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 …

The fast solar wind's high speeds and non-thermal features require that considerable
heating occurs well above the Sun's surface. Two leading theories seem incompatible: low …

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 present results from three-dimensional hybrid-kinetic simulations of Alfvénic turbulence
in a high-β, collisionless plasma. The key feature of such turbulence is the interplay between …

The dissipative mechanism in weakly collisional plasma is a topic that pervades decades of
studies without a consensus solution. We compare several energy dissipation estimates …

Abstract The Integrated Science Investigation of the Sun (ISIS) is a complete science
investigation on the Solar Probe Plus (SPP) mission, which flies to within nine solar radii of …

Does overall thermal equilibrium exist between ions and electrons in a weakly collisional,
magnetized, turbulent plasma? And, if not, how is thermal energy partitioned between ions …

The dissipation of magnetized turbulence is an important paradigm for describing heating
and energy transfer in astrophysical environments such as the solar corona and wind; …

A Hybrid Vlasov–Maxwell (HVM) model is presented and recent results about the link
between kinetic effects and turbulence are reviewed. Using five-dimensional (2D in space …