How can we solve the problem of substorms? (A review)

被引:7
|
作者
Ponomarev, E. A. [1 ]
Sedykh, P. A. [1 ]
机构
[1] Russian Acad Sci, Siberian Div, Inst Solar Terr Phys, Irkutsk 664033, Russia
基金
俄罗斯基础研究基金会;
关键词
D O I
10.1134/S0016793206040177
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The works in the alternative direction of magnetospheric studies are reviewed. In contrast to the traditional approach, where the basis process is magnetic field line reconnection, transformation of kinetic energy into electromagnetic one at the bow shock front is the basis process in the proposed approach. It has been indicated that this new paradigm makes it possible to overcome the main difficulties that remained within the scope of the previous paradigm. It has been briefly demonstrated how several following processes and phenomena are explained within the scope of the new approach: (1) transformation of the solar wind kinetic energy into the electromagnetic energy; (2) electromagnetic energy transfer into the magnetosphere; (3) organization of the system of bulk currents, formation of field- aligned currents from the magnetosphere, and compatibility of these currents with the ionospheric current systems; (4) shape, value, and dynamics of the particle precipitation auroral regions; and (5) substorm expansion (auroral breakup). Other possibilities of the new approach and paradigm replacement consequences are briefly considered.
引用
收藏
页码:530 / 544
页数:15
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