CW-cavity ringdown spectroscopy of carbon dioxide isotopologues near 1.5 μm

被引:69
作者
Perevalov, B. V.
Kassi, S.
Romanini, D.
Perevalov, V. I.
Tashkun, S. A.
Campargue, A.
机构
[1] Univ Grenoble 1, CNRS, UMR 5588, Spectrometrie Phys Lab, F-38402 St Martin Dheres, France
[2] Russian Acad Sci, Inst Atmospher Phys, Lab Theoret Spect, Tomsk 634055, Russia
基金
俄罗斯基础研究基金会;
关键词
carbon dioxide; CO2; cavity ring down spectroscopy; CRDS; effective Hamiltonian;
D O I
10.1016/j.jms.2006.05.009
中图分类号
O64 [物理化学(理论化学)、化学物理学]; O56 [分子物理学、原子物理学];
学科分类号
070203 ; 070304 ; 081704 ; 1406 ;
摘要
The absorption spectra of carbon dioxide in natural isotopic abundance and with 99% enrichment in C-13 have been recorded by CW-cavity ringdown spectroscopy in two specific spectral regions: 5957-6122 and 6745-6833 cm(-1). The spectra were obtained at Doppler limited resolution by using a CW-CRDS spectrometer based on fibered DFB lasers. The typical sensitivity of 5 x 10(-1) cm(-1), allowed for the detection of lines with intensity as weak as 5 x 10-29 cm/molecule. More than 2900 line positions of the six major isotopologues contributing to the spectra ((CO2)-C-12-O-16, (OCO)-O-16-C-12-O-17, (OOO)-O-16-O-12-O-18, (CO2)-C-13-O-16, (OCO)-O-16-C-13-O-17 and (OCO)-O-16-C-13-O-18), were measured and assigned on the basis of their respective global effective Hamiltonian models. For comparison, only 507 lines are provided by the HITRAN database in these spectral regions. The band by band analysis has led to the determination of the rovibrational parameters of a total of 52 bands, 30 of them being newly reported. Most of the observed line positions show an agreement close to the experimental uncertainty (1-2 x 10(-3) cm(-1)) with the predictions of their respective effective Hamiltonian models. However, the quality of the predictions degrades for the minor isotopologues reaching maximum deviations of 0.35 cm(-1) in one specific case. For several bands, rovibrational transitions with J values between 60 and 90 could be newly detected. While an excellent agreement is observed with the line positions predicted by the Hamiltonian models, the comparison of these observations with the line positions listed in the HITRAN database or extrapolated by using the best FTS rotational constants available in the literature has evidenced significant deviations. (c) 2006 Elsevier Inc. All rights reserved.
引用
收藏
页码:241 / 255
页数:15
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