Theory of type II and type III solar radio bursts

Details Theory of type II and type III solar radio bursts Theory of type II and type III solar radio bursts

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978raf....20.1379z&link_type=abstract

(Radiofizika, vol. 20, no. 9, 1977, p. 1379-1398.) Radiophysics and Quantum Electronics, vol. 20, no. 9, Mar. 20, 1978, p. 951-9

Physics

Shock Wave Propagation, Solar Magnetic Field, Type 2 Bursts, Type 3 Bursts, Collisionless Plasmas, Electron Beams, Plasma Waves, Solar Corona, Solar Wind

Scientific paper

Radio emission from collisionless shock waves propagating across and along the coronal magnetic field is investigated. A theory of solar type II radio bursts is outlined which emphasizes the role of quasi-linear relaxation of fast electron beams during their dispersion in the solar-wind plasma. The efficiency of plasma-wave transformation into electromagnetic waves as a result of induced scattering in source regions of type III bursts is analyzed. The possible role of a modulational instability in the generation of stria-type bursts is also considered.

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