Abstract
We study the axisymmetric inertial oscillations in a confined monopolar vortex under the influence of background rotation. By first focusing on the inviscid linear dynamics, and later studying the effects of viscosity and of a no-slip bottom, we characterize the effects of rotation and confinement. It was found that background rotation allows for oscillations outside the vortex core even with frequencies larger than 2Ω, with Ω the background rotation rate. However, confinement is necessary for the system to sustain oscillations with frequencies smaller than 2Ω. Through the analytical solution for a small perturbation of a Rankine vortex, we obtain five regimes where the oscillations are qualitatively different, depending on their frequency. Numerical results for the linear inviscid waves sustained by a Lamb-Oseen vortex show a similar behavior. The effects of viscosity are twofold: the oscillations are damped and the vortex sustaining the oscillations is modified. When a no-slip bottom is considered, a boundary layer drives a secondary motion superimposed on the inertial oscillations. In this case, the vortex is quickly damped, but the oscillations persist due to the background rotation. © 2009 American Institute of Physics.
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CITATION STYLE
Duran-Matute, M., Kamp, L. P. J., Trieling, R. R., & van Heijst, G. J. F. (2009). Inertial oscillations in a confined monopolar vortex subjected to background rotation. Physics of Fluids, 21(11), 1–13. https://doi.org/10.1063/1.3258670
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