The polarization and directivity of solar-flare hard X-ray bremsstrahlung from a thermal source

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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.

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