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

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Annular horizontal penetration 392<br />

8.6 Time-dependent simulation (Ra = 3.1×10 13 )<br />

Figures 8.42-8.56 show the solution <strong>of</strong> 3D time dependent simulation <strong>of</strong><br />

the horizontal penetration test case at the higher Ra using the k-ε-AWF. In the<br />

steady-state simulation, it has been observed that results are not completely<br />

symmetrical, specially inside the tube away from the open end <strong>of</strong> the tube.<br />

That is why time dependent calculations have been carried out for this case, to<br />

reach a better understanding how flow develops in the horizontal penetration.<br />

In the time dependent calculations, the normalized time step is set equal<br />

to 0.19,normalized by D2<br />

V0 (where D2 is the diameter <strong>of</strong> the tube and V0 =<br />

√ gβ∆ΘD2) and the implicit scheme is employed for time descritisation. In<br />

each time step, it is set to iterate 20 times unless it gets to convergence criteria<br />

(all residuals below 10 −3 ).<br />

Figures 8.42-8.45 show the velocity contours within the central, X=0, longi-<br />

tudinal (y-z) plane. For the vertical, V, velocity component, Figure 8.43, as was<br />

also the case at the lower Ra number, Figure 8.18, the non-uniformity <strong>of</strong> the<br />

contours suggests the presence <strong>of</strong> large-scale flow structures, which change<br />

with time, both within and outside the penetration. It is difficult to detect a<br />

Rayleigh number effect from these comparisons. By contrast, the correspond-<br />

ing comparisons for the axial velocity, Figures 8.44 and 8.19, show that at the<br />

higher Ra the axial velocity field shows no signs <strong>of</strong> unsteadiness whereas at<br />

the lower Ra, the effects <strong>of</strong> large-scale unstable structures are clearly evident.<br />

This leads to the conclusion that at the higher Ra, the unstable flow structures<br />

are less influential.<br />

Figures 8.46-8.51 show contours <strong>of</strong> the vertical and axial velocities and <strong>of</strong><br />

the <strong>turbulent</strong> kinetic energy within a number <strong>of</strong> cross-sections inside the pene-<br />

tration, at Z=0.23, 0.46, 0.69 and 0.87 and at different times. <strong>The</strong> contours <strong>of</strong> the<br />

instantaneous vertical velocity, in common with those at the lower Rayleigh<br />

number <strong>of</strong> Figures 8.21 to 8.24, show flow oscillations within the penetration,<br />

but perhaps with smaller amplitude. While, also in common with the lower<br />

Ra behaviour, these oscillations considerably weaken at the exit, Z=0.87, they<br />

can still be detected, but confined to the region below the inner pipe.

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