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- W2095328664 abstract "the conditions during the Voyager 1 flyby. Our model shows that the ionotail and the magnetotail bend in a direction opposite to the convection electric field. This is validated with the total force on the incident flow species derived from basic plasma equations. We also present a simulated impact map for the oxygen ions of the flow with total O + precipitation rate 1.3 � 10 24 s � 1 at Titan’s exobase. Although this rate indicates that the plasma conditions above the exobase do not inhibit O + precipitation on the exobase, the direction of the O + flow is shown to turn drastically near the exobase. The energy deposition of the medium-weight flow ions (such as O + ) thus seems to be orders of magnitude larger than the energy deposition by pickup ions formed near Titan. However, the lightweight flow ions (H + ) are effectively deflected by the magnetic barrier formed around Titan." @default.
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- W2095328664 date "2007-12-01" @default.
- W2095328664 modified "2023-09-28" @default.
- W2095328664 title "Oxygen ions at Titan's exobase in a Voyager 1-type interaction from a hybrid simulation" @default.
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- W2095328664 doi "https://doi.org/10.1029/2007ja012348" @default.
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