This paper summarises some of the recent progress that has been made in understanding
astrophysical plasma turbulence in the solar wind, from in situ spacecraft observations. At …

The Sun's outer atmosphere is heated to temperatures of millions of degrees, and solar
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …

In situ measurements of the solar wind have been available for almost 60 years, and in that
time plasma physics simulation capabilities have commenced and ground‐based solar …

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 …

The near-Earth space is a unique laboratory to explore turbulence and energy dissipation
processes in magnetized plasmas thanks to the availability of high-quality data from various …

Turbulence plays a key role in the conversion of the energy of large-scale fields and flows to
plasma heat, impacting the macroscopic evolution of the heliosphere and other …

The physical foundations of the dissipation of energy and the associated heating in weakly
collisional plasmas are poorly understood. Here, we compare and contrast several …

We report the results of a direct comparison between different kinetic models of collisionless
plasma turbulence in two spatial dimensions. The models considered include a first …

The current state of the art thermal particle measurements in the solar wind are insufficient to
address many long standing, fundamental physical processes. The solar wind is a weakly …

We investigate the nature of magnetic turbulent fluctuations, around ion characteristic
scales, in a fast solar wind stream, by using Cluster data. Contrarily to slow solar wind …