Analyzing O2 and O3 production and destruction pathways in the Martian atmosphere

Details Analyzing O2 and O3 production and destruction pathways in the Martian atmosphere Analyzing O2 and O3 production and destruction pathways in the Martian atmosphere

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..457s&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.457

Physics

Scientific paper

Ozone and molecular oxygen are of central importance for the Martian atmosphere, since they have a significant impact on the photochemical stability of the main atmospheric constituent, CO2, and are suitably observable species. Their abundance is controlled by chemical pathways which will be investigated in this contribution. In order to achieve this, we apply a unique algorithm, called the Pathway Analysis Program - PAP to the results of the JPL/Caltech photochemical column model of the Martian atmosphere.

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