Hard X-rays and the electron component of solar flares

Details Hard X-rays and the electron component of solar flares Hard X-rays and the electron component of solar flares

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983kosis..21..476d&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 21, May-June 1983, p. 476-479. In Russian.

Physics

3

Solar Electrons, Solar Flares, Solar X-Rays, Bremsstrahlung, Electron Energy, Interplanetary Space, Venera Satellites

Scientific paper

An analysis is presented of simultaneous measurements performed by Venera 11, 13, and 14 of the spectra of solar electrons and hard X-rays in the range of energies from 30 keV to 1 MeV. It is shown that gamma(X) = gamma(e) + 1 describes the relation between the spectrum index of electrons measured in interplanetary space and the spectrum index of solar-flare X-rays. This relation is characteristic for a thin target of excitation of X-ray bremsstrahlung.

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