NASA NTRS · 19940023385
Mars ozone: Mariner 9 revisited
Abstract
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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Lindner, Bernhard Lee. 1994-02-07. Mars ozone: Mariner 9 revisited. https://ntrs.nasa.gov/citations/19940023385
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