A comparison of the height distributions of solar flare hard X-rays in thick target and thermal models

Details A comparison of the height distributions of solar flare hard X-rays in thick target and thermal models A comparison of the height distributions of solar flare hard X-rays in thick target and thermal models

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8119990e&link_type=abstract

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Mathematics

Atmospheric Models, Bremsstrahlung, Height, Solar Flares, Solar X-Rays, Spatial Distribution, High Temperature Plasmas, Mathematical Models, Photons, Spatial Resolution, Sun, Thermal Emission

Scientific paper

The height structure of hard X-ray bremsstrahlung emission in solar flares is computed for two different models of bremsstrahlung production: emission from a descending beam of nonthermal electrons, and thermal emission from a coronally confined hot plasma. It is shown how these models give rise to hard X-ray spatial distributions which are distinguishable by current instrumentation, and that, therefore, the models may be distinguished by such spatially resolved hard X-ray measurements.

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