CIHM Microfiche Series (Mlonographs) iCMH Collection de microfiches (monographles) Technical and Bibliographic Notes / Notes techniques et bibliographiques Th« InstHut* hat atttmpltd to obtain th« bttt original cow avaHable for filming. Features of this copy which may be bibliographically unique, which may aRer any of the images in tha reproduction, or which may significantly changa the utual mtttwd of fflming ara chedced below. □ Coloured covers / Couveiture de couleur □ Covers damaged / Couverture endommagie □ Covers restored and/or laminated / Couveiture restaur^e et/ou pelliculie I Cover title missing /lje ttre de couveitwe manque I Cotourad maps/ Cartas giegrapNquat an eodmr □ Coloured ink (i.e. other than blue or black) /* Encre da couiaur (i.*. atiba qua blaue ou noira) □ Cotoured plates and/or illustratk>ns / PItnchas atfou ikistratfona an coulaur □ Bound with other material / Rell« avee d'autraa docwnaMs □ Only edition available / SeulaMMondiaponMa □ light Unding may cause shadows or distortk>n along Interior margin / La reikire serr^e peut causw da rombre ou da la tfMnion la ioi^ da la marga int^rieure. □ Blank leaves added during restorations may appear within the text. Whenever possible, these have been omMadftom filming / Use peut que certaines pages blanches ajout^es iors d'une restauration spparaissent dans ie texte. mais. torsque cela itait posaiMa. eat pagaa pas M fftniaa. Additional comments/ Peginetlon ia CommamalraasuppMmanlaiias: pagination L'instRut a mierofUmi Ie meilleur exemplaire qu'il lui a M possibia de se procurer. Les details da cat exem- plaire qui soni peut-«tre unk)ues du point da vua bibR- ographkpe. qui peuvent nwdKler une image reproduile. ou qui peuvent exiger une modificatkm dans la mllho- de normale de filmage sont indk)u<s ci-dessous. I [ Coloured pagas/Pagas da couiaur [71 Pages damagad/P»oaaandofwnag4as □ Pages restored and/or laminated / Pages rastaurlaa aUMi paiReuliaa Pages discotoured, stained or foxed / Paget d<eoloiiat,taehatefv p-j^jin I I Pages detached/ Pages cf^t:. ' J I I Showthrough/Tiansparencci □ Quality of print varies / Quaia* inigaia de rimpresskm □ includes supplementary material / Con^and du materiel si^^mentaire □ Pages wholly or partially obscured by errata slips, tissues, etc., have been refilmed to ensure the best possible Image / Les pages totatamant ou partiellement obscurcies par un feuillet d'errata, une pehire, etc.. ont M film^es k nouveau de fa(on k obtenir la maiaura image posiribla. □ Opposing pages with varying colouration or dIseoiouratkNW ara flbned iwfea 10 antura ttw batt possible image / Les pages s'opposant ayant des colorations variables ou des d^cotoratlons sont likn<as deux fois afin tfoManir la maMaura hnaga follovs: p. 199-200. coBM suit: p. 199-200. tOx 14x 18x 22x 26x 30x I I I I i I 1 I I I 1-/1 I I ITTl Ifx 20x 24x aix 12s 92x Th« copy filmed h«r« hM bMn raprwIiiMrf ttin l n to th« flMMTOWty of: University of Toronto Gerstein Sciences Information Centre Th« imagM appMring hara ara tha bast quality pesaibia conaMaring tha condition and lagibillty of tho orltliiol eopv oftd in hoopi n g wMi tiw Origifiol e o p loa In printod popor oovors aro Mmod bag Inning wiiti tfia front oow and anding on tha last paga with a printod or Hluatratod Impraa •ion. or tha back eovor whan approprlata. All othar original copiaa ara fllmad boginning on tha first paga with a printad or Hluatratod Imprao- alon. and onding on tho loot pofo wMi o printod or WiMtfscod improoalont Tho laat racordad frama on aach microflcho shall contain tha symbol (mooning "CON- TINUED"!, or tho symbol ▼ (mooning "iNO"). whiolMvor oppMoOa IMopo. platao. charts, ate., moy bo fiimod ot diffarom raduetien ratios. Thoaa too iorgo to ba antiraiy includad in ona axposura ara fllmad beginning in tha uppar laft hand eomor, loft to right and top to bonom, as many frames as raquirad. Tha