Abstract Information regarding the acceleration of electrons in solar flares may be deduced from the hard X ray emission they produce through bremsstrahlung. From these observations, the electron energy spectra and temporal evolution as well as some characteristics of the ambient medium can be deduced through models. Here, a model of hard X ray emission is briefly presented and some of the results are discussed in the light of hard X ray observations and acceleration processes.
Electron spectra deduced from solar hard X-ray bursts
Advances in Space Research ; 4 , 2-3 ; 153-156
1984-01-01
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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