One more feature of the 11-year cycle of solar activity

Details One more feature of the 11-year cycle of solar activity One more feature of the 11-year cycle of solar activity

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67.1109z&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Sept.-Oct. 1990, p. 1109-1111. In Russian.

Mathematics

Probability

Annual Variations, Faculae, Solar Activity, Solar Cycles, Probability Density Functions, Solar Flares, Statistical Analysis, Sunspots

Scientific paper

A statistical analysis of multiyear data on the main indices of solar activity was performed in order to identify differences in their probability distribution functions at the extremum epochs of the 11-year cycles. It is shown that, when passing from the minimum to the maximum periods (according to a given index), large values of spot formation indices, flare activity, and the number of faculae in the sun's polar regions increase to a considerably lesser extent than small values, this difference reaching a factor of 230.

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