Solar magnetic field and rotation

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/187

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DC Field	Value	Language
dc.contributor.author	Gokhale, M. H	-
dc.date.accessioned	2005-01-08T05:18:01Z	-
dc.date.available	2005-01-08T05:18:01Z	-
dc.date.issued	1988	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 73-80	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/187	-
dc.description.abstract	Sun’s highly inhomogeneous asymmetrical, and time dependent magnetic field plays a vital role in the non-Radiative energy transport that maintains the inhomogeneous asymmetrical and time dependent atmosphere of the sun so much hotter that the surface. Along with convection, Sun’s radiation plays an important role in maintaining the highly inhomogeneous and time dependent magnetic field of the sun. Here I briefly review our knowledge of magnetic field and rotation the two interrelated attributes of the sun on various scales.	-
dc.format.extent	282774 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar magnetic field	en
dc.subject	Solar rotation	en
dc.title	Solar magnetic field and rotation	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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