Retrieval of carbon monoxide content in the atmosphere from high resolution atmospheric spectra
T.Yu. Chesnokova1, M.V. Makarova2, A.V. Chentsov1, Yu.V. Voronina1, V.I. Zakharov3,4, N.V. Rokotyan3, B. Langerock5
1V.E. Zuev Institute of Atmospheric Optics of Siberian Branch of the Russian Academy of Science, 1, Academician Zuev square, Tomsk, 634055, Russia
2Saint-Petersburg State University, University Embankment, 7-9, St. Petersburg, 199034
3Ural Federal University named after the first President of Russia B.N. Yeltsin, 620083, 51 Lenina, Ekaterinburg, Russia
4Institute of Mathematics and Mechanics of Ural Branch of Russian Academy of Sciences, Russia, 620990, Ekaterinburg, S. Kovalevskaja st., 16
5Royal Belgian Institute for Space Aeronomy BIRA-IASB, 3-Avenue Circulaire B-1180 Brussels, Belgium
Keywords: монооксид углерода, атмосферное пропускание, спектроскопические базы данных, carbon monoxide, atmospheric transmission, spectroscopic databases
Abstract
Carbon monoxide CO is a marker of the atmosphere pollution caused by fires and combustion engines emission. The regular monitoring of the CO content in the atmosphere is needed to control the air quality. In the work, the results of CO atmospheric total content retrievals from the solar spectra recorded by Fourier spectrometers placed in Saint Petersburg (59.88N, 29.83E) and Kourovka (57.038N, 59.545E) stations, are presented. The impact of the difference in CO absorption line parameters in modern spectroscopic data bases on accuracy of the CO atmospheric content retrieval from the high resolution spectra is estimated.
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