Occurrences of Flares with Type II and IV Radio Events in Interacting Sunspot Groups in the Course of Revolutions

Details Occurrences of Flares with Type II and IV Radio Events in Interacting Sunspot Groups in the Course of Revolutions Occurrences of Flares with Type II and IV Radio Events in Interacting Sunspot Groups in the Course of Revolutions

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984baicz..35..273k&link_type=abstract

Bulletin of the Astronomical Institute of Czechoslovakia, vol. 35, p.273

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Scientific paper

Using data from 11-year solar cycle No. 20, it was found that flares with type II radio bursts are more than twice as frequent and flares with type IV bursts nearly twice as frequent in sunspot groups which developed close to each other or which merged in the course of revolutions as in isolated sunspot groups. With both types the occurrence of these flares is concentrated in the revolution of the so-called sunspot group interaction (their approximation, merging).

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