A total of 6071 transition wavenumbers of the 2 , 3 , 5 , and 6 fundamental bands of H 3 13 CF and 1689 frequencies of the rotational transitions in the v 2 ϭ 1, v 3 ϭ 1, v 5 ϭ 1, and v 6 ϭ 1 vibrational states have been fitted simultaneously by taking into account various Coriolis interactions, l-t
2ν3 Band of 12CF4 and Its Simultaneous Analysis with ν3
✍ Scribed by T. Gabard; A. Nikitin; J.P. Champion; G. Pierre; A.S. Pine
- Publisher
- Elsevier Science
- Year
- 1995
- Tongue
- English
- Weight
- 847 KB
- Volume
- 170
- Category
- Article
- ISSN
- 0022-2852
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✦ Synopsis
A nearly Doppler-limited spectrum of the (2 \nu_{3}) band of the ({ }^{12} \mathrm{CF}{4}) molecule between 2536.0 and (2599.8 \mathrm{~cm}^{-1}) was recorded at (T=77 \mathrm{~K}) using difference-frequency laser spectroscopy. The simultaneous analysis of the ground (G.S.), (v{3}=1), and (v_{3}=2) states was performed using an isolated band model to sixth order in the tetrahedral formalism. Fourteen hundred seventy-five transitions were assigned through (J=35) to the (F_{2}) and (E) vibrational components of the (v_{3}=2) level. A total of 1864 transition frequencies were fit simultaneously ( (10002 v_{3}-) G.S. newly assigned transitions together with (575 \nu_{3}) - G.S. and (289 \nu_{3}-\nu_{3}) transitions already reported in the literature). The ground state constants were improved. Interactions with the (v_{3}+2 v_{4}) and (4 v_{4}) bands are proposed to explain some of the discrepancies observed in the (2 v_{3}) band. (c) 1995 Academic Press. Inc.
📜 SIMILAR VOLUMES
A total of 4892 transition wavenumbers of the 2 , 3 , 5 , and 6 fundamental bands of H 3 12 CF and 1469 frequencies of the rotational transitions in the v 2 ϭ 1, v 3 ϭ 1, v 5 ϭ 1, and v 6 ϭ 1 vibrational states have been fitted simultaneously by taking explicitly into account various Coriolis intera
Using a Fourier transform spectrometer, we have recorded the spectra of ozone in the region of 4600 cm 01 , with a resolution of 0.008 cm 01 . The strongest absorption in this region is due to the n 1 / n 2 / 3n 3 band which is in Coriolis interaction with the n 2 / 4n 3 band. We have been able to a