English

Formation of Plasmoid Chains in Magnetic Reconnection

Solar and Stellar Astrophysics 2015-05-13 v1 Plasma Physics Space Physics

Abstract

A detailed numerical study of magnetic reconnection in resistive MHD for very large, previously inaccessible, Lundquist numbers (104S10810^4\le S\le 10^8) is reported. Large-aspect-ratio Sweet-Parker current sheets are shown to be unstable to super-Alfv\'enically fast formation of plasmoid (magnetic-island) chains. The plasmoid number scales as S3/8S^{3/8} and the instability growth rate in the linear stage as S1/4S^{1/4}, in agreement with the theory by Loureiro et al. [Phys. Plasmas {\bf 14}, 100703 (2007)]. In the nonlinear regime, plasmoids continue to grow faster than they are ejected and completely disrupt the reconnection layer. These results suggest that high-Lundquist-number reconnection is inherently time-dependent and hence call for a substantial revision of the standard Sweet-Parker quasi-stationary picture for S>104S>10^4.

Keywords

Cite

@article{arxiv.0903.0542,
  title  = {Formation of Plasmoid Chains in Magnetic Reconnection},
  author = {R. Samtaney and N. F. Loureiro and D. A. Uzdensky and A. A. Schekochihin and S. C. Cowley},
  journal= {arXiv preprint arXiv:0903.0542},
  year   = {2015}
}

Comments

submitted to Phys. Rev. Lett

R2 v1 2026-06-21T12:17:50.627Z