Articles | Volume 23, issue 6
https://doi.org/10.5194/angeo-23-2171-2005
https://doi.org/10.5194/angeo-23-2171-2005
15 Sep 2005
 | 15 Sep 2005

Creation of the substorm current wedge through the perturbation of the directly driven current system: a new model for substorm expansion

G. Rostoker and E. Friedrich

Abstract. The past four decades have seen a considerable amount of research on the study of magnetospheric substorms, and over most of these years the expansive phase of the substorm has been associated with the development of a three dimensional current system that has been termed the substorm current wedge. This current system has been thought to be a consequence of the short-circuiting of crosstail current through the ionosphere, and is viewed as a distinctive current system operating independently from the directly driven current with which it co-exists. The purpose of this paper is to show that the substorm current wedge should be viewed as an equivalent current system rather than a real current system. It will be shown that the magnetic perturbation pattern associated with the current wedge can be modeled as purely a perturbation of the directly driven current system in the midnight sector.

Keywords. Magnetospheric physics (Auroral phenomena; Current systems; Magnetotail; Storms and substorms