We briefly review helicity dynamics, inverse and bidirectional cascades in fluid and
magnetohydrodynamic (MHD) turbulence, with an emphasis on the latter. The energy of a …

This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …

Ninety-nine percent of ordinary matter in the Universe is in the form of ionized fluids, or
plasmas. The study of the magnetic properties of such electrically conducting fluids …

We present three-dimensional direct numerical simulations and an analytic model of
reflection-driven magnetohydrodynamic (MHD) turbulence in the solar wind. Our simulations …

Most of the visible matter in the Universe is in the form of highly turbulent plasmas. For a
long time the turbulent character of astrophysical fluids has been neglected and not well …

Dust storms are typical dispersed two-phase atmospheric turbulence involving electrified
charged dust particles. Previous observations have demonstrated that clean-air atmospheric …

Low-frequency turbulence in Saturn's magnetosheath is investigated using in situ
measurements of the Cassini spacecraft. Focus is put on the magnetic energy spectra …

Parametric instability, inverse cascade and the 1/f range of solar-wind turbulence Page 1 J. Plasma
Phys. (2018), vol. 84, 905840106 c Cambridge University Press 2018 This is an Open Access …

We report the experimental observation of intermittency in a regime dominated by random
shock waves on the surface of a fluid. We achieved such a nondispersive surface-wave field …

One of the most important predictions in magnetohydrodynamics is that in the presence of a
uniform magnetic field b 0 e^∥ a transition from weak to strong wave turbulence should …