Results 21 to 30 of about 6,328 (164)
Earth and Planetary Physics, 2018 Wave-particle interactions triggered by whistler-mode chorus waves are an important contributor to the Jovian radiation belt electron dynamics. While the sensitivity of chorus-driven electron scattering to the ambient magnetospheric and wave parameters ...
Jing Huang +6 more
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Earth and Planetary Physics, 2018 We present preliminary results of a new global Magnetohydrodynamics (MHD) simulation model of the Jovian magnetosphere. The model incorporates mass loading from Jupiter's satellite Io, the planet's fast corotation, and electrostatic coupling between its ...
YuXian Wang +4 more
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Variability of Jovian ion winds: an upper limit for enhanced Joule heating [PDF]
Annales Geophysicae, 2007 It has been proposed that short-timescale fluctuations about the mean electric field can significantly increase the upper atmospheric energy inputs at Jupiter, which may help to explain the high observed thermospheric temperatures.
M. B. Lystrup +8 more
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Modeling of the Jovian Magnetosphere [PDF]
Annales Geophysicae, 2005 This paper presents a global model of the Jovian magnetosphere which is valid not only in the equatorial plane and near the planet, as most of the existing models are, but also at high latitudes and in the outer regions of the magnetosphere. The model
I. I. Alexeev, E. S. Belenkaya
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A Passive Probe for Subsurface Oceans and Liquid Water in Jupiter's Icy Moons [PDF]
, 2014 We describe an interferometric reflectometer method for passive detection of subsurface oceans and liquid water in Jovian icy moons using Jupiter's decametric radio emission (DAM). The DAM flux density exceeds 3,000 times the galactic background in the neighborhood of the Jovian icy moons, providing a signal that could be used for passive radio ...
arxiv +1 more source
Observations of electromagnetically coupled dust in the Jovian magnetosphere [PDF]
Astrophys.Space Sci. 264 (1999) 247-256, 1998 We report on dust measurements obtained during the seventh orbit of the Galileo spacecraft about Jupiter. %which had a close flyby at Ganymede. The most prominent features observed are highly time variable dust streams recorded throughout the Jovian system.
arxiv +1 more source
Detectability of H2-Ar and H2-Ne Dimers in Jovian Atmospheres [PDF]
Journal of Astronomy and Space Sciences, 1997 The detection of jovian hydrogen-hydrogen dimers through the clear telluric 2-micron window(Kim et al. 1995, Trafton et al. 1997) suggests possibility to detect noble gases in the form of dimer with hydrogen in jovian atmospheres.
Young-Key Minn +3 more
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Juno Observations of Ion‐Inertial Scale Flux Ropes in the Jovian Magnetotail
Geophysical Research Letters, 2021 Two ion‐inertial scale magnetic flux ropes are identified in the Juno magnetic field measurements in the dawnside Jovian magnetotail. Previously reported plasmoids in this region had typical diameters of several Jovian radii (RJ).
Yash Sarkango +7 more
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Solar Control on Jupiter's Equatorial X-ray Emissions: 26-29 November 2003 XMM-Newton Observation [PDF]
Geophys.Res.Lett. 32 (2005) L03S08, 2005 During November 26-29, 2003 XMM-Newton observed soft (0.2-2 keV) X-ray emission from Jupiter for 69 hours. The low-latitude X-ray disk emission of Jupiter is observed to be almost uniform in intensity with brightness that is consistent with a solar-photon driven process.
arxiv +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
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