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Vibrational dependence of line coupling and line mixing in self-broadened parallel bands of NH 3

机译:线耦合和线混合在NH 3 中的线耦合和线路混合中的振动依赖性

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AbstractLine coupling and line mixing effects have been calculated for several self-broadened NH3lines in parallel bands involving an excited ν2mode. It is well known that once the ν2mode is excited, the inversion splitting quickly increases as this quantum number increases. In the present study, we have shown that the ν2dependence of the inversion splitting plays a dominant role in the calculated line-shape parameters. For the ν2band with a 36cm?1splitting, the intra-doublet couplings practically disappear and for the 2ν2and 2ν2- ν2bands with much higher splitting values, they are completely absent. With respect to the inter-doublet coupling, it becomes the most efficient coupling mechanism for the ν2band, but it is also completely absent for bands with higher ν2quantum numbers. Because line mixing is caused by line coupling, the above conclusions on line coupling are also applicable for line mixing. Concerning the check of our calculated line mixing effects, while the present formalism has well explained the line mixing signatures observed in the ν1band, there are large discrepancies between the measured Rosenkranz mixing parameters and our calculated results for the ν2and 2ν2bands. In order to clarify these discrepancies, we propose to make some new measurements. In addition, we have calc
机译:<![cdata [ 抽象 线耦合和线路混合效果已经计算出几种自扩大的NH 3 并行带中的行涉及激励ν 2 模式。众所周知,一旦ν 2 模式是兴奋的,因此随着该量子数的增加,反转分离很快就会增加。在本研究中,我们已经表明,ν 2 反演分裂的依赖性在计算的线形参数中起着主导作用。对于ν 2 带36cm ?1 拆分,拆分耦合实际上消失,而且对于2¼ 2 和2ν 2 - ν 2 频带具有更高的分裂值,它们完全不存在。关于双际双击耦合,它成为ν 2 频段的最有效的耦合机制,但它也完全没有ν< CE:INF LOC =“POST”> 2 量子号。由于线路混合是由线耦合引起的,因此在线偶联的上述结论也适用于线混合。关于我们计算的线混合效果的检查,虽然目前的形式主义很好地解释了在ν 1 乐队中观察到的线混合签名,但在测量Rosenkranz混合参数和我们的计算结果为ν 2 和2ν 2 频带。为了澄清这些差异,我们建议进行一些新的测量。另外,我们有calc

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  • 作者

    Q. Ma; C. Boulet; R.H. Tipping;

  • 作者单位

    NASA/Goddard Institute for Space Studies and Department of Applied Physics and Applied Mathematics Columbia University;

    Institut des Sciences Moléculaires d’Orsay (ISMO) CNRS Univ. Paris-Sud Université Paris-Saclay;

    Department of Physics and Astronomy University of Alabama;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 光学;
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