89 citations · 156 across the 7 of their papers we have counts for
7 papers
Investigating Magnetic Field Fluctuations in Jovian Auroral Electron Beams
A. Salveter, J. Saur, G. Clark +4
The Juno spacecraft provides a unique opportunity to explore the mechanisms generating Jupiter's aurorae. Past analyses of Juno data immensely advanced our understanding of its aur…
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…
Source of radio emissions induced by the Galilean moons Io, Europa and Ganymede: in situ measurements by Juno
C. K. Louis, P. Louarn, B. Collet +13
At Jupiter, part of the auroral radio emissions are induced by the Galilean moons Io, Europa and Ganymede. Until now, except for Ganymede, they have been only remotely detected, us…
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…
Effect of a magnetosphere compression on Jovian radio emissions: in situ case study using Juno data
C. K. Louis, C. M. Jackman, G. Hospodarsky +13
During its 53-day polar orbit around Jupiter, Juno often crosses the boundaries of the Jovian magnetosphere (namely the magnetopause and bow shock). From the boundary locations, th…
Observation of Turbulent Magnetohydrodynamic Cascade in the Jovian Magnetosheath
N. Andrés, R. Bandyopadhyay, D. J. McComas +6
We present the first estimation of the energy cascade rate in Jupiter's magnetosheath (MS). We use in-situ observations from the Jovian Auroral Distributions Experiment (JADE) and…
Jupiter's inhomogeneous envelope
Y. Miguel, M. Bazot, T. Guillot +13
While Jupiter's massive gas envelope consists mainly of hydrogen and helium, the key to understanding Jupiter's formation and evolution lies in the distribution of the remaining (h…