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• W2003610557 startingPage "1479" @default.
• W2003610557 abstract "Saturn encounter trajectories of Pioneer 11, Voyager 1, and Voyager 2 passed through the noon-dusk quadrant of the middle magnetosphere during approach and through dawn-midnight outbound. Intensities of energetic electrons (≥0.6 MeV) were an order of magnitude higher inbound than outbound at 6–15 Rs, even though the same (Pioneer 11) or higher (Voyager 1 and 2) intensities were expected outbound for stably trapped electrons with azimuthally symmetric distributions. Explanations include electron drift shell asymmetry arising from (1) magnetopause compression by the solar wind and/or (2) dusk-to-dawn electric field associated with solar wind driven convection within the magnetosphere. Theoretical and numerical calculations indicate that maximum effects of the electric field are expected at L-dependent drift resonance energies in the range of the maximum observed asymmetries. Maximum intensities would then be expected on the dusk side of the middle magnetosphere where “bannana”-shaped drift shells are expected near the resonance energies. Since some of the asymmetric drift shells would not extend around to the dawn side, minimum intensities would be expected there as observed. Further analysis and modeling will be needed to assess the relative effects of the electric field magnetopause compression, and other possible causes. Full local time coverage of energetic particles by the Cassini Orbiter mission would be invaluable for additional constraints on the magnetospheric electric and magnetic fields." @default.
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• W2003610557 date "1998-01-01" @default.
• W2003610557 modified "2023-10-09" @default.
• W2003610557 title "Local time asymmetry of drift shells for energetic electrons in the middle magnetosphere of Saturn" @default.
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• W2003610557 doi "https://doi.org/10.1016/s0273-1177(98)00022-2" @default.
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