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利用振动拉曼激光雷达进行平流层温度监测。第1部分:气溶胶和臭氧干扰。

Stratospheric temperature monitoring using a vibrational Raman lidar. Part 1: aerosols and ozone interferences.

作者信息

Faduilhe Denis, Keckhut Philippe, Bencherif Hassan, Robert Laurent, Baldy Serge

机构信息

Laboratoire de Physique de l'Atmosphère, Centre National de la Recherche Scientifique, Université de La Réunion, 15 Avenue René Cassin, 97715 Saint-Denis Messag Cedex 9, La Réunion, France.

出版信息

J Environ Monit. 2005 Apr;7(4):357-64. doi: 10.1039/b415299a. Epub 2005 Feb 23.

Abstract

Lidar measurements of temperature for the upper troposphere and lower stratosphere are commonly derived by the Raman technique. Lidar signals derived from vibrational Raman processes have been subjected to numerous simulation tests to examine their sensitivity to the presence of aerosols and ozone in the atmosphere. The influence of aerosols characteristics (wavelength dependence of aerosol extinction and particle phase function) and of ozone concentration on Raman temperature profiles is estimated. Simulations indicate large temperature deviations for post-volcanic conditions. For a Raman backscatter at 607 nm, bias is below 1 K for a total optical depth less than 9 x 10(-3) in the case of a stratospheric contamination and less than 6 x 10(-3) for a tropospheric contamination. The effect of aerosols depends on phase function and a few parameters such as altitude, optical depth and the shape of the high-altitude cloud. The wavelength dependence of aerosol extinction has some influence only for severe post-volcanic conditions (Scattering Ratio, SR >2). For a Raman backscatter at 387 nm, bias is larger and can be significant even in background aerosol conditions. Changes in the ozone density profile lead to significant Raman temperature deviations only for some specific conditions. Results suggest that both aerosol and ozone corrections are necessary to obtain an accuracy better than the 1 K requested for most atmospheric applications.

摘要

对流层上部和平流层下部温度的激光雷达测量通常采用拉曼技术。源自振动拉曼过程的激光雷达信号已经历了大量模拟测试,以检验它们对大气中气溶胶和臭氧存在的敏感度。估算了气溶胶特性(气溶胶消光的波长依赖性和粒子相函数)以及臭氧浓度对拉曼温度廓线的影响。模拟结果表明,火山喷发后的情况下存在较大的温度偏差。对于607 nm处的拉曼后向散射,在平流层污染情况下,当总光学厚度小于9×10⁻³时偏差低于1 K,在对流层污染情况下偏差低于6×10⁻³。气溶胶的影响取决于相函数以及一些参数,如高度、光学厚度和高海拔云的形状。气溶胶消光的波长依赖性仅在严重的火山喷发后情况下(散射比,SR>2)有一定影响。对于387 nm处的拉曼后向散射,偏差更大,甚至在背景气溶胶条件下也可能很显著。臭氧密度廓线的变化仅在某些特定条件下会导致显著的拉曼温度偏差。结果表明,为了获得优于大多数大气应用所要求的1 K的精度,气溶胶和臭氧校正都是必要的。

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