Mariner 9 Ultraviolet Spectrometer Experiment: Seasonal Variation of Ozone on Mars

Details Mariner 9 Ultraviolet Spectrometer Experiment: Seasonal Variation of Ozone on Mars Mariner 9 Ultraviolet Spectrometer Experiment: Seasonal Variation of Ozone on Mars

Feb 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973sci...179..795b&link_type=abstract

Science, Volume 179, Issue 4075, pp. 795-796

Physics

33

Scientific paper

Ozone is observed to be present in the polar regions of Mars and to have a seasonal variation. In the summer, the amount present in the polar atmosphere is less than 3 micrometer-atmospheres. In the fall, ozone increases in amount and is found in association with the formation of the polar hood. In winter, the maximum amount of ozone is present, 57 micrometer-atmospheres over the polar hood and 16 over the polar cap. In spring, the amount over the polar cap decreases monotonically until by the beginning of summer the ozone disappears. Ozone is not observed in the equatorial region during any season.

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