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The atmosphere of Saturn - An analysis of the Voyager radio occultation measurementsThe Voyager 1 and 2 probes' radio links were used to study both the northern and southern latitudes of Saturn during occultation by that planet, yielding electron number density profiles for the ionosphere, and gas refractivity, number density, pressure, temperature, and ammonia abundance data for the troposphere and stratosphere. From the vertical pressure profiles obtained at different latitudes, it is possible to determine the size and shape of Saturn's isobaric surfaces.
Document ID
19850052796
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lindal, G. F.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Sweetnam, D. N.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Eshleman, V. R.
(Stanford University Stanford, CA, United States)
Date Acquired
August 12, 2013
Publication Date
June 1, 1985
Publication Information
Publication: Astronomical Journal
Volume: 90
ISSN: 0004-6256
Subject Category
Lunar And Planetary Exploration
Accession Number
85A34947
Distribution Limits
Public
Copyright
Other

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