The escape coefficient of electrons generated in solar flares

Details The escape coefficient of electrons generated in solar flares The escape coefficient of electrons generated in solar flares

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987izssr..51.1825d&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia (ISSN 0367-6765), vol. 51, Oct. 1987, p. 1825-1827. In Russian.

Physics

3

Interplanetary Medium, Particle Production, Solar Electrons, Solar Flares, High Energy Electrons, Microwave Emission, Particle Acceleration, Solar X-Rays, Spectral Energy Distribution

Scientific paper

The escape efficiency into interplanetary space of high-energy electrons generated in solar flares of different importance is examined. A numerical assessment is made of the measure of this efficiency, i.e., the escape coefficient, defined as alpha = Nes/Nt, where Nes and Nt are the number of escaping and accelerated electrons, respectively. The present investigation is based on an analysis of electron events and X-ray bursts recorded by the Venera 13 and 14 probes as well as data on radio bursts connected with these events.

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