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arxiv: 0903.0542 · v1 · pith:EOMTAX4Snew · submitted 2009-03-03 · 🌌 astro-ph.SR · physics.plasm-ph· physics.space-ph

Formation of Plasmoid Chains in Magnetic Reconnection

classification 🌌 astro-ph.SR physics.plasm-phphysics.space-ph
keywords reconnectionplasmoidchainsformationmagneticsweet-parkeragreementcall
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A detailed numerical study of magnetic reconnection in resistive MHD for very large, previously inaccessible, Lundquist numbers ($10^4\le S\le 10^8$) 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 $S^{3/8}$ and the instability growth rate in the linear stage as $S^{1/4}$, 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 $S>10^4$.

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