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Oscillations, Waves, and Interactions - GWDG

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94 D. Ronneberger et al.<br />

(wavenumber) x (pipe radius)<br />

12<br />

10<br />

8<br />

6<br />

4<br />

2<br />

0<br />

−2<br />

−4<br />

−6<br />

−8<br />

U<br />

U<br />

U<br />

0.6 0.8 1.0 1.2 1.4<br />

frequency [kHz]<br />

Figure 13. Dispersion relations of a m = 0 mode in a lined duct with dimensions according<br />

to Fig. 1. The flow velocity of the uniform compressible mean flow has been varied between<br />

0.1 ≤ U/c ≤ 0.3 in steps of 0.01. The real (green) <strong>and</strong> the imaginary (red) parts of the<br />

wavenumber are shown in the upper <strong>and</strong> the lower part of the Figure, respectively. The<br />

experimental data (colored, from Ref. [29]) <strong>and</strong> the corresponding theoretical values (black)<br />

refer to U/c = 0.17(+), 0.20(△), 0.23(◦), 0.25(⊓⊔). The (blue) circled cross <strong>and</strong> the dashed<br />

lines describe a bifurcation (see text).<br />

by circles which happen to appear at equivalent points of the dispersion relations,<br />

characterized e. g. by the maximum of ℜ{α}. Likewise it can only be speculated<br />

that the structure found in the theoretical dispersion relations at frequencies around<br />

1000 Hz might be related to the increase of the pressure drop that is achieved by the<br />

excitation of the antisymmetric mode at similar frequencies (see Fig. 12).<br />

The instability denoted by C in Fig. 10 <strong>and</strong> marked by the circles in Fig. 14 obviously<br />

does not rely on the compressibility of the air. The dynamics behind this<br />

instability is very similar to the Kelvin-Helmholtz instability which results from a<br />

balance of the accelerating forces that the fluid elements experience on both the<br />

sides of shear layers due to the unsteady deflection of the shear layer. In the present<br />

case the fluid flow in the interior of the duct behaves like an oscillating jet which<br />

forces the surrounding fluid in the cavities to oscillate in the azimuthal direction. So<br />

the accelerating forces are proportional to ˆη0 ω 2 in the cavities <strong>and</strong> proportional to<br />

ˆηU(ω − αU) 2 in the flow. The sum of these forces has to cancel out which yields<br />

α = (ω/U)(1 ∓ iκη) wherein κη = � ˆη0/ˆηU depends on the geometric details of the

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