called moderate because Indian lips are compared among themselves. Descriptive features are, therefore, of no great value, owing to the inaccuracy of the terms involved. Still, some. striking differences will be noticed in the following tabulations of the de- seviptive features of men from 20 to 59 years of age :— } Bridge of Nose | Form of Nose | Point of Nose - ao — | Paes o)3e | 2 | eee eee SSB) eh) Be Ceuta aele ekee | Heats | i lee Silat Gy lomeubehe & | Nass River Indians a 8 ae 0 VP hi Jn PS a! I< Salle La ate P20) bP — 1) 9") 1) 2a 85) 6 ats ta'mk't Filey AUbie 1) fo pee MMUDS [ee eG CRATE eae A Ntlakyapamuq’o’e. : SUPABES 8 |) SO Tl) Bb) SRT YG! (S| be Ag Nkamtci/nEmuQ 13 2) — 2 8 4 7 8 6 9 | Ear Lobe of Ear | 2 i ? sc | Mo] | a ts ele fzeiela le) 2 Els 3 3 2 3 Ss | eS a a Ss _ | vo — | ade = < | =) sa | NassRiverIndians|12 | 6 | 2 | 14 | 6 | 13 | 6 [15 | 58 | Kewakint) Mi | i V7 5.174" 12 9 | 20 | 26 3 ta'mk: : mesh les" 2 6 6 | 10 2 | Ntlakyapamug’o’e | 5 | 11 | — 9 7 ge ie 2 | Nkamtci/nemug .| 4 8 3 7 6 oh ee 5 This tabulation makes particularly clear the difference in the form of nose found among the various tribes. I recorded the colour of the skin according to Radde’s standard colours, and selected the forehead for my comparisons. I recorded the following tints among the various tribes :— 32 33 l1mno im’ n © r Nass River Indians 1 — — — = i 21 — 8 q i 1 Kwakiutl —- — —— 1|— Zu gakianks & fread Uta'mk't — No tte ly Qe NtlakyapamugQ’6’e — 3» Ze 6 2e— 2, Nkamtci/nEmuQ —— 2 1— — — It appears from these data that the Kwakiutl are the lightest among the people of the North Pacific coast, while the Nass River and Thomp- son Indians are considerably darker. It is necessary to consider the cephalic index of the various tribes a little more closely, because it seems that among the tribes of Fraser River children are much more brachycephalic than adults. Investigations carried on by means of extensive material do not show any such differences, and ON THE NORTH-WESTERN TRIBES OF CANADA. 547 it is likely that more extended investigations would cause the apparent difference to disappear ; but it is also possible that in this region we may find the length of head to increase more rapidly than the breadth of head, Among the Eastern Indians, and in different parts of Europe, we find a slight decrease of the cephalic index with increasing age, but in no case does the difference exceed 1 per cent. We find also that the heads of women are somewhat shorter than those of men. The following tabu- lation shows that among the northern tribes the same relations prevail, but that among the Ntlakya’pamug the heads of adults appear much more elongated than those of children. Average Cephalic Index. a g s | ¢ | % 3 oa a 3 FI & 4 3 = 4 u A 8 = wt. H 5 g A = q 3 = a 5 S eee 2 g a g 3 a 5 ane a P oi ae 3 1 sS i) a jen s fa e & A A is) Boys .| 84:0(17) | 836 (8) | °85:5(6) | 90°8 (3) | 835 (1) | 86-3(13) 86°9(12) | 89°5 (1)) 84-0(17, Girls . | 83°5(11) _— 82°5(5) 87-1 (5) | — 88°5(12) | 84°7(14)) 87-8 (3) 84-4(10) Men . | 82°7(24) | 84:7(24) | 85°5(2) | 89°8(15) | 84°9(12) | 84:9(17) | 82°6(26)! 82-0(21)| 84-0(20)| Women. 82°9(2u) — 82°9(7) | 87°5(12) | 82:3 (5) | 831(19) 82'8(33)} 81-7(17), 83-6(10) | i } ) Children | 83°8(28) _— 841(11) | 88:5 (8) | 83:5 (1) | 87°4(25) | 85°8(26) 88*2(4) | 84:2(27)| Adults . | 82°8(44) | 84°7(24) | 83°5 (9) | 88:8(27) | 84-2(17) | 84°0(36) | 82°7(59) 81-9(38), 83-9(30)| | | | i | - | | — } | | Total .