NASA NTRS · 19810060824
Saturn's magnetic tail - Structure and dynamics
Abstract
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.
Keep this discovery
Explore connections, maps & timelines
Behannon, K. W., Connerney, J. E. P., Ness, N. F.. 1981-02-20. Saturn's magnetic tail - Structure and dynamics. https://ntrs.nasa.gov/citations/19810060824
Cite the original work for its findings. Save a collection to share your selection of sources.