The corona is a layer of hot plasma that surrounds the Sun, traces out its complex magnetic
field, and ultimately expands into interplanetary space as the supersonic solar wind …

The electrons are an essential particle species in the solar wind. They often exhibit non-
equilibrium features in their velocity distribution function. These include temperature …

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 …

HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division
designed to explore the dynamic three-dimensional mechanisms controlling the physics of …

The physical foundations of the dissipation of energy and the associated heating in weakly
collisional plasmas are poorly understood. Here, we compare and contrast several …

We perform a statistical study of the turbulent power spectrum at inertial and kinetic scales
observed during the first perihelion encounter of the Parker Solar Probe. We find that often …

We report the results of a direct comparison between different kinetic models of collisionless
plasma turbulence in two spatial dimensions. The models considered include a first …

We report analytical and numerical investigations of subion-scale turbulence in low-beta
plasmas using a rigorous reduced kinetic model. We show that efficient electron heating …

The dissipation of turbulence in astrophysical systems is fundamental to energy transfer and
heating in environments ranging from the solar wind and corona to accretion disks and the …

Turbulence and kinetic processes in magnetized space plasmas have been extensively
investigated over the past decades via in-situ spacecraft measurements, theoretical models …