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Latitudinal distribution of carbon monoxide in the deep atmosphere of VenusA large number of i.r. spectra of Venus was obtained using the Near-Infrared Mapping Spectrometer (NIMS) on the Galileo spacecraft, during the February 1990 encounter. Preliminary results show an apparent increase in the tropospheric CO volume mixing ratio (vmr) in the northern polar region. Other possible explanations of the observations are examined and rejected and an increase of the CO abundance north of 47 deg N of (35 +/- 15)% is inferred. Some possible causes of this enhancement are suggested.
Document ID
19950043560
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Collard, A. D.
(Oxford University Oxford, United Kingdom)
Taylor, F. W.
(Oxford University Oxford, United Kingdom)
Calcutt, S. B.
(Oxford University Oxford, United Kingdom)
Carlson, R. W.
(Jet Propulsion Laboratory, Pasadena, CA United States)
Kamp, L. W.
(Jet Propulsion Laboratory, Pasadena, CA United States)
Baines, K. H.
(Jet Propulsion Laboratory, Pasadena, CA United States)
Encrenaz, TH.
(DESPA Meudon, France)
Drossart, P.
(DESPA Meudon, France)
Lellouch, E.
(DESPA Meudon, France)
Bezard, B.
(DESPA Meudon, France)
Date Acquired
August 16, 2013
Publication Date
July 1, 1993
Publication Information
Publication: Planetary and Space Science
Volume: 41
Issue: 7
ISSN: 0032-0633
Subject Category
Lunar And Planetary Exploration
Accession Number
95A75159
Distribution Limits
Public
Copyright
Other

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