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

dc.contributor.authorChesnokova, T.Y.
dc.contributor.authorMakarova, M.V.
dc.contributor.authorChentsov, A.V.
dc.contributor.authorVoronina, Y.V.
dc.contributor.authorZakharov, V.I.
dc.contributor.authorRokotyan, N.V.
dc.contributor.authorLangerock, B.
dc.date2019
dc.date.accessioned2019-09-16T09:36:53Z
dc.date.available2019-09-16T09:36:53Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/7354
dc.descriptionCarbon 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.
dc.languageeng
dc.titleRetrieval of Carbon Monoxide Total Column in the Atmosphere from High Resolution Atmospheric Spectra
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.subject.freecarbon monoxide
dc.subject.freeatmospheric transmission
dc.subject.freespectroscopic databases
dc.source.titleAtmospheric and Oceanic Optics
dc.source.volume32
dc.source.issue4
dc.source.page378-386
Orfeo.peerreviewedYes
dc.identifier.doi10.1134/S1024856019040031


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