One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …

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

The dissipative mechanism in weakly collisional plasma is a topic that pervades decades of
studies without a consensus solution. We compare several energy dissipation estimates …

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 …

Using a three-dimensional compressible magnetohydrodynamic (MHD) simulation, we have
reproduced the fast solar wind in a direct and self-consistent manner, based on the …

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 …

A dynamical vectorial equation for homogeneous incompressible Hall-
magnetohydrodynamic (MHD) turbulence together with the exact scaling law for third-order …

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 …

We briefly review helicity dynamics, inverse and bidirectional cascades in fluid and
magnetohydrodynamic (MHD) turbulence, with an emphasis on the latter. The energy of a …

Magnetic fields are crucial in numerous astrophysical processes within the interstellar
medium (ISM). However, the detailed determination of magnetic field geometry is notoriously …