Physics
Scientific paper
Oct 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.1904m&link_type=abstract
(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, Russia, Nov. 1-3, 1990, Materialy. A92-40776 16-93) Akademiia Nauk
Physics
Electron Acceleration, Energy Spectra, Magnetically Trapped Particles, Solar Flares, Solar Spectra, Coronal Loops, Magnetohydrodynamic Waves, Particle Precipitation, Resonance Scattering
Scientific paper
Evolution during the energy spectrum of accelerated electrons is calculated within the framework of a model of an adiabatic magnetic trap with partial precipitation into loss cones as a consequence of resonance scattering on MHD waves. An explanation is proposed for the difference discovered during the experiment between electron spectra from impulse and prolonged flares.
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