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Communication Dans Un Congrès Année : 2014

Spectral assessment of the turbulent convection velocity in a spatially developing flat plate turbulent boundary layer at Reynolds numbers up to Re θ = 13000

Résumé

A method inspired by del Alamo et al. [1] is derived to assess the wavelength-dependent convection velocity in a zero pressure gradient spatially developing flat plate turbulent boundary layer at Retheta = 13 000 for all wavelengths and all wall distances, using only estimates of the time power spectral density of the streamwise velocity and of its local spatial derivative. The resulting global convection velocity has a least-squares interpretation and is easily related to the wavelength-dependent convection velocity. The method intrinsically provides an estimation of the validity of Taylor’s hypothesis by a correlation coefficient identical to the one from [1]. The results reveal some similarities between the convection of the superstructures, the hairpin packets and the near-wall structures. The convection velocity of the superstructures is isolated by restricting the global convection velocity to the largest wavelengths. The spatial spectrum is estimated from the temporal spectrum using the frequency-dependent convection velocity. The results are consistent with a classical correlation-based evaluation.1. del Alamo, J.C., Jimenez, J.: Estimation of turbulent convection velocities and corrections to Taylor’s approximation. Journal of Fluid Mechanics 640, 5–26 (2009)
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Dates et versions

hal-01082881 , version 1 (14-11-2014)

Identifiants

  • HAL Id : hal-01082881 , version 1

Citer

N. Renard, S. Deck, P. Sagaut. Spectral assessment of the turbulent convection velocity in a spatially developing flat plate turbulent boundary layer at Reynolds numbers up to Re θ = 13000. Progress in Wall Turbulence : Understanding and Modelling, Jun 2014, LILLE, France. ⟨hal-01082881⟩
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