Dynamics of the low-altitude boundary of the penetration of low-energy solar protons into the magnetosphere

Details Dynamics of the low-altitude boundary of the penetration of low-energy solar protons into the magnetosphere Dynamics of the low-altitude boundary of the penetration of low-energy solar protons into the magnetosphere

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25....7i&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Jan.-Feb. 1985, p. 7-12. In Russian.

Computer Science

Sound

8

Earth Magnetosphere, Equatorial Atmosphere, Incident Radiation, Solar Protons, Cosmos Satellites, Diurnal Variations, Satellite Sounding, Solar Cosmic Rays, Solar Wind

Scientific paper

Polar-satellite (Cosmos and Intercosmos-17) data for 1972-1979 are used to investigate the dynamics of the low-latitude (equatorial) boundary of the penetration of solar-cosmic-ray protons with an energy above 1 MeV during geomagnetic disturbances of varying intensity. The relationship between the position of this boundary and geomagnetic activity indices and solar-wind pressure is examined. It is found that the maximum relative displacement of the boundary during increases of the geomagnetic-disturbance level occurs in the afternoon and evening hours.

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