Ne +h bl 0 Dea bs FONT = ae : ° 9¥ ee My a, we bac a Mi | Ne Se i a : Ae ke VER fe a Ree ite ni Mane: “ we hee a a aaa Wad Cu, & ai; oa y ky ot Dien 4 ’ j ae Py ee oF, 74 ' ; ‘ i ‘ 4 ‘ i t i WOM liek 4 OT at mae, tes 6 ie) hae Sta dine 2 " bod LES ete 4 1 ye Ly 2 i P ia ; { ; a: a ¥ Wy ¥ Mf ’ Rh i = 7 9 a 4) eh aN NE ibe > REPORT OF THE; SIXTY-KIGHTH MEETING OF THE BRITISH ASSOCIATION ADVANCEMENT OF SCIENCE BRISTOL IN SEPTEMBER 1898. LONDON: JOHN MURRAY, ALBEMARLE STREET, 1899. Office of the Association: Burlington House, London, W. CONTENTS. Page Mrgmors and Rules of-the Association <.............cseccsecctecneesecscsescesssees XXix Places-and Times of Meeting, with Presidents, Vice-Presidents, and Local PCEEELAPIOS ATOR COMMEDCOMENE |) 5. ..0ce0s0deeecsereigseistonsueecnonsoeaccesesies xl rusipes:and General Officers, 18381—1809. .........cc-ccccccsesccscocrcnssausecoers lii Presidents and Secretaries of the Sections of the Association from 1832 ... hii Mrs m MERTEN Beet Ines) » x.1)3a85. oo dante sekote V5. wwe acastegwes o dex deh aede dee) apoE XL hechures to the Operative Classes ..<......sccescsccecsecoscesscecssewcescsoosceadecs lxxiv Officers of Sectional Committees present at the Bristol Meeting ............ Ixxv EMME GLC ONTCIAMEOR=HOO -. a ccasscedacecascans ss ccssccaceroensstsasdcdes deoees Ixxvii Per eAEOM MPA CCOUNE = epee isccecscacsasicsisedacsoedvecetsssedeous SSeS ee ee Ixxviii Table showing the Attendance and Receipts at the Annual Meetings ...... Ixxx Report of the Council to the General Committee ............:ccc0cceceecees oe xxxii Committees appointed by the General Committee at the’ Bristol Meet- MSIE. POG a.45 55355 Sc cskyansiswnd gee thidi doinanas Baus Sean yee ee Rd sone’ Ixxxvi Communications ordered to be printed 27 extenso ...........cseecseeeceeeeeeees xevi Resolutions referred to the Council for consideration, and action if I sae vcah cach nx Rei du tean capt nacaete Gs dapusnnsdegesccéca’ x¢evi Change of Days of meeting of the General Committee and of the Committee ESTE GLA Gar ee Ce Pe Pa ee X€Vi SEEN AS UrTRLIS OF MONG Y .52. os ).o55 fcsund t +.Seansal jentdvdees +e sodneutneiveder x¢vil Places of Meeting in 1899, 1900, and 1901 ..............ccceecccdecceeeceeeeeee exe be General Statement of Sums which have been paid on account of Grants for PEER CHESUPBGGEH Vat evicss. - pais eipeescah cords Saas Riobesbes naaetere Pestacis ods 02 ¢c PUMP TNS Si Be ocd 0203 coe stant 2 46“ oun anvizn duc CONTENTS. vii Pags _ The Teaching of Science in Elementary Schools.—Report of the Committee, : consisting of Dr. J. H. Guapstone (Chairman), Professor H. KE. ARMSTRONG (Secretary), Professor W. R. Dunstan, Mr. Grorcu Grapstone, Sir Joun Lussock, Sir Puitre Maenvs, Sir H. E. Roscoz, and Professor S. P. THOMPSON .......seceeesseeseseesceseeeeesseenenseeseesecsteseeseeaesaensecsssaeeaeneeeins 438 Apprnpix.—Schedule II.—Elementary Science and Geography ...... 438 Schedule [V.—Elementary Physics and Chemistry ...... 43 Bibliography of Spectroscopy.—Report of the Committee, consisting of Pro- fessor H. McLuop, Professor W. C. Rosurrs-Austen, Mr. H. G. Manan, PUTEMn Vy mL) SIE wlNYA GHENT ci 1), EMEC EAE MsitSGi seuclais cuisla sin bans ned'ecteaed dees cetsedieaainesielt 439 The Fossil Phyllopoda of the Paleozoic Rocks.—Fourteenth Report of the Committee, consisting of Professor T, WutrsHireE (Chairman), Dr, H. Woopwarp, and Professor T. Rupprt Jones (Secretary). (Drawn up by See ESRO Te VE PEE Td ONES) )at ccs cies open snes sacra aieianasleNels. cosblasenevemeah ees 519 Canadian Pleistocene Flora and Fauna.—Report of the Committee, consisting of Sir J. W. Dawson (Chairman), Professor D. P. Penxattow,. Dr. H. Amt, Mr. G. W. LamptueH and Professor A; P. Coteman (Secretary), appointed to further investigate the Flora and Fauna of the Pleistocene Hiaiui in, ORTEGE -a nbarecesaaeeneessbhiesscaeosce coed gece sche passe mdsdder tins decbaen cece 522 APpPENDIX.—Pleistocene Flora of the Don Valley. By Professor D. P. EL AATA THO Wins B ante ceeoch i pet tee tesla sce reeies ercien cosets 525 ‘Life Zones in the British Carboniferous Rocks.—Report of the Committee, consisting of Mr. J. E. Marr (Chairman), Mr. E. J. GaARwoop (Secretary), and Mr. F. A. Barurr, Mr. G. C. Crtcx, Mr. A. H. Foorp, Mr. H. Fox, Dr. Wuerrtton Hinp, Dr. G. J. Hype, Mr. P. F. Kenpatz, Mr. J. W. _ Krexipy, Mr. R, Kinston, Mr. G. W. Lamprueu, Professor G. A. Lesour, _ Mr. G. H. Morton, Professor H. A. NicHotson, Mr. B. N. Peacu, Mr. A. _ Srrawan, and Dr. H. Woopwarp, appointed for the purpose of studying the Life Zones in the Carboniferous Rocks. (Drawn up by the DEER rt acti «cig tse duke gh gets aataphldino to" i'n cfanle Rae tine vais 25. 00(o ss Bey ONT 529 Photographs of Geological Interest in the United Kingdom.—Ninth Report of the Committee, consisting of Professor James GEIKIE (Chairman), _ Professor T. G. Bonney, Dr. Temprst AnpERson, Mr. J. E. BEepForp., Mr. H. Coarzs, Mr. C. V. Croox, Mr. E. J. Garwoop, Mr. J. G. Goop- curp, Mr. Witi1am Gray, Mr. Rosertr Kinston, Mr. A. 8. Rerp, Mr. J. J. H. Tzart, Mr. R. H. Trpppeman, Mr. H. B. Woopwarp, Mr. F. Woounoven, and Professor W. W. Warts (Secretary). (Drawn up by Dy the Secretary.) ..............:.cccceneseeceeseeseeeesencessencnecsceeeenccasneesecaneeees 530 Photographs of Geological Interest in Canada.—First Report of Committee, _ consisting of Professor A. P. Coneman (Chairman), Professor A. B. WILL- _ mort, Professor F. 0. Apams, Professor W. W. Warts, Mr. J. B. TyRRELL, and Mr. W. A. Parks (Secretary). (Drawn up by the Secretary.) ......... 546 ApprenpDIx.—Circular Letter issued by the Committee. Trish Elk Remains.—Report of the Committee, consisting of Professor W. Borp _ Dawxrns (Chairman), his Honour Depmsrer Git, Rev. E. B. SavacE, _ Mr. G. W. Lamervan, and Mr. P. M.C. Kermops (Secretary), appointed to examine the Conditions under which remains of the Irish Elk are found in RETEST GI EGIL | ins hanno: ncaemakeccu etn svcnancudctades esses cadet sectueciucanvercdseeweate 548 ‘Erratic Blocks of the British Isles—Report of the Committee, consisting of Professor E. Hurt (Chairman), Professor T. G. Bonney, Professor W. J. Sottas, Mr. C. E. De Rancz, Mr. R. H. Trppemay, Rev. 8. N. Harrison, Mr. J. Horws, the late Mr. Dueatp Bett, Mr. F. M. Burron, Mr. J. Vili REPORT—1898. Page Lomas, and Mr, P. F. Kenpatt (Secretary), appointed to investigate the Erratic Blocks of the British Isles, and to take measures for their preserva- tion, (Drawn up by the Secretary.) -...0..0......00050.00 css rcncedancuseneemenmee 552 Structure of a Coral Reef.—Report of the Committee, consisting of Pro- fessor T. G. Bonney (Chairman), Professor W. J. Sotias (Secretary), Sir ArcHIBALD GEIKTE, Professors J. W. Jupp, C. Lapworru, A. C. Happon, Boyp Dawkins, G. H. Darwin, 8. J. Hickson, and ANDERSON Srvart, Admiral Sir W. J. L. Warton, Dr. H. Hicks, Sir J. Murray, Drs. W. T. BuanrorD, C. Lz Neve Foster, and H. B. Guppy, Messis. F. Darwin, H. O. Forses, G. C. Bournz, and J. W. Greeory, Sir A. R. | Brunt, and Mr. J. C. HawxsHaw, appointed to consider a project for investigating a Coral Reef by Boring and Sounding ...........2..:.:sccsseereeees 556 The Eurypterid-bearing Rocks of the Pentland Hills.—Final Report of the Committee, consisting of Dr. R. H. TRaquarr (Chairman), Mr. M. Lacrre (Secretary), and Professor T. RUPERT JONES................. oes sad Oannaseet eee 557 The Zoology of the Sandwich Islands.—Kighth Report of the Committee, consisting. of Professor A. Newron (Chairman), Dr. W. T. BLAanForp, Professor S. J. Hickson, the late Mr. O. Satvry, Dr. P. L. Sctatmr, Mr. E. A. Suaru, and Mr. D. Swarr (Secretary) ...........:.ssscsceeseeseeeeeees 558 Zoological Bibliography and Publication.—Interim Report of the Committee, consisting of Sir W. H. Frowrr (Chairman), Professor W. A. HERDMAN, Mr. W. E. Hoyts, Dr. P. L. Sctarer, Mr. Anam Sepewicx, Dr. D. SHARP, Mr. C. D. SHERBORN, Rey. T. R. R. Stepsine, Professor W. F. R. WELDON, and eM BJA. (BATHERS (SECTCLATY)...--c-2--0--eoseosairssecetnresusqecnsesuaneiane 558 Life Conditions of the Oyster: Normal and Abnormal.—Third and Final Report of the Committee, consisting of Professor W. A. HerpMAn (Chair- man), Professor R. Boycn (Secretary), Mr. G. C. Bourns, Dr. C. A. Kony, and Professor C. S. SHERRINGTON, appointed to Report on the Elucidation of the Life Conditions of the Oyster under Normal and Abnormal Enyiron- ment, including the Effect of Sewage Matters and Pathogenic Organisms. (Drawn up by Professor HpRDMAN, Professor Boyce, and Dr. KouN.) ...... 559 - Bird Migration in Great Britain and Ireland.—Interim Report of the Com- mittee, consisting of Professor Newron (Chairman), Mr. Joun CorDEAUx (Secretary), Mr. Joun A. Harviz-Brown, Mr. R. M. Barrryeton, Rey. E. Ponsonby Knustery,.and Dr. H. O. Fores, appointed to work out the details of the Observations of the Migration of Birds at Lighthouses and Miphtships S8O-87. ....J.c.sncc-cn-scosesersices steesacesomshnuacese«ssaueeenmems 569 Index Animalium.—Report of a Committee, consisting of Sir W. H. FLowErR (Chairman), Mr. P. L. Sctatzr, Dr. H. Woopwapp, Rev. T. R. R. STEBBING, Mr. R. MacLacutan, Mr. W. E. Hoyle, and Mr. F. A. BarHer (Secretary), appointed to superintend the Compilation of an Index Animalium............ 570 Caves in the Malay Peninsula.—Report of the Committee, consisting of Sir W. H. Frower (Chairman), Mr. H. N. Ripiey (Secretary), Dr. R. Hantiscx, Mr. Crement Rerp, and Mr. A. Russet WaLzAcs, appointed to explore certain caves in the Malay Peninsula, and to collect their living and extinct BRINE wns oon dns snide o bi py caren v edhe crane on Dulane emease aaa ae alae eae 571 APPENDIX.—Report by Mr. H. N. Rmpipy.............0+ pass eoeten nanspanaay panne Canadian Biological Station.—First Report of the Committee, consisting of Professor E. E. Priyce (Chairman), Dr. T. Wxstry Mizis, Dr. A. B. Macattum, Professor Joun Macoun, Professor E. W. MacBrinz, Mr. W. T. Tuiseuron-DymR,. and Professor D. P. PENHALLOW (Secretary), on the Establishment of a Biological Station in the Gulf of St. Lawrence ......... 582 Investigations made at the Marine Biological Laboratory, Plymouth.—Report of the Committee, consisting of Mr. G. C. Bourne (Chairman),Professor CONTENTS. ix Page E. Ray Lanxester (Secretary), Professor Sypyry H. Vines, Mr, A. Supe- wick, and Professor W. F. R. WELDON ........-.:.:sseeeseeeeeeeeseesseeeeeeeeeeees OBB Report of Algological Work. By G. BREBNER .........seeeeeeetrnerreees 583 Report on Nerves of Arenicola, Nereis, &c. By F. W. GamBie, M.Sc. 584 Report on Mr. J. H. Wapsworti’s collection of material for the Study of the Embryology of Aleyonium. By Professor 8. J. Hickson, F.R.S. 586 Occupation of a Table at the Zoological Station at Naples.—Report of the Committee, consisting of Professor W. A. Herpman, Professor E. Ray Layxester, Professor W. F. R. Wxxpon, Professor 8. J. Hickson, Mr. A. Sepewrcx, Professor McInrosH, Mr. W. E. Hoyts, and Mr. Percy StapEn (Secretary) .........-...cessseccasececccssscccnasseceeeesseceonsscsanssnansseetenescenneees 587 ApprenDIx I,—The Pseudobranch and Intestinal Canal of Teleosteans. Bry gl amine GEM «oops !occcs amrseeh Chae gaa 588 » IL—(1) The Relations between Marine Animal and Vege- table Life in Aquaria. By H. M. Vernon ......... 589 (2) The Relations between the Hybrid and Parent Forms of Echinoid Larve. By H. M. Vernon ... 589 III.—On the Variation of Cardium, Donax, and Tellina. By Pag, LUNE Tans{=(00. onc oasadd copepReedeEStecoed Sac HoDOSoCOURSOUaEDee 593 » 1V.—List of Naturalists who have worked at the Zoological Station from July 1, 1897, to June 30, 1898 ......... 594 V.—List of Papers which were published in 1897 by Natu- : ralists who have occupied Tables in the Zoological SHaolOll ccs. eee cae one EPR Reps on pany ne indy 595 Photographic Records of Pedigree Stock—By Francis Gatron, D.O.L. D (Oxf.), Hon. Sc.D.(Camb.), FLR.S. ....cccccecceeeseenseceeeeeetsnseaeesssenesseneeees 597 The Climatology of Africa.—Seventh Report of a Committee consisting of Mr. _E G. Ravensrer (Chairman), Sir Jon Krrx, Mr. G. J. Symons, Dr. H. R. Mizz, and Mr. H. N. Dickson (Secretary). (Drawn up by the Chair- BT e sev cs-2ecneeeseccsssccuecascneceasenyscunsevetensbedccseecoesaasnevecasandewarsesee 603 The Mechanical and Economic Problems of the Coal Question. By T. Forster BROWN, M.Inst.C.B. ....00.......ccescccnsccnecccssccnseecesecessooescnsnsesogecnescnecs 611 \ New Instrument for Drawing Envelopes, and its Application to the Teeth of Wheels and for other Purposes. By Professor H. 8S. Hetz-SHaw, LL.D., SUES TNO tre bo A aN eck ta cuaseseesdeasavectedares seesdaccas EEL Sant h once ses 619 Screw Gauge.—Third Report of the Committee, consisting of Mr. W. H. Preece (Chairman), Lord Kutviy, Sir F. J. Bramwe tt, Sir H. TRupMan Woop, Major-Gen. Wesper, Col. Warxin, Messrs. Conran W. Cooxz, R. E. Crompton, A. Strou, A. Lu Neva Foster, C. T. Hewirt, G. K. B. Exrursrons, T. Bucxney, E. Riee, 0. V. Boys, and W. A. Pricz (Secre- tary), appointed to consider means by which Practical Effect can be given _ to the Introduction of the Screw Gauge proposed by the Association in 1884 627 e North-Western Tribes of Canada.—Twelfth and Final Report of the Committee, consisting of Professor E. B. Tytor (Chairman), Sir CUTHBERT E. Perk (Secretary), Dr. G. M. Dawson, Mr. R. G. Hatrpurron, Mr. Davin Bortz, and Hon. G. W. Ross, appointed to investigate the Physical ‘Characters, Languages, and Industrial and Social Conditions of the North- Western Tribes of the Dominion of Camada ............eceeeseeecceeeeeeeeteetenes 628 ‘ I.—Physical Characteristics of the Tribes of British Columbia. By Franz Boas and Livingston FARRAND ...........scseceseeecerees 628 Ii.—The Chilcotin. By LIVINGSTON FARRAND.....ccccccecesseeeesseees 645 x REPORT—1898. Page IlI.—The Social Organisation of the Haida. By Franz Boas ......... 648 1V.—Linguistics, “By HRANZ BOAS \......... ..5..0s.0.0+nsecnenmieaeneeee 654 V.—Summary of the Work of the Committee in British Columbia. By PRANZ BGM tees ctr sakee sists stoodes secede ss sopeesee see 667 AppENDIxX—Index to Reports, [V.-XII. oo... cede ween 684 Torres Straits Anthropological Expedition.—Interim Report of the Committee, consisting of Sir W. Turner (Chairman), Professor A. C. Happon (Secre- tary), Professor M. Fosrmr, Dr. J. Scorr-Kenrre, Professor L. C. Mart, and Professor MARSHALL WARD, appointed: to investigate the Anthropology and Natural History, of MorresiStralts. ....55.20oc..ns-0+-+nseuseeeenesateoneewnsindy 688 Silchester Excavation.—Report of the Committee, consisting of Mr. A. J. Evans (Chairman), Mr. Joun L. Myxrs (Secretary), and Mr. KE, W. Bra- BROOK, appointed to co-operate with the Silchester Excavation Fund Com- Mibhee ti, bile MR POMM LANES. .nssscccscadacvcenrensanedonaves sav ecve cd enarareQaeeanee 689 Mental and Physical Deviations from the Normal among Children in Public Elementary and other Schools——Report of the Committee, consisting of Sir Doveras Garon (Chairman), Dr. Francis WARNER (Secretary), Mr. E. W. Brasrook, Dr. J. G. Garson, and Mr. E. Wuirn Watts. (Report drawn up by the Secretary.) .......-00cc-.cessescoesceneecencrereereeecceseecoasersnenes 691 ArpEnDIx.—Table showing co-relations of conditions of defect among 1,120 children, subnormal in constitution, mental, or physical......... 692 The Lake Village at Glastonbury.—Third Report of the Committee, consist- ing of Dr. R. Munro (Chairman), Professor W. Bory Dawxrns, Sir JoHn Evans, General Prrv-Rivers, Mr. A. J. Evans, and Mr. A. BuLnzip (Secretary). (Drawn up by the Secretary.) .. ...6.....scseeeesseeseeeeneeseen ones 694 An Ethnological Survey of Canada.—Second Report of the Committee, consist- ing of Dr. G. M. Dawson (Chairman and Secretary), Professor D. P. PEn- HALLOW (Vice-Chairman), Mr. E. W. Brasroox, Professor A. C. Happon, Mr. E. S. HarrnanD, Sir Joun G. Bovriyor, Appi Cuoe, Mr. B. Suze, Asst Taneuay, Mr. C. Hitr-Tour, Mr. Davin Boyrn, Rev. Dr, ScappINe, Rev. Dr. J. Macrean, Dr. Mertn Bravcuemin, Rev. Dr. G. ParrErson, Mr. C. N. Bett, Hon. G. W. Ross, Professor J. Mavor, and Mr, A. F. TERUIN DER © ere eipase eee ee eek eee e cee siicwesct salelble Seesed soe soos eet amen 696 Apprmnpix I,—Haida Stories and Beliefs. By C. H1r1-Tovr ......... 700 . II.—Customs and Habits of Earliest Settlers of Canada. Tey GEN YAMIN OULTE: «. 00s .00s0.0esen+++cneneuaeeemaeege 709 Ethnographical Survey of the United Kingdom,—Sixth Report of the Com- mittee, consisting of Mr. E. W. Braproox (Chairman), Dr. FRancis Gatton, Dr. J. G. Garson, Dr. A. C. Happon, Dr. JosepH ANDERSON, Mr. J. Romruty Aten, Dr. J. Beppozn, Mr. W. Crooxe, Professor D. J. CunyincHaM, Professor W. Boyp Dawxrys, Mr. Arruur J. Evans, Mr. F. G. Hizron Pricn, Sir H. Howorru, Professor R. Murpoxa, General Prrt-Rivers, Mr. E. G. Ravensrein, and Mr. E, Sipyny HArrnanp (Secretary). (Drawn up by the Secretary.) .......::.ceseesseceesseeeeeeereensees 712 Functional Activity of Nerve Cells——Second Report of the Committee, consist- ing of Dr. W. H. Gasxett (Chairman), Professors BuRDON SANDERSON, M. Foster, E. A. Soudrer, J. G. McKenprick, W. D. Hariisurton, J. B. Hayorart, F. Gorcu, CO. 8. SHerrineton, and A. B. MacaLtum, Dr. J. N. Lanetny, Dr. G. Mann, and Dr. A. Wa ter (Secretary), appointed to investigate the changes which are associated with the Func- tional Activity of Nerve Cells and their Peripheral Extensions ......,........ 714 CONTENTS. _ Appanpix I—Structural Alterations observed in Nerve Cells. By II.—Excitatory Electrical Changes in Nerve. By FRancis » i1—The Effects upon Blood-pressure produced by the Intra-venous Injection of Fluids containing Choline, Neurine, and Allied Substances. By F. W. Morr, M.D., F.R.S., and W. D. Harirvrton, M.D., SOROS, “Ccapodeoscdsedosscucanu epbeasbeereet occa cogeranorc The Physiological Effects of Peptone and its Precursors when introduced into _ the Circulation. Second Interim Report of a Committee, consisting of _ Professor E. A. Scudrer, F.R.S. (Chairman), Professor C. 8. SHmRRING- _ oN, F.R.S., Professor R. W. Boycu, and Professor W. H. THompson (Secretary). (Drawn up by the Secretary.) .........ccceerecssceceeeseeeeeeereeees Fertilisation in Pheophyceex.—Report of the Committee, consisting of Pro- fessor J. B. Farmer (Chairman), Professor R. W. Purxures (Secretary), Professor F, O. Bowzr, and Professor HARVEY GIBSON .........sdssseeeeeeeees Goren, F.R:S., and G. J. Burcw, M.A.:........... .. (il xi Wi b aVWARR INGTON, WMDs <2. seccnewennccttiarseleseswsinc: 715 6 LDL Bie Sh edoadadet pishne. sh do sh Aer Seannn dt aeeeb ape cyn 30 sgrpoo noc 717 » 1V.—The Myelination of Nerve Fibres. By H. V. ANDER- 717 i V.—The Histology of Nerve Cells. By Gustav Mann, M.D. 719 720 REPORT—1898. INTERNATIONAL CONFERENCE ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY, THURSDAY, SEPTEMBER 8. Page Address by Professor A. W. Rtcxpr, M.A., D.Se., Sec. R.S., President of i; 2. Ghe ‘Conference’ 25s. .(2.< fences novice cence once cance meee ates «Se ceulek sae hoe ee nee eee 733 On the Relative Advantages of Long and Short Magnets. By Professor IES. IMABOARIS.c. ccc secon. spanebarcemeeccntc=scasceckiensccecerets «ssh tanta anne 741 On the Construction of Magnets of Constant Intensity under Changes of Temperature. By J. R. ASHWORTH, B.Sc. .......5c......000.-snssesesavessees 742 FRIDAY, SEPTEMBER 9. . On the Establishment of Temporary Magnetic Observatories in Certain Localities, especially in Tropical Countries. By Professor von Brzoxp and General RYKATOHEEE. .......0cssessa:cavescacbecssessa0sconccnaness¥asseateenoge 743 . The Application of Terrestrial Magnetism to the Solution of some Problems of Cosmical Physics. By Arrour ScHusrter, F.R.S. ......... 745 . Antrag auf Massnahmen zur systematischen Erforschung der Saecular- variationen der erdmagnetischen Elemente. Von Dr. Ap. Scumipr ... 747 . On Simultaneous Magnetic Observations. By Dr. EscHENHAGEN ......... 748 , Discussion on Monthly Means ..........::2:..ssecocsero+ssco+despecsen etna Eanes 749 . A Discussion on the Publication of the Differences between the Hourly Means of the Components of the Magnetic Force (X, Y, Z) and the Monthly Means, s.siccots..csse.ctdcssscewcncessosavdercoccsers se Cneeeeeeenam ere 749 . On Magnetic Observations in the Azores. By AtsErt, Prince of Monaco 749 . *On Magnetic Observatories in Cape Colony. By Dr. Brarrre and INF ST ORRISON «1 ccc. scree Novessscosecdvecvecesecescaceccesecslses onde eetteetea———=s 750 . Sur Je Mouvement diurne du Péle Nord d’un Barreau Magnétique suspendu par le centre de gravité. Par J. B. Carrnto eee teen ewan ee nnee MONDAY, SEPTEMBER 12. . An Account of the late Professor John Couch Adams’s Determination of the Gaussian Magnetic Constants. “By Professor W. Gry~is ADAMS, By Ri aleceaaeasta eanees ccsenn stave secs scosacssuaesvepec sf scueteurae ct sane 752 . On a Simple Method of obtaining the Expression of the Magnetic Potential of the Earth in a Series of Spherical Harmonics. By ARTHUR GH UST MY Ey Rue Was tuncsssebhs ose cs osinesasivestyesswedseaduutuceciedeps eaten 752 CONTENTS. xiii Page 8. *On Magnetic Observations at Funafuti. By Captain E. W. Crnax, R.N., MES aoe ec sa nape lane Seiscie sais Sieleludlan dua sasedrodaedoneesenssses 755 4, On the Relations between the Variations in the Earth Currents, the ) Electric Currents from the Atmosphere, and the Magnetic Perturbations. By Serre LEMSTROM.............0.ececeeeseceeeeeceeeeeeeesaeesseeaeeecsseeeeseseeees 755 5. On the Interpretation of Earth-current Observations. By ArrHur PUMPER BOLLS, sacesvnncstevsecscnbqsouctGnsssnteeucnsccosecessosnoeccnsdecevensal 756 6. On the Construction of Magnetic Observatories. By Dr. SNELLEN ...... 757 TUESDAY, SEPTEMBER 13. | A Joint Meeting with Sections A and G—the Magnetic and Electrolytic iftectsioftulectric Riail way, ..c.2c.-.:.-<-ces-ccoenscosesavevecsensercaseesssncsces 758 1. On the Disturbance of Magnetic Observatories by Electric Railways. By W. VON BEZOLD 22 ...0.....ccccescnsecntencansvesensenscsscoecserserserasere 758 2. On the Magnetic Effects of Electric Railways at Berlin. By Dr. FESCHENHIAGEN. .......2..0002--ccecevccseccsccascscsscecsccecsessrcesersrcscsaserasla 758 1. On the Form of the Isomagnet:c Lines in the Neighbourhood of the Volcano Etna. By Lurer PAtaZz0 .............ccccescsccseceecasecsen scans Moats: 2. On the Influence of Altitude above the Sea on the Elements of Terrestrial Magnetism. By Dr. van Riscknvorset and Dr. W. van BemMeten... 760 8. On the Variation of Terrestrial Magnetic Force with Altitude. By PEPOLERSOF J. LIGNAB ....-2.20-ccnvsscnaceccercnccostosenacescecnedengnccaursnossenaeas 760 Extracts from the Report of the Permanent Committee on Terrestrial Magnetism and Atmospheric Electricity to the International Meteoro- PP RMMMIMO NICE EICE! C. .0......0c0cs--snepseoavnssianhenssanenadesnvecnrsansacexedeemsrahds 761 REPORT—1898. TRANSACTIONS OF THE SECTIONS. Section A.—MATHEMATICAL AND PHYSICAL SCIENCE. Page THURSDAY, SEPTEMBER 8. Address by Professor W. E. Ayrron, F.R.S., President of the Section ...... 767 1. Report on Comparing and Reducing Magnetic Observations ............... 777 2. Lenses not of Glass. By J. W. GIFFORD ....ssccecc.ssccceeseenesnesevevnsee ves 777 3. On the Articulation and Acoustics of the Spirate Fricative Consonants. By 0. Ler, D.Lit,, M.A., FURS ii dstesdcgsar.cct a... nee ee 777 4, On the Conservation of Energy in the Human Body. By Epwarp B. Htosaend: WO, -AWWAGER: \..15.5d5 600 xe glee deans 3 as 778 5. On a Pneumatic Analogue of the Potentiometer. By W. N. Smaw, Ei nhes x soadnnas vveyh st oe0e's agen scene ade ae RON tsL > ¢ coe 778 FRIDAY, SEPTEMBER 9. 1. Comparison between Charging a Secondary Cell at Constant Potential and at Constant Current, more especially as regards Efficiency. By A. A. Oxnen and J. M. DoWALDSON 2..5.:..seeesqeeobeveestessere ck .cosgss ene 779 2. On a Magnifying Telephone. By Professor Ottver Lopes, F.R.S. ...... 782 3. “On the Measurement of Small Differences in Resistance. By E. H. Grimes, ERAS, | 2.0.2 ssacasovea0 otcebimestetbeae it reess. /-s sone 782 4, The Dynamical Theory of Refraction, Dispersion, and Anomalous Disper- gion, By Lord Kurvin, GC. V.O. 2. ccs ts seeesntie nse a- +s cee Bows. TBE 10. ., . Continuity in Undulatory Theory of Condensational-refractional Waves in Gases, Liquids, and Solids, of Distortional Waves in Solids, of Electric Waves in all Substances capable of transmitting them, and of Radiant Heat, Visible Light, Ultra-Violet Light. By Lord Ketvry, G.C.V.O.... 783 - Heat of Combination of Metals in the Formation of Alloys. By Arnx- Mapee Gan), DSc. ........agsssocsceoneseogeereuasc sites see pean cee 787 . A Platinum Voltmeter. By Professor H. L. Carnenpar, M.A., F.R.S... 788 . “On Radiation from a Source of Light in a Magnetic Field. By Professor T. Preston, F.R.S. ..... See: oorcedcoesbee Baslasepboctowneetbe sauce hte sie stein 789 . On the Discovery by Righi of the Absorption of Light in a Magnetic Field. By Stryawes P. Toompson, D.Sc., FURS. vijesececasenscses sss ssaeen seen 789 On the Dissipation of Energy in the Dielectric of a Condenser. By Epwarb B. Rosa and ARTHUR W. SMITH..........ccccccsessecscscsesesenseeces 790 Hydrometers of Total Immersion. By A, W. Warrineton, M.Sc. ...... 791 CONTENTS. XV SATURDAY, SEPTEMBER 10. DEPARTMENT I.— MATHEMATICS. Page . Report on Tables of certain Mathematical Functions............ faueemen deste’ 791 The Mathematical Representation of Statistics. By Professor F. Y. TIPE REDE UHe. eeuedsctnecacsecce cc ctcsedsncnrebscienteeenaarntinaisesa)asmWomriadens denis 791 . On the Use of Logarithmic Co-ordinates. By J. H. VINCENT............-.. 791 . Stream Line Motion with Viscous Fluids in two Dimensions, and in three Dimensions. By Professor H. S. Heve-Swaw, LL.D.............-:eeee 792 . Mathematical Proof of the Identity of the Stream Lines obtained by means of a Viscous Film with those of a Perfect Fluid moving in two Dimensions. By Sir G. G. STOKES, FLR.S. ...ceeseeeseeeeeeeee ee eteteeetennees 792 . On Graphic Representations of the two simplest cases of a Single Wave: (a) Condensational-refractional, (6) Distortional. By Lord Ketviy, ROMA) Rh oo tee ances edieidcsnnjonanseensanes a a84nsncailanas stints segs # 792 A New Method of Describing Cycloidal and other Curves. By Professor A. S. Hane-Seaw, UL.D...............02sccccscscscsceeseeeeecececcrecscncseeecneess 792 . The Recent History of the ‘Theory of the Functions used in Analysis. By E. T. WHITTAKER .-0...eeeceecceeeeeeeeeeeeeensecateeeeceetennneceeeeesenenees 793 . The Dynamical Explanation of certain observed Phenomena of Meteor Streams. By Dr. G. JonnsTonE STONEY, PLRS. 2.2... tees 793 *Survey of that part of the Scale upon which Nature works, about which Man has some Information. By Dr. G. Jonnsrong Sronezy, F.R.S....... 796 The Imaginary of Logic. By Professor G, J. STOKES ........61.0100eeeseeees 796 DEPARTMENT IJ.--MprroroLoey. . Report on the Ben Nevis: Observatory 1... 0h iio bac dee ae 796 . Report on Meteorological Photography ...........+.:s::sseeeeeeeeeeees ates 796 Report on Seismological Investigation ...........-.:..sesseeeeeeeeeee tennessee 796 . Interim Report on the Montreal Meteorological Observatory .......-+-.---- 796 A Quantitative Bolometric Sunshine Recorder. By Professor H. L. Cat- Reprints: MAL, BURG: - .. 2... sccsceceseensacescseeess sarass pSeewrais dees Samide awctaslse pate 796 6 Progress in the Exploration of the Air by means of Kites at Blue Hill Observatory, Mass., U.S.A. By A. Lawrence Rorcu, 8.B., AS Meer. 797 *A New Form of American Kite. By Professor A. Scuuster, F.RS. ... 797 8. Analogies between the Yearly Ranges of some Meteorological and Mag- netic Phenomena. By Dr. VAN RIJCKBVORSEL .........00e-seeeeeeeeeeeeeee eee 797 . The Classification of Polydiurnal Weather Types in relation to the Pro- longation of the Daily Forecast in Western Europe. By Doveras AROHIBALD, M.A., F.R.Met.Soc, .......2c0c00 ccsecnececesecceececcneteeeerersceees 798 The Rainfall of the South-Western Counties of England. By Jouy _ Hopxryson, F.R.Met.Soc., Assoc.Inst.C.H. .......ceceeeeee eee ceee nents eee eees 799 MONDAY, SEPTEMBER 12. ; *A Discussion on the Results of the Recent Solar Eclipse Expeditions ......... 801 1. Interim Report on Electrolysis and Electro-chemistry ..........::+1seeeseeees 801 2. *Dilute Solutions. By E. H. Grirrirus, F.RS. .........-..--:eeesee neers 801 3. *Conductivity of Dilute Solutions. By W. C. D. WHBTHAM ..........--++- 801 xvi wd & P. . Velocity of the Electricity in the Electric Wind. By Professor A. P. REPORT—1898. age MO TEAEN OOK reek cana n cise sicting ase oem cwiieaaeussiovod sees be egode ec lae tt =e etre 801 fp Dalton's Ioaw.- By Wet N. SHAW, HoIR.S........0000s00c.seseysiec sect ee eee eee 801 . On the Determination of the State of Ionisation in Dilute Aqueous Solu- tions containing two Electrolytes: No.2. By Professor J. G. MacGrueor 803 . The Carbon-Consuming Cell of Jacques. By S. SKINNER .............00008 804 TUESDAY, SEPTEMBER 13. ‘ discussion on the Magnetic and Electrolytic Actions of Electric Railways 805 . Report on Hlectric Standards ...........cceecsecseceeeeees si Soistiele one RRS aoa 805 . On Standard High Resistances. By F. B. FAWCBIT..................ce0seeeee 805 . *On the Electric Conductivity and Magnetic Permeability of a Series of New Alloys of Iron. By Professor W. F. Barrerr, W. Brown, and Re RAa TAA DMGMUD s 55 cn scsscceeees acobosesreobossisnns deus npattens sence teen este et enEe 805 WEDNESDAY, SEPTEMBER 14. . The Drop of Potential at the Carbons of the Electric Arc. By Mrs. MENTION is oc ce shaoivs on dened d dee Wels Saafaiicin nd boo 04 os ines SSSR ERE as tele de Cee eee aoe 805 2. Some Experiments on the Effect of Pressure on the Thermal Conductivities OneRocks:. by WDE AOS El. LUBEB, ..)...'50. saan eeseqie coup iteuastacen pele: tee eae 807 3. On the Determination of the Thermal Conductivity of Water. By 8. R. Minne, BiSe-, and Professor A. P.. CHATTOOK ..2.)..-seeeae--e- meee eee 808 4, Experiments on the Influence of Electricity on Plants. By Srxim Lem- BSINROM. cost cen edadencsecmuibuessciist oe siieaes dens stociaees ouedahie sence oat sc nem 808 5. The Action of Electricity upon Plants. By E. H. Coox, D.Sc. ............ 809 6. *Experiments with the Brush Discharge. By E. H. Coox, D.Se. ......... 810 7. The Ancient Standard Weights and Measures of the City of Bristol. By DWV Et PSATRICE 0). 0/00) isiescienicos oo se lsoecmrasiec der asetesssideteeh heats 810 8. Some Preliminary Experiments on the Luminosity produced by striking Sugar, By J. BURKE, M-A. oo... s.0.cecess.sscnscnscnsaeoenes reeset eae ea 810 9. On the Electromagnetic Theory of Reflection on the Surface of Crystals. Bysr@a as. Be CURRY. 0.0.002.2se0escnspersaracceesannnnecenet acs eta 811 Section B.—CHEMISTRY. THURSDAY, SEPTEMBER 8. Address by Professor Ff. R. Japp, M.A., LL.D., F.R.S., President of the oF oo RS OPERA. cs ass Sete ema ersie's v's os ccsn ciolidapinateiloccisls oa wie COUAERIINcL cea: ke ae 813 . On the Extraction from Air of the Companions of Argon and on Neon. By Wrtriam Ramsay and Morris W. TRAVERS ...........:seeccessceeeeseeee 828 . *On the Position of Helium, Argon, Krypton, &c., in the Periodic Classi- fication of the Elements. By Professor J. Emerson Ruynotps, F.R.S.... 830 . Report on the Electrolytic Methods of Quantitative Analysis ............... 830 *A4 new form of Stand for Electrolytic Analysis. By Dr. Hue MarsHart 830 . Report on the Continuation of the Bibliography of Spectroscopy ......... 830 ies 2. to CONTENTS. XVil FRIDAY, SEPTEMBER 9. Page Some Researches on the Thermal Properties of Gases and Liquids. By PeMeUNea YOUNG OUD SIC), Luss sa yess cacat ove daedpscewavlescpsuslaclaecesedsssGenatety 831 On the Action of certain Metals and Organic Bodies on a Photographic Rea NY.) ERUSSEEE, Ett) BES. ccyiassscssecsscgesesccperscescnsstoahe 834 . The Action of Bacteria on the aman Plate. By Percy Franx- RS HSU SSC Ho wcSsutadacctscccddcupseee oncspsupestigecbsletatebagusadsoar ates 835 . Further aa eee on the Absorption of the Réntgen Rays by Chemical Compounds. By J. H.Guapsronz, D.Sc., F.R.S , and Warr Hrpert 835 . Report on the Action of Light upon Dyed Colours .................cceeeeeees 836 . On the Cooling Curves of Fatty Acids. By Dr. A. P. Laurte and E. Il. “TEV AO) S10 SPREE ao Sec et Gh A Seed Ane NS a a a oe 836 . On the More Exact Determination of the Densities of Crystals. By BHEBIAB TRO: MRR oac arte acclees cus sane alasmemesceeebersdeneesucsueeat auearics 837 . The Equivalent Replacement of Metals. By Professor Frank CLowzs, MMSE ETE Cle Mees et ces c.iceetrie niches aaleiies salciars Sasiat gate RDONASEC ae est nieces aE 838 9. A note on Alkaline Chlorates and Sulphates of Heavy Metals By W. BEEMONGICINGON ANd AW EL, COOTE. 1... 2.cct..codeccivenovetetddivndeddcescade die 839 MONDAY, SEPTEMBER 12. “A Discussion on the recent Eclipse Expeditions ............ccccccceecceececeseccaes 840 1. Report on the Teaching of Natural Science in Elementary Schools ... .. 840: 2, *Juvenile Research. By Professor H. E. Armstrong, F.R.S. ............ 840 3. Green Cobaltic Compounds. The Result of Oxidising Cobaltous Salts in presence of Organic Salts of the Alkali Metals. By R. G. Durrant, a array oso eginkap «unm sine Yo und ade emsannssanageainat es diag tatoo. che 840 4, Bivelysis of Dorsetshire Soils. By C. M. Luxmoors, D.Sc., F.L.C.’ ...... S£1 5. Report on the Carbohydrates of Cereal Straws ............ecccseccceeeeeeccenes 842 G. Interim Report on the Promotion of Agriculture ...............ccccceecceeeees 842 TUESDAY, SEPTEMBER 13. 1. Recent Advances in the Leather Trade. By J. Gorpon Parxer, Ph.D. 842 . Diamidated Aromatic Amidines, a New Class of Colouring Matters. By BTC SE LEG N ONEUIN GG: acilsinsts cacscneicetesssalecdeccwncrendtstey Rvectncthe we dklges 845 . The Oxidation of Glycerol in presence of Ferrous Iron. By Henry J. Horstman Fenton, M.A., and Henry Jacnson, B.A., B.Se. ............ 844 . Action of Hydrogen Peroxide on Carbohydrates in the Presence of a e Salts. By R.S. Morrert, M.A., Ph.D., and J. M. Crorrs, B.A., B.Sc. . “An Experiment illustrating the Effect on the Acetylene Flame of vary- ing proportions of Carbon Dioxide in the Gas. By Professor J. PAMPIRSONPLUMUN OTDS, Heke they cots sgediaesssaceonnedssdivcencacawesaees sostesnes 845 6. On a 10-Candle Lamp to be as a Standard of Light. By A. G. 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Sinks x 5's Sisfulb\areaiale Deal, Song a “Tod ‘hay PIBAPA Tig "Moy qu sly euL sere teense eer oe ‘Su MOT osarl “ayy “ood ‘Sounog. 3) 7 TOSSEJOAg | “es sq Toqsiig Jo doysig pro7y ot “ey qUSTY on, Ssi¥iahe ieidvie\e(s givivit'aieto oumecsex vay: “Sa ‘slong jo [leq aq} ‘TOR qq S8iy eTLT, 0yU0I0J, Jo 4ISIOATU 949 JOJUSpIserg “CTT “y'w ‘uopnoT re qOssejoIg sreresees* OUNOIOT, Jo IOLBA OUL “SHA “O'W'O ‘Wosmeq urenyt AM arg Wereeeeeeeuueecettinersequaessteaanererseertenesss* BDB—B) JOH JouoIssTMIMON YSIH “ATT “H'W'O'D ‘UMS "WV PIBUOg Ig ‘aOR oy, ODOR ONOOROOF | Hs tq hs HG) “o-WwO) “qegq Sreddny, seTIVuy ag ‘U0 eu, “*****OT1BjUGQ JO VUTAOCI_ 944 LOf MOMVONPY JO 1eqstaryy oy} ‘aoR oy, streeeeececececeses* OLIBIUQ JO VOUTAOIG 949 JO JelMeIg oT} WOH oy, “*****O11B4UO JO BOUTAOIg 0} JO IOUIaAOH-JUBUAQUaL'T 844 InowoH sty Vite terteetegetecereseereeseteceeeeeeeee @DBEBD Jo WOTHLMOE, oy} JO JOWSTUIW CUI “HY W'O') “AoMuveT PHIM Ug ‘woH a4Z, ‘ESA “SW “ATT “TO “O'A'0'9 ‘UrAley ploy ‘uoH 4ySIy oUL, DUM OS OOO FOOT TIO. fa 7p “TO'A We *qs10, hey ploy ‘uo aus oul Te eteececeucveceseeec-+* epeney Jo MOIUIMOd eT JO [e1euey-IJ0n “WAH “H'W'O'D ‘Teepseqy Jo [eq 8g} ‘MOH WYSIY 04} AoueTeoxg BI, “bsg ‘WOStTIE “8 “fr "S'la “sy “TONTEM “H 'd "Ud “AW ‘mNyTeoePY “gq “VY JOssejo1g “L681 ‘81 ysnsny ‘oLNouoz, Ree ie ha et Rae eae ie “g'N'00g 107 “W'S iT SW'seary “C's “aT T0'd “g'0'N ‘SNVAR NHOLUIS tee eee ee ee ee ey "SW ‘eBpistoary “y rosseyorg eee eee eee eee eee ey ee oe aes a a rr eee eneee "“"S'0'd"A Coa y “Dsq ‘saxoorlp, "MA ee ee ee en ed "a'TT “bsg ‘ouoqyyey “A Hee eee ee rere ween wees joodzeary ‘aZa1109 AqISIOATA jo jedpourg ouL ee | oy dialeratiaaa a gee * nh “T'O'd ‘e0osoy “gq Aue Ig ete ee eee ee eee ee ee ee es ‘da’f ‘poomio,y ‘g *A\ IIS ‘eITYSBOUBT Jo JURUAINELT-ploT “Hy ‘W0#Jag jo [7eq oN4 “MOR WU SryY oy, ** ‘joodueary Jo r0AeTY pr0T “g'O'H ‘Aqaeq Jo [AB 049 ‘uoH WqQSTY ou, “bsg SHUTTIEM “HM ween 'S'T'a “bsq ‘aosdmoyy, *O ovesy ‘SW ‘ueulpiey “VY “MA TOssazorg “9681 ‘9T tequieydag ‘tooauHArT eeneee eas eee - on ios aS A£ya100g pshoy amy jo qaepyseig “CIT “TO'A “Iva ‘MHLISIT HdwSOL WIS ‘Suu “TO'd ‘Puepuey gid “saa “TO'd “qq ‘29099 “D “D IIg oe ee ee ee 2 2 a es qormsdy jo tofkepy “Daa ‘qo19.18q "A "ft ‘bag ‘horpng «ar og: | MPUSPIPUOY PIOT “MOR INSIY oT, “V'S'A ‘LOMLUUEH POT "MoH, Sty on I, OSE “ITT “Ve “bsg aIMON oy a] cL Wold] jo prsaoag UStH SVN X(pdAmy pxOT “WOH ISI og Sa NTT 'V bem ‘Wosyomoyl “Pep \ 227 X088UL JO guBUA;NOY]-pIOT ‘ ¥'y'09g “TST 1heY PIT “WOH SY OL 4 HD |israccasespatcatasvyron sverts siter nas og percent aa sues 94} JO preMS SIH “SU “AIT ‘Weysuisyem ploy ‘uo 4qSTY ONT, oe ee i ei ee irs sloyNg jo Ayun09 oy} Jo JUBMOWNAYT~"pIO'T “WF ‘OPAC Jo sMbavy_ 04} “WOH yeoyy on, ; “C681 ‘TI toqmieydeg ‘HoOrMsayT t eeeee ee eeeee ae eee ‘SOU “Sow “ora “a'qt ‘TO'd “@O'N ‘NOLIVN SYTNNOG YIS NIVLavo PAST PRESIDENTS, VICE-PRESIDENTS, AND LOCAL SECRETAR wg “bse “proqqop *E XET ‘Sa “VW ‘UTMIeg "AD = Eee ee hii REPORT—1898. TRUSTEES AND GENERAL OFFICERS, 1831—1899. TRUSTEES. 1832-70 as R. I. MurcHison (Bart.), RS. 1832-62 his TAYLOR, Esq., F.R.S. 1832-39 C. BABBAGE, Esq., F.R.S. 1839-44 F. BAILy, Esq., ERS. 1844-58 Rev. G. PEACOCK, F.R.S. 1858-82 General E. SABINE, F.RS. 1862-81 Sir P. EGERTON, Bart., F.R.S. 1872-99 Sir J. LUBBOCK, Bart., F.R.S. 1861-83 W. SPOTTISWOODE, Esq., Pres. RS. 1883 99 Lord RAYLEIGH, F.RS. 1883-98 Sir Lyon (now Lord) PLAYFAIR, F.R.S. 1898-99 Prof. A. W. RUCKER, F.R.S. GENERAL TREASURERS. 1831 JONATHAN GRAY, Esq. 1832-62 JOHN TAYLOR, Esq. F.R.S. 1862-74 W. SPOTTISWOODE, Esq., F.R.S. 1874-91 Prof. A. W. WILLIAMSON, F.R.S. 1891-98 Prof. A. W. RUcKER, F.R.S. 1898-99 Prof. G. C. FostEr, F.R.S. GENERAL SECRETARIES, 1832-35 Rev. W. F.R.S. 1835-36 Rev. W. VERNON HARCOURT, F.R.S., and F, Batty, Esq., F.RS. 1836-37 Rev. W. Vurnon Harcourt, ¥.R.S., and R. I. Murcurson, Ksq., F.R.S. 1837-39 R. I. Murcnison, Esq., F.R.S., and Rev. G. Peacock, F.R.8. t839_45 Sir R. I. Murcuison, F.R.S., and Major E. SABINE, F.R.S. 1845-50 Lieut.-Colonel E. SABINE,I.R.S. 1850-52 General E. SABINE, F.R.S., and J.F. ROoYLE, Esq., F.R.S. 1852-53 J. F. Royue, Esq., F.R.S. 1853-59 General EK. SABINE, F.R.S. 1859-61 Prof. R. WALKER, F.R.S. 1861-62 W. Hopkins, Esq., F.R.S. 1862-63 W. Hopkins, Esq., F.R.S., and Prof. J. PHILLIPS, F.R.S. 1863-65 W. Hopxins, Esq., F.R.S., and F. GALTON, Esq., F.R.S. 1865-66 F. GALTON, Esq., F.R.S. VERNON HARCOURT, 1866-68 F. GALTON, Esq., F.R.S., and Dr. T. A. Hirst, F.R.S. 1868-71 Dr. T. A. Hirst, F.R.S., and Dr. T. THOMSON, F.R.S. 1871-72 Dr.T. THOMSON,F.R.S.,and Capt. DovuGLas GALTON, F.R.S. 1872-76 Capt. DouGLAS GALTON. F.B.S., and Dr. MICHAEL FOSTER, F.R.S. 1876-81 Capt. DoUGLAS GALTON, F.R.S., and Dr. P. L. SCLATER, F.RB.S. 1881-82 Capt. DoUGLAS GALTON, F.R.S., and Prof. F. M. BALFOUR, F.R.S. 1882-83 Capt. DoUGLAS GALTON, F.R.S. 1883-95 Sir DouGLAs GALTON, F.R.S., and A. G. VERNON HARCOURT, Esq., F.R.S. 1895-97 A. G. VERNON HARCOURT, Esq., F.R.S., and Prof. HE. A. SCHAFER, E.R.S. 1897-99 Prof. E. A. SCHAFER, F.R.S., and Prof. W. C. ROBERTS-AUSTEN, C.B., F.R.S. ASSISTANT GENERAL SECRETARIES. 1831 JOHN PHILLIPS, Esq., Secretary. | 1881-85 Prof. T. G. 1832 Prot. J: D; Secretary. 2832-62 Prof. JoHN PHILLIPS, F.R.S. 1862-78 G. GRIFFITH, Esq., M.A. 1878-80 J. E. H. Gorpon, Esq., B.A., Assistant Secretary. G, GewritH, Esq., M.A., Acting Secretary. ForBES, Acting 1881 Bonney, F.BS., Secretary. 1885-90 A. T. ATCHISON, Esq., M.A., Secretary. 1890 G. GRIFFITH, Esq., M.A., Acting Secretary. 1890-99 G. GRIFFITH, Esq., M.A. — TT Presidents and Secretaries of the Sections Date and Place 1832. 1833. 1834. 1835. 1836. 1837. 1838. lini of the Association. Presidents Secretaries MATHEMATICAL AND PHYSICAL SCIENCES. COMMITTEE OF SCIENCES, I.—MATHEMATICS AND GENERAL PHYSICS. Cainbridge Edinburgh Dublin...... Bristol...... Liverpool... Newcastle 1839. Birmingham 1840. Glasgow ... 1841. 1842. 1843. 1844, 1845. 1846. _ «*1847. 1848. Plymouth Manchester Cambridge Southamp- Swansea ... 1849. Birmingham 1850. 1851. — 1852. 1853. Edinburgh Ipswich .., Belfast...... Hull eee ee wees Davies Gilbert, D.C.L., F.R.S. Sir D. Brewster, F.R.S. ...... Rev. W. Whewell, F.R.S. Rev. H. Coddington. Prof. Forbes. Prof. Forbes, Prof. Lloyd. SECTION A.—MATHEMATICS AND PHYSICS. Rev. Dr. Robinson Rev. William Whewell, F.R.S. Sir D. Brewster, F.R.S. ...... Sir J. F. W. Herschel, Bart., F.RB.S. Rey. Prof. Whewell, F.R.S.... Prof. Forbes, F.R.S...........0. Rev. Prof. Lloyd, F.R.S....... Very Rev. G. Peacock, D.D., F.R.S. Prof. M‘Culloch, M.R.I.A. ... The Earl of Rosse, F.R.S. ... The Very Rev. the Dean of Ely. Sir John F. W. Herschel, Bart., F.R.S. Prof. Powell, F.R.S. Lord Wrottesley, F.R.S. ...... William Hopkins, F.R.S....... M.A., Prof. J. D. Forbes, F.R.S., Sec. R.S.E. ../Rev. W. Whewell, D.D., F.R.S. Prof. W. Thomson, M.A., E.B.S., F.R.S.E. The Very Rev. the Dean of Ely, F.R.S. 1854, Liverpool...| Prof. G. G. Stokes, M.A., Sec. RS 1855. Glasgow .../Rev. Prof. Kelland, M.A, F.R.S., F.R.S.E. 1856, Cheltenham | Rev. R. Walker, M.A., F.R.S. Prof. Sir W. R. Hamilton, Prof. Wheatstone. Prof. Forbes, W. S. Harris, F. W. Jerrard. W. S. Harris, Rev. Prof. Powell, Prof. Stevelly. Rev. Prof. Chevallier, Major Sabine, Prof. Stevelly. J. D. Chance, W. Snow Harris, Prof. Stevelly. Rev. Dr. Forbes, Prof. Stevelly, Arch. Smith. Prof. Stevelly. Prof. M‘Culloch, Prof. Stevelly, Rev. W. Scoresby. J. Nott, Prof. Stevelly. Rev. Wm. Hey, Prof. Stevelly. Rev. H. Goodwin, Prof. Stevelly, G. G. Stokes. John Drew, Dr. Stevelly, G. G. Stokes. Rev. H. Price, Prof. Stevelly, G. G. Stokes. Dr. Stevelly, G. G. Stokes. Prof. Stevelly, G. G. Stokes, W. Ridout Wills. W.J.Macquorn Rankine,Prof.Smyth, Prof. Stevelly, Prof. G. G. Stokes. S. Jackson, W. J. Macquorn Rankine, Prof. Stevelly, Prof. G. G. Stokes. Prof. Dixon, W, J. Macquorn Ran- kine, Prof. Stevelly, J. Tyndall. B. Blaydes Haworth, J. D. Sollitt, Prof. Stevelly, J. Welsh. J. Hartnup, H. G. Puckle, Prof, Stevelly, J. Tyndall, J. Welsh. Rev. Dr. Forbes, Prof. D. Gray, Prof. Tyndall. C. Brooke, Rev. T. A. Southwood, Prof. Stevelly, Rev. J. C. Turnbull. liv REPORT—1898. Secretaries Date and Place Presidents 1857. Dublin...... Rev. T. R. Robinson, F.R.S., M.R.IA. 1858. Leeds ...... Rev. W. Whewell, V.P.R.S 1859. Aberdeen... F.R.S. 1860. Oxford...... 1861. Manchester F.R.S. Prof. G. G. Stokes, F.R.S. 1862. Cambridge 1863. Newcastle C.H., F.R.S. 1864. Bath......... F.R.A.S. 1865. Birmingham |W. Spottiswoode,M.A.,F.R.5., F.R.A.S. 1866. Nottingham|Prof. Wheatstone, D.C.L., F.R.S. 1867. Dundee F.R.S 1868. Norwich ... E.R.S. 1869. Exeter...... F.R.S. 1879. Liverpool...|J. Clerk Maxwell, LL.D., F.R.S. 1871. Edinburgh 1872. Brighton... 1873. Bradford ... 1874. Belfast...... Rev. Prof. J. H. Jellett, M.R.LA. 1875. Bristol...... Prof. Balfour Stewart, LL.D., F.R.S. Prof. Sir W. Thomson, D.C.L., F.R.S. 1876. Glasgow ... 1877. Plymouth... Pres. Physical Soe. 1878. Dublin...... Rev. Prof. Salmon, D.C.L., F.B.S. 1879. Sheffield ...|George Johnstone M.A., F.R.S. 1880. Swansea ...|Prof. W. Grylls Adams, F.R.S. Prof. Sir W. Thomson, LL.D., D.C.L., F.B.S. GD MORK. 25.0232 1882. Southamp- ton. M.A., F.R.S. The Harlof Rosse, M.A., ...|Prof. Sir W. Thomson, D.C.L., J. Tyndall, LL.D., Prof. P. G. Tait, F.R.S.E. ... D.D.,|Prof. Curtis, Prof. Hennessy, P. A. Ninnis, W. J. Macquorn Rankine, Prof. Stevelly. D.D.,|Rev. S. Earnshaw, J. P. Hennessy, Prof. Stevelly, H.J.S.Smith, Prof. Tyndall. K.P.,| J. P. Hennessy, Prof. Maxwell, H. J.S. Smith, Prof. Stevelly. Rev. B. Price, M.A., F.R.S....] Rev. G. C. Bell, Rev. T. Rennison, Prof. Stevelly. G. B. Airy, M.A., D.C.L.,} Prof. R. B. Clifton, Prof. H. J. 8S. Smith, Prof. Stevelly. M.A.,| Prof. R. B. Clifton, Prof. H. J. S. Smith, Prof. Stevelly. Prof.W.J. Macquorn Rankine,| Rev. N. Ferrers, Prof. Fuller, F. Jenkin, Prof. Stevelly, Rev. C. T. Whitley. Prof. Cayley, M.A., F.R.S.,| Prof. Fuller, F. Jenkin, Rev. G. Buckle, Prof. Stevelly. Rev. T. N. Hutchinson, F. Jenkin, G. S. Mathews, Prof. H. J. S. Smith, J. M. Wilson. Fleeming Jenkin,Prof.H.J.S. Smith, Rey. 8. N. Swann. Rev. G. Buckle, Prof. G. C. Foster, Prof. Fuller, Prof. Swan. Prof. G. C. Foster, Rev. R. Harley, R. B. Hayward. Prof. J. J. Sylvester, LL.D.,|Prof. G. C. Foster, R. B. Hayward, W. K. Clifford. M.A.,| Prof. W. G. Adams, W. K. Clifford, Prof. G. C. Foster, Rev. W. Allen Whitworth. Prof. W. G. Adams, J. T. Bottomley, Prof. W. K. Clifford, Prof. J. D. Everett, Rev. R. Harley. W. De La Rue, D.C.L., F.R.S.| Prof. W. K. Clifford, J. W. L.Glaisher, Prof. A. S. Herschel, G. F. Rodwell. Prof. H. J. 8. Smith, F.R.S. .|Prof. W. K. Clifford, Prof. Forbes, J. W.L. Glaisher, Prof. A.S. Herschel. M.A.,|J. W. L. Glaisher, Prof. Herschel, Randal Nixon, J. Perry, G. F. Rodwell. M.A.,| Prof. W. F. Barrett, J.W.L. Glaisher, C. T. Hudson, G. F. Rodwell. M.A.,| Prof. W. F. Barrett, J. T. Bottomley, Prof. G. Forbes, J. W. L. Glaisher, T. Muir. Prof, G. C. Foster, B.A., F.R.S.,| Prof. W. F. Barrett, J. T. Bottomley, J. W. L. Glaisher, F. G. Landon. D.D.,|Prof. J. Casey, G. F. Fitzgerald, J. W. L. Glaisher, Dr. O. J. Lodge. Stoney,|A. H. Allen, J. W. L. Glaisher, Dr. O. J. Lodge, D. MacAlister. M.A.,)W. E. Ayrton, J. W. L. Glaisher, Dr. O. J. Lodge, D. MacAlister. M.A.,|Prof. W. E. Ayrton, Dr. O. J. Lodge, D. MacAlister, Rev. W. Routh. Rt. Hon. Prof. Lord Rayleigh,|W. M. Hicks, Dr. O. J. Lodge, D. MacAlister, Rey. G. Richardson. ed al - ee, ae or *+ PRESIDENTS AND SECRETARIES OF THE SECTIONS. lv Date and Place 1883. 1884. 1885. 1886. 1887. 1888. 1889. 1890. 1891. 1892. - 1893. 1894. 1895. 1896. 1897. 1898. 1832. 1833. 1834. 1835. 1836. 1837. 1838. Newcastle 1839. Birmingham 1840. 1841. 1842. 1843. 1844. 1845. 1846, Southport Montreal ... Presidents Secretaries Prof.O. Henrici, Ph.D., F.R.S.|W. M. Hicks, Prof. O. J. Lodge, D. MacAlister, Prof. R. C. Rowe. 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. Aberdeen...|Prof. G. Chrystal, M.A.,|R. E. Baynes, R. T. Glazebrook, Prof, F.R.S.E. W. M. Hicks, Prof. W. Ingram. Birmingham |Prof. G. H. Darwin, M.A.,)R. E. Baynes, R. T. Glazebrook, Prof. LL.D., F.R.S. J. H. Poynting, W. N. Shaw. Manchester |Prof. Sir R. 8S. Ball, M.A.,/R. E. Baynes, R. T. Glazebrook, Prof. LL.D., F.R.S. H. Lamb, W. N. Shaw. Bath .......<. Prof. G. F. Fitzgerald, M.A.,|R. E. Baynes, R. T. Glazebrook, A F.RB.S. Lodge, W. N. Shaw. Newcastle- |Capt. W. de W. Abney, C.B.,|R. H. Baynes, R. T. Glazebrook, A. upon-Tyne| R.H., F.R.S. Lodge, W. N. Shaw, H. Stroud. Leeds ...... J. W. L. Glaisher, Sc.D.,|R. T. Glazebrook, Prof. A. Lodge, F.R.S., V.P.R.A.S. W.N. Shaw, Prof. W. Stroud. Cardiff -....: Prof. O. J. Lodge, D.Sc.,)R. E. Baynes, J. Larmor, Prof. A. LL.D., F.R.S. Lodge, Prof. A. L. Selby. Edinburgh |Prof. A. Schuster, Ph.D.,)R. E. Baynes, J. Larmor, Prof. A. F.R.S., F.R.A.S. Lodge, Dr. W. Peddie. Nottingham|R. T. Glazebrook, M.A., F.R.S.|W. T. A. Emtage, J. Larmor, Prof. A. Lodge, Dr. W. Peddie. Oxford)...... Prof. A. W. Riicker, M.A.,| Prof. W. H. Heaton, Prof. A. Lodge, F.R.S. J. Walker. Ipswich ...|Prof. W. M. Hicks, M.A.,| Prof. W. H. Heaton, Prof. A. Lodge, F.R.S. G. T. Walker, W. Watson. Liverpool...|Prof. J. J. Thomson, M.A.,|Prof. W. H. Heaton, J. L. Howard, D.Sc., F.R.S. Prof. A. Lodge, G. T. Walker, W. Watson. Toronto ...|Prof. A. R. Forsyth, M.A.,|Prof. W. H. Heaton, J.C. Gissian, J. F.R.S. L. Howard, Prof. J.C. McLennan. Bristol ...... Prof W. E. Ayrton, F.R.S. ...|Prof. A. P. Chattock, J. L. Howard, C. H. Lees, Prof, W. Watson, E. T. Whittaker. CHEMICAL SCIENCE. COMMITTEE OF SCIENCES, IIl.—CHEMISTRY, MINERALOGY. Oxford...... John Dalton, D.C.L., F.R.S. |James F. W. Johnston. Cambridge |John Dalton, D.C.L., F.R.S. | Prof. Miller. Edinburgh | Dr. Hope..............scceececeeees Mr. Johnston, Dr. Christison. SECTION B.—CHEMISTRY AND MINERALOGY. Dublin...... Dr. T. Thomson, F.R.S. .|Dr. Apjohn, Prof. Johnston. Bristol...... Rey. Prof. Cumming ......... |Dr. Apjohn, Dr. C. Henry, W. Hera- ath. Liverpool...| Michael Faraday, F.R.S....... pape. Johnston, Prof. Miller, Dr. Reynolds. Rey. William Whewell,F.R.S. Prof. T. Graham, F.R.S. Prof. Miller, H. L. Pattinson, Thomas | Richardson. . Dr. Golding Bird, Dr. J. B. Melson. |Dr. R. D: “Thomson, Dr. ‘Tf. Clark, Dr. L. Playfair. Glasgow .,.| Dr. Thomas Thomson, F.R.S. Plymouth...|Dr. Daubeny, F.R.S. ......... Manchester | John Dalton, D.C.L., F.R.S. Cork..5;.29%5 Prof. Apjohn, M.R.1.A......... OTIC osc ’ae Prof. T. Graham, F.R.S.. Cambridge | Rev. Prof. Cumming ......... Southamp- | Michael Faraday, D.C.L., ton. F.R.S. J. Prideaux, R. Hunt, W. M. Tweedy. | Dr. L. Playfair, R. Hunt, J. Graham, |R. Hunt, Dr. Sweeny. ..| Dr. L, Playfair, E. Solly, T. H. Barker. |R. Hunt, J. P. Joule, Prof. Miller, i. Solly. Dr. Miller, R. Hunt, W. Randall. lvi REPORT—1898. Date and Place 1847. Oxford...... 1848. Swansea ... 1849. Birmingham 1850. Edinburgh 1851. Ipswich ... 1852. Belfast...... Rev. W. V. Harcourt, M.A., Presidents 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. | 1853. Hull......... 1854. Liverpool 1855. Glasgow .. 1856. Cheltenham | 1857. Dublin weeeee 1858. Leeds ...... 1859. Aberdeen... 1860. Oxford seeeee 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... | ...|Dr. Lyon Playfair,C.B.,F.R.S. | Prof. W.H. Miller, M.A.,}.B.S. |W. Odling, M.B., F.R.S....... see IEYOL. Prof. J. F. W. Johnston, M.A., F.R.S, Prof.W. A.Miller, M.D.,F.R.S. 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.S. Prof. B. C. Brodie, F.R.S...... Prof. W.A.Miller, M.D.,F.R.S. | Dr. Alex. W. Williamson, F.R.S. Prof. W. A. V.P.R.S. H. Bence Jones, M.D., F.R.S.! Miller, M.D., T. Anderson, F.R.S.E. Prof. E. Frankland, F.R.S. M.D., (Dy, SH Debus, He Resse. ceagtece | \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., | F.R.S. WViemterrerkin. \H RAS: ie. cert BEA REA DEL MH Ee. Ounvcsescnecdeuee 1878, Dublin......| 1879. Sheffield ... | Prof. Maxwell Simpson, M.D., | F.R.S. Prof. Dewar, M.A., F.R.S. ... Secretaries 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. 8. 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. Livein A. B. Northcote. A. Vernon Harcourt, G. D. Liveing. H. W. Elphinstone, W. Odling, Prof. Roscoe. i Prof. Liveing, H. L. Pattinson, J. €. 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. g> /Prof. A. Crum Brown, Dr. W. J. Russell, Dr. Atkinson. Prof. A. Crum Brown, A. E. Fletcher, Dr. W. J. Russell. J.T. Buchanan, W. N. Hartley, F. 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. H. 8S. Bell, W. Chandler Roberts, J. M. Thomson. PRESIDENTS AND SECRETARIES OF THE SECTIONS. Date and Place 1880. 1881. 1882. 1883. 1884. 1885. Swansea ... Southamp- ton, Southport Montreal ... Aberdeen... 1886, Birmingham 1887. 1888. E 1889. 1890. 1891. 1892. 1893. 1894. 1895. 1896. 1897. 1898. Manchester Newcastle- upon-Tyne Leeds Cardiff ...... Edinburgh Nottingham Oxiford)...... Ipswich Liverpool... Toronto Bristol ...... lvii \Prof. W. A. Tilden, \Prof. T. E. Thorpe, Presidents Joseph Henry Gilbert, Ph.D.,| F.R.S. Prof. A. W. Williamson, F.R.S. Prof. G. D. Liveing, M.A., F.R.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. ..:... D.S8c.,| F.R.S., V.P.C.S. Sir I. Lowthian Bell, Bart., D.C.L., F.B.S. B.Sc.,| Ph.D., F.R.S., Treas. C.S. Prof. W. C. Roberts-Austen, | C.B., F.R.S. Prof. H. McLeod, F.R.S....... Prof. J. Emerson Reynolds, | Secretaries P. P. Bedson, H. B. Dixon, W. R. E. Hodgkinson, J. M. Thomson. P. P. Bedson, H. B. Dixon, T. Gough. P. Phillips Bedson, H. Bb. 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, M.D., D.Sc., F.R.S. Prof. H. B. Dixon, M.A., F.R.S., | 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. ......| Dr. Ludwig Mond, F.R.S. | ...|Prof. W. Ramsay, F.B.S....... Prof, F. R. Japp, F.B.S, ae BE. H. Fison, Arthur Harden, C. A. Kohn, J. W. Rodger. Arthur Harden, C. A. Kohn Prof. W. H. Ellis, A. Harden, C. A- Kohn, Prof. R. F, Ruttan. C. A. Kohn, F. W. Stoddart, T. K. Rose. GEOLOGICAL (anv, untit 1851, GEOGRAPHICAL) SCIENCE. COMMITTEE OF SCIENCES, IJIL.—GEOLOGY AND GEOGRAPHY. 1832. 1833. 1834. 1835. 1836. 1837. 1838, Oxford...... Cambridge. Edinburgh . Dublin...... Bristol ...... Liverpool... Newcastle. . 1839, Birmingham R. I. Murchison, F.R.S. ...... G. B. Greenough, F.R.S. ...... Prof, Jameson Bere m ese ereesenree SECTION C.—GEOLOGY AN Fed) LUDO) teas earaatesccsesves Rey. Dr. Buckland, F.R.S.— Geog.,R.I.Murchison,F.R.S. 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. Rev. Dr. Buckland, F.R.S.— Geog.,G.B.Greenough,F.R.S. | John Taylor. W. Lonsdale, John Phillips. J. Phillips, T. J. Torrie, Rev. J. Yates. D GEOGRAPHY. Captain Portlock, T. J. Torrie. William Sanders, S. Stutchbury, T. J. Torrie. Captain Portlock, R. Hunter.—G@eo- 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. lviil Date and Place 1840. 1841. 1842, 1843. 1844. 1845. 1846. 1847. 1848 REPORT—1898. Presidents Secretaries Glasgow ... Plymouth... Manchester sseteeeee se eewenee Cambridge. Southamp- ton. . Swansea... 1849.Birmingham 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.S. ... Henry Warburton, Pres. G. 5. Rev. Prof. Sedgwick, M.A., F.R.S. Leonard Horner, F.R.S. ...... Very Rev.Dr.Buckland,F.R.S. Sir H. T. De la Beche, F.R.8. Sir Charles Lyell, F.R.S., F.G.S. 1850. Edinburgh! |Sir Roderick I. Murchison, 1851 1852 1853 1854. 1855 1856 1857 1858 1859. 1860. 1861 1862 1863 1864. 1865 1866 . Ipswich ... . Belfast eeneee . Hull Liverpool.. . Glasgow . Cheltenham . Dublin pPLICLOS) i... sss Aberdeen... Oxford...... . Manchester . Cambridge . Newcastle . Birmingham . Nottingham le CEES. SECTION C (continued). William Hopkins, M.A.,F.R.S. Lieut.-Col. Portlock, R.E., F.R.S. Prof. Sedgwick, F.R.S......... Prof. Edward Forbes, F,R.S. ...|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.B.S. J. Beete Jukes, M.A., F.R.S. TBs Prof. Warington W. Smyth, F.R.S., F.G.8. Prof. J. Phillips, LL.D., F.RB.S., F.G.S. Sir R. I. Murchison, Bart., K.C.B. Prof. A. C. Ramsay, LL.D., E.R.S. W. J. Hamilton, D. Milne, Hugh Murray, H. E. Strickland, John Scoular, M.D. W.J. Hamilton, Kdward Moore, M.D., R. Hutton. KE. W. Binney, R. Hutton, Dr. R. Lloyd, H. E. Strickland. F. M. Jennings, H. E. Strickland. Prof. Ansted, E. H. Bunbury. Rev. J. C. Cumming, A. C. Ramsay, Rey. W. Thorp. Robert A. Austen, Dr. J. H. Norton, Prof. Oldham, Dr. C. T. Beke. Prof. Ansted, Prof. Oldham, A. C. Ramsay, J. Ruskin. S.Benson, Prof.Oldham, Prof.Ramsay. 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. J. Bryce, Prof. Harkness, Prof. Nicol. Rev. 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, i. W. Shaw. Prof. Harkness, Rev. J. Longmuir, H. C. Sorby. |Prof. Harkness, Edward Hull, Capt. Woodall. Prof. Harkness, Edward Hutl, 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. W. B. Dawkins, J. Johnston, H. C. Sorby, W. Pengelly. Rey. P. B. Brodie, J. Jones, Rev. HE. Myers, H. C. Sorby, W. Pengelly. |\R. Etheridge, W. Pengelly, T. Wil- son, G. H. Wright. » Geography was constituted a separate Section, under the title of the ‘Geo- graphical and Ethnological Section,’ see page lxiv. —- PRESIDENTS AND SECRETARIES OF THE SECTIONS. Date and Place 1867. 1868. 1869. 1870. 1871. 1872. 1873. 1874. 1875. 1876. 1877. 1878. 1879. 1880. 1881. 1882. 1883. 1884. "1885. 1886. 1887. 1888. 1889. 1890. 1891. 1892. 1893. 1894. 1895. 1896. 1897. 1898. Dundee Norwich ... Exeter ...... Liverpool... Edinburgh Brighton... Bradford ... Glasgow a3 Plymouth... Dublin...... Sheffield ... Swansea ... Southamp- ton. Southport Montreal ... Aberdeen ... Birmingham Manchester eee eeeee Newcastle- upon-Tyne Leeds seeeee aeteee Edinburgh Nottingham Oxford’..sss: Ipswich ... Liverpool... Toronto Bristol Presidents .| Archibald Geikie, F.B.S. R. A. C. Godwin-Austen, F.RB.S., F.G.S. Prof. R. Harkness, F.R.S., F.G.S. 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, E.R.S., F.G.S. Prof. J. Phillips, D.C.L., F.B.S., F.G.S. Prof. Hull, M.A., F.R.S., F.G.8. Dr. T. Wright, F.R.S.E., F.G.S. .|Prof. John Young, M.D. ...... W. Pengelly, F.R.S., F.G.S. Jobn Evans, D.C.L., F.R.S., F.S.A., F.G.S. Prof. P. M. Duncan, F.R.S. H. C. Sorby, F.R.S., F.G.S.... A. C. Ramsay, LL.D., F.RB.S., F.G.8. R. Etheridge, F.R.S., F.G.S. Prof. W. C. LL.D., F.R.'. W. T. Blanford, F.B.S,, 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.R.S., F.G.S. Prof. J. Geikie, LL.D., D.C.L., F.R.S., F.G.8. Prof. A. H. Green, E.R.S., F.G.S. Prof. T. Rupert Jones, F.R.S8., B.G.S. Prof. C. Lapworth, LL.D., F.RB.S., F.G.8. J. J. H. Teall, M.A., F.B.S.., F.G.S. L. Fletcher, M.A., F.R.S. Williamson, M.A., W. Whitaker, B.A., F.R.S. ... Jdioth. Marr, Sec. G.S. M.A., F.RB.S., F.R.S. W. H. Hudleston, F.R.S....... lix Secretaries E. Hull, W. Pengelly, H. Woodward. Rev. O. Fisher, Rev. J. Gunn, W. Pengelly, Rev. H. H. Winwood. W. Pengelly, W. Boyd Dawkins, Rev. H. H. Winwood. W. Pengelly, 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. 2 ¥. Adams, Prof. E. W. Claypole, W. Topley, W. Whitaker. Cc. 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. B. Bedford, Dr. F. H. Hatch, J. E. Marr, W. W. Watts. W. Galloway, J. E. Marr, Reid, W. W. Watts. H. M. Cadell, J. E. Marr, Clement Reid, W. W. Watts. J. W. Carr, J. E. Marr, Clement Reid, W. W. Watts. lement .|F. A. Bather, A. Harker, Clement Reid, W. W. Waits. F. A. Bather, G. W. Lamplugh, H. A. Miers, Clement Reid. J. Lomas, Prof. H. A. Miers, Clement Reid. ...|Dr. G. M. Dawson, C.M.G.,|Prof. A. P. Coleman, G. W. Lamp- lugh, Prof. H. A. Miers. G. W. Lamplugh, Prof. H. A. Miers, H. Pentecost. lx REPORT—1898. Date and Place Presidents Secretaries BIOLOGICAL SCIENCES. COMMITTEE OF SCIENCES, IV.—ZOOLOGY, BOTANY, PHYSIOLOGY, ANATOMY, 1832. Oxford...... Rev. P. B. Duncan, F.G.S. ...| Rev. Prof. J. 8. Henslow. 1833. Cambridge’) Rev. W. L. P. Garnons, F.L,S.|C. C. Babington, D. Don. 1834, Edinburgh .| Prof. Graham..................008 |W. Yarrell, Prof. Burnett. SECTION D.—ZOOLOGY AND BOTANY. 1835. Dublin...... SPALL. cess cassswvsccessoos ss J. Curtis, Dr. Litton. 1836. Bristol...... Rey. Prof. Henslow ..........+6 J. Curtis, Prof. Don, Dr. Riley, S. Rootsey. 1837. Liverpool...|W. S. MacLeay............c0c00 iC. C. Babington, Rev. L, Jenyns, W. | Swainson. 1838. Newcastle |Sir W. Jardine, Bart. ......... J. E. Gray, Prof. Jones, R. Owen, Dr. Richardson. 1839. Birmingham | Prof. Owen, F.R.S. ............ |E. Forbes, W. Ick, R. Patterson. 1840. Glasgow ...|Sir W. J. Hooker, LL.D.......| Prof. W. Couper, E. Forbes, R. Pat- terson, 1841. Plymouth... |John Richardson, M.D., F.R.S.| J. Couch, Dr. Lankester, R. Patterson. 1842. Manchester |Hon. and Very Rev. W. Her-| Dr. Lankester, R. Patterson, J. A. bert, LL.D., F.L.S. Turner. 1843. Cork......... William Thompson, F.L.S....\G. J. Allman, Dr. Lankester, R. Patterson. 1844, York......... Very Rey. the Dean of Man- Prof. Allman, H. Goodsir, Dr. King, chester. Dr. Lankester. 1845. Cambridge | Rev. Prof. Henslow, F.L.S...,'Dr. Lankester, T. V. Wollaston. 1846. Southamp- |Sir J. Richardson, M.D., Dr. Lankester, T. V. Wollaston, H. ton. E.R.S. Wooldridge. 1847. Oxford...... H. E. Strickland, M.A., F.R.S. Dr. Lankester, Dr. Melville, T. V. Wollaston. SECTION D (continwed).—zZOOLOGY 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. Isiii.] 1848. Swansea ...)L. W. Dillwyn, F.R.S..........| Dr. R. Wilbraham Falconer, A. Hen- frey, Dr. Lankester. 1849. Birmingham| William Spence, F.R.S. ......| Dr. Lankester, Dr. Russell. 1850. Edinburgh |Prof, Goodsir, F.R.S. L. & E. | Prof. J. H. Bennett, M.D., Dr. Lan- kester, Dr. Douglas Maclagan. 1851. Ipswich .../Rev. Prof. Henslow, M.A., | Prof. Allman, F. W. Johnston, Dr. E. F.R.S. Lankester. 1852. Belfast...... WTO PED Yio store soosonosnseescounes Dr. Dickie, George C. Hyndman, Dr. Edwin Lankester. L853. Hull....:/.0s- C. C. Babington, M.A., F.R.S.|Robert Harrison, Dr. E. Lankester. 1854, Liverpool...|Prof. Balfour, M.D., F.R.S....| Isaac Byerley, Dr. E. Lankester. 1855. Glasgow ...|Rev. Dr. Fleeming, F.R.S.E. | William Keddie, Dr. Lankester. 1856. Cheltenham | Thomas Bell, F.R.S., Pres.L.S.| Dr. J. Abercrombie, Prof. Buckman, Dr. Lankester.~ 1857. Dublin...... Prof. W. H. Harvey, M.D., Prof. J.R.Kinahan, Dr. E. Lankester, F.R.S. | Robert Patterson, Dr, W. E. Steele. + At this Meeting Physiology and Anatomy were made a separate Committee, for Presidents and Secretaries of which see p. I xiii. PRESIDENTS AND SECRETARIES OF THE SECTIONS. Date and Place 1858. Leeds 1859. Aberdeen... 1860. Oxford...... 1861. Manchester 1862. Cambridge 1863. Newcastle 1864. Bath sere eeres 1865. Birming-)|T. Thomson, M.D., F.R.S. ham ! ~ 1866. Nottingnam 1867. Dundee 1868. Norwich ... 1869. Exeter 1870. Liverpool... qi 1871. Edinburgh. 1872. Brighton ... 1873. Bradford ... |Prof. Huxley, F.R.S. ‘Dr. John E. Gray, F.R.S. Presidents lxi Secretaries C. C. Babington, M.A., F.R.S. Sir W. Jardine, Bart., F.R.S.E. ‘Rev. Prof. Henslow, F.L.S.... Prof. C. C. Babington, F.R.S. ee eee eens Prof. Balfour, M.D., F.R.S.... 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. SECTION D (continwed),—BIOLOGY. Prof. Huxley, F.R.S.—Dep.|Dr. J. Beddard, W. Felkin, Rev. H. of Physiol., Prof. Humphry, F.R.S.— Dep. of Anthropol., A. R. Wallace. —Dep. of Zool. and Bot., George Busk, M.D., F.R.S. B. Tristram, W. Turner, E. B. Tylor, Dr. E. P. Wright. ...| Prof, Sharpey, M.D., Sec. R.S.|C. Spence Bate, Dr. S. Cobbold, Dr. M. Foster, H. T. Stainton, Rev. H. B. Tristram, Prof. W. Turner. Rev. M. J. Berkeley, F.L.S.|Dr. T. S. 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., E. B. Tylor. Prof. G. Rolleston, M.A., M.D., F.R.S. F.L.S.—Dep. of Anat. and Physiol., Prof.M. Foster, M.D., F.L.8.—Dep. of Ethno., J. Evans, F.R.S. Prof. Allen Thomson, M.D., F.R.S.—Dep. of Bot. and Zool.,Prof.WyvilleThomson, F.R.S.— Dep. of Anthropol., Prof. W. Turner, M.D. Sir J. Lubbock, Bart., F.R.S.— Dep. of Anat. and Physiol., Dr. Burdon Sanderson, F.R.S.—Dep. of Anthropol., Col. A. Lane Fox, F.G.S. KE. Ray Lankester, Prof. Lawson, H. T, Stainton, Rev. H. B. Tris- tram. Dr. T. S. Cobbold, Sebastian Evans, Prof. Lawson, Thos. J. Moore, H. T. Stainton, Rev. H. B. Tristram, C. Staniland Wake, E. Ray Lan- kester. Dr. T. R. Fraser, Dr. Arthur Gamgee, E. Ray Lankester, Prof. Lawson, H. T. Stainton, C. Staniland Wake, Dr. W. Rutherford, Dr. Kelburne King. Prof, Thiselton-Dyer, H. T. Stainton, Prof. Lawson, F. W. Rudler, J. H. Lamprey, Dr..Gamgee, E. Ray Lankester, Dr. Pye-Smith. Prof. Allman, F.R.S.—Dep. of| Prof. Thiselton-Dyer, Prof. Lawson, 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 The title of Section D was changed to Biology; and for the word ‘Sub- section,’ in the rules for conducting the business of the Sections, the word ‘Deput- ment’ was substituted. lxii REPORT—1898. Date and Place Presidents Secretaries Prof. Redfern, M.D.—Dep. of Zool. and Bot., Dr. Hooker, C.B.,Pres.R.S.— Dep. of An- throp., Sir W.R. Wilde, M.D. P. L. Sclater, F.R.S.— Dep. of Anat. and Physiol., Prof. Cleland, F.R.&.-—Dep. of Anthropol., Prof. Rolleston, F.R.S. , A. Russel Wallace, F.L.S.— Dep. of Zool. and Bot., Prof. A. Newton, F.R.S.— Dep. of Anat. and Physiol., Dr. J. G. McKendrick. J. Gwyn Jeffreys, F.R.S.— Dep. of Anat. and Physiol., Prof. Macalister— Dep. of Anthropol.,F.Galton,F.R.S. 1874. Belfast 1875. Bristol 1876. Glasgow ... 1877. Plymouth... 1878. Dublin...... Prof. W. H. Flower, F.R.S.— Dep. of Anthropol., Prof. Huxley, Sec. R.S.—Dep. of Anat. and Physiol. R. 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., F.R.S. —Dep. of Anthropol., Prof. W. H. Flower, F.R.S.— Dep. of Anat. and Physiol., Prof. J. 8. Burdon Sander- son, F.R.S. Prof. A. Gamgee, M.D., F.R.S. — Dep. of Zool. and Bot., Prof. M. A. Lawson, F.L.S. —Dep. of Anthropol., Prof. W. Boyd Dawkins, F.R.S. Prof. E. Ray Lankester, M.A., F.R.S.— Dep. of Anthropol., W. Pengelly, F.R.S. 1879, Sheffield ... 1880. Swansea ... 1881. York 1882. Southamp- ton.! 1883. Southport ? Prof. H. N. Moseley, M.A., F.RB.S. Prof. W.C. M‘Intosh, M.D.,, LL.D., F.R.S. F.R.S.E. 1884. Montreal ... | 1885. Aberdeen... 1886. Birmingham|W. Carruthers, Pres. L.S., F.R.S., F.G.S8. W.'. 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. EK. 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. Schiifer. G. W. Bloxam, John Priestley, Howard Saunders, Adam Sede- 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. W. Bloxam, W. Heape, J. B. Nias, Howard Saunders, A. Sede- wick, T. W. Shore, jun. G. W. Bloxam, Dr. G. J. Haslam, W. Heape, W. Hurst, Prof. A. M. Marshall, Howard Saunders, Dr. G. A. Woods. Prof. W. Osler, Howard Saunders, A. Sedgwick, Prof. R. R. Wright. W. Heape, J. McGregor-Robertson, J. Duncan Matthews, Howard Saunders, H. Marshall Ward. Prof. T, W. Bridge, W. Heape, Prof. W. Hillhouse, W. L. Sclater, Prof, H. Marshall Ward. ' The Departments of Zoology and Botany and of Anatomy and Physiology were amalgamated. 2 Anthropology was made a separate Section, see p. Ixx. 1897. Toronto _ 1835. Dublin ~ 1836. Bristol ......|Dr. P. M. Roget, F.R.S. ...... _ 1838. Newcastle PRESIDENTS AND SECRETARIES OF THE SECTIONS. lxiii Date and Place Presidents Secretaries 1887. Manchester | Prof. A. Newton, M.A., F.R.S., F.L.S., V.P.Z.S. 1888. Bath......... W. T. Thiselton-Dyer, C.M.G., E.RB.S., F.L.S. 1889. Newcastle -| Prof. J. S. Burdon Sanderson, upon-Tyne| M.A., M.D., F.R.S. 1890. Leeds ...... Prof. A. Milnes Marshall, M.A., M.D., D.Sc., F.R.S. 1891. Cardiff...... Francis Darwin, M.A., M.B., F.R.S., F.L.S. 1892. Edinburgh |Prof. W. Rutherford, M.D., E.RB.S., F.B.S.E. 1893. Nottingham'|Rev. Canon H. B. Tristram, M.A., LL.D., F.R.S. 1894. Oxford? ...| Prof. I. Bayley Balfour, M.A., E.RS. SECTION D (continued) 1895. Ipswich ...|Prof. W. A. Herdman, F.R.58. 1896. Liverpool...|Prof. E. B. Poulton, F.R.S. ... Prof. L. C. Miall, F.R.S. ...... 1898, Bristol......| Prof. W. F. R. Weldon, F.R.S. C. Bailey, F. E. Beddard, 8. F. Har- mer, W. Heape, W. L. Sclater, Prof. H. Marshall Ward. F. E. Beddard, S. 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, 8S. J. Hickson, F. W. Oliver, H. Wager, H. Marshall Ward. ¥. E. Beddard, Prof. W.A. Herdman, Dr. 8. J. Hickson, G. Murray, Prof. W. N. Parker, H. Wager. G. Brook, Prof. W. A. Herdman, G. Murray, W. Stirling, H. Wager. G. C. Bourne, J. B. Farmer, Prof. W. A. Herdman, 8. J. Hickson, W. B. Ransom, W. L. Sclater. W. W. Benham, Prof. J. B. Farmer, Prof. W. A. Herdman, Prof. 8S. J. Hickson, G. Murray, W. L. Sclater. .— ZOOLOGY. G. C. Bourne, H. Brown, W. E. Hoyle, W. L. Sclater. H. O. Forbes, W. Garstang, W. E. Hoyle. W. Garstang, W. E. Hoyle, Prof. E. E. Prince. : Prof. R. Boyce, W. Garstang, Dr. A. J. Harrison, W. H. Hoyle. ANATOMICAL AND PHYSIOLOGICAL SCIENCES. COMMITTEE OF SCIENCES, V.—ANATOMY AND PHYSIOLOGY. 1833. Cambridge 1834. Edinburgh a ry Dr. H. J. H. Bond, Mr. G. E. Paget. Dr. Roget, Dr. William Thomson. SECTION E (UNTIL 1847).—ANATOMY AND MEDICINE. Dr. J. C. Pritchard 1837. Liverpool...|Prof. W. Clark, M.D. ......... T. E. Headlam, M.D. ......... 1839. Birmingham|John Yelloly, M.D., F.R.S.... 1840. Glasgow ...|James Watson, M.D. tee eeeeee RSECTION E.—PHYS 1841. Plymouth...) P. M. Roget, M.D., Sec. R.S. Dr. Harrison, Dr. Hart, Dr. Symonds. Dr. J. Carson, jun., James Long, Dr. J. B. W. Vose. T. M. Greenhow, Dr. J. R. W. Vose. Dr. G. O. Rees, F. Ryland. Dr.J. Brown, Prof. Couper, Prof. Reid. IOLOGY. Dr. J. Butter, J. Fuge, Dr. R. 8. Sargent. 1842. Manchester | 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. meee u044. York......... J. ©. Pritchard, M.D. ......... I. Erichsen, Dr. R. S. Sargent. 1845. Cambridge |Prof. J. Haviland, M.D. ......|Dr. R. §. Sargent, Dr. Webster. 1 Physiology was made a separate Section, see p. lxx. 2 The title of Section D was changed to Zoology. xiv Date and Place REPORT—1898. Presidents Secretaries =e . Southamp- |Prof. Owen, M.D., F.R.S. ...|C. P. Keele, Dr. Laycock, Dr. Sar- 1846 ton. gent. 1847. Oxford’ ...|Prof. Ogle, M.D., F.R.S. ......]Dr. Thomas K. Chambers, W. P. ; Ormerod. PHYSIOLOGICAL SUBSECTIONS OF SECTION D. 4850. Edinburgh |Prof. Bennett, M.D., F.R.S.E. | 1855. Glasgow ...|Prof. Allen Thomson, F.R.8. | 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. Bath......... Dr. Edward Smith, LL.D.,|J.S. Bartrum, Dr. W. Turner. F.RS. 1865. Birming- |Prof. Acland, M.D., LL.D.,)Dr. A. Fleming, Dr. P. Heslop, ham.* F.R.S. . Oliver Pembleton, Dr. W. Turner. GEOGRAPHICAL AND ETHNOLOGICAL SCIENCES. [For Presidents and Secretaries for Geography previous to 1851, see Section C, p. lvii.] ETHNOLOGICAL SUBSECTIONS OF SECTION 1846.Southampton] Dr. J. C. Pritchard weer ew eeneee D. |Dr. King, 1847. Oxford ...... Prof. H. H. Wilson, M.A. ...|Prof. Buckley. DEAS SHINO TELS MAS I og eonacian oc bosadcuadeeseanocpUBadbe G. Grant Francis. SSA Oy BITMIN HAM | 0. .00ssecqceeepgeenenss sss = esas 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.§.,|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. Ros. UL. sence IR. G. Latham, M.D., F.2.8. |R. Cull, Rev. H. W. Kemp, Dr. Norton Shaw. 1854. Liverpool... |Sir R. I. Murchison, D.C.L.,/ Richard Cull, Rey. 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...... Rey. Dr. J, Henthorn Todd,/R. Cull, S. Ferguson, Dr. R. R. } Pres. R.I.A. 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. lx.). Section E, being then vacant, was assigned in 1851 to Geography. 2 Vide note on page 1xi. PRESIDENTS AND SECRETARIES OF THE SECTIONS. Date and Place lxv Presidents Secretaries 1858. - 1859. Aberdeen... seneee 1860. Oxford 1861 1862 . Manchester . Cambridge 1863. Newcastle 1864. eee 1865. Birmingham 1866. Nottingham 1867. Dundee 1868. Norwich ... . Liverpool... . Edinburgh . Brighton ... . Bradford ... 1876. Glasgow ... 1879. Sheffield ... 1880. Swansea ... mas!.. York......... 1883. eae _ 1884. Montreal ... ‘ 1885. Aberdeen... 1886, Birmingham 1898. Sir R.I. Murchison, G.C.St.S., F.RB.S. Rear - Admiral Sir James} Clerk Ross, D.C.L., F.R.S. Sir R. I. Murchison, D.C.L.. F.R.S. John Crawfurd, F.R.S.......... Francis Galton, F.R.S.......... Sir R. I. Murchison, K.C.B., F.R.S. Sir R. I. Murchison, K.C.B., E.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, F. Galton, P. O'Callaghan, Dr. Norton Shaw, T. Wright. Richard Cull, Prof. Geddes, Dr. Nor- ton Shaw. Capt. Burrows, Dr. J. Hunt, Dr. C. Lempriére, Dr. Norton Shaw. Dr. J. Hunt, J. Kingsley, Dr. Nor- ton Shaw, W. Spottiswoode. J.W.Clarke, Rev. J.Glover, Dr. Hunt, Dr. Norton Shaw, T. Wright. C. Carter Blake, Hume Greenfield, C. R. Markham, R. 8. Watson. H. W. Bates, C. R. Markham, Capt. R. M. Murchison, T. Wright. H. W. Bates, 8. 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, C. R. ~ Markham, S. J. Mackie, R. Sturrock. T. Baines, H. W. Bates, Clements'R. Markham, T. Wright. SECTION E (continued ).—GEOGRAPHY. \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.8. 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.8.1L., F.R.S.,F.R.G.S. Capt. Evans, C.B., F.R.S....... Adm. Sir E. Ommanney, C.B. Prof. Sir C. Wyville Thom- son, LL.D.,F.R.S., F.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.R.S. Sir J. D. Hooker, K.C.S.1., CIB: EER:S. Sir R. Temple, Bart., G.C.S.L., F.R.G.S. Lieut.-Col. H. H. Godwin- Austen, F.R.S. Gen. Sir J. H. Lefroy, C.B., K.C.M.G.. F.R.S.,V.P.2.G.8. Gen. J. T. Walker, C.B., R.E., LL.D., F.R.S. Maj.-Gen. Sir. F. J. Goldsmid, K.C.S.1., C.B., F.R.G.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, HE. C. Rye, F. F. Tackett. H. W. Bates, E. C. Rye, R. O. Wood. H. W. Bates, F. E. Fox, HK. C. Rye. John Coles, E. C. Rye. , H. W. Bates, C. E. D. Black, E. C, Rye. 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. Rev. Abbé Laflamme, J.S. O’Halloran, KE. G. Ravenstein, J. F. Torrance. J.S. Keltie, J. S. O'Halloran, E. G. Ravenstein, Rev. G. A. Smith. F. T. S. Houghton, J. 8. Keltie. E. G. Ravenstein. a Ixvi REPORT—1898. Date and Place Presidents Secretaries 1887. Manchester| Col. Sir C. Warren, R.E.,|Rev. L. C. Casartelli, J. 8. Keltie, G.C.M.G., F.B.S., F.R.G.S. | H.J. Mackinder, E. G. Ravenstein. 1888. Bath......... Col. Sir C. W. Wilson, R.E.,|J. 8. Keltie, H. J. Mackinder, E. G. K.C.B., F.R.S., F.R.G.S. Ravenstein. 1889. Newcastle- |Col. Sir F. de Winton,|J. 8. Keltie, H. J. Mackinder, R. upon-Tyne| K.C.M.G., C.B., F.R.G.S. Sulivan, A. Silva White. 1890. Leeds ...... Lieut.-Col. Sir R. Lambert|A. Barker, John Coles, J. 8. Keltie, Playfair, K.C.M.G.,F.R.G.S.|_ A. Silva White. 1891. Cardiff...... E. G. Ravenstein, F.R.G.S.,|John Coles, J. S. Keltie, H. J. Mac- F.S.8. kinder, A. Silva White, Dr. Yeats. 1892. Edinburgh | Prof, J. Geikie, D.C.L.,F.R.S.,|J. G. Bartholomew, John Coles, J. 8. V.P.R.Scot.G.S. Keltie, A. Silva White. 1893. Nottingham|H. Seebohm, Sec. R.S., F.L.S., Col. F. Bailey, John Coles, H. oO. F.Z.8. Forbes, Dr. H. R. Mill. 1894. Oxford...... Capt. W.J. L. Wharton, R.N.,\John Coles, W. 8. Dalgleish, H. N. F.R.S. Dickson, Dr. H. R. Mill. 1895. Ipswich .../H. J. Mackinder, M.A., John Coles, H. N. Dickson, Dr. H. F.R.G.S. R. Mill, W. A. Taylor. 1896. Liverpool...| Major L. Darwin, Sec. R.G.S. |Col. F. Bailey, H. N. Dickson, Dr. H. R. Mill, E. C. DuB. Phillips. 1897. Toronto ...|J. Scott-Keltie, LL.D. i\Col. F. Bailey, Capt. Deville, Dr. H. R. Mill, J. B. Tyrrell. 1898. Bristol...... Col. G. Earl Church, F.R.G.S.H. N. Dickson, Dr. H. R. Mill, H. C. | Trapnell. STATISTICAL SCIENCE. COMMITTEE OF SCIENCES, VI.—STATISTICS. 1833. Cambridge | Prof. Babbage, F.R.S. .........{/J. E. Drinkwater. 1834, Edinburgh | Sir Charles Lemon, Bart.......I Dr. Cleland, C. Hope Maclean. SECTION F.—STATISTICS. 1835. Dublin...... Charles Babbage, F.R.S. ......) W. Greg, Prof. Longfield. 1836. Bristol...... Sir Chas. Lemon, Bart., F.R.S.|Rev. J. E. Bromby, C. B. Fripp, : James Heywood. 1837. Liverpool...|Rt. Hon. Lord Sandon......... W. R. Greg, W. Langton, Dr. W. C. Tayler. 1838. Newcastle |Colonel Sykes, F.R.S. .........| W. Cargill, J. Heywood, W.R. Wood. 1839, Birmingham |Henry Hallam, F.R.S..........|F. Clarke, R. W. Rawson, Dr. Ww.c. Tayler. 1840. Glasgow .../Rt. Hon. Lord Sandon, M.P.,/C. R Baird, Prof. Ramsay, R. W. F.R.S. Rawson. 1841. Plymouth... |Lieut.-Col. Sykes, F.R.S....... Rey. Dr. Byrth, Rev. R. Luney, R. W. Rawson. 1842, Manchester |G. W. Wood, M.P., F.L.S. ...|Rev. R. Luney, G. W. Ormerod, Dr, W. C. Tayler. 1843. Cork......... ‘Sir C. Lemon, Bart., M.P. ...|Dr. D. Bullen, Dr. W. Cooke Tayler. 1844. York......... ict scale Sykes, F-.R.S.,|J. Fletcher, J. Heywood, Dr. Lay- : -L.S. cock. 1845, Cambridge | Rt. Hon. the Earl Fitzwilliam|J. Fletcher, Dr. W. Cooke Tayler. 1846. Southamp- |G. R. Porter, F.R.S. ............ J. Fletcher, F. G. P. Neison, Dr. W. ton. C. Tayler, Rev. T. L. Shapcott. 1847, Oxford...... Travers Twiss, D.C.L., F.R.S.| Rev. W. H. Cox, J. J. Danson, F. G. P. Neison. 1848. Swansea ...|J. H. Vivian, M.P., F.R.S. ...|J. Fletcher, Capt. R. Shortrede. 1849. Birmingham| Rt. Hon. Lord Lyttelton...... Dr. Finch, Prof. Hancock, F. G. P. Neison. 1850 Hedinburgh |Very Rev. Dr. John Lee, | V.P.R.S.E. \Prof. Hancock, J. Fletcher, Dr, | Stark, PRESIDENTS AND SECRETARIES OF THE SECTIONS. lxvil Date and Place Presidents 1851. Ipswich ... 1852. Belfast...... £855. Hull.:.....0. 1854. Liverpool... 1855. Glasgow . Sir John P. Boileau, Bart. ... His Grace the Archbishop of Dublin. James Heywood, M.P., F.R.S. Thomas Tooke, 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 1857. Dublin 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 1872. Brighton... 1873. Bradford ... 1874. Belfast...... 1875, (1876. 1877. 1878. Bristol...... Glasgow ... Plymouth... Dublin...... 1879. Sheffield ... 1880. Swansea ... Obs VOLK. .cccees 1882. Southamp- ton. 1883. Southport Rt. Hon. Lord Stanley, M.P. His Grace the Archbishop of Dublin, M.R.1.A. Edward Baines......... accvbooor, 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.... W. Farr, M.D., D.C.L., F.R.S. Rt. Hon. Lord Stanley, LL.D., M.P Prof. f . E. T. Rogers M. E. Grant-Duff, M.P. ....... Samuel Brown ...........see000s Rt. Hon. Sir Stafford H. North- cote, Bart., C.B., M.P. Prof. W. Stanley Jevons, M.A. Rt. Hon. Lord Neaves......... Prof. Henry Fawcett, M.P.... Rt. Hon. W. E. Forster, M.P. Lord: O'Hagan “v.\....0..ccsc000e James Heywood, M.A., F.R.S., Pres. 8.8. 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. G. W. Hastings, M.P........... Rt. Hon. M. E. Grant-Duff, M.A., F.R.S. Rt. Hon. G. Sclater-Booth, M.P., F.B.S. R. H. Inglis Palgrave, F.R.S, Rev. C. H. Bromby, E. Cheshire, Dr. W. N. Hancock, W. Newmarch, W. M. Tartt. Prof. Cairns, Dr. H. D. Hutton, W. Newmarch. T. B. Baines, Prof. Cairns, S. Brown, Capt. Fishbourne, Dr. J. Strang. Prof. Cairns, Edmund Macrory, A. M, Smith, Dr. John Strang. Edmund Macrory, W. Newmarch, Prof. J. E. T. Rogers. David Chadwick, Prof. R. C. Christie, E. Macrory, Prof. J. E. T. Rogers. H. D. Macleod, Edmund Macrory. T. Doubleday, Edmund Macrory, Frederick Purdy, James Potts. E. Macrory, E. T. Payne. F. Purdy. G. J. D. Goodman, G. J. Johnston, E. Macrory. R. Birkin, jun., Prof. Leone Levi, E. Macrory. Prof. Leone Levi, E. Macrory, A. J. Warden. Rev. W.C. Davie, Prof. Leone Levi. E. Macrory, F. Purdy, C. T. D. Acland. Chas. R. Dudley Baxter, E. Macrory, J. Miles Moss. J. G. Fitch, James Meikle. J. G. Fitch, Barclay Phillips. J. G. Fitch, Swire Smith. Prof. Donnell, F. P. Fellows, Hans MacMordie. F. P. Fellows, T. G. P. Hallett, E. Macrory. 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. Rev. W. Cunningham, Prof. H. §. Foxwell, J. N. Keynes, C. ree’ ixviii Date and Place 1884. 1885. 1886. 1887. 1888. 1889. 1890. 1891. 1892. 1893. 1894, 1895. 1896. 1897. 1898. 1836. 1837. 1838. 1839. 1840. 1841. 1842. 1843. 1844. 1845. 1846. 1847. 1848. 1849. 1850. 1851. 1852. 1853, Montreal ... REPORT—1898. Presidents Sir Richard Temple, Bart., G.C.8.1., C.LE., F.R.G.S. Secretaries Prof. H. S. Foxwell, J.S. McLennan, Prof. J. Watson. Rey. W. Cunningham, Prof. H. S. Foxwell, C. McCombie, J. F. Moss. F. F. Barham, Rev. W. Cunningham, Prof. H. 8S. 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. S. Foxwell, L. L. F. R. Price. Rey. 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, L. L. F. R. Price. EB. Cannan, Prof. E. C. K. Gonner, W.A.S. Hewins, H. Higgs. E. Cannan, Prof. E. C. K. Gonner, E. Cannan, Prof. E. C. K. Gonner, W. A. 8S. Hewins, H. Higgs. E. Cannan, H. Higgs, Prof. A. Shortt. E. Cannan, Prof. A. W. Flux, H. Higgs, W. E. Tanner. T. G. Bunt, G. T. Clark, W. West. Charles Vignoles, Thomas Webster. C. Vignoles, T. W. Carpmael, William Hawkes, T. J. Scott Russell, J. Thomson, J. Tod, Henry Chatfield, Thomas Webster. J. F. Bateman, J. Scott Russell, J. Thomson, Charles Vignoles. James Thomson, Robert Mallet. Charles Vignoles, Thomas Webster. Rey. 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. John F. Bateman, C. B. Hancock, Charles Manby, James Thomson. Aberdeen...| Prof. H. Sidgwick, LL.D., Litt.D. Birmingham|J. B. Martin, M.A., ¥.8.S. Manchester | Robert Giffen, LL.D.,V.P.S.S. Bath.....20.. Rt. Hon. Lord Bramwell, LL.D., F.R.S. Newcastle- | Prof. F. Y. Edgeworth, M.A., upon-Tyne| F.S.S, Leeds ...... Prof. A. Marshall, M.A., F.8.S. Cardiff ...... Prof. W. Cunningham, D.D., D.Sc., F.8.8. Edinburgh |Hon. Sir C. W. Fremantle, K.C.B. Nottingham | Prof. J. 8. Nicholson, D.Sc., E.S.8. Oxford...... Prof. C. F. Bastable, M.A., F.S8.5. Ipswich. cs. |. Ta. Price; diac so .cs5.:-5<0-6 H. Higgs. Liverpool...|Rt. Hon. L. Courtney, M.P.... Toronto ...| Prof. E. C. K. Gonner, M.A. Bristol......| J. Bonar, M.A., LL.D. MECHANICAL SCIENCE. SECTION G.—MECHANICAL SCIENCE. Bristol...... Davies Gilbert, D.C.L., F.R.S. Liverpool...|Rev. Dr. Robinsor ............ Newcastle |Charles Babbage, F.R.S.......)R. Hawthorn, Webster. Birmingham | Prof. Willis, F.R.S., and Robt. Stephenson. Webster. Glasgow ..../Sir John Robinson ............ C. Vignoles. Plymouth |John Taylor, F.R.S. ........... Manchester| Rev. Prof. Willis, F.R.S. ...... Cork cca. Prof. J. Macneill, M.R.I.A.... ROT seesceces John Laylor, HRS. acc.ecaeeees Cambridge |George Rennie, F.R.S.......... South’mpt’n| Rev. Prof. Willis, M.A., F.R.S. Oxford...... Rev. Prof. Walker, M.A.,F.R.S. Swansea .../ Rev. Prof.Walker, M.A.,F.R.S. Birmingh’™ | Robt. Stephenson, M.P.,F.R.S. Edinburgh | Rev. R. Robinson ............... Ipswich ..,} William Cubitt, F.R.S.......... Belfast...... John Walker, C.E., LL.D., F.R.S. Hull.........) William Fairbairn, F.R.S. J. Oldham, J.. Thomson, W.S. Ward. PRESIDENTS AND SECRETARIES OF THE SECTIONS. lxix Date and Place 1854. Liverpool... 1855. Glasgow ... 1856. Cheltenham 1857. Dublin...... 1858. Leeds 1859. Aberdeen.. seenee 1860. Oxford weeeee 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 teens 1875. Bristol 1876. Glasgow ... 1877. Plymouth... 1878. Dublin ...... 1879. Sheffield .. 1880. Swansea ... 1881. York 1882, Southamp- ton 1883. Southport 1884. Montreal... 1885. Aberdeen... 1886. Birmingham 1887. Manchester 1888. Bath Presidents Secretaries John Scott Russell, F.R.S. ... W. J. M. Rankine, F.R.S. George Rennie, F.R.S. ....... Rt. Hon. the Earl of Rosse, F.R.S. William Fairbairn, F.R.S. ... .{ Rev. Prof. Willis, M.A., F.R.S. Prof.W.J. Macquorn Rankine, LL.D., F.R.S. J. F. Bateman, C.E., F.R.S.... William Fairbairn, F.R.S. Rev. Prof. Willis, M.A., F.R.8. J. ee F.R.S. Sir W. G. Armstrong, Tis D., F.R Thomas ‘Hawksley, V.P. Inst. C.E., F.G.S. Prof.W.J. Macquorn Rankine, LL.D., F.R.S. G. P. Bidder, C.E., F.R.G.S. C. W. Siemens, F.R.S.... Prof. Fleeming Jenkin, F.R.S. | F. J. Bramwell, C.E. seerecsee .|W. H. Barlow, F.RB.S. 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. C. 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. Westmacott, 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, 0, Manby, W. Smith. ......|P. Le Neve Foster, H. Bauerman. .| Chas. B. Vignoles, C.E., F.R.S. H. Bauerman, P. Le Neve Foster, T. King, J. N. Shoolbred. H. Bauerman, A. Leslie, J. P. Smith, H. M. Brunel, P. Le Neve Foster, J. G. Gamble, J. N. Shoolbred. ..|C. Barlow, H. Bauerman. E.H.Carbutt, J. C. Hawkshaw, J. N. Shoolbred. Prof, James Thomson, LL.D., A. T. Atchison, J. N. Shoolbred, John 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. . Edward Easton, C.E. .|J. Robinson, Pres. Inst. Mech. Eng. J. Abernethy, JRE ish) eppacens Sir W. G. Armstrong, C.B., LL.D., D.C.L., F.R.S. John Fowler, C.E., F.G.S. ... J. Brunlees, Pres. Inst.C.E. Sir F. J. Bramwell, F.R.S., V.P.Inst.C.E. B. Baker, M.Inst.C.E. ........ Sir J. N. Douglass, M.Inst. C.E Prof. Osborne Reynolds, M.A., LL.D., F.RB.S. W. dH. Preece, F.RS., M.Inst.C.E. 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. ‘ft. Atchison, F. Churton, H. T. Wood. A. T. Atchison, E. Rigg, H. T. Wood. A. T. Atchison, W. B. Dawson, J. Kennedy, H. T. Wood. .|A. T. Atchison, F. G. Ogilvie, E. Rigg, J. N. Shoolbred. C. W. Cooke, J. Kenward, W. B. Marshall, E. Rigg. C. F. Budenberg, W. B. Marshall, E. Rigg. C. W. Cooke, W. B. Marshall, E. Rigg, P. K, Stothert. lxx REPORT—1898. Date and Place 1889. 1890. 1891, Presidents Secretaries Newcastle- upon-Tyne Leeds eeneer Cardiff ...., W. Anderson, M.Inst.C.E. ... Capt. A. Noble, C.B., F.RB.S., F.R.A.S. T. Forster Brown, M.Inst.C.E. 1892. Edinburgh |Prof. W. C. Unwin, F.R.S., 1893. 1894. 1895. 1896. 1897. 1898. 1884. 1885. Nottingham Oxford...... Ipswich ... Liverpool... Toronto Bristol seeeee \ Montreal... Aberdeen... 1886. Birmingham 1887. 1888. 1889, 1890. 1891, 1892. 1893. 1894. 1895. 1896. 1897. 1898. 1894, 1896. 1897, Manchester Newcastle- upon-Tyne Leeds Cardiff ...... Edinburgh Nottingham Oxford ....:. Ipswich ... Liverpool... Toronto Bristol .|E. B. Tylor, D.C.L., F.RB.S. .. ... (Sir W. Tumer, F.R.S. ......... M.Inst.C.E. Jeremiah Head, M.Inst.C.E., F.C.S. Prof. A. B. W. Kennedy, F.R.S., M.Inst.C.E. Prof. L. F. Vernon-Harcourt, M.A., M.Inst.C.E. Sir Douglas Fox, V.P.Inst.C.E. ...|G@. F. Deacon, M.Inst.C.E. Sir J. Wolfe-Barry, K.C.B., FE.R.S. C. W. Cooke, W. B. Marshall, Hon. C. 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. Bb. Marshall, E. Rigg, H. Talbot. Prof. T. Hudson Beare, C. W. Cooke, W. B. Marshall, Rev. F. J. Smith. Prof. T. Hudson Beare, C. W. Cooke, W. B. Marshall, P. G. M. Stoney. Prof. T. Hudson Beare, C. W. Cooke, 8. Dunkerley, W. B. Marshall. Prof. T. Hudson Beare, Prof, Callen- dar, W. A. Price. Prof. T. H. Beare, Prof. J. Munro, H. W. Pearson, W. A. Price. SECTION H.—ANTHROPOLOGY. Francis Galton, M.A., FBS. | Sir G. Campbell, K.C.S.1., M.P., D.C.L., F.R.G.S. Prof. A. H. Sayce, M.A. ...... Lieut.-General D.C.L., F.R.S. Prof. Sir W. Turner, M.B., LL.D., F.R.S. Dr. J. Evans, Treas. R.S., F.S.A., F.L.S., F.G.S. Prof. F. Max Miiller, M.A. ... Pitt-Rivers, Prof. A. Macalister, M.D., F.B.S. Dr. R. Munro, M.A., F.R.S.E. M.A, Sir W. H. Flower, K.C.B., E.R.S. Prof. W. M. Flinders Petrie, D.C.L. Arthur J. Evans, F.S.A. ... E. W. Brabrook, C.B.°....,..+ G. W. Bloxam, W. Hurst. G. W. Bloxam, Dr. J. G. Garson, W. Hurst, Dr. A. Macgregor. G. W. Bloxam, Dr. J. G. Garson, W. Hurst, Dr. R. Saundby. G. W. Bloxam, Dr. J. G. Garson, Dr. A. M. Paterson. G. W. Bloxam, Dr. J. G. Garson, J. Harris Stone. G. W. Bloxam, Dr. J. G. Garson, Dr. R. Morison, Dr. R. Howden. G. W. Bloxam, Dr. C. M. Chadwick, Dr. J. G. Garson. G. W. Bloxam, Prof. R. Howden, H. Ling Roth, E. Seward. G. W. Bloxam, Dr. D. Hepburn, Prof. R. Howden, H. Ling Roth. G. W. Bloxam, Rev. T. W. Davies, Prof. R. Howden, F. B. Jevons, J. L. Myres. H. Balfour, Dr. J. G.Garson, H. Ling Roth. J. L. Myres, Rev. J. J. Raven, H. Ling Roth. .| Prof. A. C. Haddon, J. L. Myres, Prof. A. M. Paterson. A. F. Chamberlain, H. O. Forbes, Prof, A. C. Haddon, J. L. Myres. H. Balfour, J. L. Myres, G. Parker. SECTION I.—PHYSIOLOGY (including ExpermenTa PaTHOLOGY AND EXPERIMENTAL PsycHouocy). Oxford......|Prof. E. A, Schiifer, F.R.S.,|Prof. F. Gotch, Dr. J. 8. Haldane, M.R.C.S. Liverpool.../Dr. W. H. Gaskell, F.R.S. Toronto .../Prof. Michael Foster, F.R.S. | Prof, R. Boyce, Prof. C. 8. Sherring- M. 8. Pembrey. Prof. R. Boyce, Prof. C.S. Sherrington. ton, Dr. L. HE. Shore. Date and Place LIST OF EVENING LECTURES. lxxi Presidents Secretaries 1895. Ipswich 1896. Liverpool... 1897. Toronto ... 1898. Bristol...... SECTION K.—BOTANY. Dr. D. H. Scott, F.R.S. seneee ...|W. T. Thiselton-Dyer, F.R.S,|A..C. Seward, Prof. F. E. Weiss. Prof. Harvey Gibson, A. C. Seward, Prof. F. E. Weiss. Prof. Marshall Ward, F.R.S. |Prof. J. B. Farmer, E. C. Jeffrey, Prof. F. O. Bower, F.R.S. A. C. Seward, Prof. F. E. Weiss. ...; A.C, Seward, H. Wager, J. W. White. LIST OF EVENING Date and Place 1842. Manchester 1843, Cork ......... 1844. York......... 1845. Cambridge 1846. Southamp- ton. 1847. Oxford...... 1848. Swansea ... 1849. Birmingham 1850. Edinburgh 1851. Ipswich ... 1852. Belfast...... 1853. Hull......... Lecturer LECTURES. Subject of Discourse Charles Vignoles, F'.R.S...... Sir M. I. Brunel Feel, MN CHISON J... ccs asescee sets. Prof. Owen, M.D., F.R.S....... Prof. E. Forbes, F.R.S.......... ee eeeeseeceenee Dre RODINSONG« casvecsscsss sauce. Charles Lyell, F.R.S. ......... Dr: Walconer; HORS ...c.cccccoes 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. ........ W. R. Grove, F.R.S. ............ Rev. Prof. B. Powell, F.R.S. Prof, M. Faraday, F.R.S....... Hugh HE. Strickland, F.G.S.... John Percy, M.D., F.R.S....... W. Carpenter, M.D., F.R.S.... Dr. Faraday, F.R.S. ............ Rev. Prof. Willis, M.A., F.R.S. Prof. J. H. Bennett, M.D., F.R.S.E. Dr. Mantell, F.R.S. .........066 Prof. R. Owen, M.D., F.R.S. G.B.Airy,F.B.S.,Astron. Royal Prof. G. G. Stokes, D.C.L., F.RB.S. Colonel Portlock, R.E., F.R.S. Prof. J. Phillips, LL.D.,F.B.S., F.G.S. Robert Hunt, F.B.S....... esees 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 Siwalik 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; also 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. Ixxii Date and Place 1854. Liverpool... 1855. Glasgow ... 1856. Cheltenham 1859. Aberdeen... 1860. Oxford seecee . Manchester . Cambridge . Newcastle 1864. ee ereecee 1865. Birmingham 1866. Nottingham 1867. Dundee eeesee 1868. Norwich ... 1869. Exeter ...... 1870. Liverpool... 1871. Edinburgh 1872. Brighton ... REPORT—1898. Lecturer Prof. R. Owen, M.D., F.R.S. Col. E. Sabine, V.P.R.S. ...... Dr. W. B. Carpenter, F.R.S. Lieut.-Col. H. Rawlinson Col. Sir H. Rawlinson fe eeeeeee WR. Grove, HOB:S. cscccssecce Prof. W. Thomson, F.R.58. .. Rey. Dr. Livingstone, D.C.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. Dr. Robinson, F.R.S. ... Rev. Prof. Walker, F.R.S. ... Captain Sherard Osborn, R.N. Prof.W. A. Miller, M.A., F.R.S8. G. B. Airy, F.R.S., Astron. Royal. Prof. Tyndall, LL.D., F.R.S. Prof, Odlang, W-RGS. ..5..2..:0-. Prof. Williamson, F.R.5....... James Glaisher, F.R.S......... Prof. Roscoe, F.R.S............ 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.5....... Alexander Herschel, F.R.A.S. J. Fergusson, F.R.S..........--- Dr. W. Odling, F.R.S.......... Prof. J. Phillips, LL.D.,F.R.S. J. Norman Lockyer, F.R.S.... Prof. J. Tyndall, LL.D., F.R.S. Prof.W.J. Macquorn Rankine, LL.D., F.R.S. HAS Abels BRS ...ssschepsccace He Bs PylOr; HeRcSe. iscssstsesees Prof. P. Martin Duncan, M.B., F.R.S. PEGE MWe Ae, (CIM OTG cc: . sen cecs Subject of Discourse 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. .|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, 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 Nebule. The Scientific Use of the Imagination. Stream-lines and Waves, in connec- tion with Naval Architecture. Some Recent Investigations and Ap- plications of Explosive Agents. The Relation of Primitive to Modern Civilisation. Insect Metamorphosis. The Aims and Instruments of Scien- tific Thought. ES Date and Place 1873. 1874. 1875. 1876. 1877. 1878. 1879. 1880. 1881. 1882. 1883. 1884. 1885. Bradford ... Belfast ...... Bristol Glasgow Plymouth... Dublin Sheffield ... Swansea ... Southamp- Southport Montreal... Aberdeen... 1886. Birmingham 1887. 1888. 1889. 1890. 1891. 1892. 1893. 1894. Manchester Newcastle- upon-Tyne seeees Edinburgh Nottingham ..»|Prof. Tait, F.RS.E. , LIST OF EVENING LECTURES. lxxni Lecturer Prof. W. C.Williamson, F.R.S. Prof. Clerk Maxwell, F.R.S. 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.......... Sir Wyville Thomson, F R. s. W. Warington Smyth, M.A., E.RB.S. Prot OGlin Ge HR. Savcsesnash«0s G. J. Romanes, F.L.S......... Prof, Dewar, FURS. ccccccsesses W. Crookes, F.R.S. ren Prof. EK. Ray Lankester, F. BP 8. Prof.W.Boyd Dawkins, F.R.8. Francis Galton, F.RB.S.......... Prof. Huxley, Sec. B.S. W. Spottiswoode, Pres. R.S.... Prof. Sir Wm. Thomsca, F.R.S., Prof. H. N. Moseley, F.R.S. Prof. R. S. Ball, F.R.S. Prof. J. G. McKendrick. ...... Prof. O. J. Lodge, D.Sc. ...... Rev. W. H. Dallinger, F.R.S. Prof. W. G. Adams, F.R.S. John Murray, F.R.S.E......... A. W. Riicker, M.A., F.R.S. Prof. W. Rutherford, M.D.... Prof. H. B. Dixon, F.R.S. Col. Sir F. de Winton ......... Prof. W. E. Ayrton, F.R.S. ... Prof. T. G. Bonney, D.Sc., F.RB.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.S. Prof. L. C. Miall, F.L.S.,F.G.S. Prof. A.W. Riicker, M.A.,F.R.S. Prof. A. M. Marshall, F.R.S. Prof. J.A. Ewing, M.A., F.R.S. Prof. A. Smithells, B.Sc. Prof. Victor Horsley, F.R.S. J. W. Gregory, D.Sc., F.G.S. Subject of Discourse 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. The Challenger Expedition. 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 Paleon- 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 Diffculties in the Life of Aquatic Insects. Electrical Stress. Pedigrees. Maenetic Induction. Flame. The Discovery of the Physiology of the Nervous System. Experiences and Prospects of African Exploration. lxxiv Date and Place REPORT—1898. Lecturer Prof. J.Shield Nicholson, M.A. Subject of Discourse Historical Progress and Ideal So- 1894. Oxford...... cialism. 1895. Ipswich ...|Prof. 8. P. Thompson, F.R.S. | Magnetism in Rotation. Prof. Percy F. Frankland,|The Work of Pasteur and its various F.RB.S. Developments. 1896. Liverpool...| Dr. F. Elgar, F.R.S. ............ Safety in Ships. Prof. Flinders Petrie, D.C.L. | Man before Writing. 1897. Toronto ...|Prof. Roberts Austen, F.R.S. |Canada’s Metals. J. Milne, HIRASsa. .cseccsscesse. ..|Harthquakes and Volcanoes. 1898. Bristol...... Prof. W. J. Sollas, F.R.S. ...|Funafuti: the Study, of a Coral Island. Herbert Jackson ..........0005 Phosphorescence. LECTURES TO THE OPERATIVE CLASSES. Date and Place Lecturer Subject of Discourse 1867. Dundee......| Prof. J. Tyndall, LL.D., F.R.S.| Matter and Force. 1868. Norwich ...| Prof. Huxley, LL.D., F. R.S. |A Piece of Chalk. 1869. Exeter ...... Prof, Miller, M.D., F.R.S. ...|The modes of detecting the Com- i position of the Sun and other i Heavenly Bodies by the Spectrum. 1870. Liverpool... |SirJohn Lubbock, Bart.,F.R.S.| Savages. 1872. Brighton ...| W.Spottiswoode,LL.D. F, R.8.| Sunshine, Sea, and Sky. 1872. Bradford ...|C.W. Siemens, D.C.L., F.R.S.| Fuel. 1874, Belfast ...... Prof. Odling, F.R.S............. The Discovery of Oxygen. 1875. Bristol ...... Dr. W. B. Carpenter, F.R.S. | A Piece of Limestone. 1876. Glasgow ...|Commander Cameron, C.B....| A Journey through Africa. 1877. Plymouth...) W. H. Preece..........cssecsssees Telegraphy and the Telephone. 1879. Sheffield ...|W. E. Ayrton ..............0006 Electricity as a Motive Power. 1880. Swansea ...|H. Seebohm, F.Z.S. ............ The North-East Passage. WSBT VOrk.......... Prof. Osborne Reynolds,| Raindrops, Hailstones, and Snow- E.R.S. flakes. 1882. Southamp- |John Evans, D.C.L.,Treas.R.S.} Unwritten History, and how to ton. read it. 1883. Southport {Sir F. J. Bramwell, F.R.S. ...| Talking by Electricity—Telephones. 1884. Montreal ...| Prof. R. S. Ball, F.R.S..........| Comets. 1885. Aberdeen ...|H. B. Dixon, M.A. ............ The Nature of Explosions. 1886. Birmingham | Prof. W. C. Roberts-Austen,|The Colours of Metals and their F.R.S. Alloys. 1887. Manchester) Prof. G. Forbes, F.R.S. ...... Electric Lighting. 1888. Bath......... SirJohn Lubbock,Bart.,F.R.S.|The Customs of Savage Races. 1889. Newcastle- |B. Baker, M. Inst.C. E. .........| The Forth Bridge. upon-Tyne 1890. Leeds ...... Prof. J. Perry, D.Sc., F.R.S. |Spinning Tops. 1891. Cardiff...... Prof. 8. P. Thompson, F.R.S. | Electricity in Mining. 1892. Edinburgh |Prof. C. Vernon Boys, F.R.S.| Electric Spark Photographs. 1893. Nottingham | Prof. Vivian B. Lewes......... Spontaneous Combustion. 1894. Oxford...... Prof. W. J. Sollas, F.R.S. ...|Geologies and Deluges. USSD ipswich... |r “AS Hy Wison <...2:5)..csseue Colour. 1896. Liverpool...|Prof. J. A. Fleming, F.R.S....|The Earth a Great Magnet. 1897. Toronto ...|Dr. H. O. Forbes ............... New Guinea. 1898. Bristol......| Prof. E. B. Poulton, F.R.S. |The ways in which Animals Warn their enemies and Signal to their friends. Ixxv _. OFFICERS OF SECTIONAL COMMITTEES PRESENT AT x THE BRISTOL MEETING. j SECTION A.—MATHEMATICAL AND PHYSICAL SCIENCE. | President.—Prof. W. E. Ayrton, F.R.S. | Vice-Presidents—The Rt. Hon. Lord Kelvin, G.C.V.O., F.R.S.; Sir ' Norman Lockyer, F.R.S. ; Prof. Mascart; Prof. A. W. Riicker, Sec.R.S. ; General-Major Rykatcheff ; Prof. 8. P. Thompson, F.R.S. ; Prof. 8. Young, E.RB.S. _ Secretaries.—Prof. A. P. Chattock, M.A.; J. L. Howard, D.Sc. ; C. H. Lees, D.Sc.; Prof. W. Watson, B.Sc. (Recorder); E. T. Whit- ‘ taker, B.A. SECTION B.—CHEMISTRY. President.—Prof. F. R. Japp, F.R.S8. Vice-Presidents.—Prof. E. Noelting ; J. H. Gladstone, F. R.S.; Prof. W. Ramsay, F.R8.; A. Vernon Harcourt, F.R.S. Prof. Emerson Reynolds, F.R. 8. ; W. J. Russell, F.R.S. ; W. Biakcodones E.R.S. i irice C0, A. Kohn (Recorder); F. ‘Wallis Stoddart; T. K. Rose. SECTION C.—GEOLOGY. President.—W. H. Hudleston, F.R.S8. Vice-Presidents.—R. Etheridge, F.R.S. ; Prof. T. Rupert Jones, F.R.S. ; . EE. B. Wethered ; W. Whitaker, F. R. S.; Rev. H. Winwood. Secretaries.—G. W. ampiodts Professor i. A. Miers, F.R.S. (Re- . corder); H. Pentecost. SECTION D.—ZOOLOGY. | President.—Prof. W. F. R. Weldon, M.A., F.R.S. Vice-Presidents.—Francis Galton, D.C.L., F.R.S. ; Prof. Francis Gotch, M.D., F.R.S. ; Prof. W. A. Herdman, D.Sc., F.R.S8.; Prof. O. C. Marsh ; Henry Woodward, LL.D., F.R.S. Secretaries. — Prof, R. Boyce ; Walter Catan M.A.; Dr. A. J. Har- rison ; W. E. Hoyle, M.A. (Recorder). SECTION E.—GEOGRAPHY. _ President.—Col. G. Earl Church, F.R.G.8. _ Vice-Presidents.—Col. F. Bailey, Sec. R.S.G.S. ; Prof. Boyd Dawkins, F.R.S. ; Colonel J. Farquharson, C.B. ; J. Scott Keltie, LL.D., Sec. R.GS. ; ; B. Leigh Smith; F. F. Tuckett ; General Sir Charles We Wilson, K.C.B., “R, RS. Secretaries. —H. N. Dickson, F.R.G.S.; H. R. Mill, D.Sc. F.R.G.S. (Recorder) ; H. C. Trapnell, LL.B. lxxvi REPORT—1898. SECTION F.—ECONOMIC SCIENCE AND STATISTICS, President.—J. Bonar, M.A., LL.D., F.8.8. Vice-Presidents.—Prof. E. C. K. Gonner, M.A., F.S.S.; L. L. Price, M.A., F.S.S.; Prof. W. Cunningham, D.D., F.S.S.; Rev. Canon Glazebrook, M.A. Secretaries.—E. Cannan, M.A., F.S.S.; Prof. A. W. Flux, M.A., FSS. ; H. Higgs, LL.B., F.S.S. (Recorder) ; W. E. Tanner, M.A. SECTION G.—MECHANICAL SCIENCE. President.—Sir John Wolfe-Barry, K.C.B., F.R.S., M.Inst.C.E, Vice-Presidents.—W. Proctor Baker; Sir Frederick Bramwell, Bart., D.C.L., F.R.S.; T. Forster Brown, M.Inst.C.E.; G. F. Deacon, M.Inst.C.E. Secretaries.—Prof. T. Hudson Beare, F.R.S.E. (Recorder); Prof. J. Munro, M.Inst.M.E. ; H. W. Pearson, M.Inst.C.E.; W. A. Price, M.A. SECTION H.—ANTHROPOLOGY, President.—E. W. Brabrook, C.B., F.S.A. Vice-Presidents—A. J. Evans, F.8.A.; Sir John Evans, K.C.B., F.B.S. ; Dr. Francis Galton, F.R.S. ; C. H. Read, F.S8.A. ; Dr. Paul Topinard ; Prof. E. B. Tylor, F.R.S. Secretaries—H. Balfour ; J. L. Myres, M.A., F.S.A. (Recorder); G. Parker, M.D. SECTION K,—BOTANY. President.—Prof. F, O. Bower, Sc.D., F.R.8. Vice-Presidents.—Prof. H. Marshall Ward, Se.D., F.R.S.; Dr. D. H. Scott, F.R.S. ; Francis Darwin, F.R.S. a C. Seward, F.R.S. (Recorder); Harold Wager; J. W. hite. OFFICERS AND COUNCIL, 1898-99. PRESIDENT. SIR WILLIAM OROOKES, F.R.S., V-P.O.S. VICE-PRESIDENTS. The Right Hon. the Fart of Ducr®, F.R.S., F.G.S. The PrRInctpat of University College, Bristol. The Right Rev. the Lorp BisHop of Bristol, D.D. The Master of The Society of Merchant Venturers The Right Hon. Sir Epwarp Fry, D.O.L., F.R.S., of Bristol. 4 FAS.A. JoHN BEDDOF, Esq., M.D., LL.D., F.R.S. Sir F. J. BRAMWELL, Bart., D.O.L., LL.D., F.R.S. Professor T. G. BONNEY, D.Sc., LL.D., F.R.S., F.S.A., The Right Worshipful the Mayor of Bristol. ¥.G.8. PRESIDENT ELECT. Professor MrcHAEL Foster, M.D., D.C.L., LL.D., Sec. B.S. VICE-PRESIDENTS ELECT. His Grace the LornD ARCHBISHOP OF OANIER- The MAJOR-GENERAL COMMANDING THE SOUTH- EASTERN DISTRICT. Bury, D.D. The Most Hon. the MARQUIS OF SALISBURY, K.G., The Right Hon. A. AkrRs-DouGLAsS, M.P. M.A., D.C.L., F.R.S. The Very Rev. F. W. FARRAR, D.D., F.R.S., Dean The Right Worsbipful the Mayor or Dovrr. of Canterbury. The Right Hon. LorD HERSCHELL, G.O.B., D.C.L., Sir J. Norman LockyYER, K.C.B., F.R.S., F.R.A.S, LL.D., F.R.S. Professor G. H. Darwin, M.A., LL.D., F.R.S. GENERAL SECRETARIES. Professor E. A. ScHArER, LL.D., F.R.S., University College, London, W.C. Professor W. 0. ROBERTS-AUSTEN, O.B., D.O.L., F.R.S., Royal Mint, London, E. ASSISTANT GENERAL SECRETARY. G. GrirrirH, Esq., M.A., College Road, Harrow, Middlesex. GENERAL TREASURER. Professor G. CAREY FosTERr, B.A., F.R.S., Burlington House, London, W. LOCAL SECRETARIES FOR THE MEETING AT DOVER, E, WOLLASTON KNocKER, Hsq., O.B. | W. H. PENDLEBURY, Esq., M.A. LOCAL TREASURER FOR THE MEETING AT DOVER. A. T. WALMISLEY, Esq., M.Inst.C.E. ORDINARY MEMBERS OF THE COUNCIL. Boys, C. VERNON, Esq., F.R.S. PREECE, W. H., Esq., O.B., F.R.S. Oreak, Captain E. W., R.N., F.R.S. Price, L. L., Esq., M.A. Darwin, F., Esq., F.R.S. REYNOLDS, Professor J. EMERSON, M.D., FREMANTLE, Hon. Sir O. W., K.C.B. F.R.S. GASKELL, Dr. W. H., F.R.S. . Suaw, W. N., Esq., F.R.S. HALurBURTON, Professor W. D., F.R.S. TEALL, J. J. H., Esq., F.R.S. Harcourt, Professor L. F. VERNON, M.A. THISELTON-DYER, W. T., Esq., C.M.G., F.R.S. HERDMAN, Professor W. A., F.R.S. THOMPSON, Professor S. P., F.R.S. KEL, J. Scott, Esq., LL.D. THomsoON, Professor J. M., F.R.S. Macmanoy, Masor P. A., F.R.S. TILDEN, Professor W. A., F.R.S. Marr, J.E., Esq., F.R.S. Tyxor, Professor E. B., F.R.S. MELDOLA, Professor R., F.R.S. Unwin, Professor W. C., F.R.S. Povutton, Professor E. B., F.R.S. WHITE, Sir W. H., K.C.B., 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 LUBBOCK, Bart., M.P., D.C.L., LL.D., F.R.S., F.L.S, The Right Hon. Lord RAYLEIGH, M.A., D.C.L., LL.D., F.R.S., F.R.A.S. Professor A. W. RUCKER, M.A., D.Sc., Sec. B.S. PRESIDENTS OF FORMER YEARS. The Duke of Argyll, K.G.,K.T. Sir John Lubbock, Bart.,F.R.S. | SirArchibald Geikie, LL.D.,F.R.S. Lord Armstrong, C.B., LL.D. Lord Rayleigh, D.C.L., F.R.S. Prof, J.S.Burdon Sanderson,F.R.S. Sir Joseph D. Hooker, K.C.S.I. , | Sir Wm. Dawson, O.M.G., F.B.S. | The Marquis of Salisbury, K.G., Sir G. G. Stokes, Bart., F.R.S. Sir H. E. Roscoe, D.C.L., F.R.S. F.R.S. Lord Kelvin, G.O.V.O., F.R.S. Sir F. J. Bramwell, Bart., Sir Douglas Galton, K.C.B., F.R.S. F.R.S. Prof. A. W. Williamson, F.R.S. Sir W. H. Flower, K.C.B., F.R.S. | Lord Lister, D.O.L., Pres. R.S. S. Prof. Allman, M.D., F.R.S. Sir F. A. Abel, Bart., K.0.B., F.R.S. | Sir John Evans, K.C.B., F.R.S. Sir Wm. Huggins, K.O.B., F.R.S. GENERAL OFFICERS OF FORMER YEARS. F. Galton, Esq., F.R.S. | P. L. Sclater, Esq., Ph.D., F.R.S. j Sir Douglas Galton, K.O.B..F.R.S. Prof. Michael Foster, Sec. R.S. Prof. T. G. Bonney, D.Se., F.R.S8. | A. Vernon Harcourt, Esq., F.R.S. 4 G. Griffith, Esq., M.A. Prof. A. W. Williamson, F.R.S. | Prof. A. W. Riicker, Sec. R.S. AUDITORS. Dr. J. H. Gladstone, F.R.S. | Dr. D. H. Scott, F.R.S. | Sir H. Trueman Wood, M.A. Ixxvili REPORT—1898. Dr. THE GENERAL TREASURER’S ACCOUNT, 1897-98. RECEIPTS, f s ds Balance brought forward .......:.cscccecseceecseneeescsccesonceseenss 2396 0 4 Life Compositions ......csccssssoccseecesnseeseccereresssensersvenesegs - 120 0 O New Annual Members’ pe cue Depebers’ cellos de> tues ee pane - 218 0 0 Annual Subscriptions Ciss.22- pecconccnusavescocssccccensccscevescensoss 465 0 0 Members of American ‘Association _ Be caused aee ev nasAvoedasenansne 159 0 O Sale of Associates’ Tickets ..........csssccecssessersccsscssseccccescses 648 0 0 Sale of Ladies’ Tickets .......cc.-csssencoscsneccescrscsssesenccscscees (103 0 0 Saleio£, PUDLCALIONS Wesstrecss>sescusDscesssecoss>ccsessesssscsecetersrs 175 17 O Interest on Deposit at Liverpool Bank .............scseseeecenee 24 5 6 Dividend On COnsols pp aaeccacesacsvacsasenesccsnaceccsocsescescecvoush 200 7 4 Dividend on India 3 per Cents ...........ssssecerereceeersseseecesnee 104 8 O Unexpended Balance of Grant returned by the Committee for the Calculation of certain Integrals ............sseeeeeeeeee 10 0 0 £4623 18 2 Investments. £ ee” Consols .....seeeees Ae edy ssecs ves aesieep sone ea creme 7537 3 6 ANGI ETICENES. scosstasneassssossssceventunentne 3600 0 0 £11,137 3° 5 ——————— ARTHUR W RUCKER, General Treasurer. GENERAL TREASURER’S ACCOUNT. lxxix from July 1, 1897, to June 30, 1898. Cr. 1897-98. EXPENDITURE. Expenses of Toronto Meeting, including Printing, Adver- tising, Payment of Clerks, &C. ......csscsssssssesseeccerreseeereee 108 9 7 Rent and Office Expenses .......ssssssscssesseeeseeesececeeseesseeeees 6016 0 PaaS eccestestcasecacccecstasseasess 0 Printing, Binding, &c. ............... 7 Payment of Grants made at Toronto: Ss. d. Electrical Standards..... aalaitle « eiale Bieta Miatals aie apoocacsae. Ge 0) ty Seismological Observations.......e+eeeeeeeeeeseeeeeens 75 0 0 Abstracts of Physical Papers.........es0.++0+ -- 100 0 0 Calculation of certain Integrals . ~~ 1070) 0 Electrolysis and Electro-chemistry ......... .. 35 0 0 Meteorological Observatory at Montreal.. Asicisisis\a\aiaiere 50 0 0 Wave-length Tables of the Spectra of the Blements . esisaj 420" ,0; 0 Action of Light upon Dyed Colours..........essseee0e8 8 0 0 Erratic Blocks......see.ssees Ae oa ne |< CUP RO CONE ae 2a 0 Investigation of a Coral POL 5 ages aati clo wicsalanin cass wee, RAD VOR.O Photographs of Geological Interest .........++-- ateioieta€ enlOc 0! 0 Life-zones in British Carboniferous Rocks..........- sen b0) 0 Pleistocene Fauna and Flora in Canada..........++ an veter 2a 0) 10. Table at the Zoological Station, Naples ...... edie voce’ nee LOGr Ol 0, Table at the Biological Laboratory, Plymouth.......... 14 0 0 Index Generum et Specierum Animalium..........-... 100 0 0 Healthy and Unhealthy Oysters ......... 30 0 0 Climatology of Tropical Africa ..... ane 10 0 0 State Monopolies in other Countries........... - 15 0 0 Small Screw Gauge ..........2--+- Gcidhe joistejaiateletaraiave iene 10 0 North-Western Tribes of Canada Saleieistoia! «le 0\s'e @aldials 0 0 Lake Village at Glastonbury..........seeeeecesecece 0 Silchester Excavation .........- Biel smivale sie.ciacicinietevais 0 Ethnological Survey of Canada. SEaisla ielele's s(a:cislejncisisiaicle 0 Anthropology and Natural History of Torres Strait... . 125 0 0 Investigation of Changes associated with the Functional Activity of Nerve Cells and their Peripheral Exten- sions . 5 Rta Oe slalelitetela/tls vieyaiaic@ aalere on.cis s'n/einioaimiaye ear kO URE O) Fertilisation in “Pheophycese Wialeide wis eleiaiaicie ofc ee hetieoaeteus Low Oi..0 ¥ Corresponding Societies Committee........ asta waielatsicis.en: M2 Ume Une U) 1212 0 0 In hands of General Treasurer : On deposit at Liverpool (National Provincial Bank) -ccccuswacscdsasctuascldocst ese. Susteee sseveensest MO GNSE A. uk At Bank of England, Western ‘Branch £219 11 1 Less Cheque not presented ............... 37 100 ee ek 1703 3 8 Bethy @asiiin: Wanders tees cgcss cece sce aenstacssause seen aanmasasacadeagas Oy 4 £4623 18 2 I have examined the above Account with the books and vouchers of the Associa- tion, and certify the same to be correct. I have also verified the balances at the bankers on Current and Deposit Accounts, and have ascertained that the Invest- ments are duly registered in the names of the Trustees. W. B. KEEN, Chartered Accountant, 3 Church Court, Old Jewry, E.C. eee July 12, 1898. ERBERT MCLEOD é D. H. Soorr . } Auditors. Ixxx REPORT—1898. Table showing the Attendance and Receipts Presidents Date of Meeting Where held 1831, Sept. 27...... York . 1832, June 19...... Oxford _ 1833, June 25...... Cambridge | a 1834, Sept. 8 ...... Edinburgh .. Sir T. M. Brisbane, D.O0.L 1835, Aug. 10...... Dublin ..... : 1836, Aug. 22...... Bristol ... .| The Marquis of Lansdowne 1837, Sept. 11......| Liverpool ............... 1838, Aug. 10...... Neweastle-on-Tyne... 1839, Aug. 26......| Birmingham ., 1840, Sept. 17...... Glasgow... 1841, July 20 ...... Plymouth .. ‘ 1842, June 23......| Manchester ..| The Lord Francis Egerton 1843, Aug. 17...... Cork: ese .| The Earl of Rosse, F.R.S. ... 1844, Sept. 26 ...... MOVE cee: 1845, June l9...... Cambridge .. 1846, Sept. 10 . ...| Southampton ¢ 1847, June 23 Oxford: Vif .| Sir Robert H. Inglis, Bart 1848, Aug. 9. Swansea... 1849, Sept. 12. Birmingham 1850, July 21 ...... 1851, July 2......... 1852, Sept.1 ...... 1853, Sept. 3 1854, Sept. 20...... 1855, Sept. 12...... 1856, Aug.6 ...... 1857, Aug. 26. 1858, Sept. 22. 1859, Sept. 14...... 1860, June 27...... 1861, Sept. 4 1862, Oct. 1 1863, Aug. 26 1864, Sept. 13 1865, Sept. 6 1866, Aug. 22 1867, Sept. 4 1868, Aug. 1869, Aug. 1870, Sept. 1871, Aug. 2 1872, Aug. 1873, Sept. 1874, Aug. 1875, Aug. 1876, Sept. 1877, Aug. 1878, Aug. 1879, Aug. 1880, Aug. 1881, Aug. 1882, Aug. 23...... 1883, Sept. 19...... 1884, Aug. 1885, Sept. 1886, Sept. 1887, Aug. 1888, Sept. 1889, Sept. 1890, Sept. 1891, Aug. 1892, Aug. 1893, Sept. 1894, Aug. 1895, Sept. 1896, Sept. 1897, Aug. 18...... 1898, Sept. 7 ....| Montreal .. .| Aberdeen , ....| Bath ....| Newcastle- ea ne,, .| Leeds i : ‘ Edinburgh .| Oxford .. 4 Eivenpoala Ki dinburgh Gute ees Dublin .. Leeds ... Aberdeen .. Cambridge ............ Newecastle-on-Tyne. Bath. scce..stheneveeese Birmingham, Nottingham . Southampton . Southport Nottingham. Ipswich .. Toronto ., Bristol “| The Rev. W. Buckland, F.R.S. .| The Rev. A. Sedgwick. F.R.S. ..| The Rey. Provost Lloyd, LL.D. . "| The Rev. W. Whewell, F.R.S. _.| The Rey. G. Peacock, DD. ..... __| Sir Roderick I. Murchison, Bart. f “| The Marquis of Northampton , .| The Rey. T. R. Robinson, D.D.. . | G. B. Airy, Astronomer Royal . ..| Lieut.-General Sabine, F.R:S. . ..| William Hopkins, F'.R.S........... ..| The Earl of Harrowby, F.R.8. ..| The Duke of Argyll, F.R.S. . ..| Prof. C. G. B. Daubeny, M.D..... or ..| The Rev. Humphrey Lloyd, D.D....... ..| Richard Owen, M.D., D.O.L. . ..| H.R.H. The Prince Consort . ..| The Lord Wrottesley, M.A. .. .| William Fairbairn, ioap Di, R. s ..| Sir William G. Armstrong, O.B. . .| Prof. J. Phillips, M.A., LL.D. "| Dr. C. W. Siemens F.R.S. pian ...| Prof..A. Cayley, D.C.L., ERS... .| Prof. Lord Rayleigh, ERS. .| Sir F. A. Abel, C.B., PRS. "| Sir A. Geikie, LL.D. ERS. _.. .| Prof. J. S. Burdon Sanderson | "| Sir Douglas Galton, F.RS.. = .| Sir Joseph Lister, Bart., Pres. B.S. ine ‘| Sir W. Crookes, FURS. ......c.0e0-+- The Earl Fitzwilliam, D.C.L. The Ear! of Burlington, F.R.S., The Duke of Northumberland . The Rey. W. Vernon Harcourt, The Marquis of Breadalbane. Sir John F. W. Herschel, Bart. Sir David Brewster, K.H. ....... The Rev. Professor Willis, ALAC Sir Charles Lyell, Bart., MLA. ......... William R. Grove, Q. C., F.R.S Dundee .. The Duke of Buceleuch, K.C. B. Norwich ..| Dr. Joseph D. Hooker, F.R.S. Exeter ..... ..| Prof. G. G. Stokes, D.C.L. .... Liverpool .. .| Prof. T. H. Huxley, LL.D..... Edinburgh ..| Prof. Sir W. Thomson, LL.D. . Brighton .. ..| Dr. W. B. Carpenter, F.R.S. Bradford .. 3.| Prot. A. W. Williamson, ERS. Belfast . .| Prof. J. Tyndall, LL.D. JPRS. - Bristol .. ...| Sir John Hawkshaw, ©. E. ERS. Glasgow ..| Prof. T. Andrews, M.D., F.R.S.. Plymouth ., ...| Prof. A. Thomson, M.D., F.R.S....... JD Eoin eee ...| W. Spottiswoode, M.A., T. Soo sees Sheffield... ...| Prof. G. J. Allman, M.D.. F.R.S Swansea... ...| A. O. Ramsay, LL.D., F.R.S....... York .| Sir John Lubbock, Bart., F.R.S Sir Lyon Playfair. K.C.B., FRS....... .| Birmingham .........| Sir J. W. Dawson, C.M.G., F.R.S....... Manchester .... .| Sir H. E. Roscoe, D.C.L., F.R.S. Sir F. J. Bramwell, F.R.' B. Prof. W. H. Flower, ©.B., RS. Or WwW: Hugzins, ERS The Marquis of Salisbury,K.G.,F.R. 8. Sir John Evans, K.OB., E.RS. ... * Ladies were not admitted by purchased tickets until 1843, Old Life Members New Life Members o6) ee Oe ee ee + Tickets of Admission to Sections only. ATTENDANCE AND RECEIPTS AT ANNUAL MEETINGS. lxxxi at Annual Meetings of the Association. Attended by el Sums paid receivenan ies Account Old New Meas during the fi ania Year Annual | Annual mates Ladies |Foreigners} Total Meeting °P oe Members | Members wnGSS —_ — cd —_ _ 353 —_ —_ 1831 _- — — _ _— _ — —- 1832 _ —s — _ — 900 -— —_ 1833 — — = — _ 1298 — £20 0 0 1834 SS — a _ — — _ 167 0 0 1835 _ _ — _ — 1350 — 435 0 1836 — _ = _ _— 1840 — 922 12 6 1837 _— _ _ 1100* _— 2400 -- 932 2 2 1838 — = = = 34 1438 — 1595 11 0 1839 = = — = 40 1353 _ 1546 16 4 1840 46 317 _ 60* — 891 —_— 1235 10 11 1841 75 376 33f 331* 28 1315 _— 144917 8 1842 71 185 _ 160 —_— — _— 1565 10 2 1843 45 190 9 260 — — — 98112 8 1844 : 94 22 407 172 35 1079 = 831 9 9| 1845 65 39 270 196 36 857 — 685 16 0 1846 | 197 40 495 203 53 1320 — 208 5 4 1847 54 25 376 197 15 819 £707 0 0] 275 1 8 1848 93 33 447 237 22 1071 963 0 OO} 15919 6 1848 128 42 510 273 44 1241 1085 0 0} 34518 0 1850 61 47 244 141 37 710 620 0 0 391 9 7 1851 63 60 510 292 9 1108 1085 0 0 304 6 7 1852 56 57 367 236 6 876 903 0 0 205 0 0 1853 121 121 765 524 10 1802 1882 0 0 380 19 7 1854 142 101 1094 543 26 2133 2311 0 0 480 16 4 1855 104 48 412 346 9 1115 1098 0 0 73413 9 1856 156 120 900 569 26 2022 2015 0 0 507 15 4 1857 111 91 710 509 13 1698 1931 0 0 61818 2 1858 125 179 1206 821 22 2564 2782 0 0 684 11 1 1859 177 59 636 463 47 1689 1604 0 0 766 19 6 1860 184 125 1589 791 15 3138 3944 0 0] 1111 5 10 1861 150 57 433 242 25 11 1089 0 0} 129316 6 1862 154 209 1704 1004 25 3335 3640 0 0] 1608 3 10 1863 182 103 1119 1058 13 2802 2965 0 0/ 128915 8 1864. 215 149 766 508 23 1997 2227 0 0| 1591 7 10 1865 218 105 960 771 11 2303 2469 0 0/|175013 4 1866 193 118 1163 771 7 2444 2613 0 0/1739 4 0 1867 226 117 720 682 45t 2004 2042 0 0/1940 0 0 1868 229 107 678 600 17 1856 1931 0 0| 1622 0 0 1869 303 195 1103 910 14 2878 3096 0 0] 1572 0 0 1870 311 127 976 754 21 2463 2575 0 0] 1472 2 6 1871 280 80 937 912 43 2533 2649 0 0] 1285 0 0 1872 237 99 796 601 nol 1983 2120 0 0} 1685 0 0 1873 232 85 817 630 12 1951 1979 0 0| 115116 0 1874 307 93 884 672 17 2248 2397 0 0| 960 0 0 1875 331 185 1265 712 25 2774 3023 0 0| 1092 4 2 1876 238 59 446 283 11 1229 1268 0 0] 1128 9 7 1877 290 93 1285 674 17 2578 2615 0 0 72516 6 1878 239 74 529 349 13 1404 1425 0 0} 1080 11 11 1879 171 41 389 147 12 915 g99 0 0 yi Nf 1880 313 176 1230 514 24 2557 2689 0 0 476 8 1 1881 253 79 516 189 21 1253 1286 0 0} 1126 111 1882 330 323 952 841 5 2714 3369 0 0 | 1083 3 3 1883 317 219 826 74 26 & 60 H.§ 1777 1855 0 0| 1173 4 0 1884 332 122 1053 447 6 2203 2256 0 0 | 1385 0 0 1885 428 179 1067 429 11 2453 2532 0 0 995 0 6 1886 510 244 1985 493 92 3838 4336 0 0| 118618 0 1887 399 100 639 509 12 1984 2107 0 0| 1511 0 5 1888 412 113 1024 579 21 2437 2441 0 0} 1417 O11 1889 368 92 680 334 12 1775 1776 0 0 789 16 8 1890 Mf 341 152 672 107 35 1497 1664 0 O| 102910 0 1891 ") 413 141 733 439 50 2070 2007 0 0| 86410 0 1892 Py 6 328 _ 57 773 268 17 1661 1653 0 0 907 15 6 1893 435 69 941 451 77 2321 2175 0 0 683 15 6 1894 4, 290 31 493 261 22 1324 1236 0 0 977 15 5 1895 383 139 1384 873 41 3181 3228 0 0| 1104 6 1 1896 286 125 682 100 41 1362 1398 0 0/}] 105910 8 1897 327 96 1051 639 33 2446 2399 0 0| 1212 0 0 1898 ————EE————————————————————S SSS SSS a aareereeeeenll ss $ Including Ladies, § Fellows of the American Association were admitted as Hon. Members for this Meeting. 1898, e lxxxil REPORT—1898. REPORT OF THE COUNCIL. Report of the Council for the Year 1897-98, presented to the General Committee at Bristol on Wednesday, September 7, 1898. The Meeting held at Toronto last August was attended by a represen- tative body of members from the British Isles and from the Dominion ‘of Canada, and bya large number of scientific men from the United States of America and from the Continent of Europe. The success of the Meeting had been confidently anticipated in view of the experience of the Montreal Meeting in 1884, and that this anticipation was fully realised was largely the result of the unremitting exertions of the Local Officers and Committee at Toronto, and the support which was received from the Government of the Dominion, the Government of Ontario, and the City of Toronto. A Permanent Committee on Terrestrial Magnetism and Atmospheric Electricity was appointed at the Meeting of the International Meteoro- logical Conference at Paris in 1896. The members of this body were desirous of holding a Conference with other magneticians, and at the suggestion of Professor Riicker, who is President of the Committee, the Council decided to invite the Committee to hold the Conference at Bristol during the Meeting of the British Association. This invitation was accepted, and it was decided that the Conference should meet asa Department of Section A, and that the foreign magneticians who might attend should have all the privileges of foreign members of the Associa- tion. The Council have reason to believe that this arrangement will work satisfactorily, and that the Conference will be well attended. The Council have nominated the Master of the Society of Merchant Venturers to be a Vice-President of the Association for the Meeting at Bristol, in addition to the Vice-Presidents elected at the last meeting of the General Committee. The Council have received Reports from the General Treasurer during the past year, and his Accounts from July 1, 1897, to June 30, 1898, which have been audited, will be presented to the General Committee. The Council have been informed by Professor Riicker that he does not intend to offer himself for re-election as General Treasurer after the Bristol Meeting. Professor Riicker has held this post since 1891, and the Council desire to put on record their sense of the important services which Professor Riicker has rendered to the Association during this period. The Council recommend that Professor G. Carey Foster, F.R.S., be appointed General Treasurer in succession to Professor Riicker. The Council have to deplore the loss by death of Lord Playfair, who had been one of the Trustees of the Association since 1883. The Council have nominated Professor Riicker as Trustee, the other Trustees being Lord Rayleigh and Sir John Lubbock. The Council have elected the following men of Science who have attended Meetings of the Association to be Corresponding Members :— Professor C. Barus, Brown University. Professor E. W. Morley, Cleveland, M. C. de Candolle, Geneva. Ohio. Dr. G. W. Hill, West Nyack, N.Y. Professor C. Richet, Paris. Professor Oskar Montelius, Stockholm. | Professor W. B. Scott, Princeton, N.J. The Council were invited to nominate one or two Members to give REPORT OF THE COUNCIL. lxxxili evidence before the Committee appointed by the Government to report on the desirability of establishing a National Physical Laboratory, and at their request Professor G. Carey Foster, F.R.S., and Professor W. E. Ayrton, F.R.S., gave evidence before this Committee. A Report has been presented to Parliament, and the Council trust that the delibera- tions of the Committee will result in the establishment of a National Laboratory. In regard to the Resolutions referred to them for consideration and action, if desirable, the Council have to report :— (1) That the Council appointed a Committee to consider the desira- bility of approaching the Government with a view to the establishment in Britain of experimental Agricultural Stations similar in character to those which are producing such satisfactory results in Canada. The Committee having reported that much is already being done in this direction by County Councils and Agricultural Societies, advised that the co-operation of these bodies should first be invited. The Committee was re-appointed for this purpose, and sent in a Report, the principal recommendation of which was adopted by the Council, and is as follows : ‘Your Committee recommend that the Board of Agriculture be in- formed that, in the opinion of the British Association, there is an urgent need for the co-ordination of existing institutions for agricultural research, and that the Association hopes that steps may be taken towards this end, including the strengthening of the scientific work of the Board of Agri- culture and the provision of the means for dealing adequately with scien- tific questions which may come before it.’ At the request of the Council this Report was brought by the Presi- dent to the notice of the President of the Board of Agriculture, from whom the following reply was received :— Board of Agriculture, 4 Whitehall Place, London, S.W., 26th July, 1898. Srr,—I have laid before the Board of Agriculture your letter of the 18th inst., and I am desired to express to the Council of the British Association for the Advancement of Science the thanks of the Board for the attention which the Council have been so good as to give to the important subject of agricultural research. The Board will not fail to bear in mind the views set out in the Resolution com- municated to them in the letter above referred to. Iam, Sir, your obedient servant, P. G. CRAIGIE, Assistant Secretary. Sir John Evans, K.C.B., F.R.S., &c., President of the British Association for the Advancement of Science, Burlington House, W. (2) That a Committee was appointed to report to the Council whether, and, if so, in what form, it is desirable to bring before the Canadian Government the necessity for a Hydrographic Survey of Canada, and that the following formed the Committee :—Professor A. Johnson (Chairman and Secretary), Lord Kelvin, Professor G. H. Darwin, Admiral Sir W. J. L. Wharton, Professor Bovey, and Professor Macgregor. The Committee reported to the Council, and it was decided, in con- formity with the recommendation contained in the Report, that the following Resolution should be sent to the Canadian Government :— ‘The Council of the British Association have learnt with regret that the Government of the Dominion of Canada is contemplating the discon- tinuance of their Tidal Survey of Canadian Waters. Whilst the work already carried out is primarily connected with Hydrography and Navi- e2 Ixxxiv REPORT—1898. gation, they consider that Science will incur a great loss if the work of the Survey is discontinued. They would, therefore, urge on the Govern- ment the desirability of continuing the Tidal Survey as heretofore.’ The President transmitted the Resolution to the Governor-General, who forwarded it to the Government of the Dominion of Canada for their favourable consideration. The Council have received the following in reply :— Extract from a Report of the Committee of the Honourable the Privy Council, approved by His Excellency on the 20th June, 1898. On a Report dated 25th April, 1898, from the Minister of Marine and Fisheries,. stating that he has had under consideration a letter, dated 9th March, 1898, from the President of the British Association for the Advancement of Science, enclosing a resolution adopted at a meeting of the Council of the Association, urging the desira- bility of continuing the Tidal Survey as heretofore. The Minister recommends that the Association be informed that, in view of the limited appropriation made by Parliament, it has been deemed advisable to defer the prosecution of the Survey for the present, and to confine the work to the maintenance and operations of the Tidal gauges already established, and the preparation of tide. tables. The Committee submit the same for your Excellency’s approval. JOHN J. MCGEE, Clerk of the Privy Council. (3) That a Committee was appointed by the Council to consider the: following Resolution : ‘That, in view of the facts (a) that a Committee of Astronomers appointed by the Royal Society of London, in consequence: of a communication from the Royal Society of Canada, has recently con- sidered the matter, and has arrived at the conclusion that no change can now be introduced in the “‘ Nautical Almanac ” for 1901, and (6) that few English astronomers are attending the Toronto meeting of the Association : the Committees of Sections A and E are not in a position to arrive at. any definite conclusions with respect to the Unification of Time; but they think it desirable to call the attention of the Council to the subject, in which the interests of mariners are deeply involved, with the view of their taking such action in the matter as may seem to them to be desirable.’ Several members of this Committee had also served on the Committee of the Royal Society, and after careful re-consideration of the whole question the Committee saw no good reason for dissenting from the con- clusion which had been recently adopted by the Royal Society, and reported in the following terms :— ‘The Committee report that, as there is a great diversity of opinion amongst astronomers and sailors as to the desirability of the adoption of civil reckoning for astronomical purposes, and as it is impossible to carry out such a change in the “ Nautical Almanac” for the year 1901, they do. not recommend that the Council of the British Association should at present take any steps in support of the suggested change of reckoning.’ The President has transmitted this Report to the Royal Society of Canada. In their Report last year at Toronto the Council informed the General Committee that the establishment of a Bureau for Ethnology was under the consideration of the Trustees of the British Museum. Since that date, the following letter, addressed to the President, has been received : British Museum, December 15, 1897. Dear Sir John Evans,—Referring to a letter of May 19 last, from Lord Lister, as. President of the British Association for the Advancement of Science, requesting the Trustees of the British Museum to consider whether they could allow a Bureau for ——————————————— eee Pe REPORT OF THE COUNCIL. lxxxv Ethnology for Greater Britain to be established in connection with the Museum, I am directed by the Trustees to inform you that they are quite of opinion that such a Bureau might be administered in connection with the Ethnographical Section of their collections with advantage both to the objects in view of the Association and to the enlargement of the British Museum collections. They are, therefore, willing to accept in principle the proposal of the British Association, and they would be ready to take the necessary steps for carrying it into effect so soon as certain re-arrangements affecting space, &c., which are now taking place within the Museum, shall have been finished, as it is expected, in the course of the coming year. Believe me, yours very truly, E. MAUNDE THOMPSON, Sir John Evans, K.C.B., D.C.L, LL.D., &c. &c. The Report of the Corresponding Societies Committee for the past year, together with the list of the Corresponding Societies and the titles of the more important papers, and especially those referring to Local Scientific Investigations, published by those Societies during the year ending June 1, 1898, has been received. The Corresponding Societies Committee, consisting of Mr. Francis Galton, Professor R. Meldola (Chairman), Sir Douglas Galton, Dr. J. G. Garson, Sir J. Evans, Mr. J. Hopkinson, Mr. W. Whitaker, Mr. G. J. Symons, Professor T. G. Bonney, Mr. T. V. Holmes, Sir Cuthbert E. Peek, Mr. Horace T. Brown, Rev. J. O. Bevan, and Professor W. W. Watts, is hereby nominated for reappointment by the General Committee. The Council nominate Mr. W. Whitaker, F.R.S., Chairman, and Mr. T. V. Holmes, Secretary, to the Conference of Delegates of Corre- sponding Societies to be held during the Meeting at Bristol. The Council announce with very great regret the loss that they have recently sustained by the death of Dr. John Hopkinson, F.R.S8. In accordance with the regulations the retiring Members of the Council will be :— Edgeworth, Professor. Symons, Mr. G. J. Horsley, Mr. Victor. Ramsay, Professor W. The Council recommend the re-election of the other ordinary Members of the Council, with the addition of the gentlemen whose names are dis- _ tinguished by an asterisk in the following list :— Boys, C. Vernon, Esq., F.R.S. Preece, W. H., Esq., C.B., F.R.S. Creak, Captain E. W., R.N., F.R.S. *Price, L. L., Esq., M.A. Darwin, I’., Esq., F.R.s. Reynolds, Professor J. Emerson, M.D , Fremantle, The Hon. Sir C. W., K.C.B. E.R.S. *Gaskell, Dr. W. H., F.R.S. Shaw, W. N., Esq., F.R.S. - Halliburton, Professor W. D., F.R.S. Teall, J. J. H., Esq., F.R.S. Harcourt, Professor L. F. Vernon, M.A., Thiselton-Dyer, W. T., Esq., C.M.G. M.Inst.C.E. F.R.S. Herdman, Professor W. A., F.R.S. Thompson, Professor S. P., F.R.S. *Keltie, J. Scott, Esq., LL D. Thomson, Professor J. M., F.R.S. *MacMahon, Major P. A., F.R.S. *Tilden, Professor W. A., F.R.S. Marr, J. E., Esq., F.R.S. Tylor, Professor E. B., F.R.S. Meldola, Professor R., F.R.S. Unwin, Professor W. C., F.R.S. Poulton, Professor E. B., F.R.S. White, Sir W. H., K.C.B., F.R.S. An invitation to hold the Annual Meeting of the Association in the year 1900 at Bradford, and an invitation from Cork for a future Meeting, have been received, and will be presented to the General Committee on Monday, September 12. Ixxxvi REPORT—1898. CoMMITTEES APPOINTED BY THE GENERAL COMMITTEE AT THE Bristol: MEETING IN SEPTEMBER 1898. 1. Receiving Grants of Money. Subject for Investigation or Purpose Members of the Committee Making Experiments for improv- ing the Construction of Practical Standards for use in Electrical Measurements. {And 751., last year’s grant not | expended. | Seismological Observations. To assist the publication ‘Science Abstracts.’ of Experiments on the Heat of com- bination of Metals in the forma- tion of Alloys. Chairman.—Lord Rayleigh. Secretary.—Mr. R. T. Glazebrook. Lord Kelvin, Professors W. E. | Ayrton, J. Perry, W. G. Adams, | Oliver J. Lodge, and G. Carey Foster, Dr. A. Muirhead, | Mr. W. H. Preece, Profes- sors J. D. Everett and A. Schuster, Dr. J. A. Fleming, Professors G. F. FitzGerald and J.J. Thomson, Mr. W. N. Shaw, Dr. J. T. Bottomley, Rev. T. C. Fitzpatrick, Professor J. Viriamu Jones, Dr. G. John- stone Stoney, Professor S. P. Thompson, Mr. J. Rennie, Mr. E. H. Griffiths, Professor A. W. Riicker, and Professor H. L. Callendar. Chairman.—Prof. J. W. Judd. Seeretary.—Professor J. Milne. Lord Kelvin, Sir F. J. Bramwell, Professor G. H. Darwin, Mr. Horace Darwin, Major L. Dar- win, Professor J. A. Ewing, Professor C. G. Knott, Professor R. Meldola, Professor J. Perry, Professor J. H. Poynting, Pro- fessor T. G. Bonney, Mr. C. V. Boys, Professor H. H. Turner, Mr. G. J. Symons, and Dr. C. Davison. Chairman.— Professor ; D 30 Botany. *Farmer, Professor J. B.—Fertilisation in Pheophycee ...... 20 0 0 Darwin, Mr. F.—Assimilation in Plants .........-...2.s000e0 00s 20 O 0 *Stebbing, Rev. T. R. R.—Zoological and Botanical Publica- tion A. sae. iss beads fee , os PE S10 IG Corresponding Societies, *Meldola, Professor R.—Preparation of Report .............. 25 0 0 21,4955) 0 * Reappointed. SYNOPSIS OF GRANTS OF MONEY. xclx The Annual Meeting in 1899. ~The Annual Meeting of the Association in 1899 will commence on Wednesday, September 13, at Dover. The Annual Meeting in 1900. The Annual Meeting of the Association in 1900 will be held at Brad- ford. The Annual Meeting in 1901. _. The Annual Meeting of the Association in |1901 will he held at Glasgow. ne c REPORT—1 898. General Statement of Sums which have been paid on account of Grants for Scientific Purposes. 1834. 8: a. Tide Discussions ......+ esau tees 20 0 0 1835 Tide Discussions ..........000+ 62 0 0 British Fossil Ichthyology ... 105 0 0 £167 O OU 1836. Tide Discussions .........+ee++s 163 0 0 British Fossil Ichthyology ... 105 0 0 Thermometric Observations, RG rmiiseisa siceeusucccscssshevsceras 50 0 0 Experiments on Long-con- tinued Heat .........ccceseeee 17 1 0 Rain-Gauges .......escsecseeoeees 913 0 Refraction Experiments ...... 15 0 0 Lunar Nutation............ss006 60 0 0 Thermometers .......eeseeseeeee 15 6 0 £435 0 O 1837 Tide Discussions .........ses00s 284 1 0 Chemical Constants ............ 2413 6 Lunar Nutation.............0660. 70 0 0 Observations on Waves ...... 100 12 O Tides at Bristol .........:0s..2.0e 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 SAT OMECUCTS « sececcss create cctestesie 1118 6 £922 12 6 1838 Tide Discussions ............64+ 29 0 0 British Fossil Fishes............ 100 0 O Meteorological Observations . and Anemometer (construc- HHO) “Seo oso sbaneeanasoasags 100 0 O Cast Iron (Strength of) ...... 60 0 0 Animal and Vegetable Sub- stances (Preservation of)... 19 1 10 Railway Constants ............ 41 12 10 IBTISLOLMLIGES eyetunwatcascatsepe 10 Explorationof RaygillFissure 20 Naples Zoological Station ... 80 Albuminoid Substances of RICE Masncacscasdaceacneces «scons 10 Elimination of Nitrogen by Bodily Exercise............... 50 Migration of Birds ............ 15 Natural History of Socotra... 100 Natural History of Timor-lant 100 Record of Zoological Litera- SED etic hs pendsesceecnos< sacs: 100 Anthropometric Committee... 50 £i 126 So C0 Sooo OoCCONWOS COSY H1O CO SOOO OCOOHOCSCOCSOSS®S Or SONS, O° eSs FS =) CBI) SOOO. OS), (Oe OO Se 2S. Eo: ao! Coco so soc S'S. ic ooo | _ i = 1885. £ Meteorological Observations on Ben NeViS........sseseeees 50 Isomeric Naphthalene Deri- ALU CSerescnesns ss e-seeteeeneee - 15 0 0 West Indian Explorations ... 100 0 0 Flora Of China .........sssssee0e 25 0 0 Naples Zoological Station ... 100 0 0 Physiology of Lymphatic SV SOC: Seistivmace es)- veisaue ite 25 0 0 Experiments with a Tow-net 516 3 Natural History of Friendly TSIANGS): -bseaepscecnsed ence tree 100 0 0 Geology and Geography of Atlas Ranges c...s.<.> Ose ke 10 0 0 Erratic Blocks /.............06.0: 15 0 0 Photographs of Geological IMERESE 5.5.0. ttectesweces esate: 20 0 0 Underground Waters ......... 10 0 0 Investigation of Elbolton Wave rncctsetossscateedaceatescters 25 0 O Excavations at Oldbury Hill 10 0 0 Cretaceous Polyzoa ............ 10 0 O Naples Zoological Station ... 100 0 0 Marine Biological Association 1710 0 Deep-sea Tow-net ............... 40 0 0 Fauna of Sandwich Islands... 100 0 0 Zoology and Botany of West India, Islands <<......sssesseece 100 0 0 Climatology and Hydrography of Tropical Africa......... .. 50 0 O Anthropometric Laboratory... 5 0 0 Anthropological Notes and Queries iic-cer co, osesarheetarare 20 -0 0 Prehistoric Remains in Ma- Shonaland) \..ccuscsisnce tones 50 0 0 North-Western Tribes of Canada Vilesaseesdasessers cases 100 0 0 Corresponding Societies ...... 25 0 0 £864 10 O 1893. Electrical Standards............ 25 0 O Observations on Ben Nevis... 150 0 0 Mathematical Tables ......... 15 0 O Intensity of Solar Radiation 2 8 6 Magnetic Work at the Fal- mouth Observatory ......... 25 0 0 Isomeric Naphthalene Deri- VALVES faaterecocdedtres scene te 20 0 0 HirraticuBlocks” .t. seanieeetppne staat cas 40 Anthropometrical Measure- 0 ments in Schools ............ Dee Mental and Physical Condi- tion of Children............... 20 0 ae 0 5 £583 1 Oo 1895. ae Electrical Standards........... . 26 0 Photographs of Meteorological iPhenomenday,. -....:tsecnseexey 10 0 Marth Wremors: .-....2iveesessdas 75 0 Abstracts of Physical Papers 100 0 Reduction of Magnetic Obser- vations made at Falmouth Observatory <..i..ccsecseweees 50 0 Comparison of Magnetic Stan- GANS fuses sous sedi seetene 25 0 Meteorological Observations On Ben Nevis .......s0ceessneee 50 0 Wave-length ‘lables of the Spectra of the Elements... 10 0 Action of Light upon Dyed WOlOUTS Sie... stese <-deweweaponed 4 6 Formation of Haloids from Pure Materials ...........0..- 20 0 Isomeric Naphthalene Deri- MAULVESte tea wwiddecs cssruserete 30 0 Electrolytic Quantitative An- BUIVEISE.. sascvecavencectasorsseeas 30 0 Mirtatic BLOCKS) )2:s 10 0 0 Photographs of Geological HE TES ines ceieaceeeceias eoaa tents 145 0 0 Remains of the Irish Elk in the Isle of Man ............... Wy gh Un Table at the Zoological Sta- tion Naples! saruneeeee 25 0 0 Ee: £1,212 00 General Meetings. On Wednesday, September 7, at 8 p.m., in the People’s Palace, Bristol, Sir John Evans, K.C.B., D.C.L., LL.D., resigned the office of President to Sir William Crookes, F.R.S., V.P.C.S., who took the Chair, and delivered an Address, for which see page 3. On Thursday, September 8, at 8.30 p.m., a Soirée took place in the Clifton College. On Friday, September 9, at 8.50 p.m., in the People’s Palace, Professor W. J. Sollas, M.A., F.R.S., delivered a discourse on ‘ Funafuti: the Study of a Coral Island.’ On Monday, September 12, at 8.30 p.m., in the People’s Palace, Herbert Jackson, Esq., delivered a discourse on ‘ Phosphorescence.’ On Tuesday, September 13, at 8.30 p.m., a Soirée took place in the Clifton College. On Wednesday, September 14, at 2.30 p.m., in the Museum, the con- cluding General Meeting took place, when the Proceedings of the General Committee and the Grants of Money for Scientific Purposes were explained to the Members. The Meeting was then adjourned to Dover. [The Meeting is ap- painted to commence on Wednesday, September 13, 1899.] ADDRESS BY SIR WILLIAM CROOKES, F.RS., V.P.CS. PRESIDENT. For the third time in its history the British Association meets in your City of Bristol. The first meeting was held under the presidency of the Marquis of Lansdowne in 1836, the second under the presidency of Sir John Hawkshaw in 1875. Formerly the President unrolled to the _ meeting a panorama of the year’s progress in physical and biological sciences. To-day the President usually restricts himself to specialities connected with his own work or deals with questions which for the time are uppermost. To be President of the British Association is undoubtedly a great honour. It is alsoa great opportunity and a great responsibility ; for I know that, on the wings of the Press, my words, be they worthy or not, will be carried to all points of the compass. I propose first to deal with the important question of the supply of bread to the inhabitants of these Islands, then to touch on subjects to which my life work has been more or less devoted. I shall not attempt any _ general survey of the sciences; these, so far as the progress in them demands attention, will be more fitly brought before you in the different Sections, either in the Addresses of the Presidents or in communications from Members. Before proceeding with my address I wish to refer to the severe loss the British Association has sustained in‘the death of Lord Playfair. With Sir John Lubbock and Lord Rayleigh, Lord Playfair was one of the _ Permanent Trustees of our Association, and for many years he was _ present at our meetings. It would be difficult to overrate his loss to British science. Lord Playfair’s well-matured and accurate judgment, his scientific knowledge, and his happy gift of clothing weighty thoughts in persuasive language, made his presence acceptable, whether in the council chamber, in departmental enquiries, or at light social gatherings, where by the singular laws of modern society, momentous announcements are sometimes first given to the world. Lord Playfair (then Sir Lyon B2 4 REPORT—1898. Playfair) was President of the British Association at Aberdeen in 1885 ; his Address on that occasion will long be remembered as a model of pro- found learning and luminous exposition. And now I owe a sort of apology to this brilliant audience. I must ask you to bear with me for ten minutes, for I am afraid what I now have to say will prove somewhat dull. I ought to propitiate you, for, to tell the truth, I am bound to bore you with figures. Statistics are rarely attractive to a listening audience ; but they are necessary evils, and those of this evening are unusually doleful. Nevertheless, when we have pro- ceeded a little way on our journey I hope you will see that the river of figures is not hopelessly dreary. The stream leads into an almost unex- plored region, and to the right and left we see channels opening out, all worthy of exploration, and promising a rich reward to the statistic explorer who will trace them to their source—a harvest, as Huxley expresses it, ‘immediately convertible into those things which the most sordidly practical of men will admit to have value, namely, money and life.’ My chief subject is of interest to the whole world—to every race— to every human being It is of urgent importance to-day, and it is a life and death question for generations to come. I mean the question of Food supply. Many of my statements you may think are of the alarmist order ; certainly they are depressing, but they are founded on stubborn facts. They show that England and all civilised nations stand in deadly peril of not having enough to eat. As mouths multiply, food resources dwindle. Land is a limited quantity, and the land that will grow wheat is absolutely dependent on difficult and capricious natural phenomena. Iam constrained to show that our wheat-producing soil is totally unequal to the strain put upon it. After wearying you with a survey of the universal dearth to be expected, I hope to point a way out of the colossal dilemma. It is the chemist who must come to the rescue of the threatened communities. It is through the laboratory that starvation may ultimately be turned into plenty. The food supply of the kingdom is of peculiar interest to this meeting, considering that the grain trade has always been, and still is, an important feature in the imports of Bristol. The imports of grain to this city amount to about 25,000,000 bushels per annum—8,000,000 of which consist of wheat. What are our home requirements in the way of wheat? The con- sumption of wheat per head of the population (unit consumption) is over 6 bushels per annum ; and taking the population at 40,000,000, we require no less than 240,000,000 bushels of wheat, increasing annually by 2,000,000 bushels, to supply the increase of population. Of the total amount of wheat consumed in the United Kingdom we grow 25 and import 75 per cent. So important is the question of wheat supply that it has attracted the attention of Parliament, and the question of national granaries has been mooted, It is certain that, in case of war with any of the Great Powers, . pa ADDRESS. 5) wheat would be contraband, as if it were cannon or powder, liable to capture even under a neutral flag. We must therefore accept the situation and treat wheat as munitions of war, and grow, accumulate, or store it as such. It has been shown that at the best our atock of wheat and flour amounts only to 64,000,000 bushels—fourteen weeks’ supply—while last April our stock was equal to only 10,000,000 bushels, the smallest ever recorded by ‘Beerbohm’ for the period of the season. Similarly, the stocks held in Europe, the United States, and Canada, called ‘the world’s visible supply,’ amounted to only 54,000,000 bushels, or 10,000,000 less than last year’s sum total, and nearly 82,000,000 less than that of 1893 or 1894 at the corresponding period. ‘To arrest this impending danger, it has been proposed that an amount of 64,000,000 bushels of wheat should be purchased by the State and stored in national granaries, not to be opened, except to remedy deterioration of grain, or in view of national . disaster rendering starvation imminent. This 64,000,000 bushels would add another fourteen weeks’ life to the population ; assuming that the ordinary stock had not been drawn on, the wheat in the country would only then be enough to feed the population for twenty-eight weeks. I do not venture to speak authoritatively on national granaries. The subject has been discussed in the daily press, and the recently published _ Report from the Agricultural Committee on National Wheat Stores brings together all the arguments in favour of this important scheme, together with the difficulties to be faced if it be carried out with necessary com- pleteness. More hopeful, although difficult and costly, would be the alternative of growing most, if not all our own wheat supply here at home in the British Isles. The average yield over the United Kingdom last year was 29-07 bushels per acre, the average for the last eleven years being 29°46. For twelve months we need 240,000,000 bushels of wheat, requiring about 8,250,000 acres of good wheat-growing land, or nearly 13,000 square miles, increasing at the rate of 100 square miles per annum, to render us _ self-supporting as to bread food. This area is about one-fourth the size of England.! A total area of land in the United Kingdom equal to a plot 110 miles square, of quality and climate sufficient to grow wheat to the extent of 29 bushels per acre, does not seem a hopeless demand.” It is doubtful, however, if this amount of land could be kept under wheat, and the necessary expense of high farming faced, except under the imperious pressure of impending starvation, or the stimulus of a national subsidy or permanent high prices. Certainly these 13,000 square miles would not be available under ordinary economic conditions, for much, perhaps all, the land now under barley and oats would not be 1 Appendix A. 2 The total area of the United Kingdom is 120,979 square miles; therefore the required land is about a tenth part of the total. 6 REPORT—1898. suitable for wheat. In any case, owing to our cold, damp climate and capricious weather, the wheat crop is hazardous, and for the present our annual deficit of 180,000,000 bushels must be imported. A permanently higher price for wheat is, I fear, a calamity that ere long must be faced. At enhanced prices, land now under wheat will be better farmed, and therefore will yield better, thus giving increased production without increased area. The burning question of to-day is, What can the United Kingdom do to be reasonably safe from starvation in presence of two successive failures of the world’s wheat harvest, or against a hostile combination of European nations? We eagerly spend millions to protect our coasts and commerce ; and millions more on ships, explosives, guns, and men ; but we omit to take necessary precautions to supply ourselves with the very first and supremely important munition of war—food. To take up the question of food-supply in its scientific aspect, I must not confine myself exclusively to our own national requirements. The problem is not restricted to the British Isles—the bread-eaters of the whole world share the perilous prospect—and I do not think it out of place if on this occasion I ask you to take’with me a wide, general survey of the wheat supply of the whole world. Wheat is the most sustaining food grain of the great Caucasian race, which includes the peoples of Europe, United States, British America, the white inhabitants of South Africa, Australasia, parts of South America, and the white population of the European colonies. Of late years the in- dividual. consumption of wheat has almost universally increased. In Scandinavia it has risen 100 per cent. in twenty-five years ; in Austro- Hungary, 80 per cent. ; in France, 20 per cent. ; while in Belgium it has. increased 50 per cent. Only in Russia and Italy, and possibly Turkey, has the consumption of wheat per head declined. In 1871 the bread-eaters of the world numbered 371,000,000. In 1881 the numbers rose to 416,000,000 ; in 1891, to 472,600,000, and at the present time they number 516,500,000. The augmentation of the world’s bread-eating population ina geometrical ratio is evidenced by the fact that the yearly aggregates grow progressively larger. In the early seventies they rose 4,300,000 per annum, while in the eighties they increased by more than 6,000,000 per annum, necessitating annual additions to the bread supply nearly one-half greater than sufficed twenty-five years ago. How much wheat will be required to supply all these hungry mouths. with bread? At the present moment it is not possible to get accurate estimates of this year’s wheat crops of the worid, but an adequate idea may be gained from the realised crops of some countries and the promise of others. To supply 516,500,000 bread-eaters, if each bread-eating unit is to have his usual ration, will require a total of 2,324,000,000 bushels for seed and food. What are our prospects of obtaining this amount ? According to the best authorities the total supplies from the 1897-98 — —- ADDRESS. 7 harvest are 1,921,000,000 bushels.!. The requirement of the 516,500,000 bread-eaters for seed and food are 2,324,000,000 bushels ; there is thus a deficit of 403,000,000 bushels, which has not been’ urgently apparent owing to a surplus of 300,000,000 bushels carried over from the last harvest. Respecting the prospects of the harvest year just beginning it must be borne in mind that there are no remainders to bring over from last harvest. We start with a deficit of 103,000,000 bushels and have 6,500,000 more mouths to feed. It follows, therefore, that one-sixth of the required bread will be lacking unless larger drafts than now seem possible can be made upon early produce from the next harvest.? The majority of the wheat crops between 1882 and 1896 were in excess of current needs, and thus considerable reserves of wheat were available for supplementing small deficits from the four deficient harvests. But bread- eaters have almost eaten up the reserves of wheat, and the 1897 harvest being under average, the conditions become serious.*? That scarcity and high prices have not prevailed in recent years is due to the fact that since 1889 we have had seven world crops of wheat and six of rye abundantly in excess of the average. These generous crops increased accumula- tions to such an extent as to obscure the fact that the harvests of 1895 and 1896 were each much below current requirements. Practically speak- ing, reserves are now exhausted, and bread-eaters must be fed from current harvests—accumulation under present conditions being almost impossible. This is obvious from the fact that a harvest equal to that of 1894 (the greatest crop on record, both in acre-yield and in the aggregate) would yield less than current needs.* It is clear we are confronted with a colossal problem that must tax the wits of the wisest. When the bread-eaters have exhausted all possible supplies from the 1897-98 harvest, there will be a deficit of 103,000,000 bushels of wheat, with no substitution possible unless Europeans can be induccd to eat Indian corn or rye bread. Up to recent years the growth of wheat has kept pace with demands. As wheat-eaters increased, the acreage under wheat expanded. The world has become so familiarised with the orderly sequence of demand and supply, so accustomed to look upon the vast plains of other wheat-growing countries as inexhaustible granaries, that, in a light-hearted way it is taken for granted that so many million additional acres can be added year after year to the wheat-growing area of the world. We forget that the wheat-growing area is of strictly limited extent, and that a few million acres regularly absorbed, soon mount to a formidable number. The present position being so gloomy, let us consider future prospects. What are the capabilities as regards available area, economic conditions, and acreage yield of the wheat-growing countries from whence we now draw our supply ? 1 Appendix B. * Appendix C. % Appendix D. 4 Apppendix E. io 8) REPORT—1898. For the last thirty years the United States have been the dominant factor in the foreign supply of wheat, exporting no less than 145,000,000 bushels. This shows how the bread-eating world has depended, and still depends, on the United States for the means of subsistence. The entire world’s contributions to the food-bearing area have averaged but 4,000,000 acres yearly since 1869. It is scarcely possible that such an average, under existing conditions, can be doubled for the coming twenty-five years.! Almost yearly, since 1885, additions to the wheat-growing area have diminished, while the requirements of the increasing population of the States have advanced, so that the needed American supplies have been © drawn from the acreage hitherto used for exportation. Practically there remains no uncultivated prairie land in the United States suitable for wheat-growing. The virgin land has been rapidly absorbed, until at present there is no land left for wheat without reducing the area for maize, hay, and other necessary crops.” It is almost certain that within a generation the ever increasing popu- lation of the United States will consume all the wheat grown within its borders, and will be driven to import, and, like ourselves, will scramble for a lion’s share of the wheat crop of the world. This being the outlook, exports of wheat from the United States are only of present interest, and will gradually diminish to a vanishing point. The inquiry may be restricted to such countries as probably will continue to feed bread-eaters who annually derive a considerable part of their wheat from extraneous sources. But if the United States, which grow about one-fifth of the world’s wheat, and contribute one-third of all wheat exportations, are even now dropping out of the race, and likely soon to enter the list of wheat- importing countries, what prospect is there that other wheat-growing countries will be able to fill the gap, and by enlarging their acreage under wheat, replace the supply which the States have so long contributed to the world’s food? The withdrawal of 145 million bushels will cause a serious gap in the food supply of wheat importing countries, and unless this deficit can be met by increased supplies from other countries there will be a dearth for the rest of the world after the British Isles are suffi- ciently supplied. Next to the United States, Russia is the greatest wheat exporter, supplying nearly 95 million bushels.? Although Russia at present exports so lavishly this excess is iade provisional and precarious. The Russian peasant population increases more rapidly than any other in Europe. ‘The yield per acre over European Russia is meagre—not more than 8°6 bushels to the acre— while some authorities consider it as low as 4°6 bushels. The cost of production is low—lower even than on the virgin soils of the United States. The development of the fertile though somewhat overrated 1 Appendix F. ? Appendix G, ? Appendix H. ADDRESS. 9 ‘black earth,’ which extends across the southern portion of the empire and beyond the Ural Mountains into Siberia, progresses rapidly. But, as we have indicated, the consumption of bread in Russia has been reduced to danger point. The peasants starve and fall victims to ‘ hunger typhus,’ whilst the wheat growers export grain that ought to be consumed at home. Considering Siberia as a wheat grower, climate is the first considera- tion. Summers are short—as they are in all regions with continental climates north of the 45th parallel—and the ripening of wheat requires a temperature averaging at least 65° Fahr. for fifty-five to sixty-five days. As all Siberia lies north of the summer isotherm of 65° it follows that such region is ill adapted to wheat culture unless some compensating climatic condition exists. As a fact, the conditions are exceptionally unfavourable in all but very limited districts in the two westernmost governments. The cultivable lands of Western Siberia adapted to grain- ' bearing neither equal in extent nor in potential productive powers those of Iowa, Minnesota, and Nebraska. There are limited tracts of fair pro- ductiveness in Central Siberia and in the valleys of the southern affluents of the Amoor, but these are only just capable of supporting a meagre population. Prince Hilkoff, Russian Minister of Ways and Communications, declared in 1896 that ‘Siberia never had produced, and never would pro- duce, wheat and rye enough to feed the Siberian population.’ And, a year later, Prince Krapotkin backed the statement as substantially correct. Those who attended the meeting of the British Association last year in Canada must have been struck with the extent and marvellous capacity of the fertile plains of Manitoba and the North-West Provinces. Here were to be seen 1,290,000 acres of fine wheat-growing land yielding 18,261,950 bushels, one-fifth of which comes to hungry England. Ex- pectations have been cherished that the Canadian North-West would easily supply the world with wheat, and exaggerated estimates are drawn as to the amount of surplus land on which wheat can be grown.' Thus far performance has lagged behind promise, the wheat-bearing area of all Canada having increased less than 500,000 acres since 1884, while the exports have not increased in greater proportion. As the wheat area of Manitoba and the North-West has increased the wheat area of Ontario and the Eastern provinces has decreased, the added acres being little more than sufficient to meet the growing requirements of population. We have seen calculations showing that Canada contains 500,000,000 acres of profitable wheat land. The impossibility of such an estimate ever being fulfilled will be apparent when it is remembered that the whole area employed in both temperate zones for growing all the staple food crops is not more than 580,000,000 acres, and that in no country has more than 9 per cent. of the area been devoted to wheat culture.? 1 Appendix I, 2 Appendix J. Pp Pp 10 REPORT—1898, The fertility of the North-West Provinces of the Dominion is due to an exceptional and curious circumstance. In winter the ground freezes to a considerable depth. Wheat is sown in the spring, generally April, when the frozen ground has been thawed to a depth of three inches. Under the hot sun of the short summer the grain sprouts with surprising rapidity, partly because the roots are supplied with water from the thawing depths. The summer is too short to thaw the ground thoroughly, and gate-posts or other dead wood extracted in autumn are found still frozen at their lower ends. Australasia as a potential contributor to the world’s supply of wheat affords another fertile field for speculation. Climatic conditions limit the Australian wheat area to a small portion of the southern littoral belt. Professor Shelton considers there are still fifty million acres in Queensland suitable for wheat, but hitherto it has never had more than 150,000 acres under cultivation. Crops in former days were liable to rust, but since the Rust in Wheat conferences and the dissemination of instruction to farmers, rust no longer has any terrors. I am informed by the Queens- land Department of Agriculture that of late years they practically have bred wheat vigorous enough to resist this plague. For the second season in succession, the wheat crop last year was destroyed over large areas in Victoria ; and in South Australia the harvest averaged not more than about 32 bushels per acre after meeting Colonial requirements for food and seed, leaving only 684,000 bushels for export. In most other districts the yield falls to such an extent as to cause Europeans to wonder why the pursuit of wheat-raising is continued. New Zealand has a moist climate resembling that of central and southern England, while South Australia is semi-arid, resembling western Kansas. Only two countries in the world yield as much wheat per acre as New Zealand—these are Denmark and the United Kingdom. Not- withstanding the great yield of wheat, due to an equable climate, New Zealand finds fruit and dairy farming still more profitable. The climatic conditions favourable to wheat are also conducive to luxuriant growths of nutritious grasses. Thus the New Zealander ships his butter more than half-way round the world, and competes successfully with Western Europe. During the last twenty-seven years the Austro-Hungarian population has increased 21:8 per cent., as against an increase of 54°6 per cent. in the acreage of wheat. Notwithstanding this disparity in the rates of increase, exports have practically ceased by reason of an advance of nearly 80 per cent. in unit consumption. There can be little doubt that Austro-Hungary is about to enter the ranks of importing nations, although in Hungary a considerable area of wheat land remains to be brought under culti- vation. ! Roumania is an important wheat-growing country. In 1896 it pro- ? Appendix K. | _ ADDRESS. 1} duced 69,000,000 bushels, and exported 34,000,000 bushels. It has a considerable amount of surplus land which can be used for wheat, although for many years the wheat area is not likely to exceed home requirements. France comes next to the United States as a producer of wheat ; but for our purpose she counts but little, being dependent on supplies from abroad for an average quantity of 14 per cent. of her own production. ‘There is practically no spare land in France that can be put under wheat in sufficient quantity to enable her to do more than provide for increase of population. Germany is a gigantic importer of wheat, her imports rising 700 per cent. in the last twenty-five years, and now averaging 35,000,000 bushels. Other nations of Europe, also importers, do not require detailed mention, as under no conceivable conditions would they be able to do more than supply wheat for the increasing requirements of their local popula- tion, and, instead of replenishing, would probably diminish, the world’s stores. The prospective supply of wheat from Argentina and Uruguay has been } greatly overrated. The agricultural area includes less than 100,000,000 acres of good, bad, and indifferent land, much of which is best adapted for pastoral purposes. ‘There is no prospect of Argentina ever being able to devote more than 30,000,000 acres to wheat ; the present wheat area is about 6,000,000 acres, an area that may be doubled in the next twelve years. Butthe whole arable region is subject to great climatic vicissitudes, and to frosts that ravage the fields south cf the 37th parallel. Years of systematised energy are frustrated in a few days—perhaps hours—by a single cruelty of Nature, such as a plague of locusts, a tropical rain, or a devastating hail storm. It will take years to bring the surplus lands of Argentina into cultivation, and the population is even now insufficient to supply labour at seed time and harvest. During the next twelve years, Uruguay may add a million acres to the world’s wheat fields ; but social, political, and economic conditions _ seriously interfere with agricultural development. At the present time South Africa is an importer of wheat, and the regions suitable to cereals do not exceed a few million acres. Great expectations have been formed as to the fertility of Mashonaland, the: ‘Shiré Highlands, and the Kikuyu plateau, and as to the adaptation of _ these regions to the growth of wheat. But wheat culture fails where the _ banana ripens, and the banana flourishes throughout Central Africa, _ except in limited areas of great elevation. In many parts of Africa insect _ pests render it impossible to store grain, and without grain-stores there _ can be little hope of large exports. North Africa, formerly the granary of Rome, now exports less than 5,000,000 bushels of wheat annually, and these exports are on the decline, owing to increased home demands. With scientific irrigation, Egypt 12 REPORT—1898. could supply three times her present amount of wheat, although no increase is likely unless the cotton fields of the Delta are diverted to grain grow- ing. In Algeria and Tunis nearly all reclaimed lands are devoted to the production of wine, for which a brisk demand exists. Were this land devoted to the growth of wheat, an additional five million bushels might be obtained. The enormous acreage devoted to wheat in India has been declining for some years, and in 1895 over 20,000,000 acres yielded 185,000,000 bushels. Seven-eighths of this harvest is required for native consumption. and only one-eighth on an average is available for export. The annual increase of population is more than 3,000,000, demanding an addition to the food-bearing lands of not less than 1,800,000 acres annually. In recent years the increase has been less than one-fourth of this amount.! In surveying the limitations and vicissitudes of wheat crops, I have endeavoured to keep free from exaggeration, and have avoided insistance on doubtful points. I have done my best to get trustworthy facts and figures, but from the nature of the case it is impossible to attain complete accuracy. Great caution is required in sifting the numerous varying current statements respecting the estimated areas and total produce of wheat throughout the world. The more closely official estimates are examined, the more defective are they found, and comparatively few figures are sufficiently well established to bear the deductions often drawn. In doubtful cases I have applied to the highest authorities in each country, and in the case of conflicting accounts have taken data the least favour- able to sensational or panic-engendering statements. In a few instances of accurate statistics their value is impaired by age ; but for 95 per cent. of my figures I quote good authorities, while for the remaining 5 per cent. L rely on the best commercial estimates derived from the appearance of the growing crops, the acreage under cultivation, and the yield last year. The maximum probable error would make no appreciable difference in my argument. The facts and figures I have set before you are easily interpreted. Since 1871 unit consumption of wheat, including seed, has slowly increased in the United Kingdom to the present amount of 6 bushels per head per annum ; while the rate of consumption for seed and food by the whole world of bread-eaters was 4:15 bushels per unit per annum for the eight years ending 1878, and at the present time is 4-5 bushels. Under present conditions of low acre yield, wheat cannot long retain its dominant posi- tion among the food-stuffs of the civilised world. The details of the impending catastrophe no one can predict, but its general direction is obvious enough. Should all the wheat-growing countries add to their area to the utmost capacity, on the most careful calculation the yield would give us only an addition of some 100,000,000 acres, supplying at the average world-yield of 12:7 bushels to the acre, 1,270,000,000 bushels, ? Appendix L. ADDRESS. ts just enough to supply the increase of population among bread-eaters till the year 1931.! At the present time there exists a deficit in the wheat area of 31,000 square miles—a deficit masked by the fact that the ten world crops of wheat harvested in the ten years ending 1896 were more than 5 per cent. above the average of the previous twenty-six years. When provision shall have been made, if possible, to feed 230,000,000 units likely to be added to the bread-eating populations by 1931—hby the complete occupancy of the arable areas of the temperate zone now parti- ally occupied —where can be grown the additional 330,000,000 bushels of wheat required ten years later by a hungry world? What is to happen _ if the present rate of population be maintained, and if arable areas of sufficient extent cannot be adapted and made contributory to the subsist- ence of so great a host ? Are we to go hungry and to know the trial of scarcity? That is the poignant question. Thirty years is but a day in the life of a nation. Those present who may attend the meeting of the British Association thirty years hence will judge how far my forecasts are justified. Tf bread fails—not only us, but all the bread-eaters of the world — what are we to do? We are born wheat-eaters. Other races, vastly superior to us in numbers, but differing widely in material and intellectual progress, are eaters of Indian corn, rice, millet, and other grains; but none of these grains have the food value, the concentrated health-sus- taining power of wheat, and it is on this account that the accumulated experience of civilised mankind has set wheat apart as the fit and proper food for the development of muscle and brains. It is said that when other wheat-exporting countries realise that the States can no longer keep pace with the demand, these countries will extend their area of cultivation, and struggle to keep up the supply parz pass with the falling off in other quarters. But will this comfortable and cherished doctrine bear the test of examination ? Cheap production of wheat depends on a variety of causes, varying greatly in different countries. Taking the cost of producing a given quantity of wheat in the United Kingdom at 100s., the cost for the same amount in the United States is 67s., in India 66s., and in Russia 54s. We require cheap labour, fertile soil, easy transportation to market, low taxation and rent, and no export or import duties. Labour will rise in price, and fertility diminish as the requisite manurial constituents in the virgin soil become exhausted. Facility of transportation to market will be aided by railways, but these are slow and costly to construct, and it will not pay to carry wheat by rail beyond a certain distance. These considerations show that the price of wheat tends to increase. On the other hand, the artificial impediments of taxation and customs duties tend to diminish as demand increases and prices rise. } Appeniix M,. 4 REPORT— 1898. T have said that starvation may be averted through the laboratory. Before we are in the grip of actual dearth the Chemist will step in and postpone the day of famine to so distant a period that we, and our sons and grandsons, may legitimately live without undue solicitude for the future. It is now recognised that all crops require what is called a ‘dominant’ manure.. Some need nitrogen, some potash, others phosphates. Wheat pre-eminently demands nitrogen, fixed in the form of ammonia or nitric acid. All other necessary constituents exist in the soil; but nitrogen is mainly of atmospheric origin, and is rendered ‘fixed’ by a slow and precarious process which requires a combination of rare meteorological and geographical conditions to enable it to advance at a sufficiently rapid rate to become of commercial importance. There are several sources of available nitrogen, The distillation of coal in the process of gas-making yields a certain amount of its nitrogen in the form of ammonia; and this product, as sulphate of ammonia, is a substance of considerable commercial value to gas companies. But the quantity produced is comparatively small; all Europe does not yield more than 400,000 annual tons, and, in view of the unlimited nitrogen required to substantially increase the world’s wheat crop, this slight amount of coal ammonia is not of much significance. For a long time guano has been one of the most important sources of nitrogenous manures, but guano deposits are so near exhaustion that they may be dismissed from consideration. Much has been said of late years, and many hopes raised by the discovery of Hellriegel and Wilfarth, that leguminous plants bear on their roots nodosities abounding in bacteria endowed with the property of fixing atmospheric nitrogen; and it is proposed that the necessary amount of nitrogen demanded by grain crops should be supplied to the soil by cropping it with clover and ploughing in the plant when its nitrogen assimilisation is complete. But it is questionable whether such a mode of procedure will lead to the lucrative stimulation of crops. It must be admitted that practice has long been ahead of science, and for ages farmers have valued and cultivated leguminous crops. The four- course rotation is turnips, barley, clover, wheat—a sequence popular more than two thousand years ago. On the Continent, in certain localities, there has been some extension of microbe cultivation; at home we have not reached even the experimental stage. Our present knowledge leads to the conclusion that the much more frequent growth of clover on the same land, even with successful microbe-seeding and proper mineral supplies, would be attended with uncertainty and difficulties. The land soon becomes what is called ‘ clover sick ’ and turns barren. There is still another and invaluable source of fixed nitrogen. I mean the treasure locked up in the sewage and drainage of our towns. Individually the amount so lost is trifling, but multiply the loss by the ~———— ————————————<— << = CUCU! ADDRESS. he number of inhabitants, and we have the startling fact that, in the United Kingdom, we are content to hurry down our drains and water courses, into the sea, fixed nitrogen to the value of no less than 16,000,000/. per annum. ‘This unspeakable waste continues, and no effective and universal method is yet contrived of converting sewage into corn. Of this barbaric waste of manurial constituents Liebig, nearly half a century ago, wrote in these prophetic words : ‘ Nothing will more certainly consummate the ruin of England than a scarcity of fertilisers—it means a scarcity of food. It is impossible that such a sinful violation of the divine laws of Nature should for ever remain unpunished ; and the time will probably come for England sooner than for any other country, when, with all her wealth in gold, iron, and coal, she will be unable to buy one-thousandth part of the food which she has, during hundreds of years, thrown recklessly away.’ The more widely this wasteful system is extended, recklessly returning to the sea what we have taken from the land, the more surely and quickly will the finite stocks of nitrogen locked up in the soils of the world become exhausted. Let us remember that the plant creates nothing ; there is nothing in bread which is not absorbed from the soil, and unless the abstracted nitrogen is returned to the soil, its fertility must ultimately be exhausted. When we apply to the land nitrate of soda, sulphate of am- monia, or guano, we are drawing on the earth’s capital, and our drafts will not perpetually be honoured. Already we see that a virgin soil cropped for several years loses its productive powers, and without artificial aid becomes infertile. Thus the strain to meet demands is increasingly great. Witness the yield of forty bushels of wheat per acre under favourable conditions, dwindling through exhaustion of soil to less than seven bushels of poor grain, and the urgency of husbanding the limited store of fixed nitrogen becomes apparent. The store of nitrogen in the atmosphere is practically unlimited, but it is fixed and rendered assimilable by plants only by cosmic processes of extreme slowness. The nitrogen which with a light heart we liberate in a battleship broadside, has taken millions of minute organisms patiently working for centuries to win from the atmosphere.! The only available compound containing sufficient fixed nitrogen to be used on a world-wide scale as a nitrogenous manure is nitrate of soda, or Chili saltpetre. This substance occurs native over a narrow band of the _ plain of Tamarugal, in the northern provinces of Chili between the Andes and the coast hills. In this rainless district for countless ages the con- tinuous fixation of atmospheric nitrogen by the soil, its conversion into nitrate by the slow transformation of billions of nitrifying organisms, its combination with soda, and the crystallisation of the nitrate have been steadily proceeding, until the nitrate fields of Chili have become of vast commercial importance, and promise to be of inestimably greater value in 1 Appendix N. 16 REPORT—1898. the future. The growing exports of nitrate from Chili at present amount to about 1,200,000 tons. The present acreage devoted to the world’s growth of wheat is about 163,000,000 acres. At the average of 12:7 bushels per acre this gives 2,070,000,000 bushels. But thirty years hence the demand will be 3,260,000,000 bushels, and there will be difficulty in finding the necessary acreage on which to grow the additional amount required. By increasing the present yield per acre from 12-7 to 20 bushels we should with our present acreage secure a crop of the requisite amount. Now from 12-7 to 20 bushels per acre is a moderate increase of productiveness, and there is no doubt that a dressing with nitrate of soda will give this increase and more. The action of nitrate of soda in improving the yield of wheat has been studied practically by Sir John Lawes and Sir Henry Gilbert on their experimental field at Rothamstead. This field was sown with wheat for thirteen consecutive years without manure, and yielded an average of 11-9 bushels to the acre. For the next thirteen years it was sown with wheat, and dressed with 5 ewt. of nitrate of soda per acre, other mineral consti- tuents also being present. The average yield for these years was 36:4 bushels per acre—an increase of 24:5 bushels. In other words, 22°86 lbs. of nitrate of soda produce an increase of one bushel of wheat. At this rate, to increase the world’s crop of wheat by 7-3 bushels, about 1} ewt. of nitrate of soda must annually be applied to each acre. The amount required to raise the world’s crop on 163,000,000 acres from the present supply of 2,070,000,000 bushels to the required 5,260,000,000 bushels will be 12 million tons distributed in varying amounts over the wheat-growing countries of the world. The countries which produce more than the average of 12-7 bushels will require less, and those below the average will require more ; but, broadly speaking, about 12,000,000 tons annually of nitrate of soda will be required, in addition to the 1} million tons already absorbed by the world. It is difficult to get trustworthy estimates of the amount of nitrate surviving in the nitre beds. Common rumour declares the supply to be inexhaustible, but cautious local authorities state that at the present rate of export, of over one million tons per annum, the raw material ‘ caliche,’ containing from 25 to 50 per cent. nitrate, will be exhausted in from twenty to thirty years. Dr. Newton, who has spent years on the nitrate fields, tells me there is a lower class material, containing a small proportion of nitrate, which cannot at present be used, but which may ultimately be manufactured at a profit. Apart from a few of the more scientific manufacturers, no one is sanguine enough to think this debatable material will ever be worth working. If we assume a liberal estimate for nitrate obtained from the lower grade deposit, and say that it will equal in quantity that from the richer quality, the supply may last, possibly, fifty years, at the rate of a million tonsa year; but at the rate required to augment the world’s LL 2—<$- ADDRESS. 17; supply of wheat to the point demanded thirty years hence it will not last more than four years. I have passed in review all the wheat-growing countries of the world, with the exception of those whose united supplies are so small as to make little appreciable difference to the argument. The situation may be summed up briefly thus :—The world’s demand for wheat—the leading bread-stuff—increases in a crescendo ratio year by year. Gradually all the wheat-bearing land on the globe is appropriated to wheat-growing, until we are within measurable distance of using the last available acre. We must then rely on nitrogenous manures to increase the fertility of the land under wheat, so as to raise the yield from the world’s low average— 12-7 bushels per acre—to a higher average. To do this efficiently and feed the bread-eaters for a few years will exhaust all the available store of nitrate of soda. For years past we have been spending fixed nitrogen at a culpably extravagant rate, heedless of the fact that it is fixed with extreme slowness and difficulty, while its liberation in the free state takes place always with rapidity and sometimes with explosive violence. Some years ago Mr. Stanley Jevons uttered a note of warning as to the near exhaustion of our British coalfields. But the exhaustion of the world’s stock of fixed nitrogen is a matter of far greater importance. It means not only a catastrophe little short of starvation for the wheat- eaters, but indirectly, scarcity for those who exist on inferior grains, together with a lower standard of living for meat-eaters, scarcity of mutton and beef, and even the extinction of gunpowder ! There is a gleam of light amid this darkness of despondency. In its free state nitrogen is one of the most abundant and pervading bodies on the face of the earth. Every square yard of the earth’s surface has nitrogen gas pressing down on it to the extent of about seven tons—but this is in the free state, and wheat demands it fived. ‘To convey this idea in an object-lesson, I may tell you that, previous to its destruction by fire, Colston Hall, measuring 146 feet by 80 feet by 70 feet, contained 27 tons weight of nitrogen in its atmosphere ; it also contained one-third of a ton of argon. In the free gaseous state this nitrogen is worthless ; combined in the form of nitrate of soda it would be worth about 2,000/. For years past attempts have been made to effect the fixation of atmospheric nitrogen, and some of the processes have met with sufficient partial success to warrant experimentalists in pushing their trials still further ; but I think I am right in saying that no process has yet been brought to the notice of scientific or commercial men which can be con- sidered successful either as regards cost or yield of product. It is possible, by several methods, to fix a certain amount of atmospheric nitrogen ; but to the best of my knowledge no process has hitherto converted more than a small amount, and this at a cost largely in excess of the present market value of fixed nitrogen. The fixation of atmospheric nitrogen therefore is one of the great 1898. c 18 REPORT-—1898. discoveries awaiting the ingenuity of chemists. It is certainly deeply important in its practical bearings on the future welfare and happiness of the civilised races of mankind. This unfulfilled problem, which so far has eluded the strenuous attempts of those who have tried to wrest the secret from nature, differs materially from other chemical discoveries which are in the air, so to speak, but are not yet matured. The fixation of nitrogen is vital to the progress of civilised humanity. Other dis- coveries minister to our increased intellectual comfort, luxury, or con- venience ; they serve to make life easier, to hasten the acquisition of wealth, or to save time, health, or worry. The fixation of nitrogen is a question of the not far distant future. Unless we can class it among certainties to come the great Caucasian race will cease to be foremost in the world, and will be squeezed out of existence by races to whom wheaten bread is not the staff of life. Let me see if it is not possible even now to solve the momentous problem. As far back as 1892 I exhibited, at one of the Soirées of the Royal Society, an experiment on ‘The Flame of Burning Nitrogen.’ I showed that nitrogen is a combustible gas, and the reason why when once ignited the flame does not spread through the atmosphere and deluge the world in a sea of nitric acid is that its igniting point is higher than the temperature of its flame—not, therefore, hot enough to set fire to the adjacent mixture. But by passing a strong induction current between terminals the air takes fire and continues to burn with a powerful flame, producing nitrous and nitric acids. This inconsiderable experiment may not unlikely lead to the development of a mighty industry destined to solve the great food problem. With the object of burning out nitrogen from air so as to leave argon behind, Lord Rayleigh fitted up apparatus for performing the operation on a larger scale, and succeeded in effecting the union of 29:4 grammes of mixed nitrogen and oxygen at an expendi- ture of one horse-power. Following these figures it would require one Board of Trade unit to form 74 grammes of nitrate of soda, and therefore 14,000 units to form one ton. To generate electricity in the ordinary way with steam engines and dynamos, it is now possible with a steady load night and day, and engines working at maximum efficiency, to pro- duce current at a cost of one-third of a penny per Board of Trade unit. At this rate one ton of nitrate of soda would cost 26/7. But electricity from coal and steam engines is too costly for large industrial purposes ; at Niagara, where water power is used, electricity can be sold at a profit for one-seventeenth of a penny per Board of Trade unit. At this rate nitrate of soda would cost not more than 5/. per ton. But the limit of cost is not yet reached, and it must be remembered that the initial data are derived from small scale experiments, in which the object was not economy, but rather to demonstrate the practicability of the combustion method, and to utilise it for isolating argon. Even now electric nitrate at 5/, a ton compares favourably with Chili nitrate at 7/. 10s. a ton ; and at 2 : : 7 : | ADDRESS, 19 all experience shows that when the road has been pointed out by a small laboratory experiment, the industrial operations that may follow are always conducted at a cost considerably lower than could be anticipated from the laboratory figures. Before we decide that electric nitrate is a commercial possibility, a final question must be mooted. We are dealing with wholesale figures and must take care that we are not simply shifting difficulties a little further back without really diminishing them. We start with a shortage of wheat, and the natural remedy is to put more land under cultivation. As the land cannot be stretched, and there is so much of it and no more, the object is to render the available area more productive by a dressing with nitrate of soda. But nitrate of soda is limited in quantity, and will soon be exhausted. Human ingenuity can contend even with these apparently hopeless difficulties. Nitrate can be produced artificially by the combustion of the atmosphere. Here we come to finality in one direction ; our stores are inexhaustible. But how about electricity ? Can we generate enough energy to produce 12,000,000 tons of nitrate of soda annually? A preliminary calculation shows that there need be no fear on that score ; Niagara alone is capable of supplying the required electric senergy without much lessening its mighty flow. The future can take care of itself. Theartificial production of nitrate is clearly within view, and by its aid the land devoted to wheat can be brought up to the 30 bushels per acre standard. In days to come, when _ the demand may again overtake supply, we may safely leave our suc- cessors to grapple 30 the stupendous food problem. And, in the next generation, instead of trusting mainly to food- stuffs which flourish in temperate climates, we pedbatiy shall trust more and more to the exuberant food-stuffs of the tropics, where, instead of one yearly sober harvest, jeopardised by any shrinkage of the scanty days of summer weather, or of the few steady inches of rainfall, Nature annually supplies heat and water enough to ripen two or three successive crops of - food-stuffs in extraordinary abundance. To mention one plant alone, Humboldt—from what precise statistics I know not—computed that, acre for acre, the food-productiveness of the banana is 133 times that of wheat—the unripe banana, before its starch is converted into sugar, is said to make excellent bread. Considerations like these must in the end determine the range and _ avenues of commerce, perhaps the fate of continents. We must develop and guide Nature’s latent energies, we must utilise her inmost workshops, ‘we must call into commercial existence Central Africa and Brazil to redress the balance of Odessa and Chicago. Having kept you for the last half-hour rigorously chained to earth, disclosing dreary possibilities, it will be a relief to soar to the heights of pure science and to discuss a point or two touching its latest pultevenietts c2 20 REPORT—1898. and aspirations. The low temperature researches which bring such renown to Professor Dewar and to his laboratory in the Royal Institution have been crowned during the present year by the conquest of one of Nature’s most defiant strongholds. On the 10th of last May Professor Dewar wrote to me these simple but victorious words : ‘This evening I have succeeded in liquefying both hydrogen and helium. The second stage of low temperature work has begun.’ Statice hydrogen boils at a temperature of 238° C. at ordinary pressure, and at 250° C. in a vacuum, thus enabling us to get within 23° C. of absolute zero. The density of liquid hydrogen is only one-fourteenth that of water, yet in spite of such a low density it collects well, drops easily, and has a well-defined meniscus. With proper isolation it will be as easy to manipulate liquid hydrogen as liquid air. The investigation of the properties of bodies brought near the absolute zero of temperature is certain to give results of extraordinary importance. Already platinum resistance thermometers are becoming useless, as the temperature of boiling hydrogen is but a few degrees from the point where the resistance of platinum would be practically nothing, or the conductivity infinite. Several years ago I pondered on the constitution of matter in what I. ventured to call the fourth state. I endeavoured to probe the tormenting mystery of the atom. What is the atom? Is a single atom in space solid, liquid, or gaseous. Each of these states involves ideas which can only pertain to vast collections of atoms. Whether, like Newton, we try to visualise an atom as a hard, spherical body, or, with Boscovitch and Faraday, to regard it as a centre of force, or accept the vortex atom theory of Lord Kelvin, an isolated atom is an unknown entity difficult to conceive, The properties of matter—solid, liquid, gaseous—are due to molecules in a state of motion. Therefore, matter as we know it involves essentially a mode of motion ; and the atom itself—intangible, invisible, and incon- ceivable—is its material basis, and may, indeed, be styled the only true matter. The space involved in the motions of atoms has no more preten- sion to be called matter than the sphere of influence of a body of riflemen —the sphere filled with flying leaden missiles—has to be called lead. Since what we call matter essentially involves a mode of mction, and since at the temperature of absolute zero all atomic motions would stop, it follows that matter as we know it would at that paralysing temperature probably entirely change its properties. Although a discussion of the ultimate absolute properties of matter is purely speculative, it can hardly be barren, considering that in our laboratories we are now within moderate distance of the absolute zero of temperature. I have dwelt on the value and importance of nitrogen, but I must not omit to bring to your notice those little known and curiously related elements which during the past twelve months have been discovered and partly described by Professor Ramsay and Dr. Travers. For many years my own work has been among what I may call the waste heaps of the ADDRESS. 2] | mineral elements. Professor Ramsay is dealing with vagrant atoms of , an astral nature. During the course of the present year he has announced _ the existence of no fewer than three new gases—krypton, neon, and , metargon. Whether these gases, chiefly known by their spectra, are true unalterable elements, or whether they are compounded of other known or unknown bodies, has yet to be proved. Fellow workers freely pay tribute to the painstaking zeal with which Professor Ramsay | has conducted a difficult research, and to the philosophic subtlety brought to bear on his investigations. But, like most discoverers, he has not escaped the flail of severe criticism. There is still another claimant for celestial honours. Professor Nasini tells us he has discovered, in some volcanic gases at Pozzuoli, that hypo- thetical element Coronium, supposed to cause the bright line 5316-9 in the spectrum of the sun’s corona. Analogy points to its being lighter and more diffusible than hydrogen, and a study of its properties cannot fail to yield striking results. Still awaiting discovery by the fortunate spectro- seopist are the unknown celestial elements Aurorium, with a characteristic line at 5570°7—and Nebulumn, having two bright lines at 5007:05 and 4959-02. J The fundamental discovery by Hertz, of the electro-magnetic waves predicted more than thirty years ago by Clerk Maxwell, seems likely to develop in the direction of a practical application which excites keen interest—I mean the application to electric signalling across moderate distances without connecting wires. The feasibility of this method of _ signalling has been demonstrated by several experimenters at more than one meeting of the British Association, though most elaborately and with many optical refinements by Oliver Lodge at the Oxford meeting in 1894. But not until Signor Marconi induced the British Post-Office and Foreign Governments to try large scale experiments did wireless signalling ‘become generally and popularly known or practically developed as a “special kind of telegraphy. Its feasibility depends on the discovery of a singularly sensitive detector for Hertz waves—a detector whose sensitive- ‘ness in some cases seems almost to compare with that of the eye itself. ‘The fact noticed by Oliver Lodge in 1889, that an infinitesimal metallic gap subjected to an electric jerk became conducting, so as to complete an electric circuit, was rediscovered soon afterwards in a more tangible and ‘definite form and applied to the detection of Hertz waves by M. E. Branly. Oliver Lodge then continued the work, and produced the vacuum filing-tube coherers with automatic tapper-back, which are of acknowledged practical service. It is this varying continuity of contact ‘under the influence of extremely feeble electric stimulus alternating with - mechanical tremor, which, in combination with the mode of producing the waves revealed by Hertz, constitutes the essential and fundamental - feature of ‘wireless telegraphy.’ There is a curious and widely spread misapprehension about coherers, to the effect that to make a coherer work 22, REPORT—1898. the wave must fall upon it. Oliver Lodge has disproved this fallacy. Let the wave fall on a suitable receiver, such as a metallic wire or, better still, on an arrangement of metal wings resembling a Hertz sender, and the waves set up oscillating currents which may be led by wires (enclosed in metal pipes) to the coherer, The coherer acts apparently by a species of end-impact of the oscillatory current, and does not need to be attacked in the flank by the waves themselves. This interesting method of signalling—already developing in Marconi’s hands into a_ successful practical system which inevitably will be largely used in lighthouse and marine work—presents more analogy to optical signals by flash-light than to what is usually understood as electric’telegraphy ; notwithstanding the fact that an ordinary Morse instrument at one end responds to the move- ments of a key at the other, or, as arranged by Alexander Muirhead, a siphon recorder responds to an automatic transmitter at about the rate of slow cable telegraphy. But although no apparent optical apparatus is employed, it remains true that the impulse travels from sender to receiver by essentially the same process as that which enables a flash of magnesium powder to excite a distant eye. The phenomenon discovered by Zeeman, that a source of radiation is affected by a strong magnetic field in such a way that light of one re- frangibility becomes divided usually into three components, two of which are displaced by diffraction analysis on either side of the mean position and are oppositely polarised to the third or residual constituent, has been examined by many observers in all countries. The phenomenon has been subjected to photography with conspicuously successful results by Professor T. Preston in Dublin and by Professor Michelson and Dr. Ames and others in America. It appears that the different lines in the spectrum are differently affected, some of them being tripled with different grades of relative intensity, some doubled, some quadrupled, some sextupled, and some left unchanged. Even the two components of the D lines are not similarly influenced. Moreover, whereas the polarisation is usually such as to indicate that motions of a negative ion or electron constitute the source of light, a few lines are stated by the observers at Baltimore, who used what they call the ‘small’ grating of 5 inches width ruled with 65,000 lines, to be polarised in the reverse way. Further prosecution of these researches must lead to deeper insight into molecular processes and the mode in which they affect the ether ; indeed already valuable theoretic views have been promulgated by H. A. Lorenz, J. Larmor, and G. F. Fitzgerald, on the lines of the radiation theory of Dr. Johnstone Stoney ; and the connection of the new phenomena with the old magnetic rotation of Faraday is under discussion. It is interesting to note that Faraday and a number of more recent experimenters were led by theoretical considerations to look for some such effect ; and though the inadequate means at their disposal did ! ADDRESS. 23 not lead to success, nevertheless a first dim glimpse of the phenomenon was obtained by M. Fievez, of the Royal Observatory at Brussels, in 1885. It would be improper to pass without at least brief mention the remarkable series of theoretic papers by Dr. J. Larmor, published by the Royal Society, on the relationship between ether and matter. By the time these researches become generally intelligible they may be found to constitute a considerable step towards the further mathematical analysis and interpretation of the physical universe on the lines initiated by Newton. : In the mechanical construction of Réntgen ray tubes I can record a few advances : the most successful being the adoption of Professor Silvanus P. Thompson’s suggestion of using for the anti-cathode a metal of high atomic weight. Osmium and iridium have been used with advantage, and osmium anti-cathode tubes are now a regular article of manufacture. As long ago as June 1896, X-ray tubes with metallic uranium anti- cathodes were made in my own laboratory, and were found to work better than those with platinum. The ditliculty of procuring metallic uranium prevented these experiments from being continued. Thorium anti- cathodes have also been tried. Rontgen has drawn fresh attention to a fact very early observed by English experimenters—that of the non-homogeneity of the rays and the dependence of their penetrating power on the degree of vacuum ; rays generated in high vacua have more penetrative power than when the vacuum is less high. These facts are familiar to all who have exhausted focus tubes on their own pumps. Réntgen suggests a convenient phrase- ology ; he calls a low vacuum tube, which does not emit the highly penetrating rays, a ‘soft’ tube, and a tube in which the exhaustion has been pushed to an extreme degree, in which highly penetrating rays pre- dominate, a ‘hard’ tube. Using a ‘hard’ tube he took a photograph of a double-barrelled rifle, and showed not only the leaden bullets within the steel barrels but even the wads and the charges. Benoit has re-examined the alleged relation between density and opacity to the rays, and finds certain discrepancies. Thus, the opacity of equal thicknesses of palladium and platinum are nearly equal whilst their densities and atomic weights are very different, those of palladium being about half those of platinum. At the last meeting of the British Association visitors saw—at the McGill University—Professors Cox and Callendar’s apparatus for measur- ing the velocity of Réntgen rays. They found it to be certainly greater than 200 kilometres per second: Majorana has made an independent determination, and finds the velocity to be 600 kilometres per second with an inferior limit certainly of not less than 150 kilometres per second. It may be remembered that J. J. Thomson has found for cathode rays a velocity of more than 10,000 kilometres per second, and it is extremely unlikely that the velocity of Réntgen rays will prove to be less. 24 REPORT— 1898. Trowbridge has verified the fact, previously announced by Professor 8. P. Thompson, that fluor-spar, which by prolonged heating has lost its power of luminescing when re-heated, regains the power of thermo-lumi- nescence when exposed to Réntgen rays. He finds that this restoration is also effected by exposure to the electric glow discharge, but not by expos- sure to ultra-violet light. The difference is suggestive. As for the action of Réntgen rays on bacteria, often asserted and often denied, the latest statement by Dr. H. Rieder, of Munich, is to the effect that bacteria are killed by the discharge from ‘hard’ tubes. Whether the observation will lead to resuits of pathologic importance remains to be seen. The circumstance that the normal retina of the eye is slightly sensitive to the rays is confirmed by Dorn and by Réntgen himself. The essential wave-nature of the Réntgen rays appears to be con- firmed by the fact ascertained by several of our great mathematical physicists, that light of excessively short wave-length would be but slightly absorbed by ordinary material media, and would not in the ordinary sense be refracted at all. In fact a theoretic basis for a compre- hension of the Réntgen rays had been propounded before the rays were discovered. At the Liverpool meeting of the British Association, several speakers, headed by Sir George Stokes, expressed their conviction that the disturbed electric field caused by the sudden stoppage of the motion of an electrically charged atom yielded the true explanation of the phenomena extraneous to the Crookes high vacuum tubes—phenomena so excellently elaborated by Lenard and by Réntgen. More recently, Sir George Stokes has re-stated his ‘pulse’ theory, and fortified it with arguments which have an important bearing on the whole theory of the refraction of light. He still holds to their essentially transverse nature, in spite of the absence of polarisation, an absence once more confirmed by the careful experi- ments of Dr. L. Graetz. The details of this theory are in process of elaboration by Professor J. J. Thomson. Meantime, while the general opinion of physicists seems to be settling towards a wave or ether theory for the Réntgen rays, an opposite drift is apparent with respect to the physical nature of the cathode rays ; it be- comes more and more clear that cathode rays consist of electrified atoms or ions in rapid progressive motion. My idea of a fourth state of matter, propounded in 1881,! and at first opposed at home and abroad, is now be- coming accepted. It is supported by Professor J. J. Thomson :? Dr. Larmor’s theory* likewise involves the idea of an ionic substratum of matter ; the view is also confirmed by Zeeman’s phenomenon. In Ger- many—where the term cathode ray was invented almost as a protest against the theory of molecular streams propounded by me at the Sheffield meeting of the British Association in 1879—additional proofs have been 1 Phil. Trans., Part 2, 1881, pp. 433-4. : * Phil. Mag., October 1897, p. 312. % Thid., December 1897, p. 506. ADDRESS. 25 produced in favour of the doctrine that the essential fact in the pheno- menon is electrified Radiant Matter. The speed of these molecular streams has been approximately measured, chiefly by aid of my own discovery nearly twenty years ago, that their path is curved in a magnetic field, and that they produce phosphorescence where they impinge on an obstacle. The two unknown quantities, the charge and the speed of each atom, are measurable from the amount of curvature and by means of one other independent experiment. It cannot be said that a complete and conclusive theory of these rays has yet been formulated. It is generally accepted that collisions among particles, especially the violent collisions due to their impact on a massive target placed in their path, give rise to the interesting kind of extremely high frequency radiation discovered by Roéntgen. It has, indeed, for some time been known that whereas a charged body in motion constitutes an electric current, the sudden stoppage, or any violent acceleration of such a body, must cause an alternating electric disturbance, which, though so rapidly decaying in intensity as to be practically ‘dead beat,’ yet must give rise to an ethereal wave or pulse travelling with the speed of light, but of a length comparable to the size of the body whose sudden change of motion caused the disturbance. The emission of a high-pitched musical sound from the jolting of a dustman’s cart (with a spring bell hung on it) has been suggested as an illustration of the way in which the molecules of any solid not at absolute zero may possibly emit such rays. Tf the target on to which the electrically-charged atoms impinge is so constituted that some of its minute parts can thereby be set into rhyth- mical vibration, the energy thus absorbed reappears in the form of light, and the body is said to phosphoresce. The efficient action of the phos- phorescent target appears to depend as much on its physical and mole- cular as on its chemical constitution. The best known phosphori belong to certain weli-defined classes, such as the sulphides of the alkaline-earthy metals, and some of the so-called rare earths; but the phosphorescent properties of each of these groups are profoundly modified by an admix- ture of foreign bodies—witness the effect on the lines in the phosphor- escent spectrum of yttrium and samarium produced by traces of calcium or lead. The persistence of the samarium spectrum in presence of over- whelming quantities of other metals, is almost unexampled in spectro- _ scopy: thus one part of samaria can easily be seen when mixed with three million parts of lime. Without stating it as a general rule, it seems as if with a non- _ phosphorescing target the energy of molecular impact reappears as pulses so abrupt and irregular that, when resolved, they furnish a copious supply of waves of excessively short wave-length, in fact, the now well-known Réntgen rays. The phosphorescence so excited may last only a small fraction of a second, as with the constituents of yttria, where the duration of the different lines varies between the 0:003 and the 0:0009 second; 26 REPORT—1898. or it may linger for hours, as in the case of some of the yttria earths, and especially with the earthy sulphides, where the glow lasts bright enough to be commercially useful. Excessively phosphorescent bodies can be excited by light waves, but most of them require the stimulus of electrical excitement. It now appears that some bodies, even without special stimulation, are capable of giving out rays closely allied, if not in some cases identical, with those of Professor Réntgen. Uranium and thorium compounds are of this character, and it would almost seem from the important researches of Dr. Russell, that this ray-emitting power may be a general property of matter, for he has shown that nearly every substance is capable of affecting the photographic plate if exposed in darkness for sufficient time. No other source for Réntgen rays but the Crookes tube has yet been discovered, but rays of kindred sorts are recognised. The Becquerel rays, emitted by uranium and its compounds, have now found their companions in rays—discovered almost simultaneously by Curie and Schmidt—emitted by thorium and its compounds. The thorium rays affect photographic plates through screens of paper or aluminium, and are absorbed by metals and other dense bodies. They ionise the air, making it an electrical conductor; and they can be refracted and probably reflected, at least diffusively. Unlike uranium rays, they are not polarised by transmission through tourmaline, therefore resembling in this respect the Réntgen rays. § Quite recently M. and Mme. Curie have announced a discovery which, if confirmed, cannot fail to assist the investigation of this obscure branch of physics. They have brought to notice a new constituent of the uranium mineral pitchblende, which in a 400-fold degree possesses uranium’s mysterious power of emitting a form of energy capable of im- pressing a photographic plate and of discharging electricity by rendering air a conductor. It also appears that the radiant activity of the new body, to which the discoverers have given the name of Polonium, needs neither the excitation of light nor the stimulus of electricity ; like uranium, it draws its energy from some constantly regenerating and hitherto unsuspected store, exhaustless in amount. It has long been to me a haunting problem how to reconcile this apparently boundless outpour of energy with accepted canons. But as Dr. Johnstone Stoney reminds me, the resources of molecular movements are far from exhausted. There are many stores of energy in nature that may be drawn on by properly constituted bodies without very obvious cause. Some time since I drew attention to the enormous amount of locked up energy in the ether ; nearer our experimental grasp are the motions of the atoms and molecules, and it is not difficult mentally so to modify Maxwell’s demons as to reduce them to the level of an inflexible law and thus bring them within the ken of a philosopher in search of a new tool. It is possible to conceive a target capable of mechanically ADDRESS. 27 sifting from the molecules of the surrounding air the quick from the slow movers. This sifting of the swift moving molecules is effected in liquids whenever they evaporate, and in the case of the constituents of the _ atmosphere, wherever it contains constituents light enough to drift away molecule by molecule. In my mind’s eye I see such a target as a piece of metal cooler than the surrounding air acquiring the energy that gradually raises its temperature from the outstanding effect of all its encounters with the molecules of the air about it; I see another target of such a structure that it throws off the slow moving molecules with little exchange of energy, but is so influenced by the quick moving missiles that it appropriates to itself some of their energy. Let uranium or polonium, bodies of densest atoms, have a structure that enables them to throw off the slow moving molecules of the atmosphere, while the quick moving molecules, smashing on to the surface, have their energy reduced and that of the target correspondingly increased. The energy thus gained seems to be employed partly in dissociating some of the molecules of the gas (or in inducing some other condition which has the effect of rendering the neighbouring air in some degree a conductor of electricity) and partly in originating an undulation through the ether, which, as it takes its rise in _ phenomena so disconnected as the impacts of the molecules of the air, must furnish a large contingent of light waves of short wave-length. The shortness in the case of these Becquerel rays appears to approach without attaining the extreme shortness of ordinary Réntgen rays. The reduction of the speed of the quick moving molecules would cool the layer of air_to which they belong ; but this cooling would rapidly be compensated by radiation and conduction from the surrounding atmosphere ; under ordi- nary circumstances the difference of temperature would scarcely be per- ceptible, and the uranium would thus appear to perpetually emit rays of energy with no apparent means of restoration. The total energy of both the translational and internal motions of the molecules locked up in quiescent air at ordinary pressure and temperature is about 140,000 foot-pounds in each cubic yard of air. Accordingly the quiet air within a room 12 feet high, 18 feet wide, and 22 feet long contains energy enough to propel a one-horse engine for more than twelve hours. The store drawn upon naturally by uranium and other heavy atoms only awaits the touch of the magic wand of Science to enable the Twentieth Century to cast into the shade the marvels of the Nineteenth. Whilst placing before you the labours and achievements of my com- rades in Science I seize this chance of telling you of engrossing work of my own on the fractionation of yttria to which for the last eighteen years I have given ceaseless attention. In 1883, under the title of ‘Radiant Matter Spectroscopy,’ I described a new series of spectra produced by passing the phosphorescent glow of yttria, under molecular bombardment im vacuo, through a train of prisms. The visible spectra in time gave up 28 REPORT—1898. their secrets, and were duly embalmed in the Philosophical Transactions. At the Birmingham meeting of the British Association in 1886 I brought the subject before the Chemical Section, of which I had the honour to be President. The results led to many speculations on the probable origin of all the elementary bodies—speculations that for the moment I must waive in favour of experimental facts. There still remained for spectroscopic examination a long tempting stretch of unknown ultra-violet light, of which the exploration gave me no rest. But I will not now enter into details of the quest of unknown lines. Large quartz prisms, lenses, and condensers, specially sensitised photo- graphic films capable of dealing with the necessary small amount of radia- tion given by feebly phosphorescing substances,! and above all tireless patience in collating and interpreting results, have all played their part. Although the research is incomplete I am able to announce that among the groups of rare earths giving phosphorescent spectra in the visible region there are others giving well defined groups of bands which can only -be recorded photographically. I have detected and mapped no less than six such groups extending to \ 3060. Without enlarging on difficulties, I will give a brief outline of the in- vestigation. Starting with a large quantity of a group of the rare earths in a state of considerable purity, a particular method of fractionation is applied, splitting the earths into a series of fractions differing but slightly from each other. Each of these fractions, phosphorescing in vacuo, is arranged in the spectrograph, and a record of its spectrum photographed upon a specially prepared sensitive film. In this way, with different groups of rare earths, the several invisible bands were recorded—some moderately strong, others exceedingly faint. Selecting a portion giving a definite set of bands, new methods of frac- tionation were applied, constantly photographing and measuring the spectrum of each fraction. Sometimes many weeks of hard experiment failed to produce any separation, and then a new method of splitting up was devised and applied. By unremitting work—the solvent of most difficulties—eventually it was possible to split up the series of bands into various groups. Then, taking a group which seemed to offer possibilities of reasonably quick result, one method after another of chemical attack was adopted, with the ultimate result of freeing the group from its accom- panying fellows and increasing its intensity and detail. As I have said, my researches are far from complete, but about one of the bodies I may speak definitely. High up in the ultra-violet, like a faint nebula in the distant heavens, a group of lines was detected, at first feeble and only remarkable on account of their isolation. On further puri- fication these lines grew stronger. Their great refrangibility cut them off ' In this direction I am glad to acknowledge my indebtedness to Dr. Schuman, of Leipzig, for valuable suggestions and detail of his own apparatus, by means of which he has produced some unique records of metallic and gaseous spectra of lines of short wave-length. ee el clr \ ADDRESS. 29 from other groups. Special processes were employed to isolate the earth, and using these lines as a test, and appealing at every step to the spectro- graph, it was pleasant to see how each week the group stood out stronger and stronger, while the other lines of yttrium, samarium, ytterbium, «c., became fainter, and at last, practically vanishing, left the sought-for group strong and solitary. Finally, within the last few weeks, hopefulness has emerged into certainty, and I have absolute evidence that another member of the rare earth groups has been added to the list. Simultaneously with the chemical and spectrographic attack, atomic weight determinations were constantly performed. As the group of lines which betrayed its existence stand alone, almost at the extreme end of the ultra-violet spectrum, I propose to name the newest of the elements Monium, from the Greek povos, alone. Although caught by the searching rays of the spectrum, Monium offers a direct contrast to the recently discovered gaseous elements, by having a strongly marked individuality ; but although so young and wilful, it is willing to enter into any number of chemical alliances. Until my material is in a greater state of purity I hesitate to commit myself to figures; but I may say that the wave-lengths of the principal lines are 3120 and 3117. Other fainter lines are at 3219, 3064, and 3060. The atomic weight of the element, based on the assumption of R,0;, is not far from 118—greater than that accepted for yttrium and less than that for lanthanum. T ought almost to apologise for adding to the already too long list of ele- ments of the rare earth class—the asteroids of the terrestrialfamily. But as the host of celestial asteroids, unimportant individually, become of high interest when once the idea is grasped that they may be incompletely coagulated remains of the original nebula, so do these elusive and insig- nificant rare elements rise to supreme importance when we regard thein in the light of component parts of a dominant element, frozen in embryo, and arrested in the act of coalescing from the original protyle into one of the ordinary and law-abiding family for whom Newlands and Mende- leeff have prepared pigeon-holes. The new element has another claim to notice. Not only is it new in itself, but to discover it a new tool had to be forged for spectroscopic research. Further details I will reserve for that tribunal before whom every aspirant for a place in the elemental hierarchy has to substantiate his claim. These, then, are some of the subjects, weighty and far-reaching, on which my own attention has been chiefly concentrated. Upon one other interest I have not yet touched—to me the weightiest and the farthest reaching of all. No incident in my scientific career is more widely known than the part I took many years ago in certain psychic researches. Thirty years 30 REPORT—1898. have passed since I published an account of experiments tending to show that outside our scientific knowledge there exists a Force exercised by intelligence differing from the ordinary intelligence common to mortals. This fact in my life is of course well understood by those who honoured me with the invitation to become your President. Perhaps among my audience some may feel curious as to whether I shall speak out or be silent. I elect to speak, although briefly. To enter at length on a still debatable subject would be unduly to insist on a topic which—as Wallace, Lodge, and Barrett have already shown—though not unfitted for dis- cussion at these meetings, does not yet enlist the interest of the majority of my scientific brethren. To ignore the subject would be an act of cowardice—an act of cowardice I feel no temptation to commit. To stop short in any research that bids fair to widen the gates of knowledge, to recoil from fear of difficulty or adverse criticism, is to bring reproach on Science. There is nothing for the investigator to do but to go straight on, ‘to explore up and down, inch by inch, with the taper his reason’ ; to follow the light wherever it may lead, even should it at times resemble a will-o’-the-wisp. I have nothing to retract. I adhere to my already published statements. Indeed, I might add much thereto. I regret only a certain crudity in those early expositions which, no doubt justly, militated against their acceptance by the scientific world. My own knowledge at that time scarcely extended beyond the fact that certain phenomena new to science had assuredly occurred, and were attested by my own sober senses, and better still, by automatic record. I was like some two-dimensional being who might stand at the singular point of a Riemann’s surface, and thus find himself in infinitesimal and inexplicable contact with a plane of existence not his own. I think I see a little farther now. I have glimpses of something like coherence among the strange elusive phenomena ; of something like con- tinuity between those unexplained forces and laws already known. This advance is largely due to the labours of another Association of which I have also this year the honour to be President—the Society for Psychical Research. And were I now introducing for the first time these inquiries to the world of science I should choose a starting-point different from that of old. It would be well to begin with telepathy ; with the fundamental law, as I believe it to be, that thoughts and images may be transferred from one mind to another without the agency of the recognised organs of sense—that knowledge may enter the human mind without being communicated in any hitherto known or recognised ways. Although the inquiry has elicited important facts with reference to the Mind, it has not yet reached the scientific stage of certainty which would entitle it to be usefully brought before one of our Sections. I will there- fore confine myself to ‘pointing out the direction in which scientific investigation can legitimately advance. If teiepathy take place we have ~rrur ADDRESS. 3] two physical facts—the physical change in the brain of A, the suggester, and the analogous physical change in the brain of B, the recipient of the suggestion. Between these two physical events there must exist a train of physical causes. Whenever the connecting sequence of intermediate causes begins to be revealed the inquiry will then come within the range of one of the Sections of the British Association. Such a sequence can only occur through anintervening medium. All the phenomena of the universe are presumably in some way continuous, and itis unscientific to call in the aid of mysterious agencies when with every fresh advance in knowledge it is shown that ether vibrations have powers and attributes abundantly equal to any demand—even to the transmission of thought. It is sup- _ posed by some physiologists that the essential cells of nerves do not actually touch, but are separated by a narrow gap which widens in sleep while it narrows almost to extinction during mental activity. This con- dition is so singularly like that of a Branly or Lodge coherer as to suggest a further analogy. The structure of brain and nerve being similar, it is conceivable there may be present masses of such nerve coherers in the brain whose special function it may be to receive impulses brought from without through the connecting sequence of ether waves of appropriate order of magnitude. Réntgen has familiarised us with an order of vibra- tions of extreme minuteness compared with the smallest waves with which we have hitherto been acquainted, and of dimensions comparable with the distances between the centres of the atoms of which the material universe is built up ; and there is no reason to suppose that we have here reached the limit of frequency. It is known that the action of thought is accom- panied by certain molecular movements in the brain, and here we have physical vibrations capable from their extreme minuteness of acting direct on individual molecules, while their rapidity approaches that of the internal and external movements of the atoms themselves. Confirmation of telepathic phenomena is afforded by many converging experiments, and by many spontaneous occurrences only thus intelligible. The most varied proof, perhaps, is drawn from analysis of the sub-conscious workings of the mind, when these, whether by accident or design, are brought into conscious survey. Evidence of a region, below the threshold of consciousness, has been presented, since its first inception, in the _ Proceedings of the Society for Psychical Research ; and its various aspects _are being interpreted and welded into a comprehensive whole by the perti- nacious genius of F. W. H. Myers. Concurrently, our knowledge of the _ facts in this obscure region has received valuable additions at the hands _ of labourers in other countries. To mention a few names out of many, the observations of Richet, Pierre Janet, and Binet (in France), of Breuer and Freud (in Austria), of William James (in America) have strikingly illustrated the extent to which patient experimentation can probe sub- liminal processes, and can thus learn the lessons of alternating personali- ties, and abnormal states, Whilst it is clear that our knowledge of 32 REPORT—1898. subconscious mentation is still to be developed, we must beware of rashly assuming that all variations from the normal waking condition are necessarily morbid. The human race has reached no fixed or changeless ideal ; in every direction there is evolution as well as disintegration. It would be hard to find instances of more rapid progress, moral and physical, than in certain important cases of cure by suggestion—again to cite a few names out of many—by Liébeault, Bernheim, the late Auguste Voisin, Bérillon (in France), Schrenck NGuetar (in Germany), Forel (in Switzer- land), van Eeden (in Holland), Wetterstrand (in Sweden), Milne-Bramwell and Lloyd Tuckey (in England). . This is not the place for details, but the vis medicatrix thus evoked, as it were, from the depths of the organism, is of good omen for the orl evolution of mankind. A formidable range of phenomena must be scientifically sifted before we effectually grasp a faculty so strange, so bewildering, and for ages so inscrutable, as the direct action of mind on mind. This delicate task needs a rigorous employment of the method of exclusion—a constant setting aside of irrelevant phenomena that could be explained by known causes, including those far too familiar causes, conscious and unconscious fraud. The inquiry unites the difficulties inherent in all experimentation connected with mind, with tangled human temperaments and with obser- vations dependent less on automatic record than on personal testimony. But difficulties are things to be overcome even in the elusory branch of research known as Experimental Psychology. It has been characteristic of the leaders among the group of inquirers constituting the Society for Psychical Research to combine critical and negative work with work leading to positive discovery. To the penetration and scrupulous fair- mindedness of Professor Henry Sidgwick and of the late Edmund Gurney is largely due the establishment of canons of evidence in psychical research, which strengthen while they narrow the path of subsequent explorers. To the detective genius of Dr. Richard Hodgson we owe a convincing demonstration of the narrow limits of human continuous observation. It has been said that ‘Nothing worth the proving can be proved, nor yet disproved.’ True though this may have been in the past, it is true no longer. The science of our century has forged weapons of observation and analysis by which the veriest tyro may profit. Science has trained and fashioned the average mind into habits of exactitude and disciplined perception, and in so doing has fortified itself for tasks higher, wider, and incomparably more wonderful than even the wisest among our ancestors imagined. Like the souls in Plato’s myth that follow the chariot of Zeus, it has ascended to a point of vision far above the earth. It is, henceforth, open to science to transcend all we now think we know of matter, and to gain new glimpses of a profounder scheme of Cosmic Law. An eminent predecessor in this chair declared that ‘by an intellectual necessity he crossed the boundary of experimental evidence, and discerned in that matter, which we in our ignorance of its latent powers, and not- withstanding our professed reverence for its Creator, have hitherto covered _—=_-” - =~ = ADDRESS. 30 with opprobrium, the potency and promise of all terrestrial life.’ I should prefer to reverse the apophthegm, and to say that in life I see the promise and potency of all forms of matter. In old Egyptian days a well-known inscription was carved over the portal of the temple of Isis :—‘I am whatever hath been, is, or ever will be ; and my veil no man hath yet lifted.’ Not thus do modern seekers after truth confront Nature—the word that stands for the baffling mysteries of the universe. Steadily, unflinchingly, we strive to pierce the inmost heart of Nature, from what she is to re-construct what she has been, and to prophesy what she yet shall be. Veil after veil we have lifted, and her face grows more beautiful, august, and wonderful, with every barrier that is withdrawn. APPENDIX. In preparing the part of this Address dealing with the world’s supply . and demand for wheat, and the conclusions based thereon, I have been materially assisted by Mr. C. Wood Davis, of Kansas, U.S.A. Apart from information obtained from Mr. Davis’s articles in ‘The Forum,’ the ©North-Western Miller,’ the ‘New York Sun,’ and other papers, I am indebted to him for valuable manuscript information on matters of detail. Mr. Davis appears to be the only person dealing with this problem in a manner to determine such essential factors as average acre yields for long periods, unit requirements for each of the primary food staples of the temperate zones, and the ratios existing during different recent periods between the consuming element and acres employed in the production of each of such primary food staples. His scientific method enables him to ascertain the acreage requirements of the separate national populations, and of the ‘bread-eating’ world asa whole. Information has also been obtained from the ‘ Agricultural Returns of the United Kingdom,’ the official ‘ Reports on Agricultural Depression,’ and the Annual Reports of the United States Secretary of Agriculture ; likewise from papers and articles by Sir John Lawes, Sir H. Gilbert, Major Craigie, Mr. W. E. Bear, Mr. Warington, Professor E. M. Shelton, Mr. R. F. Crawford, Dr. Newton, and Mr. W. Walgrave Chapman. The ‘Journal of the Royal Agricultural Society,’ the ‘Journal of the Royal Statistical Society,’ _ the ‘Journal of the Board of Agriculture,’ and other periodicals have also been laid under contribution. I am also indebted to the various official publications of the Government of Canada, the Department of Agricul- ture, Queensland, and to friends all over the world. NS Last year there were under corn crops in the United Kingdom :— Wheat . ; . 3,025 sq. miles, producing 56,296,000 bushels. Barley . : . 38,447 A Oats) -. 5 . 6,580 i Total é . 13,052 7 1898, D 31. REPORT—1898. There is now about as much area under mixed cereals as would have to be devoted solely to wheat to make our country self-supporting. B.—The World’s Wheat Crop of 1897-98 from Contributory Areas.’ Bushels Bushels United States . - - 510,000,000 | Uruguay, Brazil, ke. . f 9,000,000 France : r ; - 240,000,000 | Portugal . . ® ‘ 7,000,000 Russia and Poland . . 230,000,000 | Servia F 5 + r 6,000,000 Austria-Hungary : . 135,000,000 | Holland . 2 A ; 5,000,000 Germany , : A . 105,000,000 | Denmark F ‘ 5,000,000 Spain . j j , - 96,000,000 | Sweden and Norway . ‘ 5,000,000 Italy . 3 d ; . 82,000,000 | Greece : ‘3 ; A, 4,000,000 Trans-Caucasia and Siberia 64,000,000 | Switzerland ; : 4 4,000,000 _ Argentina . 5 4 - 60,000,000 | Bosnia, Montenegro, Cy- United Kingdom : . 56,000,000 prus, &c. A : a 4,000,000 Canada , & 5 . 55,000,000 | South Africa . - - 4,000,000 Roumania . : ; - 483,000,000 rs Caucasia (Northern) . - 40,000,000 1,890,000,000 Australasia . ; - 38,000,000 Addimports from Asia Bulgaria . s ‘ . 80,000,000 and North Africa . 31,000,000 ‘Turkey in Europ : - 22,000,000 ——-—- Belgium . ; : . 16,000,000 Total available wheat Chili . Fi : A . 15,000,000 supply . : . 1,921,000,000 Table showing the Variations in the Bread-eating Populations and the Available Supply of Wheat in the Five Yearly Periods from 1878 to 1897, in Millions of Bushels, and Annual Averages. S z 1 Say) | Bread- Wheat Imports | Remain- - Supply | eating | grown by | from Asia {ders from Total Required in excess Years ‘ available | for seed Popula- | ‘Contribu- | and North | former of year’s feng tory areas’ Africa harvest | SUP ply, |, and food fect 1877-81 | 407-0 1797-0 13°8 1744 1985°2 1812°8 172°4 1882-86 | 432°8 1937°6 41-4 294-0 2273°0 1946:0 327-0 1887-91 | 4608 2043°5 43°2 260°2 23469 | 2102:0 2449 1892-96 | 490°9 2199:2 23°6 265°4 2488-2 2233°8 2544 | 1897-98 | 510°0 1890-0 31:0 3000 2221°0 2310°0 | Deficit | 89:0 C, The ‘ world’s demand’ for wheat is as follows :— Bushels Bushels ~ United Kingdom, about . 180,000,000 | Spain . : ; - 10,000,000 Belgium. : : - 24,000,000 | Portugal . 5 : : 4,000,000 Germany . : : . 35,000,000 | Greece : é 4 ¢ 4,500,000 Holland. : ; - 13,000,000 | Islands and tropical lands. 28,000,000 Switzerland 7 ; . 13,500,000 SSS SS France : : : . 40,000,000 Total 8 a » 356,000,000 Sweden ; A x y 4,000,000 D. Between 1882 and 1897 the wheat crops were so abundant that over 1,200 million bushels were added to our stores, beside large accumulations of rye. During this time of golden harvests, the exports from Russia increased, ? Outside the better known areas of wheat supply a certain proportion of wheat comes from India, Persia, Syria, Anatolia and North Africa. But it is impossible to get accurate figures as to acreage and yield from these countries; as bread-eaters derive less than one per cent. of their supplies from these outlying sources, it is con- venient to call the ordinary areas ‘ contributory areas,’ and to deal with the external areas no further than to show the volume of imports yielded from year to year. or Ov ADDRESS. in consequence of the Russian decline in unit consumption of 13:5 per cent. These reserves have been gradually drawn upon, but enough still re- mained to obscure the fact that the 1895-6 harvest was 75,000,000 bushels, and the 1896-7 harvest was 138,000,000 bushels below current needs. The following table' has been compiled from statistics carefully collected by Mr. Davis and other observers. The prophetic figures are on the assumption that population, unit consumption, and steady development will increase during the next forty-three years as they have increased since 1871 :— Food and Seed? ans With yields F Requiring Ay | Date Bread-eaters required tas 5 averaging 12°7 per unit. Se whsat bushels acreage | Bushels required 1871 371,000,000 415 1,540,000,000 121,000,000 | 1881 416,000,000 4:38 1,822,000,000 143,000,000 | 1891 472,600,000 4°50 2,127,000,000 167,000,000 | 1898 516,500,000 4-50 2,324,000,000 183,000,000 1901 536,100,000 4°50 2,412,000,000 190,000,000 1911 603,700,000 4:50 2,717,000,000 214,000,000 1921 674,000,000 4:50 3,033,000,000 239,000,000 1931 746,100,000 4:50 3,357,000,000 264,000,000 | 1941 819,200,000 4:50 3,686,000,000 290,000,000 | To supply these bread-eaters, the world inhabited by bread-eating populations grew the following quantities of wheat in each of the desig- nated five-year periods :— Bushels—Annual average Acres—Annual average | Years 1871-75 1,580,000,000, grown on 131,000,000 | 1876-80 1,746,000,000 5 143,000,000 | 1881-85 1,926,000,000 33 152,000,000 1886-90 1,987,000,000 5 154,000,000 1891-95 2,201,000,000 > 159,000,000 4 T have taken the unit consumption including seed at 4:5 bushels and the yield _ per acre at 12°7 bushels per annum, this being the average of the whole world. The exact yield varies with the country in which wheat is grown, as shown by the following table :— Average Yield of Wheat per Acre in— ‘ Bushels Bushels Denmark d 3 ‘ . 41:8 | Poland 16:2 United Kingdom . ‘ : . 291 | Canada . 15:5 New Zealand. : : . 25°5 | Argentina 13:0 Norway . ‘ 5 : 3 7 Zo | Ttaly =: : : 12-1 _ Germany . : ; ; . 23:2 | United States (mean) 12:0 - Belgium. 4 , ° ; 1 cb) |. india: 3 : 9°2 Holland . : ; ‘ : . 21:5 | Russia in Europe . Be rS6 France . : F F 194 | Algeria . ; ‘ : ‘ eh etn Hungary ; . ; i 18:6 | South Australia ; saree) Roumania ; ; 18:5 | Australasia , ; p e 68 Austria . 16°3 2 The seed quota is kept constant at 0°6 bushel per unit per annum, but the unit food requirements are found to increase in each five-yearly period.. There has been a steady increase of unit wheat requirements by reason of the decrease of unit con- sumption of rye, maslin, spelt, and buckwheat, D2 36 REPORT—1898. Within the same periods wheat was imported from Asia and North Africa by the ‘bread-eating ’ countries as follows :— Years Bushels—Annual average Acres—Annual average 1871-75 8,000,000, the net product of 750,000 1876-80 12,000,000 4 “ 1,120,000 1881-85 36,000,000 * a 3,360,000 1886-90 39,000,000 - 5 3,640,000 1891-95 | 34,000,000 ny + 3,200,000 Broadly speaking, 2,000 million bushels are now consumed in the countries where they are grown, either as food or for seed, while the balance is exported. E. At the present time the disproportion is even higher, owing to unit consumption gradually increasing from year to year, accompanied by slow shrinkage in the wheat area. | é | Per cent. of Increase — 1871 1884 1897 or Decrease in Twenty-six Years Population . - | 371,000,000 | 432,800,000 | 510,000,000 375 increase. Wheat acres . . | 125,800,000 | 154,300,000 | 158,000,000 25°6 increase. Rye acres : . | 111,000,000 | 110,300,000 | 106,500,000 4:1 decrease. The area planted with the two great bread-making grains is actually less now than thirteen years ago, despite enormous additions to the population. The area under all the bread-making grains is absolutely 2-2 per cent. less than thirteen years ago, notwithstanding an increase of one- fifth in requirements for bread. F. Notwithstanding this expansion the supplies of wheat were hardly sufficient for the food demands of the world. As the area under wheat has increased that under rye has diminished, with the result that scarcely an acre has been added to the world’s wheat and rye since 1890; and there was in 1897 a deficit in the two principal bread-making grains of more than 600,000,000 bushels. G. Stocks of wheat and flour in the United States were, relatively to population, probably never smaller, if so small as now. The following table (from Bradstreet) shows the visible supply of wheat in the States on June 1 since 1893 :— © Bushels Bushels 1893 F : + 93,700,000 1896 ; ; . 71,300,000 1894 é ' - 80,500,000 1897 ‘ : . 389,200,000 1895 : = - 72,800,000 1898 : : - 32,500,000 ADDRESS. 37 H. In 1896 the area under wheat in the Governments of Russia and _ Poland was 36,000,000 acres. But the yearly consumption of wheat per head during the last ten years has declined 14 per cent., and the consump- tion of bread is quite 30 per cent. less than is required to keep the popu- lation in health. The grain reserved for seed has likewise decreased—the peasantry limiting their sowing with the rise of taxation. The reduction of 14 per cent. in the unit consumption of bread in Russia has added, during the last eighteen years, 1,360,000,000 bushels to the general wheat supply. This factitious excess temporarily staved off scarcity in Europe. IF In the year 1897 there were 2,371,441 acres under cultivation in Manitoba, out of a total of 13,051,375 acres. The total area includes water courses, lakes, forests, towns, and farms, land unsuitable for wheat- growing, and land required for other crops. J. The most trustworthy estimates give Canada a wheat area of not more than six millions of acres in the next twelve years, increasing to a maxi- mum of twelve millions of acres in twenty-five years. The development of this promising area necessarily must be slow, since prairie land cannot be laid under wheat in advance of a population sufficient to supply the needful labour at seed time and harvest. As population increases so do home demands for wheat. Acreage, Crop, and Exports of Wheat from Canada from 1891 to 1896. Year Population Acres Total bushels | Bushels exported 1891 4,833,000 | 2,690,000 62,600,000 3,000,000 egg). 4,885,000 2,910,000 49,700,000 | 10,200,000 W893) ~~ 4,936,000 2,800,000 42,700,000 | 11,000,600 1894. 4,986,000 2,550,000 44,600,000 | 11,000,000 1895 5,040,000 2,560,000 57,500,000 9,200,000 1896. 5,090,000 2,700,000 40,800,000 | 10,400,000 1897 5,140,000 2,900,000 56,600,000 / 8,000,000 The net exports average 8,970,000 bushels yearly, being 24-3 per cent. of the net product. K. The land under wheat in Austro-Hungary, according to the latest official figures, is eleven million acres. The 1897-8 crop, including that of Croatia-Slavonia, is fifty-five million bushels below that of 1896-7, and as exports during the last five years have averaged less than 4,000,000 bushels per annum, the imports of wheat are expected to be large. ~ REPORT—1898. i So long ago as April 16, 1891, the following statement by a leading Indian economist appeared in the ‘Daily Englishman’ of Calcutta :— ‘People do not realise the fact that all the wheat India produces is required for home consumption, and that this fact is not likely to be realised until a serious disaster occurs, and that even now less than 9 per cent is exported. It is a self-evident fact that a slight expansion of consumption, or a partial failure of crops of other food grains, will be sufficient to absorb the small proportion now exported. Besides, we have a steady increase of consumption, in consequence of the natural growth of the population, as well as in the gradual improvement of the condition of a considerable part of the people in the cities. I believe that, com- paratively speaking, India will in a few years cease to export wheat, and soon thereafter become an importing country.’ M. An average wheat crop on the 1897-8 acreage would be 2,070,000,000 bushels. Adding to this 1,270,000,000 bushels, makes a grand total of 3,340,000,000 bushels. But the estimate in Appendix D shows that in the year 1931 the bread-eaters will require 3,257,000,000 bushels. Thus there will be in 1931 a deficiency of 17,000,000 bushels, unless the average yield per acre be increased. N. Sir Andrew Noble informs me that a first-class battleship would carry about sixty-three tons of cordite, and we may suppose that in a general action forty tons of this would be expended. Now at Trafalgar, Nelson had twenty-seven line-of-battle ships, and the allied forces thirty-three. If we suppose a similar number of modern battleships and first-class cruisers to be engaged, and each to expend forty tons of cordite, the total volume of nitrogen set free would be 302,400 cubic metres, or about 3580 tons, equivalent to 2,300 tons of nitrate of soda. co DB ‘ REPORTS ON THE ‘STATE OF SCIENCE.- ——— gg eee » ; REPORTS ON THE STATE OF SCIENCE. Corresponding Societies Convmittee.— Report of the Committee, con- sisting of Professor R. MELDoLA (Chairman), Mr. T. V. HOLMES (Secretary), Mr. FRANCIS GaALTon, Sir DotGLas GATon, Dr. J. G. Garson, Sir J. Evans, Mr. J. Hopkinson, Mr. W. WHITAKER, Mr. G. J. Symons, Professor T. G. Bonney, Mr. CUTHBERT PEEK, Mr. Horace T. Brown, Rev. J. O. Bevan, and Professor W. W. WATTS. The 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 Bristol. The Council nominated Mr. W. Whitaker, F.R.S., Chairman, and Mr. T. V. Holmes, Secretary to the Bristol Conference. tions were confirmed by the General Committee at a meeting held at. Bristol on Wednesday, September 7. The meetings of the Conference were held at University College on Thursday, September 8, and Tuesday, September 13, at 3 p.m. The following Corresponding Societies nominated as delegates’to represent them at the Bristol meeting :— Andersonian Naturalists’ Society Belfast Naturalists’ Field Club. Belfast Natural History and Philosophical Society Berwickshire Naturalists’ Club . Birmingham Natural History and Philoso- phical Society. Bristol Naturatists’ Society Buchan Field Club Burton-on-Trent Natural History and Archeological Society. Caradoc and Severn Valley Field Clu Cardiff Naturalists’ Society 4 - Chesterfield and Midland Counties I tution of Engineers b nsti- Professor M. Laurie, D.Sc. William Gray, M.R.I.A, Alexander Tate, M.Inst.C.E. G. P. Hughes, J.P. Alfred Browett. F. W. Stoddart. John Gray, B.Sc. Philip B. Mason, F.L.S. Professor W. W. Watts, F.G.S- J. T. Thompson, M.B. M. H. Mills, M Inst.C.E, These nomina- 42 REPORT—1898, Croydon Microscopical and Natural History Club. Dorset Natural History and Antiquarian Field Club. East Kent Natural History Society . Essex Field Club Federated Institution of Minas Tingiffeass Glasgow Geological Society Glasgow Natural History Society Hampshire Field Club. . Hertfordshire Natural History Society Holmesdale Natural History Club Ireland, Statistical and Social Inquiry Society of Isle of Man Natural History and Anti- quarian Society Leeds Naturalists’ Club 5 Liverpool Engineering Society . ° Liverpool Geographical Society Liverpool Geological Society Malton Field Naturalists’ and Scientific Society. Manchester Geographical Society . . Manchester Geological Society . Manchester Microscopical Society Norfolk and Norwich Naturalists’ Society North Staffordshire Naturalists’ Field Club North of England Institute of Mining Engineers Northamptonshire Natural History Society Perthshire Society of Natural Science Rochdale Literary and Scientific Society Scotland, Mining Institute of . Somersetshire Archeological and Natural History Society. South Eastern Union of Scientific Societies Toronto Astronomical and Physical Society Tyneside Geographical Society . Warwickshire Naturalists’ and ‘Arche logists’ Field Club. Woolhope Naturalists’ Field Club. Yorkshire Geological and Polytechnic Society. Yorkskire Naturalists’ Union . 5 W. F. Stanley, I'.G.S. Dr. H. Colley March. Mrs. Edith Abbott. T. V. Holmes, F.G.S. M. H. Mills, M.Inst.C.E. J. B. Murdoch. G. F. Scott-Elliott, M.A. T. W. Shore, F.G.S. J. Hopkinson, F.L.S. Miss Ethel Sargant. Professor Bastable, M.A. P. M. C. Kermode. Harold Wager, F.L.S. Professor H. §. Hele - Shaw, M.Inst.C.E. Professor Gonner, M.A. Professor Herdman, F.R.S, M. B. Slater, F.L.S. Eli Sowerbutts, F.R.G.S. Mark Stirrup, F.G.8. F. W. Hembry. Clement Reid, F.G.S. Dr. Wheelton Hind, F.G.S. T, Forster Brown, M.Inst. C.E. Beeby Thomson, F.G.S. Dr. H. R. Mill, F.8.S.E. J. R. Ashworth, B.Sc. James Barrowman. Lieut.-Col. J. R. Bramble, I°.S.A. Dr. G. Abbott. W. F. Denning, F.R A.S. G. E. Smithson. William Andrews, F.G.S. Rev. J. O. Bevan, M.A. William Cash, F.G.S8. Harold Wager, F.L.S. First Conference, Bristol, September 8, 1898. The Corresponding Societies Committee were represented by Mr. W. Whitaker (Chairman of the Conference), Dr, Garson, Mr. Hopkinson, Professor Meldola, Mr. G. J. Symons, and Mr. T. V. Holmes (Secretary). delegate present, was taken as read :— The following Report, a copy of which was in the hands of every » CORRESPONDING SOCIETIES. 43 The Corresponding Societies Committee of the British Association beg leave to submit to the General Committee the following report. The Committee observe with satisfaction that the corresponding societies steadily increase in number, and that the total number of the members composing them also increases. For example, in the British Association Report of the Bath Meeting in 1888 there is a list of 55 corresponding societies, having a total of 18,950 members. The Toronto Report of last year shows 69 corresponding societies, having a total of 22,395 members. On the other hand, the average number of members in each society appears to have slightly decreased, having been between 344 and 345 in 1888, and between 324 and 325 in 1897. But this is accounted for by the collapse of the two federations—the Midland Union and the Cumber- land and Westmoreland Association—and the withdrawal of the Royal Scottish Geographical Society between the two periods. For in 1888 these three associations numbered among them 4,006 members, as many as would be found in eleven or twelve average societies. The Committee are also pleased to know that as the great majority of the societies, the main purpose of whose existence is local scientific inves- tigation, are now on the list of corresponding societies, the index of their more important papers approximates to completeness more and more each ' year as a record of local work. But they nevertheless regret the absence from their index of papers read before certain societies of more or less importance which from various causes are not on their list. Primarily by the term ‘local’ the British Association implies that a society so classed has its headquarters out of London. But it can hardly be expected that societies which have long flourished in cities such as Edinburgh and Dublin will feel that they are ‘local,’ as they might be justified in doing if their headquarters were at Aberdeen or Belfast, Leeds or Birmingham, or as if they recognised some county as their sphere of action. Then, many societies have been formed for the study and advancement of some science or group of sciences in various parts of the country, with little reference to local phenomena, which societies appeal to their members rather as being conveniently near than in any other way. But though societies such as have just been alluded to may be little more ‘local’ in feeling and in the nature of their work than London societies it must sometimes happen that papers devoted to local scientific investigations are published by them. The Committee therefore regret the absence from their list of papers of local interest which have been published by such societies as the following : The Royal Irish Academy, Royal Dublin Society, Institution of Civil Engineers of Ireland, Royal Society of Edinburgh, Botanical Society of Edinburgh, Royal Physical Society of Edinburgh, Liverpool Biological Society, Liverpool Naturalists’ Field Club, Manchester Literary and _ Philosophical Society. Fortunately, in most cases, information as to the titles and authors of _ papers read before local societies which are not corresponding societies of the Association may be obtained from the ‘ Official Year-book of the Scientific and Learned Societies of Great Britain and Ireland,’ C. Griflin & Co., London. The ‘ Year-book’ appears every spring, and contains lists of papers read in the previous year. It will be found that the ‘ Year-book’ and the British Association ‘ Index’ combined leave little to be desired by the inquirer after papers on any locality in the British Isles. 44 REPORT—1898., The following Societies have been added to the list of the Corresponding Societies : — The Astronomical and Physical Society of Toronto. The Hull Geological Society. The South-Eastern Union of Naturalists’ Societies. The Chairman, Mr. Whitaker, then opened the proceedings. He said that it had become usual to bring some special subject for discussion before the first meeting of the Conference. On that occasion he wished to draw their attention to that of Coast Erosion. All persons were interested in the scenery of our shores, whether living in counties border- ing the sea or wholly inland. Moreover, some counties having a coast line had few or no local scientific societies, and might need help from others farther from the sea. It was now possible to obtain maps on the scale of six inches to the mile for all localities, and on these measure- ments could be made from the edge of the cliffs, at any given time, to the nearest roads, footpaths, hedges, cottages or other objects, and the amount of land lost since the map was made could be accurately ascer- tained. Of course, all such measurements should be dated. . Very good work had been done in the past with old one-inch maps, but many pre- cautions were necessary in using them which were needless with six-inch maps. In illustration of the loss which has been sustained in certain places, he might mention Sheppey. The Geologists’ Association had made three excursions there. On their first visit the church and church- yard of Warden were untouched. Some years later the churchyard was found to have been partly destroyed, and coffins were seen sticking out from the edge of the cliff. This year neither church nor churchyard could be seen, There was another form of encroachment by the sea which had been well displayed during a recent visit of the Geologists’ Association to Aldeburgh in Suffolk. There they found many cottages, sheds, and gardens more or less injured, or even destroyed by the heaping up of masses of shingle in or against them, the result of a storm in Novem- ber 1897, which had caused much damage over many miles of our coast. Much injury to land adjoining the sea was often done by blown sand, which here and there had been driven to considerable heights, and covered areas of some breadth, as he had recently seen on the northern coast of Cornwall. The help of the photographer was extremely valuable in giving an unas- sailable record of a past state of things; the damage done by natural forces being often greatly obscured in a comparatively short period of time. The photo-theodolite might often be found useful in this matter. Turning to the economical aspect of the question, Mr. Whitaker remarked that there were two things especially worthy of attention, (1) the removal of shingle from the shore, (2) the quarrying of stone on the faces of sea cliffs. There were certainly some places at which the removal of shingle from the shore should never be allowed ; nowhere should it be permitted without some thought as to the probable result. And the quarrying of stone on the face of a sea cliff often had a powerful influence in aid- ing the erosive agencies of Nature. Archzxologists would be interested in noting spots where old British camps had been partly destroyed by the sea ; examples of which he (Mr. Whitaker) had noticed on the Chalk of Dorset, and on the much harder rocks which form the cliffs of northern Cornwall. Observations of this kind were not only cal- culated to make us realise the differences between the outlines of the CORRESPONDING SOCIETIES. 45 coast now and in prehistoric times, but they alsoled us to try and imagine the probable changes of the future. His remarks were intended simply to start a discussion on a subject in which he had always taken great interest. Mr. T. V. Holmes said that, as secretary of the Corresponding Societies Committee, he had been requested to write to three gentlemen, known as having taken much interest in Coast Erosion, to ask them if they would be good enough to take part in this discussion. One of these gentlemen, Captain McDakin, regretted his inability to attend, the other two, Mr. W. H. Wheeler and Mr. A. T. Walmisley, were, he believed, present. The Chairman had also asked Prof. Armstrong, Mr. Cornish, and Mr. Spiller to attend. Mr. W. H. Wheeler had a paper to read on this subject on Monday, which embodied the results of his observations on Coast Erosion. In his opinion the movement of shingle along the shore was due to the action of the tides and not of the winds. Professor H. E. Armstrong recommended the taking of photographs by means of the photo-theodolite instead of in the ordinary way. Mr. Gray said, that the Belfast Naturalists’ Field Club had already noted a great many points with regard to Coast Erosion in their district, and were going to issue a special report on the subject next year. ; Mr. A. T. Walmisley had always advocated the protection of the foreshore by means of groynes. Sea-walls were very useful in the pro- _ tection of cliffs when placed not close to, but a short distance in front of, _ the cliff to be protected. Waves then might rush up the face of the wall without touching the cliff. _ Mr. Vaughan Cornish had come to the conclusion that the protection of one part of the shore was a bad thing for the rest of the district. Considering how restricted was the area with which lords of manors, corporations, and local authorities of all kinds concerned themselves, he thought that no local work of shore protection should be begun till it had been sanctioned by a Government Board. In any study of the results of Coast Erosion, the Coastguard would be able to render most valuable assistance. They were aiways tramping along the shore, they were to a considerable extent trained observers, and they might be simultaneously at work all round the British Isles, if the consent of the Admiralty could be obtained to their co-operation in the study of Coast Erosion. Mr. G. J. Symons mentioned, in illustration of the danger of allow- ing people to do as they pleased on the shore, that his grandfather at the beginning of this century was building martello towers on the southern shores of England. One day he observed some men in a boat off Bognor taking stones to the mainland, and with them building a house. His grandfather warned them that the sea would reclaim the stones some day. And recently he had learned that the people there a been put to much trouble in endeavouring to restrain the inroads of the sea. Mr. Clement Reid referred to the waste of land along the west coast ; and said that it was most necessary in that district to have the new ordnance survey maps. Mr. J. Spiller gave details as to the encroachments of the sea at Southwold in Suffolk. Quite recently masses of shingle had been thrown AG REPORT—1898, on the land so as to cover a whole pasture field. Nothing had hitherto been done to check these inroads beyond the provision of groynes. Many old landmarks had disappeared, and the gun-battery was a thing of the past. He thought Government intervention desirable, and that it would be a good thing to obtain the co-operation of the Coastguard in noting the changes on our shores. Mr. Tate said that the amount of Coast Erosion differed very much in different districts. In some quarters there seemed to be a feeling in favour of restrictions on the protective measures allowable in any given case. It would, however, be difficult to obtain Government regulation unless it should appear that there was a manifest public need for it. Mr. Wheeler thought that the retention of a considerable mass of shingle in front of a place would furnish a better protection than a sea wall. He greatly approved of an attempt to obtain the services of the Coastguard in making a survey of the coast, as at present he had found it very difficult to get trustworthy evidence, the most opposite stories being told in almost every case. People did not know because they did not really observe, while the occupation of a Coastguardsman neces- sarily made him observant. He did not approve, however, of general Government regulations. Mr. Scott-Elliot thought that it would be a very good thing to obtain the co-operation of the Coastguard. Professor Meldola remarked that the general opinion certainly ap- peared to be in favour of an attempt to obtain the approval of the Admiralty for their wish to secure the co-operation of the Coastguard, and the Conference would be acting within its powers in sending up a recommendation on the subject. He would therefore move :— ‘That the Council of the British Association be requested to bring under the notice of the Admiralty, the importance of securing systematic observations upon the erosion of the sea coasts of the United Kingdom, and that the co-operation of the Coastguard might be profitably secured for this purpose.’ Mr. Wheeler asked whether the matter should not be referred to the Coast Erosion Committee of the British Association. The Chairman reminded the last speaker that the labours of that Committee were ended. He thought that the Coastguard were perfectly capable of doing the work proposed, and that they would be pleased to do it. Discussion then ensued on various points of detail, among others on the question where specimens of shingle collected at certain spots in order to note its movements along our shores should be stored. In this Messrs. Wheeler, Shore, Symons, and Gray took part. Professor Meldola remarked that the resolution did not commit either the Admiralty or themselves to any particular line. Should the Admiralty ask how it -was suggested that the Coastguard should make observations, then it might be for that Conference to draw up rules for their adoption. Mr. Gray seconded the resolution, and after some remarks from Mr. Sowerbutts, Professor Meldola, the Chairman, and Mr. Hopkinson, it was put to the meeting and carried. Professor Meldola then announced that he had just received the following letter from Professor Watts :— CORRESPONDING SOCIETIES. 47 Corndon, Worcester Road, Sutton, Surrey : September 7, 1898. Dear Sir,—It might be as well to report to the Conference of Dele- gates that the B. A. Geological Photographs Committee has formed a collection of duplicate photographs and slides, which can be sent during the winter to any local scientific society desiring to make use of them. Tt consists of about 250 prints in two albums, and about 100 lantern slides. Faithfully yours, W. W. Warts. Dr. Abbott wished to know if there would be any opportunity of discussing the subject of the Federation of Local Societies at that meeting of the British Association. The Chairman thought that it might be brought forward at the next meeting of the Conference. Second Meeting of the Conference, September 13. The Corresponding Societies Committee were represented by Professor Meldola, Mr. Whitaker, Dr. Garson, Rev. J. O. Bevan, Mr. Hopkinson, Mr. G. J. Symons, and Mr. T. V. Holmes (Secretary). The Chairman (Mr. Whitaker) announced that action had been taken with regard to the Resolution on Coast Erosion passed at their last meeting. It had been submitted to the Committees of the Geological and of the Geographical Sections, both of which unanimously supported the recommendations contained in it. Dr. Garson then took the chair, Mr. Whitaker being obliged to leave. Uniformity of Size of Pages of Scientific Societies’ Publications. Professor 8. P. Thompson said that he had been asked to bring before the Conference a matter on which a Committee of the British Association had already made one Report, and still continued to exist, with the intention of making another. This question was the importance of adopting one or two uniform standard sizes for the pages of scientific publications. All who were engaged in any kind of scientific investigation were greatly indebted to the reprinted papers on the subjects in which they were interested which were sent to them by their fellow workers. And all recognised the great advantage given by uniformity in the size of their pages, which permitted them to be bound together and per- manently preserved. The great desirability of promoting uniformity in size of page had caused Section A some four years ago to promote the formation of a Committee whose object was to prescribe the adoption of certain standard octavo and quarto sizes. The Report of this Committee would be found in the Ipswich Report of the British Association, pp. 77— 79 (1895). The Peas octavo size recommended was : Paper demy, the pages measuring 14 cm. x22 cm., or, when uncut, 53in.x8#in. The width, measured from the stitching to the outer edge of the printed matter, to be 12 cm., or 48in., and the height of the printed portion, including the running headline, to be 18 cm., or 7 in. 48 REPORT—1898. The standard quarto size: Paper demy, the pages measuring, when uncut, 22 cm. x 28-5 em., or 8fin. wide x 11} in. high. Letter-press not to exceed the measurements of 74 in. by 9 in. It was also desirable that each article should begin a page, and that, if possible, it should begin on a right-hand page. It is then practicable to bind that article with others without binding up with it the last page of another. Many other details dealing with what is desirable in scientific publications may be found, with illustrations, in the Report of the Committee in the Ipswich volume. A method of splitting printed pages, useful in separating successive articles in a journal, for collections of pamphlets, was incidentally described.! The Chairman (Dr. Garson) remarked that they were greatly in- debted to Professor Thompson, who had raised a question of much practical importance. Professor Meldola thought that they were much indebted to Professor Thompson for bringing this matter forward. To endeavour to promote the uniformity of size which had just been advocated was one of the original functions of these Conferences, and he hoped that the suggestions of Professor Thompson might bear fruit. It was the duty of the Corre- sponding Societies Committee to collect the publications of the Correspond- ing Societies at Burlington House, but, on gazing at the shelves on which they lay, a great want of uniformity in size became manifest. Some societies also did themselves injustice as regards paper and printing. Mr. Tate was glad that the matter had been brought forward, on account of the great advantage arising from being able to bind together papers and pamphlets issued by various societies. He would bring the subject before the Society he represented. Mr. Clement Reid suggested that the original paging should be pre- served in reprints. The Rev. J. O. Bevan hoped that when the matter was brought before the Corresponding Societies by the delegates the general interest in uniformity might be dwelt upon, as many societies might otherwise feel indifferent towards it. Mr. Gray said that as most papers on local subjects were reprinted, these suggestions would probably determine the form of the reprints. Mr. Abbott thought that it would be well if the secretaries of societies issuing publications irregular in size and form had their attention drawn to the subject. ; Mr. Hopkinson was acquainted with the publications of most of the local societies, and thought that the number which were irregular in size and form was very small indeed. The chief offenders were socie- ties which, from want of sufficient funds, published reprints from local newspapers. He thought each paper should begin at the top of a ' At the request of the Chairman of the Committee, the following note is added on the method of splitting a page of printed matter described verbally to the Com- mittee :—Gum to each face of the page that is to be split a rather larger leaf of paper of a thin tough quality—resembling bank-note paper. The projecting edges should not be gummed. Let them become quite dry. Procure two small wooden rollers, about 7 inches (or more) long and 3 inch (or less) in diameter. Then put the edges of the prepared page between the rollers, and, grasping them in the hands, 60 roll the respective edges of the two leaves around the rollers as to peel them or tear them away from one another. The use of the rollers is to prevent the page from tearing irregularly. Finally, soak off the two leaves in water. Not every kind of printed paper can be split without tearing.—S. P. T. CORRESPONDING SOCIETIES, 49 page; but the suggestion that each paper should begin on the right- hand page could not always be adopted on account of the loss of space which would sometimes occur thereby where there were many short papers. The present discussion would probably be of more service in guiding new societies than in causing alterations in the publications of old ones, which would spoil the uniformity of a set of volumes. _°.The Chairman, Dr. Garson, thought that they should give their best thanks to Professor Thompson for bringing this matter before them. The time also was opportune, as we were nearly at the close of the nineteenth century, and the beginning of another century would be an excellent period for the commencement of a new series in cases where it was desirable in the interests of uniformity. The suggestion that reprints might be of one uniform size, even if the original publication were not so, ‘was one of great importance. It might be worth while to take up the question of publications next year as a special subject, and it would be a good thing if the delegates would consider the matter during the winter and consult their societies upon it, so as to be able to discuss it with authority upon another occasion. The Rey. J. O. Bevan suggested that they might ask the Corresponding Societies to come to some conclusion upon this question, and forward it to the secretary of the Committee. Professor Meldola said that they would be quite prepared next year to name those societies which were offenders with respect to uniformity. Mr. Hopkinson had pointed out that they were few in number. Mrs. Abbott suggested that it would be a good thing to offer information on the subject to as many societies as possible. Lieut.-Col. Bramble asked what was to be done in the case of societies which had no delegates present. The Chairman replied that the report cf the Conference was sent to every society on their list. And any information applied for by other ‘societies would be given. f Section A. Mr. G. J. Symons, representing Section A, said that there was only one matter to which he wished to draw attention. Professor Milne, as most of them knew, was making some highly important observations on earthquake tremors. But he was then working in a house in the Isle of Wight, which was in so bad a sanitary state that many fears were enter- tained with regard to his health. It had been suggested that there were houses in Richmond Park well suited to be the scene of Professor Milne’s labours, and that it might be well to approach the Government to see whether one of them could be obtained for him. If not, perhaps some rich man, on being made acquainted with the case, might lend a house for a few years. Nothing sumptuous was asked for, only quarters which were water-tight and healthy. Section C. Mr. Beeby Thompson said that a fine specimen of a Dinosaur had recently been discovered near Northampton. It would, however, bea very expensive task to uncover it carefully, and it was necessary that the work 1898, E 50 REPORT—1898. should be proceeded with without delay. He wished therefore cither to obtain a grant from the British Association, or to induce any rich people who might hear of the case and be interested therein, to assist in pro- viding the necessary funds. The Chairman (Dr. Garson) thought that an effort should be made to bring the matter before the scientific societies of Northampton. Mr. Gray stated that the Society he represented was second to none in its efforts to collect geological photographs. He thought much more might be done by other societies in that work. Section H. The Chairman wished to draw the attention of the Conference to the Ethnographical Survey, an investigation in which few local societies were co-operating. Full directions for guidance in the various departments of the work might be obtained from the papers issued by the Ethnographical Survey Committee. The amateur photographer would find a wide field of action in noting physical characteristics. The important point was to get a common standard of size, a very convenient one being one-seventh of the natural size. Another department was that of the ancient monuments and general archeology of a district. Then came the collection of its folklore, and the noting of local names and dialects. Mr. Gray said that the Society he represented had much sympathy with the objects of the Ethnographical Survey Committee, especially as regards the cataloguing of antiquities. He hada list of all the Holy Wells of Antrim and Down, together with photographs of them. He much wished to obtain the co-operation of the Royal Society of + | —0°49 | —0°72 | —0°92 | —116 | —1°97 | —3°32 | —4:72 | —5:12 | —5°03 | —3-74 | —1'52 July. . + | —0°65 | —0°82 | —1:16 | —1°34 | —2°00 | —3-40 | —4:53 | —4°74 | —4°84 | —3°86 | —1-66 August . -| —0°92 | —1°15 | —1:28 | —1°67 | —2°00 | —2°93 | —3-98-| —4:71 | —4-44 | —3-01 | —0-22 September . | —1:16 | —1:27 | —1°47 | —1°99 | —2:22 | —2-49 | —3-13 | —3-79 | —3°66 | —2°31 | +0:35 October . - | —151 | —116 | —1-11 | —]:02 | —0-94 | —1-19 | —1°38 | —1-93 | —2-90 | —3-02 | —1:55 November « | —1-21 | —0°82 | —0°75 | —0°68 | —0°53 | —0°72 | —0:97 | —1:20 | —1°75 | —1:90 | —0-77 December + | —117 | —0:80 | —0-46 | —0°31 | —0°36 | —0°52 | —0:77 | —0°80 | —0°92 | —1-09 | —0-30 Spring . - | —111 | —1:03 | —0°95 | —1-:09 | —1-11 | —1:20 | —1°63 | —2-43 | —3:28 | —3°08 | —1-56. Summer . + | —0°66 | —0°81 | —1:06 | —1°30 | —2°03 | —3:30 | —4°51 | —4:95 | —4°84 | —3°64 | —1-:22 Autumn . + | —1:20 | —119 | —1:29 | —1:56 | —1-72 | —2'20 | —2°83 | —3-48 | —3°67 | —2:78 | —0-47 Winter . - | —1:25 | —0°92 | —0°68 | —0-53 | —0°52 | —0-60 | —0°83 | —0°97 | —1:29 | —1-45 | —0°51 The Year. —1°05 | —0°99 | —0-99 | —112 | —1°35 | —1:82 | —2°45 | —2°96 | —3:27 | —2°74 | —0-94 Excess of the quiet days value Spring . . | +080 | +0°77 | +0°61 | +0°40 ) +040 ) +0:34 | +016 | —O-14 | —0-44 ) —0°55 | —0°81 Summer. . | +0°47 | +047 | +0-42 | +038 | +034 | +026 | 0-00 | —o-10 | —0-32 | 0°39 | 034 Autumn. . | +044 | +0°57 | +0°55 | +0°36 | +018 | —0-14 | —0°32 | —0°52 | —0°66 | —0-74 | —0-7 3 Winter . «| +0°70 | +0°54 | +0°29 | +0-11 | +002 | —0°07 | —0°31 | —0-44 | —0°51 | —0°55 | —0 -46 The Year. + | +0°61 | +0°59 | +0°47 | +0°31 | +0°23 | +010 | —0°12 | —0°30 | —0-48 | —0-56 | —0°58 . Observations made at the Royal Observatory, Greenwich, 1890-1894, il ON COMPARING AND REDUCING MAGNETIC OBSERVATIONS. Noon 1 | | ae | 7 | we | 9 | \ 20 21 to tw 91 bo oo . of extreme magnetic disturbance. 41-28 +178 42°30 ; | q +199 i +-2'84 +1°80 +1°83 43:17 . +402 +2°46 +1'85 +132 + 2°02 +216 +3'22 +148 4261 43°61 +521 45°34 45°37 44:35 4472 +598 45:95 44:92 43°50 42°39 4472 +481 45°62 42°83 +340 44°44 +6742 +6°93 +6'42 +5°70 +613 +6°93 +6°64 +5°78 +413 +3°04 +593 +6:08 + 6°45 +3°52 42:97 44:38 46-05 46°54 46°03 45°99 46°39 46:27 45°70 45-28 43°57 42°89 +5°66 +614 +5°75 +314 +450 +5°50 +517 49:10 43°22 +468 $485 $482 45-20 45°33 44°63 +400 43°84 42°47 42°30 44-95 4512 44:16 42:29 +3°95 41-43 41:91 42°61 4311 43°20 43°79 43°76 42°47 42-10 4218 41-48 41:56 +2°54 +3°58 +2°25 +149 +2°47 after elimination of the non-cyclic increment. ; +0°87 . +118 +170 +111 +2'86 +144 +1°30 +3:07 +3°41 +138 +1:28 +098 + 2°52 +2'93 +457 +423 +5°75 +431 +433 +5:90 +538 +3'87 +311 +1:87 +3°37 +3°66 +572 +6°05 +6°62 +5°64 +6°04 +6°77 +577 +492 +3°68 +2°52 +2°91 43°75 +5°22 +5°49 +6°08 +5°62 +6°52 +5°96 +4°95 +469 +3:07 +2°38 +1:89 +2°80 +3°67 +3:93 +427 +458 +532 44:27 +313 +3°42 +2°10 +179 +123 41°44 +1°60 +233 +2°40 +323 +3°32 +218 +152 +1'88 +1:29 +1°04 +179 +0°83 40°73 +0°32 41:05 +0°98 +1:90 41°44 +0°41 +0°53 +111 +0°62 +0°52 +0°70 —daz | —0-85 | —i-44 | 1-77 —0'10 | —0:77 | —1:46 | —1:92 —0°66 | —1-:11 | —1°62 | —1°85 —0'56 | —0-91 | —1°05 | —1:24 —0:05 | —0-40 | —0°66 | —0°81 +0°38 | +0:07 | —0-:08 | —0-15 +0:27 | 0:00 | —0-27 | —0-41 —0-41 | —055 | —0-61 | —0-97 —0°68 | —1°32 | —1-42 | —1°54 —0-72 | —1°60 | —2°30 | —2:56 —0°53 | —1°34 | —1:87 | —2°11 —017 | —1:06 | —1:78 | —2°05 —0:44 | —0°93 | —1°38 | —1°67 +0:20 | —O'11 | —0:34 | —0-46 —0'60 | —1:16 | —1-44 | —1-69 —0-27 | —1:08 | —1-70 | —1:98 —0'28 | —0°82 | —1:21 | —1°45 +0°01 | —0°59 | —0°97 | —1°31 +0°21 | —0°30 | —0°80 | —1°07 —0°48 | —0°64 | —0-91 | —1-02 —0'21 | —019 | —0°05 | —0:27 —0'30 | —044 | —0°41 | —0-22 +0°42 | +0:29 | +0°30 | +0:24 +0:08 | +014 | +0:10 | +0:06 —0:13 | —0-28 | —0'31 | —0°52 —0:05 | —0'36 | —0°31 | —0:27 +0°05 | —0°38 | —1-04 | —1-25 —0'10 | —0°57 | —1:00 | —1°19 —0°02 | —0°46 | —0°91 | —1-24 —0'16 | —0:38 | —0:59 | —0-79 +0:07 | 0:00] 0:00 | +0:03 —0:04 | —0°34 | —0°55 | —0°68 —0:04 | —0:54 | —0°96 | —1:25 —0°04 | —0°32 | —0°53 | —0°67 +0:28 | +0°55 | +0°79 | +0°88 —013 | +011 | +0:34 | +0-49 +0°56 | +0°82 | +0°89 | +1°01 +023 | 40:54 | +074 | +0°73 +0:24 | +050 | +0°68 | +0°78 92 REPORT—1898. Taste II.—Diwrnal Inequality of Horizontal Force from Hour | Midn. 1 | 2 | 3 | ft | 5 | 6 | 7 8 | 9 | 10 Including all days excepting those January. .|] + 4) +5] +9 | +14 | +33 | + 55] +57 | + 55] + 21] — 39) — 96 February «| + 38} +16 | +3 | +4 |] 415 | + 40|) 454 | + 45) + 7] — 68 | —-117 March . .| + 45/ +34 | +32 | +33 | +28 | + 35] +36 | + 6] — 64] —160 | —220 April . -| + 90) +73 +45 +35 +24 | + 27) +11 | — 35 | —114 | —222 | —300 May ‘ + 67| +48 | +28 | +14 | +1 | — 25} —61 | —127 | —198 | —245 | —253 June : + 66) +47 +30 +25 +17 | —18| —78 | —155 | —235 | —287 | —290 July . -| + 65 | +50 +35 +21 + 8 | —18} —70 | —141 | —220 | —281 | —303 August . .| + 95/ +84 | +59 | +49 | +38 | +, 4] —54 | —147] —248 | —319 | —322 September .| +100] +85 | +76 | +62 | +51 | + 51| +7 | — 61] —166 | —241.| —274 October . .| + 83 | +82 | +78 | +83 | +89 | +100] +86 | + 44] — 47 | —172 | —254 November .| + 41} +35 | 427 | 487 | +54 | + 70] +77 | + 65| + 7] — 80] —147 December ~-| + 5] +4 a +17 +35 | + 58) +73 | + 67 | + 51} — 9) — 65 Spring . + 56 | "+41 | 427 | 424 | +92 | + 34] 434 | + 5] — 57] —150| —219 Summer . -| + 66) +48 +31 +20 + 9 | — 20} —70 | —141 | —218 | —271 | —282 Autumn. ./ + 93] +84 | +71 | +65 | +59 | + 52 |) +13 | — 55 | —154 | —244 | —283 Winter . +17) +15 +13 +23 +41 | + 61} +69 | + 62] 4+ 26 | — 43 | —103 The Year .| + 58| +47 | +35 | +23 | +33 | + 32] +11 | — 32 | —101 | —177 | —220 From five selected quiet days in each month January . +12) +15 | +17 | +18 | +40 | + 53] +55 | + 47) + 17] — 43] — 94 February -| + 45 | +36 +16 +17 +20 | + 86] +39 | + 57] + 17 | — 59} —128 March . .|/ + 69| +54 | +43 | +34 | +24 | + 88] +42 | + 9] — 61] —163 | —212 April . + 86 | +482 +62 +44 +42 | + 43) +33 | — 4] — 82] —195 | —275 May 3 + 82} +61 | +37 | 422 0 |—19| —54 | —133 | —220 | —275 | —965 June . + 72} +449 +37 +36 +18 | — 14} —75 | —151 | —224 | —276 | —272 Tei! 9 e + 78) +63 | +39 | +30 | 424 0| —55 | —110 | —184 | —253 | —288 August . -| + 90] +77 +68 +55 +51 | + 17] —33 | —130 | —221 | —299 | —308 September .| +101} +77 | +64 | +40 | +35 | + 19] —29 | —101 | —183 | —257 | —263 October. .| + 63] +60 | +59 | +66 | +65 | + 73] +68-| + 37] — 35 | —144 | —295 November .| + 39] +41 | +37 | +38 | +56 | + 65| 475 | + 55] — 9 | —102] —173 December ./— 5] —11 | —14 | —6 | +9 | + 25] +446 | + 44] + 99] — 24] — 75 Spring . -| + 67'| +57 +40 +32 +29 | + 39] +88 | + 21) — 42 | —139 | —205 Summer. .j| + 77 | +58 | +38 | +29 | +14 | — 11] —61 | —131 | —209 | —268 | —275 Autumn. ./ + 8/ +71 | +64 | +54 | +50 | + 36] + 2 | — 65 | —146 | —233 | —265 Winter . «| +15) +15 +13 +17 +35 | + 48|} +59 | + 49 | + 12] — 56 | —114 The Year .| + 61] +50 | +39 | +33 | +32 | + 98/49 | — 32] — 96 | —174 | —215 Excess of the quiet days value Spring . -| + lly; +16 +13 | +8] +7/[+ 5) +4 ]+ 16); 4+15/+11]4+ 7 Summer . -| +11] +10) +7} 49/45 /)/+ 9] +9/]+10/ + 9/4 3/4 7 Autumn. -|— 8] —13 -—7 -11 —9}-—16}] -—11 | —10;} + 8} +11] 4+ 18 Winter. .|— 2 0 0} —6/}—6 }—18} —10 | —13}—14] — 13] —11 The Year -|+ 3] +3 |] +4 0}; —-1/;]— 4} —2 O;+ 5) + 3) 4+ 5 = ——_—— 7 = ee es a ON COMPARING AND REDUCING MAGNETIC OBSERVATIONS. Observations made at the Royal Observatory, Greenwich, 1890-1894. 11 Noon 93 | a | as | a | at | as | 39 | 20 |» | » | 2 of extreme magnetic disturbance. —112 ;}— 92 ;— 41; —8| +3 {[— 5) + Gy + 22) + 31) + 28) + 21) + 13) + 16 —139 | —109 | — 64] —20 | +15 | + 36] + 36] + 35] + 37) + 42] + 39 |) + 27] + 33 Eoigeii--iss | — 67) +7 | +48 | + 54 | + GL) + 77) + 86) + 90) +7) + 66 | + 73 —297 | —209 | —111| —25 | +45 | + 94 +118 | +134 | +143 | +137 | +124 | +109 | +104 —21g | —146 | — 77] —7 | +48 | +106 | +161 | +199 | +191 +167 | +133 | +105 | + 89 —245 | —170 | — 84] +1 | +79 | +128 | +178] +210 | +220 | +194 +154 | +118 | + 95 —970 | -177 | — 89| —2 | +77 | +127 | +169 | +210] +216 | +199 | +159 +129 | +106 —971 | —171 | — 60] +19 | +69 | +102 | +127] +159} +180 | +171 | +162) +146 | +128 246 | —133 | — 45] +8] +30 | + 33] + 50] + 83 | +114| +113} +101 +103 | + 99 —260 | —204 | —123| —57 | —17 | — 5| + 24] + 58) + 72| + 84) + 88 | + 86 | + £2 —162 | —128 | — 77] —44 | —22 | + 3] + 25] + 31 | + 33] + 33] + 42 | + 42] + 38 ea = 87 .| — 65)| =28 | —18)||— 1 | ee 842 10} 4 | 8) re 8 —918 | —157 | — 81| —13 | +36 | + 61| + 72| + 82| + 89/ + 90} + 78| + 67} + 70 —o44 | —164 | — 93] — 3 | +68 | +120 | +169 | +206 | +209 | +187 | +149 | +117} + 97 —959 | —169 | — 76] —10°| +27 | + 43 | + 67 | +100 | +122 | 4123 | +117 | +112 | +103 —124 | —102 | — 58| —27 | —12 | — 1] +13] + 21/ + 2 + 21 | + 22 | + 19} + 21 —211 | —148 | — 74] —13 | +30 | + 56 | + 80 | +102 |'+111 | +105 | + 91 | + 79 | + 73 after elimination of the non-cyclic increment. —132 | —108 ;— 60; —19); —6)— 2) +19 —158 | —139 | — 96| —38 | —7 | + 9| + 27 —212 | —161 | — 77| — 8 | +44 | + 38| + 36 —276 | —217 | —132| —49 | +26 | + 66) + 89 —201 | —144 | — 65] + 8 | +60 | +120) +152 —243 | —155 | — 80| +11 | +94 | +113 | +146 —260 | —189 | —103 | —11 | +70 | +122/ +152 —262 | —163 | — 60| +24 | +78 | + 96 | +106 —207 |— 83 | + 8] +51 | +39 | + 28} + 43 —238 | —190 | — 99| —41 | —8] + 5] + 36 —178 | —154 | —106| —46 | — 5 | + 23| + 47 — 95 | — 83 | — 47] —10 O | + 21] + 44 —215 | —172 | —102} —32 | +21 | + 38) + 51 —241 | —163 | — 83| + 3 | +75 | +118) +150 —236 | —145 | — 50] +11 | +36 | + 43] + 62 —135 | —115 | — 71| —25 | —4 | +14] + 37 —207 | -149 | — 76 | —11 |] +32 | + 53] + 75 above the all days value. + 3 )—15 | — 21) —19 | —15 | — 23| — 21 a 0} +6) +7|- 2;-19 +23 | + 24 | +26) +21 | +9 ON so —-ll |-13 |—13/ +2] +8) 415] + 24 + 4/- 1 {—-— 2] +2 +2{— 3}—-— 5 94 REPORT—1898. Tas.e III.—Diwrnal Inequality of Vertical Force from Hour | Midn. 1 | 2 | 3 | 4 5 | 6 | 7 | 8 | 9 | 10 Including all days excepting those January. .{ —20 | —25 { —33 | —34 | —37 | —33 { —27 | —18 | —13 | —22 | — 21 February .| —15 | —31 | —38 | —34 | —29 | —22 | —26 | —25 | —10 | —19 | — 52 Mareh , .| —33 | —45 | —48 | —44 | —41 | —23 | -17 | + 5 +12 | -—23 | — 71 April . .| —8 | —28 | —34 | —32 | -20 | —8] +8 | +31 | +22 | —29 | — 91 May ; +4 | —14 | —18 | —i6 | + 2} +14:| +18 | +11 | —19 | —78 | —148 Tune’ . -| —5 | —15 | —95 | —21 | —4 417 |, +18 | +13 | —17 |, =69 4} —190 July . «| —20 | —40 ) —46 | —37 | —16 | 411 | +20 | +17 | —2 | —47 | — 93 August . .| —20 | —40 | —43 | —35 | —19 | +2 | +19 | +39 | +28 | —22 | — 78 September .| —28 | —44 | —55 | —62 | —51 | —45 | —33 | — 2 | —10 | —48 | — 83 October. .| —28 |, —41 | —52 | —55 | —59 | —52 | —42 | -19 | —1 | —14 | — 47 November .| —18 | —29 | —42 | —42 | —42 | —41 | —35 | —29 | —20 | —298 | — 44 December .| —22 | —34 | —39 | —36 | —31 | —20 | —23.]| —12 | —7 |} —11 | — 20 Spring . .| —19 | —35 | —40 | —37 | —30 | —18 | —12 | +4] +8 | —24 | — 71 Summer. '.| —7.| —23 | —30 | —295 | —6 | 444 | +19 | +14 | —13 } —65 |'—190 Autumn. .| —25 | —42 | —50 | —51 | —43 | —32 | —19 | +6 | +6 | —28 | — 69 Winter . .| —20 | —29 | —38 | —37 | —37 | —31 | —28 | —20 | —13 | —20 | — 28 mpeavear «| 18 [eae |emag | 2870 eens etrmler=10 4° 4 1 | cuas| ssaeeleeze From five selected quiet days in each month January . -| —16 —21 |,-—31 | —25 —24 —22 —19 —10 +2/!+3j)+ 3 February .| —7 | —30 | —35 | —24 | -—10] +4 0} +2) +20, +7 | — 22 March . .| +4/—8|—8]—21] +45 | 419 | +19 | +42 | +36 | —13 | — 65 April . .| +9|+9)|}—6] +7] +18 | +27 | +33 | +59 | +49 | — 4 | — 62 May . «| +24 | 428 | 423 | +28 | +43 | 450 | +48 | +40 | +6 | —63 | —139 June - «| +18 | +10 | +15 | +18 | +27 | +47 | +44 | +89 | + 6 | —57 | —103 July . _.}| +17 | 411 | +4 | +10 | 430 | 455 | +51 | 451 | 421 | —18 | — 75 Auguss . .| —14 | -11 | —9]—3]| 47 | +24 | +43 | +69 | +58 | — 4 | — 60 September .] +23 | +5 | +7 | +4) +11 +17 | +18 | +35 | +12 | —34 | — 89 October . Area —7 —14 —19 —20 -l7 —8|+6 +13 | —4 | — 55 November .| —16 | —19 | —19 | —21 | —le | —4 | —2 | +3] +419 / io} 16 December .| —24 —25 —23 Pale —11 +6 — 6 +38 +3 — 4 | — 15 Spring . .| +2 | —10 | —16 | —6 | +4 | +17 | +17 | +34 | +35 | — 3] — 50 Summer. .| +20 | +16 | 414 | +17 | +33 | +51 | +48 | +43 | 411 | —46 | —106 Autumn. 5 0 —4 —5 —-6)-—1 +11 +18 | +37 +28 —14 | — 68 Winter . .| —19 | —22>| —24 | —19 | -—17 | —7} —9|]—1|]+8)] +4]/— 9 i The Year -} t+1{—-5 | —8{—4 | +5 | 418 | +18 | +28 | +20 | —15 | — 58 Excess of the quiet days value Spring . . | +21 +25 ) +24 | +31 ) +34 { +35 |] +29 | +30 | +27 ) +21 | + 21 Summer . |. #27 +39 +44 +42 +39 +37 +29 +29 +24 | 419 | + 14 Autumn. | +25 +38 +45 +45 +42 +43 +37 +31 +22 | 414-1) 4 1 Winter . «| +21 | + 7)" | +18 | +20) Gp24 | Spa9 | +18] +21 | Span eee — The Year .| +19 | +27 | +31 | +33 | +34 | +85 | +28 | +27 | +93 | +19 | + 14 ON COMPARING AND REDUCING MAGNETIC OBSERVATIONS. 95 Observations made at the Royal Observatory, Greenwich, 1890-1894, | 11 Noon 13 14 | 15 | 16 | 17 | 18 | 19 20 21 | 22 23 of extreme magnetic disturbance. ’ — 16) — 26, — 7) +27 +43 | + 53) + 53) + 50) + 47|/ + 37) +21 +7 — 6 | — 61| — 59| — 32| +7 +448 | + 70| + 75] 4 74| + 69| + 58] +37 +13 + 2 —112 | —117! — 76} +11 454 | +101 | +121 | +112 | +103 | + 78| +58 +28 —-11 —150 | —172 | —132 | —48 +23 78 | +118 | +133 | +120 | + 95 | +70 +40 +14 + —198 | —198 | —137| —59 | +12 | + 73 | +124 | +156 | +153 | +126] +95 | +64 | +33 —169 | —167 | —116 } —48 | +12 | + 75 | +118] +136 | +134 | +109] +76 | +45 | +23 + + =146 | —153 | —121 | —51 | +20 77 | +128 | +144 | +131 | + 99] +63 | +45 | +17 = 194) —192 | — 84) —15 4) -+-51 95 | +109 | +105 | + 82| + 56] +29 | +5 | —18 = 1087] ‘—102 | — 51 | +17 +77 | +119 | +131 | +122 | +107) + 85 | +57 +17 —15 — 78| — 63 | — 23| +25 | +82 | +110 | +107) + 92] + 84] + 61 | +36 | +2 | —25 —'45|—28| + 3) +41-| +70 | + 82| + 74] + 68] + 58| + 43 | +23 0\)| z=19 =17)=— 5| +4 4]. +297 | +46 | 4+ 52) + 47 | + 42 | + 32) + 26) +16 |] +1 | —16 —108 | —116 | — 80! —17 442 | + 83 | +105 | +106 | + 97 | + 77 | +55 +27 +2 —171 | —173 |.—125 | —53 | +15 | + 75 | +123 | +145 | +189 | +111] +78 | +51 | +24 —102 | — 96 | — 53] +9 | +70 | +108 | +116 | +106 | + 91| + 67 | +41 | + 8 | —19 = 26) = 20) o|.+32 | +53 | + 62] + 58] 4+ 53] + 46 | 4+ 35] +20 | +3 | —14 | —102 | —101 — 64} —7 | +45 | + 82] +100 | +103 | + 93) + 73:| +48 | +22 | — 2 after elimination of the non-cyclic inerement. ae P= 10 0} +25) +40 ) + 88; + 30; + 28; +18) +15) —47 —8) —5 dB) — 42+} — 23] — 2 | 482°) 4-40 | + 88) 4 29} 18] 418) +13 | +0 | +1 —123 | —146 | —109| —45 | +31 | + 70| + 69] + 63] + 47 | + 45] +35 | 423 | +11 —132 | —160 | —136| —59 | +6 | + 41| + 60| + 66] + 59] + 50] +34 | +25 | +7 —200 | —213 | —146 | —61 | — 3 | + 54| + 93] 4106] + 91] + 70] +55 | +35 | +31 _ | 168 | —ies | —123 | —63 | —10 | + 39] + 71 | + 91] + 84] + 77| +46 | +37 | +28 —143 | —179 | —148 | —74 | —29 | + 31 | + 76 | + 88] + 78] + 56] +44 | +26 | 417 —109 |;—120 | — 93 | —17 | +25 | + 49] + 59 | + 56 | + 32/'+ 17) +10 | —5 | —14 —128 | —129| — 85| —37 | +14 | + 40| + 49] + 50] + 54] + 55] +48 | +33 | +427 — 89| — 82; — 55| —13 +32 | + 63 | + 61] + 52 | + 49] + 43] +433 +26 +13 Prag 97 | — 4) +98 | +35 | + 321 4+ 35) + 21) 410) + 9) —6) —8) —5 —11}/— 5|+ 9} +22 +29 | + 37 | + 31] +17) + 13 o| —8 —8 —19 — 98| —116 | — 89| —35 | +23 | + 50] + 56] + 53] + 41] + 38] 427 | +20 | +6 —170 | —187 | —139 | —66 | —14 | + 41| + 80} + 95] + 84] + 68| +48 | +33 | +25 —109 | -110 | — 78 | —22 | +24 | + 51} + 56] + 53] + 45] + 38] +30 | +18 | +9 — 20) —14| ¢ 2] +95 | +35 | + 36] + 32/422) 4+.14|/+ 8} —6} —8] —10 aon! - — 99 | —107 | — 76 | —25 | +17 | + 45| + 56] + 56] + 46/ + 38] +25 | +16 | +8 above the all days value. + 10 0) — 9) —18 | —19 |] —33 | — 49) — 53; — 56 | — 89| -—28) —7) +4 + 1) — 14} —14}) —13 | —29 | — 34] — 43 | — 50] — 55 | — 43 | —30 | —18 | +1 — 7| — 14} — 251) —31 | —46 | —57 | — 60| — 53} — 46) — 29] —11 | +10 | +28 + 6)'+ 6) + 2] —7 } -18 | — 26 | — 26-| — 31} — 32] — 27} —26 | —11}] +4 +) 828 Gil, —18 We 18 ~23 | — a1 |— 4 =—o4g i Seay sp | 9 4 "6" ||) 210 96 REPORT—1898. _ Taste TV.—Diwrnal Inequality of Declination and Horizontal First Quarter . Second Quarter Third Quarter. Fourth Quarter The Year. First Quarter . Second Quarter Third Quarter. Fourth Quarter The Year. . First Quarter . Second Quarter Third Quarter. Fourth Quarter The Year. > First Quarter . Second Quarter Third Quarter. Fourth Quarter The Year. . First Quarter . Second Quarter Third Quarter. Fourth Quarter The Year. : First Quarter . Second Quarter Third Quarter. Fourth Quarter The Year. (After elimination of the Jmia.| 1 | 2 s[e[s |e fa|e fo | w Declination, , 7 v y / , / ‘4 / / / —1:33 | —1:18 | —0:97 | —0-94 | —0°94 | —0:89 | —1°11 | —1°52 | —2-12 | —2-11 | —0-93 —0°67 | —0:76 | —0:94 | —1:21 | —1:75 | —2°66 | —3:76 | —4:58 | —4:80 | —3-77 | —1°45, —0°91 | —1:08 | —1:30 | —1-67 | —2:07 | —2:94 | —3:88 | —4-41 | —4°31 | —3-06 | —0°51 —1:30 | —0:93 | —0-77 | —0°67 | ~0°61 | —0:81 | —1-04 | —1-31 | —i-86 | —2-00 | —0:87 —1:05 | —0:99 | —0°99 | —1-12 | —1:35 | —1:82 | —2:45 | —2'96 | —3-27 | —2°74 | —0:94 Declination, —1:28 }—1-18 )—1:02 | —0-97 | —1-03 ; —1-:09 | —1-26 | —1°67 } —2:31 | —2:26 | —0-86 —0°66 | —0:78 | —0-97 | —1-23 | —1-84 | —2:89 | —3:88 | —4:74 |\—4-93 | —3-84 | —1-25 —0°99 | —1-11 | —1:34 | —1°67 | —2°18 | —3-04 | —3:95 | —4°53 | —4-48 | —3-04 | —0-29 —1:26 | —0-90 | —0-76 | —0°69 | —0-75 | —0-83 | —1-12 | —1-41 | —1-97 | —2-11 | —0°86 —1:05 | —1:00 | —1:02 | —1:14 | —1-45 | —1:96 | —2:55 | —3-09 | —3-42 | —2-81 | —0-82 Lacess of Declination +0:05 | 0:00 } —0:05 ; —0:03 } —0:09 ; —0:20 | —0:15 | —0°15 ; —0-19 | —0-15 ) +0:07 +0:01 | —0:02 | —0:03 | —0-02 | —0-09 | —0:23 | —0-:12 | —0-16 | —0-13 | —0-07 | +0:20 —0°08 | —0:03 | —0-04 | 0-00 | —0-11 | —0:10 | —0-07 | —0-12 | —0-17 | +0:02 | 40-22 +0:04 | +0:03 | +0:01 | —0-02 | —0-14 | —0:02 | —0:08 | —0-10 | —0-11 | —0-11 | +0-01 0:00 | —0:01 | —0:03 | —0-02 | —0:10 | —0:14 | —0-10 | —0-13 | —0-15 | —0-07 | +012 Horizontal Force, + 42)+ 35) + 25)4 23/4 28)4+ 42/4 45/4 38;-— 9 )— 88)—145 + 80/+ 64/+ 45/4 34/4 20/+ 3]— 32/— 96 |—175 | — 249 | — 271 + 90|+ 72)+ 57|+ 42|+ 37])+ 12]— 39 |—114 |—196 | — 270 | — 286 + 32/+ 30/4 27/4 33/+ 43/4 54/4 63/+ 45/— 5|]— 90]—158 + 61/+ 50/+ 39/4 3314 3214 28/4 91-— 32|— 96 }—174 | —215 Horizontal Force, + 34)+ 26/;+ 25)+ 26)+ 36)4 56/+ 59)+ 55)4+ 12)— 65 )—197 + 74/4 66)+ 53/4 52/4 43/4 34/— 1]— 56 |--139 |—216 |—258 +°75|)+ 74/+ 59])4 57/4 49/4 30/— 14|— 82 | —166 | — 242 | —977 + 29/+ 28/+ 30/4 40/4 53})+4 68/4 74/+ 57/+4 10]— 70|—145 + 53/4 49|+4+ 42])4 44/4 45]4 4714 29/— 6|/-— 71 !—148 |— 202 Excess of Horizontal Force - 8;— 9 O;+ 3);+ 8)+ 14)+4+ 1444+ 17)+ 21)4 23)4+ 18 — 6/+ 2)+ 8/4 18}+ 23/+ 381]}4 31])/4+ 40/4 36/4 33}+ 13 — 15/+ 2/+ 2/+ 15/+ 12/4 18]+ 25}+ 32/+ 30/4 28/+ 9 — 3/— 2/+ 3/+ 7]4+ 10]}+ 14]+4+ 11] + 12/4 15]+ 20]4 13 — 8/— 1)/+ 3)/+ 11/4 13]4 19}+ 20/4 26/4 25/4 26)4 13 ——————— ss Sr ON COMPARING AND REDUCING MAGNETIC OBSERVATIONS. 97 Force at Greenwich and Kew on Quiet Days, 1890-1894, compared. non-cyclic increment.) m fron] a |u| | wf || oi» | a | » ee Ee a nee Greenwich. 41°84 | 44:27 | 45°35 | 44-90 | +3°59 | +2°01 | +0°84 +0:22 | —O11 | —0°38 | —0°60 | —0:73 | —0:91 at Kew. 40:04 } +011 } +0°17 | +014 ) +018 40°11 ) +0:04 ; —0°04 | +0:01 ; +0°03 0:00 | +0°03 } +0:05 40°15 | +0:23 | +0-29 | +0:21 | +016 | +0:04 —0:07 | —0-08 | —0:08 | —0:07 | —0:08 | —0:03 0:00 40:25 | +0°34 | +0°43 | +0°26 | +017 0:00 | —0-08 | —0-12 | —0-16 | —0'14 | —0-11 | —0'17 | —018 +0:09 | +015 | +0:25 | +013 | +013 | +0°09 0:00 | —0:04 | —0:04 | —0:09 | —0°10 | —0°08 | +0:01 +012 | +0°21 | 0-29 +018 | +016 | +005 | —0:03 | —0:07 | —0-07 | —0-06 —0°07 | —0:06 | —0-04 Greenwich. mig7 |—136 )}— 78|— 22|+ 10)+ 15)+ 97 )+ 46|/+ 61)+ 66)+ 54)+ 42 )+ 44 — 247 |—172|}— 92]|— 10/+ 60]+100 4129 | +157 | +167 | +149 | +131 )+ 111 |}+ 94 — 243 |—145|— 52/+ 21/+ 62)+ 82 +100 ! +132 | +154 | +145 | +132 }+ 107 |+ 99 —170|—142|— 84/— 32/— 4)+ 16/+ 42)+ 55]+ 64|/+ 59/+ 47/+ 36 |+ 38 Ken Saeias )— 74 ;— 3L;— 4)+ 2)4+ 9) 35 y+ 50; + 49;4+ 42)+ 33 ;+ 35 — 244 |—176|]—104|}— 32|/+ 32/+ 69 4105 | +129 |} +143 |+126|/+114/+ 99 [+ 86 — 236 |—148 |— 66] + + 43/4 64/4 89/4119 |+134]/4+126)+121/+ 94 | + 95 —160 |—137|— s7}— 44]/— 17}/— 4]4 28|+ 43 )4+ 52) + 45/+ 39/4 34 |+ 35 at Kew. + 12)+ 81+ 4}— 9)— 14)- Lope 1S ee en, |e 1 8 8 + 8/— 4]/— 12|/— 22|— 28)— 31)/— 24)/— 28/— 24)/— 23/-— 17/— 12 |- 8 + 7T/— 38|— 14/-— 18|— 19|—- ig |— 11 }— 13 |— 20|/— 19j)— hj— 13 )—. 4 + 10}/+ 5/— 8i— 12)/— 13)— 20\/— 14)/— 12|/— 12)/—- 4/— 8/— 2/-— 3 + 8i+ 2/— TI]— 1]- 19 |}— 20}/— 17|/— 16)— 17)— 18)—- wi- g9/— 6 | 98 . REPORT—1898. TaBLe V.—Diurnal Inequalities at Greenwich and Kew on quiet days (As observed, no correction for non-cyclic Hour | Midn. | 1 2 | 3 | 4 5 | 6 | 7 | 8 | 9 10 Declination. ' March— i / / ’ i / ’ ' , ’ Greenwich .| —13] —Il1 —07) —11{] —16} —15] -18] —28|] —44] -—44}] —217 Kew . -| —l2}] —10] —11] —10] —16] —1:5] —19 |] —28] —44] -—45] —2:5 ExcessofKew | +01 | +01] —04] +01 0-0 00 | —01 | 0-0 0-0 O1| —04 June— Greenwich .| —03 | —04/ —10| —13 |] —24] -—35|) —48 | —51/ -—49] -—3:9 |} —1-7 Kew < -}| —03) —05} —09 | —17] —23] —36 |] —49) —56} —50] —37| —16 Excess of Kew 00} —O1} +01] —04) 401] —O1);) —U1| —65} —O1] +02! +01 September— Greenwich .} —16] —19] —16} —15] —14] —18] —25 |} —32] —31] —20 0-0 Kew « .| —23/ —23 | —23 |] —21] —25 | —26 —32 | —42 | —41] —26)} 401 ExcessofKew | —0'7] —04| —07|) —06 | —11]} —08! —07! -—1:0] -—10] —06] +01 December— Greenwich ./| —05| —06] —05} —06 |} —05 |} —07| —08| —09 | —11] -—13 |] —06 Kew = -| —O7}) —05) —05 | —05 | —05 | —07 | —0-'9 | —1:0] —11] —14] —64 Excessof Kew | —02 | +01 00 | +01 00! OO}; —01, —O1; OO] —0O1]| +02 Horizontal Force. March— | | Greenwich + 6 A | Pee) ere eee 3 | + 3/41|—7] -17| —24 Kew. -| + 6] + 3} + 3] + 3] + 3] + 5) + 6) + 4] — 3] —13] —22 Excess of Kew 0; -1 Oo; +i1)4+1 Bab eG ot) ess) eee 2 June— | . Greenwich 6/ +7 6 7) +1] — 2! — 8} —17!] —25|] —29|) —33 Kew 5 -| + 5] + 4] + 5] + 4} + 38] + 2] — 5} —12] —20 29| —34 Excess of Kew 1) —s38 ) = 1) = ssa oie a 4 8] + 8] St 0; -1 September— x Greenwich +11 4) +5) = 5) eee oy 1 — 6] —18] —28} —28 Kew 4 -| +10) £7) + 6] +5) +5] +°5 Oo}; —*6 | —18 |}-—27 | -— 29 ExcessofKew | — 1 Oo; +1 0 1 0};--— 1 0 oj; +4i1;};=-41 December— | | Greenwich .| + 2/] + 1 Oo{|—1,],+1)] + 2! +2!) 41) —1}]—7)] — Mow jf. vs Oo; +1) —1)]—1)] +1] + 2] + 2) +1] — 1] — 4] —10 ExcessofKew | — 2 0}; —-1 0 0 0 0 | 0 0 3 uf Vertical Force, March— | | : Greenwich +1]/-1/]/—1]—8 3/ — 1] 4+ 1) + 6| + 5] — 2] — 8 corr eet. | b= 1 0 Oj; +1} 4+ 2) + 3) + 5) + 7} + 5 Oo; —§ ExcessofKew | — 2} + 1|/ +1] + 4 DME sy pe 44) o|; + 2 0 June— | Greenwich -} — 1|/-— 2) — 2} — 2) —9 0 3); + 5; +2} —1]—7 Kew cigs sees 00 2) ts eae eat ee) 4 B53 eect Ol 7 ExcessofKew | + 1 0o|-1 Oo; + 1] + 1; 1 0o';—1)/441 0 September— | ; Greenwich 2 0 1 1 2) +1] 4+ 2) + 4/ + 2} — 2) —10 Kew, nfo 6) — 5) —- 4) — 35 =F owe —fo4 0; + 2] 0), = 44) -—F0 ExcessofKew | — 8} — 5] — 5| — 4 4/—3}] — 2}; — 2] — 2} — 2 0 : / | December— | PF Greenwich 2 1 2 0 i 0 0 0 0] +41 0 Kew. ~-| — LJ —1],—1]-1 —1}—-— 2; —2 2} — 1) — 27) — 2 ExcessofKew | — 2| — 2 3/—1 Pe a a = J — ‘yaa ee In this Table the Values of Horizontal and ON COMPARING AND REDUCING MAGNETIC OBSERVATIONS. 99 eee mpared, for the Equinoctial and Solstitial Months of the Year 1894. increment being here applied.) . Noon 13 | 14 | 15 | 16 | 17 18 | 19 20 21 | 22 23 Declination. , vy ’ ’ , / , / , / i , , 415 | +40] +59] +55] +38] +20] +09] +05] +03] —02] —04 —07 —0:9 41:1 | +46] +61) +5:°9 | +42] +21 | +09] +05 | +04 00} —02| —04 —0'8 —04/] +06] +02) +04] +04) +01 0:0 00} +01] +02] +02 +03 +071 410] 43°83} +52] +49 | 442] 437] +21] 41:5] +08] +0°7 |] +09 +08 —10 411} +41] +59] +450] +43] +36] +20] +14] +09] +06 | +06 +0°6 —10 +01] +03] +07] +01] +01] —O1} —O1] —O1] +01] —O1] —03 —02 0:0 428) 449] +57] +48] +33] 421] 403] +04] —03] —05 | —06 —0'8 —12 +36 | 45:9] +74] +60] 43:7] +21] +07] +03 00 | —0-4| —03 —0'4 —0°9 +08) 41:0] +17) +12 | +04 00 | —O1} —O1} +03] +02} +03] +04 +0°3 +07 | 41:3 | 42:2] 426] +21] 41:2] +08] +04 00 | —O1 |] —O04 —l1 —12 +07 | 41:7) +26 | +26] 42:2] +12] +05] +02] —O1) —05 | —07 —10 —1°0 00 | +04) +04 00 | +01 00 | —03 1 —O2 1 —O1] —O4 | —O3| +01 +02 Horizontal Foree. —25|} —19|] — 9 o; +5] +7] + 8{ + 9} +10] +01 +10 + 8 +10 aa — 18 | — 9) — 3) + 2] + 6] + 41.4 7] +7) + 8) + 7 +7 + 9 +1/+41 0; — 3} — 3] — 1] —- 47 —.2/ =] 3] — 3] — 3] -— 1 -—1 ‘ —33| —25| —20| — 9] +11] +20] +20] +23) +27) +23) +18 +18 +14 ‘ —30| —21/ —11} — 3] + 7| +16] +18] +22] +22 )'°+18) +16 +14 + 9 3) 4/ +9 6; —4]/—4]/—-—- 2};—-—1} -—5 5 D} 4 — 5 | —25| —14/| -— 3 0 2) + 3) + 6] + 9} +11] +15) +14 +11 + 9 —24} —16} —5| — 4; — 2 oOo; + 4] +10] +13) +15] +15) +15 +14 t}—2|/—- 2); —# 4); -— 3] - + 1] + 2 Oo; +1 + 4 + 5 -13 12}; —6;-1 1 5 9 8 7 7 3 0 + 1 —10 TyTN te ERIE Nie SSR ie Soe ale ao ee Ce We + 1 + 2 +3|+ 2 0o| —2!|-—- 3] -— 3 4,—-1/1—-1] -—11!--1 +1 +1 Vertical Poree. —13 15| —11 2 5) +7 6} + 6 4 6} + 6) + 5 +2 —aaie—de | — §| — 3) + 3] + 6| + 5} + 3] +2) +2 0 0 0 Oo); +1] + 3 1f— 2) —1] = b} = 3] —|2 5} — 6 -— 5 — 2 —14/ -13}| —11 6 Oo} + 6) +7) +11) +11 8/ 4+ 5 5 — 1 Ae eee) SS he Le Te] OP EO fe) OP ee TP eS + 2 + 1 ieronmeeraa oS tok Dy be Bf = 2] — ill — 2 -— 1 + 2 17} —15/} —10 4) +3] + 5| + 5| + 5] + 6 8| + 6 3 + 3 =—15} —11)—6)/— 2| + 3| #7] + 8] 4-7/4 Th 4+ 7] +7 +7 + 7 2 4|/ +4 2 Oe: Si se Suh EBs Dea) 4 1 4 + 4 + 3] + 3/ + 3) + 3] + 3/ + 3 Oot = 3} — 4} — 5] — 5] — 4 — 6 —-1/-1 O} +2) + 3] + 4] + 2] + 1 Oo} + i{+ 1 +1 + 2 —4/]/—4/—3)-1 Oo; +1/+ 2] + 4) + 4 G6} + 6 + 5 8 Vertical Force are in c.g.s, measure x 10°. ; H2 100 REPORT—1898. Taste VI.—-Diurnal Inequalities and Diurnal Range at Declination Sums of Hourly Diurnal Range Values of Diurnal Inequality (corrected er mga rae Greenwich Kew Month or Quarter Cor- Cor- K-G pected rected as As Ob-| _ for As Ob-| for made pene Kew |K-G sa ealis a-b one pes a—b | Cyclic Incre- Incre- ment ment b , t t ' ' , ’ ’ , ’ January a . | 28°24 | 29°52 |+1:28] 4:98 | 4:78 |}+0:20| 5:22 | 4:99 |4+0:23/)+0-21 February : . |34:56 135-95 41:39] 5°54 | 5-41 |+0°13| 5-72 | 5-64 |+0:08/+0-23 March . : . |45°60 | 47-58 |4+1:98| +944 | 9:36 | +008] 9:78 | 9-73 |+0:05|+0-37 April. 3 . |48°68 | 51°45 |4+ 2°77] 10°78 |10°76 | +0-02/ 11°30 | 11-26 |+0:04|/+0°50 May 5 = . |58:02 | 59°32 |+1:30) 11°70 | 11-62 |+0-08) 12-00 | 11-93 |+0:07}+0°31 June. : . 158-02 | 59:26 | +1:24)10°76 | 10°76 0:00} 11:18 {11-25 |—0:07|+0:49 July 5 : . |58:20 | 57-46 |—0-74} 11°30 | 11°36 |—0:06 | 11:18 11-29 —0:11|—0°07 August . ; . {5712 |60°14 |+3°02}11°38 |11-48 |—0°10/ 12:16 |12:23 |~0-07|4+0°75 September . . |50°18 | 55°04 14486} 9°50 | 9:56 |—0-06| 10°50 | 10-47 | +0:03|+0-91 October . : . |43°68 | 45°48 |+1-80| 7:94 | 7:94 0:00} 8:54 | 852 '|+0-02/+0:58 November. . |30°92 | 32:59 |+1°67] 5°60 | 5:58 |+002| 5:92 | 5-88 |+0-04/+0°30] December . . | 22:82 | 24:03 | +1:21| 3°98 | 3:80 |+0:18} 4:02 | 3:97 |+0:05|+0:17 First Quarter . |36:13 |37°68 |4+1:55) 665 | 652 |+0:13| 6-91 | 6-79 |+0:12|+0-27 Second Quarter . |54:91 |66°68 |+1-77| 11-08 |11:05 |+0-03| 11-49 | 11-48 | +0-01]+0-43 Third Quarter - |55°17 | 57-55 | + 2°38] 10°73 | 10°80 |—0-07| 11-28 | 11:33 |—0-05|+0°53 Fourth Quarter . | 32°47 | 34:03 e 1:56] 5°84 | 5°77 |+0°07| 616 | 6:12 |+0-04/+0:35 Mean. ° - {44°67 | 649 |4+1°82) 857] 853 |+0:04] 8:96 | 8-93 | +0:03}+0-40 ' : ON COMPARING AND REDUCING MAGNETIC OBSERVATIONS. 101 f Greenwich and Kew on Quiet Days, 1890-1894, compared. - ass. SS....88808 SS. ee Horizontal Force Sums of Hourly Diurnal Range Values of Diurnal Inequality (corrected aids a | for Non-cyclic Incre- Greenwich Kew Month or Quarter Cor- Cor- K-G reored ie as As Ob-| for As Ob-| .£°F made served| Non- | g_% |servea| Nom- | a—o | Cyclic cyclic %. cyclic Incre- Incre ment ory 187 | +10] 172} 180} -—8]| —7| January 230 | +20| 214] 205] +9 | —25 | February 298 | +9]| 290] 282] +8| —16| March 405 | +13 | 386] 381} +5 | —24 | April 449 | +17} 428] 411 | +17] —38 | May A77 | +11 | 484 | 429} +5 | —48 | June 465 | +6] 444] 436 | +8 | —29 | July 476 | +15 | 450} 433 | +17 | —43 | August 381 | +14 386 | 372 | +14] -—9 | September 319 | +30] 332] 317 eC 15 | —2 | October 253 | +11 | 234) 245] —11 —8 | November 146 | 141 +5 |) 140; 142 —2 +1 | December 51) 238 | +13 | 225] 222 +3 | —16 | First Quarter 457 | 444] +13] 416} 407} +9 | —37 | Second Quarter 253 | 238 | +15 | 235| 234] +1 | —4 | Fourth Quarter 452 | 441 |] +11 427 414 | +13 | —27 | Third Quarter 2045 | 1893 | —2 353 | 340] +13] 326] 319 +7 | —21 | Mean | 102 REPORT—1898. Taste VII.—Won-cyclic Increment at Greenwich and Kew on Quiet Days, 1890-1895, compared. Declination Horizontal Force Vertical Force | : $ s Month Non-cyclic | Number of Indi- |} Non-cyclic | Number of Indi- Non-cyclic Number of Indi- Esgartes Increment | vidual Months Increment vidual Months Increment vidual Months Green- Green- Green- Green- = Green- Green- ah Kew righ Kew wich Kew Th Kew at Kew Shin Kew é ' |+ o —-l4+ o = + o—|/+ oF + 0-|+ o- January ./+047/+0°63! 4 0 216 O Ol] +53] +4501/6 00/5 01 —4 -—52 |}3 0 3/0 0 6 February . |+0'45|+0°33| 4 0 2/4 0 2/| +63] +57/5 01/5 1 0 —44 +5/0 06/3 0 3 March. |+0:27/+918/ 3 3 0}3 O 3) +34] +2815.01]/]5 1 0 —45 +13 ||) 0 5 12 3 2 April -|4+017/4+012)4 1 118 1 2)) 4451 420/5 0 1/4 11 —4 —22;2 04/2 0 4 May. + |+013/+0°07/ 3 0 3)3 0 3]| +39] +388/5 01/5 1 0 —4 —12/22 2/3 0 8 June. - {+0°05/—0°17/} 4 0 233 0 3i] +27] +22/5 0 1/4 11 —20 —-28 ;1 14/1 0 5 July. —015|—0°23/ 2 1 3/3 0 3]/ +31] +27)/4 0 2/4 2 0 +6 -—13 |3 0 3/1 0 5 August . |—0°35/—0°30} 1 1 4/1 1 4]} +34] 4371/6 00/5 0 1 -—9 —-8/1 2 3/38 03 September |—0°33}+0:12} 2 0 4/3 0 3]/ +38 | +38/5 01/6 0 0 —14 +30 |}2 22/383 1 2 October . |—0:20/+0:03| 1 0 5/2 1 3i| +69] +50/6 00/6 0 0 —12 +65 | 2.1 3 138 O83 November |+0:13}+018/ 3 1 2/3 1 2] +60] +53/5 01/6 00 —44 —19 | O 2:5 1208 December. |—0:27|—0°10} 1 0 5)1 2 3] +293} 415/5 01/5 01 —34 —6/]10 5/2 038 1st Quarter |+0-40 |+0:38 — — +50 | +45 = = —31 Sah a = 2nd Quarter | +012 |+0-01 — —_ +37 | +27 = = —i 9) oe = = 3rd Quarter |—0°28 |—0-14 — — +34] +84 = =s 6 “fs = aes 4th Quarter |—011/+0:04) — = SEDI E39) ee SS 230" | ens on Mean + |+0°03/4+0:07; — — +43 | +36 = — —19 | —8 = _ Totals of ; Months .| — | — |32 7 33/35 6 31) — | — |e2 010/60 7 5|| — — {18 9 45 [95 3 49% * The vertical force magnetograph at Kew was out of action in November and December 1890, reducing the months from seventy-two to seventy. Taste IX.—Non-cyclic Increment at Greenwich and Kew on Quiet Days, for Years, compared. Declination Horizontal Force Vertical Force ‘ Year z : Greenwich Greenwich Kew Greenwich Kew {| ’ 1890 — 0:23 +19 +23 —12 +15* t 1891 + 0°08 437 +23 Fe 12 | 1892 — 0:20 +67 +53 —39 —20 1893 + 0°15 +44 +40 —24 —26 1894 + 0°24 } +33 +33 —4 +12 1895 + 0°15 +57 +44 —27 —15 Mean PD: + 0°03 448 +36 —19 a8 * This value depends on ten months only. See note to Table VII. ON COMPARING AND REDUCING MAGNETIC OBSERVATIONS. 103 TABLE VIIL.—Won-cyclic Increment at Greenwich on Quiet Days, 1889—1896. Declination Horizontal Force | Vertical Force Non-cyclic Increment Non-cyclic Increment Non-cyclic Increment Difference Individual Months Greatest Monthly Value | Difference Individual Months Greatest Monthly Value Least Monthly Value | Difference Individual Months a Ron ek mR at 2 piee~ Tall ital te — ee SR a ys es S| nr w Ls) Bae GS OS Oo De). So) VO 2) o's: a 8 Fk ek ek eK Lr CO Le OD wD » | to ow Ist Garter 2nd Quarter 3rd Quarter 4th Quarter ere war oO +, oO woraanwr wo ow Nwnwnro ono *, N WD o of KF OY Fe & Totals of Months 38 10 48]; — 104 REPORT—1898, TaBLE X.—Won-cyclic Increment at Greenwich on Quiet Declination Month, Quarter, or Year | Preceding | Midnight | Noon to Neem | ASA | CE | keay=n| man P mm ' ' a ' ' xi ' January - - : —0:04 +0°05 +0716 +0:06 —0:01 February . : : +0°05 + 0:25 +0°40 +0:22 +003 March . é : —0°35 +0°25 +047 +0:06 +019 April . 5 —0°81 +014 +0°60 —0O11 + 0°25 May . ° = : +019 +013 +0°25 +0°22 —0:09 June . . ‘ : —0:28 + 0°04 +011 —0:08 +0:12 July . a ; : —0°31 —0°15 + 0°44 +0:06 —0°21 August . : : . —021 — 0°23 —0:04 —013 —0:10 September . 5 é —0:12 -031 +011 —0°01 —0°30 October - : 3 —079 —0:24 +031 —0:24 0:00 November . 5 : —0°12 + 0:06 +021 + 0:04 +002 December . ‘ ‘ —0°31 —0°28 +063 +0:16 —0:44 First Quarter : : --0°11 +0718 +0°34 +011 +0°07 Second Quarter . F --0°30 +010 + 0°32 +001 +0:09 Third Quarter. ‘ —0:21 — 0:23 +017 —0:02 —021 Fourth Quarter . i —0°41 -—0:15 +0:38 — 0:02 -—0:13 Mean : ; : — 0:26 —0:02 +0:30 + 0:02 +0°04 1889. : 5 : —0:22 -0O11 + 0:06 0:08 —0:03 1890. : : —0:09 —0:23 —0:02 — 0:06 -—017 MS91 5) - ; ; —018 +0:08 +0°49 +0715 —0:07 1892 2 “ 4 +001 —0:20 +045 + 0:23 —0:43 1893. : : . —012 +015 +036 +012 + 0:03 1894. ; : : —0°53 +0°24 +0°24 —015 +0°39 1895. ° Se rac —0°48 +0°15 +0716 —0:16 +0°31 1896. : . 5 —0:47 —0:27 +0°70 +012 -—0°39 ON COMPARING AND REDUCING MAGNETIC OBSERVATIONS. 105 Days, as variously determined, compared, 1889-1896. Horizontal Force Vertical Force Preced- | Midnight pret Preced- |Midnight |Noon to ing Noon| to Mid- | fl- | 4 (p+f)| ,_,, |ingNoon| to Mid- |, fol- ee : - 3 (ptf) to Noon | night | lowing to Noon| night |lowing| *°_,,° |™-” p m oon Pp Fp Noon +32 +30 | + 8 +20 +10} -—4 -— 1 —17| —Iil +10 +4 +58 +50 +27 +31 —15 — 48 —49 —32 —16 +45 +42 | 4 6/ +26 | +16) —45 —36 | -28| -37 | +1 +21 +52 +55 +38 +14 —27 + 8 —22 —25 +33 +61 | +48 Gara “| 41s) Rear Sof wae lie gl acs +29 +35 | +380) +380 | + 5] -—12 —14 | —33| -23 | + 9 - 9 +34 | +47] +19 | +15] -—20 0 | -19| -19 | +19 —20 +32 | +47| +13 | +19] —10 =— 7% | —18,) =14°)| + 7 +13 +32 — 4 + 4 +28 — 46 —18 —19 —32 +14 +42 +56 +28 +35 +21 —34 —18 + 9 -—12 — 6 +20 +41 +22 +21 +20 —38 —43 —3l —34 -— 9 +44 +11 —12 +16 -— 5 —20 —22 — 3 —11 —11 +27 +43 +21 +24 +19 —21 — 28 —31 —26 - 2 +37 +45 +28 +32 +13 —22 -— 3 —13 —17 +14 — 6 +33 +30 +12 +21 —25 - 8 —19 —22 +14 +35 +36 +13 +24 +12 —31 — 28 -— 8 —20 | - 8 +23 +39 | +23 +23 +16 —25 -—17 | -18 —21 +4 +12 +19 eee +13 Pale —25 == (Shep = taal IA 4-6 iver ao: | + 5) +11 4 + 8) —19 Se eet) Cia ee oe ae | 6b |, “4380 1% 4h) 289 = ger) SON, Sb ees +44 +67 | +26} +385 | +32) —47 —39 | -19|; -—33 | — 6 +19 +44 | 427} 423 | +21) —53 —24 |—7}| -30 | + 6 +23 +33 +21 +22 +11 + 8 - 4 —39 —15 +11 +29 +57 +18 +24 +33 — 26 —27 —23 —24 -— 3 +43 +38 + 8 +25 +13 —34 —11 —24 |) -—29 +18 106 REPORT—1898. TaBLE XI.—Diurnal Range at Greewwich as Declination Horizon-| Quiet Days b—c Quiet Days Month, ea leet ie oo = > a ee eo Quarter, or | Year Cor- Cor- rected rected As for Great- |} Least As for Ob- Non- All est |Month-| Differ- Menn Ob- | Non- b served | cyclic} a—b | Days |Month-| ly ence served | cyclic | %— Incre- ly Value Incre- _ ment Value ment a b c , a b / / / ‘ ‘ / ‘ / January | 5°04 4°81 | +023] 5.58 | +0°7 | —33 4°0 |—0°77 || 188 179 +9 February .| 606 | 5:85 |+021] 711 | —02 | —32 | 3:0 |-126 || 257 | 232 | +25 March . .| 9:03 | 8:96 |+007| 944 | +05 | —o'8 | 1:3 |—018/] 319 | 299 | +20 April . .| 1080 | 1078 | +002] 1115 | +11 | -1:3 | 24 |-—037 |] 442 | 423 | 419 May . «| 11-00 | 1097 | +003 | 10-72 | +17 | -15 | 32 |+025 || 454 | 435 | +19 June . «| 10:88 | 1086 | +002 | 1085 | +17 | -1:3 | 3:0 |+001 || 479 | 464 | +15 July . .| 10:79 | 1084 |—0:05 | 1095 | +05 | -o08 | 1:3 |—o1 || 456 | 444 | +22 August. .| 10-77 | 1084 |—0-07 | 1069 | +18 | —o8 | 26 |+015 |] 471 | 457 | 414 September .| 9:54 | 9:59 |—005| 940 | +18 | -12 | 3:0 | +019 || 413 | 397 | +16 October. .| 7:47 | 7-49 |—002| 806 | 00 | -15 | 15 |—0'57 |! 353 | 329 | +24 November .| 5-21 | 5:12 |+009| 628 | —01 | —28 | 27 |—116 |] 951 | 241 | +10 December .| 4:09 | 4:01 | +008] 519 | —03 | —1:9 } 16 |—1-18 |} 147 | 147 0 Ist Quarter .| 671 | 654 /+017] 728] — | — | 28 |-074 |] 265 | 237 | +18 2nd Quarter . | 10:89 | 10:87 | +002 | 1091 | — | — | 29 |—004 |) 458 | 441 | +17 3rd Quarter .| 10:37 | 1042 |—005| 1035 | — | — | 23 |+0-07 || 447 | 433 | 414 4th Quarter .| 5:59 | 5:54 |+005] 651] — | — | 1:9 |-0-97/]] 950 | 239 | +11 Mean. .| 8:39 | 8:34 /+005| 876 | — | — | 25 |—o-42|/ 352 | 337 | +15 1889. Sw | «6-45 | 6-48 |—0-03] 667 | +11 | —07 | 18 |—O-19 |} 261 | 252 | +9 1890. s| 678 681 |—003 | 7:20 | +05 | —13 18 | —0°39 263 256 +7 1891 . -{| 818 | 808 | +010} 846 | +07 | —14 21 | —0:38 350 338 +12 1892 « «| 975 978 |—0°03 | 962 | +17 | —12 29 | +016 398 370 +28 1893 . . {| 1013 | 10°06 | +0:07 | 10-40 “+18 —15 28 | —0'34 || 428 414 +14 1894 lw - | 9:02 889 | +013] 945 | +05 | —17 22 | —056 414 403 +11 1895 . .| 878 | 875 | +003} 964 | +18 | —33 51 | —0'89 380 360 +20 1896 . «| 801 790 | +011] 864 | +18 | —3:2 50 | —074 326 306 +20 Mean. : — _ _ —_— _ = 30 oa _ _ — ON COMPARING AND REDUCING MAGNETIC OBSERVATIONS. variously determined, compared, 1889-1896. 107 Vertical Force ital Force |) b—c Quiet Days b—c Cor- an [Oe et one | a | BE: | a | ace | 4, face Days er. e i hike! Mean aerved apeile a Days rig sees a : ental Mean WRIGA Value ae Wee Value ¢c a b ¢ 163 | + 73) — 51) 104 +16 114 100 +14 | 109 +22 | — 44 66 -9 200 + 95} — 5] 100 +32 125 131 — 6 175 +22 | —127] 149 —44 313 + 59} — 53] 112 —14 216 221 —5 257 +13 | —109 | 122 —36 447 + 33} — 88] 121 —24 245 243 + 2 298 —13 | —162| 149 —55 449 + 64] —117}| 181 —14 312 309 + 3 356 +17 | —105 | 122 —47 496 + 68} —108| 176 —52 257 253 +4 303 +26 | —118 | 144 —50 496 — 4 | —123] 119 —52 253 252 +1 277 +44 | — 79} 123 —25 470 + 64} — 82] 146 —13 212 210 + 2 233 +26 | — 70 96 —23 393 | + 64] — 51] 115 +4 195 194 +1 217 +26 | —101 | 127 —23 338 | + 38; — 91] 129 -—9 157 157 0 196 +17 | — 61 78 —39 212 +101 | — 26] 127 +29 115 114 +1 157 + 4 }—101 |] 105 —43 (150 | +16} —37| 53 | —3 || 105 96 | +9 | 105 | +35 |— 44] 79 =9 225 _ _ 105 +12 | 152 151 +1 180 — _ 112 —29 Meee | — | is9 | —93 || avi | aes | +3] 319 | — | — | 138 | +81 453 _ —- 127 —20 220 219 +1 242 _ _ 115 —23 233 _ _ 103 +6 126 122 +4 153 _ _ 87 —31 344 _ — 124 —7 192 190 + 2 224 _ —_ 113 —34 248 | + 66 | — 42] 108 +4 163 163 0 168 +35 | — 52 87 —5 253 + 44 | — 46 90 +3 176 170 + 6 173 +44 | — 66] 110 —3 323 + 73) — 55] 128 +15 192 189 +3 222 +22 | —101} 123 —33 402 + 64] —123| 187 —32 228 231 — 3 257 +31 | — 79] 110 —26 413 + 90} —108} 198 +1 202 199 +3 233 417 | —118]} 135 —34 411 +101 | — 77} 178 —8 197 192 + 5 248 417 | —1¢2] 179 —56 370 + 95] — 66] 161 —10 191 187 +4 242 +26 | —127] 153 —55 331 + 38) -117/ 155 —25 190 190 0 245 — 9 | —109} 100 —55 — ont no ane = — — 125 _ 151 108 Taste XII.—£wcess of Absolute Values of Magnetic Elements on Quiet Days at February . June . . September . October . November . December . Ist Quarter 2nd Quarter 3rd Quarter 4th Quarter Mean 1889 . ° 1890 . . 1891 . . 1892 1893. 1894 . . 1895. . 1886 . Totals of Months . REPORT—1898. Greenwich above the Values of the All Day J'abulation, 1889-1896. Declination Difference to Ce ll a aa a ap Se, to w o tw bo _ os Ln — i — i — a —) nu» owe © * Individual Months wo oo i] w wo Dm wo Mm 8 ~ oO woo me me wl Horizontal Force Greatest Monthly Excess | | Least Monthly Excess | Difference | tobe tt Ft tt tH + Ft H+ + + + + + + + t+ t+ t+ + + + Individual Months oo =m wo two ol ow NN 2k A HM AN DD wy (— eet — 2 — lee — el — Gel — es — ee — ee — ee — to oF Fe Of o o.oo o& o @ .o' © ap OO = Be WO DH HT oH 70 1 25 Soa ae SO a a Pa ae Greatest Monthly Excess Vertical Force Least Monthly Excess | —106 | Difference Excess aN WP Oa eI eae ee ee ee Individual Months ooocm6UcomUCcCOOUCUCcCOUhrPMH OF Oe KO i - no ns oOo eke, OO OH w& — ae — ee — ee — See — J ~ d 45 7 a ee ree eh DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 109 An Account of the late Professor Joun Coucn Apams’s Determination of the Gaussian Magnetic Constants. By Professor W. GRYLLS ADAMS. I propose to give the Conference a short account of the work done by my brother on the theory of terrestrial magnetism, and to give his determina- tion of the Gaussian magnetic constants. This work was first taken up by the late Professor John Couch Adams just fifty years ago, not long after the discovery of the planet Neptune. I find from his papers, which he delivered to me before his death, and which he asked me to examine to see if they could be brought into form for publication, that the earliest work which he did on this subject was begun in the year 1849, and that he was led to it by the study of the translation of Gauss’s Memoir on the Theory of Terres- trial Magnetism given in Taylor’s ‘Scientific Memoirs’ which was published in 1841. Gauss himself says in that memoir that he was stimulated to undertake the work on the publication of Sabine’s map of the total intensity in the seventh Report of the British Association (7.e. in 1837), but that the data are very scanty for the accurate determination of the magnetic constants. For their accurate determination data should be supplied from accurate observations of magnetic declination, horizontal intensity, and dip, taken at stations uniformly distributed, as in a net- work, over the surface of the Earth. Not only fifty years ago, when Gauss wrote, but even to the present day, the progress made in the theory of terrestrial magnetism has suffered from the lack of data derived from observations, because even now there are few magnetic Observatories in existence, and those few are for the most part grouped very close together, leaving other parts of the Earth, and especially the southern hemisphere, almost entirely wanting in the facts of observation without which all theories can be but visionary. ; In his calculations on the magnetic potential of the Earth and on the theoretical expression of the magnetic components X, Y and Z, to the north, to the west, and vertically downwards respectively, Gauss expressed them for any point of the Earth’s surface in series consisting of quantities to which he gave the name of magnetic constants, with coefficients involving Legendre’s coefficients, and which are functions of the colatitude of the point. From the very imperfect data which he possessed, Gauss determined the numerical values of the magnetic constants by his equations up to terms of the fourth order—z.e. he determined the values of the first twenty- four magnetic constants, three of the first order, five of the second, seven of the third, and nine of the fourth order. No one could be more conscious of the fact than Gauss himself was that his data were so meagre and so insufficient that he could by no means rely on the values derived from them, and I fear that even now, at the end of the nineteenth century, we must say with him that the observed facts are far too scanty and that our stock of observations is still too small to enable us to get out trustworthy values of the magnetic potential and the magnetic elements for a given epoch. For this purpose the observa- tions should be strictly contemporaneous, and we require more Observa- tories where continuous records are taken. For Gauss’s method, which was also the method followed in practice by 110 REPORT—1898. my brother, it is important for the accuracy and trustworthiness of the resulting values of the magnetic constants that the observations shall be taken from stations distributed as uniformly as possible over the Earth’s surface ; whereas we see that in the northern hemisphere the Observatories which exist are very unequally distributed, and that in the southern hemisphere there are only three first-class magnetic Observatories where continuous records are taken, viz. those of Batavia, Mauritius, and Melbourne. For the more ready development of the theory of terrestrial magnetism, Professor J. C. Adams established simple and convenient relations between successive Legendre’s coefficients and their derived differential coefficients regarded as functions of the colatitude 6 = cos". Taking P, to represent Legendre’s n coefficient, he employed the notation Qn to denote the value of d™Pp., dp ™ (= wy and found certain simple and useful relations between successive values of Q for different values of 2 and m. He also employed the symbol G7’ to represent the Gaussian function n-m_(n—m) (n—m - Ly n—m—2 & M 2(2n— 1) i and found it convenient to employ the symbol H” as = G™ (1—,°)** He worked out very simple relations between successive values of G for different values of n and m, and proceeded to determine the numerical values of these functions (1) for every degree of latitude on a sphere, and (2) for every degree of the geographical colatitude on a spheroid of eccentricity equal to that of the Earth itself. He also obtained very simple relations between successive values of H and its differential coefficients for different values of » and m, and expressed the magnetic potential V and the magnetic forces X, Y and Z in terms of these symbols H™. He also determined the values of these functions H7” for belts of latitude 5° apart (1) on a sphere, and (2) on a spheroid whose eccentricity equals that of the Earth’s surface. Two distinct schemes of calculation were employed to determine the numerical values of G” and also of H” for different values of 2 and m, including all values of 2 and m from 0 to 10, and these calculations were made by different people and the results of the calcula- tions compared to ensure the accuracy of the results. In the case of the spheroid, the functions G" and H” are regarded as functions of the geographical colatitude 0, and » = cos 6, and the symbols G’” and H’” are the same functions of the geocentric colatitude 6” of the same point, ‘where p’ = cos 6. A new theorem giving the values of G’—G’ for different values of m and m is established, by means of which the accuracy of the calculated values of G and G’ may readily be tested. Taking V to represent the magnetic potential at a point of the Earth’s spheroidal surface where A is the longitude, @ the colatitude, and r the distance from the Earth’s centre, X, Y and Z the magnetic forces in three directions at right angles to one another, X being the force towards the north perpendicular to the Earth’s radius, Y the force perpendicular to the DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 111 geographical meridian towards the west, and Z the force towards the Earth’s centre ; also taking cos €=p, we have rdé r dp r dp’ reed ON es Cede ry sin Ody 7 ‘aX o, dV as if east longitudes be considered positive. There are two systems of values of V corresponding to magnetic forces whose origin is situated inside and outside the Earth’s surface respectively, and by a convenient notation we may readily distinguish these two systems of values. Making use of the functions denoted by H” which I have above de- fined, and taking g;’ and hj’ to represent the Gaussian magnetic constants, gx and h7 are coefficients of cos mA and sin mA respectively in the series of terms representing the magnetic potential. The value of the magnetic potential V for magnetic forces whose origin is situated in the interior of the Earth is expressed by a series of terms of the form 1 go” +1 [He (gn cos mMA+A™ sin md) | Taking g™, and h™, to represent the values of the magnetic constants corresponding to this term of the series for forces situated outside the Earth’s surface, the corresponding term in the magnetic potential will be o"(Hir(g™, cos mX&+H™,, sin md)]. Hence Ve=> a Hor cos mA-+h™ sin md) +2 ol Hing", cos m\ +h™, sin md) | In the values of X, Y and Z there will be terms arising from each of these series of terms for V, and we may conveniently express them by modifying the notation in the same sense by using 7 subscript to refer to internal forces, and —n subscript to refer to external magnetic forces, or forces whose origin is outside the Earth’s surface, i.e. corresponding to negative powers of (). r The corresponding terms are in the value of X, Fp?) Ze (9m cos mA--AM sin. ma) gee? dp. } dH™ and r"-(1—p?) on (gm, COS MA+h™, sin mX) 5 Be 112 REPORT—1898. in the value of Y, 1 caval —p?)-} m A” (gm sin mk—h™ cos md) and 7”-"(1—p?)-} m H7? (g@, sin mA—h™, cos m2) ; in the value of Z, n+1 H" sy Hi (gi cos mA +h" sin mX) and —nr"- H™ (g™, cos m\ +h™, sin md = It is also proved that (1— 2)! GE = (nm) Hemp (1-2) Be and (1—p?)! = we 1 (n—m) H™1_} (n+m) H® 1 - and these relations are often useful in expressing the terms in the value of X. It is found convenient to employ the notation with n and —n subscript more generally to refer to internal and external forces respectively, and in this sense the following notation is employed. Let Vv" = a H" and V", = 7" H", and let Xp = a [b (nm) Heh — 3 (nem) Bey be the coefficient of (9% cos m+” sin mX) in the expression for X, the force towards the north, and let X”, be the corresponding coefficient of (gz, cos mA +h”, sin mx) in the expression for X arising from forces outside the Earth’s surface. Then X", = 7° [} (n—m) Hp} (n-+m) Hy} Using the notation Y”' and Y”™,, and also Z” and Z™, in the same way for the forces Y and Z, we have the potential V=2[Vi'(gr cos md +h” sin md)]+ 2[V™, (9%, cos MA-+h™, sin md)], X= T[LAN(gi' cos mA +H? sin md)] + 3[X™,,(g™, cos MA+H™, sin mX)], Y= =[Yin(gi' sin m\ —h7" cos mA)] + 2[Y™,,(9™, sin mA—h™, cos md)], Z= >[Zr(gz cos m\ +h” sin mX)]+3[Z™,(9™, cos mr +h”, sin md) ]. Collecting coefficients of cos m\ and sin m) in the values of V, X, Y and Z respectively : The coeflicient of cos m\ in V is 3(V™g"+V™,g" n)s ” ” ” x ” S(Xrgn + xg n)> ” ” ” a ” S(Yrm+ Y™,h",), ” ” ” Zo X(Zrgt+ 22,9"). , DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 115 The coefficient of sin m\ in V is 3(V"24+V™,h",), X ,, SCXRAT +X, h™,,), Ys, SLi gn + gn)» Z ” SZ + Zh), s2 ” ” ” Pd ” ” oP] ” in which n takes all integral values for a given value of m. In a portion of his work, in which he treats of the definite integral of the product of two Legendre’s coefficients, Professor Adams proves the well known formule, which I believe were first proved by Legendre, that when and 7, are different from one another a! | Py P, du = 0, f cal and that when n,= », Ly) Qn+1 (ee He also proves that if ie a1 aP, ts (l—p, 3 dp” 1 text th OOF dy OI PB dy. en J O2 QR du = Ty |_ Pe Pn Hence if n and 7, are not equal 1 | Qt Qi du = 0. Ny But if n,=n, then o emndet.,, (em)! 2 jet eek (n—m) ! oye aD Hence if mm =(o) | on and TI" = [ee | m, n+m)! +m)! it follows that , 1 | am Ti du=0 ; and, when n=7,, we have 1 1 5 a m2 __ (n—m)! m2 eae = P,)?d jam ao (n+m) ! [_,(@) qi: -In+1 ix nd It is also shown that (n—m)! me ci as RT Dk And therefore, when 7 and , are not equal, we have . i H” .H" dy = 0, si 1898. I 114 REPORT—1898. and, when 2,=, we have { ay. du = ioe ost F at From the above formulz we see that, on a sphere of radius unity, Xt = (n=) Hp —mp(1 8)! He = (12) = mp(1 —p?)) He —(n4+m) He, 5 also Yr = m(1l—p?)? cc and Zr = (n+1)H”. Hence pYy— XP = (n4-m) Hr, and aes = (n—m)H"*}, also (l—p?)'¥" = mH". From these formule we find fede [eye lH) (ZE) aut [tay and also = Mont)? | ERY dut n— my | (EE) date (ER, These definite integrals reduce to _ n(n+1) ib (H")'dp. Hence since Z"'=(n+1)H™, we have [ ardut |) Cerraet fF eyrdu= (n+) (2n41)]) (nap (n— suk n+m ’ =e S.. we a fee Putting », for in the above equations we get pYn—xm — (nr, +m) ee, eym +X™ = (n,—m) Hm, and (1—p°)F¥® =mH™. Combining these formule we get hwy — Xp) (eV Xe) + eVe+XP) (WV +X") 4 (1—pyYeve = XTX + YT Yn =3(2 +m) (2, +m)He 1H" 4 1(n—m) (n, —m) B"H +14 PHA” ; ny, hence j _XnXndut ic Y"rY"dp = 0, DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 1d) since we have seen that for any value of m and different values of n and n,, the value of ny 1 | HeH"dp = 0. sii For the same reason 1 | ZZ" dp = 0. =1 ny Now let us consider the application of these formule to the determination of the numerical values of the magnetic constants of terrestrial magnetism. For a given value of p (7.e. for a given latitude) we have a series of terms forming the coefficients of cos mA and sin mA, in the values of the mag- netic potential and of the magnetic forces X, Y, and Z, which are of the forms a, H+ Oy, Hm + &e. Gy, x a, Xn + &e. a, Y"+a, Y™ +&e. a, LZ” +a, Zm + &c. where a,, a,,, &c., are the magnetic constants to be determined. The numerical values of H”, X™, Y™, and Z™ for different values of m and m must be calculated, and in any belt of latitude of breadth corre- _ sponding to the numerical value taken for du, these coefficients must be equated to the values of the forces as derived from the magnetic observa- tions taken in that belt of latitude. The values of the magnetic forces X, Y, and Z are derived for every 10° of longitude and every 5° of latitude from the declination (8), the dip (:), and the horizontal force (w), as given in the charts from which the observations are obtained. These values of the forces X, Y, and Z are analysed forbelts of latitude 5° in breadth around the Earth’s surface by - a formula of the type a+, cos (+0, sin \+a, cos 2A+6, sin 2+ ke, If we take x,, to represent the coefficient of cos md in the expansion of the value of the force X for a given belt of latitude corresponding to the colatitude 0 = cost: then, a, X™ +a, X™ +a, X™+&C.=2 ps where x,, is derived from the observations. Similar equations, involving on one side the magnetic constants a,, a,,, &c., and on the other the values derived from the observations, must be formed for all the successive different belts of latitude from the north pole to the south pole—z.e., for all values of between 1 and —1. The numerical values of X™, X™, &c., as well as the values of H7 (as above defined), have been determined for every degree of latitude and recorded for future use, but, in the actual determinations of the magnetic constants which have been made, belts of latitude 5° in breadth have been taken, or 80 has been taken as 5°, and the area of the belt is pro- portional to du. Supposing the observations equally distributed over the surface of the globe, or supposing the weight of any determination proportional to the surface of the corresponding element about the point of observation, then the weight of each of the above equations is proportional to dn, and multiplying the equation in X for each value of by X7’, and 12 116 REPORT—1898. summing up the separate equations for the whole surface of the Earth, we get the final equation— 1 1 1 a, | (XMPdut+ | xen XT dp + ke. =| XO. oe = —l =i) Similarly, the final equation for a, is found by multiplying the above equations by X13’, Y/”, and Z"' respectively, and we get 1 uf 1 a, | X”X” du + «| (Xm )'dp +he=| Xn x, Ofte =] —1 | In the same way, if v,, denote the coefficient of sin mA or —cos md in the value of the force Y as derived from observations, we have (an Yn) = Yv and the final equations for finding a, and a, respectively will be ie 1 «a (Y")2du + ap, iB YY" du + ke. =| Y" y,, dp, =i ah 1 Bae. ae | ye yn Mean | (Y")? dude. ={ Y" yy, Ut —l 1 Combining the final equations for a, from X and Y together, we have auf (X24 (Y")2] du= fi X" 2, du+ j Y" oy, Ap, since the coeflicients of «,, and all the other terms on the left-hand side of this equation vanish when the integration is taken all over the Earth’s surface. 1 1 1 Hence o,. n(n + 1) ah (HL)? dp =| Kno du tle Vy, dus —1 se s !(n+m)! A . (2n—1)/? (2n+1) 1 eo Xa, dp -| LP Yn Up = Sit 1.€. a, X 2n(n +1) [1.3.5 Similarly, by putting n, for n, we may get the value of a,,. In the same way the final equation for finding a, from the equations for Z would give us 1 1 1 «.| (Zi)? du + «f Zn Zn" dy + be=| Li 5 Okie =a —J —1 1 1 or a,(m + 1)? | (H")? du =| Z™ 2, ap, Since i Zr Z" dp =0 ; Si -1 —1I ‘a Ympiye (om)! (n-tm) ! a iT so [1. 3.5... (Qn—1)PQn+1) =|) mn If we take into account separately the parts of the magnetic force at a point due to the internal and external centres of magnetic force, the DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 117 general terms of the coefficient of cos m) in the potential function will be th of the form (Si + Pyr | 15 bigs and the corresponding coefficients in X, Y, and Z will be— in X= (Sat Bar") [ sem) — Yntm) Ee | | in (l1—p?)' Y= (: = +Bn yn ‘) mH"; : nt L)a v in Z =(‘ +1)cq _ mB, 1” ‘| Hr. a+ 2 ys If then, as before, we put r=1, we shall have the final equation for a, as follows : a,[ | xray +) (ny? det (n+) [area | =f +B [| (X")2dp + {¢ = (Yr)? du—n(n +1) K (Ee)? de | 1 =| B.S a+ in Se qu (n+ 1)[ mm, ply = 1 where the coefficient of 8,,=0. And a.[ i (X")? du + i (Y")2dys —m(nt1)f (H™)2 au] —1. +B, [| (Xm)? dj +] (Yr)? dut nf (Hs)? dp] 4 =f si 3 | 1 1 " =|. X" ay a+ ‘Yrynde—nl H” =, dp, =! where the coefficient of a, = 0. Hence «a, and /3, are separately determined from the equations (n— ee a ! Zeal Wr ge ORE fel =| x x" m 30 5 qr \ ya Ym dut+(nt+ if H em du 1 (n—m) !(n+m)! WE 3.5... (2n—1)P =| Xpondut Yn udn—nl F Hz, du. my and Pye a Thus generally from the values of X and Y we derive (an + B,)2n(n+ 1) ie b. 2 es aoe =(2n+1) [|> ay dpe +{ "yn a | = sy 118 REPORT—1898. and from the values of Z we derive 1 1 [( ai )a,—n3, | | (H")? du = | Hz, dy =I 7 The above theory assumes that the integration is taken over the whole surface of the Earth, and that the observations are uniformly distributed over the Earth’s surface, otherwise the coefficients of the neglected terms on the left-hand side of these equations will not vanish, and each equation may have other terms which are too important to be neglected, and so it will not be so easy to separate the magnetic constants from one another. Let us now take into account the spheroidal figure of the Earth. Let r, 6’, X be the polar co-ordinates of a point on the spheroidal surface referred to the Earth’s centre as origin and axis of figure as initial line ; let 0 be the geographical colatitude (the: angle which the normal makes with the axis), and let 1 = cos @ and «= cos 0’. The angle of the vertical y = 0’—90. The values of the sines and cosines of these angles for values of 0 differing by 1° from 0° to 90° have been computed, the eccentricity e of the elliptic section in the plane of the meridian being derived from Bessel’s dimensions of the Earth as given in Encke’s tables in the ‘ Berliner Jahrbuch,’ 1852. The expressions for the magnetic potential and for the magnetic forces X, Y, and Z, in terms of the Gaussian magnetic constants g™, h” will be of the same form as those given above (see p. 4). Where X is the total force towards the north perpendicular to the Earth’s radius, Y the total force perpendicular to the geographical meridian towards the west, Z the force towards the Earth’s centre, or dV ius Wav = —— — tee 8 gat F On) rde” rsind’ dy’ dr (east longitudes being considered positive). If X’ be the horizontal force in the meridian towards the north, Y’ the horizontal force perpendicular to the meridian towards the west Z! the vertical downward force on the spheroidal surface of the Earth, then X’/=X cos ¥4+Z sin p i Z' =—X sin ¥+Z cos yf. We may conveniently denote the values of the coefficients of grcosm\ and fh” sinm. in the potential function and in the forces X’, Y’, and Z’ by the symbols V’", X’™, Y’", and Z’" respectively. If r be the radius vector, »=cos 6 and p/=cos 6’, then vn ele H’™, and V/™=r" H’™ ntl “1 H’” being the same function of p’ that H™ is of p. The expressions for the magnetic forces on the spheroidal surface of the Earth will be as follows :— Taking a, and /3, to represent magnetic constants depending on in- DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 119 ternal and external sources of magnetic force respectively, the coefficient of cos m\ in the general term of the potential function V is (ta + Bur"). pd The coefficient of cos mA in the general terms of the forces X, Y, and Z are— ay n— L d a Ue for X, az + Bot ‘) (1—p!?)! a for Y, (aa aie Br me) m(1 =p?) 1s ae for Z, eC dies ere ) : pnt In the following investigation of the coefficients of cosm, &e., in which m remains the same, whilst may have different values, it will be convenient to denote H” by H,, X” by X,, &c. We will denote the corresponding quantities on the spheroid by H’,, X’,, &c., and regard them as functions of p’, 6’ being the geocentric colatitude. Taking the equatorial radius =1, 6S an element of the Earth’s surface and e the eccentricity, and taking into account only the terms to the order ¢?, we have zi =1+e%u?, snp=e'u(1—p?)! to the order e?, 7 / y! = cos 0—sin 0 sin ¥ = p—e®n(1—p2) eet SPC: fad and e = — 2n(1—e7p?) ; . 1 EEN 109 =. also oe jiee ale e2p?, andr? = 1 — > Gir. / Regarding H’, and Lid &c., as functions of pp’, we have by Taylor's Uy - theorem— / 2 2 d HL, 2 H’,=H,,—e?4(1 — 2”) a to the order e?, fad dH’, dH , 7H and SiS Me Ey 2 62 1 (Me pe) ee : du! du é pe B ) dy? ? from which we derive the value of X,, for the spheroidal surface — d H’ Me Saltese See 8 n=(1—p!® dul = (1 = pay 022) 40% (Lp)! [nt 1)— | Ho du 1l—yp? If now we erbatiintc the values of X, Y, and Z in terms of H’,, C7 als Gest : pie c., in the equations— X/=X cos W+Z sin y, Bias, Z’ =—X sin W+Z cos y,. 120 REPORT—1898. , the expressions for the magnetic forces become — aH’. ag re aey + a 1 X'= (S + Br ) al +2 +[ee ry —n ea H’, sin Y+similar terms, bs =( eat By?) mH’,(1 —p?)-?+similar terms, pnt Te (1—p?) sin-ap nt? Zi=— (25+ Be + kp tl ae —n pe] H’, cos )+similar terms. 7 ta dW’ Jn these expressions for the magnetic forces the values of H’,, = 8 fied dH, &c., in terms of H,, &e., are substituted for each belt of latitude, and due these theoretical expressions derived from the potential function for a given belt of latitude, and containing the magnetic constants, are equated to the corresponding coefficients derived from the magnetic observations taken in that belt of latitude. In the case of the spheroid, as in the case of the sphere, the values of the forces X, Y, and Z derived for every 10° of longitude from the obser- vations of declination, inclination, and horizontal force are analysed for belts of latitude 5° in breadth around the Earth’s surface by a formula of the type— G+a, cos (+6, sin (\+a, cos 2A+6, sin 24+ ke., and the coefficients of cosm\, sinmA, in this expansion are equated respectively to the coefficients of cos mA, and sin m\ in the expansion in terms of the potential function and magnetic constants as given above : thus for the force X, if a,, a,,, a,, &c., stand for the magnetic constants, and if a,, be the coefficient of cos mA as derived directly from the obser- vations, then a, X/'+a,, X/" +a,, X/%4-&e., =x m) _ oe equations are obtained from the expressions for the forces Y’ and Z’. The values X/", Y’, and Z/”, taken in these equations, are the values derived for the spheroidal surface of the Earth from the potential function, and these equations not only include the magnetic constants which were determined by Gauss, of the class indicated by a in the above equation, but they also include magnetic constants which may be spoken of for distinction as the £ class, 7.e. including those forces which depend upon sources outside the surface of the Earth. The full values, then, of the coefficients of the magnetic constants will be of the following form: DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 121 For the a class— 2 4 ag" +2 il ate n+l] : Xin=_). E (n—m) Hm —3(n-m)H2 | cos pp tty sin y, 5 [ Lape) Hr | n +1 Z'™= as | Mom) —t(n+ my He | sind) + — 1 gt? +2 H’" cos w. Ib For the class, which may be denoted by X’",, Y’",, and Z",, x =r" "(4 (n—m) HT 1_1T(n+m)H’""] cos y—nr" A’? sin y, 5 piel =r" "[m(1 —p!?)- ts Wd B Z™, =—r" {h(n —m)H/"*? —3(n+m) HH" | sin pP—anr"™ Hy cos Vp. The numerical values of these expressions for all values of m from 0 to 10, and for all values of » from 1 to 10 for the spheroidal surface of the Earth, have been calculated from the values of » for every 5° of colatitude, and form the coefficients of the magnetic constants g””, hj’, and g™,, A”, of the a and 3 class respectively in the equations for the determination of these constants. The number of magnetic constants contained in these equations which have been completely formed is thus 120 of each class, or 240 magnetic constants in all, in place of the 24 constants of the a class which were previously determined by Gauss, Regarding the Earth as a spheroid of revoiution, the values of p’=cos 6’, where 6/ is the geocentric colatitude, have been determined for every ‘5° of geographical colatitude. Also the values of cos y/, sin ¥/, ©, @m, and os H’™ have been calculated for every 5° of geographical colatitude (i.e. for the above values of ,’) for all values of m and m from 0 to 10. 3 The weights of the observations of the magnetic elements for these belts of latitude have also been determined on the assumption that the weight is proportional to the area of the corresponding portion of the Earth’s surface. The values of H’” as a function of the geocentric colatitude having been determined for every 5° of geographical colatitude on the spheroid, we next proceed to determine from them the values of X’”, X’,, Y’"; pS Z™, and Z/™,, X/"(=X™ cos + Z™siny), X/™,, Z/™ (=—X7 sind + Zr cosy) and Z’",, the resolved parts of the expressions for the horizontal and ver- tical forces in the plane of the meridian on the spheroid. These values are required in the formation of the equations of condition, and their numerical values are calculated for every 5° of geographical colatitude as well as for the Equator and the Poles. These values of a as é&c., have been calculated and recorded in tables for all values of » and m from 0 to 10, and have been employed as the theoretical coefficients of the magnetic constants g™, h”, &c., in the equations of condition. n? Formation of the Equations of Condition. When x—® is even, the value of X” contains only odd powers of p, and the values of Y” and Z” only even powers, and similarly when »—m is odd, the value of X” contains only even powers of », and the values of 122 REPORT—1898. Yy7 and Z” only odd powers. Hence, if the coefficient of cos mA in either of the quantities X, Y, Z be denoted by a,, and the coefficient of sin mA by 6,, for a given north latitude, and if a’,,, 6’,, denote the similar quantities for the corresponding south latitude, then we have, when 7—™m is even, 3(4m, a @'m) = >(X" mt Xm roa § and 4 (On —8' m) = S(XTAT Ke - $n +5'n) =UYrg™+Y™,97%,), and —43(a,, + a, )=S(Yra™ + Y™,h™,), B(Gin + Om) = 2(Zrgn+-Z™,g™,), and 4(By +5) = =(LZrhm + Zm,h™,), - and when »—™m is odd 4(On +2 m)=S(Xg" + X",g™,), and (by +5’ _)=>(X7h™ 4+ X™h™,), Bb n—O'n) =S(Virgn+¥rgr,), and —3(a,—a',)=S(YrA™+ Y™,h™,), B(Gn— OU n= A(LZrgr +29"), and 4(b,—B',)=S(Lrh™ + Z™,h™,,). Hence the equations for the quantities h”™ and h”, will be found from the equations for g” and g”,, when m—m is even, by substituting 3(6,—0'n) for 4(a,,—a’',) in the equations for X, —3(Gn +m) for £(b,,+6',,) in the equations for Y, and 3(6,,+0',,) for $(a, +») in the equaticns for Z. And similarly the equations for 4” and h”,, will be found from the equations for gv and g”,, when n—™m is odd, by substituting (On +0',) for $(a,,+a',,) in the equations for X, —}3(4,—a',,) for $(b,—6',) in the equations for Y, and 4(6,,—0',) for 4(a,,—a’,,) in the equations for Z. In the first solution of the equations, the absolute terms (i.e. the terms derived from the observed values of the magnetic elements) are taken from Sabine’s magnetic charts for the period about 1845, as published in the ‘ Philosophical Transactions of the Royal Society.’ In the second solution, the observed values of the magnetic elements are taken from the Admiralty charts for 1880 prepared by Captain Creak, kindly lent by the Lords of the Admiralty. The values of X, Y and Z are calculated for every 10° of longitude and every 5° of latitude from the declination (8), the dip (:), and the horizontal force (w) as given in the charts. Then the values of X, Y and Zare analysed for belts of latitude 5° in breadth around the earth by the formula %+a, cos A-+6, sin A+a, cos 2A+6, sin 2A + &e. The values of these coefficients for the different belts of latitude were obtained and tabulated. Then if a,,and b,, denote the values of two of these coefficients for a given northern latitude, and a’,,, b’,, the correspond- ing values for an equal southern latitude, then the values of }(a,,+a',), 2(Gn—@'n), 3(bmn+8'm), and 4(5,,—b’,, ) and of their logarithms are deter- mined. The values of these quantities are determined for each of the periods for which the magnetic constants are required. Each system of equations of condition will involve a single value of m combined with all even values of , or with all odd values of x. There will be one system for the coefficients X”, X”,, another for the coefficients Y”, Y™, and a third for the coefficients Z”, Z”,,. ——- si‘ tP:é‘( (ast EN ee DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 123 Each belt of latitude will contribute an equation to each system. The belts, 5° in breadth, are distinguished by the letters (a), (b), (c), &c., starting from 873° N. latitude. Then if P, Q, R be quantities given by observation we shall have equations of the form XP GF AX GARE +X 9+ &e.=P, Ye gt+Y 4g M+ Vrgr+Y¥ "9 "%+&e.=Q, ZY gt +209 + ZP P+ Z% 9% +&e.=R, for even values of , and Similar equations with other quantities P’, Q’, R’, given by observation, for odd values of x. Thus for latitude 60°, the set (f) will furnish the three following equations to the respective systems X, Y, Z, corresponding to m=4, 1 _[9-6479108] g!—[9-6397698] y! ,—[9-3739435] g!—[9-3627519] gt =P, [9-7120302] g/+[9-7022392] g!,+[9°5314878] g{+[9-5173452] g! ,=Q, [95118188] g!—[9-4012092] g!,+[9-4766723] gi—[9-3934121] 94,=R; and the three following to the similar systems corresponding to odd values of 7, —[9-5471920] g!—[9:5374280] g4,—[9-1267947] g!—[9°1145742] o! =P, [9:6499180] 94 +[9-6379512] g!,+[9-3653414] 4 +[9:3490233] 9 =Q’, [9°5284778] g!—[9-4344144] 4, +[9-3682450] g!—[9-2923736]g!,—=R’. These equations of condition are multiplied by the weights w,, w,, &c., of the observations for their respective belts of latitude, the weight of each equation from the set (s) corresponding to 24° on each side of the equator being 4 w,. Then the final equation for each magnetic constant g’” is formed by multiplying each equation so formed by the coefficient of g” in the corresponding equation of condition, and adding together the resulting coefficients of g” from the different sets (s), (r), (q), &ec. To form this final equation for each constant multiply each equation of condition by / weight and then multiply the resulting equation by the co- efficient of that constant g” in it which has to be determined. Then integrating or adding up the coefficients of the several magnetic constants, we get the equation in the form S[(XM)2e0] gh + SL XT Ke] 9, +e. = >[X™ w. P], with similar equations for Y and Z for even values of m, and with other similar equations with P’, Q’, R’, for odd values of x. We shall have a separate final equation for each value of n ; thus the final equation for g” is [Xt Xhw gn +X", Xi, w g™, + (Xn)rw gi + ke.] =X", w P, (3) for even values of 7,, and a similar expression with P’ instead of P for lo odd values of 7). Then adding up, for any constant g™, the coefficients in the final } Where [9°6479108] is employed to express the number of which 9°6479108 is the logarithm. 124 REPORT—1898. equations for all the different belts of latitude we have the final equation from the series (X), which may be represented by the form Sl XT XM. w] gi? + ZX™, KM. w]g™, + S[(X™)? w] gm + de. => [X™. w. P](4) Equations similar to the above will be derived from the series (Y) and from the series (Z). These equations may be solved separately, and the values of the magnetic constants determined from each series, taking series (X), series (Y), and series (Z) separately. The series (X) and the series (Y) may also be conveniently combined into one equation in the same way as the above equations for different latitudes in X have been combined, in which case the coefficient of g”™ in the final equation for g” will be >[ Xe X™. w]+S[Y" Y™. w], and the coefficient of g” in the final equation for g” will he >(Xr)?w + SCY") ?20. We have seen above that in the case of a sphere the coefficients of each of the magnetic constants in this equation (4), except the coefficient of g’", will vanish. The corresponding coefficients on the spheroid will be small, depending on the value of the square of the eccentricity ; but’ this will only be the case when the summation is taken all over the surface. The right-hand side of the equation becomes under these conditions S[X". P.w]+ 3[¥".Q.w] for the equation of g” in turn for all values of m,. Hence when the successive belts are sufliciently near together the coefticient of (7"’+9”,) in the final equation for g” is approximately 1 nin+1)| (Hy? dy a or, _2(n-+1) (@—™) !(n+m)! + ~ ntl ~A[L8D penn)’ and, as before, the right-hand side of the equation becomes [ X".P.du+ | "Ym" Q.dp. -1 = In the present state of our knowledge as to the values of P, Q, R, &c., which are derived from the observations of the magnetic elements, the charts giving the values of those elements are exceedingly defective for our purpose, and the observations taken in high latitudes are not sufficiently numerous and appear to be doubtful—no great reliance can be placed upon them. Under these circumstances we propose to solve these equa- tions, taking into account the data as derived from magnetic observations over the portion of the surface of the Earth between latitudes 673° N. and 674° S., taking only the equations of condition for belts between these latitudes, and taking only those terms in these equations for values of m from 0 to 6 and for values of m from 1 to 6 inclusive. These equations will give values for 48 constants, and no equation will contain more than three unknown quantities. DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 125 The coefficients 3[X”X” .w], &e., on the left-hand side of the above equations of condition will be the same for gm and for h”, but the right- hand sides cf the equations »[X7"w P], &e., the absolute terms derived from the observations, will be different. Hence the equations for solu- tion may be conveniently arranged as follows. From (X) taken separately m Ym m ; Mm \27 75] ym bs ] t *] t > [x XM .wlgn TF S[ (Xm) wlgn + &e.= f Rene os and 3[X™X"™.w]i"-+ S[(X")Pw]h™ + &e.= Peri): From the series for (X) combined with the series for (Y) we may also solve the equations, of which the type will be as follows : {s[X™ X™ 2] 4+ 3[¥"™ Y" w]} g™ + (2[(X)e] + LCL) gt + he. = (APSIE Term) and {3[(X" X"w)]+2/Y7 Yirw]} hz + {3[(Kz)'eo] + S[(Wmyro]} fn + he, = (APseiute term) the absolute terms being derived in this case from the series for (X) and for (Y) combined. In general the values of the same constants derived from these equations will differ somewhat from one another, and the ques- tion arises which solution will give the truer value. Probably in the present state of our knowledge of the magnetic elements over the surface of the Earth the equations derived from the series for (X), (Y) and (Z) combined, for all latitudes from 673°S. to 674° N., will give the most trustworthy values of the constants of terrestrial magnetism, that we may hope to attain from any magnetic charts derived from observations previous to the Admiralty Charts of 1880. Let us illustrate the mode of solving these final equations by taking the case given above, in which m=4 and n odd, taking the equations of condition up to latitude 774° inclusive, and combining the equations for X, Y and Z, supposing the constant corresponding to negative values of 72 to be non-existent. We will include the terms involving n=7. The coefficients for gj and hi being the same, we may take a! to stand for either (1) gj or (2) 3, taking the absolute term for g in the first case a oe in a second, ad the final equations for gj and 43 for the period 1845 may be written thus : From (for g$) (for hi (X) 3:4034960 uf—-3898572 at= 2416593 or _orsabes, (Y) 9°4158541 af+-4092903 aj=-0589245 or +°3418323. (Z) 15°3871472 a$+-0223528 af=-4657356 or +:1824818. Adding these together, we have 28°2064973 af + 0417859 aj ="7663194 or 5084078 (a). Similarly the final equations for ai and A} may be written thus : (X) —'3898572 af+:2637326 af=-0204205 or -0140404. (Y) +4092903 af+:3081774 aj=-0454171 or 0373065. (Z) '0223528 af+ 6536612 at=-0056358 or 0882180. 126 REPORT—1898. Adding these together, we have (for g!) (for ft) 0417859 af+1:2255712 aj=-0714734 or 1395649 ((). Eliminating a} from the equations (a) and (8) we have 1:2255093 aj=-0703382 or :1388117. 1 Hence g!==-0573951, and A4=-1132686. Substituting in the first equation, we get gi='0270832 and hi=:0178567. Hence it appears to be important to take gj and fj into account, as they are larger than gj and hj. Similarly in solving the equations with m=4 and n even, it is found that g3= 0029684, hi=-0217744 9s= 0642604, hi=-0603230. So that gj and hj are more important than gj and hij. The relative importance of magnetic constants of different orders is well shown by the solution of the final equations for h?, h3 and A; for the period 1880. Keeping in the terms containing 7, the final equations derived by combining the equations for X, Y and Z are 241400624 13—-2579706 A2—-1213933 A7=-19111, — ‘2579706 h3+2°1784697 h2—-0719819 hi=-13841, —+1213933 43—-0719819 h2++1887180 hi= —-02852. The solution of these equations gives the values hz=-00794, h?=-06041, h?=—-12298 British units. Converting these into c.g.s. units we get h2=-000366, h2=-0027855, h2= —-00567. Comparison with the tables shows that the effect of keeping in the constant fA? is to make a considerable change in the values of the con- stants A} and h3. The corresponding equations for g}, g} and g; are —14-62295=24:1400624 g§—:2579706 g2—°1213933 g —1:11044= — -2579706 g3+2°1784697 g3—-0719819 9; 05785= — 1213933 g3—-0719819 g2+°1887180 92, and the solution of these equations gives the values g3= — ‘613670, g2= — 592789, g7= —°314308 British units, or G3= — 028295, g?= —-027332, gj= —:014492 c.g.s. units. These values of g} and g G5 do not differ much from the values previously obtained, which are given in the following table. Let us further illustrate the mode of solvi ing these final equations by taking the case of m=0 and m odd. Since the observations of magnetic elements in high latitudes appear to be doubtful, we will form the equations of condition, taking into account the data only up to 675° N. and 8. latitudes. 1 The two extra magnetic constants gy} and f+ here determined make up the number of constants which have been determined to 50. DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 127 ‘The formation of the final equations for g%, g? and g3 will then be as follows : from equations for (X) 53°D75026=7°6331952 gi—1138565 9 —-088674792, — 2:456863= —-1138565 9! + 2°8880836 g$—-1765112 9%, —-4538875 = — 0886747 g}—"1765112 g3+ 3955108 gf ; from equations for (Z) 85-065860=12-0636234 g§—2:1413469 g§—-7000106 9g?, —16-292662= —2 1413469 g8+2°7856531 g§—-4744250 9f, —4-6678164= —-7000106 gi— 4744250 g§ + 4394974 gf. Solving the equations for (X) we get p=7 01229, g = — 56367, g3='17302. These values agree almost exactly with those found from the whole of the equations for (X) up to latitude 775°. Solving the equations for (Z) we get g=6-951666, = — "524544, and y= — 11476. These values agree very closely with those found from the whole of the equations for (Z) to the same latitude. The values of g? and g? agree fairly well with those found from the equations for (X), but the values of gj have opposite signs. Probably the neglected term in g$ may have some influence on this result. Taking the negative values of » into account, let us find approximately what values of 7°,, 9°. 9°; Will bring the two sets of results into harmony. This may be done by substituting g?+g°, for g} in the (X) equations, and g), — poate for g° in the (Z) equations. Hence we get (=6-971874, 9°,="040416, Y= — 541312, 9? ,= — 022358, gi =:01605, and g° = "15697. Hence the constant g°, seems to be of great importance. The values found for the two first of the above constants are, in in British units, by Gauss by Erman gi=T-0155 gi=6'9417 g§=— ‘1430. = — “4069. The values of these constants, derived from the above series of equa- tions for (X), (Y) and (Z), combined for all latitudes from 675° S. to 675° N., ee fi=6-98081 and y®=—-523986 for the period (1842-45) from Sabine’s charts. The values derived for the above constants from the above equations of condition, taking m from 0 to 4 and n from 1 to 4 only and neglecting the other terms (i.e. taking those only which were determined by Gauss), are g{=6:9777 and g’= —-5310 for the same period. The values of the constants given in the two following tables are derived from the combined equations for (X), (Y) and (Z) to equations (e) inclusive (i.e. between latitudes 674° S. and 675° N.), supposing the constants corresponding to negative values of » to be non-existent. 128 REPORT—1898. The second of these tables gives the values of the constants when we include in the equations only those twenty-four constants which are taken into account by Gauss himself. This table also includes the values (in British units) of these constants as determined by Gauss, and also by Erman. Table of the (The sign + is understood when no sign is given.) “alues of the Magnetie Constants as derived (1) from Sabine’s Charts in the * Phil. Trans.’ of the Royal Society (1845), and (2) from the Admiralty Charts for 1880, expressed in British Units, and converted into c.g.s. Units. 1880 1845 British C.G.8. British 698081 321871 6'87176 — 0275845 —'00127187 | 158464 — *523986 —°'0241595 — 58113 — *67352 —°0310546 — *73195 70513465 | ‘00236748 "27987 — ‘30013 —'0138385 — ‘07904 *602567 0277832 52644 —1:065495 — ‘0491279 —1:11386 *678817 ‘0312989 ‘91030 — ‘712584 — ‘0328558 — ‘79880 — *784390 — ‘0361666 — ‘61614 — °272348 — 0125575 — ‘59065 — ‘007649 — 0003527 — ‘11506 — ‘607671 — 0280185 — ‘61198 — 331346 — ‘0152777 — 41928 — °661354 — ‘0304937 — *58220 *300535 0129382 15864 — °044994 — 0020746 — *06274 ‘076635 0035335 12123 — *023517 — ‘0010843 — -011915 "241583 011139 *37369 ‘002980 *0001374 — ‘02346 02715 0012508 00433 *064652 0029810 07682 — ‘01512 —'0006970 =, — *01435 — ‘009531 —°0004394 — 02154 ‘003132 ‘0001444 — ‘00047 —1:254179 — 0578277 —1:30780 ‘039069 0018014 “28051 *297611 0137222 "16224 — 119841 — 0055256 — *23026 "5291705 "0243990 “58114 — °144530 — ‘0066640 — -06162 — °254829 — ‘0116484 — ‘27960 — ‘088692 — 0040894 ‘00861 "214592 “0098944 *11316 — ‘025210 —°0011624 "06455 — 069335 — 0031969 — ‘17877 — 146981 — ‘0067770 — *10697 084794 0039097 09392 “009588 0004421 “02851 "123986 ‘0057167 11457 ‘021780 00100425 ‘02029 01799 ‘0008295 02489 060462 0027878 “03984 — ‘00864 — ‘0003984 — 00414 — ‘049244 — 0022705 — ‘02920 — 005664 — 0002612 00390 C.G.S. 316843 9073065 — 026795 — 033749 012904 — 0036446 024273 — 051358 041972 — 036831 — ‘028409 — 027235 — 0053054 — 0282172 — ‘019332 — 026844 0073145 — ‘0028928 0055896 — 0005494 0172301 —'0010818 0001996 0035421 — 0006615 — ‘0009933 — 0000218 — 0602998 0129335 0074808 — 010617 026795 — 002841 —0128917 ‘0003968 "0052175 0029737 — 0082428 — 0049321 0043306 70013145 0052826 ‘0009355 . 0011477 0018370 — ‘0001908 —0013465 ‘0001799 DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 129 Comparison of the Values of the Magnetic Constants in British Units as deter- mined (1) by Gauss, (2) by Erman, (8) by Adams for 1842-45, (4) by Adams for 1880, with their yearly rate of increase from 1845 to 1880. Adams Yearly rate Constants Gauss Erman 1849-45 | 1880 of change gn 70155 6 9417 69777 6°8558 — *00325 g3 — 1672 + *0262 — ‘0124 + ‘1624 00466 g3 — 1430 — ‘4069 —- 5310 — 6194 — ‘00236 gr — $249 — °5937 — 6309 — ‘7207 —'00239 gi “6746 6149 "6145 5358 — 00210 hy —1:3545 —1:3036 —1:2622 —1:3166 —'00145 gh —1:0981 — °9659 —1:0598 —1:1014 —00111 ht — ‘0457 + ‘0156 + °0421 + °2818 00639 gh 9316 6477 ‘7300 “9505 “00588 hi +3622 3567 2631 1243 — ‘00370 Gua * —1:1563 — °8330 — “6904 — ‘7507 —00161 ht + °4858 — *0693 — ‘1081 — 2252 — ‘00312 93 + ‘0037 + ‘0271 — ‘0083 — ‘1154 — 00286 hz — °2956 — ‘2741 — °2547 — ‘2792 — 00065 93 — 5546 — ‘6664 — 6006 — ‘6057 —-00014 hg — 1725 — ‘1347 — *0884 + ‘0079 00257 Uri — ‘3470 — 3282 — ‘3376 — 4226 — "00227 aD *3226 2353 *2160 1169 — 00264 Gs + ‘0106 — °0276 — ‘0450 — 0627 —'00047 hi — 1421 — ‘1572 — ‘1470 — ‘1070 ‘00107 gi 1498 1455 0764 1209 00119 hi — ‘0013 + ‘0654 + 0847 + 0938 00024 9% + '0313 + 0194 + °0030 — *0234 —*00070 ht 0241 “0240 0218 0203 — 00004 The multiplier for the conversion from British units into c.g.s. units is 0046108. It will be seen on examining these tables(1) that g? and gfare numerically very much larger than g?, and (2) that the values of g? from the same. equations differ greatly according as g3 is or is not included, the value of gi being —‘0276 when gf is included, and —-:0124 when g? is excluded. It also appears from the comparison of the solutions when the equations of condition are included up to 774° latitude with the solutions above (1.e., stopping at 674° latitude) that g3=—-0126 in the first case, and —-0276 in the second case, and that this arises from the fact that the sum of the absolute terms in the final equation for g? is +:08815 when we stop at latitude 675°, and —-07184 when we proceed to latitude 774°. Hence a wide variation in the value of g3 is to be expected in the two cases, even when gf is included in both sets of equations. It also appears from the above tables that those constants in the values of which Gauss and Erman greatly differ are those which have undergone the greatest apparent changes in the interval from 1845 to 1880, and that the values for 1845 now determined for the most part agree more nearly with those of Erman than with those of Gauss.! The values of the magnetic constants have been determined from the » It should be remembered that before the excellent Admiralty charts of 1880, prepared by Captain Creak, the magnetic charts of the world were based on obser- vations which were insufficient and not distributed widely or regularly enough over the earth’s surface to lead us to expect a close agreement between the results of Gauss’s theory as derived from the earlier observations as compared with the later more trustworthy observations. 1898. K 130 REPORT—1898, equations for (X) and (Y) and from the equations for (Z) separately as well as from the equations for (X), (Y) and (Z) combined, and their values have been compared. Also their values have been determined in each case (1) by including all the equations up to (e), 7.e. between latitudes 674° N. and 674° S., and (2) by including all the equations up to (c), i.e. between latitudes 775° N. and 773° S., The following table gives the comparative values of the magnetic constants in British units, as deduced from different magnetic elements :— 1845 1880 From X Z, From X z or X and Y or X and Y ge 7012 6°952 6°869 6°877 g2 — ‘009 — ‘089 + ‘159 + ‘179 ge — ‘564 — 525 — ‘578 — ‘aT4 g — 596 — *846 — °800 — ‘630 ge + 173 — ‘115 + 245 + *329 g — 148 — ‘646 — ‘056 / — 005 gt 597 “605 497 536 ga —1:089 — 1-052 —1-097 | — 1-122 UE “682 675 “807 ‘973 gk — °704 — °726 — ‘709 — $73 ge — *858 — °722 — ‘620 — +643 Ge — ‘260 — ‘299 — +343 — "842 ga ‘000 — ‘013 — ‘098 — 126 93 — 596 — 617 — ‘590 — 628 G2 — 353 — 313 — 413 — +423 gz — ‘678 — *647 — ‘574 — ‘586 9k 416 206 156 165 g3 — °037 — -051 — ‘078 ~ ‘051 gi 093 “064 126 117 = — 028 — 019 — 032 + ‘005 g 221 "259 242 483 Gi — ‘001 + °006 — ‘018 — 028 g 023 030 029 — *016 gz 055 073 073 081 G2 — 013 — 017 — ‘013 — ‘016 Ge — O11 — -009 — 025 — 019 gé — 002 + 008 001 — ‘002 hi —1:287 —1-240 —1°273 —1°321 hi “043 "035 229 309 hi "285 299 190 152 hi — 192 — ‘063 — 284 — 192 hi 534 503 724 478 hi — ‘110 — 168 — ‘366 + 1223 hz — ‘247 — 260 — °265 — ‘289 h2 — ‘095 — ‘083 — ‘029 — ‘035 h2 176 *245 133 100 hz + 068 — 098 + °037 + 078 hz — ‘O11 — 120 — 172 — 176 he — ‘150 — 145 — ‘117 — -099 hz O77 091 092 096 = + ‘029 — *007 031 027 hz 026 205 135 098 hk 021 022 030 012 ht 025 012 051 003 hé 050 ‘070 054 028 hz — ‘009 — -008 — ‘006 — ‘002 he — 041 -- *056 — 029 — ‘029 DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 131 Another method of testing the accuracy of the work of determination of the magnetic constants is to substitute their values in the theoretical expressions for X, Y and Z, and to compare the results with the values of X, Y and Z as taken from the charts. For this purpose we have to form for each parallel of latitude the value of the expression 3 (4m +m) = Xigi + Kgs + Keys + (Xigh+ Xigi+ Xigé) cos A+ (Koha + Xihjg+ Xphj) sin r + (X2g2-+ X22) cos 2A + (X2h2+ X2Az) sin 2 r + (Xigi+ X8g3) cos 3A + (XfAj+ Xfhs) sin 3A + X4gt cos 44 + Xigi cos 5A + Xfhj sin 44+ XFh§ sin 5 A ; and also the value of the expression 2(Gm ay a») = Xoo a5 Xigt + Xe 8 + (Xigi+ Xigi+ Xig}) cos \+ (Xii+ Xi} + XZAt) sin d + (X3g3+ X3g?+ K2g8) cos 2d + (Kphp+ Xhi+ Xphe) sin 2V + (X3g3+ Xig2) cos 3A + (X3hj + XZh#) sin 3 r + (Xigi+ Xigs) cos 4d + (Xihi+ Xshg) sin 4 A + X595 cos 5A+ Xég8 cos 6A+ XZAF sin 5A + X Gh sin 6A; and then to form the sum and difference of these expressions for the yalues of X in northern or southern latitudes respectively, which may then be directly compared with the charts. Similar expressions must be formed in the same way for Y and Z for each parallel of latitude, and their sums and differences taken as in the case of X. When the values of the magnetic constants had been determined, they were substituted in the equations of condition for each belt of latitude, the terms of which when added up gave the theoretical value of the abso- lute term for that latitude. This calculated value of the absolute term may then be compared with the value of the corresponding absolute term derived from the observation which has been used in the solution of the equations. The following table gives some of these comparisons between the calculated and observed values of the absolute terms of the equations of condition for the period 1880, in the values of X and Z for gi, for A i and n odd, and for X, Y and Z for both g” and hi’ for m=1 and n odd. The observed values are taken from the Admiralty charts, and are the values used in the solution of the equations, and it will be seen by the comparison of the calculated and observed values that a chart drawn to give the results of the calculations would not differ much from the Admiralty charts. As a further test of the accuracy of the work in such laborious and extensive calculations, it is interesting to compare the values of the Gaussian constants as determined by different investigators from the observations for different epochs. K2 _- - 069-3— 089-3— — = 860- 6FI- — = * 60 - (8) - _- O19-3— £89-5— = - GFL #61 186-1 8ee-T ears Ha (| — _ 819-6— 189-3— _- — B08- BBE 899-6 699-6 r) Se0L 1) — _ £29.3— 189.3— _ — 8+ LIS. 668-8 816-8 | etron le Cay = — 0£9-6— 899.6— - — 6FL- ge. LIL LIL “2 “‘o08. (9) a _ 0FS-3— 919-3— - - 190-1. 600-T £929 862-9 * * 99a (ut) = _- SIF-3— IGF-3— - — 628-1 OPT FOL 896-2 * —* 908 (ur) = = | BFS £10-6— = = 08¢-T £PP-T £168 608-8 eres OD) am sea 80-6 — 010-5— = = LI9-T 899-1 0FO-6 190-6 * * 60h GD — - PIS: I— Fo8-1— — - PPT 169-1 08:6 018-6 “— Rosy. = _ 11¢-1— GF. — _ = 609-1 969-T £9F-01 987-01 S009) Cm) — = 882-I- | 9FB-1— — = 989-1 66F-T $20-1T 980-1T ee we) — = €£0-I— #96. — => _ FPP PPE-T ST9-TT SL9-1T “Se =mo00) ) = = | 081. — 069: — _- = Gee-L 6PL-L 660-21 190-21 * "949 (@) = — | = cor. — - _ _ 926+ _ SPF-Z1 “ya o00,- CP). = = | = | Fg = — = ¥69- — BSL-2L “= © oGh) (0) = — = 19. — - —- — SOPs = PLG-ZL * * 608 (q) = = | = 120. — oa 3 a 161 — OILS * '"o9g (8) Zz Z Z = 182-T— sIetT— || = = 99%. ole. =— = S962 886-2 “e* 2550:" (8) oO 866-I— FIS-IT— 90+ 910+ PLE OBE F8T- 161+ BCG-L TPG. Ne cae (2) — £08-T— 618-T— Ifl Tol Sie egg. abe. 698- TOLL 90T-L Pe. eee (dy) 11g-T— 868-1— FPG + 993+ BLE. 00F- BGT o6F- 968-9 888-9 * * eat (d) 1le-I— e8e-T— L148. 668: SbF. O9F- 109: 99. 909-9 869-9 * * 608 (0) eB Ole-T— L88-1— £e9. are. 18a. Tee: 98% LPo. 092-9 6FS-9 * * 993 (a) & B08-1— 988-1 — 989- SOL. 119. 909+ 068: 99F- 198-3 198.9 * * 60g (ur) a 883-T— 638-1— 6F8+ IL8: 189+ GLO 093- 928. ShP-9 BEF Pana ods 4G) Q 993-T— o1g-1— T00-T 960-1 GPL. LoL. 910: laaG 166-4 986-F * * e0F (3) = 616-I— 186-T— €SL-T e9LL ¥08- FEB: FIL— 690: — 919. 929-6 D STAM) 9LT-IT— $o6-1— 986-1 PEGI B88. $88: 886-— €8o- — 090-F 890.5 * "909 (a) WLI— O1S-1— 188-1 683-1 198. 186- 8h. — o8y — | 819-8 689-8 * * 989 (8) 690-[— FOLI— || OlmT 886-1 G18. | 996. 699-— Lg — | 660-8 160-8 oe oD Oa Sa) £00-I- | FILI— GFT 6FG-T 698. 66+ $99— | ¥6L. — OL9G | 819% oe 690 £8} = 990-1~ = G8T-T = | BIO-T — 968- — = FILS * o0L (PD : — P0-1— _ ZOL-T — GG0-T = 696. — | _ | 009-1 * * 6G (2) — 166. — || = 180-1 _ 620-1 = ¥00-[— — 910-1 J) 3? 0s™(a) - 696. — = 616 _ 120-1 — 920-T— _ 0F9-0 * + 998 (8) paaresqo pazBno[sp paarlesqo pezs[noleg pearasqo peyernoleg paarasqo paqepnorep paaresqo payeMoep 4 x Kk x x sopnaney ppo uv pu [=u 107 ppo uw pus [=w 107 ppo wu pus [=u 10,7 ppo vu pus [=w 10 ppo uw pus 0=w IOT uBayy {Y Joy suolgunby a2 uy 14 x0; suoyyunby oq9 UT 04 toy suorqenby 013 UT i] inn) wu u nae ‘O88 yoodgy ay2 of wy pun wb buyymsrgaq of suoyondy ey? fo suey agnjosgy yz fo samyA paawasggQ pun pajvjnojyg ay, fo waf v uaaajaq wosruduog a on 133 The following tables give some comparisons. The first of these tables ives the values of the first twenty-four constants (i.e, of those to the fourth order) as determined by Gauss for 1830, by Erman and Petersen, by Adams (1) from Sabine’s charts for the epoch from 1842-45, and (2) from the Admiralty charts for 1880, and by Neumayer for 1885, as pub- lished in Berghaus’ ‘ Physical Atlas.’ DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 1829 ; 1830 1845 1880 1885 Constants pean Gauss Adams Adams Neumayer g° +°320074 + 323477 321871 *316843 *815720 g3 + 001210 —*007708 —'001272 ‘007306 ‘007906 g3 — ‘018763 — 006593 —*024159 — ‘026795 — 024363 ge —°027377 — 038035 — 031055 — 033749 — ‘034395 It + 028353 + 031106 027783 *024273 024814 ga — ‘044537 —'050635 —°049128 —°051358 — ‘049798 gh + 029863 + 042956 "031299 | *041972 “039560 gi — 038405 —°0538291 —°032856 — ‘036831 — ‘030597 hi —'060109 — ‘062456 —'057828 — 060300 — ‘060258 hi +°000720 — 002107 ‘001801 012933 012999 hi + 016446 +°016700 013722 ‘007481 ‘007383 hk —°003197 + 022402 — "005526 — 010617 —°011877 z + 7001249 + 000172 -- 000353 —*005305 —*005667 93 — ‘030728 —'025575 —'028018 — ‘028217 —'027857 92 — 015592 —'016000 —'015278 —'019332 — 019754 h2 —°012637 — 013631 — 011648 — ‘012892 — 012604 he — 006211 — ‘007955 — ‘004089 000397 — 000443 E + 010851 + ‘014876 “009894 *005217 ‘007147 gi — 001272 + 000488 — ‘002075 — ‘002893 —'003270 gi + 006708 + 006909 “003533 "005590 ‘006842 hs — 007248 — 006552 —°006777 — 004932 — 005492 he + 003014 — ‘000062 -003910 004331 005121 gi + 000895 —°001442 ‘000137 —'001082 — 000849 ht + 001109 +°001109 “001004 “000935 “000968 Tf we had expressed the magnetic potential and the magnetic forces, X, Y and Z in terms of the functions Q”, Q”, &c., instead of in terms of H™, H™, &c., we should have obtained another series of magnetic constants but the two series are related to one another, and the one series may be derived from the other by multiplying each constant in one series by a factor depending on the values of m and m. Thus let a™ and 6" be two magnetic constants derived from the function Q” (as defined above), and let a, and £, be the corresponding Gaussian magnetic constants as derived from the function Hy. Then these magnetic constants a7 and 67’ are connected with a, and 8, by the relations @ PBn_Qn 1.3.5 * * + * (Qn—1) Gao Oy (~—m) ! for a given value of m ; and similarly On, Bm — Qn, = 1.3.5 *** * (2m,—1), ; fo, H,. (m—m) ! ‘ and in particular Gye Pas Qn—a 1.3.5 > +++ (2n—5) a -() Sie : ar (n—m—2) ! dinars Quen — 13.5 * +++ (n+) HS), (n—m-+2)! and Gira Onis 134 REPORT—1898. then we may find the final equations for a, and 6, from the final equations for a, and £, respectively by multiplying the final equations by Q,. and then substitute the values of a, and £,, in terms of a, and 6, respectively. Hence, in the final equations for a, and £,, the coefficient of a, or of B, will be multiplied by (%) on (= eh Cea)" H,, (n—m) ! in order to find the coefficients of a, and 6, respectively. Also the coefficients of a,_, or of B,,, in the same equations will be multiplied by Qn-Qn-2 op 1:35 °° 7 (2n—1).1.3.5 ++ + + (Q2n—5) HE (n—m) i” (n—m—2) ! to find the coefficients of a,_, and 6, _, respectively. And the coefficients of a,,. and £,,, will be multiplied by Q,Qne2 op 1-3-5 °° °° (2n—1).1.3.5-> + + +(2n+38) HU. (n—m) ! (n—m-+2)! to find the coefficients of a,,. and 6,,». Or generally the coefficients of a, and 8, in the final equations for a, and B, will be multiplied by — to find the coefficients of a,, and b,,, in the corresponding final equations. Hence the constants a and 6” will have to be multiplied by Qi 5 ties Hy nome cc ley me e ma a) in order to obtain the corresponding by the factor - Gaussian constants a, and ,. Again, let A,, B, be two magnetic constants connected with a, and /,, by the relations ay, pas - +--+ (2n—1) A, B, H, [(n—m)! (n+m) !]* Then the values of the magnetic constants A,, B,, &c., as determined from the function II,, can be converted into the corresponding Gaussian magnetic constants derived by means of the function H,, by multiplying each magnetic constant A” or B” for each value of m by the factor Ty 1.3.5 * Seen 1) H” [(n—m)! (n+m) ie In his paper in Vol. I., No. 1 of ‘ Terrestrial Magnetism,’ published January, 1896, at the Chicago University Press, Dr. Ad. Schmidt has introduced a symbol R%, which is connected with the symbol II” employed above by the relation Ri=vV (2n+1)e TI? where e=1 when m=0, and e=2 when m >0. DETERMINATION OF THE GAUSSIAN MAGNETIC CONSTANTS. 135 Hence in Sn ne LOnpecd VIL (2 ere } FETT 8.5 On a By means of this factor the magnetic constants determined by Professor A. Schmidt for 1885 may be converted into Gaussian magnetic constants, for the sake of comparison with the magnetic constants as determined by Adams for 1880, and by Neumayer and by Fritsche for the epoch 1885. Comparison. of the Values of Gaussian Magnetic Constants to the Sixth Order in Centimetre-gramme-second Units. Adams Neumayer Schmidt Fritsche 1880 1885 1885 1885 9 316843 *315720 -317346 “31635 9 0073065 007906 -007849 00526 93 —-026795 — 024363 —-023415 — ‘02556 9. — -033749 — 034395 —-034781 —-04014 2 012904 st 013320 01208 9° — 003645 a —-003932 — 01285 1 -024273 024814 023556 02414 gh —-051358 —-049798 —-048954 — 04962 a ‘041972 039560 -037750 ‘03807 gx —-036831 — -030597 — 028389 —-03104 g: —-028409 = — 040125 — ‘03028 1 — 027235 _ — 004089 —+01686 G3 —-005305 — 005667 —:005868 —-00589 G3 —028217 — 027857 — ‘027667 — ‘02667 92 — ‘019332 —-019754 — 020192 — 02128 G2 — 026844 = —-021920 —-01961 G2 0073145 = -008082 00572 Gg —-002893 —+003270 — 003158 — ‘00368 Gg 005590 006842 006463 -00601 Gg —000549 = —:000780 — 00272 G3 017230 = 015668 01503 Wr — 001082 —-000849 —-001176 —-00063 @ -000200 — 000147 00134 93 003542 = ‘00118 -00200 g2 —-0006615 = = — -00064 G —-000993 = _— —-00032 gs —-000022 == _ -00029 ht —+060300 —-060258 — 059842 —-05914 ni -0129335 012999 012432 -01307 hi 007481 007383 009073 ‘01005 Ai —:010617 —°011877 —'015772 — 01381 ht 026795 = 027312 03647 hi —-002841 — —-017039 —-01796 hy — 012892 —-012604 —-013342 —‘01230 hz -000397 —-000443 — 000512 -00013 hz 0052175 007147 006691 00652 he 002974 = 002549 -00227 he —:008243 — —-009699 —-01122 hg — 004932 —005492 -- 005396 — ‘00555 a3 004331 005121 004706 00525 hz ‘0013145 = 001093 —-00049 hi 005283 = -006267 00757 ht 0009355 000968 000555 -00103 ht 001148 Ss 001692 00132 hg 001837 wa 001377 -00346 hi —-000191 = = — "00043 he —-0013465 — = 00186 ns 000180 = = 00011 136 REPORT—1898. The above table gives the values in ¢.g.s. units of the Gaussian magnetic constants, as determined by Adams for the epoch 1880, and by Neumayer for 1885, by Schmidt for 1885, and by Fritsche for 1885. The last two determinations by Schmidt and by Fritsche were derived from the observations employed by Neumayer, and the values of the Gaussian constants, corresponding to those published by Schmidt in the first number of the journal ‘Terrestrial Magnetism,’ are obtained by multiplying each magnetic constant by the value of the above factor Rn ¢ Hn © that constant. n Stream-line Motion of a Viscous Film. [Ordered by the General Committee to be printed in extenso. | (I.) Experimental Investigation of the Motion of a Thin Film of Viscous Fluid. By Professor H. 8S. Here-Suaw, LL.D. Art the International Congress of Naval Architects at the Imperial Insti- tute in July of last year the author read a paper on the ‘Nature of Surface Resistance,’ and there showed by means of lantern experiments that the flow of water round solids of various forms could be made visible by injecting air into the flowing water. In response to an invitation from the Institute of Naval Architects to read a second paper on the subject, he endeavoured to investigate the nature of a very well defined border line which existed in all the experiments when air was used, such as by employing water under various conditions, injecting coloured fluid into the flowing mass on the skin of the bodies in the path of fiow. In endeavouring to investigate the markedly different condition of flow at the surface, instead of using a thick sheet of water of from three-eighths to half an inch, a thin sheet of water was employed the thickness of which was not greater than that of the abovementioned border line. The result of doing this was to reveal a different state of flow in the water, in which, though the air method now failed, colour bands remained stable and enabled the behaviour of the water to be clearly seen. | The hypothesis had been advanced in the first paper that, while the general body of the water in the thick sheet was moving with sinuous or turbulent motion, the water near the skin (which of course corresponds with that of the thin sheet) was in a state of parallel flow. The author, by means of a formula which Professor Lamb was good enough to furnish him with, found that within reasonable limits of error true stream line flow took place under these conditions, and gave a number of illustrations of this method of obtaining the form of stream lines round bodies of various cross section and in channels of various forms. (1.) The Two Lines of Research possible by means of the Method of Thin Sheets. It is obvious that there are two lines of research for which this method might be employed. The first of these is the investigation of the properties of fluids by using sheets of different thicknesses and varying ' The reproduction of the experimental results and diagrams which illustrated the reading of this paper are given in Engineering and The Engineer. ON STREAM-LINE MOTION OF A VISCOUS FLUID. 137 conditions of velocity of flow in questions of such importance as dis- continuity of fluid motion and viscosity. The second purpose for which this might be employed was obviously to investigate the nature of stream line forms in many cases in which mathematical investigation was impossible, not merely for the case of flowing water, but in ‘applications to heat and electricity. It was in experimenting with various liquids with the first mentioned object in view that much better results were obtained than those given with water, and after working out the test case with various fluids (including water) under new and more rigorous conditions, these results, together with certain new experiments, are brought before the Associa- tion. (2.) Description of Improved Apparatus. In the earlier apparatus the main body of water was supplied in a thin sheet by the pressure from the mains, coloured water being intro- duced from a small reservoir kept under pressure by means of a hand pump. Since exhibiting these experiments in the earlier part of the year at the Royal Society, improvements have been made both in the general mode of applying the fluid to the lantern apparatus, and also in the lantern apparatus itself, thus rendering the appliance suitable for either physical or engineering lecture purposes, as well as for actual experi- mental work. The arrangement consists of a lantern and two vessels, one containing clear liquid and the other coloured liquid, connected by two pipes with the lantern-slide. A pipe leads to the reservoir of compressed air, which is attached to a circular cap, with which the vessels of liquid are con- nected. Taps enable the connection between the lantern-slide and receiving-vessels to be adjusted, the annular pipe with which the air. is connected passing down to the bottom of the connecting-vessels, whereas the taps are so arranged that the pressure of air from the reservoir comes upon the surface of the liquid in each vessel. The containing vessels- which have been used up to the present are ordinary glass aérated water- bottles, capable of sustaining 2001b. per square inch. At the head of the pipe on each containing-vessel a separate pressure gauge can be attached, as well as on the reservoir itself, so that the pressures can be adjusted accurately for any particular experiment. If different liquids are required to be used, they can be connected with the circular head, without the necessity of disconnecting the other containing- vessels. The chief object with which this arrangement was designed, however, was to enable high pressures, such as from 1001b. to 200 lb. per square inch, to be employed when very thin sheets of liquid are used, a high Sagi being necessary under such conditions in order to insure the ow. With regard to the lantern slide itself, the original apparatus, although effective, was troublesome to make and manipulate, and did not insure absolute uniformity of the thin sheet, or lend itself to rapid changes. The new device merely consists of a small brass block containing two chambers. It has two pipes projecting from it, communicating with the chambers, one pipe being connected with the vessel of clear, and the other with the vessel of coloured, fluid. The small brass block is merely inserted between two plates of glass, together with a third exactly the same thickness as itself. By then making in thin cardboard, paper, lead 138 ' REPORT—1898. foil, or other material a border, together with the required obstacle or channel, and clamping the whole together, an effective and simple lantern- slide is obtained. (3.) Result of using Liquids other than Water. The four liquids other than water which were experimented with were castor oil, glycerine, alcohol, and mercury, of which glycerine is so entirely and surprisingly satisfactory in every respect as to make it undoubtedly the best material which the author had hitherto worked with for obtain- ing stream-line figures, and the whole results shown at the reading of the present paper were obtained by using glycerine. Of course after the glycerine has once passed through the lantern slide the coloured portion has mixed up with the clear, and it can only be employed again for colour bands, but at the same time the thickness of the sheet of flow being small, while the velocity with which perfect results can be obtained is low, there is no reason why this material should not be always employed. Alcohol has such a low viscosity that it can be employed in sheets of remarkable tenuity ; but these sheets have naturally the disadvantage of giving colour bands so thin as to be scarcely capable of photographic reproduction, while the volatile nature of this substance makes it not altogether desirable in close proximity to an are lamp. Mercury is of course opaque, but its great density compared with its viscosity makes it most valuable in connection with some experiments, and its lines of flow can be traced if it is not quite pure by marks it leaves on the glass. It is, however, troublesome, since it cannot be used in con- nection with brass taps or with the brass lantern apparatus. Castor oil also proved troublesome to work with. (4.) Measurements made to compare the Flow with Water, Glycerine, and Alcohol in Test Cases, and Explanation of these Results. In the test cases above referred to Professor Lamb kindly sought for and obtained an equation for the stream lines round a cylinder in a parallel channel, and the results of the measurements, although warranting the use of water under these conditions, showed that the flow was not in absolute agreement with the lines plotted from the formula. The author then remarked :—‘A though the differences are appreciable, they are to some extent of a nature which must be attributed to the great difficulty, in the first place, of making sufficiently accurate mechanical arrangements, and also from the fact that it takes some little time to plot down the results ; and that, during this time, it is extremely difficult with the present appliances to keep a perfectly steady and uniform pressure both of the colouring bands and the main body of the water, when each comes from a separate source. Beyond this, however, there is no doubt that the stream lines are slightly pushed away from the obstacle at the point of greatest velocity, 2.¢., abreast the mid-section. This may be due to the slight effect of viscous resistance parallel to two containing glass boundaries.’ In view of the importance of the matter it seemed worth while to attempt a new and more accurate comparison of the experimental results with the flow for a perfect fluid. In the previous case the ’ ON STREAM-LINE MOTION OF A VISCOUS FLUID. 139 formula used was only an approximation, though used within limits that should give a very fair accuracy. Now it was not really necessary to use the special formula for a channel at all, since if one of the cases be taken in which exactly mathematical results can be obtained for an infinite fluid —e.g., a cylinder—it is only necessary to form a border for a given value of the stream function, and the test could be made and stream lines suitably plotted within the artificial border. Glycerine is capable of being used at very low velocities, and is absolutely steady in flow—indeed, owing to its viscosity the lantern slide may be actually removed with the pipes dis- connected, and after a lapse of even half an hour the stream lines remain perfectly clear and distinct. It therefore seemed possible to make an absolutely severe and final test, and the case of a cylinder and infinite width of fluid were taken, the stream lines being plotted from the well- known formula. This plotting was done by Mr. E. Brown, B.Sc., University and 1851 Exhibition Scholar, who kindly undertook this particular work for the author, besides rendering him valuable assistance with the experiments for the present paper. On plotting the ae lines on a large scale, it was noticed that at a distance from the cylinder corresponding to the distance at which colour bands had previously been admitted, the stream lines were by no means equally spaced, and moreover they were far from parallel to the direction of flow of the fluid at infinity. To overcome this difficulty the stream lines were extended to such a distance from the cylinder that they became for all practical purposes parallel to the direction of flow at infinity. The thin film slide was lengthened by a corresponding amount. Further, it was noticed that at that distance the lines on the diagram, which represent the theoretical stream lines, have a displacement from the lines which correspond to the equal spacing of the stream lines only actually attained at infinity. The colour bands were therefore admitted to the film by holes which were so spaced as to correspond with the dis- placement of the theoretical lines. The following three conditions were therefore introduced into the test experiment, viz.— 1. Theoretical stream line as boundary. 2. Longer film. 3. Unequal spacing of stream lines. It was then found that the actual colour bands were in absolute agreement with the theoretical lines. It must be remarked that in the previous verifications referred to the author had been content to throw the lantern picture so as to most nearly approximate with the theoretical diagram, which involved an obvious displacement of the section of the cylinder itself, but in the present case no such approximation was allowed in the border ; the obstacle in the lantern itself was placed in absolutely exact position, so as to coincide with the border on the plotted diagram. It need scarcely be said that this result was not obtained without much laborious work, and it is highly gratifying to know that the correctness of the result has been verified mathematically in the accompanying paper by Professor Sir G. G. Stokes, the conditions which it there states as necessary—viz., considerable viscosity and very thin sheet—being both found necessary in order to obtain the theoretically correct result. It should be noted that on the large scale in which the comparisons were made by the lantern there is not the slightest 140 RKEPORT—1898. difficulty in detecting minute variations, and no hesitation or doubt as to when accurate agreement is obtained. Both water and alcohol have been tried in a similar test case, although the conditions are much more difficult to comply with in these cases, thin sheets, such as y;\; th of an inch, which have to be used, making the experiments much more difficult. The results of stream-line flow by this method may therefore be received with confidence, and a number of cases of stream lines have been obtained by using glycerine. These experiments were made in the first case with the view of studying discontinuity under conditions which involve a severe test of the stability of the thin film, which was through- out of a thickness of ,},th of an inch, and in all cases forty-one colour bands were used within a width of about 3 inches. Without the figures themselves, which, as already mentioned, are published elsewhere, it is impossible to do more than describe the general results; but it may be said that the difference between using square corners and rounded edges is very marked ; indeed, it was a matter of surprise to find the flow main- tained so well over the sharp edge at all. It is evident that the liquid which actually adheres to the edge of the obstacle enables a definite though very minute rounding to take place at the corners, as is visible by a close examination of the photographs. This was especially marked in one case on one side of an experiment, whereas on the other side, when the entering colour band actually touches the edge, the sharp corner takes effect upon it, and completely breaks it up, destroying the continuity of flow. It may be said that in these examples the narrow portion of the orifice is so small that it is impossible to detect the separate bands which pass © through that portion ; these colour bands, nevertheless, emerge quite distinct from each other, and finally assume their original position in the wider portion of the channel. One example may specially be mentioned, viz., that of a flat plate inclined at 45° to the stream. The agreement of this case with the theoretical result of Professor Lamb the author has previously been able to verify in the case of water, but even with the greatest care it was always possible to tell in which direction the stream was flowing. With glycerine, however, the colour bands are practically identical before and behind the plate ; and if it were not for the point being clearly evident at which the central divided band reunites, it would be impossible to tell which way the stream is flowing. This point of union of the two portions of the central band is extremely interesting, as a careful measurement of it verifies the exact position at which the central stream line meets the plate, and is found to agree precisely with the mathematical solution of the problem. (5.) Method of Investigating Effects of Variable Resistance. In order not to prolong the present paper beyond reasonable limits, the author will only briefly mention a method by which variable resistance can be dealt with. If within the thin sheet of flowing liquid an obstacle of some transparent material less in thickness than the sheet itself be placed, the flow will take place partly over the obstacle and partly round it. This effect will correspond to that of an obstacle through which fluid can flow, but which opposes resistance greater than the remaining portion of the thin sheet. ON STREAM-LINE MOTION OF A VISCOUS FLUID. 141 The converse effect can be produced by making a part of the thin sheet rather deeper than the remaining portion. This of course will correspond to the flow through an obstacle of similar shape, which opposes less resistance than the surrounding space. The effects are obviously the same as would be produced in the first case by a dia-magnetic body, and in the second case by a para-magnetic body, and by varying the relative thickness of the different portions of the sheet it is clear that the effects which would be given by the body of any known resistance (7.e., of any value of ,) can be produced. The author at first attempted to produce these results by very thin sheets of glass. It was seen that where the stream meets the edge an effect corresponding to refraction is produced, but that while in the case of the plate touching at both edges, although the velocity must obviously be greater over the portion where the plate is partly obstructing the channel, that is, makes the channel rather shallower, the width of the colour bands remains the same. When, however, the obstacle does not touch the edges, the effect is to produce very much wider bands over the obstacle itself and narrower bands on either side, these bands giving an indication of the great difference of velocity which results from the greatly increased resistance over the surface of the obstruction. Instead of considering merely the actual width of the bands, it is of course possible, and generally more convenient, to consider the number of bands in a given space. This method is applied to a circular hole in a plate of different cross sections to the film itself, which is placed across the entire width of the channel, and the number of bands or stream lines in a given space in the hole or well is obviously greater than in the surrounding portion—.e., the bands are close together, and the velocity correspondingly greater. This result evidently represents the effect of placing in a uniform magnetic field a circular cylinder of soft iron—i.e., a para-magnetic body. This sufficiently indicates the method, but other examples may be given, the first two representing para-magnetic and dia- magnetic cylinders, which are cases which can be dealt with by means of mathematics ; also two other cases of cylinders of rectangular section, representing respectively the result with para- and dia-magnetic bodies, which are cases it has been hitherto impossible to deal with by mathe- matical methods. (6.) The Effect of Using a Wedge-shape Section. The author attempted to solve the problem of obtaining the flow round a solid of revolution by using a wedge-shaped section, the obstruc- tion being also represented by a wedge representing a segment of the body, the thinnest part of the wedge corresponding to the axis of revo- lution. Professor Stokes has been good enough to look into this matter, and has found that the partial differential equation which the stream-line function must satisfy in the case of a slender wedge of viscous fluid is dy dy 3 du_ kay pity hace 1) da? dy? y dy ’ x being measured parallel and y perpendicular to the edge ; whereas, for a perfect fluid flowing axially over a solid of revolution, generated by the ‘ 142 REPORT—1898. revolution round the edge of the wedge of the body interrupting the flow in the wedge of fluid, the equation is Py Py 1 dy_o dx? dy? ydy ” which is not the same as the other, and therefore the stream lines are not the same in the two cases.! If we compare together the case in three dimensions given by Pro- fessor Lamb of the flow of a perfect fluid round a sphere and the case actually obtained by this method with glycerine, it will be noticed, as might have been expected, that the lines round the section of the sphere are crowded much more closer together for physical reasons which are easily explained ; for it is obvious that, as the whole of these effects depend upon viscosity, the effect of viscosity diminishes in the thicker portion of the wedge in such a way as to make the general velocity of flow greater, and hence the stream lines round the obstacle are not deflected from their path to the same extent as they would be if they were of uniform flow in a parallel portion of the stream. One result, however, of great interest was obtained, and that was that with less viscous fluids, such as water, the exact point at which the colour bands broke up could be traced by this method, and the flow studied side by side with stream-line motion. This leads the author, in conclusion, to bring forward an experiment upon continuity with thick sheets, which it may be interesting to show, as indicating clearly the great difference between the flow according as the motion is sinuous or otherwise, and particularly as throwing some insight into the birth of eddies, at the sharp edges of the body. The obstacle itself is of wedge-shape cross section, the edges of the wedge being ground as sharply as possible. Coloured liquid is now allowed to flow behind the plate by means of a small orifice, and the effect can be immediately seen. As long as the water is flowing steadily, the shape of the curves formed by the clearly marked border between the dead water and the water flowing over the edges of the plate agrees more or less with that given by calculation. When, however, the flow, instead of being steady, takes place in a series of impulses, the: exact character of the succession of eddies formed at the sharp edges of the plate is clearly seen. 1 Since this paper was read Professor Sir G. G. Stokes has further investigated the matter, and has been able to obtain the equation of the stream lines for the case of a slender wedge of a viscous fluid interrupted by a wedge forming a section of a sphere, which he finds in terms of polar co-ordinates to be as follows :— a’ int @= = nt ) sin @=constant. The two following equations, therefore, may, for convenience, be expressed thus : Case of flow of perfect fluid round a sphere: ( Ve <) 7? sin? @= constant. 73 Case of slender wedge with spherical sector : (: - a) 7* sin* = constant ; and Professor Stokes remarks that the equation shows, even without plotting, the general character of the difference between the wedge lines and spherical lines. ON STREAM-LINE MOTION OF A VISCOUS FLUID. 143 (II.) Mathematical Proof of the Identity of the Stream Lines obtained by Means of a Viscous Film with those of a Perfect Fluid moving in Two Dimensions. By Sir G. G. Stoxgs, /.A.S. The beautiful photographs obtained by Professor Hele-Shaw of the stream lines in a liquid flowing between two close parallel walls are of very great interest, because they afford a complete graphical solution, experimentally obtained, of a problem which, from its complexity, baffles the mathematician, except in a few simple cases. In the experimental arrangement liquid is forced between close parallel plane walls past an obstacle of any form, and the conditions chosen are such that whether from closeness of the walls, or slowness of the motion, or high viscosity of the liquid, or from a combination of these circumstances, the flow is regular, and the effects of inertia disappear, the viscosity dominating everything. I propose to show that under these conditions the stream lines are identical with the theoretical stream lines belonging to the steady motion of a perfect (7.¢., absolutely inviscid) liquid flowing past an infinitely long rod, a section of which is represented by the obstacle between the parallel walls which confine the viscous liquid. Take first the case of the steady flow of a viscous liquid between close parallel walls. Refer the fluid to rectangular axes, the origin being taken midway between the confining planes, and the axis of = being perpen- dicular to the walls. As the effects of inertia are altogether dominated by the viscosity, the terms in the equations of motion which involve products of the components of the velocity and their differential coefficients may beneglected. Gravity, again, need not be introduced, as it is balanced by the variation of hydrostatic pressure due to it. The equations of motion, then, with the usual notation, are simply dp. (du , du os) dx (a ih dy? a dz? ]’ with similar equations for y, v and 2, w, » being the coefficient of vis- cosity. A the present case the flow takes place in a direction parallel to the walls, so that w=0, and the third equation of motion gives 2 = 0} 'so Ps that » is constant along any line perpendicular to the walls. The velo- cities w, v, vanish at the walls, and along any line perpendicular to the walls are greatest in the middle. As by hypothesis the distance (2c) between the walls is insignificant compared with the lateral dimensions of the obstacle, the rates of variation of u and v when x and y vary may be neglected compared with their variation consequent on that of z. Hence the equations of motion become simply dee" dee” dy" ae? @) which must be combined with du dv he esa temal()i 2 da i dy : .) Over an area in the plane wy, which is small compared with the obstacle, though large compared with c?, the whole velocity and each 144 REPORT—1898. component vary, as we know, as c?—<* ; so that if w', v' denote the mean components along a line perpendicular to the walls 2 o2 usu! (1 _ 2 os se (1 _ *), and (1) and (2) give : 1 a + Sones wae —— ote (3) If W be the stream-line function, taken, say, with reference to the mean velocities w!, v', dy= u'dy—v'dx, and the elimination of p from the first two equations (3) gives de dy? i (4) ' The general partial differential equation (4), combined with the condition that the boundaries shall be stream lines, serves to determine completely the function Y. It may be remarked that the lines of equal pressure are the orthogonal trajectories of the stream lines, and can therefore be drawn from the photographs. If we suppose the stream lines equally spaced out in a part of the fluid where the flow is uniform in parallel lines, the velocity at any point will be inversely as the distance between consecutive stream lines. This statement is subject to a qualification which will be mentioned presently. Let us turn now to the other problem, that of determining the stream lines for the irrotational motion in two dimensions of a perfect liquid flowing past an infinitely long body, a transverse section of which, by two close parallel planes, would form the obstacle in our thin plate of highly viscous liquid. In this case the stream line function satisfies the same partial differential equation (4) as before, and the conditions at the boundaries are the same, namely, that the boundaries shall be stream lines. Therefore, notwithstanding the wide difference in the physical conditions, ‘the stream lines are just the same in the two cases. In this latter case they cannot be almost realised experimentally by means of an almost perfect fluid on account of the instability of the motion. The orthogonal trajectories of the stream lines are lines of equal velocity-potential, but not in this case lines of equal pressure. It may be objected that the stream lines cannot be the same in the two cases, inasmuch as the perfect liquid glides over the surface of the obstacle, whereas in the case of the viscous liquid the motion vanishes at the surface of the obstacle. This is perfectly true, and forms the qualifi- cation above referred to ; but it does not affect the truth of the propo- sition, which applies only to the limiting case of a viscid liquid confined between walls which are infinitely close. Any finite thickness of the stratum of liquid will entail a departure from the identity of the stream lines in the two cases, which, however, will be sensible only to a distance from the obstacle comparable with the distance between the walls, and therefore capable of being indefinitely reduced by taking the walls closer and closer together. ON TABLES OF CERTAIN MATHEMATICAL FUNCTIONS. 145 Tables of Certain Mathematical Functions.—Report of the Committee, consisting of Lord Kertvin (Chairman), Lieut.-Colonel ALLAN CUNNINGHAM (Secretary), Professor B. Price, Dr. J. W. L. GLAISHER, Professor A. G. GREENHILL, Professor W. M. Hicks, Major P. A. Macmanon, and Professor A. LopGe, appointed for calculating Tables of certain Mathematical Functions, and, of necessary, for taking steps to carry out the Calculations, and to publish the results in an accessible form. Tur new ‘Canon Arithmeticus’ is a set of tables showing the solutions of the congruence of 2*=R (mod. m) forall prime moduli (m=p) < 1000, and also for all powers of primes as moduli (m=p”’, p,? &e.) < 1000. The tables are twofold, one showing the value of R to argument x, the other showing the value of x to argument R. The tables are on the same plan as Jacobi’s ‘Canon Arithmeticus,’ differing therefrom only in that the same base 2 is used throughout, whereas Jacobi uses a primitive voot of each prime as base; these primitive roots (e.g. 967) are often very inconvenient for purposes of practical computing. The tables are now complete (in MS. 133 foolscap sheets), and ready for printing. All the work has been done by two independent computers : the work of each has been checked with that of the other ; all discrepancies found have been examined anew and set right. Experiments for improving the Construction of Practical Standards for Electrical Measurements.—Report of the Committee, consisting of Professor G. CAREY Foster (Chairman), Mr. R. T. GLAZEBROOK (Secretary), Lord Ketvin, Professors W. E. Ayrron, J. PERRY, W. G. Apams, and OLiver J. Lopar, Lord Ray.eicu, Dr. A..- Murruead, Mr. W. H. Preece, Professors J. D. EVERETT and A. Scuuster, Dr. J. A. Fueminea, Professors G. F. FirzGEraLp and J. J. THomson, Mr. W. N. Suaw, Dr. J. T. Borromiey, Rev. T. C. Firzpatrick, Professor J. VirtamMu Jones, Dr. G. JOHN- STONE STONEY, Professor 8. P. Taompson, Mr. J. Rennie, Mr. E. H. Grirritas, Professor A. W. Ricker, and Professor A. G. WEBSTER. AVPENDIX PAGE I. Comparison of the Standard Coils used by Professors J. Viriamu Jones and W. £. Ayrton in their determination of the absolute resistance of Mercury with the Standards of the Association. By R.'T. GLAZEBROOK, F.R.S. . 147 Il. On the Determination of the Temperature Coefficients of treo 10-ohm Standard Resistance Coils (Nos. 3873 and 3874) used in the 1897 deter- mination of the ohm. By M.Souomon. . a - : - - Lol II. =" Ampere Balance. By Professor W. E. AYRTON and Professor J. V. ONMASEenrrame rota 3 |. Be hE deh é 5 pein” Ade 6 mpebnllng Tue work of testing resistance coils has proceeded as usual during the year. The following is a list of the coils tested and of the values found in “ia ee of the list published in the Report for 1896 :— : L 146 REPORT—1898. TABLE. No. of Coil | Resistance of Coil in Ohms! Temperature Miliofif 333 4c? aeypat ¢, No. 459 9:9953 13-49 Elliott, 322 o, No. 460 099662 13'6° Elliott, 357 ; F -o No. 461 9°9938 13°5° Elliott, 356 G, No. 462 ‘99921 136° mot, S68. eS, 6, No. 462 100 (1—:00051) 134° Nalder,5329 . |, @, No. 464 100 (1—-00049) 12:8° Nalder,5330. . . ¢, No. 465 | 1000 (1—-00083) 12-6° adn. Co.” eaten G, No. 466 | ~ 1:00032 15.8° Muirhead, 6271. . . QD No. 467 99722 15:9° Elliott, 329 =... @ No. 469 99994 15-9° Paul, 39 =... No. 470] 10-0029 166° Paul, 50 ee TE ¢, No. 471 1000 (4:00048) 167° Nalder, 3873 . . ¢, No. 367 9-9901 13-9° Nalder, 3874 . .; ¢, No. 362 9:9896 13-9° Resistance in B.A. Units BAU Te 0) 8 ee lay G No. 468 1:00021 17-42 The most interesting of the coils are those numbered G, 362, 367, 389, 390. (See Appendix I.) Of these iy 367 and Ki 362 are two ten-ohm coils of platinum silver and Nos. g, 389 and ¢, 390 are two tenth-ohm coils of manganine ; the values of these are given in Appendix I, These were made for Profes- sor J. V. Jones’ experiments on the value of the standard of resistance, and were compared with the standards of the Association in 1893 and 1894. It appears from the further comparisons, an account of which is given in the Appendix to this report, that Gg, 367 has changed by possibly three or four parts in one hundred thousand, but that no appreciable variation has occurred in the other coils, The temperature coefficients of the two ten-ohm coils have recently been determined with great care by Mr. M. Solomon in Professor Ayrton’s laboratory. An account of the determination is given in Appendix IT. Another coil of interest is a British Association unit, one of those originally made by Matthiessen in 1862 or 1864, which has been in India since that date. This coil was brought home by Professor R. Ll. Jones, A careful comparison with the standards shows that it is correct at 16°3°. According to the stamp on the coil, it was originally correct at 16°2°. PRACTICAL STANDARDS FOR ELECTRICAL MEASUREMENTS, 147 In consequence of his appointment as Treasurer of the Association, Professor Carey Foster has resigned the position of Chairman of the Committee, which he has held for many years. The Committee in asking for reappointment recommend that Lord Rayleigh be the Chairman. The standards of the Association have, since the opening of the Caven- dish Laboratory, been kept at Cambridge in the custody of the Secretary. Mr. Glazebrook has now left Cambridge for Liverpool, and the Committee at a meeting in London agreed that Mr. Glazebrook be authorised and requested to retain the custody of the standards. In consequence, the various standards will in the course of the autumn be installed in the Laboratory of University College, Liverpool. At the Toronto Meeting the Committee agreed that it was a matter of urgent importance that the general question of the absolute measurement of electric currents should be investigated, and a grant of 75/. was made for the purpose. During the year Professors Ayrton and J. V. Jones have concluded some preliminary experiments with this object, and have designed a form _ of current weighing apparatus calculated to give results of great accuracy. Drawings of the apparatus have been laid before the Committee and the details of its working explained to them. The estimated cost of the apparatus is 280/.; to meet this the grant of 75/. made last year remains in hand. After careful consideration and discussion the Committee, at their meeting at Bristol, agreed unanimously to the following resolution :— The Committee, having heard from Professors Ayrton and J. V. Jones an account of their preliminary experiments on the absolute determination of the ampére and their plans for the construction of an absolute ampére balance, are of opinion that, in view of the importance of the proposed experiments, application should be made for leave to retain the unexpended ey 751, of the grant made last year, together with a further grant of 2251. Accordingly the Committee ask for reappointment and apply for the above grant. They recommend that Lord Rayleigh be Chairman, and Mr. R., T. Glazebrook Secretary. APPENDIX I. Comparison of the Standard Coils used by Professors J. Viriamu Jones and W. EH. Ayrton in their determination of the absolute resistance of Mercury with the standards of the Association. By R. T. Guaze- BROOK, F.R.S. These coils consist of two tenth-ohm standards of manganine, and two tenth-ohm standards of platinum silver. _ The method employed in comparing the tenth-ohm standard is de- scribed in the Report of the Committee for 1894 (Oxford Meeting) ‘ Re- port,’ p. 128. In certain of the experiments the same mercury cups were used as in 1894 ; in others, the cups used by Professor J. V. Jones in his absolute measurements were employed. The Standard Coils made use of were the following :—Elliott, No. 269 ; Elliott, No..270; and Nalder, 3716, the last being a ten-ohm standard, the others units. The following values were found :— L323 148 REPORT—1898. Nalder, 4274. o 389, R.T,G.’s mercury cups used ° “100049 14:2 4 A - : . 1100051 141 . Fr 100045 14:3 ” ” - - . 100030 134 ” ” ° : . °100054 15:7 ” ” : > « . °100050 16° J.VJ.’s > : : . *100030 131 » x : 4 . 100042 13:7 R.1.G.’s : : ; . °100044 13-7 9 &e 5 ‘ . °100042 14:1 J.VWJ.’s zy ; 2 * 100043 141 Mean : : 3 ; : 100044 14:2 Nalder, 4275. "390. —_— R.T.G.’s mercury cups used é . 1100060 14:4 ” 7 F . *100061 14:4 a4 a 100057 14:5 a , 100040 13°4 45 ah : . °100063 158 “ a : . . 100056 161 J.V.J.’s % ; : . 7100045 131 Ay 4 5 . *100052 13°7 R.T.G.’s ¥ 4 ; . *100055 13:7 - % : : . °100054 14:1 J.V.J.’s 4 : 5 . 100055 14:1 Mean ; : 5 100054 14:3 The values found in 1894 were ee yaly 100050 and -100053 in each case at 15:2°, and the differences are probably within the errors of observation. If all the individual observations for both 1894 and 1897 be Fie.l. No. 4274. Fig. 2. No. 4275. 60 oe “e 4s° 16° 17° Results of observations on the *1 ohm coils used by Professors Ayrton and J. V. Jones. Observations in 1894, thus e Observations in 1897, thus + The horizontal divisions are 0°1 C. The vertical divisions are ‘000005 ohm. plotted, they will be found to overlap each other, and it is difficult to assert that there has been any change. If any exists it is certainly very small. PRACTICAL STANDARDS FOR ELECTRICAL MEASUREMENTS. 149 This is shown in figs. 1 and 2, in which the observations indicated by dots give the results of the 1894 experiments, those indicated by crosses the experiments of 1897. At a glance the observations do not appear very good, but it must be remembered that the vertical ordinates are drawn to a very large scale, the division being five-millionths of an ohm. For both coils the resistance appears to reach a maximum at about 15°5° C. The ten-ohm coils were compared in the usual manner on the Carey Foster bridge with the Standard Coil, Nalder, 3716. The following are the values found :— Nalder, 3873. G, 367. Date Value Temperature December 9, 1897 : H 9:9913 14:3 at cE ; ; 9:9917 14-4 7 16 paar : : 9:9891 13°5 6 DS» ata : : 9°9877 13°15 os 30,3 - : 9:9909 14:2 Mean. . : : : 9-9901 | 13°9 Nalder, 3874. ©, 362. December 9, 1897 : - 9:9907 14:3 = “i ; : 9°9911 14:3 % igh Bes 3 : 9:9886 13°5 - PA eae F z 9:9873 1371 “ 30) 3 : : 9:9904 14:05 Mean ,. : : 5 99896 139 The values found in 1893 and 1894 were as follows :— For 3873, 9:9919 at 14°8°. If we take the temperature coefficient as ‘(0028—the value given by Messrs. Nalder—this becomes 9°9894 at 13:9°. Thus the coil appears to have risen in value by -0007 ohms ; while for 3874, the value found was 9°9926 at 14:9°. Messrs. Nalder give the temperature coefficient as 003, and this leads to the value, 9°9896 at 13:9°, agreeing exactly with the observations of December 1897. The results of these observation are shown in figs. 3 and 4._ The dots refer to the 1893 observations, the crosses to those of 1897. It appears that No. 3874 has not changed ; with regard to No. 3873, a change is indicated. As to this change, it appears from the note-book that there was some doubt as to the temperature of one of the observations in 1893; it is recorded as 14° ; the observation shows that the temperature must have been about 13°7°. Furthermore, the value of the ten-ohm standard used for 3873 was not definitely determined in 1893. If allowance is made 150 REPORT—1898. for these two facts, the value of 3893 at 13°-9 is raised to 9:9923 ; thus the curve shown in fig. 3* is obtained, and the apparent change in "value ig reduced to about 0003 ohms, or three parts in one hundred thousand. On the whole, then, I conclude that 3873 has changed since 1893 by about Fig. 3. No. 3873. Fig. 4. No. 3874. fac had wal ee | a 4-H See er eS Se Result of observations on the 10-ohm coils, used by Professors Ayrton and J. V. Jones. Observations of 1893, thus e Observations of 1897, thus + The horizontal divisions are 0:1° C. The vertical divisions are ‘0002 ohms. Fig. 3*. No. 3873. Revised. EEE aR ae tt YL de hey Observations of 1893, corrected to final value of|10-ohm standard, shown thus e Observations of i897, thus + this amount, while 3874 has remained stationary in value. The dis- crepancy between this conclusion and that given, by Mr. Solomon in Appendix IT. depends on the different values employed for the tempera- ture coefficients. ra PRACTICAL STANDARDS FOR ELECTRICAL MEASUREMENTS. 151 The vaiues of these coefficients obtained over so short a range are not of much importance. Still, in view of Mr. Solomon’s determination, they may be given. They are: For 3873, :000283; and for 3874, 000277, These values are relative to the standard coils of the Association. APPENDIX IL. On the Determination of the Temperature Coefficients of Two 10-Ohm Standard Resistance Coils (Nos. 3873 and 3874) used in the 1897 Determination of the Ohm. By M. Sotomon. In the determination of the ohm made by Professor W. E. Ayrton _and Professor J. Viriamu Jones in 1897 (Report, 1897, p. 212), four standard resistance coils were used, two of which had a resistance of 10 ohms each, and two of 0:1 ohm each. Values for the temperature co- efficients of these coils had been calculated from four accurate determina- tions of their resistance made, two by Mr. Glazebrook in 1894 and 1897, and two by the Board of Trade in 1896 and 1897 (‘The Electrician,’ vol. xl., p. 39). The values thus obtained neither agreed with one another nor with the coefficients given by the makers, Messrs. Nalder Bros. & Co. It therefore became necessary to make as accurate a determination as possible to endeavour to find the correct values for the coefficients. The following Paper gives the results of the tests made on the two 10-ohm coils (Nos. 3873 and 3874), the tests on the other two coils being not yet completed. These two coils are of the B.A. pattern, and are made of platinum silver wire. A preliminary series of tests made on one of the coils showed that to attain the required accuracy special precautions would have to be taken to keep the coils at steady temperatures. Each coil was therefore placed in an oil bath, the temperature of which was automatically regulated. In making the determination of the tempera- ture coefficient of one coil, the other was used as a standard, and was kept at a constant temperature throughout the whole series of tests. - The coil under test was maintained at a steady temperature for some time, and a measurement of the difference of resistance between it and the standard was then made by means of a Carey Foster bridge. The temperature of the coil being tested was then altered and a fresh measure- ment taken, this being repeated for several temperatures. The apparatus used in the measurements was. arranged in the following manner. The standard coil was placed in an oil bath with two vessels, in the inner of which the coil itself and a carefully standardised thermometer were immersed. In the outer bath was the bulb of an alcohol thermo- meter, the mercury index of which, when the temperature rose too high, completed the circuit of an electromagnet and battery, and caused the gas which heated the bath to be put out. On the bath then cooling the circuit of the electromagnet was broken, and the gas turned on and re- lighted by a bypass. This thermostat was very sensitive, the temperature of the inner bath rarely varying so much as 0°05° C. in a day, and in a run of ten days undergoing a maximum variation of 0°3° C. The ther- mostat in which the coil under test was placed was not so sensitive, but was designed to work over a greater range of temperature. The coil and thermometer were placed in an inner bath, and in the outer bath was a large brass bulb filled with alcohol. The expanding alcohol either passed into a small reservoir, or, when the passage to this was closed by 152 REPORT—1898. shutting a stop-cock, it expanded into one arm of a glass U tube, thereby forcing a mercury index at the bottom up the other arm; this index cut off the gas supply by closing the aperture of the inlet tube. On cooling the index sank; the gas was turned on and relighted by a bypass. Regulation of the temperature accordingly did not take place until the path leading to the reservoir was closed, so that regulation at any desired temperature could be obtained by leaving the stop-cock open until that temperature had been reached. In this case, as also in the other thermostat, the bath was not heated directly by the gas jet, but a baffle plate was interposed. The daily variation of temperature with this apparatus was about 0:2° C., but the changes were so slight and so slow that the probable error introduced would be less than that caused by error in reading the thermometer. The bath was always kept at a constant temperature for some hours before readings were taken. With these arrangements it was safe to assume that the temperature of the coil was the same as that read off from the thermometer. The terminals of the coil dipped into mercury cups in one end of a pair of stout copper rods, half an inch in diameter, the other ends of which rested in mercury cups on a Carey Foster bridge. The leads from each of the coils were of very small and approximately equal resistance, so that no appreciable error could be introduced by alteration in their resistance with change of atmospheric temperature. Also, as a part of each lead was inside the thermostat, heat lost by conduction along the leads would be withdrawn from this part and not from the coil itself. The measurements were made with a Carey Foster bridge, the platinum silver slide wire of which had been previously calibrated. This wire was 50 centimetres long, and had a resistance of 0:001859 ohms per half centimetre at 13°5° C., and was graduated in half millimetres. Correction was made for alteration in the resistance of the wire due to change in its temperature, an increase of 1° C. producing an increase of 0-000011 ohms in the resistance of half a centimetre. Determinations of the difference of resistance between the two coils were made at intervals of about an hour, and if two or three quite consistent readings could be taken these were considered as correct, but where discrepancies occurred the mean of several results was taken. The slight changes in the temperature of the standard were easily allowed for, since it could be assumed that for such small changes the two coils had the same temperature coefficients. So if the standard, instead of being at the temperature ¢, were at the tempera- ture ¢+6, and if the coil under test were at the temperature ¢’, it was assumed that the standard was at temperature ¢, and the coil under test at the temperature ¢/—8. There are four principal sources by which error can be introduced— viz., error in obtaining the correct position of balance, error in the vaiue of the temperature coefficient of the slide-wire, error in reading the temperature of the standard coil, and error in reading the temperature of the coil under test. As regards the first of these, the sensibility of the arrangement was such that a change of half a millimetre in the position of the slider produced a deflection of about a centimetre on the galvano- meter scale, so that balance could easily be obtained correct to 005mm. The error due to not knowing the temperature coeflicient of the slide-wire with certainty will not be great, as all the measurements were made at temperatures near to 13°5° C., at which temperature its resistance was known. The greatest error is introduced in reading the thermometers PRACTICAL STANDARDS FOR ELECTRICAL MEASUREMENTS. 153 which were graduated in tenths of a degree, each division being about 06mm. in length, so that the temperatures could not be read with cer- tainty to less than 0-02°C. If all these errors should be made in one direction in making one determination of difference of resistance, and all in the opposite direction in making a second, there is a possible maximum error of about 3 per cent. in the value of the temperature coefficient calculated from these two determinations. This is, however, highly im- probable, and, moreover, makes no allowance for taking the mean of several readings. The error in the temperature coefficient is probably not greater than | per cent., if as great. The following summarises the results of the experiments :— Ten-Ohm Standard Coil, No. 3875. A series of tests was made on this coil in the manner above described, lasting from March 22 to April 1, 1898. Determinations were obtained of the difference between the resistance of No. 3873 at six different temperatures, and the resistance of No. 3874 at 16°70° C., with the following results :— Excess resist. in ohms of Change of Temperature of No. 3873 No. 3873, above No. 3874, resist. per at 16°70° C. 1° C. (a) 16°31° C. —0:001896 -— ——-—-=~ 0:00307 (b) 19°338° C. +0:007380 ~=~-= == 0:00291 (e) 22°10° C. +0:01545 =-<=7 >>> 0-00291 } (d) 22:43° C. +0:01639 -=<=7~==-=0:00278 ) (e) 25-43° C. 002470) —aa—— == 0100277 fi (f) 26°22° C. +0:02678 -—-———==-0:00274 From readings a, 5, c, and e, and from the measurement of the resist- ance of the coil made by Mr. Glazebrook in December, 1897, giving Ry3.0=9°9901 ohms, we get R,=9-9398 (1 +0-000397¢—0-000002(4)22). After testing this coil the other coil (No. 3874) was tested, and then three check tests were made on this coil with the following results :— Temperature of Excess resistance in ohms above No. 3874, No. 3878 at 16°70° C. (g) 19°62° C. + 0:008398 (A) 15°95° C. — 0:003074 (A) 18°13° ©. | + 0°003704 These points lie well on the curve obtained in the former tests (see fig. 5). From the formula given above the coil will have the correct resistance of 10 ohms at 17-0° C. To compare the temperature coefficient here obtained with those 154. REPORT—1898. previously determined we have four measurements of resistance, as follows:— A. My. Glazebrook in March, 1894. Resistance = 9°9923 ohms at 14°8°C. ; 4: B. Board of Trade in Nov., 1896. . = 9°992994 » L4°86°C: C. Board of Trade in Aug., 1897. aS =10:00712 spl 4973°:G: D. Mr. Glazebrook in Dec., 1897. 3 = 9:9901 ne LBS. These furnish data for calculating the temperature coefficient, and we have also the value given by the makers, Messrs. Nalder Bros. & Co. :— Temperature Coefficient from Observer 1 Henge i f coefficient per these tests for ee 1° C, same range | | Messrs. Nalder Bros. & Co. | 17:0° —22-0°C. 0:000276 0000303 Tests AandC , : 14°8° —19°3°C. 0:000331 0-000315 ays . Ox43 : . | 14°86°—19°3° C. 0:000320 0:000315 PF = f |/ 13159 1424° 6, 0:000299 0000330 D ana Ce. 3 J} SBS — 19:32 C. 0:000317 0:000317 This table shows that the coefficients calculated fhaxn tests B and C Fie. 5. 9 LRGESS resistance in ohms “@ 0 16 17 18 19 2 tf 22 23 24 25 26 27 Temperature ta°t Curve showing change of resistance of 10-ohm standard coil, No. 3873, with change of temperature. Ordinates give excess of resistance of 387 3 above 387 4 at 16-70° C. and from tests D and C are both in very close agreement with those I obtain for the same range of temperature. Ten-Ohm Standard Coil, No. 3874. A series of tests on coil No, 3874, lasting from May 19 to May 31, PRACTICAL STANDARDS FOR ELECTRICAL MEASUREMENTS. 155 1898, were made, and in addition we have one result from the tests on coil No. 3875. Altogether we have the following :— Temperature of No. 3874 (a) 16-70° C. (b) 17-46° C. (c) 18:08° C. (d) 19:09° C. (e) 21°37° ©, (f) 22:22° 0. (g) 24:46° C. Excess resist. in ohms of “CHiahee of No. 3874, above No. 3873, ere ie ike 1° C. —0:00095 ~~~ -___ + 0:00159 —-—=—=== 0:00334 363 ——— — > 7 0'00332 + 0:003868 === = 2 = ===-0:00323 +.0:00689-= === T_ _ = =>==— 0:00306 + 0:01882 ——= ee yal : + 001641 -~-_~ -= 7 eae +0 02264——=-— -——— From readings a, ¢,e and g, and Mr. Glazebrook’s determination of the resistance in December, 1897, which gave Ry:..=9°9896 ohms, we get R,=9°9313 (1 4+.0:000481¢—0:000004(2)z?). Check tests were made on this coil after those on coil No. 3873 been made, and gave the following results :— had Temperature of Excess resistance in ohms above No. 8,873 No. 3874 at 17°25° C (h) 187°C. +0°00583 (hk) 20°15° C. +0-01040 All the nine points lie on a smooth curve (see fig. 6). make the coil correct at 16:9°C. Fia@. 6. 024 éxcess resistance (n ohms. ~82 Mt 4% ee aay eee es oy Si APA peo ve a ce Baad | Sicpon tee 7a] @ 19 2 2 22. 23 24 Tempereture ia a These tests Curve showing change of resistance of 10-ohm standard coil, No. 3874, with change of temperature. Ordinates give excess of resistance of 387 4 above 3873 at 17:25° C. For purposes of comparison we have a similar set of data to those used 156 REPORT—1898. for the other coil. The four measurements of resistance gave the following — results :— A. Mr. Glazebrook in March, 1894. Resistance = 9°9926 ohms at 149°C. B. Board of Trade in Nov., 1896. ~ = 9:993213 se edl4-91° °C; C. Board of Trade in Aug., 1897. ms = 10-00775 ie 19:3°'C: D. Mr. Glazebrook in Dec., 1897. = 99896 s 139° C. ” From these we get the following values for the temperature coefli- cient :— Coeff. from these Observer Bee tare cam ete. Per tests for same range Messrs. Nalder Bros. & Co. | 17:0° —22:0° C. 0:000300 0:000316 Tests AandC :} . | 149° —19°3° C. 0:000346 0:000336 } BandC . . | 14:°91°—19-3° C. 0000333 0:0003836 eae D . a lioeiee lal, 0:000279 0:000365 > Diand.¢ 2 : ol s292 — 193°C; 0000338 0:000341 Here again the same two sets of tests, viz., tests B and C, and tests D and C, give values for the temperature coefticient very nearly equal to those I obtain for the same range of temperatures. Since for both coils the temperature coefficients that I obtain agree with those calculated from the three last measurements of resistance— namely, the two measurements by the Board of Trade and Mr. Glaze- brook’s last test—these experiments seem to show that the coils have not changed since 1896, but that the resistances as measured in 1894 were a little lower than those that would now be obtained at the same tempera- tures. This conclusion may be better illustrated by calculating what would be the resistances at the temperatures of the various tests, on the assump- tion that the coefficients I obtain are correct, and that Mr. Glazebrook’s last test (in December, 1897) is correct. We then get the following :— ane o Resistance as measured Resistance as calcu- Temperature of test Shing lated an chats | uo ht = H 148°C. (A) 9-9923 99930 wo | 1486° C. (B) 9-9930 9:9931 em Ne OTS .9 g.20c9 > ey 10-0071 10-0071 139°C. (D) 9-9901 9:9901 149°C, (A) 9:9926 9:9932 14:91°C. (B) 99932 99932 CIE HOTEY. 19:39 O6 -.-( Gy 1000775 100079 139°C. (D) 9:9896 99896 Thus we see that the 1894 measurements (A) are too low by as much as 7 parts in 100,000 in the case of coil No. 3873, and 6 parts in 100,000 in the case of No. 3874. In the case of the other two measurements the calculated results only differ from the observed results by 1 or 1°5 parts in 100,000. These experiments were carried out in the laboratory of the Central Technical College, South Kensington, and I am much indebted to Pro- fessor Ayrton and Mr. T. Mather for their valuable guidance and advice. PRACTICAL STANDARDS FOR ELECTRICAL MEASUREMENTS. 157 “APPENDIX III. An Ampére Balance. By Professor W. E. Ayrton, /.2.S., and Professor J. Vintamu Jonss, 7.2.8. The Report of the Committee on Electrical Standards for 1897 ended with the following paragraph :—‘ It thus appears to be a matter of urgent importance that a redetermination of the electrochemical equivalent of silver should be made and that the general question of the absolute measurement of electric currents should be investigated. . . .’. This work we were asked by the Committee to carry out, and a grant of 75/. was voted in its aid. We were thus led to examine into the methods which had been employed by Lord Rayleigh, Professor Mascart, and others, for determining the absolute value of a current, as well as to consider some other methods which have not, as far as we know, been hitherto used. After much consideration we decided to adopt a form of apparatus which, while generally resembling the type employed by some previous experimenters, possessed certain important differences, and, before expending any part of the grant of 75/., to construct, without expense to the British Association, the following preliminary Ampére Balance. On a vertical cylinder about 17 inches high and 6°8 inches in diameter we wound two coils, about 5 inches in height, separated by an axial distance of 5 inches. The coils consisted each of a single layer of about 170 convo- lutions of wire and were wound in opposite directions. From the beam of a balance there was suspended, inside this cylinder, a light bobbin about 4 inches in diameter, on which was wound a coil about 10 inches long consist- ing of a single layer of 360 convolutions, and the whole apparatus was so adjusted that when the beam of the balance was horizontal the inner and outer coils were coaxial and the top and bottom of the inner suspended coil were respectively in the mean planes of the outer stationary coils. This arrangement was adopted because with coils consisting of only one layer the geometrical dimensions could be accurately determined, and because the shapes of the coils lent themselves to the use of the con- venient formula, readily expressible in elliptic integrals, for the force, F, between a uniform cylindrical current sheet and a coaxial helix, viz. :— F=yy, (M,—M,) where y is the current per unit length of the current sheet, y, the current in the helix, and M, and M, the coefficients of mutual induction of the helix and the circular ends of the current sheet.} The value of a particular current of about 0°63 ampére having been determined absolutely by means of this apparatus, the rate at which it would deposit silver under specified conditions was ascertained indirectly, by observing its silver value on a Kelvin balance which had been kept screwed down in a fixed position for several years past and which had been calibrated many times during that period by reference to the silver voltameter. The result of this preliminary investigation showed that the silver value of the true ampere was so nearly equal to the reputed value, viz. 1-118 milligramme per second, as to require the use of an apparatus still more _ * See Proceedings of the Royal Society, vol. 63: ‘On the Calculation of the Coefii- cient of Mutual Induction of a Circle and a Coaxial Helix, and of the Electro- magnetic Force between a Coaxial Current and a Uniform Coaxial Circular Cylindrical Current Sheet.’ By Professor J. V. Jones. 158 REPORT—1898. perfectly constructed, and therefore of a much more expensive character, to enable the error, if any, in this value to be ascertained with accuracy. We, therefore, started on the design of the instrument, of which we now submit the working drawings, and for the future construction of which we would ask for a grant of 300/. including the unexpended grant of 75/. voted last year. And we anticipate that this new piece of appa- ratus may prove worthy of constituting a national Ampére Balance, the counterpoise weight for which will be determined purely by calculation based on the dimensions of the instrument, the number of convolutions of wire in the three coils, and the value of the acceleration of gravity at the place where the instrument may be permanently set up. In this par- ticular it will differ entirely from the ‘ Board of Trade Ampere Standard Verified 1894,’ which has had its counterpoise weight adjusted so that the beam is horizontal when a current passes through the instrument, which will deposit exactly 1-118 milligramme of silver per second under specified conditions. In fact, the proposed Ampére Balance and the existing Ampére Standard will differ exactly in the same way as doa Lorenz apparatus and the ‘ Board of Trade Ohm Standard Verified, 1894.’ We have to express our thanks to Mr. Mather for taking charge of the construction and use of the preliminary apparatus, for checking all the calculations in connection with the determination of the electroche- mical equivalent of silver that was made with it, as well as for superinten- ding the making of the working drawings of the new Ampére Balance. We have also to thank Messrs. W. H. Derriman and W. N. Wilson, two of the students of the City and Guilds Central Technical College, for their cordial assistance in carrying out the work. Electrolysis and Hlectio-chemistry.—Interim Report of the Committee, consisting of Mr. W. N. Saaw (Chairman), Mr. KE. H. Grirritus, Rey. T. C. Firzpatrick, Mr. W.C. D. WHETHAM (Secretary), on the present state of our knowledge in Electrolysis and Electro-chemistry. Tue grant of 35/7. made last year has been expended in improving the apparatus for experiments on the electrical properties of solutions. Measurements have been obtained by Mr. Whetham of the electrical conductivity at 0° C. of dilute solutions of potassium chloride, barium chloride, potassium ferricyanide, potassium bichromate, and sulphuric acid. The freezing points of identical solutions have been observed by Mr. E. H. Griffiths. The measurements are sufficient to indicate that important and unexpected results will be obtained. The reduction of the observations is not yet completed, and, in consequence, the account of the experiments is not ready for publication. The apparatus is now in working order, and it is hoped that measure- ments may be obtained for other salts. Unfortunately the room in Mr. Griffiths’s laboratory where the experiments have been carried out is no longer available, and some considerable expense must be incurred in reconstituting the arrangement in a different situation. To meet this and the additional expenses incidental to the continuance of the observa- tions it is estimated that at least 25/. will be required. The Committee accordingly ask for reappointment, with the addition of the name of Mr.S8. Skinner, one of the Demonstrators at the Cavendish Laboratory, and with a grant of 25/7. i a ON THE USE OF LOGARITHMIC COORDINATES. On the Use of Logarithmic Coordinates. By J. H. Vincent, D.Sc., A.R.C.Sce. [Ordered by the General Committee to be printed im extenso. | PLATES I-III. INTRODUCTION . - : ; : . : : Definition and an example of a translatant . CONSTRUCTION OF AN IMPEDANCE CHART The equation represents a translatant . The resistance line. ‘ : ile Jy 3 ; : E The self-induction line , The complete impedance curve Mechanical device for drawing above Scale lines : : ; : How to use the chart. - . - * : : 4 DISCUSSION OF A NON-TRANSLATANT CONSTRUCTION OF A CHART FOR WAVES ON A FROZEN SEA Short wave gravity and elasticity lines . : Short wave curve . : : : : 5 4 Above to be made general. = : : - The scale lines - . ; : : : c c E c Recapitulation . F 3 5 ‘ : = 5 ANOTHER METHOD OF TREATING THE SAME NON-TRANSLATANT The long wave elasticity line . : - 9 : - : Short wave elasticity line. ‘ ; . . Complete elasticity curve F é s . : The two gravity lines and complete gravity curve . The two complete curves are translatants Translation of the elasticity and gravity curves Scale lines for the two complete curves . Scale lines for thickness : é : : : : 3 On several outstanding matters connected with the chart. 159 THE Use oF LOGARITHMIC COORDINATES TO FIND AN APPROXIMATE EQUATION CONNECTING A SERIES OF EXPERIMENTAL RESULTS TRI-DIMENSIONAL LOGARITHMIC COORDINATES : 2 " 2 SEMI-LOGARITHMIC COORDINATES . 3 , ‘ THE GRAPHICAL COMPUTATION OF THE HYPERBOLIC FUNCTIONS The meaning of a straight line on the chart . : . . . Theeuline . : ‘ , : i Other lines . 3 ; F ( 3 ; : é : 3 Semi-logarithmic graph of sinhw . : . , 5 ; Of coshu . ‘ é ; ‘ , . ‘ - Of cosech u and sech uw . . Fi 4 f : ; 5 ‘ Of tanh uand cothu . , A A : : 6 4 Points in the geometry of these curves. ‘ . . . . CONCLUSION s ‘ A $ : ; c * . ° . INTRODUCTION. 1. In discussing experiments upon the passage of gases through porous plates Professor Osborne Reynolds employed a method of plotting curves,! in which the logarithms of two variables are used to find the points on a new curve. This new curve Professor Reynolds calls the logarithmic homologue of the one from which it is derived, and pointed out the ’ Sir John Herschel used the logarithmic chart in reducing photometric observa- tions, Art. 285, Cape of Good Hope Observations, 160 REPORT—1898. following useful property possessed by the homologues. (We may omit the adjective when no ambiguity is likely to arise.) ‘If for two curves (1) and (2) x,=ax, and y,=by,, then a}=2} + log a and yi=y} + log b ; or the logarithmic homologues will all be similar curves, but differently placed with regard to the axes, such that the one curve may be brought into coincidence with the other by a shift of which the coordinates are log a and log 8.’} It should be noticed that this shift of the homologue is one of pure translation. The graphic method of homologues was again used by Professor Reynolds in discussing experiments on the flow of water,” 2. Mr. Human has since patented the manufacture of sheets of paper ruled logarithmically. A short account of the use of logarithmic coordinates may be found in Greenhill’s ‘ Differential and Integral Calculus,’ 1896 edition; directions for the use of the ruled sheets, with a number of easy examples, are supplied by the publishers of the ruled paper, and the valuable aid to computation which this method gives may now be considered well known. 3. The power of readily moving homologues on the logarithmic paper to represent changes in the original equation was greatly facilitated by the invention of scale lines by Mr. Boys.* To explain the use and method of construction of scale lines Mr. Boys drew a chart of wave and ripple velocities, which by its wonderful generality was calculated to emphasise the power of the new method of discussing curves by means of their homologues. Definition and an Example of a ‘ Translatant.’ 4, Let us consider the equation which is the equation that Mr. Boys took to illustrate the method. Iti of the form ; b 2—=ar+—. v=a Ty Let a, b, v, and X become a’, b’, v AVA ae and X a] ads The equation remains unaltered ; thus, if g, 7, and p all change, it is possible, by merely shifting the homologue, to represent the new equation. The homologue of this equation possesses the property of translation. 5. It is of great service in any subject to have a definite nomenclature, and a cwrve whose homologue possesses this property with respect to any particular quantity might be called a ‘translatant’ with respect to that quantity. The term translatant can also be applied without risk of confusion to the homologue. 6. Definition.—A curve or its homologue is a translatant with respect to any quantity when an arbitrary change in that quantity is equivalent 1 Phil. Trans., 1879, Part IL. p. 753. 2 Ibid., 1883, Part III, p. 947. 3 Published by Beaves and Stephenson, 8 Princes Street, Westminster. 4 Nature, July 18, 1895, p. 272. Plate 1 68 Report Brit. Assoc, 1898. 2 == i t i fe pShe iii Sy Sh ! a if te : tee BS — }—t > ane NN x {] i) < Y N Set Me 5 5 \ 8 y ‘ oy i) yu A V S is a i) Ne “ a RESISTAN | e ee ON THE USE OF LOGARITHMIC COORDINATES. 161 to the transformation x=ax,, y=by,, where a and b are some deter- minate constants. Many curves which occur in physics are translatants with respect to all the quantities which are found in the equation; such curves are particularly suitable for treatment by logarithmic coordinates, CoNSTRUCTION OF AN IMPEDANCE CHART. 7. As a second example of a translatant, let us take the equation I?= R?+ 47°L?n?; which gives the impedance of a circuit whose resistance is R, self-induction L, and subject to a periodic electro-motive force of frequency n, all expressed in some consistent system of units. Regarding m as the independent variable, a chart may readily be constructed giving the value of I for any values of R, L, and 7 ; that is, we can in a few minutes produce what amounts to a complete table of the impedance of all circuits subject to a periodic electro-motive force of any frequency. The equation represents a translatant,' for if R and L become R’ and L’ respectively, the equation remains unaltered if n and I be also changed / / into 7 m and ze I. The first step is to draw the homologue for arbitrary values of Rand L. Let R=2 and L=-002, these numbers being such as might occur in practice, when L and R are expressed in henrys and ohms. 8. The Resistance Line.—If I depended only on the value of R, this would be represented on the chart by a straight line I=2. The line is marked ‘ Resistance Line’ (see fig. 1). 9. The Self-induction Line.—If I were a function of L and x only, then the value of I would be given by I=2zrLn. The homologue of this equation is a straight line, making an angle of 45°, with the increasing direction of the axis of m. To draw it in the proper position of the chart some one point on it must be found; thus, if »=100,I1=1-256. The line is marked ‘Self-induction Line’ on the chart. 10. The Complete Impedance Curve.—The actual impedance is due to both effects, and the curve showing the relation of I to the other quanti- ties concerned runs above the resistance and self-induction lines; it is most distant from either line at their point of intersection, and approaches them asymptotically. The curve very soon, however, becomes practically coincident with the straight lines. The curved portion of the homologue may be drawn by the arithmetical computation of a series of points on the curve; it may, however, be drawn with facility by the following device. 11. Mechanical Device for Drawing the Curved Portion of the Homo- logue.—For any value of read off on the chart the value of I due to each effect. (In this case the value due to R is constant. It should be noted that when the separate effects are represented by straight lines it is only necessary to read off values through the range 7 to 10 », all other values being given at once by appropriately shifting the decimal place.) } The homologue of any equation of the form y'=aa™ + da” is a translatant. For : _ , _ n i . : if a, b, z, 4" become a’, b’, "x/ ca ate cae sie . y', the equation is unaltered. 1898. M 162 F REPORT—1898. Take a millimetre scale and a sheet of squared paper ruled in millimetres. Mark off OP and OQ at right angles, these lines being taken to represent the magnitude of the two effects. PQ is the length required, being the. root of the sum of the squares of the two separate effects. 12. It must next be shown how to adapt the homologue for any values of R and L, This is done by means of scale lines, A scale line is a line drawn on the chart and graduated by the logarithmic rulings of the paper. It is so placed as to read directly the particular value of the quantity to which it refers, such reading being the indication of the position of the homologue on the paper, and is the magnitude of the quantity in the equation which the homologue represents in its present position. 13. Scale Line for R.—If R, n, and I be all multiplied by the same quantity the equation is unaltered ; thus when R becomes mR the homo- logue is to be moved a distance log m to the right, and log m upwards. The direction of translation is along the self-induction line, which could be used as a scale line; in fact any line not parallel to the axis of 7 could in this case be used as a scale line, the numbers of the graduations being identical with the impedance. In the chart a line at 45° to the axes is drawn and marked ‘Scale Line for Resistance.’ The direction of motion of the homologue is, in this case, parallel to the scale line. Scale Line for L.—If L and nm vary inversely the value of I is unchanged. If L become mL the homologue must be moved to the left through a distance log m. The scale line must then be parallel to the axis of impedance ; when the homologue moves any distance to the left the point of intersection of the self-induction and scale lines will then move upwards by the same amount. To avoid specially graduating the scale line it is drawn through a point on the self-induction line where the impedance reading has the same significant figures as the value of L, for which the self-induction line is drawn. The scale line on the chart is drawn through the point of intersection of I=2 with the self-induction line. 14. To find the proper position of the homologue for any value.of R and L, move the whole curve with its attendant resistance and self-induc- tion lines by a motion of pure translation until the resistance and self- induction lines cut their respective scale lines at the appropriate readings for R and L. Discussion oF A NON-TRANSLATANT. 15. Even in the case of some curves which are not translatants the labour of plotting their equations may be greatly reduced by the use of this method. To illustrate this let us take an equation which does not represent a translatant curve. Professor Greenhill has given the theory of waves on a frozen sea in his article ‘Wave Motion in Hydrodynamics.’! By retaining a term for the density of the solid in this investigation we have the velocity of pro- pagation and the wave-length connected by the equation 2 (9% “Seal ve ( eae? 222) wu (f+ ors coth x a x)? ? American Journal of Mathematics, vol. ix. No. 1. ON THE USE OF LOGARITHMIC COORDINATES. 163 where w, \, g have their usual significance, and e=thickness of the solid assumed uniform E=Young’s modulus for the solid p=density of the liquid s=density (not superficial density) of the ice h=uniform depth of the liquid, all expressed in some consistent system of units throughout this discus- sion. 16. Fundamental Assumption.—Let us assume that h is large enough compared with ts for us to write a 5 . coth anh =] r without appreciable error. The equation now becomes gx 27eH uw? = 27 prs ik 27es pr which is of the form b " ch + < reece This is a non-translatant ; if we regard \ and w as the independent and dependent variables, and change a, 6, and ¢ into a’, b’, and c’, it is impos- sible to find two numbers ” and m such that the equation / a/m\ + —. VOTE nu? = is identical with the preceding. ConstRucTION OF A CHART FOR WAVES ON A FROZzEN Sra. 17. Short Wave Gravity and Elasticity Lines.—When } is sufficiently small for unity to be negligible compared with i the equation becomes w= ar? + s where mare A des? and 72e7 i ao 164. REPORT—1898. For a, B, A, and p write 4 /ab! 4 /a'b! a’, BX Sa are ab The equation is unaltered ; this shows that it is a translatant. If the first term only in the right-hand member had to be considered, the homo- logue would be a straight line, making an angle of 45° with the increas- ing direction of the axis of A, on the chart ; if the second term only were present this also would be represented by a straight line sloping in the opposite direction and to the same extent. To put these lines in the chart it is only necessary to calculate one point on each, and to draw through this point the line in the proper direction. These lines are drawn on the chart for the case when E!}=6 x 10%, g=981, e=100, p=s=1. They are marked ‘Short Wave Gravity and Elasticity Lines.’ (See fig. 2.) 18. Short Wave Curve.—To represent the united effect of gravity and elasticity these two lines must be joined by a curve. The whole will then be the homologue of the equation wu? = a4, The curve is asymptotic to the short wave lines ; it very soon becomes practically identical with them. It is symmetrical about a line parallel to the axis of w drawn through the point of intersection of the straight lines ; only half need be computed, the other half being put in by geo- metry. The curve may conveniently be drawn by the method of § 11. 19. It must next be shown how to adapt this curve to any values of a and 8. It has been already shown that it is a translatant, and thus the curve will not have to be redrawn, but merely shifted about. 1 Most of the experimental investigations into the physics of ice have been con- cerned with the viscosity and not the elasticity. Professor Greenhill, in the paper already cited, remarks that ‘ice was the first substance for which an experimental determination of E was attempted, as described in Young’s Lectures on Natural Philosophy.’ Morgan (Nature, May 7, 1885) points out that the value quoted in Thomson and Tait’s Nat. Phil., Art. 686, is ten times too great. McConnel (Proc. Roy. Soc., March 1891, p. 343) gives the following values for E :— 92,700 kilos per sq. c.m. (Moseley), Phil. Trans., 1871 23,632 33 (Reusch), Nature, xxi. 504 60,000 + (Bevan) The last value is, presumably, computed from Bevan, Phil. Trans., 1826, Part 2, Paper 21. Turning these values into c.g.s. units we obtain, to the nearest sing’e significant figure— 9 x 10° (Moseley) 2 x 10° (Reusch) 6 x 10'° (Bevan) McConnel considers Moseley’s value too great, and implies that Reusch’s method was unreliable. By recomputing Bevan’s value I obtain 5 x 10'". From this it seems that the value of E for ice is somewhere about 6 x 10’ inc.g.s. units; in drawing the first short wave elasticity line on the chart it appeared unne- cessary from a physical standpoint to allow for the density of ice and water when the value of E was so uncertain. Plate2. 68 Repor = \ NC "1 a I AZ) ¥ J ao/ XN eee ee ates. | | | | oy F = = = Ss = | as Bae = & > ss 2 5 5 2 Ris > 2 iss = & = 5 os & = = 3 = a 2: ieee } - ack | Fie: } com Ss = = | 3 NO ee ee = 3 3 Ma | ¢ Fa 5 ay * is | E aR g & 3 \§ & N | s | 4 motte th é Ll CLiisSae Agqbake £3 Baa $8 <% 3 q slebaap a ieee # : giguss oF EF SEuaR 25 st = iba eigtgen Ne & eases te By 33 ON THE USE OF LOGARITHMIC COORDINATES. 165 90. The Scale Lines—A change in a or #3 is equivalent to a definite shift of one of the short wave lines, keeping it parallel to itself. This shift might obviously by proper graduations be measured along any line not parallel to the line shifted. By giving the line, along which we wish to measure either of these translations, a proper inclination we can make the lines already on the chart divide this line with the proper logarithmic graduations for a or (3, as the case may be. 21. Scale Line for a.—This scale line will show how to move the short wave gravity line and the curved portion so as to adapt the chart to new values of gravity, density of liquid and solid, and thickness. The short wave gravity line is the homologue of we=anr?2. r F Tf a become na and \ become ——— the value of w is unchanged. 1 Therefore a shift to the left of }log must be made when « becomes n a ; a point on the short wave gravity line must move one large square to the left when the point of intersection on scale moves through two large squares. The scale line will then make an angle tan™! 2 with axis of X. Tt must be graduated so that its readings increase as we move upwards on the scale line ; the point in which it cuts the short wave gravity line must read the «a appropriate to values of g, Z, ¢, s, and p in § 17. But the graduation of the u axis must be utilised to save regraduating the scale line. Thus, look for the value of « on the w line ; or 10*”a where 7 is a whole number; a parallel to axis of \ through this point cuts the short wave gravity line in a point through which the scale line may con- veniently be drawn. The graduations are then those of the axis of w multiplied or divided by some positive integral power of 10. The scale line is inserted on the chart and marked ‘Scale Line for a.’ 22. Scale Line for (3.—This scale line shows how to move the short wave elasticity line and the curved portion so as to allow for changes in the values of the density, elasticity, and thickness of the solid. (The short wave elasticity line is not affected by a change in the density of the liquid.) The short wave elasticity line is the homologue of Tf 3 becomes 7/3 and \ becomes \/7X, w is unchanged. A scale line for /3 is inserted on the chart. _ To use the scale lines, move the figure consisting of the two short wave lines and the curve derived from them, without rotation until each of the short wave lines cuts the corresponding scale line in the proper point. The whole operation can easily be accomplished by the use of tracing paper. This translation will obviously move the curve to the correct new position. 23. Complete Curve obtained from Short Wave Curve.—There is now on the chart a curve and two scale lines which enable that curve to be shifted so as to represent ' waar 4F 166 REPORT—1898. for any values of g, p, e, s, and E. The complete curve to represent must now be drawn. The above equation can be written z BY ak Ga eee where a, /3, and ¢c have been previously defined. When the short wave curve has been placed in its proper position on the chart, calculate c from the equation . Qares c= ; P From each value of w, as read on the chart, the length x {log (A+c)—log c} has to be subtracted. The slide rule is an instrument specially designed for the purpose of adding and subtracting logarithms ; the operation of drawing the complete curve can be performed by one setting of a slide rule, without other numerical computation. The top scale on Davis’s 10-inch slide rule is the same size as the scale of Human’s paper ; to find a point on the complete homologue set the right hand 1 on the top scale of the sliding piece under the appropriate value of c on the right hand top scale of the rule ; the rule as thus set is a table of division of all numbers by c. Add any desired value of \ toc; look for \+c on the top scale and take off distance from the middle ‘1’ of top slide (if — is less than 10) to A+¢ on top scale. This length is log(A+c)—loge. Take off this distance on a pair of proportional compasses set to reduce to one-half. This is the length by which the point on the short wave curve must be dropped to become a point on the complete homologue. Without resetting the rule repeat the operation with other values of 2.1 In this way the complete homologue may be drawn without much trouble, and with only so much mental labour as is involved in adding the chosen value of \ to the appropriate value of c. 24, Kecapitulation.—We have now upon the chart a curve which is the homologue of the complete equation for waves on a solid covering Qh rt case where g, E, e, p, and s have the values given in sect. 17 is represented on the chart by a thick curved line running beneath the short wave curve. The arithmetical operations necessary to get’ a curve to represent the liquid of sufficient depth for coth to be taken equal to unity. The ‘ Tf the scale of rule have any size other than that of chart the same method may be used by setting the proportional compasses properly. The whole operation can be performed without a slide-rule on the chart. Draw a straight line through left hand bottom corner of the paper at an angle tan-! 2 with the horizontal. Use the projection of the left hand coordinates as the one on which to read A+c¢ and ¢; use the horizontal scale to read off length +{ log (A+ce)—log ec}. ; ON THE USE OF LOGARITHMIC COORDINA'TES. 167 equation for any values of the quantities involved consist merely in the computation of a, 3, and ec. Thus it is possible to obtain by means of logarithmic coordinates a- curve giving wu for any value of \ without a single operation of the nature of substituting arbitrary values for a variable in the equation. If it had been merely desired to draw such a curve the task might be regarded as completed ; but the equation under discussion may be made to yield many interesting illustrations of the method of homologues. Some of these will now be dealt with. AnorHerR MrrHop oF TREATING THE SAME NON TRANSLATANT. 