Diffusion regions and 3D energy mode development in spontaneous reconnection
arXiv:1906.03964 · doi:10.1063/1.5098129
Abstract
The understanding of magnetic reconnection in three-dimension (3D) is far shallower than its counterpart in two-dimension (2D) due to its potential complication, not to mention the evolving of the spontaneously growing turbulence. We investigate the reason for reconnection acceleration on the characters and development of diffusion regions and sheared 3D energy modes (energy modes that are not parallel to the anti-parallel magnetic fields) during the turbulence building stage. We found that multiple reconnection layers emerge due to the growth of 3D sheared tearing instability. Diffusion regions on adjacent reconnection layers form an inflow-outflow coupling that enhances the local reconnection. Further coupling of the existing energy modes breeds new energy modes near the current sheet edge. As reconnection layers span and interact with each other across the whole current sheet, global magnetic energy consumption accelerates. The significant contribution of 3D energy modes and their interaction to the reconnection rate enhancement seems to be independent on magnetic diffusivity. On the other hand, the global guide field changes the layout of 3D reconnection layer thus determines whether the system is fast-reconnection-preferable.
arXiv comment13 pages, 14 figures
References in corpus (15)
- Reconnection in a Weakly Stochastic Field
- Fast Reconnection in High-Lundquist-Number Plasmas Due to Secondary Tearing Instabilities
- Plasmoid-Induced-Reconnection and Fractal Reconnection
- Numerical Tests of Fast Reconnection in Weakly Stochastic Magnetic Fields
- Scaling laws of resistive magnetohydrodynamic reconnection in the high-Lundquist-number, plasmoid-unstable regime
- Magnetic reconnection and stochastic plasmoid chains in high-Lundquist-number plasmas
- Turbulent Magnetohydrodynamic Reconnection Mediated by the Plasmoid Instability
- X-point collapse and saturation in the nonlinear tearing mode reconnection
- Disruption of sheetlike structures in Alfvénic turbulence by magnetic reconnection
- Collisionless Reconnection in Magnetohydrodynamic and Kinetic Turbulence
- Magnetohydrodynamic turbulence mediated by reconnection
- Statistics of Reconnection-Driven Turbulence
- Self-generated turbulence in magnetic reconnection
- Three-dimensional Spontaneous Magnetic Reconnection
- Three-Dimensional MHD Magnetic Reconnection Simulations with Finite Guide Field: Proposal of the Shock-Evoking Positive-Feedback Model