Abstract
Carbon monoxide (CO) is a marker of the atmospheric pollution caused by fires and combustion engine emissions. The regular monitoring of the CO content in the atmosphere is needed to control air quality. In this work, the results of CO atmospheric total column retrievals from the solar spectra recorded by Fourier -transform spectrometers at the St. Petersburg (59.88° N, 29.83° E) and Kourovka (57.038° N, 59.545° E) stations are presented. The impact of differences in CO absorption line parameters in modern spectroscopic databases on the accuracy of the CO atmospheric total column retrieved from high resolution spectra is estimated.
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Funding
This work were financially supported by the Program of Fundamental Investigations by State Academies of Sciences (project АААА-А17-117021310147-0) and the Russian Foundation for Basic Research (grant no. 18-05-00011 “Study of reactive gases in the atmosphere by means of FTIR spectrometry”), as well as the project No. 3.6064.2017/8.9 within the basic part of the state assignment and the financial support by Resolution no. 211 of the Russian Federation Government, contract No. 02.A03.21.0006. The discussion of the results and preparation of the publication were supported by the Russian Foundation for Basic Research (grant no. 18-55-53 062 “Monitoring and study of gaseous and aerosol pollution of the atmosphere and greenhouse gases in Moscow and Beijing, based on satellite and ground high resolution spectroscopic technologies”).
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Chesnokova, T.Y., Makarova, M.V., Chentsov, A.V. et al. Retrieval of Carbon Monoxide Total Column in the Atmosphere from High Resolution Atmospheric Spectra. Atmos Ocean Opt 32, 378–386 (2019). https://doi.org/10.1134/S1024856019040031
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DOI: https://doi.org/10.1134/S1024856019040031