Abstract Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …

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 …

This paper presents a theoretical framework for understanding plasma turbulence in
astrophysical plasmas. It is motivated by observations of electromagnetic and density …

The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere - IOPscience This
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …

We consider ion heating by turbulent Alfvén waves (AWs) and kinetic Alfvén waves (KAWs)
with wavelengths (measured perpendicular to the magnetic field) that are comparable to the …

This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …

We develop a one-dimensional solar-wind model that includes separate energy equations
for the electrons and protons, proton temperature anisotropy, collisional and collisionless …

Wavelet analysis can be used to measure the power spectrum of solar-wind fluctuations
along a line in any direction (θ, ϕ) with respect to the local mean magnetic field B 0. This …

Radio observations discovered large-scale non-thermal sources in the central Mpc regions
of dynamically disturbed galaxy clusters (radio haloes). The morphological and spectral …

The zeroth law of turbulence states that, for fixed energy input into large-scale motions, the
statistical steady state of a turbulent system is independent of microphysical dissipation …