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Composition and thermal profiles of the Jovian upper atmosphere determined by the Voyager ultraviolet stellar occultation experimentDuring the occultation of the star Regulus (B7 type) by Jupiter as seen from the Voyager 2 spacecraft on July 9, 1979, two absorbing regions were detected. Between 911 and 1200 A, H2 was absorbing over a 600 km altitude range. Above 1300 A, the rapid increase of the absorption by the hydrocarbons was observed over an altitude interval of approximately 100 km with a height resolution of 3 km. The analysis of these absorption features has provided the height profiles of molecular hydrogen, methane, ethane, and acetylene, as well as the thermal profile in the upper atmosphere of Jupiter. Combining the Voyager ultraviolet spectrometer results with other data, such as those obtained by the Voyager infrared and radioscience instruments, has yielded a comprehensive model of the composition and structure of the atmosphere of Jupiter.
Document ID
19810056402
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Festou, M. C.
(Michigan Univ. Ann Arbor, MI, United States)
Atreya, S. K.
(Michigan Univ. Ann Arbor, MI, United States)
Donahue, T. M.
(Michigan, University Ann Arbor, MI, United States)
Sandel, B. R.
(Michigan Univ. Ann Arbor, MI, United States)
Shemansky, D. E.
(Michigan Univ. Ann Arbor, MI, United States)
Broadfoot, A. L.
(Southern California, University Tucson, AZ, United States)
Date Acquired
August 11, 2013
Publication Date
July 1, 1981
Publication Information
Publication: Journal of Geophysical Research
Volume: 86
Subject Category
Lunar And Planetary Exploration
Accession Number
81A40806
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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