The abundance, vertical distribution and origin of H2O in Titan’s atmosphere: Herschel observations and photochemical modelling-Reference-Cited by-同舟云学术

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The abundance, vertical distribution and origin of H2O in Titan’s atmosphere: Herschel observations and photochemical modelling

Published:2012-11 Issue:2 Volume:221 Page:753-767
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Moreno Raphael,Lellouch Emmanuel,Lara Luisa M.,Feuchtgruber Helmut,Rengel Miriam,Hartogh Paul,Courtin Régis

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference76 articles.

1. Titan’s aerosol and stratospheric ice opacities between 18 and 500μm: Vertical and spectral characteristics from Cassini CIRS;Anderson;Icarus,2011

2. Composition and chemistry of Titan’s stratosphere;Bézard;R. Soc. Lond. Philos. Trans. Ser. A,2009

3. Carbon monoxide on Jupiter: Evidence for both internal and external sources;Bézard;Icarus,2002

4. Collision-induced rototranslational absorption spectra of N2–N2 pairs for temperatures from 50 to 300 K;Borysow;Astrophys. J.,1986

5. Collision-induced rototranslational absorption spectra of CH4–CH4 pairs at temperatures from 50 to 300K;Borysow;Astrophys. J.,1987

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