25. Long Wave Elasticity Line If the motion were controlled by elasticity alone the equation would be and if \ were so large that . could be neglected with respect to unity, the above becomes b 2— Y trig The straight line on the chart marked ‘ Long Wave Elasticity Line’ is the homologue of this equation. It makes an angle tan? with the decreasing direction of the axis of A, and in the diagram is placed for the case when e, E, and p have the values above quoted. b 26.—Short Wave Elasticity Line.—This is the homologue of Was ch? and is already on the chart, for the case when the quantities concerned have the values already taken. 27.—Complete Elasticity Curve.—lf the waves were governed by elasticity alone, the homologue showing the value of w for a given value of \ would be coincident with the short wave elasticity line when \ was small, with the long wave elasticity line when \ was great, and would run beneath both lines and leave them to the greatest extent where they eross. To draw the complete elasticity curve we have only to multiply each wu by VA — which can be done by one setting of the slide rule as iF previously shown. _ 28. The Two Gravity Lines and Complete Gravity Curve.— By exactly similar methods the two gravity lines and the complete gravity curve can be inserted on the chart. The long wave gravity line is the homologue of w=dan., The short wave gravity equation is a urn? Cc and the complete gravity curve is got by mechanical computation, by the 168 REPORT—1898. same setting of the slide rule as used for the complete elasticity curve, from equation ! 29. The Two Complete Curves are Translatants.—If in the gravity equation 1 lal : cn are Pw a,c, \, and wu are written a’, c!, ——, w _, the equation is unaltered. Cc ac Therefore it is a translatant with respect to a and c. Similarly the elasticity equation is a translatant. Subsequently it will be shown how to shift the elasticity and gravity curves to allow for changes in e, E,g, p,and s; but in whatever position the two curves may be on the chart the complete homologue of the equa- tion in which both effects appear is found by the method explained in § 11. 30. Translation of the Elasticity Curve-—I. New values for e. In the elasticity equation it is seen that if e becomes ne and \, mA: w remains unaltered. Thus to find new position of elasticity curve move it to the right through a distance log n. II. New values forE. If E becomes xE and wu becomes w/m equation is unaltered. Thus to shift the elasticity curve move it through e log n upwards. III. New values for s. When s becomes ns, \ becomes nA and w R becomes wn-?, the equation being unaltered. Thus to adapt to new : 3 values of s move curve log n to right, and 5 log w downwards. } It is perhaps worth noting that the complete elasticity curve could have been computed from and the long wave elasticity line. Also the complete gravity curve could have been obtained from yee A+e and the long wave gravity line. But in the fraction both numerator and c denominator change, and a separate setting of the slide rule would be necessary for every new point found on the complete curve. ON THE USE OF LOGARITHMIC COORDINATES. 169 TV. New values for p. If p changes to mp then wv and X must become r nu and —. vi 31. Translation of the Gravity Curve.—New values for e. Tf e, X. and uw are changed to ne, nd, and /un the gravity equation is unaltered. Thus if e becomes ne move the complete gravity curve log m to the right and : log 2 upwards. It is unnecessary to show that similar translations may be found for changes in g, p, and s. 32. Scales Lines for Complete Gravity and Elasticity Curves.—Two scale lines would be needed for each curve to permit of complete generality. Thus the gravity curve would have scale lines for changes in g and in se we ' ek se ; - ; the elasticity curve, scale lines for —— and —. These scale lines would p p all be put in on the same principles as those in the former part of this aper. i P33. Scale Lines for Thickness.—Two scale lines are inserted on the chart marked ‘ Elasticity Scale Line for Thickness’ and ‘Gravity Scale Line for Thickness.’ The first of these lines will be understood at once from paragraph 30, I. From paragraph 31 the direction of motion of the gravity curve in order to adapt it to new values of e must make an angle tan ~ : with the in- a creasing direction of the ordinate of \. Any line drawn on the chart in this direction can be made use of as a scale line. It is convenient, how- eyer, to have the scale line placed in a position so that it cuts the complete gravity curve or its attendant short and long wave gravity lines on the ~ chart. The scale line has been drawn at the appropriate inclination through a point on the short wave gravity line where \=10000. Now the thickness of ice is here 100 ; if the scale line be marked 100 at this point it must be graduated in either direction, so that when the curve (and its attendant lines) is moved along the direction of the scale line, the point of intersection of the short wave gravity line and the scale line shail read the thickness on the latter. The scale line must be graduated by a loga- rithmic scale, so that the readings increase ten-fold for every large square moved through to the right : this is done at once by the graduations on the paper without making a special logarithmic scale. The complete curve for the case when the values of g, p, s, E are the same as before and e=1 is inserted on the chart. It cuts the elasticity scale line for e at graduation 1. If it were only desired to make the chart give at once all values for w and \ when one other quantity such as e was varied the second method of treating the original equation would be the better ; but it would become somewhat confusing to use a succession of scale lines in order to adapt the chart to changes in a number of the quantities concerned. If more than one of these has to be altered it would be more convenient to employ the former method. It must be noted that the complete curve is calculated from the position of the gravity and elasticity curves by the method of $11. A small portion only joining the two branches has to be drawn, as the 170 REPORT—1898, complete curve soon becomes indistinguishable from the two component curves. On Several Outstanding Matters in Connection with the Chart. 34. The long wave lines of the chart may be joined by a curved portion to represent the complete long wave curve, which is the homologue of b Ra Uw OAT ae This may be obtained by using the method of the root of the sum of two squares ; or it may be got by one setting of the slide rule from the short wave gravity curve, this latter curve being the homologue of a b u?==—)? + — c rane b\Xr =(a\+_) — (« +5). In this case the A being read directly from the chart no thought is necessary in the operation, the lengths being simply transferred by the proportional compasses. On the chart when p, s, p, E have the quoted values and «=100 the complete homologue to the original equation is practically coincident with the long wave curve in the curved portion of the latter. 35. It is interesting to compare one of the homologues of the original equation with the wave and ripple curve of Mr. Boys. In the latter on the left we have the capillary ripples where the curve is straight, then the curved portion as far as the point of minimum velocity represents ripples, in the propagation of which gravity has an increasing influence : this is followed by a curved portion in which the surface tension effect is waning, and the gravity influence waxing ; finally we have the straight portion which represents waves in which the influence of capillarity is negligible. The shape of the curve on the chart varies as the quantities g, e, E, p, and s alter,as has already been seen. The elasticity and gravity branches always become coincident with the short wave elasticity and long wave gravity branches as we pass to the left and right respectively through a sufficient range. Consider now the complete curve on the chart representing approxi- mately the facts when the solid is ice and the liquid water and e=1. Waves whose length is less than about 420 correspond to ripples ; when the wave length falls below about 80 we have the analogues of capillary ripples. "36. The value of \ for which wis a minimum is a solution of the equation P+ 2cr4 — 3b A— 2be_,, a a obtained by differentiating the original equation and putting em The ordinary practical way of solving this equation (by numerical compu- tation) is by Horner’s method. It has only one real root which is approxi- mately 419 with e=1. This root is at once given approximately by the eo ON THE USE OF LOGARITHMIC COORDINATES. Lal chart, and also the minimum value of w is obtained at once by inspection without the trouble of substituting A=419 in the original equation. Logarithmic coordinates may be of use to find the roots of equations of high orders. 37. Lhe Homologues of Equations representing the Relation of u to X when <=some constant.—In the original equation let c=. The equa- tion becomes gy , 2n3E ant. Bf eae ol a ig. 2rs P For all values of ) included in the chart gx may be neglected with aT 23 respect to 3” # ; the homologue is a straight line identical with the elas- ticity scale line for thickness (if we take EH, p, s as before). In the same way horizontal lines drawn through the points of intersection of lines X =2, \=3, &e. with the elasticity curve for ice 1 unit thick give the velocity of propagation of waves on ice which is always x, . &e. thick. The size of the waves makes no difference so long as we confine ourselves within the maxv- mum range of Xon the chart. This process cannot, however, be continued indefinitely ; even when e becomes - the line becomes slightly bent upwards as A approaches 10°; when e= = or less the relation is expressed by the long wave gravity line already on the chart. A horizontal line v=245000 gives the velocity of propagation of waves when e=)/1°61 ; no matter what E may be, the velocity of waves whose length is 1°61 times the thickness of the ice (when p=s=1) is equal to the velocity of propagation of sound in the ice. The line is marked ‘Sound Line’ on tbe chart. Tue Usz or Locarirumic CooRDINATES TO FIND AN APPROXIMATE EQUATION CONNECTING A SERIES OF EXPERIMENTAL RESULTS. 38. In practical science this arithmetical problem often arises. If the numbers are merely to be recorded graphically it is always better to plot them logarithmically, as the sensitiveness of the record is independent of the distance of a point from the origin. Jf the law which governs the numbers is a straight line law, as is often the case, of course ordinary section paper should be employed. But if on plotting the curve on squared paper it seems to follow some other law, recourse should be had to logarithmic plotting. If the observer com- mences by trying to find an equation of the form y=an" by arithmetic he will probably restrict his trial to simple values of a and _k. By the use of logarithmic paper he avoids the trouble of looking up the logarithms (as Herschel had to do) and gains in accuracy. 172 REPORT—1898. As an example we will find equations connecting two series of experimental numbers (kindly furnished by Mr. Bruce Wade, of Trinity College, Cambridge). In fig. 3 these two curves are plotted logarithmically. They are each represented very nearly by straight lines, and the equations may be ob- Hinge. a EH fo i 4 1 fi | x ———> tained from the figure at once, the power of y being a tangent and the coefficient of x a reciprocal of an intercept. (ajay Ler. (6) of @=29e. When the equation connecting the values is of the form P=aatt ba" + Ke. the same method could be employed. TRI-DIMENSIONAL LOGARITHMIC COORDINATES. 39. The construction of a surface to represent the mutual algebraic relationships of three variables is in general a matter of great labour, involving the computation of a series of curves which have then to be placed at appropriate distances apart, and the surface constructed so as to pass through all the curves. Many equations in physics lend themselves very readily to discussion by nfeans of tri-dimensional logarithmic coordi- nates. Writing down a few which occur, we have pv=Ré, — Q=cr, ron /—. As one of the simplest of such equations we may take v?=gh, which is the equation of seismic ocean waves. Regarding v, g, h all as variables, the surface representing the equa- tion in logarithmic coordinates is drawn in fig. 4. This figure is a tri- metric projection of a model of the logarithmically ruled planes and the homologue of the surface v?=gh. It is obvious that scale lines could be used to represent changes in the quantities occurring in equations involving more variables. 174 REPORT—1898. SEMI-LOGARITHMIC COORDINATES. 40. For some purposes it would be an advantage to plot the logarithm of one variable against the real value of the other. For instance, suppose it were desired to find the logarithmic decrement of an amplitude which we were investigating. This could be done by setting out the logarithms of swings against the number of the vibration. If the logarithmic decre- ment did not vary the curve would be a straight line, and the logarithmic decrement would be proportional to the tangent of the angle which this line makes with the decreasing direction of the axis of the number of the swing. If, however, the logarithmic decrement varied with the time, the tangent to the curve at any point would give the logarithmic decrement at that instant. This example is only one of many which suggest them- selves ; the usefulness of the method in practical work would chiefly depend on the fact that it is easier to ‘smooth out’ a series of points which should be in a straight line than it would be to draw a logarithmic curve with an elastic rod, as would have to be done if the results were plotted on ordinary square paper. THE GRAPHICAL COMPUTATION OF THE HyprrRBoLic FUNCTIONS. 41. By the use of semi-logarithmic coordinates it is easy to construct a chart which shall give the values of the six usually used hyperbolic functions for a given value of the independent variable. I have drawn a diagram of this sort which has an accuracy of about one in two hundred, and hope to be able to publish one on a larger scale which shall have a greater accuracy. For the sake of clearness let the logarithmic scale be regarded as the vertical one and the scale of equal parts as horizontal ; further, let the component logarithmic scales in the vertical scale be equal toa unit of length on the horizontal scale. 42. The Meaning of a Straight Line on the Chart.—If a straight line be drawn arbitrarily on such a chart (see fig. 5) it gives a series of values for uw and f such that— J=10 c=: where / is the reading on the logarithmic scale and w that on the horizontal scale ; c is the reading on the logarithmic scale of the point of intersection of the line with the vertical line w=o ; & is the tangent of the angle which the line makes with the increasing direction of the axis of w. _ Thus any curve having an exponential equation of the form §: —elew is traced at once by drawing a straight line on the semi-logarithmic chart. No numerical computation is necessary ; the value of c is marked on the ° vertical scale when w=o ; if k be then marked on the vertical line through w=1, a line joining this last point to the point /=1, w=o (which may be called the origin) gives us the graph of T=. A line parallel to this through the first marked point gives the graph of S=ch, vVX——— mil flate 3. TTT TTT URUUUUUOHEOROSORE HTT OTT HUET TEE UEEEUT IUNIUGUERUG EEO nn CUUPEAAAUUONUONUEHOUROGUONOOSOONONNONRONUH NOPUUUUTET AG sSUTELEGEE TOG EE TTT TTT SLUT ST nase Hime! Hilt < < Ne Eo rs z ca E = 4 E = 5 5 IAAT a 3S Pi 68a Report Brit. Assoc. 1598, Hi I WUT ET Hill Ht Il ! - ! AHI HII HT A CUNSNNNLLLNATTH HY rfl! il mil HAH Mitt i MI UU elf ARI mM mi ii) TTT I) AM TT | | Ulityy ae TUustrating mes ie TI. Vincent's Paper on the Use of Logarithmic Coordinates. er i ATT i ss HATTA a | i Ht) | Hill INTENT TTT MITT Mitt | an nl NH qi ! is 1 MU . 6,—Bemi-Logarithmlo Ohart of tho Hyporbolio Functions, AE a ON THE USE OF LOGARITHMIC COORDINATES. 175 A line through the origin and the point f=10, w=1, gives S=10", and this line (which is at 45° to axis of wu, since log 10=1 by hypo- thesis) is a table of common logarithms ; the readings | of the w scale are the logarithms of the readings of the J scale. For a line representing y= ke the w is in any case the logarithmic of / to the base 4, so that the semi- logarithmic chart constitutes an infinite series of logarithmic tables to any base. 43. To draw a line representing e“. This line passes through the origin and the point f=e, uw=1l. The e“line is a table of natural logarithms, « being the natural logarithmic of / The accuracy with which such graphic tabulation may be performed is limited by the size and accuracy of the graduations. The size of the w graduations is a matter of choice, as semi-logarithmic charts have to be made and cannot be bought. The logarithmic scales are only obtain- able in one size on the ruled paper, but other logarithmic scales can be obtained from slide rules. Semi-logarithmic charts are free from the defect of ordinary gaol paper (as regards the proportionate accuracy of plotting) in the vertical direction. The percentage accuracy of the horizontal scale varies as the distance from zero of the abscissa. 44, To proceed to compute the hyperbolic functions other straight lines must be ruled on the chart. These are inserted without computa- tion. The line representing f=*~ is parallel to the e“ line, and is drawn through the point f=:5, w=0. The reflexions of these lines in the line f=1 give us the e“ and 2e~“ lines, while a line drawn through f==‘5, w=0, parallel to the last two, gives us —— 45, The Semi-logarithmic Graph of Sinh w.—Any point on this curve is found by reading off the values of a and = from the appropriate lines for a chosen value of 7. Subtract the latter from the former numerically and mark the result on the vertical scale through uw. In this way the curve can be readily drawn. 46. The Cosh w Curve.—This is conveniently drawn at the same time as the sinh w curve, the values being added. Both curves are asymptotic to the a line. 47. The Graphs of Cosech w and Sech u.—These functions being the reciprocals of those just traced, we have only to make the diagram symmetrical about the line he 1 to obtain the two new curves, They are asymptotic to the line 2e— 48. The Graphs of Tanh u ‘and Coth u.—These are drawn in from the sinh w and cosh w curves; the vertical distances between these curves 176 REPORT—1898. when set out above f=1 give the coth w curve, and when set out. below, the tanh w curve.! 49. A figure constructed thus forms a check on more elaborate numerical computation. It should be noticed that it can be drawn almost entirely by graphical methods, the only numerical value required being the number e. It is obvious that the semi-logarithmic chart provides a short and easy method of calculating the coordinates of catenaries of which cosh w (on squared paper) is one. On some Points in the Geometry of the Semi-logarithmic Graphs of the Hyperbolic Functions. 50. If we write down the other hyperbolic functions of «w when sinh w=a we find that the values of the six functions are identical with Fic. 6. those of wu’, where w’ is defined by sinh —— The six equations thus obtained may be expressed by saying that any function of @ is equal to that function of a’ which stands opposite to it in the table— sinh cosech cosh coth tanh sech. Thus (see fig. 6) if a straight line such as AA’ be drawn perpendicular to the axis of w and C be the intersection of this line with any of the six curves (in the figure with coth u); then if a straight line be drawn parallel to the axis of w to cut the curve indicated in above table at the point c (in this case cosh w) a vertical straight line through c will cut all When w is small, put tanh w=u and coth w=". ON THE USE OF LOGARITHMIC COORDINATES. Anz) the curves in values for f which are equal, each to each, to the inter- sections on the first straight line. Thus on the diagram the figure Aa’ is a rectangle whose sides AA’, aa' are bisected by the axis of wu, and the lines aA, bB, cC, a’ A’, 6'B’, e'C’ are all equal and parallel. This property would be of great value in the origination or verification of tables of these functions. If D be the intersection of the sinh and coth curves, it follows that DD’d'd is a rectangle whose sides are parallel and perpendicular to the axis of w. If Q be the intersection of sinh w and cosech uv, Q must lie on the axis of wu. It follows at once that EQE’ is a straight line perpendicular to the axis of w. 51. For the point E we have eh — et = a whence et= 14/2, e“= /2—1 Thus when w has the value given by (w=°88 approximately), sinh w=cosech w=1_ cosh w=coth w= VJ 2_ fA) sech w=tanh uw. a) The lines w=2 and w=} are inserted in fig. 6. RR’ is divided into four equal parts by E, Q, E’. 52. The value of w which makes cosh w=cosech w is given by sinh 2u=2, whence Gif o+ 7 eM / 5—2. The value of wu is given by 2Mu=logio ( /5+-2); and is approximately 0°72. The value of cosh w is given by 2 cosh? w=cosh 2u4+1 =/d+1. Thus 5+1 cosech w—=cosh w= a all sinh w=sech w= py pied tanh w= Vv a 1 a 1898. N 178 REPORT—1898. coth w= v a 1 53 When sinh w=2 Os=sK and cosh w=/5 cosech u=} sech w= — tanh w=— mS | oy and coth w= to] Sinh u/=} has the same values for the functions according to the table in § 50. On the figure we have FK= /5, i.e., the vertical reading at F is /5. GK=2 : II iE The lines FG, HK, KH’, G’F’ are equal. 54. To find uw when sinh w=coth uw, we have u=sinh w% =log, (sinh w+ V7 sinh? w+ 1 V5+1 5+1 Mulog : +/ va w=1-06 approximately. whence ConcLUSION. 55. It may be noticed that just as some equations are more suited to plotting by means of semi-logarithmic coordinates than by logarithmic coordinates, so advantage may be gained by having only one, or two, of the axes in three dimensions graduated logarithmically. The more frequent use of logarithmic geometry would tend to simplify many theoretical investigations, and, apart from theory, the aid which the method gives in computation seemed to be sufficient justification for the publication of this paper. In conclusion I wish to thank Professor J. J. Thomson for several valuable suggestions. Cavendish Laboratory, Cambridge. ON SEISMOLOGICAL INVESTIGATION. . 179 Seismological Investigations.—Third Report of the Committee, con- sisting of Mr. G. J. Symons (Chairman), Dr. C. Davison and Mr. Joun MILNE (Secretaries), Lord Ketvin, Professor W. G. ApvamMs, Professor T. G. Bonney, Dr. J. T. Borromury, Mr. C. V. Boys, Sir F. J. BRaMwELL, Mr. M. Watton Brown, Pro- fessor G. H. Darwin, Mr. Horace Darwin, Major L. Darwiy, Mr. G. F. Deacon, Dr. G. M. Dawson, Professor J. A. Ewine, Professor C. G. Knott, Professor G. A. Lesour, Professor R. MELDoLA, Professor J. PERRY, Professor J. H. Poyntine, Dr. Isaac Roperts, and Professor H. H. Turner. Drawn up by Secretary, JOHN MILNE. CONTENTS. PAGE I. Progress made towards the Establishment of Karthquake-observing Stations round the World. By JOHN MILNE. - : c - . 179 II. Notes on Special Earthquakes. By JOHN MILNE . - & ° . 185 Ill. Catalogue of Earthquakes recorded in Tokio, December 17, 1896, to December 16,1897 . : F ; F : é : : g . 189 IV. Earthquakes recorded at Shide (Isle of Wight), Edinburgh, Bidstone, and certain Stations in Hurope, with Discussion on the same. By JOHN MILNE. + : : : : : 5 : : : : . 191 V. On Certain Characteristics of Earthquake Motion. By JOHN MILNE , 218 VI. Magnetometer Disturbances and Earthquakes. By JOHN MILNE. . 226 VII. Suboceanic Changes in Relation to Earthquakes. By JOHN MILNE . . 251 VIII. A Time Indicator, By JoHN MILNE - : » 255 IX. On the Civil Time employed Throughout the World. “By Joun MILNE » 255 X. Great Circle Distances and Chords of the Earth. By JOHN MILNE, » 256 XI. Certain Small Fractions of an Hour. By SHINOBU HIROTA . . . 257 XII. Harthquake Observations in Italy and Europe. By JOHN MILNE . . 258 XIU. Preliminary Examination of Photograms obtained with the Seismometer in the Liverpool Observatory. By W. E. PLUMMER . é : . 272 XIV. A List of Reports relating to Earthquakes, published by the British Association : : : : 5 - : . . : . 276 I. Progress made towards the Establishment of Larthquake-observing Stations in various Parts of the World. Ty the report for 1897 there will be found a copy of a circular inviting co-operation in the establishment of a seismic survey of the world, which, with the kind assistance of the Foreign, Colonial, and India Offices, was forwarded to many countries and colonies. The result of these communi- cations, together with private correspondence, has been to establish or arrange for the establishment of instruments at twenty-two stations. The following notes indicate the position we hold in regard to these stations, and the direction in which further co-operation may be expected. The instruments at Shide, in the Isle of Wight, are indicated as Nos. 1 and 2, but it is only No. 1 that is of the type recommended by this com- mittee. No. 2 consists of a pair of horizontal pendulums writing on smoked paper. Both were purchased by Government grants from the Royal Society. N 2 180 REPORT—1898. 1. Canada: Toronto. Meteorological Observatory. Professor R. F. Stupart, Director. The instrument (No. 3) reached this station during the meeting of the British Association in August, 1897, when arrangements were made for its installation in a small building outside the Magnetic Observatory. It has already yielded several good seismograms, the most important being that of a. West Indian earthquake on December 29. This and other disturbances were also recorded in the Isle of Wight, and are described in this report. Much trouble was occasioned by the frequency and magni- tude of ‘tremor’ storms, especially on frosty nights. Although the marked character of these was reduced by copious ventilation, Professor Stupart writes me that with the hope of getting rid of them altogether he intends to move the instrument inside the main building of the observatory. This instrument was provided by the Meteorological Observatory, Toronto. 2. U.S.A.: Cambridge, Mass. Harvard University.—Professor E. C. PrcKERING. This instrument (No. 4) was shipped from London in September, 1897. On April 13, 1898, Professor Pickering wrote that the instrument, ‘which was purchased by the Harvard University, is to be shipped to their observatory in Peru. 3. India: Madras. Nungumbaukum. The Astronomical Observatory. Dr. Micnin Smiru. This instrument (No. 5), after being tested in the Isle of Wight, was delivered at the India Stores in October, 1897. It is now in Madras. It was provided by the Indian Government. ‘4. Spain: Cadiz. San Fernando. Instituto y Observatorio de Marina. ; Captain J. VINIEGRA. For this instrument (No. 6) the thanks of our committee are due to Mr. R. K. Gray, at whose expense it was constructed. It was shipped in December, 1897, and Captain Viniegra has sent a sample of its records, together with a plan of the observatory, showing the position in which it is installed. 5. US.A.: Philadelphia, Penn. Strathmore College. Professor S. J. CUNNINGHAM. This instrument (No. 7) was constructed at the expense of Mr. Joseph Wharton, 206 Philadelphia Bank Building, Philadelphia, and presented by him to the above institution. It was shipped from here in November, 1897. Mr. Wharton very kindly offers further co-operation in the work of this committee. Professor Cunningham has written describing the installation. 6. Japan: Tokio. Imperial University.—Dr. F. Omori. In a despatch, dated November 22, 1897, Her Majesty’s Minister, Sir Ernest Satow, has the honour to inform Lord Salisbury that he communicated with the Japanese Government respecting our circular to which a reply ON SEISMOLOGICAL INVESTIGATION. 181 was received from Baron Nishi to the effect that the authorities concerned have decided to co-operate with the British Association. The instrument (No. 8) was shipped in February, 1897. 7. England: Surrey. Richmond, Kew Observatory.—Dr. CHARLES CHREE, J.R.S, The instrument (No. 9) was delivered on March 8, 1898. It was pur- chased by the Kew Committee, and is now in operation. 8. Canada: British Columbia, Victoria.—E. Barnis Rewp. The instrument (No. 10) was sent on March 21, 1898, to the care of Professor Stupart, who will see to its installation. It was paid for by means of the British Association grant given in Toronto, 1897. 9. Java: Batavia. Magnetisch en Meteorolgisch Observatorium. J. P. VAN DER Srox, Director. This instrument (No. 11) was shipped May 1, 1897. It was purchased by the Dutch Government. 10. Africa: Cape Town. The Observatory.—D. Giut, F.RS., Director. On March 19, 1897, Dr. Gill placed our circular before the Admiralty recommending that co-operation be granted. He also pointed out to the Lords Commissioners of the Admiralty that the British Association Committee undertook the labour and cost of discussing results. The instrument (No. 21) was purchased by Her Majesty’s Government. 11. South America: Argentina. Cordova. The Observatory. W. G. Davis, Director. In Nevember last, after showing Mr. Davis seismograms, he visited Mr. Munro’s workshop, where he ordered an instrument. This instrument (No. 14) was shipped from London on May 13, 1898. 12. India: Bombay. Colaba. The Magnetic and Meteorological Obscrvatory. N. A. F. Moos, Director. The orders for instruments to be established at Bombay and Calcutta originated through a letter of recommendation from the Government of India, Department of Revenue and Agriculture, dated October 7, 1897, addressed to Her Majesty’s Secretary of State for India. 13. India: Calcutta. Alipore. Meteorological Observatory. (See Note relating to the Bombay Instrument.) These instruments (Nos. 12 and 13), which were purchased by the Indian Government, were delivered at the India Stores on April 27, 1898. 14, Mauritius: Royal Alfred Observatory —tT: F. Cuaxton, Director. On April 29, 1897, Mr. Claxton wrote that if our committee were prepared to grant 25/. towards an instrument he might spare 25/. from the Government Grant for 1898. Mr. Claxton’s offer was accepted, and the instrument (No. 17) was despatched in July, 1898. 182 REPORT—1898. 15. New Zealand: Wellington.Sir James Hector, F.R.S. Sir James Hector referred our circular to the New Zealand Govern- ment, who agreed to ask Parliament for the necessary grant to purchase instruments. On July 30, 1897, Sir James ordered two instruments (Nos. 16 and 20). The former of these was despatched in June, and the latter was despatched on August 31, 1898. 16. Egypt: Cairo. Abbasich. The Observatory. Mr. W. J. Wilson, Inspector-General of Irrigation for Upper Egypt, forwarded to the Ministry of Public Instruction our circular, with the result that H.E. Yacoub Artin Pasha, Under-Secretary of State for Public Instruction, directed that an instrument should be supplied to the above observatory. This (No. 22) will be despatched in September, 1898. 17. Scotland, Paisley. The Coats Observatory. The Rev. Andrew Henderson, Chairman of the Coats Observatory Committee, kindly brought our circular to the notice of that body, with the result that an instrument (No. 18) was ordered on February 21, 1898. It was sent to Paisley in July. 18. Mexico. On May 25 C. Romero, Esq., Acting Chargé d’Affaires at the Mexican Legation, 87 Cromwell Road, London, wrote the Chairman of our com- mittee that he was carrying out instructions received from the Minister of Encouragement (Fomento) of the Mexican Government to purchase a horizontal pendulum. This instrument (No. 19) was despatched on August 15. 19. Syria; Beyrout. Protestant College.—Professor R. H. West, Director. On the recommendation of Professor R. H. West an instrument (No. 15) was ordered for the observatory at the above college. It was despatched in June, 1898. Professor West says that all records will be at our disposal. 20. U.S.A.: Washington, D.C. Coast and Geodetic Survey. W. W. Dorrrexp, Superintendent. Mr. Dutftield wrote on July 16, 1897, that to take up the work proposed would need special authorisation and consequent provision of means. He would send copies of our circular to the United States Naval Observatory, Dr. J. G. Porter, Director of the Cincinnati Observatory, and to the Director of the Lick Observatory. 21. U.S.A.: Washington, D.C. US. Naval Observatory. Professor WM. HARKNESS. On July 19, 1897, Professor Harkness wrote saying that he hoped in the not distant future conditions may present themselves enabling him to co-operate. 22. S.A.: Colombia, Bogota. A despatch, dated August 12, 1897, from Montagu Villiers, Esq., British Vice-Consul at Bogota, to the Marquis of Salisbury stated that ON SEISMOLOGICAL INVESTIGATION. 183 the Director of the National Observatory at Bogota hoped before long to purchase the necessary instrument and co-operate in the work of our committee. 23. Australia: Sydney. The Observatory.—H. C. RussetL, F.R.S., Director. Mr. Russell regretted that, owing to want of funds, he was unable to take a share in the work. He will let us know whether his own pendulum is of any use. 24. China: Shanghai. Zikawei Observatory.—L. FRoc, S.J. ~ On April 5, 1897, Father Froc wrote regretting that he had neither the means nor the facility to establish an instrument at Zikawei, at which place, he states, the most severe shocks originating in Japan are not experienced. 25. Malta: Gozo. The College.—Rev. Jamns Scorzs, S.J, Father Scoles, writing from Beaumont College, Old Windsor, said : ‘No doubt some interesting results would be obtained in Malta, but in the College there no one has sufficient leisure to attend to such a work, nor are there any funds available.’ 26. Spain: Cadiz—W. G. FORSTER. Mr. Forster would like an instrument were he at a more favourably placed station, but not where he is. 27. Brazil: Rio de Janeiro. The Observatory —TuxE DIRECTOR. On April 20, 1897, the Director of this observatory wrote that he had received through Her Majesty’s Minister, Sir Edmund Constantine Henry, the circular issued by this committee. Last June a similar pro- posal had been received from Dr. Gerland, of Strassburg, to which he had replied favourably. Because nothing further had been heard from Dr. Gerland, the observatory at Rio was prepared to undertake the observa- tions we proposed. The letter concludes with instructions respecting payment for the instrument. On Jan. 20, 1898, the Fereign Office forwarded to me the translation of a note which Her Majesty’s Minister at Rio de Janeiro had received from the Brazilian Government, from which it appears that they are not disposed to co-operate in the scientific observations indicated by this committee. 28. Hawaii: Honolulu—W. J. Kenny, Her Majesty's Acting Commissioner and Consul-General. Shortly after the death of Commissioner Hawes, Mr. T. R. Walker, Acting British Consul-General, placed our circular before Professor W. D. Alexander, who wrote on July 16, 1897, that the proposed station would have to be established in connection with the Hawaiian weather service or at Oahu College, but at present he did not think that the necessary . funds were available. The subject should be taken into consideration by the next legislature. On December 27 Commissioner W. J. Kenny wrote suggesting that seismological investigations be taken up in Hawaii, and if I could send a seismograph he would see to its installation and working. 184 i REPORT—1898. ; 29, Physikalisches Central Observatorium.—Admiral Ryxatcunrr. Wass,-Ostr., 23 Linci Haus No. 2, 12/24, February, 1898. St. Petersburg. The Russian Meteorological Office think of establishing two instru- ments of the type recommended by the Seismological Committee of the British Association. It would, however, be first necessary to obtain the opinion of the directors of observatories where the instruments might be installed. Copies of instructions respecting the working of the instru- ments were required. Three copies of instructions were forwarded to St. Petersburg on March 3, 1898. 80. Kaiserliche Akademie der Wissenschaften, Wien. March 5, 1898. The earthquake commission of the above Academy inquired respecting the cost of a seismometer. I replied stating the price of instrument and its accessories, gave the address of the maker, and sent the Toronto Report for 1897. 31. Australia: Melbourne. The Observatory.—P. Baraccui, Esq. The Director of the above observatory wrote on February 1, 1898, in reply to the circular issued by our committee that he had applied to the Victorian Government to take part in our work, and had laid the matter before Section A of the Australian Association for the Advancement of Science. It is hoped that co-operation may be extended to us in the early future. The following abstract of a report of the Seismological Committee, of the Australian Society for the Advancement of Science is taken from ‘Symons’ Monthly Meteorological Magazine,’ March 1898, p. 26 :— ‘ Sersmological Commuttee. ‘This report was presented by the Secretary, Mr. George Hogben, M.A., of Timaru, New Zealand, and stated that the most interesting result ‘of the labours of the observers was the fact, based upon rough calculations, that the great South Australian earthquake of May 10, 1897, proceeded from a line parallel to the coast near Beachport and Kingston, and was possibly due to a sliding of one part of the crust upon another, such as forms what is called in geology a “fault.” This was probably deep, but the later and slighter shocks were surface ones, caused by readjustments of the immediate crust. The subject was still under investigation by the Secretary. But Mr. Hogben pointed out that it was as part of a world- system of seismological observations that the work of the Committee might be most useful. An international seismological committee had been set up, embracing all the ablest workers in every part of the world, and in co-operation with that committee were committees of the British Associa- tion and of the Royal Society. They desire especially to be able to track the microseismic vibrations or minute earthquake waves, which travelled from the sources of disturbance all round the earth’s surface, or it might be right through the solid mass of our world (if it is solid). The speed of these finer waves was many times greater than that of the larger waves felt by us, reaching a velocity as great as 12 miles per second, or even more. For the purpose of observing them the international committee had agreed upon a certain type of instrument—the horizontal pendulum— ee ——— i ON SEISMOLOGICAL INVESTIGATION. 185 to be used by all stations alike, as it was important that instruments of the same kind and of the same degree of sensitiveness should be employed for purposes of comparison.’ 32. Norway: Hammerfest. Dr. F. Nansen very kindly offered his co-operation in an endeavour to establish the station ‘ farthest north.’ 38. Ireland : Dublin. Professor W. F. Barrett is actively endeavouring to establish a station in Ireland, towards which I understand that Lord Ardilaun has given substantial support. It is interesting to note that this co-operation, and that referred to in notes (4) and (5), followed lectures bearing on a seismic survey of the world II. Notes on Special Earthquakes. 34. Foreign, Colonial, and Indian Offices. I was able to inform the Foreign and Colonial Offices that the official notification stating that there had been interruption of two West Indian cables connecting us with Venezuela on December 31 probably referred to the effects of a submarine earthquake, which happened at 11.30 a.m. on December 29 (see p. 214). I received letters of thanks for the information, the correctness of which was not confirmed until March 1. From the Foreign, Colonial, and Indian Offices I have received many communications relating to the establishment of instruments abroad and other matters connected with the work of this committee. These are referred to under other sections. 35. Correspondence respecting Earthquakes in the West Indies. Mr. Secretary Chamberlain directed that the following two despatches should be sent to me, adding that if I were disposed to interest myself in the matter he would take steps to obtain information on points about which it might be deemed worth while to make inquiry. The first despatch is from the Governor of the Leeward Islands, and the second from the Administrator of Montserrat :— Springfield House, St. Kitts : February 28, 1898. Si1r,—I have the honour to transmit to you the duplicate of a despatch from the Commissioner of Montserrat reporting that several severe shocks of earthquake have recently occurred in that island, which have caused considerable damage to buildings, although it does not appear that any lives have been sacrificed. 2. Mr. Baynes remarks in paragraph 5 of his despatch that these shocks of earthquake have been of frequent occurrence since the floods of November, 1896 ; a fact to which I have had occasion to refer in previous correspondence. 186 REPORT—1898, 3. What has caused this to be the case I am not prepared to say ; but I agree with Mr. Baynes that the subject is one of peculiar interest, and I should be glad if it could form the subject of scientific investigation. I have, &e., F. FLEemine. The Right Hon, JoSsEPH CHAMBERLAIN, M_.P., P.C. Commissioner’s Office, Montserrat : February 21, 1898. Str,—On Tuesday, the 15th instant, severe shocks of earthquake occurred in this island, which have since been followed by shocks of nearly equal severity, and have caused considerable damage to buildings. 2. The principal shock was at 11.16 a.m. on Tuesday, and was the most severe I have ever experienced. This was followed by shocks so numerous as to seem almost continuous until 3.45 p.m., when there was one of equal severity but shorter duration ; and during the rest of the day and the following night numerous shocks continued to be felt. On Friday, at 7 Am. and 4.25 p.m., and on Sunday, ‘at 9.20 a.m., very severe shocks occurred, and in the intervals minor shocks have been of constant occurrence. 3. The windmill tower at Gage’s Estate has been seriously damaged, and the chimneys on the Grove, Dagenham’s, Weeke’s, Gage’s, Paradise, and White’s Estates have sustained injury. One house at Gage’s has been so much damaged as to be made uninhabitable, and several houses in various localities have been injured. St. George’s Church and St. Anthony’s Church and Rectory have also sustained some damage. 4, The only serious damage to any Government building has been at the Poor House, where the walls of a small detached building have been so seriously damaged that it has been necessary to remove the inmates. There are cracks in the walls of the Court House and Treasury, but these appear to be superficial. On the public roads, especially those of recent construction, large quantities of earth and boulders have been shaken from the cliffs on to the roadway, but no further damage is reported. Several breaks in the water pipes supplying the town occurred through landslips in the ravines through which the pipe track passes, but these injuries were at once repaired. 5. These shocks of earthquake have been of frequent occurrence since the flood of November, 1896, and in my letter of May 3 last I gave some account of them up to that date. Of late they have greatly increased in severity. Some months ago a number of shocks occurred in Guadeloupe, but I have no recent information from that island. With this exception they have not been felt in the neighbouring islands. They would there- fore appear to be of local origin, and some disturbance of the volcanic springs in Gage’s Mountain has evidently taken place. The subject is one of peculiar interest, and seems to be well deserving of scientific investi- gation. I have, &c., Epwarp BAyngEs, Commissioner. His Excellency Sir F. FLEMING, K.C.M.G. The following two letters bearing on the same subject are also of interest :— ON SEISMOLOGICAL INVESTIGATION. 187 Richmond Hill, Montserrat, West Indies: March 2, 1898. Dear S1r,—I beg to inform you that since the flood of November 29, 1896, which caused great injury to life and property in this island, innumerable shocks of earthquake have been experienced. There are in this island several craters and sulphur springs, and there are also a few hot-water springs, all of which go to prove that the volcanoes here are by no means extinct, and it is thought by some per- sons that the mouth of one of the numerous craters has been filled up by a landslip caused by the above-mentioned flood, on the night of which there were several shocks of earthquake—the first experienced in Mont- serrat for a great number of years. It is possible that the filling up of this crater has been the cause of all the earthquakes we have been feeling here lately. Since November 1896 there have been experienced at least one _ thousand shocks of earthquake. The most severe shocks took place on the following dates :—November 29, 1896 ; April 22, 24, 25 and 29, 1897 ; July 28, 1897 ; December 4, 1897 ; February 15, 18 and 20, 1898. Those on February 15 exceeded all the others in point of severity. Some persons state that there were eighty-one shocks that day, of which forty-one were felt in three hours. The shock on April 29, 1897, though one of the longest, was felt throughout this portion of the West Indies, but was of slight force, and, notwithstanding its very long duration, did no injury here, though a great deal of damage was done at Pointe-a-Pitre, in the neighbouring French island of Guadeloupe. All the other earthquakes have been entirely local, having not even been noticed at Antigua, an island about thirty miles away, though those in April were felt at the isolated rock of Redonda, a few miles off the north coast of this island. Only the most severe earthquakes have been mentioned above ; but scarcely a day passes without our feeling a few shocks, and excluding * February 15 as many as thirty shocks have been felt in one day. During the last month or two the smell of sulphur from the craters has been very strong and disagreeable, silver tarnishing in town very easily. All the earthquakes seem to have had the same direction, viz., from *Gage’s’ Mountain, where the Soufritre is located (see Admiralty Chart of Montserrat), with the exception of that of April 29, which appeared to come from the direction of Guadeloupe, viz., the south. I am thankful to say that the shocks are usually of very short duration, averaging four or five seconds. Some of the oldest inhabitants of the island affirm that the worst shock, on February 15 (11.16 a.m.), was just as severe as the great earth- quake of 1843, but being of shorter duration did not do so much damage. Several buildings have been very badly damaged. Innumerable cracks have appeared in nearly every stone building in the island, including the Court Hall and the churches. These shocks of earthquake, which have been continually felt for the last sixteen months (i.e. since November 1896), are causing great anxiety among the inhabitants, and it is not known but that they may culminate either in a volcanic eruption or the numerous stone buildings, weakened 188 REPORT—1898. as they already are by these continual shocks, must in course of time be thrown to the ground unless the earthquakes cease. The whole subject seems well deserving of scientific investigation. The Government of the island is in a very bad financial state, and could not afford any pecuniary aid to an investigation, though it would doubt- less give as much encouragement as possible to the investigators ; but probably in the interests of science your committee or some other scien- tific society would bear the expense of making a scientific investigation which would be most interesting to science in general. Official reports in connection with the recent earthquakes have doubtless been sent to the Secretary of State for the Colonies, and I would suggest your communicating with the Colonial Office in considering the question ; but if your Society cannot send out a scientist I should be glad if the substance of this letter could be published in the English newspapers, and perhaps some scientist would take the matter up. I am, dear Sir, yours faithfully, H. pe Courcy HaAmizton, Fellow of the Royal Colonial Institute. JOHN MILNE, Esq., Secretary, Seismological Investigation Committee, London. Extract from Letter of Joseph Sturge, Esq., Wheeley’s Road, Birmingham, dated February 3, 1898. ‘JT think you may be glad to know of a somewhat curious phenomenon that has taken place in a small island in the West Indies, Montserrat, with which I am connected. ‘The island is the tip of a submarine mountain : it is 12 miles long by 7 wide, and 3,000 feet high. The sea is 2,000 fathoms deep all round the island. There are sulphureous springs of hot water which emit vapour, but no more active volcanic action, and for forty years there have been no serious earthquakes and very few noticeable ones. ‘On November 29, 1896, there was an extraordinary rain-storm, 20 inches of rain falling in the centre of the island in about twelve hours. Since that time the island has been subject to constantly recurring slight shocks of earthquake. They come almost every day, and sometimes several ina day. They do not do much harm, but keep people more or less in a state of alarm, and the curious problem is what happened on the day of the rain-storm that set the earthquakes going. ‘The sulphur springs have emitted a much more copious volume of gas since the change, so that silver now goes black three miles off. ‘It may be worth while to mention that in 1880 there was a similar flood in the neighbouring island of St. Kitts, and that the same night there was a volcanic disturbance in Dominica (150 miles from St. Kitts), and a boiling lake came into existence among the mountains there.’ On April 15 Mr. Sturge writes that the earthquakes increased in frequency and violence until the end of February. Almost all stone buildings were more or less injured. Since then there has been a great drought, coincidently with which the shocks have almost entirely ceased. Js this a propter hoc or only a post hoc ? ON SEISMOLOGICAL INVESTIGATION. 189 Ill.— Catalogue of Earthquakes recorded by a Gray-Milne Seismograph at the Central Meteorological Observatory, Tokio, December 17, 1897, to January 27, 1898. (Continuation of Catalogue commencing in the British Association Report, 1886. Maximum Maximum Period and | Period and a a Amplitude of i te of we} z Be | ‘ é Horizontal ertica: 4 No. | 3 | Day Time = Direction Motion Wotion. Bios of I EI A secs.| mm. | secs. | mm. —————————_ —————————————Ee anna 1896. H. M. 8. M.S. 1,816| XII. | 17 117 25 A.M. |0 47] S.S.E., N.N.W. | 0:2 1:9 02 04 quick sae) yy 17 6 14 06 P.M. | — — — = = = slight 1,818 9 20 5 03 38 a.M. | — — — == — = Ps 1,819 me 29 7 06 06 AM. | — — = = 7 3 % 1897. 1,220) I 8 5 57 25 AM. | — — — — = +. slight HGH | 4, 9 9 27 18 a. | — = cis ww Se = * 1,892] ,, 13 | 6 3939 am. | — = as aes 258 ae cf 1,823 Er 16 10 58 52 A.M. | -- — — 7 = = A 1,824) » 7 0 49 28 aM. |3 32) N.E.,S.W. 07 40 02 | 03 | clocks stopped, slow 1,825] 5, 17 5 36 36 A.M. | — — == = = = slight 1,826) 5 18 9 27 03 P.M. | — — — — pes = a 1,827} 5 20 10 46 22 A.M. | — — —_ = — = Z 1,828] 5; 23 212 42 pm. | — — — ae = Pam - 1,829; ,; 25 1 48 55 pM. | — — —- — = ‘= ie 1,830) ,, 27 3 46 38 PM. | — — = = a ae < 1832)| II. 1 10 33 35 P.M. | — — — = — — Me 1,832] ,, 4 213 46 P.M. | — — = = a3 pa F 1,833] ,, 4 3 51 56 P.M. | — — = = 2% 3 1,834] 4, 7 4 38 33 P.M. |5 47) N.W.,S.E. O7 17 —_ _ weak, slow 1,835) ,, 8 5 25 17 AM. | — = — = as a2) Fe 1,836| ,, 8 8 07 51 am. | — = Bie a SEN a i 1,837] 5, 9 10 1 35 pM. | — — = Aa = 2, cS = 1,838) ,, 11 0 5218 am. | — = = = = Ss es 1,839) ,; 11 7 2412 AM. | — — — — — = is 1,840} ,, 13 21911 am. | — = = — pas aé ie y 1,841) ,, 17 9 13 56 p.m. | — = = ate = an Ka 1,842) ,, 18 8°11 30 P.M. | — — 2 = = = a 1,843] ,, 20 9 52 28 P.M. | — — —_ = = = - 1,844] ,, 21 0 0417 P.M. | — — — = _— a ne . 1,845| 28 1 14 58 A.M. |2 22) N.N.W.,S.S.E. | 14 3H PaO |i 0s2 i ; 1,846] Ill.| 5 | 114 20 pm. | — = a aa LEP Fas s 1,847) ,, 5 5 27 41 P.M. |0 37 8.W., N.E. 0:2 06 O1 O1 quick 1,848] ,, 6 | 53612 am. | — = — — Sse | slight 1,849} ,, 7 3 22 46 p.m. | — — — = ms x2 cs 1,850] ,, 13 | 10 14 55 a.m. | — = = = Re, A - 1,851} 5, | 14 | 206 25 pm. | — = BSW | BB & 1,852) ,, 17 6 13 58 A.M. | — _ — = = pas > 4 1,853] ,, 20 5 32 34 aM. | — — ae = = — e 1,854] 5; 26 | 21157 am. | — = = ee El wt 2 3 1,855] 5 27 | 74926 pm. | — = ae a BES apes 1,856] 30 | 916 41 pm. | — = 2 a =| ee ‘9 1,857] IV. 3 8 30 45 am. | — = = nat BE | ab s 1,858), 4 | 3 32 38 am. | — = a3 uD Ss oo ss 7 1,859 ” 13 3 47 52 AM _ —_ — —, — = n 1,860) ,, 16 0 13 37 a.m. | — = = a BE ag eae a | 1,861 ” 16 3 42 08 A.M. | — — — = = Ss: Fs 1,862] ,, 24 | 9 48 49 PM. | — = = = BR is 1,863 ” 27 10 31 54 P.M. — _ — = —e a os 1,864 ” 30 403 06 P.M —— _ — —e — ies “ 1,865 3 4 42 59 AM. | — — = = mt ae ue ‘ 1,866 ” 3 6 29 39 A.M. | — —_ — — A nd ie 1,867] ,, 4 | 11 36 47 pM. | — = 33 ak ae a ei 1,868 ” 5 8 57 21 P.M. | — —_— = = Fa, — at y 1,869) ,, 6 | 6 46 35 am. | — -- La Se Ee het e 1,870 ” 6 7 34 0 AM = — — = a Sy i ‘ Beri) 6 | 94051 4m. | — = AN RS Var, ° | 1,872 ” 6 7 53 43 PM. | — —s = = = 25 a 1,873| 5, 7 | 25915 am. | — — ae ee i | 1,874! ,, 9 1110109 am | — — oe = ae = Ee 190 REPORT—1898. CATALOGUE OF EARTHQUAKES—continued. : Maximum Maximum Period and | Period and et a Amplitude of |Amplitude of 2 : s a. Horizontal Vertical Nature of No. 8 | Day Time S Direction Motion Motion Shock =| 2) A secs. | mm. |secs. | mm. H. M.S. M.S. 1,875| V. 12 3 30 11 A.M. | — _ = _ = _ slight 1,876] , | 12 | 61936 pw. | — - = [= f= : 1,877| » 13 2 28 59 pM. | — _ _— — — _ quick L378 18 | 1009 49 am. | — _ — — — _ slight 1,879 7 19 6 25 13 aM. | — _— = = >= — » 1880!) us 23 923 0 PM. |3 40) N.W., S.E. 157, 17 _ _ slow 1,881 ” 27 | 10 25 32 a.m. | — — = = _ - slight 1,882] VI ll 9 59 31 am. | —’ _ _— _ — _ 5 1,883 ” 13 11 24 14 A.M. | — — => = = — » 1,884] ,, 18 1 23 40 =M. | — —_ = = — _ ” 1,885} , 19 2 03 43 A.M. | — _ = = — _— ” 1,886 ” 22 12218 pm. | — _ = = — _- ” 1,887} _,, 27 5 48 23 am. |1 12) S.E., N.W. sli}ght sli ght quick 1,888| VII. 8 11 33 44 P.M. | — — = = —— slight 1,889] ,, 21 | 101252 pu. | — — — — —-|— * 1,890 <4 22 9 54 53 a.m. | — _ = — — _ ” 1,891 9 22 6 31 44 p.m, |4 34] W.S.W.,E.N.E. | 1:3 73 0-2 03 slow, weak 1,892] ,, 22 6 50 57 pM. | — — — — —|— slight 1,893| ,, 28 3 30 50 pM. | — — — — —|— a 1,894| ,, 29 6 3459 am. | — = = —_ —-}|— = 1,895] ,, 29 6 57 46 a.m. | — _ _ _ — _ » 1,896 = 29 10 31 54 AM. | — _ — — = = ” 1897) 5,, 29 10 44 50 p.m. |1 50) N.N.W.,S.S.E 07 07 slight - 1,898 OF 31 6 51 30 am. | — _ = _ —_ _ ” 1,899 | VIII. 2 2 02 47 a.m. | — _ — = _— _- » 1,900 = 4 10 19 22 p.m. | — _ — — =< — » abt. G01 ,, 5 912 23 a.m. |7 0 _ _— — _ _ slow, weak 1:902|'' ,, 5 929 22 am. | — — — = — | — slight 1,903 3 5 9 45 51 A.M. | — = = —= = po ” 1,904 - 5 10 21 09 a.m. | — _ _ _ _ _ = 1,905 Bs 5 10 44 23 aM. | — — — — — _— » 1,906 5 5 11 31 04 a.m. | — == = — — — ” 1,907 5 420 40 pM. | — _ _ —_ _— _ S 1,908 a 5 6 54 42 PM. | — = = = cs 3 ” 1,909 is 6 3 59 30 AM. | — _ _- _ _ _ ” LO, ug 6 415 39 am. | — _ _ — — _ a 1,911 4 6 8 48 57 A.M. | — = =e = = a ” 1,912] ° ,, Soi) 237009: Aaa a) — — _— = —-|]— * 1,913 4 8 11 55 36 a.m. | — = — = os oS » 1,914| ,, 8 6 28 46 A.M. | — _ _ — = = » OTS, sy 12 | 10 51 04 am. | — _ = ~ _ _ » 1,916] ,, 16 | 1148 01 am. | — _ — _ —-|—- os VOLTA” Gs 16 | 453 33 pm. |3 0| N.N.W., ESE, | 10 3 a slow, weak 1,918] , | 16 | 5 36 25 pM. | — = Se lee slight 1,919] ,, 16 6 11 35 pm. | — a = zk = r - 1,920/ ,, 18 | 11 55 27 am. | — = a as eS a= : 1,921 ae 21 0 28 16 AM. | — _ _— _ _ _ » 1,922] ,, 21 6 29 28 am. | — —_ — _— a = 1,923 3 22 0 23 58 A.M. | — _ = — = i » 1,924 25 25 5 14 33 AM. | — _ — — == == » 1,925] ,, 27 | 108 46 am. | — _ — — —-|—- = 1,926 a 27 6 19 20 A.M. | — _ _ == == — ” LT gy 27 8 46 19 AM. | — _— — _ - _ » 1,928) ,, 28 402_0 PM. | — _ = = — = 2 1,929| Ix 8 | 11 44 36 am. |1 15) N.N.E., SSW. | 08 06 slig} ht quick, weak 1,930 2% 11 14013 PM. | — — _— _— _ — slight 1,931] ,, 21 9 02 12 A.M. | — = = = Te = A 1,932; ,, | 23 | 6 27 03 am. | — _ —~/—-]—-]-— 1,933{ ,, 26 95918 PM. | — _ = — = = ae 1,934) X. 2 9 45 19 P.M. |3 25) W.S.W., E.N.E. at 1:8 0-4 0-2 quick, weak 1,935) ,, 7 140 02 pm. | — _ — _ _ _ slight 1,986] ,, 13 | 516 57 pw. | — = — = _ — 5 1,937} 5, 15 | 10 57 47 pm. | — — _— _ = = ” 1,938) , | 17 | 75405 pm. | — = — =e | = of 3 1,939 “9 20 3 01 18 P.M. |2 0 S.E., N.W. 03 1:0 0:2 0-3 weak, quick 1,940 °° 25 10 11.10 A.M. |0 50} N.N.W., S.S.E. | 02 05 _— — quick 1,941) ,, 26 | 1018 39 p.m. | — — _ _— —{- slight 1,942! XI. 2 1 42 26 am. | — — _ _ -/i- » teeta ar i ON SEISMOLOGICAL INVESTIGATION. 191 CATALOGUE OF EABTHQUAKES—continued. ee ee EERE EEINCEISSSSIN SEES Maximum | Maximum Period and | Period and a a Amplitude of |Amplitude of = : 3S be i Horizontal Vertical Nature of No.| co | Day Time ¢ Direction Motion. Motion Shock | 5 A secs. | mm. | secs, | mm. H. M.S. M.S A 1,943} XI. 5 6 44 11 aM. | — — — — — — slight 1,944] ,, 9 9 39 28 AM. | — _ _ - _ — ” 1,945) ,, 11 5 29 53 am. | — _ _ _ _ _ a 1,946) ,, 13 3 06 36 A.M. | — > = = _ _ » 1,947| ,, 13 6 16 24 A.M. | — _ —= _ — = ” 1948| ,, 14 913 43 AM. | — = = _ =— = ” 1,949] ,, 15 6 06 39 AM. | — _ _ _ _— _ # 1,950| ,, 16 8 03 16 AM. | — _ — _ _ = ” O61 | 19 | 10 16 22 AM. | — — — — —|— x 1,952| ,, 20 3 05 01 AM. | — _ _ _ — _ *” 1,953] ,, 22 | 10 04 36 A.M. | — _ _ _ —_ _ 39 1,954] ,, 23 5 56 54 pM. | — _— — — — | — a 1,955| ,, 24 9 06 54 AM. | — — — — —) || = S 1,956; ,, 27 0 12 56 AM. | — —_ — —_ _ _ + 1,957 | XII. 2 | 112315 pm. | — _ — _— _— _ BS 1,958] ,, 3 924 0am. | — — = = _ = » 959) ,, 4 918 10 a.m. |1 14] SS.W.,N.N.E. | 08 05 _ — quick 1,960) ,, 5 8 08 21 A.M. | — _ _ _ — a slight A1,961| ,, 6 2-03 45 A.M. | — _ —_ —_ —— — of 1,962| ,, 7 5-25 31 P.M. | — _— _ _ — _ =a 1,963; ,, 8 56 23 11 P.M. | — _ — _ _— _— ie 1,964; ,, 10 8 04 42 pM. | — — —_ — _ — = 1,965; ,, 12 6 40 49 A.M. | — _— = _— _ _— id 1,966; ,, 13 10 57 57 P.M. | — _— _— —_ _- _— a 1,967) ,, 16 8 47 43 P.M. | — — — _ _ _— a 1,968; ,, 17 9 26 19 P.M. | — _ —_ —_ —_— _— if 1,969; ,, 19 3.16 26 A.M. | — — _ _— — _ = 1,970! ,, 19 1 21 26 p.m. | — —_ = — —|— ys OTL | *y 21 5 14 41 aM. | — _ _ — _— — = 1,972) ,, 23 3 36 11 AM. | — _— —_ _— _ —_ = 1,973| , 23 8 45 53 AM. | — —_ —_ — _ _— x 1,974| ,, 23 0 26 04 P.M. | — _— — _— — — a 1,975) -,, 95 | 1 03:27) Pw, | — = = = = |S 1,976| ,, 24 3 36 26 PM. | — _ — — -- _ a ir 26 4 41 25 P.M. |3 20 S.E., N.W. 12 14 _— _— weak, slow 1,978) ,, 31 | 11 6214 PM] — — — _— — _ slight 1898. 1,979; I. 5 5 21 01 pM. | — _ —_ — — {| — = 1,980) ,, 13 8 16 22 am. | — _ — — — — i gst} ,, 14 30 — — — — _— TV.—EARTHQUAKES RECORDED AT SHIDE, AND ALSO AT OTHER STATIONS. Earthquakes recorded with a Milne Horizontal Pendulum at Shide, Isle of Wight, 1897-98. The time used is Greenwich mean (civil) time. Midnight =24 or 0 hours. P.T.s=preliminary tremors. Duration means the interval of time over which movements continued. An asterisk (*) indicates Earthquakes which are discussed separately, or of which seismograms are reproduced. No. | Date Time of Com- Remarks mencement 1597. H. M. S. 96* | Mar. 23 16 19 12 Small. O7*"| May 96 22 44 20 33 98* + 9 | 23 50 88 | Large. Exact commencement lost. P.T.s at least 3m. Duration 47m. 192 REPORT—1898. EARTHQUAKES RECORDED AT SHIDE, ETC.—continued. Time of Com- mencement iio 20 Sor9 48 45 4 56 44 9 34 22 Remarks. Moderate. P.T.s6m. Duration 36m. Small. Moderate. Smali. Large. P.T.s 17m. Duration 2h. Large. Exact commencement lost. Period of large waves 15s. Range 10mm. Assam. P.T.s exceed 10m. Small. Duration 10m. Origin, ” ” 7m. a » 10m. Three maxima. * zs 16m. ” r ” 8m. ” ” 8m. Ends 20h. 43m. 15s. Large. Origin, Albania. Small. ; Slight. Origin, Epirus. Small. Very large. P.T.s 7m. Two large maxima. Moderate. Commencement lost. Small. Very large. P.T.s 30m. Duration over 3h. Origin, Japan. Slight. Ends 8h. 56m. 22s. Small. ” Moderate. P.T.s 2m, 44s. ” ” 4m. Small. Large. P.T.s 8m. Duration 40m. PA » 8m. 4 38m. - » 40m. + 2h. 56m. E. of Borneo. Large. P.T.s 43m. Duration 2h. 56m. E. of Borneo. Slight. Ends 13h: 20m. 20s. Small. ” Moderate. Duration 27m. Small, Large. P.T.s 41m. Duration 2h. 30m. > 42m; + 2h. 33m. Slight. Ends 3h. 28m. 29s. Small. About this time. Small. aster Sao en Large. Small. Duration 22m. Origin, Origin, +, =~. a Re ee ee ON SEISMOLOGICAL INVESTIGATION. 193 EARTHQUAKES RECORDED AT SHIDH, ETC.—continued. Time of Com- mencement Remarks No. Date 152* | Nov. 25 10 1 48 Large. Ends 12h. 153* | Dec. 11 10 4 31 | Small. Duration 45m. 154 Brie fe 10 20 58 Moderate. 155* » 17 | 1830 0 | Slight. Ends 10m. 30s. on 18th. » 156* » 28 | 20 54 21 | Moderate. P.T.s 8m. Duration 24m. Observed in Toronto at 20h. 24m. 37s. 157* » 29| 114048 | Large. P.T.s 19m. Duration 1h. 22m. 28s. Origin, N. of Hayti. Observed in Toronto 1lh. 32m. 29s. 158* — — Dec. 29 to Jan. 1, slight tremors. 1898. 159 | Jan 3| 1441 2 | Small. 160 7 BA ealisaers Palla + 161* = 24 23 45 49 Large. P.T.s 16m. Duration 33m. Onsmoked paper, NS component, 8m. 34s. Toronto, 13m. 30s. on the 25th. 162* “ 29 | 13 44 8 | Small. P.T.s5m. 47s. Duration 13m. 1s. 163* » 29] 15 525 | Large. P.T.s 9m. 30s. Duration 1h. 1m. Smoked paper, NS component, 15h. 5m. 26s. 164* | Feb. 8 36 13 | End 9h. 19m. 28s. Record on smoked paper. 5 165 5 7 | 23 35 20 | Small. 166 » 8 1 47 32 fe 167 ” 8 168 “5 9 169 Be veh 22 BT 36 ” Duration 15m. UB) &3 and three others within 54m. Nots.—On February 5, about 9 A.M., when there were slight disturbances in Catania, Catanzaro (Calabria), Rome, and Livorno, and February 18, between 16h. 30m. and 17h. 30m., when there were feeble movements recorded at Catania, Ischia, Rocca di Papa, and Rome. The clock driving the photographic film at Shide had stopped. On the 5th it will be observed that a record was obtained on smoked paper. Note on the Edinburgh Bifilar, Extracted from a Letter received from Mr. Tuomas Huatu, of the Royal Observatory, Edinburgh. An inspection of the photograph shows but little trace of the diurnal wave. Measurements of the change of position of the light spot for every four hours throughout the month of March 1898 results in an irregular curve, which apparently indicates a slight movement to the north from noon to midnight, and to the south from midnight to noon. Maximum and minimum thermometers are being established in the bifilar room. _ _The mean of daily measurements between February 28 and April 2 indicate that the new movement of the light spot corresponds to a tilt of 174 of the frame. The photographs have not been subjected to the examination necessary to show whether there is a lunar effect. The instrument was first mounted in March 1894, at Carlton Hill, and removed to its present site, on Blackford Hill, in October 1895. It was mounted with photo-recording apparatus in August 1896. A second pendulum purchased out of grant from the Scientific Research Committee of sets - Society was mounted in May 1898. . 0 194 REPORT—1898. Movements recorded by a Darwin Bifilar Pendulum at the Royal Observatory, Edinburgh. Director, Dr. R. CopELand. The instrument was presented to the Observatory by the late M. ANTOINE D’ABBADIE in 1894. H. M. 8. 1 104 June 3 10 57 O | Slight oscillations and widening of line. 2 105 | a 12 J1 18 0 Ends at 13h. 12m. 3 116 | Huecct 13 40 0 | Fine oscillatory disturbance until 14h. 4m, 4 119 Aug. 5 1 239 | Fine oscillatory disturbance until 1h. 40m, 30s. 5 131 Sept. 17 15 55 O | Small oscillatory disturbance until 16h. 5m. 6 132 an lt, 18 2 0 Small oscillatory disturbance until 18h. 12m. 7 133 c 20 19 56 O Small oscillatory disturbance until 20h. 28m. Smaller oscillations 20h. 17m. to 20h. 28m. 8 134 sat gel 6 7 30 | Like preceding until Gh. 38m. 30s. 9 139 Oct 3 14 58 O | Very slight tilt to N. 10 140 55 iS) 028 O Small oscillatory disturbance until 50m. 11 141 HA 20 15 20 O Small oscillatory disturbance until 15h. 33m. 12 146 Noy. 14 15 29 O Tilt to N. 13 163 Jan. 29 1515 O | Small oscillatory disturbance until 15h. 25m. Observations at Rocca di Papa. By Dr. A. Cancani. : Instruments described on pp. 264-266. No. mee Dati ig Seal Maximum Remarks 1897 HM. S Hy) Mes: 1| 100 | May 23 — 13 17 10 | Small undulation. 2! 104 | June 38 54 30 | 10 34 O]| Endat10h. 40m. Period 24s, 3} 105 » 12/1118 Oj] 11 47.10 | At1llh.36m. Period 16s. 4/116 | July 21 = 13 50 O| At13h.45m. Period 10s. 5 | 117 sree — 11 26 0 — 6] 119 | Aug. 5 0 32 40} 1 8 380] End 2h. 12m, Tol boo » 26/16 46 30|17 O O| Period 18s. 8} 124 » 26] 22 8 30] 22 15 30 | End 22h. 30m. 9 | 131 | Sept. 17 | 15 50 0} 15 55 O | Period 18s. 10 | 132 » 17;1748 0/18 6 O — 11 | 433 » 20/19 25 0] 19 40 OJ] Period 18s, End 21h. 5m. 12 | 134 » 21] 58382 8] 5 46 O| End7h. 13 | 140 | Oct. 19] O 5 30] 051 O| Period 32s. At 25m. End 1h, 15m. 14] 141 » 20]}15 O 0] 15 80 O| End17h. Period 16s. 15 | 157 | Dec. 29] 1156 0/12 5 30| End 12h. 23m. H.W. component 1898 large. N.S. small. 16 | 161 | Jan. 24 | 23 49 0; O15 15 | End 45m., January 25 17 | 162 » 29]13 39 O| 13 39 17 | End 18h.45m. E.W. component. —| — — 13 40 0 — End 13h. 40m. 30s, N.S. component . small, 18 | 163 | Jan. 29/15 5 15/1511 O} Max.in P.Ts. 15h. 9m.50s. Waves commence 15h. 10m. 45s. —_ — —_— — 15 11 45 | End 15h. 40m. for E.W. — |, — — —_— 15 13 30 | N.S. component not so distinct. ———— ON SEISMOLOGICAL INVESTIGATION. 195 Records from W. E. Plummer, Esq., Liverpool Observatory, Bidstone, Birkenhead, Instrument a Darwin Bifilar Pendulum, provided by the British Association. No. ~ or] our wonbor Shide No. Date Time Remarks 1897. H. 12 20 to 12 18 10,, 722, 1 rd nee 16 50 ,, 18 7 12 16 18 M. 25 19 30 20 55 30 Small. Very small. Small. September 20 to 22 records not taken, Motion 0'008. Small. September 28 to October 1 records not taken. Small. October 24 to 26, records imperfect. Slight disturbance. October 29 to November 21 instrument dis- mounted. Displacement 0:12. Slight and irregular. ” Slight. ” Displacement O72 Slight disturbance. Very slight. January 20 to 22 clock stopped. Uncertain and very slight. Moderate. Slight. as movement. ”» ” »” ” Most considerable disturbance. Mo- tion 0/17. Disturbance. Slight. Moderate. On 15th no record. Trace irregular. Slight, Slight Trace irregular, Slight. Moderate. 02 196 REPORT—1898. Records received from Professor Kortazzi, Nicolaiew. The recording instrument was a von Rebeur-Paschwitz Horizontal Pendulum. Max = maximum. Dur = duration. . Commence- No. oeee Date ment Remarks 5 G.M.T, 1897 Fiery Eig PS: 1 97 May 5 | 22 12 0] Max. 22h,27m. Dur. th. 2 99 » 13 |12 2 0} Very large. P.T.s18m. Dur. 2h. 8m. 3 | 100 » 23 | 12 48 0 | Moderate. Max. 13h.9m. Dur. 59m. 4 101 aoe 23 57 O| Large. P.T.s 9m. Max. 20m. Dur. lh. 4m. No observations from June 3 to 29. 6 | 113 June 30 3 50 0} Moderate. Max. 4h.16m. Dur. 44m. 6 | 115 July 17 7 48 O|} Small. Max. 7h. 50m. 5s. Dur. 26m. fay) 116 » 21 | 138 43 O} Large. Dur. 35m. P.T.s 4m. Si aly i, 22 9 52 0 = 3 ofr. Prom Wart a pects: Aug. 2 |15 29 0] Small. ,, 10m. 10 | 119 . 5 0 17 0} Very large. Max. 31m. Dur. 3h. 35m, 11 122 a6 16 32 O} Small. Max.16h. 46m. Dur. 45m. 12 | 123 pi 2b. | 62 AO eG 3 » 21h. 57m. » 42m. 13 | 131 Sept, 17 | 15 40 0/j Very large. Max. 15h. 45m. Dur. 44m, Origin, Tashkent. 14,| 132 » 17 |18 O 0O| Small. Details lost. ¥ 15 | 133 » 20 | 19 23 30] Very large. Max. 19h. 29m. 5s. Dur. 4h. 16 | 134 gen! 4 57 0 | Very large. Max. 5h. 7m. The end lost. 17 | 138 Oct. 6 Zaz 680 | 7 Max. 13h. 30m Dux 1h. 36m. 18 140 eae 0 13 O| Very large. Max. 42m. Dur. 3h. lm. Pts Fm: 19 | 141 » 20 | 14 49 0] Very large. Max. 15h. 37m. Dur. 3h. 4m. P.T.s 11m. 20 | 153 Dec. 11 | 10 9 0} Moderate. Max. 10h. 28m. Dur. 1h. 10m. 21 156 | » 28 | 20 53 0] Small. Max. 21h. 4m. 30s. ~Durn } 29m. 22 | 157 | » 29 | 11 47 O| Small. Max. 11h. 55m. and 12h. 7m. 1898 Dur. 2h. 5m. 23 | 161 Jan, 24 | 23 49 30] Very large. Max. 5m. Dur. 37m. 5s. 24 | 162 » 29 ; 13 33 O |} Small Dur. 19m. 25 =| 163 » 29 |15 4 0} Very large. Max. 15h. 10m. Dur. 58m. —_—_—_—_—_—_=—_—=—=—“_—$—<—<—<—<—_—_———————————— ~ ON SEISMOLOGICAL INVESTIGATION. 197 Earthquakes recorded at Shide and also at Distant Localities. For a collective statement regarding earthquakes recorded in Italy I am indebted to Professor P. Tacchini, Director of the R. Ufficio Centrale di Meteorologia e di Geodinamica al Collegio Romano, Via del Caravita N° 7, Roma. He writes me that records from Padua have not been received since August 1897. Professor Stupart’s records from the Meteorological Observatory, Toronto, date from December 28, 1897. The Shide Numbers Rome Rocca di Papa Padua Sienne Pavia Ischia Italy generally Catania Toronto Edinburgh Bidstone Lt | Nicolson 8 | | | || _ — i) | iS a | | | Lie | 198 REPORT—1898. Observations at the R. Osservatorio di Catania e dell’ Etna. By Dr. A. Riccd. 1897-1898. Instrument a long pendulum, p. 259. : Commence- No. ow Date ment’ Remarks : G.M.T, H M.S. 1 100 Mar. 23 13 20 61] Small 2 101 af 24 O 51 46 | Small. Also 1h. Om. 2s. and Lh. 5m. 49s. 3 104 June 3 Drvbsee 42, ms Duration lh. 35m. 37s. 4 105 ARCs 11 17 22) Very large. Duration 4h. 51m. 38s. Max. range 32mm. Period of large waves lls. 5 116 July 21 13 39 4] Moderate. P.Ts. Im. 23s. Duration ih. 15m. 29s. 6 117 " 22 9 4 653 | Small. Exact commencement lost 7 118 Aug. 2 TDP OMEILT el 5's, ae 2 35 8 119 ; 5 0 24 35] Moderate. P.Ts.10m.29s. Duration 2h. 40m. 53s. 9 131 Sept. 17 15 15 6560] Small. Duration 2h. 36m. 47s. 10 133 4 20 LOM Ze - Period of large waves 11‘5s. Duration 2h. 10m. 45s. 11 134 “~ 21 5 29 32 | Small 12 138 Oct. 2 | 13 381 51 | Small. Period of large waves1ls, Du- ration 32m. lls. 13 140 “s 19 0 6 36 Small. Period of large waves 12s. Du- ration 52m. 42s. ; 14 141 x 20 14 49 26 |.Small 15 153 Dec.~ 11 9 51 28] Small. P.Ts. 14m. 21s. Duration ih. 20m. 54s. ’ 16 157 AS 29 11 29 10] Small. Period of large waves 23s. Du- ration 1h. 30m. 50s. 17 162 Jan. 29 |14 4 41] Large. P.Ts.1h.2m.19s. Range 18mm. Duration lh. 33m. 51s. Deductions based on the Preceding Records. In order to determine the areas over which each of the earthquakes recorded at Shide had been perceptible a list of these (see p. 191) was sent to observatories at the following places :— ; Edinburgh,* Bidstone,* Strassburg, Padua, Rome,* Rocca di Papa,* Catania,* Ischia, Nicolaiew,* Charkow, Potsdam,* Toronto.* Replies have been received from those stations marked with an asterisk. Dr. P. Tacchini, Director of the Ufficio Centrale di Meteorologia e di Geodinamica at Rome, in replying, called my attention to several earth- quakes which had been well recorded in Italy, but which did not appear on my list. A re-examination of my seismograms led to the discovery of certain of these, and the numbers on the Shide list were increased from 160 to 169. Records which ought to be strictly comparable are those from Shide, Toronto, and other stations at which the free horizontal pendulums adopted by this committee have been established. The records from Strassburg, Nicolaiew, Potsdam, and from stations at which there are free horizontal pendulums of the von Rebeur-Paschwitz or Ehlert types, provided that these instruments have been adjusted with like degrees of sensibility, should also be comparable amongst themselves. ON SEISMOLOGICAL INVESTIGATION. 199 If, however, certain of these instruments have been so arranged that their stability is feeble, or, in other words, so that their free period is large as compared with that of others, they can hardly be expected, even when placed side by side, to yield similar seismograms. A small horizontal pendulum with a period of, say, 50 seconds and a large multiplication may be continuously in movement over a considerable period of time. This being the case, it may often happen that the exact commencement of an earthquake may not be determinable. In the Strassburg records, for example, we find commencements of movement given so many minutes in - advance of other stations in Europe that for the present, at least, we are inclined to accept the conclusions to which they lead with some reserve (see Earthquake No. 83). In Italy there is a great variety of instruments which, for the most part, record with ink upon the surface of paper, or by means of indices writing on smoked paper. The ordinary pendulums vary in length from a few metres up to 25 metres in length. In Catania, for example, there is a pendulum 25 metres in length, carrying a bob of 300 kgs., and with writing indices multiplying its movements 12°5 times. It appears that these exceedingly long pendulums are sometimes affected by the action of the wind upon the building in which they are suspended. When this occurs it becomes difficult to determine with exactness the time at which an earthquake has its commencement. The horizontal pendulums are also characterised by their great size. The horizontal booms of such instruments at Rocca di Papa, which carry 25 kgs. near their outer end, are 2:7 metres in length, the tie running to a point 5°25 metres above the foot of each boom. They write with ink on a band of paper moving at a rate of 60 cm., or 2 feet, per hour. The open diagrams obtained from both types of instrument are excellent (see p- 207). Unfortunately, the enormous dimensions of these instruments preclude any extensive adoption by private observers. When these dimensions are reduced, as, for example, with the ordinary pendulums, the smaller of these, not having sufficient multiplication or inertia to over- come the frictional resistance of writing indices, fail in a greater or lesser degree to record the small preliminary tremors, with the result that the time at which an earthquake commences is apparently retarded. It is probably sometimes this which explains the great difference in the recorded times at which earthquakes originating at great distances have announced themselves at different recording stations in Italy and Europe. For description of instruments in Italy and at Strassburg see pp. 258-272. Since writing the Report for 1897 I have obtained a list. of records from Japan and the catalogue issued from time to time by Professor Pietro Tacchini in the ‘ Bollettino della Societa Sismologica Italiana.’ Mate- rials extracted from these sources enable me to throw further light upon records published in 1897. Wo. 1, June 15, 1896. (B.A. Report, 1897.) This is the disastrous shock the sea waves accompanying which occa- sioned the loss of nearly 30,000 lives on the N.E. coast of Japan, a description of which will be found in the Report for 1897. 200 REPORT—1898. Velocity of Propagation of Earth-waves. ice Ma pak, Maa 48. Time at origin. =) 10 Gol a0 Padua . . PLO AGN Time to travel. E s peay Ischia . : . ‘10 450 29 Sa . 119.2829 Rocca di Papa + $0) 456.4 18 4s oa i tO J » 26; V8 Catania (about) . 11 O O 5 heii eta E ool ene Rome . P a ee eee) fe. 47a a teste ; . 48 20 Distance on | Distance on kgs ere ppg a arc kms. chord kms. per sec. per Bee. Padua. : : 3 9490 8592 99 8-9 Ischia ; . : a 9879 8910 8-4 76 Rocca di Papa . : . 9879 8910 65 58 Catania . é : : 9990 8993 57 5-1 Rome : : ; : 9879 8910 3-4 3:0 Instruments employed, Padua . . Microseismograph (Vicentini) Pendulum, 1:5 m. Bob, 50 kgs. Free period, 2°4 secs. Multiplication by indices, 70 to 80. Ischia. . Horizontal Pendulum. Bob,12kgs. Free period, 11 secs. Rocca di Papa. Pendulum,15m. Bob, 200 kgs. Catania . . Pendulum, 25°3m. Bob, 300 kgs. Rome . - Pendulum, 8m. Bob, 100 kgs. ‘ No. 83, February 7, 1897. (B.A. Report, 1897). Bs eS Pts. 26min. 40 secs, Duration, 1hr. 6 mins. Strassburg 7 45 4 Horizontal pendulum and photo record. Edinburgh 7 49 7 Bifilar pendulum and photo record. Padua 7 49 30 Pendulum (Vicentini). Ischia 7 50 6 Horizontal pendulum, 12 kgs. Potsdam . 7 55 O Horizontal pendulum and photo record. Nicolaiew Wea we 4 + 55 5 Shide et TO OENS c 4 + Rocca diPapa. 8 20 0 Pendulum, 15 m., 250 kgs. Catania . 8 22 43 Pendulum, 25 m., 300 kgs. Rome 8 25 0 Pendulum, 16 m., 200 kgs. Tokio 7 38 33 Duration by seismograph, 5:47. Slow movement. At Ischia the period of the large waves reached 18-5 secs. The natural period of the pendulums in the meridian and at right angles was 12-9 secs. and 16:4 secs. At Rocca di Papa there were also two horizontal pendulums carrying 30 kgs., and with periods of 20secs. The N.S. component commenced at 8hrs. 25 mins., and the E.W. component at 8 hrs. 23 mins. 40 secs. At Catania the N.W.-S.E. component commenced at 8 hrs. 22 mins. 43 secs. ; N.E.-S.W. component commenced at 8 hrs. 27 mins. 49 secs. Velocity of Propagation.—For reasons similar to those given for Earth- quake No. 100, I shall assume that this disturbance had the same origin as No. 100, and that it occurred at least 2 mins. 30 secs. earlier than it was ON SEISMOLOGICAL INVESTIGATION. 201 noted in Tokio. The time at which it originated is therefore 7 hrs. 36 mins. On this assumption the following table has been calculated :— : Distance on : Velocity on | Velocity on — emake are in degrees pega are ae chord Ea. and kms. *| per sec. per sec. M. S. S Strassburg é 9 4 85:2 = 9457 8592 170 15:0 Edinburgh n 13 7 85:0 = 9435 8592 12:0 109 Padua 5 2 13 30 85°5 = 9490 8592 a ey 106 Ischia + 4 14 6 89:0 = 9879 8910 11°6 105 Potsdam . A 19 0 797 = 8846 8172 ET 71 Nicolaiew. Piles 77:5 = 8658 8000 6:8 63 Shide : 4 23° (3 86°5 = 9601 8700 70 63 Rocca di Papa. | 44 0 89:0 =9879 8904 37 3:3 Catania . ; 46 43 90:0 = 9990 8993 35 3:2 Rome é : 49 0 89:0 = 9879 8910 33 30 No. 84, February 7, 1897. (B.A. Report, 1897.) H M.S. Shide . : : é : : 7 . 23 54 50 (Corrected) Potsdam - : ¢ : = : SeEZ Seon) 20 No. 85, February 13, 1897. (B.A. Report, 1897.) Hy Me Se Shide 2 Sad Potsdam ame ytaU, Rome 2) 5. 1b0 Nicolaiew 29-6 aM Edinburgh Qe at ele Strassburg - ‘ 2 31 54 Not recorded at Catania, Teal and Rocca ai en No. 86, February 13, 1897. (B.A. Report, 1897.) Hoy Mes 8s M.S. Shide . : 5 . - 15 23 36 Duration 9 20 Potsdam : : ¢ Slop 5, 3.0. No. 87, February 15, 1897. (B.A. Report, 1897.) H. (M.." [8s Nicolaiew . a é é : : : 3 < ue 22re12. 10 Edinburgh . ‘ é ‘ ‘ ‘ - - 5 Cy Oe ete. O Potsdam . Z DO POO At Shide on the night of ie 15th-1 oth Hot et were intermittent switchings of the boom. February 19, 1897. At Shide instrument not working. He aM {S: Padua. F - 20 51 23 / Verona 4 . 20 58 O Pendulum (Vicentini) Rome. . . 20 59 50 Ischia . , . 21 1 25 Period reached, 22°6 secs. Catania. . 21 5 25 N.E-S.W.component. Period reached, 32 secs. ” A - 21 #6 42 S.E_N.W. Rocca di Papa . 21 11 0 ; 202 REPORT—1898. Het FM, Pye Pavia . : - 21 42 12 Pendulum, 44m. 40kgs, Nicolaiew . oe te a Potsdam : a2 S20 (about) Strassburg . - 21 11 39 §S.W.—N.E. component . : o) | 2D Memes) tu. Wi Edinburgh . eee etsor 70 Japan . - 20 41 O Not recorded in Tokio No, 88, February 20,1897. (B.A. Report, 1897.) H. WGK (8. H, M. 28. Shide . 3 - O 17 47 Four separate maxima ending1 16 27 Rocca di Papa . 23 55 O Onthe 19th Verona . : «) O RlZe 10 ! Padua . - -o Of 0 Ischia . s - O 15 35 Period reached, 29 secs. Rome 0 15 40 Catania . O 15 47 Pavia 0 16 30 Strassburg 0 11 15 S.W.-N.E. pendulum Nicolaiew . op oe plies ie: Potsdam OI 0. Edinburgh 0 32 #O At nearly all the above stations several distinct maxima were observed. No. 91, March 2, 1897. (B.A. Report, 1897.) HM 5. Shide . : 221) Asp aL Ischia . A - 21 25 22 KE. and W. horizontal pendulum, 12 kes. Nicolaiew . oue21 Tay ph Potsdam . *. 21 22 0 (about) 7 March 7, 1897. At Shide record hidden by small tremors. H. M. 8. Rocca di Papa. : : . : : - 4 51 O (about) y Tokio . 5 . > : . = . - 6 24 46 No. 93, March 16, 1897. (B.A. Report, 1897.) H M. Ss. M. Shide . 2 ; é : ‘ 7 @ 30-28 Duration. 5 ed Nicolaiew . 5 ‘ = 5 26. Blea: No. 96, March 28, 1897. On this day the following cables were reported as having been inter- rupted :—Tenedo-Dardanelles, Malta-Alexandria, Emden-Vigo (Bay of Biscay), and the Aden-Zanzibar. A shock was also reported from Montreal. A small disturbance was noted at Shideat 4 hrs. 19 mins. 12 secs. P.M., but it is not likely that it was connected with any of the above events. No. 97, May 5, 1897. Bag.) pss Shide . . - » 22 44 20 Small Nicolaiew . . - 22 12 0 With maximum at 22 hrs. 27 mins., which probably corresponds with the Shide record a i ce i el Not recorded in Italy, ON SEISMOLOGICAL INVESTIGATION. 203 No. 98, May 9, 1897. Tt is remarkable that this earthquake, with two maxima and a range of motion of 6 mm., does not appear to have been recorded in Europe. I should be inclined to place its origin west of Great Britain. No. 99, May 183, 1897. Hy My 8s Shide . : ° ; . : : . 12 16 24 Moderate Nicolaiew - : : : - - 12> -2) 0 Very large Apparently not recorded in Italy. It most likely originated to the east of Russia (see No. 97). No. 100, May 23, 1897. In Tokio, on the above date, a long, slow earthquake was felt at 12 hrs. 23 mins. G.M.T. In Hakodate and Sendai the times given are 12 hrs. 20 mins. and 12 hrs. The time records render it probable that the origin was nearer to Sendai than to the other places; whilst the character of the motion recorded in Tokio and Hakodate makes it probable that the focus of the disturbance would be 200 or 300 miles from those laces. With this assumption the time at the origin, which is likely to be in the Tuscarora Deep, would be about 2 mins. 30 secs. earlier than the Tokio record. The time registers are therefcre as follows :— He Mee Ss o M. Ss. Time of origin . i/V12 20!) 30 Nicolaiew . s . 12 48 O Time to travel 76 27 30 Ischia 4 5 SAS) bt Bie ins! 89 36)939 Shide F - = pli wills A Cece EP 86 54 50 Rocca di Papa . S io. i 10 ante, eps 89 56 40 Catania z ee 20 <6 1s AE BS 91 59 36 with one exception, increase with the distance of the same to the four observing stations. From the magnitude of these intervals it is not unlikely that only the maxima phases of motion have been recorded, the preliminary tremors having been so small that they are not shown upon the seismograms. Velocity Table, Velocity in km. per — Arce Chord reat Arc Chord Nicolaiew 2 ¢ .| 76°= 8436 km.| 7829 km. 51 47 Ischia a . és nl Ooo 5 Oey S910, 5 45 4 Shide a 5 $ . | 86°= 9546 ., 8668 ,, 2°8 26 Rocca di Papa. 2 Sal OOe = GOTO! sss 8910 ,, 29 2°6 Catania . ; i aH 91S = T0101) 4 9069 ,, 2°8 2°5 No. 101, May 24, 1897. : , H M. OS. Nicolaiew (23rd) ‘ 5 StS : . 23 57 O Large Shide. A 5 a ; 4 : - O 18 659 Moderate Catania . F - - O 51 46 Small Also recorded at other stations in Italy. 204 REPORT—1898. No. 104, June 3, 1897. Hy) pang 8: Catania. : - 5 : é ? ; : > _ Oo Dp) ae Rocea di Papa” . c : ; : : - : - 9 54 30 Shide . : : : : : : , . : YI 19% SH ALS Edinburgh . : : : : : 5 : : « S10 670 Nicolaiew not working. Also recorded at other stationsin Italy. At Shide there are three maxima phases of movement. Wo. 105, June 12, 1897. This earthquake is one which created so much destruction in Assam that it is intimated, in order to repair roads and buildings of the Public Works Department only, more than thirty-five lakhs of rupees will be required. The total cost of the earthquake is probably many times this sum. To meet the expenditure for the restoration of roads, &c., appli- cation has been made for a grant from the Imperial revenues, and we have here an illustration, which is repeated yearly, of the manner in which an earthquake in a distant country may affect directly or indirectly the finances of people in this country. To mitigate the effects of these disasters it is necessary that the ordinary practice of the engineer and builder should be modified, and to this end I am glad to say that this Association has lent support by the publication of several reports bearing upon construction in earthquake countries. The more important of these were issued in 1889 and 1891, and the substance of them has been most carefully considered in connection with the reconstruction of railways and other works now in progress in North-eastern India. This earthquake, which had its origin in a well-known seismic district, is probably the most severe and disastrous which, during historical times, has been experienced in this region. One evidence of this is the snapping and overturning of a number of ancient monoliths in the Khasi Hills. J. C. Arbuthnott, Deputy Commissioner of this district, who describes these stones, says :—‘ It would possibly give people in England an idea of the severity of the shock were the Druidical stones at Stonehenge and Stennis, in Orkney, similarly overthrown or broken in two.’ Similar evidence is found in the destruction of a stone bridge in the Kamrup district of very great antiquity. Records.—In the Isle of Wight, strange to say, the movements of the ground commenced whilst the photographic film was being renewed, an operation that only happens once a week. ‘The time record, therefore, only refers to maxima phases of motion and those which followed. The greatest range of motion was 15 mm., corresponding to a change in slope of about five seconds. A horizontal pendulum recording N.-S. motion on smoked paper indi- cated a maximum range of motion of 10 mm. and a period of 15 seconds. The following are the time records :— Bee. Poe. Shide 3 s - 11 29 10 Max. The preliminary tremors exceed 10 minutes ; therefore the commence- ment may have been 11 hrs. 19 mins. Catania . - So ir 22 Rocca di Papa . teat 18° 0 Edinburgh . : et 18" 70 Strassburg . : Soe Rs 2 Batavia. : - 11 16 40 Byelectrometer disturbance. ON SEISMOLOGICAL INVESTIGATION. 205 Velocity of Propagation : Time at origin, 11 hrs. 5 mins. 1 sec. Velocity Velocity on are. on chord. M Sz Km. Kun. Time to reach Catania . F 64° 12. 21 9°5 9:0 Rocca di Papa 65° 13. 59 86 81 Edinburgh . (ule 13 49 9:3 88 Strassburg . 66° 13 31 9:0 85 Shide ; 72° 14 59 88 8-2 The maximum angular tilting, as indicated on the photographic film, would be about five seconds of arc. Since writing the above several papers bearing on this earthquake have been received. From one, by Dr. G. Agamennone,! I have combined two tables giving the velocities of propagation on arcs of the preliminary tremors (P.T.s) and the long waves (L.W.s), and added notes respecting the character of the instruments yielding the records on which these determinations were made. Dis- tance P : : from | Observing Gur. | re | TW | ee at ee. Station of P.T.s | Kms. per sec. | Kms. per sec. Pendulum Ku. H. M. 8. ll 4 6 or 400 | Calcutta . Tah yy) eee ONS am — _ — — 5980 | Petersburg -| » 17 0} 80 or 93 | 2°59 or 2-78 | H.P. photo- graphic 7020 | Potsdam . Pel all Oy ie 8:0) seal O — — | H.P. photo- graphic 7150 | Catania . -| » 17 4] 88,, 10°8 | 2°51 ,, 2°65 | Long pendulum writing 7150 | Portici . Siler LO SStbis we lOrd) 2a wero = 7170 | Mineo Sil ye =O) |) Oe eS — — _ 7170 | Ischia by -| 9 17 2) 90,, 111 | 2°63 ,, 2°78 | H.P. writing 7220 | Spinea . | a SG: 81, 98 — — — 7240 | Padua. .| 4, 17 0} 92 , 11-4 | 2°66 ,, 2:81 | Pendulum writ- in 7250 | Velletri . PIE ME TMO OG 25 1 ih4: Soe Phe 7250 | Rocca di Papa. | ,, 17 5 8:9 ,, 10°99 | 2°66.,, 2°82 | H.P. writing 7260 | Rome 4 i an) Wy fae | 92 ,, 11°3 | 2°67 ,, 2°82 | Long pendulum writing 7310 | Florence . Solis Se 00) 8:6. 5,7 00:5 — — — 7330 | Wilhelmshaven. | ,, 18 9] 81,, 97 | 2°52 ,, 2°66 | H.-P. photo- graphic 7390 | Livorno . Silerss) ge, 0) |F1974.75. 1 0°G — —_— — 7440 | Pavia 3 sale, 18. 2 86 ,, 10°5 | 2°73 ,, 2°90 — 7560 | Utrecht . » 17 0, 96,, 11°9 | 2°37 ,, 249° | Magnetometer 7700 | Grenoble . les 10 «L’| S44, 10-1 _- _ — 7840 | Paris , ai 20 6) 6:4 5, .6:0 — —- | Magnetometer 7970 | Edinburgh ail, 18 0 94 ,, 115 | 2:78 ,, 2°93 | Bifilarpendulum photographic Mean 83 o0r10°6 | 2°61 or 2°76 * Tend, della R, Accad. dei Lincei, vol. vii. 1889, pp. 265-271. 206 REPORT—1898. It is worthy of note that we have here instances where higher velo- cities have been obtained from the records of instruments with frictional writing indices than from those where the records have been photographic, from which it must be inferred that the former indicated earlier phases of motion than the latter. At Rome the long waves had a period of 10 seconds and a maximum amplitude of 12’’.. The complete length of these waves, as computed from the above data, would be 54 kms., and the height of their crests about half a metre. When in Italy (see last section of this report) I saw the original seismograms of this earthquake at nearly all the stations I visited. The preliminary tremors and the greater portion of the succeeding heavy motion, as given by two different instruments, are reproduced (figs. 1, 2 and 3) from the ‘ Bollettino della Societa Sismologica Italiana,’ vol. ili, No. 9. They are appended to a paper by Dr. Cancani, describing his horizontal pendulums and the Assam earthquake. The upper figures show the E.—W. and the N.-S. motion as recorded by the large horizontal pendu- lums (for a description of which see p. 265). The lower figure gives the corresponding motion, as obtained from an ordinary pendulum of 250 kgs. and 15 m. in length, the movements of which are multiplied 12-5 times. The original diagrams are about two-and-a-half times greater than the present reproduction. The horizontal pendulums when writing have a complete period of 22 seconds. With the Indian earthquake the maximum range of motion was for the N.-S. component 5:5 cm., and for the E.-W. component 4 cm. The maximum change in the vertical for the N.-S. component was 13’. The 15 m. pendulum showed a change of 12”, whilst with a third inStru- ment, a simple pendulum, 7 m. in length, it was 10. For the large waves the complete period was 18 seconds. For these waves, with a velocity of 2‘7 kms. per sec., their length becomes 48-6 kms. If 7=length of wave, and a=the maximum angle of tilting, then height of a wave = = tan a = 45 cm. Tv No. 106, June 12, 1897. HM.) 78. Shide . = s - 19 53 19 Duration 10 mins. Strassburg . : . 19 23 27 t08 hrs. 35 min. 7 secs. with maxi- mum at 7 hrs. 51 mins. 33 secs. and 8 hrs. 0 min. 31 secs. Not recorded in Italy or Russia. No. 107, June 13, 1897. H. M. Ss. M. Shide . ° . - 2 “ : . 7 39 33 Duration 7 Strassburg . > - ‘ : 5 : Ww 28 55 Not recorded in Italy or Russia. No. 112, June 24, 1897. A disturbance was recorded in Ischia, Padua, and Rome, but it com- menced about 20 hrs. 30 mins., and not at 19 hrs. 34 mins. 53 secs., as noted at Shide. eet (‘tavoueg oJfopy) “LEST ‘ousnTy ZI ‘[esueg 9 WUSSY Ip ‘AOI ‘OIpUL o[[ap OJOWOIIOT, WIG] Ip OJeISoIjoMOMSIG ‘edeg Ip vODOY—'E “DIV ‘SN 9[v}UOZTIO OJopueg "LEST ‘ousNTH ZI ‘edeg Ip voooy ‘aIpuy eTap oyomemey—'zZ ‘IW na "G81 ‘ouSsnTyH ZI ‘[esueg o WesSY Ip VIOULAOIg ‘eIpuy o][ap OJoMMAIIET, “M-"M S[e}UOZIIO Ojopueg vedeg ip vo00y—'T “DIT 208 REPORT—1898. No. 118, June 30, 1897. : Bo nie! 16; Shide . : : : : ; : : : . 4.39 33 Nicolaiew . ; - - : - ° 5 5 - 3s poe 0 Not recorded in Italy. No. 114, June 30, 1897. H. M. s. Shide . : x . z c - 2 . (Loses In Italy about . . : : : : - : - JA oo 6 Origin Epirus. No. 115, July 17, 1897. aS Shide . ; : “ 3 : : s : PE (ms Nicolaiew : . : : : : : : : a a) Not recorded in Italy. No. 116, July 21, 1897. H OM. 8S. M. 8. Shide . » . 13 33 32 Preliminary tremors . m0 Nicolaiew . . 13 43 =O +5 5 4 0 Catania : +, 135 39) 34 ~ os 1 23 Rocca di Papa . 13 50 0 (maximum) Edinburgh . . 13-40 0 *Also noted at other stations in Italy. Wo. 117, July 22, 1897. “ Origin Japan : H OM «Ss. Shide before .11 20 O Rocca di Papa . 11 26 0 (maximum) Catania . . 9 4 58 (exact commencement lost) Nicolaiew apo. oe, O Tokio 3 . 9 381 44 Duration 4 mins. 34secs. Slow movement. No. 118, August 2, 1897. H: “MES: Shide < . : . 15 46 39) All small, and it is likely that Catania. 4 s ; a5 80) aL the records refer to different Nicolaiew és 5 > LS S290 shocks. Wo, 119, August 5, 1897. This earthquake was felt over the whole of Japan, from Nemuro, in the north-east, to Nagasaki, more than 1,000 geographical miles distant, in the south-west. The following notes taken from the ‘Japan Weekly Mail ” of Saturday, August 7, give the times at which movements were observed at different towns lying between the above-mentioned places. These times are expressed as Japan mean time, which is exactly nine hours in advance of Greenwich mean time. The earthquake of Thursday morning was of very long duration, but fortunately, owing to its gentleness, no damage was done. Starting at 9 hrs. 11 mins. 56 secs. A.M., the motion continued for 7 mins. 59 secs., the vibrations moving from E. to W. Four minor shocks were felt at 9,23, 10, and 11.31 o’clock the same morning, ON SEISMOLOGICAL INVESTIGATION. 209 Hakone, 9 a.m. (August 5), A strong earthquake was felt here this morning at about 9.20 o’clock Tt lasted for several minutes, but was quite regular (horizontal) in its movement. The Japanese say that they seldom have such a long or strong earthquake here, and they rushed out of their houses very quickly. Shizuoka (August 5). A slight earthquake was felt here at 9.20 a.m. Sendai (August 5). A strong earthquake occurred here this morning at 9 o’clock. Mito (August 5). A strong gale swept over the locality last night, and this morning a sharp earthquake was felt here. Mayebashi (August 5). An earthquake occurred here this morning at half-past 9 o’clock. Uyeda, Shinshu (August 5). An earthquake was felt here this morning at half-past 9 o’clock. The earthquake is also reported from :— Gifu, 7.57 A.M., slight. Gifu, 9.11 A.M., feeble. Nagasaki, 8.06 A.M., slight. Utsunomiya, 9.12 A.M., feeble. Kumagaya, 9.07 A.M., strong. Tokio, 9.12 A.M., feeble. Ishinomahi, 9.10 A.M., strong. Yokosuka, 9.12 A.M., feeble. Mito, 9.10 A.M., strong. Nagoya, 9.13 A.M., feeble. Aomori, 9.11 A.M., strong. Ahita, 9.20 A.M., feeble. Yamagata, 9.11 A.M., strong. Choshi, 9.12.A4.M., slight. Mayebashi, 9.11 A.M., strong. Numazu, 9.12 A.M., slight. Niigata, 9.12 A.M., strong. Nemuro, 9.12 A.M, slight. Kofu, 9.12 A.M., strong. Kushiro, 9.13 A.M, slight. Puhushima, 9.10 A.M., feeble. Hachihi, 9.15 A.M., sight. Nagano, 9.11 A.M., feeble. By reference to the catalogue of earthquakes recorded at the Central Meteorological Observatory in Tokio, p. 190 (Nos. 1901 to 1908), it will be seen that on the 5th the first disturbance was followed by seven smaller disturbances. From these reports, and from private correspondence with Japan, we learn that the movements were slow. This means that the period of the earth waves would be about three seconds. This being so, experience teaches us that places like Tokio were at a distance of 200 or 300 miles from the origin of the disturbance. The fact that movements commenced at and near to Tokio at about the same time they commenced at and near to Nemuro, whilst at Ishino- maki, Mito, Aomori, Yamagata, and other places lying between Tokio and Nemuro, movements commenced one or two minutes earlier, leads to the conclusion that the origin was off the east coast of Japan. From the time observations generally, the locus sought for may be placed ww be as centre of a circle which would approximately pass through Tokio, : P 210 REPORT—1898, Niigata, and Nemuro. This would ‘lie about 150 miles east of Sendai, at a depth of 4,000 fathoms, exactly at the bottom of the Nippon slope of the Tuscarora Deep. This is practically the same origin as that given for the shock of June 15, 1896,! as it is for many other disturbances which have shaken the whole of the Japanese islands. Facts to be noticed about this particular group of earthquakes are that they are the largest, that they originate along the base of the steepest slope, and that it is only occasionally that they are accompanied by sea waves. The disturbance of June 15, 1896, was accompanied by waves which resulted in the loss of nearly 30,000 lives, whilst the shaking of the ground was barely percep- tible at Tokio. The earthquake about which I now write as a producer of earth waves which could be felt was much more marked than that of June 15, and yet sea waves were not recorded. The inference is that the earthquake of August 5 was not accompanied by any marked displace- ment of large bodies of material at the bottom of the ocean, and its origin ‘was practically beneath the sub-oceanic crust. It is therefore possible that we have in the Tuscarora earthquakes examples of disturbances due to accelerations in the secular flow of a quasi-rigid subterranean material under the influence of continental load. If this is the case we should expect to find records of local magnetic perturbation. Velocity of Propagation of Earth Waves. Assuming the origin of the earthquake to have been 250 geographical miles to the north-east of Tokio, and the wave to have been propagated to that place at a rate of about 8,000 feet per second, then the time at which the earthquake originated in G.M.T. was August 5, 9 mins. 23 secs. G,.M.T.—Times at which Preliminary Tremors commenced in Europe. H. M. 8. M. §. Shide . . ; . O 22°35 Time to travel Z A 2 T8sl2 Rocca di Papa . 0 32 40 5 os ‘ " - 23.17 Catania F : . O 24 35 is 3 A 3 15 12 Nicolaiew . : .017 O a . ; i Don Edinburgh , : .1 2 30 Pr » (Large waves?) 53 7 Apparent Velocity of Preliminary Tremors. Distance Velocity in km. per sec. a On Are On Chord | On Are | On Chord Nicolaiew . a : .| 76°= 8436 km 7829 18? 172 Shide : 4 5 » |. 86° = 9546.50,, 8668 11 10 Rocca di Papa . : GO Se Skenls) 55 8910 7 63 Catania . : “ Sele WS cKO! a 9069 11 9:9 Wo. 120, August 16, 1897. H M. Sz Shide . . . . 8 6 29 Italy about . : - §8 15 O at Catania, Ischia, Rome, Rocca di Papa. Tokio . 3 5 . 7 58 33 Duration 3 mins. Slow movement. 1 Also see British Association Report, 1896, p. 153. | Shide 5 Nicolaiew . : Tokio Shide Nicolaiew . Rocca di Papa . ON SEISMOLOGICAL INVESTIGATION. 211 No. 122, August 26, 1897. And at, several places in ae Tokio Shide | Rocca di Papa ; And other stations in Italy. Shide Catania . Edinburgh . Nicolaiew . o_o Rocca di Papa . And other Italian stations. Origin probably Tashkent. Shide Edinburgh Nicolaiew . Rocca di Papa fg At 16 32 -0 14 46 30 16 8 46 No. 123, August 26, 1897. HM. S . 21 40 30 21 40 0O 21 19 20 No, 124, August 26, 1897. HA MSs: : 22 13 14 . 22 8 30 No. 181, September 17, 1897. H. M.S. 15 59 58 Preliminary tremors. 15 15 50 Small TD 2555 4,0 15,40... 0 lay -bO) 0 No. 182, September 17, 1897. TE ee Ms Ss M. 17 59 58 Preliminary tremors. 8 1S il 0) 18 O O Details lost 17 48 O And other Italian stations. The similarity of the Shide seismograms for Nos. 131 and 132 suggests that they originated at or near the same place. Shide Edinburgh Catania . Rocca di Papa Nicolaiew No. 133, September 20, 1897. ie ae M. 19 24 47 Large. Preliminary tremors, 40 19 56 O 19 25 2Small 19 265 0 19 23 30 Very large Also at other stations in Taly. Batavia F Shide . Edinburgh Catania . Rocca di Papa Nicolaiew - 19 14 30 by disturbance of an electrometer No. 134, ae aa 21, 1897. M. M. 28 Bl Large. Preliminary tremors. 43 Ie, 30 32 Small moa aw bo Ze) 8 57 0 Very large Also at other Italian MiGs apt 212 REPORT—1898. The above earthquake evidently refers to one of two shocks which were felt in Sandakan, on the north coast of Borneo, at 1.10 p.m. local time (about 5.20 a.m. G.M.T.) on September 21. It was sufficiently severe to crack a house and stop the town clock. These and other shocks accompanied the throwing up of a volcanic island in E.L. 115° and N.L. 5° 14’, about which on October 25 the ‘Times’ writes as follows :— ‘A New Votcanic Istanp.—The ‘Straits Times’ of September 29 states that, according to telegraphic advices from British North Borneo, an earthquake was felt at Kudat on September 21, as also a slight tremor at several places along the coast. About the same time a new island was thrown up from the sea between Mempakul and Lambeidan, 50 yards from the mainland, opposite Labuan, The island is of clay and rocks, and measures 200 yards long by 150 yards broad and 60 feet high. The island appears to be increasing in size, and emits inflammable gas in several places, with a strong smell of petroleum gas. The earthquake was not felt at Labuan.’ Comparing this disturbance 134 with 133, both which are large at Shide and Nicolaiew but small in Italy, we have an example of earthquakes apparently from the same origin, and as measured by the distance to which they propagated their vibrations of equal intensity, but which had very different effects locally. The former only slightly disturbed a magneto- graph in Batavia, 13° or 1,400 kms. distant, whilst the second created marked disturbances in such instruments at Batavia and other places, p. 243. Also the second was felt severely in Kudat and Sandakan (but not at Labuan), and is reported in the newspapers, whilst the first is passed without notice. : The similarity of the Shide seismograms for 133 and 134 also suggests that these shocks originated at or near the same locality. No, 135, September 21, 1897. Hye me iB? Hi) MP8s Shide : : 5 ° : : - ll 36 44tol3 20 20 About 13 hours in Central Italy there was a violent earthquake, which was recorded at all the observatories in Italy. It is hardly likely that this is represented by the latter portion of the slight disturbances at Shide. No. 138, October 2, 1897. E.. | Mp8: HM. 6S Shide . 13 36 389 Moderate Duration. 0 27 0O Catania . 13 31 51 3 nO ss2r ad Nicolaiew. 12 56 30 Very large - 1, (36° 40 Also at Rome. Tokio SONA Oi FS. gh ‘3 - 0 3 25 by seismograph No. 139, October 3, 1897. By as Shide ‘ 5 : : 4 shy TB aS Edinburgh = : a or -) 7) 14-585 90 Slight tilt to N. ON SEISMOLOGICAL INVESTIGATION. 213 No. 140, October 19, 1897. H. M. . . H. M, 8 Shide ; 0 6 52 Preliminary tremors. 41 Duration 2 30 0 Edinburgh O28 0 * 0 32 O Catania 0 6 36 Small 9 0 52 42 Rocca di Papa . oa | ies as (0) Fs li OF 30 Nicolaiew 0 13 ._0 Very large. P.T.s 7 is & er Also at Rome and Ischia. No. 141, October 20, 1897. Howey ES M. Pye IP Ss Shide + . 14 43 29 Preliminary tremors. 42 Duration 2% 33 0 Edinburgh wr te 20) 0 - Qa SUB Bea) Catania . 14 49 26 Small Rocca di Papa . 1a ig Clo s(t a Pie AN foe eV Nicolaiew . 14 49 O Verylarge. P.Ts 11 4 3 42 Also at Rome and Ischia. The similarity of the Isle of Wight seismograms for Nos. 140 and 141 together, that in each case the aentaines icone commenced its records 6 or 7 minutes after the Isle of Wight, indicate that these earthquakes had a similar origin. No. 142, October 23, 1897. H. M. &. Shide eae OO Atabout. 3 15 Oa disturbance was noted at Catania, Ischia, and Rome. No. 146, November 14, 1897. H. M. s. M. Shide : E . : . ae tans) 35 Duration 22 Edinburgh ; : : . So a FAS ee) Tiit to N. Not recorded in Europe. No. 152, November 25, 1897. H. M. s. Mi Shide i : é A H PP LO) el eas Duration 2 0 Catania . 3 ‘ z : a LOR Woes A te 23 Yo. 153, December 11, 1897. H. M. Ss. i. M. 5 Shide ¥ - 10 4 31 Small Duration 0 45 O Catania . . 9 51 28 P.T.s 14h. 21m. small - 1 20 54 Nicolaiew . 10 9 O Moderate re el Oe Tokio. . 9 40 49 Slight No. 155, December 17, 1897. H. M. Ht REM: sek Shide c Se ityass 0 Up to Dec.18 10 30 OU Slight ltaly, a a shock, Dec. 18 about 7.30 a.m. No. 156, December 28, 1897. } eh aes M.S. M. Shide . e200 64” 21 Moderate. P.Ts 8 UV Duration . 24 Nicolaiew crew? 163'" 'O Small 3 229 Toronto . - +20 124 37 » Pat spi * 10 a ei 214 REPORT—1898. Tt will be observed that we have here the records from three instru- ments not controlled by the friction of writing pointers, and therefore fairly comparable. No. 157, December 29, 1897. 1 epee ee mu. Ss. HM «6S Shide ; . 11 40 48 Large P.T.s 19 49 Duration 1. 22 28 Catania . 5 29 0 A 1 30 50 Rocca di Papa. 11 56 O = 0) 2i4.10 Nicolaiew . » 11-47’ -sOsF Sarai > 2 on 0 Toronto . . 11 32 29 No preliminary tremors in 1 Ona O Port-au-Prince. 11 22 7 Near the origin Also at other stations in Italy. In connection with this earthquake Professor R. F. Stupart, of Toronto, sends me the following note taken from the ‘U.S. Monthly Weather Review,’ January 1898 :— ‘December 29th. 6hrs. 32 mins. 43 secs. A.M., Port-au-Prince, Hayti, W.I. ‘ Professor T. Scherer reports as follows :—“ A severe earthquake was experienced at Port-au-Prince, lasting 1 minute and 31 seconds. The following are the conclusions to be drawn from the curves traced by the Secchi seismograph at the meteorological observatory of the College of St. Martial :— «« The entire phenomenon consisted of five consecutive shocks, the total duration of which was 48 seconds, and of a series of feeble move- ments very perceptible to an attentive observer. The first shock lasted 8 seconds: it began from east-north-east and from west-south-west. — The vertical component was quite strong at about the fifth second. The ~ movement immediately began with more force in the horizontal direction and less in the vertical : this lasted 11 seconds, and the direction from which it came was more toward the east. The third shock lasted 3 seconds, and was characterised by a very regular oscillatory movement. The first shock was the strongest, Jasted 10 seconds, began from the north-east, and died away in the south-west, with a vertical component that was scarcely appreciable. All the other movements, after the forty- eighth second, were feeble with the same horizontal direction. During all this time the seismic pendulum described ellipses in the sand whose major axes varied from north-east through the south to south-west. The Bertelli microseismometer was for a long time agitated, and finally main- tained a north-south direction. «« The same earthquake was felt in the neighbourhood of Port-au-Prince and with the same features. It seems to have been very violent in the interior on the island of Dominica.”’ This earthquake had a submarine origin, and interrupted the Cape Haytien-Puerto Plata and Puerto Plata-Martinique cables, together with the Dominican land lines. No. 158, December 29, 1897, to January 1, 1898. During this interval slight tremors were recorded at Shide. In Italy, — on December 29, between 11 hrs. 30 mins. and 13 hrs,, perturbations were recorded in several observations. On December 31, at about 17 hrs., a slight disturbance at Ischia and Florence was noted. ON SEISMOLOGICAL INVESTIGATION. 215 No. 161, January 24, 1898. Hy aca 8% HM S Shide 3 . 23 45 49 LargeP.T.s16mins. Duration . Oo 33° 0 Rocca di Papa 23 49 .0 % a1 056) 10 Nicolaiew . . 23 49, 30 Very large + 0 37 30 Toronto (25th). O 13 30 P.T.s 13 mins. 80 secs. No. 162, January 29, 1898. Be Me “B: Hw, 1S Shide 2 . 13 44 8 SmallP.T.s5mins.47secs. Duration 0 13 1 Catania . . 14 +4 41 Large P.T.slh.2m.19s. 5 1 33 51 -Rocca di Papa . 13 39 O 3 Om ape Nicolaiew . . 13 33) Oh Smail -s OLLI G Also at other stations in Italy. No. 168, January 29, 1898. HA. M. s. H. M. =) Shide é . 15 5 25 Large P.T.s9mins.9secs. Duration 1 1 0 Edinburgh a Bilisyrna lay ye: = 0. 10750 Rocca di Papa . 15 5 15 ~ 0 35 +O Nicolaiew . - 15 %44 =O Very large 33 0 58 O Laibach . saat ts paumem [ere ay i 0 49 #O At Shide the period of the large waves was 10 secs. The records evidently indicate the severe earthquake in Asia Minor, re- specting which London papers published the following Reuter telegram :— © Constantinople, February 3, 1898. ‘The earthquakes in Asia Minor continued at intervals from Saturday till Monday. At Balikesri, the military prison, two minarets and fifteen houses were totally destroyed, and every house in the town was more or less damaged. Twenty persons were killed and fifty injured. ‘Considerable damage was done also at Bighadidj, Inegeul, and other villages, though with what loss of life is unknown.’ No. 164, February 5, 1898. H. M. s. H. M. s. Shide . . . 8 36 13to9 19 28 Record on.smoked paper About 9hrs. perturbations were observed in Catania, Rome, Livorne, &e. From the preceding lists and notes it appears that between March 23, 1897, and February 16, 1898, 74 earthquakes were recorded at Shide, 38 of which were also recorded in Europe or America. The following are sketches of Seismograms obtained at Shide, Pots- dam, and Toronto. The times given are for the commencement of movements. Other phases of movement may be calculated on the assumption that for Shide, Nos. 85 to 138, 45 mm.=1 hour ; Nos, 140 to 157, 60 mm.=1 hour. Potsdam, 20 mm,.=1 hour. Toronto, 60 mm.=1 hour. 2.8.11 A.M. 0.16.24 P.M. ie No. 85.—Shide, Feb. 13, 1897. No. 99.—Shide, May 13, 1897. 216 REPORT—1898. 9.57.18 A.M, —_——— ee I Ie On No. 104.—Shide, June 3, 1897. 0.32.51 p.m, No. 105.—Shide, June 12, 1897. 1.33.32 P.M. No. 116.—Shide, July 21, 1897. iV ——4[ =» No. 19.—Shide, Aug. 5, 1897. 10.13.14 p.m. Se oe No. 124.—Shide, Aug. 26, 1897. ara oe —_—__— No, 124.—Potsdam. a ON SEISMOLOGICAL INVESTIGATION. 217 3.59.58 P.M. 5.59.58 P.M. Nos, 131 and 132.—Shide, Sept. 17, 1897. 7.24.47 PM. No. 133.—Shide, Sept. 20, 1897. jis agro No. rls 5.28.51 am. No. 134,—Shide, Sept. 21, 1898. ey) No. 184.—Potsdam. 1.36.39 P.M. Do H fn, —— eee h — No. 138,—Shide, Oct. 2, 1897. No, 138,—Potsdam. No, 140,—Shide, Oct. 18, 1897. 218 REPORT—1898. No. 140.—Potsdam. 2.43.29 P.M. No. 141.—Shide, Oct. 20, 1897. LN ne “i Litebhhmoene——— 8.54.21 P.M. No. 156.—Shide, Dec. 28, 1897. 8.24.39 P.M. — Hee No. 156.—Toronto. 11.40.48 a. No. 157.—Shide, Dec. 29, 1897. 11.32.20 am. fh No. 157.—Toronto, V. On Certain Characteristics of Earthquake Motion. 1. The Character of Earth Waves near to their Origin. From the feelings of those who reside in earthquake districts, and more definitely from seismograms, we have learned that the movements of the ground constituting an earthquake of moderate intensity, which in an epifocal area may shake badly constructed chimneys and loosen tiles upon a roof, as observed at distances of approximately 20 or 100 miles from its origin, consist of preliminary vibrations, a shock or shocks separated by more or less irregular waves, and a series of concluding vibrations. At distances of from 100 to 200 or 300 miles the pre- liminary vibrations may not be felt, or even recorded, on an ordinary seismograph, and instead of a shock or shocks we obtain a record of a series of long-period but irregularly recurring waves. These movements a ON SEISMOLOGICAL INVESTIGATION. 219 give rise to a sensation not unlike that felt upon a floating stage rising and falling upon a swell. The movement of hanging pictures and that of seismographs indicate that an intermittent tilting is taking place. The heavy masses of metal in bracket seismographs, conical pendulums, and other instruments, no longer act as steady points, but swing fitfully with varying amplitudes from side to side, and, rather than giving records of horizontal displacement, they are roughly recording the maximum slopes of the earth waves which tilt the supporting piers. Beyond the 300-mile limit nothing is felt, and it is seldom that an ordinary seismograph, writing with frictional indices, gives a record. Now and then, where the friction of writing pointers has been exceedingly low, records of unfelt earthquakes have been obtained from ordinary seismographs. It was the magnitude of these diagrams obtained by the writer, coupled with numerous observations made by astronomers on the movement of the bubbles in levels, the tilting of water in ponds, and kindred observations, which enabled him, in 1883, to venture the opinion that with suitable instruments the movement of all large earth- quakes might be recorded in any portion of the world (see ‘ Harthquakes and other Earth Movements,’ Int. Sci. Series, pp. 226 and 342). The ample manner in which this has been confirmed is known to all seismo- logists. Preliminary Tremors.—The period of these, as recorded on seismo- graphs with frictional indices, has varied between } and ;}, of a second. Along paths of from 1 to 4 geographical degrees (111 to 444 kms.) the velocity is apparently about 2 kms. per second. This, however, is the velocity of the larger waves, which the preliminary tremors most certainly outrace. Strange to say, we know less about the difference in rate of _ propagation of these small movements and their larger followers over short ranges than we do over long ranges. As a working hypothesis, founded on the interval of time that elapses between the screaming of pheasants and the arrival of sensible motion and the records of seismo- grams, I anticipate that this interval will be found to be about 10 seconds for about every 100 kms. of travel ; that is, if a shock originates at a dis- tance of, say, 200 kmns., these preliminary tremors may be noticed 20 seconds before the arrival of pronounced motion. If this is so, then the velocity of propagation for preliminary tremors over short ranges will be about 2-5 kms. per second. If, for the time being, we accept this factor, then if J is the length of a wave, ¢ its period, and v its velocity, because l=vt with a period of 51, second, the length of a wave is about 125 km. (410 feet). Their amplitudes, as shown on seismograms, are exceedingly small, say >> mm. Large Waves.—The large waves have periods of from 1 to 2-5 seconds, which, with velocities of 2 kms. per second, would indicate lengths of 2 to 5 kms. (6,560 to 16,400 feet). The maximum amplitudes of these, which represent shocks which will shatter ill-constructed chimneys, lie between 20 and 70 mm. Concluding Vibrations. —Seismograms clearly show waves having periods of from 3 to 5 seconds, the lengths of which may therefore reach as much as 10 kms. (32,800 feet). 220 REPORT—1898. Figures like the above, representing the length of seismic waves, although especially for the large waves we can rely upon the data for velocity and period, must yet be accepted with great caution. For the earthquake of October 28, 1891, as recorded in Tokio, it would appear that seismographs were tilted through an angle of about one-third of a degree, whilst the actual height of the waves was about 10mm. If these measurements, referred to symmetrically, formed wave-surfaces, the con- clusion is that the lengths of the waves did not exceed 20 or 40 feet ; the difference between which and, say, 1,600 feet is so great that all confidence in the determination of wave-lengths is apparently destroyed within an epifocal area, or, to be more precise, within five or six miles of an origin. Where waves can be seen rolling down a street, we are here at least cer- tain that the distance from crest to crest-of an earth-wave is measured by 10 or 20 feet rather than by hundreds or thousands of feet. 2. On the Velocity of Propagation of Large Waves. From the table on p. 221, where we find the length of arc along which motion may have travelled, the velocity of the preliminary tremors along sach a path and the duration of their movements, which is the interval of time by which they outraced the succeeding large waves, it is easy to calculate the velocity with which these waves were propagated. The results of such calculations, together with results obtained from somewhat different data by von Rebeur-Paschwitz and Dr. A. Cancani, are given in the following table :— Velocities of Large Waves in Km. per sec. Von Rebeur Cancani Are Along are Along chord along chord along chord ° 20 271 271 1 to 2°5 2°5 60 28 27 — 27 80 2-9 27 3 to 3°5 = 110 33 2°8 -— 31 | 3. On the Character of Earth-waves after having travelled Great Distances. The following remarks are based on records of earthquakes obtained at distances from their origin so great that movement of the ground could not be felt, whilst ordinary seismographs failed to indicate any movement of the piers on which they rested. Many of them, for example, refer to seismo- grams obtained in Europe or England of earthquakes which originated at places so far distant as Japan. Preliminary Tremors. Velocity.—In the Report for 1897 (p. 173) a table is given of the highest apparent velocities with which the preliminary tremors of about seventy disturbances have been propagated over or across arcs of great circles on the earth’s surface. These arcs have varied in length from about 2° to 156°. The observations on arcs of from 2° to 18° and from 70° to 85° have been fairly numerous. For arcs of intermediate length the observations were only three or four, but inasmuch as these take up ON SEISMOLOGICAL INVESTIGATION. vp A | their proper position on a curve of velocities, it may be assumed that they are the result of fairly accurate observations. This also applies to the two or three records on wave paths exceeding the 85° limit. In the original diagram (‘ Report’ for 1897, p. 174) those observations which by reference to orginal records are found untrustworthy are surrounded by circles. The general results arrived at are easily remembered. If it is assumed that motion is propagated rownd the earth, then the velocities over arcs of 20°, 30°, 40° up to about 100°, which have lengths of 2,200, 3,300, 4,000, and 11,100 kilometres, are about 2, 3, 4, and 11 kilometres per second. Along wave paths less than 20° the velocity of 2 kilometres per second remains constant. For arcs greater than 100° the velocity apparently increases at a rate somewhat less than the rate at which the length of the arc increases. With the hypothesis that the vibrations travel along paths approxi- mating to chords through the earth, then the above velocities must be reduced. The actual velocities obtained as mean values from a number of observations are given in columns 9 and 10 of the following table :— Table showing the Relationship between the Apparent Velocities with which Preliminary Tremors are propagated round or through the Earth, and dimen- sions of the same, Sc. The first fou Velocities are derived from Observations. The last two are inferred." Diff. in < 4 Length | Length re Asa,.| Velocity Velocity De- Length} Max. |Average A Aver- c grees ee oF Cota of Are |Depth of| Depth of Bees age of Le / of eae Deration of oni Radius | 204_ | Chord | Chord Ch f\Depth yl] REE lad | BR etsy fen ects Are a acus= | Chord |in Kms.|in Kms. oe Ghord.||, BE" See: RETIRES.) ao Tes ° Kms. 6,360 Kms. Tana on Are onChord 20° 2220 2208 12 97 67 97 818 2°75 2°75 0 to 4 60° 6660 6360 300 | 853 608 29:20 | 24°6 6 57 20 80° 8880 8175 707 1487 1053 38°8 324 82 75 30 to 34 110° | 12210 10419 1791 2712 1977 52 44-4 11 9:3 41 to 43 140° | 15540 11952 3588 4197 3149 64:8 56 13°8 ? 9-9 unknowa 180° | 19980 12720 7260 6360 5097 79°6 71 17-4? M11 ey It will be observed that the quantities given in the eighth column are approximately four times those in the ninth column. In questions relating to the direction taken by a wave in passing through the earth, it must be remembered that this may not necessarily be along a chord, but in consequence of refraction follow a path that is curved, Apparent Duration of Preliminary Tremors. The following table gives the time intervals by which preliminary tremors have outraced the longer period and larger waves constituting the main portion of various earthquake disturbances. Beneath these time records, inclosed in brackets, the distances of the various observing stations from epifocal areas are given in geographical degrees or kilo. metres :— 1 See British A'sociation Report, 1897, p. 174. 222 | REPORT—1898. Apparent Duration of Preliminary Tremors. (m=minutes ; s=seconds.) bo 7 * H © a © = Ey 2 ad g | 3 2/13 B58) ¢ | 2 | A:fosoledgeae 1 ae ca) ‘Ss 2 3 he og 2 5 4 a so] Be BZ ag 2 a 2) ue hee eaal se) S| 3) Bee eae 5 | re) wm Wie We oe fe Bio oe le ey epee a |e Oct. 27. 48m.| 40m.| __ al eF eats ~~ = sactingo }|{ 1804 (1042) (204°) Z Nov. 2, ™. | o4m 35 4 23 = #2 = ak = =e = Mexico } { 1894 }(102°) : fg Merida, { Apr. 28, is =. | 1 = ms ons ie ‘< iy pew Venezila t Fane 1b i 27m. | 30m.| 32m.| 29m une po) pe: -| 32m. Shree me A = es a { 1H50 oo hone (86°) | (84°) | (88°) |(88) | Japan Oct. 18, 18m. am wre 2 is uns = 86° — _ a momo} /{ 192" Pct) | — Gio } { Nov. 4, ay Fi ee. pie 23 antl ae — | (eeey = == a is en AS 13m. | 34m. | 34m Oct. 31,f 14m.{ __ an Seeiesarm. | o> * | 20m. m. m. n. > see Myles iauee (71°) (86°) ade ie Men baa | if ee Japan, } { Apr. 17. Ts ahs or “= =a = = — — a (80°) (81°) enn Mar 16 24m. Fant ar. 16, A hee we ze =. = me =, = as ae =e Philippines | { 1892 | (78°) Luzon } { ” 7625) Fo i | ema (amma Mi da) ea Neo May 11) 33m. feb, s ls af ae — © )27m: of ws = Pad n pea "TED } { 1892 (719-2) } { oy. eo Wiis) eel ge) Resin pa ae || ei eae —. , Ares —-|>-|j- ” 1892 4 (71°) - Jan. 18, ee “= #2 23 ae = és = mn — — = » } { 1895 || 73™ ies } { Dec. 20) __ i uf nak = Be bi — | ase) = =% ss Quetta 1899 ol SoG! OEP pink. OLE ier a AM UR SD fh 8) NEY ie } { 1893 (45°°7) Asia Minor, } { Apr.16f ae =i = = Gries) = pes a = = =e = Amed,. f epi € On. *, —- —_— — — _ _ ° le re ob as ea, (ee pee a te, ; (15°) May 23. = a or a 2 = a es _ = a Thebes } { 1t08 Om. | — ott E: = Bucharest } { Ose Ma = = ae — ry 7 an fea Ge) } { Jan. 25 = is 2s ae == = = — (9°) = _— — — Naples 1893 ‘ Mount Aug. 10 mes 2} | ese ee a } | 1853 = = a (9°) June 29) 12m.) 4m. | _ | _ | 4m. | 6m. Lite mes -{/—};—}]—] = Cyprus 1896 | (12°) | (17°) (18°) | (19°) | (gy | (5°) care 7m. | 14m.| 5m. m. rg bie Iceland j { Aug: 26) im. | Wm | — | — | 10m] — (30°) (33°) (21°) | (16°) Hei 1896 Gs ) at a ke ee Sept.21, moi 2. ype * a3} po ise as le at 1896 | 7™ | (209) (21°) eA fat Feb. 19, = rior 26m.| — 21m. or = — =— llm.| — Japan | 1897 10m. | 20m. Sh Junel2 Pk = = = — — |8m.?)10m.?} — — a Assam — { ore | ee a Aug.4,[ __ pins wtb ta &, als ee oie ey be, Japan| 1897 ° 40m. & Sept.20. Ree ce. Uae 2 Age Nee N. Borneo } { 1807 a) rip | ane Dec. 29. ae 2 et <4 = _ — — | 4%. | — — oa Hayti } \ 1897 | — | | (64°) ee ee ee ON SEISMOLOGICAL INVESTIGATION. 223 Apparent Duration of Preliminary Tremors. ee eeeeeeeeeeeeee—eeeEeyeeye————————eEeEeEEEEe bo 28 Ea el tess 5 2 a fs ie =F nO ¢| 2 | 8s co — Ss a n Z 23 e\/2/2|#8|gel2|/3|2| 2/2 |e8| 2 |e8 S Ovi pos seed Mh ares ead} vamp |S poe of BY Persian Gulf, | Kishim, Jan. 7 _ _ _ — | 13m. |} 15m.?} 13m — _ — 2. | 2 1897" q mbria, Jan. 4 ze, 2h ee = = = ae oe | 19, 1897 j oe TA a Sicily, Calabria, | Feb. 11-12, Brie OIG Sanne REE OPEN core eo 2a eee. SAS ea hob eieitls Ly ary 1897 / | | ‘Romana, Apr. ‘s Ei Lap) os it is é& pel | pen en == fe 3, 1897, a | os Romana, Apr. Se Si ll a= el ealiGeal: -47 ie ale 3, 1897 ‘ae ital oat These time intervals and their corresponding distances are shown graphically in the following figure, in which the free curve indicates the general result towards which the observations point :— Fia. 4. ‘ 4 ] ; , Min 180 ——«*160 140 72 Intervals by which Preliminary Tremors have outraced Long-period Waves. 224 REPORT—1898. Inasmuch as these records have been obtained from different types of instruments which have had different degrees of sensibility, it is clear that they cannot be regarded as individually comparable ; but when plotted on squared paper and taken in groups, it is evident that these time intervals increase with the length or depth of the wave-path over or at which a disturbance has travelled. In a few instances, as for example in the case of disturbances originating near Japan, Borneo, and Hayti, which have been recorded by the same or similar instruments in the Isle of Wight and Toronto, such observations are comparable, and they take up expected positions on the average curve of duration drawn through the groups of observations which are not so strictly comparable. The expectation from this is that this curve will, by future observa- tions, be found to be approximately correct. An inspection of the same shows that the preliminary tremors up to distances of 12° or 15° only outrace the succeeding waves by intervals seldom reaching a minute. On paths between 20° and 85° the intervals are proportional to the length of the arc, but beyond this range it seems that they may increase at a somewhat higher rate. Between Europe and Japan, or a distance of 85°, observations have shown that the interval by which the larger waves are outraced varies from 30 to 34 minutes. If we take 32 minutes as an average, then it is easy to compare what should be expected, and what has been observed on ranges lying between 20° and about 100°. This is done in the following table :— . Japan to Shide, 85° Observation, 32 minutes. Borneo to Shide, 112°, 42 min. expected. 3, 40 to 43 i Hayti to Shide, 62°, 23 ,, 3 i 20 x Hayti to Toronto, 20°, 7 ,, > », about 4 55 Although these observations indicate a working rule, enabling us to determine the distance of an origin from an observing station which, with a knowledge of the surface configuration of our globe and localities where seismic activity is frequent often, are the means of locating an epicentre, the last of the series suggests that the duration of the preliminary tremors are more directly connected with the depth of a wave-path rather than its length, as represented by the arc of a great circle. Trial, however, shows that the duration of preliminary tremors is not proportional to the length of the chord along which it may be supposed the movements travelled, or to its maximum or average depth. The table on p. 221, which is derived from fig. 4, shows that the dura- tion of preliminary tremors in minutes is, for the given ranges, nearly equal to the square root of the average depth of the chord expressed in kilometres. On the Period of Earthquake Waves at Great Distances from their Origin. All that we know about the period of earthquake waves after they have travelled great distances is derived from the open diagrams of the Italian workers, a few records obtained in the Isle of Wight, and a single but exceedingly valuable record obtained by Dr. F. Omori when in Pots- dam. ‘The Italian and Isle of Wight records were obtained from simple or horizontal pendulums writing on smoked paper. The Potsdam record, which refers to an earthquake originating in Japan on February 19, 1897, ON SEISMOLOGICAL INVESTIGATION. 225 is photographic, and shows the movements of a pair of von Rebeur pen- dulums. It has yet to be described. In the following few examples of records referring to period the fol- lowing abbreviations are used :— Pt. = Preliminary tremors, the periods of which are expressed in seconds, Lw. = Large waves, 33 = sy Pe Pp. =Simple pendulum, the length of which is given in metres, ‘These pendulums have multiplying indices. H.P. = Horizontal pendulums. G.L. = Geodynamic level (see p. 263, also ‘ B.A. Report,’ 1896, p. 227). The first name refers to the place at which a given earthquake originated. 1895. Jan.18. Japon. At Rome P. 16m. gave for Lw. 164s. , July 8. Caspian Sea. ,, Ischia G.L. Sem ayth cdot YOR Aug. 9. E. Italy. , Rome P.16m. ,, ,, ,, 88s. and Pt. ‘46s. ,», Rocca di Papa P. 7m. gave for Lw. 7s. ,, Padua P. gave for Lw. 40s. ,, Ischia H.P. (with a natural period of 11s ) gave Pt. 6s. to 12s., and Lw. 20s. to 50s. », Catania gave Pt. 3s., Lw. 15:5s. ,, Rome P. 8m. gave 21s., P. 16m. 14s. to 20s. ,, Ischia H.P. gave Pts. 4s., Lw. 10s. ,, Rocca di Papa P. gave Pt. 4s., Lw. 6s. 1896. June 15. Japan. 1896. June 29. Cyprus. a Aug. 26. Iceland. , Rome P. 16m. gave Lw. 10s., P. 8m. gave Lw. 10s. ,, Rocca di Papa P. 15m. gave Lw. 14s., P. 7m. gave Lw. 14s. ,, Ischia H.P. gave Lw. 18s. ,, Ischia H.P. gave Lw. 60s. down to 13s. ,, Rocca di Papa H.P. Lw. 30s. to I4s., ?. m gave Lw. 14s., P. 15m. 30s. and 14s. ,, Rome P. 16m. 8s. to 13s. ,», Catania P. Lw. 48s. to 72s., Pt. 14s. to 28s. », Rome P. 16m. gave 11'5s. ,», Catania Lw. 15s. to 18s.; also 8s. to 16s. ,», Rocea di Papa P. 15m. gave I4s., H.P. gave 16s., P. 7m. gave 16s, ,, Ischia H.P, 2 2s. to 17s. », Ischia H.P. gave Pt. 2°5s., Lw. 19s. ,», Rocca di Papa H.P. gave about 17s. » Rocca di Papa H.P. gave 18s. ,, Ischia H.P. 6s. to 25s. » Padua P. gave 35s. to 16s., Ischia H.P. gave 25s. to 12s. ,, Catania P. 25m. gave 6s. to 18s. - June 12. N.E. India. », Shide H.P. gave 15s. “3 Aug. 31. Japan. As Sept. 6. Iceland. * Sept. 22. Tiflis. ef Nov. 1. Tashkent. 1897. Jan. 10. Persian Gulf. When reading the above records it must be remembered that they refer to the shortest and longest periods which were observed, or to waves with the smallest and largest amplitudes. Near to an origin, after a shock, a disturbance dies out with an increasing period, but at a great distance from an origin the maximum movements which: probably corre- spond to a shock or shocks are those which have the longest period. Also the fact must not be overlooked that the records refer to seismo- grams obtained from different instruments, located at different stations, and that it is not certain that comparisons are made between similar sages motion. The following table is therefore tentative, and when C Q 226 REPORT—1898. we are in possession of records more strictly comparable it may be sub- ject to considerable alteration :— ‘ oie Period in Seconds Distance from Origin in Degrees Preliminary Tremors Large Waves 0 to 3 ‘05 to °2 1 to 4 8 to 10 42 av 23 to 28 2:2 19 35 to 40 62 ab 85 3 to 8 20 to 60 All that this table tells us is that both preliminary tremors and large waves exhibit a marked increase in period as they travel, and, whatever the period of a given wave may be in the vicinity of its origin when it has travelled a distance represented by a quarter of the circumference of the earth, its period has increased twentyfold. VI. On Certain Disturbances in the Records of Magnetometers and the Occurrence of Earthquakes. By Joun Mitne. Although we are aware that the records from certain magnetic obser- vatories rarely, and then only slightly, show that the magnetographs have been disturbed at or about the time of large earthquakes, it is certain that at other observatories these movements of the ground are accompanied and possibly preceded by perturbations as shown upon magnetograms of a very marked character. In some instances these disturbances have evidently resulted from the mechanical shaking to which the magnetic needles have been subjected, but there are other cases where such an explanation is not so clear. To determine how far these movements may be attributed to mechani- cal action, whether there is any reason to suppose that certain of them may be the result of magnetic influences, to explain the observation that what are apparently similar earthquakes with like origins are accompanied by different results at the same observatory, and generally with the object of throwing additional light upon a class of phenomena which at present are not well understood, I have collected the materials contained in the following notes. In addition to sending the list of ‘ Earthquakes recorded at Shide, 1897-98’ (see p. 191), to various earthquake observatories, the same was forwarded to magnetic observatories at the following places : Kew, Stony- hurst, Greenwich, Falmouth, Potsdam, and Bombay. Accompanying the list there was a request that the same might be returned with notes respecting any magnetometer perturbations which might have been noted at about the times of the earthquakes which were more pro- nounced. Some time later I drew up a second list of earthquakes which had been recorded in Italy, Germany, and England, the greater number of which had originated at great distances from these countries, and appended to the same a request similar to that attached to the Shide list. On April 5 this was forwarded to magnetic observatories at the following places :— Pawlowsk (Odessa), Kasan and Tiflis, (Russia), Irkutsk (Siberia), Prague, Vienna, and Pola (Austria), O-Gyalla (Hungary), Utrecht (Holland), Nice and Perpignan (France), Copenhagen (Denmark), Madrid ON SEISMOLOGICAL INVESTIGATION. 227 (Spain), Coimbra (Portugal), Kew, Greenwich, and Stonyhurst (England), Zi-ka-wei and Hong Kong (China), Manila (Philippine Islands), Batavia (Java), Mauritius, Melbourne (Australia), Loanda (West Africa), Havana (Cuba), Toronto (Canada), Washington (United States), Bombay (India), Tokio (Japan). Earthquakes recorded in Germany, Italy, and England, many of which originated at great distances from these Countries. The time employed is Greenwich Mean Time. Magnetometer Disturbances | 8 ae n | eg | al No.| Date Hour Origin : 3 3 s . & E Eg g 2 | g re MiS/S181/0/ 8/2 Sele] 8] S18 D|a|> AGE tT sigin isi | s) ea |= | o| H. M Peaks} 1889. Hy Medd 1 | Apr. 18} 5 21 a | Japan : —)|— || 2 | July 11) 10 22 p} Quetta. = he == S| 3} , 28| 3 30 p | Japan ‘ -— | Bali. | 6 Op : : | a) 5 | Aug. 25| 7 37 p| Greece. . |— | — —| 1891. | | 6 | Oct.27} 938 p| Japan. . _ ea; Brea 1892 7 | Mar. 16} 122 p| Manila. . —|—j|—! 8 mo” 5 22 Pp 0 je Ale 9 | Apr. 19} 11 30 a | California . = 10 | May 12} 5 43 a] Japan . .|—|— — pak 11 | Oct. 19} 4 21a *s Sy hee =) 12|Nov. 4} 5 24p fe as Gee i Si 13 » 27) 5 57 p | California. = Sy waDec. 9) 1194 | Japan .. — =5 15| ,, 20| 0 34a | Quetta. | Bi 1893. 16 | Jan. 28} 11 46 p| Italy . .|—|-- = ai pent!) 419 a) Zante ... = Mepeens 2) 0O39a; 4, i. | Panes) 5° 7 p| Japan t . Be ey | 20 ” ” 7 4 p ” a7 ae mh 21 » 9] 613 p| Turkey. . |— —|— == —| 22 wees, 9 40 p| Japan . . — = Es 23 ale. Op . aw at 24 ” 13 5 0 p Quetta etd —— hes 25) ; 16) 5174] Japan. . Aaa es 26 7” 0 4 p ” —— Z| Setewectigisn | ,, 4 = 28 ” oo» 2 18 p ” . — 29 » 22} 1116p 3 4 MI 30 | Mar. 2} 11 6 p/ Turkey. =| =| = oe =F 31 » 14) 6 20a| Italy . = a || 5 201 610p | Zante: | 33 » 23} 843 p| Japan . . = = = 34 | Apr. 8/ 151 p/|S.W. Ger- many —|— |— |— eid us 35 » “LT 5 48 a | Zante rs Ect bas 36 » 23) 1 32 p | Italy — 37 » 29| 6 2p Fs Hh 228 REPORT—1898. EARTHQUAKES RECORDED IN GERMANY, ITALY, AND ENGLAND—continued. Magnetometer Disturbances | Peli ; FL No.| Date Hour Origin Mf a | Sp at le KH flee 2 Z -s ‘al olo/a\/sicle/S/Sel Sie] ala MSE /S | S| ole 8) 61 Sle | 3 Po is) ele 38 |May 2] 9 58a . al 39 » 18] 2 39 p Hf ee 40 ey AIG) Sale Sto oe wo: — 4 41 > 28] ouoe) Pp |sGreece.) —-|-— | — _ _ 42 |June 3| 4 25 p| Unknown . — |! = —| | ASS ie) aie eLO CLO’ pal Italy fee. | 44 Pn Mle goed) p 2 oer pet by le |i 45 » 13) 11 5a 3 : 46 » 14] 6 47 a | Greece . 47.| July 3/10 5a PS RE 48 » 5| 11 24 a | Italy 49 » 10} 014p 5 50 /Aug. 2} 1 43a 5 aS pla erent As| 0 (ber, FG = 52 ee (16) +7 42) p s att Lee) She 6:10) Oo Dipel We. a 54 ae) f 489 5 (== on 1894. 55 | Mar. 22| 10 37 a | Japan . . | —| — = == = |— 56 | Apr. 20| 5 42 p| Greece. . | || 57 » 27] 7 55 p rfotiheccy v8 == | — js 58] ,, 29| 3 25 a| Venezuela. ee 59 | June20| 5 45 a) Japan . . = 60 | July 10| 10 30 a | Constanti- | nople . |—}—)|— | = 61 by eal) ee alae on es os = | 62 | Oct. 7| 11 40a/ Japan. . a 63]. 4,) 2219" Oa si gy 2 Ved | eu | vale 64| ,, 27| 9 8 p| Argentina. | —|— ——- 1895. | ) 65 | Jan. 18} 237 p| Japan . . te SS 66 | July 8} 10 43 p | Caspian Sea he et) ;—|— |} —|— | — | 67 | Aug. 9! 5 38 p/| E.Italy . as 2.1/2 ae 68 | Nov. 13) 9 31 p | W.Asia Mi- | NOLS euaes is ba 1896. } 69 | June15| 11 46 a | Japan . . |-—|— — he hes 70 | ,,. 29] 9 2p} Cyprus. . | a ess 71 | Aug. 26} 11 22 p | Iceland. . = i — 72 5 ol) 8 23a | Japan . . <8) Gu = Pal 73 |Sept. 6) O 2a/| Iceland. . _ { (eae Ke 74 » 14/10 30a/N.W. Asia { Minor La 75 » 22) 4 53 a | Tiflis SES obs Canes 76| Nov. 1| 5 18a) Tashkent . rea 4) -2= be 1897 | | ) Jan. 10} 9 18 p | PersianGulf au =f) June 12| 11 29 a | N.E. India. | —|— ) — = = aie Aug. 5| 0 22a) Japan. . = | Sept.20) 7 24 p | E. Borneo. | | —) » 21) 628 Bt GO as ey <% Dec. 28| 8 54p|W.Indies.; | | | | ) » 29} 11 404 | . | = | | | t | | ON SEISMOLOGICAL INVESTIGATION. 229 The chief feature in this list is that with one exception it refers to earthquakes of which we know the origin. The exception is No. 42, and it is here included because it refers to an earthquake which probably dis- turbed the whole of the globe, and had a duration greater than any yet recorded. In Japan I recorded it as having a duration of 5 hrs. 24 mins. In Strassburg it continued 11 or 12 hours. In the columns for magnetometer disturbances, especially for Kew and Mauritius, it must not be inferred that the marks necessarily indicate any- thing more than that slight magnetic perturbations have occurred at about the times specified. The Potsdam, Wilhelmshaven, and Pawlowsk records date from 1895. Farther information has been obtained from the earthquake catalogues published from time to time by Professor Pietro Tacchini in the ‘ Bollettino della Societa Sismologica Italiana.’ These records date only from 1895, and refer to Utrecht, Potsdam, Wilhelmshaven, and Pawlowsk. What has been gathered from these lists, together with that from replies to circulars, more of which may yet be expected, is tabulated in a uniform manner in the following lists :— , 0, as, for example, ‘ Potsdam = 0,’ means that the magnetographs at Potsdam were not disturbed. D means Declinometer or the unifilar record. H means Horizontal Force record. V means the Vertical Force, or Lloyd’s balance record. The times are given in hours and minutes G.M.T. Replies relating to the List on p. 191. (Zarthquakes recorded at Shide, Isle of Wight, 1897-98.) 1. Records from the Kew Observatory, Richmond, Surrey. Superintendent, Dr, CHARLES CHREE, J/.R.S. Dr. Charles Chree, F.R.S., superintendent of the above observatory, tells me that he and Mr. Baker have looked at the curves, chiefly for horizontal force, at the times of the large movements in the Shide list, and he points out that near these times—as near any other set of arbitrary times—there are movements of the ordinary magnetic small wave type. Such movements go on for hours, if not for days; and by some the view is held that they are always, or nearly always, existent, and might be seen if we had only delicate enough instruments and an open time scale. When earth movements have affected the trace there is a ‘burr,’ but such a ‘burr’ might be equally well caused by an assistant entering the room with keys or a knife in his pocket. In only one case—No. 104, June 3— was there evidence of a movement not due to natural magnetic causes, excepting one on October 20, No. 141, which might more naturally be assigned to human creation. The June 3 movement would pass for an earthquake, but it took place at an hour when there are frequent move- ments in the building, as absolute meteorological observations are taken then. Traces free from small movements, excepting the vertical force, are rare. On a moderately disturbed day the movements are in dozens, or rather hundreds. In the following list the numbers refer to those on the Shide list, and if these are followed by =0 this means that at the corre- sponding dates the magnetometers were not disturbed: 98=0. 104. At 230 REPORT—1898. 119=0. 10 a.m. a slight movement, apparently not magnetic. 116=0. 131=0. 132=0. 133 probably =0. 134=0. 140=0. 141. At 2.58 P.M. movements probably due to an assistant. 145=0. 157=0. 163. A slight movement, about 2.50 p.m., of a doubtful kind. Records from the Royal Observatory, Greenwich. Through the kindness of the Astronomer Koyal, the following note relating to the Shide register, p. 191, were drawn up by Mr. Nash :— Shide No. Movements noted at Greenwich. Sistine » Small movement in H and D at 23h. 30m. JOR Mats . 51 * Ae about 12h. 20m, 100. : a3 < , at 13h. 15m. OT Sie . Very small movements in H and D. LOZ a s5 ; Aa 5 ‘ D. LOS. Aas Small movements in H and D at 4h. 45m. # 104*" . Small wave in H and D at 9h. 50m. NOS Fs . Very small movement in D at 11h. 45m. TUG. . Small =n in D at 19h. 55m. ORE re 3 5 wave in H and D at 7h. 30m. 10s. : i movement in H at 10h. 55m. TNO =A 5 5 wave in H at 20h. 15m. TL . * movement in H at 14h, 15m. 1 ie . Very small fluctuations in H and D. GRE 2 : es » movement in D at 15h. 10m. 118* ” i “A in D and H, Gh. 10m. to 6h, 45m. 120 ay * P in H and D at 21h. 45m. 122 es » wave in D. 123 Small decrease in H and D at 15h. 10m. 125* “ +» wave in H and D at lh. 20m. 130 . Very small movement in H about 19h. 28m. 131 « Small movement in H. 132% . » wave in H and D at 28h. 50m. 134 > movement in H and D at 13h. 40m. + 136 .- Wave in H and Dat Oh. 15m. L3Ts Small movement in H at 14h. 40m. 142 3 os in H and D 3h. 30m. 143 + Wave in D. 144 4 + movement in H at 9h. 48m. 147* Active movements in Hand D, commencing a 4h. 155 Small a in H and D. 156 . Very small ,, in D. 160 . Small 3 in H, again in D & H, 17h. 40m. to17h. 45m. We have here 33 instances where it is possible that a connection may exist between earthquake movements and the movements of magnetic needles. In the cases marked with an asterisk the movements of the needles preceded those of the ground. ee lee SES ULC ON SEISMOLOGICAL INVESTIGATION. 231 Replies relating to the List on p. 227. — Magnetometer Movements noted at the Kew Observatory, Richmond, Surrey, England. Superintendent, Dr. Cuartes Carne, F.2.S, ma ns Month! D Time of | M Distunh No. 5 oh : ont ay Earthquake | agnetometer Disturbances 1889. | H. M. 1 fete) STN 18 5 21 A.M. | D and H no trace of earthquake. The previous two days were very quiet except for some small movements on the 17th—1 to 3 P.M. and 5 to 7 P.M. 2 5 | VIE-| (25 7 37P.M. | On D some very small, apparently ordinary, magnetic movements about 7.37. On H small movements—all say on 25th—the largest between 4 and 6 P.M., but no trace of earth- quake. The 24th distinctly quiet, but for slow moderate movements of D about 10 P.M. 1892. 3 10 We 12 5 43 a.m. | D trifling movements, but they look magnetic. H shows no trace of earthquake. On the 11th very quiet. H shows lots of small movements, the largest (not big) shortly before midnight. 4 11 X. 19 4 21am. | D and H no earthquake movement. Noon 17th and 10 p.m. on 19th many varied movements. The fastest large change of H on the 18th about 5 and 8 P.M. Sharp change of D on 18th between 5 and 5.30 P.M. 5 12 XI 4 5 24p.M.|/D many small movements, but no certain earthquake. No trace of earthquake on H. Many small dis- turbances on the 4th up to 4.30 P.M. ; pretty sudden commencement on the 4th about 2.29 A.M. 19 A.M. | Dand H no trace of earthquake. On the 8th many smallish movements from 8 A.M. to 11 P.M. Largest on D about noon. 6 14 | XII. i) i893. 1 II. 9 6 13 p.m. | Certain small movements might be earthquake effect, but there are several not dissimilar at no great time interval. The 9th, but for many small vibratory movements, w2s quiet. The 8th was generally quiet. A small slow movement of H at 10.40 to 1].20 P.M. 11 6p.m. | No trace of earthquake on D. Some movements but apparently magnetic, on H. ‘The 2nd was generally quiet. On the 1st two well-marked move- ments last 7.20 to 8.30 P.M. 9 ol Il. 14 6 20 a.m. | No trace cf earthquake on D and H. 13th and 14th, on the whole, quiet ; on 13th some slow waves cn H between 1.45 and 8 PM., alsoon D about 12.30 to 2 P.M. and about 6 P.M. 3 te 8 30 III. to REPORT—1898. MAGNETOMETER MOVEMENTS—continued. List |Month| Day make | Magnetometer Disturbances == ——! 11 H. M. Soils ame 1 51 P.M. | No trace of earthquake of E or H. D a little irregular, but nothing special, at 151. The 8th and 7th generally quiet, but many small vibrations on D on 7th and early on the 8th. 42 VI. 3 4 25 P.M. | Some slight movements, apparently magnetic. The 3rd and 2nd gene- | rally quiet. A few small movements | on D on the 2nd and early on the 3rd. 45 VI. 13 11 5 A.M. | No trace of earthquake on H or D. On the 12th H shows a slight hump from 0 to 1 A.M., otherwise very quiet; D shows a lot of very small movements, a noticeably sharp one about 6.15 A.M., and a hump on curve from midnight to 1 A.M. Magnetometer Movements noted at the Royal Observatory, Greenwich y from | 1889 to 1896. Drawn up by Mr. P. H. CowEtt. [For a more detailed description see the Greenwich volumes. | No. on < 3 Time of Beginning of Magnetometer ae et ees oe Earthquake = Distnrban eos 1889. H. M. 1 1 IV. 18 5 21 A.M. | Very small, from 17d. 9h, A.M. to 6h. P.M. 2 2 VII. 11 10 22 P.M. | 2h. P.M. 3 Bes VALI || 25 7 37 P.M. | From noon. 1891. Tesolin oe | O9sS PM lien. Ab. Abmerps Me 1892. 5 if III. 16 1 22pm. | From 15d. 8h. P.M. to 16d. 3b. A.M. 6 10 IV. 12 5 43 A.M. | Smalldisturbance from 11d.11h.30m.P.M. q 11 X. 19 4 21 A.M. | Storm from 17d. noon. 8 12 XI. 4 5 24 p.m. Ps » 4d. 2h. A.M. 9 13 = 27 5 57 P.M. | From 26d. 2h. 30m. A.M. to 5h. A.M. 10 14 XII 9 119A... | Disturbance from 8d. 2h. A.M. to mid- night. a7, ) eae eleanor. || Rrom 19d. 10,30. P20. 1893. 12 16 I. 28 11 46 p.m. | From Oh. 30m, A.M. 13 ik - 31 | 419 A.M. » 1h, 30m. a.m. 14 19 If. 6 5 7 P.M. || Storm from 4d. noon to 6d. noon, Sub- 15 20 as ss 7 4PM. sequently a large disturbance. 16 21 4 9 613 p.m. | From 9d. 6h, P.M. 17 22 8 Al 9 40 P.M. 18 23 “f 1l OPM. | 19 26 Pre Mites JUS 5 17 A.M. Considerable disturbance from 165d. 20 26 ast alee 0 4PM | lh. P.M. ON SEISMOLOGICAL INVESTIGATION. bo ee) vo MAGNETOMETER MOVEMENTS—continued. No. on : oe : Time of Beginning of Magnetometer eee | Month! | Day Earthquake ~~ Disturbances p. 227 H. M. 27 3 21 7 13 A.M. | Disturbancefrom 20d. 5h. P.M. tol0h. P.M. 28 “e n 2 18 P.M. . », 21d. noon. 29 = 22 11 16pm. | Slight ,, » 22d. noon — princi- pally at 8 P.M. 30 IIL. 2 lit 6PM. From 10h. 30m. P.M. 31 x 14 6 20 A.M. 7rols AGM: 33 os 23 8 43 p.M. | Very small disturbance from 6h. P.M. 34 IV. 8 1 51 P.M. 53 ms - 7 lh. to 10h. A.M. 35 17 5 48 a.m. | Disturbances from 16d. 3h. P.M. Small disturbance 17d. 4h. A.M. 38 V. 2 9 58 AM. | A small, sharp disturbance 1d. 10h. P.M. 39 ie 18 2 39 P.M. Disturbance at noon. 40 Py 19 13. A.M. |; Small at 18d. 8h. P.M., and a smaller at 19d. lh. A.M. 41 5 23 8 38 p.m. | At 6h. P.M. 42 VI. 3 4 25p.M. | Register interrupted for Visitation Day. 43 a3 ai 10 10 p.m. | A great disturbance 6d. 9h. P.M. Fluc- tuations subsequently. 44 Es 11 9 9Pp.M. | Disturbance from 10d. 7h. P.M. Aon AV LL. 3 | 10 54m. | Very small disturbancesince 2d. 11h. A.M. 51 | VIII 4 0 52 A.M. | From 3d. 7h. P.M. 52 of 6 7 42 P.M. | Storm beginning 6d. 4h. A.M. 53 5 10 9 9P.M. | From 3h. P.M. 54 a4 14 7 48 p.m. | Very small disturbance 5h, 30m. P.M. 1894. 55 III. 22 10 37 A.M. | Storm commences 21d. noon. 56 IV. 20 5 42 p.m. | Fluctuations from 5h. A.M. 57 5 27 7 55 P.M. | Slight irregularity at 3h. A.M. 58 3 29 3 25 A.M. | From 1h. A.M. 59 VI. 20 5 45 A.M. | Moderate disturbance for some time past. Wave at 4h. A.M. 60 VII. 10 10 30 A.M. | From 9d. 8h. P.M. 62 X. 7 | 11 40 a.m. » 6h. AM, 63 sy 22 9 OAM. » Oh, A.M. 64 i 27 9 8PM. yi) DHAES MM 1895. 65 1 18 2 37 P.M. | From 17d. noon. 66 VIl. 8 | 10 43 P.M. » 6h. A.M. and 1h, P.M. 67 | VIII 9 5 38 P.M. » Sh. AM. 68 XI. 13 9 31 P.M. » «th. PM. 1896. 69 VI. 15 11 46 A.M. | From 14d. 2h. Am. to 15d. 3h. A.M. Sharp waves 14d. 3h. 30m. to 6h. P.M. 70 7 29 9 2PM. | From 3h. P.M. to midnight. Waves 6h, 30m. to 9h. 30m. P.M. “TL. je VLbE 26 11 22 p.m. | Almost continuous from 23d. 2h. P.M. to 25d. 9h. P.M. 72 3 31 8 23 a.m. | From 29d. noon to 30d. noon. Marked at 29d. 4h. P.M. (i IX. 6 0 24M. | From 4d. noonto5d.10h. p.m. Marked on 5d. 8h. 30m. to 10h. A.M. 234. REPORT—1898. It will be observed that these records, unlike those in the next register for Utrecht, do not refer to ‘burr’-like markings produced at the time of earthquakes, but to magnetic movements which have had a considerable duration, and which commenced some hours before the occurrence of the earthquakes to which they are in juxtaposition. For fourteen earthquakes it will be noticed that there is no corre- sponding magnetic disturbance, but, singularly enough, at least ten of these earthquakes were small, originating, for example, in Italy, the mechanical movements accompanying which were not recordable even at so short a distance as England. Apparently, therefore, the greater number of perturbations recorded at Greenwich have only preceded very large earthquakes representing internal adjustments of the earth’s crust. Something analogous to this will be found in the Zikawei register, p. 245. Magnetometer Disturbances recorded at the Royal Meteorological Institute of the Netherlands, Utrecht. Director, Dr. M. SNELLEN. N Bot Monti | D: nee: Magnetometer Disturb | oO. Ip. 227 | on 7 ay Earthquake Magnetometer Disturbances 1689. H. M. 1 Se al Vel eal: | 10 22 p.m. | D 10h. 42m. max. at 10h. 50m.,and llh. lm. H 10h. 39m., with max. at 10h. 41m., 10h. 52m., 11h. 2m.,and 13h. 20m. 1so9l. 2a lo X. 27 9 38 P.M. | D 9h. Om. 8s.; 9h. 28m.; 9h. 44m. 50s. ; | 10h. 2m.; 10h. 8m.; 10h. 32m. H.=0. 1892. 11 30 A.M. | D and H 11h. 33m. 5 43 a.m. | D and H 7h. 14m.? 13893. . 5 16 1 28 11 46 P.M. | D 9h. 24m.; 10h. Om.; llh. 2m. H 9h. 26m.; 10h. Om. 6 26 Il. 16 0 4pm. | D 10b. 46m.; 11h. 34m.; 11h. 56m. H 10h. 48m.; 11h. 24m.; 12h 4m. Tf 30 Ill. 2 11 6PM. | D1lh.56m. H 11h. 56m. 8 33 23 8 43 p.m. | D 8h. 54m. H not registering 9 34 TV. 8 1 51pm. | D lh. 42m.; th. 56m. H ih. 40m.; lh. 57m. 10 36 23 1 32pm. | D2h.40m. H 2h. 40m. 11 38 Ve 2 9 58 Am. | D 9h. 51m.; 9h. 58m. H 9h. 51m.; 9h. 58m. 12 40 — 19 1 SAM | Dih.19m. H= 0. 13 41 23 8 38 P.M. | D7h.36m. H 8h. 20m. p if 43 aM. | Aug. 1, D 11h. 20m. p.m, ; 11h. 36m. P.M. H 11h. 36m. P.M. 1894. 15 55 Ill. 22 10 37 A.M. | D 10h. 27m.; 19h. 26m., &c. H 10h. 27m.; 1jh. 21m., &c. 16 57 Ve 27 7 55 P.M. | D 7h. 57m. H 7h. 57m. 17 59 Not registering 18 60 | VII. | 10 10 30 a.m. | D 10h. 28m. H 10h. lm.; 10h. 32m. 19 63 X. 22 9 OAM. | D7h. 51m. H 9h. Om. 20 64 — 27 9 8pm. | D 9h. 0m.; H 9h. 8m. ON SEISMOLOGICAL INVESTIGATION. 235 MAGNETOMETER DISTURBANCES—continued. No. on | | Tj f No. | List |Month| Day E bene oe Magnetometer Disturbances p. 227 | | arthquake | 1895. Ziee|P66, | Ville jens 10 43 p.m. | D10h.27m. H 10h, 26m. 1896. 22 69 Vi. 145; jl 46 a.m. |] D 11h. 23m. H 11h. 26m. 23 vel VIII. 26 11 22 p.m. | D1lh. 30m. H 11h. 28m. 24 73 IX, 6 0 2am. | D12h. 7m. H 12h. 8m. 25 76 XI. 1 5 18 D 5h. 31m. H 5h. 23m. 4897. 26 78 VE; 12 11 29 aM. | Dilh. 18m.; 11h. 58m. H 11h. 56m. (See records from Bombay.) 27 rN pg 8 5 0 22am. | Di1h.4m. H Oh. 59m. 28 $l IX, 21 5 28am. | D6h. 24m. H 6h. 20m. To the above is added 1896, August 27, D, 10h. 54m., H, 10h. 55m., which agrees with an earthquake recorded in Europe, as, for example, at Catania at 10.52. Out of the Utrecht records there are apparently thirteen instances, viz., Nos. 2, 5, 9, 11, 13, 14, 15, 18, 19, 20, 21, 22, and 26, in which the magnetometer perturbations have preceded the records of the seismographs by intervals varying between a few minutes and two hours. The disturbances due to earthquakes are usually easily distinguished from ordinary magnetic disturbances and from those produced artificially, as for example by the approach and removal of masses of iron. A copy of these disturbances was forwarded to Dr. Charles Chree, who very kindly compared the same with his own records obtained at Kew. The results were as follows :— No. 2. Nothing special at the times specified. For several days about this date innumerable small movements occurred from time to time. . D, a little movement about 11.25, but not at times stated. H, small movement at 10, but various similar movements both before and after. » 9. D, no movement at 1.42, 1.51, or 1.56. H, asmall movement at 1.57. » ll. D, nothing at the time stated. H, nothing at 9.51 or 9.58. », 13. D, numerous very small tremors for some hours before and after time stated. H, nothing at 8.20. » 14. D, nothing at 11.20 or 11.34, or 1.34 A.M. on the 2nd. H, nothing at 11.36 P.M. on the Ist. » Lb. a disturbed this and previous day. Hundreds of movements. », 18. D, nothing at 10.28 specially. Very small tremors 10.25 to 11.30. H, nothing at 10.1; burr on curve at 10.35. » 19. D, microscopic tremors about 7.48 and later. H, nothing at 9.0. », 20. D, considerable magnetic movement 6 to 10 p.M. Nothing special at 9pm. H, ditto. 21. D, nothing at 10.27 or 10.43. H, nothing at 10.36 or 10.43. » 22. D, nothing at 11.23 or 11.46 a.m. H, lot of tiny tremors 10 A.M. to 1 P.M. ; nothing special at 11.26. » 26. D, nothing at 11.18, 11.29, or 58 ; but at 11.38 somewhat abnormal jerk, and small movement at 11.50. H, nothing at 11.29. Movement that might well be an earthquake from 11.47 to 12.10. This is certainly not a normal magnetic movement. or ” Referring to the Utrecht times given for the above thirteen cases, Dr. Chree says that in some cases there was in progress either a moderately 236 REPORT—1898. developed magnetic storm, or a series of vibrations such as are every now and then conspicuous for some time—hours or days. At such times fifty or a hundred tiny wobbles may be observed within a comparatively small time, and it would be almost impossible, in fact, not to have one within a minute or so of any specified time. Magnetic Disturbances recorded at Det Danske Meteorologiske Institut, Copenhagen. Director, Dr. ADAM PAULSEN. | No. on| Time of No. | ae lies Day Earthquake Magnetic Disturbances 1893. H, M. 1 30 Ill. 2 11 OPM. | Very weak traces inH F at1lh.3m.P.M. 2 34 DV; 8 1 51 P.M. | Shocks in D and H at 2h. 3m. to | 2h. 13m. P.M. 1894. SN bey f 1% 27 | 755 P.M. | Disturbances by details not received (J. M.) 4 60 | VIL. 10 10 30 A.M. | Commenced 10h. 36m. A.M. At 10h. 39m. severe shock, succeeded by ¢ several shocks until 10h. 52m. A.M. 5 61 VII. 12 2 17 P.M. | Between 2h. 15m. and 2h. 21m. P.M. 1895. 6-))|_ 66)- ||: Valde 8 | 10 43 Pm. | Between 10h. 47m. P.M. and 11h. 12m P.M. Severe shocks particularly in HE. 1896. XI. ; 1 | 5 18 A.M. | Traces of earthquakes between 5h. 22m. | | | and 5h. 28m. 1897. 8 | 78 | Vie | ao | 11 29 A.M. | Severe shocks between 11h. 18m. and 1lh. 57m. A.M. Magnetometer Disturbances recorded at the K. K. Anstalt fiir Meteorologie und Erdmagnetismus, Wien, Oesterreich. Director, Dr. J. M. PERNTER. = | = He; os | Time of ye No. | <<" Month) Day Earthquake Magnetometer Disturbances Pa | 1893. H. M. 1 34 IV. 8 1 51 p.m. | Apparently strong movement 2 42 VI. 3 4 25 P.M. | Strong swinging ia) 0 52) WELL. 6 7 42 P.M. | Much disturbed 1896. 4 | 69 | VI. | 2 | 11 46 A.M. | On the 16th much disturbed ON SEISMOLOGICAL INVESTIGATION. 257 To the above is added the disturbance caused by the Laibach earth- quake, April 14, 1895, at 10.18 a.m. The origin of No. 1 was South-west Germany ; that of No. 2, which is one of the largest and longest earthquakes yet recorded, is unknown ; No. 52 was in Italy ; while 69 was in Japan. : The magnetographs are but rarely disturbed, and then, with one exception, only by local shocks. Magnetometer Disturbances recorded at the K. und K. Hydrographisches Amt. Pola. Tae Drrecror. No. on | Time of No. ae ak | Day Earthquake Magnetometer Disturbances 1893. H. M. 1 10 IL. 1 0 39 A.M. | 10h. 45m. P.M. (?) 2 21 — 9 613 P.M. | 3h. 35m. P.M. and 5h. 5m. p.m. 3 54 | VIII.| 14 7 48 P.M. | 4h. 37m. P.M. 1894. 4 55 | IIL. 22 10 37 A.M. | 10h. A.M. 5 61 | VII. 12 217 P.M. | 1h. 10m. P.M. 1895. 6 65 I. 18 2 37 P.M. | 55m. P.M. 7 67 | VIII. 9 | 5 38 P.M. | 1h. 5m. P.M. 1897. 8 77 I. 10 918 P.M. | 8h. 35m. P.M. 9 | 18 | IX. 21 5 28 A.M. | lh. 10m. P.M. To the above is added a magnetometer disturbance, April 14, 1895, 10 hrs. 22 mins. p.M., which probably corresponds to an earthquake /el¢ and recorded throughout many parts of Italy, April 14, at 10 hrs. 18 mins. (in Rome). The origin of this was near Laibach, in Austria. For the earthquakes recorded but aot felt in Europe, the Pola dis- turbances, with one exception, are from one to four hours in advance of the seismograph records. Meteorological Office, Toronto, Canada. Director, Professor R: F. Stuparr. Professor Stupart writes me that he has compared the list of earth- quakes with the magnetometer traces prior to their disturbance by the electric trams, and does not find upon them any irregularities at the specified times. Magnetometer Disturbances recorded at Bombay Government Observatory. N. A. F. Moos, Director. In the list on p. 238 the earthquakes referred to are those which were recorded in Europe. Several of these had submarine origins the positions of which are unknown (see List, p. 227). The peculiarity of the movements of the magnets, the fact that they are disturbed hy movements which are not perceptible, that the same movements originated at great distances, and that in some instances they REPORT—1898. 238 “ fi « ; F0000- £0000- fT eer eee OOUOT “UISIIQ “WV “Ugg “Tg ‘oywndyQawa ‘Tg “ydog “poyavur yo“ 10000. 20000. H ‘N'Y GF G [gtoqmaydag - F0000- £0000: If “ 68 I ps ae | , “Treulg | 0000. £0000- iH ‘Wd OF O 5 sf 5 ‘Soy g “UOWVANp f *IKV “UI “Tg *T ToQTMOAONT OSTV “ISTE ON UO “KY “IOs "YO 09 “Wa ‘Ur OS “UIT ‘OE 10q0990 "TLeUIg | eQQ00. ¢0000- H i AT IL TE 19q0390 ‘smmoy] Z “uoBINp sIK'V “WIEg "YR ‘oYENbYRIVO ‘Te ysnSuy “Teg | 90000. £0000. GtH | {agy ETE! 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Fic. 6. en POT No. 2, July 12, 1889, SE No. 3, Aug. 7, 1889. Y . 12, June 8, 1891. —aaa No. 13, May 16, 1892, a No, 15, Jan. 11, 1893. —— No. 18, Nov. 5, 1893. No. 34, Sept. 21, 1897. SE Usual type. Sketches of Magnetometer Disturbances recorded at Bombay. N. A. F. Moos. : Fig. 7. Bombay, June 12, 1897. Disturbance of Declination Needle. Multiplication, 2i times. N. A. F. Moos. . In the Bombay Magnetic and Meteorological Observations Mr. Moos 24.0 REPORT—1898. describes in some detail the disturbances he noted in connection with the Assam earthquake of June 12, 1897. Dines’ Pressure Tube Anemometer Chart did not show any trace of atmospheric disturbance. The barograph trace was, however, disturbed, the maximum effect being about 1 min. later than the maximum disturb- ances in the declination and vertical force magnetograms. These instru- ments are of the Kew pattern. The needle of the declinometer has a period of 5:33 seconds, and the disturbance it suffered is here shown enlarged about 2} times. The time of vibration of the needle of the horizontal force magnetograph, which shows an equally large disturbance, is 8 seconds. The disturbance in the vertical force magnetograph, which is also pronounced, continued over three minutes. There are fourteen fairly regular waves in 29 mins.; that is, the magnet which, if mechani- cally disturbed and allowed to return to rest, would do so in double swings of 5-33 secs. came to rest with periodic movements, each of which had a duration of two minutes. In Europe the earth-waves from the earthquake had periods of from 10 to 15 secs., and it is likely that when they passed Bombay their periods would be about five seconds. It is difficult to understand how a movement of this description would result in the displacements recorded; and, as Mr. Moos points out, it is equally difficult to see why earth-waves could mechanically cause a change in the scale reading of this type of instrument. His conclusion is that the seismic convulsion was in some way the cause of a magnetic action, every seismic wave having its companion effect in a magnetic wave. ‘ The following is a summary of disturbances of magnetic needles at various observatories by the shock of June 12, 1897 (see Earthquake No. 105, p. 204) :—Time at origin, about 11 hrs. 4 mins. a.m.; arrival of pre- liminary tremors in Europe, about 11 hrs. 17 mins.; arrival of large waves in Europe, about 11 hrs. 47 mins. Place D H V Remarks H. M. H. M. / eer NG) He Ma) a Bombay . | 11 14-11 16 11 11-11 14 11 14-11 19 | Ist Shock 11 17-11 43 max. |; 11 45 End 11 19-11 23 | 2nd Shock Batavia . | 11 £2 JJ 23,11 34, 11 29 max. 4 Shocks for H 11 37,11 54 | Utrecht . | 11 17-11 19 max. | 11 45-12 20 | Dhas two max. 11 45-12 3 |}. 12: 3b=31"'30 | of 1O&15mm., which for H are 10&7 mm. Wilhelms- | 11 19-11 2h (ecibiher fe ik 319) 11 26-11 59 haven | 11 44-12 0 | Pawlowsk | ei fy | Max. of H at | | J1 19-11 42 | | Tihy22mi ParaSaint | 11 27 Pati 7 | Small Maur | Kew . | Small& doubtful Copen- hagen | Disturbed Magnetographs at Lyons, Perpignan, Pola, Vienna, Uccle, and Lisbon were not disturbed. The barograph disturbance at Bombay was at 11 hrs. 14 mins. to 11 hrs. 21 mins., with max. at 11 hrs. 13 mins. ; the electrometer dis- turbance at Batavia was at 11 hrs. 16 mins. (exact). aa ON SEISMOLOGICAL INVESTIGATION. 241 Magnetometer Disturbances recorded at the Royal Alfred Observatory, Mauritius. Disturbances are indicated as: s=small; vs=very small; a=abrupt ; va=very abrupt ; sa=small abrupt. Director, T. F. Craxton, Esq. No. on . No. list |Month| Day Mi acckb Magnetic Disturbances p. 227 1889 ul i IV. 18 5 21 A.M. | H 7h. 35m. A.M.-8h. 10m. vs, 9h. 45m.— 10h. Om, vs, 11h. 10m.—13h. 10m. 2 2 VII. 11 10 22 p.m. | H 3h. 40m. P.M.—4h. 40m. vs, 5h. 30m.— 6h. s, 7m. vs. V 3h. 40m.—6h. 10m. vs 3 3 VII 28 { 3 30 P.M.) | H 5h, 50m, P.M.—th. 30m. vs, 7h. 10m.— 6 OP.M.)| 9h. 10m. vs, 10h. 10m. to 2 A.M. on 29th, vs 4 5 | VIII 25 7 37 P.M. | H 3h. 40m. P.M.—5h. 20m. vs, 5h. 50m.— 6h. 40m., 7h. 37m.—Yh. 10m. vs. V 4h. 10m.—8h. 10m. vs 1891 5 6 X. 27 9 38 P.M. | H 4h. 40m. P.M.—d5h. 40m., 7h. 30m.— | | | 8h.10m.s. D 4h. 46m. vs—7h. 35m. vs | 1892 6 |7&8) III. 16 |; 122PpmM.)| H 15d. 8h. 40m. pP.M—9h. 20m. V (5 22 pM.) 9h. 10m.—9h. 20m. a 7 11 X. 19 421 A.M. | H7h.0m. A.M.-7h. 40m. vs. D 4h.10m.— 5h. 40m. vs. V 4h, 40m.—5h. 10m., 7h. Om.—7h. 40m. vs 8 12 XI. 4 56 24 P.M. | H 2h. 28m. A.M.—5h. 40m. vs. D, like H, also on the 5th. V, like H, also on the 5th, sa 9 14 | XII 9 119 AM. | H 8d. 8h. 10m. A.M. and 11h. 10m.- 5h. 10m. p.m. s. D like H, but vs. V 8h. 10m.-1h. 10m. P.m. 1893 10 16 I. 28 11 46 P.M. | H 7h. 25m. p.m.-1lh. 10m. vs, 29d. 9h. 10m. a. V 7h. 38m. p.M.-7h. 43m., 8h. 10m.—8h. 20m. 11 19 II 6 5 7 P.M. | H 1h. 10m. P.mM.-7d. 9h. 10m. A.M. vs 12 21 — 9 6 13 P.M. | H 6h. 10m. P.M —7h. 10m. vs, a wave 13 22 —- 9 940Pp.M. | H 10h. 10m. P.M.—10h. 40m. vs, 10d. Oh. 10m. A.M. vs, 1h. 40m. vs. D 10d. 4h. 10m. a—5h. 10m. vs lf | 24 —_ 13 5 Op.M. | H 4h. 10m. P.m.-5h. 10m. vs. D 11h. 50m. A.M. -12h. Om. vs 16 | 25 — 16 5 17 AM. | D 15d. 4h. 10m. A.M. s_S8h. 40m. vs, 9d. 40m. P.M.-1lh. 40m. vs, 16d. Jhr. 10m. A.m.-5h. 10m. s. V 15d. | 9h. 40m. P.M.-10h. 40. H, a small magnetic disturbance, february 14-18 | 16 30 Ill. 2 ll 6AM. | H 11h. Om. P.M.—Oh. 10m. A.M. shallow wave 17 31 — 14 6 20 A.M. | H 5h. 50m. A.M.-1h. 11m. P.M. Ey 85433 —_— 23 8 43 P.M. | H 5h. 40m. P.M. s 19 34 Vis 8 1 51 P.M. | H 5h. 10m. A.M.-11h. 10m. s. D like | H but faint 20 35 — 17 5 48 a.m. | D 4h. 40m. A.M. vs J 1898. REPORT—1898. MAGNETOMETER DISTURBANCES RECORDED AT THE ROYAL ALFRED OBSERVATORY, MAURITIUS—continued. No. on | , list |Month| Day oe ot 3 Magnetic Disturbances p. 227 | q 37 | 29 | 6 2pm. | H 6h. 40m. P.M. vs ool Se 18 2 39P.M. | H 9h. 40m. A.M. s-lh. 10m. P.M. vs, 2h. 40m.—3h. 25m. s. D 1h. 10m. P.m.— | | 4h. 10m. P.M. vs 41; — 23 8 38 p.m. | H 10h. 25m. P.M.-llh. 10m. s wave. j D same as H, but vs wave 42 | VI 3 | 425 p.m. | H 2d. 10h. 10m. p.m.—3d. Oh. 10m. A.M. vs, Oh. 40m. A.M.-2h. 10m. vs 44 — 11 | 9 9PM. | H 8h. 10m. P.M.-10h. 10m.s wave. D same as H, but vs wave 52 | VIII.| 6 | 7 42pm. | H 4h. 45m. A.M., 7b. 40m.—8h. 10m. va, | | and movements until 4h. 1lm. P.M. D like H, but not abrupt | 1894 55 | Ill. | 22 | 10 87 A.M. | H small movements all day. Active | | from 8h. 10m. A.M.—9h. 10h., but vs. | | D same as H 58 | IV. | 299 | 3254.m. | H 28d. 4h. 10m. p.M.-5h. 10m. P.M. s, : 29d. 8h. 10m. A.M—lOh. 10m. A.M., 11h. 10m.-Oh. 10m. P.M. vs, Oh. 30m. | j P.M.-2h. 10m. vs, 6h. 50m. 8h. 10m. | D 29d. 8h. 10m. A.M.—10h. 10m. vs, | 6h. 50m. P.M._8h. 10m. vs. V_ occa- | sional small movements, 29d. 8h. 10m. A.M.—3h. 10m. P.M. 59. |. VI. 20 | 5 45 AM. | H19d.4h.10m. P.M. sa, 21d. 1h. Om. A.M. | D 20d. 4h. 10m. A.M.—8h. 10m. s. | / V 20d. 7h, 40m. A.M. vs 62 | IX. | 7 | 11 404M. | H 11h. 40m, vs 64 | — | 27 | 9 SPM. | H 8h. 15m. p.M.-11h. 40m.s wave. D ' like H. V like H, but vs 1895 65 , I. j 18 ) 237 P.M. | H 9h. 10m. Am.—Jh. 25m. P.M, vs | } | / tremors, 4h. 10m. P.M.—6h. 10m. P.M. | / | | wave, 8h. 10m. p.M.—9h. 10m. P.M. | D 2h. 10m. A.M.—4h. 10m. A.M. vs, V | 8h. 10m. P.M.-9h. 10m. P.M. s wave 66 | VIl.; 8S | 10 43 pM. | H 9d. 4h. 10m. A.M.--7h. 40m., 9h. 10m.— . | | 4h, 10m. P.M., 5h. 10m. P.M.-7h. 25m., 8h. 25m.-10h. 25m. vs tremors | H 5h. 10m. p.m.—7h. 10m. vs, 9h. 25m. / / P.M.-Oh. 25m. A.M. vs 68 | XI. 13 | 9 31pm. | H 7h. 40m. p.M.-8h. 40m. P.M. wave, ) 10h. 10m. to midnight occasional s tremors. D 7h. 40m. P.M.—8h. 40m. . | P.M.s wave. V like D or a) oro) Li} 1896 ]1 46 A.M. | H 7h. 40m. A.M.—10h. 10m. P.M.,a small | disturbance. D and V like H | 9 2PM. | H 12h. 19m. P.M.-30d. Ih. 10m, A.M., | slight movements 42 OLE de 1 | 8 23 AM. | V 29d.11h.10m. P.M.-20d. 0h. 10m. A.M., / 8h. 10m. A.M.-9h. 10m. A.M. 75 IX. | 22 | 4 53 a.m. | V 4h. 10m. 4.M.—5h. 10m. vs —_ ON SEISMOLOGICAL INVESTIGATION. 243 MAGNETOMETER DISTURBANCES RECORDED AT THE ROYAL ALFRED OBSERVATORY, MAURITIUS—continued. No. on : No. | List | Month} Day Harthquak * Magnetic Disturbances p. 227 1897 40 LIC I, 10 918 P.M. | H 4h. 40m. P.M. va, small distance after until midnight. V like H 41 78 VI. 12 | 11 294.M. | H 2h. 10m. P.M. a 42 80 IX. 20 7 24p.M. | D th. 10m. A.M.-5h. 10m. vs 43 | 81 IX. 21 | 5 284M. | H 5h. 40m. A.M—10h. 10m. vs 44 83 | XII. | 29 | 11 40 A.M. | H small disturbance all day, sharp at 4h. 15m. P.M.-4h. 35m _ V like H, only very small An examination of the above table, for which I am indebted to Mr. T. F. Claxton, the Director of the Royal Alfred Observatory, shows the following results :— Cases in which magnetic needles have been disturbed at intervals varying between a few minutes and 30 hours before an earthquake, 32. Cases in which magnetic needles have been disturbed at intervals varying between a few minutes and 6 hours after an earthquake, 11. Case in which the disturbances of magnetic needles have accompanied an earthquake, 1. Observations at the Magnetic and Meteorological Observatory, Batavia. By Dr. J. P. vaN DER STOK. June 12, 1897 (Assam Earthquake) (see Earthquake No. 105), G.M.T. BH. MAS, Horizontal Force, first shock 5 c . : 11 23 40 AM. + » second ,, S : : - 11 34 40 3 awe third ©, : 11 37 40 » last Po ‘ ; . : 6 11 54 40 Declination, mid. of motion . : 3 A P ° 22 £0 Vertical Force, maximum 3 11 29 40 Electrometer (Mascart), exact commencement . ll 16 40 September 20, 1897 (see Earthquake No. 1383). H MM. S&S. Horizontal Force . 5 . 5 cl : 7 16 20 P.M. very small. ‘Electrometer . 6 x : > 5 : 7 14 20 large. The declinometer and balance were not disturbed. September 21, 1897 (see Earthquake No. 134). H: MM. Bet Meng 18 He aM." si Horizontal Force , ° e 5 19 20AmM.5 24 20 5 25 20 5 30 20 535 20 5 39 20and 5 42 20 Declination at . 3 5 . 5 26 20 4.mM. slight. Vertical Force . < . 5 5 23 20 (maximum). Duration 20 mins. 5 Electrometer . 21 20 A.M. (commencement). The distance from Batavia to the origin of these last two disturbances is 1,500 kms. The last of them also “disturbed magnetometers in the Mauritius, Bombay, Pola, and Utrecht. R2 244 REPORT—1898. Fig. 8. ee ee Bifilar, Sept 20. Eqke. 133, aI ‘ A a . Electrometer, Sept. 21. Eqke. 134. Electrometer, Sept. 20, Eqke. 133. : > Bifilar, June 12, Eqke. 105. — eee Bifilar, Sept. 21. Eqke. 134. Vertical Force, June 12. Eqke. 105. Magnetometer and Electrometer disturbances. Batavia, 1897. Magnetometer Disturbances noted at the Magnetisch en Meteorologisch Observatorium, Batavia. Month} Day Hour | Magnetometer Disturbances | | | No. on | No. List p. 227 1892 H. M. 1 | 15 | XII. | 20 | 0 34 A.M. | Dec. 19, 11h. 3m. p.m. Very slight. 1893 2 | 21 | I | 9 | 6 13 P.M. | Gh. 19m. p.m. Pretty distinct. 1895 8 BB: ie le 18 2 37 P.M. | 2h. 14m. p.m. Faint (?). 4 66 | VIL. 8 10 43 p.M. | 4h, 5m, p.m. to 4h. 11m, P.M, Clear(?). MAGNETOMETER DISTURBANCES NOTED AT BATAVIA—continued. ON SEISMOLOGICAL INVESTIGATION. 245 No. on | No. | List |Month| Day Hour Magnetometer Disturbances p. 227 1896 5 “| VIDE: |: 26 11 22 p.m. | 2h. 45m. p.m. and 2h. 49m. P.M. 6 76 XI. 1 5 18 A.M. | Nov.2,11h. 58m, AM. to 0h, 8m. P.M, (2) | 1897 7 ee) aac 12 11 29 A.M. | 11h. 25m, A.M. to 11h, 50m. A.M. Strong.} 8 80 IX. 20 7 24p.M. | 7h.17m. P.M.to7h.33m. P.M. Notstrong. 9 81 IX. 21 5 28 A.M. | 5h. 24m, A.M, to 5h. 45m, A.M. Strong. | _ Magnetometer Disturbances noted at the Observatory, Zikawei, China. nore oe 15 16 No. on List |Month| Day Hour Magnetometer Disturbances | p. 227 | ee | 1889 | H. M. 1 Vi: 18 5 21 A.M. | 2h. 54m. and 4h. 24m. Small serrations. 4 (LUE ets} 6 Op.m. | 4h. 49m. to lh, 54m, Small notched movements. 1891 6 X. 27 9 38 P.M. | 9h.39m, A remarkable mechanical dis- | | | turbance. See ‘La Nature,’ 1892, No. 975, p. 149. 1892 if II. 16 | 1 22 p.m. | 1h. 54m. to 5h. 54m. Slight agitation. 1l Xx. 19 9 41 A.M. | Perturbations the day before and after. On the 4th, perturbations from 2h. 9m, A.M, 1893 19 IL. 6 5 7Pp.M. | 3h. 54m., trepidations, Large pertur- bations at 5h. 27m. 24 II. 13 5 Op.M. | 4h. 14m. to 5h. 4m. Slight undulations. 25 II. 16 5 17 A.M. |, All day on the 16th and 17tha great per- turbation, but nothing exceptional at the time of the earthquake. 44 VI. 11 9 9PM. | 3h.54m. to 9h.9m. Light undulations. 53 | VIII.| 10 9 9Pp.M. | 3h.54m. to 7h. 54m. Small serrations. 1894 55 | III. 22 10 37 A.M. | Great perturbations on the 22nd and 23rd, but nothing special at the time | of the earthquake. 59 VI. 20 5 45 A.M. | Two days of remarkable perturbations, but nothing remarkable at the time of the earthquake. 62 xe a 11 40 A.M. | 9h. 54m. A.M. to 3h. 54m. P.M. Slight serrations. 64 X. 27 9 8 P.M. | 3h.54m. to 9h.54m, Marked oscillations. | 1895 65 I, 18 2 37 p.m. | 11h. 54m. to 1h. 54m. Several insigni- ficant movements. 67 | VIII. 9 5 38 p.m. | At 3h. 54m. a disturbance lasting two days began. 246 REPORT—1898. Father Chevalier, who kindly sent me the above notes, remarks that the most striking feature of the comparison appears to be that there is no relation between earthquakes and magnetic disturbances. ) = 0279 March 5 48 P.M + :0841 || July 3 20 P.M + +0690 a 1132 ,, — 0732 || ,, 936, — +1038 35 5 27 A.M + 0221 || ,, 438 AM. | + 0351 a 1elires py}, — ‘0337 : DOs S45, + 0048 April 4 31 P.M + ‘0803 || August . 4 57P.M. | + 0642 3 | 10 30 »,, — *0592 Asa Me 11 24 ,, | — :0727 aa 3 43 A.M + °0210 |) Fe 5 57 AM + ‘0738 35 eat.“ coay gilt O12 it Ps | 11 32, — ‘0612 ‘TasLE III. \ | January February, March April May June July August at aa a“ “a “i ad Noon | —0:005 | +6:009 | —0-001 | +0-011 | +0-001 | +-0:019 | —0:017 | —O-014 | 1p.m.| — -003 |— -006 | + -017 |— 002 | + O11 | + :004 | + -019 | — -012 ; 2,, |— ‘007 | —--008 ; — -013 | — 004 | — ‘O11 | — ‘008 | + 004 | + -003 1 3,, | + ‘017 }— :012 | — :006 | + :017 | — ‘008 }— ‘010 | — -021 / + ‘O11 fete, | 003) + “O13 | 000 | — 005 | + 010 | + -005 | — ‘O14 | + ‘018 fees jt 006 | + 005 | + 022) = 003 | — 019 | + 013 | — ‘005 | + -016 er) | + 003 | -01E + 013 | — 010 | — “001 | — 005 | + 006 | — “007 1 7, |— 019 | — :001 | — ‘011 000 | + °013 | — 015 | — ‘001 | — -014 ; 8, | + °010 | — -014 | — -017 | + -006 | + -005 | + -009 | + -001 | — -017 | 9,, | + 006 | + ‘001 | — :020 | + :022 | + 003 |} + *001 | — -001 | -- :019 10,, | + 005 | + -013 | + -003 | + 012 | —.-024 | + -004 | + -001 | +. -008 Te 000 | — -002 | + -007 | + -:003 | — -009 | — -010 000 | + -006 : Midnt. | — 009 | — ‘015 | — 004 | — ‘017 | — -011 | — -005 | — ‘001 | + -019 ( LAM.) + °021 | + -003 | + -002 | — ‘006 | + -008 019 “000 | — -002 | 2, |— 002 | — :002 | — ‘011 | + -602 | — -008 006 | — -009 | + -007 | 3, | + 003 | — ‘001 | — -019 | — 019 | — -006 |} — 008 | + 015 | + -005 fee; | + OOD | + O15 | + “O16 | — “014 | + 006 | + “008 | — 003 | —_-022 Po, |— 0137 — 008 | + 010 | + 001 | — 006 |— 019 ‘000 | + +005 | 6,, | + 003 | + :021 | — -003 ; — :007 | + 014 | — -013 |} — :001 | + 021 ; 7, |— 019} + -002 | ~— -001 | + *003 | + 025 | + ‘017 | + -009 | — ‘O11 mein | — “007 | — :002,| +, 00% | — 014 | — O01, | —,-014 | +7006) — 010 | 9, | + 006} + :002 | + 014 | — :016 | + :012 | + -001 | + -016 | + -013 }10,, |— :008 | + :007 | — 016 | + 022 | + -007 | — ‘001 | — -007 | — :003 | 11 ,, |— :010 | — ‘006 | — :008 | + -009 | — -002 | — ‘G05 | — -019 | + -007 The meaning of the positive sign in Table II. and elsewhere is that the spot of light has travelled towards the east. So far as Table II. shows anything, it exhibits a tendency for the first eastern elongation, that in the afternoon, to occur earlier in the day as the year advances, also that the amplitude of the afternoon excursion, whether east or west, is greater than that in the morning, and that the maximum effect occurs in T 2 276 REPORT—1898. the summer months. It would be wrong to insist too strongly even on these tendencies considering that only a part of one year has been examined, and certainly premature to suggest any physical interpretation. I hope, however, that this partial result may prove of sufficient interest to induce the Committee to sanction further inquiries of the same nature, for which I think the instrument is peculiarly well fitted. Lastly, I give in a tabular form (Table III.) the difference (C—O) between the mean monthly result at each hour of the day, derived from the photograms, and the values computed from the interpolation equation. XIV. Reports on Seismological Investigations published by the British Association. PAGE 1841. Report on Instruments to record Earthquakes in Scotland and Ireland. Drawn up by Lord GREENOCK and DAVID MILNE i 46-50 1842. Report on Registering Shocks of Earthquakes in Great Britain. By DAVID MILNE . : ; ‘ : 92-98 1843. Report on Registering Shocks of Earthquakes. WM. BUCKLAND, DAVID MILNE 5 5 - 120-127 1844. Report on Earthquake Shocks in n Scotland. DAVID MILNE : . 85-90 1847. Report on Geological Theories of Elevation and Earthquakes. WILLIAM HOPKINS, M.A., F.R.S. . j ‘ 33-92 1850. First Report on the Facts of Earthquake Phenomena. ROBERT MALLET, C.E., F.RS. : : 1-89 1851. Second Report on the Facts of Earthquake Phenomena. ROBERT MALLET, C.E., F.R.S. : . 272-320 1852. Third Report on the Facts of ‘Earthquake Phenomena. Roserr MALLET, C.E., F.R.S.. ‘ied 1854. Third Report (continued) on the Facts of Earthquake Phenomena. ROBERT MALLET, C.E.,F.RS. 1-326 1854. Report on Earthquakes and Seismometers. Col. PortLocK, 5A ee 370-372 1858. Fourth Report on the Facts of Earthquake Phenomena. Robert MALLET, C.E., F.R.S.. 1-136 1861. Experiments at Holyhead on the Transit Velocity ‘of Waves analogous to Earthquake Waves. ROBERT MALLET, C.E., F.R.S. 201-236 Reports on the Earthquake Phenomena of Japan, drawn up by John Milne, were issued, under varying titles, yearly from 1881 until 1895. In 1895 the ‘Earth Tremor’ Committee, appointed to investigate earth tremors in Great Britain, issued the last of a series of Reports dated 1893, 1894, and 1895, the Secretary being Mr. C. Davison. In 1896 Committees on the Earthquake Phenomena of Japan and Earth Tremors were united under the joint secretaryship of C. Davison and J. Milne for the purpose of carrying on seismological investigation, and have issued their First, Second, and Third Reports. The British Association has issued since 1841 about thirty-seven Reports relating to earthquakes. METEOROLOGICAL OBSERVATIONS OF BEN NEVIS. 277 Meteorological Observations of Ben Nevis.—IReport of the Committee, consisting of Lord McLaren, Professor A. Crum Brown (Secre- tary), Sir Jonny Murray, Dr. ALEXANDER BucHan, and Professor CopeLaND. (Drawn up by Dr. BucHaN.) Tur Committee was appointed, as in former years, for the purpose of co- operating with the Scottish Meteorological Society in making meteoro- logical observations at the two Ben Nevis Observatories. The hourly eye observations by night as well as by day, which are a specialty of the Ben Nevis Observatory, were made with complete regu- larity during the year 1897 by Mr. Angus Rankin, the superintendent, and his assistants. The Directors of the Observatories tender their best thanks to Messrs. T. S. Muir, A. Drysdale, M.A., B.Sc., John 8. Begg, T. G. Kay, D. Macrae Aitken, A. Aitken, George Ednie, and T. Kilgour for the invaluable help they have rendered as volunteer observers during the past year, by which the much-needed relief has been given to the members of the regular staff. In addition to this, Messrs. Muir and Drysdale have given much time and labour in discussing, under the superintendence of the Directors, the observations made in the summer months at the intermediate station, together with the observations at the two Observatories at the same time, in connection with the weather which prevailed at the time, more especially the anticyclones and the cyclones which occurred. The result, which the Directors consider to be of con- siderable value, will be referred to in a subsequent part of this report. Table I. shows for 1897 the mean monthly and extreme pressures and temperatures ; amounts of rainfall, with the number of days of rain, and the days on which the amount equalled or exceeded one inch; the hours of sunshine ; the mean percentage of cloud ; the mean velocity of the wind in miles per hour at the top of the mountain ; and the mean rainband at both Observatories. The mean barometric pressures at Fort William Observatory are reduced to 32° and sea-level, but those at the Ben Nevis Observatory only to 32°. TABLE I. “1897 Jan, | Feb. |March| April | May | June | ae | Aug. | Sept. | Oct. Nov. | Dec. | Year Mean Pressure in Inches. Ben Nevis Ob- } 25°255 | 25°285) 24889) 25°199) 25°350| 25°482) 25-463) 25-229) 25-356) 25-504) 70 a aa all servatory Fort William | 29-937] 29902] 29°453) 29°800| 29917] 29°986| 29°927| 29°657| 29885 30°057| 30°072) 29°661|29°855 Differences .] 4°682| 4°617| 4°564| 4:601| 4°567| 4504] 4°464| 4-428] 4°529| 4°553) 4:593| 4°571| 4°557 Mean Temperatures. BenNevisov-| 20 | 283 | of | 284! a3 | she | ast 48s | 381 363 | a86| of3 | ava servatory Fort William | 35:7 | 40:5 | 41-6 | 43:3 | 481 | 551 | 58:5 | 58:7 | 51:0 | 488 | 45:6 ) 396 | 47-2 Differences .| 16:7 | 14:2 | 17-1 | 17-9 | 15°83 | 149 | 134 | 15:9 | 15:9 | 125 | 12:0 | 123] 148 Extremes of Temperature, Maxima. r ° | | BenNevisOb-| 311 | 37°3 | 364 | 378} 483| 580 | 640 aire | 483 | 388:| 'sf0| aba | efo servatory | Fort William | 51:0 | 545 | 52-7 | 60-1 | 70:6 | 77-1 | 80-4 | 77:0 | 67:6 | 61-9 | 57-8 | 54:9 | 804 Differences .| 19°9 | 17:2 | 16:3 | 22°3 | 223 | 191 | 164 | 168 { 193 [| 93 | 58 | 155 | 164 278 REPORT—1898. TABLE I.—continuwed. 1897 | Jan. | Feb. |Mareh| April | May | June July Aug. | Sept. | Oct. | Nov. | Dee. | ae i Extremes of Temperature, Minima. | / : s if ° ° ° ° ° | ° ° | ° ° ° ° ° ° Ben eal 4:0 | 12°77 | 102) 11°3 | 16°9 | 24°7 | 29°0 | 33°7 | 25:0 | 17°6 | 13:0 | 17:0 40 servatory | Fort William | 243 | 25-6 | 263 | 27-2 | 308 | 40°9 | 41-1 | 43-4 | 34°8 | 288 | 26:2 21-9) 21-9 Differences .| 20°3 | 129 | 161] 15°9 | 13:9 } 16°2 | 12:1 97; 98] 2] 132] 49 | 179 Rainfall, in Inches. | Ben NevisOb- | 3:42| 16°22| 17:24] 6:55] 10°91] 8-46] 14°13 | 11°88 | 17-04 a8 17°78} 20°07 ;155°78 servatory | } Fort William | 1°67) 8:06) 8-47] 4:24 | 479) 412) 6:93 5°24) 9°75] 6°28) 6°50} 11:79) 77°84 Differences .| 1:75] 816{ $77! 2:31| 612] 4:34] 7:20 | 6°64 7:29| 5:80] 11:28 8:28 | 77°94 Number of Days 1 in. or more fell. Ben Nevis Ob- 0 5,2 oi8 0 3 2 6 2 7 4 8 7 49 servatory | MersWilbem | Ota aif beow ae) o | a [oa | Agohoak ll an healed Differences . 0 ae 2 2 5 1 3 3 7 | 4 35 Number of Days 0:01 in. 07 more fell. BenNevisOb-| 16 16 23 17 18 18 18 23 | 26 20 |! 20 23 | 238 servatory Fort William} 14 20 25 14 19 19 Ta’ "25" tees 17 20 23 234 Differences .| 2 | —4 | —2 Se pete ls —. 0 ONE 4 3 0 0 4 Mean Rainband (scale 0-8). BenNevisOb-} 1:0 | 2 2°6 21 70 hale I? 4 273) 2°4 | 27 17 2-0 2:3 21 servatory | Fort William | 2-1 | 2:8 43 3°3 31 38 ol a7 42 | 3°6 | 36 36 34 Differences ./ I'l “18 17 1:2 tet 26 b= eal li! 15 19 16 l3e] 13 Number of Howrs of Bright Sunshine. Benes Db-| 22 22 21 98 | 159 77 | 170 35 87 80 43 27 841 servatory { Fort William 40 27 59 158 200 139 | 188 | 107 | 112 94 | 38 22 | 1,184 Differences . 18 5 38 60 | 41 62 18 72 25 14 —5 | —5 343 Mean Hourly Velocity of Wind, in Miles. 4 Ben Nevis Ob-| 22 | 18 | 23 | 14 | 14 13 | 12 13 1 12 20 13 | 18 16 servatory | \ Percentage of Cloud. Ben NevisOb-| 89 88 | 95 79 71 89 72 92 87 73 82 89 84 servatory Fort William | 69 79 79 62 60 79 68 76 70 60 77 71 71 Differences .| 20 9 16 i 1l 10 4 16) 17 13 5 18 13 At Fort William the mean atmospheric pressure for the year was 29°855 inches, being 0-011 inch higher than the average of the forty years, 1856-95. The mean at the top of Ben Nevis, reduced to 32° only, was 25-298 inches, and was nearly the average of the observations made since the opening of the Observatory in December 1883. The difference for the two Observatories was thus 4°557 inches for the year, being nearly the average difference of past years. At the top of the mountain the absolute highest pressure for the year was 26:029 inches in September ; and at Fort William 30°584 inches in December. The differences from the mean monthly pressure very greatly exceeded the averages in October and November, the excesses respectively being for Fort William 0-278 inch and 0-280 inch, and at the top of Ben Nevis 0-234 inch and 0-242 inch. The evidently anticyclonic character of the ee eee eee 7 METEOROLOGICAL OBSERVATIONS OF BEN NEVIS. 279 weather of these two months is well shown by the mean temperatures of the two Observatories, thus :— Fort Ben Nevis William. Observatory. oO ° Change from September to October —2:2 +1:2 5 », October to November a —3'2 —27 i » September to November — 54 —15 On the other hand, when the weather is strongly cyclonic, the reverse holds good. Thus in March the mean pressure was 0°300 inch under the average of March, the weather being decidedly cyclonic, when the change of temperature from February to March was +1°-1 at Fort William, but —1°°8 at the top of the mountain. The following shows the deviations of the mean temperature of the months from their respective averages :— Fort To of William. Ben Nev vis. Difference. ° ° January . —3°5 Bald —0°3 February 1-4 2-4 1:0 March 15 07 —08 April —2:2 —2:1 01 May —1:9 —0°5 14 June —0'6 1:3 1:9 July 1:2 4:8 3°6 August 1-2 29 ners September —2:3 —2'8 —0°5 October . 1:2 50 38 November 3:8 56 18 December —0°3 2:3 2°6 Year 0-0 1:0 1:0 Hence, owing to the frequent occurrence of well-marked and long-con- tinued anticyclones, the mean annual temperature at the top of the mountain was relatively one degree higher than that of Fort William ; and the differences of the means of some of the months—notably of July and October—were very striking. The absolutely highest temperature for the year recorded for Fort William was 80°'4 on July 15, and at the top 64°°0 on July 16. The absolutely lowest temperature was 20°-0 at Fort William on December 23, and at the top 4°°0 on January 25. The most noticeable feature of the extreme temperatures at the top is the high extremes during October and November when the anticyclonic type of weather was predominant. In November, temperature rose on the 4th to 52°:0, being higher than that recorded in any previous November. As regards the extremes of temperature, the difference between the two maxima was greatest in April and May, when it was 22°°3, and least in October and November, when it was respectively 9°°3 and 5°°8; and the difference between the two minima greatest in January, when it was 20°°3, and least in December, when it was only 4°°9. The registration of the sunshine recorder at the top shows 813 Boies out of a possible 4,470 hours, being 118 hours more than in 1895, and 57 hours more than in 1896. This number of 813 hours is greater than any annual amount recorded since 1891, but is 157 hours fewer than in 1888, when the hours of sunshine numbered 970. The number 813 is 18 per 280 REPORT—1898. cent. of the possible sunshine. The maximum was 170 hours in July, and the minimum 21 hours in March, these being respectively the absolutely largest and the smallest numbers of hours of sunshine recorded in any previous July and March. At Fort William the number of hours for the year was 1,184, being the largest annual number recorded since 1891, when the number was 1,220 hours. The maximum was 200 hours in May, and the minimum 22 hours in December. As regards the 22 hours in December, this number is larger than that of previous Decembers since 1890. Theannual number of hours, 1,184, at Fort William is 34 per cent. of the possible sunshine there. In the subjoined Table II. there are given for each month the lowest observed hygrometric readings :— Tasie II. _— Jan. | Feb. | Mar. | April| May | June July | Aug. | Sept.} Oct. | Nov. | Dec. io} ° ° ° ° o ° ° ° °o ° Dry Bulb . | 25:7 | 26°0 | 23°9 | 29:2 | 39°38 | 47°9 | 52°77 | 51:0 | 31°3 | 48:5 | 49°6 | 28:9 Wet Bulb . - | 188 | 191 | 21-9 | 21°8 | 27-1 | 36°8 | 36°8 | 38:9 | 27°5 | 34°9 | 34°9 | 20°8 Dew-point = . |-17°8 | -16°1 99 | -41 | 10°6 | 23:3 10°3 | 26°38 | 17-4] 199 | 187 | -88 Elastic Force . - | °018 | °020 | *067 | 036 | 069 | +125 | *104 | *146 | °095 | -107 | ‘101 | ‘028 Relative Humidity 13 14 52 22 28 37 26 39 55 bl 28 18 (Sat.=100) Day of Month 2 12 5 22} 20 4 13 2 9 25 4 22 Hour of Day .__. |Midn. 7 a.m. 10a.m.17 am. 4 a.m. 3 a.m. |8 a.m. |10p.m.9 a.m. |ila.m./10a.m./3 a.m. | | Of these lowest monthly humidities, the lowest occurred in January, when the dew-point was —17°°8 ; the elastic force of vapour ‘018 inch, and relative humidity 13. Very low humidities also were recorded in February and in December. Just as happened in the previous year, no very low humidity occurred in September, the lowest relative humidity being 55. At the Ben Nevis Observatory the mean percentage of cloud was 84, which is nearly the average, the maximum being 95 in March and the minimum 70 in November ; and at Fort William the mean was 71, the maximum being 78 in November and the minimum 60 in May. The mean rainband (scale 0—8) observations at the top was 2:1 for the year, the maximum being 2°7 in September and the minimum 1-0 in January. At Fort William the mean for the year was 3°4, the maximum being 4:3 in March and the minimum 2°] in January. The mean hourly velocity of the wind at the top of Ben Nevis was 16 miles per hour, being the highest since 1891 ; the maximum velocity was 23 miles in March, and in January the number was 22 miles, The lowest velocity was 12 miles in July and again in September, this being the lowest minimum hitherto recorded in any previous year. The rainfall for the year was 154-76 inches, or fully 6 per cent. above the average. The previous large annual rainfalls exceeding the above were 197-95 inches in 1890, 17874 inches in 1891, and 165°77 inches in 1893. The largest monthly amount was 20:07 inches in December, and the smallest 3°42 inches in January, or only 22 per cent. of the average rainfall of the month. The heaviest fall on any single day was 4:52 inches on the 25th of February. At the top of the mountain rain fell on 238 days, and at Fort William on 234 days, these being respectively twenty-two days and four days under the averages. At the top the maximum number of rainy days was ee te ania METEOROLOGICAL OBSERVATIONS OF BEN NEVIS. 281 26 in September, and at Fort William twenty-four in March, and the minimum number sixteen in January and again in February at the top, and fifteen in April at Fort William. During the year the number of days on which 1 inch of rain or more fell was forty-nine at the top and fourteen at Fort William ; at the latter place an inch of rain did not fall on any day in January, April, and June. At the top this amount was exceeded on eight days of November, and _ seven days both in September and December. Auroras are reported to have been observed on the following dates :— February 26 ; March 3, 29, 30, 31; April 2, 5, 6, 23, 24, 25 ; October 1 ; December 20, 21, 22, 23, 24 ; the number being thus relatively few, the sun spots being near the minimum of the eleven-year period. St. Elmo’s Fire was seen on March 10, 24; May 13 ; December 29, 30. Zodiacal Light, not observed during the year. Thunder and lightning was reported on April 15; August 5; December 8, 29. Lightning only, July 24; August 1, 2, 4, 13. Solar Halo, March 30; April 27 ; May 27 ; August 1, 3; September 10, 11, 26 ; October 4, 20. Tunar Halo, January 13, 21; February 12; May 13; August 9, 12, 22; October 4 ; November 10, 16. As stated in our last Report, the observations at the intermediate station on Ben Nevis, at a height of 2,322 feet, were resumed in the summer months. The observations were made from July 19 to September 30, by Messrs. T.S. Muir of the Royal Hill School of Edinburgh, Alexander Drysdale, B.Sc., Dollar, and A. Aitken. By the great enthusiasm and self-denial of the observers, aided by several self-recording instruments gifted by Mr. J. Y. Buchanan, an invaluable complete series of hourly observations have been obtained. Hence, for the first time, complete series of hourly observations have been secured at heights of 42 feet, 2,322 feet, and 4,407 feet, the three places being in the same line and differing but little in horizontal distance from each other. These hourly observations from the three Observatories on Ben Nevis are really indispensable data in investigating the problems relating to the vertical gradients of the temperature, pressure, and humidity of the atmosphere and its movements. Messrs. Muir and Drysdale have undertaken, under the superinten- dence of the Directors, the laborious work of discussing these observations, and at the Meeting of the Scottish Meteorological Society, Mr. Muir sub- mitted an elaborate preliminary report. Among the important results either disclosed or indicated in the discussion may be noticed the relations which obtain between different vertical distributions of temperature and pressure on the one hand, and cyclones and anticyclones on the other, thus :—When the reduced barometer at the Ben Nevis Observatory, for a series of observations, comes out higher than that of Fort William, the accompanying disturbance of temperature takes place inthe lower half of the mountain, that is, below the intermediate station, and denotes the approach of an anticyclone. Conversely, when the reduced Ben Nevis Observatory barometer reads lower than that of Fort William, then the disturbance of temperature takes place in the upper half of the mountain, and denotes the approach of a cyclone. In the further prosecution of this line of research, it has been arranged that in the summer of 1898, in addition to the hourly observa- tions, the observers make temperature and humidity observations at 282 REPORT—1898. different heights above and below the level of the intermediate station. The observer takes with him dry and wet bulb thermometers (Assmann’s) with which the temperature and humidity are observed. Special atten- tion is given to the particular height where at the time the more rapid changes of temperature and humidity occur, which are so striking features on the slopes of Ben Nevis, of the cyclones and anticyclones as they sweep past the mountain. These observations will continue to be made for some time at short intervals, to which are added eye observa- tions, such as mist and haze as they appear or disappear ; of marked changes of wind, both direction and force ; of the heights of the clouds on the neighbouring heights and mountains, of the rainfall, &e. Mr. Omond has undertaken a discussion of the hourly observations at the three observatories, carried out in sequence from day to day, with the view of ascertaining, among other points, the times which elapse between the first appearance of the indications of a cyclone or anti- cyclone, and its actual arrival in the British Islands. Dr. Buchan has been for some time engaged in the preparation of a paper on the annual rainfall of Scotland, and its variations from year to year in different parts of the country. In carrying out this inquiry, the relation of the whole subject to the sun-spot period of eleven years is under consideration. The last four periods, commencing respectively 1855, 1866, 1877, and 1888, are alone dealt with. The result is that the mean annual variation of the rainfall of Scotland, considered as a whole, from 1855 to 1897, shows a course of variation for the eleven years period closely accordant with the variation of the sun spots. As the sun spots increase from the minimum to the maximum in the sixth year of the period, the rainfall is under the average; but as they fall from the maximum to the minimum during the next five years, the rainfall is above the average. __ The averages have been calculated for upwards of 300 stations in Great Britain, and the remarkable result has been arrived at that, for stations in the west, well open to the westerly winds from the Atlantic— and such stations are numerous—the above relation between the distribu- tion of the rainfall and the sun spots during the eleven years periods obtains without exception in the strongest marked form. An examination of the annual direction and force of the wind for the eleven years period has been made, and sorting the results into two groups, comprising respectively N.W., N., N.E., and E. winds, which may be regarded as dry winds, and 8.E., 8., S.W., and W. winds as wet or rain-bringing winds, the following is the striking result: the maximum occurrence of the dry winds is coincident with the years when sun spots are increasing to the maximum and the rainfall is under the average ; and the maximum occurrence of the wet winds is coincident with the years when sun spots are diminishing towards the minimum and the rainfall is above the average. Further, the minimum force of the wind is during the former half of the eleven years period when the sun spots are increasing, and the maxi- mum when they are falling to the minimum. In your Committee’s last report it was intimated that there is in course of construction a map for each day of each of the years over which the Ben Nevis Observations extend, on which is entered the amount of the day’s rainfall at 120 places in Scotland ; the storms of wind from the night and day observations at the Scottish Lighthouses ; hours of sun- METEOROLOGICAL OBSERVATIONS OF BEN NEVIS. 288 shine ; fog, in hours’ duration ; thunderstorms ; halos, auroras, and other phenomena. These are collated with the bi-daily weather maps of the Meteorological Council, and also with the hourly observations of the Ben Nevis Observatories. These have been designed mainly to see what light would thereby be cast on the dynamic effects produced by the con- densation and precipitation of the aqueous vapour of the atmosphere. Now, among other matters, these maps reveal the existence of two very different types of westerly winds. One type has the wind unusually strong and steady, nearly in the same direction at the top of Ben Nevis as at sea level, with the hygrometer showing a great humidity at both observatories, and continuing long and steadily humid. Under these cenditions the accompanying rains are more than ordinarily heavy, and virtually overspread all Scotland. The other type is accompanied by a wind at the top of the mountain, nearly in a direction the opposite to what obtains at sea-level at the time, with the hygrometer at one or both observatories indicating great fluctuation in the amount of vapour. Under these conditions the rains deposited do not penetrate far east- wards, and even in strictly western situations are neither very heavy nor protracted. Somewhat analogous to these westerly winds are the accompanying phenomena of easterly winds, with the notable exception that easterly winds bring with them a rainfall that seldom penetrates to any consider- able distance inland from the east coast. Now in the case of districts which are well protected by mountains in the west-south-westerly direction, but well open to the rain-bringing south- easterly winds, it happens that their curves of rainfall for the sun spot period are diametrically opposite to the rainfall curves of strictly western districts. These local climatological considerations have an important bearing on the methods to be employed in collating the spots of the sun with the varying phenomena of meteorology. The Application of Photography to the Elucidation of Meteorological Phenomena.—EHighth Report of the Committee, consisting of My. G. J. Symons (Chairman), Professor R. Mentpoua, Mr. J. Hoprxinson, Mr. H. N. Dickson, and Mr. A. W. CLAYDEN (Secre- tary). (Drawn up by the Secretary.) Tue work has been continued throughout the year whenever possible, and the number of separate observations made in the course of the last three years amounts to more than 200, about 150 of which were observa- tions of high-level clouds. It has been found that the low-level cumulus clouds very frequently fail to give any results, as the parallax due to the base line often gives two such very different pictures that no corresponding points of the cloud ean be identified. For such clouds a base line of 100 yards would be ample. With the present base line of 200 yards it is not possible to be sure of getting a reliable measurement unless the cloud is at a height of at least 2,000 feet. Some slight difficulty has been experienced in so drawing the vertical and horizontal lines as to intersect exactly in the centre of the disc given by the image of the sun, . This has been especially the case with negatives 284. REPORT—1898. which give a very dense image of the sun with a considerable amount of deposit around it. But a local reduction of the image has obviated most of the difficulty. This is effected by applying a weak reducer, in the form of a dilute mixture of hyposulphite of soda and ferricyanide of potassium. The plate is wetted, and when the gelatine is thoroughly moistened the reducer is applied with a paint brush to the parts which are too dense. The image of the sun may thus be brought down to any convenient density without risk of diminishing the value of the plate. It is not easy to effect the reduction without showing some streaks and irregular markings, but for the purpose in view these are of no importance. Few measurements have so far been possible in the winter months, not a single opportunity having presented itself during December, January, or February, and very few during November or March. The determina- tions made are, therefore, difficult to compare with those which have been made elsewhere, and of which only the mean value has been published, and it is possible that the greater average altitudes observed may be partly explained bythe absence of observations during these winter months. Great altitudes seem especially frequent in hot weather under thunder- storm conditions, in which case the clouds may frequently form at five or six different levels, reaching in some cases to such a height as 80,000 or 90,000 feet, which is three times as great as the mean given for the same type of cloud by the International Meteorological Committee in 1894. Under similar circumstances around the margins of large thunder depressions clouds of the alto-cumulus and cirro-cumulus “ty pes also reach altitudes much greater than the usually accepted means. At the same time instances are not wanting in which clouds which cannot be distinguished from those types by their appearance occupy much lower levels. Observations made in different months and at different times of day show a well marked rise of the various cloud planes in hotter weather, and an equally well marked rise during the morning and early afternoon. Both phenomena are, as we should expect, considerably varied by the changes in atmospheric pressure, the greatest altitudes having been recorded at the beginning of a barometric fall after a prolonged spell of anticyclonic conditions, while the lowest altitudes seem to accompany or follow a.series of cyclonic disturbances. There seems reason for suspecting that the high-level clouds reach greater altitudes over the West of England than at other places where observations have been taken, but the variations in the level of a particular type of cloud are so great from week to week, and sometimes even within a single day, that a very prolonged series of determinations ought to be secured before a comparison is made with the researches which have been carried on elsewhere. : The installation remains in an efficient state, little trouble having been experienced with the electrical arrangements, in spite of the long drought and consequent poor ‘ earth.’ The Secretary proposes to continue the work, and if possible to move the whole installation, which is now arranged with an east and west base line, to some neighbouring site with the line north and south, whereby observations in the early morning and late afternoon will be greatly facilitated. As he is willing to continue to bear the expense no grant is sought, but the Committee ask to be reappointed. 9% 4. iA. ON THE ACTION OF LIGHT UPON DYED COLOURS. 285 The Action of Light upon Dyed Colours.—Report of the Committee, con- sisting of Dr. T. E. THorPE (Chairman), Professor J. J. HUMMEL (Secretary), Dr. W. H. Perkin, Professor W. J. RussELL, Captain ABNEY, Professor W. Stroup, and Professor R. MELDOLA. (Drawn up by the Secretary.) Tue Report of the Committee presented this year refers to the results obtained during the year 1896-97, in which period a large number of wool and silk patterns, dyed with various natural and artificial brown and black colouring matters, were exposed to light. It is with regret that the Committee have to announce the death of James A. Hirst, Esq., in whose grounds at Adel, near Leeds, all the patterns experimented upon since 1892 have been exposed. Mr. Hirst took great interest in the work of this Committee, and the same interest is shown by his son, E. A. Hirst, Esq., who has expressed the pleasure it gives him in being able to aid in the continuation of the work. The general method of preparing the dyed patterns and the manner of exposing ; them under glass, with free access of air and moisture, were the same as already adopted in previous years. Each dyed pattern was divided into six pieces, one of which was pro- tected from the action of light, while the others were exposed for different periods of time. These ‘periods of exposure’ were made equivalent to those adopted in previous years by exposing, along with the patterns, special series of ‘standards,’ dyed with the same colouring matters as were then selected for this purpose. The standards were allowed to fade to the same extent as those which marked off the ‘fading period’ in previous years, before being renewed, or before removing a set of dyed patierns from the action of light. The patterns exposed during 1896-97 are, therefore, comparable, in respect of the amount of fading action to which they have been submitted, with the dyes already reported upon. The patterns were all put out for exposure on July 22, 1896, eppatn sets being subsequently removed on the pecans dates ‘August 2 22, September 29, November 5, 1896 ; May 22 , September 6, 1897. Of these five ‘ periods of exposure ’ thus marked off, periods 12; 3 were equivalent to each other in fading power, whereas periods 4 and 5 were each equivalent to four of the first period in this respect ; hence five patterns of each colour have been submitted respectively to an amount of fading equal to 20,7, and 11 Jee that of the first ‘fading period’ selected—viz. July 22 to August 22, 1896. The dyed and faded patterns have been entered in pattern-card books in such a manner that they can be readily compared with each other. The following tables give the general result of the exposure experi- ments made during 1896-97, the colours being divided, according to their behaviour towards light, into the following “five classes : Very fugitive, fugitive, moderately fast, fast, very fast. The initial numbers refer to the order of the patterns in the pattern- books. The S. and J. numbers refer to Schultz and Julius’s ‘Tabel- larische Uebersicht der kiinstlichen organischen Farbstoffen.’ In the case of colouring matters » requiring mordants, the particular 286 REPORT—1898. mordant employed is indicated in brackets after the name of the dye- stuff. The colours marked thus (*) appear to be somewhat faster than the rest of the class in which they are placed. BROWN COLOURING MATTERS. Crass I. Very Fueirive CoLours. (W001.) The colours of this class have faded so rapidly that at the end of the first ‘fading period’ (July 22 to Aug. 22, 1896) only a very faint colour remains, or it has become very materially altered in hue. At the end of the fifth period (about one year) all traces of the original colour have disappeared, the woollen cloth exhibiting merely a yellowish, brownish, or greyish tint, according to the colour of the original pattern. Azo Colours. Wool Book XII. Basic Colours. 1. Leather Brown R. Constitution not published. at 2. Chrysoidine AG. From aniline and wm-phenylene-diamine. S. and J. III. 16. 3 3. Chrysoidine FF. From aniline and m-toluylene-diamine. - 8. Leather Brown V. Constitution not published. Direct Cotton 1. Titan Brown Y. Constitution not published. Colours. 2. Benzo Brown 5R. From Primuline and phenylene-diamine. S. and J. III. 110. ‘ *4. Cloth Brown (red shade). From benzidine, salicylic acid, and a-naphthol-sulphonic acid NW. S. and J. III. 193. +i 13. Benzo Brown G. From sulphanilic acid and Bismarck Brown. 8. and J. III. 273. 25. Hessian Brown MM. From sulphanilic acid, tolidine, and resorcinol. §. and J. III. 278. sory Colours. Wool Book XII. Direct Cotton 21. Mikado Brown M. Constitution not published. Colours. Norrs.—In the case of Chrysoidine AG and FF, and Cloth Brown, the colours alter very rapidly during the first ‘period of exposure,’ the altered colours then fade more slowly, without any further change in hue. Cuass II. Fucirive Conours. (Woot.) The colours of this class show very marked fading at the end of the second ‘fading period’ (August 22 to September 29, 1896), and after a year’s exposure they have entirely faded, or only a brownish, drab, or grey tint remains. Azo Colowrs. Wool Book XII. Acid Colours. 1, ResorcinBrown. From m-xylidine, sulphanilic acid, and resorcinol. 8. and J. III. 163. . Fast Brown G. From sulphanilic acid and a-naphthol. S. and J. IIL. 165. ; 4, Acid Brown G. From aniline and m-diamido-azo-benzene-p-mono- ulphonic acid. §8. and J. II. 136. bo a i ti i i ON THE ACTION OF LIGHT UPON DYED COLOURS. 287 Wool Book XII. Acid Colours. 7. Naphthylamine Brown. From naphthionic, acid and a-naphthol. 8. and J. III. 92. io 8. Sulphamine Brown. From a-naphthylamine and nitroso-6-naph- thol-sodium-bisulphite. §. and J. III. 57. ey 9. Acid Brown R. From naphthionic acid and Chrysoidine. S. and J. II. 91. “ 10. Alkali Brown. From Primuline and m-phenylene-diamine. 8S, and J. III. 110. x 11, Fast Brown 3B. From f-naphthylamine-sulphonic acid Br and Wool Book XIII. a-naphthol. §. and J. III. 103. Basic Colours. *1. Chrome Brown RO (Cr). From naphthionic acid and a-naphthol. S. and J. IIL. 92. 35 *2. Chrome Brown BO (Cr). Constitution not published. = *3. Chrome Brown R(Cr). Constitution not published. PS 4. Nut Brown. From m-toluylene-diamine and m-toluylene-diamine. 8. and J. ITI. 174. rr *5, Bismarck Brown 2G. From wm-phenylene-diamine and m- phenylene-diamine. §,. and J. III. 172. 53 *6. Leather Brown. From amido-p-acetanilide and m-phenylene- diamine ; products treated with HC]. §S. and J. III. 160. a. *7, Leather Brown O. Similar to Leather Brown. f Direct Cotton 8. Diazochromine BS. Constitution not published. Colours. 11. Toluylene Brown R. From sulphanilic acid and Bismarck Brown sulphonic acid. a 15. Direct Brown Y. From m-amido-benzoic acid and Bismarck Brown. 8. and J. III. 275. - 19. Cloth Brown (yellow shade). From benzidine and salicylic acid and dioxy-naphthalene (2:7). S. and J. III. 194. $5 26. Catechu Brown. From Bismarek Brown and m-phenylene diamine. S. and J. II. 220. 7 27. Congo Brown VBB. Constitution not published. + *28. Catechu Brown DDX. Constitution not published. 9 *29. Catechu Brown DDDX. Constitution not published. es *30. Hessian Brown B. Constitution not published. re *31. Azo Brown. Constitution not published. = *32. Toluylene Brown R. Constitution not published. 7 *33. Benzo Brown. Constitution not published. = *34. Benzo Brown BR. Constitution not published. + *35. Benzo Brown B. From naphthionic acid and Bismarck Brown. 8. and J. III. 274. % *36. Benzo Brown NB. Constitution not published. a *37. Toluylene Brown M. Constitution not published. - *38. Toluylene Brown B, Constitution not published. ae *39. Cotton Brown A Constitution not published. 5 *40, Cotton Brown N. Constitution not published. ai 42. Toluylene Brown VO. Constitution not published. 34 44. Toluylene Brown 2BO. Constitution not published. $3 46. Benzo Black Brown. Constitution not published. . 47. Sulphon Brown R. Constitution not published. si *48. Sulphon Dark Brown. Constitution not published. Direct Cotton 2. Diazo Brown R (extra). Constitution not published. Azotised Colours and developed with 8-naphthol. developed. *3. Zambesi Brown G. Constitution not published. Azotised and developed with toluylene-diamine. % 4. Diazo Brown G. Constitution not published. Azotised and developed with £-naphthol. is 5. Zambesi Brown 2G. Constitution not published. Azotised and developed with toluylene-diamine. + 6. Diazo Brown Y. Constitution not published. Azotised and developed with 8-naphthol. 5 7. Diazo Brown V. Constitution not published. Azotised and de- veloped with 8-naphthol. 288 REPORT—1898. Wool Book XIII. Direct Cotton *8. Diamine Brown V. From benzidine and amido-naphthol-sulphonic Colours acid and m-phenylene diamine. §. and J. III. 182. Azotised developed. and developed with phenylene-diamine. Natural Colouring Matters. Mordant 6. Sanderswood (Cr). Pterocarpus santalinus (wood). Colours. 7. Barwood (Cr). Baphia nitida (wood). + *8. Ventilago (Cr). Ventilago madraspatana (root-bark), 10, Camwood (Cr). st 11. Limawood (Cr) (Cu). Czesalpinia echinata (wood). a *13. Catechu (Cr). Areca catechu (extract). Nores.—Leather Brown and Leather Brown O might almost equally well be classed as ‘ moderately fast’ colours. In the first ‘fading period’ they become somewhat greyish in hue, but the altered colour fades very gradually, leaving at the end of a year a fairly good drab-grey colour. Crass III. Moprrarery Fast Contours. (Wo00z.) The colours of this class show distinct fading at the end of the second period (August 22 to September 29, 1896), which becomes more pro- nounced at the end of the third period (September 29 to November 5, 1896). A pale tint remains at the end of the fourth ‘ period of exposure’ (November 5, 1896, to May 22, 1897), and at the end of a year’s exposure the colour has entirely faded, or at most only traces of colour remain. zo Colours. : Wool Book XII. Acid Colours. *3. Azo Acid Brown. Constitution not published. 5 6. Fast Brown. From xylidine-mono-sulphonic acid, and a-naphthol. 8. and J. IT. 80. A 12. Fast Brown. From naphthionic acid, and resorcinol. §S. and J. III. 164. Pr 14. Diamond Brown. Constitution not published. Direct Cotton 7. Congo Brown G. From sulphanilic acid and benzidine, with Colours. resorcinol and salicylic acid. S.and J. III. 269. a 9. Thiazine Brown G. Constitution not published. 9 . Congo Brown R, From a-naphthylamine-sulphonic acid L and benzidine, with resorcinol and salicylic acid. S. andJ. III. 270- + 14. Hessian Brown 2BN. Constitution not published. eS 16. Hessian Brown 2B. From sulphanilic acid and benzidine, with resorcinol. §. and J. III. 277. ae 17. Thiazine Brown R. Constitution not published. a 20. Diamine Bronze G. From benzidine, with salicylic acid and amido - naphthol - disulphonic -acid-H-azo-m-phenylene-diamine- 8. and J. IIT. 263. 3 41. Diamine Brown M. From benzidine, with salicylic acid and ‘y-amido-naphthol-sulphonic acid. - 43. Diamine Brown B. From benzidine, with phenyl-y-amido-naphthol- sulphonic acid. 5 45. Benzo Dark Brown. Constitution not published. Direct Cotton *1. Diamine Cutch. Constitution not published. Naphthylene Violet Colours azotised and developed with sodium carbonate. §.and J. III. developed. 256. Azoxy Colours. Direct Cotton 22. Mikado Brown 2B. Constitution not published. Colours. 23. Mikado Brown G. Constitution not published. Pe 24. Mikado Brown B. Constitution not published. FL. Sh teen SE —————— Eee SC CC eee oe ON THE ACTION OF LIGHT UPON DYED COLOURS. 289 Natural Colouring Matters. Wool Book XIII. Mordant Colours *Ventilago (Cu) (Fe). Ventilago madraspatana (root-bark). PH Sanderswood (Cu) (Fe). Pterocarpus santalinus (wood). 5 Barwood (Cu) (Fe). Baphia nitida (wood). = Camwood (Cu) (Fe). Norrs.—Diamine Brown M loses its reddish hue and becomes appa- rently darker during the first ‘fading period’; the altered colour fades slowly, and finally leaves at the end of a year a pale drab colour. Azo Acid Brown acquires a more yellowish hue during the first ‘fading period’ ; the colour then fades very gradually without further change of hue, leaving at the end of a year a very pale brown. It might fairly well be classed as a ‘ fast colour.’ The Mikado Browns are by no means so fast to light as the Mikado Oranges and Yellows : they experience the greatest change in depth of colour during the first ‘fading period’; the altered colour, which is yellower than the original one, then fades very gradually, and leaves at the end of a year a fairly good buff colour. Crass IV. Fast Cotours. (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 exposure’ a pale shade remains, which at the end of the year’s exposure still leaves a pale shade. Azo Colours. Wool Book XII. Direct Cotton 5. Toluylene Brown G. From toluylene-diamine-sulphonic acid and Colours. m-phenylene-diamine. §. and J. III. 241. ae 6. Direct Cotton Brown R. From amido-nitroso-stilbene-disulphonic acid and aniline. Natural Colouring Matters. Wool Book XIII. Mordant Colours. 12. Cochineal (Cr). Coccus cacti (insect). Cuass V. Very Fast Contours. (Woot.) 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. Oxyketone Colowrs. Wool Book XIII. Mordant Colours. Alizarin Bordeaux B (Cr) (Cu). Tetra-oxy-anthraquinone (1.2.5.8). Quinalizarin. 8. and J. IIL 403. “E Alizarin Bordeaux G (Cr) (Cu). “5 Alizarin Bordeaux GG (Cr) (Cu). hy Alizarin Maroon (Cr) (Cu). Amido-purpurin. §. and J. III. 394, ” Alizarin Brown (Cr) (Fe). Diamido-alizarin. = Anthracene Brown (Cr) (Fe). Tri-oxy-anthraquinone (1.2.3) Anthragallol. §. and J, III. 396. 1898, U 290 REPORT—1898. Natural Colouring Matters. Wool Book XIII. Mordant Colours. Morinda Root (Cr) (Cu) (Fe). Morinda citrifolia (root). y Mang-kudu (Cr) (Cu) (Fe). Morinda umbellata (root-bark). . Chay Root (Cr) (Cu) (Fe). Oldenlandia umbellata (root). 3 Munjeet (Cr) (Cu) (Fe). Rubia cordifolia (root). “ Madder (Cr) (Cu) (Fe). Rubia tinctorum (root). a Lac-dye (Cr) (Cu) (Fe). Coccus ilicis (insect). Cochineal (Cu) (Fe). Coccus cacti (insect). Additional Colours. Oxidation Colour. Chromogen I. (1.8) Dioxy-naphthalene- (3 . 6) disulphonic acid ; oxidised with bichromate of potash. 8. and J. III. 504. BLACK COLOURING MATTERS. Cuass I. Verry Fuaitive Cotours. (WOootz.) Azo Colours. Wool Book XIV. Acid Colour. 4. Violet Black. From p-phenylene-diamine, with a-naphthylamine and a-naphthol-sulphonic acid NW. S&S. and J. III. 502. Direct Cotton 1. Nyanza Black B. From p-phenylene-diamine-azo-a-naphthyl- Colours amine and amido-naphthol-sulphonic acid +. 2. Tabora Black R. Constitution not published. 4 Nores.—During the first ‘fading period’ Violet Black changes to a dull vinous red colour. Crass II. Fuairive Cotours. (WO00t.) Azo Colours. Wool Book XIV. Acid Colours. 6. Azo Nigrine R. From phenol-disulphonic-acid-azo-a-naphthyl- amine and £-naphthol. s 12. Wool Black. From amido-azo-benzene-disulphonic acid and p-tolyl-8-naphthylamine. 58. and J. III. 139. 13. Jet Black G. Constitution not published. af 19. Phenylene Black. From a-naphthylamine-disulphonic acid-azo-a- naphthylamine and diphenyl-m-phenylene-diamine. 8S. and J. IL. 152. 21. Anthracite Black R. From a-naphthylamine-disulphonic acid and a-napht hylamine-azo-dipheny!-2-phenylene diamine. 26. Azo Acid Black B. Constitution not published, is 27. Azo Acid Black G. Constitution not published. Direct Cotton 10. Direct Deep Black T. Constitution not published. Colours 11. Columbia Black 2B. Constitution not published. is 12. Columbia Black B. Constitution not published. 13. Oxy Diamine Black N. Constitution not published. is 14, Union Black 8. Constitution not published. 35 16. Oxy Diamine Black SOOO. Constitution not published. is 18. Columbia Black R. Constitution not published. Direct Cotton 1. Diamine Black BH. From benzidine, and y-amido-naphthol-sul- Colours phonic acid, and amido-naphthol-disulphonic acid H; developed developed. with Fast Blue Developer AD. 2. Diazo Black B. From benzidine and a-naphthylamine-sulphonic acid L; developed with §-naphthol. ” ft — — —- —_— | eee eee — ON THE ACTION OF LIGHT UPON DYED COLOURS. 291 Wool Book XIV. Direct Cotton *3. Diamine Black ROO. From benzidine and f-amido-naphthol- Colours sulphonic acid; developed with Fast Blue Developer AD. developed 8. and J. III. 187. $ 4. Diazo Black R. Constitution not published. Developed with B-naphthol. + 5. Diazo Black H. Constitution not published. Developed with B-naphthol. " *8, Diamine Black BO. From ethoxy-benzidine and amido-naphthol- sulphonic acid y; developed with Fast Blue Developer AD. 8. and J. III. 229. Oxazine Colours. Basic Colours. 1. Cotton Black. Constitution not published. Natural Colouring Matters. Mordant Colours. Limawood (Fe). Czsalpinia echinata (wood). Nortes.—The following colours acquire a reddish or purplish tint during the fading process: Azo Acid Blacks B and G, Columbia Blacks B and R, Union Black $8, Oxy-diamine Black SOOO, Diamine Black RO and BO. An olive tint is acquired by Direct Deep Black T. Crass IIT. Moperarety Fast Cotours. (Woot.) LInduline Colours. © Wool Book XIV. Acid Colours. *9. Nigrisine. Sodium salt of aninduline-sulphonicacid. S.and J. III. 475. a3 *10. Brilliant Black EB. Constitution not published. Basic Colours 2a. Nigrisine J. Condensation product of p-nitroso-dimethyl- aniline 4 3a. Nigrisine. Similar to Nigrisine J. S. and J. III. 502. Azo Colours. Acid Colours *5. Naphthol Black 4R. Constitution not published id 8. Jet Black R. From amido-benzene-disulphonic-acid-azo-a- naphthylamine and phenyl-a-naphthylamine. S. and J. III. 150. 3 11. Naphthylamine Black. From a-naphthylamine-disulphonic- acid-azo-a-naphthylamine and a-naphthylamine. S. and J. III. 153. 3 *41. Acid Black B. Constitution not published. Fs 16. Acid Black 2B. Constitution not published. ay *17. Naphthol Black 6B. From a-naphthylamine-disulphonic acid- azo-a-naphthylamine and £-naphthol-disulphonie acid R. 8. and J. III. 154. ce *18. Naphthol Black 3B. Constitution not published. ss *20. Victoria Black B. From sulphanilic acid-azo-a-naphthylamine and 8-naphthol-sulphonic acid S. §S. and J. III. 149. a *22. Naphthol Black B. From £-naphthylamine-y-disulphonic acid- azo-a-naphthylamine and £-naphthol-disulphonic acid R. S. and J. III. 157. » 25. New Victoria Black Blue. Constitution not published. ” 28. Naphthylamine Black 6B. Constitution not published, ”» *29. Victoria Black Blue. Constitution not published, ” 30, Naphthylamine Black 4B. Constitution not published. » 31. New Victoria Black B. Constitution not published. 3 *32. Victoria Black G. Constitution not published. ” *33. Victoria Black 5G. Constitution not published. ” 34. New Victoria Black 5G. Constitution not published. U2 292 Wool Book XIV. Basic Colours. *3. Direct Cotton 3. Colours. > Je} — pd Direct Cotton Colours 6 developed ib Mordant Colour RASH - Chicago Grey. “1 ore REPORT—1898. Diazine Black. From Safranine and phenol. Benzo Black Blue G. From benzidine-disulphonic acid, with a-naphthylamine-azo-a-naphthol-sulphonic acid NW and a-naphthol-sulphonic acid NW. S. and J. III. 266. Lenzo Black Blue R. From tolidine, with a-naphthylamine- azo-a-naphthol-sulphonic acid NW and a-naphthol-sulphonic- acid NW. S.and J. III. 266. Benzo Black. Constitution not published. Benzo Black § extra. Constitution not published. Diamond Jet Black OO. Constitution not published. Constitution not published. Diamine Jet Black 8S. Constitution not published. Diamine Black HW. Constitution not published. Benzo Black Blue 5G. From benzidine-disulphonic acid, with a-naphthylamine-azo-dioxynaphthalene-sulphonic acid S and dioxynaphthalene-sulphonic acid 8. S. and J. III. 267. Diazo Brilliant Black B. From tolidine and a-nuaphthylamine- sulphonic acid L; developed with B-naphthol. Diazo Brilliant Black R. Constitution not published. De- veloped with B-naphthol. Chrome Black (Cr). Constitution not published. Diamond Black (Cr). From amido-salicylic-acid-azo-a-naphthyl- amine and a-naphthol-sulphonic acid NW. S. and J. III. 159. Diamond Black NG (Cr). Constitution not published. 3. Diamond Black GA (Cr). Constitution not published. ” 1 » 3. 4 iz e Natural Colouring Matters. Mordant Colours. Logwood (Cr) (Fe*). Hmatoxylon campechianum (wood). Cochineal (Fe*). Coccus cacti (insect). Nores.—The colours dyed with the two Nigrisines are medium shades of grey : they do not alter materially in hue during the fading process, and at the end of the third period of exposure they still appear as pale greys. The following colours alter very little in hue while fading, and fade so gradually that they might fairly well be thought worthy of being classed as ‘Fast Colours :’ Nigrisine, Brilliant Black EB, Acid Black B, Naphthol Blacks 3B and 6B, Victoria Blacks B, G, and 5G, Victoria Black Blue. Diazine Black acquires a somewhat yellowish cast at the end of the first period of exposure, ard then fades so slowly that even at the end of a year a full grey shade remains. Several of the artificial black colours in this class are quite as fast to light as the black obtained with logwood on chromium mordant ; some indeed seem to be more permanent, and they do not acquire the characteristic olive tint of the faded logwood and chromium black. With iron mordant logwood gives a somewhat faster black than that obtained with chromium ; the same appears to be the case with Chrome Black and the various marks of Diamond Black. Crass IV. Fast Corours, (Woot.) Azo Colowrs. Wool Book XIV. Mordant Colours. 5. Chrome Black (Fe). Constitution not published. af 6. Diamond Black (Fe). From amido-salicylic acid-azo-a naph- thylamine and a-naphthol-sulphonic acid NW. S. and J. III. 159. At 7. Diamond Black NG (Fe). Constitution not published ~~ 8. Diamond Black GA (Fe). Constitution not published. ON THE ACTION OF LIGHT UPON DYED COLOURS. 293 Oxyketone Colowrs. Mordant Colours * Alizarin Black SW (Cr) (Fe). Sodium bisulphite compound of dioxy-naphthoquinone. S. and J. IIT. 385. * Alizarin Bordeaux G (Fe). Constitution not published. * Alizarin Bordeaux B (Fe). Tetra-oxy-anthraquinone (1.2.5.8), Quinalizarin. §. & J. III. 403. ” Crass V. Very Fast Contours. (WO0L.) Oxyketone Colowrs. Wool Book XIV. f i Mordant Colours Alizarin Bordeaux GG (Fe). Constitution not published. Sik Patterns. Most of the foregoing colours were also dyed on silk, and the patterns were exposed to light along with the woollen patterns. The relative fastness of the various colours is generally the same as on wool, and a special classification for silk seems unnecessary. The Carbohydrates of the Cereal Straws.—Third Report of the Com- mittee, consisting of Professor R. Warineton (Chairman), Mr. ManninG PRENTICE, and Mr. C. F. Cross (Secretary). (Drawn up by Mr. Cross.) Tur work, which was carried out in the agricultural season of 1897, has been reported upon in a paper published in the ‘Journal of the Chem. Soc.’ 1898, p. 459. The purpose of these later investigations was to trace the effect of removing the seed-bearing organs upon the carbo- hydrates of the stem. The results were, however, negative, adding another confirmation to the conclusion previously arrived at, that the carbohydrates of the stem tissues are built up with a constant ratio of ‘furfural-yielding’ to normal hexose carbohydrates. Further evidence was also obtained that these two groups of carbohydrates are in the earlier stages of growth similarly attacked by boiling dilute acids, and after such hydrolysis are similarly fermented by yeast. It must in fact be admitted that as condensation to furfural is by no means an exclusive characteristic of C; Carbohydrates, there is no evidence whatever that the furfuroids of the barley straw are, in the early stages of growth, pentose-anhydrides or pentosanes. There now appears in the ‘Journ. Fed. Inst.’ Brewing, 1898, p. 438, an article by Tollens under the title ‘On the Carbohydrates of Barley and Malt, with special reference to the Pentosanes,’ in which, as a result of yeast fermentations of the products of acid hydrolysis of brewers’ grains, the author arrives at the following conclusions :—‘ From the behaviour of these furfural-yielding substances on fermentation we are forced to the view that they behave, to some extent, similarly to the ordinary hexoses, and somewhat different from the pentoses, for when brought into contact with yeast they exhibit certain manifestations of fermentation ; but they give rise to the formation of but little alcohol and much acid. It must be concluded from this that the furfural-yielding substances . . . contain a certain amount of other substances more susceptible to fermentation than “ota and xylose. They may contain glycuronic acid or oxycellu- loses... . We are very glad to have this confirmation from so great an authority 294 REPORT—1898. as Professor Tollens, and we will not quarrel with his decision ‘ to retain the old name pentosanes for this group of substances,’ instead of ‘ the indefinite name of furfuroids proposed by Cross and Bevan.’ We will only remark that, as the idea has been abandoned that they are exclusively and defi- nitely pentosanes, it appears more logical to adopt a term of corresponding significance, We ourselves have recently carried out a more extended series of fermentation experiments which further define these products, and the results of this work will be published in the course of the autumn. Generally, the position for which we have long contended may be taken as fully established, viz. that the plant worla affords a group of furfural- yielding bodies, probably carbohydrates, which are susceptible of fermen- tation by yeast. , . We have next resumed the study of the problem of the relationship of such compounds to the normal hexoses, on the basis of the purely chemical probabilities. We have previously shown that furfuroids are produced from the hexoses by many processes of oxidation. One such process, which we had overlooked, appeared from the researches of Fenton in the province of the dicarboxylic acids to be capable of extension to other hydroxy compounds, such as the carbohydrates—that is, the action of hydrogen peroxide in presence of iron salts. A research in this direction has led to positive results. We have not only succeeded in producing furfuroids in some quantity—7 to 9 per cent. of the hexaldoses—but we find that dicar- bonyl derivatives are produced reacting with phenylhydrazine acetate in the cold to form dihydrazones, which appear to be osazones. We have published a preliminary account of this research in the ‘Journal -of the Chem. Soe.’ 1898, p. 463, and since the publication of the paper we have been joined in the investigations by Dr. R. S. Morrell. Results have been obtained confirming and extending those of our preliminary paper, and these wili be published in the course of the autumn. We have every ex- pectation that the investigations will lead to results of physiological significance by elucidating processes actually taking place in the plant- cell. The Electrolytic Methods of Quantitative Analysis.