mental program to study the IR spectra of gas phase organics of interest to Titan. After a preliminary work covering In the frame of a program of systematic studies to determine the case of nitriles (Cerceau et al. 1985), we have estabor reassess the absolute intensities of gas phase organics of int
Absolute IR Band Intensities of Diacetylene in the 250-4300 cm−1 Region: Implications for Titan′s Atmosphere
✍ Scribed by M. Khlifi; P. Paillous; C. Delpech; M. Nishio; P. Bruston; F. Raulin
- Publisher
- Elsevier Science
- Year
- 1995
- Tongue
- English
- Weight
- 336 KB
- Volume
- 174
- Category
- Article
- ISSN
- 0022-2852
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✦ Synopsis
The infrared spectrum of (\mathrm{C}{4} \mathrm{H}{2}), butadyine (also called diacetylene), has been experimentally investigated in the region from 250 to (4300 \mathrm{~cm}^{-1}) using a Fourier transform spectrometer. A total of 12 bands have been analyzed. For each band, the characteristic wavenumber has been deduced and the values of the absolute band intensities have been systematically determined together with their associated uncertainties. The results provide important data for planetary studies. In particular, a better estimate of the mean stratospheric abundance of butadiyne in Titan's atmosphere is obtained: its value is about (50 %) higher than previously reported. 1995 Academic Press. Inc.
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