Energy transfer in turbulence under rotation

Michele Buzzicotti, Hussein Aluie, Luca Biferale, and Moritz Linkmann
Phys. Rev. Fluids 3, 034802 – Published 21 March 2018

Abstract

It is known that rapidly rotating turbulent flows are characterized by the emergence of simultaneous upscale and downscale energy transfer. Indeed, both numerics and experiments show the formation of large-scale anisotropic vortices together with the development of small-scale dissipative structures. However the organization of interactions leading to this complex dynamics remains unclear. Two different mechanisms are known to be able to transfer energy upscale in a turbulent flow. The first is characterized by two-dimensional interactions among triads lying on the two-dimensional, three-component (2D3C)/slow manifold, namely on the Fourier plane perpendicular to the rotation axis. The second mechanism is three-dimensional and consists of interactions between triads with the same sign of helicity (homochiral). Here, we present a detailed numerical study of rotating flows using a suite of high-Reynolds-number direct numerical simulations (DNS) within different parameter regimes to analyze both upscale and downscale cascade ranges. We find that the upscale cascade at wave numbers close to the forcing scale is generated by increasingly dominant homochiral interactions which couple the three-dimensional bulk and the 2D3C plane. This coupling produces an accumulation of energy in the 2D3C plane, which then transfers energy to smaller wave numbers thanks to the two-dimensional mechanism. In the forward cascade range, we find that the energy transfer is dominated by heterochiral triads and is dominated primarily by interaction within the fast manifold where kz0. We further analyze the energy transfer in different regions in the real-space domain. In particular, we distinguish high-strain from high-vorticity regions and we uncover that while the mean transfer is produced inside regions of strain, the rare but extreme events of energy transfer occur primarily inside the large-scale column vortices.

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  • Received 30 October 2017

DOI:https://doi.org/10.1103/PhysRevFluids.3.034802

©2018 American Physical Society

Physics Subject Headings (PhySH)

Fluid Dynamics

Authors & Affiliations

Michele Buzzicotti1,*, Hussein Aluie2,†, Luca Biferale1,‡, and Moritz Linkmann1,§

  • 1Department of Physics and INFN, University of Rome “Tor Vergata,” via della Ricerca Scientifica 1, 00133, Rome, Italy
  • 2Department of Mechanical Engineering, University of Rochester, Rochester, New York 14627, USA

  • *michele.buzzicotti@roma2.infn.it
  • hussein@rochester.edu
  • biferale@roma2.infn.it
  • §linkmann@roma2.infn.it

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Issue

Vol. 3, Iss. 3 — March 2018

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