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Spatial and temporal characterization of phase fluctuations in non-Kolmogorov atmospheric turbulence

机译:非Kolmogorov大气湍流中相位波动的时空特征

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摘要

Atmospheric turbulence severely limits the performance of ground-based imaging and laser propagation systems. Some observational results, showing atmospheric turbulence which does not obey Kolmogorov's theory, have prompted the study of optical propagation through non-Kolmogorov turbulence. This paper presents a theoretical approach to analyse the spatial and temporal characterizations of phase fluctuations in non-Kolmogorov turbulence. The spatial structure function, the temporal structure function and the temporal power spectrum of phase fluctuations are derived. The generalized coherence length rho(0), the characteristic frequency f(R) and the characteristic time tau(R) are expressed as functions of the index structure constant along the propagation path and the wind velocity. The long exposure MTF, the short exposure MTF and the imaging Strehl ratio are computed. [References: 24]
机译:大气湍流严重限制了地面成像和激光传播系统的性能。一些观测结果表明大气湍流不符合Kolmogorov的理论,这促使人们研究通过非Kolmogorov湍流的光学传播。本文提出了一种理论方法来分析非Kolmogorov湍流中相位波动的时空特征。推导了相位波动的空间结构函数,时间结构函数和时间功率谱。广义相干长度rho(0),特征频率f(R)和特征时间tau(R)表示为沿传播路径和风速恒定的索引结构的函数。计算长曝光MTF,短曝光MTF和成像斯特列尔比。 [参考:24]

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