AbstractWe present typical examplesof Prognoz-10 ion (E>15 keV) and electron (E> keV) flux observations as the spacecraft crosses the low and mid-latitude magnetosheath and the foreshock. Both leakage from magnetosphere and bow shock acceleration contribute to magnetosheath populations. A statistical survey using 6 months of measurements reveals that the occurence of high ion and electron fluxes depends upon Kp. For the same Kp, the probability of high ion occurence is much higher in the magnetosheath than in the upstream region. In the upstream region, the occurence of high ion fluxes depends upon the distance to the bow shock and on the angle ΘBn.
Medium energy particle perspective from magnetopause to upstream region: Prognoz-10 data
Advances in Space Research ; 14 , 7 ; 39-42
1994-01-01
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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