| 83°5(73) | 84:4(32) | 83°8(21) | 88°7(35) | 84°1(18) | 85:3(61) SBC Be 5(59) 84:0(57) It appears from this comparison that even if the greater brachy- cephalism of the children on Fraser River should be the etfect of a pecu- liar law of growth, the general relations of the cephalic indices of adults would remain unchanged, so that the preceding considerations remain unaltered when the total series or the adults alone are considered. It is necessary to treat two groups of tribes a little more fully, namely, the Bilqula and the Ntlakya’pamug. The tables show clearly that the Bilqula are closely related to the Kwakiutl type, with which they have the high face and nose in common. The differences between the divisions of the Ntlakya’pamug have been discussed above. It remains to point out the probable cause of these differences. It is evident that the lower divi- sions, particularly those of Spuzzum and the Uta'mk't, are more alike to the Harrison Lake type than the divisions farther up the river. It is also evident that the Nkamtci’‘nEmug resemble the Shuswap more than any other division of the Ntlakya’pamug. A detailed comparison is given on the following table, which also in- cludes the Oregonian Tinneh. Jt will be seen that, on the whole, an approach between the forms of Harrison Lake and that of the Shuswap is found. But the Ntlakyapa- muQ’o’e occupy, in many respects, an exceptional position. Their heads are narrow, their faces are lower and narrower than those of their neigh- bours. They are narrower than those of any other Indians, with the ex- ception of the Hoopa and Oregonian Tinneh, while the Shuswaps have a face as broad as the average Indian face. These differences between the absolute measurements of the face are also expressed in the indices. The NN2 ~ F . 189 REPORT 548 = (one. €8 | (O19-€8 rs (COILS er | (6) Lett | (ODT-6FI | COTG-08T | CoaersT | * — GeUUNL uriwoseI( e3 = == Cieiget (F) 8-FST = (OS)FSST | * * deasnyg (epegL | NDzt8 | (2DL-18 | (6) FSF | CODy-LEL | T'9-FIT | (9T)O-LF1 | (FIDO-TST | (@DLLET | * * ONUIAU,10jWeYN (62)9-FL | (6¢)8-18 | (e@)8-48 | Cate ed8-96E | (62)¢-31T | (ee L-LFT | (g2)8-8LT (FL)OEST | * 0,0, ontuvdesepN QDLFL | (216-08 | (DTS | (62) LF (616-681 | (LDE-EIT | (61Z-1ST | (6T)T-O8T | (2T)eESt | ° * 4.900,210, (#) 1-18 | G) 8-21 | (¢) ¢-e8 | G) G-1p | (©) 9-FFT | (Gg) O-8TT | (G) 8-19T | (S) &FBT | CGDLZST | * : * wunzzndg (OD9-2L | (G) #82 | (O1)9-28 (ODF (ZE-0FT | (ZDE-601 | (6D6-E9T | (ZT)0-9LT | (8) GOST | * * exe uosTIEH xepuy | xepuy xapuy afONT avg | 908 iT psa pro DeeN wert | Spor | JO3TFPH | Jo upreg 30 gazieqy | Jo qpeag | Jo yysuery | MPS ate | “UwauUo 1M — “Sz Ualainspa WT fo sabpsaa V =. (G1)T-¢8 — (61)0-S¢ | (02)0-9FT Coase: CZT | (6T)0-8ST | (61)6-88T | CO9)8F9T | * menuuh uvuo0del(, (Coro-F2 | (ord9-e8 | (oa)F-e8 | Co19-¢¢ | (COL)S-6FI | (COLO-EZT | (OT)L-09T | COT)8-T6T | CePGL9T | * * dvasnyg (91)9-82 | (G1)8-28 | (2F)¢-c8 | (GT)e-29 | (1G)F-LFI | (G1)9-TZT | (12)9-F9L | (186-881 | (G1)LG9T | ° * OnMIAU,loyMeyN Gee. | “9-18 | (¢8)9-e8 | (gD¢-2¢ | (e2)z-9FT | (8D)F-6IT | (9z)L-E9T | (92)6-98T | (FF)L39T | * 9,0, 0nmeudedyelN (216-62 | (21)e-18 | (19¢¢e8 | (et]-Eg | (ST)L-8bT | (ZT)L-TZT | (8Le-89T | (812-981 | (ZTOT9T | ° * * 4. y00/29 9) (10-62 | CenF-o8 | (z1)o-e8 | (ene-es | Cers-st1 | CeDz-6tt | (a1z-691 | (212-981 | (ZaJeooT |*° * * wmzandg (1D0-22 | (2%-92 | (¢e)8-88 | (iDs-2¢ | (ete-1st | (1Ds-stt | (es-F9T | (GI0-e8T | (TDosst | * * oyery uostuey xopuy vs xopul xopuy 980 NT OOP iT 9007 pro pRet{ Joes weg | aeoy | SoqMP eH | 30 aapeerg | Jo aydieyy | Jo yapearg | Jo yysaaq | NS SRL ‘uayy—'syuawmainsnayy fo sabosaay ON THE NORTH-WESTERN TRIBES OF CANADA. 549 cephalic index decreases rapidly as we go up Fraser River, but it is higher among the Shuswap than among the Nkamtci/neEmug. The facial index increases quite regularly from Harrison Lake to the Shuswap, but we must remember that the face of the Ntlakyapamug’d’e is much smaller than that of the Shuswap and that of the lower divisions of the Ntlakya’- pamug. The nasal index is so variable that we cannot draw any con- clusions from its average values. It seems, therefore, that there is a disturbing element among the Ntlakyapamug’'e which conceals among them the gradual approach of forms