skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Fast reconnection in high-Lundquist-number plasmas due to the plasmoid Instability

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.3264103· OSTI ID:21274237
;  [1]; ;  [2]
  1. Center for Integrated Computation and Analysis of Reconnection and Turbulence, University of New Hampshire, Durham, New Hampshire 03824 (United States)
  2. Center for Integrated Computation and Analysis of Reconnection and Turbulence, Dartmouth College, Hanover, New Hampshire 03825 (United States)

Thin current sheets in systems of large size that exceed a critical value of the Lundquist number are unstable to a super-Alfvenic tearing instability, referred to hereafter as the plasmoid instability. The scaling of the growth rate of the most rapidly growing plasmoid instability with respect to the Lundquist number is shown to follow from the classical dispersion relation for tearing modes. As a result of this instability, the system realizes a nonlinear reconnection rate that appears to be weakly dependent on the Lundquist number, and larger than the Sweet-Parker rate by nearly an order of magnitude (for the range of Lundquist numbers considered). This regime of fast reconnection is realizable in a dynamic and highly unstable thin current sheet, without requiring the current sheet to be turbulent.

OSTI ID:
21274237
Journal Information:
Physics of Plasmas, Vol. 16, Issue 11; Other Information: DOI: 10.1063/1.3264103; (c) 2009 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 1070-664X
Country of Publication:
United States
Language:
English