A complex of active regions in April-August 1980 period

Details A complex of active regions in April-August 1980 period A complex of active regions in April-August 1980 period

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983baicz..34..277i&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 34, no. 5, 1983, p. 277-281.

Astronomy and Astrophysics

Astronomy

1

Solar Activity, Sunspots, Solar Flares, Solar Magnetic Field, Solar Rotation

Scientific paper

Evidence is presented that a group of active flare regions formed a complex of flare activity. The regions were observed during the SERF program of the Maximum Solar Year in May and June, 1980. The evidence is based on the following characteristics of the complex: the influence of differential rotation on the individual components of the complex; magnetic field structures and the behavior of magnetic fluxes in the complex components; the occurrence of quasi-synchronous flares in active regions of the complex. In an analysis of these characteristics it was confirmed that there is a close physical connection between the activities of individual active regions and a complex of activity. The complex of activity is estimated to have lasted at least 5 months between April and August, 1980 and was most active and compact during the month of June.

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