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Experimental characterization of the transition region in a rotating-disk boundary layer

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Experimental characterization of the transition region in a rotating-disk boundary layer

Muhammad Ehtisham Siddiqui, Benoît Pier, Julian F. Scott, Alexandre Azouzi, Roger Michelet

To cite this version:

Muhammad Ehtisham Siddiqui, Benoît Pier, Julian F. Scott, Alexandre Azouzi, Roger Michelet.

Experimental characterization of the transition region in a rotating-disk boundary layer. Seventh IUTAM Symposium on Laminar-Turbulent Transition, Jun 2009, Stockholm, Sweden. pp.573-576,

�10.1007/978-90-481-3723-7_103�. �hal-00633241�

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Experimental characterization of the transition region in a rotating-disk boundary layer

Muhammad Ehtisham SIDDIQUI, Benoˆıt PIER, Julian SCOTT, Alexandre AZOUZI, Roger MICHELET

Abstract A series of experiments were performed to study the transition from lami- nar to turbulent flow for the boundary layer over a rotating disk and to compare with theoretical results. The mean flow profile measured in the laminar region is found to be in excellent agreement with analytical results, and the spatial growth of natural disturbances matches linear theory predictions. A hot-wire sensor was positioned at different spatial locations to determine the evolution of natural disturbances. Spec- tral analysis at high resolution and ensemble-averages of velocity time series have been carried out to distinguish different flow regimes.

1 Introduction

The flow due to a rotating disk has been used as the canonical configuration for the study of 3D boundary layers [7]. It exhibits a self-similar exact solution [1]. The basic-flow solution displays a constant boundary layer thicknessδ=

pν/Ω, where νis the kinematic viscosity andΩthe disk rotation rate. Such boundary layers give rise to strong instabilities leading to the formation of cross-flow vortices, as already noticed experimentally by Gregory, Stuart and Walker [8].

Throughout this study, the axial coordinate Z and radial coordinate R are non- dimensionalized byδ. The rotating-disk flow is known to display a sharp transition from laminar to turbulent regimes at a nondimensional critical radius R≃510 [7, 3].

Lingwood [2] found this transition location to precisely coincide with onset of local absolute instability at Rca≃507. More recently, a fully nonlinear analysis [4] has revealed additional aspects of primary and secondary instabilities and has further contributed to the understanding of the complex flow dynamics prevailing near the transition region.

Muhammad Ehtisham SIDDIQUI (muhammad.siddiqui@ec-lyon.fr)

Laboratoire de m´ecanique des fluides et d’acoustique (CNRS – Universit´e de Lyon).

Ecole centrale de Lyon, 36 avenue Guy-de-Collongue; 69134 ´´ Ecully cedex, FRANCE.

1

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2 Authors Suppressed Due to Excessive Length

2 Experimental setup

The present rotating-disk facility consists of a glass disk, 500 mm in diameter, ro- tated at constant angular velocityΩ, up to 1500 rpm (see fig. 1). The maximum out-of-flatness was found to be less than 50 microns. The disk has constant angu- lar velocityΩ to within 0.05%. A high-precision two-axes traversing mechanism is used for hot-wire sensor positioning with radial and axial precisions of 20µm and 2µm respectively. The traversing mechanism and velocity measurements are controlled and recorded by a dedicated computer. A constant-temperature hot-wire anemometer is used for velocity measurements.

Fig. 1 Left: experimental setup consisting of a glass disk and a traversing mechanism, right: a close-up of the traversing mechanism for positioning the hot-wire probe.

3 Mean-velocity profiles

Circumferential mean-velocity profiles are measured at different radial locations.

Fig. 2 shows measurements (symbols) obtained atΩ =950 rpm, plotted together with the laminar similarity profile (solid line). Velocities are nondimensionalized by RδΩ. At the lower radii, R≤470, the measured velocity profiles are found to precisely follow the laminar profile (fig. 2a). For 490≤R≤530 (fig. 2b), the ve- locity profiles are significantly different from the theoretical profile for 1<Z<4, and≤10% flow correction is observed, but the flow is not yet fully turbulent. For R550 (fig. 2c), a strong mean flow correction extends up to Z=16, this boundary- layer thickening is characteristic of a fully turbulent regime.

