{ "id": "1106.5777", "version": "v2", "published": "2011-06-28T19:42:27.000Z", "updated": "2011-09-28T04:17:17.000Z", "title": "Nonlinear small-scale dynamos at low magnetic Prandtl numbers", "authors": [ "Axel Brandenburg" ], "comment": "7 pages, 6 figures, ApJ, in print", "journal": "Astrophys. J. 741, 92 (2011)", "doi": "10.1088/0004-637X/741/2/92", "categories": [ "astro-ph.SR" ], "abstract": "Saturated small-scale dynamo solutions driven by isotropic non-helical turbulence are presented at low magnetic Prandtl numbers Pm down to 0.01. For Pm < 0.1, most of the energy is dissipated via Joule heat and, in agreement with earlier results for helical large-scale dynamos, kinetic energy dissipation is shown to diminish proportional to Pm^{1/2} down to values of 0.1. In agreement with earlier work, there is, in addition to a short Golitsyn k^{-11/3} spectrum near the resistive scale also some evidence for a short k^{-1} spectrum on larger scales. The rms magnetic field strength of the small-scale dynamo is found to depend only weakly on the value of Pm and decreases by about a factor of 2 as Pm is decreased from 1 to 0.01. The possibility of dynamo action at Pm=0.1 in the nonlinear regime is argued to be a consequence of a suppression of the bottleneck seen in the kinetic energy spectrum in the absence of a dynamo and, more generally, a suppression of kinetic energy near the dissipation wavenumber.", "revisions": [ { "version": "v2", "updated": "2011-09-28T04:17:17.000Z" } ], "analyses": { "keywords": [ "nonlinear small-scale dynamos", "small-scale dynamo solutions driven", "kinetic energy", "low magnetic prandtl numbers pm", "rms magnetic field strength" ], "tags": [ "journal article" ], "publication": { "journal": "The Astrophysical Journal", "year": 2011, "month": "Nov", "volume": 741, "number": 2, "pages": 92 }, "note": { "typesetting": "TeX", "pages": 7, "language": "en", "license": "arXiv", "status": "editable", "inspire": 916410, "adsabs": "2011ApJ...741...92B" } } }