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 …

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 solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their
interaction is governed by complex physical processes and creates heliospheric regions …

Aims. The aim of this work is to demonstrate that the probe-to-spacecraft potential measured
by RPW on Solar Orbiter can be used to derive the plasma (electron) density measurement …

Solar wind is a highly turbulent medium exhibiting fluctuations ranging from the solar
sidereal rotation period to proton and electron gyroperiods. Their amplitudes show …

The understanding of inertial-scale dynamics in the heliosheath is not yet thorough.
Magnetic field fluctuations across the inner heliosheath (IHS) and the local interstellar …

The transfer of energy from large to small scales in solar wind turbulence is an important
ingredient of the long-standing question of the mechanism of the interplanetary plasma …

During the lifetime of the Cluster mission, the inter‐spacecraft distances in the solar wind
have changed from the large, fluid, scales (∼ 104 km), down to the scales of protons (∼ 102 …

The properties of inertial-and kinetic-range solar wind turbulence have been investigated
with the arbitrary-order Hilbert spectral analysis method, applied to high-resolution density …