Comparison of line-by-line and band models of near-IR methane absorption applied to outer planet atmospheres

Author:

Sromovsky L.A.,Fry P.M.,Boudon V.,Campargue A.,Nikitin A.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference47 articles.

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2. The near-IR spectrum of Titan modeled with an improved methane line list;Bailey;Icarus,2011

3. The abundances of methane and ortho/para hydrogen on Uranus and Neptune: Implications of New Laboratory 4–0 H2 quadrupole line parameters;Baines;Icarus,1995

4. Boudon, V., Nikitin, T., Gabard, T., Wegner, C., Rey, M., Tyuterev, V.G., 2011. Theoretical modelling of the methane absorption spectrum for planetary applications. EPSC Abstracts, EPSC-DPS2011-115 6, 00.

5. Temperature dependence of the absorption spectrum of CH4 by high resolution spectroscopy at 81K: (II) The icosad region (1.49–1.30μm);Campargue;J. Quant. Spectrosc. Radiat. Trans.,2010

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