Solar activity

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