2014
DOI: 10.1017/jfm.2013.623
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Libration-driven multipolar instabilities

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 terrestial 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 anal… Show more

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Cited by 12 publications
(15 citation statements)
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“…This Poisson equation is solved with the algebraic multigrid method BoomerAMG (Henson & Yang 2002). Discussions regarding the performance of this code can be found in Marti et al (2014) and Cébron et al (2014).…”
Section: Numerical Validation and Discussionmentioning
confidence: 99%
“…This Poisson equation is solved with the algebraic multigrid method BoomerAMG (Henson & Yang 2002). Discussions regarding the performance of this code can be found in Marti et al (2014) and Cébron et al (2014).…”
Section: Numerical Validation and Discussionmentioning
confidence: 99%
“…This method was confirmed in the multipolar stability analysis in a librating deformed cylinder and sphere in Ref. 47. A general formula of the typical growth rate for each calculation of σ inv is given for f around the resonant forcing frequency…”
Section: E Growth Ratesmentioning
confidence: 78%
“…30,47 An analogous equation can be made for a j . Since inertial modes exist within a frequency from [−2, 2], the resonance condition in (14) allows for the existence of elliptical instability in flows from | f | = 0 − 4.…”
Section: Elliptical Instabilitymentioning
confidence: 99%
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“…This instability develops in rotating fluids when the streamlines are deformed into ellipses. Its linear growth, due to the resonance of two inertial waves with the elliptical basic flow, is well described both theoretically [2,[9][10][11] and experimentally [3][4][5]12]. The nonlinear saturation of the elliptical instability remains poorly understood, but it is the relevant regime to describe vortex core breakdown [13], as well as dissipation and magnetic field generation in planetary cores [14].…”
mentioning
confidence: 99%