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 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 …

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 …

We analyze precipitating electron fluxes connected to 18 crossings of Io's footprint tail
aurora, over altitudes of 0.15 to 1.1 Jovian radii (RJ). The strength of precipitating electron …

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 …

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 …

Juno performed two close flybys of Io and found enhanced field‐aligned proton fluxes are
absorbed by Io. These protons are absorbed at mass input rates comparable to previous …

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

We present a physical mechanism for generating∼ GeV ions in the Jovian radiation belts.
The mechanism is called relativistic turning acceleration (RTA) and involves a special form …

Using Juno‐measured> 30 keV electrons, three regions with substantial ultraviolet
emissions were identified previously for Jupiter's main aurora (excluding the polar cap): low …