between the Harrison Lake type and that of the Shuswap. This fact does not seem surprising, as it is likely that mixture has taken place along Fraser River. The low values of the breadth of face remind us of the Tinneh tribes of Oregon and California, and I do not consider it unlikely that we may find here the effects of an admixture of Tinneh blood. However the peculiarities of the Ntlakyapamuq’d’e may be explained, the fact remains that the Ntlakya’pamua, who represent a people speaking one language, are physically by no means homogeneous. The upper and lower divisions indicate clearly the effect of mixture with the neighbour- ing tribes ; while the central group, ‘the real Ntlakya’pamua,’ present peculiarities of their own, which may be the old characteristics of the Nilakya’pamug, or which may be due to admixture of Tinneh blood. The gradual change of type along Fraser River proves clearly that these tribes must have occupied these regions for very long times, and that the population has been very stable. The differences in type between the divisions of this people offer an excellent example of the fact that linguis- tic and anatomical classifications do not follow the same lines ; that people who are the same in type, and must therefore be related in blood, may speak different languages ; and that people who differ in type may speak the same language. It remains to give a review of the number of children of women of the tribes which I investigated. The data obtained by means of this inquiry allow us to understand the causes of the diminution in numbers among these Indians, and suggest at the same time a possible remedy for this sad fact. I give here the number of living and deceased children of all the women whom I measured, arranged according to ages. When we direct our attention to the average number of children of women of more than forty years of age, we find the following result :— Nass River Indians - : . 4°8 children ( 6 cases) Kwakiutl : . nop cf 20 J 55 Uta’mk't ; 5 3 - 3 Ope cf CET NtlakyapamuQ’d’e - § Stites, FF sre +) Nkamtci/nEmuQq . a Z - 8 a Gots. ) Although the number of observations is small, the general result is undoubtedly correct, and agrees with the relative number of children in the villages of the various groups, the number being very small among the Kwakiutl, and much larger among the other tribes. The number of chil- dren among the Ntlakya’pamug equals that found among the tribes of other parts of North America, while that of the Kwakiutl is much smaller. The cause of the diminution of the tribes becomes clearest when we consider that group of mothers who may just begin to have adult chil- dren, that is, between the ages of thirty-five and forty-five years. At Ages of Mother 550 REPORT—1895. Fs sro sued | oOo faraan oo Ca ee oo tt g s |————— ? FI g suog rice ro ence Ace ace | AN olsen co a to | sroqysneq | il Ciel Jan alin Gh | a suog | « fealpligitalistaa aye! alee Jaan 3 sraqy.sneq J» Dads aw | “| Jan 7 ey S Oe as = & suog |~ a || Colne] nq Ana mon % a mE BS bo | sraqysneqg al | Jan ala ao | [a ll dea liom oa 4 suog Io Lil d [1s ot ee due Lor | 3 S sreyysneq ial | | | a3 a | 3 suo a e |_2 3 [| | | = bo | sxaqysneq a | | = oe aa ithe eve ar 4 sug a 1 | | | == S | sraqysueq | lllalteal a | die Ae a i Bog: Seats 2 ee | g smog al | |+alRa] S| belhe lie Han | < So | sreqysneq | Aeetos toate teal Peylenct ala | c= Se re suog | alal] |] a+ | tan OHA | q oi SSeS R | sxequsneq | § | o | lan | | |~ g wt Ae Sohit Tedt ras is g 3 S suog} s | | eli] laad ile ped Sages fel li & creo n s es i Oe 5 8 Go) be | ssaqysneq | § 44 Se] ] lal | & |e Ss al] ia Nel AS) Alo S = Q S iz ey = + IS » = suog | Ronn ol) het Tee So Cul Ra | = | 2 ae 8 $ ~~ ce) SadIysne Sx 4 rico SS anwl[a 5 S U, fea 5 | | Jaa i = | rc a — 3 A suog nia |= | | Arce aA | aA ~ bao] a & tp | Staqysneg J |x hl | Halal ac] ja | a | pe 4 suog Jan ed | | | Jrnta 4 3 sioqysneq | |e J Ja Jan | | a ov 3 a A stiog nr] | ala JH and | Sh a to «| Stoqusneqg [ a | Ja] | | no | S = = 4 suog Jala | | ae a | ! 