Abstract In July 2016, NASA's Juno mission becomes the first spacecraft to enter polar orbit
of Jupiter and venture deep into unexplored polar territories of the magnetosphere. Focusing …

Previous Juno mission event studies revealed powerful electron and ion acceleration, to
100s of kiloelectron volts and higher, at low altitudes over Jupiter's main aurora and polar …

The ultraviolet spectrograph instrument on the Juno mission (Juno-UVS) is a long-slit
imaging spectrograph designed to observe and characterize Jupiter's far-ultraviolet (FUV) …

The most intense auroral emissions from Earth's polar regions, called discrete for their
sharply defined spatial configurations, are generated by a process involving coherent …

While the terrestrial aurorae are known to be driven primarily by the interaction of the Earth's
magnetosphere with the solar wind, there is considerable evidence that auroral emissions …

Jupiter displays the most powerful auroral emissions in our solar system, which result from
strong energy dissipation in Jupiter's surrounding space environment. Although mass and …

Auroral processes are exhibited by every planet and satellite with a collisionally thick
atmosphere and an internal magnetic field sufficiently strong to stand off the solar wind or …

Jupiter's bright persistent polar aurora and Earth's dark polar region indicate that the planets'
magnetospheric topologies are very different. High-resolution global simulations show that …

An extended series of FUV images obtained on 7 days during winter 2000–2001, with fixed
pointing, yielded highly accurate tracking of emisson features as Jupiter rotated. They …

We present a review of observations and theories of the dynamics of Jupiter's
magnetosphere from Pioneer to New Horizons. We suggest that Jupiter's solar wind–driven …