Computer Science
Scientific paper
Aug 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980artsa..15...94p&link_type=abstract
(International Seminar of Magnetosphere, Ionosphere and Interplanetary Space, 2nd, Warsaw, Poland, June 21-23, 1979.) Artificial
Computer Science
Energetic Particles, Magnetic Storms, Proton Flux Density, Proton Precipitation, Dynamic Response, Equatorial Atmosphere, Explorer 45 Satellite, Intercosmos Satellites, Plasmapause, Proton Energy
Scientific paper
Proton flux dynamics for energies exceeding 0.5 MeV is studied on the basis of Intercosmos-5 data obtained at the commencement of the main phase of the magnetic storm of February 24, 1972. Intercosmos-17 observations of energetic proton precipitation are compared with simultaneous observations performed by Explorer-45 of 1-560 keV electrons and 1-800 keV protons in the equatorial plane. A detailed analysis is given of two successive injections of ring-current particles and energetic particles detected by Explorer-45. Observations at low and high altitudes were used to analyze the mechanism of energetic proton precipitation during magnetic storms.
Kudela Karel
Kuznetsov Sergei N.
Popielawska Barbara
Vakulov P. V.
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