eat 7 ite ; eee itt i tlh ttt f — Sg ae a a = et eS REPORT OF THE - TWENTY-SECOND MEETING BRITISH ASSOCIATION FOR THE ADVANCEMENT OF SCIENCE; HELD AT BELFAST IN SEPTEMBER 1852. LONDON: JOHN MURRAY, ALBEMARLE STREET. | 1853. ; PRINTED BY RICHARD TAYLOR. AND WILLIAM FRANCIS, RED LION COURT, FLEET STREET, Sao CONTENTS. Page Ossecrs and Rules of the Association .........scseeeeseseeseeeneneenenes Sill Places of Meeting and Officers from commencement .........ss6e00008 = XVI Table of Council from commencement ..........0.sseseeseseerseseseeeeeee XViil BPRCASUTEL S ACCOUNE cin esecen nec centes cee ceesecconvecnisivessoeswessscussanecs XX ae PME NEN EE 8 7 oc cca anaes cc atedeccacaasasuccedgtivsstenesssss. SxaE Officers of Sectional Committees .........sssccceeececeee ceeeeeecseeeveee | SXili Corresponding Members.. Dede W ed eee asd PERI Report of Council to the Gogionl Bilanaltens egies). eed 0d Report of the Parliamentary Committee .......:ssccsseeeeeetteeetereeeee | XXIK Recommendations for Additional Reports and Beaten in Science xxxii Dynopsis of Money Grants ......sescocsedeercercsesesccccepredsevetsccsedsase” XXXV Arrangement of the General Meetings ............sssessscoceecescseees ves xl Beeniress of the Presidenitay. <. Jas tpa.auascabacecged vas ictves veces das bande eee xii » REPORTS OF RESEARCHES IN SCIENCE. Third Report on the Facts of Earthquake Phenomena. Catalogue of recorded Earthquakes from 1606 B.c. to a.p. 1850. By Robert MAL DET, Cols, MBDA. tie Gicays senseieserss Wien phe SN Es'sp$E <= anpteonvbank. ty 12 Twelfth Report of a Committee, consisting of H. E. StrickLanp, Esq,, Professor Dauseny, Professor Henstow, and Professor Linpiey, appointed to continue their Experiments on the Growth and Vitality RES ORE swiss aaaad neem gn eanh «cast seb eace ape menue Tao dn dalek Paeisamnes 177 iv CONTENTS. Page Report on Observations of Luminous Meteors, 1851-52. By the Rev. Bapen Powe tt, M.A., F.R.S., F.R.A.S., F.G.S., Savilian Professor of Geometry in the University of Oxford ...........cccecsecenceseceeevecs 178 On the Influence of the Solar Radiations on the Vital Powers of Plants growing under different Atmospheric conditions. By J. H. Guap- AMONIEA ENG DD Su coctiocseeccsescceccsee'asia ses cwciesecudessleases adeuet Mee dae @eemeere A Manual of Ethnological Inquiry; being a series of questions concern- ing the Human Race, prepared by a Sub-committee of the British Association for the Advancement of Science, appointed in 1851 (con- sisting of Dr. HopGKin and Ricuarp CuLt, Esq.), and adapted for the use of travellers and others in studying the Varieties of Man ... 243 Mean Temperature of the Day and Monthly Fall of Rain at 127 Stations under the Bengal Presidency, from official Registers kept by Medical Officers, for the year 1851. By Colonel Syxes, F.R.S. ............... 252 On Experiments on the Laws of the Conduction of Heat. By J. D. IDGRBESS cl eS sb Ornin mete seciccsicostteccd cscs chavacsoas ovorcs ast eeoameeee TLOU On the Chemical Action of the Solar Radiations. By Roperr Hunt... 262 On the Composition and GEconomy of the Flax Plant. By Dr. HopcEs, F.C.S., Professor of Agriculture, Queen’s College, Belfast, and Chemist to the Chemico-Agricultural Society ..........:.sseeeeeeeeeeeee 273 The Freshwater Fishes of Ulster, as enumerated in the MSS. of the late WitiaMm TuHompsoy, Esq.. President of the Belfast Natural History and Philosophical Society. Contributed by Rosert PATTERSON, Reqs atid’ James: R. GARRETT BsG.: fie. sasncenes seve os onceccs ds exnvasavsaee ee Supplementary Report on the Fauna of Ireland. By the late WitL1AM Tuompson, Esq., President of the Belfast Natural History and Phi- PGsopHiCal HOCLY... c onan 5 PRINCE OF CANINO’S Zoological Notices ...++++ssecsresserersrsnsersrereeseeer ee Professor DicKIE’s Remarks on the Distribution and Habits of Echinus lividus Professor E. Forpes on a New Map of the Geological Distribution of Marine Life, and on the Homoiozoic Belts ccccwvcccsonssassexvceusardsiesceeaae)aqqcensenci procured in the Neighbourhood of Belfast .--++.sssssssrssssrrsesteersteeertress Mr. Joun Grarncer’s Catalogue of the Shells found in the Alluvial Deposits Of Belfast..ccccssssscseceeccseceeccecas ceeuseeseeeccneres Boe, acaie vce = eaaemaae Sendoseer Rev. Tuomas Hincxs on a peculiar Organ which oceurs on some of the Ma- rine Bryozoa, and which appears to indicate a Difference of Sex ...+++++++++ Mr. Tuomas H. Huxvey’s Researches into the Structure of the Ascidians ... Mr. Gzorce C. HynpMAN on a New Species of Acaleph from Belfast Bay... Mr. Wit11aM Ocixsy on the Geographical Distribution of Animals im con- nection with the Progress of Human Civilization sessesesesecneneneneeeeneeeees Professor OWEN on the Homologies of the Cranial Vertebrae ...ccreceeseeereeres Mr. C. W. Pnacn on some Fishes, Crustacea and Mollusca found at Peterhead Dr. Wyvitiz T. C. THomson on the Character of the Sertularian Zoophytes PHYSIOLOGY. : Pate CiperenitacacaenAacnro tas senesacnsstmamennyabasenarsnTernatessinry sgrernconsaehi=* 420%. Professor T. 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SC f.5) ‘fqo100¢ E RO ee es ee 8D ‘Sed “SU Oo BT Od WL “A Is qedoxy Jo uapiserd ‘NOLdUIMWVHLUON JO SINOUVI 24 eri 's evslejalorwiels pin sce’ “s'yy'a ‘arepy JUNODSTA “L'a ‘oyng jo smbueyy oxy, SW CVI ‘WeMog Jorg AoW OL, “SUA “A “Auoqneg sossajorg “Wa “bsa ‘purpy yyzomuo yy -asy J ‘Sowa “ad “waqSUTUI} 83 AN po uvod eu “Aa A190, *pl0jxO, i “Zest ‘ee vung ‘auo0axo “Sta “WAL “LOqTEAN wWoqory ‘Aexy ) JO ace ayy OF *d* W ‘ is ae) a “bsg ‘“janoojsqy [jeuyong “xy seuopy, S$ ott *** P1OJXO JO AVISIOATA) BY} 1OF “AW is treba enter eee se ween ears eens AAISIVATUL) 99 JO AOTJaouryH-ar, oy, | ‘SUA “T'O'a “Med ‘SITONI AUUVH LUAGOU UIS sesso sure “pr0jxo Jo doystg ploy UL ‘SUA ‘essoy jo req oy, Pe eek: ac ToMog "Jord ‘Sd “dW “Ua “Jorg El dpaseishabe nev chals ola otetaneta foe) tateregare states "Sa “pxoyxXQ Jo doyste prory ot,7, age “bso ‘Apooyy ‘OcH | cree eee BR. ‘oot “TOE “alt “4g ‘woyMeIg “OFSI ‘OI toquiajdag ‘NoLaWVHENOS “L 231005) I A Is SHsIg Aina 4 -ceecccfzivus accee Coe Cop Guaer Aig SIO eee! Te 8S OO NOSIHOR AN Amar MOUACOU AIS - DODO SORMOREL ch /\¢ ‘aoysiow[eg JUNODSTA "TO" ‘oj ysy ploy tereeererpeor YSnoLOgIeA JO [AVA IT, *AaySOYOUT MA JO SMDIVAT oY, . ‘ II. Table showing the Names of Members of the British Association who have served on the Council in former years. Acland, Sir Thomas D., Bart., M.P., F.R.S. Acland, Professor H. W., B.M., F.R.S. Adamson, John, Esq., F.L.S. Adare, Edwin, Viscount, M.P., F.R.S. Ainslie, Rev. Gilbert, D.D., Master of Pem- broke Hall, Cambridge. Airy, G. B.,D.C.L., F.R.S.,Astronomer Royal. Alison, Professor W. P., M.D., F.R.S.E. Ansted, Professor D. T., M.A., F.R.S. Argyll, George Douglas, Duke of, F.R.S. Arnott, Neil, M.D., F.R.S. Ashburton, William Bingham, Lord, D.C.L. Babbage, Charles, Esq., F.R.S. Babington, C. C., Esq., F.L.S. Baily, Francis, Esq., F.R.S. Balfour, Professor John H., M.D. Barker, George, Esq., F.R.S. Bengough, George, Esq. Bentham, George, Esq., F.L.S. Bigge, Charles, Esq. Blakiston, Peyton, M.D., F.R.S. Boileau, Sir John P., Bart., F.R.S. Boyle, Right Hon. David, Lord Justice-Ge- neral, F.R.S.E. Brand, William, Esq. Brewster,Sir David,K.H.,D.C.L.,LL.D.,F.R.S. Principal of the United College of St. Sal- vator and St. Leonard, St. Andrews. Breadalbane, John, Marquis of, K.T., F.R.S. Brisbane, General Sir Thomas M., Bart., K.C.B., G.C.H., D.C.L., F.R.S. Brown, Robert, D.C.L., F.R.S. Brunel, Sir M. I., F.R.S. Buckland, Very Rev. William, D.D., Dean of Westminster, F.R.S. Burlington, William, Earl of, M.A., F.R.S., Chancellor of the University of London. Bute, John, Marquis of, K.T. Carlisle, George Will. Fred., Earl of, F.G.S. Carson, Rev. Joseph. Cathcart, Lt.-Gen. Earl of, K.C.B., F.R.S.E. Chalmers, Kev. T., D.D., late Professor of Divinity, Edinburgh. Chance, James, Esq. Chester, John Graham, D.D., Lord Bishop of. Christie, Professor S. H., M.A., Sec. R.S. Clare, Peter, Esq., F.R.A.S. Clark, Rev. Prof., M.D., F.R.S. (Cambridge). Clark, Henry, M.D. Clark, G. T., Esq. Clear, William, Esq. Clerke, Major Shadwell, K.H., R.E., F.R.S. Clift, William, Esq., F.R.S. Cobbold, John Chevalier, Esq., M.P. Colquhoun, J. C., Esq., M.P. Conybeare, Very Rev. W.D., Dean of Llandaff, M.A., F.R.S. Corrie, John, Esq., F.R.S. Currie, William Wallace, Esq. Dalton, John, D.C.L., F.R.S. Daniell, Professor J. F., F.R.S. Dartmouth, William, Earl of, D.C.L., F.R.S. Darwin, Charles, Esq., F.R.S. Daubeny, Prof. Charles G. B., M.D., F.R.S, De la Beche, Sir Henry T., C.B., F.R.S., Di- rector-General of the Geological Survey of the United Kingdom. Dillwyn, Lewis W., Esq., F.R.S. Drinkwater, J. E., Esq. Durham, Edward Maltby, D.D., Lord Bishop of, F.R.S. Egerton, Sir Philip de M. Grey, Bart., F.R.S. Eliot, Lord, M.P. Ellesmere, Francis, Earl of, F.G.S. Enniskillen, William, Earl of, D.C.L., F.R.S. Estcourt, T. G. B., D.C.L. 2 Faraday, Professor, D.C.L., F.R.S. Fitzwilliam, Charles William, Earl, D.C.L., F.R.S. Fleming, W., M.D. Fletcher, Bell, M.D. Forbes, Charles, Esq. Forbes, Professor Edward, F.R.S. Forbes, Professor J. D., F.R.S., Sec. R.S.E. Fox, Robert Were, Esq., F.R.S. Gassiot, John P., Esq., F.R.S. Gilbert, Davies, D.C.L., F.R.S. Graham, Professor Thomas, M.A., F.R.S. Gray, John E., Esq., F.R.S. Gray, Jonathan, Esq. Gray, William, jun., Esq., F.G.S. Green, Professor Joseph Henry, F.R.S. Greenough, G. B., Esq., F.R.S. Grove, W.R., Esq., F.R.S. Hallam, Henry, Esq., M.A., F.R.S. Hamilton, W. J., Esq., Sec.G.S. Hamilton, Sir William R., Astronomer Royal of Ireland, M.R.1.A. Harcourt, Rev. William Vernon, M.A., F.R.S. Hardwicke, Charles Philip, Earl of, F.R.S. Harford, J. S., D.C.L., F.R.S. Harris, Sir W. Snow, F.R.S. Harrowby, The Earl of. Hatfeild, William, Esq., F.G.S. Henslow, Rev. Professor, M.A., F.L.S. Henry, W. C., M.D., F.R.S. ; Henry, Rev. P.S., D.D., President of Queen’s College, Belfast. Herbert, Hon. and Very Rev. William, late Dean of Manchester, LL.D., F.L.S. Herschel, Sir John F. W., Bart.,D.C.L., F.R.S. Heywood, Sir Benjamin, Bart., F.R.S. Heywood, James, Esq., M.P., F.R.S. Hill, Rev. Edward, M.A., F.G.S. Hincks, Rev. Edward, D.D., M.R.I.A. Hodgkin, Thomas, M.D. Hodgkinson, Professor Eaton, F.R.S. Hodgson, Joseph, Esq., F.R.S. Hooker, Sir William J., LL.D., F.R.S. Hope, Rev. F. W., M.A., F.R.S. Hopkins, William, Esq., M.A., F.R.S. Horner, Leonard, Esq., F.R.S., F.G.S. Hovenden, V. F., Esq., M.A. Hutton, Robert, Esq., F.G.S. Hutton, William, Esq., F.G.S. Ibbetson,Capt. L. L. Boscawen, K.R.E., F.G.S. Inglis, Sir Robert H.,Bart.,D.C.L.,M.P.,F.R.S. Jameson, Professor R., F.R.S. Jeffreys, John Gwyn Jeffreys, Esq. Jenyns, Rey. Leonard, F.L.S. Jerrard, H. B., Esq. Johnston, Right Hon. William, Lord Provost of Edinburgh. Johnston, Professor J. F. W., M.A., F.R.S. Keleher, William, Esq. Kelland, Rev. Professor P., M.A. _ Lansdowne, Henry, Marquis of,D.C.L.,F.R.S. Lardner, Rev. Dr. Latham, R. G., M.D., F.R.S. Lee, Very Rev. John, D.D., F.R.S.E., Prin- cipal of the University of Edinburgh, Lee, Robert, M.D., F.R.S. Lefevre, Right Hon. Charles Shaw, Speaker of the House of Commons. Lemon, Sir Charles, Bart., M.P., F.R.S. Liddell, Andrew, Esq. Lindley, Professor John, Ph,D., F.R.S. Listowel, The Earl of. . Lloyd, Rev. Bartholomew, D.D., late Provost of Trinity College, Dublin. Lloyd, Rev. Professor, D.D., Provost of Trinity College, Dublin, F.R.S. ‘Lubbock, Sir John W., Bart., M.A., F.R.S. Luby, Rev. Thomas. Lyell, Sir Charles, M.A., F.R.S. MacCullagh, Professor, D.C.L., M.R.I.A. Macfarlane, The Very Rev. Principal. MacLeay, William Sharp, Esq., F.L.S. MacNeill, Professor Sir John, F.R.S. Malcolm, Vice Admiral Sir Charles, K.C.B. Manchester, James Prince Lee, D.D., Lord Bishop of, Meynell, Thomas, Jun., Esq., F.L.S. Middleton, Sir William, F. F., Bart. Miller, Professor W. H., M.A., F.R.S. Moillet, J. L., Esq. Moggridge, Matthew, Esq. Moody, J. Sadleir, Esq. Moody, T. H. C., Esq. Moody, T. F., Esq. Morley, The Ear! of. Moseley, Rev. Henry, M.A., F.R.S. Mount-Edgecumbe, Ernest Augustus, Earl of. Murchison, Sir Roderick I., G.C.St.S., F.R.S. Neill, Patrick, M.D., F.R.S.E. Nicol, D., M.D. Nicol, Rey. J. P., LL.D. Northumberland, Hugh, Duke of, K.G., M.A., F.R.S. Northampton, Spencer Joshua Alwyne, Mar- quis of, V.P.R.S. Norwich, Edward Stanley, D.D., F.R.S., late Lord Bishop of. Norwich, Samuel Hinds, D.D., Lord Bishop of. Ormerod, G. W., Esq., F.G.S. Orpen, Thomas Herbert, M.D. Orpen, J. H., LL.D. Owen, Professor Richard, M.D., F.R.S, Oxford, Samuel Wilberforce, D.D., Bishop of, F.R.S., F.G.S. Osler, Follett, Esq. Palmerston, Viscount, G.C.B., M.P. Peacock, Very Rev. George, D.D., Dean of Ely, F.R.S. Peel, Rt. Hon. Sir Robert, Bart., M.P., D.C.L., F.R.S. Pendarves, E., Esq., F.R.S. Phillips, Professor John, F.R.S. Porter, G. R., Esq. Powell, Rev. Professor, M.A., F.R.S. Prichard, J. C., M.D., F.R.S. Ramsay, Professor W., M.A. Reid, Lieut.-Col. Sir William, F.R.S. Rendlesham, Rt. Hon. Lord, M.P. Lord Rennie, George, Esq., V.P.R.S. Rennie, Sir John, F.R.S. Richardson, Sir John, M.D., F.R.S. Ritchie, Rev. Professor, LL.D,, F.R.S. Robinson, Rev. J., D.D. Robinson, Rev. T. R., D.D., Pres. R.I.A., F.R.A.S., Robison, Sir John, late Sec.R.S.Edin. Roche, James, Esq. Roget, Peter Mark, M.D., F.R.S. Ronalds, Francis, F.R.S. Rosebery, The Earl of, K.T., D.C.L., F.R.S. Ross, Capt. Sir James C., R.N., F.R.S, Rosse, William, Earl of, M.A., M.R.I.A., President of the Royal Society. Royle, Professor John F., M.D., F.R.S. Russell, James, Esq. Russell, J. Scott, Esq. Sabine, Col. Edward, R.A.,Treas. & V.P.R.S. - Saunders, William, Esq., F.G.S. Sandon, Lord. Scoresby, Rev. W., D.D., F.R.S. Sedgewick, Rev. Professor Adam, M.A.,F.R.S. Selby, Prideaux John, Esq., F.R.S.E. Smith, Lieut.-Colonel C. Hamilton, F.R.S. Spence, William, Esq., F.R.S. Staunton, Sir George T., Bart., M.P., D.C.L., F.R.S. St. David’s, Connop Thirlwall, D.D., Lord Bishop of. Stevelly, Professor John, LL.D. Stokes, Professor G. G., F.R.S. Strang, John, Esq. Strickland, H. E., Esq., F.G.S. Sykes, Lieut.-Colonel W. H., F.R.S. Symonds, B. P., D.D., late Vice-Chancellor of the University of Oxford. Talbot, W. H. Fox, Esq., M.A., F.R.S. Tayler, Rev. J. J. Taylor, John, Esq., F.R.S. Taylor, Richard, Jun., Esq., F.G.S. Thompson, William, Esq., F.L.S. Tindal, Captain, R.N. Tod, James, Esq., F.R.S.E. Traill, J. S., M.D. Turner, Edward, M.D., F.R.S. Turner, Samuel, Esq., F.R.S., F.G.S. Turner, Rey. W. Vigors, N. A., D.C.L., F.L.S. Vivian, J. H., M.P., F.R.S. Walker, James, Esq., F.R.S. Walker, Joseph N., Esq., F.G.S. Walker, Rey. Robert, M.A., F.R.S. Warburton, Henry, Esq., M.A., M.P., F.R.S. Washington, Captain, R.N. West, William, Esq., F.R.S. Western, Thomas Burch, Esq. Wharncliffe, John Stuart, Lord, F.R.S. Wheatstone, Professor Charles, F.R.S. Whewell, Rev. William, D.D., F.R.S., Master of Trinity College, Cambridge. Williams, Professor Charles J.B., M.D.,F.R.S. Willis, Rev. Professor Robert, M.A., F.R.S. Wills, William. Winchester, John, Marquis of. Woollcombe, Henry, Esq., F.S.A. Wrottesley, John, Lord, M.A., F.R.S. Yarrell, William, Esq., F.L.S. Yarborough, The Earl of, D.C.L. Yates, James, Esq., M.A., F.R.S. BRITISH ASSOCIATION FOR THE THE GENERAL TREASURER’S ACCOUNT from 2nd of July RECEIPTS. * £9. a Es, Sa. To Balance brought on from last account .............cc..ceeseeeeeeees 693 5 11 Life Compositions at Ipswich and since ..............08 rec oe Se 909 0 0 Annual Subscriptions at Ipswich and since ............cs0eeesseeee 202 0 0 Associates’ Subscriptions at Ipswich ................seccceeessneeenes 244 0 0 Harpies? Tickets at Mpswiehl es 0.i% . sovicesdessscacedescseseseideeasece 141 0 0 IG AE OTR POSH testes irae tsar taste E et ce vanccosiectasnceescca scene 5.0 0 - Dividends on Stock (eighteen months’ Dividends on £3500 eo MEM CENESMOUNGIN) Ce is Panahes Pease vs isoseesalasodeossie eens ccs 152 18 3 From the Sale of Publications :—Reports, Catalogues of Stars, &c.:— RVOLU TGR Gare epee senataets § duty cee tpl edetansse Ss 018 0 Draka decenteer Asada sta: a ited cus rete pee Th oe 016 0 Rib idbentiey ok tie vaess (ac sisGe nasties bigs Ss oboe lywd 0 SEU meen as Saeccoh tte cede losis uiandtrat ives 013 0 GS hace ee hae See yeneacecccccessecceeess 1 iii Bi Weta tcals catyassadt se oc uiccoecstas Medaet dare en 016 6 UNM tetas RECN so escercnas ccenterascnite 015 0 Oh Sav cdyenanveccnccann 2p Ortassostesen eat Meenas 215 0 Laan cepa re Peo ARSE COOBL ARES Secon OAD O LD eer eerccet geuet ib esasa. Sass 5. vccs caput 010 6 D2 tes tn der tires k Sema Ne nak cee. sac eteney ease 016 0 Di Seneragnaaan trate fe-assseucy sretesewarsccanehs iL GES Ee Micine stone teedecnade mpeaicvaacindniearrsches es 2 0 0 ee Aa Schnsmsnddeciee sosuckteccerntecteseatae 015 0 UG? 5 essd6 ne beer sane en eo (en ed sSSonp voemnreteane 5 8 0 NZ) Septesi vais cateds Stent daeaanien ery mes anaaats 2 8 0 ED Ceseasaressaetred Pi des os Saveanebates Bass 5 6 8 UM peer pcaseatmetUats osviecssddcns ON corns 6410 0 British Association Catalogue of Stars.........cccsssceeeeeues 56 3 6 Lalande’s Catalogue of Stars............ gedsuscurpushesaacerteed 5 3 0 Lacaille’s Catalogue of Stars..........0s00ssscsssssessovecesonde 016 0 Dove’s Isothermal Lines ...........seseseseseees adenae « eseaeen 9 ed Lithographic Signatures ......seccsssees Ser pane nad teadrasaaacen 0, 7940 —_——_ 162 13 1690 17 6 Audited and found correct, CHARLES C. BABINGTON, Auditor. ADVANCEMENT OF SCIENCE. 1851 (at Ipswich) to 1st of September 1852 (at Belfast). PAYMENTS. £sda & s&s a For Sundry Printing, Advertising, Expenses of Ipswich Meeting, and Petty Disbursements made by General and Local Trea- PRMCE Sn estes ate seh cigat pie steiay a ceiver cases stele s.sicw si sis iP acuaultecawitucpe ee paas 206 14 2 Printing Report of 20th Meeting (paid on Account) ............00 300 0 0 Engraving, &c. for Report of the 21st Meeting ..............c0s000 17 610 Salaries, Assistant General Secretary and Accountant, (eighteen AULD) acc acne a5 co wnachieersasaccucsciancesicenaas dopwieve aueslars sored 525 0 0 Moyers tsothermal Lines) \iicencesecess cn ccscogesssscnssessensscecesacas 100 0 0 Maintaining the Establishment at Kew Observatory :— Balance of Grant of 1850 .........csesseccseeusecnseetrneeneees aie west DOL! oO atigOh Grant TONE BOM clips sca dedstceroecdsssscsceovassexesuensees 204 4 8 . —— 23317 8 On account of Grant— For Experiments on the Conduction of Heat .............00008 5° 2 9 Influence of Solar Radiations ...........cccececacneasceeteeeoeees 20 0 0 For a Geological Map of Great Britain and Ireland ......... 1 00 Researches on the British Annelida........... peasinas a anun seit pice 10 00 Data OyNOE SECON M aetebuestenasdovemwar ae dries canoccbcensatlacts wana 10 6 2 Sirength Of Boiler Plates ......s0r.dsesessssecccevscadceccucedeees 10 0 0 Balance at the Bankers.........s00.csessssssceeeeenecvees Da ASN Aes ois 22617 3 Ditto in the hands of the General Treasurer and Local Treasurers 1012 8 Se a7 9) Tt vA ve t 1, s 1690 17 6 OFFICERS AND COUNCIL, 1852-53. TRUSTEES (PERMANENT). Sir Roperick I.Murcuison,G.C.St.S.,F.R.S. The VeryRev.Gzorcz Peacock,D.D., Dean Joun Tayxor, Esq., F.R.S. of Ely, F.R.S. PRESIDENT. COLONEL EDWARD SABINE, R.A., Treasurer and Vice-President of the Royal Society. VICE-PRESIDENTS. The Eart of ENNISKILLEN, D.C.L., F.R.S. Rev. T. R. Rozrnson, D.D., Pres.R.LA., The Ear of Rosse, M.A., M.R.I.A., Presi- F.R.A.S. dent of the Royal Society. Grorce GABRIEL STOKES, F.R.S., Lucasian Sir Henry T. De ta Becue, C.B., F.R.S., Professor of Mathematics in the University Director-General of the Geological Survey of Cambridge. of the United Kingdom. Joun Streve.ty, LL.D., Professor of Natural Rey. Epwarp Hrincxs, D.D., M.R.LA. Philosophy in Queen’s College, Belfast. Rey. P. S. Henry, D.D., President of Queen’s College, Belfast. PRESIDENT ELECT. Wir1am Hopxuys, Esq., M.A., V-P.R.S., F.G.S., Pres. Cambr. Phil. Soc. VICE-PRESIDENTS ELECT. The Eart of Caruisxe, F.R.S. Cuartes Frost, Esq., F.S.A., President of The Lorp LonpEssorovuGH, F.R.S. the Hull Lit. & Philos. Society. Micwaet Farapay, D.C.L., F.R.S., Pro- Wixxram Sreence, Esq., F.R.S, fessor of Chemistry in the Royal Institu- Lt.-Colonel W. H. Syxzs, F.R.S. tion of Great Britain. Cuar.tes WuHeatstong, Esq,, F.R.S., Pro- Rey. Apam Sepewrck, M.A., F.R.S., Wood- fessor of Experimental Philosophy in King’s wardian Professor of Geology in the Uni- College, London. versity of Cambridge. LOCAL SECRETARIES FOR THE MEETING AT HULL. Henry Cooper, Esq., M.D., V.P. Hull Lit. & Phil. Soc. Beruet Jacoss, Esq., President of the Hull Mechanics Institution. LOCAL TREASURER FOR THE MEETING AT HULL. Epmunp Smiru, Esq. ORDINARY MEMBERS OF THE COUNCIL. J. C. Apams, Pres.R.A.S. Joun P. Gassror, F.R.S. Prof. OwEn, LL.D., F.R.S. C. C. Banineton, F.R.S. Witiram R, Grove, F.R.S. Francis Ronaups, F.R.S. Professor BELx, Sec.R.S. Rozert Hutton, F.G.S. SirJ.Ciarx Ross, R.N.,F.R.S. Prof.Dauseny, M.D.,F.R.S. James Heywoop, Esq.,M.P. Prof.H.E.SrrickLanp,F.R.S. Sir P. Ecrrton, Bart., F.R.S. Rev. Dr. H. Luoyn, F.R.S. Lt.-Col. W. H. Syxzs, F.R.S. Professor E. Forses, F.R.S. Sir C. Lemon, Bart., F.R.S.. Prof. Wanker, M.A., F.R.S. Professor GRAHAM, F.R.S. Prof, W. H. Mriiuer, F.R.S. Lorp Wrotrestey, F.R.S. EX-OFFICIO MEMBERS OF THE COUNCIL. The President and President Elect, the Vice-Presidents and Vice-Presidents Elect, the Ge- neral and Assistant-General Secretaries, the General Treasurer, the Trustees, and the Presi- dents of former years, viz. The Earl Fitzwilliam. Rev. Dr. Buckland. Rey. Professor Sedgwick. Sir Thomas M. Brisbane. The Marquis of Lansdowne. The Earl of Burlington. Rey. W. Y. Harcourt. The Marquis of Breadalbane. Rev. Dr. Whewell. The Earl of Ellesmere. The Earl of Rosse. The Dean of Ely. Sir John F. W. Herschel, Bart. Sir Roderick I. Mur- chison. Sir Robert H. Inglis. The Rev. Dr. Robinson. Sir David Brewster. G. B. Airy, Esq., the Astronomer Royal. GENERAL SECRETARY. J. Forzes Royte, M.D., F.R.S., Prof. Mat. Med. & Therap. in King’s College, London. ASSISTANT GENERAL SECRETARY. Joun Pures, Esq., F.R.S., York. CENERAL TREASURER. Joun Tartor, Esq., F.R.S., 6 Queen Street Place, Upper Thames Street, London. LOCAL TREASURERS. William Gray, Esq., York. Professor Ramsay, Glasgow. C. C. Babington, Esq., Cambridge. G. W. Ormerod, Esq., Manchester. William Brand, Esq., Edinburgh. J. Sadleir Moody, Esq., Southampton. J. H. Orpen, LL.D., Dublin. John Gwyn Jeffreys, Esq., Swansea. William Sanders, Esq., Bristol. J. B. Alexander, Esq., Ipswich. W.R. Wills, Esq., Birmingham. Robert Patterson, Esq., Belfast. AUDITORS. J. W. Gilbart, Esq. J. P. Gassiot, Esq. C. C. Babington, Esq. Ee OFFICERS OF SECTIONAL COMMITTEES. XXill OFFICERS OF SECTIONAL COMMITTEES PRESENT AT THE BELFAST MEETING. SECTION A.—MATHEMATICS AND PHYSICS. President. Professor William Thomson, M.A., F.R.S. L. & E. Vice- Presidents. J.C. Adams, F.R.S. Sir David Brewster, K.H., F.R.S.; Right Rev. Dr. Denvir, Sir W. R. Hamilton, Astron. Royal for Ireland; Rev. Dr. Lloyd, F.R.S.; Professor Stokes, F.R.S. Secretaries. W.J. Macquorn Rankine; John Tyndall, Ph.D.; Professor Dixon, F.T.C.D.; Professor Stevelly. SECTION B. CHEMISTRY AND MINERALOGY, INCLUDING THEIR APPLICATION TO AGRICULTURE AND THE ARTS. President.—Thomas Andrews, M.D., F.R.S. Vice-Presidents. Professor Apjohn, M.R.I.A.; Professor Connell, F.R.S.E. ; Professor Graham, F.R.S. Secretaries. Professor Hodges; Professor Ronalds; Dr. Gladstone. SECTION C.—GEOLOGY AND PHYSICAL GEOGRAPHY. President.—Lieutenant-Coionel Portlock, R.E., F.R.S. Vice-Presidents. Richard Griffith, F.G.S.; Sir H. De la Beche, F.R.S.; James Smith, Esq., F.G.S. Secretaries, James Bryce, F.G.S.; James MacAdam, F.G.S.; Professor M‘Coy, F.G.S.; Professor Nicol, F.G.S. SECTION D.—ZOOLOGY AND BOTANY, INCLUDING PHYSIOLOGY. President. W. Ogilby, Esq. Vice-Presidents. Professor Allman; Professor Walker Arnott; Dr. Robert Ball; Professor E. Forbes; Professor Owen. Secretaries. George C. Hyndman, Esq. ; Edwin Lankester, Esq., M.D., F.R.S. ; Dr. Dickie. SECTION E.—GEOGRAPHY AND ETHNOLOGY, President.—Colonel Chesney, R.A., D.C.L., F.R.S., F.R.G.S., &c. Vice-Presidents.—Sir R. I. Murchison, G.C.St.S., F.R.S., Pres. R.G.S.; Rev. Dr. E. Hincks. Secretaries.—Richard Cull, Esq., Hon. Secretary Ethnological Society, London ; Robert MacAdam, Esq.; Norton Shaw, M.D., Assistant Secretary Royal Geogra- phical Society, London. SECTION F.—STATISTICS. President.—His Grace the Archbishop of Dublin. Vice-Presidents.—Lord Dufferin; Mountiford Longfield, Esq., LL.D. ; Major Thomas A. Larcom, R.E.; Lieutenant-Colonel Sykes, F.R.S.; Valentine Whitla, Esq. ; the Earl of Mayo; James Heywood, Esq., M.P., F.R.S. Secretaries.— Professor Hancock, LL.D. ; James MacAdam, Jun., Esq.; Professor Ingram, F.T.C.D. SECTION G.—MECHANICAL SCIENCE. President.—James Walker, Esq., C.E., LL.D., F.R.S. L. & E. Vice-Presidents.—William Fairbairn, C.E.; John Godwin, Esq., C.E.; C. Lan- yon, Esq., C.E.; Alex. Mitchell, Esq., C.E. Secretaries.—John Frederick Bateman, Esq.; Charles B. Hancock, Esq. ; Charles Manby, Esq., Sec. Inst. C.E.; James Thomson, Esq., C.E. XxXlv REPORT—1852. CORRESPONDING MEMBERS. Professor Agassiz, Cambridge, Massa- | Dr. Langberg, Christiania. | chusetts. M. Leverrier, Paris. 4 M. Arago, Paris. Baron de Selys-Longchamps, Liége. — - 3 M. Babinet, Paris. Dr. Lamont, Munich. | Dr. A. D. Bache, Philadelphia. Baron von Liebig, Munich. p| Professor H. von Boguslawski, Breslau. | Professor Gustav Magnus, Berlin. | Mr. P. G. Bond, Cambridge, U.S. | Professor Matteucci, Pisa. Monsieur Boutigny (d’Evreux), Paris. Professor von Middendorff, St. Peters- Professor Braschmann, Moscow. | burg. ; Chevalier Bunsen (Prussian Embassy), | Professor Nilsson, Sweden. | London. | Dr. N. Nordengsciold, Finland. Prince Charles Buonaparte, Paris. | Chevalier Plana, Turin. M. De la Rive, Geneva. M. Quetelet, Brussels. Professor Dove, Berlin. | Professor Pliicker, Bonn. M. Dufrenoy, Paris. | M. Constant Prevost, Paris. Professor Dumas, Paris. Professor C. Ritter, Berlin. Dr. J. Milne-Edwards, Paris. | Professor H. D. Rogers, Philadelphia, Professor W. B. Rogers, Virginia. Professor H. Rose, Berlin. Professor Ehrenberg, Berlin. Dr. Eisenlohr, Carlsruhe. Professor Encke, Berlin. | Baron Senftenberg, Bohemia. Dr. A. Erman, Berlin. | Dr. Sihestrom, Stockholm. Professor Esmark, Christiania. | M. Struvé, St. Petersburg. Professor G. Forechhammer, Copenhagen. | Dr. Svanberg, Stockholm. M. Frisiani, Milan. | Dr. Van der Hoeven, Leyden. Professor Asa Gray, Cambridge, U.S. | Baron Sartorius von Waltershausen, Professor Henry, Washington, U.S. Gotha. Baron Alexander von Humboldt, Berlin. | M. Pierre Tchihatchef, (Russian Em- M. Jacobi, St. Petersburg. bassy), Paris. Professor Kreil, Prague. Professor Wartmann, Lausanne. ; M. Kupffer, St. Petersburg. 4 REPORT ON THE PROCEEDINGS OF THE COUNCIL IN 1851-52, AS PRESENTED TO THE GENERAL CoMMITTEE AT BELFrast, WEDNESDAY, SEPT. 1, 1852. “J, With reference to the subjects referred to the Council by the General Committee at Ipswich, the Council have to report as follows :— (a) The Council having requested the President, Mr. Airy, to use his best endeavours to obtain from Government a grant towards the publication of Mr. Huxley’s Zoological and Anatomical Researches, made during the voyage of H.M.S. ‘ Rattlesnake,’ have been informed by Mr. Airy that the Govern- ment have expressed their inability to make a grant for that purpose in the present year: the Council recommend that the application should be re- eated. ‘ (6) The Council requested the President, Mr. Airy, to communicate to Her Majesty’s Government, and to the Court of Directors of the East India Company, the recommendation approved by the General Committee, that the necessary aid should be given for the speedy publication of the Bo- tanical Researches of Drs. Hooker and Thomson, Captain Strachey and Mr. Winterbottom, so as to constitute, by combination with former publications, a general Indian Flora. The Council have been informed by Mr. Airy, first, that Dr. Hooker is engaged under an instruction from Government, in arranging his materials for publication, in three volumes, the first of which will not be ready before November 1852; and that no immediate application e REPORT OF THE COUNCIL. XXV for further assistance is required ; and secondly, that, having ascertained the state of preparation of Dr. Thomson’s researches, he has laid the case fully before the Court of Directorsin a letter to Mr. Melvill, to which he has as yet received no reply. (ce) The Council requested the President, Mr. Airy, to make the necessary application to the Court of Directors of the East India Company to afford Captain Strachey such aid as would enable him to publish his explorations in the Himalaya Mountains and in Thibet, with the necessary maps and illustrations; and have learned from Mr. Airy that he has been informed that the Chairman of the Court of Directors has signified his intention of giving to Captain Strachey the assistance contemplated by the Association, and that he has therefore taken no further step. “TI. The President, as one of the Committee for Tidal Observations in the Atlantic appointed by the General Committee at Ipswich, has communicated to the Council the Memorial which the Tidal Committee has presented to Government. It is as follows :— “*We beg leave to make to Her Majesty’s Government a representation with which we have been charged by the British Association for the Ad- vancement of Science, respecting the importance of ‘sending out a ship or ships to extend our acquaintance with the phenomena of the Tides of the Atlantic Ocean. « «The importance of an acquaintance with the phenomena of the Tides, both for practical and theoretical purposes, is sufficiently obvious, and has been recognised by the Government of this country in many ways. At most of the points of our own coast, and at several places in other countries, observations have long been made which suffice for most of these purposes. But perhaps it is not generally understood how far these observations, hitherto, are from giving us such a connected knowledge of the subject as may enable us to follow the course of the tide over any considerable portion of the Ocean. Even with regard to our own shores, such accurate know- ledge hardly existed till observations were made and continued for a fortnight at the coast-guard stations of Great Britain and Ireland in June 1834, and again in June 1836. On the latter occasion application was also made to foreign maritime states, to make a similar and simultaneous series of obser- vations, the Duke of Wellington, at that time Foreign Secretary of State, promoting the object in a manner which procured from them the most cordial and effective co-operation. The results of these observations were inserted and discussed in the Philosophical Transactions for 1836 (Part II.); and, in consequence, the course of the tides along the shore from the Strait of Gibraltar to the coast of Norway, was made out, as to some general features and also along the coast of the United States. But beyond these limits we may be said to have no connected knowledge of the course of the tides of the Atlantic; and even within these limits it is impossible, for want of other observations, to counect those which were made; for instance, the tides on the American and the European shores. Along the coasts of Africa and of South America we are ignorant of the course and progress of the tides, although we know some of the phanomena at detached points, and know some of them to be remarkable and perplexing. Nor is it at all likely that these defects in our knowledge will be removed by any collection of de- tached observations. It is only by systematic observations made with the express view of connecting our knowledge on this subject, and pursued from place to place, as the results themselves suggest, that we shall ever obtain a general view of the facts. Such observations might be made in no long XXvl REPORT—1852. time if an expedition were sent out with this special and exclusive object ; and might, in that case, be so conducted as to lead with certainty to the result. «“ «The best mode of making observations would, probably, be found to be to place observing parties at certain distances along the coast, the intervals being various according to the nature of the phenomena; and to direct them to make simultaneous observations for a few daysyand then to proceed farther along the coast with the expedition; or the tides at any place might (on any day) be referred to the moon’s transit, and this would afford suffi- cient means of comparison with any neighbouring case, unless the phzno- mena were peculiar. In this way the progress of the tide-wave along the coasts of Africa and America would be determined; from what points it diverges, and towards what points it converges ; the latter points being, it is presumed, generally those of very high tides, such as occur on the east coast of Patagonia. With these observations, combined with others at oceanic islands, the general course of the tide elevation might be traced ; and if this were done for the Atlantic, it would be the first time that the course of the tide in such an ocean-space has been made known to us. “ “Ino OO Oo BID ment at Kew Observatory 171 15 11 9 0 0 0 0 8 1849. Electrical Observations Kew Observatory ...... Maintaining Establishment abiditio® kOe A Te Vitality of Seeds.......... 5 On Growth of Plants...... 5 Registration of Periodical Phenomena .......... Bill on account of Anemo- metrical Observations.... at 10 13 £159 19 1850. Maintainmg the Establish- ment at Kew Observatory 255 Transit of Earthquake Waves 50 Periodical Phenomena .... 15 Meteorological Instrument, Azores...... BF aie nrg: alo oOo OfFn Oo Colo ocSo 1851. Maintaining the Establish- ment at Kew Observatory (eludes part of grant in BE iis ote teh vin hth 309 Experiments on the Theory Ge testis. oar rs tare Periodical Phenomena of Animals and Plants .... 5 Vitality of Seeds.......... 5 Influence of Solar Radiation 30 Ethnological Inquiries .... 12 Researches on Annelida.... 10 20 £391 Crooconeo NI OOCORS 1852. Maintaining the Establish- ment at Kew Observatory (including balance of grant for IBS) 4p). ken tawl 23 Experiments on the conduc- tion of Heat Influence of Solar Radiations Geological Map of Ireland Researches on the British HANG lidayee homre eects tin 1-5 Vitality of seeds........., 1 Strength of Boiler Plates 10 £304 AlJoOno cow NS/oneo oow @ xl REPORT—1852. Extracts from Resolutions of the General Committee. Committees and individuals, to whom grants of money for scientific pur- poses have been entrusted, are required to present to each following meeting of the Association a Report of the progress which has been made; with a statement of the sums which have been expended, and the balance which remains disposable on each grant. Grants of pecuniary aid for scientific purposes from the funds of the As- sociation expire at the ensuing meeting, unless it shall appear by a Report that the Recommendations have been acted on, or a continuation of them be ordered by the General Committee. In each Committee, the Member first named is the person entitled to call on the Treasurer, John Taylor, Esq., 6 Queen Street Place, Upper Thames Street, London, for such portion of the sum granted as may from time to time be required. In grants of money to Committees, the Association does not contemplate the payment of personal expenses to the Members. In all cases where additional grants of money are made for the continua- tion of Researches at the cost ak the Association, the sum named shall be deemed to include, as a part of the amount, the specified balance which may remain unpaid on the former grant for the same object. General Meetings. On Wednesday, Sept. Ist, at 8 p.m., in May Street Church, Sir Roderick I. Murchison, G.C.St.S., F.R.S., on the part of G. B. Airy, Esq., M.A, D.C.L., F.R.S., Astronomer Royal, resigned the office of President to Colonel Edward Sabine, R.A., Treas. and V.P. R.S., who took the Chair at the General Meeting, and delivered an Address, for which see p. xli. On Thursday, Sept. 2nd, a Soirée took place from 8 to 10 P.M., in the rooms of Messrs. Workman, which had been arranged for the purpose. On Friday, Sept. 3rd, at 8 p.m., in May Street Church, G. G. Stokes, F.R.S., Lucasian Professor of Mathematics at Cambridge, delivered a Dis- course on some recent discoveries in the properties of Light. On Saturday, Sept. 4th, at 8 p.m., a Soirée took place in the rooms of Messrs. Workman. On Monday, Sept. 6th, at 8 p.m., Colonel Portlock, R.E., F.R.S., delivered a Discourse on the recent discovery of Rock-salt at Carrickfergus, and the geological and practical considerations connected with it. On Wednesday, Sept. 8th, at 3 p.m., the concluding General Meeting of the Association was held in May Street Church, when the Proceedings of the General Committee, and the grants of Money for scientific purposes were ex- plained to the Members. The Meeting was then adjourned to Hull*. * The Meeting is appointed to take place on Wednesday, the 7th of September, 1853. ADDRESS BY COLONEL EDWARD SABINE, RA,, TREASURER AND VICE-PRESIDENT OF THE ROYAL Society. GENTLEMEN OF THE BritisH ASSOCIATION, My first duty in addressing you from this Chair, must be to express my | grateful thanks for the high honour you have conferred upon me by placing me in so distinguished a position. My acknowledgements are due in the first place to the gentlemen of Belfast, who by their Provisional Committee brought my name before the Council as that of a person whose nomination to the Presidency would give satisfaction at Belfast; next, to my colleagues in the Council, who adoped the suggestion of the Provisional Committee, strengthening it by their approval; and finally, to the General Committee (the governing body), by whom it was confirmed. The strong attachment which I am known to have felt for so many years to the British Association will be my best guarantee that no endeavours shall be wanting on my part to perform the duties of the Office to the utmost of my power. i Gentlemen, we meet for the third time in the Sister Kingdom, on the invitation, which has been most welcome to us, of a part of the kingdom which has furnished to the British Association so large a proportion of dis- | tinguished members actively engaged in almost every department of science. On our arrival, we find ourselves surrounded by faces familiar to us in the | recollections of many previous meetings, and long recognised as amongst the “warmest and steadiest friends of our Association. Our meeting is graced “and honoured by the presence of Her Most Gracious Majesty’s representa- tive in Ireland. With ample and excellent accommodation liberally provided in the fullest anticipation of our wants, and with the evidence which forcibly impresses itself on every side of rapidly increasing prosperity, opening a wide pr ae xhii REPORT—1852. field for the practical applications of science, our satisfaction in assembling here would be complete, were it not clouded by the absence of one friend who would have been among the foremost to have welcomed us to this meeting which he prepared, the Naturalist of Ireland, whose memory will long be honoured and cherished by the members of the British Association. The ever-increasing activity of the various branches of science embraced by the British Association is such, as to render it scarcely possible to com- prehend within the limits of an address of the usual length, even a brief review of the progress made in the seven departments which constitute our Sections. In the selection which I have thus found myself compelled to make, I have been guided by a practical principle, which appears not unsuited to an Association in which the Presidency is an annual office, viz. that the President for the year should notice by preference those subjects with which he is most familiar, in which the Association as a body have taken a part, or which are likely to be discussed at the meeting over which he presides. Among the subjects which are likely to come before the Mathematical and Physical Section, there is none perhaps of greater importance, or requiring more careful consideration, than the question whether the time is arrived, when the establishment of an Observatory in the Southern Hemisphere, fur- nished with instruments of suitable optical power for the examination of the Nebule of the southern heavens, and devoted exclusively to that branch of sidereal astronomy, should be again brought under the consideration of Her Majesty’s Ministers. I need not occupy your time by restating on this occasion the reasons both of scientific and national concernment, which in- duced the two principal Scientific Institutions of the United Kingdom, con- jointly, to recommend to those entrusted with the administration of public affairs, the formation of an establishment of this description in some fitting part of Her Majesty’s southern dominions. I would rather refer you to the memorial presented to Government by the Earl of Rosse on the part of the Royal Society, and by Dr. Robinson on the part of the British Association, not only because it contains such a complete and formal exposition, as may be most advantageously consulted by those who will now be called upon to take part in the reconsideration of the subject, but also because it appears to me to furnish an admirable model both in spirit and in matter, for communi- cations designed to fulfil the important purpose of conveying in an official form the opinions and suggestions which the united body of scientific men of this Kingdom may desire from time to time to bring under the considera- tion of the Executive. In the discussions which took place at a former period, the only difficulty ~ which appeared to be apprehended in reference to the successful working of such an establishment, arose from a doubt whether mirrors of the required magnitude could be repolished, as they would frequently need to be, on the spot. This difficulty has now it is understood been entirely removed by the improvements which the noble Earl, the President of the Royal Society, to t ADDRESS. xii whom science is so deeply indebted for the instrumental means of prosecuting these researches, has made in the apparatus for repolishing the mirrors, and in the instructions for the guidance of those who may have occasion to employ it, which his own great personal experience has enabled him to prepare. ; In this happy country, in which men are free to consider and to discuss the propriety of public support being given to undertakings conducive to national honour, and are encouraged to do so by the experience that public men of all parties who succeed each other in administration, seek to be guided by en- lightened public opinion, we may justly entertain the full conviction that - meastires which from their intrinsic importance deserve to be adopted will sooner or later obtain the consideration they merit. When such propositions ate brought in the first instance,—as in the class of subjects with which we are here concerned it is desirable they should be,;—before those public bodies which are justly regarded as possessing the highest scientific authority in this country, and as most competent to judge of them, they cannot be too carefully considered and discussed, before by their adoption they become invested with the authority and weight which those bodies have it in their power to impart: But when after due deliberation they have been so adopted, it is equally fitting that those publie bodies should be true to their own convictions, and should steadily persevere in urging on all proper occasions, both publicly and pri- vately, the measures which they believe will‘add to their country’s honour, as well as to that general advancement of science by which all nations benefit freely and alike in proportion tu their degree of mental cultivation. That an Observatory for the purpose specified, in a part of the globe where it can render peculiar service, and where we possess facilities which other nations do not possess, will ere long be established, no one I believe entertains a doubt. The importance was admitted by the Ministry to whom the reeom- mendation was made, the only question with them appearing to be one of time. When therefore we view the intrinsic merit of the proposition itself, the general interest which it has excited at home and abroad, and its already; to a certain extent, favourable reception by Government, we cannot doubt ‘that we have but to persevere, and by a judicious selection of times and opportunities the object will be secured. It will be for the Members of the ‘Mathematical and Physical Section to consider in the first instance, and for 3 the General Committee, subsequently, to consider and decide whether any Official step shall be taken by the British Association in the present year. Should such be your decision, it will be the duty of the Officers and Council of the Association to confer with the President and Council of the Royal _ Society, and in conjunction with them to take such steps as may appear most fitting to bring the subject again, and in the most impressive manner, under the consideration of the Authorities of the State. On the former occasion it was thought most respectful to abstain from any suggestion in regard either to a suitable locality, or to the Astronomer who might be advantageously xliv REPORT—1852. selected to direct an establishment of this novel description. Such may still be deemed, perhaps, the least exceptionable course; but at the same time it may be desirable that it should be fully known, that we are not unprepared. on these and other points, if it be the pleasure of Her Majesty’s Government to desire our opinion. Hitherto the researches of Sidereal Astronomy, even in their widest exten- sion, had manifested the existence of those forces only with which we are familiar in our own solar system. The refinements of modern observation and the perfection of theoretical representation, had assured us that the orbits in which the double stars, immeasurably distant from us, revolve around each other, are governed by the same laws of molecular attraction which determine the orbits of the planetary bodies of our own solar system. But the Nebulz have revealed to us the probable existence in the yet more distant universe, of forces with which we were previously wholly unacquainted. The highest authorities in this most advanced of all the sciences, acknowledge themselves unable-even to conjecture the nature of the forces which have produced and maintain the diverse, yet obviously systematic arrangement of the hosts of stars which constitute those few of the Spiral Nebule which have been hitherto examined. Hence the importance of increasing our knowledge of the variety of forms in which the phenomena present them- selves, by a similar examination of the Southern Heavens to that which Lord Rosse is accomplishing in the Northern Heavens; hence also, we may believe, in great measure, the devotion with which his Lordship has directed the un- precedented instrumental power which he has created almost exclusively to the observation of nebule. But whilst we cannot but admire the steadiness of purpose with which an object regarded as of paramount importance is un- deviatingly pursued, we can scarcely forbear to covet at least an occasional glance at bodies which from their greater proximity have more intimate relations with ourselves, and which, when viewed with so vast an increase of optical power, may afford instruction of the highest value in many branches of physical science. In our own satellite, for example, we have the opportu- nity of studying the physical conformation and superficial phenomena of a body composed, as we believe mainly at least, of the same materials as those of our own globe, but possessing neither atmosphere nor sea. When we re- flect how much of the surface of the earth consists of sedimentary deposits, and consequently how large a portion of the whole field of geological research is occupied with strata which owe their principal characteristics to the ocean in which they were deposited, we cannot but anticipate many instructive lessons which may be furnished by the points of contrast, as well as of resem- blance, which the surface of the moon, viewed through Lord Rosse’s telescope, may present to the best judgement we are able to form of what the appearance of the earth would be if similarly viewed, or with what may be more difficult perhaps to imagine,-what we may suppose the earth would appear if it could be stript of its sedimentary strata, which conceal from us for the most — ADDRESS. xlv part the traces of that internal action which has played so large a part in moulding the great outlines of the present configuration of its surface. It is understood that Lord Rosse himself participates in the wish that such an examination of the surface of the moon should be made, and, should the desire of the Association be expressed to that effect, is willing to undertake it in conjunction with one or two other gentlemen possessing the necessary physical and geological knowledge. It will be for the Members of the As- sociation to determine the form in which a Report on the “ Physical Features of the Moon compared with those of the Earth” may most appropriately be requested. In connection with Astronomy, I permit myself to notice the publica- tion, now in progress, of two works of considerable magnitude and value, because they do honour to the science and public spirit of the part of the United Kingdom in which we are assembled; I refer to the Markree Catalogue of Ecliptic Stars, and to the results of the Observations at the Armagh Observatory. The establishments from which these publications emanate belong to the class which owe their endowment and support to private munificence, but by the extent and character of the work they per- form entitle themselves to rank with the Institutions, which in this and other countries testify the liberality of a nation’s patronage. The Markree Observatory, which has already distinguished itself under the personal - superintendence of its founder, amongst other services by the discovery of one of the thirteen planets by which our knowledge of the solar do- main has been enriched in the last seventeen years,—will hereafter take its position amongst the establishments which have most largely contributed to the perfection of modern astronomy by its catalogue of the approximate places of all the stars in the ecliptic down to the twelfth magnitude inclusive ; by which catalogue the detection of any still undiscovered planetary bodies belonging to our system will be greatly facilitated. One volume has already been published in the year which has elapsed since our Ipswich Meeting, and "a second is in preparation, and both, by the aid of funds supplied from the annual grant now placed at the disposal of the Royal Society, to be applied - in the advancement of science. The publication of the results of the ob- servations of the Armagh Observatory, since it has been under the very able direction of Dr. Robinson, has been for some time a desideratum. At the instance of the Royal Irish Academy it was recommended by the Irish Executive, but without success. It is now being accomplished by aid _ from the same source as the Markree Catalogue. I have the more satis- faction in noticing these appropriations in favour of Irish science from funds designed for the general benefit of the United Kingdom, because they indicate _ the fairness and equality with which the distribution of those funds is ad- ministered: it is also I believe strictly in character with the prevailing principles which sanction public aid, that it should be given, when needed, to 1852. d xlvi REPORT—1852. those who, as in the case of these private observatories, have already largely contributed from their own resources. The Mathematical and Physical Theories of Zight have afforded subjects for many interesting and profitable discussions in Section A, and have usually had one day in the six specially allotted to them. Those discussions will derive a more than usual interest at this meeting from the remarkable dis- covery recently made by Prof. Stokes, that under certain circumstances a change is effected in the refrangibility of light, and from the advantage we possess in having amongst us on this occasion the eminent mathematician and physicist by whom this most important contribution to the science of physical optics has been made. His researches took their origin from an unexplained phenomenon discovered by Sir John Herschel and communicated by him to the Royal Society in 1845. A solution of sulphate of quinine exa- mined by transmitted light, and held between the eye and the light, or between the eye and a white object, appears almost as transparent and colour- Jess as water; but when viewed in certain aspects and under certain incidences of light, exhibits an extremely vivid and beautiful celestial blue colour. This colour was shown by Sir John Herschel to result from the action of the strata which the light first penetrates on entering the liquid; and the dispersion of light producing it was named by him epipolic disper- sion, from the circumstance that it takes place near the surface by which the light enters. A beam of light having passed through the solution was to all appearance the same as before its entrance ; nevertheless it was found to have undergone some mysterious modification, for an epipolised beam of light, meaning thereby a beam which had once been transmitted through a quini- ferous solution, and had experienced its dispersive action, is incapable of fur- ther epipolic dispersion. In speculating upon the possible nature of epi- polised light, Prof. Stokes was led to conclude that it could only be light which had been deprived of certain invisible rays which in the process of dispersion had changed their refrangibility and had thereby become visible. The truth of this supposition, novel and surprising as it at first appeared, has been confirmed by a series of simple and perfectly decisive experiments ; showing that it is in fact the chemical rays of the spectrum more refrangible than the violet, and invisible in themselves, which produce the blue superficial light in the quiniferous solution. Professor Stokes has traced this principle through a great range of analogous phenomena, including those noticed by Sir David Brewster in his papers on “Internal Dispersion,” and has distin- _ guished between: “ cases of false internal dispersion” or “ opalescence,” in which the luminous rays are simply reflected from fine particles held in me- chanical solution in the medium, and those of “true internal dispersion,” or “fluorescence,” as it is termed by Mr. Stokes. By suitable methods of ob- servation the change of refrangibility was detected, as produced not only by transparent fluids and solids, but also by opake substances; and the class of ADDRESS. xlvii media exhibiting “fluorescence” was found to be very large, consisting chiefly of organic substances, but comprehending, though more rarely, some mineral bodies. The direct application of the fact, as we now understand it, to many highly interesting and important purposes, is obvious almost on the first an- nouncement. The facility with which the highly refrangible invisible rays of the spectrum may be rendered visible by being passed through a solution of sulphate of quinine or other sensitive medium, affords peculiar advantages for the study of those rays; the fixed lines of the invisible part of the solar spectrum may now be exhibited to our view at pleasure. The constancy with which a particular mode of changing the refrangibility of light attaches to a particular substance, exhibiting itself independently of the admixture of other substances, supplies a new method of analysis for organic compounds which may prove valuable in organic chemistry. These and other applica. tions of the facts as they are now explained to us, will probably form subjects of