Global fit analysis including the ν9+ν4-ν4 hot band of ethane:: Evidence of an interaction with the ν12 fundamental

被引:13
作者
Cooper, J. R. [1 ]
Moazzen-Ahmadi, N. [1 ]
机构
[1] Univ Calgary, Dept Phys & Astron, Calgary, AB T2N 1N4, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
vibration-torsion-rotation; infrared spectra; atronomical species; internal rotation;
D O I
10.1016/j.jms.2006.05.017
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 v(9) fundamental band of ethane occurs in the 12 pm region. It is the strongest band of ethane in a terrestrial window and is commonly used for the identification of ethane in the Jovian planets. The v(9) + v(4) - v(4) band occurs in the same region; neither can be analysed as an isolated band, since both are embedded in the torsional bath of the ground vibrational state. We report here two global fit models including data from both of these bands as well as the v(3) fundamental and the v(4), 2v(4) - v(4), and 3v(4) torsional transitions. The first is restricted to -5 <= K Delta K <= 15 in the hot band and gives an excellent fit to the included data. Three resonant interactions are identified in this fit-a Coriolis interaction with two resonant cases between the v9 torsional stack and that of the ground vibrational state (gs) and a resonant Fermi interaction between the v3 fundamental and the gs. Hot band lines with KAK < -5 are influenced by a fourth perturbation, with a crossing at -11 <= K Delta K <= -10, which has been attributed to an interaction with the v(12) fundamental. A second fit, demonstrating a promising treatment of this interaction, is also presented. (c) 2006 Elsevier Inc. All rights reserved.
引用
收藏
页码:51 / 58
页数:8
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