Physics
Scientific paper
Jul 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980kosis..18..572k&link_type=abstract
Kosmicheski Issledovaniia, vol. 18, July-Aug. 1980, p. 572-579. In Russian.
Physics
Charged Particles, Interplanetary Magnetic Fields, Interplanetary Medium, Radiant Flux Density, Solar Flares, Solar Wind Velocity, Electron Energy, Energy Spectra, Proton Energy, Solar Electrons, Solar Protons
Scientific paper
The propagation characteristics of charged particles generated by a solar flare are studied on the basis of Mars-7 and Prognoz-3 data obtained at different distances from the sun. It is shown that the nature of electron intensity variations at electron energies above 40 keV and proton energies of 0.2 to 20 MeV is determined by changes in the structure of the interplanetary medium, i.e., changes in solar wind velocity and interplanetary magnetic field parameters.
Kazarian M. S.
Kuzhevskii B. M.
Maduev V. L.
Mineev Iu. V.
Shestopalov I. P.
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