Results 61 to 70 of about 6,328 (164)

Map of Jupiter's Radiation Environment From Juno's In‐Situ Observations

open access: yesJournal of Geophysical Research: Planets, Volume 130, Issue 3, March 2025.
Abstract Since its orbit insertion on 4 July 2016, the Juno spacecraft has orbited Jupiter in a highly elliptical, polar orbit. With every orbit, Juno's line of apsides migrates, increasing the angle relative to the Jovian equator. Therefore, the spacecraft traverses across the inner regions of the radiation belt, where energetic particles are trapped.
M. Herceg   +9 more
wiley   +1 more source

A Survey of Magnetic Field Line Curvature in Jovian Dawn Magnetodisc

open access: yesGeophysical Research Letters
The Jovian magnetosphere is highly dynamic, influenced by both solar wind and internal processes associated with the rapid planetary rotation and Io's volcanic activities.
W. D. Gu   +8 more
doaj   +1 more source

Bursty Variations of Jovian 6cm Radio Emissions and Quasi-Periodic Jupiter's Polar Activities [PDF]

open access: yesarXiv, 2012
In reference to Jupiter south polar quasi-periodic 40-50 min (QP-40) activities and the model scenario for global QP-40 oscillations of the Jovian inner radiation belt (IRB), we validate relevant predictions and confirmations by amassing empirical evidence from Ulysses, Cassini, Chandra, Galileo, XMM-Newton, and Advanced Composition Explorer for ...
arxiv  

Electron Densities in Jupiter's Upper Ionosphere Inferred From Juno Plasma Wave Observations

open access: yesJournal of Geophysical Research: Planets, Volume 130, Issue 3, March 2025.
Abstract Juno's highly eccentric polar orbit takes it to perijove distances of ∼ ${\sim} $1.06 RJ ${\mathrm{R}}_{J}$ on each orbit. For the first perijove, this occurred just north of the jovigraphic equator, but has precessed north by about a degree per orbit over the mission.
W. S. Kurth   +17 more
wiley   +1 more source

Origin of the Different Architectures of the Jovian and Saturnian Satellite Systems [PDF]

open access: yes, 2010
The Jovian regular satellite system mainly consists of four Galilean satellites that have similar masses and are trapped in mutual mean motion resonances except for the outer satellite, Callisto. On the other hand, the Saturnian regular satellite system has only one big icy body, Titan, and a population of much smaller icy moons.
arxiv   +1 more source

In situ evidence of the magnetospheric cusp of Jupiter from Juno spacecraft measurements

open access: yesNature Communications
The magnetospheric cusp connects the planetary magnetic field to interplanetary space, offering opportunities for charged particles to precipitate to or escape from the planet.
Y. Xu   +15 more
doaj   +1 more source

Forward and Inverse Modeling for Jovian Seismology [PDF]

open access: yes, 2012
Jupiter is expected to pulsate in a spectrum of acoustic modes and recent re-analysis of a spectroscopic time series has identified a regular pattern in the spacing of the frequencies \citep{gaulme2011}. This exciting result can provide constraints on gross Jovian properties and warrants a more in-depth theoretical study of the seismic structure of ...
arxiv   +1 more source

Evaluating Poly‐D,L‐Lactic Acid for Lower Eyelid Rejuvenation: Efficacy and Safety

open access: yesJournal of Cosmetic Dermatology, Volume 24, Issue 3, March 2025.
ABSTRACT Background Injectable fillers like PDLLA offer a novel approach to addressing lower eyelid rejuvenation. Despite their growing popularity, comprehensive studies on newer products like PDLLA are limited. Aims This study evaluates the efficacy and safety of PDLLA (Juvelook, VAIM Inc., Seoul, Korea) for treating tear trough deformities in Korean ...
Jovian Wan   +7 more
wiley   +1 more source

Revisiting Jovian-Resonance Induced Chondrule Formation [PDF]

open access: yes, 2014
It is proposed that planetesimals perturbed by Jovian mean-motion resonances are the source of shock waves that form chondrules. It is considered that this shock-induced chondrule formation requires the velocity of the planetesimal relative to the gas disk to be on the order of > 7 km/s at 1 AU.
arxiv   +1 more source

Conditions to Consider When Choosing Fillers

open access: yesJournal of Cosmetic Dermatology, Volume 24, Issue 3, March 2025.
ABSTRACT Background The selection of dermal fillers in aesthetic medicine often relies on factors such as cost, immediate outcomes, and practitioner experience. However, incorporating knowledge of fillers' rheological properties, such as viscoelasticity and cohesiveness, allows for more precise product selection tailored to patient needs and treatment ...
Gi‐Woong Hong   +4 more
wiley   +1 more source

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