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

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

Direct evidence of an inertial-range turbulent energy cascade has been provided by
spacecraft observations in heliospheric plasmas. In the solar wind, the average value of the …

The solar wind, a continuous flow of plasma from the sun, not only shapes the near Earth
space environment but also serves as a natural laboratory to study plasma turbulence in …

The physical foundations of the dissipation of energy and the associated heating in weakly
collisional plasmas are poorly understood. Here, we compare and contrast several …

The description of the local turbulent energy transfer and the high-resolution ion distributions
measured by the Magnetospheric Multiscale mission together provide a formidable tool to …

For the solar wind, a wealth of observational evidence indicates that turbulence is an
important dynamical process for velocity (v), magnetic (b), and other related fluctuations at …

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

Abstract The Parker Solar Probe mission has shown the ubiquitous presence of strong
magnetic field deflections, namely switchbacks, during its first perihelion where it was …

Plasma turbulence is studied via direct numerical simulations in a two-dimensional spatial
geometry. Using a hybrid Vlasov-Maxwell model, we investigate the possibility of a velocity …