Solar activity

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/186

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DC Field	Value	Language
dc.contributor.author	Gokhale, M. H	-
dc.date.accessioned	2005-01-08T05:13:56Z	-
dc.date.available	2005-01-08T05:13:56Z	-
dc.date.issued	1988	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 63-72	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/186	-
dc.description.abstract	Sun could have had a nice and perfect spherical symmetry in its atmosphere and probably no variations on time scales smaller than hundreds of thousands of years if (i) the energy produced in its core could be transported out and way by Radiative processes alone, (II) it was not rotating and (iii) it had no magnetic field. But then perhaps it would not have been as interesting as it is for so many of us have gathered here after travelling long distances inspite of the hazards offered by the “Tamil Nadu Bundh”.	-
dc.format.extent	723647 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar activity	en
dc.subject	Sunspots	en
dc.title	Solar activity	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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