Spotless flares and the associated radio continuum emission

Details Spotless flares and the associated radio continuum emission Spotless flares and the associated radio continuum emission

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..111..103r&link_type=abstract

(Observatoire de Paris, CNRS, CNES, et al., CESRA Workshop on Particle Acceleration and Trapping in Solar Flares, 2nd, Aubigny-s

Physics

10

Continuous Radiation, H Alpha Line, Solar Flares, Solar Radio Emission, Solar Cycles, Solar X-Rays

Scientific paper

Twenty-four spotless flares of H-alpha importance not less than 1 which occurred during the 21st cycle of solar activity are studied. The spotless flares could be grouped in three categories according to their location and time history of the associated active region. The association of the flares with radio events was based on relative timing and on the flare importances. Weak microwave gradual rise and fall events were frequently recorded during the occurrence of the spotless flares. A few flares from the sample could be associated with impulsive and complex microwave bursts. Only in one case an association of a spotless flare with a significant metric type II/IV event seems to be justified.

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