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 …

Turbulent magnetic reconnection is believed to occur in astrophysical plasmas, and it has
been suggested to be a trigger of solar flares. It often occurs in long stretched and …

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 …

High time-resolution solar wind magnetic field data are employed to study statistics
describing intermittency near the first perihelion (∼ 35.6 R⊙) of the Parker Solar Probe …

Abstract Parker Solar Probe (PSP) and SolO data are utilized to investigate magnetic field
intermittency in the solar wind (SW). Small-scale intermittency (20− 100 di) is observed to …