Directional change of tracer trajectories in rotating Rayleigh-Bénard convection

Kim M. J. Alards, Hadi Rajaei, Rudie P. J. Kunnen, Federico Toschi, and Herman J. H. Clercx
Phys. Rev. E 97, 063105 – Published 18 June 2018

Abstract

The angle of directional change of tracer trajectories in rotating Rayleigh-Bénard convection is studied as a function of the time increment τ between two instants of time along the trajectories, both experimentally and with direct numerical simulations. Our aim is to explore the geometrical characterization of flow structures in turbulent convection in a wide range of timescales and how it is affected by background rotation. We find that probability density functions (PDFs) of the angle of directional change θ(t,τ) show similar behavior as found in homogeneous isotropic turbulence, up to the timescale of the large-scale coherent flow structures. The scaling of the averaged (over particles and time) angle of directional change Θ(τ)=|θ(t,τ)| with τ shows a transition from the ballistic regime [Θ(τ)τc with c=1] for ττη, with τη the Kolmogorov timescale, to a scaling with smaller exponent c for τητTL, with TL the Lagrangian integral timescale. This scaling exponent is approximately constant in the weakly rotating regime (Rossby number Ro2.5) and is decreasing for increasing rotation rates when Ro2.5. We show that this trend in the scaling exponent is related with the large-scale coherent structures in the flow; the large-scale circulation for Ro2.5 and vertically aligned vortices emerging from the boundary layers (BLs) near the top and bottom plates and penetrating into the bulk for Ro2.5. In the viscous BLs, the PDFs of θ(t,τ) and scaling properties of Θ(τ) are in general different from those measured in the bulk and depend on the type of boundary layer, in particular whether the BL is of Prandtl-Blasius type (Ro2.5) or of Ekman type (Ro2.5). When it is of Ekman type, a stronger dynamic coupling exists between the BL and the bulk of the flow, resulting in similar scaling exponents in BL and bulk.

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  • Received 8 March 2018

DOI:https://doi.org/10.1103/PhysRevE.97.063105

©2018 American Physical Society

Physics Subject Headings (PhySH)

Fluid Dynamics

Authors & Affiliations

Kim M. J. Alards1,*, Hadi Rajaei1, Rudie P. J. Kunnen1, Federico Toschi1,2,3, and Herman J. H. Clercx1

  • 1Fluid Dynamics Laboratory, Department of Applied Physics, Eindhoven University of Technology, P.O. Box 513, 5600 MB Eindhoven, The Netherlands
  • 2Centre of Analysis, Scientific Computing, and Applications W&I, Department of Mathematics and Computer Science, Eindhoven University of Technology, P.O. Box 513, 5600 MB Eindhoven, The Netherlands
  • 3Istituto per le Applicazioni del Calcolo, Consiglio Nazionale delle Ricerche, Via dei Taurini 19, 00185 Rome, Italy

  • *k.m.j.alards@tue.nl

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Vol. 97, Iss. 6 — June 2018

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