A time-dependent photochemical model for Titan's atmosphere and the origin of H2O
LM Lara, E Lellouch, M González, R Moreno…
Index: Homann; Wellmann Berichte der Bunsengesellschaft/Physical Chemistry Chemical Physics, 1983 , vol. 87, # 7 p. 609 - 616
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Citation Number: 8
Abstract
... 2012) for both of the chemical schemes used here, which maintains CO 2 stratospheric profiles in ... In the Jupiter/SL9 case, shock chemistry at plume re-entry has produced CO and ... Furthermore, while CO is chemically stable, any newly injected H 2 O is progressively photolysed ...
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