TL;DR
This paper investigates how centrifugal gravity and rotation influence acoustic modes in fluid-filled ellipsoids, providing a refined wave equation and numerical solutions relevant for experimental rotation rate measurements.
Contribution
It derives an exact wave equation for acoustic velocity in rotating fluids under centrifugal gravity and applies polynomial spectral methods for solutions, advancing understanding of acoustic modes in rotating ellipsoids.
Findings
Centrifugal acceleration affects acoustic frequencies at high rotational Mach numbers.
The polynomial spectral method accurately solves the wave problem in ellipsoids.
Experimental regimes with high compressibility gases can reach measurable effects.
Abstract
The acoustic modes of a rotating fluid-filled cavity can be used to determine the effective rotation rate of a fluid (since the resonant frequencies are modified by the flows). To be accurate, this method requires a prior knowledge of the acoustic modes in rotating fluids. Contrary to the Coriolis force, centrifugal gravity has received much less attention in the experimental context. Motivated by on-going experiments in rotating ellipsoids, we study how global rotation and buoyancy modify the acoustic modes of fluid-filled ellipsoids in isothermal (or isentropic) hydrostatic equilibrium. We go beyond the standard acoustic equation, which neglects solid-body rotation and gravity, by deriving an exact wave equation for the acoustic velocity. We then solve the wave problem using a polynomial spectral method in ellipsoids, which is compared with finite-element solutions of the primitive…
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