Adiabatic and non-adiabatic processes in thermal models of solar hard X-ray bursts

Details Adiabatic and non-adiabatic processes in thermal models of solar hard X-ray bursts Adiabatic and non-adiabatic processes in thermal models of solar hard X-ray bursts

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8114943e&link_type=abstract

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Physics

Adiabatic Equations, Nonadiabatic Theory, Solar Flares, Solar X-Rays, Bremsstrahlung, Coronal Loops, Magnetohydrodynamics, Mathematical Models, Solar Corona, Solar Magnetic Field, Space Plasmas

Scientific paper

The processes by which the observed characteristics of the hard X-ray
bremsstrahlung, emitted from a solar flare loop, are modulated, are
investigated. This leads us to a set of inversion formulae, giving the
behavior of physical variables in terms of observable quantities. The
method is applied to recent observational data.

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