Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..409b&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Mar.-Apr. 1990, p. 409-419. In Russian.
Astronomy and Astrophysics
Astronomy
6
Coronal Loops, Interplanetary Space, Particle Acceleration, Proton Flux Density, Solar Flares, Solar Protons, Current Sheets, Solar Radio Bursts, Solar X-Rays, Temporal Distribution
Scientific paper
Based on an analysis of the dynamics of flare bursts and proton fluxes, it is argued that particles accelerated in high coronal current sheets during the formation of postflare loop systems may significantly contribute to the greater-than-10-MeV proton fluxes near the earth. The associated flares are characterized by prolonged X-ray and multicomponent radio emission with a soft peak flux density spectrum. The analyzed solar particle events are characterized by unusually enhanced proton peak intensities at about 10 MeV in the interplanetary medium and by soft energy spectra.
Bazilevskaya Galina A.
Chertok I. M.
Fomichev V. V.
Sladkova A. I.
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