First line shape analysis and spectroscopic parameters for the ν11 band of 12C2H4
KAUST DepartmentClean Combustion Research Center
Physical Sciences and Engineering (PSE) Division
MetadataShow full item record
AbstractAn accurate knowledge of line intensities, collisional broadening coefficients and narrowing parameters is necessary for the interpretation of high-resolution infrared spectra of the Earth and other planetary atmospheres. One of the most promising spectral domains for (C2H4)-C-12 monitoring in such environments is located near the 336 gm window, through its v(11) C-H stretching mode. In this paper, we report an extensive study in which we precisely determine spectroscopic parameters of (C2H4)-C-12 v(11) band at 297 +/- 1 K, using a narrow Difference-Frequency-Generation (DFG) laser with 10(-4) cm(-1) resolution. Absorption measurements were performed in the 2975-2980 cm(-1) spectral window to investigate 32 lines corresponding to where, J'ka',kc'<- Jka,kc, 5 <= J <= 7; 0.5 <= K-a <= 6 and 1 <= K-c <= 14. Spectroscopic parameters are retrieved using either Voigt or appropriate Galatry profile to simulate the measured (C2H4)-C-12 line shape. Line intensities along with self-broadening coefficients are reported for all lines. Narrowing coefficients for each isolated line are also derived. To our knowledge, the current study reports the first extensive spectroscopic parameter measurements of the (C2H4)-C-12 v(11) band in the 2975-2980 cm(-1) range. (C) 2016 Elsevier Ltd. All rights reserved.
CitationEs-sebbar E, Mantzaras J, Benilan Y, Farooq A (2016) First line shape analysis and spectroscopic parameters for the ν11 band of 12C2H4. Journal of Quantitative Spectroscopy and Radiative Transfer 184: 297–307. Available: http://dx.doi.org/10.1016/j.jqsrt.2016.07.021.
SponsorsResearch reported in this publication was supported by the King Abdullah University of Science and Technology (KAUST).