Semi-empirical calculation of 12CH3D-H2 broadening coefficients and their temperature-dependence exponents for rovibrational lines in parallel bands-Reference-Cited by-同舟云学术

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Semi-empirical calculation of 12CH3D-H2 broadening coefficients and their temperature-dependence exponents for rovibrational lines in parallel bands

Published:2019-05 Issue: Volume:229 Page:157-165
ISSN:0022-4073
Container-title:Journal of Quantitative Spectroscopy and Radiative Transfer
language:en
Short-container-title:Journal of Quantitative Spectroscopy and Radiative Transfer

Author:

Dudaryonok A.S.,Lavrentieva N.N.,Buldyreva J.

Funder

LIA SAMIA

Russian Foundation of Fundamental Research

Publisher

Elsevier BV

Subject

Spectroscopy,Atomic and Molecular Physics, and Optics,Radiation

Reference24 articles.

1. Methane and its isotopologues on Saturn from Cassini/CIRS observations;Fletcher;Icarus,2009

2. Parameterization of radiative heating and cooling rates in the atmosphere of Jupiter;Kuroda;Icarus,2014

3. The application of new methane line absorption data to Gemini-N/NIFS and KPNO/FTS observations of Uranus’ near-infrared spectrum;Irwin;Icarus,2012

4. Titan's atmosphere as observed by Cassini/VIMS solar occultations: CH4, CO and evidence for C2H6 absorption;Maltagliati;Icarus,2015

5. Monodeuterated methane in the outer solar system. I Spectroscopic analysis of the bands at 1.55 and 1.95 microns;Lutz;Astrophys J,1983

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