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

被引:1
|
作者
Yoon, Young Dae [1 ,2 ]
Moore, Thomas Earle [3 ]
Wendel, Deirdre E. [4 ]
Laishram, Modhuchandra [1 ]
Yun, Gunsu S. [2 ,5 ]
机构
[1] Asia Pacific Ctr Theoret Phys, Pohang, South Korea
[2] Pohang Univ Sci & Technol, Dept Phys, Pohang, South Korea
[3] 3rd Rock Res, Scarborough, ME USA
[4] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
[5] Pohang Univ Sci & Technol, Div Adv Nucl Engn, Pohang, South Korea
基金
新加坡国家研究基金会;
关键词
magnetic reconnection; plasma beta; SHEAR EVIDENCE; DEPENDENCE; MAGNETOPAUSE;
D O I
10.1029/2024GL112126
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
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.
引用
收藏
页数:9
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