1961
DOI: 10.1364/josa.51.001219
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Infrared Spectrum of Acetylene*

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1964
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Cited by 32 publications
(10 citation statements)
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“…In order to derive the acetylene concentration from atmospheric spectra or from spectra of astrophysical objects, spectroscopic data as line parameters are necessary. As soon as 1961, Wiggins et al [7] measured line positions in 11 bands located between 2500 and 4150 cm −1 with a low resolution of 0.03 cm −1 . This set included the 5 bands studied in this work.…”
Section: Introductionmentioning
confidence: 99%
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“…In order to derive the acetylene concentration from atmospheric spectra or from spectra of astrophysical objects, spectroscopic data as line parameters are necessary. As soon as 1961, Wiggins et al [7] measured line positions in 11 bands located between 2500 and 4150 cm −1 with a low resolution of 0.03 cm −1 . This set included the 5 bands studied in this work.…”
Section: Introductionmentioning
confidence: 99%
“…For each band, the fitted parameters which are the vibrational transition dipole moment squared and the Herman-Wallis coefficients, are given inTable 8, together with the vibrational dipole moments squared. The calculated values 2 calc R have been obtained using Eqs (7)(8)(9). with the values of…”
mentioning
confidence: 99%
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“…The rotational and rovibrational spectra of acetylene, C 2 H2, have been extensively investigated by both the infrared and Raman methods, see, e.g., references [1][2][3][4]. This paper reports a study of the vibration-rotation infrared spectrum of C2H2 between 2500cm -1 and 2800cm -I .…”
Section: Introductionmentioning
confidence: 99%
“…This paper reports a study of the vibration-rotation infrared spectrum of C2H2 between 2500cm -1 and 2800cm -I . This wavenumber region has been examined by Wiggins et al [1] and Lafferty and Thibault [5] and, more recently, by Palmer et al [3]. It was felt that the improvement in resolution and in signal to noise ratio allows us to resolve more lines and so to carry out a more detailed analysis, considering especially the effects of the Fermi and/-type resonances.…”
Section: Introductionmentioning
confidence: 99%