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

The complex interaction between shocks and plasma turbulence is extremely important to
address crucial features of energy conversion in a broad range of astrophysical systems. We …

The physical foundations of the dissipation of energy and the associated heating in weakly
collisional plasmas are poorly understood. Here, we compare and contrast several …

We perform a statistical study of the turbulent power spectrum at inertial and kinetic scales
observed during the first perihelion encounter of the Parker Solar Probe. We find that often …

The statistics of intermittent ocean turbulence is the key link between physical understanding
of turbulence and its global implications. The log-normal distribution is the standard but …

We present estimates of the turbulent energy-cascade rate derived from a Hall-
magnetohydrodynamic (MHD) third-order law. We compute the contribution from the Hall …

Abstract Recent Parker Solar Probe (PSP) observations of inner heliospheric plasma have
shown an abundant presence of Alfvénic polarity reversal of the magnetic field, known as" …

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 …

Abstract The Parker Solar Probe mission has shown the ubiquitous presence of strong
magnetic field deflections, namely switchbacks, during its first perihelion where it was …