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Nature, 2008
Planetary aurorae are formed by energetic charged particles streaming along the planet's magnetic field lines into the upper atmosphere from the surrounding space environment. Earth's main auroral oval is formed through interactions with the solar wind, whereas that at Jupiter is formed through interactions with plasma from the moon Io inside its ...
Stallard, T +7 more
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Planetary aurorae are formed by energetic charged particles streaming along the planet's magnetic field lines into the upper atmosphere from the surrounding space environment. Earth's main auroral oval is formed through interactions with the solar wind, whereas that at Jupiter is formed through interactions with plasma from the moon Io inside its ...
Stallard, T +7 more
openaire +3 more sources
AIP Conference Proceedings, 1990
Observations of the long‐term variations in the motions and morphology of the cloud systems in the atmospheres of Jupiter, Saturn, Uranus and Neptune have been hampered by terrestrial atmospheric effects, a limited range of accessible band passes, the necessity to sacrifice spectral resolution to achieve reasonable spatial resolution, and the inability
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Observations of the long‐term variations in the motions and morphology of the cloud systems in the atmospheres of Jupiter, Saturn, Uranus and Neptune have been hampered by terrestrial atmospheric effects, a limited range of accessible band passes, the necessity to sacrifice spectral resolution to achieve reasonable spatial resolution, and the inability
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Reviews of Geophysics, 1983
The 1979–82 quadrennium was a time of unprecedented excitement and achievement in Jovian magnetospheric physics, highlighted by the traversais by Voyager‐1 and ‐2 (V‐1, ‐2) in March and July 1979. Our knowledge has been expanded immensely by Voyager observations and their interpretations, and this review is devoted largely to them. Not to be overlooked,
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The 1979–82 quadrennium was a time of unprecedented excitement and achievement in Jovian magnetospheric physics, highlighted by the traversais by Voyager‐1 and ‐2 (V‐1, ‐2) in March and July 1979. Our knowledge has been expanded immensely by Voyager observations and their interpretations, and this review is devoted largely to them. Not to be overlooked,
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Reports on Progress in Physics, 1998
Sang Joon Kim, Dong Hun Lee, Yong Ha Kim
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Sang Joon Kim, Dong Hun Lee, Yong Ha Kim
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Advances in Space Research, 1986
The current understanding of the plasma, magnetic field, and plasma wave characteristics of the near and distant Jovian magnetotail is discussed. The properties of these two regions are compared, with particular emphasis given to the data on the distant tail obtained by Voyager 2.
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The current understanding of the plasma, magnetic field, and plasma wave characteristics of the near and distant Jovian magnetotail is discussed. The properties of these two regions are compared, with particular emphasis given to the data on the distant tail obtained by Voyager 2.
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Images of embedded Jovian planet formation at a wide separation around AB Aurigae
Nature Astronomy, 2022Thayne Currie +2 more
exaly
Moist convection drives an upscale energy transfer at Jovian high latitudes
Nature Physics, 2022Lia Siegelman +2 more
exaly
2015
On June 27, 363, Jovian was crowned Roman emperor after the sudden death of Julian during Rome’s Persian campaign. To get the Roman army safely out of Persian territory, he concluded a treaty with Shapur II at the cost of surrendering regions and strongholds, among them the city of Nisibis.
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On June 27, 363, Jovian was crowned Roman emperor after the sudden death of Julian during Rome’s Persian campaign. To get the Roman army safely out of Persian territory, he concluded a treaty with Shapur II at the cost of surrendering regions and strongholds, among them the city of Nisibis.
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