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dc.contributor.authorToureille, M.en
dc.contributor.authorKoroleva, A. O.en
dc.contributor.authorMikhailenko, S. N.en
dc.contributor.authorPirali, O.en
dc.contributor.authorCampargue, A.en
dc.date.accessioned2024-04-22T15:53:42Z-
dc.date.available2024-04-22T15:53:42Z-
dc.date.issued2022-
dc.identifier.citationToureille, M, Koroleva, AO, Mikhailenko, SN, Pirali, O & Campargue, A 2022, 'Water vapor absorption spectroscopy and validation tests of databases in the far-infrared (50–720 cm-1). Part 1: Natural water', Journal of Quantitative Spectroscopy and Radiative Transfer, Том. 291, 108326. https://doi.org/10.1016/j.jqsrt.2022.108326harvard_pure
dc.identifier.citationToureille, M., Koroleva, A. O., Mikhailenko, S. N., Pirali, O., & Campargue, A. (2022). Water vapor absorption spectroscopy and validation tests of databases in the far-infrared (50–720 cm-1). Part 1: Natural water. Journal of Quantitative Spectroscopy and Radiative Transfer, 291, [108326]. https://doi.org/10.1016/j.jqsrt.2022.108326apa_pure
dc.identifier.issn0022-4073
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access; Bronze Open Access; Green Open Access3
dc.identifier.otherhttp://manuscript.elsevier.com/S0022407322002618/pdf/S0022407322002618.pdf1
dc.identifier.otherhttp://manuscript.elsevier.com/S0022407322002618/pdf/S0022407322002618.pdfpdf
dc.identifier.urihttp://elar.urfu.ru/handle/10995/132480-
dc.description.abstractThe rotational spectrum of water vapor in natural isotopic abundance has been recorded by high resolution (≈ 0.001 cm-1) Fourier transform spectroscopy at the AILES beam line of the SOLEIL synchrotron. The room temperature absorption spectrum has been recorded between 50 and 720 cm-1 using five pressure values up to 7 mbar and an absorption pathlength of 151.75 m. Line parameters were retrieved for the five recorded spectra and then combined in a global list of 2867 water lines with line intensity ranging between a few 10–26 and 10–19 cm/molecule. 454 of the measured lines are newly observed by absorption spectroscopy. The spectral calibration based on a statistical matching with about 700 accurate reference line positions allows for line center determinations with an accuracy of 5 × 10–5 cm-1 for well isolated lines of intermediate intensity. The large spectral coverage, the achieved position accuracy and sensitivity of the constructed line list make it valuable for validation tests of the current spectroscopic databases. Six water isotopologues (H218O, H216O, H217O, HD18O, HD16O, and HD17O) were found to contribute to the spectrum. The line position comparison to the recent HITRAN2020 spectroscopic database and to the W2020 line lists of H216O, H217O and H218O, [Furtenbacher et al. J. Phys. Chem. Ref. Data 49 (2020) 043103; https://doi.org/10.1063/5.0030680] shows an overall very good agreement. Nevertheless, a number of significant deviations are observed. Part of them has an amplitude largely exceeding the W2020 claimed error bars. On the basis of the experimental data at disposal for the main isotopologue (1310 transitions), the best agreement is achieved with the positions calculated using the effective Bending–Rotation Hamiltonian [Coudert et al. J Mol Spectrosc 2014;303:36–41. https://doi.org/10.1016/j.jms.2014.07.003]. © 2022 Elsevier Ltden
dc.description.sponsorshipCentre National de la Recherche Scientifique, CNRSen
dc.description.sponsorshipRussian Science Foundation, RSF, (18–11–00024 -Π)en
dc.description.sponsorshipFunding text 1: This work became possible due to the Project No 20210051 supported by SOLEIL Synchrotron Team. SNM activity was supported in the frame of the Russian Science Foundation, grant no. 18–11–00024-Π. The support of the CNRS (France) in the frame of International Research Project SAMIA is acknowledged.en
