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 …

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 …

The complex nonlinear dynamical phenomenon described as turbulence, is known to have
a great impact on fluids, magnetohydrodynamic systems, and on plasmas. This paper …

A Hybrid Vlasov–Maxwell (HVM) model is presented and recent results about the link
between kinetic effects and turbulence are reviewed. Using five-dimensional (2D in space …

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 …

A review of spectral anisotropy and variance anisotropy for solar wind fluctuations is given,
with the discussion covering inertial range and dissipation range scales. For the inertial …

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

The anisotropic nature of solar wind magnetic turbulence fluctuations is investigated scale
by scale using high cadence in situ magnetic field measurements from the Cluster and ACE …

We present a measurement of the scale-dependent, three-dimensional structure of the
magnetic field fluctuations in inertial range solar wind turbulence with respect to a local …

The solar cycle dependence of various turbulence quantities and cosmic-ray (CR) diffusion
coefficients is investigated by using OMNI 1 minute resolution data over 22 years. We …