Statistical Analysis of the Equatorward UV Auroral Emissions of the Jovian Southern Hemisphere
Abstract This study presents a comprehensive statistical analysis of Jupiter's southern UV auroral emissions, with a focus on the secondary oval and equatorward injection signatures. Utilizing Hubble Space Telescope (HST) data, the frequency, location, and intensity of these auroral features are systematically evaluated, considering their variation ...
Diego Moral‐Pombo +2 more
wiley +1 more source
Study of USNO photographic plates of the Galilean satellites
Program available at: http://www.imcce.fr/hosted_sites/naroo/program.htmlInternational audienceAbout 500 photographic plates of the Galilean satellites made with the 26-inch refractor of USNO in Washington DC from 1967 to 1998 were digitized and reduced ...
Robert, Vincent
core +2 more sources
Delivery of Dust Particles from Protoplanetary Disks onto Circumplanetary Disks of Giant Planets
The principal regular satellites of gas giants are thought to be formed by the accumulation of solid materials in circumplanetary disks (CPDs). While there has been significant progress in the study of satellite formation in CPDs, details of the supply ...
Natsuho Maeda +5 more
doaj +1 more source
Preliminary feasibility study of soft-lander missions to the Galilean satellites of Jupiter [PDF]
Feasibility study of soft lander missions to Galilean satellites of ...
Spadoni, D. J., Price, M. J.
core
Propagation Dynamics of Fast Electron Beam and Its Electron Cyclotron Maser Emission
Abstract Fast electron beams (FEBs) and coherent radio bursts both are very common plasma activity phenomena in the cosmos. The electron cyclotron maser (ECM) instability driven by FEBs trapped in magnetic fields can directly amplify radio wave radiations.
Ling Chen +3 more
wiley +1 more source
New Global Map of Io’s Volcanic Thermal Emission and Discovery of Hemispherical Dichotomies
By combining multiple spacecraft and telescope data sets, the first fully global volcanic heat flow map of Io has been created, incorporating data down to spatial resolutions of ∼10 km pixel ^−1 in Io’s polar regions.
Ashley Gerard Davies +4 more
doaj +1 more source
Abstract In this study, we propose a new mechanism to explain the observed particle flux at discrete energies in the flux tubes connecting to the wakes of the Galilean moons, first reported by Sarkango et al. (2024, https://doi.org/10.1029/2023gl107431) and referred to as “banded flux.” We demonstrate the proposed mechanism using test particle ...
W. W. Eshetu +4 more
wiley +1 more source
Hot Spot Detections and Volcanic Changes on Io during the Juno Epoch: Orbits PJ5 to PJ55
We report volcanic changes on Io since the last Galileo (2002) and New Horizons (2007) flybys as observed by NASA’s Juno spacecraft, examining Io’s volcanism down to the local scale (200 K at 325 individual sites of volcanic activity has been generated ...
Jason E. Perry +3 more
doaj +1 more source
Not just gas: How solids-driven torques shaped the migration of the Galilean moons
Context. A crucial aspect of formation models for the Galilean moons of Jupiter is that the objects survive rapid inward orbital migration. Aims. The primary aim of this study is to investigate the orbital migration of the Galilean moons by incorporating
Gonzalez-Rivas L. +3 more
doaj +1 more source
Plasma Properties at the Orbits of Ganymede and Callisto: Survey of Juno Data
Abstract The space environment around the Galilean moons is important for understanding the interaction of the magnetospheric plasma with their magnetosphere (in the singular case of Ganymede), their atmospheres and surfaces. Juno's orbital evolution brought the spacecraft close to the orbits of Ganymede and Callisto on multiple occasions over several ...
Reign Pagaran +4 more
wiley +1 more source