dc.description.sponsorshipFunding text 2: This work became possible due to the Project No 20210051 supported by SOLEIL Synchrotron Team . SNM activity was supported in the frame of the Russian Science Foundation , grant no. 18–11–00024 -Π. The support of the CNRS (France) in the frame of International Research Project SAMIA is acknowledged.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherElsevier Ltden
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.rightspublisher-specific-oaother
dc.sourceJournal of Quantitative Spectroscopy and Radiative Transfer2
dc.sourceJournal of Quantitative Spectroscopy and Radiative Transferen
dc.subjectFAR INFRAREDen
dc.subjectROTATIONAL SPECTRUMen
dc.subjectWATER ISOTOPEen
dc.subjectWATER VAPORen
dc.subjectDATABASE SYSTEMSen
dc.subjectHTTPen
dc.subjectISOTOPESen
dc.subjectSYNCHROTRON RADIATIONen
dc.subjectWATER ABSORPTIONen
dc.subjectWATER VAPORen
dc.subjectFAR INFRAREDen
dc.subjectLINE LISTSen
dc.subjectLINE POSITIONSen
dc.subjectROTATIONAL SPECTRAen
dc.subjectSPECTRA'Sen
dc.subjectSPECTROSCOPIC DATABASEen
dc.subjectVALIDATION TESTen
dc.subjectWATER ISOTOPEen
dc.subjectWATER VAPOURen
dc.subjectWATER-VAPOR ABSORPTIONen
dc.subjectABSORPTION SPECTRUMen
dc.subjectATOMIC ABSORPTION SPECTROSCOPYen
dc.subjectDATABASEen
dc.subjectFTIR SPECTROSCOPYen
dc.subjectWATER VAPORen
dc.subjectABSORPTION SPECTROSCOPYen
dc.titleWater vapor absorption spectroscopy and validation tests of databases in the far-infrared (50–720 cm-1). Part 1: Natural wateren
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/acceptedVersionen
dc.identifier.doi10.1016/j.jqsrt.2022.108326-
dc.identifier.scopus85136545067-
local.contributor.employeeToureille M., Univ. Grenoble Alpes, CNRS, LIPhy, Grenoble, 38000, Franceen
local.contributor.employeeKoroleva A.O., Univ. Grenoble Alpes, CNRS, LIPhy, Grenoble, 38000, France, Institute of Applied Physics, Russian Academy of Sciences, Nizhniy Novgorod, Russian Federationen
local.contributor.employeeMikhailenko S.N., V.E. Zuev Institute of Atmospheric Optics, SB, Russian Academy of Science, 1, Academician Zuev square, Tomsk, 634055, Russian Federation, Climate and Environmental Physics Laboratory, Ural Federal University, 19, Mira av., Yekaterinburg, 620002, Russian Federationen
local.contributor.employeePirali O., SOLEIL Synchrotron, L'Orme des Merisiers, Saint-Aubin 91192, Gif-Sur-Yvette, France, Université Paris-Saclay, CNRS, Institut des Sciences Moléculaires d'Orsay, Orsay, 91405, Franceen
local.contributor.employeeCampargue A., Univ. Grenoble Alpes, CNRS, LIPhy, Grenoble, 38000, Franceen
local.description.firstpage743
local.description.lastpage767
local.issue9-10
local.volume291
dc.identifier.wos000848617300005-
local.contributor.departmentUniv. Grenoble Alpes, CNRS, LIPhy, Grenoble, 38000, Franceen
local.contributor.departmentInstitute of Applied Physics, Russian Academy of Sciences, Nizhniy Novgorod, Russian Federationen
local.contributor.departmentV.E. Zuev Institute of Atmospheric Optics, SB, Russian Academy of Science, 1, Academician Zuev square, Tomsk, 634055, Russian Federationen
local.contributor.departmentClimate and Environmental Physics Laboratory, Ural Federal University, 19, Mira av., Yekaterinburg, 620002, Russian Federationen
local.contributor.departmentSOLEIL Synchrotron, L'Orme des Merisiers, Saint-Aubin 91192, Gif-Sur-Yvette, Franceen
local.contributor.departmentUniversité Paris-Saclay, CNRS, Institut des Sciences Moléculaires d'Orsay, Orsay, 91405, Franceen
local.identifier.pure78229f19-aa04-4d5e-9a19-dac13861f1dauuid
local.identifier.pure30845381-
local.description.order108326
local.identifier.eid2-s2.0-85136545067-
local.identifier.wosWOS:000848617300005-
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