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The acetylene spectrum in the 1.45 μm window (6627-7065 cm-1)
被引:4
作者:
Lyulin, O.
[1
,2
]
Vasilchenko, S.
[1
,2
]
Mondelain, D.
[1
]
Kassi, S.
[1
]
Campargue, A.
[1
]
机构:
[1] Univ Grenoble Alpes, LIPhy, CNRS, F-38000 Grenoble, France
[2] VE Zuev Inst Atmospher Opt SB RAS, 1 Academician Zuev Sq, Tomsk 634055, Russia
基金:
俄罗斯科学基金会;
关键词:
Acetylene;
C2H2;
Line intensity;
CRDS;
Spectroscopic database;
HITRAN;
OUTER SOLAR-SYSTEM;
TRANSFORM ABSORPTION-SPECTRUM;
LINE INTENSITY MEASUREMENTS;
MONODEUTERATED METHANE;
M REGION;
SPECTROSCOPIC DATABASE;
HIGH-RESOLUTION;
(C2H2)-C-12;
CRDS;
ABUNDANCE;
D O I:
10.1016/j.jqsrt.2020.107057
中图分类号:
O43 [光学];
学科分类号:
070207 ;
0803 ;
摘要:
The high-resolution absorption spectrum of acetylene has been recorded at room temperature by high sensitivity cavity ring down spectroscopy (CRDS) in the 6627-7065 cm(-1) region. The studied spectral range corresponds to a spectral interval of very weak absorption (an acetylene transparency window). The positions and intensities of more than 6500 lines are determined in the considered interval where previous intensity information was mostly missing. On the basis of previous studies and on effective Hamiltonian predictions, 3062 (C2H2)-C-12 462 (C13CH2)-C-12 and 104 (C2HD)-C-12 absorption lines belonging to a total of 123 vibrational bands are assigned. For comparison, the HITRAN2016 database provides line parameters of only ten (C2H2)-C-12 bands in the same region. Spectroscopic parameters of 113 upper vibrational levels were derived from standard band-by-band fits of the line positions (typical rms values of the (obs.-calc.) deviations are better than 0.003 cm(-1)). Many bands are found to be affected by perturbations. The vibrational transition dipole moment squared and Herman-Wallis coefficients of 47 bands were derived from a fit of the measured intensity values. In order to generate a recommended line list in the region, the derived spectroscopic parameters and Herman-Wallis coefficients were used to compute the line parameters for these 47 bands while experimental position and intensity values were kept for the other bands. Overall, the obtained recommended list including a total of 5260 transitions will help to fill a spectral gap around 1.47 mu m where very scarce spectroscopic information is provided in the current spectroscopic databases. When compared to the HITRAN list in the region, some important deviations concerning both line positions and line intensities are evidenced as a result of inaccurate high J extrapolations. (C) 2020 Elsevier Ltd. All rights reserved.
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