Differences of distribution functions of solar activity indices at 11-year cycle extremum epochs.

Details Differences of distribution functions of solar activity indices at 11-year cycle extremum epochs. Differences of distribution functions of solar activity indices at 11-year cycle extremum epochs.

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990bsold...4...96z&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 4/90, p. 96 - 99

Mathematics

Probability

Solar Activity: Sunspots

Scientific paper

A significant difference of empirical probability distribution functions of a number of solar spots W at the 11-year cycle extremum epochs has been established: relatively large W at the cycle maximum are increased to a considerably less extent than small ones. The distribution functions of the radioemission density at 2800 MHz frequency differ slightly; on the contrary, higher intensities are by 10 - 20% greater than the low ones.

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