Approaching the Asymptotic Regime of Rapidly Rotating Convection: Boundary Layers versus Interior Dynamics

S. Stellmach, M. Lischper, K. Julien, G. Vasil, J. S. Cheng, A. Ribeiro, E. M. King, and J. M. Aurnou
Phys. Rev. Lett. 113, 254501 – Published 15 December 2014

Abstract

Rapidly rotating Rayleigh-Bénard convection is studied by combining results from direct numerical simulations (DNS), laboratory experiments, and asymptotic modeling. The asymptotic theory is shown to provide a good description of the bulk dynamics at low, but finite Rossby number. However, large deviations from the asymptotically predicted heat transfer scaling are found, with laboratory experiments and DNS consistently yielding much larger Nusselt numbers than expected. These deviations are traced down to dynamically active Ekman boundary layers, which are shown to play an integral part in controlling heat transfer even for Ekman numbers as small as 107. By adding an analytical parametrization of the Ekman transport to simulations using stress-free boundary conditions, we demonstrate that the heat transfer jumps from values broadly compatible with the asymptotic theory to states of strongly increased heat transfer, in good quantitative agreement with no-slip DNS and compatible with the experimental data. Finally, similarly to nonrotating convection, we find no single scaling behavior, but instead that multiple well-defined dynamical regimes exist in rapidly rotating convection systems.

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  • Received 17 July 2014

DOI:https://doi.org/10.1103/PhysRevLett.113.254501

© 2014 American Physical Society

Authors & Affiliations

S. Stellmach1,*, M. Lischper1, K. Julien2, G. Vasil3, J. S. Cheng4, A. Ribeiro4, E. M. King5, and J. M. Aurnou4

  • 1Institut für Geophysik, Westfälische Wilhelms-Universität Münster, Münster D-48149, Germany
  • 2Department of Applied Mathematics, University of Colorado Boulder, Boulder, Colorado 80309, USA
  • 3School of Mathematics and Statistics, University of Sydney, Sydney NSW 2006, Australia
  • 4Department of Earth, Planetary and Space Sciences, University of California, Los Angeles, California 90095-1567, USA
  • 5Miller Institute and Department of Earth and Planetary Science, Berkeley, California 94720-4767, USA

  • *stephan.stellmach@uni-muenster.de

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Vol. 113, Iss. 25 — 19 December 2014

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