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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1135

Full metadata record

DC Field	Value	Language
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
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 ) Thomas Royds (1923 - 1937)

Files in This Item:

File	Description	Size	Format
paper-38.pdf		863.33 kB	Adobe PDF	View/Open

DSpace JSPUI