The Evolution of Collisionless Magnetic Reconnection from Electron Scales to Ion Scales

Author:

Liu Dongkuan,Huang KaiORCID,Lu QuanmingORCID,Lu SanORCID,Wang RongshengORCID,Ding Weixing,Wang Shui

Abstract

Abstract It is generally accepted that collisionless magnetic reconnection is initiated on electron scales, which is mediated by electron kinetics. In this paper, by performing a two-dimensional particle-in-cell simulation, we investigate the transition of collisionless magnetic reconnection from electron scales to ion scales in a Harris current sheet with and without a guide field. The results show that after magnetic reconnection is triggered on electron scales, the electrons are first accelerated by the reconnection electric field around the X line, and then leave away along the outflow direction. In the Harris current sheet without a guide field, the electron outflow is symmetric and directed away from the X line along the center of the current sheet, while the existence of a guide field will distort the symmetry of the electron outflow. In both cases, the high-speed electron outflow is decelerated due to the existence of the magnetic field B z , then leading to the pileup of B z . With the increase of B z , the ions are accelerated by the Lorentz force in the outflow direction, and an ion outflow at about one Alfvén speed is at last formed. In this way, collisionless magnetic reconnection is transferred from the electron scales to the ion scales.

Funder

Key Research Program of Frontier Sciences CAS

Strategic Priority Research Program of Chinese Academy of Sciences

National Science Foundation of China

Fundamental Research Funds for the Central Universities

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

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4. Collisionless magnetic reconnection in the magnetosphere;Chinese Physics B;2022-08-01

5. Magnetospheric Physics in China: 2020–2021;Chinese Journal of Space Science;2022

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