— Fifth 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. HucH Marsuatu, Mr. A. E. FLETCHER, and Professor W. CARLETON WILLIAMS. PAGE The Determination of Zinc. By Professor W. CARLETON WILLIAMS, B.Se. - 296 The Determination of Nickel and Cobalt (Part T.). By HuGH MARSHALL, D.Se., F.R.S.L. ; - : : : 5 : , d : : . 300 A CONSIDERABLE portion of the experimental work in progress last year has now been completed, and the investigations on the determination of zinc, cobalt and nickel are included in the present Report. Further work on the determination of bismuth, the first portion of which was published in the third report of the Committee, is in hand, but is not yet ready for publication. It is proposed to proceed with the study of the methods for separating cobalt, nickel, iron and zinc respectively from other metals. The Committee ask for reappointment, without further grant. ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. The Determination of Zinc. 295 By Professor W. Carteron WIix.iaAms, B.Sc. Reinhardt and Ihle Warwick, H. Ss. Bibliography. Author Journal Year| Vol.| Page| Composition of Electrolyte Wrightson,F,. . . Zeits.anal.Chem. | 1876 | 15 297 | Ammonium hydrate Mimllot; A... els Bull. Soc. Ohim. | 1877 | 32 482 | Potassium cyanide Riché, A, . f : Compt. Rend. .| 1877 | 84 226 | Ammonium sulphate, hydrate, and acetic acid Parodi, G., & Maseazzini, A. | Zeits.anal.Chem. | 1877 | 16 469 | Ammonium acetate ‘ oa ee Ate Bere ie J . | 1877 | 10 | 1098 lean? acetate and citric - a5 ¥ » | Zeits.anal.Chem. | 1879 | 18 587 acid Beilstein, A.,and Jawein,J. | Ber. . ¥ - | 1879 | 12 446 | Potassium cyanide Alkali acetate, tartrate or ci- aoe + trate Luckow, C. e . «| Zeits.anal.Chem. | 1880; 19 1 Ammonium hydrate Potassium cyanide Classen, A.,and Reis, M.A. | Ber. . “ . | 1881 | 14 | 1622 | Ammonium oxalate J. prakt. Chem. .| 1881 | 24 193 | Potassium oxalate Millot, A. . hy 2 . | Bull. Soc. Chim.. | 1882 | 37 339 | Alkali hydrate Riché,A. . 5 - . | Ann.Chim,etPhys.| 1882 | 13 508 | Ammonium sulphate and sul- phuric acid = ( Hydrochloric acid ; as amalgam Luckow, 0. . 3 . | Chem. Zeit, 1885 9 338 {Sulphuric acid ; a¢ amalgam ( Sodium phosphate, ammonium Moore,T. . . « «| Chem. News 1886 | 53 209 earbonate, and potassium { cyanide Brand, A. . . . . | Zeits.anal.Chem. | 1889 | 28 581 | Sodium pyrophosphate and ammonium carbonate Ammonium oxalate Kohn, C. A., & Woodgate, J. | J.Soc.Chem,Ind. | 1889 8 256 |/ Ammonium sulphate and hy- drate Gibbs, W. . a . Amer. Chem. J.. | 1891 | 13 570 | Sulphate; as amalgam Nahnsen, G. x = Berg. u. hiitten. | 1891 | — 393 | Sulphuric acid Zeit. Smith, E. I.,and Muhr, I. | J. Analyt.& App. | 1891 5 488 | Tartaric acid and ammonium Chem. hydrate Ammonium oxalate ; as amal- 5 On gam Mermmann (Gs. <6 6 | Ber.’ : . | 1891 | 24 | 2749 WecbAniG: neiaamda Aenoniaes ( hydrate ; as amalgam Riidorff, F. . a 5 . | Zeitsangew.Chem.| 1892 | — 198 | Sodium acetate and acetic acid . . | Zeits.anorg.Chem.) 1892 1 285 | Formate and formic acid Vortmann,G. . : . | Monatsh. Chem.. | 1893 | 14 536 | Potassium tartrate and sodium hydrate Ber. = c J ( ara y * | 1894 27 2060 | (Ammonium or potassium oxa- GisssenjA. 5 Od Seer: i a ne See 1894 1 280 || late and tartaric acid Thomiilen,H. . = Zeits. Electro- 1894 | 1 304 | { Sodium acetate and acetic acid Chem. | % | Potassium oxalate and sulphate Jordis,E. . A 2 Zeits. Electro- 1895 - “ ) Ammonium lactate, glycollate, C4 . Chem. 655 | and sulphate Nossensiin, H. . : . | Zeits. Llectro- | 1895 2 183 | Ammonium lactate, glycollate, Chem. and sulphate Nicholson, H.H.,& Avery,S. | J. Amer. Chem. | 1896 | 18 654 | Sodium formate Soe. Wagner, E. . ry . Zeits, Llectro- | 1896 2 614 | Ammonium oxalate and tar- Chem. taric acid mie ws . . . | Zeits. lectro- | 1896 3 19 | Ammonium oxalate and tar- Chem. taric acid Wolman, L. . . . - | Zeits. Electro- | 1897 3 539 | Comparison of different me- Chem. thods for estimating zine The preceding references show that a large number of electrolytic pro- cesses for the estimation of zinc have been proposed during the last twenty years, many of which are said to yield accurate results. Seven of these methods have been investigated. Since the completion of these experi- ments in 1897, a comparison of the different methods for the estimation of zinc has been published by Wolman (v. ante). This has made further work on the simple estimation of zinc unnecessary ; our comparative con- 296 REPORT—1898. clusions are contrasted in the sequel. The methods examined were based on the deposition of zinc from a solution containing :— i. Sodium pyrophosphate. ii. Alkaline oxalate in neutral or alkaline solution. iii, Alkaline oxalate in presence of potassium sulphate. iv. Potassium or ammonium oxalate and free tartaric acid. v. Potassium cyanide. vi. Potassium cyanide and sodium phosphate. vii. Ammonium lactate and ammonium sulphate. In the following experiments the zinc was always present as sulphate, and the metal was deposited in platinum basins, which were protected from the action of the zinc by a deposit of copper, which extended three or four millimetres beyond the surface of the liquid, during the electrolysis. The basins are coppered by means of a hot solution of copper ammonium oxalate containing free oxalic acid, with a current density of 0°5 to 1 ampere ; the operation only requires two or three minutes. Unfortunately, the layer of copper must be renewed for each zinc determination.. Experi- ments were made with the object of protecting the platinum with layers of gold or silver, but, on the whole, better results were obtained with the coppered basins. If the zinc is deposited on the unprotected surface of the platinum a black stain is produced, when the zinc. deposit is dissolved in acid. According to Vortmann (Ber. 24, 2753) the black deposit con- sists of finely divided platinum. The end of the reaction was generally ascertained by tilting the vessel or increasing the volume of the solution, so that the liquid came in contact with an unaltered layer of copper. In a small number of determinations the end was ascertained by hanging a narrow strip of metallic copper over the side of the basin ; if the colour of the copper remains unchanged, the precipitation of the zinc is complete. As the last traces of zinc are deposited with difficulty the current density is always increased to one ampere at least towards the end of the operation. The deposit was washed with water without interrupting the current. It was finally washed with alcohol and dried at 80°. No signs of oxidation were noticed. I.— Deposition of Zine from Solution of Pyrophosphate. Brand’s method is simple and accurate. The solution of zine salt is mixed with 4 grme. of sodium pyrophosphate and with about 5 c.c. of a saturated solution of ammonium carbonate ; water is added until the liquid measures 120 or 150 c.c., and the mixture is electrolysed. The zinc is obtained as a bright bluish-white deposit, adhering firmly to the basin. Experi- | Zinc taken: | Zine found: C.D.400 Time: | E M.P, Error in ment grme. grme. Amperes hours Volts mgrme, 1 0:2342 02347 0:2 Uf a= +05 2 _ 0:0507 0:0502 02 —1:0 a = —05 3 0-0733 0:0738 0:16—0°8 7 = +05 4 0°1551 01551 0-45 6 = 0-0 5 0:2174 0:2171 0°53 — 2: 4 75 -—0°3 6 0°2185 0:2190 05 -1 4 | 91. fide elt egtlanaatwayt 77 +05 | _—- ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 297 II.—Deposition of Zinc from Solution of Double Oxalate. In 1881 Classen, and also Reinhardt and Thle, suggested the addition of potassium or ammonium oxalate, or of both oxalates, to the zinc salt. The electrolysis is carried on at the ordinary temperature. The method yields good results when the quantity of zinc does not exceed 0-2 grme. ; when larger quantities of zinc are taken the deposit is liable to be dull and spongy instead of firm and bright. Experi- | Zinc taken: | Zine found: C.D.100 Time: | E.M.F, Error in ment grme. grme. Amperes hours Volts milligrms, 1 0°1635 0:1638 0:18 3 4:0 +03 2 0:2103 0:2098 0:67 4 4:0 —0°5 3 0°3154 0°3148 0:22 4 37 —06 4 0:1087 071091 0:2 5 4:0 +0°4 5 0:0384 0:0382 0:2 4 4:0 —0°2 6 0:0362 0:0359 0:2 4 4:0 —0°3 7 0:2044 0:2043 0°22 4 4:0 —O1 8 0:2044 0°2041 0°22 4 39 —0°3 9 0:0719 0:0717 0:22 4 4:0 —0:2 10 0:1087 0°1084 0:22 4 4:2 —0°3 11 0:0740 0:0740 0:22 4 6:0 0:0 12 0:2861 0:2852 0:22 4 4:0 —0°9, loose, spongy In experiments 1, 2, 3 and 12 the zinc salt dissolved in water was poured into a hot solution of potassium oxalate (8 grme.); in 4 and 5 ammonium oxalate (8 grme.) was substituted for the potassium salt ; and in experiments 6 to 11 a mixture of potassium oxalate (6 grme.) and ammonium oxalate (2 grme.) was used. This mixture gave the best results. III.—Deposition of Zine from Solution of Alkaline Oxalate and Sulphate. The addition of potassium sulphate (3 grme.) to the potassium oxalate (4 grme.), as recommended by Miller and Kiliani, does nat appear to improve the process. Experi- | Zinc taken: | Zine found: C.D.100 E.M.F. | Error in R 2 ment grme., grme. Amperes Volts | mgrme. emarks il 02044 0:2032 0-4 4 —1:2 Black spots 2 0:1051 0:1047 0:14 4 -—0-4 Bright 3 0:0732 0:0733 0°17 6 +01 Black spots + 0:2729 0:2726 0:28 78 —03 Bright 5 0:0740 0:0734 0-2 4 —06 Bright The zine is deposited as a bright, firmly-adhering film, occasionally marked by black spots. Classen quotes experiments in the fourth edition of his ‘ Quantitative Analyse durch Elektrolyse’ showing that this method yields low results. IV.-—Deposition from Hot Solution of Alkali Oxalate in Presence of Tartaric Acid. The solution of zinc sulphate is mixed with 4 grme. of potassium or ammonium oxalate, diluted with water, and electrolysed at a temperature of 298 REPORT—1898. about 60° C. After the current has passed through the mixture for three minutes, the solution is acidified with tartaric acid, and kept acid through- out the operation by the addition of a 6 per cent. solution of tartaric acid. Wagner recommends that the hot solution should be electrolysed with a current of 0:2 ampere for fifteen minutes ; 5 c.c. of 6 per cent. tartaric acid solution are added and the current density increased to 0:5 ampere. The addition of the acid is repeated at intervals of fifteen minutes, In the following experiments Wagner’s directions were followed, with the exception that the tartaric acid was slowly added from a burette instead of in quantities of 5 c.c. A large excess of acid is to be avoided, and its addition should not be continued up to the end of the operation. The current is continued until the mixture has a neutral or feebly acid reaction, in order to prevent a small quantity of the acid tartrate of potas- sium or ammonium separating out. Experi-| Zinc taken: | Zinc found: C.D.100 E.M.F.) Time: °C Error in ment grme. grme. Amperes_ | Volts | hours a mgrme. 1 0°2103 0:2098 0°56 4 3 60 —0°5 2 0:0580 0:0582 05 8 3 60 +02 3 0°0435 0:0436 0°56 6 3 60 +01 4 0:2339 0:2344 0°56 8 3 60 +0°5 5 0:0909 0:0929 0-4 6 23 60 +2 6 0:2446 0:2457 0°5 8 2s 60 +1:1 7 0°1087 0°1092 0-5 6 24 60 +0°5 8 0:0363 0:0369 0-5 6 24 60 +06 Bright, firmly-adhering deposits were obtained. In experiments 1 to 6 potassium oxalate was used ; in 7 and 8 ammo- nium oxalate was employed. In 5, 6 and 7 the mixture was strongly acid when the electrolysis was stopped. V.—Deposition from Solution in Potassium Cyanide. The solution is neutralised if necessary with potash, and a 20 per cent. solution of potassium cyanide is added until the precipitate redissolves. A large excess of cyanide is to be avoided. Experi-| Zinc taken: | Zine found: C.D.400 E.M.F.| Time: | Error in ment grme. grme. Amperes Volts | hours | mgrme. | °° KCN 1 0°2209 0°2213 05 8 6 +0°4 55 2 0:2175 0:2187 0°5 8 6 +1:2 6 3 0°2198 0:2209 0°5 8 7 +11 5 4 0:2173 0°2189 0-4 8 7 +1°6 7 5 0:0732 0:0728 0-4 8 42 —0-4 5 A bright film is obtained which leaves a smal] quantity of black deposit undissolved when treated with acid. The residue collected from several analyses proved on examination to be carbon. The presence of carbon no doubt accounts for the high results obtained. The platinum electrodes are attacked by the cyanide in this and in the following process. Ee ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 299 VI.— Deposition from Solution of Zine Phosphate in Potassium Cyanide. Moore recommends the precipitation of the zinc from sodium phos- phate solution as rapid and complete. Potassium cyanide is added to the mixture to redissolve the precipitate. Ammonium carbonate is then added, and the mixture electrolysed at 80° C. Experi-| Zinc taken: | Zine found: C.D.499 |E.M.F.| Time: ‘0 Error in ment grme. grme. Amperes Volts | hours : mgrme. 1 0°1630 0°1556 0-9 57 2 80 —T4 2 0:2174 0:2091 1:53 78 2 80 —83 3 0°2174 0:2133 06-11 73) 22 80 —41 4 0°1451 0:1433 0-4 75 6 60 —1°8 5 0°1569 0-1564 0:3 75 53 60 —05 6 0:2016 0:2023 0-4 v5) 6 60 +07 ih 0:2175 0:2187 0°5 8:0 6 60 +12 Experiments 1 to 3 show that the precipitation is not complete in two and a half hours. The method cannot be considered rapid. The deposit is firm and bright. On solution in acids a small quantity of carbon remains. VII.— Deposition from Solution of Ammonium Lactate and Sulphate. Jordis recommends the addition of 5-7 grme. of ammonium lactate and 2 grme. of sulphate to the zinc salt. The solution is acidified with lactic acid, and the hot solution electrolysed in a platinum basin. A mechanical stirring arrangement should be used. The operation lasts about one hour and a half. The author states that when 0°3 grme. of . zine are used the error does not exceed 1 milligramme. The following determinations were made without a stirring arrange- ment :— Experi- Zine taken ; Zine found : C.D.100 Time: Error in ment grme. grme. Amperes hours mgrme. 1 O-1571 071559 05-1 2 —12 2 0:2558 0°2558 0:5 2 0-0 3 0:1839 0°1850 0:5 2 +1:1 4 0:1813 0-1779 0°5 2 —3-4 Conelusions.—Both the methods in which potassium cyanide are used yield too high results and are objectionable on account of the action of the cyanide on platinum. Small quantities of zinc not exceeding 1 deci- gramme can be accurately determined by either of the three oxalate methods or by Brand’s pyrophosphate process. For larger quantities of zine Classen’s oxalate process (IV.) in presence of free tartaric acid and Brand’s method are recommended. These conclusions agree with Wol- man’s ! as regards the accuracy of the oxalate methods and the inaccuracy of the Beilstein cyanide process, but differ as to the merits of Brand’s pyrophosphate method, which Wolman condemns. Wolman also recom- mends Riché’s method, in which a slight excess of ammonia is added to the zinc solution and the mixture acidified with acetic acid, C.D. ))0°1—0°2 1 Zeits. Hlectro-Chem., 1897, 3, 540. 300 REPORT—1898. ampere, 4 volts, 3 hours. He also obtained excellent results with the process of Vortmann and Foregger. Three grammes of pure caustic soda are added to the neutral zinc solution. At a temperature of 50°, with a current density of 0:5 to 1:5 amperes, the precipitation of the zinc is com- plete in one hour and a half. The Determination of Nickel and Cobalt. (Part I.) Sy Hucwu Marsnatt, D.Sc., FRSL. Bibliography. Author Journal Year | Vol. | Page Composition of Electrolyte Gibbs, W. . r < . | Zeits.anal.Chem, | 1864 3 334 Ammonium hydrate *Mansfeld Direction . . | Zeits.anal.Chem. | 1872 | 11 1 Ammonium hydrate *Wrightson, F. , . - | Zeits.anal.Chem. | 1876 | 15 297 Ammonium hydrate Herpin,— . > ° . | Zeits.anal.Chem. | 1876 | 15 335 Ammonium hydrate Riché, A. . : 5 - | Compt.rend, .| 1877] 85 226 Ammonium hydrate *Schweder, E: P. . . - | Zeits.anal.Chem, | 1877 | 16 344 Ammonium sulphate and hydrate *Ohl, W. . « « «| Zeits,anal.Ohem. | 1879] 18 523 Ammonium hydrate { Alkali acetate, tartrate, citrate Ammonium hydrate { Potassium cyanide * Fresenius, F,, and Zeits.apal. hem, | 1880 | 19 314 ere sulphate and *Luckow, C. . 5 . - | Zeits.anal.Chem. | 1880 | 19 1 Bergmann, F. hydrate *Olassen, A., and Reis, M.A. | Ber. . : - | 1881 | 14 | 1622 Ammonium oxalate Riché,A. . 4 . . | Ann.Chim.etPhys.| 1882 | 13 508 Sulphuric acid *Moore,T. . . J . | Chem. News - | 1886 | 53 209 Phosphoric acid *Brand,A. . ° . . | Zeits,anal.Chem, | 1889 | 28 581 Sodium pyrophosphate Ammonium oxalate - *Kobn,C.A.and Woodgate,J. | J.Soc.Chem.Ind. | 1889] 8 | 256 Ee sulphate’ .and Potassium cyanide *Gibbs, W. . > . . | Amer. Chem. J.. | 1891 | 13 570 Sulphate ; as amalgam Het J. Anal.& App. Tartaric acid and ammonium *Smith, E. F. and Mur, F.. { er } 1s91| 5 | 488 { aie Ammonium sulphate and *Riidorff, F. . 2 a - | Zeits.angew.Chem.| 1892 | — 3 | hydrate Sodium pyrophosphate 5 Ammonium hydrate *Freudenberg, H.. . - | Zeits.phys.Chem. | 1893 | 12 97 { ignition cance ee *Vortmann,G. . = - | Monatsh. Chem.. | 1893 14 536 Alkali cyanide; as hydrate *Classen, A. . ° ° - | Ber, . = - | 1894 | 27 | 2060 Ammonium oxalate Oettel, F. . 3 4 . | Zeits.Electrochem.| 1894 1 196 Ammonium sulphate and hydrate - . Sodium sulphate and ammo- Riidorff, F. . . Ss . | Zeits.angew.Chem.| 1894 | — 388 { nium hydrate *Thomilen,H. . . . | Zeits.Hlectrochem.} 1894 1 304 Ammonium sulphate and hydrate * The references marked with an asterisk refer to both nickel and cobalt, the remainder to nickel only. Of the various methods of determining nickel and cobalt electrolyti- cally, that employing the sulphates in presence of ammonium sulphate and ammonia is by far the best known and most frequently employed. Next to it Classen’s oxalate method and Brand’s pyrophosphate method are probably those most frequently referred to. Of these three the former is, primd facie, the preferable one, owing to the great simplicity of work- ing it and the everyday character of the reagents employed, which are readily obtainable in a pure condition. Unless other methods can be shown to have a marked superiority in some important respect, we may assume that it will continue to be the general method for ordinary work, though the others might prove advantageous in special circumstances. The greater part of the investigation so far has therefore been devoted chiefly to a study of this method, and although only a limited number of experiments have been carried out with the other methods, the results ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 301 obtained indicate that it is not excelled by any of the latter, for the determination of nickel. The apparatus employed for most of the determination consisted of the usual cathode basins of about 200 c.c. capacity, roughened on their internal surface, with perforated anodes of watch-glass shape. In some experi- ments with small quantities of substance ordinary platinum crucibles were employed in place of the basins; in these cases a stout platinum wire coiled at the end served as anode. The electrical measurements were made by means of Davies’ ammeter and voltmeter, described in the third report of the Committee. ! When the large basins were employed the solutions were generally made up to a volumeof 130-135 ¢.c. This left plenty of room for further additions, in case these should be found necessary, and the active cathode surface was then approximately 100 sq. cm., so that the ammeter readings corresponded to current density as generally stated. With the crucibles the volume was 18-20 c.c., and the cathode surface was roughly calculated to be 20-25 c.m. The salts‘employed for analysis were generally the ammonium double sulphates, specially prepared for the purpose. Sometimes these were directly weighed out for each experiment, but solutions of known strength were also prepared, and measured quantities taken for various determina- tions. For-some experiments the pure chlorides were employed. It was considered unnecessary to analyse the material by the other usual methods, as they are not more accurate than the electrolytic process. The results were simply judged relatively to one another, that result being considered best which gave the lowest percentage result, provided, of course, the metal was completely deposited in each case. Great attention was also paid to securing deposits of good general appearance, as a bright, lustrous, and firmly coherent deposit is always much more satisfactory and much less liable to be injuriously affected. A dark powdery-looking deposit was therefore considered unsatisfactory, even although the numerical result came out all right. It is usually recommended to test for complete deposition by with- drawing, from time to time, portions of the liquid and adding hydrogen sulphide or potassium thiocarbonate. If this is done, however, the current must be continued for some time after no reaction is observed, otherwise a distinct quantity of metal may be left in solution. It was several times found that the whole volume of liquid after decantation gave a very dis- tinct reaction, although none was visible when a small portion was tested. It was therefore considered more convenient to determine what time was necessary for average experiments conducted under suitable conditions, and to adhere to this generally, unless there were marked indications, for example in the rate of decolourisation, that deposition was not pro- ceeding normally. The decanted liquid was always tested, and any case of incomplete deposition duly noted. In the case of nickel the liquid can simply be poured off at the con- clusion of the experiment, and the basin quickly rinsed with distilled water, as the deposit undergoes no apparent deterioration by such treat- ment, provided it is carried out quickly. In the case of cobalt it is not quite safe to work in this way, as the deposit is more liable to tarnish, and it is preferable, if the best results are desired, to employ the usual 1 Transactions, 1895. 302 REPORT—1898. siphon arrangement for decanting and washing without interruption of the current. After thorough rinsing with distilled water, and draining, the deposits were next treated with a few cubic centimetres of absolute alcohol, and finally dried in the steam oven. In each vase the outside of the basin was carefully wiped clean and rubbed with chamois leather. Previous to beginning a determination the clean basins were not ignited, but treated in the same way as when they contained deposits, in order that the two weighings might be made under as nearly as possible similar con- ditions. It was found that basins, cleaned by hydrochloric acid and treated as above, fluctuated in weight both upwards and downwards on successive occasions. This at first seemed to indicate considerable liability to error, and yet very concordant results were obtained. The discrepancies would seem to be due to the difficulty of removing the last traces of a deposit by means of hydrochloric acid. It almost appears as if slight alloying took place, for the surface of the platinum becomes marked up to the level at which the liquid has stood during several experiments. From time to time the basins were cleaned as thoroughly as possible by means of nitric acid, ignition, treatment with concentrated hydrochloric acid, &ec. The substances to be added to the solution must of course be free from any metal which can be deposited electrolytically. Those employed were tested by means of ammonium sulphide and also by performing a blank experiment. Both the ammonium sulphate and the ammonia were em- ployed in the form of ‘ 20 per cent.’ solutions, i.e. 100 c.c. contained 20 grme. of substance. The required quantities were measured out approximately in graduated tubes or pipettes, and the total volume made up to 130 c.c., or whatever volume was desired, by adding the necessary quantity of dis- tilled water. Determination of Nickel. The determination of nickel by the ammonium sulphate and ammo- nia method presents no great difficulty, and exceedingly good results are easily obtainable in ordinary circumstances. The first experiments were carried out in order to determine the general conditions under which the best results are obtained. From these the following were adopted as standard conditions for quantities of nickel ranging from 0:1 to 0°5 grme. or more, the volume of solution in that case being always about 130 to 135: ¢.¢.::— Substances added to Solution: 5 grme. of ammonium sulphate (25 c.c. of stock solution), and 5 grme. of ammonia (25 c.c. of stock solution). Current: 0°5-0-8 ampere per 100 sq. cm. of cathode ; potential differ- ence of electrodes 3-3:5 volts. Temperature: Ordinary temperature of laboratory (15°-30°C. In warm weather the temperature rises to the latter amount by the heating effect of the current). Time : 33-4 hours. Under these conditions the metal is completely separated as a firmly adherent, well-coloured, and reguline deposit, entirely soluble in dilute hydrochloric acid. In appearance it differs but slightly from the interior surface of the basin. It undergoes no apparent change when left for several days exposed to air, and the weight also remains constant. In successive or simultaneous experiments results are frequently obtained differing by less than would correspond to 0:0001 grme. in the weight of the deposit. ee " 'ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 303 Although the above conditions may be considered as practically en- suring a good deposit, it must not be supposed that they need always be strictly adhered to. Considerable latitude is allowable in certain respects. The influence which each factor exerts may next be considered. If ammonium sulphate is omitted or added in insufficient quantity, the ' resulting deposit is dark and rough. The amount stated may be largely exceeded, however, without influencing the character of the deposit. The only effect which a considerable excess of ammonium sulphate seems to possess is possibly to make it slightly more difficult to completely remove the last traces of metal ; that it does so is not quite certain. The proportion of ammonia is more important. When nickel salts are electrolysed with a platinum or other non-soluble anode, nickelic hydroxide is formed on the anode. This does not take place if a sufficient quantity of free ammonia is present, hence the necessity for employing the amount stated. If much less is taken, a brownish-black deposit forms on the anode, and causes loss of nickel if not removed. If noticed, it must be dissolved by interrupting the current and adding more ammonia. If the experiment has been left unattended for the usual period of four hours, the formation of nickelic hydroxide involves prolonging the electrolysis for a further period till all the redissolved nickel is deposited. It is therefore much more satisfactory always to add sufficient ammonia at the beginning. The above-mentioned quantity may be exceeded by several grammes with- out very marked effect, but a greatly increased quantity retards deposi- tion, and may cause an unequal deposit. The quantity of ammonia which is necessary apparently depends chiefly on the strength of current employed, not so much on the amount of nickel present. During the electrolysis ammonia is neutralised at the anode, but with a weak current the partially neutralised liquid is replaced by fresh solution sufficiently rapidly to keep the liquid at the anode alkaline, even although there may not be a great amount of free ammonia present. The current density may vary somewhat, but should not be greatly increased. If that is done, the deposit suffers in quality, being much rougher ; the rate of deposition is increased, principally in the earlier stages. With a weaker current than that stated good deposits are still obtained, but the operation is more prolonged. When the quantity of metal to be deposited is not very great, a current density as low as 0°3 ampére may be employed, but it is advisable to decrease the quantity of ammonia (though not of ammonium sulphate) in that case. With a current density of 0:15 ampere it is not possible to get good deposits, even with small quantities of metal, if the usual quantity of ammonia is employed (7.e. 5 grme.) ; the metal forms irregular patches, and much remains in solution even after prolonged electrolysis. By diminishing the amount of ammonia to 1 grme., or even less, these drawbacks are practically removed. One grme. of free ammonia is sufficient to prevent formation of nickelic hydroxide with the last-mentioned current, even when the quantity of nickel is considerable, say 0:2 grme. For most of the experiments in the latter part of this investigation, using 0-15—0-2 grme. of nickel, a current density of 0°6—0-7 ampére was adopted as generally the most suitable. There is no special advantage in conducting nickel determinations at temperatures higher than the ordinary. Deposition is then somewhat more rapid, but sometimes less regular, and the quality of the deposit is apt to suffer. As such determinations require more frequent attention 304 REPORT—1898. than is the case with cold solutions, it is much more convenient to employ the latter. The time stated is sufficient for all ordinary quantities of metal under the other conditions given. For small quantities it may be curtailed somewhat, but it is preferable rather to reduce the current and the pro- portion of ammonia. Even when the quantity of metal is considerable, the great bulk of it is deposited in a relatively short time, and it is the removal of the last portions which prolongs the duration of the ex- periment. In connection with the electrolysis of nickel sulphate solutions, the formation of nickel sulphide has sometimes been noted, becoming evident when the deposit is dissolved in dilute hydrochloric acid, as a slight black insoluble residue. Though this was observed in several experiments, it was not possible to fix the particular conditions which determine it. Apparently it is not formed to any appreciable extent under the general working conditions specified above. Where it is possible to select the quantity of metal to be used in a determination 0°15 to 0-2 grme. will be found to be very convenient. For many purposes, however, the quantity available may be much less than that. In dealing with small quantities there is no need to employ the ordinary large electrolytic basins unless a large volume of solution cannot well be avoided. Very good determinations can be carried out in ordinary platinum crucibles. In that case the quantity of ammonium sulphate and of ammonia should bear the same proportion to the volume of the solution as when the ordinary apparatus is employed. With a crucible holding about 20 c¢.c. of solution that would mean barely one gramme of ammonia and of ammonium sulphate, while the current to correspond would be about 0°15 ampére. It has been found that in this way deposi- tion is more rapid than when working with a large volume of solution containing the same quantities of metal and ammonia, and with the same actual current (not same current density). When working on a small scale with small quantities of metal, there is, of course, less liability to accidental errors, owing to the more compact nature of the deposit, and the greatly diminished size of the vessel to be handled. Numerous experiments have been carried out in order to determine the influence which may be exerted by other substances present in the solution during electrolysis; partly to discover if any are decidedly beneficial, but chiefly to find out those which are distinctly objectionable. Potassium or sodium sulphate cannot be employed in place of the ammonium salt without very considerably lowering the character of the resulting deposits ; they are invariably dark and rough, but with care the numerical results are hardly, if at all, affected. The presence of these salts, however, is not of itself harmful, for perfectly good deposits can be obtained by employing ammonium sulphate along with them in the usual manner. Until recently it was quite generally stated that the presence of chlorides in the solution was objectionable, but this has been contradicted by F. Oettel,! and the present experiments fully confirm his result. Ammonium chloride may be added in considerable quantity along with the sulphate, or it may be employed in place of it ; the resulting deposits and the numerical results obtained are in all cases excellent. There is a pcint to ' Zeits. Electrochem., 1894, p. 194. ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 305 be noted, however. In several experiments with chloride present it was found that there was deposition of nickelic hydroxide on the anode, although the normal quantity of ammonia was employed. This is pro- bably due to the destruction of ammonia at the anode in this case, over and above that lost by neutralisation. If the discharged chlor-ions act like free chlorine, we can compare the action with sulphate and with chloride, as represented by the equations 12NH, + 680, +6H,O=6(NH,),8O, +30, 16NH, +12Ci=12NH,Cl+2N, Assuming that these are the only actions which take place, it is evident that for the same quantity of current the quantity of free ammonia lost is one-third greater with the chloride. It is therefore advisable in this case to increase the amount of ammonia to 6 to 7 grme., unless a weaker current is employed. In cases where nickel is to be deposited from a solution originally containing chloride only, ammonium chloride might perhaps be employed with advantage in place of ammonium sulphate. The formation of sulphide would then be quite impossible. Nitrates, unless present only in small quantity, should be destroyed previous to electrolysis, as their presence considerably retards the deposi- tion of the metal. This is evident from the much longer time necessary to decolourise the solution. In course of time the nitrate becomes reduced by the current, and the deposit ultimately obtained is perfectly good, being,, in fact, exceptionally lustrous in appearance. The presence of phosphates in the solution is immaterial, provided the precipitation of nickel phosphate is avoided when the ammonia is added. To reduce the risk of precipitation, the ammonia should be added last of all, after the ammonium sulphate and water, and it can be taken that it is all quickly mixed with the liquid. Perfectly good results may also be obtained by using ammonium phosphate alone in place of the sulphate. What has been said of phosphate applies equally to arsenate, a matter of considerable importance in connection with the assay of nickel ores. There is apparently not the slightest reduction to arsenite, which would undergo further reduction to arsenic. The decanted liquid gives no trace of an immediate precipitate on the addition of hydrochloric acid and hydrogen sulphide. The presence of arsenite is wholly inadmissible, as in that case the deposit is quite black, powdery, very loosely coherent, and contains large quantities of arsenic. If it is desired to determine nickel in solutions. containing arsenic compounds, it is therefore necessary either to completely oxidise them or to remove them previous to electrolysis. Chromates have a very marked and striking effect. The presence of a very small quantity completely prevents deposition, even when electrolysis is continued for a long time. When present it would therefore be neces- sary to get rid of them by one of the ordinary methods before proceeding to determine the nickel electrolytically. The addition of sulphites to baths for electroplating with nickel has been recommended, and experiments were tried with varying quantities of ammonium sulphite present in solution. The resulting deposits are exceedingly bright and lustrous, but this seems to be the only advantage. An excessive quantity retards deposition somewhat, so that there is no open benefit attending the use of sulphite for analytical work. This : x 506 \ REPORT—1898., applies also to the employment of borax, which is recommended as a In presence of it deposits of very good appearance are obtained, though not so brilliant as in the case of sulphite, and the results are otherwise quite normal. constituent of some plating baths. Nickel Determinations in Nickel Ammonium Sulphate. | | go | = Wei ght Reagents Volume Current BALE | Temp No. | taken, | 20ded in Isqintion| © Pio | “Votts' | °C Grammes | Ampere | c Grme. C.C. 1 1°0701 | 5 Am,SO, 130 0°7-0°6 | 3°3-3°8 | 13-20 5 Amm. 2 2°7372 =3 x 0°8-0°7 | 3°1-3°3 | 12-20 3 5°4462 4 » | | O7-0°6 | 3°1-3°4 | 14-20 4 0°5300 cs 4 0°7-0°6 | 2°7-3°2 | 13-22 5 01966 oa | oo» 0°6-0°5 | 3°3-3°5 | 14-21 5a | 01452 es pe 0°7-0°6 | 3°7-3°2 3-22 6 11700 |10Am,S0, 5 0-7-0°6 | 2°9-3°3 | 12-21 ; 5 Amm. 7 1:0134 {15 Am,SO, + 0°7-0°G | 2°9-3°2 | 12-21 5 Amm. 8 11309 | 5 Am,SO, 3 10 | 40 13-27 5 Amm. 9 1:2193 | 5 K,SO, P- 0'7-0°6 | 3°6-4°0 | 12-22 5 Amm. 10 1:3726 | 9 K,SO, a 0'7-0°6 | 5°3-3°7 | 12-20 5 Amm. 11 1:2959 | 5 Am,SO, = 0'7-0°6 | 3°1-3°5 | 14-22 3 K,SO, 5 Amm. 12 1°6255 | 3 Am,SO, 9 0°7-0°6 | 2°8-3°5 | 13-20 2 AmCl 5 Amm., 13 1:1033 | 5 AmCl 0°7-0'6 | 2°9-3°6 | 12-21 5 Amm 1, later 14 0:9420 | 6 Am,SO, » 07 3°2-3°4 | 11-22 1 KNO, 5 Amm. 15 10116 | 5 Am,SO, 140 0°7-0°6 | 35-4 13-22 2 Am,HPO,! 5 Amm. 16 10738 | 5Am,HPO,) 130 0°7-0°6 | 3°5-4 11-23 6 Amm. 17 11428 | 3 Am.SO, » 0'7-0°6 | 36-4 12-2. : 2Am.HAsO, 5 Amm, 18 1:3833 | 5 Am,SO, 140 0°8-0°7 | 3°2-3°8 19-30 2Am,HAsO, 5 Amm. 19 1:1365 | 5 Am,SO, 130 0°7-1°0 | 3°6-4°1 | 10-22 5 Amm. 1 Am,S0, 20 1:2097 |10 Am,SO, 5 0°9-1'7 | 3°1-3°7 | 13-23 5 Amm., | 21 11775 | 4 Am.SO, “J O'7-0°6 | 5°4-3°9 | 15-24 2 Na,B,O, 5 Amm 22 1:3827 | 5 Am,SO, i 0°8-0°7 3-3'°3 | 12-22 1 Am,Cr,0, 5 Amm, 23 0°9431 | 5 SO, “S 07-11 3-3°5 | 11-26 0°01 K,CrO, | 5 Amm. | 24 14621 | 5 Am,SO, “g 0°7-0°6 | 3°3-3°8 | 10-22 1MgS0,7H,O | | 5 Amm. | Time. Hours Weight Pe of = Nature of e Deposit. = Deposit Remarks Grme. a 01571 | 14°66 | Very good _ 04018 | 1468 | Good Slight reactio. 0°8002 | 1469 | Rough, E * dark 0°0780 | 14°72 Fair —_— 0:0286 | 14°57 | Very good _ 00210 | 14°46 = Distinct reac- tion O1717 | 14°67 ss — 0°1487 | 14°67 LA _ 01663 | 14:71 | Rough Very slight reaction 01795 | 1472 | Dark, —_ rough 0:2013 | 14°67 | Very dark — & rough 01903 | 14°68 | Very good = 025391 | 1471 | Good — . 01626 | 14°74 | Very good -_ 0:1378 | 14°63 | Very good) Marked reac- tion 01486 | 14°69 | Very good = 0°1580 | 14:71 | Very good - 0°1677 | 14°67 | Very good ~ 0:2032 | 14°69 | Very good ad 0:1671 | 14°70 | Very good) Distinct re- action 01794 | 14°83 | Very good - 01732 | 14:71 | Very good _- 0°0003 _ No metal _ deposited = = - — 02149 | 14°70 | Dull, but | Faint reactio: The employment of various organic salts in the determination of nickel has sometimes been recommended, but, generally speaking, the presence of organic substances in the solution appears to be objectionable, In some | ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS, 307 cases (tartrates or citrates, for example) the resulting deposits are of very good external appearance, but frequently the numerical results are high and the deposits leave a distinct brownish residue when dissolved in dilute acid ; further, the presence of considerable quantities of organic salts may retard deposition. This apparently does not apply to owalates. While, on the whole, the use of organic salts, in dealing with ordinary straight- forward depositions, appears to be attended with no real benefit, but in some cases the reverse, it is quite possible that they may be employed with advantage in certain separations. The influence of salts of the alkali metals when present in the solution has already been discussed. It is sometimes stated that the presence of magnesium salts is objectionable, but this dves not seem to be the case to any considerable extent, when only moderate quantities are present. The deposits obtained in the experiments tried were somewhat rougher than otherwise, and the results a trifle high. The metals of the alkaline earths are of course excluded in presence of _ sulphate. Neither is it possible to determine nickel by deposition from solutions containing these metals by replacing the ammonium sulphate by the chloride. In that case alkaline liquid attracts carbonic anhydride from the air in sufficient quantity to give a distinct deposit of carbonate, so that the results obtained are much too high. The examination of the behaviour of other metallic salts brings us to the question of the electrolytic separation of nickel from other metals, which will not be discussed fully here. It may be stated generally, how- ever, that those metals which yield ammoniacal solutions are deposited electrolytically along with nickel, The most important of these are copper and zinc. The former can be removed by electrolysis in acid solution. The presence of even a relatively small quantity of zinc greatly retards the deposition of nickel, but ultimately both metals are completely removed from solution. Determination of Cobalt. _. The electrolytic estimation of cobalt has apparently not been the subject of so much investigation as that of nickel ; it is generally stated __ to be exactly similar in method to that of nickel, no further instructions _ being given. There is, however, a very considerable difference in the two ~ eases. Good nickel deposits are obtainable with the greatest ease, but _ the reverse is the case with cobalt, and the best conditions for depositing the one are by no means the best for the other. Tf an experiment with cobalt is conducted under the standard con- ditions given for nickel, the metal is not completely precipitated, and a very poor deposit is obtained. Apparently ammonia has a much greater effect in this case than with nickel, prohably due to the formation of stable cobalti-ammonium compounds. On the other hand, the tendency to form cobaltic hydroxide on the anode is not nearly so great, and the quantity of ammonia can be reduced as low as 1-5 grme. Even then, four hours is barely sufficient for complete deposition with moderate quantities of metal, using cold solutions. The best determinations obtained even with small quantities were very much inferior to those of nickel as regards the physical character of the deposit, and an extended series of experiments was carried out in the hope of securing the metal in better condition. These experi- ments varied considerably as regards the composition and proportions of x 2 308 REPORT—1898. the reagents employed, the current density, &c., but they led to no marked improvement. It had been decided to adopt 5 grme. of ammonium sulphate and 1:5 grme. of ammonia to 130 c.c. of liquid as the standard solution, and the influence of other substances present was being investi- gated as in the case of nickel, when, quite unexpectedly, a solution of the problem was indicated. The influence of nitrates was being studied, in the expectation that it would be at least as marked as with nickel, probably more so. This was found to be the case, 1 grme. of ammonium nitrate was sufficient to prevent the decolourisation of the solution even when the current was passed for several hours longer than would other- wise have been necessary. The experiment was continued overnight, and in the morning the solution was found to be quite decolourised, and on decantation proved to be free from cobalt. The deposit was bright and lustrous, much superior to any formerly obtained, but not so white as a good nickel one. Most important of all, the percentage result, which in former cases with complete precipitation varied mostly from 15:05 to 15-10, had in this case fallen to 14°90. Acting on this, experiments were conducted with varying quantities of ammonium nitrate, when it was found that satisfactory results were obtained with only 0°2 grme. of the salt, but that less was not of much benefit. The presence of nitrate of course increases the time necessary for complete deposition, but, if so desired, this can be counteracted by con- ducting the electrolysis at a higher temperature, say about 60°C. A good deposit can still be secured when {hat is done, and the duration of the experiment need not exceed about four hours. If time is no object the electrolysis may still be conducted at the ordinary temperature, and even a larger quantity of ammonium nitrate employed. Assuming that it is desired to keep the time limit fairly low, the following may be taken as standard conditions for quantities of cobalt, from 0:1—0°3 grme., the volume of solution, as usual, being about 130 c.c. Reagents added : 5 grme. of ammonium sulphate, 2 grme. of ammonia, and 0-2 grme. of ammonium nitrate. Current : 0‘5—0°8 ampére per 100 sq. em. of cathode surface ; 3—3°5 volts. Temperature : About 60° C. Time: 4 hours. The deposits obtained under these conditions are generally fairly gocd, but there is not the same regularity of results that is obtainable with nickel. The metal in this case is much more readily altered by various reagents, and greater care is necessary in the treatment of the deposit. As already stated, it is advisable to remove the liquid and wash the basin, in the first instance, by means of siphons without breaking the circuit. As in the case of nickel, an excess of ammonium sulphate is com- ° paratively unimportant, though in some of the earlier experiments, conducted at ordinary temperature without nitrate, it seemed as if the last traces were more difficult to remove in presence of much of this salt. The amount of ammonia is more important here than in the case of nickel, as already indicated, the latter metal being apparently less liable to attack by ammoniacal solutions than cobalt. The proportion of ammonia should therefore be kept as low as possible, not only because the necessary time is thereby diminished, but also because better and more regular i i a> %> { ” . ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS, 309 deposits are secured. The quantity stated above is greater than that formerly mentioned, because there is a greater loss with warm solutions than at the ordinary temperature. The temperature should not be allowed to rise too high, otherwise ixregular deposits may result, and there may be excessive loss of ammonia. A very small flame is sufficient to keep the liquid warm enough. Tn dealing with small quantities the remarks made with reference to nickel apply with greater force here ; for accurate results the quantity of ammonia and strength of current should both be moderated, or the whole experiment carried out on a reduced scale. Thus, it was found that a certain volume of cobalt solution which gave 0:0612 grme. of cobalt when electrolysed in a large basin in the usual way, gave only 0:0601 grme. in a simultaneous determination carried out on a reduced scale in a platinum erucible ; although deposition was quite complete in the latter case, the result is decidedly lower, and this is explained by the fact that the deposit was entirely soluble in hydrochloric acid while the former left a slight black residue. A similar pair of experiments at another time gave 0-0603 and 0:0595 grme. respectively, again showing an advantage in favour of the crucible experiment. The influence of other substances present in the solution is in many cases similar on the whole to what was found to be the case with nickel. There are, however, some exceptions to be noted in this respect. In the early cobalt experiments without nitrate, ammonium chloride was occasionally tried in place of sulphate, and the results thus obtained seemed generally superior. One of the best results obtained was got by employing 10 grme. of ammonium chloride and 2°@rme. of ammonia. It was found, however, that solutions containing both chloride and nitrate were rather erratic in their behaviour, sometimes giving very poor and irregular deposits. It is also more difficult to regulate the quantity of ammonia in such cases. If it is desired to determine cobalt in a solution containing ammonium chloride, it would appear preferable to conduct the electrolysis without the addition of ammonium nitrate. The most striking difference from nickel is shown when cobalt solutions are electrolysed in presence of arseniate. We have seen that the presence of ammonium arseniate in large quantity has no effect on the nickel deposit. This is far from being the case with cobalt. Deposition is re- tarded, the deposit is very dark and rough, and the numerical result is far too high. The deposit contains a large quantity of arsenic, but the ' solution is apparently free from arsenite. Metallic cobalt would appear to be readily attacked by ammoniacal arseniate solution, which is pro- bably reduced to arsenite. But any arsenite formed would be promptly reduced electrolytically to arsenic, which would contaminate the deposit. Another point which shows how unsafe it is to assume that what holds for nickel does so also for cobalt is the behaviour in presence of zine salts. This comes into the domain of separations, but it may be mentioned here. With small quantities of zinc in presence of nickel, the deposit obtained by the usual method contains the whole of both metals, as already noted. In the case of cobalt a solution containing zinc gives on electrolysis by the ordinary method a deposit which is not very good in appearance, but is practically normal as regards numerical result. The decanted liquid gives a pure white precipitate of zinc sulphide on the addition of hydrogen sulphide. To what extent, if at all, this difference depends on the some- ao ew 310 REPORT—1898. what different conditions prevailing in the two kinds of experiments has not yet been investigated. Chromates completely prevent precipitation as with nickel. With some oryanic salts, tartrates for example, the deposits are of very goo appearance, but the results are apt to be too high, as in the case of nickel. Cobalt Determinations in Cobalt Ammonium Sulphate. Weight is Volume! ,_.. of Salt ae ae of jeecereent i.M.F.| Temp. |Time.| of Per | Nature of Remark tiken. | © G ee Solution Ampere| Volts °C. |Hours| Deposit.| Cent. | Deposit StS Grme, yee C.C, ele Grme. | 1:2740 | 5 Am,SO, 139 | 0°68 38 13-25 4} 01905 | 14°95 | Dark and! Very distinct 5 Amm, | irregular reaction 1°3660 “9 » | 0'°5-0°7 | 3°7-4°0 = Fe 0:2013 | 14°74 | Bad, black! Very marked | | / reaction 0°5344 ee re Leo es +) hy 0:0775 | 14°50 =4 5 | 12264 | 5 Am,SO, a 0-7-0'°6 3°83 a 4 01838 | 14°99 | Poor Slight reac- 2 Amm. 0°8845 |10 Am.SO, = rie I o'd, 55 7 01327 | 15:00 3 2 Amm. 13488 |10 Am,SO, ny 0°75-0°'7 3°7-3-4 | 13-30 5 01847 | 13°69 \ 6 Amm. 14139 | 5 Am,SO, ef 0°8-0°7 39 11-27 4 02129 | 15°06 | Fair 1 Amm. | reaction 0°4 ,, later 10189 | 5 Am,SO, o 13 5-4:2 15-45 3h 01526 | 14°98 |Dark,poor) Distinet re- 5 Ainm. } action 15960 | 5Am,HPO, » 0°8-0'7 | 4-3°7 17-40 4 02102 | 15°05 | Poor Very distinet 2 Amm. reaction 10027 (10 AmC1 4 0°8-0°85 3°3 15-30 ” 01501 | 14°97 | Fair No reaction 2 Amm. | 13011 | 5 Am,SO, » | O7-O0°6 | 31-34 | 45-55 32 071963 | 15°09 | Dark rs 15 Amm 19674 | 5 Am.SO, 7: § 3-3°6 | 45-50 2 02950 | 15°00 3 15 Amm. | 11169 | 5 Am.SO, ” 0:7-S°68| 35-4 | 16-30 | 24 01664 | 14:90 | Very good 15 Amm | / 1:0 AmNO, | 14069 | 5 Am,SO, » | 9°75-0°7 | 3°1-3°5 | 60-80 4 02092 | 14°87 es 2 Amm. | 0-2 AmNO, | ) | 11443 | 5 Am,SO, » | 07-06 | 36-4 16-30 | 53% | 0°1707 | 1492 | Dark 2 Amm., | | 0'1 AmNO 13728 | 5 Am.S0, » | 0°850°6 34 60-70 4 02053 | 14°95 | Good, 2 Amm. rough 0-2 AmNO, | 0°3682 a és a a * . 0:0554 | 15°05 | Very good 1:0001 nr * 072 | 31-33 | 50-60 a 01503 | 15°03 | Fairly | good 1:0001 AS *s 0°7-0°6 | 3°0-3°4 “5 ct, ‘01497 | 14:97 | Good > 3°0207 5 a 0°65 31 60 44 04535 | 15°01 | Fair Deposit not all soluble’ 04028 tB5 24 0°6-0°7 | 3°2-3°5 | 60-70 | 33 0:0612 | 15°19 = co 0°4028 | 08 Am,SO,} 19 O'7-0°5 32 50 es 0-0601 | 14°92 a Deposit all 0-4 Amm. soluble 0:03 AmNO,, | 10001 | 5 Am.SO, 130 06 a 40-60 4 0°1691 _ a Partly inso- 2 Amm. 0-2 AmNO,, 2Am,HAsO, 1:0001 |5Am,HAsO,) , | 4, 31 50-65 y 01723 — Black and | 2 Amm. / spongy 10001 | 5 Am,SO, ee es 2:8-3'1 | 60-70 4} 0°1511 | 15°11 | Fairly Left — slight 2 Amm. good residue 0:2 AmNO, 2MgS0O,7H,O Other Electrolytic Methods, As already stated, the great majority of the experiments so far carried out have dealt with the ammonium sulphate and ammonia method, as it . ON THE ELECTROLYTIC METHODS OF QUANTITATIVE ANALYSIS. 311 seems on the whole preferable for ordinary simple determinations. The further investigation of other methods will be conducted more from the point of view of their application to special cases, such as separations. The tabulated experiments given in this paper are only a small portion of those obtained, as experiments were often repeated under similar or slightly varying conditions, so that general opinions might be more con- fidently formed. In the case of cobalt especially the total number of experiments was considerable, owing to the much greater difficulty of obtaining deposits which were really satisfactory. The selection has not been made so as simply to give a series of the most concordant results, but may be taken as fairly representative. In conclusion, I have to express my indebtedness to my brother, Mr. Ralph Marshall, for assistance in carrying out the routine work of numerous experiments during the latter part of the investigation. Tsomeric Naphthalene Derivatives.—Report of the Committee, consisting of Professor W. A. TILDEN (Chairman) and Dr. H. E. ArM- STRONG (Secretary). ALTHOUGH it is established that when betanaphthol is acted on by bromine, at first bromine enters the hydroxylated nucleus in position 1, and in the second place the non-hydroxylated ring in position 3’, the structure of tribromonaphthol remains undetermined ; but it is certain that the third bromine atom is introduced either into position 3 or into position 4, as both these are occupied in tetrabromonaphthol. Considerable difficulty has been experienced in settling this point. Meanwhile, in extending the inquiry, in order to obtain complete infor- mation of the influence on substitution exercised by the OH group in betanaphtnol, the discovery has been made that the two possible homo- nucleal forms of tribromonaphthol are both produced when betanaphthol is acted upon by three molecular proportions of bromine. The crude product cannot be directly purified, but by converting it into acetate and repeatedly extracting this with boiling acetone, about half is dissolved ; the residue almost entirely consists of the acetate, of the tribromobeta- naphthol already described by Armstrong and Rossiter. A further quantity of this acetate is obtained by fractionally crystallising the solu- tion, and also about 15 to 20 per cent. of the acetate of a new tribromo- betanaphthol. Although the two isomerides resemble each other very closely, and cannot be directly separated, their derivatives differ consider- ably ; thus— A. and R. New fe} fe) Tribromobetanaphthol . : : F : - mp. 155 159 re a acetate > A f 4 seep 149 as benzoate » 187 164 Nitrodibromobetanaphthol he lo6 163 Dibromobetanaphthaquinone . plod) 187 The comparative investigation of the dibromonaphthoquinones ob- tained from the tribromonaphthols and other sources is being undertaken with the object of determining their constitution and that of the naphthol derivatives from which they are prepared. That melting at 171°, obtained 7 3812 REPORT—1898, as the principal product of the action of nitric acid on dibromobeta- naphthol, is converted by alkali into a dibromohydroxyalphanaphtho- quinone, and therefore does not contain a bromine atom in position 4. As the dibromoquinone melting at 150°, obtained from the tribromo- naphthol melting at 155°, is converted by alkali into a condensation product, it appears probable that the tribromonaphthol from which it is derived is the 1; 2:4: 3’ compound. The writer is indebted to Mr. W. A. Davis for carrying out these experiments. Mr. Davis has obtained interesting results by comparatively studying the amounts of ether formed on boiling the various naphthol derivatives with alcohol and sulphuric acid. Whilst betanaphthol gives as much as 85 per cent. of the amount of ether indicated by theory, 1 bromobeta- naphthol yields only about 10 per cent., and an even smaller proportion is obtained from 1 : 3’ dibromobetanaphthol, although 3’ bromobetanaphthol yields about 70 per cent. of the theoretical amount of ether. 61 21941°8 455604 1 ‘is 55 21942'8 4554-20 1 Ba 455416 ,, , an 21951-7 4552-72 In 4552°66 ,, . eS 219588 4549-65 3 4549'57 ,, » “a 21973°6 4548-00 2 454795 ,, a a 21981°6 4541°68 1 454143 ,, 1:24 a 22012°2 4531°32 2 4531:25 ,, 5 ea 220625 4529°80 In 452975 ,, mn 8 22069°9 (4528°80) 6 452878 ,, 28:80R. i 7 22074'8 4525°31 2 4525°27 ,, a5 3 22091°'8 314 REPORT—1898. ITRON—continued. Wave- Reduction to length Intensity Vacuum ees) Spee oat Cl and Previous Observations |~ Getoion naracter 1 brequency AS —— in Vacuo 4522°80 2 29-79 K.& 4520-41 1 aot ana 126.| 61 221041 4517°68 1 451764 ld ” ” 22115'8 451549 if 4515°36 “2 ” ” ’ 22129°2 451431 1 4514-29 » ” ” 22139°9 4494-74 2 4508-40, eee 221748 494°74 5 ee a ie ” 7 D 8 4491:58 1 areite » 94725 KR. | 12:3 6:2 22242-0 4490°24 1 4490-19 a? ” ” 22260°9 . 4489-88 1 448984 2h 7 ” ” 22264°3 4489'34 In 4489-08 |, SP her = ” 222661 4488°3 1b 4488-26 ” ” 22268°8 4485:82 1 4485-77 a ” ” 22274 4484-40 2 4484-36 4 Hg Tas ” 22286°3 4482°94 1 4489-86 i ” ” 22293'3 4482-40* 4 4482-35 ¥ ” ” 22300°6 4480°31 i 4480°26 PS | ” ” 22303°3 4479°76 1 4479°73 » ” ” 22313°7 4476-19 5 4476-20 24 ” ” 22316°4 4469°54 2 4469-53 ” ” ” 22334-2 4466:70 5 4466°70 oe. edi ” 22367°5 4464-91 1 Sacaca 122 | ,, 22381-7 4462-15 ln 4462/11 an ” ” 22390°7 . 4461-80 3 4461-75 9 ” ” 22404°5 4459-28 4 4459-24 te ” ” 22406°3 4458-22 In 445835 ” » 22418'9 4456-46 1 4456-46 ” ” ” 224243 4454-89 1 22 ” ” 22433:1 4454-53 2 x ” ” 22441°0 4451-70 ele (eee mS 2449-9 4450-46 1 4450°44 22 ”? ” pre (4447-90 3 QF 4 . ” 9 22463°4 ance 3 ee » 47°90 R. a iS 224763 4443-00 ii 4442-97 a3 ” ” 22499°3 4442-51 4 4442-46 | |» ” 225011 4440-05 1 4439-96 oa ae 22503°6 4438°50 il 4438°50 4 ” ” 22516°1 4437-06 1 4487-04 od ” ” 22523'9 4435°31 yt 443527 # ” 9 22531:2 4435°20 1 a” ” » 225401 4433-97 1 4433-98 ” ” 22540°7 4433°39 2 443332 ” » 22547-0 4432-73 4432-68 = ” ” 22549°9 4430°79 D 4430°74 Re, eH ” 22553°3 4430°35 1 443032 121 | 63 22563-0 4427-49 3 4497-44 » ” ” 22565°3 4424-6 lb 4424-96 a ” ” 225799 4422-74 3 4499-67 ” ” 22595 4419:93 1 ih ay ” a) 226041 4419-70 1 } » ” 22618°5 4415-98 1 ” ” Ree 4415-29 8 Moc 9 ” 26387 4413-70 1 ge elt ee 22642'3 44109 lb | ” ” 22650°4 ” ” 22664'8 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 315 TroN—continued. Wine piction to length Intensity see Oscillation Spark and Previous Observations Frequency Spectrum Character Pe hi in Vacuo A 4409°44 1 1-21 | 63 22672°3 4409°34 1 4409°25 K.& R. f <5 22672°8 4408°59 2 440854 a sy 8 22676°7 4407°89 2 *4407-80 fee BASED pass ” 22680°5 4405°65 1 per kee 22691°8 440494 10 440488 K.& R. ys oF 22695°5 440160 1 5 34 22712°7 4401-50 a 4401-46, 1 ee 22713'2 4400°55 In ist Mie bs 22718°1 4396°88 in | 49 ” 227371 4392-50 in | 1.20 cs 22759°8 439115 1 *4391-152 R. 4 A 22766°8 4389°4 In 438935 K. & R. ‘s * 22776 4388°61 2 4388°57 ff * As 22780°0 4388°07 2 438801 zs $s s 22782'8 4385°55 1 438540, i x 22795°9 4384°39 2 4384:38 rs “ 22801°9 4383-71 10 4383°70 . 53 22805°4 4382-96 1 ” ” 22809°3 4379:40 In 437936 _s,, * A 22827°9 437696 In 437689 % 1:20 | 63 22840°6 4376710 4 437604 9 sr LOZ S;, a 22845:1 437467 1 437459 K. & * % 22852°6 4373°74 1 4373°67 "3 “ a 22857°4 4370°52 1 4370°59 ,, 3 A 228742 4369°96 3 4369-89 GAGA es, Ph 22877°2 4368°11 1 4368:00 cs f 6:4 22886'8 4367°75 2 4367°68 x + 8 22888°7 436613 in 436602 __,, a 5 22897°2 4361°5 In 2 5 22921 4361:0 in 2 a 22924 4358-68 1 435862 r Sp 22936°3 4357°73 In 38 22941°3 (4352-90) 3 4352°86 » PLORAe1S Fs 22966°8 4351°89 2 4351°67 ” if “+ 2297271 4346°63 1 434666 7 % 5 22999°9 4343-80 1 4343°81 xz , 5 230149 4343°37 1 4343°39 ,, es A) 23017°2 4338°89 1 Bs 35 23041:0 4338°39 1 4338°38 A! o ar 23043°6 4337-22 5 4337:14 ” ” 23049°8 4334-55 1 5 * 230640 4330°35 In s i 23086°4 4330°15 In 5 “P 23087°5 4328:02 1 432802 9 45 rp 230989 4327:22 2 4327°22 ss, a a 23103°1 432687 1 432686 ,, ay 3 23105°0 4326°50 1 0 a 23107°0 4325-94 10 $4325°92 so Oa) Ets, 33 23110°0 4321-93 1. 4321-90 3 “A Pe 23131°4 4321°67 1 x - 23132°8 4321-55 i a 3 23133°4 4320°92 1 4320°89 7 + e 23136'8 * Double. { Triple. 316 Wave- length Spark Spectrum Intensity and Character 4318-75 4315:26 4314-46 4312°88 4312-48 4312°31 4309°51 4309°16 4308-70 4308°06 430559 4304-76 430332 4302-67 4302°32 430094 4299-43 4298-17 4296°73 4295°12 4294-32 4292°4 4291°62 4291:05 4290°55 4290:08 4289-47 4289-0 428827 4287-10 4286'55 4285 56 428313 4282°60 4280:00 4279°65 427833 4277-6 427680 4276:27 4276-11 427402 4273-42 4272°53 4271-93 4271°32 4269:90 4269-78 4268°86 4267°95 4267-68 4267°56 4267-08 La] i=] Ste veep, Peer gita kn eaters Soe Seer, ee a In on bet) oH 1 ll el hl lll de REPORT—1898. Tron—continued. Previous Observations Reduction to” Vacuum A nN 4315°21 4314-43 4312-28 4309-50 4309714 G 4307-96 4305°58 430466 4303°25 4302°68 4302°31 4300°86 4299-42 4298-16 4296°56 4295:08 4294°26 4292-36 4291-69 4290°99 4290°50 4290°04 4289-84 4289:08 4288:25 4287:05 4286°58 4285°57 4283°20 4282-58 4279:99 427959 4278°35 4276°80 427399 4272°61 4271:93 4271°30 4269-89 426887 *4267-97 4267-08 4318°78 K. & R. » ‘941 KR. * Double. 6-4 Oscillation Frequency in Vacuo 23148°5 23167°2 231715 231800 231821 23182°4 23198°1 23200°0 23202°4 23205°8 23219°1 23223°6 23231°4 23234'9 23236°8 23244'2 23252°4 23259°2 23267:0 232757 232801 23290 232947 232978" 23300'5 23303°1 23306°4 23309 233129 233193 23322'3 233277 23340°9 23343°8 233580 23359°9 233671 23371 23375°5 23378'4 23379°2 23390°7 233940 23398'8 23402°1 23405°5 234132 23413'9 23419°0 23424-0 23425°4 234261 23428°7 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave length Spark Spectrum Intensity and Character 4265°35 4264-85 4264-34 4260°64 4259-07 4258°76 4258°40 4256°40 4255°61 4255:25 425506 4254-45 4251-55 4250°95 (4250°30) 4248-37 424758 4246-14 4245°32 4943'45 4249-82 4240°46 4239:88 4238-90 4238°10 4237-22 4236-09 4233-74 4233-26 4931-9 4229'83 4229:58 4227-60 4226'88 4226:53 4226-06 4225-57 4994-63 4224-26 4223'30 4992-35 4220-46 4219:51 4217-67 4216-29 4215-56 4213-77 4210°52 4208-73 4207-26 4206'84. 4206°33 4205°69 4204-10 4202'86 In ln 1 10 i 1 i 6 B RP ROO NRWRE RP RWW PRE QOH Be eee o Q & Fe a SORT NIRS IAD ICD ROI HNC a 0 tote Ait > IRoN—continued. Reduction to Vacuum Previous Measurements A+ ae. A 4265°37 K. & R. LAT } 6:5 426488 » ” 426437 ,, 9 te 426064 v7 1% + 4259°06 = * is 495875, al ae 4258-43, ee 4256°32 = Pill ieee, 4255°64 % " PS ” ” 4255:08 . fr = 4254:45 jah), (LOOMER I ys = S 6-6 4250:93 = % * 4250:°28 > = & 4248°35 ee s & 424760. ,, a r 4246-18 ¥ is is 4245°39 ‘ ae -, 4243°44 _ 1:16 * 4242°85 wv = . 4240°50 Ps bs & 4239°90 pe 45 > 4238°98 . is eS 4238°14 ra i. x 4237-26 fe Wass a 4236°09 - a fe 4233°76 a ih x 423325 os + s 4229°86 ~ a . 4229°61 es = a 4227-60 5 a % 4226°84 - he P 4226°52 ss * * 4226:08 “a “ ie 4225°61 a * - 422463 x ¥ if 4224:27 a Rs S 4223°40 * + B 4222°35 ee 2 * 4220°44 7 Es es 4219-47 aS % - 4217°69 a + 7 4216:28 - * a 4215:52 e 1:16 - 4213°75 3 x < 4210-48 * Ra 2 420871 pe % 3 4207:22 as ee a 4206°78 <5 RS a 4205°63 es 115 2 4204-07 a "3 he 4202°85 > ‘ = Oscillation Frequency in Vacuo 234382 23441:0 23443°8 234642 23472°8 23474°5 23476°5 23487°5 23491:9 23493'9 234949 23498°3 235142 23517°6 235212 23431°8 235362 23544-2 23548°8 23559°1 23562°6 23575 7 23579:0 23584°4 23588°9 23593°8 236001 236132 236159 23623 23635:0 23636°4 23647°5 23651°5 23653°5 236561 236588 236641 23666-2 23671°6 256769 23687°5 23692°8 23703'2 23710°9 237150 237251 237434 23753°5 23761-8 237642 23767-1 23770°7 237797 23786-7 ol? 318 REPORT—1898. Tron—continued. Wave- length Spark Spectrum 4202-20 4201-07 4200°13 4199-27 4198-86 4198-50 4196-46 4195-75 4195-50 4191-80 4191°61 4188-00 4187-22 4185-03 4182:54 4181-94 4179-01 4178°16 4177-74 4176-70 4175°77 4175:06 4174-10 4173:59 4172:88 4172-29 4171:80 4171-05 4168-07 4165°57 41638 4161-63 4161-2 4158-94 (4157:95) 4156-93 4164-92 4154-61 415410 4152°32 4150:40 4149-49 4147°79 4145-68 4145-45 4144-62 4144-06 4143-54 4142-01 4140-02 4139-85 4137-12 4136-68 4136°31 4134°83 Intensity and Character | Previous Observations Reduction to Vacuum i=) RP WE WNNDE ERNE ED NNER Rw Wen OHDHN so 4202°15 K. 4201-01 420001 4199°19 4198-75 4198-42 4196°66 4195-71 4195-46 4191:72 4191°57 4187°92 4187:17 4184:99 4182:46 4181°85 417895 417811 4177°66 4176-62 417571 4174:98 4174:00 4173°52 4172°81 4172-20 4171-79 4170:99 416796 4165:51 4163°74 4161°57 416113 4158-89 4157-91 4156°88 4154-95 4154:57 4154-04 4152:25 4150°42 4149-44 4147-74 4145-29 4144-72 4143°96 4143°50 4141°94 413996 4137-06 4136°58 4134-77 054 R. 936 R. Oscillation Frequency in Vacuo 23790°5 23796°9 23802'1 23807:0 23809°3 23811°3 23822°9 23826°9 23828°4 23849°4 23850°5 23871°1 23875°5 23888-0 23902:2 23905°6 23922°4 23927°3 23929°7 23935°6 239410 23945°1 23950°6 ‘ 23953°5 23957°6 23961°0 23963°8 239681 23985'2 23999°6 24010 24022°3 24025 24037°9 24043°6 24049°5 24061°2 240629 240659 24076°2 240874 24092°6 24102°4 241147 24116-0 24120°9 24124:1 24127°2 24136°1 24147-7 24148°7 241646 241672 24169'3 24178°0 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave- length Spark Spectrum 4134-54 4134-03 4133-73 4133-05 (4132-24) 4128°89 4127-92 4127-74 4126:35 4126-05 4125-78 4123-90 4122-69 4121-99 4120°37 4118-72 4115:1 411461 4113-14 4109-99 4109-23 4107°65 4106-60 410640 4104-32 4101:73 4101°45 4100-92 4100:37 4098-37 4096'85 4096'16 4092'5 4091-76 4091-2 4090:2 4089-40 4088°73 4088°15 4087-26 4085:50 4085'16 408460 4083-96 4083-72 4082-60 4082-28 4081°47 4081:02 4080°40 4080°02 407852 4077°85 407681 Intensity and Character Mme OOR RR Ee BB i=} Io et at rat a Het 29 ISH BD BO BO et BD GH BOB B BB ears Roe eit pp te wn wee H fF TRoN—continued. 319 | Reduction to Vacuum yo as Previous Observations |- Tee Aa Bow in Vacuo A 413450 K. & R. 114 6°8 24179'7 4133°96 ‘9 aa - 24182°7 4133°67 oc a * 24184°4 4132°96 3 * f 24188°4 4132715 a * “ 241932 4128°91 +7 1:13 #3 24212°8 4127°86 9 ™ r 24218°5 4127°68 5 i i 24219°5 4126°25 i . = 24227°7 412594 3 - ~ 24229°5 412571 Fe * . 24231:0 4123°81 a ; 3 242421 4122°59 i * # 24249-2 4121°88 # Ap PH 242533 4120°28 95 a » 242629 4118-62 Ef a 5 24272°6 4114°98 *H a - 24294 4114:53 ye) Oa eEelan hy A 24296°'8 411308 9 » FA 24305°5 4109°88 rf ; 5 24324-2 ~ 4109°23 o ,, 3 24328°7 4107°58 $34 (OSGIEV LOO,» 5 24338:0 4106°55 fs RE; is 24344:2 4106°37 Pe a # 24345°4 4104:20 PH Lb P 24357°8 4101:76 op 5 # 24372°9 4101°37 3 My Fr) 24374:'8 4100°82 A s Fe 243780 4100°26 3 :, # 243812 4098:26 3 3 6:9 243930 4096°67 a oa 7 24402:1 4096-06 a ty 4 244062 4092-43 = 1:12 ie 24428 4091:66 or 3 a 24432°5 4091°12 - - 24436 4090717 a % 3 24442 4089:°28 Fr 3 #8 24446°6 4088°65 os D a 24450°6 4087°95 cf a a 244540 4087°16 3 ‘ a 24459-4 4085°38 FA e Ps 24469°9 4085:07 3 :, Pe 24471°9 408459 a . an 24475'3 4083°90 3 3 a 24479'1 4083°70 if } ms 24480°6 4082°55 Pe A Pe 24487°3 4082°20 a :; A 24489°2 4081°67 ’ (ences) Ay hae 24494-1 4080:°96 7s * % 24496°8 4080-30 mf 4 is 24500°5 4079°91 - ‘, An 24502°8 4078-41 nA ‘. a 245118 4077-74 pe + 3 24515'8 4076°72 of 245221 320 REPORT—1898. Iron—continued. ae Ree to TE * acuum rate Pow Previous Observations Spectrum | Character nash ee A 4074:97 3 407487 K. & R. 112 6:9 4073°97 2 4073°84 4) SOLS MREE rs} 4071-92 10 407179, » | oo 4070-96 2 4070°85 ,, Bede 4068715 3 4068:07 ” | ” | ” 4067°77 1 ” ” 4067-45 2 4067°36 ” ” ” 406712 3 4067-04 ” | 49 ” 4066°77 1 4066°66 ” ” | ” 4065:57 1 406548 aay ne 406461 1 4064°55 ” | ”» | ” 4064°35 i 4064°55 ” ” | ” 4063°75 10 4063°63 » » | » (4062-60) 3 406251, ope tae 406213 In 406200, » | 9 4061°3 1b 4061:24 » ” ys 4059°89 1 4059-80 ” ” ” 4059°75 1 ” ” Or. f 4058-99 405893 1 | 4058°86 ” ” ” 4058°40 1 4058°30 » ” ” 4057°55 1 4057-43 ” ” ” 4055°58 1 4055'63 fe - 5 4055712 In 405512 » ” ” 4054°95 in 4054°94 “5 1-11 33 4054:00 in 4054:25 ” ” ” 4053°37 In 405331 ” ” ” 4052'8 1n 405275 ss, pt Nera 4052°6 In 4052°56 Bs By iy | tise 405212 In 4052°03 ” ” ” 4051°52 In 4051°40 +h “A + 4050°86 In 4050°83 5 + 70 4050:02 2 4049:92 + + rr 4049°50 1 4049°40 ” ” ” 4049-03 In 404882 , ‘S75Ri , a 4047'46 1 4047°40 ” ” ” 4045°98 10 4045-90 + 3 os 404479 2 4044°69 »” ” ” 4044-08 2 4044-00 » » ” 4042:00 2 4041°44 ”? ” ” 4040°86 2 4040°74 as ° = 4038°95 In 4038°83 ” ” ” 403465 1 4034'59 “ + “ 4033'82 1 ”» ” 4033°24 1 4033716 ” ” ” 4032°80 2 4032°72 7 ” ” 4032°14 2 4032°06 ” ” ” 4030:89 2n 4030°84 +" oF = 4030°69 2 4030°60 ” ” ” 4030°37 1 4030°26 ” ” ” 4029'80 2 4029°72 ” ” 4025°99 1 4025-93 » ” ” 4024:°94 2 402486 ” ” ” 4024°26 1 4024 20 + Le oF 4022-05 3 4022°25 oP Oscillation Frequency in Vacuo 24533'2 24539°2 24551°5 24557°3 24574°3 245766 24578°5 24580°5 24582°6 24589'9 245957 24597°3 24600'9 24607'9 24610°7 24616 246243 24626°2 24630'1 24633-4 24638°5 246505 24653°3 24654°3 2466071 246639 24667-0 24669-0 24671°5 24674'8 246791 24684-2 24687°4 24690°3 24699'9 24708-9 247162 24720°5 247332 24740:2 24751:9 24778-3 24783-4 24787-0 24789°7 24793-7 | 24801-4 24802°6 94804-6 248081 i] 24831°6 24838°1 24842°3 24855°9 —_ Wave- ength Spark Spectrum 401842 4017-29 4016-57 401470 4013-96 4011°50 (4009:86) 4009°37 4008-95 4007°41 4006'79 4006-47 4005-94 400540 © 400305 4003-91 4002-75 4002-20 4001-80 4001:49 4001'37 4000°60 4000°35 3998°16 3997°52 3997°10 3996-11 399422 3990'50 3990:00 398629 3985°48 3984:09 3982°35 398190 3977-89 3976:97 3976°72 3973°75 3972°55 3971-47 3970-51 3969°40 396858 396810 3967°58 3966°75 3966°20 396466 3963-25 3961:30 3960°40 3957°15 3956°82 3956'58 1898. Intensity and Character Reet beet et G0 Be ae pce ee ee Eo rete Gath A et HR, Heh BB Meow wr oar ts Q OR eee eSB ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 321 TrRoN—continued. Reduction to Caprg Oscillation Previous Observations Frequency x Li in Vacuo A 4018:36 K. & R. peistn | 70 24878°4 4017°23 - Pirds ” 24885°4 4016°55 5 HORS 5 oe 24889°9 4014-63 s | 1:10 ” 24901°5 401391 a % 3 24906'1L 401149 3 PA 24921:9 4009°80 ” ” ” 249315 ” ” 24934'6 4008:97 Pe me ” 24937°2 4007°36 ee i ” 24946°8 4006 71 is as ” 24950°6 4006°39 ” ” ” 24952°6 ” ” 24955'9 400533 Pe i ” 24959°3 4005:07 #3 3 ” 24961°5 4003°88 e Sie + eee, 24968°6 4002°77 9 3 T1 249757 F ” 24979°2 4001 77 a + 7 24981°7 ” ” 24983°6 ” ” 249843 4000°57 PA Ys ” 24989°2 4000°36 x6, » ” 24990°7 399816 ty) 9 op 25004:4 3997°49 Fr} af Fr 25008°4 3997:06 s 9 A 25011:0 3996:08 ” | ” ” 25017°2 3994:22 3 o ne 25029°0 3990°48 - “A bs 250524 3989-94 = a a 25055-°6 3986°27 3 wee 7 25078°9 398546 i ieee. a 25084:0 *3984:08 i OGTR, - 25092°7 - Pe 25103°7 3981°87 * iy 3 25106°5 3977°83 Pe zy rE 251319 3976°95 5 45 on 25137-7 3976°71 3 is * 25139°3 3973-75 109 | 3 251580 i re 251656 3971°41 + - ap 251725 3970°51 a 3 " 251786 3969°34 + a on 25185°6 396855 i - 25190°8 396805 - Be Pr 25193°9 3967°51 3 6 oe 251972 3966°70 * 59 * 25202°5 396616 - 59 Pe 252060 3964°61 . 35 3 25215°7 3963°24 is hs a 25224-7 3961-24 y 3 rh 252371 396038 ies 5 4 25242°9 395717 3 * # 25263°6 3956°77 ES es i 25265-7 3956-54 & 3 a3 252673 * Double. Sf REPORT—1 898. Iron—continued. Reduction to ——_—.. * Double. aca Intensity Vacuum ae Spark oe ; Previous Observations Teotaeeee Spectrum erecuet A+ ‘Ley in Wao. A 3955°50 In Mr. — 3953:25 1 ened K. & R. 1:09 7:2 252741 3952°74 » 3952-71 4 ” ” 25288'4 3951°30 2) 3951-25 ” ” ” 25291°7 (3950°10) 3 3950-05 ” ” ” 25300°9 3948-88 4 3948-87 ae ” ” 25308°6 3948°31 3 3948-23 z ” ” 25316°4 3947-64 2 3947-64, » | oo» 253201 3947°10 1 39471 1 ae ” | ” 253244 3945°22 if n 3945-22 a ” | ” 25327°9 3945-00 In 3945-00 i Boot) 398 25339°9 3943°45 i] 3943-43 ”? ” ” 25341°3 3942°55 2 *3949-54. 22 555 RB ” ” 25351°3 3941:40 ln 3941-40 v cl eau ” 25357°1 3940°99 2 3940-98 4 ” ” 26364°5 3939-06 In ue ” ” 25367°1 3937-67 i| ” ” caneg 3937-42 il ¢ 7) ” ” 5388°5 3935-90 2 Sel ae hes 25390-1 3935-41 1 apakaOe 108 | » 25399°9 393418 ] v2 ” ” 25403°1 3933°80 8 Ca “4 ” ” 25411°1 3933-05 1 ae ” ” ‘5 25413°5 3932-75 2 3932-71 |, bok 25418;4 3931-96 ] 44 ” ” 254203 3931-22 1 7) ” ” 25425°4 3930°43 6 hae P ” ” 25430°2 3929°82 1 de ” ” 25435°3 3929-26 1 99: ” ” 25439°3 3928-09 7 ccadaa| ” ” 25442°9 3926-06 9 3926-05 -Y. ” ” 25450°6 3925°76 ] 3925°74 dy ” ” 25463°6 3925°33 In 392531 | ” ” 25465°6 3923-05 6 3923-00. ” » 25468°4 3920°40 5 3920°36 ‘be ” ” 254832 3919°17 +14 $919°18 oF. ” ” 25500°4 3918°75 3 3918-74. ee ” ” 25508°4 3918-47 3n 3918-49 ti ” ” 25511°1 ae yn 3 3917-29 7 ” | ” pete 916784 3 me fe < ” ” ‘4 3914-39 t ae aces ee 25523'6 3913-74 ] 3913°74 3? ” ” 25539°6 3910°95 1 3910-95 di ” ” 25543°8 3909:95 In 3909-95 iy ” ” 25562-0 3908:°06 l 3908-02 sd ” ” 25568°6 3907-60 J 3907-58 2 ” 73 25580°8 3906°87 in 3906-84 id ” ” 255839 3906-59 5 390658 | ” ‘3 255886 3906°2 1n ? ” ” 25590°5 3904-00 2 ° ” ” 25593°0 3903-65 1 BBO) «ob 5 ds ee 25607°5 8903-09 ¢ 2. ” ” 25609'7 3900-63 1 oe” are 25613-4 oo 25529°6 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 3 JRon—continued. Reduction to 2 od 3 pee: Intensity Vacunm Oscillation S 8 ih and | Previous Observations |~ |, Frequency g Loeb | Character ; i in Vacuo pectrum | Ae he a Bou9'84 6 389980 K. & R. 1:08 | 7-3 256348 3899°12 1 389913, :: 5 25639°5 3898-05 4 3898-05 si, s 25646°6 3897°58 1 Seg754 «,; -COBRI-;. 1 ¥ 25649°6 3895°78 5 389575, 1:07, |» 25661°5 3894-10 1 389409, ; 5 25672°6 3893-50 3 3893-47, ¥ 25676°5 3892:05 2 389202, . As 256861 3890°96 1 389094 . . 25693°3 3888°95 2n 3888-92, 5 > 25706°6 3888-65 6 388863, L, * 25708°6 3887°18 5 SGT |, 4 ; 25718'3 3886-41 8 388638 : ; 25723°4 3885-63 3 388561 _,, 5s ” 25728°6 3885:30 1 388525, . % 25730°7 3884-49 2 388446, ; - 257361 388344 2 388339, * s 25743'1 3278:71 8 387882, ¢ * 25775°5 387815 7 387812 —,, 4 257782 3876°15 1 387614 ,, + A 26791°5 3873-89 4 387388, 2 * 25806°5 3872°65 6 387261 —,, » 25814'8 3871-88 3 387186, ¥ 4 258200 3869°69 2 386969, % . 258346 3868-03 1 386803, * fs 25845-6 3867°33 3 386733, .. 3 25850°3 3865°67 6 386565, 4 ; 25861-4 3863'86 1 386387, ¥ i 258736 3861:46 1 386146 ,, ‘- ‘ 25889°6 3860-07 9 386003, , 4 25899-0 3859°36 4 385934, ‘ : 25903:7 3857:03 1 " is 25919°4 385651 8 3856-49, 0Gl| 5s 25922°9 3855°45 In 385545, 4 - 25930'0 385452 In 385451, 4 i" 25936'3 3853'6 1b 385360 __,, Ss = 25943 385271 2 385271, Bee oka: 25948°5 3850-99 3: 385096, te oe 25960°0 3850°69 1 ee Uae 25962°1 3850°15 6 S8b011. «,, om Vicuee 25965°7 3848-47 1 3848-42, AR files 259771 3846-91 3 384696, ;, Ys 25987°6 3846:54 2 3846-55, F ‘. 25990°1 3846-18 1 384618, i, 259925 3845-82 1 384584, ;, is 259950 3845:30 1 3845:30 ,, - r 259985 3844-45 In a. 26004:3 3843-41 4 3843-40, bass 26011°3 3841-21 8 384119 4 "a 26026:2 3840-61 8 384058, hs Agnes 26030'2 3839°87 2 SBAD TS. | 45 ia 26035°3 3839-40 4 383938, ee 26038'4 3838-2 lb ¥ is 26047 383725 1 383727, f ‘ 26053-0 3836-44 2, 3836-48 —,, .. 4 26058°5 ¥ 2 324. REPORT—1898. TroN—continued. Reduction to | ie | Intensity Vacuum Spark and Previous Observations iS Character 1 Spectrum ie aw! A 383482 1 1:06 | 7:3 383438 8 3834:37 K. & R. — ” 383344 3 3833°44 fe ” ” 3832°4 1b ” ” 383177 1 ” ” 3830°96 1 3830°95 9 ” ” 3830°53 In 3830°54 ” ” ” 3829°85 1 3829°86 9 ” ” 3829°56 1 3829°59 ae ” ” 3829°25 l 3829 30 ” ” ” 3827°98 9 3827°96 ” ” ” 3826°96 1 3826'99 Ay ” ” | 3826°04 9 3826:04 ” ” ” | 3825710 i ” ” 382458 7 382458 ” ” ” 3821-96 2 3821-98 ” ” ” 3821°30 4 3821°32 e ” ” 3820°57 9 3820°56 ” ” ” 3819°80 In 3819°75 AD ” ” 3817°77 In 3817°84 = as T4 2816°46 1 3816°48 ey 1:0 ” 3815°99 9 3815:97 a ” ” 3814°90 1 3814°94 ” ” ” | 3814°65 2 3814°66 ” ” ” } 381401 il 3814:03 ” ” ” | 3813°77 1 3813°77 ” ” ” | 3813-12 5 3813°12 ” ” ” | 3812-04 In 3812:03 9 ” ” 3810°87 1 3810°89 a ” ” | 3809°70 1 3809°70 se, ” ” | 3808°85 1 3808'86 ” ” ” | 3807°65 2 3807°68 ” ” ” | 3806-81 4 380684, 4 % | 3806734 1 3806°36 ” ” ” | 3805-48 5 380547 i, “4 ” 380415 1 380415 “a cis ” 3802-40 1 380241 rs Hs Fi 3801°87 In ” ” 3801-80 1 3801-81 a 7 ” 3799-70 ‘é 3799-68 “0 ” ” 3798°68 6 3798°65 + ” ” 3797'64 4 3797°65 ” ” ” 379515 6 3795°13 =) ” ” 379448 2 379446 i ” ” | 379400 1 3793:99 + ” ” 3793°60 In 3793°60 a ” ” 3792-29 1 3792°28 “f ” ” 3790°92 1 3790°88 ss ” ” 3790°23 3 3790°22 e ” ” 3789°31 1 3789°31 + ” ” 378802 5 378801 “ ” ” | 3787:30 1 3787°30 a5 ” ” | 3786°82 2 378681 ‘3 ” ” 3786°30 2 3786'30 ” ” ” 378606 3 378607 Oscillation Frequency in Vacuo 26069'5 26072°5 26078'9 26086 26090'3 26095'8 26098'8 26103°4 26105"4 26107°5 26116'1 26123-1 26129°4 261358 26139'4 26157°3 26161'8 26166'8 261721 26185'9 26194'9 26198'1 26205 6 26207'3 26211'7 26213°4 26217°8 262253 26233°3 26241'4 26247°2 26255'5 26261°3 262646 26270°5 26279°7 26291'8 26296'4 26295°9 26310°5 26317°5 26324:7 26342:0 26346°7 26350-0 26352'8 26361°9 26371°4 263762 26382°6 26391°6 26396'6 26400:0 26403'6 264053 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Iron—continued. Reduction to 3: ) pa ) Wave- Intensity bs es Pen and | Previous Observations ark | pesicom Character ae i- 3782:°07 In 378205 K. & R. 1:05 | 7:4 3781°31 1 378131 ” ’ ” 3779-59 1 3779°58 ” ” ” 377864 1 3778°63 i ” ” 377756 1 3777°56 » ” ” 3777-22 1 3777°20 7 Fee FA 3776°67 it 3776°58 +5 | 1:04 ite ee 3774-95 1 377495, ea 3 3773°83 1 377384 ” ” ” 3771°10 In Rare pre 3770°44 1 3770743 oF aes ” 377013 1 3770°12 ” ris aa 3768°14 il 3768715 » ” ” 3767°32 {( 3767°31 "7 | ” ” 3766:78 1 3766-74 a, easy , 3766-20 1 376619 ,, ress ‘i 3765°70 5 3765-66 ro Tess ” 3763-91 7 376390, | » 37631 1b | ” ” 3762:2 1b 3762°30 ” ” ” 3761°50 In 3761°52 = iaitiss ” 3760°68 2 3760°66 ” a) ’ 3760°19 3 3760°17 ” ” ” 3769°62 1b ” ” 3759°35 1b 3759°30 ae 1mirSs ” , 3758:92 1 betes Ss fiartas 3758°39 8 3758°36 ” | ” ” 3757°60 1 3757°60 “p PP ” 3757-08 2 3757 06 - ” ” (3756-21) 1 375617 + titi ss ” 375462 In *3754'63 ». 002 Ritesy,; 3 3753°74 3 375374 “- | 99 ” 3753°4 in 7) eal ee 3752°56 1 3752°57 ” aie lee 93 3752:2 1b ” } ” 3749°64 10 3749°61 ~- beth Ss ” 8749-05 2 374906, linea ” 3748°41 Tf 3748°39 =p tS iliss ” 3747-02 2 *3747:09 so (O04 Dal aiiess ” 3746°55 1 3746°56 ” ” ” 3746:04 if 3745°95 2 ” ” 3745-71 16 3745°67 ” ” ” 3744:70 1 : ” 3744-60 il ” ” 3744:20 1 3744:21 ” ” ” . 374358, | | 3743 51 7 { 3743°45 - | ” | ” 3742°73 al 3742°77 ” ” ” 3741°95 In ” ” 3740°9 in ” ” 3740°39 i! 3740°44 A “3 ” 3740°18 il 3740°22 3 ” ” 3739-65 1 3739°73 Fr ” ” 3738°40 3 3738°44 a? PP ” 3737-27 8 3737°27 1:0: ” ” * Double, Oscillation Frequency in Vacuo 26433°2 26438°5 26450°5 26457:2 26464°7 26467-1 264710 26483°0 26490°9 26510:0 26514°6 26516°8 26530°8 26556'6 265404 26544°5 26548:0 26560°6 26566 26573 26577 6 26583°4 26586'9 26590°9 26592°8 26595°9 26599°6 26605°2 26608°9 26615°1 26626°4 26632°6 26635 26641°0 26644 26661°7 26665°9 26670°5 26680°4 266837 26687°4 26689-7 26696°9 266976 26700°5 26705°4: 26711°0 267165 26724 26727°7 26729-2 267330 26741°9 26750:0 326 REPORT—1898. IRoN—continued. | | aaa ue Reduction to ee Intensity | y Vacuum bee Spark and | Previous Observations |—— oe Spectrum Character eee Hrequency ne = in Vacuo 3725°44 3 3735" oR Teche 3735°01 10 313500 ea ee srr 3733°46 6 3733°46 $4 | Dow 193 26766°2 3732°50 4 373254 2 | ‘i | V 26777°3 3731-05 1 8731:07 4 rh ” 26791°4 3730°51 2 3730°53 p? ” ” 26794°6 3728'78 a 3728°81 id » ” 26798°5 3727-78 7 1 oe es 26810°9 3l2t'23 2 372713 4 fi ” 76 | 26818:0 3727-02 2 2 ” eee 3725°60 1 5 ” ” | “ 23°5 3724-49 3 ha » |» 26833-7 3722-73 6 3722°69 ad ” ” 26841-7 3722-06 1 3722:07 a2 ” ” 26854-4 3721-68 In 3721°69 sig ” | ” 26859°2 3721°35 1 3721°41 2 ” ” 26862-0 3720°10 8 3720-07 dd ” ” 26864°4 371853 1 3718-55 + 2 ” | 26873°4 3716754 3 8716°59 ay | ” ” | 268847 3716°01 if 3716 04 Ld 9 ” 26899°2 3711°52 1 3711°54 ” \ ” | ” 269030 3711°33 14 3711°35 a | °F ea ” 26935°5 3709°40 6 3709:37 z td } ” 26936'9 | 370806 5 3708:03— latte 26950-9 | 3708:01 | 2 ” hee Ap ae ms 3707°65 | In - | 2? | ” 61:0 | 3707-16 2 Boche ‘f nea ptt 26963'7 | 3705°73 6 3705°70 4 ” | ” 26967°2 370459 3 aig |e 2697-6 3703°95 1 3703:96 e? ” ” 26985'9 3703°81 1 3703°83 4d | ” } ” 26990°6 370367 1 3703'68 ad | ” | ” 26991°6 3702-60 1 ies: 3” ee 26992-6 370217 1 3702°16 ee tongs » 270005 3701-20 4 3701:20 Wa | ” ” 27003°6 3698-75 1 3698-73 “4 | ” | ” 27010°7 3697-58 2 369758, Lea» 270286 (369520) | 3 369518 |. 1302 | os 27037'1 3694-13 4 iat ie ane 27054°5 3693°20 1 369316 Ry | ” ” 27062°4 2 ~ ’ } on 3690 87 2 3690°86 3 ee!) ” 27069-2 3690°60 | 1 3690°60 = ” ” 270863 3689°57 | 3 3689°58 a? ” i ” 27088°3 3688°64 In 3688°65 a? | ” | ” 27095'8 3687°70 3 3687°77 sos | ” ” 27102-7 3687°55 6 3687°58 ¥? | ” ” 27109°6 3687-24 1 368721 ” ” 27110°7 3686°38 1 3686-40 a } ” ” 27113°0 365613 3 368610 ,, ee i 27119°3 3684-25 4 3684-24 » | oo» 271211 3683-19 3 3683°18 a | ” | 2? 27135:0 3682°35 4 368235 eee Na Me 271427 368088 | Ib ” an ee 27148-9 3680-90 | 3680-06 bea 3680:03 a? jn | ” 271597 4 ” ” 27165'8 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 327 Jron—continued. ie | ; aaa to | ave- acuum * . I i Oscillation fe per = Previous Observations |——7]____ Frequency | igscbram | Character A+ x mn ua 3678:97 1 3678-99 K. & R. bROe |) FF | 27173°8 Sorvwias| - 4 3677-76 —,, rt tear 27183°1 Soig4en.'| 2 367742 —s, heme ot 27185°3 3676-42 | 2 367644 ,, Leone ol) 27192°7 B674:88 1 367489 _,, asm |) as 27204°1 36746 | In 367455, AGS hss 27206 367092 {| 1 367095 eae (ea | 272334 3670-19 2 367020 __,, eras yt 55 27238°8 3669°63 3 366965, lip pr ea 27243-0 366926 | 1 3669°29 __,, ath 5 al 27245°8 366811 | In 366811 _,, Tne eee 27254:3 366738 = 1 3667-45 —,, a | 27259°7 366638. = = _In 3666-41 re a 27267°2 3664-71 In 366474 _s, SPAN ye] 27279°6 3663°56 In 366360 __,, pet... | 272882 3662-98 ln 366304, le taereot 27292'5 365963. | 2 365965 ls tx ‘ 27317°5 365807 | in 365807 _,, Be ah 273291 3657-25 | 1 365727 —, POU) ss at 27335'3 3656°33 1 365637 __,, = c 273421 3655-70 In nf | 27346'8 3655°57 1 365560, em ont 273478 3653-71 1 365390, ass in el 273617 3651-60 4 365161 a, Le (as etal 27377°6 3650-40 2 3650°42 ” | ” ” | 27386°6 3650-13 1 3650714 _s,, 3 * 27388°6 3649-62 4 364965 so, Wats . 27392°4 3649°41 1 364944, as * 27394:0 (3648-00) 9 * 364799, re me | 27404°6 8647-56 1 3647-57, 33 Ae 27407°3 3645:93 2 3645:96 fixes ve 27420°1 3645-65 1 364563, lpastaateett? casamatt 27422:3 3645-20 ew 364522, le Os | 27425°6 3643-80 In 364380, lanes a € 27436°2 3640:53 5 364053, a‘ a 27460°8 3638-42 4 363844, Boh 78 274767 3637-98 1 363798 _,, neue x 27480:0 3637:40 1 363739 _,, ese ae Ae 274844 3637-11 1 363716, lsbas FF 27486°6 3636-77 1 3636-73 si, Pers ne 27489°1 3636-32 1 363632 —,. % a | 27492°5 36353 1n 363539 si, tpt , 27500 3634-8 1b 363480 _,, (pars - 27504 3634-45 In 363448 le bey 8 275067 3633-97 In 363398 a ae 27510°3 3633:12 1 363316 _,, a ee 27516'8 3632°65 1 363271, Wyobes 0 275203 3632715 2 363220 ,, mend i S/ 27524-0 3631-64 10 363162, eng +, >| 27528:0 * 3631-23 2 3631:23_——s, | 275311 3630°50 1 363050 __,, WERE ii 5s 27536'6 3628-0 In 3627-91 _,, A 27556 3625:27 1 3625:30 _,, vi Es 27576°4 3625:00 In 3624-95, . 2Q7578°4 3624-5 In 3624-46, 2 al} anes ————— 328 Wave- length Spark Spectrum 3623-92 3623°58 3623°31 3622715 3621-7 3621°60 3620°65 3619°7 3618°92 3618-50 3617-90 3617-44 3616-68 3615-30 36148 3614-27 3613°6 3613°3 3613°1 3612°6 3612°24 3610°82 3610°30 3609°51 3609-02 3607°30 3606°S5 3605°60 3605-40 3603°96 3603°35 3602°64 3599-77 3599-30 3597-20 3596°3 3595°4 3594-78 3589°58 3589°24 3589°05 3588°75 358787 3587°56 358710 3586-25 3585°85 3585-49 358510 3584-81 3583-48 3582-35 REPORT—1898) ITRoN—continued. Intensity and Character ella dal a ol alas DS eB OO OUR ROT et ee Reduction to | Vacuum nee Oscillation Previous Observations ti, Frequency AG iL in Vacuo A 3625°94 K,& R. 101 | 7°8 27586°6 2623°58 5 a a 27589-2 3623°33 * “= “a 27591°3 3622715 = ane ae 27600°1 3621°87 aA Pn hemee 27604 3621°61 - ieutoetss 27604°3 3620°62 oe Seale 27611°6 3619°89 | = { 361954” | sf | 3618°92 “4 + - 27624'8 3618°54 » ” ’ 276280 3617-94 2 1:00 Po 27632°5 3617°47 "ad 5 3 2763671 3616°76 | > hate” pe ween ee 3615°41 “dl sy Pa 4 27652°4 3614:78 ee e a 27656 3614-26, ok) = 2reeoe { 3613°75 | ane | 3613-58 | ” | ” 3 | 27665 3613-26 a NO ori ; 27668 3613710 oases 3 27669 . a - 27673 3612°25 43 ries, Fe 27675°9 3610-86 - ‘a AS 27686°7 3610-29 a = 5 27690°7 ewe seile = o55 276968 3608:99 fs heey i ee 27700°6 eee Si. G 27713°8 3606-83 __s,, rEtee wry 277172 3605:62 4, pikes te # 27726°8 ‘i Be 27728'4 3603°98 ie 1 a 27739°5 3603°34 z= 277442 3602°64 se $5 ae | 27749°6 3599°77 = [Paks ace Mt 277718 3599-30 . ron ile | 277754 3597:22 B reGGhy to 27791'6 3596°35 Ae y | 27799 3595°43 > 3 sv) Al 27806 3594-71 “ ; 79 | 27810°2 3589°58 4 cae, aS 27850°5 3589°25 - hisses 27853°1 3589-05 ” | Pease be 278546 3588°75 5 es i 27857'0 3587-87 * jae of 27863'8 3587°55 » HF . 2786671 3587-10 “A ee ee 27869°8 3586°24 a oa ee: 278764 3585°84 , an 27879°5 3585°43 - Sane a oc 278823 358508, “3 ne 27885'3 3584:78 a eerie » 278876 3583°45 ie ¥ pas 27897°9 3582°32 ;. | hammers 27906°7 ——— ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 329 TRON—continued. ie. Reduction to length Intensity Vacuum Oscillation Spark and Previous Observations Frequency Spectrum Character ee bes in Vacuo r 3581°36 10r 8581°32 K. & R. 1:00 | 7.9 279145 3578°78 1 3578°80 “5 Se ler 279346 3578°53 1 357849 3 ee aes 27936°5 3577°8 in 0:99 | ,, 27942 3576°90 1 3576°89 i ea 27949°3 357617 in Sere il, ,; +a epee: 279550 3575°52 1 357549 + * i 27960°1 3574-04 2 357400, Te ee 279716 3573°55 1 3573°52 ae 3 es 27975'5 3572°75 In 357279 i, ef i 27981°7 357213 2 357212, ‘3 ‘ 27986'6 3571°38 1 3571°34 - 34 rf 27992°5 3570-42 8 3570°45 s VT) eta ee 28000-0 357018 8 357023, aa ae 28001°9 3569'12 1 3569-:09 34 : 28010'2 3569-00 1 3568-94, A is 28011°2 3568-55 1 356853, | ; 280147 3567-20 1 356715 mth 2 28025°3 3566'75 In 356670, . x 28028'8 3566-25 In 3566-46, : My 28032'8 3565°54 8r 356550 + aie 28038'4 3564-67 1 356461. + OP ars 28045°2 3562-0 1b ‘ i 28066 3560°83 1 356081 _,, ell ee 28075'4 3559°65 1 3559°62_—iw, - ‘ 28084'3 3558°68 6 3558°62 e - 280924 3557-02 3 355699 __,, 4 ‘ 28105'3 3555-09 5 355504, i 4 28120°8 3554-7 In 3554-62 fi A 28124 3554:32 1 355424, 2 4 28126°9 355391 2 3553'84 —_, ¢ Ps 28130'1 3553-01 si 355295, eat <., ght =) eee 3552-28 1 355224, iin, nied ms he 3549-98 1 3549°97 sp POLAR TEE 8:0 28161°2 | 3548-17 1 354813, e " 28175'5 3547-33 1 354731 4 . 281822 3545°76 2 3545°74 —_, ‘ a 281947 | 3544-75 1 3544-74, i a 28202°7 3543-82 1 3543-78, I i 2821071 3543-60 In 354353, Z Hs 28211-9 3542-21 5 354220, 2 . 28223-0 3541-23 4 3541-22, gs iliard 282303 | 3540-90 In 3548-82, vi %: 28233°4 (3540 27) 1 354024 ., -266R) ,, : 28238-4 3538-06 1 3538-01, : Pol 28856 3537-88 1 3537°84 _,, 098 |. 282575 | 3537-68 1 3537°60 45 2 oe 28259'1 3536°59 4 353665 ,, is ki 28267-8 3533'36 3 353330, 3 "| 982937 3533-12 2 3533-08, % a 28295'6 3530°55 1 3530-48, Z 3 283162 352997 2 3529°90 45 “ Ps 283209 3527-94 2 352790, si :: 28337°2 352683 | 2 3526-76, - 28346-1 352660 | 3 352651 | ae ae 28347:9 300 REPORT—1898. TRON—continued. | bid inigiey | | Warten re Spark oy | i vati : : a ark Chavackde Previous QCbservations 1 eaaeuy 7 | | axe Bios in Vacuo 3526°31 4 . 352631 3526-25 K.& R. | 098 | 8 san co 0:98 | 8-0 28350°3 2 2 = ” ” 2 5 ar) ahasin 1 3524°34 ” ’ | 28365 7 Seo ! 352415 fi , ” 28365'7 nt ee e 34 28367°1 sa a * » | 283781 a , 2521°93 : ” | ne 28381°5 — 2 3521°36 s ” ” 283850 a) : 3518-96 és ” ” 28389'7 3513-96 5 351650 ,, : | ad depen 3513°17 ln 351391, oa 281499 3510-65 1 351315 __,, ct sl 281563 3510-0 ih See ag ‘ $1 DSt7T5 3508-63 1 350995, i | geen 3506°64 1 350858 jogs "| ggag3 co y » | © 28498'1 3505°20 eect gee | aa t 3505°15 } ”” 9 3504 ’ . z BuO : ae | 01 3498-00 5 3400°64 —,, yf | apser 3497-26 349792 55 i » 285107 B 3497, 97 | ’,, 28579: 3495-44 2 Sl 7 34949 fa 3495°37 y atl 286005 3493-63 2 3494-76, i "| 38605” 3490-73 3493°78 i 5 28615 6 349065 ” ” 28615°4 3489°82 1 a 348982 3489-74. Be 986467 9 3486" | ” ” 28646: 3483°15 1 cae 3478:80 In 3483-09, af ; 8701.5 3478-00 In 347869, if ‘ 287374 3476-85 5 347793, . ; os74t-1 3475-6] 7 ie a " " ass 347459 1 3475°52 _,, it ” | 387688 3471-46 9 347451, fs . 287723 3469-97 1 3471-40, # . 28798-2 3400-97 1 3469-91 p ” 8:2 287982 315023 Sen ee ” 28810°5 345894 3468-99 4 ” ” 28817°5 3466-01 7 ie ; 25002 3460-04 1 3465°95 —s, ‘ 8843-4 3458-44 1 See = . : 28895: 3457-05 In 345839 yy o%v6 | 8906-6 : 345839 | x 28906'6 3453°13 1 a 3452-41 3 345310, ‘5 $ 8951-0 3452°16 2 345235, i i 289571 3451:80 In 34 hos 2952 3450°47 9 51:99, ‘ 28962-2 3447-43 9 3450°41 —,, i Wey 289734 3445-30 4 3447-37, badge 280989 (344403) 5 3445-22, i “ 290169 3449-89 1 3443-96, i i 29027°5 3442°51 1 3442°75 yy ‘ 4 290878 3441°16 6 3442-44 ,, Ce 2040-4 344077 | 344107, fi ; 29051°8 7 344069 |, Fs sais 290551 is As 29055'1 7: ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE j Iron—continucd. ELEMENTS. 331 Wayve- Intensity : : Tae) and Previous Observations ark debs aa Character 3440°02 1 3439°93 K. & R. 3438-42 1 3438°36 ,, 3438°19 1 343802 _—s, 3436°25 In 343606 ,, 3433°72 1 3433°64 3431-98 1 343190 __,, 3428°35 2 3428:26 ,, 342729 5 3427-21 —,, 3426°81 2 342671 sy, 342653 2 342644 3425°17 1 3425:08 __,, 3424-45 3 342436 ,, 3422°82 2 3422°68 a 342269 __,, 3418°6€ 3 341858 ,, 3417:99 3 3417:92_—, 3415-70 1 341561 3413°31 5 3413:22 3411°50 1 341143 ,, 8410°30 1 3410°26_,, 340762 6 8407°55 i, 3406°96 2 3406°88 __,, : 3406°62 In 340650 ,, ‘566 KR. 3404'50 3 340441 3402-42 2 340233 __s,, 3401-68 1 340160 __,, (8399-49) 5 3399°39 ,, 3398-45 In 3398'29 si, 3397-75 In 339768 ,, 3397-10 1 3397-05, 3396°1 1b 339613 sy, 339546 In 339472 1 339465, 3392°80 3 3392°74 i, 3392-43 2 3392°37 sé, 3392°13 1 3392712 _—, 3389°85 1 3389°83 ,, 3387°50 1 338748 _,, 3384-11 2 3384:05 338384 1 3383°80 __,, 3383-00 1 3382-52 1 338248 3381°15 In - 3380°25 3 338017 ,, 337911 2 337911, 3378°76 2 3378°77 i, 3372-90 1 3372°90 3372°18 i 337218 337092 4 3370°87 sy, 3369°69 3 3369°62 3366°92 2 336688 3361-31 1 3361°03 __,, 3360°2 1b 3358-4 1b 335841 —,, 3356°49 1 335644, Reduction to Vacuum ] Pw eas 2A 0:96 | 82 ” / ” ” | ” ” | ” ” ” A $3 ” ” ” ” ” ” ” } ” ” | ” ” ” ” ” | ” ” | | 39 ’ 0-95 3 ” ” ” ” ” ” ” ” ” ” ” ” ” ” a ” | ” ” | ” 2 | ” ” | ” 2 al ” ” | ” ” a 8-4 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” | ” ” | ” ” | ” ” | ” ” ” ” 0:94 7 ” ” ” ” ” ” ” ” ” ” a 8:5 ” ” Oscillation Frequency in Vacuo 29061°4 29074'9 290769 29093°3 29114-7 29129°4 29160°3 29169°3 291734 291757 29187°3 29193°5 29207°4 29208°6 29242°9 29248°7 29268°3 29288°8 29304'3 29314°6 29337°7 293434 29346'3 29364'6 29382°5 29389°2 29407°9 29416°9 29422°9 29425°6 29437 29442°7 29449°1 29465°8 29469-0 29471°6 29491°4 295119 29541°5 295438 29547°6 295554 29567'3 295752 29585'2 29588°3 29639°7 29646°0 29657°1 29667'9 29692°3 29741°9 29752 29768 29784°5 32 REPORT—1898. | IRON —continued. Wave- Reduction to length a hed Vacuum eesti: Spark an Previous Observations. |~ | ou Ch: Frequenc Spectrum aracter eee | i 3 a eat 3355°35 7 i = 3354-14 : hes | 0-94 | 8:5 297947 3351°89 1 f a ” | ” 29805°4 3351-83 1 | 3351°85) ” } 9 29825-4 3351°63 1 3351-65 | dese ” 298260 3349-48 1 a eas | ethsee, jh 95 29827-7 3349-11 1 / ” ” eaten (3348-01 1 - eat eee 850-2 ue 1 Soiree 31329°7 3188-92 1 3188-96, ., - 31349°7 3188-70 In 318867 _,, ., Be 31351°8 3187-40 1 318735, 4 - 313646 3186:87 3 318683 _,, 4 Ss 313699 3185°43 In 3185°34 i, 4 a 31384-0 3184-98 1 3185-00 _,, :, $ 313885 318324 1 318311 _,, ., bs 31405°6 3181-67 1 318160 _,, 0°89) | ,, 31421:1 318085 | In 3180°85 _,, ee, 90 31429+1 318032 2 3180°30 _,, ., “3 314344 3179°61 2 317961 __s, 4 2 31441-4 3179-07 1 317906, % 5 31446:7 3178-09 1 317808 __,, leet, 6 314564 3177-64 3 317764, [rea Z 31460°9 317554 1 317553, 3 B 31481-7 3171-43 1 317144, be . 31522'5 3170-47 1 3170-43 __s,, - - 31532'1 3167-96 4 316797 — ,, a ii 31557°1 3166°52 1 316655, - 3 31571-4 3165:95 In 316597 _,, # = 31577°1 3162-90 1 :, 3 31607°6 3162-05 1 316204 __,, . Ss 31616°1 3160°74 1 3160°74 _ * 31629°2 ‘| 3159-0 1b 315908 ___s, % is 31647 ‘| 3157:97 1n 315799, , f 31656°9 3157-12 1 315715, :, a 31665°4 (315432) 5 315429, :. a 31693°6 |} 3153°33 In 315331 Lose ic 31703'5 ‘| 3151-46 1 315142, A 31722°4 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 335 TRON—continued. w. | Reduction to | length Intensity } | acoum | Oscillation Spark | and Previous Observations | (aan | Frequency Spectrum | Character ap (ee in Vacuo A 3144-88 1 | 3144-61 K.& R. 089 | 91 31788°6 3144-08 1 3144-06 5 ” ” 517967 | 3142°95 1 | 3142-97 Fa ” oF 31808°1 | 3142752 In 314254 _,, ” ” 31812°5 | 3140°48 In 3140°47 ie 0:88 is 31833°2 3140:00 In 3140-00 » ” ” 31838°0 3135°49 2 3135°51 ” HeMaye 95 31883°8 3134:20 1 313421 ” » | oo” 31897:°0 3133°17 ln ” | ” 31907°5 / 3126-25 In 312625 =, Leia ee 319781 | 3125°77 1 3125°77 7 HAM | ge 31983:0 | 3120-50 1 3120°54 - fst | mss _ 32037:0 3119-60 1 3119°58 + | 49 ”» 32046°3 3116°70 if 3116°73 iz . | a 32076:1 3114-40 1 Ie oerriay Mie oe 32099°7 3106°65 In 3106°59 op hed Aa 32079'8 3105°65 In 3105-69 pe Vhs snes SE een 32090:2 3105°25 ln Metso AIP -y5 321943 3100-76 2 3100°77 os Osta. 32241:0 3100-44 2 | ” ” 32244°3 3100 05 2 3100°04 8 iake, A 32248:3 3098-30 1 3098-25 Pe mt 3 32266°6 3096-45 1 psy Ae 32285'8 3091°70 2 3091°67 ap ; oo» ” 32335°5 3089°5 In 3089°64 5 ely as 32359 3083°85 2 308381 ” ” 9:3 32417°7 3078°9 1b A Fi 32470 3077°30 2 3077°32 is Bs oh 32486°7 3075°84 2 3075°80 - “4 a 32502°1 3068°27 In 3068°25 ” ” ” 32582°4 3067-35 3 3067°30 BS + + 32592°1 3065°50 in 3065-40 % 4 7 22611°8 i £ 3062°47 > : 3062-33 2 | 3062.29 \ . 086 | ,, 326456 3059-20 3 305919 * +} op 32679°0 3057°56 3 3057°55 a = -- 32696°5 3056-95 In ” ” 32703:0 3055-40 1 3055°35 3 s Pr 32719°6 3053°17 1 305315 ” » ” 327434 (8047:72) 3 3047°71 ae a 9°4 32802°0 3045-1 1b 304516, 4 ” 32830 3042°77 1 3042°75 6 fi = 32855°4 3042712 1 3042713 oe af - 32862°5 3041-88 1 3041°83 - aD 328650 3041-80 1 ” ” 32865'9 3040°55 1 3040-54 e A A 32879°4 3037-50 3 3037°54 re - no 32912°4 3081-75 1 3031°74 Pa a _ 329749 3031°34 1 3031°31 Se Rs $ _ 32979:3 3030°25 1 3030°24 re aA a 32991°2 3026-57 1 3026°57 * - = 33031°3 3025-96 2 3026-00 Fe a =n 330380 3025-75 1 3025-75 a ° ss 33040°3 3024-14 1 3024-13 Pe a 95 33057-7 3021-18 2 3021:15 pe 0°85 aa 33090:1 36 REPORT—1898. Iron—continued. / Reduction to | ns Intensit Vacuu | ength by T= if mit ge Spark an Previous Observations 7 eg a oT Ska Spectrum Character 1 : $ y A+ LN in Vacuo | A 3020°79 2 | 90990: - ep =e 3020-60 2 i ia 0°85 | 95 33094-4 3019'11 . i} 83019: ” ” } 330965 3017-73 1 Ree fai 1 Ps 33112°8 3016°30 uf 3016-29 au ” | ” 33128°0 3016-05 ln 3016-04 ij i hl ees 33143°7 3011°60 1 3011-57 an ” 7 33146°4 3009-70 2 3009-66, et), Yas 331954 3008°26 2 | 3008-23 a } ” | ” | 33216°4 3007-42 | 1 | 300730 .. ° 2 » | 832823 3003°19 | 1 | 3003-14 ” ” | ” | 332416 300280 | 3 | 3002-74 x eA tS) 332884 3001:08 | 2 | 3001-05 a in? ” 33292°8 3000°57 | 1 3000°56 am H tid ” | 33311°8 3000:20 In i af | ” ” | ne 2999-65 2 | 9999- (aie noe 21°6 2997-45 1 25 ae Hes tT 33327-7 2994'56 3 | 9994-54 | OE S| OR 33352°1 2990°51 1 2990-48 a ” | ” 33384°3 2987-41 i. 2987-40 3 Mister 2 ” 33429°5 2985°70 4 2985-65 23 } age ” 33464°2 2984/97 6 2984-92 2 | ” ” 33483°4 2983°71 2 2983-68 a2 } 99 ” 33491°6 2982-20 1 2982-31 y | 0-84 ” 335047 2981°59 1 2981-54 us | 8 ” 33522°7 2981°12 In ” fruits ” Br teen 2980°70 In 2 “62 | ” ” 335348 2979°48 1 Aad my, fe ge ” 33539°6 2976°70 1 2976-66 a ” ” 33553°3 2976°05 1 os ” ” eked 2973°39 A 5 fle) ” 35920 2973°28 2 hie 3 ” ” |33622 0 2970°64 2 2970°60 2 ” ” 336233 2970°25 2 297020 ee. a4 33653°1 2970°05 1 Be ” ” 336575 2969°63 1 ” ” | sate 2969°53 1 ‘ ” rm 336645 2967°03 2 ae * ” ” 33665°7 2965°39 | 2965°35 a, ” ” | 336940 2965:17 2 2965'12 sf ” ” 33712°7 9964°76 if 2964-72 ay, ” ” 33715°2 2964:25 1 2964-30 # ” a8 33719°8 2961°40 1 2961-30 ¥ ” ” / 33725°6 2960711 1 2960-07 3 ” re | 33758°1 2959°70 1 2959-76 ie ” ” 33772'8 (2957°49) 1 2957-48 2 Poy » | 337775 2954-06 2 2953-99 oy eae? » | 33802°8 2953°88 3 2953-86 33 ” ” 338420 2950°35 In 2950°34 ag ” ” 338441 2948°52 1 2948-52 p? ” ” 33896°7 2948-00 2 2948-00 |, ” ” 33905-6 2947-78 3 2947-77. ” ” 33911°6 2944-55 4 2944.49 » ” 239141 2941°46 1 294142 ” 98 339512 — ” 0°83 ap | 33986°9 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 337 IRoN—continued. Reduction to Wave- é length Reo CPT ad pe Oscillation par. revious Observations | |, requenc @peetram Character ie. _ in vacko. A 2939-62 1 0:83. | 9:8 ; 2937-02 2 ' 34008:2 ey a 2936-99 K. & R. ¥ ve 34038'3 2929-13 2 2929-20 ” ” 34099°5 2926-71 3 292665 Rah ak tne 2925°52 1 292543, x ds be ee 2923-99 1 2993-94, “ - peel 2 gsi | | eesso | |) ataee 2920-82 1 2920-76 ” ” 342115 291814 1 291811 C = oe 291 7°65 In 2917-58, 4 58°6 2917-20 In ; ” ? ae 2912-27 1 2912: t ” : 2910:9 1b oT * a ” ae 2907°98 1 2907-94 ” ” 2907-60 1 2907°59 2 % ” pone 2906°25 1 2906:23 ”? ” nd 3 pig 2902-57 In 290255, os2 | 7 4398°7 2902:03 In 290202, ” 34442°3 2901-52 1 2901-46, 2 ” 34448°7 2899-50 1 2899-49 ; ” 344548 2897-37 2 2897: 3 ” ” 34478'8 289769, 2895'35 2 2 gee pes 34504°2 2895:17 1 289511, mig) 180 34528-1 2894-90 2 : ” ” 34530°3 2894-65 1 9894-59 ” » 34533°5 ges | i jae Ctr) ees 2887-95 1 2887°88 era ae 346136 #2887°4 In 2887-43 |. ” 34616°6 a en 2884-9 1b ai ln 34639'8 2883-80 3 2883:80 . & 653 2880'89 3 288084 ¢ ” 34666°5 2879-35 1 r » 34701°5 2877°38 1 2877°37 ” ” 347201 287686 2 287680, _ ” 34743:8 2875-44 2 287535, eS ” 34750'1 2874:27 1 2874-24 * : ”» » 9 34767°3 2873-49 4 287348, Pen gt 34781-4 2872-47 3 987238 Re 34790°9 2871°19 2 287116, ” 34803-1 2640 | 1 7 | 2 | Basae8 ‘ 1 2869: % ig ‘6 2869:28 1 Sg a ie tee? 248404 96 7 2868-94 a sd pees 236632 |, 1 286668 ” ‘ 34851-1 ose | | ok | BeBe : 1b 3 ” 33 2863-95 1 2863-92, O81 | 34901 2863 53 1 2863°46 ”» ” 34906°7 2861-26 1 2861:29 ” ” 34911°8 27 | 349395 1898. > » , Zz 338 REPORT—1898. TRON —continued. Reduction to icy Intensity Vacuum Oscillation aie and Previous Observations | ———__~__ Frequency Spar Character | 1 in Vacuo Spectrum Nu: prea A 2858°95 In 285896 K.& R. 081 | 10:1 34967°8 285840 5 2858'41 55 Fi 25 349745 2857°53 1 ” ” 349852 2857°28 2 2857°29 s 6 “c 34988°2 2857:07 In 2857:09 - a = 34990°8 2856°52 ln as - 34997'5 2856°25 1 2856719 + a Fr 35000°8 2855°77 3 2855°75 * > 8 35006°7 2853°85 In 2853°81 es “r % 35030°3 2853°33 In ; + as 35036°7 2853°02 In 2853°02 i as Fe 35040°5 2852°24 1 Mg 2852°19 A Sy " 350501 (2851°90) 2 2851-85 4 a Pr 350542 2849°70 2 2849-67 Ss ” rh 35081°3 2849:02 1 ” ” 35089°7 2848-52 2b 2848°77 . = a 35095'9 2848°15 2 284813 or as 10:2 35100°3 2847-34 i ” ” 35110°3 2845'8 2b 2845°75 A * - 35129 2845°72 1 ” ” 35130°3 2845°51 In ” ” 351329 2844:08 2 2844-04 By his 3 351506 2843°75 1 - aS 35154-7° 2843°58 1 2843°69 “6 * 3 351567 284343 in 2843°30 “5 33 3 35158°6 2842°85 In 2842-96 = hy 3 35165°8 2842°20 Ll 2842-46 * 5 i 35173°8 2841-47 iL 2841°32 a i 3 35182°9 2840°82 3 2840°73 a + 4 35190°9 2840°46 2 2840-50 Ay 55 * 35195-4 2839°85 2b 2839°66 a 5 i 35202°9 (2838°23) 1 283819 ry ‘ a 35223°0 2837°43 1 ” ” 352330 2836°63 1 ” ” 35242°9 2836°31 1 2836°45 Pa Sy 45 35246-9 2835°82 4 2835-76 4 7 FA 352530 2835°58 1 2835°51 ay a rn 35256-0 2833°3 1b 5 is 35284 2832°57 2 2832°47 “6 :, s 35293°4 2831°67 5 4) oy 353046 2831°15 1 2831:04 °°, “5 = 3531 1-1 2828-75 3 282887 4%, sy rn 35341°1 2828-02 1 2827°98 + 5 = 35350°2 2827-55 2 2827-68 * ; “5 353561 2826°16 1 2826:07 ; ‘f 35373°5 2825°85 1 282575 E , F 35377 + 2825°66 2 2825°60 080 5 35379°8 2823-41 3 2823°32 * -. 10:3 35407°9 2819°45 1 2819°35 i >) “A 35457°6 2817-60 In 2817°55 .; f A 35480°9 2817°25 In ” ” 35485°3 2813-74 1 2813°67 tes Es - 35529°6 281340 2 2813°36 “a 35533°9 2812°2 In 2812°36 Ps f r 35549 2811°36 1 2811:23 zn > . 35559°7 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 339 TRon—continued. Wave- Intensity length and Previous Observations Spark Character Spectrum 2810°0 1b 2807:10 2 2807:038 K. & R. 2805°91 1 2805°87 uA 2805744 In 2805°02 1 2804°64 2 2804°56 Fe 280413 In 280413 on 2803°72 In 2803°68 > 2802°82 2 Mg?) 2802-76 i 280118 In Mn) 2801:15 + 2800°9 In 2800°73 By 2799°83 1 2799°87 93 2799°42 2 2799°34 Pei 279840 1 Mn| 2798:31 A 2798-06 1 2797-92 ] 2797°82 6 27975 1b 2796°9 1b 2796°91 is 2795°65 3 Mg; 279558 os 2794:9 In 2795:00 a | 2794-02 3 279397 of | 2793:40 1 | 2792-55 ] 2792°44 fs | 2791-94 1 2791:84 | 2791:65 1 279151 7 1 2791-20 1 2790°70 1 2789°87 1 2789°87 A) 2788:23 3n 2788°19 Be 27875 1b 278546 3n 2785°25 ss | 2784:43 1 2784-40 Er 2783'81 a 2783°75 FS | 2781:96 1 2781:89 $3 | 2780°9 1b 278093 fe | 2780-19 1 2780°28 =: 2780:07 1 2779-40 5 2779°34 “A | 2778-96 1 2778°89 Be 2778°34 2 2778'29 FP 2778-01 2 277815 3 2777-15 1b 2776:31 1 2776°47 oF 2775°5 In 2774°82 3 2774°76 rf 2773°38 1 2773°28 aH 27726 In 2772'56 Ay 2772°23 2 277215 as 2771°70 ul 2771-34 1 2771°30 ” 2770°64 2 2770°75 i=] EA Go Oy SU C3 SUR IRS C800 He re ea Bae be teal gies aera ee cas a low WAndwnwrne-E Previous Observations 245267, | 245155, 245128 , 244993 i, } 2448°88 i, 2447°81 3 2447-25, 244653, 2446°30 i, 2445°68 ,, 244523, 2444-58, 244394, 244268 ss, 2441-73, 244025, 2439-82, 2439°36 i, 2438:27 243733, 2436-45 2435-93, | 2435-04 243354, 2432-97 2432-34, 243138 | : 2431-08 | | 2430°16 + 2429:53 2429-00, | 2428-41, 2427-11, : 2426-46, | * Double. Reduction to | Vacuum 1 a+ | =- A 0°80 | 12:0 ” ” ” | ” ” ” ” ”~ ” | ” ” | ” ” | ” ” ” ” ” ” | ” ” | ” ” } 7 ” ” ” ” ” | ” | ” ” ” ” ” | ” ” | 7 ” 0 ” } ” ” | 12-1 ” ” bid 0 ” ” ” ” ” ” ” ” ” ” 7? bh) ” ” ” ” ” ” 3? 9 ” ” ” ” 3) : bb | ” | ea ” ” ” | 1 ” ” ” th) ” ” 3° ” 2 |) ” ” ” 7 ” | ” 9 | ” ” ” a ie Oscillation Frequency in Vacuo 407273 407345 40740'3 40745°1 40754'7 407810 40782°8 40784:3 40799°6 40804:3 408065 408148 40816°3 40824°3 40841°2 40849°2 40862°7 40868°6 4087371 40876°6 408843 40894-9 40906°1 409275 409349 40944:0 40950°8 40963°5 40968°8 40975:0 40982-4 41001°4 41009°3 410182 41027:0 41033°7 41040°8 41056:0 4£1060°7 41067°5 41080°1 41090°8 411009 41117°3 411229 411249 411371 41141°0 41149°5 41155°7 41160°4 41187-1 41185°5 41196°5 412084 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 349 Wave- length Spark Spectrum Intensity and Character 2425°73 2425°41 2424-70 2424-49 2424°18 2423°28 2423°00 2422-75 2421-98 2421-82 24210 2420-1 2419-42 2418-7 2418-6 2417-91 2416°75 2416°54 241585 2415°49 2415-12 2414-16 2413-36 2412-57 2411°95 2411°72 2411°15 2410-59 2409°78 2409-43 2408:80 2408:00 2407-08 2406°73 240618 2405°89 2405°82 240498 240449 2403°92 2402:70 2402-37 2402-14 2401-45 2400-40 2399°31 2398°77 2398°05 2396°80 2395'73 2395°51 239498 2394°20 2393'35 2393'13 ke Or OT bo H bo & Be Ob Were wwob bebe i=] BB i=) Bb lomo” Pe eas NS Ni a any Haat ot a RO IROL Sat CO SS BB mee Woh At logon Irnon—continued. Previous Observations 2425-68 K.& R. 2424-22, 249325, 2422-73, 2421-79, 2421-02, 242039, 2419-49, 2417-94, 2416-68, 2416-00 ,, 241529, 241337 241245, 2411-79, 2411-16 _,, 241056, 240813 4, 240672 45 2405-02, 240448 ,, 240267 240223, 240160 ,, 240125, 240039, 239931, 2398-29 2395°62 oy, 239433, Reduction to | | Vacuum Oscillation Frequency in Vacuo 41212°5 41217°9 41230°6 412336 41238-7 41254-2 | 41259:0 f 41263-2 41276°3 ! 412979-1 | 41293-0 41308°4 | 41320:0 413323 { 413340 =f 41345'8 41365:7 | 41369°3 41381°1 41387°3 41393'6 41410-0 41423'8 41485-3 41491-3 41502:1 41515°9 41568-1 41576:6 41586-4 41607°5 41437:2 41447°9 414519 41461°7 41471°6 41531°8 41537°9 41547-4 41552-4 415536 41613:2 41617°2 41629-2 41647°4 41666°3 41675°7 41688:2 417099 417285 41732°4 41741°6 41755:2 41770°1 41773°9 50 REPORT—1898. Iron—continued. Reduction to Mare Intensity | Vacuum. Oscillation Spark and : Previous Observations | i | Frequency Spectrum | Character 1) Ree | cht, in Vacuo | | ' 2392°75 in 2392°70 K. & R. 080 | 12-4 | 41780°5 2392:27 In Ash » 3 417889 2391°59 4 2391:53 ee (ap pS 41800°L 2391°10 in 1 igs ” 41809°4 2390°92 In rhe “ 41812°5 2390°31 In | 99 Wee: 418232 2390-04 in 2390-03 " ee id Bete 418279 2389°51 1 ” ” | 418372 2388°71 7 238871 35 WO Bel” <3, Peat | 41851-2 2388-46 2 2388-42 9 Bef. sR 41855°1 238828 2 ” » | 41859°7 2387°51 3 : ” ” | 41872°2 2386:53 2b. | ¥ » | 41889-4 2385°10 2 2385°07 sy, ” 2 419146 2384:49 5 238448 ” ” ” 41925°3 2383°40 4 ” ” 41944°5 2383°17 2 | 2383°24 ” ” 125 41948°5 2383-00 2 | ” rH 41951°4 2382°13 9 2382715 » 222 BR ” ” 41966°7 2380-86 5 2380°82 _,, s ty | 41989-1 2380°35 1 ” 2 419981 2379°36 tf 2379°38 ” ” ” 42015;6 2379-05 1 cr er | 42021°1 2378°57 2 ” yo] 42029°6 2377:63 1 ” rr | 42046°2 2376:60 6n 237654 ne ” reas 4 420644 2373-30 6 2375°30 “A Af ‘an! 42087°4 2374-61 af 237459 ” ” ” | 42099°7 2373°82 8 2373°79 ree TIE Lite “h es 42013°7 2372-73 4 237265, sal » i) es 2372°50 In ” 35 et 421371" 2371-90 1b . * 3 421478 2371°52 1 237k ” ” ” | 491546 2371:07 In ” ’ 421626 2370°60 3 2370°56 + a te as 42170°9 2370-17 5n ” Pe || 42178°6 2369-33 1 2369°55 a ” a || 42193°5 2368°69 8 2368°66 “ uns 12°67 | 42206°4 2367-00 H 1 ” | ” | 42235°0 2366-69 3 2366°66 ” ‘ ” ” | 42244°] 2365°92 2n 2365°61 3; Dame |lenecne 42954:2 (2364-90) (4 2364'88 ay) OO Uae a a gl 422725 2364-00 | 3n 2363°81 ” ” ” | 42288°6 2363°68 | In ” / ” | 422943 2362-23 4 236211 i, > has 42320°3 2361-83 3 ” ” 42327-4 2360-42 5 2360°37 ” ” ” 42352°8 2360:08 5 2360-06 ” 9h] 99 42358°8 2359-68 2 ” | ” / 42366:0 2359-23 7 2359°16 F iithss, Ls v5) Be 423751 2358-43 1 ay fh op fe 42388:5 2357°10 3 3. il. oar 424124 2356°55 1 ” / ” i 42422°3 2355°50 2b 2355°37 o “+ ey 42440°2 2355°29 2 ” ” 424450 EE EE ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 351 IRoN—continued. = cat he to | ayve- / F acuum c ; length Intensity Previous Observations : eet ae Spark pis 1 in Trae z Spectrum Character mee = to) 235500 5 2354:93 K. & R. 0:80 | 12°6 42450:2 2354-59 5 » | 127 | 42460:7 2353°75 | 2b ” | » 42472°6 *2352°50 2n » | oo» 42495°3 2352712 | 1 ” | 42502°1 2351-84 il ” ” 42507°4 2351°31 } 6 2351-22 ” ” | ” 425168 2350°72 in 2350°50 ” ” ” 42526°5 2350°33 ln ” CE nl 42534°6 2349-45 In ” ” | 42550-4 234840 | 7 2348-28 ,, ‘385 R.] ,, ra 42569°5 2346-80 In ” ” | 42598°5 2346°37 In ” ” 42611°1 2346:0 in ” ” } 426130 2345743 6 2345°29 ” ” | ” | 42623°4 234440 5 2344:°37 a y ae 3) 42642] 2344-05 3 he ee si 42648°5 2343°58 9 2343'52 ” ‘57 R. ” 2 42657°'1 2342°36 1 ” ” 42679°3 2342-07 1 » ” 42684-6 2341-33 1 ” ” 42698:0 2341-04 il ” ” 42703°3 2340°55 Qn 234030 » | 128 42712°2 2339°50 3 ” ” 427313 2339°05 1 ” ” 42739°6 2338°09 8 233808 ” ” ” 42757°2 2337°65 1 9 ” 42765°0 2336°97 2n ” ” 42777°6 2335°55 2n ” ” 42802°9 2335°25 1 ” ” 42808°4 2334°5 lb 2334:83 ” ” ” 42822°9 2333°84 1 ” ” 42835°0 2332°88 8 2332°87 ” ” ” 42852°7 2332-62 i » ” 42857°5 2331°41 7 2331°38 ” ” ” 42879°7 2331°18 1 ” ” 42883°9 2330°60 in ” ” 42894°6 2330°17 ln ” ” 42902°5 2329°44 2 2329-67 ” ” ” 42916-0 232803 2 ” ” 42944-0 2327-49 6 2327-40 = an 12:9 42951°8 2326-95 In ef) 9 42961'8 2326-43 2 ” | ”» 42971°4 2325°80 1b owe Bea 42983-0 2325°65 2 ” ” 42985'8 2325-38 2 ee HE 42990°8 2324-60 In ” ” 43005°3 23232 1b A ” 430330 2322°43 1 3 43045-6 2321°76 2 ” ” 430582 2320°44 2 2320°42 49 fe nN 43082-4 2318-62 2 4 = 431181 2318-41 1 2318°23 9 _ 7s 431201 | 2317-40 2n 2317°32 a ie 43138°9 | * Double. 2313-38 231317 2312'10 2311:33 231017 2309-04 2308-80 2307-75 2307°37 2306-45 2306'06 230478 2303'87 2303°63 2303°42 2301°74 2301°50 2301:20 2300°48 2300°19 2299:27 2298-68 (2298-25) 2297-76 2296:96 2296°87 2296-72 22.96'3 2295°8 2294-68 2294-48 2293-89 2293-20 2292-90 2292°57 2291-69 2991-21 2290-60 2288'8 2287-65 2287°31 228410 2283-74 2283'3T 2279:98 2276-07 2274-13 2272°13 2271°87 2270-40 2268-91 226858 Intensity and Character Fee Yt te EC Pee Eg Pe eed CRS GS Pee i=] BO et ee cell el eel el ed ed REPORT—1898. TRon—continued. Reduction to | Vacuum Previous Observations a A+ Rin 0-80 | 12:9 ” ” 2314-10 K. & R. » | 130 931317, rae 231240 =, Ki “ ” ” 2309-04, : “4 ” ” ” ” 230635 ,, ¥ fe ” ” 230482, cA - ” ” 2303-52, oe 2301-:75 i, * % aie ” 2” 230020 ~—,, = ‘ 2299-30 7 ” ” 2298-24 fe ee 299785, “ i 2297-04 c ‘ ” ” | ” ” | 2296-23, :. et 229445 a Bie 9293-90, % E: ” ” 229956, i _ 229118 he lh ore 2290-61, ef . ” ’ 228770, » | 1382 298737 ag a - 298412 <3 & oF ” 228315 —,, re a 2980:05 sy, 2 a 227607 ~—iy, € 227409, » | 1R8 yt) ae ee | 227047 —,, al eee 226896, " > | Oscillation Frequency in Vacuo 43 166°9 431845 432013 43213°8 432177 43237-7 4325271 43273'8 433950 43399°5 433192 43323°4 43343°7 43351:0 433751 433932 43396°7 43400°7 43432-4 43436°9 434425 43456°1 43461°6 43478°6 43590°1 43598°3 435075 43522°7 435244 435272 435352 43544-7 43559'9 43569°7 43581°0 435941 43599°8 43606°1 43622'8 43632°0 43643°6 43677°9 43699°8 437063 43767-7 437746 437817 43846:'8 43922°2 43959°6 43998-2 44003°3 44031'8 44056°7 440671 wo Pes ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. le dea Wave- 3 length . Spark . Spectrum Intensity and Character Tron—continued. 309 Previous Observations 2268-20 2267°64 2267°14 2266°77 2266:32 2266-05 226465 2264-42 2263°30 2262°75 2262:36 2260-92 2260-20 2260:13 2259-62 2257:90 2257-00 2256'49 2955'82 2255:24 2254-42 2254-25 2254-14 2253°18 2251-97 2251-62 2251-03 2250°24 2249-20 2247-80 2247-00 2245-64 2244-38 2243-23 2242-68 2249-40 2241-90 2241-56 2240°63 ‘| 2239-70 ‘| 2239-18 2238-71 2238:33 2237-96 2237°66 2235 93 2235°58 2234-00 2239-19 2231-64 2228-88 2227-68 2227-55 2227-45 2997-93 1898. =] 5 RB Soros eet anon ae emer ak ey re ey gee eg ge Re RFF OIRO SDS RIS et te pm mh Fre ed Ree toh 2266°37 226451 2263°37 2260°83 22453 2249-9, K.& kh. ” Reduction to Vacuum Oscillation Frequency in Vacuo 44074-6 440854 44095°1 44102°4 44111-1 44116-4 44143°6 44148°1 44169-9 44180°6 44188-2 44216°4 44230°5 44230°8 44241°8 442754 44293:2 44303°2 443164 44327°8 44343°9 44347°3 44349-4 44368°3 44392-2 444187 44410°6 44426-2 44446:7 444744 41490°3 44517:2 44542°2 445651 44576°0 44581°6 44591°5 445983 44616°8 41635:3 44645°4 44655°0 44662°6 44670°0 446965 44710°5 44717°5 44749°2 447854 44896°5 44852°0 44876°2 44878°8 44880°8 44885-2 AoA 354 REPORT—1898. ® Tron—continued. Reduction to Wane. Tasty | -"Vacnne Oscillation aaa k and Previous Observations Frequency s pee Character 1 in Vacuo pectrum A fie 2224-55 1 0°80 | 13:7 44938°6 2293-56 2 " a 44980°1 229253 1 ie it 44959°3 2221-25 2 - ig 44996-0 2220-48 3 i 45021°6 | 2219-97 2 * * 45032-0 2218-90 2 45053°7 2217-15 1 rs - 45189°2 2215-88 In 2 fs 45115-0 2215°22 In a 13°83 45128°5 | 2214-20 In 9214-1 L. & D. ars 4. 45149°2 | 22913:74 3 hate e 45158°6 221119 1 4 ss 45210:7 2209'78 1 i i 45239°6 | 220918 2 icant 5, 45251-9 2208-54 2 * &: 45265°0 | 2206:68 1 . “3 45303°1 | 2206-30 2n az A 45310°9 1 9201-72 In » | 139 45486'1 2200°81 1 i me, - 45423°9 220044 1 22002 é - 45431°6 219886 In bs us 454642 2196-14 1 . » 45520°5 2192-30 1 | AAO 45600°2 2192-08 1 Nea 4 45604°8 2191-94 1 < af 45607°7 2189-12 1 3 ‘A 45666°5 | 2187-82 1 lame i 45793°7 2187-40 1 . ” 45702°4 2187-28 1 : 2 45704-9 2186792 i 2286'8 a ; - 45712°6 218656 1 if € 45719°9 2183°85 i 2283°7 35 os 45776°7 alaQep 1 Ps 55 a Lael 45845°8 2178-15 1 2278-0, Lae . 45996'4 2177-10 1 ONG GEO' = ss 45918°6 2176-68 1 ee ‘ 45927-4 | 217554 2 Wes a 459515 | 2174-95 1 Nes 4 as 45963°9 2174-77 1 hers S 45967'8 | 2173-07 1 x . 46003:8 2167-90 1 oH. tae 461134 2167-50 1 2167-4 4, i é 461219 216681 Z L i 46136'6 2164°40 1 1. es n 46188:0 2162-08 2 i is 46237°6 2161-18 i “ on 46256°8 2152-42 1 5 glee 46445-0 2151-9 In < a 46455°9 2151-15 1 “ : 46472'5 2150-67 1 “s 5 46482-9 2147-74 1 » | 144 46546:2 2146-06 1 Bs x 46531°6 2136°50 1 :; 14°5 46791°0 2136-00 1 = a 46812-0 9) ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 355 Tron—continued. Reduction to | pee: Intensity Vacuum Oscillation ene ; and Previous Observations | Frequency Spar Char: : 1 | in Vac Spectrum aracter ie pe acuo if | i A i=) oS ae 2097-60 1 | O80 | 14:8 | 47658°7 2097-48 1s is ge | 47661°4 2087:54 ii ois 14:9 | 478884 : 2079-00 1 Fe 15-0 | 48085:0 2068°25 In 5 15:1 | 483349 TunestEN (SPARK SPECTRUM). ‘Exner and Haschek : ‘ Sitzber. k, Akad. W. Wien,’ civ. (1895), cv. (1896), evi. (1897). 1 Wave-leneth | Reduction to | | ae P Vacuum | Natt Spark See Previous Measurements , ——____| Tasers (lowland Character (Angstrém) | i D4 in Vacuo | A 4844-7 1 1:33 3) -5°7 20635 4694-1 2n 1:29 | 59 21297 4692 0 2n 1:28 a U 21307 4687-9 1 a 9 21326 4683-7 2 5 et 21345 4682 § 1 i laienae | 21349 4681-4 1 Sols 21355 4680°8 6 4680°6 Thalén acy staan! 21358 4679°8 1 sy is 21362 4679°3 1 3 ea 21365 4678°8 1 ne Weer d | 21367 4677°9 1 “, 3 21371 46769 1 ar eer 21376 4675-4 In Oe Sr ore 21383 4675°2 In ah ee | 21383 4672-4 1 a . 21396 4671-9 1 x 21399 4671°6 1 - 21400 4668°7 1 4 | 214138 4666-0: 2 i. sie 21425 4665°0 In eet Dred 21430 4664-1 In poles ea 21434 46632 1n Mp) Fae | 21438 46621 1 epee A pau 4661-7 1 “ za 21445 4661-4 1 7. saa 21447 4660°0 6 46606 ,, StS eae 21453 4653°3 1 46596 ,, Ly See, age at 21461 4657-6 © 4 Ht aeeea iy 21464 46555 In ee Nis 21474 4654-4 In Nao 7 i See te 21479 4650°9 2n ee Me eye 21495 4646°3 1 ie 93 | 21517 4645°3 1 trae tas ol 21521 4645-1 1 HA een 21522 4642-7 2 Eee) al 2 | 21533 4640-4 1 eA are 21544 AAQ 356 REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. | | Reduction to sheik | Intensity : a . is Vacuum Oscillation (Rowland) | aracter gstro ae a in a0 | x {i — fom 46380 In 1:27 | 5:9 21555 46374 in ” ” 21558 | 46362 1 * 21563 46348 2 5 6:0 21570 4633°3 In * 5 21577 4632°7 in ” »” 21580 4631°8 In + x 21584 | 4629:9 1 7 4 21593 | 4629°5 1 ; y ” 21595 i 4629-0 1 - + 21597 | 4628°6 1 7 3 21599 1 4627'8 In ” 7 21603 | 4627°4 In 9 5 21604 | 46271 In ” ” 21606 | 4626°3 In 4 a 21611 | 4625°4 In - S5 21614 | 4623°9 In ~ a 21621 | 46235 1 a 21623 | | 4620°8 1 ss ‘ 21635 : 4616'6 In 1:26 x 21655 | 4615:0 1 3 5 21662 | 4613:50 4 ” ” 21669'5 | 4610-0 2 3 55 21686 / 4609:0 In = + 21691 | 4606°6 il i - 21704 | 4604:8 2 ‘3 . 21710 | 4603°5 1b 1:26 | 6:0 21717 4601°6 1b ts x 21726 4601:0 1 ” ” 21728 | 4600°6 1 ms i 21730 - 4600°1 2 a * 21733 | 4598-4 1 F 4 21741 4592-60 4 wear es 217682 458892 4 S. 5 21785°6 4587°8 In x 7 - 91791 4586°9 2 - a 21795 | 4586°1 1 se Bs 21799 | 4585°5 In i Fe 21802 ' 4584:8 In ess i 21805 4582'2 1 ieee a 21818 4579°8 In 1:25 ns 21829 | 45783 2 m = 21836 1 4575-2 In a os 21851 | 4572-8 1 a 21862 |. 4572°6 1 ~ A 21863 | 4571-9 1 e s 21871 | 4570°80 4 a a 21872°0 | 4569:3 in 3 3 21879 | 4567-6 - 4n ie 21887 | 4567-3 In 3 4 21889 | 4566°3 1 * i 21894 |. 4565-4 1 - i, 21898 45641 1 61 21904 4563°7 i ¥ 21906 45621, . x 21914 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. TUNGSTEN (SPARK SPECTRUM)—continued. { Reduction to | Wave-length | Vacuum Spark Intensity | previous somnentt Oscillation geen | cattle | nesta) ae | (Rowland) | Character a ee ies in Vacuo | A 4561°6 1 1:25 61 21916 | 4560°4 1 a fe 21922 4559°0 1 ” ” 21929 4556°8 1 sf * 21939 | 45553 in a “ 21946 ' 4554°22 8 ” ” 21951°6 4552°6 1 3 3 21959 | 4551°9 2 5 at 21963 4550°4 1 ” ” 21970 4549°8 In 9 ” 21973 4546°5 1 $3 ra 21989 4545°6 In 55 or 21293 45446 In 5 % 21998 4543°6 2 fy BS 22003 4542°9 1 1:24 aa 22006 4542°0 1 7 35 22011 4540°3 il ” ” 22019 4539°8 fe ’ ” 22021 4536°6 2 35 a 22037 4535'0 2 ” ” 22045 4534°6 2 ” ” 22047 4532°3 1 ” ” 22058 4530°5 1 ” ” 22067 4529'8 u e ie 22070 4528-6 In ” ” 22076 4527°3 i ” ” 22082 4522-9 In » ” 22104 4520°0 In 8 22118 4519°1 al ” ” 22122 4517°4 1 A * 22131 4516°5 in 5 a 22135 4515'8 Jn } 4 22138 — 4514-1 1n Fe 5 22147 45131 2 x ie 22152 4512°8 2 "i = 22155 4511°0 1 oe FF 22162 4509'6 1 re % 22169 4509°3 1 Ps . 22170 4508'9 1 5 a 22172 4508'4 1 7 +) 22175 — 4504°8 2 1:23 as 22193 4504:0 2 3 AS 22196 45031 1 5 - 22201 4502°3 1 os 22205 — 4500°3 1 = on 22215 | 4500-2 1 =p ee 22215 ~A498-6 * 2 ” ” 22223 | 4497-8 1 - 3 22227 — 4497-0 1 aa 6:2 22231 | 4496°4 In a . 22234 4495-4 1 = ¥ 22239 4494-7 1 7 % 22242 4494-0 2 3 * 22246 44924 1 ms i 29954 1 ” » 22266 4 4490-0 308 REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. | Reduction to | Wave-length | tntensity | ’ Vacuum Oscillation Spark and Previous Measurements | Frequency Spectrum Character | (Angstrém) | 1 in Vacuo (Rowland) A+ a Anta {== = ——. 6 os ee oe | at i 4489°1 ove || 123 | 62 | 22970 4488°5 1 7 al 22273 | 4487°8 ] | he Ws 22277 4487°5 In a , 22278 4485°3 1 Sse eae 22289 4484°33 6 ” ” 22293°7 4482:0 1 = = 22305 4481°5 2 mee . 22308 4480°5 il : +4 % 22314 4479-0 1 | 3 - 22320 44786 1 | ~ =f 22321 44760 1 an 4 22335 4475°7 1 | a “ 22337 4475:0 In Mo 7 a 22340 4474-1 2 a a 22345 } 4473-0 1 a bs 22350 4472°6 1 . m 22352 44720 1 s 5s 22355 4471°6 1 | : Fw il 22357 44699 1 Bs » 22366 4468°8 2 1:22 a 22371 4466°9 2 RS a 22881 4466°5 2 = 5 22383 4465°8 1 7 pee 22386 4463-5 1 5 “5 22398 _ 4463-1 1 é. se 22400 4462°6 il 3 7 22402 4460°6 2 a D 22413 4459-3 1b e c 22419 4.4584 1 is ‘ 22424 44582 1 3 + 22425 4456-2 i : - 22435 4454-9 il Pa ey 22441 4452°3 1 x . 22454 4450-4 1 a ;, 22464 4449-9 1 ~ :. 22466 4449-0 2 5 oc 22471 4445-2 2 $5 i 22490 4444-6 1 “ ss 22493 4444-2 1 5, + 22495 4443-1 il . as 22501 4442°8 1 is aS 22502 4442-5 1 5 -b 22504 4441:9 2 5 - 22507 4439°8 1 a eee 22518 4439°0 2 eas ita 22522 4438°5 1 ae Uacens 22524 4437°6 1 és + 22529 4437-0 2 Sab Maes 22532 4435°8 1 esse, 0 es 22538 4435-1 1 Mo Ke) | 22541 4433°7 In ea Ss ee 22549 4433-1 1 [Se tea 22552 4432-2 1 [7-915 aa 22556 44309 | In tag Gi 22563 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 359 TUNGSTEN (SPARK SPECTRUM )—continued. , } Reduction to _ Wave-length Intensity . | Vacuum Oscillation | | Spark and Previous Measurements | Frequency (Gowland) Character (Angstrém) gar | ie in Vacuo | t Xx | : | oa = ae A ee ae 4429-0 1 | 121 | 63 22572 4428-6 1 | nl Last 22574 4427-6 1n ee eae 22580 : 4425-6 1 eat || Bo 22590 4425-1 1 * | ‘5 22592 4423-8 3 coal. Sosy 22599 t 4429-8 In ee ee 22604 4422-5 1 a Weal Pay 22605 4421°9 2 ies Rall ie 22609 4421-1 1 Hundt 22613 4420°6 2 re See 22615 4419-4 1 De ae 22622 4418-9 1 mig ry ae 22624 4418-6 1 a 7 22626 4415°8 1 ay ee 22640 4413-4 1 eee ee 22652 4413-2 1 i i 22653 4412-4 1 Mo ef x 22657 4411-5 it } ” ” 22662 4411-1 1 iets o 22664. 4410-0 1 x ct 22670 4409-6 In ae tc 3 22672| 4408-8 1 = a 22676 t 4408 42 4 sala ty 22677°6 4406-1 2 rm ae 22690 i 4404-8 1 ow ee 22697 t 4403°5 1 - 22703 | 4402-8 1 | in Fos = 22707 | 44003 in: | bas % 22720 4396-9 1 | x im 22737 4395-1 1 Cobia Ge 22747 4394-5 1 j 2 22750 4393°8 2 120} Gis 22753 4390-9 | < ie 22768 4389-9 2 S me 22774 4387-9 In eae a are 22784 4387°5 1 Re vine: 22786 4386-7 1 ss 4 22790 4385-01 4 Bs fe 22798:7 | 4383-6 4 is - 22806 4381-8 In , f 22816 4380-1 1 Fa ;, 22825 4379°3 1 s > 22829 — 4878-72 4 = “ 22831-4 — -ABIT-5 In ual a, 22838 (4373°8 In et 22857 4373-0 In ie 2 22862 4372°5 2 4 is 22864 _ 4371°8 1 :§ , 22868 4370-8 1 A 2 22873 4368-7 1 BPE 22884 4366-20 4 ome 64: 22886°3 ‘4364-90 4 As ee 22903°6 43616 2 ML, cass 22921 4361-1 1 : ae 22924 350 Wave-length | Spark Spectrum (Rowland) 4360-0 4359°3 43586 43580 43565 4355°2 43542 4348-23 4347-0 43463 4345-9 4345-1 4343-2 4342-4 4341-3 4339-5 4339-1 4338-6 4338-2 4335:70 4332-0 4330°7 4326-9 43251 | 4324-6 | 4329-9 | 4321-5 | 4320-4 | 43186 | 43168 43163 4315°3 4313-1 4312°3 ! | } 43123 4311-0 43102 43100 4309-3 4309-0 4308°0 4307:00 4306°3 4305'S 43056 | 4305:1 | 4303-4 4302-6 4302-27 4301-1 4299-0 4297-6 4297-2 4295°7 4294-77 TUNGSTEN (SPARK SPECTRUM)—continucd. REPORT—1898. Intensity and Character Previous Measurements (Angstrém) Reduction to Vacuum a+ | 1 — t=] i=] Ll ce ee ce SI ol ol cre cl el cel el I ol cl BB 4302-0 Thalén 4295-0 = Oscillation Frequency in Vacuo 22930 22933 22937 22940 22948 22955 22960 22991-5 22998 23002 23004 23008 23018 23023 23029 23038 23040 23043 23045 23057°9 23078 23085 23105 23115 23118 23127 23134 23140 23150 23159 23162 23167 23179 23181 23183 23190 23195 23196 23200 23203 23207 23211°5 23216 23218 23220 23222 23231 23236 23237-0 23244 23255 23263 23265 23273 232776 _ ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 361 TUNGSTEN (SPARK SPECTRUM)—continued. Wave-length F Reduction to | i Spark ee Previous Measurements Vacuum ees ome | ectrum Aicntavs eae “requenc (Rowland) oe iscsi) ee 1 in Naa | A 4294-1 2 ae = | 4293-0 i 118 | 65 23282 4292°8 in ” 2 23288 ) 4292-0 er » 2 23289 / 4291-5 In ” ” 23293 | 4290'1 1 ” ” 23296 ; 4289°3 1 ” ” 23303 4288-4 A ” %” 23308 42870 m one ee 23313 4286:0 vA ” ” 23320 4285-0 2 ” ” 23326 42838 ] ” oe) 23331 4283:0 ln ” ” | 23338 4282-0 al ” ” } 23342 4281-4 : In ” ” | 23348 4280°5 In ” ” 23351 4279-0 1 17} 4 { 23356 4278°5 il ” une 23364 42778 1 Meal Meee ets 4277-4 1 117} 65 | 23371 4276-92 4 Mo ” , 23373 4276-0 1 ” . 233748 4275-65 4 » s 23380 42750 i ” ” 23381°8 4274-70 4 ” e 23386 4273-7 2 - » | 28387-0 4272-3 1 » » | 23893 4271-8 1 ” 2 23401 42709 il ” 9 23403 4270-8 1 > 23408 4269-9 2 » oe ie 4269-52 ; oH ae = & 93414 4268°8 . 4269°0 Thalén . - 23415-3 42681 1 ” ” 23420 4267-9 1 ”» i 23424 ‘ 4266-6 2 ” ory 23425 4265-0 1 » 5 23432 4263°50 4 ” ” 23441 4262-4 1 » . 23448-4 4260-42 4 ee ae 23455 4259-9 1 is : 23465°4 4259°52 4 3s = 23469 42585 1 » ” 234703 4257:3 1 ” ” 23476 4257°0 1 ” ” 23483 4255°6 1 ” : 23485 4254-3 3 . ‘. 23492 4254-1 al 2 ” 23500 4252°6 In ” ” 23501 42518 iin See 66 23508 4250°8 1 ” oa 23512 4250-1 In ” ” 23518 4249°5 1 ” ” 23522 4248°8 1] ” ” 23525 4248-2 1 ” ” 23529 be) ” 23532 362 REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. | Reduction to | . length . Beli [Wan an Intensity | Preyi ious Measurements | 2 Ee Oscillation P d oe | Spectrum Ch ae (Angstriim) fe [4 Frequency (Rowland) aracter Bases bo in Vacuo | | | | |] | |} — | 4247-6 1 117) 66 23536 4247°3 1 : ss 23537 4246-0 1 ‘i | 23545 4245-6 1 ol ae 23547 ) 4244-45 4 bap Ree 23553°6 4243°8 1 ret ame 23557 : 4243°4 1 ee, lee 23549 | 4241-50 4 on es 23570:0 4241-0 1 dl tis 23572 1 4240°8 1 nol wh. Pegeye 4240-4 1 a: 2 23576 4240-1 il e x 23577 | 4238-6 1 * is 23586 | 4236°6 1 ed awk eee 4235°5 il 5 is 23603 4234-4 2 oy me 23609 4233-0 1 oe 23617 4232°6 1 Rote hae 23619 | 4231-9 1 Be a 23623 | 4231°8 1 lees fs 23624 4231-4 1 = ‘ 23626 42313 1 | s i, 23626 , 4230°0 In | _ = 23634 | 4229'1 1 | = A 23639 ae 5 1 | ., es 23642 227-6 1 % ts 23647 120. 8 6Ca x ie 23652 | 1296-4 “| < s 23654 42257 1 3 % 23658 4225-0 2 [ey : 23662 4224-9 2 * a 23662 4224-1 da. 4 - 23667 4222-2 2 7 * 23677 4222-0 1 ¥) “ 23678 4221°5 1 ao at 23681 4220-7 it i. 5 23686 | 4220°5 1 Key 23687 . 4219-50 4 Hi i tie: 236929 4219-2 1 ee L's 23694 | 4218-7 1 is =] 23697 4216-0 1 a 7 23712 4215-60 6 5 e 237148 | 4215-1 1 i z 23717 4214'5 1 ., % 23721 4214-0 1 - i 23723 42135 1 ie e 23726 42129 1 . . 23730 | 42115 1 Pann o 23738 | 4210-4 1 : | x 23744 / 4210°3 ] ” ” 23744 H | 4209°7 In | ot eka’ op 23748 420712 4 ee 23762°6 4206°3 2 ia ee 23767 4205°6 Ins 3 ts oe 23771 | 4204-52 4 | game eae 237773 { NN | Reduction to | | Wave-length | | ; | ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Spark Spectrum (Rowland) 4203°8 4202-0 4201°3 42009 4200°5 4200°1 4199°7 4198-9 41987 41983 4197°9 4197-4 4197°3 4193-9 4193-0 4189°3 4187-0 41860 4185°5 4183°7 4183°6 4183-0 4182°6 41815 4180-4 4178-7 4178-0 4177-0 41769 4176-0 4175-70 4175-2 4174-6 4172-9 4172'1 4171-9 4171-23 4170:60 4168-80 4168-3 4166-9 4166-2 4165-7 4164-9 4164-0 4163-0 41616 4161-0 4160-4 4160-0 4159-0 41571 41548 4153-2 4152°6 TUNGSTEN (SPARK SPECTRUM)—continued. - Vacuum Intensity | Pyevyious Measurements | cad and 9 ng | = . (Angstrém) | Character ie Dy Oscillation Frequency in Vacuo D 6°6 : 115 | Peal amlan a Varese ea a ee =] =] clara ll hag ~ pa aaa DeRReRee =) ee =) i=} fe ee cel cell cell eel 9 ol: oll sl oe x 6B BRED ee eee 23781 23791 23795 23797 23800 23802 23804 23809 23810 23812 23814 23817 23818 23837 23842 23863 23876 23882 23885 23895 23896 23899 23902 23908 23914 23924 23928 23934 23934 23939 239414 23944 23947 23957 23962 23963 23967°0 239707 23981°0 23984 23992 23996 23999 24003 24008 24014 24022 24026 24029 24031 24037 24048 24062 24071 24074 363 REPORT—1898. ois) i=) = TUNGSTEN (SPARK SPECTRUM)—continued. W. casae ‘ Reduction to ave-leng 5 Spark Intensity Previous Measurements Mecuhes Oscillation Spectrum eae (Angstrém) | 5 Frequency (Rowland) Character Nee as in Vacuo 4151°8 1 TAs) 1G 24079 41511 1 8, ay 24083 4150°6 1 3s < 24087 41500 1 be wo 24089 4149°8 1 is “3 24091 4149°5 1 # ee 24092 4149°3 In is ie 24093 4148°3 1 > 8 24099 4146°8 2 :, - 24108 4145°3 2 ; és 24117 4144°6 1 rf a 24121 4143-1 1 “ » 24130 4142°3 2 * oe 24134 4141°6 1 in “3 24138 4140°9 1 = 3 24142 4140-4 1 is 3 24145 41401 i E. af 24147 4139°3 1 rs 24152 4138°5 1 Xs s 24156 4138°3 1 - e 24158 4138-1 1 2: 2 24159 4137-63 4 ve 241616 , 41375 4 cs - 24162 4136°5 1 a a 24168 4134-7 In a % 24179 4133°6 2 ‘ € 24185 4132°3 © 1 55 of 24193 41380°9 1 PIS 5, 24201 4130°6 1 me Yi 24203 4130°2 1 ii 24905 4127-0 1 a 24994 4126°9 2 fa : 24224 41252 1 sf Ae 24934 4123-0 1 ; ‘ 24247 4122-7 1 -. 5 24249 4122:0 1 A a 24253 4120°8 1 . be 24260 41190 1 s 3 24971 4118-22 4 es 24975-5 41148 1 # < 24296 4114-2 2 is < 24299 4113-9 1 a ., 24301 41124 a i = 24310 41118 2 s x 24313 4110°6 2 ze f. 24320 4109-90 4 3 5 24324-7 4108°5 1 f - 24333 4107°9 1 es 3 24336 4106°8 a S 3 24343 4104:0 1 - 5 24359 4102°90 6 - #3 243662 4101'8 1 3 24373 4101-0 1 3 ie 24377 4099-2 2 _ 69 24388 4097-2 1 7 * 24400 ON WAVE-LENGTH TA = BLES OF THE SPECTRA OF THE ELEMENTS. 365 TUNGSTEN (SPARK SPECTRUM)—continued. ifave-Tength ; Reduction to Spark Intensity | Previous Measurements Vacuum illati eran na (Angstrim) Lan a Oscillation (Rowland) Character 7 1 Hrequaney Ree ane in Vacuo A 4096-6 69 | eg bs 1.13 6:9 24403 4094:3 In ET cos ae 4093'3 1 Heit eres rete ; 112 - 24423 2091-3 1 ” ” 24428 4091-2 1 Nag) ots iE 4090°8 1 ” ” 24436 4090°3 1 is is ine 4089°6 i ” » 24441 40889 5 ” hod 24445 40885 = ” ” 24449 4087°6 i ” ” 24452 40871 1 “ mr te ~ ” 3 24460 4083'9 tna ” ” 24476 40831 5 ” ” 24479 4081-45 4 » ” 24484 4081°3 1 ” ” 24494:°2 Peas : : - 24495 40791 ‘i » ” 24506 4078°3 1 ” ” 24508 4077-9 > » ” 24513 4075°7 i ” ” 24515 ye ” » (| 24589 othe : " : 24544 4070'7 2 ” ” 24544 4070-03 6 apn aris one : ¢ 7 245629 4065°5 ; ” ” 24581 Gene : > = 24590 4063'8 1 ” ” 24593 4060-9 7 ” ” 24601 ae ; r f 24618 4059-2 In 4 ‘ Fieae 4058-0 1 ” ” 24628 4087°5 i ” ” 24636 fora ; Hota 24639) fore i a) te 24643 40552 1 ” ” 24649 4033° 1 ” ” 24653 lances i EEL | oy 24663 ale ; * - 24669 4050'1 te ” ” 24675 ie : etl at 24684 as : “: 24694 ate : ‘A ~ 24696 ecb 7 ‘2 : 24704 4044-1 1 ” ” 24710 0 4042.5 1 ” ” 24720 4041°7 1 ” ” 24730 4041-2 1 fi ip See 40407 ; 9» i" 21738 | 4040-0 1 » ” 24741 ” ” 24745 366 REPORT—1898. . TUNGSTEN (SPARK SPECTRUM)—continued. f 3 Reduction to | | ve- . m x 5 i bier st inieuete Previous Measurements ee Cuelistion ’ Spectrum itenoter (Angstrém) 1 nace! (Rowland) A+ ar “te EN. = | ee | 4039: 1 111 | 7-0 24749 : 4037°8 1 5 hf 24759 | 4037:0 1 :. * 24764 40353 1 nd . 24774 : 4033°9 A = . 24783 | 4032'5 In a ‘ 24792 : 4031-6 1 4 * 24797 ! 4031-4 1 3 » | 24798 4030-0 1 3 S 24807 4029:7 1 | a / 24809 4029-0 1 . d 24813 4028-9 1 i; i 24814 4028-4 In a a 24817 4025-6 1 1 ee 24834 402571 1 iy 24837 ; 4024-9 1 | 24838 4022-8 1 ‘3 . 24851 4022-1 1 a 2 24856 4020-8 1 Sa 24864 4019-7 In s “a 24870 4019-3 2 , : 24873 4017-0 1 a < 2488744 > | 4016-2 1 3 i 24892 4015-32 4 1:10 - 24897°6 | 4013-9 1 " fe 24906 4013°8 i : . 24907 | 4013-2 1 Ea 4 24911 4012-2 1 > i" 24917 4012-0 1 s x 24918 | 4011:8 i fe Fs 24919 4011-1 1 > 35 24924 | 4011-0 1 x . 24924 4010:3 1 if is 24929 4009-7 1 z 24933 4008-90 8 > » 24937-5 4007-0 1 i, id 24949 4005-7 1 a ss 24957 4005-3 1 if . 24960 4004-1 1 iY . 24967 4003-8 1 : 71 24969 | 4002-8 1 5 3 24976 4001°5 1 a o 24984 4000°7 1 a 24989 3998-7 1 ees 25001 3998-2 1 | - is 25004 ) 3997-8 1 :. . 25007 | 39973 1 A i 25010 3997-1 1 af . 25011 3995-0 A = + 25024 3993-8 1 if ‘ 25032 3992°5 1 4 _ 25040 3991°3 1 rene” (eA 25047 3990°5 1 a Vow 25053 3988'8 af 3 :. 25063 | 3988°5 1 ” } ” 25065 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 367 TUNGSTEN (SPARK SPECTRUM)—continued. a acth, | Baction to ave-len. : j a F } Spark Tyensity Previous Measurements i Quel tation \ Spectrum = (Angstriim) Re eM (Rowland) Character | ao At ses in Vacuo es 39880 i Pte1O) ti Tek 25068 | 3987°5 1 a re 25071 | 3987-1 1 nee 5 25074 ae Hi eae s 25079 : me Mm 25088 3984-2 1 eae FS 25092 3983'40 4 ie x 25097'1 Sale 2 Vos _ 25114 980-0 1 ba a 25119 3979°3 4 eee 2 25123 3977-8 1 if is 25133 39765 In i ey rs 25141 3975°9 1 | 1:09 a 25145 39755 1 ee 3 25147 3972°5 1 - 53 25166 39107 ‘ no Pa hgenge i } “ 99 177 | 3969°3 1 a * 25186 39651 6 Ue 4 25213 3964-2 1 ia 25219 ) soe1-7 ; an eels ee 3961- x i 25235 3960°8 1 3 7 25240 3960°1 In a * 25245 3959°5 In es “; 25249 | 3958-9 1 ve a 25253 3957-6 1 3 x 25261 3957-2 1 = is 25263 39557 2 i 72 25273 3953'8 1 al ec 25285 | 3953'5 1 = FS 25287 3953-2 2 i a 25289 3953'0 1 ” ” 25290 | 3952'3 1 ee ee 25295 3051-1 ; sa Pg as es . 2 | 3950°3 2 ‘pee ae 35308 . 3948'8 1 leer 25317 3948°3 1 a a 25320 3046-5 i os lacey | arse ; e 5332 3945-0 2 Ks * 25342 | 3944:3 2 x “ 25346 | 3942-5 1 ey es 25358 3941-7 i eur fe eeane ie . = nA 25363 394171 1 We * 25367 3940°6 1 - * 25370 rs io) ies 3937-2 2 . i 95392 3935°5 2 1:08 a 25403 3935:2 1 7m i 25405 3931-7 ° 1 A es 25427 393171 il =. is 25431 REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. | | Wave-length | nase Reduction to Bececite | and y Previous Measurements i ccaicses Oscillation (Rowland) | Character (Angstrém) 1 Hneanency Nee LA in Vacuo ; | rN 3930°7 1 me, “ie » 3930°5 i aie she Bere 39280 1 ” W 25435 3996-2 1 ” ” 25451 3995'3 1 ” Fema 25463 39249 | 1 ” ” 25469 3994-6 1 ” ” 25471 | 2993-1 1 ” ” 25473 | 3922°9 1 ” ” 25483 ceieeine | 21 i 4s 25494 3918-5 1 » ” 25511 29178 1 » ” 25513 3917-6 1 ” ” 25518 29155 on ” ” 25519 39143 In » ” 25533 3913-8 1 ” ” 25540 | 3913-5 1 at Cai 25544 | 3913-0 1 ” ” 25546 3911°5 1 ” ” 25549 3909-4 1 ” ” 25559 3907°5 1 ” ” 25572 39061 1 , ” 25586 3906-0 1 ” ” 2559¥ 39058 1 ” “fi 25595 3904-2 1 ” ” 25596 39035 1 oe ” 25606 39031 1 ” ” 25611 | 3902-0 1 ” ” | 25614 3901°5 1 ” | 25621 3901:0 1 ” ” 25624 3900-0 1 a a ere 3899-0 1 ” | 25634 3898-2 9 ” 3 | 25641 3897-07 A ” ” 25646 3895'8 In oe 4ds. sae Re 1:07 |) 5 25662 3893-7 1 ” ” 25672 3893-0 2 3 ¥ ae | 3899-4 1 ” ” 25680 3891-0 1 ” » 25686 3889-5 os ” ” 25693 2888-7 iy ” A 25703 3888-2 1 ” ” 25709 3886-9 1 ‘s 4 rt | 3886-5 i . i 25720 | 8884:2 1 t i ee | 3884:0 1 th] ” 25738 | 38835 in x F pale 38827 In se ae pp 3881'50 4 ee oe Beans i * ‘3 25755°9 3879'7 1 4 4 aul Bera 3 < 25768 | 38792 ‘i 4 Fs 25770 rr 25772 “ , ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 9369 TUNGSTEN (SPARK SPECTRUM)—continued., } Bel ; ie he to ave-length . acuum ee Shark” py Previous Measurements |. Oscillation Soe Chaater (Angstrim) 1 one (Rowland) } A+ re Be Chie 3873°7 1 1:07 | 7:3 25775 88783 1 7 : PAY Ait | 38779 i i “A 25780 38775 2 2 ” 25783 3876°2 In i ; 25791 38760 2 Ff =“ 25793 38747 2 Fe he et) 25801 3872.8 2 al en ee a n ” ” 25 88718 In ” ” 25821 3870°8 in Fi We ag 25827 3869°6 In ce ae 25835 3868°7 1 el asta 25841 8868-05 4 Bee ears 25845°5 3867°5 1 awl es 25849 3866:°2 al sh or 25858 3865°5 1 al eee 25863 3864-6 2 Waa fips 25869 3863'8 1 Acer or aed 25874 3863-0 1 en eae 25880 3862°7 1 Shee tse 25882 3861°3 1 eel es 25891 3861°2 1 ie 4 een 25893 3860°1 2 Py ae 25899 3859°5 2 5 * 25903 8859-0 1 - % 25906 3857°6 1 Rita RE 25916 3857°5 ~ 1 a py 25917 3857-0 2 ” » | 25920 3856°6 2, TOG sii yy 25923 3830°7 i he ar. aes O° ” | ” ae 3895'5 1 x is 25930 3850 i sal tee ee 3854" uf 7 1 2594 3853°0 i zs f on 25947 385L-70 4 Fi % 25955'3 38513 1 5 Fe 25958 a 1 oF 0 ae . 2 PF 50 2598: 3846°32 4 eee i Wes 25991°6 3846°0 1 Sy rates 25994 3844-5 i ia. PAW Los 26004 3843'S 1 sem We bdes 26009 3843'5 1 a eer 26011 3842-6 2 a eet 26017 3841-2 | In je Meas Wael Ohss 26027 3840-5 1 a ah 26031 3839-4 | 1 al, Nr dl 26039 8838-6 2 Saal Gas 26044 3838-1 1 ‘ ae | 26048 3837-9 1 al ary 26049 ee 2 Poet cerns ft 26052 cf 1 Pe J anne 26057 33800 | In 5a lit ene 4 26062 1898. BB 370 REPORT—1898. TUNGSTEN (SPARK SpECTRUM)—continucd. Wave tenet Tuten oe to | Suecneie and Previous Measurements hvathes wegen Sheers eee 7 (Rowland) | Character (Angstxiim) x, | |) Veco | 1 a ig nN | | 383513 £ ee = 3834-4 1 1-06 | 73 26067-4 38343 1 | ” | ” 26073 8833°1 it ” | ” 26073 3832°8 | 1 | ” ” 26082 38325 | 1 | eae 26084 3830°9 In | ” | ” 26086 3830°7 1 } ” | ” 26097 3830°4 l | | ” | ” 26098 | 3830°0 1 Naeem th 26100 | 3829°3 1 ‘ EO AP oes 26103 | 38281 ee aes | fata cl 26107 | 3827°4 | lb | 1 193 26116 | 38263 | ee aie 26120 . 8825-6 1 Et | eeeeD 26128 | a 3824°6 2 | op) MN SSaetesl 26134 tg 3823°2 2 | » | oo” 26140 i 3823:'0 1 | ” ” | 26149 3822°3 | 1 en | 26150 3821°8 | In ” | ” i 26155 38206 | 2 at he 26159 38192 1 ” ” 26167 381971 1 ” | ” 26176 | 38180000 | Ine” | «| » 26438 3780°91 4 4 oR ” 26441°3 37783 J. | ” » 26460 3777-5 2 | ” ” 26466 B7T4:3 2 ” ” 26488 3772°6 1 | 9 75 26500 3772°2 i ” ” 26502 37700 1 ” ” 26518 3769°4 1 ” ” 26521 3768-62 4 ‘a » 26527°4 3768-0 1 ” ” 26531 3767°5 1 ” ” 26535 37673 1 ” ” 26536 3767-0 1 boy ” 26538 3765°5 1b | ” ” 26549 3764-6 af | ” ” 26555 3764-0 1 | Pas * 26559 3763°2 1 ” ” 26565 37617 1 or ” 26576 37615 1 oy ” 26577 } 37605 Diet) ene 26584 ) 3760°3 2 . . * 26586 | 3759°3 1 ” ” 26593 3758-4 1 ” ne 26599 3757-0 on | re ae 26609 37550 1 | oo» ” 26623 37549 i i ” ” 26624 3753°T 2 3 ” 26632 37533 1 i ” ” 26635 3751°5 1 ” ” 26648 3750°8 1 " ” 26653 3748°4 it } a 5 26670 8747-9 1 Ko 26674 =«~BT47-6 1 / Ls, ) 26676 3747-0 1 | oo” 4 26680 3745:70 4 Ve es a 26689'8 7 ST44-4 a | ” ” 26699 x 3744-2 1 ” ” 26700 _ -BT43°5 1 | . 3 26705 87427 1 i ” ” 26711 3741°9 4 | ” ” 26716 | BB? oe REPORT—1898. TUNGSTEN (SPARK SPECTRUM) —continucd. | | | Reduction to fps Intensity ne Pn SS Tae _ | Vacuum Oscillation | Spaatens and | rev it fa aan a Frequency | ) ‘ 5 = Anestrin i / | (Rowland) Paarere | 8 ie oveet eae in Vacuo ) | ae | 3739°7 Tee | | 1-04 | 75 26732 3739°3 1 |» ks 26735 3738 9 rc} a - 26738 3737°1 Bo | ee et ae 26751 3735:38 6 foros 9» 26756°4 37355 1 . a 26762 3733-7 1 |" tatters 26775 | 37335 1 cae + 26777 | 3732-7 In * 3 26782 | B7B2-1 1 ime: - 26787 | 3731-9 1 oo ss 26788 37306 1 thw ee = 26797 3729-9 1 ih his 3 26802 | ¥ 3729-4 ] im 3 26806 \ a 3728-5 In aes “. 26812 | a 3726-2 il 3 ff 26829 | a 3725:3 1 “s 26835 | @ | 3724-6 1 Tope i 26841 ) | 3729-7 il era B 26854 | 3721-3 2 | ae x 26864 3720°7 1 is 5 26869 | 3720-0 2 (ae x: 26874 | 8719°6 2 |) die ol : | ” | ” 2 % 3708°68 4 Whee i teter 26956°2 3708-09 4 ee el dae 26960°5 3706-2 Ib Pree! | at 26974 3705°5 1 Pe a pe 26979 3703°4 1 Nee oe 26980 37048 il ae a a 26984 3704-4 1 Pe ee ae 26987 3703-4 1 MDC ee 26994 ves) ln | aie od ; | ” ’ 3702°4 1 | ” | ” 27002 | 3701:9 1 a es 27005 | 3700‘Taond ip | af hd ae 27014 | 8699-5 1 | = 4 27023 3698-7 1 Pa Rae 27029 3698-6 a] | Bey a0) mee 27029 ee RON7 ss, cond) cL ) M022, ts, 27037 | Wave-length Spark Spectrum (Rowland) 3696-9 36965 36962 3694-70 3693°8 3693-6 3692-8 3692-00 3690°3 3689-9 3689-7 3689-2 3688-6 36884 36881 3687-4 3686-7 3686-4 3685°6 3685-5 3685:2 36847 3683-9 3683-3 3682-22 3680°8 3679°9 3679-3 3677°6 3676°3 3675°5 36749 36729 3671°9 36715 3670-6 3670-2 3669°3 36687 3667°6 3667°5 36671 | 3665-7 | 3664-7 | 3662-7 3663°3 36616 3661°2 3660-1 3659-2 365805 3GA7-75 8657-5 3656-7 36566 | { Intensity and Character Previous Measurements a (Angstriém) n Mo = ° a a eg a PIN ae athe! Fete RS) Pe Rn a ea wn BPH ADR RRR Ree TUNGSTEN (SPARK SPuCTRUM)—continued. (ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 37 ” od Reduction to Vacuum A. ~ Oscillation Frequency in Vacuo 27042 27045 27047 270582 27064 27066 27072 27079-0 27090 27093 27094 27098 27103 27104 27106 27111 27117 27119 27125 27125 27128 27131 27137 27142 27149°8 27165 27167 QTLTL 27184 27193 27199 27294 27218 27226 27229 27235 27238 27245 27250 27258 27259 27262 27272 27279 27287 27290 27302 27305 27314 27320 27329°3 273315 27333 27339 27340 BYE REPORT—1898. TUNGSTEN EG i anil hci ! na Reduction to | | Vacuum | ea Intensity | Previous Measurements | | Oscillation ; Spectrum | Gy ne P| (Angstriim) le | Frequency (Rowland) haracter ) En cn | in Vacuo } .| cs ee 101 | 77 | 97348. 3654-7 1 | & + 27354 | 3654-2 2 | ap alieaas 27358 3653°3 2 ” | ” 27365 36515 1 s ~ 27378 3650-0 1 ts ae 27389 3649-0 1 | 1, » 27397 3647°9 1 | nae . 27405 3646-72 Bid: | I debe taae 274142 | 8645-78 6 | cass ” 27421°3 | 36443 1 | + She Pd aa 27432 3644-0 1 ee Le oe 27434 | 3643-6 1 fae Nan 27437 es on a | 1S ae . 27438 36431 | 1 i. 4 » 27441 iiss | on, Hig ‘DD ee eer | 27453-1 3640-1 1 | ei nee 27464 3640-0 1 | Su tle os: 27465 | 3639-2 1 Pe Lu heii) 27471 | 3638-0 1 erie s. 27480 | 3637-4 1 ET tee 27484 3636 8 1 | Pan ee = 27489 | 3635-4 In aR ae a 27499 . 3635-2 1n Mo are + 27501 , oan ! Pevssis tft ihe 27511 bo 9b50' ” | ” 27514 3632°7 1 | ane ee cs 27520 | | 3631-5 1 | mand ie 27529 | | 36310 i ule 27533 . | 36309 1 | is | > 27533 , | 3630°4 1 Tees ey, 27537 a | 3630-2 1 | aca | “4 539 i 3629-1 2 27547 ” ” i 36265 1 D stas-tenltaee 27567 | | 3625° 8 1 | bye del aha 27572 . 3625°5 1 ke Sisal sass 27574 36251 | 1 | le lags 27577 | 3624:3 1 eee, alee 27584 | 2623-6 1 ares i Pa 27589 | 3623-1 1 rey UA 27598 3622°9 1 eee a 27594. | 3621-4 1 | eae 5 27606 | | 3620 7 1 tal ee 27611 a | 3620-0 1 ia Ree 27616 (7 | 36196 inet Tan ee 27619 | | 3619-3 1 | See at ee 27622 i* | 36185 1 hare 27628 \- 3617-72 6 1:00 | ,, 27633-9 36169 1 A 27640 3616°5 1 a) ey 27643 3616 2 1 aes ¥2 27645 3615-6. 1 ” ” 27650 | 36150 1 hens i 27655 3614-6 1 et Ee a 27658 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 3575 TUNGSTEN (SPARK SPECTRUM)—continued. SR tenctt | Reduction ave-length : | Spark Tene Previous Measurements | ue pombe Oscillation Spectrum Geeta: (Angstrém) 1 Frequency (Rowland) | xe <~ in Vacuo 3613-97 8 1:00 78 27662°6 3612-00 4 Wha: es 276777 3611:0 In eg en “5 27685 | 3608-9 iT ee seen Wane ess: 3607°6 In statin Was 27711 3607°3 2 eee ap 27714 3606°7 1 ¥ At 27718 3606°4 1 » eM 27720 3605 6 1 oe Herds 27727 | 3605°2 1 * 4 27730 3604 iti 1 ” | ” 27738 | 3603°9 1 ” ” 27740 3603-0 ibe, ” ” 27747 3601-7 1 hs fc 27757 | 3601-2 i! | ab Ses Ae 27761 3600:6 In sp ap 27765 3599-0 ] + ch 27777 8597'8 1 | a 4 27787 | 35963 1 Seen dj 27798 35956 1 | ae 7 27804 3595-2 1 Piles 79 27807 3595-0 1 Maen ay 27808 35946 1 We ess FP 27812 35941 1 eae omer, 27815 3593°6 1 alee Pr 27819 3592°55 3 op ' 27827°5 3590'9 1 on 5 27840 35905 In cf - 27843 | 3589°9 1 a 3 27845 | 3589°7 In oF + 27849 3588°7 In or . 27851 35871 1 iy asa ” 27870 3586 3 in ; lates % 27876 3585'8 In ; x an 27880 3585°3 In 1) Wis oa 27884 3585°0 1 heehee oe 27886 3584'8 1 6 4G 27888 3583'5 2 “- ' 27898 3582°8 1 An a 27903 3582-7 1 55 i. 27904 3582:0 2 + tS 27909 3581-2 2 3 aS 27916 35798 in dite, 27927 3578°6 in ” | 27936 3577°6 1 0:99 a 27944 3576°0 1 op “f 27956 3575'S 2 a3 a 27962 3574-0 1 Hs a 27972 3573°5 1 a5 > 27976 3572°6 8 3 “ 279824 3572°2 1 a “i 27986 3571:0 UI rf Ar 27995 3570°3 2 5 ae 28001 3569°8 1 Ls Mie 28005 co ~I ior) Wave-length Spark Spectrum (Rowland) REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. Intensity and Character Previous Measurements (Angstr6ém) 3569°7 3569°3 3569°1 3568°2 3567°6 3565'8 3565°7 3565°5 35645 35642 3563°6 3562°6 3561°5 3559°8 3559'0 3558°5 35584 3557°3 3557-2 3556-1 3555°35 35546 35541 3554-0 3553:0 35523 3551°6 3551:0 3550°8 3550°2 3549°23 3548°3 3546°5 3545-40 3544-6 3544-3 3543°3 3542°3 3541-7 3541°3 3540°8 3540°4 3540°0 3539°5 3538°6 3538-2 3537°5 3536-47 3536°6 3535-4 3534-5 3532°8 3532°7 35314 3531-1 MRR RDF DR DHE RRR HR RP RP RP ENDER RE NOR RRR RP RP RB RP RP RE RP RP RRR RP NNR RRR RR Rr NP Pe Reduction to Vacuum A+ — 0:99 9 ” ” ” ” ” } 9 ” ” ” ” ” ” ” ” ” ” ” ” 3? ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” | ” o ” ” ” ” ” ” ” 7 ” ” ” “1 8-0 ” ” bb) ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” Or98" sh 33 Oscillation Frequency in Vacuo 28007 28009 28010 28017 28022 28036 28037 28039 28046 28049 28054 28061 28070 28083 28090 28094 28095 28103 28104 28113 28118°7 28195 28129 28129 28137 28143 28148 28153 28155 28159 28167°1 28175 28189 281976 28204 28206 28214 28222 28227 28230 28234 28237 28241 28245 28252 28255 28261 28268°8 28276 28277 28285 28298 28299 28309 28312 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 377 Wave-length Spark Spectrum (Rowland) TUNGSTEN (SPARK SPECTRUM)—continued. Intensity and Character Previous Measurements (Angstrim) 3530°9 3530-7 3529-72 3528-9 3528°8 3528'1 3527°8 3526-9 3525-7 3524-6 3524-3 3523-6 3523-2 3522-2 3522-1 3521-0 3520-2 3518-9 3518-6 3517-5 3517'1 3516-3 35161 3515-1 3514-3 3513-0 3512-2 35118 35113 3510-6 3510-1 3509-4 3509:1 3508-89 3508-0 3507 3 3506-6 3506-3 3504-9 3504-8 3503-88 3503-1 3502-2 3501-4 3500°3 3499-7 3498-9 3498-2 3498-0 3496-9 3496-0 3495-40 3493-2 3492-1 3491-2 eee ee Rear tee ee aie sae pB 5 Oe TL ae el eae ~ al al pla Reduction to Vacuum ae A+ = vr — a 0-98 3:0 ” ” ” ” 3 ” ” ” ” ” ” ” ” ” bh) ” ’ ” ” ” ” ” 0” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” | ” ” ” ” ” ” ” ” ” ” ” ” ” » ” * $1 ” ” ” ” ” ” ” ” ” ” ” ” »” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” hs ” 0:97 oA Oscillation Frequency in Vacuo 28313 28315 28322°9 28329 28330 28336 28338 28346 28355 28364 28366 28372 28375 28383 28384 28393 28399 28410 28412 28421 28425 28431 28433 28441 28447 28458 28464 28467 28471 28477 28481 28487 28489 28490°9 28498 28504 28510 28512 28523 28524 28531°7 28538 28545 28552 98561 28566 28572 28578 28580 28589 28595°9 28601 28619 28628 28635 BY] REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. lw Tenet Reduction to “aes 1 ave-length illati Spark ino? | Previous Measurements bier? 4 Wee | | Chowiond) Character (Angstrom) es | a in Vacuo | | | | | 34903 aie tl | 097 | 81 28643 3489-9 1 ime ae | tk: 28646 | 3489 5 in? al Ron baa 28650 | 3488-7 1 eat |e 28656 3488-6 1 | Ra itraty 8 28657 . 3487-1 1 er = 28669 | 3486°32 4 | 1) Sia oe 28675°4 3485°5 1 | a & 28682 3485°3 1 / od tine] 28684 | 3483°5 1 ath ane 28699 | 3482°8 1 arce ie ae 28705 | 3481°5 1 / Pi sdaM |S ce Pant 28715 3480°6 1 | ages ante 28723 3480°3 1 | ie Weare 28725 3479-0 inh ie oe S: 28736 3478-0 2 ad | eae 28744 BATT -2 2. | ge: a 28751 3476°6 2 | gee) Setbpte. 28756 347555 4 ineethe deere 2 28764:3 3475°45 4 a 28765°2 3474-2 In lat es a 28776 3473-0 1 | be eee |) Epos 3472-4 1 ee thee a, 28791" 3471°9 1 | [ie 4 28795 3470°5 ‘tnt tA ae 8-2 28806 34702 Int moi | lee i 28809 3469°3 lit) 21] eis a 28816 3468°3 2 x 3 28825 : 3468-0 1 fs a 28827 3467-6 1 | | Reps 28830 3467-0 1 | f et 28835 ; 34665 1 | we deer te 28840 = 3466-0 1 = at 28844 3465-2 1 Peeing Hairy 28850 3464-6 2 Let -s. a 28855 3463-70 6 ‘ fe | 28862°7 3462:7 In Pitino) 28871 - 3462-2 In ete Shee 28875 | # 3461-7 1 He teas | 28880 | 3460°3 1 ee) ete 28891 3459°8 1 ” | ” 28895 : 3459°6 1 leas Daal tg 28897 3458°8 1 WO:S6E4\ 0s, 28904 3458-4 1 me, Se 28907 | 3457°8 a | ya 3 28912 | 34565 1 ross 0 28923 34551 2 | ie Fla 28935 3454-0 1 | AD Hilt aoe 28944 3452-9 In FS Sia FIL es 28953 | 3452°6 2 eh sen 28956 | 3452-0 1 a ital 28961 | 8451-9 1 nf bi 28962 , | 3451:3 1 el 28967 ; | 3450°8 1 f Fs 28971 | 3450°3 1 labs 63 28975 j i“ ’ Dad ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 957 9 TUNGSTEN (SPARK SPECTRUM)—eontinued. Wawve-leneth Reduction to ave-ien . I ‘ A Spark : Bey Previous Measurements aE oe Spectrum Glare tad (Angstriim) | ¥ in Vacuo , (Rowland) racer | 2S: a | A 3450-00 4 | 096 | 82 | 28977°3 3449-5 1 . ee >; 28982 | 3449-0 1 3 se 28986 3448-4 2 | . ae | 28991 | 3448-2 1 i iy 28993 | a | ae ; ” | ” é 34466 1 wat ‘cpah 94720006 / 3445°8 1 my Ree 29013 sus | Peon eae 3444-7 1 e 29022 | 3444-2 ey | aaa i 29026 3443-2 2 Nas iy 29035 3442-1 1 are “ 29044 3440-80 6 Fe ee, ch en 29054-8 3438-8 1 ae is 29072 3438-2 1 7 lana 29077 3435-7 2 . cs 29098 3434-8 ik s z 29106 3433-9 1 es a: 29113 31323 in ease hi n | ” ” ~” ” 3431-7 In oe 2 29132 3430°8 2n bees a 29140 3430-4 1 29143 , { ” ” 1 3407 8 : . + pale . : ‘ i ” | ” 2 34263 1 en 29178 3426-0 1 yes: 29181 3425-6 1 a a 29184 31246 2 ely coat 3423-3 1 Cael aca 29204 | 3422'8 1 ii - 29208 | 3421-4 1 > 29220 | 34193 1 Peete mbe et cea 3418-6 rf bred 29244 3418-4 1 be ¢ 29245 3417-7 1 095 |, 29251 . as 1 * f 29252 | 3416-78 4 : si 29259°0 3415-4 2n . nt 29271 ss | 3 | aaa : a 4 ; 29287 : 3412°8 2 ‘ - 29293 ee In # i 29300 3409-3 i is ates oo In Ss $3 29324 : 6 2 a9 ~ 29338 a | 1 ale eae 7 2 e A 29346 3406-2 1 . 3 29350 380 REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. Wave-length ahs Reduction to | Rent and Pie revious Measurements skeet Oscillation + (Rowland) Character | (Angstréim) | 1 | Frequency At ,T | in Vacuo | 34062 | 1 Peete eae | Saegee oy 095 | 83 29351 | 3404-3 1 ” ” 29362 34042 1 ” ” 29367 | 3408°8 1 ” ” 29367 3402°8 1 ” ” 29371 3402:2 if ” ” 29380 3402:03 | 6 ” » 29385 | 3401-5 | iL ” ” 29385°9 3401-0 it ” ” 29391 | 3400-7 1 ” ” 29395 | 3400°2 | 1 ” | ” 29398 H 3399:07 6 | ” ” 29402 33983 9 jo» ” 29411°5 cy ia ” ” 29418 3397°4 | ¥ ” ” 29424 3396°5 : 1 ” ” 29426 3396-0 | 1 » wrt 29434 3395-0 1 ” ” 29438 3394-6 | 9 2. Se) 29447 3393°7 In ” ” 29451 3393°1 if ’ ” 29458 3392°5 1 ” + 29464 3391°7 1 H ” ” 29469 3390°5 on {fa age | eens 29479 3389°7 1 | ” ” 29486 3389°0 7 ” ” 29493 3387°8 | 2 ” aay, 29499 3387:0 if | ” ” 29510 3386-7 ] | oa : 29517 3386°2 | Ll ” ” 29519 | 8386°0 | 1 8 As 29524 3385'1 1 ” ” 29525 33845 1 roe a | atx 29534 3384°4 1 ” ” 29538 3384-0 l ” ” 29539 | 3383°3 2 ” ” 29543 | 3382-4 1 ” ” 29549 3382-0 1 ” ” 29557 3381°2 2 ” ” 29560 3379°'8 uf ” ” 29567 3379°3 2 Hiss ” 29580 3378:7 1 ies ” 29584 3378-4 1 ene : 29589 3378°3 | 1 ” i 29592 33775 1 ” ” 29593 3377-0 i Of | ,, 29600 3376°25 8 ” ” 29604 3375 3 1 ” ” 29610-4 | 33743 1 ” ” | 29619 | 3373-4 if ” ” 29628 |. 3373°0 1 33h syle 29636 {| 3d72'4 2 ” ” 29639 ” ” 23644 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 381 TUNGSTEN Sa Sr me, i — | co to i Ve-len 1 - acuum * ° ry Intensity | preyjous Measurements eer | Oscillation Spectrum and (Angstrém) a 1 | gig et | (Rowland) Character 5 =~ | in Vacuo iwaat i pi. Rae F : 3371-7 | 1 0-94 | 8-4 | 29651 3371°3 1 in a0 29654 3370°7 1 - er 29659 | 3370-4 il ” ” 29662 3370:0 1 aes ine 29666 3369°9 1 oc WN 29666 3369-2 1 TI apd 29673 3368-3 In etal a | 29681 3367°8 1 Sa Ba 29685 3367°5 1 cit Peo al 29688 3366-8 2 s as | 29694 3366°5 1 saree “ 29696 3366-0 i :. ¥ 29701 33653 1 5 a 29707 3364:9 1 % & 29711 33640 2 ” ” | 29719 3363'5 2 f med 29723 3362°5 1 Aneas » | 29732 336271 i ” ” j 29735 3361-20 4 pee » | 29742:9 3360°5 2 ae 85 29748 3359°3 1 ie i 29759 3358-72 6 Wa Sees t pial aa | 29764°8 3357°8 1 Bes oe 29772 3357-2 1 eA 5 29778 3356°5 1b f a 29784 3355-9 1 < 2 29789 3355°5 1 \aeedoa Nees 29793 335571 1 LAS ow etc 29796 33547 2 chat hh & 29800 3354-2 1 ad aes 29804 83540 | 1 i. z 29806 3353°8 ] Be at 29808 3353/1 2 teas her || pu 29814 3352°5 2 pee Ae 29819 3352:0 1 BE ae: 29824 3351°6 jn 6 « 29828 | 3350-2 ib is ms 29840 3349-6 1 aid de 29845 3349-4 2 eee Rec 29847 ! 3349-0 2 Coens mye 29851 | . 8348-4 2 he ee 29856 . 3347°8 1 . s 29861 | 3347-2 1 - a 29867 3346-2 it Ks = 29876 - 3345-8 2 eee ae? 29879 3345-6 1 real pee 29881 3344-5 1 Auta ee 29891 3343-60 4 nse ; 29899°4 3343-28 4 Bee, Sirti 29902:2 3342-63 6 A - 29908'1 3341:3 | 1 a ee 29919 3340°3 1 se EES 29928 3339°7 1 Soni 29934 | 3339-1 2 Ante at aaee 29939 | 382 REPORT—1898. TUNGSTEN (SPARK SpECTRUM)— continued. | Reduction to . bibs te epg | Previous Measurements | “ua Wea Tin Spectrum (Angstrém | in Vacuo H | (Rowland) Character | ) | a) Nias | ) bo ct ala | | a { ' = | t 3338-7 2 1093 | 85 29943 | | 33383 1 ees ae 29946 i | 3338°0 In / re lame rt) 29949 ‘ | 3836-7 oy ean ae 29961 . | 3836-1 1 | (Secs 1| ey 29966 | 38335°6 1 : # 29971 | 33348 1 : : 29978 | 3384-0 1 1 es 29985 3331-7 2 aoe eo 30006 | 33308 In cee | ae 30014 | 3328 1 Oe we 30037 | 8327°8 1 eee | ae 30041 | 3327-2 1 3 a 30046 3326°3 2 : 3 30054 | 3326-2 1 eal ee 30055 | 3325°7 i 2 ” H ” 30060 | | 3325°0 1 # 8:6 30066 | 3324-2 1 ” ” 30073 | | 33235 1 3 3 30080 | 3322:6 1 . me 30088 ) 3321°7 1 ” ” 30096 | 8321:2 1 ” ” 30101 | 3321-1 1 = 3 30102 * | 8320°5 1 a a 30107 | 3320-4 1 ini RS 30108 3318-7 1 : " s 30123 33185 1 “f a 30125 S30S-Omeon| a Joker ome 30130 | 3317-0 1 seat (ee 30139 | 33161 1 | _ -s 30147 3315-2 1 | ¥ 5 30155 3314-4 1 he Mess 5 30162 3313°6 1 ) | ” ” 30170 3312-4 1 ss ” 30181 3311°6 2 | Ee ob 30188 33103 2 sd es 30200 3309°6 1 leon as 30206 3309-2 1 eran! tas 30210 | | 33083 2 eee Poe: 30218 | 8306-2 4n Fe Peetare| BES 30237 $305°5 1 ee y 30244 | 83046 2 ers | bee 30252 | 88045 1 [Seem eee 30253 | 3303-8 1 aan he 30259 |. 3303°3 1 ae (I Mate 30264 ' 3303-0 1 Saedp has 30267 3302-0 1 a \PeP 30276 3301:3 1 *, . 30282 3301:0 2 . ff 30285 | 3299°7 1 ov2 | ,, 30297 32988 1 eae Pa 30305 32983 | 2 ew Ors 30310 S20 ro Wire 2 Se ss 30317 ] . Wave-length ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Spark Spectrum (Rowland) 3296°3 32952 32943 3293°8 3293°0 32917 3291°5 3291-1 3291-0 3290°6 3290°3 329071 3288°8 3288-0 3286-70 3285°8 32837 3282°7 3282-0 5280°2 3279°5 3277°8 3277-6 3277-0 3276°5 3275:7 32749 32732 32720 32717 3270°3 32702 3269 7 3269-0 3268°6 3268°3 3267°6 3266°7 3266:0 3265°2 3264:2 3263°2 3262°37 3261-2 3260°8 3260°3 3259-4 3257°8 325671 3255-7 3255°0 32543 3252°5 3261°2 3250-2 TUNGSTEN (SPARK SPECTRUM)—continued. Intensity and Character | Reduction to Vacuum Previous Measurements | ° (Angstrém) A+ i. Oscillation Frequency in Vacuo 5 a a bet Rt Rb SD OO DD OO ee et Sea ia ae 30328 30338 30346 30351 30358 30370 30372 30376 30377 30381 30383 30385 30397 30405 30417:0 30425 30444 30454 30460 30477 30483 30499 30501 30507 30511 30519 30526 30542 30553 30555 30569 30570 30575 30581 30585 30588 30595 30603 30609 30617 30626 30636 30643°9 30655 30658 30663 30671 30687 30703 30706 30713 30720 30737 30749 30758 385 384 REPORT—1898. TUNGSTEN (SPARK SPECTRUM) —continued. | | Reduction to Wave-length . Vacuum eee "Spade Intensity / Pravious Measurements Oscillation Spect and ° fs Frequency (Rowland) Character | (Angstrom) ane ie in Vacuo . rN asa dee | a a 3248°7 i 0-91 88 30775 3247°9 1 ” 5) 30780 3247°6 if ” 3 30783 32464 1 ” ory BOT9L B245°4 1 ” : 30804 3243°50 4 Tee | 30822°1 3243-2 2 pera ts 30825 324271 2 ae) 3 30835 341-2 1 Peete 3240-0 In ; 30855 3238°9 1 ” ” 30866 3238°5 1 Ae | 30869 32383 v1 Bd) hale a 30871 3237-2 1 ¥ | 30882 32360 1 » - 30893 3235°9 1 » 5 30894 Beas b 1 ar 30902 32346 at : ” 30907 32338 ol oe aa 30914 2233°3 2 all rag 30919 3232°2 1 ” ) 30930 3231°6 1 39 oo 30935 3230°9 1 a 3 30942 3229°7 1 Soee Mae waa 30954 | 3229°5 dj Tova tannins 20956 | ~~ 3229'0 af % 3 30960 | 3297-9 1 is - 30971 1 3227-4. 1 os Pe 30973 | 32267 2 8 oS 30982 3224-9 1 ” ” 31000 3224-0 1 . ” 31008 3223°3 In . 55 31015 3222°7 i ” ” 31021 3222-1 1 ” ” 31027 3221°3 2 7 ss 31034 3221-1 in ” : 31036 3220°2 1 OOO ie 31045 3220°0 1 is Be 31047 3218°9 1 3 * 31058 3218°7 1 ” oe 31059 3217°6 1 “5 a 31070 321673 2 “o 8-9 31083 3215°68 4 ” ” 310887 shee ao 3213-4 1 Keo ah 31111 3213°2 1 % BS 31113 321271 1 ore Tees 31123 32112 1 >| 2 hee 3210°9 1 oo 3210-7 1 ho eee | 31137 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 385 . TUNGSTEN (SPARK SPECTRUM)—continued. i am Reduction to ave-length . re 4 Seng eer Previous Measurements |_ Me soain Pane ocinea Character (Angstrém) rr + in Vacuo 3210°0 2 0-90 | 89 31144 3208°6 1 ” ” 31157 3208°3 1 » ” 31160 3208 :2 1 » ” 31161 3207°8 1 ” ” 31165 3207°6 i ” ” 31167 3207°3 2 ” ” 31170 ; 3206°7 1 5 os 31176 3206-4 2 ” ” 31179 3205°7 1 of 2 31185 3205°6 1 ” ” 31186 3205°3 1 ” ” 31189 3204°5 1 cn » 31197 3203°7 1 a3 ” 31205 3203°43 4 ” 2 31207°6 3202°2 1 “e 4 31220 3202-0 1 ” ” 31221 3201:7 2 ae “: 31224 3200°5 In ” ” 31236 3200°1 1 9 + 31240 3199-4 1 ” ” 31247 3199-0 2 oS “7 31251 3198-4 2 ” ” 31257 3197°5 2 ” ” 31265 31965 1 = “5 31275 31960 1 ” » 31280 3195°8 if “6 5 31282 3194-7 2b “e ‘ 31293 3193°8 2 9 » 31302 3193:2 1 ee = 31308 3193°0 il is a 31310 | 3192°3 1 * ” 31316 | 3192°2 1 Pr Fe 31317 3191°6 2 ” ” 31323 3191-0 2 #9 a 31329 ‘| 31893 2 a |- 81346 3188°5 1 PS 3 31354 " 31880 1 “- Ns 31359 : 3187°8 i | * Ps 31361 3187:1 | 2 ” ” 31367 3186°4 1 i a 31374 3185-0 1 % - 31388 ; 3184°4 } 1 ” » 31394 3184-0 1 3 “ 31398 3183°5 1 } 4 3 31403 3182°8 al 5 aly | 31410 3182°2 1 4 31416 31818 1 0°89 a 31420 3180°8 i +s 9-0 31430 3180°2 1 = 3 31436 3179°60 4n ” ” 31441'5 3178°7 In ce a 31450 31781 2 A As 31456 3177°2 2 - - 31465 3176-7 | 1 31470 1898, a * cc 386 REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. | Reduction to Weredengib Intensity | Previous Measurements Vacuum Oscillation } Ss ms 22 (Angstrém) } Frequency pecirunt Character 8 VataG (Rowland) Ne x 317610 4 089 | 9:0 31476-2 31751 1 : ; 31486 3174-7 1 2 a6 3173°6 1 ”» ” 31501 31728 1 4 és 31509 SLTL6 1 ” ” 31521 31714 ] ” ” 31523 31702 1 “ : 31535 3170-0 1 3 5 31537 31685 In st ‘ 31552 3167-9 1 * 3 31558 3167-7 1 if A 31560 3167-0 1 é és 31567 3166'S In 5 af 31572 ae 1 f 31580 el6b4 1 is ‘ 31583 31648 i a1 home 31589 a 1 s is 31592 3164-4 1 . Ki 31593 3163°6 2 - 3 31602 3162°2 1 4 ee 3162-0 1 2 : oleae 3161°3 1 a i eet 31607 1 ae i 31630 3160°20 4 ib eee 316346 3159-0 4b is 7 31647 31570 In Ss .. 31667 Blob 1 5 9 eS 31680 3165°5 1 e eee alba 1 pales 31685 3154-2 1 ‘ é oe _s 1 iz 31709 31524 9 2 : te 31516 1 ‘i mie 3151°3 2 i orene a de 2 is a 31738 ape 1 oe We 31739 | eager 1 3 ie 31756 . | 31470 1 re ee 31758 iano 1 ih oe 31769 . | 31463 9 z athe | 3145-7 2 c. i 31780 | 31455 1 : : 31789 Fane 2 Stel 31793 (ores oe 2 aie ae 31805 3143-0 1 : : Bat: B1esS 1 ee oa 31809 3142-0 4 ; : ane 3140°3 1 ” ” 31835 3140-2 1 Ye hee 31394 1 Bi Gia 31844 ep 1 ot | oe eee 31379. 1 % f 31859 Viger 1 ote 31862 ( ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 9337 TUNGSTEN (SPARK SPECTRUM) —continued. \f Reduction to | ae eit Previous Measurements Veta eee an my requene Goclaea) Character = ree - in vaste | 3137-2 1 | O88 | M1 31867 3135°9 1 ? 2 31880 31358 1 _ 9% 31881 3133'8 2 < é 31901 3132-6 1 - # 31913 3131-2 1 = a 31928 3130-4 1 re - 31936 3129-7 2 . s 31943 31290 2 ps i 31950 3127:7 2 7 - 31963 3127°3 1 cs _ 31967 3126°3 2 ee es 31978 3125-7 i i x 31984 3125°3 1 i a 31988 3124-5 In ss A: 31996 3123°5 2 PA 4 32006 3121°9 In Mo re ee 3) 32023 3121-0 1 a : 32032 3120-7 1 - s 32035 3120°1 2 & 5 82041 3119°6 1 a ie 32046 3119-4 1 =" i 32048 31183. 1 2 - 32060 3117-5 2 “7 be 32068 3116-0 In e a 32083 3115-4 1 Pe *: 32090 3115°3 1 s if 32091 3113-6 ] s is 32108 3113°3 1 ta 92 |- 32111 3112°7 2 > ae 32117 31124 1 . 32121 3112-3 1 ae ES 32122 3111°8 1 x a 32127 31111 2 , 32134 3110°6 2 - om _ 82139 3108-6 b, - b 32160 31083 1 eZ. 4 32163 | =3107°9 2 i ‘e B2167 31075 1 i x 32171 3107°2 2 i: 5 32174 3106°5 2} ma 2 32185 3106-1 1 i e 32186 3105-9 1 ie i. 32188 3104-9 1 = 24 32198 3104:3 1 ¥ < 32204 8103-7 1 he md 32211 3103-4 1 ie ¥ 32214 3103-0 In i . 32218 3102-2 | 2 a 55 32226 3101-2 1 1 O87 5, 32237 3100°7 2 Rs = 32242 3100°2 In A a 32247 — 3099°0 1 leas o 32259 3098-7 1 iy, ae fe 32263 . 3098-4 1 Ke ‘. 32266 eae 388 REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. Wavelet Tatonsiby Reduction to spate and Previous Measurements Se a ee (Rowland) Character (Angstrém) j "requency A+ a in Vacuo ES A 3096°5 1 rege. 3096:0 2 0.87 9:2 32286 3095°3 i ” ” 32291 3095:0 1 » ” 32298 30947 1 ” ” 32301 3094°0 1 ” ” 32304 3093°6 2 ” ” 32312 3093°3 1 ” = 32316 3092°3 1 ” ” 32319 3091-9 1 ” - 32329 3091:7 1 ” - 32334 3091-2 1 ” ” 32336 3090°7 1 ” ” 32341 3090°5 1 ” ” 32346 3089-2 1 » : 32348 3089-1 1 ” sa 32362 3088°3 1 ” ” 32363 30881 1 ” ” 32371 3087°5 2 ” ” 32373 3086-4 2 ” 7 32380 3085°4 1 ” : 32391 3085°0 2 ” ” 32402 3084'4 il ” 32406 3083-6 2 » iF 37412 3083-2 1 ” 9°3 32421 3082-2 2 ” ” 32425 3081°9 2 ” ” 32435 3081°1 2 ” ” 32439 3080-7 1 ” ” 32447 3080°0 1 ” ” 32451 3079°3 i ” ” 32459 3079-0 if ” ” 32466 30783 ] ” ” 32469 3077°63 6 ” ” 32476 3076°9 1 ” ” 32483°2 3076-0 2 » ‘s 32491 30753 In ” ” 32501 30740 g ” ” 32508 30733 2 : = 32522 30727 2 a ss 32529 307 1 8 24 ” ” 32536 3071-3 2 : 5 32545 3069°3 2 » : 32551 3068°6 1 ” ” 32572 3068-2 1 ” ” 32579 3067°9 2 ” ” 32583 3067°6 2 ” ” ; 32587 3067-0 24 ” ” 32590 3065°1 1 ” 4 32596 3065°0 1 ” ” 52616 306471 2 ” ” 32617 3063°3 1 ” ” 32627 3063-0 1 * 4 32636 3062'8 1 » és 32639 3061-7 2 086] ., 32641 ” » 32653 wer “ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 389 TUNGSTEN (SPARK SPECTRUM)—continued. | Wave-length 3 Spark Spectrum (Rowland) 3061-0 3059°8 3059°7 3059°1 30585 3057°5 3056-2 3055-7 3055°5 3055 1 3055-0 3054-1 3053-5 3051:8 3051-42 30506 30500 3049-8 3049-0 3048.6 3047-6 3047-1 3046-5 3045-6 3045-2 3044-4 3043-7 3042-2 3041-8 3041-0 3040-3 3039-6 3039-3 3038-7 3038-0 3037-7 3037-4 3036-7 3035-4 3035-2 3034-2 3033°9 3033-7 3032-5 3032-0 3031-0 3030-3 3029-9 3029'5 3028 9 3028-7 3027°8 3027°3 3026-7 | Intensity | Previous Measurements | and (Angstrém) | Character COI SI 0 OS a OS Ol al OS a ll el el cel oe 5 i=] i=} 3025-9 Dt ol ol cel cell ool el ool SO SO oe ol oe oe on Reduction to Vacuum A+ Oscillation Frequency in Vacuo 32660 32673 32674 32680 32687 32697 32711 32717 32719 32723 32724 32734 32740 32759 32762°2 32771 32778 32780 32789 32793 32804 32809 32816 32825 32830 32838 32846 32862 32866 32875 32882 32890 32893 32900 32907 32911 32914 32921) 32936 32938 32949 32952 32954 32967 32973 32983 32991 32995 33000 33006 33008 33018 33024 33030 33039 390 REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. Wave-length Spark Spectrum (Rowland) 3024-9 3024-58 3023 6 3022-9 3022:7 3022°6 3021-7 3021-0 3020-7 3020°3 3019-6 3019-4 3018-6 3017-9 3017-4 3017-1 3015'6 3014-9 3014-6 3013-7 3013-2 3012-1 3011-7 3011-2 3011-0 3010-7 3009°6 3008°8 3008-0 3006'5 3006-3 3005°3 3004-8 3004-2 3004-0 30037 3003-0 3002'8 3002-2 3001:9 3000°9 3000°6 3000-3 2999°6 2998-7 2998-0 2997-7 2997-6 2996-9 2996-5 2996-0 2995°7 2995-4 2995°3 3025°2 Intensity and Character Previous Measurements (Angstrém) 6B l=] La cl lc el el Sl ld Sc cl le ce ce Se ee Reduction to Vacuum At+ in Vacuo Oscillation Frequency 33251 33253 33265 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 391 TUNGSTEN (SPARK SPECTRUM)— continued. Reduction to Wave-length Lnitendit V. ens. . on ea y Previous Measurements . oe Oscillation (Rowland) Character (Angstrom) 1 Hrequency A+ neh in Vacuo a le A 29948 we : 0:85 | 9-6 33381 2993°6 2 f? ‘i aoa 2992°9 1 pas ouae 2992-0 2 2 s ae 2991°5 1 e 2 catia 2990-7 1 % ‘: an 2989-5 1 f é: pare 2988°8 1 s - eae 2988-6 1 E. bers, 2987°3 2 i es 6 2986-4 1 v4 pe sade 2986-1 1 fe i pet: 2985°9 1 $ is 2984-9 1 & t py 2984:5 1 i E ade 98a 1 * x 33496 2983-6 1 @ a oaeye ae 1 i f 33507 _ 2982°6 1 § 4 ee mips ; 0-34 |, 33518 2981-6 1 é is et 2980°7 In Pe * cata 2979-9 2 ” ” 33539 2979-2 1 E ‘ oocee 2978°3 1 ? Sate Apts i is Es 33566 905.0 1 a ss 33570 2007-6 2 fs . 33574 2976-9 1 - ve 33579 ae? d S B 33582 2975°7 In 3 is ae 2975'1 1 i % pet ane 4 ‘ 33602 “ 3 m8 i 33610 ams A *: fe 33623 ae) : s 3 _ 33625 ts - % E 33627 ae : ks ¢ 33632 2971-4 1 ig %s aoa 2971-0 1 x x aaa He : sit 9% 33649 2970-0 1 x : bey as : x 33660 ee : 4 . 33662 4 2969-0 1 # ¥ pee =a : F ¥ 33671 BS) 2967-1 1 x 33698 2967-0 1 if E ee { ae : i 33694 | 2966-2 1 aimee 33703 | 2965:6 1 é is 53710 mes i & i 33710 | 2964-5 2 Pe % mee | 2962-6 1 4s orede | 33744 92 REPORT—1898, TUNGSTEN (SPARK SPECTRUM)—continued. Reduction to Wave-length Vacuum Spark Intensity | Previous Measurements Oscillation Spectrum and (Angstrim) 1 Frequency (Rowland) Character Nee -- in Vacuo 2961°8 1 0°84 | 97 383753 2961:0 2 Ws ra 33762 2960°3 1 a: = 33770 2960°1 1 ” " 33773 2960-0 1 ” ” 33774 2959:0 In AS a 33785 2958°0 1 Ss + 33797 2967°4 1 A ” 33803 29573 L - * 83805 2956°8 1 +3 ‘ 33810 2956°5 1 ” ” 33814 2955°3 1 A = 33828 2955'0 2 a 3 33831 2954-0 1 5 ty 33842 2953°9 1 - = 33844 2953°0 1 * A 33854 2952°3 4 Fn 33862 2951-0 1 . a 33877 2950°5 2 z ss 33883 2949°2 1 m1 4 33898 2948°5 1 :: . 33906 29483 1 - _ 33908 2947:8 In 9 as 33914 2947°5 1 as : 33917 2947-0 2 en 5 33923 2946-0 In A es 33934 2945:3 1 “ 9°8 33942 2944:6 2 a 7 33950 2943°5 1 a3 33963 2943-2 1 - Fé 33967 2942-7 1 0°83 D 33972 2942°3 ] si N 33977 2941-6 1 a 83985 2941°4 1 ” ” 33987 2941°1 1 a - 33991 2940°8 1 ” » 33994 2940°3 2 a 34060 2939°0 2n ” ” ; 34015 2937-7 1 ” ” 34030 2937-2 1 >: ‘ 34036 2936°7 2 ef sa 34042 2935°7 1 " i 34053 2935°3 1 s 3 34058 2935-0 2 i : 34062 2933-0 1 5 j 34085 2932-7 1 ; 3 34088 2932°0 1 ‘ . 34096 2931°6 1 " é 34101 2931-0 1 . hs 34108 2930-0 2 is i; 34120 2929-1 1 a 34130 2928-7 1 a * 34135 2928°2 1 “ 5 34141 2928-0 A sy _ 34143 2927°9 1 ” ” 34144 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 393 TUNGSTEN (SPARK SPECTRUM)—-continued. Reduction to Wave-length I : Vacuum here Spark ntensity Previous Measurements Oscillation Spectrum | (4 and (Angstrém) 5 a nei (Rowland) haracter nee to in Vacuo 2927-1 1 083 | 9:8 34154 eer 1 a Aen 34155 2025°9 2 i 34168 2925°1 2 Se ., 34177 east 1 Ab hecs? 34189 2923°6 2 34194 2923°2 1 is 53 34199 2922/0 1 it hoes 34213 oh 1 we 1 Od 34293 es 1 i G 34224 zoty'G 1 ath 34241 2919-1 1 y, a 24247 cae 2 og eee 34252 av18'3 1 i ‘ 34257 2917-7 In 5 i ae 34264 B10 In a lt at 34272 “canal 1 wh es 34275 2915°6 1 ne ee 34288 2915°2 1 a 34293 2914-7 1 pa ee 34299 es 1 at ee 34302 eet 1 rb ae 34311 ee 2 thos 34324 ae 1 a 34327 he 2 FOB ost 34333 eee 2 sella 34358 se 1 er RES 34363 ool 2 eb hss 34371 alee I yh Where 34374 eo 1 tie 34383 aos l eles 34385 2906-5 2 Ae 34396 ea 1 ee 34405 pee 1 wa 34410 a ae oat eee oad 1 meh ae 34417 2904-3 2 ca As 34422 ee 2 082) |» 34429 ea. 1 me i ee 34441 “ho I as 34445 fae 1 er ee 34451 a 2 a ee 34457 “UN 1 wy 34461 coh l oto sy 34470 2899-0 1 MB get 34485 eT 1 See 34488 2898-4 1 a he 34492 oackygl 1 pen a 34500 = bid He Wy Regs 34505 2396°5 2 » | 100 34514 Ne 2 Ayal 34519 2895:0 y | A o 34532 2394-3 1 Web d 34541 2893°8 1 ¥ 3 34547 a u ffeil Sad 34549 394 REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. aa aes Reduction to pores Intensity | Previous Measurements | Yaga Oscillation Spectrum and (Angstrém) i Frequency (Rowland) | Character A+ <~ in Vacuo 28930 1 ” ” 34556 2892°6 1 ” ” 34561 2892°2 1 ” ” 34566 2891°6 1 ” ” 34573 2891°1 1 ” a3 34579 2890°7 1 ” ” 34584 2889°9 2 ” ” 34593 2889°5 1 ” ” 34598 2888'8 i ” ” 34606 2888°4 1 ” ” 34611 2887-7 1 ” ” 34620 2887°0 2 A + 34628 2886°5 1 7 on 34634 2885°'8 1 5 a 34642 2885'6 1 ” ” 34645 2885:0 1 i 3 34652 2884:°3 2 a5 or 34660 2883°3 if of 3 34672 2882°5 2 7 3 35 34682 2881°7 2 + 5 34692 2880°8 1 A m0 34703 2880°3 1 = A 34709 2879°6 1 “a 3 34717 2879°3 1 Mo A 35 34721 2878°4 1 4 oy 34732 28783 it Es “3 34733 2877-1 1 7A Pa 34747 2875°3 1 5 5 34757 2876'1 1 - Pa 34759 2875°6 1 5 oF 34765 2875°3 1 ~ - 34769 2874:7 1 a 5 34776 28740 1 ee = 34785 2873°5 al As « 84791 2872°8 1 a 10°1 34799 2872:0 1 Fs 5 34809 2871°5 1 3 = 34815 2871:0 1 5 = 34821 2870°8 1 A 5 34823 2869°7 1 . 9 34837 2868°7 2 _ Fe 34849 28680 1 - a 34857 2867°8 1 A 6 34860 2867'5 1 aS 34864 2866'8 1 55 34872 2866°7 1 > 4 34873 2866°5 1 ns brelese 34876 2866°2 1 © Lahey 34879 2865°9 1 a A 34883 2865°5 1 ‘ ¥ 35642 2804-7 1 ‘ 4 35644 2804:3 1 x ae 35650 2804-0 1 ft 35653 2803-7 2 vt Z 35657 28033 1 . : 35662 2803°1 1 a i 35665 28027 1 " 35670 2802°5 1 bs re 35672 2802-2 1 j 4. 35676 2801-6 1 “ sf 35684 2801°3 2 -. q 35688 2800-2 1 z ; 35702 2799-22 4 C 10-4 35713°8 2798°5 In , 35723 2797°6 In ‘ sah i] 35735 2797°1 In a : 35741 2796°3 1 * i 35752 2795:7 2 a a 35759 27938 1 “f 3 35784 2793-2 1 ¥ f 35791 2792'8 a x .. 35796 2792-0 if a3 s 35807 2791-9 1 _ z 35808 2790°6 2 ” ” 35825 27903 1 = Hl 33828 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 397 TUNGSTEN (SPARK SPECTRUM)—continued. Wave-length Spark Spectrum (Rowland) Intensity and Character Previous Measurements (Angstrém) 2789°3 2788°7 2788'2 2786°5 2785'8 2785°3 2784°4 2784-2 2783°9 2783°3 27827 2782°3 2780°5 27795 2778'8 27781 2717-7 2776-7 27752 27747 27742 2772°8 2771-2 2770°7 2770-2 27700 27692 2768°5 2768°2 2767°7 2767-2 2766°5 2765:5 2765.0 2764°40 2762-7 2761-6 2760°8 2760°6 2759°6 2759°5 2757°9 2757:3 2756°8 2755°1 2753°3 2753-2 2751°6 2750°8 2750-4 2750°2 2749°4* 2749-0 2 * 1 il 2 1 5 2 1 1 1 1 1 2 2 1 2 1 1 2 1 2 1 1 1 1 1 1 1 2 1 1 2 1 2 4 In 2 2 1 a J 1 1 1 1 1 2 il 1 in 1 1 2 1 * Double. Reduction to Vacuum At i x Oscillation Frequency in Vacuo 0°80 10-4 35841 35849 35855 35877 35886 35893 35904 35907 35911 35919 35926 35931 35955 35968 35977 35986 35991 36004 36022 36029 36035 36054 36074 36081 36087 36090 * 36101 36110 36114 36120 36127 36136 36149 36155 361637 36185 36200 36210 36213 36226 36227 36248 36256 36263 36285 36309 36310 36331 36342 36347 26350 36361 36366 398° REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. Wave-length ee g one ae Previous Measurements ty i Sis: eer ti ectrum an Ae erates requenc (Rowland) Character (Angetrém) A+ Boy in Facts A 2748-4 2 079 | 106 36374 2747:°0 1 39 ‘a 36392 2746°9 1 ” ” 36394 2746°5 2 ey, 3 36399 27451 1 ” ” 36418 2743°3 a 99 a 36441 2743°2 1 5 ” 36443 2743°0 2 ” ” 36445 2742°6 2 + e 36451 2742°1 1 ” PA 36457 2741°3 1 0:78 ” 36468 2741:0 2 ” ” 36472 2740°3 1 ” 9 36481 2739°7 2n on » i 36489 27386 ln “ ” 36504 2737-9 In 9 ” 36513 2737°0 © i! Pn ” 36525 2736°7 1 ” ” 36529 2735°9 In a ” 36540 2734:8 2 ” ” 36555 27334 1 ” ” 36573 2732-0 1 “7 ” 36592 2 | 9731-2 In S 9» 36603 2730-9 In os % 36607 2730-0 1 ” ” 36619 2729°3 a ee ”” 36628 2729-0 1 “ 9 36632 2728°5 i ” ” 36639 2728-1 In ” ” 36645 2727-7 1 ” ” 36650 2726:7 2 s 10:7 36663 2725:6 1 Sr ay 36680 2725-2 1 *p ” 36684 2724-5 1 ys a 36693 | 2722-8 D ” ” 36716 2721-7 1 or A 36731 2720°6 2n “e P 36746 2719-9 1 a5 ” 36755 2719-0 1 op ” 36767 } 2718-1 2 °F at 36779 2717-2 1 rm ap 36792 / 2716-9 1 ‘a ” 36796 | 2716:4 2 “5 or 36802 2715-4 2 a ” 36816 2714:5° In 1 Posy ” 36828 | 2714:0 1 yy 53 36835 27135 In Je aig * 36842 2712-7 2n 99 a 36853 2711°8° 1 » ” 36865 2710°9 2 F. + 36877 2710-4 1 ” ” 36884 2709-7 - 1 | a9 ” 36893 2708°9' 1 ae ” 36904 2708°7 2 7 a 36907 2707'8 1 Ih ears - 36919 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. Wave-length | Spark Spectrum (Rowland) 2707-1 2706°8 2706-0 2705°8 2703-6 2703-2 2702°22 27016 2700°6 2700°3 2699°4 2698°6 2698°1 2697-80 2696-0 2695°1 2694-7 2694°6 2694-2 2692-7 2692-0 2691:2 2689°2 2688°4 2687-7 2687-2 2686-6 2685°5 2685°3 2684°6 2683°8 2683-4 2681°7 2680°8 2679-78 2679-2 2678-1 2676°5 2676-1 2675-4 26749 26743 2673°2 2672:9 2671-7 2670°6 2669-5 2668°2 2667:9 2666°7 2666-2 26659 26652 2664-41 26641 TUNGSTEN (SPARK SPECTRUM)—continued. Intensity and Character pi 6B bot tat FRO) RO Fat Bot HRD Ft BD HRD BO BD BD Et BD BB PRE ED DEPEND NDP PREP EP EDEN EP REE DDE eee be deb Previous Measurements ° (Angstrém) Reduction to Vacuum A+ oe A 0-78 | 10:7 ” »” ” ” ” ” ” ” Be 10°8 ” ” ” »” ” ” ” ” ” ” O77 + »” ” ” ” ” »” » ” ” ” »” »” » ” ” ” ” ”) ” ” » ”» ” »” ” ” ” ” ” ” » ” ” ” ” ” ”» ” ” ” ” ” ” ” ” ” - 10°9 Oscillation Frequency in Vacuo 36929 36933 36944 36947 36977 36982 369958 37004 37018 37022 37034 37045 37052 37056°4 37081 37093 37099 37100 37106 37126 37136 37147 37175 37186 37196 37202 37211 37226 37229 37238 37250 37255 37279 37291 37305°7 37314 37329 37351 37357 37367 37374 37382 37397 37402 37418 37434 37449 37467 37472 37489 37496 37500 37510 37520°9 37525 tal 3) 99 400 Wave-length Spark Spectrum (Rowland) 2663°7 2663°0 2662°4 2661°8 2660°8 2659°9 2659°4 2658°10 26580 2657°5 2656°7 26562 2655°7 2654°7 26545 2653°7 2652°1 26515 2651°1 2650°4 2650°0 2649°8 264781 2646°9 2646°2 2645°7 2644°7 26441 2643°3 26431 2641:1 2639 6 2639'2 2638-7 2638'3 2637°2 2636°7 2635°4 2634'9 2634°0 2633°2 26329 26314 2630°4 2629°6 2629'1 26283 2628 1 26278 2626°9 2626°5 26263 2625°7 2625°2 2624°0 REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. Intensity and Character i=] ee ee eee 5 te ee ae er he ee ee ee ae Previous Measurements (Angstrém) Reduction to Vacuum 1 At xX 077 | 109 ” ” ” ” ” ” ” ” ” ” ” ” ” 2 ” ” ” ” ” ” ” ” 0-76 | 11-0 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” 2” ” ” ’ ” ” ” ” ” ” ” ” ” ” ” ? ” ” ” ” ” ” ” ” ” ? ” ” ” ” ” ” ” a 111 ” ” ’ ” ” ” ” ” ’ ” ’ ” ” i ” ’ { 29 ” ” Oscillation Frequency in Vacuo 37531 37541 37549 37558 37572 37584 37591 37609°0 37611 37618 37630 37637 37644 37658 37661 37672 37695 37703 37709 37719 37725 37728 377501 37769 37779 37786 37800 37809 37820 37823 37852 37874 37879 37886 37892 37908 37915 37934 37941 37954 37966 37970 37992 38006 38018 38025 38036 38039 38044 38057 38062 38065 38074 38081 38099 I ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 401 TUNGSTEN (SPARK SPECTRUM)—continued. -Wave-length Spark Spectrum (Rowland) 2622°9 2622-3 2621°7 2620°8 2620:25 2619-2 2618-0 2617°2 2616-7 2615°48 26144 2613'8 2613-1 2612°8 2611:9 2611-4 2610-7 26103 2609-2 2608-4 2607°1 2606°5 2606°4 2605:9 2605°5 2604:5 2604-2 2603-6 2603-07 2602°58 2602-1 2601°5 2601-2 2600°9 2599-7 2598-9 2598-5 2597-9 2596-9 2596-2 2595°6 2594-9 2593:8 2593-4 2592°9 2592-6 2591°5 2589-7 2589-20 2588°5 2587°9 2587°5 2587-2 2586°6 2586°3 1898. Intensity and Character bee Tee rea RO EB BD at — B ee oe a ell So el ll ell ol ll ol el ed ee Oe em ry o i=) Cell ell eel ell sel ec ee ee Previous Measurements Q (Angstrom) Reduction to Vacuum 1 A+ —=— O76 | 111 » ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ”» ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” 75 | 11: 0° 11:2 32 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” bh) ” ” ” ” ” ” bh) ” ” ” ” 4 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” th i ee Oscillation Frequency in Vacuo 38115 38123 38132 38145 38153-2 38169 38186 38198 38205 38222°8 38239 38247 38258 38262 38275 38283 382933 38211) 38315 38327 38346 38355 38356 38363 38369 38384 38389 38397 38405-0 38412-2 38420 38428 38433 38437 38455 38467 38473 28482 38496 38507 38516 38526 38542 38548 38556 38560 38577 38604 38510°8 38621 38630 38636 38641 38650 38654 DD 402 REPORT—1L898, TUNGSTEN (SPARK SPECTRUM)—continued. Reduction to Wage Intensity | Pyevious’ Measurements yponum Oscillation speeerani pa (Angstrém) : ~ Frequency (Rowland) Character Pe a savers 25857.° | 1 0-75 | 11:3 38663 26851 / 1 5; c 38672 2584-2 2 je i 38686 2583.3 1 * i 38699 2582'5 1 is 3 38711 BbeRiS 1 i : 38714 2681:22 4 is Z 38730°1 258015 1 53 38744 2579°8 1 i ite 2579°60 4 Z i‘ 28754-4 2579°32 4 ” ” 38758°6 2578-7 1 ‘ f atte 2578-2 1 ; = 38776 2577°8 1 : s Hil 2577°5 1 i é 38786 2577-2 1 3 fi 38791 2576°7 1 , i 38798 2576-2 9 ? : mth 2576-0 2 é 38809 2574-9 = : : mec 2574-1 in = 3 38838 2573-8 1 : : 38342 ies 1 ee 8s. 38848 2573-2 1 is . 38851 es 1 - : 38859 9572-4 1 ‘ : 38863 2572-30 4 é e 38864-4 257145 4 cs ees 38877-3 aos 1 , hee 38903 2568°7 2 . Re 38919 she 1 < a 38933 ala 1 oe © 38934 2567-4 2 3 - 38939 2566°8 1 a is 38948 25666 1 Ee « 38951 2566-2 1 x = 38957 2565°7 1 a! 38965 fatite In O74} 38984 20637 2 aay eS 38995 2563-4 - 1 : = eae 2563-22 4 : ae 2562°5 2 3 39013 25622 | 1 3 : ate aoe eee nae | 39023 2561°5 1 a # 39029 25607 | 1 3 f 39041 25599 | 1 < 39053 25594 | 3 cee ties 39061 25579 | 2 af - 39084 ple Ra at ee 39091 2557-1 1 . i 39096 2556°9 1 x _ 39099 2656'6 1 39103 * Double. 3 a“ ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 4.95 TUNGSTEN (SPARK SPECTRUM)—continued. _ Reduction to aa Intensity Previous Measurements | Veruc Oscillation (Angstrém) . gays AF ie A Irs O74 | 11-4 39114 3 4 391255 5 39131 * re 39134 99 Ph 39148 : 39157 : a 39171 = 39174 = s 39185 - ‘ 39189 = ‘ 39203 A a 39206 ae init 39222 39224 l 39228 - 39238 ‘ 39250 39262 39276 39285 ss = 39298 39307 ¥ 39333 " 95 39336 39344 39361 39370 = 4s 39375 ” ” 39377 39386 e 39397 39411 | DRED ee he bo bo bo bo ee =] 6b 39414 39428 39440 39451 39459 39465 39470 39472 39479 39484 39500 39504 39518 39520 39526 39529 39536 39542 39550 39573 | 39581 39584 Bs 39592 DD2 Dt ee eee ene en CnC Ce ee Clee Oren w 2 se + ve SSS Ss 8 404 REPORT—1898, TUNGSTEN (SPARK SPECTRUM)—continued. Ww sae Reduction to eo Intensity Previous Measurements Yacuns Oscillation Spectrum eae (Angstrém) r Frequency (Rowland) Character res —- in Vacuo 25248 1 0-74 | 11°6 39595 252471 2 ” is 39606 2523°5 1 = ce 39615 252-4 1 a 7 39617 2522°9 1 2 ; 39625 2522'8 1 i; if 39626 2522°08 4 A > 39637°2 25211 1 : 3 39653 2520'4 l _ : 39664 25200 1 B i 39671 2519°0 1 re . 39686 2518'6 1 rs . 39693 251871 2 i _ 39700 2517°3 2 C13 = 39713 aby 1 » | on 39718 2516'1 2 oS ae 39732 201577 1 i z 39738 2515°3 2 4 39745 25144 2 . : 39759 2514°3 2 : Z 39761 25139 2 “ ns 39767 2513-2 2 * ei 39798 2512-7 2 . 7" 39786 9512" 1 ‘ 39795 2511°7 if ae 11:7 39802 2511°3 1 4 if 39808 2510°9 1 nS * 39814 2510°52 4 es 39820'7 2505°9 1 . ¥ 39830 2509'6 1 J 39835 2508°6 1 re is 39851 2507°9 102 = mt 39862 25071 1 ‘ - 39875 2506'S 1 i AF 39879 2506-0 2 a 2 39892 2505°5 In = 2 39900 2504-7 In i A 39913 2503°6 In 7 . 39930 2502-0 1 - ie 39956 2501°8 ] J “4 39959 2501-0 1 . i 39972 2500-4 “aL vital See 39975 2500°1 2 ‘ ie 39986 2499-7 1 cf a 39993 2499-2 2 s Lt 40001 24989 1 ine ; 40006 2498-2 In [a # 40017 2497-75 2 i 2 40028 2496-6 2 is a 40042 2495°5 1 | Fe a 40060 2495°3 1 . * 40063 2494-9 1 a 3 40070 2494-1 In [ee aha 40083 2492-9 2 y y 40102 24922 2 late Ana 40112 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. | Wave-length Spark Spectrum (Rowland) TUNGSTEN (SPARK SPECTRUM)—continued. Intensity and | Previous Measurements Character (Angstriiin) 2491°7 2490°6 2490-2 2489°9 2489°35 2488-92 2488°2 2487°5 2487°3 2486°3 2485°6 2484-7 24843 2484-0 2483°6 2482°1 2481°6 2480°9 2480°2 2479-1 2478°9 2478°7 24783 2477°93 2477°2 2476°6 24757 2475°6 2474-3 24742 2473°9 2473°2 2472°4 2471°7 2470 9 2469'9 2469°2 24684 2467°4 2466°5 24659 24656 2465°2 2464°6 2464-2 2464:0 2463°2 © 2462°8 2462°3 2461-9 2461-4 24612 2460°4 2459°8 2459°6 Re D RH RR eb bb be Dee Eee be Ree be i=] °O [=a Sf=| Hee be B Baa ak ae re Bt Fk A RO Reduction to Vacuum Oscillation Frequency in Vacuo 405 40121 40139 40145 40150 40159- 40166 40178 40189 40192 40208 40220 40234 40241 40246 40252 40276 40285 40296 40307 40325 40328 40332 40338 403445 40356 40366 40381 40382 40403 40405 40410 40421 40435 40446 40459 40475 40487 40500 40516 40531 40541 40546 40553 40563 40569 40572 40586 40592 40600 40607 40615 40619 40632 40642 40645 ee Oo 4.06 REPORT—1898. +g TUNGSTEN (SPARK SPECTRUM)— continued. ——— : oe oe | Wave-length 5 ) ae e a4: | Spark Thtensity Previous Measurements | Oscillation — | geen | chhed| | nun 1] Breaueney (Rowland) pee tere ere | 2459: 1 0-72 120 40652 2458-7 2 of y 40660 aon | (s || eee 24565 1 4 s i888 2456°1 1 is & 40703 2455-9 2 és % 40706 2454-9 i _ = 40723 2154-8 1 vi A 40725 2453 1 fi Ks 40741 2452-9 1 . 3 40756 | 2452-0 1 ‘ 40771 2450-3 1 e ia 40799 | |) =|] gt] | ae 2148-2 2 i Ls 40834 re) 4 é 51 | 2446°50 4 ” ” 40862°7 | 2445-5 1 if b 40879 | 2444-9 if ” ” 40889 | Sass 1 oly et | eae 2441-6 1 Mel hig? 40945 2441-4 1 ig S 40948 2439-9 1 . A 40973 pres i mide i. | 2491-1 2 o71/ . 41292 Bp | 24206 2 Oe 8 ee. 41300 te > : ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 407 ‘o Wave-length Spark Spectrum (Rowland) 2420-0 2419-4 2418-2 2417-9 2417°6 2416-0 2415°7 2414'8 2414-2 24133 2412°8 2411°9 2411-6 2411-4 2411-2 2410°5 2409°5 2409°3 2408°3 2407°8 2407-2 2406 6 2406°3 2406 0 2405°6 2405°3 2404:9 2404°3 24034 2402-4 2399°9 2399°2 2398°1 2397-12 2396'2 2395-6 2395-4 2395:1 2394-4 2393°2 2393:0 2391°8 9391-2 2390°9 2390°4 2389-8 2389°3 2388°8 2388-6 2387°7 2386-5 2386-2 2385°5 2385°3 2383'5 Intensity and Character TUNGSTEN (SPARK SPECTRUM)—continued. Previous Measurements (Angstrém) Reduction to Vacuum Oscillation Frequency in Vacuo Fe ene ee een BSL et bet att Std OR as to eSNG rt RD et Pt th et tt 0 fet tt 41310 41321 41341 41346 41351 41379 41384 41399 41410 41425 41454 41449 41454 41458 41460 41473 41490 41494 41511 41520 41530 41540 41546 41551 41558 41563 41570 41580 41596 41614 41656 41669 41688 417043 41721 41731 41735 41740 41752 41773 41777 41798 41808 41813 41822 41833 41841 41850 41854 41869 41890 41896 41908 41911 41943 408 REPORT—1898. TUNGSTEN (SPARK SPECTRUM)—continued. a eee Reduction to Wave-length 2 wach eet Spake Tnjensty Previous Measurements Cooter Spectrum | (yp, en t (Angstrém) : iregateiicy (Rowland) pracker A+ | >= cuo 2382°7 1 O71 | 12:5 41956 2382-4 1 f r 41961 2382-0 1 0 | hoe 41969 2381°8 1 Ona 41972 2381-4 1 4 ‘ 41979 238 1°2 1 x Af 41983 2380°9 1 bs = 41988 2380°4 i! , 41997 2380°3 1 e A 41999 2379°7 1 2 ie 42009 23782 il ee fe, 42036 2377-1 1 i ts 42055 2375:9 1 = ns 42076 23745 2 ie ‘: 42101 2373 7 1 0:70 * 42115 2373°4 1 33 i 42121 2372-7 2 mi i 42133 2371:9 1 a if 42147 2371°1 1 as a 42162 2370°1 2 eo 42179 2369:0 . = oa 42199 23684 2 » | 126 42210 2367°8 al a 4. 42990 2367°2 1 a a 42221 2366:7 1 a - 42240 - 2365°9 1 ee s 49254. 2365°5 1 v4 42261 2364-4 2 é me 49981 2364-1 1 os ~ 42286 2363°5 1 = bs 42297 2362°2 2 ss ns 42320 2361-7 1 “ :, 42329 23613 1 at eas 49337 2359-4 1 ee: 49371 2358-9 2 ei Boe 42380 2358-1 1 pens ae 42394 2357-4 1 lee 42407 2356-9 1 a ee 42416 2353-7 1 ” | 437 42473 2353°5 if a E 42477 2351°6 1 fi ee 42511 2008 1 ph 49517 2350°4 1 . si 42533 2349:9 T G a 42542 2349°4 2 . d 42551 2a882 2b # ; 42573 2346:5 1 A 5 42604 2345-0 1 a 49631 2344°5 1 4 ‘ 42640 2343°7 2 vi 4 42655 2341°4 1 x if 42696 2389'7 1 » | 128 42728 2339°1 1 id 42738 2337°7 1 z. a 42764 tii 1 Ag (a 42781 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. TUNGSTEN (SPARK SPECTRUM)—continued. Wave-length Spark Spectrum (Rowland) Intensity and Character Previous Measurements “4 (Angstrém) 2336°0 2335-2 2334-7 2333°9 2333:2 2332-2 2331°6 2330°6 2329°5 2328°4 2327 6 2326°7 23260 2324-7 23240 2323°1 2321:0 2319-0 2318-0 23147 23142 2313-0 2310°7 23099 2307°1 2305°8 2302°7 2301°9 2300°5 2299-4 2298-9 2298°5 2297°2 2295°7 2294°3 2293°2 2291°6 2290°8 2288°8 2284°8 2284-1 2283:4 2282'1 2281-4 2281°1 2280°7 2278°3 22779 2275°3 2272°7 2270°5 2266-5 2264°6 2263'3 2262°6 wee ee BSB Ll cell cel ell oe el ee SO Od 5 B Q ~— a aa a eral a ae Bee ee Pe Reduction to Vacuum 1 _— A+ x 0-70 | 12°8 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” 12°9 ” ” ” ” 0°69 = ” ” ” ” ” ” ” ” ” ” ” ” ” 13:0 ” ” ” ” ” ” ” ” ” ” ” ” ” ” " 13-1 ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” ” bh) Aa 13:2 ” ” ” ” ” ” ” ” ” ” ” ” ” 0°68 i + 13°3 ” ” ” ” ” ” ” ” - 13°4 Oscillation Frequency in Vacuo 42795 42810 42819 42834 42847 42865 42876 42894 42915 42935 42950 42966 42979 43003 43016 43053 43072 43109 43128 43189 43198 43221 43264 43279 43331 43356 43414 43429 43456 43477 43486 43494 43518 43547 43573 43594 43625 43640 43678 43755 43768 43781 43806 43820 43825 438338 43879 43887 43937 43988 44030 44108 44145 44170 44184 409 410 REPORT—1898., - TUNGSTEN (SPARK SPECTRUM)—continued. Reduction to Wave-length : Vacuum ison ta ee coed Previous Measurements vee Gneaenteios . Sa aay Clincaster , (Angstrém) A+ i- in Vacuo 22603 1 0-68 | 134 44299 2259-4 1 t a 44247 2258-4 im cs a 44266 2257-4 1 : i 41286 2256-7 1 . 44299 22552 1 i, ‘ 44329 2251°6 1 e 2 44400 2250-9 1 | 185 44413 2950°2 1 . ¥ 44426 2249°5 1 F 4 44440 2248-7 1 < if 44456 22459 1 « if 44512 22453 1 ‘ 44523 2243-8 1 A s 44553 2243-0 In x e 44569 2241-4 1 Z S 44601 2240-2 In ms : 44625 2937-1 1 ~ | 186 44687 2935-6 1b A . 44717 9931-4 1 = 44801 2999-6 1 oe7 | | 44837 2227-0 In id 44889 2226-1 In | 13-7 44908" 2222-3 1 44984 2221-7 1 a es 44997 2219-4 1 “4 ‘ 45043 2218-0 1 a : 45072 9216-2 1 ss 45108 22155 1 ¥ i: 45123 9215-1 1 "| 13:8 45131 2208°7 1 ? 45262 2206°7 1 : Es 45303 2204-4 1 ft 45350 2201-1 1 "| 1359 45418 2198-9 1 i é 45463 2198-2 1 2 : 45478 2197-7 1 ty i 45488 2196-0 1 e ‘ 45523 2194-9 1 Hs i 45546 21952 1 ; 4 45581 2189-7 1 ” | 140 45654 2186°7 1 ‘ 4 45717 2186-0 In . ‘ 45732 2182-2 1 a a 45811 2166-2 1 066 | 14:2 46150 2163°7 1 is cs 46203 2161-2 In i : 46257 2153-7 1 | des 46418 21525 1 = ; 46444 2146-2 1 | | 144 46580 | ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 411 Pratinum (SparRK AND Arc SpEctTRA). Kayser: ‘ Abhandl, kéngl. Akad. Wissensch. Berlin,’ 1897. Exner and Haschek: ‘ Sitz. kaiserl. Akad. Wissensch. Wien,’ civ. (1895), cv. 1896, cvi. (1897). ‘ | Wave-length Intensity Reduction to __._ ee and Previous Vacuum Oscillation | Bienes and. Character Observations | |—_______| Frequency | Haschek oho _ (Angstrém) eset ee Vacuo | Spark Spark | Are A 5861-074 2 1:60 | 46 17057'1 5845:050 | 4 5845°1 Thalén | 1°59 ” 17103°9 5840-354 | 5 iy 9 LTT 5763'778 3 1°57 4:7 17345:0 5762877 3 :, ” 17347°7 5728°369 | 0 1:56 ” 17452°3 5700°672 | 0 155 | 48 17537-0 } 5699°190 | 1 A ” 17541°6 5684-908 | 2 55 FA 17585°6 5660°245 2 1:54 » 17662°3 5626:077 4 1:53 ” 17769°6 5514°324 4 1:50 | 4:9 18129°7 | 5478°722 6 54781, = 5:0 18247°4 5475:996 | 6 54756, 1-49 ” 18256°5 5469°714 | 2 - - 18277°5 5452984 0 fA “ 18333°6 5391-010 | 4 1:47 51 18544:°3 | 5388-105 2 5389°6 ” ” ” 185543 | 5869°188 4 53676 a, op ” 18619-7 | 5324:799 0 1:45 ” 187749 | 5819:540 0 » ” 18793°5 | | 5306:493 0 _ » 18839°8 5301-182 6 53016 ,, 52 18858°5 | 52957918 | 0 ‘ + 18877°3 | | 5286°289 On 1:44 » 18911:7 | 5275-008 On ™ 45 189521 5265°290 0 ” ” 18987°1 | 5260°982 3 ” ” 19002°7 | 5257-609 On ” ” 190149 5227°782 | 6 52262 ~=«a 1:43 5 19123°4 5208°775 | 0 142 | 33 19200°4 5194:050 1 ” ” 19247°5 P 5118-583 | 1 1:40° Ly 19531°4 5095:950 On 1:39 | 5-4 19618-0 5059°658 5 50596 ,, 1:38 + 19758°8 5050-006 1 ” ” 19796°5 5044°645 6 5 bs 19817°6 5044194 4 ” » 19819°4 5038°681 “0 ” ” 198411 5037°859 On _ by 19844:3 5033°686 4 es - 19860°7 5002°762 2 1:37 5°56 19983°5 4998123 2 43 be 200020 4980°532 1 1:36 bs 20072°7 4879-700 4 48791 ,, 1:34 5:6 20487 5 4862°577 0 1:33 § 20559°6 4854-067 4 5 5-7 20595°6 i | 4831°371 0 1:32 ¥ 20692°4 4772°467 1 1:31 5°8 20947:7 4746°046 1 1:30 FP 210644 4739°924 1 5 i 21091°6 Nors.—In the arc spectrum the intensities are estimated on a scale from 0 to | 10 : 0 denoting a very weak line. 412 REPORT—1898, PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Exner and Haschek Spark 4640°8 4640°5 4577:0 4560°2 4558°9 45548 45543 4552°62 45480 4546:3 4523°2 45212 4514°3 4511°3 4510°9 4505'0 4498-93 4495-0 4493-4 4492-7 4484:8 4482°2 4481-9 4473°7 4471°8 4458-9 4457:2 4453-3 4448°8 4445°7 4442-73 44375 4411°5 4410°9 4409°0 4392-0 4372:0 43645 4358°5 4351°3 4347-0 4341°9 4334:8 43272 Kayser Are 4737-722 4684:255 4658-105 4650°192 4639:984 4580°828 4580-685 4577:584 4560°209 *4554-759 *4552°586 4552°116 4548-056 4523-192 4521-099 4511-417 *4498-926 4493-350 4484882 4481°808 4473-633 *4445-710 *4442-730 4437-470 4414-420 4411°580 *4391-999 4364°624 4358°522 4343°852 4334-827 *4327°243 Intensity and Character Spark} Arc 2 4 5 1 u 4 2 2 In 4 1 4 1 1 4 2 + 5n 2 1 3n i 1 5n 1 5n 1 1 5n 1 1 4 6 a 1 3 1 1 5n 1 1 3 1 3n 1 iL 1 In 1 1 4 4 6 1 4n 2 In 3 1 In 2 4 1 1 4 In 2n 2n 1 0 1 In 2 4 4 Reduction to Previous Vacuum Observations a (Angstrém) ve I A 1:30 | 58 1:28 59 1:27 BN ” ” 1°25 6:0 ” ” Hi 61 ” ” ” ” ” ” 4551'9 Thalén 55 i ” ” ” ” ” ” 1:24 ‘, 4521 Huggins As oe ” ” ” ” ” ” 1:23 as 4498°3 Thalén os iS 2 62 ” ” ” ” ” ” ” ” ” ” ” » ” ” 1:22 u ” ” ” ” ” ” ” ” 4442-1] ” ” »” ” ” 1:21 6°3 ” ” ” ” 4389°5 ,, 1:20 a a 6:4 ” ” 119 Ne ” ”» ” ” ” ” ” ” 43270 ,, 53 5. Oscillation Frequency in Vacuo 21101°4 21342°2 214620 21498°6 215459 2182471 21824°8 21839°6 21922:7 21929 21949-0, 21951 21959°4 21961°7 21981°3 21990 22102°2 22112°4 22146 22159°9 22162 22191 22221°4 22241 22249-0 22252 222909 22304 223062 223470 22356 22421 22429 22449 22472 22487°4 22502°5 225292 22646°7 22661°3 22665 22675 22762°4 22866 229051 22937°2 22944 22998 23014:7 23025 23062°6. 23103-0 * Rowland 4554-828, 4562594, 4498930, 4445°713, 4442-723, 4891-996, 4327320. a ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 413 PLATINUM (SPARK AND ARC SPECTRA)—continued. Wavye-length Intensity Reduction to a and Previous Vacuum Oscillation | Exner and Character Observations |———~—_—_| Frequency Haschek oa ers lose | C(Angstrém) i 1__ | in Vacuo Spark = Spark} Arc x 4309°3 In 118 | 64 23199 4291-2 4291:070 | 1 2 (Rowland) be 6:5 23298°5 4288°6 4288215 | 1 4 4288217 BR. 9 ” 23313°2 4281-905 1 of ee 23347°6 4275-2 1 117 » 23384 4274-2 4274:042 | 1 2 % < 23390°6 4271°2 In a re 23406 4269°7 4269411 | In 2 in “ 234159 4263°8 4263°664 | In 2 oh + 23447°5 426071 1 a ” 23467 4251:277 1 2 6°6 23515°7 4247-8 4247°838 | In 1 ” ” 23534°8 4226°85 Ca 4 116 3 23661-7 4223°8 1 > ve 23669 4222°7 1 ” ” 23675 4221-2 1 _ 9 23683 4214-2 1 ip of 23723 4213°3 1 + rf 23728 4211°5 i 3 23738 4205'8 2n 115 iy 23770 4202°2 1 * cp 23790 4201°5 4201:374 2 ” ” 237952 41945 1 %5 67 23834 4192°55 4192-577 | 4 4 ‘589, . 55 23846°0 4185°7 2n ns 5 23884 4170'S 1 * 3 23971 41675 1 1:14 +p 23988 41665 1 5 5 23994 4164:72 4164709 | 4 4 SCP. ep if a 24004:6 4163°5 2n ” ” 24012 4159-0 1 FS ic 24037 4148°5 1 a" 6'8 24098 41343 1 +t H 24181 4133°7 -2n ” ” 24185 4132°5 1 is © 24192 4129°7 1 1:13 A 24208 4118°86 4118°854 | 6 5 828 =, > Os 24271°8 4092°5 4092°426 | 1 3 421 ,, 1:12 | 69 24428°5 4090'5 1 ” ” 24440 4087'7 1 ” ” 24457 { 4081°631 Ii 627, " a 24493'1 | 4078°1 1 3 A 24514 4072°2 2 5 -F 24550 4066°5 4066 087 | 1 2 S098 ys; 5 7 24586'8 4063'0 1 ” ” 24605 4061-9 1 3 . 24612 40607 : In Fi = 24619 4055-0 4054928 | 1 2 SPAT ey Le . 24654-4 4051-2 1 % 7:0 24677 4050°2 1 Pe = 24683 4046°55 4 ” ” 24705°4 40343 1 ” ” 24780 4024-0 1 ” ” 24844 4021 “4 1 | ” ” 24860 4014°3 Ty 1:10 5 24904 414 REPORT—1898. PLATINUM (SPARK AND ARC SPECTRA)— continued. Wave-length Intensity Reduction to an Previous Vacuum Oscillation Exner antl Character Observations © —_—____| Frequency Haschek ‘ges mm = (Angstrom) re 1 in Vacuo Spark aC Spark | Are : en 4007°5 1 1:10 | 7:0 24946 4002-7 4002°649 | 1 2 i 71 24576°3 3996°7 3996°720 | 1 3 ‘722 BR. 3 53 250134 3980°746 1 ” ” 25113°8 3979-0 herd: In - 5 25125 3976°5 3976°460 | 1 1 " ' 25140°9 3975°8 1 1:09 pe 25145 3972-0 1 » aA 25169 39713 1 4 " 25174 397071 2 a 3 25181 3969-3 1 r = 25186 3968°5 Ca 6 ‘3 3 25191 3966748 3966507 | 6 3 504, 5 7 25204:0 3961-7 1 “4 43 25235 3458-0 1 5 a 25258 3953:1 3953°780 | In 1 a5 7:2 25285:0 | 3950°6 In *) ‘ 25305 3948-4 3948550 | 1 4 539, “ a3 25318 6 39310 1 1:08 5 25432 3930°5 1 2 et | Bpase. | 3927:1 1 5 $i 25457 | 3926°6 1 . Ke 25460 3925°50 3925°483 | 4 4 486, D ; 25467°4 3923712 3923:105 | 8 =) 106, + .) 25482°8 3911-1 3911045 | 1 3 050 _,, ” Pe 25561°4 3910°6 1 ki * 25564 3908°5 1 i 73 25578 3906°433 2 s 3 25591°5 | 3904-4 3904°534 3 93 25604-0 3903°864 2 oh + 256084 3902°3 1 _ Ae 25619 | 3900-90 3900°873 | 4 4 874 59 a 25628°0 3898-92 3898°880 | 4 4 886 4 a 25641°1 3895°5 1 1:07 25663 3894-9 1 i As 25667 3892-0 In 3 #5 25688 3890°5 In ¥ 5 25696 3889'2 In wi a 25705 | 3887°5 1 = “ 25716 3885°3 In - er 25731 3884'3 In 3 * 25737 3883°3 in A m0 25744 3881°1 In Aa - 25759 3875-83 4 Pp = 25793°6 3873-7 In 7 - 25808 3868-60 4 “3 5 25842 3863'3 1 a 4 25877 3856°5 1 1:06 + 25923 38548 In b _ 25934 3852°7 il fe ss 25948 3847°6 in - 5 25983 38453 i 3 #5 25998 3843-8 1 3 » . | 26009 3838'3 2 7 i 26046 3837°8 In id , | 26049 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 415 PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Intensity Reduction to and Previous Vacuum Oscillation Exner and K Character Observations = |——________ Frequency Haschek suey = SS (Angstrém) a 1_ | in Vacuo ne Spark | Are + > in | 1:06 | 7-3 | 26067 1 26081 i 26106 1 ” ” 26121 6 * 26178°7 2 1:05 74 26203 26250 | 26259 | 1 é | 26270 1n ” ” 26286 1 is », | 26290 26299 i - , | 26821 In ” ” 26365 1 A "| 26379 1 ot , | 26386 In 2 «| 26411 In 104, ,, | 26471 In . | 26483 In , rs 75 | 26509 In 1. ears ; 26527 2 si | | 26585 26541 2 ” ” 26559 n be ns 26578 26625 26659 4 | 26666 | 3818°827 26678 26686 26703 S ky 26726 + 5 26735 103 | ” | 9676c i cp 26786 + 3 26791 7 3 26810 ” 76 26814 26819 3 26834 1” o6g53 i ” | 96856 26897 " ” | 96932 667, 5 " 26970°6 3 - 26981 27016 4 059, an ST hee : ” | 97095 102 | ” | 97056 *) i 27088 ‘BBA, s , | 271105 123 =O, cy 77 27142°8 * Pe Pears a he a | [=] . < - i=} 3706°685 3700-070 3687-582 3683169 > BH Oe eee ee be ee be Dee ee w 416 REPORT—18Y8. PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Intensity Reduction to j ee Previous Vacuum Oscillation ae pi | Kayser Observations Serr rae Frequency asche I = iyi | Anosten in V: Spark | . Are Spark | Are (Ang yeromy) sie Le ta es a | , 3681°3 3681:227 | 1 0 209 R, 1:02 | 77 | 271571 3680°8 1 mt ‘i 27160 an eae = | aa j a | ” ” 27196 36752 | 3676107 | 2 1 . - 27202-4 36743. | 3674207] 6 4 ‘191, § hs 272090 3672°2 3672165 | 6 4 142 ,, fe ie 272942 36686 | 3668564] 1 1 - x 27251-0 sts ee > |e | Sas 7) j F ” b] 27 3663°5 3663-239 | 1 beat 249, 2 ” | 97290-5 3662-0 1 ; 27300 3659°6 3659°571 | 1 re | 564 ,, ie ” | 97317-9 654 . ; 735 3654-2 3654-132 | 1 11/4] i ” | 97358-6 3653°5 1 | Ri is 27363 3652°5 3652-411 | 1 arth = $s 27371°5 3651'S 1 | . ” 27376 3643°3 3643331 | 6n | 6 313, is | 297439°7 3639-0 3638-956 | 6 6 944, a 78 | 27472-6 3687°3 2 - s 27485 36367 1 - é 27490 3636°5 1 mn 2 27491 3629 0 3629-025 | 6 3 ‘017 _,, ‘. a 27547°8 3628°3 3628-275 | 8 5 272, Ss i 27553°5 3627°8 4 i 2 27557 3625-4 : ii 27575 36227 In % e 27596 3621°8 3621°839 | 1 2 TA ee a » | 276025 3617°3 1 1:00 | ,, | 27637 3615-4 3615°443 1 0 ” ” 276514 3611-0 3611-057 | 2 2 | 060 ,, : i: 27684-9 stb | 2 | dias | 3605-4 In | ol ow pare | 3602-9 1 ss F 27748 | 36024 | In ae hee 27751 | | 3594-4 | in » | .79 [37613 | 3589-2 1 Pere Fe E 27853 1) Seeger} | 1 / he « 27865 1 35871 | 1 / fh ees d 27870 | 35858 | 1 OT ae 27880 | 3585-4 1 ce: a ieese 27883 | 3583-2 1 1 | 9» pete 27900 | 3578-8 1 V1 = 27934 | 35780 1 | O99} 27941 | 35776 1 _ 4 27944. | ) 3574-2 4 a HOE 27970 | 3573°5 ‘ r 27976 | 3572'3 1 ia ” | 97985 | 3571-4 ; i 2” ” 27992 3568-5 ¥ t 28015 3565-4 In | “ss 3 28039 3559°9 ln i 7 . 28083 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 417 ——— PLATINUM (SPARK AND ARC SPECTRA)—continued. Exner and Haschek 3523°7 3522°6 3519°7 35186 35149 3513°7 3505°9 3503°6 35026 3498-3 3498-0 3492-0 3491-1 3490-2 3487°8 3485°3 3483°5 3482-4 3480°6 3476°9 3474°9 8471-4 3464-1 3460-9 8459-7 3455-9 3454-2 3453-9 8449-0 8448-5 3447-9 84415 3434-9 3431-9 1898, Wave-length Kayser Arc 3528°700 3514869 3505°848 3498°321 3491155 3488°877 3485°430 3483-588 3472-080 3464-097 3454'290 3448-523 3452-000 Intensity ne rs ee Gh ee to eon ae eee m=) ict PND ROK — Bp DREN RP RYH and Character Spark} Arc In to Previous Observations (Angstrém) °691 ‘887 835 308 141 411 ‘561 080 285 ” »” A+ Reduction to Vacuum a _ r Oscillation Frequency in Vacuo 79 | 28089 28002 28103 28122 | 28136 28148 28159 28170 28171 28173 28201 28212 28234 28272 28286 28306 28331:0 28346 28350 28371 28380 28404 28412 28442°6 28452 28515°7 28534 28542 28577°0 28580 28629 28635°7 28644 286544 286463 28682:'8 28697°9 28707 28723 28753 28770 28793°1 28799 28859°3 28886 28896 | 28928 28941°3 28945 28986 28989°7 | 28995 29049 29105 29129°3 EE 418 REPORT—1898. PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Intensity | Reduction to zi and | Previous | Vacuum iecoriend Character | Observations - Haschek ei teat hs. | (Angstrém) 1 A+ a Spark gt Spark) Are | a 3431-495 oy | 0:96 | 83 3428-0 3428079 | 4 | 4 | 110 R. ~ ¥ 3426-9 8496887 | 2 | 2 880 ,, 5 7 34257 ” ” 3424'8 4 + 3422-1 | . ” 3421-2 3420°493 | 1 O74 a + 3418°311 0 | of + | 3417-1 3417-227 | 1 Dee | 0°95 3 | 3414-4 3414610 | 1 2 5 ¥ §409°3 if ” ” 3408°6 3408-286 6 } 7 j 277 ” ” ” 3407°7 if: | ” ” 3406-7 3406:733 | 1 el "0 > 3405°9 il | | ” ” 3404-°7 2 | | ” 23 3385-0 1 ey ! 3 8-4 3384:0 2 | ” ” 3374-2 In 0°94 a 3373°2 3372960 | 1 0 r 6 3368°7 3368626 | 1 a. | ¥ Rep : | 3367-2 3367°139 | In 4 | “135, S45 Plies * 3357°2 ° a | 4, | 85 3344-1 3344-031 | 2 Be -037—5, Seay 5 3343°7 1 | | ” ory 3343°2 al: | ” ’ 3342°1 3342-429 | 1 1 | ; §341°3 if | | ” 9 3340°4 In ory ” 3339'8 it or ” | 3338°4 In | 0°93 : 3338'1 3338-214 | 1 cana q, - 3336°3 In \-) 5, 3334-1 In | \iay t | 3883°3 Tre | * : 3327-4 3327:234 | 1 | °°0 ey 3326°1 1 } ” 2 3325-9 3325°861 | 1 2 | 5 Ks 3324-2 ite “f 86 3323-9 3323914 | 2 6 921 | |) “ae 3323-2 ee | ¥ © 3322°8 1 } } | ” ” 3321-6 ier | a > 3319°8 1 \3 Gaps | 3318-6 fet / | a | “Ris In | DEB 53315°6 1 | ” | ” 3315°2 3315:186 | 4 4 182 ,, Ree |g 3313:186 | ‘ee ¥ ‘4 3312-6 3312614 | 2 Ba 7 ; | 33121 3311-959 | 1 2 at 5; “s | 3811-5 311504 | 1 | at a hn | '3310°2 - 1 ee ! pete. 5: | 3308-0 Lee] 2 1 H 3307°8 29133°5 Oscillation Frequency in Vacuo 29162°5 29172°7 29183 29191 29214 29227°3 292459 292552 292776 29323 293319 29337 293454 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 419 PLATINUM (SPARK AND Arc SpecTRA)—continued. Wave-length | Intensity Reduction to and Previous Vacuum Oscillation Exner and ¢ . Character Observations —| Frequency Haschek Ais (Angstrém) 1 in Vacuo Spark Are Spark] Arc Me) ab 3305°9 tH 0-93-| 86 | 30240 3304°3 1 4 30255 3303-0 1 is , 30267 33019 3302015 | 8 8n ‘996 R. web Le 3300-070 | in re 3° ee, | 3298-688 | On 092 | 4 ie . ; 1 ” ” tt 32933 | 3293-820 o | a if 30351°3 3293-615 | 0 ss » | 308531 3292-6 | 1 a i} 30363 3291°5 L | f ; 30378 3290-4 | 3290:363| 4 az. 370 “4, “ 4 30383°2 3288-6 2n is 87 | 30399 3287-8 In “mel dw! 30407 3286'8 3287:245 | 1 a eh ase 30411-9 3285°6 3285°367 | 2 0 3 , 30429°3 3284-9 1 5 i 30434 3284-6 ft | iF é 30436 3283-4 3283-443 | 2 2 436 ,, \ - 30447°2 3283°336 2 “332, , 5 30448-1 3282-6 1 2 ; 30455 3282-0 3282104 | 2 5 “097 5, 5 3 a $279°9 1 o ; : 3278°6 ty 4 ie 4 30492 3277°5 7 is 4 30502 32740 6 “ 4 30535 3273'1 1 | COORe 30543 3272:1 1 ® ; 30553 3270°8 1 is ; 30565 » 8269-3 sl K + | 80579 3268-5 8268557 | 2 | 4 | 570, 2 A 30585°8 3267-1 1 aia, 39600 3266°5 a a 30605 3266-2 1 é ». 30608 3265°5 1 ‘5 i. 30615 3264-2 1 U é 30627 32639 3263'737 | 1 1 is x mies 0 1 ” 79 6 3261818 | 2 4 a ie AS J 30649 0 3261-202 | 1 2 is : 30654:9 3259°866 | 2 4 $59 ,, 0-91 » | 30667-4 3259-282 | 1 1 3 » | 30672:9 3258-551 | 1 0 2 7 30679°8 3256°634 | 1 1 3 > 30697°9 3256048 | 4 6 038, 2 ys | 807034 3255°356 | 1 0 i ia apie? 1 ” 7 ¢ 1 < | i 30718 3253°319 0 eee 2 30729°1 3252785 | » | 88 | 307340 3252117 | 2 5} 103 » ma ue 30740-4 | 3250-481 | 2 Ae || ‘475 yy “ | . 30755-9 | 3248843 | 1 0 | ta |e 30771°4 | 3248-623 2 (ey ie 30773°5 | 3247-388! 6 Bie Jo) eS aera 2 420 REPORT—1898. PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Intensity Reduction to and Previous Vacuum Oscillation Exner and Character Observations |———7~——— | Frequency Haschek deg —S— (Angstrém) a+ | 1_ | im Vacuo Spark Spark | Are | a 3246:0 1 0:91 88 30798 3243°8 3243-533 | 2 2 si » | 30821:8 3242°9 3243-224 | 1 0) - af 30824°8 3241-6 3241°652 | 1 1 ‘ 2 20839°7 3240°9 1 * é 30847 3240°3 3240°324 | 2 5 325) ite = - 30852°4 3239°4 2 i ” | 30861 32368 1 ss ” | 30886 3235°8 In ” | 30896 323358 | 3233-550] 4 5 ‘B41, e ” | 30917-0 3230-42 | 3230-401 | 4 5 ‘406 ,, Z "| 30947-1 3229-4 1 4 ” | 30957 3227°3 3227°305 | 1 2 290 5 * o 309768 3225-5 1 ss ” | 30994 3224-1 1 i | 31008 3223-7 3223928 | 1 0 rd _ 31009°2' 3222-930 0) - = 31018-9' 3222-6 3222°680 | 1 0 4 ” | 31021-3 3221-416 0 is » | 31033-4 3220°9 3220-904 DS Wet 0:90 m5 31038-4 32197 1 = - 31050 3218-9 3218:972 | In 9 - Bi 31057:0 3218-603 1 é ” | 31060-6 3216°5 In é a 31081 3213°5 In 35 8:9 31110 8212-4 3212°502 | 1 2 AnD ey ef Es 311195 3208-968 0 fe , | (B1N53:8 3207-247 0 i », | 81169° 3204-27 3204165 | 6 6 AGL os Es 3 31200°4 3203-1 1 é , aie 3202°6 1 és ” | 31216 3201-9 1 uf ” | 31993 3201-0 4 . » | amie 320079 | 3200848 | 4 4 ‘830 4, : ” | 319328 3199-1 3199°215 1n 0 x A 312487 3199-076 0 2% » | 312501 3198-0 | 2 “4 | eee 3196-5 acs : | ere 3194-4 1 ¥ ” | 31296 3194-2 1 . ” | 31298 3192°6 3192-635 | 1 3 ok, | ee 31913 3291-604 | 2 | 0 ” | 313933 3189-2 Pe "ok. Ta 3188-3 | 2 ; ” | 31356 3185-7 aes yi "| telat 3184-7 a es, (eee 3183-6 | In : ” | 31409 31815 | In oso | 2 | 314938 317971 3179-650 | 2 1 $ 9-0 31441:0 3177-8 SSCL NE i a ie Bi 31460°2 31763 3176081 | 1b | in | 2 ” | 314764 3175-0 3174-959 1 2 ; "| 314875 31747 es ) ¥ ” | 31490 3173°5 1 eee 31502 31703 | I Com 31534 ” ‘ ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 421 PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Exner and Haschek ee Spark 3169°L 3169-006 3168°4 3167°5 3164°6 8160°1 3160°314 3159°26 3159 841 3156°70 3156°686 3155'8 3154°858 3149°5 3148°6 3146°3 3146°2 31443 31420 3141:767 3139-51 3139-503 31378 31373 3136381 3135°1 3134-413 3133°785 3133°5 3133°443 3132°187 3127-1 3126°3 BL24:1 2122°8 3123-065 3122-1 3122°192 3121°3 3121:0 3119°9 3119-911 3119:0 3118547 3118°1 3117-4 3117-0 31156 31145 31130 3112°718 3111:8 3109°5 3108 7 3108°2 3104:8 3104:170 3104:0 3103:°704 3103°231 8102-4 3102-710 3101-1 3101-077 31001 3100-146 30980 3098°887 3097°1 3089°3 3089-780 3088'1 3088 677 Intensity and Character Spark] Arc 1 1 1 in ln 1b 1 4 0 4 5 1 1 1 1 in 2 2. 2 4 4 7 1 1 0 1 1 1 2 4 0 2 In In In 0 In 0 1 1 2 4 1 0 In ln 2 1b 1b 1b 0 1b 1 1 1 1 0 2 2 1 1 0 2 4 4 4 1 On 1 1 0 1 0 Previous Observations Ss (Angstrém) “683 OR. ct =) or S Reduction to Vacuum Oscillation Frequency 1 in Vacuo 31546-6 31553 31562 31591 31633'5 31638-2 31669:8 31679 31688'1 31742 31751 31774 if ¥i 31785 31795 ¥ 31820'1 31843°1 31860 31865 31874°8 31888 31894:8 31901-1 319047 31917°4 fb a 31969 31978 32000 32010:7 32019°7 32029 32032 32043-1 32053 32057°1 32062 32069 32073 32088 32099 321171 32127 32150 of Sd 32159 32164 32205°5 32210°4 32215°3 a 32220-7 32237°6 32247°3 322604 32279 32355'6 323671 22 REPORT—1898. 0] PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Tnbensity and bee Beane to revious mae and K Character Observations saan Oscillation aschek AUP BOT sl ipa a eae ne ° ee Fre Are (Angstrém) 1 Hrequency Spark a Snark | Are = A+ = in Vacuo 3087°31 ) a 3084 9 te to 1 u 0°87 92 | 32381°4 3084-1 3084-217 | 2 3 ” 9 32405°9 3082°5 3082:779 1 0 ” ” 32413°9 3076°8 2 ” ” 32469°3 3076°1 1 ; ” ” 32492 3075'122 0 ” ” 32499 3074°3 3074°938 1 1 ” ” 32509'8 3072°1 3072:042 2 5 042 B ” ” 32511°7 3070°3 3070°369 | 1 9 ae ee ” » 32542°3 3069°8 3069207 | 1 2 ” » | 325601 3067°9 1 = ”? ” SopLEs 3064-6 3064°825 ” ” 586 3063°6 neers 2 ‘824, ” . seu5? 3062-845 ” » 2632 oe a O86 | ,, 32640-0 stk 3061-905 1 ” ” alent k 3059° = ” ” b 3059°2 ae a ss “749, ” » | 32678-1 3058-5 In ” ” 32679 3057°5 in ” ” 32687 3056°1 3056°719 2 (0) ” ” 32697 3055°5 3055-402 3 4 ” ” 32705'5 30549 3054°8 if Dyn ” ” 32719°6 3054-4 on ” re 327261 3049°6 1 ” ” 32730°4 3049-2 1 ” 94 | 32782 304871 3048-6 1 on ” ” 32786 3047'3 2 |» ” 32792°5 3045'8 il ” ” 32807 3044°9 1 ” ” 32823 3012°8 3042°7 a ” ” 32832 3041:3 na nee a 745, ” ” 32855°6 3040°8 1 =. ” ” 32871:1 crete 3039-612 0 > ” odds “ Bien . ” ” 2 is 303455 3036'554 : 6 563 ” ” ” 32922°7 3033°6 1 ” ” 32945 3031-20 4 ” »” 32955 3029°6 1 Lr) ” 32980°8 30282 1 ” » Boer 3026°5 3026744 ” ” 14 3025°3 soa ine ; 4 » ” 33032°6 3025-179 9 ” v_ | 33041°1 3022°9 3022-957 1 3 2, ” 33054°8 ~3021+1 1 085 | 4, | 330707 3020°7 1 ” ” Sate 3 . ” ” 5 3019-0 "Peas » |» | 331085 3017°95 3018: 5 ” ” 114 3017°35 3017-460 ri : 983», » » | 33125:0 7 ” ” 33131:1 PLATINUM (SPARK AND ARC SPECTRA) —continued. Wave-length Kayser Are | | “ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 423 30157510 3015013 3014°636 3012°498 3010051 3005°911 3004269 3003°400 3002°585 3001°504 2998-087 2994°916 2989°915 2988913 2988177 2984 565 2983°882 2982-414 2978:179 2974:252 2969-965 2967:596 2960°864 2959°825 2959-219 2958°650 Oscillation Frequency in Vacuo So bo bo bo PRN HORHEH oor a a bo Pepe HDD BB 6B Bee ee ee f=] Rrk tt i=) 331524 33157°9 | 331620 | 33185°5 33195 | 33203 33212°5 33234 33239 33258'3 332765 332861 33287 33297°3 $3309-4 33322 33333 33345°1 33368 33380°3 33398 33415 3343671 334474 | 33455°6 33468 33485 33490 334961 33503°8 33513 33520°3 33546 33554 33568°0 33594 33603 33612'3 33622 33640 33660°7 33673 33687°6 33719 33722 33741 33748 33759 33764:3 33776-0 33783°0 33789°5 33802 33821 33831 4.24 REPORT—1898. PLATINUM (SPARK AND ARC SPECTRA)—continued. Wavye-length Intensity Reduction to ‘ and Previous Vacuum Oscillation Exner and K Character Observations ~, _ | Brequency Haschek pope ' (Angstrém) ane 1_ | in Vacuo Spark Are Spark | Are A 2954°6 In 084 |} 97 33836 2954:1 In + * 33842 29513 2951°341 1 2 ” ” 33873°2 2950°3 2950°929 1 0 fe 55 33877°9 2949°3 2949900 | 1 2 * cf 33889°8 2948-844 0 “r Py 33901°9 2947°6 In iW Fy 33916 2947°0 In i =F 33923 2946°3 1 “ ss 33931 2944-8 2944879 | 2 3 of 9°8 33947°4 2943°2 1 a5 ” 33967 2942'8 2942-880 4 0°83 ” 33970°5 2941°908 0 ” ” 33981°7 2941:219 2 ” ” 33989°7 2939°4 1 " 5 34011 2938°9 2938°935 | 2 4 3 ¥ 34016°1 29382 In ¥ mA 34025 2937°3 1 7 a 34035 2936°7 1 i os 34042 2934-7 1 as A 34065 2933°3 2933°S37 | 1 0 ” ” 34075°2 2931-7 2 53 5) 34100 2930°9 2930:904 | 2 4 B a 34109°4 2929°89 2929:903 | 6 8r 4 34121°1 2928-7 i Bs i 34135 2928°3 2928°226 | 1 4 As 3 34140°5 2927-040 i ” ” 341544 2925°2 1 B a 34176 2924 9 2 a 1 34179 2922°381 0 $ : 34208°9 2921°5 2921-498 3 ‘ BS 34219°2 2921-336 1 95 9:9 34221-0 2919-43 2919°451 4 A 3 34243°1 2918°2 1 “ . 34258 2917-7 1 5 ay 34264 29167505 2 = 5 342777 2915-278 0 4 > 34292°1 2914-2 2914-443 | 2 0 a A 34302°0 2913-65 2913655 | 4 4 49 3 34311-2 2913361 2 ie 3 34314:7 2912°35 2912884 | 4 0 9 ” 34320°4 2911888 0 ‘ is 34332°1 2910°6 2910°569 | 4 3 s, A 34347°6 29102 1 . és 34352 2908928 0 3 * 34367°0 2908'1 2908008 | 1 4 99 + 34377°9 2905°9 2906001 | 2 4 Bs 3 34401°7 2904258 0) As 3 34422°3 2903-129 0 0°82 ” 34435°7 2901-798 0 : of 34451°5 2901°282 2 FA 99 34457°6 2900-903 0 % = 34462°2 2899-80 2899764 | 4 ] sj ye 34475°7 2898:03 2897-988 | 4 5 ‘3 i 34496°8 2897:2 1 * “5 34506 ao ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 425 PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Exner and Haschek ioe Spark re 2896:245 2895°7 2894:02 2893°984 2893°4 2893°335 2891:873 2891°170 2891-030 2890°54 2890-495 2889°8 2888:2 2888-307 2885°5 2885°447 2884-583 2883-0 2882°7 28809 2878'823 2877-61 2875°9 2875°22 2871'8 2870-4 2870°572 2870:2 2868-783 2867:°06 2866°1 2865°22 2863-0 286271 2860-80 2859°5 *2858'5 2855-866 2854-7 2854781 2853-484 2853-1 2853°207 2852°3 2851-0 2849°8 2849:241 2848-0 2848°406 2845°5 2844-4 2842-1 2840-0 2839°1 2839°345 2838-5 2838°1 2837-643 2837:3 2837°338 2836°5 28348 2834°815 2831°6 2831:981 2830°43 2830402 2828°9 2827'8 2826°5 28246 2825192 Intensity and Character nore lll ae tl ad NNR =) bt et Rt ee OD BB NH Pee PDP =] B 6B me bo BB a eo a to ee Spark} Are L For NNOOPD oOo ft Re) om noo NO WW Previous Observations (Angstrém) Reduction to Vacuum Oscillation Frequency in Vacuo * Double, 345174 34524 345445 34552°1 34569°7 345781 34579°8 34586'1 34595 34612°3 34646°6 346571 34676 34680 34701 34726°5 3474171 34762 34769°9 34811 34826°2 34831 34848:0 34868°8 34881 34891-2 34918 34929 34945°2 34961 34973 35005°5 350189 35034'8 35038°1 35049 35065 35087:0 350971 35133 35147 35175 35201 35209'1 35220 35230°4 352341 35245 35265°4 35300'8 35320°5 35339 35353 35369 35385°6 426 REPORT—1898., PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Intensity Reduction to and Previous Vacuum Oscillation Exner and Kayser Character Observations: © |}———___—— Frequency Haschek ie oS eS (Angstrém) ee 1 in Vacuo Spark Spark} Arc A 2823°3 2822°602 | 2 2 0:80 | 10:3 35409 2822°5 In a A 35418:0 2822-273 0 ” ” 354221 2821-179 0 ” ” 354359 2819-0 1 4 Fy 35463 2818°6 2818-741 1 2 ” ” 35466°5 2818°4 2818354 | 1 4 2 ” 354715 2817°3 2n Be 3 35485 2816°1 1 2? ” 35500 2815°5 1 33 5 35507 2814-1 2814121 | 2 0 A, 3 35524°8 2813°5 2813:080 | 1 2 2 » 35537°9 2810°921 0 yy 5 35565°2 2809-7 2 F 55 35581 2808-9 2 5 os 35591 2808-7 2808:603 | 1 4 5 3 355946 280771 2807-396 | 1 0) * ” 35609°8 28067151 0 “5 5 35625°7 2805°3 in 5 = 35637 2803°5 2803°338 | 1 6 a = 35661°4 2802°8 1 a 3 35668 2801°8 1 ja * > 35681 2800°1 2800-560 | In 0 iy 3 35696°3 2799°7 1 35 se 35708 279871 in ; 10-4 35728 2797°8 2 - 9 35732 2795°5 2796165 | 2 ik 3 a 35752'8 279432 2794304 | 6 5r - is 357767 27937 2793736 | 2 2 es ee 35783°9 2793°3 2793°372 | 2 4 2 ” 35788°7 2791°8 in a s 35809 2790°987 0 a 3 358192 2790°593 0 ” 2” 358243 2789°8 1 5 = 35835 2789°5 1 ; > 35838 2788-6 2788728 | 2 0 # x 35848°2 2784:7 ib 2 oY 35900 2783°6 1 0-79 r 35914 2782°7 i! A % 35926 2779°2 1 <4 ds 35971 2777-558 0 93 = 35992°4 2777°0 2776°859 | 1 0 53 3 36001°5 27767111 uf ss » | 986011°2 277488 2774:880 | 6 2 “4 10°5 360271 2774°306 3 as - 360345 2774:0 2774095 | 1 4 B rs 360372 2773°6 2773°696 | 2 2 » ” 36042-4 2772°925 4 af a 36052-4 2771-78 ‘2771750 | 4 4r ” ” 86067°8 2769°8 2769°940 | 1 4 ” ” 36091-4 2769°0 i +3 35 36101 2767°4 1 4 %§ 36125 2766°6 2766'764 | 1 5 » » 361329 2764-2 In ” 2 36166 2763°30 2763°299 | 4 0 rf > 361781 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 427 PLATINUM (SPARK AND ARC SPECTRA)—continued. Reduction to Wave-length Intensity —---__-- -—____— and Previous Vacuum Oscillation meer nnd Character Observations Frequency Haschek | S*Y8e* |__|} (Angstriim) nea 2 in Vacuo Spark Spark | Arc 5 es 27615 1 0-79 | 105 | 36202 2759°8 2759°424 | 1 0 ¥ » | 36229-0 27587 2758'333 | 1 2 i "| 362433 2758164 0 i ” | 362456 271875 2757:799 | 2n | 2 4 ” | 36250: Q755°7 1 =) ” | 36278 275503 | 2755003 | 4 4 ‘ "| 36987-1 2754-327 0 ‘ ” | 36296-0 2753957 3 fe ¥ 36300°8 2753°8 2753°850 | 2 2 if ” | 363023 2753°3 1 < ” | 36310 = : | ee on be] ” 2752-0 1 $i ” | 36887 2751-4 1 ‘ | | 85888 27500 1 ; 1106 | 36353 2749°3 2 fj , | 36862 2747-7 747-701 | 2 | 4 fy | 363835 2747-0 1 “ ’ | 36393 2746°6 1 i ” | 36398 2745-4 $2. # " 1 36414 2745-0 2744-928 | 1 2 ¢ ” | 36420-2 2743°5 1b sf 1. |) 36aa8 2742-4 1 . ” | 36454 2741-5 In 073 | ° | 36466 31396 t Beopre || gem 2738-5 2738-569 | 2 4 a ” | 365058 2737-6 2737-656 | 1 2 O ” | 365169 2736'886 0 ” | 36527°2 2735'8 2 ” | 36542 27345 2734-584 | 1 2 ¥ ” | 365581 2734-08 | 2734:057| 4n | 8r it ” | ©36565-0 2733°725 br 4 ” | 365695 2732-1 In ; |) | Saeon 2729-9 2730-002 | 1. | 5 bata | Semis 2727-5 1 : "| | 36658 2726-55 4 » | 107 | 36666 2725-433 2 z: » | 36680°8 2721-8 1 4 » | 36730 a nibs [ee 2719-20 | 2719195} 4 6r 6 ” | 36765-8 2717-75 | 2717-709 | 4 0 i ” | 36785-0 27158 2715'866 | 1 2 . ” | 36809-9 2714-613 0 ” | 36827-0 2713-1 2713-215 | 2 4 a ” | 36845:9 2711-0 2 z » | 86876 us 2 | Be 2706-05 | 2705-985 | 4 br x ” | 369444 ee 3 ee y ’ ” 6 270250 | 2702-484] 6 6r ” | 108 | 369922 27012 2701-208 | 1 0 37009°6 428 REPORT—1898, PLATINUM (SPARK AND ARC SPECTRA)—continued. ee Wave-length Intensity Reduction to and Previous Vacuum | Oscillation Exner and Character Observations |_|——______ Frequency Haschek ced Sacer, ome (Angstrém) A+ it in Vacuo Spark 4 Spark | Arc x 2699°5 1 0-78 | 10:8 37033 “ 2698°55 2698498 | 4 6 0-77 ” 37046°8 2697°3 in + “ 37063 2696-069 0 > rp 37080°2 26943 2694:314 | 1 4 ” ” 371045 2694°1 1 on = 37107 2692°3 2 ds + 37132 2689°5 2 ” ” 37171 2688°352 2 ; ” = 371867 2681:9 a 55 oo 37276 2680:2 1 =: A 37300 : 2679°3 2 “4 =F 37312 26773 2677':232 | 2 5r a 10°9 37341-1 2677:0 1 5 rp 37344 26762 1 iy 3 37356 2674:'8 2674649 | 2 4 ” ” 373772 2673°707 0 nv ”» 37390°3 2672°8 1 ” > 37403 2668°8 2668°748 | In 0 % “ 37459°8 2666°8 1 4 AS 37487 2664:8 2664-723 | 1 2 “ 37516°5 2662°0 1 F Fe 37555 2661-6 1 a ch 37561 2659-60 2659:535 | 6 10r + > 37589°6 2658°8 2658°790 | 1 2 5 3 37600°2 2657'8 1 ms 55 37614 2656°907 0 F 2 ” 37626°8 2653°867 0 @76 | 11:0 37669°8 2651°5 1 4 + 37704 2651-00 2650°938 | 4 4r Ba a 377115 * 2647:00 2646-969 | 4 6r ‘ * a3 37768°0 2645-4 2645°453 | 1 4 = = 37789'7 2639°8 2639°434 | 1 5 a + 37876-0 2639°3 2 es +, 37878 2635°7 2635°372 | 1 0 ” ” 37934°3 26349 2 Ry “5 37941 2631-2 1 =e 111 37994 262813 2628122 | 6 ir ” ” 38038°9 2627°5 2627-484 | 1 4 *9 Ff 38048°2 2625-41 2625°419 | 6 2 Bs 5 38078:0 2623-1 In a " 38112 2621°5 1 a * 38135 2620°9 1 + a 38144 2619°6 2619977 | 2n 0 ” ” 38157°1 2619°668 4 E3 fe 38161°6 261675 2616°839 | 4 0 ” ” 38202°5 2614°701 2 ” ” 882342 2613°8 2613°337 | In 0 a a 38254'1 2613:204 0 ” ” 38256'2 2612°7 1 7 ss 38264 2611°8 1 0, re Wes 38277 2611:2 1 0°75 +9 38286 2608°8 1 * 11:2 38321 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 429 Wave-length Exner and Haschek ba bee Spark 2608:0 2608:333 2607:0 2606°126 2603°5 2603°2 2603:223 26027182 2600-2 2599°986 2599°4 2599°148 2598'2 2595'8 2596081 2595°3 2590°8 2587°890 2585'8 2582°9 2582°415 26794 2578°9 25781 2577:0 2574:7 2574580 2574°2 2572°70 2572°723 2568°4 25661 2564-0 2564-263 2562°5 2560-4 2560°438 2556°9 2555°6 25548 2552°6 2552:2 2552326 2549°4 2549°552 2548:194 2546°986 2546°562 2544-807 2544:0 2544-042 2542°8 2541°3 2541°433 2539°1 2539°285 2538°361 2536-4 2536°581 2536:063 2534-5 2533-0 2531°9 2529°499 2526°0 25244 2523'6 2522°616 2520°6 2520°356 2519-0 2517:273 PLATINUM (SPARK AND ARC SPECTRA)—continued. Intensity and Character Spark | Arc In 0 In 0 a 1 + 0 In 2 1 0 1 2 4 1 1 2 1 1 2 1 1 2 In 1 2 1 4 0 2 1 1 0 1 1 0 1 1 1 1 1 3 In 3 0 0 0 2 1 4 1 il 2 ln 3 0 In 4 2 1 1 1 2 1 In 1 0 1 0 1 1 Previous Observations (Angstrém) Reduction to Vacuum A+ A Oscillation: Frequency in Vacuo 0°75 11:2 38327°5 38347 383599 38399 384028 38418°1 38450°5 384629 38477 38508°4 38520 38587 38630°2 38662 38712°1 38757 38765 38777 38794 38829°8 38836 38858'1 38923 38958 38986:2 39013 390444 39099 39118 39131 39164 39168°5 392112 39232°0 39250°5 39257-2 39284-2 39296°1 39315 39336'4 39369°6 39384-0 39411:7 39419°6 39444 39467 39485 39521°9 39577 39602 39614 396313 39665°3 39687 397140 / Oscillation Frequency in Vacuo 39739°2 39747-9 39763-0 39765°7 39788 39797 39819°4 39851°3 39892-4 39922°3 39939°1 39973'9 40010°9 40020 400332 40053°8 40099 40107 40125 40145°3 40154 40167°9 40193°7 40254:8 40256'9 40290'1 40301 40308 40325 40353'6 40376 40387 40420°7 40441 40456°1 40481°5 405149 40597 40614-2 40635°9 40657 40718 40786°8 40795°5 40879 40896 40918 40925°4 40968°8 40979°4 41025'8 41063°3 41079 43 0 REPORT—1898. PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Intensity Reduction to | and | Previous Vacuum hietand Character Observations Haschek | aS a (Angstrém) AE 1 Spark = Spark} Arc | ate 2515°6 2515666 | 2 3 073 | 116 2515°1 2515119 | 1 3 ” ” 2514°165 | 2 ” ” 2513°98 2513°999 6 0 ” ” 2512°6 1 ” ” 2512:0 1 ” ‘ 2510°604 0 ” 117 2508°5 2508°589 1 3 ” » 2505°9 2506014 | In 4 ” ” 2504128 2 ” ” 2503:°075 2 ” ” 2500°895 0 ” ” 24986 2498°592 2 4 ” * 2498:0 1 ” ? 2497°3 2497-197 In 1 ” ” 2495°95 2495:910 4 4 ” ” 2493-1 1 3) ES 2492-6 1 ” ” 2491°5 il ” ” 2489-7 1 ” ” 2489-00 2488-819 4 4 ” ” 2487:15 2487-216 6 4r ” ” 2483°4 2483°452 1 2 ” | ” 2482-10 2483-312 | 4 2 toe -£ 24813 2481-270 | In | 2 ee be 2480°6 1 sO0G0S 2480°2 oS yo dha te 2479°1 ee uaa a 5: 2477°365 0 53, dee 2476-0 a | wae 2475°3 i | ”» ” 2473°247 0 ” ” 2472:0 In ” ] ” 2470'9 2471092 | In | 83 Pte J 2469°4 2469°537 In 0 0-72 Bi 2467°70 2467504 | 6 | Gr | a 4 2462°5 In | 4 ” 2461'1 2461:474 | 1 / O *5 3 2460°160 1 3 ” 2458:9 In | » | 120 2455°2 | 1 ” ” 2451°0 2451-046 1 | (ated a9 5a 2450°58 2450°527| 4 | 2 4) 5] 2445°5 1 ” ” 24445 In a 4 2443-2 ae et eal 2449-75 4-4] A CHS 244071 2440°158 2) ar ss Netines: 2439-53: ee) | * i. 2436-7 2436-771 | 1 | 4r ys x 2434-62 2434-551 | 4 | O Pome: 2433°6 A . boats Faen 2432-9 | [alt | 41091 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 401 PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Intensity -| and Bee and eae | . Character aschek en Spark Spark | Are 2432-0 1 2429-4 2429186 |; In 2 2428°2 2428-206 | In 8r 2426-7 2426:523 | 1 2 2425-05 2424964 | 6 2 2423°3 rad 2422°6 }+ In 2421-00 2420912 | 4 0 2418°1 2418-151 | 2 | 3 2417-9 aa | 2415-0 thet 2413°3 2413°138 ; In 1 2412-1 In 2410-4 In 2406°7 1 2405°7 In 2405°0 1 2403°180 4r 2403'1 In 2401°959 a 2491°1 2401-089 | 1 1 2400°4 ae 2396°72 2396'762 | 4 0 2396°2 2396:243 | 1 2 2395°6 1 2391°856 | O 2390°8 ag 2389.7 2389°615 ; 1 | 3 2387°4 2387-448 | 1 | O 2386°6 2386886 | In 0 2384-4 In 2383°7 2383'732 | 1 4 2382 0 1 2381-4 1 2380-035 0 2379-0 et 2377°28 (i 2375-7 iim} 2375'1 ee 23748 ta 2373-4 | 2373°0 ie 23717 1 2369°9 1 2368°4 2368°357 il tr 2368°1 1 2366°6 1 2365°5 1 23648 1 2364-0 net 2357-7 | 2357°656 } 1 | O 23572 2357181 | In | 4r 2356-4 2356415 0 1 ) 2353°123 | 0 Previous Observations (Angstriim) Reduction to Vacuum REA) Fo A O72 | 1271 ” ” 3 12°2 ” bb) ” , ”° ” bh) ” 071 a ” ” thd ” ” ” ” ” ” 12:3 ” ” oh ” ” ” ” ” ” » ” ” ” ” ” ” bh) ” a 12°4 ” ” ” ” ” ” 3” ” ” ” ” ” ’ ” 3” bh) ” ” fo 12°5 ” ” »” ” ? ” * ” ” ” ” ” ” ” Lar 07 a ” ” th) » th] ” a 12°6 ” ’ a9. ” ” b>) ? ” 39 29 ” ’ ” ” ” Pe 127 Oscillation Frequency in Vacuo 41106 411539 41170°4 41199°1 41225°6 41254 41266 41294°6 41341°7 41346 41396 41427°6 41445 41475 41538 41556 41568 41599-2 41601 41620°4 41635-4 41647 41710°6 41719°7 41731 4179671 41815 41835°3 41873'3 41883°1 41927 419387 41969 41980 42003°6 42022 42052°4 42080 42091 42096 42121 42128 42151 42183 42210°7 42215 42242 42262 42274 42289 42402°3 42411-0 42424-7 42484°1 432 REPORT—1898. PLATINUM (SPARK AND ARc SPECTRA)—continued. Wave-length Intensity Reduction to oa Previous Veodaay oipceiliation Exner and hae Character Observations Frequency Haschek me is a (aa (Angstrém) “Le in Vacuo Spark Spark | Are 2351°5 1 19°F 42513 2348°6 1 : 42566 2347°239 0 = 42590°5 2346°822 0 42598°2 2343-4 2343°468 1 0 . 42659'1 2342°8 1 5: 42671 2340°2 2340°255 1 2 12°8 427175 2339°5 1 53 42731 2339°1 1 - 42739 2335°2 i a 42810 232674 23267185 In 2 12:9 42975°9 2323°2 1 ‘ 43031 2320°1 In 2 43089 2318'3. 2318°371 1 2 a 43020°9 23154 2315°58 In 2 e 430728 2314'2 1 13:0 43199 2313°7 1 * 43208 2312°9 Jn 55 , 43223 2310°9 2 oh 43260 23081 2308:12 In 3 = 43312°3: 2307'8 1 a 43318 23063 1 e 43347 2305'8 2305°72 1 2 - 433574 2304°6 1 43379 23043 1 > 43384 2302°5. 1 = 43418 22975 1 13:1 43513 22961 2 ss 43539 22937 if * 43585 2292°8 1 Re 43602 2292:0 1 ES 43617 2291:7 1 e 43623 2289°6 1 an 43663 2288-4 4n 13-2 43686 2287°7 2 * 43699 2286'8 1 ne 43716 22859 i a 43733 2285:'3 1 a 43745 2281°6 1 s 43816 2280°9 1 m 43829 2276°4 i He 43917 22746 In | 13:3 43951 2271:9 ipee, - 44003 2270°1 In | 44 44038 2269°1 eer i 44057 22685 1 a 44069 2267°5 1 5, 44088 2266°T In x a 44104 2264:3 In _ 44151 2263°6 1 ” 44164 2263-0 i 13:4 44176 2259°8 1 5 44238 2259:0 1 is 44254 2256°4 In a3 44305 ON WAVE-LENGTH TABLES OF THE SPECTRA OF THE ELEMENTS. 433 PLATINUM (SPARK AND ARC SPECTRA)—continued. Wave-length Intensity | Reduction to a and Previous Vacuum Oscillation Baneriand Character Observations : Frequency Haschek Keer) | (Angstrém) A+ i in Vacuo Spark Are Spark | Arc Na | : 2254°8 1 O68 | 13:4 44336 2253'3 1 ” ” 44366 2251°6 2 a ” 44400 2250'7 1 6 13:5 44417 2247-4 In = “ 44482 2245°6 In Re on 44518 2242°7 in 0°67 5 44576 2235°4 In 3 13:6 44721 2229°1 1 ” ” 44848 2218°4 In “5 13-7 45064 2210-4 ln ~ 13°8 45227 2210°0 1 op a 45235 2205°1 1 ” ” 45336 1 2204-0 1 is 4) 45358 : 2202°0 1 ” 13:9 45399 2192 4 In 066 | 14:0 45598 2190°4 in 3 as 45640 2177-0 1 < c 14:1 45921 2150°4 1 p 14:3 46489 2149°8 1 7 A 46502 2148:9 1 A “4 46521 2144°4 In 065 | 14-4 46619 2130°7 i ” 14°5 46918 Phe 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 Joun Lussock, Sir Paitie Maanus, Sir H. E. Roscog, and Professor 8. P. THompPson. : | | PAGS ' APPENDIX.—Schedule IT.—Elementary Science and Geography 5 : . 438 } Schedule IV.—Elementary Physics and Chemistry : : . 438 Your Committee are able to report that the quantity, if not the quality, _ of the teaching of Science subjects in Elementary Schools has made _ progress during the past year. The following table, made up from the _ return issued by the Education Department, gives the figures for the . scientific class subjects as compared with English. In the report for last _ year it was mentioned that the number of school departments taking _ object lessons would greatly increase, as the Government code of regu- _ lations announced that they would become obligatory in the three lower standards on and after September 1, 1896. We now see the result, so far _ as the schools are concerned whose school year ended between August 31, 1898. FF A34 REPORT—1898. 1896, and August 31, 1897, but the full effect cannot appear until the next year’s return, the whole of which will be within the obligatory period. Class pep este eran 1890-91 | 1891-92 | 1892-93 | 1893-94 | 1894-95 | 1895-96 | 1896-97 English 19,825 | 18,175 | 17,394 | 17,032 6-380 15,327 | 14,286 | Geography . ; . | 12,806 | 13,485 | 14,256 | 15,250 | 15,702 | 16,171 | 16,646 | Elementary Science . 173 788 | 1,073 | 1,215 | 1,712 | 2,237 | 2.617 | Object Lessons . 4 — = = = | — 1,079 | 8,321 The number of departments in ‘schools for older scholars’ for the year 1896-97 was 23,080, all but 10 of which took one or more class subjects. But History was taken in 5,133 departments, and needlework (as a class subject for girls) in 7,397 departments, and sundry minor subjects in 1,056, making, with the other four subjects of the table, a total of 55,456. This shows an average of more than 23 class subjects to each depart- ment; but it must be borne in mind that the same subject is not always taken in all the standards, in which case three class subjects will appear in the return. Tt was remarked in the, last report that ‘the increased teaching of scientific specific subjects in the higher standards is the natural con- sequence of the greater attention paid to natural science in the lower part of the schools.’ The following table shows the correctness of this inference :— 2 | Specitiz Subjects.—Children | 1891-92| 1892-93 | 1893-94 | 1894-95 | 1895-96 | 1896-97 | : Algebra . : : . | 28,542 | 31,487 | 33,612 | 38,237 | 41,846 | 47,225 | | Euclid . ; : : 927 1,279 1,399 1,468 1,584 | 2,059 | | Mensuration . : . | 2,802 3,762 4,018 5,614 6,859 | 8,619 | | Mechanics 4 2 . | 18,000 | 20,023 | 21,532 | 23,806 | 24,956 | 26,110 | Animal Physiology . . | 13,622 | 14,060 | 15,271 | 17,003 | 18,284 | 19,989 | Botany . : : . | 1,845 1,968 2,052 2,483 29968 eis. oi | Principles of Agriculture. | 1,085 909 | 1,231} 1,196] 1,059[ 9825 | Chemistry ; ; - | °1,985 | 2,387 3,043 3,850 4,822 5,545 Sound, Light, and Heat . | 1,163 1,168 1,175 914 937 1.040 Magnetismand Electricity | 2,338 2,181 3,040 3,198 3,168 | 3,431 | Domestic Economy . . | 26,447 | 29,210 | 32,922 | 36,239 | 39,794 | 45,869 | Total - - . | 98,706 | 108,434 | 119,295 | 134,008 | 146,305 | 164,089 | It appears that the mathematical subjects still command the most favour on the part of the teachers, Algebra having taken a very remark- able lead. All the physical sciences have increased even more than might have been expected from the increase of scholars. The Principles” of Agriculture is the only subject that shows an actual decrease. Estimating the number of scholars in Standards V., VI., and VII. at 615,000, the percentage of the number examined in these specific subjects as compared with the number of children qualified to take them, is 266 : but it should be remembered that many of the children take more than one subject for examination. The following table gives the percentage for wy -< ON THE TEACHING OF SCIENCE IN ELEMENTARY SCHOOLS. 4135 _ each year since 1882, and shows that Science is gradually recovering from , the great depression of about eight years ago :— 1882-83 . ~—.-—«:29°0 percent. | 1890-91 . 20:2 per cent. % Mega-84.. 2605 » 5, 1891-02 pi. 197 measee-85 . . 226), DE Ons cae MD us me 1885-86 .. .-199 ,, eee 209 fear. Segts 2:5 Ce ao) aa ote» deameaae 1887-88 . . 169 - ,, 189596 49497 > eeeebG. te LTO) PEIG Og 26S 5 ‘ i . 1889-90 The Returns of the Education Department here given 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, 1898. 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 7 | 1890-91 pia 2,293 4 1891-92 113 26,674 : 1892-93 156 40,208 1893-94 183 49,367 1894-95 208 52,982 1895-96 246 62,494 1896-97 364 86,638 1897-98 322 70,626 The last year shows an apparent falling-off in the teaching of this subject, but, as has been mentioned above, the Government having made _ the giving of object lessons obligatory in the lower standards, 442 Depart- ments, with 75,993 children, have already adopted them. This has caused a reduction in the teaching of ‘Elementary Science’ under that _ name ; but, taking the two subjects together, this must be regarded as a _ very considerable gain. ___ The Education Department continues to meet the objection against the _ limitation under the Code by which only two class subjects are allowed to _ be taught, by adding combined courses of study. This year a new course of this character has been introduced into Schedule II., described as ‘Elementary Science and Geography Combined.’ And as, under the present regulations, one of the class subjects must be such as can be taught by means of object lessons in the lower standards, some such subject as the combined one above mentioned must be taken. A copy of the scheme is _ given in the Appendix, by whichit will be seen that in the lower standards _ the phenomena of the land and water are to be illustrated experimentally _ as an introduction to Geographical Science. : A similar principle has been adopted in respect of the specific subjects. Hitherto Chemistry has formed a course of itself, and Physics has been : divided into two separate courses, the one dealing with Sound, Light, and Heat, and the other with Magnetism and Electricity ;- but they formed only three out of the nineteen subjects from which choice could be made. FF2- 436 REPORT—1898. A separate course of Elementary Physics and Chemistry combined has now been introduced, which is set out in the Appendix, and which is admirably adapted for experimental investigation at the hands of the students themselves. The work under the Evening Continuation Schools Code continues to progress, as will be seen from the following table :— Units for Payment Science Subjects England and Wales London School Board 1893-4 | 1894-5 | 1895-6 | 1896-7 | 1893-4 1894-5| 1895-6 396 -7 Euclid. ; . 595 | 1,086 1,648] 2,270 10 29 7 — Algebra . ; -| 3,940 | 6,657 | 10,374) 14,260} 316 | 302 | 535 | 714 Mensuration . . | 14,521 | 32,931 | 41,772] 50,748] 279 374 452 369 Elementary Physio-| 2,554 | 4,045 6,590) 6,325 37 9 5 — graphy Elementary Physics | 6,500 | 7,850 6,749} 5,183 T9200") Ts24129 and Chemistry Science of Common] 6,223 | 10,350 | 12,906) 18,293} 231 262 | 468 | 556 Things Chemistry ; .| 3,484 | 7,814 8,222} 9,641} 212 | 455 | 404] 488 Mechanics ; j 841 | 1,148 1,458} 2,196) 230] 197 | 209] 127 Sound, Light, and 500 | 1,046 861} 1,156 — 15 11 7 Heat Magnetism and Elec-} 2,359 | 4,451 5,073} 6,990} 662] 776 | 783 | «939 tricity Human Physiology .| 5,695 | 8,395 7,825, 10,047 91 68 56 49 Botany . . : 336 547 905} 1,080 5 91 97 32 Agriculture. .| 8,579 | 4,991 4,694) 4,061 _— = = = Horticulture . ; 458 | 1,140 1,812} 1,911 _— == = a= Navigation : : 42 69 142 99 = = == = Totals ; - | 51,607 | 92,520 | 111,031)134,260 | 2,152 | 2,778 | 3,179 | 3,410 It is again evident that the mathematical subjects are rapidly increas- ing in favour, and that Agriculture is decreasing. It will be noticed with satisfaction that the Science of Common Things is receiving greatly in- creased attention, but it is a matter of regret that there is a decrease in the time given to Elementary Physiography, and still more so in the case of Elementary Physics and Chemistry. Agriculture would become a more valuable and probably a more popular subject of study if a really good practical course were devised. An important change has been taking place in Scotland. The code of the Scotch Education Department now admits of the possibility of gain- ing the full class grant although only two subjects are taken. As one of these must be English, and in the higher standards provision must be made for history or geography, or both, the teaching of science as a class subject has been greatly reduced during the last two years. Buta new article in the Code for 1895 offers a special grant of a shilling on the average attendance of boys who are satisfactorily taught ‘elementary science’ ; and this hasfar more than made up the deficiency. In fact the aggregate total of children learning elementary science in the Scotch schools has risen from 34,151 in 1894-95 to 85,671 and 133,855 respec- tively in the two succeeding years. Your Committee have frequently referred to the anomaly that pupil ee “7 Ee OO Ee ea chi ae - ON THE TEACHING OF SCIENCE IN ELEMENTARY SCHOOLS. 457 teachers are not obliged to receive any instruction in Natural Science, although they may have to give instruction in such subjects, either specifically or in the form of object lessons ; indeed, if they should be in charge of a class of the three lower standards it would be obligatory upon them to give such object lessons. A Departmental Committee, consisting of the Rev. T. W. Sharpe, Her Majesty’s Chief Inspector of Schools, as Chairman, and several Inspectors and Principals of Training Colleges and Pupil-teacher Centres, have reported upon the pupil-teacher system. They recommend that the age for entering as pupil teachers should be raised, and that the interval between the elementary school and their apprentice- ship should be passed at a secondary school. This would by no means ensure that the young people would receive any instruction in Science during that period of their career. No alteration is proposed in the optional Science Course prescribed by the Code of the Education Depart- ment, except that the Queen’s Scholarship examination is to be limited to the elementary stage of Physiography prescribed in the syilabus of the Science and Art Department. With regard to the College Course the recom- mendation is singularly weak, Science being placed as an optional subject, without any definite course of study prescribed. For the first two years it is laid down that of the optional subjects not more than two must be taken out of a list of four or six respectively, some of which from their very nature are almost sure to be taken in preference. An important letter has been addressed to the Right Hon. Sir John Gorst by Sir Philip Magnus, the Chairman of the Joint Scholarship Board, in conjunction with the Chairmen of its four educational committees. They point out the necessity of securing the proper training of those who will be teachers of scientific subjects, and that the instruction of pupil- teachers in science is now often carried on, under great pressure, by a system of cram, and even by persons who have not themselves any satis- factory knowledge of medern scientific methods. They suggest as a remedy that the first part only of the elementary stage, Physiography, be compulsory ; that the teaching of this subject be recognized only where it is given with proper accessories, all pupils performing the experiments in a series of at least twenty-four lessons of two hours’ duration; and that inspectors should be required particularly to report whether proper apparatus and accessories are provided. In last year’s report your Committee referred to what Mr. Heller was doing in respect of the teaching of Science in the schools of the London School Board. He has since obtained a better appointment at Birming- ham, but the syllabus of lessons which he prepared is still employed in the schools. This of course requires that the masters and mistresses should be qualified for carrying it out, and for this purpose classes of twenty-four hours are conducted for their benefit by the Science Demonstrators. These gentlemen have lately agreed upon two separate syllabuses for masters and mistresses, which follow in general the scheme they are expected to teach to their scholars. The classes of a similar kind that have been carried on hitherto have been appreciated by the teachers, and the Board are increasing their laboratory and other accommodation for the purpose. It is recognised that it will be necessary to continue these teachers’ courses for some years, in order to overcome the difficulty which now exists in consequence of the general want of practical experiment in such instruction in Science as has been given in the course of training of most class teachers, 438 REPORT—1898. APPENDIX. Schedule 1I1.