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Expressions for the spherical-wave-structure function based on a bump spectrum model for the index of refraction

机译:基于凹凸光谱模型的折射率的球面波结构函数的表达式

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Abstract: New spectra models have recently been developed for the spatial power spectra of temperature and refractive index fluctuations in the atmospheric boundary layer showing the characteristic 'bump' just prior to the dissipation ranges. Theoretical work involving these new models has led to new expressions for the phase structure function associated with a plane optical wave, although most experimental work has involved spherical waves. Following techniques similar to those used for the plane wave analysis, new expressions valid in geometrical and diffraction regimes are developed here for the phase structure function of a spherical optical wave propagating through clear-air atmospheric turbulence. Useful asymptotic formulas for small separation distances and the inertial subrange are derived from these general expressions.!
机译:摘要:最近开发了新的光谱模型,用于大气边界层中温度和折射率波动的空间功率谱,显示出在耗散范围之前的特征“凸点”。尽管大多数实验工作都涉及球面波,但涉及这些新模型的理论工作已导致与平面光波相关的相结构函数的新表达式。遵循类似于平面波分析的技术,此处开发了在几何和衍射形式下有效的新表达式,用于通过晴空大气湍流传播的球形光波的相结构功能。从这些一般表达式可以得出有用的渐近公式,用于较小的分离距离和惯性子范围。

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