papers

Publications (9)

astro-ph.EP2025

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…

astro-ph.EP2024

Effect of magnetospheric conditions on the morphology of Jupiter's UV main auroral emission, as observed by Juno-UVS

L. A. Head, D. Grodent, B. Bonfond +9

Auroral emissions are a reflection of magnetospheric processes, and, at Jupiter, it is not entirely certain how the morphology of the UV main emission (ME) varies with magnetospher…

astro-ph.EP2025

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…

physics.space-ph2025

Jupiter's ultraviolet auroral bridge: the influence of the solar wind on polar auroral morphology

L. A. Head, D. Grodent, B. Bonfond +9

Jupiters ultraviolet aurora frequently shows a number of arcs between the dusk-side polar region and the main emission, which are denoted as bridges. This work presents a largely a…

astro-ph.EP2025

The Pedersen and Hall Conductances in the Jovian Polar Regions: New Maps based on a Broadband Electron Energy Distribution

G. Sicorello, D. Grodent, B. Bonfond +9

The ionospheric Pedersen and Hall conductances play an important role in understanding the exchanges of angular momentum, energy and matter between the magnetosphere and the ionosp…

astro-ph.EP2025

Spatial variability of CH4 and C2H2 absorptions in Jupiter's auroral regions from Juno-UVS observations

J. Vinesse, B. Bonfond, B. Benmahi +8

Color ratios derived from molecular hydrogen emissions provide valuable diagnostics for the energy of precipitating electrons and the structure of the auroral atmosphere. We aim to…