Line Asymmetry and Magnetic Fields

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/388

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DC Field	Value	Language
dc.contributor.author	Livingston, William	-
dc.date.accessioned	2005-04-08T03:59:11Z	-
dc.date.available	2005-04-08T03:59:11Z	-
dc.date.issued	1984	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 4, pp. 7-9	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/388	-
dc.description.abstract	The measurement of the asymmetries of Fraunhofer lines shows promise as a diagnostic of convection at the surface layers of the Sun and Stars. We discuss today the observational evidence that the asymmetry, and by inference granular convection, is inhibited by surface magnetism	en
dc.format.extent	102040 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Line Asymmetry	en
dc.subject	Convection	en
dc.subject	Fraunhofer lines	en
dc.title	Line Asymmetry and Magnetic Fields	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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