Kinetic-scale Topological Structures Associated with Energy Dissipation in the Turbulent Reconnection Outflow

被引:6
|
作者
Huang, S. Y. [1 ]
Zhang, J. [1 ]
Xiong, Q. Y. [1 ]
Yuan, Z. G. [1 ]
Jiang, K. [1 ]
Xu, S. B. [1 ]
Wei, Y. Y. [1 ]
Lin, R. T. [1 ]
Yu, L. [1 ]
Wang, Z. [1 ]
机构
[1] Wuhan Univ, Sch Elect Informat, Hubei Luojia Lab, Wuhan 430072, Peoples R China
来源
ASTROPHYSICAL JOURNAL | 2023年 / 958卷 / 02期
基金
中国国家自然科学基金;
关键词
VELOCITY-GRADIENT TENSOR; MAGNETIC RECONNECTION; SOLAR-WIND; INTERMITTENT DISSIPATION; SECONDARY RECONNECTION; FLUX ROPES; WAVES; INVARIANTS; STATISTICS; DYNAMICS;
D O I
10.3847/1538-4357/acf847
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Assisted by the Magnetospheric Multiscale mission capturing unprecedented high-resolution data in the terrestrial magnetotail, we apply a local streamline-topology classification methodology to investigate the categorization of the magnetic field topological structures at kinetic scales in the turbulent reconnection outflow. It is found that strong correlations exist between the straining and rotational part of the velocity gradient tensor as well as the magnetic field gradient tensor. Strong energy dissipation prefers to occur at regions with high magnetic stress or current density, which is contributed mainly by O-type topologies. These results indicate that the kinetic structures with O-type topology play a more important role in energy dissipation in turbulent reconnection outflow.
引用
收藏
页数:8
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