A cold, corotating plasma inside 6 RJ with ions of sulfur, oxygen, and sulfur dioxide.
High-energy trapped particles inside 6 RJ with significantly enhanced abundances of oxygen, sodium, and sulfur.
Hot plasma near the magnetopause predominantly composed of protons, oxygen, and sulfur.
Jovian radio emission at kilometer wavelengths, which may be generated by plasma oscillations in the Io plasma torus.
Corotating plasma flows unexpectedly far from Jupiter in the dayside outer magnetosphere.
Evidence suggesting a transition from closed magnetic field lines to a Jovian magnetotail at about 25 RJ from Jupiter.
Whistler emission interpreted as lightning whistlers from the Jovian atmosphere.
[1]Adapted from a paper by E. C. Stone and A. L. Lane in the Voyager 1 Thirty-Day Report.
[2]Adapted from a summary prepared by E. C. Stone and A. L. Lane for the Voyager 1 Thirty-Day Report.
