On the Role of Nonthermal Electrons in EUV and X-ray Line Emissions from Solar Flares

Details On the Role of Nonthermal Electrons in EUV and X-ray Line Emissions from Solar Flares On the Role of Nonthermal Electrons in EUV and X-ray Line Emissions from Solar Flares

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997japa...18...57b&link_type=abstract

Journal of Astrophysics and Astronomy, Vol. 18, p.57

Astronomy and Astrophysics

Astrophysics

Solar Flares: X-Ray, Euv Line Emission, Non Thermal Particle Distribution

Scientific paper

The energy and angular distribution of electrons as a function of column densities initially for monoenergetic and monodirectional electron beams and incidence angles of 0(degree), 30(degree) and 60(degree) have been studied by combining small angle scattering using analytical treatment with large angle collisions using Monte Carlo calculations. Using these distributions, X-ray and EUV-line flux have been studied as a function of column density. It is observed that the line flux increases with the increase in column density, becoming significant at intermediate column densities where the electron energies and angular distributions have a non-Maxwellian nature.

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