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The Aggregate Behavior of Branch Points . - Branch Point Density as a Characteristic of an Atmospheric Turbulence Simulator

机译:分支点的聚集行为。 -支点密度是大气湍流模拟器的特征

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The Atmospheric Turbulence Simulator used in testing in the Atmospheric Simulation and Adaptive-optic Laboratory Test-bed at Air Force Research Laboratory, Directed Energy Directorate's Starfire Optical Range is configured based on three characteristics; Fried's parameter, r_0, the Rytov number, σ_X~2, and the Greenwood Frequency, f_G. All three may be estimated from open loop data as a means of verifying the simulated turbulence conditions for a given test configuration. However, unlike r_0 and f_G, the Rytov number isn't directly calculated. Instead the scintillation index is estimated from intensity measurements. At low Rytov values, (< 0.3 - 0.4), this measurement can approximate the Rytov number, however beyond a Rytov of 0.4 this parameter becomes saturated. Branch Points begin to appear after the Rytov value exceeds 0.1. In this work the behavior of the branch point density is examined to determine its viability as another parameter for calibration our turbulence simulator.
机译:空军研究实验室的大气模拟和自适应光学实验室测试台中用于测试的大气湍流模拟器是根据以下三个特征配置的,定向能源局的星火光学范围是:弗里德的参数r_0,Rytov数σ_X〜2和格林伍德频率f_G。可以从开环数据估计所有这三个,作为验证给定测试配置的模拟湍流条件的一种方法。但是,与r_0和f_G不同,Rytov数不是直接计算的。而是根据强度测量值来估算闪烁指数。在低Rytov值(<0.3-0.4)时,此测量值可以近似Rytov数,但是超过Rytov 0.4时,此参数变得饱和。 Rytov值超过0.1后,分支点开始出现。在这项工作中,将检查分支点密度的行为,以确定其可行性,作为校准湍流模拟器的另一个参数。

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