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 …

This review covers the work of the three decades since the first spectroscopic identification
of the H 3+ molecular ion outside of the laboratory in 1988, in the auroral atmosphere of the …

The Juno spacecraft's polar orbits have enabled direct sampling of Jupiter's low‐altitude
auroral field lines. While various data sets have identified unique features over Jupiter's …

Jupiter's aurorae are produced in its upper atmosphere when incoming high-energy
electrons precipitate along the planet's magnetic field lines. A northern and a southern main …

At Jupiter, part of the auroral radio emissions are induced by the Galilean moons Io, Europa
and Ganymede. Until now, except for Ganymede, they have been only remotely detected …

The Juno spacecraft crossed flux tubes connected to the Io footprint tail at low Jovian
altitudes on multiple occasions. The transits covered longitudinal separations of …

A large set of observations of Jupiter's ultraviolet aurora was collected with the Hubble
Space Telescope concurrently with the NASA‐Juno mission, during an eight‐month period …

Abstract ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …

Jupiter hosts intense auroral activity associated with charged particles precipitating into the
planet's atmosphere. The Galilean moons orbiting within the magnetosphere are swept by …

Dawn storms are among the brightest events in the Jovian aurorae. Up to now, they had only
been observed from Earth‐based observatories, only showing the Sun‐facing side of the …