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Estimating and measurement of atmospheric optical turbulence according to balloon-borne radiosonde for three sites in China

机译:估计和测量大气光学湍流,根据中国三个地点的气球传导无线电

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摘要

The distribution of optical turbulence (C-n(2) profiles) is the fundamental parameter closely related to the design and application of optoelectronic systems. Since systematic direct measurements of optical turbulence for many climates and seasons are not available, it is useful to estimate C-n(2) effectively from the routine meteorological parameters. The C-n(2) profiles are estimated by routine meteorological parameters based on the Tatarskii model, and the estimated results are compared with the corresponding radiosonde measurements from the field campaigns at Rongcheng (122.37 degrees E, 37.15 degrees N), Taizhou (121.42 degrees E, 28.62 degrees N), and Dachaidan (95.35 degrees E, 37.74 degrees N) in China. The agreement between the estimation model and the measurement is very close, except for a portion of the atmosphere where it showed considerable difference. Additionally, statistical operators are used to quantify the performance of the estimated model, and the statistical results also show that the estimated and measured C-n(2) profiles are consistent well. Furthermore, the integrated parameters (such as the Fried parameter, r(0)) from radiosonde measurement are 7.92 cm, 5.39 cm, and 3.68 cm at Rongcheng, Taizhou, and Dachaidan, respectively. Therefore, the C-n(2) profiles and their characteristics in these typical climate sites provide useful information to assess the effect of laser transmission in the atmosphere, which are usually used in the design of optoelectronic systems and astronomical site testing. (C) 2020 Optical Society of America
机译:光学湍流的分布(C-N(2)轮廓)是与光电系统的设计和应用密切相关的基本参数。由于许多气候和季节的光学湍流的系统直接测量不可用,因此有效地从常规气象参数估计C-N(2)。 CN(2)轮廓通过基于Tatarskii模型的常规气象参数估计,并且将估计的结果与荣成(122.37摄氏度,37.15度N),台州(121.42度E ,28.62度N)和Dachaidan(95.35摄氏度,37.74度N)。估计模型与测量之间的协议非常接近,除了它显示相当差异的大气层。此外,统计运营商用于量化估计模型的性能,统计结果还表明估计和测量的C-N(2)型材是一致的。此外,荣城,台州市和大阿达丹的综合参数(如炒参数,R(0))分别为7.92厘米,5.39厘米和3.68厘米。因此,C-N(2)型曲线及其在这些典型的气候站点中的特性提供了有用的信息,以评估激光传输在大气中的效果,这些效果通常用于光电系统和天文部位测试的设计。 (c)2020美国光学学会

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  • 作者单位

    Chinese Acad Sci Anhui Inst Opt &

    Fine Mech Key Lab Atmospher Opt Hefei 230031 Peoples R China;

    Chinese Acad Sci Anhui Inst Opt &

    Fine Mech Key Lab Atmospher Opt Hefei 230031 Peoples R China;

    Chinese Acad Sci Anhui Inst Opt &

    Fine Mech Key Lab Atmospher Opt Hefei 230031 Peoples R China;

    Chinese Acad Sci Anhui Inst Opt &

    Fine Mech Key Lab Atmospher Opt Hefei 230031 Peoples R China;

    Chinese Acad Sci Anhui Inst Opt &

    Fine Mech Key Lab Atmospher Opt Hefei 230031 Peoples R China;

    Chinese Acad Sci Anhui Inst Opt &

    Fine Mech Key Lab Atmospher Opt Hefei 230031 Peoples R China;

    Chinese Acad Sci Anhui Inst Opt &

    Fine Mech Key Lab Atmospher Opt Hefei 230031 Peoples R China;

    Chinese Acad Sci Anhui Inst Opt &

    Fine Mech Key Lab Atmospher Opt Hefei 230031 Peoples R China;

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  • 正文语种 eng
  • 中图分类 光学;
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