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SAMBO-GEOS: On three-dimensional substorm dynamics — A case study for 4 March 1979
Authors:LL Lazutin  AA Khrushchinsky  TV Kozelova  AO Melnikov  Ya Sakharov  G Kremser  WK Riedler  KM Torkar  K Glassmeier  J-P Treilhou  A Pedersen  G Gustafsson  R Pellinen  J Kangas
Institution:1. Polar Geophysical Institute, 184200 Apatity, Murmansk Region, USSR;2. Max-Planck-Institut für Aeronomie, D-3411 Katlenburg-Lindau, FRG;3. Institute for Space Research, Austrian Academy of Sciences, Inffeldgasse 12, A-8010 Graz, Austria;4. Institut für Geophysik, Universität Münster, FRG;5. Centre d''Etude Spatiale des Rayonnements, Toulouse, France;6. ESTEC, Domeinweg, Noordwijk, Netherlands;7. Uppsala Ionospheric Observatory, Uppsala, Sweden;8. Finnish Meteorological Institute, Helsinki, Finland;9. University of Oulu, Oulu, Finland
Abstract:For investigations of the isolated magnetospheric substorm the ground-based and satellite geophysical data are discussed. The active phase of the substorm has two parts: an active-convective phase and a classical active phase. The analysed data show that the breakup of the substorm takes place at closed and not very much stretched magnetic field lines.
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