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 overview is an assessment of the gyrokinetic framework and simulations to compute
turbulent transport in fusion plasmas. It covers an introduction to the gyrokinetic theory, the …

This paper presents a theoretical framework for understanding plasma turbulence in
astrophysical plasmas. It is motivated by observations of electromagnetic and density …

Turbulent plasmas generate a multitude of thin current structures that can be sites for
magnetic reconnection. The Magnetospheric Multiscale (MMS) mission has recently …

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 …

Kinetic plasma turbulence cascade spans multiple scales ranging from macroscopic fluid
flow to sub-electron scales. Mechanisms that dissipate large scale energy, terminate the …

Wavelet analysis can be used to measure the power spectrum of solar-wind fluctuations
along a line in any direction (θ, ϕ) with respect to the local mean magnetic field B 0. This …

This paper presents a complete theoretical framework for studying turbulence and transport
in rapidly rotating tokamak plasmas. The fundamental scale separations present in plasma …

A new analytically and numerically manageable model collision operator is developed
specifically for turbulence simulations. The like-particle collision operator includes both pitch …

Nonlinear gyrokinetics is the major formalism used for both the analytical and numerical
descriptions of low-frequency microturbulence in magnetized plasmas. Its derivation from …