Thermodynamic Constraints on the Lower Atmosphere of Venus-Reference-Cited by-同舟云学术

Thermodynamic Constraints on the Lower Atmosphere of Venus

Published:2017-08-21 Issue:7 Volume:1 Page:422-430
ISSN:2472-3452
Container-title:ACS Earth and Space Chemistry
language:en
Short-container-title:ACS Earth Space Chem.

Author:

Jacobson Nathan S.¹^ORCID,Kulis Michael¹,Radoman-Shaw Brandon²,Harvey Ralph²,Myers Dwight L.³,Schaefer Laura⁴,Fegley Bruce⁵

Affiliation:

1. NASA Glenn Research Center, Cleveland, Ohio 44135, United States

2. Case Western Reserve University, Cleveland, Ohio 44106, United States

3. East Central University, Ada, Oklahoma 74820, United States

4. Arizona State University, Tempe, Arizona 85281, United States

5. Washington University, St. Louis, Missouri 63130, United States

Funder

Division of Astronomical Sciences

National Aeronautics and Space Administration

Publisher

American Chemical Society (ACS)

Subject

Space and Planetary Science,Atmospheric Science,Geochemistry and Petrology

Link

https://pubs.acs.org/doi/pdf/10.1021/acsearthspacechem.7b00067

Reference64 articles.

1. Measurements of the Venus lower atmosphere composition: A comparison of results

2. Cloud structure on the dark side of Venus

3. Von Zahn, U.; Kumar, S.; Niemann, H.; Prinn, R.InVenus;Hunten, D. M.; Colin, L.; Donahue, T. M.; Moroz, V. I., Eds.University of Arizona Press:Tucson, AZ, 1983; pp299–429.

4. The composition of the atmosphere of Venus below 100km altitude: An overview

5. Composition of the atmosphere of Venus below the clouds

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