Lattice Boltzmann solutions of the three-dimensional planetary geostrophic equations

Clicks: 3
ID: 302082
1999
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Abstract
We use the lattice Boltzmann method as the basis for a three-dimensional, numerical ocean circulation model in a rectangular basin. The fundamental dynamical variables are the populations of mass- and buoyancy-particles with prescribed discrete velocities. The particles obey collision rules that correspond, on the macroscopic scale, to planetary geostrophic dynamics. The advantages of the model are simplicity, stability, and massively parallel construction. By the special nature of its construction, the lattice Boltzmann model resolves upwelling boundary layers and unsteady convection. Solutions of the model show many of the features predicted by ocean circulation theories.
Reference Key
openalex_W2123960926 Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors Rick Salmon
Journal journal of marine research
Year 1999
DOI
10.1357/002224099321514079
URL
Keywords Keywords not found

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