Computer Science – Sound
Scientific paper
Jul 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kosis..23..642v&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 23, July-Aug. 1985, p. 642-646. In Russian.
Computer Science
Sound
1
Electron Precipitation, High Energy Electrons, Magnetic Storms, Magnetospheric Instability, Outer Radiation Belt, Satellite Sounding, Cosmos Satellites, Electron Diffusion, Energy Spectra, Intercosmos Satellites
Scientific paper
The dynamics of the outer belt of high-energy electrons for various geomagnetic conditions was studied in March 1979 on the basis of spectrometer measurements on Intercosmos-19 (0.3-2 MeV) and on Cosmos-900 (0.8-1.2 MeV). A strong magnetic storm was studied during which the diffusion velocity increased under the effect of sudden impulses. This led to the development of a fast diffusion wave with a shift of the electron maxima at all energies studied toward lower L values; this wave determined the propagation of disturbances induced by the injection of storm plasma into the magnetosphere. Such waves may be a partial cause of the rapid appearance of high-energy electrons (up to several MeV) after magnetic storms.
Dronov V. A.
Kovrygina L. M.
Kratenko Iu. P.
Mineev Iu. V.
Volkov I. B.
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