The theory of nearly incompressible magnetohydrodynamics (NI MHD) was developed
largely in the early 1990s, together with an important extension to inhomogeneous flows in …

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

ABSTRACT A three-dimensional magnetohydrodynamic (MHD) model for the propagation
and dissipation of Alfvén waves in a coronal loop is developed. The model includes the …

We derive a weak turbulence formalism for incompressible magnetohydrodynamics. Three-
wave interactions lead to a system of kinetic equations for the spectral densities of energy …

An emerging paradigm for the dissipation of magnetic turbulence in the supersonic solar
wind is via localized small-scale reconnection processes, essentially between quasi-2D …

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 …

We analyze three-dimensional numerical simulations of driven incompressible
magnetohydrodynamic (MHD) turbulence in a periodic box threaded by a moderately strong …

Context. A large-scale magnetic field permeates our Galaxy and is involved in a variety of
astrophysical processes, such as star formation and cosmic ray propagation. Dust …

Context. The magnetic field strength in interstellar clouds can be estimated indirectly from
measurements of dust polarization by assuming that turbulent kinetic energy is comparable …