Occurrence of Flares with Type II and IV Radio Bursts in Relation to Sunspot Group Types

Details Occurrence of Flares with Type II and IV Radio Bursts in Relation to Sunspot Group Types Occurrence of Flares with Type II and IV Radio Bursts in Relation to Sunspot Group Types

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984baicz..35..261k&link_type=abstract

Bulletin of the Astronomical Institute of Czechoslovakia, vol. 35, p.261

Astronomy and Astrophysics

Astronomy

Scientific paper

The occurrence of flares was statistically processed, separately for those with type II and type IV radio bursts, in relation to the sunspot groups in which these flares took place. The period in question is cycle No. 20, 1966 - 1976. Zurich and magnetic typification were taken into account. As compared with flares accompanied by type II bursts, flares with type IV display an enhanced tendency to occur in more complex active regions in which more magnetic energy is accumulated in a small space (type δ). The occurrence of flares with type II and type IV bursts in the course of cycle No. 20 shows an anomalous behaviour, in particular a conspicuous decrease of occurrence from 1970 to 1971.

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