MacCormack's explicit time-marching scheme is used to solve the full Navier±Stokes unsteady, compressible equations for internal ¯ows. The requirement of a very ®ne grid to capture shock as well as separated ¯ows is circumvented by employing grid clustering. The numerical scheme is applied for axisy
Numerical modelling of two-dimensional and axisymmetric gravity currents
✍ Scribed by M. D. Patterson; J. E. Simpson; S. B. Dalziel; N. Nikiforakis
- Publisher
- John Wiley and Sons
- Year
- 2005
- Tongue
- English
- Weight
- 129 KB
- Volume
- 47
- Category
- Article
- ISSN
- 0271-2091
- DOI
- 10.1002/fld.841
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✦ Synopsis
Abstract
A series of two‐dimensional (2D), axisymmetric and three‐dimensional (3D) numerical flow simulations using an implicit large Eddy simulation (ILES) are carried out for gravity‐driven fluid flows. The results are compared directly with experiments undertaken to test the model. Two‐dimensional results show that the Large Eddy algorithm is successful in modelling a gravity current's large scale structure. Examination of the 3D results shows that macroscopic features of the flow (the lobe and cleft instability) observed at the interface between the light and dense fluid are also modelled well. Copyright © 2005 John Wiley & Sons, Ltd.
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