Other
Scientific paper
Jan 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cosre..30..444s&link_type=abstract
Cosmic Res., Vol. 30, No. 4, p. 444 - 452
Other
Scientific paper
Flare-associated increases in the flux of charged particles generated at various solar longitudes in 1972 - 1973 are analyzed. The measurements were carried out on the Prognoz satellites and the Mars-7 space probe. The behavior of the particle fluxes was determined by two interplanetary disturbances of the solar wind. One component of the solar wind was of flare origin, while a second was not directly associated with the flare. The latter component was observed a few hours before the flare-related disturbance arrived at the Earth's orbit. This component of the solar wind could not be linked with any solar flares. It was probably formed by coronal ejections of matter unrelated to flares. The structural features of this component of the flux, found from direct data on the solar wind and the magnetic field, are similar to structural regions in the flare-related flux. This complex structure of the interplanetary medium affected the behavior of the charged particles generated during a flare. Magnetic traps associated with these structural regions completely controlled the behavior of "soft" particles. The behavior of the "hard" particles can be described by diffusion models. The energy boundary between the soft and hard particles varies from one event to another. It is determined by the characteristics of the source and of the interplanetary medium.
Kolesov Ya. G.
Petrov V. M.
Shavrin P. I.
Shestopalov I. P.
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