231 citations · 474 across the 8 of their papers we have counts for
4 papers · 1 filter
Turbulence and Vorticity in Galaxy Clusters Generated by Structure Formation
F. Vazza, T. W. Jones, M. Brüggen +4
Turbulence is a key ingredient for the evolution of the intracluster medium, whose properties can be predicted with high resolution numerical simulations. We present initial result…
Vorticity, Shocks and Magnetic Fields in Subsonic, ICM-like Turbulence
David H. Porter, T. W. Jones, Dongsu Ryu
We analyze high resolution simulations of compressible, MHD turbulence with properties resembling conditions in galaxy clusters. The flow is driven to turbulence Mach number $\math…
MHD Turbulence Simulation in a Cosmic Structure Context
T. W. Jones, D. H. Porter, D. Ryu +1
The gaseous media of galaxy clusters and cosmic filaments, which constitute most of the baryonic matter in the universe, is highly dynamic. It is also probably turbulent, although…
Cluster Turbulence: Simulation Insights
T. W. Jones, David H. Porter, Dongsu Ryu +1
Cluster media are dynamical, not static; observational evidence suggests they are turbulent. High-resolution simulations of the intracluster media (ICMs) and of idealized, similar…