The local magnetic field induces many types of anisotropy in plasma turbulence, changing
the rate of energy transfer and affecting the propagation of energetic particles. It is …

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 …

Magnetic fields are ubiquitous in the universe (Parker 1979, Zeldovich et al. 1983). Their
interaction with an electrically conducting fluid gives rise to a complex system–a …

The current understanding of magnetohydrodynamic (MHD) turbulence envisions turbulent
eddies which are anisotropic in all three directions. In the plane perpendicular to the local …

We investigate the anisotropy of Alfvénic turbulence in the inertial range of slow solar wind
and in both driven and decaying reduced magnetohydrodynamic simulations. A direct …

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

A discussion of the advantages and limitations of the concept of critical balance (CB), as
employed in turbulence phenomenologies, is presented. The incompressible …

We present direct numerical simulations of inhomogeneous reduced magnetohydrodynamic
(RMHD) turbulence between the Sun and the Alfvén critical point. These are the first such …

We present an analytical study of subproton electromagnetic fluctuations in a collisionless
plasma with a plasma beta of the order of unity. In the linear limit, a rigorous derivation from …

Magnetohydrodynamic Turbulence Mediated by Reconnection - IOPscience This site uses
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