Ca II K Emission from the Solar Chromosphere

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/356

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DC Field	Value	Language
dc.contributor.author	Sivaraman, K. R	-
dc.date.accessioned	2005-02-10T13:33:18Z	-
dc.date.available	2005-02-10T13:33:18Z	-
dc.date.issued	1986	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 6, pp. 11-18	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/356	-
dc.description.abstract	The role of the Ca II K line as a reliable diagnostic of the chromospheric activity on the Sun is reviewed. The chromospheric structures seen in this line serve as good indicators of the photospheric magnetic structures and also mimic the morphological changes in the surface magnetic features associated with the solar cycle. Similar changes can be expected to take place in other sun-like stars and could therefore be used as a diagnostic for inferring the kind of structures of surface magnetic fields in them.	en
dc.format.extent	266774 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Ca II K emission	en
dc.subject	solar chromosphere	en
dc.title	Ca II K Emission from the Solar Chromosphere	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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