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.
Authors
- G.S. Yun (ORCID: https://orcid.org/0000-0002-1880-5865)
- Modhuchandra Laishram (ORCID: https://orcid.org/0000-0002-8644-1434)
- Young Dae Yoon (ORCID: https://orcid.org/0000-0001-8394-2076)
- D. E. Wendel (ORCID: https://orcid.org/0000-0002-1925-9413)
- T. E. Moore (ORCID: https://orcid.org/0000-0002-3150-1137)
Institutions
- Pohang University of Science and Technology (KR)
- Goddard Space Flight Center (US)
- Asia Pacific Center for Theoretical Physics (KR)
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
Funders
- National Aeronautics and Space Administration
- National Research Foundation of Korea