Published November 2008 | Version v1
Journal article

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

  • 1. Laboratoire de Physico-Chimie de l'Atmosphere, UMR CNRS 8101, Universite du Littoral Cote d'Opale, 189A Av. Maurice Schumann, 59140 Dunkerque (France)
  • 2. Institut UTINAM, UMR CNRS 6213, Universite de Franche-Comte, 16, Route de Gray, 25030 Besancon Cedex (France)
  • 3. Harvard-Smithsonian Center for Astrophysics, Atomic and Molecular Physics Division, 60 Garden Street, Cambridge, MA 02138-1516 (United States)
  • 4. Laboratoire de Physique des Lasers, Atomes et Molecules, UMR CNRS 8523, Batiment P5-135, Universite de Lille 1, 59655 Villeneuve d'Ascq Cedex (France)

Description

The room-temperature nitrogen- and oxygen-broadening coefficients of hydrogen cyanide spectral lines have been measured in the 0.5-3 THz (17-100 cm-1) frequency range (purely rotational transitions with 5≤J≤36) 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 the HITRAN 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

Availability note (English)

Available from http://dx.doi.org/10.1016/j.jqsrt.2008.08.005

Additional details

Identifiers

DOI
10.1016/j.jqsrt.2008.08.005;
PII
S0022-4073(08)00178-7;

Publishing Information

Journal Title
Journal of Quantitative Spectroscopy and Radiative Transfer
Journal Volume
109
Journal Issue
17-18
Journal Page Range
p. 2857-2868
ISSN
0022-4073
CODEN
JQSRAE

Optional Information

Copyright
Copyright (c) 2008 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.