2010
DOI: 10.1016/j.jsv.2010.04.010
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Low-wavenumber turbulent boundary layer wall-pressure measurements from vibration data on a cylinder in pipe flow

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Cited by 38 publications
(26 citation statements)
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“…The squared magnitude of the spatial Fourier transform of the mode shape function of a structure is usually called the wavenumber sensitivity function or wavenumber filter shape function, and is often used to calculate the coupling between exciting pressure fields and mode shapes for rectangular panels [1][2][3][4] and cylinders, 5,6 both under fluctuating wall pressure excitations. It can be also used to calculate the radiation efficiency of rectangular panels in the wavenumber domain.…”
Section: Introductionmentioning
confidence: 99%
“…The squared magnitude of the spatial Fourier transform of the mode shape function of a structure is usually called the wavenumber sensitivity function or wavenumber filter shape function, and is often used to calculate the coupling between exciting pressure fields and mode shapes for rectangular panels [1][2][3][4] and cylinders, 5,6 both under fluctuating wall pressure excitations. It can be also used to calculate the radiation efficiency of rectangular panels in the wavenumber domain.…”
Section: Introductionmentioning
confidence: 99%
“…The conditioned spectral density noise removal technique is illustrated using data obtained by Bonness, Capone, and Hambric [4]. They measured cylinder vibrations and TBL dynamic wall pressures from a thin-walled 0.15 m diameter aluminum cylinder internally filled with water (pipe-flow) flowing at 6.1 m/s.…”
Section: Measured Datamentioning
confidence: 99%
“…The parameters characterizing the turbulent boundary layer are supposed to be known: U  is the flow velocity, c U , the convection velocity, δ is the boundary layer thickness, and w  the wall shear stress. From these parameters and the wall pressure models proposed in the literature [2][3][4][5], we can define the spectrum of the wall pressure fluctuations acting on the plate. The auto spectrum density of the wall pressure   pp S  is evaluated here considering Goody's model [8] whereas the normalised cross spectrum density is evaluated using the Corcos's model [2].…”
Section: Presentation Of the Problemmentioning
confidence: 99%
“…2 -The spectrum of the wall pressure fluctuations is evaluated from the TBL parameters estimated in the previous step and by using one of the models proposed in the literature. Some of them are expressed in the space -frequency domain (like the famous Corcos model [1]) whereas as others are expressed in the wavenumber -frequency domain (like the no less famous Chase model [2]); Discussion about different models and comparison with experiment can be found in [3,4] for the frequency auto spectrum and in [5,6] for the normalized wavenumber cross spectrum;…”
Section: Introductionmentioning
confidence: 99%