Mars ozone: Mariner 9 revisited

Details Mars ozone: Mariner 9 revisited Mars ozone: Mariner 9 revisited

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994rmus.nasas....l&link_type=abstract

In its Reanalysis of Mariner 9 UV Spectrometer Data for Ozone, Cloud, and Dust Abundances, and Their Interaction Over Climate Ti

Computer Science

Atmospheric Composition, Dust, Mars Atmosphere, Ozone, Ultraviolet Spectroscopy, Abundance, Mariner 9 Space Probe, Remote Sensing, Variability

Scientific paper

The efficacy of the UV spectroscopy technique used by Mariner 9 to remotely measure ozone abundance at Mars is discussed. Previously-inferred ozone abundances could be underestimated by as much as a factor of 3, and much of the observed variability in the ozone abundance could be due to temporal and spatial variability in cloud and dust amount.

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