New High-Resolution Analysis of the 3ν3 and 2ν1 + ν3 Bands of Nitrogen Dioxide (NO2) by Fourier Transform Spectroscopy
New High-Resolution Analysis of the 3ν3 and 2ν1 + ν3 Bands of Nitrogen Dioxide (NO2) by Fourier Transform Spectroscopy
复制标题
利用傅里叶变换光谱法对二氧化氮 (NO2) 的 3ν3 和 2ν1 + ν3 谱带进行新的高分辨率分析
DOI:
10.1006/jmsp.2000.8064
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发表时间:
2000
影响因子:
1.4
通讯作者:
C. Rinsland
中科院分区:
文献类型:
--
作者:
T. Stephen;A. Goldman;A. Perrin;J. Flaud;F. Keller;C. Rinsland
Abstract Using new high-resolution Fourier transform spectra recorded at the University of Denver in the 2-μm region, a new and more extended analysis of the 2ν 1 + ν 3 and 3ν 3 bands of nitrogen dioxide, located at 4179.9374 and 4754.2039 cm −1 , respectively, has been performed. The spin–rotation energy levels were satisfactorily reproduced using a theoretical model that takes into account both the Coriolis interactions between the spin–rotation energy levels of the (201) vibrational “bright” state with those of the (220) “dark” state. The interactions between the (003) bright state with the (022) dark state were similarly treated. The spin–rotation resonances within each of the NO 2 vibrational states were also taken into account. The precise vibrational energies and the rotational, spin–rotational, and coupling constants were obtained for the two dyads {(220), (201)} and {(022), (003)} of the 14 N 16 O 2 interacting states. From the experimental line intensities of the 2ν 1 + ν 3 and 3ν 3 bands, a determination of their vibrational transition moment constants was performed. A comprehensive list of line positions and line intensities of the {2ν 1 + 2ν 2 , 2ν 1 + ν 3 } and the {2ν 2 + 2ν 3 , 3ν 3 } interacting bands of 14 N 16 O 2 was generated. In addition, assuming the harmonic approximation and using the Hamiltonian constants derived in this work and in previous studies (A. Perrin, J.-M. Flaud, A. Goldman, C. Camy-Peyret, W. J. Lafferty, Ph. Arcas, and C. P. Rinsland, J. Quant. Spectrosc. Radiat. Transfer 60, 839–850 (1998)), we have generated synthetic spectra for the {(022), (003)}–{(040), (021), (002)} hot bands at 6.3 μm and for the {(220), (201)}–{(100), (020), (001)} hot bands at 3.5 μm, which are in good agreement with the observed spectra.