Inertial wave activity during spin-down in a rapidly rotating penny shaped cylinder

In an earlier paper, Oruba et al. (J. Fluid Mech., vol. 818, 2017, pp. 205–240) considered the primary quasi-steady geostrophic (QG) motion of a constant density fluid of viscosity $\nu$ that occurs during linear spin-down in a cylindrical container of radius $L$ and height $H$, rotating rapidly (an...

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Published inJournal of fluid mechanics Vol. 915
Main Authors Oruba, L., Soward, A.M., Dormy, E.
Format Journal Article
LanguageEnglish
Published Cambridge, UK Cambridge University Press 25.05.2021
Cambridge University Press (CUP)
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Abstract In an earlier paper, Oruba et al. (J. Fluid Mech., vol. 818, 2017, pp. 205–240) considered the primary quasi-steady geostrophic (QG) motion of a constant density fluid of viscosity $\nu$ that occurs during linear spin-down in a cylindrical container of radius $L$ and height $H$, rotating rapidly (angular velocity $\varOmega$) about its axis of symmetry subject to mixed rigid and stress-free boundary conditions for the case $L=H$. Direct numerical simulation (DNS) of the linear system at large $L= 10 H$ and Ekman number $E\leqslant \nu /H^2\varOmega =10^{-3}$ by Oruba et al. (J. Fluid Mech., vol. 888, 2020, p. 44) reveals significant inertial wave activity on the spin-down time scale. That analytic study, for $E\ll 1$, builds on the results of Greenspan & Howard (J. Fluid Mech., vol. 17, 1963, pp. 385–404) for an infinite plane layer $L\to \infty$. At large but finite distance from the symmetry axis, the meridional (QG-)flow, that causes the QG-spin-down, is blocked by the lateral boundary, which provides the primary QG-trigger for inertial wave generation. For the laterally unbounded layer, Greenspan and Howard identified, in addition to the QG-flow, inertial waves of maximum frequency (MF) $2\varOmega$, which are a manifestation of the transient Ekman layer. The blocking of these additional MF-waves by the lateral boundary provides an extra trigger that complements the QG-triggered inertial waves. Here we obtain analytic results for the full wave activity caused by the combined trigger ($\text {QG}+\text {MF}$) that faithfully capture their true character.
AbstractList In an earlier paper, Oruba et al. (J. Fluid Mech., vol. 818, 2017, pp. 205–240) considered the primary quasi-steady geostrophic (QG) motion of a constant density fluid of viscosity \(\nu\) that occurs during linear spin-down in a cylindrical container of radius \(L\) and height \(H\), rotating rapidly (angular velocity \(\varOmega\)) about its axis of symmetry subject to mixed rigid and stress-free boundary conditions for the case \(L=H\). Direct numerical simulation (DNS) of the linear system at large \(L= 10 H\) and Ekman number \(E\leqslant \nu /H^2\varOmega =10^{-3}\) by Oruba et al. (J. Fluid Mech., vol. 888, 2020, p. 44) reveals significant inertial wave activity on the spin-down time scale. That analytic study, for \(E\ll 1\), builds on the results of Greenspan & Howard (J. Fluid Mech., vol. 17, 1963, pp. 385–404) for an infinite plane layer \(L\to \infty\). At large but finite distance from the symmetry axis, the meridional (QG-)flow, that causes the QG-spin-down, is blocked by the lateral boundary, which provides the primary QG-trigger for inertial wave generation. For the laterally unbounded layer, Greenspan and Howard identified, in addition to the QG-flow, inertial waves of maximum frequency (MF) \(2\varOmega\), which are a manifestation of the transient Ekman layer. The blocking of these additional MF-waves by the lateral boundary provides an extra trigger that complements the QG-triggered inertial waves. Here we obtain analytic results for the full wave activity caused by the combined trigger (\(\text {QG}+\text {MF}\)) that faithfully capture their true character.
In an earlier paper, Oruba et al. ( J. Fluid Mech. , vol. 818, 2017, pp. 205–240) considered the primary quasi-steady geostrophic (QG) motion of a constant density fluid of viscosity $\nu$ that occurs during linear spin-down in a cylindrical container of radius $L$ and height $H$ , rotating rapidly (angular velocity $\varOmega$ ) about its axis of symmetry subject to mixed rigid and stress-free boundary conditions for the case $L=H$ . Direct numerical simulation (DNS) of the linear system at large $L= 10 H$ and Ekman number $E\leqslant \nu /H^2\varOmega =10^{-3}$ by Oruba et al. ( J. Fluid Mech. , vol. 888, 2020, p. 44) reveals significant inertial wave activity on the spin-down time scale. That analytic study, for $E\ll 1$ , builds on the results of Greenspan & Howard ( J. Fluid Mech. , vol. 17, 1963, pp. 385–404) for an infinite plane layer $L\to \infty$ . At large but finite distance from the symmetry axis, the meridional (QG-)flow, that causes the QG-spin-down, is blocked by the lateral boundary, which provides the primary QG-trigger for inertial wave generation. For the laterally unbounded layer, Greenspan and Howard identified, in addition to the QG-flow, inertial waves of maximum frequency (MF) $2\varOmega$ , which are a manifestation of the transient Ekman layer. The blocking of these additional MF-waves by the lateral boundary provides an extra trigger that complements the QG-triggered inertial waves. Here we obtain analytic results for the full wave activity caused by the combined trigger ( $\text {QG}+\text {MF}$ ) that faithfully capture their true character.
ArticleNumber A53
Author Oruba, L.
Dormy, E.
Soward, A.M.
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  surname: Oruba
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  organization: 1Laboratoire Atmosphères Milieux Observations Spatiales (LATMOS/IPSL), Sorbonne Université, UVSQ, CNRS, Paris, France
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  givenname: A.M.
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  surname: Soward
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  email: ludivine.oruba@latmos.ipsl.fr
  organization: 2School of Mathematics and Statistics, Newcastle University, Newcastle upon Tyne NE1 7RU, UK
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  givenname: E.
  orcidid: 0000-0002-9683-6173
  surname: Dormy
  fullname: Dormy, E.
  email: ludivine.oruba@latmos.ipsl.fr
  organization: 3Département de Mathématiques et Applications, UMR-8553, École Normale Supérieure, CNRS, PSL University, 75005 Paris, France
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Snippet In an earlier paper, Oruba et al. (J. Fluid Mech., vol. 818, 2017, pp. 205–240) considered the primary quasi-steady geostrophic (QG) motion of a constant...
In an earlier paper, Oruba et al. ( J. Fluid Mech. , vol. 818, 2017, pp. 205–240) considered the primary quasi-steady geostrophic (QG) motion of a constant...
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SubjectTerms Angular velocity
Boundary conditions
Cyclones
Cylinders
Direct numerical simulation
Ekman layer
Fluid mechanics
Free boundaries
Inertial waves
JFM Papers
Laplace transforms
Mathematical models
Mechanics
Physics
Rotating cylinders
Rotation
Symmetry
Velocity
Viscosity
Vortices
Wave generation
Title Inertial wave activity during spin-down in a rapidly rotating penny shaped cylinder
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Volume 915
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