New assignments in the 2 μm transparency window of the 12CH4 Octad band system

被引:59
作者
Daumont, L. [1 ]
Nikitin, A. V. [1 ,2 ]
Thomas, X. [1 ]
Regalia, L. [1 ]
Von der Heyden, P. [1 ]
Tyuterev, VI. G. [1 ]
Rey, M. [1 ]
Boudon, V. [3 ]
Wenger, Ch. [3 ]
Loete, M. [3 ]
Brown, L. R. [4 ]
机构
[1] Univ Reims, UFR Sci Exactes & Nat, UMR CNRS 6089, Grp Spectromet Mol & Atmospher, F-51687 Reims 2, France
[2] SB RAS, VE Zuev Inst Atmospher Opt, Lab Theoret Spect, Tomsk 634021, Russia
[3] Univ Bourgogne, CNRS, UMR 5209, Lab Interdisciplinaire Carnot Bourgogne, F-21078 Dijon, France
[4] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
Methane; Intensities; Spectra; Transparency window; Titan; Long path FTS; Octad; EMPIRICAL LINE PARAMETERS; POLYATOMIC-MOLECULES; CM(-1) REGION; SPECTROSCOPIC DATABASE; 1ST ASSIGNMENT; METHANE; SPECTRA; STRENGTHS; TRANSITIONS; SIMULATION;
D O I
10.1016/j.jqsrt.2012.08.025
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
This paper reports new assignments of rovibrational transitions of (CH4)-C-12 bands in the range 4600-4887 cm(-1) which is usually referred to as a part of the 2 mu m methane transparency window. Several experimental data sources for methane line positions and intensities were combined for this analysis. Three long path Fourier transform spectra newly recorded in Reims with 1603 m absorption path length and pressures of 1,7 and 34 hPa for samples of natural abundance CH4 provided new measurements of (CH4)-C-12 lines. Older spectra for (CH4)-C-13 (90% purity) from JPL with 73 m absorption path length were used to identify the corresponding lines. Most of the lines in this region belong to the Octad system of (CH4)-C-12. The new spectra allowed us to assign 1014 new line positions and to measure 1095 line intensities in the cold bands of the Octad. These new line positions and intensities were added to the global fit of Hamiltonian and dipole moment parameters of the Ground State, Dyad, Pentad and Octad systems. This leads to a noticeable improvement of the theoretical description in this methane transparency window and a better global prediction of the methane spectrum. (C) 2012 Elsevier Ltd. All rights reserved.
引用
收藏
页码:101 / 109
页数:9
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