Physics
Scientific paper
Jul 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982kosis..20..560z&link_type=abstract
Kosmicheskie Issledovaniia, vol. 20, July-Aug. 1982, p. 560-565. In Russian.
Physics
Current Sheets, Electron Distribution, Interplanetary Magnetic Fields, Solar Flares, Solar Radio Bursts, Electron Energy, Solar Position, Solar Wind
Scientific paper
A correlation is established between maximum fluxes of electrons with energies exceeding 30 keV from solar flares and the maximum intensity of radio bursts with a wavelength of 10 cm. It is shown that the propagation conditions are most favorable when the flare is located near the projection of the sector boundary of the interplanetary magnetic field onto the solar surface. The electron flux becomes appreciably less intense when the flare is located at the center of the sector in a local magnetic-field region with a sign that is different from its direction in this sector.
Kovrizhnykh O. M.
Livshits Moisey A.
Zeldovich M. A.
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