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Journal of Geophysical Research: Space Physics, ISSN 2169-9380, 08/2017, Volume 122, Issue 8, pp. 7985 - 7996
.... This signature, called the satellite footprint, takes the form of a series of spots located slightly downstream of the feet of the field lines passing through the moon under consideration... 
Jupiter | Europa | satellite footprint | aurora | Ganymede | SPOTS | ASTRONOMY & ASTROPHYSICS | MODEL | WAKE | Jupiter satellites | Computer simulation | Moon | Auroras | Electron acceleration | Satellites | Hemispheres | Northern Hemisphere | Rotating plasmas | Spots | Static models | Electric fields | Downstream
Journal Article
Journal of Geophysical Research: Space Physics, ISSN 0148-0227, 01/2011, Volume 116, Issue A1, p. n/a
...1. Introduction Satellite‐magnetosphere interactions occur when a satellite orbits close to its parent planet, deep inside the planet's magnetosphere... 
satellite interactions | UV aurora | Alfvén waves | IO PLASMA TORUS | ACCELERATION | ALFVEN WAVES | BEAMS | ASTRONOMY & ASTROPHYSICS | GALILEO | TURBULENCE | PARALLEL ELECTRIC-FIELDS | FOOTPRINT | FLUX TUBE | JUPITER | Atmospheric sciences | Magnetism
Journal Article
Journal Article
2007, Cambridge planetary science series, ISBN 0521850037, Volume 7, xvi, 355
The most powerful volcanoes in the Solar System are not on Earth, but on Io, a tiny moon of Jupiter. Whilst Earth and Io are the only bodies in the Solar... 
Io (Satellite) Volcanism | Planetary volcanism | Io (Satellite) Volcanoes | Volcanism | Remote sensing | Io (Satellite)
Book
Geophysical research letters, ISSN 0094-8276, 2017, Volume 44, Issue 18, pp. 9225 - 9232
We compare observations from the Juno/Waves radio experiment with simulations of radio «arcs» in the time‐frequency plane resulting from the Io‐Jupiter... 
decametric | Jupiter | ExPRES | Juno/Waves | radio | GEOSCIENCES, MULTIDISCIPLINARY | Io | Waves | Juno | RADIO EMISSIONS | Auroral oval | Jupiter satellites | Stability | Computer simulation | Satellite sensing | Emission | Radio | Cyclotrons | Remote sensing | Emissions | Earth | Satellites | Simulation | Jupiter probes | Instability | Galilean satellites | Wind observation | Physics | Astrophysics
Journal Article
Journal of geophysical research. Space physics, ISSN 2169-9402, 2019, Volume 124, Issue 5, pp. 3236 - 3254
Journal Article
The Astrophysical Journal Letters, ISSN 1538-4357, 07/2004, Volume 609, Issue 2, pp. L99 - L102
... PLASMA–DRIVEN EVOLUTION OF SATELLITE ATMOSPHERES R. E. Johnson Engineering Physics and Astronomy Department, University of Virginia, P.O. Box 400238, Charlottesville... 
Planets and satellites: Individual (Callisto, Europa, Ganymede, Io, Titan) | Planets and satellites: Formation | planets and satellites : formation | STABILITY | Ganymede, Io, Titan | OXYGEN ATMOSPHERE | EUROPA | TITAN | MOLECULES | TORUS | ASTRONOMY & ASTROPHYSICS | NITROGEN | SURFACE | ATOMS | EXOSPHERE | planets and satellites : individual (Callisto, Europa
Journal Article
Icarus (New York, N.Y. 1962), ISSN 0019-1035, 2017, Volume 292, pp. 208 - 217
In the magnetospheres of Jupiter and Saturn, the intense interaction of the satellites Io, Europa, Ganymede and Enceladus with their surrounding plasma environment leaves a signature in the aurora of the planet... 
Aurora | Footprint | Jupiter | Europa | Ganymede | IO FOOTPRINT | FLUX TUBE | TORUS | IMAGES | ASTRONOMY & ASTROPHYSICS | AURORAL FOOTPRINT | EMISSION | MORPHOLOGY | Magnetic fields | Plasma physics
Journal Article
Geophysical Research Letters, ISSN 0094-8276, 06/2017, Volume 44, Issue 11, pp. 5308 - 5316
..., and the footprints of Io, Europa and Ganymede. The extended Io “tail” persists for ~3 h after the passage of the satellite flux tube. Multi... 
aurora | Jupiter | GEOSCIENCES, MULTIDISCIPLINARY | IONOSPHERE | SPOTS | ULTRAVIOLET | MODEL | EMISSION | IO FLUX TUBE | MORPHOLOGY | Temporal distribution | Fluctuations | Jupiter satellites | Auroras | Emission | Flux | Orbits | Regions | Mathematical morphology | Emissions | Satellites | Depletion | Spatial distribution | Space missions | Circularity | Jupiter probes | Infrared radiation | Footprints | Europa | Structures | Onboard | Polar regions | Ganymede
Journal Article
Journal of Geophysical Research: Space Physics, ISSN 2169-9380, 12/2015, Volume 120, Issue 12, pp. 10,317 - 10,333
.... The extreme ultraviolet spectrograph on board the HISAKI satellite continuously observed the IPT from the end of December 2013 to the middle of January 2014... 
electron heating | Io plasma torus | EXCEED | HISAKI | Jovian magnetosphere | VARIABILITY | EXTREME-ULTRAVIOLET SPECTROSCOPE | EARTH-ORBITING SATELLITE | ATOMIC DATABASE | ASTRONOMY & ASTROPHYSICS | CYCLOTRON WAVES | CASSINI UVIS OBSERVATIONS | MAGNETOSPHERE | NEUTRAL CLOUDS | JUPITER | Plasma | Geophysics | Spacecraft | Electrons | Jupiter satellites | Wavelengths | Heating | Brightness | Hot electrons | Longitude | Jupiter (planet)
Journal Article