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 nature of small-scale turbulent fluctuations in the solar wind is investigated using a
comparison of Cluster magnetic and electric field measurements to predictions arising from …

The past decade has seen a flurry of research activity focused on discerning the physics of
kinetic scale turbulence in high-speed astrophysical plasma flows. By 'kinetic'we mean …

A three-dimensional, nonlinear gyrokinetic simulation of plasma turbulence resolving scales
from the ion to electron gyroradius with a realistic mass ratio is presented, where all …

We present a combined observational and theoretical analysis to investigate the nature of
plasma turbulence at kinetic scales in the Earth's magnetosheath. In the first decade of the …

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 …

The description of the turbulent spectrum of magnetic fluctuations in the solar wind in the
kinetic range of scales is not yet completely established. Here, we perform a statistical study …

A new path for the generation of a sub-ion-scale cascade in collisionless space and
astrophysical plasma turbulence, triggered by magnetic reconnection, is uncovered by …

Electron scale solar wind (SW) turbulence has attracted great interest in recent years.
Considerable evidence exists that the turbulence is not fully dissipated near the proton …