Propagation of nonrelativistic electrons in the solar wind, and type III radio bursts

Details Propagation of nonrelativistic electrons in the solar wind, and type III radio bursts Propagation of nonrelativistic electrons in the solar wind, and type III radio bursts

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sval....3...88k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 3, Apr. 1977, p. 170-174.) Soviet Astronomy Letters, vol. 3, Mar.-Apr. 1977, p. 88-91.

Astronomy and Astrophysics

Astronomy

Electron Beams, Plasma-Particle Interactions, Solar Wind, Type 3 Bursts, Electrostatic Waves, Plasma Oscillations, Solar Flares, Time Response

Scientific paper

It is shown that the two-component structure of fluxes of electrons with energies of several tens of keV produced during solar bursts, as revealed in experiments aboard the Prognoz satellites, can be explained by a plasma mechanism of interaction of particle fluxes with the interplanetary medium. Estimates of electron beam stabilization by nonlinear processes are made.

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