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 …

The electrodynamic coupling between Io and Jupiter gives rise to wave‐particle interactions
across multiple spatial scales. Here we report observations during Juno's 12th perijove (PJ) …

Water‐group gas continuously escapes from Jupiter's icy moons to form co‐orbiting
populations of particles or neutral toroidal clouds. These clouds provide insights into their …

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 …

Juno's highly inclined orbits provide opportunities to sample high‐latitude magnetic field
lines connected to the orbit of Io, among the other Galilean satellites. Its payload offers both …

We characterize the precipitating electrons accelerated in the Europa‐magnetosphere
interaction by analyzing in situ measurements and remote sensing observations recorded …

The Juno spacecraft had previously observed intense high frequency wave emission,
broadband electron and energetic proton energy distributions within magnetic flux tubes …

Abstract On days 2023‐364 and 2024‐034, the Juno spacecraft made close passages of
Jupiter's moon Io, at altitudes of about 1,500 km. Data obtained from the first flyby, when the …

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 …

At Jupiter, part of the auroral radio emissions are induced by the Galilean moons Io, Europa,
and Ganymede. Until now, they have been remotely detected, using ground‐based radio …