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FLOW AROUND A CYLINDER - istiarto

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– 4.41 –<br />

Wall function for the � equation. The turbulent kinetic-energy dissipation for cells<br />

neighboring the wall is defined by Eq. 4.84. This can be easily implemented as follows:<br />

� set all coefficients related to the neighboring cells to zero:<br />

a E � a W � a N � a S � a T � a B � 0<br />

� set the coefficient at cell P to unity: aP = 1<br />

� set the source terms by (see Eq. 4.84):<br />

c m�1 �<br />

b � �P �<br />

� �<br />

3 4 m�1<br />

kP<br />

� � n,P<br />

3 2<br />

m�1<br />

where kP is already computed in the previous step<br />

(4.93)<br />

Wall function and pressure correction. Since the discharge across the wall is zero, the<br />

p<br />

coefficient of the boundary node B in Eq. 4.68 is set to zero: aB � 0 . The pressure<br />

correction at the boundary node is obtained by direct extrapolation from the cell center P:<br />

c c<br />

pB � pP .<br />

4.5.5 Symmetry boundary<br />

At the symmetry plane, for example at the east face (see Fig. 4.9), the convective<br />

transport across the plane and the shear stress along the plane are zero. These properties<br />

make the velocity at E be easily obtained from the projection of the velocity at P to the<br />

plane. For the scalar variables, k and �, an approximation is used by extrapolating the<br />

values at P to the boundary E. The following expressions thus apply at symmetry<br />

boundaries:<br />

Fig. 4.9 Symmetry boundary.

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