Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978sva....22..338v&link_type=abstract
(Astronomicheskii Zhurnal, vol. 55, May-June 1978, p. 586-597.) Soviet Astronomy, vol. 22, May-June 1978, p. 338-344. Translati
Astronomy and Astrophysics
Astronomy
1
Particle Motion, Solar Flares, Solar Protons, Solar Radio Emission, Microwave Emission, Particle Acceleration, Plasma Layers, Solar Corona, Solar Electrons, Type 3 Bursts, Type 5 Bursts
Scientific paper
The main characteristics of the cited intense complex solar radio event, which was associated with an active-region proton flare, are discussed. A model for the motion of electrons ejected from the acceleration region is proposed along with a scenario for the generation of the main components of the event by such electrons. Estimates of the number of electrons responsible for the various bursts associated with the event are compared. The high-frequency cutoff observed for the associated Type III bursts is explained in terms of cyclotron absorption in certain layers of the magnetoactive coronal plasma.
Melnikov Victor F.
Vedeneev Iu. B.
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