High sensitivity cw-cavity ringdown and Fourier transform absorption spectroscopies of 13CO2

被引:78
作者
Ding, Y
Macko, P
Romanini, D
Perevalov, VI
Tashkun, SA
Teffo, JL
Hu, SM
Campargue, A
机构
[1] Univ Grenoble 1, CNRS UMR 5588, Spectrometrie Phys Lab, F-38402 St Martin Dheres, France
[2] Univ Sci & Technol China, Lab Bond Select Chem, Hefei 230026, Peoples R China
[3] Comenius Univ, Fac Math Phys & Informat, Bratislava 84248, Slovakia
[4] Russian Acad Sci, SB, Inst Atmospher Opt, Lab Theoret Spectroscopy, Tomsk 634055, Russia
[5] Univ Paris 06, CNRS, Lab Phys Mol & Applicat, F-75252 Paris 05, France
基金
中国国家自然科学基金; 俄罗斯基础研究基金会;
关键词
(CO2)-C-13; cavity ringdown spectroscopy; Fourier transform spectroscopy; effective Hamiltonian model;
D O I
10.1016/j.jms.2004.03.009
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 spectrum of (CO2)-C-13 has been recorded by cw-cavity ringdown spectroscopy with a new set up based on fibered DFB lasers. By using a series of 31 DFB lasers, the spectrum of carbon dioxide could be recorded in the 6130-6750 cm(-1) region with a typical sensitivity of 5 x 10(-10) cm(-1). The spectrum has also been recorded between 4400 and 8500 cm(-1) with a Fourier transform spectrometer associated with a multi-pass cell (maximum path length of 105 in). The new observations obtained both by FTS and CRDS represent a significant extension of the available data. For instance, more than 4000 line positions were measured and assigned in the CRDS spectrum while only 232 line positions are listed in the HITRAN database. Altogether, the band by band analysis has led to the determination of the rovibrational parameters of 65, 7, and 24 bands for the (CO2)-C-13-O-16, (OCO)-O-16-C-13-O-17, and (OCO)-O-16-C-13-O-18 isotopomers, respectively. As some observed line positions show significant deviations from the predictions of the effective Hamiltonian model, the new observed line positions were gathered with the data available in the literature to refine the set of effective Hamiltonian parameters of the (CO2)-C-13-O-16 isotopic species. The refined set of 96 effective Hamiltonian parameters reproduces more than 14 650 line positions of (CO2)-C-13-O-16 with an RMS = 0.002 cm(-1). A detailed comparison with the line positions retrieved from Venus spectra and the line list provided by HITRAN is also presented and discussed. (C) 2004 Elsevier Inc. All rights reserved.
引用
收藏
页码:146 / 160
页数:15
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