Abstract Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …

One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …

In this review we will focus on a topic of fundamental importance for both astrophysics and
plasma physics, namely the occurrence of large-amplitude low-frequency fluctuations of the …

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 …

We show the first three dimensional (3D) dispersion relations and k spectra of magnetic
turbulence in the solar wind at subproton scales. We used the Cluster data with short …

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 …

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 …

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 …