Characteristics of the penetration of solar protons into the earth magnetosphere during the event of 24-25 April 1979

Details Characteristics of the penetration of solar protons into the earth magnetosphere during the event of 24-25 April 1979 Characteristics of the penetration of solar protons into the earth magnetosphere during the event of 24-25 April 1979

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kosis..24..468g&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 24, May-June 1986, p. 468-471. In Russian.

Computer Science

Magnetospheric Proton Density, Solar Protons, Solar Terrestrial Interactions, Capture Effect, Earth Atmosphere, Fine Structure, Geomagnetic Latitude, Intercosmos Satellites, Magnetic Storms, Spatial Distribution

Scientific paper

The latitude profiles and the dynamics of penetration boundaries of 0.9-8.0-MeV solar protons are examined with reference to Intercosmos-19 data and compared against the locations of the external capture boundaries of electrons with eneregies of 40 keV or greater, 0.3-0.6 MeV, and 0.9-1.2 MeV. Data on the fine structure of the development of magnetospheric substorms and storms are discussed.

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