William H. Matthaeus

TL;DR: This paper shows that both of these effects of a non-Galilean invariance caused by a density-dependent coefficient in the convection term can be eliminated exactly in a lattice Boltzmann-equation model.

TL;DR: In this paper, the authors measured the total energy, cross helicity, and magnetic helicity of the solar wind at 1, 2.8, and 5 AU, and found that the magnetic heliometry typically lies at scales larger than the magnetic correlation length, consistent with the expectations of the inverse cascade and selective decay hypotheses of three-dimensional MHD turbulence theory.

TL;DR: In this paper, the development of anisotropy in an initially isotropic spectrum is studied numerically for two-dimensional magnetohydrodynamic turbulence, due to the combined effects of an externally imposed dc magnetic field and viscous and resistive dissipation at high wave numbers.

TL;DR: In this paper, the authors examined wind observations of inertial and dissipation range spectra in an attempt to better understand the processes that form the dissipation ranges and how these processes depend on the ambient solar wind parameters (interplanetary magnetic field intensity, ambient proton density and temperature, etc.).

TL;DR: In this article, the authors proposed a model of the solar wind as a fluid which contains both classical transverse Alfvenic fluctuations and a population of quasi-transverse fluctuations.