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Oxygen, nitrogen and air broadening of HCN spectral lines at terahertz frequencies

Authors :
Chun Yang
Jeanna Buldyreva
Gaël Mouret
Arnaud Cuisset
Francis Hindle
François Rohart
Robin Bocquet
Iouli E. Gordon
Laboratoire de Physico-Chimie de l'Atmosphère (LPCA)
Université du Littoral Côte d'Opale (ULCO)-Centre National de la Recherche Scientifique (CNRS)
Univers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) (UTINAM)
Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC)
Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC)
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 (PhLAM)
Université de Lille-Centre National de la Recherche Scientifique (CNRS)
Harvard-Smithsonian Center for Astrophysics (CfA)
Harvard University-Smithsonian Institution
Source :
JOURJOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER, JOURJOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER, 2008, 109 (17-1), pp.2857-2868
Publication Year :
2008
Publisher :
Elsevier BV, 2008.

Abstract

International audience; The room-temperature nitrogen- and oxygen-broadening coefficients of hydrogen cyanide spectral lines have been measured in the 0.5–3 THz (17–100 cm1) frequency range (purely rotational transitions with 5pJp36) by a continuous-wave terahertz spectrometer based on a photomixing source. An improved version of the Robert and Bonamy semiclassical formalism has been used to calculate the oxygen-broadening coefficients and resulted in a good agreement with these measurements. The nitrogen and oxygen data are combined to provide the air-broadening coefficients as used by theHITRAN database. A significant difference is observed between the measured and tabulated values for transitions with high values of the rotational quantum number. A new polynomial representation is suggested for inclusion in HITRAN. A similar polynomial expression has been derived for the nitrogen broadening to aid the studies of Titan’s atmosphere.

Details

ISSN :
00224073
Volume :
109
Database :
OpenAIRE
Journal :
Journal of Quantitative Spectroscopy and Radiative Transfer
Accession number :
edsair.doi.dedup.....28ca7bd7dd1d48c85d7a40b9e4d8f468
Full Text :
https://doi.org/10.1016/j.jqsrt.2008.08.005