𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Stratospheric NO_2 retrieval from solar absorption spectra in the ν_3 and ν_1 + ν_3 infrared bands

✍ Scribed by Coffey, M. T. ;Mankin, William G. ;Goldman, A.

Book ID
115334393
Publisher
The Optical Society
Year
1986
Tongue
English
Weight
791 KB
Volume
25
Category
Article
ISSN
1559-128X

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

The 3ν1 and ν1 + 3ν3 − ν2 Absorption Ban
The 3ν1 and ν1 + 3ν3 − ν2 Absorption Bands of 16O3
✍ S. Bouazza; A. Barbe; J.J. Plateaux; J.M. Flaud; C. Camypeyret 📂 Article 📅 1993 🏛 Elsevier Science 🌐 English ⚖ 240 KB

Using a high-pressure \(\times\) path length sample of ozone it has been possible to record at high resolution ( \(0.006 \mathrm{~cm}^{-1}\) ) the \(3-\mu \mathrm{m}\) absorption region of this molecule. A thorough analysis of the spectra has been performed allowing one to assign for the first time

Infrared Spectrum of Ozone in the 4600 a
Infrared Spectrum of Ozone in the 4600 and 5300 cm−1Regions: High Order Accidental Resonances through the Analysis of ν1+ 2ν2+ 3ν3− ν2, ν1+ 2ν2+ 3ν3, and 4ν1+ ν3Bands
✍ 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

High-Resolution Infrared Spectra of the
High-Resolution Infrared Spectra of the ν2, ν3, ν4, and 2ν3 Bands of 32S16O3
✍ Arthur Maki; Thomas A. Blake; Robert L. Sams; Nicolae Vulpanovici; Jeffrey Barbe 📂 Article 📅 2001 🏛 Elsevier Science 🌐 English ⚖ 183 KB

New measurements are reported for the infrared spectrum of sulfur trioxide, 32 S 16 O 3 , with resolutions ranging from 0.0015 cm -1 to 0.0025 cm -1 . Rovibrational constants have been measured for the fundamentals ν 2 , ν 3 , and ν 4 and the overtone band 2ν 3 . Comparisons are made with the earlie