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

The complex interaction between shocks and plasma turbulence is extremely important to
address crucial features of energy conversion in a broad range of astrophysical systems. We …

Despite decades of study of high-temperature weakly collisional plasmas, a complete
understanding of how energy is transferred between particles and fields in turbulent …

Our understanding of processes occurring in the heliosphere historically began with
reduced dimensionality-one-dimensional (1D) and two-dimensional (2D) sketches and …

The pressure–strain interaction describes the rate per unit volume that energy is converted
between bulk flow and thermal energy in neutral fluids or plasmas. The term has been …

We discuss the phenomenon of energization of relativistic charged particles in three-
dimensional incompressible MHD turbulence and the diffusive properties of the motion of …

We study the nature of pressure-strain interaction at reconnection sites detected by NASA's
Magnetospheric Multiscale Mission. We employ data from a series of previously published …

A novel multispacecraft technique applied to Magnetospheric Multiscale Mission data in the
Earth's magnetosheath enables evaluation of the energy cascade rate from the full Yaglom's …

Continuum Vlasov simulations can be utilized for highly accurate modelling of fully kinetic
plasmas. Great progress has been made recently regarding the applicability of the method …