Extension of the Electron Diffusion Region in a Guide Field Magnetic Reconnection at Magnetopause

被引:24
|
作者
Zhong, Z. H. [1 ]
Zhou, M. [1 ]
Tang, R. X. [1 ]
Deng, X. H. [1 ]
Khotyaintsev, Y. V. [2 ]
Giles, B. L. [3 ]
Paterson, W. R. [3 ]
Pang, Y. [1 ]
Man, H. Y. [1 ]
Russell, C. T. [4 ]
Burch, J. L. [5 ]
机构
[1] Nanchang Univ, Nanchang 330031, Jiangxi, Peoples R China
[2] Swedish Inst Space Phys, SE-75121 Uppsala, Sweden
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
[4] Univ Calif Los Angeles, Dept Earth Planetary & Space Sci, Los Angeles, CA USA
[5] Southwest Res Inst, San Antonio, TX USA
基金
中国国家自然科学基金;
关键词
DISSIPATION;
D O I
10.3847/2041-8213/ab7b7c
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The structure of the electron diffusion region (EDR) in different plasma regimes is an outstanding question related to magnetic reconnection. Here we report a long EDR that extended at least 20 ion inertial lengths downstream of an X line at the Earth's magnetopause, which was observed by the Magnetospheric Multiscale mission. This EDR was detected in the exhaust of an asymmetric magnetic reconnection with a moderate guide field, the reconnection rate of which was similar to 0.1. It corresponds to strong positive energy dissipation (J . E' > 0) and enhancement of electron nongyrotropy. The energy dissipation was contributed by the electron jet and non-ideal electric field along the outflow direction, which suggests that the EDR probably plays more important roles in the energy conversion in magnetic reconnection than previously thought. Our result could be a significant step toward fully understanding the structure of the EDR.
引用
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页数:7
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