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.
SAMBO-GEOS: On three-dimensional substorm dynamics — A case study for 4 March 1979
Advances in Space Research ; 5 , 4 ; 171-174
01.01.1985
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch