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Structure of a turbulent boundary layer studied by DNS
KTH, School of Engineering Sciences (SCI), Mechanics. KTH, School of Engineering Sciences (SCI), Centres, Linné Flow Center, FLOW.ORCID iD: 0000-0001-9627-5903
KTH, School of Engineering Sciences (SCI), Mechanics. KTH, School of Engineering Sciences (SCI), Centres, Linné Flow Center, FLOW.
KTH, School of Engineering Sciences (SCI), Mechanics. KTH, School of Engineering Sciences (SCI), Centres, Linné Flow Center, FLOW.ORCID iD: 0000-0002-9819-2906
KTH, School of Engineering Sciences (SCI), Mechanics. KTH, School of Engineering Sciences (SCI), Centres, Linné Flow Center, FLOW.ORCID iD: 0000-0002-2711-4687
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2011 (English)In: Direct and Large-Eddy Simulation VIII, 2011, 9-14 p.Conference paper, Published paper (Refereed)
Abstract [en]

Turbulent boundary layers constitute one of the basic building blocks for understanding turbulence, particularly relevant for industrial applications. Although the geometries in technical but also geophysical applications are complicated and usually feature curved surfaces, the flow case of a canonical boundary layer developing on a flat surface has emerged as an important setup for studying wall turbulence, both via experimental and numerical studies. However, only recently spatially developing turbulent boundary layers have become accessible via direct numerical simulations (DNS). The difficulties of such setups are mainly related to the specification of proper inflow conditions, the triggering of turbulence and a careful control of the free-stream pressure gradient. In addition, the numerical cost of such spatial simulations is high due to the long, wide and high domains necessary for the full development of all relevant turbulent scales. We consider a canonical turbulent boundary layer under zero-pressure-gradient via large-scale DNS. The boundary layer is allowed to develop and grow in space. The inflow is a laminar Blasius boundary layer, in which laminar-turbulent transition is triggered by a random volume force shortly downstream of the inflow. This trip force, similar to a disturbance strip in an experiment (Schlatter and Örlü, 2010; Schlatter et al., 2009), is located at a low Reynolds number to allow the flow to develop over a long distance. The simulation covers thus a long, wide and high domain starting at Re θ =180 extending up to the (numerically high) value of Re θ =4300, based on momentum thickness θ and free-stream velocity U ∞. Fully turbulent flow is obtained from Re θ ≈500. The numerical resolution for the fully spectral numerical method (Chevalier et al., 2007) is in the wall-parallel directions Δx +=9 and Δz +=4, resolving the relevant scales of motion. The simulation domain requires a total of 8⋅109 grid points in physical space, and was thus run massively parallel with 4096 processors.

Place, publisher, year, edition, pages
2011. 9-14 p.
Series
ERCOFTAC Series, 15
National Category
Fluid Mechanics and Acoustics
Identifiers
URN: urn:nbn:se:kth:diva-86852DOI: 10.1007/978-94-007-2482-2_2ISI: 000323091800002Scopus ID: 2-s2.0-84964844899OAI: oai:DiVA.org:kth-86852DiVA: diva2:501082
Conference
Direct and Large-Eddy Simulation 8, Eindhoven - The Netherlands, July 7-9 2010
Note

QC 20120411

Available from: 2012-02-13 Created: 2012-02-13 Last updated: 2013-12-19Bibliographically approved

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Schlatter, PhilippBrethouwer, GeertJohansson, Arne V.Henningson, Dan S.

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Schlatter, PhilippLi, QiangBrethouwer, GeertJohansson, Arne V.Henningson, Dan S.
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