2008
DOI: 10.1175/2007jas2410.1
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3D Chaotic Model for Subgrid Turbulent Dispersion in Large Eddy Simulations

Abstract: We introduce a 3D multiscale kinematic velocity field as a model to simulate Lagrangian turbulent dispersion. The incompressible velocity field is a nonlinear deterministic function, periodic in space and time, that generates chaotic mixing of Lagrangian trajectories. Relative dispersion properties, e.g. the Richardson's law, are correctly reproduced under two basic conditions: 1) the velocity amplitudes of the spatial modes must be related to the corresponding wavelengths through the Kolmogorov scaling; 2) th… Show more

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Cited by 21 publications
(26 citation statements)
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“…It is also an indication that different dispersion regimes may overlap due to particle separation being influenced more by characteristic lengths of the velocity field than by characteristics times, 47 and generate possible statistical bias. Hence the need to complement fixed-time statistics with fixed-scale statistics.…”
Section: Resultsmentioning
confidence: 99%
“…It is also an indication that different dispersion regimes may overlap due to particle separation being influenced more by characteristic lengths of the velocity field than by characteristics times, 47 and generate possible statistical bias. Hence the need to complement fixed-time statistics with fixed-scale statistics.…”
Section: Resultsmentioning
confidence: 99%
“…in analogy with chaotic cellular flows (Solomon and Gollub, 1988;Crisanti et al, 1991;Lacorata et al, 2008). Further, the suppression of the vertical dynamics below the mixing layer is included in terms of a damping term ϒ(z) = exp(−|z|/L), multiplying the vector potential .…”
Section: The 3-d Klmmentioning
confidence: 99%
“…Direction angles and phases are random variables kept constant along each realization and uniformly distributed in [0, 2π). Following Lacorata, Mazzino & Rizza (2008), where relative dispersion properties were analysed via a multiple-scale kinematic velocity field, we distribute spatial modes according to a given density factor (here √ 2): q i+1 = √ 2q i . Wavelengths follow from the usual definition λ i = 2π/q i .…”
Section: A Simple Model For the Small-scale Velocity Fluctuationsmentioning
confidence: 99%