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Hard turbulence in rotating Rayleigh-Bénard convection

K. Julien, S. Legg, J. McWilliams, and J. Werne
Phys. Rev. E 53, R5557(R) – Published 1 June 1996
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Abstract

We report a transition to hard turbulence in rapidly rotating Boussinesq convection at high Rayleigh and Taylor numbers. The probability density for vertical vorticity develops exponential tails, as in nonrotating hard-turbulent convection, whereas the temperature and velocity retain Gaussian distributions. The Nusselt-number scaling with Rayleigh number for the rotating hard-turbulent state is identical to that for nonrotating laboratory experiments, viz., Nu∼Ra2/7.

  • Received 10 April 1995

DOI:https://doi.org/10.1103/PhysRevE.53.R5557

©1996 American Physical Society

Authors & Affiliations

K. Julien1,2, S. Legg1,3, J. McWilliams2,3, and J. Werne2

  • 1Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder, Colorado 80309
  • 2National Center for Atmospheric Research, Boulder, Colorado 80307
  • 3University of California, Los Angeles, Los Angeles, California 90095-1565

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Vol. 53, Iss. 6 — June 1996

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