Line Asymmetry and Magnetic Fields

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