Full 3D correlation tensor computed from double field stereoscopic PIV in a high Reynolds number turbulent boundary layer

The turbulence structure near a wall is a very active subject of research and a key to the understanding and modeling of this flow. Many researchers have worked on this subject since the fifties Hama et al. (J Appl Phys 28:388–394, 1957 ). One way to study this organization consists of computing the...

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Bibliographic Details
Published inExperiments in fluids Vol. 50; no. 4; pp. 839 - 846
Main Authors Foucaut, Jean-Marc, Coudert, Sebastien, Stanislas, Michel, Delville, Joel
Format Journal Article Conference Proceeding
LanguageEnglish
Published Berlin/Heidelberg Springer-Verlag 01.04.2011
Springer
Springer Verlag (Germany)
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Summary:The turbulence structure near a wall is a very active subject of research and a key to the understanding and modeling of this flow. Many researchers have worked on this subject since the fifties Hama et al. (J Appl Phys 28:388–394, 1957 ). One way to study this organization consists of computing the spatial two-point correlations. Stanislas et al. (C R Acad Sci Paris 327(2b):55–61, 1999 ) and Kahler (Exp Fluids 36:114–130, 2004 ) showed that double spatial correlations can be computed from stereoscopic particle image velocimetry (SPIV) fields and can lead to a better understanding of the turbulent flow organization. The limitation is that the correlation is only computed in the PIV plane. The idea of the present paper is to propose a new method based on a specific stereoscopic PIV experiment that allows the computation of the full 3D spatial correlation tensor. The results obtained are validated by comparison with 2D computation from SPIV. They are in very good agreement with the results of Ganapthisubramani et al. (J Fluid Mech 524:57–80, 2005a ).
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ISSN:0723-4864
1432-1114
DOI:10.1007/s00348-010-0928-7