The density distribution and physical origins of intermittency in supersonic, highly magnetized turbulence with diverse modes of driving
The mass density distribution function of supersonic turbulence is approximately lognormal. Here we review some of the most popular nonlognormal models.
Dec 1, 2022
Magnetized compressible turbulence with a fluctuation dynamo and Reynolds numbers over a million
The results from the world's largest MHD turbulence simulation are on the arXiv -- everything from cascades, scale-dependent alignment, to anisotropy and plasmoid instabilities.
Oct 1, 2022