notice in the Chemical and Physical Sections, and a still higher interest may be expected from the discussion of the principle itself, and of the founda- tion on which it rests. A discovery of this nature cannot be otherwise than extremely fertile in consequences, whether of direct application, or by giving rise to suggestions branching out mure and more widely, and leading to trains of thought and experiment which may confer additional value on the original discovery, by rendering it but the first step in a still more extensive generalization. As the interest of this discovery is not confined to a single branch of science, the Officers, with the approbation of the Local Committee, have requested Mr. Stokes to favour the Association with an exposition of the subject at an evening meeting, when the members of the different sections may be able to attend without prejudice to their respective sectional duties : and in that view I have thought that this brief introductory notice might not be misplaced, a notice which I cannot conclude without adverting to the gratification which all who cultivate science in this part of the United _ Kingdom must feel at the rising eminence of their highly accomplished fellow-countryman. Among the subjects of chemical inquiry which may well deserve the attention of a combination of philosophers, perhaps few could more usefully occupy their joint labours than the revision of the Equivalent Numbers of the Elementary Bodies. This is a task which must necessarily require the co- operation of several properly qualified individuals, if it be accomplished within anything like a reasonable period of time. Most of the Numbers now in use depend upon experiments performed by Berzelius, at a time when the methods of research then known were inadequate, even in such hands, to determine these constants with an accuracy sufficient for the wants of science at the present day. So much has this been felt to be the case, that many of the most accomplished chemists now living have undertaken extensive and laborious, though isolated researches, upon the combining quantities of d2 xviii REPORT—1852. some of the most important elements. But much more than has been already performed still remains undone. Such a subject it is believed might be highly proper for consideration by the Chemical Section, to whose notice it would be introduced by the distinguished chemist, Dr. Andrews, who pre- sides over that Section, and than whom no one could be named as more competent to estimate the importance of such a revision, or to judge more truly of the qualifications that would be required for its execution. We are deprived by the illness, I trust only temporary, of our valued asso- ciate Prof. James Forbes, of the Report he would have given us of the progress of the experiments which he has undertaken at the request of the Association to test the Theory of Heat. But this branch of Physics abounds more perhaps than any other at the present time in subjects which may be most profitably discussed. The theory of Heat has made great advances within the last ten years. Mr. Joule has by his experiments confirmed and illustrated the views demonstrated about the end of the last century by Davy and Rum- ford regarding the nature of heat, which are now beginning to find general acceptance. He has determined with much accuracy, the numerical relation between quantities of heat and of mechanical work. He has pointed out the true principles upon which the mechanical value of any chemical change is to be estimated, and by very careful experiments he has arrived at numerical expressions for the mechanical equivalents in some of the most important cases of chemical action, in galvanic batteries, and in combustion. These researches appear to be laying the ground-work for the ultimate formation of a Mechanical Theory of Chemistry, by ascertaining experimentally the mechanical equivalents expressed in absolute motive force of the thermic, electric and magnetic forces. Mathematical developments of the theories of heat and electro-dynamics, in accordance with these principles, are given in various papers by MM. Helmholz, Rankine, Clausius and Thomson, published principally within the last two years. In discussing these subjects the Sec- tion will have a great advantage in being presided over by the last-named of these gentlemen, a native of Belfast, who at so early an age has attained so high a reputation, and who is taking a leading part in the investigations to which I have referred. In connexion with the subjects of Heat, I would advert to the experiments in which Mr. Hopkins is engaged for investigating the possible influence of high pressure on the temperature at which substances, in a state of fusion, solidify—an inquiry which was shown by Mr. Hopkins, in a report recently presented to the British Association, to have an important bearing on the questions of the original and present state of the interior of the earth. It is well known that the temperature of the earth increases as we descend, and it has been calculated that at the rate at which the increase takes place in such depths as are accessible to us, the heat at the depth of eighty or a hun- dred miles would be such as to fuse most of the materials which form the solid crust of the globe. On the hypothesis of original fluidity, and assuming ; ADDRESS. xls that the rate of increase known to us by observation continues further down, and is not counterbalanced by a considerable increase in the tempe- rature of fusion occasioned by pressure, the present state of the earth would be that of a solid crust of eighty or a hundred miles in thickness, enveloping a fluid nucleus. Mr. Hopkins considers this state to be inconsistent with the observed amount of the precession of the equinoxes, and infers that if the temperature of fusion be considerably heightened by pressure, the conclusion _ must be unavoidable that the earth is solid at the centre. Mr. Hopkins is assisted in these experiments, which are carried on at Manchester, by the well-known engineering knowledge of Mr. Fairbairn, and the equally well- known experimental skill of Mr. Joule. The principal difficulties attending the experiments with substances of low temperatures of fusion have been Overcome, and strong hopes are entertained of success with substances of more difficult fusibility. ‘The pressures employed are from three to four tons to eight and ten tons on the square inch. The latter is probably equal to the pressure at several miles beneath the earth’s surface. From Heat the transition is easy, and by many may be deemed natural, to Terrestrial Magnetism, a science which, more perhaps than any other, has profited by the impulse and systematic direction communicated to it by the British Association, and which perhaps more than any other required such external aid. In the infancy of a science, the phenomena of which present on our first acquaintance with them a great appearance of complexity, the path by which its progress may be advanced may be by no means easy to discern ; and individual explorers inay well, under such circumstances, be discouraged by doubts whether their labour will be recompensed by pro- portionate success, as well as disheartened by the little sympathy which is usually given to investigations which hold out but little immediate prospect ___ of practical utility. Some there have been however from time to time, who, & impressed with a persuasion of the position which magnetism deserves to _ take, and which sooner or later they believe it will take, amongst the phy- _ sical sciences of the highest order, have not spared this precursive labour, and have been uniformly conducted by it fo the same general conclusion, viz. that in order to obtain a sufficient foundation of facts upon which to ) raise a fitting superstructure of inductive reasoning, it would be necessary to q organize a system of cooperative research, in which the labours of many - might be united agreeably to concerted arrangements ; and that as such re- searches would require to be carried on nearly at the same epoch at many distant parts of the globe, for which private resources were inadequate, public assistance must be sought. That this conclusion was extensively recognised . and acquiesced in is sufficiently attested by the readiness so renerally mani- _ fested by governments and individuals in all countries where mental cultivation is regarded to take part in the general system of magnetic cooperation pro- posed by this country in 1838. Inthe years which have since elapsed, the energy and zeal of those who have engaged in these researches have accumu- dak or 1 REPORT—1852. lated a mass of observations, which, as the fruit of systematic and concerted labour, is, I believe, wholly unprecedented. The labour of digesting, com- paring, and coordinating the body of facts thus obtained may certainly be stated to be not less than that expended in obtaining them; and as the one process must necessarily be in great measure carried out subsequently to the other, we are only now beginning to reap the first-fruits of this great co- operative undertaking in the bearing of its results upon theory, At the Ipswich meeting of the British Association, I was requested by the General Committee to draw up a report on the state and progress of the magnetic researches consequent on the application of the British Association to Her Majesty’s Government in 1838. I regret that, from the other very pressing duties above alluded to, I have not been able to complete this report in time to present at this meeting, but as I may assume, from the request just made to me, that the subject retains with the British Association the interest which it there so happily acquired, I may venture to avail myself of this opportunity to make a very few remarks on some of its most important results; confining myself for the most part to results obtained by persons of our own country as the direct and immediate consequences of the recommendation of the British Association, leaving to a more fitting occasion a more general and comprehensive view. We recognise in terrestrial magnetism the existence of a power present everywhere at the surface of our globe, and producing everywhere effects indicative of a systematic action ; but of the nature of this power, the cha- racter of its laws, and its economy in creation, we have as yet scarcely any knowledge. The apparent complexity of the phenomena at their first aspect may reasonably be ascribed to our ignorance of their laws, which we shall doubtless find, as we advance in knowledge, to possess the same remarkable character of simplicity which calls forth our admiration in the laws of mole- cular attraction. It has been frequently surmised, and the anticipation is I believe a strictly philosophical one, that a power which, so far as we have the means of judging, prevails everywhere in our own planet, may also prevail in other bodies of our system, and might. become sensible to us, in the case of the sun and moon particularly, by small perturbing influences mea- surable by our instruments, and indicating their respective sources by their periods and their epochs, As yet we know of neither argument nor fact to invalidate this anticipation; but, on the contrary, much to invest it with a high degree of probability. Be this however as it may, we have in our own planet an exemplification of the phenomena which magnetism pre- sents in one of the bodies of our system, on a scale of sufficient mag- nitude, and otherwise convenient for our study. Accordingly the first object to which the British Association gave its attention was to ob- tain a correct knowledge of the direction and amount of the magnetic force generally over the whole surface of the globe corresponding to a definite epoch. It has been customary to represent the results of magnetic ADDRESS, hi observations by three systems of Lines, usually called isogonic, isoclinal, and isodynamic lines. [Lines of equal horizontal direction, of equal inclination, and of equal force.] | In the maps of these lines existing in 1838, large spaces of the earth’s surface were either blank, or the lines passing across them were very imperfectly supported by observations. In the more frequented parts, where observations were more numerous, the dis- crepancies of their dates impaired their suitability for combination; for the position and configuration of the magnetic lines has been found to undergo a continual process of systematic change, with the causes of which we are as yet wholly unacquainted, but which has obtained the name of secular change to distinguish it from periodical variations of known and limited duration. Amongst the most marked deficiencies in these maps, were the greater part of the extra-tropical portion of the southern hemisphere,—the British pos- sessions in North America, and British India;—magnetic surveys of these were expressly recommended, and the practicability and advantage of making the observations on board-ship, and of thus extending them over the surface of the ocean, were pointed out. It is most pleasing to recall to recol- lection, and gratifying to acknowledge from this chair, the favourable manner in which the recommendations of the British Association were received by Her Majesty’s Government and by the East India Company, and how promptly and effectually they have been carried out. The blanks in the southern hemisphere have been filled up by maritime expeditions appointed expressly for the purpose. Magnetic surveys have been completed of British North America at the expense of our own Government, and of the Indian Archipelago at that of the East India Company, and India ‘itself is now in progress; whilst from the zeal of our naval officers contributions have flowed in from almost every accessible part of the ocean. The coordi- nation and mutual connection of so large a mass of materials is necessarily a work of time, but is progressing steadily towards completion, and when pre- sented in one connected view, will form the groundwork on which will securely rest a general theory of terrestrial magnetism corresponding to the present epoch. Until these combinations and calculations are performed, it would be obviously premature to speak of numerical values by which the magnetic forces at’ one part of the globe may be compared with those of another, or with forces of other descriptions; and for the same reason it is desirable to abstain for the present from notices of the geographical positions which particular lines, or as some may deem them, critical points in the magnetic resultants may occupy on the earth’s surface at the present epoch. Such notices could only be as yet provisional and liable to the amendments which more exact and extended calculation must be expected to produce. But thus much may be safely stated in reference to the general character of the three systems of lines which have been spoken of, that when derived afresh and exclusively from the observations of the last few years, they do most fully confirm the general conclusions derived from the observations of earlier lii REPORT—1852. date, which were submitted to the British Association in the Report on the * Variations of the Intensity of the Magnetic Force at different points of the Earth’s surface,” which preceded the recommendations of 1838. The mnagnetic phenomena, or as it is now customary to call them, the three mag- netic elements, appear to be everywhere and in both hemispheres the resultants of a duplicate system: of magnetic forces, of which one at least undergoes a continuous and progressive translation in geographical space, the motion being from west to east in the northern hemisphere, and from east to west in the southern. It is to this motion that the secular change in all localities is chiefly if not entirely due, affecting systematically and ac- cording to their relative positions on the globe, the configurations and geo- graphical positions of the magnetic lines, and producing conformable changes in the direction and amount of the magnetic elements in every part of the globe. The comparison of the earlier recorded observations with those of the present epoch gives reason to believe, that viewed in its generality, the motion of the system of forces which produces the secular change has been uniform, or nearly so, in the last two or three centuries. Under favourable conditions the regularity of this movement can be traced down to comparatively very minute fractions of time; by the results of careful observations continued for several years at the observatory of St. Helena, where, in common with the greater part of the district of the South Atlantic, the secular change of the declination exceeds eight minutes in the year, and from its magnitude therefore may be advantageously studied,— every fortnight of the year is found to have its precise aliquot portion of the annual amount of the secular change at the station. This phenomenon of secular change is undoubtedly one of the most remarkable features of the magnetic system, and cannot with propriety be overlooked, as too frequently it has been, by those who would connect the phenomena of terrestrial magnetism generally, mediately or immediately, with climatic circumstances, relations of land and sea, or other causes to which we are assuredly in no degree entitled to ascribe secular variation, and who reason therefore as if the great magnetic phenomena of the earth were persistent instead of being as they are subject to a continual and progressive change. It may confidently be affirmed that the secular magnetic variation has no analogy with, or resemblance to, any other physical phenomenon with which we are acquainted. We appear at present to be without any clue to guide us to its physical causes, but the way is preparing for a future secure derivation of its laws to be obtained by a repetition, after a sufficient interval, of the steps which we are now taking to determine the elements corresponding to a definite epoch. The periodical variations in the terrestrial magnetic force, which I have before adverted to as distinguished from its secular change, are small in com- parison with the force itself, but they are highly deserving of attention on account of the probability that by suitable methods of investigation they may be made to reveal the sources to which they owe their origin and the 4 q a 7 ' a a =| ADDRESS. lait agency by which they are produced. They formed accordingly the subject of a distinct recommendation from the British Association, which met with an equally favourable reception. To investigate these variations by suitable instruments and methods, to separate each from the others, and to seek its period, its epochs of maximum and minimum, the laws of its progression, and its mean numerical value or amount, constituted the chief purposes for which magnetic observatories were established for limited periods at certain stations in Her Majesty’s dominions, selected in the view that by a combination of the results obtained at them, a general theory of each at least of the principal periodical variations might be derived, and tests be thus supplied whereby the truth of physical theories propounded for their explanation might be examined. We are just beginning to profit by the collocation and study of the great body of facts which have been collected. Variations corresponding in period to the earth’s revolution around the sun, and to its rotation around its own axis, have been ascertained to exist, and their numerical values ap- proximately determined in each of the three elements, the Declination, In- clination, and Magnetic Force. We unhesitatingly refer these variations to the sun as their primary source, since we find that in whatever part of the globe the phenomena are observed, the solstices and equinoxes are the cri- tical epochs of the variation whose period is a year, whilst the diurnal varia- tion follows in all meridians nearly the same law of local solar hours. To these unquestionable evidences of solar influence in the magnetic affections of the earth, we have now to add the recently ascertained fact, that the mag- netic storms, or disturbances, which in the absence of more correct know- ledge were supposed to be wholly irregular in their occurrence, are strictly periodical phenomena, conforming with systematic regularity to laws in which the influence of local solar hours is distinctly traced. But, whilst we recognise the sun as the primary cause of variations whose _ periods attest the source from whence they derive their origin, the mode or _ modes in which thé effects are produced constitute a question which has been _ and may still be open to a variety of opinions: the direct action of the sun as being itself a magnet, its calorific agency occasioning thermo-electric _ and galvanic currents, or in alternately exalting and depressing the magnetic _ condition of substances near the surface of the earth, or in one of the consti- _ tuents of its atmosphere,—have been severally adduced as hypotheses afford- ing plausible explanations. Of each and all such hypotheses the facts are the _ only true criterion ; but it is right that we should bear in mind that in the pre- sent state of our knowledge, the evidence which may give a decided counte- nance to one hypothesis in preference to others does not preclude their possible coexistence. The analysis of the collected materials and the disentanglement of the various effects which are comprehended in them, are far from being yet complete. The correspondence of the critical epochs of the annual variation with the solstices and equinoxes rather than with the epochs of maximum | and minimum temperature, which at the surface of the earth, in the subsoil liv REPORT—1852. beneath the surface, or in the atmosphere above the surface, are separated by a wide interval from the solstitial epochs, appears to favour the hypothesis of a direct action; as does also the remarkable fact which has been established, that the magnetic force is greater in both the northern and southern hemi- spheres in the months of December, January, and February, when the sun is nearest to the earth, than in those of May, June, and July, when he is most distant from it: whereas if the effects were due to temperature, the two hemispheres should be oppositely instead of similarly affected in each of the two periods referred to. Still there are doubtless minor periodical irregular variations yet to be made out by suitable analytical processes, which, by their possible accordance with the epochs of maximum and minimum temperature, may support in a more limited sense, not as a sole but as a coordinate cause, the hypothesis of calorific agency so generally received, and so ably advocated of late in connection with the discovery by our great chemist and philosopher of the magnetic properties of oxygen and of the manner in which they are modified and affected by differences of temperature. It may indeed be difficult to suppose that the magnetic phenomena which we measure at the surface of the globe, should not be in any degree influ- enced by the variations in the magnetic conditions of the oxygen of the atmosphere in different seasons and at different hours of the day and night ; but whether that influence be sensible or not, whether it be appreciable by our instruments or inappreciable by them, is a question which yet remains for solution by the more minute sifting of the accumulated facts which are now undergoing examination in so many quarters. To justify the anticipation that conclusions of the most striking character, and wholly unforeseen, may yet be derivable from the materials in our possession, we need only to recall the experience of the last few months, which have brought to our knowledge the existence of what may possibly prove the most instructive, as it is certainly at first sight the least explicable, of all the periodical magnetic variations with which we’ have become ac- quainted. I refer to the concurrent testimony which observations at parts of the globe the most distant from each other bear to the existence of a periodical variation or inequality, affecting alike the magnitude of the diurnal variations, and the magnitude and frequency of the disturbances or storms. The cycle or period of this inequality appears to extend to about ten of our years; the maximum and minimum of the magnitudes affected by it being separated by an interval of about five years, and the differences being much too great, and resting on an induction far too extensive, to admit of uncer- — tainty as to the facts themselves. The existence of a well-marked magnetic period which has certainly no counterpart in thermic conditions, appears to render still more doubtful the supposed connexion between the magnetic and calorific influences of the sun. It is not a little remarkable that this periodical magnetic variation is found to be identical in period and in epochs of maxima and minima with the periodical variation in the frequency and magnitude of ADDRESS. ly unremitting labour. From a cosmical connexion of this nature, supposing it to be finally established, it would follow, that the decennial period which we measure by our magnetic instruments is, in fact, a solar period, mani- fested to us also by the alternately increasing and decreasing frequency and magnitude of obscurations on the surface of the solar disc. May we not haye in these phenomena the indication of a cycle or period of secular change in the magnetism of the sun, affecting visibly his gaseous atmosphere or photosphere, and sensibly modifying the magnetic influence which he excicises on the surface of our earth? The determination of the figure and dimensions of the globe which we - inhabit may justly be regarded as possessing a very high degree of scientific interest and value, and the measurements necessary for a correct knowledge thereof, have long been looked upon as proper subjects for public underta- kings and as highly honourable to the nations which have taken part in them. Inquiries in which I was formerly engaged led me fully to concur with a remark of Laplace, to the effect that it is extremely probable that the first attempts were made at a period much anterior to those of which history has preserved the record; the relation which many measures of the most remote antiquity have to each other and to the terrestrial circumference strengthens this conjecture, and seems to indicate, not only that the earth’s cireumference was known with a great degree of accuracy at an extremely ancient period, but — that it has served as the base of a complete system of measures the vestiges of which have been found in Egypt and Asia, In modern times the merit of re- suming these investigations belongs to the French nation, by whom the are of the meridian between Formentera and Dunkirk was measured towards the close of thelast century. The Trigonometrical Survey of Great Britain, commenced in 1783, for the specific object of connecting the Observatories of Greenwich and Paris, was speedily expanded by the able men to whom its direction was then confided into an undertaking of far greater scientific as well as topo- graphical importance, having for its objects on the one hand the formation of correct maps of Great Britain, and on the other the measurement of an are of the meridian, having the extreme northern and southern points of the Island for its terminations. A portion of this are, amounting to 2° 50’, viz. _ from Dunnose in the Isle of Wight to Clifton in Yorkshire, was published in _ the Phil. Trans. in 1803. As the whole arc, extending from Dunnose to Unst and Balta, the most northern of the Shetland Islands, would comprise - more than 10°, and as nearly half a century had elapsed since the publication | the solar spots which M. Schwabe has established by twenty-six years of use, and by those who were interested for the scientific character of the nation, that the general results of the Survey applicable to scientific purposes should at length be given to the world. Accordingly, at the Birmingham Meeting lvi REPORT—1852. deputation to confer with the Master-General of the Ordnance, and a similar resolution was passed about the saime time by the President and Council of the Royal Society. On communicating with the Master-General, it appeared that the want of special funds for the requisite calculations formed the only obstacle, a difficulty which was happily immediately surmounted by an appli- cation of the President and Council ef the Royal Society to Lord John Russell, then First Lord of the Treasury. The Report of the Council of the British Association to the General Committee at the Meeting of the last year at Ipswich, contained an official statement from the Inspector-General of Forti- fications of the progress of the reduction and examination of the observations preparatory to the desired publication, and concluded with expressing the expectation of the Director of the Survey, that he “should be able to furnish for communication to the British Association that would probably assemble in 1852, the principal results obtainable from the geodetic. operations in Great Britain and Ireland.” By a recent letter to my predecessor from Captain Yolland of the Royal Engineers, who is entrusted with the direction of the publication, I am enabled to have the pleasure of announcing that the “ printing of the observations made with the Zenith Sector, for the determi- nation of the latitudes of stations between the years 1842 and 1850, is finished, and will be presented in time for the meeting of the British Asso- ciation, and that the calculations connected with the triangulation are rapidly advancing towards their completion.” In the meantime the great are of Eastern Europe has been advancing with unexampled rapidity and to an extent hitherto unparalleled. Originating in topographical surveys in Esthonia and Livonia, and commenced in 1816, the operations, both geodesical and astronomical, have been completed be- tween Izmail on the Danube and Fugleness in Finnmarken, an extent of 252 meridional degrees. Next to this in extent is the Indian are of 21° 21! be- tween Cape Comorin and Kaliana; and the third is the French are already referred to of 12°22’. It appears by a note presented to the Imperial Academy of Sciences at St. Petersburgh by M. Struve, that a provisional calculation has been made of a large part of the great are of Eastern Europe, and that it has been found to indicate for the figure of the earth a greater compression than that derived by Bessel in 1837 and 1841, from all the ares then at his command,—Bessel’s compression having also been greater than La- place’s previous deduction. It is naturally with great pleasure that I perceive that the figure of the earth derived by means of the measurement of ares of the meridian approximates more and more nearly, as the ares are extended in dimension, to the compression which I published in 1825 as the result of a series of Pendulum Experiments, which, by the means placed by Govern- ment at my disposal, I was enabled to make from the equator to within ten degrees of the pole, thus giving to that method its greatest practicable ex- tension. The observations hitherto made on the ¢ides of the ocean have been insuf- 4 ADDRESS. lvil ficient to furnish such a connected knowledge of the subject as would enable us to follow the course of the tide over any considerable portion of the ocean, and in the opinion of persons most competent to judge, it is only by systematic observations specially directed for the purpose, that this connected knowledge is likely to be obtained. Accordingly a resolution was passed at the Ipswich Meeting of the Association, appointing a Committee to prepare a Memorial to Her Majesty’s Government, representing the importance of determining the progress of the tide-wave along the coasts of Africa and South America by an Atlantic Tidal Expedition. This Memorial was presented to Govern- ment by my predecessor, and, having been referred to the Hydrographer, has been most favourably reported upon. We may therefore expect that the survey will be very shortly commenced. The recent researches of Captain _ Beechey, which have given a new and unexpected view of the tidal movements of the ocean, show how much yet remains to be learnt respecting the tides even for the practical purposes of navigation. _ The facts derived a few years since from the barometrical observations at St. Helena, showing the existence of a lunar atmospheric tide, have been corroborated in the last year by a similar conclusion, drawn by Captain Elliot of the Madras Engineers from the barometrical observations at Singapore. The influence of the moon's attraction on the atmosphere produces, as might be expected, a somewhat greater effect on the barometer at Singapore, in lat. 1° 19’, than at St. Helena, in lat. 15° 57'. The barometer at the equator appears to stand on the average about 0006 in. (more precisely 0°0057, in lat. 1° 19') higher at the moon’s culminations than when she is six hours distant from the meridian. We have received from our valued corresponding member Prof. Dove, for presentation to this Meeting, an important continuation of his researches on the temperatures at the surface of the globe. In former communications he has furnished us with maps showing, so far as observation permits, the : isothermals of the whole globe in every month of the year. He has now _ given us, first; the normal temperatures of each parallel of latitude in each P month; being the average of all the temperatures in that parallel in such - month; and second, the abrormal temperatures, or the difference between the 1 temperature of each place and the mean temperature of its parallel. From - these again are formed lines of abnormal temperature for each month, sur- _ rounding and marking out those districts or localities, which, from peculiarities _ of the surface or other causes affecting the distribution of heat, are charac- "terized by excessive abnormal heat or abnormal cold. The importance of _ these researches on the general theory of the causes which interfere with the equable distribution of heat according to latitude is obvious. _ The activity which has prevailed so greatly of late, in the collection of meteorological data, has been almost exclusively confined to that portion of the surface of the globe which is occupied by land, although the portion lviii REPORT—1852. covered by the ocean is not only much greater in extent, but is also better suited for the solution of several meteorological problems. Many striking examples might be adduced to show that it is “systematic direction,” and not “individual zeal” in naval men, which has been wanting, and it has been therefore with great satisfaction that meteorologists have learnt that a pro- position has recently been made from the United States Government to the British Government, to undertake, conjointly and in cooperation, a system of meteorological observations, to be made -at sea in all ships belonging to the naval service of the two countries, and sufficiently simple to be parti- cipated in by the merchant service also. In a partial trial which has been already made of this system in the United States, it has been found to produce results which, exclusive of their scientific bearing, are of great importance to the interests of navigation and commerce, in materially shortening passages by the knowledge of prevailing winds and currents at particular seasons. The practical advantages arising from the coordination of the observa- tions in the Hydrographic Office of the United States, and of the circu- lation of the charts of the winds and currents, and of the sailing direc- tions founded on them, have been such and so appreciated, that there are now, as it is stated, more than 1000 masters of American ships en- gaged in making them. The request for British cooperation in an uh- dertaking so honourable to the country in which it originated, was referred in the spring of this year by the Earl of Malmesbury to the President and Council of the Royal Society for a Report; from which I permit myself to quote the concluding sentence, in the persuasion that it would find an echo, if necessary, in every part of the United Kingdom, and that it cannot fail to be promptly acted upon by the Government of a country in which maritime interests hold so prominent a place :—“To the Government of this country the demand for cooperation and for the interchange of obser- vations is most earnestly addressed by the Government of the United States; and the President and Council of the Royal Society express their hope that it will not be addressed in vain. We possess in our ships of war, in our packet service, and in our vast commercial navy, better means for making such observations, and a greater interest in the results to which they lead, than any other nation; for this purpose every ship which is under the control of the Admiralty, should be furnished with instruments properly con- structed and compared, and with instructions for using them; similar in- structions for making and recording observations, as far as their means will allow, should be given to every ship that sails, with a request that they will transmit the results to the Hydrographer’s Office of the Admiralty, where an adequate staff of Officers or others should be provided for their prompt examination, and the publication of the improved charts and sailing directions to which they would lead; above all, it seems desirable to establish a prompt communication with the Hydrographer’s Office of the United States, ADDRESS. lix so that the united labours of the two greatest naval and commercial nations of the world may be combined, with the least practicable delay, in promoting the interests of navigation.” Amongst the most valuable results which the Physical Sciences may expect to obtain from this extensive system of nautical observation, we may reckon the construction of charts of the isothermals of the surface of the ocean cor- responding to every month in the year, similar to Dove’s monthly isothermals of the temperature of the air; and a knowledge of the normal condition as well as the abnormal variations, with their special causes and effects, of the great Gulf-stream which connects the shores of the Old and New World, and in its normal effects is influential in many ways on the climate of the United States and Western Europe, whilst its abnormal effects are principally known, so far as we are yet aware, by the peculiarities of climate they oceasionally produce on the European side of the Atlantic. Of the extent, depth, and limits of this remarkable current in ordinary and extraordinary years we are as yet very imperfectly informed. Of the zoology of the great tracts of ocean which are covered by its banks of: seaweed, we know nothing beyond the fact that they are the habitation of a countless number of oceanic animals,— giving rise possibly to deposits which may have distinctive characters from littoral deposits or from those of marine estuaries. But doubtless, we can now estimate only a very small part of the advantages which Terrestrial Physics as well as Hydrography and Navigation would derive from the concurrent exertions of the two great maritime nations in the way that has been pointed out. The analogy of the configuration of the land and sea on the north of the continents of Asia and America, has for some time past caused an opinion to be entertained that the sea on the north of the Parry Islands might be as open as it is known to be throughout the year in the same latitude on the north of the Siberian Islands. The expectation that Wellington Strait might, as the continuation of Barrow’s Strait, prove a channel of communication from the Atlantic into that part of the Polar Ocean, has been considerably strengthened in the last year by the discoveries which we owe to the hardi- _ hood and intrepidity of our merchant seamen. The access to the Polar covery or of scientific research, are amongst the few geographical problems of high interest which remain to be solved; and we may confidently look for a solution, in the direction at least that has been adverted to, by the | up the discovered traces of Sir John Franklin’s vessels. The success which the Kew Observatory Committee have had in their un- _ dertaking to make Standard Thermometers, encourages us to hope that they _ will be equally successful in the endeavour in which they are now engaged _ to introduce a greater degree of precision in the construction of meteorological instruments generally, as well as in the more delicate kinds which are so fre- lx REPORT—1852. quently required in physical experiments. An establishment has long been a desideratum in which instruments for various physical researches employed in foreign countries should be tried in comparison with the instruments used here, and the relative merits of each examined, and in which new and pro- mising inventions and suggestions should receive a practical trial. Amongst its other services rendered to Science and to the country, the British Associa- tion is now entitled to claim the merit of having organized an establishment which appears extremely well-suited to supply this deficiency, and needs only more extensive means to supply it to any required extent. The applications which have been made to Kew in the past year by Profs. Forbes and Thomson for thermometers of particular kinds, required in very delicate experiments in which those gentlemen are engaged, and by the Admiralty for Standard Ther- mometers for very low temperatures to be employed by the Arctic Expeditions, show that the advantages to be derived from such an establishment are already beginning to be recognised ; and as these become more known and felt, it may confidently be anticipated that means will not be wanting for such an exten- sion of the establishment at Kew, as may be necessary to meet fully the public requirements. The desire which isso frequently manifested- by voyagers and travellers in distant countries to contribute to our knowledge of terrestrial physics, would be greatly aided by increased facilities afforded to them of obtaining suitable and well-assured instruments, and still more if practical instruction or advice could be added. It is not from deficiency of interest, or of a desire to be useful in such inquiries, that our British travellers do not reap the full advantages of the great opportunities which they possess, so much as from the absence of any provision for supplying instruments on which reliance can be placed with practical instructions for their use. In no department is the “systematic direction,” which it is the object of the British Association to communicate to the sciences generally, more needed than in Physical Geography. To carry this desirable purpose into effect, might with great propriety and public benefit be made to form a branch of the duties of the Kew Observatory. In compliance with a resolution of the Council, the Kew Committee have made arrangements for four aéronautic ascents in the Nassau Balloon, chiefly for the purpose of investigating the laws of the decrement of temperature and of aqueous vapour in ascending into the atmosphere. The two first of these ascents took place on the 17th and 26th of August, attaining in each case between 19,000 and 20,000 feet, and will be the subject of a commu- nication to the Association, which will doubtless excite much interest, from Mr. Welsh of the Kew Observatory, who was charged by the Superintend- ing Committee with the conduct of the observations. The opportunity which the Observatory furnishes to the Association, of a convenient locality, presenting many facilities for carrying on a series: of delicate experiments, has been taken advantage of by Professor Stokes for experiments in which he is engaged on the Index of Friction in different ADDRESS. lxi Gases. Experiments reported by myself to the Royal Society in 1829, showed that the retardation of a pendulum vibrating in different gases was not proportionate to their respective densities, but appeared to depend also on some inherent quality, whereby the different gases present different degrees of resistance to the motion of bodies passing through them. I was interrupted in the prosecution of this subject by a recall to military duty, and I now rejoice to see it in hands so far more able to do it justice. The Parliamentary Committee appointed at the Ipswich meeting to watch over the interests of Science, consisting of Members of the British Asso- ciation who are also Members of the Legislature, have this morning made their first Report to the General Committee, and some notice of the subjects which have chiefly occupied them in the past year may not be unacceptable to the Members of the Association at large. One of these subjects is that of Scientific Pensions. It is known to all that since the commencement of the reign of Her present Majesty pensions to the amount of £1200 have been at the disposal of the First Minister of the Crown, to be granted each year in recompense of civil services, chiefly, though not exclusively, in literature and science, and that several persons of various degrees of literary and scientific eminence have received pensions accordingly, many of which have given much public satisfaction. On examining the appropriations which have been made in the fourteen years since this fund became available, it appeared that only about thirteen per cent., or an eighth part of the whole amount, had been allotted to scientific pensions. Considering this to be a proper subject to be brought under the notice of Government, Lord Wrottesley, the Chair- man, and Sir R. H. Inglis, one of the Members of the Committee, obtained an interview with the Earl of Derby for that purpose. The readiness of Government to attend to such representations has been fully shown in the scientific pensions granted in the present year, amounting to nearly a third _ of the whole sum available for the year. These pensions have been granted, on the recommendation of the President of the Royal Society,—to Mr. Hind, who has the unique distinction of being the discoverer of no less than six out of the twenty-five known planets of the solar system,—to Dr. _ Mantel, so well known for his successful researches in palaontology,—and to Mr. Ronalds, for the electrical and kindred researches in which he has been engaged for so many years. The intimate association of the scientific _ services of Mr. Ronalds for several years past with the Observatory of the _- British Association at Kew, must render this last selection peculiarly gra- ‘ tifying to our Members. } Another subject which has occupied the attention of the Parliamentary _ Committee in the last year, is one to which their attention was requested by _ the Council of the Association, with a view of carrying into effect the desire _ of the General Committee for a more cheap and rapid international commu- _ nication of scientific publications. The credit of the first move towards the accomplishment of this desirable object is due to the Government of the 1852. e Ixii REPORT—1852. United States, by whom an arrangement was made for the admission duty free of all scientific books addressed as presents from foreign countries to all institutions and individuals cultivating science in that country, such books being sent through the Smithsonian Institution, by whom their further dis- tribution to their respective destinations was undertaken. This arrangement was notified to our Government through the British Minister at Washington, and a similar privilege was at the same time requested for the admission duty free into England of books sent as presents from the United States to public institutions and individuals cultivating science in this country, under such regulations as might appear most fitting. This proposition gave rise to communications between the President of the Royal Society and the Chair- man of the Parliamentary Committee on the one part, and the Treasury and the principal Commissioner of Customs on the other; the result of which has been the concession of the privilege of admission, duty free, into England of scientific books from all countries, designed as presents to institutions and individuals named in lists to be prepared from time to time by the Royal So- ciety, after communication with other scientific societies recognized by charter, under the regulation, however, that the books are to be imported in cases addressed to and passing through the Royal Society. This arrangement has come into operation; and it may be interesting to notice, as giving some idea of its extensive bearing, that the first arrival from the United States which has taken place under these regulations consists of packages weighing in all no less than three tons. There is another branch of the same subject which is more difficult to arrange, viz. the international com- munication by post of scientific pamphlets and papers at reduced rates of postage; the Parliamentary Committee have directed their attention to this part of the subject also, and I earnestly hope that their exertions will be successful. Allusions have been made by influential men, and in influential places, to a direct representation of Science in Parliament; and we frequently hear opinions expressed that Parliament might be improved by a greater admix- ture of men who might be chosen as the representatives of the intellectual cultivation of the nation, amongst those who represent its material interests. The benefit which the Legislature might derive from a change of this descrip- tion, is a question rather for statesmen than for men of science, and would be quite unsuitable for discussion here: but in respect to the influence which such change would exercise on Science itself and on its cultivators, it does belong to us to consider both its probable advantages and disadvantages. I have no hesitation in expressing as an individual opinion, my belief that the possible gain would be incaleulably outweighed by the too certain evils; and that scientific men cannot too highly value and desire to retain the advantage they now possess in the undisturbed enjoyment of their own pursuits un- troubled by the excitements and distractions of political life. Some there are amongst us, and some there ever have been, who, born to a station which ADDRESS. lxili brings with it public duties, but gifted with a strong natural taste for the pursuits of science, do manage to succeed in a greater or less degree in com- bining both. Success is in such cases the more honourable, and is the more admired, because it manifests the strength of the original disposition, and in- dicates how much more might probably have been accomplished by an undivided attention. The economy of human labour points specially to such ‘men as the most suitable representatives of science in the legislature of which _ they already form a part. The selection from amongst them of a certain number to be particularly charged with the duties of watching over and pro- moting the interests of science, either with Government or in the Legislature appears in this view a most happy expedient. We cannot read over the _ names of the noblemen and gentlemen who form the Parliamentary Committee _ of the British Association, without being satisfied that science would not be likely to be more honourably or more ably represented by any system of direct representation ; nor can we look to the discretion and practical wisdom with which the proceedings of the Committee have been conducted in the first year of its existence, without being impressed with the belief that it is destined to render important services both to the country and to ourselves. Gentlemen, I have now occupied fully as much of your time and attention as I can venture to trespass upon, and yet have found it impossible to com- prehend within the limits of a discourse all the topics to which I would gladly have called your notice, even in those branches of knowledge in which I may consider myself least uninformed, in three of the seven departments into which our science is divided. I have left wholly untouched those wide fields of Geology and Natural History, which would of themselves have furnished fitting subjects for an address of still longer duration. No one can be more sensible of this, and of many other imperfections and deficiencies, _ than the individual who addresses you; yet, if he has not wholly failed in _ the purpose he designed—if the impression which he has endeavoured to _ convey, however faint may be the image, be true to that which it is intended _ to represent,—you have not failed to recognise the gratifying picture of _ British Science in the full career of energetic action and advancement, press- _ ing forward in every direction to fill the full measure of the sphere of its activity in the domain of intellectual culture ; regardful on the one hand of the minutest details in the patient examination of natural faets, and on the other hand diligent in combining them into generalizations of the highest order, by the aid of those principles of inductive philosophy, which are the | surest guide of the human intellect to the comprehension of the laws and order of the material universe. a aay ea Oras? peer ne Porras? Sa Ne tt at Pia oe es : - 4 Y REPORTS. * THE STATE OF SCIENCE Third Report on the Facts of Earthquake Phenomena. By Bowens MALLET, Cult M.R.LA. ERRATA IN MR. MALLET’S SECOND REPORT ON EARTHQUAKES. Since the printing of the preceding Report the following errata have been discovered :— In page 288, line 5 from bottom, for 0'-014206 read 0'-014286. -— 289, line 14, for 0'013910 read 0'-013903. —— — line 30, for 0'"41743 read 0'"41726. —— — lune 31, for 0"-013914 read 0"-013909. [The preceding corrections apply also to the table of chronograph ratings at foot of p. 289. ] In page 290, line 2, for 0013914 read 0'013909. — —- — for 0""006956 read 0"-006954. —— 293, line 1, for ratio read rate. —— 298, line 33, for 307-05 read 307°50. ——— 299, line 12, for 9:607 read 9°609. —— 306, line 13, supply a comma after the word “ dial”’. —— 306, line 4 from bottom, supply a comma after “ dial ”’. These errors are all small, and affect the results within limits much less than those of the differences between one experiment and another. A single arithmetical mistake remains however to be noticed, which alters consider- ably the constant of wave transit im sand as deduced from the experiments ; namely, that in page 292, line 3 from bottom, *8 was read instead of *3, at the beginning of the number representing the average of col. 4. The result of the subtraction should therefore be 3!'"411639 instead of 2!911639, and hence the gross rate of transit in sand =774°568 feet per second. Using this corrected number in the calculation (p. 307) of the distance lost in raising the wave in the seismoscope, and applying throughout the small corrections mentioned above, the true rates of transit are— LETS} 07 RES A Apapeemee nocpoooececsocopocoanscen 824915 feet per second. In discontinuous Granite .......seeceeee 1306°425 be In more solid Granite .......c.seeseeeee 1664°574 - which numbers should therefore be substituted for those given in pp. 307, 308. This correction still further removes any probability of aérial commotion having at all interfered in the Killiney experiments: see pp. 303-305. The Catalogue of Earthquakes contained in Mr. Mallet’s Report will be continued in the next volume. 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"192 “d ‘sgouaidg So] Ins “Mey ‘nosseyeg ‘Thr ‘d ‘cZ8l & GIST ep eudepreg ua asviO A ‘VIOUIIL I Op }19q | Y *AVYD 9] *peoy “1199 §xtuomyD sJ9[segq *peoy “1199 ‘dezyoneyog § puryssg "GOs “d ‘ayeyos ayostueder ‘snurzu0yy “LL ‘d ‘orzuaat, ‘oct “dm 4 ‘grmkg ua a8vAOA ‘aTTeA BI[EP O1}01g ~jpuesoy “LOT pue “114 0} apem s]jeq ey} pus ‘uayeYys o10M sojdaajg “OT9T 94 PMoys yuo styy Jo ayep 9y3 ‘TLL T “dag YICT aq} Jo onbrpadojodoug jeumor at} 0} durptoooy “41 pauInd pue sshoy v uodn Tl9} YOOr Jo ssvur yeois e oyenbyyava sig} Surg Ree tome e ener eee ee te ee reese seers sees ee tesssesssseseneese® Pee OO eter tee meee tH Hest ees arasaesesenssssessseesssreeestens ‘291} @ JO SOAVIT 9Y} OHI] WayeYS OOM ST[eA OIL, Seen teen ee nee enenpeseneres Cee rereoeseserseoesereoeees See were weer see toaneeneseene eee eeeeeersserenereseaaees “SIRS asey}. 