Analyses of FT spectra of C2v ozone isotopologues in the 4500-5700 cm-1 region: 16O18O16O, 18O16O18O and 18O3

被引:4
作者
Barbe, A. [1 ]
De Backer, M. -R. [1 ]
Starikova, E. [2 ,3 ]
Thomas, X. [1 ]
Tyuterev, Vl. G. [1 ]
机构
[1] UFR Sci Exactes & Nat, Grp Spectrometr Mol & Atmospher, UMR CNRS 7331, F-51687 Reims 2, France
[2] SB RAS, VE Zuev Inst Atmospher Opt, Lab Theoret Spect, Tomsk 634021, Russia
[3] Tomsk State Univ, Lab Quantum Mech Mol & Radiat Proc, Tomsk 634050, Russia
关键词
Ozone isotopologues; Fourier transform spectroscopy; Resonance coupling; Effective Hamiltonian model; Vibrational predictions; HIGH-RESOLUTION SPECTRA; CW-CRDS SPECTRA; FOURIER-TRANSFORM SPECTROMETER; O-16/O-18; ISOTOPOLOGUES; LINE POSITIONS; CAVITY RING; INFRARED-SPECTRUM; SPECTROSCOPY; BANDS; MOLECULE;
D O I
10.1016/j.jqsrt.2014.07.018
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
This work continues the systematic investigation of high resolution infrared spectra of O-18 enriched ozone isotopologues in the 4500-6300 cm(-1) spectral range. So far, the (OOO)-O-16-O-18-O-16 and (OOO)-O-18-O-16-O-18 spectra have been recorded and analysed using Fourier Transform Spectrometer (FTS) below 5000 cm(-1) and using high sensitivity Cavity Ring-Down Spectroscopy above 6000 cm(-1). In order to fill the gap between 5000 and 6000 cm(-1), new infrared spectra were recorded with the Reims FTS. The analyses of the 2v(1)+v(2)+3v(3) band of (OOO)-O-16-O-18-O-16 and of the 5v(3), v(1)+2v(2)+3v(3) and v(1)+5v(3) bands of (OOO)-O-18-O-16-O-18 are reported. New v(1)+2v(2)+3v(3) and v(1)+5v(3) bands of O-18(3) were also observed and analysed. Observed line positions were fitted using effective Hamiltonian models accounting for the dark state perturbations. The derived band centres and rotational constants are in a good agreement with new theoretical calculations from the molecular potential function. (C) 2014 Elsevier Ltd. All rights reserved.
引用
收藏
页码:51 / 63
页数:13
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