Magnetic flux in the solar convective envelope inferred from the initial observations of the sunspots

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1718

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DC Field	Value	Language
dc.contributor.author	Hiremath, K. M	-
dc.contributor.author	Lovely, M. R	-
dc.date.accessioned	2007-07-09T11:25:02Z	-
dc.date.available	2007-07-09T11:25:02Z	-
dc.date.issued	2007-09	-
dc.identifier.citation	Astrophysical Journal, Vol. 667, pp. 585 – 590	en
dc.identifier.uri	http://hdl.handle.net/2248/1718	-
dc.description.abstract	Different life spans of the sunspots suggest their origin at different depths and by measuring magnetic fluxes from their first observation on the surface, one can estimate the strength of magnetic flux at different anchoring depths. From the SOHO/MDI magnetograms, we infer the strength of magnetic flux and rate of emergence of magnetic flux at different anchoring depths in the solar convective envelope by measuring initial magnetic fluxes of the well developed sunspots on the ..........	en
dc.format.extent	267213 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	University of Chicago Press	en
dc.relation.uri	http://www.journals.uchicago.edu/doi/abs/10.1086/520842	en
dc.subject	Sunspots	en
dc.subject	Bipolar spots	en
dc.subject	Magnetic filed	en
dc.subject	Magnetic flux	en
dc.title	Magnetic flux in the solar convective envelope inferred from the initial observations of the sunspots	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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