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 solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …

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 …

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 …

The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere - IOPscience This
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …

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 …

We report on the observation of fine-scale structure in the outer corona at solar maximum,
using deep-exposure campaign data from the Solar Terrestrial Relations Observatory-A …

We investigate the radial dependence of the spectral break separating the inertial from the
dissipation range in power density spectra of interplanetary magnetic field fluctuations …

We present three-dimensional direct numerical simulations and an analytic model of
reflection-driven magnetohydrodynamic (MHD) turbulence in the solar wind. Our simulations …

We present direct numerical simulations of inhomogeneous reduced magnetohydrodynamic
(RMHD) turbulence between the Sun and the Alfvén critical point. These are the first such …