Phys. Rev. Lett. 78, 666 - 669 (1997)

Physical Regimes and Dimensional Structure of Rotating Turbulence

Download: PDF (147 kB) or Buy this Article (Use Article Pack) Export: BibTeX or EndNote (RIS)

V. M. Canuto and M. S. Dubovikov
NASA Goddard Institute for Space Studies, 2880 Broadway, New York, New York 10025

Received 24 June 1996

Numerical simulations of rotating turbulence have given rise to “unexpected results”: An increasing Ω did not lead to the “expected” route to a 2D state. A recent model of turbulence leads to a new number N  =  K(νΩ)-1 (K and ν are turbulent kinetic energy and viscosity) so that DNS (direct numerical simulation) and LES (large eddy simulation) correspond to N<1 and N>1. In the first case, the energy cascade is suppressed, while in the second case there exists an inertial spectrum which is an equilibrium of quasi–2D-3D modes. With these ingredients, we reproduce DNS and LES data.


©1997 The American Physical Society

URL: http://link.aps.org/abstract/PRL/v78/p666
DOI: 10.1103/PhysRevLett.78.666
PACS: 47.27.Te, 47.32.-y

[ Abstract  |  Previous article  |  Next article  |  Issue 4 ]