Other
Scientific paper
Mar 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976kosis..14..239v&link_type=abstract
Kosmicheskie Issledovaniia, vol. 14, Mar.-Apr. 1976, p. 239-247. In Russian.
Other
1
Anisotropy, Solar Activity Effects, Solar Cosmic Rays, Mars Probes, Satellite-Borne Instruments, Solar Flares, Solar Wind
Scientific paper
An attempt is made to find the causes for the increase in cosmic ray intensity characterized by a unique phenomenon where the proton and electron fluxes toward the sun exceeded the particle fluxes coming from the sun. This event, recorded in September 1973 by the Mars 4, 5, and 7 spacecraft, is attributed to a favorable combination of such factors as the fact that the solar flares at that time were located on one side and the satellites on the other side of the plane of the solar equator; that the inclination of the solar axis was maximal (7 degrees), while the first and subsequent flares occurred in the southern solar hemisphere, so that the dense equatorial solar plasma layer was traversed by the cosmic ray flux. Other factors were the specific characteristics of the given phase of the 20th cycle of solar activity and the nature of the injection and diffuse-convective propagation of the cosmic rays.
Chuchkov E. A.
Gorchakov E. V.
Ignat'ev P. P.
Kontor N. N.
Liubimov G. P.
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