Photochemistry and diffusion in Jupiter's stratosphere: Constraints from ISO observations and comparisons with other giant planets

By J. Moses, T. Fouchet, B. Bézard, G. Gladstone, E. Lellouch, H. Feuchtgruber. 2005

203 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/38a803aee2ddfa121a7eb0f867fe09cf20bff2f9

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

1. Jon Fortney
2. N. Madhusudhan
3. M. Marley
4. A. Showman
5. M. Line
6. Laura Kreidberg
7. Michael C. Liu
8. J. D'esert

In Atmospheric Science

1. M. Marley
2. Jon Fortney
3. A. Showman
4. D. Saumon
5. Michael C. Liu
6. N. Madhusudhan
7. T. Dupuy
8. J. D'esert

Citations in the corpus

• Synthetic Spectra and Colors of Young Giant Planet Atmospheres: Effects of Initial Conditions and Atmospheric Metallicity (2008, background): “There is also a long history of modeling non-equilibrium chemistry in Jupiter,and recent estimates ofKzz in Jupiter’s radiative atmosphere range from 102 to 104 (Bézard et al. 2002; Moses et al. 2005).”
• NEAR-INFRARED SPECTROSCOPY OF THE EXTRASOLAR PLANET HR 8799 b (2010, background): “The gas giants in our solar system have moderate values of Kzz in their stratospheres (∼102–105 cm2 s−1; Saumon et al. 2006)14 with substantially 14 Note that Kzz is much higher in the convective regions of solar system giant planetary atmospheres than the radiative zone, reaching values of ∼106–109”
• NO THERMAL INVERSION AND A SOLAR WATER ABUNDANCE FOR THE HOT JUPITER HD 209458B FROM HST/WFC3 SPECTROSCOPY (2016, methodology): “…approach taken within the solar system community: molecular abundances (or their profiles) are directly retrieved from the data (whether in situ or remotely) and then compared to chemical models (e.g., Moses et al. 2005; Greathouse et al. 2005; Visscher, Moses, & Saslow 2010; Orton et al. 2014).”
• VULCAN: An Open-source, Validated Chemical Kinetics Python Code for Exoplanetary Atmospheres (2016, unknown): “…NIST 1992BAU/COB411-429 NIST R233 H + O+ M −−→ OH+ M k0 = 1.30×10−29 T−1.000 k∞ = 1.00×10−11 NIST 1986TSA/HAM1087 Moses et al.(2011) R235 OH+ H + M −−→ H2O+ M k0 = 3.89×10 −25 T−2.000 k∞ = 4.26×10−11 T−0.230 NIST 1992BAU/COB411-429 NIST 2008SEL/GEO5085-5095 R237 H + CH+ M −−→ CH2 + M k0 =…”
• Planetary Spectrum Generator: An accurate online radiative transfer suite for atmospheres, comets, small bodies and exoplanets (2018, background): “, Venus [21], Jupiter/Saturn [22], Neptune/Uranus [23] and Titan [24]).”