Sunspot Groups as Tracers of Sub-surface Processes

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DC Field	Value	Language
dc.contributor.author	Gokhale, M. H	-
dc.date.accessioned	2008-08-12T08:47:35Z	-
dc.date.available	2008-08-12T08:47:35Z	-
dc.date.issued	2000-12	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 21, No. 3 – 4, pp. 155 - 160	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2248/3063	-
dc.description.abstract	Data on sunspot groups have been quite useful for obtaining clues to several processes on global and local scales within the sun which lead to emergence of toroidal magnetic flux above the sun's surface. I present here a report on such studies carried out at Indian Institute of Astrophysics during the last decade or so.	en
dc.format.extent	671506 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2000JApA...21..155G	en
dc.subject	Sunspot Group	en
dc.subject	Solar Cycle	en
dc.subject	Solar Rotation	en
dc.title	Sunspot Groups as Tracers of Sub-surface Processes	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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