The magnetosphere of Uranus at 1986 solstice (the time of the Voyager 2 flyby). Upper left and right panels show the configuration at different phases of the planet’s 18-hour spin period (see Bagenal, Ann. Rev. Earth Planet. Sci., 20, 289, 1992). The lower panel shows a numerical simulation of the helical magnetotail (Toth et al., JGR, 109, A11210, 2004).
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In situ and remote observations of the ultraviolet footprint of the moon Callisto by the Juno spacecraft, Nature Communications, 2025 (https://www.nature.com/articles/s41467-025-62520-4)
Credits: NASA/JPL-Caltech/MSSS/SwRI/Kevin M. Gill/Björn Jónsson/Jason Perry/Jonas Rabia/Vincent Hue
A Comprehensive Set of Juno In Situ and Remote Sensing,Observations of the Ganymede Auroral Footprint, Geophysical Research Letter, 2022 (https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2021GL096994)
Credits: NASA/JPL-Caltech/MSSS/SwRI/Kevin M. Gill/Björn Jónsson/Bertrand Bonfond/Vincent Hue