Dynamic Mode Transitions and Intermittent Features of Magnetic Reconnection at the Magnetopause: MMS Observation

Abstract By analyzing continuous Magnetospheric Multiscale observations at the magnetopause boundary layer, combining both magnetohydrodynamic and kinetic signatures, we have successfully captured dynamic magnetic reconnection processes in exceptional detail. Our results demonstrate that magnetic reconnection exhibits rapid transitions between distinct operational modes, characterized by: (a) primary single X‐line reconnection punctuated by intermittent secondary reconnection, leading to large‐scale multiple X‐line formations; (b) stable single X‐line reconnection with oscillating X‐line positions; (c) rapid switching of reconnection X‐lines between opposite sides of the spacecraft; and (d) transient suppression occurring during otherwise steady reconnection periods. These observations provide definitive evidence for the inherently dynamic and intermittent behavior of magnetopause reconnection, revealing its capacity for swift configuration changes under varying conditions.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-10-13
DOI
https://doi.org/10.1029/2025gl117887
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.00

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article

Dynamic Mode Transitions and Intermittent Features of Magnetic Reconnection at the Magnetopause: MMS Observation

Gongqin Liu, Tieyan Wang, Jiang Liu, M. W. Dunlop et al.
Geophysical Research Letters
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article

Dynamic Mode Transitions and Intermittent Features of Magnetic Reconnection at the Magnetopause: MMS Observation

Gongqin Liu, Tieyan Wang, Jiang Liu, M. W. Dunlop, Jinsong Zhao, Tianmei Yang, Jinbin Cao, Xiangcheng Dong, K. J. Trattner, Erfeng Zhao, Xiang Li, Xiu Sun, X.‐K. Wang
article en

Abstract

Abstract By analyzing continuous Magnetospheric Multiscale observations at the magnetopause boundary layer, combining both magnetohydrodynamic and kinetic signatures, we have successfully captured dynamic magnetic reconnection processes in exceptional detail. Our results demonstrate that magnetic reconnection exhibits rapid transitions between distinct operational modes, characterized by: (a) primary single X‐line reconnection punctuated by intermittent secondary reconnection, leading to large‐scale multiple X‐line formations; (b) stable single X‐line reconnection with oscillating X‐line positions; (c) rapid switching of reconnection X‐lines between opposite sides of the spacecraft; and (d) transient suppression occurring during otherwise steady reconnection periods. These observations provide definitive evidence for the inherently dynamic and intermittent behavior of magnetopause reconnection, revealing its capacity for swift configuration changes under varying conditions.

Geophysical Research LettersVol. 52(20)
University of Colorado Boulder (US), Yunnan University (CN), Purple Mountain Observatory (CN), European Centre for Space Applications and Telecommunications (GB), Laboratory for Atmospheric and Space Physics (US), Beihang University (CN)
National Natural Science Foundation of China, Natural Environment Research Council
Openalex Percentile: Top 80%
Ionosphere and magnetosphere dynamics
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