Standard calculation in Code_Saturne involves incompressible or dilatable flows, but not compressible ones. To be more precise, we solve (in the standard module) the following mass conservation equation:[code:1]div(rho.u) = 0[/code:1]
In your case, you have to use the compressible module, activated by usppmo.
David<br /><br />Post edited by: David Monfort, at: 2010/03/27 22:23