Physics
Scientific paper
Sep 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...99..189m&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 99, Sept. 1985, p. 189-217. Research supported by Koninklijke Nederlandse Akademie van Wete
Physics
19
Solar Flares, Solar X-Rays, X Ray Imagery, Bursts, Chromosphere, Energy Dissipation, Light Curve, Solar Electrons, Thermal Emission
Scientific paper
An analysis is conducted of the X-ray imaging data obtained for three flares of markedly different characteristics in order to distinguish the relative efficiencies of heating and acceleration in the primary energy release. The computed hard X-ray distribution and energy deposition due to accelerated electrons, with beam and ambient plasma parameters appropriate to each of the observed events, are convolved with the Hard X-ray Imaging Spectrometer instrument response and compared with observations. In view of the results obtained, the observed emission was primarily due to the strong heating that is intrinsic to a reconnection process within the region of interaction between two magnetic structures seen in the soft X-ray data. Attention is also given to the heating effect of a beam, due to Coulomb losses, during its passage through the flare loops.
Machado Marcos E.
Rovira Marta G.
Sneibrun C. V.
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