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Titel Quantification of CO2-formation pathways in the Martian Atmosphere
VerfasserIn Joachim Stock, Christopher Boxe, Lee Grenfell, Ralph Lehmann, Beate Patzer, Heike Rauer, Yuk Yung
Konferenz EGU General Assembly 2011
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 13 (2011)
Datensatznummer 250051014
 
Zusammenfassung
The chemical composition of terrestrial planetary atmospheres can be critically influenced by the presence of trace species, which in turn, can act in catalytic cycles, affecting the concentrations of major atmospheric gases, by providing alternative chemical reaction routes (i.e., chemical pathways). Since the number of chemical species and reactions in such complex systems can be very large (and hence, also the number of chemical pathways), it is, generally, a challenging task to identify the important chemical pathways that determine the abundance of major species. Therefore, effective methods for the investigation of such reaction networks are required. In order to analyze the CO2-dominated atmosphere of Mars, we use a new analysis tool (i.e., Pathway Analysis Program - PAP), which is capable of identifying and also quantifying all chemical reaction pathways in a reaction network. For this study, we apply PAP to the Caltech-JPL 1-D Mars photochemical model to identify and analyze the dominant chemical processes involved in CO2-production in Mars’ atmosphere. Results of our analysis with respect to the dominant catalytic chemical cycles, governing Martian atmospheric CO2 will be discussed.