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

We propose a phenomenological model for incompressible magnetohydrodynamic
turbulence. We argue that nonlinear-wave interaction weakens as the energy cascade …

ABSTRACT A numerical study of strong kinetic-Alfvén turbulence at scales smaller than the
ion gyroscale is presented, and a phenomenological model is proposed that argues that …

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 …

Magnetic field lines in astrophysical plasmas are expected to be frozen-in at scales larger
than the ion gyroradius. The rapid reconnection of magnetic-flux structures with dimensions …

We construct a database from ACE spacecraft measurements of solar wind magnetic field
fluctuations at 1 AU which resolves∼ 2 decades in frequency at the high end of the inertial …

We present numerical studies of three-dimensional electron magnetohydrodynamic (EMHD)
turbulence. We investigate the cascade timescale and anisotropy of freely decaying, strong …

We investigate properties of plasma turbulence from magnetohydrodynamic (MHD) to sub-
ion scales by means of two-dimensional, high-resolution hybrid particle-in-cell 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 …