Revisiting the Sulfur‐Water Chemical System in the Middle Atmosphere of Venus
Author:
Affiliation:
1. Department of Earth and Planetary Sciences University of California Santa Cruz CA USA
2. LESIA, Observatoire de Paris, PSL University, CNRS, Sorbonne University, University Sorbonne Paris City Meudon France
Funder
National Science Foundation
China Scholarship Council
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JE006195
Reference47 articles.
1. Vertical profiling of SO2 and SO above Venus’ clouds by SPICAV/SOIR solar occultations
2. A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO
3. Chemical Cycling in the Venusian Atmosphere: A Full Photochemical Model From the Surface to 110 km
4. Water vapor near Venus cloud tops from VIRTIS-H/Venus express observations 2006–2011
5. Water vapor near the cloud tops of Venus from Venus Express/VIRTIS dayside data
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