A possible generation mechanism of Type III-like solar radio bursts

Details A possible generation mechanism of Type III-like solar radio bursts A possible generation mechanism of Type III-like solar radio bursts

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...134..268z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 134, no. 2, May 1984, p. 268-272.

Astronomy and Astrophysics

Astrophysics

3

Plasma-Particle Interactions, Solar Corona, Solar Electrons, Type 3 Bursts, Circular Polarization, Cyclotron Radiation, Plasma Frequencies, Plasma Waves, Radio Frequencies, Solar Magnetic Field, Wave Excitation

Scientific paper

It is shown that Type III-like bursts can be generated by streams of energetic solar electrons in the regions where the cyclotron branch of plasma waves is strongly excited. This hypothesis explains such properties of Type III-like bursts as shorter duration at a fixed frequency and faster frequency drift compared with analogous parameters of Type III bursts and some others.

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