The propagation of solar cosmic rays in the presence of complex structures in the interplanetary magnetic field

Details The propagation of solar cosmic rays in the presence of complex structures in the interplanetary magnetic field The propagation of solar cosmic rays in the presence of complex structures in the interplanetary magnetic field

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ge%26ae..28..830k&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 28, Sept.-Oct. 1988, p. 830-832. In Russian.

Computer Science

Interplanetary Magnetic Fields, Kinetic Equations, Particle Acceleration, Solar Cosmic Rays, Solar Protons, Lines Of Force, Magnetic Mirrors

Scientific paper

The propagation of solar-cosmic-rays (SCR) protons in the event of August 1, 1967 observed by Venera-4 is investigated on the basis of a numerical solution of the SCR propagation equation. It is shown that the behavior of the SCRs can be explained most completely if the presence of loops or magnetic mirror structures is assumed in the interplanetary magnetic field.

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