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The computation of turbulent natural convection flows - Turbulence ...

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Numerical Implementation 132<br />

<strong>The</strong> matrix coefficient that links the near wall node and the wall is set to zero.<br />

Regarding the non-wall boundary condition, three types <strong>of</strong> boundary con-<br />

ditions are employed in the study. Two <strong>of</strong> them are inlet and outlet boundaries<br />

across which the fluid is entrained into the <strong>computation</strong>al domain and exits it<br />

respectively. <strong>The</strong> other boundaries employed in the present work are treated<br />

as symmetry boundaries. At this type <strong>of</strong> boundary, the fluid neither enters to<br />

the domain nor exits.<br />

A fixed constant temperature is set for the inlet boundary condition and<br />

zero gradient condition is imposed for the rest <strong>of</strong> the variables. Zero gradient<br />

conditions are also set for all variables at the outlet <strong>of</strong> the <strong>computation</strong>al do-<br />

main. For the symmetry boundaries, the component <strong>of</strong> velocity perpendicular<br />

to the boundary is set to zero and zero gradient conditions are imposed to the<br />

rest <strong>of</strong> the variables.<br />

5.8 Simulation <strong>of</strong> inclined cavity<br />

<strong>The</strong> most expedient way to simulate inclined cavity <strong>flows</strong> was to rotate the<br />

coordinate system and consequently the velocity components relative to the<br />

vertical, as shown in Figure 5.4. This means that the gravity vector now has<br />

components in both the x and y directions.<br />

x<br />

y<br />

ψ<br />

H<br />

Hot Wall<br />

g y<br />

g<br />

g x<br />

Cold Wall<br />

Figure 5.4 – Schematic <strong>of</strong> the inclined cavity.<br />

<strong>The</strong> components <strong>of</strong> gravity acceleration are:<br />

L

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