Electron scale coherent structure as micro accelerator in the Earth’s magnetosheath

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作者
Zi-Kang Xie
Qiu-Gang Zong
Chao Yue
Xu-Zhi Zhou
Zhi-Yang Liu
Jian-Sen He
Yi-Xin Hao
Chung-Sang Ng
Hui Zhang
Shu-Tao Yao
Craig Pollock
Guan Le
Robert Ergun
Per-Arne Lindqvist
机构
[1] Peking University,Institute of Space Physics and Applied Technology
[2] Macau University of Science and Technology,State Key Laboratory of Lunar and Planetary Sciences
[3] Max Planck Institute for Solar System Research,Geophysical Institute
[4] University of Alaska Fairbanks,Shandong Provincial Key Laboratory of Optical Astronomy and Solar
[5] Shandong University,Terrestrial Environment, Institute of Space Sciences
[6] Denali Scientific,Department of Astrophysical and Planetary Sciences
[7] Heliophysics Science Division,Department of Space and Plasma Physics
[8] NASA,undefined
[9] Goddard Space Flight Center,undefined
[10] University of Colorado LASP,undefined
[11] KTH Royal Institute of Technology,undefined
来源
Nature Communications | / 15卷
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摘要
Turbulent energy dissipation is a fundamental process in plasma physics that has not been settled. It is generally believed that the turbulent energy is dissipated at electron scales leading to electron energization in magnetized plasmas. Here, we propose a micro accelerator which could transform electrons from isotropic distribution to trapped, and then to stream (Strahl) distribution. From the MMS observations of an electron-scale coherent structure in the dayside magnetosheath, we identify an electron flux enhancement region in this structure collocated with an increase of magnetic field strength, which is also closely associated with a non-zero parallel electric field. We propose a trapping model considering a field-aligned electric potential together with the mirror force. The results are consistent with the observed electron fluxes from ~50 eV to ~200 eV. It further demonstrates that bidirectional electron jets can be formed by the hourglass-like magnetic configuration of the structure.
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