Adiabatic and Non-Adiabatic Processes in Thermal Models of Solar Hard X-Ray Bursts.
STANFORD UNIV CA INST FOR PLASMA RESEARCH
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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. Author
- Nuclear Physics and Elementary Particle Physics