研究目的
To verify the performance of TanSat instruments and model the column-average dry-air mole fraction of atmospheric carbon dioxide (XCO2) surface based on flight test data.
研究成果
The modeling of the XCO2 surface based on the flight test of the TanSat instruments fell within an expected and acceptable range, with urban areas showing higher XCO2 concentrations. Future work will consider the impact of clouds and aerosols and utilize the CO2 strong absorption band for more comprehensive analysis.
研究不足
The presence of clouds and aerosols could influence XCO2 measurements, and the CO2 strong absorption band at 2060 nm was not used due to cost constraints.
1:Experimental Design and Method Selection:
The study involved a flight test of TanSat instruments to measure near- and short-wave infrared (NIR) reflected solar radiation in the absorption bands at around 760 and 1610 nm. The high accuracy surface modeling (HASM) platform was used to fill gaps in XCO2 data.
2:Sample Selection and Data Sources:
The flight test area covered about 11,000 km2 in Jilin Province, including various underlying surfaces. Data included flight test L1B data and ground synchronous observations.
3:List of Experimental Equipment and Materials:
Instruments included a spectrometer covering two NIR spectral bands, sonde measurements for atmospheric profiles, and a Greenhouse gas online laser analyzer for CO2 concentration.
4:Experimental Procedures and Operational Workflow:
The workflow included retrieving XCO2 using a full physics retrieval algorithm, establishing an approximate XCO2 surface via regression modeling, and using HASM for high accuracy surface modeling.
5:Data Analysis Methods:
The study used the SCIATRAN radiative transfer model for synthetic spectra generation and the Levenberg-Marquardt method for inversion.
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