Please use this identifier to cite or link to this item: http://elar.urfu.ru/handle/10995/132480
Title: Water vapor absorption spectroscopy and validation tests of databases in the far-infrared (50–720 cm-1). Part 1: Natural water
Authors: Toureille, M.
Koroleva, A. O.
Mikhailenko, S. N.
Pirali, O.
Campargue, A.
Issue Date: 2022
Publisher: Elsevier Ltd
Citation: Toureille, 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.2022.108326
Toureille, 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.2022.108326
Abstract: The 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 Ltd
Keywords: FAR INFRARED
ROTATIONAL SPECTRUM
WATER ISOTOPE
WATER VAPOR
DATABASE SYSTEMS
HTTP
ISOTOPES
SYNCHROTRON RADIATION
WATER ABSORPTION
WATER VAPOR
FAR INFRARED
LINE LISTS
LINE POSITIONS
ROTATIONAL SPECTRA
SPECTRA'S
SPECTROSCOPIC DATABASE
VALIDATION TEST
WATER ISOTOPE
WATER VAPOUR
WATER-VAPOR ABSORPTION
ABSORPTION SPECTRUM
ATOMIC ABSORPTION SPECTROSCOPY
DATABASE
FTIR SPECTROSCOPY
WATER VAPOR
ABSORPTION SPECTROSCOPY
URI: http://elar.urfu.ru/handle/10995/132480
Access: info:eu-repo/semantics/openAccess
publisher-specific-oa
SCOPUS ID: 85136545067
WOS ID: 000848617300005
PURE ID: 78229f19-aa04-4d5e-9a19-dac13861f1da
30845381
ISSN: 0022-4073
DOI: 10.1016/j.jqsrt.2022.108326
metadata.dc.description.sponsorship: Centre National de la Recherche Scientifique, CNRS
Russian Science Foundation, RSF, (18–11–00024 -Π)
Funding 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.
Funding 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.
Appears in Collections:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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