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Imaging observations of Jupiter's sodium magneto-nebula during the Ulysses encounterJupiter's great sodium nebula represents the largest visible structure traversed by the Ulysses spacecraft during its encounter with the planet in February 1992. Ground-based imaging conducted on Mount Haleakala, Hawaii, revealed a nebula that extended to at least +/- 300 Jovian radii; it was somewhat smaller in scale and less bright than previously observed. Analysis of observations and results of modeling studies suggest reduced volcanic activity on the moon Io, higher ion temperatures in the plasma torus, lower total plasma content in the torus, and fast neutral atomic clouds along the Ulysses inbound trajectory through the magnetosphere. Far fewer neutrals were encountered by the spacecraft along its postencounter, out-of-ecliptic trajectory.
Document ID
19920074362
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mendillo, Michael
(NASA Headquarters Washington, DC United States)
Flynn, Brian
(NASA Headquarters Washington, DC United States)
Baumgardner, Jeffrey
(Boston University MA, United States)
Date Acquired
August 15, 2013
Publication Date
September 11, 1992
Publication Information
Publication: Science
Volume: 257
Issue: 5076
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
92A56986
Funding Number(s)
CONTRACT_GRANT: NAGW-2679
Distribution Limits
Public
Copyright
Other

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