Tesseral Harmonics of Jupiter from Static Tidal Response
نویسندگان
چکیده
منابع مشابه
Radio Emission from Jupiter
Three reviews of radio emission from Jupiter have appeared recently (1, 2, 3) and at least one more is currently in press. The present review primarily covers work since 1961. It would be not too strong to suggest that explanations of Jupiter's emission now are in the second generation, with most observational phenomena fairly well established. The salient observed features are not widely known...
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We study global inertial-modes with the purpose of unraveling the role they play in the tidal dissipation process of Jupiter. For spheres of uniformly rotating, neutrally buoyant fluid, we show that the partial differential equation governing inertial-modes can be separated into two ordinary differential equations when the density is constant, or when the density has a power-law dependence on r...
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Having studied the structure and properties of inertial-modes in a neutrally buoyant, uniformly rotating sphere (Wu 2004), we examine here their effect on tidal dissipation in Jupiter. The rate of tidal dissipation caused by resonantly excited inertial-modes depends on the following three parameters: how well coupled inertial-modesare to the tidal potential, how strongly dissipated inertial-mod...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2019
ISSN: 1538-4357
DOI: 10.3847/1538-4357/ab0c03