When discussing research in physics and in science more generally, it is common to ascribe
equal importance to the three components of the scientific trinity: theoretical, experimental …

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 …

Modelling the transport of cosmic rays (CRs) in the heliosphere represents a global
challenge in the field of heliophysics, in that such a study, if it were to be performed from first …

In situ measurements of the solar wind have been available for almost 60 years, and in that
time plasma physics simulation capabilities have commenced and ground‐based solar …

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 …

How turbulent energy is dissipated in weakly collisional space and astrophysical plasmas is
a major open question. Here, we present the application of a field-particle correlation …

High resolution, fully kinetic, three dimensional (3D) simulation of collisionless plasma
turbulence shows the development of turbulence characterized by sheetlike current density …

We examine the radial evolution of correlation lengths perpendicular (${\lambda} _
{C}^{\perp} $) and parallel (${\lambda} _ {C}^{\parallel} $) to the magnetic-field direction …