Numerical simulation of orbitally shaken viscous fluids with free surface
SUMMARY Orbitally shaken bioreactors are an emerging alternative to stirred‐tank bioreactors for large‐scale mammalian cell culture, but their fluid dynamics is still not well defined. Among the theoretical and practical issues that remain to be resolved, the characterization of the liquid free surf...
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Published in: | International journal for numerical methods in fluids Vol. 71; no. 3; pp. 294 - 315 |
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Main Authors: | , , , , , |
Format: | Journal Article Publication |
Language: | English |
Published: |
Chichester, UK
John Wiley & Sons, Ltd
30-01-2013
Wiley Subscription Services, Inc |
Subjects: | |
Online Access: | Get full text |
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Summary: | SUMMARY
Orbitally shaken bioreactors are an emerging alternative to stirred‐tank bioreactors for large‐scale mammalian cell culture, but their fluid dynamics is still not well defined. Among the theoretical and practical issues that remain to be resolved, the characterization of the liquid free surface during orbital shaking remains a major challenge because it is an essential aspect of gas transfer and mixing in these reactors. To simulate the fluid behavior and the free surface shape, we developed a numerical method based on the finite element framework. We found that the large density ratio between the liquid and the gas phases induced unphysical results for the free surface shape. We therefore devised a new pressure correction scheme to deal with large density ratios.
The simulations operated with this new scheme gave values of wave amplitude similar to the ones measured experimentally. These simulations were used to calculate the shear stress and to study the mixing principle in orbitally shaken bioreactors. Copyright © 2012 John Wiley & Sons, Ltd.
Orbitally shaken bioreactors are an emerging alternative to stirred‐tank bioreactors for large‐scale mammalian cell culture, but their fluid dynamics is still not well‐defined. Among the theoretical and practical issues that remain to be resolved, the characterization of the liquid free surface during orbital shaking remains a major challenge because it is an essential aspect of gas transfer and mixing in these reactors. |
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Bibliography: | ArticleID:FLD3658 istex:8A6C2B3E3F75848A85DC14D7A83E81C9B9A38CD1 ark:/67375/WNG-ZGD51RR2-1 ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0271-2091 1097-0363 |
DOI: | 10.1002/fld.3658 |