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 …

We review the range of applications and use of the curlometer, initially developed to analyze
Cluster multi‐spacecraft magnetic field data; but more recently adapted to other arrays of …

The dissipative mechanism in weakly collisional plasma is a topic that pervades decades of
studies without a consensus solution. We compare several energy dissipation estimates …

Heliospheric plasma turbulence plays a key role in transferring the energy of large‐scale
magnetic field and plasma flow fluctuations to smaller scales where the energy can be …

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 …

The first computations of the compressible energy transfer rate from∼ 0.2 up to∼ 1.7 au is
obtained using Parker Solar Probe (PSP), Time History of Events and Macroscale …

For the first time, Parker Solar Probe (PSP) observed the sub-Alfvénic solar wind where the
solar wind bulk speed drops below the local Alfvén speed for an extended period of time …

The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is
studied in combination with the remote-sensing observation of the coronal source region …

This Letter reports the first observational estimate of the heating rate in the slowly expanding
solar corona. The analysis exploits the simultaneous remote and local observations of the …

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" …