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- W2153719704 abstract "Abstract Jupiter's moons, embedded in the magnetized, flowing plasma of Jupiter's magnetosphere, the plasma seas of the title, are fluids whose highly non-linear interactions imply complex behavior. In a plasma, magnetic fields couple widely separated regions; consequently plasma interactions are exceptionally sensitive to boundary conditions (often ill-specified). Perturbation fields arising from plasma currents greatly limit our ability to establish more than the dominant internal magnetic field of a moon. With a focus on Ganymede and a nod to Io, this paper discusses the complexity of plasma-moon interactions, explains how computer simulations have helped characterize the system and presents improved fits to Ganymede's internal field." @default.
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- W2153719704 date "2010-01-01" @default.
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- W2153719704 title "Medicean Moons Sailing Through Plasma Seas: Challenges in Establishing Magnetic Properties" @default.
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- W2153719704 doi "https://doi.org/10.1017/s1743921310007271" @default.
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