Semi-empirical calculations of line-shape parameters and their temperature dependences for parallel bands of monodeuterated methane perturbed by nitrogen

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TitreSemi-empirical calculations of line-shape parameters and their temperature dependences for parallel bands of monodeuterated methane perturbed by nitrogen
Type de publicationJournal Article
Year of Publication2017
AuteursBuldyreva J., Lavrentieva N.N, Dudaryonok A.S
JournalJOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER
Volume203
Pagination355-366
Date PublishedDEC
Type of ArticleArticle
ISSN0022-4073
Mots-clésJ- and K-dependences, Monodeuterated methane, N-2-broadening coefficients, N-2-induced shifts, Outer planets, Planetary atmosphere, Semi-empirical calculation, Temperature dependence
Résumé

Theoretical nitrogen-pressure broadening and shift coefficients as well as their temperature-dependence characteristics for (CH3D)-C-12 (J, K) lines in the parallel (Delta K=0) nu(3) band are calculated by a semi-empirical approach based on analytical Anderson-type expressions corrected to account for the real curved trajectories. The parameters of the correction factor are adjusted on some recent experimental data for room-temperature line-broadening coefficients, and the unknown CH3D polarizability in the excited vibrational state is determined from a few measurements of room-temperature line-shifts. After validation by comparison with a set of measured values from the literature, this approach is employed for massive calculations of line-shape parameters for enlarged ranges of rotational quantum numbers (0 <= J <= 70, 0 <= K <= 20) requested by atmospheric/astrophysical applications and spectroscopic databases. The temperature-dependence characteristics are obtained for the range 200-400 K recommended for HITRAN. Given the negligible vibrational dependence of CH3D line-widths, our calculated broadening coefficients and their temperature-dependence exponents can be also used for other CH3D-N-2 parallel bands. (C) 2017 Elsevier Ltd. All rights reserved.

DOI10.1016/j.jqsrt.2017.02.014