Pulse beam heating of solar atmosphere

Details Pulse beam heating of solar atmosphere Pulse beam heating of solar atmosphere

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991baicz..42...22k&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 42, Feb. 1991, p. 22-30.

Astronomy and Astrophysics

Astronomy

5

Atmospheric Heating, Electron Beams, Magnetohydrodynamics, Solar Atmosphere, Solar Flares, Electron Energy, Radiative Heat Transfer, Solar X-Rays, X Ray Spectra

Scientific paper

The response of the solar atmosphere to pulse beam heating was computed using a one-dimensional hybrid code. Whereas the hydrodynamic part of this program was used to compute the atmospheric response, the pulse beam decelerated by electron-electron interactions in the dense layers of the solar atmosphere is represented by particles. In this new description of the electron beam, the finite transit time of electrons accelerated in flare loops is taken into account and the hard X-ray radiation has been computed directly.

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