Jupiter's satellite auroral footprints are a consequence of the interaction between the Jovian
magnetic field with co‐rotating iogenic plasma and the Galilean moons. The disturbances …

Observations of the Jovian upper atmosphere at high latitudes in the UV, IR and mm/sub-
mm all indicate that the chemical distributions and thermal structure are broadly influenced …

Auroral brightness and color ratio imagery, captured using the Juno mission's Ultraviolet
Spectrograph, display intense emissions poleward of Jupiter's northern main emission, and …

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 …

Reflected sunlight observations from the Ultraviolet Spectrograph (UVS) on the Juno
spacecraft were used to study the distribution of acetylene (C2H2) at Jupiter's south pole …

We present comparisons of precipitating electron flux and auroral brightness measurements
made during several Juno transits over Jupiter's auroral regions in both hemispheres. We …

Jupiter's satellite auroral footprints are a manifestation of the satellite‐magnetosphere
interaction of the Galilean moons. Juno's polar elliptical orbit enables crossing the magnetic …

Jupiter's main auroral emissions usually form auroral curtains surrounding the magnetic
poles. Most explanations for this auroral feature are based on corotation enforcement …

Ionospheric conductivity perpendicular to the magnetic field plays a crucial role in the
electrical coupling between planetary magnetospheres and ionospheres. At Jupiter, it …

Eleven transient bright flashes were detected in Jupiter's atmosphere using the ultraviolet
spectrograph instrument on the Juno spacecraft. These bright flashes are only observed in a …