Analysis of Titan CH4 3.3μm upper atmospheric emission as measured by Cassini/VIMS-Reference-Cited by-同舟云学术

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Analysis of Titan CH4 3.3μm upper atmospheric emission as measured by Cassini/VIMS

Published:2011-08 Issue:2 Volume:214 Page:571-583
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

García-Comas Maya,López-Puertas Manuel,Funke Bernd,Dinelli Bianca M.,Luisa Moriconi Maria,Adriani Alberto,Molina Antonio,Coradini Angioletta

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference47 articles.

1. Ancillary data services of NASA’s Navigation and Ancillary Information Facility;Acton;Planet. Space Sci.,1996

2. Vertical profiles of HCN in Titan’s atmosphere from non-LTE emission at 3microns by Cassini/VIMS observations;Adriani;Icarus,2011

3. CH4 nonlocal thermodynamic equilibrium in the atmospheres of the giant planets;Appleby;Icarus,1990

4. Vibrational–vibrational and vibrational–translational/rotational processes in methane, oxygen gas-phase mixtures;Avramides;Mol. Phys.,1983

5. The atmospheres of Saturn and Titan in the near-infrared first results of Cassini/VIMS;Baines;Earth Moon Planets,2005

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