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Updated: May 2, 2026

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Assembly and Characterization of an External Driver for the Generation of Sub-Kilohertz Oscillatory Flow in Microchannels
Published on: January 28, 2022
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Rapidly rotating cylinder flow with an oscillating sidewall.
Juan M Lopez1, Francisco Marques2
1School of Mathematical and Statistical Sciences, Arizona State University, Tempe, Arizona 85287, USA.
Summary
Numerical simulations reveal robust inertial waves in rapidly rotating cylinders driven by sidewall oscillations. These waves, resembling Lord Kelvin
Area of Science:
- Fluid Dynamics
- Rotating Systems
- Wave Phenomena
Background:
- Inertial waves are fundamental in rotating fluid systems.
- Previous studies often faced challenges with driving mechanisms causing instabilities.
Purpose of the Study:
- To numerically simulate and theoretically analyze inertial waves in a rapidly rotating cylinder.
- To investigate the role of time-periodic sidewall forcing on inertial wave generation.
- To explore the robustness and experimental realizability of these driven inertial waves.
Main Methods:
- Numerical simulations of fluid flow in a rotating cylinder with axial sidewall oscillations.
- Detailed theoretical analysis of internal shear layers.
- Comparison with inviscid eigenmodes and ray tracing techniques.
Main Results:
- Inertial waves in the form of shear layers are present when oscillation frequency is less than twice the rotation frequency.
- For rapid rotations, waves approximate Lord Kelvin's inviscid predictions.
- The oscillating Stokes layer and corner discontinuities act as robust driving mechanisms.
Conclusions:
- The system provides a physically realizable and robust method for studying inertial waves.
- Inertial waves remain stable across a wide range of parameters, unlike other experimental setups.
- The findings offer a promising platform for experimental investigations of inertial waves.
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