China's First Infrared Occultation Spectrometer (GaoFen-5/AIUS) Monitoring Atmosphere Above Antarctic: Evaluation of Methane Profiles

The atmospheric infrared ultraspectral sounder (AIUS) is China's first infrared occultation spectrometer onboard the GaoFen-5 satellite. This instrument provides measurements in the near-infrared and mid-infrared spectral regions with a spectral resolution of 0.02 cm<inline-formula><te...

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Published inIEEE journal of selected topics in applied earth observations and remote sensing Vol. 17; pp. 7946 - 7956
Main Authors Liu, Shuanghui, Li, Xiaoying, Xu, Jian, Shi, Hailiang, Guo, Yuhang, Zhang, Xingying, Ge, Shule, Wang, Yapeng, Wang, Hongmei, Cao, Xifeng, Rao, Lanlan, Shi, Jiancheng
Format Journal Article
LanguageEnglish
Published Piscataway IEEE 2024
The Institute of Electrical and Electronics Engineers, Inc. (IEEE)
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Summary:The atmospheric infrared ultraspectral sounder (AIUS) is China's first infrared occultation spectrometer onboard the GaoFen-5 satellite. This instrument provides measurements in the near-infrared and mid-infrared spectral regions with a spectral resolution of 0.02 cm<inline-formula><tex-math notation="LaTeX">^{-1}</tex-math></inline-formula>, monitoring key greenhouse gases like methane (CH<inline-formula><tex-math notation="LaTeX">_{4}</tex-math></inline-formula>). In this study, we have developed a physics-based retrieval algorithm for accurately deriving CH<inline-formula><tex-math notation="LaTeX">_{4}</tex-math></inline-formula> mole fraction profiles from infrared absorption spectra. The retrieval algorithm is applied to the AIUS and successfully obtains CH<inline-formula><tex-math notation="LaTeX">_{4}</tex-math></inline-formula> mole fraction profiles from January to December 2019 over Antarctic. The validation results show that the retrieval algorithm has a satisfactory performance using AIUS measurements, with average relative standard deviation of the differences less than 7.2% throughout the altitude range of 10-70 km.
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ISSN:1939-1404
2151-1535
DOI:10.1109/JSTARS.2024.3381651