# M-Star Solve

M-Star CFD uses direct numerical simulations (DNS) for laminar and transitional systems, and large eddy simulations (LES) for turbulent systems. The robustness of these time-accurate approaches eliminates the ambiguity associated with traditional turbulence models. It captures transient flow patterns that cannot be resolved using time-averaged CFD, and correctly predicts the effects of scale-up on flow dynamics.

Simulations can be executed on Windows or Linux environment, across arbitrary numbers of CPUs and compute nodes.