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兴隆大气湍流气球探测
引用本文:吴晓庆,曾宗泳,马成胜,翁宁泉,肖黎明.兴隆大气湍流气球探测[J].量子电子学报,1996(4).
作者姓名:吴晓庆  曾宗泳  马成胜  翁宁泉  肖黎明
作者单位:中国科学院安徽光学精密机械研究所
基金项目:国家高技术863-308资助
摘    要:本文分析了1994年12月15~22日河北兴隆折射率结构常数气球探测的主要结果。表明:兴隆冬季观测的湍流比昆明强,相干长度rO平均为6.4cm。不仅低层湍流较强,而且对流层顶附近有一较强湍流层。夜间垂直分布廓线可以用Hufnayel-Valley模式来拟合。

关 键 词:光学湍流,高度分布,模式

Observations of Atmospheric Turbulence by Balloon-borne Instrument at Xinlong Station
Wu Xiaoqing,Zeng Zongyong,Ma Chengsheng,Weng Ningquan,Xiao Liming.Observations of Atmospheric Turbulence by Balloon-borne Instrument at Xinlong Station[J].Chinese Journal of Quantum Electronics,1996(4).
Authors:Wu Xiaoqing  Zeng Zongyong  Ma Chengsheng  Weng Ningquan  Xiao Liming
Abstract:Main observational results of the structure coefficient of the atmospheric refractive index C: are given. They were obtained by a balloon-borne instrument at Xinlong Station, Hebei province from December 15 to 22,1994. It shows that the turbulence at Xinlong Station is stronger than Kunming's. The average value of coherence length is 6.4 cm. Not only is there a strong turbulence within the boundary layer, but also in the tropopause region. The night-time data may be fitted by Hufnagel-Valley model.
Keywords:optical turbulence  vertical distribution  model
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