About The Origin Of High Energy Electrons In The Inner Radiation Belt

A large flux of &gt; 100 MeV electrons were registered in the inner radiation belt on low-altitude satellites. The origin of that flux is discussed. It appears that slow radial diffusion (Do = 10-13 1/s) gives a low probability for penetration of these electrons to small L from the boundary of magnetosphere because of synchrotron radiation energy losses. It is found that they can enter to the inner belt region without such losses after great magnetic storms when high speed radial diffusion sometimes takes place. Two great storms on 8-9 Feb.] 986 and 24 March 1991 are examples when one can directly observe a penetration of energetic electron fluxes into magnetosphere. The assumption about their Jovian origin is discussed. © 1994.572201204Baker, Blake, Highly relativistic electrons in the Earth's outer magnetosphere: 1. Lifetimes and temporal history 1979–1984 (1986) Journal of Geophysical Research, 91 (4 A), p. 4265Baker, Higbie, Do Jovian electrons influence the terrestrial outer radiation zone? (1979) Geophysical Research Letters, 6, p. 531Blake, Kolasinski, Injection of electrons and protons with energies of tens of MeV into L < 3 on 24 March 1991 (1992) Geophysical Research Letters, 19, p. 821Dmitrenko, Komarov, Tverskoy, (1987) Geom. i Aeronom., 27, p. 488Galper, Dmitrenko, (1981) Kosmich. Issled., 19, p. 645Ginzburg, Malishev, Pustovetov, (1992) Proc. Cosm. Ray Conf., Uzbekistan, Samarcand, 1, p. 230Gusev, Pugacheva, (1983) J. geophys., 52, p. 247Gusev, Pugacheva, (1984) Planet. Space Sci., 32, p. 29Gusev, Pugacheva, (1991) Izv. AN SSSR, ser. phys., 53, p. 22000Tverskaja, (1986) Geom. i Aeronom., 26, p. 5864Voronov, Galper, (1986) Pisma v JETF, 43, p. 24