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Computational Study of Roughness-Induced Boundary-Layer Noise

机译:粗糙度引起的边界层噪声的计算研究

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As a first step toward predicting rough-wall boundary-layer noise, the sound radiated from a single hemispherical roughness element and a pair of roughness elements in a turbulent boundary layer at Re_θ = 7500 is investigated. The roughness height is 3.6% of the boundary-layer thickness, or 95 wall units. The flowfield is obtained from large-eddy simulation, and the results are validated against experimental measurements. Acoustic calculations are performed based on the Curie-Powell integral solution to the Lighthill equation for an acoustically compact hemisphere. The sound radiation is dominated by unsteady drag dipoles and their images in the wall. It is found that the spanwise dipole, which has been overlooked in previous studies of roughness noise, is of larger or similar strength compared with the streamwise dipole, and the viscous contribution to the drag dipoles is negligible in comparison with the pressure contribution. Important flow features contributing to sound radiation are identified by examining the unsteady surface-pressure field and the surrounding flow structures. Pressure fluctuations are strongest on the upstream part of the hemispheric surface near the base due to impingement of incoming turbulent eddies and their interaction with horseshoe vortices. On the back surface of the hemisphere, pressure fluctuations are relatively weak, indicating that shear-layer separation and vortex shedding do not produce significant self-noise from the hemisphere. In the case with two hemispheres, the wake of the upstream hemisphere is found to significantly enhance sound radiation from the downstream hemisphere, particularly in the streamwise direction and at high frequencies.
机译:作为预测粗糙壁边界层噪声的第一步,研究了湍流边界层中Re_θ= 7500时从单个半球形粗糙度元素和一对粗糙度元素发出的声音。粗糙度高度为边界层厚度的3.6%,即95个壁单元。流场是从大涡流模拟获得的,并且针对实验测量结果进行了验证。声学计算是基于居里-鲍威尔(Light)方程的居里-鲍威尔(Curie-Powell)积分解,用于声学上紧凑的半球。声音的辐射主要由不稳定的偶极子及其在墙上的图像决定。发现在以前的粗糙度噪声研究中被忽略的翼展方向偶极子与流态偶极子相比具有更大或更相似的强度,并且与压力贡献相比,对阻力偶极子的粘性贡献可忽略不计。通过检查不稳定的表面压力场​​和周围的流动结构,可以确定有助于声辐射的重要流动特征。由于进入的湍流涡流的冲击及其与马蹄涡的相互作用,压力波动在靠近基座的半球表面的上游部分最强。在半球的背面,压力波动相对较弱,表明剪切层分离和涡旋脱落不会从半球产生明显的自噪声。在具有两个半球的情况下,发现上游半球的尾迹显着增强了来自下游半球的声音辐射,特别是沿流向和高频。

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