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Mariner 9 ultraviolet spectrometer experiment - Seasonal variation of ozone on Mars.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.
Document ID
19730036421
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Barth, C. A.
Hord, C. W.
Stewart, A. I.
Dick, M. L.
Anderson, G. P.
(Colorado, University Boulder, Colo., United States)
Lane, A. L.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Date Acquired
August 7, 2013
Publication Date
February 23, 1973
Publication Information
Publication: Science
Volume: 179
Subject Category
Space Sciences
Accession Number
73A21223
Distribution Limits
Public
Copyright
Other

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