This paper presents a theoretical framework for understanding plasma turbulence in
astrophysical plasmas. It is motivated by observations of electromagnetic and density …

The role of turbulence in various astrophysical settings is reviewed. Among the differences
to laboratory and atmospheric turbulence we highlight the ubiquitous presence of magnetic …

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 …

We develop a one-dimensional solar-wind model that includes separate energy equations
for the electrons and protons, proton temperature anisotropy, collisional and collisionless …

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 …

In the presence of magnetic helicity, inverse transfer from small to large scales is well known
in magnetohydrodynamic (MHD) turbulence and has applications in astrophysics …

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

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 …

Strong incompressible three-dimensional magnetohydrodynamic turbulence is investigated
by means of high-resolution direct numerical simulations. The simulations show that the …

The question is addressed as to what extent incompressible magnetohydrodynamics can
describe random magnetic and velocity fluctuations measured in the solar wind. It is …