Properties of Near-Earth Magnetic Reconnection from In-Situ Observations

被引:66
|
作者
Fuselier, S. A. [1 ]
Lewis, W. S. [2 ]
机构
[1] Lockheed Martin Adv Technol Ctr, Palo Alto, CA USA
[2] SW Res Inst, San Antonio, TX USA
关键词
Magnetic reconnection; Magnetosphere; Magnetospheric multiscale; Plasma physics; FLUX-TRANSFER EVENTS; COLLISIONLESS RECONNECTION; DAYSIDE MAGNETOPAUSE; FIELD RECONNECTION; DIFFUSION REGION; SHEET BOUNDARY; PLASMA SHEET; SOLAR-WIND; CUSP; CLUSTER;
D O I
10.1007/s11214-011-9820-x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Many properties of magnetic reconnection have been determined from in-situ spacecraft observations in the Earth's magnetosphere. Recent studies have focused on ion scale lengths and have largely confirmed theoretical predictions. In addition, some interesting features of reconnection regions on electron scale lengths have been identified. These recent studies have demonstrated the need for combined plasma and field measurements on electron scale lengths in the reconnection diffusion regions at the magnetopause and in the magnetotail. They have also indicated that measurements, such as those that will be made by the Magnetospheric Multiscale mission in the near future, will have a significant impact on understanding magnetic reconnection as a fundamental plasma process.
引用
收藏
页码:95 / 121
页数:27
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