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首页> 外文期刊>Journal of Fluid Mechanics >Noise generation mechanisms for a supersonic jet impinging on an inclined plate
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Noise generation mechanisms for a supersonic jet impinging on an inclined plate

机译:超声速射流撞击斜板的噪声产生机理

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Noise generation mechanisms for a perfectly expanded supersonic Mach number M=1.8 turbulent jet impinging on a 45 inclined plate are investigated for a Reynolds number of 1.6 x 10(6) employing a large-eddy simulation. Excellent comparisons with experimental acoustic far-field measurements and pressure measurements on the impingement plate are obtained. Two local maxima are identified in the far-field overall sound pressure levels in the 75 degrees and 120 degrees observer directions, which arc associated with different noise generation mechanisms. The peak frequencies in the spectra with Strouhal numbers of St = 0.2 for 75 degrees and St = 0.5 for 120 degrees match the experimental measurements. The jet-impingement region generates pressure waves that propagate predominantly in the 120 degrees observer direction, The noise generation in this region is attributed to vortex stretching and tearing during shear-layer impingement, and shock oscillations that are induced by the motion of downstream convected vortical flow structures. The second peak in the overall sound pressure distribution at 75 degrees is associated with noise sources located in the wall jet. The noise generation in the wall jet is associated with supersonically convecting large-scale coherent flow structures that also interact with tail shocks in the wall jet causing large localized pressure fluctuations. Strongly coherent flow structures are identified by applying proper orthogonal decomposition (POD) to the unsteady flow field. The frequency characteristics of the most energetic POD modes are distinctly different based on which energy norm is chosen. The most energetic entropy-based POD modes contain a peak frequency of approximately St = 0.4-0.6, while the most energetic turbulent kinetic-energy-based POD modes appear to be dominated by lower-frequency content. The causality method, based on Lighthill's acoustic analogy, is used to link the acoustic noise signature to the relevant physical mechanisms in the source region. A differentiation is made between the application of normalized and non-normalized cross-correlation functions for noise source identification and characterization.
机译:利用大涡模拟研究了雷诺数为1.6 x 10(6)的完美扩展超声速马赫数M = 1.8湍流射流撞击45斜板上的噪声产生机理。获得了与实验声远场测量值和冲击板上压力测量值的出色比较。在75度和120度观察者方向的远场总体声压级中确定了两个局部最大值,这与不同的噪声生成机制相关。 Strouhal数在75度时St = 0.2,在120度时St = 0.5的频谱中的峰值频率与实验测量值匹配。射流冲击区产生的压力波主要沿观察者方向120度传播。在该区域产生的噪声归因于剪切层冲击过程中的涡旋拉伸和撕裂,以及下游对流涡旋运动引起的激波振荡。流结构。整体声压分布在75度处的第二个峰值与位于壁流中的噪声源相关。壁射流中产生的噪声与超声对流的大型相干流动结构有关,这些结构也与壁射流中的尾部冲击相互作用,从而引起较大的局部压力波动。通过对非恒定流场应用适当的正交分解(POD),可以确定强相干的流动结构。根据选择哪种能量范数,最有活力的POD模式的频率特性明显不同。基于能量最高的基于熵的POD模式包含大约St = 0.4-0.6的峰值频率,而基于能量最高的基于动能的POD模式似乎以较低的频率含量为主。基于Lighthill声学比喻的因果关系方法用于将声学噪声信号链接到源区域中的相关物理机制。在归一化和非归一化互相关函数的应用之间进行区分,以进行噪声源识别和表征。

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