On the fine structure of the Wolf number solar activity index

Details On the fine structure of the Wolf number solar activity index On the fine structure of the Wolf number solar activity index

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..157k&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Solar Activity, Wolf Numbers: Fine Structure

Scientific paper

The fine structure of the Wolf number index W of the solar activity is presented by three components: secular, 11-year cycle, and quasi-biennial. It is suggested that the quasi-biennial oscillations are the main features of the 11-year cycles. The attempt to simulate them by analytical functions is presented. The spectral properties of the whole W values time-series are discussed. A conception of the Sun as a magnetic variable star is suggested.

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