The relation between the electron and X-ray bremsstrahlung spectra in solar flares

Details The relation between the electron and X-ray bremsstrahlung spectra in solar flares The relation between the electron and X-ray bremsstrahlung spectra in solar flares

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..641d&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Sept.-Oct. 1980, p. 641-644.) Soviet Astronomy Letters, vol. 6, Sept.-Oct. 1980, p.

Astronomy and Astrophysics

Astronomy

Bremsstrahlung, Plasma-Electromagnetic Interaction, Solar Electrons, Solar Flares, Solar Spectra, Solar X-Rays, Electron Beams, Electron Flux Density, Energy Dissipation, Power Spectra, Steady State, X Ray Spectra

Scientific paper

The spectrum of X-ray bremsstrahlung photons is calculated for an
exponential spectrum of radiating electrons injected in a solar flare.
In a thick-target model the photon spectrum will be steeper than the
initial electron spectrum, unlike the case when the electrons are
injected with a power-law spectrum.

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