A. Bershadskii
Published 2016-07-07Version 1
It is shown, using results of recent direct numerical simulations, that spectral properties of distributed chaos in MHD turbulence with zero mean magnetic field are similar to those of hydrodynamic turbulence. An exception is MHD spontaneous breaking of space translational symmetry, when the stretched exponential spectrum $\exp(-k/k_{\beta})^{\beta}$ has $\beta=4/7$.
Buoyancy driven turbulence and distributed chaos
Distributed chaos and turbulence in Bénard-Marangoni and Rayleigh-Bénard convection
Superfluid (quantum) turbulence and distributed chaos
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