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‘eutXuIg pue esnd ee ‘Quoweyar e19A pur {7Zz9T ‘ode jsjol pue ‘uMoIYZATAAO sysa0F “4JoTO suTeJUNOUT |-a1 UT} pue ‘4ysvod japIs UIo}sva dy} WOA|-eY se Iey se papuay “a2 {0}0UI9I10} ULAS [ap OsioosIp |‘dn polp o19M sayy] ‘punoid oy} ur pouedo jay} mo sj omy |'*g pue*N SuruunroUT|-xe ospy ‘soydeNy jo oot10ysy ‘eSog ‘uoyUy StAX, “d= |sqyorQ “SAAT, s10y} ysoy suosted QOO‘Z[ PUe juey, s1oM pomor je ur Ae] paanfur ysour|Aj10 oYy UT pue ‘esng Tt +4 ‘adoay op “yoIq ‘sto[suey |‘oyxenbyyzea siqy Aq ssay JO aLoW pou ueeq jeas ay} OIpuBdIN |sooejd oy, ‘snoyjeyT pues eyeurziden “u00N {-jouoIy) 9p “Way S*peoy ‘[OO|surAey se pauoUUL ore sose][IA pUL SUMO} AVI JUG PUL d10JOT FY|PAY poyse] syooys op joy} Jo seoutaoad ay} uy|"og Ajae —— ‘uordnsza Ur sem sojst Wediy oy} Ul oURBO[N A *skep A4.10F ‘Wave oy} ut pousdo syaro Aur ‘paumaz Joqjesoye Surysey *SUOTIOT) VINO, {TT ‘d ‘OIZUaATAlaIOM OLLZULZLD PUR, OD[VJLII JO SUMOZ AGT] rere |syooys guapora AmB] OMT Kep~ —— *19G049Q [WUN syeAra4 -u14e s10q30 fq pue‘fep ames oy} UO syooys 1aq}0 GT Aq pamorfog ‘DUD aap ue Burkes JO 901I} OY} poqseyT "692 ‘d ‘720 ‘907 ‘oxorg|**'*** ~pamfut yonu sea aejnoysed ut orezuReVD *‘yooys yuapotaA Ara,q{ tt ttt? VLIQETED Uy|"F [Idy “9ZgT a ‘9 ‘g v "¢ %G ‘I 73 ON THE FACTS OF EARTHQUAKE PHENOMENA. ees a rt tarp bey oo “e101IVQ fopooseyy Stoop tdureg ‘eavst0g “mas ~pivapy paeapy Aq ‘uasieg op “4stpy ‘ou “ou ‘yoy *A Aq pojonb uaad IefMoyIed sty} UO sastyver} [etoaas pue {-proy ‘Tog { 06¢ ‘d “AT"} ovfag $048 “d ‘720 -907 “1013 -iney ‘79d ‘TEgT ue ‘steduerg aindieay £ 99-29 “dd ‘o110y, efaq "RITOIG Vljop torsey idm ‘ereqoy ‘anbiulapeoy uoroeT[09 “yruoryy) S,purpeIM ‘{"*peoxy ‘]]09 { purnieg ‘HOH “A f'peoy "TI09 “alns 49 ‘ggg ‘d ‘OE9I ue ‘sieduerg aimosapy Speoy "T10Q '°729 *a07 ‘rane "290 “AIX "3 “410d 49 “STH $0.1099°T £698 ‘d ‘Zouoiy9 o[qeyz, ‘1ayjney “Iatayos ‘oer ‘Yor JO aporuoAyH 943 sajonb Uva, f"peoy TODO ‘ purenig ‘anbimapeoy w01097[09) oy “yderdoan -quy, ‘ouapyed ‘ovr “L91 “4 ‘8291 [TA] "TINO id mm *ule{UNOUL BY} JO apis ‘ZZ pure 1Z ames oY 42 UOdnAa years e Aq Jaqye Ieak oT} eu} q JO 200} jusaM4oqI4SIN PeMmorfog ‘aFeT[IA ay Jo yxvd yeaud v pakoasaq| streets eee yooys yuapora Ar9A ylayy ye 1s0joot Jo aSeTTE A |-qaq "SeQT : (j) uustqoaze0 ay} Jo Burkes “118 OY} OFUT paster sadtasuIayy ‘SUOITAUD 942 «joy. 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onay) ‘Wd € ynoqe ‘iq -eg pur ‘onbiunieyy ‘soopeqieg ‘ens “Uy JO s}svoo a4} UGC) "aUIT} YORI 4YBreTy ssa] @ 09 ‘a10M soul} |, IAW IO ANOF pa.simd90 SuMog pue Surqge SI, ‘peateored Suraq Surggdue —ATao.teos 489M 9} UO ‘puLst oq} JO ysvoo 4svo pue Yr0u 94} uO aseuep jo [eap yvo1d v Sulop pue ‘yeyoung Suyepunut ‘sap qsoysty 9}, saoqe 4993 GT Jo WySIey oy} 0} pauinyor ATUappns se uoy} pue ‘sooed OT JO 7U94x9 OY} 04. ng Aygoa yod seas tH i ( ‘anbrury -IR]| 48 pyaf sem yooys ou 9eyy shes (gp “day ‘g3ehoA) ypjoquinyy *a "18900 BT} JO S19}VA\ 911} oO uoyom a4 Aq sarp “UF 18944 94} Ul payxreu FOL aTOA sqOaTO Szt ‘Mog Str ‘ur ayenbyyzea aq] 19972 SMOY 194 UeYY ssovT! ft 1852 REPORT 172 *IeIeIQI) ynoqe s{qIsuesUT ‘anbimaproy 101499T[09) anette emote tote ee eset emer eeteeneee “paforjsep a10M Buury punoie saseyiA Auvu pue zulog o[qog *1g]8M snomydjns 3no mary} pue ‘pouedo yjiva oY} Uaoooueg 4e JOATI ayy JO YoU ay} dvan ‘euurypy pue ‘osey ‘asnoyy dojeg ‘Qsnoyy puvpiaquing peanfur taqmeoag pig aqy "16F "dg “4d ‘| “JOA ‘sway, [LY dlueyy sojv] Fut1mo9900 se pauoyUsM syooys oy], “gaoqe sv IN ON.“ proy “T1990 S*suBLy, "ld SO ee teem et emereeaeeeee ewer ee ee etna et tthe teeseensere *(auryY ay} Jo UIseq 944 ul sayenbyjava uo 103;e] 949 JO Toulsut ay} aes) AeTIIg “J 0} SNIY -IRW "YO “IW Wor woYvoruntuMI0d @ ‘g[eg ye yey} 10g ‘ayenbyava UOQSTT BU} 107 2Ao0ge pajonb s1oyNy pred @ osor vos au} quayorA or0ur “ONT souMTE 910M SYOOTS O13 UOT 2U} 0} TAQ 94} WOT Aep SI} Jo wW'a TT FVPOOYS SIUPTEITVIGINFY/syoos SY, “AwyTeAGTH |G ——— — sieesenenereeeseeseereressleceecereccernsvereeereee* LUE XIS JO JAY poysery ut “ermnos iy ayy ‘pupey| "> fo ar ain RE OF TE gy pee SBM {ST} WO PoNUTzWOD Osye MOgSIT 38 1914905 Q1aM syooys ey] “FU STS SVM *W'd Z 4B ooys oy? rVqpeaqry + “BIsnTepuy WL [Jw Jo ysou pus ‘pipe 4@ yUaTorA OIOUI SVM JY ** [eI “nosy oy} 4B seynu sreyeaqty yt Wd Z *paydooxa eruoreyeg ‘arredg jo afoyM eq qsoulye pue ‘visnjepuy ‘WY 0€ yOT “syooys siour Aueul (AJoyeANIIB 9.10UL UdAIS JOUITATIIYIING ‘ges, Arenuer (ZT poyep 19939, & UL pa -LouaUt) 194] 14S ‘laqmieoaq] pig ayy *ySnologjweyyy 310.7 pue sty} woeaajoq siayjo aayeay Aq JO YyNOs sey ysys pomoyoy ‘Aep siya |-ugq Ayg ‘vuueyy 42 streeeseesesecesseeesereeesltQ MOOUS quajorA y|‘eayeuung jo purjst oy uy} —- —— —— “9UI1y 104s AIOA B pa -4S8e] £094Ip BINID FY *soas g 0} G WOT O yooys UWsTOIA “BOLIFY UL BNAD YW} OIG Tayyer @ awyeIqTN yy TeNRIQEN BYP f *ponuyuod srereeeesesleMQ0qS OU} UOgst'T IV seeeercee uede uogst] IV e “OTe 78 FPF yooys aug ‘uoqgsry “QUIT] OUIOS 1OF [72 panutjzuod a10joq Arp aureooq suse, ayy |Aep oy} JO syooys oyTjeq}? wo os[y “"W'd OT FG WO, S9TT} FY patand ‘areg ye Aep oures “WOgst y's “AON “SSS -d1 JUOWIBAONI 9], a 173 ON THE FACTS OF EARTHQUAKE PHENOMENA. ‘UMOP UMOIYY Ose o10M SAOUTIITYO autos sTodeuuy yy “WOysog Jo YNOS saTIUML YE 10 OZ ajenqiog 4e sov{d usye, oAvY 0} payatoder sem uoydnia uy ‘UAOp UMOIg) oraM skouuTIyO Saourlg ep azjezey f¢eg ‘d (oor woqy ‘payeySe yonum orem oanqIUINg “‘peoy “1199 ‘gi-— ‘dd -{ ‘Joa |pue smoputa oy uojsog yy “xapunt3 4ue\sIp SepP-6eP “dd “xI[x [0A ‘suery, [TY q\ex!] suotsopdxe Aq oynuTu e ynoqge Aq papadarg *g0URIY Op VINIIET £ “ASIP “unos S ‘UMOp UMOIYY ‘HOY ‘A S*peoy ‘[[op|u9eq savy 0} pres ore sosnoy orlYspxOJorOZy Uy “ggg ‘d ‘onbimapeoy woroayfoo|"** diys @ axl] [jez pue asi 07 powioas yJIva ayy, “Aqyuenb o81e] Ul yno suaeo Joye YOIyM *LIG ‘d *xI]X *[OA ‘suezy, ‘[IYq|wosy ‘1eau urejUNoM v ut porvedde Suruado uy “UOQSTT 4@ 4]9} Se pouOTUoUL 91e syOOYS Ou UOT 247 07 T3g 943 Wor “pornfur sBurpynq Tayo aUIOS PUL ‘MaxeYs svar [VIPS ot} OsTe OR ‘O73 jaTIAOG FW “UMOP WMO} OOM SyOOYS TaUTIOF “STH ‘on eee e eevee erro ese ssee cnet tees ereewetss Hast eeeseEeseepesseas poyeyise yonur sea JoyeM oy, *aoue SGU STDS STU TUES poyoouuo0d aq 0} posoddns sea sorpuy 489 AA OY} ULINOG.Ie FT SUTIVI “yg 4e vas aq} JO Jutmoy pur Suiqqa a[qeyaeur “01 y ‘ayenbyja1v9 sty} psouartedxa auuy ode, Jo 4sea sonseay Qf uea0GQ onuely 949 ur diqs y “A[Sno -1St1poid asor ves ayy, “4ST OY} JO yey} sv qeais sv ‘[esnj10g JO 48v00 94} Woy sonseg] 09 ‘PAS 1 qT 199q DAVY OF pres st “HINOL F°SUBIY, “[Yq (0371 joy? peqsisar pey YOY sasnoy atios uogsry yy\yooYS @ kep siqy uC rr eer rrr iy “yo} Usaq Suraey sv peuonueM st yooys ON ‘Joryostar autos pesneopue ‘meying ut joodopaeyy reou -our Surquia1; sorb B JO Suysisu0d ‘estou P2[qnopa Y}1M sooys qUdTOIA 910M pue Joyjoue sued 19978 Ajeyeripammy = wor} -Isod 1aUI10F $}t WO. 9993 OT Uaq YSIY 40ay 0€ JO 904 YW “1ay40 yoea uodn Bey 186 REPORT—1852. an immense large substance, which he described to be like a ball of fire, coming down from the sky quite perpendicular till within fifteen yards of the earth, when it suddenly disappeared.” 1841. Nov. 11.—One of our servants saw three falling stars in the course of milking, about 7" p.m. She described them as passing from E. to W. in the N.W. quarter of the heavens, as being of the first magnitude, and leaving trains. (South Herefordshire.) 1841. Nov. 12.—The day had been rough and showery, with a high wind from W. or W.S.W., and a little hailin some places, but the evening twilight was very clear, during which, about the same hour and in the same quarter as last night, our servant saw two considerable falling stars with trains. About 6"30™there was afaint light in the N. horizon, which I then thought indicated a slight tendency to an aurora, but I afterwards found it accompanied the edges of dark clouds in various parts of the sky. Until 9" I was detained indoors at L. (South Herefordshire) ; from that time till 9° 45™, I kept as sharp a look out as a speedy walk over a bad path permitted, but saw nothing until about 98 40™, when a meteor of an orange-colour appeared low in the S.E. to the right of Rigel, and about the size of that star ; its course was short, rapid and flickering, descending gradually towards the S. I did not perceive any train. 10" 30™ there was a fine meteor of the 1st magnitude, orange-coloured, with a train, in the E. quarter, shooting, as the former, in a line directed from Leo ; it was not seen by me. Two smaller ones afterwards, one with a train, which one I did not see, had short courses from the same direction in the E. or S.E. quarter, in the space of the next 7™ or §™. But between 10° 35™ and 10° 40", a small point was perceived towards the feet of the Great Bear, not far above the N.E. horizon, drawing a small train after it, and rapidly increasing in size as it rose with a steady course, in such a way as to prove that it was really drawing near from an incalculable distance in an apparently straight line. It grew brighter and brighter, as did its splendid and beautiful train, and it as- sumed an orange-yellow hue; it passed a few degrees N. of the zenith, but not quite so far N. as Cassiopeia, and still continued to increase as it de- scended towards the W. horizon, but it seemed to become fainter and to be extinguished before it reached it ; but trees partially obscured this portion of its course. It was seen by three others besides myself, my father, Mr. T. and his son, and it appeared to all of us except my father, to be attended, when at its height, with a hissing sound, but aloud rushing wind prevented any cer- tainty as to this point. Its appearance was like that of a magnificent rocket, and the impression of absolute height, speed, and projectile force, was truly sublime. Its size appeared to me greater than Venus, but not so vividly brilliant. The length of its course might be 5 or 6 seconds. At 11" 5™a stormy cloud in the N.E. horizon had a faint luminosity attendant upon its upper edge. A shower afterwards came on. At 11'45™, a storm, which had passed to the E.N.E. horizon, was followed by a similar light, which was very evident 5™ afterwards amongst dark patches of cloud. Our friends also saw what appeared like a light cloud somewhere towards the S.W. horizon, and wondered at it in the absence of the moon. 10™ after midnight the E. ho- rizon continued light, though the clouds had left it. I watched the S.E. quarter pretty frequently from 11° till 1" 30™, Nov. 13, but no meteor was seen after the large one, uor could J see anything during a short examination at 3" 30™ and 4°30". The distinctness with which I saw the light of the Welsh furnaces [20 or more miles distant] upon my walk about 9" 30", though the sky was very clear, except low in the horizon, was very unusual indeed. The air was not favourable for delicate astronomical observations, the diameters of the stars, according to Sir W. Herschel’s remark, appearing A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 187 enlarged. Miss H. N., who watched from half-past 1" till morning, informed me that she saw thirteen meteors ; the finest, which ran a longer course, were between 5" and 6". None of them, however, seem to have been remarkable either for brilliancy or trains. 1841. Dec. 10.—Eleven shooting stars were counted between 11" and 12° at night, by a person in Hampshire. . “The greater part proceeded from a N.W. direction, some far less brilliant than others, and their light of a silvery whiteness.” 1842. Aug. 9.—About 10" (as near as I can judge) I looked out for two or three minutes for the periodical meteors, but saw nothing, though the sky was very clear: my father thought he perceived a flash of lightning in the S. horizon. But on looking out about 10" 30™ (having been called by him upon the appearance of a falling star), I counted in about one-fourth of the hea- vens, or possibly one-third, 8 or 9 in as many minutes, two of which were brighter than any fixed star, and of an orange-colour; one left a beautiful train. I heard that two had been seen by a servant, between 9" and 10%, bright, and in immediate succession, but passing in different directions; and one of those 8 or 9 (which one’I did not see) appeared to my father to de- viate from the general direction of the others, which was towards the S. For about 15™ afterwards I saw no more, and gave up the observation. No- thing could be seen during a minute or two, about 1" 30™ on the following morning, or again at 2° 45™, except perhaps one meteor the latter time, but Iam not sure. (South Herefordshire.) The meteors on this night were seen by several persons in the neighbour- hood. 1842. Aug. 10.—The night was cloudy and rainy. Aug. 11.—I was out much during the evening and early part of the night, but saw nothing. 1842. Aug. 13.—Extract of a letter from a correspondent in Hampshire. “The scene was truly magnificent. I saw thirteen shooting stars within the space of half-an-hour, between 11 and 12, and S. saw one shoot at the same time that I did not witness, making fourteen. Three of them had beautiful trains, two in the 8.W., with trains something like the tail of the comet of 1818; colour of these two a silvery whiteness ; one was of surpassing beauty and brilliancy ; they both proceeded in a southerly direction. The third ap- peared near the Polar star, and proceeded towards the 8.E. This was less brilliant than the two preceding ones, of the same colour, but had a curious flickering motion in the train; the streams of light radiated towards the cen- tre of the train, something like this figure ES . It was very beau- tiful indeed, and what I had never before witnessed. ‘The motion too was less rapid than that of the two preceding ones.” 1842. Aug. 27.—A little before 9" p.m., the sky being overcast with thin clouds, a glow of dusky red light appeared between me and a thick hedge be- side which I was riding, and which was very dark ; from its peculiarity of ap- pearance, its being chiefly visible to one eye, and its duration (however short), I felt more inclined to refer it to (the reflexion of) a great meteor than to lightning, of which there was no appearance, though the weather was close and warm. The clouds were thin and foggy, and had no electrical appear- ance. (South Herefordshire.) 1842. Sept. 3.—Between 9" and 10" p.m., an unusual number of falling stars were seen, probably seven or eight in about 20™. 1844. Aug. 9.—Several fine falling stars, more numerous than the average, were seen (at Gloucester). Mr. H. W., who was observing with me, told me that for some nights previously, but especially last night, they were still more 188 REPORT—1852. numerous and brilliant at Minehead in Somersetshire, and that he saw one very curious appearance, resembling a serpentine train of sparks. He de- scribed them as generally visible towards the S.E. All those that we noticed ténight had a similar general direction from N.E. to S.W. 1844. Aug. 10.—A few falling stars were noticed (at Gloucester) moving in the same direction as last night, but one was observed which presented the singular appearance of a comparatively slow, and as it were difficult progress in the opposite direction. 1846. July 25.—A workwoman near Gloucester, returning home about 10" P.M., Saw a meteor of considerable magnitude. It was of the size and colour of the moon, and she compared its light to that of day. According to her account, it seemed as though it proceeded downwards from an opening cloud, and was instantly withdrawn into the cloud again; but probably this retro- grade motion may have been a deception. It was in the N. or N.E. at a con- siderable altitude. [This meteor was described in the ‘ Illustrated London News.’ ] 1847. March 19.—Extract of a letter from a lady. “ On the evening of Friday, March 19, A. and I left Albion Road [ Hol- loway ] about half-past 8. Not any stars were then visible, but when we were in Highbury Place, A. called my attention to what we thought a fire-balloon ascending slowly. It was in the west, a little inclining to the south. As it passed on slowly to the west its intense brilliance convinced me that it was not an earthly thing. When it appeared to be over Hampstead (but as high in the heavens as the sun is at 6 o'clock in the evening when the days are longest), it shot forth several fiery coruscations, and whilst we were gazing at it, broke into an intensely radiant cloud. This cloud sailed on slowly, and we never took our eyes off it. At this time the stars were shining. When we were in the gravel path opposite to Highbury Terrace, the cloud was rather higher in the heavens, and more to the W. It cast a most brilliant light on the houses there, brighter than moonlight, and unlike any light I ever saw. It appeared of a blue tint on the bricks, but there was no blue light in the cloud itself. Suddenly over the radiant cloud appeared another cloud std more brilliant, but I now felt so awe-struck that I cannot say precisely how long they hung one over the other, before the most wonderful sight happened. Perhaps they remained so for two or three minutes, when from the upper cloud a small fiery ball (about the size that the largest planets appear to the naked eye) dropped into the lower cloud, and was instantly absorbed. Soon after another similar ball dropped from the upper to the lower cloud; and then a ball apparently four or five times the size of the two preceding fell from one cloud to the other in the same wonderful way. Shortly after this both clouds disappeared, apparently absorbed in the heavens, though I did see a few particles of the brilliant clouds floating about for a minute or so. Pre- sently the moon appeared considerably to the northward of the place where the clouds had hung. We then saw the bright light across the heavens which you told me was zodiacal light, which lasted for more than an hour.” 1847. Aug. 10.—A little after 10" p.m., several large and beautiful falling stars, with fine trains, appeared to descend in the S. in pretty quick succes- sion ; and on the whole the meteors of this kind certainly much exceeded the average between 10" and 11° 30™. Most of them fell in the above-men- tioned direction, but the track of a small one, near the latest time of obser- vation, pointed towards the N.W. Several of them were noticed two or three nights ago. [Reference is then made to an account of shooting stars in a letter in the ‘ Times,’ dated Aug. 17, and this follows. ] The Hereford Journal of Sept. 8, 1847, contains also the following :—“M. A. Frére, of Montizon, ‘A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 189 has stated that on the night of the 11th ult. he counted more than fifty shooting stars in the course of two hours, viz. from 11 to 1. Most of them were seen in the Milky Way, and a few towards its edges. The direction of all, how- ever, was by the Milky Way, and towards the S.W. horizon.” + 1847. Sept. 14.—About 9" 48™ p.m., as I was looking (or going to look) through a telescope towards the S., a light caught my left eye towards the E. horizon. I turned immediately, but only caught a glimpse of a meteor of a yellow or reddish colour, about the brightness of Jupiter or Venus, which had descended through the N. Fish, to the S. of Aries, in a course a little in- clined towards the N., and had become invisible behind a building, leaving a narrow red streak, at first of considerable brightness, but fading very rapidly. Its course must have been of 20° or 30° in length, before hidden near the ho- rizon. (Gloucester, I believe.) 1848. Nov. 17.—During a brilliant aurora witnessed by me at the ex- treme W. verge of Herefordshire, three falling stars of considerable magnitude were seen, one with a long course and fine train. 1850. Aug. 12.—A few minutes after 11" (Greenwich time) a beautiful meteor shot across Cygnus, then at a great elevation in the meridian. I do not know whether I caught its first appearance ; but its brilliancy drew the attention of my left eye, while the other was at the telescope. Its course was from W. to E. and not rapid, extending for perhaps 10° or 12° till I lost it behind the top of a tree. Its light was intense, much brighter than that of Venus, and of a beautiful clear blue colour: in the middle of its course it seemed to be extinguished, and then broke out again as bright as before. I think it left no train. Nearly an hour before I had noticed a much smaller one, falling in quite a different direction, low in the S.8.W. perpendicular to the horizon. This meteor was seen at Highfield near Nottingham, by Mr. Lowe, as appears by his letter in the ‘ Times.’ He calls its colour, however, yellow. (South Herefordshire.) 1850. Aug. 24.—A little after 10" p.m., a fine yellow meteor fell from near the zenith to a Aquile, as large as Venus. 1850. Oct. 5.—While looking with my 51 feet achromatic at a consider- able star, probably of about 7 mag., I saw in the field a bright point of light, of nearly the same size and appearance, and at no great distance, which imme- diately vanished. It seems to have been a small and instantly extinguished meteor. It had I believe a reddish tinge. 1850. Nov. 29.—About 9%, or from 9" to 9" 10™ p.m. Greenwich time, I caught an oblique sight of a very beautiful meteor of a yellowish colour and considerable size, which seemed to run a very short course at a great alti- tude, a few degrees W. of the zenith, and I believe among the stars of Gloire Frederici ; but I did not exactly note the place, as finding it had left a bright and beautiful, though short train, I endeavoured to turn the telescope upon it; but before I could succeed, the train had disappeared, and I then could not exactly identify its place. [This meteor is mentioned in the ‘ Times,’ in two letters, dated Barnstaple and Brixton Road.] 190 REPORT—1852. II. Meteors observed by Hrnry Lawson, Esq., F'.R.S. (assisted by T. CANE, Esq., and H. Apams, Esq.), at Hereford, during the November Epoch of 1841. Communicated by E. J. Lowe, Esq. oy. 11. From Noy. 12. From hm hm 7 15 till 8h 35™ none seen. 293. 12 24 alt. 20° towards horizon in No. 253. 8 35 from Ursa Minor to Cygnus, a S. direction. with slight train. 294, 12 25 from Cassiopeia to Ursa 254. 8 45 from Ursa Minor to Lyra. Minor. 255. 8 55 between Pleiades and Ursa 295. 12 50 alt. 90°. Minor, with slight train. 296. 12 52=2nd mag. Between Cas- 256. 8 57 passing down through Ursa tor and Great Bear. Major. 297. 13 10 alt. 400, from W. to S. 257. 9 4Anear Polaris to the Great 2 Declining. Slight train. Bear. Soon became 298. 13 11 from zenith to Great Bear. cloudy. 299. 13 33 alt. 70° from N. to S. Nov. 12. : 300. 13.34 train of light, from Ursa 258. 7 O from Cassiopeia towards Major to S. Polaris. Very faint. 301. 13 45 from Castor, downwards. 259. 7 29 near Pleiades. 302. 13 46 from Capella to N.W. 260. 7 30 from Cassiopeia to Ursa 303. 14 0 from Cassiopeia to N.E. Minor. Bright. 304. 14 8 from W. to Ii. through the 261. 8 15 from Polaris. Pointers. 262. 8 30 from E.to W. Small. 305. 14 17 from Great Bear towards W. 263. 8 35 from W. to E. 306. 14 32 8° towards N. 264. 8 36 from W.toE. Alt. 90°. 307. 14 40 from Pointers towards W. 265. 8 37 from E.to W. Alt. 25°. 308. 14 45 from N.E.to N.W. Alt. 306. 266. 8 40 =1st mag. from E. to W. 309. 14 45 from N.W. to W. Alt. 12°. Alt. 45°. Train of light, 310. 14 46, flashes in Ursa Major. 267. 8 44 from E. to W. Small. Alt. 311. 15 1 from Orion downwards. 40°. 312. 15 2 from Orion downwards. 268. 9 Ofrom W.toN. Alt. 40°. 313..15 3 from alt. 40° in East down- 269. 9 23 from E.toN. Alt. 30°. wards. 270. 9 43 from E.to W. Alt. 30°. 314. 15 4 from E.to W. Alt. 30°. 271. 9 48 from zenith to N. Alt. 40°. 315. 15 15 train of light. From Leo 272. 9 54from E.to N. Alt. 60°. to Ursa Major. 273. 10 0 from Cassiopeia to Polaris. 316. 15 16 crossed Orion to W. 274. 10 1 from Ursa Minor to Ursa 317. 15 17 from Ursa Major to W. ho- Major. rizon. 275. 10 2 from between Castor and 318. 15 17 from Ursa Major to W. ho- Pollux to Ursa Major. rizon (following the path 276. 10 5 as bright as Vega from me- of the other). ridian. Alt. 15° down- 319. 15 18 from Orion downwards. wards to E. 320. 15 22 from Gemini, southwards. 277.10 6 from near Pleiades to Cas- 321. 15 22 from E. to N. Alt. 20°. tor. Train of light. 278. 10 15 from E.to S. Alt. 10°. 322. 15 25 from Leo downwards. 279. 10 20 from W. to E. Alt. 20°. 323. 15 27 through Orion downwards. 280. 10 40 from zenith to Castor. 324. 15 29 from N. to 8. through Ursa 281. 10 44 from Rigel to Batelguex. Major. 282. 10 45 from Pleiades to Castor. 325. 15 30 from Orion to Sirius. 283. 10 45 from E. to W. as large as 326. 15 32 to W. Alt. 70°. Sirius. Of a bluish-green 327. 15 35 from Polaris, downwards, colour and with a train with train of light 70° long. 328. 15 37 from E. to S. Alt. 10°. 284. 10 48 from zenith to W. 329. 15 40 from zenith to Polaris- 285. 10 49 from W. to E. Alt. 20°. 330. 15 45 from Sirius to §8.E. horizon. 286. 10 54 from W. to E. Alt. 80°. 331. 16 2 from Castor. 287. 12 0 from Pleiades to Castor. 332. 16 6. Alt. 20°. 288. 12 | from Castor to Procyon. 333. 16 10 from zenith to W. Train of 289.12 2from N.E.toS. Alt. 20°. light. 290. 12 15 alt. 20° in S.E. moved to- 334. 16 10 from zenith to E. wards horizon. 335. 16 14 from Castor to E. 291. 12 16 towards N.E. Alt. 25°. 336. 16 30 due E. Downwards from 292, 12 21 from Great Bear to horizon. an alt. of 20°. 191 By M. Buuarp, B.A. HSER REED SESE EP REF SEPNEET ES 1 -anhojDjv) S$ PIB[NG “AJ U2 Stoagzapy snowno psow ay7z fo mar4 A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. =) Lo} I @ bow @ es a Fd Ss D ~~ = -) =~] S i~ ‘~ S$ s Lo | > ~ = a=) S 8 -Z2 x Do a sx Ss | — — 192 REPORT—1852. Hour. Bright- | Velo- | Mean places for | Mean places for Apparent | ness and] city or 1840 of A. 1840 of B. Greenwich| Magnitude. | Colour. | Dura-}————j———__ Mean Time ‘ tion. | R.A. hm i s 9 21 25 11 34 53 May 22/11 45 00/y Orionis 4 |July 5/11 38 00\e Orionis 5 6/11 34 00\2 Orionis 6 | Aug. 12/10 00 53! Geminorum 12|10 7 00/|Sirius x3 12/10 14 50)a Orionis 12|10 15 45/a Arietis 12/10 21 00 12/10 43 00|e Arietis . 12/12 20 40|a Arietis 12/12 24 00|¢ Arietis 12/12 14 50|Sirius x6 12/12 25 00/4 Pegasi 12|12 38 00 |Sirius x8 13/11 12 52|\y Pegasi 13/12 53 00|Sirius—0'1 ... 13|10 3 00|« Arietis 13/11 53 00|Sirius x 2°5 ... 13|12 18 00|é Pegasi 13 | 12 23 4 Orionis 15 |12 18 6B Orionis 15 |12 31 B Orionis 15 | 12 37 15|12 45 B Pegasi «s+... 15 | 12 49 B Orionis 15 |12 49 Aldebaran 15 |12 58 15|138 11 16/10 15 19/10 27 7 | 9°80 Sirius 7| 9 33 00 \a star, 3rd mag.|White .. 1l| 9 26 Sirius x 4 Blue 11/10 21 Aldebaran 11/10 22 Aldebaran 22| 9 48 94/11 53 24/12 6 1a9 19 15 |10 17 150 15} 11 22 15/11 35 15} 11 52 Fl etal 6|11 3 Sec|p oll 69 22 10; 6 34 Aer eee 356 12 13| 9 39 ionis ...... K 332 25 |~— 2 55 | 335 45 75 00 |\— 3 338 | 66 39 A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. Mean places for 1840 of C. Place of Observation. Lat. 450 59 46-6 +50 59 46-6 450 59 46-6 449 26 29 49 26 29 +50 59 46-6 450 59 46-6 450 59 466 450 59 466 450 59 466 450 59 +50 59 +50 59 450 59 +50 59 450 59 450 59 42 54:7 |450 59 +2 54:7. |4+50 59 +2 54-7 |450 59 42 54-7 +2 54: 42 42 4 4 4 6: 6: 6° 6: 6° 6: 6: 6- 6: 6: 6: 6: 6: 6° 6- 6: 6- 6 6 6 6 6 6 6 6 6 6 6 6 6 6 6 6 6 6 ”) 6 AVY 4 4 4 4 4 4 4 4 4 4 4 46: 46: 46- 46° 46° 46° 4 6 SUGGS SVAN ON 193 = () ei Train or sparks. Remarks. g & oO | Ff A most splendid meteor, giving light all}) 7 over the country. noise. See fig. 4 Explosion without as With a train of light and nebulous ball. Passing through a small Vb Ye Cirrocumulus. A very beautiful meteor, having a nebulous appearance, train of light. No. 16, alike. No. 14. See fig. 3 in Map. an Rather a brilliant object. aa C. Bulard, Esq. Here a rather curious phenomenon took place. When No. 27 was in C, No. 28 vanished at C, fig. 10. |A beautiful meteor with train of light. \34. Seen in the field of telescope while ob- serving Neptune. The given places are for 1800. 35. Train of light. 37. This meteor has not been observed ex- cept the light which emanated from it from the zenith and which was very bril- liant indeed, and so intense was it that the observer thought it safer to take a shelter in-doors. ° = e This is the curious meteor of which a draw- ing is given in the Map. It showed a dark side, and then a bright one. See fig. 9. = oO Mr. Lowe’s MS. Cn a REPORT—1852. — ern Witte < aise sa White ... arenes ‘|White ... Bright- | Velo- ness and | city or Mean places for Mean places for 1840 of B. colour. | Dura- tion. 1 0: a Aldebaran...|Blue...... 0-5 Reo tenet Blue......| 1:0 behets Blae-.sc |e esr White 2-0 caer Bldecscses| Ouse ahs set Blue......| 1:0 iraaoiwcs Blue......| 2:0 eouaine Blue......| . 1:0 a Arietis «.....|Blue...... 0:5 Seecse Blue......| 0:5 hessicien Blué:c-<.-| EO oes Bluez<...|) cane eek anncs Blue....-.| 0°5 Seawaseae Blue......| 0-5 Sodenowa: Blue......| 1:0 Pete's White 05 sabia Blue......| 0:5 none Blue......| 0°5 becuse White . 05 Reuceees Blue......| 2:0 Be ree Blue.....-| 05 gers Blue......| 2°0 Savas Blue......| 0°5 aint Blue......| 10 padegsisa Byvessszec|) ew seas Blue......| 1:0 Paste White 0-75 Br cs Blue......| 05 Ee Blue.. ...| 0°5 see Blue......| 05 een aieess Blue......| 1:0 Raia Red. sues) se IZ. ..creeee Blue...... 05 @ Lyre......-.- Blue...... 1:0 Se Blue......| 0°75 Sar hiiees, Blue......} 1°5 coanes Blue......| 05 Sewanee: Blue......| 1-0 Leet Blue......| 05 ence Red ......| 0°5 — 9 20| 19 05 |—-12 4 2000} 708| 24 64 00 | 2000] 806 1400| 2317| 4 25 00 | 825 88 | 16 é 34 46| 11 40| 26 20 00 | 28 39| 14% 1835 | 25 00| 129 19 23| 514] 14 33 27 | 5100} 26 246) 1754 |— 3¢q 9 30 | 195 00 74 16 45 | 160 00| 124 10 00 | 6930) l¢ 23 56| 72 02| 23 024 | 149 00| 01 15 47 | 196 30} 14 8 00 | 14400} 95 115|18900| 4 128 00 |+ 4 30 | 119 30 |+135 92 00 [+23 16 | 87 1 |425 White ...| 0:2 191 53 |+ 6 40 | 197 23 + 6) R.A. Decl. 26 9 38 45 99 44| 59 36 58 40 | 8 29 83 10| 612 332 6| 14 8 15 35 | 30 34 $510 |- 4 8 126 29 | 12 45 181 40 |= 9 16 212 17| 7011 124 55 14 44 223 22 | 21 51 189 23 6 Bé Borealis. 3 Borea 172) 11 4 29 275 44 | 23 50 274 51 2 } 154 59 | 59 OC 231 47 1 3& 313 9 | 435 253 33 | 42 4¢ 277 53 | 31 3k 290 20 1 30 01 | 55 13 31 | 49 430| 42 355 00 | 23 4 857 45 | 14 4 20 44 | 20 4 155 88 | 58 4 A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 195 E ee for Place of Observation. Train or sparks. Remarks. Observer. Reference. i R.A. Decl. |L. from G. Lat. | | | | ° 4 m 8 fe} 16 55 |42 54-7 [450 59 4 22 00 |+2 547 |450 59 4 62 33 |42 54-7 |450 59 4 3 28 |-42 547 |450 59 4 — 242 |42 547 |450 59 466 5 25 |42 54:7 |450 59 466 17 23 |+8 20:0 |+50 30 00 [Ascending slowly. 9 44 |+8 20:0 |4+50 30 00 |A beautiful meteor with two successive fire- 18 00 |+8 20-0 |+50 30 00 balls. | Explosion without noise. See +8 20:0 |+50 80 00 fig. 7, 10" 57™ 0°. Fig. 8, 104 57™ 48, 6 i Ascending slowly. 6 pst ga SRESSS, oo i—) a Co Senos s Fl eal — al om eS BK | — or oo ~\ BB : ie J ifs i ' 66 32 |+8 20:0 |+50 30 00 10 39 |+8 20:0 |+50 30 00 17 29 |4+2 54-7 |150 59 466 0 35 |+2 54:7 |4+50 59 46-6] - 23 45 |+2 54:7 |4+50 59 46°6/This meteor passed exactly over the follow- ing stars. — 137 |4+2 547 |450 59 466 +2 54:7 |450 59 466 +2 54-7 |450 59 466 42 54:7 |450 59 466 46°6 66 6 42 547 |450 59 +2 54:7 |450 59 46: +2 547 |450 59 46: —4 29-97|4.49 26 29 —4 22:97|449 26 29 —4 22-97|449 26 29 —4 22-27|4.49 26 29 —4 22-27/449 26 29 +2 547 |450 59 46 +2 54:7 |450 59 46 +2 547 |4+50 59 46 +2 54-7 |450 59 46 +2 547 |+50 59 46 |A fine meteor with train of light. 42 54-7 1450 59 46 +42 54-7 |450 59 46 +2 54-7 |450 59 46 +2 54:7 |+50 59 46 +2 54:7 |+50 59 46 +2 54:7 |+50 59 46 |A beautiful meteor having the appearance +2 54:7 |+50 59 46 of a blue ball. +2 547 |450 59 46 +2 547 |450 59 46 +2 54-7 |450 59 46 +2 547 |450 59 46 is oe Ss C. Bulard, Esq. Mr. Lowe’s MS. +2 54:7 |4+50 59 46 |A beautiful meteor, of ared colour, inclining +2 54:7 |+50 59 46 towards orange, perhaps on account of +2 54:7 |150 59 46 its proximity to the horizon. +2 54-7 |450 59 46 +2 547 |450 59 46 42 54-7 |450 59 46 +2 54-7 -|450 59 46 +2 547 |450 59 46 +2 547 |450 59 46 +2 54-7 |450 59 46 2 , Cn 196 REPORT—1852. Hour. ; Velo- | Mean places for Mean places for * Apparent Bright: | ity or 1840 of A. 1840 of B. ate. Gr ‘ch! Magni ness and reenwic agnitude. | Colour Dura- Mean Time tio R.A. Decl. R.A. Decl. 1851. |h m s 8 Pan k, 0 Ben| a Boas 104| Feb. 21/12 20 00|Lyra............ Blue...... 05 178 10 |+ 7 30 | 170 00 |4 6 54 21/13 8 30\Virgo ......... White ...| 0-5 144 00 |+26 45 | 188 50 |+26 52 21/13 30 30/Virgo ......... White ...| 0-25 | 216 14 |+381 4 | 219 00 |+84 00 22)13 30 30/|Sirius ......... Blue...... 05 175 13 |+15 28 | 163 27 |+17 00 26) 8 58 30)\Aldebaran .../Red...... 15 196 37 |+41 00 | 191 40 |+34 24 Mar. 24/13 56 30)|Lyra............ Blue...... 05 15 33 |+86 27 | 348 51 |4+83 29 Apr. 19/10 30 30/Arcturus ...... Blues. 2.: 2-0 214 00 |+89 00 | 205 28 |+20 00 19} 9 45 30 |Lyra............ Blue...... 10 128 54 |+18 13 | 127. 6 |+10 12 | 22|10 47 30 |Lyra............ Blues... 05 227 6 |— 8 80 | 230 00 |— 8 5 28) 9 40 30|Lyra............ Bluey..00: 05 180 00 |+ 2 40 | 170 32 |— 4 00 28) 9 50 30)Regulus ...... White 0:25 | 185 24 |—14 30 | 181 00 |—15 00 28) 9 55 30)Regulus ...... White ...| 0:25 | 184 00 |—16 00 | 180 00 |—20 00 30) 11 40 30|Lyra............ Blue...... 05 263 00 |+ 4 40 | 259 00 |— 0 00 July 21/10 40 30 |Lyra............ Blue......| 0-5 3 1 |+28 52 2 5 |+21 37 21/11 23 46\Aldebaran ...j/Red...... 1:0 353 8 |+45 40 1 18 |+50 12 21}11 28 40|Lyra............ Blue...... 05 348 14 |+26 50 | 354 56 |+31 30 21/11 46 40|y Arietis ...... Blue...... 0:25 | 857 44 |4+46 59 2 30 |4+42 20 21/11 49 10|y Arietis ...... Blue...... { 0:25 10 15 |+88 5] 12 20 |4+28 5 21)11 56 25 |y Arietis ...... Blue...... 0:25 28 30 |+81 30] 380 5 |+25 11 30/10 53 10|y Arietis ...... Blue...... 0:25 20 44 |+29 14 | 26 4 |4+28 50 30)11 0 2/|Lyra............ Bine:..... 15 349 21 |+380 00 0 30 |+45 11 30) 11 19 40|Sirius ......... Blue...... 0:25 | 840 25 |+23 40 | 342 20 |4+20 00 30) 11 23 10|y Arietis ...... White 0:5 0 9 |+53 38 | 359 10 |4+52 10 30) 11 53 10|Lyra............ Blue...... 0°5 857 14 |+45 11 9 58 |4+48 25 30)11 56 25 |Lyra............ Blue...... 0:25 0 30 |4+29 00 2 34 |+30 38 30/11 56 30|Sirius ......... Blue...... 05 6 40 |+59 15 | 350 15 |+66 21 80}12 1 10|Lyra............ Blue...... 0:25 18 45 |+59 17 | 15 35 |459 32 30/12 5 55 |\y Pegasi ...... Bines-6.0% 0:25 | 358 26 |+388 48 2 30 |+39 49 30) 12 12 10 {Sirius x2...... Blue: .s 1:0 24 45 |448 15 | 35 00 |+52 18 Aug. 3) 9 48 15 |Lyrax2 ...... Blue...... 05 333 40 |+29 18 | 338 24 |+25 00 3/10 27 45|Lyrax2 ...... Blue...... 0:25 | 848 15 |+22 46 | 348 40 |415 50 3/10 29 00|/Lyrax2 ...... Blue...... 0-25 22 3/447 4] 28 31 |+41 34) 3/10 33 45 |Lyrax2 ...... Blue...... 0:25 | 846 5 |429 18 | 351 35 |4+382 50 3/10 54 50|Lyra............ Blue...... 05 357 14 |4+ 4 24 | 2053] 58 24 3/11 2 50|Lyra............ Blues..... 0:25 | 359 8 |+80 18 | 345 13 | 38 27 3/11 14 30|Lyrax4 ...... Blue...... 0:5 10 00 |— 3 25 032|— 8 5 3/11 22 20\Lyrax4 ...... Blues, 002 0:25 | 353 59 |4+28 41 | 348 41] 15 56) 3/12 8 20\Lyrax4 ...... Blue...... 05 34 45 |4+ 7 85 | 27 15 3 20 3/12 12 40|Lyrax4 ...... White ...] 0:5 5 36 |—10 35 0 38 |—15 17, 3/12 16 10|Lyra—0:25 .../Blue...... 0:25 31 8 |4+11 00} 38440}; 11 15) 3} 12 36 10 |Lyra—O-25 ...|Blue...... 0:25 36 5/4189 81 | 40 25 | 34 24 3) 12 46 10 |Lyra—0-25 .../Blue...... 0:25 4 2\)-—138 6 1 38 |—18 24 3/12 56 30|Sirius ......... Blue...... 05 80 57 |+17 23 | 27 9] 14 81) 3) 12 59 30|Lyra..:......... Blue... 0:25 40 20 | 3710] 385 12]. 36 40) 3/13 1 20/|Lyra............ Blue...... 0-5 538 4] 8252] 52 36| 27 40) 3/13 14 20|Lyra............ Blue...... 0:25 56 4| 17 2)| 5629) 12 34% 3/13 28 15 |Lyra............ Blue...... 1-0 43 31 | 2042] 4537) 19 7 17| 9 44 30/|Lyyra............ Blue...... 05 257 14 | 43 27 5°37 | 48 45 | 17/10 25 30|Lyra............ Buel sees 0-5 268 14| 16 40] 265 1 12 41 17/10 36 30|Lyra............ Blue...... 0:25 | 262 17 1 19 | 257 46 |— 1 59 | 17| 9 49 30|Lyra............ Blue...... 0:25 | 239 00 4 40 | 286 50 2 20) 20; 9 50 1|Lyra............ Blue...... 10 17 40} 12 30] 2149] 16 37 21;10 2 1 |Lyvra............ Blue...... 05 181 52| 57 00/176 54] 56 20) Sept. 3/13 26 30/Siriusx3....,./Blue...... 10 828] 4024} 1019] 26 50° Mean places for 1840 of C. cA ° yf 163 4 |4 4 29 133 20 |425 5 224 11 |436 30 150 00 |-+16 00 190 58 |4+28 25 +77 00 | | 195 00 |+ 5 00 | 123 43 |— 1 37 | 232 31 |— 9 31 | 163 00 |—13 55 | 178 00 |—18 00 ~| 178 00 |—22 00 | 257 00 |— 7 00 3 5 |+16 00 oo a —) _— i) R.A. Decl. ~~. 2 ee i } Place of Observation. L. fromG. Sr Or Sr &r oro Or ot i Lalas sree ANAS YVAN Lat. ° / 450 59 450 59 +50 59 450 59 450 59 450 59 450 59 450 59 450 59 450 59 450 59 450 59 450 59 450 45 450 45 450 45 450 45 +50 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 +50 45 450 45 +50 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 450 45 25 25 A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. Train or sparks. Train. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. |Train of light. -|Train of light. |Train of light. Train of light. Train of light. Train of light. Train of light. Train of light. Remarks. 197 | Observer. | Reference. a i C. Bulard, Esq. yo Mr. Lowe’s MS (is ee ee SS eS eee 3 198 REPORT—1852. . IV. Observations of Luminous Meteors, 1851-52. Com- Date! Hu Appearance or Brightness MWtain or aparks Velocity or te: snl magnitude. and colour. hsb duration. —————— ——— nnn nn nnn ae 1851. | h m | July 4/11 16 30° |=twice 2 ......s0.ee. Orange - red,|Small separate balls. 3 secs., slowly; at ! the separate last vanished sud-j- | balls _ blue, 80.6 denly. || | very bright. QC) oF G00 at ies Fd Jeegi%0 came more purple. | 2011 5 ......)=twice 4} ......... ealRedt esos ce Slight tail .......... Sandi He SEC. svcccactvecsc ca TUS0D ve. -s(As’a spark ieers.ot0e 5. Orange-red .../Slight tail ...........6+8 one [OPZISEC. Cnescecess al 29/10 36 ...... ‘Small, indistinct ...... WellOw:.- veleives= Gou denveapaessne=teeee ayes |LISGGe dueneanen Cuan 29] 8 58 30.../Very small ......eccssc|.secessneceeseeeee|oceseeree Seger ecg ceret seesseee-[Almost instantanes| : ous. } 30} 8 25 ...... =to Saturn,.,......... Much brighter|Long tail of sparks .........]2 S€CS. sessesssrsevees than Saturn; orange. 8 50 .,....,=2nd mag.,.......00e =8rd mag., |Continuous streak .........{1 sec.3 rapid sree yellow. | 9 A veeeee}=Srd MAG. eserereres ..|Orange, =3°5|\Composed of many sepa-j2 secs.; slowly ... mag. rate sparks. ; Noy. 3] 5 32 ....../6 times size of Saturn|Pale orange,|Slight tail ,........-++.++++ 12 SECS. ...e00e and after 15° move- ment turned bluish. lO The above is a sketch of it. | 4) 5 30 ...... 2 size Of ( sseeeeeeeee(Orange and |No sparks ..,...sereseeeeee Several seconds ..4) prismatic. | 11| 7 49 30... 8 5 30... 12) 7 56 ...... Li te ee 14/10 45 ..,... REPORT—1852. Velocity or | Very bright ............ Much brighter|Leaving bright train, cu-|3-5 sees. ....esce0 J than Vega. | rious path, thus :— 4 Small Preece ee Cee eC CO Cees eee e eer rere Titi i rere ere rere eee reer rs seeensee .-|0°5 sec, weeeeenee i Very small ...... sesconl ING 555.0.-0500-[ee ce sbiatane APereoryiccaer +++eee(Less than 1 sec. Ac SN AuEM tate nesenyen|adns'soneacr sess an=| ocdeeucedncnarsnepet sane manda Less than 1 sec. «« == 2G MAL riagss ens sess Brighter than|Sparks .......... nayiiise ine erste dG Glld tips 2nd mag. ; { orange-réd. = 1 =2nd Mag, ....00..00+0/ Saber cinsnt arene Train of light .....00+...5+.|scssvesgescsesescueane A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 203 General remarks. Place. Observer. Reference, Direction or altitude. —— ——+ ——> | $< fidwaybetween Vegaand Altair\...... seeeereeeseeesee++|Castle Donington|W. H. Leeson,|Mr. Lowe’s MS. to below Delphinus. Esq. ‘om # to x Draconis...,,....... Aurora at the time.|Ibid....... Sab an'enal Ail gan ao ‘om near 9 Draconis to about]........cseeceseees ++-«-(Obser”, Beeston |Id. ..........08... No, 76 Urs Majoris. First seen R.A. 12° 53’,N.P.D. 31°; | disappeared R,A. 12 32™, _N.P.D. 26° 20’. rom ¢ Andromede to 3 Piscium].........00-ssseeseeeees MBidaxanstanessessgs| ies ens deaureten see Brom No, 72 to ¢ Piscium ..,e0|s., oc SMRETMARY os. |cocscconessissansasceasesearouese Passed 5° above Pegasi, and moved|# obliquely north-| ward, its path) forming an jangle} of about 20° with) horizon. It moved) over 4°very slowly; it made a stop and) partially disap-| peared before it finally vanished. Feb. 1/10 13 ...... Size of Mars ...... . |Orange......... Continuous train............ Slowly; duration 1 sec. 18)10 55 ...... Small, =3rd mag. ...!....s0...008 ease loeeuceveseences Wt seneccrc. sas Slowly ...060...e008 | PAN IONS YS aap oe SGT eerie Not so bright|No tail....... Wick icecnsesecs Duration 1-5 sec. J ; as 2nd mag. DEIGOU DA Vales nhclcarcssstase- doesn herersen|esniasauee co obeypelitereise ceases RR bs savecanvees|eontanmennnenents ct : 8 50) esas vba seusevetbosdeosen’ seas Viveebseveusleasszsecussss sisssbsebe Pe eer Pet eet Seneemm April 8/10 19 ...... Small scc.ceteeweces ees BORE a. Bie All ew ee sas Meche ach tase ewes temeneem Rapid 9/9 39° seis Small ites le eeeviiess Ble Waites Train: csscucstexoe. tts .ueneee Rapid ....... 12)10 40 ...... Sallie cocs cet ace cas ccclecco@e el Uescbscon|ecsocs cocnnasesecastassencceaqten|ss@ueueeamr rams WORDS) ccc. SINAN See e aiee cde bce sccal be ncvavesseckascc|baudessccstnqeenveceuderavensens Rapid ...... WZe AQ iecaces|SIWIAU apanmpaeanenans 13)13 12 ...... =4th mag Blue.....cebeos- IT WO Sparks ...00....5-.se0000 Instantaneous ..... : / . ES WAV cot 00 Pensa nares: Mellawish bed) |!.;..-.s00s0%--Fact oaaeesteaee T R60. onus. =. 20 Brighter than 21/10 45 ...... == ONO MMAR ssesss0ness6 Orange sae eeo Stream of light ............ Slowly ......00+.+08 - 26) 9 40 ...... Sitalgeese eset e ee cnkc| cies csseces biscclevcsccasenovesspenebesedseenbacas|:cchegeammmnes ~osce ODO yea.aKs Sal eee aeeceweccrseuloecececcstercks ds |evwenatcocoesstsiuapbnsnseccevsses|-mcseeeeeenegs 7 HO! 20 ... 04. Sti AUC renee ena ln bac onusos¥acua| to tesesven eaanercuereseauecke seals asegeateiedes May 10/11 0.25.8 Small COR eRe eee OHH en BETH R eee E EEE E HE SHEE EES H TE ee EHH ea EHH eas eS He ewasnl HEH EHTS SETH EEE ene eee A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 207 ie Direction or altitude. General remarks. Place Observer. Reference. from 4 between yand 6 Andro-].......:s.c.sccsecesuues Highfield House |E. J. Lowe, Esq.|Mr. Lowe’s MS. mede perpendic. down. From y Urse Majoris betweenl.................0.0206- WDids.vccvedsns esse 1s a ee renner tae Ibid. m and ¢ Ursz Majoris, nearly _ perpendic. down. From 4 to 1 Ursa Majoris ......)..........ccccceseseeees MDG sa se 4h cesene Ls SE aaa cee Oe Ibid. Asse Over 15° in 3 Secs. ......|....cccccecoscstescacese Darlington, Dur-|J. Graham, Esq. |Ibid. ham. MEMS leevinecscnaewhsasavoceeccdvalaccsssctsseenssventences Mbidis Socsks socal LUG Ue ae Ibid. wh From midway between @ and ¥)................00c0000 Highfield House|E. J. Lowe, Esq.|Ibid. Urs Majoris, fading away at Observatory. | about R.A. 13°30’,N.P.D. 44° |From 30° above 8.S.W, horizon]...... ESL Tbidsississsss.ceeve Td. vids tsiviveans Ibid | perpendic. down. From @ Ursze Majoris through ¢.....40......csceseeees TbIdsisiiiiicecns ea) (; Capen ery | 15) Ursz Minoris ; moved slowly towards « Cephei, fading when 3° from that star. |Moved downwards, passing].........06.....cceees. Dbid:. dsaditisesss cllTd eee iwi Ibid. | slightly E. of Procyon. |A very large meteor reported a|..........cc0c.secs0eee. Thid..........cc00s Td. ccssbiivinitans Ibid being in N.; unluckily I was not observing at the moment. _ My brother saw the reflexion and registered it as a flash of _ lightning. From 3 Cephei towards Arcturus|...........0ccseceecs000 DDG. ixnaeahedihscut Ids. .onv tt ivewl v. {[bid. from 3 Hydree perpendic. downl...............cecceee0. Ibid. ‘ To vioas itt e¥ ...{Ubid MMMEEACEOSS LCONIS ..,......].....0ceeessceeerctenecs HTC Piers eee OP ie ee Ibid. I ana oc cc ese. |eseaeecean done dSeacéeas Dd types. eee 1G Seen eet a Ibid MRUMSNGA VICGINIS © .....-000...|sceccseeeeneesececccsaes Ide ee. osecee: [Ws Ea Spay areret Ibid. m Caput Medusz to < Bootis|Two spark meteors|Bath Observa- |Id. ............... Ibid side by side; moved] tory. very rapidly, appa- rently at no very great elevation. About 30’ above Mars; moved|Well-defined circu-|Mr. Lawson’s Id. ............... Ibid 1° towards Pollux. lar disc. Observatory, Bath. from 3 Cassiopeiz towards W..,|..............seceee0ee. Highfield House |[d. ............... Ibid _ a Slight inclination. ynwards from 4 Virginis ...)...............ceeeeeee Tuts Hae aaa he eR tbe Ibid. SENEMOMECOUIS =... sctsc| teks ee. 12) fo Bi eae 113 baleen. Ibid OAT CYLATIED FERR Aneel Bailie ieee on Velie! MDGs sececb ca cae oui UG Ba ee ere cee: ae Tbid. pendic. down in N.N.W. ...}..........cseeccecueeeee DIG: eeseat ss csscae A.S.H.Lowe,Esq.| Ibid. REPORT—1852. Appearance and Brightness Velocity or Date i, nighitnde, sett caton Traigggr sparks, Duration. 1852. | hm July 3/10 30 ...... 6 times 2/, gradually|Pale blue......|Long streak......... paae ene Slowly, 8 secs. ... diminished in size. 1210 47 30° |< at opp. .........]... afigdoa: vadeed we(Li@Lt & CLAM cs edecccabetaneses 2° SECS. .csccevsever NSINO 4G) See sielesorssecpeeacences ses Banas (OM Alas ca cee, che Retains cs aveeasegopeee wade cuman Horizontally from } through ¢ Ser- pentis. AES OP csdosieeses pecenmalee eras ahesarcen Small ....... Su Bcos bet ncecotcanrerpccuaacs ...../Through zenith from S.E. to N.W,| 19/11 10 ......). ste piotiese trio ana aecices/et = Brilliant ..... ./Leaving a lengthened train|Fell parallel with milky way, pass- ing near # Cygni,) moving to E. VO) S9 15" 9) =—Andimap. ..2.-..sa0- Colourless_ ...Continuous streak ......... Slowly, 1-2 sec. ... M2 Geese. « SOU El DAR tae denses «ales Colourless ...\Continuous streak ......... 0°2 sec., rapid... 22/11 59 57° |=3rd mag. ............ Colourless ,..|Continuous train...........+ O°2)SeCs«). 3.0c.ceeeam 12 0 30...;=3rd mag. ...... +e+.+.(Colourless ...\Continuous train.........++ O°2 SEC. secreroevees 23/11 45 ......=3rd mag. ..... Fgee0% Colourless .../Continuous train............ O-lesec......c0ere ae Aug. 5/10 32 p.m. |Bright........... conan Red. shisceiesses Wath, train ......scctieestes «neal euneeeeeeretone. ete 10 43 ...... DMA eaaves awe tasoe ess |senaearpossst arias Faint train .........scccsecses Rapid... 022205. «2 GTO RAS ihes news| MOLCON cc. ssidoetuerinsicas|armosienthiececanns|acnsensdosnsuiesincesttiogtecesbsctas| eemaetee see te aathen cams LOWSS scene MleheOtss 3, .-cndecesencs| ste vaca cess otences| aoe cavteesesoreasceee Spide ch ulelnwe| Seton Cagis ce erveae 4 1011 5 ...... Wie IGI Seaeecice-occobococd - Pesieedecscassoad| unoceasedevsves «capecdusendses see) ndieaimeeanctmn ers a 1D 9D 7 s2-|MebEOr: ...60.5 Seeweess BCOS-OnCOe Es CNEL HES ECO InDOLOSDEEr conaccrisstcc Jo|- stueRareBeseee eset PO eee seas MeCbeOL sce. svc ctuscesses|sccossascesensssua|soactinrresSensiuoepesaveveet tides] Witeeten neem ntetee am LUG astiod Metepreeeocastesre-r-|oeeeacace ssepsscas lseesiocieauslanesiassesniis< ine elenn| SONaaee ek ee team ML LO ethsas MIGTCOM ncescdetiessoeren|addeaess st atasasie Wathytraim -.s.ecdecscoccsune deen pirere peste sven % | ee IMCREOR. cot ideaseslncenctlacetoaaue das sovbae|seaus ca eas acisaeelzeaoe suds odes See Ree ee ee eee 15| 9 52 ...... Meteor........ Racecar SalacGeleceveus ses asl sdieises sobs aia avin va ore etiee's aceite] Meeteee eee ware V. Observations of Luminous Meteors made at the Observatory, Stone 1851. MIB. 0 LO] vvanaecerapabes hon vessccssescstahesetesisival souinudcecsas oasens| =e sin’. cpi enlace aden ofenmecems enacen Mneemametentten LON. Savecweduepea|seresesecdensacsaen ts ss IBIUC sen esses ITPA, cs secnslsectensene pee nes aeeeenaas aeetaner sone 20/10 3 p.m. |Brighter than a star of the Ist mag. whee eernee medz to Markab. A train as long as twice the distance from « Andro- ‘Slow; visible di ring 4 secs. QO SL Ty ——..- ! In an instant it changed its | course a second time, became as brilliant as at its first ap- _ pearance, fell in a direction | nearly perpendic. to horizon _ and disappeared midway be- |_ bling mass of light. ‘rom < Herculis to } Corone Borealis. Direction or altitude, ————$——— an =. Near ¢ Ursee Majoris, above x Draconis through Polaris to +Cephei. _Iil-defined trem- from y Cygni to a point 2° be- _ low Deneb, it then changed its course and proceeded about 3° in horizontal direction, growing less and less bright, _ till at length scarcely visible. tween Deneb & @ Pegasi. BPPPP PS ese ssrercvessccrernrcccseseseee wee eee i meteors from N. to S. un- Cassiopeia. PEPER Rese recess ensnserseeeeesesevels General remarks. ee rere A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. Place. Near Dreux(Eure & Loire), France Castle Donington Hse -Pacadnna spare Highfield House |A. S. H. Lowe,|Ibid. Esq. OO ny Coneeee Did 0 cvsncsass Ed: rise: Seneae 3 Ibid Eisai piesisnan rece skrnaxuos UD eves eaeecc [Eo apes wos Eide [ Beeston. depdesiRa antes tens anit Observatory, E. J. Lowe, Esq.|Ibid Recreate Sues nae sa DIGS, Seba acaced Gs: cescvohess tena Ubids Ruisicsg Space sta ces Mbidaer Sirius ...........+...|Bluish white . 10 9 ......{Ist mag. ..e..seeee wehive |ieeenedteeeenes 9 FS ee an 3rd mag. ...... an acavcdlecvoeesstees tes aoe Aug. 3)19 27 ......|Gradually dying away)......... wes cvanid and suddenly= Ist BO SDA ec 5c] 200 WA ates sae cena Rca naveesrenacser 10 55 30* |4th mag. ....... aedewsen|teiecs sss paseeras 11 26 ....../4th mag. ....... Cidesetalateaceernees boat 9 57 p.m. [4th mag. ...........-. caf WRITE: .o8s030e 5ILO 16 p.m. f..-..0e0e0 gsnsWemets .++...|Reddish, bril- liant. 7| 9 40 p.m. |2nd mag. ...........08. Blue, very brilliant. 11} From (MMCTE OS renertaraccocss|asececsses Anctince .|Continuous line of light...|1 Se. ......+0s. place, lasted about one minute. Tail or streak, lasted tWO)..ccacesesestscsece stout minutes. seelsaaaic ts dice ceeruees sessecee(Lell and dissipated at 10° alt. INO train’ ..7. ces oaecenes LG BOD poate scan fee Ibid. and B Capric. ae Ursa Major ............06 Passed downwards.|St. Ives, Hunts..|J. King Watts...|Ibid. ow Ursa Major ............06. From N. to S....... Ubi wsesestesepanc LG Gs ee raguesece dec Ibid. BRIBES | cate ds..nsecsnreesee Passed to N. ...... [Lt Beane ee are oe Sap ack) Ibid. ic $ directions, 5 generally|Moon full; atmo-|Haverhill......... Mr. and Mrs. W.|/MS. communicated. towards S., 2 towards N. sphere hazy. Boreham. See diagram, App. No, 7. 218 REPORT-—1852. Sept. 18] 9 52 p.m. |Small ....see-eree seers ALE weette coos |nesenstas hceusocelenserees eerie 19} 9 8 p.m. [Large .....-..ese secee{BIUISH ...cecccc[eceseeceeccececeseneeeeeasooeens 20/10 25 p.m. |Large and brilliant ...|White ......... Beautiful sparks and bright|Slow.......++..+» vaag 21) 9 23 p.m. |Srd mag. .....-.+-eeeee MEG asubso eee Rapid .. i Slow..... 22| 9 35 p.m. |Large and beautiful . Velocity or Appearance and Duration. Brightness i magnitude. Train or sparks. and colour. wweeee |Z WAP « pce cwesnenerene eeveee| APIUUPILEL = cccvsseveses ccc be | MSU MAR. cocccctsccvceeefecscssccsoussocccs 9 27 p.m. |Large and bright...... Very _ bright/Train continuous.........++- and _ white, increased un- til it disap- in brilliant. 2| 7 30 pan. |An ill-defined lumi- Bright white,|.......csssesresesseennseeeeeeess nous patch or band, gradually in- longer diameter,| creased = in slightly-inclined. brightness, then decrea- sed and dis- appeared. eneeee seevee{/NTCCU LOLI soceseneesee aadcclcauwes ceeapysccevelscemetisiogans ones sebasuemssnwece=s| sb ues sale aes violet. Illumination |No explosion, disappeared|About 5 secs «4 more than| suddenly, leaving no half moon,| track, except a whitish tinged with} trace at the upper part blue. of its course. 19/11 Op.m.|Bright meteor, one- fifth full moon, star- Tee Re peared witho explosion. senseetetwomlereseseecsereacere avcleccosecccecsececvenel eeeeee Rapid eooeet err ee pevjecccecccnccspeosccieccvcsccessouesaas see ses * This day an immense meteor was A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 219 ‘Direction or altitude. General remarks. Place. Observer. Reference. - a Seneath Polaris .......... isle through Perseus downward . through Ophiuchus above » . Phrough.Aquila above y through Capric., slanting down Jame as last, slightly curved .. through y Cor. Bor. from un- der Polaris. seeeee Beno ee erate tesa steno ees Selow Virgo to west .....ss.s008 selow Ursa Major to west ‘rom Ursa Major to west ...... assed the whole length of Ursa Major from ‘south to north, eee OO eer and in its progress rendered some of his stars invisible. down about 45° to S.W. Hrom near Polaris, passed Ursa re (see sketch in Appen- alt. 25° to alt. 20°. ll perpendicularly down, ap- }) parently into the sea. eee Cee eeeeeee Peon seeeeeee Oxford. OOP r reer Peery Pee Oe eee ewes rsssceeees Cee ever eeeeeeeret teens Passed S....ececsseee Exploded with a brilliant light. Near windows, also re- ported by Mr. Lowe. In a storm, accom-|Several eecerses Rey. J. Slatter... i MS. communicated to Prof. Powell. Ibid. Ibid. Ibid. Ibid. Ibid. Ibid. ..|[bid. Ibid. vd bvwrtandina dithering tag mia Td hats eantibis. tu Idisiis..ee ..|Gamekeeper a5 To the W. of UrsalIbid...........0048. Td; ; scasaeved...s.. Major. ; a little north of zenithl........... Ga eqats Boake Caleutta ...... ...|Correspondentto Dr. Buist. Farnham,|Mr. G. W. Hewitt Surrey. om. ae to N.N.E., from|Altitudestakenfrom|Rose Hill,Oxford.|Seen by some of Mr. Slatter’s family. places|Several commu- © below Cor. Bor. from near]......ceccceccssseeeeees Rose Hill,Oxford.|Rev. J. Slatter...|Ibid. Polaris. om Lyra down to the west ...|....sssssecseseseees ..../St. Ives, Hunts. JJ. King Watts...|Ibid. RUAN: GOT! .c.svcndecpenec|svacessttsvcseneoeca ....{Garsington, near|Rev. T. Master-|Verbal communica- Oxford. man. tion to Prof. A Powell. GWEESVewssessaciserccedseces Pe POLE Hea Beech cevececcch piney vesees[LDid. .|MS. communicated} to Prof. Powell. Ibid. Ibid. Ibid. Bombay Times, App. No. 4. MS. communicated to Prof. Powell, see App. No. 8. MS. communicated to Prof. Powell, from Rey. J. Slatter. Bombay Times. panied by arush-| near Bombay.| nicated to Dr.| See App. No. 6. ing sound and a Buist. noise as if of a falling mass. Gs we sesstesssseeseese (ose Hill near|Brother of Rey.|MS. communicated Oxford: J. Slatter. to Prof. Powell. 220 REPORT—1852. Appearance and Brightness : Velocity or Date. a. magnitude. and colour. sete: iea Duration. 1851. | h m ' Nov. 4| 5 0 p.m. [Brilliant .........c00cee[escccceseeessenees Fell slowly towards the W.]........ er) in a curve concave to 1 horizon. 10 2:p.m. |Large ....sscsrssseeneee Ee ROE ne Arann | 24/10 15 p.m. [Large ...........ceeeeee Purplish, bril- arya eae'e sve lelatetbiels Ge lee’ liant. 25| 7 G a.m. [2nd mag..........00000 Pale yellow jane|¢sssb ens corpesensceewahoneeusens About 1 sec. «..... 1852. Mar. 12] 9 28°...... rial setddeacsanchases WSS! Sah wicins| pesciean cen icemeiiesen asvcecaeacinnt Slow: diecstes.tec¥eced 10) Sire. LAR BO eosne aster senioaces White, bril-|Sparkling, and _ stopped|Slow.......... Neteaee liant twice in its progress. April 20/11 25 ...... Ist Mag. ......ceccsseee|sossecenaeeccecees|ecerteneeeneeesccsnensasseoessees|seceeeaneeees dol sdeoeeet Till 35 oe. Atl MQ. .....secesveecclesccnsveetececcacelenscescesassesensseeeseeesesceeselacsuasenege seeeeeebeooes % Capella % Capella T B + B A Auroral beam. % aloes aathie B C Course of meteor. Pst i! rt Mea Lie vulbd ss repeat me A Cc . TRUBS? £../4ER mega lanes adescesees)anasers sveesercer|sveseessoasecs cP assassevesensonceasea 12 25 ..000. == JUPILEL. eens soceesacs White ....00... Fine sparks ¢ . May 14/10 33 30° |=Vega .....