𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Analysis of the 2ν1 + 2ν2 + ν3 Band of Ozone

✍ Scribed by A. Barbe; S. Mikhailenko; V. Tyuterev; A. Hamdouni; J.J. Plateaux


Publisher
Elsevier Science
Year
1995
Tongue
English
Weight
223 KB
Volume
171
Category
Article
ISSN
0022-2852

No coin nor oath required. For personal study only.


📜 SIMILAR VOLUMES


Analysis of the 2ν1+ ν2+ 2ν3Band of Ozon
✍ A. Barbe; S. Mikhailenko; J.J. Plateaux; Vl.G. Tyuterev 📂 Article 📅 1997 🏛 Elsevier Science 🌐 English ⚖ 275 KB

The 2nu1 + nu2 + 2nu3 band of ozone, occurring in the 4780 cm-1 region, has been observed for the first time, using a Fourier transform spectrometer, at 0.008 cm-1 resolution and using a large path length pressure product. Assignments of vibration-rotational transitions have been made up to J = 48 a

New Analysis of 2ν1 + ν2, ν1 + ν2 + ν3,
✍ S. Mikhailenko; A. Barbe; J.J. Plateaux; Vl.G. Tyuterev 📂 Article 📅 1999 🏛 Elsevier Science 🌐 English ⚖ 198 KB

The 2600 -2900 cm Ϫ1 spectral range is revisited for an accurate determination of line intensities of the 2 1 ϩ 2 , 1 ϩ 2 ϩ 3 , and 2 ϩ 2 3 bands of ozone. The fit on 1702 energy levels of ( 012), (111), and (210) states determined from observed transitions with J max Յ 61 and K a max Յ 17 gives a r

Infrared Spectrum of Ozone in the 4600 a
✍ A. Barbe; J.J. Plateaux; S. Mikhailenko; Vl.G. Tyuterev 📂 Article 📅 1997 🏛 Elsevier Science 🌐 English ⚖ 334 KB

The very weak bands nu1 + 2nu2 + 3nu3 and 4nu1 + nu3 of 16O3 have been observed for the first time, using the Fourier transform spectrometer (FTS) of Reims and the usual experimental setup providing a large product p x l of approximately 38 Torr x 36 m. The upper levels of these A-type bands which a

Line Positions and Intensities of the ν1
✍ S. Mikhailenko; A. Barbe; Vl.G. Tyuterev; L. Regalia; J.J. Plateaux 📂 Article 📅 1996 🏛 Elsevier Science 🌐 English ⚖ 272 KB

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

H280Se: High-Resolution Study of the 2ν1
✍ J.M. Flaud; C. Camypeyret; P. Arcas; H. Burger; H. Willner 📂 Article 📅 1994 🏛 Elsevier Science 🌐 English ⚖ 449 KB

Using high-resolution Fourier transform spectra of monoisotopic \(\mathrm{H}_{2}{ }^{80} \mathrm{Se}\) recorded in the 1.8 and \(1.55-\mu \mathrm{m}\) regions. an extensive analysis of the \(2 \nu_{1}+\nu_{2}, \nu_{1}+\nu_{2}+\nu_{3}, 3 \nu_{1}, 2 \nu_{1}+\nu_{3}\), and \(\nu_{1}+\) \(2 v_{3}\) band

The ν1+ ν2+ 2ν3and ν2+ 3ν3Bands of16O3
✍ S. Bouazza; S. Mikhailenko; A. Barbe; L. Regalia; Vl.G. Tyuterev; J.J. Plateaux 📂 Article 📅 1995 🏛 Elsevier Science 🌐 English ⚖ 178 KB

The infrared spectra of 16 O 3 have been recorded in the 3700 cm 01 region, with a Fourier transform spectrometer at 0.008 cm 01 resolution. A White-type cell, ᐉ Å 32.16 m, filled with 42.8 Torr O 3 was used. This spectral region corresponds to the n 2 / 3n 3 and n 1 / n 2 / 2n 3 bands. The n 2 / 3n