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Direct numerical simulations of intrusive density- and particle-driven gravity currents

Francisco, E. P.; Espath, L. F.R.; Laizet, S.; Silvestrini, J. H.; Calo, V. M.

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Authors

E. P. Francisco

LUIS ESPATH LUIS.ESPATH@NOTTINGHAM.AC.UK
Assistant Professor

S. Laizet

J. H. Silvestrini

V. M. Calo



Abstract

In the present study, mesopycnal flows are investigated using direct numerical simulations. In particular, intrusive density- and particle-driven gravity currents in the lock exchange setup are simulated with the high-order finite-difference framework Xcompact3d. To account for the settling velocity of particles, a customized Fick's law for the particle-solution species is used with an additional term incorporating a constant settling velocity proportional to the concentration of particles. A general energy budget equation is presented, for which the energy can migrate across the domain's boundaries. The relevant main features of intrusive gravity currents, such as front velocity, energy exchanges, sedimentation rate, deposit profile, and deposit map are discussed with the comparison between two- and three-dimensional simulations. In particular, the influence of the Grashof number, the interface thickness, the energy exchanges, the sedimentation process, and how the presence of more than one particle fraction may change the flow dynamics are investigated. The results are in good agreement with previous experiments and theoretical work, in particular for the prediction of the front velocity. For the particle-driven case, the suspended mass evolution along with the sedimentation rate suggests the occurrence of three different stages. In the first stage after the lock release, the particle mixture tends to suspend itself due to gravitational forces. Once most of the particle-mixture mass is suspended, the current intrudes while increasing its velocity, reaching its kinetic energy peak. In the last stage, the particles are deposited at a nearly constant sedimentation rate. As a result, the front velocity constantly decelerates.

Citation

Francisco, E. P., Espath, L. F., Laizet, S., Silvestrini, J. H., & Calo, V. M. (2022). Direct numerical simulations of intrusive density- and particle-driven gravity currents. Physics of Fluids, 34(4), Article 045116. https://doi.org/10.1063/5.0087595

Journal Article Type Article
Acceptance Date Mar 27, 2022
Online Publication Date Apr 13, 2022
Publication Date Apr 1, 2022
Deposit Date May 18, 2022
Publicly Available Date May 18, 2022
Journal Physics of Fluids
Print ISSN 1070-6631
Electronic ISSN 1089-7666
Publisher American Institute of Physics
Peer Reviewed Peer Reviewed
Volume 34
Issue 4
Article Number 045116
DOI https://doi.org/10.1063/5.0087595
Public URL https://nottingham-repository.worktribe.com/output/7955254
Publisher URL https://aip.scitation.org/doi/abs/10.1063/5.0087595
Additional Information This article may be downloaded for personal use only. Any other use requires prior permission of the author and AIP Publishing. This article appeared inE. P. Francisco, L. F. R. Espath, S. Laizet, J. H. Silvestrini, and V. M. Calo , "Direct numerical simulations of intrusive density- and particle-driven gravity currents", Physics of Fluids 34, 045116 (2022) https://doi.org/10.1063/5.0087595 and may be found at https://aip.scitation.org/doi/10.1063/5.0087595

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