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Multispectrum fitting of line parameters for 12C2H2 in the 3.8-μm spectral region

✍ Scribed by D. Jacquemart; N. Lacome; J.-Y. Mandin; V. Dana; O.M. Lyulin; V.I. Perevalov


Publisher
Elsevier Science
Year
2007
Tongue
English
Weight
341 KB
Volume
103
Category
Article
ISSN
0022-4073

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✦ Synopsis


Using FT spectra (Bruker IFS 120, unapodized FWHM resolution E 0.001 cm À1 ) of acetylene 12 C 2 H 2 , absolute positions and intensities have been measured for about 250 lines between 2600 and 2800 cm À1 in the n 2 þ n 1 5 and ð3n 4 þ n 5 Þ 0 þ cold bands, and in the n 1 À n 1 5 ; n 3 À n 1 4 ; and

These measurements improve the accuracy of wavenumbers previously available and lead to individual line intensities for the first time in this spectral region. A multispectrum fitting procedure has been used to retrieve line parameters from five experimental spectra recorded at different pressures. The frequencies of the n 3 band of 12 C 16 O 2 allowed to perform an absolute wavenumber calibration. The accuracy of the amount of 12 C 2 H 2 in the sample has been checked using the 3n 1 5 cold band around 2100 cm À1 , and has been estimated to be around 72%. The average absolute accuracy of the line parameters obtained in this work has then been estimated to be 70.0002 cm À1 for line positions, and 75% for line intensities. For each studied band, the vibrational transition dipole moment squared value has been determined, as also empirical Herman-Wallis coefficients. A complete line list containing positions and intensities for the five strongest bands around 3.8 mm has been set up for atmospheric applications.


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Intensities of about 320 lines of the 12 C 2 H 2 molecule, belonging to 7 parallel bands, are measured in the 1.3, 1.2, and 1 mm spectral regions, with a mean accuracy around 3% or 7% depending on the spectral region. Vibrational transition dipole moment squared values and Herman-Wallis coefficients

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branches of the 5 perpendicular band. These lines with J values ranging from 1 to 23 and K from 0 to 9 (K Յ J) are located in the spectral range 1416 -1573 cm Ϫ1 . The collisional halfwidths are obtained by modeling each spectral line with a Voigt and a Rautian profile. The noncorrelated Rautian mod