Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Formation of Plasmoid Chains in Magnetic Reconnection

Journal Article · · Physical Review Letters
 [1];  [2];  [3];  [4];  [2]
  1. Princeton Plasma Physics Laboratory, Princeton University, Princeton, New Jersey 08543 (United States)
  2. EURATOM/UKAEA Fusion Association, Culham Science Centre, Abingdon, OX14 3DB (United Kingdom)
  3. Department of Astrophysical Sciences/CMSO, Princeton University, Princeton, New Jersey 08544 (United States)
  4. Rudolf Peierls Centre for Theoretical Physics, University of Oxford, Oxford OX1 3NP (United Kingdom)
A detailed numerical study of magnetic reconnection in resistive MHD for very large, previously inaccessible, Lundquist numbers (10{sup 4}<=S<=10{sup 8}) is reported. Large-aspect-ratio Sweet-Parker current sheets are shown to be unstable to super-Alfvenically fast formation of plasmoid (magnetic-island) chains. The plasmoid number scales as S{sup 3/8} and the instability growth rate in the linear stage as S{sup 1/4}, in agreement with the theory by Loureiro et al.[Phys. Plasmas 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 quasistationary picture for S>10{sup 4}.
OSTI ID:
21364675
Journal Information:
Physical Review Letters, Journal Name: Physical Review Letters Journal Issue: 10 Vol. 103; ISSN 0031-9007; ISSN PRLTAO
Country of Publication:
United States
Language:
English