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Effects of atmospheric light scattering on spectroscopic observations of greenhouse gases from space: Validation of PPDF-based CO_2 retrievals from GOSAT

机译:大气光散射对空间温室气体光谱观测的影响:验证GOSAT基于PPDF的CO_2检索

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摘要

This report describes a validation study of Greenhouse gases Observing Satellite (GOSAT) data processing using ground-based measurements of the Total Carbon Column Observing Network (TCCON) as reference data for column-averaged dry air mole fractions of atmospheric carbon dioxide (X_(CO_2)). We applied the photon path length probability density function method to validate X_(CO_2) retrievals from GOSAT data obtained during 22 months starting from June 2009. This method permitted direct evaluation of optical path modifications due to atmospheric light scattering that would have a negligible impact on ground-based TCCON measurements but could significantly affect gas retrievals when observing reflected sunlight from space. Our results reveal effects of optical path lengthening over Northern Hemispheric stations, essentially from May–September of each year, and of optical path shortening for sun-glint observations in tropical regions. These effects are supported by seasonal trends in aerosol optical depth derived from an offline three-dimensional aerosol transport model and by cirrus optical depth derived from space-based measurements of the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) instrument. Removal of observations that were highly contaminated by aerosol and cloud from the GOSAT data set resulted in acceptable agreement in the seasonal variability of XCO2 over each station as compared with TCCON measurements. Statistical comparisons between GOSAT and TCCON coincident measurements of CO_2 column abundance show a correlation coefficient of 0.85, standard deviation of 1.80 ppm, and a sub-ppm negative bias of −0.43 ppm for all TCCON stations. Global distributions of monthly mean retrieved X_(CO_2) with a spatial resolution of 2.5° latitude × 2.5° longitude show agreement within ∼2.5 ppm with those predicted by the atmospheric tracer transport model.
机译:本报告介绍了温室气体观测卫星(GOSAT)数据处理的验证研究,该实验使用地面上总碳柱观测网络(TCCON)的测量值作为大气中二氧化碳的柱平均干燥空气摩尔分数(X_(CO_2 ))。我们应用了光子路径长度概率密度函数方法来验证从2009年6月开始的22个月中获得的GOSAT数据中的X_(CO_2)检索。该方法可以直接评估由于大气光散射而引起的光路修改,而对光路修改的影响可忽略不计基于地面的TCCON测量,但是在观察来自太空的反射阳光时,可能会显着影响气体回收。我们的研究结果揭示了北半球站光学路径延长的影响,基本上是每年的5月至9月,以及热带地区日照观测的光学路径缩短的影响。由离线三维气溶胶传输模型得出的气溶胶光学深度的季节性趋势,以及由正交偏振(CALIOP)仪器对云气溶胶激光雷达进行天基测量得出的卷云光学深度,都支持了这些影响。从GOSAT数据集中删除了被气溶胶和云高度污染的观测结果,与TCCON测量结果相比,每个站的XCO2季节变化都可以接受。对于所有TCCON站,COSAT色谱柱丰度的GOSAT和TCCON同步测量之间的统计比较显示出相关系数为0.85,标准偏差为1.80 ppm和亚ppm负偏差为-​​0.43 ppm。空间分辨率为纬度2.5°×经度2.5°的月平均X_(CO_2)的全球平均分布与大气示踪剂传输模型预测的一致,在约2.5 ppm范围内。

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