+...00e00- White ......... Fine sparks % w seaees About July 12) 9 59 p.m.|Apparent diameter|Very _ bright,/Noted shape Moved towards the} | G.T. little inferior to full| ruddy co- N. very rapidly.) ‘ moon. lour. tail pointing to south. | Duration of visi- bility about 2 secs) il 13/10 0 p.m. |Larger than 2. As it/Bright orange-|Disappeared without sepa-|About 2 secs. ...+. (London fell brilliancy in-| red, chan-| ration; no explosion. time.) creased; then seem- gingto near- | ed to decrease and} lywhite,and ! again toincreasetill] then red disappearance. again. : Teil 29) 9 45 p.m. |=2nd mag., but gra-|Bluish white .|,...scsesccssecssseeeereeceresneeleeeenes sabteeveccecevs of dually decreased till] . =5th. Aug. 3] 9 15 p.m. |At first like a smalll..... snecesbuceses For about 15° gradually|Train ...sesscsseseed | (G.m.T.) | star, intensely bright increased in magnitude, | became brilliant, though white (as if inflamed), =2 diam. of 9 when brightest, and continued through about 30°, when it suddenly resumed its first appearance (as if burnt out) and continued onward some distance further. A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 221 ‘Direction or altitude. General remarks. Place. Observer. Reference. _—— | a et | Appeared first below and a little/Perhaps the same|St. John’s Lodge,|Miss G. R. Smyth|MS. communicated to the right of the moon, in} as one seen in| Stone, near to Prof. Powell. S.E.alt. Estimatedabout 35°.) Nottingham;vide| Aylesbury. Mr.Lowe’s Catal. From Polaris running northward].........ccccsssssseeees St. Ives, Hunts,.,|J. King Watts...|Ibid. Left of Ursa Major tc north ...)..ccecccesccseessseeeees Tid. ...sceveeseves RAW eouseseec, soe. Lbids Perpendicular down ............ Below Leo Minor .|/Huggate ......... Rey. T. Rankin .|Ibid. From the Pleiades to the north]........s......sseceeees St. Ives, Hunts. .|J. King Watts...|Ibid From Polaris to the N.W.......|.. migdilewseddeasneenevee Tbidesv......ceasee TG. *eosteceresssee.| EDIO. From Ursa Major to 2° N. of|During Aurora ...|Rose Hill, nearjRey. J. Slatter...|Ibid. | Mars. Oxford. [From Capella .........0+...0000.. [The meteor f fell downwards till apparently near the auroral haze, and then started aside into a wavy course, as if repulsed. + followed downwards unin- terruptedly. It was as if ¢ had been repulsed by similar electric force and exhausted it. See figure above. | pm Capella ....c....sssceseseees MDA sais sarceatoa sete EDD ics deisissweet Hey cseceesaccues tee Ibid. From 1° W. of Spica to Crater .|Ibid..........sesce008 TDid ee cv eae. Rds saettsdsaonee Tbid. From Spica to Crater, curvelIbid.............c0000: Heys Pr Seenney pacer: Tdsssenieas ate terse Ibid. curving upwards, intensely incandescent at the endof the curve, Altitude about. 30° above west/Seen at Glasgow,|Dunse, Wm. Stevenson .|Ibid. point of horizon. Helensburgh, Lat. 55° 47/N. Perth, &c. Long. 2° 23’W. ‘Appeared in N.N.W. at alt. 20°|........sscee eneceeee -.(Carlisle. | SeenJJohn Carrick |Communicated to | fell nearly vertically or a little also 90 miles} Moore, Esq. Prof. Powell, | to E, W. of Carlisle. through Mr. Fa- raday. See App. No. 9. Path perpendicular to a line, .........ccsseecceeeees Victoria Park, |W. R. Birt, Esq.|MS. communicated joining Polaris and the Upper London. to Prof. Powell. Pointer ; greater part of course’ above that line, and thence _ down to horizon. m a Lyre to past B Scor-|About 2 secs., velo-|Oxford.......2.... Mr. G. A. Row-|Ibid. pionis. city uniform. ell. 222 REPORT—1852. Velocity or Appearance and Brightness Duration. pour. magnitude. and colour. Train or sparks. —— hm 4 i] so OD e rene | Se LSb WOARi kk wixssncde| reveals cha gunineds (Cds esedegleswesegeasiees teeeeevas[envaneecesenessenenereed 8] 9 40 p.m. [Small ....0.0c....se¢se9| WHILE cevecoses vacate vicsej. 2k. csanstist a Reine te 9 42 p.m. SyAll a veatscbscserdvpa set WHACC) Si ss vaste lscacan Set eeneeeeeees eeereeceeeses Rapid sees eeceseseree 9] From — [80 shooting stars ...|.sscscsssssesreeeslecnsnssrsenestteeerecessstenserss|eeeeesnteanannaneneneagal BO DS: wees 1 brilliant .,........00)...eeeeeeeseeeeeee(Path illuminated for 30 or , 40 secs. 10 21 p.m. |Large ...... rapraena vas| VUueOte ters sres}anacs=sseacenasetesasn sosocenscs{ APLC: sccvenceeesverae 10 30 p.m. |) Magnitudes full 1st|Mostly stellar |Almost all left a luminous|Velocity as usuall a down to 5th or 6th. train. noticed. Duration No. counted in 1’ to 5” or 6”, 10 40 p.m.!j northern sky.. 9 » = Ad os No. counted in 11 5pm. southern sky.. 13 ll a ee northern sky.. 12 4 ee he oy No. counted in ll 45 p.m southern sky.. 14 No. counted in 7 eae northern sky.. 12} - y Night ld i No. counted in cloudy. 0 35 am.*|{ Southern sky.. 18 —i78 9 20 pam. (Large .......c..0-sss0e| Whitish red...|Drilliant .....ssdaspasasvonvaal us sdGriseeesivaalltadll 11 12 pm. ae counted in 9 22 p.m. [Small crcreesscseveseve] WHItE 2. cccvecloccesccescccsessconneseesseeceese(S1OWs ss sascssecenecneh 9 47 p.m. [Large ..........sseccee-|Reddish ...... Many brilliant ‘sparks, and|slow. endl a train similar to arocket, h thus ; | n+ t Slee ee | 9 53 p.m. [Small ........... seve WIG i. Se nm ac ow wee Sa Bl WeiS% acess 9 59 p.m. |Small ....... arias sobee White ... + ~~ + Sa, SNR A eae ARs Cee ' 10 1 p.m. |Large ....... ape eenonanc| NVIIEE Sips ecu Brilliant: ..0.c0sssesessoestose{AlaWWoee veide db te eed ae 10 1 p.m,*|Large ......... seccreres| WIIG ccseseee.| Brilliant seesssseeeesesecerses|SlOWsssssesereeeeeenes * On this evening,|which was ver,y clear, many other meteojrs were visible be sides the above, chieflly in the field b|etween Polaris, Ursa Majo\r and Lyra, five of six being visible at thje same time, gioing in various directions. Many the whole even-|None particu-|........... FidecatversveedevvesceleoadaucsamWersdveneiaa ing, 17 in 20 mins.| larly _ bril- | (from 105 45™, to) liant. | 11) 5™,) A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. Direction or altitude. General remarks. From near Cassiopeia towards| Velocity moderate, | N.N.E. Through 14°. 2 secs. We Mickacescsececscesss Reon carcerce From Ursa Minor . MURR E fAL csonasasssnaccs|Gdetccescccpis vedecec ane Poe eeeeC eee ee ees Creer ee eee rere ere ree Nearly all moved to S. or\The meteors were | S.S.W. In northern sky a| distributed over _ few moved to N.W. and E. all parts of the sky; the place from which they proceeded _ap- peared to be in the northern sky, somewhere be- tween Perseus and the Pole, but this is uncertain. same time, thus : “at each 45°. facing S.E. Place. 223 Observer. Reference. —~—-——,. — Mr. G. A. Rowell/MS. communicated to Prof. Powell. St. Ives, Hunt-|J. King Watts,|Ibid. ingdonshire. Esq. TBId seer iteceseces es Lat eceakbwecvencse Ibid eeacerees St. Ives, Hunt- ingdonshire. Diunse: .cssevestes Il from E. to W. Downwards|From a window|Oxford crossed each other’s path, and both shining at the seer eeennene Esq., and Mrs.) 11. W. W. Bore- ham. J. King Watts,|MS. communicated| Esq. to Prof. Powell. ‘Wm. Stevenson |Ibid. (Esq. OO e eH eee E DEO b er eeesenereresseneseceee From « Cephei to St. Ives, Hunt- J. King Watts, Tbid. the S., then be- ingdonshire, came stationary several seconds and threw o j some largesparks before it expired. From Ursa Major. |Ibid....... dane Sanins Tae. veewes RP hee Ibid. MTT eset iv cccupssissesssoscene From a@ Lyre |Ibids............60 | Bihepaneettenae ays Ibid. ES through Cygnus to zenith. SI ne ee From zenith to W. |Tbid............0.6 1G Bee ene »...|Lbid. et From Ursa Major|Ibid.,,...,.......+. LG Ee aac Poe Ibid. downwards. | ch manatees To Ursa Major ,../Ibid,.....,......068 Tides i siiecessces ,...(Lbid Dee ivcccdvenscee Peete ees eeneeeenes From Cygnus*. * * These two meteors Mr. G. A. Rowell|\Communicated to Prof. Powell. 224 Date. 1852. Aug. 10 Hour. hm From 9 57 to 10 57 From 10 0 to ui 0 9 2p.m. 9 8 p.m. 9 18 p.m. 9 27 p.m. 9 27 30° 9 28 p.m. Nearly as large as 1st}Commenced Appearance and REPORT—1852. Brightness Train or sparks, Velocity or magnitude. and colour. Duration. 23 shooting stars ...|.. awecltaeekes aeiees Se ge aceh oeheah vailsdieasts Jaca laladalaes Manns, ae Numerous ; one large].........e0e..0e0 With long horizontal train|..... REPEC CEOS. Star. POCA EA dyes csosensusee| WiEte, NCTCH-|.x. 0c sedesccssevcenste seeeeeseeee(Obliquely — across Between 2nd and 3rd)...... iieecver ls a mag. 2nd mag.......+ e+seee-(Bluish-white Small; Srd mag.....ocleccsersescccsveres Between 2nd and 3rd).......sseee.seeee mag. mag. star, sed rapidly in brilliancy un- til its extinc- tion. with consi- derable bril- lianey,which graduallydi-) minished as it proceed- ed, as if it were a long narrow cone of light, the base being first illumi- nated with great bril- liancy, and the apex ve- ry dim, as under. <2 SS ee Colour _ bril- liant white, with silver greyish tinge. passed along. vanished. eee teem e rere eee e ee ee en aeneee Cassiopeia, about) half a degree N. of y. Obliquely towards the horizon, a lit- tle to E of y Pe- gasi: Slight scintillations as it|Shot from midway between Cassio- peia and Ursa) Major, towards, a Urse Majoris, where it became extinguished. | rateits Pia Meeks ca ceiceevinacescatee From Cassiopeia td B Pegasi. ‘Slight train, which quickly|From Cassiopeia te : wards a Ursa Majoris, nearly) parallel to thé course of the stal seen by Mr. Hard) ing ; From Cassiopeia to wards Ursa Ma jor across f Cas) siopeiz. | 4 A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 225 Observer. Reference. W. W. Boreham,|MS. See Appendix, Esq. No. 11. Correspondent to|Ibid. Derby Mercury W. R. Birt, Esq.|Ibid. W. R. Birt, Esq.,|Ibid. and J. Hard- ing. J. Harding, Esq.|Ibid. REPORT—1852. Appearance and Brightness Velocity or Train or sparks. Date. Hour. magnitude. and colour. Duration. | 1852. | h m Aug 10) 9 34 p.m. |Small «.....+0-....s00s Bright ...00000+|,ccscssssesecessosocees soeeceees From below 6 & Ursz Minoris f Ursee Majoris Q 37 PM. |-cecsesereccrseseseneeeserslecescencnees sanblal ese O ese sanaheabaanisanessnaneane From Algz obliq ly toward the hi rizon. 15| 9 5 p.m. |Small, brilliamt ......)......sssssseeeeeeleeeeeeeeee mateensdeasaee viscutuelauaeeesseacedsssehee q OSB eens Small, globular ...... Bright bluish-|...........sseesecseeeeeseene assc| eeodesteeees becca white. { Immediate- |Very similar .........|... eeeceeceeres Sclanseneen ss sdvadscesceucseaceuswel tenteannarsse< steam : ly after last. Ln | eee Light, =2nd mag....|.......sesseeseses|ee Gecaceccadswadescdsasecssscuadsltgteeesnt ss ceemenamm ‘ 22) 7 44 p.m. |Nearly=half moon...|Brilliant clearLeft a train in its path .,.|Slow; several se- white light. conds. APPENDIX, Containing original details of various observations of Meteors communicated by the respective observers to Prof. Powell. ° No. 1.—It may be important for comparison to mention that in the Phil. Mag., Jan. 1839, will be found observations of 54 shooting stars, seen in the night of Noy. 12-13, 1838, at 109 York Street, Whitechapel, by W. R. Birt, Esq. No. 2.—Further particulars of the Meteor shower, April 19-20, 1851. (See last Report, App., Nos. 23, 24, 25, 29.) “ Meteors.—We have been favoured with the following from Madras on the subject of the shower of meteors visible all over India on the 19th or 20th of April. By a blunder of our own we mistook the Bombay date, and made it Saturday the 19th, when it ought to been Sunday the 20th; and on this night accordingly the shower was seen here, at Poona, and at Cawnpore. | With all these coincidences we came to the conclusion that our Kolapore — correspondent, who gave an account of them, had also mistaken-the date, and that there had been one shower only. As he makes no sign of recantation, A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 227 Direction or altitude. General remarks. Place. Observer. Reference. en re SS ae fe pene adn Victoria Park,|/W. R. Birt, Esq. |See Appendix, No. London. 10. NE gt RSs dsiSdiacs a dois v's se vvigsaad|spansbomeld gain. dblite de sore] LUA as bana canes cht sty ienteakpe Qe axen(LDIG hove 6 Cassiopeize to S.E. for|.......c...seescseeeeees POIs cc ee eee scenets 1s eet bie fateh ot Ibid. No. 12. above 3°. ugh Pegasus’ square ......|..sseseeesseeess saiSaeye Ibid .....+...4+ spades Jcpesevecceaass Ibid. °N. of B Cassiopeize towards|..........cs00sseesesen bide cede ieee Ci Bs Ee psec Ibid. Pole. m W. to E. with a slight]...............:c0see0e St. Ives, Hunt-/J. King Watts,|MS. Letter. curve, from near a Lyre to ingdonshire. Esq. beyond «@ Persei. we now come to the conclusion that there were two showers on two suc- cessive nights, bearing a very close resemblance to each other. The following description is one of the most copious and clear that we have met with; it is from the pen of one of the oldest and ablest of our observers in India:— *¢On the evening of Saturday the 19th of April, I was sitting in a _verandah of the Government House at Madras, facing to the eastward, from about 3 past 8 to Z past 10. From the height of the verandah I could see _ the sky to about an altitude of 60° or 65°, and about one-fourth of the horizon _ between north-east and south-east. During the period above stated I counted not less than forty meteors, of different magnitudes and brightness. The flight of the whole was from north and north-east to south and south-west. Some _ of them commenced their flight at a point of the heavens invisible to my eye, _ whilst others came into sight whilst on their career, from my left-hand. Some burned out (if I may use the expression) whilst visible, and others disap- peared whilst yet burning to my right-hand. I heard no explosions, though some of the largest left a bright streak or tail, the trace of which remained _ for several minutes. The greater part of the time it was brilliant moonlight, _ Which detracted greatly from the effect of the meteors. Me No. 3. (Continued from the same).—*‘ During the period between the &.- Q2 228 REPORT—1852. 29th of April, 1851, and the 6th of May the atmosphere at Madras was com- pletely overcast with dense clouds. On the night of the 2nd of May (Friday), at 10 o’clock, there was every symptom of the subsequent gale. At the hour I state, I observed in the south-east quarter a very extensive circular illumination of the clouds, which continued for above a minute. The space in the clouds so lighted up might, I estimated, be about 10° in diameter, but owing to the dense state of the atmosphere and the lowness of the clouds, I saw nothing of the meteor, which doubtless covered the circular illumination. I infer that the meteor was flying towards me, that is, from south-east to north-west, because the shape of the illumination in the clouds did not vary. “¢QOn the night of the 22nd of this month, I was sitting, as is my wont, under an awning on the terrace of my bungalow at Ennore (11 miles north of Madras): I could see in altitude about 75°. About 3 past 10 o’clock, a very brilliant and large meteor came within the range of my sight, and fell apparently perpendicularly in the sea (Bay of Bengal). From the moment it became visible to me it rather increased into size and brilliancy than other- wise, and was in full blaze when it disappeared behind the sand-hills in front of my bungalow, which is not above a quarter of a mile from the sea-shore. The colour of this meteor, which seemed to be as large as an 84lb. shot (qu.), was bright purple and green mingled, and it left a luminous tail or streak, which did not wholly disappear for about two minutes. “« Last night (the 23rd) I saw another meteor in the same quarter, but neither of the dimensions nor brilliancy of that of the preceding night. The flight was from north-west to south-east, and it burned out before it had got within 10° of the horizon.—Ennore, 24th of May, 1851. “Our correspondent mentions.a very brilliant meteor seen from Madras some months since before sunset; it swept clean across the sky, and was so light and of such magnitude that it caused a glare over the landscape even at this early hour. This is the third meteor within the year that has been visible in daylight in India; that seen to explode on the 30th of November, 1850, near Bissunpore at 3 p.M.,—the stone was afterwards picked up ;—-and that seen near Beerbhoom at 9 p.M. on the 8th of January, 1851.” [See last Re- port. ]|—Bombay Times, June 4, 1851. No. 4.—‘ A correspondent of the Bengal Hurkaru, subscribing himself ‘W. M.,’ gives the following interesting account of a meteor which he had ob- served on the night of the 19th of September :— «<¢ A splendid meteor burst over Calcutta last night about 11 P.m., and I send this notice to you that it may serve as a record of the event. On the 13th, 14th, and 15th, the atmosphere was dry and its general movement from south-west, the lower clouds also moved from south to west, little wind and occasionally sultry and oppressive. On the 16th and 17th a storm or squall brewed in the south-east during the afternoon, but did not visit us. On the 18th of September the clouds and atmosphere during the forenoon moved from south-west ; the weather dry and close. Between 3 and 5 p.M. nimbus clouds passed over quietly from north-west to east, with scarcely a breath of air. After 5 p.M. the aspect of the sky was again dry. The chirping of the crickets was unusually loud, and the weather close and sultry. About 11 p.m. the sky was © clear, but the stars were not brilliant, and there was no wind, when a most splendid meteor lighted up in zenith or a little north of it, and shot down half-way to south a little west, illuminating the landscape as if the full or half-moon had suddenly appeared on high. The meteor was a bright ball of . A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 229 light appearing to be of a size equal to one-fifth the area of the full moon: it was star-shaped, its light brilliant with a faint tinge of blue, but its light re- flected from surrounding objects had a green tinge even in the sky ; and in its progress there was a curdling appearance in the sky, about ten or fifteen degrees in advance of it, as if cirrus or fleecy clouds, very gauzy and thin, were retreating from it and crowding on each other, or more like a very thin and watery solution of white paint brushed over a smooth and polished surface and then invaded by the finger. The white particles fly from the finger with the repelled liquid, and form a white fleecy circle at a little distance all. round it. The meteor endured as long as a person would require to take five or six steps at a quick march and disappeared at once, from perfect brightness to nothing, leaving no apparent track where it was extinguished : but in the upper part of its course, a little south of zenith, there was a milky or phos- phorescent line, its thickness that of the little finger, and tapering towards the south ; and between its southern point and the spot where the meteor vanished, a clear space of some degrees without any evidence of a track. There was no appearance of an explosion, nor did I hear any sound. I am not quite certain of the hour, but I think the church clocks were chiming eleven a few minutes after the meteor disappeared. Shortly after a light southerly air sprung up, and during the night the temperature was low, approaching to cold.’”—Bombay Times, Oct. 3, 1851. No. 5.—“ On the Ist of June last, about 83 p.m., while there were clouds around, cirrostratus overhead, and moderatesouth-east wind blowing,a splendid meteor shot-from zenith towards south: it gave a light like that of the moon when it is four days old, and turned to a green star just before it disappeared. This meteor was preceded by four days of dry and sultry weather.”—Jbid. No. 6.—“ Some singular phzenomena occurred during the thunder-storm of Thursday evening, Sept. 25, 1851, which seem well-worthy of record. Exactly at a quarter past ten, when the thunder was at its loudest, the inha- bitants of the northern end of the Fort were alarmed with the sound as if of a large mass of something rushing violently through the air, the noise resembling that of a huge cannon-shot passing close by ; and immediately » afterwards a tremendous crash was heard, as if the mass had impinged on the ground or penetrated some of the buildings; nothing however could yester- day morning be discovered in the neighbourhood. The whole closely re- sembled what is mentioned as having occurred in Ross-shire in August 1849, when a huge mass of ice was found to have fallen. The rain was at this time falling so furiously, the night was so dark in the intervals between the flashes of lightning, and these last so bright and frequent, that a meteor of any size might have “swept unheeded by;” yet appearances look very much as if something of this sort had fallen, and we should recommend observers | to be on the outlook for the corpus delictimore than likely at the same time to have dropped into the sea. A tumbler half-full of water, on the side- - board of a house near the Mint, fell in two about seven in the evening, im- mediately after a vivid flash of lightning! We have it now before us; it is cut almost as clean asunder as if cloven with a knife. The storm abated somewhat after eleven, having apparently gone round to the west and south- west : half an hour after midnight it again got round to east, and several loud peals of thunder were heard; the lightning throughout was almost continued. Shortly after one all was tranquil again."— Bombay Times, Sept. 27. “ The Meteor.—The writer of the following most interesting notice has our grateful thanks ; we trust to hear further of the matter from the lighthouse, 230 REPORT—1852. or those on board the outer light-vessel. We have no doubt whatever that this was a meteor or fire-ball of large dimensions which has fallen into the sea :— ‘It may be of interest to you, with reference to the notice in to-day’s paper of the storm on the night betwixt Thursday and Friday, to know that I was last evening informed by a seafaring friend of mine, who was, at the time the Times describes the rushing sound to have been heard, sitting on the deck of a vessel in harbour watching the storm, that he saw what appeared to be an immense mass or ball of electric fluid fall perpendicularly (as it were) into the sea, apparently near the outer light-vessel: the persons in charge of this craft may probably be able to afford further information.’ ”—Zbid. Sept. 29. “Some further particulars of the fall of the meteor which occurred during the thunder-storm of Thursday evening noticed in our two last issues, have since then been received. The mighty rushing sound and violent concussion perceived by hundreds of persons in the Fort, was so in exactly the same manner in Colaba, a mile to the southward,—at Ambrolie, two and a half miles + to the north-west,—as it was in the Roadstead, a mile to the eastward. All the parties between these two extremes of nearly four miles give exactly the same account of the matter. The sound was said to proceed from the northward as of that of a body passing right over head towards the south, and striking the ground at no great distance. As these phenomena are spoken of by all parties as nearly identical, the meteor must have passed when at its nearest at a di- stance of ten or twelve miles at least. We want more information on the sub- jeet; the smallest contributions will be acceptable: only one party who has communicated with us actually saw it rush through the air, and observed it fall near the outer light-ship.’—Jdzd. Sept. 30. “ The Meteor of last Thursday.—The following notice of the meteor of Thursday last, Sept. 25, closely corresponds with what has already reached us : had our correspondent been able to yive us anything like an exact idea of the interval which elapsed betwixt the fire-ball being seen and the sound being heard, we might have formed an estimate of the distance of the falling body, if the hissing spoken of was in reality the same as the rushing through the air described by other observers. We shall be happy to receive the further communication our correspondent promises us. ‘ My wife and I had been watching the lightning for some time at the door of our bungalow, but feel- ing very much fatigued, being an invalid, I retired to the sofa, and had scarcely done so when my wife called out that she saw a ball of fire fall into the sea in the vicinity of the outer light-ship. The heavens appeared to open at one spot, from which it descended. This took place between the hours of ten and eleven-p.m. Neither of us noticed at that time any peculiar noise, but at a later hour I said, Listen to the conflict going on amongst the elements: they seemed hissing one another for some moments. 1 recollect many years since, when residing at Sidmouth, on the coast of Devon, during a violent storm, a large ball of fire fell into the sea, illuminating the whole re- gion; but in those years little or no notice was taken of these things.’ ”— Ibid. Oct. 2. No. 7.—Meteors seen by Mr. and Mrs. W. W. Boreham, Aug. 11, 1851, from 10 to 11 o'clock. Right ascension of zenith 19 20™ to 20" 20™, t a a 231 . a 7 a we”: a) “aa Ay sa 3 _-ouny po07r104 A Soe Me paewe Se. ete te cnt 4 > 3 be ; 5 = “110 mi - —“aifol! 6 ese we A Dn sie of sf : 41 Sage oS wae 3 pe A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. No. 8.—Diagrain of Mr. Hewitt’s meteor, Sept. 20, 1851. 232 REPORT—1852. No. 9.—Extract of a note from John Carrick Moore, Esq., Corswall, Stranraer, N.B. Addressed to Mr. Faraday. “On the evening of Tuesday, the 13th of July, 1852, I happened to observe a very brilliant meteor. I was walking on the bridge of Carlisle when it oc- curred. It resembled a large star, but certainly bigger than Jupiter, which was shining bright at the time. It was about N.W. or perhaps N.N.W., and seemed to fall vertically, or with a very slight inclination to the E. I guess the altitude when it first appeared to have been about 20° above the horizon. [I am aware that persons not in the habit of using instruments generally ex- aggerate altitudes; but still I do not think it could have been less.] The co- lour was a bright orange-red ; as it fell, the brilliancy increased ; it became nearly white, and then again a very bright red, and disappeared without di- viding. The night was still, there were no clouds, and not the slightest sound was perceptible. I do not think it could have been two seconds visible. It had scarcely disappeared, when the clock of Carlisle, set to railway, that is London time, struck 10. “J would mention a circumstance, which I thought I noticed, but in which, as the time was so short, I may be deceived. The meteor appeared after the brilliancy increased, suddenly to become dim, and then again to shine out in its greatest brightness, which was at the moment of its disappearance. It seemed so near, that I tried to mark the spot where it fell. Mr. Hyslop, the clergyman of Kirkcolm, tells me he also saw it on the shore of Loch Ryan, about 90 miles as the crow flies to the west; he expected it also to fall near him. Mr. H. tells me it seemed to him to fall with a considerable slope to the east. He did not observe the dimness after the first increase of brilliancy, which I have mentioned, and of which I feel rather confident ; the more so, that I did not expect it, and never heard of such being observed before.” No. 10.—Extract of a letter to Prof. Powell from W. R. Birt, Esq. “11a Wellington Street, Victoria Park, London, Aug. 11, 1852. “My dear Sir,—I have the honour to transmit to you the enclosed obser- vations of luminous meteors witnessed by myself and a friend, Mr. J. Hard- ing, last evening in the Victoria Park. The two classes of shooting stars are very apparent, viz. those stars that nerease in brilliancy during their progress, and those that decrease as they proceed. The first star seen by myself, at 94 9™ p.m., is an instance of the first class, and that seen by Mr. Harding, at 95 28™ p.m., is a fine instance of the second. The description by Mr. Harding appears to be very accurate: I regret I did not catch it, but the figure given well describes the appearance presented by the meteor seen on the evening of July 29th, an account of which I forwarded you. The paths of the whole of the stars now sent, if prolonged, meet in the constellation Camelopardalis, and may be regarded as confirmatory of the point of divergence being in this constellation at this period of the year....... The same feature which I noticed three years since was well brought out last evening, viz. the retrograde move- ment of the meteors towards the southern and eastern part of the heavens, and the direct movement of those in the northern and western,—confirmatory of the idea that the real movements of the meteors are of a planetary nature and opposed to the motion of the earth in its orbit, unless they should be com- paratively at rest as the earth passes through the group. ‘“‘T have the honour to be, my dear Sir, “ Yours very respectfully, “ Rev. Professor Powell.” “W. R. Birt.” A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 233 No. 11.—Letter from Mr. W. W. Boreham to Prof. Powell, with diagrams of meteors. a “ Haverhill, Aug. 13, 1852. “ Dear Sir,—I enclose three diagrams of the approximate paths of 80 on Aug. 9, and 23 on Aug. 10. . “On the former evening I was assisted by Mrs. Boreham; on the 10th I observed alone, looking westward. “There was one very remarkably brilliant meteor at 10° 58™ on the 9th, the path of which was illuminated for 30 or 40 seconds (marked *). “ Trees interfered with my seeing it perfectly. “T am, dear Sir, yours most truly, “ Rev. Prof. Powell.” “Won. W. BorEHAM.” Fig. 1. North. West. | East. South. Aug. 9, 1852, from 10" 25™ to 10% 55" mean time. Right ascension of zenith 19" 40™ to 204 10", 234 REPORT—1852. Fig. 2. North. South. Aug. 9, 1852, from 10" 55™ to 11" 30™ mean time. Right ascension of zenith 20" 10™ to Ob 45™, No. 12.—Note from W. R. Birt, Esq., to Prof Powell. “‘ Observations of Luminous Meteors seen at 114 Wellington Street, Vic- toria Park, London, by W. R. Birt. 1852, Aug. 15, 9° 5™ p.m.—A very small luminous meteor passed just above ( Cassiopeie towards the south-east, its visible part less than half a de- gree ; it was very brilliant for its size, which was less than a star of the third magnitude. “©1852, Aug. 15, 9" 8™p.m.—A small globular meteor, between second and third magnitude, passed about midway between a Andromedz and (3 Pegasi; it appeared to describe a somewhat curved path, but very slightly so, within and nearly parallel to the sides of the square formed by a, ( and y Pegasi and a Andromede ; its motion was from the line joining a Andromedez and 6 Pe- gasi to that joining a and y Pegasi. “ Immediately afterwards another very similar meteor described a very similar and nearly parallel path about the same distance, east of a Andromede and a Pegasi, as the former star was west of them: both these meteors very closely resembled the falling stars designated b, No, 4 and 5, observed on the A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 235 Fig. 3 North. South. Aug. 10, 1852, from 9» 57™ to 10°57™ mean time. Right ascension of zenith 19" 15™ to ~ 208 15™. 10th of August, 1849 (see Report, 1849, pp. 51, 52). The approximation of the parallelism of their paths clearly indicates them to have been two distinct bodies ; colour a bright bluish white. : « Aug. 15, 9* 10™ p.m.—A bright meteor fully of the second magnitude shot across the Milky Way about half a degree north of (3 Cassiopeiz towards Polaris. “Upon comparing the path of this star with that observed on August 10, ‘9° 2™ p.m. (1852), it will -be found that their paths cross at rather a consider- able angle, the star of August 10 moving from Capella towards Cygnus, ~ which would be slightly erratic from the general direction of movement wit- nessed on that evening. The direction of the star seen this evening at 9" 14™, is considerably at variance with the motion of the other three, indicating that the body was certainly moving (¢. e. with its true motion) in a different di- rection.” No. 13.—Communication from the Rev. W. Read, M.A., to Professor Powell. “ Croydon, Surrey, Aug. 12, 1852. “J have the honour to transmit an account of a singular pheenomenon wit- 236 REPORT—1852. nessed by myself and my family on the morning of the 4th of September, 1850. “JT was then residing at the Vicarage, South Mimms, Middlesex, in a situation peculiarly favourable for astronomical observation. “T had been engaged for several consecutive days in observing the planet Mercury during his approach to the sun; partly to test the accuracy of my power of observation by the calculations of the Nautical Almanack, but chiefly to remark how nearly I could trace the planet in his course to the sun, before he should be wholly lost in his rays. “For this purpose I used the most careful adjustments my instrument was capable of, and continued my observations without noticing anything peculiar. “When, however, on the morning of the 4th of September I was preparing my equatoreal before it was fixed on the planet, I observed, passing through the field of view, in a continuous stream, a great number of luminous bodies ; ‘and I cannot more correctly describe the whole appearance, than by employ- ing the same language which I used when I communicated the circumstance to the Royal Astronomical Society, in the Monthly Notices of Dec. 13, 1850, and Dec. 12th, 1851. “ When I first saw them I was filled with surprise, and endeavoured to ac- count for the strange appearance by supposing that they were bodies floating in the atmosphere, such as the seeds of plants, as we are accustomed to wit- ness them in the open country about this season; but nothing was visible to the naked eye. “ The sky was perfectly cloudless ; and so serene was the atmosphere, that ~ there was not a breath of wind through the day, even so much as to cause any perceptible tremor of the instrument; and I subjected the luminous bodies to examination by all the eye-pieces and coloured glasses that were needful; but they bore every such examination just as the planets Mercury and Venus did, both of which were frequently looked at by me, for the pur- pose of comparison, during the day ; so that it was impossible I could resist the conclusion (much as I was early disposed to hesitate) that they were real celestial bodies moving in an orbit of their own, and far removed beyond the limits of our atmosphere. “ They continued passing, often in inconceivable numbers, from 3 past 9 A.M., when I first saw them, almost without intermission, till about 5 past 3 P.M., when they became fewer, passed at longer intervals, and then finally ceased. “‘ The bodies were all perfectly round, with about the brightness of Venus, as seen in the same field of view with them; and their light was white, or with a slight tinge of blue; and they appeared self-/uminous, as though they did not cross the sun’s disc; yet when seen near him they did not change their shape, or diminish in brightness. “They passed with different velocities, some slowly, and others with great rapidity ; and they were very various in size, some having a diameter, as nearly as I could estimate, about 2”, while others were approaching to 20". ‘ past 3 I saw nothing peculiar, though I waited till 11 p.m. ; but have since been in- formed that at 3 past 11 (it is believed on the same night) a meteor of amazing brilliance and size, and passing in the same direction and about the same al- titude, was observed by Mr. Ballan of Wrotham Park, in the immediate neighbourhood of South Mimms. A CATALOGUE OF OBSERVATIONS OF LUMINOUS METEORS. 237 “T repeated my observations the following morning, and then saw one such single body pass in the same direction as those of the preceding day. “They occupied a tolerably well-defined zone of about 18° in breadth ; and, though with some exceptions, their direction was due east and west. Their motion was perfectly uniform, so far as I was able to follow them with the instrument at liberty; and they were observed continuously by myself and members of my family, accustomed to the use of instruments, both by day and night. «‘ The telescope I employed on this occasion is one of 34 feet focal length, and 23 inches aperture, by Mr. Dollond, of faultless performance and mounted equatoreally by Mr. Jones of Charing Cross, the circles divided by Mr. Rothwell of London, and reading off to 5!'. “IT understand that a similar phenomenon has been witnessed by Mr. Cooper of Markree Castle, County of Sligo, though I have not communicated with that gentleman on the subject; but I take the opportunity of subjoining a portion of the contents of a letter to me from Charles B. Chalmers, Esq., F.R.A.S., now residing at Jugon, Cotes du Nord, France. “‘ He thus writes :—‘ About the latter end of the year 1849, I witnessed a phenomenon similar to that which you saw in September 1850, in every re- spect, excepting that I thought some of the bodies were elongated, though certainly the majority were globular; and their brightness appeared to me about equal to that of Venus, as seen at the same time. “‘ 30. Are children exposed, and from what causes, whether superstition, want of subsistence or other difficulties, or from deformity, general infirmity, or other causes of aversion ? 31. What is the practice as to dressing and cradling children, and are there any circumstances connected with it calculated to modify their form; for example, to compress the forehead, as amongst the western Americans; to flatten the occiput, as amongst most Americans, by the flat straight board to which the child is attached ; to occasion the lateral distortion of the head, 248 : REPORT—1852. . by allowing it to remain too long in one position on the hand of the nurse, as amongst the inhabitants of the South Seas? 32. Are there any methodsadopted, by which other parts of the body may be affected, such as the turning in of the toes, as amongst the North Ameri- cans; the modification of the whole foot, as amongst the Chinese? 33. How are the children educated, what are they taught, and are any methods adopted to modify their character, such as to implant courage, ‘impatience of control, endurance of pain and privation, or, on the contrary, submission, and to what authorities, cowardice, artifice ? 34. Is there anything remarkable amongst the sports and amusements of children, or in their infantile songs or tales? : 35. At what age does puberty take place? 36.. What is the ordinary size of families, and are there any large ones ? 37. Are births of more than one child common? What is the proportion of the sexes at birth and among adults ? 38. Are the children easily reared ? 39. Is there any remarkable deficiency or perfection in any of the senses? It is stated, that in some races sight is remarkably keen, both for near and distant. objects. 40. To what age do the females continue to bear children? and for what period are they in the habit of suckling them? 41. What is the menstrual period, and what the time of utero-gestation ? 42. Are there any ceremonies connected with any particular period of life ? 43. Is chastity cultivated, or is it remarkably defective, and are there any classes amongst the people of either sex by whom it is remarkably cultivated, or the reverse, either generally or on particular occasions ? 44, Are there any superstitions connected with this subject ? 45. What are the ceremonies and practices connected with marriage ? 46. Is polygamy permitted and practised, and to what extent ? 47. Is divorce tolerated, or frequent ? 48. How are widows treated ? 49. What is the prevailing food of the people? Is it chiefly animal or vegetable, and whence is it derived in the two kingdoms? Do they trust to what the bounty of nature provides, or have they means of modifying or controlling production, either in the cultivation of vegetables, or the rearing of animals? Describe their modes of cooking, and state the kinds of condi- ment which may be employed. Do they reject any kinds of aliment from scruple, or an idea of uncleanness? Have they in use any kind of fermented or other form of exhilarating liquor, and, if so, how is it obtained? What number of meals do they make? and what is their capacity for temporary or sustained exertion ? 50. Describe the kind of dress worn by the people, and the materials em- ployed in its formation. What are the differences in the usages of the sexes in this respect? Are there special dresses used for great occasions? and, if so, describe these, and their modes of ornament. Does any practice of tat- tooing, piercing, or otherwise modifying the person for the sake of ornament, prevail amongst the people? N.B. Such modifications not to be blended with other modifications used as signs of mourning, &c. 51. Have the people any prevailing characteristic or remarkable modes of amusement, such as dances and games exhibiting agility, strength or skill? 52. Are games of chance known to the people, and is there a strong passion for them ? 53. Do the people appear to be long- or short-lived? If any cases of extreme old age can be ascertained, please to state them. Such cases may hl a ETHNOLOGICAL INQUIRY. 249 sometimes be successfully ascertained by reference to known events, as the previous visits of Europeans to the country. Is there a marked difference between the sexes in respect of longevity ? 54. What is the general treatment of the sick? Are they cared for, or neglected? Are any diseases dreaded as contagious, and how are such treated? Is there any medical treatment adopted? Are there any super- stitious or magical practices connected with the treatment of the sick? What are the most prevailing forms of disease, whence derived, and to what extent ? Is there any endemic affection, such as goitre, pelagra, plica, or the like? With what circumstances, situations, and habits do they appear to be con- nected, and to what are they referred by the people themselves ? 55. Where there are inferior animals associated with man, do they exhibit any corresponding liability to, or exemption from disease ? 56. Do entozoa prevail, and of what kind? 57. What is the method adopted for the disposal of the dead? Is it generally adhered to, or subject to variation ? 58. Are any implements, articles of clothing, or food, deposited with the dead ? : 59. Is there any subsequent visitation of the dead, whether they are disposed of separately, or in conjunction with other bodies ? 60. What is the received idea respecting a future state? Does this bear the character of transmigration, invisible existence about their accustomed haunts, or removal to a distant abode ? Buildings and Monuments. 61. What are the kinds of habitations in use among the people? Are they permanent or fixed? Do they consist of a single apartment, or of several? Are the dwellings collected into villages or towns, or are they scattered, and nearly or quite single? If the former, describe any arrange- ment of them in streets or otherwise which may be employed. 62. Have any monuments been raised by the present inhabitants or their predecessors, and more especially such as relate to religion or war? State their character, materials, and construction. If they are still in use amongst the people, state this object, even if they should be of the simplest construction, and be little more than mounds or tumuli. If these monuments are no longer in use, collect, as far as possible, the ideas and traditions of the natives re- garding them, and, if possible, have them examined by excavation or other- wise, taking care to deface and disturb them as little as possible. 63. In these researches be on the look out for the remains of the skeletons of man or other animals ; and, if discovered, let them be preserved for com- parison with those still in existence. Works of Art. 64. Let works of art, in metal, bone, or other materials, be likewise sought and preserved, and their similarity to, or difference from implements at present in use amongst the people of the district, or elsewhere, be noted. Have they any kind of commerce or exchange of commodities with the people of other tribes or countries, civilized or uncivilized ? and, if so, what are the articles which they give and which they take in exchange? Is this trade or barter in continued or irregular operation, or periodical by means of fairs, stated journeys to or visits from other people ? 65. Name the people and channels of this trade. 66. Is it of long standing, or recent ? 67. Has it undergone changes, when and how? 250 REPORT—1852. 68. When a people display their ingenuity by the extent or variety of their works of art, it will not only be desirable to describe what these are, but also the materials of which they are constructed, the modes in which these ma- terials are obtained, the preparation which they undergo when any is required, and the instruments by which they are wrought, Such particulars will not only throw light on the character and origin of the people, but will, directly or indirectly, influence the commercial relations which may be profitably entered into when commerce alone is looked to. When colonization is con- templated, the facts contained in the replies to these queries will point out the mutual advantages which might be obtained by preserving, instead of annihilating, the aboriginal population. Domestie Animals. Are there any domestic animals in the possession of the people? Of what species are they? Whence do they appear to have been derived, and to what variety do they belong? Have they degenerated or become otherwise modified? To what uses are they applied? Government and Laws. 69. What is the form of government? Does it assume a monarchical or democratic character, or does it rest with the priests ? 70. Are the chiefs, whether of limited or absolute power, elective or hereditary ? 71. Is there any division of clans or casts ? 72. What are the privileges enjoyed by or withheld from these? 73. What care is taken to keep them distinct, and with what effect on the physical and moral character of each ? 74. What laws exist among the people? How are they preserved? Are they generally known, or confided to the memory of achosen set of persons? What are their opinions and regulations in reference to property, and espe- cially the occupation and possession of the soil? Does the practice of hiring labourers exist among them ? 75. Have they any knowledge or tradition of a legislator, to whom the formation of laws is ascribed ? 76. Do they rescind, add to, or modify their laws? and how ? 77. Are they careful in the observance of them? : 78. What are their modes of enforcing obedience, and of proving and punishing delinquency ? 79. How are judges constituted? Do their trials take place at stated periods, and in public? 80. How do they keep prisoners in custody, and treat them? 81. What are the crimes taken cognizance of by the laws? Is there gra- dation or commutation of punishment ? Geography and Statistics. 82. Briefly state the geographical limits and character of the region inha- bited by the people to whom the replies relate. 83. State approximately the number of inhabitants. As this is an im- portant, but very difficult question, it may not be amiss to point out the modes in which the numbers may be ascertained. The people themselves may state their number with more or less accuracy, but it should be known whether they refer to all ranks and ages, or merely comprehend adult males, who may be mustered for war, or other general purpose requiring their combination. In this case state the apparent proportion between adult males and other are ETHNOLOGICAL INQUIRY. 251 members of families. The number of habitations in a particular settlement may be counted, and some idea of the average numbers of a family be given. Where the people inhabit the water-side, the number and dimensions of their craft may be taken, and some idea of the proportion between the number of these and of the individuals belonging to them, may be formed. In drawing conclusions from observations of this kind, it will be necessary to have due regard to the different degrees of density or rarity, in which, from various causes, population may be placed. 84. Has the number of inhabitants sensibly varied, and within what period ? 85. If it have diminished, state the causes; such as sickness, starvation, war, and emigration. When these causes require explanation, please to give it. If the inhabitants are on the increase, is this the result of the easy and favourable circumstances of the people causing an excess of births over deaths, or is it to be assigned to any cause tending to bring accessions from other quarters? State whether such causes are of long standing, or recent. 86. Is the population generally living in a manner to which they have been long accustomed, or have new relations with other people, and consequently new customs and practices, been introduced ? 87. If the people, being uncivilized, have come under the influence of the civilized, state to what people the latter belong, how they are regarded, and what is the kind of influence they are producing*. State the points of their good influence, if any, and those of an opposite character, as the introduction of diseases, vices, wars, want of independence, &c. 88. Is there any tendency to the union of races? how is it exhibited, and to what extent ? Social Relations. 89. What kind of relationship, by written treaty or otherwise, subsists between the nation and other nations, civilized or not? Have they any intercourse by sea with other countries? Do any of them understand any European language? Or are there interpreters, by whom they can commu- nicate with them ? 90. Are they peaceable, or addicted to war? Have they any forms of declaring war, or making peace? What is their mode of warfare, either b sea or land? their weapons and strategy ? What do they do with the slain, and with prisoners? Have they any mode of commemorating victories by monuments, hieroglyphics, or preservation of individual trophies, and of what kind? Have they any national poems, sagas, or traditions respecting their origin and history? Where Europeans have introduced fire-arms, ascertain the modes of warfare which have given place to them. State whatever particulars respecting their origin and history are derived, either from traditions among themselves or from other sources. Religion, Superstitions, Sc. 91. Are the people addicted to religious observances, or generally regard- less of them ? 92. Do they adopt the idea of one great and presiding Spirit, or are they polytheists ? 93. If polytheism exist, what are the names, attributes, and fables connected with their deities, and what are the modes in which devotion is paid to each? * This question will comprise the existence of missions—the success or the want of it from causes connected with missionaries themselves or others. - 252 REPORT—1852. Are any parts of the body held sacred, or the reverse? Do they offer sacri- fices, and are they of an expiatory character, or mere gifts ? 94. Have they any sacred days or periods? fixed or moveable feasts, or religious ceremonies of any kind, or any form of thanksgiving or other observance connected with seasons ? 95. Have they any order of priests, and if so, are they hereditary, elective, or determined by any particular circumstance? 96. Is the religion of the people similar to that of any other people, neigh- bouring or remote? If different, are they widely so, or dependent on par- ticular modifications, and of what kind ? 97. In what light do they regard the religion and deities of neighbouring tribes? 98. Is there any idea of an inferior order of spirits and imaginary beings, —such as ghosts, fairies, brownies, and goblins ; and how are they described ? 99. Have they any notions of magic, witchcraft, or second sight? © 100. What ideas are entertained respecting the heavenly bodies? Have they any distinction of stars, or constellations? and if so, what names do they give them, and what do these names signify ? 101. Are they in any manner observed with reference to the division of the year, and how? : 102. If time is not divided by observations of those bodies, what other mode is adopted? and do observances connected with them rest with the priests or chiefs? 103. When the traveller, by personal acquaintance with the language, or by means of competent assistance from interpreters, can freely converse with the people, it will be desirable that he should form some idea of their amount of intelligence, their tone of mind with regard to social relations, as respects freedom, independence, or subserviency, and their recognition of moral obli- gations, and any other psychological character which observation may detect ; and more especially such as may contribute to an estimation of the probable results of efforts to develope and improve the character. In using this little manual, it should be borne in mind that it is not a mere guide to inquire into those tribes that are threatened with extinction, nor to make out.certain details which are desiderata in our knowledge of the people of any given locality, but is intended to direct inquiry generally respecting the varieties of man. Mean Temperature of the Day and Monthly Fall of Rain at 127 Stations under the Bengal Presidency, from official Registers kept by Medical Officers, for the year 1851. By Cotonet SyYKEs, F.R.S. 3 [Ordered to be printed entire among the Reports. ] Dr. GrorGceE Lames, late Physician-General in Bengal, has been good enough to transmit to me the following analysis of official meteorological returns, made by medical officers of the Bengal Presidency to the Medical Board in Calcutta. They are limited to the returns of mean daily temperature and fall of rain, the extreme difficulty of getting barometers conveyed in safety to distant stations, not one in three sent over reaching its destination in an efficient state, having left the great majority of medical officers without the means of determining the varying pressure of the atmosphere; and with regard to the moisture in — ‘ TEMPERATURE AND RAIN IN BENGAL. 