A layer of ozone detected in the nightside upper atmosphere of Venus-Reference-Cited by-同舟云学术

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A layer of ozone detected in the nightside upper atmosphere of Venus

Published:2011-11 Issue:1 Volume:216 Page:82-85
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Montmessin F.,Bertaux J.-L.,Lefèvre F.,Marcq E.,Belyaev D.,Gérard J.-C.,Korablev O.,Fedorova A.,Sarago V.,Vandaele A.C.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference26 articles.

1. Cloud structure on the dark side of Venus;Allen;Nature,1984

2. The temperature of the Venus mesosphere from O2 (a1Δg) airglow observations;Bailey;Icarus,2008

3. Mariner ultraviolet spectrometer;Barth;Science,1971

4. Introduction to the special section: Observations of the atmosphere of Mars with SPICAM spectrometers on board Mars Express;Bertaux;J. Geophys. Res.,2006

5. A warm layer in Venus’cryosphere and high-altitude measurements of HF, HCl, H2O and HDO;Bertaux;Nature,2007

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