Dynamo and Alfvén effect in MHD turbulence

Details Dynamo and Alfvén effect in MHD turbulence Dynamo and Alfvén effect in MHD turbulence

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005iat..work..102m&link_type=abstract

"Proceedings of the workshop on "Interdisciplinary Aspects of Turbulence" Ringberg Castle, Tegernsee, Germany, April 18 - 22,200

Astronomy and Astrophysics

Astrophysics

Scientific paper

This extended abstract reports a spectral relation between residual and total energy, as well as the influence of an imposed mean magnetic field on the spectra. The proposed physical picture, which is confirmed by accompanying direct numerical simulations, embraces two-dimensional MHD turbulence, globally isotropic three-dimensional systems as well as turbulence permeated by a strong mean magnetic field. The results have direct implications on the current understanding of the energy cascade in MHD turbulence.

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