Small-scale-field Dynamo

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dc.creatorGruzinov, A.
dc.creatorCowley, S.
dc.creatorSudan, R.
dc.date1996-11-22
dc.date.accessioned2026-07-07T10:57:48Z
dc.date.available2026-07-07T10:57:48Z
dc.descriptionGeneration of magnetic field energy, without mean field generation, is studied. Isotropic mirror-symmetric turbulence of a conducting fluid amplifies the energy of small-scale magnetic perturbations if the magnetic Reynolds number is high, and the dimensionality of space d satisfies 2.103 < d <8.765. The result does not depend on the model of turbulence, incompressibility and isotropy being the only requirements.
dc.description11 pages Plain TeX, no figures, Accepted by Phys. Rev. Lett
dc.identifierhttps://arxiv.org/abs/astro-ph/9611194
dc.identifierhttp://arxiv.org/abs/astro-ph/9611194
dc.identifierPhys.Rev.Lett.77:4342-4345,1996
dc.identifierdoi:10.1103/PhysRevLett.77.4342
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186881
dc.subjectAstrophysics
dc.titleSmall-scale-field Dynamo
dc.typetext

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