Magnetohydrodynamic (MHD) Turbulence is of critical importance for many problems and sub-fields of astrophysics. This includes star formation, the dynamics of the interstellar medium, cosmic ray physics, galaxy evolution, and heat transport in galaxy clusters.

 

The purpose of the CATS database is to foster increased collaboration between different groups working on simulations of astrophysical turbulence and to provide open source simulation resources to the broader community of researchers interested in turbulence.