Small-scale-field Dynamo

Details Small-scale-field Dynamo Small-scale-field Dynamo

1996-11-22

arxiv.org/abs/astro-ph/9611194v1

Phys.Rev.Lett.77:4342-4345,1996

Astronomy and Astrophysics

Astrophysics

11 pages Plain TeX, no figures, Accepted by Phys. Rev. Lett

Scientific paper

10.1103/PhysRevLett.77.4342

Generation 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.

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