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• W1976646676 abstract "This study reports direct detection by the Cassini plasma spectrometer of freshly-produced water-group ions (O{sup +}, OH{sup +}, H{sub 2}O{sup +}, H{sub 3}O{sup +}) and heavier water dimer ions (H{sub x}O{sub 2}{sup +}) very close to Enceladus and where the plasma begins to emerge from the Enceladus plume The data wcre obtained during two close (52 and 25 km) flybys of Enceladus in 2008, and are similar to ion data in cometary comas. The ions are observed in detectors looking in the Cassini ram direction at energies consistent with the Cassini speed, indicating a nearly stagnant plasma flow in the plume. North of Enceladus the plasma slowing commences about 4 to 6 Enceladus radii away, while south of Enccladus signatures ofthe interaction are detected as far as 22 Enceladus radii away." @default.
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• W1976646676 date "2009-07-15" @default.
• W1976646676 modified "2023-09-27" @default.
• W1976646676 title "Cassini detection of Enceladus' cold water-group plume ionosphere" @default.
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• W1976646676 doi "https://doi.org/10.1029/2009gl038923" @default.
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