Results 41 to 50 of about 3,808 (204)

Influence of the Jovian Current Sheet Models on the Mapping of the UV Auroral Footprints of Io, Europa, and Ganymede [PDF]

open access: yesJournal of Geophysical Research: Space Physics
The in situ characterization of moon‐magnetosphere interactions at Jupiter and the mapping of moon auroral footpaths require accurate global models of the magnetospheric magnetic field.
J. Rabia   +6 more
semanticscholar   +1 more source

Properties of Electrons Accelerated by the Ganymede‐Magnetosphere Interaction: Survey of Juno High‐Latitude Observations [PDF]

open access: yesJournal of Geophysical Research: Space Physics
The encounter between the Jovian co‐rotating plasma and Ganymede gives rise to electromagnetic waves that propagate along the magnetic field lines and accelerate particles by resonant or non‐resonant wave‐particle interaction. They ultimately precipitate
J. Rabia   +18 more
semanticscholar   +1 more source

Energetic Charged Particle Observations During Juno's Close Flyby of Ganymede

open access: yesGeophysical Research Letters, 2022
On 7 June 2021, NASA's Juno mission obtained unique measurements of Ganymede's magnetosphere during a close flyby that brought the spacecraft within ∼1,000 km of its surface.
G. Clark   +21 more
semanticscholar   +1 more source

Alternating North‐South Brightness Ratio of Ganymede's Auroral Ovals: Hubble Space Telescope Observations Around the Juno PJ34 Flyby

open access: yesGeophysical Research Letters, 2022
We report results of Hubble Space Telescope observations from Ganymede's orbitally trailing side which were taken around the flyby of the Juno spacecraft on 7 June 2021.
Joachim Saur   +19 more
doaj   +1 more source

Geophysical Characterization of the Interiors of Ganymede, Callisto and Europa by ESA’s JUpiter ICy moons Explorer

open access: yesSpace Science Reviews
The JUpiter ICy moons Explorer (JUICE) of ESA was launched on 14 April 2023 and will arrive at Jupiter and its moons in July 2031. In this review article, we describe how JUICE will investigate the interior of the three icy Galilean moons, Ganymede ...
T. Van Hoolst   +56 more
semanticscholar   +1 more source

The Ganymede Laser Altimeter (GALA) on the Jupiter Icy moons Explorer (JUICE) Mission

open access: yesSpace Science Reviews
The Ganymede Laser Altimeter (GALA) on the Jupiter Icy Moons Explorer (JUICE) mission, is in charge of a comprehensive geodetic mapping of Europa, Ganymede, and Callisto on the basis of Laser range measurements.
H. Hussmann   +75 more
semanticscholar   +1 more source

A Comprehensive Set of Juno In Situ and Remote Sensing Observations of the Ganymede Auroral Footprint

open access: yesGeophysical Research Letters, 2022
Jupiter's satellite auroral footprints are a manifestation of the satellite‐magnetosphere interaction of the Galilean moons. Juno's polar elliptical orbit enables crossing the magnetic flux tubes connecting each Galilean moon with their associated ...
V. Hue   +26 more
semanticscholar   +1 more source

Thermal Convection in the Core of Ganymede Inferred from Liquid Eutectic Fe-FeS Electrical Resistivity at High Pressures

open access: yesCrystals, 2021
The core of Ganymede is suggested to be mainly Fe but with a significant proportion of S. Effects of S as a core constituent are freezing-point depression, allowing for a molten core at relatively low core temperatures, and modification of transport ...
Joshua A. H. Littleton   +2 more
doaj   +1 more source

Aurora on Ganymede [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 2013
We present four sets of ultraviolet images of Ganymede acquired with the Hubble Space Telescope (HST) from 1998 to 2007, all of which show auroral emission from electron excited atomic oxygen. The three different hemispheres of Ganymede captured in the observations show strikingly different emission morphologies.
McGrath, Melissa A.   +5 more
openaire   +2 more sources

Measuring Ganymede’s Librations with Laser Altimetry

open access: yesGeosciences, 2019
Jupiter’s moon Ganymede might be in possession of a subsurface ocean located between two ice layers. However, from Galileo data it is not possible to unambiguously infer the thickness and densities of the individual layers.
Gregor Steinbrügge   +4 more
doaj   +1 more source

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