CA II K2V spectral features and their relation to small-scale photospheric magnetic fields

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4101

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DC Field	Value	Language
dc.contributor.author	Sivaraman, K. R	-
dc.contributor.author	Livingston, W. C	-
dc.date.accessioned	2008-12-17T16:38:18Z	-
dc.date.available	2008-12-17T16:38:18Z	-
dc.date.issued	1982-10	-
dc.identifier.citation	Solar Physics, Vol. 80, No. 2, pp. 227 - 231	en
dc.identifier.issn	0038-0938	-
dc.identifier.uri	http://hdl.handle.net/2248/4101	-
dc.description	Open Access	-
dc.description.abstract	Although the Ca ii K232 network is known to be cospatial with magnetic elements there has been doubt as to the magnetic origin of the fainter K2V points. We demonstrate that weak magnetic elements also lie at the roots of the K2V points, and because the latter are numerous they may contribute sensibly to the integrated light profile of Ca ii K.	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Co.,	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1982SoPh...80..227S	en
dc.relation.uri	http://www.springerlink.com/content/p2718j3330533052/	en
dc.rights	© D. Reidel Publishing Co.,	en
dc.subject	K Lines	en
dc.subject	Photosphere	en
dc.subject	Solar Magnetic Field	en
dc.subject	Solar Spectra	en
dc.subject	Calcium	en
dc.subject	Magnetic Signatures	en
dc.title	CA II K2V spectral features and their relation to small-scale photospheric magnetic fields	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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