The structure and dynamics of a large-scale plasmoid generated by fast reconnection in the geomagnetic tail

被引:5
|
作者
Ugai, M. [1 ]
机构
[1] Ehime Univ, Res Ctr Space & Cosm Evolut, Matsuyama, Ehime 7908577, Japan
关键词
Magnetospheric physics; Magnetotail; Storms and substorms; TRAVELING COMPRESSION REGIONS; EARTHS MAGNETOTAIL; GEOTAIL OBSERVATIONS; CURRENT SHEET; FIELD; SUBSTORMS; MECHANISM; EVOLUTION; COMPUTER; MODEL;
D O I
10.5194/angeo-29-147-2011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
As a sequence of Ugai (2010b), the present paper studies in detail the structure and dynamics of large-scale (principal) plasmoid, generated by the fast reconnection evolution in a sheared current sheet with no initial northward field component. The overall plasmoid domain is divided into the plasmoid reconnection region P and the plasmoid core region C. In the region P, the magnetized plasma with reconnected field lines are accumulated, whereas in the region C, the plasma, which was intially embedded in the current sheet and has been ejected away by the reconnection jet, is compressed and accumulated. In the presence of the sheared magnetic field in the east-west direction in the current sheet, the upper and lower parts of the reconnection region P are inversely shifted in the east-west directions. Accordingly, the plasmoid core region C with the accumulated sheared field lines is bent in the north-south direction just ahead of the plasmoid center x = X-C, causing the magnetic field component in the north-south direction, whose sign is always opposite to that of the reconnected field lines. Therefore, independently of the sign of the initial sheared field, the magnetic field component B-z in the north-south direction has the definite bipolar profile around X-C along the x-axis. At x = X-C, the sheared field component has the peak value, and as the sheared fields accumulated in the region C become larger, the bipolar field profile becomes more distinct.
引用
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页码:147 / 156
页数:10
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