Chemical kinetic model for the lower atmosphere of Venus
By V. Krasnopolsky. 2007
155 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/b1d100e59c0bba2c12e52f654c899b2b32bce45b
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In Astronomy and Astrophysics
- V. Wilquet
- K. McGouldrick
- D. Titov
- N. Ignatiev
- V. Krasnopolsky
- J. Chaufray
- François Leblanc
- Jean-Loup Bertaux
In Atmospheric Science
Citations in the corpus
- Clouds and Hazes of Venus (2018, background): “This may be due to breakdown of cloud particles below the cloud deck (Krasnopolsky 2007).”
- A photochemical model for the Venus atmosphere at 47–112 km (2011, methodology): “This height is the upper boundary in the chemical kinetic model for the Venus lower atmosphere (Krasnopolsky, 2007), and some results of that model may be used as the lower boundary conditions in our model.”