253 the atmosphere and fixing dew-points, although several medical officers kept registers of the dry- and wet-bulb thermometers (there not being any hygro- meters on Daniell’s plan in use), yet the registers appeared so little satisfac- tory, that Dr. Lambe did not think it desirable to include them in the analysis. The daily mean temperature was determined by daily observations from three to six in number; but as these were made during the day and not at all at night, the mean temperature is necessarily higher than the mean of the 24 hours would be. Proper precautions were taken against direct radi- ated or reflected heat, by the thermometers being placed in the hospitals or in the surgeons’ houses, properly shaded and with a northern aspect ; but the errors of construction in the instruments do not appear to have been generally verified ; they are not to be relied upon therefore for absolute results; but as_ the same mode of observation obtains throughout, the different meteorological records have a relative value to each other which makes them acceptable. The records of the pluviometer are more free from objections than those of the other instruments, and they contain some highly interesting results respecting the unequal distribution of rain, and in support of the facts adduced by myself from Western India, and by Mr. Miller from Cumberland, testifying that the rain-fall. becomes a maximum in mountainous districts at a certain height, and then diminishes as the height increases. For the reasons previously assigned, I shall cireumscribe my observations on temperature within narrow limits ; but as the stations are arranged in groups, within certain areas of latitude and longitude, some few facts of interest may be selected. For instance, in the Calcutta group of 15 stations, within lat. 19° 48’ and 25° 42! N. and long. 85° 49' and 89° 14' E., Cuttack, in lat. 20° 28’, has a lower mean daily tempe- rature in January than Balasore, a degree further N.; but in February this is reversed, but reversed again in a marked manner in March, April, May and the remaining months until September, when Cuttack becomes hotter than -Balasore ; but in October it is reversed again. The maximum daily mean temperature in this group is 99° in May at Kishnaghur, lat. 23° 24’, long. 88° 22' E. The next is the Dacca group of 19 stations between the parallels of lat. 20° 8' and 27° 31'N., and long. 90° 17! and 95° 1'E. The same discre- pancies are observed here as in the preceding, of the higher latitude having a higher mean daily temperature than the lower in some months, witness Buri- saul, lat. 22° 35’, temperature in January 66°, while Sylhet, lat. 24° 53/, in the same month is 67°:7 Fahr. The highest daily mean temperature in this group is 88°°6 at Burisaul in May. The next group of 10 stations is in ascending the Ganges from Hazareebaugh, lat. 24° 0', to Darjeeling, lat. 27° 3!, at 7000 feet above the sea*; and from Gyah, long. 85° 3’, to Dinagepore, long. 88° 41’. The highest daily mean temperature is at Gyah in Behar, lat. 24° 48!, viz. 96°°9 in May+. The next is the Benares group of 7 stations, from Mirzapore, lat. 25° 9, to Goruckpore, lat. 26° 46’, and from long. 82° 6! Sultanpore to long. 83° 37! Ghazeepore. The highest mean temperature is 101° in May at Sultanpore, in a higher latitude than any station of the group * Cherrapoonjie and Decca are in the same group, the former at 4500 feet above the sea ; the latter is on the Delta of the Brahmaputra. Their difference of latitude is 1° 33’ 35”; their difference of mean temperature in May is 19°-1, which would give 235 feet to a degree. In October the difference is 13°-7, which gives 329 feet to 1° Fahr. T Darjeeling at 7000 feet, and Sarun on the plains differ 174 miles in latitude; the difference of mean daily temperature in May is 31°1, giving 225 feet for each degree of temperature ; but in December the difference of mean temperatures is only 14%8, giving 473 feet for each degree of temperature. Tirhoot and Darjeeling differ 55 miles in lat. The difference of the mean temperature in May is 30°, giving 233 feet to 1°; the difference in December is 17%-4, giving 102 feet to a degree. ; 254 REPORT—1852. except Goruckpore, and at 1050 feet above the level of the sea. The next group is in the N.W. Provinces, and consists of 18 stations, from lat. 21° 51’ Baitool to lat. 27° 23' Futteghur, and from long. 77° 45' Hoshungabad to long. 81° 54! Allahabad. The highest mean temperature is 103° in May at Myn- poorie, lat. 27° 1', and 100°-1 at Allahabad and Nursingpore, the former in lat. 25° 27' on the confluence of the Ganges and Jumna. The daily mean temperatures run very high in May and June at all the stations in this group. The Agra group, embracing Rajpootana, has 9 stations, but the observations are incomplete. The highest mean daily temperature at Agra, lat. 27° 10', was 96°°1 in June. The Meerut and Delhi group has 13 stations, embra- cing Almorah at 5500 feet, from Budaon, lat..27° 50', to Deyrah, lat. 30° 19’, and from Delhi, long. 77° 13', to Almorah, long. 79° 41'. The highest mean temperature is 104° at Goorgaon, 38 miles south of Delhi, lat. 27° 53’, in June, and at Delhi, lat. 28° 31', the temperature in May is 98°°6. The Umballa group of 11 stations embraces Simla, at 7500 feet, and other hill stations. At Ferozepore, on the Sutlege and Simla, differing 9 miles, in lat. 30° 57! and 31° 6’, the highest mean temperature at both is respectively in June, 97°°5 and 69°:2; the difference of elevation giving 220 feet for each degree of difference of temperature in the month of June; but in the month of January the difference of mean daily temperatures, 40° and 55°-9, gives 397 feet for each degree of temperature. The last group takes us to the Punjab, where there are 25 stations between Mooltan, lat. 30° 10', and Peshawur, lat. 34° 0', and Kohat, long. 71° 26’, to long. 76° 19' Kangra. Lahore in this group is 1180 feet above the sea, and Peshawur 1068; and I presume none of the stations, excepting probably Mooltan, have a lower elevation than these. The returns are defective, but it would appear a very high daily mean temperature exists in somemonths, notwithstanding the comparatively high latitude; Mooltan, lat. 30° 10’, temp. 99°°4; Jehlum, lat. 32°55', temp. 97°; and Mean Meer, at Lahore, lat. 31° 33', temp. 98°°2, allin June. The general results would seem to indicate that the daily mean temperature in the summer months increases with the latitude ; that is to say, that the daily mean temperature in lat: 32° in June, July and August, is greater than in lat. 22°. The rain-fall manifests in a marked manner, as I have formerly had occasion to show, the great discre- pancies in the fall-within very limited areas ; and in the increase in the fall up to certain maximum elevations. In the case of Calcutta and Barrackpore, only 9 miles separate in latitude and 44 in longitude, the fall of rain respectively for 1851 was 64°16 and 42°75, differing 22 inches. Hooghly is 20 miles N. of Calcutta, and differs only 6 miles in longitude, but the fall was only 36 inches, differing from Calcutta 28 inches. Barrackpore is intermediate between Calcutta and Hooghly, and only 13 mile west of the longitude of Barrackpore, but the difference in the rain-fall is 62 inches. All these three places are on the Ganges, on the same level, about 20 feet above the sea. Burdwan, which is 40 miles N. of Calcutta and 28 miles W., had only a fall of 28 inches ; but more remarkable still, Midnapore, 8 miles south of Calcutta and 59 west of it, had only 22°78 inches; while Cuttack, 76 miles south and 13° of longitude west, had 50°17 inches. In the Dacca group, which contains the hill station of Cherraponjie in the Cossya hills, the most extraordinary discrepancies occur. Chittagong, only 13 miles south of the latitude of Calcutta, but 33° to the E., has 86°33 inches of rain, and lying under the same meridian as Cherraponjie, which is 116 miles N. of Chittagong, at an elevation of 4500 feet, it has 524-02 inches of rain less than Cherraponjie, at which station the almost incredible quantity of 610°35 inches fell in 1851; and that this deluge is no mistake of record, independently of the official report which I quote, I have a letter from Professor Oldham in confirmation of the fact, who spent the mon- TEMPERATURE AND RAIN IN BENGAL. 255 soon of 1851 at Cherraponjie, and kept a separate record : 50 feet 10inches depth of water may be said to have fallen chiefly in 7 months, for in November and December there was not a shower ; inJanuary only 3of an inch, in February 3-05 in., and in March 1d inch. The S.W. monsoon would appear to commence in April with 67 in., followed by 115°15 in May, 147-20 in June, 99°40 in July, 103-9 in August, 71:7 in September, and 40°3 in October; so that the vapour from the south passed over Chittagong, and little of it was condensed until it reached Cherraponjie and the Cossya hills. But the discrepancy in the fall in the neighbourhood of Cherraponjie itself is not the least remarkable cir- cumstance. Sylhet, which lies below Cherraponjie 23 miles to the S. of it, and only 7 miles to the W., had only 209-85 in. of rain; the fall at the prox- imate places differing 400°5 in. The greatest fall in any month at Sylhet was 43°35 im May. The explanation of this extraordinary fall at Cherraponjie is in the physical circumstances connected with its location. The station is on the Cossya hills, at 4500 feet above the sea, facing the south; and the vapour from the Bay of Bengal, floating at a height of about 4500 feet, passes over the plains of the Deltas of the Ganges and Brahmapootra, and first impinges upon the Cossya hills, and is immediately condensed by the lower temperature at the hills ; and then comparatively little of the vapour reaches the higher regions, as is the case in the Western Ghauts of India, where the maximum condensa- tion takes place also at about 4500 feet. This is shown at Darjeeling, 1500 feet above Cherraponjie, 134 miles to the N., and 3° of longitude to the W. of Cherraponjie, the fall being only 125-20 in.; and yet rain fell in every month of the year, the maximum fall being 31 in. in June. The rain-tables are not complete for Simla at 7500 feet, but the maximum fall in the mon- soon months was only 17:95 in. in July and 11°65 in August, the most rainy months; so that there can be no question but that the fall does net exceed that at Darjeeling, and we have then the fact that those stations so widely separated in India as Simla, Darjeeling and Dodabetta on the Neilgherries, at about an elevation above the sea of from 7000 to 8400 feet, have about the same amount of rain-fall ; while the lower elevations of 4500 feet in the peninsula of India have the maximum fall, ranging from 300 to 600 inches. It will scarcely be desirable to make further comment upon the rain-tables; but it may be stated generally, that as the latitude is increased, and westing made, from Cal- cutta the mean annual fall appears to decrease, the fall at Ferozepore being as low as 23 in. ; but the discrepancies in the fall in neighbouring localities con- tinue, as is manifest in the case of Goruckpore, lat. 26° 3/, long. 83° 13/, having 61°70 in., Azimghur, 42 miles south and 9 miles east, having only 39°96in. The rain-tables from the Punjab are incomplete. The above meteorological observations suggest to us to be cautious in ge- neralizing from local facts, not less with regard to temperatures and falls of rain, than on the supposed law fixing a fall of one degree of Fahrenheit for a _ certain number of feet of ascent into the atmosphere. 256 REPORT—1852. Abstract of Mean Temperature of the Day and Fall of Rain from Registers kej N.W. Provin a Fi January. February. March. April. May o2 3 _————_-——— & a = Mean Mean Mean Mean Mean ee SoA tempe- _ _ |tempe- _ _ |tempe- ___ |tempe- ___ |tempe- = 5 rature| Rain. | rature | Rain. | rature | Rain. | rature| Rain. | rature 2S 4H of the of the of the of the _| of the Festa day. day. day. day. day. ft. 6 RT Pree (ieee | ine lo: cll clin gall eect | il Calcutta .....-|18'11|22 33° 20°34| 71°2| 0°07| 76°01| 2°41] 85°5| 1°05 88°7| 3°75| 92°9 Barrackpore----| -- 25°4.| 72°5| 0°24) 70°5 | 1°17 85°7| 0°24 go" | 2°79} 95°5] | Hooghly ..---- 26°34) 68°5| 0°95| 68" | 0°65) 804) -. | 85° | 2°10 89° | Jessore «++++: ° 10°30| 64° | 040/72" | oro | 80" | ovo 86° | 3°85] 94° Kishnughur - . : 22'20| 70° | 2°50| 69° | 1°20) 94° -« | 96° | 2°60] 99° Burdwan ..---- «es 52°20] 70°5| 0°30| 76°5 | 110) 83° | 0°30 86° | o'40]| 90° Moorshedabad 76 13°20| 63° | 0°20] 65°5 | 1°65) 79°2| -- 83° | 2°35] 88° Rungpore...--- ai 14°50| 65°3| 1°10 | 68°7 | o'10| 79°8| o*50 82°6| 3°70| 862 Bauliah ...--- - 33°45| 66°3| ++ | 716 | 0°60} 81°3| 0-20 85°9| 0'23| 9o°8 Beerbhoom ° 34°00] 69°5| -- | 7372 0°60} 82°7| 1°16] 86°9| 2°50| 92°2 Bancoora .-.--- - 6°31] 71°9| 0°90] 74° | 0°93 82°4| 110] 89° | 4°22] 95° Balasore ..---- . 58-11] 72°9| 0°50| 74°9 | 0°27 85°83 | 1°20| 87°5| 3°35| 96 Midnapore . 19'25| 69° | 0°26 69° | 0°23) 74° | 1°54) 81°5| 1°74 87° Poorie ....---> : 49°10| 71°6| -- |75°6 | ongo 82° .- | 85° | roo} 88° Cuttack .....- 54°15] 72° | o'10| 78° | o'0g| 82°5| 0°25] 86" 1°66| 94° | \Dacca ...----- 22 23°40| 67°3| 0°69/ 71" | 0°99} 82°5] -- | 84° 4°28 | 88°2 Akyab .....-.- Cay fag ee 76'9| .. | 83° fis. |855% Sandowy ------ 78 81 es ais : 85° | ot50] 83°5 Ramree .----- 65°5 66 fey A ZON 775| ++ | 81 Chittagong 47°30| 67°7 72°9 | r'90| 80°3| .. | 81°7| 2°55] 80°6 Tipperah ....-- 5°40] 69°2| o° 75 714 | 125| 77° | «- | 82°r| 5°50] 83°3 Burisaul ....-- 17° | 66° 72°6 | 2*50| 82°5| .. | 84°8| 3°18] 88°6 Pubna .....--- 70°3| O° or 74° | 1%60| 80°7| .. | 84:2) 2°30] 87°5 Bogra .....--- wae. | 6x" | 0°72| 68:2 | x70] 76° | 1°22) 83°5| 1°20 86°8 Mymensing 24°20] 62° | 0°75 | 64°7 | 3°25| 75°2| 0°50] 77°3| 573° 82'8 Sylhet .......- ae : 50°30| 67°7| 0°30 | 69°6 | 4°50 76°5| 2°15| 77°7|19°35| 81°5 Cherraponjie - -/ 4500 : 43°55| 53°7| 0°75| 55°2 | 3°05| §5°3| 1°30] 67°1|27°60| 69°3 | Gwalparah ae “"|g90 go" | 64°2| 0°70| 6671 | 0°70 76'1| r'05| 77°6 \10°20| 79°3 Gowahuttee 47°10| 6674.) 0°51] 68°3 | c47| 77°5 145 78°9| 5°57| 812 Cachar......-.- 92 47°17| 62°5| -- | 66 ste hla O77 77°7 \t2°11| 81°6 Seebsagur 60° | 0°84| 62°3 | 4°39] 79°5| 1 “06 72'°8| 8°85| 77°6 Tezpore : g2 50°10] 65°2) .- 65°2 | 1°87| 74° | 2°07] 77°3| 427] 79°72 Debroghur 95 1° | 63°6| 0°61] 63°7 | 5°49] 73°2| 2°25) 73°5| 9°43 762 Nowgong A... oeats Ae .. |66°5 | 2°85] 72°4| 2°10] 75°8| 8°55) 79° Dinapore~.... 85 5*10| 63°6| 1°75 | 67°7 | 1° 78°5| 2° 87°8| -. | 96°4 Tirhoot .....- 85 26°15] 61°8| 3°75 | 65°2 | 1°45] 75°7| 0°90 84'2| -- | 919 Dinagepore 88 41°00| 69° | o'80|71" | 0-80 82°5 | 0°30| 8975 | 0°70] 94°5 Purneah ......| -- 87 33°00] 64°5| 2°12) 65°5 | 3°25] 71°5| 1°50 88° | 2°00] 84°5 Darjeeling -..-| 7000 + 188 18°40] 40°9] 3°45|41°7 | 2°40 51°8| 4:00] 55°3| 4°55] 61°9 Sarun --.....- *s 85 29°12] -- 75°5 92°5 =| 93° Monghyr .-...- Hazareebaugh .. Gyah ........ Bhaugulpore .. 6| 86 43°38) 65°5 o'85 68° res 76°5| or20| 8475] «+ | 92°5 85 3°16] 70° | 0°30] 72° r25| 79°8| -- | 91° 8 96°9 } 87 o'00|°66'7| 0°75 | 72°5 | 1°50] 80° | or00 86°5| 0°80] 92°5 Benares ....-- Goruckpore ...-. Azimghur...... Sultanpore .... 83 3°12] 64°3| 2°31] 67°38 | 1°60) 74°5 0°65| 87°3| -- | 963) $3 22°6 | 62'2| 3°60) 65:4 | o'20} 75° | 020 82'g| ot10| 90°8} 83 13°20] 64°3| 3°80| 66'9 | 108] 76° 0°60] 81°9| 0°80} 84°83 | TEMPERATURE AND RAIN IN BENGAL, 257 A y Medical Officers at Civil and Military Stations in Bengal and the for 1851. September. October. November. December. an Mean Mean Mean Mean 3 pe- tempe- tempe- tempe- Rain-fall. rature} Rain. |rature| Rain, |rature| Rain. he of the of the of the is day. day. day. ° in. a in. =, in. in. 1 83°r | 16°25 | 78:5 TREE! Oeics 64°16 84°5 | 10°80 | 74°9 67°3 42°75 82°7| 10°00 | 71°2 62°5 36°00 . 86° | 7°15 | 80 pe 40°30 5 84° | 2°50] 75° | -. | 66° 57°70 5 82° 5°65 | 73° | O60] .. 28°20 5 83° | 710 | 75° | 0°00 | 68° 40°48 7 80" | 3°20 | 79° af 70°6 74°60 I 81°3] 3°30 | 72°2] o17 | .. 31°56 6 82° | 4990 | 7573] ++ | 69°7 32°06 6 | “2 | 2°90 | 7375} =. | 73°7 31°04 5 83° | gt10 | 72" | ors | 55°5 30°79 5 77° || 7°34°| 69° 62° 22°78 7 83° pilown dow|n 76" 72°6 79° | 11°65 75° 50°17 : 81°9 | 12°70 | 75°7 69°5 68°93 83° | 14°09 | 81°5 75°I| 2°52 | 155707 ; 81°3 | 10°90 | 80°7| 1°30 | 74°7] 0°62 178°48 ) 77°2| 10°75 | 72°8| +. | 67°5| o42 |} 86°33 ) 78'4./13°50 | 72-7] .. | 661] .. 95°95 81-8) 21°15 | 756] .. 69°5 94°47 81°6| 5°75 EA MB 66° 39°05 oe 6°00 os .. 51°44 81°7 | 10°70 74° Genet 6723) 109"90 78°4.| 20°40 | 73°G| .. 69° | 045 | 209°85 68°2 | 40°30 | .. ee ae ale 610°35 77°9| 885 | 716] .. 65°38) .. 116"10 80°3| 3°68 | 75-1] 0°38 | 69'x o°50 | 52°74 80'9 | 11°26 | 76*1] 2°00 68°3] 048 | 102°84 79°2| 638 | 71°4] 0°05 | 65°38} or50 85°18 79°4| 3700} 71:2] .. 66°1| 0°30 | 63°49 | 17°73 |) Fs ee do fe 106°95 O'T| 7°00 | 70°6| o-40 | 66° | 2:00] 83-45 815) 3°75 | 71° 62°3 3r 80" | 4°50 | 69 62°2 33°38 85° | 6°50 | 80 73° 46°70 798) 3°75 | 71°7 65° | .. 53°39 55°38} 9°40 | 50°4| ot10 | 4a°8] oro 125°20 80'2| 3°40 | 63° 59°6 80°5] 6°65 | 7o"5}| .. Se 36°66 73°5| O90 | 69°5} O85 | 64°7 32°06 83" | 2°50 | 65°3] on50 | 652 24°65 82° | 7°90 | 72° ++ | 66°5 42°45 816] 3°85 | 73°1 68°3 37°06 80°8 | 11°60 | 7074 63°2 61°70 813] 7°20 | 7173 64°3 39°96 258 REPORT—1852. 3 a January February. March £3 é s 33 as! 2 Mean Mean Mean ae g *& —_|tempe- tempe- tempe- ae 3 8 rature| Rain. | rature Rain. | rature| Rain Be A 4 of the of the of the fer} a day. day. | day ee eens re eee ee eee ey seen seen ee ORAS a fcc aoe cual, wot : Pema ates Bolundshuhur. Ajmere. a sere we eeee we eee eet Mean tempe- rature of the day. August. Rain. September. Mean tempe- rature of the day. ——- ||} —_____, Rain, in. , October. Mean tempe- rature of the day. Rain. O57 2°36 2:95 TEMPERATURE AND RAIN IN BENGAL. November. Mean Rain. in. 0’°00 ool 0°59 o"50 0°20 259 December. Mean tempe- 32°02 38°37 27°81 25°08 82°31 25°76 TABLE. a Fa January. February. March. April. May. o” Py ee ee > ot | 8a 3 = Mean Mean i 23 = ED tempe-|___— {tempe-}_— oe a =I rature | Rain, | rature} Rain. Ee A iS of the of the <> heed day. day. ft. Pas 9 =a Wir i in. a in. ELMIRA ciafe icles] | o = sees sees oe 0°S4 o- I‘o9g Landour ......| -- sien S160 B59 -\5 || 4O'7 1. we Paneeput. Rhotuck ...... Lahore ......--| 1180] 31 35°0 | 74 22°0 | 53°6| 2'40| -. eo. ha -- | 81°3] roo Jullunder ....| .. | 31 19°30175 36°45] 57°4| 3°20] 59°9] 3°42] 69°1| -- | 79°9| 0°20 Hooshearpore ..| .. | 31 31°30|75 57°45] 51° | 6°75] 51°4| 4°75] 7o"2| .- | 81°8| -- =e Kangra........ -» |32 6°10) 76 19°5 | 49°3| 7°25] 57°6] 3°65] 68°7| o'g0] 781] 0°25] 82°5 NOWINICSIE [-rec'scl| oe eras see oe ie oe oe 82°75] .- oe +. {104° Mean Meer ...-| .- | 31 33°10] 74 24°30] 55°8| 0°58] 59°7| 2°47] 71°4| 0°08] 83°5] -- . Nakoda ...... -- |32 7°0|75 30°25] 55°3| 3°28] 61° | 2°17] 71°99] 0°29] 83:4] 0°20 Kurtapore ....| .. | 31 26°40] 75 32°30] 57°2| 2°58| 60°9| 2°40] 70°1| 0°37] 82° | oO°50 Peshawur...... 1068 | 34 075 | 71 38° | 488] 3°24] -- i ie Salar as oe ae “a Kohat .......- »» 133 32°301 71 26°25] 50°5| 3°24] 58°5] 2°02] 67°3| 1°65] 77°7| 1°15] 88° | ovo) Rawulpindee .-| .- | 33 34°40] 73 5°20] 49°8| 3°59| 57°21] 6°08] 55°1| 2°61| 74°2| 2°50| 86°9| 2°7 Murrie......-- ae Are occ oe Bp Z. AE bse ac ob “2 Te Jhelum.......+. +» |32 55°10] 73 45°25] 53°1| 3°73| 60° | 3°50] 71°8| 1°56] 85°3] 1°35] 86° . Wuzeerabad....| .. | 32 26°20/74 9°50] 53°8| -- | 61°9] -- | 68:5] .. | 818] .- | grtx . Sealkote ...... Se pictete Sele i) BAee le esc, | SO bile el OSSD rere Ae -» | 79°5 DheraGhazeeKh.| .. weit SAD a} 56 or ae Sr or ay Sar I RCER DheraIsmael Kh. 58 ae : re 92° Ghoojarea +. yace see 50° 59° 69°5 Ghee go" Mooltan .....-| -- | 30 10°40] 71 33°25] 51° 58°5 9 80°38 89°4 Shapore .....- ote aids secs | 48°5 53°5 59°5 735 73°5 Shaikapoora....| .. eis ater 59° 66°5 ae 6° 88° Ghoojrat. Jhung. Leia. Mozuffergur. 260 REPORT—1852. On Experiments on the Laws of the Conduction of Heat. By J. D. Forsss, F.R.S. L. & E. I REGRET to state that my experiments have been altogether suspended since the time of my last report by a severe illness which occurred just when I was about to renewthem. Consequently only a trifling amount of the sum voted in 1851 for prosecuting the experiments has been expended; not is it my wish at present to have a fresh grant of money, as it is altogether uncertain when they may be recommenced. I have not, however, neglected to examine narrowly the results of the experiments already made, so far as they have been reduced. I am glad to say that they appear to be very consistent, and the experimental numbers to be worthy of preservation as valuable data in the science of heat. It is with more reserve that I communicate any conclusions affecting the basis of the theory of conductivity as commonly received. But having been in possession for more than a year of a result which seems highly probable, if not quite certain, I am unwilling to withhold it longer on account of an outstanding difficulty which I have not been able satisfactorily to remove. The result is this, that in the case of iron (the only one yet tried) the flux ON THE LAWS OF THE CONDUCTION OF HEAT. 261 _ (continued.) July. August. September. October. November. December. rature| Rain. of the of the day. . day. a y, in 1°78 | 85°9 88°3 86° 76°2 66 59°4. 86 85°6 86°6 80°9 64°6| .. | 59°2} o712 3°00 | 81°8 . 81°9 83'5 78'4 59°5| 1°90 | 57°4| oO°50 ine oe 1°5 864 89°1 87°5 776 64 o*60 | 59°4| o*10 1°54 | 87°3 90°3 go'l 82° 66°4.| x09 | 60°4 1°25 | 87°5 906 : 82°6 68°5| 1°35 | 60°6| o'25 + | 95°5 88°7 87° 74 60°6 57°5 0°98 | 92°1 904 o. 57°9 58 3°79 | 85°5 83°2 85°7 76°2 45° -- | 684 66°7 62°1 62°8 ge 84° 55° 88°3 g2"1 88-7 85 67° 61 84°1 81°7 84° 64°5 58°6 oe 62° ee 63° : a .. 89°5| = + 82° 25 . he 58° 223) tak ORTH at Mage O2 ail Merk S6sg)}) Pe. 68°4 ee «= | | 8675) 4. 81° os . a 56° 93 93° 67 of heat through the solid is not in a simple direct proportion to the difference of temperature of two contiguous thin slices, but varies in a less rapid’ pro- portion; or, the conductivity diminishes as the temperature increases. My experiments were so framed as to give the numerical relation between the conductivity and the temperature ; but though the numbers, given by expe- riments under circumstances essentially different, substantially agree, I do not as yet feel justified in assigning a numerical value to the effect of tem- perature on the conductivity of iron, until the possible disturbing effect of the cause which I have mentioned shall be better ascertained. I take this opportunity of expressing my acknowledgements to Professor Kelland for the advice which he has, with his usual kindness, from time to time afforded me. I still hope to be able to renew these experiments, and I shall not cease to devise plans for their improvement ; in the meantime I Intend to put on record both the principles of the method and the direct results obtained, as well as the reductions; and also the manipulations which experience has taught me, and which I believe will be found of use to any future observer. Ambleside, 25th August, 1852. 262 REPORT—1852. On the Chemical Action of the Solar Radiations. By Rosert Hunt. (1). Tue following results are offered as a small instalment of an exten- sive system of examination which I have undertaken. The object in view is to determine, with all the accuracy possible, the relation which each coloured ray of the prismatic spectrum bears to the chemical action which takes place upon the different agents employed in the production of the sensitive surface. Since different media exhibit very various degrees of absorbent action upon the chromatic rays, as well as on the chemical rays, of the spectrum, by employing them we obtain indications by which we may determine the relation in which these phenomena stand to each other. (2). The plan upon which I am proceeding is this. Having obtained a very extensive series of coloured glasses, and by the solution of chemical compounds, procured a still more varied set of transparent ccloured solu- tions, I analyse the luminous spectrum of a well-formed vertical opening be- tween two knife-edges, by passing the spectrum through a particular absorb- ent medium. The spectra are obtained, first, by means of an excellent flint- glass prism ; again, by one of crown-glass of faultless purity, the manufac- ture of Messrs. Chance, Brothers, of Birmingham; and, thirdly, by a hollow prism, in which I have the means of employing fluids of very different re- fracting powers. For obtaining the chemical impression of the spectrum, I procure a flame-like chromatic image of great intensity, 1 inch in length, from a vertical opening in my steel plate. I have adopted this as my measure throughout, dividing it into 100 equal parts: thus, all the numbers employed are intended to express inches, or the one-hundredth part of an inch. (3). The first part of the present Report is devoted to the examination of the prismatic spectrum by coloured glasses of various kinds. ‘The numbers affixed may appear somewhat irregular, but as they correspond with a very extensive series, over many of which I have no control, but which are well known to me by these numbers, and can always be obtained, I have thought it best to retain them. I have however adopted the plan of numbering my paragraphs, so that in referring back there will be no difficulty in comparing the chemical with any particular luminous spectrum. As I hope to present to the next meeting a far more complete examina- tion of this subject, I refrain from offering a single speculation, contenting myself for the present with the record of careful observations and exact experiments. The lines a a! indicate throughout the length of the normal spectrum. ANALYSIS OF SPECTRUM BY ABSORBENT Mep1A.—No. 1. (A.) Series of Yellow Glasses. (4) 16. Deer yELLow. Colouring matter Carbon, fig. 1.-The Fig. 1. ordinary red raysvery intense, but partaking more of ascarlet colour from the mixture of yellow than a pure red ; the orange and red rays blend so perfectly that it is difficult to define their boundaries. Combined, these rays occupy ‘12. The yellow rays are reduced to a line of bright light equal to‘10. Beyond these the green rays ap- pear very intense, and occupy a well-defined space equal to *25. Blue and violet rays, confined within a space equal to *38, appear somewhat more luminous than the green, presenting no decided colour, but appearing rather as a patch of a pale neutral tint. (5) 15. StRAw-yELLow. Silver stain upon one surface only.—Shortens the spectrum by two-thirds of the violet, so that its entire length is reduced —” ON THE CHEMICAL ACTION OF THE SOLAR RADIATIONS. 263 to *80; the other rays continue unchanged, exhibiting a tolerable degree of intensity. When concentrated by a lens the violet ray is seen to suffer yet further extinction relatively to the other rays. (6) 18. Meprum YELLOow, believed to be Charcoal.—The red ray exhibits more crimson from the introduction of blue ; orange and yellow well-defined ; green ray somewhat shortened, but exhibiting considerable intensity, and well- defined. The blue ray reduced to a small band, and the rays beyond are only indicated by a pale stream of light, neutral in colour. (7) 14. Brown yeLtow, by Carbon, fig. 2—Red Fig. 2. Fig. 3. and yellow rays are considerably reduced ; the green is well-defined, shading off into blue, of which a faint portion alone remains, the space beyond appearing ra- ther a lavender colour than violet. (8) 17. Derr yELLow, by Iron, fig. 3.—This spec- trum consists of four well-defined and nearly equal circles, or rather oval spaces. No blue can be de- tected in the spectral image; the green rays occupying Uy ; i | re the place of the blue; the yellow rays considerably ex- ———% a’ tended ; the red rays are well-defined, but on the upper edge a band of scarlet or deep orange is detected when the eye has become accustomed to the light. The violet has more red than usual in the rays; and at the upper edge, after long gazing, is seen a faint line of neutral gray, the lavender ray of Herschel. (9) 45. A vELLow cass, having a peculiar pink hue—Does not pro- duce any change on the coloured rays of the spectrum; it appears to pro- long the yellow by reducing the upper edge of the orange aud the lower edge of the green. (10) 113. VERY DARK SMOKY BROwN.—AIl blue flowers appear of a deep red brown. Purple and claret-coloured flowers lose all their blue, and appear red. The red, orange and green rays only are visible through this glass, and the illuminating power of those is very considerably diminished. (11) 114. A LIGHTER BROWN THAN 113.—A very much more decided action on natural colours than 113. An examination of the spectrum shows that the red rays are slightly shortened; the orange and yellow rays blend, the yellow coming out in much purity ; the green rays are well-defined, but cut off somewhat sharply at the more refrangible end. Beyond these, by accustoming the eye to the light, a faint trace of blue becomes gradually apparent. (B.) Series of Red Gilasses. (12) 50. Pink GLass(not very clear), fig. 4.—The illuminating powers of all the rays considerably reduced. The violet rays are lengthened and the indigo lost; the blue also considerably short- ened. The influence of this glass is of a very marked character in separating the rays from each other, every ray visible being well marked out. The orange rays are only made out after long exa- mination as a line of inconsiderable width edging the red rays. g By using two thicknesses of this glass, and a spectrum concen- y trated by a lens, the orange rays are brought out as a well-marked tb ra’ band, edged by two black lines. (13) 13. VioLer GLass, fig. 5.—Ist. Rays passed through the glass to the prism. The spectrum appears divided into two distinct parts. The illuminating power of all the rays lessened. In the lower section (1, a), red, orange and green are visible; blue and violet occupying the space 6. If Fig. 4. 264 REPORT—1852. the spectrum is concentrated by a lens and then examined through this glass, the images appear as in (2a), joined by a thin neck of a neutral tint. Few spectra are more beautiful than this when all the extraneous light is cut off, each colour being so very distinctly and clearly made out, the lower illumination enabling the eye to examine it without weariness or confusion. (14) 12. Rep crass (Gold), fig. 6.— The spectrum becomes an oval spot of intense red- ness with a prolongation of the same colour; the red oval comprehending all the rays from the upperend fig. 6. Fig. 7. of yellow to the end of ordinary red, and the prolongation ds a flowers observed through it appear far more red than under ordinary circumstances. The spectrum separated into two long ovals, one, 6, being violet, and the other, e, exhibiting the red and green rays only, the spectrum being very considerably shortened at the least refran- gible end. i) ee aa (16) 119. VioLert.—This glass obstructs but a very small quantity of light, and its action upon the spectrum is not very decided. The red rays are seen in great beauty and purity extending over the space covered by the orange rays; the yellow is very pure, but the green is some- what diminished in intensity, and also in length. The violet rays are prolonged into the blue, thus shortening the latter, which are however very brilliant. (17) 48. A deep and not very pure violet.—The red rays are slightly shortened at the lower end, but they appear extended as they in- ,, 8 crease in refrangibility, so that the orange and yellow rays present a a long band of a pale orange tint uniform throughout. The blue -~ rays are sharply cut off from the violet, the interposing indigo being nearly black; the violet rays being themselves exceedingly beau- tiful and clear. (18) 104. Lirac GLass (Manganese), fig. 8.—Reds of flowers seen in strong contrast with the leaves, which appear darker from the loss of their yellow. The yellow rays of the spectrum are nearly obliterated ; red shortened; green is gradually lost in black sha- dow, and all the other rays blended in an intense oval patch of blue. (C.) Series of Green Glasses. (19) 36. ApPLE.GREEN GLASS.—The red rays are shortened one-half, the yellow extends into the orange, and is sharply cut off without any blend- ing at the edge of the red; on the more refrangible side the green encroaches considerably on the yellow, and upwards into the blue; Fig. 9. the violet by extending into the blue obliterates the indigo. (20) 33. INTENSE GREEN, fig. 9.—All the rays below the orange are cut off; the yellow and green form one tint of pale pea-green. The blue rays are very light in colour, losing but little of their illuminating power, and these are fringed with a deep band of indigo ; no violet rays apparent. (21) 34. Green. Copper of great brilliancy, tig. 10.—The red below the orange cut off; does not shorten the violet end, but pro- duces a great extension of the blue ; the green rays encroach consi- g 7 extends to the edge of the blue. b (15) 117. VIOLET-COLOURED GLAss, fig. 7.—Blue §: @ a a | ON THE CHEMICAL ACTION OF THE SOLAR RADIATIONS. 265 derably on the yellow. The chemical action commences at18 from Fig: 10. the line a'; the orange occupies the space of *10, the yellow about “16, but blending with the green; this is not easy of exact deter- mination; the green occupying about °25, and the blue and vio- let *38. There is a considerable loss of light in the spectrum. (22) 120. GREEN GLASS acting powerfully on all the reds of flowers, &c.—Cuts off one-half the red, extends the yellow, and con- sequently reduces the green of the spectrum. The blue is shortened by an extension of the violet. Although the reds of the least re- frangible end of the spectrum suffer considerably, those which are most refrangible pass this glass (copper) freely. (23) 121. GREEN GLass (Copper ).—Reduces the reds of spectrum ; brings the violet down on the blue; but the violet less red than ordinary. (24) 122. GREEN GLAss.—Nearly the same as the last (121). Fig. 11. There is little change on the lower rays, but the blue and violet rays are reduced to one-half their ordinary linear dimensions. (25) 116. DEEP 1RON-GREEN, fig. 11.—All the reds of flowers observed through this glass become nearly black. The spectrum exhibits two spots of pure crimson; perfect blackness between them. A spot of yellow of great purity, from which the green shades off into a light blue, which becomes very bright, and then passes into a line of indigo. The violet is entirely wanting. (26) 115. A PALE SMOKY-GREEN.—Acts but*very slightly upon any of the rays. (27) 44. DEEP IRON-GREEN, fig. 12.—Cuts off the lower red rays ; admits the permeation of the orange rays freely. The green very much blended with the yellow, so that it is only by adjusting with great care that a line of yellow can be seen. ‘The blue and violet rays suffer scarcely any change, the lengths of these rays being rela- tively as follows :—green ‘30, blue °25, violet ‘15. (28) 6. INTENSE COPPER-GREEN.—The spectrum appears as orange, green, blue and violet. The yellow rays are entirely want- ing ; a very thin line of red appears at the lower end of orange; the violet is considerably reduced by the loss of red. = In all the deep greens we find the violet rays almost entirely destroyed owing to the removal of the red. It is from results of this character that I am led to believe the violet rays to be due to a reappearance of red rays amongst the more refrangible ordinary rays. (29) 52. YELLOWISH-GREEN GLAss.—This glass has but very slight ac- tion on the spectrum, defining more perfectly than ordinary the limits of the _ violet, but producing no sensible change on any other of the chromatic rays. (30) 107. Licut Green.—The reds of flowers are Jost, the flowers ap- pearing purple. Yellows are also lost, the yellow blossom of the Elder tree, &e. becoming pure white. The violet rays are considerably cut off; the other rays are well-defined, but more green and less yellow than ordinary. (31) 119. Licut BoTTLE-GREEN.—Produces no evident change on na- tural colours ; its action on the spectrum is merely to define the spaces of the rays without producing any other change. (32) 110. Deep BOTTLE-GREEN.—Natural blues are blackened, and the __ paler reds suffer slightly. This glass cuts off all the most refrangible rays ; a band of violet, or blue with some red, is seen lining the edge of the green. _ The green rays very brilliant, and yellow passing to whiteness ; the red rays suffering scarcely any change. 266 REPORT—1852. (33) 102. OLIVE-GREEN.—-Green of spectrum somewhat more yellow; the violet diminished by an elongation of the indigo; the violet appearing as a border to the indigo only. (34) 103. Deep oLIvE-GREEN.—Red flowers not to be distinguished from the green leaves; spectrum diminished to red, yellow and green rays, the red being very much reduced in extent, and the yellow and orange blended. (D.) Series of Blue Glasses. (35) 49. A LIGHT BLUE, fig. 13.—The spectrum is represented Fig. 13. in its three primary rays, suffering a little reduction in length ; when a concentrated by a lens a little violet appears at the extreme edge. of the blue. Natural objects do not suffer much change when ob- served through this glass; purple flowers lose more of their red than blue, and violet-coloured ones appear nearly pure blue. (36) 46. INTENSE COBALT-BLUE, fig. 14.—The ordinary red ray disappears, and a pure crimson ray, the extreme red, is seen below the lower edge a! of the ordinary spectrum and extending up to the mean yellow. All the rays but the blue, which becomes very intense, and a trace of violet at v, are ob- 1 Fig. 14, 2. literated, the red rays being sharply cut off at aula y, between which and the blue a dark band appears. When concentrated by a lens, the spectrum is changed, as shown in (2). The lower crimson ray at a’ becoming a defined circle, surrounded by a band of intense black- ness, which extends to the second circle at y, which; instead of being crimson, as was conti- nued in the neck of (1), is now of a lavender hue, from the mixture of some yellow with the red, the blue is condensed, the black at the lowest edge being an intense indigo. (37) 3. CoMBINED BLUE AND GREEN GLASSES, fig. 16.—Looking at the spectrum through these glasses, every trace of red is obliterated, the resulting spectrum being a pure green and blue. Making the rays pass from fig. 16. the prism to a lens (fig. 15), and causing the concentrated rays to Fig. 15. a es permeate this combination, the result is somewhat more decided. The spec- trum is not shortened at the most refrangible end, but the red of the violet is entirely removed, forming a pure blue patch equal to *8. Over the space marked g the green is far more luminous than over any other part, and the rays gradually darken towards the lower end. (38) 105. DEEP COBALT-BLUE, fig. 17.—The red of flowers, as of the Fuchsia, &c., is entirely lost, and not to be distinguished from the green leaves. The surface of leaves appears a grey or blue, with a few exceptions ; the Arbor vite assumes a red-brown colour, remarkable from the striking contrast it makes with the surrounding trees. The leaves of the Currant and several ‘anhtel ON THE CHEMICAL ACTION OF THE SOLAR RADIATIONS. 267 - other plants appear red on their under surface when examined through this giass, the light falling on the upper surface, and being trans- Fig. 17. mitted. Yellow Nasturtiums become of an intense brown. Blue Larkspurs not to be distinguished from the leaves. The violet and blue rays form a large oval, which, encroaching on the green, reduces it to a line bordering the lower edge of the blue. Yellow, a well-defined circular spot, ordinary red obliterated, and the extreme red forming a well-defined circular image quite surrounded by a black band. A prism of crown-glass gives the same result, as does also the hollow prism filled with Castor oil. The extension of this spectrum is remarkable. (39) 108. PALE GREY-BLUE appears to act most upon the yellow of natural objects, but produces no marked difference in the general tints. Its action on the spectrum is very slight; the yellow ray is somewhat reduced in size, and appears whiter than ordinary; and the green ‘is lessened by the blue ray encroaching on it. (40) 112. A smMoxy-BLUE.—No effect on colours generally; increases the extent of the violet and diminishes the blue. The yellow suffers, green passing into it; orange lost in the red. (41) 111. Biug-Grey.—Produces a slight, but by no means a marked change on the colours of natural objects; defines more perfectly the line between the blue and violet, and by lowering the yellow gives a more de- cided margin to the green. (42) 118. Pate BLUE, fig. 18—The reds of flowers are nearly Fig. 18. lost when observed through this glass, all extraneous light being —g—* shut off from the eyes. The red rays of the spectrum are thrown into two circles, and the yellow into a well-marked patch. The green rays are well defined; blue and indigo do not appear to suffer change. The red of the violet is completely lost. (43) 123. LicHT coBALT-BLUE.—The red of the spectrum is brought into a well-defined oval, the yellow very distinct; the green rays are considerably reduced. The blue rays extended, and con- a’ sequently the violet rays are much diminished. = (44) 47. Deep puRPLE GLAss.—Red, orange, green, and blue rays ad- mitted ; violet only distinguished after long examination. When concen- trated by a lens, the violet becomes quite visible as a well-defined band of coloured light. (E.) Miscellaneous. _ (45) 101. SMOKE-COLOURED GLAss.—Does not appear to alter the co- _ lours of natural objects observed through it. Blue of spectrum nearly ob- - literated, but the indigo and violet rays are extended; entire length of spectrum is not lessened. The most remarkable feature is the way in which _ the spectrum is extended over the violet end, proving the existence of red rays far down in the ordinary blue rays. (46) 106. A GREY GLAss.—Removes some red from the violet and shortens it. All the rays lose in luminous power, otherwise they do not _ appear, relatively, to change. _ (47) 115. SMOKE-COLOURED, HAVING A GREEN TINT.—Scarcely any action on either of the rays; there is a little loss of light. (48) 151. GLASS VERY SLIGHTLY sMoKy.—No change can be detected when this glass is interposed. 268 REPORT—1852. CuemIcat SErRIEs, No. 1. —— Chemical Spectra obtained after the Prismatic Spectrum has been analysed by the interposition of Transparent Coloured Screens. PHOTOGRAPHIC AGENT. Collodio-iodide of Silver on Glass Plates*. The numbers preceding the coloured glass employed, refer to the numbers attached to each particular medium in the previous series. No. 1. Those following the colour refer to the paragraph. (49). Normat Spectrum, formed by a very pure flint-glass prism.—Light admitted between two knife-edges, separated {th of an inch, and generally passed through a hole of the same diameter in an inner screen. The chro- matic image was received on a white tablet in a perfectly black box; its length, when most accurately adjusted, was 1 inch and j ths, but for con- venience this has been reduced to 1 inch and divided into 100 parts, and re- latively to this all the chemical spectra have been corrected (1:2). (50). Without any interposed medium, fig.19.—Chemical Fig. 19. action commences °40 above the lower end of red,and from this point extends to the length of 15 inch. Over the space covered by the red and orange rays are indications ‘of a well-defined circle of protective action ; immediately above this a dusky brown commences, forming a kind of fringing which is extended to ‘60, and in a similar manner it bounds the whole of the spectrum. This is due to diffused light, which I always find bordering the spectrum. Over a space equal to *i0 a well-defined black space ap- pears, then the action weakens, but is still strong over °7, when it again increases just at the end of the violet, and is somewhat sharply cut off at 1-90 above 0, or lowest red, presenting an image similar to that represented in the margin. Placing the glass at a small angle, and ob- serving the spectrum by reflexion, the lower dark space comes out very strongly, and the whole space above it appears of a dark semi-metallic purple shaded by a dusky brown border. Glasses (A.) Yellow Media. Fig. 20. (51) 16. Deep yELLow (4), fig. 20.—Chemical ac- tion commencing over the region of the indigo and violet rays, the most intense action appearing to take place about the line H of Fraunhofer, It forms eventually a well-defined oval, the greatest amount of darkening going on in the centre of the impressed spectrum, a protected band, well-defined from the other parts of the surface, in * The collodion was made with gun-cotton which had been pre- pared with nitrate of potash and sulphuric acid. This being well washed was dissolved in ther. Iodide of potassium was dissolved in spirits of wine and iodide of silver added so long as it would take up any, and two drachms of this were mixed with one fluidounce of the collodion. The solution of silver employed was 30 grains to the fluidounce of distilled water. The image was always developed by pyrogallic acid. is very decidedly protected from change. Upon placing the _ glass in a solution of hyposulphite of soda, and allowing it to _ remain for some time, the variations of action are more ap- _ parent :—lIst, the very dark centre; 2nd, a band of much a ieee! ie weaker action; 3rd, a far more energetic band surrounding the whole ; and 4th, a protected band extending from the lower point far below this as a protected circle, as indicated by the shading in the figure. (52) 18. Mepium yveELLow (6), fig. 21.—Chemical action _ commences above the yellow ray, upon the confines of, but 7 the green, commencing *40 above lower red, the space oc- cupied by the green rays being impressed as a well-defined oval of the length of *25, then a neck of very much lower in- tensity of ‘20; a large and well-defined oval 90 in length, exhibiting the greatest degree of intensity in the middle space, shaded off to the edges. The length of impressed spectrum 1:40, and from the zero a! to end of chemical action 1°85, or length of action beyond luminous spectrum at @°85. Here we have an extinction of the violet and indigo rays; and over the space occupied by the blue rays a comparatively weak action, this action being continued with very much energy over the space occupied by the dark rays. The indication of protected spaces around the spectrum is less evident than in many other examples. (53) 114. LicHT RED-BROowN (11), fig. 22—Action com- mencing at “75 and extending with tolerably uniform inten- sity to 1°60, and gradually shading off to 1°85. At the lower end the action descends slowly to ‘65. A brown line of _ shading appears around this spectrum, but this is probably due to dispersed light, since this shading is considerably increased when many clouds are floating about. Glasses (B.) Red Media. ON THE CHEMICAL ACTION OF THE SOLAR RADIATIONS. 269 contrast with the little darkening from extraneous light beyond the luminous image. The space between a and the lower end of the impressed spectrum Fig. 21. a (54) 13. VioLer cLass (13), fig. 23.—Chemical action commences at *60 above 0, and is then continued with tolerable uniformity to 1°35, a faint sha- ding being prolonged about 15 further, or 50 beyond the luminous spectrum. The long dark oval in the interior of the spectrum exhibits a more intense chemical action than the other portion; this darkened space appears to Fig. 24. belong mainly to the upper oval of the luminous Fig. 23. | spectrum and over the dark space beyond it. In | some other experiments, during a period when | thesky was covered with light white clouds, and consequently when the intensity of the sunshine was varying, the chemical limits were subject se to constant changes, commencing sometimes as | high as °70 and terminating at -30. |. (55) 104. Lizac exass (18), fig. 24.—Che- mical action commences at *75 and ceases en- | tirely at 1-25, forming thus one small patch of L changed silver, commencing near the line H, and “occupying but about one half-inch of space. 4 270 REPORT—1852. More than half of the bluerays are inactive, the action being confined to the space of the violet and the lavender rays. 5 (56) 12. Rep (Gold) (14), fig.25.—A great number jj of experiments have been made with the hope of detecting some chemical action on the iodized collodion by the bright crimson rays which permeate this glass. In no instance have I been successful; instead of obtaining any indication of change, the only result has been the occa- sional evidence of a protecting action over the spot on which the oval red patch, described in the analysis of the spectrum, falls when diffused radiations have acted on the sensitive surface generally. Glasses (C.) Green Media. (57) 36. BRIGHT APPLE-GREEN (19), fig. 26.— Action appears singularly divided. Two spaces of most intense action, corre- sponding with the green and violet rays as shown at y, v, these being surrounded with a band of a chocolate-brown colour. By placing the glass in a strong solution of the hyposulphite of soda the outer band is readily dissolved off, but the ovals y, v resist for a long time the action of the solvent, dissolving indeed, only when the film of col- lodion separates from the glass. (58). The former result was obtained in London. On repeating the experiments at a a’ Falmouth, a very different result was ob- . tained. The action commencing at ‘60, and continuing to 1°60, an extended though much weaker action is prolonged to °35. The experiments having ~ been repeated several times in both localities under precisely the same con- ditions as regards prism, size of opening between knife-edges, length of spectrum, &c., these results indicate some peculiar atmospheric conditions. These, however, can only be determined by several sets of experiments at different times. (59) 6. INTENSE COPPER-GREEN (28), fig. 27. —Intense action, producing a bronzed line, commences at ‘60 and extends to 1°10, or over a space equal to°50. A weak action extends down to ‘45, marking the space occupied by the green ray. A similar modified action extends upward to 1°60. By long exposure a light fringe appears over the space occupied by the yellow rays, the actual chemical spec- trum being 1°35 in length. The fringe around ; the lower part of the spectrum, which is not readily explained, is a tolerably constant re- = sult. It may possibly arise from some refrac- tion of the rays near the Fraunhofer line B, within the glass plate. (60) 34. Green (Copper) (21), fig. 28.— Action commences at ‘60, and it is continued : | oe ee eee eee _ which appear to go on within the chemical spectrum. _ tends up to 2°20. The inner portion of this spectrum much more intense over this section than on any other _ the complete production of metallic silver in a state of brown edge, but does not act in the slightest degree on | the inside oval space. The spectrum obtained without f any interposed medium is, upon collodion, of less extent than that now described; it is, usually, a long flame- ON THE CHEMICAL ACTION OF THE SOLAR RADIATIONS. 271 with full intensity to 1°15. This forms a well-defined dark olive-green oval spot; it is somewhat smaller at the upper end; the chemical action is then continued faintly to 1-35, and still more faintly to 1°60. At the lower end the impressed image descends to ‘50, and a faint border of dusky brown sur- rounds the spectrum, which is impressed over a'space equal to 1°5. The prin- cipal action is limited to the blue and the rays above it. , (61) 33. INTENSE GREEN (20), fig. 29.—The action hereon _ Fig. 29. the most sensitive collodion plates is exceedingly slow, and after © an exposure of five minutes in the brightest sunshine, the only ——_——* indication of any chemical action is the appearance of a faint spot near the line H. This when acted on by the pyrogallic 6 acid becomes very dark, and another spot a little beyond the violet rays makes its appearance. (62). In the camera obscura, which has been devised for working with the very sensitive and beautiful collodion process in the open air, yellow glasses have been introduced for the a’ purpose, as it was thought, of cutting off the chemical rays, at the same time as light enough was admitted to enable the operator to see his work. The results obtained (see Yellow Media) clearly prove that rays, chemically active for collodion, pass the yellow media very freely; some green glasses, as the above, offer much more obstruction, but red glasses ap- pear to be still more effective. c (63) 44. DEEP IRON-GREEN (27).—The action of this spectrum is very slow, and confined to the limits between the mean green ray and the extreme violet. In agreat many experiments the spectrum impressed has been always limited to the space °50; that is, it has commenced in the middle of the luminous spectrum and terminated with the violet rays. Very weak hypo- sulphite of soda washes off the darkened portion so readily, that I am led to infer that it is an exceedingly superficial dust upon the surface only. (64) 116. ANOTHER DEEP IRON-GREEN (25).—By long-continued action there is scarcely a trace of any chemical change. Here we have an example of a spectrum in which the blue class of rays, ordinarily called the chemical rays, are very brilliant, yet they are chemically inactive upon this most sen- sitive photographic preparation. Fig. 30. Glasses (D.) Blue Media. (65) 105. DEEP COBALT-BLUE (38), fig. 30.— The rapidity of action with this medium prevents the marking of many of the more remarkable gradations of change Chemical action commences between °70 and 1°70, and ex- appears the lightest, but in reality ‘the action has been part, and the semi-transparency of this portion is due to fine division. Ammonia will dissolve off the outer dark shaped band of 1°60 or 1°70 in length, and of uniform : intensity throughout. The operation of the cobalt-blue we 272 REPORT—1852. glasses on the spectrum indicates’ some peculiar influences, which require more extensive study than they have yet received. The remarkable difference between the luminous and the chemical spectrum is very striking, and it ap- pears to indicate the independent existence of the actinic or chemical rays. (66) 3. CoMBINATION BLUE AND GREEN (37), fig. 31.—The spectrum impressed by long exposure commences at -45 and terminates sharply at 1-0, there being no indication of any action beyond the visible spectrum. It will be found by examining the drawing of the luminous spectrum obtained when the light has passed this combination of Fig. 31. Fig. 32. glasses, that the action commences at the lower a edge of the green rays. ‘The whole space im- Dir’. as pressed has equal intensity throughout, with a brightening of the silver in the middle. (67) 49. A Licur BLUE (35), fig. 32..—The action commences at the lower edge of the blue rays ‘55 from 0, and extends to 1:40, when it is suddenly interrupted. Considering the usual character of blue glasses, and that this one is Ong an unusually transparent nature, it will be ue- cessary to subject it to a much more search- ing examination than it has yet veceived. That the chemical change is very superficial, is proved by the rapidity with which the hyposulphite of soda removes the impression. (68) 46. CopaLt-BLUE (36), fig. 33.—Action com- mencing at °75, extending with full euergy to 1°50; at the lower edge it is continued with faint shading to °55, and even some very slight continuation to ‘0, which is to be detected by placing the collodion glass plate upon a sheet of white paper and viewing it at a small angle, and shading off at the most refrangible end, until at 2°10 all action appears to cease. This is the greatest extension of the spectrum which up to this date (August 20, 1852) has been obtained; and in two experiments made in very intense sunshine at noon-day, a well-marked spot has been obtained °10 below 0, as marked in the drawing. This spot will be found to correspond with one of Sir John Herschel’s heat spots, and may possibly be referred to some peculiar chemical action due to the so-called pa- rathermic rays. The presence of vapour, in the form of light cloud or mist, however attenuated, appears to ob- struct this peculiar class of rays. (E.) Miscellaneous Series. (69) 101. SMOKY-COLOURED GLASS (46), fig. 34.— Che- mical action commences at “70 and extends to 1:90. At the least refrangible end the impression descends faintly to *50. The maximum of action is within the limits of the visible most refrangible rays, the most intense spot being near Fraunhofer's line H. Those media which have been employed in the analysis of the prismatic spectrum, and are described in the optical series, put which do not appear in the chemical one, have been omitted, until further experiments confirm, or the contrary, the results which have been obtained. a Bt THE FLAX PLANT. 