Jupiter's Aurora

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The Jovian Auroral Distributions Experiment (JADE) on the Juno Mission to Jupiter (2017, background): “Auroral observations suggest that Juno will move through structures that are ∼1000 km across (Clarke et al. 2004), so JADE is ideal for studying these regions.”
Response of Jupiter's and Saturn's auroral activity to the solar wind (2009, background): “…compared with auroral emissions from the magnetic footprints of the satellites and theoretical modeling have demonstrated that the main auroral oval maps along the field to a distance about 20–30 Jovian radii (RJ), in the middle magnetosphere far from the solar wind boundary [Clarke et al., 2004].”
Plasma interactions of exoplanets with their parent star and associated radio emissions (2006, background): “These engines produce bright polar UV auroras at northern and southern magnetic field line footprints in the atmosphere and associated radio emissions above them (Prangé and Zarka, 2003; Clarke et al., 2004).”
On the origin of aurorae on Mars (2006, background): “[2] Aurorae are observed throughout the solar system [Clarke et al., 2004], and occur where charged particles have access to an atmosphere along magnetic field lines [McIlwain, 1960].”