Anisotropy and differential spectrum of energetic solar particles at 0.8 AU

Details Anisotropy and differential spectrum of energetic solar particles at 0.8 AU Anisotropy and differential spectrum of energetic solar particles at 0.8 AU

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2392m&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Computer Science

Energetic Particles, Energy Spectra, Proton Beams, Solar Spectra, Particle Beams, Wave Fronts

Scientific paper

The paper presents a comparative analysis of the temporal and spatial characteristics of the growth of charged-particle fluxes during events on Jan. 5 and 6, 1983. The temporal and spatial profiles were measured on the Venera 13 and 14 probes. It is shown that the existence of a considerable anisotropy (about 70 percent) at the growth phase is connected with particle diffusion within a quasi-trap formed by a shock wave.

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