The abundance of CH3D in the atmosphere of Titan, derived from 8- to 14-μm thermal emission
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference41 articles.
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1. Measurement of CH3D on Titan at Submillimeter Wavelengths;The Astronomical Journal;2019-05-07
2. Temperature-dependent high resolution absorption cross sections of propane;Journal of Quantitative Spectroscopy and Radiative Transfer;2016-10
3. Temperature dependences of self- and N-2-broadened line-shape parameters in the nu(3) and nu(5) bands of (CH3D)-C-12: Measurements and calculations;J QUANT SPECTROSC RA;2016
4. Temperature dependences of N2-broadening and shift coefficients in the ν6 perpendicular band of 12CH3D;Journal of Quantitative Spectroscopy and Radiative Transfer;2015-09
5. FT-IR measurements of cold C3H8 cross sections at 7–15μm for Titan atmosphere;Icarus;2013-11
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