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超声速湍流边界层气动光学的实验研究

Experimental investigation on aero-optics of supersonic turbulent boundary layers.

作者信息

Ding Haolin, Yi Shihe, Zhu Yangzhu, He Lin

出版信息

Appl Opt. 2017 Sep 20;56(27):7604-7610. doi: 10.1364/AO.56.007604.

DOI:10.1364/AO.56.007604
PMID:29047740
Abstract

Nanoparticle-based planar laser scattering was used to measure the density distribution of the supersonic (Ma=3.0) turbulent boundary layer and the optical path difference (OPD), which is quite crucial for aero-optics study. Results were obtained using ray tracing. The influences of different layers in the boundary layer, turbulence scales, and light incident angle on aero-optics were examined, and the underlying flow physics were analyzed. The inner layer plays a dominant role, followed by the outer layer. One hundred OPD of the outer layer at different times satisfy the normal distribution better than that of the inner layer. Aero-optics induced by the outer layer is sensitive to the filter scale. When induced by the inner layer, it is not sensitive to the filter scale. The vortices with scales less than the Kolmogorov scale (=46.0  μm) have little influence on the aero-optics and could be ignored; the validity of the smallest optically active scale (=88.1  μm) proposed by Mani is verified, and vortices with scales less than that are ignored, resulting in a 1.62% decay of aero-optics; the filter with a width of 16-grid spacing (=182.4  μm) decreases OPD by 7.04%. With the increase of the angle between the wall-normal direction and the light-incident direction, the aero-optics becomes more serious, and the difference between the distribution of the OPD and the normal distribution increases. The difficulty of aero-optics correction is increased. Light tilted toward downstream experiences more distortions than when tilted toward upstream at the same angle relative to the wall-normal direction.

摘要

基于纳米颗粒的平面激光散射被用于测量马赫数为3.0的超声速湍流边界层的密度分布以及光程差(OPD),这对气动光学研究至关重要。结果通过光线追踪获得。研究了边界层中不同层、湍流尺度和光入射角对气动光学的影响,并分析了潜在的流动物理机制。内层起主导作用,其次是外层。外层在不同时刻的100个光程差比内层更符合正态分布。外层引起的气动光学对滤波尺度敏感。当由内层引起时,它对滤波尺度不敏感。尺度小于科尔莫戈罗夫尺度(=46.0μm)的涡对气动光学影响很小,可以忽略;验证了马尼提出的最小光学活性尺度(=88.1μm)的有效性,忽略尺度小于该值的涡,导致气动光学衰减1.62%;宽度为16网格间距(=182.4μm)的滤波器使光程差降低7.04%。随着壁面法向与光入射方向夹角的增大,气动光学变得更严重,光程差分布与正态分布的差异增大。气动光学校正的难度增加。相对于壁面法向方向以相同角度向下游倾斜的光比向上游倾斜时经历更多的畸变。

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