CRDS detection and modelling of vibrational bands of 18O3 approaching the dissociation threshold (7400–7920 cm−1). (August 2015)

• Record Type: Journal Article
• Authors: Starikova, E.; Mondelain, D.; Barbe, A.; Tyuterev, Vl.G.; Kassi, S.; Campargue, A.
• Is Part Of: Journal of quantitative spectroscopy & radiative transfer. Volume 161(2015:Nov.)
• Page Start: 203
• Page End: 214
• Publication Date: 2015-08
• Subjects: Ozone -- 18O3 -- Cavity Ring Down Spectroscopy -- Effective Hamiltonian model; Spectrum analysis -- Periodicals; Radiation -- Periodicals; Analyse spectrale -- Périodiques; Rayonnement -- Périodiques; Radiation; Spectrum analysis; Periodicals; 543.0858
• DOI: 10.1016/j.jqsrt.2015.04.001
• Languages: English
• ISSNs: 0022-4073

Abstract

Abstract: The absorption spectrum of the 18 O3 isotopologue of ozone is recorded by CW-Cavity Ring Down Spectroscopy between 7400 and 7920 cm −1 . The typical noise equivalent absorption of the recordings is α min ≈1×10 −10 cm −1 allowing for the detection of extremely weak vibrational bands located only a few % below the dissociation limit. The absorption spectrum also includes the weak 3 A2 (000)–X(110) hot vibronic band at 7877.53 cm −1 affected by predissociation broadening. Overall, about 1000 lines were rovibrationnally assigned to six vibrational bands. Their line positions were modelled using effective Hamiltonian models covering three vibrational interacting systems and involving several "dark" states perturbing observed transitions. Line positions could be reproduced with rms deviations on the order of 0.01 cm −1 . The dipole transition moment parameters of the six bands were determined from the retrieved line intensities. The obtained set of effective parameters and the experimentally determined energy levels were used to generate a list of 1461 transitions provided asSupplementary materials . Highlights: Cavity Ring Down Spectroscopy of 18 O3 between 7400 and 7920 cm −1 . 1017 Transitions assigned to six A-type vibrational bands. Upper vibrational states located a few % below the dissociation limit at 8560 cm −1 . Effective operator modelling of the spectra. Good agreement with ab initio values for the band centres and rotational constants.