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Libration-driven multipolar instabilities

Published online by Cambridge University Press:  02 January 2014

D. Cébron ,
S. Vantieghem  and
W. Herreman
D. Cébron*
Affiliation:
Institut für Geophysik, Sonneggstrasse 5, ETH Zürich, CH-8092 Zürich, Switzerland
S. Vantieghem
Affiliation:
Institut für Geophysik, Sonneggstrasse 5, ETH Zürich, CH-8092 Zürich, Switzerland
W. Herreman
Affiliation:
Université de Paris-Sud (LIMSI-CNRS), BP 133, F-91403 Orsay CEDEX, France
*
†Email address for correspondence: [email protected]
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Abstract

We consider rotating flows in non-axisymmetric enclosures that are driven by libration, i.e. by a small periodic modulation of the rotation rate. Thanks to its simplicity, this model is relevant to various contexts, from industrial containers (with small oscillations of the rotation rate) to fluid layers of terrestrial planets (with length-of-day variations). Assuming a multipolar $n$-fold boundary deformation, we first obtain the two-dimensional basic flow. We then perform a short-wavelength local stability analysis of the basic flow, showing that an instability may occur in three dimensions. We christen it the libration-driven multipolar instability (LDMI). The growth rates of the LDMI are computed by a Floquet analysis in a systematic way, and compared to analytical expressions obtained by perturbation methods. We then focus on the simplest geometry allowing the LDMI, a librating deformed cylinder. To take into account viscous and confinement effects, we perform a global stability analysis, which shows that the LDMI results from a parametric resonance of inertial modes. Performing numerical simulations of this librating cylinder, we confirm that the basic flow is indeed established and report the first numerical evidence of the LDMI. Numerical results, in excellent agreement with the stability results, are used to explore the nonlinear regime of the instability (amplitude and viscous dissipation of the driven flow). We finally provide an example of LDMI in a deformed spherical container to show that the instability mechanism is generic. Our results show that the previously studied libration-driven elliptical instability simply corresponds to the particular case $n= 2$ of a wider class of instabilities. Summarizing, this work shows that any oscillating non-axisymmetric container in rotation may excite intermittent, space-filling LDMI flows, and this instability should thus be easy to observe experimentally.

JFM classification

Instability: Parametric instability Geophysical and Geological Flows: Rotating flows Geophysical and Geological Flows: Topographic effects
Type
Papers
Information
Journal of Fluid Mechanics , Volume 739 , 25 January 2014 , pp. 502 - 543
Copyright
©2013 Cambridge University Press 

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