Gyrosynchrotron instability in a plasma with a beam of moderately relativistic electrons

Details Gyrosynchrotron instability in a plasma with a beam of moderately relativistic electrons Gyrosynchrotron instability in a plasma with a beam of moderately relativistic electrons

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..147..157c&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 147, no. 1, p. 157-168.

Physics

2

Magnetohydrodynamic Stability, Plasma-Particle Interactions, Relativistic Electron Beams, Solar Flares, Solar Radio Bursts, Synchrotron Radiation, Absorptivity, Electron Distribution, Emissivity, Masers

Scientific paper

The possibility of gyrosynchrotron instability development in a plasma with moderately relativistic electrons is revealed. The absorption and emission coefficients are numerically calculated for a Gaussian distribution function of these electrons. It shows the presence of emission bands Delta-omega where the absorption coefficient mu is negative, and their dependence on the half-width (Delta-nu) of the Gaussian as well as on the observation angle alpha is established. The results obtained are applied for the interpretation of microwave bursts registered during solar flares.

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