The features of solar proton propagation in interplanetary space

Details The features of solar proton propagation in interplanetary space The features of solar proton propagation in interplanetary space

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4..153e&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 4 (A85-2

Computer Science

Forbush Decreases, Interplanetary Space, Proton Precipitation, Satellite Observation, Solar Protons, Venera 11 Satellite, Cosmic Rays, Galactic Radiation, Particle Motion, Solar Activity Effects

Scientific paper

In the course of its flight the Venera-11 space probe, launched in September, 1978, gradually deviates westward from the sun-earth line and explores the interplanetary space regions farther and farther from the earth. It is of interest, therefore, to compare the Venera-11 data with the IMP-8 data. Such an analysis was made by Ermakov et al. (1981) for April, 1979. Here the period of July-August, 1979, is examined when Venera-11 moved in azimuthal direction from 45 to 50 deg relative to the sun-earth line and in radial direction from 1 AU in July to 0.85 AU in August.

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