Enablement or Suppression of Collisionless Magnetic Reconnection by the Background Plasma Beta and Guide Field

How magnetic reconnection is triggered or suppressed is an important outstanding problem. By considering pinching of a current sheet that has formed at non-equilibrium, we show that the background plasma beta is a major controlling factor in the onset and nature of magnetic reconnection. A high plasma beta inhibits a current sheet from pinching down to kinetic scales required for collisionless reconnection, while a low beta facilitates it. A simple adiabatic model provides a good prediction for the reconnection-enabled regions in thickness versus peak plasma beta space, which are confirmed by a series of particle-in-cell simulations with varying initial parameters. A strong dependency of the peak reconnection rate on the plasma beta is clearly predicted with reconnection being favored in low beta conditions. A finite guide field is an additional source of reconnection suppression, consistent with previous observations that reconnection requires a large enough magnetic shear angle for high-beta situations.

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Publication Details

Journal
Geophysical Research Letters
Published
2024-11-21
DOI
https://doi.org/10.1029/2024gl112126
Citations
5
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
1.66

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article

Enablement or Suppression of Collisionless Magnetic Reconnection by the Background Plasma Beta and Guide Field

G.S. Yun, Modhuchandra Laishram, Young Dae Yoon, D. E. Wendel et al.
5 citations
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
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article

Enablement or Suppression of Collisionless Magnetic Reconnection by the Background Plasma Beta and Guide Field

G.S. Yun, Modhuchandra Laishram, Young Dae Yoon, D. E. Wendel, T. E. Moore
article en
5 citations

Abstract

How magnetic reconnection is triggered or suppressed is an important outstanding problem. By considering pinching of a current sheet that has formed at non-equilibrium, we show that the background plasma beta is a major controlling factor in the onset and nature of magnetic reconnection. A high plasma beta inhibits a current sheet from pinching down to kinetic scales required for collisionless reconnection, while a low beta facilitates it. A simple adiabatic model provides a good prediction for the reconnection-enabled regions in thickness versus peak plasma beta space, which are confirmed by a series of particle-in-cell simulations with varying initial parameters. A strong dependency of the peak reconnection rate on the plasma beta is clearly predicted with reconnection being favored in low beta conditions. A finite guide field is an additional source of reconnection suppression, consistent with previous observations that reconnection requires a large enough magnetic shear angle for high-beta situations.

Geophysical Research LettersVol. 51(22)
Pohang University of Science and Technology (KR), Goddard Space Flight Center (US), Asia Pacific Center for Theoretical Physics (KR)
National Aeronautics and Space Administration, National Research Foundation of Korea
Openalex Percentile: Top 16%
Ionosphere and magnetosphere dynamics
1.66
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