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 …

This paper summarises some of the recent progress that has been made in understanding
astrophysical plasma turbulence in the solar wind, from in situ spacecraft observations. At …

This paper presents a theoretical framework for understanding plasma turbulence in
astrophysical plasmas. It is motivated by observations of electromagnetic and density …

We present two-temperature, radiative general relativistic magnetohydrodynamic
simulations of Magnetically Arrested Discs (MAD) that launch powerful relativistic jets. The …

We show the first three dimensional (3D) dispersion relations and k spectra of magnetic
turbulence in the solar wind at subproton scales. We used the Cluster data with short …

Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In
addition to the presence of magnetic field, the differences with neutral fluid isotropic …

We present results from three-dimensional hybrid-kinetic simulations of Alfvénic turbulence
in a high-β, collisionless plasma. The key feature of such turbulence is the interplay between …

The nature of small-scale turbulent fluctuations in the solar wind is investigated using a
comparison of Cluster magnetic and electric field measurements to predictions arising from …

The accretion flow around the Galactic Centre black hole Sagittarius A*(Sgr A*) is expected
to have an electron temperature that is distinct from the ion temperature, due to weak …

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 …