Photochemistry of Planetary Atmospheres
By R. Rodrigo, L. Lara. 2002
178 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/c07915e06b13d62922b202ef9b75663bf29552cc
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
In Atmospheric Science
- Jon Fortney
- James Schottelkotte
- E. Miller-Ricci
- J. Lustig-Yaeger
- Sara Seager
- M. Line
- J. Kasting
- D. Sasselov
Citations in the corpus
- THE ATMOSPHERIC SIGNATURES OF SUPER-EARTHS: HOW TO DISTINGUISH BETWEEN HYDROGEN-RICH AND HYDROGEN-POOR ATMOSPHERES (2008, methodology): “We obtain UV cross-sections for the major constituents of the atmosphere from Yung & Demore (1999).”
- ABIOTIC O2 LEVELS ON PLANETS AROUND F, G, K, AND M STARS: POSSIBLE FALSE POSITIVES FOR LIFE? (2015, background): “A good example is a planet interior to the habitable zone that loses its water by way of a runaway or moist greenhouse (Kasting 1988, 1997, 2010; Wordsworth & Pierrehumbert 2013).”
- CHARACTERIZING TRANSITING EXOPLANET ATMOSPHERES WITH JWST (2015, background): “These processes come in a variety of flavors including, but not limited to vertical and horizontal mixing (Prinn & Barshay 1977; Cooper & Showman 2006), photochemistry (Yung & Demore 1999), ion chemistry (Lavvas et al. 2008), and biology (e.g., Holland 1994).”