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 …

Alongside magnetic reconnection, turbulence is another fundamental nonlinear plasma
phenomenon that plays a key role in energy transport and conversion in space and …

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

This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …

Despite decades of study of high-temperature weakly collisional plasmas, a complete
understanding of how energy is transferred between particles and fields in turbulent …

The magnetorotational instability (MRI) is a fundamental mechanism determining the
macroscopic dynamics of astrophysical accretion disks. In collisionless accretion flows …

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 …

Horizon-scale observations from the Event Horizon Telescope (EHT) have enabled
precision study of supermassive black hole accretion. Contemporary accretion modeling …