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• W2109162012 abstract "We have developed a one‐dimensional, diurnally averaged, photochemical model for Jupiter's stratosphere that couples photodissociation, chemical kinetics, vertical diffusion, and radiative transport. The predictions regarding the abundances and vertical profiles of hydrocarbon compounds are compared with observations from the Infrared Space Observatory (ISO) to better constrain the atmospheric composition, to better define the eddy diffusion coefficient profile, and to better understand the chemical reaction schemes that produce and destroy the observed constituents. From model‐data comparisons we determine that the C 2 H 6 mole fraction on Jupiter is (4.0 ± 1.0) × 10 −6 at 3.5 mbar and (2.7 ± 0.7) × 10 −6 at 7 mbar, and the C 2 H 2 mole fraction is (1.4 ± 0.8) × 10 −6 at 0.25 mbar and (1.5 ± 0.4) × 10 −7 at 2 mbar. The column densities of CH 3 C 2 H and C 6 H 6 are (1.5 ± 0.4) × 10 15 cm −2 and (8.0 ± 2) × 10 14 cm −2 , respectively, above 30 mbar. Using identical reaction lists, we also have developed photochemical models for Saturn, Uranus, and Neptune. Although the models provide good first‐order predictions of hydrocarbon abundances on the giant planets, our current chemical reaction schemes do not reproduce the relative abundances of C 2 H x hydrocarbons. Unsaturated hydrocarbons like C 2 H 4 and C 2 H 2 appear to be converted to saturated hydrocarbons like C 2 H 6 more effectively on Jupiter than on the other giant planets, more effectively than is predicted by the models. Further progress in our understanding of photochemistry at low temperatures and low pressures in hydrogen‐dominated atmospheres hinges on the acquisition of high‐quality kinetics data." @default.
• W2109162012 created "2016-06-24" @default.
• W2109162012 creator A5024602666 @default.
• W2109162012 creator A5044704721 @default.
• W2109162012 creator A5048466695 @default.
• W2109162012 creator A5057771393 @default.
• W2109162012 creator A5081508890 @default.
• W2109162012 creator A5087028059 @default.
• W2109162012 date "2005-08-01" @default.
• W2109162012 modified "2023-10-14" @default.
• W2109162012 title "Photochemistry and diffusion in Jupiter's stratosphere: Constraints from ISO observations and comparisons with other giant planets" @default.
• W2109162012 cites W1481597652 @default.
• W2109162012 cites W1496128888 @default.
• W2109162012 cites W1501888605 @default.
• W2109162012 cites W1534620796 @default.
• W2109162012 cites W1534942013 @default.
• W2109162012 cites W1542801225 @default.
• W2109162012 cites W156945926 @default.
• W2109162012 cites W1608146267 @default.
• W2109162012 cites W1640780733 @default.
• W2109162012 cites W1648382482 @default.
• W2109162012 cites W1715392501 @default.
• W2109162012 cites W1965000806 @default.
• W2109162012 cites W1965340484 @default.
• W2109162012 cites W1965972466 @default.
• W2109162012 cites W1966505324 @default.
• W2109162012 cites W1966991386 @default.
• W2109162012 cites W1967149364 @default.
• W2109162012 cites W1968011551 @default.
• W2109162012 cites W1968736794 @default.
• W2109162012 cites W1970173684 @default.
• W2109162012 cites W1970234628 @default.
• W2109162012 cites W1970251751 @default.
• W2109162012 cites W1973988821 @default.
• W2109162012 cites W1975690430 @default.
• W2109162012 cites W1976123559 @default.
• W2109162012 cites W1977179100 @default.
• W2109162012 cites W1977580484 @default.
• W2109162012 cites W1980084383 @default.
• W2109162012 cites W1981766989 @default.
• W2109162012 cites W1984303322 @default.
• W2109162012 cites W1984753018 @default.
• W2109162012 cites W1985442138 @default.
• W2109162012 cites W1986035035 @default.
• W2109162012 cites W1988888286 @default.
• W2109162012 cites W1989570161 @default.
• W2109162012 cites W1990147493 @default.
• W2109162012 cites W1990533714 @default.
• W2109162012 cites W1992940482 @default.
• W2109162012 cites W1995018450 @default.
• W2109162012 cites W1995851907 @default.
• W2109162012 cites W1996002628 @default.
• W2109162012 cites W1996213930 @default.
• W2109162012 cites W1996606603 @default.
• W2109162012 cites W2002224283 @default.
• W2109162012 cites W2003674417 @default.
• W2109162012 cites W2003806445 @default.
• W2109162012 cites W2004840453 @default.
• W2109162012 cites W2005394860 @default.
• W2109162012 cites W2009442138 @default.
• W2109162012 cites W2009511968 @default.
• W2109162012 cites W2010397808 @default.
• W2109162012 cites W2010542794 @default.
• W2109162012 cites W2010711431 @default.
• W2109162012 cites W2012065836 @default.
• W2109162012 cites W2012479771 @default.
• W2109162012 cites W2013432358 @default.
• W2109162012 cites W2013871882 @default.
• W2109162012 cites W2013951679 @default.
• W2109162012 cites W2015776919 @default.
• W2109162012 cites W2016608754 @default.
• W2109162012 cites W2016649425 @default.
• W2109162012 cites W2017821891 @default.
• W2109162012 cites W2018043796 @default.
• W2109162012 cites W2018328868 @default.
• W2109162012 cites W2018494158 @default.
• W2109162012 cites W2020364964 @default.
• W2109162012 cites W2023678071 @default.
• W2109162012 cites W2023708794 @default.
• W2109162012 cites W2025148659 @default.
• W2109162012 cites W2026910687 @default.
• W2109162012 cites W2027097154 @default.
• W2109162012 cites W2027142007 @default.
• W2109162012 cites W2027689899 @default.
• W2109162012 cites W2028432729 @default.
• W2109162012 cites W2028497374 @default.
• W2109162012 cites W2029655924 @default.
• W2109162012 cites W2029887523 @default.
• W2109162012 cites W2030321146 @default.
• W2109162012 cites W2030632917 @default.
• W2109162012 cites W2030930689 @default.
• W2109162012 cites W2031296121 @default.
• W2109162012 cites W2033338051 @default.
• W2109162012 cites W2034116495 @default.
• W2109162012 cites W2034846051 @default.
• W2109162012 cites W2036542241 @default.
• W2109162012 cites W2036986820 @default.
• W2109162012 cites W2037796515 @default.
• W2109162012 cites W2038116868 @default.
• W2109162012 cites W2038631728 @default.

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