Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...237.1015e&link_type=abstract
Astrophysical Journal, Part 1, vol. 237, May 1, 1980, p. 1015-1023.
Astronomy and Astrophysics
Astrophysics
36
Bremsstrahlung, Heat Flux, Polarization (Waves), Solar Flares, Solar X-Rays, Anisotropy, Conductive Heat Transfer, Directivity, Electron Beams, Mathematical Models, Maxwell-Boltzmann Density Function, Photons, Temperature Effects
Scientific paper
The polarization and directivity of hard X-ray bremsstrahlung from a thermal source consisting of a region in which a thermal flux drives a pair of steel collisionless conduction fronts were evaluated. The conduction fronts are symmetrically driven from a central region, heated by the flare energy dissipation process. By comparing results with similar calculations based on a nonthermal thick-target electron beam model of the source, it was aimed to determine the degree to which the observed polarization and directivity of solar flare hard X-rays favor either model. Results which exhibit significant polarization and directivity of the hard X-ray radiation emitted by the source are produced by using Maxwellian electron-phase-space distribution functions modified to take into account a directional heat flux and a steady direct current in the X-ray source, and a fully relativistic treatment of the bremsstrahlung emission process. The results are consistent with solar hard X-ray anisotropy and polarization observations to date, although these observations are too crude to be conclusive.
Brown John C.
Emslie Gordon A.
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