CA II K bright points and the solar cycle

Details CA II K bright points and the solar cycle CA II K bright points and the solar cycle

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...94..235s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 94, Sept. 1984, p. 235-238.

Physics

2

Chromosphere, K Lines, Solar Cycles, Solar Spectra, Calcium, Fine Structure, Secular Variations, Spectroheliographs

Scientific paper

Number counts of the bright points that populate the interior of the Ca II network in the solar chromosphere for four solar cycles have been made. It is found that the number of these fine structures during the solar maximum exceeds that during the minimum phase on an average by 30 percent. 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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