Quite time convection electric field properties derived from keV electron measurements at the inner edge of the plasma sheet by means of GEOS 2
Creators
- 1. Toulouse-3 Univ., 31 (France)
- 2. Max-Planck-Institut fuer Aeronomie, Katlenburg-Lindau (Germany, F.R.)
- 3. Danish Space Research Inst., Lyngby
Description
From an analysis of the local time distribution of the electron upper energy limit reached by the geostationary satellite GEOS 2 in cutting through the innermost part of the electron plasma sheet during fairly quite condition the following results have been obtained, among others: An electric field model given by E = -grad(AR4 sinphi), with the dusk singular point of the forbidden region boundary at 1500, instead of at 1800 MLT, is in quite good agreement with the observations. This means that effects due to the shielding by the hot plasma of the inner magnetosphere from the convection electric field are quite strong in situations of low disturbance level. The quiet time convection electric field strength at 2100 MLT in the geostationary orbit obtained from this analysis varies in the range 0.15 - 0.3 keV/Rsub(e). Six hours earlier or later in the satellite orbit the convection field is 4 times stronger. Also when the convection field varies, some information about its magnitude can be obtained from the keV electron measurements. (author)
Availability note (English)
MF available from INIS under the Report Number.Files
12624648.pdf
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Additional details
Publishing Information
- Imprint Pagination
- 54 p.
- Report number
- KGI--052
INIS
- Country of Publication
- Sweden
- Country of Input or Organization
- Sweden
- INIS RN
- 12624648
- Subject category
- S58: GEOSCIENCES;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- EARTH MAGNETOSPHERE; ELECTRIC FIELDS; ELECTRON SPECTRA; ELECTRONS; EXPERIMENTAL DATA; GEOS SATELLITES; KEV RANGE; PLASMA SHEET
- Descriptors DEC
- DATA; EARTH ATMOSPHERE; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; INFORMATION; LEPTONS; NUMERICAL DATA; SATELLITES; SPECTRA