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

Physics of Plasmas · 2009 · Vol. 16(11) · pp. 112102–112102
A. BhattacharjeeYi-Min HuangHang YangB. N. Rogers

Abstract

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. The scaling of the growth rate of the fastest growing 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 an order of magnitude (for the range of Lundquist numbers considered). This regime of fast reconnection appears to be realizable in a dynamic and highly unstable thin current sheet, without requiring the current sheet to be turbulent.

Ionosphere and magnetosphere dynamicsMagnetic confinement fusion researchDust and Plasma Wave PhenomenaPhysicsPlasmoidIconCitationDownloadPlasmaWorld Wide WebComputer scienceMagnetic reconnectionNuclear physics
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References
Instability of current sheets and formation of plasmoid chains
Physics of Plasmas · 2007 · 669 citations
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Fast reconnection in high-Lundquist-number plasmas due to the plasmoid Instability · Scinovex