Calibration on the Sun for stellar magnetic fields

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4466

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DC Field	Value	Language
dc.contributor.author	Sivaraman, K. R	-
dc.contributor.author	Bagare, S. P	-
dc.contributor.author	Gupta, S. S	-
dc.contributor.author	Kariyappa, R	-
dc.date.accessioned	2009-05-19T15:13:45Z	-
dc.date.available	2009-05-19T15:13:45Z	-
dc.date.issued	1987-07	-
dc.identifier.citation	5th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun., pp. 47 - 50	en
dc.identifier.uri	http://hdl.handle.net/2248/4466	-
dc.description	Restricted Access	-
dc.description.abstract	The intimate association between the surface magnetic fields and the Ca II K-line emission known to exist on the Sun, holds a promise for using this property to detect the presence of global magnetic fields on Sun-like stars. A large number of K-line profiles were obtained over a variety of plages on the Sun and related the 1A emission flux centered at the K3 minimum for these profiles with the corresponding values of the longitudinal component of the magnetic field. This provides a calibration for detecting and estimating the surface magnetic fields on stars.	en
dc.language.iso	en	en
dc.publisher	Springer	-
dc.subject	Astrophysics	en
dc.subject	Calibrating	en
dc.subject	Stellar Magnetic Fields	en
dc.subject	Sun	en
dc.subject	Surface Properties	en
dc.subject	Calcium	en
dc.subject	Emission Spectra	en
dc.subject	K Lines	en
dc.title	Calibration on the Sun for stellar magnetic fields	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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