大气与环境光学学报 ›› 2025, Vol. 20 ›› Issue (6): 703-712.doi: 10.3969/j.issn.1673-6141.2025.06.002

• 大气光学 • 上一篇    

成都地区大气光学湍流廓线估算方法比较

张梦 1, 倪长健 1,2*   

  1. 1 成都信息工程大学大气科学学院, 四川 成都 610225; 2 成都平原城市气象与环境四川省野外科学观测研究站, 四川 成都 610225
  • 收稿日期:2023-06-01 修回日期:2023-07-12 出版日期:2025-11-28 发布日期:2025-11-24
  • 通讯作者: E-mail: ncj@cuit.edu.cn E-mail:ncj1970@163.com
  • 作者简介:张梦 (1998- ), 女, 硕士研究生, 主要从事大气环境与大气光学方面的研究。E-mail: Zhangmeng_0705@163.com
  • 基金资助:
    国家重点研发计划项目 (2018YFC0214004, 2018YFC1506006) , 四川省科技厅应用基础研发项目 (2021YJ0314)

Comparison of methods for estimating atmospheric optical turbulence profiles in Chengdu

ZHANG Meng 1, NI Changjian 1,2*   

  1. 1 College of Atmospheric Science, Chengdu University of Information Technology, Chengdu 610225, China; 2 Chengdu Plain Urban Meteorology and Environment Observation and Research Station of Sichuan Province, Chengdu 610225, China
  • Received:2023-06-01 Revised:2023-07-12 Online:2025-11-28 Published:2025-11-24

摘要: 大气光学湍流廓线是大气光学湍流强度垂直分布形态的表征, 也是环境空气质量演化的重要指示因子。本 文基于成都市温江区2020 年2 月的雷达探空资料, 分别利用Coulman外尺度模型、Thorpe 尺度方法和Hufnagel-Vally 5/ 7 模式估算了该地区对流层中下层 (< 5 km) 的大气光学湍流廓线,探讨了不同大气光学湍流廓线估算方法的适用性。 结果表明: (1) 利用Coulman 外尺度模式估算的大气光学湍流廓线与L波段风廓线雷达实测的大气光学湍流廓线基本 一致, 二者的相关系数为0.70; (2) Thorpe 尺度的估算结果与实测结果的相关系数为0.60, 二者在4 km高度以下呈现 出较好的一致性, 量级偏差主要出现在4~5 km高度区; (3) Hufnagel-Vally 5/7 模式的估算结果未能准确地反映实际大 气光学湍流廓线的变化特征, 其相关系数为0.15。总之, 基于Tatarski 参数化方法的Coulman 外尺度模型在该地区取 得了最优的估算结果, 为成都及其他下垫面相似区域的大气光学湍流廓线的估算提供了方法支撑。

关键词: 大气光学, 光学湍流, 风廓线雷达, 估算方法, 成都地区

Abstract: The atmospheric optical turbulence profile is not only a representation of the vertical distribution of atmospheric optical turbulence intensity, but also an important indicator of the evolution of ambient air quality. Based on the radar sounding data of Wenjiang District, Chengdu City, China, in February 2020, the atmospheric optical turbulence profiles in the middle and lower troposphere (< 5 km) are estimated in this work by using Coulman outer scale model, Thorpe scale method and Hufnagel-Vally 5/7 model respectively, and the applicability of the different methods for estimating atmospheric optical turbulence profiles is discussed. The results show that: (1) The atmospheric optical turbulence profile estimated by Coulman outer scale model is basically consistent with that measured by L-band wind profiler radar, with a correlation coefficient of 0.70. (2) The correlation coefficient between the estimated results of Thorpe scale method and the measured results is 0.60, and the two results show good consistency below 4 km height, and the magnitude deviation in the 4–5 km height range. (3) The estimated results of Hufnagel-Vally 5/7 model can not accurately reflect the changing characteristics of the real atmospheric optical turbulence profile, with a correlation coefficient of 0.15. In summary, the Coulman outer-scale model based on Tatarski parameterization method has achieved the optimal estimation results in the district, which provides a methodological support for the estimation of atmospheric optical turbulence profiles in Chengdu and other regions with similar underlying surface.

Key words: atmospheric optical turbulence profile, wind profile radar, estimation method, optimization; Chengdu region

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