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近地面大气光学湍流外尺度的实验研究
引用本文:王倩,梅海平,钱仙妹,饶瑞中.近地面大气光学湍流外尺度的实验研究[J].物理学报,2015,64(22):224216-224216.
作者姓名:王倩  梅海平  钱仙妹  饶瑞中
作者单位:1. 中国科学院安徽光学精密机械研究所大气光学中心, 中国科学院大气成分与光学重点实验室, 合肥 230031; 2. 中国科学院大学, 北京 100084
基金项目:国家自然科学基金(批准号: 41205010)资助的课题.
摘    要:分析了含有外尺度的Von-Karman湍流空间相关函数模型, 并利用光纤湍流空间传感阵列的实测数据, 根据拟合算法获得了大气光学湍流空间外尺度的值及日变化, 对模型的适用性进行了实验验证. 将空间相关函数理论与空间多点同步测量的数据相结合, 尽可能清晰地展现了几种适合用相关函数描述的湍涡尺度. 结果表明, 在1.8 m的草地上, 大气光学湍流的外尺度呈现出白天较大、夜间较小的日变化趋势, 正午前后均值约为0.44 m, 夜间约为0.3 m. 有三点需要说明: 其一, 当两点间距恰好等于外尺度时, 其空间相关系数为0.26, 当两点间距超过外尺度之后, 仍具有一定的相关性; 其二, 积分尺度代表了湍涡尺度的平均值, 该值略小于外尺度; 其三, 湍涡的最大尺度所对应的湍流空间相关性为0, 其值略大于外尺度. 不难发现: 湍涡三种尺度的日变化与湍流强度的日变化趋势非常相似. 以空间布点探测的方法获取湍流特征尺度, 结果直观, 而且能够直接验证湍流空间相关函数模型, 所以可在一定程度上促进湍流空间结构特性的研究.

关 键 词:大气光学湍流  空间相关函数  外尺度
收稿时间:2015-05-13

Experimental investigation of the outer scale in atmospheric optical turbulence near the ground
Wang Qian,Mei Hai-Ping,Qian Xian-Mei,Rao Rui-Zhong.Experimental investigation of the outer scale in atmospheric optical turbulence near the ground[J].Acta Physica Sinica,2015,64(22):224216-224216.
Authors:Wang Qian  Mei Hai-Ping  Qian Xian-Mei  Rao Rui-Zhong
Institution:1. Key Laboratory of Atmospheric Composition and Optical Radiation, Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, China; 2. University of Chinese Academy of Sciences, Beijing 100084, China
Abstract:In this article, the Von-Karman model of turbulence spatial correlation function which contains the parameter of outer scale is analyzed. Then, the experimental data of air refractive index variation obtained from a high quality fiber optical turbulence sensing array are used to evaluate the outer scale of atmospheric optical turbulence as well as its diurnal variation through the algorithm of nonlinear fitting. The results validate the suitability of the Von-Karman model. By combining the theory of correlation function with the spatially distributed and simultaneously measured data, three kinds of turbulence spatial scales described by correlation function are revealed as clearly as possible. Results show that the values of outer scale in atmospheric optical turbulence 1.8 m above the grassland tend to be larger in the daytime and smaller in the night. The mean value around noon is 0.44 m, while in the night it becomes 0.3 m. Here, three of the important views should be noted. Firstly, when the displacement of two points is just equal to the outer scale, their correlation coefficient is 0.26, and when it exceeds the outer scale, there is still a certain value of correlation coefficient. Secondly, the integral scale represents the averaged value of scale in the vortex of optical turbulence. And, it is slightly smaller than the outer scale. Thirdly, when the distance of two points equals the biggest scale of vortex in optical turbulence, the correlation coefficient tends to zero, and the value of biggest scale is slightly bigger than the outer scale. It is easy to find that the diurnal variation tendencies of the three spatial scales are similar to that of intensity in optical turbulence. The method of obtaining the characteristic scales by spatially arranged and simultaneously measured optical turbulence is direct, and the results can be considered as the evidence to prove the models of correlation function including the Von-Karman model. So, it promotes the research on the property of spatial structure to a certain extent.
Keywords:atmospheric optical turbulence  spatial correlation function  outer scale
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