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..103f&link_type=abstract

Solar Physics, Vol.111, NO. 1, P. 103, 1987

Physics

6

Scientific paper

We studied 24 spotless flares of Hα importance > 1 which occurred during the 21st cycle of solar activity. The spotless flares could be grouped in three categories according to their location and time history of the associated active region. Our 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 our 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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