next up previous contents
Next: 2D-case Up: ISNaS - incompressible flow Previous: 3D-case

Space discretization of the continuity and momentum equations

  In this section we describe the space discretization of the continuity and momentum equations in the inner region. Discretizations due to the boundary conditions are treated in Section 7.

The equations describing the mean velocity field in incompressible turbulent flow follow from the momentum equations by the Reynolds decomposition of the instantaneous velocity field into a mean and a fluctuating part. The momentum equations in general co-ordinates read (see [34], formula 5.2)

 

with the deviatoric stress tensor given by

 

Here, is the contravariant mean velocity, the density, p the mean pressure, some external force per unit volume, dynamic viscosity and the turbulent stress tensor ( denotes contravariant velocity fluctuation), which has to be specified. This specification is accomplished by a two-equation eddy-viscosity turbulence model. This will be presented in Section 6. When calculating laminar flows, the turbulent stresses are set to zero.
In the present version all coefficients may depend on space, time and previous computed solutions. However, with respect to the density a correct implementation is only guaranteed for is constant. Furthermore, the discretization presented below has been carried out as if the flow is assumed laminar.
The continuity equation reads (see [34], formula 5.1):

 

As unknowns the fluxes are used.
Equations (4.1), (4.2) and (4.3) are discretized by a finite volume method.
We distinguish between the 2D and the 3D case.




Tatiana Tijanova
Wed Mar 26 10:36:42 MET 1997