LITERATURE <>f THE BPECTROSCOPE. 



< )m tin- presence of dark lines in the solar Bpectram which correspond 

 closely to the lines of the Bpectram of oxygen. 



Draj Am.T. Jour. Sci., (8) 16,266 66 j Nature, 18. I 



Bi iblatter, 3, 188 A.bs. i; Jour. Chera. Soc., 36. '.''.'7. 



M> aure de ('intensity de quelqaes raits obscures du Bpectre solaire. 

 Gouy. Comptea Rendus, 91, 888 ; Jour. Chi M 



Beiblatter, 5. 16 i A.bs.). 



Dunkle Linien des Sonnenspectrums. 



Jahresber. d. Chemie, 16, 107, 110. 



A method of examining refractive and dispersive powers by prismatic 

 reflection. 



Wollaston (W. H.). Phil. Trans. (1802), 866. 



Ursache ihr nn^leichen Intensitiit der dunklen Linien im Bpectram der 

 Sonne. 



ZOUner (F.). Ann. Phys. u. Chem., 141. 878. 



10, Displacement of the solar spectrum. 



Note on the displacement of the solar spectrum. 



Hennessey (J. II. N.). Proc. Royal Boc., 22. 219. 



Ohservations on the displacement of lines in the Bolar spectrum cansed 

 by the Sun'.- rotation. 



Young (C. A. I. Aim-r. JoUT. Sri.. 12 121 - 



1 1, Kclijitc Spectra. 



On the solar eclipse of Dec. 22, 1870, observed at Keres, in Spain. 

 Abbay (R.). Monthly Notices Ajtronom. Boc., 31. 60 



Observations on the total eclipse of the Bun of 1869. 

 A.bbe (0.). Am.T. Jour. - 8,264 



I >n the total solar eclipse of May IT. 1882. 



\V de W and Bhuatei \ Phil. Trans., 175. 268 271 ; 

 Pi B j kl Si • . 35. l.'.l [A '' S tture, 



26 



Eclisse totale del 22 Die. 1870. 



\ \ Pal( rmo, i v 7<). 



On the results of the pic observations of the solar eclipc 



July 29, L8W 



17, 121-6. 



