Some features characterizing the intensity variations of electrons with energies of 40-500 keV in interplanetary space

Details Some features characterizing the intensity variations of electrons with energies of 40-500 keV in interplanetary space Some features characterizing the intensity variations of electrons with energies of 40-500 keV in interplanetary space

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983izssr..47.1810a&link_type=abstract

(Seminar po Solnechnoi Aktivnosti i Solnechnym Kosmicheskim Lucham, Leningrad, USSR, Nov. 1982) Akademiia Nauk SSSR, Izvestiia,

Other

Electron Energy, Interplanetary Space, Jupiter (Planet), Solar Planetary Interactions, Anisotropy, Flux (Rate), Prognoz Satellites, Solar Activity Effects, Solar Wind Velocity

Scientific paper

Mars-7 and Prognoz-3 measurements of electron fluxes with energies of
40-500 keV in interplanetary space are examined. An analysis of the
intensity, anisotropy, and variations of fluxes near leading shock
fronts, as well as a comparison with data from other spacecraft,
indicates that these electron fluxes have a Jovian origin.

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