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不对称磁重联X线的取向与稳定性

Orientation and Stability of Asymmetric Magnetic Reconnection X Line.

作者信息

Liu Yi-Hsin, Hesse M, Li T C, Kuznetsova M, Le A

机构信息

Department of Physics and Astronomy, Dartmouth College, Hanover, NH, USA.

Department of Physics and Technology, University of Bergen, Bergen, Norway.

出版信息

J Geophys Res Space Phys. 2018 Jun;123(6):4908-4920. doi: 10.1029/2018JA025410. Epub 2018 May 31.

DOI:10.1029/2018JA025410
PMID:30364510
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6196328/
Abstract

The orientation and stability of the reconnection x line in asymmetric geometry is studied using three-dimensional (3-D) particle-in-cell simulations. We initiate reconnection at the center of a large simulation domain to minimize the boundary effect. The resulting x line has sufficient freedom to develop along an optimal orientation, and it remains laminar. Companion 2-D simulations indicate that this x line orientation maximizes the reconnection rate. The divergence of the nongyrotropic pressure tensor breaks the frozen-in condition, consistent with its 2-D counterpart. We then design 3-D simulations with one dimension being short to fix the x line orientation but long enough to allow the growth of the fastest growing oblique tearing modes. This numerical experiment suggests that reconnection tends to radiate secondary oblique tearing modes if it is externally (globally) forced to proceed along an orientation not favored by the local physics. The development of oblique structure easily leads to turbulence inside small periodic systems.

摘要

利用三维粒子模拟研究了不对称几何结构中重联x线的取向和稳定性。我们在一个大模拟域的中心引发重联,以尽量减少边界效应。由此产生的x线有足够的自由度沿最优取向发展,并且保持层流状态。伴随的二维模拟表明,这种x线取向使重联率最大化。非旋转变压力张量的散度打破了冻结条件,这与其二维对应情况一致。然后,我们设计一维较短的三维模拟来固定x线取向,但长度要足够长,以允许最快增长的斜向撕裂模增长。这个数值实验表明,如果重联在外部(全局)被迫沿着局部物理不支持的取向进行,那么它倾向于辐射出二次斜向撕裂模。在小周期系统中,斜向结构的发展很容易导致湍流。

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本文引用的文献

1
On the Collisionless Asymmetric Magnetic Reconnection Rate.关于无碰撞非对称磁重联率
Geophys Res Lett. 2018 Apr 28;45(8):3311-3318. doi: 10.1002/2017GL076460. Epub 2018 Mar 6.
2
Electron Crescent Distributions as a Manifestation of Diamagnetic Drift in an Electron-Scale Current Sheet: Magnetospheric Multiscale Observations Using New 7.5 ms Fast Plasma Investigation Moments.电子月牙分布作为电子尺度电流片中抗磁漂移的一种表现:利用新的7.5毫秒快速等离子体探测矩进行的磁层多尺度观测
Geophys Res Lett. 2018 Jan 28;45(2):578-584. doi: 10.1002/2017GL076260. Epub 2018 Jan 30.
3
Why does Steady-State Magnetic Reconnection have a Maximum Local Rate of Order 0.1?为什么稳态磁重联的最大局部速率约为0.1 ?
Phys Rev Lett. 2017 Feb 24;118(8):085101. doi: 10.1103/PhysRevLett.118.085101. Epub 2017 Feb 21.
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Magnetospheric Multiscale Satellites Observations of Parallel Electric Fields Associated with Magnetic Reconnection.磁层多尺度卫星对与磁重联相关的平行电场的观测。
Phys Rev Lett. 2016 Jun 10;116(23):235102. doi: 10.1103/PhysRevLett.116.235102.
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Science. 2016 Jun 3;352(6290):aaf2939. doi: 10.1126/science.aaf2939. Epub 2016 May 12.
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Bifurcated structure of the electron diffusion region in three-dimensional magnetic reconnection.三维磁重联中电子扩散区的分叉结构。
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7
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