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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 22, issue 12
Ann. Geophys., 22, 4299–4310, 2004
https://doi.org/10.5194/angeo-22-4299-2004
© Author(s) 2004. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 22, 4299–4310, 2004
https://doi.org/10.5194/angeo-22-4299-2004
© Author(s) 2004. This work is distributed under
the Creative Commons Attribution 3.0 License.

  22 Dec 2004

22 Dec 2004

Two satellite study of substorm expansion near geosynchronous orbit

Ø. Holter2,1, P. Galopeau2, A. Roux2, S. Perraut2, A. Pedersen1, A. Korth3, and T. Bösinger4 Ø. Holter et al.
  • 1Department of Physics, University of Oslo, Oslo, Norway
  • 2Centre d’étude des Environnements Terrestre et Planétaires, CNRS-Université Versailles Saint-Quentin, Velizy, France
  • 3Max-Planck-Institut für Aeronomie, 37191 Katlenburg-Lindau, Germany
  • 4Department of Physics, University of Oulu, Oulu, Finland

Abstract. During several time intervals in 1979–1980 the satellites GEOS-2 and SCATHA were situated relatively close on the nightside of the Earth at geosynchronous distances. Several substorm events were identified during these periods. The event considered in this paper was recorded on 22 May 1979, when the satellites were separated by less than 30min in local time around 21:00 LT. The observed 45 to 60 s delay of magnetic signatures observed at the two s/c indicates a westward expansion of ~7.7°/min. At the two s/c, the magnetic signatures are, in particular for the azimuthal magnetic field components, quite different. At GEOS-2, being close to the magnetic equator, the dominant feature is a dipolarization with a weak field-aligned current signature corresponding to a symmetric current which cancels at the equator. On SCATHA, however, being close to the current sheet boundary, the azimuthal magnetic field indicates a strong field-aligned Birkeland current structure. On both s/c the first indication of an approaching substorm was an increase in the high energy ion flux followed by a reduction in the flux intensity of energetic electrons and a further tailward stretching of the magnetic field, starting ~2min before the onset of the magnetic field dipolarization. The tailward stretching, the observed variations of the magnetic field components, and the subsequent dipolarization are interpreted in terms of an azimuthally tilted field-aligned current system passing the s/c on the tailward side from east to west. The westward expansion and dipolarization observed at the two s/c are consistent with the propagation of a Rayleigh-Taylor type instability. The increased radial ion flux corresponds to the ExB-drift due to the substorm associated electric field.

Key words. Magnetospheric physics (storms and substorms; plasma waves and instabilities; current systems)

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