HOMARD-Code_Saturne : Computational Fluid Dynamics |
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The first 3D test is run with the FATHER case. It simulates the thermal
evolution after a junction between two pipes
No error indicator is available in Code_Saturne for that modelisation; so a
physical field is chosen to indicate the cells to split. For this case, the
eddy energy seems to be suitable to follow the stream. |
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| CPU time/CPUstep | ||
| Sequence #1 | 116 480 hexas | 41.3s |
| 1st adaptation | 5.6s | |
| Sequence #2 | 117544 hexas | 46.0s |
| 2nd adaptation | 1.7s | |
| Sequence #3 | 120790 hexas | 40.7s |
| 3rd adaptation | 1.8s | |
| Sequence #4 | 129374 hexas | 43.8s |
| 3th adaptation | 1.9s | |
| Sequence #5 | 131054 hexas | 44.6s |
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