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dc.contributor.authorDucreux, É.
dc.contributor.authorGrouiez, B.
dc.contributor.authorRobert, S.
dc.contributor.authorLepère, M.
dc.contributor.authorVispoel, B.
dc.contributor.authorGamache, R.R.
dc.contributor.authorRégalia, L.
dc.date2024
dc.date.accessioned2024-05-13T06:36:30Z
dc.date.available2024-05-13T06:36:30Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/13254
dc.descriptionH2O is an important molecule in the quest to better understand the evolution of solar system. In the study of Venus and Mars CO2-rich atmospheres (around 96 % of their composition) and because of the space instruments constant improvements, the planetary community needs spectroscopic data as accurate as possible. Continuing from our previous study [JQSRT 231, 126(2019)], new spectra of H2O perturbed by CO2 were measured with our new experimental set-up in the 2.7 µm region to compare with the previous results. After the improvement in the determination of the partial pressure of water vapor, the line parameters were then determined with a multispectrum fitting procedure using a Voigt profile in the same way as in [JQSRT 231, 126(2019)]. This led to characteristic W-shape residuals that have been improved using beyond-Voigt profiles. Our investigation showed that considering the speed dependence of collisional line parameters is essential to obtain better line-shape parameters in the considered experimental conditions.
dc.languageeng
dc.titleMeasurements of H2O broadened by CO2 line-shape parameters: Beyond the Voigt profile
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeHigh resolution infrared spectroscopy
dc.subject.freeLine shape parameters
dc.subject.freeWater vapor
dc.subject.freeCarbon dioxide
dc.subject.freeLine profiles
dc.subject.freePlanetary
dc.subject.freeatmospheres
dc.source.titleJournal of Quantitative Spectroscopy and Radiative Transfer
dc.source.volume323
dc.source.pageA109026
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/j.jqsrt.2024.109026
dc.identifier.url


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