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 …

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 …

An overview is given of important properties of spatial and temporal intermittency, including
evidence of its appearance in fluids, magnetofluids and plasmas, and its implications for …

The past decade has seen a flurry of research activity focused on discerning the physics of
kinetic scale turbulence in high-speed astrophysical plasma flows. By 'kinetic'we mean …

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 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 …

Learning from successful applications of methods originating in statistical mechanics,
complex systems science, or information theory in one scientific field (eg, atmospheric …

We present a combined observational and theoretical analysis to investigate the nature of
plasma turbulence at kinetic scales in the Earth's magnetosheath. In the first decade of the …

Electron scale solar wind (SW) turbulence has attracted great interest in recent years.
Considerable evidence exists that the turbulence is not fully dissipated near the proton …

The nature of subproton scale fluctuations in the solar wind is an open question, partly
because two similar types of electromagnetic turbulence can occur: kinetic Alfvén turbulence …