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被动差分吸收光谱法测量气体浓度时Ring效应的影响及修正研究
引用本文:张英华,谢品华,司福祺,彭夫敏,窦科,李素文.被动差分吸收光谱法测量气体浓度时Ring效应的影响及修正研究[J].光谱学与光谱分析,2009,29(2).
作者姓名:张英华  谢品华  司福祺  彭夫敏  窦科  李素文
作者单位:中国科学院环境光学与技术重点实验室,中国科学院安徽光学精密机械研究所,安徽,合肥,230031
基金项目:国家高技术研究发展计划(863计划) 
摘    要:基于散射光、利用痕量气体指纹吸收特性反演气体浓度的方法称为被动差分吸收光谱法(passive DDAS).因其具体结构简单,易于平台搭载等优点近年来获得了长足发展.被动DOAS中利用太阳散射光作为光源解析大气污染气体柱浓度时,会受到太阳弗朗和费光谱的"填充线"即Ring效应的强烈影响,尤其是对浓度很低的痕量气体,致使不易获取其浓度、影响其测量精度.文章以反演大气中NO2气体为例,介绍了稳定天气条件下Ring效应造成的影响、分析了Ring效应影响与太阳天顶角的关系,提出了根据不同太阳天顶角选取不同Ring光谱参与拟合的修正方法,并且利用该处理方法反演了在3天稳定天气条件下不同仰角下的斜柱浓度.实验证明该修正方法的可行性.

关 键 词:散射光  痕量气体  Ring效应  被动差分吸收  太阳天顶角

Ring Effect and Correction Studies while Retrieving Trace Gas Concentration with Passive DOAS
ZHANG Ying-hua,XIE Pin-hua,SI Fu-qi,PENG Fu-min,DOU Ke,LI Su-wen Key Laboratory of Environmental Optical & Technology,Anhui Institute of Optics & Fine Mechanics,Chinese Academy of Sciences,Hefei ,China.Ring Effect and Correction Studies while Retrieving Trace Gas Concentration with Passive DOAS[J].Spectroscopy and Spectral Analysis,2009,29(2).
Authors:ZHANG Ying-hua  XIE Pin-hua  SI Fu-qi  PENG Fu-min  DOU Ke  LI Su-wen Key Laboratory of Environmental Optical & Technology  Anhui Institute of Optics & Fine Mechanics  Chinese Academy of Sciences  Hefei  China
Institution:ZHANG Ying-hua,XIE Pin-hua,SI Fu-qi,PENG Fu-min,DOU Ke,LI Su-wen Key Laboratory of Environmental Optical & Technology,Anhui Institute of Optics & Fine Mechanics,Chinese Academy of Sciences,Hefei 230031,China
Abstract:The method of retrieving the concentration of trace gases using of the diagnostic absorption of trace gases based on the scattered sunlight is called passive DOAS.It has been developed so fast in recent years because it remains simple and is prone to being combined with different platform.While retrieving the column density of trace gases with the scattered sunlight as light source,it will be affected strongly by solar Fraunhofer lines,which is also called Ring effect.It makes it hard to retrieve trace gase...
Keywords:Scattering light  Trace gases  Ring effect  Passive DOAS  Solar zenith angle  
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