On the Assessment and Uncertainty of Atmospheric Trace Gas Burden Measurements with High Resolution Infrared Solar Occultation Spectra from Space
On the Assessment and Uncertainty of Atmospheric Trace Gas Burden Measurements with High Resolution Infrared Solar Occultation Spectra from Space
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空间高分辨率红外太阳掩星光谱大气微量气体负荷测量的评估和不确定度
DOI：
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发表时间：
1996
期刊：
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通讯作者：
A. Goldman
中科院分区：
文献类型：
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作者：
C. Rinsland;M. Gunson;R. Salawitch;M. Newchurch;R. Zander;M. Abbas;M. Abrams;G. Manney;H. Michelsen;A. Chang;A. Goldman
大气痕量分子光谱仪是一种高分辨率傅里叶变换光谱仪，它利用临边几何中的红外掩星探测从低地球轨道测量大气成分。在1985年首次飞行后，ATMOS参加了1992年、1993年和1994年的大气应用和科学实验室（ATLAS）1、2和3号航天飞机任务，在9年的时间里总共进行了440次掩星测量。这套超过30种大气痕量气体包括CO2、O3、N2 O、CH 4、H2O、NO、NO2、HNO 3、HCl、HF、ClONO 2、CCl 3F、CCl 2F 2、CHF 2Cl和N2 O 5。分析方法在整个使命年中不断修订，最终形成了“版本2”数据集。光谱误差分析的背景下，支持精度估计报告的配置文件;此外，系统的不确定性评估的光谱数据库的质量进行了描述和列表与其他实验进行比较。
The Atmospheric Trace Molecule Spectroscopy (ATMOS) instrument is a high resolution Fourier transform spectrometer that measures atmospheric composition from low Earth orbit with infrared solar occultation sounding in the limb geometry. Following an initial flight in 1985, ATMOS participated in the Atmospheric Laboratory for Applications and Science (ATLAS) 1, 2, and 3 Space Shuttle missions in 1992, 1993, and 1994 yielding a total of 440 occultation measurements over a nine year period. The suite of more than thirty atmospheric trace gases profiled includes CO2, O3, N2O, CH4, H2O, NO, NO2, HNO3, HCl, HF, ClONO2, CCl3F, CCl2F2, CHF2Cl, and N2O5. The analysis method has been revised throughout the mission years culminating in the ‘version 2’ data set. The spectroscopic error analysis is described in the context of supporting the precision estimates reported with the profiles; in addition, systematic uncertainties assessed from the quality of the spectroscopic database are described and tabulated for comparisons with other experiments.