High-energy electrons in the outer radiation belt during magnetic storms

Details High-energy electrons in the outer radiation belt during magnetic storms High-energy electrons in the outer radiation belt during magnetic storms

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2231g&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Computer Science

High Energy Electrons, Magnetic Storms, Outer Radiation Belt, Cerenkov Counters, Cosmos Satellites, Time Lag

Scientific paper

An analysis is made of Cosmos-900 Cerenkov-counter data on fluxes of outer-radiation-belt electrons with energies of 15-30 MeV for the period March 30, 1977 to October 10, 1979. The dependence of the electron delay time on the maximum Dst amplitude is analyzed. It is shown that the generation of high-energy electrons in the outer belt is evidently delayed by several days as compared with the generation of electrons of lower energies.

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