Room temperature self- and H2-broadened line parameters of carbon monoxide in the first overtone band: Theoretical and revised experimental results
Creators
- 1. Department of Physics and Astronomy, University of Lethbridge, Lethbridge, AB (Canada)
- 2. Federal Scientific Research Centre "Crystallography and Photonics" of Russian Academy of Sciences (FSRC "Crystallography and Photonics" RAS), Leninsky pr. 59, Moscow 119333 (Russian Federation)
- 3. Institut de Physique de Rennes, UMR CNRS 6251, Université de Rennes 1, Campus de Beaulieu, F-35042 Rennes (France)
- 4. Science Directorate, NASA Langley Research Center, Hampton, VA (United States)
Description
Lorentz self- and H2-broadened half-width and pressure-induced shift coefficients, line mixing coefficients as well as line center positions and intensities were obtained using a nonlinear least square fitting technique for 48 (P(24) to R(23)) ro-vibrational transitions belonging to the first overtone (2←0) band of 12C16O at room temperature. All spectra in the 4146 to 4332 cm−1 spectral interval were fitted simultaneously employing four line shape functions: the Voigt, Speed Dependent Voigt, Rautian and Speed Dependent Rautian profiles. The collisional line mixing effect has been observed and investigated as an asymmetry in the analyzed line profiles. A semi-empirical Exponential Power Gap Law method was used to estimate the self- and H2-broadening coefficients and the collisional line mixing parameters. Additionally, a classical approach was applied to calculate the half-width coefficients of transitions in the 2←0 band for carbon monoxide broadened by H2 and for pure CO. The classical approach based on a simple computational method, ensures the molecular motion is correctly characterized in 3 dimensions. The calculations used vibrationally independent intermolecular interaction potentials. The variation of CO half-width coefficients with rotational quantum number J≤24 was computed and compared with measurements. The agreement between the theoretical broadening coefficients is better for pure CO rather than for the CO-H2 system. - Highlights: • Self- and H2-broadened line parameters for transitions in the 2←0 band of CO at 298 K are reported. • Line intensities, pressure shifts, line mixing and speed dependence parameters are presented. • Calculations of self- and H2-broadening coefficients of CO using classical impact theory are included.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.jqsrt.2017.04.008Additional details
Identifiers
- DOI
- 10.1016/j.jqsrt.2017.04.008;
- PII
- S0022-4073(16)30878-0;
Publishing Information
- Journal Title
- Journal of Quantitative Spectroscopy and Radiative Transfer
- Journal Volume
- 203
- Journal Page Range
- p. 309-324
- ISSN
- 0022-4073
- CODEN
- JQSRAE
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 49049520
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY;
- Descriptors DEI
- CARBON MONOXIDE; COBALT; MIXING; NONLINEAR PROBLEMS; QUANTUM NUMBERS; TEMPERATURE RANGE 0273-0400 K; VELOCITY
- Descriptors DEC
- CARBON COMPOUNDS; CARBON OXIDES; CHALCOGENIDES; ELEMENTS; METALS; OXIDES; OXYGEN COMPOUNDS; TEMPERATURE RANGE; TRANSITION ELEMENTS
Optional Information
- Copyright
- Copyright (c) 2017 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.