A preliminary note on the displacement to the violet of some lines in the solar spectrum

dc.contributor.author	Royds, T
dc.date.accessioned	2006-06-29T05:32:18Z
dc.date.available	2006-06-29T05:32:18Z
dc.date.issued	1914-04-18
dc.identifier.citation	Kodaikanal Observatory Bulletin No. 38, pp. 59-69	en
dc.identifier.uri	http://hdl.handle.net/2248/1135
dc.description.abstract	The majority of the metallic lines in the solar spectrum are shifted to the red when compared with their positions in the electric are. There are, however, many exceptions. In the tables at the end of this paper I give the results of some comparisons of are spectra (chiefly iron) with the spectrum of the centre of the sun`s disc for the study of these exceptions	en
dc.format.extent	884046 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar spectrum	en
dc.title	A preliminary note on the displacement to the violet of some lines in the solar spectrum	en
dc.type	Article	en