The solar-active-region latitudinal distribution peculiarities

Details The solar-active-region latitudinal distribution peculiarities The solar-active-region latitudinal distribution peculiarities

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..414k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Mar.-Apr. 1988, p. 414-421. In Russian.

Astronomy and Astrophysics

Astronomy

1

Latitude, Secular Variations, Solar Activity, Spatial Distribution, Long Term Effects, Solar Cycles

Scientific paper

Analysis of solar short-lived active region (SAR) data during 1969 - 1981 allows quantitative description of the SAR latitudinal distribution peculiarities in the solar cycle. Latitudinal inhomogeneity of SAR appearance on the solar surface is found. The law of the SAR mean latitude decrease during the solar cycle (Spörer law) is described quantitatively. The two 22-year active region cycles having 11-year phase shift are shown to coexist constantly on the Sun.

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