{ "id": "0903.0542", "version": "v1", "published": "2009-03-03T14:30:31.000Z", "updated": "2009-03-03T14:30:31.000Z", "title": "Formation of Plasmoid Chains in Magnetic Reconnection", "authors": [ "R. Samtaney", "N. F. Loureiro", "D. A. Uzdensky", "A. A. Schekochihin", "S. C. Cowley" ], "comment": "submitted to Phys. Rev. Lett", "categories": [ "astro-ph.SR", "physics.plasm-ph", "physics.space-ph" ], "abstract": "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 $S>10^4$.", "revisions": [ { "version": "v1", "updated": "2009-03-03T14:30:31.000Z" } ], "analyses": { "subjects": [ "52.35.Vd", "52.35.Py", "94.30.cp", "96.60.Iv" ], "keywords": [ "magnetic reconnection", "plasmoid chains", "large-aspect-ratio sweet-parker current sheets", "standard sweet-parker quasi-stationary picture", "instability growth rate" ], "tags": [ "journal article" ], "publication": { "doi": "10.1103/PhysRevLett.103.105004", "journal": "Physical Review Letters", "year": 2009, "month": "Sep", "volume": 103, "number": 10, "pages": 105004 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 814629, "adsabs": "2009PhRvL.103j5004S" } } }