On the peculiarities of the fine structure of the 11-year solar cycle for various indices of solar activity.

Details On the peculiarities of the fine structure of the 11-year solar cycle for various indices of solar activity. On the peculiarities of the fine structure of the 11-year solar cycle for various indices of solar activity.

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992bsold...8...76v&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 8/92, p. 76 - 81

Physics

Scientific paper

Data on main extrema of the fine structure of the 11-year solar cycle are given for indices of the total area of photospheric faculae (Sf) for 1878 - 1976, density of the solar radio emission flux at 2800 MHz (F2800) for 1954 - 1986, total area of prominences (Spr) for 1964 - 1976, and the number of grouped solar flares (Nf) for 1966 - 1986. It is shown that the fine structure of the 11-year solar cycle, especially multi-peaks of its epoch of maximum, is characteristic for all considered indices of solar activity. Simplification of the fine structure especially for F2800 and Sf has been discovered.

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