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dc.contributor.authorKarlovets, E. V.en
dc.contributor.authorKassi, S.en
dc.contributor.authorTashkun, S. A.en
dc.contributor.authorCampargue, A.en
dc.date.accessioned2022-05-12T08:27:43Z-
dc.date.available2022-05-12T08:27:43Z-
dc.date.issued2021-
dc.identifier.citationThe Absorption Spectrum of Nitrous Oxide between 8325 and 8622 cm−1 / E. V. Karlovets, S. Kassi, S. A. Tashkun et al. // Journal of Quantitative Spectroscopy and Radiative Transfer. — 2021. — Vol. 262. — 107508.en
dc.identifier.issn0022-4073-
dc.identifier.otherAll Open Access, Green3
dc.identifier.urihttp://elar.urfu.ru/handle/10995/112074-
dc.description.abstractThe weak high-resolution absorption spectrum of natural nitrous oxide has been recorded by high sensitivity cavity ring down spectroscopy (CRDS) near 1.18 µm. The frequency scale of the spectra was obtained by coupling the CRDS spectrometer to a self-referenced frequency comb. The room temperature recordings, performed with a pressure of 1 Torr, cover the 8325-8622 cm−1 spectral interval where previous observations were very scarce. More than 3300 lines belonging to four N2O isotopologues (14N216O, 14N15N16O, 15N14N16O, and 14N218O) are measured with a position accuracy better than 1 × 10−3 cm−1 for most of the lines. Line intensities at room temperature range between 1.2 × 10−25 and 3.8 × 10−30 cm/molecule. The rovibrational assignments were obtained by comparison with predictions based on the global modeling of the line positions and intensities performed within the framework of the method of effective operators. The band-by-band analysis led to the determination of the rovibrational parameters of a total of 47 bands. All identified bands belong to the ΔP= 14-16 series of transitions, where P=2V1+V2+4V3 is the polyad number (Vi= 1-3 are the vibrational quantum numbers). Among these bands, only five were previously observed and bands of the ΔP= 15 series are reported for the first time. Local resonance perturbations affecting two bands are identified and analyzed. The position and intensity comparisons to the HITRAN2016 and HITEMP2019 spectroscopic databases are discussed. The HITRAN line list is limited to only four (calculated) bands of the 14N218O isotopologue in the studied region while ΔP= 15 bands are missing in the HITEMP list. The present work will help to improve future versions of the spectroscopic databases of nitrous oxide, a strong greenhouse gas. © 2021 Elsevier Ltden
dc.description.sponsorshipThis work is jointly supported by CNRS (France) in the frame of the International Research Project “ SAMIA ” with IAO-Tomsk.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherElsevier Ltden1
dc.publisherElsevier BVen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceJ. Quant. Spectrosc. Radiat. Transf.2
dc.sourceJournal of Quantitative Spectroscopy and Radiative Transferen
dc.subjectCAVITY RING DOWN SPECTROSCOPYen
dc.subjectHIGH-RESOLUTION SPECTRAen
dc.subjectHITEMPen
dc.subjectHITRANen
dc.subjectLINE INTENSITIESen
dc.subjectLINE POSITIONSen
dc.subjectN2Oen
dc.subjectNITROUS OXIDEen
dc.subjectABSORPTION SPECTRAen
dc.subjectGREENHOUSE GASESen
dc.subjectLIGHT MEASUREMENTen
dc.subjectNITROGEN OXIDESen
dc.subjectQUANTUM THEORYen
dc.subjectSPECTROMETERSen
dc.subjectCAVITY RING DOWN SPECTROSCOPIESen
dc.subjectHIGH RESOLUTION ABSORPTION SPECTRUMen
dc.subjectROOM TEMPERATURE RANGESen
dc.subjectROVIBRATIONAL ASSIGNMENTen
dc.subjectSERIES OF TRANSITIONen
dc.subjectSPECTROSCOPIC DATABASEen
dc.subjectTEMPERATURE RECORDINGen
dc.subjectVIBRATIONAL QUANTUM NUMBERen
dc.subjectABSORPTION SPECTROSCOPYen
dc.subjectABSORPTIONen
dc.subjectCOMPARATIVE STUDYen
dc.subjectDATABASEen
dc.subjectMODEL TESTen
dc.subjectNITROUS OXIDEen
dc.subjectPERFORMANCE ASSESSMENTen
dc.subjectSPECTRAL ANALYSISen
dc.subjectSPECTRAL RESOLUTIONen
dc.titleThe Absorption Spectrum of Nitrous Oxide between 8325 and 8622 cm−1en
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/submittedVersionen
dc.identifier.doi10.1016/j.jqsrt.2021.107508-
dc.identifier.scopus85099874664-
local.contributor.employeeKarlovets, E.V., Harvard-Smithsonian Center for Astrophysics, Atomic and Molecular Physics Division, 60 Garden St, Cambridge, MA, United States, Tomsk State University, Laboratory of Quantum Mechanics of Molecules and Radiative Processes, 36, Lenin AvenueTomsk 634050, Russian Federation; Kassi, S., Univ. Grenoble Alpes, CNRS, LIPhy, Grenoble, 38000, France; Tashkun, S.A., V.E. Zuev Institute of Atmospheric Optics, 1, Academician Zuev squareTomsk 634055, Russian Federation, Ural Federal University, Climate and Environmental Physics Laboratory, 19, Mira Avenue, Yekaterinburg, 620002, Russian Federation; Campargue, A., Univ. Grenoble Alpes, CNRS, LIPhy, Grenoble, 38000, Franceen
local.volume262-
dc.identifier.wos000642458300008-
local.contributor.departmentHarvard-Smithsonian Center for Astrophysics, Atomic and Molecular Physics Division, 60 Garden St, Cambridge, MA, United States; Tomsk State University, Laboratory of Quantum Mechanics of Molecules and Radiative Processes, 36, Lenin AvenueTomsk 634050, Russian Federation; Univ. Grenoble Alpes, CNRS, LIPhy, Grenoble, 38000, France; V.E. Zuev Institute of Atmospheric Optics, 1, Academician Zuev squareTomsk 634055, Russian Federation; Ural Federal University, Climate and Environmental Physics Laboratory, 19, Mira Avenue, Yekaterinburg, 620002, Russian Federationen
local.identifier.pure20545964-
local.description.order107508-
local.identifier.eid2-s2.0-85099874664-
local.identifier.wosWOS:000642458300008-
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