A photochemical model for the Venus atmosphere at 47–112 km

By V. Krasnopolsky. 2011

161 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/f7b3908daeb8c8df8c5dbd957231e3001b739957

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Aerospace Engineering

1. J. Lustig-Yaeger
2. David Crisp
3. A. Lincowski
4. Giada N. Arney
5. V. Meadows
6. T. Robinson
7. R. Luger

In Astronomy and Astrophysics

1. A. Lincowski
2. V. Meadows
3. J. Lustig-Yaeger
4. Giada N. Arney
5. David Crisp
6. N. Ignatiev
7. V. Wilquet
8. K. McGouldrick

Citations in the corpus

• Clouds and Hazes of Venus (2018, background): “26, potentially including hundreds of possible reactions (Krasnopolsky 2012; Zhang et al. 2012), produce sulphuric acid vapour in the middle atmosphere of Venus.”
• Evolved Climates and Observational Discriminants for the TRAPPIST-1 Planetary System (2018, methodology): “…is typically modeled in sections: by thermochemistry, which dominates the lower atmosphere below the cloud deck (e.g., Krasnopolsky 2013), and by photochemistry, which is responsible for the directly observable altitudes at and above the cloud deck (e.g., Krasnopolsky 2012; Zhang et al. 2012).”