English

Marginal Stability of Sweet-Parker Type Current Sheets at Low Lundquist Numbers

Plasma Physics 2018-06-06 v2 Solar and Stellar Astrophysics Space Physics

Abstract

Magnetohydrodynamic simulations have shown that a non-unique critical Lundquist number ScS_c exists, hovering around Sc104S_c \sim 10^4, above which threshold Sweet-Parker type stationary reconnecting configurations become unstable to a fast tearing mode dominated by plasmoid generation. It is known that the flow along the sheet plays a stabilizing role, though a satisfactory explanation of the non-universality and variable critical Lundquist numbers observed is still lacking. Here we discuss this question using 2D linear MHD simulations and linear stability analyses of Sweet-Parker type current sheets in the presence of background stationary inflows and outflows at low Lundquist numbers (S104S\le 10^4). Simulations show that the inhomogeneous outflow stabilizes the current sheet by stretching the growing magnetic islands and at the same time evacuating the magnetic islands out of the current sheet. This limits the time during which fluctuations which begin at any given wave-length can remain unstable, rendering the instability non-exponential. We find that the linear theory based on the expanding-wavelength assumption works well for SS larger than 1000\sim 1000. However we also find that the inflow and location of the initial perturbation also affect the stability threshold.

Keywords

Cite

@article{arxiv.1802.07162,
  title  = {Marginal Stability of Sweet-Parker Type Current Sheets at Low Lundquist Numbers},
  author = {Chen Shi and Marco Velli and Anna Tenerani},
  journal= {arXiv preprint arXiv:1802.07162},
  year   = {2018}
}