Troubleshooting LES

The following troubleshooting quantities allow you to analyze the results of large eddy simulations:

Subgrid Kinetic Energy

The subgrid scale turbulent kinetic energy kSGS (Eqn. (1497)) is a physical by-product of the Simcenter STAR-CCM+ flow. LES always uses a subgrid scale model—Smagorinsky or WALE—which in turn directly computes turbulent viscosity. Within this computation is an implicit level of subgrid kinetic energy.

You may need to post-process the SGS Turbulent Kinetic Energy field function in certain kinds of Simcenter STAR-CCM+ cases. For example, in Lagrangian simulations that include turbulent dispersion, subgrid kinetic energy is contained in turbulent fluctuations that the calculation has not taken into account. Therefore this field function can provide an approximate analysis of these unresolved fluctuations.

The values for subgrid kinetic energy are affected by the Ct parameter in the Smagorinsky expert properties or WALE expert properties.

Smagorinsky Subgrid Scale Wall Damping Function

The Smagorinsky subgrid scale model can give inaccurate scaling at walls, so the Van Driest damping function fv (Eqn. (1389)) modifies the length scale closer to the wall. Visualizing this factor as a field function (SGS Wall Damping Factor) allows you to see the extent of the domain that is affected by this damping function.