Miranda is a radiation hydrodynamics code designed for large-eddy simulation of multicomponent flows with turbulent mixing. Additional physics packages include magneto-hydrodynamics, self-gravity and thermonuclear fusion. The hydro package is based on tenth-order compact (Pade) schemes for spatial differencing, combined with fourth-order Runge-Kutta timestepping. Applications to date include interfacial instabilities (RT, RM, and KH), ICF implosions, ablation physics, supernovae, the LIFE chamber, and classical fluids experiments (e.g., drop tanks, shock tubes, etc.).
Please contact Andy Cook if you have questions or comments.