—Course D. ‘ Elementary Science and Geography combined.’ Standards I., II., and I1I.—Annual courses of about thirty object lessons, of which elementary geography should form a part, beginning with the simplest phenomena which the children can observe :—land, water, the form of the earth, the sea, hills, valleys, rivers, proceeding to notions of locality and distance, and the means of representing all of these by modelling in sand or other material, and by a map, with special reference to the map of England. The other object lessons should include some of the various subjects suggested in this Schedule under the head of Elementary Science. ” Standard IV. —Geography of England, physical and political. Lessons on animals and on materials used in agriculture, or in some simple manufactures. Standard V.—Geography of the British Isles, with some knowledge of India, and one or more of the Colonies. Lessons on means of locomotion, and on processes used in agriculture or manufacture. Standard V1i.—Geography of Europe, physical, political, and com- mercial. Lessons on the physical laws that determine climate, animal] life, locality of certain industries, &c. Standard VII.—The work of the preceding years, with special know- ledge of the British Empire, and of those portions of the world with which we are engaged in commerce. Distribution of the races of mankind. Schedule 1V.—Specific Subjects. (13.) ‘ Liementary Physics and Chemistry.’ 1st Stage.—Properties of common stuffs ; relative density of solids and liquids ; flotation of solids. The barometer and thermometer ; their use ; graphic representation of daily readings. Solution: water as a solvent ; solubility of metals, &c. in acids ; crystallisation of salt, soda, alum. 2nd Stage.—Evaporation and distillation ; heat absorbed in fusion of ice and in conversion of water into steam ; density of ice ; change in den- sity of water on heating ; moisture in air ; wet and dry bulb thermometer. Study of iron rusting, and of combustion of candle, gas, oil, phosphorus ; effect on metals of heating in air ; discovery of active constituent of air. 3rd Stage.—Chalk and lime ; the burning of chalk or limestone ; action of muriatic acid on chalk or limestone ; carbonic acid ; reformation of chalk. Discovery of carbonic acid in air ; its formation by combustion of carbonaceous materials and in respiration. Study of action of muriatic and vitriolic acids on zinc ; combustion of the gas obtained, and discovery of the composition of water. Presence of air and solids dissolved in water ; sea water ; hardness of water. ee ee ee Sa ee Toe a ON THE BIBLIOGRAPHY OF SPECTROSCOPY. ‘439 Bibliography of Spectroscopy.—eport of the Committee, consisting of Professor H. McLeop, Professor W. C. Roserts-AusTEN, Mr. H. G. Manan, and Mr. D. H. NaGEt. Tue collection and verification of titles of papers on spectroscopy is being continued, and a list is appended which brings the catalogue of spectro- scopic literature up to the end of 1897. It is proposed to continue the work of the Committee up to the end of the year 1899, after which date the commencement of the International Catalogue of Scientific Papers will render further procedure on the part of the British Association unnecessary. The Committee are strongly of opinion that it is most desirable that the separate instalments of the catalogue published at’various dates in the Reports of the Association should be (at the conclusion of the work) collected, arranged as one continuous list of papers, and reprinted as a whole. This would appear to be the only way of obtaining the full value of the catalogue as a work of reference for those engaged on the subject of spectroscopy. One of the members of the Committee is quite willing to - undertake the whole work of rearrangement of the matter and passing it through the press. The only question is the expense of printing, which will be certainly not less than 1207. Some of this might be met by grants from the Association and from other scientific societies which possess libraries ; and, to avoid actual loss, a charge might be made for each copy of the catalogue. The matter need not be settled until next year, but in the meantime the Committee hope that it will have the earnest consideration of the Association. The Committee therefore ask to be reappointed. PAPERS ON SUBJECTS CONNECTED WITH SPECTROSCOPY. Continuation of the List published in the Report for 1894. {Im cases where it has not been found possible to verify a reference, the latter is placed in brackets, in the same column as the title of the paper. A list of the chief abbreviations used will be found at the end of the catalogue. ] us INSTRUMENTAL. 1892. J.S.Ames , . | The Modern Spectroscope. I. The | ‘ Astron. and Astrophys.’ Concave Grating in Theory and | xi. 28-42. Practice. (Feb.) J. EH. Keeler . . | The Modern Spectroscope. II. The | ‘ Astron. and Astrophys.’ Star Spectroscope of the Lick | xi. 140-144. Observatory. (Keb.) H.C. Pickering .| The Modern Spectroscope. III. | ‘Astron. and Astrophys.’ The Objective Prism. (March.) xi. 199-203. 440 C. A. Young . H. Deslandres W. Grosse . J. E. Keeler , G.E.Hale , - L. Becker . W. Huggins . H. F. Newall. L. E. Jewell , ' M. T. Edelmann A. E. Tutton . N. von Konkoly C. Féry . . F. L. O. Wads- worth. REPORT—1898. INSTRUMENTAL, 1892, 1893, 1894. The Modern Spectroscope. IV. The New Spectroscope of the Halsted Observatory. (April.) Spectrograph zur Messung von Sternbewegungen. (Dec.) Spectrophotograph der Pariser Sternwarte. (Dec.) 1893. The Modern Spectroscope. VI. The Spectroscope of the Alle- ghany Observatory. (Jan.) The Spectroheliograph. (Feb.) The Modern Spectroscope. VII. The Spectroscope of the Royal Observatory, Edinburgh. (June.) The Modern Spectroscope. VIII. The Tulse Hill Spectroscope. (Sept.) On a Combination of Prisms for a Stellar Spectroscope. (Read Nov. 13.) 1894. The Object-glass Grating. (Jan.) . Hisendrahtbolometer zur Unter- suchung vom Wiarmespectrum. (Feb.) An Instrument of Precision for obtaining Monochromatic Light of any desired Wave-length; and its use in investigating the Optical Characters of Crystals. (Read Feb. 1.) Ein solides lichtstarkes Sternspec- troscop. (Mar.) Réfractométre 4 cuve chauffable. Application 4 la mesure des corps gras. (Read July 30.) A New Arrangement for Large Spec- troscope Slits, (July.) An Improved Form of Littrow Spec- troscope. (July.) ‘Astron. and Astrophys.’ xi. 292-296. *Naturwiss. Rundschau,” vii. 676; ‘ Beiblitter,’ xvii, 448-449 (Abs.) ‘Naturwiss. Rundschau,” vii. 676 (Abs.) ‘Astron. and Astrophys.” xii, 40-50. ‘Astron. and Astrophys;’ xii. 241 — 257; ‘ Bei- platter,’ xviii. 89 — 90. (Abs.) ‘Astron. and Astrophys.” xii. 542-545, ‘Astron. and Astrophys.” xii. 615-619. ‘Proc. Phil. Soc. Gamb,’ viii. 138 — 141; ‘ Zeitschyr.. f. Instrumentenkunde,’ xiv. 369 -— 370; ‘ Bei- blatter,’ xix. 323 (Abs.); ‘Nature,’ xlix. 379(Abs.), ‘Astron. and Astrophys. xiii, 44-48; ‘Nature,” xlix. 300-301 (Abs.) ‘Electrotech. Zeitschr.” xv. 81-82; ‘ Beiblitter, xviii. 749-750 (Abs.) ‘Proc. Roy. Soc.’ lv. 111- 113 (Abs.); ‘ Beiblat- ter,’ xviii. 835 (Abs.) ‘Centralzeit. f. Opt. u- Mech.’ xv. 61-64. °C. R. cxix. 332-334: ‘ Beiblaitter, xix. 168 (Abs.) ‘Amer. J. Sci.’ [3], xlviii. 19 — 20; ‘ Beibliitter,’ xviii. 996-997 (Abs.) ; ‘ Nature,’ 1. 326 (Abs.) ‘Phil. Mag.’ [5], xxxviii. 137-142; ‘ Beibliitter,’ xix. 59 (Abs.) oe ee a SSS eee ON THE BIBLIOGRAPHY OF SPECTROSCOPY. C. Féry.. M. Gliiser L. Mach E, L. Nichols . J. Scheiner H. Crewe and R. Tatnall. C, Pulfrich A. Konig, N. von Konkoly F, Miiller ‘F. L. O. Wads- worth. INSTRUMENTAL, 1894, Application de l’autocollimation a la mesure des indices de réfrac- tion. (Read Aug. 15.) Die Umkehrung der Natriumlinie. (Aug.) Ueber meter. ein Interferenzrefracto- (Aug.) A New Form of meter. (Sept.) Spectrophoto- Ueber structionen, neuere — Spectroscopcon- (Sept.) On a Method of Mapping the Spec- tra of Metals. (Oct.) Ueber eine neue Spectroscopcon- struction. (Oct.) Ein neuer Spectroscopspalt mit Doppelbewegung. (Oct.) A Spectroscope with Fixed Arms. (Oct.) Kin neues (Nov.) Spectrophotometer. Ein neues photographisches Spec- troscop. (Nov.) Zur Absorption des Natriumlichts durch Natriumdampf. (Dec.) The Modern Spectroscope. IX. Fixed-arm Spectroscopes. (Dec.) AAY °C. BR.’ cxix. 402 - 404; ‘ Beiblatter, xix. 168 (Abs. ) ‘ Zeitschr. f. phys. u. chem.. Unterr.’ vi. 303; ‘ Bei- blatter,’ xviii. 561 (Abs.) ‘Zeitschr. f. Instrumen- tenkunde,’ xiv. 279-283; ‘Proc. Phys. Soc.’ xiii. 61 (Abs.) ‘Phys. Review,’ ii. 138- 14L; ‘Beiblitter, xix, 241-242 (Abs.) ‘Zeitschr. f. Instrumen- tenkunde,’ xiv. 316-324 ; ‘Beiblatter, xviii. 1045. (Abs.) ; ‘ Proc. Phys. Soc.” xiii. 60 (Abs.) ‘Phil. Mag.’ [5], xxxviii. 379-386; ‘ Beiblitter,” xix. 783 (Abs.) ‘Zeitschr. f. Instrumen- tenkunde,’ xiv. 354-363 ; ‘Proc. Phys. Soe.’ xiii. 60 (Abs.); ‘Zeitsehr. f. anal. Chem.’ xxxiv. 744 (Abs.) ; ‘ Beiblitter,’ xix. 328-329 (Abs.) ; ‘Astrophys. J."1.. 335-349. ‘Zeitschr. f. Instrumen- tenkunde,’ xiv. 364-366 ; ‘ Proc. Phys. Soc.’ xiii. 6 (Abs.) ‘Phil. Mag.’ [51, xxxviii. 357-351 ; * Beiblitter,” xix. 782-783 (Abs.) ‘Ann. Phys. u. Chem’ [N.F.], liii. 786-792; ‘Nature, li. 334 (Abs.) ;. ‘Proc. Phys. Soc.’ xiii. 64 (Abs.) ‘Centralzeit. f. Opt. u.. Mech.’ xv. 73-74; ‘ Bei- blatter,’ xviii. 997 (title). ‘ Zeitschr. f. phys. u. chem. Unterr.’ viii. 95-96 ; ‘ Bei-- blatter,’ xix. 625 (Abs.) ‘ Astron. and Astrophys.” xiii. 835-819; ‘Nature,’ li. 325 (Abs.) AA2 A. H. Borgesius E. L. Nichols. Fr. L. O. Wads- worth, J. EH. Keeler . Be Ly. "0: worth. Wads- De Thierry . hal ° - K, Angstrém . W.Crockes . 4 A. Belopolsky . W. Huggins . W. Hallwachs J. Young and G. R. Darling, C. V. Zenger . REPORT—1898, INSTRUMENTAL, 1895, Beschreibung eines Interferenzre- fractometers. Molecularrefraction und Dispersion einiger Salze in Lésungen. (Jan.) A Method for the Study of Trans- mission Spectra in the Ultra- Violet. (Jan.) The Modern Spectroscope. X. General Considerations respecting the Design of Astronomical Spec- troscopes. (Jan.) On a Lens for Adapting a Visually- corrected Refracting Telescope to Photographic Observations with the Spectroscope. (Feb.) The Modern Spectroscope. XI. Some New Designs of Combined Grating and Prismatic Spectro- scopes of the Fixed-arm Type ; and a New Form of Objective Prism. (Mar.) Sur un nouvel appareil dit ‘héma- spectroscope-comparateur.’ (Read April 8.) Ueber eine einfache Methode zur photographischen Darstellung des infraroten Spectrums. (Read April 10.) (K. Gesellsch. Wiss. Upsala.) The Slit of a Spectroscope. (April.) On the Spectrographic Perform- ance of the Thirty-inch Pulkowa Refractor. (May.) The Modern &pectroscope. XII. "he Tulse Hill Ultra-Violet Spec- troscope. (May.) Bemerkungen zu einer Arbeit des Hrn. Borgesius iiber ein Inter- ferenzrefractometer. (June.) A Method of Transferring Gases to Vacuum Tubes for Spectroscopic Examination. (July.) L’éclipsoscope, appareil pour voir la chromosphére et les protubé- rances solaires. (Read Sept. 2.) ‘Verslagen en Mededer- lingen d. K. Akad. Am- sterdam,’ 1894, 1895, 99- 103; ‘ Ann.Phys. u. Chem.’ [N.F.], liv.221-243 ; ©Bei- blitter,’ xix. 168-169 (Abs.);— ‘Proc. Phys. Soc.’ xiii. 217-218 (Abs.) ‘Phys. Review,’ ii. 302- 304; ‘ Beibliatter,’ xix. 426 (Abs.) ; ‘Proc. Phys. Soc.’ xiii. 169 (Abs.) ‘ Astrophys. J.’ i. 52-79. ‘ Astrophys. J.’i. 101-111 ; ‘ Beiblitter,’ xx. 25 (Abs.) ‘ Astrophys. J.’ i. 232-260; ‘ Beibliitter,” xx. 196 (Abs.) oC. Shc (CX mp Wie ‘Zeitschr. f. anal. Chem.’ xxxiv. 744 (Abs.); ‘Chem. News,’ xxi. 209 (Abs.) ‘J. de Phys.’ (3], v. 32 (Abs.); ‘Phys. Rey.’ iii. 137-141; ‘ Beiblitter,’ xx. 196-197 (Abs.); ‘Proc. Phys. Soc.’ xiv. 125 (Abs.) ‘Chem. News,’ Ixxi. 175; ‘Zeitschr. f. Instrumen- tenkunde,’ xv.302 (Abs.) ; ‘Beiblitter,’ xix. 782 (Abs.) ‘ Astrophys, J.’ i. 366-371 ; ‘ Beiblatter,’ xx. 25 (Abs.) ‘Astrophys. J.’ i. 359-365. ‘Ann. Phys. u. Chem, [N.F.], lv. 282-287. ‘Chem. News,’ Ixxii. 39; ‘J. Chem. Soc.’ Ixx. II. 3 (Abs.) *C. R’ cxxi. 406-408; ‘ Nature,’ lili. 424 (Abs.) ee KH. Spée . . R. Neumann. C. Pulfrich , FF. L. O. Wads- worth. A. Belopolsky . H, Deslandres H. Haga ° : B. Kolbe F. L. O. Wads- worth. A. Belopolsky A. H. Bruére C, Pulfrich . THE BIBLIOGRAPHY OF SPECTROSCOPY. INSTRUMENTAL, 1895, 1896. Projet d’une spectroscope réali- sant le phénoméne d'une éclipse totale du soleil. (Read Oct. 12.) (Oct.) Schulapparat fiir Brechung und Zuriickverfiigung des _ Lichtes. (Oct.) Hin neues Refractometer. Univer- salapparat fiir refractometrische und spectrometrische Untersnch- ungen. (Nov.) The Modern Spectroscope. XIII. A New Multiple Transmission Spectroscope of great Resolving Power. (Noy.) The Modern Spectroscope. XIV. Fixed-arm Concave Grating Spec- troscopes. (Dec.) Expériment basé sur le principe Doppler-Fizeau. 1896. Méthode pour étudier les varia- tions de vitesse radiale des astres avec defaiblesinstruments. (Jan.) Hine Aufstellungsweise des Row- land’schen Concaygitters. (Jan.) Ein handliches Lichtbrechungs- apparat. (Jan.) The Modern Spectroscope. XV. On the Use and Mounting of the Concave Grating as an Analysing or Direct Comparison Spectroscope. (Jan.) On the Performance of an Auxi- liary Lens for Spectrographic In- vestigations with the 30-inch Refractor of the Pulkowa Obser- vatory. (Feb.) A Comparison of Two Concave Rowland Gratings. (Feb.) Appareil universel pour les mesures de réfraction et de dispersion (Feb.) AAS ‘Bull. Acad. Belg.’ xxx. 274-276; ‘Nature,’ liii. 309 (Abs.); ‘ Beibliitter,’ xxi. 513 (Abs.) ‘ Zeitschr. f. phys. u. chem. Unterr.’ viii. 357-358; ‘Beiblatter, xx. 363 (Abs.) ‘ Zeitschr. f. Instrumen- tenkunde,’ xv. 383-394; ‘Zeitschr. f, physikal. Chem.’ xviii. 294-299; ‘J. Chem. Soc.’ Ixx. II. 161 (Abs.) ‘Proc. Phys. Soc.’ xiv. 6-7 (Abs.); ‘Beiblitter, xx. 191-192 (Abs.) ‘ Astrophys. J.’ ii. 265-282. ‘Astrophys. J.’ il. 3570- 382. ‘Mem. spettr. ital’ xxiii. 123-124; ‘Nature,’ lii. 515 (Abs.) * Astr. Nachr.’ cxxxix. 241- 244; ‘Beiblitter,’ xxi. 343-344 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], lvii. 389-393; ‘Proc. Phys. Soc.’ xiv. 123-124 (Abs.) ‘Zeitschr. f. phys. u. chem. Unterr.’ ix, 20-24. ‘ Astrophys. J.’ lil. 47-62 ; ‘Beiblitter, xxi. 334 (Abs.) ‘Astrophys. J.’ iii. 147- 149; ‘Beibliatter,’ xxi. 334 (Abs.) ‘Phys. Review,’ iii. 301-— 305; ‘Proc. Phys. Soc.’ xiv. (Abs.), 123; ‘Bei- blitter,’ xx. 653 (Abs.) ‘J. de Phys. [3], v. 73-79. Add F. L. O. Wads- worth. H. F. Newall : C. Pulfrich . . H. F. Newall. ” ® FF. L. O. Wads- worth. ESO. “hord 4 G. E. Hale and F. L. O. Wads- worth. F. L. O, Wads- worth. W. Huggins . F. Walleraut . M. Berthelot . G.E.Hale . f REPORT—1898. INSTRUMENTAL, 1896, 1897. The Modern Spectroscope. XVI. A Simple Optical Device for com- pletely Isolating or Cutting-out any desired Portion of the Ditfrac- tion Spectrum, and some further Notes on Astronomical Spectro- scopes. (March.) The Modern Spectroscope. XVII. Description of a Spectroscope (the Bruce Spectroscope) recently con- structed for use in connection with the 25-inch Refractor of the Cam- bridge Observatory. (April.) A New Form of Refractometer. (April.) ; On the Spectroscope used in con- nection with the 25-inch Refrac- tor. (Read May 25.) A Suggestion for a Form of Spectro- heliograph. (Read May 25.) The Modern Spectroscope. XVIII. On the Conditions of Maximum Efficiency in the Use of the Spec- trograph. (May.) The Spectroscope of the Emerson- McMillin Observatory. (June.) The Modern Spectroscope. XIX. The Objective Spectroscope. (June. ) The Modern Spectroscope. XX. On a New Form of Fluid Prism without Solid Walls, and its Use in an Objective Spectroscope. (Noyv.) 1897. On an Automatic Arrangement for | giving Breadth to Stellar Spectra on a Photographic Plate. (Jan.) Sur un appareil permettant de mesurer les indices de réfraction des minéraux des roches. (Read Feb. 8.) Nouvel appareil pour l’application de l’analyse spectrale a la recon- naissance des gaz. (Read Mar. 15.) Note on a Form of Spectrohelio- graph suggested by Mr. H. F. Newall. (March.) ‘Astrophys. J.’ iii. 192; ‘Beiblitter,’ 334-335 (Abs.) 169- Xxi. ‘Monthly Not. R. A. 8.’ lvi. 98-110; ‘Astrophys. J.’ iii. 266-281. ‘Astrophys. J.’ iii, 259- 266. ‘Proc. Phil. Soc. Camb.’ ix. 179 (Abs.) ‘Proc, Phil. ix. 179-183: ‘Astrophys. J.’ iii. 321- 347; ‘ Beiblitter,’ xxi, 335 (Abs.) Soc. Camb.’ ‘ Astrophys. J.’ iv. 50-53. ‘Astrophys. J.’ iv. 54-78; ‘Beiblatter,’ xxi. 335-— 336 (Abs.); ‘Nature,’ liv. 256 (Abs.) ‘Astrophys. J.’ iv. 274- 277; ‘Nature,’ lv. 110- 111 (Abs.); ‘ Beibliatter,” Xxi. 862 (Abs.) ‘Astrophys. J.’ v. 8-10; ‘Beiblitter” xxi. 521 (Abs.) 'C., Ri ‘exxive polo-slie ‘Chem. Centr.’ 1879, I. 663-664 (Abs.); ‘Bei- bliitter, xxi. 509 (Abs.) °C. R, ecxxiv. 525-5283 ‘Chem. Centr.’ 1897, I. 940 (Abs.); ‘ Nature,” ly. 503 (Abs.); ‘Chem. News,’ Ixxv. 179 (Abs.); ‘J. Chem. Soc.’ Ixxii. 298 (Abs.); ‘Ann. Chim. et Phys.’ [7], xi. 43-473 © Beiblatter, xxi. 514 (Abs.) ‘Astrophys, J.’ v. 21h- 213. NE ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 445 INSTRUMENTAL, 1897—EMISSION SPECTRA 1885, 1891. M. Hamy ©. Leiss . e S. F. Burford F. Dupont . C. Leiss . ° P. Fuchs ' W. Hallwachs J. Nulander . S. P. Langley J. M. Eder W. N. Hartley 0. Neovius Nouvelle lampe 4 cadmium pour la production des franges d’interfé- rence, 4 grande différence de marche. (Read April 5.) Die neuerere Spectrometermodelle der R. Fuess’schen Werkstitte in Steglitz bei Berlin. (April.) The Oleorefractometer. (May) Lumiére jaune pour polarimétre. (June.) Ueber neuere spectrophotograph- ische Apparate. (Nov.) Ueber electrische Entladungsréh- ren zur wissenschaftlichen Spec- tralanalyse und deren Herstellung (‘ Zeitschr. f, Glasinstr.-Industrie,’ vi. 174-177, vii. 4-6). Differentialspectrometer _(‘ Verh. Ges. Naturforsch. Frankfurt, 1897, p. 54). Sur un spectro-photométre construit pour distinguer directement les raies telluriques dans le spectre solaire. (‘Ofvers. af Finska Vet. Societat Férhandl.’ xxxix., 9 pp.) ine EMISSION SPECTRA. 1885. Observations on Invisible Heat Spectra, and on the Recognition of hitherto unmeasured Waye-lengths. (Aug.) 1891. Neue Banden und Linien im Emis- sionspectrum der Ammoniak- oxygenflamme. (Read Mar. 5.) On the Physical Characters of the Lines in the Spark Spectra of the Elements. (Read April 16.) Om skiljandet af knivets och Syrets linien i Luftens Emission-spek- trum. (Read Oct. 14.) ‘C. BR.’ exxiv. 749-752: ‘Chem. News,’ Ixxy. 202 (Abs.) ‘Mechaniker,’ v. 113-115. ‘J. Soc. Chem. Ind.’ xvi. 411; ‘Chem. Centr.’ 1897, II. 232 (Abs.) ‘Bull. Soc. Chim.’ [3], xvii. 584; ‘ Beiblitter,’ xxi. 985 (Abs.) ‘Zeitschr. f. Instrumen- tenkunde,’ xvii. 321~— 334, 357-371; ‘ Beiblit- ter,’ xxii. 221-222 (Abs.) ‘Beiblatter,’ xxii. 218 (titles). *Beiblitter,’ xxi. 730-73] (Abs.) ‘Beiblatter,’ xxii. [24] (title). ‘Amer. Assoc. Rep.’ 1885, 55-75; ‘Phil. Mag.’ [5], xxl. 394-409. ‘Wien. Anz.’ xxviii. 44-47; ‘ Beiblatter,’ xvii. 204-206 (Abs.) “Proc. Roy. Soc.’ xix. 448-451; ‘Astron. and Astrophys.’ 1892, 223- 228. ‘Bihang. till. K. Svensk. Vet. Akad. Handl.’ xvii. Afd. I. No. 8, 69 pp.; ‘ Beibliitter,’ xvii. 563— 564 (Abs.) : AAG E. Pringsheim W. L. Dudley H. Kayser . . B. W. Snow . J.M. Eder . V. Schumann ‘ W. N. Hartley : J. M. Eder and E. Valenta. J.S. Ames J. M. Eder and E. Valenta. | | | | . | Ueber das REPORT—-1898. EMISSION SPECTRA, 1892, 1893. Das Kirchhoff’sche Gesetz und die Strahlung der Gase, I. Die Strah- lung des Natriums, (Jan.) The Colours and Absorption Spectra of thin Metallic Films and of In- candescent Vapours of the Metals, with some Observations on Elec- trical Volatility. (March.) Ueber die Linienspectren Ger Ele- menten der ersten und zweiten Gruppe des Mendeléef’schen Sys- tems. (April.) : Ueber das ultrarothe Emission- spectrum der Alkalien. (June.) Beitrige zur Spectralanalyse. I. Ueber das Emisgjgnspectrum der Ammoniakoxygenflamme. II. Ueber die Verwendbarkeit des Funkenspectrums verschiedener Metalle zur Bestimmung der Wel- lenlange im Ultraviolette. (Read Nov. 3.) Ueber eine neue ultraviolett-emp- findliche Platte, und die Photo- graphie der Lichtstrahlen kleinster Wellenlangen. (Read Nov. 10.) Methods of observing the Spectra of easily Volatile Metals and their Salts, and of Separating their Spec- tra from those of the Alkaline Earths. (Read Dec. 1.) Ueber einige neue Linien im brech- barsten ultravioletten Emission- spectrum des metailischen Cal- ciums. (Read Dec. 1.) 1895. - | On the Probable Spectrum of Sul- phur. (Jan.) ' Ueber das Emissionspectrum der elementaren Silicium, und den spectrographischen Nachweis dieses Elementes. (Read Jan. 19.) Linienspectrum des elementaren Kohlenstoffes in Inductionsfunken, und iiber das ultraviolette Funkenspectrum nasser und trockener Holzkohle. (Read Jan. 19.) ‘Ann. Phys. u.. Chem.’ [N.F.], xlv. 428-459. ‘Amer. Chem. J.’ xiv. 185— 190; ‘J. Chem. Soc.’ Ixii. 1037 (Abs.); ‘ Ber.’ xxvi. (Ref.), 387-38 (Abs.); ‘Zeitschr. anal. Chem.’ xxii. 573 (Abs.) ‘Chem. Zeitung.’ xvi. 533- 534, : ‘Ann. Phys. u. Chem.’ [N.F.], xlvii. 208-251; ‘J. Chem. Soc.’ lxiv. II. 58 (Abs.) ‘Denkschr. Akad. Wien,’ lx. 1-24; ‘ Beiblitter,’ xviii. 910-912 (Abs.) ‘Wien, Anz.’ xxix. 230_ 231; ‘Naturw. Rund- schau,’ ix. 16 (Abs.); ‘ Nature, xlix. 254 (Abs.) ‘J. Chem. Soc.’ lxiii. 138- 141; ‘Chem. News,’ lxvi. 313 (Abs.) ‘Wien. Anz.’ DARBY Xxix, @252- ‘Astron. and Astrophys.’ xii. 50-51; ‘Chem. News,’ Ixvii. 40; ‘Ber.’ xxvi. (Ref.) 366 (Abs.) ‘Wien. Anz.’ xxx. (1893), 19-217 ‘Wien. Anz.’ xxx. (1893), 21-94, - so = F.Paschen , ON THE BIBLIOGRAPHY OF SPECTROSCOPY. J. M. Eder and E. Valenta. J. Parry. . KE. C. C. Baly. . VY. Schumann J. M. Eder and E. Valenta. B. Hasselberg : E. Pringsheim ss. H. Wilde . J. M. Eder and E. Valenta, B.M. Snow . H. C. Vogel H. Kayser and C. Runge. EMISSION SPECTRA, 1893, Ueber das Emissionspectrum des Koblenstoffes und _ Silicium. (Read Jan, 19.) The Spectrum of Iron and the Periodic Law. (Jan.) Separationand Striation of Rarefied Gases under the Influence of the Electric Discharge. (Read Feb. 10.) The Hydrogen Line, Hg, in the Spectrum of Nova Aurigz and in the Spectrum of Vacuum Tubes. (Feb.) Ueber das ultraviolette Linien- spectrum des elementaren Bor. (Read April 13.) Note on the Spectroscopy of Sul- phur. (April.), Das Kirchhofi’sche Gesetz, und die Strahlung der Gase. II. Die Strahlung von Lithium, Thallium und Kalium. (April.) The Spectrum of Thallium, and its Relation to the Homologous Spectra of Indium and Gallium. (Read April 20.) Ueber den Verlauf der Bunsen’- schen Flammenreactionen im ultravioletten Spectrum. (Read July 9.) On the Continuous Spectrum of Sodium. (Amer. Assoc. Report.) (Aug.) On the Continuous Spectrum of the Alkalies [Sodium]. (Aug.) The Infra-red Spectra of the Alkali Metals. (Nov.) Ueber die Bezeichnung der Linien des I. (Noy.) Ueber die Spectren der Elemente. VII. Blei, Arsen, Antimon, Wismuth. (Read Dec. 7.) Ueber die Emission der (Dec.) Gase. Wasserstoffspectrums. | Die Spectren von Zinn, | 447 *Denkschr. Akad. Wien, Ix. 241-268 ; ‘ Beibliitter,” XVill. 753-756 (Abs.) ‘Nature, xlv. 253-255; ‘ Beiblatter, xvii. 748-749 (Abs.) ‘Proc. Phys. Soc.’ xii. 147— 153; ‘Chem. News,’ Ixvii. 95 (Abs.) ‘Astron. and Astrophys.’ xii. 159-166; ‘ Nature,’ xlvii, 425 (Abs.) ‘Denkschr. Akad. Wien,’ lx. 307-311; ‘ Beibliitter, Xvili, 752-753 (Abs.) ‘Astron. and Astrophys.’ xii. 347-349; * Bei- blatter,’ xviii. 86 (Abs.) ‘Ann. Phys. u. Chem,’ [N.F.], xlix. 347-365. ‘Proc. Roy. Soc.’ lili. 369- 372; ‘ Ber. xxviii. (Ref.), 218 (Abs.) ‘Denkschr, Akad. Wien,’ (1893), lx. 467_476 ; « Bei- blatter,’ xviii. 909-910 (Abs.) ‘Phys. Review, i. 296_298 : ‘ Beiblitter, xviii, 997 (Abs.) ‘Proc. Amer. Assoc.’ 1893, 79-80 (Abs.) ‘Phys. Review,’ i. 221-223. ‘Astr. Nachr?’ exxxiy. 95- 96; ‘Nature,’ xlix. 162: ‘ Beibliitter,’ xviii. 670 (Abs.) ‘Abhandl. Akad. Berlin, 1893, 21 pp.; ‘Ann. Phys. u. Chem.’ [N.F.], lii. 93— 113; ‘Nature,’ xlix. 509 (Abs.) ‘Ann. Phys. u. Chem. [N.F.], li. 1-39; ‘Nature,’ xlix. 376 (Abs.); ‘ Phil. Mag.’ [5], xzxvi. 551-552 (Abs.); ‘Proc. Phys. Soc.’ xiii. 13 (Abs.) 448 M.Eisig . E. Pringsheim W. N. Hartley H. Kayser and C. Runge. H. Kayser and C, Runge. J. I. Rydberg ©, Kirn . . TH. P. Lewis and E. 5. Ferry. ©. A. Mebius . #. Paschen J. M. Eder and E. Valenta. W.N. Hartley REPORT—1898. EMISSION SPECTRA, 1894. Das Linienspectrum des Sauer- stoffes. (March.) Bemerkungen zu Hrn. Paschen’s Abhandlung ‘ Ueber die Emission erhitzten Gase.’ (March.) On Variations observed in the Spectrum of Carbon Electrodes, and on the Influence of one Sub- stance on the Spectrum’‘of another. (Received Jan. 13. Read April 19.) Beitriige zur Kenntniss der Linien- spectra. (April.) Ueber die Spectra von Zinn, Blei, Arsen, Antimon, Wismuth. (April.) Beitrige zur Kenntniss der Linien- spectren. (April.) Ueber die Aehnlichkeit der Licht- emission einer nachleuchtenden Geissler’schen Réhre mit dem Beginne des Gliihens fester Korper. (May.) The Infra-red Spectrum of the Metals. (May.) Ueber die Glimmentladung in der Luft. (Read May 9.) Ueber die Emission der Gase. (May.) Ueber das Spectrum des Kaliums, Natriums und Cadmiums bei verschiedenen Temperaturen. (Read June 7.) Flame Spectra at High Tempera- tures. Part II. The Spectrum of Metallic Manganese, of Alloys of Manganese, and of Compounds containing that Element. (Read June 14.) ’ ‘Ann. Phys. u. Chem. (N.F.], li. | 747-760; ‘J. Chem. Soc.’ lxvi. II. 265-266 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], li. 441-447; ‘Nature,’ xlix. 547 (Abs.); ‘Proc. Phys. Soe.’ xiii. 25 (Abs.) ‘Proc. Roy. Soc.’ lv. 344— 349; *Nature.’]. 141-142 (Abs.); ‘J. Chem. Soc.’ Ixvili. II. 432 (Abs.); ‘ Beiblatter,’ xviii. 1046 - 1047 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], li. 114-118. ‘Ann. Phys. u. Chem.’ [N.F.], lif, 93-118; ‘J. Chem. Soc.’ Ixvi. II. 303- 304 (Abs.); ‘ Nature,’ 1. 118 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], lii. 119-131. ‘Ann. Phys. u. Chem.’ [N:F.], ii. 381-384; ‘Proc. Phys. Soe.’ xiii. 17 (Abs.); ‘Nature,’ 1. 188 (Abs.) ‘Johns Hopkins Univ. Cire.’ xiii. (No. 112), 74— 76; ‘Beiblatter,’ xix. 242 (Abs.) ‘Bihang till K. Svensk. Akad. Handl.’ xx. Afd. I. No. 1, 1-38; ‘Ann. Phys. u. Chem.’ [N.F.], liv. 520- 543; ‘Nature, li. 620 (Abs.) ‘Ann. Phys. u. Chem.’ (NEY), sautic209=23iee © Proc. Phys. Soc.’ xiii. 13 (Abs.) ‘Denkschr. Akad. Wien,’ Ixi. 347-364; ‘Ber’ Xxvili. (Ref.), 270 (Abs.) ‘Proc, Roy. Soc.’ lvi. 192- 193 (Abs.); ‘Chem. News,’ lxx. 2-4, 15-16; ‘Nature,’ 1. 238 (Abs.) : ‘J. Chem. Soc.’ Ixviii. II. 432 (Abs.); ‘Beibliitter,’ xviii, 997-998 (Abs.) ON THE BIBLIOGRAPHY OF SPECTROSCOPY. W. N. Hartley B. Hasselberg F. Aymonnet. A. de Gramont M. Glaser W.N.Hartley . G. D. Liveing and J. Dewar. F. Paschen L. Thomas E. Kottgen F. Paschen . B. Hasselberg V. Schumann, : 1898, EMISSION SPECTRA, 1894. Flame Spectra at High Tempera- tures. scopic Phenomena and Thermo- chemistry of the Bessemer Pro- cess. (Read June 14.) Ueber das Linienspectrum des Sauerstotis, (June.) Sur les radiations calorifiques comprises dans la partie lumi- neuse du spectre. (Read July 9.) Sur le spectre de lignes du soufre, et sur sa recherche dans les com- posés métalliques. (Read July 2.) Funkenspectra mittels der In- fluenzmaschine. (Aug.) New Methods of Spectrum Analy- sis, and on Bessemer Flame Spectra, (Aug.) Preliminary Note on the Spectrum of the Electric Discharge in Liquid Oxygen, Air, and Nitro- gen. (Aug.) Die genauen Wellenlingen der Banden des ultrarothen Kohlen- siure- und Wasserspectrums. (Aug.) Sur la constitution de lare élec- trique. (Read Oct. 29.) Untersuchungen der spectralen Zusammensetzung verschiedener Lichtquellen. (Nov.) Notiz iiber die Giiltigkeit des Kirchhoff’schen Gesetzes von der Emission. (Dec.) Untersuchungen tiber die Spectra der Metalle im_ electrischen Flammenbogen. I. Spectrum des Chroms. Vom Wasserstoffspectrum Part III. The Spectro- | 44.9 ‘Proc. Roy. Soc.’ lvi. 193- 199 (Abs.); ‘ Nature,’ 1]. 261-262 (Abs.); ‘J. Chem. Soc.’ Ixviii. II. 432-433 (Abs.); ‘ Beiblitter,’ xviii. 997-998 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], lii. 758-761. (Cap Rs (cxixey 151-154. ‘Beiblitter, xix. 64 (Abs.) °C. R. cxix. 68-70; ‘ Bei- blitter,’ xviii. 912 (Abs.) ; ‘Chem News,’ Ixx. 49 (Abs.); ‘J. Chem. Soc.’ Ixvi. II. 434-435 (Abs.) ‘ Zeitschr. f. phys. u. chem. Unterr.’ vi. 303-304; ‘ Beibliitter,’ xviii. 559 (Abs.) ‘Brit. Assoc. Rep.’ 1894, 610-611; ‘ Beiblatter, xx. 26 (Abs.) ‘Phil. Mag.’ [5], xxxviil. 235-240; ‘J. Chem. Soc.’ Ixvili. II. 33-34 (Abs.); ‘Ber.’ xxviii. (Ref.), 4-5 (Abs.) ; ‘ Beiblitter,’ xix. 60 (Abs.) ‘Ann. Phys. u. Chem.’ (N.F.], liii, 334-336 ; ‘Proc. Phys. Soc.’ xiii. 15 (Abs.) °C. RB’ cxix. 728-730; ‘Nature,’ li. 47 (Abs ) ‘Ann. Phys. u. Chem.’ [N.F.], iii. 793-811; ‘ Nature,’ li. 334 (Abs.) ‘Ann. Phys. u. Chem. [N.F.], li. 40-46: ‘Proc. Phys. Soc.’ xiii. 13 (Abs.) ‘Handl. K. Svens. Vet. Akad.’ xxvi. 32 pp.; ‘ Bei- blitter,’ xviii. 837 (Abs.) ‘Jahrb. f. Photogr.’ viii. 59_64; ‘ Beibliitter,’ xviii. 752 (Abs.) GG 450 Lord Rayleigh and | W. Ramsay. W. Crookes W. N. Hartley H. A. Nowland and | Rk. R. Tatnall. B. Hasselberg G. W. A. Kahlbaum H. F. Newall. H. A. Rowland and tt ht. Tatnall. E. C. C. Baly. M. Lerthelot REPORT—1898. EMISSION SPECTRA, 1895. Argon, a New Constituent of the Atmosphere. (Read Jan. 31.) On the Spectra of Argon. Jan. 31.) (Read On the Spark Spectrum of Argon as it appears in the Spark Spec- trum of Air. (Read Jan. 31.) The Arc Spectra of the Elements. I, Boron and Beryllium. (Jan.) | Untersuchungen iiber die Spectra der Metalle im electrischen Flam- menbogen. II. Spectrum des Titans. (Read Feb. 13.) (‘ Handl. K. Svensk. Vet. Akad.’ xxviii. No. 1, pp. 32). Ueber den neuentdeckten Be- standtheil der Atmosphiire, das Argon, (Feb.) Note on the Spectrum of Argon. (Read Feb. 21.) The Arce Spectra of the Elements. II. Germanium. A Possible Explanation of the Twofold Spectra of Oxygen and Nitrogen. (Read March 21.) Sur l’argon et sur l’hélium. (Read March 25.) ‘Phil. Trans.’ elxxxvi. A, 187-141; ‘ Proc. Roy. Soc. lvii. 265-287; ‘Chem. News, Ixxi. 651-59; ‘Zeitschr. f. physikal. Chem. xvi. 344-369; ‘ Beiblatter,’ xix. 276-279 (Abs.); ‘J. Chem. Soc.’ lxx. II. 99-106 (Abs.) ‘Phil. Trans.’ clxxxvi. A. 243-251; ‘Proc. Roy. Soc. Ivii. 287-289; ‘Chem. News,’ lxxii. 66— 69; ‘Zeitschr. f. physi- kal. Chem.’ xvi. 369-379 ; ‘Ber. xxviii. (Ref.), 176 (Abs.) ; ‘ Beibliitter,’ xix. 331-332 (Abs.) ‘Proc. Roy. Soe.’ lvii. 293- 296; ‘Beiblatter,’ xix. 625 (Abs.) ‘Astrophys. J.’ i. 14-17; ‘Beiblatter, xix. 424 (Abs.) r ‘ Beiblitter,’ xx. 304(Abs.) ‘Verh. naturf. Gesellsch. d. Basel, xi. 151-173; ‘Beiblatter, xix. 461 (Abs.) ‘Proc. Roy. Soc.’ lvii. 346— 350; ‘Nature, li. 454; «Chem. News,’ lxxi. 115- 116; ‘Astrophys. J.’ i. 372-376; ‘Ber.’ xxviii. (Ref.), 838 (Abs.) ‘ Astrophys. J.’i. 149-153 ; ‘ Beibliitter,’ xx. 29 (Abs.) ‘Proc. Roy. Soc.’ lvii. 468— 469; ‘Chem News,’ Ixxi. 169-170(Abs.) ; ‘Nature,’ li. 550 (Abs.) ; ‘J. Chem. Soc.’ Ixviii. 11. 469 (Abs.) \G, R?. ‘exx, 1660-661; ‘Ber.’ xxviii. (Ref.), 318 (Abs.); ‘Nature,’ li. 552 (Abs.); ‘Chem. News,’ Ixxi. 176. —_ - == ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 45] W. Crookes W. Ramsay H. W. Vogel . : P. T. Cleve . A. de Gramont J. N. Lockyer 5 W. Ramsay Lord Rayleigh J. S. Ames J. Evershed;. W. R. E. Hodgkin- son. L. Palmieri . EMISSION SPECTRA, 1895. The Spectrum of the New Gas from Cléveite. (Read March 27.) Discovery of Helium in Cleveite. (Read March 27.) Terrestrial Helium. (Read March 27.) Ueber das sogenannte kiinstliche Spectrum von Charles E. Benham. (Read March 8.) Sur la présence de Vhélium dans la clevéite. (Read April 16.) Sur les spectres de sélénium et de quelques séléniures naturels. (Read April 8.) On the New Gas obtained from Uraninite. Notes I. IL, III. (Read April 25, May 9.) On a Gas showing the Spectrum of Helium, the reputed cause of D,, one of the Lines of the Coronal Spectrum. Preliminary Note. (Read April 25.) On Argon. (Lecture at Royal Institution, April 5.) The Spectrum Researches of Pro- fessor J. M. Eder and E. Valenta. (May.) | Experiments on the Radiation of Heated Gases. Argon in Minerals. (May.) (May) . A proposito della riga dell’ Helium apparsa nello spettro di una sub- limazione vesuviana nel 1881, ed ora riveduta da Ramsay e da Cléve nella Clevite o Cléveite. (Read May 4.) ‘J. Chem. Soc.’ Ixvii. 1108-1109 ; ‘Chem.’ News,’ Ixxi. 151; ‘ Ber. xxviii. (Ref.), 839 (Abs.) ; ‘ Beiblatter,’ xix. 624 (Abs.); ‘ Nature,’ li. 543- 544; ‘Proc. Chem. Soc.’ xi. 60-61. ‘Proc. Chem. Soc.’ No.150, 59-60; ‘Chem. News,’ lxxi. 151. ‘Proc. Chem. Soc.’ No. 150, 59-60; ‘Nature,’ li. 512, 543. ‘Verhandl.phys. Gesellsch. Berl.’ xiv. 45-47. °C. RY exx. 834; ‘ Beibliit- ter,’ xix. 568 (Abs.); ‘J. Chem. Soc.’ Ixviii. J1.347 (Abs.) “Cx VR. Cxe 1778-780; ‘Ber.’ xxviii. (Ref.), 320 (Abs.); ‘ Beibliitter,’ xix. 566 (Abs.); ‘J. Chem. Soc.’ Lxviii. II. 338 (Abs.) * Proc. Roy. Soe.’ lviii. 67— 70,113-119 ; ‘ Beibliitter,’ xix.729 (Abs.); ‘ Nature,’ li. §, 55-56; ‘Chem. News, Ixxi. 295; ‘ Ber.’ xxix. (Ref.), 161 (Abs.) ‘Proc. Roy. Soc.’ lviii. 65— 67; ‘Chem.’ News,’ lxxi. 211; ‘ Ber.’ xxviii. (Ref.), 839 (Abs.); ‘Nature,’ its, 7. ‘Chem. News,’ Ixxi. 299- 302, 310-312; * Nature,’ lii. 159-164. \ Astrophys. J.’ i. 445-446; ‘Nature,’ lii. 275-276. ‘Phil. Mag.’ 460_476. ‘Chem. News,’ Ixxi. 248; ‘ Beiblitter,’ xix. 597-598 (Abs.) ‘Rend. R. Accad. Napoli,’ [3], i. 121-122; ‘ Beibliit- ter,’ xx. 531 (Abs.) [5], are. G G2 452 J. N. Lockyer W. Ramsay W. Ramsay and J. N. Collie. W. Ramsay, J. N. Collie, and M. Travers. C. Runge . . » « ° A. Schuster B. Brauner . H. Deslandres ” * REPORT—1898. EMIssIon SPECTRA, 1895. Sur l'analyse spectrale des gaz dégagés par divers minéraux. (Read May 20.) Sur l’argon et Vhélium. ‘(Read May 13.) Argon in Minerals. (May) . “ Helium, a Gaseous Constituent of Certain Minerals. Part 1, (Read May 2.) The Short Wave-lengths of the Spark Spectrum of Aluminium. (May.) On the Line Spectra of the Ele- ments. (May.) Sur les spectres cannelés. May 6.) (Read Note on Gases of the Helium and Argon Type. (June.) Découverte Mune troisi¢me radia- tion permanente de l’atmosphére solaire dans le gaz de la clévéite. (Read June 17.) | Etude spectrale des charbons du four électrique. (Read June 10.) "Co R.”, exx. 1103-1104 s ‘Beiblitter, xix, 566- 567 (Abs.); ‘ Ber.’ xxviii. (Ref.), 592 (Abs.); ‘J. Chem. Soc.’ Ixviii. II. 430-431 (Abs.); ‘ Proc. Phys. Soc.’ “xiii, -341 (Abs.); ‘Chem. News,’ xxi. 281 (Abs.) ‘Cc. R. cxx. 1049-1050; ‘Chem. News,’ Ixxi. 259 (Abs.) ; ‘ Nature,’ lii. 96 (Abs.); ‘ Beiblatter,’ xix. 531 (Abs.) ; ‘ Ber.’ xxviii. (Ref.), 448 (Abs.) ‘Chem. News,’ Ixxi. 268 ; ‘Beiblaitter, xix. 597- 598 (Abs.) ‘Proc. Roy:= Soe._ lyin: 81-89; ‘J. Chem. Soc.’ Ixviii. 684-701; ‘ Bei- blatter,” xix. 673-674 (Abs.); ‘ Nature,’ lii. 55 (Abs.) ‘ Astrophys. J.’ i. 433. ‘Nature,’ lii. 106-108 ; ‘ Beibliitter,’ xx. 530-531 (Abs.) “Ca JR.) 1exx ee daieoaso ‘ Beiblatter,’ xix. 788- 789 (Abs.) ; ‘Proc. Phys. Soc.’ xiii. 306 (Abs.) ‘Chem. News,’ Ixxi. 271; ‘J. Chem. Soe.’ Ixviii. II. 347 (Abs.); ‘ Ber.’ xxviii. (Ref.), 904-905 (Abs.); ‘ Beiblitter,’ xix. 675 (Abs.) °C. BR’ cxx. 1331-1333 ; ‘ Ber.’ xxviii. (Ref.), 1045 (Abs.); ‘ Beibliatter,’ xix. 693 (Abs.); ‘Chem.News,’ Ixxii. 12 (Abs.); ‘ Proc. Phys. Soc.’ xiii. 340 (Abs.); ‘ Nature,’ lii. 216 (Abs.) *C. R.’ \ cxx, 1259-21260; ‘Chem, News,’ Ixxii. 9; ‘Proc. Phys. Soc.’ xiii. 344 (Abs.); ‘ Nature,’ lii. 192 (Abs.) ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 453 J. N. Lockyer C. J. Lundstré6m W. Ramsay, J. N. and M. Collie, Travers. C. Runge C. Runge and F. Paschen, J. M. Eder and £. Valenta. F. Exner Haschek. W. Huggins . F. Paschen W. Ramsay C. Runge and F. Paschen. H. Crew and O. H. Rasquin, and KE. EMISSION SPECTRA, 1895. On the New Gas obtained from Uraninite. Notes IV. V. (Read June 13.) Flame Spectra observed at Swedish Bessemer Works. (Read June 20; revised Oct. 18.) Helium, a Constituent of Certain Minerals. (Read June 20.) Terrestrial Helium. (June) . Ueber das Spectrum des Helium. (Read June 20.) Ueber die verschiedenen Spectren des Quecksilbers. (Read July 5.) Ueber die ultravioletten Funken- spectren der Elemente. I. Mit- theilung. (Read July 11.) Helium. (July) . . Ueber Gesetzmiissigkeiten in dem Spectren fester K6rper und iiber eine neue Bestimmung der Son- nentemperatur. (Read July 6.) Argon and Helium in Meteoric Iron. (July.) Ueber die Bestandtheile des Cléveitgases. (Read July 11.) Note on the Spectrum of Carbon. (Aug.) ‘ Proc. Roy. Soe.’ lviii.191- 195; ‘Nature,’ lii. 214; ‘Chem. News,’ lxxii. 4-5, 271-272,283; ‘Beiblitter,’ xix. 825 (Abs.); ‘Ber.’ xxix. (Ref.), 161 (Abs.) ‘Proc. Roy. Soc.’ lix. 76 - 98 ; ‘ Beibliitter,’ xx. 367 (Abs.) ‘J. Chem. Soc.’ Ixvii. 684— 701; ‘Nature,’ lii. 306- 308, 331-334. ‘Nature,’ lii. 128; ‘ Chem. News,’ lxxi. 283; ‘ Bei- blitter,” xix. 624-625 (Abs.) ‘ Sitzungsb. Akad. Berlin,’ xxx. 639-643; ‘ Bei. blatter,’ xix. 884-885 (Abs.); ‘Proc. Phys. Soe.’ xiii, 345-346 (Abs.) ‘Denkschr. Akad. Wien,’ ]xi, 401-430; ‘Ann. Phys. u. Chem,’ [N.F.], lv. 479— 502; ‘J. Chem. Soc.’ Ixx.) I. 223) .\(Abs5)); ‘ Ber.’ xxviii. (Ref.), 270 (Abs.); ‘ Proc. Phys. Soc.’ xiv. 47 (Abs.) ‘Sitzungsb. Akad. Wien,’ civ. Abth. Ila, 909- 962; ‘ Beiblitter, xx. 693 (Abs.); ‘ Proe. Phys. Soc.’ xiv, 238 (Abs.) ‘Chem. News,’ Ixxii. 27; ‘Beiblatter,’ xix. 730 (Abs.) ‘Gott. Nachr.’ i895, No. 3, 294-305. ‘Nature,’ lii. 224-225; ‘Beiblatter,” xix. 729 (Abs.) ‘Sitzungsb. Akad. Berlin,’ xxx. 759-763; ‘ Bei- blatter,’ xix. 885-886 (Abs.) ; ‘Phil. Mag.’ [5], xxxix. 297-303; ‘ Chem. News,’ Ixxii. 181-182 (Abs.); ‘Proc. Phys. Soc.’ xiii. 393-394 (Abs.) ; ‘Nature,’ lii. 520-522 (Abs.) ‘Astrophys. J.’ ii. 105. 103- H. Crew and O. H. Rasquin. W. Crookes . W. N. Hartley H. Kayser . ” H,F.Reid . W.Le Conte Stevens E. Wiedemann and G. C. Schmidt. L. J. Troost and V. R. Ouvrard. J. M. Eder and E. Valenta. J. N. Lockyer F.Paschen , REPORT—1898. EMIssIon SPECTRA, 1895. Note on the Magnesium Band at =5007. (Aug.) The Spectrum of Ramsay’s Com- pound of Argon and Carbon. (Aug. 11.) The Spectrum of Helium. (Aug.) On the Thermo-Chemistry of the Bessemer Process. (Read Aug.7.) The Blue Spectrum of Argon. (Aug.) Note on Helium and Argon. (Aug.) Preliminary Note on the Radiation of Incandescent Platinum. (Aug.) Recent Progress in Optics. (Aug.) Ueber Lichtemission organischer Substanzen im _ gasfdrmigen, fliissigen und festen Zustand. (Aug.) Sur la combinaison du magnésium avec largon et avec lhélium. (Read Sept. 2.) Ueber das rothe Spectrum des Argons. (Read Oct. 24.) The New Mineral Gases. (Oct.) . On the Existence of Law in the Spectra of Solid Bodies and ona New Determination of the Tempe- rature of the Sun. (Oct.) ‘Astrophys. J.’ ii. 100- 102; ‘ Beiblitter,’ xx. 30 (Abs.) ‘Chem. News,’ Ixxii. 99; ‘J. Chem. Soc.’ lxx. II. 2 (Abs.); ‘Ber.’ xxviii. (Ref.), 840 (Abs.) ‘Chem. News,’ Ixxii. 87- 89; ‘Nature,’ lili. 428- 430; ‘J. Chem. Soc.’ Ixx. | WTI Cabs); ‘Ber.’ xxviii. (Ref.), 840 (Abs.) ; ‘Proc. Phys. Soc.’ xiv. 161-162 (Abs.) ; ‘Zeitschr. anal. Chem.’ xi. 6-13. ‘Journ. Iron and Steel Inst.’ xlviii. 95-121 ; ‘ Nature,’ lii. 426-427 (Abs.) ‘Chem. News,’ Ixxii. 99- 100; ‘J. Chem. Soc.’ lxx. II. 2 (Abs.); ‘Ber.’ xxviii. (Ref.), 840 (Abs.) ‘Chem. News,’ lxxit. 89; ‘ Ber.’ xxviii. (Ref.), 840 (Abs.); ‘J. Chem. Soc.’ lxx. II. 19-20 (Abs.) ‘Astrophys. J.’ ii. 160- 161; ‘ Beiblitter,’ xx. 27-28 (Abs.) ‘Amer. J. Sci.’ 1. 277- 286, 377-386; ‘ Nature,’ liii. 233-238. ‘Ann. Phys. u. Chem,’ [N.F.], lvi. 18-26; ‘ Na- ture,’ lii. 611 (Abs.); ‘Proc. Phys. Soc.’ xiii. 471-472 (Abs.); ‘J. Chem. Soc.’ Ixx. IT. 86- 87 (Abs.) °C. R. cxxi. 394-395; ‘J. Chem. Soc.’ Ixx. II. 99 (Abs.) ‘Sitzungsb. Akad. Wien,’ civ. 218-220; ‘ Monats. f. Chem.’ xvi. 893-895 ; ‘Ber.’ xxix. (Ref.), 7-8 (Abs.) ; ‘ Beiblatter,’ xx. 126 (Abs.); ‘ Chem. News,’ Ixxii. 289-290. ‘Nature,’ lit. 547-549. ‘ Astrophys. J.’ il. "202- 211; ‘Nature,’ lili. 38 (Abs.) ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 45 H. A. Rowland and R. R. Tatnall. H. Wilde e . C. Bohn. : H. Crew . J.M. Eder and E. Valenta. A. de Gramont H.A. Hill. A. Killas and W. Ramsay. J. N. Lockyer ” e . G. J. Stoney . . A, A. Michelson . A. Schuster . 5 E. Wiedemann and G. C. Schmidt. EMISSION SPECTRA, 1895. The Arc Spectra of the Elements. Ill. Platinum and Osmium. (Oct.) Helium and its Place in the Natural Classification of Elemen- tary Substances. (Read Oct. 1.) Ueber Flammen und leuchtende Gase. (Noyv.) Photographic Maps of Metallic Spectra. (Nov.) Ueber die Spectren von Kupfer, Silber und Gold. (Read Nov. 7) Sur l’analyse spectrale directe des composés solides, et plus spéciale- ment des minéraux. (Noy.) Additional Notes on Argon and Helium. (Noyvy.) Examination of Gases from Certain Mineral Waters. (Read Noy. 28.) On the Gases obtained from the Mineral Eliasite. (Read Nov, 21.) On the New Gas obtained from Uraninite. Note VI. (Read Noy. 21.) On Prof. Runge and Paschen’s Photographs of the Spectrum of the Gas from Cléveite. (Read before Phys. Soc. Nov. 22.) On the Broadening of Spectral Lines. (Nov.) On the Evidence to be gathered as to the Simple or Compound Character of a Gas from the Con- stitution of its Spectrum. (Nov.) Spectralbeobachtungen an ver- diinnten Diimpfen von Metallen und Verbindungen, (Read Nov. 12.) Gr ‘Astrophys. J.’ ii, 184— 188; ‘ Beibliitter,’ xx. 365 (Abs.) ‘Phil. Mag.’ [5], xl. 466- 471; ‘J.Chem. Soc.’ Ixx. II. 165-166 (Abs.) ‘ Zeitschr. f. physikal. Chem.’ xviii. 219-239 ; © Beiblitter,” xx. 276 (Abs.) ; ‘ Proc. Phys. Soc.’ xiv. 2-3 (Abs.) ‘Astrophys. J. ii. 318- 320. ‘ Denkschr. Akad. Wien,’ Txili, 189-235; ‘ Bei- blatter,’ xx. 366 (Abs.) §C) Rl” cxxi. . d21-123 ‘Bull. Soc. Chim.’ [3], xili._xiv. 945-947 ; ‘ Ber.’ xxviii. (Ref.), 1048 (Abs.) ‘Amer. J. Sci.’ 1. 359-376. ‘Proc. Roy. Soc.’ lix., 68- 69; ‘Nature,’ liii. 191; ‘Chem. News,’ lxxii. 295. ©Proc. Roy. Soc.’ lix. 1-3; ‘Nature,’ lili. 190-191; ‘Chem. News,’ Ixxii. 283; ‘ Beiblitter,” xx. 314 (Abs.) © Proc. Roy. Soc.’ lix. 4-8; ‘Nature, lili. 163-164 (Abs.); ‘Chem. News,’ lxxii. 271-272; ‘Bei- blitter,’ xx. 314 (Abs.) ‘Nature, liii. 94-95 (Abs.); ‘Chem. News,’ Ixxii. 266— 267 (Abs.) ‘Astrophys. J.’ ii. 251- 263; ‘Beiblitter,’ xx. 532-533 (Abs.) ‘Chem. News,’ lxxii. 224. ‘Sitzungsb. phys. med. Soc. Erlangen, xxvii. 127-144; ‘ Beibliitter,’ xx. 693-694 (Abs.); ‘Naturw. Rundschau,’ xi. 429-431 (Abs.) J. M. Eder and E. Valenta. 8. Friedlinder Ch, Moureu R. Nasini and F. Anderlini. E, Demarcay J.M.Eder , O, Postma W. Crookes J.M. Eder . * C. Runge and F. Paschen. W. A. Tilden J. N. Collie and W. Ramsay. W. J. Humphreys and J, F. Mohler. REPORT—1898. EMISSION SPECTRA, 1895, 1896. Ueber die verschiedene Spectren des Argons. (Vorliufige Mittheil- ung). (Read Dec. 19.) Ueber Argon, (Dec.) . 6 Sur la présence de largon et de Vhélium dans une source d’azote naturelle. (Read Dec. 2.) Sopra alcuni fatti relativi all argon. (Read Dec. 1.) Spectres électriques. (Texte 91 pp., Planches 20.) Ueber ultravioletten Absorptions- und Enmissionsspectren (‘ Verh. Ges. Naturf. u. Aerzte,’ II. 1. Halfte (1895), 78). Hiniges tiber Ausstrahlung und Absorption. (Inaug.-Diss. Am- sterdam, 1895, 94 pp.) 1896. Das Spectrum des Heliums . . Bemerkung zu Herren C. Bohn’s Abhandlung ‘ Ueber Flammen und leuchtende Gase.’ (Jan.) On Crookes’s Spectrum of Helium. (Jan.) An Attempt to Determine the Con- dition in which Helium and the Associated Gases exist in Mine- rals. (Read Jan, 23.) On the Behaviour of Argon and Helium when submitted to the Electric Discharge. (Read Feb. 13.) . Effect of Pressure on the Wave- lengths of Lines in the Arc Spec- tra of Certain Elements. (Feb.) ‘Sitzungsb. Akad. Wien,” civ. Abt. II.a, 1171-1177; * Monatsh. f. Chem.’ xvii. 50-56 ; ‘ Ber.’ xxix.(Ref.), 341 (Abs.); ‘ Beibliitter,’ xx. 531-532 (Abs.) ; ‘J. Chem. Soc.’ Ixx. IL. 405 (Abs,) ; ‘Proc. Phys. Soc, xiv. 236-27 (Abs.) ‘Zeitschr. f.. physikal. Chem.’ xix. 657-667 ; ‘Beiblitter,” xx. 775 (Abs.); ‘J. Chem: Soc.’ lxx. IL. 457 (Abs.); ‘Chem. News,’ Ixxiv. 179-180 (Abs.) SC. Ry cxxi, (S19=820i5 ‘Chem. News,’ Ixxii. 310. ‘Rend. R. Accad. d.Lincei,’ [5], iv. II. Sem. 269-290; * Beiblatter,” xx. 315 (Abs.) ‘ Beiblitter, xix. [58] (title). ‘Beiblitter,’ xxii. 98 (Abs.)} ‘Zeitschr. f. anorg. Chem.” xi. 6-13; ‘Beiblatter, xx. 275 -276 (Abs.) ‘Zeitschr. f. physikah Chem.’ xix. 20-24; ‘ Bei- blitter, xx. 276-277. (Abs.) ‘Nature,’ lili. 245; ‘ Bei. blitter,’ xxi. 633 (Abs. ) ‘Proc. Roy. Soc.’ lix. 218— 224. ‘Proc. Roy. Soe.’ lix, 257— 270. ‘ Astrophys. J.’ iii. 114— 118; ‘Beiblitter, xx. 533 (Abs.) H. Kayser J. Landauer . C. W. Baldwin F, Exner Haschek. and E. A. Gamgee E. Haschek J. N. Lockyer W. Ramsay W. N. Hartley H. A, Rowland and R. R. Tatnall. W. N. Hartley and H. Ramage. H. Kayser J. F. Mohler and L. E, Jewell. J. M. Eder and E. Valenta. A. de Gramont 457 ‘Chem. Zeitung,’ xx. 195— 196; ‘Chem. News, lyxiv. THE BIBLIOGRAPHY OF SPECTROSCOPY. EMISSION SPECTRA, 1896. Die Fortschritte der Spectro- scopie. (Feb.) 307-309. Die Spectral-Analyse. (Braun- schweig, 174 pp.) (Feb.) A Photographic Study of Arc Spectra. I. (March.) Ueber die ultravioletten Funken- spectra der Elemente, II. III. IV. (Read March 19.) On the Relations of Turacin and Turacoporphyrin to the Colouring Matter of the Blood. (Read March 19.) Ueber die ultravioletten Funken- spectra der Elemente. (Read March 19.) On the New Gas obtained from Uraninite. (Seventh Note.) Re- marks on Messrs. Runge and Paschen’s Diffusion Experiment. (Read March 19.) Helium, a Gaseous Constituent of Certain Minerals. Part II. Den- sity. (Read March 19.) The Determination of the Compo- sition of a ‘White Son’ by a Method of Spectrographic Analy- sis. (Read April 23.) The Are Spectra of the Elements. IV. Rhodium, Ruthenium, and Palladium. (April.) On the Occurrence of the Element | Gallium in the Clay Ironstone of the Cleveland District of York- shire. (Preliminary Notice.) (Read May 7.) Ueber die Spectren des Argons. (Read May 7.) On the Wave-lengths of some of the Helium Lines in the Vacuum Tube, and of D, in the Sun. (May.) Spectralanalytische Untersuchun- gendes Argons. (Read June 11.) (‘ Denkschr. Akad. Wien,’ Ixiv. 39 pp.) (June.) Spectres de dissociation des sels fondus, métaux alkalins, sodium, potassium, lithium. (Read June 15.) ‘Chem. News,’ xxiii. 70- 71 (Review). ‘Phys. Review,’ iii. 370- 380; ‘ Beiblitter,’ xx. 774 (Abs.) ‘Sitzungsb. Akad. Wien,’ cv. Ila, 389-436, 503- 574, 707-740. ‘Proc. Roy. Soc.’ lix. 339- 342. ‘Wien. Anz.’ xxxili. 75-76 (Abs.) ‘Proc. Roy. Soc.’ lix, 342- 343; ‘ Beibliitter,’ xx. 775-776 (Abs. ) ‘Proc. Roy. Soc.’ lix. 325— 330. ‘J. Chem. Soc.’ lxix. 842— 844; ‘Chem. News,” Ixxiii, 229 (Abs.) ‘Astrophys. J.’ iii. 286— 291. ‘ Proc. Roy. Soc.’ lx. 35-37. ‘Sitzungsb. Akad. Berl.” 1896, 551-564; ‘ Astro— phys. J.’ iv. 1-17; ‘Bei- bliitter, xx. 976 (Abs.) ‘Astrophys. J. iii. 355. 351— ‘Wien. Anz.’ xxxiii. 161 (Abs.); ‘Beiblitter,’ xxi. 129 (Abs.) ‘C. RY exxii. 1411-1413 ;. ‘ Beiblitter, xx. 698 (Abs.); ‘Chem. News,” lxxiv. 12 (Abs.) A. de Gramont W. N. Hartley H. Kayser . H. Wilde : M. Bamberger G, Magnanini W. Ramsay and J. N. Collie. J. R. Rydberg W.Spring . W. Wien F H. Crew - J. R. Rydberg P, Barriére . Birkeland ., O. J. Lodge and B. Davies. W. N. Hartley W. Crookes .. REPORT—1898. EMISSION SPECTRA, 1896. Sur le spectre du phosphore dans les sels fondus et dans certains produits métallurgiques. (Read June 29.) Sur les spectres des métalloides dans les sels fondus. Soufre. (Read June 8.) Remarks on the Origin of some of the Lines and Bands observed in the Spectra from Swedish Besse- mer Works. (Read June 20.) The Spectra of Argon. (June) On the Spectral and other Pro- perties of Thallium in Relation to the Genesis of the Elements. (June.) Ueber den Nachweis von Argon in dem Gase einer Quelle in Perch- toldsdorf bei Wien. (Read July 9.) Intorno alla ipotesi della colora- zione degli joni. (July.) Sur Vhomogénéité de l’argon et de Vhélium. (Read July 27.) Die neue Grundstoffe des Cléveit- gases. (July.) Sur la couleur et le spectre lumineux de quelques corps organiques. (July.) Ueber die Energievertheilung im Emissionsspectrum eines schwart- zen K6rpers. (July.) Normal Spectrum of the Zinc Are. (Aug.) The New Elements of Cléveite Gas. (Aug.) Lucium, a New Element. (Sept.). Sur un spectre des rayons catho- diques. (Read Sept. 28). Extension of the Visible Spectrum. (Sept.) Argon and Helium. (Oct.) . The Alleged New Element, Lucium. (Noyv.) *C. R.’ exxii. 1534-1536 ; ‘Chem. News,’ Ixxiv. 41 (Abs.); ‘ Nature,’ liv. 239 (Abs. ) *C. RY cxxii. 1326-1328 ; ‘ Beiblitter, xx. 693 (Abs.) ‘Proc. Roy. Soc.’ lix. 98— 101; ‘ Beibliitter,” xx. 367 (Abs.) ‘ Astrophys. J. iv. 1-17. ‘Chem. News,’ Ixxiii. 304- 305; ‘ Beiblatter,’ xxi. 633 (Abs.) ‘Monatsh, f. Chem.’ xvii. 604-612. ‘Gazz. chim. ital.’ xxvi. II. 92-96; ‘ Beiblatter,’ xxi. 30-31 (Abs.) °C. R. cxxiii. 214,916; ‘Beiblitter, xx. 823 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], lviii. 674-679 ; ‘Nature, liv. 455-456 (Abs.) ‘Bull. Acad. Belg. [3], Xxxli. 43-51; ‘ Beiblat- ter,’ xxi. 31 (Abs.) ‘Ann. Phys. u. Chem.’ [N.#.], lviii. 662-669 ; ‘Nature,’ liv. 455 (Abs.) ‘ Astrophys. J.’ iv.135-137. ‘ Astrophys. J.’ iv. 91-96; ‘Chem. News,’ Ixxiv. 238-239. ‘Chem. News,’ lxxiv. 159; ‘Beiblitter, xx. 930 (Abs.) °C. R? exxiii. 492-495. ‘Nature,’ liv. 622. ‘Chem. News,’ Ixxiv. 209; ‘ Beiblatter, xxi. 632- 633 (Abs.) ‘Chem. News,’ Ixxiv. 259- 260; ‘ Beibliitter, xxi. 86 (Abs.) OT ee ee ee a re —- , 4 ON THE BIBLIOGRAPHY OF SPECTROSCOPY. F. Exner and E. Haschek. W. J. Humphreys. 0. J. Lodge and B. Davies. O. Schott 3 F. Schutzenberger and Boudouard. A. Swinton . W.N. Hartley and H. Ramage. B. Hasselberg A.Langlet < J. R. Rydberg V. Schumann F M. Berthelot FF. Exner and E. Haschek. A. de Gramont W.N. Hartley and H. Ramage. H. Muraska and M. Kasuya, 459 EMISSION SPECTRA, 1896, 1897. Ueber die ultravioletten Funken- spectra der Elemente. V. (Read Nov. 19.) A Further Study of the Effect of Pressure on the Wave-lengths of Lines in the Are Spectra of Cer- tain Elements. (Nov.) Extension of the Visible Spectrum. (Nov.) Ueber (Nov.) electrische Capillarlicht. Sur les terres du groupe yttrique contenues cans les sables mona- zités. (Read Noy. 16.) Extension of the Visible Spectrum. (Nov.) On the Occurrence of Gallium in the Clay-iron-stone of the Cleveland District of Yorkshire. Determina- tion of Gallium in Blast-furnace Iron from Middlesbrough. (Read Dec. 17.) Untersuchungen iiber die Spectra der Metalle im electrischen Flam- menbogen, III. Kobalt und Nickel. (‘ Handl. K. Svensk. Vet. Akad.’ xxviii. No. 6, 44 pp.) Priifung von Kolm auf Helium (Oefvers. K. Vet.Acad. Stockholm,’ liii. 663-664). Studien iiber das System der Spec- tren (‘Verhandl. Ges. Deutsch. Naturf. u. Aerzte,’ ii. I. Hilfte, 53). Von den brechbarsten Strahlen und ihrer photographischen Aufnahme. ‘Vi 1897. Recherches sur Vhélium. (Head Jan. 18.) Ueber die ultravioletten Funken- spectra der Elemente. VI. VII. VIII. IX. (Read Jan. 21, July 8.) Spectres des métalloides dans les sels fondus: silicium. (Read Jan. 25.) On the Dissemination of some of the Rarer Elements, and the Mode of their Association in Common Oresand Minerals. (Read Jan. 21.) Das Johanniskiiferlicht und die Wirkung der Diaimpfe von festen und fliissigen K6rpern auf photo- graphische Platten. (Jan.) ‘Sitzungsb. Akad. Wien,’ cv. II.a, 989-1013 ; ‘Wien. Anzeiger,’ 1897, 7. ‘Astrophys. J.’ iv. 262; * Beibliitter,’ 336-337 (Abs.) 249_ EX. ‘ Nature,’ lv. 33. ‘Ann. Phys. u. Chem.’ PNB) dix, (68=772;; ‘Nature,’ lv. 214 (Abs.) ‘C. R, exxiii. 782-788 ; ‘ Nature,’ lv. 95 (Abs.) ‘Nature,’ lv, 32-33. ‘Proc. Roy. Soc.’ Ix. 393- 407. ‘Beiblitter, xx. 692-693 (Abs.); ‘Astrophys. J.’ iv. 212-233, 288-304, 343-366, v. 38-49; ‘Nature,’ lv. 111 (Abs.) ‘Beiblitter, xxi. 674 (Abs.) ‘Beiblitter, xx. [81], title. ¢ Jahrb. f. Photogr.’ x. 42— 45; * Beibliitter,’ xx. 975-976 (Abs.) SO. Ry exsdv.4 lils—119 ‘Nature,’ lv. 311 (Abs.) ‘Sitzungsb. Akad. Wien,’ evi. ILa, 36-53, 54-68, 337-356, 494-520. °© R. cxxiv. 192-194; ‘J. Chem. Soc.’ Ixxii, 238 (Abs.) ‘J. Chem. Soc.’ Ixxi. 533- 547; ‘Chem. News,’ lxxix. 129-130 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], Ixiv. 186-192; “Chem. Centr.’ 1898. I. 697-698 (Abs.) 460 J. Trowbridge and T. W. Richards, J. 8S. Ames and W. J. Humphreys. A. de Gramont W.N. Hartley and H. Ramage. O. Lohse fs W. Ramsay and M. W. Travers. W. A. Tilden . M. W. Travers J. Trowbridge and T. W. Richards. W. N. Hartley G. Urbain and E. Budischovsky. H, Kayser H. Becquerel. W. N: Hartley and H. Ramage. G. Le Bon REPORT—1898. EMISSION SPECTRA, 1897. The Spectra of Argon. (Jan.) On the Spectra of Heavy and Light Helium. (Feb.) Spectres de dissociation des sels fondus; miétalloides, chlore, brome, iode. (Feb.) On the Spectrographic. Analysis of some Commercial Samples of Metals, of Chemical Preparations, and of Minerals from the Stassfurt Potash Beds, (Read Feb. 18.) Untersuchungen des _ violetten Theiles einiger linienreichen Metallspectra. (Read Feb. 18.) The Gaseous Constituents of Cer- tain Mineral Substances and Na- tural Waters. (Read Feb. 4.) On the Gases Enclosed in Crystal- line Rocks and Minerals. (Read Feb. 4.) Some Experiments on Helium. (Read Feb. 4.) The Multiple Spectra of Gases. (Feb.) Experiments on the Flame Spec- trum of Carbon Monoxide. (Read March 18.) Recherches sur les sables mona- zités. (Read March 22.) On the Spectrum of Hydrogen. (April.) Explication de quelques expéri- ences de M. G. Le Bon. (Read May 10.) A Spectrographic Analysis of Tron Meteorites, Siderolites, and Me- teoric Stones. (Read May 19.) (‘ Proc. Roy. Soc. Dublin’ [N.8.], viii. Part 6.) Sur les propriétés de certaines radiations du spectre. (Read May 24.) ‘Amer. J. Sci.’ [4], iii. 15- 20; ‘Phil. Mag. [5], xliii. 77-83; ‘Nature,’ lv. 305 (Abs.) ‘ Astrophys. J.’ v. 97-98 ; ‘Beiblitter,’ xxi. 514 (Abs.) ‘Ann, Chim. et Phys.’ [7], x. 214-234. ‘J. Chem. Soc.’ lxxi. 547— 550; ‘Chem. News,’ Ixxy. 161 (Abs.) ; ‘Chem. Centr.’ 1897, I. 665 (Abs.) ‘Sitzungsb. Akad. Berl’ 1897, 179-197. ‘Proc. Roy. Soc.’ lx. 442— 448; ‘Beiblatter,” xxi. 300 (Abs.) *Proc. Roy. Soc.’ Ix. 453- . 457; ‘ Nature,’ lv. 381- 382 (Abs.) ; ‘Chem. News,’ Ixxv. 169-170. ‘Proc. Roy. Soc.’ Ix. 449-453 ; ‘ Beibliitter, xxi. 300 (Abs.) ‘Amer. J. Sci.’ [4], iii. 117-120; °‘ Nature, lv. 406 (Abs.) ; ‘Phil. Mag.’ [5], xliii. 135-139. ‘Proc. Roy. Soc.’ 1xi. 217— 219; ‘Beiblatter, xxi. 735 (Abs.) °C. RY cxxiv. 618-621; ‘Chem. News,’ lxxv. 181- 182. ‘Astrophys. J.’ v. 243; ‘Beiblatter,” xxi. 734 (Abs.) ‘C. RY cxxiv. 984-988 ; ‘Chem. News, xxv. 280- 281. ‘Nature,’ lvii, 546 (Abs.) ; ‘Chem. News,’ Ixxvii. 121-122. ‘OC. R. cxxiv 1148-1151. — ———— J. S. Ames and _ W.J. Humphreys. W.Arnold . W. Huggins and Mrs. Huggins. _W. J. Humphreys . P. E. Lecoq de Boisbaudran. ” ” J. N. Lockyer ” . . C. E. Mendenhall and F. A. Saun- ders. A. de Gramont » s W. N. Hartley ON THE BIBLIOGRAPHY OF SPECTROSCOPY. EMISSION SPECTRA, 1897. Note on the Effect of Pressure upon the Series in the Spectrum of an Element. (June.) Ueber Luminescenz. (June) On the Relative Behaviour of the Hand K Lines of the Spectrum of Calcium. (Read June 17). Changes produced by Pressure in the Wave Frequencies of the Lines of Emission Spectra of Elements. (June.) Examen de quelques _ spectres. (Read June 8.) Examen de quelques spectres. (Read June 21.) On the Unknown Lines observed in the Spectra of Certain Minerals. (Read June 4.) Further Observations of Enhanced Lines. (Read June 17.) Preliminary Note on the Energy Spectrum of a Black Body. (June.) Observations sur les spectres des composés. (Read July 23.) Spectres de dissociation des sels fondus. Métaux alcalins, sodium, lithium, potassium. (Read July 23.) Sur le spectre du carbone. July 19.) (Read Sur le spectre des lignes du car- bone dans les sels fondus. (Read July 26.) On the Spectrum of Cyanogen as produced and modified by Spark Discharges. (Recd. July 13.) 461 ‘Johns Hopkins Univ. Circ.’ xvi. 41-42; ‘ Phil. Mag.’ [5], xliv. 119-122 ; ‘ Chem. News,’ Ixxvi. 21~— 22; ‘Beiblatter,’ xxi. 974-975 (Abs.); ‘Chem. Centr.’ 1897, II. 324 (Abs.) ‘Ann, Phys. u. Chem,’ [N.F.], lxi. 313-329. ‘Proc. Roy. Soc.’ lxi. 433- 441; ‘Beiblitter, xxi. 735-736 (Abs.); ‘Na- ture,’ lvi. 262 (Abs.) ‘Johns Hopkins Univ. Cire.’ xvi, 43-44; ‘ Bei- blatter,’ xxii. 219-221 (Abs.) °C. RY exxiv. 1288-1290. °C. R.’ exxiv. 1419-1421. ‘Proc. Roy. Soc.’ Ix. 133- 140; ‘J. Chem. Soc.’ Ixxii. II. 293 (Abs.); ‘Nature,’ liv. 261-263 (Abs.) ‘Proc. Roy. Soe.’ xi. 441_— 444; Beibliatter, xxi. 975 (Abs.) ‘Johns Hopkins Univ. Circ.” xvi. 47; ‘Phil. Mag.’ [5], xliv. 136. ‘ Bull. Soc, Chim.’ [3], xvii. 774-778; ‘Chem. Centr.’ 1897, II. 787-788 (Abs.) ‘Bull. Soc. Chim.’ [3], xvii. 778-782; ‘Chem. Centr.’ 1897, II. 785 (Abs.) S@l Re (exxv, 1722176: ‘J. Chem. Soc.’ Lxxii. II. 533-534 (Abs.) °C. BR.’ cxxv. 238-240; ‘J. Chem. Soc. lxxii II. 533-534 (Abs.); ‘Beiblitter, xxi. 973-— 974 (Abs.) ‘Proc. Roy. Soc.’ lx. 216- 221; ‘J. Chem. Soe.’ Ixxii. II. 293-299 (Abs.) ; ‘ Beiblatter,’ xxi, 734- 735 (Abs.) 462 C. Runge and F. Paschen. P. Zeeman ,. ° W. J. Humphreys . A.C. Jones . C. Runge and F. Paschen. G. A. Hemsalech W. J. Humphreys . J. R. Rydberg = H. Wilde 5 A. de Gramont 7 R. Nasini, F. Ander- lini, and R. Sal- vadori. Spectres de dissociation des REPORT—1898. EMISSION SPECTRA, 1897. Ueber die Serienspectra der Ele- mente Sauerstoff, Schwefel und Selen. (July.) Doublets and Triplets in the Spec- trum produced by External Mag- netic Forces. (July.) Changes in the Wave Frequencies of the Lines of Emission Spectra of Elements. (Aug.) Ueber einige Emissionsspectra des Cadmiums, Zinks und der Haloid- verbindungen des Quecksilbers und einiger anderen Metalle. (Aug.) On the Spectra of Oxygen, Sul- phur, and Selenium. (Aug.) On some New Lines in the Spark Spectrum of Aluminium. (Sept.) Changes in the Wave Frequencies of the Lines of Emission Spectra of Elements; their dependence upon the elements themselves and upon the physical conditions under which they are produced. (Oct.) The New Series in the Spectrum of Hydrogen. (Oct.) On Triplets with Constant Differ- ences in the Line Spectrum of Copper. (Oct.) Sur quelques nouvelles lignes spec- trales de Yoxygeéne et du thallium. (Read Nov. 8.) sels 27.) Spectres de dissociation des fondus; soufre. (Read Dec. sels fondus ; phosphore. (Read Dec. 27.) Spectres de dissociation des com- posés phosphoreux solides. (Read Dec. 27.) Gas delle terme di Abano dei sof- fioni boraciferi della Toscana, e gas combustibili dell’ Apparino Bolognese. (ead Dec 17.) ‘Ann. Phys. u. Chem, [N.F.], Ilxi. 641-686; ‘Chem. Centr.’ 1898, I. 298-299 (Abs.); ‘Na- ture,’ lvi. 388 (Abs.); ‘Science Abstr.’ i. 10 (Abs.); ‘J. Chem. Soc.’ Ixxii. IT, 533 (Abs.) ‘Phil. Mag,’ [5], xliv. 55- 60. ‘Brit. Assoc. Report,’ 1897, 556-557. ‘Ann. Phys. u. Chem.’ [N.F.], Ixii. 30-53; ‘J. Chem. Soc. lxxii. II. 534 (Abs.); ‘Science Abstr.’ i, 10 (Abs.) ‘Brit. Assoc. Report,’ 1897, 555 (Abs.) ‘ Phil. Mag.’ [5], xliv. 289- 291; ‘J. Chem. Soe.’ Ixxii. II. 534 (Abs.); ‘Beibliitter” xxi. 975 (Abs.) ‘ Astrophys. J.’ vi, 169-232. ‘ Astrophys J.’ vi. 233-238. ‘Astrophys. J.’ vi. 239- 243; ‘Beiblitter’ xxii. 153-154 (Abs.) °C. RY” cexxy. 705-7095 ‘Beibliitter, xxii. 219 (Abs.); ‘J. Chem. Soc.’ Ixxix. IT. 105 (Abs.) ‘ Bull. Soc. Chim.’ [3], xix. 54-57; ‘Chem. 1898, I. 550 (Abs.) ‘Bull. Soc. Chim.’ [3], xix. 57-58; ‘Chem. Centr.’ 1898, I. 549-550 (Abs.) ‘ Bull. Soc. Chim.’ [3], xix. 58-59; ‘Chem. News,’ Ixvii. 88-90. f ‘Gazz. chim. ital.’ xxviii. I. 81-153; ‘Chem. Centr.” 1898, I. 917 (Abs.) . Centr.” — Z. P. Bouman : Haschek. : A. L. Foley , _ B. Hasselberg H. Kayser = H.Konen ,. G. B. Rizzo , Widmark 4. E. Wiedemann v_ A. Maschek ,. C. Wf. Wolff . A. Hasterlik F. Exner and EF. ON THE BIBLIOGRAPHY OF SPECTROSCOPY. - | Emission und Absorption von Quarz und Glas bei verschiedenen Tem- peraturen. (Inaug. Dissert. Am- sterdam, 1897, 91 pp.) | Ueber die ultravioletten Funken- spectra der Elemente. X. (‘ Wien. Anz.’ 1897, 254.) - | Arc Spectra (‘Phys. Review,’ v. 129-152). Untersuchungen iiber die Spectra der Metalle im electrischen Flam- menbogen. IV. Das Spectrum des Mangans. (‘ Handl. Svensk. Vet. Akad.’ xxx. No. 8, 20 pp.) c Ueber die Bogenspectra der Ele- mente der Platingruppe (‘ Ab- handl. Akad. Berlin,’ 1897). . | Ueber dieSpectren des Iod. (Inaug. Dissert. Bonn, 72 pp.) Argon (‘ Atti Accad. Torino,’ xxxii. 50 pp.) -» | Im griinzen for det synliga spek- trum (‘Oefvers. K. Vet. Akad. Stockholm,’ liv. 287-309). - | Ueber Spectralerscheinungen (‘ Verhandl. Ges. Deutsch. Naturf. u. Aerzte,’ II. 1. Hiilfte, 66). dh ABSORPTION SPECTRA. 1886. Ueber eine spectroscopische Me- thode zum Nachweis des Blut- farbenstoffes (‘Pharm. Central- halle,” xxvii. 317-320, 326-330, 340-343). 1838, - | Ueber den spectroscopischen Nach- weis minimaler Blutmengen im Harn, sowie in anderen Fliissig- keiten (‘ Pharm, Centralhalle,’ viii. 637-639). 188). « | Kritische Studien iiber die bisheri- gen Methoden zum Nachweis fremder Farbstoffe im Weine. Cinaug. Dissert. Erlangen, 1889.) EMISSION SPECTRA, 1897—-ABSORPTION SPECTRA, 1886, 1888, 1889. ‘Zittingsverl. Akad. Am- sterdam,’ 1896-7, 438_ 442; ‘Beiblitter, xxi. 589 (Abs.) ‘ Beiblatter,’ xxii. [17] (title). ‘Beibliitter,’ xxii. 152 (Abs. ) ‘Beiblatter, xxii. [57] (title). ‘Beiblatter,’ xxii. [44] (title). ‘Beiblitter,’ xxii. [11] (title). ‘Beiblatter, xxi. [115] (title). ‘ Beiblitter, xxi. [111] (title). ‘Beiblatter, xxi. [85] (title). ‘Ber.’ xix. (Ref.), 584 (Abs.) ‘Ber’ xxi. (Ref.), 315 (Abs.) | ¢ Beibliitter’ xiv. 281 (title), AGA REPORT—1898. ABSORPTION SPECTRA, 1890, 1891, 1892, 1893. B. Hasselberg . | Untersuchungen tiber das Absorp- | ‘Handl. K. Svensk. Vet. tionspectrum des Broms. (Read | Akad, xxiv. No. 3, 53 pp. Oct. 8.) N. A. Monteverde. | Sur la chlorophylle. ‘ : . | ‘Ann. Agronom.’ xviii. | 268-270; ‘J. Chem. Soc.’ Ixii, 1155-1156 (Abs.) 1 1891. P. Dittrich . . | Ueber methiimoglobinbildende | ‘ Arch. f. exper. Pathol. u. | Gifte. (Oct.) Pharmakol.’ xxix. 247- | 281; ‘Ber.’ xxv. (Ref.), | 913 (Abs.) i 1892. H. Bertin-Sans and | Sur la formation de loxyhémoglo- | ‘C. R.’ cxiv. 923-926; ‘J. J. Moitessier. bine au moyen de l’hématine et | Chem. Soc.’ Ilxii. 1017 d'une matiére albuminoide. (Read | (Abs.) April 11.) A. H. Church . . | Researches on Turacin, an animal | ‘ Phil. Trans.’ clxxxiii. A. pigment containing copper. (Read | 611-530. April 28.) K. Olszewski and | Propriétés optiques de l’oxygéne | ‘ Bull. intermat. de l’Acad. A. Witkowski. liquide. (May.) Sci. de Cracovie, 1892, 340-3483 ; ‘ Naturw. Rund- schau,’ vili. 75 (Abs.); ‘Chem. Centralbl.’ 1893, I. 595 (Abs.); ‘J. Chem. Soc.’ Ixiv. II. 353 (Abs.) A. Brun. e. «| Note sur le spectre d’absorption | ‘Arch. de Genéve’ [3], des grenats almandines. (Read | xxviii. 410-412; ‘Zeit- July 7.) schr. f. Kryst. u. Min.’ xxiv. 621 (Abs.); ‘ Bei- blatter,’ xx. 31-32 (Abs.) S. Forsling . . | Om Absorptionspectra hos Didym | ‘ Bihang till K. Svensk. och Samarium i det ultravioletta | Vet. Akad. Handl.’ xviii. spektret. (Read Nov. 9.) I. No. 10, 32 pp.; ‘ Bei- blitter,’ xviii. 562 (Abs.) A. Gortz . . | Ueber spectrometrische Affinitiits- | ‘Beiblitter, xvii. [16] bestimmungen. (Diss. Tiibingcn, | (title). 1892, 574 pp.) H.Graebe . . | Unterschungen des Blutfarbstoffes | ‘ Zeitschr. f. anal. Chem.’ auf sein Absorptionsvermogen fiir | xxxili. 771-772; ‘Chem. violette und ultraviolette Strahlen. | News,’ lxxii. 9-11; ‘ Bei- | (Inaug. Dissert. Dorpat, 1892.) blatter,’ xx. 127 (Abs.) 1895. W. Ackroyd . . | On the Origin of Colour, Iodine | ‘Chem. News, Ixvii. 27, and JIodine Solutions. (Read |, 64-65, 111-112. Feb. 10.) G. Magnanini . | Intornoallaipotesi dellacolorazione | ‘ Rend. It. Acad. d. Lincei’ degli joni. (Read April 9.) [5], ii, I. sem. 369-376 ; ‘Zeitschr. f. physikal. Chem.’xii.56-62; ‘J.Chem. | | Soc,’ lxiv. If. 510 (Abs.) Ae pe A heer es ON THE BIBLIOGRAPHY OF SPECTROSCOPY. G. Magnanini and T. Bentivoglio. VY. Schumann. G. Kriiss and E. Thiele. G. B. Rizzo G. Hiifnmer Fs E. Schunck and L. Marchlewski. A. E. Garrod . J. M. Eder and E. Valenta. J. Janssen P, Sabatier . 1898. 465 ABSORPTION SPECTRA, 1893, 1894. Intorno allo spettro di assorbi- mento delle soluzioni di alcuni cromo-ossalati della serie bleu. (Read July 2.) Das Absorptionsspectrum des Bromsilbers bei steigender ‘Tem- peratur. Ueber die Lésungzustand des Iod, und die wahrscheinliche Ursache der Farbenunterschiede seiner Lésungen. (Jan). 1894. Sulle proprietaé delle linee e delle bande negli spettrid’assorbimento. (Jan.) Neue Versuche zur Bestimmung der Sauerstoffcapacitét Blutfarb- stoffs. (Feb.) Zur Chemie der (March.) Chlorophyll. A Contribution to the Study of the Yellow Colouring Matter of the Urine. (Received Feb. 5. Read April 26.) Absorptionsspectren von farblosen und gefirbten Glisern, mit be- sonderen Beriicksichtigung des Ultraviolett. (Read May 4.) Sur les spectres de l’oxygéne aux hautes températures. (Read May 7.) Spectres d’absorption du bromure cuivrique. (Read May 7.) ‘Rend. R. Accad. d. Lincei’ [5], ii. II. sem. 17-23 ; ‘Gazz. chim. ital.’ xxili. II. 444-451; ‘ Ber.’ xxvi. (Ref.), 926-927 (Abs.) ; ‘ Beiblatter,’ xvii. 926 (Abs.); ‘J. Chem. Soc.’ Ixvi. IT. 129 (Abs.); ‘Chem. News,’ Ixix. 157 (Abs.) ‘Jahrb. f. Photogr.’ vii. (1893), 160-165; ‘Bei- blatter,” xvii. 1060-1061 (Abs.) ‘ Zeitschr. f. anorg. Chem.’ vii. 52-81; ‘J. Chem. Soc.’ Ixvi. II. 445-446 (Abs.) ‘Il Nuovo Cimento,’ xxxv. 132-136; ‘Beiblitter,’ xviii. 836-837 (Abs.) ‘ Arch, f. Anat. u. Physiol. 1894, Physiol. Abth. 130-176. ‘Am. Chem. u. Pharm.’ celxxviii. 329-345; ‘J. Chem. Soc.’ Lsvi. I. 341- 342 (Abs.) ‘Proc. Roy. Soe.’ lv. 394— 407, ‘Denkschr. Akad. Wien,’ 1894, 285-295; ‘ Bei- platter, xix. 61-64 (Abs.) ‘OC. R, exviii. 1007-1009 ; ‘J. Chem. Soc.’ Ixvi. II. 337 (Abs.) ; ‘ Ber.’ xxvii- (Ref.), 278-279 (Abs.) ; ‘Beiblitter, xviii. 837— 838 (Abs.) *C. RY exviii. 1042-1045 ; ‘Ber.’ xxvii. (Ref.), 489- 490 (Abs.) ; ‘ Beibliitter,’ xvili. 838 (Abs.); ‘J- Chem. Soc.’ lxvi. IT. 504 (Abs.); ‘Chem. News,’ lxix.. 257-258 (Abs.) ; ‘Nature,’ 1. 72 (Abs.) Hi 466 P. Sabatier , H. Becquereland C. Brongniart. T. Ewan ® . Meckeand Wimmer A. E. Garrod . Fi C, Haacke , ‘ N. A. Monteverde . E. Schone E. Thiele A. Btaré tS .Schunck . M > . Etard . ° REPORT—1898. ABSORPTION SPECTRA, 1894, 1895. Spectres d’absorption des solutions bromhydriques de bromure cuiy- rique. (Read May 21.) La matié¢re verte chez les Phyllies, orthoptéres de la famille des Phasmides. (Read June 11.) On the Absorption Spectra of Dilute Solutions. (Read June 21.) Nachweise von Blutflecken. (Nov.) Heematoporphyrin in Normal Urine. Spectrophotometrische Untersuch- ungen iiber die Hinwirkung von Salzsiure auf einige Substitutions- producte des Fuchsins. (Diss. Tiibingen, 1894, 49 pp.) De la _ protochlorophylle (‘ Bot. Centralblatt,’ lix. 284). Absorption Spectrum of Ozone (Russ. Nat. and Phys. Congress, Moscow, 1894, No. 10.) 1895. Spectrophotometrische Untersuch- ungen der verschiedenfarbigen Iodlésungen, (Jan.) Pluralité des chlorophylles. Deux- iéme chlorophylle isolée dans la luzerne. (Read Feb. 11.) Contributions to the Chemistry of Chlorophyll. (Read Feb. 14.) Sur lorigine moléculaire des bandes absorption des sels de cobalt et de chreme. (Read May 13.) “CO. RY exviii. 1144-1146; ‘Chem. News,’ lxix. 275 (Abs.); ‘Ber.’ xxvii. (Ref.), 490 (Abs.); ‘Beibliitter,’ xviii. 1048 (Abs.); ‘J. Chem. Soc.’ Ixvi. IL. 373 (Abs.) ‘C. RY exvili. 1299-1308; ‘Chem. News,’ Ixix. 312 (Abs.); ‘Ber.’ xxvii. (Ref.), 517 (Abs.) ‘Proc. Roy. Soe.’ li. 117- 161. ‘Zeitschr. f. anal. Chem.’ xxxlv. 129-131; ‘Chem. News,’ lxxi. 238. ‘J. Physiol.’ xvii. 349-352; ‘J. Chem! Soe.’ Ixviii. II. ° 55 (Abs.) ‘ Beiblatter,’ xx. 64 (title). ‘Ann. Agronom.’ xxi. 90 (Abs.) ; ‘J. Chem. Soc.’ Ixvili. I. 429-430 (Abs.) ‘Chem. News,’ lxix. 289 (Abs.) ‘Zeitschr. f. physikal. Chem. xvi. 147-155; ‘ Beiblitter,’ xix. 426-427 (Abs.) ; ‘Proc. Phys. Soe.’ xiii. 113-114 (Abs.); ‘ Ber. xxviii. (Ref.), 720 (Abs.); ‘J. Chem. Soc.’ Ixviii. II. 193-194 (Abs.) °C. R. cxxe 328-331 oo, Chem. Soe.’ Ixviii. I. 389 (Abs.) ‘Proc. Roy. Soc.’ lvii. 314— 322. *C. RY cxx. 1057-1060; ‘Ber.’ xxviii. (Ref.), 592 (Abs.) ; ‘ Beibliitter,’ xix. 568 (Abs.); ‘ Proc. Phys. Soc,’ xiii. 310-311 (Abs.) ; ‘Chem. News,’ Ixxi. 269 (Abs.); ‘Nature,’ lii. 96 (Abs.) ; ‘J. Chem. Soc.’ Ixx, IT. 133 (Abs.) v ON THE BIBLIOGRAPHY OF SPECTROSCOPY. E. Merritt. . ° T, Ewan . J. Janssen , F BE. Aschkinass ; G. D. Liveing and J. Dewar. J. Pauer - . F. Hamburger 2 G. Magnanini : G. H. Bailey . - G. Kriiss and H, Kriiss. ABSORPTION SPECTRA, 1895. On the Absorption of Certain Crystals in the Infra-red, as de- pendent onthe Plane of Polarisa- tion: (May.) On the Absorption Spectra of Di- lute Solutions. (Read June 21.) Note sur la loi d’absorption des bandes du spectre de l’oxygeéne. (Read June 17.) Ueber das Absorptionspectrum des fliissigen Wassers und tiber die Durchlissigkeit des Augen- medium fiir rothe und ultrarothe Strahlen. (July.) Sur le spectre d’absorption de lair liquide. (Read July 15.) Ueber die Absorptionsspectra einiger Verbindungen im damp- formigen und fliissigen Zustand. | (Read July 7.) Ueber Farbenwechsel verdiinnter Lésungen von chromoxalsaurem Kali. (Aug.) Intornoallo spettro di absorbimento dialcuni cromosolfocianati. (Read Aug. 11.) The Spectrum of the Haloid £alts of Didymium. (Sept.) Hine neue Methode der quantita- tiven Spectralanalyse. (Sept.) 1 467 ‘Phys. Review, 1i.424—441 ; ‘ Beiblitter, xix. 694-695 (Abs.); ‘ Proc. Phys. Soc.’ xiii. 310 (Abs.) ‘Proc. Roy. Soc.’ lvi. 286- 287, lvii. 117-161; ‘ Ber.’ Xxvill. (Ref.), 411 (Abs.) ; ‘ Beiblatter,’ xviii. 998- 999, xix. 888 (Ahs.); ‘J. Chem. Soc.’ Ixviii. II. 433-434 (Abs.) ; ‘Nature,’ 1, 491 (Abs.) *C. R.’ cxx. 1306-1310; ‘Proc. Phys. Soc.’ xiii. 341- 342 (Abs.); ‘ Nature,’ lii. 303-304 (Abs.); ‘ Bei- bliitter,’ xx. 534 (Abs.) ‘Ann.Phys.u.Chem.’[N.F.], ly. 401-422 ; ‘ Nature,’ lii. 382 (Abs.); ‘ Froc. Phys. Soc.’ xiii, 436 (Abs.) °C.RY cxxi. 161-164; ‘ Bei- blitter, xx. 31 (Abs.); ‘Proc. Phys. Soc.’ xiii. 403 (Abs.); ‘Chem. News,’ Ixxii. 65 (Abs.) ; ‘Nature,’ lii. 312 (Abs.); * Ber.’ xxix. (Ref.), 63 (Abs.) | ‘Sitzungsb. phys. med. Soc. Erlangen, xxvii. 120-126; ‘Beiblitter, xx.696(Abs.); ‘Chem.Centr. 1896,’ 1.1122 (Abs.); ‘J. Chem. Soc’ xxii. II. 395 (Abs.) ‘Ann.Phys.u.Chem.’[N.F.], lvi. 173-174; ‘J. Chem. Soc.’ xx. II. 86 (Abs.) ‘Gazz. chim. ital.’ xxv. IT. 373-379 ; ‘ Beiblitter,’ xx. 695-696 (Abs.); ‘ Ber.’ xxix. (Ref.), 269 (Abs.) ; ‘J. Chem. Soc.’ Ixx. II. 345 (Abs.) ‘Brit. Assoc. Rep.’ 1895, 773; ‘ Beibliitter, xx. 31 (Abs.) ‘ Zeitschr. f, anorg. Chem.’ x. 31-43; ‘ Beiblitter,’ xe. 26) (CADS isle Brac: Phys. Soc.’ xiv. 14 (Abs.) ; ‘J. Chem. Soc.’ Ixx. lI. 215 (Abs.); ‘Ber.’ xxix. (Ref.), 147-148 (Abs ) HH 2 468 G. D. Liveing and J. Dewar. R. Mohlau and K. Uhlmann. B. Paulowski. . E. Schunck and L. Marchlewski. Lecoq de Eoisbau- dran. G. Kriiss = A. E. Garrod , J. Georgenburger . H, C. Poinsen = O. Postma . P. H. Bayrac and C. Camichel. L. Marchlewski BE. Schunck and L. Marchlewski. | REPORT—1898. ABSORPTION SPECTRA, 1895, 1896. On the Refraction and Dispersion of Liquid Oxygen, and the Absorp- tion Spectrum of Liguid Air. (Sept.) Zur Kenntniss der Chinazin- und Oxazinfarbstoffe. (Oct.) Ueber Allofluorescein. 14.) (Read Oct. Zur Chemie des (Oct.) Chlorophylls. Sur un élément, probablement nou- veau, existant dans les terbines. (Read Nov. 18.) Beziehungen zwischen Zusammen- setzung und Absorptionsspectrum organischen Verbindungen. Nach- trag. (Dec.) A Contribution to the Study of Uroerythrin. Hemoglobin and its Derivatives (‘Pharm. Zeitschr. Russ.’ xxxiv. 102-104). Ang-Khak,Chines Pilzfarbstoff zum Farben der Esswaaren. Einiges iiber Ausstrahlung und Absorption. (Inaug.-Diss. Am- sterdam, 1895, 94 pp.) 1896. Sur l’absorption de la lumiére par des dissolutions d’indophénole. (Read Jan. 27.) Die Chemie des Chloropbylls. (Hamburg, 82 pp.) (Jan.) Contributions to the Chemistry of Chlorophyll; Phylloporphyrin and Hematoporphyrin : a comparison. (Read Jan. 30.) ‘Phil. Mag.’ [5], xl. 268- 272; ‘J. Chem. Soc’ Ixvili. II. 471 (Abs.); ‘ Chem. News,’ lxxii. 154; ‘Ber.’ xxix. (Ref.), 110 (Abs.) ‘Ann. Chem. u. Pharm.’ cclxxxix. 128-130; ‘J. Chem. Soc.’ Ixx. I. 166- 169 (Abs.) ‘ Bex. xxviil. 2360-2362. ‘Ann. Chem. u. Pharm.’ celxxxix. 81-107; ‘J. Chem. Soc.’ Ixviii. I. 296— 297 (Abs.) ‘C. RY cxxi. 709; ‘ Bei- blatter, xx. 276 (Abs.) ; ‘ Nature,’ liii, 96 (Abs.) ‘Zeitschr. f. physikal. Chem.” xviii. 559-562 ; ‘Beiblitter,” xx., 197 (Abs.); ‘J. Chem. Soc.’ xx. II. 285 (Abs.) ‘J. Physiol.’ xvii. 439- 450; ‘J. Chem. Soc.’ Ixviii. I. 315-316 (Abs.) ‘Chem. GOentr.’? 1895, I. 701-702 ; ‘J. Chem. Soc.’ Ixx. II. 485 (Abs.) ‘Chemiker Zeitung, xix. II. 1311; ‘Chem. News,’ Ixxil. 105. ‘Beibliitter, xxii. 98 (Abs.) “C, R.. Cxyxigeig3—lone ‘Ber.’ xxix. (Ref.), 166 (Abs.); ‘J. Chem. Soe.’ Ixx. IL. 345-346 (Abs.) ; ‘Chem. News,’ lxxili. 95 (Abs.); ‘Nature,’ _liii. 335 (Abs.); ‘ Beibliitter, xxi. 740 (Abs.) ‘Chem. News,’ ]xxil'. 23 (Review). ‘Proc. Roy. Soc.’ lix. 233- 239. oe ON THE BIBLIOGRAPHY OF SPECTROSCOPY. A.Gamgee . A. Tschirch . ‘ A.Gamgee W. Spring. B, Tollens . . EK. Schunck and L. Marchlewski. A.Tschirch , B. Donath , WV. Agafonoff . A. &tard G. Eberhard . J.M.Eder , A. won Hiibl . A. Lumiére and L. Lumiére. E. Schunck and L. Marchlewski ABSORPTION SPECTRA, 1896. On the Absorption of the Extreme Violet and Ultra-violet Rays of the Solar Spectrum by Hemo- globin, its Compounds, and Certain of its Derivatives. (Read Feb. 13.) Der Quarzspectrograph und einige damit vorgenommene Untersuch- ungen von Pflanzenfarbstoife. (Read Feb. 28.) On the Relation of Turacin and Turacoporphyrin to the Colouring Matter of the Blood. (Read Mar. 19.) Sur la couleur des alcoéls com- parée 4 la couleur de eau. (Read March 7.) Ueber den Nachweis der Pentosen mittels der Phloroglucinsalzsiure-. absatzmethode. (Read April 18:) Zar Chemie des Chlorophylls. (Read May 11.) Zur Chemie des _ Chlorophylls. (Read Jane 22.) Bolometrische Untersuchungen liber Absorptionsspectra tiuores- cirender Substanzen und iitheris- cher Oele. (July.) Sur l’absorption du spectre ultra- violet par les corps cristallisés. (Read Sept. 28.) Les spectres des chlorophylles. (Read Nov. 16.) Die Schirmwirkung der Farben- sensibilisatoren, (‘ Photograph- ische Rundschau,’ x. 42-46, 76- 80). Die Wirkung von Farbensensibili- satoren bei orthochromatischen Platten. Die Schirmwirkung der Farben- sensibilisatoren. Ueber der Orthochromatismus Zur Chemie des Chlorophylls. (IV. Abhandlung.) 469 ‘Proc. Roy. Soc.’ lix. 276— 279; ‘Arch. de Genéve’ [3], xxxiv. 585-588; ‘Bei- blatter,’ xx. 650, 696-697 (Abs.); ‘Nature,’ liii. 478-479 (Abs.) ‘Ber. deutsch. bot. Ge- sellsch.’ xiv. 76-94 ; ‘Na- turw. Rundschau,’ xi. 240-241 (Abs.); ‘ Bei- blatter” xx. 535-536 (Abs.) ‘Proc. Roy. Soc.’ lix. 339- 342; ‘ Nature,’ liii. 574— 575. ‘Bull. Acad. Belg.’ [3], Xxxi. 246-256; ‘ Bei- blitter, xx. 535 (Abs.) ‘Ber.’ xxix. 1202-1209. ‘Ber.’ xxix. 1347-1352. ‘ Ber” xxix. 1766-1770. ‘Ann. Phys. u. Chem.’ [N.F.], lviii. 609-661; ‘Nature,’ liv. 455 (Abs.) °C. RY exxiii. 490-492 ; ‘Chem. News,’ Ixxiv. 204-205; ‘Arch. de Ge- néve [4], ii. 249-264; ‘ Beiblatter, xxi. 227- 228 (Abs.) *C. R.’ cxxiii, 824-828; ‘Beiblitter, xxi. 32 (Abs.) ‘Beiblatter, xx, 982 (Abs. ) ‘ Jahrb. f. Photog.’ x. 166— 167; ‘Beiblatter,’ xx. 981-982 (Abs.) ‘Jahrb. f. Photog.’ x. 289- 293; ‘Beiblatter, xx. 982 (Abs.) ‘ Jahrb. f. Photog.’ x. 146— 151; ‘Beiblitter, xx. 983 (Abs.) ‘Ann. Chem. u. Pharm.’ eexe. 306-313; ‘Ber,’ xxix. (Ref.), 415 (Abs.) REPORT—1898. ABSORPTION SPECTRA, 1896, 1897. M. Ransohoff . . | Ueber die Verteilung des Absorp- | tionsvermégens einiger einfach- erer Kohlenstoffverbindungen im ultraroten Gebiete des Spek- trums. (Inaug. Dissert. Berlin, 1896, 32 pp.) A. Tschirch Untersuchungen reiner Blattfarb- stoffe mit dem Quartzspectro- graphen : Beziehungen des Chlorophylls zum Blut. O. Wallach . Ueber das Absorptionsvermégen gewisser ungesiittiger Ketone fiir die violetten Lichtstrahlen. (‘Géttingen. Nachr.’ 1896, Heft 4, 1-5). E. Wiedemann and | Fluorescenz und Verbindungs- G.C. Schmidt. | spectra organischer Dimpfe. A. Wroblewsky ., AnwendungdesGlan’schen Spectro- | photometers auf die Tierchemie. I. Quantitative Bestimmung des Hamoglobins im Blute. II. Quan- titative Bestimmung der Rhodan- salze im Speichel (‘ Anz. Akad. Krakau,’ 1896, pp. 306-309, 386— 390). 1897. O. Lohse . Untersuchung des violetten Theils einiger linienreicher Metall- spectra. (Read Feb. 18.) Beitrag zur Kenntniss der Disper- sion und Absorption der ultra- rothen Strahlen in Steinsalz und Sylvin. (March.) The Additional Colouring Matters of Fucus vesiculosus. (March.) Dédoublement de la bande fonda- mentale des chlorophylles. (Read June 14.) H. Rubens and A. Trowbridge. C. Watson . A. Etard Die spectroscopische Blutunter- suchung. (June.) L. Lewin a B. J. Pauer. Absorption uJtravioletter Strahlen durch Dimpfe und Fliissigkeiten. (June.) Ueber die Absorption von ultra- rothen Strahlen in doppelbrech- enden Krystallen. (July. J. Konigsberger ‘ Beibliitter” xxi. 737-740 (Abs.) ‘Phot. Mittheil’ xxxii. 397-399. ‘Chem. Centr. 1897, i. 372-374; ‘ Beiblitter,’xxi. 633-634 (Abs.); ‘J. Chem. Soc.’ lxxiv. I. 194 (Abs.) ‘Jahrb. f. Photog.’ x. 14- 15. ‘Chem. Centr.’ 1897, ii. 532 (Abs.); ‘ Beiblatter,’ xxi. 573 (Abs.) | *Sitzungsb. Berl. Akad! 1897, 179-197 ; ‘ Nature,’ lvi. 62-63 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], lx. 724-739. ‘Nature,’ lv. 508. °C. R’ cexxiv. 1351-1354; ‘ Nature,’ lvi. 191 (Abs.); ‘ Beiblitter,’ xxi. 740-741 (Abs.); ‘Chem. Centr’ 1897, II. 207 (Abs.) ; ‘J. Chem. Soe.’ Ixxii. I. 575-— 579 (Abs.) ‘Arch. der Pharm.’ cexxxv. 245-255; ‘Chem. Centr.’ 1887, II. 381 (Abs.); ¢* J. Chem. Soc.’ Ixxii. II. 534 (Abs.) ‘Ann. Phys. u. Chem.’ [N-F-.], Ixi. 363-379. ‘Ann. Phys. u. Chem.’ [N.F.], Lxi. 687-704. ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 471 ABSORPTION SPECTRA, 1897—-PHYSICAL RELATIONS, 1884, 1887, 1888, 1889. G. Dimmer , Z. Donoginy . H. Haertes . J. Konigsberger J. Stscheglajew W. Spring H. Mercezyng. H, F. Weber . W. C. Rontgen G. Mengarini. Ueber die Absorptionsspectren von Didymsulphat und Neodidymam- monnitrat (‘Wien. Anz.’ 1879, 254). Die Darstellung des Hiimochromo- gens als Blutreaction, mit beson- derer Beriicksichtigung des Nach- weises von Blut im Harn. Differentialdiagnose zwischen Kohlendunst- und Leuchtgasver- giftung. (Inaug. Dissert. Berlin.) Ueber die Absorption von ultra- roten und ultravioletten Strahlen in doppelbrechenden Krystallen. (Inaug. Dissert. Berlin, 1897, 33 pp-) Dispersion anomale dans les solu- tions de fuchsine. Sur les spectres d’absorption de quelques corps organiques inco- lorés, et ses relations avec la structure moléculaire. (‘Arch. de Genéve’ [4], iii. 437-463.) TV, PHYSICAL RELATIONS. 1884. Sur les propriétés focales des ré- seaux. (In Russian.) 1887. Die Entwickelung der Lichtemis- sion gliihender fester Korper. (Read June 9.) 1888. Ueber den Hinfluss des Druckes auf die Brechungsexponenten von Schwefelkohlenstoff und Wasser (‘ Ber. oberh. Ges. f. Natur- und Heilkunde, Giessen, 1888, xxvi. 58-60). 1889. Ueber das Maximum der Licht- stiirke im Sonnenspectrum. (June.) ‘ Beiblatter,’ (title.) xxii. [17] ‘Arch. f. Anat. u. Physiol.’ exlvilil. 234-243; ‘J. Chem. Soc.’ Ixxii. II. 468 (Abs.) ‘Chem. Centr.’ 1897, II. 529 (Abs.) ‘Beiblatter,’ xxi. 414-416 (Abs.) ‘J. Russ. Phys. Chem. Soc.’ xxviii. II. 41-55; ‘ Bei- blitter,’ xxi. 409 (Abs.) ‘Bull. Acad. Roy. de Belg.’ [3], xxxili. 165-195; ‘Ree. des Trav. Chim. des Pays- Bas’ [2], xvi. 1-25; ‘Chem. Centr.’ 1897, I. 1114-1115, IT. 8-9 (Abs.); ‘J. Chem. Soc.’ Ixxiv. IT. 201 (Abs.); ‘ Beiblatter,’ xxi, 975-976 (Abs.) ‘Sitzungsb. d. Krakauer Akad.’ ix. 257-279; ‘J. Soc. Phys.-Chim. Russe,’ xv. 92-102; ‘ Beibliitter,’ viii. 121-122 (Abs.) ‘Sitzungsb. Akad. Berl, 1887, 491-504; ‘Bei- blatter,’ xvii. 1052-1054 (Abs.) ‘Untersuchungen zur Na- turlehre der Menschen und der Thiere,’ xiv. 119- 137; ‘Nature,’ xli, 374 (Abs.); ‘ Beiblatter,’ xiv. 376-377 (Abs.) 472 J. Trowbridge ‘ L. H. Siertsema R. Nasini and T. Costa. B. T. Geronyi . W. de W. Abney and E.R. Festing. F. Dussaud J.S. Ames , F. Maclean F. Zecchini V. Schumann. J M. Eder . REPORT—1898. PHYSICAL RELATIONS, 1890, 1891, 1892. On Electrical Oscillations in Air, together with the Spectroscopic Study of the Motions of Molecules in Electrical Discharges. (May.) Der Jamin’sche Interferentialrefrac- tometer und einige mit ihm ausge- fiihrten Brechungsindicesbestim- mungen. (Inaug. Dissert. Gron- ingen, 1890.) 1891, Ueber die Veriinderungen des Re- fractions- und Dispersionsverm6- gens des Schwefels in seinen Verbindungen. (Regia Universita degli Studi d. Roma. Instituto Chimico. Roma, Tipografia della R. Accad. d. Lincei, 1891, 147 pp.) Misura dell’ indice di rifrazione d’ un prisma. (Oct.) 1892. Colour Photometry. Part III. (Read Jan, 28.) Sur la réfraction et la dispersion du chlorate de soude cristallisé. (Read Feb. 4.) The Modern Spectroscope. I. The Concave Grating in Theory and Practice. (Feb.) Photographies spectrales obtenues avec un réseau de Rowland. (Read April 1.) Rifrazioni atomiche degli elementi rispetto alla luce gialla del sodio. (Read Sept. 4.) Ueber eine neue ultraviolettemp- findliche Platte, und die Photo- graphie der Lichtstrahlen klein- ster ‘Wellenliingen. (Read Noy. 10.) Ueber die Verwendbarkeit der Funkenspectrum verschiedener Metalle zur Bestimmung der Wel- lenlinge im Ultravioletten, mit Bezug auf das Spectrum des Son- nenlichtes, Drummond ’schen, Mag- nesium- und electrischen Bogen- lichtes. (Read Dec. 9.) ‘Proc. Amer. Acad.’ xxvi. 325 (title). ‘ Beibliitter,’ xiv, 801-803 (Abs.) ‘Beiblatter, xvii. 111-115 (Abs.) ‘ Riv. scient. industr.’ xxiii. 221-226. ‘Phil. Trans.’ clxxxili. A. 531-565. ‘Arch. de Genéve’ [3], xxvii. 380-405, 521-535; ‘Zeitschr. f. Kryst.u.Min.’ xxiv. 619-621; ‘Bei- blitter, xx. 23-24 (Abs.) ‘Astron. and Astrophys.’ xi, 28-42. ‘Séances de la Soc. franc. de phys.’ 1892, 165-166 ; ‘Beiblatter,’ xviii. 568 (Abs.) ‘Rend. R. Accad.d. Lincei’ (5), i. II. sem. 180-187 ; ‘Beiblitter,’ xvii. 115- 116 (Abs.); ‘Ber,’ xxv. (Ref.), 936 (Abs.) ‘Wien. Anz.’ xxix. Jahrg. (1892), 230-231 ; ‘Chem. News,’ Ixvi. 306 (Abs.) ‘Wien. Anz.’ xxix. Jahrg. (1892), 264-265. H. 0. G. Ellingen . W J. Macé de Lé- pinay. F. Paschen ¥. Zecchini J. H. Gladstone H. A. Rowland H. Ruoss ‘ J. W. Briihl . H. Kayser and C. Runge. G. Carrara « A. Ghira ° Th. Liebisch . H. A. Rowland 8. P. Langley THE BIBLIOGRAPHY OF SPECTROSCOPY. 473 PHYSICAL RELATIONS, 1892, 1893. Der Brechungsindex electrischer Strahlung in Alcohol. (Dec.) Sur la double réfraction du quartz (‘ Ann. Fac. des Sci. de Marseille,’ No. 1). 1893. Bolometrische Untersuchungen im Gitterspectrum. (Jan.) Sul potere rifrangente del fosforo. II. Potere rifrangente degli acidi del fosforo e dei loro sali sodici. (Read Jan 8.) Some Recent Determinations of Mo- lecular Refraction and Dispersion. (Read Feb. 10.) Gratings in Theory and Practice. Part I. (¥eb.) Bestimmung des Brechungsexpon- enten fiir Fliissigkeiten durch Spiegelablesung mit Fernrohr und Scala. (Feb.) Die Spectrochemie des Stickstoffs. (Vorlaufige Mittheilung.) (Read Mar. 25.) Die Dispersion der Luft. March 23.) (Read Influenza degli alogeni sul valore ottico dei doppi legami. (Read April 30.) Sulla refrazione atomica del boro. (Read April 9.) Ueber die Spectralanalyse der In- terferenzfarben optischzweiaxiger Krystalle. I. (April.) A New Table of Standard Wave- lengths. (April.) Latest Investigations with the Bo- lometer at the Astrophysical Ob- servatory of the Smithsonian Institution, (Read May 27.) ‘Ann. Phys. u. Chem, [N.F-.], xlviii. 108; ‘ Riv. scient. industr.’ xxv. 71 (Abs.) ‘J. de Phys.’ [3], i. 23-31 ; ‘ Beiblatter,’ xvi. 288-289 (Abs.) ‘Ann. Phys. u. Chem, [N.F.], xlviii. 273-306. ‘Rend. R. Accad. d. Lincei ’ [5], ii. I. sem. 31-38; ‘Gazz. chim. ital.’ xxiii. I. 109-120; ‘Ber.’ xxvi. (Ref.), 187-188 (Abs.) ‘ Proc. Phys. Soe.’ xii, 153- 160 ; ‘Chem. News, Ixvii. 94-95 (Abs.); ‘ Nature,’ xlvii. 429 (Abs.) ‘Astron. and Astrophys.’ xii. 129-149 ; ‘ Phil. Mag.’ [5], xxxv. 397-419. ‘Ann. Phys. u. Chem’ [N.F.], xlvili. 531-535; ‘Zeitschr. f. physikal., Chem.’ xi. 697 (Abs.) ‘Ber.’ xxvi. 806-809 ; ‘ Bei- bliatter, xvii. 740 (Abs.) ‘Abhandl. Akad. Berlin,’ 1893, 82 pp.; ‘ Nature,’ xlviii. 60 (Abs.) ‘Rend. R. Accad.d. Lincei ’ [5], ii. I. sem. 353-358 ; ‘ Beiblatter,’ xvii. 742-744 (Abs.) ‘Rend. R. Accad.d. Lincei’ (5], ii. I. sem. 312-319 ; ‘Gazz. chim. .ital.’ xxiii. I. 452-462; ‘Ber. xxvi. (Ref.), 573 (Abs.) ; ‘ Bei- blitter,’ xvii. 1047-1048 (Abs.); ‘J. Chem. Soc.’ lxiv. II. 517-518 (Abs.) ‘Gott. Nachr.’ 1893, 265- 266; ‘Beiblatter, xviii. 575-576 (Abs.) ‘Astron. and Astrophys. xii. 321-347. ‘Astron. and Astrophys.’ xiii. 41-44; ‘ Beiblatter,’ xviii. 709 (Abs.) , A74. F. Zecchini . C. Trapesonzjanz . K. Zimanyi . J. F. Eijkman L. E. Jewell . H, Krone . W. M. Watts . E. Lommel , R. Nasini . F. Zecchini , H. Dufet a G. Lippmann. A. A. Michelson REPORT—1898. PHYSICAL RELATIONS, 1893. Sopra un notevole caso di accresci- mento anomalo nel potere ri- frangente delle base feniliche. (Read May 21.) Ueber die Molecularrefraction stickstoffenthaltender Substanzen (Aldoxime und Ketoxime). (Read June 8.) Die Hauptbrechungsexponenten der wichtigeren gesteinbilden- den Mineralien bei Na-Licht. (July.) Recherches réfractométriques. (Aug.) An Absolute Scale of Intensity for the Lines of the Solar Spectrum and for Quantitative Analysis. (Aug.) Weiteres tiber Farbenphotogramme von Spectren. (Aug.) Wave-length Tables of the Spectra of the Elements and Compounds. (Report of the Committee.) (Aug.) Objective Darstellung von Inter- ferenzerscheinungen in Spectral- farben. (Sept.) Coefficiente critico in relazione colla formula (z—1)/d. (Read Sept. 3.) Sul potere rifrangente del fosforo. III. Potere rifrangente di alcune combinazioni organiche del fos- foro. (Read Oct. 1.) Sur les indices de réfraction du spath @’Islande. (Read Noy. 9.) Photographie des couleurs. (Read Nov. 3.) Light Waves and their Application to Metrology. (Nov.) ‘Rend. R. Accad. d. Lincei’ (5], ii. I. sem. 491-494; ‘Gazz. chim. ital.’ xxiii. II. 42-46; ‘Ber.’ xxvi. (Ref.), 863-864 (Abs.) ; ‘Beiblitter,’ xvii. 1048 (Abs.) ‘Ber.’ xxvi. 1428-1433; ‘ Beiblatter,’ xviii. 335- 336 (Abs.) ‘Zeitschr. f. Kryst. u. Min.’ xxii. 321-358; ‘Bei- blatter, xviii. 577-578 (Abs.) ‘Rec. des. trav. chim. des Pays-Bas, xiii. 13-33; 157-197 ; ‘J. Chem. Soc.’ lxvil. IT. 33, 65 (Abs.) ‘Astron. and Astrophys.’ xii. 815-821; ‘ Bei- blitter,’ xviii. 670 (Abs.) ‘ Phot. Mittheil’ xxx. 133 135, 148-150; ‘Bei- blatter,’ xviii. 192 (Abs.) ‘Brit. Assoc. Rep.’ 1893, 387-437, ‘Ann. Phys. u. Chem.’ [N.F.], 1. . 325-328 ; ‘ Nature,’ xlix. 46 (Abs.) *Rend.| B. Accadi> a: Lincei’ [5], ii. II. sem. 127-136; ‘Gazz. chim. ital” xxiii. \576—587% ‘Ber.’ xxvi. (Ref.), 928 (Abs.) ‘Rend. R.Accad. d. Lincei’ [5], ii. II. sem. 193-199 ; ‘Gazz. chim. ital.’ xxiv. I. 34-42; ‘Ber. xxvi. (Ref.), 929-930 (Abs.); ‘ Beiblatter, xviii, 454— 455 (Abs.); ‘J. Chem. Soe.’ lxvi. IT. 221 (Abs.) ‘Bull. Soc. frang. de Min’ xvi. 149-178; ‘Séances de la Soc. frang. de phys.’ 1894, 95-96; ‘ Beiblatter,’ xix. 638 (Abs.) * Séances de la Soc. fran¢. de phys.’ 1893, 248. ‘Nature,’ xlix. 56-60. a J. Joly » V. Berghoft J. F, Eijkman W. Zenker G. Lippmann R. Nasini J. Verschaffelt P. Bary . H. Dufet G. Gennari J. H. Littlewood G. Moreau ON THE BIBLIOGRAPHY OF SPECTROSCOPY. . R, Nasini and G. Carrara. 475 PHYSICAL RELATIONS, 1893, 1894. On the Influence of Temperature upon the Sensitiveness of the Photographic Dry Plate. (Read Dec. 20.) Bestimmung der Brechungsex- ponenten von Schwefel und Phos- phorlésungen im _ Schwefel- kohlenstoff nach der Prismen- methode mit Fernrohr und Scala. (Dissert Marburg. 1893.) Recherches réfractométriques Ueber die Entstehung der Farben im Lippman’schen Spectrum. 1894. Sur la théorie de la photographie des couleurs simples et composées par la méthode interférentielle. (Read Jan. 15.) Sul potere rifrangente dei composti contenenti il carbonile. (Read Jan. 13.) Application du réfractométre 4 Yétude des réactions chimiques. (Read Jan. 6.) Sur les indices de réfraction des dissolutions salines. (Read Feb. 2.) Indices du spath d’Islande. Dis- cussion des résultats. (Read Feb. 16.) Sul potere rifrangente dell’ alcool furanico, dell’ acido piromucico e dei suoi eteri. (Read Feb. 4.) Method for Determining the Refrac- tive Index of a Solution which is available when the Solution is not Homogeneous. (Read Feb. 23.) Dispersion rotatoire magnétique infra-rouge du sulfure de car- bone. (Feb.) Sul potere rifrangente dell’ ossigeno, dello zolfo, e dell’ azoto nei nuclei heterociclici. (Read Feb. 22.) , ‘Proc. Roy. Soc. Dubl.’ viii. (N.S.), 222; ‘Nature,’ xlix. 379 (Abs.) ‘Beiblatter, xviii. (title). [5] ‘Rec. trav. chim. des Pays- Bas,’ xii. 157-197, 268- 285; ‘J. Chem. Soc.’ Lxvi. II. 173 (Abs.) ‘Jahrb. f. Photogr.’ vii. (1893), 114-121; ‘ Beibliit- ter,’ xviii. 568 (Abs,) «OC, RY exviii. 92-102; «J. de Phys. [3], iii. 97-107. ‘Gazz. chim. ital.’ xxiv. I. 157-169; ‘J. Chem. Soc.’ Ixyi. II. 301-304 (Abs.) ‘Bull. Acad. Roy. de Belge,’ [3], xxvii. 49-84; ‘ Bei- blatter,’ xviii. 746-747, 833-834 (Abs.) ‘Séances de la Soc. frang¢. de phys.’ 1894, 78. ‘ Séances de lat Soc. franc. de phys.’ 1894, 95-96, ‘Rend. R. Accad. d. Lincei ’ [5], ili. I. sem. 123-129 ; ‘Gazz chim. ital.’ xxiv. I. 246-255; ‘J. Chem. Soc. Ixvi. II. 302 (Abs.); ‘ Ber.’ Xxvil. (Ref.), 426 (Abs.) ; ‘Beiblatter, xviii. 666 (Abs.) ‘Phil. Mag’ -[5], xxxvii. 467-470; ‘ Beibliitter,’ xviii. 905-906 (Abs.) ; ‘Proc. Phys. Soc.’ xiii. 74-76. ‘Ann. chim. et phys.’ [7], i. 227-258 5- “Natures xlix. 370 (Abs.) © Gazz. chim. ital.’ xxiy. I. 256-290; ‘J. Chem. Soc.’ Ixvi. II. 302-303 (Abs.); ‘ Ber.’ xxvii. (Ref.), 375-376 (Abs.); ‘ Bei- blatter,’ xviii. 834 (Abs.) 476 €. Runge A. Ghira = q G. B, Rizzo , ‘ A. Ghira % : H. Jahn and G. Moller. G. Gennari . A. Konig , W. de W. Abney K, Angstrém . A. Schuster , A. E. Tutton . L. Arons ; BF. Aymonnet. REPORT—1898. PHYSICAL RELATIONS, 1894. On a Certain Law in the Spectra of some of the Elements. (Feb.) Rifrazione atomica di alcuni ele- menti. Potere rifrangenti delle combinazioni organo-metalliche. (Read March 18.) Sull’ estensione della legge di Kirchhoff intorno alla relazione fra | assorbimento e l’emissione della luce. (Read March 11.) Potere rifrangente delle combina- zioni organo-metalliche. (Read April 15.) Ueber die dispersionsfreie Mole- cularrefraction einiger organ- ischer Verbindungen. (April.) Spettrochimica del cumarone e dell’ indene. (Read May 20.) Ueber die Anzahl der unterscheid- baren Helligkeitstufen und Spec- tralfarbentone. (May.) Measures of the Wave-lengths of Contrast Colours. (Read June 21.) Einige Bemerkungen anlisslich des bolometrischen Arbeiten von Fr. Paschen. (June.) On Interference Phenomena. (June.) Refractive Indices of the Sulphates of Potassium, Rubidium, and Cxsium. (Read June 7.) Ueber _ Dielectricititsconstanten fester und Brechungsexponenten geschmolzener Salze. (July.) Sur les radiations calorifiques com- prises dans la partie lumineuse du spectre. (Read July 2.) ‘Astron. and Astrophys.’ xiii. 128-130. ‘Rend. R. Accad. d. Lin- cei’ [5], ili. I. sem. 297-. 300, 332-3388; ‘ Gazz. chim, ital.” xxiv. I. 309- 327; ‘ Beiblatter,’ xviii. 906-907 (Abs.); ‘J. Chem. Soe.’ Ixvi. I. 415-~ 416 (Abs.) : ‘ Ber.’ xxvii. (Ref.), 377-378 (Abs.) ‘ Atti R. Accad. d. Torino,’ xxix. 424-433 ; ‘ Beiblat- ter, xviii. 835-836 (Abs.) ; ‘Nature,’ xlix. 606 (Abs.) ‘Rend. R. Accad. d. Lin- cei’ [5], iii. I, sem. 391- 393; ‘Gazz. chim. ital.’ xxiv. 324-327, ‘Zeitschr. f. physikal. Chem, xiii. 385-397; ‘ Ber.’ xxvii. (Ref.), 547 (Abs.) ; ‘ Beiblatter,’ Xvili. 831-833 (Abs.); ‘J. Chem. Soc.’ lxii. IT. 265 (Abs.); ‘ Nature,’ xlix. 582 (Abs.) ‘Rend. R. Accad. d. Lin- cei’ [5], iii. I. sem. 499- 503; ‘Gazz. chim, ital.’ xxiv. I. 468-474; ‘Bei- blatter,” xviii. 907 (Abs.) ‘Nature,’ 1. 192 (Abs.); ‘Ann. Phys. u. Chem’ [N.F.], liii. (Abhandl. phys. Ges.), 55 (Notice). ‘Proc. Roy. Soc.’ lvi, 221- 229; ‘Beiblitter, xix. 179-180 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], li. 6509-514; ‘Proc. Phys. Soe.’ xiii. 13 (Abs.) : ‘Phil. Mag.’ [5], xxxvii. 509-545. ‘J. Chem. Soe.’ Ixy. 666- (ire ‘Ann.Phys.u.Chem.’[N.F.], lili. 95-108 ; * Proc. Phys. Soc.’ xiii. 16 (Abs.) °C. R.’ cxix. 50-52; ‘ Bei- blitter,’ xviii. 908 (Abs.); ‘Chem. News,’ lxx. 62 (Abs.) ; ‘Nature,’ 1, 287 (Abs.) le be ON THE BIBLIOGRAPHY OF SPECTROSCOPY. H. Hallwachs ‘ C. Féry. . J. E. Keeler . S. P. Langley ta G. Moreau , ° F. Paschen . . ” . - G. J. Stoney . W. M. Watts . R. de Muynck H. Crew and R. Tatnall. I. Zoppellari . PHYSICAL RELATIONS, 1894, Ueber Lichtbrechung und Dichte verdiinnter Losungen. (July.) Application de l’autocollimation a4 la mesure des indices de réfrac- tion. (Read Aug. 13.) The Magnesium Spectrum as an Index to the Temperature of the Stars. (Aug.) On Recent Researches in the Ultra- red Spectrum. (Read Aug. 11.) Nouvelles recherches sur la région infra-rouge du spectre solaire. (Read Aug. 13.) De la périodicité des raies d’ab- sorption des corps _ isotropes. (Read Aug. 20.) Ueber die Dispersion des Fluorits im Ultraroth. (Aug.) Ueber die Dispersion des Stein- salzes im Ultraroth. (Aug.) Bolometrische Arbeiten. (Aug.) . On the Cause of the Spurious Double Lines sometimes seen with Spectroscopes, and the Slender Appendages which accompany them. (Aug.) Wave-length Tables of the Spectra of the Elements and Compounds. (Report of Committee.) (Aug.) Ueber die Brechungsexponenten von wasserigen Cadmiumsalzlé- sungen. (Sept.) On a New Method of Mapping the Spectra of Metals. (Oct.) Sulla rifrazione atomica del selenio. (Read Oct. 2.) A77 ‘Ann.Phys.u.Chem.’[N.F.], li. 1-133 ‘Nature,’ 1. 515 (Abs.) °C. RY cxix. 402-404. ‘ Astr. Nachr.’ exxxvi. 77— 80; ‘ Nature,’ 1. 364-365 (Abs.) ‘Brit. Assoc. Rep.’ 1894, 465-474; ‘Nature, li. 12-16 (Abs.) ‘C. R. cxix 388-392; ‘ Beiblitter,’ xviii. 1045— 1046 (Abs.); ‘Chem. News, Ixx. 114-115 (Abs.); ‘Nature,’ 1. 420 (Abs.) °C. RY cxix. 422-425. ‘Ann.Phys.u.Chem.’[N.F.], lili. 301-333; ‘Nature,’ 1. 635 (Abs.); ‘Proc. Phys, Soc.’ xiii. 14 (Abs.) ‘Ann.Phys.u.Chem.’[N.F.], lili. 337-342; ‘ Proc. Phys. Soc.’ xiii, 15 (Abs.) ‘Ann. Phys.u.Chem.’[N.F.], lili. 287-800; ‘Proc. Phys. Soe.’ xiii. 14 (Abs.) ‘Brit. Assoc. Rep.’ 1894, 583-585; ‘ Beibliatter,” xix. 423 (Abs.) ‘Brit. Assoc. Rep.’ 1894, 248-267, ‘Ann.Phys.u.Chem.’[N.F.], liii, 559-563; ‘ Ber. xxviii. (Ref.), 7 (Abs.); ‘J. Chem. Soe.’ Ixviii. IT. 33 (Abs.); ‘Proc. Phys. Soc,’ xiii. 12 (Abs.) ‘Phil. Mag.’ [5], xxxviii. 379-386. ‘Gazz. chim. ital.’ xxiv. IT. 396-407; ‘Rend.R.Accad. d. Lincei’ [5], iii, IT. sem. 330-338; ‘ Ber,’ xxviii. (Ref.), 54 (Abs.) ; ‘Beiblatter,” xix. 487~— 488 (Abs.); ‘J. Chem. Soc.’ Ixviii. II, 249-250 (Abs.) F. Paschen . V. Berghoft J. Violle 4 A. Belopolsky P. Bary . . B. Brunlhés , A. Hupe = A. A. Michelson E. Carvallo . E. L. Nichols. H. A. Rowland M. Camiche! REPORT—1898. PHYSICAL RELATIONS, 1894, 1895. Die Dispersion des Fluorits und der Ketteler’sche Theorie der Dis- persion. (Nov.) Bestimmung der Brechungsexpo- nenten von Schwefel- und Phos- phorlésungen nach der Prismen- methode mit Fernrohr und Scala. (Nov.) Sur la température de l'are élec- trique, (Read Dec. 3.) Ein Project zur Reproduction der Verschiebung von Spectrallinien bewegter Lichtquellen. (Dec.) Variation de V'indice de réfraction avec le degré de concentration des solutions aqueuses des sels. Sur la vérification des quartz paralléles. Bolometrische Arbeiten. Die Rotationsdispersion ultrarother Strahlen im Quartz. (Progr. Real- schule Charlottenberg, 1894, 48 pp-) Les méthodes interférentielles en métrologie, et 1 établissement dune longueur d’onde comme unité absolue de longueur. 1895. Spectres calorifiques. (Jan.) : The Distribution of Energy in the Spectrum of the Glow-Lamp. (Jan.) Preliminary Table of Solar Spec- trum Waye-lengths. I-X. (Jan.) Absorpticn de la lumieére dans les cristaux. (Read Feb. 15.) ‘Ann.Phys.u.Chem.’[N.F.], liii. 812-822. ‘Proc. Phys. Soe.’ xiii. 65 (Abs.) ‘Zeitschr. f. physikal. Chem.’ xv. 422-436; ‘ Ber. xxviii. (Ref.), 101-102 (Abs.); ‘ Beiblitter,’ xix. 327 (Abs.) ; ‘ Proc. Phys. Soc.’ xiii. 106 (Abs.) ; ‘J. Chem. Soc.’ Ixviii. II. 97 (Abs.) *C. RY’ exix. 949-950; ‘Chem. News,’ lxx. 306 (Abs.) 2 * Astr. Nachr.’ exxxvii. 34— 36; ‘Nature,’ li. 233-234 (Abs.) ; ‘ Beiblitter,’ xix. 418-419 (Abs.) ‘J. Soc. fran¢. de phys.’ 1894, 78. ‘J. de Phys.’ [3], iii, 22- 28; ‘Proc. Phys. Sos.’ xiii. 62-63 (Abs.) ‘Beiblitter? xix. 501-502 (Abs.) is ‘J. de Phys,’ [3], iii. 5-22; ‘Proc. Phys. Soc.’ xiii. 62 (Abs.) ‘Ann. de Chim. et Phys.’ [7], iv. 1-79; ‘ Beiblatter,’ xix. 566 (Abs.); ‘ Proc. Phys. Soc.’ xiii. 223-224 (Abs.) ‘Phys. Review,’ ii. 260- 276; ‘ Beiblatter, xix. 783-784 (Abs.); ‘Proc. Phys. Soc.’ xiii. 169 (Abs.) ‘Astrophys. J.’ i. 29-46, 130-145, 222-231, 295- 304, 360-369, 377-392; ii. 45-54, 109-118, 188- 197, 306-315, 377-392; ‘Beiblatter, xix. 422 (Abs.) ‘ Bull. Soc. frang. de phys.’ 1895, 50-56; ‘ Proc. Phys. (Soc! xl. sl6% (Abs.) ae aes _ A. Konig R. Neuhaus E. P. Lewis V. Schumann A. Konig Rubens. E. Merritt C. Runge A. Schuster _ F. Anderlini G. A. Borel P. T. Cléve Sir J. Conroy HH. Ebert . . and H. J. H. Gladstone and W. Hibbert. PHYSICAL RELATIONS, 1895. Ueber die Anzahl der unterscheid- baren Spectralfarben und Hellig- keitstreifen. (Feb.) Ueber die Photographie in natiir- lichen Farben. (Read Feb. 8.) The Infra-Red Spectra of the Elements. (Read Apiil 25.) Zur Photographie der Lichtstrahlen kleinster Wellenliingen vom Luft- spectrum jenseits 185°2 uu. (Read April 25.) Ueber die Energievertheilung im Spectrum des ‘Triplex-Gasbren- ners und der Amylacetatlampe. (Read May 10.) Ueber den Dichroismus von Kalk- spath, Quarz und Turmalin fiir ultrarothe Strahlen. (May.) Die Wellenliingen der ultraviolet- ten Aluminiumlinien. (May.) Sur les spectres cannelés. May 6.) Sopra alcuni questioni relative alla rifrazione atomica dell’ ossigeno. (Read June 17.) Recherches sur la réfraction et la dispersion des radiations ultra- violettes dans quelques substances cristallisées. (Read June 24.) Sur la densité de lhélium. June 4.) On the Refractive Index of Water at Temperatures between 0° and 10°. (Read June 20.) On the Electromagnetic Nature of | the Solar Radiation, and on a | New Determination of the Tem- perature of the Sun. (June.) The Molecular Refraction of Dis- solved Salts and Acids. (Read June 6.) (Read | (Read | ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 479 ‘Zeitschr. f. Psychol. u. Physiol. d. Sinnesorg.’ viii. 375-380; ‘ Bei- blatter,’ xix. 642 (Abs.) ‘Verhandl. Phys. Ges. Berl.’ xiv. 17-24; ‘Na- ture,’ li. 503-504 (Abs.) ‘Johns Hopkins Univ. Cire.’ xiv. 70 (Abs.); ‘Beiblitter, xix. 784 (Abs.) ‘Wien. Anz.’ 1895, xi. 121-122. ‘Verhandl. phys. Ges Berl.’ xiv. 51 (Notice) ‘ Nature,’ lil. 167 (Abs.) ‘Ann. Phys.u.Chem.’[N.F.], lv. 49-64; ‘Nature,’ lii. 189 (Abs:) ‘Ann. Phys.u.Chem.’[N.F.], ly. 44-48; ‘Nature,’ lii. 189 (Abs.) *C. RR’ exx. 987-989; ‘Nature, lii. 71 (Abs.) * Gazz. chim. ital.’ xxv. II. 127-162; ‘Ber. xxviii. (Ref.), 973-974 (Abs.); ‘J. Chem. Soc.’ lxx. II. 229-230 (Abs.) ‘Arch. de Genéve’ [3], xxxiv. 134-137, 230-249; *C. R. exx. 1404-1406 ; ‘ Beibliitter,’ xx. 42(Abs.); ‘Proc. Phys. Soc.’ xiii. 54 (Abs.) Ci Re (exx, 1212/5) “Na- ture,’ li. 586; ‘Chem. News,’ Ixxi. 201-202. Proc. Roy. Soe.’ Ilviii. 228-234; ‘ Nature,’ Iii. 455-456 (Abs.); ‘ Bei- bliitter,’ xix. 881 (Abs.) ‘Astrophys. J.’ ii. 55-57; ‘Nature,’ lii. 232 (Abs.) J. Chem. Soe.’ Ixvii. 831_- 868; ‘Proc. Chem. Soc.’ xi. 120-121 (Abs.); ‘Chem. News,’ Ixxi. 313 (Abs.); ‘ Beiblitter,’ xx. 195 (Abs.); ‘Ber, xxix. (Ref.), 265 (Abs.) 480 E. P. Lewis O. Wiener W. F. Edwards J. ¥. Eijkman F, Paschen H. Rigollot . J. Bernstein . J. H. Pillsbury W. le C. Stevens A. Witz. a Lord Rayleigh J. H. Gladstone G. D. Liveing and J. Dewar. W. M. Watts. REPORT—1898. PHYSICAL RELATIONS, 1895. The Measurement of some Standard Wave-lengths in the Infra-Red Spectra of the Elements, I. II. (June.) Farbenphotographie durch K6rper- farben und mechanische Farbenan- passung in der Natur. (June.) Some Notes on Molecular and Ato- mic Refraction. (July.) Recherches réfractométriques, (July.) Ueber Gesetzmiissigkeiten in den Spectren fester Korper, und tiber eineneue Bestimmung der Sonnen- temperatur. (Read July 6.). Action des rayons infra-rouges sur lesulfure d’argent. (Read July 15.) Das Beugungspectrum des querge- streiften Muskels bei der Contrac- tion. (Aug.) A Scheme of Colour Standards. (Aug.) Recent Progress in Optics (‘ Rep. Amer. Assoc.’) (Aug.) Kclairage par luminescence. (Read Aug. 5.) The Refraction and Viscosity of Argon and Helium. (Sept.) On Specific Refraction and the Periodic Law, with reference to Argonandother Elements. (Sept.) On the Refraction and Dispersion of Liquid Oxygen. (Sept.) Wave-length Tables of the Spectra of the Elements and Compounds (Report of Committee.) (Sept.) ‘Astrophys. J.’ ii. “1-25, 106-108; ‘ Beiblitter, xx. 28-29 (Abs.) ‘Ann. Phys. u. Chem,’ [N.F.], lv. 225-281; ‘Nature,’ lii. 279 (Abs.) ‘Amer. Chem. J.’ xvii. 473-506: ‘J.Chem. Soc.,’ Ixviil. II. 429-430 (Abs.) ‘Rec. Tray. Chim. des Pays-Bas,’ xiv. 185-202 ; ‘J. Chem. Soc.’ Ixx. II. 133 (Abs.) ; ‘ Ber.’ xxix. (Ref.), 73 (Abs.) ‘Nachr. Ges. Wiss. Gdét- tingen’ (1895), 294-304 ; ‘Proc. Phys. Soe.’ xiv. 44 (Abs.) *C. RY ecxxi. 164-166; ‘ Beiblitter,’ xix. 891- 892 (Abs.); ‘ Chem. News,’ lxxii. 80 ¢Abs.) ; ‘Proc. Phys. Soc.’ xiii. 397 (Abs.); ‘J. Chem. Soc.’ lxx. II. 3 (Abs:) ; ‘Nature,’ lii. 312 (Abs.) ‘Arch. f. d. gesammte Physiol. 1xi. 285-290; ‘Naturw. Rundschau, x. 540-541. ‘Nature,’ lii. 390-392. ‘Nature,’ liii. 233-238. Si@) ee * Chem. 104-105. ‘Brit. Assoc. Rep.’ 1895, 609 (Abs.); ‘ Chem. News,’ Ixxii. 224; ‘Chem. Centralbl.’ 1895, ii. 1112 ; ‘Beiblitter, xx. 192 (Abs.) ‘Brit. Assoc. Rep.’ 1895, 609-610; ‘Chem. News,’ Ixxli, 223-224. ‘Phil. Mag.’ [5], xl. 268- 272; ‘Chem. News, Ixxii. 154; ‘ Beiblitter,’ xx. 193 (Abs.); ‘Ber.’ xxix.(Ref.), 110 (Abs.) ‘Brit. Assoc. Rep.’ 1895, 273-340. exxi. 306-308 ; News,’ I xxii. Settee yeah ey ON A. Pfliiger . J. W. Bruhl A. A. Michelson A. de F. Palmer, jun. ¥. Paschen , W. H. Perkin F. Aymonnet : W. Hibbert H. A. Rowland KR. W. Wood . . KE. von Aubel. A. A. Michelson 1898, THE BIBLIOGRAPHY OF SPECTROSCOPY. PHYSICAL RELATIONS, 1895. Anomale Dispersionscurven einiger fester Farbstoffe. (Oct.) Ueber das .Wasserstoffhyperoxyd. Spectrometrische Bestimmungen, (Read Nov. 11.) The Broadening of Spectral Lines. (Nov.) On the Wave-length of the D, Helium Line. (Nov.) Ueber die Wellentliingenscala des ultrarothen Fliissspathspectrums. (Nov.) Influence of Temperature on the Refractive Power, and on the Re- fraction Equivalents of Acetyl- acetone and of Ortho- and Para- Toluidine. (Read Nov. 21.) Sur le déplacement spectrale du maximum calorifique __ solaire. (Read Dec. 30.) The Gladstone ‘ Law’ in Physical Optics, and the True Volume of | Liquid Matter. (Dec.) Preliminary Table of Solar Wave- lengths. XI-XV. (Dec.) Ueber die Absorptionsspectrum der Lésungen von Iod und Brom iiber der kritischen Temperatur. Sur les densités et les indices de réfraction des mélanges de l’alde- hyde ou de l’acétone avec l’eau, The Metre in Terms of Wave-length of Light. (Bureau Internat. des Poids et Mesures, xi. 1-237.) 481 ‘Ann. Phys. u. Chem. [N.F.], lvi. 412-432; ‘Nature,’ liii. 94 (Abs.) ; ‘Proc. Phys. Soc.’ xiii. 469 (Abs.) ‘Ber.’ xxviii. 2858-2860 ; ‘J. Chem. Soc.’ Ixx. II. 162-163 (Abs.) ‘ Astrophys. J.’ ii. 251-263. ‘ Amer. J. Sci.’ [3], 1. 357— 358 ; ‘ Phil. Mag.’ [5], xl. 547-548 ; ‘J. Chem. Soc.’ lxx. II. 405 (Abs.); ‘ Bei- blatter, xx. 197 (Abs.) ; ‘Chem. News,’ Ixxiii. 14 (Abs.) ; ‘ Nature,’ liii. 190 (Abs.); ‘Proc. Phys. Soc.’ xiv. 159 (Abs.) ‘Ann. Phys. u. Chem. [N.F.], lvi. 762-767. ‘J. Chem. Soe.’ Ixix. 1-6; ‘Chem. News,’ lxxii. 288 (Abs.) ; ‘ Beiblitter,’ xx. 529-530 (Abs.) ‘C. R. exxi. 1139-1141; ‘Nature, liii. 239 (Abs.) ; ‘Chem. News,’ lxxiii. 47 (Abs.) ; ‘ Beibliitter,’ xx. 537 (Abs.); ‘ Proc. Phys. Soc.’ xiv. 44 (Abs.) ©Phil. Mag.” [5], xl. 321— 345; ‘ Proc. Phys. Soc.’ xiii. 670-697 ; ‘ Bei- blatter, xx. 193-195 (Abs.) ‘Astrophys. J.’ iii, 141- 146, 291-296, 356-373 ; iv. 106-115, 278-287. ‘ Zeitschr. f. physikal. Chem.’ xix. 689-695 ; ‘ Phil. Mag,’ [5], xli. 423.. 431; ‘ Beiblatter, xx. 776 (Abs.); ‘J. Chem. Soc.’ Ixx. II. 458 (Abs.) ; ‘ Ber.’ xxix. (Ref.), 765 (Abs. ) ‘J. de Phys.’ [3], iv. 478_ 482; ‘ Beiblatter” xx. 195-196 (Abs.); ‘ Ber.’ xxix. (Ref.), 72 (Abs.) ‘Proc. Phys. Soc.’ xiv. (Abs.), 102. It A82 TV. Perreau , J. Stscheglajew P. Zeeman , J. HE. Keeler . 5 Lord Rayleigh B. Walter W. J. Humphreys and J. F. Mohler. M. Le Blane and P. Rohland. A. J. Moses and E. Weinschenk, J. N. Lockyer ¥. Perreau » - REPORT—1898. PHYSICAL RELATIONS, 1895, 1896. Etude expérimentale de la disper- sion et de la réfraction des gaz. Sur la dispersion anomale de la lumiére dans les solutions de fuchsine. Messung des Brechungsindex des gliihenden Platins (‘ Zittingsversl. Akad. Amsterdam,’ 1895, 116-119). 1896. Recent Researches bearing on the Determination of Wave-lengths in the Ultra-Red Spectrum. (Jan.) On some Physical Properties of Argonand Helium. (Read Jan. 16) Ueber des festen Fuchsins. die Brechungsexponenten (Jan.) Effect of Pressure on the Wave- lengths of Lines in the Are Spectra of Certain Elements. (Feb.) Ueber den Einfluss welchen die electrolytische Dissociation, der Wechsel des Aggregatzustandes und des Loésungsmittels auf das Lichtbrechungsvermégen einiger Stoffe austiben. (Feb.) Ueber eine einfache Vorrichtung zur Messung der Brechungsexponenten kleiner Krystalle mittelst Total- reflexion. (Feb.) The Shifting of Spectral Lines. I. (March.) Etude expérimentale de la dis- persion et de la réfraction des gaz. (March.) ‘J. de Phys.’ [3], iv. 411- 416; ‘Beiblitter, xx. 192-193 (Abs.); ‘ Proc. Phys. Soc.’ xiv. 160- 161 (Abs.) ‘J. de Phys.’ [3], iv. 546— 551; ‘ Beiblatter, xx. 272-273 (Abs.); ‘ Proc. Phys. Soc.’ xiv. 125-126 (Abs.) ‘ Beiblitter,’ xx.548 (Abs.) ‘ Astrophys. J.’ ili. 638- 7, ‘Proc. Roy. Soc,’ lix. 198— 208; ‘Zeitschr. f. physi- kal. Chem.’ xix. 364-372 ; ‘ Beibliitter, xx. 312-313 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], vii. 394-396 ; ‘Proc. Phys. Soc.’ xiv. 124-125 (Abs.) ‘ Johns HopkinsUniv.Cire. xv. 35-37; ‘ Beiblitter,’ xx. 533 (Abs.) ; * Proc. Phys. Soc.’ xiv. 282-283 (Abs.) ;_ ‘ Astrophys. J.’ iii. 114-137. > ‘Zeitschr. f. phggeen’ Chem.’ xix. 261-286 ; ‘ Beiblatter,’ xx. 364-365 (Abs.) ; ‘J. Chem. Soc.’ lxx. II.345 (Abs.) ; ‘Ber.’ xxix. (Ref.), 759-760 (Abs.) ‘ Zeitschr. f. Kryst. u. Min.’ xxvi. 150-155; ‘ Bei- blitter,’ xx. 872 (Abs.) © Nature,’ liii. 415-417. ‘Ann, Chim. et Phys.’ [7], vii. 289-348; ‘ Bei- blitter, xx. 643-645 (Abs.) nS a ON A. E. Tutton . : C. Viola i W.de W. Abney . W.N. Hartley G. Lippmann. bh . G. D. Liveing J. F. Mohler and L. E. Jewell. A, Schuster . W. H. Perkin J. H. Gladstone F.Paschen , A. E, Tutton. THE BIBLIOGRAPHY OF SPECTROSCOPY. PHYSICAL RELATIONS, 1896, Connection between the Atomic Weight of Contained Metals and the Crystallographical Characters of Isomorphous Salts. The Volume and Optical Relationships of the Potassium, Rubidium, and Cesium Salts of the Monoclinic Series of Double Sulphates, R,M(SO,)., 6H,O. (Read March 19.) Metodo per determinare I’ indice di rifrazione della luce di un mine- rale nelle lamine sottili. (Read March 15.) Note on Photographing Sources of Light with Monochromatic Rays. (Read April 30.) On the Temperature of Certain Flames. (Read April 23.) On Colour Photography by the Interferential Method. (Read April 23.) Colour Photography. (Lecture at Roy. Inst., April 17.) On Photographing the whole Length of a Spectrum at once. (Read April 27.) On the Wave-length of some of the Helium Lines in the Vacuum Tube, and of D, in the Sun. (April.) Note on the Results of Messrs. Jewell, Humphreys, and Mohler. (April.) On Magnetic Rotatory Power, es- pecially of Aromatic Compounds. (Read May 18.) The Relation between the Re- fraction of the Elements and their Chemical Equivalents. (Read June 4.) Ueber Gesetzmiissigkeiten in den Spectren fester Kérper. (June.) Vergleichung der Resultate der Untersuchungen tiber die ein- fachen und doppelten K, Rb und Cs enthaltenenen Sulphate, und daraus abgeleitete Schlussfolge- rungen iiber den Ninfluss des Atomgewichte auf die Krystallo- graphische EHigenschaften. (June.) A838 ‘J. Chem. Soc.’ Ixix, 344— 507. ‘Rend. R. Accad. d. Lineei’ [5], v. II. sem. 212-216 ; ‘Zeitschr. f. Kryst. u. Min.’ xxvii. 430 (Abs.); ‘ Beiblatter,’ xx. 874-875 (Abs.) ; ‘ Proc. Phys. Soc.’ xiv. 237-238 (Abs.) “Proc. Roy. Soc.) ls; 13— 5: ‘J. Chem, Soc.’ Ixix. 844- 847. ‘ Proc. Roy.Soc.’ lx. 10-13 ; ‘Chem. News,’ lxxiii. 213- 214, ‘Chem. News,’ Ixxiv. 275- 276, 285-286. ‘Proc. Phil. Soc. Camb.’ ix. 141-142; ‘ Beiblatter,’ xxi. 30 (Abs.); ‘ Nature,’ liv. 94 (Abs.) ‘Astrophys. J.’ iii. 351- 355; ‘Beiblitter,’ xxi. 336 (Abs.) ‘Astrophys. J.’ ili. 292; ‘Beiblitter, xxi. 706 (Abs.) ‘J. Chem. Soc.’ xix. 1025- 1257; ‘ Beiblatter, xxi. 254-256 (Abs.) ‘Proc. Roy. Soc.’ Ix. 140- 146; ‘ Beibliitter, xxi. 26-27 (Abs.) “Ann. Phys. u. Chem.’ [N.F.], lviii. 455-493. ‘Zeitschr. f. Kryst. uw. Min’ xxvii. 252-265; ‘Beiblitter, xxi. 196 (Abs.) 184. A. Hanke ; A. PAliiger C. Viola. A. Cotton a A. Konig F. Aymonnet . J. F. Mohler . E. }*. Nichols. W. J. Humphreys . W.J.Pope . H. Rubens ., J, $V bruh A. Hagenbach REPORT—1898. PHYSICAL RELATIONS, 1896. ‘Ueber die Refractionsiiquivalente | der Elemente. (Read July 2.) Zur anomalen Dispersion absor- birender Substanzen. (July.) Ueber eine Methode zur Bestim- mung des Brechungsvermogen der Mineralien im Diinnschliff. (July.) Recherches sur l'absorption et la dispersion de la lumiére par les milieux doués du pouvoir rota- toire. (Aug.) Quantitative Bestimmungen an complementiiren Spectralfarben. (Read July 20.) Sur les maxima périodiques des spectres. (Read Sept. 28.) The Effect of Pressure upon Wave- length. (Oct.) Das Verhalten des Quartzes gegen langwellige Strahlen, untersucht nach derradiometrischen Methode. (Read Oct. 22.) A further Study of the Effects of Pressure on the Wave-lengths of Lines in the Arc Spectrum of Certain Elements. (Nov.) The Refractive Constants of Crys- talline Salts. (Read Nov. 5.) Ueber das ultrarote Absorptions- spectrum von Steinsalz und Sylvin. (Read Nov. 6.) Stereochemisch-spectrische suche. I. (Dec.) Ver- Ein Versuch, die beiden Bestand- theile des Cléveitgases durch Diffusion zu trennen. (Dec.) ‘Sitzungsb. Akad. Wien,’ ev. Il.a, 749-777 ; ‘Wien. Anz,’ xxxili. 176 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], lviii. 670-673. ‘Min. petr.Mitth’” (Tscher- mak), xvi. 150-154; ‘Zeitschr. f. Kryst. u. Min,” xxvii. 430; ‘ Bei- blatter,’ xxi. 233 (Abs.) Ann. Chim. et Phys.’ [7], viii. 347-432; ‘J. de Phys.’ [3], v. 237-244, 290-303; ‘ Beiblitter,’ xx. 882-883, xxi. 35-36 (Abs.) Sitzungsb. Akad. Berl.’ 1896, 945-949. °C. BY exxiil. 645-647; ‘Chem. News,’ Ixxiii. 246; ‘ Beiblatter,’ xxi. 31 (Abs.) 3 ‘Astrophys. J. iv. 175- 181; ‘ Beiblitter, xxi. 737 (Abs.) . Sitzungsb. Akad. Berl.’ 1896, 1183-1196 ; ‘ Phys. Review, iv. 297-313; ‘Ann. Phys. u. Chem, [N.F.], lx. 401-417. Astrophys. J.’iv. 249-262. J. Chem. Soc.’ lxix. 1530- 1546; ‘ Proc. Chem. Soc.’ xii. | (1896),- S777 (Abs.); ‘Zeitschr. f. Kryst. u. Min’ xxviii. 113-134: ‘Chem. News, lxxiv. 268-269 (Abs.); ‘Chem. Centr.’ 1897, I. 3-4 (Abs.) ; ‘ Beiblitter,’ xxi. 347-348 (Abs.) ‘Verhandl. Phys. Soc. Ber- lin,’ xv. 108-110; ‘ Bei- blatter,’ xxi. 130 (Abs.) ‘Zeitschr. f. physikal. Chem?” xxi> 385-413; ‘ Beiblitter,’ xxi. 224-226 (Abs.) ‘Ann. Phys. u. Chem.’ (N.F.], lx. 124-133. “Ne H. Rubens and E. F. Nichols. J. F. Eijkman Vy. A. Julius. O. Wallach P. Zeeman J. W. Briihl . G. C. Comstock H. A. Rowland G. Tammann . J. Traube 2” THE BIBLIOGRAPHY OF SPECTROSCOPY. A8 Cx PHYSICAL RELATIONS, 1896, 1897. Ueber Wiirmestrahlen von grosser Wellenliinge. (Read Dec. 17.) Recherches réfractométriques Sur le quartz fondu, et les bandes dinterférence dans le spectre des fils de quartz. Ueber Refractions- und Disper- sionsvermégen einer Reihe iso- merer Kampfer (‘ Gdttingen. Nachr.’ 1896-69-73). Influence of Magnetism on the Light emitted by a Substance (‘Zittingsversl. Akad. Amsterdam,’ Oct. 31 and Noy. 21, 1896). 1897. Spectrometrische Bestimmungen. (Read Jan. 25.) Hydrazin, Wasserstofthyperoxyd, WV asser. (Read Jan. 25.) On the Application of Interference Methods to the Determination of the Effective Wave-length of Light. (Jan.) Preliminary Table of Solar Spec- - trum Waye-lengths. XVI. XVII. XVIII. (Jan.) Ueber die Aenderung der Brech- ungscoefiicienten bei der Neu- tralisation, der Bildung und Verditinnung von Lésungen. (Jan.) Ueber die Atomrefractionen von Kohlenstoff, Wasserstoff, Sauer- stoff und den Halogenen. (XVI. Abhandlung.) (Read Jan. 11.) Ueber die Atomrefractionen des Stickstoffs. XVII. Mittheilung. (Read Jan. 11.) On the Mode of Printing Maps of Spectra. (Discussion at the meet- ing of the Roy. Astron. Soc. on Jan &.) Sitzungsb. Akad. Berl.’ 1896, 1393-1400; ‘ Ann. Phys. u. Chem.’ [N.F.], lx. 418-462; ‘Phys. Re- view,’ iv. 314-323; ‘ Na- ture,’ lv. 329, 524 (Abs.) ‘Rec. trav. chim. des Pays- Bas,’ xv. 52-60; ‘ Bei- blatter,’ xxi. 27-28 (Abs.) ‘Arch. néerland. xxix. 454-466; ‘ Beibliitter,’ xx. 539 (Abs.) ‘ Beiblitter,’ xxi. 732-733 (Abs.) ‘Nature,’ lv. 192, 347, 370 (Abs.) “Ber.” . Xxx: 158-162 ; ‘Chem. Centr.’ 1897, I. 534 (Abs.) ; ‘ Beibliitter,’ xxi. 511 (Abs.) ‘Ber.’ xxx. 162-172; ‘ Bei- blatter, xxi. 407-409 (Abs.) ‘ Astrophys. J.’ v. 26-35 ‘Beiblitter, xxi. 52 (Abs.); ‘Science Abstr i. 12 (Abs.) ‘Astrophys. J. v. 11-2F 109-118,181-193 ; ‘ Phys Review,’ v. 11-25. ‘Zeitschr. f. physikal. Chem.’ xxi. 537-544; ‘Beiblatter,’ xxi. 969- 970 (Abs.) ‘ Ber.’ xxx. 39-42 ; ‘Chem. Centr.’ 1897, I. 403-404 (Abs.) ‘ Ber.’ xxx. 43-47; ‘Chem. Centr.’ 1897, I. 404 (Abs.) ‘ Astrophys. J. vy. 216-217 (Abs.) 486 F. Zecchini . F.G. Kohl . O. J. Lodge J. B. Hayeraft F.Paschen . ; P. Zeeman . : J. W. Briihl . P.deHeen , N. Egoroff and N. Géorgiewsky. G.LeBon . A, E. Tutton . ¥. L. O. Wadsworth | W. H. Wright . | . | Spectrochemie des Stickstoffs. REPORT—1898. PuHysicA", RELATIONS, 1897. Sul potere rifrangente delle mes- colanze di due liquidi. (Read Jan. 8.) Die assimilatorische Energie der blauen und violetten Strahlen des Spectrums. (Read. Feb. 26.) The Influence of a Magnetic Field on Radiation Frequency. (Read Feb. 11.) Luminosity and Photometry. (Read March 4.) Ueber Gesetzmiissigkeiten in der Spectren fester Kérper. (March.) On the Influence of Magnetism on the Nature of the Light emitted by a Substance. (March.) Vv. (April.) Détermination de la partie du spectre qui développe la plus grande proportion d’infra-électri- cité. (Read April 5.) Sur la polarisation partielle des radiations émis par quelques sources lumineuses sous l’influence du champ magnétique. (Read May 3.) Sur les propriétés de certainesradia- tions du spectre. (Read May 24.) Connection between the Crystal- lographical Characters of Isomor- phous Salts and the Atomic Weight of the Metals contained. A com- parative crystallographic study of the normal selenates of potassium, rubidium, and cesium. (Read May 20.) On the Resolving Power of Tele- scopes and Spectroscopes for Lines of Finite Width. (May.) A Method of correcting the Curva- ture of Lines in the Spectrohelio- graph. (May.) ‘Gazz. chim. ital.’ xxvii. 358-383 ; ‘Chem. Centr.’ 1897, I. 1193 (Abs.); ‘Beibliitter, xxi. 732 (Abs.); ‘J. Chem. Soc.’ lxxii. II. 470 (Abs.) ‘Ber. Deutsch. Bot. Ges.’ xv. 111-124; ‘Chem. Centr.’ 1897, I. 867 (Abs.) ‘Proc. Roy. Soc.’ Ix. 513- 514. ‘Proc. Roy. Soc.’ lxi. 49 50; * Beibliitter,’ xxi. 972 (Abs.); ‘ Nature,’ lv. 525 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], Ix. 662-723 ; ‘Nature,’ liv. 311 (Abs.) ‘Phil. Mag.’ [5], xliii. 226- 239; ‘Astrophys. J’ v. 332-347. ‘Zeitschr. f. physikal. Chem.’ xxii. 373-409 ;‘ J. Chem. Soc.’ Ixxii. II. 297 (Abs.) ; ‘ Beibliitter,’ xxi. 586-588 (Abs.); ‘ Chen. Centr.’ 1897, II. 81-83 (Abs.) ‘Bull. Acad. Belg.’ [3], Xxxlli. 321-323; ‘ Bei- blitter, xxi. 651 (Abs.) ‘C. R. cxxiv. 949-951 ; ‘ Beibliitter, xxi. 645- 646 (Abs.) °C. R, exxiv. 1148-1151. ‘J. Chem. Soc.’ lxxi. 846-— 920; ‘Proc. Chem. Soc, xiii. 115-118 (Abs.); ‘Chem. Centr.’ 1897. II. 12, 562 (Abs.) ; ‘ Beibliit- ter,’ xxii. 84-85 (Abs.) ‘Phil. Mag.’ [5], xliii. 317- 343. ‘Astrophys. J.’ v. 325- 327; ‘Beibliitter,’ xxii. 98 (Abs.) 8S. Abati = A. St. C. Dunstan, M. E. Rice, and C. A. Kraus. J. H. Gladstone and W. Hibbert. W. Huggins and F. W. Very. 0. J. Lodge A. Lumiére and L. Lumiére. C. F. Mabery and E. J. Hudson. D. W. Murphy J. S. Ames and W.J. Humphreys W. J. Humphreys . F. L. O. Wadsworth P. Zeeman. . N. Egoroff and N. Géorgiewsky. THE BIBLIOGRAPHY OF SPECTROSCOPY. PHYSICAL RELATIONS, 1897. Sul potere rifrangente e dispersivo del silicio nei suoi composti. (Read June 12.) Preliminary Note on the Broaden- ing of the Sodium Lines by Intense Magnetic Fields. (June.) The Molecular Refraction of Dis- solved Salts and Acids. II. (Read June 17.) On the Mode of Printing Maps of Spectra and Tables of Wayve- length. (June.) Further Note on the Influence of a Magnetic Field on Radiation Fre- quency. (Read June 3.) Application de la photographie 4 la mesure des indices de réfraction. | (Read June 21.) Refractive Power of Hydrocarbons (from Petroleum) and their Chlo- rine Derivatives. (June.) Spectral Photometry. (June) Note on the Effect of Pressure upon the Series in the Spectrum of an Element. (June.) Changes produced by Pressure in the Wave Frequencies of the Lines of Emission Spectra of Elements. (June.) Tables of the Resolving Power of Spectroscopes. (June.) Lignes doubles et triples dans le spectre, produites sous l’influence dun champ magnétique extérieur. (Read June 21.) Ueber Doublets und Triplets im Spectrum,verursacht durch iiussere magnetische Kriifte. I. II. (‘Zit- tingsversl. Akad. Amsterdam,’ 1897, 13-18, 99-102.) (June.) Sur la polarisation partielle des radiations lumineuses sous l’influ- ence du champ magnétique. (Read July 5.) 487 ‘Gazz. chim. ital.’ xxvii.; Il. 437-455; ‘Chem. Centr. 1898, I. 437-455. ‘Amer. J. Sci.’ [4], iii. 472-474; ‘ Beiblatter,’ xxi. 767 (Abs.) ‘J. Chem. Soc.’ Ixxi. 822- 833; ‘ Beiblatter, xxi. 966 (Abs.); ‘Chem. Centr. 1897. II. 459 (Abs.) * Astrophys. J.’ vi. 55-57. | «Proc. Roy. Soe.’ lxi. 415- 415; ‘Nature, lvi. 237- 238. °C. RY” exxiv. 1438-1440: ‘Beiblitter, xxi. 965 (Abs.); ‘Nature, Ivi. 216 (Abs.) ‘Amer. Chem. J.’ xix. 482— 485; ‘J. Chem. Soc.’ Ixxii. I. 451-452 (Abs.) ; ‘Chem. Centr.’ 1897, II. 259 (Abs.) ‘Astrophys. J.’ vi. 1-21; ‘Science Abstr. i. 10 (Abs.) ‘Johns Hopkins Univ. Cire.’ xvi. 41-42; ‘ Phil. Mag.’ [5], xliv. 119-122 ; ‘Chem. News,’ lxxvi. 21— 22; ‘Beiblitter, xxi. 974-975 (Abs.); ‘Chem. Centr.’ 1897, II. 524 (Abs.) ‘Johns Hopkins , Univ. Circe.’ xvi. 43-44; ‘ Bei- blatter,’ xxii. 219-221 (Abs.) ‘ Astrophys. J.’ vi. 27-36. °C. RY exxiv. 1444-1445. ‘Phil. Mag. [5], xliv. 55— 60; 255-259; iC. Re exxiv. 1444-1445; ‘ Bei- blitter,’ xxi. 765-767 (Abs.) ©C., Rep pexxva gkGeliy ‘Beiblitter, xxi. 899- 900 (Abs.) 488 J, Konigsberger C.E.Mendenhalland | F, A. Saunders. J. H. Pillsbury J. Larmor W. Ramsay and M. W. Travers. A. Schuster . W. M. Watts W. Konig P.Zeeman ., A. Cornu ; W. J. Humphreys . A. A. Michelson A, Cotton , H. A. Rowland A. Cotton , 5 W. Ramsay and M. W. Travers. REPORT—1898. PHYSICAL RELATIONS, 1897. Ueber die Absorption von ultra- rothen Strahlen in doppelbrechen- den Krystallen. (July.) Preliminary Note on the Energy Spectrum of a Black Body. (July.) Spectrum Colour Standards. (July.) The Influence of Pressure on Spec- tral Lines. (Aug.) On the Refractivity of Certain Mix- tures of Gases. (Aug.) Constitution of the Electric Spark. (Aug.) Wave-length Fables of the Spectra ef the Elements and Compounds. (Report of Committee.) (Aug.) Beobachtung Phinomers. des (Sept.) Doublets and Triplets in the Spec- trum, produced by External Mag- netic Forces. (Sept.) Sur l’observation et l’interprétation | cinématique des phénoménes dé- couverts par M. le Dr. Zeeman. (Read Oct. 18.) Changes in the Wave Frequencies of the Lines of Emission Spectra of Elements; their dependence upon the elements themselves and upon the physical conditions under which they are produced. | (Oct.) Optical Radiation in a Maenetic Field. (Oct.) Procédé simple pour constater le changement de période de la lumi- ére du sodium dans un champ magnétique. (Read Noy. 29.) Corrections and Additions to Pro- fessor H. A. Rowland’s Table of Solar Spectrum Wave-lengths. (Nov.) Sur la polarisation de la lumiére émise par une flamme de sodium placée dans un champ magnétique. (Read Dec. 17.) On the Refractivities of Air,Oxygen, Nitrogen, Argon, Hydrogen, and Helium. (Read Dec. 9.) Zeeman’schen ‘Ann. Phys. u. Chem,’ [N.F.], Ixi. 687-704; ‘Science Abstr.’i. 7(Abs.) ‘Phil. Mag.’ [5], xliv. 136 ; ‘ Beiblatter, xxi. 733 (Abs.) ‘Science’ [2], vi. 89-91 ; ‘Beiblatter, xxi. 972 (Abs.) ‘ Brit. Assoc. Report,’ 1897, 555-556. ‘ Brit. Assoc. Report,’ 1897, 587-588 (Abs.) ‘ Brit. Assoc. Report,’ 1897- 550; ‘ Electrician,’ xxxix. 585 (Abs.); ‘ Beibliitter,’ xxi. 1011 (Abs.) ‘ Brit. Assoc, Report,’ 1897, 75-127. ‘Ann. Phys. u. Chem [N.F.], Ixii. 240-248. ‘Phil. Mag. [5], xliv. 55- 60. °C. RJ exxv. 555-561: ‘Science Abstr.’ 1. 8-9 (Abs.) ‘Astrophys. J. vi. 169- 232; ‘Science Abstr.’ i. 11-12 (Abs.) | ‘Astrophys. J.’ vi. 48-54; ‘Science Abstr’ i. 9 (Abs.) ‘C. R.’ cxxv. 865-867. ‘Astrophys. J.’ vi. 324— 392. °C. BR.’ exxy. 1169-1172. ‘Proc. Roy. Soc.’ lxii. 225- 232; ‘Chem.Centr.’ 1898, J. 429-430 (Abs.); ‘ Bei- bliitter,’ xxii. 217 (Abs.) ON THE BIBLIOGRAPHY OF SPECTROSCOPY. A. Broca . B. Dijken J. Ehlers O. Kamerlingh K.R. Koch . W. Konie . M. Konowalow W. A. Kowalewski . E. Prior. 5 H. Rubens V. Schumann E.G. A. ten Siethoft PHYSICAL RELATIONS, 1897. Les variations de période des raies spectrales (‘Rev. générale des Sciences,’ viii. 955-939). Die Molecularrefraction und Dis- persion einiger wasserigen Salz- lédsungen in Zusammenhang mit der Dissociation. (Inaug. Dissert. Groningen, 1897, 67 pp.) Die Absorption des Lichtes in eini- | gen pleochroitischen Krystallen. | (Inaug. Diss. Géttingen.) (‘ Neues Jahrb. f. Min. u. Geol.’ (Beilage), xi. 259-317. Een Brief van Prof. E, van Aubel betrekking hebbende op de proeven van den Heer Ch. Fiévez over de werking van het magnetisme op den aard der Spectra (‘Zittings- versl, Akad. Amsterdam,’ v. 356- 359). Ueber das Verhalten der Dielectri- citiitsconstante und des Brech- ungsexponenten im magneti- schen Felde. Einfache Demonstration des Zee- man’schen Phiinomens. Données concernant le pouvoir réfringeant des combinaisons azo- tées. Sur le volume atomique et la ré- fraction atomique des chlorures des acides alkyle-phosphoreux. Ueber H. Tornée’s spectrometrisch- ariiometrischen Bieranalyse mit Hilfe des Differentialprisms von W. Hallwachs (‘ Forsch. Ber. tiber Lebensm. u. ihre Bez. z. Hyg,’ iv. 304.) Ueber Wirmestrahlen von grosser Wellenliinge. (‘ Verhandl. Ges. Deutsch. Naturf. u. Aerzte,’ 1i. 54— 56). Von den brechbarsten Strahlen und ihrer Photographiren-Aufnahme. Verklaring van het doer Dr. P. Zee- man gevonden lichtverschijnsel in het oog (*Zittingsversl. Akad., Amsterdam,’ v. 351-355), | 489 ‘Beiblitter, xxii. [29] (title). ‘Zeitschr. f. physikal. Chem.” xxiv. 81-113; ‘Chem. Centr.’ 1897, I. 383 — 384 (Abs.); ‘ Bei- blitter,” xxi. 333, 970- 971 (Abs.) ‘ Beiblatter, xxii. 157-159 (Abs.) ‘Beiblitter,. xxi. [89] (title). ‘Ann. Phys. u. Chem.’ [N.F.], Ixiii, 132-136. ‘Ann. Phys. u. Chem.’ [N.F.], lxiii. 268 — 272; ‘ Nature,’ lyii. 402 (Abs.) ‘J. Russ. Phys. Chem. Soc.’ xXXvii.412-421 ; ‘ Zeitschr. f, physikal. Chem.’ xxiii. 553-554; ‘ Beibliitter,’ xxi. 966-968 (Abs.) ‘J. Russ. Phys. Chem. Soc.’ xxix. 217-222; ‘Chem. Centr.’ 1897, IL. 3338-334 ; ‘ Beibliitter,’ xxi, 968- 969 (Abs.) ‘Chem. Centr.’ 1898, I. 138. ‘ Beibliitter,’ (title). xX. [85} ‘Jahrbuch f. Photog.’ xi, 24-25. ‘Beibliitter,’ (title). xe [39] 490 REPORT—1898. PHYSICAL RELATIONS, 1897—FLUORESCENCE, 1887, 1895. J. Stscheglajew H. T. Simon . C. Soret, A. Borel, and E. Dumont. F. Swartz . c H. Torné6e . inh (ERM Oy worth. Wads- G. Weiss » « P. Zeeman . c ” ‘ Z. P. Bouman . K. Noack : F M. Berthelot . Dispersion anomale dans les solu- tions de fuchsine. Ueber ein neues photographischen Photometrirverfahren, und seine Anwendung auf die Photometrie des ultravioletten Spectralge- bietes. Ueber die Brechungsindices der blauen und griinen Lésungen von Chromalaunen (‘Arch. de Ge- néve,’ 1897, iv. 376-381). Ueber den Atomrefractionsindex des Fluors’ (‘ Bull. Akad. Belg.’ [3], xxxiv. 293-307). Spectrometrisch - ardometrische Bieranalyse (‘ Pharm. Centr.-H.’ XXxvili. 871-873). Sur le pouvoir séparateur des lu- ettes et des spectroscopes pour les raies de largeur finie. Mesure des indices de réfraction Ueber Doublets und Triplets im Spectrum, verursacht durch dus- sere magnetische Krifte. — III. (‘ Zittingsversl. Vet. Akad. Amster- dam,’ 1897, 260-262.) Measurements concerning Radia- tion Phenomena in the Magnetic Field. . (‘ Zittingsversl. Vet. Akad. Amsterdam, 1897, 408-411). Emission und Absorption von Quarz und Glas bei verschiedenen Tem- peraturen. (Inaug. Dissert. Am- sterdam, 1897, 91 pp.) Vv. FLUORESCENCE. 1887. Verzeichniss fluorescirender Sub- stanzen, nach der Farbe des Fluo- rescenzlichtes mit Literatur- nachweisen (‘Schriften d. Na- turf.-Gesellsch. Marburg,’ xii. 155 Ppp.) 1895. Observations sur Yargon; spectre de fluorescence. (Read April 16.) ‘J. Russ. Phys. Chem. Soc.’ xxviii. II. 41-55; ‘ Bei- blatter,’ xxi. 409 (Abs.) ‘ Jahrb. f. Photogy.’ xi. 38- 55. ‘ Beiblitter,’ (Abs.) x1,” Saffoll ‘Chem. Centr.’ 1897, II. 1042-1044 (Abs.) ; ‘ Bei- blatter,’ xxii. 150-151 (Abs.) ‘Chem. Centr. 1898, I. 270-271. | «J. de Phys, [3], vi. 409- 425. ‘J. de Phys.’ [3], vi. 681 - 690. 167 ‘Beiblitter’ xxii. (Abs.) ‘Phil. Mag,’ [5], xlv. 197— 442; ‘Beibliatter, xxii. 167 (Abs.) ‘ Zittingsversl. Akad, Am- sterdam,’ 1896-7, 438- 422; ‘Beibliitter,’ xxi. 589 (Abs.) ‘Beiblatter, xii. 86 (Notice). “GR. oCxx, ae e00r ‘ Ber.’ xxviii. (Ref.), 409- 410 (Abs.) ; ‘ Beiblatter,’ xix. 567 (Abs.); £J.Chem. Soc.’ Ixviii. II. 337-338 (Abs.); ‘Chem. News,’ Ixxi. 212-213; ‘ Nature,’ li. 622 (Abs.) a a id ON THE BIBLIOGRAPHY OF SPECTROSCOPY. A91 FLUORESCENCE, 1895, 1897--ASTRONOMICAL APPLICATIONS, 1891, 1892. _ MM. Berthelot . E. Dorn and H. Erdmann. E. Wiedemann and G. C. Schmidt. » ” . H. Krone - C. Dunér . A. M, Clerke. ~ Nouvelles études sur la fluores- cence de l’argon, et sur sa combin- aison avec les éléments de la benzine. (Read June 24.) Ueber das von Berthelot beschrie- bene Fluorescenzspectrum des Argons. (July.) Ueber Luminescenz von festen K6rpern und festen Lésungen. (Oct.) Fluorescenz des Natrium- und Ka- lium - Dampfes, und Bedeutung dieser Thatsache fiir die Astro- physik. (Read Nov. 12.) Fluorescenz und Verbindungs- spectra organischer Dampfe. 1897. Ueber das des Natriums. (Read Feb. 5.) Absorption des Lichtes, Fluor- escenz, Phosphorescenz. WD, Fluorescenzspectrum | | *C. RY? exx. 1386-7390 ; | ‘Ber,’ xxviii. (Ref.), 1046 | (Abs.) ; ‘ Beiblitter,’ xix. | 826-827 (Abs.) ; ‘Chem. News, Ixxii. 13-14; ‘J. | Chem. Soc.’ lxviii. IT. | 498-499 (Abs.); ‘Proc. Phys. Soc’ xiii, 361 (Abs.); ‘ Nature, lii. 239 (Abs.), 255-256. ‘Ann. Chem. u. Pharm.’ ceclxxxvii. 230 — 232; ‘Ber.’ xxviii. (Ref.), 725 (Abs.) ; ‘ Beibliitter,’ xix. 731 (Abs.); ‘J. Chem. Soc.’ Ixx. II. 2 (Abs.) ; ‘Chem. News,’ Ixxii. 78 (Abs.) ‘Ann. Phys. u. Chem.’ {N.F.], lvi. 201 — 254; © Nature,’ lili. 94 (Abs.) ‘Sitzungsb. phys. med. Soc. Erlangen,’ xxvii. 164-109; ‘Nature,’ liii. 250-251 (Abs.); ‘Ann. Phys. u. Chem.’ [N.F.] lvii. 447-453 ; ‘J. Chem. Soc.’ Ixx. II. 346 (Abs.) ; ‘ Astrophys. J. ili. 207— 212.) ‘ Jahrb. f. Photogr.’ x. 14— 15. ‘Verhandl. phys. Gesellsch. Berlin,’ xvi. 37-40; ‘ Bei- blatter, xxi. 417 — 418 (Abs.) ‘ Jahrb, f. Photogr,’ xi, 81- 87. ASTRONOMICAL APPLICATIONS. 1891. Untersuchungen tiber die Rotation der Sonne. (Read Feb. 14.) 1892, The New Starin Auriga. (April.) ‘Acta Soc. Sci. Upsala’ ls], xiv. “IE78; |° Ber blatter, xvi. 430 — 431 (Abs.) ‘Contemporary Review,’ April 1892 ; ‘ Astron. and Astrophys.’ xi. 503-513; ‘Beiblitter, xvii. 207- 208 (Abs.) 492 G.E. Hale . M. von Konkoly G. E. Hale »” E. von Gothard E. C. Pickering W. W. Campbell G. E. Hale W. W. Campbell W. Sidgreaves H.C. Vogel . W. W. Campbell J. E. Keeler . H. C. Vogel . REPORT—1898. ASTRONOMICAL APPLICATIONS, 1892, 1893. Solar Photography at the Ken- wood Astrophysical Observatory. (May.) Spectroscopische Beobachtungen an der Sternwarte von O’Gyalla in Ungarn. (Read June 20.) The Ultra-violet Spectrum of the Solar Prominences. (Aug.) A Remarkable Solar Disturbance. (Aug.) . | Photographs of Solar Phenomena obtained with the Spectro-helio- graph at the Kenwood Observa- tory. (Aug.) Das Spectrum des neuen Sternes in Auriga in Vergieich mit demjeni- gen einiger planetarischen Ne- bel. (Read Oct. 17.) Report of the Harvard College Observatory. (Oct.) The Spectrum of Nova Aurige in February and March 1892. (Noy.) Some Results and Conclusions de- rived from a Photographic Study of the Sun. (Nov.) The Motion of (Noy.) Nova Aurigze. Note on the Revival of Nova Au- rige. (Dec.) Untersuchung iiber die LHigen- bewegung der Sterne im Visions- radius auf spectrographischen Wege. 1893. of Holmes’s and (Jan.) The Spectra Brookes’s Comets. Holmes’s Comet. (March.) Spectrum of (1892, III.) Ueber den neuen Stern im Fuhr- mann. (Read March 16.) | ‘ Astron. and Astrophys.’ xi. 407-417, 603-604; ‘ Bei- blatter,’ xvii. 752 — 753 (Abs.) ‘Math. u. Naturwiss. Ber. aus Ungarn,’ x. 240-245. ‘Astron. and Astrophys.’ xi. 602 ; ‘ Beibliitter,’ xvii. 126 (Abs.) ‘Astron. and Astrophys,’ xi. 611-613 ; ‘ Beibliitter,’ xvii. 126 (Abs.) ‘Astron. and Astrophys. xi. 603-604 ; ‘ Beibliitter,’ xvii. 126 (Abs.) ‘Math. u. Naturwiss. Ber. aus Ungarn,’ x. 246-249 ; ‘Beiblatter, xviii. 101- 102 (Abs.) ‘Nature, xlvii. 403-404 (Abs.) ‘ ‘Astron. and Astrophys.’ xi. 799-811; ‘Nature,’ xlvii. 133 (Abs.) ‘Astron. and Astrophys.’ xi. 811-815; ‘Chem. News,’ Ixvii. 4-5 (Abs.) ; ‘Beiblitter, xvil. 753 (Abs.) ‘Astron. and Astrophys.’ xi. 881-882; ‘Nature, xlvii. 256 (Abs.) ‘ Astron. and Astrophys.’ xi. 882-885; ‘Nature, xlvii. 256 (Abs.) ‘Publ. d. Astrophys. Obs. Potsdam, vii. I. Theil, No. 23, 1-166;. ‘ Bei- blatter, xvii. 128-129 (Abs.) ‘Astron. and Astrophys.’ xii. 57; ‘ Nature,’ xlvii. 235. ‘Astron. and Astrophys.’ xii. 272-273; ‘Nature,’ xlvii. 578 (Abs.) ‘Abhandl. Akad. Berlin,’ 1893, 60 pp.; ‘Bei- blatter, xvii. 932-933 (Abs.) OE a de ak Fes ee. J. &. Keeler . ' A. Belopolsky H. Deslandres M. Fleming . O. Knopf A. D. Risteen G. Miller W. W. Campbell J. i. Keeler . ” i. C. Pickering W. 8.58. Monck ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 493 ASTRONOMICAL APPLICATIONS, 1893. Visual Observations of the Spec- trum of 8 Lyre. (April.) Le spectre de létoile variable B Lyre. (Read May 12.) Spectrum der ‘ Nova Aurigie,’ 1892, beobachtet in Pulkowa. (May.) Sur la recherche de la couronne solaire en dehors des éclipses totales. (Read May 23.) Stars having Peculiar Spectra. | (June.) Die Schmidt’scheSonnentheorie und ihre Anwendung auf die Methode der spectroscopischen Bestim- mung der Rotationsdauer der Sonne. (Habilitationschrift, June 1893, 44 pp.) The Sun’s Motion through Space. (June.) Photometrische und spectroscop- ische Beobachtungen auf dem Gipfel des Santis. (Publications des Astrophys.Observ. zu Potsdam, viii. I. 5.) (July.) The Spectrum of the Rordame- Quénisset Comet. (Aug.) The Spectrum of Comet 2 1893. | (Aug.) The Nature of the Spectrum of Nova Aurigeze. (Aug.) Wave-lengths of the Two Brightest Lines in the Spectrum of the Nebule. (Aug.) Observations of Comet & 1893. (Aug.) The Constitution of the Stars. (Oct.) The Spectra and Proper Motion of Stars. (Nov.) ‘Astron. and Astrophys.’ xii. 350-361; ‘ Bei- blitter, xviii. 100-101 (Abs.); ‘Nature,’ xlvii. 616 (Abs.) ‘Bull. Acad. St. Peters- burg’ [4], xxxvi. 163-195. ‘Bull. Acad. St. Peters- burg’ [4], xxxv. 399-420 ; ‘Nature,’ xlix. 23 (Abs.) ‘C. RB. cxvi. 1184-1187; ‘Beiblitter, xviii. 672 (Abs.) ‘Astron. and Astrophys.’ xii. 170, 546-547, 810-811. * Astr. Nachr.’ cxxxiv. 105— 120; ‘Beiblitter, xvii. 930-931 (Abs.) |*Astron, J, xiii. 74-75; ‘Nature,’ xlviii. 208-209 (Abs.)_ ‘Naturwiss. Rundschau,’ vili. 325-327. ‘ Astr. Nachr.’ exxxiii. 150- 152; ‘Nature, xlviii. 379 (Abs.) ; ‘ Beiblitter,’ xviii. 766 (Abs.) ‘Astron. and Astrophys.’ xii, 652-653. ‘Astron. and Astrophys.’ xii. 722-730; < Astr! Nachr.’ cxxxiii. 337-343 ; . ‘Nature,’ xlvili. 524(Abs.) ‘ Astron. and Astrophys.’ xii. 733-736 ; ‘ Beiblitter,’ xviii. 566 (Abs.) ; ‘Nature,’ xlix. 18 (Abs.) ‘Astron. and Astrophys.’ xii. 650-651; ‘ Nature,’ xlviii. 401 (Abs.) ‘Astron. and Astrophys.’ xii. 718-722; ‘Bei- bliitter,’ xvili. 673 (Abs.) ‘Astron. and Astrophys.’ xii. 811-812. 494. E. C. Pickering EPs J. Wilsing . C. A. Young. W. W. Campbell H. Deslandres T, E. Espin A. Belopolsky E. Gothara ¥F. Kriiger T, E. Espin.. A. Belopolsky W. W. Campbell H, Deslandres J. Fényi . H. Kayser’ . ’ REPORT—1898. ASTRONOMICAL APPLICATIONS, 1893, 1894. A New Star in Norma. (Noyv.) The Spectrum of (Nov.) Ueber die Bestimmung von Bahn- elementen einiger Doppelsterne aus spectroscopischen Messungen der Geschwindigkeitscompon- enten. (Nov.) Note on the Chromosphere Spec- trum. (Oct.) Hydrogen Envelope of the Star D.M. +30° 36’ 39”. (Dec.) Sur Ja recherche de la partie de Yatmosphére coronale du soleil projetée sur la disque. (Read Dec. 26.) Stars with Remarkable Spectra. (Dec.) Les changements dans le spectre du B Lyre. Studien tiber das photographische Spectrum der planetarischen Nebel und des neuen Sterns. Catalog der farbigen Sterne zwi- schen dem Nordpol und 23 Grad stidlicher Declination, mit beson- derer Beriicksichtigung des Spec- traltypens. 1894. | | Nova Norme. | Report of the Wolsingham Obser- | vatory. (Jan.) On the Motion of ¢ Herculis in the Line of Sight. (Feb.) Spectrum of Nova Norme. (Tele- gram received at Kiel, Feb. 15.) Recherches spectrales sur la rota- tion et les mouvements des pla- nétes. (Read Feb. 25.) On Two Great Protuberances. (Feb.) Ueber den Einfluss der Spalten- weite auf das Aussehen der Kometenspectra, (March.) ‘ Astr. Nachr.’ cxxxiv. 101- 102; ‘ Beibliitter,’ xviii. 768 (Abs.); ‘ Astron. and Astrophys.’ xiii. 40-41 ; ‘Nature,’ xlix. 300 (Abs.) ‘ Astr. Nachr.’ exxxiv. 101- 102; ‘Nature,’ xlix. 162- 163 (Abs.) ‘ Astr. Nachr.’ exxxiv. 89_- 92; ‘Beiblatter, xviii. 673 (Abs.) ‘Nature,’ xlv. 28; ‘ Bei- blitter,’ xvii. 830 (Abs.) ‘Astron. and Astrophys.’ xii. 913-914; ‘ Nature,’ xlix. 210 (Abs.) °C. RY cxvii. 1053-1056 ; ‘Beiblatter, xviii. 563 (Abs.) ‘Astr. Nachr.’ exxxiv. 123-— 128; ‘ Nature,’ xlix, 183- 184 (Abs.) ‘Mem. spettr. ital.’ xxii. 101-111; ‘ Nature,’ xlviii. 301 (Abs.) ‘Mem. spettvr. ital.’ xxi.169- 173; ‘ Beiblatter, xvii. 754 (Abs.) ‘Publications d. Stern- warte in Kiel,’ viii. 145 pp.; Beiblatter,’ xviii. 98 (Notice). ‘Nature,’ xlix. 300 (Abs.) ‘Astron. and Astrophys.’ xiii. 130-136. ‘ Astr. Nachr.’ exxxv. 311- 312; ‘Nature,’ xlix. 397. °C. RR’ exx. 417-425; ‘ Beiblitter, xx. 35 (Abs.); ‘ Proc. Phys. Soc.’ xiii. 165 (Abs.); ‘ Nature,’ li. 422 (Abs.) ‘ Astron. and Astrophys.’ xiii. 122-128; ‘ Beibliit- ter,’ xix. 173 (Abs.) ‘Astr. Nachr.’ cxxxv. 1-10; ‘ Beibliitter,’ xviii. 766-767 (Abs.) : W. H. Pickering W. W. Campbell H, Deslandres E. C. Pickering H.C. Vogel . M. Fleming . A. Fowler . E. H. Hills . H. Kayser . J. N. Lockyer E. C. Pickering W. W. Campbell ” T. E. Espin . M. Fleming . J. E. Keeler , ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 49: we ASTRONOMICAL APPLICATIONS, 1894. A Study of Nova Aurigz and Nova Norme. (March.) Observations of the New Star in Norma. (April.) Photographie de la chromosphere solaire. (Read April 16.) New Variable Stars in Sculptor, Scorpio, Ophiuchus, and Aquila. (April.) Bemerkungen zu der Abhandlung des Herrn Prof. H. Kayser ‘Ueber den Einfluss der Spalten- weite auf das Aussehen der Kometenspectra.’ (April.) Stars having Peculiar Spectra. (May.) Gale’s Comet. (May) . . The Total Solar Eclipse of April 16, 1893. Report on Results ob- tained with the Slit Spectroscope. (Received March 7. Read May 10.) Ueber den Hinfluss der Spaltweite auf das Aussehen der Kometen- spectra. (May.) Preliminary Report on the Results obtained with the Prismatic Camera during the Total Solar Eclipse of April 16, 1893. (Read May 10.) The New Star in Norma. (May) . The Wolf-Rayet Stars. (June) Spectra of the Great Nebula of: Orion and other well-known Nebule. (June.) Catalogue of Stars with Remark- able Spectra. (June.) Stars having Peculiar Spectra. (June.) The Spectra of the Orion Nebula and of the Orion Stars. (June.) ‘Astron. and Astrophys.’ xiii. 201-204; ‘ Bei- bliitter,’ xix. 175 (Abs.) ‘ Astr. Nachr.’ exxxy. 131— 132; ‘ Nature,’ xlix. 586 (Abs.) °C. RY exviii. 842-844, ‘ Astr. Nachr.’ cxxxv. 161— 164; ‘Nature,’ xlix. 6(S (Abs.) ‘ Astr. Nachr.’ exxxv. 105— 108; ‘ Beiblatter, xviii. 766-767 (Abs.) ‘ Astr. Nachr.’ exxxv.195 198; ‘Nature’ 1. 3 (Abs.) ‘ Nature,’ 1. 36-37, ‘Proc. Roy. Soc.’ lvi. 20- 26:5. ‘Nature? 7) 236 (Abs.) fi Astr. Nachr.’ cxxxv. 221— 224; ‘Nature,’ xlix. 489 (Abs.) ‘Proc. Roy. Soc.’ lvi. 7-S (Abs.); ‘ Beiblatter,’ 914 (Abs.); ‘Nature,’ 1. 118_ 119 (Abs.) ‘Astron. and Astrophys.’ xiii, 398; ‘ Beiblatter, xix. 68 (Abs.) ‘Astron. and Astrophys.’ xiii. 448-476; ‘Nature,’ 1.181 (Abs.) ; ‘Beibliitter,’ xix. 67-68 (Abs.) ‘Astron. and Astrophys.’ xiii, 384-398, 494-501 ; ‘Nature,’ 1. 254 (Abs.); ‘Beiblatter, xix. 68 (Abs.) * Astr. Nachr,’ cxxxy. 265— 274. ‘Astron. and Astrophys.” xiii. 501-503. ‘Astron. and Astrophys.’ xiii. 476-493; ‘Nature,’ 1, 254 (Abs.); ‘Bei- blatter,’ xix. 68 (Abs.) LOG J. N. Lockyer ” *, I’, Renz . EK. Demargay . H. Deslandres J. Evershed . R. Lehman-Filhés . H. Deslandres W. Huggins . : J.i. Keeler . H. C. Vogel A. Berberich . J. &. Keeler and J. Scheiner. A. Belopolsky A. Fowler . REPORT—1598. ASTRONOMICAL APPLICATIONS, 1894. On the Photographic Spectrum of the Great Nebula in Orion. (Read June 21.) Preliminary Note on the Spectrum Changes in 8 Lyra. (Read June 21.) Beobachtungen der Nova Aurige. (June.) (T) Sur la simplicité du samarium. (Read July 23.) Images spéciales du soleil données par les rayons simples, qui corre- spondent aux raies noires du spectre solaire. (Read July 9.) The Corona Spectrum. (July) Ueber die Bestimmung einer Dop- pelsternbahn aus spectroscopischen Messungen den im Visionsradius liegenden Geschwindigkeitscom- ponenten. (July.) Recherches sur les mouvements de latmosphére_ solaire. (Read Aug. 27.) Note on the Spectrum of the Great Nebula in Orion. (Aug.) The Magnesium Spectrum as an Index to the Temperature of the Stars. (Aug.) On the Spectrum of 8 Lyre. (Aug.) Neue Untersuchungen iiber Nebel- spectra. (Sept.) J.inien im unteren roth-gelb-griinen Theile des Spectrums yon 8 Orionis (Rigel.) (Sept.) Etude sur le spectre de létoile variable 5 Cephei. (Read Oct. 12.) Das Spectrum von 6 Cephei. (Oct.) Mira Ceti. (Nov.) . 7 ; ‘Proc. Roy. Soc.’ lvi. 285— 286 (Abs.); ‘ Astron. and Astrophys.’ xiii. 574-575 (Abs.) ‘Proc. Roy. Soc.’ lvi. 278— 285; ‘Astron. and As- trophys.’ xiii. 575-581. ‘ Astr. Nachr.’ exxxyv. 389- 394; ‘Nature,’ 1. 254 (Abs.) ‘¢@. RR. cxix. “163-164: ‘ Beibliitter, xviii. 619 (Abs.) “Co Re Cxises d4S=ible- ‘Chem. News,’ Ixx. 71- (Abs.); ‘ Nature,’ 1. 307- 308 (Abs.); ‘ Beibliitter,’ xix. 67 (Abs.) ‘Nature, xlvili. 268; ‘Beiblitter, xviii. 563 (Abs.) * Astr. Nachr.’ exxxvi. 17- 30. . °C. BR.’ cxix. 457-460 ‘ Beibliitter, xix. 333 (Abs.) ; ‘ Nature,’ 1. 468 (Abs.) ‘Astron. and Astrophys.’ xiii. 568-569. ‘ Astr. Nachr.’ cxxxvi. 77— 80; ‘ Beiblitter,’ xix. 60 (Abs.). ‘* Nature,’ 1. 364— 365 (Abs.) ‘Astron. and Astrophys.’ xiii. 561-568. ‘Naturw. Rundschav,’ ix. 477-479. ‘Naturw. Rundschau,’ ix. 476 (Abs.) ‘Bull. Acad. St. Peters- burg’ [5], i. 267-306; ‘ Nature,’ li. 282 (Abs.) ‘ Astr. Nachr.’ exxxvi. 281— 284; ‘Astrophys. J.’ i. 160-161; ‘ Beibliitter,’ xx. 40 (Abs.); ‘ Nature,’ li. 21 (Abs.) ‘Nature,’ li. 40. we ee ee ee eit « Py i etsde a). ON THE BIBLIOGRAPHY OF SPECTROSCOPY. J. N. Lockyer A. Belopolsky H, Deslandres J. N. Lockyer E. C. Pickering A. Belopolsky A. Cornu 2 A. A. Michelson E. C. Pickering W. W. Campbell H, C. Vogel H Poincaré . J. Fényi F The Sun’s Place in Nature. (A course of lectures to working men, delivered in the Museum of Practical Geology, Nov.—Dec.) Observations of Sun-spot Spectra, 1879-94. (Read Noy. 22.) Hin Project zur Reproduction der Verschiebung von Spectrallinien bewegter Lichtquellen. (Dec.) Sur la vitesse radiale de ¢ Her- culis. (Read Dec. 31.) On the Photographic Spectrum of y Cassiopeiz. (Read Dec. 13.) Stars having Peculiar (Dec.) Spectra. Sur le renversement de la raie D, du spectre solaire. Spectroscopie solaire , : On the Conditions which Affect the Spectro-photography of the Sun. (Jan.) Discovery of Variable Stars by their Photographic Spectra, (Jan.) 1895. Recent Changes in the Spectrum of Nova Aurigs. (Jan.) Neuere Untersuchungen tiber die Spectra der Planeten. I. Il. (Read Jan. 17.) Observations au sujet de la com- munication précédente de M. Deslandres. (Read Feb. 25.) A Very Large Solar Protuberance Observed on Dec, 24, 1894. (March.) 497 ASTRONOMICAL APPLICATIONS, 1894, 1895. ‘Nature,’ li. 374-377, 396— 399, 565-569, 590-592; lii. 12-14, 156-158, 204-— 207, 253-255, 327-329, 422-495, 446-450. ‘Proc. Roy. Soe.’ lvii. 199- 201; ‘Nature, li. 448- 449; ‘ Beiblitter, xx. 33 (Abs.) ‘ Astr. Nachr.’ cxxxvii. 34- 36; ‘ Nature,’ li. 233-234 (Abs.) ; ‘ Beiblitter,’ xix. 418-419 (Abs.) "0. Re: exix:, 1252-1254; ‘ Beiblitter,’ xix. 431-432 (Abs.); ‘ Nature,’ li. 260 (Abs. ) ‘ Proc. Roy. Soc.’ lvii. 173- 177; *Nature; It. 425 (Abs.) ‘Astr. Nachr. cxxxvii. 71-74; ‘Nature, li. 304 (Abs.) ‘Mem. spettr. ital” xxiii. 89-93; ‘Naturw. Rund- schau,’ ix. 55 (Abs.); ‘Beiblatter,> xix. 422- 23 (Abs.) ‘Annuaire du Bureau des Longitudes,’ 1894, 169- 172; ‘ Nature,’ xlix. 397 (Abs.) ‘Astrophys. J. i. 1-95. ‘ Beibliitter, xix. 428 (Abs.) ‘ Astrophys. J.’ i. 27-28; ‘Beiblatter, xix. 431 (Abs.) ‘ Astrophys. J.’ i. 49-51; ‘Beiblatter, xix. 432 (Abs.); ‘ Nature,’ li. 347 (Abs.) ‘Sitzungsb. Akad. Berl.’ 1895, 5-25; ‘ Astrophys. J. i. 196-209, 273-284 ; ‘ Beiblitter, xix. 429 (Abs.); ‘Proc. Phys. Soe.’ xiii. 261-262 (Abs.) “C@)- R2 cxxa) 420242 ‘Proc. Phys. Soc.’ xiii. 166 (Abs.) ‘ Astrophys. J.’ i. 212-215; ‘ Beiblitter,’ xx. 33 (Abs.) KK 498 W. Iluggins . H. Deslandres L. E. Jewell . Hf. Deslandres T. EK. Espin . M. Fleming J. E. Keeler . A. Orbinsky . W. W. Campbell W. Huggins J. E. Keeler . J. N. Lockyer Hi. Seeliger . REPORT—1898. ASTRONOMICAL APPLICATIONS, 1895. Note on the Atmospheric Bands in the Spectrum of Mars. (March.) Rayonnement ultraviolet de la couronne solaire pendant l’éclipse totale du 16 avril 1893. (Read April 1.) The Spectrum of Mars. (April) Recherches spectrales sur les anneaux de Saturne. (Read May 27.) Comparaison entre les spectres du gaz de la clévéite et de l’atmo- sphere solaire. (Read May 20.) Stars with (May.) Remarkable Spectra. Stars having Peculiar Spectra. Eleven New Variable Stars. (May.) A Spectroscopic Proof of the Meteoric Constitution of Saturn’s Rings. (May.) Nouvelle méthode de détermina- tion des vitesses radiales des étoiles. (May.) A Review of the Spectroscopic Observations of Mars. (June.) Solar and Terrestrial Helium. (June.) Conditions Affecting the Form of Lines in the Spectrum of Saturn. (June.) Spectrum of the Orion Nebula. (Read June 21.) Bemerkung tiber die Rotation des Saturnringes. (June.) ‘Astrophys. J.’ i. 193- 195; ‘ Beibliatter,’ xx. 36 (Abs.) ‘C. R, exx. 707-710; ‘ Bei- blitter,” xx. 33 (Abs.) ; ‘Proc. Phys. Soc.’ xiii. 222 (Abs.) ; ‘ Nature,’ li. 576 (Abs.) ‘Astrophys. J. i. 311- 317; ‘Beiblatter, xx. 36 (Abs.); ‘Nature,’ lii. 37 (Abs.) © OP RY *exx, lbb=10bs: ‘Proc. Phys. Soc.’ xiii. 308-309 (Abs.) ; ‘Nature,’ lii. 144 (Abs.) ‘C. RR. cxx. 1112-1114; ‘Beiblitter, xix. 568 (Abs.); ‘Chem. News,’ Ixxil. 14-15; ‘ Proc. Phys. Soc. xiii. 3871 (Abs.); ‘J. Chem. Soc.’ xviii. II. 431 (Abs.) ; ‘ Nature,’ lii. 120 (Abs.) . ‘Astr. Nachr’ cxxxvii. 369-376; ‘Nature,’ lii. 86 (Abs.) ‘ Astrophys. J.’ i. 411-415. ‘ Astrophys. J. i. 416-427; ‘Beiblatter,” xx. 38 (Abs.); | ‘ Nature,’ lii. 164-165 (Abs.) ‘Astr. Nachr.’ cxxxvili. 9-12; ‘ Nature, lil. 155 (Abs.) ; ‘ Beiblitter,’ xx. 202 (Abs.) ‘ Astrophys. J.’ il. 28-44; ‘Beiblatter, xx. 37 (Abs.) ‘Chem. News,’ Ixxi. 283 ; ‘ Beiblatter,’ xix. 634- 635 (Abs.) ‘ Astrophys. J.’ ii. 63-68 ; ‘Beiblitter, xx. 200 (Abs.) * Phil. Trans.” clxxxvi. A, 73-91 ; ‘ Nature,’ li. 471— 472 (Abs.) ¢Astr. Nachr.’ cxxxviii. 99-102; Beibliitter, xx. 38 (Abs.) ee _- els Hales j.i . W. Huggins . 4 J.Janssen . : J DW. W. Campbell F. Kriiger W.W. Campbell . ” a | C. Runge and F. Paschen. | A. Belopolsky 2 ‘ W. W. Campbell eblemine ., . = J.E. Keeler . ‘ € J. N. Lockyer 5 H.C. Vogel . ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 499 ASTRONOMICAL APPLICATIONS, 1895. Preliminary Note on the D, Line in the Spectrum of the Chromo- sphere. (July.) On the Duplicity of the Sclar Line D,. (QJuly.) Sur la présence de la vapeur d'eau dans latmosphére de la planéte Mars. (Read July 29.) A Spectrographic Determination of Velocities in the System of Saturn. (Aug.) The Spectrum of Mars. (Aug.) . Spectroscopic Observations of Coloured Stars. (Aug.) Observations of the B Band in Stellar Spectra. (Sept.) The Visible Spectrum of the Trifid Nebula. (Sept.) Helium and the Spectrum of Nova Aurigz. (Sept.) Spectrographische Untersuchungen des Saturnringes. (Oct.) Stars whose Spectra contain Bright and Dark Hydrogen Lines. (Oct.) Some New Variable Stars. (Oct.) A New Star in the Constellation Carina. (Oct.) Note on the Rotation of Saturn’s Rings. (Oct.) Photographies des spectres des étoiles. (Read Oct. 21.) Ueber das Vorkommen der Linien des Cléveitgas-Spectrums in den Sternspectren, und iiber die Classi- fication der Sterne vom ersten Spectraltypus. (Read Oct. 24.) ‘Astr. Nachr, 227-230; ‘Nature,’ lii. 327 (Abs.) ; ‘ Beiblitter,’ xx. 198 (Abs.) ‘Astr. Nachr. exxxviii. 229-230; ‘ Beibliitter, xx, 198 (Abs.) (CAGhS VOxxin 238=03/ne ‘Beiblitter” xx. 36 (Abs.) ; *Proé. Phys. Soc.’ xili, 376 (Abs.); ‘Na- ture,’ lii. 514 (Abs.) 127— EK ‘Astrophys. J.’ ii. 135; ‘ Beiblitter,’ 201-202 (Abs.) ‘Publications of the As- tronomical Society of the Pacific, vi. No. 27, 228~ 236; ‘Nature, li. 132 (Abs.) ‘ Astrophys. J.’ ii. 148-159. ‘ Astrophys. J.’ ii. 163. ‘ Astrophys. J,’ ii. 161-162. ‘Nature, lii. 544. ‘ Astr. Nachr.’ cxxxix. 1-4, 210-214. ‘ Astrophys.J.’ ii. 177-183; ‘Nature,’ liii. 15 (Abs.) ; ‘ Beiblitter, xx. 3872- 373 (Abs.) olo ‘Astrophys. J.. ii. 198-201. ‘Harvard Coll. Observ. Cire. No. 1 (Oct. 30); ‘ Nature,’ liii. 63 (Abs.) | ‘ Astr. Nachr.’ cxxxix. 5-6; ‘Nature,’ lii. 655 (Abs.) ; ‘Beiblitter, xx. 370 (Abs.) °C. BR.’ cxxi. 546; ‘Na- ture,’ lii. 660 (Abs.) ‘Sitzungsb. Akad. Berl.’ xl. 947-958 ; ‘ Proc. Phys. Soc.’ xiv. 161-164 (Abs.); ‘ Beiblitter, xx. 372 (Abs.); ‘Astrophys. J. ii. 333-346; ‘ Nature,’ liii. 448-449 (Abs.) KK2 CXXXViii. ', + 500 REPORT—1898. ASTRONOMICAL APPLICATIONS, 1895, 1896. A. Belopolsky H. Deslandres C.B. Frost . J. N. Lockyer A. W. Roberts H. Deslandres M. Fleming G. E. Hale E. C. Pickering H. Deslandres A. Brester . A. Belopolsky G.E. Hale . L. E. Jewell, J. F. Mohler, and W. J. Humphreys. J. Fényi F ‘ Recherches sur les déplacements des raies dans le spectre de Saturn et de son anneau. (In Russian.) (Nov.) Recherches spectrales sur l’étoile Al- tair. Reconnaissance d’un mouve- ment orbital et dune atmosphere. (Read Noy. 4.) Note on a Differential Method of Determining the Velocity of Stars in the Line of Sight. (Nov.) On the Variable Stars of the 6 Cephei Class. (Read Nov. 21.) Short Period Variability. (Noy.) . A Method of Investigating the Velocity of Stars in the Line of Sight with Small Instruments. (Read Dec. 13.) Stars having Peculiar (Dec.) A New Star in Centaurus. Spectra. (Dec.) On the Wave-length of the D, Line in the Spectrum of the Chromosphere. (Dec.) A New Star in Carina. (Dec.) Spectroscopie astronomique . 1896. The Variability of Red Stars. (Jan.) Observations des raies renversées dans le spectre des protubérances, faites 4 Poulkova. (Feb.) Notes on the Application of Messrs. Jewell, Humphreys, and Mohleyr’s Results to Certain Problems of Astrophysics. (Feb.) Note on the Presence of the ‘ Re- versing Layer’ in the Solar At- mosphere. (Feb.) On Two Solar Protuberances, ob- served July 15 and Sept. 30, 1895. (March. ) ‘Bull. Acad. St. Peters- burg’ [5], iii. 379-408 ; ‘Beiblitter, xx. 370 (Abs.) ‘C. R? cxxi. 629-632; ‘Chem. News,’ lxxii. 269 (Abs.) ; ‘ Nature,’ liii. 38 (Abs.); ‘ Beiblatter,’ xx. 372 (Abs.) ‘Astrophys. J.’ li. 235-236; ‘ Beiblitter, xx. 371 (Abs.) ‘Proc. Roy. Soc.” lix. 101- 106; ‘Nature,’ lili. 262- 263 ; ‘ Beiblitter,’ xx. 700 (Abs.) ‘ Astrophys. J.’ ii. 283-292; ‘Nature,’ lili, 162-163 (Abs.) ‘The Observatory, xix. 49-52; ‘ Nature, liii. 255- 256 (Abs.) ‘ Astrophys. J. ii. 354— 359. ; ‘Harvard Coll. Observ. Cire.’ No. 4 (Dec. 20); ‘Nature,’ liii. 256. ‘ Astrophys. J.’ ii, 384-385. ‘ Astr. Nachr.’ cxxxix. 119_- 120; ‘Beiblatter,’ xxi. 345 (Abs.) ‘Report of the Paris Ob- servatory,” 1895, 22-23; ‘Nature, liv. 162 (Abs.) ‘Knowledge,’ xviii. 251- 253; ‘Nature,’ lili. 248— 249. ‘Mem. spettr. ital.’ xxv. 23-26. ‘Astrophys. J. ii. 156— 161. ‘Astrophys. J. ii. 138= 140; ‘ Beiblitter,’ xx. 527 (Abs.) ‘Astrophys. J.’ iii. 200. 192- _- ——— a ee ee eee ee z ON THE BIBLIOGRAPHY OF SPECTROSCOPY. E. C. Pickering H.C. Vogel . L. E. Jewell . : J. N. Lockyer Th, Arendt . F. Maclean . J. Trowbridge J. N. Lockyer E. C. Pickering W. W. Campbell H. Deslandres L. E: Jewell . BE. C. Pickering ” J. E. Keeler . M. Fleming . | The 501 ASTRONOMICAL APPLICATIONS, 1896. Algol Variable, B.D.+17° 4367. (March.) Ueber das Spectrum von Mira Ceti. (Read March 26.) The Spectrum of Mars. (April) The Total Eclipse of the Sun, April 16, 1893. (Read April 30.) Die Schwankungen im Wasser- dampfgehalte der Atmosphire auf Grund — spectroscopischer | Untersuchungen. (May.) Photographs of the Spectra of Twenty-three Helium Stars; also Photographs of the Spectra of Six Stars of the 3rd Magnitude, show- ing the Transition from Type to Type. (Read May 8.) Carbon and Oxygen in the Sun. (May.) On the Unknown Lines observed | in the Spectra of many Minerals. (Read June 4.) Ten New Variable Stars. Observations of (July.) Observations of the Total Solar Kclipse of April 16, 1893. (Report.) (July.) On Mr. Jewell’s the Spectrum of Mars. Researches on the Solar Rotation. | (Aug.) Stars having (Aug.) A New Spectroscopic Binary, py, Scorpii. (Aug.) Peculiar Spectra. The Detection of the Lines of Water Vapour in the Spectrum of a Planet. (Sept.) Stars having Peculiar Spectra. New Variable Stars in Crux and Cygnus. (Nov.) (June.) | | ‘Astrophys. J.’ iii. ‘ Astrophys, J.’ iii. 200. ‘Sitzungsb. Akad. Berl.’ 1896, 395-399; ‘Proc. eae Soc.’ xiv. (Abs.) 233-234; ‘ Beibliitter,’ xxi, 345 (Abs.); ‘Na- ture,’ liii. 612 (Abs.) 255— 258; ‘Beibliitter,’ xxi. 342 (Abs.) ‘Proe. Roy. Soc.’ lx. 17- 19 (Abs.) ; ‘ Nature,’ liv. 46 (Abs.) ‘Ann.Phys.u.Chem.’[N.F.], lviii. 171-204. ‘Monthly Not. R. A. 8.’ lvi, 428-429; liv. 158 (Abs.) ‘Nature,’ ‘Amer. J. Sci’ [4], 1. 329- 333; ‘Phil. Mag.’ [5], xli. 450-454; ‘Nature,’ liv. 91-92 (Abs.) ‘Proc. Roy. Soc.’ Ix. 133- 140; ‘ Beibliitter, xxi. 129-130 (Abs.) ‘Harvard Coll. Obs. Circ.’ No.7; ‘ Nature,’ liv. 206— 207 (Abs.) ‘Astrophys. J.’ iv. 79-80. ‘Nature, liv. 3801-302 (Abs.) ‘Astrophys. J.’ iv. 138; ‘ Nature, liv. 526 (Abs.) ‘Astr. Nachr, cxli. 170; ‘Nature,’ liv. 404 (Abs.) ‘Harvard Coll. Observ. Circe? No: Ll 725 pps ‘Nature,’ liv. 527 (Abs.) ‘Astrophys. J.’ iv. 137- 138. ‘Harvard Coll. Observ. Circe.” No. 12, 2 pp.; ‘Nature,’ lv, 8t (Abs.) 502 J, N. Lockyer “ E. C. Pickering M. Fleming , C. Runge and F. Paschen. A, Cornu ; A. Belopolsky H. Deslandres W. Huggins , Sir J. N. Lockyer . ” E, C. Pickering L. E. Jewell . » > H. Kayser. REPORT—1898. Preliminary Report on the Results obtained with the Prismatic Camera during the Eclipse of 1893. (Read Noy. 19.) Relative Motion of the Starsin the Line of Sight. (Nov.) A New Spectroscopic Binary in Puppis. (Noy.) Stars having Peculiar Spectra. Eight New Variable Stars, in Cetus, Vela, Centaurus, Lupus, Scorpio, Aquila, and Pegasus. (Dec.) Oxygen in the Sun. (Dec.) . 1897. Spectres des Ctoiles, &c.. . The Spectroscopic Geminorum. (Jan.) Photographie d’une protubérance extraordinaire. (Read Jan. 25.) Binary a, Carbon in Bright-line Stars. Celestial Eddies. (Jan.) The Question of Carbon in Bright- line Stars. (Jan.) (Jan.) The Approaching Total Eclipse of the Sun. I-VI. (Jan.—Sept.) The Spectrum of ¢ Puppis. (Jan.) Oxygen in the Sun. (Feb.) . The Coincidences of Solar and Metallic Lines. (Feb.) Spectrum of ¢ Puppis. (Feb.) ASTRONOMICAL APPLICATIONS, 1896, 1897. ‘Proc. Roy. Soc.’ lx. 271- 272. ‘Harvard Coll. Observ. Cire” No. 13, 2) pp.; ‘Nature,’ lv. 137 (Abs.) ‘Harvard Coll. Observ. Cire.’ No: 14, 1 p.3 ‘Na- ture,’ lv. 137 (Abs.) ‘ Astrophys. J.’ iv. 354-359. ‘Astrophys. J.’ iv. 317- 319; ‘Nature,’ lv. 303 (Abs.) ; ‘ Beibliitter,’ xxi. 518 (Abs.) | ‘Ann. Bureau des Longi- tudes,’ 1896,, 359-368 ; ‘Proc. Phys. Soc.’ “xiv. 74-75 (Abs.) ‘Astrophys. J. v. 1-7; ‘Nature,’ lv. 352 (Abs.) 171-173; XXL. OLS Ol Re exxiv. ‘ Beibliitter,’ (Abs.) ‘Nature,’ lv. 316. ‘Nature,’ lv, 249-253. ‘Nature, lv. 304-305. ‘ Beiblitter,” xxii. 155 (Abs.) ‘Nature,’ Ivi. 154-157, 175-178, 318-321, 365- 368, 392-395, 445-449. ‘ Astrophys. J.’ v. 92-94; ‘Harvard Coll. Observ. Circ.’ Nov. 16, 2 pp.; ‘Nature,’ lv. 352 (Abs.); ‘Beiblitter,” xxi. 512 (Abs.) ‘ Astrophys. J.’ v. 99-100 ; ‘Bleiblitter,” xxi. 518 (Abs.) ‘ Astrophys. J. iii. 89-113; ‘Beibliitter, xxi. 339 (Abs.) ‘Astrophys. J! v. 95-96 ; ‘ Beiblatter” xxi. 521 (Abs.) eS a ee J. N. Lockyer A. Fowler . P.deHeen , J. N. Lockyer F. McClean E. C. Pickering A. Schuster ” O W. W. Campbell J. E. Keeler . P.deHeen . Sir J. N. Lockyer . H. F. Newall. C. A. Young . J. Evershed . J. E. Keeler . Sir W. Huggins ON THE BIBLIOGRAPHY OF SPECTROSCOPY, 503 ASTRONOMICAL APPLICATIONS, 1897. On the Iron Lines Present in the Hottest Stars. Preliminary Note. (Read Feb. 18.) The Chemistry of the Stars. (March.) Photographie de la chromosphére du soleil, et constitution de cet astre. (Read March 6.) On the Chemistry of the Hottest Stars. (Read March 25.) Note on Comparative Photographic Spectra of Stars to the 33 Magni- tude. (Read March 25.) Stars having Peculiar Spectra. (March.) Note on the Chemical Constitution of the Stars. (Read March 25.) Oxygen in the Sun, (March) (April) Spectroscopic Observations of Mars in 1896-7. (May.) Note relative 4 la photographie de Yatmosphére solaire. (Read June Spectroscopic Notes. 5.) The Approaching Eclipse of the Sun. (June.) The Total Solar Eclipse of Aug. 9, 1896. Report on the Expedition to Kid Island. (Read June 17.) On the Classification of Stars of the 5 Cephei Class, (Read June 17.) On the Appearance of the Cleéveite and other New Gas Lines in the Hottest Stars. (Read June 17.) On some Spectroscopic Determina- tions of Velocity in the Line of Sight made at the Cambridge Observatory. (Read June 11.) On the Reversing Stratum and its Spectrum, and on the Spectrum of the Corona. (Aug.) The Corona Spectrum. (Sept.) Measurement by means of the Spectroscope of the Velocity of Rotation of the Planets. (Read Sept. 23.) Sur les spectres des composantes colorées des étoiles doubles. (Read Oct. 11.) ‘Proc. Roy. Soe.’ Ix. 475~ 476; ‘Nature,’ lv. 452- 453; ‘ Beiblitter, xxi. 520 (Abs.); ‘J. Chem. Soc.’ Ixxii, II. 469 (Abs.) ‘Knowledge, xx. 77-78; ‘Nature,’ ly. 447 (Abs.) ‘Bull. Acad. Belg.’ [3], xxxili. 205-210. ‘Proc. Roy. Soe.’ Ixi. 148- 209. * Proc. Roy. Soe.’ lxi. 213- 216 ‘Harvard Coll. Observ. Circ” No. 17, 2 pp. ‘Proc. Roy. Soc.’ lxi. 209- 213. ‘ Astrophys. J.’ v. 162-163. ‘ Astrophys. J.’ v. 233-242. ‘ Astrophys. J.’ v. 328-3 ‘Bull. Acad. Belg.’ [3], Xxxili. 800-803. 154-157, ‘Nature, Ivi. 175-178. ‘Proc. Roy. Soc.’ Ixi, 444- 445 (Abs.) ‘Proc. Roy. Soc.’ Ixi. 445- 455. *Proc. Roy. Soc.’ lxii. 52— GT. ‘Monthly Not. R. A. S$? lvii. 567-577. 155-— ‘Astrophys. J.’ vi. 157. ‘Nature,’ lvi. 444. ‘ Brit. Assoc. Report,’ 1897, 729-731. °C. RY cxxv. 512-514. 504 REPORT—1898. ASTRONOMICAL APPLICATIONS, 1897-METEOROLOGICAL APPLICATIONS, 1891, Sir W. Huggins R. J. Aitken . A. Belopolsky E. C. Pickering J. NR. Rydberg W. W. Campbell J. M. Schaeberle \ ad 7. H. Wright A. Belopolsky G. E. Hale H. F. Russell A. Crova A. Fowler . G. Miiller 0 G. Meyer . 1892, 18938, 1894. Sur les spectres des étoiles princi- pales du trapéze de la nébuleuse dOrion. (Read Oct. 11.) Variations in the Spectrum of the Orion Nebula. (Nov.) New Investigation of the Spectrum of B Lyre. (Nov.) Spectrum ofa Meteor. (Nov.) On the Constitution of the Red Spectrum of Argon. (Nov.) On the Variations observed in the Spectrum of the Orion Nebula. (Nov.) Observations of the Spectrum of the Orion Nebula. (Nov.) Variations in the Spectrum of the Orion Nebula. (Nov.) Researches on the Spectrum of the Variable Star 7 Aquile. (Dec.) On the Presence of Carbon in the Chromosphere. (Dec.) | Motion of some Stars in the Line of Sight. (Report of the Cambridge Observatory.) yt. °C, R.’ exxv. 514-51 ‘ Astrophys. J.’ vi. 365. ‘Astrophys. J.’ vi. 337. ‘Harvard Coll. Obs. Cire.’ (Nov. 20); ‘Nature,’ lvii. 101; ‘Science Abstr.’ i. 4 (Abs.) ‘Astrophys. J. vi. 338- 348; * Beiblitter,’ xxii. 154 (Abs.) ‘Astrophys. J.’ vi. 363- 864; ‘Science Abstr.’ i. 4 (Abs.) 328- ‘ Astrophys. J.’ vi. 364— 365. ‘Astrophys. J.’ vi. 365- 366. ‘Astrophys. J. vi. 393- 399. ‘Astrophys. J. vi. 412- 414; ‘Nature,’ lvii. 374 (Abs.) ‘Nature,’ lvi. 270 (Abs.) METEOROLOGICAL APPLICATIONS. 1891. The Analysis of Diffused Light. (‘ Amer. Meteorol. Journ.’ Nov. 1891.) 1892. Spectrum of Lightning. (July) 1893. | Photometrische und spectroscop- ische Beobachtungen angestellt auf dem Gipfel des Siintis. 1894. Ein Versuch das Spectrum des Blitzes zu photographiren (Feb.) ‘Nature, xiv. 189-190 (Abs.) ‘Nature,’ xlvi. 268; ‘ Bei- blitter,’ xvii. 125-126 (Abs.) ‘Publ. d. Astrophys. Obs. Potsdam, viii. 1-101; ‘ Beiblitter, xvii. 1063- 1065 (Abs.) ‘Ann. Phys. u. Chem,’ [N.F.], li. 415-416; ‘ Nature,’ xlix. 427 (Abs.); ‘Phil. Mag.’ [5], xxxvil. 420-421 (Abs.) x » % 4 _— = ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 505 METEOROLOGICAL APPLICATIONS, 1895, 1896, 1897 CHEMICAL RELATIONS, M. Berthelot. O. Simong A. Ricco L. E. Jewell . T. G. Eakins . G. Henslow . J. W. Briihl . 1885, 1890, 1891, 1892. Remarques sur les spectres de |‘C. RR. cxx. Yargon et de Vaurore boréale. (Read March 235.) Ueber periodische Aufnahmen des Sonnenspektrums vom Gipfel des Piks von Teneriffa (3711 m.) (‘Verhandl. Ges. Naturf. u. Aerate,’ II. 1. Hiilfte (1895), 85.) 1896. Righe spettrali atmospheriche os- servate sull’ Etna, a Nicolosi in Catania. (June.) The Determination of the Relative Quantities of Aqueous Vapour in the Atmosphere by Means of the Absorption Lines of the Spectrum. (Dec.) 1897. Dr. Arendt’s Spectroscopic Investi- gation of the Variation of Aqueous Vapour inthe Atmosphere. (April.) ‘VEEL, CHEMICAL RELATIONS. 1885. On Allanite and Gadolinite (‘ Proc. Colorado Sci. Soc.’ li. 1885). 1890. A Contribution to the Study of the Relative Effects of Different Parts of the Solar Spectrum on the Assimilation of Plants (‘ Proc. Linnean Soc.’ Noy. 6, 1890). 1891. Untersuchungen tiber die Terpene und deren Abkimmlinge (‘ Ab- handl.’ III. 1V.) (Read Oct. 29, Nov. 18.) 1892. Untersuchungen iiber die Terpene und deren Abkémmlinge (‘Ab- handl.’ VIII. IX.) (Read May 23.) 662-663 ; ‘Ber, xxviii. (Ref.), 318 (Abs.) ; ‘ Beiblatter,’ xix. 567 (Abs.); ‘ Proc. Phys. Soc.’ xiii. 289 (Abs.); ‘J. Chem. Soc.’ Ixvili. II. 337 (Abs.); ‘Nature,’ li. 552 (Abs.) ‘ Beibliitter, xix.[59](title) ‘Mem. spettr. ital.’ xxv. 127-134; ‘ Beiblitter,’ xx. 978 (Abs.); ‘ Nature,’ liv. 280-281 (Abs.) ‘Astrophys. J.’ iv. 324- 342; ‘Nature,’ lv. 258 (Abs.) ‘Astrophys. J.’ v. 279. 281. ‘Chem. News,’ lili. 282; ‘J. Chem. Soc.’ 1. 779 - 780 (Abs.) ‘Nature,’ xliii. 72 (title). ‘Ber’ xxiv. 3373-3416, 3701-3737; ‘ Beiblitter,’ xvii. 30-32 (Abs.) ‘Ber’ xxv. 1788-1796, 1796-1813; ‘ Beibliatter,’ xvii. 30-32 (Abs.) 506 REPORT—1898. CHEMICAL RELATIONS, 1892, 1893. J. W. Briihl . Ueber Dipropargyl und Benzol. (Read July 20.) Ueber Oxyaurine und Oxyaurincar- bonsiuren. II. Mittheilung. (Read Aug. 11.) Zur Kenntniss der Oxazinfarbstoffe. (Read Oct. 6.) Methods of Observing the Spectra of easily Volatile Metals and their Salts, and of Separating their Spectra from those of the Alkaline Earths. (Read Dec. 1.) N. Caro. - : R. Nietski and A. Bossi. W. N. Hartley 1893. . | A Revision of the Atomic Weight of Barium. (Read Jan. 11.) T. W. Richards J. M. Eder and E. | Ueber das Emissionspectrum der Valenta. elementaren Silicium, und den spectrographischen Nachweis dieses Elementes. (Read Jan. 19.) Some Remarks on the Examination of the Rare Gadolinite Earths, and in particular on Determining the Equivalents of these Earths by converting the Oxide into the Sulphate. (Jan.) The Spectrum of Iron and the Periodic Law. (Jan.) G. Kriiss 5 J. Parry. . “i Untersuchungen iiber asymme- trische Bicarbonsiiuren. (Read Feb. 6.) Spectrochemie des Stickstoffs. I. (Vorliufige Mittheilung.) (Read Mar. 27.) Sul tiophosgene polimero. May 7.) J. W. Briihl . ” e G. Carrara. (Read G. Gennari . dell indene. (Read May 20.) Ueber die Molecularrefraction stickstoffenthaltender Substanzen (Aldoxime und Ketoxime). Read | June 8.) C, Trapesonzjanz C. Graebe and A. | Ueber Oxyderivate des Anthra- Philips. chinolinchinon. (Sept.) - | Spettrochimica del cumarone e | ‘ Ber.’ xxv. 2638-2646 ‘Ber’ xxv. 2671-2675. ‘ Ber.’ xxv. 2994-3005. ‘J. Chem. Soe.’ Ixiii. 138- 141; ‘Chem. News,’ Ixvi. 313 (Abs.) ‘Proc. Amer. Acad.’ xxviii. 1-30; ‘Chem. News, Ixviii, 232-233, 269-271, 283-284. ‘Wien. Anz.’ xxx. (1893), 19-21. ‘Chem. News,’ Ixvii. 32- 33, 40-42. Y ‘Nature,’ xlv. 253-255; ‘Beiblatter,’ xvii. 748— 749 (Abs.) ‘Ber.’ xxvi. 337-345. ‘Ber’ xxvi. 806-809. ‘Rend. R. Accad. d. Lincei’ [5], ii. I.sem. 421-425 ; ‘Beiblatter, xviii. 334— 335 (Abs.) ‘Rend. R. Accad. d. Lin- cei’ [5], iii. I. sem. 499- 503; ‘Gazz. chim. ital.’ xxiv. I. 468-474; ‘ Bei- bliitter,’ xviii. 907 (Abs.) *Ber” xxvi. 1428-1433; ‘ Beiblitter, xviii. 335- 336 (Abs.) ‘Ann. Chem. u. Pharm.’ eclxxvi. 21-35; ‘J. Chem. Soc.’ Ixiv. I. 670-671 (Abs.) J. W. Briihl . V. Schumann : F. Tiemann and P. Kariiger. F. Tiemann and Fr. W. Semmler. J. Verschaftelt R. Nasini and F., Anderlini. R. Nasini and G. Carrara, J. W. Briihl . A. Ghira : ; G. Gennari . H. A. Rowland . THE BIBLIOGRAPHY OF SPECTROSCOPY. 507 CHEMICAL RELATIONS, 1893, 1894. Ueber einige EHigenschaften und die Constitution des freien Hy- droxylamins und seine Homologen. Spectrochemie des Stickstoffs. II. (Read Oct. 14.) Ueber ein neues Verfahren zur Herstellung ultraviolettempfind- liche Platten. (Read Oct. 12.) Ueber Oct. 9.) Veilchenaroma. (Read Ueber Verbindungen der Citral- (Geraniol-)Reihe. (Read Oct. 9.) 1894. Application du réfractométre 4 Yétude des réactions chimiques. (Read Jan. 6.) Sul potere rifrangente dei com- posti continenti il carbonile. (Read Jan. 21.) Sul potere rifrangente dell’ ossi- geno, dello zolfo, e dell’ azoto nei nuclei eterociclici. (Read Feb. 22.) Neue Beitriige zur Frage nach der Constitution des Benzols. (Read Mar. 27.) Potere rifrangente delle combina- zioni organo-metalliche. (Read April 15.) Spettrochimica del camarone e dell’ indene. (Read May 10.) The Separation of the Rare Earths. (May.) | | | ‘Ber,’ xxvi. 2508-2520. ‘Sitzungsb. Akad. Wien, cli. Il.a, 994-1024; ‘Bei- blitter,’ xviii. 456-457 (Abs.) ‘ Ber,’ xxvi. 2675-2708. ‘Ber.’ xxvi. 2708-2729. | ‘ Bull. Acad. Roy.de Belge,’ [3], xxvii. 49-84; ‘ Bei- blitter,’ xviii. 746-747, 833-834 (Abs.) ‘Rend. R. Accad. d. Lincei’ [5], iii. I. sem. 49-58; ‘Gazz. chim. ital.’ xxiv. I. 157-169 ; ‘Ber.’ xxvii. (Ref.), 244 (Abs.) ; ‘ Bei- blitter,’ xviii. 665 (Abs.) ‘Gazz. chim. ital.’ xxiv. I. 256-290; ‘Zeitschr. f. physikal. Chem.’xvii. 539- 544; ‘Proc. Phys. Soc.’ xiii. 397 (Abs.); ‘J. Chem. Soc.’ Ixvi. II. 302-303 (Abs.); ‘ Ber.’ xxvii. (Ref.), 375-376 (Abs.) ; ‘ Beiblatter,’ xviii. 834 (Abs.) ‘J. prakt. Chem.’ [2], xlix. 201-294; ‘Ber? xxvil. 1065-1083 ; ‘ Nature,’ xlix. 614 (Abs.); ‘J. Chem. Soe.’ Ixvi. I. 366- 367 (Abs.) ‘Rend. R. Accad. d. Lincei’ [5], iii. I. sem. 391-393; ‘Gazz. chim. ital.’ xxiv. I. 324-327; ‘ Beiblitter,’ xviii. 906-907 (Abs.) ‘Rend. R. Accad. d. Lincei’ [5], ili. I. sem. 499-503 ; ‘Gazz. chim, ital. xxiy. I. 468-474. ‘ Johns Hopkins Univ. Cir- cular, xiii. 73-74 ; ‘ Chem. News, lxx. 68-69; ‘J. Chem. Soc.’ Ixvi. TI. 449- 550 (Ahs.) 508 A. de Gramont W. Crookes . : W. N. Hartley Mecke and Wimmer (. Haacke A. Rtard K. Schunck W. Ramsay P. F. Cléve H. Moissan A. de Gramont G. Kriiss and H. Kriiss. A, de Gramont M. Konowalow H. Rigollot . REPORT—1898. CIEMICAL RELATIONS, 1894, 1895. Sur le spectre de lignes du soufre, et sur sa recherche dans les com- posés métalliques. (Read July 2.) The Separation of the Rare Earths. (Aug.) New Methods of Spectrum Analy- sis, and on SBessemer Flame Spectra. (Aug.) Nachweise von Blutflecken. (Nov.) Spectrophotometrische Untersuch- | ungen tiber die Hinwirkung von Salzsiiure auf einige Substitutions- producte des Fuchsins. (Diss. Ttibingen, 1894, 49 pp.) 1895. Pluralité des chlorophylles. _Deux- iéme chlorophylle isolée dans la luzerne. (Read Feb. 11.) Contributions to the Chemistry of Chlorophyll. (Read Feb. 14.) Discovery of Helium. (Read Mar. 27.) Sur la présence de l’hélium dans la clévéite. (Read April 16.) Action du fluor surl’argon. (Read May 9.) Analyse spectrale directe de miné- raux. (June.) Eine neue Methode der quantita- | tiven Spectralanalyse. (June.) Sur l’analyse spectrale directe des minéraux et de quelques sels fondus. (Read July 8.) Nitrirende Wirkung der Salpeter- siiure auf den Character gesittigten Verbindungen besitzende Kohlen- wasserstoffe und deren Derivate. (Read July 29.) Action des rayons infra-rouges sur le soufre d’argent. (Read July 15.) ‘C. R. cxix. 68-70; ‘ Bei- blatter,’ xviii. 912 (Abs.); ‘Chem. News,’ Ixx. 49 (Abs.); ‘J. Chem. Soc.’ Ixvi. II. 434-435 (Abs.) ‘Chem. News,’ lxx. 81-82. ‘ Brit. Assoc. Rep.’ 1894, 610-611 ; ‘ Beibliitter,’ xx. 26 (Abs.) ‘Zeitschr. f. anal. Chem, xxxiv. 129-131; ‘Chem. News,’ lxxi. 238. ‘ Beiblitter,’ xx. 64 (title). °C. BR. exx, 328208)" oo. Chem. Soc.’ lxviii. I. 389 (Abs.) ‘Proc. Roy. Soc.’ lvii. 314- 322.. ‘J. Chem. Soe.’ lxvii. 1207— 1108; ‘Chem. News,’ lxxi. 151; ‘ Ber.’ xxviii. (Ref.), 839 (Abs.); ‘ Beibliitter,’ xix. 624 (Abs.) ‘C. RY exx. 834; ‘ Ber.’ xxviii. (Ref.), 373 (Abs.) ; ‘Nature, li. 622-623 (Abs.); ‘Chem. News,’ Ixxi, 212. ‘ Proc. Roy. Soe.’ lviii. 120- 121. ‘Bull. Soc. frang. de Min,’ xviii. 171-374. ‘ Zeitschr. f. anorg. Chem.’ x. 31-43. Cy BR.” sexxi, @ZIE123: ‘ Beiblatter, xx. 30-31 (Abs.) ; ‘J. Chem. Soc.’ lxviii. II. 470-471 (Abs.); ‘Chem. News,’ lxxii. 103 (Abs.) ‘Ber.’ xxviii. 1852-1865. ‘C.°R’ exxi. 164-166 ; ‘ Ber.’ xxix. (Ref.), 63-64 (Abs.) C. Runge and F. Paschen. W. Ramsay C. Bouchard . G. Kriiss and H. Kriiss. J. W. Briihl . H. Wilde 2 R. Mohlau and K. Uhlmann, DB. Paulowski. E, Schunck and L. Marchlewski. A. Killas and W. Ramsay. A, de Gramont THE BIBLIOGRAPHY OF SPECTROSCOPY. 509 CHEMICAL RELATIONS, 1895. Bestandtheile (Read July 11.) Ueber die Cléveitgases. A Possible Combination of Argon. (Aug.) . | Sur la présence de l’argon et de Vhélium dans certaines (Read Sept. 2.) eaux minérales. Eine neue Methode der quantita- tiven Spectralanalyse. (Sept.) Spectrochemie des Stickstofts. II. IV. (Read Oct. 1.) Helium and its Place in the Natural Classification of Klemen- tary Substances. (Read Oct. 1.) Zur Kenntniss der Chinazin- und | Oxazinfarbstoffe. (Oct.) Ueber Allofluorescein. 14.) (Read Oct. Zur Chemie des (Oct.) Chlorophylls. Estimation of Gases from Certain Mineral Waters. (Read Noy. 28.) Sur l’analyse spectrale directe des composés solides, et plus spéciale- ment des minéraux. (Noy.) des | CK ORE mete ‘Sitzungsb. Akad. Berlin, EXxIVe| (O9= (Oo od. Chem. Soc.’ Ixx. II. 1-2 (Abs.) ‘Chem. News,’ Ixxii. 51; * Beiblatter,’ xix. 730 (Abs.) ; ° Ber.’ xxviii. (Ref.), 839-840 (Abs.) ; ‘J. Chem. Soc.’ Ixx. II. 20 (Abs.) 392-394 ; ‘ Beiblitter, xix. 827 (Abs.); ‘ Ber.’ xxviii. (Ref.),836 (Abs.) ; ‘Chem. News,’ - Ixxij. 152-153 ; ‘Proc. Phys. Soc.’ xiii. 456 (Abs.); ‘J. Chem. Soc.’ Ixx. II. 99 (Abs.) CXxi. ‘ Zeitschr. f. anorg. Chem.’ x. 31-43; ‘ Beiblatter,’ xx. 26), (Abs: SoRroe: Phys. Soc.’ xiv. 14 (Abs.); ‘J. Chem. Soc.’ Ixx. II, 215 (Abs.); ‘Ber.’ xxix. (Ref.), 147-148 (Abs.) ‘Ber.’ xxviii. 2388-2406 ; ‘Zeitschr. f. physikal. Chem.’ xvi. 193-225, 226— 241, 497-611, 512-524; ‘ Beibliitter, xix. 564— 565 (Abs.) ; ‘ Proc. Phys. Soc.’ xiii. 328-330 (Abs.); ‘J. Chem. Soc.’ Ixviii. IT. 194, 250-251 (Abs.) ‘Phil. Mag.’ [5], xl. 466— 471; ‘J. Chem. Soc.’ lxx. II. 165-166 (Abs.) ‘Ann. Chem. u. Pharm.’ e¢lzxxix,) 128130): «s, Chem. Soc.’ xx. I. 166— 169 (Abs.) ‘ Ber.’ xxviii. 2360-2362. ‘Ann. Chem. u. Pharm.’ eclaxxix, Sl-—lO@sauah. Chem. Soc.’ Ixvili, I. 896- 397 (Abs.) ‘Proc. Roy. Soc.’ lix. 68— 69. ‘Os, Rep (Gree leei23 ‘Bull. Soc. Chim.’ [3], xlii._xiv. 945-947 ; ‘ Ber.’ xxviii. (Ref.), 1048 (Abs.) 510 Li ‘Troost’ and Lie} Ouvrard. G. Kriiss ° ° Rk. F. d’Arcy and W. B. Hardy. J. Stas. A : L. Marchlewski . E. Schunck and L. Marchlewski J. W. Briihl . = J. Landauer . ° G. Kraemer and A. Spilker. E. Jiinger and A. Klages. J.W. Briihl . oa REPORT—1898. CHEMICAL RELATIONS, 1895, 1896. Sur Vorigine de JVargon et de Vhélium dans les gaz dégagés par certaines eaux minérales. Dec. 2.) Beziehungen zwischen Zusammen- setzung und Absorptionsspectrum organischen Verbindungen. Nach- trag. (Dec.) Note on the Oxidising Powers of Different Regions of the Spectrum in relation to the Bactericidal Action of Light and Air. Recherches chimiques et études spectroscopiques sur différents corps simples. (Complete works of Stas, pub. at Brussels.) 1896. Die Chemie des Chlorophylls. (Hamburg, 82 pp.) (Jan.) Contributions to the Chemistry of Chlorophyll ; Phylloporphyrin and Heematoporphyrin: a comparison. (Read Jan. 30.) Spectrochemische des a- Claisen. (Feb.) Die Spectral-Analyse. schweig, 174 pp.) (Feb.) (Braun- Ueber das Cyclopentadien im Stein- | kohlentheer, das Indin der Fett- | reihe. (Read Feb. 24.) Ueber Halogenderivate des Cam- phens und Hydrocamphens. (Feb.) Spectrochemische Untersuchung des a- und 8-Formylphenylessig- esters. (Vorliufiger Bericht.) (March.) (Read | Untersuchung | und £-mesityloxidoxal- | siiuren Methyls und Aethyls von | (Vorlaufiger Bericht.) | ‘6. RB. Sexxing TOB=800 |: ‘Chem. News,’ lxxii. 309— 310. ‘Zeitschr. f. physikal, Chem.’ xviii. 559-563 ; ‘ Beiblatter” xx. 197 (Abs.); ‘J. Chem. Soc.’ lxx. II. 285 (Abs.) | ‘J. Physiol.’ xvii. 390-393 ; ‘J. Chem. Soc.’ Ixviii. II. 57 (Abs.) ‘Chem. News,’ Ixxii. 177— 179, 188-190, 203-205, 215-216, 226-227, 239- 241, 248-251, 259-261, 274-276, 301-304, 311- BZy Ixxiil bat ees, 29-31, 39-40, 51-52, 66— 68, 80-81, 88-90, 113- 114, 124-126, 135-137, 147-149, 159-161, 171- 173, 183-184, 192-193, 204-206, 216-218, 224- 225, 241-242, 249-250, 262-264. ‘Chem. News,’ Ixxiii. 23 (Review). ‘Proc. Roy. Soc.’ lix. 233- 239, ‘Ann. Chem. u. Pharm.’ cexci. 137-146 ; ‘ Bei- bliitter, xx. 871 (Abs.) ‘Chem. News,’ Ixxiii, 70- 71 (Review). ‘ Ber.’ xxix. 552-561. | ‘ Ber.’ xxix. 544-547. ‘Ann. Chem. u. Pharm.’ ccxe. 217-225; * Ber.’ | xxix. (Ref.), 484 (Abs.); * Beiblatter, xx. 871 (Abs.) ¥. Tiemann and R. | Ueber Schmidt. ” ” KH. Demarcay. ee H. Ritthausen B.Tollens , : W. N. Hartley . E. Schunck and L. Marchlewski A. Tschirch , H. Wilde . W.N. Hartley and H. Ramage. O. Buss . ‘ F) H. Kriiss A < E. Wiedemann and E. Riegler . : > ; G. C, Schmidt. : E. Schunck and L. Marchlewski. ON THE BIBLIOGRAPHY OF SPECTROSCOPY. oll CHEMICAL RELATIONS, 1896. die Verbindungen der | ‘ Ber.’ xxix. 903-926. Citronellalreihe. (Read March9.) | Ueber Homolinalool, (Read | ‘ Ber.’ xxix. 691-695. March 9.) Sur un nouvel élément contenu dans | ‘C. R.’ cxxii. 728-730; les terres rares voisines du sama- rium. (Read Mar. 23.) Ueber Galactit aus den Samen der gelben Lupine. (Read March 23.) Ueber den Nachweis der Pentosen mittels der Phloroglucinsalzsiiure- absatzmethode. (Read April 18.) The Determination of the Compo- sition of a ‘White Sou’ by a Method of Spectrographic Analy- sis, (Read April 23.) Zur Chemie des Chlorophylls. (Read May 11.) Zur Chemie des _ Chlorophylls. (Read June 22. On the Spectral and other Pro- perties of Thallium in Relation to the Genesis of the Elements. (June. ) On the Occurrence of Gallium in the Clay-iron-stone of the Cleveland District of Yorkshire. Determina- tion of Gallium in Blast-furnace Iron from Middlesbrough. (Read Dec. 17.) Beitriige zur Spectralanalyse eini- ger toxicologisch und pharma- kognostisch wichtiger Farbstoffe, mit besonderer Beriicksichtigung’ des Ultraviolett. Ueber ein neues Verfahren in der quantitativen Spectralanalyse (‘ Verhandl. Ges. Deutsch. Naturf. u. Aerzte, II. 1. Hiilfte, 76-77.) Die Bestimmung des Alkokols und Extractes im Wein auf optischem Wege. Cnaug. Diss.) Photochemische Zersetzung von NaCl, KCl, NaBr und KBr unter dem Einfluss von starkbrechbaren ultrayvioletten Lichte. Zur Chemie des Chloropbylls. (IV. Abhandlung.) ‘Ber. xxix. ((Ref.);e00= 380 (Abs.); ‘J. Chem. Soc.’ Ixx. II. 475 (Abs.); ‘Proc. Phys. Soc.’ (Abs.) xiv. 226. ‘ Ber.’ xxix. 896-899. ‘ Ber.’ xxix. 1202-1209. ‘J. Chem. Scc.’ Ixix. 842- 844: ‘Chem. News, lxxili, 229 (Abs.) ° Ber.’ xxix. 1347-1352. ‘Ber.’ xxix. 1766-1770. ‘Chem. News,’ xxiii. 304— 305; ‘Beiblatter, xxi. 633 (Abs.) ‘Proc. Roy. Soc.’ lx. 393— 407. ‘ Beiblatter, xxi. 130-131 (Notice). ‘ Beiblitter,’ xx. (title). [31] ‘ Zeitschr. f. anal. Chem.’ RkKVee iol; © ber xx (Ref.), 599 (Abs.) ‘Jahrb, f. Photogr.’ x, 15. ‘Ann. Chem. u. Pharm. cecxc. 306-313; ‘ Ber.’ xxix. (Ref.), 415 (Abs.) A. Wroblewsky W. N. Hartley and H. Ramage. K.D.Chruschtschoft G. Urbain and E. Budischovsky J. W. Brihl W.N. Hartley and H. Ramage. — 4, Lewin — i= B. Hasselberg I. Knoevenagel REPORT—1898. CHEMICAL RELATIONS, 1896, 1897. Anwendung des Glan’schen Spectro- photometers auf die Tierchemie. I. Quantitative Bestimmung des Hamoglobinsim Blute. II. Quan- titative Bestimmung der Rhodan- salze im Speichel (‘Anz. Akad. Krakau,’ 1896, pp. 306-309, 386- 390). 1897. On the Dissemination of some of the Rarer Elements, and the Mode of their Association in Common Oresand Minerals. (Read Jan. 21.) On the Spectrographic Analysis of some Commercial Samples of Metals, of Chemical Preparations, and of Minerals from the Stass- furt Potash Beds. (Read Feb. 18.) Sur les terres de monazite. (Read March 18.) Recherches sur les sables mona- zités. (Read March 22.) Spectrochemie des Stickstoffs. V. (April.) A Spectrographic Analysis of Iron Meteorites, Siderolites, and Me- | teoric Stones. (Read May 19.) (‘ Proc. Roy. Soc. Dublin’ [N.S.], viii. Part 6.) Die spectroscopische Blutunter- | suchung. (June.) | | | Note on the Chemical Composition | of the Mineral Rutile. (June.) in der hydro- Untersuchungen | (June.) aromatischen Reihe. ‘Chem. Cenir.’ 1897, ii. 532 (Abs.); ‘ Beibliitter,’ xxi. 573 (Abs.) | ‘J. Chem. Soc.’ xxi. 533-— 547; ‘Chem. News,’ lxxix, 129-130 (Abs.) ‘J. Chem. Soc.’ lxxi, 547- 550; ‘Chem. News,’ Ixxv. 151(Abs.); ‘ Chem.Centr,’ 1897, I. 665 (Abs.) ‘J. Russ. Phys. Chem. Soc.’ xxix. 206-208; ‘ Chem. Centr.’ .1897, II. 329 (Abs.) ;_ ‘ Nature,’ lvi. 276; ‘ Beiblitter, xxi, 920 (Abs.) “C. R., cxxiv. 618-621); ‘Chem, News,’ Ixxv’181- 182. ‘Zeitschr. f. physikal. Chem.’ xxii. 373-409 ; «J. Chem. Soc.’ lxxii, II. 297 (Abs.) ; ‘ Beiblitter,’ xxi. 586-588 (Abs.); ‘Chem. Centr. 1897, II. 81-83 (Abs.) ‘ Nature,’ lvii, 546 (Abs.) ; ‘Chem. News,’ Ixxvii. 121-122. * Arch. der Pharm.’ cexxxv. 245-255 ; ‘Chem. Centr.’ 1887, II. 381 (Abs.); ‘J. Chem. Soc.’ Ixxii. II. 534 (Abs.) ‘ Astrophys. J.’ vi. 23-26; ‘Chem. News,’ Ixxvi.102— 104; ‘ Chem. Centr.’ 1897, Il. 712 (Abs.) ‘Ann. Chem. u. Pharm.’ cexcvii. 113-203 ; ‘Chem. Centr.’ 1897, II. 696-702 (Abs.) ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 513 CHEMICAL RELATIONS, 1897—THEORETICAL PAPERS, 1890, 1891, 1892. R. Lespieu Recherches sur les épidibrom- hydrines et les composés propar- gyliques. (June.) J. R. Rydberg The New Series in the Spectrum of Hydrogen. (Oct.) H. Wilde . Sur les poids atomiques de l’argon et de Vhélium. (Nov.) B. Hasselberg Ueber das Vorkommen des Vanads | in den Scandinavischen Rutilarten (‘ Bihang till Handl. Svensk. Vet. Akad.’ xxii. I. No. 7, 7 pp.) Sur la nature des gaz obtenus des deux minéraux ceritiques du Caucase. G. P. Tschernik Z. Donoginy . . Die Darstellung des Hiimochromo- | gens als Blutreaction, mit beson- derer Beriicksichtigung des Nach- weises von Blut im Harn. H. Tornée Spectrometrisch - ariometrische Bieranalyse. (‘ Pharm. Centr.-H.’ XXXViii. 871-873.) TX. THEORETICAL PAPERS. 1890. Ueber die specifische Brechung-, Volumen- und Refractionsaquiva- lente von sieben aus C, H und O bestehenden Fliissigkeiten, nach den Formeln von Beer (Landolt), Lorenz, und Ketteler. (Inaug. Dissert. Bonn, 1890, 53 pp.) M. Korten 1891. On the Determination of the Orbit of a Double Star from Spectro- scopic Observation of the Velocity of the Components in the Line of Sight. (March.) A. A, Rambaut 1892. C. Runge and G. J. | The Line Spectra of the Elements. Stoney. (Letters.) (May.) | G. J. Stoney . | On the Line Spectra of the Ele- ments. (July.) 1898. ‘Ann, Chim. et Phys.’ [7], xi. 232-288; ‘ Chem. Centr.’ (1897), II. 180- 183 (Abs.) ‘Astrophys. J.’ vi. 238; ‘ Beiblatter,’ 153 (Abs. ). °C, RY exxv. 649-651 ; ‘J. Chem. Soc.’ Ixxiv. II, 115 (Abs.) ‘ Astrophys. J.’ v. 194-198. 233— XXii. ‘J. Russ, Phys. Chem. Soc.’ xxix. 291-302; ‘Chem. Centr.’ 1897, II. 674-675 (Abs.) ‘Arch. f. Anat. u. Physiol.’ exlviii. 234-243; ‘J. Chem. Soc.’ Ixxii. II. 468 (Abs. ) ‘Chem. Centr.’ 1897, I. 270-271. ‘ Beiblatter,’ xiv. 769-772 (Abs.) ‘Monthly Not. Roy. Astr. Soc.’ li, 316-330, ‘Nature,’ xlvi. 29, 100, 126, 200, 247, 268; ‘ Bei- blatter, xviii. 559-560 (Abs.) ‘Nature,’ xlvi. 268-269. LL 514 R. R. Tatnall. W.J.Sollas . R. Nasini - &G, W. Colles . M. Aymonnet M. Kuhfahl 8. Pagliani . H.C. Vogel . A. Cornu e C. Runge . ° R. Lehmann-Filhés G. Moreau , H. Rubens , R. Nasini i Ph. A. Guye . a REPORT—1898. THEORETICAL PAPERS, 1892, 1893, 1894. A New Proof of a Fundamental Equation of the Spectrometer, (Dec.) 1893. The Law of Gladstone and Dale as an Optical Probe. (Read Jan. 18.) Sul potere rifrangente per un raggio di lunghezza d’ onda infinita, (Read Feb. 19.) Distances of the Stars by Doppler’s Principle. (April.) Sur les mawima périodiques des spectres. (Read Aug. 7.) Die Ablenkung des Strahles beim Prisma. (Aug.) Sulle equazioni della refrazione della luce. (Read Aug. 20.) Ueber die Bezeichnung der Linien des I. Wasserstoffsspectrums. (Nov.) Vérifications numériques relatives aux propriétés focales des réseaux diffringents plans. (Read Dec. 26.) 1894. On a Certain Law in the Spectra of some of the Elements. (Feb.) Ueber die Bestimmung einer Dop- pelsternbahn aus _ spectroscopi- schen Messungen der im Visions- radius liegendenGeschwindigkeits- componenten. (July.) De la périodicité des raies d’absorp- tion des corps isotropes. (Read Aug. 20.) Priifung der Ketteler-Helmholtz’- schen Dispersionsformel. (Aug.) Coefficiente critico in relazione n—1 (Read formula Sept. 14.) Détermination du poids moléculaire des liquides. (Read Nov. 12.) colla ‘Astron. and Astrophys.’ xi. 932-933; ‘ Beiblitter,’ xvii. 824-825 (Abs.) ‘Proc. Roy. Soc. Dubl.’ EN.S.], __vili. = 4572166 (Abs.); ‘ Beiblatter,’ xviii. 995-996 (Abs.) ‘Rend. R. Accad.d. Lincei’ [5], ii. I. sem. 161-166 ; ‘Beiblitter, xvil. 739 (Abs.) ‘Amer. J. Sci.’ [3], xlv. 259-267. ‘C. R.’ exvii. 304-306, 402- 405; ‘ Nature,’ xlviii. 536 (Abs.) ‘ Zeitschr. f. phys. u. chem. Unterr.’ vi. 301. ‘Rend. R. Accad. d. Lincei’” [5], ii. II. sem. 107-112. ‘ Astr. Nachr.’ cxxxiv. 95- 96; ‘Nature,’ xlix. 162 (Abs.) *‘C. R. cxvii. 1032-1039 ; ‘Nature, xlix. 239-240 (Abs.) ‘Astron. and Astrophys.’ xiii. 128-130. ‘ Astr. Nachr.’ cxxxvi. 17- 30. ‘OC, R. exix, 422-425; ‘Beiblitter, xix. 494 (Abs.) ; ‘ Proc. Phys. Soc.’ xiii. 108-110 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], iii. 266-286 ; ‘Nature,’ 1. 635 (Abs.) ; ‘Naturwiss. Rundschau,’ ix, 389-391. ‘Gazz. chim. ital.’ xxiii. II. 576-587; ‘J. Chem. Soc” Ixvi. II, 173-174 (Abs.) ‘C, RY cxix. 852-854; ‘J. Chem. Soc.’ lviii. II. 99 (Abs.) ee W. F. Edwards G. Lippmann . G. F. Fitzgerald A. Konig H. Rubens F. Paschen H. Poincaré R. Reiff . F. Zecchini B. Galitzin G. J. Stoney ON THE BIBLIOGRAPHY OF SPECTROSCOPY. ol cr THEORETICAL PAPERS, 1894, 1895. A New Formula for Specific and Molecular Refraction. (Dec.) Sur la théorie de la photographie des couleurs simples et composées par la méthode interférentielle. 1895. On some Considerations showing that Maxwell’s Theorem of Equal Partition of Energy among the Degrees of Freedom of Atoms is not inconsistent with the various Internal Movements exhibited by the Spectra of Gases. (Read Feb. 14.) Ueber die Anzahl der unterschied- baren Spectralfarben und Hellig- keitsstufen. (Feb.) Die Ketteler-Helmholtz’sche Dis- persionsformel. (Feb.) Dispersion und Dielectricititscon- stante. (March.) Sur le spectre cannelé. (Read April 8.) Zur Dispersionstheorie. (May) Sopra una nuova formola per espri- mere la rifrazione specifica dei liquidi. (Read July 9.) Zur Theorie der Verbreiterung der Spectrallinien. (Aug.) On Motions competent to produce Groups of Lines which have been observed in Actual Spectra. (Read Sept. 13.) ‘ Amer. Chem. J.’ xvi. 625- 634; ‘J. Chem. Soc.’ lxviii. II. 193 (Abs.); ‘ Ber, xxviii. (Ref.), 452 (Abs.); ‘Beiblatter,” xix. 420 (Abs.); ‘Chem. Centralb.’ 1895, i. 313-314. ‘J. de Phys.’ [3], iii. 97- 107; ‘Proc. Phys. Soc.’ xiii. 63-64 (Abs.) ‘Proc. Roy. Soc.’ lvii. 312- 313; ‘Nature,’ li. 452- 453. ‘ Zeitschr. f. Psychol. u. Physiol. d. Sinnesorgane,’ viii. 375-680. ‘Ann. Phys. u. Chem.’ [N.F.], liv. 476-485; ‘Proc. Phys. Soc.’ xiii. 258 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], liv. 668-674; ‘Proc. Phys. Soc.’ xiii. 284 (Abs.) SC? GRe i oxx: 7572762: * Beiblatter, xix. 788~- 789 (Abs.) ; ‘Nature,’ li. 599 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F-], lv. 82-94, ‘Gazz. chim. ital.’ xxv. II. 269-284 ; ‘J. Chem. Soc.’ lxx. II. 285 (Abs. ‘Ann. Phys. u. Chem.’ [N.F.], lvi. 78-99; ‘Na- ture,’ lii. 611 (Abs.) ‘Brit. Assoc. Rep.’ 1895, 610-612; ‘Chem. News,’ lxxii, 225-226; ‘Bei- bliatter,’ xx. 531, 691-692 (Abs.) LL2 T.F.F.See . E. v. Lommel A. Garbasso H. Steigmiiller Wilsing . A. Belopolsky J. Larmor E. Carvalho W. Wien C. G. Abbott and F. E. Fowle. L. Rummel J. Traube é * H. Steigmiiller REPORT—1898. THEORETICAL PAPERS, 1895, 1896 Theory of the Determination by means of a Single Spectroscopic Observation of the Absolute Di- mensions, Masses, and Parallaxes of the Stellar Systems whose Orbits are known from Micro- metrical Measurements; with a Rigorous Method for Testing the Universality of the Law of Gravi- tation. (Oct.) Verbreiterung der Spectrallinien. Continuirliches Spectrum. Damp- fungsconstante. (Nov.) | Sulla luce bianca. Beziehung der Brechungsexponen- ten isotroper Substanzen aus Molecularformel und specifischem Gewicht derselben. (Vorliufige Mittheilung.) (Stuttgart, 1895.) Zur homocentrischen Brechung des Lichtes im Prisma. 1896. Spectrographische Untersuchungen liber Jupiter. (Jan.) On the Absolute Minimum of Optical Deviation by a Prism. (Read Feb. 24.) Sur l’absorption de la lumiére par les milieux doués du pouvoir rota- toire. (Read May 4.) Ueber die Hnergievertheilung im Emisslonsspectrum eines schwart- zen Korpers. (July.) The Longitudinal Aberration of a Prism. (Oct.) Spectra of the Alkalies. (Read Nov. 12.) (‘ Roy. Soc. Victoria,’ 1896, 260-263.) Lichtbrechung und Dichte. XV. (Read Nov. 23.) Beziehung der Brechungsexpon- enten organischer Fliissigkeiten aus Molecularformel und speci- fischem Gewicht derselben. (Stutt- gart, 1896, 24 pp.) ‘Astron. and Astrophys.’ xii, 812-815; ‘Astr. Nachr.’ cxxxix. 18-26; ‘Nature,’ iii, 15-16 (Abs.) ; ‘ Beiblitter, xx. 370 (Abs.) ‘Ann. Phys. u. Chem, [N.F.], lvi. 741-745. ‘Atti d. R. Accad. d. Torino, xxx. 186-192; ‘Il Nuovo Cimento’ [4], i. 305, 307 (Abs.); ‘Proc. Phys. Soc.’ xiii. 312 (Abs.) : ‘Beiblatter,’ xx. 528-529 (Abs.) ‘Zeitschr. f. Math. u. Phys.’ xl. 353-362. ‘ Astr. Nachr.’ cxxxix. 209- 214; ‘Beiblatter, xxi. 342 (Abs.) ‘Proc. Phil. Soc. Camb.’ iv. 108-110. ‘C. R. cxxil. 985-988; ‘ Beiblatter, xxi. 35-36 (Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], lviii. 662-669. «Amer. J. Sci.’ [4], ii. 255- 257; ‘Beiblatter, xxi. 407 (Abs.) ‘Beiblitter, xxi, 937 (Abs.) ‘ Ber. “xxix: 2732-2742; ‘Beiblatter, xxi. 509- 510 (Abs.) ‘ Beibliitter,’ xxi. 28 (Abs.) A P. Lugol A. 8. Herschel J. Traube J. Larmor G. F. Fitzgerald A. Anderson . H. Poincaré J.J. Balmer . L. Rummel F. L. O. Wadsworth A. Garbasso . T. M. Thiele . H. Becquerel . J. Larmor A. Garbasso and G. Garbasso. Minimum de THE BIBLIOGRAPHY OF SPECTROSCOPY. 517 THEORETICAL PAPDRS, 1897. déviation dans le prisme. The Rydberg-Schuster Law of Ele- mentary Spectra. (Jan.) Ueber die Atomrefractionen von Kohlenstoff, Wasserstoff, Sauer- stoff, Stickstoff und den Haloge- nen. XVI, XVII. (Read Jan. 11.) The Influence of a Magnetic Field on Radiation Frequency. (Read Feb. 11.) | Note on a Cause for the Shift of Spectral Lines. (March.) On the Maximum Deviation of a Ray of Light by a Prism. May 25.) (Read | La théorie de Lorentz et les expé- riences de Zeeman. (June.) Eine neue Formel fiir Spectral- wellen. (Read June 7.) (‘ Ver- handl. Naturforsch.-Gesellsch. Basel,’ 1897, Heft 3, 448-463.) On the Spectra of the Alkalies and their Atomic Weights. (Read June 10.) (‘Roy. Soc. Victoria,’ 1897, 75-78.) Ueber das Auflésungsvermogen von Fernréhren und Spectroscopen fiir Linen von endlicher Breite. (June.) ' Sul modo di interpretare certe es- perienze del Signor P. Zeeman di Leida. (July.) On the Law of Spectral Series. (Aug.) Sur une interprétation applicable au phénoméne de Faraday et au phénoméne de Zeeman. (Read Nov. 8.) On the Theory of the Magnetic Influence on Spectra, and on the Radiation from Moving Ions. (Dec.) Sur la forme de la perturbation dans un rayon de lumiére solaire (‘Arch. de Genéve ’ (1897), iii. 105— 113), ‘J. de Phys.’ [3], vi. 21-23 ‘Nature, lv. 271. ‘Ber.’ xxx. 38-47; ‘ Bei- blaitter, xxi. 510-511 (Abs.) ‘Proc. Roy. Soc.’ lx. 514- 515. J. V. ‘ Astrophys. 210— 211. ‘Proc. Phil. Soc. Camb.’ ix. 195-197 ; ‘ Beiblatter, xxi. 406-407 (Abs.) ‘ Eclairage Electrique,’ xiii. 481-489. ‘Ann. Phys. u. Chem.’ [N.F.], lx. 380-391 ; ‘ Na- ture,’ lv. 137-188; ‘ As- trophys. J.’ ¥. 199-209. ‘ Beiblitter,’ xxi. 973(Abs.) ‘Ann. Phys. u. Chem.’ [N.F.], lxi. 604-620. ‘Il Nuovo Cimento’ vi. 8-14; ‘Eclairage Elec- trique,’ xiii. 276-277. ‘ Astrophys. J.’ vi. 65-76. °C. RY’ cxxv. 679; ‘J. de Phys.’ [3], vi. 681-688. ‘Phil. Mag.’ [5], xliv. 503- 513. ‘Beiblitter, xxi. 123 (title). REPORT—1898. List of the Chief Abbreviations used in the above Catalogue. Abbreviated Title. Amer. J. Sci. Ann. Agron. Ann, Chem. u. Pharm. Ann. Chim et Phys. Ann. de Chim. . 4 Ann. Obs. Bruxelles Ann. Phys.u.Chem.[N. FJ Arch. de Genéve Arch. f. Anat. u. Phy siol. Arch. f. d. gesammte Physiol. Arch. f. exper. Pathol. u. Pharmakol. Arch, néerland. Astr. Nachr. Astrophys. J. . Attid. R. Accad. d. Lincei Beiblatter : ; Ber. . Bied. Centr. Bot. Zeitung Bull. Astron. Bull. Soc. Chim. Bull. Soc. Min. de France Bull. Acad. Belg. Chem. Centr. GC, Rz Denkschr. "Akad. Wien. Dingl. J. . A Gazz. chim. ital. Gottingen. Nachr. Handl. Svensk. Vet. Akad. Jahrb, f. Photogr. . Chem. Soc. . J. de Phys. . Physiol. . prakt. Chem. 3 . Russ. Phys.-Chem. Soe. Cy C4 Cy cy . Soc. Chem. Ind. . Soc. frang. de Phys. Math. u. naturwiss. Ber. aus Ungarn. Mem. spettr. ital. Monatsb. Akad. Berl. oy cy Monatsh. f. Chem. Month. Not. R.A.S. . Oefvers. af K. Vet. Akad. Forh. Full Title. American Journal of Science (Siiliman’s). Annales Agronomiques. Annalen der Chemie und Pharmacie (Liebig). Annales de Chimie et de Physique. Annales de Chimie. Annuaire de l’Observatoire de Bruxelles. Annalen der Physik und Chemie [Neue Folge] (Wiedemann). Archives des Sciences Physiques et Naturelles (Genéve). Archiy fiir pathologische Anatomie und Physiologie und fiir klinische Medicin (Virchow). Archiv fiir die gesammte Physiologie (Pfliiger). Archiv fiir experimentelle Pathologie und Pharmakologie. Archives néerlandaises des Sciences exactes et natu- relles (Haarlem). Astronomische Nachrichten. The Astrophysical Journal (Chicago). Atti della Reale Accademia dei Lincei. Beiblaitter zu der Annalen der Physik und Chemie (Wiedemann). Berichte der deutschen chemischen Gesellschaft. Biedermann’s Centralblatt fiir Agriculturchemie. Botanische Zeitung. Bulletin Astronomique (Observatoire de Paris). Bulletin de la Société Chimique de Paris. : Bulletin de la Société Minéralogique de France, Bulletin de Académie royale des Sciences, des Lettres et des Beaux-Arts de Belgique. Chemisches Centralblatt. Comptes Rendus de l’Académie des Sciences (Paris). Denkschriften der Akademie der Wissenschaften in Wien (Mathematisch-naturwissenschaftliche Classe). Dingler’s polytechnisches Journal. Gazzetta chimica italiana. Nachrichten von der Georg-August-Universitiit und der k6nigl. Gesellschaft der Wissenschaften (Gottingen). Handlingar K. Svenska Vetenskaps Akademiens (Stock- holm). Jahrbuch fiir Photographie (Eder). Journal of the Chemical Society of London. Journal de Physique. Journal of Physiology. Journal fiir praktische Chemie. Journal of the Russian Physico-Chemical Society (in Russian). Journal of the Society of Chemical Industry. Journal de la Société frangaise de Physique. Mathematische und naturwissenschaftliche Berichte aus Ungarn. Memorie della Societa degli spettroscopisti italiani. Monatsberichte der Akademie der Wissenschaften zu Berlin. Monatshefte fiir Chemie (Wien). Monthly Notices of the Royal Astronomical Society of London. Oefversigt af K. Svenska Vetenskaps Akademiens Fér- handlingar. ON THE BIBLIOGRAPHY OF SPECTROSCOPY. 519 List of the Chief Abbreviations—continued. Abbreviated Title. Phil. Mag. 5 Phil. Trans. . Phot. Mittheil. Phys. Review Phys. Revue . Proc. Phys. Soc. Proc. Roy. Inst. Proc. Roy. Soc. 5 Rec. des. trav. chim. des Pays-Bas. Rend. R. Accad. d. Lincei Riv. sci. industr. . Sitzungsb. Akad. Berl. Sitzungsb. Akad. Miinchen Sitzungsb. Akad. Wien Sitzungsb. phys.-med. Soc. ‘Erlangen. Skand, Arch. f, Physiol. . Verh. phys. Gesellsch. Berlin. Wien. Anz. ' . Zeitschr. f. anal. Chem. Zeitschr. f. anorg. Chem. . Zeitschr. f. Kryst. u. Min. Zeitschr, f. physikal.Chem. Zeitschr. f. phys. u. chem. Unterr. Zeitschr. f. physiol. Chem. Zeitschr. f. wiss. Micro- scopie. Full Title. London, Edinburgh, and Dublin Philosophical Mazazine. Philosophical Transactions of the Royal Society of London. Photographische Mittheilungen (Vogel), Physical Review. Physikalische Revue. Proceedings of the Physical Society of London. Proceedings of the Royal Institution of Great Britain. Proceedings of the Royal Society of London. Recueil des travaux chimiques des Pays-Bas. Rendiconti della Reale Accademia dei Lincei. Rivista scientifico-industriale. Sitzungsberichte der Akademie der Wissenschaften zu Berlin. Sitzungsberichte der kéniglich baierischen Akademie zu Miinchen. Sitzungsberichte der Akademie der Wissenschaften zu Wien. Sitzungsberichte der phys.-medicinischen Societit zu Erlangen. Skandinavisches Archiv fiir Physiologie (Leipzig). Verhandlungen der physikalischen Gesellschaft zu Berlin, Anzeiger der k. Akademie der Wissenschaften zu Wien. Zeitschrift fiir analytische Chemie, Zeitschrift fiir anorganische Chemie. Zeitschrift fiir Krystallographie und Mineralogie. Zeitschrift fiir physikalische Chemie. Zeitschrift fiir physikalischen und chemischen Unterricht. Zeitschrift fiir physiologische Chemie. Zeitschrift fiir wissenschaftliche Microscopie. Lhe Fossil Phyllopoda of the Paleozoic Rocks.—Fourteenth Report of the Committee, consisting of Professor T. WILTSHIRE (Chawman), Dr. H. Woopwarp, and Professor T. Rurert JONES (Secretary). (Drawn up by Professor T. Rupert JONES.) ConrTENTS. SECTION PAGE I. Dithyrocaris: species and distribution. . 519 II. Dipeltis, as defined by Schuchert, not a Phyilapod « 521 Il. A. Pritsch’s Bohemian Estheria : 521 $ I. In our First Report on the Paleozoic Aaa (presented to the Association in 1883) the genus Dithyrocaris was included in the Tabular List at page 216 of the Reports for 1883 (1884), as being ‘ ridged along the back (like Apus),’ and as ‘being ridged and sometimes prickled.’ It was referred to as occurring in Carboniferous and Devonian strata. _ In the Fifth Report (made in 1887), at page 63-66, we enumerated all the known and reputed species of the genus. Thanks to the obliging courtesy of friends and correspondents, we are now enabled to state that we can distinguish the following species found in the British Islands and elsewhere :— 520 REPORT—1898. Polynoe, Lepidonotus, Sigalion, Sthenelais, Aphrodite, Halosydna, Nereis, Nephthys, Glycera, Capitella, Terebella, Cheetopterus, and one of two: undetermined Sabellids. Ophryotrocha and larve of Terebella and of Polyophthalmus were also experimented with. The method was that of Ehrlich as modified by Allen (‘Q.J.MS.,’ ON THE MARINE BIQLOGICAL LABORATORY, PLYMOUTH. 585 1894), and the stain as fixed by the ammonium molybdate solution (after Bethe’s recipe). The preparations were dehydrated and cleared by slow diffusion into xylol or cedar-wood oil. At first I employed an injection of a ‘1 per cent. solution of methylene-blue, but I soon found that better results could be obtained by rapidly dissecting out the nervous system and watching the progress of the stain under the microscope. The best temperature for rapid staining of unaltered nerve-fibres is about 65° F., while in passing the preparations through alcohol a low temperature is advisable, otherwise the stain is liable to be washed out. Nereis, Polynoe, and Halosydna gave the best results. The elements of the nerve-cord of Wereis diversicolor, though delicate, are rapidly stained before the fibres have time to ‘bead.’ The number and arrange- ment of the nerve-elements in this species are still occupying my attention. Unfortunately only a couple of specimens of Halosydna gelatinosa were obtained during my stay at Plymouth. The somewhat short nervous system, the ease with which it can be exposed, and the stoutness of many of the fibres, are great advantages in dealing with this species. With regard to the tubicolous Polychets, my experience agrees with that of other observers. The method that gives excellent results in Nereis, at the same time and under the same conditions, fails to stain differentially the elements of the cord in Arenicola or Chetopterus. Out of a large number of preparations of Arenicola Grubii a few only show the course of a small number of nerve-fibres. I hope, however, by modifying the stain to obtain better results than heretofore. In conclusion, I wish to tender my sincere thanks to Mr. E. J. Allen, the Director of the Plymouth Laboratory, for placing the resources of the laboratory at my disposal, and especially for his kind assistance and advice. Report on Mr. J. H. Wanvswortn’s collection of material for the Study of the Embryology of Alcyonium. By Professor 8. J. Hickson, F.R.S. On arriving at the laboratory on December 31, Mr. Wadsworth found in one tank (which I will call Tank I. in this report) sixteen healthy colonies of Alcyonium, which had been placed there twenty-four hours previously by Mr. Allen. The water in this tank contained a number of embryos in different stages of development up to the stage they reach in twenty-four hours. These were all removed and preserved, some in corrosive subli- mate and acetic acid, some in Hermann’s fluid, and some in Mix. No. 3 (chloroform, acetic acid, and absolute alcohol). In another tank (Tank II.) there were about sixty colonies, many of which were not in a healthy condition. In the water of this tank there were numerous embryos, some of which were clearly abnormal and unhealthy. Thirty- six of the colonies from this tank were removed to fresh sea-water in Tank IIT. . During his stay at Plymouth Mr. Wadsworth collected at different times the embryos that were found free in the water of these three tanks, and preserved them in various reagents, noting, in each case, carefully the time that had elapsed since the water was free from embryos. On January 3 a female colony was placed in a bell jar by itself, a quantity of ripe sperm was added to the water, and Mr. Brown’s agitator employed for keeping the water in the bell jar in motion. Some of the embryos shot out by this specimen were preserved ten hours afterwards in the corrosive-acetic mixture, the remainder were isolated and pre- 586 REPORT—1898. served, some on January 5, at 10.30 a.m., in Hermann, others on J. anuary 5, at 8.10 p.m., in No. 3 mixture. The use of this method was not, on the whole, satisfactory, as many of the embryos obtained in the last series were clearly moribund ; but as some of the oldest embryos of the series were perfectly healthy, and show beautiful karyokinetic figures in the sections, it is probable that renewed experiments with it would be successful. Another female colony, together with a male colony, were isolated in a bell jar which was allowed to float in one of the tanks. The embryos collected from this were at first healthy, but after twenty hours the water became foul and the embryos died. These two experiments, to isolate individuals and to endeavour to obtain the exact ages of the embryos and others that were tried, have given me some data, but cannot be said to have been thoroughly satis- factory. Mr. Wadsworth’s time during his stay at the laboratory was very largely occupied in collecting and preserving the embryos that were found free in the large tanks, and these have yielded some very fine series, the most successful of which are those preserved in Rabl’s fluid and in the No. 3 mixture. Before leaving the laboratory Mr. Wadsworth cut open a number of female colonies and preserved the eggs from the ecelentera. Since Mr. Wadsworth’s return a very large number of complete series of sections through the embryos have been cut, stained, and mounted, and I have carefully examined them, making notes and drawings of interesting points. As the work is not yet finished, and there are still many speci- mens to examine, it would be premature to do more than to point out some of the results of the investigation. These results are given only provisionally, and will be subjected to confirmation or the reverse before being finally published with the illustrations. 1. The ovum of Aleyonium is never fertilised before it leaves the body of the parent. 2. Soon after leaving the polyp the ovum enlarges, probably by the absorption of water, and the membranes covering it are broken and lost. 3. The nucleus which is at the edge of the ovum diminishes in bulk, and is then dissi- pated and lost to view. No karyokinetic figures accompany these changes in the nucleus. JI may add here that these observations confirm the results I have obtained from material collected in the winters 1893-4, 1895-6, 1896-7. 4. Another nucleus, much smaller than the germinal vesicle, may be found in the ovum in what appear to be later stages. This is accom- panied by archoplasm (?), and travels towards the centre of the ovum and then fragments. 5. Segmentation is very irregular in Alcyonium, as it is in Renilla, according to Wilson. Sometimes embryos with four, eight, or an irregular small number of well-defined blastomeres are to be found, but more fre- quently—perhaps normally—no segmentation occurs for some time, and then the embryo segments into twenty or more tightly-packed blastomeres, the outlines of which cannot be seen from the outside at all. 6. In all the well-preserved embryos which are segmented the nuclear structure is clear and definite, and in most of my series beautiful karyo- kinetic figures may be seen in one or more of the segments. 7. A complete series of the later stages of development up to the time of the formation of the mouth has been obtained. This series will be studied when the earlier stages have been more satisfactorily worked out. : $ % 4 i % * 5 THE ZOOLOGICAL STATION AT NAPLES. 587 Occupation of a Table at the Zoological Station at Naples.—Report of the Comnuittee, consisting of Professor W. A. HERDMAN, Professor EK. Ray Lanxester, Professor W. F. R. WeEtpon, Professor S. J. Hickson, Mr. A. SEp@wick, Professor McInroso, Mr. W. E. Hoy e, and Mr. Percy SLavEn (Secretary). APPENDIX PAGE I—The Pseudobranch and Intestinal Canal of Teleosteans. By JAMES F.GEMMILL 3 - ; : é é : é : . 588 Il.—(1) The Relations between Marine Animal and Vegetable Life in Aquaria. By H.M. VERNON . : : : : : ; . 589 (2) The Relations between the Hybrid and Parent Forms of Echinoid Larve. By H.M. VERNON . A 589 IIl.— On the Variation of Cardium, Donax, and Tellina. By J. PARKINSON 593 IV.— List of Naturalists who have norked at the Zoological Station from July 1, 1897, to June 30,1898 . i , 5 és 3 : . 594 V.—List of Papers which were published in 1897 by Naturalists who have occupied Tables in the Zoological Station . c 3 : - 595 Tue table in the Naples Zoological Station hired by the British Associa- tion has been occupied during the past year by Mr. James F. Gemmill, Mr. H. M. Vernon, and Mr. J. Parkinson. Mr. Gemmill, who occupied the table from August 20 to November 12, was engaged in investigating certain points in the anatomy of the osseous fishes. Mr. Vernon held the table from October until the middle of January, and continued his investigations on the conditions of animal life in marine aquaria, with a view to determine the relations existing between marine animal and vegetable life. Mr. Vernon also made careful experimental researches on the relations between the hybrid and parent forms of echinoid larve. Mr. Parkinson occupied the table from October 25 to April 26, and devoted himself to the investigation of the variation of certain lamelli- branchs. Each of these gentlemen has furnished a report upon the work done, which will be found appended. Your Committee has again to remark with gratitude on the kindness of Professor Dohrn in allowing the terms of occupancy in these cases to run concurrently, at least during part of each period. Without this courteous treatment on the part of Professor Dohrn, the Committee would have been unable to meet the wishes of the several workers. An application for permission to use the table during the ensuing year has been received from Mr. H. Lyster Jameson, for the purpose of making investigations on the anatomy of the Gephyrea. He wishes to go to Naples at the beginning of October and to remain six months. This application is recommended by your Committee, and they trust that the General Committee will sanction the payment of the grant of 100/., as in previous years, for the hire of the table in the Zoological Station at Naples. The progress of the various publications undertaken by the station is summarised as follows :— 1. Of the ‘Fauna und Flora des Golfes von Neapel’ no monograph 588 REPOoRT—1898. has been published during the past year, but several are in course of preparation. 2. Of the ‘Mittheilungen aus der zoologischen Station zu Neapel,’ vol. xli., part 4, with 12 plates; and vol. xiii., part 1, with 11 plates, have been published. 3. Of the ‘ Zoologischer Jahresbericht,’ the Bericht for 1896 has been published. 4, A new Italian edition of the ‘Guide to the Aquarium’ has been published. The details extracted from the general report of the Zoological Station, which have been courteously furnished by the officers, will be found at the end of this report. They embrace lists (1) of the naturalists who have occupied tables since the last report, and (2) of the works published during 1897 by naturalists who have worked at the Zoological Station. I.—The Pseudobranch and Intestinal Canal of Teleosteans. By James F, GEMMILL. I occupied a table at the Naples Zoological Station between the end of August and the beginning of November, 1897. My work there had to do mainly with certain points in the anatomy of the osseous fishes ; in particular, with the distribution, structure, and development of the pseudo- branch, and with the intestinal canal. Over fifty species of teleosteans were examined. A. Pseudobranch. 4 As far as the general anatomy and relations of this organ are con- cerned, I could only, in the case of the greater number of species examined, go over ground which was worked out long ago by Joh. Miller. Records were, however, made for a certain number of species not included in his list. But in every case, which was carefully examined, the great fact established by Joh. Miller that the pseudobranch is supplied by oxygenated blood was found to hold good. Comparative details as to the presence and degree of modification of the pseudobranch were specially noted whenever possible in allied species and genera. In this connection the flat fishes were found to form an interesting group. On the whole a good series of stages was obtained, illustrating on the one hand the gradual disappearance of the organ in question, and on the other its passage from a free projecting condition to one in which it is encapsuled and glandular. The microscopical structure of the organ was investigated in a certain number of species. The results obtained agree in the main with what had been previously described, but there was also found in some cases (e.g. Serranus gigas), external to the layer of large polygonal cells which lies superficial to the capillaries in each lamella, another layer of flattened scale-like cells. These persist even when the pseudobranch becomes encapsuled and glandular, though in that case they do not form a continuous stratum, but are represented by scattered squamous cells lying between adjacent lamellz. A study of the development of the gland in Hippocampus brevirostris and Syngnathus acus by the method of serial sections of embryos was begun. The lophobranch group was chosen for investigation, because in the adults of this group the pseudobranch presents every appearance of THE ZOOLOGICAL STATION AT NAPLES. 589 being in uninterrupted series with the ordinary gills ; that is to say, it lies far back, being just in front of the first permanent gill cleft, and it shows the characteristic tufted structure of the lophobranch gill. I was unable at the time to complete my observations on its development, but they were advanced enough to convince me that the conclusion arrived at for other osseous fishes by Joh. Miller and Anton Dohrn held good also for the lophobranchs—namely, that the pseudobranch originates in front of the hyomandibular cleft and groove, and that therefore it is homo- logous so far with the spiracular pseudobranch found in many of the cartilaginous fishes. B. Intestinal Canal. The intestinal canal of osseous fishes is well known for its extreme variability in regard to length windings and mesenteric relations. I hoped by studying these points in the comparatively large number of species placed at my disposal to be able to define the characteristic tendencies in the way of morphology which might be expected to be shown by a series of examples ranging from the simpler to the more complex forms of intestinal tube. As a result, I have come to these conclusions for all the fishes I examined : 1. That in any given case the anatomy of the intestinal tube can be regarded either as corresponding directly to, or as being easily derivable from, some one out of a small number of typical forms. 2. That the typical forms themselves constitute a natural series, of which the more complex members can readily be derived from the simpler. Not the least interesting part of my observations had to do with the changes in the morphological scheme indicated above that are produced in the case of certain groups which vary in general form more or less con- siderably from the ordinary piscine type, e.g. in the pleuronectids, which are flattened laterally, or in Lophius Piscatorius, where the flattening is dorsoventral, kc. Here also must be included those fishes which have the vent carried forward to the front of the abdomen. In all these cases the modified course of the intestinal tube can still be referred to one or other of the typical forms indicated above, by taking in each instance the special factors at work into consideration. In addition to investigation, one of the objects of my visit to Naples was to get some knowledge@f the working of a marine zoological station. For furthering this, as well as for every assistance in work, I have to acknowledge the kindness and courtesy of the station staff. I consider it a very great privilege to have occupied a table at the Naples Zoological Station, and I hereby tender my sincere thanks to the Committee of the British Association for having afforded me that privilege. II.—(1) The Relations between Marine Animal and Vegetable Life in Aquaria ; (2) The Relations between the Hybrid and Parent Forms of Echinoid Larve. By H. M. Vernon. In the report which I furnished last year, I described the work on which I had been engaged during my occupancy of the British Association table at Naples between the months of April and June. I continued to work at the Zoological Station till the middle of the following January, but I only held the British Association table from October onwards, I 590 REPORT—1898. being transferred to the Oxford table during July, August, and September. As it is scarcely possible to describe only those portions of the work I was engaged upon when occupying the British Association table, I will now furnish a brief report of the whole of the work I undertook during my stay at Naples. In my last year’s report I stated that I was investigating the condi- tions of animal life in marine aquaria. I continued to work on this subject for several months, and have embodied my results in a paper which will shortly be published in the ‘ Mittheilungen aus der zoologischen Station zu Neapel,’ and which is entitled ‘The Relations between Marine Animal and Vegetable Life.’ An abstract of the paper has already been published.! It is on this account unnecessary to describe the research in any detail ; but I should like to take this opportunity of drawing attention to thescope and practical bearing of the work, as it might thereby be brought to the notice of some persons who are interested in the subject, but who, judging from the title of the paper, might imagine it did not concern them. Thus the original object of the work was to determine how the nitrogenous matter excreted by marine animals into the water is removed, and what parts the various forms of vegetable life and other agencies play in the process. This subject is of interest from its practical bearing on questions relating to the efficient maintenance of marine aquaria, whilst from the theoretical standpoint it is of importance to our comprehension of the changes taking place under natural conditions in the open sea. The method of investigation was a triple one—viz., chemical, physiological, and bacteriological. The chemical procedure consisted in determining the free and ‘albuminoid’ or organic ammonia present in the water by the well- known method of Wanklyn, Chapman, and Smith. The physiological procedure consisted in allowing the fertilised ova of the sea-urchin (Strongylocentrotus lividus) to develop in the various specimens of water, and then, after eight days’ growth, killing and measuring the larve in groups of fifty, in order to determine the changes produced in their size. The bacterial quality of the water was tested by counting the number of colonies obtained on gelatin plate culture. The three chief vegetable agencies concerned in the purification of the water are—(1l) the macroscopic alge ; (2) the diatoms and microscopic alge ; (3) the bacteria. It was concluded that under natural conditions in the open sea the bacteria form the most important of these purifying agencies. Thus, as considerably the larger portion of the water of the ocean extends to depths such that no trace of light can penetrate, it follows that no chlorophyll containing organism can exert an influence on it. As B. Fischer? has shown, however, bacteria are everywhere present. Now it was found that if the impure aquarium water was kept in darkness for about three weeks, it might become as pure, in respect of the ammonia it contained, as open sea water collected 10 kilométres from the shore. Judged by the physiological standard, however, it was not nearly so pure. Thus larve grown in it were on an average only 7°5 per cent. larger than those grown in the impurified aquarium water, whilst those grown in the open sea-water were 16°0 per cent. larger. In marine aquaria it seems probable that bacteria play a considerable part in maintaining the purity of the water, even though the water may be stored for but very short periods ! Proc. Roy. Soc. vol. \xiii. p. 155. 2 « Ergebnisse der Plankton Expedition der Humboldt-Stiftung,’ Die Bakterien des Meeres (Ed. iv. M.g.) “refpied ~ diag THE ZOOLOGICAL STATION AT NAPLES. 591 in dark reservoirs, where the bacteria can most efficiently exert their in- fluence. Thus, at Naples, it was found that the pipes conducting the water from the reservoirs to the rooms were coated internally with a layer of bacterial slime, and that in its passage along these pipes the water under- went considerable purification. For instance, water drawn off from one of the taps was found to contain from 26 to 82 per cent. less free ammonia and from 16 to 25 per cent. less organic ammonia than the water in the supplying reservoir. Also, larvae grown in such water were increased about 7°8 per cent, in size. Probably, in marine aquaria, a more powerful purifying influence than the bacterial is exerted by the diatoms and minute alge. Thus sand collected from the bottom of one of the tanks was found to be impregnated with this vegetable growth, which clung to each grain and particle. On filtration of aquarium water through this sand, no less than 94 per cent. of the free ammonia, and 18 per cent. of the organic, were removed. Again, on filtering water in a continuous stream through a layer of sand which originally contained no vegetable matter, this matter was gradually deposited from the water, and the sand gradually developed a capacity for purification which became more and more marked with time. Such a vegetable filter is very sensitive to any variation in the flow of water. Thus, if the rate of flow were diminished from the maximum of one litre in three minutes to one litre in fifty minutes or more, there was no longer any purification, but the amount of freeammonia in the water was increased about threefold. This result is of some practical importance. It teaches us that the layer of slime which is deposited on the bottom and sides of the tanks of marine aquaria, and which consists largely of diatoms and algx, is a most valuable purifying agent, provided it be in layers thin enough for an adequate amount of water to circulate to all parts cf it. Once, however, the lower layers are insufficiently supplied, they begin to decompose, and become a source of contamination. It was found that a sand filter, even when kept for weeks in darkness, continued to exert a purifying influence. In this case the influence must have been due to bacteria, and not to chlorophyll containing organisms. This bacterial filter acted most efficiently with a slower rate of filtration, and was not nearly so sensitive to a diminution or cessation in the flow of water. With regard to the purifying agency of the macroscopic alge, experiments were made on the purifying effects of green weeds such as Ulva, and of red weeds such as Gelidewm. Their action was not found so favourable as that of diatoms and minute alge, and of bacteria, in con- sequence of the difficulty experienced in getting them to live healthily in the impure aquarium water. To the other results obtained it is not possible to refer here at any length. Thus the action of sunlight on the water was investigated, it being found that though an immediate germicidal effect was brought about, the ultimate effect, on withdrawal of the adverse influence, was slight or absent. Again, the effects of increased aération were investi- gated, but the influence exerted appeared to be but slight. Numbers of experiments were made upon the fouling effects of various animals on the water. As a rule, larve grown in water fouled by most organisms were increased in size by, on an average, 4:1 per cent., whilst in water fouled by sea-urchins they were diminished in size by 6°9 per cent. Fish and crabs appeared to effect about ten times as much contamination of the water as molluscs and holothurians, whilst dead and 592 REPORT—1898. putrefying sea-urchins effected about ten times as much contamination as did the various living animals examined. In the full paper are given numerous determinations of the specific gravity of the aquarium water, and of the amounts of ammonia and nitrites present ; also experiments on the effects of introducing various salts into the water. To these it is unnecessary to refer here. During the last two or three months of my stay at Naples I was working on another subject, ‘The Relations between the Hybrid and Parent Forms of Echinoid Larve,’ but I had also been making occasional experi- ments on this subject whilst engaged on the research just described. I also worked out some of the material obtained on my return to England. An account of this work is in course of publication in the ‘ Phil. Trans. Roy. Soc.’, an abstract having already appeared in the ‘ Proc. Roy. Soe.’ vol. 63, p. 228. The object of the research was to determine systematically, during the nine months’ period I was working at Naples, the exact relationship of structure and size existing between certain hybrid and parent echinoid larval forms. Eight different species of echinoids were worked with, but the large number of observations were confined to three of them. Upon the cross Spherechinus 2 Strongylocentrotus ¢& twenty-two experiments were made, The hybrids were most easily obtained in the summer months, few or none of the ova being cross-fertilised in the winter. It was found that the majority of the hybrids obtained in May, June, and July were of an almost pure Sphere- chinus type, only a third or less of them being of an intermediate or Strongylocentrotus type. In November, on the other hand, only about a sixth were of the maternal and five-sixths of the paternal type. Finally, in December and January, all the hybrid larve were of the paternal type. As regards the reciprocal cross of Strongylocentrotus 9 and Sphere- chinus 6 a fair number of ova were cross-fertilised in April, May, and June, but no plutei were obtained. In July and August, on the other hand, 29 per cent. of the ova developed to eight days’ plutei. In November and December, with one exception, not only were no plutei obtained, but, as a rule, not a single ovum was cross-fertilised. These extraordinary variations in the capacity for cross-fertilisation seem to be due to varia- tions in maturity which the sexual products undergo with change of season. Thus in the summer months most of the Strongylocentrotus individuals contain but very small quantities of ripe sexual products or none at all. Also it was found that the normal plutei obtained in July and August were 20 to 30 per cent. smaller than those obtained in April and May, and also in November and December. At intermediate times the larve were of intermediate size. We see, therefore, that the Strongylocentrotus ° Spherechinus § hybrid is only formed at the time when the Strongylocentrotus ova have reached their minimum of maturity ; whiist in the case of the reciprocal hybrid it follows that as the maturity of the Strongylocentrotus sperm increases it is able to transform first a portion and then the whole of the hybrid larvee from the Spherechinus to its own type. In other words, the characteristics of the hybrid offspring depend directly on the relative degrees of maturity of the sexual pro- ducts. On crossing Hchinus 2 with Strongylocentrotus g it was found that even more of the cross-fertilised ova developed to plutei than of the directly fertilised ones, and also that these plutei were, on an average, 8 per cent. /arger than the pure parental larval forms. In the reciprocal THE ZOOLOGICAL STATION AT NAPLES. 595 eross, however, only about 1 per cent. of the ova reached the pluteus stage, and these plutei were 13-2 per cent. smaller than the pure maternal larve. Crosses were also effected between the forms mentioned and Arbacia pustulosa, Echinocardium cordatum, LEchinocardium mediterraneum, Dorocidaris papillata, and Echinus acutus. Also the various colour varieties of Sphwrechinus were crossed, a distinct diminution of fertility being found to exist between dissimilar varieties. With the colour varieties of Strongylocentrotus, however, this was not the case. In conclusion, I wish to offer my thanks to the Committee of the British Association for the privilege of being allowed to hold the table, as well as to the authorities at the Zoological Station at Naples for their invariable kindness and for the facilities they were able to afford me in my work. How great these were may be gathered from the fact that I was able to carry on the chemical, physiological, and bacteriological por- tions of my work simultaneously. As regards echinoid material also I was afforded an absolutely unlimited amount, and as regards the artificial fertilisations I was enabled, when necessary, to keep fifty or more large jars of plutei developing at one and the same time. III.—On the Variation of Cardium, Donax, and Tellina. By J. PARKINSON. It was my intention in visiting the Zoological Station at Naples during the winter of 1897-98—i.e. from November to April inclusive— to attempt an investigation on the reproduction of certain Ascidians. However, a short visit to Plymouth, with some subsequent study, early in last year raised sundry objections, and on reaching Naples in the begin- ning of November I gave up the subject which has just been mentioned, taking in its place the one which appears at the head of this report. I began upon the genus Arca, comparing the variation in certain propor- tions exhibited by the commoner species of that genus one with another, but found after several attempts that the confined space in which the animals grew, due to the nature of’ their attachment, raised great diffi- culties in the way of forming any true estimate of their natural variation. I then proceeded to the genus Cardium, and subsequently to the genera Donax and Tellina, comparing the variation in the chosen proportions of the several species one with another, as in the case of Arca. Here I was more successful ; but in finding a reasonably certain, and, at the same time, fairly quick method of measuring, as well as in overcoming the difficulty of obtaining definite points from which to measure, much time was spent. The work is now undergoing entire revision in the laboratory at University Ccllege, London. Material for subsequent investigation was also obtained from such experiments as the resistance of Pecten to diluted sea-water, but this has not yet been studied. Although a con- siderable number of measurements have been made, I have not at present reached that degree of certainty which makes it desirable that results should be given in length. It gives me great pleasure to testify to the extreme kindness shown by all the members of the station at Naples, especially to Signor Lo Bianco for the efforts he made to satisfy my rather large demands for material. To Professor Weldon my warmest thanks are gratefully given for the very kind help-he has afforded me not only by letter, but since I returned to England. In doing such work as that indicated above this has been simply invaluable. 1898. QQ 594 IV.—A List of Naturalists who have worked at the Zoological Station from REPORT— 1898. the end of June 1897 to the end of June 1898. Duration of Occupancy Arrival Departure Num- State or Institution ber on Naturalist’s Name whose Table List was made use of 970| Dr. D. Carazzi . Italy 971| Prof. F. 8. Monticelli * 972| Dr. F. Bottazzi. A 973| Dr. G. Mazzarelli ik 974| Dr. A. Romano . is 975| Dr. V. Diamare * S 976| Dr. A. Russo . - 977| Dr. F. Mazza 2 . 978} Dr. R. Hesse Wiirtemberg 979| Mr. J. F. Gemmill British Association 980} Prof. F. Ezokor Austria . : 981 | Prof. E. Drechsel Switzerland 982| Mr. K. R. Menon Cambridge 983| Dr. A.G. H. van Gen- | Holland . P deren-Stort . 984| Prof. G. B. Grassi | Italy F . 985| Prof. W. Krause | Prussia . 986} Stud. O. Fragnito | Italy 987| Dr. F. Doflein. . Bavaria . - 988} Dr. H. Driesch . Prussia 989| Dr. C. Herbst . “ - : A ° 990| Mr. K. A. Buddicom. | Oxford . ; 991} Dr. E. Albrecht . | Bavaria . 3 992) Mr. J. Parkinson British Association . 993] Dr. S. Metalnikoff Russia . 5 994| Dr. B. M. Davis . | Smithsonian Tnstit, aa 995| Dr. T. Beer . | Austria . ri 996| Dr. E. O. Hovey « | Columbia Table s 997| Dr. G. Duncker Hamburg : : 998| Baron J. Uexkiill Prussia . : : 999| Dr. T. Adensamer Austria . ‘ 1,000} Dr. W. Stempell Prussia 5 3 1,001) Prof. J. Nusbaum Austria . : 1,002} Stud. W. Schreiber . e : A ‘ 1,003 | Mr. E. Goodrich Oxford . 3 5 1,004} Mr. M. Hill = i 5 ; , 1,005 | Dr. G. Tagliani. Italy 1,006} Dr. G. Jatta . ‘ a ¢ 1,007 | Prof. A. Della Valle . i, . fi » 1,008 | Dr. Count C. Attems. | Austria . . § 1,009| Dr. F. Studnicka fs ; ‘ r 1,010} Prof. K. von Barde- | Saxony . . . leben 1,011| Prof.R. Bergh. . | Zoolog. Station . 1,012} Dr. H. Zwiesele. Wiirtemberg , b 1,013| Dr. A. Fischel . Austria j 1,014| Prof. K. Mitsukuri Zoolog. Station 3 1,015 | Prof. R. Burckhardt. | Switzerland . ‘ 1,016| Dr. E. Sauerbeck ay 1,017} Dr. G. Wetzel . Prussia 1,018 | Prof. L. Jost . | Strasburg . 1,019] Prof. F. Oltmanns . | Baden : 1,020] Dr. R. Hesse Wiirtemberg - 1,021} Stud. G. Bugge. Hesse : 1,022| Prof. F. Schiitt . . | Prussia . é q July 1,1897| Aug. 1,1897 ” 19, 20, ” Dec. 31, ,, Sept.29, ,, ” > Octi:! 