NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The magnetosphere of UranusThe Voyager 2 encounter with Uranus on January 24, 1986, is described. It is noted that the combination of the orientation of the Uranian rotation axis with respect to the solar wind direction, and of the Uranian magnetic dipole axis with respect to the rotation axis, is a unique circumstance in the solar system. The Uranian magnetosphere is neither convection-dominated nor corotation-dominated, but rather a unique combination of both.
Document ID
19880063862
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Belcher, J. W.
(MIT Cambridge, MA, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1987
Subject Category
Lunar And Planetary Exploration
Accession Number
88A51089
Funding Number(s)
CONTRACT_GRANT: JPL-953733
CONTRACT_GRANT: JPL-957781
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available