Semi-empirical calculations of line-shape parameters and their temperature dependences for the ν6 band of CH3D perturbed by N2
- 1. V.E. Zuev Institute of Atmospheric Optics, Siberian Branch of the Russian Academy of Sciences, 1 Akademishian Zuev square, 634021 Tomsk (Russian Federation)
- 2. Institut UTINAM, UMR 6213 CNRS, Université Bourgogne Franche-Comté, 16 Route de Gray, 25030 Besançon cedex (France)
Description
Highlights: • Calculations of CH3D–N2 line widths and shifts for large ranges of quantum numbers. • Theoretical evaluation of temperature-dependence parameters for widths and shifts. • Theoretical line-lists for collisional widths, shifts and their temperature dependences. (J, K)-line broadening and shift coefficients with their temperature-dependence characteristics are computed for the perpendicular (ΔK = ±1) ν6 band of the 12CH3D-N2 system. The computations are based on a semi-empirical approach which consists in the use of analytical Anderson-type expressions multiplied by a few-parameter correction factor to account for various deviations from Anderson's theory approximations. A mathematically convenient form of the correction factor is chosen on the basis of experimental rotational dependencies of line widths, and its parameters are fitted on some experimental line widths at 296 K. To get the unknown CH3D polarizability in the excited vibrational state v6 for line-shift calculations, a parametric vibration-state-dependent expression is suggested, with two parameters adjusted on some room-temperature experimental values of line shifts. Having been validated by comparison with available in the literature experimental values for various sub-branches of the band, this approach is used to generate massive data of line-shape parameters for extended ranges of rotational quantum numbers (J up to 70 and K up to 20) typically requested for spectroscopic databases. To obtain the temperature-dependence characteristics of line widths and line shifts, computations are done for various temperatures in the range 200–400 K recommended for HITRAN and least-squares fit procedures are applied. For the case of line widths strong sub-branch dependence with increasing K is observed in the R- and P-branches; for the line shifts such dependence is stated for the Q-branch.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.jqsrt.2018.03.006Additional details
Identifiers
- DOI
- 10.1016/j.jqsrt.2018.03.006;
- PII
- S0022407317308890;
Publishing Information
- Journal Title
- Journal of Quantitative Spectroscopy and Radiative Transfer
- Journal Volume
- 212
- Journal Page Range
- p. 75-87
- ISSN
- 0022-4073
- CODEN
- JQSRAE
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 53005600
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- APPROXIMATIONS; LEAST SQUARE FIT; LINE BROADENING; LINE WIDTHS; METHANE; POLARIZABILITY; QUANTUM NUMBERS; SHAPE; TEMPERATURE DEPENDENCE; TEMPERATURE RANGE 0273-0400 K
- Descriptors DEC
- ALKANES; CALCULATION METHODS; ELECTRICAL PROPERTIES; HYDROCARBONS; MATHEMATICAL SOLUTIONS; MAXIMUM-LIKELIHOOD FIT; NUMERICAL SOLUTION; ORGANIC COMPOUNDS; PHYSICAL PROPERTIES; TEMPERATURE RANGE
Optional Information
- Copyright
- Copyright (c) 2018 Elsevier Ltd. All rights reserved.