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dc.contributor.authorRégalia, L.en
dc.contributor.authorThomas, X.en
dc.contributor.authorRennesson, T.en
dc.contributor.authorMikhailenko, S.en
dc.date.accessioned2021-08-31T15:05:00Z-
dc.date.available2021-08-31T15:05:00Z-
dc.date.issued2019-
dc.identifier.citationLine parameters of water vapor enriched by 18O from 6525 to 8011 cm−1 / L. Régalia, X. Thomas, T. Rennesson, et al. — DOI 10.1016/j.jqsrt.2019.06.031 // Journal of Quantitative Spectroscopy and Radiative Transfer. — 2019. — Vol. 235. — P. 257-271.en
dc.identifier.issn224073-
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access, Bronze3
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85068800312&doi=10.1016%2fj.jqsrt.2019.06.031&partnerID=40&md5=82c96f1782ea1b46800c02d4f88be444
dc.identifier.urihttp://elar.urfu.ru/handle/10995/102703-
dc.description.abstractThis study is a continuation of experimental efforts on the analysis of the near-infrared absorption spectrum of water vapor. Our previous studies were focused on water vapor in natural isotopic abundance. Now we are interested in the H2 18O water isotopologue. New spectra of water samples enriched by 18O were recorded between 6400 and 9400 cm−1 in Reims with the Connes-type Fourier Transform Spectrometer, built in our laboratory. The spectra were recorded at room temperature with a H2 18O abundance enrichment of about 95% and a non apodized resolution of 0.010 cm−1. Pressure varied from 2 to 13 torr and the absorption path length was from 67 cm to 1001 m. This article presents the results of the analysis of the first part of the whole recorded spectral range below 8000 cm−1. About 8100 absorption lines were found in the recorded spectra with an absorption path length from 8 to 88 m between 6525 and 8011 cm−1. Overall, 7993 lines were assigned to 8647 transitions of six water isotopologues (H2 16O, H2 17O, H2 18O, HD16O, HD17O, and HD18O). Ninety-eight lines with intensity values between 6 × 10−27 and 1.45 × 10−25 cm/molecule were left unassigned. More than 870 H2 18O, H2 17O and HD18O lines were observed for the first time. The observed line positions allow to obtain about 90 new or corrected rotation-vibration energy levels of H2 18O and H2 17O. Comparison of line positions and intensities with literature data are presented and discussed. Some examples of disagreements between the measurements and data from the literature are presented in the last part of this article. © 2019 Elsevier Ltden
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherElsevier Ltden
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceJ. Quant. Spectrosc. Radiat. Transf.2
dc.sourceJournal of Quantitative Spectroscopy and Radiative Transferen
dc.subject18Oen
dc.subjectFTS SPECTRAen
dc.subjectINFRARED SPECTROSCOPYen
dc.subjectLINE INTENSITY MEASUREMENTSen
dc.subjectWATER VAPORen
dc.subjectABSORPTION SPECTROSCOPYen
dc.subjectFOURIER TRANSFORM INFRARED SPECTROSCOPYen
dc.subjectINFRARED DEVICESen
dc.subjectINFRARED SPECTROSCOPYen
dc.subjectLIGHT ABSORPTIONen
dc.subjectSPACECRAFT INSTRUMENTSen
dc.subjectSPECTROMETERSen
dc.subjectWATER VAPORen
dc.subjectABSORPTION LINESen
dc.subjectFOURIER TRANSFORM SPECTROMETERSen
dc.subjectISOTOPIC ABUNDANCESen
dc.subjectLINE INTENSITIESen
dc.subjectNEAR INFRARED ABSORPTION SPECTRUMen
dc.subjectROTATION VIBRATIONen
dc.subjectWATER ISOTOPOLOGUESen
dc.subject^18Oen
dc.subjectWATER ABSORPTIONen
dc.subjectABSORPTION SPECTRUMen
dc.subjectEXPERIMENTAL STUDYen
dc.subjectINFRARED SPECTROSCOPYen
dc.subjectNEAR INFRAREDen
dc.subjectOXYGEN ISOTOPEen
dc.subjectWATER VAPORen
dc.titleLine parameters of water vapor enriched by 18O from 6525 to 8011 cm−1en
dc.typeReviewen
dc.typeinfo:eu-repo/semantics/reviewen
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1016/j.jqsrt.2019.06.031-
dc.identifier.scopus85068800312-
local.contributor.employeeRégalia, L., Université de Reims Champagne Ardenne, CNRS, GSMA UMR 7331, Reims, 51097, France
local.contributor.employeeThomas, X., Université de Reims Champagne Ardenne, CNRS, GSMA UMR 7331, Reims, 51097, France
local.contributor.employeeRennesson, T., Université de Reims Champagne Ardenne, Reims, 51097, France
local.contributor.employeeMikhailenko, S., Climate and Environmental Physics Laboratory, Ural Federal University, 19, Mira av., Yekaterinburg, 620002, Russian Federation, Laboratory of Theoretical Spectroscopy, V.E. Zuev Institute of Atmospheric Optics, SB RAS, 1, Academician Zuev square, Tomsk, 634050, Russian Federation
local.description.firstpage257-
local.description.lastpage271-
local.volume235-
dc.identifier.wos000485334200026-
local.contributor.departmentUniversité de Reims Champagne Ardenne, CNRS, GSMA UMR 7331, Reims, 51097, France
local.contributor.departmentUniversité de Reims Champagne Ardenne, Reims, 51097, France
local.contributor.departmentClimate and Environmental Physics Laboratory, Ural Federal University, 19, Mira av., Yekaterinburg, 620002, Russian Federation
local.contributor.departmentLaboratory of Theoretical Spectroscopy, V.E. Zuev Institute of Atmospheric Optics, SB RAS, 1, Academician Zuev square, Tomsk, 634050, Russian Federation
local.identifier.puree29c550b-b86c-40cc-80de-f37c50266633uuid
local.identifier.pure10269425-
local.identifier.eid2-s2.0-85068800312-
local.identifier.wosWOS:000485334200026-
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