Accelerated electrons and hard X-ray solar flare radiation in the model with reverse current

Details Accelerated electrons and hard X-ray solar flare radiation in the model with reverse current Accelerated electrons and hard X-ray solar flare radiation in the model with reverse current

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..837l&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, July-Aug. 1990, p. 837-844. In Russian.

Astronomy and Astrophysics

Astronomy

Electron Acceleration, High Temperature Plasmas, Solar Flares, Solar Radiation, Solar X-Rays, Electric Fields, Energetic Particles, Plasma Currents

Scientific paper

The behavior of accelerated electrons escaping a high-temperature plasma inside a flare loop is investigated; it was assumed that the direct current of accelerated nonthermal electrons is balanced by the reverse current of surrounding cold-plasma particles. The fast-electron distribution function and the electric field of the reverse current were determined from the solution of the self-consistent kinetic problem, and the X-ray bremsstrahlung polarization was calculated. The effect of the reverse current upon the results is discussed.

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