Turbulence

Most fluid flows of engineering interest are characterized by irregularly fluctuating flow quantities.

Often these fluctuations are at such small scales and high frequencies that resolving them in time and space comes at excessive computational costs. Instead of solving for the exact governing equations of turbulent flows (Direct Numerical Simulation), it is less expensive to solve for averaged or filtered quantities and approximate the impact of the small fluctuating structures. Turbulence models provide different approaches for modeling these structures.

The turbulence models that are implemented in Simcenter STAR-CCM+ can be subdivided into two categories:

  • Models that provide closure of the Reynolds-Averaged Navier-Stokes (RANS) equations.
  • Scale-resolving simulations that solve for large scales of turbulence and model small-scale motions. These are Large Eddy Simulation (LES) and Detached Eddy Simulation (DES).

Most simulations will rely on the first approach. The second approach (LES and DES) is best used after carefully reviewing the applicable literature to gain confidence that the grid resolution requirements can be met and that the computational costs incurred by resolving the small time and length scales are indeed justified.

It is generally recognised that all existing turbulence models are approximate representations of the physical phenomena of turbulence. The degree of approximation in a given model depends on the nature of the flow to which it is applied. The characterization of the circumstances which give rise to 'good' and 'bad' performance must be based mainly on experience.