Actions for Latitude and local time dependence of precipitated low energy electrons at high latitudes

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Latitude and local time dependence of precipitated low energy electrons at high latitudes

Author
Gustafsson, G.
Published
Aug 1, 1972.
Physical Description
1 electronic document
Online Version

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Summary
Data from particle detectors on board the satellite OGO-4 were used to study the precipitation of electrons in the energy range 0.7 to 24 keV. The latitude dependence of these particles in the local time region from midnight to dawn was investigated in detail. The analysis shows that the precipitation of particles of energies 2.3 to 24 keV is centered at an invariant latitude of about 68 deg at midnight with a clear shift in latitude with increasing local time and this shift is more pronounced for lower energies. The highest fluxes of particles in this energy interval are measured at midnight and they decrease rapidly with local time. The data in the energy range 2.3 to 24 keV support a theory where particles are injected in the midnight region from the tail gaining energy due to a betatron process and then drift eastwards in a combined electric and magnetic field. The main part of the electrons at 0.7 keV show a different behavior. They seem to undergo an acceleration process which is rather local, sometimes giving field aligned fluxes which may be super-imposed on the background precipitation.
Other Subject(s)
Collection
NASA Technical Reports Server (NTRS) Collection.
Note
Document ID: 19720025133.
Accession ID: 72N32783.
NASA-TM-X-66035.
X-645-72-293.
Terms of Use and Reproduction
No Copyright.
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