Turbulent flows are characterized by the non-linear cascades of energy and other inviscid
invariants across a huge range of scales, from where they are injected to where they are …

Turbulent intermittency plays a fundamental role in fields ranging from combustion physics
and chemical engineering to meteorology. There is a rather general agreement that …

This book presents an introduction to, and modern account of, magnetohydrodynamic
(MHD) turbulence, an active field both in general turbulence theory and in various areas of …

A review of the present status of the theory of magnetic reconnection is given. In strongly
collisional plasmas reconnection proceeds via resistive current sheets, ie quasi-stationary …

We report the results of an extensive numerical study of the small-scale turbulent dynamo.
The primary focus is on the case of large magnetic Prandtl numbers Pr m, which is relevant …

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 …

Direct numerical simulations of decaying and forced magnetohydrodynamic (MHD)
turbulence without and with mean magnetic field are analyzed by higher-order two-point …

The scaling properties of three-dimensional magnetohydrodynamic turbulence with finite
magnetic helicity are obtained from direct numerical simulations using 512 3 modes. The …

A comprehensive picture of three-dimensional 3D isotropic magnetohydrodynamic MHD
turbulence is presented based on the first 5123-mode numerical simulations performed …

This paper gives a review of some recent work on intermittency, non-Gaussian statistics, and
fractal scaling of solar wind magnetohydrodynamic turbulence. Model calculations and …