Resonant and non-resonant flows in longitudinally and latitudinally librating spheres

被引:3
|
作者
Lin, Yufeng [1 ]
Hollerbach, Rainer [2 ,3 ]
Noir, Jerome [4 ]
Vantieghem, Stijn [4 ]
机构
[1] Southern Univ Sci & Technol, Dept Earth & Space Sci, Shenzhen 518055, Peoples R China
[2] Univ Leeds, Dept Appl Math, Leeds LS2 9JT, England
[3] Isaac Newton Inst Math Sci, 20 Clarkson Rd, Cambridge CB3 0EH, England
[4] Swiss Fed Inst Technol, Inst Geophys, Sonneggstr 5, CH-8092 Zurich, Switzerland
基金
英国工程与自然科学研究理事会; 瑞士国家科学基金会;
关键词
INERTIAL OSCILLATIONS; SPHEROIDAL CAVITY; FLUID MOTION; DRIVEN; ELLIPSOIDS; PRECESSION; WAVES; MODES;
D O I
10.1063/5.0142705
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
We investigate the linear response to longitudinal and latitudinal libration of a rapidly rotating fluid-filled sphere. Asymptotic methods are used to explore the structure of resonant modes in both cases, provided that the nondimensional libration frequency is in the range ? & ISIN; [ 0 , 2 ]. High-resolution numerics are then used to map out this entire frequency range, picking out both the resonant peaks as well as the non-resonant troughs in between. The kinetic energy is independent of the Ekman number E at the peaks and scales as E 1 / 2 at the troughs. As the Ekman number is reduced, down to E = 10 - 10 for longitudinal libration and E = 10 - 9 for latitudinal libration, the frequency response also exhibits an increasingly fractal structure, with more and more peaks and troughs emerging. The spacing between peaks is seen to follow an E 1 / 2 self-similarity factor. However, detailed examinations of some of the more prominent troughs shows that their widths follow an E & SIM; 0.23 self-similarity factor.
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页数:15
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