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• W2167154018 abstract "We introduce a simple turbulence model for smoke animation, qualitatively capturing the transport, diffusion, and spectral cascade of turbulent energy unresolved on a typical simulation grid. We track the mean kinetic energy per octave of turbulence in each grid cell, and a novel net rotation variable for modeling the self-advection of turbulent eddies. These additions to a standard fluid solver drive a procedural post-process, layering plausible dynamically evolving turbulent details on top of the large-scale simulated motion. Finally, to make the most of the simulation grid before jumping to procedural sub-grid models, we propose a new multistep predictor to alleviate the nonphysical dissipation of angular momentum in standard graphics fluid solvers." @default.
• W2167154018 created "2016-06-24" @default.
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• W2167154018 date "2008-07-07" @default.
• W2167154018 modified "2023-10-03" @default.
• W2167154018 title "Evolving sub-grid turbulence for smoke animation" @default.
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• W2167154018 doi "https://doi.org/10.5555/1632592.1632594" @default.
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