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 …

In this article, we state and review the premises on which a successful asymptotic closure of
the moment equations of wave turbulence is based, describe how and why this closure …

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

We present an analytical study of subproton electromagnetic fluctuations in a collisionless
plasma with a plasma beta of the order of unity. In the linear limit, a rigorous derivation from …

Using a three-dimensional compressible magnetohydrodynamic (MHD) simulation, we have
reproduced the fast solar wind in a direct and self-consistent manner, based on the …

It has long been known that the energy in velocity and magnetic field fluctuations in the solar
wind is not in equipartition. In this paper, we present an analysis of 5 yr of Wind data at 1 AU …

Shell models of hydrodynamic turbulence originated in the seventies. Their main aim was to
describe the statistics of homogeneous and isotropic turbulence in spectral space, using a …

The nonlinear interaction between counterpropagating Alfvén waves is the physical
mechanism underlying the cascade of energy to small scales in astrophysical plasma …

The energy spectrum of magnetohydrodynamic turbulence attracts interest due to its
fundamental importance and its relevance for interpreting astrophysical data. Here we …