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The outer magnetosphereSimilarities between the Saturnian and terrestrial outer magnetosphere are examined. Saturn, like earth, has a fully developed magnetic tail, 80 to 100 RS in diameter. One major difference between the two outer magnetospheres is the hydrogen and nitrogen torus produced by Titan. This plasma is, in general, convected in the corotation direction at nearly the rigid corotation speed. Energies of magnetospheric particles extend to above 500 keV. In contrast, interplanetary protons and ions above 2 MeV have free access to the outer magnetosphere to distances well below the Stormer cutoff. This access presumably occurs through the magnetotail. In addition to the H+, H2+, and H3+ ions primarily of local origin, energetic He, C, N, and O ions are found with solar composition. Their flux can be substantially enhanced over that of interplanetary ions at energies of 0.2 to 0.4 MeV/nuc.
Document ID
19850051837
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Schardt, A. W.
Behannon, K. W.
Lepping, R. P.
Carbary, J. F.
Eviatar, A.
Siscoe, G. L.
Date Acquired
August 12, 2013
Publication Date
January 1, 1984
Subject Category
Lunar And Planetary Exploration
Accession Number
85A33988
Funding Number(s)
CONTRACT_GRANT: NAGW-333
CONTRACT_GRANT: NAGW-87
Distribution Limits
Public
Copyright
Other

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