When discussing research in physics and in science more generally, it is common to ascribe
equal importance to the three components of the scientific trinity: theoretical, experimental …

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 first radial alignment between Parker Solar Probe and Solar Orbiter spacecraft is used
to investigate the evolution of solar wind turbulence in the inner heliosphere. Assuming …

Abstract The Parker Solar Probe (PSP) entered a region of sub-Alfvénic solar wind during
encounter 8, and we present the first detailed analysis of low-frequency turbulence …

A primary goal of the Parker Solar Probe (PSP) Mission is to answer the outstanding
question of how the solar corona plasma is heated to the high temperatures needed for the …

The 2D+ slab superposition model of solar wind turbulence has its theoretical foundations in
nearly incompressible magnetohydrodynamics (NI MHD) in the plasma beta∼ 1 or≪ 1 …

One of the most important early results from the Parker Solar Probe (PSP) is the ubiquitous
presence of magnetic switchbacks, whose origin is under debate. Using a three-dimensional …

We propose a turbulence-driven solar wind model for a fast solar wind flow in an open
coronal hole where the solar wind flow and the magnetic field are highly aligned. We …

Abstract Parker Solar Probe (PSP) observed a large variety of Alfvénic fluctuations in the fast
and slow solar wind flow during its two perihelia. The properties of Alfvénic solar wind …

Small-amplitude fluctuations in the magnetized solar wind are measured typically by a
single spacecraft. In the magnetohydrodynamics (MHD) description, fluctuations are typically …