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Mars: Water Vapor Observations from the Viking OrbitersThe global distribution of the water vapor has been mapped at low resolution throughout the period from the northern summer solstice to the following equinox. During this seasonal period the water vapor underwent a gradual redistribution, the latitude of maximum column abundance moving from the northern polar area to the equatorial latitudes. The total global vapor content remained approximately constant at the equivalent of about 1.3 cu km of ice. The various data obtained indicate that the residual polar caps are composed of water ice.
Document ID
19780027508
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Farmer, C. B.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Davies, D. W.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Holland, A. L.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Laporte, D. D.
(Hughes Santa Barbara Research Center Goleta, Calif., United States)
Doms, P. E.
(California, University Los Angeles, Calif., United States)
Date Acquired
August 9, 2013
Publication Date
September 30, 1977
Publication Information
Publication: Journal of Geophysical Research
Volume: 82
Issue: 28
Subject Category
Lunar And Planetary Exploration
Accession Number
78A11417
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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