following diagrams iUuatrata tho inotliods L'M«mplair« film* fut w p r od yh sriM A to University of Toronto Gerstein Sciences Information Centre Lm imagM suivantM ont *t* reproduitM avac la plus grand soin. compta tanu da la condition at da to nattat* da raaampto^ film*, at an Ua aiiamptolraa ariginaua dont to aoiraartwra an papiar aat iniprinida aont fHmda an eomman^ant par to pramiar ptot at an tarminant soit par la darniira paga qui comporta una amprainta d'impraasion ou d'llluatratiMi. soit par la sacond ptot. aaton to eas. Toua toa awtraa aaamptoiraa O fl g inaui i sont fHmda an eowwianyant par to pfaniMva paga quI aonipwta tma ampraints d'impraasion ou d'illustration at an tarm inpm par to damtora paga qui eomparta una taito Un daa symbolas suivants apparaitra sur la damiira imaga da ehaqua micrefieha. salon la eaa: to aymboto signifto "A tUIVRI". to vynNMia ▼ atgnma rf iv • Laa canaa. ptonchaa. tabtoaux. ate., pauvant *tra fltomte A rfaa tMiM da rMuatton dtftArants Lorsqua to documant ast trap grand pour itra raproduit an un saul cliche, il ast film* A partir da i'angto supAriaur gaucha, da gaucha i droita. •t da haut an baa. an pranant to nombra tflmataa nteaaatira. Laa dto y p mm aa anivbnta 1 2 3 3 6 J) Rrprtnted (or privutc < in nl,itii>n irom The AsT«OMiV!»K'Al Joi-BNAt, \ XI. MI, Ni>. s. M'"' 1-0 DESIR.\BILITY OF OBSERVATIONS OF THE SOLAR ROTATION AT THE I IMI S OF ECI.IPSK Tn th'' lini'-^ <>l' --pt'itrii from the solar limi) tluTc lilt iiilini; of such nature as to alft'it the mcusurfments of tht- velocity of tlio sun's rotation from the displacements of these h'nes. The mapni- tude of till- olTi'it varies from line to line, \ arious fa(tor> eon- tribute to the blendinR oi spectra." The factors oiu ratinj; l)etween the moon and the point of ohser\-ation arc nearl\ eliminated just before and after totality, when only the limb under observation is visible. To inv( stijiate the problem a i)o\verful sju'i troseope (proilucinj; .spectra of scale alK)Ut i mm to i .\) is necessary an<l a large image of the sun preferred. The region of the ft-group is su^>;este(l because the effect of liKmlini; is known for the /' lines and others near them, and because iodine and chlorine conii>ari>on spectra are available. It is ver>' desirable that such observations be made at the eclipse of June S, so that terrestrial souri tsof lilended spi'ctra may be removed in order to investigate the s»>lar and inter- planetary sources. The observations need not interfere with those during the precious seconds of totality. At least one ])art\- is ])lanninj;' to make ileterminat ions of tlic speed of rotation of the corona from displacements of the coronal lines at the time of total eclipse on June 8. In view of the fact that Deslandres. ("ami)bell. and Bosler haxc obtained \ahu- of this speed of from ,^ to 4 km j>er second, it is very imjMjrtanl that every precaution be taken to keep check on the errors that beset such measurements, in this regard I would suggest that the si>ec- troscope be used to determine the \ilocit\- of rotation of the re\ersini; laver by observations of the last and west limbs of the ■ Journal •■>' Ihr Royai .1 \lro>iomii ,tl Sm ni i lo, Joi iqi6; Astrophysiittl Joiirmtl, 44, 177 -i.Sg, ami i<)<), n>i6. •K<lwin B. Frost, Popular AslroHomy, a6, no, iqiS. Ml), ^inil .t4i 45 7 1 300 MFSOR COSTKIBl'TfOSS ASD NOTES sun before and after totality of eclipse, using a comparison sjH-c- trum and empioyinK precisely the same ntethoti in determining the velocity from the coronal lines. In this way otu- can jud^c as to the reliability of the latter. If it is im{K)ssihle to use an arc or a spark comparison spectrum, the stronger iodine absorption lines or the narrow strips of continuous spectrum between them may be found suitable in the neighborhood of X 530^. Ralph t. DeLiry Dominion .\stbunomic.\l Ubservatory, Orr\w\ April 1, 1918