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 near-Earth space is a unique laboratory to explore turbulence and energy dissipation
processes in magnetized plasmas thanks to the availability of high-quality data from various …

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

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 …

Magnetic energy around astrophysical compact objects can strongly dominate over plasma
rest mass. Emission observed from these systems may be fed by dissipation of Alfvén wave …

Wave-particle resonance, a ubiquitous process in the plasma universe, occurs when
resonant particles observe a constant wave phase to enable sustained energy transfer …

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 Vlasov equation describes collisionless plasmas in the continuum limit and applies to
many fundamental plasma energization phenomena. Because this equation governs the …

Heliospheric plasma turbulence plays a key role in transferring the energy of large‐scale
magnetic field and plasma flow fluctuations to smaller scales where the energy can be …