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CaIIK bright points and the solar cycle

โœ Scribed by K. R. Sivaraman

Publisher
Springer
Year
1984
Tongue
English
Weight
202 KB
Volume
94
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

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.

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