Hot plasma pressure variations on the geostationary orbit on the base of Gorizont satellite data

Plasma and energetic particles pressure distribution is studied using data from the plasma and energetic particle experiment (0.1 – 133 keV) onboard the Gorizont-35 geostationary satellite for the period from 11 to 25 March 1992. The analysed period consists of relatively quiet time, small geomagnet...

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Veröffentlicht in:Physics and chemistry of the earth. Part C, Solar-terrestrial and planetary science Solar-terrestrial and planetary science, 2000, Vol.25 (1-2), p.55-58
Hauptverfasser: Riazantseva, M.O, Sosnovets, E.N, Teltsov, M.V, Vlasova, N.A
Format: Artikel
Sprache:eng
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Zusammenfassung:Plasma and energetic particles pressure distribution is studied using data from the plasma and energetic particle experiment (0.1 – 133 keV) onboard the Gorizont-35 geostationary satellite for the period from 11 to 25 March 1992. The analysed period consists of relatively quiet time, small geomagnetic storms, SC and the time of the northern orientation of the IMF. The calculations show that the basic contribution to the total particle pressure was made by ions at the energy from 0.1 to 12.4 keV. The derived average value of the calculated pressure (∼1 nPa) points to the important role of the geostationary orbit plasma population in the formation of the magnetosphere pressure balance and of the near-Earth magnetic field distortion.
ISSN:1464-1917
DOI:10.1016/S1464-1917(99)00036-7