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三维激波湍流中的电子尺度重联

Electron-Scale Reconnection in Three-Dimensional Shock Turbulence.

作者信息

Ng J, Chen L-J, Bessho N, Shuster J, Burkholder B, Yoo J

机构信息

Department of Astronomy University of Maryland College Park MD USA.

NASA Goddard Space Flight Center Greenbelt MD USA.

出版信息

Geophys Res Lett. 2022 Aug 16;49(15):e2022GL099544. doi: 10.1029/2022GL099544. Epub 2022 Aug 15.

DOI:10.1029/2022GL099544
PMID:36247516
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC9539853/
Abstract

Magnetic reconnection has been observed in the transition region of quasi-parallel shocks. In this work, the particle-in-cell method is used to simulate three-dimensional reconnection in a quasi-parallel shock. The shock transition region is turbulent, leading to the formation of reconnecting current sheets with various orientations. Two reconnection sites with weak and strong guide fields are studied, and it is shown that reconnection is fast and transient. Reconnection sites are characterized using diagnostics including electron flows and magnetic flux transport. In contrast to two-dimensional simulations, weak guide field reconnection is realized. Furthermore, the current sheets in these events form in a direction almost perpendicular to those found in two-dimensional simulations, where the reconnection geometry is constrained.

摘要

在准平行激波的过渡区域已观测到磁重联现象。在这项工作中,采用粒子模拟方法对准平行激波中的三维重联进行了模拟。激波过渡区域是湍流的,导致形成具有各种取向的重联电流片。研究了具有弱引导场和强引导场的两个重联位点,结果表明重联是快速且瞬态的。利用包括电子流和磁通量输运在内的诊断方法对重联位点进行了表征。与二维模拟不同,实现了弱引导场重联。此外,这些事件中的电流片形成方向几乎垂直于二维模拟中发现的方向,在二维模拟中重联几何结构受到限制。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a499/9539853/9969eed06325/GRL-49-e2022GL099544-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a499/9539853/d203c9c12426/GRL-49-e2022GL099544-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a499/9539853/d58bcbe05228/GRL-49-e2022GL099544-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a499/9539853/8091f3d7db5d/GRL-49-e2022GL099544-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a499/9539853/9969eed06325/GRL-49-e2022GL099544-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a499/9539853/d203c9c12426/GRL-49-e2022GL099544-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a499/9539853/d58bcbe05228/GRL-49-e2022GL099544-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a499/9539853/8091f3d7db5d/GRL-49-e2022GL099544-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a499/9539853/9969eed06325/GRL-49-e2022GL099544-g003.jpg

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本文引用的文献

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Laboratory Observations of Electron Heating and Non-Maxwellian Distributions at the Kinetic Scale during Electron-Only Magnetic Reconnection.仅电子磁重联过程中动力学尺度下电子加热和非麦克斯韦分布的实验室观测
Phys Rev Lett. 2022 Jan 14;128(2):025002. doi: 10.1103/PhysRevLett.128.025002.
2
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Phys Rev Lett. 2021 Oct 8;127(15):155101. doi: 10.1103/PhysRevLett.127.155101.
3
Magnetotail reconnection onset caused by electron kinetics with a strong external driver.
由具有强外部驱动因素的电子动力学引起的磁尾重联起始。
Nat Commun. 2020 Oct 7;11(1):5049. doi: 10.1038/s41467-020-18787-w.
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Electron magnetic reconnection without ion coupling in Earth's turbulent magnetosheath.地球湍动磁鞘中无离子耦合的电子磁重联。
Nature. 2018 May;557(7704):202-206. doi: 10.1038/s41586-018-0091-5. Epub 2018 May 9.
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Model of Hall reconnection.霍尔重联模型。
Phys Rev Lett. 2008 Nov 28;101(22):225001. doi: 10.1103/PhysRevLett.101.225001. Epub 2008 Nov 24.
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Tail reconnection triggering substorm onset.尾部重新连接引发亚暴起始。
Science. 2008 Aug 15;321(5891):931-5. doi: 10.1126/science.1160495. Epub 2008 Jul 24.