Dynamo and Alfvén effect in MHD turbulence

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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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