Retrieval of Carbon Monoxide Total Column in the Atmosphere from High Resolution Atmospheric Spectra


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Resumo

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.

Sobre autores

T. Chesnokova

V.E. Zuev Institute of Atmospheric Optics, Siberian Branch, Russian Academy of Sciences

Autor responsável pela correspondência
Email: ches@iao.ru
Rússia, Tomsk, 634055

M. Makarova

St. Petersburg State University

Email: ches@iao.ru
Rússia, St. Petersburg, 190334

A. Chentsov

V.E. Zuev Institute of Atmospheric Optics, Siberian Branch, Russian Academy of Sciences

Email: ches@iao.ru
Rússia, Tomsk, 634055

Yu. Voronina

V.E. Zuev Institute of Atmospheric Optics, Siberian Branch, Russian Academy of Sciences

Email: ches@iao.ru
Rússia, Tomsk, 634055

V. Zakharov

B.N. Yeltsin Ural Federal State University; Institute of Mathematics and Mechanics, Ural Branch, Russian Academy of Sciences

Email: ches@iao.ru
Rússia, Yekaterinburg, 620002; Yekaterinburg, 620990

N. Rokotyan

B.N. Yeltsin Ural Federal State University

Email: ches@iao.ru
Rússia, Yekaterinburg, 620002

B. Langerock

Royal Belgian Institute for Space Aeronomy BIRA-IASB

Email: ches@iao.ru
Bélgica, Brussels, 1180

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