Saturn's magnetic tail: structure and dynamics

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
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container_end_page 755
container_issue 5825
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container_title Nature (London)
container_volume 292
creator Behannon, K. W
Connerney, J. E. P
Ness, N. F
description 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.
doi_str_mv 10.1038/292753a0
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subjects Humanities and Social Sciences
multidisciplinary
news-and-views
Science
Science (multidisciplinary)
title Saturn's magnetic tail: structure and dynamics
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