Results 21 to 30 of about 66 (64)
Abstract Jupiter's moon Callisto orbits in a highly variable magnetospheric environment depending on its position relative to the Jovian current sheet. The Juno and Galileo missions have visited the Jovian magnetosphere and crossed Callisto's orbit several times in a variety of configurations, providing an opportunity to better characterize Callisto's ...
T. Le Liboux +23 more
wiley +1 more source
Super‐Corotating Flows in Plasma Disk Within 30 Jupiter Radii
Abstract Plasma circulation and magnetic reconnection are crucial for understanding the dynamics of Jupiter's magnetosphere. Previous studies identified hundreds of reconnection sites at distances of 50–100 RJ ${\mathrm{R}}_{J}$ from magnetic field signatures.
Jian‐Zhao Wang +9 more
wiley +1 more source
Acceleration of Energetic Electrons in Jovian Middle Magnetosphere by Whistler‐Mode Waves
Abstract An abundant multi‐MeV electron population beyond the orbit of Io is required to explain the intense inner radiation belt (electrons >50 ${ >} 50$ MeV) at Jupiter and its synchrotron radiation. In order to better understand the synergistic effect of radial transport and local wave‐particle interactions driven by whistler‐mode waves on the ...
Y.‐X. Hao +13 more
wiley +1 more source
Jupiter's Whistler‐Mode Belts and Electron Slot Region
Abstract The spatial distribution of whistler‐mode wave emissions in the Jovian magnetosphere measured during the first 45 perijove orbits of Juno is investigated. A double‐belt structure in whistler‐mode wave intensity is revealed. Between the two whistler‐mode belts, there exists a region devoid of 100 s keV electrons near the magnetic equator at 9
Y.‐X. Hao +13 more
wiley +1 more source
Dawn‐Dusk Asymmetry of Plasma Flow in Jupiter's Middle Magnetosphere Observed by Juno
Abstract Based on plasma observations from Juno's Jovian Auroral Distributions Experiment instrument and forward modeling, we investigate the dawn‐dusk asymmetries within Jupiter's magnetosphere between 10 and 40 RJ ${\mathrm{R}}_{J}$. On the dawnside, the flux tubes are depleted characterized by low density and near rigid‐corotation velocity, with a ...
Jian‐Zhao Wang +8 more
wiley +1 more source
Abstract Plasmoids and magnetic field dipolarizations are reconnection‐related phenomena often resulting in reconfiguration of the magnetic field and energetic particle acceleration in planetary magnetotail. Building on the work of Blöcker et al. (2023) (10.1029/2023JA031312), we selected seven specific events from their magnetic field dipolarization ...
A. Blöcker +4 more
wiley +1 more source
Abstract Jupiter's moon Europa contains a subsurface ocean whose presence is inferred from magnetic field measurements, the interpretation of which depends on knowledge of Europa's local plasma environment. A recent Juno spacecraft flyby returned new observations of plasma electrons with unprecedented resolution.
F. Allegrini +17 more
wiley +1 more source
Energetic Charged Particle Measurements During Juno's Two Close Io Flybys
Abstract On days 2023‐364 and 2024‐034, the Juno spacecraft made close passages of Jupiter's moon Io, at altitudes of about 1,500 km. Data obtained from the first flyby, when the spacecraft was on magnetic field lines connected to both Jupiter and Io, revealed deep flux decreases.
C. Paranicas +9 more
wiley +1 more source
Energetic Oxygen and Sulfur Charge States in the Outer Jovian Magnetosphere: Insights From the Cassini Jupiter Flyby. [PDF]
Allen RC +12 more
europepmc +1 more source
The "Puck" energetic charged particle detector: Design, heritage, and advancements. [PDF]
Clark G +19 more
europepmc +1 more source

