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 …

The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …

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 …

To the naked eye, turbulent flows exhibit whirls of many different sizes. To each size, or
scale, corresponds a fraction of the total energy resulting from a cascade in five dimensions …

The complex nonlinear dynamical phenomenon described as turbulence, is known to have
a great impact on fluids, magnetohydrodynamic systems, and on plasmas. This paper …

Kinetic plasma turbulence cascade spans multiple scales ranging from macroscopic fluid
flow to sub-electron scales. Mechanisms that dissipate large scale energy, terminate the …

We present results from particle-in-cell simulations of driven turbulence in magnetized,
collisionless, and relativistic pair plasmas. We find that the fluctuations are consistent with …

It has recently been proposed that the inertial interval in magnetohydrodynamic (MHD)
turbulence is terminated at small scales not by a Kolmogorov-like dissipation region, but …

High time-resolution solar wind magnetic field data are employed to study statistics
describing intermittency near the first perihelion (∼ 35.6 R⊙) of the Parker Solar Probe …

The understanding of the fundamental properties of turbulence in collisionless plasmas,
such as the solar wind, is a frontier problem in plasma physics. In particular, the occurrence …