Evolutionary electron beam and MHD two stream instability in solar radio burst models

Details Evolutionary electron beam and MHD two stream instability in solar radio burst models Evolutionary electron beam and MHD two stream instability in solar radio burst models

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983baicz..34...18k&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 34, Jan. 1983, p. 18-22.

Astronomy and Astrophysics

Astronomy

1

Electron Beams, Magnetohydrodynamic Stability, Stellar Models, Stream Functions (Fluids), Type 3 Bursts, Distribution Functions, Electron Acceleration, Time Dependence

Scientific paper

This paper represents a contribution to the theory of type III and IIIb solar radio bursts. It tries to clarify the role of the MHD two stream instability in the case of the evolutionary electron beam. It is shown that, in this case, the generation of the MHD two stream instability depends on strong depression of quasilinear relaxation (caused by a bump-on-tail instability). The results of this paper are compared with the ideas used in Smith's and de la Noë's (1976) model of type IIIb burst.

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