The present analysis substantially improves the spectroscopic characterization of near infrared OCS in a window region (3850-4200 cm À1 ) important for atmospheric studies of Venus. Previous studies in this spectral region cataloged numerous OCS line positions, but accurate line intensities were mea
Measurements of line positions and strengths of HD18O and D218O in the 2500–4280 cm−1 region
✍ Scribed by Robert A. Toth
- Publisher
- Elsevier Science
- Year
- 2005
- Tongue
- English
- Weight
- 234 KB
- Volume
- 742
- Category
- Article
- ISSN
- 0022-2860
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Continuing the systematic study of ozone high-resolution infrared spectra, we present in this paper the measurements and analyses of line positions for the 18 O 16 O 18 O isotopomer. In the range 900-5000 cm À1 , corresponding to the observed spectra, 15 bands are analysed: and5m 3 . As in the case
High-resolution spectra of gas mixtures of HDO, D 2 O, and H 2 O were obtained with a Fourier-transform spectrometer with path lengths up to 433 m. The spectra were analyzed to obtain line positions and strengths of over 6000 transitions of HDO and D 2 O. For HDO, these included the (000)-( 000), (