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- W1998691206 abstract "We developed a line-by-line heating and cooling rate model for the stratosphere of Jupiter, based on two complete sets of global maps of temperature, C2H2 and C2H6, retrieved from the Cassini and Voyager observations in the latitude and vertical plane, with a careful error analysis. The non-LTE effect is found unimportant on the thermal cooling rate below the 0.01 mbar pressure level. The most important coolants are molecular hydrogen between 10 and 100 mbar, and hydrocarbons, including ethane (C2H6), acetylene (C2H2) and methane (CH4), in the region above. The two-dimensional cooling rate maps are influenced primarily by the temperature structure, and also by the meridional distributions of C2H2 and C2H6. The temperature anomalies at the 1 mbar pressure level in the Cassini data and the strong C2H6 latitudinal contrast in the Voyager epoch are the two most prominent features influencing the cooling rate patterns, with the effect from the ‘quasi-quadrennial oscillation (QQO)’ thermal structures at ~20 mbar. The globally averaged CH4 heating and cooling rates are not balanced, clearly in the lower stratosphere under 10 mbar, and possibly in the upper stratosphere above the 1 mbar pressure level. Possible heating sources from the gravity wave breaking and aerosols are discussed. The radiative relaxation timescale in the lower stratosphere implies that the temperature profile might not be purely radiatively controlled." @default.
- W1998691206 created "2016-06-24" @default.
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- W1998691206 date "2013-11-01" @default.
- W1998691206 modified "2023-10-01" @default.
- W1998691206 title "Radiative forcing of the stratosphere of Jupiter, Part I: Atmospheric cooling rates from Voyager to Cassini" @default.
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- W1998691206 cites W1965972466 @default.
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- W1998691206 cites W1970251751 @default.
- W1998691206 cites W1970903567 @default.
- W1998691206 cites W1972700013 @default.
- W1998691206 cites W1973988821 @default.
- W1998691206 cites W1974836642 @default.
- W1998691206 cites W1979168888 @default.
- W1998691206 cites W1983233022 @default.
- W1998691206 cites W1985442138 @default.
- W1998691206 cites W1986955963 @default.
- W1998691206 cites W1987277052 @default.
- W1998691206 cites W1989570161 @default.
- W1998691206 cites W1992940482 @default.
- W1998691206 cites W1994145256 @default.
- W1998691206 cites W1996277899 @default.
- W1998691206 cites W1997808327 @default.
- W1998691206 cites W2003429967 @default.
- W1998691206 cites W2004754032 @default.
- W1998691206 cites W2006502554 @default.
- W1998691206 cites W2006953709 @default.
- W1998691206 cites W2008126355 @default.
- W1998691206 cites W2008777117 @default.
- W1998691206 cites W2008942212 @default.
- W1998691206 cites W2010542794 @default.
- W1998691206 cites W2011354068 @default.
- W1998691206 cites W2018553592 @default.
- W1998691206 cites W2023594453 @default.
- W1998691206 cites W2024748895 @default.
- W1998691206 cites W2025112091 @default.
- W1998691206 cites W2026910687 @default.
- W1998691206 cites W2027097154 @default.
- W1998691206 cites W2028618158 @default.
- W1998691206 cites W2031442685 @default.
- W1998691206 cites W2032623901 @default.
- W1998691206 cites W2034049985 @default.
- W1998691206 cites W2034606276 @default.
- W1998691206 cites W2040047112 @default.
- W1998691206 cites W2043110535 @default.
- W1998691206 cites W2050877941 @default.
- W1998691206 cites W2052447352 @default.
- W1998691206 cites W2053335368 @default.
- W1998691206 cites W2057143449 @default.
- W1998691206 cites W2061695724 @default.
- W1998691206 cites W2061830681 @default.
- W1998691206 cites W2064850689 @default.
- W1998691206 cites W2068237720 @default.
- W1998691206 cites W2072198384 @default.
- W1998691206 cites W2075594667 @default.
- W1998691206 cites W2080949216 @default.
- W1998691206 cites W2083302566 @default.
- W1998691206 cites W2083940878 @default.
- W1998691206 cites W2087070363 @default.
- W1998691206 cites W2091776521 @default.
- W1998691206 cites W2092477793 @default.
- W1998691206 cites W2094758735 @default.
- W1998691206 cites W2109162012 @default.
- W1998691206 cites W2116881784 @default.
- W1998691206 cites W2117018191 @default.
- W1998691206 cites W2121565644 @default.
- W1998691206 cites W2126281183 @default.
- W1998691206 cites W2126427649 @default.
- W1998691206 cites W2135455558 @default.
- W1998691206 cites W2141319951 @default.
- W1998691206 cites W2146916780 @default.
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- W1998691206 cites W2158647937 @default.
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- W1998691206 cites W2165412090 @default.
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- W1998691206 cites W2256578114 @default.
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- W1998691206 doi "https://doi.org/10.1016/j.pss.2013.07.005" @default.
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