Photochemistry of Saturn's Atmosphere: II. Effects of an Influx of External Oxygen

By J. Moses, E. Lellouch, B. Bézard, G. Gladstone, H. Feuchtgruber, M. Allen. 2000

138 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/fda9236b762170f32ed6eb7c959259d723b8b87e

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Citations in the corpus

• VULCAN: An Open-source, Validated Chemical Kinetics Python Code for Exoplanetary Atmospheres (2016, unknown): “…1992BAU/COB411-429 NIST 1986TSA/HAM1087 R241 H + C2H2 + M −−→ C2H3 + M k0 = 1.05×10 −07 T−7.270 exp(−3630.0/T ) k∞ = 9.13×10−12 exp(−1220.0/T ) NIST 1986TSA/HAM1087 NIST 1984WAR197C R243 H + C2H3 + M −−→ C2H4 + M k0 = 1.50×10 −11 k∞ = 6.40×10−11 T 0.200 Fahr et al.(1991) Harding et al.(2005)…”
• Photochemistry and diffusion in Jupiter's stratosphere: Constraints from ISO observations and comparisons with other giant planets (2005, methodology): “[47] Gladstone et al. [1996] [see also Moses et al., 2000a; Summers and Strobel, 1989; Romani and Atreya, 1988] have performed general sensitivity studies to illustrate how hydrocarbon mixing ratios change with such factors as the overall magnitude of Kh, the slope of the eddy diffusion…”
• Dynamics and Disequilibrium Carbon Chemistry in Hot Jupiter Atmospheres, with Application to HD 209458b (2006, background): “First, photochemical dissociation can elevate the concentrations of phtochemical products above equilibrium levels (Moses et al. 2000).”
• DISEQUILIBRIUM CARBON, OXYGEN, AND NITROGEN CHEMISTRY IN THE ATMOSPHERES OF HD 189733b AND HD 209458b (2011, background): “The molecular diffusion coefficients are described in Moses et al. (2000a).”
• The deuterium abundance in Jupiter and Saturn from ISO-SWS observations (2001, methodology): “At pressures less than 0.4 mbar, the temperature profile was primarily based on stellar occultation measurements (Hubbard et al. 1997; see Moses et al. 2000b).”