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 …

Kinetic energy transfer in compressible isotropic turbulence is studied using numerical
simulations with solenoidal forcing at turbulent Mach numbers ranging from 0.4 to 1.0 and at …

Reconnection and turbulence are two of the most commonly observed dynamical processes
in plasmas, but their relationship is still not fully understood. Using 2.5 D kinetic particle-in …

We present estimates of the turbulent energy-cascade rate derived from a Hall-
magnetohydrodynamic (MHD) third-order law. We compute the contribution from the Hall …

The plasmoid instability in evolving current sheets has been widely studied due to its effects
on the disruption of current sheets, the formation of plasmoids, and the resultant fast …

In the context of space and astrophysical plasma turbulence and particle heating, several
vocabularies emerge for estimating turbulent energy dissipation rate, including Kolmogorov …

Many high-energy astrophysical systems contain magnetized collisionless plasmas with
relativistic particles, in which turbulence can be driven by an arbitrary mixture of solenoidal …

A familiar problem in space and astrophysical plasmas is to understand how dissipation and
heating occurs. These effects are often attributed to the cascade of broadband turbulence …

Many questions remain about the compressibility of solar wind turbulence with respect to its
origins and properties. Low plasma beta (ratio of thermal to magnetic pressure) …