Numerical Simulations

Scale-dependent alignment in compressible magnetohydrodynamic turbulence
Scale-dependent alignment in compressible magnetohydrodynamic turbulence

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 spectrum of magnetized turbulence in the interstellar medium
The spectrum of magnetized turbulence in the interstellar medium

The energy spectrum and key turbulence statistics from ISM-style turbulence.

May 16, 2025

Comparison of magnetic diffusion and reconnection in ideal and resistive relativistic magnetohydrodynamics, ideal magnetodynamics and resistive force-free electrodynamics
Comparison of magnetic diffusion and reconnection in ideal and resistive relativistic magnetohydrodynamics, ideal magnetodynamics and resistive force-free electrodynamics

Relativistic reconnection is very similar across a broad range of plasma models!

Mar 25, 2025

Fundamental MHD scales -- II: the kinematic phase of the supersonic small-scale dynamo
Fundamental MHD scales -- II: the kinematic phase of the supersonic small-scale dynamo

The supersonic turbulent dynamo, relevant to the cold ISM and thin accretion disks, is very different from the incompressible Kazanstev theory.

Jan 31, 2025

Magnetized compressible turbulence with a fluctuation dynamo and Reynolds numbers over a million
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.

May 29, 2024

Growth or Decay - I: universality of the turbulent dynamo saturation
Growth or Decay - I: universality of the turbulent dynamo saturation

The saturation of the turbulent dynamo is universal to the initial seed magnetic field!

Sep 1, 2023

The density distribution and physical origins of intermittency in supersonic, highly magnetized turbulence with diverse modes of driving
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

Energy balance and Alfvén Mach numbers in compressible magnetohydrodynamic turbulence with a large-scale magnetic field

Oct 1, 2022

Fundamental scales in the kinematic phase of the turbulent dynamo

Jul 1, 2022