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 in | Journal of fluid mechanics Vol. 915 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
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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. |
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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. |
Author_xml | – sequence: 1 givenname: L. orcidid: 0000-0003-0230-8634 surname: Oruba fullname: Oruba, L. email: ludivine.oruba@latmos.ipsl.fr organization: 1Laboratoire Atmosphères Milieux Observations Spatiales (LATMOS/IPSL), Sorbonne Université, UVSQ, CNRS, Paris, France – sequence: 2 givenname: A.M. orcidid: 0000-0001-5536-5718 surname: Soward fullname: Soward, A.M. email: ludivine.oruba@latmos.ipsl.fr organization: 2School of Mathematics and Statistics, Newcastle University, Newcastle upon Tyne NE1 7RU, UK – sequence: 3 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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Cites_doi | 10.1175/MWR-D-19-0185.1 10.1002/qj.49711247114 10.1017/S0022112008002711 10.1017/jfm.2014.304 10.1038/nphys2984 10.1007/s00376-014-4063-x 10.1103/PhysRevFluids.3.013502 10.1017/jfm.2019.1064 10.1017/jfm.2017.134 10.1126/science.1135650 10.1175/1520-0469(2001)058<0421:ASDOHL>2.0.CO;2 10.1175/1520-0469(1968)025<1034:TCIARF>2.0.CO;2 10.22499/2.6401.004 10.1175/1520-0469(1974)031<2081:SAOTLV>2.0.CO;2 10.1017/S0022112088000485 10.1175/1520-0469(1979)036<0140:ASITLV>2.0.CO;2 10.1146/annurev.fluid.33.1.231 10.1017/S0022112063001415 10.1017/9781139024853 10.1175/1520-0469(1987)044<0542:AAITFT>2.0.CO;2 10.1146/annurev.fl.06.010174.001353 10.1103/PhysRevFluids.4.074701 10.1080/03091929.2019.1692829 10.1017/S0022112095000516 |
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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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