Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In
addition to the presence of magnetic field, the differences with neutral fluid isotropic …

A long-standing problem in magnetic reconnection is to explain why it tends to proceed at or
below a normalized rate of 0.1. This article gives a review of observational and numerical …

Magnetic reconnection converts, often explosively, stored magnetic energy to particle
energy in space and in the laboratory. Through processes operating on length scales that …

Global hybrid (electron fluid, kinetic ions) and fully kinetic simulations of the magnetosphere
have been used to show surprising interconnection between shocks, turbulence, and …

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 …

An emerging paradigm for the dissipation of magnetic turbulence in the supersonic solar
wind is via localized small-scale reconnection processes, essentially between quasi-2D …

We present the results of 3D particle-in-cell simulations that explore relativistic magnetic
reconnection in pair plasma with strong synchrotron cooling and a small mass fraction of …

A new path for the generation of a sub-ion-scale cascade in collisionless space and
astrophysical plasma turbulence, triggered by magnetic reconnection, is uncovered by …

We develop a framework for studying the statistical properties of current sheets in numerical
simulations of magnetohydrodynamic (MHD) turbulence with a strong guide field, as …

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