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- W171304513 abstract "It is a commonly accepted hypothesis that convective motions are responsible for most flows in planetary and stellar fluid layers, and in particular that convective motions are responsible for planetary dynamos, as it is the case on Earth today. However, the validity of the convective dynamo model can be questioned in certain planets. Besides, even in planets where the dynamo is of convective origin, additional driving mechanisms may significantly modify the organization of fluid motions in their core. The same question holds for all large-scale flows in any fluid layer of astrophysical bodies, such as atmospheres of gas giants, subsurface oceans of icy satellites, and convective/radiative zones of stars. In particular, three mechanical forcings present at the planetary scale remain largely unknown regarding their fluid mechanics and planetary consequences: libration, precession, and tidal distortions. Combining analytical studies with numerical simulations and laboratory experiments, we show here that libration and tides can drive highly energetic turbulent flows, which could for instance participate in the generation of Jupiter bands and in the generation of the past Moon magnetic field. The key point is that flows are excited by resonance mechanisms such as the elliptical instability, where the harmonic forcing only acts as a conveyor to extract energy from the huge reservoir related to the rotational dynamics of planetary systems. Even small forcing can thus have important consequences." @default.
- W171304513 created "2016-06-24" @default.
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- W171304513 date "2013-12-24" @default.
- W171304513 modified "2023-09-25" @default.
- W171304513 title "Flows Driven by Harmonic Forcing in Planetary Atmospheres and Cores" @default.
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- W171304513 doi "https://doi.org/10.1007/978-3-319-00116-6_6" @default.
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