4 Spectral analysis

Fourier spectra were calculated from the azimuthal velocity time series for different radii at Z=1,1.5,2,2.5,3,4 andΩ=950 rpm (fig. 3). At low radii R≤450, flat spectra are observed with uniform background noise level. For R470 and Z≤2.5,

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0 1 2 3 4 5 6 7 8

0 0.2 0.4 0.6 0.8 1

Z

V (a) Analytical

R = 350 R = 400 R = 410 R = 420 R = 430 R = 440 R = 450 R = 470

0 1 2 3 4 5 6 7 8

0 0.2 0.4 0.6 0.8 1

Z

V (b) Analytical

R = 490 R = 500 R = 510 R = 520 R = 530

0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16

0 0.2 0.4 0.6 0.8 1

Z

V (c)

Analytical R = 550 R = 560 R = 570 R = 590 R = 600

Fig. 2 Mean azimuthal velocity profiles at various radii, with=950 rpm. (a) Laminar flow regime. (b) Weakly nonlinear regime, mean-flow corrections in the region 1<Z<4. (c) Fully turbulent regime, strong mean-flow correction extends up to Z=16.

there is a band of amplified frequencies, with a maximum amplitude nearω/Ω 30. The harmonics of the fundamental frequency start to appear for R≥500, which is an indication that nonlinearities are developing. For R≥530, the harmonic peaks give way to fully developed spectra, characteristic of the turbulent regime. Further away from the disk surface, the weakly nonlinear regime is bypassed and a sudden transition from laminar to turbulent flows occurs (fig. 3c).

100 10000 1e+06 1e+08 1e+10 1e+12

0 150 300

P(ω)

ω/Ω (a)

600 570

550 530

520 470 500

’Z = 1.0’

100 10000 1e+06 1e+08 1e+10 1e+12

0 150 300

ω/Ω (b)

600 570

550 530

520 470 500

’Z = 2.0’

100 10000 1e+06 1e+08 1e+10 1e+12

0 150 300

ω/Ω (c)

600 570

550 530

520 500

’Z = 4.0’

Fig. 3 Fourier power spectra for time series with=950 rpm at Z=1,2,4 and 450R600

Fig. 4 represents high-resolution power spectra with dω/Ω=0.005, obtained by recording time series over very long time intervals. These high-resolution spectra display the features of fig. 3 superposed with a set of discrete narrow peaks, located at every integer multiple of the disk rotation rate. The discrete part of those spectra corresponds to components of the fluctuations that have the same periodicity as the disk and that are probably stationary with respect to the disk surface. These narrow

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4 Authors Suppressed Due to Excessive Length

100 1000 10000 100000 1e+06 1e+07 1e+08 1e+09 1e+10 1e+11 1e+12

0 150 300

P(ω)

ω/Ω (a)

100 1000 10000 100000 1e+06 1e+07 1e+08 1e+09 1e+10 1e+11 1e+12

25 26 27 28 29 30 31 32 33 34 35

P(ω)

ω/Ω (b)

100 1000 10000 100000 1e+06 1e+07 1e+08 1e+09 1e+10 1e+11 1e+12

25 26 27 28 29 30 31 32 33 34 35

P(ω)

ω/Ω (c) 600

470 450

Fig. 4 High resolution power spectra with=950 rpm at Z=2: (a) for R=500, (b) close-up, showing discrete spectral components. (c) for R = 450, 470, 500, 510, 520, 530, 550, 600.

frequency peaks are particularly visible at radial locations 500≤R≤550, where the low-resolution spectra display a weakly nonlinear harmonic regime. This discrete spectral component is not observed in the laminar boundary layer for R<470 and appears to be suppressed by the turbulent regime for R≥550.

5 Conclusions and outlook

In the present experimental study we have distinguished different flow regimes.

Mean azimuthal velocity measurements have been performed and were found to follow precisely the theoretical profile in the laminar flow regime. High-resolution spectra of azimuthal velocity time series, recorded over a long duration, are found to consist of continuous and discrete parts in which the discrete part of the spectra is made up of narrow peaks with the same periodicity as the disk. Work in progress consists in implementing a new control method [5, 6] to modify the naturally se- lected flow dynamics.

This research is financially supported by the Agence nationale de la recherche (ANR, project “Microsillon”).

References

1. T. von K´arm´an, Z. Angew. Math. Mech. 1, 232–252, 1921.

2. R. J. Lingwood, J. Fluid Mech. 299, 17–33, 1995.

3. R. J. Lingwood, J. Fluid Mech. 314, 373–405, 1996.

4. B. Pier, J. Fluid Mech. 487, 315–343, 2003.

5. B. Pier, J. Eng. Math. 57, 237–251, 2007.

6. B. Pier, Proc. R. Soc. Lond. A, 459, 1105–1115, 2003.

7. H. L. Reed and W. S. Saric, Annu. Rev. Fluid Mech. 21, 235–284, 1989.

8. N. Gregory, J. T. Stuart, W. S. Walker, Phil. Trans. R. Soc. Lond. A 248, 155–199, 1955.

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