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Rotation period for a subsurface source in the NNTeB of JupiterDuring two consecutive apparitions of Jupiter, 1968-69 and 1969-70, 12 and 9 spots were observed in the North North Temperature Current B (latitude about 35 N). Drift curves were extended on the basis of LPL Jupiter photographs. It is shown that the two source areas for these groups of spots are probably the same, and define a rotation period of the common subsurface source very close to that of System 3.
Document ID
19740019214
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Solberg, G.
(Arizona Univ. Tucson, AZ, United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Publication Information
Publication: Commun. of the Lunar and Planetary Lab.: Commun. Nos. 173-183, Vol. 9, Part 5
Subject Category
Space Sciences
Accession Number
74N27327
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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