4)-45; Sept.14, ,, Oct. 13, ,, Noy.12, ,, Oct. 10, ,, Sept.22, May 14, 1898 Dec. 12, 1897 Nov. 20, _,, Oct: 75 3 Nov. 7, May 5, 1898 ” > ” Mar. 1, ,, Apr. 26, ,, June 1,1898 Dec. 3, 1897 Apr. 14, 1898 Dec. 4, 1897 Apr. 15, 1898 Feb. 22, ,, Apr.16, ,, A ea eine ” as ” ” 14, ” ” 14, ” EE a | Num- ber on List 1,023 1,024 1,025 1,026 1,027 1,028 1,029 1,030 1,031 1,032 - ; r 1 1,033 1,034 1,035 1,036 1,037 1,038 1,039 1,040 1,041 1,042 1,043 THE ZOOLOGICAL STATION AT NAPLES. 59! IV.—A LIsT OF NATURALISTS—continued. Naturalist’s Name State or Institution whose Table was made use of Duration of Occupancy Prof. H. Ludwig Miss H. O’Neill Prof. H. W. Conn Prof. Dr. Mottier Prof. H. Hoyer . Dr. J. Sobotta . Dr. H. Lebrun . Mr. W. Swingle Dr. A. Russo. p Prof. Miss M. Willcox Prof. K. Lampert Mag. N. Koltzoff Miss H. von Siemens. Prof. A. Nicolas Dr. C. Alessi Mr. F. Schaible Dr. D. Carazzi . Dr. G. Mazzarelli Cand. H. F. Nierstrase Prof. J. Ogneff Dr. M. Gardner Prussia - Zoolog. Station Smithsonian Instit. . Austria . ; Prussia Belgium . : : Smithsonian Instit. . Italy American Table Wiirtemberg . Russia. : Zoolog. Station Women Italy.” Wiirtemberg . Italy Holland . Russia ” Arrival Departure Mar. 10,1898} Apr. 14, 1898 3° 11, ” ” 2, ” ” 11, ” ” 24, ” » 12, ”» ” 18, ” nm 1G; |; June 6, ,, ai Ss ay) ||P Mauve Seats ” 18, ” ea eer Aen Apr. 28, ,, Apr: 6; 4; May 4, ,, ” 9, »” ” 20, ” ” 10, ” ” 7, ” ” ll, ” ae ” 12: ” ” 29; ” ” 13, ” ” 15, ” sme Ae ee v5 June22, ,, ” 25, »” ” 15, ” ” 26, ” zat? ” Bile ” a May 10, , — June 25, ,, -= ” 25, ” ‘a . V.—A List of Papers which were published in the Year 1897 by the Naturalists who have occupied Tables in the Zoological Station. H. Boruttau . ° ta N.Iwanzoff . = “ EH. Goodrich . ‘ 5 P. Celesia G. Brandes . : = ” W. T. Swingle 5 ° G. Schneider . ° e ¥. M. MacFarland . . A. Russo . : . J.Sobotta . ° . Methylenblau. vol. 40, 1897. Notes on the Anatomy of Sternaspis. Sul differenziamento delle proprieta inibitorie e delle [ Der Elektrotonus und die phasischen Aktionsstréme an marklosen Cephalopodennerven. Physiologie,’ 66 Bd., 1897. Muskelelemente der Holothurien und ihr Verhalten zum ‘Arch. Mikr. Anat.,’ Bd. 49, 1897. On the Nephridia of Polycheta. Tyrrhena, and Nephthys. ‘Archiv. f. d. ges. Part I., On Hesione, ‘Quart. Journ. Micr. Science,’ Tbid. funzionicoordinatrici nella catena gangliare dei crostacei decapodi. 1897. Zur Begattung der Dekapoden. Bd. 17, 1897. 5 5 . Die Spermatozoen der Dekapoden. * Biol. Akad. Wiss.,’ Bd. 16, 1897. Sphacelariaceen. 1897. angelus. Abth, f. Anat. u. Ontog., Bd. 10, 1897. Sul coridetto canale problematico delle Oloturie. Soc. Nat. Napoli,’ vol. 11, 1897. Amphioxus. 1897. lanceolatus. QQ2 ‘ Atti Soc. Ligustica Sc. Nat. e Geogr.,’ vol. 8, Centralblatt,’ ‘Sitz. Ber. k, Preuss. Zur Kenntniss der Kern- und Zellsheitung bei den ‘Jahrb. f. wiss. Botanik.,’ Bd. 30, Ueber die Niere und die Abdominalporen von Squatina ‘ Anat. Anz.,’ Bd, 13, 1897. Cellulére Studien an Mollusken-Hiern. ‘Zool. Jahrbiicher.’ ‘ Boll. Beobachtungen iiber den Gastrulationsvorgang beim ‘ Verh,-Phys.-Med. Ges. Wiirzburg,’ Bd. 31, Die Reifung und Befruchtung des Eies von Amphioxus ‘Archiv f. micr. Anatomie,’ Bd. 50, 1897. 596 V. Diamare G. v. Koch Th. Beer J. Ogneff A. Romano QO. Van der Stricht H. Driesch F. Noll A. Borgert F. K. Studnicka K. Kostanecki C. Herbst G. Mazzarelli . V. Faussek ” J. H. Hyde G. Tagliani R. Krause A. Fischel W. Krause J. v. Uexkiill . A. Bethe. REPORT —1898. Anatomie der Genitalien des Genus Amabilia. ‘ Centralbl. Bakteriologie,’ Bd. 21, 1897. Die Genera Amabilia u. Diploposthe, Nachtrag. Ibid. Bd. 22, 1897. Das leitende Element des Nervensystems u. seine topo- graphischen Beziehungen zu den Zellen. 1. Mitth. ‘Mitth. Zoolog. Station, Neapel,’ Bd. 12, 1897. Entwickelung von Caryophyllia cyathus. bid. ; Accomodation des Cephalopodenauges. ‘ Archiv. f. d. ges. Physiologie, Pfliiger,’ Bd. 67, 1897. Ueber die Entwickelung des electrischen Organes, bei Torpedo. ‘Arch. Anat. Phys.,’ Phys. Abth., 1897. Sopra le fibre commessurali del Proencefalo dei Selacei- ‘Monitore Zoolog. Ital.,’ Anno 8, 1897. Les ovocentres et le spermatocentre de Y’ovule de Thysa- nozoon Brocchi. ‘ Verhandl. Anat. Ges.,’ 1897. Ueber den Werth des biol. Experiments. ‘Arch. Entw.- Mechan.,’ Bd. 5, 1897. Von der regulaéren Wachsthums- u. Differenzirungs- fahigkeit der Tubularia. JZbid. Pfropf- u. Verwachsungsversuche mit Siphoneen. ‘Sita Ber. Nat. Ver. Bonn. Beitrage zur Kenntniss der in Stilolonche zanclea und Acanthometridenarten vorkommenden Parasiten. ‘ Zeitschr. Wiss. Zoologic,’ Bd. 63, 1897. Ueber das Gewebe der Chorda dorsalis und den sog, Chordaknorpel. ‘Sitz. Ber. Bohm. Ges. Wiss.,’ 1897. Ueber die Herknuft der Centrosomen der ersten Furchungs- spindel bei Myzostoma glabrum. ‘ Anzeiger K. Akad. Wiss. Krakau,’ 1897. Ueber die zur Entwickelung von Seeigellarven nothwen- digen anorganischen Stoffe, ihre Rolle und ihre Vertret- barkeit. ‘ Arch. f. Entw. Mechanik,’ Bd. 5, 1897. Contributo alla conoscenza delle ‘Tylodinide, nuova famiglia del gruppo dei Molluschi tectibranchi. ‘ Zool. Jahrbiicher,’ Abth. f. Systematik, Bd. 10, 1897. Untersuchungen tiber die Entwickelungsgeschichte der Cephalopoden. ‘Travaux Soc. Imp. des Naturalistes, St. Petersbourg,’ vol. 28, 1897. Biologische Beobachtungen iiber Lamellibranchiaten. Ibid. . Beobachtungen tiber die Secretion der sogenannten Speicheldriisen von Octopus macropus. ‘ Zeitschr. f. Biologie,’ Bd. 35, 1897. Considerazioni morfologiche intorno alle cellule nervose colossali e alle cellule nervose giganti del medolla spinale di alcuni teleostei. ‘ Monitore Zool. Ital.,’ Anno 8, 1897. Ueber Ban und Function der hinteren Speicheldriisen der Octopoden. ‘ Sitz. Ber. K. Preuss. Akad. Wiss., Bd. 51, 1897. Experimentelle Untersuchungen am Ctenophorenei. I,Von der Entwickelung isolirter Theile. ‘ Archiv. Entw.- Mechanik,’ Bd. 6, 1897. : F Die Farbenempfindung des Amphioxus. ‘Zool. Anz./ Bd. 20, 1897. Der Schatten als Reiz fiir Centrostephanus longispinus. ‘ Zeitschr. f. Biologie,’ Bd. 37, 1897. Ueber Reflexe bei den Seeigeln. Zdid. Das Nervensystem von Carcinus inends. Ein anatomisch- physiologischer Versuch. I Theil, 1. Mitthlg. ‘ Archiy- Micr. Anatomie,’ Bd. 50, 1897. ° Idem, 2 Mitthlg. 7 a THE ZOOLOGICAL STATION AT NAPLES. 597 A, Bethe 3 , . Vergleichende Untersuchungen iiber die Function des Centralnervensystems der Arthropoden. ‘ Archiy. f. d. ges. Physiologie,’ Bd. 68, 1897. F.S. Monticelli. . Dictiomyxa Trinchesii g. sp. n. di Rizopode marine. * Boll. Soc. Nat., Napoli,’ vol. 11, 1897. ©. Child . 5 : . A Preliminary Account of the Cleavage of Arenicola cris- tata, with Remarks on the Mosaic Theory. ‘Zool. Bulletin Univ. Chicago,’ vol. 1, 1897. Photographie Records of Pedigree Stock. By Francis Gatton, D.C.L. (Oxf.), Hon. Sc.D.(Camb.), F.R.S. [PLATE IV]. Tr is my purpose shortly to communicate with the Councils of some of the Societies who publish stud or herd books, urging the systematic collection of photographs of pedigree stock and of more information about them than is now procurable. Believing that if my proposals were carried into effect, they would greatly facilitate the study of heredity, I desire, before approaching the Societies, to submit my intended proposals to the criticism of a scientific body, and none seems more appropriate for the purpose than the Zoological Section of the British Association. The following remarks are based on the Ancestral Law, which will be explained. Its purport is to measwre the importance to the breeder of taking into account the various members of the ancestry of the animals he proposes to mate together, so much of the heritage coming on the average from each of them. Then the methods of utilising this bulky knowledge will be discussed, that of composite portraiture being one means of dealing with numerous photographs ; another way is by obtain- ‘ing measures, which can be arithmetically combined, from the photographs themselves, provided they have been taken in accordance with certain simple instructions. Next, the plan will be explained by which the Societies referred to above might initiate and maintain a systematic col- lection of photographs and other information useful to breeders, which should become self-supporting. Lastly, an allusion will be made to the huge waste of opportunities of advancing the art of breeding that goes on unchecked. The Ancestral Law.—I have lately shown how the general knowledge that offspring can inherit peculiarities from the various members of their ancestry as well as from their parents may be superseded by a definite law whose nature was first suggested to me by theoretical considerations. Being subsequently in a position to verify its accordance with a large number of pertinent facts, I submitted the results to the Royal Society in a communication entitled ‘On the Average Contribution of each Several Ancestor to the Total Heritage of the Offspring.’! My theory was thoroughly examined from fresh points of view by Professor Karl Pearson, F.R.S., in one of his remarkable ‘Contributions to the Mathematical Theory of Evolution,’? in which he showed that the theory accorded with other observations, and accounted for other conclusions that had already been reached. Assuming, then, that the Ancestral Law may be accepted ' Proc. Roy. Soc., 1897. * Ibid., 1898. 598 REPORT—1898. as at least approximately true, it will be found most serviceable in show- ing the relative importance and range of the data which breeders must take into account, if they pursue their art with thoroughness. The law is that, on the average, the two parents contribute between them one-half of the total heritage of the offspring, that the four grandparents contribute between them one-quarter, the eight great-grandparents one-eighth, and soon. Consequently, since 5+4+¢+7's5+&c.=1, the whole of the heri- tage is accounted for. The same law may be stated in another form, namely, that each parent contributes on the average one-quarter, each grandparent one-sixteenth, each great-grandparent one sixty-fourth, and soon. It is a property of the first series of fractions that each term is equal to the sum of all those that follow (4 being equal to }+4+),+&e. ; } to $+ );+&c.), therefore it results that if genealogical knowledge should cease with the grandparents, inasmuch as they contributed one-quarter, another quarter of the heritage will remain indetermined ; if it ceases with the great-grandparents one-eighth will remain indetermined ; if with the next ascending grade, one-sixteenth, &c. [It must be understood that the law is intended to apply only to what may be called plain heredity, that is to cases where qualities are capable of blending freely, or, if they refuse to blend, where they present them- selves as alternative possibilities. The necessary modifications have yet to be investigated when it has to be applied to hybrid heredity, and to those partial forms of hybridism which occur in cross-breeding, especially in plants, where two parental qualities seem to produce a third and dif- ferent quality in the offspring. Again, it takes no notice of prepotency, because it considers prepotency as likely to occur with equal frequency in each and all of the ancestral places, but when the prepotencies of par- ticular ancestors are known or suspected it is easy to take them into account. Similarly the law takes no cognisance of the prepotency of one sex over the other, which must be allowed for in those particular races and qualities where it is known to exist. Lastly, as it relates to averages, its predictions will be truer for the mean of many offspring than for any one of them in particular. However, as we know that fraternal variation admits of being defined with mathematical precision for any measurable quality in any race, the diminution in trustworthiness when a predic- tion relating to a fraternity is applied to a single member of it, is easily calculated. | The ancestral law specifies the number, the grades, and the relative importance of the ancestors whom breeders must take into account, in order to predict with any given degree of certainty the most probable character of the future produce. It clearly shows the necessity of a much more comprehensive system of records than now exists. A breeder ought to be in a position to compare the records of at least the four parents of the animals he proposes to mate together, in respect to the qualities in which he is interested. More especially he ought to have access to photo- graphs which indicate form and general attitude far more vividly than verbal descriptions. But the information in stud and herd books is too meagre for the requirements of the breeder, while the photographs pub- lished in newspapers and elsewhere are inadequate for making complete genealogical collections. Utilisation of the Records.—My principal suggestion is that a system of collecting photographs should be established, which would be serviceable PORTRAITS of RACE HORSES and COMPOSITES of them. Total of exposure £ z H A.12—Sir Visto. —Solare 5 A; 86 to breeders. alsovns affor ‘be shown t self-support important doneif ¥ fas been i possible to ‘ancestors 0 under spec miight be An hat with the p and decide ideas. Til of their s supplemen clash oF co which are ance of th derived fi ancestral ‘amend it Thave oft directly ir ‘Suppose tt to himsel ticulars al AS a just | Comps photogray combine i two paret the ances a mental in practic exch port sites whi traits are them to : fold with by a va rtions. Raconter Hencefor ‘tWo sma sure of 2 to givon First, 1, \ 1s” Sag . * . ON PHOTOGRAPHIC RECORDS OF PEDIGREE STOCK. 599 to breeders. They should be serviceable to them not only as portraits, but also as affording means of obtaining measurements of the animal. It will be shown that the system might be easily initiated, and be afterwards self-supporting, but for the moment it will be convenient to take these important conditions on trust, and to begin by considering what could be done if we had the photographs. I will suppose, then, that the system has been in successful operation for many years and that it has become possible to obtain photographs of the parents, grandparents, and other ancestors of each of a large number of pure-bred horses and cattle taker under specified conditions. We have to explain how such photographs might be employed in improving the art of breeding. An habitual study of the form of each pure-bred animal in connection with the portraits of all its nearer ancestors would test current opinions and decide between conflicting ones, and it could not fail to suggest new ideas. Likenesses would be traced to prepotent ancestors and the amount of their several prepotencies would be defined ; forms and features that supplement one. another, or, as it is termed, ‘nick in,’ and others that clash or combine awkwardly, would be observed and recorded: conclusions which are based on incomplete and inaccurate memories of the appear- ance of the several members of the ancestry would be superseded by others derived from a study of their actual photographs. The value of the ancestral law would be adequately tested, and it would be possible to amend it where required. Thus the effects of organic stability, to which I have often called attention, have yet to be dealt with if they are not in- directly included in the law as it stands. Lastly, it is not unreasonable to suppose that every important stallion or bull would have a pamphlet all to himself, with photographs of his ancestors, and with appropriate par- ticulars about each of them. Such pamphlets would become recognised as a just form of advertisement. Composite Photography.—It may be said that, even if all the ancestral photographs were spread in full view on a table, no human brain could combine into a single mental image the peculiarities in feature even of the two parents, and of the four grandparents, in the proportion laid down by the ancestral law. Thereis, however, a method by which a substitute for a mental picture may be obtained, which may possibly prove serviceable in practice. Jt is by making composites of the photographs, allotting to each portrait its appropriate time of exposure.! I submit a few compo- sites which I have made of the heads of racehorses : the component por- traits are from the earlier numbers of the ‘ Racing Illustrated.’ I enlarged them to an uniform scale, reckoning from the middle of the eyeball to the fold within the nostril, cut them out to get rid of the confusion introduced by a variety of background, and then combined them in various pro- portions. Especially I took six, those of (A) Sir Visto, (B) Solaro, (C) Raconteur, (D) St. Marnock, (E) Speedwell, and (F) Salebeia, which will henceforth be distinguished by those letters. With the plate, stop, and the two small electric lamps that I used for illumination, it required an expo- sure of 240 seconds, say of 12 units of time, each consisting of 20 seconds, to give a good copy of any one of the portraits, so I proceeded as follows :— First, I made a composite of A and B, allowing 6 units of exposure to each ae Composite Portraits, Watwre, 1878; Composite Portraiture, Jowrn. Phot. Soc., 600 REPORT—1898 of them, or 12 units in all; then I made another composite of A, B, and the four others, allowing 4 units to A, 4 units to B, and 1 unit to each of the four others, forming a total as before of 12 units. So while the com- posite which I will call A 6, B 6, illustrates the combined features of the two parents, that of A 4, B 4,C 1, D1, E.1, F 1 illustrates those of two parents and four grandparents in the proportions laid down by the ances- tral law. I proceeded similarly with C, D and with C, D and the other four, and again with HE, F and with E, F and the other four ; I submit these six composites. Of course the process could be extended indefinitely, working backwards to include as many previous generations of ancestors as desired, and it might be equally well applied to portraits of other animals than horses, including men and women, whose features combine unex- pectedly well in composites, though one sex be bearded and the other not. A composite may be made of any separate part of an animal, but hardly of the whole animal at once, because each separate joint is liable to be flexed differently in the different portraits. The ears of the horses in the illus- tration indicate what would then occur. This is not the place to enter further into the details of composite making, which I have now reduced to a very simple process whose accuracy is evidenced by the identity of the composites that have been re-made at different times from the same com- ponents. The specimens I submit would have been better if they had been made from the original photographs and not from photo-process copies of them, still they will serve to gauge the amount of information which composites are likely to give to the breeder. They should be care- fully scrutinised and compared, when more differences and points of interest will be found than are apparent at a first glance. Measurement of Photographs.—A. photograph considered merely as a portrait tells about as much of an animal as can be gathered from a single view of it ; it defines the contour, the slope of the shoulders, the set of the head, the forms and the positions of the limbs, but this is by no means all that is obtainable from a photograph. It may be so taken that measurements made upon the photograph, after certain corrections have been applied to them, will be nearly as good as those made on the animal itself. Now, measurements are of the highest importance to the theoretical study of heredity, for science is based on numerical data, and the science of heredity is no exception to the general rule. Its progress depends primarily upon the power of procuring large collections of measurements of the same parts, which admit of being combined in any proportions by simple arithmetic. It matters little what limb, or bodily part, or faculty is the subject of measurement, because laws which are true for one particular quality, and for one particular race of animals or plants, will presumably apply with small modifications to any other quality and race. Therefore it would be no unworthy occupation for a scientific man to devote years of labour to carefully measuring each of many parts in the photographs of offspring and their ancestry, and to discuss the results by the elaborate methods of the higher statistics. The photographs of which I speak are assumed to have been taken under the following conditions. They would represent side views of the animals and therefore be comparable on equal terms so far as position is concerned. The animals would have been photographed at a distance of not less than thirty feet from the camera, in order to avoid sensible distortion of the portrait. They should be taken while standing ON PHOTOGRAPHIC RECORDS OF TEDIGREE STOCK. 601 on hard ground, that the feet may be clearly shown, and no mistake arise about their heights. The height of the camera above the ground and its distance from the animal should be roughly measured and noted. Lastly, two direct measurements of the height of the animal should be made, one at its withers, the other at its croup. The photo- graph now becomes more than a mere picture, because the recorded data, together with others afforded by the photograph itself, supply corrections that will cause the measurements made upon it to correspond with more or less accuracy to those made on the animal itself. Of course, their correspondence would not be so exact as it would be in photographs taken in a ‘hippometric’ laboratory provided with marked lines on the ground and walls, but such a laboratory is impracticable on many grounds. Thoroughbred horses are so easily frightened in unfamiliar places and at unfamiliar objects that the best plan is to photograph them leisurely among their accustomed surroundings. It is difficult and dangerous to apply tapes and calipers, which tickle and irritate, for thoroughbred horses are exceedingly sensitive, timid, fidgety, and often vicious, while they are supple and sudden in their movements of offence. Measurements of the two vertical heights, made in the usual way, are comparatively easy to manage. I find, moreover, that vertical measurements of all kinds may be made quickly and accurately without touching the objects at all, by means of a simple instrument which I roughly put together for trial. [I submit its working part.| Its principle is that of a collimator, with additions and modifications. It seems very suitable for use at agricultural and other shows where many animals are collected. Though many useful measurements can be made on a plain photo- graph, it would be a decided gain to select two, three or more important osseous protuberances, such as can be easily felt, and to mark their positions by sticking on the animal small wafers of sufficiently adhesive paper—say, one quarter of an inch in diameter. The corresponding marks on the photographs will be too small to attract notice, but they are easily found when looked for, and afford excellent points from which to measure. I may add that measurements I have made, and had made, both on horses and on their photographs, show that the relative dimensions of horses differ considerably. If some five different measurements were made on an adult racehorse, it would be as easy to identify him by a ‘ Bertillon process ’ as it is to identify prisoners. It will be observed that the measured height of the animals at the wither and croup, supply a scale for vertical measures on the photograph at those points. If the line to which vertical measures are drawn on the photograph be the one that touches the edge of the feet nearest to the camera, a slight and simple correction has to be made. There is difficulty in respect to the relation between the vertical and the horizontal scales, but less so than might be anticipated, for the tilt of the camera is found closely enough by a rough knowledge of the height of the camera and its distance from the animal, combined with data supplied by the photograph itself. Again, the length between the rounded ends of the body, and the diameters of the limbs, are not sensibly affected by the animal standing very slightly askew. The necessary corrections admit of being easily found from appropriate tables. It is curious in how many different ways the required corrections may be determined when the range of available 602 REPORT—1898. measures is slightly increased. J have already discussed the question fora different and more complicated series of data in ‘ Photographic Measure- ments of Horses and other Animals’ (Vature, Jan. 6, 1898), which will show the general character of the problem, but I cannot enter into par- ticulars now. The primary question is, will photographers and grooms take the proposed measurements with sufficient correctness, and are any additions to them feasible? To settle this question, many experiments should be concentrated by more than one photographer upon the same quiet and well-measured animals. These ought to determine the trust- worthiness of the results according to the data in use, and would show the minimum of effort that is necessary to afford the required degree of accuracy. I should be content if the average error in the calculated height and length of the horse did not exceed one inch, or say one-and-a-half per cent. Systematic Collection of Photographs.—It remains to consider what has hitherto been taken for granted—the best method of starting a systematic collection of photographs of pedigree stock. My proposal is to suggest to the principal Societies which publish stud or herd books, that they should proceed as follows : (1) To arrange with a photographer to store such negatives as the Society may hand over to his charge ; he undertaking to supply prints from them to the public at a moderate cost and under reasonable regulations. (2) To invite owners of pure-bred stock to send to the Society with which they are in connection, a negative photographic plate of each of the animals which they use for breeding, and which are therefore adult, on the understanding that if the negative be accepted by the Society it will be handed over to the photographer. (3) Only those negatives will be considered suitable for acceptance (a) which are of good quality ; (b) which do not transgress specified limits of size ; (c) which scrutiny shows to be strictly side views ; (¢) which have been taken at a distance from the animal of not less than 30 feet ; and (e) which show the animal standing on hard ground. (4) The following information is to be stamped or written on the negative in such a way as to be clearly legible in the prints : (1) the name and sex of the animal, (2) year of its birth, (3) year and month of taking the photograph, (4) heights at its withers and croup, (5) height of camera and its distance from the animal. (5) The Society shall order an asterisk to be affixed to the name of each animal entered in its stud or herd book, when the photographic negatives of its sire and dam have been accepted. It seems to me that a system such as this would be efficient, self-support- ing and acceptable to all parties. Breeders would be pleased that photo- graphs of their animals should be publicly recognised as serviceable for the advancement of their art. Owners of valuable animals are almost sure to order photographs of them on their own account, so the gift of the negatives to the Society would deprive them of nothing. The asterisks applied to the names of the offspring would be a valued distinction, and would help ON PHOTOGRAPHIC RECORDS OF PEDIGREE STOCK. 603 to introduce the system. Later on, when they had become common, the absence of an asterisk would excite suspicion and require explanation. Lastly, the printing of the photographs would be self-supporting. I have already expressed a belief that the custom would arise of printing a separate pamphlet for every important stallion or bull, containing its photograph and those of its nearer ancestors, together with other appropriate information. Larger publications of a more costly kind would doubtless be issued under the auspices of each Society, to correspond with an awakened demand for fuller information on the antecedents of pedigree stock. - Printed Records.—As regards useful additions to the printed matter in stud and herd books, I would now merely allude to the need for them, and to the propriety of carefully reconsidering how much of real utility could be asked for from breeders that they would supply willingly and truthfully. The measurements of adult animals, of which I spoke, would be appropriate entries. An accumulation even of these during two or three generations would be exceedingly valuable, considering how many coherent results in the science of heredity have been derived from obser- vations of human stature, though limited to comparatively small numbers of parents and their offspring. Conclusion.—The amount of money annually spent in rearing pedigree stock is enormous ; so is the care and thought bestowed upon it, and so also is its national importance. The non-preservation of adequate records of pedigree stock is a cruel waste of opportunity, and has been most preju- dicial to the acquirement of a sound knowledge of the art of breeding. If the scheme I have sketched be found feasible, it will cause much to be noted that has hitherto been overlooked, and much that is commonly observed to be placed permanently on record, instead of being ill remem- bered and soon wholly forgotten. The Climatology of Africa.—Seventh Report of a Committee consisting of Mr. E. G. RAveNsTEIN (Chairman), Sir Jonn Kirk, Mr. G. J. Symons, Dr. H. R. Miu, and Mr. H. N. Dickson (Secretary). (Drawn up by the Chairman.) MeEreoroLocicaL returns have reached your Committee, in the course of last year, from twenty-six stations in Tropical Africa. Niger Territories.—No returns have been received from Wari since the hostile operations against Benin, and there is reason to believe that the instruments at that station have been destroyed. Mr. E. G. Fenton has forwarded three months’ observations from Old Calabar. These will be published as soon as a full year’s record is to hand. The promised abstracts of observations from several stations in the territories of the Royal Niger Company have not hitherto been received. Lambarene (Ogowai).—The set of instruments lent to the late M. Bonzon of the ‘ Missions Evangéliques’ has been returned to Paris. The Rev. M. Coillard, well known for his excellent work in the Barotse country, and a trustworthy observer, having expressed a desire to purchase these instruments for 6/., the Committee have gladly accepted this offer, as a station in that part of Africa is much wanted. The set has been 604. REPORT— 1898. repaired and completed, and the thermometers have been re-verified at Kew. British Central Africa.—The organisation of the Meteorological service in British Central Africa has been intrusted to Mr. J. McClounie, the head of the scientific department of that Protectorate. From the great interest taken in the work by Mr. Alfred Sharpe, H.M.’s Commissioner, and Captain W. H. Manning, his deputy, we may fairly expect that the climatological conditions of this Protectorate will soon become thoroughly well known. The grant made by the Foreign Office has enabled Mr. McClounie to equip two Second Order stations (Zomba and Fort John- ston) and ten climatological stations. Mr. Moir, meanwhile, has resumed his work at Lauderdale, and Mr. McClounie is endeavouring to enlist the co-operation of planters and other residents. Returns for from three to four months have already been received from ten stations, including one from Kambola, on the Tanganyika Plateau, from Dr. J. G. Mackay. The instruments lent to the late Mr. Buchanan have been recovered, with the exception of the mercurial barometer, but they were found by Mr. McClounie to be in a sad state of disrepair. british East Africa.—Returns from nine Government stations have been received up to the end of 1897. These returns, owing to the occa- sional illness of the officials charged with the observations, and temporary absences, are not as complete as could be desired, but in default of some- thing better they have added considerably to our knowledge of the climatological conditions of this Protectorate, especially as regards the rainfall. We have succeeded in obtaining a description of the instruments in use at most of these stations, and copies of the Kew certificates having been kindly furnished by Mr. R. H. Scott, secretary of the Meteorological Council, we were able to correct the observations received for instrumental errors. The exposure, in many instances, seems to be objectionable, and the occasional visit of a Meteorological Inspector to all these stations would prove of great value. In addition to the above, we have received a full year’s return from the Scottish Missionaries at Kibwelzi. These returns include hourly observa- tions for thirteen international term-days, and are by far the most com- plete received, up till now, from British East Africa. Uganda.—Returns of the level of Victoria Nyanza, up to the end of July, have been received. The mutiny of the Sudanese unfortunately interrupted these valuable observations, but they have since been resumed. Your Committee have decided to discontinue lending instruments, although they will always be pleased to advise as to purchase and use of them, and to prepare and publish results. Having transferred the instruments in Nyasaland to H.M.’s Com- missioner, and sold those formerly at Lambarene to M. Coillard, the only instruments still the property of the Committee are a set at Bolobo, on the Congo; a set at Kibwezi in East Africa ; a set (probably injured beyond repair) at Wasi; an earth-thermometer in Uganda, and a rain- gauge at Golbanti. . Lastly, a set of instruments, purchased to replace one lost by Mr. Herdman, is about to be restored to the Committee. The abstracts appended have been prepared by the chairman of the Committee. Your Committee propose that they be re-appointed. They do not ask for a grant, merely requesting authority to expend the 6/. received from the sale of instruments to M. Coillard. o ~ ON THE CLIMATOLOGY OF AFRICA. 605 ! | : | Mombasa, 4° 4' S., 39° 42’ #., 60 feet. ‘ Observers: J.J. W. Pigott (to April 1896), and C. R. Craufurd. . eee ee] Mean Temperatures Humidity Rain f Pressure) “Temes Te 7, ¥ : f Atnio- | Daily | 55 = = eas Month ° B | Range 52 | 25 EI an pphere 8 é Dry | Wet | Mean| Mean 4,,./ “i Dew 83 a3 = g iga3 : "Sb © |9A.M.|9A.M.| Max.| Min. | Point] #8 |58| a | 8 g2- | Pre aa 1 a aa Se | rae lt — jo | Ins WWPse..| In. In. ° : | gonuary .| 29814 | 883 | 780 | e83 | 765 | a8 | tz ghz | Go| res | ear fa | | 2 | 736 February . 839 | 85°6 | 76-4 | 8271 | 76-2 | 848 | 781 | 81-4 | G7 | 740 | *837 17 00 6: = March .| ‘821 | 87:3 | 784 | 842 | 782 | 86-4 | 796 | 83:0 | 68 | 76-0 | 897 | 77 | 2:80] 8] 1-10 April ‘ *811 | 89:0 | 785 | 83°5 | 77-7 | 87-0 | 802 | 886 | OS | 756 | “884 77 2°08 | 12 55 May “| .go4 | ges | 74:9 | 80-5 | 75°0 | 83:9 | 77-5 | 80:7 | 5:4 | 743 | 847 | 82 | 10-93} 11 | 4°31 June. : “951 | 84:8 | 72°4 | 783 | 744 | B31 | 75-0 | 790 | 81 | 729 | -806 83 437 | 9) 1:05 July . 80°017 | 83°3 | 71-9 | 76°7 | 72°3 | 828 | 73-1 | 78-0 | 9-7 | 7U°4 | °743 80 2°77 8! -64 ‘August | | 30-002 | 863 | 70-9 | 77-0 | 728 | 93:3 | 72:8 | 780 | 105 | 711 | -759 | 82 | 491] 13 | 1-05 September | 29:962 | 838 | 724 | 78:8 | 75-2 | 82-8 | 739 | 783 | 89 | 73:8 | -832 | 85 | 2:05| 9 |. -48 October -955 | 843 | 71-9 | 79°0 | 75:2 | 81:8 | 744 | 781 | 7-4 | 73-7 | -830 | 83 | 2:39] 7 | 1-00 November | 933 | 833 | 70-0 | 79°6 | 74°9 | 75:7 | 734 | 746 | 2:3 | 73:0 | B11 | 81 | 27-67 | 12 | 4-28 December . 870 | 85:3 | 70°0 | 81-2 | 77°7 | 79:7 | 74:3 | 77-0 54 | 765 | -910 85 4°86 | 3 | 2:23 | Year. 29-906 | 89:0 | 70:0 | 80:3 | 756 | 82:9 | 75:8 | 79:3 | 7-1 | 73:8 | -832 | 1 | 65-24 | 94| 4:31 1897 / | : ‘| January . | 29°879 | 86°3 | 72°9 | 82°9 | 81:3 | 83:3 | 75-4 | 79°3 Tg | 80°9 1:053'| 94 100} 2 “50 February. | “871 | 883 | 74-9 | 811 | 765 | 85°3 | 79-4 | 823 | 5-9 | 74:8 | -B30] 81 00 | 0. fi | March “:| -832 | 88:3 | 76-9 | 848 | 81-0 | 95:6 | 80-1 | 828 | 5:5 | 798 |1-014| 85 | 163) 2! 1-50 April || -898 | 883 | 749 | 81°83 | 784 | 845 | 784 | 815 | G1 | 77-2 | 933] 86 |15-42|10| 3-95 May. .| -893 | 86-3 | 71-0 | 786 | 769 | 83:3 | 749 | 791 | 84 | 76:3 | -904] 92 | 25:40 | 10| 5:50 June. .| -948 | 823 | 729 | 77-9 | 744 | S13 | 74:3 | 77:8 | 7-0 | 73:0 | -811| 85 | -38| 2] -34 July. . *949 | 81:3 | 72°9 | 781 | 74°9 | 80°3 | 73°9 | 77:1 64 | 73°6 828 | 86 278 | 1| 2:78 August || -987 | e083 | 731 | 77-6 | 741 | 801 | 749 | 775 | 52 | 727 | -803| 85 | 11] 2] 65 September | 968 | 823 | 720 | 79-2 | 74:7 | 80°9 | 74:6 | 77:8 | 63 | 73:0 | -809| 83 | 151| 8| -34 tober *929 | 83:3 | 72:0 | 80°6 | 76:2 | 81°8 | 72-7 | 77-2 91 | 74°6 *854 | 83 2°82 | 3 | 2:30 | November 870 | 86:3 | 72:0 | 83°8 | 781 | 85:5 | 73:4 | 794 | 121 | 76-0 897 | 78 bl | 2 26 December. *827 | 86°3 | 72:0 | 82°3 | 769 | 86°3 | 731 | 797 | 1dL | 749 | -864 | 78 00; Oo}; — Year. . | 29904 | 883 | 71-0 | 80-7 | 77-0 | 832 | 75-4 | 793 | 78 | 756 | -ga6| 85 {5256 | 42) 5-50 known. Month Weaver, Capt. £. Takaungu. Lat. 3° 41’ S., Long., 39° 52' £. Observers: Ja. uf Taubman, J. W. P. McClellan, Ch. Wise, D. Wilson, and A. Rustomji. Goldie- Rain, 1896 Rain, 1897 2 we iz 3 ae a = 3 2 = — #/a|gei a] 4 | ge < a a ss In. In. In. | In. - | 0:00 0 cs 3 15 5 00 0 _ — a “47 4 7 33 - | 2°46 3 9 “00 - |10°20 | 14 21 513 | 421 9 8 “20 - | 400 9 9 2°05 -| £18 11 13 “61 . “90 3 13 “48 - | 152 3 7 1°80 . y 17 = = instruments in use are by Negretti & Zambra. The corrections for the Barometer (No. 1,564) are not ae The attached thermometer reads 0°40° higher than the dry bulb thermometer, A Had we accepted the readings of the latter in computing the pressure, the difference would have amounted to only —-001 inches. The thermometers were verified at Kew,in the dates mentioned below, and the corrections which had then to be applied to them were as follows :— No. 4590 (dry bulb), September 1889: up to 72°, 00; at 82°,40'1; at 929,+0-1. No. 4596 (wet bulb), September 1889 : at 32°,-0-1; at 42°, 52°, 62° and 72°, 0:0; at 82° and 92°, + 0:1. No. 1358 (max. therm.) June 1890: at 64°, —0°7° No. 1458 (min. therm.), January 1891: up to 32°, 0:0 ; at 32°, 42°, 52°, 62° and 70°, —0'1. The instruments are placed in the Hall, under the Sub-Commissioner's office, 5 feet from the ground of the floor. Therain-gauge stands in the open space on the roof of the office. No observations were recorded on Sundays (rainfall excepted), and in 1897 the office was closed also |) during Jubilee week (June 22-27) and Christmas week | (December 25-31). The barometrical observations have been reduced to 32° F., and to Standard gravity in Lat. 45°, but not to sea-level. The mean t»mperature is assumed to be the mean of all max. and min., and is therefore too high, 606 REPORT—1898. Shimoni ( Wanga), 4° 38' S., 39° 21' #. Observers: D. Wilson, J. W. Tritton, D. Macquarie, J. W. McClellan. ¢ 2 Mean Humidity Rain Prevailing Wind at 9 A.M. a3] Temp. BS Month £3 =| 9 aa. >2| 2 # es g Bae . BES Ss| 22 lal 2 2 ES | N. NE! E. /S.E) S. |S.W.| W. |N.W.) Cal. a ee le 5 |o 5 o a Dry| Wet Fea |e | < a | ———— ee — = — —_|—_|—_|—_—|—_|——_ —|-—__}|—__} 1896 Ins leo ino iam aoe ec. in. In, January . « |29°773 | 8574) 79°4| 77°3) *936) 77 22 | 2 18 | — | 11 4); 2)— 4}/—/; 10|— | February (1-17). |29°774 | 85°5| 78°5| 76:0) +895) 73 00; O| — |—]| 2 2;/—}—} —|— 3] — arches pet ie pee eee) a) | | Ee ee ee ee eee April (10-29) =. |29°797 | 82°3/ 79°7/ 77-8; -950| 86 | 2-09 6 | 122|—)}—}— 1/10 3} 6) —|— May . . « |29°797 | 79°6| 74°5| 72°6| *800| 79 | 12°64 | 23 | 2°43 | — | 1| — | —|{ 13 18);—| —|— June . . ~ |29°S05 | 78°1| 75°0| 73°8} *832) 87 | 444] 10} 11l | —}|—j)|—]} 1}/—} 28/;—}] —}]— July . . « |29°819 | 75°9| 73°4) 72-4) +794] 89 | 2°60 | 16 60; —|—}—]—|] 4) 26) 2) —j— August . - |29°918 | 75°8) 73°5| 72°6| °799| 89 | 5:24 | 16 85 | —|—-|—] 3 8} 19 1; —|= September . « |29°809 | 76°6| 73°8| 72°7| *801] 87 | 2°35 8 61}; —|}—}]—| 1 8 Prt 4; —|— October : . |29°797 | 79°1| 76°0| 74°8) *862} 86 “56 3 28)— |) — 1 3 | 16 8{/ 3); —|— November . « |29°791 | 79°1| 76°8| 760) °896) 91 | 23°04 | 20 | 525) 2/—|] 4) 4] 4 9| 4 3{— December . . |29°778 | 83°8) 81°6| 81-0} 17054) 92 | 3°39 | 7 87 |} 3) 3/16) 2)— 3/— 4),— Year . » |29°805 | 80°1 76°5| 75°2) *874) 85 | 56°57 |L11 | 4°25 5 | 17 | 27 | 17 | 63 | 1384 | 20] 20) — 1897 In| >|.1|.]| Im |Pec.| m. | In January . « |29°774 | 84°5) 82°5) 81-0) 1087) 89 | 1:09 | 3 | 1:00] 1 3/24); 3);—); —|}—}] —|— February . — . |29°773| 8571| 80°8) 794) 1:002| 85 “00 yp — fo | 7) = — | SS ] Se March. . + |29°770 | 85°0) 82:4) 816} 1076} 89 | 2°37 | 7) 53 1 4/22) 3 1; —|}—] —/— April . . » |29°784 | 81°3) 80°1| 79°7| 1°012] 95 | 17°42 8 | 460 | — |} — 7 6 8 8] 1 —/|— May . . _ . |29:783|79:1|781|77-7| -949] 96 | 19:96 | 93 | 400} —|—|—]—]| 8| 19] 1] 3]— June . ° » |29°802 | 77°7 75°9) 75°2| + °873| 92 | 1:25 i 38} —|—|—|—|]16; 14j/—] —]}] — July . . - |29°808 | 76°9| 76°1| 75°8} *890] 97 | 493 | 12) 172|—}]—| 5|}—)} 6) 20);/—}] —|]— August . « |29°810 | 76°8| 75°7| 75°3) *875| 95 | 3°45 | 17 89 |} —|—] 6 6 6; 13);—]; —|;— September . . |29°804 | 77°8| 76°6) 76°2} *901] 95 | 1:29 | 7 67) —|—|—)| 2] 21 5|— 2);— October . « |29°796 | 80°1| 78°2| 77:5} °942) 92 | 2:27] 8 "95 | —|—|—]19 7 5j--| —|— November . » |29°781 | 83-1] 81:2) 80°6] 1:042| 92 | 272) 7) 100} 2)}—] 3)14] 7 1/1; —j]— December. « |29°775 | 84-2/ 82-2/ 81-6} 1-076] 92 | 00) 0/ — | 7/—/11}—] 9} 4}/—] —]— Year . . « |29°788 | 81°0| 79°1) 79°3) *977| 92 | 56°75 109 | 4°60 | 11 8 105 | 53} 89/ 89] 3 5|— Norge.—The barometer is by Adie (M.O, 693). It was verified at Kew in December 1888, and the following corrections have to be applied to the readings :—at 29°5 in., —-004; at 30 in., 30°5 in., and 31 in., —’005. The correction for the attached thermometer is +0°1. The wet bulb thermometer is by Negretti & Zambra (No. 4576). It was verified at Kew in September 1889, when it was found that the correction for all readings over 52° F. was +0'1. 4 The rain-gauge, by Casella (No. 334), diam. 8 in., was found to be practically correct. The recorded ‘ dry bulb ’ readings are from the thermometer attached to the barometer. The instruments are exposed in a lime and stone room on the ground floor of the Government Office which has three large windows, and a stone ceiling. The rooms above have a galvanised roof. The barometer readings have been reduced to 32° F. and Lat, 45°, but not to sea-level. Lamu, 2° 16' S., 40° 54’ F. Observers: Capt. A. L. Rogers, K. Macdougali, W. B. Comyn, Chas. Faria (Postmaster). Mean Humidity Rain Mean Humidity Rain 3 Temp. Temp. Month 9 AM. ee lariat |e a 9am. | 2 | HE IES) B 37 Be | oe |sS| 58 12/25 Ba | 62 iss] 5 |B les S65 | aa leg] o |s|es Q3ian laa| o @ |e Se ————|Ag | 2 jee) 8 |A| s* |——_|Ag | #8 joe] & | 4 lem Dry | Wet Am) < || Dry| Wet A ia) < ss 1896 1897 5 5 o In. | P.c.! In. In pala q n., | P.c.)" In. In. January . «| 848 | 782 | 75:7 “888 |) 74 00 | O} — _ |] 83:9 811] 80°2 | 1:028) 88 03 | 1 | 03 February . | 848 | 782 | 75:7 *888 | 74 15 1 ‘15 || 83°6| 81-4) 80°7 | 1°046| 91 00 | 0} — March. ° - | 85°0 | 78°6 | 76:2 *903| 75 | 2°10 | 3 | 1°55 || 84:8) 82:0] 81-1 | 1:060| 89 00; 0} — April . . . | 845 | 796 | 77°8 °951| 81 | 3°33 8 | 1:23 || 83°0) 82°4) 82:2 | 1:099| 97 | 14°73 | 13 |825 | May . » | 8L:7 | 774 | 757 *888/ 82 | 7°06 | 17 | 1:03 80°8) 80°1) 79°9 | 1:017| 97 | 4:97 8 |1°60 June . ° - | 799 | 752 | 73°7 *818| 83 | 8°63 | 17 | 3°57 || 79°2) 76°6| 75°6 *885 | 89} 2°14] 3 j1°3L] ~ July . . - | 791 | 763 | 75°6 *885 | 89 | 1°66 9 *55 || 78°1| 75°8| 75:0 “865 | 90 | 4°14 7 \217 August e - | 787 | 75°0 | 735 *825| 84 | 1°54 | 11 "46 || 78°7| 75°4] 74:1 *842| 86 | 139 | 4 | 69 September . 785 | 743 | 726 *800| 82 | 1:77 7 “44 || 79°2| 75°6| 74:2 *844| 85 | 4:78 | 4 [3°37 October . . | 82:3 | 76:0 | 73:7 *829| 75 73 3 +36 || 81°1] 75:8) 73:3 *832 | 77 00 | 0; — November . | 8r6 | 79°0 | 781 *960| 89 | 12°96 | 14 | 3°57 || 83:2| 77-9) 76°0 *B886 | 79 10] 1) 10 December . - | 83" 80°5 | 79°5 | 1:002} 88 | 1:36 | 2} 1°16 || 83°7) 80°5) 79:4 | 1004) 86 00} O| — Year . . - | 820 | 77-4 | 757 *886 | 81 | 41:29 | 92 | 3°57 || 81°6| 78°7| 77-6 “951 | 88 | 32°28 | 41 |825 The thermometers are exposed in the open Post Office. They were verified at Kew in September 1839, a the following corrections are to be applied to the readings :— Dry bulb : Negretti & Zambra, No. 4,572: at all temperatures above 62°, up to 92°, +0°1. 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R & uUvoyy | UBITT) 6 a L 6 g L : n ec | | J681 UTR pee. aanssatgq tnodv A qniog Mod ea cee ge ainqyeradmay nveayy ay ‘tat ead ~ D Le el ee Ge ee eee FO) et See Basie eee eee eee ‘UOSLAIN UYOL PUY UOSIA, MaYIQnTY ‘aay 3 suanwasgqQ *720f 066'S “MH 189 oLE “FUOT “S 9B 0B '2PT = "eaauqry ie 610 REPORT— 1898, Variations in the Level of Victoria Nyanza. | Lake Level Rain | i Decades | - Port Port Port Port Alice ; ; we) Alice | gaubwa | Victoria || ieazis noon ae | 9.30 A.M. || ——— = | Amt. Days Days Tn. In. | In. In. January, I. —3:00 —351 —353 “08 2 1 Il. —2'70 —2'51 —211 “47 2 5 TT oie a A —1:90 —2°57 —1°'93 1:20 2 0 February, I. . 3 -| —8'00 —153 —1:58 121 7 6 TT: Scte ay p'|| | 2°00 — ‘83 20, |), 59 3 2 iG et : sf —1'70 —1:99 — ‘47 | 1:82 3 1 March, tate ; +} | =170 —113 — 23 \| 1:08 2 2 aT ake J 5 —1°30 —2:03 — 08 | 97 5 3 III. —1'55 —2'02 ‘79 | 1:92 9 3 April, ie 05 — ‘78 1:02 1°94 ti) 7 Th, 1°40 1:47 3°77 743 10 5 III. 3°10 2°87 5°00 4:37 9 4 | May, Tey } 4°65 417 4°57 1°67 7 5 ais 4:95 4°60 1:42 1°51 6 1 Iil. 6°85 3°75 1°42 7:37 9 6 June, IT. z 7°30 4:57 4:67 1°46 5 6 Il. 710 710 7:02 "26 1 5 III. 5°40 5°60 512 “45 2 3 July, 1. 4°85 5:09 4:67 1:05 3 1 II. 4°50 1-72 | 3°92 "62 3 2 III. ' 3°68 4:50 4:52 | 1:22 4. 3 We = as ee ‘sit pa ae at i Notes. The observations at Port Alice were made by Mr. Fred Pordage, at Lubwa’s by Mr. W. H. Wilson, and, at Port Victoria by Mr. C. W. Fowler. For the position of these stations see the Sixth Report, for 1897. ; All observations are referred to the mean lake-level at each station for the year 1896. On comparing’ the Results for 1897 with those for 1896 it will be found that during the last decade of July the lake-level was 3°27 in. higher than during the corresponding decade of 1896, and this notwith- standing that on January 1, 1897, the level of the lake stood 3°6 in. below the Datum level, whilst on January 1, 1896, it stood 7°8 in. above it. This difference in level is due to the heavier rainfall of 1897. The lake was lowest in the beginning of the year, highest in June. The extreme range during the seven months for which records are available amounted to 8 in. at Port Alice, to 9°7 in. at Lubwa’s, and to 7:5 in. at Port Victoria. j For remarks on the conditions governing the rise and fall of lake, see last year’s Report. ' Correction: In column 5 of last year’s table, instead of 15-40 read 1°54. | . Mean Lake Level || Fluctuations’ | H | Months inex | |e Rain Fall } Port Port Port t Port = Alice | E™>W4 | Victoria || Alice | YW" | Victoria || ForeAee jf 1896 fe) 1806 In. In. In. In. In. | In. days January... —2:00 | —2°85 | —250 || 2:50 250 2°75 1:75 5 February —220} —1-45 | —-77 || 2-00 4:00 3:00. || 262 | | 13 March —116 |} —173 | — 18 || 150 | 4-75 150 =|, 3:97 16 April 1:52 119 | 3:26 |] 5-00 6:00 500 | 1374 | | 26 May 518 416 | 244 || 2-00 4:00 6°00 |; 1055 | | 29 June 6°60 5°76 5°60 3°50 5°75 450 || 238 | ;.8 July 432 | 3:94 437 | 1:50 | 5°75 2:00 289 | | 10 That is, difference between the lowest and highest level during each month. ON MECHANICAL AND ECONOMIC PROBLEMS OF THE COAL QUESTION. 61] The Mechanical and Economie Problems of the Coal Question. By T. Forster Brown, M.JInst.C.h. [Ordered by the General Committee to be printed in extenso.] Wiruin the limits of a Paper it is practicable only to touch upon some of the more important of these problems ; and the writer would refer those who desire to investigate more fully the economic side of the question to Prof. Jevons’ work, ‘The Coal Question,’ Prof. Hull’s ‘Coal Resources at the Close of the Nineteenth Century,’ Mr. Leonard Courtney’s Address to the Statistical Society in December, 1897, a Paper by the present writer read before the Economic Section of the British Association in 1891, and ‘The Coal Supplies of the World,’ by Mr. Benjamin Taylor, a Paper pub- lished in the July number of the ‘ Nineteenth Century.’ To discuss all the suggestions as to substitutes for coal which have been made from time to time, up to and including the present meeting of the British Association, would require an exhaustive paper on that subject alone; but it is confidently submitted that so long as coal can be produced at a moderately cheap cost, having regard to the carbon it con- tains, it will always remain by far the most economical and convenient of power producers. Coal Resources. It is general knowledge that our coal resources extend over wide areas in several parts of this kingdom in beds or seams of varying thick- ness and quality existing at various depths below the surface, and gene- rally situate at no great distance from the seaboard; and it may be assumed that the public are also aware that the most available and valuable of these resources are the first to be attacked and exhausted. The coal seams which are workable by free drainage levels, without pumping or winding, are naturally the first to be worked in a virgin coal- field ; and such resources as these were probably the main source of our coal supply up to about the middle of the present century. Next follow the best of the thick seams of coal accessible at a reasonable depth, varying from a few yards to two thousand feet or thereabouts ; and these resources, which were originally much larger than they are now, are, and will be for a considerable time, the principal source of our coal supply ; and, lastly, the thin and inferior seams existing at shallow depths, and all the seams below two thousand feet or so down to the extreme limit of workable depth, and these larger resources are still practically intact. It is difficult to induce the public to realise the supreme importance of the fact that it is only the best and cheapest of our coal resources which supply our existing output. The writer has pointed out in a previous paper that, without some great and radical change in our internal policy, applied to counteracting an increasing cost, the amplitude of the total estimated coal resources and their duration is not the probable true limit, in time, of our commercial supremacy ; for, under ordinary circum- stances, this will be measured by the duration of the best and cheapest of our coal resources only, and from which we now derive probably 95 per cent. of our annual coal outputs. It is suggested that the position in figures, adopting Professor Hull’s RR2 612 REPORT—1898. estimate of the total coal resources of the kingdom in seams of two feet and upwards in thickness, and existing at depths below the surface not exceed- ing four thousand feet in the year 1900, would be . 81,683,000,000 tons And deducting from this quantity the writer's esti- mate in 1900 of the resources of best coal re- maining within a depth below the surface of two thousand feet, about the limit probably of cheaply worked coal. . . . 15,000,000,000 _,, Leaving approximately... . . . . =. 66,683,000,000 _,, of best coal existing between a depth of two thousand and four thousand feet below the surface, and of. thin and inferior seams at all depths to the limit of four thousand feet. Allowing for a small gradual increase of output from deep and inferior seams during the next fifty to sixty years, and assuming an average out- put for fifty years of best coals within a depth of two thousand feet at 220,000,000 tons per annum, exclusive of thin and inferior seams, we shall have exhausted eleven-fifteenths of our best resources about the year 1950, and have arrived at a stage when our whole annual output will be composed of a rapidly-increasing proportion of deep, thin, or inferior coals, and the proportion of our cheapest-worked coals will rapidly decrease. It will be apparent, however, that at the end of fifty years we shall still have coal resources remaining, workable, it is true, at a gradually increasing cost, but sufficient for the supply of the nation at an average output of 250,000,000 tons a year for upwards of a period of 250 years. But in working this very large residuum a greater cost in working, due to natural causes, is inevitable ; and that this extra cost will gradu- ally increase year by year after the best and cheapest coals are exhausted is undoubted, however successfully the skill of the mining and mechanical engineer may be brought to bear in mitigating this effect, and unless additional measures can be adopted, outside the province of the engineer, to counteract it by cheapening the carriage of the coal on the surface, and reducing materially all other charges, such as labour rates and taxes, &c., the effect of this increasing cost will be of serious moment to the nation. The fact of the coalfields of Great Britain being situate at no great distance from convenient ports and home centres of consumption has had, and will continue to have, an.important bearing upon the rapid develop- ment of our coal resources, and adds immensely, of course, to the intrinsic value of our coal resources as a whole. ‘The general cost of our coal will, of course, increase in proportion to the percentage of thin and deep coal worked to the whole annual output, until the increased cost of the whole of our coal production due to natural causes, such as depth, thinness of seams, &c. (however much this may be neutralised by improved mechanical and mining appliances), will be so increased as to seriously and permanently hamper our progress commer- cially by increasing the cost of our home manufactures and steam shipping, increasing the cost of navigating our steamers, and lessening thereby the amount of our coal exports, increasing also the cost of our imports of raw material and food supplies, and generally gradually taking from us for the benefit of other nations our home and foreign trade. The progress of this item of increased cost of our coal may be gradual and comparatively imperceptible for fifty years, or thereabouts, owing to ON MECHANICAL AND ECONOMIC PROBLEMS OF THE COAL QUESTION. 613 the continual development of the unopened portions of our coaltields and the resources of good and thick seams still unworked in existing collieries, but after fifty years or so this progress will be much more rapid. It will now, therefore, be convenient to consider in what direction it may be practicable to improve our existing appliances for working coal, and otherwise reduce the cost of working deep and thin seams of coal in the future. This naturally divides itself into, first, the improvements which may be achieved by the mechanical and mining engineer, and, secondly, what changes in our charges for transit and other items of cost which come more properly within the province of the Economist than the Engineer, are possibly practicable. Dealing first with the improvements which may be effected by the mechanical and mining engineer, these may be divided into—(a) improve- ments which may be effected equally applicable to existing collieries and future coal mining ; (6) improvements which can be effected applicable especially to the working of coal from great depths. Under the head of (a) we have— 1. Mechanical application of machinery for cutting thin seams’ and exceptionally hard thick seams. 2. Improvements which may be effected in underground haulage. 1. Coal-cutting Machinery. Machines may be classed as below :— (a) Heading machines. (6) Machines adapted for working in headings or ‘ rooms.’ (c) Machines adapted for continuous ‘ longwall ’ faces. (d) Percussive drills mounted on wheels for use in headings, rooms, or ‘longwall’ faces. 2. Improvements which may be effected in Underground Haulage. This comprises primary and secondary haulage: primary comprising the haulage between the bottom of the shaft and points upon the haulage roads, within a varying but moderate distance from the working coal face, and secondary haulage being the conveyance of the coal between these points and the working face. The writer sets out the various systems of haulage, and states the cost of primary haulage to be from 2d.-to 4d. per ton perimile. Secondary haulage the writer suggests improvements in, and states the present cost is from ls. 2d. to 1s. 8d. per ton per mile. Improvements which may be effected, applicable especially to Working Coal from Great Depths. Namely :—(1) Winding and Pumping ; (2) Ventilation ; (3) Dealin with high temperatures. 1. Winding and Pumping. The mechanical difficulties arise chiefly in the design of winding engines. Special winding plant and appliances associated therewith are required for producing large outputs from an increased depth to com- pensate for the heavy increase in capital outlay, and in loss of interest due to the extra time required in establishing a deep winning. 614. " REPORT— 1898. Of late years much progress has been made in new coal winnings, in improvements in winding engines by compounding, balancing, and in some cases condensing, and in the quality of the wire ropes ; and in the future it is suggested that progress must be looked for in the application of compound engines, working with a separate condenser, raising heavier loads at a higher piston speed, but with somewhat smaller drums, with a balance rope somewhat heavier than the winding rope, to assist in starting the load from the bottom and arresting the load as it arrives at the surface. The writer gives further details as to improvements practicable. Experience has shown that except under special circumstances, such as the workings approaching the Millstone Grit or Mountain Limestone, porous rocks underlying the Coal Measures, feeders of water in the Coal Measures proper at great depths are rare, and pumping water, although very expensive, will not materially operate in increasing the cost of deep coal mining. 2. Ventilation. So far as the obtaining of a sufficient quantity of air for ventilating deep mines is concerned, no difficulty exists. The higher temperature, provided the shafts and air roads in the mines are large enough, will rather facilitate the supply of air. Improvement in useful effects in the exhaust fans which are now nearly universally employed for ventilating deep mines is practicable. 3. Increase of Temperature due to Depth. This is a most serious obstacle to deep mining. It is well known that the temperature of the stratification increases with depth at the rate of about one degree Fahrenheit in every 60 feet, and adopting this ratio we reach a temperature of 91° at 2,500 feet, 99° at 3,000 feet, and according to Professor Hull the temperature at a depth of 4,000 feet will be 116°. And manifestly, inasmuch as in deep mining it will be necessary to take precautions against explosions by damping the dust and otherwise creating a certain amount of moisture in the atmosphere, which further increases the high temperature difficulties, it is difficult to see how coal, even at from 3,000 to 4,000 feet, can be worked without great increase in the cost due to the reduced amount of work which can, at a high temperature, be performed by manual labour. Tt has been suggested that the difficulty may be overcome by artificially cooling the air admitted to the mine, but the immense volume of air » necessary in a deep colliery, probably from 300,000 to 400,000 cubic feet per minute, and the rapid rate at which after cooling, in passing along the passages of the mine, the temperature increases, render any application of the freezing process, as far as present appliances go, out of the question. This process may, however, be practicable for cooling the smaller currents of air required in very deep metalliferous mines. It has, however, been observed that in longwall working, as compared with pillar and stall working, the temperature of the air does not rise so rapidly owing to the fact that the current in its progress through the mine does not come into contact with so much of the strata, and in passing through long passages in a mine, the air has a tendency to cool the exposed surface of the passages, and so reduce the heating effect of the sides of the ON MECHANICAL AND ECONOMIC PROBLEMS OF THE COAL QUESTION. 615 passages, and the writer suggests that a very material and possibly suffi- cient reduction of temperature may be looked for even to a depth of 4,000 feet, if the present practice in the best modern deep collieries is adopted of not only working the coal ‘longwall’ and upon the Midland system of few passages near the face of working, but systematically packing the spaces from which the coal has been excavated, thus reducing the parts of the mine exposed to the currents of air to the lowest practi- cable limit, namely the air passage and simple working faces ; and by carrying the intake airways as direct as possible to the point of working, and making the working face in as straight a line as practicable, it may be possible to reduce the natural temperature of the stratification alongside the air passages at from 3,000 to 4,000 feet in depth in this way by from 15° to 25° Fahr. Even at this reduced temperature, which would mean over 90° at 4,000 feet in depth, labour cannot be applied without considerable difficulty ; but it would be apparently possible at all events to work the best of the seams at this:depth at an increased cost. Practically, in the absence of any mechanical process for artificially cooling the air at the point where it is required to be used in the working face, the alternative suggested may be effected if the air passages and currents of air are made large enough, and the sides of the passages and the gob or excavated spaces as far as practicable sealed up. Before dealing with the second question, namely : What changes in our charges for transit and other items of cost are possibly practicable ? it may be of interest to review shortly the general progress of coal mining in this and other countries at the present day. Taking Great Britain to begin with, the cost of working coal has even at the present time under existing conditions a tendency to increase. This is chiefly due to the greater cost of labour and the extra charges for rates and taxes. The first item is undoubtedly increasing, and this is not altogether due to less work being performed by the workmen for a given wage, but partly to the cost of larger staffs and improved appliances to meet the requirements of the various Coal Mines Regulation Acts ; and whilst the precautions required by these Acts undoubtedly have added to the expense of working, they have also resulted in the saving of life, and, therefore, so far as this charge adds to the cost, it is an addition which cannot be a subject of regret to the community. There has also latterly been a gradual tendency to an increase in rates and taxes, which are now avery serious impost on coal mining, and, unfortunately, in the mining districts where the coal-owners are the largest ratepayers, they have little or no control over the expenditure of the proceeds of local rates. This item of rates and taxes is, in fact, growing without check, and unless something can be done to stop wastetul expenditure, it is likely to be a most serious charge upon coal mining in this country. Then again, a further addition to the cost is imminent by reason of the Workmen’s Compensation Act. And some increase is also caused by thin seams now being worked in some of the smaller districts where the thick seams have been exhausted. Then also. some deeper pits have been opened with perhaps a higher average cost, due to depth ; in fact natural causes have begun to operate to a small extent. On the other hand, considerable economies have been achieved within the last twenty-five years by using high pressure steam, a better class of 616 REPORT— 1898. boiler, economisers for using highly-heated water for boilers, increased outputs from existing mines, reducing the cost of the staff and appliances, improved methods of underground working, better realisation of the by- products from the coke, improved ventilation and precautions for dust laying, reducing the number and risks of explosions ; and in some districts, such as South Wales, material reductions in railway carriage have as the result of competition been achieved within that period. So that to summarise the position of the cost of working, whilst con- siderable economy has been achieved in some directions, natural, physical and other difficulties have increased the cost of working coal in Great Britain. So far, however, as the Western Hemisphere is concerned, similar conditions will probably more or less apply to the German coalfield, and elsewhere in Europe—z.e. the costs of production in these countries will have a tendency also to increase slowly. In the case of Germany, our main European competitor, the railway and canal rates for minerals are, per ton per mile, the writer believes, already much below the rates prevailing in this country, and therefore there is not the margin for future reductions in these rates which ought to exist in Great Britain, where the railways are not as yet the property of the State. And in regard to our competition with European coalfields, taking Germany as possessing probably the largest and most accessible coalfield, the conditions of greater depths and higher costs will be likely to either immediately follow or precede the operation of the same causes in Great Britain ; but the competition we have to fear in the Western Hemisphere is that of the United States of America. There coalfields exist of enormous extent, twenty times the original areas of our coalfields, and already the cost of producing coal in America is below the cost of raising coal in Great Britain. The annual production in the States is proceeding by leaps and bounds. In 1883 it was 102,868,000 tons ; in 1890 it was 140,883,000 tons ; and in 1896 it was 171,416,000 tons. Mr. Courtney contends that lesser cost of production in America will be permanently operative, and the difference in favour of that country is likely to increase. Probably this is so, in some degree, but the immediate cause of the difference in favour of the States as against Great Britain is due chiefly, the writer suggests, to the enormous extent of the American coalfields, making it practicable to work very large annual quantities from those areas near the outcrop by free drainage levels, without pumping or winding ; in fact the States as regards their facilities for raising coal cheaply are much in the position Great Britain was fifty to sixty years ago. If the coal output of the United States continues to increase in the present ratio, the time will arrive, no doubt, when shafts must be sunk to considerable depths and pumping and winding resorted to, thereby increasing the average cost, and bringing the natural conditions in that country more in line with those which prevail in this country. The enormous extent of outcrop coal in the American fields will, however, enable that nation to maintain probably for many centuries a comparatively Jow cost of working. The States coalfields moreover, although generally distant from the Atlantic seaboard, by reason of the cheaper capital cost of the American railways and better application of the rolling stock for mineral traffic, ON MECHANICAL AND ECONOMIC PROBLEMS OF THE COAL QUESTION. 617 such as wagons carrying a very much larger proportion of profit load to deadweight and long leads, are able to convey coal at about one-quarter of the cost per ton per mile which the best and most economically worked of our English railways now charge to convey minerals in this country. Fortunately for us the American coalfields are situate some distance from the Atiantic seaboard. It is true that in regard to the item of dead- weight our railways could also in this country considerably reduce their costs by increasing the size of their mineral wagons, but there exist again other possibly more serious competitors even than America, which may ultimately shut out the whole of the Eastern markets for manufactures both from Europe and America—namely, China and Formosa. In China enormous coalfields are believed to exist containing coals of the best qualities, and only requiring capital development in railways and docks and manufactures to enable it to become the greatest of our future com- petitors, and to develop an extraordinary source of wealth. The extremely low cost of labour alone will probably handicap the Western nations to an extent which at present cannot be measured, and whether the period when this competition will be seriously felt is distant, or imminent, the fact itself of these coalfields existing in a country densely populated by a clever and industrious race should enforce the lesson to Great Britain of setting her house in order. The argument may be even stronger as regards the coalfields of Formosa,! under Japanese rule, of which less is known, but where probably coal will be found near the seaboards and in a parallel position, as regards facilities for export, to our own coal deposits. Summarising the position, some portion of the increased future cost of working our coalfields can and will be met by improved mechanical appliances in winding, hauling, pumping, and in cutting thin seams, and by mining skill in improved ventilation, lighting, checking the increase of temperature due to depth, raising larger quantities from each shaft, and a partial readjustment of the cost of labour and royalties. The last named are already in process of being dealt with when the conditions require it (see the Mining Royalty Commission Report of a few years ago) ; but there will still remain a growing margin of increased cost which cannot be dealt with either by the mechanical or mining engineer. There remains the question, therefore, What can be done in other directions to counteract the inevitable increase of cost in working? The writer suggested in 1891, and now repeats that proposal with even greater force, the time available being lessened by seven years, that the nation should take the necessary steps now when it is practicable to acquire the reversion of railways and docks, to enable the cost of railway carriage for minerals, goods, and passengers, and dock dues to be ultimately reduced if required to the bare cost of working. All capital invested in drainage, water, lighting, schools, parks, &c., ought to be also repaid within the next sixty or sixty-five years, to admit of a permanent reduction in the incidence of rates and taxes. Assume for the moment that this country were in the position of, say the Continental States, in regard to the railways belonging to the State, that all the capital expended upon railways, docks and harbours, water, gas and electric lighting, and in all public improvements, &c., belonging ' Mr. Warington Smyth informs me that there are few, if any, convenient harbours in Formosa, that on the eastern part of the island there exists a range of high mountains, and on the western side the sea is very shallow for a great distance from the coast. 618 REPORT—1898. to public bodies had been repaid. If this were so the State could reduce the cost of carrying minerals, goods, and passengers nearly 50 per cent., the rates and taxes would be lessened, and the cost of living greatly reduced, lessening the cost of labour, and making this kingdom from its temperate climate perhaps one of the pleasantest and most economical of residential countries in the world. The reductions in the rates of carriage of minerals and goods, and in dock dues and terminal charges, and in rates and taxes, would with mechanical and mining improvements probably so neutralise the gradual increase of the cost of our coal as to enable our coalfields to maintain their position as competitors with the Western Hemisphere for probably another two and a half centuries. We should be able also to maintain our Army and Navy, and the cheap living cost would facilitate the gradual and successful introduction of industries requiring much labour, and the nation would have that long period in which to complete the repayment of the National Debt. The paying off of the National Debt now in progress is undoubtedly a commendable operation of itself, but if we are to suffer collapse com- mercially in half a century, or thereabouts, if the whole debt were paid off in the meantime the relief would only be temporary, but if on the other hand a similar annual sum to that applied to the repayment of this debt, or more, if required, were set apart for purchasing the reversion of the railways, &c., and providing legislative means of checking and raising of capital for public purposes, except with stringent provisions for repayment, then the nation would have ample oppertunities left of paying off the National Debt in the future, after these other and more imperative economies have been provided for. If we look for a moment at the reverse side of the picture, and assume that the nation will do nothing to guard against the danger of commercial collapse which will take place upon the exhaustion of our cheaply-worked coal resources, we shall be in the position of being saddled with the large amount of capital invested in railways, docks, and public works, amount- ing, it is estimated at the present time, to approaching 1,500 millions of money, with no opportunity of paying off this capital. The cost of our manufactures will rise, our foreign markets will in consequence be curtailed, resulting in a large proportion of our population being thrown out of employment, our income and means of supporting our Army and Navy will rapidly decrease, and Great Britain must gradually sink to the position of a secondary power. Existing and immediately succeeding generations, therefore, cannot be justified, under the circumstances of the enormous advantages they are receiving, and will for half a century yet receive, from the working of the most valuable portion of our coal resources, in neglecting to adopt some well-considered and comprehensive scheme for dealing successfully with the inevitable future difficulties indicated with the great object of extend- ing the duration of the prosperity of this nation far into futurity. ON A NEW INSTRUMENT FOR DRAWING ENVELOPES. 619 A New Instrument for Drawing Envelopes, and its Application to the Teeth of Wheels and for other Purposes. By Professor H. 8. Heve-Suaw, DL.D., MInst.C.E. [Ordered by the General Committee to be printed in extenso.] THE present paper is divided into two parts, the first dealing with a description of the various forms of the new instrument, the second dealing with the various examples of its use as a trammel for drawing curves, and of its application for various purposes, such as the teeth of wheels, blowers, and other revolving bodies where more or less accurate contact is required, necessitating the formation of an envelope to a curved outline previously described. A communication which may be regarded as supplementing the present paper has been read in the Mathematical Department of Section A (see p. 136), dealing with the applications of the instrument for the con- struction of cycloids and involutes, and for the drawing of ellipses and other curves. Some time ago the author devised an arrangement for exhibiting to his students the envelope of any plane figure revolving about a fixed axis upon another revolving surface, the two rolling together upon a pair of imaginary pitch circles. This arrangement merely consisted of two sheets of paper turning on drawing pins as centres, while a small wheel, with a number of projecting needle points on its edge, simultaneously engaged both sheets of paper, thereby compelling them to revolve together. This wheel of course was really in contact with the two imaginary pitch circles. It was then seen that it was not necessary to employ the actual pitch circles, as auxiliary circles would serve the same purpose and would not necessitate the paper or cardboard being actually punctured by the small needle points. Moreover, the circles were formed separately on each sheet so long as the respective wheels were connected by one axle, and narrow- milled rollers could be used instead of the roller with needle points. What was more important, the space left when parts of the surface cutting the pitch circles, such, for instance, as the spaces in tooth gearing were actually removed, did not prevent the continuous rotation of the two sheets of paper. A pencil outline round the boundary thus left could be drawn in a number of positions close to each other, thereby giving the required envelope for the corresponding teeth required to gear with those originally formed. Fig. 1 shows the instrument, which had two pairs of roller or disc wheels (connected by one axle), one above and one below the moving surfaces of the cardboard. With this instrument very little slip took place, and it was found that students could easily use it without having had any previous experience. There are three ways in which a given curved outline of any form working about a fixed centre could be obtained. 7 (1) By stencilling in the outline of the revolving sheet beneath. (2) By photographs, when the two surfaces moved over one another with a fairly rapid movement. ma 620 REPORT—1898. (3) By placing the original curve above the other in a series of con- secutive positions, and in each position drawing round the outline with a pencil or pen. This latter method proved to be by far the most satisfactory, and fig. 2 gives one or two examples of the mode in which the outline of the required envelope is thus produced. Fig. 3 is a more compact form of the instrument, in which, in order to obtain circles of different diameters, a sliding centre was used. In these cases there is a certain amount of inconvenience from the axle of the upper pair of edge runners, and although the frame was inclined, yet the axle itself prevented the curve being conveniently drawn, and the arrangement, shown in figs. 4 and 5, indicate the method by which the necessary driving shaft could be kept entirely beneath the sur- ON A NEW INSTRUMENT FOR DRAWING ENVELOPES. 621 face of the paper, and by the use of an equal pair of spur wheels the upper axle is done away with. Fie. 3: Fig. 4. CCD DIY} 11) \ CHL, In many cases much larger circles were required than could be 622 REPORT—1898. obtained on any ordinary board, and fig. 6 shows a side view of one of a pair of ratchet wheels which could be employed so as to do away with entirely the necessity for even one continuous axle. The ratchet wheels on either side are successively moved an equal distance by adjusting the position of two stops, one of which is shown in figs. 4 and 5. Hence for each successive position, the two pitch circles on the respective sheets of cardboard travel an equal distance, just as if they were really rolling upon each other. : Fig. 6. Still even with this appliance circles are often required of incon- venient size, while for drawing hypocycloidal and other curves the fixed centre of one moving surface has its position above the moving portion of the other. An arrangement, shown in fig. 1, of sliding bars, had been adopted to overcome this difficulty, but it was obvious that the use of actual centres of rotation were often very inconvenient, since it limited the size of the rolling pitch circles, and what is believed to be an entirely new method of obtaining circles of any size was devised, which does not involve the use of an actual centre at all. This method may be briefly described as the use of two pairs of edge runners, the intersection of the axis of each pair ON A NEW INSTRUMENT FOR DRAWING ENVELOPES. 62% giving the virtual centre for the rotation of the paper. It is obvious that a circle with any radius can be at once obtained by turning the direction of the axis of one pair of wheels relatively to the other, for example, when the axes are placed parallel to each other, an infinite radius is obtained, that is, the curves drawn upon the paper is a straight line. From this it will be seen that the range of the instrument is largely extended, and that instead of using an instrument of a very large size, together with trammels for setting out large wheel teeth, such teeth, even for wheels of thirty or forty feet in diameter or of a rack, can be obtained by using a small and compact instrument. The principle of the action is explained by the diagram (fig. 7), in which is shown the upper rollers A and B of each pair of rollers through which the sheet of cardboard passes. The position of the pair of rollers A is fixed, while the frames carrying the pair represented by B can Fa. 7. turn about a vertical axis. In the position shown in full lines, the centre of rotation is the intersection of the axis of A and B at O, and the fixed point P would therefore draw the arc M P N if the sheet of paper was moved by combination with the two pairs of wheels at A and B. If, how- ever, the pair of rollers B are turned into the position a, 6,, the centre of rotation becomes O,, and the pencil at P would describe the arc N, P M,. If, on the other hand, it were turned in the position of a, b,, the centre of rotation would be O,, and the arc would now be N, PM.,. It will be noted that the points O,, O, are outside the turning paper, and that there is nothing to prevent these centres moving away to an infinite distance in either direction by changing the position of the pair of rollers at B until their axis of rotation is parallel to that of the pair A. The accuracy with which the circles are drawn having been thoroughly tested by constructing a simple trammel on this principle, the complete instrument shown in figs. 8 and 9 was constructed. From fig. 9 it 624 REPORT—1898. will be seen that a graduated circle (the divisions on which were found by calculation) is used in order to set the auxiliary pair of rollers so as to give any required radius. The corresponding upper pair of rollers is afterwards turned into the required position, so that the axes of the upper und lower rollers are parallel. In the figure they are shown turned back upon a hinge in order to insert the cardboard, after which they are turned down, and a weight placed upon a projecting pin so as to insure the requisite friction when in action. Fic. 8. An examination of fig. 8 will show that not only can the auxiliary pair of rollers be lifted up, but that the frame carrying the main rollers can also be turned back about pivots which are shown at the end of the frame. It may also be noted that the plane surface upon which the cardboard moves can now be made of glass, since actual pivots for the centres are no longer required. This enables the two moving pieces of cardboard to slide easily, and is very much cleaner to use than a wooden or metal surface. The main spindle under the glass plate through which motion can be transmitted to both sheets of cardboard by turning the milled heads at either end has upon it a pair of bevel wheels which gear with a third bevel wheel carried upon a vertical axis. This arrangement is for the purpose of drawing various forms of cycloidal curves for setting out the teeth of wheels for which the two sheets of paper are required to ON A NEW INSTRUMENT FOR DRAWING ENVELOPES. 625 revolve in opposite directions. The bevel wheels can be thrown in or out of gear, to either enable this to be done or the main spindle to be coupled up in one piece, so as to revolve in the ordinary manner. It may also be pointed out that not only cycloidal but involute and other classes of rolling curves may be drawn by means of this instrument. Examples of the simplest forms of applying this instrument are shown in figs. 10,11, and 12. The upper part of the figure shows an out- line selected, and the lower part the result of tracing in a number of consecutive positions the outline of the selected figure, the result being an envelope representing the profile of the curve or ‘gear’ which would engage with it. Fig. 10. In fig. 10, in which the selected form is a radial square tooth of rect- angular section, it is clear that a portion of the envelope required for contact as the tooth is coming into gear is swept away or removed as the selected profile is coming out of gear ; hence it would be impossible to find an envelope corresponding with the selected form which would work smoothly in practice, or avoid considerable ‘ back- lash.’ The next case chosen for the profile is that of the standard American screw thread. In this case the resulting envelope gives a tooth which would work quite smoothly, but the normal of the surface in contact nearly always is ina direction which would result in considerable pres- sure upon the bearings of the two shafts. Fig. 12, in which an ordinary cycloidal tooth has been taken for the profile, gives, as a result, another tooth of cycloidal form, and shows that the HN action would not only be perfectly smooth, and that there . Ss 1898. REPORT 626 Fig. 11. Fie. 12. od ON A NEW INSTRUMENT FOR DRAWING ENVELOPES. 627 would be no ‘back-lash,’ but that the angle of contact is such as to enable the requisite force to be transmitted from one tooth to another under entirely satisfactory conditions. In figs. 10, 11, and 12 there are certain clearly marked pairs of curves, which might respectively be called the curves of ‘approach and recess’ contact, and < approach and recess clearance,’ and it will be seen that the two halves of each curve forma cusp. If these curves afterwards cross, as in fig. 10, it may be said that the envelope will not work satisfactorily with the profile, whereas if they do not cross, as in figs. 11 and 12, the two forms will work smoothly together in contact. By means of this instrument a large number of profile forms and envelopes have been drawn for wheel and rack teeth of various forms, also outlines for revolving pairs required to work in contact, such as Root’s blowers, rotary-engines, water-meters, &c.; but the foregoing examples are sufficient to illustrate the method. The author would conclude by acknowledging the kind assistance of his former student, Mr. E. Brown, B.Sc., Victoria University Scholar, in working out the necessary details and preparing the drawings. Screw Gauge.—Third Report of the Committee, consisting of Mr. W. H. Preece (Chairman), Lord KeEtvin, Sir F. T. BRaMweEL, Sir H. Trueman Woop, Major-Gen. WEBBER, Col. WATKIN, Messrs. ConraD W. Cooke, R. E. Crompton, A. Strou, A. Le NEvE Foster, C. T. Hewirr, G. K. B. Exvpsinstone, T. Buckney, E. Rigg, C. V. Boys, and W. A. PRICE (Secretary), appointed to consider means by which Practical Effect can be given to the Introduction of the Screw Gauge, proposed by the Association in 1884. Durine the last year your Committee has been in continued communica- tion with the Pratt and Whitney Company, Hartford, Connecticut, U.S.A., regarding the production of the gauges for the British Association screw threads referred to in their last report. Several sets of gauges, of certain numbers only, have been produced by the firm, who were not satisfied with their exactness. They have recently informed your Committee that they are taking up the matter again on new lines, and expect to produce the gauges shortly of the required accuracy. Your Committee have been in corr espondence with Professor M. Thury, of Geneva, in order to ascertain with what degree of accuracy the thread used by Swiss watch and clock makers, and systematised by him, has been produced. An examination of a considerable number of screws supplied to the Committee by Professor Thury shows that the Swiss thread is not produced with greater accuracy than the British Association thread. Mr. C. Vernon Boys, F.R.S., has been added te the Committee. Your Committee asks to be reappointed, with a grant of 2/. 18s. 10d., in addition to the sum of 17/. 1s. 2d., the balance of the last grant drawn but unexpended. S$s2 628 REPORT—1898. The North-Western Tribes of Canada.—Twelfth and Final Report of the Committee, consisting of Professor K. B. TyLor (Chairman), Sir CuTHBERT HK. PEEK (Secretary), Dr. G. M. Dawson, Mr. R. G. Haureurton, Mr. Davip Boy.z, and Hon. G. W. Ross, appointed to investigate the Physical Characters, Languages, and Industrial and, Social Conditions of the North-Western Tribes of the Dominion of Canada. PAGE I. Physical Characteristics of the Tribes of British eh by FRANZ Boas and LIVINGSTON FARRAND . : . 628 Il. The Chileotin, by Livineston FARRAND g ¥ : : . 645 Ill. The Social Organisation of the Haida, he Franz Boas : é ; . 648 IV. Linguistics, by FRANZ BOAS . ; 654 V. Summary of the Work of the Committee i in British Columbia, by FRANZ ‘Boas 667 APPENDIX.—Index to Reports, 1V.-XII. : : : . 684 THE following Report contains the results of field-work undertaken under the auspices of the Committee during the summer of 1897. The work was carried out by Messrs. Franz Boas and Livingston Farrand. ar Jo‘on| -oay |28T/FST/EST GBT TSTOST/GLT 821 LL1 SLT SL T\FLT SLL BLT TLTOL1\69T, 89T LOT 99T SOT|FOT)S9T|Z9T/LITO9T 691/81\ LST 991 9ST Fares oe TST OST)6FT all fe) | : ‘uayy £0 aingnirg 631 ON THE NORTH-WESTERN TRIBES OF CANADA. Dette ate les tit UBS ile atid lie EI TAPAS TET DULCE Re eet S61) | | £61 Osetia SUSIE Calle et (CaS teste F Ll bdaaaa | [al ieee Te sa at | [a | maaan Haalal[ala| lan Ia tt lae|lafaa Intetaart tall] | I61/061/68T S81 PST Ja | |aaaannaHon £81 doa lanan AMMAAAMH Jaa | | ator [11 | | aed [arate | | 681 TL} itleaetd lane PLUELT Lh ss Lae ete an tS he} Phi tl lan |adde SLT TAI OLT Ia ea hs: OI Se ales ba | | | 69T\89T TERT ee esr | Tee aiid) LOT 99T G9T|POT umryooTIGO dunbayobmays (IOAN TOSBIyZ) YOOoT[LT (aye'T wostapuy) Jaoo] [TT : : : * oayery WOsTIe yy ONUAT,1OFUIBy N * 9,0, onuredesyeyy is ? ; * 9.3[00/B7.0. uinzzndg TQ0TeA c : * welyqsmisy, * SUBIPUT JOATY ssByy 5 5 a A epreH OQuay - aaa aa Tete! se TALETS TAILS [eee teeta! 906/902 $06 861/L61|/961 S6T|F6T £61 uauos fo poopy fo yzbuat Nn nN Nn [= | |Hamm |o Baad [are | aoe RANKS [a] adaand |] lan 661 a orl alililellilwae | [tara lan [oo blisatlateatali= O8T | ea ee ee re rela hiss lhl ee ee ee 6LT SLT | } LT. 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Nee) aly oll lee Cr okee ser ac ae fa 1 1-08 sf fe ee ad a eH tt mel el td 2 eo Pe | Cr coszepty) sooo pry z oT OE re] 2 pre fee foe oc fe re re z oF L-9¢ SSN De We Es sleet me te NO ai | ea Ne ial ell Sian lanl eee eee er ml geet [Pe Uy y = L Lg SF |p rele — FE |- 8 fm be sh ed as oT 5 boua, Ay, IAW a g 3-19 Se te te ee ee et | a cll: ae = 1B G-1S Cn IS ra re AS ee tees Ae ee a | | a LS ea iS) oT 0-49 St ret ee SRS tac bea tay tarp a | ee rd 9-08 ee ee Pe ee ee |e 1 og le | ol eeepoedrecehy 8 6-06 sauna Wien (Wesel Seems ihi (feseees Macs) eS a eo a a ep Ty : Qh], | fe ee |e Le ee | a ee SS ae ae een es) Pe oe ee 8988) | ospr04 : eaten? SOrLT iit jo raqumayy V | #9 | €9 | 29] I9 | 09 | 6g | 89 bg 99 | 99 | $$ | eg | 39 | TS | OG | GF | SF | LF | OF ony ee ‘want fo s90x fo 1ybory REPORT— 1898. 636 sasep Jo Iaquinyy sasep jo requinyy L-9€ ¥-9E 6-7& G-9E 8-5E 0-9§ G-6§ 8-F& §-8& 1-96 asRIOAV &-6§ G-OF 9-07 8-8§ 9-68 8-LE €-68 L-6& 9-6F 8-8& ¥-6§ 8-68 L-0F ase1aay | | Jprrntmanals 4 | | awnwoad al[aloolnon ‘uautoyy fo asoxy fo yRpnILg Adriw | AOAGc OH oer | | o | AaNPcow ‘uayy fo asony fo yIpooug Jalo| |aana |e | * UHOOTITD ounbarLobuays (19ATY JoseIq) ooo TTT (exe wosrepuy) ye0o][vT ¢ * 9,0 0nuededsyeyyN boua AyIMVy * .¥nsz[9H ernbirg URIYSUTS J, epleH OQue], “wy ‘ uryoo(rg ounbay, cbuapyg ; sdoojmvy (AOATY IOsvIy.) OOO VT ‘(oYe] Uostopuy) yooo][rT : ; OuMIAU 10} Wey N * [JOTeA boue Ay IMy * 089112 ° Rend Meeencnoy iy . UeIUSMIST, SUBIPU]T IOATY sseN : epreH 9qU47, 6& ‘ 637 gL LI ON THE NORTH-WESTERN TRIBES OF CANADA. saseQ jo Jequin 18 i6/8 |lé |e le lr lz @/Ti/—lelesi/tri/r)/—)/—-j— 2S Oo Se eh Tea ¢ | OL] 9t] 03| 11/6 | zt18 1g] + =P eleG) Pal 9) ele patie | Gani ic aaleete oes SOL TO alee leas steal Gall ella Te Se Lo lae Ce @ a CSD Pe taal Ge Gill ace a ney ’ 11/1914 | IT] oT] of] 8 |¢g Tire I ee MGy Hye Get ypslleas sa aN eal eet line allies (hey sualhey Gag 8 eel gl pel — eee zoo fa ch el crm ea ples oe “owe a 6) SSI Pt le ae le Lee Be mee WT Beal lie ee me en Pe Ol Aan @-|—=|8 1¢ 16 | 11) $-| 8 | srl 2 SEU eects Mem Rel eah ee be oho 68 |88 | 48 |98 |S8 | #8 |e8 138 | Ts |o8 } * UrZOOTIYO, oyredeuong * dugye,199 ounbay,obuay9 * (woary qOOOULYT * (oye q0orllT * @yvrT uostiepy Jasery) wosiepuy) OuwAU, IO Mey NT 9,0, onmedekyepyN 9-407 ,29 1) * uwnzzndg pemrojopun ‘IOATY Losely JO Vqypaq pawsozapun ‘PyNIy RAST * pamioz ‘boug, Ax, IAW * pemzojepun ‘epnbitg UBIYSUIIS, -opun SUBIPU] IOATY sseny epreH £ aQuly, g) quad ag Ti) a a a a a RTE aes oT Te TESTS ET ES ae ai ee Se *SaUAS 107 0.L, ‘wapuy Yppvaig-yzhuoT REPORT—1898. 638 91 1-28 ease Bed bag ORG DEA Evlhica PN RUIEP Rae ae eee 8 9-28 Bhat ES) Te Blew bbe 8) Bok! Ba Vee We Dealers eed oh Seo Sales * + (umbgy -oburayyg) deasnyg iat ¥-08 Soa | aca este Neale Gn Gaal mae |e cal T iil ea ae ae Cy Josey) yeoorry 61 Gg a ea, eal eel A OES PTO a 198: sb ie Sen | Te A cee id 3 CLO eai a ae g 1-18 a pe eel Pe |e ieee Ta ee et tl I — oo | —— UBIYsUISy, 7 £08 | 4mm em Ht pl tt tt fp a |e |] ae =H | es es - . 1 Quay, yo roquny | *84y [68 | se 18 | 98 | 98 | #8 | e8}-ce]ts| os | ez | sz | a |-on | ox HL €h "qu90 19g | UawUMoy, fO vapuy JownT 9¢ 68 | Ti/—i—/tTI—iti—ielesigi¢eisisitie|/el—/—iri—l2i—i-—i1t U1}O9TIIO 6g $18 |—|—/|TJ—|TJ—{| tT} ti—|t]s] 3) tlir}si/2ielrisi1titl/—| 1) 2 | Comnbasobumpg) deasnyg rat Pee es | BolT ae ep) | | ee ee errr ra Bee ee eT ie a ae eee] Te Le Le | eee acorns aT 208 |—|—|—|—|—|—-|—|-| th} ej—le|—itlelelri-ciriti—lel|—-i—|-. > - wemsonsy 6 90R ed ital tl cl—i|—l-le ler lle epreH 1 aQuel jo roqmny| °28t4v | 96|F6) €6 | @6| 16) 06 |68| 88/28] 98| 98/78/ es) ce] Ts 08] 62} ez| 22/92/92 FL) e2| @D "qu90 10d _ ‘wayy fo xapuy yorong 639 ON THE NORTH-WESTERN TRIBES OF CANADA. a ox | egz |—|—|—|-|- J ri tii tlt leit] 3 j-j ) icici 2 iti teat ticici-j-|-y-]° 8 SCOT ES fsabel else a ths SRG te} tr) tj tlel-jelele)e tte rit}t/1j-—— | | 1 | (ounbayebuayg) deasnyg SNR Pe ef gt et alee LTT tts telat titi." 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H = x Jo ‘ot aay (60T|T01 001)66 86 6 96 26/F6)86 66) T6)06 68 88/18/98 e8)F8)e8]e8 18/08/62 82 12)9L/94)/FL/8z/22)T2|02 69 89|29 99 99 o/e9 9 19,09/69/89|Z¢|99/¢¢ quad Jeg “Uao4A, JO LAPUT IVSVAT a 98 ae, |—l|—|—-|tl/—|2i—| tie} si—izi—|tiegisiele|e¢)]e/t}ri—j|—|tij—-}/til—i—i-|° *¢ 8 ROTTED 6 rue |—|—|—l|ei|rtiritl]ele|e|/tj—js|rlie|e}e;r}ej—jrirj1r}r}1tjJ—|/—-|—|—i—|* ~* + @umba_obmaps) deasnyg 81 eee |—|—l—|tl—|rJ—-l—J—l—-J—-l—|rj—i rt} r}ri—-itl—i ty} ej—l—j—-l—l—i—] ii tl: ot * Geant aesenz) se0onrT rae 7 PT |e ee rete rea Te MT To a meet Te [mal til—|tlJ—l—|—-|—|—|—}* ++ @ ye cosseptry) ye00mT FaQeay soseQ a eBvIeay |68/88| 18| 98] 98] F8| e8|s8/18| 08! 62) 8L/ 22/92/92) FL] EL) 02/12 /02|69|89|29|99|99)/ F9/e9|e9|T9\0O9}° * * * * * * "9ua0 tog ‘uayy fo wapuy pDSDAT REPORT—1898. 640 g8 g-29 See Vion ga) Goal op iPS | z Bele epee * urjooTrYD 88 #29 0 feta Ft fe St Fee an | € Pea ote tee ‘ * (Oumnbay,ob | -WaTI9) demsnyg a1 6-89 Tote ARS eae alt Themis IP eee if ire * CY doserq) yooorry aI 0-89 Reyes, CY Mey pci) op ele I pais 6ery ("J dosrepuy) ya0oqTrT 1 aqua] sasey 3 #99 | 6-59 68S #19 V-6F |6-8F |F-8F | Ol . . joroquny § °PF°AV | O.0g | g.59 9.29 OTS | 209 /0.09 g.6F | 0-6F | 2-84 | 0.8% | arozy f yeas ‘way f0 burygges gybrazy fo xopuy g1 or alee ie 1 T I g z = OI409TIG0 82 5h i a a g g td = Counbayob | “wayg) deasnyg #1 ee Se I 3 I = * CY Jaserg) yo00r[vT 61 LFF ee I g g I = (J wosrepuy) yeoo][r] | * aqQeuy | (Ee ee Me RN ec has Sr paicatal fe Aes ak | 88880 JO] 4g, | 6-8F| FB 6-L4| FLF 7 bh $-0F 7-06) OV ok roquinyy |°°1AV 85) 0.95) 0.251 0.08 B 0-€F 0.05) $.68| 0-6¢| moxy f ia Ss 9& LE II ae Sasep jo Joquinyy ¥-bF LOP FF Ltt OSBIOAV F 4 are mio ON BBP I6-LP PLP 0-8F |9-LF |0-L% \P-OF O-9F ‘uauogy, fo wap fo yzbuay fo xapur a a a ee See ee mk 6 6 6-8F g-8h co Sa a ar ee ee " * wq09TITO : (ounbgy -“obuapg) deasnyg CY qoserq) yeoorry CT uosrepuy) yooorry gb, or * ‘quae rag mory | ‘wayyy fo wip fo yzbuay fo xapur 641 ON THE NORTH-WESTERN TRIBES OF CANADA, -uowo Af fo burps yyboxy jo vapuy ; B i] ST 0-60T i T 6 I! Giz e/a ae | G ¢ 6 | ? : UyooTIGO | 83 ©'SOL I re I 9 13 ES ee ee ¢ g if (Surbir Spmmnneieemecta iat G-E0T a = 3 g Po: =| a0 é ~ I I * Goaty tosvrq) q@0ozlrT 61 £01 z Layee j g t (ere a 3 — | (@4vT uosrepuy) ee soseg ; S ; 5 q ees foxedemy | CereAY SOT | LOL | 90 | SOT | FOT |, GOL | GOL | TOT | Oot 66 quad Jed waUlo Af JO yona.t- sobunt f0 vopuy eg F-F0L pl) Slee ee learal Sop | eg SF ee ee UTJOOTIIO 1g I-40 I I Tease ae @ |Ss| S6e 1) 6 a S I 6 | — | & \(oumbay obumayy9)deasnyg ra @-FOT ae ee Seal gual We P| e@ |) — ste = f Hap Se Geant seser) yeoorr ral 9-C0T I ~> I I PCL Tea Sak Sx | | (@4e'T uosrepuy) sooo] | | 1 OQUhT, en er SAB eee A s (ral e= PSS eeeee es fo waqmny | OSAV | OTT! GOT) 80T | LOT | 90T | SOT | FOT | SOT | GOT | TOT | OOT | GG | 86 quad 1a Ss ‘uayy fo yavat-ahurg fo xapuy ral 7-29 em lial arpa hog: ep ey | ge il ae hcg leer ee uyooryy | 8G 8-69 S I eet eee oat Stig z G Cr a (oumbay,obura[3g) deasnyg tI 9-69 I ~ |e ons eed Me Meek eC id i T ot | — | — | *, Geary reser) ye007IrT GT 8-19 I a T | =) 6 Boj | oS eel ste [p= | Bal FP 8) eney momepay recor * OQUy sosty Foc | GF9 | FES | GED | HES] GS) F3G| 619) FIG] 6-09) £09, 6.6F | F-6F eek: Be ee Saale yo xoquinyy | OAV os9 | 949 | 059 | 29 | Oe] @-29| 02g] 9.19] 0.19] 2.09] 0.09| 9.6F| 0.6 | TOM aa 642 REPORT—1898. A short analysis of the material contained in the preceding tables and in previous Reports of the Committee allows us to dis- tinguish with certainty three distinct types of man among the natives of British Columbia. These are the northern type, embracing the Haida, Nass River Indians, and Tsimshian ; the Kwakiutl type, embracing the Bilqula, Hé‘iltsuk-, Awi’ky’énéq, and the tribes of the Kwakiutl ; and the Thompson River type, embracing the Lillooet and Thompson River Indians. These types may be characterised by the following measure- ments :— | Northern Type Kwakiutl Type Thompson. River Type Mea M M Average Error Average | eae Average stor I. Men. mm, mm. mm. Stature . F c 5 1675 + 7:40 1645 + 5°90 1634 + 7:90 Length of Head. ; 1946 | +0°80 188°7 | +1:19 1865 | +055 Breadth of Head . F 160°6 | +0°67 159:0 | +1:00 155°9 | +0°52 Breadth of Face . .| 1537 | 40°85 | 151-4 | +0°54 | 147-4 | 20-41 Height of Face ; .| 121°6 | +087 128:0 | +0°67 1203 | 4071 II. Women. Stature . : F . | 1542 | +5:70 1537 +5°90 1540 +500 Length of Head. . | 1856 | +0°88 1869 | 41°64 179°5 | 40°53 Breadth of Head . : 153°2 | +0:90 154:3 | 41:44 150°0 | +0°41 Breadth of Face . 4 143°9 + 0°80 144°3 + 0°64 1388 + 0°40 Height of Face . .| 1143 | 40°93 1193 | 40°82 | 1125 | +054 There are good indications of the existence of other types, but they cannot be distinguished with absolute certainty from the types enumerated here. It seems very probable that an examination of the Lillooet of Pemberton Meadows will establish beyond a doubt the existence of the peculiar type which in the Seventh and Tenth Reports of the Committee was named the Harrison Lake type, which is characterised by a very broad and very short head, small stature, large nose, and small face. Our measurements of the Lillooet were undertaken with a view of determining the existence of this type, but they did not extend far enough south. The characteristics of the Coast Salish of Washington and Southern British Columbia are doubtful, because the prevalent practice of deforming the head does not permit us to compare their head measurements with those of other tribes. Their faces show the same breadth as those of the other coast tribes, but their noses are much lower and flatter than those of the Kwakiutl. The Kamloops and other Shuswap tribes are closely allied to the Thompson River type, but it seems that the dimensions of their heads are a Jittle larger, their statures a little higher. The Chilcotin resemble the Shuswap much, but their faces are flatter, their noses not so highly elevated over the face. A study of the profiles of these types shows several important phenomena that are not elucidated in the tables of measurements. The northern type shows, on the whole, a rounded forehead ; a nose which tends rather to be concave than convex, with the exception ON THE NORTH-WESTERN TRIBES OF CANADA. 645 of a few individuals; short point of the nose, slight elevation of nose, long upper lip, and rather thick mouth. The Kwakiutl type shows a flat forehead, which is largely due to artificial deformation ; a decidedly convex nose with short point, highly elevated over the face, and a less protruding mouth. It is very remarkable that the characteristic features of this type are so strongly marked in the female that the differences between the northern type and this type are more strongly noticed in women than in men. The Thompson River type has a very prominent, convex nose, with long point. The nose has a great elevation over the face. We give the cross-sections of the face, laid through the tragus and lower rim of orbits for the various types. In order to make the differences clearer we have drawn a middle or composite outline for each type, which show clearly the considerable breadth of face prevailing on the coast and the flatness of the nose of the northern type. \ \ ‘ ‘ ’ ’ i] 1 ' ' ' ’ ‘ 1 ‘ ' 1 ' H Cross-sections of Face laid through the Tragus and the Lower Rim of the Orbit. —— Average cross-section of the Kwakiutl, Haida, and Tsimshian. ---- Average cross-section of the Ntlakyapamug and Kamloops. The following table contains a number of repeated measurements, the first measurement having been taken in September 1894, the second in June 1897, the interval being two years and nine months. It will be seen that on the whole the measurements show a close agreement ; but it appears that the error of observation for the measurements of the body, except for stature and finger-reach, is very considerable. The nasal index is also very unsatisfactory on account of the smallness of the measure- ments that are contained in it :— 1898. REPORT 644 80+ | cO-— | BO+}] TLI+}] 80+] 20-—|] 90-] 20—| FO-—] OOF | BOF] BT+] OL+] FOF sieprnoys jo 0 xo) £16 1-26 8-16 6-36 G16 6-26 G18 8-16 G26 ¥-26 9-06 0-83 826° | L136 Renee a 6I— | 60—| 88— | 80—| 20+) OC —| 6E— | LE-| BE-—| BOF] SO—| BO—|] LO) L2T— Zurgy1s yq310y Jo xopuy T-¢¢ 0-8¢ 8-8¢ £69 9.69 6.4S 9.¢¢ T-g¢ L-G¢ 0-¢¢ TLS 8-49 L-¢9 LS . y 86+ | 96+ | BO-—}] €OF TO+!] 9O+ |] GI+)] 80+] BO+] OOF | 82-—|] LO0-] 60+ | 6IT+ * yoval-1esuy jo xepuy O00T &-FOL £-FOL Lor &-S0T 6-10 &- TOT 1-66 9-601 £-FOL T-801 8-901 Lor 0-FOL 80+ | Le+ | b+ |] GCI+ |] €O+] SO-—] TEI+|] LI+] 00+] cO+ |] SOF] T+] 80+ = MLIe Jo 14SUs] Jo xepuy ¥-Gb ¥-OP G0F LPP 9-F LEPr O-8P 6-6P 8-6P GPP LG LP LCP = BO+ | 96+} GO+ | BOF! 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The Chilcotin tribe occupies a territory lying chiefly in the valley of the Chilcotin River. They are somewhat isolated in situation, though on the east they are only separated from the Shuswap by the Fraser River. Between these two tribes, however, there is little intercourse. Toward the north their nearest neighbours are the related Tinneh tribe of Carriers or Porteurs; and while distance prevents frequent communication, they regard each other as more or less akin, and the relations are cordial. On the west a pass leads over the coast range to Bella Coola; and, as many Chilcotin make annual expeditions to the coast, they are fairly familiar with the people of that region. Toward the south the only tribe at present with whom they come in contact is the Lillooet, and with them but seldom. Intercourse with the coast Indians, and particularly with the Bella Coola, was formerly much more frequent than now, for the reason that the early seat of the Chilcotin was considerably farther west than at present, while the Bella Coola extended higher up the river of that name into the interior. The results of this early intercourse is seen very clearly in ~ certain of their customs, and particularly in details of their traditions. In former times and down to within about thirty years the centre of territory and population of the Chileotin was Anahem Lake, and from here they covered a considerable extent of country, the principal points of gathering beside the one mentioned being Tatlah, Puntze, and Chizaikut Lakes. They extended as far south as Chilco Lake, and at the time of the salmon fishing were accustomed to move in large numbers down to the Chilcotin River to a point near the present Anahem Reservation, always returning to their homes as soon as the fishing was over. More recently they have been brought to the eastward, and to-day the chief centres of the tribe are four reservations—Anahem, Stone, Risky Creek, and Alexandria— the first three in the valley of the Chilcotin, and the last named, consisting of but a few families, somewhat removed from the others, on the Fraser. Besides these there are a considerable number of families leading a semi- nomadic life on the old tribal territory in the woods and mountains to the westward. These latter, considerably less influenced by civilisation than their reservation relatives, are known by the whites as Stone Chilcotin or Stonies. Although subjected to more or Jess intimate intercourse with the whites for a comparatively short period, the Chilcotin have assimilated the customs and ideas of their civilised neighbours so completely that their own have largely disappeared except possibly among the families still living in the mountains, whom it was not practicable to reach. The following notes were obtained with considerable difficulty, but the information was for the most part confirmed by the independent testimony of different individuals. As regards the social organisation, persistent inquiry failed to disclose any traces of a clan system. The family unit was the family in the con- tracted sense, viz., the parents and unmarried children. Marriage was ordinarily monogamous, but many men had two wives. Recognised blood relationship was and is always an absolute bar to marriage, and at present this recognition seems to extend no further than first cousins. There seem to have been no local preferences in contracting marriages. Marriage 646 REPORT—1898. with an individual of the same village was not regarded as more desirable than one with a person from another locality, nor vice versd. Of laws of inheritance information is rather doubtful. It was stated that in former times upon the death of a man the widow received nothing, while his relatives as far as cousins divided the estate equally. It did not descend to the children alone, To-day if a man dies the widow inherits all, apparently in trust for the children, the sons, if there be such, managing the property. No information was obtained as to the pro- cedure in case the widow remarries. The above change of custom, if true, strongly suggests missionary influence. If an unmarried man dies leaving property it is said that his relatives as far as cousins divide the estate. A man never married his brother’s widow—she was still regarded as his own sister. Social ranks are not apparent at present, but there were formerly nobility, common people, and slaves, corresponding to a great extent to the system of the coast tribes. Wealth and the giving of feasts were the means of obtaining higher rank, and this seems to have been open to the lower class provided they had the means. Slaves were captives. From time immemorial, before the splitting up and settling upon the reserva- tions, there seems to have been a head chief known as A’nahem, whose seat was at Anahem Lake, and whose influence extended over the whole tribe. The last great chief of that name died a few years ago, and his son is now the so-called chief of the Anahem Reservation, Shamans, or medicine-men, are known by the term ‘di’yi’n,’ which denotes any person of extraordinary powers who is supposed to have extra- human aid, and he becomes such by reason of some remarkable dream or experience. The deliberate candidate for such honours was accustomed to go away alone to the top of some mountain or other desolate place and there fast for several days, during which time the favourable dream might or might not come to him. The favourable dream was usually a vivid one of some animal or bird, and this became his protector and helper ever afterward. The di’yi/n would then always wear some distinctive mark of his protector, such as teeth, claws, wings, feathers, &c. Aside from success in hunting and war, special powers were obtained in the cure of disease. The method of treatment was first the singing of the particular song of the di’yi’n, which was his own property and used by no one else. The song was usually acccmpanied by dancing, but not always. Then followed the application of the hands to the body of the patient, and usually suck- ing through the hands placed over the diseased spot, thus drawing out the sickness. The hands were then held up in front of and above the face, and, being suddenly opened, the sickness would be sharply blown out into the air, and so expelled. Occasionally, after sucking the di’yi’n would open his hands and show a grasshopper or other object, which he exhibited as the cause of the illness, and which had been thus removed. During such treatment the di’yi’n usually carried a pouch containing certain charms, and, while wearing certain insignia as above stated, he did not dress in any particular robe as far as could be learned. Anyone might become dryi/n, even young boys and girls. In former times the winter houses of the Chilcotin were the ordinary circular subterranean lodges, the excavation being about four feet in depth. There are none of these in existence to-day. The summer lodges were rectangular in shape, made of bark stretched over poles, and with only the roof and back covered, the front and two sides being thus left open. They ON THE NORTH-WESTERN TRIBES OF CANADA. 64.7 were ordinarily built in pairs facing each other and with a common fire between. At the present time the winter houses are of logs, often very well built, and in summer tents are used, canvas for the purpose being obtained from the whites. It was said that formerly the canoes of this tribe were made of bark stretched over wooden ribs. Both bow and stern were sharp, and were not raised above the level of the rest of the canoe. The largest of these canoes would carry about ten men. Later and at the present time the canoes are dug-outs from single logs. Cooking was done by roasting or boiling, the latter by means of hot stones in water-tight baskets of bark or woven fibre. The hot stones were manipulated by tongs of wood. The weapons used in war were bows and arrows and war clubs, the latter made of a stout stick about the length of the arm with a stone head fastened by leather thongs. None of these weapons are now in existence apparently. Spears with points made of the horn of the mountain sheep were used in hunting, but not in war. The arrow points were of stone. Fishing spears with detachable heads of bone were formerly very common, but are now rarely seen, and a large bone hook fastened to a rod like a gaff was also sometimes used. In war a sort of woodén armour was worn over the chest and back as far down as the waist. This protection, in shape like a sleeveless shirt, was made of tough sticks about an inch in diameter, fastened together with leather thongs, and was sufficient to turn arrows. The head was also protected by a thick leather cap covering the entire head except the face. According to the only obtainable account of war decorations, the upper part of the face was painted black and the lower part red, Besides the leather helmet, war head-dresses were worn of the skins of birds and of the heads of animals, so arranged that the beak or mouth came forward over the forehead. The most popular skin for such head-dresses was said to have been that of the raven. Any man who was a diyi’n would wear the skin of his own protecting bird or animal. Ear ornaments were formerly quite universally worn by both sexes, and usually in the form of small buttons of various materials attached to short strings and suspended from the lobes of the ears, which were pierced for the purpose. Older people are still found with pierced ears, but the pendants are seldom seen. Rings were also worn in the ears, but the Chilcotin say that this was a coast custom which they adopted, and was not so common as the other. : Nose.ornaments of rings and straight bars inserted through the septum were also worn. One old man further described a lip ornament as a small straight bar piercing the upper lip, but this was not confirmed, and no description of labrets was obtained. Tattooing appears to have been pretty universal, the face, chest, arms, and legs being the parts most favoured. Little information as to designs could be obtained, but it was asserted that there was no difference in the designs used by the two sexes. This is of course doubtful. The materials used in the tattooing process were bone needles and charcoal. In general the decorative art of the Chilcotin was very slightly developed. They did not carve their weapons or utensils, and the basketry designs were and are of the simplest character. It was said that in the old days cremation was used in the disposal of the dead, the ashes being afterwards buried. Since the arrival of the 648 REPORT—1898. missionaries ordinary burial has been practised, the graves being protected by a low fence of logs. The traditions of the Chilcotin are particularly interesting as showing the influence of their coast and inland neighbours, details of foreign origin being clearly traceable. Their chief tradition is of Léndix’tcux, a being half man and half dog, who came to the Chilcotin country from the north-west, and is their culture-hero. The story recites the adventures of Léndix-teux and his three sons on their journey through the land. These adventures are chiefly with animals who before that time had been dangerous to man, but who were now overcome and made harmless. Methods of hunting and various arts were then taught to the people who previously had been wretched and ignorant. The widespread conception of the culture-lero asa trickster is especially well exemplified in this tale. In the other traditions obtained, none of which are as full nor as important as the Léndix‘tcux myth, but which cover a wide range of subjects, the raven is possibly the chief character, some of the stories in which he figures being identical with the raven tales of the coast, while others are apparently independent in origin. Few myths regarding natural phenomena were heard, and those which were told are of doubtful origin. The general impression was made of a not very rich independent mythology, but of surprising receptivity to foreign influences. III. The Social Organisation of the Haida. Dy Franz Boas. In the Fifth Report of the Committee I briefly described the social organisation of the Haida according to information obtained from a few Indians from Skidegate. I pointed out (p. 823) that the tribe is divided into two phratries, each of which consists of a number of clans the members of which are connected by ties of consanguinity, not by an imaginary relationship through the totem. I also pointed out that the clans sometimes bear the names of the places at which their houses stand. Since this statement was made I have had opportunity to in- vestigate the social organisation of the Tsimshian and of the Kwakiutl in greater detail. The result of these inquiries on the Tsimshians was published in the Tenth Report of the Committee, and of those on the Kwakiut! in the Report of the United States National Museum for 1895 (pp. 311-738). These investigations proved that among the southern — tribes of the Pacific coast the village community was the primitive unit, and that clans originated through the coalition of village communities. During the past summer I had an opportunity of investigating the social organisation of the Haida in somewhat greater detail, although not as thoroughly as might be desired. The information thus obtained cor- roborates the views expressed in the Fifth Report of the Committee, and emphasises the fact that the village community is the constituent element of the phratry. In order to make this clear I will first of all give a list of the Haida families. The two Haida phratries are called Gyit’ina’ and K’oa‘la, and every family belongs either to the one or to the other group. Each family has a number of emblems which are commemorative of certain events in the earliest history of the family. The name of the chief of each family is hereditary. For purposes of comparison I give the list of villages recorded by Dr. G. M. Dawson in his Report on Queen Charlotte Islands (Report of Progress, Geological Survey of Canada, 1878-79, Montreal, 1880). a ON THE NORTH-WESTERN TRIBES OF CANADA. 64.9 Kix-on (Dawson, /.c., p. 162 B). Not in my list ; perhaps identical with Ia’k’o ? (see below). Gyit'ina’ : Koa'la : Ky10'st’s (Dawson : Kioo-sta, p. 162 B). Sta’stas ov Saiigatl la’‘nas. Chief: K’drnsi (=glacier). Crests : Frog, beaver, raven, eagle. Chief's grave: Frag. An ancestor of the Sta/stas family met a giant frog in Tsiqoa'grts. Girls when reaching maturity wear a hat that is painted green (tlt’z’ndadjang), the paint being obtained in the river Naédze’n. Houses: 1, K’égengr nas. 2, K-oé’kyitsgyit. 3, Kun nas. 4, Nakhoda‘das. 5, Skyil nas. Skyil is the mistress of copper who endows with wealth those who meet her. 6, Sk olhaha’yut. 7, Naxa’was. _ K’a'was. Chief: Ktltené’. Crests: Beaver, sg'a’ngo, eagle. The sg‘a’ngo is a man who was transformed into a monster because he was living on raw fish and birds. He lives inacave. He has long ears and wears a high hat. He carves birds as though they were large game and carries the parts home separately. When he throws them down it gives a loud noise. House : G-otnas. K-a/nguatl la’nai. Chief: Tagyia’. Crests: Frog, eagle, beaver. Togyit’inai’, Chief: Kuns. Crest: Eagle. Tostlengilnagai’. Chief: Gwaisganrngk’aiwa's. Crests : Tsilia‘las (killer whale with raven wings), killer whale, bear, thunder-bird. (The two last named belong to the village Too of Dawson, p. 170 B.) Ti’8’6 and Di’pENs (Dawson: Tartance, p. 162 B). Koala : Gyit’ina’: Koala: Gyit’ina’ : K’oa'la : Yak‘ la’‘nas. Chief: Grsawa’k. Crests: Bear, moon, dog- fish, killer whale, wolf, devilfish. K-aoké/owai. Chief: G:atso’En. Crests: Killer whale, owl, bear, woodpecker. Koé'tas. Chief: Hotsrln’ng. Crests: Bear, killer whale, moon. Ts’atl la’nas. Chief: Gyit’ing‘oda’ and Kunkoya’n. Crests: Halibut, eagle, beaver, land otter (the Jast said to have been adopted recently). S’ale‘ndas. Chief: Ildzaunak:a'tlé. Crests: Frog, beaver, starfish, evening sky. Near D4’prns. Tas la’nas. Chief: Sk-ana’]. Crests: Land otter, killer whale, woodpecker, cirrus. K-anc (Dawson: Kung, p. 163 B). Sak‘a’nas, Chief: Gula’c. Crests: Eagle, sculpin, beaver. Kya‘nusla, Chief: Ha’nsgyinai. Crest: Killer whale. 650 REPORT—1898. WI'Ts’A. Gyit’ina’: Wi'ts’a gyit’inai’. Chief: Etlgyiga.) Crests: Eagle, hum- Totlgya gyit’inai’. Chief: Steétlta. ming-bird, beaver, Tséts gyit’inai’. Chief: Nasgi’tl. sculpin, skate Dzos haedrai’. Chief: Guinia’. (ts’etg-a). These families have the same crests. They live short distances apart. Ta’An (near Wi'ts’a. Dawson: Ya4n, p. 163 B). Koala: Stl’enge la’nas. Chief: Nena‘k’enas. Crests: Killer whale, hawk, bear. Gyit’ina’: (Tséts gyit’inai’, moved to Ia’an from Wi'ts’a a few years ago). G-at’aiwa’s (Dawson: Ut-te-was, p. 163 B). Koala: Skyit’au’k6. Chief: Cigai’, Crests: Killer whale, grizzly bear, black bear. Gyit'ina’: Gyitins. Chief: Ska-ina’. Crests: Eagle, beaver, seulpin. Sg'adzé’guatl la’nas. Chief: Skyiltk’atso. Crests: Eagle, beaver, sculpin. Koala: Sg-aga’ngsilai. Crests: Killer whale, bear. Har'ts’ av. Koa'la: Ganyak oi nagai. Chief: Kyilstlak-. Crests: Killer whale, bear. K’aya'ne (Dawson: Ka-yung, p. 163 B). Koa'la: Yagun kunilnagai’. Chief: Skyilkié’s. Crests: Bear, ts ’pm’a’s, killer whale. Gyit’ina’: Saqgui’ eyit’inai’. Chief: Naok‘adzo’t. ] Crests : Eagle, Ky’ia'ltkoangas. Chief: Kodai’. beaver, sculpin. These two groups are considered branches of one family. Koala: T’és kunilnagai’. Chief: Yatl’ink‘. C a ae ean DVia/lmn kunilnagai’. Chief : Sena’t. PA alee The three groups Kunilnagai’ in K’aya’ng are branches of one family. Ta’GEN (about three miles north-east of Masset). Gyit’ina’: Dlia’len k-éowai’. Chief: Ha’yas. Crests : Eagle, raven, sculpin, frog. Said to be related to the Sta/stas. Koala: Kun la’nas. Chief : K-ogi’s, Crests: Bear, ts’zm’a’s, killer whale. Nasku’n (Dawson : Nai-koon, p. 165 B). Gyit’ina’: Naéku’n stastaai’. Chief: Ts’on. Crests the same as those of the Sta’stas, of whom they are the branch from Naéku’n. Tsiqua’gis stastaai’. . Chief : Skyila’d. Crests the same as those of the Sta’stas, of whom they are the branch from the river Tsiqua’gis. ON THE NORTH-WESTERN TRIBES OF CANADA. 651 K’oa'la : Qua/dds. Chief: tl’ea’ls. Crests : Bear, killer whale, hawk, rainbow, stratus. The Stl’enge 1a’nas are considered a branch of the Qua‘dos, who are at present in Asegoa’n, Alaska. It is said that the qua’dds were in the habit of catching eaglesin snares. One day a man caught a hawk in his snare. Another one stole it, leaving, however, one of the hawk’s talons. This led toa quarrel, and a fight ensued, during which the family divided. Those who emigrated became the Stl’Enge la/nas. For this reason both use the hawk and also the same personal names. (Dawson : A-se-guang, p. 165 B.) Koa/la: I was told that there was a branch of the gua’dds at the place who moved to Skidegate. TiLK ‘Aicitr (Skidegate). Gyit’ina’: Gyit’ins. Na yi’ans qa‘edra; Na s’a/gas qa’edra. Chief : Sg'édxgi’ts. Crests : Raven, wasq, dogfish, eagle, sculpin. Gyitingyits’ats. Chief: Sg-a’nigyik-é’do. Crests : Sculpin, eagle, wa'ts’at (a fabulous personage.) Tsaagwi’ gyit’inai’. Chief: Wina’ts. Crests: Sculpin, eagle. Koala: Tsaagwisguatl’adegai’, Chief: Logd’t. Crests: Killer whale, gyitg-a/lya (a fabulous being), ts’Em’4’s. T)gaio la’‘nas. Chief; Do’ana’. Crests the same as the preceding family. Tai‘otl lanas. Chief: K-aiiga’o. Crests: Black bear, killer whale. Koga/ngas. Chief: K-oé'sgutnung’n/ndals. Crests: Killer whale, ts’zm’a’s. Tie-A/1t (Gold Harbor ; Dawson : Skai-to, p. 168 B). Koala: Tlga/itgu la’nas. Chief: Nenkyilstla’s. Crests: Moon, killer whale. Gyitina’: Tlg-a'it gyit’inai’. Chief: Gana'i. Crests: Raven, eagle, sculpin. Kvoa'la : Stasausk’é’owai: Chief: Sg:anayi’en. Crest: Ts’ilia’/las (killer whale with raven wings). Skoa’tl’adas. Chief: G-dlentkyinga’ns. Crests: Sea-lion, killer whale, ts’rm’a’s, thunder. K-ar's’un (Dawson : Kai-shun, p. 168 B). Gyit‘ina’: Kvai/atlla‘nas. Chief : Nana’riskyilqo’es. Crests : Beaver, frog, eagle. (Dawson : ‘Cha-atl, p. 168 B.) Kvoa'la : tlga/itgu la‘nas. (Same as above, under Tlg-a’it.) K’v’NA (Skidans, Dawson : Koona, p. 169 B). Koa'la : Tlk-inotl la/nas or K-agyalsk-é/owai. Chief : Gudék:a inga/o. Crests: Bear, moon, mountain goat, killer whale, storm 652 REPORT—1898. cloud, cirrus, rock slide. Part of this family is called Kyils qa’edrai. (Dawson: Tlkinool, p. 168 B.) Gyit’ina’ : K’unak‘é'owai. Chief: Gyitk’o’n. Crests : Dogfish, eagle, frog, monster frog, beaver. T’ano’ (Tl, Dawson : Tanoo, p. 169 B). Gyit’ina’ : K’unak‘é’owai (same as in K’u’na). Tségoatl la'nas or Laqski’yek. Koala: Kv’adas k-é’owai. Chief: Gyaqkutsa’n. Crests: Killer IAr whale, wolf, ts’Em’A’s, Sga’nguai (Nensti’ns, Dawson : Ninstance, p. 169 B). Gyit’ina’ : Gyit’i’ns. Chief: Nensti’ns. Crests: Beaver, eagle. Koala: Qalda’ngasal. Chief: Ts’ini’. Crests: Bear, killer whale, ts’em’a’s. The villages on Hippah Island are not contained in my list. A comparison of the list of families given here with that of the Skidegate families published in the Fifth Report of the Committee, p. 822, shows that the lists are fairly reliable. I give here both lists for purposes of comparison :— Skidegate. (Fifth Report. Informant Informant: E/densa of Johnny Swan) Masset Gyit’ina: Nayi’ans qa’etqa. Gvity’ Na yi’ans qa’‘edra Na’sa’'yas qia’etqa. ee i Na s’a’gas qa’edra. Djaaquigi't’enai’. Tsaéagwi’ gyit’inai’. Gyitingits’ats. Gyit’ingyits’ats. K’0’a'la: Naékun k-eraua’i. — Djaaqui’sk-‘uatl’adaga'i. Tsaagwiscuatl’adegai’. ‘ 5 Sie Tiqaiu 1a’nas. Tlg-aio ]a’nas. K-astak-éraua‘i. — — Taiodtl la’nas. —- K-og‘a’ngas. It will be noticed that the Gyit’ina’ families agree in both lists, while the Koa’la show certain discrepancies. It may be that the Naékun- k-erauai’ are the family from Asegua’n referred to above as removed to Skidegate. It will be noticed that a great many family names are town names. Such names are Sangatl ]a’nas, K-a/nguatl la’nas, Yak‘ la/nas, Tlg:aio la’‘nas, &c. Others signify ‘the gyit’ina’ of a certain place’ ; for instance : To gyit’inai’, Wits’a gyit’inai’, Tsiagwi gyit’inai’. Still others seem to signify ‘the k”oa/la of a certain place,’ for instance: To stlengilnagai’, Ya/gun kunilnagai, D]’ia/lzn kunilnagai. Another series of names signify ‘the people of a certain place,’ or ‘those born at a certain place,’ such as DV'ia‘len k-éowai’, K’una k‘eowai’, and Dzos haedrai’. These facts indicate that each family formed originally a local unit, so that each village would seem to have been inhabited by one family only. The present more complex village communities originated through the ON THE NORTH-WESTERN TRIBES OF CANADA. 653 coalition of several families in one village, each retaining its own name and organisation. On the other hand, families divided, and are for this reason present in different villages. This is the case with the Sta’stas, whom we find under the name of Sta’stas at Ky’ii’st’a, as Naékun stastaai’ in Naéku’n, and as Tsiquagis stastaai’ in the same village. The Yak‘ la/nas are partly in their old village Da’drns, partly in Tlenk:oa’n (Klinquan, Alaska); the Ts’atl la’nas are partly in Da’deEns, partly in Gaugya’n (How-aguan, Alaska). Part of the Stastas have even drifted to the Stikink‘oan of the Tlingit. The Yak‘ la’nas have a branch among the same tribe, where they have amalgamated with the Nanaa’ri family (Haida: Nan’a‘ngi). A number of families left Queen Charlotte Islands in consequence of a quarrel, and form now the Kaigani. According to Dr. Dawson the event took place about 170 years ago (about 1730). The following families are said to have emigrated entirely : The S’alz’ndas to Sakoa’n (Shakan); the Koé'tas to the same place; the K-aok:é’owai to G-augya’n (How-aguan) ; and the Tas ]a’nas to Kasaa/n. . It is clear, therefore, that the present arrangement of families is the result of a long historical development, and that in the orginal organisation of the tribe the village community was a much more important element than it is at present. It is also instructive to investigate the distribution of totems among these families. I. Gyit#ina! (18 distinct families). Eagle, ‘ . 17 families Starfish : 1 family Beaver . ; Ea 2s ee Humming-bird fatve Sculpin De? ss Skate (?) . Rae Frog : AP aah Monster-frog . aay | aes Raven . : ae© «34 Wa'ts’at . ‘ send so ts Dogfish . Die 33 Wasq UY Fi Halibut . 1 family Sg‘a/ngo ada Land-otter Le Evening sky Lint ine II. K’oa'la (22 distinct families). Killer whale . . 21 families Devilfish 1 family Black bear. Be | ae Owl 1 Ese Ts’Em’A’s . iat ade Land-otter Meets, Moon . 4a ,, Grizzly bear Lee Woodpecker ee Sea-lion . : Gh ee Tsilia’las aor Mountain-goat Eh ieee Thunder-bird igh ns Gyitg'a/lya Poh ts Hawk . Ye eae Rainbow. ‘ a oN to lie down, pa'it nmé’gia. DIMINUTIVES. Diminutives are also formed by means of reduplication. It seems that the prevailing form of reduplication consists in a repetition of the first syllable as far ws the first vowel, with a tendency of throwing back the accent of the word to tlic reduplicated syllable. Diminutive deer, emé' its cmeE’méits. black bear, speé'te spa’ paats. Friend, snu'koa bad, kES large, qzu'm bird, spEzu'zu NUMERALS. nu/nkoa. kukbEEst. qbzu'zum. spEyu’zu. There are three sets of numerals: simple cardinals used for counting inanimate objects ; and two reduplicated sev-es, one used for counting animals, the other fur counting human beings. Inanimate Animate Personal 1, pai’a, pé’ia piii’a pa pea. 2, sé@ia sé'sla sisai’a. s P vy kéak'tla’s | 2 * ala. Ie-Aale-blal pain +4]4!%e 3, k-aatla’s, k-éak:tla’s | et-nattia’s kak-aak tla's. 4, mis mo’ms mii’smust. 5, tei/ikst tei’tciEkst tci’tcizkst. Megha ! ( t]a’k-amakst Nakane: | Ms 6, tla’k‘:amakst { tlatla'k-amakst f tlatla’k-‘amakst. tet’tctk2 hin: 2 7, tew'tka alate } tei'tcutk-a, Me air pid’ps(t) hieels eel © 8, pid’ps(t) 1 Fioio' eect) ; Pipio ps(t). 9, tE/meEt pai’a tE'mEt piii’a th’meEt pa’pea. ae ah { o’pEnakst \e ee at 10, O pEnaks | op’o’pEnakst ; OPO pEnakst. 11, o’pEnakst Et pé'ia o’pEnakst Et pii’a op’>’pEnakst Et pa'pea —— se “a ON THE NORTH-WESTERN TRIBES OF CANADA. 657 20, sil o’pEnakst 30, k-at o’pEnakst 40, mit o’pEnakst 50, tci’éks 0’pEnakst 60, tla’k‘umakst 0’pEnakst _ 70, tet'tk:at o’pEnakst 80, pidpst o’pEnakst 90, temEt péto’pEnakst tEmet pi 0’pEnakst 100, qatst pé’k-Enakst qatst pé’k-Enakst 200, sii’as qatst pé’k-Enakst 300, k-i/ak ta’s qatst pé’k-Enakst 400, mis qatst pé’k-Enakst The numerals five, six, ten, one hundred, are clearly compounds of -afst, hand. I presume five is a compound of the stem ¢ca, which is found in the numeral one in Siciatl nzteia'l@, Snanaimuq nze'ts'a, Sk-qd'mic xtc’d'i, Lku'figen ne'tsa; so that tev't-kst would mean one hand. Nine may be translated literally ‘less one.’ The same classification that is used in the cardinal numbers is used in indefinite numerals; for instance— Same as inanimate. Inanimate Animate Personal Sew kwé’niq kwi'kwinEQ kwé'nkwinq. DISTRIBUTIVE NUMERALS. Distributive numerals are formed from the cardinals by means of reduplication. They have the same three classes that were found in the cardinal series. TInanimate Animate Personal 1 to each paapai’a péapai'a papii/pia. es séasai’a asiasé’sea siasai'a. “ { k-aak-aatla’s Ea py eet Pa cantata See Re eatlas ; k-aak-aatla’s k aak-aatla’s. Ae 8 musEmi's moamod’ms musmi‘smust. ae teiatci’Ekst eae tlaatla’k-amakst ee ee tetiatci’tlk'a ; ea News apes pepio'pst Same as inanimate. omer tE/mEt péapai’a LO 25 OpEd’ pEnakst THE PRONOUN. PERSONAL PRONOUN. Independent Dependent. I ntca’wa --(k)En. thou awe! —-(k)", Q. he teini’tl a we EnEmé'mutl —-kt. ye pia’pst —p or —mp; they teinku’st — POSSESSIVE PRONOUN. _ The possessive pronoun has a number of forms analogous to those of the Shuswap. Their use has not beceme clear to me. I give here the various forms and a few’ examples of their use. my — tlen— len— QEn— thy a— tla— la— Qa— his —8s Q—s our —kt,—ut your —p,—m their — os F 1898 tg 658 REPORT—1898. Feamples: neu'tEm, my object. nski'Qaza, my mother. ntcitg, my house. aga’a tla kamu’t, this is thy hat. to’a la kamu't, that is thy hat. kEnu’Q tlEn ska’qa, my horse is sich. kEnu’Q nska’qa, my horse is sich. The two plural forms in -A¢ and in -ut are not exclusive and inclusive. ska/tsont, our father. ska’tsakt, our father. tci’tqut aqa’, that is our house. I am inclined to consider the prefixes ¢1-, /-, and Q- which appear combined with the possessive pronoun as verbal particles. ‘The close relation between pos- sessive pronoun and intransitive verb becomes clear in the imperfect sense, in which the object possessed is incorporated between the verb and the pronominal suffix : kmnugska’qakEn, my horse nas sick = sick horse I. but kEnu’Q tlEn ska’qa, my horse is sick. kEnuQska’qak*, thy horse was sick=sick horse thou. but keEnu’Q tla ska’qa. or kEnu’Q a ska’qa, thy horse is sick. These constructions may be compared with the inflexion of the adverb that accompanies the verb (see below). The prefix Q- seems to indicate the relation to the indirect object of the sentence: pipHi’tsEn Qa kamu’t, Z lost it for thee thy hat. pipsta’na nkamu’t, Z lost my hat. But I found also: tla ska’ga pii/istgtcEms tlEn katsk, thy horse killed for me my elder brother. INTRANSITIVE VERB. The intransitive verb may be inflected by means of suffixes or by means of auxiliary verbs, which latter form various tenses. Aorist Present kgnu’QkeEn, J am sick. (o)aqkEn kEnu’Q, Z am sick. kEnu’Qk*, thou art sick. (o)aqk" kEnu’Q, thou art sick. kEnu’Q, he is sick. (o)aq kEnu’q, he is sick. kenv‘kt : : (o)aqkt (kEn)kEnu’q, we are sick. kEnkEnu’Qkt \ me are sich. (o)aqp (kEn)kEnu’q, ye are sick. kEnu’Qp, ye are sich. (o)ax kEnkEnu’q, they are sick. krnkeEnu’Q (tcinku’st) kenv’Q teinku’st } BEA Future I. Future II. hwi'kEn(tea)riit, Z shall sleep. rvitkEn hwi, Z shall sleep’ hwik*(tca)ra‘it, thow wilt sleep. raitk" hwi, thou wilt sleep. &e. &e. Imperfect oa/qkEn tlem tlaha‘ns, J was eating. &c. When the intransitive verb is accompanied by an adverb the latter takes the pronominal ending, being treated like an auxiliary verb. tlakamé’Q(k)En skEnu’Q, I am always sich. tlakamé’Q(k)a skEnu’Q, thou art always sick. tlakameé’Q(k) skEnu'Qs, he is always sich. tlakame’Qekt skEnu’Q, we are always sick. tlakamé’Q(k)ap skEnu’Q, ye are always sich. tlakamé’Q(k) skEnkEnu’Qs, they are alvays sick. 2 gate etre, ON THE NORTH-WESTERN TRIBES OF CANADA. 659 The verb with negative is treated in the same manner: tala’kmn skEnu’Q, J am not sick. &e. The conditional mode is characterised by the prefix a- and the suffix -w. teu’ktcen, to finish eating (=to finish with mouth). atcu’ktcEnuEn, if I finish eating. ateu’ktcEnug, if thow finishest eating. atcu’ktcEnus, if he finishes cating. atcu’ktcEnut, 2f we finish eating. atcu'ktEnup, if ye finish eating. atcuktceu'ktchnus, if they finish eating. The negative conditional present is formed in the following way : atE’mos(ta)kEn skEnu’Q, if I am not sick. atE’mos(ta)ka skEnu’Q, if thou art not sick, atE/mos(ta)k skEnu’Qs, if he is not sick. atE/moskakt skEnu’Q, if we are not sick. ath/moskap skEnu'Q, if ye are not sick. atE'mos(ta)ks kEnkEnu’Qs, if they are not sick. The negative conditional past : taskEta/kEn skEnu’Q, if Z had not been sich. The interrogative is formed by the suffix -En: kgenu’QkEnkn, am J sick ? kEnu/QktEn, are we sich ? kEnu’Qkoan, art thou sick? kEnu’/Qp’En, are ye sick ? kEnu’QEn, is he sick ? kEnkenu’QEn, ave they sick ? A periphrastic interrogative is formed by the dubitative particle ska : skaka skEnu'Q, perhaps thou art sick. skagap skEnu/Q, perhaps ye are sick. skaak skEnu’Qs, perhaps he is sich. It will be noticed that wherever the verb appears with an adverb or a particle it has the prefix s-, which makes verbal nouns, and that the third person has the suffix -s, which corresponds to the possessive pronoun. These forms are therefore identical with possessive nominal forms. TRANSITIVE VERB. The transitive verb incorporates the pronominal object as follows : to see. | Subject Object = I | thou he we | ye they i x , me —_ wi/ktcrmuQ wi/ktcrms — wi/ktcrp wikté/QsEtcina [ | thee wi/ktcrn — wiktst wiktst _ wikté/QsEtst » him wi kEnr wiktqQ wikts wiktrm wiktp wikté/QsEtEm | us 7 ? wi'ktis — wi'ktip (?) | wikté/QsEtéis | ye wi'ktimen — wi'ktimrs wi'ktimrt — wikté’ QsEtEmis | them wikt@/QsEnE | wikt@/QszmuQ tee thomten } wité/QsEt—Em]| wiktp wikté/QsEtEm t uv2 660 REPORT—1898. Verbs which have the accent on the last syllable form the following series : k-diEntci’t, to talk to someone. Subject Object = a he Bebe Ss bel ee : a! I “thou he we | ye } me _— kdienter’mug k*diEntcE’ms _ | k-Gienteéi’p thee kdiEntci/n — k‘diEntci’s kdiEntc?'t _ him k*diEnta’na k*diEnta/uQ k-diEntE’s kdiEntr’m | k-diEnta’p ee tantoalt kdirnté'is eRe ag us — k*Oikntee!'ip { eoimntelit } _ kdiEnte’ip ye k-diEntd/imEn _— kéirnti/imas | k‘dirntd/imet =e them k-Oienté’QsEna | kdiEntée’QsEmuQ| k‘diENtE’s k‘dinnté/gsEtEm | kdiknta’p An analysis of these forms shows that most of them originate by composition, the pronominal object following the verb, the pronominal subject following the pronominal object. The pronominal object suffixes seem to have the following forms : me, —tcEM us, —ti thee, —tc ye, —tim (for —tip) him, — them, —téQs The pronominal subject suffixes have the following forms: I, —En we, —t thou, —Q ye, —p he, —s they, —s But they are much more irregular than the objective suffixes. The conditional is formed in the same manner as that of the intransitive verb by means of the prefix a- and the suffix -us: awi/ktcEnus, if I see thee. awikté’QsBnous, 7f J see them. awiktipus, ¢f thow seest us. PASSIVE PARTICIPLE. tou’m, to stab. tot, stabbed. ni’/kEn, to cut. nikt, cut. From this participle the passive is formed: oaq tot, he has been stabbed. IMPERATIVE. The imperative of the transitive and intransitive verbs are formed in the same manner, second person singular by -a, second person plural by -dsa: tlaha’nza, eat / d'pita, eat it! tlaha’nzosa, eat ye / o'pitoza, eat ye it ! The future serves as an exhortative: Qwikt tlaha’ns, let us eat! or, me shall eat. The Ntlakya’pamug distinguishes between the transitive verb with determined object and without object. The latter is derived from the stem of the transitive verb by the ending -EM: aqkEn tct/um, I am working. aq tcuta’na, ZT work at it. aqkEn pé’gqEm, Z am hunting aq pé/qEna ksmé'its, J am hunting deer. Qwé'im, he is looking. Qwe’és, he is looking for it. tl’Em6’pEn, to chop. aq tl’Em6’pEna, I chop it. mé’Qima, hick! mé’Qita, hick it! é'tlem, to sing. é'tlEna, I sing it. ; pu’istEm, to hill (one). pu'istEna, TZ hill it. qostE’m, to love. aqostE‘na, Z love it. aes frien tele -_——_ ON THE NORTH-WESTERN TRIBES OF CANADA. 661 The relation to the indirect object is expressed by the suffix -Q, which precedes the pronominal ending : na’qtEm, /o0 give. k-dientci't, to talk. na’qEna, Z give it. k'é6iEnteu’tEmst, he talks about thee. na‘qtgEna, I give it to him. k dikntcu'tEmast, he talks in thy behalf. é'tlem, fo sing. aq é'tlina, T sing it. aq @/tleqna, T sing aq é’tlemgna, J sing pwistem, to kill. pu’istina, Z ill it. it for him. Sor him. piisgena, I hill it for some- body. Qui tsukhé'tcemua, write me a letter. Qui tsuk-Qé’tcEmug, write a letter for me. puists sk-a'k-qas, he hills his own dog. piistgts sk-a/k-qas, he hills his (another man’s) dog (=he hills his dog for him). DERIVATIVES. I rezorded the following derivatives : Quotative Putative Dubitative Affirmative Exhortative Causative Inchoative Durative Frequentative : Potential ' Facultative Desiderative Intensive Copulative Reciprocal Reflexive —oko —nka —-nuk —n —matl 25) —W1iQ —miQ Reduplication ’, —2’a —EnwatlEn —mamEn —ap —a-us —tuaQ —teut kEnu’Q’oko, it is said he is sich. kEnu’Qnka, he may be sick. kEnu’qQnuk, he is sick, I think. kEnw’QEn, indeed, he is sick. pia’ pstEn, indeed, it is ye! fuitamatl, do lie down ! pwit, to lie down. pwitsrna, I lay it down. nk’ iQ, to swim. nka'igsena, Tsvim a horse. snuyawi'iQ, to become possessed of money. kistEwi'iQ j + Pirated kEstuwé’EQ } o turn bad. iawi'iQ, to turn good. Qinuwi'iQ, it begins to be a long time. kEnugEemi’QkeEn, J am always sich. skEnkEnu’Q, one who is repeatedly sick. k-éak-ea’ap, one who is repeatedly indisposed. oaq nikEni’kEna, J cut it repeatedly. totoata’na, I stabbed him repeatedly. qaquatsta’na, I tie it repeatedly. hai'mz'akEn, Z might do the same. teu'umz’akEn, I might work, I ought to work. tlahansEnwatlkrn, to le able to eat. réitEnwa’tlgn, to be able to sleep. tlahansma’/mEnkmn, JZ desire to eat. ro‘itma’mEnkeEn, J desire to sleep. stlahans’a'p, to eat much. nmanqEma’p, to smoke much. stlk-a’us, together. cinzia’us, brothers. snukua/us, friends. qamana’us, enemies. ktqua’usks, he breaks it in tro (=he halves it). qatstua’Q, tied to vach other. puistua’Q, to kill one another. tla‘k‘tuag, to hill each other. iamintua’Q, to have friendly feelings towards one another. stlk‘auzEmtua’Q, to put together. MEQEtci't, to hick oneself (also to hick without hitting anything). wikeEntcu'tkrEn, J see myself. nikEntcu’tken, ZT cut myself. The reflexive is sometimes used as a simulative: nikiapEntci't, to make oneself like a coyote=to act Foolishly. ; kEnugstci’'t, to make oneself sick, or to act like a sich person, 662 u, ut, towards, to. tu, tut, from. REPORT—1898. PREPOSITIONS. Examples: uii’a, towards here, this way. ulgkeEn ut teitg, J go into the house. ut stkamlo’ps ané/soan, (when) I went to Kamloops. tii’a kaka’/o awi'kEna-us, (when) J saw it from far away. tugai’a, tukai’a, from here. tutci’a, tuktci’/a, from there. tuto’a, tukto’a, /7om there. tla/kmn tut Nkamtci'n, Z came from Spences Bridge. ktci/QkEn tut Nkamtci’n, J departed from Spences Bridge. tlak tut estcite, Z came from the house. tlak tua tcite, Z came from a house. CONJUNCTIONS. pEt, and, connecting words designating persons : snukua’us (1) aé’t(2) a (3) SEQua’pamug (4) pEt (5) ha (6) Psqié/qunEm (7), Friends together (1) now (2) the(3) Shuswap (4) and (5) the(6) Chileotin (7). Et, and, connecting all words not designating persons: sqi/its Et camnq, wood and stone. SUBSTANTIVALS. I designate by the term substantivals nominal suffixes, which are used for specifying adjectives, substantives, and verbs : —k-én, head. —us, face. —ane, ear. —aks, nose. —tcin, mouth, language. —anz, tooth. —iapsam, neck. —aqeEn, upper part of arm. —iiqkmn, body. —ikmn, bach. -——akst, hand. —ist, stone. —uciap, fire. —ko, —atko, water. —iimua, land. qazumk'é'n, big-headed. ihus, pretty. qazuma’ne, big ear. koa/néthm, he has piercing pains in his ear. tciawa’ks, nose bleeds. ntlakyapamuatci’n, Wtlakyapamue language. teuktcin, to finish with mouth, i.e., to finish eating. péatci’n, one word. kliqutltci’n, another language. zaqiapsa'm, long neck. nzaqiapsa'm, long-necked. kaupa’qrn, broken arm. tska’qin, wing, armpit. zaqa’qrEn, long-armed. qzumii’qkEn, big body. pii’qkEn, one body. mitcaki’kEn, to sit on back. pauta’kst, swollen hand. teumEna’kstEn, to point with hand. kaupa’‘kstkEn, I have broken my hand. pic’ist, one stone. piu'ciap, one fire. nkui’sko, to fall into water. qazuma’tko, great lake. nza'qko, long lake. ntlk‘a’tko, wide lake. ksii'imuaq, bad land. ihi’/imuag, nice land. kagu'imua, dry land. pit'‘imuag, one country. ON THE NORTH-WESTERN TRIBES OF CANADA. 663 —atle, house. qazuma’'tlq, large house. 6épa'tla, house burns down. —aus, trail. Eniamina/us, trail for hauling = waggon-road. teutlqua‘usEnuq, thow pointest out the way to him. —iiuk-, tree. iha’ink’, a nice tree. kunkQi/iuk-, how many trees? mitcak'a’iuk-, sitting on a tree. ok-ona'yuk-, rotten tree, wood. kaya'yuk’, green wood. k’é’qiuk’, hard wood tree. za'qiak:, long tree. —tlp, species of trees and bushes. s’'atk'tlp, yellow pine. sk’atlp, fir. —atldzig, bush. pea'tldzig, one bush. kunkga'tldzig, how many bushes? —zanz, driftwood. —aqans, board, plank. kunkgqa’ns, how many planks ? —alks, clothing for upper part of body. smutlatsa’lks, woman’s gown. —itsa, covering for body. spEk‘1'tsa, white blanket. ntltsask-aqai'tsa, horse skin. pak-ui’tsa, to shiver with fear. —autl, canoe. qzuma’utl, big canoe. pia’utl, one canoe. —als, knife. spéia'ls, one knife. qzuma'ls, large knife. —lrmuq, sack, bottle, box. tlina’tlemugq, bireh bark vessel. —ka, spoon, cup, bucket, pail. pia’ka, one spoon. —akmn, bag, bundle. pia’ken, one bag. —iiqmn, rope. pia/iqEn, one rope. —tim, hollow thing. ntsikti’m, empty vessel. —uza, round thing. piu’za, one round thing. spek-o'za, white round thing. —uzEM, group of. piu’zEm, one group of things. —aski, song. stliea’ski, dancing song. —men, instrument. tsuk'me’n, pencil. niamé’n, tool for hauling. Substantivals sometimes appear in combination : —icinatlq door = mouth of house. vkamtcina'tla, entrance of house. mitcaktcina’tla, to sit in the doorway. Some of the substantivals are developing into classificatory terms, such as are found in the Tsimshian :— —aks nose ; point of a horizontal pole. mitcak‘a’ks, to sit on a@ point. —kén head ; top of a long, upright object. mitcak’k-é’n, to sit on top of. —ikEn back ; middle of long thing. mitcak‘i’kEn, to sit in middle of a long thing —aiuk: tree, long thing. piai'uk: tik sqéts, one (long thing) salmon. piai’uk: tik ting, one (long thing) vein. —a-itQ flat thing. pia’itQ stsuk:, one sheet of paper. pia‘itQ ma’nta, one piece of canvas (manta, Spanish). —kén head, round thing. piak-é'in tkan’za, one (round thing) egg. 664 REPORT—1898. Vocabulary of the Chilcotin Language. The Chilcotin form a branch of the Tinneh stock. The following vocabulary is designed on the lines of the vocabularies given in the Sixth and Tenth Reports of the Committee. Since I am not familiar with the grammatical structure of the language. the vocabulary must be held subject to revision : English Chilcotin English Chileotin man tinné, ta’yan. all houses kaunétlan k*ho. woman tsé’ké. hettle nosai’. boy kyénl. bow atlthé’n, datsa/nk’a my girl ésk‘é tsé’/k'é (=fe- arrow k’a. male child). axe tshéntl. Sather apa knife pala’. thy mother inku’l. jack-hnife gyi/nalki’k. my husband sak‘a’n. canoc ts’é. my wife saa't. MOCCASINS ke. my child sEsk @'i, pipe k’a’tsai, my elder brother so’nar. mooden pipe titcEn k’a’tsai. my younger brother sik-i’l. tobacco tsrilyo’. my elder sister sii'té. glove bat. my younger sister —_sit@'z. shy yé't’a. Indian téntlxoté’n. sun sha. my people sétlté’s. moon, a/ldzi. my head sErtsE’. star SEn. my hair sErtsa'ra. cloud k’és my face sEné’m. smoke tlit. my forehead sEtséeku’tl. day k’antsi’n. my ear hétsa’ra (?). night etl’. my eye sEna’ra. morning k’apEna’q. my Nose sétsi/nix:. evening ngaratlra’t]. my mouth SEO’. noon satsana’s. my tongue sErtsdll. midnight sotézni’. my tooth SErO’. spring Erotlts’E’n, my beard sEta’ra. summer dan. my neck sEk’6's. autumn q@’Enk‘i’z,! my arm sEka'n. ninter qa’i. my hand stla’. wind né’nts’E. my fingers sulats’é’i. thunder @/ndi. thy fingers nélats’é’i. lightning tou'e. _ my thumb sElaitch6r. rain nagutlti’x’. my first finger sElaskE’t. snow nadjé's. my second finger sElané’. jive kon. my third finger sElara’. mater tho. my fourth finger sElastE’t. ice ku‘dlu. jinger nail lak’n’n. earth nEn. my body sEnée’s, sea ya tho. my chest sédzi'y. river tsiré’nli, yik-o’. my belly SEbE't. lake péi. my breasts sEts’0’r. snom mountain tsatl. my leg sEts’E/n. hill tétlku'tl. my foot srk'é’. island nnu. big toe k @laitchd’r. salt JEsa'l (Chinook jar- toe nail k-élak’n’n. gon). my bone suku't. stone tshé. my heart sEtsi'y (? see chest) tree titci/n. my blood sEti'l. black pine tcinti’ (?). chief néte'il’i’n. all trees titcinga’ts’éi. 4 ouse kho. Fuel tséz. ' This ‘z’ is exceedingly weak, so much so that part of the breath escapes laterally, giving it a decided ‘1’ tinge. ON THE NORTH-WESTERN TRIBES OF English tail dog black bear deer, buck =e mosquito snake bird feather ming tail of bird foot of bird. Foolhen goose duck loon teal duck bald-headed eagle young eagle Jish salmon trout Jish tail white black red blue yellon, green large large river small small lake small creck strong old man young good bad a bad man dead sich Chilcotin kye. tlén. SEs, tayé’s. nési' ily. asts’B’z. ts’iH. tlarash’n, pE (?). tcus. pEt’a’, pEt’sE’n. dandzp’n. nad’atsw’l. da’kin. shaiky. tla'i. kyérs. dEk’a’i. pEkyilarai’t. tléyé’l. tlet’é’s. dildi'l. détltsa’. dzlts6’r. intea’. kuntcak’6. ntsdédl. péngo ntsodl. tcarénligo ntodl. nadént’i’. dagolduin. k’a’néralitl (?). tlaago’su. péKunidyi't. dené’tla atltsE’n. daltsha’n, dEnéita’. * CANADA. 665 English Chilcotin cold gEzk’a’z. warm g0zé'lgun, Ds siit. thou né’in. he a/yin. we two nantini']té (7). me kaqonétla/‘n. all kats’é'i. Many tlaa'tla. jar tlaagosh’t. near intltidyil. below kigyaq. to-day k’andzi'n. to-morron k’apE’n. yesterday atlqatlda’. he speaks the truth atVa’risEn. yes ha’‘a. no qa'tada’. nothing daq. one éntli’y. two na’ké. three tha’. four de’i. Jive askonla’, sia tlgyanthai’. Seven gyétlgatlgyaneé'lt’é. eight k’aHiné'lt’é. nine tigyalagontané'lt. ten tlt’a’una. twenty natl’a’una. thirty thatlya’una. forty détlyauna. one hundred nélagau'néldétl’auna. to eat ats'iyé’. to drink thatsété. I walk sétrasts’a’tl. to dance tsEnadai’H. to sing tsigdyé’n. I want to sleep ntastHé’tl. I sleep satlagaitlqé’n (?). to speak iazétld’i‘ky. In the Tenth Report of the Committee (p. 33) I have compiled the known words of the Tinneh dialect that in former times was spoken in the Nicola Valley. I have compared these words with Chilcotin and Nétca'ut’in words, first by asking for the equivalents of the English words, then by pronouncing the Nicola Valley words. In a number of cases I obtained equivalents which showed close correspondence. English woman black bear ram of mountain sheep ene of mountain sheep mountain sheep lake trout snake bear berry horn arron: child tahe it! Nicola Valley tsik’hi, tsé-akai’ sass, sus, sas sisia’ni tpai ti-pi sipai'i tlosHo’ ti/nEH (até) ke (qe) étltcot (I may give you) Chilcotin tsé’ké SEs cicia’n cépai’ te'pi sa/pai tlarash’nh ti’niH até’ ka kéi éntltci’t Nétca’ut’in ts’e’/ku sas sriya’n spai’a sapai’ tlagk’s tEniTlt ate k’a yige’itltcut 666 REPORT—1898. These words agree very closely on the Nicola Valley dialect and in Chilcotin. Only three among these twelve words differ in a manner which cannot well be explained by difference of perception and transcription. They are the following: ene of mountain sheep Nicola: tpai Chileotin: gdpai’ — Néted'ut’in: spai'a. snake tlosHo’ tlarasE’i tlagE’s. lake trout sipai’i sa’pai sapai’. Since three words were collected from more than one individual, and by three different collectors, it seems likely that there existed an actual difference between these dialects in regard to these words. The following words of the Nicola Valley dialect was not understood by either Chilcotin or Nétca’ut’in when read by me. In a number of cases I obtained the equivalents of the English words in the two last-named dialects. Nicola Valley English Chilcotin Nétca'ut’in t-haeh Man tinné, ta’yan _— tine’ tet’-hutz man — = thate man — _ nootl man — = hdalhiltu’ tai a fish — — taki'nktcin a sish — - zalke’ke ground-hog téti/ihy tétni’ tsho buck of deer nési’ny yésts’étine’ tEqo’ztz soap-berry no’/ruc nawa’c notl-ta-ha’t-se } notlqa’tzi ie currant tqaltsE’l (?) = qtlona’zi ta-ta-ney,’ | 5 tét-ta-a-ne’ knife pala’ ali’s ta-a’-ni J tsaé spoon k-a’nin sE/nts’atl ska-kil-ih-kane rush mat gultli’s hutlz’s naltsi’tse arron-head duntai’ nwntai tlutl packing line qetla’ntiy qétla’t iy ti-li-tsa-in give me the spoon ! nnan té k'a’nint — n-shote give it to me! nna te pin-a-lé-él-i-itz take care! sotséIné’tlé wo’nli a’we ge come here, child -— I have omitted the numerals in the comparison, because I suspect that those recorded by Mr. Mackay (Z.c., p. 33) are not numerals, but various words which the informant enumerated as known to him. I think that this is the case, because many of them agree nearly or quite accurately with other words of our list. Mr. James Teit, who collected a number of words from the Indians, first called my atten- tion to this fact. The following list shows these agreements: . Numerals Other words one, Sa-pe sa-pie, trout. two, tun-ih tin-ih, bear-berry. three, tlohl tlotl, packing line (Teit). fowr, na-hla-li-a — Jive, e-na-hle — siz, hite-na-ke — seven, ne-shote n-shote, give it to me! eight, k-pae t-pae, ewe of mountain sheep. Nine, Sas sass, bear. These agreements and the fundamental differences between these numerals and those of all other Tinneh dialects make the series more than doubtful. Although the apparent differences of a small vocabulary like the present have no great weight, I am inclined to think that there wasa difference between the Chilcotin and the Nicola Valley dialect. The language was, however, evidently very closely related to the Chilcotin, while it differed considerably from the Carrier dialects. om ON THE NORTH-WESTERN TRIBES OF CANADA. 667 V. Summary of the Work of the Committee in British Columbia, By FRanz Boas. At the time when the Committee instituted their investigations, the inhabitants of the Pacific coast of Canada were less known than those of any other part of the North American Continent, with the exception, perhaps, of the tribes of California. What little we knew was based on the brief descriptions of early travellers, or on indirect information obtained from investigators who had been working in the regions to the north and to the south. The only noteworthy work done in recent times was that by Dr. G. M. Dawson during his frequent geological expeditions to British Columbia. But three important problems remained to be solved ; the numerous languages of the coast were still unclassified, and the number of their dialects was not definitely known ; the physical characteristics of the tribes had never been investigated ; it was not known if they repre- sented one homogeneous type, or if several types were found in the Province. Finally, the study of the customs of the various tribes offered a number of difficult problems in regard to the origin and significance of several phenomena. Material advance has been made by the efforts of the Committee in all these directions. The number of languages and dialects is now known, and it does not seem likely that additional ones will be discovered. The following languages are spoken in British Columbia :—Athapaskan or Tinneh in eight dialects; Tsimshian in three dialects ; Haida in two dialects ; Wakashan in two divisions, the Kwakiutl with three dialects, and the Nootka with two dialects ; the Salish in four main divisions with eleven dialects, and the Kootenay. In this enumeration, dialects which may be classed as well developed and pronounced provincialisms have not been counted, but only such dialects as show distinct differences in voca- bulary and grammar, so that intercommunication between the tribes speaking them is, even in the case of the most closely affiliated dialects, not easy. We count, therefore, in all, thirty dialects, which have been here classed, according to their affinities, under six linguistic stocks. Grammatical sketches of all these dialects have been obtained ; but a few only are known tolerably well. These are the Kwakiutl and the Tsimshian. All the others require much fuller investigation than they have heretofore received. . While the present state of our knowledge of these languages does not permit us to assume that the number of stocks to which they belong is smaller than the number given above, we may call attention at this place to the morphological relations of some of these languages, which suggest the desirability of further inquiries into their early history. Haida and Tlingit—which latter is spoken in southern Alaska—have a number of morphological traits in common. While all the other languages of the North Pacific coast use reduplication for grammatical purposes, no trace of reduplication is found in these two languages. There is no gender, and no well-defined form for a plural or distributive. Com- _ pound nouns are very numerous, the composition being effected by juxta- position. Words of two, three, and more components, which do not modify each other, occur. Local adverbs, which always retain their independent forms, frequently enter into compound words of this kind. In both languages there are four forms of the personal pronoun. In the 668 REPORT—1898. independent pronoun, the selective and the ordinary forms may be dis- tinguished. The pronoun of the transitive verb differs from that cf intransitive verbs, the latter being identical with the objective form of the former. In this respect there is a close analogy between the Haida and Tlingit, and the Siouan languages. The Tsimshian presents an entirely different type of language. We find a plural based largely on reduplication. The pronouns are suffixed to the verb. Words are formed almost exclusively by means of prefixes. The system of numerals is very complex, as there are different sets of numerals for various classes of objects. The southern group of languages—the Kwakiutl, Salish, and Chemakum (which last is spoken in the northern part of the State of Washington)— have a series of very peculiar traits in common. Most prominent among these is the occurrence of what Trumbull has called ‘ substantivals,’ which play so important a part in the Algonkin languages. Such are, primarily, parts of the body ; furthermore, designations of localities, of fire, water, road, blanket, domesticated animals (7.¢., in olden times, the dog), and many others. These substantivals do not occur in any other northern language, and must be considered one of the most important character- istics of the languages in question. All these languages use reduplication and diresis for forming collective forms and plurals of verbs. The demonstrative pronoun is used very extensively, and serves for distin- guishing locations of object or action according to the three forms of the personal pronoun ; namely, such as are located near the first, second, or third person. Besides these, a great many locative suffixes are used. Whenever an adverb accompanies the verb, the former is inflected, while the verb remains unchanged. When a transitive verb is accompanied by an adverb, the latter always takes the suffix of the pronominal subject, while the verb takes that of the pronominal object. The Kootenay presents still another type of language. It incorporates the object in the same way as the Mexican does, the noun itself being embodied in the verb. It has very few substantivals, if any, but forms compounds by verbal composition, like the Tinneh (Athapascan) and Siouan. While in the preceding class we find, for instance, compounds expressing states of the hand, of water, fire, &c., we find here compounds expressing actions done with the hand, the foot, or other instrument- alities ; and in the water, the fire, or in other localities. It seems that there is no reduplication. It is worth remarking that these types of language are characterised by a few very general features that they have in common, and that dis- tinguish them from the other groups that are found in contiguous areas. The Haida and Tsimshian are spoken in the extreme north ; the Kwakiutl, Salish, Chemakum, in the whole southern portion of the Province, and they adjoin the Algonkin, with whom they have a few peculiarities in common. The Kootenay is not far separated from the Shoshonean languages, which resemble it in several particulars. We may therefore well say that the languages of the North Pacific coast belong to several morphological groups, each of which occupies a continuous area. The investigation of the physical characteristics of the Indians of British Columbia has resulted in establishing the fact that the people are by no means homogeneous. As compared to the Indians east of the Rocky Mountains and farther south, they have in common a lighter com- plexion and lighter hair ; but the shapes of their heads and faces differ ON THE NORTH-WESTERN TRIBES OF CANADA. 669 considerably. Three types may easily be distinguished—the northern type, represented by the Haida, the Indians of Nass River, and the Tsimshian ; the Kwakiutl type ; and the Thompson River type. These types may be characterised by the following measurements :— |: a | Northern Type | Kwakiutl Type ! Laie Sar & eal ——__---— ~ | ) Avennge| [een | Avenge| eer || Averese| Stor I. Men. mim. mm. mm. Stature. : : a fe 1675. jl) 4°7°40 1645 +590 || 1634 +790 | | Length of head . . | 1946 | +080 || 1887 | 42:19 | 1865 | 40°55 | Breadth of head . .| 1606 | +067 || 159°0 | +100 | 1559 | 40°52 | | Breadth of face . .| 153-7 | +£0°85 151-4) \),3:0°54),)) 1474, 20-41 | Height of face . ‘ 121°6 +0°87 || 128-0 +067 | 1203 +072 | Il. Women. | Stature. . . .| 1542 | 25-70 | 1587 | 4590 || 1540 | 45:00 | Length ofhead . .| 1856 | +0-88 1869 | 41-64 } 1795 | +0°53 Breadth ofhead . . | 1532 | 40:90 | 1543 | 2144 | 1500 | 20-41 Breadth of face | .| 1439 | 4080 || 1443 | 20-64 || 1888 | 20-40 | Height of face. | 1143 | + 0:93 119-3 |. +0°82 | 112°5 | 4054 | i They may be described as follows: All these types are of medium stature, and their arms are relatively long, their bodies short. Among the northern type we find a very large head. The transversal diameter is very great. The same may be said of the face, which has an enormous breadth. The height of the face is moderate, and therefore its form appears decidedly low. The nose is often concave or straight, seldom convex. The noses of the women are decidedly concave. Its elevation over the face is slight. The point of the nose is short. The dimensions of the head of the Kwakiutl are similar to those of the northern types, but the head seems to be slightly smaller. The face shows a remarkably different type, which distinguishes it fundamentally from the faces of all the other groups. The breadth of face is nearly the same as that of the northern type, but its height is enormous. The same may be said of the nose, which is very high and comparatively narrow. The point of the nose is short: its elevation is also very great. The nasal bones are strongly developed, and form a steep arch, their lower ends rising high above the face. For this reason convex noses are found very frequently among this type. Convex noses also prevail among the women, and for this reason the difference between the female form of the Kwakiutl and the female form of the northern type is very great. _ The Thompson River type is characterised by a very small head, both diameters being much shorter than those found on the coast, while the proportions are nearly the same. The transversal diameter of the face is much shorter than that of the coast Indians, being nearly the same as that found among the Indians on the plains. The face is much lower than that of the Kwakiutl type, and also slightly lower than that of the northern type. The nose is convex and heavy. Its point is much longer and heavier than the point of the noses of the coast types. There are good indications of the existence of a few other types, but they cannot be distinguished with certainty from the types enumerated 670 REPORT—1898. here. It is probable that further measurements will show that the tribes of Harrison Lake and the Gulf of Georgia represent a fourth type. The distribution of the types of man in British Columbia has an important bearing upon the much discussed question of the classification of mankind ; while some anthropologists have maintained that all classi- fication must be based upon considerations of language, others maintain as rigorously that the main consideration must be that of physical type. The data collected by the Committee show clearly that neither of these contentions is entirely correct. We have seen that certain tribes—such as the Bilqula, who linguistically belong to the Salish group—physically belong to another group. This shows that the two phenomena do not go hand in hand, but that they constantly overlap. The classification of mankind according to physical characteristics takes into consideration only the effects of heredity and environment upon the physical type of man. Race mixture, isolation, and effect of environment will be reflected in the results of these classifications. But there are evidently cases in which a slow infiltration of foreign blood takes place, while language and customs remain unaltered or changed to but a slight extent. The Bilqula branched off from the Coast Salish at an early time, and retain the Salish language ; but there has been an infiltration of Kwakiutl blood and of Athapaskan blood, which has entirely changed the physical features of the tribe. With this infiltration of foreign blood came foreign words and foreign cultural elements, but they were not sufficiently powerful to change the original speech of the people. It is clear, from these considerations, that the three methods of classi- fying mankind—that according to physical characters, according to lan- guage, and according toculture—all reflect the historical development of races from different standpoints ; and that the results of the three classifica- tions are not comparable, because the historical facts do not affect the three classes of phenomena equally. A consideration of all these classes of facts is needed when we endeavour to reconstruct the early history of the races of mankind. Tt will be sufficient to point out in this place a few of the more general results of the studies conducted by the Committee on the cultures of the primitive people of British Columbia. In the Reports of the Committee only brief abstracts were given of the mythologies and traditions of the tribes, but full collections were made ; and a comparison of these has led to the following results :—The culture of the coast tribes of the Province is quite uniform. It has reached its highest development in the district extending from Queen Charlotte Islands to northern Vancouver Island. As we depart from this region, a gradual change in arts and customs takes place, and together with it we find a gradual diminution in the number of myths which the distant tribes have in common with the people of British Columbia. At the same time a gradual change in the incidents and general character of the legends takes place. We can in this manner trace what we might call a dwindling-down of an elaborate cyclus of myths to mere adventures, or even to incidents of adventures, and we can follow the process step by step. Wherever this distribution can be traced, we have a clear and undoubted example of the gradual dissemination of a myth over neighbouring tribes. The phenomena of distribution can be explained only by the theory that the tales have been carried from one tribe to its neighbours, and by the tribe which has newly acquired them in turn to its own neighbours. It is not ee a ON THE NORTH-WESTERN TRIBES OF CANADA. 671 necessary that this dissemination should always follow one direction ; it may have proceeded either way. In this manner a complex tale may dwindle down by gradual dissemination, but new elements may also be embodied in it. It may be well to give an example of this phenomenon. The most popular tradition of the North Pacific coast is that of the raven. Its most characteristic form is found among the Tlingit, Tsimshian, and Haida. As we go southward, the connection between the adventures becomes looser, and their number less. It appears that the traditions are preserved quite fully as far south as the north end of Vancouver Island. Farther south the number of raven-tales which are known to the Indians diminishes very much. At Nahwitti, near the north point of Vancouver Island, thirteen tales out of a whole of eighteen exist. The Comox have only eight, the Nootka six, and the Coast Salish only three. Furthermore, the traditions are found at Nahwitti in the same connection as farther north, while farther south they are very much modified. The tale of the origin of daylight, which was liberated by the raven, may serve as an instance. He had taken the shape of the leaf of a cedar, was swallowed by the daughter of the owner of the daylight, and then born again ; afterwards he broke the box in which the daylight was kept. Among the Nootka, only the transformation into the leaf ef a cedar, which is swallowed by a girl and then born again, remains. Among the Coast Salish the more important passages survive, telling how the raven by a ruse compelled the owner of the daylight to let it out of the box in which he kept it. Thesame story is found as far south as Grey’s Harbour in Washington. The adventure of the pitch, which the raven kills by exposing it to the sunshine, intending to use it for calking his canoe, is found far south, but in an entirely new connection, embodied in the tradition of the origin of sun and moon. But there are also certain adventures embodied in the raven myths of the north, which probably had their origin in other parts of America. Among these may be mentioned the tale of how the raven was invited and reciprocated. The seal puts his hands near the fire, and grease drips out of them into a dish, which he gives to the raven. Then the latter tries to imitate him, but burns his hands, &c. This tale is found, in one or the other form, all over North America, and there is no proof that it originally belonged to the raven myth of Alaska, Other examples may be found in the collection of traditions published by F. Boas.! The proposition that dissemination has taken place among neighbour- ing tribes will probably not encounter any opposition. Starting from this point of view, we may advance the following considerations :— If we have a full collection of the tales and myths of all the tribes of a certain region, and then tabulate the number of incidents which all the collections from each tribe have in common with any selected tribe, the number of common incidents will be the larger the more intimate the relation of the two tribes, and the nearer they live together. This is what we observe in a tabulation of the material collected on the North Pacific coast. On the whole, the nearer the people, the greater the number of common elements of traditions ; the farther apart, the less their number. ‘ Indianische Sagen von der Nord-Pacifischen Kiiste Amerikas, pp. vi-363. Berlin, 1895, 672 REPORT—1898. But it is not the geographical location alone which influences the dis- tribution of tales. In some cases, numerous tales which are common to a certain territory stop short at a certain point, and are found beyond it in slight fragments only. These limits do not by any means coincide with the linguistic divisions. An example of this kind is the raven legend, to which reference has been made. It is found in substantially the same form from Alaska to northern Vancouver Island ; then it sud- denly disappears almost entirely, and is not found among the southern tribes of Kwakiutl lineage, nor on the west coast of Vancouver Island, although the northern tribes, who speak the Kwakiutl language, have it. Only fragments of these legends have strayed farther south, and their number diminishes with increasing distance. There must be a cause for such a remarkable break. A statistical inquiry shows that the northern traditions are in close accord with the tales of the tribes as far south as the central part of Vancouver Island, where a tribe of Salish lineage is found ; but farther they do not go. The closely allied tribes immediately south do not possess them. Only one explanation of this fact is possible, viz., lack of assimilation, which may be due to a difference of character, to continued hostilities, or to recent changes in the location of the tribes, which has not allowed the slow process of assimilation to exert its deep- acting influence. The last may be considered the most probable cause. The reason for this opinion is, that the Bilqula, another Salish tribe, who have become separated from the people speaking related languages, and who live in the far north, still show in their mythologies close relations to the southern Salish tribes, with whom they have many more traits in common than their neighbours to the north and to the south. If their removal had taken place very long ago, this similarity in mythologies would probably not have persisted, but they would have been quite amalgamated with their new neighbours. We may also extend our comparisons beyond the immediate neighbours of the tribes under consideration by comparing the mythologies of the tribes of the plateaus in the interior, and even of those farther to the east, with those of the coast. Unfortunately, the available material from these regions is very scanty. Fairly good collections exist from the Athapaskan tribes, from the tribes of Columbia River, and—east of the mountains—from the Omaha, and from some Algonkin tribes. When comparing the mythologies and traditions which belong to far-distant regions, we find that the number of incidents which they have in common is greater than might have been expected ; but some of those incidents are so general that we may assume that they have no connection, and may have arisen independently. There is, however, one very character- istic feature which proves beyond cavil that this is not the sole cause of the similarity of tales and incidents. We know that in the region under discussion two important trade routes reached the Pacific coast—one along the Columbia River, which connected the region inhabited by Shoshonean tribes with the coast, and indirectly led to territories occupied by Siouan and Algonkin tribes ; another one which led from Athapaskan territory to the country of the Bilqula. A route of minor importance led down Fraser River. A study of the traditions shows that along these routes the points of contact of mythologies are strongest, and rapidly diminish with increasing distances from these routes. On Columbia River the points of contact are with the Algonkin and Sioux ; among the Bilqula they are with the Athapaskan. This phenomenon can hardly a 4 i tales all over the continent. The tabulations which have been made 7 ‘ ON THE NORTH-WESTERN TRIBES OF CANADA, 673 be explained in any other way than by assuming that the myths followed the line of travel of the tribes, and that there has been dissemination of include the Micmac of Nova Scotia, the Eskimo of Greenland, the Ponca of the Mississippi Basin, and the Athapaskan of Mackenzie River ; and the results give the clearest evidence of extensive borrowing. The identity of a great many tales in geographically contiguous areas has led to the assumption that, wherever a great similarity between two tales is found in North America, itis more likely that it is due to dissemina- tion than to independent origin. But without extending these theories beyond the clearly demonstrated truths of transmission of tales between neighbouring tribes, we may reach some further conclusions. When we compare, for instance, the legend of the culture hero of the Chinook, and that of the origin of the whole religious ceremonial of the Kwakiutl Indians, we find a very far- reaching resemblance in certain parts of the legends, which makes it certain that these parts are derived from the same source. The grand- mother of the divinity of the Chinook, when a child, was carried away b a monster. Their child became the mother of the culture-hero, and by her help the monster was slain. In a legend from Vancouver Island a monster, the cannibal spirit, carries away a girl, and is finally slain by her help. Their child becomes later on the new cannibal spirit. There are certain intermediate stages of these stories which prove their identity _ beyond doubt. The important point in this case is that the myths in - question are perhaps the most fundamental ones in the mythologies of these two tribes. Nevertheless, they are not of native growth, but —partly at least—borrowed. A great many other important legends _ prove to be of foreign origin, being grafted upon mythologies of various tribes. This being the case, it follows that the mythologies of the various ‘ _ tribes as we find them now are not organic growths, but have gradually developed and obtained their present form by accretion of foreign material. _ Much of this material must have been adopted ready made, and has been adapted and changed in form according to the genius of the people who borrowed it. The proofs of this process are so ample that there is no reason to doubt the fact. Weare therefore led to the opinion that, from mythologies in their present form, it is impossible to derive the con- clusion that they are mythological explanations of phenomena of nature observed by the people to whom the myths belong, but that many of them, at the places where we find them now, never had such a meaning. If we acknowledge this conclusion as correct, we must give up the attempts at offhand explanation of myths as fanciful, and we must admit that also explanations given by the Indians themselves are often secondary, and do not reflect the true origin of the myths. It may be well to explain this point of view a little more fully. Certainly the phenomena of nature are the foundation of numerous myths, else we should not find that the sun, moon, clouds, thunderstorm, the sea, and the land play so important a part in all mythologies. But it seems that the specific myth cannot be simply interpreted as the result of observation of natural phenomena. Its growth is much too complex. In most cases the present form has undergone material change by disintegra- tion and by accretion of foreign material, so that the original idea is at best much obscured. ao the objection might be raised to this argument that the ; xx 674 REPORT—1898. similarities of mythologies are due, not only to borrowing, but also to the fact that, under similar conditions which prevail in a limited area, the human mind creates similar products. While there is a certain truth in this argument, so far as elementary forms of human thought are concerned, it seems quite incredible that the same complex product should originate twice in a limited territory. The very complexity of the tales and their gradual dwindling down, to which reference has already been made, can- not possibly be explained by any other theory than by that of dissemination. Wherever geographical continuity of the area of distribution of a complex ethnographical phenomenon is found, the laws of probability exclude the theory that in this continuous area the complex phenomenon kas arisen independently in various places ; but they compel us to assume that the distribution of this phenomenon in its present complex form is due to dissemination, while its composing elements may have originated here and there. In the Old World, wherever investigations on mythologies of neigh- bouring tribes have been made, the philological proof has been considered the weightiest ; that is to say, the proof of borrowing has been considered the most satisfactory whenever, together with the stories, the names of the actors have also been borrowed. We cannot expect to find such borrow: ing of names to prevail to a great extent in America. Even in Asia the borrowed names are often translated from one language into the other, so that their phonetic resemblance is entirely destroyed. The same pheno- menon is observed in America. In many cases the heroes of myths are animals, whose names are introduced in the myths. In other cases, names are translated, or so much changed, according to the phonetic laws of various languages, that they can hardly be recognised. Cases of trans- mission of names are, however, by no means rare. We will give only a few examples from the North Pacific coast. Almost all the names of the Bilqula mythology are borrowed from the Kwakiutl language. A portion of the great religious ceremony of the Kwakiutl has the name ‘tlokoa’la.’- This name, which is also closely con- nected with a certain series of myths, has spread northward and southward over a considerable distance. Southward we find it as far as the Columbia River, while to the north it ceases with the Tsimshian ; but still farther north another name of a part of the ceremonial of the Kwakiutl is substi- tuted, viz., ‘nd/ntlem.’ This name, as designating the ceremonial, is found far into Alaska. But these are exceptions ; on the whole, the custom of translating names and of introducing names of animals excludes the application of the linguistic method of investigating the borrowing of myths and customs. We will next consider the social organisations of the coast tribes in connection with certain peculiar customs which have been described in the Reports of the Committee, viz., the secret societies. The northern tribes have materna] institutions, and are divided into a number of clans, which have animal totems. The clans are not con- sidered descendants of the totem animal, but claim that the ancestor of each clan had a meeting with the totem animal, in which the latter became his friend and helper. The Kwakiutl are divided into a number of clans, most of which have animals for their totems. Most of these totems are explained in the same manner as those of the northern tribes, while others are considered direct descendants of the totem animal. Among the ON THE NORTH-WESTERN TRIBES OF CANADA. 675 Kwakiutl we find a mixture of paternal and maternal institutions, but the son is not allowed to use his father’s totem ; he acquires the right to his totem by marriage, receiving at that time the totem of his wife’s father. When, later on, his daughter marries, the right to the totem descends upon her husband. In this manner the totem descends in the maternal line, although indirectly. Each clan has a certain limited number of names. Each individual has only one name ata time. The bearers of these names form the nobility of the tribe. When a man re- ceives the totem of his father-in-law, he at the same time receives his name, while the father-in-law gives up the name, and takes what is called ‘an old man’s name,’ which does not belong to the names constituting the nobility of the tribe. Among the Kwakiutl and Bilqula this social organisation holds good during the summer, while during the winter ceremonials it is suspended. During this time the secret societies take the place of the clans. Accord- ing to tradition, these societies have originated in the same manner as the clan originated. One of the ancestors of the clan met the presiding spirit of one of the societies, and was initiated by him. This seems to be the general form of tradition explaining the origin of ‘secret societies among all North American tribes. All those who have been initiated by the same spirit, and who have received from him the name, privileges, and secrets of the ceremonial, form a secret society. The most important among the societies on the North Pacific coast are those of the cannibals, the bears, the fools, and the warriors. The number of names composing a secret society is limited in the same manner as the number of names composing the clan. Membership in a secret society may be obtained in two ways : by marriage, in the same way as the acquisition of the totem ; and by killing the owner of a certain name. Totem and secret society are not connected inseparably ; but the one may be transferred to one person, the other to another. In order to understand this curious system clearly we must remember that the Salish tribes which are found south of the Kwakiutl are divided into village communities ; while their northern neighbours—the Tsimshian, the Haida, and the Tlingit—are divided into maternal clans. The Kwakiutl have been strongly influenced from both sides. The traditions explaining the totems and the secret societies refer, as stated before, to the initiation of the ancestor of the clan. They are analogous to the traditions of the acquisition of the Manitou. All the tales referring to this subject have approximately the following incident : _ A youth undergoes a ceremonial fasting and purification, and thus acquires the faculty of seeing a spirit, who becomes his protector. The traditions of the coast tribes explaining the origin of clans have the same contents. There is only one difference : the protecting spirit has appeared to the ancestor of the clan, and is now inherited by their descendants without personal initia- tion. In this respect the similarity between the traditions of the secret socie- ties and those referring to the Manitous is much closer, since it is necessary that each new member be initiated by the presiding spirit of the society. Therefore every new member has to undergo the same ceremonies which other Indians undergo at the time of reaching puberty. The beliefs of : the Chinooks of Columbia River are similar to those of the northern tribes, although among them the idea of the acquisition of the totem has been more clearly preserved. They believe that a man can acquire only that spirit who belonged to his ancestors in the paternal line, but the relation xx 2 676 REPORT—1898. of this spirit to the individual is identical with that of the Manitou to the eastern Indian. It can be clearly shown that the development of the family Manitou into the family totem has taken place owing to the influence of the northern tribes. In order to make this clear, it is necessary to consider for a moment the clans of the Kwakiutl somewhat closely. In examining the names of the tribes, it will be seen that very often the name of the tribe is the collective form of the name of its ancestor. At the same time a subdivision of the tribe, one of its clans, may have the name ‘ The Family of the Ancestor,’ while the other clans have different names. It seems that this proves that the first clan formed the original stock of the tribe, and that the other clans joined it lateron. This theory is strength- ened by two considerations : first, it is stated that each clan originally had its village at a certain place, which it left later on in order to join others. Almost all these places can be proved to be ancient village sites. Secondly, many clans have names which may be translated, as ‘ Inhabit- ants of such and such a place,’ while nowadays they live with the rest of the tribe in the same village, and have no distinct claims to the territory the name of which they bear. This seems to prove that the present social organisation of the tribe is a late development, and that originally the Kwakiutl were in the same stage of development as their southern neighbours, among whom the social unit is the village commu- nity, and who have no crests. The northern tribes have clearly defined totems, which are inherited in the maternal line, and which have animal names and animal crests. While among these tribes the totem of the whole clan is founded on the tradition belonging to the whole clan, the subdivisions of the latter are explained in exactly the same manner as those of the Kwakiutl clans. The artistic bent of these people has taken hold of these traditions, and has thus formed the crest for the clan and for its subdivisions. There is little doubt that the plastic art of the northern tribes was a most import- ant factor in developing their social system. In the south, where this art begins to disappear, the village community takes the place of the clan with animal totem, while among the tribes located between these two groups, among whom the plastic art is well developed, although not as highly as in the north, there is an intermediate form of social system. It is therefore likely that the development of the social system discussed here has taken place in the northern part of British Columbia. The northern tribes of _Kwakiutl lineage show clearly that their ideas have been influenced by the animal totem of the northern tribes. They have adopted toa great extent the maternal descent and the division into animal totems of the northern tribes. The social organisation of the Hé@iiltsuk-, one of the most northern tribes of Kwakiutl lineage, is similar to that of the Tsimshian, while their southern neighbours, the inha- bitants of Rivers Inlet, who speak the same dialect, retain the more complex organisation of the Kwakiutl ; but they have mainly maternal descent. It is an interesting fact that a great many of the clan legends of the Kwakiutl are very insignificant, while others have important mythical bearings by which they are closely connected with the mythological concepts of the people. It seems probable that clan legends first found their way to the Kwakiutl by marriages with women of northern tribes, whose traditions, according to the customs of the northern region, were ON THE NORTH-WESTERN TRIBES OF CANADA. 677 inherited by the woman’s children. This must have given an important impulse to acquiring or inventing similar traditions on the part of other clans, since their possession was undoubtedly considered a prestige. Probably the fastings of young men and the subsequent hallucinations have furnished the greater part of the material for these legends. It is necessary to consider at this place a few characteristic traditions which belong to the cannibal society of the tribes of the northern and central parts of the coast. The most widely diffused tradition on this subject seems to have originated among the Hé'iltsuk:, but it has spread southward tothe Kwakiutl. It is told that a young girl was carried away by the cannibal spirit. Her four brothers searched for her, and with > g 2 2 = x ) g eee ie ie fbr hee 8 to 4 3 a S 4 _ = i — oa reed —_——_ — wey + + n mes! =a spy © ® 3 “4 © A 3 2 A a g em 2 Boe ode (eit | ele le | gis | = 4H a a 4 A 4 4 wl 8 z ECan ie: FZ a | A a a | A P le 3 = e S £ PI 2 3 PI 8 o Lio} o fo) oS i) io) oy o ° o 2 EI L 2 E nD ra D2 R a R | < © 3 z Se Z. Zi2 | g ¢ z £ ae Sus p | 2 a | 2 = g Z beat be | a aie eg | Sua isle MS Wega ialiisiiab lie Weis eg heals alae eae alesis ale lial eeillig CS el) SRE ae alae ee lelelel2 4 | ERIS eh re heehee lh a SE £\2|4 lg |e | 8 ua litae)|iosaniteae tiie. || ¢ = & met xt ie = ; VElElElSlelf]elel'l SEE CEE WEE A ET ESE eS eal ela le HAE alc) aye We AS We a lee | capital of the | JEIEB)ZIS)2)/2)/8) 21S) 2) ss) e 1S eI ee ele) Sel Sele) el] el eee) e)3)s)a)8 B/B)/a}e/2\2)2 Bl/a)ei|alale)s e present gene | CIEL |) 2 sete ig ula celle lsc (natal lsat ee) eis} *l|eyele | + IL sage = 2 2 | es the orphans | | call 2 2 | 2 Es 2 2 aeeat Re 2|4/ 4] | SOE | 2 2 with vigour by - —- =\= a = . | = ee eS SS ES ee i | port it, because | B. | | F. | 3B F \ F | ¥ Feo || Fe F F| FE d with some of } 40 au 40 || 40 | 90 65 | 65 | 70 | zo | 80 | go |) ga | 93 || 97 26 | 28 | a9 | 29 intimately con- Height standing 1,770 | 1,680 |1,604 1,698 | 1,670) 1,681 }1,602*/1,618 (1,700 1,682") — }1,641 911,686 |LA75 | 1,582) — | — 1,604 | 1,493 |1,686 | 1,6387) 1,491 | 1,677 | 1,547 |)498*) 1,542 1, forced arate | Height of shoulder 16487 |1,402 | 1,282 |1,902 1,838 1,10 |1,921 |1,996 | ng00 | — }1,820 |1,206 {1,182 1,263) — | — 2 | 1,928 | | 1,268 |1,212 1,288 | 1,286 ft to him. It Length of arm 672) 658} 624) 676} 620 | 690) 695| 551) Go| c19 | 6a4| O14 o | — == Git | 650) 718) 677 | 20 855 | 666 capiiers | Finger-reach 1,859 |1,649 )1,640 |1,714 |1,098 |1,705 | 1,078 |1,726 |1,710 |1,052 }1,722 1,702 1,681 | — -|- jsi6 1449 [1,622 | 1,592 | 1,044 | 1,508 | 1,606 |1,594 | 1,658 1,516 | 1,604 | and that they Height sitting eT | B44 | 848 | 830 | 619 880 | 850) 865 | #28 | — — | — || 608 | 6232) veo | sa9| 766 | 760) 835) 788 | 787 | | 768 | 601} 00 | . sents ara Width of shoulders 408 | 406 | 382) 400 | 836 380 | 416 | 890 | gos | Bos | — — } — || 280] 316 | 373 | 355 335 | S64) 852) 829 | 360] B74 | 9358] 848 | 325] 380) 950) x5) 448) 3107) Bel) 323) 390 335 | Ms on = =! ae | z | a pall a3 peices Les | Saez Es s : Length of head 180 | 188) 176 | 177 | 188} 182 182 | 188 | 192 | 172 188 | 181 1a | 176 i yo5 | 171 | ¥ tsa | 169) 176 | 188| 186) 172) 474) 188] 175} 177) 175) 181] 184) 173) 181) 180) 172) 178) 183) 188 Breadth of head 167} 165| 168} 166) 158 | 157 158 | 167] 168 | 168 167 | 14a 168 ier) 152 | 155 | 148 | i67| 154) a47| “167 | 164! x47] 154) 149] 16x | 163) 162) 147] 4G] 164) 98] 157] 157] 155] ioL} 148 Height of face 116} 120) 118} 116) 119 | 121 n6 |} 4 0 106] 110} 110} 107/) 92) 90 | 115 | 112] 109) 102) 111] 106) 106] 108] 112] 110 | 109} 120] 113] 120) 111) 106) 124) 120) 101) 118) 189 Breadth of face 45] 146} 144 al iis | 148 143 | 167 14 49 | 148} 144) 140) 127 | 198 | 139} 198] 136) 199] 144) 142 1s5 | 140)} 198) 184 ya | iso] 138] 142) 147 lasso | ast] as9) 137) 142] 110 Height of nose 2. 48| 66] 60} 62) 49 50 ol AT 60 62 ti] 64 2 | a) 42) 47 43] 49] 41] 44) 40) 49) 48] de} 44 15| 45) 49] 44] 49] 50) 56) 66) 49) 58) a3 ¢ Rreadth of nose - | fo} 41 | 40} 42) 40] 85) 42] 3a] 58 39 so} a1] a3] 43]) st) s2] so] sa] si] so] 40] a | 37| 89} 38 | s2| a4| s4] 38] 99 | 98) SB] 32) 37) 39] 36 Length-brendth index. 856 | 82 | 995 887 | 905 926 | 881) 850 | gon] B84] 876 | 901] B61) B95] B29] KOO ase | 790| 867 | 602 |) 21] 96) seo | 4o8| o1| ass | 895) ave | S65) a85| s14| G20 | gi4| S69) 12) 795) 9¢8] Bis | 872) 918] s7a epee : 74) 748 | 779 | 843| 797] 794] 780 $10 | 703) 882 | a8) 520] 868} 800] Box) 720] B13) 7O4 711 | 769) 764 | 764 |) 724 87] siz | sor} 734) 71) 746) 785] 740) 12] Bea] As) SoH) BLO) B45) 755) 728) Sea) BoB) 787 Bisel sare 972 | 763 | 762| 778] 736 ») 800) 758/816 | 840) 75:0] O60} 804] 745) 309] BLO) TKO 187 1) 769) go4| 706 | 827 \ 820 681 | 791 | 688 | 878) 93:2 028 | 765 | 771|.s18| se4| sos | 76¢| 773] S64] 796) 760) S19} a82) 765) 7 ee ao 2} 437 | 432) 426) 460] 431 | 421) 492) 404) 416) 454 405 439/449] 460| 455 | 460) — | 434] 463) tea] soa} — | — | 419 | 465 | 34 | 457 420 | 4s6| 154) 440) 422) 467) 457) 4a7| 4n2| 409) 442] 482] 428 cay EP [aie ge jas ee Peepers {66 |104-6 )1024 | 1000 | 108-0 | 1024 |10461 | 102 | 1050 | 105: | 1088 | 100-2 1025 os: |1004 } 105-4 } 107-4 }1063,) — }1027 |1101 | 1065 1056 | — | — |10n6 | 107%6 |1025 |1047 | 1027 | 101-0 |101'8 | 1086 | 104-6 | 102-9 | 08:5 | 1011 | L0K1 | 108 | 1004 1028 }1082 ae io Bs os bis me jaa pa ig 635 | 633) G12) 622) 618} GOO] B11 | 515] 494 482 | O87 | GID | 642 650) 625) 500) BIL) S24) — 624) 508) — - 634 ul 499] 652] 611 | G10] 630] 608| 628} G3) 512) Gre) Brs| Gk1| 493) 516) B34) BLS : = : : _Tedex of width of shoulders. | 2601| 228 | 208| 293 | 299) any 22% | 205 | 290] 2921 219! 250 290 288 |. 266] 229) 293) aaa | — 238) 28} — | — | or | 284] 296) an4| 217 | oa 209 | 235 | 237] 238 | x29 | a4] 223] 2n9| 238] 285] 19-97) 299] 221 | 224) 236) 256 ‘Son of No, 18; measured barefoot on sprace boughs. * Son of No, 16; meagured with shoes om spruce boughs. * Measured with shoos on spruce boughs. * Father of No, 2; left Jog aliort; measured with shoes on spruce boughs. » Father of No, 1; measured with shoes on spruce boughs, * Father of No. 41, * Mother of No, 1, * Doughtor of No. 22, [North-Western Tribes of Canada. 2 82:2 80:0 673 an 42-2 99°4 23°7 55:2 43°9 103°6 53:2 22°2 45°3 105°6 51:3 22°8 § Mother of No. 56. 97 | 98 | 99 | 100 | 101 | 102 | 103 | 104 | 105 gS ay, “a a oe © Ae o A Ba g ) I ome | soe | ale | Sr) ale Se eit le | e-) s | s | hee 8 ry <3} oO mM io] = 8 eee ee a le re | gle aes ss 's ee fa ‘3 sg 8 & & 3 3 o q (>) © | r=] rat q r=] aS) xe) = 5 oe Hee 5 5 5 5 5 = a - a ot & x ios Fy a 4 4 —Q Q [ee] ¥. | Bm | MB F. B. Beer bos. B. Pk oy 30 | 35 | 40 | 60 | 60 | 60 | 60 | 6 | 65 | 70 | 70 1,494 | 1,650 | 1,570 | 1,328 | 1,487 | 1,517 |1,563 | 1,480 | 1,492 |1,480 | — 1,238 | 1,297 | 1,274 | 1,056 | 1,205 | 1,241 | 1,281 | 1,226 | 1,229 |1,194 | — 618 | 674] 662| 584| 675 | 671| 667| 634| 654| 676| — 1,485 | 1,581 | 1,560 | 1,375 | 1,571 | 1,555 | 1,560 | 1,456 | 1,508 |1,545 | — 808 | 835 | 866| 708} 764] 793| 792] 760} 746| 720| — 336 | 344 | 372] 295] 340] 319] 348] 313] 336] 332] — 173 | 186 | 186| 164| 176] 183] 190] 178] 182) 180| 189 150 | 159| 150| 153| 151 | 148] 169] 153| 155 | 148| 154 112} 119| 118| 101| 109] 114] 113] 126] 114] 113] 109 139/ 149| 142] 133] 140] 140] 150| 144| 141 | 143] 144 49/ 51] 45] 45| 52] 45] 54| 54] 52] 48/| 50 Aonmeag ts 37) ae || -86.(\ as de | 37] 8s | 40 76 86-7 | 85:5 | 806] 93:3] 85:8] 809] 83:7] 86-0] 85-2 82-2) 81°5 83:1.| 75-9 | 77-9 [Worth- Western Tribes 1. Sdatliumu (continued), = IL. Females | = a ; = See SaTRESa Sar == lSyeneet | a7 61 | 66 | | 7 7 | 78 | 79 a1 | ss | s3 | 64 | 85 | 86 | a7 | #3 | 89 | 90 | 1 | 2 105 eae == A =|) || sd Ee LIE | | = = eee | | ln elas | |inamil eat | ; | ye el as Wee 2 ie 2 ce] | a lle Dales | 4 | | A Walelals gle 2) 3/3 Bleleiglel/aie} ‘3 | 8. | 53 S13) e) Ep || 38 | Name 2 }2)/4/)/2 /e/s 3/68/3 EP ee 4 2/8/32 | Soles ee A et EP 3) 8 s EE IER | Eye: 2 si7lé z qj Hebel icccin lias et Sh || eli |) tS =|s “2 del to tet 8 heat S)/e/e£ | & | | | 2 e | \3 | S | | 5 | —— =I I |- - |e = = [ae ==) | ea eS fe ee | | | | | | | 1 i | | | | | | | | | | | | | | ) | i | | | | | 5 as A | 5 bie] es | 8 | 3 | | 8 etl } 3 | 5 5 | 3 | ep es Eerie i 3 WS eas es [ace year ep rece Gal 2e ey ee ey EP ae Aes syd 2 Be les lese cg As Flalfiigielalelzlalalelelalelalelalalaialglelaigieii lala eleieibieveieiiielel gaia: i B/2/F 1s /2/2)8)5 alelsleleleievelele le (ISS lS EFI E LSI SE) SIS lS iS 2/2 /S/S12 122i ae || s in = = A = = = = is Sx joe | se Pe 7 = = a =|) = = | = = S a = | & a | = = = | a | a) a | a ala |ala | « | a | | a | a | aja | | | ld | Wile! | ea net \. 2 a | a es | ae jee |Z =| eee | ce Observer 8. | B. | B a | Oa B. | Bla |B) oe) Re] Be] Bw | BB B | ¥ | Age 28 ao | 40 | 40 | 40 | 40 | 58 | 60 | oo | co | 6 | 7 |) 6 | 8 | 12 | 18 20 | 20 | 80 - ~ = -_—— aati j—|— | ——| -— |—_| mo. | mm. mm. mm. | mm. | mm. | mm. mm, | mm mm. | mm, | mm. |] mm. | mm. | mm. | mm mm, | mm. m. | mm. | sanding | 1160 | 1,275 | 1,208)) 1248 | 1,604 | 1,645 | 1,603 | 1,631 1,607 | 1,625 1,686 1,665 |1,648 |) 974 | 1,174 | 1,284 | 1,628 1,682 | 1,560 08 | 144 shoulder | 958 | 926 |1,007 | 960 | 1,080 1,309 | — 1,294 |1) 1,822 | 1,285 |1,260 }1,876 |) 747 | 948 | 1,080 | 1,249 1,260 | 1,296 1,282 | 1,238 | Length of arm | 610) 490) 667 | 622 698 | j 112 | | | 761) 700) 785 |) 411} 502! 569 603) 698 6s3 | 618 | Finger-reach }1,280 | 1,150 jit alata 1,531 |1,515 | | 1,666 | 1,788 | 1,654 | 1,679 |1,660 } 1,630 | 1,720 |1,718 1,758 | 1722 |1,689 | 1,681 |} 985 |1,168 | 1,807 | 1,977 | 1,688 | 1,616 |1,675 | 1,602 |1,690 | 1606 | 1,600 |1,485 | 1,581 | Beat | 893) 696 | 650) 622 | 920) asa | 923 | sao | 535| s40| 00] 804) 875| 803| 905} as: 792] 828 | 846 || 525) 46 | 690} 703 | 785 | 749) 870) 827) 780) S07 77k | 808) 835 | Width of shoulders | 261] 264] 298] 266 | sor | } 408 | 402 | 382 | 986] see] 985) 968 396) 84 | 406 | 400 944 || 922 258 | 286 | 830] 942) 429) 375) 356) 358) 346 938 | 836 | 344 | 5 altar eeast roa ere ‘\orerl| | Saleen at 3 zr == = er | pat = =) See foal bears | areas | ee | ee el eT | poeret ot beat | 378) 168) 176) 370 187 | 182) | io} 700 | 187) 189) 192 | 12} 190) 192] 188 195 | 192 | 187 || 164) 157| 166} 181] 177| 166| 185) 172) 185) 181| 174 176 | 181) 181 | 168} 131) 179 186 | | Breadth of bead | 157 152 | 160 | 163 6 | 158 | 107 | 16 166 | 162 | 157 ug 103 | 154 169 168 161 160 M8 189 | 141} 160) 164) 16) 166) 156 156 9) 149) 149 M46 156) 4s 159 | Height of face |} 89) 101 | 104 | 105 8 | 120 | 126] 123) 118] 119 | 118) 123 2} 120) 125 190 19 119 121 |) on 101 | 101 | ue 108 4) 119 109 105 Ml) 17 117} 108 1s 118 ug Breadth of face | 127} 125] 127) 126 198} 151) 148) 153] 198 | 150| 156) a4] 149) 149] 146) 147 153 | 150 14 |) nig | 123) 193] ra] 185) 141) 144 138 aso} 131} 140} 135) 142) 141 149 | Sea Of nose ] 42] 40] oo} 42] si} co| 62] 55] 51) 55| ct} co| oo) o7| or] 67 oa] 54] 67] 65 | 4¢| 44] 52] 46] G1) 44 42] 42] 40] 48] 49] 39] 45} 46 51 | Breadth of os | 4) 31) as] 31} | 42] 38 38} 38} 40) 38) 48| 39] 34] 35 44] 44] 97) 88 2%) %) 92) 83) a6) 39) 37 86 33] 34} 34] 96 $3) = SS eae | — _ — |. — _— = —— — ——| — a - i ‘Length-breadth index 902| 905! 909)! 9 | | q i | 55 \% : fe th index | 92] 905 | 909! 990 775 | 868 | o6 | 874) 839 | B84 | 857 | 818) 808] BOK) FO2| BIG | BLO | 746 | 849 |) 802 885 | 849 | 829] 864) 880] SES) 902 897 869 855 a ace 760 | 408 | B14 | 633 922| 796 | 851 865 | 798 | 76: | 872 | seu | 842 | B84 778'| 798 | 762) 840 s71| 621 | 842] 824 | B44 | B44) 757 61 500 799 779 | 814 | 753 |x index ‘| | 760 | 788 627 | 10 | 781 745 | OO1 | TAL | O79 | O84 | 696) O14 B16 | 816 | 649) 691 595 | 665 | 727 | 635 | 782) 765) 841 83:3, aT 627 | 822 673 ae BLS Index of arm eallaralline sen lincailnccal =S\ mel Ir a a | = alee — ee | el ae Fi aa 163 | 2 Siara 22 | 146 | 405 | 428 | 429) 454 455) 447 436) — A496 | 446) 440) 4490) 487) 426 ATL | 485 | 440 | 4b8 422 | 429} 445 | 4393 | 452) 485 | 440) 436) 447) 447) 449 456 | 456) 442] 456 43:5 | 422 | 439] 45 441 | 428 seal Totes ott poe ae [eee | 997 1028 | 1008 | 1024 |1008 |1054 | 1050 | 1036 | 1084 | 104°) | 1066 | 108-2 | 102-9 | 1052 | 101-4 | 105-8 | 1020 1002 | 1097 | 1047 | 1023 | 990 | 994 | 1018 {1032 1041 [1081 | 108-2 | 102-0 | 1025 | 108-6 | 1053. 1044 | 1045 | 1096 | 1069 1020 | 994 | 1036 | 1056 | 102-5 | 100-0 = 1oh1 ie : — index of height sitting > | 2 | 7 oy 2 tr i U ou + — east an asi | $94) G14 | Bi2) 518) BIT | 642) 608) 688 21 | 564) 506] 520) 521) 512] sea] o30| 547 ora | 504) 531} 516 || 539) 551 | 589] oLa| 516] B10) 597 soa | 21 | o20 528 | so6 | os | ors 539 | 552] 532 522] 508 | 514 | 501 | Ee ders. | 218) 24-9] 296 | 299] 218] 200 | 215 | 220 os | 251 | 292| 241 | 220 | 246 | 225] 243 232| 255 | 228) 210] 921 1 216 ua] 927 | 231 | a2] 29% v5] 213} 244} 204 ae s10j] 5285) 32:88 * Son of No, 95 on of No. 60. * Bon of No. 70. ‘Father of No.8, re a © One hand sti * Daughter of No. 10 (IT). atelbee oNo: $8. 68th Report, Brit. [North-Western T'ribes of Canada. 3 1. StlatluTribes. ce. Stlatliwmnn i —— ; II. Females ae Seas oo Bete & eb ee ets = 4 Number. 11 12 13 14 | 15 16 ae = S ° , a # & & 3s Name. 5 3 a } 2 é. a » sl ot =] 5 < < a) mei ES a ee Peay | z | | nied jssese 2 | oe | go no ag Bo eB seu ere 5 a, | @8 | gs Be Be | Be | £8 | ge | 882/858 SS ao ma a Bes te mes | pss Set Tribe . Ye Rai! Sine s=- | ay | SOF a 3 PS Si | S'S | Digs | S oie | Sp raed Os | OF | wae | woes in ns esa ee | =D. | din®n | a = S x, = si onl qa | Be a si | sj dic Observer B. B. B. B. B. i. ee Age 1J 19 23 40 45 55 a —— : | mm, mm. mm, mm. mm, | mm. Height standing 1,343 1,587 1,553 1,612 1,503 1,592 Height of shoulder | 1,080 1,285 1,263 | 1,360 1,220 1,310 Length of arm 586 | 682 690 681 672 662 Finger-reach . 1,373 1,643 1,625 1,618 1,612 1,605 Height sitting 711 786 794 860 800 793 Width of shoulders 284 372 332 828 | 337 354 |= | Length of head 170) — 174 174 174 186 185 Breadth of head 149 147 147 143; 148 | 157 | Height of face 107 | s-:116 114 120 | 108 106 Breadth of face 128 | 136 133 137 141 145 Height of nose 45 | 48 48 54 47 46 Breadth of nose 29 | 34 34 41 36 36 a eae z ach Length-breadth index | 876 | 84:5 84-5 821 796 84:8 Facial index . 83°6 85:3 85:7 87°6 730 731 Nasal index . 64:4 70'8 70°8 159 766 78:3 Index of arm. 43°77 | 42:9 44:5 42°53 44°8 416 Index of finger-reach | 102-2 103°5 104°6 100°4 107°3 100'8 Index of height sitting) 53-1 49°4 51:2 53-4 53:3 | 49°9 Index of width of shou) 21:2 23:4 21:4 20-4 23°5 | 22:3 68th Report, Brit. Assoc., 1808.] latlioma. nn Half-bloods I. Males 2. Slatliumu mixed with Shuscaup and Tribe Observer B. B, B. B. 4 24 30 30 40 mm, mm. mm. | mm. i Lait 1,603 | 1,609 Height of shoulder oo | 1298 hong 1,462 1.290 | 203 | — | Length ofarm 47)| (ony — 608 759 662 | o77 | — | Finger-reach 1,160 1,006 = 1,390 Lin 13H 1,627 | 1,616 _ Height sitting 636 564 704 HO 864 B80 = Width of shoulders 253 | 302 207 | | a7 | as2 | 385 | 350 Length of bead 176 | 182 al 185 19 | 187 | eadth of Lead 5 164 163 | 157 | 186 | Height of face oo | | 116 1a 19 |} 142 Breadth of face 129 151 M5 145 150 Height of nose 45 | 45 46 51 63 | Breadth of nose a | 0! 43 a | 50 / 2 | Leogth-breadth index | S43 (901 BBL 822 834 Facial {odex TAG B20 0 708 08 | aeT 880 Naval index 6 | ota 489 | onD 636 765 | 786 Index of arm -| 400 | 422 4G | 42 42:0 = Index of fnger-reach 1012 1009 104-9 1025 1016 1022 = Index of height silting wos | ci | 025 | 630 so | so | — Index of width of shoulders. | 299 | 47, |] 289 | oop 0 | 20) — ¥ Son of No. 37 (lia) 1,685 783 1 1 * Father of No. 91 (1, b). [Yoru other Tribes. Andresi mm, S48 080 5x6 | a0 sw6 O14 TI, Females PEI) SCR] ret 3 Bate] ect ty 2 ¥. Shuswap M. Suita 690 | 631 1,026 | 1,518 | 860 | a2 Td | a7) | ard 7) ) adr | tan Ho) ut | 120 136 | 133 | 487 44 1s | Gt uM a4 1 Ho | ao 467 | 870 70x | 769 | a9 | 405 | don 1085 | 1040 | 1004 sou | v2 | oa | 234 | ora | ou | | | Western Tribes of Canada, Kaltei/on 500 a7 186 148 103 ma | 47 | 86 706 | 730 | 756 | ry 107 6u3 3 7a 78:8 in | 100% 90 [North-Western Tribes of Canada. 4 45 46 47 48 49 | 50 51 52 53 54 55 56 | | s = a 2 5 a g g a ; q = 8 a a 3) # a a 4S f 2 3 = o Fa g AY & ra I S 3 9 = a BH 3 5 < iS Sg Ha) 5 be < 2 eh See a Seno it a a La) s) | o o o mY, av. oye ul ested a Pa ae AY. 4 BY. 4 a4 Pee ee oe Be Pe Be | eee 5 S) 5 Sit) theme ool eS: S a o 2 2 S) 2) o 5 =| tos o cs o q g ) SI fs} 3 3 os = } op fe} 3 a ° Sy NS ee ead ae eee i a = = = = . R =) TA eee) Soe | es 2 Se pe 2 ee F. EF B. F. B. F. F, B. B. F. F, B. 50 50 50 50 50 55 55 55 55 55 55 58 mm. mm. mm. mm. mm, mm, mm. mm. mm. mm. mm. mm. 1,683 '°}1,648" 1,668 | 1,640 | 1,633 | 1,690 | 1,662 | 1,630 | 1,638 | 1,639 1,578 | 1,640 1,354 |1,333 | 1,377 | 1,319 | 1,340 | 1,336 | 1,361 | 1,336 | 1,320 | 1,351 1,254 | 1,333 740 718 746 741 722 764 viral 707 700 704 703 735 ( 1,762 1,708 | 1,717 | 1,744 | 1,718 | 1,647 | 1,774 | 1,680 | 1,600 | 1,704 1,666 | 1,696 838 846 846 830 864 852 863 854 822 850 846 807 334 370 381 391 403 358 375 378 351 375 353 369 17] 183 189 185 185 192 186 189 187 191 179 190 178 14) 157 161 159 165 168 155 157 148 157 161 158 155 19; 118 122 118 oly 118 133 127 115 115 110 120 118 14} 149 154 146 153 158 143 150 147 144 152 147 148 53 52 49 55 54 56 55 48 53 49 51 53 5 ] 39 38 40 42 44 38 40 39 40 42 43 42 91)| 85°8 | 85:2 | 85:9 | 89:2 | 87:5 | 83:3] 83:1] 79:1] 82:2] 89:9.] 83-1 | 87:0 81} 79:2 | 79:2 | 80°8 | 76:5 | 74:7 | 93:0] 847) 78:2] 79°99 | 72-4 | 81-6] 79:7 '76)| 73°6 | 73:1 | 81°6 | 76:4 | 81-5 | 67-9 | 72:7 | 81:3] 75:5 | 85-7 | 84:3 | 79-2 44:0 | 43:5 | 44-7 . 45°2 | 443 | 45:2 | 46:4] 43:4 | 42:7 | 42:9 | 44:5] 44-9 |104-1 |103°6 | 102-9 | 1063 1052 | 97-5 |106-7 | 103-1 | 97-7 | 104-0 | 108-6 | 103-4 49°9 | 51:3 | 50:7 | 506 53:0 | 50°4 | 52:0 | 52-4] 501 | B18 | 53:5 | 49:2 | 19:9) | 23:8 22°8 ) 23°8 | 24-7 || QU) 22-6) 23:2 | B14 22°9 | 22:3 | 22:5 ‘© Father of No. 15. 1 Father of No. 84. NT rh et [North-Western Tribes of Canada, 4 3. Siema'olequma. = 1, Males z Number S 1 lez avg] a 9 | 10] m | 12 | a9 | 14 | 18 17 | 18 | 19 | 20 | 2 23 26 | 26 | 97 | 28 | so.) st | 92) | 3) sa |/ 95) ) se | a7 | 38) [a9 | 40 | a 4a | 44 | a5 | a6 | i wa | 55 | 66 s | re | 5 2 | | | =i a ite | a)e)e | 4 |-& | snes = | | reer || 5 8 Ss Meal ise lt eelics: |arllngelus } | = = 5 5 a 3 EB) 21a 3/3 * 3 = g s x 5 4 \ = g = 2 “ 3 5 B/Z 2/3 | 2 Call | 2 g | ls log s Name ; 4} e |e Bla aalestily sisi }3/3)8])/38)42)43) 2] 2 22 8 |3 S003! | jeuiee ele)e/s)s)2ia] 48 4 | | = es ielel/el2l8 2/3/| ase ea lpeallnceallesallecallbsalliee e)2)2)2 WON es EES || EE ee REO ete EL | et Fy 3 3 a) 3) 4 }8 a | 4 |e) |S te ees |) 2 | 3 | SPER ch ce ie ito tee) eee tis eR ees We) |) ce NS pees eet ah cel ll cel ey Ui |= Ss)? |) 3 = s | 2 3 a | 6 5 | a aii | 5 5 | | = = ) | | | | | | | | | | | | |¥3 | ¢ 22 | | “2 2 |g a me 2 oe || a Bo ibe d a |e Ig Veil cel ere ey |e] Pew. Woe g ay ect yee deed e | @ lig | ta Is Sz] 4/4] 2] 2] 4 ee ee | s\|4|4/% oa. Si rahi) cd nnd Se COINS See SA cee | cme lice ullieae legal eenl SI er et ill se lg EO SERN HE che! ECU) HIE ed meet ied oe ae er Eee REED Ce ibe eee ct Ice |] > alee lalaetetaiele tela iahe ls le lei elas felaietale ty (alg Wa laleseliameadlesal (ola iaieiWelpededs |e | mele 22 la lz ie Z/2/a]4 Pal = 2/2/2 Enliery llr 2 | 3 Z| 3 : E 4/3 t ie 3 ei 4 sisi |g |e 2 | 6 | 3 yeaa Selassie lala le leele FFP UGE 2S Sls Slee e lel Bal Bal eel ele le ls le lelelalalile|e lela eleleleleien = =| = 2/2/68 |2 eD|P Ch Vas a2) 3/3 & 5 6 | 3 BS |e a ea ace ag | ® liad anita 4/2/68 ys eal fis S8/Ele|s | 1 | B. B. | B B | 3 | a | a fa |e B B | B. Bi} e |) a | ela |e le} a | w]e Fr Bjm ir] e |e |r | B F | a 8 wo | 10 | 12 | a2 | a | aa | 4 15 | a6)| a7 82/35 | a5 | a5 |/as)] a7 | ase) 40 | 40 | 40 | 40 | 40 45 | 46 | 45 | 4a | oo | | 56 | G5 | 65 | os | 68 | om, | om. | mm. | mm. am mom: | mm. F mm, | mm. mm, | mm. . | mm. | men. om. | om, | mm om. | om. | mom. | mm. | mm. | mo. | mm. | mm Height standing 1,236" 1,246 [1 1,566 | 1,605 1,676 | 1,614 0 | 1,690 | 1,617 1,681 4 1,711 |1,748 1,680 | — 10" 1,544 16480) 1,868 | 1,640 Height of shoulder : | 900 | 983) o87 1,266 } 1,880 |1,370 1,858 | 1,855 [1,422 1,360 | — {1,200 |1,288 /1354 [1,998 |1,377 |1,519 | Length farm. 514 607 | G10) 19 | SAI 710 | 772} 737 757 | 108 | 766 745} — | o72| oss 718 | 76) TAL Finger-reach ~ | 1218 | 1,182 | 1,203 [1,243 1,301 | 1,426 [1,340 | 12 |1,488 | 1,402 | 1,696 | 1,078 | 1,604 | 1,047 | 1,786 | 1,66: 1097 | 1797 | 1,748 | 1,090 1,796 | — |1,658 | 1,607 ros 1717 | 1,744 Height sitting 6 698 | 698 | 672) G77) 705) 778) 719 | 834 | 770| 780| 798| 868) B97 $15 | 900 | 859) 870 $48 | — | 898] BaL 816 | 816 | 830 Width of shoulders 263 | 285 | 300 289) 312) 935| 362] a73 877 | 406 | 395] 350 378] — | sx6| 373| s31 | 370 301 | ie sces| ee = soe Bos =| & 3 = |e i | Length of head. 176 | 178 7 178 | 177 isi | 181 196} 190] 169] 152] 191 185 | 187] 181 | 182 1s9 185 Breadth of head ‘ 151 | 166 146 155 | 154 | 168 | 160} 158) 101 103) 161 159 149} 161 357) 155) 162) 161} 167 156) 151) 168} 167 | 157 | 101 165 Height of face 96] 110] 99 | 108 m4} 1 120} 116] 128] 124} 119] 190 120 110} 128 T9g]} 322) 11g) 124) 124 131) 417} 121} 111) 118 | 122 17 Breath of face. 128 | 192 | 130) 130 142) 194 | 188 150} 4} asa] isn] 148) 154 148 198} 148 Wet} 161) 165} 158] 153 144) 149) 151] 162) 149 | 164 158 Height of nose. is 49} 40) 41 43] 49 | 46 si} 49] 67] 65] 51] at is 49] 51 pa] 55 | 50] 52] 65 65| so] 52 B8)] 88 62 65 Breath of nose 5: 31|} 35 | so] st 37| 38] 98 42} 42] ar] 42] 44] a2 a7 40] 44 43] 42] 43/ 39| 39 41] av] s7}_ 38] 30] se] so] as | 40] 42) Length-brealth index . sca] are] 819 | asa | Koo} sco] 812 | 767) 870 870! 901) g2| 803 874 | 823 | o1o 361 S64 se 80-90] 87 sor | 805 35 so2| soa | 701 | ssa| sza] s7a| so2) aos| en2| sov| 592] 3) su 22 Faclalinder. 2. 760| 998] 761 | s00| 754] sis} 804) a20| 502 788 404 | 800 seo | S10 Sit BL | 827 769) 81 | 707} Si) 856) 795] S08 810) sus} s80/ S21) 909] srs | 801 | 730/ 702] 72] sos 705 oa) | g17| 782] 700] 724) S16) 797 ae 70s | 714| 900) 829] 857 | 720| 727] 771| s60 | 05 Ao 719 | 76 699 77a | 741 s08| sii] si6| sox) aso | 827) 704 750 so4| 800 | O73 760| soo} 70) 781 | Siu) 704 e79 | 727 765 | 867 | 813 | 792 es Sa lsat Weal A om geal ase lasail ao) eaia) igen AegeRil ial 5 Secale tit is | aoa| ae 7) 420 | 40 - = «| 496) 445) 41a | 405 | 423] ato! 424) 450) 489] 430) 453] 490 | Aa) 404 404 455 | 439 | 462 424] 457 | 438] as2] ano} sau] 429] 400 | 447 407 | 450 | 453 | Jo1 — | 46 48 401 | 444) dbo] 45 | 447) aga | 403) 452) 404 faz | 429) 445) 09 pecreach Jos |1032 | 97% | 998 1018 1033 | 995 |1006 |10n5 | 996 | 1080 | 1061 | 1087 | 1024 1084 1048 | 1080 | 102 1008 | — |10¢0 |1019 |101'8 |103.0 1088 }105:3 | 1050 |1088 }106:3, 1081 | 104-4 | 1044 ors | 1058 }1069 | — | 99 JorT 1004 |1080 1024 1068 1052 975 | 1067 977 | 1040 | 1056 }1084 Todex of height sitting . a4 | 671 6 | 658) 546| Geo| co] 518) 6a7 | b10| O45 avo | 6u| 028 627 27 | 526 | 510 524 | 5u4 11] s1G) 688 612) 627] so1| n22) BA) G30 54) 550) 6 so | oa) cos) — |/n91] 610] 499) 013) 07| 600) 680} 04) 020 ie nay Be ane Jodex of width of shoulders. | 291 | 282] 212| 220 | 205) 220 | 202) 298 | 188] o10| 210) 191 | 209 200 232 | 236 | 290 24 | 280 227 | 248 | 220) 295] 229) avo] 208] sro) eta) sto] 255) 213 ava] a ge) — | ars | ete] 199 | are | 228) 20%) 2 226 4 | 223 - | _i_ —— - — = = 7 aa ‘i 7. e W Father of N w BL. * Son of Now 4iand H4 * Brother of No. 9, + Brothor of Nos. 8 and 09. * Sirothier of Nos. 6 and 09, * Brother of No, 6, * Brother of No, 78, Son of No. 45, "Father of No. 1 (IV). Father of No, 9. Father of No. 15, Father of No. 84 oa ty a pine ee [North-Western Tribes of Canada. 5 02 | 103 | 104 | 105 | 106 | 107 | 108 | 109 110 | 111 112 | 113 2 2 & = eee tes | |) ee +a le | BTS Meee ties |e js | 4 | eB | ei] a ies | g < 4 'e) & a q FI D = & a o 4 a] vy o 4 4 4 rid fee |e |e |e | 8) 8B | Bl et a L ee | oO Sy: Ed) Ne SI LS ae es to me == Bee |e) ei elie lel el|a] aie Meee be lB (el ele le | el a | < Ss) o me 5 S) Ss) = S) i F F, B. B F B. B. F. F. B. F, 0) 50 50 50 50 55 55 58 60 65 65 70 m. mm mm, mm. mm. mm, mm. mm, mm, mm mm, mm, 89 | 1,534 | 1,506 | 1,470 | 1,510 | 1,551 | 1,520 | 1,617 1,614 | 1,495 | 1,525) — 89 | 1,240 | 1,232 | 1,208 | 1,245 | 1,238 | 1,234 1,323 | 1,332 |1,226 | — — 21} 670; 664; 703; 665} 708! 686] 707] 751 670 | — = 38 | 1,540 | 1,507 {1,570 | 1,550 | 1,621 | 1,571 1,633 | 1,644 | 1,520 | 1,543 | — 66} 808 | 792; 769] 780} 812] 800} 842] 790] 750 807 | — 45] 331 | 333] 318] 314] 328] 330] 332] 345] 312 337 | — feyetee | 172); 180} 174} 178} 178] 183| 178 | 170 187 | 190 bt | 154/ 145) 150/ 149] 154] 153] 146| 155 143 | 149] 155 17} 114/ 112] 110] 111 EE TOR IT NT Os 6109 120 ited) 137} 185) 136 | 137 | 139| 137] 147] 138 141 139 19 50 49 50 45 51 50 54 52 43 52 48 36 37 35 32 35 37 39 38 37 39 35 41 2 | 865 | 843 83:3] 85:6! 865] 85:9] 79:8] 886] 841 79-7 |} 81:5 ‘2 | 82:0 | 81:8} 81:5 | 81:6} 83:2] 82:7] 85:4! 79-6 | 79:3 77:3 | 86:3 ‘5 | 740} 71-4 | 64:0 | 77-8 | 72:5 | 78:0 | 70-41! 71:2! 90-7 67:3 | 85-4 3 | 43:8 {| 44:0 | 47-8 | 44:0 | 45:7] 451 | 436] 466] 45-0) _ — 1 | 100-4 | 100-0 |} 106-8 | 102-6 | 104-5 | 103-4 | 101-0 | 101:9 | 101-7 1012 | — 5 | 528 | 525 | 52:3 | 51:7 | 52:4! 526] 52:0] 49:1 | 50:3 53°), .— 7 | 216 | 221 | 21-6 | 208 | 21:2} 21:9| 20:5 | 21-4! 20-9 | 223 | — 16 Mother of No. 3. =) i=} 68th Report, Brit. Assoc., 1898.] aad F 4 North-Western Tribes of Canada, 5 7 4 }. Stlemao!lzquma (continued), = | I. Mal = - = = — = —- ~= = — = = =| 2 — | IL. Females =. ler | 5s | 60 | 60 | oi | c2 | 6s sata SS — — — — ~— = + — = 23 28 (ee se | 63 | -64 [Ves | 66 | oz | 6s | 69 | 7 | m1 | 72 | 7 | 74 | 76 | 76 | 77 | 78 80) | st |) 82) |e fa | eof 86 far fe | 509m fon fae | 98 [oe [ise [ae] or | 98) [90 | soo | son | tos | tos | r04 | x05 | 06 [tor 08 a0 | vio | una | 12)| is X | i | Ee —_ : s 2) Z| = a eet j2|/2 | SH Bale: No Weaece|fea|itas lige alla Ig 5 lites |e < | 2 | eS ks ile 2 | a A - | 13/3 SS /elalewayslelelelaislslPlaglslelevele|alelela pl/e|2 |e Z |) 2 2 2 3 > Pel lle |e tenis 2 le|e|/2)2l]2/3 alauerelelileleleleiflaldialglilsiiltial: 26 Valles i 2/2/83 z ap eoleaie | 2)|3 | 2 3 ihe sg | 8 |i i | | alles baa tees |r 2|/8]6 g het | Sith ts SWE EN fae (le cs ©) ‘ Baie . 3 Bul von lien 3 eal aa a) ete IS | | | - - - — =} -| |\— — = SS | ——— = | | | i | | | | | | | | %\|gs\ 2 || Il | | | | | | | | | 5 B l=3| 3 ais 2 lg = z 2 Ells |: “4 2 2 Z 4 | 4/12 g “| 2.| 8 | | u 4 e|4|4)4 4 5 6 |42| 8 lesa) |e | Shek |}ele]/2£)/2)4)48 2 $12) )2)e1¢)2) 2 meen se lcs || aol hist 38 slal4)2ie)2e138 2 S| s 1/32] % eye ye)/2)2)5)8)/8)]/2/8 a/3|4| EO] WE IVSNINSE ae eS eS alns AVE )/4)é |4)3)s] 4 | reuleeal B) 4s | 8 We |S 8 & bts e 22 =| Sites cn a s = s ma =| =p LE! = = 2 =eirs: 1 2 |S s = = = < Fa s | = 7 2 g 4 2 =| 2] 8 |24/3 Sieea esi lean lcselea ca ee (eseileeellediinenled \3 ey Se AEP WE ea) ee ep | q\si=|3|2 Fle g\s JwelZl/azls|/ei3ie 3 med 0] 7S | Mea | eas Sia) 3 |e | 38 [3 )4 s a et eh et Ie 4 Eb eh ep eo el PE er We We Ss) | 2 | & =) (EP |) 5 = | a/R/S)ela)2i2 é | 6 |aa| = ail? 2 2/2/@)/2@/2)/s)2)8 2 it fel |p ee || é|a]3 2/2 & = 6|a 2/6 |/d|/5) 2 | | | = LL z | : serer “3 oe | P| ¥ BBB BE tear D y | | fa [e i yx |nleln| | x |B |e | & |e |B E =). 80s ROG BBO Ree 6s fe | @ 7 |e [oo fos fog) a a0 an fan fae [fas fas fae fae loan | am faz |) as: |%20 Jeo | a2 a2 | ae foes | 28 56 | 55 | 68 | 60 | us | oo . = = =a al alee eal =a palais F \SsheaearlS = a ae a aes (OC ec Seiieapding © =| | 704 1,602 pa poe ian, aR Alera nets lresov 169 11590 Wis6h [1,620 |1.017 | 1,614 | 1,405 | 1,585 | — eight of shoulder jaaze 1,279 |1,305 | 1,897 |1,298 | 1,319 7a1)|'764 |\ 600 rey fier 1,170 1,238 - F AL Had 3 | 166 266 ft “ See =| 759) 701) 723) 785) 797) 722 )) a96 | 407 | 451 49 661 | 704 706 676, 670 708 = Fxer-reach -|- 1,002 | 1,678 |1,703 )1,595 | 1,681 998 | 985 {1,104 1,689 1,584 | 1,688 | 1,693 1,510] 1,550 } 1,021 1,683 - Let sitting =. -| 1 765) sa] 855 816 oti | p92 826 779 | | si9| 821 £08 7s0| s12| soo] S42 = Fath of shoulders 361 339} 380] 308 aio | 99 366 as | 35 | 345 Eau a4] sa] 330 | saz _ ‘es i. \ a0 | 29 305 4 351 i 5 36 | pr cag ey PEEL ye) FSCO CTE 11 | 467 | 159 | 166 180 | 185 480) 161] 181 | 166] 183 | 11| iva 1eo | i71| 18a | i) 175 180) 174) 175] 178) 188 190 Lg 9 oN HE ary) Say oT | tea) a5 | an | 148 157 | 156 149 | 158 | 150 168 ui7| 146} 162] 137) 164 150} 149) 164] 153) 146 165 poeiieares 120 | 118) 418) (322) 921 | a) 70} o1| o 14 121 nz) 19] 11) 105 1s} y19| 120) 17) 14 no} m1} 14) us} 17 120 | Bro eee 183') 140.) 350) 153) 148 ier an 1 146 143 140) 117 145 | 139 136} 134] 160) 14) 199 1s5| 136} 197| 130] 187 139 Helge bo Drees fea) A) CL) a7 | 36 | 37 | 43) a7] a4] 46 60 45) 47 | 52] 45 bi] ss] 48| | 0 to] 45) 51} 50) Gt 48 Breadth of nose 4) 40) 40) auf as) — | ar |\ as | sa i 33\| 35 ao | 37 »| si] 34] 8] 30} se] 36] asl 37 s2] 35] sz] 39] 98 mn ena eae ] 888) 802) 860) 834] 7861 ao1| #20) Kon! BOT) KL 570. var? | sua | ave | x08 | 007| 879 sea | sro) 522) &| #65 | 13 | 693 68 Yacial index a a | 797) *LK | 705 | 769 | 7406 | 724 | 747 | 706 144 7s1| g41 | 839 i 400! 12] 820] 818 B15 ee Het 769) 105) 745) — | ss8| 917) 892) 764 | 972 814 S26 508 S07) | 75) 740)) Td | 640) Chey [Wiexotarm. . 441 | 458 | 457] 455 | 492 | 482] 440 | 440 Ava |4s)|v4g4)| azo (laze | Gis ave | aay |)4ea | age | 408 462 | 438 | 455) 450 | 457 410 | 137 43) 198) 440] 478 | oe Index of finger-reach . .| — usa |1o 7 | 105 | 1000 | 104-4 | 1014 | 101-9 1018 101-5 Jaon7 {103-9 Jo00 | 968 |103-9 }105.9 |101-a | 107-7 1054 |1032 |1026 | 1011 | 1027 | 1016 | 108-8 1661 | 1004 | 1000 | 1008 |1026 | 1016 Index of height sitting. -| 524) 508) cio| 524| coa| soe | 492} 621 BAB | seo! sit) 553) 514 Gio GOR 536 | 530) 526) 524 684 | 528 550 525 | ov) OL | O24 rit 2 2 b 2: a)" . on) 09 216 | 22 216 | 212 Index of width of shoulders. | 210] 296 | 220| 20] 211 | 241] 297217 | 210 220 | 225 | 217 299) 922| 298] 19 251 | 284 | 217 | 240 A) 358 28.2 ay¢| 24 | 206 | 208) ™ Slater of No. 72. W6ierofNow6andB | x @ Sister of No. 1, 1 Daughter of No, 46, \s Daughter of No. 7 (LV.). \" Mother of No. 3. le 5 Sa en le CS = —— ee -— ie Ea 68¢h Report, Brit. Assoc., 1898.] — I. Males Number. 57 58 59 60 61 62 63 64 x) 2 i) | a Name 8 E E ei x 3 6 2 q oS Lm n fo ow 3 iS ss a 5 . | n ' rs © 4 | o 8 a & 3 2 5 2 | 3 q See wig ee ie On) Stel ae Tribe a rs} po o o | “s 0 q = ° an x ° I = Qa s 3 r= id a a g < P| Ay Ss < S) a “si | fs Observer B. B. B. F. B. F, ¥. Bs Age 60 60 60 60 65 65 65 68 mm. | mm. | mm. |} mm. | mm. | mm. | mm. | mm. Height standing 1,718 | 1,512 | 1,546 | 1,591 | 1,704 | 1,528 | 1,662 | 1,660 Height of shoulder 1,422 | 1,185 | 1,279 | 1,305 | 1,397 | 1,298 1,349 | 1,362 Length of arm 759 692 704 723 735 737 722 731 Finger-reach . — 1,683 | 1,602 | 1,673 | 1,703 | 1,595 | 1,681 | 1,692 Height sitting 901 | 767 | 785 | 833] 855! 774! 9816] 865 Width of shoulders 361 356 339 380 358 368 376 361 Length of head 189 177 176 193 181 | 195 188 193 Breadth of head 160 159 | 157 166 151 | 165:°5|) 149 166 Height of face 120) 113) 13) 122] 121 | 117 117 | 114 Breadth of face 153 | 149 150} 153] 148 | 153 149 | 147 Height of nose 52 55 | 54 56 51 | — 56 | 59 Breadth of nose 44; 40, 41 41 38 — 44 43 Length-breadth index . 84-7 | 898 | 89:2| 860} 93-4 |°s51| 793] 86-0 Facial index . 784 | 75-8 | 75:3 | 79:7 | 81:8 | 76:5 | 78:6 | 77:6 Nasal index . 846 } 72:7 | 75:9 | 74:5 | 74:5 | — 786 | 72°9 Index of arm. 44-1 | 45°38 | 45:7 | 45°5 | 43:2 | 48:2] 43:5] 44:0 , 4 Index of finger-reach — |111°3 | 103-7 | 105-2 | 100-0 | 104:4 | 101-1 | 101-9 Index of height sitting . 52-4 | 508] 51:0] 52:4] 50:31 50:6] 49:2] 52-1 Index of width of shoulders. | 21:0] 23:6 | 22:0 | 23-9 | 21:1 | 244 OMT SoU, “1 Sister of No. 72. 4. Silemas'lequma and Other Tribes mixed, b. Silatuma, Sikentsoqe ae 1 Males | Ii, Females ] 1. Males ] I. Fer I] T Males aa ] =I =a = a ee ora al 7 Sao = ———_________ = ; Es es ae SaaS pease a Ca I Es | Py ii ye [EE le | 5 ; : lelglele el 3 | }2)42/8/3)2]2,/ 8 as | z 3 | = | aes) 98. Bla i |i) &] rs stile Sane 2 é is.) 9) Ea a | 2 | ~ A AMEN lex Sa lisailmealeauieaminen | ao ceilis 3 g Bj 2) 2 | = | 2/2 £ 2 |% 2/32] 4 | : S| 2) s|/e&\/2/4 5 5 glelalaelaieeleiele)"|a)a)|4 3 | 8) 2 2 | ie u eal & 6 | 3) 4 & ia | —— = | 1 ) i | i) ale - + - | | | | Hag ema el P| ie i | 43 |4- a3 | z Ie lz 2 |i a lee | / 3 23 2 g|zisls Suis SSN Ta mal z | 52/33 (22 38) 4 ajeials ala alalai#| 8} el e|e elej2lfi)el;elelelelaele! a ‘ 2/\7= 2 a | g E g g & g 3 | 2 g g 3 g 3 3 g Tite Ss, Si 32/32 a3\ 2 B) se } 2 | 8 g |g g) el) ee) a | ai] | ela Weer acca camel | alld Wee Wee ila 2a |3°| 2323 || & glElile ela|s CRE EEE zlala Ble )e leave) a laeleisielela ag | a | os | Ps 2 E 3 4 | i | | ag | 4 | | zat | (a | | | Observer Be vw. | ¥ 2) || eK B. | 2. | Axe | 10 | 12 | 12 | 9 | o | ju | 0 | 10 | | om) om. om mm. mm mm, | mo. | mm. | mm, |) me, | min, mo.) mm,| mu. | ma, | mr. | mm, | mm, | mm. | mm, Height star 6 1A43' 1,530 1611 1,680 1,690 1,318) 1.286 | TATS* 1414?) 1,145 | 1,255 4 140s | 1455 | 1,650 | 1,406 | 1,569 | 1,614 | 1425 i 1,288 | 1065 Height of shoulder 1,159 1,290 1,318 1434 1,395 1,060 | 1,010 18 1,146 |} 905 | 1,009 ub {1,170 Wout 1175 | 1,000 }1,100 Length of arma Gis) 702| 748) 751 | 737 595 554 | asa | 072! 609 635 || 520 | 687 Finger-reach 1498 1,637 1,764 1,711 1,765 1,356 1418 | 1,042 )1,564 [iz || 125 1103 Height sitting 728 | as6 380 696 715| #12 87% 781 || cos | Width of sboolders uo! 378! S354 281 a7 SUL) 265 Length of heal igs) 189) 185 | 176 186 | 179! 183 Jam) is | a6 Breadth of bead 159) 163) 159 165 150 162, NG 158 151 | 185) 163 Height of face 4 123} 124 ns oo) 1 108) 113) 122 We 106 | 112 Breadth of fare z | 5° ««152 «152 ISL Wt 186 | WG 188) WS |) M2 | uo) 134 } 127) 131) 127) 134) 129) 134) 136 124| 129) 127) 126) 126} 130 137 | Mefght of nose oo) 8| 47] av} fo) az) ot] 40) 48) 44) 48) a4) 42 42} 40] 44] 49) 42] an) 45) a7 | Breadth of nose 38) 38) 41 a5 | at} 39 | Jo) 40) st} 36 33} 30] 33| 32] ss| 35] 35| a7 Length-breadth iniler #31 KEG | BLO) B62 85-9. 018 TR] 85 8h0 | rr | 800 | 895 gis | 838) 852) so2| s58| si | 822) are Facial index fs | 765) 81) 816 ALO i TL) 769) 796 703 | 769) $90 | 833 64 806) 784) B11) sit} 811! 900) S90] 764 Nasal index AIS | Ro) 820 724 W744) 799 O78 v8 909 | 898 | 774 857 786 | 760| 750| 744 | 786) 796) 775) 737 Toler of arm (07 464 465 401 456 | 458] 440 | 458) 424 450) 488 | 450 | 401 | to] ant | 425] 400) 192] 495 avy | 458) 410 ab 426 484] — | 408) 461) 401) 450) 409) 4060 Index of finger-reach 1038 1036 hove. 1050 103% | 1005 1021 1064 | 998 1009 | 1062 | 1030 105% 1052 10L5 | 1026 | 1026 | 1006 | 1004 | 1032 | 106-0 | 1003 105°9 1031 | 100-7 | 1028 | 104°8 | 1045 | 1005 | 101-9 | 100-2 1059 1028 | 1007 | 102-9 | 1000 | 1014 | 103-0 |} 105-9 | 1054 | 106-1 Index of height sitting. | 605 | 629| 547 | BAB) G37) GLK | COG) B91| 601] 481) BIG} co1| c10| G20] ca4| ch| ooo] cso] c22) ox2| o6c| O68 532) oti) 596) G19 | — | 518) ce4] sa8| 090 o21| 540 | 32] ceo} Ges) — | s40] 30) ot1| oo- Isdexof width otsboalders | 236) 254 | 220) a20| 24) 224) 29) 297) 200) i95)| 9a | 294] a8 | 220] 211 | 295] 227] 252] 200) se0| 238] 208 asa] 220 | 216 | sea] 230] aa] sro] avs | a4 224) 240 | 228| 232) 215) — | 923] 231) 237) ava Son of No.6 (II1,) * Father of No, 89 (IIL) ) Drother of No. 3. 4 Brother of No, 1. * Brother of No. 6. * Sister of No, 4. 68h Report, Brit. degoe., 1898.) _ (Worth: Western Pribes of Canada. 7% 7. Buonaparte. 8. Shusirap Half-bloods. == | 1. Males IL Females 1. Males Il. Females 100 | 105 | 107 Namber see|| | G SU) [ao an [2 oe ya 6 7 | 8 1 1s | 19 | 20 | 21 ian — il Sale i le ; = = Alea | l@ 3 gs | 5S] 8 {if ) ce 2 rc 2| 3 3 g/|2 jane = - 8 | = 2 | £2 | = | zg] | | 2 a sa 3 | a et |e 2 5 | 3 |ae | z | | 3 2 E\s “ | 3 ria a ! 5 S\4 a Si | |. | Tall 4 = | | = 2) se old eae a lg ow &| ¢g| 6 Ea E | 13 | § £)€/2)2)2 |e leat] é)2)2) 8) = lee teats 22 |2e| 3 | lee = | 2) Ig g/S/o}/o]}5 RRBs) oo} 5 |/6) 5] 6 |g gea| o3 3a /E | a ae te a | 3 a|2)2 2 )2 |SeiR2e s]2]2)2|2 a: aa) 24 2 a |3 Tribe Biilgilieed = | 2s |gee 2/43/43) 8 | ss o32l a= a3] 5s Ga $2 fs | 2/2)2) 2/4/2283) 2) 2) 2] 2 | 5 | Ss cealee bes! 2a | 62 é He Ee a\= 9 EERE RN Efe ecco) oc: 2/2 | ee eee] ce ag | ar 2 $A e |e Ja |R|a}sa bal otsteai| s\ alal|a Eel eles | oe Ld = & : | | | | | |_ = Ea ball la! « Eni Observer © - -| B B. Fr. F. F. BR B. | B. B. b ; fey ae 5 4 \o) 0} 43) | 36 re a Ee ae [om | mm, | mm.) mm. | mm. | mom. | mm. | mm Height standing - * = 1,022 1,155" 1,198 1,787 14277 1, 2 |1,601 1,510 | 1,552 eight of shoulder «| 755 | 901 | 962 1101 | 1,142 1,322 | 1,211 | 1,290 Length of arm A | 401} 496) 527) o27| on 706 Finger-reach. . «| 1,064 | 1,163 |1,245 | 1,440 | 1,500 1727 | 1210 1,016, Height sitting 52 | 636 | 633| 730] 768| 913) 858 | Goa) 722) 716 ws Width of shoulders 232 | 266) 250) 310) 825) 397) 385 § 274) 301880 a Length of bead {aor | 173| a67| 174] 173| 189) 181 | 474) 100 142 Breadth of bead | 10] 149) 149) 150) 155 } 1455) 130 pad Height of face. wa! 101) 96) 101 108 99° 105 os, Breadth of face. ©. | 121] iz2| as} 128] 133 126 137 126 y27| 129) 1M 10 Height of noc 4, 43) 45) 41) 43) 47] WW) 48 | | a we) 4G) 45 49 Breadth of nose , a | | { | mn! | si) aill! (a7 a ace Es 1 | pa] Vengib-breadth index . | 2] e61| 692] 602) ooo | B10 | 850 463 858 86 | 869) 815 m1 |Facillindex. . | 750| 828) 703| 780) s12| ao2| 887 |) 766] 850 740 720 | 829) 767| 820) 867 77 | sid] 709 785 jBaeel oder) a elf SL 78s) | 750 al 724) 774 | 727 || 727) Th) 721 857 | 696 | 825 | 755 | 829 BOD) | LO) | eae Ds | | is] fz | ae Wohexotam . | 395 | 42m | 499] 454| 448 | 494 | 909) 499| 452] a1 | ai7| 4s) goa | ana] 425 | 440) 405] 407) 432] 405) 448) 411} — | 40n| 450) 429] 439) 460) 44a) ao | 447 Tedex ol Gngertesch . 104 |1007 |1089 | 104-5 |1056 |1047 |1082 1022 |101'6 |1044 |1061 |1057 | 97:5 |100% |1011 | 998 |1041 |1068 |105-0 | 1023 | 980 |1060 ||1000 | — |1033 | 995 |102%5 | 1008 |1057 |1024 |1060 | 1010 Index of height siting | Gi0| 648 | 628 | 629] 530 G14 |) 662) 661! 642) Gi3| oa! 562! 623] 648 | GON) GOO) 521 | 528) Da2| 504] 599 || GOO) — | B24) 620) 529) 729) 536) 628) 628) 525 Todexof width of boulders. | 227 | 929 | 208| 225 | 297 | 291| 291) 292] 299| 266) 295 | 232 || 221 | ave] a05| 210] 220| 216 | a0] 221] 219] 296]] 220] — | 224 | 218] 220] avd) sto] 224] 228) 287 * Brother of Nos 4 and 6, * Brother of Nox 2 and 6, » Brother of Now. 2 and 4, * Trrother of No. 2 rother of No, 1, * Hirothor of No. 18. * Brother of No. 7. ANNO - * Tirother of No. 0 * Not lovel ground; measured with sliocs * Sister of No. 12. Sister of No. 1); 1 Sister of No. 4. 