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Linear stability of Poiseuille flow over a steady spanwise Stokes layer
KTH, Skolan för teknikvetenskap (SCI), Teknisk mekanik, Strömningsmekanik och Teknisk Akustik. Department of Aerospace Sciences and Technologies, Politecnico di Milano, via La Masa 34 20156 Milano, Italy.ORCID-id: 0000-0002-6712-8944
Laboratoire d'Hydrodynamique (LadHyX), CNRS-École Polytecnique, F-91128 Palaiseau, France.
Department of Mechanical Engineering, PSE Division, KAUST, 23955 Thuwal, Saudi Arabia.
Department of Aerospace Sciences and Technologies, Politecnico di Milano, via La Masa 34 20156 Milano, Italy.
2023 (engelsk)Inngår i: Physical Review Fluids, E-ISSN 2469-990X, Vol. 8, nr 10, artikkel-id 103902Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

The temporal linear stability of plane Poiseuille flow modified by spanwise forcing applied at the walls is considered. The forcing consists of a stationary streamwise distribution of spanwise velocity that generates a steady transversal Stokes layer, known to reduce skin-friction drag in a turbulent flow with little energetic cost. A large numerical study is carried out, where the effects of both the physical and the discretization parameters are thoroughly explored, for three representative subcritical values of the Reynolds number Re. Results show that the spanwise Stokes layer significantly affects the linear stability of the system. For example, at Re=2000 the wall forcing is found to more than double the negative real part of the least-stable eigenvalue, and to decrease by nearly a factor of 4 the maximum transient growth of perturbation energy. These observations are Re dependent and further improve at higher Re. Comments on the physical implications of the obtained results are provided, suggesting that spanwise forcing might be effective to obtain at the same time a delayed transition to turbulence and a reduced turbulent friction.

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American Physical Society (APS) , 2023. Vol. 8, nr 10, artikkel-id 103902
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URN: urn:nbn:se:kth:diva-339034DOI: 10.1103/PhysRevFluids.8.103902ISI: 001137926500002Scopus ID: 2-s2.0-85174798522OAI: oai:DiVA.org:kth-339034DiVA, id: diva2:1815528
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QC 20240301

Tilgjengelig fra: 2023-11-29 Laget: 2023-11-29 Sist oppdatert: 2025-02-09bibliografisk kontrollert

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