The tangential velocity and normal stress are prescribed at the boundary, i.e.:
From equation (7.7) it is clear that we can calculate and as and are zero, otherwise we have to make an assumption about and . In the remainder of this section we assume that
at the boundary.
From and equation (7.22) follows the stress
at the boundary in the computational domain.
Boundary condition (7.45) influences the two ''tangential''
velocity cells (see Figure 7.5) and the ''normal'' velocity
half-cell (see Figure 7.6).
The and ''tangential'' cells (bottom boundary) are built in
a similar way as the inner cells. The only difference is that virtual
velocity components and pressures are eliminated by linear extrapolation.
For example for the bottom boundary we get:
The normal velocity half-cell at the bottom boundary. The discretization of the convective term gives
Terms with the factor are the only terms where we need a
linearization procedure, since and are given at the
boundary.
We use the following discretization of the stress tensor:
where is given by . So
the right-hand side gets the contribution:
The virtual velocities introduced by formula (7.51) are eliminated
by linear extrapolation. Just as in 2D is the pressure evaluated in the
points (1,0,1), (-1,0,1), (0,1,1) and (0,-1,1) instead of (1,0,0),
(-1,0,0), (0,1,0) and (0,-1,0).