Spatial-temporal features of the penetration of solar cosmic rays into high-latitude regions of the earth's magnetosphere according to data of the Intercosmos-19 satellite

Details Spatial-temporal features of the penetration of solar cosmic rays into high-latitude regions of the earth's magnetosphere according to data of the Intercosmos-19 satellite Spatial-temporal features of the penetration of solar cosmic rays into high-latitude regions of the earth's magnetosphere according to data of the Intercosmos-19 satellite

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984kosis..22..594g&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 22, July-Aug. 1984, p. 594-598. In Russian.

Computer Science

Sound

Earth Magnetosphere, Incident Radiation, Satellite Sounding, Solar Cosmic Rays, Intercosmos Satellites, Magnetic Storms, Solar Protons, Spatial Distribution, Time Response

Scientific paper

An analysis is made of intensity increases of solar-cosmic-ray (SCR) protons with energies of 0.5-8.0 MeV in the polar regions during the intense magnetic storm of April 3-5, 1979. The penetration of the protons is examined together with variations of the location of the high-latitude capture boundary of electrons with energies of 0.3-0.6 MeV, 0.6-0.9 MeV, and greater than 0.1 MeV. Fluctuations of the boundary locations of different penetration regions are disclosed along with rapid pulsations (with a period of 15-20 sec) of protons. Particle data are compared with magnetometer measurements, and the periods of proton pulsations are found to be well-correlated with the real geomagnetic field.

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