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Mars ozone: Mariner 9 revisitedThe 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.
Document ID
19940023385
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Lindner, Bernhard Lee (Atmospheric and Environmental Research, Inc. Cambridge, MA, United States)
Date Acquired
September 6, 2013
Publication Date
February 7, 1994
Publication Information
Publication: Reanalysis of Mariner 9 UV Spectrometer Data for Ozone, Cloud, and Dust Abundances, and Their Interaction Over Climate Timescales
Subject Category
Lunar And Planetary Exploration
Accession Number
94N27888
Funding Number(s)
CONTRACT_GRANT: NASW-4614
Distribution Limits
Public
Copyright
Public Use Permitted.

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