Role of non-thermal electrons on the generation of X-ray and EUV lines in solar flares

Details Role of non-thermal electrons on the generation of X-ray and EUV lines in solar flares Role of non-thermal electrons on the generation of X-ray and EUV lines in solar flares

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.148...75b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 148, no. 1, Oct. 1988, p. 75-84.

Astronomy and Astrophysics

Astrophysics

1

Electron Distribution, Extreme Ultraviolet Radiation, Solar Flares, Solar X-Rays, Electron Energy, Incident Radiation, Monte Carlo Method, Particle Collisions, Solar Spectra

Scientific paper

The energy and angular distributions of electrons have been studied by combining small angle scatterings using analytical treatment with large angle collisions using Monte Carlo calculations as a function of column density for initially power-law electron distributions and incidence angles of 0, 30, and 60°. Using these distributions the X-ray and EUV line flux as a function of column density has been computed. The calculated flux is compared with the observations.

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