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Sound propagation through and scattering by internal gravity waves in a stably stratified atmosphere

机译:声音在稳定的分层气氛中通过内部重力波传播和散射

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摘要

A stably stratified atmosphere supports propagation of internal gravity waves (IGW). These waves result in highly anisotropic fluctuations in temperature and wind velocity that are stretched in a horizontal direction. As a result, IGW can significantly affect propagation of sound waves in nighttime boundary layers and infrasound waves in the stratosphere. In this paper, a theory of sound propagation through, and scattering by, IGW is developed. First, 3D spectra of temperature and wind velocity fluctuations due to IGW, which were recently derived in the literature for the case of large wave numbers, are generalized to account for small wave numbers. The generalized 3D spectra are then used to calculate the sound scattering cross section in an atmosphere with IGW. The dependencies of the obtained scattering cross section on the sound frequency, scattering angle, and other parameters of the problem are qualitatively different from those for the case of sound scattering by isotropic turbulence with the von Karman spectra of temperature and wind velocity fluctuations. Furthermore, the generalized 3D spectra are used to calculate the mean sound field and the transverse coherence function of a plane sound wave propagating through IGW. The results obtained also significantly differ from those for the case of sound propagation through isotropic turbulence. (c) 2005 Acoustical Society of America.
机译:稳定的分层大气支持内部重力波(IGW)的传播。这些波导致温度和风速在水平方向上高度各向异性的波动。结果,IGW可以显着影响声波在夜间边界层中的传播以及平流层中的次声波。本文提出了一种通过IGW传播和通过IGW传播声音的理论。首先,归因于IGW的温度和风速波动的3D光谱(最近在文献中针对大波数的情况得出)被概括为考虑小波数。然后将广义的3D频谱用于计算具有IGW的大气中的声音散射截面。所获得的散射横截面对问题的声频,散射角度和其他参数的依赖性与质量随温度和风速波动的冯·卡曼光谱通过各向同性湍流进行散射的情况在质量上有所不同。此外,广义的3D频谱用于计算通过IGW传播的平面声波的平均声场和横向相干函数。获得的结果也与通过各向同性湍流传播声音的结果显着不同。 (c)2005年美国声学学会。

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