2012
DOI: 10.1016/j.icarus.2011.06.016
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Sulfur chemistry in the middle atmosphere of Venus

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Cited by 189 publications
(202 citation statements)
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“…This likely has contributed to the redistribution of volatile mass, as the larger number of potential activation sites results in a more even distribution of mass, hence smaller and more numerous droplets. Another consequence of this is that the larger number of cloud droplets overall results in a larger number of droplets able to reach higher altitude via eddy diffusion in our model, possibly providing a source for observed enhancements of sulfuric acid vapor at high altitudes (Zhang et al 2012). As to the question of why this should occur only at mid-latitudes, the answer at this point would be mere speculation.…”
Section: Coagulation Effects On Full Domain Modelmentioning
confidence: 85%
“…This likely has contributed to the redistribution of volatile mass, as the larger number of potential activation sites results in a more even distribution of mass, hence smaller and more numerous droplets. Another consequence of this is that the larger number of cloud droplets overall results in a larger number of droplets able to reach higher altitude via eddy diffusion in our model, possibly providing a source for observed enhancements of sulfuric acid vapor at high altitudes (Zhang et al 2012). As to the question of why this should occur only at mid-latitudes, the answer at this point would be mere speculation.…”
Section: Coagulation Effects On Full Domain Modelmentioning
confidence: 85%
“…•• H 2 S reaction occurs in a low-energy manner and is strongly exothermic. Note that the SO 2 mixing ratio in the middle atmosphere is the highest among the sulfur gases (17,18) implying that the SO 2 + H 2 SO 4…”
Section: Significancementioning
confidence: 99%
“…The thermal reactions of SO 3 and SO with H 2 SO 4 •• H 2 S clearly explain this anticorrelation. These thermal reactions not only provide useful mechanistic insights into an important sink of sulfur gases below 90 km in the Venus atmosphere, but may also help in understanding the mixing profiles of SO and SO 2 at higher altitudes (1,17,18,(32)(33)(34)(35)(36). At 96-km Venus atmosphere, the rates of the SO 3 hydration and the SO 3 photolysis are found to be comparable (17), which is suggestive of the fact that nearly half of the sulfur in H 2 SO 4 goes into SO 3 and produces the inversion layers of SO 2 and SO.…”
Section: Significancementioning
confidence: 99%
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