Saturn's magnetic tail: structure and dynamics

Voyager 1 magnetic field observations have provided evidence of a saturnian magnetic tail. Tail current system distributions are inferred through comparison of the observations with a realistic magnetotail current system model. Temporal variations observed in the tail were probably produced by solar...

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Veröffentlicht in:Nature (London) 1981-08, Vol.292 (5825), p.753-755
Hauptverfasser: Behannon, K. W, Connerney, J. E. P, Ness, N. F
Format: Artikel
Sprache:eng
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Zusammenfassung:Voyager 1 magnetic field observations have provided evidence of a saturnian magnetic tail. Tail current system distributions are inferred through comparison of the observations with a realistic magnetotail current system model. Temporal variations observed in the tail were probably produced by solar wind variations.
ISSN:0028-0836
1476-4687
DOI:10.1038/292753a0