273 - On the Composition and Ciconomy of the Flax Plant. By Dr. HopcGEs, F.C.8., Professor of Agriculture, Queen’s College, Belfast, and Chemist to the Chemico-Agricultural Society. Next in importance to the study of the substances which serve man for food, is the investigation of the composition and ceconomy of the materials which yield him clothing. Among the plants which, from the most remote anti- quity, have been valued for their textile adaptation, those of the Linacez family—and especially the Linum usitatissimum, a native of our own country, and widely spread over Europe, and also found in Hindostan and North America—have occupied a prominent place; the flax plant, we have reason to believe, having been cultivated for its fibre in the earliest seats of civi- lization, and manufactured in the tents of the patriarchal fathers of our race. We find that it was worn in the temples, and the microscope has demon- strated that it was entombed in the sepulchres of Egypt. It also appears that its valuable qualities were known to the ancient tribes of northern and western Europe. A complete account of the flax plant, and its industrial applications in Ireland, should include—l1st, the history of flax cultivation in Ireland; 2nd, an account of the processes of cultivation ; 3rd, an examination of the chemical composition of the plant; 4th, an account of its technical preparation. The second division of the subject, however, belongs so exclusively to the practical department of agriculture, that its consideration may at present be properly omitted; and though it would be out of place to occupy much time in this Section with the first division, yet a few remarks may be permitted, for the purpose of exhibiting the attention which, from a very remote period, seems to have been directed to flax cultivation in this country, and as illus- trative of its vast importance to the inhabitants of the province in the com- mercial capital of which we are now assembled. 1. The History of Flax Cultivation in Ireland.—From the earliest pericds, we have reason to believe that the inhabitants of this island were acquainted, with the valuable qualities possessed by the fibre of the flax plant, and manu- factured it for clothing. By whom, however, or from what country it was introduced, we have no satisfactory record; for the assertion made by some _ writers, that the Phcenicians were the instructors of the Irish people, is totally destitute of historical foundation. Our Irish name for flax is Lhin, which word is also applied to thread, while the term Anairt, which is used to express a kind of coarse linen cloth worn by the peasantry, Dr. O'Donovan, _ of Queen’s Coliege, whose extensive and valuable researches in connexion _ with the native records of this kingdom are so well known, informs me has _ no cognate term in any language with which he is acquainted, and is evidently a word of great antiquity. In the Brehon laws, also, we find it enjoined that the Brughaidhs or farmers must be acquainted with the mode of working flax. The linen shirt, dyed yellow, indeed, appears to have been a national dress ; and the celebrated jesuit, Edmund Campion, speaking of the “ meere”’ Irish, describes their fondness for capacious linen garments. “ Linen shirts,” he Says, “the rich doe weare for wantonness and bravery, with wide hanging sleeves, playted; thirtie yards are little enough for one of them.” ‘The importance of flax cultivation in Ireland appears to have been fully recognized by the English government, as may be inferred from the number of legislative enactments and grants for its encouragement. In 1809, we find that govern- ment appropriated the sum of £20,000 for this purpose. The exertions of Several national societies have also been directed to the promotion of flax 1852. T 274 REPORT—1852. cultivation ; and by the labours of the Royal Dublin Society, the parent of all our agricultural associations, important improvements were introduced in the management of this crop. Since the establishment, in 1841, of the Royal Flax Improvement Society of Ireland—an association of proprietors and ma- nufacturers, which was originated, and holds its meetings in this town—there has been expended of money, collected by subscriptions from members, £8000, and of money granted by the government to the Society, for the pro- motion of flax cultivation in the south and west of Ireland, £4000. Yet, notwithstanding the efforts which have been-made by governments and societies to stimulate the culture of flax, and though the total extent of the crop produced last year was estimated by the Census Commissioners as equal to 138,619 acres, the value of which would be about £1,700,000, this produce is only about a fourth of that annually required by the rapidly increasing manufactures of the United Kingdom. Though flax is at present cultivated in almost every part of Ireland, yet it is in Ulster that this branch of industry has attained its chief development. Of the 138,619 acres of flax grown in 1851, only 14,893 acres were beyond the bounds of this province. It is in Ulster, also, that the principal seats of its manufacture are to be found. 2. The Composition of the Flax Plant.—In reference to the third division of the subject, I conceive that the most satisfactory method will be to com- municate the history of a crop grown by myself for experimental purposes, the progress of which I was able carefully to watch, from the sowing of the seed till its conversion into dressed flax for the market. Some of the details which I have collected, though of importance in the study of agricultural science, have not been hitherto much attended to in this country. The field selected for the experiments was situated about a mile anda half from Belfast; it has a south-west aspect, and the soil is a sandy loam, composed of transported materials, such as are common in the districts sur- rounding Belfast. It had been occupied as a grazing field for four years, and allowed to produce rich crops of thistles and ragweeds. Its chemical examination proved that it contained a fair supply of all the ingredients re- quired for the purposes of cultivation: 100 parts had the following compo- sition :—-- Ciranic mthets oes ee) OOO MURS E OF NOM sieck cut hottest obs eA PIAA 0 CRS yeos'e,s vacate gear ae ©, O Darnntate Gene” eon ge oe, POF mulphate- Of lima... ee es OF Phosphate of lime .........../... 018 Carbonate of magnesia .......... 0:06 Salts of potash and soda.......... 240 Insoluble siliceous matters ........ 83°32 99°54 Water in the sample .... 3°00 Textural composition.—Clay, fine sand, and organic matters.... 16°50 Coarse sand and gravel ...........-.. 83°50 100:00 Progress of the Crop.—-On the 16th of April, 1851,a portion of the field, measuring exactly 70 yards by 70, which had been prepared by spade labour ‘in winter, was reduced to a fine tilth by harrowing and rolling, and sown THE FLAX PLANT. 275 with two and a half bushels of clean Riga seed of superior quality. The weather had been dry for some time; but in the evening, after the sowing, 0°300 inches of rain fell. On the 28th of April the young plants appeared above the soil. Mean temperature, from 16th nae 46°°5 Fahr. Quantity of rain ..... . 1:385 inch. On the 14th of May the pra tie of the field was green; each plant con- sisted of two leaves. May 31.—Each plant, with root, measured about 6 inches. Eight plants were taken for examination, and were found, when all traces of adherent earth were removed, to weigh 36 grs. They were dried at 212°, and care- fully incinerated in a platinum vessel, and were found to be composed as follows :— Per-centage composition. Fresh plants. Dry. Wate E Sc. deliv Sige <(BOTS 83°833 Organic matters .... 5°09 14°139 8'7°446 Inorganic matters 0°73 2°028 12°554 y 36°00 100-000 100°000 June 26.—Two plants, with roots, were taken from the same part uf the field as those last examined. The plants were just about to flower. Height of each above surface of soil, 223 inches. Both together weighed 60 grs. Per-centage composition. Fresh plants. Dry. Water 81:917 Organic matters ...... 16°837 2 5) Inorganic matters...... 1°246 6°89 100:000 _. 100-000 _ June 28.—The plants were in flower. Mean temperature, from their first appearance above the soil (60 days), 53°°7 Fahr. July 7.—One plant in flower was taken. Height, 29 inches. entire plant, 26:05 grs. Weight. of Per-centage composition. Fresh plants. Dry. Water... cc aay ss 73°32) Organic matters........ 25°144 94°25 Inorganic matters ...... aoa 5°25 100°000 100-000 July 28.—One plant of flax, in seed, was taken; height above ground, 31 inches, root 53 long; length from ceri of the ‘Feld to the first branch 24 inches. The weight of the entire plant was.71°1 grs. About 5 inches ‘of the lower end of stem had become yellow. Per-centage composition. Fresh plant. Dry. Water. : 52. Pst ane’ 69°210 Organic matters... .. 30°045 97°58 Inorganic matters ..,... 0°745 2°42 100°000 100°00 fue, 276 REPORT—1852. The plant was cut into three portions, which were separately incinerated, with the following results :~- 1. Root and lower part of stem weighed, dried, 6°60 grs., gave 0°094 ash, 1°424 per cent. 2. Capsules and branches, dry, weighed 9:47, gave +293 ash, 3:094 per cent. 3. Middle portion, dry, weighed 5°53, gave *143 ash, 2.584 per cent. August 10.—-One plant taken; entire length, with root, 37 inches; length from surface of soil to branches, 29 inches; stem of a light straw colour ; leaves withered on 10 inches of stem; capsules 10 in number——seeds green ; weight of entire plant 71 grs.; branches and capsules 31°8 grs.; water in plant 45°336 grs.; solid matter in ditto 25°665 grs.; inorganic matter in ditto 1-006 gr. Per-centage Composition. NV AtCRs ttre ig wale ots a 63°852 Organic matters ........ 34°732 96°08 ASH cas unpie tee Scie dautyen ol ARO 3°92 Total.. 100-000 100-00 August 25.-The pulling of the crop was begun—a plant was taken and examined; weight of entire plant 62°40 grs.; weight of capsules 22°50 grs. Per-centage Composition of Stem. In fresh plant. Dry. AWPU aSY et ott anerie Ate ses emer olay B 56°64 Organic matters ........ 41°97 96°80 , Aplin cuit paukias eh ce sn LOD 3°20 Total.. 100-00 100°00 The crop was placed in stooks, and remained in the field until the 8th of September, when it was weighed at the Cregagh Steeping Works. At this period the air-dried straw was found to contain 12-2 per cent. of water, and the bolls 11°84 per cent. The weight of the produce of the experimental field (straw and bolls), air- dried, was 7770 lbs., for which the sum of £12. 9s. 9d. was obtained. Amount of Nitrogen and Inorganie Matters in the Straw and Capsules, as pulled on the 25th August, dried at 212°. In the straw. In the bolls. 1. Nitrogen, percent..... 0°53 1:26 2; Ash, per eent:..<.... 3°20 4077 Composition of the Inorganic Matter of the Crop. 100 parts of the ash of the straw and capsules had respectively the fol- lowing composition :— Ash of straw. ‘Ash of capsules. Potash 2 saad snr iene a 20°32 16°38 Sacdanhur ace ae meouies geo Or 6°25 Chloride of sodium ...... 9°27 12°98 Weiner. hacer ian 19°88 13°95 Te ee 4°05 ool Oxide of iron .......... 2:83 0:38 Bulepmrie aed fy) ....3.. Ts 1451 Phosphoric acid ........ 10°24 23°26 Carbonic acid .......... 10°72 6°37 Silica Seeeiiee els 53 1280 0°67 Total.. 99°31 99°02 THE FLAX PLANT. 277 One of the earliest among those who directed their attention to the che- mical composition of flax, was a distinguished member of this Association, Sir Robert Kane. Since that time analyses of the ash of the straw of flax have been published by Professor Johnston of Durham; by Messrs. Mayer and Brazier, and by Mr. Way in England ; by Leuchtweiss in Germany ; and by the reporter. The only examination however of the proximate constituents of the plant, so far as I am aware, consists of an analysis of the seed by Leo Mayer. It is, indeed, strange that a plant, the straw of which has afforded oc- cupation to the industry of so large a portion of the world in all ages, and the preparation of which, for commercial purposes, consists in acting upon its proximate constituents, should not have been more carefully studied. Having been for some time engaged with investigations in this important department, I shall, on some other occasion, bring forward the details of my analyses. At present I shall merely state the general results of the examination of a spe- cimen of flax-straw taken from the experimental crop. A preliminary exa- mination having indicated the presence of a volatile oil, a quantity of the stems of the plant, carefully deprived of the seed capsules, was distilled with water containing common salt, and from the distillate, which was without action on litmus, I obtained an oil of a yellow colour; 5 lbs. of the fully- grown fresh stems afforded about 10 grs. of this oil, which had an agreeable penetrating odour, and suggested the peculiar smell which is remarked on entering a room where flax is stored. In my examination of the proximate constituents of the plant, the straw, coarsely powdered, was placed in an extraction apparatus, and successively treated with ether, absolute alcohol, water, dilute hydrochloric acid, and weak solution of potash. The solutions obtained on examination were found to contain a fat oil, wax, traces of chlo- rophyle, a peculiar green resin, a gum resin, which presented some of the characters of the principle which Pagenstecher termed linine, and described as existing in the Linum catharticum or “purging flax,” but could not be identified with it, a modification of tannic acid, which afforded a gray preci- pitate with perchloride of iron, but was not affected by solutions of isinglass or tartar emetic, gum, not affected by solution of borax or basic silicate of potash, a brown colouring matter, albumen, caseine, starch, pectine, cellulose, and salts. The following table exhibits the action of the various solvents employed :-— 1. Soluble in wether ........ kd se had 2°83 9, Soluble in absolute aleohol ...... eae, 3. Soluble in water ......-....+..-- 5:92 4. In dilute hydrochloric acid ........ 22°76 5. In dilute solution of caustic potash.. 16°39 6. Cellulose and salts.............0.. 48°58 100:00 [ shall now proceed to the fourth division of the subject, and describe the various methods which are adopted for the purpose of preparing the flax plant for the spinner. I shall not in this place allude to the economy of its seed, but confine myself to the management of the fibre of the plant, to a which, of superior quality, is the main object of the flax-growers of ster. When a portion of the straw, as it is termed, of the flax plant is examined, it is found to consist of three parts: first, of a woody, central, hollow column, which the microscope shows to be composed of cellular tissue ; second, of a tubular sheath, composed of long and firm bast-cells; and thirdly, of a deli- ’ 278 REPORT—1852. cate covering of epidermis. By rubbing a piece of dried flax-straw between the fingers, the woody central part and delicate epidermis can be readily broken to pieces, while the tough fibres of the bast-cells will be found to re- main but little injured. Those tough fibres, which are capable of being split into filaments of extreme delicacy, constitute the raw material of our greatest national manufacture. In the country farm-houses and manufacturing towns of Ulster, they afford employment to thousands of our people, and are made to assume almost innumerable forms. They are moulded into the costly lace and beautiful cambric. They cover our tables, and supply us with “fine linen,” equal to that which was once the pride of Egypt. The coarser fibres give stout sails to our ships, and even the refuse rejected by the spinner is worked up into a cheap and substantial material for covering our farm-houses, while the sweepings of the Belfast warehouses are sold to the paper-makers of England, and used to produce the broad sheets upon which the Times and Morning Chronicle newspapers are printed. To separate this invaluable fibre from the worthless parts connected with it is the first step in its preparation for the spinner. Numerous plans have been proposed for this purpose, both by scientific and practical men. The examination of the plant shows us that its parts are bound together by gummy and resinous substances, and that vegetable jelly fills its cells. The separa- tion of the fibre, therefore, merely by mechanical means, as might be expected, cannot be perfectly accomplished; yet at various times patents have been taken out for the application of machinery for this purpose; and in 1815 the Linen Board expended £6000 in the attempt to introduce into Ireland a ma- chine which had been invented by a Mr. Lee. One of those machines was lately sold as lumber at the White Linen Hall in this town. In other countries the dry preparation has also been tried, and though it has been found capable of producing a coarse, discoloured fibre, adapted for inferior fabrics, such as bagging, &c., yet it has been nearly discontinued. The specimens on the table will serve to illustrate the results of this method of treatment, as pursued in the jail at Cork, where it serves to give useful employment to the prisoners. From the earliest times only one method has been found capable of yielding the textile material in a condition adapted for every purpose, and possessing all the qualities demanded by the spinner, viz. the decomposition, by the process of fermentation, of the adhesive substances which connect together the bast fibres and the ligneous tissues of the straw. It is by this pro- cess, variously modified in the arrangements for conducting it, that nearly all the fibre produced in the great flax-growing countries of Europe is at present prepared. In many parts of Germany the fermentation is induced by ex- posing the flax, spread in the fields, to the influence of the air and moisture ; while in Belgium, which is justly regarded as the model country for flax management, the practice of enclosing the straw in wooden frames, and im- mersing it in the waters of rivers until the necessary changes are produced, is in many places adopted and found to yield fibre of superior quality. In Ireland, at the present time, two modifications of the system of fermenta- tion are in use—one of which consists in steeping the straw in pools of water in the open air at ordinary temperatures, while, according to the other method, the steeping is transferred from the farm to the factory, and the fermentation accelerated by employing water maintained at an elevated temperature. The former method of steeping has prevailed in this country and in other parts of Europe to some extent from the earliest times; and though it has been asserted by some writers, without, however, any authority for the statement, that the ancient inhabitants of this island prepared the flax in the same rude THE FLAX PLANT. 279 manner, by beating the unsteeped straw, as observed among some of the people of the South Sea Islands, yet we may, I think, infer from the number of places to which the name “poll a lin,” t. e. flax hole, is applied, that they steeped in water. The plan followed by the farmer, who adopts the plan of steeping the flax on his farm in the open air, is to excavate a pond in con- nection with some convenient stream. The dimensions preferred are from twelve to eighteen feet broad, and about four feet deep. The quality of the water employed requires careful consideration, hard waters being found ma- terially to interfere with the process; ferruginous waters also are avoided ; aud in those districts where the steeper is obliged to make use of them, the flax acquires a dark tinge, which the bleacher finds it difficult to remove. From the action of the salts of iron upon the modification of tannic acid, which I have shown to exist in the straw, we can readily understand that the presence of iron in the water of the steep-hole must be prejudicial. As the oozing of water from the adjoining soil also frequently produces discoloration of the flax, careful steepers place on each side of the-pond a small drain, to prevent the entrance of drainage waters. The flax, after pulling, is prepared for steeping by removing the seed capsules, or bolls, by means of a simple machine, composed of a number of iron teeth, about eighteen inches long, screwed to a socket of wood, and fixed perpendicularly on a long bench, upon which the workmen sit. The bolls are separated from the stems by the work- men taking a handful of the flax, spreading it out, and drawing it through the teeth of the ripple, as the machine is termed. Sometimes, however, the steeping does not take place until the flax has been stored for some time, and has become so dry that the fibre would be liable to injury by using the common rippling-machine. In such cases the seed is beaten off by means of a “ beater,” formed of a block of wood furnished with a curved handle. In England, where the flax plant is cultivated more for supplying food for eattle than for its fibre, the value of its nutritious seed is acknowledged by every farmer; but in Ireland, unfortunately, industrial knowledge is only beginning to influence the practice of the agricultural population. It is in Ulster that the chief progress has been made. The Royal Flax Society has diffused much useful information ; and another institution, the Chemico-Agri- ~ eultural Society, by its lectures and publications, has also contributed, in no small degree, to overcome ancient prejudices. Yet it must, I fear, be regarded by this meeting as but little creditable to our agriculture, that, though annu- ally nearly 650,000 qrs. of flax-seed and 70,000 tons of flax-seed cake are pur- chased by the farmers of the United Kingdom from foreign countries, only about one-tenth of the seed grown in this country is saved, the remaining portion, by the prejudices or indolence of the farmer, being consigned to the steep-hole. : In placing the bundles of flax in the steeping-pond, they are arranged in regular rows, placed in an inclined position, so that the tie which confines the straw in one bundle rests upon the root end of the preceding bundle ; the bundles of flax of equal length being arranged in different parts of the pond. When the pond is filled, a thin layer of straw or rushes is spread evenly over the flax, and on this covering old sods are placed, so as to keep the bundles from rising above the water. In a day or two, according to the temperature of the season, fermentation commences in the pool, and in warm weather in from eight to ten days, at other times in from twelve to fourteen, the steeping and retting, as the process is usually termed, is completed. During the steeping the water acquires a dark brown colour, carbonic acid is disengaged in great abundance, and the surface becomes covered with a gelatinous scum. To remove this matter it is usual to allow a gentle current 280 REPORT—1852. of water to flow over the surface of the pond from the supplying stream, as, when it is allowed to remain, the colour of the flax is found to be injured. Various methods are resorted to in this and other flax-growing countries, to ascertain the proper period for the removal of the flax from the pond. Thus the Silesian steepers take some stalks of the Hax from the pits, and place them on the surface of the water. If the stalks sink they remove the flax, but if they swim they allow the steeping to continue for some days longer ; while the Irish farmer, day after day, when the fermentation has fairly commenced, anxiously tests the progress of decomposition by drawing a few stalks from one of the flax bundles and breaking them across in two places, about two inches apart. If he can readily pull away the central woody column without tearing the filaments of bast which surround it, he considers that the period has arrived for removing it from the pit. It is easy to perceive that the peculiar series of changes which facilitate the breaking up of the various organic compounds which compose the struc- ture of the flax plant, must, in our fickle climate, where so many sudden alterations of temperature occur, be liable to frequent disturbance, and that the progress of the fermentation, in the shallow steeping-pools, must be exceedingly irregular and uncertain. It is not, indeed, to be wondered, that, notwithstanding the closest supervision, the most experienced steepers should frequently be deceived, and that one part of the flax should be too much decomposed while another part has not properly experienced the altera- tions which facilitate the complete separation of the valuable material. The disagreeable odour evolved from a flax-pool must be familiar to those who have travelled in the north of Ireland in the steeping season, and the black hue which the streams in some country districts acquire at that period, from the refuse waters of the pools being allowed to fall into them, excites the surprise of strangers. It is interesting to discover, amongst those wonderful records, not merely of the military achievements, but of the rural occupations and manufactures of the ancient inhabitants of Egypt, which have come down to us on the walls of their temples, that the steeping of flax and its preparaticn for their “fine linen,” was conducted nearly, we may conclude, in the same manner as by our farmers at the present time. The drawings exhibit to us large wooden vats for containing the flax-straw, and men are represented carrying water to fill them. To render the history of the crop complete, it is necessary to give some account of the treatment which the flax undergoes on its removal from the steeping-pool. I shall confine myself to a description of the ordinary system of this country. The first operation to which it is subjected is what is tech- nically termed grassing, which consists in spreading the steeped straw in thin and even layers upon pasture ground, for from six to ten days, according to the season, frequently turning it during its exposure, that the air may act equally on every part of it. By grassing the eremacausis of the woody matter and loosening of the fibre is still further promoted, and the colour of the flax also improved. After grassing, the straw is either stored up in stacks, for subsequent treatment, or at once subjected to the action of machines which break up and remove the brittle woody parts. To break up the woody matters so as to facilitate their removal in the ordinary practice of the farm, a simple machine, termed “the break,” is employed. It consists of two wooden frames, each of which is furnished on one side with a number of parallel angular bars, so arranged, that, when the frames are connected together by a hinge, the angular surfaces of the bars on one frame are received into the hollows formed between the bars of the other. One of the frames is permanently fixed on THE FLAX PLANT. 281 a support, while motion is communicated to the other frame by means either of an iron spring, or by an elastic pole of wood attached to it and connected with a treadle, upon which the workman presses with his foot. By placing a handful of the straws between the frames, and pressing upon the treadle, the moveable frame descends and bruises, or breaks the inelastic woody matter, while the supple fibre is uninjured. So prepared, the straw is ready for the second and final operation, which it undergoes before it is transferred from the farm to the factory. Steeping and grassing have destroyed the co- hesion between the various structures of the straw, the break has fractured the woody matters, it only now remains to liberate completely the valuable textile material from its worthless encumbrance. This is effected on the farm by means of a simple implement of manual labour; an improved form has been introduced from Belgium. It consists of a thin blade of wood, attached to a handle, and an upright wooden stand, with a notch cut on one side, in which the workman inserts a handful of the steeped and bruised flax, and turning the flax so as to present every part to the implement, by the blows of the “scutcher” the brittle and broken weody matters, technically termed “shoves,” are knocked away, and at the same time any very short or injured fibres are removed, producing what is known as “scutching tow.” Some- times bits of “shove” adhere so closely to the bast fibre, that the workman requires to scrape them away by means of a blunt knife. Amongst the various obstacles which impede the extension of flax cultiva- tion to the south and west of Ireland, is the difficulty of obtaining experienced scutchers; and serious loss has frequently been sustained, by persons who have attempted the preparation of the crop, from the want of that skilled labour which is available in almost every part of Ulster. Thus it was found that while the northern scutchers can turn out from 12|bs. to 141bs. of fibre per day, the workmen in the south and west have not been able to prepare more than from 5lbs. to 6 lbs. daily, and frequently not more than 2 lbs. It is therefore of great importance to this country that government is about to afford encouragement to the erection of machinery for scutching, in districts where skilled workmen cannot be obtained. Even in Ulster, for some years the opinion has begun to prevail, that, as in other departments of our manu- factures, hand labour must, in the preparation of the flax fibre, give place to machinery, and “ scutch-mills,” where the work is performed for the farmer, are to be found in all our flax-growing districts. The fibre of the flax, prepared either by manual labour, or in the seutch- mill, is ready for market, and is sold according to its quality, at prices ranging from £30 to £150 per ton. It is not yet, however, suitable for the opera- tions of the spinner. In the same bundle there exist fibres of various quali- ties ; and it is also necessary that the filaments should be arranged in parallel “reeds.” They must be sorted and hackled. “ Hackling ” consists in draw- ing the mass of fibres through sets of iron teeth, fixed in a stand of wood, which, like the teeth of a comb, separate and arrange the fibres, and remove all broken pieces. Thus treated, flax is rendered fit for its various textile uses. Produce of Fibre, §e—The amount of rippled flax-straw, viz. 5824 lbs., obtained in my experiment, considerably exceeded the ordinary produce of the farmer. From the returns of the Royal Flax Scciety, and from my own inquiries, I would estimate the average produce of a statute acre, in the north of Ireland, of air-dried flax-straw, with bolls, at two tons, which by the seeding machine are usually reduced to 3360 lbs. By the various processes of the rural manufacturer, the amount of dressed flax or fibre obtained ave- 282 REPORT—1852. rages from four to five cwt. per acre. Some time ago I made an experiment at one of the country scutch-mills nearBelfast, for the purpose of ascertaining the relative proportions of the various qualities of fibre, and also the distri- bution of the inorganic matters. The flax employed had been steeped in the usual way, and was found to contain 1°73 per cent. of inorganic matters :-—— 4000 lbs. of air-dried straw produced of — DIT ESSGM CH Rincte Mets veth-wc ov ekaisinuasussaiane teeteanue 500 lbs. 1 ENVECEPUN ON? ants hr NRE eee nn tate eaa ent 1 1474) | sie (GOnise ch Wane tetas each d. Mimosy 580 acc aonet ethene OSS 824 lbs. An examination of the amount of ash which the above materials respec- tively contained, showed that its distribution was as follows :— In the flax............ 4°48 lbs. of inorganic matters. In the fine tow........ 2°08 In the coarse tow...... 2°56, or in all 9°12 lbs. So that 59°08lbs. of the inorganic matters, which the crop had withdrawn from the field, remained locked up in the woody shoves, which, as obstinately resisting decomposition, are used for fuel, while 9°12 lbs. were carried away in the dressed flax and tow sold to the spinner. Accelerated Fermentation—The Patent System.—For so far, we have con- sidered the preparation of the flax fibre solely as constituting a part of the ordinary farm operations of this country. Where the necessary amount of intelligence prevails among the agricultural community, with regard to the proper cultivation of the crop and its after treatment, as is the case in Belgium, in some provinces of which country frequently 10 per cent. of the cultivated area is devoted to its production, and in Ulster, where we find that, in 1851, one out of every 44 acres was under flax, experience has taught the farmer, that even with the various disadvantages attendant upon the old and uncer- tain methods of management, it is capable of yielding considerable profit to the grower. Notwithstanding, however, the efforts which have been made by societies and government to extend the cultivation of the crop to those di- stricts in the south and west of the kingdom, where, for various reasons, it was most important that the means of occupation which it was found to afford in Ulster should be rendered available, great difficulties were experienced, both from the deficiency of skilled labour and the want of convenient markets for the produce. Fortunately, at a time when great discouragements had been ex- perienced by those who had entertained the expectation that the fertile soils of the south of Ireland were destined to render our manufacturers independent of the supplies of foreign countries, the attention of the flax-growers of Ulster was directed to a system of flax management, proposed by an American named Schenck, which appeared to remove all the difficulties of the old system, and promised completely to revolutionize the ceconomy of the crop. In the method of Mr. Schenck, as in the old system, a process of fermentation is employed for the separation of the fibre; but instead of the steeping being conducted in the open air in shallow pools, it is made a factory operation, and the requisite changes are accelerated by placing the rippled flax in water maintained at an elevated temperature. ‘This method is not new, but had been proposed by Professor Scheidweiler in Belgium, and tried in this country several years before the arrival of Mr. Schenck. It also appears to have been employed by the Malays and the natives of Bengal; but it is to the late THE FLAX PLANT. 283 Mr. Schenck, and his successors, Messrs. Bernard and Koch, that the credit of organizing establishments for working the process is to be ascribed. The advantages which the new system presented were most important :— Ist. By leading to the establishment of factories for the steeping of flax, and the purchase of the crop from the farmer, who would thus be relieved from the trouble of its preparation, it rendered it possible to extend the cul- tivation of the crop beyond the bounds of the ordinary flax-growing districts. 2nd, It introduced greater certainty and ceconomy into the preparation of the fibre. 3rd. It prevented the destruction of the valuable seed, and also increased the per-centage of fibre. With these advantages, as might be expected, the new system made rapid progress, and establishments were erected, not merely in Ireland, but in England and Scotland, and the attention of several Con- tinental countries was also at once directed to it. To enable you completely to understand the system of management pur- sued at these establishments, one of which those interested in the subject will have an opportunity of inspecting in the neighbourhood of Belfast, I shall continue the description of the treatment of the experimental crop, of which I have already given a portion of the history. When the crop had been completely air-dried, by exposure in the field, so as to yield, as al- ready stated, in the straw, when dried at 212°, only 12 per cent. of water, it was removed to the steeping-works at Cregagh. It was there placed in stacks, and after some time prepared for steeping. The first operation for this purpose is the removal of the valuable bolls or capsules. This, in these _ establishments, where the cost of labour is carefully considered, is usually most expeditiously and perfectly effected by means of a machine composed of two massive cast-iron rollers, to which motion is communicated by a belt from the steam-engine. Between these the flax is passed and the capsules bruised, so that the seed can be readily shaken out. Having been deprived of its bolls by this machine, it was found that the 7770 lbs. of flax plants were reduced to 52 ewt., or 5824 lbs. Of the portions of the plant removed by the seeding machine, 910 lbs. con- sisted of clean seed, 1036 lbs. of husks, leaves, and sand. The vats to which the flax is now removed are formed of wood, strongly bound together by hoops, the oval shape being preferred. They are furnished with false bottoms, pierced with holes beneath, through which, by means of a coil of pipe, as re- presented in the drawing, steam is conveyed. The flax having been placed in the vats, with the bundles resting on the butt or root ends, and in single layers, as in the ordinary steeping-pools, a wooden frame is fixed above them, so as to prevent their rising out of the water during the fermentation. The vats are now filled with water, so as completely to cover the flax, and the steam- cock opened so as gradually to raise the temperature to 90° F. The overseers are furnished with thermometers, and instructed carefully to main- tain the temperature at that point day and night. Reckoning from the time at which the steam is admitted to the vats, the duration of the steeping averages about sixty-six hours. When the object is to obtain a very fine fibre, the retting is continued for a longer period. The method of ascer- taining the proper period for the removal of the flax from the water is the same as has already been described as relied on by the common steeper. The loss experienced by the seeded flax in steeping was 13 cwt. Drying.—When the steeping is completed, the flax is carried from the vats to an adjoining apartment of the factory, and placed in layers upon tables, and fixed by women in the drying holders. These consist of two wooden rods, 284 REPORT—1852. 5} feet long, between which a thin layer of flax is secured, by passing metal rings over the ends of the holders, fifty holders being employed for about 1 ewt. of flax. Thus secured, the holders are carried to open drying sheds, and suspended from cross-beams. In three days, in favourable weather, the drying is completed; but in damp weather it is placed in a hot chamber, to heat which the waste steam of the steam-engine is employed. Breaking and Scutching.—As in the patent steeping establishments a sufficient number of skilled workmen could not be at all times obtained, a new impulse was given to the invention of machines capable of performing the work of the hand-scutcher, and several ingenious and beautiful mecha- nical arrangements have been proposed, both for breaking and scutching the flax. In this department Belfast has produced some excellent examples, and the machines of Messrs. M’Adam, Brothers and Co., and of Mr. Richard Robinson, are to be found in almost every flax-growing district both in this country and in England. From the 52 ewt. of seeded straw, the produce of the experimental crop, there remained 6 cwt. 1 qr. 2 lbs. of marketable fibre. After the introduction of the new system, and that several establishments were occupied in the preparation of fibre, objections were made to the quality of the material, and considerable doubts were expressed, both with regard to the amount of produce obtained, and its adaptation for its various uses. These objections, however, were at the time removed by experiments instituted by experienced manufacturers, both in this country and at the admi- rably-conducted works of the Messrs. Marshall in Yorkshire. In Messrs. Marshall’s experiments, samples of the products of which are on the table, flax-straw grown in Holland was the material employed; the steeping of a portion was conducted at two establishments, on Schenck’s system, while another portion from the same lot was steeped in Holland in the ordinary way. The results were regarded as in all respects confirmatory of the supe- riority of the patent process; and a Committee of the Royal Flax Society also reported, that all objections with respect to any injurious influence of the accelerate fermentation on the strength and bleaching qualities of the fibre had been shown to be groundless, and that the yield of the fibre was greater than when “the old, slovenly, and uncertain process of watering” was prac- tised. The process of fermentation, as conducted in the patent establishments, so far as my investigatious have extended, does not appear in any respect to present phzenomena different from what I have observed in the ordinary steeping-pools of the country, when only rippled flax is employed. Usually, in eight or ten hours after the flax had been placed in the vats, a copious extrication of gas is observed, and sometimes the vat becomes covered with a head of froth, like the vat of the brewer; and at this period an odour is evolved in the establishment closely resembling that of the brewery. The gas evolved at this period is chiefly carbonic acid. The liquid at the same time exhibits a slight acid reaction. As the process continues the tem- perature rises, so that an additional admission of steam is seldom required to maintain the liquid at from 85 to 90 degrees. ‘Towards the conclusion of the operation, usually in about 60 hours, the escape of gas becomes less abun- dant, and a covering of slimy matter collects on the surface of the liquid. The steep-water at this period has a light brown colour, is transparent, and closely resembling bitter ale. It is strongly acid to litmus, but the original blue colour of the test-paper is restored on drying. Its taste at first is rather agreeably acid, but followed by the peculiar THE FLAX PLANT. 285 plant-like taste of the flax. Contrary to what has been stated in some reports on this subject, the liquid I found, at the conclusion of the process, yields nearly a trace of acetic acid, and in numerous experiments no trace of the evolution of sulphuretted hydrogen could be detected at any stage of the fer- mentation. When the flax is allowed to remain in the vats after the usual time, a new series of changes, and a fresh and rapid extrication of gas, take place. I have made, during the last three years, numerous experiments with respect to the composition of the steep-water from several establish- ments, and also from the common steep-pools, which afforded me some inter- esting results, and satisfied me that the fermentation which is induced by steeping flax in water resembles the so-called butyric acid fermentation, merely traces of acetic acid, and invariably large quantities of butyric acid, having been detected in every case. In fact, the fragrant butyric ether, so extensively employed in the preparation of pine-apple rum, and in flavouring confectionery, might readily be obtained in large quantities from the stinking waters of the flax-pool. _ Gconomy of the Flax Water.—With regard to the refuse waters of the vats, some years ago, upon the opening of Mr. Schenck’s establishment in Belfast, I made an analysis of the water in which the flax had been steeped, which confirmed the conclusions to which I had been conducted, from my examina- tions of the waters of the country steep-ponds, that an opinion which had been promulgated by scientific authority, of the possibility of restoring to the fields of the farmer all the ingredients abstracted from the soil during the growth of the flax, by means of the steep-water and other refuse parts of the plant, was not, even supposing that these matters could be ceconomically employed as manure, which is impossible, supported by investigations with respect to the amount of fertilizing ingredients which they contained. Chemistry is, I conceive, contributing in no small degree to the progress of agricultural knowledge. It has even already introduced greater ceconomy into many departments of the farmer's business, and has opened up to him new sources of fertilizing agents. Sut in some cases it is to be feared that the chemist has himself raised obstacles to the reception of agricultural science by the practical agriculturist, by proposals which, though capable of being carried out in the laboratory, are totally inapplicable in the great operations of the husbandman. To ascertain exactly the effect produced by steeping, and the composition of the steep-water, I obtained from the works at Cregagh a sample of flax- _ straw unsteeped, a portion of steeped straw taken from the same lot, and a gallon of the steep-water taken from the vat immediately after the removal of the flax. The composition of the ash obtained by burning the extract of the steep-water, and the samples of the straw, is given in the Table. The spring-water employed at the works is moderately hard, indicating, on Dr. Clarke’s scale, § degrees. It was not considered necessary to deduct the in- gredients supplied in it, as these would add but little to its fertilizing value. An imperial gallon of the liquid of the vat was found to contain, in grains and tenths,— Organic matters ............... 136°7 Inorganic matters ............... 131*4 Total solid matters ...... 268'1 286 REPORT—1852. Composition of the Ash of the Flax-straw before and after steeping, and of the Inorganic Matters of the Steep-water. 100 parts of each respectively contained— Unsteeped Steeped Ash of the flax. flax. steep water. Motash ser ee LS 11°40 19°31 ee ee ee ee 5°33 4°17 he Chloride of potassium .... ore ae 3°83 Chloride of sodium ...... 6°47 3°28 21°94 te ee oe ees 18°86 17°69 8:23 Ween aes a 5°50 10°18 Oeide afaron 2. SS SO 5°76 Re) Sulphuric acid): 20) .... ° 11°16 4°07 6°10 Phosphoric acid.......... 9°63 11°87 Stil Carbonic acid’ *..: .. 7... ° 10°37 20:06 23°30 PONGHY. <. . ae 15°23 15°78 1°12 2 Wire Bima fupte a ee aaa & = bi 0°60 100°43 99°58 99°77 Ash per cent. in the straw . . 3°89 2°59 ape 100 grs. of the dried extract of the steep-water contained 1°56 nitrogen, =1-89 grs. of ammonia; therefore an imperial gallon would be capable of supplying 5 grs.; and a vat containing 3000 gallons of water, 251, lbs., worth about 1s. 2d., and would convey to the fields of the farmer about the same weight of phosphoric acid. By the kindness of the proprietors of the Patent Steeping-Works at Cregagh, who have liberally given me an opportunity of inspecting the books of their establishment, I am enabled to give the following average statement of the changes which 100 tons of flax undergo, when treated by Schenck’s process. 100 tons of air-dried flax-straw yield— Tons. 1. By Seeding—33 tons of seed and husks, leaving of seeded flax.. 67 2. By Steeping—67 tons of seeded flax yield of steeped straw .... 39°5 3. By Scutching—39$ tons of steeped straw yield of dressed flax.. 5°90 EUROS IG BS To 17 Seon ee a EERSTE Tv VR 1:47 Flax Cotton—The irregularity in the supply of cotton, the raw material of an important allied branch of English manufacture, and of which it is cal- © culated the mills of the United Kingdom require annually a quantity equal to 1000 tons daily, has at various times suggested attempts to convert our indigenous flax into a form which might render it capable of being spun with the ordinary cotton machinery. It appears that attempts to produce from flax a substance possessing the properties of cotton, were many years ago made by a Swede named Des Charmes, and that in 1775 Lady Moira com- municated to the Society of Arts some experiments which, suggested by those of the Swede, she had made in this country. Her ladyship’s experiments are to us peculiarly interesting, as her letters show that they were carried on at her seat, the present residence of David Ker, Esq., M.P., only twelve miles distant from Belfast. Neither Des Charmes’ nor Lady Moira’s experiments: seem to have led to any practical application of the proposed substitute for the foreign material; and though subsequent trials for the same purpose were made by various persons, the public do not appear to have placed any confidence in their plans. Lately, however, the project has been revived by a Brazilian gentleman, the Chevalier Claussen, known to the public as the inventor of an ingenious loom. This gentleman has been more successful than ~ THE FLAX PLANT. 287 his predecessors in exciting attention, and his processes have been described by several chemists of reputation in England, as affording a new and beauti- ful application of the powers of chemistry to practical purposes. In every part of Europe, indeed, much interest has been excited by the accounts which have been published respecting his discoveries, which were regarded as cal- culated to render Great Britain nearly altogether independent of foreign supplies of cotton. The proposals of M. Claussen were not confined to cot- tonizing flax, but also embraced a method of preparing long-line or fibre for the flax-spinner, substituting for fermentation the more rapid action of a weak solution of caustic soda, followed by boiling, or simple immersion in water, acidulated with sulphuric or muriatic acid. The material employed for the production of his cotton was at first unsteeped flax-straw; but at present I find that the flax in its original state is not used, and that the refuse tow of the scutch-mills is preferred. This limitation of the application of M. Claussen’s patent removes some of the objections which were urged against his original proposal to cut up valuable flax, so as to produce what the opponents of the invention regarded as an inferior article ; now, however, it is merely the waste tow of the scutching-mill, which can be purchased at from £4 to £7 per ton, that is used in M. Claussen’s establishments: and from this, as the interesting series of samples which have been kindly supplied to me by Dr. Ryan show, a beautiful material, capable, it is stated, not merely of being spun with cotton machinery, but of being combined with wool, silk, and other fibres, and exhibiting, apparently, that increased affinity for colouring matters which Mr. Mercer has found to be possessed by cotton fibre, acted upon by caustic alkali, has been obtained. The first operation at M. Claussen’s works is to pass the tow through a carding and hackling machine, for the purpose of arranging its fibres parallel; so straight- ened, it is cut by another machine (somewhat similar in its operations to the chaff-cutter of the farmer) into pieces of about one and a half inch in length, and is then conveyed to the steeping vats. The vats are placed side by side; and by means of a cradle and a travelling railway, the tow can be transferred from one to the other, as required. It is, in the first place, steeped for twenty-four hours in a cold solution of caustic soda, of 1° Twad- del. The next step is to plunge it in another vat containing a similar solution, but furnished with a steam-pipe, so that the liquid can be kept at a boiling temperature for two hours. - The peculiar part of the process, or the Claus- senizing of the tow, is commenced by transferring the material prepared, as described, to a third vat, which holds a solution containing 5 per cent. carbonate of soda. It is allowed to remain immersed about an hour, so as to be completely saturated with this liquid, and is then raised from the vat and placed in a solution vontaining about one-half per cent. of sulphuric acid. In the bath of sulphuric acid it is alleged that important chemical and me- chanical changes are effected in the character of the flax fibre. It is stated that it becomes at once changed, as if “ by a new instance of natural magic,” from a damp aggregation of flax to a light expansive mass of cottony texture, increasing in size, like leavening dough or an expanding sponge; and this material, it is asserted, can be produced at a cost not exceeding 214d. per Ib., which is considerably below the price at which cotton can be grown and imported from the United States or any other cotton-producing country. By a simple process of bleaching, and subsequently “carding,” the tow thus modified assumes both the texture and appearance of foreign cotton, and can at once be employed by the cotton-spinner. With such alleged advantages to recommend it, it was not wonderful that M. Claussen’s proposal attracted the attention and excited the sympathies of Mr. Porter and other eminent ceconomists, and that the late Lord Lieutenant 288 REPORT—1852. of Ireland, the Earl of Clarendon, should desire that a scheme which promised such important results to this country, so deeply interested in the production of flax, should be carefully tested on a proper commercial scale. An inquiry having been committed to Sir Robert Kane, Director of the Museum of (Economic Geology, I was requested, together with Professors Blyth and Murphy of Cork, to make such investigations as might properly ascertain the value of the various methods proposed. But, unfortunately, the mechanical arrangements which had been made by M. Claussen’s agents, to illustrate the production of the new material from unsteeped flax, were not capable of affording satisfactory results; and, though some trials with tow proved more successful, it was found impossible to carry out the object of the inquiry at the locality selected. I am informed that it is the intention of the patentees to solicit a full investigation of the methods pursued in their operations at works which they have established near London, and where, they state, the material is produced in large quantities. The real value however of Claussen’s substitute for cotton must be decided by the ex- perience of the manufacturers of England. With regard to the ceconomy of the processes, it would be improper to give an opinion until the investigation which M. Claussen solicits has taken place. The specimens show what can be made from the waste tow of the spinner; and it is interesting to find both Berthollet and Gay-Lussac, many years ago, pointing out the advantages which appear here to be realized from the conversion of tow into a substitute for cotton. I have now to request attention to a new process, entirely different from any of those which have been described, and the first public announce- ment of which I am permitted by the patentees to make to this meeting. The methods adopted are the invention of Mr. Watt, a countryman and namesake of the great philosopher. In this process neither fermentation nor the action of acid nor alkaline solutions are employed, the separation of the fibre from the useless matters of the straw being effected by subjecting the stems to the action of steam, and afterwards by pressure applied by powerful rollers. In the first place, Mr. Watt proposes to take seeded flax, and to ex- pose it to steam, at the ordinary pressure of the atmosphere, in a close cham- ber, of peculiar construction, so as to soften and dissolve out the gummy and other soluble matters. The chambers which he employs are square vessels constructed of wood, or of plates of cast iron, and provided with false bottoms, formed of the perforated iron plates used in malt-kilns. Two doors are placed in the ends of the chambers, for putting in and removing the flax. The top of each vat is formed of cast-iron plates so arranged as to constitute a shallow tank for containing water, and through which, extending for some inches above the surface of the water, passes an iron pipe, which commu- nicates with the interior of the chamber. To the opening of this pipe a valve is fixed, which can be opened or closed as required. Resting upon the false bottom, there is an arrangement of pipes, which are intended to act like the vomiter, or throw-pipe of the bleacher. The process is commenced by placing the flax in bundles, as received from the seeding machine, on the false bottom, until the chamber is nearly filled. The doors are then secured by screws, and steam is discharged into the chamber by a pipe which passes between the bottoms, and for some time allowed to escape through the valve- pipe in the roof, so as to remove the volatile oil contained in the straw. After some time the valve is closed; and the escape of the steam being pre- vented, it penetrates through the mass of the flax, softening’ and loosening its various parts. Water is now admitted into the metal tank, and the steam, which strikes against the cooled roof of the chamber, is condensed and made to descend in showers of distilled water, by which the soluble and softened THE FLAX PLANT. 