Physical Regimes of Two-dimensional MHD Turbulent Reconnection in Different Lundquist Numbers

Using two-dimensional MHD simulations in different Lundquist numbers S , we investigate physical regimes of turbulent reconnection and the role of turbulence in enhancing the reconnection rate. Turbulence is externally injected into the system with varying strength. Externally driven turbulence cont...

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Veröffentlicht in:	The Astrophysical journal 2022-02, Vol.926 (1), p.97
Hauptverfasser:	Sun, Haomin, Yang, Yan, Lu, Quanming, Lu, San, Wan, Minping, Wang, Rongsheng
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysical magnetism Astrophysics Burst astrophysics Energy conversion Interplanetary magnetic fields Interstellar magnetic fields Kelvin-Helmholtz instability Kinetic energy Magnetic fields Magnetic reconnection Magnetohydrodynamic turbulence Magnetohydrodynamics Plasma astrophysics Plasma physics Plasmas (physics) Solar magnetic fields Solar magnetic reconnection Solar physics Turbulence
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