Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/186
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dc.contributor.authorGokhale, M. H-
dc.date.accessioned2005-01-08T05:13:56Z-
dc.date.available2005-01-08T05:13:56Z-
dc.date.issued1988-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 9, pp. 63-72en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/186-
dc.description.abstractSun 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.extent723647 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectSolar activityen
dc.subjectSunspotsen
dc.titleSolar activityen
dc.typeArticleen
Appears in Collections:Kodaikanal Observatory Bulletins (1905 - 1997 )
IIAP Publications

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