Abstract
Voyager 2 plasma wave and plasma probe measurements from February 1981 suggest that phenomena associated with a well defined tail of Jupiter have been detected at a distance of about 6,200 RJ. This indicates that Saturn's magnetosphere will be affected by the jovian tail and that by comparing Voyager 1 and 2 observations information on the physics of Saturn's magnetosphere can be obtained.
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Scarf, F., Kurth, W., Gurnett, D. et al. Jupiter tail phenomena upstream from Saturn. Nature 292, 585–586 (1981). https://doi.org/10.1038/292585a0
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DOI: https://doi.org/10.1038/292585a0
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