New aspects of the April 27, 1981 flare

Details New aspects of the April 27, 1981 flare New aspects of the April 27, 1981 flare

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..146..199k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 146, no. 1, p. 199-202.

Physics

3

Gamma Ray Bursts, Solar Flares, Solar Radio Bursts, Coronal Loops, H Alpha Line, Plasma Pinch, Solar Limb, Solar X-Rays

Scientific paper

Very interesting radio bursts, observed during the well-known solar flare of April 27, 1981 are presented. While the sequence of reverse drift bursts, U-bursts, and radio flux depression on 9.375 GHz can be explained within the beam bombardment and evaporation model, the narrowband dm-spikes uniquely organized in 'necklace' structures seem to indicate the interaction of flare loops. Arguments in favor of the plasma emission model of narrowband dm-spikes were found.

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