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CA II K bright points and the solar cycle

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dc.contributor.author Sivaraman, K. R
dc.date.accessioned 2008-09-22T16:06:25Z
dc.date.available 2008-09-22T16:06:25Z
dc.date.issued 1984-09
dc.identifier.citation Solar Physics, Vol. 94, No. 2, pp. 235 - 238 en
dc.identifier.issn 0038-0938
dc.identifier.uri http://hdl.handle.net/2248/3777
dc.description.abstract We have made number counts of the bright points that populate the interior of the Ca II network in the solar chromosphere for four solar cycles. We find that the number of these fine structures during the solar maximum exceeds that during the minimum phase on an average by 30%. The contribution due to this excess number would need to be taken into account while explaining the variation in the Ca II K emission profiles of the integrated sunlight from the solar minimum to the maximum. en
dc.language.iso en en
dc.publisher Springer en
dc.relation.uri http://www.springerlink.com/content/k067tlk932363615/ en
dc.subject Ca II Network en
dc.subject Solar Chromosphere en
dc.subject Solar Cycles en
dc.subject Ca II K emission profiles en
dc.subject Integrated Sunlight en
dc.subject Solar en
dc.title CA II K bright points and the solar cycle en
dc.type Article en

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