Topological analysis of three-dimensional magnetic reconnection in SPERF-AREX for simulated magnetopause events

Author:

He Xianglei1ORCID,Mao Aohua123ORCID,Apatenkov Sergey4ORCID,Wang Zhibin5ORCID,Sun Mengmeng1,Zou Jitong1ORCID,Wang Xiaogang123ORCID

Affiliation:

1. School of Physics, Harbin Institute of Technology 1 , Harbin 150001, China

2. Laboratory for Space Environment and Physical Sciences, Harbin Institute of Technology 2 , Harbin 150001, China

3. China-Russia Belt and Road Joint Laboratory on Advanced Energy and Power Technology, Harbin Institute of Technology 3 , Harbin 150001, China

4. Department of Earth's Physics, St. Petersburg State University 4 , St. Petersburg 198504, Russia

5. Sino-French Institute of Nuclear Engineering and Technology, Sun Yat-sen University 5 , Zhuhai 519082, China

Abstract

A scientific research device for geospace physics, the Space Plasma Environment Research Facility (SPERF), is going to be in operation this year at the Harbin Institute of Technology, China. One of its laboratory simulation platforms, the Asymmetric Reconnection EXperiment (AREX), is designed to investigate the asymmetric magnetic reconnection relevant to the process in the dayside magnetopause of the Earth. As a ground-based experimental platform, AREX emphasizes three-dimensional (3D) asymmetric driving features with topological similarity relevant to dayside reconnection. Thus, in this paper, we focus on topological analysis based on numerical simulation of AREX reconnection processes. 3D topological features in various scenarios relevant to magnetopause reconnection in different interplanetary magnetic field (IMF) conditions are investigated by adjusting setup parameters of plasma sources and magnetic coils. The simulation results reveal that the plasma distribution of asymmetric reconnection in SPERF-AREX is analogous to that at the magnetopause. Various types of the 3D magnetic topology relevant to typical IMF conditions, including the X-line and the A–B null chain structures, are, respectively, identified and analyzed in detail.

Funder

National Natural Science Foundation of China

National Magnetic Confinement Fusion Energy R&D Program of China

Heilongjiang Touyan Innovation Team Program

China-Russia Belt and Road Joint Laboratory on Advanced Energy and Power Technology

Heilongjiang Provincial International Innovation Research Center for Plasma Physics and Applications

Publisher

AIP Publishing

Subject

Condensed Matter Physics

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