289 extractive matters are washed out and carried below the false bottom, and conveyed by pipes into a reservoir and preserved. It is, however, proposed at intervals, during the operation, to allow the flax liquid to accumulate until it rises above the false bottom, and then, by the pressure of the steam, to cause it to ascend in the throw-pipes, and to descend in streams over the straw, so as completely to wash away all the softened matters. In about ten hours the entire operation may be completed, though the patentee regards it advantageous to subject the flax to the action of the steam for from twelve to eighteen hours. The second part of Mr. Watt’s process consists in submitting the straw, as it is removed, softened and swollen, froin the steam chambers to the success- ive action of two pairs of very heavy iron rollers, somewhat resembling the seeding rollers used in the hot-water steeping establishments, for the purpose both of quickening the drying process, and of expressing any adherent colour- ing or glutinous matter. By this operation, also, he finds that not only is the drying facilitated, but that a considerable portion of the enveloping cuticle of the stems is removed, and that the separation of the fibre in scutching is rendered more perfect by the bruising and splitting up of the woody parts consequent upon the longitudinal pressure to which they are exposed under the rollers. This new method, which is in operation at present in the extensive works of Messrs. Leadbetter in this town, appears to offer most striking ad- vantages. It is peculiarly adapted for rendering the separation of the fibre a manufacturing operation. No disagreeable smelling odours are evolved ; and, if experience confirms the expectations of the patentees with respect to the quality of the fibre obtained, and the comparatively low expenditure required in its production, the new process will, in no trifling degree, contribute to the extension of flax cultivation in this country. A striking peculiarity of this process, and one which renders it exceedingly - interesting to the scientific agriculturist, is, that it offers the only satisfactory method of ceconomizing the matters which are dissolved from the flax plant in its treatment. The dark liquid which accumulates in the lower chamber of the vat can be obtained in a most concentrated form; it is totally free from the disagreeable odour of the flax-pool, and experiments which have been tried prove that it is found by pigs a palatable and nutritious food. I have to apologize for the length to which this Report has extended, and I _ feel that some of the details which I have included in it may appear uuneces- sary to those who are familiar with the various process of the flax manufac- ture; but as many persons present, though acquainted with the beautiful fabrics, which, in every market in Europe and America, attest the skill and ingenuity of the linen manufacturers of Ulster, have probably now for the first time visited a district which, like the north of Ireland, on every side exhibits, in its steeping-establishments, busy flax-mills and extensive bleach- _ greens evidences of the advantages which this country has derived from the eultivation and skilful management of the flax plant, I trust, that, whilst in- _ specting the various processes to which our manufacturers have liberally invited _ the attention of the members of the Association, the outline which I have en- _ deavoured to give them of the economy of the crop may tend to increase their interest in this important department of our national industry. And if my remarks on the composition of the plant and the various plans proposed for _ the preparation of its valuable fibre should induce any of those whom I have the honour to address to undertake investigations which may contribute to improve either the agricultural or technical management of the crop, the present visit of the British Association will be regarded, if possible, with still greater satisfaction by the manufacturers of Ulster. 1852. U RESO Pm on % 290 REPORT—1852. The Freshwater Fishes of Ulster, as enumerated in the MSS. of the late Witt1AM Tuompson, Esq., President of the Belfast Natural History and Philosophical Society. Contributed by Ropert Par- TERSON, Esq. and JAMEs R. Garrett, Esq. Tse contributors of this paper stated that they had prepared it from their late friend’s MSS., in consequence of a suggestion which had been made to them, to the effect that an accurate catalogue of the freshwater fishes of Ulster would, on the present occasion, be interesting to many who had not before had an opportunity of observing the physical features of the North of Ireland. The several species of fish which inhabit purely fresh water for at least a por- tion of the year, and which Mr. Thompson had noted as having been found in the province of Ulster, were enumerated thus :— Cobitis barbatula, Linn. Esox lucius, Linn. Salmo salar, Linn. (—— Salmulus.) —— Enox, Linn. —— trutta, Linn, Perea fluviatilis, Linn. Gasterosteus aculeatus, Linn., including the several varieties figured in Yar- rell’s British Fishes, viz. G. trachurus, Cuv. & Val. ——— semiarmatus, Cuv. § Val. _ -—— leiurus, Cuv. & Val. brachycentrus, Cuv. & Val. —— spinulosus, Cuv. & Val. pungitius, Linn. Gobio fluviatilis, Will. Tinca vulgaris, Cuv.? Send ao Cyprinus carpio, Linn. / considered in- ? i digenous, Abramis Brama, Cuv. —— fario, Linn. ferox, Jard. — umbla, Linn. (S. Salvelinus, Don.) Coregonus Pollan, Thomp,. Platessa flesus, Cuv. Anguilla acutirostris, Yarr. —— mediorostris, Yarr. latirostris, Yarr. (2). Petromyzon marinus, Linn. fluviatilis, Linn. Planeri, BZ. Ammocetes branchialis, Cu». Buggenhagii, pond. (Cyprinus ——, Bloch). Leuciscus erythrophthalmus, Cuv. Supplementary Report on the Fauna of Ireland by the late William Thompson, Esq., President of the Belfast Natural History and Philosophical Society. Robert Patterson and James R. Garrett, Esqs., the two gentlemen by whom this communication was brought forward, gave the following explana- tion as to the circumstances under which it was prepared :—At the Meetings of the British Association held in the years 1840 and 1843, Mr. Thompson presented Reports on the Fauna of Ireland, drawn up by him at the request of the Association, Shortly after his untimely decease in February last (1852), his MSS. were—in pursuance of directions contained in his will— handed over to the two gentlemen above-named, with a view to publication, so as to complete his work on the Natural History of Ireland, thrée vols. of which—on the Birds of Ireland—had appeared during the author’s lifetime. On examination of these MSS., a memorandum was found containing a list of the papers which it had been Mr. Thompson’s intention to submit to the Belfast meeting of the Association, and, amongst others, there was specified a supplement to his former reports. The materials of this Supplement were also discovered, partly arranged, and it was considered desirable that the ON THE FAUNA OF IRELAND. 291 author’s intentions should be carried out as far as possible. The remaining volumes of “The Natural History of Ireland” being in course of preparation for the press, the present communication was confined to an enumeration of the several species of animals now recorded as Irish, but which had not been made known at the date of the publication of Mr. Thompson’s previous reports, Div. VERTEBRATA. Class MamMMaAtia. Vespertilio Nattereri, Kuhl, ......... M‘Coy, in Ann. Nat. Hist. vol. xv. p. 270. Delphinus tursio, Fabr. vieseseeseseees Gray, in Ann. Nat. Hist. vol. vii. p. 84. Class Avs. Vultur fulvus, Linn....ccssecccoeeeee Yarrell, Br. Birds, ed. 2. vol. i. p. 1; Thomp. Nat. Hist. Ireland, vol. i. p. 84. Aquila Neeviay Brisson ...sciscocssees «. Yarr. Br. B. vol. i. p. 10; Thomp. N, H. Ire. vol. i. p. 13. Circus cineraceus, Mont, (sp.).+s...... Thomp. N. H. Ire. vol. i. p. 427, Motacilla alba, Linn., Gould .......0. “ >» p. 218 Alauda cristata, Gould........ seesecceee Yarr. Br. B. vol, i. p. 455. Alcedo Aleyon, Linn. ......ccsscccevees Thomp. N. H. Ire. vol. i. p. 373. Hirundo purpurea, Wilson ......... .« Yarr. Br. B. vol. ii. p. 257. Perdix rufa, Mont. s.....ssccccevesesses Thomp. N. H. Ire. vol. ii. p. 65. Charadrius cantianus, Latham ...... 3: » p- 104, Grus cimerea, Bechst. ......secesceeeeee 3 » p13. Botaurus lentiginosus, Mont. (sp.)... 5 » p. 168. Ciconia alba, Brisson .ccccsscescsseeses aes op. 175. Selon Brehmi, Kaup...secccssereess 53 vol. iti. p. 447. inga platyrhynca, Temm. ........04.. es vol. ii. p. 282. — Schinzii, Bonap. ......s.cecseeoee = » p- 297. — Bonapartei, Schlegel. .......0000 ce 32" By OT — rufescens, Vieill. ......00000. soseee M‘Coy, in Ann. Nat. Hist. vol. xv. p. 271, — Temminckii, Leister ............ Thomp. N. H. Ire. vol. ii. p. 302. Crex Bailloni, Vieil/. (sp.) .....0 Cate 3 >» p- 32), Gallinula Martinica, Gmel. ...... Zaades a bh) POOLE Anser Canadensis, Gel. (sp.) ......- a vol. iii. p. 24. — egyptiacus, Linn. (sp.) ......0. wa >» p: 64. Tadorna rutila, Pallas (sp.)...... ee 4 st Ps GB, Anas Americana, Gel. ...........004 i pea ean Oidemia perspicillata, Linn. (sp.) ... 3 » p. 118, Mergus cucullatus, Linn. ....... ooonae re » p. 161. ria leucophthalmus, Faber ......... 3 PAR ie + 1 Sterna Velox, Ruppel ....sssecsssecere 55 » p. 266. _ ——leucopareia, Natterer .......+.... 5 oy =p. 298. _ —— leucoptera, Meissner & Schinz.. M‘Coy, in Ann. N. H. vol. xv, p, 271 ; Thomp. fy N. H. Ire. vol. iii. p. 307. Larus Bonapartii, Rich. & Swains.... Fr » p. 317. _ Procellaria glacialis, Linn. ........+00 5 3 p. 406, Class Pisces. Cottus Groenlandicus, Cuv. § Val.... Specimen in Dublin University Museum, ob- tained by Dr. Ball at Youghal; another procured by Mr. Wm. Andrews from Dingle Bay, Feb. 1850. Sebastes Norvegicns, Cuv. & Val. ... em from Dingle Bay by Mr. Wm. An- drews. , Pagellus erythrinus, Cuv. § Val. .... Taken on south-west coast by the same gen- tleman, u2Z 292 _ * REPORT—1852. Cantharus lineatus, Mont. (sp.) ...... Ann. N. H. vol. xvii. p. 313. Brama Raii, Cuv. § Val....... esp s sagas 5 vol. xv. p. 311. Xiphias gladius, Linn.? ...........0008 55 vol. xviil. p. 314. Cepola rubescens, Linn. .........00006 Obtained by Dr. Farran on southern coast, Dec. 1848. Scopelus borealis, Nillson ..... Str At Ann. N. H. vol xx. p. 171. Platessa limandoides, Jenyns ..... ... Obtained by Mr. W. Todhunter off Cape Clear, in winter of 1848. Pleuronectes Armoglossus, Schn....... Obtamed by Mr. W. Todhunter on Galway coast, Sept. 1848. Solea pegusa, Yarr......... Saree gee Obtained by Mr. W. Todhunter on Galway coast, Sept. 1848. Echeneis remora, Linn. ........000600. Ann. N. H. vol. xviii. p. 314. Syngnathus ophidion, Linn. ......... 55 vol. i. (new series) p. 63. Orthagoriscus oblongus, Schn. ...... Specimen obtained near Tramore (Co. Water- ford), in Sept. 1845 ; now im the Collection of the Dublin Nat. Hist. Society. Acipenser huso, Linn. ......... seoseeee Ann. N. H. vol. xx. (1847) p. 172. Scymuus borealis, Flem.? .........00+ Mr. R. Ball (MS.). Amphioxus lanceolatus, Pallas (sp.).. Ann. N. H. vol. xviii. p. 314. Div. INVERTEBRATA. Moutusca. Testacellus Maugei, Férussac ........ . Ann. N. H. vol. xx. p. 174. Succinea oblonga, Drap....... genetovas a vol. vii. (new series) p. 501. Acteon viridis, Mont. (sp.) .......00. 3 vol. xv. p. 314. Eolis violacea, Alder & Han. ......... . a vol. xv. p. 313. Alderia modesta, Lovén (sp.) ......... Allman, in Ann. N. H. vol. xvii. p. 1}. Idalia aspersa, Lovén (sp.) .......0.005 Thomp. in Ann. N. H. vol. i. (new series) p.63. Polycera punctilucens, D’Orb. ........ my My vol. xv. (1845) p. 313. Doris obvelata, Johnst. .........ec000 as a o p- 311. Ulidiana, Thomp. ....--.2.s2cee- a ss or} p- 312. Aplysia nexa, Thomp. ..........00cc000 mes : tS p. 313: Orbis foliaceus, Phil. .........c..c0c005 dn ws vol. iii. (n. s.) p. 351, Bulleea pruinosa, Clark .......e..ec00- ee = 99 p- 381. Utriculus y EL OWN x osnesceeetee 5 Le vol. xv. (1845) p. 314. Volvaria subeylindrica, Brown ....... = _ Bs p. 315, Cylichna (Bulla) strigella, Loven .... 5 3 vol. vii. (n. s.) p. 501. Bulla mammillata, Phil. ............ e $ % vol. i. (n. s.) p. 351. prodicta, Brows s x scccvecsotess 5 us vo]. xy. (1845) p. 314. Bulla? acuminata, Brug. .........000.+- s : vol. ii. (n. s.) p. 35], Ovula patula, Penn. (sp.) ........+++ aes is a vol. xviii. (1846) p. 384. Pleurotoma Farrani, Thomp. ........ 5 = vol. xv. p. 316. coarctata, Forbes.........seescsees By A vol. xx. p. 174. — striolata, Scacchi .........0 aie es 3 vol. xvil. p. 384. brachystoma, Phitl. ..........0. 40 bt . A p. 384. a OVIPUL RE UE. cee tarerogcessass cece 3 - i323.) pr cea LEVERS HULDES” ©, hile csthsczetentees = 8 vol. xviii. p. 383, Ulidiana, Thomp: .........00600- 4 ms vol. xv. p. 316. Triton elegans, Thomp. ..........006+ 5 id irre poly Fusus Sabini, Gray ..........00.00ee008- te 55 vol. ili. (n.s.) p. 352. Buccinum Zetlandicum, Forbes ...... ss 3 vol. xv. (1845) p. 316. Nassa varicosa, Turt. (sp.) .....-000+++ a A vol. xvii. p. 383. Trichotropis borealis, Brod. § Sow.. a a vol. iii. (n. s.) p. 352. Natica Montagui, Forbes .......0....008 Bs Ss vol. xviii. (1846) p. 384, sordida, amit’, Sisecest. Atees. ss nA a vol. iii. (n. s.) p. 352. Odostomia crassa, Thomp. .......006+- , ® Es vol. xv. (1845) p. 315. -Eulima nitida (Melania), Lam. ...... re i; vol, ili. (n. s.) p. 352. Stylifer Turtoni, Brod......sccsceveees af 55 3 oi p. 351. ON THE FAUNA OF IRELAND. 293 Rissoa Warreni, Thommp. .....+...006. .. Thomp. in Ann. N. H. vol. xv. (1845) p. 315. fulgida, Mont. (sp.).-0..0ssseseee F ivy vol. iii. (n. s.) p. 351. proxima, Alder .scceccssseeeseess a 34 vol. xx. (1847) p. 174. inconspicua, Alder .......sssse++s a fa a p: 173. Costulata, Risso ...cccescseeeeees & fh vol. xv. (1845) p. 315. abyssicola, Forbes ........0s.e+0e at - vol. ii. (n. s.) p. 351. 2% Lacuna Montacuti, Turt..........00000s 5 pe vol. xx. (1847) p. 173. Scissurella crispata, Flem. ......+00++ 4 4 vol. vii. (n.s.) p. 501. Emarginula crassa, Sow. ...... maege des + fe vol. xviil. (1846) p. 384, Puncturella noachina, Linn. (sp.) .... es rs vol. vil. (n.s.) p. 501. Chiton Hanleyi, Bean.............00+0.. 5 4 vol. iil. (n. s.) p. 352. Pecten similis, Laskey ........seeceveses ss 5 vol. xyii. (1846) p. 385, FUCL, Gimeliticescecscevscreccesseccer 4 4 9» . p. 385. Area raridentata, S. Wood ..+......... re &: ae p- 385. Nucula Polii, Phil. ........ccceeeeuceees as vol. tii. (n. s.) p. 352. decussata, Sow. ......++8 Ree wy he vol. xx. (1847) p. 174. Modiola vestita, Phil. .....cccccsseceees s a vol. xv. p. 318. Galeomma Turtoni, Sow.........ceceees 3 vol. iil. (u. s.) p. 352. Montacuta oblonga, Turt. ............ 5 “3 vol. xviii. (1846) p. 385. Lucina lactea, Poli (sp.) ......seeeeee0 * es 3 p- 385. Cardium Loveni, Thomp..........00.0++ a rs vol. xv. p. 317. Ervilia castanea, Mont. (sp.) ......... a e vol. ill. (n. s.) p. 352. Amphidesma intermedia, Thomp. .. 3 6 vol. xv. (1845) p. 318. Tella pygmexa, Phil...........00c0e00 ne % vol. i. (n.s.) p. 63. —- balaustina, Lini.......scesceseceee 3 $5 vol. xviii. (1846) p. 385. Neera cuspidata, Olivi (sp.) ...-..... fs 3 fd p. 385, Teredo bipalmulata, Del. Chia. ...... ps i vol. xx. p. 237. Didemnum gelatinosum, Edw. ...... = A vol. i. (n. s.) p. 64. Ascidia grossularia, Van Beneden ... i 33 re p- 63, — tubularis, Miill. ..........cccec00s 4 4 _ p- 63, virginea, Ford. & Han. ......... s $3 vol. iil. (u. s.) p. 352. Botrylloides rubrum, M. Edw. ...... Ae “ % p: 353. rotifera, Hdw. .....csesesecceeseees we es vol. xviii. (1846) p. 386. — albicans, Hdw........cccccecceseees By 3 $3 p- 385. Botryllus smaragdus, Edw. ..........+. * = vol. i. (n. s.) p. 64. violaceus, Edw. ...ccccssecscecees Ba ps 5 p- 64. Amoroucium albicans, Edw. ......... 3 a 4 p- 64. Aplidium fallax, Johnst. .........0..06 . a vol. iii. (n. s.) p. 352, CIRRHIPEDA. Adna anglica, Leach ....scs.ceseseeeee Ann. N. H. vol. xviii. p. 386. CRUSTACEA. Obisium maritimum, Leach............ Ann. N. H, vol. xviii. p. 386. Stenorhynchus tenuirostris, Leach... Ee vol. xx. p. 237. Eurynome scutellata, Risso............ 5 » p. 238. Polybius Henslowii, Leach ......4..... = vol. xy. p. 319. See PONTE: 65260000048 -sssesegereesnaoes Dr. Scouler, in Ann. N. H. vol. xvii. p. 176. Pagurus Forbesii, Bell..........1.sec00e Dr. Melville, in Ann. N. H. Sept. 1851, p. 236. Gebia deltura, Leach ......6..... cca Ann. N. H. vol. xx. p. 239. Crangon fasciatus, Risso .......sc00s008 5 vol. i. (n. s.) p. 64. — sculptus, Bell ..............000 :... Dr. Melville, in Ann. N. H. Sept. 1851, p. 236. — bispinosus, Bell ...........2c0e00e oe be p- 236, Hippolyte Thompsoni, Bell............ Bell, Brit. Crust. p. 291. — Pandaliformis, Bell..... sostaeene 35 p- 289. Sag This shell has, since Mr. Thompson’s decease, been identified by S. Hanley, Esq. as _ Rissoa Beanii : found in shell sand in deep water,—mouth of Belfast Bay. 294 REPORT=1852. Cynthia —— ? Thomp. (J. V.) ....- Ann. N. H. vol. xx. p. 240. Themisto brevispinosa, Goodsir ...... 5 » p. 240. Orchestia Dee teprscessenttesccuees a 9 ~=«p. 242, Amphithée fucicola, Leach (sp.)...... 4: » p.- 242. — rubricata, Mont. (sp.) ...+.+...00e : » =p. 249. RESET Soe sa ti syeacecuestdgecescaes rr 3 (pe ae Gammarus marinus, Leach ..........+. r » pastes — campylops, Leach ......+...0008 a » p. 242. longimanus, Leach (sp.)......... = >» p- 242. —— punctatus, RIGIINGEs) (ocunsWesveseaes i » p-243. Opis typica, Kroyer .......s00+ eo vescss 3 op. 2438. Anonys GADD) taasaecarteaeceassUeeesoes.e re 3 pe 24a. Teese ater ane Teele eectte takes 5 3 peed: Gaais faleatus, Mont. (sp.) -...++... i » p. 244. Hyperia Latreillii, Edw. ..........00... 54 » p. 244. Galba, Mont. (sp.) .....00sse00ee Ss 5p. 244 Lestrigonus iat Feradacweiatties oeuece OY » p. 244, Caprella lobata, Miill. cohaee Peadctienes a » p. 244, tuberculata, Goodsi7 ..........4. BR. » p. 244. acuminifera, Leach .......seese00e Ad 35 . 245. Idotea acuminatum, Leach? ......... 9 vol. iii. (n. s.) p. 354. Tanais Dulongii, Audouin (sp.) ...... a vol. xx. p. 245. Jera albifrons, Mont. (sp.) ....+2...+0+ “p > p- 245. Praniza cerulata, Mont. (sp.)? ...+.- . vol. i. (new series) p. 65. Spheroma Prideauxiana, Leach...... x vol. xx. p. 245. — Griffithsi, Leach MSS.? ...... sf » p. 246. Cymodocea truncata, Mont. (sp. SS op » p. 246. Cirolana hirtipes, Hdw. .....++-seeees se sp. 246. Eurydice pulchra, WGCQCW ioe ovens snuee on » P- 246. Bopyrus hippolytes, Kroyer ......+.. vol. i. (new series) p. 65. ——— (TEW) ....scereeiersseeerssceeeneees “Foundi : Galathea in Belfast Bay” [Thomps. ny re MSS. Sida crystallina, Mill. (sp.) Edw. ‘O1y) 5) Aleadetopsenoccegie, causecrrmaoess Am RS ne Daphnia crystallina, Mill. Entom. os p: 6 Lynceus lamellatus, Miill. ...... ited: rs vol. xvii p- 386. Cypris reptans, Baird? .....-....066 ey %5 p- 386, Canthocarpus minuticornis, Mill. (sp-) % vol. xx. p. 247. Cetochilus septentrionalis, Goodsir.. i p- 247. Notodelphis ascidicola, Allman ...... . Proc. Roy. Irish Aviad: April 1847. “Caligus minutus, Otto, Nordm.’ BBs bo RAG R Mo. Ann. N. H. vol. xx. p. 247. diaphanus, Nordm. ..........006+ 4 p: 247. —— Stromii, Baird.........ccceceeseees = vol. iii. a s.) p. 354. CUrtUS, KOyer...ccoceeserseeeeeees re vol. xx. p. 247. ——- TAPAX, HAW. \pesedesccsccasaaseesees fx vol. iii. (n. s.) p. 357. m—— Minlleri. cscnsisaracsstestccdtadesees a rs p: 357. — Nordmanni, Edw. ............40. s 9 p: 357. pectoralis, Kroyer ...scccceseeees = vol. xx. p. 247. Trebius caudatus, Kroyer .......064. - » p.248. Chondracanthus gibbosus, Kroyer ... es » p.-248. Lernzopoda galei, Kroyer .........++ is » p- 248. Nymphon Johnstoni, Goodsir......... mr vol. xv. p. 319. —— spinosum, Goodsir ............66 eH ee p- 319. femoratum, Leach .........ss0008 was vol. xx. p. 249. Phoxichilidium globosum, Goodsir.. Ff 3s (Pargeoe Munna Kroyeri, Goodsir.......0....... 5 » p-247. Pasithoe vesiculosa, Goodsir ...,..... a vol. xv. p. 319. gina? longispina, Kroyer... ” vol, xx. p. 245. ON THE FAUNA OF IRELAND. 295: i ANNELIDA. *Udonella caligorum, Johnst.......... Ann. N. H. vol. xv. p. 320. Borlasia alba, Thomp. .......seseseeveee * >» p- 920. octoculata, Johnst. .......s0.see0 ns vol. xvii. p. 388. —— purpurea, Johnst. .....seseeeeees a » p. 388. Olivacea, JOANST. ..scessessevecsees 39 a p- 388. Planaria cornuta. Miill. ...........606 Ae vol. xv. p. 320. VOSCA, Miill......cececccccescscsoees oe » p. dal. lactea, Mill. ....cecesseccecceeees re vol. xvii. p. 388. — nigra, Miill........ (oMeR AEA dy et p- 389. torva, Miill.......... Bou eoadere ° ps a p- 389. flexilis, Dalyell w..ssecccscscecees a vol. iii. (n. s.) p. 354. ANECHUSA, [cdteasseee vec o'eniee adeaces's 8 vol. vii. (n. s.) p. 501. Nemertes melanocephala, Johnst. ... = vol. xviii. (1846) p. 387. Nephelis octoculata, Moquin-Tandon a 4 p: 389. Glossiphonia Eachana, Thomp. ...... = 5 p. 389. Pontobdella levis, Blainville ......... i; ¥ p. 391. Tristoma coccineum, Cu. .......00000 a vol. xx. p. 175. Euphrosina foliosa, Aud. & Edw. ... My vol. iii. (n. s.) p. 355. “ Octobothrium (?) Merlangi_ ...... 356 (Octostoma Merlangi, Kuhn), Nord. 3 a it ForAMINIFERA. Rotalina communis, D’Orb. ......... Ann. N. H. vol. xx. p. 179. Rotalia crassula, Mont. (sp.) ---++.++- » Rawrpry Neel ay Guttulina communis, D’Orb, ......... as f p- 175. Quinqueloculina semilunaris, D’ Ord. as » p.175. “ Quinqueloculina cora, D’Orb..... i \ 175 semilunaris, var.?”” Wood ... a a Pp. Triloculina minuta, Brown (sp.) «+--+ 3 » p- 175. Globulina gibba, D’ Orb. ............ oy fy 3 pleas Spirolina subarcuatula, Mont. (sp.)... S. irecpe fo. Arethusa lactea, Mont. (sp.) «++ week ni » p-l76. ENtTozoa. Tetrarhynchus megacephalus, Rud.... Ann. N. H. vol. vii. (n. s.) p. 501. Echinorhynchus gigas, Rud. ....+.... “ eS p- 501. EcHINODERMATA. Brissus lyrifer, Forbes ....ssseecsseseace Ann. N. H. vol. xviii. p. 393. Holothuria inherens, Miill............ sy ss vol. xv. p. 321. —— niger, COUCH. ...rsecccerserssseseees Obtained by Mr. W. Todhunter on west coast, Sept. 1848. f — Pid aewesaveesoduescinaeaeneWdnne .. Ann. N. H. vol. xvii. p. 393. Thyone raphanus, Duben & Koren... % vol. xx. p. 176. Chirodota digitata, Mont. (sp.) s+... 5A vol. xv. p. 321. Syrinx Harveii, Forbes ........sss000 — granulosus (M*‘Coy in Ann. N. f y vol. xviii. p. 393. H. vol. xv. p. 272) ...... ite aDadesee 2c eiscdtccevsecceensesesceeeees | LWO Specimens found under stones, on beach at Tory Island, by Mr. Hyndman.— Thomp. MSS. | —— Forbesii, M‘Coy ...scescseseseseee Ann. N. H. vol. xv. p. 273. —— tenuicinctus, M‘Coy ......... me > a 76S Sipunculus 2 oc cacamsaenaucdneacena ««. [From Belfast Bay. Intermediate in some respects between the genera Syrinz and Si- punculus.— Thomp. MSS. | * Included by Mr. Thompson amongst the Crustacea in Ann. N. H., but subsequently noted by him as belonging to the Annelida. 296 REPORT—1852. Priapultis ——-? sssssessseeeseeseseeees M‘Coy in Ann. N. H. vol. xv. p. 273. [Not distinct from P. caudatus—W. T.] Seen eee Keen eee eEE OOS eenste eo ACALEPHA. Velella subemarginata, Thomps....... Aun. N. H. vol. xv. p. 321, | ZOOPAYTA. Syncoryna Listeri, Van Ben. (sp.) ... Aun. N. H. vol. xvii. p. 394, Gorgonia verrucosa, RAN: Shicosins cose i vol. iii. (n. s.) p. 356. Turbinolia milletiana, Defrance ...... Bs vol. xviii. (1846) p. 394. Corynactis Allmani, Thomps. ......+++ es ie p- 394. Dysidea? papillosa, Johnst. «..+. «+. 394 (Zoanthus Couchii) ......ssseeeeeeeee 4 PM ae Lucernaria campanulata ......s..e+e08+ W. H. Harvey and W. Andrews, Esqs. Tluanthos Scoticus, Forbes .......++.++ Ann. N. H. vol. xv. p. 322. Alecto granulata, Edw. ...s+0..-ssee+ Bs vol. xx. p. 176. major, JOhnst. .....+--sseees pabbicls 53 vol. ili. (n. s.) p. 357. —— dilatans, JOMNSE. ...0cc..sccscecere = 3 p- 357. Hippothoa sica, Cowch ..+-+-eee+e+++ a vol. i. 33 JapatiDs Cellepora Skenei, Ellis & Soland.(sp.) eS vol. xv. (1845) p. 322. Lepralia simplex, Johnst. --+.+++++++ a vol. iii. (n. s.) p. 357. Hyndmanni, Johnst. ......++++-- - 53 - p. 37. —— granifera, Johist. ....++++eseeee — annulata, Fabr. (sp.) Johnst.... PP es p- 357. == PERCH, JONMSEsn s.-svecnsrecrsceee zs a p. 357. reticulata, Macgillivray ......... —— innominata, var.? Couch. ...... } 357 (description, not figure) Johnst... 4 2 ota Ball, JORNSE.vcacvacessesecsccoces 3 3 p- 357. —— trispinosa, Johnst. sseseeseeeeee Bs = p- 357. coccinea, Abilgaard.....rs0+++++- * 45 p- 357. violacea, Forbes ....+ceessseeeenes : concinna, (Busk MS.) ......... labrosa, (Busk MS.) «..ss0-00... Eschara foliacea .....-.seseeeseeseeeeeee Obtained by Mr. W. Todhunter off Cape Clear, winter of 1848. Retepora cellulosa, Linn. (sp.) «+++. Ann. N. H. vol. xv. p. 322. AMORPHOZOA. Halichondria hispida, Mont. Wern. Mem. vol. ii. p. 86. pl. 5. figures > Dr. Scouler in Ann. N. H. vol. xviil. p. 396. 1&2; Johnst. B.S. p.98 ...... TINGUIATISeaneces pes aee cine se Wedleneeas See Dr. Johnston in Berw. Club, Proc. vol. ii. p- 196. Note.—Mr. Thompson’s MSS. contain references to several sponges in his collection, which he considered to be of species not previously described. They are now in the Museum of the Belfast Natural History and Philosophical Society. ON THE METEOROLOGY OF BIRMINGHAM. 297. Observations on the Meteorology of Birmingham. By Wiuu1aM Wits, Esq., F.G.S. THE accompanying Tables have been compiled from a Meteorological Register kept at the Birmingham Philosophical Institution. The observations for temperature, pressure, rain and wind, extend over a period of eight years, from 1837 to 1844 inclusive. The dew-point tables embrace a period of five years, from 1838 to 1842 inclusive ; and the evapo- ration tables the two years of 1843 and 1844 only. The whole of these observations, with the exception of those for the four months from August to November 1844, were made by the late Dr. Ick, the Curator of that Institution, whose accuracy as an observer is well known; the observations for the excepted months were made by a gentleman who acted as his sub- stitute during his last illness, and continued to do so for a short time after his death, and as they bear internal marks of care and accuracy, I have not hesitated to ineorporate them with those of Dr. Ick. This Register came into my possession during an official connection with - the above-mentioned Institution, and from the care with which it appeared to have been kept, the long period over which it extends, and the importance of Birmingham as a meteorological station, it occurred to me that a reduction of the recorded observations was likely to repay the necessary labour, and that the results would probably form an acceptable contribution to this de- partment of knowledge; and the rather so, that with the exception of Mr. Osler’s papers on the winds, contained in the Reports of the Association, I am not aware of the existence of any long-continued series of trustworthy observations on the Meteorology of Birmingham. I will briefly notice the subjects of these observations, and recapitulate their chief results. 1. Temperature (Tables I. ty VII.).—The instruments were placed in the shade, for the first two years 43 feet, and subsequently about 38 feet above: the ground, and about 437 and 470 feet respectively above the mean level of the sea, the place of suspension being nearly in the centre of the town of Birmingham. In consequence of breakages, the same instruments were not employed throughout the whole series of observations, so that it has not been possible to submit them to verification. The self-registering thermometer was of Rutherford’s construction. The mean monthly and annual temperatures are deduced in Tables I., II, III.,—first, from continuous daily observations at 9 a.m. and 3 p.m. local time ; secondly, from the highest and lowest daily markings of the self-regis- tering thermometer ; and thirdly, from the highest and lowest annual indica- tions of the same instrument. The mean annual temperature for eight years, as deduced,— Ist. From the daily observations at 9 a.m. and 3 P.M.,is........ 49°90 2nd. From the highest and lowest daily observations of the self- registering thermometer....... so SATE, dL See ike PRR eases’ AO*17 3rd. From the highest and lowest yearly observations of the self- registering thermometer........... babys hh REISE 50°00 4th. The mean temperature of the five years, from 1838 to 1842 inclusive (see Table XXI.), which excludes the year 1837 and the unusually warm years 1843 and 1844, is........ 49°694 Of these amounts some portion is doubtless due to the great number of our manufacturing and domestic fires. In Table IV. is shown the distribution of the temperature through the several meteorological seasons, with the differences from the mean. 298 REPORT=~1852. The Tables III., V., VI. exhibit the mean range of the self-registering thermometer through the several years, months and seasons, with the differ- ences from the seasonal and annual means. The mean annual range of temperature is 64°°25, and the mean monthly range 32°51 ; while the greatest monthly range, that of April, is 6°49 in excess, and the least monthly ranges, namely, those of November and December, are severally 4°95 in defect from the general mean. - In Table VII. is given the number of days on which the self-registering thermometer was at or below 32°; the average yearly number being 53. 2. Barometric pressure (Tables VIII., IX., X., XI.).—The instrument employed was a standard barometer of Newman’s construction, of *546 in. bore, with moveable brass scale, and which had been compared with the flint-glass barometer at the Royal Society’s rooms. The cistern was 18 feet above the ground, and about 44:7 feet above the mean level of the sea. The Tables VIIT., [X., X. exhibit the mean monthly and annual barometric pressure, deduced from observations at 9 A.M. and 3 p.M., corrected for tem- perature, with its distribution through the several meteorological seasons, the corresponding barometrical ranges, and the differences of pressure and range between each season, and the general mean of the several seasons. The mean annual barometric pressure is 29'381 inches, from which the greatest yearly difference in excess is +°084 in., and in defect —109 in. In Table XI. is shown the mean monthly and annual pressures as derived from the highest and lowest of the pressures at 9 A.M.and 3p.mM. The mean annual pressure thus obtained is 29:303 in., differing from the mean of the two daily observations by ‘078 in. only. In the synoptical Table X XI. the barometric pressure is resolved into its gaseous and vapour constituents; and their mean monthly amounts, shown for the period of five years, comprised in the dew-point register, namely, from 1838 to 1842 inclusive, with their respective differences from the several annual means :— Inches. The mean annual gaseous pressure is...... 29°065 Ditto vapour pressure ...... 0... 026000 ee "324 Total pressure (from 5 years’ observations)... 29°389 This result differs from that obtained from the mean of the daily obser- vations for eight years by only +-008 in. 3. Rain (Tables XII. to XV.).—The receiver of the rain-gauge was placed 38 feet above the ground, and about 470 feet above the mean level of the sea. The quantities which fell were registered daily at 9 a.m. The average annual amount was 25°258 in. The tables show the distribution of the aggregate annual amounts through the several months and meteorological seasons, with the differences from the means; and also the number of days on which rain fell in each year and season, and their mean monthly and annual numbers. The greatest excess in any year above the average amount was in 1839, when it amounted to about +3°907 in., and the greatest deficiency in 1844, when it amounted to —5:332 in., making a total difference between the two years of 9269 in. The mean monthly quantity is 2-105 in., which, on the average of eight years, is exceeded in November, February, July, August, September, and October, in the order of enumeration, The smallest monthly amount falls in April, and next to that month, in December, after which fol- low, in order of dryness, March, May and June, - The greatest quantities of rain fell in the several seasons in the following order, namely, autumn, summer, winter, spring, ON THE METEOROLOGY OF BIRMINGHAM. 299. 4, Dew-point (Tables XVI. XVII.).—The dew-point register extends over five years, from 1838 to 1842 inclusive. The Table XVI. shows the monthly and annual means as derived from observations made daily at 9 a.m. and 3 P.M. with Daniell’s hygrometer. ’ The mean annual dew-point from Table XVI. is 44°95, while the same result deduced in Table XVII. from the highest and lowest monthly dew- _ point at the above-mentioned hours is 44°18. : Adopting the first quantity, 44°95, the mean annual dryness of the climate of Birmingham is 4°95, and its mean humidity (complete saturation being represented by unity) is =0°707 ; and consequently the weight of vapour in a cubic foot of air is =3°03 grs., and the quantity required for saturation about 1°28 gr. 5, Evaporation (Table XVIII.).—The amount of evaporation is recorded _ for two years only, namely, 1843 and 1844; and was registered daily at 9 a.m., by Howard’s evaporation gauge, which was placed 37 feet above the ground. In 1843 the greatest amount took place in the months of June, July and August, and the least in February ; while in 1844 the greatest amount took ~ place in the months of May, June and July, and the least in December. : The total amount of evaporation was, for 1843, 32°166 in., and for 1844, _ 85°113 in. 6. Winds (Tables XIX. XX.).--The Table XIX. records the direction of the winds at 9 a.m., through the several months of the years 1837 to 1844 inclusive; Table XX. being a summary of the aggregate number of the several winds throughout that period, with the corresponding barometric _ pressures, reduced to 32°, with their variations from the mean. The mean of _ the barometric pressures at 9 A.M. was 29°403 in.; differing only by +°014 in. from the mean of the observations at 9 a.m. and 3 p.m.; and the forces, as shown by the pressures, balance each other to the hundredth of an inch. The prevailing winds at Birmingham are from the S.W., S., and S.S.W. in - the order indicated. Of 2914 registered winds, not fewer than 906, or nearly one-third, blew from those quarters alone; namely, from the S.W. 341, from _ the S. 300, and from the S.S.W. 265. _ It is an anomalous fact, of which I do not understand the cause, that the _ barometer is lower with the S.E. than with the S.W. winds, the mean pres- & * — sure with the S.E. winds being 29°191, and with the S.W. winds 29347. ~ Conelusion.—In the synoptical Table XXT. the meteorological elements of ~ temperature, pressure, and dew-point, during the five years for which the “materials of comparison exist, are brought into juxtaposition; and in the ap- pended curves (Plate V.) these elements are represented graphically. sila It is not my intention to enter into any enumeration or discussion of the _ Many interesting deductions suggested by the before-mentioned tables. I _ May, however, remark, in general, that they exhibit some important results in comparison with similar tables constructed from data derived from other ~ localities, and show a marked difference between the climate of the south- western and other parts of our island and its interior; and illustrate, more- over, the influence of situation and local circumstances, even at moderate distances, in modifying the general laws of climate, and their influence on human health, longevity, and enjoyment. _ The striking accordance of form between the accompanying curves and ‘similar ones formed by numerous observers, from facts obtained at different ~and widely separated places, is strongly corroborative of the simplicity, uniformity, and universality of the laws by which the great agencies of me- teorologic change are restrained from destructive irregularity and excess, ~ and controlled and adjusted, with the nicest exactness, to the exigences of animal and vegetable existence. ; Ti —_— a 4 300: REPORT—1852. Tasie I.—Mean Monthly and Annual Temperature from daily observations 4% Differences from Years. Dec. Jan. Feb. Mar. April. May. June. —— | | | um | | | ° °o 1937. | 38:73 | 3830 | 43:34 | 37-03 | 42:02 | 5215 | 63-43 1838, | 40°72 | 29°34 | 3286 | 42°38 | 4485 | 53:18 | 59:58 1939. | 39°81 | 37-92 | 41°32 | 41°32 | 47:88 | 57-00 | 56-47 1840. | 38°94 | 40°12 | 39°73 | 42-22 | 54°61 | 55°67 | 60°71 1841. | 35°19 | 35-41 | 37°12 | 49°21 | 49°31 | 59°55 | 61°73 1842. | 40°81 | 33°80 | 41°01 | 45°38 | 51°10 | 55°34 | 61-06 1843. | 4670 | 39°64 | 36°74 | 43°03 | 49:26 | 52-41 | 57°26 1844. | 4549 | 40°56 | 36°27 | 41-75 | 54:83 | 54°73 | 61°53 _—— | ——$—— ————— Means...| 40°924 | 36°886 | 38°548 | 42°79 49232 | 55°003 | 60°221 Tase I]—The Highest and Lowest Monthly Temperature by the Self- Monthly and Annual Means, and the Dif- 1837. 1838. 1839. 1840. Month . High. | Low. | Mean. | High.| Low. | Mean.| High. | Low. Mean. | High. | Low. | Mean. |} ° ° Dec...) 55°0 | 23-00 28-00 | 3850 | 52-00! 28-00] 40-00 |p Jan....| 51:0 | 25°50 20:00| 35°50| 54:00| 22-00| 38°00 |f Feb. ...| 54:0 | 28°25 22:50 | 38°75 | 51°50} 25°00 38°25 |e Mar...) 49:0 | 19-00 29-00 | 38:50| 57°50] 25-00| 41°25 If Apr....| 58:5 | 27°50 27°50| 49°75 | 81:50] 33°50| 57°50 May ...| 69:0 | 34:00 30°50 | 54:25 | 74:00] 38:00] 56-00 § June...) 79°0 | 39-00 41°00 | 59°50| 80°50] 43-00] 61°75 July ...| 79-0 | 47:00 45°00 | 60:50| 75°50] 46°00| 60°75 §/ 42°50 | 60°75} 82°00] 46°50) 64°25 # 42°50| 56°25] 74°00| 38°00] 56009 36°00] 51°00] 60:00) 34:00} 47-00 30°00] 42°50} 58°50) 27°50} 43-00% Aug....| 76°0 | 44°50 Sept ..| 67°5 | 42°00 Oct. ...| 68°5 | 33°00 Nov..-.| 56°5 | 27°50 Means.| 63°6 | 32°52| 48°05) 63°16| 31:96] 47°56] 65°58 | 32-04] 48°81 | 66°75 33°87 | 50°31 Diff. fr.|An. M. —1:12 —1°61 —0°36 +114 Mean of the 8 years 49°°17. Tasrez III.—Showing the Highest and Lowest Temperature of each yea the Means d 1837. 1838. 1839. 1840. Highest ...... 79:0 June 23. 73-0 August 27. 79:0 August 2. 82-0 August 9.) Lowest ......| 190 March 24. | 9°0 January 20.| 20°0 January 30.} 22°0 January € Mean Temp...| 49°0 43°5 49°5 52°0 Ann.Range.,.| 60°0 69:0 59:0 60°0 » Mean of the extremes of Temperature 50°. ON THE METEOROLOGY OF BIRMINGHAM. 301 ~ t 9 A.M. and 3 p.m. for 8 years, from 1837 to 1844 inclusive, with the he General Mean. July, | Aug. | Sept. Oct. Nov. {Annual Means,|Differences from Annual Means. 65°43 | 62°61 | 56:61 | 53-23 | 45-37 49-604 — *299 62°03 | 61:54 | 57:38 | 51-40 | 41°62*| 48-073 —1°830 62°93 | 62°02 | 57:86 | 51-45 | 45-43 50°117 4-214 59°57 | 65:62 | 54:85 | 49:59 | 44-08 50°392 + +489 59°85 | 61°63 | 59°93 | 49-26 | 42:12 50°025 + +122 61°85 | 61-16 | 57:85 | 46°88 | 42-62 49-905 + -002 61°28 | 63:12 | 61-79 | 47-31 | 43-60 50°178 +4 275 63°06 | 59:59 | 61:06 | 49-75 | 42-61 50-935 41-032 62:00 627161 | 58°416 | 49-608 | 43-056 49-903 egistering Thermometer for 8 years, from 1837 to 1844 inclusive, with the erences from the Mean of the 8 years. 1841. 1842. High. | Low. | Mean. | High.| Low.| Mean. | High. 23-0 | 37-25 | 51:50] 23-00] 38-75 | 58-00 120 | 31-00 | 42:00] 21-50! 31-75 | 53°50 17°5 | 35°00: | 53°50! 25-00] 39-25 | 48°50 320 | 49°75 | 57-50] 31-50] 44:50 | 62-00 340 | 52°50 | 76:50] 30-:00| 53-25 | 67-00 40°0 | 62:50. | 70-00} 39:50] 54-75 | 70-00 40°0 | 56-25 | 85:00] 44:00! 64:50 | 71-50 445 | 59:25 | 76:00] 45-00| 60-50 | 78:00 45°0 | 61°50 | 86°50] 45-00! 65-75 | 82:50 39°0 | 60:00 | 77-00; 42-00| 59-50 | 79-00 360 | 47°50 | 58-00| 29-00| 43°50 | 64:50 22°0 | 39-25 | 52-00] 32:00! 42-00 | 55-00 66°62 32°0 49°31 | 65°46] 33°87] 49-66 | 65-79 |. +014 +0°49 bt ? fom 1837 to 1844 inclusive, by the Self-Registering Thermometer, with uced therefrom. 1842, 1843. 1844. 865 August 18. | 825 August 18. | 95-0 July24&Sept.l. 185 February 16. | 21:0 February 23. Mean of the yearly Range 64°25, 302 - REPORT—1852. Tas_LE [V.—Temperature of the Meteorological Seasons, and Differences = from the Means for 8 years, from 1837 to 1844 inclusive. Difference Difference Difference Difference Years. | Winter.} from | Spring. from |Summer.| from |Autumn.} from Mean. Mean. Mean. Mean. > —_—— — ——__——— ° ° ° ° ° fe} fe] ° 1837. 40°45 +1:67 43°73 —5°28 63°82 +2°36 50°40 +0°05 1838. 34:30 4°48 46°80 —2°21 61°05 —0°41 50°13 —0°22 | 1839. 39°68 -+0°90 48°73 —0°28 60°47 —0°99 51°58 +1:23 { 1840. 39°59 +0°81 50°83 +1°82 61:96 +0°50 49°17 —1:18 { 1841. 35°90 —2°88 52°69 +3°68 61°07 —0°39 50°43 +0°08 | 1842. 38°54 —0°24 50°60 +1°59 61°35 —011 49°10 —1:25 © rf 1843. 41°02 2°24 48°23 —0°78 60°55 —0°91 50°90 +0°55 | 1844, 40°77 +1:99 50°43 +1°42 61°39 —0:07 51:14 +0°79 ye pe Ae Eee ne eee see | | ae eee Means...| 38°78 |... 49°01 | wes. 6146 |. 50:35 } Mean Annual Temperature 49°-9, Means of the Seasons. Difference from Mean of the Year. Winter ciccccrsssecses 38°78 Winter ....ssceee0e 1112 Spring .....ccecuecee 49°02 Spring ....scee — 89 Summer j.cecrseres 61°46 Summer .iosee 1156 Atttumn,,...¢ccc..:008 50°35 Atttumn.......6 45 TasLe V.—Monthly Range of the Self-Registering Thermometer for 8 years, from 1837 to 1844: inclusive. Month.| 1837. 1838. 1839. 1840. 1841. 1842. 1843. 1844. |Means. — | |. ° ° ° o ° ° ° Dec....} 32°00 | 27:50 | 27:00 | 24:00 | 30:50 | 29:50 | 26-00 | 24-00 | 27-56 Jan....| 25:50 | 37:00 | 31:00 | 32:00 | 38:00 | 20:50 | 27:50 | 29:00 | 29-93 Feb. ...| 25°75 | 23:50 | 32:50 | 2650 | 35:00 | 28:50 | 30:00 | 25°50 | 28-40)» Mar.,..} 30°00 | 33-00 | 3300 | 32:50 | 35:50 | 26-00 | 36-00 | 30°50 | 32°06) Apr....| 31-00 | 34:50 | 44:50 | 48:50 | 37-00 | 4650 | 38-00 | 32:50 | 39-00 May |..| 35°00 | 40°00 | 47:50 | 36:00 | 45-00 | 30:50 | 33-00 | 39-00 | 38-25 June...) 40-00 |32:00 | 37:00 | 37:50 | 32:50 | 41-00 | 29:50 | 39-00 | 36-06 July ...| 3200 | 25:50 | 31-00 | 29:50 | 29:50 | 31:00 | 32-00 | 37:50 | 31-00 Aug....} 3150} 3300 | 36:50 | 35°50-} 33-00 | 41:50 | 36:50 | 38:00 | 35-69 Sept... 25:50 | 28-00 | 27:50 | 36-00 | 42:00 | 35-00 | 42:50 | 45-00 | 35-20 Oct. |..| 35°50} 29:50 | 30-00 | 26-00 | 23-00 | 29:00 | 33:50 | 29°00 | 29-43} Nov ..| 29:00 | 31°00 | 25°00 | 31:00 | 34:50 | 20:00 | 25-00 | 25:00 | 2756 me | a ts | ee | a | | | RS | RS | SR! Means.| 31:06 31:21 33°54 32°92 34°62 31°58 32°46 32°75 | 32°51] ON THE METEOROLOGY OF BIRMINGHAM. 303 Tasre VI.—Range of Temperature in the several Meteorological Seasons from the Self-Registering Thermometer, and Differences from the Means for 8 years, from 1837 to 1844 inclusive. Difference Difference Difference Difference | Years. | Winter.| from | Spring. | from |Summer.| from | Autumn. Mean. ~ Ree ae ag aI a 44441111 KAaAKsarnsan Mean Range of the four Seasons 42875. Mean Range of each Season. Diff. from the Mean Range of the four Seasons. Winter .......00000.. 35°0 Winter .....c000.. —7°875 Spring c..sccccccsrere 49°5 Spring ..seseesveee —+-6°625 SUMMEF,......ss000002 39'S SumMELsresee..e046 S875 Autumn....sseeere we 475 ‘ Autumn.,..c.0008 +4°625 1 ene Taste VII.—Number of days in each year, from 1837 to 1844 inclusive, in which the Temperature was at or below 32°. Months. 1837.| 1838.| 1839.} 1840.] 1841.} 1842.) 1843.| 1844, ee December ....| 9 | 7 9 | 12 | 18 6 2 1 January ssc) 9 26 18 9 16 21 9 6 February.......+: 5 23 8 12 13 ¥) 16 20 March,.s.sssreene} 20 3 10 13 1 1 10 8 April ...sseyeeee| 15 6 7 4 5 May 8800, A) 5a oTReh, 5 ses ait nu iv 1 ; October cesreseee} ase ee Ds Ss Ga 3 5 1 November .....- 4 9 1 4 8 1 3 5 304 REPORT—1852. TasLe VIII—Mean Monthly and Annual Barometrical Pressure, from ob- (corrected for 1837. 1838. 1839. 1840. , Months. ———— SS eee 9 a.m.|3 p.m. |Means.| 9 a.m. ! 3 p.m. |Means.| 9 a.m. | 3 p.m. |Means.| 9 A.M. | 3 P.M. |Mear jin. in. in. in. in. in. jin. in. in. in. in. in. | December ......|29°227 |29°245 |29°236 |29°349 |29°367 |29°358 |29-464 |29-452 |29-458 |29°123 |29°109 |29:] January ........- -402| °392| °397| °378| °376| °377|.-360} +127] -243/ ‘177; 034) 279| +264) -271| °247| °199| -223] -517| °513| °515| °504| 464) -4 May .cisooress..| °415}] °390 -402| °356| °339) °347| -409} -402} -405] °383) °359] °3 June ..cce0s....| °469| °446| -457| °296| +281] +288] -383] 335] °359] °510} °502| ‘9 JUlyy hecevtee.. -434| -408| -421| °399| -406} °402]- -273| -340| -306| -408 *394| “4 August ..........) *406] °434) -420| 402) -321 *361| -414| +396] °405 | 494) °445| *4 September ......| °362| °277] °319| °415| -434) *424|) +033) 028 030) +369) °319) * October .........) °574| °530] °552 |29-428 |29°383 |29-405| +425) -424| -424| °575| °552] ‘5 November ......{29°275 |29°252 |29°263 ee 28-980 |28:831 |29°118 |29°100 |29°199 29°21) 29°137 |29°1) Annual Means 29:377 29:272| * 29-322 29'3 Diff. from Mean —-004 | —-109 —-059 Taste IX.—Barometrical Pressure iu the several Seasons, with the Differ- ences from the Mean for 8 years, from 1837 to 1844 inclusive. Difference Difference Difference Difference Years. | Winter.| from Spring. from |Summer.} from |Autumn.| from Mean. Mean. Mean. Mean. | ——$<$——= | —$—$—— | —_—. in. in. in. in, in. in. in. in. 1837. | 29°331 —*029 | 29°367 —'046 | 29°422 +:'004 | 29°378 +:044 1838. *256 —'104 261 —'152 *350 — ‘068 *220 —'114 1839. 361 +:001 384 —029 Bia) —'065 "188 —'146 1840. 186 —'174 “518 +:°105 "450 +032 “361 +027 1841. “462 +102 “410 —'003 *430 +°012 232 — 102 1842. "412 +:052 “431 +018 544 +°126 “401 +067 1843. °340 —-020 *378 —*035 *455 +:037 *457 +123 1844. | 29°531 +174 | 29558 +'145 | 29°339 —'078 | 29°434 +:100 — | | | 2 | | | | | rrr Means...| 29°360 | ....- 7 Be I a Te 29°418 waded 29°334 Mean of the 8 years 29°381. Means of the Seasons. Differences from Mean of 8 years. Winter............... 29°360 Winter.....seoss.0.0. "O21 Spring ..t2--...00-... 29:413 Spring ........ see +7032 Summer .........00- 29-418 Summer ......e00.-- +037 ] ON THE METEOROLOGY OF BIRMINGHAM. | 305 ervations at 9 A.M. and 3 P.M. daily, for 8 years, from 1837 to 1844 inclusive Temperature). : 1841. 1842, 1843. 1844. Means. M. 3 p.m. |Means.| 9 a.m. | 3 p.m. |Means.| 9 A.M. | 3 p.m. |Means.| 9 a.m. | 3 p.m. (Means. Se ee | eT en | en ne OS Ee ay ” 29°689 |29°692 29-257 |29-188 |29°222 /29°644 29-657 29-650 |29-894 |29-889 |29-891 [29-457 |29-449 |29-453 838) “342° -588| +544) -566/ +126) +273] +199] -562| +547] +554] -369| -329| -348 HD) °338/ °343) 467) -431| -449| -197/ +143] -170| +163] -133| -148] -284| -269| -277 4) 401) +422) +406) -377/ -391| +502| -485| -493) +267] -386/ +326] -402| -399| -400 7 | °886) “411 +318) -595/ +456) -319/ -310/ -314| -682) -646| -664/ -413| -422| -417 M4} 389) 396° +452) -439| -445/ -335/ -318| -326| -699| -671| -685| -431| -413| -499 | 481) *504) -588/ 551) +569) -408) -387| -397/ -493/ -466| -479| +459] -431| -445 WD) 379) °369) -497) +499; -493/ -503/ -456| -479! -455| -434| -444| -416| -414| -415 9) 419) 416) 581) -550/ +570) *507/ -470| -488| -055| +133! -094| -409| +396] -403 I) 274) -291| +442) -393/ -417) -739/ -718| -728| -593| -900] +746| -408| -418| -413 BS) 152) 115) +556) +534] +548) -262| +264] -263} -215| -210] -212| -389| +381] -385 29°280 |29°289 29-249 29:225 |29:237 |29-397 |29-366 |29°381 |29-356 |29-335 |29-345 |29-323 |29-335 |29-304 E 29-382 29:447 29°407 29-465 |Final Mean. .....29:381 i +:001 +:066 +026 +:084 Taser X.—Range of Barometrical Pressure in the Meteorological Seasons, as observed at 9 a.m. and 3 p.m. for 8 years, from 1837 to 1844 inclusive, and Differences from the Means. Difference Difference Difference Difference Years. | Winter.| from Spring. from |Summer.| from |Autumn.| from Mean. Mean. Mean. Mean. f in. in. in. in. in. in. in. in. 1837. 1-587 —°263 1134 —'172 1403 +273 1894 + °270 1838. 1°843 —007 1-732 +426 1°158 +028 27028 + *404 1839. 1:599 —'251 1°233 —'073 1°055 —'075 1°424 — ‘200 1840. 1:988 +:138 1°303 —°003 1-250 +120 2°299 + °675 1841 1806 —044 1:266 —-040 1:116 —'014 1661 | + -037 | 1842, 1°699 — ‘151 1361 +°055 ‘918 —'212 1°784 + +160 | 1843 27401 +°551 1:125 —'181 1075 —*055 1459 — °165 id 1844, 1881 +'031 1-298 — 008 1-069 —°061 “444 —1:180 | Means hk 17) ane SRG ee 8s. ja ee ee ee 1624 | Mean Annual Range 1-477. 1. i i Means of the Seasons. Differences from Mean Annual Range. = a en 1850 5 a +373 RS 1:306 Spring,’ ¥it.ts.... —171 ry Summer............00 1-130 Summer ............ —'347 nang Antamn .).400.4i... 1624 Autumn ......086... +:147 x 306 Tasie XI.—Mean Monthly and Annual REPORT—1852. Barometric Pressure, deduced from for 8 years, from 1837 to 1844 in- 1837. 1838. te aa oe Months. 9 A.M. 3 P.M. 9 A.M. 3 P.M. High. | Low. | Mean.} High. | Low. Meal High. | Low. | Mean. | High. | Low. | Mean. ee ee ee eS in. in. in. in. in. in. in. in. in. in. in. in. 9 Det. ...5<- 199-800.|28°520 |29°160 |29°837 |28-453 |29°145 |29-924 |28°723 29°323 |29°931 |28°675 |29°303 Jan. ...... 30:030| -793| °411| -997| °700| :348| -865| -824 |29°344| 835} 809 "322 | Feb. ...... 29-883| -645| °264| °784| 443] °113} *868) -088 28:977| °833| °181| *007 March *871| -748| -309| °867| °747| °307| -941) 503 \29°222 *907| °534 |29°220] April +881 |28:846| -°363| °878\28°755| °316| °698/ °620| -159 "624| +209 |28:916 | May ...... -778 |29-034| -406| °783/29°'129| -456| -828| -920| “374| °786| 962 29°374 June...... -799 29:021| -410| -743|29°015| °379)| +700 [28-973 336 °690|28:983} °336 July...... -776 28-669 | °222| °780 28-453] -116| 656 29:066| 361 645 |29°012| °328 AUg....++- *856| -903| °379| °813| °883| °348| °645|28:542| -093 “601 |28°573| +087" Sept...... 29°803! +533) °168|29°781| -520| +150) :937| -695 *316| °915| °652) 283) Oct........30°137| °730| °433/30°114| 558 *386| -929 128705 29:317| °898 \28°795 |29°346 ° Nov....... 29-803 28-395 |29-099 |29°798 28-243 29-020 |29°879 oe 28-894 |29°844 |27:969 |28-906 . Annual M eans......... 29°302 29°257 29°226 29°202 Diff. fom Fi Mean —00i —°046 —077 —'10P TaBLe XI.—_ 1841. 1842. Months. 9AM 3 P.M. 9 A.M. 3 P.M High. | Low. | Mean. | High. | Low. Mean. | High. | Low. | Mean. | Iigh. | Low. | Meam a a ST a =e SS SS eS in. in. in. jin. in. ‘in. in. in. in. in. in. in. December. ...|30°257 '28°716 29-486 |30°199 |28°789 |29°494 29-726 |28°519 |29°122 |29°717 \28°469 |29:0 29:970| 451) -210;29°979| °519) °249|30°097) “754 425 |30:097| +398 29:993| °557| °275| ‘944] °599| +271 |30°092 *680| °386 30-044} 636) “34 30°044 | “778| 411) -983| °879| -431 29°896| °787| °341)|29°878| -889 8 29°786 | 921) °353| °770 -961| °365(29°955] -°872| °413| -900| -884/ 39 296 28°766, -296| -819 28677) +248 |30:021 28-660! +340) 961 /28°692| °32 933 29°057 -495| °878|29°019| 448 29°874 |29-177| 525} *802 29°072| 46 Jaly..oseevstt er} O49 '28'817| -268| °718|28:-962| °340| -952} °108| 530 ‘962| °093| 52 August.....-.4. -834| .-953| -393| °782)29°080| -431| 990 |29:287 *638| °944|29°202| 57] September ...| °726] °623| :174| °691 28-752 +221 29-831 |28°841| °336 |29°802 |28-958 | “38 October ...... 743) °345| -044| °579| +454) °016 (30-095 *320| °207/|30°064| °415| °2é November ...|/29°975 |28°314 29°144 |29-934 imal 29170 |30 096 a 29:204 30:028 |28°329 |29:1 Ann. Means...|..-...-00.+ 29°296 29°307 29°372 | 29°34 Diff. from Final Mean —'007 +004 +:069 +0 PPM eae x ss ON THE METEOROLOGY OF BIRMINGHAM, “the Highest and Lowest Monthly Observations at 9 a.m. and 3 P.M. _ clusive (corrected for Temperature). 307 daily i 1839. 1840. ‘ 9 A.M. 3 P.M. 9 A.M 3 P.M igh. | Low. | Mean. | High.| Low.| Mean. | High.| Low. | Mean. High. | Low. | Mean. n. in. in. in. in. in. in. in. in. in. in. in. 29°874 |28°755 | 29°314- |29-941 28-788 | 29-364 |29-761 \28:545 29°153 |29°741 |28°573| 29°157 992] -393 192 “989 | +463 *226 |29°852| +568 ‘210 "867 | *236 “051 | 9855] -848 351 *872| °855 363 |30°029 28-089 059 |29°999 |28-041 “020 593) °797 “195 083 | +765 174 |30°076 |29-258 *667 |30°050 |29-230 640 998} °810 “404 955] °813 "384 |29°760 |29-064 "412 |29°756 |29:079 “417 695} °851 273 *694) +825 259 ‘916 |28°820 *368 908 |28°773 340 703 *789 246 *668} -812 *240 “741 |29°245 "493 *721 |29°208 “464 —*746 \28°713 4229 728} °759 243 816 |29-002 409 *809 |28:999 404 +753 29°021} 29°387 *692| -698) 29°195 ‘807 28°566 “186 *769| °723 246 +418 28:389 | 28-903 ‘475 | +384] 28929 |29-782) -344 063 |29°744| +459 101 800! °851/ 29-325 *808| °926| 29°367 |30:195! -667 431 |30°166 |28-695 | 29-430 19°644 28°644 | 29-144 [29-636 |28-686| 29°161 |30-025 28-300 29:162 |29-993 |27-°896| 28-944 = a te 29°247 29°242 29°301 29°268 y —056 —-061 —-002 ~035 ( Continued.) 1843. 1844, ~ _ ca leans: i 9 aM 3 P.M. 9 a.m. 3 P.M. Hi gh. | Low. | Mean. | High. | Low. | Mean. | High. | Low. | Mean. | High. | Low. | Mean.| 9 a.m. |3 p.m. ce. in. in. in. in. in. in, in. in. in. in. in. in. in. 0-042 28°883 |29-462 |30-024 |28°874 |29-449 |30:085 |29-424 |29°754 |30:065 |29-310 |29°687 29°347 |29°336 072 |27-671 |28°871 |30-037 |27-716 |28°876 |29-976 |28-711 |29°343 |29°946 |28°731 |29-338 "251; +176 9°704 |28°570 |29°137 |29°680 |28°486 |29-083 |29°729| -204 128-966 |29:730| -243 129-986 177| °148 967 |29°013| +490} °935| -942| -438 |30-096 |28-798 |29-447 |30-040 |28:816 |29-428 *385| °378 '*672 |28°906) -289| -663|} °842| +252} -051/29-:179| -615 |30-010|29-196| -603 *376|) °331 *786 |29°039| :412| °757| °961| °359 /30°044! -410] -727 29-967] -402] -684 399 °381 7683 |28°816| +249} +712 /|28-753| +232 /29°736| -187! +461] °735|] -191 463] 402! -378 '*800 |29°005| -402| -756/29°090/ +423] -804 29°042| :423| 783 |29°026| -404] -355| -348 9°828| -039| -433 29808! -001| -404| -880/28-817| -348 857 |28°811] +334] -357| -327 126 |29°348| -737 |30-097 |29-288| -692| -920/29-273| -596| -916/29:276| -596 ‘287 | °294 714 |28°758| +236 |29°703/28°667| -185| -848 28'506{ °177| °855/28°476] °165| -271| -267 9°922 |28-866 |29°394 |29-908 |28-880 |29°394 |29-917 28-525 |29-221 129-893 128-550 29°22] |29-158 |/29-124 i ok i Ma 29-342 29°315 29°465 29-409 |29-314 |29-291 ‘2 ; +:039 +°012 +-120 +:106 + Final Mean 29-303 in. : 5 AY, REPORT—1852. 308 PST 0 LEST mousy ‘savak g 10J suosvag [vorSopo109JoFA] [eAAOS oY} SulAnp weYySurMNg yw UrEYyY—y]]PX aTavy, 11¢-¢— 6¢8-I+ 82E-I+ €1L-I+ 69¢-4— 8eL-E+ L10-6—- PSh-I+ “ut mors “BIT ‘uRay Tenuuy) “Aqyuend ‘uray, woy aouarTayI( LEP-GS 926-61 9L6-L6 G9L-96 OSL-L6 618-26 G91-66 OZF-8S 166-96 “Ur jenuuy T1¢-¢— 668-I+ 82E-I+ €1Z-1+ ¢9¢.4— 83L-e+ L10-6- #SF-I+ “ut ‘ua, WO dUaIAYIC LEGS 966-61 916-L6 G9L-96 G1-L2 GL8:66 G9T-66 GPSS 166-92 “aL €hS-E CBL-G GLL-S GP 66-6 GOL-P G6L-¢ SPL-€ GG-Z “1 662-2 CPPS tL 688-0 Le 86-0 GSE-% 68-1 9.2 oat “Aquywenty Ayrea *AON ‘PO L19-0—- ZEs-0— ¢0¢-0+ 81z-6+ S1l-I— 8eL-It+ L¥L-I— LEL-0- “ut LL8- 098-2 SF9-L 08¢-8 660-01 G9L-9 C10-6 01-9 O€L-Z “ur | “Un y wat | ov | goer 9L6-3— G69-F | O1¢-I—- G93-E | L08-0- | Z06-0+ eLF-L ¢80-4+ 098-9 | ¢1%-0—- 9¢L-1- Gec-¢ | 0960+ | cEez-¢ | 709-T+ 6S¢-0+ 088-2 1F8-0+ 919-¢ | $06-T— 9¢1-0— GI¢-9 | G9LI-— | O010-€ | 690-I+ 61LF+ 068-11 | 092-0— S10-F | 892-0—- 12¢-0— 0G4-9 | 082-0+ CGG.G 861-I— 6040+ | 086-4 69-0— 9FLF | 36L-o+ “UL *ul “UL “ul “ul ‘UBdT, ULO.y) , “uvay UOT] , “uve, UOL EO ERCHICG y a a! i saps nt eli S1S-¢ 901-5 862-9 GII-Z O19-€ 689-9 CPLD G8E-F G99-2 “Ul “1OJUT AA, ““SUvay “PPT “SP8L “OFS “TPS “OFST “6E81 “SE8T “LE8T *SIvOq “sUBATA, OY} WOIJ SOOUDIAYICT OY} YI ‘aArsnjour GEE-S £06 £10 [66-2 GOL-F 89-1 [69-3 GhS-3 13 96-6 6L-€ ¢o9-T §-€ IL-6 68-1 8PL-1 LLG L¥-% GSES 96-F GFS-0 G09-6 Ill 90-6 60-6 L¥-P 80-6 88-1 “ur ‘oune €18-1 Ghs-0 C16-¢ 6F-G C10-4 G8E-6 GS-0 GES 180-T “UL “ART G96-1 9€9-T 602-6 868-1 GOF-T 6-0 69-6 | 980-6 8E-T ¥2-0 St6-1 10-1 8PL-G GL-T 8-0 GG¢-0 69-3 66-1 G60-6 8-€ 9F-1 FL-G G96-T 66-1 oce-0 8F-0 crI-0 F0-6 GGL. L8L-1 €9-1 ¢98-T ¥0-6 GS-1 vE-1 8-1 GPT 10: ¢69-0 69-1 68-1 G{T-1 Sel-¢ £6-£ 1 “ur “Ww ul mut “ul yudy | ‘yorepy "aul “ure 22] ‘uBaTA [RAOUL BY} WOsy soOUaIAyIG oy} pure ‘surayAT [enUUW pure ATYIUOP OY} YPM “vax pnv YOY yous soy arsnjour PFET 0} 1EQT woay ‘savod g Suranp weySurmrg ye uley— [TX TTavVL ““SUBOTA “PRST “EPL “OPSL “TF8T “OFST “6E8T “8E8L “LE81 "Sava _ Os eeSSSSSSSe 61-002 wees | Z0.06 vee | oy 65 Mahe oF vere | ogg [ssneayy a GL-4e— 00-99 29-€ — | 00-26 | GL-0I— | 00-6¢ FI- Te 18-9 — OFF | “FFT = st-8 + | 00-60 | 8&0 + | 0099 | caz+ | 00.25 8 + eo | 6G — | O8F | ‘eh8T GL0L— | 00-061 29-6 — | 00-9F | GL-eI— | 00-9 r+ 6 $9.8 + 0-65 | ‘SrST Gait 00-12 | 8€4 + | 00-89 | ¢2ag+ | 00-8¢ eat as £E-01— 0-0F | “IF8T Gat + 00-202 see + |} 00-66 | ¢z-¢ + | 00-G¢ rI- 1g 29-9 + 0-46 | “OF8T GZ-2o+ 00-€22 8EFIt+ | 00-04 | Gaz + | 00-2¢ iS) 6g $9.9 + 0-49 | "6E8T cz-0 + 00:10 29-4 — 00-8F | S26 + | 00-66 6+ #¢ £8-01- 0-0F | ‘8Est Go-L + 00-202 oor — 00-1 | GJ.4 — 00-2F 9 + 1¢ €9-4 + 0-8¢ | “Es ‘uBoy, [enUUY|*reak ay} Ul|'Ueey WOW], “uvayy Wo), ‘uRay, WO.) , ‘UBoyy WOT) , ' | wWoy-prg | step ruse Seca pg ieee sans EBCRCICG f aupds sauaTIyIC TRUE. | SOR a ie i ari SN En al ae ee “AAISNOU! PEST 0} LEST wWouy ‘savad g 10g suosvag [eoISopos0a}0TA] OY} UT [[ey UTeY YyoryA uo she jo FIquNnN— AX ATIAV T, *¢/.00% T9quInN [enuUY ue ON THE METEOROLOGY OF BIRMINGHAM. €IL-Ge | 991-3 jC suing ; €L-9T 991 606 061 | €1e G0ZG | $23s 106 606 082-0 | SOF |'"*""* toquia0ag ee-0c | 8t | zo | te | zt | o@ | 92 | of | ot [rr* zaquosoy GI@-T | O1¢-L |°°""** saquiaaoyy | 000-61 12 GZ It ix | 61 a | CSL ct ** FaqoqoO 002% | 029-4 |°""""'** taqo309 0S2-91 €1 6 | #1 az | «(06 aoN ST LT ttt" taquiaydag 000-€ | GIg-¢ |" taquiaydag 629-91 91 91 aL 1g ST 61 AE} LT op asn’ny OfL-F | 3266 |" ysn8ny 006-81 SI 12 cI tad & 61 of | st [vs Ame LOL | Star [or Ae | S29.F1 Ol SI 6 ST fat 6 | 232 Oot jot oung O86-G | FO9-G [UT oun r 0G3-ST L 12 | 91 SI } 61 Ot | 9t | gst |" * Ken C98-F | O6FE [ott sep GLE-Z1 G 02 9 sl | 9 6 61 OT jee udy 19 | O9LE [ow pady ee dent | 61 |. ere) ser gr fs OZ f GE | AT [tees qarepy OF6-G | GBT [rr yore 006-ST 8I FI SI FI SI AL | Tt | Lt poe Arenagqag 66-0 | GFO-T [ct Axenaqog Oelkt | Of | 12} St | of | ot | tak 6 6T [rts Arenuee O86-T | GPG |-**"""** Arenuere G3L-LT Ol I 92 L 02 61 02 ae Of'***** Taquiaoaqy “ur “Ul | Reg etl , ‘raquimyy | , : : ; : : ; . . FF8L €F81 SU}UOPL Sano “1 PHBL | “SPSL | SPSL | IFS | OFST | 6E8T BE8I | “LE8T SUFUOPY : “bEST ‘suvopy Ajawax pue pue ePgt seat ayy 10¥ “MV G Je Ayqyaoyy, Oy} YI “Oarsnpour PHgT 07 LST woxy ‘sxeok g ayy Sutanp ave A pue ‘ SoqoUl UI UOI eA —' —"Al Sah Le ie your ur uoyesodeaq—]ITAX LTAV, R00 N yova mt weysurmig 98 TBS Cie BOnr ur sht N “AEX TIEvE, nea Me TP, Fainghs << oe on. a — = — * > 5 a REPORT—1852. Tasie XVI.