The emergence of isolated coherent vortices in turbulent flow.
Abstract
A study is made of some numerical calculations of two-dimensional and geostrophic turbulent flows. The primary result is that, under a broad range of circumstances, the flow structure has its vorticity concentrated in a small fraction of the spatial domain, and these concentrations typically have lifetimes long compared with the characteristic time for nonlinear interactions in turbulent flow (i.e. an eddy turnaround time). When such vorticity concentrations occur, they tend to assume an axisymmetric shape and persist under passive advection by the large-scale flow, except for relatively rare encounters with other centres of concentration. These structures can arise from random initial conditions without vorticity concentration, evolving in the midst of what has been traditionally characterized as the ‘cascade’ of isotropic, homogeneous, large-Reynolds-number turbulence: the systematic elongation of isolines of vorticity associated with the transfer of vorticity to smaller scales, eventually to dissipation scales, and the transfer of energy to larger scales. When the vorticity concentrations are a sufficiently dominant component of the total vorticity field, the cascade processes are suppressed. The demonstration of persistent vorticity concentrations on intermediate scales - smaller than the scale of the peak of the energy spectrum and larger than the dissipation scales - does not invalidate many of the traditional characterizations of two-dimensional and geostrophic turbulence, but I believe it shows them to be substantially incomplete with respect to a fundamental phenomenon in such flows.
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Coherent vortices preferentially exist in regions where absolute vorticity or potential vorticity gradients vanish, as they can then arise spontaneously in barotropic or quasigeostrophic flows and remain stable.
“Coherent vortices preferentially exist in regions where absolute vorticity or potential vorticity gradients vanish, as they can then arise spontaneously in barotropic or quasigeostrophic flows and remain stable (e.g., McWilliams 1984;Marcus 1988Marcus , 1993)).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as McWilliams 1984
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Mechanisms of Jet Formation on the Giant Planets
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- Authors
- Mcwilliams, J. C.
- Affiliations
- NSF National Center for Atmospheric Research (US)
- Corresponding author
- Mcwilliams, James C.
- ORCID
- Mcwilliams, James C.
- Venue
- Journal of Fluid Mechanics
- Publisher
- Cambridge University Press (CUP)
- Published
- 1984-09
- Volume
- 146
- Pages
- 21-43
- ISSN
- 0022-1120 (ISSN-L)
- 1469-7645
- OpenAlex
- W2996439688
- Cited by
- 1,131
- References
- 29
- Citations by year
- 2026: 19 · 2025: 13 · 2024: 20 · 2023: 17 · 2022: 23 · 2021: 19 · 2020: 22 · 2019: 18 · 2018: 23 · 2017: 17 · 2016: 19 · 2015: 15 · 2014: 25 · 2013: 20 · 2012: 25
- FWCI
- 23.82
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Journal of Fluid Mechanics (publishedVersion)
- Topics
- Physical Sciences › Engineering › Computational Mechanics › Fluid Dynamics and Turbulent Flows
- Physical Sciences › Engineering › Computational Mechanics › Computational Fluid Dynamics and Aerodynamics
- Physical Sciences › Earth and Planetary Sciences › Oceanography › Oceanographic and Atmospheric Processes
- Keywords
- coherent vortices, isolated vortex, two-dimensional turbulence, geostrophic turbulence, vorticity concentration, energy cascade, eddy turnover time, axisymmetric vortex, intermediate scale
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