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 …

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 …

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 …

An overview is given of important properties of spatial and temporal intermittency, including
evidence of its appearance in fluids, magnetofluids and plasmas, and its implications for …

Shock waves, as shown by simulations and observations, can generate high levels of
downstream vortical turbulence, including magnetic islands. We consider a combination of …

Shortly after the seminal paper “Self-Organized Criticality: An explanation of 1/f noise” by
Bak et al.(1987), the idea has been applied to solar physics, in “Avalanches and the …

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

The significant influences of turbulence in neutral fluid hydrodynamics are well accepted but
the potential for analogous effects in space and astrophysical plasmas is less widely …

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 …

Solar wind observations and magnetohydrodynamic (MHD) simulations are used to probe
the nature of turbulence heating. In particular, the electron heat flux, electron temperature …