3 sraqysneq Ml lal ll dea Jn | 3 o ———S 3 A suog dr | | Jana ar | a R w | sxominer | oe} | | t | |e | & & ae Sie = e sug lI] Jen 1] ON THE NORTH-WESTERN TRIBES OF CANADA. 551 these ages they will have children who are not yet mature, but a portion of these children will be adults. If the population were to remain stable, the number of children would have to be considerably more than twice that of the mothers. The actual distribution is shown by the following figures :— Nass River Indians 3 mothers of 35-45 years of age have 5 living 4 dead children. Kwakiutl , . 14 7 AK Ce, See * Uta'mk't . . 8 3 8 OIF, aay iy Ntlakyapamuq’d’e. 8 3 rr, R47) 20 Fe Nkamtci/nEmuq . 3 * 53 Bie > v3 s ty This table shows how exceedingly unfavourable the conditions are among the Kwakiutl, as fourteen mothers have produced considerably less than eight mature children. The figures prove also that a very slight improvement of the sanitary conditions among the Ntlakya’pamug would produce an increase of the population. The cause of the extremely unfavourable conditions among the Kwa- kiutl becomes particularly clear when the mothers are grouped in decades. When this is done we find the following result: — Age of mother : : . 20-30 30-40 40-50 50-60 60 and more. Average number of children . 2:7 21 16 5:2 4-9 That is to say, the maximum sterility is found among women who are now from forty to fifty years old, that is, who became mature about twenty-five or thirty years ago. This agrees closely with the time when the Kwakiutl sent theiz women most extensively to Victoria for purposes of prostitution. During the last decade a number of influential men among the tribe have set their influence against this practice, and we see at the same time a rapid increase in the number of children. The young women who have now an average number of 2:7 children may hope to regain the number of children which their grandmothers had. But the only hope of preserving the life of the tribe lies in the most rigid suppres- sion of these visits of women to Victoria, which are still continued to a considerable extent, and in an effort to stamp out the diseases which have been caused by these visits. II. Tue Tirnnen Trise or Nicota VALLEY. In his Notes on the Shuswap People of British Columbia! Dr. G. M. Dawson first called attention to a Tinneh tribe which used to inhabit the Nicola Valley, but which has become extinct. Some notes on the history of this tribe were given by Dr. Dawson according to information obtained from Mr. J. W. McKay, formerly Indian Agent at Kamloops, who hasan extensive knowledge of the Indians of the interior. As parts of this information conflicted with reports which I had received, and as it seemed desirable to gather as much information as possible on this tribe, I resolved to visit them in the course of my investigations. Owing to pressure of time I had to give up the intended journey, and requested Mr. James Teit, who is thoroughly familiar with the Ntlakya’pamugq, to try to collect as much information as possible on the tribe. He visited Nicola Valley early in March 1895, and reports the results of his work as follows :— 1 Trans. Royal Soc. Canada, vol. ix. 1891, sect. ii. p. 23. led) 002 RETORT-—1895. ‘T saw the three old men who are said to know the old Stiwi'Hamug language, which was formerly spoken in Nicola Valley, and found that they only remembered a few words of what they had heard from their fathers. One of them could only give me five or six words, another one twelve, and another one twenty. As many of these words were the same, I only obtained twenty distinct words and three phrases. I also learned two place-names used by them which I think are probably Tinneh.