Daytime high-latitude profile of solar-cosmic-ray protons with EP not less than about 1 MeV

Details Daytime high-latitude profile of solar-cosmic-ray protons with EP not less than about 1 MeV Daytime high-latitude profile of solar-cosmic-ray protons with EP not less than about 1 MeV

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983kosis..21..577i&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 21, July-Aug. 1983, p. 577-583. In Russian.

Computer Science

Sound

1

Daytime, Satellite Sounding, Solar Cosmic Rays, Solar Protons, Auroral Zones, Cosmos Satellites, Interplanetary Space, Latitude, Magnetospheric Instability

Scientific paper

Data from Cosmos 480, 900, and 1067 are used to examine the structure of the daytime high-latitude solar-cosmic-ray (SCR) protons in conditions of moderate and intense magnetic disturbance during the SCR increases of April 18, 1972 and April 3, 1979. These increases were accompanied by a significant north-south asymmetry in SCR proton intensity above the polar caps. In addition, a comparison is made between SCR proton fluxes observed in the auroral zone and in interplanetary space.

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