Azimuthal plasma pressure reconstructed by using the Aureol-3 satellite data during quiet geomagnetic conditions
Abstract
The azimuthal distribution of magnetospheric plasma pressure was studied using the precipitating particle fluxes observed by the low-altitude polar-orbiting Aureol-3 satellite. The data from the 18 March 1982 event was used to calculate the pressure along the satellite trajectory during quiet geomagnetic conditions. The magnetic flux tube volumes for the field-lines, corresponding to the points of measurement at the satellite trajectory, were calculated by using Tsyganenko 96 magnetic-field model. The gradients of the plasma pressure along the isosurfaces of the volume of the magnetic flux tube per unit flux were estimated, and the field-aligned currents were calculated assuming that the condition of the magnetostatic equilibrium is valid. The results obtained were compared with the [J. Geophys. Res. 81 (13) (1976) 2165] field-aligned current distribution. © 2003 COSPAR. Published by Elsevier Ltd. All rights reseved.
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Título según WOS: | Azimuthal plasma pressure reconstructed by using the Aureol-3 satellite data during quiet geomagnetic conditions |
Título según SCOPUS: | Azimuthal plasma pressure reconstructed by using the Aureol-3 satellite data during quiet geomagnetic conditions |
Título de la Revista: | ADVANCES IN SPACE RESEARCH |
Volumen: | 33 |
Número: | 5 |
Editorial: | ELSEVIER SCI LTD |
Fecha de publicación: | 2004 |
Página de inicio: | 737 |
Página final: | 741 |
Idioma: | English |
URL: | http://linkinghub.elsevier.com/retrieve/pii/S0273117703006410 |
DOI: |
10.1016/S0273-1177(03)00641-0 |
Notas: | ISI, SCOPUS |