Hα Solar Flare Activity in Bou 2030 and 2032, SERF Interval, October 6-8, 1979

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

During the SERF interval of the SMY, October 4 to 9, 1979, observations of regions Bou 2030 and 2032 were coordinated. The analysis of H-alpha observations indicates that, contrary to expectations, flares initiated in magnetically simple sunspot groups. The enhanced occurrence of flares was located in an area with pronounced changes of polarity and structure of the background field. In analysing the pre-flare situation in a particular active region, therefore, it is necessary to know the characteristics of the large-scale field as well.

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