An overview is given of important properties of spatial and temporal intermittency, including
evidence of its appearance in fluids, magnetofluids and plasmas, and its implications for …

The complex nonlinear dynamical phenomenon described as turbulence, is known to have
a great impact on fluids, magnetohydrodynamic systems, and on plasmas. This paper …

Measurements of the elliptic flow, v 2, of identified hadrons (π±, K±, K s 0, p, p¯, ϕ, Λ, Λ¯, Ξ−,
Ξ¯+, Ω−, Ω¯+) in Au+ Au collisions at s NN= 7.7, 11.5, 19.6, 27, 39, and 62.4 GeV are …

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

In the lower solar coronal regions where the magnetic field is dominant, the Alfvén speed is
much higher than the wind speed. In contrast, the near-Earth solar wind is strongly super …

We present a new algorithm for the discretization of the non-relativistic Vlasov–Maxwell
system of equations for the study of plasmas in the kinetic regime. Using the discontinuous …

Weakly collisional and collisionless plasmas are typically far from local thermodynamic
equilibrium (LTE), and understanding energy conversion in such systems is a forefront …

Observed turbulence in space and astrophysics is expected to involve cascade and
subsequent dissipation and heating. Contrary to standard collisional fluid turbulence, the …

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 …

A statistical relationship between magnetic reconnection, current sheets, and intermittent
turbulence in the solar wind is reported for the first time using in situ measurements from the …