1 Sistor of No. 14. Bister of No, 6; Sister of No. 11, | North-Western Tribes of Canada, 8 II. Females | | 48 | 49 | 50 | 51 s2 | 53 | 54 qd a 3 © 8 ] cee |) Se) | Ste | | 2 | el & 5) SS Sc a = (= o|| § | a Vy See = a 8 @ hig (S" | | | = eS ar) b.. S | ee Os ee |) Oe | So aan ea ana | | | | | =|| A & A & A A A a a a 5 es Ss 3S Ss ue) ‘2 pe) 3 HE < 3 3S cleowepe fe )eie|é|s | 8s) sis eu. +: | a | | | | | SS S| | Sol GA aa ee Ee foe F. | &B. | eek eh Be Rk Bee eee 55 55 55 | 55 55 6 9 11 12 13 20 mm. | mm. | mm mm. | mm. rm. | Mmm. | mm. | mm, | mm mm. 1,540 {1,580 |1,594 {1,588 |1,635'3|1,097 |1,320'\1,37015|1,317 {1,487 |1,580 1,285 |1,283 {1,293 |1,815 [1,353 || 840 {1,037 /1,131 {1,045 {1,210 |1,315 644 | 705 | 708 | 693 | 731 || 454 | 576 | 647 | 596 | 670 | 722 — 11,636 [1,686 [1,591 (1,695 |/1,092 |1,348 |1,504 [1,383 [1,518 /|1,652 816 | 825 | 835 | 839 | 845 || 618 | 727 | 724 | 717 | 788 | 799 360 | 363 | 380 | 346 | 323 || 245 | 266 | 296 | 298 | 300 | 314 178 | 183 | 186 | 188 | 184 || 167 | 170 | 173 | 169 | 181 | 181 155 | 162 | 158 | 165 | 157 |} 140 | 151 | 149 | 146 | 142 | 145 | 124 | 129 | 112 | 121 | 125 92 95 | 110 | 112 | 106 | 112 146 | 149 | 150 | 151 | 145 || 117 | 134 | 133 | 127 | 1382 | 133 57 50 | 51 54 57 40 40 47 42 42 40 36 | 41 43 39 40 29 36 34 33 | 36 36 87-1 | 885 | 849 | 87-8 | 85:3 || 83-8 | 888 | 861 | 86-4 | 78:5 | 80-1 84:9 | 866 | 74:6 | 801 | 862 || 78°6 | 709 | 82-7 | 88-2 | 80:3 | 84-2 | 63:2 | 820 | 84-3 | 72:2 | 701 || 72:5 | 90°0 | 723 | 786 | 85-7 | 90:0 | el ae bee fk Sa 41:8 | 446 44-5 | 436 | 44-6 || 41:3 | 43°6 | 47-2 | 45-2 | 45-0 | 45-7 | — 1085 [105-8 |100-2 |103-7 || 99:5 [102-1 |109°8 {105-0 |102-1 |104-6 | | 53-0 | 52:2 | 525 | 52°8 | 51-5 || 56-2 | 55-1 | 52:8 | 54:3 | 52-9 | 506 | | 23-4 | 23:0 | 23:9 | 21-8 | 197 | 228 20:2 | 21:6 | 22:6 | 20-1 | 19-9 er; 5 and 10. 4 Daughter of No. 68. 1s Daughter of No. 38. 68/1 Report, Lrit, Astoc,, 1898.) By, Chileon [North Weatewn Tribes of Canada, = 1. Males = =, == = = —— == La = Toe Sales IL Females ae : Ley sf ah ef eh |e ao fa fas) |) na aa |) ae] te] az jaa |) 01) /) 20!) || ar) |ifea) Fes ree |) 250 isons: 20 | 30 | 3 2 5) 38 3 F Nesters E | ] 5 | I JB) | | l. | | a7) | 38 | ED ee || 37 |) 38 | 39 | 40 2 [4a [a | as en |s0) | 0 |) 02)))) sa | iT | j | — | | { s = Ss ie | | | e | | | § |= Calle 3 Balle | | \4 2 | ire Q e = Shale ta iadls ia SN Se ts Is i 6 cl ede ep ey Ila rep eseeliore A ese \ ce. {| 3 Ps iy z 2] 3|3 5 | BS) SB las) SAS a es see Ss eee | gas eg Seale ag lg fe eet a/_/2 a/2]e/2)/8 2/8 Name |= 4 SE Se EERIE ER FOR SENG iiss (cle IT tel AE GRIEG re Wen ESM Er ER WEE TER EE | eI Ee wT ER ta || F S | Ag | a1 a iss |e he le =| a |e e|/Zi/aj/2/s)e)e)=|2 8|4|4 z 1 = | Jel eieia) sia | )/é6)/e|4 eyP reise) s8)alal eta ies | | | a 5 \aa| 8 | S| Wye Tee 4) = II bom NUT Aste ———— = ; 1 | in| ial = aa i = / : 1 j | | | | | | i i | / i 1 i =] an i 1 } | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | gis | & Er ll i | = = | Cr enN er |) Gel ceecedcr heen tog a ee | a | | | || Sans Saleculpcal | 13 | et Nera es SS See Wis ene I a/3 /3e 2/218 /8 |s)8)2 843138 Ta } 4] | 22 122 Ses 2 2) 22 B/E |S)81/2/3)8 18/8 )8) 8 1218 |® S | 3 | 6 aléeialaiéiala Wesin | ecteamesen esial|i sal eet || ea allltie etl eal | | \6 6 ejeisjslslsajea SiS /S (S/S /S Sls (Si clslsls | | | | | | | | ato) je] | =| | | |__| je | —___—— = = = all — |= "= leat Saal as = i— Oberer ajo je |e} pieilele]e)o|e | ole |e |e [oF |e F(a |e Br |e | @ | oo B. ip EA ee Ee 11 |) 12 20 | 36) || 95 || 95 || 9s 80 | 30 | 30 | 30 | so | at | 35 | 40 | 40 | 40 | ac | 45 oan law = al alles ee ce sa (a [ee |S eile el oe eal es sa ell tans | ae log «= HuI0X|1/0907),2667)1940 1.28 *)1308 1,276 sas: fias0 27 fins 1,610 1,670 11,634 1,613)) 1,688 1,035 "7/1,007 1,820'41,3700 of shoulders 855 | — [1,014 (1,094 [1,062 1,037 1,003 1444 11,605 {1,426 [1,404 1,817 1,346 1,916 {1,863 | 840 {1,097 1,181 Length of arm 5 44 | — | 535 orl | 566 | bas 536 755 | 762 704 722 693 | 731 |) 454 | 575 | Giz each > i290 3 1,835. 1,290 1,314 4,832 [1,648 {1,826 |1,78 1,688 | 1,672 1,591 11,695 1,092 [1,348 {1,504 6 — | 710 | oso | 887 | 919 | 19 | — 87 | — | 885 | 850 | go1 | svi | S03 | s10 | sus aso | 845 | ois | 727 | 724 riaih Gt shouides aE Tear | 255 898 | 406 | 72 | 370 sot | 396 857 | 948 | 351 | 985 | 338 | 355 | 353 a6 | 328 || 245 | 266 | 296 Leogibof head . « «| 163 178 | 167 | 176 | 109 192 | 190 | 187 | 190 195 | 191 | 188 | 181 | 195 | 168 | 1st | 191 | 194 | 189 | 189 | 181 | 186 | 160 | 179 | 185 | 182 | 178 18h |) 107 | 170 | a7s | aco Breadth of head a 8 48 | 152 | 7 | 149 163 | 160 | 167 | 153 1et | 166 | 161 | 168 | 168 | 165 | 150 | 66 | 155 | 13 | as9 | 148 | 162 | 152 | 156 | 158 | 109 | 155 | 157 | 140 | 151 | 149 | 146 | Height of face ars 104 | 111 | 10k | 98 120 | 191 | 130 | 127 iz | igs | ai | aiz | 129 | 10 | 121 | ise | age | ayo | 195 | 11 | 126 | 121 | 125 | 120 | 124 | 124 | 9a} 95} 110 | 113 | Bresth of face ; 190 | 131 | 130 | 192 150 | 154 | 161 | 147 148 | 162 | 152 | 153 | 148 | 154 | 197 | as5 | 147 | 149 | 151 | 145 | 347 | 144 | a49 | 144 | 150 | 146 145 |] 117 | 134 | 183 | 197 Height ofnose . 43} 46] 46) 39 | a4] 47 | 44 | 49) co] 03 | a7 | to | oo) 56) 49 S| ca) 65) 49) 54] 56) co} cs} sa} 58} 55] 65] 65 | o1] o8| os} oo | 67 67) 40} 40] 47 | 42 Breadth ofnose . . | 31] 82} St} 35] 88) 38 | at | s9 | 42] 89 | 38) 38 38 | 41 | 38 | 38 98] 38} 42] 48] 40] 39) BA] 42) 87] 87] 40) 41] 44] 40] 42] 36] 41] 36 40 | 20 )]| 88) Bd} 88 Length-breadth index . . | $39) ‘saa | o10 | 400 | 882 | gou | 787 | #21 | 807 | 850 | B19 851 89 | 812 | 810 | a05 | 856 | 852 | ars | 86a | H41 | 869 | ao | a7 | Bro | asa | ses | 17 | 709 | 862 | Bia | sre | 871 | 44 | 87a | Bou | o29 | ora #53 | se | aun | c61 | aoa | 785 Vocalinder. . . ./ 795 800 | 847 | 800 | 742 | 780 | 498 | 780 | B84 | 818 | 857 951 | 762 | 884 | 80-0 | 401 | gor | Ro4 | 848 | 89x | 995 | so | go4 | 8o9 | 796 | 705 S44 | 883 | 852 | 857 | 872 | 81:6 | 90% | 857 | seo | a¥9 | aay | B20 | a19 862 || 780 | 709 | s27 | e82 | so Naalioer . .. | soo | a3 | 21 | 798 | 721 | cow | o74 | 698 | 804 | 808 | 773 | 790 | ako | 746 mT | 804 | 649 | o79 | 792 | 601 | 770 | 73:5 | 709 | tH | esa | Teo | 794 | 764 | ROT | 741 | G96 | 680 | 745 | 712 | 712 | 727 | 745 | 800 | 784 | 807 | o79 | 745 | 22 ToL | 725 | 900 | 724 | 786 | 857 ieee ara 5 a1) — [424 495 [ass [41a [ass [aro | — [442 [ag | 456 | ace | 495 490 [468 | 457 | 459 | 426 | 496 | 440 Jada | 430 | 496 | asa | 497 | 432 | 480 | 438 | 457 | arr |/4e9 | ase | an [doa faz | 4d | 448 | asc | 4: 455 |418 | 400 | 445 [ase | 446 | 419 | 436 | 472 | a2 | a0 Index of fngerresch . . 1017 996 | 998 | 999 1020 | 995 | 99% los0 | — |Lo45 |1030 j1054 1016 |104-0 1027 [106-0 |1004 |1050 |101'5 [1057 {1096 [1038 |1008 |1041 j109:9 1048 |1022 /1062 |1039 f1043 [1023 |1o38 LOTS |1042 [1055 |1os4 1037 1064 |1o03 lors | — [1085 /1058 [1002 jloa7 | 995 [1021 jt08'8 [1050 j1021 Index of height sitting. | 551 | 550] — | cM | — | ote | oes | cos | — | 519 | o17 | oe | 547 | 498 set | 592 | 537 | ovo |o2d | o27 | — | o20 | oon | 497 | 530 | ors | — | can | o85 | 605 | oan | 505 | 507 | 530 | 490 | ory | oxo | ot | oV9 = jovo | sea | oxo | ove | ore |) o62 | oon | ope | ots | 020 | Index of width of shoulders. | 228 | — | 218 | 200 | 212 | ays | 207 |199 | — | 201 | 218 | 292 | 220 | 217 a9 | 214 | 295 | g29 | 229 | 215 | 220 | 219 | 204 | 190 | 227 | 245 | 299 | 205 | 240 | 209 | 219 | 223 | 209 | 229 | 206 | 295 | a1 | 295 | 228 25 | 234 | 230 | 209 | 208 | 197 | e24 | 202 | 210 | 226 | 202 ‘Eon of Nol *Sonof No.2), *SouofNo.28, ‘SonofNo.48. * Munchback. * SonofNo.48 7 Cousin of No, 18, —_* Father of No. 1; cousin of No 12; son of Nos) 41 and "Father of No.2" Father of No. i," Fatherof No, 51, |" Father of No. 18, "Father of Nox Gand 10, Daughter of No 68. '* Daughter of No, $8. — == oe al OSth Repu = 3 Name © Tribe . Observer Height standin}, Finger-reach , Height sitting Width of shoul | Vorth- Western Tribes, Canada, 9b. Chileotin, Half-blood. | Male || 10. Carrier, ‘) Males Length of head Breadth of hea Height of face Breadth of face Height of nose Breadth of nose Length-breadth Facial index . Nasal index . Index of arm . Index of finger- Index of height Index of width ——— Mother of No. 61. 76 2 3 4 || 5 a <3 | ss | 1 5 ime | o a4 ~ 1D eS | 5p I Ste. ies & iz § 5 = = 43 | 5 | @ 2 ie 5 ' |] } | \ | et: | } | | | | | Do | o8 Nuves gq | | tS q sf & g a a3 a we Lee) So Se os = S | gia || § § ge 8 | 35 4 3 a Bo || = 2 | 24 Boy ae ‘s) S) Sr aaa a A |g | 3 i Ps | ar eo ) | apis: | =e F Hee Bee it Be Boole Be |r Bech sagen tw a A, \ 70 |. 75 12 17> |) 18 1) Boot es 13 1,548 | — | — |/1,495 || 1,685 | 1,654 | 1,775 | 1.535 || 1,423 1,288 | -- | — {1,192 |/1,364 | 1,328 | 1,477 | 1,265 | 1,170 me =| || “eos |) Tel | 725 | TTF) 7OO>|) 668 1,624 | — | — [\1,577 ||1,757 | 1,702 | 1,705 | 1,647 || 1,495 sig| — | — || 763 || 855| se2| 931 | 775 || 765 same =) ell saa) || 37a| Seal sve (> apg ll teas 171| 169| 175 || 185 || 190} 185 | 196] 179'|| 180 154| 149] 149 || 151 || 164] 156] 160] 153 | 159 114 | 197| 106 |} 107 |] 129] 121 | 141 | 130|| 112 143! 140] 136 || 136 || 152] 146] 155] 140 || 131 54 58 53 || 47 59 51 58 53 44 | 36| 39] 39 35 36°| 37) 39) “37 j| < 38 90:1 | 88:2 | 85-1 || 81:6 || 863 | 84:3 | 81-6 | 85:5 || 88-3 797 | 907 | 77:9 || 787 || 849 | 82:9 | 91:0 | 92:8 | 85:5 | 66-7 | 67-2 | 73:6 || 745.1 61-0 | 72:5 | 672 | 69:8 || 72:7 : | 458| — | — || 44:9 || 447] 43:9 | 403 | 45:5 || 46:3 1049 | — | — |/105-5 || 104-3 |102°9 | 96-1 | 107-3 || 105°1 528} — | — || 51-2 || 50:9 | 52:2 | 52:3] 503 || 53:9 213| — | — || 22:8 || 222 22:0 | 21:0 | 281 | 17°5 4oe., 1893, (Worth- Western Tribes, Canada, 9b, Chilcotin, 9a, Chileotin (continued), Halfslood. 10, Cavvier, : es Females (oontinved) | arate Males Number 58 Jer | | c6 | cz | 6 o9 | vo | 1 | 72] zs | 4 I 2 5 1 fa (al a | ane 3 2/23 | S38 5 STE Se ees act 2 2 | 8 a|4 Z Zs a |e} 3 — —|—| - SSS = S| — I | z= isl = 5 = 5 2A, 3 g 5 | 3s =| ae a2 | as > EN) a ee 5 a Fl: 25 | 26 | 90 | a0 | 30 | a5 | 38 | 45 | 47 | 56 mp. | mm no.| mm.| mom. | mm. | om ‘om, | mm. 1,556 1,604 1,571 |1,608 11,050 1,555 | 1,543, 1,002 1,776 |1,535 P 1254 1,964 1303 1906 |1,30) 1,294 1,228 1,281 1,264 1,285 jt |2,265 Length of ann OH 738 G55 | 75 690 | o91 680 | 657 | 683 O81 117 | 700 Finger-reach 1,590 1,718 1,560 1,018 1,085 1,000 1,667 | 1,524 | 1,639 4,502 bis Helgbt sitting — | poi} ss} aio Bil as2 836 | TAL) 709 | 931 Width of sboaldi SIR 32 343 373° HG | B37) 362 874 | Length of heed -| 18s 180 176 172180183184 7 196 | 170 | 160 Breadth of bead . =| 163 119 16 157 155 161 165 100)) -26a)/) 150) Height of face 110 m4 uy 160 14 18k 116 MATS 1180) LS Bresdih of fae 160} 145° 189/138 Mi 6 139 | 143-48 135 165)) 1401), 181 Height of nose | 49) 48) 49) 45 49| 56) 39| BL) 51 45 68))) 1687, asl Breadth of nose 36| 36) 37| 35 so} 8] 97] so) 41| 35| se fees RE) | Length-breadih index - | 890) 896) BO | KB | HS4 | BNO] ONE | B72) B47 | 875! 902 816 | 865 = Facial index 733) 779 777 826) 858) B30) 822) 895 885 | 819 10) are 7 Nasal index s18| 860 778| 776) 612) 7a! 910 804 086 S712) OSB Le Index of rm. +) 448) 452) 420 473) 4o4| 431! 497 | 498 1 428 are 4 {405 | 105 hes) Be Tndex of Gioger-reach - 102% |1060 1003 1009 | 1066 |1021 |1017 | 997 |1011 1057 1080 1082 10s] — ]10110}) 1000); 1060 } 1008 |1ok9 | — | — |}1065)) eet} | 1080 POS eR Index of befght sitting — | 534 550 529) 6a9| 507) odo | 082] 519) os | 025 O19 — | cos} os4| c05| 525) c28| — | — || 5v2|| boo) o22) nau ie | ae } a3 | a9) 220] 2 Index of width of hoalders | 205 | 298| 215) 207| 206] 214 296 | 920) 223) 234 | 210 | 206 — | 215] 224 | 200) 217 213 | |e PERE Ee ey eo Partly mixed with Carrier. + Danghter of No. 69. \ Mother of No. 18, Mother of No. 60, # Mother of No, Ol, ( [North-Western Tribes of Canada. 10 untci’nemua = 1i. Half-blood 13. Okanagan. 13a. Okanagan od with Nilakya'pamua. half-blood. swap. fan | Males | _ Female i Males Female | Male Numi 14 | $f 2 ae 4 a ieee oa 1 | | | | St ep | | 4 Paes, Fs Boe ae | S = | ‘1 — x ' 3 | 5 | | A : Sth \| | Se | i = | | 1| I A ) | | | a =| | a = a a St | s Bae Jf) 2 &| | es | é | ig 2 ES ep = ee a § | : ~ > ‘ o | An a | ss fe) EX) me . Is : atest a| & = i ret | ie | | a fash | Obse} B. F. | B BE | BL) B F \| \| = | Age | 30 ie | 15 || 4 | mi} i} i | 12 |---| i 2 mm. | mm. | wm. mm. | mm. | mm.) mm. ) mm. Heig}1,674 1,412 |1,393 || 1,402 | 1,292 |1,442 | 1,554 | 1,432 Heig] 1,364 1,142 }1,112 || 1,127 | 1,024 | 1,142 | 1,256 | 1,172 Leng) 737 | 609 -619 599 564] 602 G84 634 Fing41,748 | 1,475 1,434) 1,43 1,323 {1,452 | 1,622 | 1,446 Heigl 393 | 724 | 746) © 739 683 | 733 | 836 — | 726 Wid} 398 321} 320, 316 oss | 296) 362 | 310 188 g6| 180|| 156 | 183] 198 || 179 176 Bread 158 } 153 | 1851 143 150] 146} 155 116 Heig] 119 | 107) 104 99 || 100] 116 110 95 143 132) 133 || 127 || 128-| 127)) 141 129 49 V-"4a| 451° 41 42| 47 4 | 3 36 33 34 29 31] 39 32 | 3 i = 840 823 | 839 || 923 | 820| 777 | 866 83-0 83:2 81-1 | 782 |) 780 | 781] 906 | 780 | 73°6 73°5 | 767) 7G || 707 | 738| 830) 727 | 721 ——— | = = =) 44°] | 432 | 445 || 428 || 437] 418 || 441 | 44-3 4104-4 1045 |1029 | 1022 | 102-4]100-7 | 104-4 ! 101-0 535 51-3) 537 || 52:8 || 629 | 544 |) 53:9 | 50:8 23°8 | 99-8| 2301) 226 | 221] 206) 234 | 21-7 Uta'ngt. Female Nomber 1 2 | 11d. Ura'ngt ant i. lle. Na = Uf. Nakyapannug’o'é and other pamug'de. tribes mie Female Females 6 7 8 10 | ap 13 | Observe F ¥ th i B Fr B. B. B B. B a ‘ mM) 46 co 65 16 | 66 0 | 00 o analhiea flan | a ae, ial oe, en Height stand IAG 1,102 1460" 0 1,673 |1,510} 1,500 | 1,467 f 1187 1,014 5 282 | 1,278 | 1,273 | 1,185 far 500 632 = ca 690 | oss] 658 | Finger-reac 144s {1 = 1,028 17783 {1.710 | 1,610 [1,600] 4,568, Tieight sittin 7 - | | 830 —| Bu Width of Te 33; 2 WT $42 B48 38 | 350 1 he 7 M7 192 73 | 188 184 | Breadth of t 156 61 1s it Hiss } 151 16} ght of fa 99! 101) 101 108 7] i) f fo 151 10 1 in 13 1s 0 40 43 18 wo i a | 37 a i) 40 a breath ind 97a 764 “or 21 800 618 812 sit | 60| 897 850 7k ue 708 O42 | 610 oon 166 “ua| 422 43 = 169 490)| 447 124 ch 1029 | 1045 1 1022 =_ 1057 1024 {1030 1002 1003 sitting m6) 022] a | ot | o7 | =) = || Fro 586 || dex of width of shoulders .| 238! 231] 918 ao | — || | 222| a9) 994 29 |) 11g. Nkantetnenua. Man 60 4,670 IAI 819 1,850 Wh Vkantevnrnua mixed with [Worth- Western Tribes of Canada, . Half-blood Nelakya'panua Males 186 | 180 158 | 101 107 182 1s 30 423 Sil) 782 fo, a8 92) 406 1046 | 102-9 ia! 537 299 | 290 13. Okanagan, 10 13a. Okanagan Half-Blood. Female Males Tene Male t iy i 1 ah 3 1 i, F, | &. i F. u 13 1,402 1432 1127 1,172 oak 1416 155 isa} 188 1 150 | 146 00 too || 115 127 128 | 127 10 i2] 47 u 7 os] u9 o23 | 820] 777 740 | 781] 906 707 | 78} 850 428 | 4a7|are|| 441 | 1022 | 1924 |1007 |) 1044 628 bed | O30 205 | 4 ¥ Sister of No, 4 [North-Western Tribes of Canadd. il 718. Heiltsuk . Half- II. Females esac 6 a. es ere ton is |). 12) | rs Vo ne We ae : io = aia | — cate S) } See ee 0 a m | Poems |e Pe) a fe) ee he eee is) ee)" |} 2) 8) e ieee «| | | Z | | | | =] 8 poe = | s 3 | 4 | ci oO ic) 23 ime ec a fou sey ea a 0) a oS i a a sas pea | 2 | | 2] é a. era a) 3 a. ee} lee octet ees rl fac} im) a . i=) | : a a | a | | Meeeraoer | Bb eR Ob Rh Wh Be pie 60 | 70 20 25 | 40 50 55 | 60 35 ek aaa ae —|_—— mum, mm, mm, mm mm, mm. mm mm. mm 1,568 | 1,623 |1,574 | 1,414 |1,533 | 1,465 | — / 1,443 |1,618 1,285 | 1,326 | 1,301 | 1,158 1,265 |1,210 | — |1,181 | 1,305 754 | 743| 718| 633| 633 | 640| — | 667| 733 1,780 |1,774 | 1,654 |1,486 | 1,528 [1,543 | — | 1,536 | 1,723 ee | SiG: | — | S88 | 765, — | — 5 398 {| 358| 375 | 332| 351/ 360; — | — | 393 185 | 190| 185 | 181] 179/ 181! 184| 186| 185 170| 170| 155 | 153] 162] 155| 167} 167] 156 126| 127] 112] 120! 123] 113] 118] 114) 124 163} 159} 146] 141| 165] 162] 148/ 150! 143 ba} 52| 45| 50| 62] 48| 49| 47] 52 47| 42| 37/ — | 40| 38/ 43} 40] 33 91:9 | 89:5 | 838! 84:5 | 905 | 85:6 | 90:3 | 844 84:3 173 | 799 | 767 | 85:1 | 79:4 | 74:3 | 79:7 : 76:0 | 86:7 81:0 | 808 | 822) — | 769 | 792) 87-8) 851 | 635 48-0 | 459 | 45:7] 449] 41:4] 436] — | 463 | 455 114-2 |109:3 }105*1 | 105-1 | 99-7 |105°3 | — | 106-4 | 1068 Pee | SiG) —= | 548 | 51-4.) — rl Loe = 29:9 | 245 | — | =. | odes 26:4 | 22:1 23°9 | 23°5 a4 | 264 | 230)| 295! 920 . =< Aesoe., 1898] 12, Tlingit. 18. Haida. [North-Western Pribes of Canada. 1h ——<—— Sa =e = Vt. Trinehian 15. Gyitkshon. 16. Yieka’. 17. Bi'lyula. 1S. Heittauk | | Baik : ch See a = ——— Se SS — is ] ] P eee ood, : = - || 1. Males IL. Females | Males Males I. Males We I. Mates | Malt: Namber Gpeacieeen {yt 7 | 9 | a0 | a = = >) — ——— j= = = es — —— = = ra a d ae 4 | 6 nee DAE Can fanttall WD | FSC) tae eS 1 a|3 1 2 “1 | DC ean ee |) u | 16 i Ee ] | (lz Veni pe (ial eh esa eee| alll ll =a eeal oe ean se = eel ae a a | a oe }2] 7] 23\8. 3: Nese hie Z Alle ile FORE Aiba ie | | Namen yee es mies ge (A5 | Bs ja |] & |) | = Bhs is 2 | ae Je |2e| & iS a 3,2 | s/s a3\3e 22 22 a le) 4 g | é \ 24 [2 \esle)e)2)\e le g |g E Liles | se|g 5% allie au roe 3 | 3 |e 2123/5) 2 |e | xis | AMS e | Cc | = 2 212 3 3 | g | 8 |az 2 | g=| 2 (2/218 | | = == =: Sa Se FB 5 2 | So Cs EWE Webi | ite |) et iS I | | | | it | | Z| | ale > | fan ae iam = —-!= = ar Se = 3. ] | 2) | | | | yon tl = eS zp | a | ee es | 23 /S2/ = 3 |=] 5 | | = |e 2 z Fa | 3 4 = E | & wh) 3) 3 cl o | selagl| 3 2 S = 2 = 3s | mules Tribe : 2 cI Say | 30/8 Biase | ae 2 | $2\s¢| = = en 3 =z 3 |3 es ri ies tos | 2 22 {se lase Be) ee) = & 2 ¢ r z Vee 2 hese ies | is Ea 32 | tee | ata fad 2 | on] & 5 2 = = | =i |] ie | | ao | aei|iac | > 3 A | s a } a | Sailh t au heal z = | i { = | | sien Bl] a aa ee a relia |—|— ee | es El ee | Pe is = s | | I. B. | B. | op. | B. |B. |B. |B. B. | 3.) B || a. | yy. | Fe req) ne (fae |e ¥ ; Ane a gee 13 | 4 | a9 | a imeealivearlaeni | | caer - =} = - == —== so 18 | | SE | 28 2S | (2 | | sa | as | 45 | 48 | 0) || 20 | go | 2 | a0 | co | oo | 10 35 15 mo. | mm | om. | mm se | errel| bers | to a | =| ] | — —— = = = - — — Height standing - . 72 | 1,654 wy mom. | mm. | mm. | mo. | mm, | mm, | | mm. | mm. 1. | am . | 7 He mm. | om. | mm. | mm, | mut. | mom, ear ee Hl eal beset es {1,048 | 1,008 |1,462 |1.500 {1,628 | 1.6508, 19801760 | 17a2 / 104 | Torres 1t8 (10% 1ye6o | yon | 720 | 102 |e | 1/608 1785 1,000 | 1.697 {rani 1,683 | 1tes | —" [1448 |a\610, ae | : syed] 390)) it 4a16)/2.292 1.246 | — | 4s fair |1,203 | 1,833 | 1,207 /i,o08 |aya4u [1,198 |1,902 |1,978 |1,a10 || 1,105 | 1,004 |) 1,060 | 1,888 | 1,924 | }1an7 [1,904 | fans 1,205 |1,210) — Finger-reach = - 1,810 1,483 | 1486 719 | ox} oso) 1a) 713) ose) 633} — | zo | 701 oes | 688) 780 | 687 —| m0} 71) 775) os) 778| 718 | 758} 741 | 738| 784) 701] oos| 7a7) 701 | 769 } csi! oss} oo) — - Height sitting oy | a 1,658 | 1,553 | 1,501 (1,631 | 1,081 | 1,654 1,660)} 1,810 | 1,802 | 1,546 |1,613 yess A765 1,677 1,830 | 1,730 | 1,792 |1,755 | 1,687 | 1,828 1,686 | 1,778 iret Ai ‘isis 1,677 ‘}1,400 1,784 }a,826 1,721 1A86 (G25, {hows Tew | sian ears elie at 792 | 528 835 | 924) o1n| 808] $18) 826 |) 817) 892 953/ 870) 800) s90| 827 | ais | 905 ])v3a)| (naz | iees. |) asa) — | — | — | (938) 4a} ees) et) — | — | 810) = ey8| 765) — ~ = = on Osi] 9 =| 996 ast) 86) siz) 360 | ao9 | 97a au | art | aco) ai | 364) 407) 364) 366) a8] 422) 495) 972] ais | 400) B01 | B08) sal | 376 35s] 376) 332) 261 - Length of heal . . | 168 go |) 493 neers — —|— —|—}= |—— | ee — — [ese aes —— =|— Breadth of beail 3 181 i a a Be oy Ey og 176 181 | 187 | 90 | 487) 1921 185| 190) 290 | to | 789 | 198! 199) 194 iss) 191| 191) 161) 190] 180 163) 141 | 185 | yoo] 185 | 181) 170 ia Height of face Alea scall ae eh Stee eee M8) 167 | 163 156) 157) 161) 160 154) 150) 160! 153! 106 166) 158) 159) 162 | 167 | 107 159 | 168) 170} 170 155) 100) 102 167 | recess a bf Mo) at |! 117 ! a Na yar) 118 | at) wn) 428) 120) 110| 122) 1 1012 | 124 | 110 16 1 | az! as! ier} ue) 120) 128) 110) 118 Height of nose Ai oa ts ee TEN) 1k 140 | 150 M9) 150) 119) 158 | to! 165} 146) tai! 162! 163 aoa] 151! we 150) 40] 11) toa) 162) 14K Divedi oBrcs eee anenat | ect ai i pal bed se fies a | 45 a7 | 50) os! oo] 2) oa] so] ia] BL) ot Bo) ol) 58) of wo ce) 4a) av) 47 oe in — — 40). 39 40] 33 us i oo 41} 09) 41 12) (38) 41] 85] 35) 42) 43) 4B) 48 ’ Length-breadth index. .| 214 | 89: sail tacall woul fae = | Le =| | mei ey ne on0 | aac] sz9| roo! sia | goa! sin} Spx! spe StL | 808 | 7H9 | S04 | ) sor sso 879| 928 | p04) aoa i . . . «| 30 z 4 o a1] 7 4 7 | | | | Nasal index . 4 4 Peal (eel ces BLO} S48) S41 80-7) 639) 797] BLS }} BLT | BSL | 873 805 | 718) Bld) 810 | 80-0 | 780 | 840 | 762] KOO | SL6 = |— i) | 833) 688 | 717 | 761) 739) 699) 864 | 786 | 760 | 684 $20) 780) 707 S10 | a1 | 774 Kid | 824) 843) 860 | 83:0 c | Indexofarmm =... | 495 | Fi Naas | 4a - =r i =|— i - — — Soa a | ates or ase ae aes Be [3 436 | 453 | 405 | 444 a2] 433 | 320) 108) — | 408] — | sar] aoa | Er (PET (es fe P| | FEC) Wea || asa | se7| ase | az0| as0| d60| 466] 4p5| as0| aso) 159] 457| aco] 04 — | 403 | 155 ae eee. oT allah ot | 1028 J107 }106-1 )10%% |106- |s08a | 107 J1oHa }1087 | 1086 J1002 |1003 }1007 | 103-4 1086 |103-0 |105:6 |106-0 |1070 | 1052 |1ova |104 |1111 | 103 | 1031 |1083 || 1005 |108-2 | 104-8 |1027 |106-4 | 106 | 104-3 | 105-2 }ross 1142 | 1099 |1051 | 1051 | 997 = peal 10658 | 5 3) Ges | 643) G69) 688) 655 | 657 | BAe) G24) GTA | GOB) G42) 521) 629) 638} 530) 628 | ror} ot7| 92) ooa| o37| san| mi) sis| s29\| oes! 626] ono! o20| soo) — | — | — | sa2| ota) cea) tox) — | — | ste) — | DAS eae (| | Index of width of shoulders. | 25:8 | 24+ pee 3 \ otshonldem.| 258 | 244 | 229 | 295 | 232] 940] 219 | 290] 255 | 228] 258] 221] 210) 224] 220] 207] — || 296 2a0| 237 || 20 | 220] 296] 287] 290 | 224 | 107] 220 | 261| 2107 /| 208 | 208 | zee | 25a) ear | 223) 2x8) 176) 241 | 202 i 12 i | Mu © a 1 Height =; ae - eight of polbY/6f second ogec\610) * Son of Nos, 6 and 14. * Father of No. 2, © Mothor of + Brother of No. 6. * Brother of S 68th Repo [North-Western Tribes of Canada. 12 20. Kwakiutl Men. nales | Number. .|17 | 18 | TOW 20 | 2h | 2a 2 3 | @ | 2 | Eile | a | 3 Ri aes a eeisenoe (oe |e: | 4 | 2 |= Ws Name . peat Suen, OS @ A fH | & < ig a | Met w | 3 ro = ss w TD eS x ral a iS) = a q = yen See ia es i = 3 tds) ee a Zz 2 ee | we! | ; oF || ig] 23 Be i & | a oS & oat on le ah 7 “s re) gs >. = aa q (=| q Rl = a = 12 ot = ot Se } e)e | = ge) 8 Sh (es) so) oe pve a | & | # (at) & | eel Fa | Ee | ge E iS Ieee) s _| y|| BIEN Me ers ese ober os | EE tee fe Stl Se aoe <8 fy malar Observer B B B B. | B B B B Age 40 40 40 52 60 || 35 45 40 3 | ‘ m. | mm. | mm. | mm | mm. | mm. | mm. | mm. | mm. Height standing,528 §| 1,457 | 1,492 | 1,508 | 1,544 | 1,462 | 1,540°1,610'"| 1,670 Height of shoul},244 | 1,192 | 1,222 | 1,223 | 1,254 | 1,203 || 1,242 | 1,310 | 1,357 Length of arm | 647 | 619 | 669) 617 | 692 679 672 | 745 | 764 Finger-reach . |,588 | 1,505 | 1,551 | 1,482 | 1,634 | 1,558 | 1,604 | 1,727 | 1,793 Height sitting |865 | 762} 800] 828| 808 | 784 |} 863 |} 843] 806 Width of shoul| 367 | 343 | 308] 356] 3438 3840 || 369) 3878] 390 Length of head 1837) 1667) 1617) 1697; 1767 1837) 1847) 189% 2052 Breadth of heaj 1547) 1467 1537) 1447) 1557) 1607) 1557) 1617) 1572 Height of face} 118 | 116) 114] 118} 120}; 119 124 | 135] 1380 Breadth of facqg 149 | 141 138 | 147] 153} 150 139 | 147] 157 50 45 49 49 52 54 56 58 53 35 36 35 35 38 36 37 36 42 Height of nose Breadth of nos Length-breadtl]84-2 7) 88:07} 95:07) 85-27) 88:17 87-47! 84:27) 85:24 76:62 792 | 82°3 | 82°6 | 80:3 | 78:4 | 79:3 || 89-2 | 91:8 | 82-8 80:0 | 71:4 | 71:4 | 73:1 | 66°7 || 66:71 | 62:1 | 79-2 Facial index . Nasal index . Index of arm. 42-4 | 44:9 | 40:9 | 44:9 | 46°56 || 43°6 | 46:3 | 45-7 103°3 | 1040 | 98:3 | 105°8 | 106°6 || 104-2 |107°3 | 107-4 52°2 | 53:7 | 54:8 | 52°5 | 53-7 |) 56°0 | 52°47) 48:3 235 | 20°'7 | 23°6 | 22°3 | 23°3 || 24:0 | 23:5 |. 23-4 ® Daughter of Nos. 6, 17. * Head flattened behind, = Sth Report, Brit. Assoc., 1898.) 19, Avov/ky'ender. (North-Western Tribes of Canada, 12 20, Kwakintl Men, amber on wi ae Waalix tha iee ha | 2 = | EE = & Ee Name = = 25 z el = = mal a | z l= lan Sale ay |23| 3z #2 = | Ze = | 22] 5 | | hee Ss = (55 = Tribe 22 m |e \3% | ae 5 ee a Se = a | ed 28 == =e | — Aa NE eS LO LE = | elf | Observer : 7) en Jl (ie Fe B |B | ; i ? oo | 65 | 17 | 20 | 20 3 | 40 | 40 | {co} a5 |46 ao oe te a as fee cS tases BS fesse PALES LS | al es om.) om.|mm mm | mm. | mm.|mo.| mm, mm. mm, me. | mm. mm. | mm. | mm. mm. | mm, | mm. | | om. | mm. | mm. | mm. | mm, Height standing. 1560 | 1,666 1,68 (1617 1,613 1,577" 1,693 11500 1,668 1,624 1,532* 1,520 1,02 1,678 | 1,620 |1,528" 1.467 |1,492 |1,608 | 1,644 | 1.462 | 1,540%1,610"" 1,670 Height of shoolder 1,867 | 1301 1801 1,307 1,208 1197 145 1846 1,94 240 1,214 | y,904 | 1,201 |3244 | 1,192 | 1,90 1254 [1,203 |) 1,242 | 1,810 | 1,307 Length of arm O73| 709) 704) 775) 689) tis | TOL) v27) 70x) 7in| G81 eso! G10) 29) os2| G70) AT) c19| cov 602 746 | 764 Finger-reach - 1,598 | 1,688 | 1,714 | 1,780 | 1,682 1,046 | 1,746 1,593 1,695 11,764 |1,608 | 1,688 1,660 | 1,620 | 1,591 {1,692 | 1,688 | 1,505 | 1,651 1,634 1,727 | 1,793 Height sitting | 847) 918 | v13) 826! B03) x67) B31) BAG BN) BBO) BIO) 520 S15) 437 | B44) 865} 762] 800 808 848 | 806 Width of sboulders | sa] 248) 3x7] 505) 975 soo! asa a71| gas| 928] s28 47] 340) a20| 351| 307] gia | 308 ua 878) 390 | — —|— i= —- = ae } <1 t Length of head | ar) tho | 10) 90 aan4 ty0* tks 1HO" 1814 170) 116) 169 182% 180%, 1895 160% 1614 160"! 1704 189 205% Breadth of head | 49) 159 I! 167# 16627 168! 161? 149% 157" 166) 152) 160] 1637 191% 160% 1643 140% 1639 144)! 105% 1014) 1574 | Height of face m4! 186 | 135 as] rot 115, 128 116 | amt m1 | ais] t08| 118) 126) 146 | 11a] 116) 114 | 118] 220 195 | 180 | Breadth of face 138 | 47 162/ 163) 166| 156) 164 148) 156) 40! 187} 142] 199) 145) 148) 149] 141] 188] 147] 168 147] 167 Height of nose 1s| oA wo) 67 | 56 so) 00} o7| 49| 47] 40) c3| 65] m1) co! 45) 49| 49) se 58) 68 Breadth of nose a7) 7 a 40 | 41} 40) 45) 98) 40) $3) 5) 96) 31] 95) 37) 95) 80) me) 85) 98 ao | 42 Length-breadth index m2 69! S11) R147 7004 asd | 8947 Bist exo | so4| 862| 904") Bs" gear 480" UFO} BOW HBS B74") 8524 766%] | Facial index . | 826 si7| asa | 876) #65 | 707) 91| 777 | anv | 79a) H89| ToL) sve) so) 777 | ei | B26 | 808] 7h4| 799) BOL) O18) S28 | Neal index 04 766 | 782 702 742 765) 748 700) 702 oTH| 145) KT5) ORG 726 | 700| goo} 714) 714) 781] 607) cor | G21) 792 Index of arm wi (92 478 428 154 4 4V8 69) M7 128 | 424) 410) 4a4 | 445 | 490 | aaa | a0o 409 | 465 | avo | 469 | 407 Index of fioger-reach 1024 1050 1101 104% 1044 1096 1002 (04 1050 | LoL [1081 | 101-2 | 101-2 | 107-4 | 1084 |108%8 | 1010 |105°8 | 106% | 1002 | 107-8 | 1074 | Todex of height sitting ey 560 ch) 665) 542| 2a a4 o28 049) 646 | o58| 656 | 513) 665) cow! s22| 67) 518) G26) 547} GOO! 5241) 499 | Jodex of width of shoulders. 214 208 295 214 win 957 | ¥o1 289 400) 20H | 212 | 280] 27 | 208| 251 | 240) 296 | 207) 280) 228 | 8-8) 200) a55 | 234 Slightly deformed. * Deformed 1 Strongly deformed. Head somewhat asymmetrical, Imbecilet * Father of No.11, * Daughter of Nos. 6,17.’ Head flattened bebind, * Mother of No. 11. * Brother of No.2 Brother of No. 1, ON THE NORTH-WESTERN TRIBES OF CANADA. 683 Papers based largely on Investigations carried on for the Commnuttee on the North-Western Tribes of Canada. 1.—Reports I.-XII. of the Committee on the North-Western Tribes of Canada. 2.—Alex. F. Chamberlain. Der Wettlauf. Hine Sage de Kitonaqa. ulm Cr- Quell, Ba. IIT. (1892), 8. 212-214. 3.—Hinige Wurzeln aus der Sprache der Kitonaqa-Indianer von Britisch- Columbien. Verh. d. Berl. Anthrop. Ges. (1893), 8. 419-425. 4.—Notes on the Kootenay Indians. Bd. I. The Name. Amer. Antiquarian, vol. xv. (1893), pp. 292-294. 5.—Notes on the Kootenay Indians, their History, &c. Bd. II. Linguistic Data. Thid., vol. xvi. (1894), pp. 271-274. 6.—Notes on the Kootenay Indians. Bd.III. Mythology and Folk-lore. Zdid., vol. xvii. (1895), pp. 68-72. 7._Sagen vom Ursprung der Fliegen und Moskiten. Am Ur-Quell, Bd. IV. (1893), S. 129-131. Contains abstracts of Kootenay legends. 8.—The Coyote and the Owl (Tales of the Kootenay Indians). Wemoirs of Intern. Congr. of Anthrop.. (1893), Chicago, 1894, pp. 282-284. 9.—A Kootenay Legend: The Coyote and the Mountain-Spirit. Jowrn. Amer. Fothk-lore, vol. vii. (1894), pp. 195, 196. 10.—Words Expressive of Noises in the Kootenay Language. Amer. Anthrop. vol. vii. (1894), pp. 68-70. 11.—New Words in the Kootenay Language. Jbid., pp. 186-192. 12.—Beitrag zur Pflanzenkunde der Naturvélker Amerikas (list of Kootenay Plant-names, with notes on their use). Verh. der Berl. anthrop. Ges. (1895), pp. 551-556. 13.—Alex. F. Chamberlain. Sulle significazioni nella lingua degli indigeni americani detti Kitonaga (Kootenay) dei termini che denotano gli stati e le con- dizioni del corpo e dell’ animo: saggio di psicologia filologica. Arch. per Vv Antropol. (Firenze), vol. xxiii. (1893), pp. 393-399. 14,—Incorporation in the Kootenay Language. Proc. Amer. Ass. Adv. Sci., vol. xliii. (1894), pp. 346-348. 15.—Word-formation in the Kootenay Language. Jbid., vol. xliv. (1895), pp. 259, 260. 16.—Kootenay Indian Personal Names. Jbid., pp. 260, 261. 17.—Franz Boas. Development of the Culture of North-West America. Science, vol. xii. p. 194. 18.—Petroglyph on Vancouver Island. Traditions of the Kootenay. Verhand- lungen der Gesellschaft fiir Anthropologie (Berlin, 1891), S. 158-172. 19.—Vocabularies from the North Pacific Coast. Proc. Amer. Phil. Soc. (1891), pp. 173-208. 20.—Chinook Jargon. Science, vol. xix., No. 474. 21.—Vocabulary of the Kwakiutl Language. Proc. Amer. Phil. Soe. (1892), pp. 34-82. 22.—Classification of Languages of the North Pacific Coast. Memoirs of the International Congress of Anthropology. Chicago, pp. 3389-346. 23.—Bella Coola Texts. Proc. Amer. Phil. Soc. (1895), pp. 31-48. 24.—Indianische Sagen von der nord-pacifischen Kitiste Amerikas (Berlin, Asher & Co., 1895), 8. vi+363. Map. 25.—The Social Organization and Religious Ceremonials of the Kwakiutl Indians. Rep. U.S. Nat. Mus. (1895), pp. 311-736. 26.—Sprachen-Karte von Britisch-Columbien. Petermann’s Mittheilungen (1896), No. 1. Map. 27.—The Decorative Art of the Indians of the North Pacific Coast. Bulletin American Museum of Natural History (New York, 1896), pp. 123-176. 28.—Franz Boas. Die Entwicklung der Geheim-Biinde der Kwakiutl Indianer. Bastian-Festschrift (1896), S. 435-444. 29.—Songs of the Kwakiutl Indians. Internat. Archiv fiir Ethnog., Supplement (1896), pp. 1-9. 30.—Traditions of the Ts’etsa’ut. Journ. Amer. Folk-lore (1896), pp. 257-268 ; and 1897. 684. REPORT—1898. INDEX TO REPORTS, IV.-XII. The references are given to the pages of the separate copies. pages of the Reports are as below :— Separate copies. PAGES iv 123 Vv Hos iif vl 1-163 vii 1-43 viii. Teval é Ix. TEA uh x 1-71 xi 1223 xii fe 6 Adoption among Kootenay, viii. 14. Awiky’énéq: Physical characteristics, xii. table. Beliefs: Bilqula, vii. 15; Kwakiutl, vi. 61, xi. 10; Shuswap, vi. 92; Songish, vi. 25; tribes of Lower Fraser River, ab-Gyl hile Bilqula: Birth, v. 41, vii. 11; current beliefs, vii. 15; death, vii. 13; houses, vii. 4; linguistics, vi. 127; marriage, vii. 12; maturity. v. 42, vii. 12; medi- cine, vii. 17; potlatch, vii. 6; mytho- logy, iv. 8, vii. 6, 13; physical charac- teristics, v. 12, vii. table 3; religion, vii. 14; secret societies, vii. 6 ; shaman- ism, vii. 15; social organisation, vii. 3; tribes, vii. 2; wars, vii. 15. Birth: Bilqula, v. 41, vii. 11; Coast Sal- ish, v. 44; Kwakinutl, v. 42, vi. 58, xi. 5; Nootka, vi. 39; Shuswap, vi. 89; Songish, vi. 20; Tlingit, v. 40; Ts’Ets’- a/ut, x. 45; T’simshian, v. 40. Boas (F.): Report on Indians of British Columbia, iv. 1-10, v. 5-97 and 6 plates, vi. 10-163, vii. 2-43, ix. 1-11, x. 2-71, xn? 123. xu, 117; 27256.;' ‘social organisation of Haida, xii. 21-27. Boas (F.) and L. FARRAND: Physical characteristics of the Tribes of British Columbia, xii. 1-17. British Columbia: Comparative vocabu- lary of languages spoken vi. i140, x. 68; food of Indians, v. 19; government and law v. 34; hunting and fishing, v. 19; implements of Indians, v. 19; mythology, iv. 6; physical characteris- tics of coast tribes, v. 11; potlatch v. 38; senses and mental character of Indians, v. 18; topography of coast, v. 6; tribes, v. 8; wars, v. 39. The corresponding Report. PAGES 1888 233-255 1889 797-893 1890 553-715 1891 407-449 1892 545-615 1894 453463 1895 522-592 1896 569-591 1898 628-688 Canoes, Chilcotin, xii. 20; Kootenay, vili. 22; Songish, vi. 14. Carrier: Physical characteristics, table 8. CHAMBERLAIN (A. F.) on Kootenay, Vill. 5=71. Charms of Kootenay, viii. 25. Chilcotin: L. Farrand, xii. 18; armour, xii. 20; canoes, xii. 20; death, xii. 20; dress, xii. 20; houses, xii. 19: indus- tries, xii. 18; inheritance, xii. 19; lo- cation, xii. 18; marriage, xii. 18; mythology, xii. 21 ; physical character- istics, xii. table 9; shamanism, xii. 19; social organisation, xii. 18; vocabu- lary, xii. 37. Childhood of Kootenay, viii. 13. Children, growth of Indian, xi. 15. Clothing of Ts’Ets’a’ut, x. 39. Coast Salish: Birth, v. 44; death, v. 45; houses, v. 22; marriage, v. 44; religion, v.51; shamanism, v. 59; social organ- isation, v. 32. Colour perception of Kootenay, viii. 11. Columbia River: Physical characteristics of tribes, vii. 24. Comox: Physical characteristics, v. 17, xi. 16. Comparative vocabulary, vi. 140, x. 68. Crania from North Pacific coast, de- formed, vi. 95. Crime among Kootenay, viii. 14. Customs of Sarcees, iv. 12. xii. Death: Bilqula, vii. 13; Chilcotin xii. 20; Coast Salish, v. 45; Héiltsuk-, vi. 58; Kootenay, v. 46, viii. 16; Kwa- kiutl, v. 43, vi. 58, xi. 7; Nisk-a’, x. 52; Nootka, vi. 43; Sarcees, iv. 15; Shus- wap. vi. 91; Songish, vi. 23; tribes of lower I'raser River, ix. 5; Ts’Ets’a’ut, x. 46; Tsimshian, v. 41. - _ ON THE NORTH-WESTERN TRIBES OF CANADA. Deformed crania from North Pacific coast, vi. 95. Dress: Chilcotin, xii. 20; Kootenay, viii. 24, Hthnology, linguistic, Horatio Hale on, viii. 1-5; of British Columbia, Horatio Hale on, v. 1-5, vi. 1-10. FARRAND (L.) and F. Boas, Physical characteristics of tribes of British Columbia, xii. 1-17. FARRAND (L.), Ethnology of Chilcotin, xii, 18-21. Festivals of Nisk’a’, x. 52. Fishing: Kootenay, viii. 20; Songish, vi. Gs ‘tribes of lower Fraser River, ix. 7. Food : Indians of British Columbia, Vv. 19; Kootenay, viii. 27; Shuswap, vi. 85; Songish, vi. 15. Future life among Tlingit, v. 46. Gambling: Sarcees, iv. 14; Songish, vi. 19. Games: Kwakiutl, xi. 10; Nisk-a’, x. 61; Nootka, vi. 38; Shuswap, vi. 89; Ts’Ets’a ut, x. 47. Genealogies of tribes of lower Fraser ’ River, ix. 3, table i. Gitamat : Physical characteristics of, vii. 20. Government and law among Indians of British Columbia, v. 34. Government of Shuswap, vi. 86. Haida: Houses, v. 22; linguistics, v. 71 ; mythology, iv. 7 ; physical characteris- tics, v. 12, 15,vii. 20, xii. 15, 42, table 11; secret societies, v. 58, vil. 48 ; shaman- ism, v. 58; social organisation, iv. 4, v. 23, 26; worship and prayers, iv. 9. HALE (Horatio), Introductory letter, iv. 1-4; ethnology of British Columbia, v. 1-5, vi. 1-10; linguistic ethnology, vili. 1-5; Sarcees, iv. 21-23. Harrison Lake: Physical characteristics of tribes, vii. table 5. Héiltsuk:: Death, vi. 58; physical cha- racteristics, xii. table 11; social organ- isation, iv. 5, v. 23, 29. History of Ts’Ets’a’ut, x. 35. Houses: Bilqula, vii. 4; Chilcotin xii. 19; Coast Salish, v. 22; Haida, v. 22; Kootenay, vill. 22; Kwakiutl, v. 22; Nisk‘a’, xi. 12; Nootka, v. 22; Shus- wap, vi. 80; Songish, vi. 11; Tlingit, v. 22; Ts’Ets’a'ut, x. 40; Tsimshian, V. 22, xi. 12. Hunting ard fishing in n British Columbia, eho Hunting: 685 Kootenay, viii. 19; tribes of lower Fraser River, ix. 7; Ts’mts’a’ut, x. 41. Implements of Indians of British Colum- bia, v. 19. Indian children, growth of, xi. 15. Indian words, transcription of, iv. 4, vi. 10, vii. 2, x. 2, xii. 38. Indians of British Columbia, reports on, iv. 1-10, v. 5-97 and 6 plates, vi. 10- 163, vii. 2-43, viii. 5-71, ix. 1-11, x. 2— 71, xi. 1-23, xii. 1-61. Industries: Chilcotin, xii. 18; Shuswap, vi. 83. Inheritance: Chilcotin, xii. 19 ; Kootenay, viii. 14. Introduction to report of Committee, by Sir Daniel Wilson, vii. 1. Kootenay: Adoption, viii. 14; canoes, viil. 22; charms, viii. 25; childhood, viii. 13; colour perception, viii. 11 ; crime, viii. 14; death, v. 46, viii. 16; dress, vili. 24; fishing, viii. 20; food, viii. 27 ; houses, viii. 22; hunting, viii. 19; linguistics, v. 93, viii. 45; manu- factures, viii. 23; marriage v. 46, 13; maturity, v. 45; medicine, vill. 29; music, viii. 17; mythology, iv. 9, viii. 31; ornaments, vill. 25; painting, viii. 16; physical characteristics, vili. 58; property and inheritance, viii. 14 ; reli- gion, vili. 15 ; report of A. F. Chamber- lain, viii. 5-71; senses and mental character, viii. 8; shamanism, v. 59, viii. 15; sign language, vili. 36; social organisation, iv. 6, viii. 12; tattooing, viii. 16; terms of relationship, viii. 12 ; tribes, viii. 6; worship and prayers, iv. 10, Kwakiutl: Birth, v. 42, vi. 58, xi. 5; cur- rent beliefs, vi. 61, xi. 10; death, v. 43, vi. 58, xi. 7; games, xi. 10; houses, v. 22; linguistics, vi. 103, xi. 17; mar- riage, v. 42; mythology, iv. 7; physi- cal characteristics, v. 12, 15, vii. 21, x. tables 3, 4,5; xii. table 12 ; religion, v- 61, vi. 58; secret societies, v. 52, vi. 62 ; shamanism, vi. 59, xi. 2; social organi- sation, v. 29, 33, vi. 56; tribes, vi. 52; worship and prayers, iv. 9. Kwakiutl type, xii. 16. Languages spoken in British Columbia, comparative vocabulary of, vi. 140. Linguistic stocks, iv. 4. Linguistics: Bilqula, vi. 127; Haida, v.71 ; Kootenay, v. 93, vili. 45; Kwakiutl, vi. 103, xi. 17; Ntlakya’pamuq, xii. 27; 686 Nisk-a’, x. 62, xi. 18; Nootka, vi. 116; Okanagon, vi. 135; Salish languages, vi. 127; Sarcees, iv. 17; Shuswap, vi. 131; Snanaimuq, vi. 128; Stla’tlumH, vi. 133; Tlingit, v. 60; Ts’Ets’4’ut, x. 66; Tsimshian, v. 81. Lku’‘igen. See Songish. Location: Chilcotin, xii. 18; Sarcees, iv. 10; Shuswap, vi. 80; Ts’Ets’a’ut, x. 34. Lower Fraser River: Physical character- istics of tribes, vii. 22; tribes, ix. 1. Lytton, Physical characteristics of Indians of, v. 18. Manufactures: Kootenay, viii. 23; Song- ish, vi. 14. Marriages: Bilqula, vii. 12; Chilcotin, xii. 18; Coast Salish, v.44; Kootenay, y. 46, viii. 13 ; Kwakiutl, v. 42; Nisk:a’, x. 54; Nootka, vi. 42; Sarcees, iv. 14; Shuswap, vi. 90; Songish, vi. 23; tribes of lower Fraser River, ix.4; Ts’Ets’a’ut, x. 45; Tsimshian, v. 40. Maturity: Bilqula, v. 42, vii. 12; Koo- tenay, v. 45; Nootka, vi. 40; Shuswap, vi. 89; Songish, vi. 22; Ts’Ets’a’ut, x. 45; Tsimshian, v. 40. Medicine: Bilqula, vii. 17 ; Kootenay, viii. 29; Songish, vi. 24. Mental character: Indians of British Co- lumbia,‘v. 18; Kootenay, viii. 8. Music: Kootenay, viii. 17; Nisk-a’, x. 50, 51; Nootka, vi. 36-38, 41, 44, 46, 48-50 ; Ts’nts’a’ut, x. 46. Mythology: Bilqula, iv. 8, vii. 6, 13; Chilcotin, xii. 21; Haida, iv. 7; Koo- tenay, iv. 9, viii. 31; Kwakiutl, iv. 7; Nisk:a’, x. 50; Nootka, iv. 8, vi. 43; Ntlakya’pamuq, iv. 8; Salish, iv. 8; Songish, vi. 27; Tlingit, iv.6; tribes of British Columbia,iv. 6; tribes of lower Fraser River, ix. 9; Ts’Ets’a‘ut, x. 47; Tsimshian, iv. 7. Nasal index of skulls, xi. 16. Nicola Valley, Tinneh tribe of, x. 30-34, xii. 18, 38. Nisk-a’: Death, x. 52; festivals, x. 52; games, x. 61; houses, xi. 12; linguis- tics, x. 62, xi. 18; marriage, x. 54; music, x. 50, 51; mythology, x. 50; physical characteristics, x. tables 1, 2; xii. table 11; religion, x. 61; secret socie- ties, x. 54; shamanism, x. 59; social organisation, x. 48; totem poles, x. 52. Nootka: Birth, vi. 39; death, vi. 43; games, vi. 38; houses, v. 22; linguis- tics, vi. 116; marriage, vi. 42; matu- rity, vi. 40; music, vi. 36-38, 41, 44, 46, 48-50; mythology, iv. 8, vi. 43; omens relative to birth of twins, vi. 39; paint- REPORT—1 898. ings, vi. 35, 40; physical characteris- tics, v. 12, 15, vii. 21; potlatch, vi. 36; religion, vi. 43; secret societies, vi. 47 ; shamanism, vi. 44; social organisation, vi. 32; tattooing, vi. 38; tribes, vi. 31. Northern type, xii. 15, 42. North Pacific Coast : Deformed crania, vi. 95; physical characteristics of tribes, vii. 18, x. 3. | Northern Oregon: Physical characteris- tics of tribes, vii. 26. Ntlakya’pamuaq: Linguistics, xii. 27 ; my- thology, iv. 8; physical characteristics, x. tables, 7-11, xii. table 10. Okanagon: Linguistics, vi. 135; physical characteristics, x. table 11. Ornamentation, Ts’Ets’a/ut, x. 43. Ornaments, Kootenay, viii. 25. Painting : Kootenay, viii. 16; Nootka, vi. 35, 40; preliminary notes, iv. 5. Physical characteristics: Bilqula, v. 12, vii. table 3; Chilcotin, xii. table 9; coast tribes of British Columbia, v.11; Comox, v.17; Gitamat, vii. 20; Haida, v.12, 15, vii. 20, xii. table 11; Indians of Lytton, v. 18: Kootenay, viii. 38; Kwakiutl, v. 12, 15, vii. 21, x. tables 3-5; Nisk-a’, x. tables 1, 2; Nootka, v. 12, 15, vii. 21; Ntlakya’pamuq, x. tables 7-11; Okanagon, x. table 11; Oregonian Tinneh, vii. table 9; Sanitch, v. 17; Sarcees, iv. 16; Shuswap, viii. 71. x. table 11; Sishiatl, x. table 5; Songish, v. 17; Ts’Ets’a’ut, x. table 1; Tsim- shian, v. 12, 15, vii. 20. Physical characteristics of tribes: Coast of Washington, vii. table 6; Columbia River, vii. 24; Harrison Lake, vii. table 5; Lower Fraser River, vii. 22, x. table 6; North Pacific coast, vii. 18, x. 3; Northern Oregon, vii. 26; Southern Oregon vii. 28. Potlatch: Bilgula, vii. 6; British Colum- bia, v. 38; Nootka, vi. 36. Preliminary notes on mythology : Bilqula, iv. 8; British Columbia. iv. 6; Haida, iv. 7; Kootenay,iv. 9; Kwakiutl,iv.7 ; Nootka, iv. 8; Ntlakya’qamugqQ, iv. 8; Salish, iv.8; Tlingit, iv. 6; Tsimshian, iv. 7. Preliminary notes on painting, iv. 5. Preliminary notes on social organisation : Haida, iv. 4; Héiltsuk’, iv. 5; Koote- nay, iv. 6; Salish, iv. 5; Tlingit, iv. 5. Preliminary notes on tattooing, iv. 5. Preliminary notes on worship and prayers : Haida, iv. 9; Kootenay, iv. 10; Kwa- kiutl, iv. 9; Salish, iv. 10; Tlingit, iv. 9; Tsimshian, iv. 9. _ Preliminary report by F. Boas, iv. 1-10. Property among Kootenay, viii. 14. =z Relationship: Kootenay, terms of, viii. 12; Salish laneuages, terms of, vi. 136. Religion: Bilqula, vii. 14; Coast Salish, vy. 51; Kootenay, viii. 15; Kwakiutl, v. 51, vi. 58; Nisk:a’, x. 61; Nootka, vi. 43; Shuswap, vi. 93; Songish, vi. 28; tribes of Lower Fraser River, ix. 9; Ts'Ets‘a’ut, x. 46; Tsimshian, v. 49. Reports on Indians of British Columbia, iv. 1-10, v. 5-97 and 6 plates, vi. 10- G3, vil. 224 ores 227 1x 1223," xii. 1-61. y 7 j ; Salish languages: Linguistics, vi. 127; terms of relationship, vi. 156. Salish : Mythology, iv. 8 ; social organisa- tion, iv. 5; worship and prayers, iv. 10. Sanitch : Physical characteristics, v. 17. Sarcees: Customs, iv. 12; death, iv. 15; gambling, iv. 14; linguistics, iv. 17; location, iv. 10; marriage, iv. 14; origin, iv. 11; physical characteristics, iv. 16 ; remarks by Horatio, Hale, iv. 21-23 ; report by EF. Wilson, iv. 10-21; shamanism, iv. 15; traditions, iv. 12. Secret societies : Bilqula, vii. 6 ; Haida, v. 58; Kwakiutl, v 52, vi. 62; Nisk-a’, x. 54; Nootka, vi. 47; Songish, vi. 26; Tsimshian, v. 56. Senses and mental character: Indians of British Columbia, v. 18; Kootenay, viii. 8. Shamanism, Bilqula: vii. 15; Chilcotin, xii. 19; Coast Salish, v.59; Haida, v. 58; Kootenay, v. 59, vili. 15; Kwa- kiutl, vi. 59, xi. 2; Niska’, x. 59; Nootka, vi. 44; Sarcees, iv. 15: Shus- wap, vi. 93; Songish, vi. 28; Tlingit, y. 58: tribes of lower Fraser River, ix. 9; Ts’Ets’a’ut, x. 45; Tsimshian, v. 58. Shuswap: Birth, vi. 89; current beliefs, vi. 92; death, vi. 91; food, vi. 85; games, vi. 89; government, vi. 86; houses, vi. 80, industries, vi, 83; linguistics, vi. 131; location, vi.80; marriage, vi. 90; maturity, vi. 89; physical characteris- ties, viii. 71, x. table 11, xii. table 7; religion, vi. 93; shamanism, vi. 93; . sign language, vi. 87; social organisa- tion, vi. 85; war, 86. Sign language : Kootenay, viii. 36 ; Shus- wap, vi. 87; Songish, vi. 25. Sishiatl, physical characteristics, x. table 5 Skulls, nasal index, xi. 16. i 7 ON THE NORTH-WESTERN TRIBES OF CANADA. 687 Slaves of Chilcotin, xii. 19. Snanaimuq: Linguistics, vi. 128. Social organisation: Bilqula, vii. 3; Chil- cotin, xii.18; Coast Salish, v. 32; Haida, iv. 4, v. 23, 26; Héiltsuk:, iv. 5, v. 23, 29 ; Kootenay, iv. 6, viii. 12 ; Kwakiutl, v. 29, 33, vi. 56; Nisk-a’, x. 48; Nootka, vi. 32; Salish, iv. 5; Shuswap, vi. 85; Songish, vi. 17; Tlingit, iv. 5, v. 23, 25; tribes of lower Fraser River, ix. 3; Ts’Ets’a/ut, x. 44; Tsimshian, v. 23, 24, 27, | Songish: Birth, vi. 20; canoes, vi. 14; current beliefs, vi. 25; death, vi. 23; fishing, vi. 16; food, vi. 15; gambling, vi. 19; houses, vi. 11; manufactures, vi. 14; marriage, vi. 23; maturity, vi. 22; medicine, vi. 24; mythology, vi. 27 ; omens relative to birth of twins, vi. 22; physical characteristics, v. 17; religion, vi. 28; secret societies, vi. 26; shamanism, vi. 28; sign language, vi. 25; social organisation, vi. 17 ; tat- tooing, vi. 22. Southern Oregon: Physical character- istics of tribes, vii. 28. Sti/‘atemag:.Physical characteristics, xii. table 6. Stla'tluma : Linguistics, vi. 133; physical characteristics, xii. tables 1, 2, 3. Stlemqd'lequm@: Physical character- istics, xii. tables 4, 5, 6. Summary of the work of the Committee, xii. 40-56. Tattooing : Kootenay, vili. 16; Nootka, vi. 38; Songish, vi. 22; preliminary notes, iv. 5. TEIT (James): Tinneh of Nicola Valley, x. 31-33 Terms of relationship: Kootenay, viii. 12; Salish languages, vi. 136. Thompson River type, xii. 15, 42. Tinneh of Nicola Valley, x. 30-34 ; James Teit on, x. 31-33. Tinneh, Oregonian: Physical character- istics, vii. table 9. Tlingit: Birth, v. 40; future life, v. 46; houses, v. 22; linguistics, v. 60 ; mytho- logy, iv. 6; shamanism, v. 58; social organisation, iv. 5, v. 23, 25; worship and prayers, iv. 9. Totem poles of Nisk‘a’, x. 52. Traditions of Sarcees, iv. 12. Transcription of Indian words, iv. 4, vi. 10, vii. 2, x. 2, xii. 38. Tribes: Bilqula, vii. 2; coast of Washing- ton, physical characteristics, vii. table 6; Columbia River, physical character- istics, vii. 24; Harrison Lake, physical characteristics, vii. table 5; Kootenay, viii. 6; Kwakiutl, vi. 52; Nootka, vi. 688 REPORT—1898. 31; Northern Oregon, physical cha- v. 49; secret societies, v. 56; shaman- racteristics, vii. 26; Southern Oregon, ism, v. 58; social organisation, v. 23, physical characteristics, vil. 28. 24, 27; worship and prayers, iv. 9. Tribes of Lower Fraser River, ix. 1; cur- | Twins: Omens relative to birth, Nootka. rent beliefs, ix. 11; death, ix. 5; fish- vi. 39; Songish, vi. 22. ; ing, ix. 7; genealogies, ix. table 1; Village of Ts’Bts’a’ut, x. 39. hunting, ix. 7; marriage, ix. 4; my- Vocabulary of Chilcotin, xii. 37. thology, ix. 9; physical characteristics, | —-— comparative, x. 68; languages vii. 22, x. table 6; religion, ix. 9; spoken in British Columbia, vi. 140. shamanism, ix.9; social organisation, | 1b i | Ts'Ets’a/ut : Birth, x. 45; clothing, x. 39; | War of Shuswap, vi. 86. death, x. 46; games, x. 47; history, | Wars: Bilqula, vii. 15 ; Indians of British x. 35: houses, x. 40; hunting, x. 41; Columbia, v. 39. linguistics, x. 66; location, x. 54; | Washington: Physicai characteristics of marriage, x. 45; maturity, x. 45; | tribes of coast, vii. table 6. music, x. 46; mythology, x. 47; orna- | WILSON (E. F.), Report by, on Sarcees, mentation, x. 43; physical character- iv. 10-21. istics, x. table 1; religion, x. 46; WILSON (Sir Daniel), Introduction by, to shamanism, x. 45; social organisation, Report of Committee, vii. 1. x. 44; villages, x.39. | Words in language of Tinneh of Nicola Tsimshian: Birth, v. 40; death, v. 41; Valley, x. 33, xii. 38. houses, v. 22, xi. 12; linguistics, v. 815 | Worship and prayers, Haida, iv. 9; marriage, v. 40; maturity, v. 40; my- Kootenay, iv. 10; Kwakiutl, iv. 9; thology, iv. 7; physical characteristics, Salish, iv. 10; Tlingit, iv. 9; Tsim- vy. )2, 15, vii. 20, xii. table; religion, shian, iv. 9. Torres Straits Anthropological Dxpedition.—Interim Report of the Committee, consisting of Sir W. TURNER (Chairman), Professor A. C. Happon (Secretary), Professor M. Foster, Dr. J. Scorr- Kewtir, Professor L. C. Misti and Professor MARSHALL WARD, appointed to investigate the Anthropology and Natural History of Torres Straits. Tue party, consisting of Drs. Haddon, Rivers, MacDougall, and Myers, and Messrs. Ray and Wilkin, left London in the ‘Duke of Westminster’ on March 10, and arrived at Thursday Island on April 22, where Dr. Seligmann joined the expedition. Dr. Haddon adds :—After various delays, Murray Island was reached on May 6; here we occupied a dis- used Mission House. The whole party stayed in Murray Island for a fortnight, and a number of anthropological and psychological obser- vations were made. As the Rey. J. Chalmers sent the ‘Olive Branch’ to take on those who wished to proceed to Port Moresby, Mr. Ray, Dr. Seligmann, Mr. Wilkin, and myself took this opportunity of crossing to the mainland. Delena was reached on May 27, and Port Moresby on May 31. In the absence of the Governor, Sir William Macgregor, Mr. Musgrave gave us every assistance, and the ‘ Peuleule,’ a small Govern- ment schooner, was put at our disposal for a fortnight. Short visits were paid to Kaile, Kappakappa, &c., and a stay of nearly a fortnight was wade at Hula. The annual dance at the neighbouring village of Babaka was witnessed and photographed. ‘This is evidently a fertility dance for the gardens, and probably also for the girls. It is similar to the famous annual dance at Kalo, which is about three and a half miles distant. At Kerepunu we saw and photographed canoes being hollowed out with stone adzes. We have photographed several processes, such as tattooing, fire making, pile driving, pottery manufacture, &c. After our return to Port ———————————— LL rr Cr ON THE TORRES STRAITS ANTHROPOLOGICAL EXPEDITION. 689 Moresby we made a short excursion to the Astrolabe Range, and measured ‘a few Taburi natives. Some mountaineers who visited Port Moresby were also measured and had their eyesight tested. Dr. Seligmann paid a visit to the Rigo district, and had not returned at the time this was written ; he will remain some time longer in this part of New Guinea. The rest of us left Port Moresby on July 7, and spent a few days in the neighbourhood of Hall Sound and in the Mekeo district. Murray Island was reached on July 20. Drs. Rivers, MacDougall, and Myers have obtained a large number of observations in experimental psychology, which promise to be of great interest. The whole of the party have enjoyed good health so far, no serious case of illness having occurred. Silchester EHacavation.—Report of the Committee, consisting of Mr. A. J. Evans (Chairman), Mr. Jonn L. Myres (Secretary), and Mr. E. W. Brasroox, appointed to co-operate with the Silchester Excavation Fund Committee in their Explorations. THE excavations at Silchester in 1897 were begun on May 3, and continued, with the usual interval during the harvest, until November 4. Theareaselected for excavation included twoinsule(X VII.and XVIII), extending from insula III. (which was excavated in 1891) to the south gate, and lying on the west side of the main street through the city from north to south (v. plan). The area in question contains about five acres. The northern margin of insula XVII. is entirely filled with the foundations of two large houses of the courtyard type, presenting several unusual features. The southern part of the ansula contained the remains of a house of the corridor type of early date, portions of apparently two other houses of the same type, and two detached structures warmed by hypocausts and furnished with external furnaces, perhaps for boilers, of which no examples have hitherto been met with at Silchester. Near one of these was discovered a well containing at the bottom a wooden tub in an exceptional state of preservation. It will be added to the collection in the Reading Museum. Insula XVIII, like XVIL., has the northern fringe entirely covered with the foundations of buildings. These belonged to one house of ‘unusual size and plan, and perhaps two other houses. The remainder of the insu/a is unusually free from buildings, and even rubbish pits. It contains, however, towards the south gate, foundations of an interesting corridor house with an attached inclosure containing six circular rubble bases. It is possible that these are the supports for stone querns, and that the building was actually a flour mill. In a well near this building were discovered two more tubs, which have been successfully raised and preserved. The architectural fragments discovered in 1897 were few in number : among them were a terra-cotta antefix, parts of two inscribed tiles and of a marble mortar, a stone slab with moulded edge, apparently portion of a pedestal or some such object, and two fragments of capitals, evidently from the basilica. The finds in bronze, iron, and bone are of the usual character. Among the bronze articles are two good enamelled brooches, several chains, and a curious socketed object surmounted by the head of an eagle—perhaps to fit on a staff. The finds in bone and glass were unimportant. 1898. Mx 690 REPORT—1898. The pottery includes a number of perfect vessels of different kinds. One of these, a jar of grey ware with painted black bands, is of unusual size, being nearly 2 feet high and 22 inches in diameter. A detailed account of all the discoveries was laid before the Society of Antiquaries on May 26, 1898, and the objects found were exhibited, as in former years, at Burlington House. The annexed plan of the Roman town shows the portions excavated down to May, 1898. Ras wD ww ow ans et a me me me a es) It is proposed during the current year to excavate the two insula south of insule XV. and XVI. (excavated in 1896). With them must also be included the ground to the south of them, a triangular piece almost as large as a third insula. When the examination of this area is completed considerably more than half the city, including the whole of the south-west quarter, will have been systematically excavated and planned. As the insu/e@ and adjoining portions now (1898) under examination cover nearly eight acres, the expenses of the excavations this year will be more than usual. The Committee therefore ask to be reappointed, with a further grant. ——— sl _— ON THE MENTAL AND PHYSICAL DEFECTS OF CHILDREN. OO] r Mental and Physical Deviations from the Normal among Children in Public Elementary and other Schools—Report of the Committee, consisting of Sir Dougtas Gatton (Chairman), Dr. FRancis WARNER (Secretary), Mr. E. W. Brasroox, Dr. J. G. Garson, and Mr. HK, Waite WALLIS. (Report drawn up by the Secretary.) PAGE APPENDIX.—Table showing co-relations of conditions of defect among 1,120 children, subnormal in constitution, mental, or physical 3 2 - 692 In presenting our sixth annual report we give a further account of those children whose mental and physical condition renders them unfitted for the public education provided in ordinary elementary day schools. The facts upon which our research is based are the recorded observations of the 1,120 children who appeared to require special care and training, a catalogue of whom was given in our last report (1897)—viz., 597 boys, 523 girls. Some account of these children is given in the Annual Report (1898) of the Childhood Society, to whom we are indebted for access to the records of those cases. _ It is by studying the co-relations of the cases, and the relative fre- quency with which the main classes of defect are associated in boys and girls, respectively arranged in age-groups, that new information is mostly obtained. This work has proved laborious, and results are given in the table appended. This statement of facts observed may be compared with the results of the examination of 100,000 children seen in ordinary schools.! The facts tabulated show that great difficulties must arise in making any provision for the proper care of these children, who are altogether below the normal or average in bodily and mental power ; they show a much greater tendency than average children to become delicate under an adverse environment, especially the girls ; this, as might be expected, is most marked in those under seven years of age. The main classes of defect are indicated in the table by symbols :— A. Defect in development of body ; B. Abnormal nerve-signs; C. Low nutrition ; D. Mental dulness. The large proportion of both boys and girls who present ‘ abnormal nerve-signs’ or irregularities in movement, balance, and response in action, shows the importance of trying to remove each such sign of brain-dis- orderliness in detail by carefully adapted physical training ; such abnor- mal conditions do not appear to pass off naturally in these children, as is shown by the fact that among cases with developmental defect, they are almost as frequent among the older as the younger children. The remarks made above show that the improvement of the brain con- ' Report on the Scientific Study of the Mental and Physical Conditions of Child- hood, with particular reference to children of defective constitution, and with recommendations as to education and training, based on 100,000 children examined. Published at Parkes Museum, Margaret Street, London, W., the office of the Childhood Society. Wawa 692 REPORT— 1895, dition of children below the average in mental and physical development, requires much labour on the part of skilled teachers, combined with good hygienic surroundings, and that such work must necessarily not be esti- mated by average results. It appears that research, founded on observation, affords results of scientific and social value, while much remains to be done before any method of mental hygiene can be firmly established. The Committee desire to be reappointed, to act. in conjunction with the Childhood Society, for the scientific study of the mental and physical conditions of children ; to assist them in presenting the results of their observations in a duly co-related form they ask a grant of 20/. in aid of their work. Taste based on the observation of 1,120 children who appeared to require special care and training on physical or mental grounds—Boys 597, Girls 523—showing the co-relation or the association of the main classes of defects in this Group. The Table rs arranged in fowr columns, giving the percent- ages for children im the Age-groups and at all ages. The percentages are taken on the number with the main class of defect. Thus: of all cases with developmental defect at all ages 90 per cent. of the boys and 92-3 per cent. of the girls were mentally dull. Of all the dull children at all ages 86°3 per cent. of the boys and 87:5 per cent. of the girls also presented abnormal Nerve- signs. 2 : ac 7 years and Ave 8-10 jAge 11 and All ages under over = B. |G |B. |G. |B. |G. |B |G. All cases with Developmental defect. AB ‘, 91:2 | 89:0 | 92°0 | 90°5 | 83°7 | 85:9 | 89'2 | 889 | Per cent. with Abnormal Nerve-signs. AC 772 | 83°5 | 69°5 | 77°0 | 48°8 | 641 | 65°2 | 7674 55 » Low nutrition. AD 90:3 | 90:4 | 91-4 | 96°0 | 87-8 | 92°3 | 90°0 | 92°3 ‘ » Mental dulness. ABC. 74:5 | 787 | 68:2 | 73°0 | 45°5 | 57:7 | 62°8 | 71°5 s » Nerve-signs and Low nutri- tion. ABD. 85°1 | 86'3 | 87-4 | 88°9 | 77-2 | 82°0 | 835 | 85°8 - » Nerve-signs and Dulness, ACD. T3T | 795 | 67°5 | 76-2 | 47-1 | 615 | 72°8 | 73'8 ES » Low nutrition and Dulness. / ASCD ‘ 72°83 | 774 | 66°9 | 73°0 | 44°6 | 57-7 | 616 | 71:0 x » Low nutrition and Dulness, and Nerve-signs. | No. ofcases—B .| 142 | 153 | 186 | 148 | 141 |115 | 469 | 418 | All cases with Abnormal Nerve-signs. AB : 5 . | 732 | 84°9 | 747 | 77-0 | 73°0 | 582 | 73:7 | 74°8 | Per cent. with Developmental defect. | BC : A . | 640 | 76°5 | 586 | 64:9 | 41°1 | 42°6 | 55°0 | 62°5 as » Low nutrition. BD 3 : - | 88°7 | 93°5 | 8675 | 91°8 | 82°3 | 85:2 | 85°9 | 90:2 3. s» Mental dulness, ABC. ° « |59°S | 751 | 554 | 62°1 | 39°7 | 39-1 | 52-0 | 60°3 + 5, Developmental defect and ee Low nutrition. ABD. . + | 683 | 82°3 | 70°9 | 75°6 | 67:3 | 55°3 | 69°0 | 72:2 is 35 Developmental defect and | Dulness. ISB CID. . « |62°7 | 75°2 | 575 | 67:8 | 39:7 | 40°8 | 53°7 | 617 a 5, Low nutrition and Dulness, {| ABCD A . | 585 | 73°9 | 54:4 | 62°1 | 39-0 | 39°0 | 50°9 | 59:7 = s, Low nutrition and Dulness, | | | and Developmental defect. | No. of cases—C «| 96 | 126 |115 |105 | 63 | 57 | 274 | 288 | All cases with Low nutrition. AC * . | 916 96°83 | 913 | 92-4 95-2 87-7 | 92°3 | 93°3 | Per cent. with Developmental defect. BC i. a - |94°8 | 92°8 | 94°7 | 92-4 | 92-0 | 85°9 | 94-2 | 91°2 ss » Abnormal Nerve-signs. cD : « | 93°7 | 95:2 | 93°9 | 96:2 | 93°6 | 89°5 | 93°8 | 94-4 » 5 Mental dulness. ABC. - | 88°5 | 91°2 | 89°5 | 87°6 | 888 | 79-0 | 89°1 | 87-4 es » Developmental defect and Nerve-signs. 1 Weal o ae . |87°5 |920 | 88-6 | 91-4 | 92°¢ | 842 | 89°0 | 90-2 “A » Developmental defect and Dulness. BCD. 92°7 | 91:2 | 93:0 | 91°4 888 | 82°5 | 92:0 | 89°5 3 » Nerve-signs and Dulness. ABCD. __ .|864 |89°6 | 87:8 | 87-6 a2 | 78:9 | S73 | 86°7 | > 5, Nerve-signs and Dulness, | and Developmental defect, ON THE MENTAL AND PHYSICAL DEFECTS OF CHILDREN. 693 r TABLE—continued. : 7 years and Agel and] gy ance | > under | 48¢ 8-10 over Allages | ae / — — j— — ——_ — Baa |B.) G. LBS |G. | Bs. 1G. | No.ofcases—D . 146 157 I77 | 159 | 144 | 115 | 467 | 431 | All Dull Children. AD é : . | 705 | 84:0 | 77-9 | 76°1 | 74-9 | 62°6 | 74:7 | 75-4, Per cent. with Developmental defect. BD 7 : . 863 | 91°0 | 90°0 | 85°5 | 80°5 | 85:2 | 86°3 | 87°5 s » Abnormal Nerve-signs. Ce Dr . . - | 616 | 76-4 | 61-0 | 63° | 40°9 | 44°3 | 55-0 | 631 o » Low nutrition. ABD. 2 . G64 | 80-2 | 74°5 | 704 | 65-9 | 55°6 | 694 | 70°0 bs » Developmental defect and “ Nerve-signs. ACD. 3 . 57-4 | 73-9 | 57-6 | 60°3 | 40°3 | 41-7 | 52-2 | 60°3 | Per cent. with Developmental defect and Low nutrition. BCD. j . | 60°9 | 73-2 | 60°5 | 60'4 | 388 | 40°8 | 53-9 | 598 | 3 » Nerve-signsand Low nutri- tion. ABCD : . 568 | 719 | 57-0 | 57°8 | 381 | 39:0 | 5171 | 58-0 Fa » Nerve-signs and Low nutri- tion, and Developmental defect, No. of cases—A B. 104 | 130 | 139 | 114 | 103 | 67 |346 | 313 | All children with Developmental defect and | Nerve-sians. ABC. ‘ | 82°7 | 88:5 | 74°1 | 80°7 | 54-3 | 67-1 | 70°5 | 80°5 | Per cent. with Low nutrition. ABD. .__ . | 93:2 | 96-9 | 95:0 | 98-2 | 99:2 | 95:5 | 93°6 | 96:5 . » Dulness. mecD . - | 792 | 86°8 | 72°6 | 80°6 | 53-3 | 6771 | 69:0 | 79°8 ' » Dulness and Low nutrition. No. of cases—A C. | 88 | 122 | 105 | 97 | 60 | 50 | 253 | 269 | All children with Developmental defect and Low nutrition. ABC. . 96°6 | 94:2 | 98:0 | 94:8 | 93-3 | 96°6 | 96-4 | 93°6 | Per cent. with Nerve-signs. ACD. A . | 95°4 | 95°0 | 97-1 | 989 | 966 | 96-0 | 96-4 96°6 9 ss Dulness. ABCD . | 94°2 | 99-5 | 96-1 | 94°7 | 91-6 | 89°9 | 94-4 | 93-0 5s » Dulness and Nerve-signs. No. of cases—A D. 103 | 132 |138 | 121 | 108 | 72 | 349 | 325 | All children with Developmental defect and Duilness. ABD. | 941 | 95-4 | 95°6 | 92°5 | 88:0 | $88 | 92°8 | 92:9 | Per cent. with Nerve-signs. AcD r, 81°5 | 87:8 | 73°9 | 79°3 | 53-7 | 666 | 70:0 | 80°0 = » Low nutrition. ABCD F 80°35 | 85°5 | 73°1 | 76°0 | 50°9 | 62°5 | 68:4 | 77-0 A » Low nutrition and Nerve- signs. No. of cases—BC. 91 | 117 |109 | 97 | 58 | 49 | 258 | 263 | All children with Mere ates and Low nutrition. ABC. ~, . 93°4 | 983 | 945 94:8 | 96°5 | 91'S | 94°5 | 95°8 | Per cent. with Developmental defect. BCD. ._ . | 97:8 | 98:3 | 98-1 | 98:9 | 96:5 | 95-9 | 97°6 | 98-0 55 » Dulness. ABCD ._.. 911 | 965 | 92°5 | 94:7 947 | 91-8 | 926 | 94-9 s » Dulness and Developmental defect, No. of cases—B D. | 126 | 143 | 161 |136 | 116 | 98 403 |377 | All children with Nerve-signs and Dulness. ABD... __ . | 76*9 | 88-1 | 81-9 | 82:3 | 81-9 | 65:3 | 80°4 | 80°1 | Per cent. with Developmental defect. BCD. ._ . {706 | 80-4 | 66:4 |70°5 | 48-2 | 49°9 | 62°5 | 68°5 a y, Low nutrition. ABCD s « | 65°8 | 78:9 | 62-7 | 67-5 | 47-3 | 45°9 | 59°3 | 663 on » Low nutrition and Develop- mental defect. No. of cases—C D. | 90 | 120 | 108 | 101 | 59 | 51 | 257 |272 | All children with Low nutrition and Dulness. Ac e + «+ « | 93°3 | 96°6 | 94°4 | 95-0 | 98:3 | 94:1 | 94:9 | 95°5 | Per cent. with Developmental defect. BC - . | 98°8 | 95°8 | 99:0 | 95°0 | 94-9 | 92°1 | 98°0 | 94:8 fa » Nerve-signs. AB G hd wd - | 92°2 | 94-1 | 93°5 | 91-0 | 93-1 | 88-1 | 93°0 | 91-9 *p » Nerve-signs and Develop- mental defect. No. of cases—A BC) 85 | 115 |103 | 92 | 56 | 45 | 244 |252 | All children with Developmental defect, Nerve-signs, and Low nutrition. ABCD . . | 97°6 | 98:2 | 99:0 | 99-9 | 98:1 | 99-9 | 98-0 | 99-0 | Per cent. with Dulness. No. of cases—A B D| 97 | 126 | 132 | 112 | 95 | 64 | 324 |302 | All children with Developmental defect, Nerve-signs, and Dulness. ABCD . - |85°5 | 89°S | 76°5 | 82°0 | 57-8 | 70°3 | 73°7 | 82°7 | Per cent. with Low nutrition, | No. of cases—A C D 24¢ | 260 | 102 | 96 | 58 | 48 |244 |260 | All children with Developmental defect, Low } nutrition, and Dulness. ABCD A .-| 98°7 | 973 | 98:9 | 95:7 | 94-7 | 93°7 | 97-9 | 96°0 | Per cent. with Nerve-signs. No. of cases—B C D! 252 | 258 | 107 | 96 | 56 | 47 |252 |258 | All children with Nerve-signs Low nutri- 4 tion, and Dulness. SaABCD . « | 93:2 | 98:0 | 93:4 | 95°7 | 981 | 95°5 | 947 | 96°8 | Per cent. with Developmental defect. 694 REPORT—1898. The Lake Village at Glustonbury.—Third Report of the Committee, con- sisting of Dr. R. Munro (Chairman), Professor W. Boyp DawkIns, Sir Jonn Evans, General Pirt-Rivers, Mr. A. J. Evans, and Mr. A. BULLEID (Secretary). (Drawn up by the Secretary.) Since presenting the last Report much progress has been made with the exploration of the Lake or Marsh Village near Glastonbury. Twelve more dwelling mounds have been examined, as well as the ground between and around them. The southern end of the settlement has been compietely explored, and the investigations have yielded much of importance. The timber substructure in this locality was in a better state of preservation and more massively made than in any part of the village hitherto examined, the arrangement of the logs being exceptionally clear. Some of the dwelling mounds were of more than ordinary interest in their construction, and from the various objects found on and around the floors, and the following observations in connection with them may be specially noticed. Mounds A, B, C,and D formed an interesting group, showing the gradual growth of the village and the construction of dwellings from time to time as they were required ; this was easily recognised in these mounds by the floor of one mound overlapping the floor of the mound immediately con- tiguous to it. The clay of mound A overlapped that of C, B and C that of D. Mound A was the latest construction, D the earliest, B and C were of intermediate date, and the dwellings may have been of contemporary erection. Mounds A, B, and C were of medium size ; the foundation of wood was strong and well arranged, especially under mound C. Mound D was remarkable for its series of baked clay hearths, and for a circular basin-shaped depression in the floor of the dwelling within a foot or two of one of the uppermost hearths. The sides and base were hard-baked, and it appeared to have had asemicircular moulded rim raised two or three inches above the level of the floor ; it measured two feet across the rim, was nine inches deep, and the sides were nearly straight, sloping downwards and inwards towards the base, which was about twenty-one inches in diameter. It contained fragments of the fallen sides and a little fire ash and charcoal. A somewhat similar depression was discovered in mound J and was described in the last Report. Dwelling mound D was also note- worthy for the number of bone needles, broken and complete, found with numerous splinters and sharp fragments of bone near them. Mound E was of large size, oval in shape, and composed of five layers of clay; it contained two hearths of stone and several of baked clay. In this dwelling mound there were found the remains of what may have formed a small furnace of baked clay, fragments of several three-cornered crucibles, and some small pieces of bronze. Mound F was small and had not the appear- ance of a dwelling mound. It contained three remarkable groups of clay hearths, each group consisting of three superimposed hearths. Associated with this mound were quantities of pottery and fire ash. Mound A A: the chief feature in this dwelling mound was the thick- ness of its clay floor, the vertical measurement of its thickest part being 10 feet ; the mound was fairly symmetrical in outline and was about 30 feet in diameter. Beneath the lowest part of the clay, and lying in a layer of brushwood and rushes, part of the framework ostensibly of a loom was discovered ; judging from its position, and from the worm-eaten condition of the wood, it had evidently been discarded and thrown away ON THE LAKE VILLAGE AT GLASTONBURY. 695 before the first dwelling belonging to this mound was erected. Amongst the timber used in the foundation of the mound were many piles and pieces of wood quite disconnected from the purposes originally intended, and evidently belonging to a previous arrangement at another part of the village. With reference to the smaller objects, these compare favourably in number with former seasons, especially with regard to pottery, bronze, iron, horn, and glass. Among the finds are the following :— Stone.—One small celt, fifteen quern stones of various sizes, shapes, and completeness. Bronze.—Thirty ; including spiral rings, fibulz and penannular brooches, pieces of tub bands, fragments of bordering, rivet-heads and studs. Jron.—Fifteen ; three more or less complete adzes, two billhooks, part of a reaping-hook, one file, and several rings. Lead.—Two spindle whorls. Glass.—Several blue beads. Worked Bone.—Fifty-five pieces ; including gouges, needles of various sizes, polishing bones, and other implements. Horn.—F¥itty ; amongst which are several hammer heads, combs, cheek pieces, a knife handle, and a die. Whorls, loomweights, sling-stones, and pottery were dug up as formerly in quantities. ° The following is a summary of the more important finds during the past seven years :— Stone.—One complete celt, and the half of a second, One flint saw. One flint arrow-head. Thirty quern stones more or less complete. One hundred and fifty whetstones and hammerstones. Bronze.—One hundred and sixty-five pieces. Iron.—Eighty. Lead.—Thitty. Amber.—Two complete beads. Jet.—One ring. Glass.—Highteen rings, beads, and pieces. Crucibles.—Fragments of about twenty. Worked Bone.—Three hundred and twenty, besides numerous pieces showing knife marks. Horn.—Two hundred and fifty-five. Kimmeridge Shale.—Kighteen, including rings and portions of armlets. Baked Clay other than Pottery.—Many triangular perforated blocks and weights of other shapes, wattle, timber, and finger-marked clay, Sling pellets of baked and unbaked clay, several thousand. Spindle whorls, one hundred and thirty-five. Perforated tusks and teeth, seven. Human Bones.—Portions of about twenty-five bodies, including four complete skulls. Pottery and bones of animals, several cart-loads. Worked Wood.—Portions of tubs, cups, and ladles ; handles, wheel spokes, parts of the framework of one or more looms, and a complete ladder seven feet high. 696 REPORT—1898., An Ethnological Survey of Canada.—Second Report cf the Committee, consisting of Dr. G. M. Dawson (Chairman and Secretary), Pro- fessor D, P. PENHALLOw (Vice-Chairman), Mr. E. W. Brasroox, Professor A. C. Happon, Mr. E. S. Harruanp, Sir Jonn G- Bovurrot, Abbé Cuoa, Mr. B. Sutte, Abbé Tancuay, Mr. C. Hiuu-Tout, Mr. Davin Boye, Rev. Dr. Scappina, Rey. Dr. J. Macuigean, Dr. Merée BeavucHemin, Rev. Dr. G. Patrerson. Mr. C. N. Bett, Hon. G. W. Ross, Professor J. Mavor, and Mr. A. F. HUNTER. APPENDIX PAGE. I. Haida Stories and Beliefs. By C.Hinu-Tout . , : , B 700 Il. Customs and Habits of Earliest Settlers ef Canada. By BENJAMIN SULTE 709 AT a meeting of the Committee held on August 20 last in Toronto the resignation of the Chairman from that office was accepted, and Pro- fessor Penhallow was nominated as Chairman ; but through a misunder- standing this proposal was not brought before the General Committee. Professor Penhailow has since consented to act as Vice-Chairman. Since the presentation of the first report of this Committee at the Toronto meeting some progress has been made in the further organisation of the work, and some results of interest have been obtained ; but the: field of work in Canada is so vast and so varied that it has thus far been found possible only to attack limited problems where special opportunities have occurred of enlisting competent observers. As pointed out in con- nection with the first report, the investigation presents two main branches = (1) That dealing with the white races, and (2) that dealing with the aborigines or Indians. These, however, are not entirely distinct, for a particularly interesting line of inquiry is that relating to the Métis or ‘ half-breeds,’ resulting from the intermixture of the whites and Indians. Nothing has yet been accomplished in the last-named field of work, but it is anticipated that some observers may soon be enlisted for it. The efforts of the Committee were to some extent handicapped in the first year of its existence by the want of any fund to be employed in the furtherance of its work ; but with the grant made by the Association at its last meeting the definite organisation of this work became possible. As a preliminary the Committee issued a general circular, together with Schedules relating to physical types. Copies of these have been distributed to each member of the Commit- tee, while large numbers of Schedule B, with proportionate numbers of Schedule A, have been placed in the hands of those who are undertaking special work. So far the Committee has distributed about 700 copies of these papers. The Schedules are, with slight modifications, the same as those issued by the Committee for Great Britain, and have been adopted tentatively until their actual use should indicate the special directions im which changes are required. It was found almost immediately that several alterations will be required in the future, the number of facial types in particular being quite inadequate to the requirements of such studies on this continent. Three sets of anthropometric instruments have been purchased. These have been distributed to Mr. Charles Hill-Tout, of Vancouver, who has ON THE ETHNOLOGICAL SURVEY OF CANADA. 697 already accomplished much good work among the coast tribes of Indians, and who proposes to continue his studies during the present summer ; to Mr. A. F. Hunter, of Barrie, Ontario, who has associated with him Dr. F. Tracey, of Toronto, and to Dr. A. C. Hebbert, of Montreal, who proposes. to make liberal use of the material to be found in the various military organisations of the city, public institutions, and also, probably, the students of the universities. The Committee has also purchased a camera specially adapted to its work in the field. This has been placed in the hands of Mr. Hill-Tout, who hopes to secure a large number of negatives during the present summer. ‘These negatives remain the property of the Committee. Communication with the Committee appointed by the American Association for the Advancement of Science for an Ethnographic Survey of the United States has been opened through its chairman, Dr. Franz Boas, and it is hoped that such co-operation may be secured as will lead to results of mutual advantage. In pursuance of a resolution of the Committee at the meeting of August 20 in Toronto, communications were opened with the several provincial governments of Canada for the purpose of obtaining, if possible, grants in aid of photographic and other registration involved in the work of the Committee. Nothing has, however, so far resulted from the com- munications referred to in the way of material aid, although some of the replies received indicate the possibility that such aid may be forthcoming in the future. Mr. David Boyle, having been commissioned by the Government of Ontario to obtain photographs of some of the Indians of the province in connection with his investigations of Iroquois religious rites, has, however expressed his intention of conducting this work as far as possible in con- formity with the requirements of the Committee’s schedule. At the meeting above referred to a resolution was also passed concern- ing the desirability of taking steps for the preservation of the Serpent Mound in Otonabee township, Ontario ; and in October last letters were addressed on the subject to the clerk of the township and to the clerk of Peterborough County Council. At a later date the former replied that his Council considered the work of preserving the mound a provincial one, while the latter stated that the County Council had sent a memorial to the Ontario Government on the subject. Further representations have since been made to the Government, and it is probable that the mound may be acquired next year. Proceeding upon the lines of investigation adopted by Mr. B. Sulte in regard to the province of Quebec, a preliminary account of which was appended to the last report, a similar inquiry has been undertaken by Mr. A. F. Hunter in regard to the composition of the population of the several counties of the province of Ontario. This is not as yet sufficiently complete for publication, but some idea of its character, and the great interest likely to attach to such a record of the foundation of the people of this province, consisting of the most varied elements, may be gathered from the subjoined preliminary analyses referring to two counties only out of the forty-two for which partial information has already been obtained. These are quoted with Mr. Hunter’s permission, and with the object, largely, of inducing a similar analysis of the equally interesting elements brought together in the peopling of New Brunswick, Nova Scotia, and Prince Edward Island. 698 REPORT—1898. Simeoe Co. ‘= Se a “ = No. Immigrants Date Townships where settled 1 i aceadehare Scots 5 ; . | 1820 | West Gwillimbury. 2 | North of England (small) . . | 1820 | Penetang Road, W. Gwillimbury. 3 | French Canadians ; : . | 1828 | Tiny. 4 | Negroes (now chiefly gone) . . | 1828 | Oro (20 families), Sunnidale. 5 | Ulster Protestants (extensive) . | 1830 | Tecumseth, Essa, Innisfil. 6 | Irish Catholic (smaller) ; . | 1830 | Adjala, Vespra, Flos, and Medonte 7 | Argyleshire Scots . 1832 | Nottawasaga, Oro. | 8 | Lanarkshire and Renfrewshire 1832 | Innisfil, Essa. | Scots | 9 | Germans (small) . ? ; . | 1832 | Nottawasaga. 10 | Londonderry 4 . | 1850 | Innisfil. 11 | Border District Scots (small) . | 1850 | Innisfil. i2 | Indians (Chippewas) (population, | — | Beausoleil and Christian Islands. | | York Co. | No. Immigrants Date | Townships where settled 55s “ a | 1 | Germans (Berczy’s 60 families) . | 1794 | Markham. | 2 | French Royalists (20 families) .| 1798 | Yonge St. (King and Whitchurch).) | 3 | Davidites (?) (from New York) . | 1800 | East Gwillimbury. | 4 | Eskdale (Dumfriesshire Scots) . | 1800 | Scarboro. | 5 | Quakers (from Pennsylvania) . | 1805 | King and Whitchurch. 6 | English (West of England) . . | 1820 | Richmond Hill (Vaughan and Markham). — | Pennsylvania Dutch . : .| — | York and Vaughan. — | Mennonists or Tunkers s .| — | Yonge St. (Whitchurch). — | Highland Scots . — | Vaughan, King. — | Annandale (Dumfriesshire) Scots — | Vaughan. — | Negroes : — | Vaughan and King. —- | Indians (Chippewas) (population, — | Georgina and Snake Islands, 118 In British Columbia the immigrant population is so newly established, and has occurred so largely by individual accretions from sources already most heterogeneous in character, that it seems scarcely possible to pursue with profit a similar method of study. The native races, however, there afford, whether from an ethnological or an archzeological point of view, a field of inquiry still wide, although daily narrowing and requiring prompt and efficient action if much is to be placed on record for posterity. Mr. ©. Hill-Tout has been able to accomplish some work in this province, in the record of such facts as have come to his notice, and these are presented in Appendix I. of this report. Mr. Hill-Tout writes as follows :— ‘IT send in some notes on the folklore of this district, which l have sought to record whenever possible on the lines suggested by the English Committee, and trust they will be found useful. I also enclose set of (3) photographs in duplicate of a rock-painting found on a cliff about twenty miles from Vancouver. The Indians of the neighbourhood know nothing of it or of its meaning. I venture no opinion upon it myself. In my next report I hope to have more to communicate. I have in hand the following :— Ss ON THE ETHNOLOGICAL SURVEY OF CANADA. 699 ‘1, Report on the Archeology of Lytton and its neighbourhood. ‘2. Folklore stories from same area. ‘3. Vocabulary and Grammar notes on the Ntlakapamuq. ‘4, Vocabulary and Grammar notes on the Squamish and Matsqui Yale, and other divisions of the Salish. ‘5, Ancient tribal divisions and place-names. ‘6. An account of a great confederacy of tribes in the Salish region of “ Chilliwack.” ‘I regard the collection of vocabularies and grammar notes from every dialect and sub-dialect as imperatively necessary for linguistic comparison The lack of these has caused me the loss of much valuable time and retarded my own labours in this field. The work on these lines already done, though excellent on the whole as far as it goes, is altogether too limited and inadequate. If we are ever to be in a position to formulate a law of permutation of letters for the languages of this region it is absolutely necessary that specimens of dialectal difference from every division of a stock be collected. It is not a simple undertaking, and will require considerable time to accomplish, but its importance cannot be over-estimated. ‘In this connection it gives me pleasure to inform the Committee that several of the leading anthropologists of Australasia have accepted the evidence of Oceanic affinities of the Kwakiutl-Nootka and Salish stocks as set forth by me in a paper presented at the recent meeting of the Royal Society of Canada. Dr. Carroll, the editor of the ‘‘ Australasian Anthropological Journal,” in particular regards the evidence as practically conclusive. ‘The photographic and anthropometric work of the Survey I hope to begin next month, the camera and instruments for which have just come to hand. ‘In concluding this report I desire to call the attention of the Committee to the fact that much important archeological work is awaiting development here for lack of funds to carry it on; the necessity for energrtically prosecuting which, without further delay if it is to be done at all, I cannot impress too strongly upon all who are interested in this work of the Survey. Every month sees valuable records defaced and obliterated, either by relic hunters or by the progress of civilisation, and the day is not far distant when all trace of the past life and conditions of the aborigines such as are contained in the middens and mounds will be entirely swept away.’ Pending a more complete analysis of the early immigrants from France to Quebec, which it is hoped may take eventually a tabular and numerical form, Mr. B. Sulte has extended the inquiry communicated to your Committee last year by following up the indications of the habits and mode of life of the early colonists by means of such contemporary records as stili exist. It is not too much to hope that eventually we may possess a very complete picture of this unique occupation of a part of the North American continent from Old France, and of the formative stages of a new French-speaking people, in all its aspects. The paper forms Appendix IT. of this report. In conclusion the Committee has to report that of the grant entrusted to it at the Toronto meeting a balance of 35/. 17s. remains. The Com- mittee asks to be reappointed and to be permitted to expend the above- 700 REPORT-—1898,. mentioned amount ; also that a further grant of 50/. may be accorded to it in aid of its investigations, which promise to be of increased importance and value during the ensuing year. APPENDIX IT. Haida Stories and Beliefs. By C. H1tu-Tour. Cosmogonical Myth and Story of the Origin of the Haida People. In the remote past Sha-ldnd ruled in his kingdom in the grey clouds that overshadowed the vast deep. All below was a dark and watery waste. At this time Yet/th, the Raven, was the chief servant of Sha-lana. One day Yetlth ventured to interfere with the conduct of affairs in Cloudland, and was cast forth into the outer world. The Raven flew back and fore over the deep until he became weary. He grew angry at finding no place where he could rest, and beat the water with his wings till it flew up into the clouds on either side of him ; and when it fell back again it was transformed into rocks, upon which he rested himself. These rocks grew and extended themselves on every side until they reached from North Island to Cape St. James. Later these rocks became changed into sand, upon which a few trees eventually sprang up and grew, and thus were the Queen Charlotte Islands brought into existence. The Raven now desired someone to assist him in his kingdom, so one day he piled up on the beach two large heaps of clam-shells near by the present site of Sisk, and then transformed them into human beings, whom he made his slaves. They were both of the same sex and female. Ina short time these two slaves became dissatisfied with their condition, and complained to their creator, the Raven, that he had mismanaged affairs in making them both of the same sex. The Raven listened in anger to their complaints, but finally altered their condition notwithstanding, and changed one of them into a man, by casting limpet-shells at her. Thus were the progenitors of the Haidas created. The Raven, growing weary of his lonely life, took the woman for his wife, but as she bore him no children he wearied of her and sent her and the man to a spot now called Skidegate. Wearying of his loneliness once more, he determined to revisit his former home in Cloud- land and secure, if possible, a beautiful wife from among the daughters of the heavenly chiefs. One bright summer morning he started off on his long journey. He soared upward over the lonely sea until the land he had created appeared to him to be a small mosquito. At last he came to the walls of heaven. He concealed himself until the evening, and then, assuming the form of a bear, scratched a hole in the wall, and thus made his entrance into his former home. The place had greatly changed since he had been an inhabitant there, and consequently he took time to con- sider everything that he saw, so as to forma similar kingdom on his return to earth. There he found that everyone was considered a god or chief, and all were submissive to the Chief of Light, who still held supreme power as of old. He also found that the Great Chief had divided his kingdom into villages and towns, into lands and seas, and had created a moon and stars, and made a great luminary to rule over all, which was called Jine the Sun. At last he was caught by the hunters of the King and brought into his presence. As the Raven appeared to be a ————eE CC ~—“—SSC*‘(S;«S ON THE ETHNOLOGICAL SURVEY OF CANADA. 701 heautiful and tame bear, he was kept as a playmate for the King’s youngest son. He now spent three years in intimate relationship with the royal family, and had sutticient time to make careful and necessary observation prior to his descent to the lower world. It was customary for the children in the Land of Light to disguise and transform themselves into bears, seals, and birds. Now it so happened that the Raven, under his disguise of bear, was strolling on the beach one evening, looking for his supper of clams, when he espied three other bears approaching him. He knew at once they were children of a great chief, and, instantly transform- ing himself into a large eagle, stole the sun, which happened to be setting at the time, also the fire-stick that was used to kindle the fires, and flew over the walls of heaven with one under each wing, together with one of the three children. When the people found that the sun had been stolen, they reported the matter at once to the King. He then ordered his land to be searched, and if they found the thief to throw him down to Het-gwau- lana, the chief or ruler of the lower regions. But a messenger arriving, who stated that he had seen a large bird flying over the walls of their city with the sun under his wing, at once all gave chase, and the Raven was followed. In his flight from his pursuers he dropped the child, who fell down through the clouds into the sea close to the Raven’s kingdom. The Raven also descended, bearing with him the sun and the fire-stick in safety to the earth. When the child fell into the sea he cried aloud for assistance, and immediately the little fishes came in a great shoal to his aid and carried him on their backs safely to the shore. These fish are very numerous around Rose-spit at the present day, and their forms, say the Haida, have remained dinted in the blue clay of that district from the day when they bore the heaven-born child ashore until now. The great chief was a lover of peace, and consequently did not allow his followers to pursue the Raven down to the earth, as Chief Het-gwau-lana might then be tempted to enter heaven and give them perpetual trouble. So the Raven was unmolested, and another sun was created in heaven by the Great Ruler, who loved light and hated darkness, Now the Raven thought that he had secured a chief’s daughter, but the child turned out to be a chief's son. The Raven loved him exceed- ingly, and built a house at Rose-spit especially for the accommodation of the child and the sun. The child grew to be very powerful, and had _ command over all animals, fish, and birds. Whenever he called to the fish they would at once appear and bear him out to sea. Whenever he wished to fly through the air he would call to the birds. They would at once come to bear him wherever he wished to go on their wings. The bears and other animals attended to his daily wants, and supplied him with salmon and berries. The animals, birds, and fish were created by the Raven for the sole benefit of this heaven-born child. The Raven also kept the sun and fre-stick in a very strong and secure room, as he was afraid that his two former slaves would return and steal them. Presently the slave-wife of the Raven returned, and begged to be re-admitted into the Raven’s society. The request was granted, and she became once more the mistress of the Raven’s household. She took a great interest in the child, and attended to his every wish. In course of time the child grew to be a handsome young man, and began to love the woman. She returned his love, and at last resolved to become his wife. The Raven seon found that they were living as man and wife, and he became very angry, and threatened to kill the woman. This treatment caused the 702 REPORT—1898., pair to escape from the house and hide themselves in the bush. When they fled from the Raven’s house they carried with them a large cedar box, in which the sun and the fire-stick were placed. Day after day, and month after month, they wandered southward without proper nourish- ment, and in great fear of the Raven. They also carried with them the box containing the sun and the fire-stick. One evening, faint and weary, they sat down near a little creek, and the woman, being very hungry, wept bitterly. Her husband walked a little distance up the stream, and at last found a dead land otter, but they could not eat it, as they had no fire with which to cook it. On the following morning they remembered that they had the fire-stick in the box they were carrying. They at once determined to see if they could produce a fire with it. They were successful, and soon had a good fire, with which they cooked the otter. Having made a hearty meal, they proceeded on their way. When they reached Cape Ball they were hungry again, whereupon the youth began to sing one of the songs taught him in heaven, and the sea receded four miles from the shore, leaving a great whale stranded on the beach. The youth surrounded the whale with a circle of stones and rocks so that it should not escape. This circle of boulders is said to exist to-day. The runaway couple lived on whale flesh until they reached the channel which divides Graham and Moresby Islands, where they settled and built a house. On this spot the village of Skidegate afterwards sprang up. Here they lived for several years in peace and prosperity, and a daughter was born to them, which caused them great joy. In course of time the daughter grew to womanhood, and was an exceedingly beautiful woman, and they would have all been perfectly happy but taat there was no prospect of a husband for the maiden. Year after year passed by, and they had given up all hopes of a husband for their daughter, when one day there came from the North Island, around the west coast, the Raven’s male-slave, whom he had made on the beach at Sisk. This forlorn creature now desired the parents to give him their daughter to wife. The father indignantly refused his request, and became very angry at what he considered a great piece of impudence on the part of a clam-shell-made man. How could such a being as he look to wed with the daughter of a heaven-born chief ! But the slave was not to be so easily repulsed. He betook himself to the woods surrounding the house, and whenever the father was away would go and talk with the mother. She regarded him as her brother, seeing that they had been created together, and told him all her secrets, and even went so far as to tell him where her husband kept the chest con- taining the sun which he had stolen from the Raven’s house at Rose-spit. This treasure was stored away in a strongly built house in the woods, where the heaven-born man would frequently go to pray to the gods in the Kingdom of Light. The woman was not wise in thus divulging the whereabouts of her husband’s precious treasure; for the slave, on asking a second time for the maiden, and receiving a good kicking from her father,! went away in great wrath, vowing that he would be revenged. As soon as night fell, having watched the chief retire to rest, he betook 1 It is interesting to note in this connection that the heaven-born man thought ncthing of taking the slave for his wife, but was much incensed at the idea of his daughter becoming the wife of a slave. We see that the same notions pre- vailed among the Haidas generally, for although a chief could marry any of his female slaves, no slave could marry a free-born woman under pain of death. - Pe. ON THE ETHNOLOGICAL SURVEY OF CANADA. 705 himself to the treasure-house, and easily entered it through the smoke- hole. He then seized a club that he found on the floor, and smashed the box to pieces, taking care not to injure the sun. When he had wrought this havoc he began to ponder upon his miserable lot in life, and presently, becoming enraged at his ill-fortune, threw down the sun and kicked it to pieces. But the broken parts, instead of falling to the ground, leaped up into the sky, the largest piece becoming a sun, the next biggest a moon, and the other pieces stars. Thus were created the Haida sun and moon and stars, according to the traditions of the ancients. When the wretched slave became calm once more he speedily realised the danger he now stood in at the hands of the heaven-born man. So before dawn of the following morning he was well on his way to his former abode at North Island. He travelled only by night, hiding himself in the forest during the day, thus avoiding the keen eyes of the Raven and a meeting with his sister's husband. At last he reached home, and for days he sat brooding over his cruel lot until the happy thought struck him that he should do as the Raven had done and go and seek a wife for himself from among the daughters of heaven. But the difficulty was how to get there. This he overcame in the following manner. Taking his bow and arrows in his hand one moonlight night he shot an arrow at the moon, which embedded itself in that luminary’s face ; he then shot another into the notch of the first and another into the notch of this again, and so on until he had a line of arrows reaching from the moon to the earth. But all this was not accomplished in one night. According to one tradition he took 364 nights over his task, which later were lengthened into 364 days and nights, which number just makes up the Haida year of 13 months of 28 days each. They account for the discrepancy between their year of 364 days and ours of 365 by saying that the slave occupied one day in climbing the arrow ladder, which has been left out of their reckoning. When the slave had completed the ladder he lost no time in climbing up it into heaven. He arrived there early in the morning, and the first thing that he saw was a beautiful woman swimming in a lake of crystal. He stealthily approached the side where she seemed likely to step ashore after her swim to await her. She presently swam in his direction, and no sooner had she put her foot upon the beach than he seized and dropped with her through the clouds into the sea close by the shore of North Island. As they descended the Raven happened to be flying near the spot, and perceiving something unusual in the air above him watched to see what it was. At first he thought it to be a pair of large eagles, but presently discovered it to be his slave and a beautiful heaven-born woman. No sooner had the slave led his prize into the house than the Raven appeared and demanded that the woman should be given over to him. The slave declining to comply with the request, the Raven became angry, seized the woman, and transformed the man into an invisible spirit and drove him away from his presence for ever. Furthermore, he cursed him and bade him wander over the land and take upon himself the task of caring for the growth and development of every living thing the Raven had created. Thus the Wanderer, as the slave is now termed by the Haidas, is always busily engaged causing the berries and roots to grow for the support of the people. Every plant, flower, and tree is under his control, and thus it is that Haida-land produces the finest trees for canoes through- out the whole northern region. At the present time the Haidas 704 REPORT—1898. believe that he is fulfilling his destiny, and they think of him with gratitude and offer him sacrifices of berries, roots, salmon, and bear-grease. These they place in hollow trees that he may eat when he feels hungry. They believe that he wanders upon the earth night and day, and will continue to do so until the end of time, when the Raven will recall him. But woe to the Haidas when this takes place ; for the trees and plants, the fish and animals, the fowls of the air, and even the very land itself will pass away and cease to be, and then will their own end come. Haida Moon Stories. In early times the Haida moon met with several misadventures, but as every tribe had a tribal moon of its own the consequences were not so serious as they wouid otherwise have been. When the Raven was in the ‘Land of Light’ he saw that each tribe there had a separate moon, and he adopted the same plan for the Haidas. The principal moon of the race is that derived from the large splinter kicked off the sun by the ‘clam-shell’ man in his anger at being refused the hand of the heaven- born man’s daughter for wife, as related in the cosmogonical lore of the Haidas. The beaver once ate up the moon of the Masset tribe, and the Raven had to supply another. The sun once chased the moon up the Naas River into the interior of the mainland, where she could find no food. About spring-time, being desperately hungry, she demanded food from her worshippers, who produced the ‘candle-fish,’ or wlakan, which were made to run up the river in great numbers for the purpose. To offset this the sun’s worshippers produced the salmon to eat up the ulakans, and it was only at the intervention of the ‘ Wanderer,’ who fought the salmon, that the little fish were rescued. The moon is not to be insulted with impunity. Once a naughty boy was sent to gather sticks for the fire, but did not want to go, urging that it was dark. His father made him go, telling him that the moon would presently rise and there would be plenty of light. The lad went and stood on the seashore to wait for the moon to rise. As it appeared above the horizon he mocked it by putting his fingers to his nose. Presently a giant came down from the moon and snatched up the boy, and he may now be seen on clear nights in the moon with a bundle of sticks over his shoulder. Nilakapamug Moon Story.—With the above may be compared the belief of the Thompson Indians. Once there was an old woman who was very meddlesome and interfer- ing. She was perpetually making mischief in the village. The people endured her as long as they could, but at last determined they could stand her no longer. They agreed to seek a new settlement and leave her behind. So each family got out their canoes, and loaded them with all their belongings and paddled away. As each left, the old woman begged to be taken on board, but was told that the canoe was too full already, that the next boat would be best for her. They all made the same excuse, and presently the last canoe passed her and she was left behind. As she sat bewailing her lot the moon rose, and she called to it to have compassion on her. The moon came down almost to the ground to see what the old woman was wailing about, and she, seizing the opportunity, leaped up into it and was carried up into the sky. In her hand as she leaped she held a little birch-bark bucket, and on clear nights she can still be seen in the moon with her little bucket in her hand. ON THE ETHNOLOGICAL SURVEY OF CANADA. 705 Haida Beliefs, dc, Frog.— Among the Haidas the frog is regarded as the embodiment of wisdom, whence the medicine-man obtains gifts from his favourite spirits. Marriage Customs.—When a man fancied a girl for his wife he went to her uncle, the brother of her mother (who alone has any voice in the matter), and make overtures to him by means of presents. The uncle being willing, the man then makes known his wishes to the young woman. She thereupon procures the assistance of her companions and prepares for the ceremony. When she is ready the man goes to her dwelling, a great feast is then made to which friends of both parties are invited, and during the course of the feast he rises and claims her as his wife in the presence of all assembled. On the following day she and her friends go to his house, when a second feast is made, after which they are regarded as man and wife. Weasel Belief. The weasel causes great alarm and fear among the Haidas. He is the heart-eater and man-slayer. He is supposed to enter the dwellings stealthily at night and pass into the man’s interior through the fundament. The weasel] then feeds upon the man’s heart and he shortly dies. This happens to those who do not honour the Raven.by doffing their caps when a bird of this species flies over heads. The Myth of Tou; or, the Little Mountain and the Spider. On the shores of Masset Inlet a long time ago lived two little mountains. One was a good mountain and the other was not. The good mountain was satisfied with his lot, with his food of hair-seal and halibut, was blessed with a good digestion, and an even temper. The bad brother Tou wanted dog-fish, and grumbled and growled all the time because the chief of the waters would not let him have his sister’s rations as well as his own. At last he determined to change his place of abode, and one moonlight night he set out on his journey. He travelled fifty miles, tearing up the ground and making a dreadful noise as he went, and finally- pulled up on the Northern Coast near Rose-spit, where the dog-fish abound. Here he stayed, and his walls of black basalt now tower 200 or 300 feet above the shore. He now gets all the dogfish he desires, but still he is not satisfied. A large spider lives in the clouds over his head, which makes itself very disagreeable to him by pulling his hair and screaming and howling in his ears. This spider caused much disquietude among the Haidas themselves also. No one would venture to go to sleep near its abode. But once a Haida warrior determined to seek out the spider and fight with it. Sohe took a barbed spear, a wooden drum, and a big whistle and went to seek the enemy. He made such a din with his drum and whistle that the spider came down to see what was the matter. When the spider perceived the man he came at him open-mouthed, screaming and growling the while. The warrior thrust his spear into the terrible creature’s jaws, which stopped its noise and prevented it from closing its mouth. To the spear _ was attached a long cord, with which the man now tethered the spider to a tree so that it could not get away. The spider finding itself fast grew terribly angry, and began to break up the mountain, and hurled large masses of it at the warrior, who had much ado to avoid them. At last 1898. ZZ 706 REPORT—1898, the spider succumbed to hunger and died ; and its body was then cut into extremely small pieces by the female relatives of the warrior. But though the spider no longer troubles Tou, he has not ceased to grumble yet. Tidal Wave Myths. The tidal waves are believed by the Haidas to be caused by three sisters who dwell on the West Coast. When they are annoyed in any way they revenge themselves by raising these great waves and smashing the canoes cf the Haidas and drowning their occupants. The devil-doctor is the only intermediary between the sisters and the people, and his services must be well paid for before he acts. Tschimose Myth. The Haidas belief in the existence of a fearful man-eating monster, who lives half in and half out of the sea. This dreadful being is seen once in about fifteen years, and his appearance presages a time of famine or pestilence and sickness. The Killer-whale Myth. When a Haida is drowned it is believed that his spirit is translated to the body of a Killer-whale. These whales were therefore formerly much honoured, and never killed by the Haidas. The appearance of one of them off the shore in front of an Indian’s dwelling is always regarded as a ‘call’ to some member of the household, who will shortly meet with his death by drowning. Land-otter Myth. The Haidas believe that the land-otter has the power to enchant men. He meets hunters and wanderers in the forest in the guise of a beautiful maiden, who says to the victim, ‘Come and sit down with me.’ The wise man is able to detect the enchantress by the pronunciation of the words she uses, and so escapes her charms. The unwary, yielding to her wiles, become her slaves, or are found wandering in the woods bereft of their senses, She is also supposed sometimes to place certain leaves which have magical qualities in the springs frequented by the people. Hence, before taking a drink the Haida first throws a little water over the right shoulder, saying at the same time, ‘ Land-otter, land-otter, go from me !’ The Thunder-eagle Myth. This widespread myth is found also among the Haidas. They regard the thunder-eagle as their deadliest foe. They suppose that he dwells as a lonely god among the most awful recesses of the mountains, and that when he is hungry he robes himself in eagle form and swoops down upon the land, darkening it with the shadow of his widespread wings, whose motions give rise to the thunder. The lightning is supposed to come from the tongue of a fish which the thunder-eagle carries under his pinions. The Mouse Myth. This myth of the mouse is one of the most firmly implanted in the minds of the Haidas. It enters very intimately into their lives. The younger members are beginning to laugh at the notions connected with it now, but their elders still firmly believe in them. To them the harmless ON THE ETHNOLQGICAL SURVEY OF CANADA. 707 little rodent is a veritable demon. They believe that its home is the stomach of human beings, and that every person has one or more of them in his stomach, If a person is bad-tempered, immoral, passionate, a liar, thief, &c., they attribute these qualities in him to the mice-demons in his stomach. Again, if a person is taken ill, his father turns all his goods and belongings out of doors ; he next proceeds to catch a mouse. Having secured one, he puts it into a small box and gives it plenty of grease to eat. He abstains himself from all food for three days. Each morning he takes the box and mouse down to the sea and drinks about a quart of salt water He then returns and throws himself on his bed, places the box containing the mouse under his pillow, and goes to sleep. He sleeps throughout the day and following night, sentinels being placed about the house to prevent anyone from disturbing him or making a noise. In the morning he rises, goes down to the beach, drinks his quart of salt water, and returns to sleep till the following morning. He keeps this up for three successive days. If during this while he imagines or dreams that a person or spirit from the invisible world has appeared and revealed to him the name of the individual responsible for his son’s illness, he straight- way rises and goes to this individual and charges him with the act, and demands his reasons for attacking his son in this manner. If, however, no vision or dream comes to him, after the third day has passed he takes the mouse in his hand and goes into every house in the place, and holds the mouse in front of each person until he is satisfied that he has found the individual guilty of the offence. If the mouse nods its head twice before anyone, it is to the Haidas plain proof that the culprit is revealed. Tn the older days this person would be found dead in the woods a little while after. If one of these harmless little creatures has scampered over any food the Haidas would never think of eating it. They believe it is then im- pregnated with poison. It is all thrown into a fire and consumed. Cloud Myth. When the clouds hang low the Haidas believe that a soul is being snatched away, and expect to see one of their number shortly die. Transmigration of Soul. The Haidas believe in the transmigration of souls in this way : If, when @ person dies, the nearest female relative of the deceased is about to be delivered of a child, the soul of the deceased will pass into the body of the new-born infant and live again. Specimens of Songs of the Haida. Berry Song. Whit squate, squate, whit squate squate A la whit, a la whit: Kalunga olthé, kalunga olthé Siamzi whé, siamzi whe whit. The above is an invocation to a bird called the ‘ whit,’ which is sup- posed to ripen the berries. It is besought to bring many large and nicely coloured ones. ZZ2 708 REPORT—1898, Ridicule Song. Yelthgowasu kingung Laou wangung, laou shugung Laou iching, laou iching Laou kanga? laou kanga ? Yelthgowasu kingun. Translation.—NotE.— Yelthgowasu is a man’s name. Yelthgowas sees it, He does it, he says it, He it is, he it is ; Did he see it ? did he see it 4 Yelthgowas saw it. Devil Doctor's Song to the Spirit of the North Wind. Ada adda di whi silthliga adi gwudakoustloga Dikwun kwul dungalthdagang alskid ada hi hi hi e. Ditto to the East Wind. Oh, hiaa, oh hiaaohiaaaa Kalke kona kishaaa A skidje a dung a thu kagwalgudied Kalke kona kish a a a ho. Nore.—‘ Skidje’ is the daughter of the mist and east wind, but has now become a diver on account of her poverty. She and her father, the east wind, are invoked to cause fair weather and keep off snow and ice. . Wind Song. Di whiskada gwe he he Di whiskada gwe he he Hangi kwungust, di whiskada agwi. Translation of above. The wind is whistling to me, The wind is whistling to me, The wind is blowing boisterously in my face. Specimen of Haida Syntax. Itil kwogada daha itil Aunguans, (Us love you our Father great ;) Altsulth heth il istaiang kit unga, (Therefore down he sent son his ;) Jesus Christ nung alth etil kaginsh is, (Jesus Christ he our Saviour is ;) Altsulth Jesus itil hagunan kwotalang, (Therefore Jesus us for died.) T am indebted to the Rev. Mr. Harrison for information on the Haidas. ON THE ETHNOLOGICAL SURVEY OF CANADA. 709 APPENDIX II. Customs and Habits of Earliest Settlers of Canada, By BENJAMIN SULTE. It is intended in this paper to explain the mode of living of the explorers, and afterwards of the first settlers on the shores of the St. Lawrence, as well as the modifications they introduced in their customs, habits, &c., in order to conform themselves to the requirements of the new country. There are two phases to be examined in connection with this : from 1535 to 1631, and from 1632 to 1660 or thereabout. Let us follow, first, the explorers of Eastern Canada, and see who they were, how they acted in regard to climate, dress, and food. The men of Cartier and Roberval (1535-44) were all Bretons and unaccustomed to residence elsewhere than at home in Brittany. The result was that most of them perished by the effect of cold, bad nourishment, disease, and despair, whilst the present French Canadian would not experience any hardship were he to find himself in the same situation. When Champlain (1604-30) describes the miseries of life in Acadia and the lower St. Lawrence, he merely states for our information that his men and himself had acquired very little knowledge in that sense above that of previous explorers. They still persisted in depending upon the provisions brought from France—salt pork, beans, flour, mostly affected by the influence of weather, time, &c., and not always abundant enough to cover the period at the end of which a fresh supply would be sent. It was considered good fortune when one or two of the men could handle a gun and shoot some game. As for the art of fishing, nobody seems to have known anything of it, and these people starved alongside of a world of plenty, since they had the rivers, and lakes, and the forests lying all around their miserable camps. The only superiority of the Champlain men over the crew of Cartier consisted in the building of a house or two, but even at this they showed rather poor conception of comfort. Chauvin, in 1599, went to Tadoussac and left there sixteen of his followers to winter, without the elementary precautions of providing them with eatables and warm quarters. In the spring of 1600 the place was found empty, and none of the men are men- tioned afterwards. The Indians had always been friendly to them, but could not take such inexperienced folks to the woods. The same thing happened to De Monts (1604-5) in Acadia, when nearly all his party died of scorbutic disease and want of food during the rough season. Champ- lain, who knew these facts recorded from the years of Cartier, did not succeed any better in 1608, when he lost twenty men out of twenty-eight. This was repeated yearly afterwards, but in smaller proportions. Even as late as 1627 the ‘winter residents’ of Quebec were ignorant of the advantage of cutting trees during the summer in order to prepare dry fuel for the October—April season. It was Pontgravé who advised them to do so, and no doubt they recognised it was a great forethought. They used to pick up whatever the wind would blow down of branches in the forest, and if that material proved insufficient on extremely cold days, then they tried their hands at felling some trees near by and supplying them in blocks to the steward’s room. No wonder that the writings of the period in question so often complained of the evil of smoke and the small quantity of heat produced by the burning of such green wood. Stoves being unknown to the hivernants in Canada, a caboose supplied 710 xl REPORT—1898, the place of that indispensable adjustment, and the men, unoccupied most of the time, slept around it, starved there, got sick and died on the spot, one after the other, as a matter of course. Father Biard, evidently ahead of his generation, once made the remark that an iron box (a stove) such as used in Germany was preferable by far to the poisonous system of caboose. The improvement made by Champlain in his house at Quebec consisted in substituting an ordinary chimney for the open fireplace above alluded to. It is likely that Louis Hebert in 1617, and Guillaume Couil- lard about 1620, built similar smoke-escapes in their homes ; they also had the good sense to fit door and window sashes so as both to close her- metically and open easily when required. These marvels were not to be surpassed for a long while after that. The equipment provided for the men of Cartier, Roberval, Chauvin, De Monts, and Champlain was not generally suitable in Canada. Slouch felt hats are not equal to fur caps in winter ; boots and shoes of European fabrics could not compete with the moccasins ; and as for overcoats, it may be said they were not fit for the climate. Gloves, trousers, and under- clothes adapted to the exigencies of 30° below zero constituted a puzzle for these people. Snowshoes and mitts were doubtless adopted at an early date from the Indians. Jt was well known throughout France that Canada was a purgatory for civilised people, and would never be settled by Christians. Building houses was not customary in Quebec until 1632, because the men (all without families) were located for the winter in what was called the fort.. As it was not intended to increase the colony, no carpenter was needed for other purposes than to keep the sbips in repair. This awkward situation remained the same during twenty-six years. What was the cause of it? Simply this: the men for Canada were recruited from the working classes (if not of the worst), through the suburbs of large cities and towns, the very individuals who were the least fit for the trials to be met in a wild country. For instance, a shoemaker is not called upon to find his daily bread and meat by sowing wheat, plant- ing vegetables, or hunting and fishing. Those men do not know how to manufacture clothing or to dress themselves appropriately ; neither can they prepare beaver or other skins to make a soft and warm garment, Their ‘ coaling’ power was also limited, for the wood standing in the forest was for them a foreign product, accustomed as they were to receive their fuel all cut up and dry at the door of their homes. Necessity, it is said, is the mother of invention ; but this only applies to people who already live by inventions, such as poor country folks—not the ‘citizens’ who depend upon the shops in their street. Furthermore, those who came to Canada ‘took no stock’ in the future of the country, and they returned to France (when not buried here) in haste, without having had time to learn much. The fur companies did not ask them to become Canadians. They had no reason to turn a new leaf and devise a means of life so completely different from their habits and aspirations. Now we will close this unfortunate period by saying that about twelve or fifteen of the youngest men, still employed in the neighbourhood of Quebec in 1631, were merged into the subsequent immigration and became equally competent with that new formation, 7e., the actual settlers. This little squad, strange to say, was all from Normandy, and every one of them educated far more than ordinary people: this was the gy pee result of a century of wrong management in the affairs of anada. ON THE ETHNOLOGICAL SURVEY OF CANADA. 711 Coming to the second phase, we have to introduce farmers of Perche, Beauce, Normandy, and Picardy, numbering forty-five, from 1632 to 1640, besides twenty-six from Champagne, Lorraine, Brie, Poitou, Maine, during the same nine years. This period gives an average of eight settlers per year only, which may be considered the proportion for twenty years afterwards. The group of Perche took the lead from 1632 and kept it for ever. They came married, bringing their farm implements, cattle, &c., and in less than two years after their arrival conquered the soil, learned how to face the climate, and made themselves literally at home, where their pre- decessors had miserably perished by scores during many years. The typical Percherons knew the way to clear the forest, because their country was covered (especially in those days) with trees. They produced all sorts of grain, poultry, cattle, pigs, &c.,and so they did in Canada from the outset. Every woman had a trade of her own—the men also. Take Beauport, near Quebec, as an example : the first ten or twelve agricultural families located there were composed of a stonemason, a carpenter, a tiler, slater or thatcher, a blacksmith (often called armourer), a miller, a shoemaker, a ropemaker, a leather-dresser, and two or three weavers. Before the clothes brought from France were worn out the ‘ Canadian’ manufacture supplied the little colony with fresh woollen stuff of various fabrics from serge and camlet to much thicker cloths, as well as linen made of their culture of flax. It soon became a saying that the ‘habitant’ (so named by contrast with the roving fur-trader) needs no help from France, except in the line of iron and steel tools and firelocks. From head to feet they could provide for themselves ; their table was well sup- plied, their houses comfortable ; in fact they lived in luxury. The culinary art had many adepts amongst them, and this has been trans- mitted through generations. The hygienic aspect of the situation must have been well understood by those early settlers, because not even the children were affected by the influence of the new climate and habits of life. Scorbutic diseases dis- appeared from 1632—that is to say, never prevailed amongst actual settlers or habitants, but continued to follow the men sent to the advanced posts for a winter or two in the pursuit of the fur trade. Boots and shoes brought from France soon became known as bottes et souliers francois, to be used indoors on special occasions only. Bottes et souliers sauvages served all other purposes at every season. The long overcoat, or capot, made of coarse woollen cloth with a nap on one side (frieze) called bwre in French, is a remarkable instance of their ingenuity. This coat has a hood attached to the collar and dropping behind : it is buttoned up and down, double-breast, and made tight around the body by a wide and long woollen sash of bright colours, altogether an immense improvement over the ‘caban’ or dreadnought-coat of the mariners, well known in England and France. Their mode of colonisation also differed from that which could have been expected, considering that in France the country people are centralised in villages somewhat away from the fields they cultivate. The first attempt made in Canada to lay out farms (1632) consisted in having them in a row facing the river and distant from one another about four arpents: each lot of land measured forty arpents deep, making one hundred and sixty square arpents for a farm. This system was adopted by the whole of the colony as it gradu- ally got settled—notwithstanding the authorities who were in favour of the formation of villages in preference to what they styled a ‘dispersed order.’ The advantage of such an arrangement is to bring the house a 712 REPORT—1898. few steps from the river ; to permit easy access to the public road situate between the house and the river; to keep social intercourse as close as possible by the vicinity of neighbours addicted to the same profession. In a case where twenty habitants so covered eighty to one hundred arpents on a line following the water’s edge, they did nothing else but open a street, and so they could visit each other with facility at all times. Four feet deep of snow in the winter was beaten down within two hours by the passage of forty or fifty horses and men. This of course was at first done on snowshoes until horses were introduced (1665), and then this arrangement worked to perfection. That was the time that the French carriole—on wheels—was dismounted, put on runners, and became the comfortable family vehicle so popular in Canada East during the snowy season. Anyone who will peruse the numerous works containing letters and documents relative to the years 1632-70 in this colony may obtain more information on this subject. In conclusion I may mention inventories (existing in original) of household effects, which afford a fair idea of the contents of the early residences, such as furniture and utensils, from 1640 to 1670. The kitchen has a special fireplace where the cook- ing was done. Two or three chimneys (brick or stone) heated the main part of the house. Wooden floors everywhere, smooth, clean, covered with rug-carpets. Sleeping rooms upstairs. Double doors and windows for the winter. A large and well-lighted cellar, with a compartment for ice to be used during the summer months. The four walls of the building made of thick lumber placed flat one over the other in a horizontal posi- tion. No chairs, but forms for two, four, or six persons. No wine, but cider and beer sometimes, also guildive, a second-class brandy, and rum. Flannel, serge, heavy cloth, linens of various descriptions, all home-made, and of which the farmer’s wife felt proud, were stored in cupboards or closets. The population came altogether from that part of France where cider and beer were most in use ; they immediately started a brewery and a plantation of apples on arriving in Canada. Guildive and rum came from France. The evident superiority of the men who came immediately after 1631 over those who had previously tried to reside here is the object I wish to impress upon the mind of the reader. The manner in which they practised agriculture, their habits, customs, dresses, all things belonging to them, were afterwards adopted by all the new comers. Such is the evidence very clearly shown by our archives. Ethnographical Survey of the United Kingdom.—Sizth Report of the Committee, consisting of Mr. E. W. BraBroox (Chairman), Dr. Francis Gatton, Dr. J. G. Garson, Dr. A. C. Happon, Dr. JOSEPH ANDERSON, Mr. J. RomiLLy ALLEN, Dr. J. BEppoE, Mr. W. Crooke, Professor D. J. CunnincHam, Professor W. Boyp Dawkins, Mr. ArtourR J. Evans, Mr. F. G. Hivton Prices, Sir H. Howortu, Professor R. Mertpoua, General Pirt-Rivers, Mr. E. G. RAvENsTEIN, Dr. H. O. Forses, and Mr. E. Sripney Hart- LAND (Secretary). (Drawn up by the Secretary.) 1. As in previous years, the Committee has had the advantage of the co-operation of several gentlemen, not members of the Association, but delegates of various learned bodies interested in the Survey. ON THE ETHNOGRAPHICAL SURVEY OF THE UNITED KINGDOM. 713 Mr. George Payne, one of the delegates of the Society of Antiquaries ; Mr. E. Clodd, Mr. G. L. Gomme, and Mr. Joseph Jacobs, representing the Folklore Society ; Sir C. M. Kennedy, K.C.M.G., representing the Royal Statistical Society ; Mr. Edward Laws, the Venerable Archdeacon Thomas, Mr. S. W. Williams, and Professor John Rhys, representing the Cambrian Archeological Association ; and Dr. C. R. Browne, a representative of the Royal Irish Academy, have continued their valuable services. Other members of the Committee are delegated by the Anthropological Institute. 2. Having last year, in its Fifth Report, recapitulated the steps taken towards the fulfilment of the duty entrusted to the Committee, it is unnecessary to do more here than make a brief record of its further proceedings. 3. At the time of the last report the Committee had appointed the _ Rev. H. M. B. Reid to carry on the work in Galloway initiated by the late Rev. Dr. Gregor, and the Rev. Elias Owen, F.S.A., and Dr. H. Colley March as special observers in North Wales and Dorsetshire respectively. 4. No complete report has yet been received from the two former gentlemen ; but the Rev. H. M. B. Reid has sent some notes of customs, in anticipation of a fuller report. Dr. Colley March devoted some weeks of the autumn of last year to inquiries and observations in Dorsetshire. His preliminary report on the folklore of the district has been received. In addition to this, he measured and took photographs of a number of typical inhabitants. Dr. March has kindly undertaken to proceed with his inquiries, and it is hoped that, if the Committee be re-appointed, a further and fuller report may be made next year. Meanwhile, the physical measurements and photographs are postponed, to be dealt with when his inquiries in the district are completed. Dr. March has also forwarded a sketch and photographs of the famous Giant of Cerne Abbas. 5. The Committee is indebted to Captain Bryan J. Jones for a report of some interesting traditions and superstitions collected by him at Kilcurry, co. Louth, Ireland, together with a careful sketch-map of the village, showing the spots believed to be haunted and the route tradition- ally assigned to the ‘ Dead Coach.’ 6. The Committee has also to acknowledge communications from Mr. John Fielder Child, of observations at Farnborough, Hants ; Mr. Adam Lander, of observations in Ross-shire, Scotland ; and the Right Rev. the Lord Bishop of Barrow-in-Furness of observations at Churt, Surrey. 7. The Committee has received, by the kindness of Mrs. and Miss Gregor, a wooden mould for making horn spoons, obtained by the late Rey. Dr. Gregor in Galloway. This interesting relic of the domestic arrangements of the past has been handed to the Folklore Society, and deposited by them in their case in the Cambridge University Museum. 8. Early in the present year the Committee, by the courtesy of the Anthropological Institute, the Royal Archeological Institute, and the Folklore Society, distributed to the members of those bodies a circular calling attention to the objects and methods of the Committee’s inquiries, and asking for assistance. Several replies were received, but, with the exception of Captain Jones’s report on the traditions of Kilcurry, the Committee regrets to be unable as yet to record any definite result. 9. In view of this the Committee desires to call attention to paragraphs 18-26 of its last year’s Report, and to emphasise the fact that, while the 714 REPORT—1898, whole scheme of the Committee’s inquiries includes a number of subjects, thus appealing to persons interested and capable of rendering assistance in various ways, it is not considered necessary for each observer to deal with them all. Having regard to the movements of population and the spread of education, some subjects, such as current traditions and beliefs, and dialect, are more immediately pressing than others equally important for the purposes of the Committee. 10. Moreover, it is a question whether the time has not arrived for considering some practicable suggestion for employing a paid and expe- rienced assistant to make observations in parts of the country which may be expected to yield results of special value for the inquiries. 11. The grant appropriated to the Committee at the Toronto meeting has not been drawn, and some balance remains in hand from that appro- priated at the Liverpool meeting. The Committee asks to be re-appointed and permitted to use this unexpended balance, and to be provided with a further grant, so as to have at its disposal the total sum of 50/. during the coming year. Functional Activity of Nerve Cells—Second Report of the Committee, consisting of Dr. W. H. GAsKELL (Chairman), Professors BURDON SanpErson, M. Foster, EH. A. Scuarer, J. G. McKeEnpricx, W. D. Hatuisurton, J. B. Haycrarr, F. Gotcu, C. 8S. SHER- RINGTON, and A. B. Macatuum, Dr. J. N. Lanaury, Dr. G. Mann, and Dr. A. WALLER (Secretary), appointed to investigate the changes which are associated with the Functional Activity of Nerve Cells and their Peripheral Extensions. APPENDIX. PAGE I, Structural Alterations observed in Nerve Cells. By W. B. WARRING- TON,MD. . ‘ ‘ . 3 : : . ; : d ». 715 Il. Hecitatory Electrical Changes in Nerve. By FRANCIS GorcH, /.2R.S., and G. J. Burcu, M.A. > 716 Ill. The Effects upon Blood-pressure produced by the Intra-venous Injection of Fluids containing Choline, Neurine, and Allied Substances. By F. W. Mort, I.D., F.R.S., and W. D. HALLIBURTON, MD. FRS. . ECT. IV. The Myelination of Nerve Fibres. By H. V. ANDERSON, UD. . e W1T V. The Histology of Nerve Cells. By GUSTAV MANN, M.D. S - ait eo Tue following investigations have been carried out during the past year :— Dr. G. Mann : Histological changes in nerve cells. Professor Boyce and Dr. Warrington: Changes in nerve cells after section of nerve fibres. Dr. J. L. Bunch : Position of cell stations on the course of sympathetic nerves. Professor Sherrington : Activity of nerve centres correlating antago- nistic muscles. Professor Gotch : Electrical changes in nerve fibres during activity. Professor Halliburton and Dr. Mott: Effects of neurine and choline upon the vascular nervous system. Professor Waymouth Reid and Dr. Macdonald: Electro-motive changes in the phrenic nerve. Dr. Anderson : On the myelination of nerve fibres. The results of several of these investigations have been already in part - ON THE FUNCTIONAL ACTIVITY OF NERVE CELLS. 715 published in the ‘ Journal of Physiology,’ and in [the ‘ Proceedings of the Royal Society,’ 1897 and 1898. In addition the following reports have been received. ; APPENDICES. I. On Structural Alterations observed in Nerve Cells. By W. B. Warrineton, J.D. A paper was published in the ‘Journal of Physiology,’ vol. xxiii, on the structural alterations observed in nerve cells :— (1) Of the anterior horns of the spinal cord after section of the osterior roots. (2) After division of the axons belonging to them. Summary of Part I. Records of observations made on eight cats and one monkey are ven. ‘i These observations show that after sections of several posterior roots, from the fifth to the ninth post-thoracic inclusive, a considerable per- centage of obviously altered cells are found : their distribution in the case of the cat is practically limited to the seventh and eighth segments, and especially to the postero-lateral group of cells in those segments. In the monkey the upper part of the seventh segment is picked out. The effect is to a very slight extent a crossed one, and presents the remarkable feature that more affected cells were found in the sixth seg- ment of the crossed side than on the side of the lesion. In the cervical region, in one case, similar but slight changes were found limited to the seventh segment ; in the other the spinal cord was practically normal. The significance of these results and of their limitation to certain cell groups is discussed, and the view adopted that the structural changes correspond to the altered functional state of motor cells deprived of the afferent impulses which impinge upon them. Summary of Part II. Observations were made on eight cats, one monkey, and on material supplied from the autopsy room (I am indebted for the material in the case of the monkey and one cat to Professor Sherrington). The observations show that— 1. Distinct and easily recognisable changes in nearly all the cells of a segment of the spinal cord are found on the side of the lesion after section of an anterior root. 2. Similar but less marked changes follow division of the facial nerve, and still less distinct alteration after division of the oculomotorius nerve. 3. The fate of such altered cells and the ultimate condition of the nucleus of origin are not yet definitely ascertained. 4, The age and nature of the animal experimented on is a factor in 716 REPORT—1898. determining the rapidity and degree of alteration met with in the nerve cells. A paper on the Morbid Anatomy of a case of lead-poisoning will appear in the spring number of ‘ Brain,’ by Dr. Laslett and myself. An examination of the various segments of the spinal cord and the corresponding nerves was made, and it was found that certain cells in the anterior horns showed changes comparable with those described after division of an anterior root, and that these altered cells were limited to these segments from which the most degenerated peripheral nerves and anterior roots were derived, the posterior roots being in all cases normal. II. On Excitatory Electrical Changes in Nerve. By Francis Gotcu, F.2.S., and G. J. Burcu, ILA. The authors have employed the apparatus described in their previous report, and have succeeded in obtaining photographic records of the movement of the mercurial meniscus of the capillary electrometer due to the electromotive changes produced in nerve in response to a single excitation. The results have been briefly set forth in communications both to the Physiological Society! and the Royal Society.2. In these communications it will be seen that the authors have studied the influence of varying conditions of the nerve upon the character of the electrical response as indicated by that of the photographic record. The records themselves are sufficiently large to permit the determina- tion of the time relations of the electromotive changes, and thus afford data for the more precise estimation of the characters of the propagated excitatory state constituting the so-called ‘nervous impulse.’ From an analysis of the records it is thus possible to obtain a history of the amount and extent of the change in any one portion of the nerve when the state of excitation reaches this portion, this state having been started in the nerve trunk by a single stimulus. When two contacts on the uninjured nerve are arranged in connection with the instrument, a change of the above character occurs, first under the proximal contact (z.e. that nearest the seat of excitation), and later under the distal one ; the algebraic sum of the two effects is a rapid biphasic change indicated in the photographic record by a spike. Each complete change under one contact only is indicated in the record by a sudden rise, followed by a prolonged tail or after effect ; the E.M.F. of the former attaining a maximum of -03 volt with great rapidity, that of the latter a maximum of -003 volt ,3,, second later. Starting with these fundamental characteristics, the authors have examined the influence of the following changes of condition : (1) electro- lytic changes produced by polarising currents ; (2) persistent electromotive changes produced by localised injury ; (3) local alterations in temperature ; (4) variations in the intensity of the stimulus ; (5) the frequent repetition of the stimulus ; (6) CO, gas, &c. The research is now being extended to comprise the electromotive effects produced in mammalian nerves, both peripheral nerve trunks and nerve roots, as also those known to exist in the spinal cord. Endeavours are also being made to obtain records of the changes in mixed nerves, roots and cord, evoked by reflex discharge of the central 1 Journal of Physiology, vol. xxii. (xxxii.). ? Proc. Roy. Soc., vol. |xiii. 1898, p. 300. ON THE FUNCTIONAL ACTIVITY OF NERVE CELLS. 217 _ nervous system, in the hope that the character of the discharge from the efferent nerve cells may be thus elucidated. The research has, so far, amply fulfilled the expectations of the authors, and it is particularly gratifying to them to feel that the results are not dependent upon the possession of a particular capillary electrometer. This is shown by the circumstance that when, owing to an unfortunate accident, the instrument was broken, a second one, made for the purpose, has given, if anything, better results than that originally employed. It appears, therefore, that any electrometer of adequate sensitiveness and sufficient rapidity will furnish records of the change, if appropriately used. Since every delicate capillary electrometer is, from the nature of things, a perishable instrument, this fact is one of great importance for the prosecu- tion of the present research. III. The Effects upon Blood-pressure produced by the Intra-venous Injection of Fluids containing Choline, Neurine, and Allied Substances. By F. W. Mort, 1.D., F.R.S., and W. D. Hatirsurton, W.D., F.R.S. In the communication on this subject published in the British Associa- tion Report last year we stated that cerebro-spinal fluid removed from cases of brain atrophy (particularly from cases of general paralysis of the insane) produces a fall of blood-pressure. From the similar result produced by choline we thought it possible that the toxic material derived from the disintegration of nervous tissues, and contained in the cerebro-spinal fluid, was choline also. We have now completed our chemical examination of the material, and proved that our supposition is correct. The fall of blood-pressure which occurs is partly of cardiac origin, but its main cause is vascular dilatation in the splanchnic area. This was investigated by the use of Barnard’s cardiometer, and by the use of air-plethysmographs applied to various organs. The intestinal oncometer used we owe to the ingenuity of Mr. A. Edmunds, B.Sc., who has described the instrument in the ‘Journal of Physiology,’ vol. xxii. 1898, p. 380. By means of section of the spinal cord, and also by the use of large doses of nicotine, we have cut out the influence of the central nervous system, and of peripheral vaso-motor stations. Choline still produces, under these circumstances, the usual fall of blood-pressure, which is there- fore due to the action of the poison on the neuro-muscular apparatus of the blood- vessels. The allied alkaloid, neurine, produces somewhat different results, and is far more toxic. There is a primary fall in arterial pressure, mainly of cardiac origin ; the slowing of the heart and deepening of respiration are very marked symptoms. Usually this is followed by a rise of pressure, due to constriction of peripheral blood-vessels. In some cases this latter phase is absent ; and in some few cases, using very small doses, the second phase only occurs. IV. On the Myelination of Nerve Fibres. By H. V. AnpErson, UD. A systematic investigation of the peripheral nervous system of man, the cat, and the rabbit has been commenced to ascertain the relative 718 REPORT—1898. progress and date of medullation of the various fibres of the cranial, spina], and sympathetic nerves. Afferent fibres have been distinguished from efferent by the use of the Wallerian method, and the number of afferent fibres in various somatic and sympathetic branches has been determined in kittens from a few days to several weeks old. At the same time the intra-spinal degeneration resulting from section of posterior roots in kittens of different ages has been traced by Marchi’s method. By these observa- tions an attempt has been made to divide the fibres of all the peripheral nerves into embryological systems, and to trace the distribution of each afferent and efferent system separately. Several experiments have also been performed according to V. Gudden’s method upon kittens and rabbits a few days old to determine— (1) the effect upon the development of a posterior root ganglion of section of the corresponding posterior roots or peripheral nerve trunk respec- tively ; (2) the changes produced in certain posterior rootlets, spinal ganglia, and cells of the spinal cord by cutting many peripheral branches, each of which contains a relatively large proportion of fibres belonging to a given embryological system ; (3) the effect upon the development of the fibres of the cervical sympathetic nerve of section of the nerve itself, or of branches of the superior cervical sympathetic ganglion ; (4) the central origin of the fibres of the cervical sympathetic nerve by the atrophy of cells following section of the nerve in very early life; and (5) the alterations in the cells of a sympathetic ganglion resulting from section of its pree- or post-ganglionic fibres respectively. I append a summary of some of the observations made : The two systems of afferent fibres, which are the first to become medullated, are found to be common to both the somatic and sympathetic nerves, and to assume their fatty sheath before the efferent visceral fibres. The two afferent systems mentioned are distinguished from each other, not only by the considerable interval between the dates of their medulla- tion, but also by the mode of their peripheral termination, the fibres of the earliest medullated system alone entering end-organs. The later medullated afferent fibres of both somatic and sympathetic nerves have not yet been fully investigated. The efferent somatic fibres do not all become medullated at the same time, and certain embryological relations have been observed between certain cranial and spinal efferent fibres. The various visceral efferent fibres also develop their medulla at different dates. Section of the posterior roots in very young animals has little, if any, effect upon the development of the corresponding posterior root ganglion, but section of the trunk of the nerve distal to the ganglion causes marked macroscopic and microscopic changes in the same duration of experiment, viz., about eight weeks. These results confirm the work of Lugaro upon the spinal ganglia of adult animals. In the second form of experiment ‘obvious changes are found, also in the posterior roots, and it is possible by this method to connect certain posterior root fibres with given afferent nerves. Early section of the cervical sympathetic nerve markedly hinders the development of the fibres of that nerve, and though some fibres become eventually medullated, they are small, and stain only a faint grey colour with osmic acid. Jn two kittens in which the internal carotid branches of the superior cervical sympathetic ganglion had been cut some days —_- °° ON THE FUNCTIONAL ACTIVITY OF NERVE CELLS. 719 previously to the commencement of medullation in the cervical sym- pathetic nerve, I found later a smaller number of fibres medullated upon the cut side, and also many atrophied cells in the ganglion; but in a third experiment, in which longer time had elapsed since the section of the same branches, there was little, if any, difference in the two cervical sympathetic nerves. I have therefore made other experiments to decide what are the results following section of post-ganglionic fibres, but the experiments are not yet complete. The section of the cervical sympathetic nerve in a young kitten appeared to have little, if any, effect upon the development of the superior cervical sympathetic ganglion. In the cord of a kitten 120 days old, in which part of the cervical sympathetic nerve had been removed on the eighth day after birth, I found that the small cells in the lateral horn of the first, second, and third dorsal segments upon the cut side were very decidedly fewer in number than upon the uncut side. I have twice repeated this experi- ment, but the spinal cords have not yet been examined. Some of my experiments by the atrophy method point clearly to the correctness of Mott’s hypothesis, that cells of Clarke’s column are con- nected with afferent nerve fibres supplying the lower limb. A preliminary account of some of the observations made has been given in a thesis for the M.D. degree at Cambridge, and it is hoped that fuller details may soon be published. V. The Histology of Nerve Cells. By Gustav Mann, WD. Over seventy different fixing methods were used, and chemically most diverse substances chosen so as to eliminate, if possible, all appearances due to arte facts. Reducing and oxidising, acid, neutral, and alkaline fixations, acid, neutral and alkaline stains, with reducing and oxidising substances added, were tried, and these results were obtained :— (1) In all nerve cells there exists a peripheral zone, destitute of Nissl’s bodies, and in this zone numerous fibrils and bundles of fibrils are seen. (2) The zone-like origin of the axis cylinder is due to a special accumulation of the plasm constituting the peripheral zone. (3) At the periphery of nerve cells the fibrils were not observed to branch. (4) Bundles of fibrils run also through the centre of cells, past the - nucleus, but the fibrils never come into contact with Nissl’s bodies. (5) In spinal ganglia two distinct bundles of fibrils may be dis- tinguished, one corresponding to the peripheral and the other to the central process. These bundles are arranged in vortices. (6) In central and peripheral multi-polar nerve-cells bundles of fibrils may be traced from dendritic processes to the axis-cylinder process, and from one dendritic process to another. (7) The thorn-like excrescences seen in Golgi preparations are arte- facts, caused by the potassium bichromate. (8) The nodes of Ranvier are only crossed by the neuro-fibrils, Photographs of wax models were taken, and the course of the fibrils traced in the following cells : Two giant cells of Malapterurus, motor cell from anterior horn of spinal cord of the ox, spinal ganglion cells of rabbit and dog, cell from spiral ganglion (cochlea) of guinea-pig, first giant cell of Amphioxus, sympathetic nerve-cell of rabbit. Photographs of nerve- 720 REPORT—1898. cells of motor, olfactory, visual area from the dog’s brain, showing fibrils, were also taken. All attempts made as yet to obtain the substance which shows a great affinity for basic dyes, and is found in Nissl’s bodies, were unsuccessful. The Physiological Effects of Peptone and its Precursors when introduced into the Circulation.—Second Interim Report of a Committee, con- sisting of Professor HE. A. ScHAFER, F.R.S. (Chairman), Professor CG. S. SHERRINGTON, F’.R.S., Professor R. W. Boyce, and Professor W. H. Tuompson (Secretary). (Drawn up by the Secretary.) Tw continuation of the above inquiry during the past year attention has chiefly been directed towards ascertaining the effects produced by albumoses and peptone upon the secretion of urine. The objects kept in view were threefold : (1) to determine the influence of the substances in question upon nitrogenous excretion at the kidney ; (2) to see if any important differences were manifested by the several substances when compared with each other ; (3) to ascertain to what extent the substances remained in or were excreted by the kidney from the animal body. The products examined were (1) Witte’s Peptone, (2) Proto-albumose, (3) Hetero-albumose, (4) Deutero-albumose, (5) Ampho-peptone, (6) Anti-peptone. The following report is to be regarded as a statement of the year’s work, and not as a finished research. The carrying out of the investi- gation was placed in the hands of the Secretary. The method adopted was as follows :—Dogs were exclusively em- ployed, the animals being anesthetised with a mixture of chloroform and ether, preceded, except in a few of the earlier experiments, by a hypo- dermic injection of a solution of morphine. The dose of morphine employed was small, under two milligrammes per kilo. of body weight. Cannule were placed in both ureters, and urine collected for definite periods before and after an injection of the substance employed. With the exception of hetero-albumose the substances were dissolved in physio- logical saline solution—‘6 per cent. sodium chloride. The quantity of solvent employed was 4 c.c. per kilo. of body weight for animals below twelve kilos. Above this weight a maximum of 50 c.c. was adopted. Hetero-albumose was dissolved in 2 c.c. per kilo. of weak caustic soda solution (-2 per cent.). The injection was made through a cannula placed in the external saphenous vein, and the substance introduced very slowly from a burette to avoid lowering of blood-pressure. The time occupied with the injection varied for the most part from fifteen to twenty minutes. A record of blood-pressure was taken from the left carotid artery, and showed that the injection of the substances could be accomplished without appreciable lowering. The record was not continuous, but was taken at minute intervals during the period of injection. While the subsequent collection of urine proceeded, a record was taken every fifteen minutes. As arule, urine was collected for one hour, then the substance was injected, and urine collected for a second hour, likewise for a third, fourth, and also for a fifth. The amount of total nitrogen and the quantity of urea were estimated in the different samples of the urine. That passed subsequent to the injection ON THE PHYSIOLOGICAL EFFECTS OF PEPTONE. 721 was also examined for the presence and amount of the albumose or peptone excreted. The results, so far as ascertained at the date of this report, will be set forth under the following headings: (1) Influence on the quantity of urine secreted ; (2) Influence on the amount of nitrogen and of urea pro- duced ; (3) Amount of peptone or albumose excreted. I. Influence on the Quantity of Urine. As will be seen in the following table, the introduction of the various substances was followed by a very large increase in the amount of urine secreted. The outflow reached its maximum in the second hour after the injection, and then gradually declined. But even at the end of four hours there was still, in the majority of cases, a decided increase, as compared with the outflow prior to the injection. A few experiments showed no increase. TaBLE I.—Showing Quantities of Urine secreted per hour in cubtie centimetres. (The injection was made at the end of the first hour, and extended over a period of 15 to 20 minutes.) Weight Quantity of Exp. |Hourl Hour 2 Hour 8 Hour 4/Hour 5] of Dog Fluid in kilos. injected I.— Witte’s Peptone. I.| 5:5 60 102 63 =), 29 | 11:8 | 50 c.c. II. { 14:5 | W7 1245 | 56 | 36 14:5 | 50 ,, / II. Proto-albumose. Vs (el2"""| 70 149 75 64 153 | 50,, XVI. | 105 i{ oe ge 37s 1075 | 71 | 215 | 126 | 80, 30m. 33°5 XX. | 15 15m, 24 83 63:5 | 17:5 i) 127 60. 15m. 25°5 | { 80m. 17°5 . : ™ XXI.| 22 1 30m. ae 21°25) 22 9 6 11°3 | 45 ,, Ill. Hetero-albumose. XXII. | 13:5 | 6 Nil | Dog | — | 13:2) 20,, KoH. 2% 45m. 33 wee, é XXVII.} 13 || 73m. 20 53 90 33°5 | 15 83 | 20 ,, NaOH. 2% IV. Deutero-albumose. XIII.) 10 ) 27°35 305 | 12 |10 |) 19°75) 50,, XIX. | 10-5 | 15-0 60 | 39 | 29 | 140 | 50.,, XXXII. 3°5 22°75 13°25| 6 | | 63 | 24.,, V. Ampho-peptone. TII.| 45 | 172 188 58 175 | 14:5 | 50 ,, We isc: 49 85 56 19°5 10°5 | 50 ,, | VI.| 3:75 | 11:25 8 | 80} 40,, | z = wield. 4S°S..), ook esl en DAs ' | XI: [0/05 11 G0 Oe 2 5/185 | 265 | 235 | 119 30, | 722 REPORT—1898. TABLE I.—continued. | |Weight Quantity of Exp. {Hour 1 Hour 2 Hour 3 Hour 4 Hour 5 of Dog Fluid | | iinkilos. injected VI. Anti-peptone. VII.| 6 51 PL | bb AZ 138 | 50 c.c VIII, | 13:25 10 16 7°25) 4:25 8-2 | 40 ,, TX...) 5°25 22 13 8 6 94 | 40,, XVII.} 8:66 38 27°5 | 18 — 15:0 | 50 ,, XVIII. | 18 78 L7Or | vu 35 160 | 50 ,, ’ 50m.10°5 | : XXVIII.| 4:3 per }us LZ | Uh 8 11°3 | 30,, = 45m.22'5 Sac: | oe d Lf XXX. | 21 we 1425 f 36 75 98) 40 | 126 8-1 | 25 ,, The figures in italic in the column for the second hour show the amount of urine passed in the number of minutes indicated. ‘The same applies, mutatis mutandis, to the subsequent tables. No marked difference was manifested by the various substances in regard to the amount of diuresis produced, except that the proportion of instances where no increase of urine manifested itself was decidedly greatest in the case of the substance anti-peptone. It is doubtful, however, if any stress can be Jaid upon diuretic influences, since control experiments made by injecting corresponding quantities of normal saline solution, without peptone or albumose, showed that a marked increase of urine, also reaching its maximum in the second hour afterwards, was produced by the solvent employed. This is illustrated in the following table :— TaBLe II.—Showing the Influence of Normal Salt Solution upon the Quantity of Urine secreted (expressed in cubic centimetres). (The injection was made at the end of the first hour, and extended over a period of 4 to 8 minutes.) Exp. * NOorwhe Hour 1 | Hour 2 16 28 15 32 21 67 12 29 16°5 76 6:25 15:25 13 12°25 Hour 3 * In Experiment No. 1 an injection of 12 c.c. of caustic soda solution, Hour 4 195 16 51 75 18°75 5:25 Weight | Quantity Hour 5 of injected Dog | per Kilo. 185 | 67k! 4 cc = 64 ,, 4 5 16 168 ,, 3° 5 23 1D ays Zee 40 14:9 ,, 3°5 11 19:5 || 2*Diey = 148 ” 3 ” Total Quantity injected .| 28° ¢c.c* 26 50 30 50 50 45 strength, was made at the end of the third hour. The above effect, produced by small quantities of normal salt solution, when introduced into the circulation, has proved to be a matter of very considerable interest, and forms the subject of a different research, which has arisen out of the present one. Some observations were made on the reaction of the urine passed before and after the injection of the proteid. showed the normal urine to be alkaline. 0:2% The majority of cases This alkaline was reduced to neutrality in the second or third hours or both, and gradually returned to a weakly alkaline condition, for the most part, before the close of the fifth hour, ON THE PHYSIOLOGICAL EFFECTS OF PEPTONE. 723 II. Influence on the Excretion of Nitrogen and of Urea. (a) Percentage Output.—The urine secreted in such large quantities proved to be very dilute, the percentage quantity of nitrogen and of urea being much reduced. The dilution ran almost parallel with the increase of urine, that of the third hour being the most dilute, and as the quantity of urine again reduced, it also became more concentrated. The following table illustrates this in detail so far as the percentage amount of total nitrogen is concerned. Taste III.—Showing the Quantity of Nitrogen per cent. in the Urine Secreted (expressed in Grammes). Exp. | Wie of | Hour 1 Hour 2 Hour 3 Hour 4 | Hour 5 I. Witte’s Peptone. I. 118 k. | 2°399 0°731 0269 0°391 | 0°575 Ti ala 5. 5 1:677 | 0:986 0°319 | 0°591 0°:795 II, Proto-albumose. XV. | GE A 5:023 1:299 0°406 0580 | 0-655 : ; (40 m.) 1-4 5 ; : VI. | 12°6 ,, 1:148 ee m.) 0389 0°218 0°308 0-641 [ (30 m.) 0°742 xx.| 127 , | 1179 |4 (5m) 0266!| 0-298 | 0-77 1512 | | G75 m5 0220 | PERG (30 m.) 0-491 : OeSE | 113, | 0-742 ee m> ose y| 070 0907 | L574 Ill. Hetero-albumose. MeXIT. | 132 ,, 2°358 |° 2°150 — — —- ; : (45 m.) 0°512 | : 3 ‘ XXVII | 83, | 0-763 { (ism) 0-392 ;| 0207 | 0864 | 0-815 IV. Deutero-albumose. XIII. | 19°75 ,, 7-767 2°380 1166 3:091 3°954 XIX. 14 ro 6°395 3802 0°820 1114 | 1°501 XXXIT 63 4, 2778 1:071 0°840 1:103 — V. Ampho-peptone. ST-| 14:5" ,, 0°568 0:293 07160 0°345 0:848 Wo 10:5’, 3°214 0728 0:290 0°283 0°896 VI. 8 5 1:714 1:294 0°790 0:269 — ; ; (40 m.) 1:369 ‘ 3 na XXIx.| 1-9 , | 1-512 { (20m) 0322} | 0339 | 0409 | 0577 VI. Anti-peptone. VER | 13:8), 4:217 0826 1:075 1:792 1:722 VIII. 82 ,, 2142 2°710 1:753 1°319 2°302 IX. idk, Pa 4:990 1:495 1:454 1-960 2°654 XVII. | 15 rh 4012 1:302 0:798 1°736 ao me XVIII. | 16 “ 2°548 0:608 0:238 0442 0°829 | ; (50 m.) 2°341 : | XXVUI | 113 ,, | 3920 be m) Lire {| 0999 | 13ic | 1288 Xxx. | 81 , | 0-792 bee m.) esp o228 | 0379 | o-91 (15 m.) 0°392 The percentage output of urea suffered a corresponding decrease, with _ return. It is not considered necessary to give a table. > 3AQ 724 REPORT—1898. (5) Output Hour by Hour.—Notwithstanding the dilute condition of the urine passed, it was found that the excretion of nitrogen and of urea, when measured hour by hour, suffered a decided increase as a result of the injection. This increase, with few exceptions, reached its maximum in the second hour (first after the injection). Part of the nitrogen increase of this hour, as will subsequently appear, is due to an excretion of proteid—albumose or peptone—with the urine. The increase of total nitrogen hour by hour is shown in the following table :— Taste 1V.—Showing the Quantity of Nitrogen excreted per Hour in the Urine (expressed in Grammes). | | I Quantity Weight | | _of N. Exp. of Dog Hour 1 Hour 2 | i a ti | aon gual I. Witte's Peptone. I} 118 k; -1319 | 4385 | -2742 | [14s ., | -2432 “7067 =| “3388 | Il. Prote-albumose. AV. | 153 ,, | -6027 “9094 6049 f (40m) -1750 |: { ‘ Pe eb } 2348 f (30m.) -2486 | } “1893 t WA nr te a 5 % (45 m.) “0638 (45 m.) 0560 (30 m.) 0567 \ L om.) 0437 | Ill. Hetero-aldumese. | 1990 <<]| = | (45m) “1691 ]! scn- | “0979 { (45 m.) 0644 } 1865 | IV ’. Deutero-albumose. “154 XIII. | 19°75,, | 5204 6545 | 3455 | ‘3704 aes “2012 XIX. }38 » | “4477 5T04 | 4922 | -4346 | 4352 | “1408 XXXII.| 63 ,, | 0972 2434 | -1113 | 0662 | — not deter- mined | | as yet V. Ampheo-peptone. TI} 145 ,, | -2556 | 5014 | 3000 | -2072 | “1485 | -1098 Vv. los a» | “2357 3567 | 2463 | -1584 | -1747 | “1483 iad 8 ,,| 0651 1455 «| 0632 | 1075 | — | "1342 coe | 44. yrs { (40 m.) “1848 i vor |. | ss | 1618 XXIX. 119 ., | 0756 |) (om) 0886 p |} 0727 1083. | “1355 1 VWI. Anti-peptone. VIL. }138 ,, | 2530 4213 | -2312 | VII. | &2 ,, | -2838 ‘2710 | -2804 TX. | 94 | -2619 3289-1890 | XVIJI6 . | 3475 | “4947 | -2194 | XVII. }16 ° ,, | °3058 “4739 =| 4046 wit Lave ; f (Om) 2458 ]| . XXVHIL 113 » | 1698 |} Crom) 012 f| 2699 (ee eee f (45m.) “1581 ' ‘ Xxx.| 81 ,,| tesa |f (552 ‘Seso |} sua ) peg st bs. a) oh abe a OM ile lp ReaD eo ON THE PHYSIOLOGICAL EFFECTS OF PEPTONE, 725 But the urea—estimated by the method of Morner and Sjogvist, which avoided the inclusion of any of the proteid—also showed a parallel increase, reaching its maximum likewise in the urine of the second hour. This is made clear by the following table. Moreover, it will be seen on examining the last column of this table, that the proteid injected could not have supplied nearly enough nitrogen to make up the increase of the second hour alone, to say nothing of the lesser increase shown in the following hours :— TABLE V.—Showing the Quantity of Urea excreted per Hour (expressed — as Nitrogen in Grammes.) Exp. of Doe Hour 1 Hour 2 Hour 8 | Hour 4| Hour 5 Poiteled I. Witte’s Peptone. I. |118 k.| 2 | ‘8679 | 2285 |-1751 |-1494 | -0863 1. 145 , | +2128 5954 | -2859 |-3025 |-2500 | -1078 II. Proto-albumose. XV. 1153 ,,| °5350 ‘7722 | ‘5507 |-3885 \:3655 | 1565 Xv1 | 12:6 ,,| -0991 { any beret 2062 |-1809 |*1198 | -1271 (30m.) +1801" xx. | 12-7 ,,| 1453 |4(75m.) -0538 ¢} +1618 |-1137 |-1172 |} +1271 (15m.) “0518 XxI. | 11-3 ,,| -1198 aaa: eae +1185 |-0660 |-0706 | -1174 Ill. Hetero-albumose. XXII. } 132 ,,| 2569 | a a ies a ae a xxvut.| 83 ,,| -0671 { ah cas 1638 |-1079 |-0937; — IV.. Deutero-albumose. XIII. | 19°75 ,, | 4499 ‘5159 | 83177 |°3105 |-2929 ) -2012 XIx.|14 || -3863 4536 | -4284 |-3636 |-3736 | 1408 2 i . i 3 not de- XxiI.| 63 ,,| 0747 1962 | -0976 |-0544 | — | Dot cS. V. Ampho-peptone. TIL. | 145 ,,) 2268 4938 | +2290 |-1552 |-1151 | -1098 v.|105 ; | -2002 2764 | -2249 |-1388 |-1554 | -1483 vi] 8 || -0443 0822 | -0426 |-o766| — | -1342 XXIX. 119 ,, | -0533 { keds on 0414 |-0846 |-1079 | “1618 VI. Anti-peptone. VII. | 13:8 ,, | °2235 -3510 | 2020 |-2408 |-2570| 1998 vill. | 8:2 > | -2307 ‘1915 | -2253 |-o711 |-0714 | -1427 1x.| 94 ”| -2959 2661 | -1288 |-1366 |-1398 | -1427 xvi. |15 >| -3108 3910 | -1911 |-2788| — | -2140 Xvi. |16 || -2439 3691 | -3379 |-2667 |-2352 | -2283 XXVIII | 11-3 ,, | +1246 Fisk ere 1418 |-1138 |-0806 | -1712 XXx. | 81 ,, |: -1385 hana Ba -1849 |-1277 |-0973 | +1156 726 REPORT—1898 The marked increase in the hourly output of total nitrogen and of urea, beyond that contributed by the proteid injected, cannot, however, be solely attributed to any influence which the substances employed might be supposed to exert upon nitrogenous metabolism. A similar though less marked influence is shown after the injection of normal salt solution alone. This is expressed in the following table, where it will be observed that the maximum effect is likewise shown in the second hour :— Taste VI.—Showing the Effects of Normal Salt Solution on the Nitrogen excreted Hour by Hour (expressed in Grammes). (N.B.—The injection of normal saline was made at the end of the first hour.) Weight | Quantity} Total of injected | quantity Dog _ | per kilo. | injected Exp. No.| Hour 1 | Hour 2 | Hour 3 | Hour 4 | Hour 5 - 1115 0956 0857 0551 ‘0767 67k. | 4 c.c.} 28 cc. 1 2 *1050 "1204 — —_ — 64, /4 ,, 26) ,, 3 "1570 "2082 *2066 0923 1120 | 168 ., |) -3~ ,, 50 ,, 4 1754 *3021 "2489 2113 2OTE Alb. 75s Woes 30D). 5 *B497 5533 “3748 "2583 2285 |149,, | 35 ,, 50 ,, 6 *2481 3181 2378 ‘2677 ‘2482 |.19:5 ,, | 25. .,, 50 ,, ic Nitrogien not dejtermined 48. os | pokes AD 5s * In Experiment No. 1, an injection of 12 c.c. of caustic soda solution, 0:2 per cent. strength, was made at the end of the third hour. A mixture of morphine and atropine was employed by mistake to inject this dog. Observations upon body temperature, taken per rectum, showed that a steady rise occurred after the injection was made. The rise generally appeared towards the end of the first hour after injecting, and for the most part continued to increase till the end of the experiment. Thus, in Experiment XXI. (proto-albumose) the temperatures were as follows:—Normal 37:4°C.; at end of first hour 37° C—the injection was then made ; at the end of the second hour, temperature 37°C. ; at the end of the third 37-8; at end of fourth 38°C. This was not the highest tempera- ture attained by any means; the maximum in several experiments reached 40° C., and in one it reached 41-2° C. This rise of temperature occurred even when the fluid injected was previously sterilised by boiling, and notwithstanding precautions to keep the animals cool while on the table. A similar rise of temperature also took place when sterilised normal salt solution was injected. In some of the experiments the maximum temperature was attained in the third hour (second after injection), followed by a return towards normal in the subse- quent hours. III. Amount of Peptone or Albumose excreted in the Urine. This was regarded as an important point to determine. It bears upon the question as to whether the substances under observation are to be con- sidered as wholly foreign to the blood, or to be looked upon in the same light as dextrose, which is excreted by the kidneys only when the amount in circulation exceeds a certain point. Previous experimenters had arrived at different conclusions with regard — ON THE PHYSIOLOGICAL EFFECTS OF PEPTONE. 727 to the reappearance of peptone at all in the urine after injection into the circulation, Schmidt-Miilherm,' who first studied the question, used large doses, and obtained suppression of urine lasting from twenty to ninety minutes. In the urine subsequently passed he detected no peptone. Fano? obtained similar results, as did also Grosjean* many years later, both likewise employing large doses. /ofmeister,4 meanwhile, had however shown that these substances reappeared very quickly in the urine, and devised an ingenious method, based upon the depth of tint given by the biuret re- action, for estimating how much proteid became excreted. He corrected his estimation by the use of the polarimeter, and came to the conclusion that 66 to 80 per cent. of the peptone introduced was expelled from the body within twenty-four hours. Owing to difficulties in the employment of these methods, neither can be regarded as capable of yielding accurate results. This is, indeed, admitted by the author, and, as we shall see, the figures he arrived at are a good deal too high. In the earlier experiments of this research, no other sufficiently reliable method of estimating the amount of peptone or albumose excreted was apparent. From the first, it was seen that the substance appeared only in the urine secreted during the hour immediately following the injection, and from the depth of the biuret tint it was obvious that not nearly all the proteid injected came out again. On more close examination it was found that the output of proteid was, as a rule, confined to the urine of the first forty or forty-five minutes succeeding the injection. It was also seen, on comparing the urea nitrogen of this period with the total nitrogen of the same time (which included that of the excreted proteid), that the whole difference was considerably ess than the nitrogen injected. But this difference included the nitrogen of other compounds than urea, which I shall subsequently call ‘extractive’. nitrogen. If a safe deduction, to represent the ‘extractive’ nitrogen, could be made, then we should have ascertained the amount of proteid- nitrogen which reappeared. Such a deduction was arrived at by basing a calculation on the ‘extractive’ nitrogen of the urine secreted immediately after the peptone or albumose ceased to come out. When this was accom- plished in forty to forty-five minutes, the urine of the remaining part of this hour furnished the basis of calculation. The same principle was, however, applied to many of the earlier experiments. The deduction in these cases was calculated on the ‘extractive’ nitrogen of the third hour, and the subtraction made from the ‘difference’ nitrogen of the whole of the preceding hour. In both cases the urine which furnished the basis of calculation was more dilute than that of the peptone (or albumose) excretion-period ; con- sequently, the amount deducted is safe, in the sense of being under rather than over the mark. In the following table, which gives a succinct statement of the facts } Schmidt-Miilheim, ‘ Beitrige zur Kenntniss des Peptons und seiner Physiolo- gischen Bedeutung,’ Archiv f. Physiolog, 1880, p. 33. ? Fano, ‘Das Verhalten des Peptons und Tryptons gegen Blut und Lymphe,’ Archiv f. Physiolog, 1881, p. 277. 8 Grosjean, ‘Recherches sur l’Action physiologique de la Propeptone et de la Peptone,’ Travail du Lab. de Physiologie de VUniv. de Litge, tome iv. 1891-92, Also Archiv. de Biologie, 1892, xi. p. 381. + 4 Hofmeister, Zeitschrift f. Physivlogis:he Chemie, 1881, p. 127. 728 REPORT—1898. arrived at, the earlier experiments (where the calculations are based on what I have called the ‘difference’ nitrogen of the whole second hour) are indicated by an asterisk :— TaBLeE VII.—Showing the Amount of Proteid excreted (expressed in Grammes.) Proteid N.+ | Per Period on Exp. Weight | Nitrogen] extractive raaihae Tae Fl rg cent, of | which Caleu- of Dog | injected | N. of 2nd tive N preneter Proteid lation is hour 5 excreted based I. Witte’s Peptone : not estimated, data insufficient. The same applies to Hetero-albumose. Il. Proto-albumose. Average 47 per cent. *XV. 1153 k.| °1565 *1372 0645 0727 46°45 One hour AVL |126 ,,| :1271 “0591 0076 0515 40°52 40 min, XX. /|12-7 = ,,| °1271 0785 0094 0691 54°37 45 min. | III. Deutero-albumose. Average (2) *XITI. | 19°75 ,,| -2012 1386 0250 1136 56°46 | One hour (urine contd. albumen) *XIX.|14 ~—,, | "1408 "1868 0159 1009 71:65 | One hour XXXII.| 63 ,, — — — — — Not as yet estimated IV. Ampho-peptone. Average 39 per cent. *V. (105 ,,[ +1483 0803 0123 0680 45°86 One hour *VI.| 8 ,,| °1342 0633 0206 0427 31°82 prac XXIX., | 119 ,,| °1618 0756 0125 0631 38°95 40 min V. Anti-peptone. Average 27°5 per cent. *VIII. | 8:2 ,,| ‘1427 0795 0344 0451 31°60 | One hour *XVIII.|16 ,,| -2283 1048 0306 0742 32°11 Bs - KXVIII} 11:3, | 1712 0518 0168 0350 20°44 50 min. XXX. | 81 ,,| 1156 "0417 0114 0303 26°21 45 | The average of amounts of excreted proteid are, for proto-albumose, 47 per cent. for deutero-albumose (not calculated); for ampho-peptone, 39 per cent. ; for anti-peptone, 27:5 percent. But even these averages are considerably too high, for two reasons : first, because they include experi- ments where the calculation is made on a longer period than the actual ‘ peptone ’-excretion period ; and, secondly, because it is fairly certain that the deduction made, for ‘extractive’ nitrogen, even in the later experi- ments, is too low. If we examine Table VI., which gives the effect of normal salt solution upon the output of nitrogen, we shall see that the augmentation caused by it is greatest in the second hour, and the same applies to urea. Consequently, it is believed that a much greater, probably twice as great, deduction might safely be made for the ‘ extractive ’ nitrogen of the excretion period in the peptone and albumose experiments. This would considerably reduce the proportion throughout, below that shown in Table VII. The experiments, therefore, would make it appear probable that ON THE PHYSIOLOGICAL EFFECTS OF PEPTONE. 729 peptones and albumoses are not wholly foreign substances to the circu- lating blood. This conclusion cannot, however, be pushed too far, since it is uncertain to what extent any given substance introduced into the cir- culation is again recoverable from the urine, nor is it certain how long the substances in question retain their identity after being so introduced. It is significant, however, in the light of Siegfried’s work, that anti- peptone remains in the system to a much greater extent than any of the other substancesemployed. Some of the experiments were performed with anti-peptone kindly supplied by Professor Siegfried, for which best thanks are here expressed. The research is still in progress. Fertilisation in Phceophyceee.—Report of the Committee, consisting of Professor J. B. FarMER (Chairman), Professor R. W. PHILLIPS (Secretary), Professor F. O. Bower, and Professor Harvey GIBSON. Tue Committee beg to report that they have again devoted the whole of the 15/. placed at their disposal to aiding Mr. J. Lloyd Williams in the prosecution of his researches on the Fucacee and Dictyotacee. Mr. Williams’s interesting discovery of the occurrence of motile antherozoids in Dictyota and Taonia was announced to the Botanical Section at the meeting at Toronto. A full description of these antherozoids has been published in the ‘ Annals of Botany ’ (December 1897). The following is a brief summary of the points to which Mr. Williams has been directing his attention more particularly :— (1) The Fertilization and Cytology of Ascophyllum and Fucus.—This investigation is in continuation of a joint research by Professor Farmer and Mr. Williams on these genera, the results of which are in course of publication in the ‘ Transactions of the Royal Society.’ (2) The Process of Fertilization in Halidrys.—Certain remarkable phenomena accompanying the act of fertilization have been observed in ipeeted Siliquosa, a description of which will appear in the paper referred to above. (3) The Zones of Growth and Periods of Maturation of the Sexual Products in Fucacee.—Mr. Williams has subjected all the species of Fucaceez in the Menai Straits to a careful and continuous examination, and his observations add greatly to our knowledge of what may be called the Natural History of these species. (4) The Examination of the Sexual Cells in Dictyota and Taonia.— The discovery of motility in the male sexual cells in these genera has already been referred to. Further, the process of fertilization has now been observed, the occurrence of parthenogenetic germination of the oospheres confirmed, and an interesting discovery of a marked periodicity in the maturation and liberation of the sexual cells in Dictyota has been made. Upon this subject the Committee are glad to learn Mr. Williams ain - submit a paper to the Section at the forthcoming meeting at ristol. Since the last meeting of the Association, Mr. Williams has been appointed Assistant Lecturer and Demonstrator in Botany at the Univer- 730 REPORT—1898, sity College of North Wales, Bangor, and he is thus favourably situated by residence at the seaside for the prosecution of the studies which he has on hand. The Committee would earnestly recommend the continua- tion of the grant for another year, and, convinced that interesting results will accrue to science as a result of Mr. Williams’s investigations, they would propose to devote it again to assisting him in his work. INTERNATIONAL CONFERENCE ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. ey 2h pernln So Fre Ae Ae = ( ; —— ALA MATTAWOAM INTERNATIONAL CONFERENCE ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. PRESIDENT OF THE CONFERENCE—Professor A. W. Ricxer, M.A., D.Sce., Sec. B.S. THURSDAY, SEPTEMBER 8. The President delivered the following Address :— Tue President of the Section of Mathematics and Physics has already expressed the pleasure with which British physicists welcome the distin- guished band of visitors who have assembled to take part in the Interna- tional Conference on Terrestrial Magnetism. None join in that welcome with more cordiality than those who are especially interested in the science with which the Conference will be occupied. To us it is a source both of gratification and pride that the International Committee, to whose action this meeting is due, should have allowed us to play the part of hosts to the eminent men from many lands who have responded to their call. Some whom we would gladly have seen here, but who have been prevented from attending by various causes, have nevertheless shown the interest which they take in our proceedings by sending written communications. Thus our meeting is as fully representative as we could have hoped. It may be interesting to those who are unaware of the fact if I remind the Conference that this is not the first occasion on which students of Terrestrial Magnetism have taken counsel together during a meeting of the British Association. Fifty-four years ago the then President of the Association, the Very Rev. George Peacock, Dean of Ely, stated in his address that the period was drawing to an end for which a series of magnetic observatories had been established by international co-operation. ‘Six observatories,’ he stated,' ‘were established, under the zealous direction of M. Kupffer, in different parts of the vast empire of Russia, the only country, let me add, which has established a permanent physical observatory. The American Government instituted three others, at Boston, Philadelphia, and Washing- ton ; two were established by the East India Company, at Simla and Sin- gapore ; from every part of Europe, and even from Algiers, offers of co-operation were made.’ The observations thus provided for were to be carried out for three years only, but, as nearly the whole of that time was spent in preparation, the period was doubled. When the term thus 1 Brit. Assoc. Rep., 1844, p. xliv. 704 REPORT—1898. fixed drew to an end, the question arose as to whether it was desirable to extend it further, and M. Kupffer (Director-General of the Russian System of Magnetic and Meteorological Observations) addressed a letter to Colonel (afterwards Sir Edward) Sabine, suggesting the propriety of summoning a magnetic congress to be held at the next meeting of the British Asso- ciation. Tn accordance with that suggestion the Congress was held during the meeting of the Association at Cambridge in 1845. The number of dis- tinguished foreigners who attended in person was considerable, in spite of the difficulties of travel fifty years ago. Amongst those who were present was M. Kupffer; Dr. Erman, of Berlin, the celebrated circumnavigator and meteorologist; Baron von Senftenberg, the founder of the Astronomical and Meteorological Observatory of Senftenberg, in Bohemia; M. Kreil, the Director of the Imperial Observatory at Prague; Dr. von Boguslawski, the Director of the Royal Prussian Observatory at Breslau; Herr Dove, Professor of Physics in the University of Berlin ; and Baron von Walters- hausen, a gentleman who had taken part in the magnetic observations of Gauss and Weber at Gottingen, and had executed a magnetic survey of portions of Italy and Sicily. In addition to these a number of well- known British men of science were invited to be present, amongst whom T need only mention the Marquis of Northampton (President of the Royal Society), Sabine, Sir John Herschel, Lloyd, Airy, Brown, and Sir James Ross, then recently returned from his celebrated expedition to the Ant- arctic Seas. Letters were also received from Wilhelm Weber, Gauss, Loomis, Lamont, Quetelet, Von Humboldt, and others. The principal question which this conference had to decide was whether ‘the combined system of British and foreign co-operation for the investi- gation of magnetic and meteorological phenomena, which [had then] been five years in progress, must be broken up.’' I will not trouble you with a recapitulation of the recommendations of the Congress, some of which have been carried out, while others have not yet been realised ; but one resolution will, I am sure, so exactly express your own sentiments that I venture to quote it, viz. : ‘That, the cordial co-operation which has hitherto prevailed between the British and foreign magnetic and meteorological observatories having produced the most important results, and being considered by us as absolutely essential to the success of the great system of combined observation which has been undertaken, it is earnestly recom- mended that the same spirit of co-operation should continue to prevail.’ Whatever changes half a century may have wrought in the problems which press upon magneticians, and in the difficulties which confront them, there can be no doubt that they are still of the same spirit as that in which this resolution was framed. It is true that we sometimes meet with the objection that interna- tional conferences of all kinds are now too numerous, and that their decisions, from their very number and complexity, cease to attract atten- tion or to command respect. Admitting that this objection is not without weight, it may be answered by two remarks. The closer union between scientific workers in different countries which these meetings encourage, the strengthening of the ties of intellectual sympathy by those of personal friendship, are in themselves good. It is surely a hopeful omen that science, as she reaches her maturity, forgets or ignores the political and 1 Brit. Assoc. Lep., 1845, p. 69. ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 735 geographical boundaries which sometimes seemed so important in her youth, and that workers for the common good are more and more learning that it is good to work in common. But there are special and cogent reasons why the science of Terrestrial Magnetism should be cosmopolitan. The advance of some sciences is most easily achieved by the methods of guerilla warfare. In a hundred different laboratories widely separated workers plan independent attacks on Nature. In different Universities and Colleges little groups are devising stratagems and arranging ambuscades in the hope of wresting from our great opponent some of the treasures which she yields only to the violent who take them by force. But for those who would unravel the causes of the mysterious movements of the compass needle concerted action is essential. They cannot, indeed, dispense with individual initiative, or with the leadership of genius, but I think that all would agree that there is urgent need for more perfect organisation, for an authority which can decide not only what to do, but what to leave undone. The advance of the science of Terrestrial Magnetism must depend upon the establishment, the maintenance, and the utilisation of the records of observatories. The bulk of the material to be dealt with must in any case be vast, and every needless addition to it, every obstacle in the way of its being readily comprehended and easily used, is a drawback which proper organisation should prevent. Thus it is wasteful to devote to the multiplication of observatories, in regions of which we know much, energy and funds which would be invaluable if applied to districts of which we know little or nothing. I take some credit to myself in that within the last few months I have assisted in checking well-intended but mistaken proposals to add to the number of the magnetic observatories which we already possess in this country. Again, it is desirable that the records of the observations should be so published as to be ready for application to the problems the solution of which they are intended to subserve, and that the individual worker should not be harassed by petty differences in the methods of presentment, which often entail on him labour too enormous to be faced. On this point something has already been done by international co-operation, and we may hope that this meeting will do much to complete the task. Lastly, there are many investigations which are now undertaken independently at irregular intervals which would be far more useful if planned in common. Thus, there has of late been a great outburst of energy in Europe devoted to magnetic surveys more detailed than have ever before been accomplished. Is it too much to hope that when the time comes for these to be repeated they may be carried out simulta- neously, and reduced by the same methods, so that we may have a mag- netic map of Europe in which no uncertainty as to the accuracy of details is introduced by the necessity for correcting for the secular change over long intervals of time ? Taking it for granted, then, that international co-operation is desirable for purposes such as these, I come next to the question of the nature of the machinery by which it shall be secured. And here I may at once state that the arrangements under which we are meeting to-day are in some respects abnormal, and that plans for the future will have to be formall or informally considered before we part. Meanwhile, it is desirable that I should state precisely the circumstances which have brought us together. 736 REPORT—1898. : The last meeting of the International Meteorological Conference was held in Paris in September 1896. It was attended by several men of science specially interested in Terrestrial Magnetism, and, perhaps on this account, a new departure was taken by the International Committee, in the appointment of a ‘Permanent Committee for Magnetism and Atmo- spheric Electricity,’ to which certain specific questions were referred. Eight gentlemen were nominated as members of this Committee, with power to add to their number. We in turn co-opted eight other mag- neticians, taking care that as far as possible all countries in which Terrestrial Magnetism is specially studied should be represented. About the same time, and, as I believe, in ignorance of the establishment of this Committee, a suggestion for the assembling of an International Conference on Terrestrial Magnetism was made in the Journal of that name by Professor Arthur Schuster. It appeared to me and to Professor Schuster himself that it would be a great pity if this suggestion resulted in the establishment of a rival organisation, and I at once submitted to the Committee the question whether, in their opinion, it was desirable that we ourselves should take the responsibility of summoning an Inter- national meeting, with the view of obtaining a wide discussion of the points submitted to us by the Meteorological Conference. This sugges- tion was approved, and, as the British Association was willing to allow us to organise the conference as a branch of Section A (Mathematics and Physics), to undertake the expense of sending out the necessary notices, to print our papers in its Report, and to extend to foreign members of the Conference all the privileges of foreign members of the Association, it was also determined that so hospitable an invitation should be accepted with the gratitude it deserved. But although the main result has been achieved, and a representative gathering of magneticians has assembled in Bristol, it cannot be denied that our relations to the various bodies with which we are connected are somewhat complicated, and that our consti- tution is devoid both of simplicity and symmetry. I take it that these facts are signs of health and vigour rather than symptoms of decay. Terrestrial Magnetism has been attracting far more attention of late years than in the not very distant past. The necessity for meeting, for common action, for common publication has been forced upon us. We have cared more for meeting than for the terms on which we were to meet, more for acting together than for drawing up an elaborate deed of partnership, more for the promotion of science than for a flawless paper constitution. Thus, and in my opinion most wisely, we have sought to attain our ends, not by starting a brand new International Association, but by making use of machinery which is already in existence, which has stood the test of time, and is, as I believe, capable of being put to new uses in meeting our wants and supplying our deficiencies. I confess, however, that in this arrangement we have been compelled to pay scant attention to the simplicity and even to the logical consistency of our schemes. We are an International Conference on special subjects —Terrestrial Magnetism and Atmospheric Electricity—summoned by a Committee owing its authority and bound to report to another International Conference of wider scope, which regards ‘our sciences as branches of Meteorology. On the other hand, this Committee is for the moment a part of the Com- mittee of the Section of Mathematics and Physics of the British Association, though it retains its right of separate meeting, more especially for the ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 737 discussion of its report to the International, Meteorological Conference. It is evident that here there is plenty of opportunity for collision between rival authorities, for confusion between conflicting jurisdictions ; but to all questions as to the precise limits of authority and jurisdiction it is sufficient to reply in the most general terms. The whole of the arrange- ments are temporary, to meet an immediate pressing need. The work of the Conference will be conducted like that of a Department of the British Association. The members of the International Committee will act as the Committee of the Department, but some of their work will be done on the General Committee of Section A, of which other magneticians will also be members. Should it be necessary, they will hold some separate meetings, and some such meetings will certainly be necessary to discuss their report to the International Meteorological Conference. These general regulations will probably suffice for all practical purposes. Tf cases occur which they do not cover, we must deal with them as they arise. With regard to the future, I do not propose to lay before you any detailed scheme, but in discussing the matter among ourselves the fol- lowing principles should, in my opinion, be adhered to. The International Meteorological Conference has held a number of successful meetings. I believe that I am correct in saying that the right to attend that Conference was at first confined to those who were officially connected with Meteoro- logical and Magnetic observatories, but that of late invitations have been more widely distributed. If the authorities of that Conference see their way to inviting in future most or all of those who are known to be specially interested in Terrestrial Magnetism, I do not see why the Magnetic Conference, which would then be constituted once in five years, should not meet all our requirements. If, however, additional meetings are necessary, I would urge that they should be held in turn in different countries, and, if possible, in connection with existing societies which play elsewhere the part taken by the British Association in this country. That a permanent committee should be established is essential, and the mode of appointing this body must no doubt be considered, but I hope that in the course of the next few days the committee may be able to discuss the whole question, and that when the next meeting of the Meteorological Conference takes place we may be able to lay before the Committee suggestions which may lead to the foundation of an Inter- national Magnetic Association on a stable and permanent basis. Another matter of great importance is the maintenance of an inter- national journal devoted to ‘Terrestrial Magnetism. This we now possess, thanks to the energy of Dr. Bauer, and I feel sure that all present will agree that such a means of intercommunication is invaluable. I believe, however, that the enterprise is threatened with financial dangers, and I desire to take this opportunity of urging all those who are interested in its success to do what they can to support it by increasing the circula- tion. There is every reason for making more use of a common journal. The records of the observatories are necessarily so bulky, that anyone who desires to obtain the facts as to the magnetic state of the earth at any given time must collect or consult a large library of quarto volumes, in some of which the magnetic facts are mingled with data interesting chiefly to the meteorologist or astronomer. It is no doubt essential that an account of all the work done at each observatory should be aaa in a collected form, and that full details of the magnetic : 3B 9 738 REPORT—1 898. observations should be given; but for many, nay, for most, purposes, those who use the records will require only final results; the means of the various elements for the year, for each month, or for any other period which may hereafter be adopted, and the diurnal variation, are in general wanted, rather than the hourly values. If these means could be published together, once a year, an enormous boon would be conferred upon mag- neticians. For special purposes the theorist will have to test his views by reference to the results published in their fullest detail; but it would be no slight gain if the more salient facts could be compared by being placed side by side in the same journal. One advantage such a system would unquestionably possess. It would impress upon the authorities of the observatories the necessity for adhering to a common form of publication. Some small beginnings have already been made. The Kew Observa- tory Committee now publish in the ‘ Proceedings’ of the Royal Society the annual means of the elements recorded by all the observatories which send their publications to Kew. By comparing two of these tables, the secular change can at once be determined. But the system is capable of extension, not merely to the normal values of the elements, but to disturbances. By common agreement, Greenwich and Pare St. Maur publish in each year the records of the same magnetic storms. If this agreement could be extended, and if the facts thus selected were brought into juxtaposition, we might hope for a fuller and more instructive analysis than is at present usual. Turning from questions of organisation, the primary business of our conference will be to discuss four questions submitted to our Committee by the International Meteorological Conference. The first two of these refer to the methods for calculating and pub- lishing the monthly means of the magnetic elements which should, in our opinion, be adopted. I will not anticipate the discussion which will take place on these points, except to say that it will be necessary to bear in mind not only what is desirable but also what is practicable in view of the resources at the disposal of the directors of the various magnetic observatories. Another question deals with the relative merits of long and short magnets, and on this point we shall have the advantage of hearing a report on the subject by M. Mascart. Lastly, there is a very important proposal for the establishment of temporary magnetic observatories at certain specified places. General Rykatcheff and Professor von Bezold present an excellent report on this subject, and I will only remind you, that whereas the accuracy of the mathematical expression of the magnetic state of the earth’s surface depends entirely on the number and position of the spots at which the magnetic elements are accurately known, the establishment of temporary observa- tories will be a costly undertaking, for the carrying out of which all the resources at the disposal of international science will have to be employed. Another point of considerable practical importance will also be brought before us. The rapid extension of electrical railways and tramways is a serious menace to magnetic observatories. From all parts of the world we hear of observatories ruined or threatened by the invasion of the electrical engineer, Toronto and Washington have already succumbed, Potsdam, Pare St. Maur, Greenwich, and Kew are besieged, and the issue largely depends upon whether these great national observatories can or cannot make good their defence. es ie _—— ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 739 It seems to be a law of Nature, ruling alike the human race and the humblest microbe, that the products of an organism are fatal to itself. The pessimist might infer that we are in presence of another instance of the universality of the application of this law, and that pure science is threatened by the very success of its practical applications. The smoke of our cities blots the stars from the vision of the astronomer, who, like the anchorites of old, flies from the world to mountains and desert places, It is only in the small hours of the morning when ‘Save pale recluse, for knowledge seeking, All mortal things to sleep are given,’ that the physicist can escape from the tremors of the trafic of a great town. Civilisation as it spreads by aid of the means that science has placed at its disposal is destroying records, and obliterating houndaries by the study of which the anthropologist and the biologist might have read far back into the history of our race. And now in turn the science of Terrestrial Magnetism, which, on the one hand, is forging another link to connect the sun and earth, and, on the other, is penetrating within the surface of the globe to depths beyond the ken of the geologist, is threatened by the artificial earth currents of the electric railway. That the crisis is serious there can be no doubt, but I will only antici- pate the fuller discussion which will take place by stating that magneticians, in common with the rest of the world, recognise the great benefit which electric traction confers upon the community at large. We are not so foolish as to desire to embark on a crusade against a great industrial improvement of which science may well be proud ; on the other hand, we must hold fast to the position that provision for the conveniences which are immediately appreciated by the public should be made with as little damage as possible to those studies which are not less for the ultimate benefit of the race. Had science, when the use of coal was introduced, been sufiiciently advanced to devise means for smokeless combustion, an evil which now in more senses than one darkens the lives of the inhabitants of our great towns might have been prevented from attaining its present gigantic proportions. We are now at the beginning of another industrial epoch, which may indeed, if power is transmitted from a distance on a large scale, brighten our skies, but which threatens to saturate the earth beneath us with electric currents. That these may interfere with the general comfort is evident from the injury which has been done to underground pipes at Washington and elsewhere. The construction of a powerful electrical railway in the immediate neighbourhood of the laboratories of a college would interfere with its efficiency, and make it impossible to perform experiments of certain types. In such a case, however, something could be done by arranging the experiments to suit the conditions under which they would have to be performed. But in the case of a magnetic observatory no such protective measures are possible. The very object of the observatory is to measure the earth’s field, and if that field is artificially altered no modifica- tion of the methods of measurement, however ingenious, can overcome this fundamental defect. I am glad to take this opportunity of acknowledging that both the danger to pure science and the necessity for obviating it have been acknowledged by those who are chiefly interested in the technical applications of science ; and in particular that one of the principal 3B2 740 REPORT—1898. technical journals, the ‘ Electrician,’ has supported the view that industry can and ought to respect the necessities of research. If, however, there be any who are inclined to ask whether the careful study of Terrestrial Magnetism has led or is leading to any definite results, or whether we are not merely adding to the lumber of the world by piling up observations from which no deductions are drawn, we may answer that, though the fundamental secret of Terrestrial Magnetism is still undiscovered, the science is progressing. In the presence of several of the most active workers I will not enter into a detailed discussion of the tasks to which they are devoting themselves ; I will only ask that the doubter should compare a good summary of the state of the science of Terrestrial Magnetism written fifteen or twenty years ago, such as that contained in the article by Balfour Stewart in the ‘Encyclopedia Britannica,’ with what would be written on the same subject to-day. Additions would have to be made to the descriptions of the instruments employed, to the discussion of the theory of the diurnal and secular change, while such questions as the reality of earth-air currents and the tracing of loci of local disturbance have only been dealt with effectively in very recenttimes. When, too, we compare the older models of the magnetic state of the earth with that devised by Mr. Henry Wilde we cannot but admit not only that a great advance has been made in forming a simple diagram of the magnetic state of the earth, but that it is possible that the model contains a very pregnant hint as to the physical construction of the earth as a magnetic body. The fact that Mr. Wilde has imitated the declination and dip with remarkable accuracy all over the surface of the earth by means of a simple arrangement of electrical currents, and by coating the oceans with thin sheet iron, has not attracted the attention it deserves. Whether the phy- sical cause thus suggested be due to the greater depth to which the under- ground isothermals penetrate below oceans, the bottoms of which are always cold, or whether the geological nature of the rocks is different below the great depressions and elevations of the earth’s surface, respec- tively may be open to question, but I am persuaded that the matter should be more fully investigated. Tn conclusion, let me once more revert to the points on which I dwelt at the beginning of this brief address. We meet with the confidence of men who know that their science is progressing, but with the mingled hopes and fears of those who still have to deal with the great unsolved problem of the causes of Terrestrial Magnetism and of its manifold fluctua- tions. This solution will be most easily attained if we are not merely content to collect facts, but if we so arrange that they shall be easily dealt with. To observe is our first duty, to organise our second, and if these be fulfilled we may hope that a theory of terrestrial magnetism will in the future crown the efforts not merely of him on whom the first glimpse of the truth may flash, but of the international co-operation which has, by way of preparation, made ‘the crooked straight and the rough places plain.’ ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 741 The following Papers were read :-— l. On the Relative Advantages of Long and Short Magnets. By Professor E. Mascarr.* [Ordered by the General Committee to be printed in extenso.] On employait autrefois des barreaux longs et lourds, sans doute par Vidée que les forces agissantes étaient plus grandes et que les résultats devaient étre plus sirs. Les barreaux de Gauss pesaient quelquefois plusieurs livres. La boussole de Gambey pour la déclination avait un aimant d’environ 50 cent. de longueur ; celui de la boussole de variations était encore plus long et les aiguilles d’inclination n’avaient pas moins de 25 cent. Depuis plusieurs années on a beaucoup réduit les dimensions des barreaux ; ce qui permit de rendre les instruments plus faciles 4 transporter, et je crois qu’au point de vue de la sensibilité on n’a fait qu’y gagner, comme pour le compas de Lord Kelvin. Considérons, en effet, un barreau de forme déterminée (tige a section rectangulaire, par exemple). Soient m la masse du barreau. p son poids. p le rayon de giration autour d’un arc transversal passant par le milieu. k = mp” le moment dinertie. M Je moment magnétique. Hla composante horizontale du champ terrestre. Désignons par les mémes lettres accentuées, m’, p’, p', k’, M’, les grandeurs correspondantes pour un aimant de méme forme dont la longueur est f fois celle du premier. On peut admettre que l’aimantation reste la méme dans les deux cas, quoique toute chose égale l’avantage restera encore pour diverses raisons aux aimants courts. On aura alors 1° Si les deux aimants sont suspendus 4 des fils sans torsion sensibl pour déterminer le produit HM, les durées d’oscillations ¢’ et ¢ donnent rapport CRYO PEM of 1) Mb a a) 35" a Sy cea) CA (1) tof 2° La torsion des fils de suspension n’est jamais nulle. Dans un fil unique la section s doit étre proportionnelle au poids du barreau (»! straction faite de l’étrier) ; par suite eee s 1 Question referred to the Permanent Committee by the Paris Meteorological Conference. 742 REPORT—-1898. D’autre part le couple de torsion c’est proportionnel au carré de la section aa Cums? Le rapport du couple de torsion au couple directeur magnétique est done (2) oY =e paride REN ge SM OHM £8 EM - , 3° Sil existe un frottement dans ]’appareil, comme pour les aiguilles montées sur pointe ou les aiguilles d’inclinaison dont les tourillons roulent sur des plans, le frottement est proportionnel au poids du barreau. Le couple directeur magnétique est lui-méme proportionnel au moment mag- nétique et, par suite, au poids. Tous les barreaux de méme forme sont done équivalents & ce point de vue. Sans aller plus loin, examinons les conséquences des équations (1) et (2). Il y a tout avantage a rendre les oscillations rapides. Si on veut les mesurer, l’opération est plus facile, sans avoir recours aux méthodes compliquées de Gauss. D’autre part, les oscillations ramortissent beaucoup plus vite et l’on n’a pas a craindre les variations de toute nature, telle que les déplacements du zéro, pendant la série des observations. La remarque s’applique encore mieux aux instruments de variations qui prennent sans retard et sans osciller la position qui convient a l'état actuel. Done supériorité des aimants courts. L’équation (2) montre aussi que le rapport du couple de torsion du fil au couple directeur magnétique est proportionnel au cube f? du rapport de symétrie et par conséquent du poids du barreau. Toutes les causes derreur qui entraine la suspension sont donc exagérées pour les barreaux lourds. On verrait de méme que les dimensions des barreaux ne jouent pas de role dans les expériences de déviation pour déterminer la valeur absolue de H, puisque les formules ne dépendent que du rapport des longueurs du barreau déviant et du barreau dévié. Enfin les causes d’erreur étrangére, telle que la présence de petits traces de fer dans l’instrument ou dans le voisinage, deviennent importants et impossibles 4 éliminer lorsque le moment magnétique et la distance des péles deviennent trop grands. A tous les points de vue il y a donc intérét a réduire autant que possible les dimensions des barreaux, si la précision des lectures d’angles reste suffisante. After considering this report the Permanent Committee passed the following resolution :—‘ Unless special reasons exist to the contrary, it is desirable that the dimensions of the magnets should be as small as possible, provided that the accuracy of the results is adequately maintained.’ 2. On the Construction of Magnets of Constant Intensity under Changes of Temperature. By J. R. Asuwortu, B.Sc. The paper describes experiments on a remarkable property of drawn steel wires. Magnets made of such wires, after a series of heatings and coolings, reach a cyclic state in which, contrary to general experience, an increase of temperature UBERSICHT ZUR ZEIT BESTEHENDEN MAGNETISCHEN OBSERVATORIEN. ZUSAMMENGESTELLT VON M. ESCHENHAGEN IN POTSDAM. 68% Report Brit. Assoc. 1898. Plate 6. ° @ OBSERVATORIEN OBSERVATORIEN. AE —— EN Bil Tersleatlerecs wad abscttes Mees Mocha Deane Qurmoat-Fersst, © Oude 1, Cap de cule Bets A Bk Fra ob Asst SRES PRESEN ENS REE PERSE GielebgewicbUlinien der Tigllcben Voulation des Erdmagns sms Tilustrating Paper by Professor von Bezold and General Rykatcheff on the Establishment of Temporary Magnetic Observatories in Certain Localities, especially in Tropical Countries, ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 743 produces an increase of magnetic moment, and decrease of temperature a decrease of magnetic moment. It is easy, by several processes which are described, to change this abnormal effect to the normal one, in which higher and lower temperatures produce lower and higher magnetic moments respectively. In passing from the abnormal to the normal state by any of these processes a stage is reached at which change of temperature neither increases nor decreases the magnetic moment, and, for changes within the atmospheric range of temperature, the intensity of such a magnet remains constant. An account is given of the behaviour at different times of magnets of constant intensity which have been tested at intervals during eighteen months. In conclusion, experiments on the cause of the abnormal thermo-magnetic effects are described. FRIDAY, SEPTEMBER 9. The following Papers were read :— 1. On the Establishment of Temporary Magnetic Observatories in Certain Localities, especially in Tropical Cowntries. By Professor voN Bezoup and General RyKaTcHeErFrF. [ Ordered by the General Committee to be printed in cxtenso.] [PLATE V.] Die nachstehenden Vorschlaige stiitzen sich wesentlich auf eine Abhandlung, welche der eine der Unterzeichneten im Jahre 1897 veréffent- licht hat.! In dieser Arbeit wurde versucht, durch Vergleichung mit den Beobachtungen die Hypothese zu priifen, dass die Krifte, welche die erdmagnetischen Erscheinungen hervorrufen, in der Erdoberflache selbst ein Potential besitzen ; auf Grund von Werthen, die ihm Herr A. Schmidt fiir je 72 um je 5 Langengrade von einander abstehende Punkte auf 4 Parallelkreisen mitgetheilt hatte, gelang der Verfasser zum Schluss, dass die in Procenten der Amplitude des Potentials ausgedriickten Abwei- chungen von jener Hypothese um den 40-45 Grad noérdlicher Breite am gréssten ausfallen, d. h. also gerade in jenen Breiten, fir welche die meisten und besten Beobachtungen vorliegen ; diese Abweichungen erreichen hier Werth bis zu 89% der Amplitude, wihrend sie in niedrigen Breiten nur wenige Beobachtungen vorhanden sind, viel kleiner sind theilweise sogar ganz verschwinden. TFiir die Theorie des Erdmagnetismus wiire es von héchster Wichtigkeit, dariiber Gewissheit zu erlangen, ob dieses Resultat nicht vielleicht durch den Mangel an Beobachtungen, besonders aus dem Aequatorialgebiete, bedingt ist. In derselben Arbeit hat der Autor auf Grund der von A. Schuster ? mitgetheilten Werthe eine Karte entworfen, welche fiir den Sommer ein anschauliches Bild vom Verlaufe der Gleichgewichtslinien des Potentials der taglichen Variation giebt ; die Darstellung der Karte bezieht sich auf den Mittag nach Greenwicher Zeit. Unter Annahme der Hypothese, dass die tigliche Variation ausschliess- lich und unmittelbar durch ein unverinderliches System von Kriaften ' Sitzungsberichte der K. Preuss. Ahad. d. Wissensch. zw Bertin, xviii. 1, April 897. * Philos. Transactions of the Royal Society of London, vol. 13), 744, REPORT—1898. hervorgerufen wird, welche die Erde umkreisen, wiirden alle auf dem- selben Parallelkreise belegenen Punkte auch die gleiche Tagesschwankung der Siid-Nord- und West-Ost-Componente des Erdmagnetismus besitzen. Dieses theoretisch abgeleitete Resultat wird durch die Beobachtungen zum Theil bestitigt ; doch liegen leider zu wenig Beobachtungen vor, um diese Frage endgiltig entscheiden zu kénnen. Ein Blick auf die Karte, von welcher eine Copie beiliegt, zeigt uns, welch’ eine hervorragende Rolle bei diesem Curvensystem die Parallelkreise 38 Grad nérdlicher Breite und 40 siidlicher Breite spielen, iiber welche die Aktionscentren fiir die tigliche Periode hinwegzuziehen scheinen, so dass es vom gréssten Werthe wire, sowohl aus den diesen Parallelkreisen benachbarten Breiten, als auch aus den zwischen beiden liegenden, d. h. aus den Tropengegenden geniigende Beobachtungen zu besitzen. Schliesslich wird in der citirten Arbeit auf die hohe Bedeutung hingewiesen, welche detaillirte bis auf die Secunde genau gleichzeitige Simultanbeobachtungen haben, die zu vereinbarten festen Terminen, wenn auch nur im Laufe eines kurzen Zeitabschnitts, anzustellen waren. Derartige Beobachtungen, wie sie auf Anregung von Herrn Professor Eschenhagen! im Jahre 1896 versuchsweise ausgefiihrt wurden, kénnen gleichfalls nur in magnetischen Observatorien gemacht werden, welche uber die ganze Erde vertheilt sein miissen. Aus diesen Griinden ware die Existenz einer Reihe von Observatorien und insbesondere unter den bezeichneten Breitengraden besonders wiin- schenswerth. Wenn wir aber die Vertheilung der bestehenden Observa- torien ins Auge fassen, die auf der Karte durch schwarze Punkte bezeichnet sind, so sehen wir, dass bloss in Europa ein hinreichend dichtes Netz von Observatorien vorhanden ist; in allen tbrigen Erdtheilen treffen wir eine deprimirende Oede an. In Bezug auf die erwahnten besonders interessanten Breitengrade geniigt die Bemerkung, dass im ganzen Aequatorialgiirtel zwischen 10° nérdlicher und 10° siidlicher Breite nur ein einziges Observatorium, dasjenige in Batavia, besteht, und dass ferner auf der siidlichen Halbkugel siidlich vom 35 Breitengrade gleichfalls nur ein Observatorium (in Melbourne) functionirt ; auf der nérdlichen Halbkugel existirt dstlich von Tiflis, zwischen dem 35 und 45 Breitengrade, auf einer Strecke von 100 Lingengraden kein einziges Observatorium, und ebenso ist weiter dstlich von Japan auf eine Entfer- nung von 140 Lingengraden auch kein Observatorium vorhanden. Fir die Untersuchung der erdmagnetischen Erscheinungen auf der ganzen Erde, fiir die Entwickelung der Theorie dieser Erscheinungen und fiir die Priifung der bisher aufgestellten Hypothesen ist es daher unumginglich nothwendig, dass die bezeichneten gegenwiirtig bestehenden grossen Liicken wenigstens fiir’s erste darauf heschranken, eine gewisse Minimalzahl, sei es auch nur tempordarer Observatorien, zu begriinden. Die Errichtung eines Observatoriums in Taschkent, die Wiederaufnahme der abgebrochenen Beobachtungen im friiheren russischen Observatorium zu Peking (resp. die Begriindung eines neuen magnetischen Observatoriums in Wladiwostok), sowie die Organisation von magnetischen Beobachtungen beim Lick-Observatorium wiirden die Liicken in der Reihe der magne- tischen Observatorien um den 40 Grad nérdlicher Breite erganzen ; im Aequatorialgiirtel kénnte die Begriindung von Observatorien in Quito, Paré, Colombo, sowie die Eréffnung der in St. Paul de Loanda und 1 Terrestrial Magnetism, vol. i. p. 55. ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 74 Dar-es-Salam bereits projectirten Observatorien den gegenwirtigen ungeniigenden Zustand verbessern. Auf der siidlichen Halbkugel miissten ausser den bereits projectirten Observatorien in Santiago de Chile und La Plata noch ein Observatorium am Cap der guten Hoffnung und ein anderes wo moéglich auf einer der Inseln St. Paul oder N. Amsterdam begriindet werden. Die Subkommission empfiehlt somit, ausser den bereits friiher projectirten, bestandigen Observatorien, sich. fiir die Begriindung folgender temporarer Observatorien zu verwenden : 1. Taschkent F : : 8 A . Russland. 2. Peking . : : : : : . China. 3. Lick-Observatorium : é : . Vereinigte Staaten N. A. 4. Quito. - ‘ : 5 6 . Ecuador. 5. Paré z : : 5 . . Brasilien. 6. Colombo. 3 . 2 : : . Anglo-Indien. 7. Cap der guten Hoffnung : 5 . England. 8. ‘St. Paul oder N. Amsterdam . ; . Eine der grossen Seemichte, z. B. Frankreich. Den hier aufgezihlten sollte sich wenigstens noch ein Observatorium in héheren siidlichen Breiten anschliessen, sei es auf den Falklandsinseln,, auf Kap Horn oder an einem anderen in diesen Breiten gelegenen Punkte. , Im Hinblick auf die Schwierigkeiten, welche die Errichtung gerade dieses Observatoriums bieten wird, schien es jedoch richtiger, keinen bestimmten Vorschlag zu machen, sondern zunichst nur eine allgemeine Anregung zu geben. After considering this report the Permanent Committee passed the following resolution :—‘ That it is desirable that temporary magnetic observatories should be established in places such as the following :—Taschkent, Peking, the Lick Ob- servatory, Quito, Para, Colombo, Cape of Good Hope, St. Paul or N. Amsterdam, Honolulu, and Point Barrow or Sitka, or some other station in a high latitude in North America. ‘That these observatories should, if possible, be provided with both absolute and variation instruments, of which the latter should be self-registering instruments, and should be established for at least seven, and, if possible, for eleven or twelve years, z.e., for a complete sunspot period.’ 2. The Application of Terrestrial Magnetism to the Solution of some Problems of Cosmical Physics. By Artuur Scuuster, /.R.S. In dealing with a subject in which a great part of the work is purely statistical, it is always advisable to keep in mind the real problems which form the ultimate: object of the statistical inquiry. It may be of interest, therefore, to the Congress to have a short summary of what I consider to be the most pressing questions of 7 physics on which the science of terrestrial magnetism may throw some ight. We know that the greater part of the magnetic forces which we observe on the surface of the earth are due to inside causes, but our information is barely sufficient at present to decide whether an appreciable portion, possibly amounting to 5 per cent. of the whole, may not have an outside origin. The outside forces must be divided into two different types, according as they are stationary in space or revolve with the earth. Stationary outside forces may be due to magnetic effects of the sun or moon, or generally to magnetic induction in that part of space. through which the earth moves. A magnetism fixed in space would give rise to a Variation haying the sidereal day for period, and if the force is of solar origin 746 REPORT—1898. there would also be an annual period. If the sun were transversely magnetised we should, in addition, have two periodicities, neither of which, as I have lately shown, is, as commonly supposed, equal to the synodical revolution of the sun, but one of which is equal to the period of sidereal revolution, and the other as much larger than the synodical revolution as that is larger than the sidereal period. Ina Presidential Address to the Royal Society(‘ Proc. Roy. Soc.,’ vol. lii. p. 305), Lord Kelvin made an appeal for the investigation of those periodicities which might be due to solar magnetism, But, on entering into the question, I find that it would be necessary to compare carefully the daily variations in the southern and northern hemispheres. At present we know too little of the movements of the magnetic needle in the southern hemisphere to attack the problem with success. I should consider it, therefore, a matter of the greatest importance to obtain comparisons in the daily curves on stations of approximately the same iatitude north and south of the equator. A few temporary observations at well-chosen places would be sufli- cient for this purpose. My investigations on the diurnal variation have led me to the conclusion that part of the effect is due to currents induced inside the earth, and the results seemed to satisfy the conclusion that the interior of our globe was a better conductor than the outer layers. But daily variations have also been observed in the earth currents which pass close under the surface of the earth, and it is doubtful at present how much of the observed daily variation is due to these earth currents. As the latter must be affected considerably by the nature of the ground, as regards its electric conductivity, it seems to me to be of interest to make observations at places not too far apart from each other on the same circle of latitude, and to compare especially the daily variations on small islands surrounded by sea with those on land stations. There, again, a short series of observations will be suffi- cient. The possibility of obtaining by means of the diurnal period information as to the electric conductivity of the interior of the earth seems to me to justify a closer investigation than the present data allow us to enter into. That component of a possible solar magnetisation which is parallel to the earth’s axis will produce a permanent effect, adding itself to the normal elements of terrestrial magnetism. Similarly, any magnetic forces which revolve with the earth, either because they have their origin in electric currents in the atmosphere, or because they are induced in space by the revolution of the earth, will produce permanent effects which can only be separated from the intraterrestrial causes by the analysis of spherical harmonics. Hence attention should be given to the gradual perfection of the calculations which, originated by Gauss, have recently been developed by Ad. Schmidt. But the first step towards the improvement in the analysis by spherical har- monics must be the definite answer to the question as to whether the whole, or nearly the whole, of the observed forces have a potential. As far as is shown by direct observations in limited regions on land, the line integral of magnetic force taken round a closed line vanishes, On the other hand, if the available observa- tions over the whole of the globe are collected, Ad. Schmidt has shown that a quite appreciable portion does not fit in with a potential. It might be thought that electric currents traverse the earth’s surface chiefly over the ocean districts or in the polar regions; but it seems almost impossible to reconcile the values obtained by Schmidt for these currents with the known facts of atmospheric elec- tricity. On the whole, it seems most probable that our measurements of magnetic forces over some of the ocean regions are affected by a systematic error. It seems to me that the whole science of terrestrial magnetism is almost at a standstill until this point has been cleared up. I believe that the greatest service that could be rendered to the science of terrestrial magnetism would be a magnetic survey over some line, passing as nearly as may be found possible along a circle of latitude round the earth. ‘Two lines, one in the northern and one in the southern hemisphere, would be better than one; but even leaving the southern hemisphere out of account, the question raised by Ad. Schmidt should be settled as soon as possible by a direct determination of the: integral line of magnetic force round the earth. ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 747 It is worth pointing out that a ship may do useful service to our subject with- out making a single magnetic observation. Ifa vessel was to start from Europe with orders to sail always at right angles to the direction of the magnetic needles, it would trace out an equipotential line and thus connect points of equal potential in the American continent and in Europe. The drift of the vessel, owing to wind and sea currents, would, of course, slightly change its course, and some corrections would be necessary, involving the approximate knowledge of the magnetic forces, which are probably known with sufficient accuracy for that purpose. If a suitable ship were to be found willing to enter on such an expedition, the value of the results would, of course, be much increased by more accurate mag- netic determination. A full discussion of the best available method for such determination seems to me to be called for, and it is probable that the beautiful marine galvanometer of Mr. Sullivan may be made useful for the purpose. Per- haps the Conference will initiate the appointment of a Cofmmittee to draw up a report on the subject. In conclusion, I may sum up the cosmical and terrestrial problems which we may hope to bring nearer their solution by magnetic observations :— 1. The possibility of magnetic induction of that part of space through which the earth is moving, either due to solar magnetisation or to some other cause. 2, The electric conductivity of space. 3. The distribution of electric currents in the atmosphere giving rise to the diurnal variation. 4, The distribution of electric currents in the atmosphere giving rise to per- manent magnetic force. 5. The electric conductivity of the interior of the earth. 6. The possibility of electric currents traversing the surface of the earth. 3. Antrag auf Massnahmen zur systematischen Erforschung der Saecular- variationen der erdmagnetischen Elemente. Von Dr. Ap. Scumipt in Gotha. Bei dem lebhaften Interesse, das man in den letzten Jahren wieder begonnen hat der erdmagnetischen Forschung zuzuwenden, ist zu hofien, dass die grossen Liicken unsrer Kenntniss von der raumlichen Verteilung der magnetischen Kraft in nicht zu ferner Zeit wenigstens einigermassen ausgefillt sein werden. Soll es indessen moglich sein, die zu erwartenden Messungen in vollem Masse auszuniitzen, so muss vor allen Dingen fiir eine hinreichende Feststellung der saecularen Aende- rungen gesorgt werden, ohne die (von ihrem selbstiindigen Werte ganz abgesehen) die Reduction der natiirlich iiber viele Jahre zerstreuten Beobachtungen auf eine bestimmte Epoche unméglich ist. Die Bestimmung der saecularen Variationen hat auch schon bisher stets die grésste Schwierigkeit und die Hauptquelle der Unsicherheit bei allen Darstellungen der erdmagnetischen Kraftverteilung gebildet, und dies wird, wenn nicht geniigende Vorkebhrungen zur Beseitigung des bestehenden Uebelstandes getroffen werden, in Zukunft immer mehr der Fall sein. Gegeniiber den gesteigerten Anforderungen an Genauigkeit, die wir heute stellen miissen und bei den verfeinerten jetzigen Messungen auch stellen kénnen, geniigt es nicht mehr, eine oft sehr ungleichartige Reihe von Messungen, die zufillig im Laufe der Jahre ungefihr an demselben Orte gemacht worden sind, zusammenzufassen und daraus—nicht selten durch Extrapo- lation— Werte der saecularen Schwankung abzuleiten. Und es macht sich immer empfindlicher merklich, wenn auf weiten Gebieten nicht einmal solche unvollkom- mene Messungsreinen vorhanden sind. Nach der jetzigen Lage der Wissenschaft miissen wir es als durchaus notwendig erachten, dass an einer nicht zu kleinen Zahl von Orien, die miéglichst gleich- miissig uber die Erde zerstreut sind, regelmiissig wiederholte Beobachtungen aller erdmagnetischen Elemente mit verglichenen Instrumenten und zwar stets genau an demselben Punkte angestellt werden, um den Einfluss von lokalen Stérungen auszuschliessen. 