—Mean Monthly and Annual Dew-Point, from Observa- 1838. 1839. 4 9am. | 3p.m. | Means. | 9a.m. | 3P.M. | Means. | 9a.M. = December ........+..: 39-08 | 40-98 | 40-03 | 37-88 | 39:05 | 38-46 | 37-24 ; GANMALY: (een ccvoscects? 27°02 28°56 27°79 34:42 35°41 34°91 39°46 Rebyiary:.*.<. <4. 000s 65°00 46°50 55°75 61:50 44:00 52°75 63°20 ; AUQUSE coocvecsceoeees 64°50 46°50 55°50 61°50 42:00 51°75 67°50 September ......... 59°00 37°00 48-00 61:00 43°50 52°25 64:50 October nvccterss.sssce 57°00 32°00 44:00 57°50 33°00 45°00 52°50 November .......0000+ 52°00 24:00 38°00 52°50 33°00 42°75 53°50 —$ | | | | | | 54:187| 31-25 | 42676) 5558 | 33-08 | 44:31 | 55°76 | Annual Means non ® ON THE METEOROLOGY OF BIRMINGHAM, 311 tions at 9 a.m. and 3 p.m. for 5 years, from 1838 to 1842 inclusive. 1840. 1841, 1842. Monthly Means. 3p.mM. | Means. | 9a.M. 3p.M. | Means, | 9 a.m. 3 p.m. | Means. oO ° ° ° 5 9 ° ° fe} 39°10 | 38°17 31:70 | 34°12 | 32°91 40°46 | 40°43 40°44 38°00 36°09 | 37:77 | 33°15 | 33°35 | 33:25 | 32:29 | 33:30 | 32°78 33:30 36°86 | 36°68 | 34:48 | 35°56 | 35°02 | 37-19 | 39°67 | 38°43 35°84 34:52 34°36 | 43°54 | 45°03 | 44°28 | 40:90 | 41°73 | 41°31 39:18 44:80 46:19 | 41:48 | 43°30 | 42:39 41:15 | 41:90 | 41:52 41°42 49°59 49°04 | 47°28 52°06 | 49°67 | 46:98 | 47:14 | 47-06 48°09 51:96 | 51°65 48°36 | 48°63 | 48:49 | 53°57 | 54:70 | 54-13 52°19 54:99 53:91 52:22 | 52:29 | 52:25 | 54-99 | 54-79 54°89 54:47 57°96 57°45 55:83 56°45 | 5614 60°25 | 61°37 60:81 56:96 48°72 | 49-11 54°48 | 55°80 | 55°14 | 53°58 | 55°16 | 54:37 52:80 44:01 43°95 46°66 | 45°95 | 46:30 | 42°89 | 43°73 | 43°31 45:45 42°78 41°41 | 39°86 | 43°60 | 41°73 | 40°82 | 42:92 | 41:87 41°70 45°10 | 44:97 | 44:08 | 45°51 44:79 45°42 | 46:40 | 45°91 44:95 50°00 ' 46°50 46°50 53°00 58°00 64:00 59°00 65°00 68°00 65°50 53°00 52°00 1840. 4 Lowest. | Means. | Highest. oO $ 30°00 | 40°25 t 24°50 | 37°50 23°00 35°00 22°50 33°25 : 28°50 | 42:25 33°50 46°25 | 38°50 49°75 a 44°50 | 53°85 : 45°50 56°50 “ 39°00 | 51°75 ‘ 34°50 43°50 " 30°50 | 42:00 a 32°87 44°32 56°70 1841, Lowest. Means. 36°75 30°75 32°25 43°50 45°25 53°25 47°25 54:00 | 57:00 53°25 44:50 38°75 44°70 1842. Lowest. Means. 37-00 31-00 37°75 41:25 42:25 47°50 54-25 53°00 58-00 54:50 42-00 41°75 45°02 and 3 p.m. for 5 years, from 1838 to 1842 inclusive, with the Monthly and deduced therefrom. Monthly Means. 38°50 3245 34°77 38°85 41°45 47°35 51:10 53°87 55°75 51:95 43°90 40°25 44°18 312 REPORT—1852. TasiLe XIX.—Winds registered daily at 9 a.m. during 8 years, from 1837 to 1844 inclusive. N.| N.N.E. | N.E.| E.N.E. | E.| E.S.E. | S.E.| S.S.E. | S.| S.S.W.| S.W.| W.S.W.|W./W.N.W.|N.W.| NeN.W. Dec eee 6 2 | Mees aac boa eel wey 6 ro] ear 6 nee Jan. ale hots one 1 . 3 ate Elias 7 yaaa 7 2 1) ees | 1 oe 3 1 6 1 8 1 Oly See 2 1 March...| 2)... 7 eed ort ae | 3 ras 1 1 1 3 f 2 1 4 April 2.3] 2) 2 2 peal, einect iain 2/|/1 4 2 lie ccc lees eas + 6 May ...| 2) 4 3 1 2}, vl ois om vive 40 “aN meso |e J 1 3 June ...|... Ses 1 aan Alok 3 2;3}) 5 3 1 ae 2 4 July Sl) exe 2 is ai oll ase ie ] 3 2 3.) 4 4 i} 3 Aug. 3 6 3 VANS Su 1 1 2 3 5 1 LS soa 1 1 Sept 2 3 4 Zi piicg 1 5 3 2 2 ‘as 2 2 1 1 Octiie. : 1 1 wae [kcs leon kt 1 AC 4 7 7 tr si ee 3 Ai 1 Nov. .../'2 1 obs nee HEP 1 2 15 6 4 2 |3 3 ‘ 1 16; 13 32 9 |17| 6 16 14 |30) 38 51 16 |32| 15 26 | 27 |358 * From the 25th to the 31st inclusive, wind not registered. 1838. Dec. 1 2 5 ais 1 3 7 5} 63 2 Osi eselt fea 1 Jan. 2 1 3 3 6) 4 if 3 3 1 aes Mae cee 1 3 Hels cenclass 4 8 3 5 2 2 1 ines mae nr 1 1 mee March 1 1 ees pe Ba 1 4 1 3 2 6 1 1 8 1 April ...| 4 1 das Aree ached mites Ho 1 4 2 3 1 2 9 1 2 May ...| 5} 5 2 4:2) 2 2 Me ais al 2 Ant osy-rehael ce beh bani coe dune =..| 2) “oe 2 ] eae 4 3 6 3 2 1 1 2 1 1 a ae Ee At Gls 4d 22 \|) 2s 1 ae eu 3 | as0 lee age ne: DR ae” Gea bro” Vi es ea CT ' oe | Solan oaks pao | lle, os ot Ca en ee Oct.......] 3 2 1 “ 1 1 zt 3 5 2 2 3 1 1 2 Noy. ...| 3 1 3 ihe: 1 5 3 3 1 ee 2 1 nee 25) 19 25 12/22) 13 24 35 {50} 31 27 12, ol 31 9 11/365 | 1839. ee Dees: ..<|ce : 1 1 5 6 | 4 2 1 at 5 1 2 31 | VANS: Goshen wee abe 1 5 2 7 5 5 3 1 1 31) Feb. toa [Oe -26GR, GN Ab CBW g) COR 28 | March.. 4 1 2 Al, 3 2 Tae Bis es se 3 | 31g i Res 2 1 ar 7 1 1 | a 2 30 | 1 ake 1 4 wes 2 3 1 7 1 31 oe SF 1614) bod | esyl-al ieee 30 + ih SF 30410) - 4.04638 | Bec] 3 Ree 31 2 Bice 5 2 5 4 2 4 3 ° 30*| 4 2 Hour’ 4 7 i | | a 1 30 Lan 3 my We) ama eae Nap De ea pa 1 | 31g 1} 1/3) 6 | 4] 2)h. 2|. 2 | 30% 25 | 21 j58| 37 | 41] 28 jai] 15 | 24] 10 [368 * Wind not registered on the 31st, 313 ON THE METEOROLOGY OF BIRMINGHAM. TaBLe XIX.—( Continued.) 1840. |Haacacscaans |S 7 E | cacy es | °. 5 ee Soe st A : a] Z| | Els co cH pegs es é : =F v4 B ie INAMeRINN emma | A ’ ~ : a E | : | TNA AMMA ON :|3 B : a E | g[ NA p pHANdA | Oo Q : se ia | eg eee ae pe oa e 19 da RN erence ae ot | a E oo $ | | & |S? NCNM RAS |x =I 5 + fb eiceds NaN so. 3N be n ea a | | | 10 4 most | x a | loa a wa Hirst) 2 se Nl mio} Poy iS mee rere sas qo g re] eli me Ne ic ei is a > won x ~ 4 o | opr onras Aaa loa % E x Al ms oittiooe rNN cela 4 ea Z Zz | ate se San a eee =e Pa RO ERE ae SES icin aiee oO. 3: * 1841. SARRASSSASSS |B SIN fff ig nAAAN a ~H st 0D 09 1 SH eH ey mI OO Hid Nd Oo AN HON tk 80) [8 ananaen:: ia |x Be SS ee - Se a mSN SNe sro oS lie : ie [ol oe ier tks wt : ar os so: eee pS ORBSRS ee piles . . . . - . ee Nees Ne lS ines: EN He ko Ff oF Or ies 1842. 1: INMeNS peae pan pees apes; 34 Pe Cee HANAN HRS | ee SN TSN Heid set Oud ade: A PS TRO eS ee 314 REPORT—1852. TABLE & 1843. .| N.N.E. | N.E.| E.N.E. E.| E.S.E. | S.E.| S.S.E. | S. S.S.W.| S.W.| W.S.W.|W. Be eft -ets ee oles a NCU Fe ice) 1) ws neat edel Slt ker tal ea tak tle 1 9°\5| Bl 2-38 3 3 aoe | Alea Mittegerct: lccle ale Wee Des aa 2| 49 Derleoe AM 5\ 2 oe a a 5 i eee A 2| 19 1 a Seals a Ar mee cil I 5 6 eae 1) ee 2 2\6 2 1 2) 2 5 3) 1-3 7 aay 1 9 FA | NS an eee 1} 2 3 L> | Ope Bli ee 3 BD oleae heey Mlsvell. sete 1 1) 1 5 4: | 4) 2 8 1 2 2 ribeye 1 Ne 5| 3 1 4 | 3 2 i, eee 1 2 Baal al 1 B agir, a2 ihe A | La 1 5 Bea aleeee 1 ay oT ie kee al ss Q}- 3 3 6- | hee A \ees | Ph (eae 1 err a" Tl 2 1D 5 Pal Be lee Pe moe 14 | 20 93 (23 11 |11| 4 (26) 28 | 46| 44 (25, 22 | 26) 22 Tapnue XX.—General Summary of the number and direction of the V 1844 inclusive, with the corresponding Barometric Pressures, red N. N.N.E. N.E. E.N.E,- E. E.S.E. S.E. Dec. 55 8 4 21 3 6 7 19 Fans others 12 6 6 6 10 6 8 fae wale 8 9 19 17 15 9 10 March...... 16 10 13 18 8 8 13 April... 16 18 18 16 7 4 8 May .....- 22 20 30 18 19 7 6 June ..... 8 4 23 14 13 5 13 DULY: yieeaone 15 7 9 2 8 1 1l Aug. 11 9 12 11 2) 6 9 Sept. ..... 6 9 20 13 6 10 14 |- SS ae 15 12 a oe 3 7 8 Noy ik: 11 9 10% 8 12 7 12 No. of © | 5 ot 148 117 195 135 116 "7 131 Stine \ 29:509 | 29°537 | 29545 | 29-482 | 29-432 | 29°349 | 29-191 ressure. Var. from +106 | +°134 | +°142 +079 | +029 —'054 | —'212 mean press. Mean Pressure of ON THE METEOROLOGY OF BIRMINGHAM. 315 finued.) 1844. N.| N.N.E. | N.E.| E.N.E. | E.| E.S.E. | S.E.| S.S.E. | S.| S.S.W.| S.W.) W.S.W.|W.| W.N.W.|N.W.| NN. W: 0 OS ee a By we oh Am 8 7 rile igs |fa ae ae ee 1 ie ea] 3) (1 reas Sites we shea beg 4s ae 2 DUS ee Blt TS hee eee ih OU > ape) a eee ie) er eT) PRES E ERD 7 1 aad | ee 3 3 | 29 ar 2 2 |1\ 1 eres eee 1 Se agin D 4 2 | 31 Well ial as tals. 2{ 2 [3a 2 4 SrcSiees 1 3 | 30 a Gl 2 «| (13 6 |1 32 lrerasealees| wae: Tel ieee Boel eee 1 1 | 31 BU: 2 he eS ley Mer | tx ale Ll eG 4 CP Ei dl ial 2 | 30 “Ee | 1 pero a eee 3| 1 ple ta 2 Fe ol eG 4 1 | 31 |G) UN 1 1 Ni mee 3 BF sien Ss 3 2 | 31 Ae ee Hi Aol he line coat lhotsvante FB ie 2 5 | 1} 2 TH ee 36 elec 1 1 1 AY AS PEE 1 Prien Ali 5 Balak ae Dae 3 2 | 31 ei lis 2 1 Pal iA ana | By 2 alae 4 7 3 1 Tae Se eae 23] 12 9/ 19 |9} 6 |13] 8 {21} 35 | 44] 30 {41} 26 | 331 17 1366 tered daily at 9 a.m. during each month of the period from 1837 to 29° Fahrenheit, and their Variations from the Mean. S.W. W.S.W. Ww. 1 23 33 18 24 : 17 24 21 24 8 18 30 ite) jee as 2 18 28 16 22 14 28 12 17 8 21 24 11 11 28 26 13 13 21 29 22 27 23 35 24 25 23 27 14 19 24 22 22 21 . 35 35 16 13 ee » | 265 341 200 229 My 286 | 29-301 | 29-347 | 29-381 | 29°369 —'102 | —-056 | —-022 | —-034 ‘ the Winds 29°403. 29°448 +-045 29-473 +070 N.N.W. 130 29°495 ee +092 Total number. 248 241 226 248 240 248 240 248 247 240 248 240 2914 €90-62¢ feetee FE: } wreeee C6-FF eeeeee 68-66 ereeee $69-6F ““SUBOT yenuuy —— ¥Z0:— 0F0-62 | FPO-— 08z- | Gae — 0L-1F 190-— 826-62 | 029-9 — | FLLEF |'''** toquieaon, £20-+ 160-62 | #00-— ze: 0c-:0 + CP-SF 220-+ IIF- sto — | g1¢6p |e 1940190 Pi 068-82 | £80-+ LIF c8-L + | 08-89 880-— 108: 088-4 + | F45-4¢ |*"*** raqutaqydag 260:— 216- 8hI-+ oLF- 10-21+ 96-96 ¢go.+ FFP. 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By James Tuomson, 4.M., Ciwwil Engineer, Belfast. [A Communication ordered to be printed among the Reports. | NuMBERLEsS are the varieties, both of principle and of construction, in the mechanisms by which motive power may be obtained from falls of water. The chief modes of action of the water are, however, reducible to three, as follows :—First, The water may act directly by its weight on a part of the mechanism which descends while loaded with water, and ascends while free from load. The most prominent example of the application of this mode is afforded by the ordinary bucket water-wheel. Secondly, The water may act by fluid pressure, and drive before it some yielding part of a vessel by which it is confined. This is the mode in which the water acts in the water-pressure engine, analogous to the ordinary high-pressure steam-engine. Thirdly, The water, having been brought to its-place of action subject to the pressure due to the height of fall, may be allowed to issue through small orifices with a high velocity, its inertia being one of the forces essentially involved in the communication of the power to the moving part of the mechanism. Through- out the general class of water-wheels called Turbines, which is of wide extent, the water acts according to some of the variations of which this third mode is susceptible. The name Turbine is derived from the Latin word turbo, a top, because the wheels to which it is applied almost all spin round a vertical axis, and so bear some considerable resemblance to the top. In our own country, and more especially on the Continent, turbines have attracted much attention, and many forms of them have been made known by published descriptions. The subject of the present communication is a new water- wheel, which belongs to the same general class, and which has recently been invented and brought successfully into use by the author. In this machine the moving wheel is placed within a chamber of a nearly circular form. The water is injected into the chamber tangentially at the circumference, and thus it receives a rapid motion of rotation. Retaining this motion it passes onwards towards the centre, where alone it is free to make its exit. The wheel, which is placed within the chamber, and which almost entirely fills it, is divided by thin partitions into a great number of radiating passages. Through these passages the water must flow on its course towards the centre; and in doing so it imparts its own rotatory mo- tion to the wheel. The whirlpool of water acting within the wheel chamber, 4 being one principal feature of this turbine, leads to the name Vortex as a suitable designation for the machine as a whole. The vortex admits of several modes of construction, but the two principal forms are the one adapted for high falls and the one for low falls. The former may be called the High-pressure Vortex, and the latter the Low-pres- sure Vortex*. Examples of these two kinds, in operation at two mills near Belfast, are delineated in Plates 1 and 2, with merely a few unimportant deviations from the actual constructions. Plates | and 2 are respectively a vertical section, and a plan of a vortex of the high-pressure kind in use at the Low Lodge Mill near Belfast, for grinding Indian cornf. In these figures AA is the water-wheel. It is fixed * These terms correspond to Hochdruckturbine, and Niederdruckturbine, used in ‘Germany to express the like distinction in turbines. fT This vortex was only in course of erection at the time of the meeting of the British Association in Belfast. The water-wheel itself, removed from its case, being light and of small dimensions, was exhibited in Section G, It is composed chiefly of thick-tinned iron plates united by soft solder. 318 REPORT—1852. on the upright shaft, B, which conveys away the power to the machinery to be driven. The water-wheel occupies the central part of the upper di- vision of a strong cast-iron case, CC; and the part occupied by the wheel is called the wheel-chamber. DD is the lower division of the case, and is called the supply chamber. It receives the water directly from the supply pipe, of which the lower extremity is shown at E, and delivers it into the outer part of the upper division, by four large openings, F, in the parti- tion between the two divisions. The outer part of the upper division is called the guide-blade chamber, from its containing four guide-blades, G, which direct the water tangentially into the wheel-chamber. Immediately after being injected into the wheel-chamber the water is received by the curved radiating passages of the wheel, which are partly seen in figure 2, at a place where both the cover of the wheel-chamber and the upper plate of the wheel are broken away for the purpose of exposing the interior to view, The water, on reaching the inner ends of these curved passages, having already done its work, is allowed to make its exit by two large central orifices, shown distinctly on the figures at the letters L,L; the one leading upwards and the other downwards. It then simply flows quietly away ; for, the vortex being submerged under the surface of the water in the tail race, the water on being discharged wastes no part of the fall by a further descent. At the central orifices, close joints between the case and the wheel, to prevent the escape of water otherwise than through the wheel itself, are made by means of two annular pieces, L, L, called joint-rings, fitting to the central orifices of the case, and capable of being adjusted, by means of stnds and nuts, so as to come close to the wheel without impeding its motion by friction, The four openings, H, H, Plates 1 and 2, through which the water flows into the wheel- chamber, each situated between the point or edge of one guide-blade and the middle of the next, determine, by tneir width, the quantity of water admitted, and consequently the power of the wheel. To render this power capable of being varied at pleasure, the guide-blades are made moveable round gudgeons or centres near their points; and a spindle, K, is connected with the guide- blades by means of links, cranks, &c. (see the Plates) in such a way that, when the spindle is moved, the four entrance orifices are all enlarged or con- tracted alike. This spindle, K, for working the guide-blades is itself worked by a handle in a convenient position in the mill; and the motion is commu nicated trom the handle through the medium of a worm and sector, which not only serve to multiply the force of the man’s hand, but also to prevent the guide-blades from being liable to the accident of slapping suddenly shut from the force of the water constantly pressing them inwards. The gudgeons of the guide-blades, seen in fig. 2 as small circles, are sunk in sockets in the floor and roof of the guide-blade chamber ; and so they do not in any way obstruct the flow of the water. M, in Plate 1, is the pivot-box of the upright shaft. It contains, fixed within it, an inverted brass cup, shown distinctly on the figure; and the cup revolves on an upright pin, or pivot, with a steel top. The pin is held sta- tionary in a bridge, N, which is itself attached to the bottom of the vortex- case. For adjusting the pin as to height, a little cross bridge, O, is made to bear it up, and is capable of being raised or lowered by screws and nuts shown distinctly on the figure. Also, for preventing the pin from gradually becoming loose in its socket in the large bridge, two pinching-screws are required, of which one is to be seen in the figure. A small pipe, fixed at its lower end into the centre of the inverted brass cup, and sunk in an upright groove in the vortex-shaft (see the Plates), affords the means of supplying oil to the rubbing surfaces, over which the oil is spread by a radial groove in ON THE VORTEX WATER-WHEEL. 319 the brass. A cavity, shown in the Plates, is provided at the lower part of the cup, for the purpose of preventing the oil from being rapidly washed away by the water*. Four tie-bolts, marked P, bind the top and bottom of the case together, so as to prevent the pressure of the water from causing the top to spring up, and so occasioning leakage at the guide-blades or joint-rings. The height of the fall for this vortex is about 37 feet, and the standard or medium quantity of water, for which the dimensions of the various parts of the wheel and case are calculated, is 540 cubic feet per minute. With this fall and water supply the estimated power is 28 horse power, the efficiency being taken at 75 per cent. The proper speed of the wheel, calculated in accordance with its diameter and the velocity of the water entering its cham- ber, is 355 revolutions per minute. The diameter of the wheel is 223 inches, and the extreme diameter of the case is 4 feet 8 inches. A low-pressure vortex, constructed for another mill near Belfast, is repre- sented in vertical section and plan in Plates 3 and 4. This is essentially the same in principle as the vortex already described, but it differs in the material of which the case is constructed, and in the manner in which the water is led to the guide-blade chamber. In this the case is almost entirely of wood ; and, for simplicity, the drawings represent it as if made of wood alone, though in reality, to suit the other arrangements of the mill, brick-work, in certain parts, was substituted for the wood. The water flows with a free upper sur- face, W, W, into this wooden case, which consists chiefly of two wooden tanks, AA and BB, one within the other. The water-wheel chamber and the guide-blade chamber are situated in the open space between the bottom of the outer and that of the inner tank, and will be readily distinguished by reference to the figures. The water of the head race, having been led all round the outer tank in the space CC, flows inwards over its edge, and passes downwards by the space DD, between the sides of the two tanks. It then passes through the guide-blade chamber and the water-wheel, just in the same way as was explained in respect to the high-pressure vortex already described; and in this one likewise it makes its exit by two central orifices, the one discharging upwards and the other downwards. The part of the water which passes downwards flows away at once to the tail race, and that which passes upwards into the space E within the innermost tank, finds a free escape to the tail race through boxes and other channels, F and G, _ provided for that purpose. The wheel is completely submerged under the surface of the water in the tail race, which is represented at its ordinary level at YYY, Plate 3, although in floods it may rise to a much greater height. The power of the wheel is regulated in a similar way to that already de- scribed in reference to the high-pressure vortex. In this case, however, as _will be seen by the figures, the guide-blades are not linked together, but each is provided with a hand-wheel, H, by which motion is communicated to itself alone. * Great stress has been by continental engineers and authors laid on the supposed neces- sity for oiling the pivots of turbines. The author of the present communication has thus been led to endeavour to find and adopt the best means for oiling pivots working under water. The oiling, however, is a source of much trouble; and he has found in the course of his experience, that pivots of the kind described above, made with brass working on hard steel, and with a radial groove in the brass suitable for spreading water over the rubbing surfaces, will last well without any oil being supplied. The rapid destruction, which is commonly reported as having been of frequent occurrence in turbine pivots, he believes may in many cases have arisen from the employment of an inverted cup like a diving-bell as one of the rubbing parts, without any provision for the escape of air from the cup. It is evident that a pivot of this kind, although under water, might be perfectly dry at the rubbing surfaces. 320 REPORT—1852. In this vortex, the fall being taken at 7 feet, the calculated quantity of water admitted, at the standard opening of the guide-blades, is 2460 cubic feet per minute. Then, the efficiency of the wheel being taken at 75 per cent., its power will be 24 horse power. Also the speed at which the wheel is calculated to revolve is 48 revolutions per minute. In connexion with the pivot of this wheel arrangements are made which provide for the perfect lubrication of the rubbing surfaces with clean oil. The lower end of the upright revolving shaft enters a stationary pivot box, K, through an opening made oil-tight by hemp and leather packing. Within the box there is a small stationary steel plate on which the shaft revolves. Within the box, also, there are two oil-chambers, one situated above and round the rubbing surface of this plate, and the other underneath the plate. A constant circulation of the oil is maintained by centrifugal force, which causes it to pass from the lower chamber upwards through a central orifice - in the steel plate, then outwards through a radial groove in the bottom of the revolving shaft to the upper chamber, then downwards back to the lower chamber, by one or more grooves at the circumference of the steel plate. The purpose intended to be served by the provision of the lower chamber combined with the passages for the circulation of the oil, is to permit the oil, while passing through the lower chamber, to deposit any grit or any worn metal which it may contain, so that it may be maintained clean and may be washed over the upper surface of the steel plate at every revolution of the radial groove in the bottom of the shaft. A pipe leading from an oil cistern, L, in an accessible situation conducts oil to the upper chamber of the pivot-box ; and another pipe leaves the lower chamber, and terminates, at its upper end, in a stop-cock, M. This arrangement allows a flow of oil to be obtained at pleasure from the cistern, down by the one pipe, then through the pivot-box, and then up by the other pipe, and out by the cock. Thus, if any stoppage were to occur in the pipes, it could be at once detected ; or if water or air were contained in the pivot-box after the first erection, or at any other time, the water could be removed by the pipe leading to the stop- cock, or the air would of itself escape by the pipe leading to the cistern, which, as well as the other pipe, has a continuous ascent from the pivot-box. Certainty may consequently be attained that the pivot really works in clean oil. The author was led to adopt the pivot-box closed round the shaft with oil tight stuffing, from having learned of that arrangement having been sucéss- fully employed by Kochlin, an engineer of Miihlhausen. As to the other parts of the arrangements just described, he believes the settling chamber with the circulation of oil to be new, and he regards this part of the arrange- ments as being useful also for pivots working not under water. In respect to the materials selected for the rubbing parts, however, he thinks it necessary to state that some doubts have arisen as to the suitableness of wrought iron to work on steel even when perfectly lubricated ; and he would, therefore, recommend that a small piece of brass should be fixed into the bottom of the shaft, all parts being made to work in the manner already explained. The two examples which have now been described of vortex water-wheels adapted for very distinct circumstances, will serve to indicate the principal features in the structural arrangements of these new machines in general. Respecting their principles of action some farther explanations will next be given. In these machines the velocity of the cireumference is made the same as the velocity of the entering water, and thus there is no impact between the water and the wheel; but, on the contrary, the water enters the radiating conduits of the wheel gently, that is to say, with scarcely any motion in relation to their mouths. In order to attain the equalization of ON THE VORTEX WATER-WHEEL. 321 these velocities, it is necessary that the circumference of the wheel should move with the velocity which a heavy body would attain in falling through a vertical space equal to half the vertical fall of the water, or in other words, with the velocity due to half the fall; and that the orifices through which the water is injected into the wheel-chamber should be conjointly of such area that when all the water required is flowing through them, it also may have a velocity due to half the fall. Thus one-half only of the fall is em- ployed in producing velocity in the water ; and, therefore, the other half still remains acting on the water within the wheel-chamber at the circumference of the wheel in the condition of fluid pressure. Now, with the velocity already assigned to the wheel, it is found that this fluid pressure is exactly that which is requisite to overcome the centrifugal force of the water in the wheel, and to bring the water to a state of rest at its exit, the mechanical work due to both halves of the fall being transferred to the wheel during the combined action of the moving water and the moving wheel. In the fore- going statements, the effects of fluid friction, and of some other modifying influences, are, for simplicity, left out of consideration ; but in the practical application of the principles, the skill and judgement of the designer must be exercised in taking all such elements as far as possible into account. To aid in this, some practical rules, to which the author as yet closely adheres, were made out by him previously to the date of his patent. These are to be found in the specification of the patent, published in the Mechanics’ Magazine for Jan. 18 and Jan. 25, 1851 (London). - In respect to the numerous modifications of construction and arrangement which are admissible in the Vortex, while the leading principles of action are retained, it may be sufficient here merely to advert,—first, to the use (as explained in the specification of the patent) of straight instead of curved radiating passages in the wheel; secondly, to the employment, for simplicity, of invariable entrance orifices, or of fixed instead of moveable guide-blades ; and lastly, to the placing of the wheel at any height, less than about thirty feet, above the water in the tail race, combined with the employment of suction pipes descending from the central discharge orifices, and terminating in the water of the tail race, so as to render available the part of the fall below the wheel. In relation to the action of turbines in general, the chief and most commonly recognised conditions, of which the accomplishment is to be aimed at, are that the water should flow through the whole machine with the least possible resistance, and that it should enter the moving wheel without shock, and be discharged from it with only a very inconsiderable velocity. The vortex is in a remarkable degree adapted for the fulfilment of these conditions. The water moving centripetally (instead of centrifugally, which is more usual in turbines) enters at the period of its greatest velocity (that is, just after passing the injection orifices) into the most rapidly moving part of the wheel, the circumference ; and, at the period when it ought to be as far as possible deprived of velocity, it passes away by the central part of the wheel, the part which has the least motion. Thus in each case, that of the entrance and that of the discharge, there is an accordance between the velocities of the moving mechanism and the proper velocities of the water. The principle of injection from without inwards, adopted in the vortex, affords another important advantage in comparison with turbines having the contrary motion of the water; as it allows ample room, in the space outside of the wheel, for large and well-formed injection channels, in which the water can be made very gradually and regularly to converge to the most contracted parts, where it is to have its greatest velocity. It is as a con- 1852. x 322 REPORT—1852. comitant also of the same principle, that the very simple and advantageous mode of regulating the power of the wheel by the moveable guide-blades already described can be introduced. This mode, it is to be observed, while giving great variation to the areas of the entrance orifices, retains at all times very suitable forms for the converging water channels. Another adaptation in the vortex is to be remarked as being highly bene- ficial, that namely according to which, by the balancing of the contrary fluid pressures due to half the head of water and to the centrifugal force of the water in the wheel, combined with the pressure due to the ejection of the water backwards from the inner ends of the vanes of the wheel when they are curved, only one-half of the work due to the fall is spent in commu- nicating vis viva to the water, to be afterwards taken from it during its passage through the wheel; the remainder of the work being communicated through the fluid pressure to the wheel, without any intermediate generation of vis viva. Thus the velocity of the water, where it moves fastest in the machine, is kept comparatively low; not exceeding that due to half the height of the fall, while in other turbines the water usually requires to act at much higher velocities. In many of them it attains at two successive times the velocity due to the whole fall. The much smaller amount of action, or agitation, with which the water in the vortex performs its work, causes a material saving of power by diminishing the loss necessarily occasioned by fluid friction. : In the Vortex, further, a very favourable influence on the regularity of the motion proceeds from the centrifugal force of the water, which, on any in- crease of the velocity of the wheel, increases, and so checks the water supply ; and on any diminution of the velocity of the wheel, diminishes, and so admits the water more freely ; thus counteracting, in a great degree, the irregularities of speed arising from variations in the work to be performed. When the work is subject to great variations, as for instance in saw-mills, in bleaching works, or in forges, great inconvenience often arises with the ordinary bucket water-wheels and with turbines which discharge at the circumference, from their running too quickly when any considerable diminution occurs in the resistance to their motion. The first vortex which was constructed on the large scale was made in Glas- gow, to drive a new beetling-mill of Messrs. C. Hunter and Co., of Dunadry, in County Antrim. It was the only one in action at the time of the Meeting of the British Association in Belfast ; but the two which have been particularly described in the present article, and one for an unusually high fall, 100 feet, have since been completed and brought into operation. There are also several others in progress ; of which it may be sufficient to particularize one of great dimensions and power, for a new flax-mill at Ballyshannon in the West of Ireland. It is calculated for working at 150 horse-power, on a fall of 14 feet, and it is to be impelled by the water of the River Erne. This great river has an ample reservoir in the Lough of the same name; so that the water of wet weather is long retained, and continues to supply the river abundantly even in the dryest weather. The lake has also the effect of causing the floods to be of long duration, and the vortex will consequently be, through a considerable part of the year, and for long periods at a time, ' deeply submerged under back-water, The water of the tail race will fre- quently be 7 feet above its ordinary summer level; but as the water of the head race will also rise to such a height as to maintain a sufficient difference of levels, the action of the wheel will not be deranged or impeded by the floods. These circumstances have had a material influence in leading to the adoption in the present case of this new wheel in preference to the old breast or undershot wheels. a FOODS, IN RELATION TO RESPIRATION AND FEEDING. 323 On the Composition of Foods, in relation to Respiration and the Feeding of Animals. By J.B. Lawes, Esq., of Rothamsted; and J. H. GiLBeErRT, PA.D., F.C.S. Durine the last twelve years our knowledge of the adaptation of food, according to its composition, to the various exigences of the animal system, has assumed much of definiteness ; and it is to the experiments and writings of MM. Boussingault, Liebig and Dumas, that we must attribute, either directly or indirectly, much of the progress that has been made. There are, however, connected with this important subject still many open questions ; and it is with the hope of aiding the solution of one or two of these, and thus providing a new starting-point for further inquiry, that we propose in the present paper to bring forward some results of our own which bear upon them, and to point out the conclusions to which they appear to us to lead. The writers to whom we have above referred, as well as many others, whether themselves experimenters or more systematic writers on the subject of the chemistry of food, may, with few exceptions, and with some limita- tions, be said to agree on two main points, viz. on the one hand, as to the connection of the nitrogenous constituents of the food, with the formation in the animal body of compounds containing nitrogen, and with the exercise of force ; and on the other, as to the general relationship of the mon-nitrogenous constituents of the food with respiration, and with the deposition of animal fat. It is indeed upon the assumption of this broad and fundamental classi- fication of the constituents of food, according to their varied offices in the animal ceconomy, that a vast series of analyses of foods have of late years been made and published; whilst, founded upon the results of these analyses, numerous tables have been constructed, professing to arrange the current articles of diet both of man and other animals, according to their comparative values as such. Among the labourers in this field of inquiry, we are much indebted to MM. Liebig, Dumas, Boussingault, Payen, Playfair, R. D. Thomson, Horsford, Schlossberger and Kemp, and others. When speaking generally then, of the various requirements of the animal organism, the more special adaptations of the several proximate compounds and ultimate elements of which our vegetable and animal aliments are made up, are, as we have already said, fully admitted ; but in attempting to apply to practice the principles herein involved by the construction of tables of the comparative value of foods, it seems to have been generally assumed, that our current food-stuffs are thus measurable rather by their flesh-forming than by their more specially respiratory and fat-forming capacities. Hence, with some limitations, the per-centage of nitrogen has always been taken as the standard of comparison. Founded upon their per-centage of nitrogen, M. Boussingault first arranged tables of the comparative values of different articles of food, chiefly in refer- ence to the dieting of the animals of the farm; and with this method Professor Liebig has expressed his concurrence. At page 369 of the 3rd edition of his Chemical Letters, he says—“ The admirable experiments of Boussingault prove, that the increase in the weight of the body in the fattening or feeding of stock (just as is the case with the supply of milk obtained from milch cows), is in proportion to the amount of plastic constituents in the daily supply of fodder.” And at page 349 of the same, speaking of the nitrogenous compounds of food, he says—“TIt is found that animals require for their support less of any vegetable food in proportion as it is richer in these peculiar matters, and cannot be nourished by vegetables in which these matters are absent.” In like manner, various specimens of flour and of bread have been arranged by Dr. R. D. Thomson ; other articles of vegetable diet by Mr. Horsford ; and x¥2 324 REPORT—1852. a large series of aliments from the animal kingdom by MM. Schlossberger and Kemp. Dr. Anderson also, in his valuable Report on the Composition of Turnips, grown under different circumstances and in different localities, has taken their per-centage of nitrogen as the measure of their comparative feed- ing value. The views which have thus led to a vast number of analyses of foods, as well as the information supplied by the analyses themselves, have contributed much to the advancement of our knowledge of the chemistry of food. It has however been found, that the indications of tables of the comparative values of foods, founded on the per-centages of proteine compounds, were frequently discrepant with those which common usage or direct experiment affords. These discrepancies have not escaped the attention of the authors of the theo- retical tables ; but they have attributed them rather to the erroneous teachings of common practice or experiments on feeding, than to any defect in the theo- retical method of estimation. On all hands, however, it has been admitted, that further direct experiment bearing upon this important subject was much needed ; and it is the acknowledgement of this necessity that seems to justify the publication, under the auspices of the British Association, the results of this kind which we have now to submit. The question to which we shall first call attention, is, whether, in the use of our current foods, under ordinary circumstances, but especially in the case of animals fattening for the buteher, the amount of food consumed, and that of increase produced, have a closer relationship to the supplies in such foods of the nitrogenous, or of the mon-nitrogenous constituents? That is to say, whether the sum of the requirements of the animal system is such, that, in ordinary circumstances, and in the use of ordinary articles of food, the measure of the amount taken, or of the increase produced, will be regulated more by the supplies of the “Plastic,” or of the more peculiarly respiratory and fat-forming constituents. According to the views upon which all the tables of the comparative values of foods are constructed, it is the supplies of the plastic elements of food chiefly, that should regulate both the consumption, and the increase in weight, of a fattening animal. If, however, we bear in mind the views which are generally entertained as to the influence of respi- ration on the demands of the system for the oxidizable elements of food, it would appear more consistent to suppose that the measure, at least of the con- sumption of food, would be chiefly regulated by its supplies of those elements. In the experiments to which we shall call attention, sheep and pigs have been the subjects. As, however, their object has partly been the solution of certain questions of a more purely agricultural character than those now under consideration, the details, as to the selection of the animals, and the general management of the experiments, will be given more appropriately in another place. Indeed, the particulars of some of the experiments with sheep, so far as their agricultural bearings are concerned, have already ap- peared in the Journals of the Royal Agricultural Society of England; and those of the rest, and also of the experiments with pigs, will probably do so shortly. It should here be stated, however, that the general plan has been to select several different descriptions of food, containing respectively various amounts of nitrogenous and non-nitrogenous constituents, the proportions of which were ascertained by analysis. ‘To one or more sets of animals to be compared, a fixed and limited amount of food of a high or of alow per-centage of nitrogen, as the case might be, was allotted, and they were then allowed to take ad libitum of another or complementary food. In this way, in obedience to the instinctive demands of the system, the animals were enabled to fix for themselves, according to the composition of the respective foods, the quantities of each class of constituents which they required. FOODS, IN RELATION TO RESPIRATION AND FEEDING. 325 In the tables which follow the results of the experiments are arranged to show— lst. The amounts respectively of the nitrogenous and the non-nitrogenous constituents consumed weekly per 100 lbs. live weight of animal. 2nd. The amounts consumed of each of these classes of constituents ¢o produce 100 lbs. increase in live weight. Summary tables of the results of the analyses of the foods are also given. In the tables showing the amounts of the constituents consumed, &c.—the weights of the animals themselves—of the foods consumed—and their per cent- ages, of dry matter, of ash, and of nitrogen—have formed the basis of the calculations. Thus, the column of nitrogenous substances consumed, is obtained by multiplying the amount of nitrogen by 6:3, on the assumption that they all exist as proteine compounds. This method of estimation will, we think, be found sufficient for our present purpose; though, as we shall have occasion to point out further on, it is frequently far from accurate, and especially when applied to succulent vegetable substances. The amounts of zon-nitrogenous constituents are obtained by deducting those of the mineral and nitrogenous constituents from the amount of the total dry matter consumed. In the tables showing the amounts of the respective constituents consumed by a given weight of animal within a given time, it is their mean weights that are taken for the calculation; namely, those obtained by adding together their weights at the commencement and at the conclusion of the experiment, and dividing by 2. In the tables showing the constituents consumed éo produce a given weight of inerease, the figures are obtained by simple rule of three; taking as the elenients of calculation, the consumption during the total period of the ex- periment, and the total increase in weight during the same period. With these short explanations we may now introduce the tables them- selves, TABLE I. Summary Table of the Per-centage Composition of the Sheep Foods. . Foods eaten by Series 1. | Mean Per-centage Results. Description of Food. Dry Matter. Ash. Nitrogen. Inclusive | Exclusive} In Fresh | In Dry | In Fresh | In Dry of Ash, of Ash. | Substance.| Matter. | Substance.| Matter. Swedish Turnips, No. 1. ...... 10:58 | 1000 | 0-577 | 5:46 0-263 | 2-49 Swedish Turnips, No. 2. ......./ 12°12 11°49 0:6382 521 0-151 1:25 American Oil-cake...........0006. 89°50 | 84:08 5°42 6:06 5:08 5°68 MESS ely cscucsesedteainees does 85°18 82-24 2°94 3°45 2:08 2°44 Clover-chaff .............s0sceees 78°61 72:33 6:28 7:99 1:85 2°35 Oat-straw Chaff ......... Seas 81:28 | 74:86 6:42 7:87 WDIRCAKE 2.2... cncesnescessonseens 87°36 81:88 5°48 6:27 5-01 5°74 Linseed, No. 1. .......0....0seee. 90°56 86:28 4:28 4-72 3°68 4:07 Rimbeed, NO 252k .0. 6. ceeieeecs 91:54 87:46 4-08 4-45 4:05 4:44 Barley ...ccccesecscecscessveveces 85°54 83:23 2°31 2-70 1-49 1-74 PAG <, o's cacngnahes'nels'n' duiestiades 91°65 89°34 2°31 2°52 151 1:65 Clover-chaff ....... Ts a waiseayieee 84°66 77:39 7:27 8:58 2-11 2°50 326 REPORT—1852. TaBLe I. (continued.) Foods eaten by Series 3. Mean Per-centage Results. Description of Food. Dry Matter. Ash. Nitrogen. Inclusive | Exclusive} In Fresh | In Dry | In Fresh | In Dry of Ash. of Ash. |Substance.| Matter. | Substance.} Matter. Norfolk White Turnips, grown by mineral manures 9°37 8:74 0°627 6°69 0°146 1:56 i aeecceece te ares oer cb Norfolk White Turnips, grown by mineral manures and ammoniacal salts ...... Norfolk White Turnips, grown by mineral manures 778 | 714 0639 | 8-21 0183 | 2:36 and rape-cake ..........se00s Norfolk White Turnips, grown by mineral manures ’ : : y DFS , rape-cake and ammoniacal 788 it mses = iti nai BAUR sacksedeecctcosceseseceere. Foods eaten by Series 4. Long Red Mangold, No. 1, ...| 12°94 | 11:94 1:002 774 0:30 2:36 Long Red Mangold, No. 2. ...} 13°14 | 12:16 0:979 7°45 0:28 2°18 —__—_—_ Means...) 13°04 | 12°05 0:990 759 0:29 2:27 Barley titeesstetecscadeaccsevecss 81°84 | 79°51 2°32 2°84 1-45 1:78 IMT ALG? oa. saceb 2S-aee cok wane eneeiiens 95°39 | 92:78 2-60 2-73 1:62 1:70 IMs GING oc Ue caeistes easctedetacs 93:76 | 85:06 8:70 9:28 4:10 4:38 ON =GHKG 208, Gales cs sbdevecedues 89:74 | 83°60 6:12 6:82 5:26 5°87 (Ea SS ae Fe eR! Ro ne a! % TABLE II. Summary Table of the Per-centage Composition of Sheep Foods (continued). Series 5. Foods eaten by Hants and Sussex Downs. Mean Per-centage Results. Description of Food. Dry Matter. Ash. Nitrogen. Inclusive | Exclusive} In Fresh | In Dry } In Fresh | In Dry of Ash. of Ash. [Substance.| Matter. | Substance.| Matter. Swedish Turnips, Lot 1. ...... 9°81 9:20 0-607 | 619 0-231 2°36 Swedish Turnips, Lot 2. ...... 10°32 9-73 0-607 | 5:87 0:301 2°61 Oil-cake .... Jedi tuessacuct sewes set 87°54 80°84 6:70 7:65 4-98 5:70 Clover-hay 2.035.002: dsecaves tes | 81:24 72°82 8:42 10°36 2-03 2°51 | — FOODS, IN RELATION TO RESPIRATION AND FEEDING. 327 Taste II. (continued.) ern ee reer Eaten by Cotswolds. en Mean Per-centage Results. Description of Food. Dry Matter. Ash. Nitrogen. In Fresh | In Dry Inclusive | Exclusive} In Fresh | In Dry Substance.| Matter. of Ash. of Ash. | Substance.| Matter. Swedish Turnips, Lot 1. ......| 10°88 | 10:37 0504 4:63 0-18 1:66 Swedish Turnips, Lot 2. ...,.. 10:70 | 10:12 0579 5°41 0:28 2°63 Swedish Turnips, Lot 3. ...... 12°60 | 11:84 0°758 6:00 0:27 2°21 Oil-Cake ......cessssecesseceeee vee) 87:54 | 80:84 6-70 7°65 4:99 5:70 Clover-hay ....0c..sseccsseseeeenee 83°66 | 76°46 7:20 8-60 2°24 2°68 Eaten by Leicesters ; and by Cross-bred Ewes and Wethers, [Leicester and South Down. ] Swedish Turnips, Lot 1. ...... 10°89 | 10:38 0:520 4:79 0:23 2-15 Swedish Turnips, Lot 2. ...,..} 11°88 | 11:26 0°623 5:23 0:25 2:14 ME CAICC: 5c. sc exeencns>aanaapanang 86°32 | 78:52 7°80 9-04 5:05 5:86 Clover-hay, Lot 1. .........20006 80°48 | 72°38 8:10 10:06 2:73 3°40 Clover-hay, Lot 2. ............00 80:08 | 71:90 8:18 10°17 2:73 3°42 TaB_eE III. Summary Table of Per-centage Composition of the Pig Foods. Eaten by Series 1. Mean Per-centage Results, Description of Food. Dry Matter. Ash. Nitrogen. Inclusive | Exclusive} In Fresh | In Dry | In Fresh | In Dry of Ash. of Ash. | Substance.| Matter. | Substance.| Matter. Egyptian Beans........ iver ea eke 88°30 83:57 4:72 5:35 4:24 4:80 Lentils, Lot 1. ..........ce.eeeee 87°30 82:42 4°87 5°58 4:52 5°18 Lentils, Lot 2. .......00...s0ee0 86:62 81-64 4:98 5°75 4:56 5°26 Indian meal, Lot J. ...........- 89:70 | 88:33 1°37 1°53 1:72 1:92 Indian meal, Lot 2. .,.......... 89°89 88°61 1:28 1-42 1:95 2°17 TAN 1: .....cddnstaveboatntaisaaees 84:79 78°77 6:02 7:10 2°61 3:08 RANEY: ( ciisicaasacednnnsacacssessap 81:86 79°72 2:14 2-61 1:83 2:24 Eaten by Series 2. Egyptian Beans..............00. 88-17 84:45 372 4:22 4-21 4-78 Lentils, Lot 1. ..,...see..seereee 89-42 86:44 2:98 3:33 4°54 5:08 GIS, LO Bok occ..sesstsoresses 89-97 85°10 4:37 5°41 4:18 4°65 amley, Lot 1. .....c..sscsessese 82°38 80°19 2°19 2:66 1:82 2-21 Batley, Hot 2s ~...0.0.0.5. gg & cs 4 3 3 Forty Hants Downs, twen- “ ty-Six WeekS .......000.. ‘3s Forty Sussex Downs, twen- 3 3 ty-six WeekS ..:...000..5 5 Ha Forty-six Cotswolds, twen- 5 5 ty WEEKS .....cccssecseeees .S) a Forty Leicesters, twenty Zs os WEEKS Site seeeeesee sete s | Forty cross-bred Ewes, iS e twenty weeks ............ § nn Forty cross-bred hase 3 B twenty weeks .......0.... Means ...... Nitrogenous Organic ——SS = — | | | Substance. _ sa | as |g. #3 jee 2" 124 62 | 186 129 | 60] 189 111 | 55 | 166 127 59 | 186 127 58 | 185 127 59 | 186 124 59 Non-nitrogenous Organic Substance. az | 32] 4". 300 | 312 | 612 318 | 302 | 620 260 | 322 | 582 261 | 358 | 619 260 | 350 | 610 261 | 355 | 616 183 | 277 | 333 | 610 Total dry Organic Substance. FOODS, IN RELATION TO RESPIRATION AND FEEDING. 331 Taste VI. Experiments with Pigs Weekly consumption of Nitrogenous and Non- nitrogenous constituents of Food per 100 lbs. live weight of animal (quantities stated in Ibs., tenths, &c.). Series 1.—Three pigs in each pen, 8 weeks. Nitrogenous Organic} Non-nitrogenous 3 : Substance. Organic Substance. & 3 cS) 6 FI ‘i imited Food, per head Complementary or 5 bo > Li ‘ood, is on oS a s per a ad libitum Food. aa = 3 = 3 F z 3 33 ae | gh peed Wiesel ae as | es eg/a"| 6 1.| None ........00 ddsisas sts Bean and Lentil WHEAl a adhe Sassen -. | 8°84 176 2.| Indian meal .........4.. ditto ...... 0°83 | 7°30 14:3 © AULT a Pee ere eee GiGtO ws sesebs 1:32) 6:39 128 4, | Indian meal and Bran... WittO « ss0.05 2°14) 4-73 9-4 Means...... 1:07 | 6-82 13°5 Be | NONE: ...i.sceccccceee ‘....| Indian meal ...... Bee aie | 19:3 6. | Bean and Lentil meal .. Cth Lisenaze 1:95 | 2-60 17:2 7.| Bran ..... eT ditto ...... 1:21| 2-74 17-9 | 8.| Bean and Lentil meal, | and Bran ........008 THO) cesess 3°05 | 2-15 14:0 Means...... 1-55 | 2°60 7-1 9. | Bean and Lentil meal...) Bran ...........00+ 3°34| 1°85 70 10. | Indian meal ............ LUC Redes 1:44} 2-46 93 _ |H1.| Bean and Lentil meal, F and Indian meal .,.| - ditto ...... 323 | 1:73 66 MEIOTIC ca6cnceacsncosescsncs Bean and Lentil ; meal, Indian meal, Bran, each dl Whittsie =s2.5: .. | 612 20-1 Means...... 2-00 | 3:04 10'8 Means of the 12 pens......) 1:54) 4°15 138 q KR | 9 { Series 2.—Three pigs in each pen, 8 weeks. 4 : MO INONOesesssscsssieassesces Bean and Lentil : meal) ig eek --- | 669) 6-69] ... | 14-5] 14:5] 21-2 _ | 2.| 3lbs. Barley meal ...... CHLOE 3, 28s 1:23 | 7-06 | 8-29] 7:3] 15:3| 22-6] 30:9 Beer Lib. Bran ..:..........0, CHILO Pie cices 0°66 | 8-07| 8:73] 2-5| 17:'5| 20:0} 28-7 _ | 4.| 8lbs. Barley meal, 1 Ib. IRREPRIN coRoe owes sce ceed Cite enews 1:95 | 4°85 | 6-80] 10:1] 10-5) 20-6] 27-4 | Means ......| 0:96| 6-67| 7-63| 5-0| 14-4| 19-4] 27-0 a SS ee Se ee ee 332 REPORT—1852. Tas.e VI. (continued.) Nitrogenous Organic} Non-nitrogenous 3 x Substance. Organic substance. Fs * z Ss | Limited Food, per head, Complementary or celeste =a Ue tee 3 : a aS per day. ad libitum Food. E : a 2 ae cE : & zy a3 83) 68) 4") a3) a8) 4") 5 MISH ENOME’ ton-n creas soleseat oes Barley meal ....., - | FOL} 3-91 23°6 | 23:6] 27-5 6.| 141b. Bean, and 14 lb. Lentil meal ......... ditto” ...... 2°81} 2:36) 5-17] 61] 13:9} 20:0] 25-2 QAM ABranerssee se eden: MEO ices ee O61} 3:45 | 4:06] 2°3 | 20°9| 23:2] 273 8.| 14 1b. Bean, 13 1b. Len- til meal, and 1 lb. IBYAN Se ecse; accuses er ditto: © .5.... 2°98| 1:66] 4:64] 7:2 | 10:0} 17:2] 21°8 Means...... 1:60| 2°84| 4-44] 3:9 | 17-1) 21:0] 25°4 QEIMNGNETcscpelecseresonine see Mixture of 1 part ; if “4 -| fi Bran,2 partsBar- ley meal, and 3 parts Bean and Lentil meal...... «- | 665] 6°65 20°6 | 20°6] 27-2 BUPITNGNC cccc.sececesvesossbee Duplicate of pen9.| ... | 7-03} 7:03 21:9} 21:9] 28-9 | INGE fs stnisased cinens oa: Mixture of 1 part Bran, 2 parts Bean and Lentil meal, and 3 parts Barley meal ...| ... | 5°86] 5:86] ... | 21-4] 21-4] 27:3 AAW INQUEST nw csoraasestespeoenee Duplicateofpenll.| ... | 6°02] 6-02] ... | 22:1] 22-1] 28-1 Means...... ~ | 639) 6:39 21:5] 21:5] 27-9 Means of the 12 pens...... 0:85 | 5°30| 615} 2:9 | 17:7| 20:6] 26:8 Means of the 24 pens...... 1:19] 4:73) 5:92] 4:1 | 15°83) 19:9] 25:8 TaBLeE VII. Experiments with Pigs.—Consumption of Nitrogenous and Non-nitrogenous constituents of Food, ¢o produce 100 lbs. increase in live weight of animal (quantities stated in lbs.). Series 1.—Three pigs in each pen, 8 weeks. Nitrogenous Organic} Non-nitrogenous 3 y Substance. Organic substance. $3 ° oO Z Og > | Limited Food, per head, Complementary or ie te ies es vs Sur pa 5 per aan ad Dbitum Food. “5/88 )/85)#28 1/28 |83] 72 PA eo} se | Ss] 8o)]/s=| se] 32 ao | fe | e= lao loe| a= 2 Da WNOnG © oan peteeusteaxkiecee Bean and Lentil MCA ies cnecly nnn vs .» | 188 | 188]... | 275 2.| Indian meal .........00. CIUGCO fe svete 12 | 102 | 114] 77 | 201 xs) Yat ivssvaceegesneeatee GittO ...4.0. 28 | 1383 | 161 | 105 | 267 4, | Indian meal and Bran... ditto “...... 38 83 | 121 | 185 | 166 Means ...... 19 | 114 | 1338 92 | 227 FOODS, IN RELATION TO RE SPIRATION AND FEEDING. 333 Tasce VII. (continued.) Nitrogenous Organic Non-nitrogenous Substance. Organic substance. : 23 z - > | Limited Food, per head, | Complement gg | 273 et fart a ee pa g| Unitsedpe nad | compere | 49/282. 143 | 22 | ze] 2 ae | 3 ae | 3 So} s easy a4 S3| a8 |4")e5 BREN inant cunsiawive sand ase Indian meal ...... a 57 .. | 378 6. | Bean and Lentil meal .. Gute oes-c- 31 | 42 62 | 275 Gaerne. se ak ditto... 18 | 40 68 | 264 8.| Bean and Lentil meal, nd) Bran. (ecascs.peces itt} dycsasc- 43 | 30 114 | 195 Means ...... 23 | 42 61 | 278 | 339 9.| Bean and Lentil meal..| Bran ...........0... 127 | 71 255 | 268 10. | Indian meal ............ ditto. 02.5: 48 | 82 311 | 309 11.} Bean and Lentil meal, and Indian meal ... ditto ......| 74 | 40 240 | 151 SEWNONE*..--.cccccscesecnces Bean and Lentil] ... | 107 w. | 350 meal, Indian meal, Bran, each ad libitum ...... Means...... 62 75 | 187 | 202 | 269 Means of the 12 pens...... 35 | 77 118 | 258 Series 2.—Three pigs in each pen, 8 weeks. MIE NOUC? jo. janie oncsessaecnane Bean and Lentil THEA ce cpeleenia ss ... | 146 | 146 317 | 317 | 463 2.| 3lbs. Barley meal ...... aNGhGre ees 20 | 117 | 137 254 | 374] 511 3.| Lib. Bran .........02.00 ditto’ 2... 12 | 140 | 152 305 | 348 | 500 4,| 3 lbs. Barley meal, 1 Ib. TEU ania «Salas ates GitLOy owas 36 89 | 125 192 | 378 | 503 Means ...... 17 | 123 | 140 267 | 354] 494 Bi INOTIG hs Seaweed cess ces Barley meal ...... 64 | 64 Hi 385 385 | 449 6.| 14 1b. Bean and 141b. Lentil meal ......... ditto ...... 50 4] 91 |] 107 | 245 | 352 | 443 Mey Wp. Bran <..-...0<0ceoss GXCEO, as .ce> 10 56 66} 38 | 341 | 879 | 445 8.| 141b. Bean, 14 1b. Len- : til meal, and 1 lb. eet ons ue aceseds