Peculiarities of propagation of charged particles in solar corona

Details Peculiarities of propagation of charged particles in solar corona Peculiarities of propagation of charged particles in solar corona

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..313m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 313-316 (SEE N85-34729 23-92)

Physics

Solar Corona, Solar Flares, Solar Flux Density, Solar Magnetic Field, Electromagnetic Wave Transmission, Interplanetary Space, Prognoz Satellites, Solar Wind, Venera 11 Satellite

Scientific paper

The influence of boundaries of the large scale unipolar magnetic regions (UMR) on the Sun upon the charged particle propagation in the solar corona and interplanetary space is investigated. Increases of the charged particle fluxes from solar flares on November 4 and 20, 1978 detected by Venera-11 and Prognoz-1 and on December 7, 1982 by Venera-13 and "GMS-2" were analyzed.

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