Observation of a Sharp Negative Dipolarization Front in the Reconnection Outflow Region

被引:24
作者
Zhou Meng [1 ,2 ,4 ]
Huang Shi-Yong [3 ]
Deng Xiao-Hua [1 ,3 ]
Pang Ye [1 ,4 ]
机构
[1] Nanchang Univ, Inst Space Sci & Technol, Nanchang 330031, Peoples R China
[2] Chinese Acad Sci, Sate Key Lab Space Weather, Beijing 100190, Peoples R China
[3] Wuhan Univ, Sch Elect & Informat, Wuhan 430072, Peoples R China
[4] Nanchang Univ, Inst Astron, Nanchang 330031, Peoples R China
基金
中国国家自然科学基金;
关键词
HIGH-SPEED FLOWS; EARTHS MAGNETOSPHERE; PLASMA SHEET; CLUSTER; FIELD;
D O I
10.1088/0256-307X/28/10/109402
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
A sharp dipolarization front (DF) has recently been detected in the Earth's magnetotail and is associated with complex kinetic effects. We present one event where a tailward propagating negative DF (with B-z decreasing sharply to negative value) was observed near a reconnection region. The thickness of the negative DF is comparable with the local ion gyro-radius/inertial length. There is a strong field-aligned current at the front. Electromagnetic whistler wave enhancements are observed around the front, associated with counter-streaming electron beams. We further compare the features of the observed negative DF with the recent kinetic simulation results, as well as the Earthward propagating DFs observed by the THEMIS spacecraft.
引用
收藏
页数:4
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