748 REPORT—1898, - Magnetische Observatorien sind dazu natiirlich keineswegs notig ; sie wiirden andrerseits, auch wenn ihre Zahl noch betrachtlich vermehrt werden sollte, nicht ausreichen. Fiir den bezeichneten Zweck geniigen, wenigstens bis auf weiteres, viel einfachere Vorkehrungen, die bereits einen grosseu Fortschritt gegentiber dem jetzigen Zustande darstellen wiirden. Wenn etwa an jenen Punkten, die man Saecularstationen nennen kénnte, von Zeit zu Zeit—etwa alle 5 Jahre—Messunger angestellt wiirden, so diirfte dies zunichst durchaus geniigen. Hs scheint mir eine der wichtigsten und dringendsten Aufgaben zu sein, Massnahmen zu beraten, die dazu dienen k6nnen, dieses Ziel zu erreichen, ohne aussergewohnliche Mittel, besonders in pecuniarer Beziehung, zu erfordern. Auf eine solche Massnahme mdochte ich besonders hinweisen, nimlich auf die wiinschenswerte Beteiligung der im Ausland stationierten Schiffe der Kriegsmarinen der seefahrenden Nationen— eine Beteiligung, die man bei dem grossen praktischen Interesse, das gerade eine zuverlissige Bestimmung der Saecularvariation fiir die Vorausbestimmung der erdmagnetischen Elemente besitzt, wohl schwerlich vergebens erbitten wiirde. Schon jetzt’ werden ja vielfach die Reisen dieser Schiffe u. a. gelegentiich zur Anstellung magnetischer Beobachtungen verwertet ; was hier gewiinscht wird, ist weniger eine starke Vermehrung solcher Messungen, als vielmehr eine planmiis- sigere und nach internationalem Abkommen geregelte Auswahl der Stationen und eine annihernd regelmissige Wiederholung der Messungen an geniigend vielen dieser Stationen, Gerade dieser letztere Wunsch ist ohne Schwierigkeit zu erfiillen, da die Schiffe der Kriegsmarinen auf ihren Reisen im allgemeinen immer wieder dieselben Punkte beriihren. Ohne dass die sonstigen Aufgaben, denen diese Schiffe zu dienen haben, beeintrichtigt wiirden, liessen sich daher an zahlreichen Orten— Hafenplitzen des Festlandes wie von Inseln—die gewiinschten Beobachtungen leicht gewinnen, etwa in der Weise, dass in einem mehrijihrigen Cyklus jeder Ort einer bestimmten Gruppe je einmal an die Reihe kiime. Ein international geregeltes Zusammenwirken der Marinen der verschiedenen Staaten wiirde dabei den Vorteil gewiihren, dass mit bestimmt begrenzten Mitteln méglichst viel erreicht werden kénnte, weil durch eine planmiissige Verteilung der Stationen die Arbeits- vergeudung vermieden wiirde, wie sie in einer zwecklosen Anhiiufung yon Beob- achtungen an identischen oder sehr nahe benachbarten Punkten lige. Es ist richtig, dass durch die im vorhergehenden vorgeschlagenen Beobach- tungen nicht allen berechtigten Wiinschen entsprochen wiirde, denn es wiirden dabei manche weitausgedehnte Gebiete keine Beriicksichtigung finden, so besonders die héheren Breiten der siidlichen Halbkugel. Aber es wiirde immerhin ein auf anderem Wege schwer zu gewinnendes, wertvolles Beobach- tungsmaterial zusammengebracht und dauernd ergiinzt werden. Die Unter- suchung jener abgelegenen, z.T. schwer zugiinglichen Gebiete miisste nach wie vor besonderen Unternehmungen vorbehalten bleiben. Auf Grund dieser, hier nur kurz angedeuteten, aber leicht weiter auszufiih- renden Betrachtungen erlaube ich mir den Antrag zu stellen: Das internationale Comitee mége— 1. Erwiigungen dariiber anstellen, wie die Gewinnung hinreichender Beobach- tungen zur fortlaufenden Ermittelung der Saecularvariation eingeleitet und dauernd gesichert werden kann ; 2. Insbesondere die hydrographischen Aemter der Kriegsmarinen aller see- fahrenden Staaten um ihre Mitwirkung dabei in der zuvor angedeuteten Weise zuersuchen, 4. On Simultaneous Magnetic Observations. By Professor Dr. EscuenyaGen. (Potsdam.) Under this head Dr. Eschenhagen gave an account of the results obtained at Potsdam by increasing the sensitiveness of the self-registering horizontal magnetic force instrument, till 1 mm. represented -000004 C.G.S. unit and 24 cms. one hour.! Under these conditions, well-marked waves of period about 30 seconds, 1 Sitz. Ber. Ahad., June 24, 1897. ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 749 and amplitude about ‘000012 C.G.S. unit, can at times be detected, and have been shown not to be due to any peculiarities of the instrument used. They occur generally between 6 A.M. and 6 p.m., but up to the present no direct effect of solar radiation on them has been proved. In the records taken at Potsdam and at Wilhelmshaven during 1895 they appear, within the limits of errors of observation, simultaneously ; but till more extensive observations have been made it is im- possible to say how far this may be general. Dr. Eschenhagen also gave an account of his further work on the frequency of occurrence of these small waves at Potsdam during the different hours of the day and the various months of the year, and exhibited curves embodying his results. He considered that these waves were of sufficient importance to justify the investigation of them being taken up by all observatories, and suggested that similar self-registering instruments should be used at all stations, and that both the north and west components should be recorded. 5.! Discussion on Monthly Means. M. Moureaux described the results of determining the monthly mean declina- tion by the various methods which have been used by magneticians. The results obtained differ considerably from each other, in two cases by 14 per cent. He considered that two means should be calculated: the first by taking all days into account, the second by taking only undisturbed days. Messrs. Rykatcheif, Mascart, Eschenhagen, Schuster, Snellen, Riicker, and Schott took part in the discussion which ensued. After the discussion the following resolution was passed by the Permanent Committee :—‘In calculating monthly means all days are to be taken into con- sideration. It is desirable to give in addition means calculated without taking disturbed days into account.’ 6.' A discussion was held as to the publication of the differences between the hourly means of the components of the magnetic force (X,Y,Z) and the monthly means. After the discussion the following resolution was adopted by the Permanent Committee :—‘It is desirable to publish the monthly means of the Geographical Components of the Magnetic Force for each month, and also the differences between the hourly means for each month and the monthly means for that month.’ 7. On Magnetic Observations in the Azores. By ALBERT, Prince of Monaco. After having perceived the capital importance of the Azores, from their geographical position, for the establishment of meteorological observatories with a view to weather predictions, I thought that these observatories might be of service to other branches of science. For instance, the communications of Messrs. Neumayer, Mascart, von Bezold and other eminent meteorologists, to the Inter- national Conference of Meteorologists in 1896 show that magnetic observations made at the Azores would offer the following advantages: (1) a situation near latitude 40° N. (page 22). (2) Remoteness from the permanent causes of perturba- tion of actual magnetic observation, such as electric lighting, tramways, and other applications of electricity ; and (3) a geographical position intermediate between Europe and America, capable of furnishing most useful indications for the comparison of the magnetic curves obtained in these two parts of the world (pp. 36 and 90). _, The examination of these considerations and different interviews which I had with M. Mascart, Director of the Bureau Centrale Météorologique of France ? Question referred to the Permanent Committee by the Paris Meteorological Conference. 750 REPORT—-1898. convinced me of the advantage which would be gained if Captain Chaves, Director of the Meteorological Observatory of Ponte Delgada, came to Europe to study the practical details of the magnetic service there. I therefore communicated my ideas to the Portuguese Government, who recalled Captain Chaves to undertake a mission in this sense. Captain Chaves, after having finished his studies at the observatory of St. Maur under the enlightened direction of M. Moureaux, has pointed out to me the importance of taking the present opportunity of magnetically reconnoitring the archipelago, as a preliminary to the definitive installation of the observatory. This would be useful, not only to determine the value of the different magnetic elements, till now almost unknown,! but besides, to determine in the island of St. Michael, which appears likely to present conditions favourable to the installa- tion of the central observatory of the Azores, the locality most suitable for the combined services of meteorology and magnetism. Feeling certain that the views of Captain Chaves are just, and well knowing his competence, being also aware that the Portuguese Geodetic Commission finished last year the survey of tke island of St. Michael, and that this year it will finish the survey of the neighbouring island of Santa Maria, I have resolved to under- take the charge of the above-mentioned magnetic reconnaissance. With this end I am now having the necessary instruments constructed; and I announce to the International Commission that I hope to be able to put Captain Chaves in the position to be able to commence the magnetic reconnaissance of the Azores towards the month of April of next year. 8. On Magnetic Observatories in Cape Colony. By Dr. BEATTIE and Mr, Morrison. 9. Sur le Mouvement diurne du Péle Nord d'un Barreau Magnétique suspendu par le centre de gravité. Par J. B. CAPELLO. [PLATES VI.-VIIL.] En combinant les variations diurnes de l’inclinaison avec celles de la décli- naison, sur un plan perpendiculaire 4 la direction de linclinaison, résulte une courbe fermée. Les variations ou écarts de l’inclinaison sont positives vers le sud, et celles de la déclinaison positives vers l’ouest. Il faut avertir que les écarts de la déclinaison doivent étre multipliés par le cosinus de V’inclinaison, afin de les projeter sur un plan perpendiculaire & la méme inclinaison. Il est intéressant de comparer ces courbes obtenues en divers points ou stations du globe. Ta 1&e Planche contient les courbes de Kew, Paris (Parc St Maur), Perpignan et Lisbonne en 1894 et 1895. Les courbes de Kew et de Lisbonne sont déduites des jours tranquils (cing jours choisis & chaque mois), celles de Paris et de Perpignan sont déduites de teus les jours. i Qeme Planche contient les courbes de Lisbonne et de Kew de 1896; de St Pétersbourg (1873-85) et des jours dits normaux, et celle de Lisbonne de 1864-72, excepté les perturbations, d’aprés la méthode du Général Sabine. La 8*me Planche contient les variations diurnes du Bifilaire, du vertical et de V'inclinaison 4 Lisbonne et Kew, 1894-95-96, 1 In fact, even the value of the Declination, one of the most important magnetic elements, is given for one and the same place, Horta in Fayal, with differences amounting to 1° 22’ in an interval of two years. Thus Preston in 1889 gives 26° 52° and the Acorn in 1891 gives 24° 30’. a — Plate 6. Lusborie 189 4 Planthe ae endu par le centre de gravite.’ Nbservatory of & inted out to _ alls reconasitis te of the obser, re resolred ts m able to pat Casi recommaissite od by Dr. Barn rrean Mognige CarELLo. sc celles de ls dei Linaicon, résiie Se rs To end, et cols étre romltiplits pe vodicalaire i le >= ors paints oa rast S* Maar), Peas 65% Report Brit. ¢ Kew 1834 Paris 1834 Popignan 8394 Lisbonne 183% Popignan O95 Kew 1895 Paris 1895 Ohague dnisite- 7 Ilustrating M. Capello's Paper ' Sur lo Mouvement diurne du Pole Nord d'un Barreau Magnétique suspendu par le centro de gravite. Plane ere Plate 6, 68% Report Brit. Assoc. 1898. Plate 7. JSC Letersburg [673-65 Lisbonne J8I6. Lusboramve 1864-72 Plance 2eme Illustrating M. Capello’s Paper ‘ Sur le Mouvement diurne du Péle Nord d’un Barreau Magnétique suspendu par le centre de gravité.’ 68 Report Brit. Assoc. 1898. Plate 8. Kew Lisbonne /m. = 00000136 cg.s. /mim-=0:°0668. Planche 3eme. | Illustrating M. Capello’s Paper ‘ Sur le Mouvement diurne du Péle Nord d’un Barreau Magnétique suspendu par le centre de gravité.’ ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 751] Retournant @ la 1° Pl. on remarque que les courbes des observatoires plus au nord sont plus rondes que celles des autres situés plus au sud. _ Ainsi, Kew de 1894 et 1895 affectent Ja figure elliptique; ensuite vient Paris avec la forme plus allongée; Perpignan encore plus étroite et mince du coté de Youest, et finalement Lisbonne, dont les courbes sont plus larges du cété de louest, et minces de lest, affectant la forme d’un oo. On voit un autre fait plus remarquable. Tandis que dans les courbes de Kew, Paris et Perpignan le mouvement vers Y’ouest, du matin au soir, est par le sud du point moyen, & Lisbonne il est par le nord, de facon que le mouvement est rétro- grade en regard des autres, Pour mieux faire ressortir cette circonstance, nous avons dans la 2°™e P], donné les courbes de Kew et de Lisbonne pour l'année 1896. Le mouvement & Kew est direct (selon les aiguilles d’une monire) ; celui de Lisbonne est invers. Nous avons vu (1*° Pl.) que la partie de la courbe du soir se déplace vers le sud, au fur et & mesure que la latitude est plus petite; on peut dire qua Lis- bonne Je déplacement est si grand qu'il traverse la courbe du matin. Il est facile de reconnaitre que les courbes plus ou moins rondes et le mouve- ment direct ou inyers dépendent de la valeur diurne ou des écarts de V’inclinaison. En effet, si la variation diurne de V’inclinaison est positive dans les heures du jour (9a.—2p.) le mouvement sera direct, et au contraire sera inyers si elle est négative dans les mémes heures. 4 Les écarts de Vinclinaison 4 Lisbonne sont négatifs dans les heures (10a,—2p.) au contraire de ceux de Kew, Paris, ete. Mais la variation diurne de l’inclinaison dépend des deux variations, ou des écarts des deux composantes H et V, comme i] 6V 6H Mi adds Dans la 3°™° PJ. on voit les variations diurnes des composantes H, V, et inclinaison & Kew et Lisbonne, d’aprés les cing jours calmes de chaque mois, dans les années de 1894-95-96. On voit que les valeurs des écarts de H & Lisbonne sont plus petites que la moitié des mémes écarts 4 Kew, et que, au contraire, les écarts du vertical sont plus grands que le double de ceux de Kew; quoiqu’ils aient le méme signe, le résultat est de changer le signe des écarts de l’inclinaison 3 Lisbonne aux heures du jour (9 ou 10a.—2p.). Afin que la forme de la courbe de Lisbonne soit semblable 3’ celle de Kew, il faudrait, du moins, doubler les variations de H, et réduire & la moitié celles de V. Nous avons fait V’expérience, et il a résulté effectivement une courbe trés semblable a celle de Kew, avec le mouvement direct &c. On pourrait ainsi attribuer ces différences aux valeurs de K, de H et de V, c'est-d-dire, & la mauvaise détermination de ces coefficients 4 Lisbonne, mais on ne doit jamais croire qu’on puisse commettre des erreurs si grossiéres, surtout en con- sidérant qu’il s’agit des différentes déterminations pendant une période de 85 années. Le but nord d’un aimant suspendu par le centre de gravité, et par un fil sans torsion, devrait décrire sur un plan perpendiculaire 4 leur direction une courbe égale ou trés semblable & celles des 12° et 2’me PJ, Un barreau magnétique cylindrique et ereux devrait étre suspendu par le centre de gravité, muni de lentilles ou de miroirs, de fagon que tous les mouvements seraient enregistrés sur un papier photographique placé sur un plan perpendiculaire & la direction de Vinclinaison, et ce papier devrait étre disloqué rapidement & la fin de chaque heure par une certaine quantité, afin que les traces ne seraient en- est facile de voir, d’aprés la formule 6i = sin? cos? ( brouillées. Je pense qu’un instrument semblable serait difficile 4 construire, surtout en conséquence de la petitesse des mouvements, mais il pourrait faire de bons Services 4 la science du magnétisme terrestre. Vo2 REPORT—1898. SATURDAY, SEPTEMBER 10. The Conference did not meet. MONDAY, SEPTEMBER 12. The following Report and Papers were read :— 1, An Account of the late Professor John Couch Adams's Determination of the Gaussian Magnetic Constants. By Professor W. Grytis ADAMS, F.R.S. See Reports, p. 109. 2. On a Simple Method of obtaining the Expression of the Magnetic Potential of the Earth in a Series of Spherical Harmonics. By ARTHUR Scnuster, /.2.S. The methods which have been employed so far to represent the earth’s magnetic potential in a series of spherical harmonics suffer from the serious defect that the different coefficients are not determined independently of each other. Thus, in the latest and most accurate computation of Adolph Schmidt, the value of the first and largest coefficient was found to be 1,872, 1,918, or 1,921, according as the expansion is supposed to end with terms of the third, fifth, or seventh order respectively. If the value of the potential were known at all points of the earth’s surface, it is well known how by a direct integration over the surface of the sphere each coefficient may be separately determined. But there are large tracts of the earth over which the magnetic forces have not been directly observed, and hence some form of interpolation is always implied in whatever method is employed. A certain amount of uncertainty results from this interpolation ; but perhaps less than is commonly supposed, owing to the fact that neglecting magnetic masses actually situated in the surface, the potential, and all its different coefficients must be continuous. A complete knowledge of the potential over any finite part of the earth’s surface is therefore theoretically sufficient to fix it all over the globe, and, at any rate, the continuity of the potential and of its derivatives facilitates and justifies the process of interpolation. The whole interest of the expansion in a series of spherical harmonics centres round the first few coefficients. It would be waste of labour to obtain a complete representation of the potential, as we know that a very large number of terms would be necessary for the purpose. The sole object of the expansion can only lie in the separation of the outside and inside forces, and for the present, at any rate, our interest in the outside forces must be confined to the first few terms, Hence I consider it a matter of great importance to obtain these terms separately in such a way that their value does not depend on the number of terms which are taken into account. I believe that the following method solves the difficulty. I write P,, for the zonal harmonic, T,” for the tesseral harmonic defined by P & yA" T,,” =sin’ 6 aa where 6 is the colatitude and p= cos 6. If it be required to represent a function, V, of 6 and the longitude X, in a series of spherical harmonics, it is known that the coefficients will depend on integrals of the form [VIy" cos od do, « being a surface element. The method I propose depends on a transformation ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 7953 which will allow the aboye integral to be expressed as a finite sum of integrals having one of the forms: | . Vcos pé cos od dédn, o Jo or | ib V sin pO cos oa dOdx. o Jo In other words, if V is expressed in a series the terms of which are of the form cos p6 cos oA or sin pé cos oA, and if equations are obtained once for all to give cos pé or sin pé in a series of tesseral harmonics, the problem of expansion is solved, though the independence of the hicher and lower terms is not necessarily secured. The first step of the procedure which is common to all methods consists in expressing V in the form a = : V=H,)+F, cosd+F, cos 2A+ ...) 1) +F/ sn vr+F,/ sin 204-05. force 7 : ( where F and F’ are functions of the colatitude. If V is given discontinuously ; as, e.g., if it is known at the points of intersect:on of a number of latitude and longitude circles, each latitude circle will give an equation of the above kind. If the number of such equations is sufficient, the values of F and F’ may be plotted in terms of 6, and by calculation or mechanical integration we may obtain the values cf F and I” either as a series FF, =a,+a, cos@+a,cos26+ . : : : (2) or in the form F, = 6, sin 6+6, sm 26+ . A : : : (3) Only one of these forms is useful for our purpose, as I proceed to show. If o be even, T,” may be expressed in the form of a finite series of the form T° = @, cos nO +a, cos (2—-2)O+ ... Hence, if « be even | T,,” cos p6d6=0 if p>n; : 0 and the integral will also vanish if p+ is an odd number. It follows that for 7 even +1 f C) | At, sin pOdp=3| T,” [cos (p+ 1) 4—cos (p—1) 6] dd = 0 =0 if p> x or if (p +7) is an even number. It follows that (o even) we may obtain a number of series in which the sines of multiples of @ are expressed, as in the following scheme, where the numerical coefficients are left out for the sake of simplicity :— sin 6 ail Bea Weve sin 26 =TigtTast . sin 6 Sige Tigh esis rv) sin (o + 1) d= er ate sin p6 = Tota tiges: + <= Whenever p is smaller than o the series begins with the term T,’or T,\, according as p be odd or evén ; but when p is larger than o the series begins with 1898, 36 754 REPORT—1898 If, therefore, F, be expanded in a series of sines, as indicated in (3), the sine functions may by (4) be expressed in tesseral harmonics, and each coefficient of 2 Z a coefficients of the sine series if m is even, and on oa coefficients if 2 be odd. Thus, the first coefficient, which is of the third degree, only requires one coefficient in the series of sines, and will be independent of all the others. For the simplest. case o=0; equations (4) resolve themselves into the well- known ones: T,,’ in the final representation of V will only depend on 4. 5 9 ~ sin 0=Py— 5 em Po Taus ie Boog op, (p28 pee — ain 28=8P, qPs 198 12h ee - ° ° . . e (5) 32 .. 45 aan 36 =5P, me P, 64. 77 5, sin 40=7P,- 7 P, Hence, to expand a function into zonal harmonics, we may, if chief attention is to be directed to the first few terms, express it in a series of the sines of multiples of 6, and substitute the above values, P, only occurs in the first equation, P, only in the second, P, only in the first and third, and so on. We may show in a similar manner that if o is odd, we must use (2) (the cosine form of the series) for F,. For the expansion of T ’ sin 6=sin7* a"Pn du? =@n41 C08 (n+ 1) O+a,-1cos(n—1)O6+ ... leads to the conclusion that 1 eae cos péduz =0 when p>n+1 and when p + 2 is even. We find thus for ¢=1 . =sT/+i T,’ + ee aks = coy = T+ ae T cos 20 = —8T,'+ 5 Ty’ + a 4.d0c ee ae Ge % cos 38= — 5T,' + os se er a cos 40= — 70,4 Te where T,’ will only occur in the first and third equations; ae generally a term n+ of degree will occur in 5 equations if 2 be even, and in > equations if x be odd. In the case of the magnetic potential the quantities which are directly observed are the forces which are connected with the potential V by the relations dV . dV Sa é Sls . ° e ° . 7 7 Y sin8 a (7) the radius of the sphere being, for simplicity’s sake, taken as unity. ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 755 {X =force to north; Y=force to west; \ =longitude measured eastward. | If Y sin 6 be expanded in a series of surface harmonics the potential V will be obtained immediately in a similar series; but somewhat difficult complications arise when V is to be obtained from the series for X. his ditticulty completely disappears in the method here proposed, for X being expressed in a series of circular function, we may integrate with respect to 6 without changing the nature of the series. The process to be employed may be summed up as follows :— Express both X and Y in the form— X=X,+X,cosk+X,cos2\+ ... +X,/sinh+X,’ sin 2A+ . Y=Y, cosd+Y, cos 2A+ ... + Y,’ sind + Y,’ sin 2A + and further express X, and Y. in Fourier’s cosine series for even and in the sine series for o odd. If V is then calculated by either of the equations (7) and the substitutions, or (5) or (6) of the corresponding equations are performed, the potential will be expressed in a series of spherical harmonics. The values of X and Y are not known in the polar region, but must be obtained by interpolation. The term zzterpolation is the appropriate one because the value of X, and Y, are known at the poles, vanishing there except for Y,. Also the first o differential coefficients of X, and the first s—1 differential coefficients of Y, will vanish at the same points. The value of Y, and Y,’ is very approximately known at the a previous investigations, and also its first differential coefficients will vanish. I have not taken account of the possibility of earth currents traversing the surface of the earth in sufficient intensity to affect magnetic forces. The investi- gations of Adolph Schmidt have shown how the problem must be treated when their influence has to be taken into consideration. ‘The general method of expansion here suggested wi!l remain the same. 3. On Magnetic Observations at Funafuti. By Captain E. W. Creak, &.N., RS. 4. On the Relations between the Variations in the Earth Currents, the Electric Currents from the Atmosphere, and the Magnetic Perturbations. By Seri Lemstrém. ; The paper contains an historical sketch of the observations and researches made on the earth currents by Lamont, Airy, Wild, Blavier, and others. The author describes the method employed by him for measuring the electromotive force of the electric currents coming from the atmosphere, and gives the evidence of the fact that the variations of earth currents occur a short time (five minutes) before the magnetic perturbations, and that the former are more numerous than the latter. From the observations in Sodankyla it is, however, proved that all magnetic perturbations are not preceded by variations in the earth currents, but that these probably are caused by electrical currents from the atmosphere to the earth, or vice versa. The proofs of that conclusion are: (1) That the magnetic perturbations in polar regions have a contrary direction to those in more southern countries; (2) That at _ the times of auroras the electrical curreut from the atmosphere varies much, and must exert on magnetic instruments a marked influence depending on their position, _ relative to the space within which this current is moving. It follows from this that we cannot find the causes of the magnetic variations, or, rather, perturbations, before we have investigated the earth currents and the electrical currents in the ‘atmosphere, The author’s experience shows that we must seek the key to these relations in 302 756 REPORT—1898. the polar regions. Researches have shown that the magnitude of these variations of the earth currents increases with the latitude in a very high ratio. When the diurnal variation in Pawlowsk has a value of O, 0008 volt, it rises in Sodankyla (7° more to the north) to O, 0600, or 75 times more. Moreover, we find from the lately published third volume of the observations from the international polar stations at Sodankyla and Kuttala that the earth currents as well as the electric currents in the atmosphere depend intimately on the belt of the maximum polar light. It will be very clearly seen that we also have a maximum belt of the earth currerts and even of the currents in the atmosphere. The paper finishes with a proposition that the International Conference on Terrestrial Magnetism and Atmospheric Electricity should discuss the two following questions: What signifi- cation must be attributed to the earth currents and the electric current from the atmosphere in the explanation of the causes of magnetic perturbations? What is to be done for the further iavestigation of the connection between the magnetic perturbations and the electric currents ? The author also proposes that the International Conference should take steps for establishing two international polar stations, one in the North of America, the other in the North of Europe, both situated in the southern border of the polar light maximum belt. In connection with both these principal stations there should be a northern by-statior, in which, us well as in the principal stations, all the magnetic variations, the earth currents, and the electric currents from the atmosphere, besides all meteorological observations, should be made simultaneously, and with self- registering apparatus of the best construction, the details of which ought to be stated by the International Conference. In connection with these observations it ought to be expressed as desirable that all magnetic observatories should, if possible, establish similar observations with as identical instruments as possible. Since the researches of the electric currents from the atmosphere require points elevated about 400 m., it seems difficult to unite these observations with those in an observatory. We, however, must remember that the electrical resistance in the circuit, from the earth to the atmo- sphere, is so great that one can put in several miles of wire without any sensible augmentation of it. It is well understood that the mountain on which an apparatus for out- or in-streaming of electricity is placed can without serious damage be far away from the observatory. 5. On the Interpretation of Larth-current Observations. By Artuur Scuuster, /.R.S. If two metallic plates are inserted into the ground and connected by a wire an electric current is found to traverse the conductor, and this is generally called the ‘earth current.’ It is not, however, obvious at first sight what the connection is between this observed current and that which traverses the ground when the earth plates are removed. The statement sometimes made, that the observation gives the difference of potential of the earth at the two points at which the plates are inserted, would be true, provided the connecting wire has a sufficiently large resistance, if earth currents were only due to chemical or thermo-electric forces. But as there can be little doubt that earth currents are chiefly, if not entirely, effects of induction, a separate investigation is necessary as to the interpre- tation to be attached to the galvanometer indications. Let A and B be two points in a line of flow of the currents traversing the earth, and consider a tube of flow passing from A to B. The specific resistance of the ground being p, let p be changed to p’ for the material enclosed by the tube. 1 determine in the first place the effect of this change of resistance on the distribution of currents. The change of resistance could be counterbalanced by an electric force—(p—p’) u acting throughout the tube, where w is the density of the undisturbed currents, and it is therefore equivalent to the introduction of an electromotive force |e--) udl in the tube of flow, d/ being an element of its length and the integration being extended from A to B. If and u are constant PR 4: ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 757 within the tube, the additional current flowing through it, owing to the change of resistance, will be (p—p') ul R+5 where R denotes the resistance of the tube, and S the resistance of the ground between A and B. If the resistivity p’ is of the order of magnitude of that of copper, it will be small compared to p, and may be neglected in the above expression. Imagine now this tube of flow between A and B to consist of two overlapping tubes, one of material equal to that of the rest of the ground, the other of copper, and let the latter tube be lifted out of the ground without altering its total resistance, but keeping its connection at A and B. The current traversing the lifted-up part will remain the same as before, provided that the electromotive forces of induction are not sufficient to produce an appreciable current in a circuit made up of the original and displaced position of the tube, a condition which will be satisfied in the case of earth currents, except perhaps at times of great magnetic storms. We have now an arrangement equivalent to that used in earth-current observa- tions, for the only effect of the earth plates at A and B will be to diminish the earth resistance S. The observed current 7 will be connected with u by the relation me pul ? R+5 The resistance R+S is measured by the introduction of an electromotive force e in the circuit; if the observed current, under these circumstances, be increased by a quantity 2’, the equation ree! piv’ will give the current density of the earth current. It is seen that w is proportional to the conductivity of the material of which the ground is made up, and that a knowledge of that conductivity, which may vary from day to day, according to the amount of moisture contained ia it, is therefore essential to a correct inter- pretation of earth-current observations. If the circuit is a long one, S may be smell compared to R, and the latter , quantity will be pe , a being the cross section of the wire, so that a we £4 2s ap which shows that the current densities in the wire and ground are in the propor- tion of their conductivities. _ The above investigation pcints to the importance of measuring the conductivity of the ground wherever earth-current observations are made. Samples of the soil taken from different depths would probably give different results, and would then indicate how the current density varies with depth. 6. On the Construction of Magnetic Observatories. By Dr. SNELLEN. A magnetic observatory should fulfil the following purposes. As it is desirable that regular observations be made in many places of the absolute values of the magnetic elements, a base-station is required for the reduction of observations. Also it is desirable to observe continuously regular variations of these elements. And, finally, there ought to be facilities for carrying on researches connected with magnetism in general. A combination of two observatories, one for absolute measurements and another for observing and recording continually the variations of the earth’s magnetism, will fulfil these conditions. It is desirable to have them in separate buildings. 758 REPORT—1898. Both should be constructed of non-magnetic substances; this 1s a necessity both for metallic connecting pieces and for the stone or other material of which the building is constructed. Another condition is that temperature variations should be reduced as much as possible, especially in the vaiiation observatory. All materials employed for the construction of the magnetic observatories at De Bilt, near Utrecht, in the Netherlands, have been subjected to a most rigorous examination as to their magnetic condition before they were accepted for the buildings, The observatory for absolute measurements consists of two rooms, one built of stone and wood, the walls being double, and the interstices filled with sawdust. It contains six pillars for making absolute measurements, at a distance from each other of four metres, to enable comparisons of instruments and methods to be made. It has no windows except in the ceiling, one above each of the pillars. The other room, of smaller dimensions, has large windows on three sides for making astro- nomical observations. The observatory for variation observations consists of two rooms, wholly sepa- rated from each other and surrounded by a corridor. The whole is enclosed in a building which has double walls, 1:60 metre thick, the interstices of which are filled with loose dry peat moss, &c. Daylight is not admitted into this observatory. Diurnal temperature variations are by these means wholly excluded. TUESDAY, SEPTEMBER 13. A joint meeting with Sections A and G was held for the purpose of discussing the Magnetic and Electrolytic Effects of Electric Railways, at which the following Papers were read :— 1. On the Disturbance of Magnetic Observatories by Electric Railways.' By W. von Buzoup, Director of the Potsdam Observatory. The demand of the authorities of the Potsdam Observatory that no electric railway with an earth return should be allowed to approach them within 15 kilo- metres having been characterised as exorbitant, the author states in this paper some of the reasons which have led to its being made. It was felt that a distance sufficiently great to prevent any possibility of disturbance should be temporarily fixed till experiments had been made to find to what distance from such railways the earth currents were still perceptible, and how these distances were affected by the condition of the soil, In the meantime it is known that a variable current like that of an electric tramway has been detected telephonically by Strecker at a distance of 17 kilometres; that at Greenwich, 6°84 kilometres from the line of the South London Electric Railway, the disturbances of the horizontal force due to the railway vary between ‘OU004 and ‘0U007 C.G.S. unit, and of the vertical force between 00004 and ‘00009 C.G.S. unit; while at Washington, 420 metres from an electric railway, the disturbances of the horizontal amount to ‘00010, and of the vertical force to ‘0030 C.G.S. unit; and at Toronto, 120 metres from a line, to 0012 and ‘0037 C.G.S. unit respectively. The effect of such disturbances on magnetic measurements, which are at present made almost universally to ‘00001 C.GS. unit, will be readily understood, and when it is remembered what important results have followed a further increase of sensitiveness of the instruments at Potsdam, the limit of 15 kilometres seems small enough. While the author is anxious that no unnecessary hindrance should be placed in the way of tramway engineers, and assures them that the limit will be lowered as soon as experiment has shown them that it can be done with safety, he points out that they have a simple remedy in their own hands—2.c. to provide an insulated return, } For the complete paper see Elektrotechnische Zeitschrift, part 24, 1898. SS ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 759 2. On the Magnetic Effects of Electric Railways at Berlin. By Dr. EscHennacGEN, of Potsdam, Dr. Eschenhagen gave an account of the experiments which had been made in Berlin to determine the effects of the electric railways there, and the way in which they decreased with distance from the line. Although up to the present the results do not justify any general statement being made, Dr. Eschenhagen anticipates important results from the method he has now adopted of using large coils in series with delicate galvanometers as detectors of earth currents. Papers on the subject were also contributed by Dr. C. Schott, Pro- fessor A. W. Riicker, Mr. W. H. Preece, F.R.S., Signor Luigi Palazzo, and Professor J. A. Fleming, F.R.S. After the discussion the Permanent Committee passed the following reso- lution :— ‘The Committee are of opinion that any sensible magnetic disturbance produced in a magnetic observatory by electric railways or tramways is seriously detrimental and may be fatal to the utility of the Observatory. They consider that special precautions should be taken to prevent such disturbances, and append as an example the provisions for the protection of the Kew Observatory inserted in a Bill passed by the English Parliament authorising the construction of an electric railway, the nearest point of which is to be at a distance of 1 kilometre from the Observatory.’ Clause for the Protection of Kew Observatory. (1) The whole circuit used for the carrying of the current to and from the carriages in use on the railway shall consist of conductors which are insulated along the whole of their length to the satisfaction in all respects of the Com- missioners of Her Majesty’s Works and Public Buildings (in this section called ‘the Commissioners’), and the said insulated conductors which convey the current to or from any of such carriages shall not at any place be separated from each other by a distance exceeding one-hundredth part of the distance of either of the conductors at that place from Kew Observatory. (2) If in the opinion of the Commissioners there are at any time reasonable grounds for assuming that by reason of the insulation or conductivity having ceased to be satisfactory a sensible magnetic field has been produced at the Observatory, the Commissioners shall have the right of testing the insulation and conductivity upon giving notice to the Company, who shall afford all necessary facilities to the engineer or officer of the Commissioners or other person appointed by them for the purpose, and the Company shall forthwith take all such steps as shall in the opinion of the Commissioners be required for preventing the production of such field. (8) The Company shall furnish to the Commissioners all necessary particulars of the method of insulation proposed to be adopted and of the distances between the conductors which carry the current to and from the carriages. The following Papers were read :— 1. On the Form of the Isomagnetic Lines in the Neighbourhood a7 | the Volcano Etna.’ By Luici PALazzo. The author made absolute determination of the magnetic elements at a number of stations in Sicily and the neighbouring small island, and relative determinations in the district surrounding each station by means of small portable instruments, In three of the islands, the rocks of which were of volcanic origin, the variations _ of the elements were found to be large and irregular, even where the constitution of 1 For full details see the Rendiconti d. Accad. d. Lincei, December 5, 1897. 760 REPORT—1898. the ground was uniform and its surface plane. He expresses the results of his deter- minations by tracing the course of the isogonic line for 10° 30’, which passes through the west and is parallel to the lines in Italy, that for 10° which passes through the centre, and for 9° 30' which passes through the east of the island and is profoundly modified by the presence of Etna, the isoclinal lines for 54°, 53° 30’, 53°, 52° 30’, 52°, which, with the exception of the 2nd and 3rd, passing respectively to the north and south of the volcano, are quite uniform, and the isodynamic line for -252, which has nearly the same shape as the isoclinals. By comparison of his results with those obtained by Christini in 1882, the author concludes that the annual changes of the elements are :— Declination . : : : : . —5'6’ Inclination . : . F A pre [1 Horizontal Intensity : : : . + *000017 2. On the Influence of Altitude above the Sea on the Elements of Terrestrial Magnetism. By Dr. VAN RiJCKEVORSEL and Dr. W. VAN BEMMELEN. The object of an investigation, which lasted from 1895-97, was to see if we could detect any influence of altitude above the sea on the magnetic elements. For various reasons, the Rigi was thought to be the mountain most suitable to our purpose, and in 1895 our observations were taken solely in order to discover if this mountain was really non-magnetic. We found that it was so. In 1896 complete series of observations were taken, both on the mountain and at its base, ata large number of stations. The discussion of these observations seemed to show a very slight decrease of the horizontal and a somewhat larger, though atill very slight, increase of the vertical component. However, this result was very doubtful, because we found at the same time that the Rigi, though certainly non-magnetic as a mass, was covered all over with superficial centres of attraction, very weak, but still causing disturbances which seriously interfered with our results. We resolved, therefore, to try again in 1897. In that year we took dips only at 198 stations, one of us always observing near the base of the mountain, the other, absolutely simultaneously with him, on tne top or on the slopes. Although this time also the small, but numerous, local disturbances were a decided drawback for the discussion, the following results were obtained : 1. We think it is proved, that if there be an influence of the height above the sea on terrestrial magnetism it is so exceedingly small as to make it unfeasible to detect it with our present surveying instruments. Therefore it is decidedly unnecessary to take altitude into account in magnetic surveys. 2. If, nevertheless, it should ultimately be found that there is such an influence, however small, it is more likely that it would be an increase of the vertical force with altitude than anything else. 3. On the Variation of Terrestrial Magnetic Force with Altitude.' By Professor J. Liznar. The author has endeavoured to eliminate the effect of the nature of the soil and shape of the surface at any point, on the variation of the magnetic force with height above the surface at the point, by basing his calculations on the results for the 205 stations in Austria at which observations of the magnetic elements have been made. He divides the stations into three groups—the first including those of altitude less than 200 metres, the second between 200 and 400, and the third above 400 metres. The mean value of an element for the stations of a group, he considers to be the value of the element for the mean altitude of the group, almost 1 The complete paper is published in Wiener Anzeiger, 1898, p. 168. ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 761 completely freed from local effects. Taking these values for the three mean stations, he finds the increase of the elements per kilometre of ascent to be as follows :— North component. . —*00034 C.G:S. Horizontal force . . —‘00029 C.G.S. West oy caeeeeten OOUO2O cm Declination . . . . +65:03' Vertical ,, . . — 00064 ,, Dip. . s - . —0°65' The variations calculated on the assumption that the earth is a uniformly magnetised sphere are much smaller, and the author considers that the discrepancy arises from the fact that part of the magnetic potential of the earth is due to an external source. Extracts from the Report of the Permanent Committee on Terrestrial Magnetism and Atmospheric Electricity to the International Meteoro- logical Conference. Constitution of the Committee. The Committee on Terrestrial Magnetism and Atmospheric Electricity appointed at Paris in September 1896 consisted of eight members. These gentlemen found that it was desirable to add to their number by co-option, and the constitution of the Committee is now as follows :— Appointed at Paris: Professor Riicker (President), Professor Eschenhagen, Professor Liznar, M. Th. Moureaux, Sig. L. Palazzo, Dr. Paulsen, Dr. van Rijckevorsel, General Rykatcheff. Co-opted: Dr. Bauer, Professor W. von Bezold, Sig. Brito-Capelio, Dr. Carlheim- Gyllenskjold, Professor Mascart, Professor T. Mendenhall, Professor A. Schmidt, Dr. C. Schott, and Professor A. Schuster. International Conference. In consequence of a suggestion, made originally by Professor Schuster, that arrangements should be made for an International Conference of those interested in Terrestrial Magnetism, the Committee decided to summon such a conference ; and the hospitable invitation of the British Association to hold the meeting in connection with that of the Association at Bristol (September 7-14, 1898) was accepted. ‘he details of the arrangements are described in the President’s address. Meetings of the Permanent Committee. The Committee held meetings on September 7, 9, 12, and 13, at which the following resolutions were unanimously approved :— A. Questions referred to the Committee by the International Meteorological Conference. (1) The following resolution of M. Dufour (Report of Paris Conference, p. 30). ‘In calculating monthly means, all days are to be taken into consideration. It is left open to each director to give in addition means calculated without taking disturbed days into account.’ This was approved by the Committee with the substitution of the words ‘ It is desirable’ for the words ‘It is left open to each director.’ The Committee were also of opinion that the quiet days chosen by the directors of the different observatories should be communicated to the President of the Permanent Magnetic Committee, and circulated by him, and also that it is desirable to inquire if it will be possible to select the same quiet days for the different observatories. (2) The resolution proposed by Professor von Bezold and M. Mascart (Report, p- 31) :— ‘It is desirable to publish the monthly means of the components X, Y, Z, and, 762 REPORT—1898. at least for the months of January and July, the differences dX, dY, dZ of the hourly means from the preceding means.’ In lieu of this the Committee adopted the following resolution :—‘It is desirable to publish the monthly means of the Geographical Components of the Magnetic Force for each month, and also the differences between the hourly means for each month and the monthly means for that month,’ (3) The resolution proposed by General Rykatcheff (Report, p. 32) :—‘It is desirable for the progress in Terrestrial Magnetism that temporary observatories should be installed in certain localities, especially in tropical countries.’ On this subject a Report was prepared, at the request of the President, by Professor von Bezold and General Rykatcheff. For the Report, and the reso- lution passed by the Committee, see p. 743. The Committee were informed by Dr. C. Schott that it was the intention of the Coast and Geodetic Survey of the United States to establish a magnetic obser- vatory at Honolulu. In the course of the discussion on the above resolution, the Committee also resolved :—3a. ‘That it is desirable to point out that observatories at great dis- tances from others should be provided with both absolute and self-registering variation instruments.’ (4) The question as to the relative advantages of long and short magnets, raised by M. Mascart at the Paris Conference (Report, p. 39). For the Report, and the resolution passed by the Committee, see p. 741. B. Resolutions passed by the Committee on matters arising during the Inter- national Conference. (1) Professor Eschenhagen made a statement to the Conference as to his recent investigations on minute disturbances made by very sensitive apparatus with a very open time scale. In view of this statement, the Committee expressed their sense of the impor- tance of the resolutions on this subject passed by the Paris Conference (Report, p. 35) and the hope that the principal observatories would carry out simultaneous observations of the character proposed. M. Moureaux informed the Committee that preparations for such observations were already complete in the observatory at Parc St. Maur. The Committee took note of the statement that Professor Eschenhagen would be willing to give information as to the construction of the instruments used by him. (2) The Committee also passed the following resolution :—‘ The Committee is of opinion that the early establishment of a magnetic observatory at the Cape of Good Hope provided with absolute and self-registering variation instruments would be of the highest utility to the science of Terrestrial Magnetism, especially in view of the Antarctic expeditions which are about to leave Europe, and that the observatory should be established at such a distance from electric railways and tramways as to avoid all possibility of disturbance from them.’ Directions were given that the proper steps should be taken to obtain the approval of the British Association for this resolution, with the request that, if approved, it should be forwarded to the Colonial Government. (8) On the motion of Professor Adolph Schmidt, the Committee resolved :-— ‘ That it is desirable that magnetic observations taken in regions not included in a magnetic survey should be repeated from time to time, care being taken to secure the identity of the point of observation.’ (4) Professor Eschenhagen was requested to draw up a detailed scheme for the exchange between the various observatories of the curves of the self-registering variation instruments taken during important magnetic storms, and to lay the scheme before the next meeting of the Conference. (5) With reference to certain inquiries which Professor Eschenhagen suggested —_———or | ON TERRESTRIAL MAGNETISM AND ATMOSPHERIC ELECTRICITY. 763 should be addressed to the Directors of Magnetic Observatories, the Committee was of opinion that, although it would be outside the scope of their duties to make the inquiries, it was desirable that the information should be collected and published. (6) After the discussion on the magnetic disturbances introduced by electric railways and tramways, a resolution was adopted by the Committee, which is given on p. 759. Future Organisation of the Committee. The Committee took into consideration their own future organisation and passed the following resolutions: ‘ It is desirable that Terrestrial Magnetism should continue to be within the scope of the International Meteorological Conference, provided that— (a) Invitations to attend that Conference are issued as widely as possible to Directors of Magnetic Observatories and to all students of Terrestrial Magnetism. (6) That the Permanent Committee on Terrestrial Magnetism and Atmospheric Electricity, as established at the Paris Conference, be continued. (c) That in future there shall be a Magnetic Section of the International Meteoro- logical Conference, which shall elect or otherwise share in the appointment of a permanent Magnetic Committee. (d) That the Magnetic Committee have power to summon an International Magnetic Conference at times other than those at which the whole of the Inter- national Meteorological (and Magnetic) Conference may meet.’ The Committee also consider that the President of the Permanent Magnetic Committee should only hold office between two successive meetings of the Inter- national Meteorological (and Magnetic) Conference. oy a Lee yi te fim? i ot adatoms, piel eta ty istsro 4 hi sher otli iy ad wes, Bin on 7 Sil of fan Bersted Weteedd te eit Aislorgane ‘ame $j Hater epatigttio” Date Yh halt eae ae: : +P oo Se a Fe sis ie Pin fe oe os Selig > fnoa Jeti Mi : far ‘ 4 ) ‘ .e tor. at ~gohs an: aathhi ae ae + ont i Weel bie AE Eagec incr és alana ie as pera | hag neal teat Lae ‘ Etiiitv wa 2 os tly priests ye’ “hy fray ew fl ee gan’ -~ s TRANSACTIONS OF THE SECTIONS. ff d 4 ’ “= vans Pt)? s 5 ’ % , oa * r 7 J are * PP Pee “aT * v ‘ a BHOTENIA AE 10 TRANSACTIONS OF THE SECTIONS. SECTION A.-MATHEMATICAL AND PHYSICAL SCIENCE. PRESIDENT OF THE SECTION—Professor W. E. Ayrton, F.R.S. THURSDAY, SEPTEMBER 8. The President delivered the following Address :— I sHatt, I feel sure, have your sympathy if I begin by referring to the great loss which mathematics and physics have sustained in the untimely and disastrous death of Dr. John Hopkinson. It has often been said that he who leads in mathe- matics at Cambridge cannot follow the engineering life of Westminster. But a striking disproof of the generality of this statement was furnished by the brilliant work in the domains of theory and practice which was accomplished by him for whom we mourn. Science has lost much, but the wife and mother has lost more, and to her, who in one day saw effaced so large a portion of her life, goes forth the expression of our grief and sorrow. A year ago Section A was charmed with a Presidential Address on the poetry of mathematics, and if amongst those who entered the Physics lecture-theatre at Toronto on that occasion there were any who had a preconceived notion that mathematics was a hard, dry, repellent type of study, they must, after hearing Professor Forsyth’s eloquent vindication of its charms, have departed convinced that mathematics resembled music in being a branch of the fine arts. Such an address, however, cannot but leave a feeling of regret amongst those of us who, engulfed in the whirl of the practical science of the day, sigh for the leisure and the quiet which are necessary for the worship of abstract mathematical truth, while the vain effort to follow in the footsteps of one gifted with such winning eloquence fills me with hopeless despair. Section A this year is very fortunate in having its meetings associated with those of an ‘International Conference on Terrestrial Magnetism and Atmospheric Electricity,’ which is attended by the members of the ‘ Permanent Committee for Terrestrial Magnetism and Atmospheric Electricity’ of the ‘ International Meteoro- logical Conference.’ It has been arranged that this Permanent Committee, of which Professor Riicker is the President, shall form part of the General Committee of Section A, and also shall act as the Committee of the International Conference, which will itself constitute a separate department of Section A. For the purpose, however, of preparing a Report to the International Meteorological Conference, and for similar business, this Permanent Committee will act:independently of the British Association. My first duty to-day, therefore, consists in expressing the honour and the very at pleasure which I feel in bidding you, members of the International Con- e rence, most heartily welcome. Among the various subjects which it is probable that the Conference may desire to discuss, there is one to which I will briefly refer as I am able todo so 768 REPORT—1898. in a triple capacity. The earth is an object of much importance, alike to the terrestrial magnetician, the telegraph electrician, and the tramway engineer ; but while the first aims at observing its magnetism, and the second rejoices in the absence of the earth currents which interfere with the sending of messages, the third seems bent on converting our maps of lines of force into maps of lines of tramway. It might therefore seem as if electric traction—undoubtedly a great boon to the people, and one that has already effected important social developments in Awerica and on the continent of Europe—were destined in time to annihilate magnetic observatories near towns, and even to seriously interfere with existing telegraph and telephone systems. Already the principle of the survival of the fittest is quoted by some electrical engineers, who declare that if magnetic observa- tories are crippled through the introduction of electric tramways, then so much the worse for the observatories. And I fear that my professional brethren only look at ie askance for allowing my devotion to the practical applications of electricity to be tainted with a keen interest in that excessively small, but none the less extremely wonderful, magnetic force which controls our compass needles. But this interest emboldens me to ask again, Can the system of electric traction that has already destroyed the two most important magnetic observa- tories in the United States and British North America be the best and the fittest to survive? Again, do we take such care, and spend such vast sums, in tending the weak and nursing the sick because we are convinced that they are the fittest to survive? May it not perhaps be because we have an inherent doubt about the justness of the survival cf the strongest, or because even the strongest of us feels compelled to modestly confess his inability to pick out the fittest, that modern civilisation encourages not the destruction but the preservation of what has obvious weakness, on the chance that it may have unseen strength ? When the electrical engineer feels himself full of pride at the greatness, the importance, and the power of his industry, and when he is inclined to think slightingly of the deflection of a little magnet compared with the whirl of his 1,000 horse-power dynamo, let him go and visit a certain dark store-room near the entrance hall of the Royal Institution, and, while he looks at some little coils there, ponder on the blaze of light that has been shed over the whole world from the dimly-lighted cupboard in which those dusty coils now lie. Then he may realise that while the earth as a magnet has endured for all time, the earth as a tramway conductor may at no distant date be relegated to the class of temporary makeshifts, and that the raids of the feudal baron into the agricultural fields of his neighbours were not more barbarous than the alarms and excursions of the tram- way engineer into the magnetic fields of his friends. A very important consideration in connection with the rapid development of physical inquiry is the possibility of extending our power of assim:lating current physical knowledge. For so wide have grown the limits of each branch of physics that it has become necessary to resort to specialisation if we desire to widen further the region of the known. On the other hand, so interlinked are all sections of physics that this increase of specialisation is liable to hinder rather than assist advance of the highest order. An experimenter is therefore on the horns of a dilemma—on the one hand, if he desires to do much he must confine hiniself more or less to one line of physical research, while, on the other hand, to follow that line with full success requires a knowledge of the progress that is being made along all kindred lines. Already an investigator who is much engaged with research can hardly do more as regards scientific literature than read what he himself writes—soon he will not have time to do even that. Division of labour and co-operation have therefore become as important in scientific work as in other lines of human activity. Like bees, some must gather material from the flowers that are springing up in various fields of research, while others must hatch new ideas. But, unlike bees, all can be of the ‘ worker’ class, since the presence of drones is unnecessary in the scientific hive. Englishmen have long been at a disadvantage in not possessing any ready TRANSACTIONS OF SECTION A. 769 means of ascertaining what lines of physical inquiry were being pursued in foreign eountries—or, indeed, even in their own. And, so far from making it easier to obtain this information, our countrymen have, I fear, until quite recently, been guilty of increasing the difficulty. For every college, every technical school in Great Britain—and their number will soon rival that of our villages—seems to feel it incumbent on itself to start a scientific society. And in accordance with the self-reliant character of our nation each of these societies must be maintained in absolute independence of every other society, and its proceedings must be pub- lished separately, and in an entirely distinct form from those of any similar body. To keep abreast, then, with physical advance in our own country is distinctly difficult, while the impossibility of maintaining even a casual acquaintance with foreign scientific literature lays us open to a charge of international rudeness. There is, of course, the German Berbldtter ; but the Anglo-Saxon race, which has spread itself over so vast a portion of the globe, is proverbially deficient in linguistic power, and consequently, till quite recently, information that was accessible to our friends on the Continent was closed to many workers in Great Britain, America, and Australia. Influenced by these considerations, the Physical Society of London, in 1895, embarked on the publication of abstracts from foreign papers on pure physics, and, as it was found that this enterprise was much appreciated, the question arose at the end of the following year whether, instead of limiting the journals from which abstracts were made to those appearing in foreign countries, and the papers abstracted to those dealing only with pure physics, the abstracts micht not with advantage be enlarged, so as to present a réswmé of all that was published in all languages on physics and its applications. The first application of physics which it was thought should be included was electrical engineering, and so negotiations were opened with the Institution of Electrical Engineers. After much deliberation on the part of the representatives of the two societies, it was finally decided to start a monthly joint publication, under the management of a committee of seven, two of whom should represent the Institution of Electrical Engineers, two the Physical Society, and three the two societies jointly. ‘Seience Abstracts’ was the name selected for the periodical, and the first number appeared in January of this year. A section is devoted to general physics, and a separate section to each of its branches; similarly, a section is devoted to general electrical engineering, and a separate section to each of its more important sub-divisions, ‘The value of ‘ Science Abstracts’ is already recognised by the British Association as well as by the Insti- tution of Civil Engineers, for those societies make a liberal contribution towards the expenses of publication, for which the Physical Society and the Institution of Electrical Engineers are responsible. At no distant date it is thought that other bodies may co-operate with us, and we have hopes that finally the scheme may be supported by the scientific societies of many Anglo-Saxon countries. For our aim is to produce, in a single journal, a monthly record in English of the most important literature appearing in all languages on physics and its many applications. This is the programme—a far wider one, be it observed, than that of the Beiblittery—which we sanguinely hope our young infant ‘Science Abstracts’ will grow to carry out. The saving of time and trouble that will be effected by the publication of such a journal can hardly be over-estimated, and the relief experienced in turning to a single periodical for knowledge that could hitherto be obtained solely by going through innumerable scientific newspapers, in many different languages, can only be compared with the sensation of rousing from a distracting and entangled dream to the peaceful order of wakeful reality. I therefore take this opportunity of urging on the members of the British Association the importance of the service which they can individually render to science by helping on an enterprise that has been started solely in its aid, and not _ for commercial purposes. The greatness of the debt owed by industry to pure science is often impressed 1898. 3D 770 REPORT—1898. on us, and it is pointed out that the comparatively small encouragement given by our nation to the development of pure science is wholly incommensurate with the gratitude which it ought to feel for the commercial benefits science has enabled it to reach. This is undoubtedly true, and no one understands better than myself how much commerce is indebted to those whose researches have brought them—it may be fame—but certainly nothing else. The world, however, appears to regard as equitable the division of reward which metes out tardy approbation to the discoverer for devising some new principle, a modicum of the world’s goods to the inventor for showing how this principle can be applied, and a shower of wealth on the contractor for putting the principle into practice. At first sight, this appears like the irony of fate, but in fact the world thus only proves that it is human, by prizing the acquisition of what it realises that it stande in need of, and by valuing the possession of what it is able to comprehend. Now, is there not a debt of which those who pursue pure science are in their turn equally forgetful—viz., the debt to the technical worker or to some technical operation for the inception of a new idea? For purely theoretical investigations are often born of technics, or, as Whewell puts it, ‘Art is the parent, not the progeny, of science; the realisation of principles in practice forms part of the prelude as well as of the sequel of theoretical discovery.’ I need not remind you that the whole science of floating bodies is said to have sprung from the solution by Archimedes of Hiero’s doubt concerning the transmutation of metals in the manufacture of his crown. In that case, however, it was the transmutation of gold into silver, and not silver into gold, that troubled the philosopher. Again, in the ‘History of the Royal Society at the End of the Eighteenth Century,’ Thomson says regarding Newton: ‘A desire to know whether there was anything in judicial astrology first put him upon studying mathematics. He dis- covered the emptiness of that study as soon as he erected a figure; for which purpose he made use of one or two problems in Euclid... . He did not then read the rest, looking upon it as a book containing only plain and obvious things. The analytical investigation of the motion of one body round an attracting centre, when disturbed by the attraction of another, was attacked independently by Clairault, D’Alembert, and Euler, because the construction of lunar tables had such a practical importance, and because large money prizes were offered for their accurate determination. The gambling table gave us the whole Theory of Probability, Bernoulli’s and Euler’s theorems, and the first demonstration of the binomial theorem ; while a request made to Montmort to determine the advantage to the banker in the game of ‘ Pharaon’ started him on the consideration of how counters could be thrown, and so led him to prove the multinomial and various other algebraical theo- rems. Lastly, may not the gambler take some credit to himself for the first suggestion of the method of least squares, and the first discussion of_the integra- tion of partial differential equations with finite differences contained in Laplace’s famous ‘ Théorie Analytique des Probabilités ? ’ The question asked Rankine by James R. Napier regarding the horse-power which would be necessary to propel, at a given rate, a vessel which Napier was about to build, resulted in the many theoretical investigations carried out by Rankine on water lines, skin-friction, stream lines, &c. For, as Professor Tait has said, ‘ Rankine, by his education as a practical engineer, was eminently qualified to recognise the problems of which the solution is required in practice; but the large scope of his mind would not allow him to be content with giving merely the solution of those particular cases which most frequently occur in engineering as we now know it. His method invariably is to state the problem in a very general form, find the solution, and apply this solution to special cases.’ Helmholtz studied physiology because he desired to be a doctor, then physics because he found that he needed it for attacking physiological problems, and lastly mathematics as an aid to physical research. But I need not remind you that it is his splendid work in mathematics, physics, and physiology, and not his success in ministering to the sick, that has rendered his name immortal. Se ea aL er ——S in TRANSACTIONS OF SECTION A. 771 Did not Kepler ask: ‘How many would be able to make astronomy their business if men did not cherish the hope of reading the future in the skies?’ And did he not warn those who objected to the degradation of mingling astrology with astroncmy to beware of ‘throwing away the child with the dirty water of its bath?’ Even now, may we not consider all the astronomical research work done at the Royal Observatory, Greenwich, as a by-product, since the Observatory is officially maintained merely for the purposes of navigation? And are there not many of us who feel assured that, since researches in pure physics and the elucidation of new physical facts must quite legitimately spring from routine standardising work, the most direct way—even now at the end of the nineteenth century—of securing for the country a National Physical Laboratory is to speed forward a Government Standardising Institute ? Lastly, as you will find in Dr. Thorpe’s fascinating ‘Life of Davy,’ it was the attempt to discover the medicinal effect of gases at the Pneumatic Institution in this city that opened up to Davy the charm of scientific research. And, indeed, the Royal Institution itself, the scientific home of Davy, Faraday, Tyndall, Rayleigh, and Dewar, owes its origin to Romford’s proposal ‘for forming in London by private subscription an establishment for feeding the poor and giving them useful employment ... connected with an institution for introducing and bringing forward into general-use new inventions and improvements by which domestic comfort and economy may be promoted,’ Coming now to physics proper, there is one branch which, although of deep interest, has hitherto been much neglected. We possess three senses which enable us to detect the presence of things at a distance—viz., seeing, hearing, and smelling. The first two are highly cultivated in man, and, probably for that reason, the laws of the propagation of the disturbances which affect the eyes and the ears have been the subject of much investigation, whereas, although to many animals the sense of smell is of far greater importance than those of seeing or hearing, and although, even in the human brain, a whole segment—a small one in modern man, it is true—is devoted to the olfactory fibres, the laws of the production and propagation of smell have received practically no attention from the physicist. For some time past it has, therefore, seemed to me to be of theoretical and practical importance to examine more fully into the physics of smell. Various other occupa- tionshave hitherto prevented my advancing much beyond the threshold of the subject, but, as it seems to me to open up what is practically a new field of inquiry for the physicist, I take this opportunity of putting on record some facts that have been already elucidated. Various odoriferous substances have been employed in the experiments, and for several of these I am indebted to Mr. W. J. Pope. Although the physicist has been allowing the mechanical side of the subject to lie dormant, the chemist, I find, has been analysing flowers and other bodies used in the manufacture of scents, and then synthetically preparing the odoriferous constituents. In this way, Mr. Pope informs me, there has been added to the list of manufactured articles, during the past seven years or so, vanilin, heliotropin, artificial musk, irone and ionone, which give the perfume of the violet ; citral, that of lemongrass ; coumarin, that of hay, and various others; and he has kindly furnished me with specimens of several of these artificial scents, together with other strongly-smelling substances. If it be a proof of civilisation to retain but a remnant of a sense which is so keen in many types of dogs, then I may pride myself on having reached a very high state of civilisation. But with the present investigation in view this pride has been of a very empty character, since I have been compelled to reject my own nose as quite lacking the sensitiveness that should characterise a philosophical measuring instrument. The ladies of my family, on the contrary, possess a nasal quickness which formerly seemed to me to be rather of the nature of a defect, since, at any rate in towns, there are so many more disagreeable odours than attractive ones. But on the present occasion their power of detecting slight smells, and the repugnance which they show in the case of so many of them, have stood 3D2 772 REPORT—1898. me in good stead, and made it possible to put before you the following modest contribution to the subject. There is a generally accepted idea that metals have smells, since, if you take up a piece of metal at random, or a coin out of your pocket, a smell can generally be detected. But I find that, as commercial aluminium, brass, bronze, copper, German- silver, gold, iron, silver, phosphor-bronze, steel, tin, and zinc are more and more carefully cleaned, they become more and more alike in emitting mo smell, and, indeed, when they are very clean it seems impossible with the nose, even if it be a good one, to distinguish any one of these metals from the rest, or even to detect its presence. Brass, iron, and steel are the last to lose their characteristic odour with cleaning, and for some time I was not sure whether the last two could be rendered absolutely odourless, in consequence of the difficulty of placing them close to the nose without breathing on them, which, as explained later on, evolves the characteristic ‘ copper’ and ‘iron’ smell. But experiment shows that, when very considerable care is taken both in the cleaning and the smelling, no odour can be detected even with iron or steel. Contrary, then, to what is usually believed, metals appear to have no smell per se. Why, then, do several of them generally possess smells? The answer is simple; for I find that handling a piece of metal is one of the most efficient ways of causing it to acquire its characteristic smell, so that the mere fact of lifting up a piece of brass or iron to smell it may cause it to apparently acquire a metallic odour, even if it had none before. This experiment may be easily tried thus: Clean a penny very carefully until all sense of odour is gone; then hold it in the hand for a few seconds, and it will smell—of copper, as we usually say. Leave it for a short time on aclean piece of paper, and it will be found that the metallic smell has entirely disappeared, or, at any rate, is not as strong as the smell of the paper on which it rests. The smell produced by the contact of the hand with the bronze will be marked if the closed hand containing it be only opened sufficiently for the nose to be inserted, and it can be still further increased by rubbing the coin between the fingers. All the metals enumerated above, with the exception of gold and silver, can be made to produce a smell when thus treated, but the smells evolved by the various metals are quite different. Aluminium, tin, and zinc, I find, smell much the same when rubbed with the fingers, the odour, however, being quite different from that produced by brass, bronze, copper, German-silver, and phosphor-bronze, which all give the characteristic ‘copper’ smell. Iron and steel give the strong ‘iron’ smell, which, again, is quite different from that evolved by the other metals. In making these experiments it is important to wash the hands carefully after touching each metal to free them from the odour of that metal. It is also neces- sary to wait for a short time on each occasion after drying the hands, since it is not until they become again moist with perspiration that they are operative in bringing out the so-called smell of metals. That the hands, when comparatively dry, do not bring out the smell of metals is in itself a disproof of the current idea that metals acquire a smell when slightly warmed. And this I have further tested by heating up specimens of all the above-mentioned metals to 120° Fahrenheit, in the sun, and finding that they acquire no smell when quite clean and untouched with the hands. Again, dealing with the copper group, or with aluminium, zo smell is produced by rubbing any one of them with dry table-salt, strong brine, or with wet salt, provided that a piece of linen is used as the rubber; but if the finger be substituted for the linen to rub on brine, a smell is observed with copper and German-silver, this smell, however, being rather like that of soda; and, whether dry salt, brine, or wet salt be rubbed on aluminium, a smell is noticed if the finger be used as the rubber, this smell being very marked in the case of the brine or wet salt. Again, although even when linen soaked in brine, or having wet salt on it, is used to rub tin, iron, or steel, a faint smell is noticed, this is much increased when the finger is substituted for the piece of linen. As a further illustration of the part played by the skin in causing metallic smells, it may be mentioned that the explanation of certain entirely contradictory Eye TRANSACTIONS OF SECTION A. 773 results, which were obtained in the early part of the investigation, when linen soaked in strong brine was rubbed on aluminium, was ultimately traced to one layer of moist linen of the thickness of a pocket-handkerchief, allowing the finger to act through it, so that an odour was sometimes noticed on rubbing aluminium with the piece of linen soaked in brine. For it was found that when two or more layers of the same linen soaked in the same brine were employed to separate the finger from the aluminium during the rubbing no smell could be detected. From the preceding it seems that the smell in these cases is evolved partly by contact with the finger, partly by the action of the solution of salt, and partly by the rubbing of the solid particles of salt against the metals. That the friction of solid particles against metals is operative in evolving smells is also illustrated by the smell noticed when iron is filed, or when aluminium, iron, or steel is cleaned with glass-paper or emery-paper in the air. Indeed, the smell thus evolved by aluminium Mrs, Ayrton finds particularly offensive. A slight smell is also noticed if iron or steel be rubbed in the air with even a clean piece of dry linen, and each specimen of the copper group, with the exception of the phosphor-bronze, which was tried in this way, gave rise to a faint, rather agreeable smell. No indication of odour could, however, be thus produced with aluminium or zinc when both the metals and the linen rubber were quite clean. It should, however, be borne in mind that all these experiments, where very slight smells are noticed, and espe- cially when the odour rapidly disappears on the cessation of the operation that produced it, are attended with a certain amount of doubt, for the linen rubber cannot be freed from the characteristic smell of ‘ clean linen,’ no matter how care- fully it may be washed. Before, then, a metal can evolve a smell, chemical action must apparently take place, for rubbing the metal probably frees metallic particles, and facilitates the chemical action to which I shall refer. All chemical actions, however, in which metals take part do not produce smell; for example, no smell but that of soda, or of sugar, respectively, can be detected on rubbing any single one of the series of metals that I have enumerated with a lump of wet soda, or a lump of wet sugar, although chemical action certainly takes place. Again, no metallic smell is observable when dilute nitric acid is rubbed on copper, German-silver, phosphor- bronze, tin, or zinc, although the chemical action is very marked in the case of some of these metals. Weak vinegar or a weak solution of ammonia is also equally inoperative. On the other hand, merely breathing on brass, copper, iron, steel, or zinc, which has been rendered practically odourless by cleaning, produces avery distinct smell, while a very thin film of water placed on iron or steel evolves a still stronger odour. Such a film, however, produces but little effect with any of the metals except these two; and if the whole series is lightly touched in succession with the tongue, the iron and steel smell as strongly as when breathed on, the German-silver more strongly than when breathed on or covered with a water film, and the other metals hardly at all. Now, as regards the explanation of these metallic smells, which have hitherto been attributed to the metals themselves. This, I think, may be found in the odours produced when the metals are rubbed with linen soaked in dilute sulphuric acid, For here, apart from any contact of the metal with the skin, the aluminium, tin, and zine are found to smell alike; the copper group also smell alike, and the iron and steel give rise to the characteristic ‘iron’ smell, which, in this case, can be detected some feet away. Now, it is known that when hydrogen is evolved by the action of sulphuric acid on iron, the gas has a very unpleasant smell, and this, Dr. Tilden tells me, is due principally to the presence of hydro- carbons.'' I have been therefore led to think that the smell of iron or steel when 1 T am informed that as all ordinary iron and steel contain, beside carbon, the elements phosphorus, sulphur, and silicon in quantities more or Jess minute, these substances, by combining with a portion of the liberated hydrogen, form compounds which have strong and characteristic odours, and, though in small quantity, con- tribute to the general effect. Of the hydrocarbons produced, the greater part consists of members of the paraffin series ; but these are accompanied by more or less 774 REPORT—1898. held in the hand is really due to the hydrocarbons to which this operation gives rise; and it is probable that no metallic particles, even in the form of vapour, reach the nose or even leave the metal. Hence, although smell may not, like sound, be propagated by vibration, it seems probable that particles of the metal with which we have been accustomed to associate the particular smell may no more come into contact with the olfactory nerves than a sounding musical instrument strikes against the drum of the ear. And the same sort of result may occur when a metal is rubbed, for, althouch in that case particles may very likely be detached, it seems possible that the function of these metallic particles may be to act on the moisture of the air, and liberate hydrogen similarly contaminated; and that in this case also it is the impurities which produce the smell, and not the particles of the metal with which we have been accustomed to associate it. This view I put forward tentatively ; and to further elucidate the matter I am about to begin a series of smell tests in various gases, artificially dried, with metals as pure as can be obtained. I next come to the diffusion of smell. From the experience we have of the considerable distance at which a good nose can detect a smell, and the quickness with which the opening of a bottle of scent, for example, can be detected at a distance, I imagined that tubes not less than 15 or 20 feet in length would be required for ascertaining, even roughly, the velocity at which a smell travels. 3ut experiment soon showed that when the space through which a smell had to pass was screened from draughts, it diffused with surprising slowness, and that feet could be replaced by inches in deciding on the Jengths of the tubes to be used. These are made of glass, which is relatively easy to free from remanent smells. When the room and tube had been freed from smell by strong currents of air blown through them, the tube was corked up at one end and taken outside to have another cork, to which was attached some odoriferous substance, inserted at the other end. ‘The tube was now brought back to the odourless room, and placed in a fixed horizontal or vertical position, and the unscented stopper was withdrawn. As a rule, immediately after the removal of the stopper, a smell was observed, which bad been transmitted very quickly through the tube by the act of corking up the other end with the stopper carrying the odoriferous material. This first whiff, however, lasted only a very short time, and then a long period elapsed before any further smell could be detected at the free end of the tube, whether that end was left open or closed between times. Finally, however, after, for example, about eighteen minutes in the case of a three-feet horizontal tube, having a large cotton-wool sponge saturated with oil of limes attached to one cork, the smell became definite and recognisable. It would, therefore, appear that the passage of smell is generally far more due to the actual motion of the air containing it than to the diffusion of the odoriferous substance through the air. And, as a striking illustration of this, the following is interesting:—After the stopper had been in contact with the odoriferous substance for some time, it, of course, acquired a smell itself, which gradually spread in the rvom in which the experiment was made. And although this smell was due simply to the exposed part of the stopper, while the air inside the tube was at one end in contact with a mass of the odoriferous substance itself, the only place where the smell could not be detected during the course of the experiment was the space inside the open end of the glass tube. And, what seemed very surprising, it was found necessary, in several cases, to blow air through the room to clear out the smell which emanated from the outside of the stopper before the smell coming along the tube from the mass of odoriferous substance which was inside it at the other end could be detected. A further proof of the important part played by of unsaturated hydrocarbons belonging to the olefine and other series. In view of the fact that marsh gas at one end of the scale and parafiin wax at the other are both practically odourless, it is doubtful whether the liquid paraffins have much smell when pure, and it would, therefore, appear probable that the hydrocarbons whieh give the peculiar odour to the hydrogen escaping from iron may be the unsaturated compounds referred to above. TRANSACTIONS OF SECTION A. 775 the motion of the air in diffusing smell was the fact that a strong smell at the free end of the tube could at any time be caused by merely loosening the stopper to which the scented sponge was attached ; for sniffing at the free end then made a draught through the tube which brought the scent with it. Further, although the glass tubes were coated outside with a thick layer of non-heat-conducting material, so as to check the formation of convection currents, due to difference in the inside and outside temperature caused by handling, the rate of travel of a smell from a given odoriferous material was found to be much quicker when the tube was vertical than when it was horizontal. But this, I am inclined to think, may have been caused by a small convection current which still was produced in spite of these precautions. For, as suggested by Dr. Ramsay several years ago, a substance must have a molecular weight at least fifteen times that of hydrogen to produce a sensation of smell at all, and, further, since camphor, with which many of my experiments have been made, has, when vaporised, a density about five times that of the air, it seems unlikely that scent vapour should ditluse much more quickly upwards through a vertical column of air than through a horizontal one. At the same time, not only are the tests with the glass tubes very striking, but the general impression which exists that smells rise—indeed the very fact that the nasal channels of animals open downwards—tends to show that, whether due to draughts or not, smells have really a tendency to ascend. And the following result obtained with glass tubes closed at one end with stoppers carrying respectively camphor, menthol, oil of limes, &c., and at the other end with corks, is instructive on this point. For, on uncorking such a tube after it had been closed for a long time and allowing the odour to stream out of it through the open air towards the experi- menter’s face, it was always found that the tube had to be brought much closer when the scent stream was poured downwards than when she was in a vertical position and it was allowed to ascend, although, when it was poured downwards, the experimenter brought her nose into as favourable a position as possible for receiving the smell, by lying down with her head thrown well back. As an illustration of the inefliciency of diffusion alone to convey a smell you will find that if you hold your breath, without in any way closing your nose either externally or by contracting the nasal muscles, you will experience no smelling sensation even when the nose is held close to pepper, or a strong solution of ammonia, or even when camphor in a minute tube is introduced high up into the nostril. Mere diffusion from the lower nasal cavity into the upper cannot apparently take place with sufficient ease to produce the sense of smell, so that an actual stream of air through the upper portion of the nose seems necessary even when the nose is a very sensitive one. This stream, for substances placed outside the nose, is produced by breathing zm, no smell being detected while breathing owt. On the other hand, if a substance be placed inside the mouth its flavour is recog- nised when the air is forced outwards through the nostrils—that is, at each expiration. Hence we may experience alternately two totally different smells by placing one substance outside the nose and the other in the mouth, the one smell being noticed in inhaling and the other in exhaling. And the latter can be increased by smacking the lips, which, I think, has really for its object the forcing of more air through the nostrils at each expiration. Experiments on the propagation of smells in a vacuum have also been com- menced in my laboratory, and the results are no less surprising than those obtained with the propagation in air. A U-tube, seven inches high, had the odoriferous substance placed inside it at the top of one limb, and a very good vacuum could be made by allowing mercury to flow out of the tube. Then the two limbs were separated by raising the mercury column, and, air being admitted at the top of the other limb, without its coming into contact with the odoriferous substance, the nose was applied at the top of this limb. When liquids like ammoniated lavender smelling-salts, solution of musk, and amyl acetate were employed, and various devices were used for introducing the liquid, and preventing its splashing when it boiled on exhausting the air, it was found that the time that it was necessary to leave the two limbs connected for a 776 REPORT—1898. smell to be just observable was reduced from a few minutes or seconds when the tube was filled with air to less than half a second for a good vacuum; with solid camphor it was reduced from twenty minutes to one second; and, when moist rose leaves were used, from fifty minutes to two seconds. But with solid particles of musk the time was not reduced below twenty minutes by taking away the air; while with dried lavender flowers and dried woodruff leaves no smell could be detected after the two limbs had been connected for many hours, and a good vacuum maintained. These experiments are, of course, somewhat complicated by variations in the amount of odorous surface exposed, but they seem to indicate that with these particular dried substances either the rate of evolution of the scent, or its rate of propagation, or both, are very slow even in a good vacuum. I have also carried out some tests on the power of different substances to absorb various scents from the air. Lard, it is well known, is used to absorb the erfume from flowers in the commercial manufacture of scents, perhaps because it has little odour of its own, and because the scent can be easily distilled from it. But if lard, wool, linen, blotting-paper, silk, &c., be shut up for some hours in a box at equal distances from jasmine flowers, dried woodruff leaves, or from a‘ — solution of ammonia, I find that it is not the lard, but the blotting-paper, that smells most strongly when the articles are removed from the box. On the other hand, when solid natural musk is employed, it is the wool that alone acquires much smell, even after the box has been shut up for days. Another noteworthy fact is the comparatively rapid rate at which grains of natural musk are found to lose their fragrance when exposed to the air. The popular statement, therefore, that a grain of musk will scent a room for years supplies but another example of the contrast between text-book information and laboratory experience. The power of a smell to cling to a substance seems to depend neither on the intensity of the smell nor on the ease with which it travels through a closed space. Musk has but a faint smell, but the recollection of the greeting of a rich Oriental survives many washings of the hands. The smell of rose leaves, again, is but faint, and it travels very slowly through air in a tube; and yet the experi- ments on its propagation in the glass vacuum apparatus were rendered extremely troublesome by the difficulty experienced in removing the traces of the smell from the glass between the successive tests. Rubbing its surface was quite ineffectual, and even the mercury had to be occasionally shaken up with alcohol to free it from the remanent smell. In fact, we found, as Moore put it: ‘ You may break, you may shatter the vase if you will, But the scent of the roses will cling to it still’ This absorption of scents by glass, and the ease with which I found that jasmine flowers could be distinguished from woodruff leaves, even when each was enclosed in a series of three envelopes specially prepared from glazed paper, and when many precautions were taken to prevent an odour being given to any of the envelopes in the operation of closing, as well as to prevent its diflusion through the joins in the paper, led me to try whether an actual transpiration through glass could be detected with the nose. For this object a number of extremely thin glass bulbs were blown from soda and from lead glass, so thin that they exhibited colours like a soap bubble, and felt, when gently touched, like very thin oiled silk, and after a little ammoniated lavender, amyl nitrite, ethyl sulphide, mercaptan, solution of musk, oil of peppermint, and propylamine had been introduced into them respec- Hii they were hermetically sealed, and placed separately in glass stoppered bottles. In some cases, on removing the stopper from a bottle after many hours, a faint odour could be detected, but so, generally, could a minute flaw after much searching ; the crack, however, being so slight that it did not allow sufficient passage of the air to prevent the bulb subsequently breaking, presumably from changes of atmo- spheric pressure. Aud in those cases where a smell was detected without any flaw being found in the glass, the subsequent breaking of the bulb put an end to further testing. The question, therefore, remains unanswered. eee TRANSACTIONS OF SECTION A. HEL In presenting this brief introduction to the physics of smell, I have aimed at indicating the vast territory that waits to be explored. That it will be found to contain mines of theoretical wealth there can be no doubt ; while it is probable that a luxuriant growth of technical application would spring up later on. Already, for example, Mrs. Ayrton unintentionally picks out inferior glass by the repugnance she shows at drinking water out of certain cheap tumblers. To conclude, I may say that one of my fondest hopes is that an inquiry into the physics of smell may add another to the list of wide regions of knowledge opened up by the theoretical physicist in his search for answers to the questions of the technical man. The following Report and Papers were read :— 1. Report on Comparing and Reducing Magnetic Observations. See Reports, p. 80. 2. Lenses not of Glass. By J. W. Girrorp. Glass passes light to A =3612, calcite to A= 2064, and quartz to A=1852, the most refrangible line of aluminium. Seventy deviations were measured between A\=7951 and \=2147. Over that range an uncorrected quartz lens F=11” gives 1:76” of chromatic aberration; when corrected by calcite this may be reduced to 0:24”. ,) — tan e, sin °h,, @) where o refers to the ordinary and e to the extraordinary wave; ¢, and ¢, denote here the angles of refraction of the ordinary and extraordinary wave respectively, 6, and 6, their respective azimuths, and «, and e, the small angles between the directions of propagation of these waves and those of their so-called rays. This condition (1) may be regarded as an equation for the determination of the angle @; we observe that it does not contain the azimuth 6 of the incident wave. It thus follows: when ordinary light strikes the surface of the given crystal at such an angle o, determined by this equation, it will be reflected as linearly polarised, as in the case of an isotropic insulator, or certain phenomena as those of interference will make their appearance; which of these phenomena occur will, however, depend upon the assumption made with regard to the behaviour of the ether-molecules in the film between the two bodies. Conversely, observations of such phenomena might throw light on the assumption to be made. The above equation for ¢ 1s, however, too general to admit of a solution; all information must thus be gained from an examination of x special cases; I have chosen the following one for the present purpose, since it appears to be of particular interest. Let one of the principal planes of the given crystal be taken as reflecting surface, and let the plane of incidence lie in one of the other two, as indicated in the annexed figure. 4 (y = reflecting plane, w y incident plane) ie The above equation for ¢ then reduces to J, sin (p—®@,) cos (b+,) — tane, sin*,=0; . : s* its derivation, into which I cannot enter here, requires considerable care, chiefly on account of the appearance of indeterminate forms. . Explicitly, it can be written ev? —(A* — B®) sin *] cos 6 =B /v?— A? sin 7 [v? + (A2—B?*) sin *], . (8) where 4, 5, Care three medium constants of the dimensions of a velocity, and v the velocity of propagation of electromagnetic disturbances in air. For isotropic insulators, i.e. A = B= C, this equation for ¢ becomes sin *@= = - c : : . (4) * C£ also P. Volkmann, Vorlesungen tiber die Theorie des Lichtes, p. 341, 812 REPORT—1898. which is identical to the condition that =e p rt p, 2 ? or, in more familiar form, that the reflected and the refracted rays form a right angle with each other. It is evident from the above simple relation that, if » and ¢ can be determined by experiment, A will be given. Even a general examination of the above special equation (3) would be too long here; I shall, therefore, confine myself to the particular case where A, B, and C are assigned given numerical values; for sulphur Boltzmann! has found the following values for the constants of electric induction : 4773 3:970 3°811. For these values the above equation (3) reduces approximately to sin °f + 51°7 sin 4 + 494°8 sin *@ —440=0, one root of which is j gp = 64° 44’; the other roots are imaginary. Similarly, we find another angle of polarisation ¢ on interchanging the above wv (A) and y (B) co-ordinate axes with each other. The general equation in must then evidently be written v* [v? + (A?—B?) sin *] cos $= A./v* = B? sin *¢ [v? — (A®— B?) sin *9]. This equation reduces for the given particular case to sin “fp — 53.35 sin *¢ + 617.53 sin * —-465=0; one root of which is p =62° 7’ 30"; the other roots are imaginary. If now we are able to determine by experiment two such critical values of ¢, characterised by linearly polarised light or other phenomena, we should then have two equations for the determination of the quantities 4 and B. Although the actual solution of these equations with regard to A and B offers difficulty, very approximate ones can always be found. Similarly, to determine the third medium-constant (, we have only to choose those principal planes of the given crystals as reflecting and incident planes, for which the above formula (2) reduces to a function of C and A or B only. 1 Cf. Pogg. Ann. 153, 1874. ‘Experimentaluntersuchung tiber das Verhalten nicht Jeitender Kérper unter dem Einflusse elektrischer Krifte.’ Also Poincaré’s Llectricité et optique, vol. i. p. 129. a i i Ee TRANSACTIONS OF SECTION B. 813 Secrion B.—CHEMISTRY. PRESIDENT OF THE SECTION.—Professor F. R. Japp, M.A., LL.D., F.R.S. THURSDAY, SEPTEMBER 8. The President delivered the following Address :— Stereochemistry and Vitalism. Or the numerous weighty discoveries which science owes to the genius of Pasteur, none appeals more strongly to chemists than that with which he opened his career as an inyestigator—the establishing of the connection between optical activity and molecular asymmetry in organic compounds. The extraordinary subtlety of the modes of isomerism then for the first time disclosed ; the novelty and refinement of the means employed in the separation of the isomerides ; the felicitous geometrical hypothesis adopted to account for the facts—an hypothesis which subsequent investigation has served but to confirm; the perfect balance of inductive and deductive method ; and lastly, the circumstance that in these researches Pasteur laid the foundation of the science of stereochemistry: these are characteristics any one of which would have sufficed to render the work eminently noteworthy, but which, taken together, stamp it as the capital achievement of organic chemistry. Physiologists, on the other hand, are naturally more attracted by Pasteur’s subsequent work, in which the biological element predominates; in fact, I doubt whether many of them have given much attention to the earlier work. And yet it ought to be of interest to physiologists, not merely because it is the root from which the later work springs, but because it furnishes, I am convinced, a reply to the most fundamental question that physiology can propose to itself—namely, whether the phenomena of life are wholly explicable in terms of chemistry and physics; in other words, whether they are reducible to problems of the kinetics of atoms, or whether, on the contrary, there are certain residual phenomena, inex- plicable by such means, pointing to the existence of a directive force which enters upon the scene with life itself, and which, whilst in no way violating the laws of the kinetics of atoms—whilst, indeed, acting through these laws—determines the course of their operation within the living organism. The latter view is known as Vitalism. At one time universally held, although in a cruder form than that just stated, it fell, later on, into disrepute ; ‘ vital force,’ the hypothetical and undefined cause of the special phenomena of life, was relegated to the category of occult qualities; and the problems of physiology were declared to be solely problems of chemistry and physics. Various causes con- tributed to this result. In the first place, the mere name ‘ vital force’ explains nothing; although, of course, one may make this admission without thereby conceding that chemistry and physics explain everything. Secondly, the older vitalists confounded force with energy ; their ‘ vital force’ was a source of energy ; 814 REPORT—1898. so that their doctrines contradicted the law of the conservation of energy, and became untenable the moment that this law was established. I would point out, however, that the assumption of a purely directive ‘ vital force,’ such as I haye just referred to, using the word ‘force’ in the sense which it bears in modern dynamics, does not necessarily involve this contradiction ; for a force acting on a moving body at right angles to its path does no work, although it may continuously alter the direction in which the body moves. When, therefore, Professor J. Burdon Sanderson writes: ‘The proof of the non-existence of a special “ vital force” lies in the demonstration of the adequacy of the known sources of energy in the organism to account for the actual day by day expenditure of heat and work,’ he does not consider this special case. The application of the foregoing principle of dynamics to the discussion of problems like the present is, I believe, due to the late Professor Fleeming Jenkin. A third ground for abandoning the doctrine of a ‘vital force’ was the discovery that numerous organic compounds for the pro- duction of which the living organism was supposed to be necessary could be synthesised by laboratory methods from inorganic materials. It is the validity of some of the conclusions drawn from the latter fact that I wish especially to consider. Recent years have, however, witnessed a significant revival of the doctrine of yitalism among the physiologists of the younger generation. It is not my intention to offer any opinion on the various arguments which physiologists of the neo-vitalistic school have put forward in support of their views; these arguments and the facts on which they are based lie entirely outside my province. I shall confine myself to a single class of chemical facts rendered accessible by Pasteur’s researches on optically active compounds, and, considering these facts in the light of our present views regarding the constitution of organic compounds, I shall endeavour to show that living matter is constantly performing a certain geometrical feat which dead matter, unless indeed it happens to belong to a particular class of products of the living organism and to be thus ultimately referable to living matter, is incapable—not even conceivably capabie—of perform- ing. -My argument, being based on geometrical and dynamical considerations, will have the advantage, over the physiological arguments, of immeasurably greater simplicity ; so that, at all events, any fallacy into which 1 may unwittingly fall will be the more readily detected. é In order to make clear the bearing of the results of stereochemical research on this physiological problem, it will be necessary to give a brief sketch of the stereo- chemistry of optically active organic compounds, as founded by Pasteur and as further developed by later investigators. Substances are said to be optically active when they produce rotation of the plane of polarisation of a ray of polarised light which passes through them. The rotation may be either to the right or to the left, according to the nature of the substance ; in the former case the substance in said to be dextro-rotatory; in the latter, levo-rotatory. The effect is as if the ray had been forced through a twisted medium—a medium with a right-handed or a left-handed twist—and had itself received a twist in the process; and the amount of the rotation will depend upon the degree of ‘ twist’ in the medium (that is, on the rotatory power of substance) and upon the thickness of the stratum of substance through which the ray passes, just as the angle through which a bullet turns in passing from the breech to the muzzle of a rifle will depend upon the degree of twist in the rifling and the length of the barrel. Ifthe bullet had passed through the barrel in the opposite direction, the rotation would still have been in the same sense ; since a right-handed (or left- handed) twist or helix remains the same from whichever end it is viewed, in whichever direction it is traversed. This also applies to optically active substances ; if the polarised ray passes through the substance in the opposite direction, the rotation still occurs in the same sense as before. This characteristic sharply distinguishes the rotation due to optically active substances from that produced by the magnetic field, the latter rotation being reversed on reversing the direction of the polarised ray. Optically active substances may be divided into two classes, Some, like quartz, LL <« i TRANSACTIONS OF SECTION B. 815 sodium chlorate, and benzil, produce rotation only when in the crystallised state ; the dissolved (or fused) substances are inactive. Others, like oil of turpentine, cam- phor, and sugar, are optically active when in the liquid state or in solution. In the former case the molecules of the substance have no twisted structure, but they unite to form crystals having such a structure. As Pasteur expressed it, we may build up a spiral staircase—an asymmetric figure—from symmetric bricks; when the stair- case is again resolved into its component bricks, the asymmetry disappears. (I will explain presently the precise significance of the terms symmetry and asymmetry as used in this connection.) In the case of compounds which are optically active in the liquid state, the twisted structure must be predicated of the molecules themselves; that is, there must be a twisted arrangement of the atoms which form these molecules. The earliest known experimental facts regarding the rotation of the plane of polarisation by various substances, solid and liquid, were discovered by Arago and by Biot. ’ After this preliminary statement as to what is understood by optical activity, we may consider Pasteur’s special contributions to the solution of the problems inyolved. Pasteur tells us, in the well-known ‘ Lectures on the Molecular Asymmetry of Natural Organic Products,’ which he delivered in 1860, before the Chemical Society of Paris, that his earliest independent scientific work dealt with the subject of crystallography, to which he had turned his attention from a conviction that it would prove useful to him in the study of chemistry. In order to perfect himself in crystallographical methods, he resolved to repeat all the measurements contained in a memoir by De la Provostaye on the crystalline forms of tartaric acid, racemic acid, and their salts. These two sets of compounds have the same composition, except that they frequently differ in the number of molecules of water of crystallisation which they contain; but whereas tartaric acid and the tartrates are dextro-rotatory, racemic acid and the racemates are optically inactive. It was probably this circumstance that decided Pasteur in his choice of a subject, for it appears that, even as a student, he had been attracted by the problem of optical activity. In the course of the repetition, however, he detected a fact which had ‘escaped the notice of his predecessor in the work, accurate observer as the latter was—namiely, the presence, in the tartrates, of right-handed hemihedral faces, which are absent in the racemates. Hemihedral faces are such as occur in only half their possible number; and in the case of non-superposable hemihedry, to which class that of the tartrates belongs, there are always two opposite hemihedral forms possible: a right-handed or dextro-form, and a left-handed or levo-form. Which is right, and which is left, is a matter of convention; but they are opposite forms, and differ from one another exactly as the right hand of the human body differs from the left: that is, they resemble one another in every respect, except that they are non-superposable—the one cannot be made to coincide in space with the other, just as a right hand will not fit into a left-hand glove. The one formis identical with the mirror image of the other: thus the mirror image of a right hand is a left hand. Such opposite hemihedral crystalline forms are termed enantiomorphs; they have the same faces and the same angles, but differ in the fact that all positions in the one are reversed in the other for one dimension of space, and left unchanged for. the other two dimensions; this being the geometrical transformation which an object appears to undergo when reflected in a plane mirror. Enantiomorphism is possible only in the case of asymmetric solid figures : these alone give non-superposable mirror images. Any object which gives a mirror image identical with the object itself—a superposable mirror image—must have at least one plane of symmetry. The hemihedry of the tartrates discovered by Pasteur is in every case in the same sense—that termed right-handed—provided that the crystals are oriented according to two of the axes which have nearly the same ratio in all the tartrates. Pasteur was inclined to connect the molecular dextro-rotatory power of the tartrates with this right-handed hemihedry; since in the racemates both the hemihedry and the rotatory power were absent. A similar connection, which, 316 REPORT—1898. however, held good only for the crystalline condition, had, as he points out, been already observed in the case of quartz, the crystals of which occasionally exhibit small asymmetric (tetartohedral) faces, situated in some specimens to the right and in others to the left; the former specimens being dextro-, the latter, levo- rotatory. The possibility of this connection was first suggested by Sir John Herschel. Pasteur’s views were confirmed by an unexpected discovery which he made shortly after. Mitscherlich had stated, in 1844, in a communication to Biot, which the latter laid before the French Academy of Sciences, that sodium ammonium tartrate and sodium ammonium racemate were identical, not merely in chemical composition, but in crystalline form, in specific gravity, and in every other property, chemical and physical, except that the solution of the former salt was dextro-rotatory, that of the latter inactive. And to make his statement still more definite, he added: ‘The nature and the number of the atoms, their arrange- ment, and their distances from one another, are the same in both compounds.’ At the time this passage appeared Pasteur was a student in the Ecole Normale. He tells us how it puzzled him, as being in contradiction to the views universally held by physicists and chemists, that the properties, chemical and physical, of substances depended on the nature, number, and arrangement of their constituent atoms. He now returned to the subject, imagining that the explanation would be found in the fact that Mitscherlich had overlooked the hemihedral faces in the tartrate, and that the racemate would not be hemihedral. He therefore prepared and examined the two double salts. He found that the tartrate was, like all the other tartrates which he had investigated, hemihedral ; but, to his surprise, the solution of the racemate also deposited hemihedral crystals. A closer examination, how- ever, disclosed the fact that, whereas in the tartrate all the hemihedral faces were situated to the right, in the crystals from the solution of the racemate they were situated sometimes to the right, and sometimes to the left. Mindful of his view regarding the connection between the sense of the hemihedry and that of the optical activity, he carefully picked out and separated the dextro- and levo-hemi- hedrai crystals. made a solution of each kind separately, and observed it in the polarimeter. To his surprise and delight, the solution of the right-handed crystals ‘was dextro-rotatory ; that of the left-handed, lzevo-rotatory. The right-handed crystals were identical with those of the ordinary (dextro-) tartrate; the others, which were their mirror image, or enantiomorph, were derived from the hitherto unknown levo-tartaric acid. From the dextro- and levo-salts thus separated he prepared the free dextro- and levo-tartaric acids. And having thus obtained from racemic acid its two component acids—dextro- and levo-tartaric acids—it was an easy matter to recompose racemic acid. He found that, on mixing equal weights of the two opposite acids, each previously dissolved in a little water, the solution almost solidified, depositing a mass of crystals of racemic acid. These two tartaric acids have the same properties, chemical and physical, except where their opposite asymmetry comes into play. They crvstallise in the same forms, with the same faces and angles; but the hemihedral facets, which in the one are situated to the right, are, in the other, situated to the left. Their specific gravities and solubilities are the same; but the solution of the one is dextro-rotatory ; of the other, levo-rotatory. The salts which. they form with inorganic bases also agree in every respect, except as regards their opposite asymmetry and opposite rotatory power. They are enantiomorphous. Pasteur, discussing the question of the molecular constitution of these acids, anticipates in a remarkable manner the views at present held by chemists. ‘ We know, on the one hand,’ he says, ‘ that the molecular structures of the two tar- taric acids are asymmetric, and on the other, that they are rigorously the same, with the sole difference of showing asymmetry in opposite senses. Are the atoms of the right acid grouped on the spirals of a right-handed helix, or placed at the solid angles of an irregular tetrahedron, or disposed according to some particular asymmetric grouping or other? We cannot answer these questions. But it can- not be a subject of doubt that there exists an arrangement of the atoms in an asymmetric order having a non-superposable image. It is not less certain that TRANSACTIONS OF SECTION B, 817 the atoms of the left acid realise precisely the asymmetric grouping which is the inverse of this,’ The idea of the irregular tetrahedron is, it may be explained, derived from the hemihedral facets. Imaginé these to develop in the case of dextro-tartaric acid until the other faces of the crystal disappear, and there results an irregular tetra- hedron. Repeat the process with a crystal of lzvo-tartaric acid, and the enantio- morphous tetrahedron—the mirror-image of the former—is obtained. We shall ¢ later that the idea, on the one hand, of two asymmetric tetrahedra, and, on the other, that of two opposite helices, given as alternatives by Pasteur to explain the grouping of the atoms within the molecules of dextro- and lwvo-tartaric acids, are in reality identical. The precision of Pasteur’s views as to the asymmetry of these acids enabled him to discover two further methods of separating them. Thus he points out that although these acids will possess equal affinity for any given symmetric base, such as potash, or ammonia, or aniline, yet.their affinities will not be equal if the base, like quinine or strychnine, is itself asymmetric ; because here the special one-sided asymmetry of the base will modify its mode of combination with the two enantio- morphous acids, The solubility is different in the case of the dextro- and levo- tartrates of the same asymmetric base ; the crystalline form, the specific gravity, the number of molecules of water of crystallisation, may be all different. Potassium dextro- and levo-tartrates are mirror images of one another; quinine dextro- and lsevo-tartrates are not. Pasteuremployed in his experiments the asymmetric base cinchonicine, which he converted into its acid racemate, and allowed the solution to crystallise. The first crystallisations consisted of pure levo-tartrate of cin- chonicine, whilst the more soluble dextro-tartrate remained in the mother liquor, from which it finally crystallised in forms totally distinct from those of the levo- tartrate. Pasteur’s third method is of physiological interest, and is, moreover, the stepping-stone to his later work on ferments. As we shall see presently, he regarded the formation of asymmetric organic compoundsas the special prerogative of the living organism. Most of the substances of which the animal and vegetable tissues are built up—the proteids, cellulose—are asymmetric organic compounds, displaying optical activity. Pasteur had shown that two compounds of inverse asymmetry behaved differently towards a third asymmetric compound. How would they behave towards the asymmetric living organism ? It had frequently been noticed that impure calcium tartrate, when mixed with organic matters, as is the case when it is obtained in the process of preparing tartaric acid from argol, readily underwent fermentation. Pasteur examined the action of the ferment (apparently a Penicillium) on ammonium tartrate—a sub- stance which had the advantage over calcium tartrate of being soluble—and, finding that the fermentation here followed a normal course, ending with the destruction of the tartrate, repeated the experiment with ammonium racemate, examining the sclution from time to time with the polarimeter. The fermentation proceeded, apparently, as before; but the solution, originally optically inactive, became levo- rotatory, the activity gradually increasing in amount until a maximum was reached. At this point the fermentation ceased. The whole of the dextro- tartrate had disappeared, and from the solution the levo-tartrate was obtained in a state of purity. The asymmetric living organism had selected for its nutriment that particular asymmetric form of tartaric acid which suited its needs—the form, doubtless, which in some way fitted its own asymmetry—and had left the opposite form either wholly or, for the most part, untouched. The asymmetric micro- organism, therefore, exhibits a power which no symmetric chemical substance, such as our ordinary oxidising agents, and no symmetric form of energy, such as heat, can ever possess: it distinguishes between enantiomorphs. If we oxidise racemic acid with nitric acid, for example, both the enantiomorphous constituents are attacked in exactly the same degree. If we heat racemic acid, whatever happens to its right-handed constituent happens equally to its left-handed con- stituent: the temperature of decomposition of both is the same. Asymmetric agents can alone display selective action in dealing with enantiomorphs. 1898, 3G 818 i REPORT—1898. By the action of heat Pasteur converted ordinary tartaric acid into racemic acid, in which process a portion of the right acid is converted into the left, an equilibrium being established ; and lvo-tartaric acid may be converted into racemic acid in the same way, the inverse change taking place. At the same time, a new tartaric acid is formed in both cases: mesotartaric acid, or true inactive tartaric acid, which resembles racemic acid in having no action on tbe plane of polarisation, but differs from it in not being separable into two acids of opposite activity. According to our present views, it contains two equal and opposite asymmetric groups within its molecule. Racemic acid is thus inactive by enter- molecular compensation ; mesotartaric acid, by zzt/amolecular compensation. ' Pasteur, generalising somewhat hastily from the few cases which he had studied, came to the conclusion that all organic compounds capable of exhibiting optical activity might exist in the foregoing four forms—dextro, levo, racemoid, and meso. As regards the dextro and levo forms, this is correct; as regards the racemvid form it is generally correct; but the meso form, as we now know, is a very special case, implying that the molecule contains two structurally identical complexes of opposite asymmetry. Were I following the exact historical order, I should introduce here Pasteur’s view that compounds exhibiting optical activity have never been obtained without the intervention of life—a view which it is the object of the present address to consider. The later developments of stereochemistry, however, throw so much light on this question, and enable us to discuss it with such precision, that we shall turn our attention to these first. Before so doing, however, we may note that, in spite of the immense growth in the material of stereochemistry, and in spite of the development of the theoretical views of stereochemists, hardly any ‘experimental method of fundamental importance for the separation and trans- formation of optically active compounds has been added to those described in Pasteur’s classical researches, although it is almost forty years since these came to a close. Perhaps Walden’s remarkable discovery of a method for the transforma- tion of certain enantiomorphs into their optical opposites without previous racemi- sation, is the only one entitled to be so classed. Pasteur was in advance of his time, and his theory of molecular asymmetry ‘was a seed that lay for many years in the ground without germinating. In 1858, just about the period when Pasteur was concluding his researches in the foregoing field, Kekulé published his celebrated theoretical paper, ‘On the Constitution and Metamorphoses of Chemical Compounds, and on the Chemical Nature of Carbon, in which he showed that, by assuming that the carbon atom had four units of affinity, the constitution wf orgatic compounds could be satis- factorily explained. This was the starting-point of the theory of chemical structure, and from that time to the present day organic chemists have been engaged, with enormous expenditure of labour, in determining the constitution or molecular structure of the carbon compounds on the lines of Kekulé’s theory. In order that Pasteur’s ideas should bear fruit it was only necessary that ‘his purely general statements with regard to molecular asymmetry should be specialised, so as to include the recognised constitution of organic compounds. It was from this union of Pasteur’s theory with that of Kekulé that modern stereo- chemistry sprang. The necessary step was taken, independently and almost simultaneously, by Van’t Hoff and Le Bel, in 1874. I will briefly state their conclusions, so far as these bear on the subject of optical activity. _ Jf we examine the structural formule of a number of thoroughly investigated optically active organic compounds, we shall find that the molecule of each contains at least one carbon atom of which the four affinities are satisfied by ‘four different atoms or groups—an asymmetric carbon atom, as it is termed. The four affinities, or directed attractive powers, of the carbon atom are not to be conceived of as lying in one plane. The simplest assumption that we can make with regard to their distribution in space is that the direction of each makes equal angles with the directions of the three others. We may express this differently by saying that the four atoms or groups attached to the carbon atom are situated at the solid angles of a tetrahedron, in the centre of which the carbon TRANSACTIONS OF SECTION B. 819 atom itself is placed. If the four atoms or groups are all identical they will be equally attracted by the carbon atom; consequently they will be equidistant from it, and the tetrahedron will be regular. If they are all different the force with which each is attracted will be different; they will arrange themselves at different distances from the carbon atom; and the tetrahedron will be irregular: it will have no plane of symmetry. Any compound of the formula CHX’Y’Z’ can there- fore exist in two enantiomorphs, applying this term to the molecules themselves— in two non-superposable forms, each of which is the mirror image of the other: thus— Fie. 1. Hig, 2. x’ nA Zz = H '\ \ \ Y’ y’ (In these figures no attempt has been made to represent the tetrahedra as irre~ gular; the opposite asymmetry is indicated merely by the opposite order of the four attached atoms or groups, In reality, however, they would be irregular, The carbon atom itself is not shown.) If we consider any particular set of three atoms or groups—for example, HI, Z’, and Y’—looking towards that face of the tetrahedron about which they are arranged, any order, thus HZ’ Y’, which is clockwise in one figure, will be counter- clockwise in the other. In like manner, a continuous curve, passing through the four atoms or groups in any given sequence, will form a right-handed helix in the one case and a left-handed helix in the other. We thus find that the foregoing _ assumptions—the very simplest that could be made—regarding the distribution of _ the four affinities of carbon and the different degree with which four different _ atoms or groups will be attracted by the carbon atom to which they are attached, lead to the asymmetric structures postulated by Pasteur to account for optical ee tame, enantiomorphous irregular tetrahedra, and right- and left-handed helices. Fic. 3. That a‘spiral arrangement, right- or left-handed, will produce rotation of the _ plane of polarisation in its own sense, may be shown by various experiments: thus in Reusch’s optically active piles of plates of mica, produced by crossing successive plates of biaxal mica at an angle of 60° to one another ; or in the twisted . . : V5 4 jute fibres recently described by Professor Bose, which, according to the direction *< /\ © © © 3G 2 ‘820 REPORT—1898. of the twist previously imparted to them, rotate the plane of polarisation of electrie waves either to the right or to the left. If two of the four atoms or groups attached to carbon are identical, there is no asymmetry, and no optical activity. ‘Thus, in a compound of the formula CH,X'Y’, which we may represent by our tetrahedral scheme as shown in fig. 3, the two hydrogen atoms are equidistant from the carbon atom; the system has a plane of symmetry passing through X’ Y’ and the carbon atom, and has therefore a superposable mirror image. lf the molecule contains only one asymmetric carbon atom, the latter may be either positive or negative, so that the substance may exist in two forms of opposite optical activity; in addition to which we may have the racemoid combination of the two, which will be inactive but separable. Mandelic acid, C,8,.CH(OH).COOH,} is a case in point: it is known in these three forms. CH(OH).COOH If, as in the case of tartaric acid, | , the molecule contains two CH(OH).COOH asymmetric carbon atoms, and at the same time consists of two structurally identical halves, then these two atoms may be either both positive or both nega- tive, reinforcing each other's effect in either case ; or one may be positive and the other negative, when, owing to the structural identity of the two halves of the molecule, the effect of the one will exactly compensate that of the other, and the compound will be inactive, but not separable. Furthermore, there may be the racemic combination of the bi-dextro- form with the bi-levo- form: a combination inactive, but separable. We have thus the explanation of the four forms observed by Pasteur. In fact, all the complex cases of isomerism that have been met with among compounds of this class—compounds structurally identical, but configuratively distinct, as it is termed—amay be satisfactorily explained, and their possible number accurately predicted, by means of the theory of the asymmetric carbon atom. I must apologise to the organic chemists among my audience for inflicting on them this very elementary exposition of what to them is a well-known theory. But outside the circle of organic chemists the theory is, I fear, far from well known. Thus, av eminent physicist, in his ‘Theory of Light,’ referring to the rotation of the plane of polarisation by liquid or dissolved substances, says: ‘ 1 am not aware that any explanation of it has ever been suggested.’ And in the ‘ Proceedings of the Royal Society ’ for the present year, another eminent physicist, after quoting with approval this purely personal confession, goes on to suggest the possibility of the molecules having a twisted structure, and points out that a right-handed twist ‘ would appear right-handed when looked at from either end,’ apparently unaware that such conceptions have been commonplaces of stereo- chemistry for the past quarter of a century at least. This brief sketch of the theory was therefore necessary in order that we may ed eres discuss Pasteur’s views on the relation between optical activity and life. Whenever we prepare artificially, starting either with the elements, or with symmetric compounds, any organic compound which, when it occurs as a natural product of the living organism, is optically active, the primary product of our laboratory reactions, however closely it may in other respects resemble the natural product, differs from it in being optically inactive. Pasteur was greatly impressed by this fact. In the Lectures delivered in 1860 he says: ‘ Artificial products have no molecular asymmetry; and I could not point out the existence of any more profound distinction between the products formed under the influence of life, and all others.’ And again, he refers to ‘the molecular asymmetry of natural organic products’ as ‘the great characteristic which establishes perhaps the only well- marked line of demarcation that can at present be drawn between the chemistry of dead matter and the chemistry of living matter.’ He would not admit that even racemoid forms, optically inactive by intermolecular compensation, might be ? The asymmetric carbon atom is represented by an italic C. : ‘ . TRANSACTIONS OF SECTION B. 821 artificially prepared; thus, to the suggestion that the malic acid which he had ob- tained from Dessaignes’s artificial aspartic acid might possibly be the racemoid form (as we now know that it is), he replied : ‘That is improbable, for then not only should we have made an active body from an inactive one, but we should have made two —a right and a left.’ The view that racemoids could not be prepared artificially did not long remain tenable. In 1860, the year in which the foregoing lectures were delivered, Perkin and Duppa, and, independently, Kekulé, obtained from dibromsuccinic acid a form of tartaric acid which Pasteur recognised as racemic acid. But the succinic acid employed had been prepared from amber, a substance of vegetable origin; and there was still the possibility that herein lay the source of the optical activity of the two constituents of the artificial racemic acid. This objection, which was raised by Pasteur himself, fell to the ground when, in 1873, Jungfleisch prepared racemic acid from Maxwell Simpson’s synthetic succinic acid, and separated it into its right and left constituents by means of the sodium ammonium salt. ‘Thus falls the barrier,’ wrote Schiitzenberger, ‘ which M. Pasteur had placed between natural and artificial products. This example shows us how reserved we must be in attempting to draw distinctions between the chemical reactions of the living organism and those of the laboratory.’ To these words, which, although written a quarter of a century ago, may fairly be taken as representing the prevailing belief of chemists at the present day, Pas- teur aeplied as follows: ‘Contrary to M. Schiitzenberger’s belief, this barrier still exists. . . . To trans- form one inactive compound into another inactive compound which has the power of resolving itself simultaneously into a right-handed compound and its opposite (son symétrique), is in no way comparable with the possibility of transforming an tnactive compound into a single active compound. This is what no one has ever done ; it is, on the other hand, what living Nature is doing unceasingly before our eyes. On this and subsequent occasions Pasteur did little more than reiterate opinions which he had previously expressed. As he himself stated, he was then occupied with other problems which absorbed his entire time and energies. ‘The result has been that the opinions have suffered neglect and even misrepresentation. Thus Ostwald, in his ‘ Allgemeine Chemie,’ translating, or rather paraphrasing, the fore- going passage, omits the word ‘ single "—which is the key to Pasteur’s meaning— and then condemns the statement as illogical. Pasteur’s point is, that whereas living Nature can make a single optically active compound, those laboratory reactions, to which we resort in synthesising such compounds, always produce, simultaneously, at least two, of equal and opposite optical activity; the result being intermolecular compensation and consequent Optical inactivity. Not necessarily implied in Pasteur’s statement, but entirely in harmony with it, is the fact that we can sometimes produce artificially a single compound containing within its molecule two equal and opposite asymmetric groups, and therefore inactive by iztramolecular compensation ; thus in the oxida- tion of maleic acid to mesotartaric acid. Let us consider the cause of this limitation of our synthetic reactions. Why cannot we produce, by laboratory processes, involving the play of symmetric forces and the interaction of symmetric atoms and molecules, sizgle optically active com- pounds? To answer that question, let us turn our attention to the mechanism of the change in which a symmetric carbon atom becomes asymmetric. A simple case of such a change, typical of all similar changes, is the transfor- _ mation of a compound, CH,X’Y’, by substitution, into CHX’Y’Z’. If we follow this process by means of our tetrahedral model, we see at once why, in our ordinary laboratory reactions, both enantiomorphs must be generated in equal quantity. The molecule of the compound, CH,X’Y’, of which the tetrahedral representation is given in fig. 3, has, as we have already seen, a plane of symmetry passing through X’Y’ and the carbon atom; and from this plane of symmetry the two hydrogen atoms are equidistant on opposite sides. Any purely mechanical, 822 REPORT—1898. symmetrie force, therefore—any force, for example, such as comes into play in the motions of the symmetric molecules of a gas or a liquid—which affects one of these hydrogen atoms in one molecule of the compound CH,X’Y’, has an equal chance of affecting the other hydrogen atom in another molecule. If the right-hand hydrogen atom in fig. 3 is replaced by the radicle Z’, we obtain the enantiomorph represented in fig. 1; if the left-hand hydrogen atom, that represented in fig. 2. The chances in favour of these two events being equal, the ratio, : Number of occurrences of event I. Number of occurrences of event II. will, if we are dealing with an infinitely great number of molecules, approximate to unity. We therefore obtain a mixture, optically inactive by intermolecular compensation. All cases of the conversion of symmetric into asymmetric compounds may be referred to the same category, no matter whether the chemical process is one of substitution or of addition, or whether the resulting molecule contains one or more asymmetric carbon atoms. Thus, in the reduction of a ketone of the formula X’.CO.Y’ to a secondary alcohol of the formula X’.CH(OH).Y’ ; in the transforma- tion of an aldehyde by the addition of hydrocyanic acid into a nitrile of an a-hydroxy-acid ; in the oxidation of fumaric acid to racemic acid—cases typifying the various additive processes in which asymmetric groupings are produced—there is one condition common to all: in the symmetric compound, with which we start, there are, in every case, two identical points of attack, equidistant from the plane of symmetry of the molecule, and the result is that the two possible events happen in equal number, so that the mixture of enantiomorphs obtained is optically in- active by compensation. We are, of course, in many cases able afterwards to separate these enantiomorphs by the methods devised by Pasteur, and thus obtain the single optically active compounds; but we cannot produce them singly as long, as we have at our disposal only the symmetric forces which we command in the laboratory. Precisely the same state of things prevails when symmetric molecules unite, under the influence of symmetric forces, to build up an asymmetric crystalline structure. When, for example, sodium chlorate crystallises from its aqueous solu- tion, the number of right-handed crystals is, on the average, as was shown by Kipping and Pope, equal to the number of left-handed crystals. The same fact was proved by Landolt by observing the optical inactivity of the mixture of micro- scopic right and left crystals obtained by adding alcohol to a concentrated aqueous solution of sodium chlorate. The two possible asymmetric events occur in equal number. Non-living, symmetric forces, therefore, acting on symmetric atoms or mole- cules, cannot produce asymmetry, since the simultaneous production of two oppo- site asymmetric halves is equivalent to the production of a symmetric whole, whether the two asymmetric halves be actually united in the same molecule, as in the case of mesotartaric acid, or whether they exist as separate molecules, as in the left and right constituents of racemic acid. In every case, the symmetry of the whole is proved by its optical inactivity. The result is entirely different, however, when we allow symmetric forces to act under the influence of already existing asymmetric, non-racemoid compounds. Thus, if we start with an optically active compound—a compound containing one or more asymmetric carbon atoms and non-racemoid—and, by appropriate chemical reactions, render asymmetric some carbon atom in the compound which was not previously so, then it does not follow that the two forms represented by the two possible arrangements of this new asymmetric carbon atom will be pro- duced in equal quantity. The compound with which we start has no plane of symmetry ; and, although there are still the two possible points of attack, one will be more exposed than the other; in fact, one mode of attack may so predominate that apparently only one asymmetric compound is formed, the other compound, if formed at all, escaping detection by the smallness of its amount. A case in point TRANSACTIONS OF SECTION B. 823° is the conversion of d-mannose by combination with hydrocyanic acid into the’ nitrile of d-mannoheptonic acid, studied by Emil Fischer, in which only one nitrile’ is formed, although there are two ways in which the hydrocyanic acid may attach: itself to the aldehyde group of the mannose. On the other hand, the same general reaction, in the union of hydrocyanic acid with ordinary aldehyde CH,.CHO —a symmetric compound —yields the right and left forms of lacto-nitrile’ CH,.CH(OH).CN in equal quantity, the two asymmetric events occurring in’ equal number, and the resulting mixture of compounds being inactive. It is the difference between guidance and no guidance: the asymmetric group present in the mannose guides into a particular path the symmetric forces which bring about: the addition of the hydrocyanic acid ; in the case of the symmetric aldehyde the result is left to pure chance. The latter action is like that of tossing a perfectly balanced coin; in the former the coin is heavily weighted on one side. ‘The say- ing, ‘les dés de la Nature sont pipés, is certainly true of living Nature and its products. ; This guiding action displayed by asymmetric compounds may even impart a bias to the crystallisation of those molecularly symmetric substances already referred to, which crystallise in enantiomorphous forms. Thus, Kipping and Pope have recently made the interesting observation that the crystals of sodium chlorate which are deposited from an aqueous solution containing 200 grams of d-glucose to the litre consist, on an average, of about 32 per cent. of right-handed to 68 per cent. of left-handed crystals, the asymmetric carbohydrate, by its mere presence, favouring the formation of the one asymmetric form of the inorganic salt at the expense of the other. These observations possibly afford a clue to the mode of action of the living organism in producing single enantiomorphs. ‘This production of single asym- metric forms may be a result of the asymmetric character of the chemical com- pounds of which the tissues of plants and animals are built up. ‘The optically active products of the organism—the carbohydrates, the terpenes, tartaric acid, asparagine, quinine, the serum of the blood, and countless others—have been formed in an asymmetric environment, and their asymmetry is an induced pheno- menon. They have been cast, as it were, in an asymmetric mould. According to this view they are a result of the selective production of one of the two possible enantiomorphous forms. The same would hold good with regard to the organised tissues themselves, developed from inherited asymmetric beginnings in the ovum or the seed, or obtained by fission. The perplexing question of the absolute origin of these asymmetric compounds I will discuss later. Another view has been put forward by Emil Fischer. In his lecture on ‘Syntheses in the Sugar Group,’ delivered before the German Chemical Society in 1890, he says: ‘Starting with formaldehyde, chemical synthesis leads, in the first instance, to the optically inactive acrose. In contradistinction to this only the active sugars of the d-mannitol series have hitherto been found in plants. ‘ Are these the only products of assimilation [of carbon dioxide and water]? Is the preparation of optically active substances a prerogative of the living organism ; is a special cause, a kind of vital force, at work here? I do not think so, and incline rather to the view that it is only the imperfection of our knowledge which imports into this process the appearance of the miraculous. ‘No fact hitherto known speaks against the view that the plant, like chemical _ synthesis, first prepares the inactive sugars; that it then resolves them into their active constituents, using the members of the d-mannitol series in building up starch, cellulose, inulin, &c., whilst the optical isomerides serve for other purposes at present unknown to us.’ There are, therefore, two opposite processes which would account for the pre- sence of optically active compounds among the substances generated in the living organism, and which we may briefly describe as selective production and selective consumption. An instance of artificial selective production is the formation of only one nitrile of d-mannoheptonic acid already cited. Selective consumption, §24. REPORT—1898. dissociated, however, from the previous production of the racemoid form, may be illustrated by the fermentation of-dextro-tartaric acid in the action, studied by Pasteur and already referred to, of a mould on racemic acid, the levo- tartaric acid remaining untouched, and by numerous similar fermentations since discovered. Selective consumption is not restricted to living ferments; various cases are known of enzymes, or soluble ferments, which can effect the hydrolysis of one glucoside, but not of its enantiomorph. As Emil Fischer, who studied this phenomenon, says: ‘ nzyme and glucoside must fit each other like key and lock, in order that the one may exercise a chemical action on the other. And a similar selective action, embracing the much more complex phenomenon of alcoholic fer- mentation, is displayed by E. Buchner’s soluble zymase obtained from yeast cells. It is true, moreover, that the organism sometimes produces both enantiomorphs. Thus the lactic ferment converts carbohydrates into racemoid lactic acid ; ordinary, or levo-rotatory, asparagine is accompanied in plants, as Piutti showed, by a small quantity of its optical isomeride; and there are other cases. _ These facts might be taken as evidence in favour of Fischer's view that selec- tive consumption is the cause of the phenomenon we are discussing. But I do not think that, in the present state of our knowledge, we can decide between the two views. For that matter both may be correct, each may explain particular cases. What I wish to point out is that Fischer's statement that the ‘ miraculous’ character of the phenomenon is eliminated by his assumption appears open to question. It is just as much, or as little, miraculous after as before. The pro- duction of a single asymmetric form, and the destruction of one of two opposite asymmetric forms, are problems of precisely the same order of difficulty, and there are only two ways in which either of thera has ever been solved: firstly, by the direct action of living matter, and, secondly, by the use of previously existing asymmetric non-racemoid compounds, which are, in the last resort, due to the action ot life. Directly or indirectly, then, life intervenes. Doubtless this will appear a very extraordinary statement in view of Jung- | fleisch’s synthesis of racemic acid and its resolution into dextro- and levo-tartaric acids by the crystallisation of the sodium ammonium salts. The process does not take place in a living organism; nor is the aid of life invoked in the shape of a micro-organism as in Pasteur’s third method of separation. No asymmetric base of vegetable origin is employed as in Pasteur’s second method, so that the indirect action of life through its products is also excluded; sodium and ammonium are symmetric inorganic radicles, and no substance of one-sided asymmetry is intro- duced from beginning to end. ‘The process is one of ordinary crystallisation; the two forms are deposited side by side, the operator afterwards picking out the right and left crystals and separating them. The reason why the two tartrates crystal- lise out and not the racemate, is that at the ordinary temperature of the air at which the crystallisation is conducted they are less soluble than the racemate. At a higher temperature, on the other hand, these solubilities are reversed and the racemate is deposited. The conditions are precisely those which govern the forma- tion or non-formation of ordinary double salts. Consequently, the overwhelming majority of chemists hold that the foregoing synthesis and separation of optically active compounds have been effected without the intervention of life, either directly or indirectly. Every manual of stereo- chemistry emphasises this point. I have already hinted that I hold a contrary opinion. I have held it for some time, but have not ventured to give public expression to it, except in lecturing to my students. I was deterred chiefly by the impression that I stood alone in my belief. I find, however, that this was a mistaken impression. In a lecture on ‘Pasteur as the Founder of Stereochemistry, which Professor Crum Brown delivered before the Franco-Scottish Society in July 1897, and which is published in the ‘ Revue francaise d’Edimbourg,’ he says, referring to the separation of enantiomorphs by crystallisation :— _‘ The question has often occurred to me: Do we here get rid of the action of a living organism ? Is not the observation and deliberate choice by which a human being picks out the two kinds of crystals and places each in a yessel by itself the ————— ee SS—~—~S~S—s—ste TRANSACTIONS OF SECTION B. 825 specific act of a living organism of a kind not altogether dissimilar to the selection made by Penicillium glaucum? But I do not insist on this, although I think it is not unworthy of consideration.’ It is this question, so precisely posed by Professor Crum Brown, that I would discuss in detail. I think we shall find that the answer to it will be in the sense which he indicates. The action of life, which has been excluded during the previous stages of the process, is introduced the moment the operator begins to pick out the two enantiomorphs. It will doubtless be objected that, if this is the case, there can be no such thing as a synthesis of a naturally occurring organic compound without the intervention of life, inasmuch as the synthetic process is always carried out by a living operator. Here, however, we must draw an important distinction. In the great majority of the operations which we carry out in our laboratories—such as solution, fusion, vaporisation, oxidation, reduction and the like—we bring to bear upon matter symmetric forces only—forces of the same order as those involved in the chance motions of the molecules of a liquid or agas. All such processes, therefore, might conceivably take place under purely chance conditions, without the aid of an operator at all. But there is another class of operations, to which Pasteur first drew attention: those into which one-sided asymmetry enters, and which deal either with the production of a single enantiomorph, or with the destruction (or change) of one enantiomorph in a mixture of both, or with the separation of two enantiomorphs from one another. We have already seen that such processes are possible only under one-sided asymmetric influences, which may take the form either of the presence of an already existing enantiomorph, or of the action of a living organism, or of the free choice of an intelligent operator. They cannot conceivably occur through the chance play of symmetric forces. We must, therefore, in classifying the actions of the intelligent operator, dis- tinguish between those actions in which his services might conceivably be dispensed with altogether and those in which his intelligence is the essential factor. To the former class belongs the carrying out of symmetric chemical reactions; to the latter, the separation of enantiomorphs. Take the synthesis of formic acid—a symmetric compound—by the absorption of carbon monoxide by heated caustic alkali. Given a forest fire and such natu- rally occurring materials as limestone, sodium carbonate, and water, it would not be difficult to imagine a set of conditions under which a chance synthesis of sodium formate from inorganic materials might occur. Ido not assert that the condi- tions would be particularly probable ; still, they would not be inconceivable. But the chance synthesis of the simplest optically active compound from inorganic materials is absolutely inconceivable. So also is the separation of two crystallised enantiomorphs under purely symmetric conditions. The picking out of the two enantiomorphs is, moreover, to be distinguished from the process of similarly separating the crystals of two different non-enantio- morphous substances, although this distinction is commonly ignored by classing both processes together as mechanical, in opposition to chemical separations. In the case of the non-enantiomorphs there may be differences of solubility, of specific gravity and the like; so that other means of separation, involving only the play of symmetric forces, may be resorted to. Such a process may justly be regarded as ‘mechanical.’ But the two crystallised enantiomorphs, as we have seen, have the same solubility—at least in symmetric solvents; the same specific gravity ; behave, in fact, in an identical manner towards all symmetric forces ; so that no separa- tion by such means is feasible. It requires the living operator, whose intellect embraces the conception of opposite forms of asymmetry, to separate them. Such & process cannot, by any stretch of language, be termed ‘ mechanical.’ Conscious selection here produces the same result as the unconscious selection exercised by the micro-organism, the enzyme, or the previously existing asymmetric compound. I need not point out that if the operator chooses to bring about the separation by an asymmetric solvent, or some other asymmetric means, he is still making use of his conception of asymmetry. He merely effects his end indirectly instead of 826 REPORT—1898, . directly. But in either case he exercises a guiding power which is akin, in its’ results, to that of the living organism, and is entirely beyond the reach of the symmetric forces of inorganic nature. In like manner, it is not of the least consequence, for the purposes of the present argument, whether the micro-organism, with which we have compared the operator, ' acts directly in fermenting one of two enantiomorphs, or whether it acts indirectly by first preparing an asymmetric enzyme which displays this selective action. The contention, therefore, of EK. Fischer, Buchner, and others, that the discovery: of enzymes and zymases ‘has transferred the phenomena of fermentation from biological to purely chemical territory, is true only as regards the immediate process, and leaves intact the vitalistic origin of these phenomena. We thus arrive at the conclusion that the production of single asymmetric compounds, or their isolation from the mixture of their enantiomorphs, is, as Pasteur firmly held, the prerogative of life. Only the living organism with its asymmetric tissues, or the asymmetric products of the living organism, or the living intelligence with its conception of asymmetry, can produce this result. Only asymmetry can beget asymmetry. Is the failure to synthesise single asymmetric compounds without the inter- vention, either direct or indirect, of life due to a permanent inability, or merely to a temporary disability which the progress of science may remove? Pasteur took the latter view, and suggested that the formation of chemical compounds in the magnetic field, or under the influence of circularly polarised light, would furnish a means of solving the problem; and Van’t Hoff also thinks the latter method feasible. As regards magnetism, Pasteur’s suggestion was undoubtedly based on a misconception; the magnetic field has not an asymmetric structure; it is merely polar, since the rotation which it produces in the plane of polarisation of a ray of light changes sign with the direction of the field. As regards circularly polarised light, I must confess to having doubts as to whether it can be regarded as an asymmetric phenomenon: the motion of the ether about the axis of the ray is ' circular, not spiral; and it is only by considering the difference of phase from point to point along the ray that the idea of a spiral can be evolved from it. In tact, are there such things as forces asymmetric in themselves? Is the geometrical conception of asymmetry applicable to dynamical phenomena at all, except in so far as these deal with asymmetric material structures, such as quartz crystals, or organic molecules containing asymmetric carbon atoms? But this is a question which I would submit to the judgment of mathematical physicists. One thing is certain—namely, that all attempts to form optically active com- pounds under the influence of magnetism or circularly polarised light have hitherto signally failed. These forces do not distinguish between the two equally exposed points of attack which present themselves in the final stage of the transformation of a symmetric into an asymmetric carbon atom. But even if such an asymmetric force could be discovered—a force which would enable us to synthesise a single enantiomorph—the process would not be free from the intervention of life. Such a force would necessarily be capable of acting in two opposite asymmetric senses ; left to itself it would act impartially in either sense, producing. in the end, both enantiomorphs in equal amount. Only the free choice of the living operator could direct it consistently into one of its two possible channels. I will briefly recapitulate the conclusions at which we have arrived. Non- living, symmetric matter—the matter of which the inorganic world is composed— interacting under the influence of symmetric forces to form asymmetric compounds, always yields either pairs of enantiomorphous molecules (racemoid form), or pairs | of enantiomorphous groups united within the molecule (meso-form), the result being, in either case, mutual compensation and consequent optical inactivity. The same will hold good of symmetric matter interacting under the influence of asymmetric forces (supposing that such forces exist) provided that the latter are left. to produce their effect under conditions of pure chance. If these conclusions are correct, as I believe they are, then the absolute origin of the compounds of one-sided asymmetry to be found in the living world is a mystery EE. rl rrr CO rr™™—S TRANSACTIONS OF SECTION B. 827 as profound as the absolute origin of life itself. The two phenomena are intimately connected, for, as we have seen, these symmetric compounds make their appearance with life, and are inseparable from it. How, for example, could levo-rotatory protein (or whatever the first asymmetric compound may have been) be spontaneously generated in a world of symmetric matter and of forces which are either symmetric or, if asymmetric, are asymmetric in two opposite senses? What mechanism could account for such selective pro- duction? Or if, on the other hand, we suppose that dextro- and leevo-protein were simultaneously formed, what conditions of environment existing in such a world could account for the survival of the one form and the disappearance of the other ? Natural selection leaves us in the lurch here; for selective consumption is, under these conditions, as inconceivable as selective production. No fortuitous concourse of atoms, even with all eternity for them to clash and combine in, could compass this feat of the formation of the first optically active organic compound. Coincidence is excluded, and every purely mechanical explana- tion of the phenomenon must necessarily fail. I see no escape from the conclusion that, at the moment when life first arose, a directive force came into play—a force of precisely the same character as that which enables the intelligent cperator, by the exercise of his Will, to select one crystallised enantiomorph and reject its asymmetric opposite. I would emphasise the fact that the operation of a directive force of this nature does not involve a violation of the law of the conservation of energy. Enantio- morphs have the same heat of formation; the heat of transformation of one form into the other is nil. Whether, therefore, one enantiomorph alone is formed, or its optical opposite alone, or a mixture of both, the energy required per unit weight of substance is the same. There will be no dishonoured drafts on the unalterable fund of energy. The interest of the phenomena of molecular asymmetry from the point of view of the biologist lies in the fact that they reduce to its simplest issues the question of the possibility or impossibility of living matter originating from dead matter by a purely mechanical process. They reduce it to a question of solid geometry and elementary dynamics; and therefore, if the attempted mechanical explanation leads to a reductio ad absurdum, this ought to be of a correspondingly simple and convincing character. Let us see how far this is the case. Life is a phenomenon of bewildering complexity. But in discussing the problem of tke origin of life this complexity cuts two ways. Whilst, on the one hand, it is appealed to by one set of disputants as an argument against the mechanical theory, on the other it affords shelter for the most unproved statements of their opponents. I will take a concrete instance from the writings of an upholder of the mechanical theory of the origin of life, the late Professor W. K. Clifford. He says: ‘Those persons who believe that living matter, such as protein, arises out of non-living matter in the sea, suppose that it is formed like all other chemical com- pounds. That is to say, it originates in a coincidence, and is preserved by natural selection. . . . The coincidence involved in the formation of a molecule so complex as to be called Ziving, must be, so far as we can make out, a very elaborate coincidence. But how often does it happen in a cubic mile of sea-water? Per- haps once a week; perhaps once in many centuries; perhaps, also, many million times a day. From this living molecule to a speck of protoplasm visible in the microscope is a very far cry; involving, it may be, a thousand years or so of evolution.’ It was easy for Clifford to write thus concerning life itself, for it was difficult for any one to contradict him. But had he been asked whether any mechanical (symmetric) coincidence would suffice to convert an infinitely great number of molecules of the type shown in fig. 8 into that shown in (say) fig. 1, to the exclu- sion of that shown im fig. 2; or whether, given a mixture, in equal proportions, of molecules of the types shown in figs. 1 and 2, any mechanical (symmetric) condi- tions of environment would bring about the destruction of one kind and the $28 é REPORT—1898. survival of the other, I think his exact mathematical and dynamical knowledge would have prevented him from giving an affirmative answer. But short of this aflirmative answer, his other statements, it seems to me, fall to the ground. I am convinced that the tenacity with which Pasteur fought against the doctrine of spontaneous generation was not unconnected with his belief that chemical compounds of one-sided asymmetry could not arise save under the influence of life. Should any one object that the doctrine of the asymmetric carbon atom is a somewhat hypothetical foundation on which to build such a superstructure of argument as the foregoing, I would point out that the argument is in reality independent of this doctrine. All that I have said regarding the molecular asymuetry of naturally occurring optically active organic compounds, and all the geometrical considerations based thereon, hold good equally of the hemihedral erystalline forms of these compounds, about which there is no hypothesis at all. The production of a compound crystallising in one hemihedral form to the exclu- sion of the opposite hemihedral form, as in the case of the tartaric acid of the grape, is a phenomenon inexplicable on the assumption that merely mechanical, symmetric forces are at work. Nor is this conclusion invalidated even if we ultimately have to admit that the connection between molecular and crystalline asymmetry is not an invariable one—a point about which there is some dispute. At the close of the lectures from which I have so frequently quoted, Pasteur, with full confidence in the importance of his work, but without any trace cf personal vanity, says :— ‘It is the theory of molecular asymmetry that we have just established—one of the most exalted chapters of science. It was completely unforeseen, and opens to physiology new horizons, distant but sure.’ J must leave physiologists to judge how far they have availed themselves of the new outlook which Pasteur opened up to them. But if I have in any way cleared the view towards one of these horizons, I shall feel that I have not occupied this chair in vain. Some of my hearers, however, may think that, instead of rendering the subject clearer, I have brought it perilously near to the obscure region of metaphysics ; and certainly, if to argue the insufficiency of the mechanical explanation of a phe- nomenon is to be metaphysical], I must plead guilty to the charge. I will, there- fore, appeal to a judgment—metaphysical, it is true, but to be found in a very exact treatise on physical science—namely, Newton's ‘Principia.’ It has a marked bearing on the subject in hand :— “A ceca necessitate metaphysica, que utique eadem est semper et ubique, nulla oritur rerum variatio,’ _ Iwill merely add that this is certainly true of the particular rerwm variatio in which optically active organic compounds originate. The following Papers and Reports were read :— 1. On the Extraction from Air of the Companions of Argon and on Neon. By Witu1aM Ramsay and Morris W. Travers. In the Presidential Address to the Chemical Section of this Association, delivered last year at Toronto, it was pointed out that the densities of helium and argon being respectively 2 and 20 in round numbers, and the ratio of their specific heats being in each case 1:66, their atomic weights must be respectively 4 and 40. If the very probable assumption is made that they belong to the same group of elements, it appears almost certain on the basis of the Periodic Table that another element should exist, having an atomic weight higher than that of helium by about 16 units, and lower than that of argon by about 20. There is also room for ———————— eet TRANSACTIONS OF SECTION B. 829 elements of higher atomic weight than argon, belonging to the same series. The search for this element was described in last year’s Address, and, it will be remem- bered, the results were negative. Reading between the lines of the Address, an attentive critic might have noticed that no reference was made to the supposed homogeneity of argon. From speculations of Dr. Johnstone Stoney, it would follow that the atmosphere of our planet might be expected to contain new gases, if such exist at all, with densities higher than 8 or thereabouts. Dr. Stoney gives his reasons for supposing that the lighter the gas the less its quantity in our atmosphere, always assuming that no chemical compounds are known which would retain it on the earth, or modify its relative amount. Therefore it appeared worthy of inquiry whether it was possible to separate light and also heavy gases from argon. The beautiful machine invented by Dr. Hampson has put it in our power to obtain, through his kindness and that of the ‘Brin’ Oxygen Company, large quantities of liquid air. We were therefore able to avail ourselves of the plan of liquefection, and subsequent fractional distillation, in order to separate the ases. On liquefying 18 litres of argon, and boiling off the first fraction, a gas was obtained of density 17 (O=16). This gas was again liquefied and boiled off in six fractions. The density of the lightest fraction was thus reduced to 13:4, and it showed a spectrum rich in red, orange, and yellow lines, differing totally from that of argon. On re-fractionating, the density was reduced further to 10°8; the gas still contained a little nitrogen, on removing which the density decreased to 9°76. This gas is no longer liquefiable at the temperature of air boiling under a pressure of about 10 millimetres ; but if, after compression to two atmospheres, the pressure was suddenly reduced to about a quarter of an atmosphere, a slight mist was visible in the interior of the bulb. This gas must necessarily have contained argon, the presence of which would obviously increase its density ; and in order to form some estimate of its true density, some estimate must be made of the relative amount of the argon. We have to consider a mixture of neon, nitrogen, and argon, the two latter of which are capable, not merely of being liquefied, but of being solidified without difficulty. Under atmospheric pressure nitrogen boils at —194°, and solidifies at —214°, and the boiling-point of argon is —187°, and the freezing-point — 190°; the vapour-pressure of nitrogen is therefore considerably higher than that of argon. The mist produced on sudden expansion consisted of solid nitrogen and argon; and for want of better knowledge, assuming the vapour- pressure of the mixture of nitrogen and argon to be the sum of the partial pressures of the two, it is obvious that that of argon would form but a small fraction of the whole. The vapour-pressure of argon was found experimentally to be 109 milli- metres at the temperature of air boiling in as good a vacuum as could be produced by our pump; but as we have only to consider the partial pressure of the argon at a much lower temperature, we do not believe that the pressure of the argon can exceed 10 millimetres in the gas. This would correspond to a density for neon of 96, The ratio between the specific heat at constant pressure and constant volume was determined for neon in the usual way, and, as was to be expected, it approximates closely to the theoretical ratio, being 1°655. We therefore conclude that, like helium and argon, the gas is monatomic. It may be remembered that the refractivity of helium compared with that of air is exceptionally low—viz.,.0:1238. The lighter gas, hydrogen, has a refractivity of 04733. It was to be expected from the monatomic character and low density of neon that its refractivity should be also low; this expectation has been realised, for the number found is 03071. Argon, on the other hand, has a refractivity not differing much from that of air—viz., 0'958. Since the sample of neon certainly contains a small amount of argon, its true refractivity is probably somewhat lower. Experiments will be carried out later to ascertain whether neon resembles helium in its too rapid rate of diffusion. The spectrum of neon is characterised by brilliant lines in the red, the orange, and the yellow. The lines in the blue and violet are few, and comparatively 830 , REPORT-—1898. inconspicuous. There is, however, a line in the green, of approximate wave-length 5,030, and another of about 5,400. A few words may be said on the other companions of argon. The last fractions of liquetied argon show the presence of three new gases. These are krypton, a gas first separated from atmospheric air, and characterised by two very brilliant lines, one in the yellow and one in the green, besides fainter lines in the red and orange; metargon, a gas which shows a spectrum very closely resembling that of carbon monoxide, but characterised by its inertness, for it is not changed by sparking with oxygen in presence of caustic potash ; and a still heavier gas, which we have not hitherto described, which we propose to name ‘xenon.’ Xenon is very easily separated, for it possesses a much higher boiling-point, and remains behind after the others have evaporated. This gas, which has been obtained practically free from krypton, argon, and metargon, possesses a spectrum analogous in character to that of argon, but differing entirely in the position of the lines. With the ordinary discharge the gas shows three lines in the red, and about five very brilliant lines in the blue; while with the jar and spark-gap these lines dis- appear, and are replaced by four brilliant lines in the green, intermediate in position between the two groups of argon lines, the glow in the tube changing from blue to ereen. Xenon appears to exist only in very minute quantity. Indeed, all of these gases are present only in small amount. It is, however, not possible to state with any degree of accuracy in what proportion they are present in atmospheric argon. Of neon, perhaps, we may say that the last fraction of the lightest hundred cubic centimetres from 18 litres of atmospheric argon no longer shows the neon spectrum, and possesses the density of argon; it may be safe to conclude, therefore, that 18 litres of argon do not contain more than 50 cubic centimetres of neon ; the proportion of neon in air must therefore be about one part in 40,000. We should estimate the proportion of the heavy gases at even less, It follows from these remarks that the density of argon is not materially changed by separating from it its companions. A sample of gas, collected when about half the liquid argon or about 10 cubic centimetres had boiled off, possessed the density 19:89; the density of atmospheric argon is 19°94, But, of course, we give this density of argon as only provisional;' for a final determination the density must be determined after more thorough fractionation. With a density of 9°6, and a consequent atomic weight of 19:2, neon would iollow fluorine and precede sodium in the Periodic Table; as to the other gases, further research will be required to determine what position they hold. [October 10, 1898.—The sample of neon alluded to above has since been found to contain a small trace of helium. The presence of this light gas has no doubt made the density of neon given in this communication somewhat too low. The actual density has not yet been determined, but the density will obviously not be materially altered W. R. ] j 2. On the Position of Heliwm, Argon, Krypton, &c., in the Pervodic Classification of the Elements. By Professor J. Emerson REYNOLDS, ERS. 3. Report on the Electrolytic Methods of Quantitative Analysis. See Reports, p. 294. 4, A new form of Stand for Electrolytic Analysis. By Dr. Hueu MarsHaAtt. 5. Report on the Continwation of the Bibliography of Spectroscopy. See Reports, p. 439. 1 July 30, 1898, as OE EE ha Fea ~ TRANSACTIONS OF SECTION B. 851 FRIDAY, SEPTEMBER 9. The following Papers and Report were read :— 1. Some Researches on the Thermal Properties of Gases and Liquids. By Sxpney Youne, D.Sc., F.R.S., University College, Bristol. Gases under moderate or low pressures are characterised by the simplicity of the laws relating to the variation of their volume with temperature and pressure. But when the pressure is greatly increased, these laws no longer hold good ; at constant temperature the product pv, instead of remaining constant, diminishes until a minimum is reached, and at still higher pressures increases again, and this increase continues up to the highest pressures that have been reached. A most important advance in the explanation of the behaviour of compressed gases and of liquids was made just twenty-five years ago by Van der Waals, who, taking into account the two facts (1) that the molecules of a gas attract one another, (2) that they occupy a finite volume, and are not mere mathematical points, proposed the formula (>+ 5) (v—b) =RT in place of the simple one pu=RT. The formula of Van der Waals expresses very well the general relations of pressure, temperature, and volume for both gases and liquids, but does not give the actual values with sufticient accuracy, and many attempts have been made to alter it in such a way as to bring about a better agreement. It is noticeable that at constant volume the formula becomes p=KT—c, where K and e¢ are constants, depending on the volume, and this simple relation has been found to hold good for gases by Amagat, and for both gases and liquids by Ramsay and myself. Within the last tew years I have investigated the behaviour of a hydrocarbon, isopentane,’ through a very wide range of volume (1‘6—4000 cc. per gram), and of normal pentane through a _ smaller range, and the data so obtained have led Rose-Innes ? to a formula -’ Re iia) 4 ence ti hos kago4| — tae, based on the simple one y= KT—c, which reproduces the observed isothermals from the largest volume to about 3°4 c.c. per gram, with a maximum error of slightly over 1 per cent. A complete investigation of this kind requires, however, a large amount of time, and can only be carried out with very stable substances of comparatively low critical temperatures; and it occurred to me about eleven years ago that a careful study of certain generalisations, deduced by Van der Waals from his formula, might yield valuable results, and perhaps indicate the direction in which the formula requires alteration. The generalisations may be stated thus :—If any two substances, A and B, are compared at pressures, P, and P,, proportional to their critical pressures, 7,, and 7,,, their boiling points (absolute temperatures), T, and '[, will be propor- tional to their critical temperatures, 6,, and 6,,, and their volumes, both as liquid, V, and V;, and as saturated vapour, x, and v,, will be proportional to their critical volumes, $., and doy. It would follow from this that at ‘ corresponding’ pressures the ratios of the actual to the theoretical density of saturated vapour, —————————— eS ,trt—t—i‘S— :. . should be the same for all substances. : It is convenient to speak of the ratio of the pressure to the critical pressure as _ the ‘reduced’ pressure, 7, the actual pressures, P,, P,, being called ‘ correspond- ing’ pressures. is ' Proc. Phys. Soc. vol. xiii. p. 602. ; Tbid., vol. xv. p. 126 ; vol. xvi. p. 11, 832 REPORT—1898. I proposed, therefore, to determine the vapour pressures and the specific volumes (both as liquid and as saturated vapour) of a considerable number of substances from low temperatures to their critical points, and in the first place I chose some compounds of elements belonging to the same group in the periodic table, as it seemed possible that some points of interest might thus arise. The first substances I examined were the four monohaloid derivatives of benzene, as well as benzene itself,' and the result of the investigation was to show that, when the haloid derivatives are compared together, the generalisation, as regards tempera- ture and pressure, hold good accurately ; hut there is this peculiarity about these compounds, that their critical pressures are equal, or very nearly so, and therefore ‘corresponding’ pressures are in this case equal pressures, The critical pressure of benzene itself is different, and when the hydrocarbon is compared with any of its haloid derivatives, the differences between the temperature ratios are much greater. As regards the volume ratios, the differences are small in all cases. The only other substances, bearing on the periodic arrangement of the elements, which have been yet examined are the tetrachlorides of carbon and tin.? The critical pressures differ considerably, and the relationship resembles _ that of the normal paraffins to each other, which will be referred to later. Many of the chlorides of the elements are very hygroscopic, and attack mercury at high temperatures, and it was thought better to postpone their further examina- tion, and to obtain the data for a few series of homologous organic compounds, Up to the present, in addition to the three lowest alcohols, investigated by Ramsay and myself, ten esters* and four paraffins * have been studied, and with the exception of the alcohols it has been observed in every case (and the same remark applies to the tetrachlorides of carbon and tin), that the ratios a at any . . . . 7 . 0, . . reduced pressure increase with rise of molecular weight. No definite relation is observable between the molecular weights and the ratios a and —. in the case of : 0 i) the esters, but with the three normal paraffins (pentane, hexane,and heptane) and the two tetrachlorides, the ratios _" increase and — diminish slightly with rise ) tt) of molecular weight. With the alcohols, on the other hand, the ratios e and i) Vv : Cia AR — are irregular and — diminish. * Another point of interest is the comparison of isomeric compounds; but up to the present the only two pairs of isomers investigated are methyl butyrate and isobutyrate, and normal and iso-pentane. In both cases there is a clear relation- ship between the ratios and the constitution, the normal and iso-compounds standing to each other in much the same relative positions as a higher and lower normal paraffin. It is worthy of remark that the volumes of a gram of all four paraffins are nearly the same (4'266—4°303) at the critical point. Looking at the data for the twenty-six substances examined, it is evident that they may be divided into groups—(1) benzene and its haloid derivatives, ether, the tetrachlorides and the paraffins; (2) the ten esters; (8) the alcohols; (4) acetic acid. The members of group (1) may be regarded as normal; the devia- tions of the ratios from constancy are small, though, as pointed out, they exhibit certain regularities; in group (2) the values of ” are rather higher, and of V yather lower than in group (1); in group (3) the ratios Z and ” are very 0 : 0 Do 1 Prans. Chem. Soc., vol. lv. p. 486. 2 Tbid., vol. lix. p. 911. 3 Thid., vol. 1xiil. p. 1191. 4 Thid., vol. lxvii. p. 1071; vol. Ixxi. p, 446; vol. Ixxiii. 675; Proc. Phys. Soc. vol. xiii. p. 602. - - 0 TRANSACTIONS OF SECTION B. 833 high ; for acetic aid . and V. are high, but 2 very low. The marked dif- 0 0 A ee ferences between the alcohols and acetic acid, and the large deviations in both cases, are probably to be accounted for by the fact that the molecules of the alcohols at moderate temperatures are polymerised in the liquid, but not the gaseous state, whilst with acetic acid there is polymerisation in both states. The ratios Le at the critical point should, according to Van der Waals, be the same for all substances, the molecules of which undergo no dissociation or polymerisation, and he gives the value of this ratio as § or 26. Now the ratio depends on the constant 6 in the equation (»+ “) (v—b) =RT, and Van der Waals takes 6 to be four times the actual volume of the molecules in unit mass of substance; O. E. Meyer, however, contends that 6=4 x 4/2 times the volume of the molecules, and it has been pointed out by Heilborn and by Guye that, if that is so, the ratio 2°6 should also be multiplied by 4/2, which would give the value 3:77. It is remarkable that the mean value for the twelve substances in group (1) is 3°77, from which it may be concluded that the molecules of these substances in the critical state are simple like those of the gas. (At the same time it is to be noticed that with the three normal paraffins and , shows a slight increase with rise of molecular weight. The ratios for the ten esters area little higher (3:87 to 3-95); decidedly higher for the alcohols, especially methyl-alcohol (4:52 —4-02), and much higher for acetic acid (5:00). It would appear from this that the molecules of the alcohols and acetic acid are polymerised to a considerable extent at the critical point, and this conclusion is supported by the generally abnormal behaviour of these substances, and agrees with that of Ramsay and Shields, that in the liquid state at moderate temperatures their molecules are decidedly complex, whilst those of the majority of the compounds examined by them are probably simple. I hope to continue the investigation of the paraffins and other hydrocarbons in order to obtain further light on the points referred to, and it will be of interest to compare the molecular volumes at the critical points, and at a series of reduced: pressures. The accurate determination of the critical constants is a matter of great importance. It is best to employ an apparatus similar in principle to that of Andrews, in which the temperature, pressure, and volume can be altered at will ;- though the critical temperature may be determined with but small error in a sealed tube, if the quantity of liquid taken is such that its critical volume is approximately equal to the capacity of the tube. With a pure substance, free- from air, two independent determinations of the critical temperature should certainly not differ by 0°:1, unless the temperature is above 300°, when the experimental difficulties are greater. The error in the determination of the critical pressure should not exceed 0:2 per cent., but the critical pressure is greatly- affected by the presence of even very small quantities of impurity (and, of course, of air); and in comparing two specimens of the same substance, one of which is known to be pure, the agreement of the critical pressure is probably the most delicate test of the purity of the other. The only method yet known by which the critical volumes can be accurately determined is the indirect one based on the ‘law of diameters’ of Cailletet and Mathias. These physicists made the very important discovery that the mean densities of liquid and saturated vapour for any ‘normal’ substance are a linear function of the temperature (or D =Dj—at where =the mean density), and since, at the critical point, the two densities are equal—or rather there is only one—the value of D at that point gives the critical density, from which the critical volume is, of course, easily calculated. I have been able to show that the 1898, 34 the two tetrachlorides 834 REPORT—1898. law of Cailletet and Mathias holds good with great accuracy right up to the critical point (with normal pentane observations were taken to within 0°-05 of the critical temperature) for all the compounds examined except the alcohols. It has, in view of these results, been suggested, I think justly, by M. Guye, that a serious deviation from the law may be taken as a proof of the existence of molecular dissociation or polymerisation. It is true that a few years ago I was under the impression that a direct determination of the critical volume was possible, and the values obtained do, indeed, bear as nearly constant ratio to the true critical volume, but they are about 14 per cent. too low. The probable explanation of the error has been given by M. Gouy, who pointed out that, at the critical point, a substance is so extremely compressible that in a long column the density increases very considerably from top to bottom, owing to the pressure exerted by the substance itself. In the course of these researches ample proof has been obtained that the views of Andrews regarding the behaviour of a substance in the neighbourhood of the critical point are correct, and also that the vapour pressure of a pure sub- stance is quite independent of the relative volumes of liquid and vapour. These points are referred to because they have been called in question by several observers during the last few years. Two of the substances examined attack mercury at high temperatures, and it was therefore impossible to determine either their vapour pressures or specific volumes by the methods employed for the other liquids. The difficulty, as regards vapour pressure, was overcome by sealing a wider tube to the lower end of the volume tube, and using such a quantity of liquid that during the observa- tions the lower end of the column was always in the wider and cold part of the tube. The height of the column of mercury in the tube must, under these condi- tions, be calculated.? A method of determining the specific volumes of both liquid and saturated vapour in a sealed tube was also devised.” When the specific volumes of the liquid are already known, this method, in a simplified form, is very convenient for determining the specific volumes of saturated vapour.® It is obviously necessary that, in order to obtain trustworthy results, pure substances must be employed and, indeed, more time has been spent in the prepara- tion of the pure substances than in the determination of their physical constants. The difficulties met with in the fractional distillation of liquids, more especially in the separation of pure hydrocarbons from petroleum, have led to an extended study of this subject, and both new apparatus * and new methods of procedure ° have been devised; it has thus been possible to separate perfectly pure normal and iso-pentane (B. P. 27°95 and 36°3) from the complex mixture of hydro- carbons in American petroleum. 2. On the Action of certain Metals and Organic Bodies on a Photographic Plate. By W. J. Russetz, Ph.D., F.RS. The author demonstrated that printers’ ink is capable of acting, in the dark, on a photographic plate; also that wood, dry copal varnish, &c., can act in the same way ; that among liquids turpentine, drying oil, the essential oils, &c., act in like manner. In addition to these and many other organic bodies, certain metals have the same property, and either in contact, or at a distance from the photographic plate, can act upon it. In this way pictures of thin surface or pictures of opaque bodies, such as skeleton leaves, lace, or paper, can be obtained. It was also shown that ordinary writing ink was perfectly opaque to this kind of action, and that even old and much faded ink was capable of stopping the action and producing a 1 Trans. Chem, Soc., vol. lix. p. 917. 2 Thid., vol lix. p. 37. 9 Thid., vol. lix. p. 125; Proc. Phys. Soc., vol. xiii. p. 617. * Chem. News, vol. xxi. p. 177; Zrans. Chem. Soc., vol. lxxi. p. 440. 5 Phil. Mag., 1894 p. 8. oe Pe GN A oy —————— << , °° e TRANSACTIONS OF SECTION B. 835 picture. The author also demonstrated that the action could pass through such media as thin sheets of gelatine, celluloid, gutta-percha, collodion, &c., and that even a picture of a metal surface is obtainable through such media. It was sug- gested that these different phenomena could be explained on the supposition that hydrogen peroxide is in all cases produced. 3. The Action of Bacteria on the Photographic Plate. By Prercy FranK- LAND, Ph.D., B.Sc., F.R.S., Professor of Chemistry in Mason University College, Birmingham. The action on the photographic plate which is exerted by uranium and its compounds, by zine and several other metals, as well as by a number of organic substances, naturally leads to the inquiry as to whether living structures may not also be endowed with the power of recording their presence by action on the sensitive film of the photographer. The author has opened up this inquiry by investigating the behaviour of bacterial cultures towards highly sensitive photo- graphic plates. Gelatine cultures of the bacillus coli communis and of proteus vulgaris were found when placed at a distance of half an inch from a photographic plate to pro- duce the same effect as light, the exposure lasting over nine days in absolute dark- ness. Definite pictures of the bacterial cultures were obtained by placing the sensitive film in actual contact with the cultivations, the exposure being extended over a period of fourteen days. Similar results were obtained with agar-agar cultivations. As this action does not take place through glass or mica, the author is of opinion that it is not due to any form of radiation, but to the evolution of volatile matter entering into reaction with the photographic film. As far as the author's experiments have gone, the action is exerted both by bacteria which liquefy (proteus vulgaris) and those which do not liquefy gelatine (6. coli communis and the typhoid bacillus). It is, however, quite possible that considerable ditferences in respect of this activity may be found to exist in the case of different bacteria, and that this property may become of importance in their diagnosis. Bacterial growths which are luminous in the dark (photo-bacterium phos- phorescens) were found to exert a still more powerful action on the photographic plate. The author proposes extending these investigations not only in connection with bacteria but also in respect to other organised structures, vegetable and animal, living and dead. 4, Further Experiments on the Absorption of the Réntgen Rays by Chemical Compounds. By J. H. Guapstonn, D.Sc. F.RS., and WatteR HIBBERT. At the two previous meetings of the British Association the authors had ex- amined the absorption of Réntgen rays, especially by metals and metallic salts. During the past year they have endeavoured to perfect the quantitative methods employed for estimating the comparative intensity of radiographs taken simulta- neously ; and to determine whether the amount of absorption is purely an atomic phenomenon, or whether the amount of rays absorbed by a compound body depends to any extent on its physical condition or manner of combination. In the experiments recorded the authors had again employed the Lummer- Brodhun photometer; and had endeavoured to get rid of irregularities of exposure by placing the objects simultaneously exposed to be radiographed at a considerable distance from the radiating point (averaging 15 or 16 inches), and rotating them during the experiment. They believe that in this way the effect upon the sensitive plates can be determined within + 2 per cent. An experiment was usually repeated about six times, and the mean taken. Among the results arrived at were the following. Finely-pounded glass gave 3H 2 836 REPORT—1898. a radiograph about 3 per cent. deeper than the same quantity of the same class when in the form of a polished plate. Paraffin gave the same amount of absorp- tion whether it was solid or liquid. Pounded crystals of sulphate of copper and ammonia gave practically the same absorption as a mere mixture of the two con- stituent salts. Finely-divided metallic copper was found to absorb about 2 per cent. more rays than the same amount of copper as black oxide or as red oxide. That there was little or no effect produced by difference of atomicity was shown by a comparison of these two oxides, and also of the two oxides of mercury, which absorbed practically the same amount. The protoxide and peroxide of lead were identical in their results; and the ferric oxalate gave only 1 per cent. less absorp- tion than the ferrous oxalate, plus as much oxalic acid as was necessary to equalise the carbon and oxygen in the two salts. The old experiment with carbon and various hydrocarbons was re-examined, with a final result which may be expressed by the figures :— Carbon ; 4 ‘ . | solid, black i : F | C | 100 Anthracene . : : », White : : dott Grea ly | 96 Naphthalene : : 3 fr ‘ Crue 93 Amylhydride . ; . | liquid, colourless Chi 96°5 Turpentine. : ; : . : : | Ci, Hi, 95 Benzene . : : -| » 5 : - | C, H, 94°5 The experiments of this year confirm the opinion previously expressed that the absorption of the Réntgen rays by a compound body is dependent upon the absorp- tion exercised by its constituents, little, if at all, modified by their physical condi- tion, or by change of atomicity, or other difference of combination. The authors are disposed, however, to ask the question—whether the law may not be more than proximately true? There is superabundant evidence that the Réntgen rays are not homogeneous. The slightly greater apparent absorption produced by the pounded glass may be due to a little reflection or refraction from the admixture of a small quantity of rays which, though they have passed through aluminum foil, have properties somewhat analogous to ordinary light. The slightly greater absorption caused by metallic copper and by black carbon may also be due to the presence of such rays. They think it possible that if these rays could he entirely sifted away, Rontgen rays would be obtained, which in their passage through a body would he affected merely by the nature of the atoms forming it, and that the law that the absorption by a compound is the mean of the absorptions due to its several constituents would be not proximately but absolutely true. An apparatus was exhibited by which the ‘ grade’ of the Rontgen rays can be investigated quantitatively. 5. Report on the Action of Light upon Dyed Colowrs.—See Reports, p. 285. 6. On the Cooling Curves of Fatty Acids. By Dr. A. P. LAURIE and HE. H. STRANGE. The melting-points of mixtures of fatty acids were determined by Heintz, and the tables are quoted in the text-books, They show that the mixtures have a lower melting-point than either of their constituents, thus showing a close analogy to the behaviour of many alloys. We therefore determined to apply to these bodies a method of investigation similar to that used by Professor Roberts Auster in his experiments on alloys. The melted fatty acids are placed in a test-tube surrounded by melting ice, and a thermal junction connected to a mirror galvanometer inserted. The results are photographed on a moving plate. The plate is calibrated by means of a second thermal junction attached to a thermometer, and immersed in a large TRANSACTIONS OF SECTION B. 837 volume of water. The cooling curves obtained in this way are of considerable interest. The fatty acids investigated have been palmitic, stearic, lauric, and myristic acids. The cooling curve of a pure fatty acid turns sharply round when the solidifying point is reached, runs straight up the plate till the solidifying is finished, and then turns sharply off again, One per cent. of another fatty acid quite perceptibly alters the shape of the curve, so that the character of a cooling curve seems a good test of purity. When a larger portion of a fatty acid is introduced a second latent heat-point is developed, the curve showing a discontinuity below the solidifying point of the mixture. As the solidifying point is lowered by introducing more and more of the second fatty acid, this discontinuity is gradually merged in the common melting-point of the mixture, thus reproducing the phenomena observed by Professor Roberts Austen in the case of certain alloys. This discon- tinuity can hardly be due to the formation of a compound, but is probably caused by the presence of the ‘eutectic alloy’in the mass. We are now repeating our ex- periments with synthetically prepared organic bodies of known constitution, and studying also the cooling curve of water. 7. On the More Exact Determination of the Densities of Crystals. By the Haru or BERKELEY. A-comparison of the several values found by different observers for the density of one and the same crystallised salt shows variations amounting in some cases to 10 per cent. As the density is assumed to be a physical constant, independent of the manner in which the crystals have been produced, these variations are probably due to errors of experiment. The chief sources of such errors are (1) imperfect measurement of temperature and volume, (2) occlusion of mother liquor, (3) adhesion of air, (4) hygroscopic nature of the salts. In the paper are described the methods devised by the author for reducing the amount of these errors. 1. Two conical pyknometers, of about 7 c.c. capacity, with thermometer stoppers and calibrated capillary side tubes, were used. One served as a counter- poise, and was treated externally exactly like the other. They were repeatedly heated to 130° C., and allowed to cool, in order to bring the glass into a con- dition of molecular rest. For determining capacity the flask filled with water was placed in a desiccator, from which the air was exhausted till, on tapping, the water boiled. After it had thus been kept boiling for some time, the flask was removed, and the stopper inserted in a position and under a pressure which were observed. After the two pyknometers had been wiped dry they were placed on the balance pans, and when the temperature had become steady and the level of the liquid in the capillary had, in consequence of evaporation round the neck, fallen below the highest graduation, the weight, the level in the capillary, and the temperature were noted. The greatest difference between any two out of eight estimations of capacity thus made was 0:00029 c.c. The liquid in which the crystals were weighed was carbon tetrachloride. Owing to the high coefficient of expansion of this liquid, special means, which are described, were devised for keeping constant the temperature of the balance case. The evaporation between the neck and the stopper was at the rate of about 0:0001 gram per minute, 2. To remove occluded mother liquor the crystals may be reduced to powder and then dried, the presumption being that the crystals will break across the €avities containing the mother liquor, and that the latter on evaporating will deposit crystals of the same kind, But the crushing process may produce change, as in the familiar case of mercuric iodide; and it is better to form small crystals in a solution kept at a constant temperature and constantly stirred. An apparatus was planned and constructed for this purpose. 3. To prevent adhesion of air, the pyknometer with the weighed crystals at bottom, together with a bulb holding a charge of carbon tetrachloride, were so 838 REPORT—1 898. connected that, when the air had been exhausted from the flask, vapour from the boiling carbon tetrachloride took its place in the interstices of the crystals. Then, by tilting the vessel, the flask was filled with liquid tetrachloride. On removing the flask the stopper was inserted as before. Eleven determinations of the density of quartz show a maximum divergence of ‘02 per cent. ‘ 4, To remove moisture retained on the surface of the crystals, a current of dry air was passed through the flask till on passing out it yielded no moisture to phosphorus pentoxide. The apparatus was then exhausted, and carbon-tetra- chloride was admitted sufficient to cover the crystals. The flask was then filled up as before. Four determinations by this method of the density of K?CO® show a maximum divergence of ‘04 per cent. 8. The Equivalent Replacement of Metals. By Professor Frank Crowes, D.Sc., Lond. it has long been known that when iron is immersed in a solution of cupric sulphate metallic copper is deposited, and an amount of iron passes into solution which is exactly able to combine with the sulphate radicle liberated from the cupric sulphate. The weights of copper and of iron which combine with the same weight of sulphate radicle have been determined by carrying out the process quantitatively, These weights are chemically equivalent to one another, for they are able to combine with the same weight of the acidulous radicle. In the case just cited the chemical change appears, at ordinary temperature and with dilute cupric solution, to follow the simple course stated. But attempts to extend this direct method of ascertaining the relative equivalents of metals cease to be direct in certain cases, owing to the complicated nature of the reactions which occur. My attention was drawn to such a complication in the case of the action of magnesium on cupric sulphate solution, and the nature of the reaction was ther investigated by R. M. Caven, B.Sc., and myself. Commaille,! Kern,? and Vitali,® had drawn attention to the facts that during the action of magnesium on cupric sulphate solution cuprous oxide was deposited with the metallic copper, and hydro- gen was evolved. These facts prove that the copper equivalent of magnesium cannot be obtained by simply weighing the magnesium which passes into solution and the deposit which was formed during the process. But we proceeded to make a fuller examination of the nature of the reaction, and to show that when it was quantitatively carried out the products enabled us to calculate the equivalents of magnesium and copper. Having obtained practically pure materials, we proceeded to study the reactions when the conditions were varied by employing hot or cold and strong or weak cupric sulphate solutions. We were met with the initial difficulty that cupric sulphate solution deposits a basic salt when it is boiled: this salt we separated and found to correspond in composition and properties to the formula 4CuSO,. 7Cu(OH),.H,O. Pickering had separated a similar salt, to which he attributed the formula 6Cu0.2S0,.5H,O. Owing to the deposition of this salt complicating the products, we avoided actual ebullition in our experiments. The action is most simple when the magnesium is immersed in a hot strong solution of cupric sulphate. Hydrogen is briskly evolved, a chocolate-coloured deposit forms, and green flakes are produced which disappear before the reaction is completed. Treatment of the brown deposit with dilute hydrochloric acid yields colourless cuprous chloride solution and a small residue of metallic copper. The hydrogen evolved was collected and measured, the metallic copper was weighed directly, and the amount of cuprous oxide was determined by dissolving it in hydrochloric acid and determining the amount of cuprous chloride thus formed by 1 Comptes Rendus, \xiii. p. 556. ? Chem. News, xxxiii. p. 236. 3 Journ. Chem. Soc., \xx. p. 419. j : j . ) 1 TRANSACTIONS OF SECTION B. 839 titrating it with standard permanganate solution in the presence of a sufficient amount of magnesium sulphate. As a result of four experiments, the average sum of the magnesium equivalents of the cuprous oxide, the copper, and the hydrogen amounted to 0'102 gram, and the average weight of magnesium used was 0:105 gram. The ratios of the weights of hydrogen, copper, and cuprous oxide produced were constant only when the conditions of the experiment were precisely similar. When the hot cupric sulphate is dilute, or when it is employed at ordinary temperature, the reaction pursues at first a similar course, but it soon becomes very considerably delayed by the formation of a green basic cupric salt, inter- mingled with colourless basic magnesium salt. Thus, the reaction on the magnesium was asually complete in ten minutes in an excess of a hot, strong solution of cupric sulphate ; but in weak and cold solutions it often extended over several days, and even a week. The percentage of hydrogen, compared with that which is equivalent to the magnesium employed, was in the case of the hot solution 34:7 ; with the cold solu- tion, it was 41°5 with weak solution, and 30°6 with saturated solution. Various explanations have been given of the causes which lead to deposition of cuprous oxide and to eyolution of hydrogen. It has been suggested that the change is due to impurity in the copper salt; this we have disproved by using a salt purified by frequent recrystallisation, and yielding 25-23 per cent. of copper (theory = 25:39) ; we have also proved the purity of the magnesium employed. Divers suggests that the evolution of hydrogen is due to the action of the mag- nesium upon free sulphuric acid, which has been formed by hydrolysis of the cupric salt. This seems to us to be an insufficient explanation of the rapidity with which hydrogen is evolved. Cold cupric sulphate solution was found to give no acid reaction with methyl-orange, although it is faintly acid to litmus paper. Yet such a solution gives an immediate evolution of hydrogen when magnesium is immersed in it, the evolution of the gas being very rapid in a hot and strong solu- tion. After carefully studying the change, we are inclined to attribute the evolu- tion of hydrogen in small degree to the presence of free sulphuric acid formed by hydrolysis in cold solution, and in greater degree to the same cause in hot solution. This involves the formation and separation of basic salt. This reaction, however, does not account for all the hydrogen evolved, and one of us will be prepared before long to advance a further explanation to account for this. Divers further suggests that cuprous sulphate is formed and almost immediately converted by the action of the basic cupric salt into cuprous oxide; this theory we also find to be untenable. ._ The immediate separation of cuprous oxide and evolution of hydrogen, without formation of basic salt, which occurs at the commencement of the reaction, may be represented by the equation : 2Me + 2CuSO, + H,O =2MeS80, + Cu,0 + H,. The action of the magnesium-zinc couple has been proved to be too slow to explain the rapid escape of hydrogen, and if this were the origin of the hydrogen, its escape would not immediately follow the immersion of the magnesiun. 9. A Note on Alkaline Chlorates and Sulphates of Heavy Metals. By W. R. Hopaxinson and A. H. Coore. Many solid sulphates, whether containing water of crystallisation or anhydrous, when mixed and gently heated with potassium or sodium chlorate give off chlorine gas in addition to oxygen. In many cases the evolution of the chlorine seems to precede that of the oxygen. With sulphates containing crystallisation water chlorine is evolved with it, as steam, on heating. Mixtures also of anhy- . drous sulphates, as those of copper and manganese with chlorates, give olf a mixture of oxygen and chlorine at temperatures very little above 100° C, 840 REPORT-—1898. The theoretical equations (1) MSO, + 2KCI10, = K,SO, + MCI1,O, and (2) MC1,0, = MCl, + 30,, where M is a divalent or a polyvalent metal, scarcely hold at all.. In the cases, lead, silver, mercury, where it seemed most likely to hold, it certainly does not ; for the dry sulphates of these metals mixed in fine powder with potassium chlorate, and very gently heated—to about 120°—give off chlorine very briskly, and the residue is a mixture of potassium sulphate and chloride, and the oxide and chloride of the other metal. In the case of lead, the peroxide is formed. In a few cases this decomposition takes place with solutions of the salts. Manganese sulphate and alkaline chlorate solution becomes brown after boiling a few minutes. We have mixed different sulphates and potassium chlorate in equivalent quantities, and endeavoured to ascertain the relation between the oxygen and chlorine evolved; but even with careful heating the results have not been very concordant. The sulphates of the following metals have been tried :— Zn, Ni, Mn, Mg, Fe, Cu, with and without crystallisation water. Ag, Hg, Pb, anhydrous, Several alums both with and without water. It may be here noted that many metallic chlorates decompose when their solutions are evaporated, even at the ordinary temperature and under reduced pressure. This is notably the case with manganese and ferric chlorates. The sulphates employed were carefully purified, and contained no free acid. SATURDAY, SEPTEMBER 10. The Section did not meet. MONDAY, SEPTEMBER 12. A Joint Discussion with Section A on the recent Eclipse Expeditions was held. The following Reports and Papers were read :— 1. Report on the Teaching of Natural Science in Elementary Schools, See Reports, p. 433. 2. Juvenile Research. By Professor H. E. Anmstrone, F.R.S. 3. Green Cobaltic Compounds. The Result of Oxidising Cobaltous Salts in presence of Organic Salts of the Alkali Metals. By R. G. Durrant, M.A. FCS. Hydrogen peroxide and other oxidising agents are capable of forming green solutions with cobaltous salts in presence of fairly concentrated solutions of potassium bicarbonate, oxalate, glycollate, acetate, citrate, malate, lactate, and succinate. Potassium may be replaced by the other alkali metals, and in some cases by ammonium, barium, strontium, or calcium. The cobalt in the green bicarbonate solutions has been shown to be present in the cobaltic state by volumetric experiments involving, (a) the maximum depth oar) ee es &«* TRANSACTIONS OF SECTION B. 841 of green, (6) the non-appearance of a precipitate, (c) the estimation of iodine liberated. A potassium salt, formed by the action of hydrogen peroxide on cobaltous oxalate dissolved in potassium oxalate, has been isolated and analysed ; the formula appears to be K,Co,(C,O,).,4H,0. This body, unlike Kehrmann’s K,Co,(C,0,),6H,O, exhibits no dichroism. It occurs in green, transparent, microscopic crystals, belonging in all probability to the rhombohedral system. The salt is very stable; its solution in water gives no precipitate with dilute calcium chloride, while concentrated calcium chloride yields minute green, needle- shaped crystals of the corresponding calcium salt. The properties of the potassium salt in regard to its behaviour when heated, solubility, lowering of freezing-point, action of acids, alkalis, reducing and oxidising agents, have been studied, from which it would appear that a structural formula KO,C—C(OH), C(OH),—CO,K Sr x AY ety pone = ox O O a a KO,C—C(OH), C(OH), — CO,K is probable, the body having lost a previously acquired atom of oxygen between the cobalt atoms. The absorption spectrum of the aqueous solution exhibits two bright bands— one in the red with centre near the C line; the other in the green with centre approximately \=5150. The absorption spectra of other cobaltous and cobaltic solutions have been studied; that of the bicarbonate green exhibits no red band, but gives a single bright band in the green with centre approximately A = 5365. There appears to be a reversal of the band in the green when cobaltous solutions are oxidised to form these green compounds. 4. Analysis of Dorsetshire Soils. By C. M. Luxmoors, D.Se., FIC. The investigation of the Dorsetshire soils, which has recently been commenced at Reading College, is not forward enough to enable us to publish any results at present, but an account of the methods that are adopted will perhaps be of interest. As the object of the work is to obtain a general knowledge of the soils of the county, the samples are taken from land lying on the various geological formations that occur, and so selected as to be, in the opinion of local agriculturists, typical of a more or less considerable area of land in the neighbourhood. Three samples of the soil of each selected field, usually along a diagonal line, are taken much in the manner directed by the Royal Agricultural Society, using, however, boxes 6 inches by 6 inches ia area and 18 inches deep, and made so that one side can be readily removed, showing the soil in section. When the boxes are opened at the laboratory the soil is separated from the subsoil, a division being made at the arbitrary depth of 9 inches, and also at any other line where a definite change in the character of the soil is manifest. The larger stones, if any, having been removed, the sample is carefully divided so as to reduce it to about one kilo- gramme ; the smaller stones and gravel are then separated by sifting under water, and the fine earth passing a sieve ;-inch mesh is dried at a moderate temperature ina copper oven. If the three samples taken from a field appear fairly similar, a mixture of them is made for analysis, but the original samples are preserved for reference. The chemical analysis of these mixed samples offers at present nothing worthy of special notice; it includes, of course, in addition to the usual complete analysis of the portion soluble in hydrochloric acid, a determination of the available potash and phosphoric acid, according to Dyer’s method. A series of mechanical 842, REPORT—1898. analyses of the soils according to a slight modification of Osborne's method of subsidence has also been commenced. ‘This enables one to determine the percentage of soil consisting of particles within certain limits of size, and thus to obtain a rough approximation to the total surface area of the soil particles. No doubt the attraction of the soil for moisture is dependent very largely upon the surface area of the particles; though certain preliminary experiments, which the author was enabled—through the kindness of Sir Henry Gilbert—to carry out at Rothamsted some time ago on the soil of the Broadbalk field, lead him to believe that the relation is not so simple as might at first sight be expected. The selection of suitable fields and the collection of samples are carried out by the agricultural staff of Reading College, and the author’s colleagues take the opportunity of making notes at the time of the various physical features of the land, &c. With a view to obtaining a thoroughly general knowledge of the soils of Dorsetshire, it is proposed to sample and analyse one hundred of them, in the manner indicated, during the course of the next five years. It is important to mention that this investigation is being carried out under the auspices of the Dorsetshire County Council, who have made a grant towards the necessary expenses. 5. Report on the Carbohydrates of Cereal Straws.—See Reports, p. 293. 6. Interim Report on the Promotion of Agriculture.—See Reports, p. 312. TUESDAY, SEPTEMBER 13. The following Papers and Reports were read :— 1. Recent Advances in the Leather Trade. By J. GorDoN Parker, Ph.D. A new and important tanning material, containing upwards of 30 per cent. of tannin, is canaigre. To light leathers, tannage with it gives suppleness and mildness. Quebracho is increasingly used. The most important change of method, however, in the manufacture of leather is the now almost universal employment of extracts, principally those of oakwood and chestnut—a method which is the indirect outcome of chemical science. Up to a comparatively recent date there was no known chemical means by which one extract could be detected from the other. The tanner’s chemist can, however, now determine between them, and also detect their adulterants, quebracho, myrabolams, cutch, divi-divi, algarobilla, &c. The extended use of extracts has brought about improved methods of estimat- ing the tanning values of materials used in tanning. The considerable ditferences in the results of analyses of one and the same sample by different chemists culminated in the holding in London of a conference, and the formation at that conference of the International Association of Leather Trades’ Chemists ; an Association from which much may be expected, particularly in the direction of the adoption of standard methods for the analysis of tanning materiais. In regard to the fermentation that takes place in tan liquors, chemistry had already afforded considerable enlightenment. One no longer talks of the waste of tannic acid and the formation of gallic acid; but the presence of acetic, lactic, and propionic acids is detected, their percentage easily estimated, and in every well- regulated tanyard their value and uses are thoroughly appreciated. The formation of mould is checked, and the action of certain antiseptics thoroughly understood. The bateing and puering of skins by means of dog and hen excrement is a standing disgrace to the leather trade. Many substances in substitution for excre- ment have been tried, but not with much success. The opinion is generally held that bacteriological action is necessary in the bateing and puering process, and Mr. a TRANSACTIONS OF SECTION B. 843 J. T. Wood and others have succeeded in isolating over twenty different kinds of bacteria from the puer and bate referred to, and in culturing the bacteria. Within the last few weeks tubes containing cultures of the bacteria which are suitable for bateing and puering purposes have, I believe, been put upon the market in Germany. This is a form of applying the excrement bate that makes it far less objectionable than heretofore. Mr. Wood has also applied bacteriological investigation to the bran drench, and he has shown that for some leathers acetic and lactic acids may be substituted for the fermenting bran. The rush after quick tanning processes is somewhat reactionary. No great success has been achieved by the various drum processes, and no leather has been made by any of them that will serve other than second-class work. Leather pro- duced by the so-called electric process is‘being worked successfully in Sweden, and the leather which is tanned in from eight to twelve weeks is to all appearance satisfactory ; it has not been commercially tried in England. There is most pro- bably what may be regarded as a rational limit of time for the conversion of hide into leather, and it is doubtful whether the time that up to now has been regarded as proper in such conversion will ever be very greatly reduced, as there is in tanning more than simple chemical combination of tannin with hide substance, In the extraction of tanning materials in the tanyard, English tanners are far behind those of America and the Continent. A large amount of available tannin is often wasted by cold extraction. Most of the large tanyards on the Con- tinent extract with warm water in closed vats, some even extracting under pressure. Analyses of over 300 samples of waste spent tan from over forty tanyards in Great Britain have shown an average of over 9 per cent. of available tannic acid. Supposing with valonia, costing 12/. per ton, and containing 36 per cent. of tannin, 5 per cent. to be thus wasted, a loss is incurred of 1/. 13s, 4d. per ton; and valonia is only one of the materials used in this country. Investigation in the case of oak bark shows 61 per cent. of tannin extracted with cold water, and 95 per cent. with water at 60°C. Valonia extracted cold gives over 70 per cent. of tannin; at 60° C. gives off the whole of it. Even with hemléck, containing only about 16 per cent. of tannin, the Americans find warm extraction pay, and the Germans years ago adopted the method. The fear of darker colour in leather arising from the use of warm extracts is much exaggerated. | Chrome leather tannage has emanated from the chemist’s laboratory, and _ leather is chromo-tanned by a two-bath process and by a one-bath process. The _ leather tanned by either method, for it is leather, has many advantages over vegetable-tanned leather. It is more elastic, more waterproof, and lighter and softer for foot-wear, except as to soles, for which its water-resisting quality makes it too slippery. Millions of dozens of skins are chromed weekly in America. Owing to the labours of the late Professor von Schroeder, it is possible now to determine at any period during the tanning process what amount of tannin a hide has absorbed, and to Professor Proctor, of Leeds, we owe our present system of analysis. As to the future, a great advance in our knowledge may be expected from the several tanning schools and research laboratories that have come into existence, but there is still a marked need of more research and of specially trained chemists with a thorough knowledge of tanning. 2. Diamidated Aromatic Amidines, a New Class of Colouring Matters, By E. Nogwtine, Professor of Chemistry, College of Chemistry, Mul- , house. ____ The benzeny]-di-phenyl-amidine, C,H; ¢=N—C,H, H \w-c =N-< Se | CH N