利用磁层多尺度任务识别2015年9月19日重联事件的磁零

S. Ekawati, D. Cai
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引用次数: 0

摘要

磁零区是指磁场消失的区域,在磁重联过程中的能量转换和粒子加速中起着至关重要的作用。此外,它们也是表征复杂磁拓扑结构的有用工具,在三维(3D)磁重联中是必不可少的。本文利用磁层多尺度(MMS)任务航天器,应用线性插值方法推导了2015年9月19日日侧重联电子扩散区(EDR)的零位置。特征值实部的符号数决定了该零附近的磁场拓扑结构。拓扑结构的变化可能与分岔或磁重联的发生有关。在这里,我们报告了第一次原位测量,在07:43:30.4左右,与报告的EDR事件相关的磁null的场拓扑从B型变为A型。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Identification of Magnetic Null on Reconnection 19 September 2015 Event using Magnetospheric Multiscale Mission
Magnetic nulls referred to a region with vanishing magnetic fields play an essential role in energy conversion and particle acceleration during magnetic reconnections. Moreover, they are also useful tools to characterize the complex magnetic topologies and are essential in three-dimensional (3D) magnetic reconnection. In this paper, we apply the linear interpolation methods to derive the null positions of the dayside reconnection Electron Diffusion Region (EDR) on 19 September 2015 using Magnetospheric Multiscale (MMS) mission spacecraft. The number of the signs of the real part of eigenvalues determines the magnetic field topology nearby this null. The change of the topology can be related to the occurrence of bifurcation or magnetic reconnection. Here, we report the first in situ measurement that the field topology of magnetic nulls changes from B type to A type at around 07:43:30.4 associated with the reported EDR event.
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