On the relation between magnetic field strength and Wilson depression in sunspots

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3491

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DC Field	Value	Language
dc.contributor.author	Bagare, S. P	-
dc.contributor.author	Gupta, S. S	-
dc.date.accessioned	2008-09-08T16:56:52Z	-
dc.date.available	2008-09-08T16:56:52Z	-
dc.date.issued	1998	-
dc.identifier.citation	BASI, Vol. 26, pp. 197 - 199	en
dc.identifier.uri	http://hdl.handle.net/2248/3491	-
dc.description.abstract	At the Solar Tower Telescope of Kodaikanal Observatory, we obtained Zeeman spectra of sunspots on their disk passage during 1979-84 (Solar max. 21). Using this data and full disk white light pictures obtained at the observatory, we are examining the possible relation between Wilson Effect(WE) and longitudianal magnetic field strength (Bl)of selected spots. Preliminary results indicate that WE does not depend upon B1. Further, a large number of spots do not exhibit WE. It appears that the magnetic field configuration, rather than field strength, plays the key role in the occurrence or absence of WE.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1998BASI...26..197B	en
dc.subject	Sunspot magnetic fields	en
dc.subject	Wilson effect	en
dc.subject	Wilson depression	en
dc.title	On the relation between magnetic field strength and Wilson depression in sunspots	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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