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LED-based Fourier spectroscopy of HD17O in the range of 10000-11300 cm−1. Energy structure of (022), (102), (080), (400), (003), (211), (051), (131), (320), (032), (112) resonating states

•The absorption spectrum of the HD17O molecule have been studied in the range 10,000–11,300 cm−1 for the first time.•Centers and intensities of 1137 spectral lines of 12 vibrational bands of the HD17O molecule were obtained.•List of 364 experimental energy lines for 9 vibrational states (102), (080)...

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Published in:Journal of quantitative spectroscopy & radiative transfer 2023-12, Vol.310, p.108753, Article 108753
Main Authors: Sinitsa, L.N., Serdyukov, V.I., Polovtseva, E.P., Scherbakov, A.P., Bykov, A.D.
Format: Article
Language:English
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Summary:•The absorption spectrum of the HD17O molecule have been studied in the range 10,000–11,300 cm−1 for the first time.•Centers and intensities of 1137 spectral lines of 12 vibrational bands of the HD17O molecule were obtained.•List of 364 experimental energy lines for 9 vibrational states (102), (080), (400), (003), (211), (051), (131), (320), and (032) was compiled. We report our investigation of the HD17О absorption spectrum in the range of 10,000–11,300 cm−1. The measurements were performed using an IFS-125 M Fourier spectrometer with a resolution of 0.02 cm−1 at a pressure of 29 mbar and an optical path length of 2400 cm. An EDEN-1L53 LED was used as a light source giving a maximum radiation intensity in the region of 0.95 µm. The absorption spectrum was analyzed using a set of software programs capable of searching for spectral lines, fitting line parameters, and making line assignments. As a result of the analysis, experimental information was obtained for the first time on the parameters of 1137 spectral lines assigned to 12 vibrational bands of HD17О, and 364 vibrational-rotational energy levels of the (022), (102), (080), (400), (003), (211), (051), (131), (320), (032), and (112) vibrational states were determined. The obtained experimental results are compared with calculated data.
ISSN:0022-4073
1879-1352
DOI:10.1016/j.jqsrt.2023.108753