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 …

Alongside magnetic reconnection, turbulence is another fundamental nonlinear plasma
phenomenon that plays a key role in energy transport and conversion in space and …

We perform a high-resolution, 2D, fully kinetic numerical simulation of a turbulent plasma
system with observation-driven conditions, in order to investigate the interplay between …

We use three-dimensional (3-D) fully kinetic particle-in-cell simulations to study the
occurrence of magnetic reconnection in a simulation of decaying turbulence created by …

Context. Recent satellite observations in the solar wind and in the Earth's magnetosheath
have shown that the turbulent magnetic field spectrum, which is know to steepen around ion …

We derive two new forms of the Kármán–Howarth–Monin (KHM) equation for decaying
compressible Hall magnetohydrodynamic (MHD) turbulence. We test them on results of a …

The properties of turbulence observed within the plasma originating from the
magnetosheath and the magnetospheric boundary layer, which have been entrained within …

Spatiotemporal properties of two-dimensional (2D) Hall-magnetohydrodynamic (MHD)
turbulence at intermediate plasma β= 2 are studied by means of Fast Iterative Filtering (FIF) …

Turbulent space and astrophysical plasmas exhibit a complex dynamics, which involves
nonlinear coupling across different temporal and spatial scales. There is growing evidence …

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