The Galilean moons play major roles in the giant magnetosphere of Jupiter. At the same
time, the magnetospheric particles and fields affect the moons. The impact of …

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 …

A spherical harmonic model of the magnetic field of Jupiter is obtained from vector magnetic
field observations acquired by the Juno spacecraft during its first nine polar orbits about the …

On 27 August 2016, the Juno spacecraft acquired science observations of Jupiter, passing
less than 5000 kilometers above the equatorial cloud tops. Images of Jupiter's poles show a …

The Jovian magnetosphere assumes a disc‐like geometrical configuration (“magnetodisc”)
owing to the persistent presence of a system of azimuthal currents circulating in a washer …

The familiar axisymmetric zones and belts that characterize Jupiter's weather system at
lower latitudes give way to pervasive cyclonic activity at higher latitudes. Two-dimensional …

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 …

We investigate spatial and temporal scales at which wave‐particle interaction of Alfvén
waves occurs in Jupiter's magnetosphere. We consider electrons, protons, and oxygen ions …

Juno obtained unique low‐altitude space environment measurements over Jupiter's poles
on 27 August 2016. Here Jupiter Energetic‐particle Detector Instrument observations are …

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 …