CA II K bright points and the solar cycle

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3777

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DC Field	Value	Language
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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