TY - CONF
T1 - Core dynamics of a strained vortex column
T2 - 30th Fluid Dynamics Conference, 1999
AU - Pradeep, Dhoorjaty S.
AU - Hussain, Fazle
N1 - Funding Information:
This research was supported by NSF grant CTS-9622302. Supercomputer time was provided by the NASA Ames ResearchC enter.
Funding Information:
This research was supportedb y NSF grant CTS-9622302. Supercomputert ime was provided by the NASA Ames ResearchC enter.
Publisher Copyright:
© 1999 by the American Institute of Aeronautics and Astronautics, Inc. All rights reserved.
Copyright:
Copyright 2016 Elsevier B.V., All rights reserved.
PY - 1999
Y1 - 1999
N2 - The instability and transition in a vortex column embedded in a plane shear perpendicular to its axis is studied via direct numerical simulations. We focus on the evolution of varicose modes (i.e. core dynamics, CD) on the column. Standing wave oscillations of vorticity, damped in the absence of shear, amplify exponentially at a rate that increases with increasing shear. The instability has a shortwave character, a low-shear cutoff at a given Re, and a low-Re cutoff at a given shear; the instability results from resonant forcing of perturbation vorticity that occurs when the CD frequency matches the angular velocity of vortex fluid, causing sustained stretching of perturbation vorticity and hence cumulative CD growth. Nonlinear CD generates strong meridional flow-whose peak velocity even exceeds vortex azimuthal velocity-and is responsible for causing transition to turbulence via two distinct mechanisms: (i) generation and subsequent roll-up of intense vorticity sheaths, and (ii) folding and reconnection of core vortex filaments. Cascade to small scales occurs in parallel with backscatter (Le. anticascade) by the pairing of rolled up vortices. The result is a fully turbulent flow, containing small-scale structures (which themselves may, as Re increases, generate finer scale vortices via selfsimilar CD). Although CD instability has a smaller growth rate than bending waves, it generates vorticity intermittency faster, which underlines its significance in transitional and turbulent flows.
AB - The instability and transition in a vortex column embedded in a plane shear perpendicular to its axis is studied via direct numerical simulations. We focus on the evolution of varicose modes (i.e. core dynamics, CD) on the column. Standing wave oscillations of vorticity, damped in the absence of shear, amplify exponentially at a rate that increases with increasing shear. The instability has a shortwave character, a low-shear cutoff at a given Re, and a low-Re cutoff at a given shear; the instability results from resonant forcing of perturbation vorticity that occurs when the CD frequency matches the angular velocity of vortex fluid, causing sustained stretching of perturbation vorticity and hence cumulative CD growth. Nonlinear CD generates strong meridional flow-whose peak velocity even exceeds vortex azimuthal velocity-and is responsible for causing transition to turbulence via two distinct mechanisms: (i) generation and subsequent roll-up of intense vorticity sheaths, and (ii) folding and reconnection of core vortex filaments. Cascade to small scales occurs in parallel with backscatter (Le. anticascade) by the pairing of rolled up vortices. The result is a fully turbulent flow, containing small-scale structures (which themselves may, as Re increases, generate finer scale vortices via selfsimilar CD). Although CD instability has a smaller growth rate than bending waves, it generates vorticity intermittency faster, which underlines its significance in transitional and turbulent flows.
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M3 - Paper
AN - SCOPUS:84963730036
Y2 - 28 June 1999 through 1 July 1999
ER -