As outlined by Klapper et al., highly accurate rotational transition frequencies of 12C16O and also of the rare isotopomers of CO are desirable because this molecule has a great importance not only as a secondary calibration standard, covering the millimeter region up to the far infrared, but also in the atmospheric and astrophysical chemistry.
Cazzoli G., Dore L., Cludi L., Puzzarini C., Beninati S. (2002). Hyperfine structure of J = 1 ← 0 transition of 13CO. JOURNAL OF MOLECULAR SPECTROSCOPY, 215(1), 160-162 [10.1006/jmsp.2002.8604].
Hyperfine structure of J = 1 ← 0 transition of 13CO
Dore L.;Cludi L.;Puzzarini C.;Beninati S.
2002
Abstract
As outlined by Klapper et al., highly accurate rotational transition frequencies of 12C16O and also of the rare isotopomers of CO are desirable because this molecule has a great importance not only as a secondary calibration standard, covering the millimeter region up to the far infrared, but also in the atmospheric and astrophysical chemistry.File in questo prodotto:
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