Electron acceleration in a coil target-driven low-β magnetic reconnection simulation

IF 4.8 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Matter and Radiation at Extremes Pub Date : 2023-09-13 DOI:10.1063/5.0149259
Jiacheng Yu, Jiayong Zhong, Yongli Ping, Weiming An
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Abstract

Magnetic reconnection driven by a capacitor coil target is an innovative way to investigate low-β magnetic reconnection in the laboratory, where β is the ratio of particle thermal pressure to magnetic pressure. Low-β magnetic reconnection frequently occurs in the Earth’s magnetosphere, where the plasma is characterized by β ≲ 0.01. In this paper, we analyze electron acceleration during magnetic reconnection and its effects on the electron energy spectrum via particle-in-cell simulations informed by parameters obtained from experiments. We note that magnetic reconnection starts when the current sheet is down to about three electron inertial lengths. From a quantitative comparison of the different mechanisms underlying the electron acceleration in low-β reconnection driven by coil targets, we find that the electron acceleration is dominated by the betatron mechanism, whereas the parallel electric field plays a cooling role and Fermi acceleration is negligible. The accelerated electrons produce a hardened power-law spectrum with a high-energy bump. We find that injecting electrons into the current sheet is likely to be essential for further acceleration. In addition, we perform simulations for both a double-coil co-directional magnetic field and a single-coil one to eliminate the possibility of direct acceleration of electrons beyond thermal energies by the coil current. The squeeze between the two coil currents can only accelerate electrons inefficiently before reconnection. The simulation results provide insights to guide future experimental improvements in low-β magnetic reconnection driven by capacitor coil targets.
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线圈靶驱动低β磁重联模拟中的电子加速
由电容器线圈靶驱动的磁重联是一种在实验室中研究低β磁重联的创新方法,其中β为粒子热压与磁压之比。低β磁重联经常发生在地球磁层中,其等离子体的特征为β > 0.01。在本文中,我们分析了磁重联过程中的电子加速度及其对电子能谱的影响。我们注意到,当电流片下降到大约3个电子惯性长度时,磁重联开始。通过对线圈靶驱动的低β重联中不同电子加速机制的定量比较,我们发现电子加速主要由电子加速器机制主导,而平行电场起冷却作用,费米加速度可以忽略不计。加速的电子产生了一个强化的幂律谱和一个高能量的碰撞。我们发现,向电流片注入电子可能是进一步加速的必要条件。此外,我们对双线圈共向磁场和单线圈共向磁场进行了模拟,以消除线圈电流直接加速电子超越热能的可能性。在重新连接之前,两个线圈电流之间的挤压只能无效地加速电子。仿真结果为指导电容器线圈靶驱动的低β磁重联的实验改进提供了指导。
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来源期刊
Matter and Radiation at Extremes
Matter and Radiation at Extremes Physics and Astronomy-Atomic and Molecular Physics, and Optics
CiteScore
8.60
自引率
9.80%
发文量
160
审稿时长
15 weeks
期刊介绍: Matter and Radiation at Extremes (MRE), is committed to the publication of original and impactful research and review papers that address extreme states of matter and radiation, and the associated science and technology that are employed to produce and diagnose these conditions in the laboratory. Drivers, targets and diagnostics are included along with related numerical simulation and computational methods. It aims to provide a peer-reviewed platform for the international physics community and promote worldwide dissemination of the latest and impactful research in related fields.
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