The deep atmosphere of Venus and the possible role of density-driven separation of CO2 and N2

Author:

Lebonnois SebastienORCID,Schubert Gerald

Publisher

Springer Science and Business Media LLC

Subject

General Earth and Planetary Sciences

Reference51 articles.

1. Crisp, D. & Titov, D. in Venus II, Geology, Geophysics, Atmosphere, and Solar Wind Environment (eds Bougher, S. W., Hunten, D. M. & Phillips, R. J.) 353–384 (Univ. Arizona Press, 1997).

2. von Zahn, U., Kumar, S., Niemann, H. & Prinn, R. in Venus (eds Hunten, D. M., Colin, L., Donahue, T. M. & Moroz, V. I.) 299–430 (Univ. Arizona Press, 1983).

3. Taylor, F. W., Crisp, D. & Bézard, B. in Venus II, Geology, Geophysics, Atmosphere, and Solar Wind Environment (eds Bougher, S. W., Hunten, D. M. & Phillips, R. J.) 325–351 (Univ. Arizona Press, 1997).

4. de Bergh, C. et al. The composition of the atmosphere of Venus below 100 km altitude: an overview. Planet. Space Sci. 54, 1389–1397 (2006).

5. Esposito, L. W., Knollenberg, R. G., Marov, M. I., Toon, O. B. & Turco, R. P. The Clouds and Hazes of Venus 484–564 (Univ. Arizona Press, 1983).

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