Flare activity prediction from the polarization distribution of microwave emission of sunspot groups

Details Flare activity prediction from the polarization distribution of microwave emission of sunspot groups Flare activity prediction from the polarization distribution of microwave emission of sunspot groups

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990leur.work..526m&link_type=abstract

Workshop held in Leura, Australia, 16-20 Oct. 1989

Computer Science

Sun: Solar Flares- Microwave Emission-Preflare Stage

Scientific paper

In this paper using one-dimensional scans of polarization distribution of microwave emission in active regions, as obtained at the Siberian Solar Radio Telescope (SSRT, lambda=5.2 cm) during 1982-1986, an analysis is made of cases of an obvious violation of the Tanaka-Enome criterion before proton flares, and a modified criterion is suggested, which takes account of the active region position on the solar disk. A comparison is made of the two criteria and it is shown that the modified criterion provides a more powerful tool for preceding the active region conditions.

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