Scale-dependent alignment is how turbulence connects to reconnection. We show that the nature of scale-dependent alignment in compressible turbulence differs from well-established incompressible theory.
May 22, 2025
The energy spectrum and key turbulence statistics from ISM-style turbulence.
May 16, 2025
Relativistic reconnection is very similar across a broad range of plasma models!
Mar 25, 2025
The supersonic turbulent dynamo, relevant to the cold ISM and thin accretion disks, is very different from the incompressible Kazanstev theory.
Jan 31, 2025
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.
May 29, 2024
The saturation of the turbulent dynamo is universal to the initial seed magnetic field!
Sep 1, 2023
The mass density distribution function of supersonic turbulence is approximately lognormal. Here we review some of the most popular nonlognormal models.
Dec 1, 2022
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
Oct 1, 2022
Jul 1, 2022