English

Diffusion regions and 3D energy mode development in spontaneous reconnection

Solar and Stellar Astrophysics 2019-09-04 v1

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.

Keywords

Cite

@article{arxiv.1906.03964,
  title  = {Diffusion regions and 3D energy mode development in spontaneous reconnection},
  author = {Shuoyang Wang and Takaaki Yokoyama},
  journal= {arXiv preprint arXiv:1906.03964},
  year   = {2019}
}

Comments

13 pages, 14 figures

R2 v1 2026-06-23T09:48:47.560Z