Inversion of bremsstrahlung spectra emitted by solar plasma

Details Inversion of bremsstrahlung spectra emitted by solar plasma Inversion of bremsstrahlung spectra emitted by solar plasma

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...288..949p&link_type=abstract

Astronomy and Astrophysics 288, 949-959 (1994)

Astronomy and Astrophysics

Astrophysics

23

Radiation Mechanisms: Thermal, Non-Thermal, Methods: Analytical, Sun: X-Rays

Scientific paper

Bremsstrahlung radiation coming from the solar atmosphere is linked to the distribution function of electrons in the solar plasma through a Volterra equation of the first kind. We have assumed the Bethe-Heitler approximation for the bremsstrahlung cross section and we have applied the SVD method to the integral equation with discrete data. Using Tikhonov's regularisation technique, reconstructions of the electronic distribution functions have been obtained, both for simulated and real data.

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