A dynamical approach, rather than the usual statistical approach, is taken to explore the
physical mechanisms underlying the nonlinear transfer of energy, the damping of the …

The nonlinear interaction between counterpropagating Alfvén waves is the physical
mechanism underlying the cascade of energy to small scales in astrophysical plasma …

Laboratory experiments provide a valuable complement to explore the fundamental physics
of space plasmas without the limitations inherent to spacecraft measurements. Specifically …

Particle velocity distributions measured in the weakly collisional solar wind are frequently
found to be non-Maxwellian, but how these non-Maxwellian distributions impact the physics …

Understanding the removal of energy from turbulent fluctuations in a magnetized plasma
and the consequent energization of the constituent plasma particles is a major goal of …

Alfvén wave collisions are the primary building blocks of the non-relativistic turbulence that
permeates the heliosphere and low-to moderate-energy astrophysical systems. However …

A shear Alfvén wave parametric instability is observed for the first time in the laboratory.
When a single finite ω/Ω i kinetic Alfvén wave (KAW) is launched in the Large Plasma …

In space and astrophysical plasmas, turbulence is responsible for transferring energy from
large scales driven by violent events or instabilities, to smaller scales where turbulent …

It is often asserted or implicitly assumed, without justification, that the results of two-
dimensional investigations of plasma turbulence are applicable to the three-dimensional …

The description of the Moffatt and Parker problem recently revisited by O. Pezzi et
al.[Astrophys. J. 834, 166 (2017) 1538-4357 10.3847/1538-4357/834/2/166] is here …