Plasma convection in the Earth's magnetosphere and ionosphere during substorms

被引:0
作者
Foerster, M. [1 ]
Mishin, V. M. [2 ]
Stauning, P. [3 ]
Watermann, J. [3 ]
Saifudinova, T. I. [2 ]
Bazarzhapov, A. D. [2 ]
机构
[1] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[2] Russian Acad Sci, Inst Solar Terr Phys, Irkutsk 664033, Russia
[3] Danish Metrol Inst, DK-2100 Copenhagen, Denmark
基金
美国国家科学基金会;
关键词
convection; field-aligned currents; substorms; M-I coupling;
D O I
暂无
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The empirical field-aligned current (FAC) and plasma convection model on which this paper is based describes the four phases of a typical substorm. 2D maps of the ionospheric electric potential (0 are shown here for the first time for each of these phases. The principal result is the identification of medium-scale ionospheric convection vortices, which are observed in addition to the well-known two large-scale DP2 convection cells. We conclude that these convection vortices are the analogue to the heterogeneities that were found earlier in the spatial distribution of the FAC density. They had been taken into account there in the framework of the conceptual model of magnetospheric generators. This model is extended in the present paper such that it also describes the above-mentioned medium-scale convection vortices. (C) 2006 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:1750 / 1754
页数:5
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