Comparison of flare bremsstrahlung resulting from energetic thermal and nonthermal electrons

Details Comparison of flare bremsstrahlung resulting from energetic thermal and nonthermal electrons Comparison of flare bremsstrahlung resulting from energetic thermal and nonthermal electrons

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...51..185d&link_type=abstract

Solar Physics, vol. 51, Jan.-Feb. 1977, p. 185-193.

Physics

5

Bremsstrahlung, Electron Energy, Solar Flares, Solar X-Rays, X Ray Spectra, Astronomical Models, Distribution Functions, Solar Spectra, Thermal Plasmas

Scientific paper

The paper investigates the behavior of the X-ray bremsstrahlung spectra resulting from two distinct types of electron distribution functions impinging on a target atmosphere during flare activity. A power-law distribution function is compared with two double-peaked Maxwellians. The results of these calculations show that it would be difficult to rule out multithermal interpretations for the emitted high-energy X-rays.

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