Other
Scientific paper
Sep 1972
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ssrv...13..827d&link_type=abstract
Ultraviolet and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas, Proceedinsg of IAU Colloq. 14, held in Utrecht, Augu
Other
4
Scientific paper
Recent observations of the energetic particles produced in solar flares indicate that the production of electrons, with energies up to about 100 keV, is a fairly common feature of small flares. In those flares the acceleration of protons and other nuclei does not extend beyond about 1 MeV. The X-ray emission often exhibits two distinct components of which the first one is produced by non-thermal, the second by thermal electrons through bremsstrahlung collisions with the ambient ions. Along with these X rays, radio emission, in the microwave region, is observed. This radio emission is usually interpreted as due to gyrosynchrotron radiation from the same electrons. In this review a discussion is presented of the processes occurring in solar flares with special reference to the acceleration and radiation processes.
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