Results 41 to 50 of about 6,029 (233)
Abstract The Galilean satellite Europa is a primary candidate for the study of ocean worlds. In anticipation of NASA's Europa Clipper and ESA's JUICE missions, we revisit the magnetic field measurements of the Galileo spacecraft. The ocean's induction response is governed by its induction amplitude and phase shift, which are a function of the ocean ...
Jason Winkenstern +2 more
wiley +1 more source
Radio detection at high time-frequency resolutions is a powerful means of remotely studying electron acceleration processes. Radio bursts have characteristics (polarization, drift, periodicity) making them easier to detect than slowly variable emissions.
Emilie Mauduit +3 more
doaj +1 more source
Antum Crater: A Window Into Ganymede's Icy Evolution
Abstract Located within the extensive dark terrain of Marius Regio, in the anti‐Jovian trailing quadrant of Ganymede, Antum crater is marked by dark‐rayed ejecta that obscure older features and reshape the surrounding landscape. This study investigates Antum and its geological context using optical and infrared data from the Voyager and Galileo ...
Federico Tosi +9 more
wiley +1 more source
Statistical Distributions of Plasma Density and Pressure in the Jovian Plasma Sheet
The Jovian plasma sheet is a key region of the Jovian magnetosphere populated by a mix of warm and hot plasma. It is the main channel for radial transport of mass and energy in the Jovian magnetosphere and provides a favorable environment for magnetic ...
Haobo Fu +7 more
doaj +1 more source
OBSERVATIONS OF THE MUTUAL PHENOMENA OF THE GALILEAN MOONS IN 2009
The instrumental and ephemeris preparation for the photometric observations of the mutual phenomena in the system of planetary satellites was conducted within the PHEMU09 project.
N. Koshkin +10 more
doaj +1 more source
In this study, observations from the Jovian auroral distributions experiment, Jupiter energetic particle detector instrument, and Magnetic field investigation instruments on Juno are used to identify signatures of magnetic reconnection at Jupiter's dawn ...
J. Montgomery +8 more
doaj +1 more source
On the Equation of State in Jovian Seismology [PDF]
AbstractWe have investigated the effect on the seismological properties of the giant planet Jupiter of different descriptions of the equation of state (EOS) of the fluid hydrogen helium envelop. Recent Jovian models by Chabrier et al. 1992 use the equation of state of Saumon et al. (1992) which predicts the PPT (plasma phase transition).
J. Provost, Gilles Chabrier, B. Mosser
openaire +2 more sources
Abstract Whistler‐mode waves play a crucial role in shaping magnetospheric electron dynamics. Using Juno's observations, we investigate these waves in Jupiter's post‐midnight‐to‐dawn magnetosphere, spanning 20–80 Jupiter radii. Our survey reveals that whistler‐mode waves predominantly occur in the lobes, while the magnetodisk remains largely devoid of ...
Z.‐Y. Liu +9 more
wiley +1 more source
Detection of Negative Carbon and Oxygen Pickup Ions From Dust Orbiting Jupiter
Abstract We report on observations of negative carbon and oxygen pickup ions (PUIs) originating from dust orbiting Jupiter. The PUIs are observed at altitudes of a few thousand kilometers (∼4,800–10,200 km) above the 1‐bar level of Jupiter's atmosphere and up to ∼11,000–15,000 km from the equatorial plane, thus providing constraints on the location of ...
F. Allegrini +14 more
wiley +1 more source
Radial Evolution of Electron Pitch Angle Distributions in the Inner Part of Jovian Magnetosphere
Abstract Previous observations in Jupiter's magnetosphere have revealed that the pitch‐angle distributions (PADs) of energetic (>∼102 ${ >} \sim 1{0}^{2}$ keV) electrons transition from pancake to field‐aligned distributions from ∼ ${\sim} $10 to 20 Jupiter radii.
Z.‐Y. Liu +9 more
wiley +1 more source

