HDO and H2O vertical distributions and isotopic ratio in the Venus mesosphere by Solar Occultation at Infrared spectrometer on board Venus Express

Author:

Fedorova A.,Korablev O.,Vandaele A.-C.,Bertaux J.-L.,Belyaev D.,Mahieux A.,Neefs E.,Wilquet W. V.,Drummond R.,Montmessin F.,Villard E.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference41 articles.

1. The analyser of space plasmas and energetic atoms (ASPERA-4) for the Venus Express mission;Barabash;Planet. Space Sci.,2007

2. Isotopic fractionation through water vapor condensation: The Deuteropause, a cold trap for deuterium in the atmosphere of Mars;Bertaux;J. Geophys. Res.,2001

3. SPICAV on Venus Express: Three spectrometers to study the global structure and composition of the Venus atmosphere;Bertaux;Planet. Space Sci.,2007

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

5. Airborne observations of the gas composition of Venus above the cloud tops: Measurements of H2O, HDO, HF, and the D/H and 18O/16O isotopic ratios;Bjoraker;Bull. Am. Astron. Soc.,1992

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