Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1764
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dc.contributor.authorHiremath, K. M-
dc.contributor.authorLovely, M. R-
dc.contributor.authorKariyappa, R-
dc.date.accessioned2007-08-13T09:32:03Z-
dc.date.available2007-08-13T09:32:03Z-
dc.date.issued2006-09-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 27, No. 2-3, pp. 333-338en
dc.identifier.urihttp://hdl.handle.net/2248/1764-
dc.description.abstractThe positional measurements of sunspots from the Kodaikanal Observatory and Solar Geophysical data are used to study the association between occurrence of the abnormal activities of big sunspot groups that were observed during the period of October-November 2003 and occurrence of the flares. During the evolution of the sunspot groups, we have investigated the temporal variations in (i) areas; (ii) rotation rates; (iii) longitudinal extents; and (iv) number of small spots produced in a sunspot group. Among all these activity variations, we find that the spot groups that experience abnormal rotation rates during their evolutionary phases eventually trigger the flaresen
dc.format.extent351152 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://www.ias.ac.in/jaa/junsep2006/absjunsep2006.html#jaa31-
dc.rights.uri-
dc.subjectSunspotsen
dc.subjectrotationen
dc.subjectextreme activityen
dc.titleThe Extreme Solar Activity during October–November 2003en
dc.typeArticleen
Appears in Collections:IIAP Publications

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