Results 21 to 30 of about 6,029 (233)
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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Constraints on Europa’s Water Group Torus from HST/COS Observations
The Planetary Science Journal, 2023 In situ plasma measurements as well as remote mapping of energetic neutral atoms around Jupiter provide indirect evidence that an enhancement of neutral gas is present near the orbit of the moon Europa.
Lorenz Roth +10 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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International Astronomical Union Colloquium, 1994 AbstractThis paper reviews a new astrophysical subject: seismology of the giant planets. Seismology is dedicated to the sounding of the interior structure of any object; on the other hand, the interiors of the Jovian planets need to be constrained, in order to improve our knowledge of their structure and of their evolution, as well as the ...
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Astrocladistics of the Jovian Trojan Swarms [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 ABSTRACTThe Jovian Trojans are two swarms of small objects that share Jupiter’s orbit, clustered around the leading and trailing Lagrange points, L4 and L5. In this work, we investigate the Jovian Trojan population using the technique of astrocladistics, an adaptation of the ‘tree of life’ approach used in biology.
Timothy R. Holt +7 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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Physical Review DThe BOREXINO experiment has been collecting solar neutrino data since 2007, providing the opportunity to study the variation of the event rate over a decade. We find that at 96% C.L., the rate of low energy events shows a time modulation favoring a correlation with a flux from Jupiter.
Ansarifard, Saeed, Farzan, Yasaman
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Cycles of activity in the Jovian atmosphere [PDF]
Geophysical Research Letters, 2017 AbstractJupiter's banded appearance may appear unchanging to the casual observer, but closer inspection reveals a dynamic, ever‐changing system of belts and zones with distinct cycles of activity. Identification of these long‐term cycles requires access to data sets spanning multiple Jovian years, but explaining them requires multispectral ...
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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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