66 citations · 198 across the 8 of their papers we have counts for
8 papers
Jupiter's UV auroral response to a magnetospheric compression event
R. S. Giles, T. K. Greathouse, R. W. Ebert +12
The highly elliptical polar orbit of the Juno mission provides a unique opportunity to simultaneously measure the compression state of Jupiter's magnetosphere and the total power e…
Synchronized Eruptions on Io: Evidence of Interconnected Subsurface Magma Reservoirs
A. Mura, R. Lopes, F. Nimmo +17
On December 27, 2024, Juno's JIRAM infrared experiment observed an unprecedented volcanic event on Io's southern hemisphere, covering a vast region of ~ 65,000 square km, near 73°S…
Super-adiabatic Temperature Gradient at Jupiter's Equatorial Zone and Implications for the Water Abundance
Cheng Li, Michael Allison, Sushil Atreya +12
The temperature structure of a giant planet was traditionally thought to be an adiabat assuming convective mixing homogenizes entropy. The only in-situ measurement made by the Gali…
Spacecraft VLBI tracking to enhance stellar occultations astrometry of planetary satellites
M. Fayolle, V. Lainey, D. Dirkx +3
Stellar occultations currently provide the most accurate ground-based measurements of the positions of natural satellites (down to a few kilometres for the Galilean moons). However…
The Io, Europa and Ganymede auroral footprints at Jupiter in the ultraviolet: positions and equatorial lead angles
Vincent Hue, Randy Gladstone, Corentin K. Louis +16
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 disturbanc…
Enhanced CH absorption within Jupiter's southern auroral oval from Juno UVS observations
Rohini S. Giles, Vincent Hue, Thomas K. Greathouse +9
Reflected sunlight observations from the Ultraviolet Spectrograph (UVS) on the Juno spacecraft were used to study the distribution of acetylene (CH) at Jupiter's south pole…