Physics
Scientific paper
Apr 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981izssr..45..609k&link_type=abstract
(Evropeiskii Simpozium po Kosmicheskim Lucham, 7th, Leningrad, USSR, Sept. 15-19, 1980.) Akademiia Nauk SSSR, Izvestiia, Seriia
Physics
Solar Electrons, Solar Flares, Solar Physics, Solar Protons, Spectral Energy Distribution, Electron Energy, Particle Diffusion, Prognoz Satellites, Proton Energy, Solar Corona
Scientific paper
The paper examines data, acquired by Prognoz 6, on flare protons and electrons with energies of 0.5-150 MeV and 0.03-3 MeV respectively which were produced by the 2N-magnitude solar flare of January 1, 1978. The spectra from this event are compared with those obtained for the flares of December 27, 1977 and December 12, 1977. The results do not contradict Zhang Gong-Liang's (1979) model of anisotropic convective proton diffusion; but it is suggested that a better description would be achieved by a model taking into account the time variations of protons and electrons, with allowance for coronal propagation.
Gros Michel
Kurt Victoria G.
Logachev Iu. I.
Pisarenko N. F.
Stolpovskii V. G.
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