Parameter Space for an O3 Layer in Mars' Past

Details Parameter Space for an O3 Layer in Mars' Past Parameter Space for an O3 Layer in Mars' Past

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1597d&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1597

Physics

Scientific paper

It has been suggested that an O3 layer might have formed on Mars under past atmospheric conditions, with consequences for photochemistry and climate. This work attempts to identify past conditions capable of supporting a significant O3 layer in a humid CO2 Martian atmosphere. Parameter space explored includes surface pressure, humidity, and insolation. Under conditions which do support a significant O3 layer, effects on atmospheric structure, loss to space, and habitability are investigated.

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