k
, epsilon
, omega
fields into the SpalartAllmaras
turbulence closure model, so that various utilities can be enabled with this model if necessary, e.g. turbulenceFields
function object.SpalartAllmaras
model.N/A
\mathrm{Re}_\tau = 180
.No known risks or user-input changes.
PS: Hi @vaggelisp, might affect or be relevant? just for your info in any case.