Results 31 to 40 of about 6,029 (233)
Dust on the Outskirts of the Jovian System
Icarus, 2002 Abstract The outer region of the jovian system between ∼50 and 300 jovian radii from the planet is found to be the host of a previously unknown dust population. We used the data from the dust detector aboard the Galileo spacecraft collected from December 1995 to April 2001 during Galileo's numerous traverses of the outer jovian system.
Krivov, A. +4 more
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The Response of Broadband Kilometric Radiation to Compressions of the Jovian Magnetosphere
The Astrophysical JournalIn the planetary magnetosphere, plasma waves act as the medium for particles to transfer energy. Jupiter is the largest planet in our solar system, and the giant magnetosphere is full of energetic particles, producing intense radio emissions.
Yuening Chen +3 more
doaj +1 more source
Ephemerides of the outer Jovian satellites [PDF]
Astronomy & Astrophysics, 2005 The results of the determination of orbits for 54 outer satellites of Jupiter based on all available observations of these satellites are presented. The problem was solved using numerical integration method applied to the equations of satellite motion. After initial conditions of integration were refined, the residuals of observations from theory were ...
openaire +4 more sources
A Specification Model of Saturn's Plasma Environment
Journal of Geophysical Research: Space Physics, Volume 130, Issue 10, October 2025.Abstract We present the first empirical‐based specification model of Saturn's plasma environment based on the analysis of all publicly available plasma moment data sets derived using multiple techniques from Cassini observations made by the Cassini Plasma Spectrometer and the Radio and Plasma Wave Science instrument.
A. Kamran +8 more
wiley +1 more source
Remote sensing of the Io torus plasma ribbon using natural radio occultation of the Jovian radio emissions [PDF]
Annales Geophysicae, 2014 We study the Jovian hectometric (HOM) emissions recorded by the RPWS (Radio and Plasma Wave Science) experiment onboard the Cassini spacecraft during its Jupiter flyby.
M. Y. Boudjada +3 more
doaj +1 more source
Journal of Geophysical Research: Space Physics, Volume 130, Issue 10, October 2025.Abstract Jupiter's auroral regions have previously been defined by broad‐scale auroral structures, but these are typically obscured by the wide array of temporal variability observed at timescales between minutes and days, making it difficult to understand the underlying magnetospheric biases driving these brightness differences.
Tom S. Stallard +9 more
wiley +1 more source
Combined Full Wave and Test Particle Simulations of the Io Footprint in the Jovian Aurora
Journal of Geophysical Research: Space Physics, Volume 130, Issue 10, October 2025.Abstract It is known that the perturbation of the co‐rotating plasma of Jupiter by Io propagates as Alfvén waves along the magnetic field lines. These waves accelerate electrons, which leads to precipitation and the formation of an auroral footprint on the ionosphere.
W. W. Eshetu +3 more
wiley +1 more source
Reconnection in the Jovian magnetosphere
Geophysical Research Letters, 1983 In the nightside Jovian magnetosphere, Voyager 1 and 2 detected signatures of reconnection. The anti‐sunward streaming events, recognized and designated as magnetospheric winds by Krimigis et al., were clearly associated with the northward inclination of the magnetic field.
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Emission of Energetic Neutral Atoms From Ganymede's Magnetosphere‐Atmosphere Interaction
Journal of Geophysical Research: Space Physics, Volume 130, Issue 10, October 2025.Abstract This study analyzes the emission of energetic neutral atoms (ENAs), generated by charge exchange between energetic protons and Ganymede's atmosphere. We also constrain the observability of such ENAs by an imaging instrument aboard a spacecraft.
C. Michael Haynes +2 more
wiley +1 more source
TOI-1670 c, a 40 day Orbital Period Warm Jupiter in a Compact System, Is Well Aligned
The Astrophysical Journal Letters, 2023 We report the measurement of the sky-projected obliquity angle λ of the warm Jovian exoplanet TOI-1670 c via the Rossiter–McLaughlin effect. We observed the transit window during UT 2023 April 20 for 7 continuous hours with NEID on the 3.5 m WIYN ...
Jack Lubin +23 more
doaj +1 more source